From X-POP3-Rcpt: wp@eigsg1 Received: from email.tuwien.ac.at by eigsg1.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for wp id AA17276; Fri, 1 Jul 94 09:55:31 +0200 Message-Id: <9407010755.AA17276@eigsg1.tuwien.ac.at> Received: from EIBYTE by email.tuwien.ac.at with DECNET-IN (PP) id <13818-0@email.tuwien.ac.at>; Fri, 1 Jul 1994 09:47:05 +0200 X-Vms-To: WP To: wp From: wp@eibyte.una.ac.at Date: Fri, 1 Jul 1994 09:47:05 +0200 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit From: AUNIW::IN%"alan@cs.bris.ac.uk" "Alan Chalmers" 23-JUN-1994 13:35:36.02 To: IN%"globillum@cs.cmu.edu" CC: Subj: Eastern Europe Directory Received: from HOSTESS.GRAPHICS.CS.CMU.EDU by Pap.UniVie.AC.AT (PMDF #12401) id <01HDVTJ88BIO934XAB@Pap.UniVie.AC.AT>; Thu, 23 Jun 1994 13:42 GMT+0100 Received: from CS.CMU.EDU by HOSTESS.GRAPHICS.CS.CMU.EDU id aa06157; 23 Jun 94 7:33:39 EDT Received: from sun2.nsfnet-relay.ac.uk by CS.CMU.EDU id aa26646; 23 Jun 94 7:33:06 EDT Received: from kukini.cs.bris.ac.uk by dir.bris.ac.uk with SMTP (PP) id <07186-0@dir.bris.ac.uk>; Thu, 23 Jun 1994 12:31:38 +0100 Received: from luna by kukini.compsci.bristol.ac.uk id aa00737; 23 Jun 94 11:33 GMT Date: Thu, 23 Jun 94 11:31:11 GMT From: Alan Chalmers Subject: Eastern Europe Directory To: globillum@cs.cmu.edu Message-id: <9406231131.aa26226@uk.ac.bristol.compsci.luna> Via: uk.ac.bristol; Thu, 23 Jun 1994 12:31:48 +0100 The latest version of the Eastern Europe Computer Graphics Contacts Directory (as it appeared at the Spring School on Computer Graphics in Bratislava in June) is now available. If you would like a copy just email me and I will send it in uuencoded compressed postscript format. Best wishes Alan Chalmers From X-POP3-Rcpt: wp@stellaris Received: from email.tuwien.ac.at by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for wp id AA08895; Tue, 2 Aug 94 15:03:54 +0200 Message-Id: <9408021303.AA08895@stellaris.cg.tuwien.ac.at> Received: from EIGVS4 by email.tuwien.ac.at with DECNET-IN (PP) id <15084-0@email.tuwien.ac.at>; Tue, 2 Aug 1994 15:00:04 +0200 X-Vms-To: IN%"globillum@cs.cmu.edu" To: wp@eigsg1.tuwien.ac.at From: @auniw, @eigvs4:in%shirley@graphics.cornell.edu Subject: Terminolgy, almost done! Date: Tue, 2 Aug 1994 15:00:04 +0200 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Received: from HOSTESS.GRAPHICS.CS.CMU.EDU by Pap.UniVie.AC.AT (PMDF #12401) id <01HFFS0FLVV49PM4L5@Pap.UniVie.AC.AT>; Tue, 2 Aug 1994 15:02 GMT+0100 Received: from CS.CMU.EDU by HOSTESS.GRAPHICS.CS.CMU.EDU id aa00531; 2 Aug 94 8:53:09 EDT Received: from MERCKX.GRAPHICS.CORNELL.EDU by CS.CMU.EDU id aa13052; 2 Aug 94 8:53:05 EDT Received: by merckx.graphics.cornell.edu (5.65/DEC-Ultrix/4.3) id AA25626; Tue, 2 Aug 1994 08:53:07 -0400 Received: by zap.graphics.cornell.edu (1.37.109.8/16.2) id AA10591; Tue, 2 Aug 1994 08:53:02 -0400 Date: Tue, 2 Aug 1994 08:53:02 -0400 (EDT) From: Peter Shirley Subject: Terminolgy, almost done! To: globillum@cs.cmu.edu Message-id: <9408021253.AA25626@merckx.graphics.cornell.edu> Content-type: text/plain; charset=US-ASCII Content-transfer-encoding: 7bit X-Mailer: ELM [version 2.4 PL23] Mime-Version: 1.0 Content-Length: 786 Now that Siggraph is over, I am about to send out the results of the terminology survey. There are two loose ends I would like to clear up first. Any help is appreciated. 1) Does anybody have a recent list of CR keywords and categories? Those are those things you see at the start of many papers-- e.g. "I.3.7 [Computer Graphics: Three-Dimensional Graphics and Realism". 2) If your mother-tongue is not english, is there a direct (or used) equivalent to the following terms? rendering realistic rendering photorealistic rendering image synthesis realistic image synthesis photorealistic image synthesis Thanks Pete "worries to much about words" Shirley shirley@barn.graphics.cornell.edu From X-POP3-Rcpt: wp@stellaris Received: from email.tuwien.ac.at by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for wp id AA16834; Thu, 4 Aug 94 16:14:40 +0200 Message-Id: <9408041414.AA16834@stellaris.cg.tuwien.ac.at> Received: from EIGVS4 by email.tuwien.ac.at with DECNET-IN (PP) id <23731-0@email.tuwien.ac.at>; Thu, 4 Aug 1994 16:10:44 +0200 X-Vms-To: IN%"globillum@cs.cmu.edu", IN%"speer@crl.com" To: wp@eigsg1.tuwien.ac.at From: @auniw, @eigvs4:in%shirley@graphics.cornell.edu Subject: Some Shirley papers on ftp Date: Thu, 4 Aug 1994 16:10:44 +0200 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Received: from HOSTESS.GRAPHICS.CS.CMU.EDU by Pap.UniVie.AC.AT (PMDF #12401) id <01HFIN1XU05C9PM842@Pap.UniVie.AC.AT>; Thu, 4 Aug 1994 16:13 GMT+0100 Received: from RI.CMU.EDU by HOSTESS.GRAPHICS.CS.CMU.EDU id aa05406; 4 Aug 94 10:00:35 EDT Received: from MERCKX.GRAPHICS.CORNELL.EDU by RI.CMU.EDU id aa29617; 4 Aug 94 10:00:08 EDT Received: by merckx.graphics.cornell.edu (5.65/DEC-Ultrix/4.3) id AA07243; Thu, 4 Aug 1994 10:00:06 -0400 Received: by zap.graphics.cornell.edu (1.37.109.8/16.2) id AA29484; Thu, 4 Aug 1994 10:00:01 -0400 Date: Thu, 4 Aug 1994 10:00:01 -0400 (EDT) From: Peter Shirley Subject: Some Shirley papers on ftp To: globillum@cs.cmu.edu, speer@crl.com Message-id: <9408041400.AA07243@merckx.graphics.cornell.edu> Content-type: text/plain; charset=US-ASCII Content-transfer-encoding: 7bit X-Mailer: ELM [version 2.4 PL23] Mime-Version: 1.0 Content-Length: 2525 Several people on this list have asked for copies of some of my hard-to-find papers, so to exploit parallelism I have put them in an ftp site. I will append a copy of the README file. site: ftp.cs.indiana.edu (129.79.254.191) directory pub/shirley (login with account "ftp" and give your email address as passwd) Good luck, and inform me if you have trouble. Pete ======================= README ======================================== Here are some postscript files for some of my old papers. euro91.ps.Z A Eurographics 91 paper on evaluating the quality of sampling patterns. Mostly of interest if you want pointers to the discrepancy literature (although Dobkins/Mitchell's more recent work ina GI93 and the 92 Renderng workshop is more complete). gi90.ps.Z My graphics interface 90 paper on hooking up bakward (Arvo) ray tracing with radiosity (a hard-coded three pass strategy). Some figures missing. The Chen et al paper from siggraph 91 is a (much) more complete application of multi-pass methods. gi91.ps.Z With Sung/Brown. An implementation paper that extends the work of Kirk/Arvo's "Ray Tracing Kernal". Includes a (sketchily described!) implementation of radiosity with non-diffuse patches that is similar to that proposed by Le Saec and Schlick at the 1990 rendering workshop. gi93.ps.Z With a cast of thousands. Describes some experience with eliminating burnout when displaying high dynamic range images. About a 12Mb ps file-- sorry! rw91.ps.Z With Wang. A Eurographics Rendering Workshop paper on sampling luminaires in ray tracing. This will be extended in a forthcoming TOG paper. rw92.ps.Z With Wang. How do you handle surfaces that are neither ideal diffuse nor ideal speculan a ray tracer? This paper doesn't give a good answer, but does argue that the answer is not simple! rw94.ps.Z With Chiu. Fleshes out Kajiya's arguments that for complex scenes, we need ray tracing approaches. tr.ps.Z With Chiu. Describes some implentational issues behind the figures in rw94.ps (Indiana U tech report). thesis Directory with a lot of out of date stuff! Probably not worth reading unless you are new to rendering. From X-POP3-Rcpt: wp@stellaris Received: from email.tuwien.ac.at by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for wp id AA20779; Fri, 5 Aug 94 19:52:46 +0200 Message-Id: <9408051752.AA20779@stellaris.cg.tuwien.ac.at> Received: from EIGVS4 by email.tuwien.ac.at with DECNET-IN (PP) id <08576-0@email.tuwien.ac.at>; Fri, 5 Aug 1994 19:49:00 +0200 X-Vms-To: IN%"globillum@cs.cmu.edu" To: wp@eigsg1.tuwien.ac.at From: @auniw, @eigvs4:in%paul.heckbert@hostess.graphics.cs.cmu.edu Subject: about the globillum mailing list Date: Fri, 5 Aug 1994 19:49:00 +0200 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Received: from HOSTESS.GRAPHICS.CS.CMU.EDU by Pap.UniVie.AC.AT (PMDF #12401) id <01HFK8YNU0M89PMA0U@Pap.UniVie.AC.AT>; Fri, 5 Aug 1994 19:51 GMT+0100 Date: Fri, 5 Aug 94 13:40:24 EDT From: Paul.Heckbert@HOSTESS.GRAPHICS.CS.CMU.EDU Subject: about the globillum mailing list To: globillum@cs.cmu.edu Message-id: <01HFK8YNU0M89PMA0U@Pap.UniVie.AC.AT> If you ever want an up-to-date list of who's on the globillum mailing list, ftp from host hostess.graphics.cs.cmu.edu the file /usr/ph/ftp/globillum/glob.mailrc . I update this file every time I change the mailing list. This file also contains non-electronic mailing addresses for some people. To join, leave, or change an address in the globillum mailing list, email to globillum-request@cs.cmu.edu -Paul Heckbert ph@cs.cmu.edu From X-POP3-Rcpt: wp@stellaris Received: from email.tuwien.ac.at by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for wp id AA27209; Fri, 19 Aug 94 19:06:37 +0200 Message-Id: <9408191706.AA27209@stellaris.cg.tuwien.ac.at> Received: from EIGVS4 by email.tuwien.ac.at with DECNET-IN (PP) id <14550-0@email.tuwien.ac.at>; Fri, 19 Aug 1994 19:02:33 +0200 X-Vms-To: IN%"globillum@HOSTESS.GRAPHICS.CS.CMU.EDU" To: wp@eigsg1.tuwien.ac.at From: @auniw, @eigvs4:in%dem@jupiter.cs.wayne.edu Subject: Position Announcement Date: Fri, 19 Aug 1994 19:02:33 +0200 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Received: from HOSTESS.GRAPHICS.CS.CMU.EDU by Pap.UniVie.AC.AT (PMDF #12401) id <01HG3RF7WTA89PMSSA@Pap.UniVie.AC.AT>; Fri, 19 Aug 1994 19:05 GMT+0100 Received: from pandora.cs.wayne.edu by HOSTESS.GRAPHICS.CS.CMU.EDU id aa08196; 19 Aug 94 12:57:28 EDT Received: from jupiter.cs.wayne.edu by pandora.cs.wayne.edu with SMTP id AA26036 (5.65b/IDA-1.4.3 for globillum@HOSTESS.GRAPHICS.CS.CMU.EDU); Fri, 19 Aug 94 12:57:07 -0400 Received: by jupiter.cs.wayne.edu (4.1/SMI-4.0) id AA11925; Fri, 19 Aug 94 12:53:28 EDT Date: Fri, 19 Aug 94 12:53:28 EDT From: dem@jupiter.cs.wayne.edu Subject: Position Announcement To: globillum@HOSTESS.GRAPHICS.CS.CMU.EDU Cc: dem@cs.wayne.edu Message-id: <9408191653.AA11925@jupiter.cs.wayne.edu> Wayne State University Department of Computer Science Faculty Positions The Wayne State University Department of Computer Science invites applications and nominations for several tenure-track positions: two in computer graphics and one in high performance computing. Candidates from related areas in computer science or computer engineering will also be considered. Candidates should have a Ph.D. in computer science/engineering or a closely related field, a strong interest in and commitment to both research and teaching and the potential for obtaining external research funding. Applications from minority and female candidates are especially encouraged. Wayne State University, located in Detroit's Cultural Center, is an urban, comprehensive research university serving 35,000 students. The Department of Computer Science has fourteen faculty members, approximately 75 Ph.D., 350 Masters and 350 undergraduate students. The faculty have many ties to local industries. Several research projects are currently being funded by these industries and federal agencies. Applicants should send a letter of intent, a statement of research and teaching interest, a resume with the names of at least three references, their addresses (including e-mail address) and telephone/fax numbers to: Dr. Narendra S. Goel, Chair Department of Computer Science Wayne State University 431 State Hall Detroit, MI 48202 Phone: (313) 577-2478 FAX: (313) 577-6868 e-mail: ngoel@cs.wayne.edu For full consideration applications should be submitted by November 1, 1994. However, applications will be accepted until the positions are filled. QUEST Wayne State University - People working together to provide quality service. Wayne State University is an Equal Opportunity/Affirmative Action Employer. From X-POP3-Rcpt: wp@stellaris Received: from email.tuwien.ac.at by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for wp id AA10732; Wed, 24 Aug 94 18:05:17 +0200 Message-Id: <9408241605.AA10732@stellaris.cg.tuwien.ac.at> Received: from EIGVS4 by email.tuwien.ac.at with DECNET-IN (PP) id <23024-0@email.tuwien.ac.at>; Wed, 24 Aug 1994 18:00:54 +0200 X-Vms-To: IN%"globillum@cs.cmu.edu" To: wp@eigsg1.tuwien.ac.at From: @auniw, @eigvs4:in%barbara.pela@cen.jrc.it Subject: global illumination & neural net Date: Wed, 24 Aug 1994 18:00:54 +0200 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Received: from HOSTESS.GRAPHICS.CS.CMU.EDU by Pap.UniVie.AC.AT (PMDF #12401) id <01HGAOQV0W689PMZE0@Pap.UniVie.AC.AT>; Wed, 24 Aug 1994 18:04 GMT+0100 Received: from CS.CMU.EDU by HOSTESS.GRAPHICS.CS.CMU.EDU id aa19070; 24 Aug 94 11:56:10 EDT Received: from dicscs1.jrc.it by CS.CMU.EDU id aa26634; 24 Aug 94 11:55:21 EDT Received: from cen.jrc.it (relay.jrc.it) by cen.jrc.it (4.1/SMI-4.1) id AA02091; Wed, 24 Aug 94 17:53:35 +0200 Received: from dpx2.isei.jrc.it by cen.jrc.it; Wed, 24 Aug 94 17:55:08 +0200 Received: by dpx2.isei.jrc.it; Wed, 24 Aug 94 18:01:25 +0200 (MET) Date: Wed, 24 Aug 94 18:01:25 +0200 From: barbara pela Subject: global illumination & neural net To: globillum@cs.cmu.edu Reply-to: barbara pela Message-id: <9408241601.AA15837@dpx2.isei.jrc.it> Hi, Somebody of you know papers or person working on "global illumination using neural net"? Barbara. From X-POP3-Rcpt: wp@stellaris Received: from email.tuwien.ac.at by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for wp id AA18099; Fri, 9 Sep 94 10:26:20 +0200 Message-Id: <9409090826.AA18099@stellaris.cg.tuwien.ac.at> Received: from EIGVS4 by email.tuwien.ac.at with DECNET-IN (PP) id <24285-0@email.tuwien.ac.at>; Thu, 8 Sep 1994 20:19:56 +0200 X-Vms-To: IN%"globillum@cs.cmu.edu" To: wp@eigsg1.tuwien.ac.at From: @auniw, @eigvs4:in%greg@hobbes.lbl.gov Subject: New version of MGF Date: Thu, 8 Sep 1994 20:19:56 +0200 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Received: from HOSTESS.GRAPHICS.CS.CMU.EDU by Pap.UniVie.AC.AT (PMDF #12401) id <01HGVRYJSA40A4LS5F@Pap.UniVie.AC.AT>; Thu, 8 Sep 1994 20:23 GMT+0100 Received: from CS.CMU.EDU by HOSTESS.GRAPHICS.CS.CMU.EDU id aa17808; 8 Sep 94 14:14:49 EDT Received: from lbl.gov by CS.CMU.EDU id aa24742; 8 Sep 94 14:11:51 EDT Received: from hobbes.lbl.gov by lbl.gov (4.1/1.39) id AA06648; Thu, 8 Sep 94 11:11:48 PDT Received: by hobbes.lbl.gov (3.2/SMI-3.2) id AA15365; Thu, 8 Sep 94 11:11:16 PDT Date: Thu, 8 Sep 94 11:11:16 PDT From: "Gregory J. Ward" Subject: New version of MGF To: globillum@cs.cmu.edu Message-id: <9409081811.AA15365@hobbes.lbl.gov> Fellow Globillumers, About a month and a half ago, I announced a new format called MGF (for Materials and Geometry Format) for exchanging scene data. I have since updated this standard to version 0.7 (still in prerelease) and announced it to the world via comp.graphics and sci.engr.lighting. If you have seen those announcements already, then you may want to skip the rest of this, but I realize that a lot of people either don't get network news or suffer from information overload and don't read it regularly. To remind you, MGF was developed by myself with help from Rob Shakespeare, Ian Ashdown and Holly Rushmeier. It will probably end up being the standard for representing light fixture geometry as part of a new IES (Illuminating Engineering Society) standard for luminaire data, but that's still down the road aways. In the meantime, I am trying to get people to play with the parser and scene/object library to work out problems in the specification and the code, and in hopes of simplifying and promoting data exchange between us research types. Here is a reprint of a recent posting... ------------------------------------------------------------------------- Announcing MGF: Materials and Geometry Format Here we have yet another proposal for a standard graphics scene representation, but with a few notable differences: 1) The material descriptions are physically-based and therefore usable for lighting simulation: radiosity and ray-tracing methods for global illumination. 2) The package includes an ANSI-C parser that makes writing a translator to any native format quick and painless. It also includes a nice library of objects and scenes culled from the Radiance distribution. 3) Use of the parser and library is free. The language was designed by the author and some other lighting and computer graphics experts/enthusiasts. It includes what it needs to include plus a little bit. It is by no means the ultimate scene description, and future attempts to improve the format must be weighed against the benefits of keeping things simple. Also, enhancements to the standard will be made in such a way that they do not place new demands on the programmers who support it. This will be accomplished by updating the parser along with the standard, so each programmer need only support those entities s/he knows how to translate. The parser will translate the rest. Some other basics about MGF: o It is a compact, human-readable ASCII format o It's syntax permits it to be embedded in TCL (I think) o It is strictly boundary-representation (for now) o It is mostly polyhedral, but supports a few conics o Vertices may be named, may have normals, and may be shared o Colors and materials may also be named and put in libraries o It supports full-spectral colors and arbitrary basis functions o It supports one-sided and two-sided surfaces o It supports rigid-body transformations and instancing o Materials may reflect, transmit and emit light To pick up the parser by anonymous ftp, look in the /www/mgf directory of hobbes.lbl.gov (128.3.12.38), or from WWW access the URL: ftp://hobbes.lbl.gov/www/mgf/HOME.html (By the way, we'd welcome links to other WWW sites, as we're isolated at the moment.) Comments are welcome. -Greg Ward Lighting Research Group Lawrence Berkeley Laboratory Berkeley, California GJWard@Lbl.Gov From X-POP3-Rcpt: wp@stellaris Received: from email.tuwien.ac.at by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for wp id AA21306; Fri, 9 Sep 94 15:55:57 +0200 Message-Id: <9409091355.AA21306@stellaris.cg.tuwien.ac.at> Received: from EIGVS4 by email.tuwien.ac.at with DECNET-IN (PP) id <10557-0@email.tuwien.ac.at>; Fri, 9 Sep 1994 15:51:26 +0200 X-Vms-To: IN%"globillum@cs.cmu.edu" To: wp@eigsg1.tuwien.ac.at From: @auniw, @eigvs4:in%erich@eye.com Subject: new radiosity bibliography, site, and maintainer Date: Fri, 9 Sep 1994 15:51:26 +0200 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Received: from HOSTESS.GRAPHICS.CS.CMU.EDU by Pap.UniVie.AC.AT (PMDF #12401) id <01HGWWW67C1SA4LTIH@Pap.UniVie.AC.AT>; Fri, 9 Sep 1994 15:55 GMT+0100 Received: by HOSTESS.GRAPHICS.CS.CMU.EDU id aa19178; 9 Sep 94 9:54:11 EDT Received: from CS.CMU.EDU by HOSTESS.GRAPHICS.CS.CMU.EDU id aa19148; 9 Sep 94 9:30:42 EDT Received: from eye.com by CS.CMU.EDU id aa00979; 9 Sep 94 9:29:53 EDT Received: from hemlock.eye.com by eye.com with SMTP (1.36.108.4/16.2) id AA03855; Fri, 9 Sep 1994 09:29:49 -0400 Received: by hemlock (1.37.109.8/15.6) id AA29225; Fri, 9 Sep 1994 09:29:49 -0400 Date: Fri, 9 Sep 1994 09:29:49 -0400 From: Eric Haines Subject: new radiosity bibliography, site, and maintainer To: globillum@cs.cmu.edu Message-id: <9409091329.AA29225@hemlock> A new release of the radiosity bibliography is now available via anonymous FTP at hobbes.lbl.gov in /pub/doc/RadBib94.Z. I've passed on maintenance of the bibliography to Ian Ashdown (72060.2420@CompuServe.COM), so please send him any updates you have. He's done quite a job updating the thing, adding more than 50% more entries to my previous bibliography, including papers from the fields of optics, remote sensing, and illumination engineering. Also, thanks to Greg for providing space on his FTP server for this resource. You may use this bibliography however you wish, though we enjoy knowing if you reprint it somewhere. Eric Haines erich@eye.com From X-POP3-Rcpt: wp@stellaris Received: from email.tuwien.ac.at by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for wp id AA28236; Fri, 23 Sep 94 17:07:37 +0200 Message-Id: <9409231507.AA28236@stellaris.cg.tuwien.ac.at> Received: from EIGVS4 by email.tuwien.ac.at with DECNET-IN (PP) id <13350-0@email.tuwien.ac.at>; Fri, 23 Sep 1994 17:07:40 +0200 X-Vms-To: IN%"globillum@cs.cmu.edu" To: wp@eigsg1.tuwien.ac.at From: @auniw, @eigvs4:in%nic@informatik.uni-rostock.de Subject: A remark on LAMBERT's law Date: Fri, 23 Sep 1994 17:07:40 +0200 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Received: from HOSTESS.GRAPHICS.CS.CMU.EDU by Pap.UniVie.AC.AT (PMDF #12401) id <01HHGJG4HJYOA4MJBH@Pap.UniVie.AC.AT>; Fri, 23 Sep 1994 17:06 GMT+0100 Received: from CS.CMU.EDU by HOSTESS.GRAPHICS.CS.CMU.EDU id aa27437; 23 Sep 94 10:56:09 EDT Received: from [139.30.5.28] by CS.CMU.EDU id aa05572; 23 Sep 94 8:53:26 EDT Received: by ceylon.informatik.uni-rostock.de id OAA11504; Fri, 23 Sep 1994 14:53:04 +0200 Received: from localhost (nic@localhost) by anne.informatik.uni-rostock.de (8.6.5/INSIDE021894) id JAA02532 for globillum@cs.cmu.edu; Mon, 5 Sep 1994 09:32:03 +0200 Date: Mon, 5 Sep 1994 09:32:02 +0200 (MET DST) From: Nico Guenther Subject: A remark on LAMBERT's law To: globillum@cs.cmu.edu Message-id: <199409050732.JAA02532@anne.informatik.uni-rostock.de> Content-type: text X-Mailer: ELM [version 2.4 PL23] Content-Length: 1777 Dear globillumers, last week I've got the SIGGRAPH-CD, and among the papers one called Generalization of Lambert's Reflectance Model by Michael Oren and Shree K. Nayar. In this paper it is shown, that the Lambert law (the way it is used in Computer Graphics) does not correctly reproduce real diffuse surfaces (like clay). That's right, and I agree. Based on this knowledge a complicated generalization somewhat analogous to the microfacet illumination model is involved. I believe, there is no need to complicate a good and simple law further, because the Lambert law as used in physics is right. However it is misinterpreted in computer graphics (and in thermal engineering - see Siegel and Howards book about Radiative Heat Transfer - too). I intended to publish a (complete) paper concerning the misinterpretation and misuse of good old Lambert in CG. However I think it is time to make the uncomplete pre-version available for discussion. (This version was published in July this year in Rostocker Informatik Berichte(1994) 15.) The paper "Illumination along convex edges" and the pictures can be ftp-ed from ftp.informatik.uni-rostock.de under /pub/graphics/edge_illu.ps.Z and edge_pictures.tar.Z. (The subdir is nearly empty because of a ftp-server-crashdown last week.) Although the final picture of "my" ;-) Lambert interpretation is missing, all important facts are included (I hope so). I know that the facts are somewhat exotic for most CG people, and it may be hard to believe in this. Just read it, and maybe we can have an interesting discussion about it. OK, I'm anxious for the responses. Greetings. Nico (nic@informatik.uni-rostock.de) From X-POP3-Rcpt: wp@stellaris Received: from email.tuwien.ac.at by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for wp id AA28622; Fri, 23 Sep 94 18:19:33 +0200 Message-Id: <9409231619.AA28622@stellaris.cg.tuwien.ac.at> Received: from EIGVS4 by email.tuwien.ac.at with DECNET-IN (PP) id <15140-0@email.tuwien.ac.at>; Fri, 23 Sep 1994 18:19:45 +0200 X-Vms-To: IN%"globillum@cs.cmu.edu" "Global Illumination" To: wp@eigsg1.tuwien.ac.at From: @auniw, @eigvs4:in%72060.2420@compuserve.com Subject: Radiosity history Date: Fri, 23 Sep 1994 18:19:45 +0200 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Received: from HOSTESS.GRAPHICS.CS.CMU.EDU by Pap.UniVie.AC.AT (PMDF #12401) id <01HHGLXJ1VIOA4MJI6@Pap.UniVie.AC.AT>; Fri, 23 Sep 1994 18:17 GMT+0100 Received: from RI.CMU.EDU by HOSTESS.GRAPHICS.CS.CMU.EDU id aa27670; 23 Sep 94 12:10:45 EDT Received: from arl-img-2.compuserve.com by RI.CMU.EDU id aa07133; 23 Sep 94 12:10:08 EDT Received: from localhost by arl-img-2.compuserve.com (8.6.4/5.940406sam) id MAA21353; Fri, 23 Sep 1994 12:10:04 -0400 Date: 23 Sep 94 12:05:56 EDT From: Ian Ashdown <72060.2420@compuserve.com> Subject: Radiosity history To: Global Illumination Message-id: <940923160556_72060.2420_FHG49-1@CompuServe.COM> Paul Heckbert asked me to forward this bit of radiosity history and personal flaming on my part to globillum. It provides evidence that we are not the first to travel this way ... >> I never did find a copy of Moon and Spencer's 1948 "Lighting Design," >> which has the first-ever examples of synthetic images created using >> radiosity techniques. > That's a great bit of trivia that I never heard before! Please share > that with the globillum mailing list! Actually, I included it as an anecdote in an upcoming article entitled "Radiosity Online: A Bibliography" that is scheduled to be published in the next issue of Computer Graphics. I also discuss it briefly in my forthcoming book. Neither discussion, however, gives all the details. For the record, then: The Illuminating Engineering Society of North America has had a long tradition of publishing the best papers from its annual conferences in the Journal of the IES (formerly "Illuminating Engineering"). While most of these papers hold little interest these days, there are still a few gems awaiting rediscovery. One of these papers is: O'Brien, P. F. and J. A. Howard 1959. "Predetermination of Luminances by Finite Difference Equations," Illuminating Engineering 14(4):209- 218 (April). whose abstract reads: Luminous flux transfer in an enclosure may be described by a system of linear simultaneous equations which are a finite difference representation of the Fredholm integral equation. Many techniques of numerical analysis, including analogue and digital computers, are applicable to the solution of these equations. The development of this method for the analysis and synthesis of lighting systems is now being prosecuted actively on a world-wide basis. Truncation errors, an inherent feature of the finite difference equations, can be reduced to acceptable levels. Additional numerical methods need to be explored for applicability to the analysis of lighting systems. The paper is interesting in its own right as an early investigation of the radiosity method. The references, however, are even more interesting. The authors note, for example, that the radiosity equation (which they refer to as simply "the fundamental equation of radiant flux transfer") was first presented by Ziro Yamauti in 1926 and H. Buckley in 1927. There are also interesting papers such as: Centeno, M. and A. Zagustin 1953. "Interflectance in Two Dimensions," Universidad Central de Venezula, Caracas. Radiosity in flatland, perhaps? Perhaps the best part of O'Brien and Howard's paper, however, is the ensuing discussion. The IESNA has had an equally long tradition of publishing the discussions and questions from the floor that follow a paper's presentation. These discussions are sometimes more valuable than the paper itself. For example, Dr. Domina Eberle Spencer had this to say about O'Brien and Howard's paper: The names of O'Brien and Howard are comparatively new to the IES. Their contribution in applying the analogue method to a solution of the basic integral equations of interflection theory by use of the finite difference approach is valuable. However, perhaps due to their comparatively brief association with the Society, they have fallen into several conceptual errors. They say that the "numerical method ... has been developed in the lighting literature only recently." May I remind the authors that nearly thirty years ago Moore and Manning and White were applying such methods to just such problems, and in 1934, the finite difference or numerical approach to the interflection problem was treated in Professor Higbie's excellent book. The new thing about the numerical method is not the method, but the proficiency with which it has recently been applied. The authors also suggests that synthesis of a lighting system is a new idea. The word "synthesis" as applied to illuminating engineering is perhaps new, but the procedure is not. The first application that Professor Moon and I made of the interflection method was to finding what methods could be used to synthesize the optimum lighting environment. We found that for nearly all shapes of rooms, the best way to satisfy the 3:1 adaptation brightness ratio was to make the entire ceiling a source of light. This, as far as we are concerned, was the beginning of luminous ceilings. The practical development of luminous ceilings has merely been a long struggle to realize the synthetic photographs which were exhibited by Professor Moon and myself at the 1946 National Technical Conference. Subsequently, we wrote an entire book on the subject, which the authors cite in their references. Dr. Spencer continues on, ending with: ... If the authors undertake the very commendable task of solving interflection problems with semi-specular surfaces or containing fog, they would do well to think enough about photometric concepts to understand the difference between the visually meaningful concept of brightness and the visually meaningless concept of emittance. The radiosity equation and Fredholm integrals of the second kind in 1926, synthetic photographs in 1946, semispecular surfaces and participating media in 1959 ... we should heed Dr. Spencer's admonishment to O'Brien and Howard that "... they have fallen into several conceptual errors." Until we conduct a thorough investigation of the illumination engineering literature, we should be careful about saying who developed what! Even better, we may discover long-forgotten ideas that are practical with the aid of modern "analogue and digital computers." I had the pleasure of meeting Dr. Spencer at the 1993 IESNA Annual Conference in Houston, Texas. She told me how she and Dr. Parry Moon created their synthetic photographs. In the absence of computers, they calculated the form factor and luminance of each patch by hand, cut out paper squares from Munsell color charts and pasted them together to form their images, which were then photographed. These photographs were reproduced in: Moon, P. and D. E. Spencer 1948. Lighting Design, Addison-Wesley, Cambridge, MA. The framed originals, Dr. Spencer told me, still hang in her office at the Department of Mathematics, University of Conneticut. In these days of instant communications via the Internet (hah!), we tend to forget that there remains an astounding amount of information and ideas available only on paper. More often than not, this information is held in storage by a few university libraries as back issues of obscure journals. This is *not good*. For those convinced that radiosity research began in 1984, consider this isolated quote from a paper written in 1943: The result is an application of the Hilbert-Schmidt theory of integral equations, which leads to the interesting conclusion that the [radiosity equation] kernel has an infinite number of eigenvalues, associated with which is one eigenfunction in the form of a hyperbolic cosine and a set of trigonmetric eigenfunctions. The solution of the inhomogeneous equation is written by means of Schmidt's formula, and it is found that for engineering purposes all the terms but the first can be neglected. The paper in question is: Moon, P. 1943. "New Methods of Calculating Illumination," Journal of the Optical Society of America 33(2):115-122 (February) where the above is added almost as an afterthought. (Does anyone know what this means?) There are no less than 48 references, of which only one is familiar -- Lambert's seminal treatise on photometry from 1760! Consider also that the Russian Academy of Sciences has been publishing important treatises on photometry and radiometry -- in Russian -- for over a century. I think we have a lot of reading to do ... Ian Ashdown, P. Eng. Research and Development Manager Ledalite Architectural Products 9087A - 198th Street Langley, B.C., Canada V3A 4P8 *** That's me -- radiosity's self-appointed gadfly! *** From X-POP3-Rcpt: wp@stellaris Received: from email.tuwien.ac.at by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for wp id AA28754; Fri, 23 Sep 94 19:43:16 +0200 Message-Id: <9409231743.AA28754@stellaris.cg.tuwien.ac.at> Received: from EIGVS4 by email.tuwien.ac.at with DECNET-IN (PP) id <16740-0@email.tuwien.ac.at>; Fri, 23 Sep 1994 19:43:38 +0200 X-Vms-To: IN%"nic@informatik.uni-rostock.de" "Nico Guenther" To: wp@eigsg1.tuwien.ac.at From: @auniw, @eigvs4:in%fournier@cs.ubc.ca Subject: A remark on LAMBERT's law Date: Fri, 23 Sep 1994 19:43:38 +0200 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Received: from HOSTESS.GRAPHICS.CS.CMU.EDU by Pap.UniVie.AC.AT (PMDF #12401) id <01HHGOWP0YPCA4MJHX@Pap.UniVie.AC.AT>; Fri, 23 Sep 1994 19:42 GMT+0100 Received: from CS.CMU.EDU by HOSTESS.GRAPHICS.CS.CMU.EDU id aa28069; 23 Sep 94 13:34:42 EDT Received: from grolsch-2.cs.ubc.ca by CS.CMU.EDU id aa07766; 23 Sep 94 13:31:10 EDT Received: (from ean@localhost) by grolsch.cs.ubc.ca (8.6.9/8.6.9) id KAA13051 for globillum@cs.cmu.edu; Fri, 23 Sep 1994 10:31:05 -0700 Date: Fri, 23 Sep 1994 10:31:00 UTC-0700 From: Alain Fournier Subject: A remark on LAMBERT's law In-reply-to: <199409050732.JAA02532@anne.informatik.uni-rostock.de> To: Nico Guenther Cc: return Message-id: <"3590*fournier@cs.ubc.ca"@MHS> Content-identifier: 3590 X400-content-type: P2-1984 (2) X400-MTS-identifier: [/PRMD=ca/ADMD=telecom.canada/C=ca/;940923103100] X400-received: by mta cs.ubc.ca in /PRMD=/ADMD=/C=/; Relayed; Fri, 23 Sep 1994 10:31:00 UTC-0700 X400-received: by /PRMD=ca/ADMD=telecom.canada/C=ca/; Relayed; Fri, 23 Sep 1994 10:31:00 UTC-0700 X400-recipients: non-disclosure:; X400-Originator: fournier@cs.ubc.ca MIME-Version: 1.0 (Generated by Ean X.400 to MIME gateway) I think we have a semantic problem here. A law (like Lambert's Law, or the ideal gas law, for example) only applies to whatever obeys it. If it looks like a tautology, it is because it is one. An ideal gas IS a gas which obeys the ideal gas law, a diffuse reflector IS a reflector which obeys Lambert's law (at least according to most optics text, see eg Born & Wolf), and therefore one should not speak of a "non-Lambertian diffuse reflector", unless one redefines what "diffuse" means, or (worse) rewrite Lambert's law but keeps the same name. From X-POP3-Rcpt: wp@stellaris Received: from email.tuwien.ac.at by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for wp id AA00329; Sat, 24 Sep 94 22:06:26 +0200 Message-Id: <9409242006.AA00329@stellaris.cg.tuwien.ac.at> Received: from EIGVS4 by email.tuwien.ac.at with DECNET-IN (PP) id <05696-0@email.tuwien.ac.at>; Sat, 24 Sep 1994 22:06:49 +0200 X-Vms-To: IN%"globillum@cs.cmu.edu" To: wp@eigsg1.tuwien.ac.at From: @auniw, @eigvs4:in%dilaura@bechtel.colorado.edu Subject: "Radiosity History" Date: Sat, 24 Sep 1994 22:06:49 +0200 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Received: from HOSTESS.GRAPHICS.CS.CMU.EDU by Pap.UniVie.AC.AT (PMDF #12401) id <01HHI87QD6WGA4MKON@Pap.UniVie.AC.AT>; Sat, 24 Sep 1994 22:05 GMT+0100 Received: from CS.CMU.EDU by HOSTESS.GRAPHICS.CS.CMU.EDU id aa29523; 24 Sep 94 16:01:12 EDT Received: from bechtel.Colorado.EDU by CS.CMU.EDU id aa13792; 24 Sep 94 16:00:47 EDT Received: from localhost.Colorado.EDU (dilaura@localhost.Colorado.EDU [127.0.0.1]) by bechtel.Colorado.EDU (8.6.9/8.6.9/UnixOps) with SMTP id OAA25627 for ; Sat, 24 Sep 1994 14:00:44 -0600 Date: Sat, 24 Sep 94 14:00:44 -0600 From: dilaura@bechtel.Colorado.EDU Subject: "Radiosity History" To: globillum@cs.cmu.edu Message-id: <199409242000.OAA25627@bechtel.Colorado.EDU> X-Authentication-Warning: bechtel.Colorado.EDU: Host localhost.Colorado.EDU didn't use HELO protocol Ian Ashdown has sent me a copy of his note (broadcast on globillum) concerning the history of radiative transfer applied to illuminating engineering. I might add the following. 1) Moon and Spenser book "Lighting Design" is a rarity but is availble from University Microfilms International, Zeeb Road, Ann Arbor, MI. I got my copy of "Lighting Design" from UMI, and although it is a xerox copy of the original it is quite serviceable. 2) A study of this book, and papers that Moon and Spencer published in The Franklin Journal, shows that their approach was to approximate the kernal that resulted from a statement, in integral equation form, of the radiative transfer problem. They didn't like, nor use, the finite element method applied to this problem. 3) The first extensive use of the finite element method to the radiatvie transfer problem in lighting was, indeed, O'Brien. He wrote of it as the "network" method, lifting an analogy from circuits. His work first appeared in CIE publications and in JOSA in the early 1950's. 4) To be blunt, many of us in the lighting engineering industry wondered what all the fuss was about when the computer graphics community started talking about "radiosity". This (silly) word is superfluous, since there has long been international agreement about terms needed in radiometric and photometric work. The ISO has the (individual governments' ceded) authority to establish such vocabulary. It looks to the CIE (international lighting commission) to do this. The latest edition of the International Lighting Vocabulary is now available. Folks at NIST know how to get ahold of it. 5) The finite element formulation of the raditive transfer problem has been used by lighting engineers for almost 50 years to solve the practical engineering problems that they have faced: typically and commonly to predict the average illuminance a lighting system produces in a room; less typically and only recently more common, to predict the illuminance a lighting system produces at a point in a room. This formulation has been used to design a lighting system, i.e. synthesize, not just to analyze. The advent of the PC produced early versions of software that increased the number of elements so that reasonably useful "synthetic pictures" could be produced. The method wasn't changed, just the size of the problem. This took place in 1982. 6) Concern with the (recent) history of technology is perhaps the fooling away of time by scholars. Perhaps. This point of view might be supported by G. Ward's recent musings about why isn't anyone really using "radiosity". For any one that really needs pictures (to show a client, to solve a lighting problem, and in general to reduce uncertainty) which are photo- graphic in their realism and accurate in their numbers, program like Radiance appear to by the industry's choice. If such pictures aren't needed, then other software IS used by the industry, and it is based on radiative transfer. So knowing our history might just be a (small) part of knowing our discipline well; and as Ian suggested might hold information and techniques that may have a new life on modern computing hardware. David L. DiLaura Senior Instructor - Civil and Architectural Engineering Assoc. Dean for Undergraduate Academic Affiars University of Colorado Boulder, CO 80309 dilaura@bechtel.colorado.edu From X-POP3-Rcpt: wp@stellaris Received: from email.tuwien.ac.at by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for wp id AA01174; Sun, 25 Sep 94 17:49:31 +0200 Message-Id: <9409251549.AA01174@stellaris.cg.tuwien.ac.at> Received: from EIGVS4 by email.tuwien.ac.at with DECNET-IN (PP) id <17929-0@email.tuwien.ac.at>; Sun, 25 Sep 1994 17:50:13 +0100 X-Vms-To: IN%"globillum@cs.cmu.edu" To: wp@eigsg1.tuwien.ac.at From: @auniw, @eigvs4:in%dilaura@bechtel.colorado.edu Subject: Post Script Date: Sun, 25 Sep 1994 17:50:13 +0100 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Received: from HOSTESS.GRAPHICS.CS.CMU.EDU by Pap.UniVie.AC.AT (PMDF #12401) id <01HHJDJ0N1E8A4ML70@Pap.UniVie.AC.AT>; Sun, 25 Sep 1994 17:49 GMT+0100 Received: from RI.CMU.EDU by HOSTESS.GRAPHICS.CS.CMU.EDU id aa00628; 25 Sep 94 12:45:23 EDT Received: from bechtel.Colorado.EDU by RI.CMU.EDU id aa12991; 25 Sep 94 12:44:43 EDT Received: from localhost.Colorado.EDU (dilaura@localhost.Colorado.EDU [127.0.0.1]) by bechtel.Colorado.EDU (8.6.9/8.6.9/UnixOps) with SMTP id KAA00468 for ; Sun, 25 Sep 1994 10:44:41 -0600 Date: Sun, 25 Sep 94 10:44:41 -0600 From: dilaura@bechtel.Colorado.EDU Subject: Post Script To: globillum@cs.cmu.edu Message-id: <199409251644.KAA00468@bechtel.Colorado.EDU> X-Authentication-Warning: bechtel.Colorado.EDU: Host localhost.Colorado.EDU didn't use HELO protocol P.S. I believe the deepest thinker (not tinkerer) in radiative transfer was Rudolf Preisendorfer. His book "Radiative Transfer on Discrete Spaces" is difficult, profound and insightful. His formalisms establish an approach to practical problems that put our work on firm mathematical and physical ground. It was published by Pergamon Press; now out of print, but available from UMI. Rudy started this work back in the 1950's when he was wrestling with the radiative transfer problems that arise in predicting light levels, contrasts, and visibilities under water. He was a Scripps for a very long time. Highly recommended. D. DiLaura From X-POP3-Rcpt: wp@stellaris Received: from email.tuwien.ac.at by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for wp id AA19338; Sat, 8 Oct 94 01:17:34 +0100 Message-Id: <9410080017.AA19338@stellaris.cg.tuwien.ac.at> Received: from EIGVS4 by email.tuwien.ac.at with DECNET-IN (PP) id <10975-0@email.tuwien.ac.at>; Sat, 8 Oct 1994 01:18:29 +0100 X-Vms-To: IN%"globillum@cs.cmu.edu" To: wp@eigsg1.tuwien.ac.at From: @auniw, @eigvs4:in%epabuice@bi.ehu.es Date: Sat, 8 Oct 1994 01:18:29 +0100 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Received: from HOSTESS.GRAPHICS.CS.CMU.EDU by Pap.UniVie.AC.AT (PMDF #12401) id <01HI0KP2RWDSA4LUZU@Pap.UniVie.AC.AT>; Sat, 8 Oct 1994 01:17 GMT+0100 Received: from EDRC.CMU.EDU by HOSTESS.GRAPHICS.CS.CMU.EDU id aa06227; 7 Oct 94 20:11:31 EDT Received: from s835cc.bi.ehu.es by EDRC.CMU.EDU id aa07514; 7 Oct 94 20:11:09 EDT Received: by s835cc.bi.ehu.es (1.37.109.4/15.6) id AA23596; Sat, 8 Oct 94 00:39:22 +0100 Date: Sat, 8 Oct 94 00:39:22 +0100 From: Eduardo Bustillo Iceta To: globillum@cs.cmu.edu Message-id: <01HI0KP2RWDSA4LUZU@Pap.UniVie.AC.AT> Subject: New free radiosity program I'm a recently graduated mechanical engineering student from Spain. As part of my end of studies project I have developed a radiosity program with the following main characteristics: -Monte Carlo integration to compute diffuse illumination: This permits to have refracted shadows, specular and diffuse reflections, blurry reflections, translucency, texture mapping and any geometry of light sources. -Adaptive subdivision: Objects with big radiosity gradients inside are dynamically subdivided during the radiosity process. -Ray tracing: A postprocess of ray tracing is used to calculate the image. The main characteristics of the algorithm used are: -Depth of field. -Stochastic anti-aliasing. -Optional 3D glasses stereo view. -Acceleration techniques: Three different user selectable techniques are incorporated: -Binary Object Partitioning -Adaptive voxel subdivision (with optimal coordinate system selection) -Z-Buffer for first ray acceleration -Geometry input: It reads 3D Studio v2 geometry files so the only geometric entity supported is the triangle. -Completely written in ANSI C: This way it may be compiled in any system. Actually, my work was done in a PC but I've tried and succeeded in compiling it with no modifications on a DEC OSF/1 and a HP-UX server. If anyone wants a copy of my program (it's free), please feel free to contact me. I am also planning to go to the US in November for about three months. The objective of my visit is to improve my english though I would like to do something interesting at the same time. If anyone knows some interesting seminar or someone who could give me a job related to 3D computer graphics (I'd work for free, of course), I would appreciate very much the information. Eduardo Bustillo Iceta Particular de Basterra 1 48990 Getxo (VIZCAYA) SPAIN Internet address: epabuice@s835cc.bi.ehu.es From X-POP3-Rcpt: wp@stellaris Received: from email.tuwien.ac.at by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for wp id AA07763; Thu, 3 Nov 94 18:23:25 +0100 Message-Id: <9411031723.AA07763@stellaris.cg.tuwien.ac.at> Received: from EIGVS4 by email.tuwien.ac.at with DECNET-IN (PP) id <26211-0@email.tuwien.ac.at>; Thu, 3 Nov 1994 18:23:41 +0100 X-Vms-To: IN%"globillum@cs.cmu.edu" To: wp@eigsg1.tuwien.ac.at From: @auniw, @eigvs4:in%barbara.pela@cen.jrc.it Subject: old papers by Fock and Yamauti Date: Thu, 3 Nov 1994 18:23:41 +0100 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Received: from HOSTESS.GRAPHICS.CS.CMU.EDU by Pap.UniVie.AC.AT (PMDF #12401) id <01HJ1W3GYOJK9BWLMR@Pap.UniVie.AC.AT>; Thu, 3 Nov 1994 18:22 GMT+0100 Received: from CS.CMU.EDU by HOSTESS.GRAPHICS.CS.CMU.EDU id aa14430; 3 Nov 94 11:28:02 EST Received: from dicscs1.jrc.it by CS.CMU.EDU id aa14920; 3 Nov 94 11:26:19 EST Received: from cen.jrc.it (relay.jrc.it) by cen.jrc.it (4.1/SMI-4.1) id AA05851; Thu, 3 Nov 94 17:24:07 +0100 Received: from dpx2.isei.jrc.it by cen.jrc.it; Thu, 3 Nov 94 17:26:40 +0100 Received: by dpx2.isei.jrc.it; Thu, 3 Nov 94 17:34:49 +0100 (MET) Date: Thu, 3 Nov 94 17:34:49 +0100 From: barbara pela Subject: old papers by Fock and Yamauti To: globillum@cs.cmu.edu Reply-to: barbara pela Message-id: <9411031634.AA06880@dpx2.isei.jrc.it> Hello, Does anyone have a copy of these old papers? Are they in english? %0 Journal Article %A Fock, V.A. %D 1924 %T The Illumination from Surfaces of Arbitrary Shape %B Transactions of the Optical Institute, Leningrad %V 28 %P 1-11 %J Transactions of the Optical Institute, Leningrad %K illuminance, Stoke's theorem %O analytic illuminance determination using Stoke's theorem (historical interest) %0 Report %A Yamauti, Ziro %D 1932 %T Theory of Field of Illumination %I Researches of the Electrotechnical Laboratory, Ministry of Communications %@ 339 %K vector flux, light fields Barbara. From X-POP3-Rcpt: wp@stellaris Received: from email.tuwien.ac.at by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for wp id AA08162; Thu, 3 Nov 94 20:06:55 +0100 Message-Id: <9411031906.AA08162@stellaris.cg.tuwien.ac.at> Received: from EIGVS4 by email.tuwien.ac.at with DECNET-IN (PP) id <29714-0@email.tuwien.ac.at>; Thu, 3 Nov 1994 20:07:10 +0100 X-Vms-To: IN%"barbara.pela@cen.jrc.it" To: wp@eigsg1.tuwien.ac.at From: @auniw, @eigvs4:in%ps@math.scarolina.edu Subject: old papers by Fock and Yamauti Date: Thu, 3 Nov 1994 20:07:10 +0100 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Received: from HOSTESS.GRAPHICS.CS.CMU.EDU by Pap.UniVie.AC.AT (PMDF #12401) id <01HJ1ZORMR9C9BWLYA@Pap.UniVie.AC.AT>; Thu, 3 Nov 1994 20:06 GMT+0100 Received: from CS.CMU.EDU by HOSTESS.GRAPHICS.CS.CMU.EDU id aa14824; 3 Nov 94 13:46:17 EST Received: from milo.math.scarolina.edu by CS.CMU.EDU id aa16210; 3 Nov 94 13:45:28 EST Received: by milo.math.scarolina.edu (4.1/6.0s-FWP); id AA01212; Thu, 3 Nov 94 13:44:59 EST Date: Thu, 3 Nov 94 13:44:59 EST From: Peter Schroder Subject: old papers by Fock and Yamauti In-reply-to: barbara pela's message of Thu, 3 Nov 94 17:34:49 +0100 <9411031634.AA06880@dpx2.isei.jrc.it> To: barbara.pela@cen.jrc.it Cc: globillum@cs.cmu.edu Message-id: <9411031844.AA01212@milo.math.scarolina.edu> Date: Thu, 3 Nov 94 17:34:49 +0100 From: barbara pela %0 Journal Article %A Fock, V.A. %D 1924 %T The Illumination from Surfaces of Arbitrary Shape %B Transactions of the Optical Institute, Leningrad %V 28 %P 1-11 %J Transactions of the Optical Institute, Leningrad %K illuminance, Stoke's theorem %O analytic illuminance determination using Stokes' theorem (historical interest) This one's in russian. It derives the double application of Stokes' theorem to the illumination kernel (note that this is not the first time [or the last] that this double contour form was derived). There appears to be a German translation of this which appeared in the same year. I say `appears' since I can't read the russian (but can read the German), but from the looks of the formulas and the figures it seems to treat the same material: @Article{fock24, author = "V. A. Fock", title = "Zur Berechnung der Beleuchtungsst{\"a}rke", journal = "Zeitschrift f{\"u}r Physik", year = "1924", volume = "28", OPTnumber = "", pages = "102--113", month = "September/October", OPTnote = "" } The earliest reference I know of with regards to the double contour integration trick is given in a textbook(!) from 1900: @Book{herman, author = "Robert Alfred Herman", title = "A Treatise on Geometrical Optics", publisher = "Cambridge University Press", year = "1900", OPTeditor = "", OPTvolume = "", OPTseries = "", OPTaddress = "", OPTedition = "", OPTmonth = "", OPTnote = "" } In fact he gives as a homework exercise a computation which has been published many years later as a unique new derivation... He simply derives this form without any reference. From the treatment it sounds like he considers it so self evident that he sees no need to give a reference. Might that mean there are even earlier references to the double contour form? I don't know, but I'd love to know. Herman also gives a most magnificent form for the integral which I haven't seen anyone use (yes, Michael, you still owe me a buck for loosing a bet on this :-)): [...] Herman gives the following form in Exercise 15, Chaper IX of his book Geometrical Optics (1900) \begin{eqnarray*} \int_{\partial{A}_1} \int_{\partial{A}_2} \cos \theta_1 \cos \theta_2 \,\, dx_2\, dx_1 & = & \int_{\partial{A}_1} \int_{\partial{A}_2} -\frac{(\vec{r}\cdot d\vec{x}_1)(\vec{r} \cdot d\vec{x}_2)} {\r^2} \end{eqnarray*} [...] A most amazing little gem. It does not become infinite and is much better behaved numerically (well, almost, it's derivative becomes infinite for r->0). Still a remarkable form. Not to mention the derivation of which is a most enjoyable exercise for the interested reader. :-) [hint: change the second application of Stokes' theorem.] Peter From X-POP3-Rcpt: wp@stellaris Received: from email.tuwien.ac.at by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for wp id AA08682; Thu, 3 Nov 94 23:39:57 +0100 Message-Id: <9411032239.AA08682@stellaris.cg.tuwien.ac.at> Received: from EIGVS4 by email.tuwien.ac.at with DECNET-IN (PP) id <05711-0@email.tuwien.ac.at>; Thu, 3 Nov 1994 23:40:21 +0100 X-Vms-To: IN%"globillum@cs.cmu.edu" To: wp@eigsg1.tuwien.ac.at From: @auniw, @eigvs4:in%dilaura@bechtel.colorado.edu Subject: Contour Integration Date: Thu, 3 Nov 1994 23:40:21 +0100 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Received: from HOSTESS.GRAPHICS.CS.CMU.EDU by Pap.UniVie.AC.AT (PMDF #12401) id <01HJ2755BG0G9BWLZB@Pap.UniVie.AC.AT>; Thu, 3 Nov 1994 23:39 GMT+0100 Received: from EDRC.CMU.EDU by HOSTESS.GRAPHICS.CS.CMU.EDU id aa15587; 3 Nov 94 17:28:11 EST Received: from bechtel.Colorado.EDU by EDRC.CMU.EDU id aa01995; 3 Nov 94 17:27:50 EST Received: from localhost.Colorado.EDU (dilaura@localhost.Colorado.EDU [127.0.0.1]) by bechtel.Colorado.EDU (8.6.9/8.6.9/UnixOps) with SMTP id PAA05549 for ; Thu, 3 Nov 1994 15:27:45 -0700 Date: Thu, 03 Nov 94 15:27:43 -0700 From: dilaura@bechtel.Colorado.EDU Subject: Contour Integration To: globillum@cs.cmu.edu Message-id: <199411032227.PAA05549@bechtel.Colorado.EDU> X-Authentication-Warning: bechtel.Colorado.EDU: Host localhost.Colorado.EDU didn't use HELO protocol Colleagues: At the risk of appearing vain, and prompted by barbara's recent request for copies of old papers by Fock and Yamaouti, may I announce that this important method has recently been applied to non-diffuse sources? I and a recent graduate student of mine presented a paper at the Illuminating Engineering Society conference in Miami Florida this past August, describing our results. We showed the process for replacing the area integral over a homogenous source (homogeneous, not diffuse) with a contour integral over its edges. I have recently worked through the details of extending this to the problem of replacing the double area integrals with double contour integrals for non-diffuse sources. In practical terms, this permits very rapid calculation of illuminances from real area sources, such as architectural luminaires. The IES papers shows that the computer time investment for the new contour integral method is approximatley 10-15 times less than the (usual) current process of discritizing an area source and applying the so-called inverse square cosine law to calculate the illuminances. The double contour integration for non-diffuse sources apparently allows the determination of non-diffuse form factors. It isn't clear yet what value this will have. I do think it will lead to cleaner and much faster approach to the non-diffuse radiative tranfer problem between surfaces. David L. DiLaura, FIEs Senior Instructor Civil and Architectural Engineering Dept. Univeristy of Colorado Boulder, CO 80309 (303) 492 4168 (voice) (303) 492 7317 (fax) From X-POP3-Rcpt: wp@stellaris Received: from email.tuwien.ac.at by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for wp id AA09143; Fri, 4 Nov 94 03:43:46 +0100 Message-Id: <9411040243.AA09143@stellaris.cg.tuwien.ac.at> Received: from EIGVS4 by email.tuwien.ac.at with DECNET-IN (PP) id <11054-0@email.tuwien.ac.at>; Fri, 4 Nov 1994 03:44:06 +0100 X-Vms-To: IN%"barbara.pela@cen.jrc.it" To: wp@eigsg1.tuwien.ac.at From: @auniw, @eigvs4:in%shinya@nttarm.ntt.jp Subject: RE: old papers by Fock and Yamauti Date: Fri, 4 Nov 1994 03:44:06 +0100 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Return-path: shinya@nttarm.ntt.JP Received: from HOSTESS.GRAPHICS.CS.CMU.EDU by Pap.UniVie.AC.AT (PMDF #12401) id <01HJ2FNAI6CW9BWMRN@Pap.UniVie.AC.AT>; Fri, 4 Nov 1994 03:43 GMT+0100 Received: from CS.CMU.EDU by HOSTESS.GRAPHICS.CS.CMU.EDU id aa15834; 3 Nov 94 21:32:53 EST Received: from tama.TAS.NTT.JP by CS.CMU.EDU id aa19725; 3 Nov 94 21:32:01 EST Received: by tama.tas.ntt.jp (4.1/tas-sh-01) with TCP; Fri, 4 Nov 94 11:31:47 JST Received: by nttmail.tas.ntt.jp (4.1/nttmail-01) with TCP; Fri, 4 Nov 94 11:31:43 JST Received: by mecl-sh.ntt.jp (4.1/MECLSH01) with TCP; Fri, 4 Nov 94 11:31:42 JST Received: by nttarm.ntt.jp (4.1/NTTcs01b) with TCP; Fri, 4 Nov 94 11:32:49 JST Date: Fri, 4 Nov 94 11:28:23 JST From: Mikio Shinya Subject: RE: old papers by Fock and Yamauti To: barbara.pela@cen.jrc.it Cc: globillum@cs.cmu.edu Message-id: <9411040232.AA08521@nttarm.ntt.jp> %0 Report %A Yamauti, Ziro %D 1932 %T Theory of Field of Illumination %I Researches of the Electrotechnical Laboratory, Ministry of Communications %@ 339 %K vector flux, light fields I found Yamauchi's paper in the Library. (BTW, the Electrotechnical Laboratory is the root of NTT laboratories). Here's the abstract: The theorie of the illumination field are treated mathematically by using the method of vector analysis. There is proposed the ``illumination vector'' to be distinguished from the field intensity which is the vector generally used. The field due to a luminous source of various emissive nature is treated in the first place and the various principal theorems to calculate the illumination are included and rearranged systematically, which have been heretofore by various authorities and the author. The field in the system of interreflecting surfaces is discussed in the second place. The fundamental integral equations are shown when the surfaces in the system are of both diffused reflection and transmission. Mikio Shinya NTT Human Interface Laboratories shinya@nttarm.ntt.jp From X-POP3-Rcpt: wp@stellaris Received: from email.tuwien.ac.at by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for wp id AA16761; Fri, 11 Nov 94 17:37:02 +0100 Message-Id: <9411111637.AA16761@stellaris.cg.tuwien.ac.at> Received: from EIGVS4 by email.tuwien.ac.at with DECNET-IN (PP) id <14183-0@email.tuwien.ac.at>; Fri, 11 Nov 1994 17:37:17 +0100 X-Vms-To: IN%"globillum@cs.cmu.edu" To: wp@eigsg1.tuwien.ac.at From: @auniw, eigvs4!relay.nl.net!in%ossfs1!mv Subject: PRESS RELEASE "IMAGINE", the Fastest Graphics and Imaging Processor Ever !!! (fwd) Date: Fri, 11 Nov 1994 17:37:17 +0100 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Received: from HOSTESS.GRAPHICS.CS.CMU.EDU by Pap.UniVie.AC.AT (PMDF #12401) id <01HJD0S3YJUO9BX4CB@Pap.UniVie.AC.AT>; Fri, 11 Nov 1994 17:36 GMT+0100 Received: from EDRC.CMU.EDU by HOSTESS.GRAPHICS.CS.CMU.EDU id aa02767; 11 Nov 94 11:22:48 EST Received: from sun4nl.NL.net by EDRC.CMU.EDU id aa01673; 11 Nov 94 11:21:10 EST Received: from ossfs1 by sun4nl.NL.net via EUnet id AA18004 (5.65b/CWI-3.3); Fri, 11 Nov 1994 17:20:50 +0100 Received: by ossfs1.arcobel.nl (4.1/SMI-4.1) id AA08026; Fri, 11 Nov 94 17:13:28 +0100 Date: Fri, 11 Nov 1994 17:13:28 +0100 (MET) From: Martin Verbruggen Arcobel Subject: PRESS RELEASE "IMAGINE", the Fastest Graphics and Imaging Processor Ever !!! (fwd) To: globillum@cs.cmu.edu Message-id: <9411111613.AA08026@ossfs1.arcobel.nl> Content-type: text/plain; charset=US-ASCII Content-transfer-encoding: 7bit X-Mailer: ELM [version 2.4 PL22] Mime-Version: 1.0 Content-Length: 3465 Hi everyone, I thought you may be interested in the following press release. The products described are available and very interesting. May be it is usefull in your developments. PRESS RELEASE Imagine, the fastest graphics and imaging processor ever Today's fastest pixel processor is a Dutch product. In fact that is what Arcobel Graphics' designers claim. At a clock frequency of up to 67 MHz their Imagine realises a peak of 330 Mips at 32-bit operations, but it can also use the same hardware to crunch 8-bit data achieving a speed of 8000 Mips. Thus the Imagine places all comparable special purpose and RISC processors in its shadow. The processor's innovative concept is based on the principle of flexible usage of available hardware, which means that this chip has a substantial advantage over its competitors. Imagine combines the best of two world: the flexibility of general purpose processors and the speed of dedicated pixel-processing hardware. The Arcobel design-team has achieved this by implementing a set of well chosen design principles. Most noticeable are the 'word length partitioning', the 'heteroge- nous partitioning' (super scalar) and 'vector/stream proces- sing'. The Imagine processor accommodates eight simultaneously executing dataprocessing units and eight internal databuses for the interconnection. Each functional unit in the chip can operate on 32-bit words, two 16-bit words or four 8-bit words in parallel. Arcobel managed to implement these principles whilst remaining compatible with RISC and CISC concepts. Thus the Imagine can be programmed as a normal processor using the C and C++ language. This programming level however is the top layer in a hierarchy of programming levels provided by the Imagine. Other levels according to Arcobel's Hierarchical Instruction Set Computer (HISC) model provide the instruction sets to write optimal code using the variable word length, super scalar and vector processing principles. Besides the realisation of the desired speed and flexibility of programming, the Imagine design proves to be very efficient in terms of basic hardware elements: Imagine contains 650,000 transistors, which is only ca. 20% of the transistor count of other modern processors. This ensures a growth path to successor chips without having to wait for new silicon technologies to become available. The Imagine design is also available as an ASIC core to create custom versions integra- ting e.g. other functions in order to decrease board component count. A full software development environment including C-compiler and Simulator/Debugger and imaging library is available with the chip. Also available from Arcobel Graphics is an S-VGA compatible Imagine PC card. As examples of applications are to be mentioned graphic workstations, Desk Top Publishing systems, colour laserprin- ters, Digital Signal Processing systems and image recognition. In multi-processor configurations applications are: top end 3D graphics systems, Interactive MultiMedia authoring systems, flight simulators and the like. Although the Imagine pixel-processing performance is on a much higher level than is the case with other processors, the Imagine will not be more expensive than a high end RISC processor. For further information please contact: Sjef ten Den Arcobel Graphics B.V. P.O. Box 3523 5203 DM 's-Hertogenbosch The Netherlands Tel +31-73444144 Fax +31-73444150 Internet: std@arcobel.nl From X-POP3-Rcpt: wp@stellaris Received: from mr.tuwien.ac.at by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for wp id AA03045; Sun, 27 Nov 94 23:07:49 +0100 Message-Id: <9411272207.AA03045@stellaris.cg.tuwien.ac.at> Received: from EIGVS4 by mr.tuwien.ac.at with DECNET-IN (PP) id <13644-0@mr.tuwien.ac.at>; Sun, 27 Nov 1994 23:06:56 +0100 X-Vms-To: IN%"globillum@cs.cmu.edu", IN%"grj@physiol.ox.ac.uk" To: wp@eigsg1.tuwien.ac.at From: in%greg%hobbes.lbl.gov%eigvs4@auniw Subject: RE: Material BRDF functions. Date: Sun, 27 Nov 1994 23:06:56 +0100 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Received: from HOSTESS.GRAPHICS.CS.CMU.EDU by Pap.UniVie.AC.AT (PMDF #12401) id <01HJZOZBIE409FMR7I@Pap.UniVie.AC.AT>; Sun, 27 Nov 1994 23:06 GMT+0100 Received: from CS.CMU.EDU by HOSTESS.GRAPHICS.CS.CMU.EDU id aa27180; 27 Nov 94 17:01:41 EST Received: from lbl.gov by CS.CMU.EDU id aa29789; 27 Nov 94 17:00:59 EST Received: from hobbes.lbl.gov by lbl.gov (4.1/1.39) id AA09676; Sun, 27 Nov 94 14:00:50 PST Received: by hobbes.lbl.gov (3.2/SMI-3.2) id AA22591; Sun, 27 Nov 94 13:59:47 PST Date: Sun, 27 Nov 94 13:59:47 PST From: "Gregory J. Ward" Subject: RE: Material BRDF functions. To: globillum@cs.cmu.edu, grj@physiol.ox.ac.uk Message-id: <9411272159.AA22591@hobbes.lbl.gov> I have posted a compressed tar file of BRDF measurements we took with our imaging gonioreflectometer (see Siggraph '92 article for details) on the anonymous ftp account of hobbes.lbl.gov in the /xfer directory. The file is called "brdfs.tar.Z", and make sure to set binary mode before retrieving it. The data format is simple. A short information header describing the material and measurement is followed by 5 columns. The first column is the incident polar angle (measured in degrees from normal). The second column is the incident azimuthal angle (measured in degrees from the predominant axis). The third column is the reflected polar angle and the fourth column is the reflected azimuthal angle. Finally, the fifth column is the BRDF at that point, in steradian^-1. I make no guarantees about this data. In particular, the data is rather noisy and I don't expect it has better than +/-3 degree geometric accuracy or better than +/-5% value accuracy. -Greg From X-POP3-Rcpt: wp@stellaris Received: from mr.tuwien.ac.at by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for wp id AA25192; Wed, 30 Nov 94 18:23:55 +0100 Message-Id: <9411301723.AA25192@stellaris.cg.tuwien.ac.at> Received: from EIGVS4 by mr.tuwien.ac.at with DECNET-IN (PP) id <11310-0@mr.tuwien.ac.at>; Wed, 30 Nov 1994 18:21:34 +0100 X-Vms-To: IN%"globillum@cs.cmu.edu" To: wp@eigsg1.tuwien.ac.at From: in%zzcgung%afs.mcc.ac.uk%eigvs4@auniw Subject: Wavelet radiosity question Date: Wed, 30 Nov 1994 18:21:34 +0100 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Received: from HOSTESS.GRAPHICS.CS.CMU.EDU by Pap.UniVie.AC.AT (PMDF #12401) id <01HK3LVHTME89FMYTH@Pap.UniVie.AC.AT>; Wed, 30 Nov 1994 18:21 GMT+0100 Received: from CS.CMU.EDU by HOSTESS.GRAPHICS.CS.CMU.EDU id aa02213; 30 Nov 94 12:04:28 EST Received: from nessie.mcc.ac.uk by CS.CMU.EDU id aa23842; 30 Nov 94 12:02:20 EST Received: from afs.mcc.ac.uk (actually mcchpc.mcc.ac.uk) by nessie.mcc.ac.uk with SMTP (PP); Wed, 30 Nov 1994 17:00:44 +0000 Date: Wed, 30 Nov 1994 16:59:33 +0000 (GMT) From: zzcgung Subject: Wavelet radiosity question To: globillum@cs.cmu.edu Cc: w.t.hewitt@mcc.ac.uk Message-id: <15322.9411301659@afs.mcc.ac.uk> Content-type: text/plain; charset=US-ASCII Content-transfer-encoding: 7bit X-Mailer: ELM [version 2.4 PL24alpha3] Mime-Version: 1.0 Content-Length: 2563 Hi, I wonder if anyone could answer a couple of questions I have on wavelet radiosity? I sent this off to comp.graphics.algorithms, but have had no response. I would mail the authors direct, but don't have their email addresses .... maybe people here can help? I've been reading Steve Gortler et al's SIGGRAPH 93 paper, and Peter Schr\"{o}der's Eurographics Workshop on Rendering 93 paper. Here is their (flatland) algorithm (everyone know TeX ?): b ~ radiosity, e ~ emitted radiosity, g ~ gathered radiosity, <> ~ inner product, \phi_{i,j}, \psi_{i,j} ~ smooth and detail functions from non-standard wavelet basis Their pseudo-code: 1: = ; 2: K = projectKernel; 3: while ( not converged ) 4: (, ) = Pull(); 5: (, ) = Gather(, , K); 6: = Push (, ); 7: = + ; 8: Display ( ); OK, so this is just repeatedly applying the projected kernel to operate on projected radiosity vector, until convergence. ( b = e + Ke + K^2 e + K^3 e + ............ ) I have two questions: a) why (line 7) do I keep adding the emitted radiosity to my current radiosity estimate, surely this should be: 7: += ; b) why do I have to Push everything to the finest level of the hierarchy before continuing with the next Jacobi iteration? I can see why I have to do this for display, but couldn't this Pull/Push come outside of the loop? I suspect that the answer may be that I can't simply add together coefficients of the functions higher up the basis function hierarchy and get the same answer as adding them together at the finest level (\phi_{L,j}). BUT, I can do this for the Haar basis, so I'm confused - is this just a simple case? question (b) is essentially: is "Push( + , + )" equal to " + " ?????? Any help much appreciated Neil ------------------------------------------------------------------------------- Neil Gatenby, Computer Graphics Unit, Dept of Computer Science, University of Manchester, Oxford Road, Manchester M13 9PL, England Tel:(+44)61 275 6095; Fax:(+44)61 275 6040; Email:n.gatenby@mcc.ac.uk ------------------------------------------------------------------------------- Strive to Survive, Causing Least Suffering Possible.... From X-POP3-Rcpt: wp@stellaris Received: from mr.tuwien.ac.at by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for wp id AA25675; Wed, 30 Nov 94 20:41:56 +0100 Message-Id: <9411301941.AA25675@stellaris.cg.tuwien.ac.at> Received: from EIGVS4 by mr.tuwien.ac.at with DECNET-IN (PP) id <14178-0@mr.tuwien.ac.at>; Wed, 30 Nov 1994 20:39:34 +0100 X-Vms-To: IN%"zzcgung@afs.mcc.ac.uk" To: wp@eigsg1.tuwien.ac.at From: in%ps%math.scarolina.edu%eigvs4@auniw Subject: Wavelet radiosity question Date: Wed, 30 Nov 1994 20:39:34 +0100 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Received: from HOSTESS.GRAPHICS.CS.CMU.EDU by Pap.UniVie.AC.AT (PMDF #12401) id <01HK3QPJOC0G9FMZEA@Pap.UniVie.AC.AT>; Wed, 30 Nov 1994 20:39 GMT+0100 Received: from CS.CMU.EDU by HOSTESS.GRAPHICS.CS.CMU.EDU id aa02408; 30 Nov 94 14:29:04 EST Received: from [129.252.12.2] by CS.CMU.EDU id aa25359; 30 Nov 94 14:25:34 EST Received: by milo.math.scarolina.edu (4.1/6.0s-FWP); id AA24657; Wed, 30 Nov 94 14:22:10 EST Date: Wed, 30 Nov 94 14:22:10 EST From: Peter Schroder Subject: Wavelet radiosity question In-reply-to: zzcgung's message of Wed, 30 Nov 1994 16:59:33 +0000 (GMT) <15322.9411301659@afs.mcc.ac.uk> To: zzcgung@afs.mcc.ac.uk Cc: globillum@cs.cmu.edu, w.t.hewitt@mcc.ac.uk Message-id: <9411301922.AA24657@milo.math.scarolina.edu> From: zzcgung Date: Wed, 30 Nov 1994 16:59:33 +0000 (GMT) 7: = + ; OK, so this is just repeatedly applying the projected kernel to operate on projected radiosity vector, until convergence. ( b = e + Ke + K^2 e + K^3 e + ............ ) I have two questions: a) why (line 7) do I keep adding the emitted radiosity to my current radiosity estimate, surely this should be: 7: += ; This is just the rule for the evaluation of the von Neumann series: (1-K)B=B^e -> B=\sum K^n B^e the latter then expands into: B:=B^e (n=0) B:=B^e+KB=B^e+KB^e (n=1) B:=B^e+KB=B^e+K(B^e+KB^e)=... (n=2) This has nothing to do with wavelets or anything. It's just the evaluation of the von Neumann series. b) why do I have to Push everything to the finest level of the hierarchy before continuing with the next Jacobi iteration? I can see why I have to do this for display, but couldn't this Pull/Push come outside of the loop? The PushPull in the inner loop is only neccessary for the non-standard realization of the operator. The reason is that the over representation (averages on all levels of the hierarchy) needs to be consolidated before you can continue. More intuitively, when a child somewhere in the subdivision tree is sending out radiosity this needs to make some contribution to the radiosity at higher (coarser) levels of averaging. Similarly if a parent has received some irradiance than that is also received irradiance at its children and needs to be communicated to them. If you use the standard realization of the operator you don't have to do this. In this case the individual levels of basis functions are linearly independent (sometimes even orthogonal). The price you pay is that you can't get away with O(n) links but O(n log n). The intuitive reason for the latter is that a given receiver basis function will have to get the contributions from all basis functions on the source (log n levels). Whereas for the non-standard operator realization we can have a full (albeit more or less coarse) description of what is going on at each level. In some sense a given level acts as a proxy for all coarser levels. It is not clear to me which one is faster, but PushPull is such a small percentage of the overall running time that I have been reluctant to try do away with it at the cost of intruducing links accross levels. Others have used the standard realization but its very hard to actually compare the cost of two rather different implementations. I prefer the simplicity of the code for the non-standard realization (but am open to being convinced otherwise). It would be an interesting experiment to see just what the difference is in a single implementation so the numbers are actually comparable. Hope this helps. Peter From X-POP3-Rcpt: wp@stellaris Received: from mr.tuwien.ac.at by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for wp id AA00952; Wed, 4 Jan 95 06:39:57 +0100 Message-Id: <9501040539.AA00952@stellaris.cg.tuwien.ac.at> Received: from EIGVS4 by mr.tuwien.ac.at with DECNET-IN (PP) id <08237-0@mr.tuwien.ac.at>; Wed, 4 Jan 1995 06:36:42 +0100 X-Vms-To: IN%"globillum@cs.cmu.edu" "Global Illumination" To: wp@eigsg1.tuwien.ac.at From: in%72060.2420%compuserve.com%eigvs4@auniw Subject: Bibliography - HELP! Date: Wed, 4 Jan 1995 06:36:42 +0100 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Received: from HOSTESS.GRAPHICS.CS.CMU.EDU by Pap.UniVie.AC.AT (PMDF #12401) id <01HLFTGVNVQ89YCHMW@Pap.UniVie.AC.AT>; Wed, 4 Jan 1995 06:36 GMT+0100 Received: by HOSTESS.GRAPHICS.CS.CMU.EDU id aa04014; 4 Jan 95 0:30:37 EST Received: from CS.CMU.EDU by HOSTESS.GRAPHICS.CS.CMU.EDU id aa03962; 4 Jan 95 0:18:27 EST Received: from dub-img-3.compuserve.com by CS.CMU.EDU id aa23891; 4 Jan 95 0:17:55 EST Received: by dub-img-3.compuserve.com (8.6.9/5.941228sam) id AAA25418; Wed, 4 Jan 1995 00:17:42 -0500 Date: 04 Jan 95 00:15:45 EST From: Ian Ashdown <72060.2420@compuserve.com> Subject: Bibliography - HELP! To: Global Illumination Message-id: <950104051544_72060.2420_FHG101-1@CompuServe.COM> HELP! I took over the maintenance of Eric Haines' RADBIB radiosity bibliography earlier this year. Happily, 1994 was a *very* good year for radiosity and global-illumination related books and papers. To date, I've found references to 5 books and 60 papers. My problem is that it is very difficult to track down some of the more obscure papers, especially university technical reports and European conference proceedings. I am therefore asking for a few minutes of your time. The following message (Biblio - 1994 Additions) contains the 1994 additions to the bibliography. (It's over 560 lines long, so download it at your peril.) If you or your graduate students have published *anything* related to global illumination this year, would you please check to see whether I have included it. If not, then I would very much appreciate having you send me the appropriate reference via e-mail. (I would appreciate receiving a copy of your paper even more!) To save you some time, here's the list of publications I've already referenced: * 1994 Illuminating Engineering Society Annual Conference * ACM SIGGRAPH '94 Proceedings * Computer Graphics Forum * Computers & Graphics * Fifth Eurographics Workshop on Rendering * 4th Discrete Geometry for Computer Imagery * IEEE Computer * International Journal of Lighting Research and Technology * LICHT * Proceedings of Pacific Graphics '94 / CADDM '94 * Proceedings of the Winter School of Computer Graphics '94 The current release of the bibliography is available via ftp from: hobbes.lbl.gov as /pub/doc/RadBib94.Z siggraph.org in the database "biblio" through the "biblook" program and through the World Wide Web at the URL: http://siggraph.org/library/bibliography/bibliography.hmtl The next release will be sometime this month. Thanks for your cooperation. Ian Ashdown, President byHeart Software Limited 620 Ballantree Road West Vancouver, B.C. Canada V7S 1W3 From X-POP3-Rcpt: wp@stellaris Received: from mr.tuwien.ac.at by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for wp id AA00956; Wed, 4 Jan 95 06:40:14 +0100 Message-Id: <9501040540.AA00956@stellaris.cg.tuwien.ac.at> Received: from EIGVS4 by mr.tuwien.ac.at with DECNET-IN (PP) id <08243-0@mr.tuwien.ac.at>; Wed, 4 Jan 1995 06:36:55 +0100 X-Vms-To: IN%"globillum@cs.cmu.edu" "Global Illumination" To: wp@eigsg1.tuwien.ac.at From: in%72060.2420%compuserve.com%eigvs4@auniw Subject: Biblio - 1994 Additions Date: Wed, 4 Jan 1995 06:36:55 +0100 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Received: from HOSTESS.GRAPHICS.CS.CMU.EDU by Pap.UniVie.AC.AT (PMDF #12401) id <01HLFTH339IC9YCHMW@Pap.UniVie.AC.AT>; Wed, 4 Jan 1995 06:36 GMT+0100 Received: from EDRC.CMU.EDU by HOSTESS.GRAPHICS.CS.CMU.EDU id aa03977; 4 Jan 95 0:18:43 EST Received: from dub-img-3.compuserve.com by EDRC.CMU.EDU id aa22672; 4 Jan 95 0:18:03 EST Received: by dub-img-3.compuserve.com (8.6.9/5.941228sam) id AAA25441; Wed, 4 Jan 1995 00:17:55 -0500 Date: 04 Jan 95 00:16:42 EST From: Ian Ashdown <72060.2420@compuserve.com> Subject: Biblio - 1994 Additions To: Global Illumination Message-id: <950104051642_72060.2420_FHG101-2@CompuServe.COM> RADIOSITY / GLOBAL ILLUMINATION BIBLIOGRAPHY - 1994 ADDITIONS *** PAPERS (60) *** %A James Arvo %T The Irradiance Jacobian for Partially Occluded Polyhedral Sources %J Computer Graphics Proceedings, Annual Conference Series, 1994 (ACM SIGGRAPH '94 Proceedings) %P 343-350 %D 1994 %A James Arvo %A Kenneth Torrance %A Brian Smits %T A Framework for the Analysis of Error in Global Illumination Algorithms %J Computer Graphics Proceedings, Annual Conference Series, 1994 (ACM SIGGRAPH '94 Proceedings) %P 75-84 %D 1994 %A H. Bao %A Q. Peng %T An Efficient Form-Factor Evaluation Algorithm for Environments with Curved Surfaces %J Computers & Graphics %V 18 %N 4 %P 481-486 %D April 1994 %A Markus Beyer %T Approximation der Rendering Equation durch Evolutionare Algorithmen %R Diplomarbeit %I Technische Hochschule %C Darmstadt, Germany %D 1994 %A Markus Beyer %A Brigitta Lange %T Rayvolution: An Evolutionary Ray Tracing Algorithm %J Fifth Eurographics Workshop on Rendering %C Darmstadt, Germany %D June 1994 %P 137-146 %A Philippe Blasi %A Bertrand Le Saec %A Christophe Schlick %T An Importance Driven Monte-Carlo Solution to the Global Illumination Problem %J Fifth Eurographics Workshop on Rendering %C Darmstadt, Germany %D June 1994 %P 173-183 %A An-Seop Choi %A Richard G. Mistrick %T A Study of Lighting System Performance in Partitioned Spaces %J 1994 Illuminating Engineering Society Annual Conference Technical Papers %I Illuminating Engineering Society, 345 East 47th Street, New York, NY 10017 %P 453-480 %C Miami, FL %D August 7-11, 1994 %A Per H. Christensen %A Eric J. Stollnitz %A David H. Salesin %A Tony D. DeRose %T Importance-driven Wavelet Radiance %R Technical Report 94-01-05 %I Department of Computer Science and Engineering, University of Washington %C Seattle, Washington %D January 1994 %A Per H. Christensen %A Eric J. Stollnitz %A David H. Salesin %A Tony D. DeRose %T Wavelet Radiance %J Fifth Eurographics Workshop on Rendering %C Darmstadt, Germany %D June 1994 %P 287-302 %A Steven Collins %T Adaptive Splatting for Specular to Diffuse Light Transport %J Fifth Eurographics Workshop on Rendering %C Darmstadt, Germany %D June 1994 %P 119-135 %A David L. DiLaura %A Jeffrey Quinlan %T Non-Diffuse Radiative Transfer I: Planar Area Sources and Point Receivers %J 1994 Illuminating Engineering Society Annual Conference Technical Papers %I Illuminating Engineering Society, 345 East 47th Street, New York, NY 10017 %P 633-660 %C Miami, FL %D August 7-11, 1994 %A George Dretakkis %T Structured Sampling and Reconstruction of Illumination for Image Synthesis %R CSRI Technical Report 293 %I Department of Computer Science, University of Toronto %C Toronto, Ontario %D January 1994 %Z available via anonymous ftp as: ftp.csri.toronto.edu:csri-technical-reports/293 %A George Dretakkis %T Simplifying the Representation of Radiance from Multiple Emitters %J Fifth Eurographics Workshop on Rendering %C Darmstadt, Germany %D June 1994 %P 259-272 %A George Dretakkis %A Eugene Fiume %T A Fast Shadow algorithm for Area Light Sources Using Backprojection %J Computer Graphics Proceedings, Annual Conference Series, 1994 (ACM SIGGRAPH '94 Proceedings) %P 223-230 %D 1994 %A Philip Dutre %A Yves D. Willems %T Importance-Driven Monte Carlo Light Tracing %J Fifth Eurographics Workshop on Rendering %C Darmstadt, Germany %D June 1994 %P 185-194 %A Pavol Elias %A Martin Feda %A Peter Ferschin %A Werner Purgathofer %T Cubic Monte Carlo Radiosity %J Proceedings of the Winter School of Computer Graphics '94 %E V. Skala %C Plzen, Czech Republic %D January 1994 %A Martin Feda %A Werner Purgathofer %T A Median Cut Algorithm for Efficient Sampling of Radiosity Functions %J Computer Graphics Forum (Eurographics '94 Proceedings) %V 13 %N 3 %P C433-C442 %D 1994 %A David A. Forsyth %A Chien Yang %A Kim Teo %T Efficient Radiosity in Dynamic Environments %J Fifth Eurographics Workshop on Rendering %C Darmstadt, Germany %D June 1994 %P 313-323 %A Neil Gatenby %T Incorporating Hierarchical Radiosity into Discontinuity Meshing Radiosity %R PhD thesis %I University of Manchester %C Manchester, UK %D 1994 %A Neil Gatenby %A W. T. Hewitt %T Optimizing Discontinuity Meshing Radiosity %J Fifth Eurographics Workshop on Rendering %C Darmstadt, Germany %D June 1994 %P 249-258 %A Reid Gershbein %A Peter Schroder %A Pat Hanrahan %T Textures and Radiosity: Controlling Emission and Reflection from Texture Maps %R Technical report CS-TR-449-94 %I Princeton University %D March 1994 %A Reid Gershbein %A Peter Schroder %A Pat Hanrahan %T Textures and Radiosity: Controlling Emission and Reflection with Texture Maps %J Computer Graphics Proceedings, Annual Conference Series, 1994 (ACM SIGGRAPH '94 Proceedings) %P 51-58 %D 1994 %A Nicolas Holzschuch %A Francois Sillion %A George Dretakkis %T An Efficient Progressive Refinement Strategy for Hierarchical Radiosity %J Fifth Eurographics Workshop on Rendering %C Darmstadt, Germany %D June 1994 %P 343-357 %A Eric P. Lafortune %A Yves D. Leuven %T A Theoretical Framework for Physically Based Rendering %J Computer Graphics Forum %V 13 %N 2 %D June 1994 %P 97-107 %A Eric P. Lafortune %A Yves D. Willems %T The Ambient Term as a Variance Reducing Technique for Monte Carlo Ray Tracing %J Fifth Eurographics Workshop on Rendering %C Darmstadt, Germany %D June 1994 %P 163-171 %A Eric Languenou %A Kadi Bouatouch %A Michelle Chelle %T Global Illumination in Presence of Participating Media with General Properties %J Fifth Eurographics Workshop on Rendering %C Darmstadt, Germany %D June 1994 %P 69-85 %A Dani Lischinski %T Accurate and Reliable Algorithms for Global Illumination %R PhD thesis %I Cornell University %C Ithaca, NY %D 1994 %A Dani Lischinski %T Incremental Delaunay Triangulation %B Graphics Gems IV %E Paul S. Heckbert %I Academic Press Professional %C San Diego, CA %D 1994 %P 47-59 %A Dani Lischinski %A Brian Smits %A Donald P. Greenberg %T Bounds and Error Estimates for Radiosity %J Computer Graphics Proceedings, Annual Conference Series, 1994 (ACM SIGGRAPH '94 Proceedings) %P 67-74 %D 1994 %A Nelson L. Max %T Efficient Light Propagation for Multiple Anisotropic Volume Scattering %J Fifth Eurographics Workshop on Rendering %C Darmstadt, Germany %D June 1994 %P 87-104 %A Christian Metge %A Rene Caubet %T A Discrete Global Illumination Method %J 4th Discrete Geometry for Computer Imagery %C Grenoble, France %D September 1994 %P 77-88 %A Stefan Muller %A Frank Schoffel %T Fast Radiosity Repropagation for Interactive Virtual Environments Using a Shadow-Form-Factor-List %J Fifth Eurographics Workshop on Rendering %C Darmstadt, Germany %D June 1994 %P 325-342 %A Karol Myszkowski %A Tosiyasu L. Kunii %T Texture Mapping as an Alternative for Meshing During Walkthrough Animation %J Fifth Eurographics Workshop on Rendering %C Darmstadt, Germany %D June 1994 %P 375-388 %A Laszlo Neumann %T New Efficient Algorithms with Positive Definite Radiosity Matrix %J Fifth Eurographics Workshop on Rendering %C Darmstadt, Germany %D June 1994 %P 219-237 %A Laszlo Neumann %T Monte Carlo Radiosity %J Computing %I Springer-Verlag %D submitted for publication 1994 %A Laszlo Neumann %A Martin Feda %A Manfred Kopp %A Werner Purgathofer %T A New Stochastic Radiosity Method for Highly Complex Scenes %J Fifth Eurographics Workshop on Rendering %C Darmstadt, Germany %D June 1994 %P 195-206 %A Jeffry S. Nimeroff %A Eero Simoncelli %A Julie Dorsey %T Efficient Re-rendering of Naturally Illuminated Environments %J Fifth Eurographics Workshop on Rendering %C Darmstadt, Germany %D June 1994 %P 359-373 %A M. Nithisoontorn %T Shooting Algorithm for Illuminance: Comparison of Prediction with Experiment %J International Journal of Lighting Research and Technology %V 26 %N 1 %P 13-18 %D 1994 %A Sumanta N. Pattanaik %A Kadi Bouatouch %T Fast Wavelet Radiosity Method %J Computer Graphics Forum (Eurographics '94 Proceedings) %V 13 %N 3 %P C407-C420 %D September 1994 %A Sumanta N. Pattanaik %A Kadi Bouatouch %T Haar Wavelet: A Solution to Global Illumination with General Surface Properties %J Fifth Eurographics Workshop on Rendering %C Darmstadt, Germany %D June 1994 %P 273-286 %A M. Paulin %A J-P. Jessel %T Adaptive Mesh Generation for Progressive Radiosity: A Ray-tracing Based Algorithm %J Computer Graphics Forum (Eurographics '94 Proceedings) %V 13 %N 3 %D 1994 %P C421-C432 %A Holly Rushmeier %T Rendering Participating Media: Problems and Solutions from Application Areas %J Fifth Eurographics Workshop on Rendering %C Darmstadt, Germany %D June 1994 %P 35-56 %A Christophe Schlick %T A Survey of Shading and Reflectance Models %J Computer Graphics Forum %V 13 %N 2 %P 121-131 %D June 1994 %A Peter Schroder %A Steven J. Gortler %A Michael F. Cohen %A Pat Hanrahan %T Wavelet Projections for Radiosity %J Computer Graphics Forum %V 13 %N 2 %D June 1994 %P 141-151 %A Francois Sillion %T Clustering and Volume Scattering for Hierarchical Radiosity Calculations %J Fifth Eurographics Workshop on Rendering %C Darmstadt, Germany %D June 1994 %P 105-117 %A Jaswinder P. Singh %T Parallel Hierarchical N-Body Methods and their Implications for Multiprocessors %R Technical Report CSL-TR-93-563 %I Computer Systems Laboratory, Stanford University %C Stanford, CA %D February 1993 %A Jaswinder P. Singh %A Annop Gupta %A Marc Levoy %T Parallel Visualization Algorithms: Performance and Architectural Implications %J IEEE Computer %V 27 %N 7 %D July 1994 %P 45-55 %A Brian Smits %T Efficient Hierarchical Radiosity for Complex Environments %R PhD thesis %I Cornell University %C Ithaca, NY %D 1994 %A Brian Smits %A James Arvo %A Donald Greenberg %T A Clustering Algorithm for Radiosity in Complex Environments %J Computer Graphics Proceedings, Annual Conference Series, 1994 (ACM SIGGRAPH '94 Proceedings) %P 435-442 %D 1994 %A A. James Stewart %A Sherif Ghali %T Fast Computation of Shadow Boundaries using Spatial Coherence and Backprojection %J Computer Graphics Proceedings, Annual Conference Series 1994 (ACM SIGGRAPH '94 Proceedings) %P 231-238 %D 1994 %A W. Sturzlinger %T Adaptive Mesh Refinement with Discontinuities for the Radiosity Method %J Fifth Eurographics Workshop on Rendering %C Darmstadt, Germany %D June 1994 %P 239-248 %A W. Sturzlinger %A C. Wild %T Parallel Progressive Radiosity with Parallel Visibility Computations %J Proceedings of the Winter School of Computer Graphics '94 %E V. Skala %C Plzen, Czech Republic %D January 1994 %P 66-74 %A Seth Teller %A Celeste Fowler %A Thomas Funkhouser %A Pat Hanrahan %T Partitioning and Ordering Large Radiosity Computations %J Computer Graphics Proceedings, Annual Conference Series, 1994 (ACM SIGGRAPH '94 Proceedings) %P 443-450 %D 1994 %A P. R. Tregenza %T Daylighting Computation: Radiosity Method Using Triangular Patches %J International Journal of Lighting Research and Technology %V 26 %N 1 %P 1-7 %D 1994 %A Clemens Tropp %T Eine Praxisorientierte Software fur Realitatsgetreure 3D-Lichtsimulation (Practically Oriented Software for Highly Realistic 3-D Light Simulation) %J LICHT %V 7/8 %D 1994 %P 578-580 %I Pflaum Verlag GmbH & Co. KG %C Munchen, Germany %O ISSN 0024-2861 %A Eric Veach %A Leonidas Guibas %T Bidirectional Estimators for Light Transport %J Fifth Eurographics Workshop on Rendering %C Darmstadt, Germany %D June 1994 %P 147-162 %A Gregory J. Ward %T The RADIANCE Lighting Simulation and Rendering System %J Computer Graphics Proceedings, Annual Conference Series, 1994 (ACM SIGGRAPH '94 Proceedings) %P 459-472 %D 1994 %A Gregory J. Ward %T Applications of RADIANCE to Architecture and Lighting Design %J 1994 Illuminating Engineering Society Annual Conference Technical Papers %I Illuminating Engineering Society, 345 East 47th Street, New York, NY 10017 %P 633-660 %C Miami, FL %D August 7-11, 1994 %P 777-791 %A Wei Xu %A Donald S. Fussell %T Constructing Solvers for Radiosity Equation Systems %J Fifth Eurographics Workshop on Rendering %C Darmstadt, Germany %D June 1994 %P 207-217 %A Wei Xu %A Donald S. Fussell %T A Fast Solver of Radiosity Equation Systems %J Proceedings of Pacific Graphics '94 / CADDM '94 %C Beijing, China %D August 1994 *** BOOKS (5) *** %E P. Brunet %E F. W. Jansen %B Photorealistic Rendering in Computer Graphics %I Springer-Verlag %C Berlin, Germany %D 1994 %O Proceedings of the Second Eurographics Workshop on Rendering, Barcelona, Spain, May 1991 %A Ian Ashdown %B Radiosity: A Programmer's Perspective %I John Wiley & Sons %C New York %D 1994 %O ISBN 0-471-30444-1 (without diskette) %O ISBN 0-471-30488-3 (with MS-Windows diskette) %A William Parsons Newhall, Jr. %B PC Graphics Unleashed %E SAMS Publishing (various editors) %I SAMS Publishing %C Indianapolis, Indiana %D 1994 %P 501-575 (Chapter 18) %O ISBN 0-672-30570-4 (includes CD-ROM) %A William Parsons Newhall, Jr. %B From Ray Tracing to Radiosity %I SAMS Publishing %C Indianapolis, Indiana %D 1995 (to be published) %O ISBN 0-672-30497-X (includes CD-ROM) %A Francois Sillion %A Claude Puech %B Radiosity and Global Illumination %I Morgan Kaufmann %C San Francisco %D 1994 %O ISBN 1-55860-277-1 *** END OF 1994 ADDITIONS *** From X-POP3-Rcpt: wp@stellaris Received: from eigmq2.tuwien.ac.at by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for wp id AA28398; Wed, 11 Jan 95 13:45:25 +0100 X-Sender: wp@stellaris.cg.tuwien.ac.at Message-Id: Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed Date: Wed, 11 Jan 1995 13:43:35 +0100 To: feda, fischel, gervautz, groeller, kopp, helwig, mazuryk, elias, scheirich, schmalstieg, stieglecker, tastl@eigvs4.una.ac.at, tobler, traxler, meyer, schindler, WP, feda, tobler, elias, neum@integra.hu, xavier@ima.udg.es, sbert@ima.udg.es From: Werner Purgathofer Subject: globillum from Peter Shirley: Terms and Symbols X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit >X-POP3-Rcpt: wp@stellaris >To: wp@eigsg1.tuwien.ac.at >From: in%shirley%graphics.cornell.edu%eigvs4@auniw >Subject: Terms and Symbols >Date: Thu, 22 Dec 1994 18:00:37 +0100 > >Received: from HOSTESS.GRAPHICS.CS.CMU.EDU by Pap.UniVie.AC.AT (PMDF #12401) id > <01HKYBK42ZAO9FOFY2@Pap.UniVie.AC.AT>; Thu, 22 Dec 1994 18:00 GMT+0100 >Received: by HOSTESS.GRAPHICS.CS.CMU.EDU id aa22195; 22 Dec 94 11:57:32 EST >Received: from EDRC.CMU.EDU by HOSTESS.GRAPHICS.CS.CMU.EDU id aa22164; 22 Dec > 94 11:32:34 EST >Received: from MERCKX.GRAPHICS.CORNELL.EDU by EDRC.CMU.EDU id aa07964; 22 Dec > 94 11:32:06 EST >Received: by merckx.graphics.cornell.edu (5.65/DEC-Ultrix/4.3) id AA06390; Thu, > 22 Dec 1994 11:32:18 -0500 >Received: by zap.graphics.cornell.edu (1.37.109.8/16.2) id AA26819; Thu, > 22 Dec 1994 11:32:04 -0500 >Date: Thu, 22 Dec 1994 11:32:04 -0500 (EST) >From: Peter Shirley >Subject: Terms and Symbols >To: globillum@cs.cmu.edu >Message-id: <9412221632.AA06390@merckx.graphics.cornell.edu> >Content-type: text/plain; charset=US-ASCII >Content-transfer-encoding: 7bit >X-Mailer: ELM [version 2.4 PL24] >Mime-Version: 1.0 >Content-Length: 1325 > >I am writing a Siggraph submission and am having my usual angst >over symbols used for radiometric quantities. If you don't think >this is important, imagine reading a linear algebra text >that uses xA = b for a linear system! Unfortunately, we have >nothing as standard as Ax=b in graphics. Here is what I have >seen used often in rendering: > > IES Heat Transfer other >power \Phi ?? >radiant exitance M B >irradiance E H \phi >radiant intensity I ?? >radiance L I >field (incoming) radiance L_f ?? >surface (outgoing) radiance L_s ?? >emitted radiance ?? ?? L, L_e > >My biggest worry is about irradiance and radiant exitance. I try >to use IES symbols when possible because they have an ANSI document >for terms and symbols, but I can't bring myself to use E (for one reason >because I am using expected values in the same paper). Should I >use H, and then use B for radiant exitance (radiosity)? If anyone >has words of wisdom for me, please share them. > >Have a happy holiday! > >Pete Shirley >shirley@graphics.cornell.edu > ------------------------------------------------------------------- Werner Purgathofer Tel. +43(1)58801 4548 Institute of Computer Graphics ( secretary: 4549 ) Technical University of Vienna Fax. +43(1)5874932 Karlsplatz 13 / 186 email: wp@cg.tuwien.ac.at A-1040 Wien / Austria ------------------------------------------------------------------- From To: Abteilung-186/2, Stochastic-Radiosity From: Werner Purgathofer Subject: globillum from Peter Shirley: Terms and Symbols Message-Id: X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Date: Wed, 11 Jan 1995 13:43:10 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit >X-POP3-Rcpt: wp@stellaris >To: wp@eigsg1.tuwien.ac.at >From: in%shirley%graphics.cornell.edu%eigvs4@auniw >Subject: Terms and Symbols >Date: Thu, 22 Dec 1994 18:00:37 +0100 > >Received: from HOSTESS.GRAPHICS.CS.CMU.EDU by Pap.UniVie.AC.AT (PMDF #12401) id > <01HKYBK42ZAO9FOFY2@Pap.UniVie.AC.AT>; Thu, 22 Dec 1994 18:00 GMT+0100 >Received: by HOSTESS.GRAPHICS.CS.CMU.EDU id aa22195; 22 Dec 94 11:57:32 EST >Received: from EDRC.CMU.EDU by HOSTESS.GRAPHICS.CS.CMU.EDU id aa22164; 22 Dec > 94 11:32:34 EST >Received: from MERCKX.GRAPHICS.CORNELL.EDU by EDRC.CMU.EDU id aa07964; 22 Dec > 94 11:32:06 EST >Received: by merckx.graphics.cornell.edu (5.65/DEC-Ultrix/4.3) id AA06390; Thu, > 22 Dec 1994 11:32:18 -0500 >Received: by zap.graphics.cornell.edu (1.37.109.8/16.2) id AA26819; Thu, > 22 Dec 1994 11:32:04 -0500 >Date: Thu, 22 Dec 1994 11:32:04 -0500 (EST) >From: Peter Shirley >Subject: Terms and Symbols >To: globillum@cs.cmu.edu >Message-id: <9412221632.AA06390@merckx.graphics.cornell.edu> >Content-type: text/plain; charset=US-ASCII >Content-transfer-encoding: 7bit >X-Mailer: ELM [version 2.4 PL24] >Mime-Version: 1.0 >Content-Length: 1325 > >I am writing a Siggraph submission and am having my usual angst >over symbols used for radiometric quantities. If you don't think >this is important, imagine reading a linear algebra text >that uses xA = b for a linear system! Unfortunately, we have >nothing as standard as Ax=b in graphics. Here is what I have >seen used often in rendering: > > IES Heat Transfer other >power \Phi ?? >radiant exitance M B >irradiance E H \phi >radiant intensity I ?? >radiance L I >field (incoming) radiance L_f ?? >surface (outgoing) radiance L_s ?? >emitted radiance ?? ?? L, L_e > >My biggest worry is about irradiance and radiant exitance. I try >to use IES symbols when possible because they have an ANSI document >for terms and symbols, but I can't bring myself to use E (for one reason >because I am using expected values in the same paper). Should I >use H, and then use B for radiant exitance (radiosity)? If anyone >has words of wisdom for me, please share them. > >Have a happy holiday! > >Pete Shirley >shirley@graphics.cornell.edu > From X-POP3-Rcpt: wp@stellaris Received: from mr.tuwien.ac.at by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for wp id AA27851; Mon, 23 Jan 95 18:24:13 +0100 Message-Id: <9501231724.AA27851@stellaris.cg.tuwien.ac.at> Received: from EIGVS4 by mr.tuwien.ac.at with DECNET-IN (PP) id <27371-0@mr.tuwien.ac.at>; Mon, 23 Jan 1995 18:20:54 +0100 X-Vms-To: IN%"globillum@cs.cmu.edu" To: wp@eigsg1.tuwien.ac.at From: in%nic%informatik.uni-rostock.de%eigvs4@auniw Subject: Color quantization Date: Mon, 23 Jan 1995 18:20:54 +0100 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Received: from HOSTESS.GRAPHICS.CS.CMU.EDU by Pap.UniVie.AC.AT (PMDF #12401) id <01HM71LBK1DC9YDRB7@Pap.UniVie.AC.AT>; Mon, 23 Jan 1995 18:20 GMT+0100 Received: from EDRC.CMU.EDU by HOSTESS.GRAPHICS.CS.CMU.EDU id aa03040; 23 Jan 95 10:10:32 EST Received: from [139.30.5.28] by EDRC.CMU.EDU id aa29078; 23 Jan 95 10:09:49 EST Received: by ceylon.informatik.uni-rostock.de id QAA12406; Mon, 23 Jan 1995 16:09:18 +0100 Received: by carl.informatik.uni-rostock.de id QAA05795; Mon, 23 Jan 1995 16:09:17 +0100 Date: Mon, 23 Jan 1995 16:09:17 +0100 (MET) From: Nico Guenther Subject: Color quantization To: globillum@cs.cmu.edu Message-id: <199501231509.QAA05795@carl.informatik.uni-rostock.de> Content-type: text X-Mailer: ELM [version 2.4 PL23] Content-Length: 978 Hi, some days ago Ian Asdown posted a pointer to some color quanti techniques. Concerning 24->8 bit quantization one has to take care of the following: Usually quantization techniques are linear ones; however our audio-visual system uses a nonlinear scale (see Weber-Fechner-law in acoustics). Hence the visual image quality of 8bit images can be improved by a simple procedure 1st - nonlinear color scaling 2nd - color quantization 3rd - invers scaling to 1st 4th - rendering Some work concerning these problems was done in 1993 as MS at CS dep. of university of Rostock. A: Joern Trilk T: Nichtlineare Farbskalierung fuer die realistische Bilddarstellung K: you see, in German This work includes visual comparison of different scaling functions like log Weber-Fechner, Cornsweet, Paeth, ... and the corresponding C-code. In addition to that you can find a good reference list (mostly in English). Maybe this is for some use to you. Nico (nic@informatik.uni-rostock.de) From To: Abteilung-186/2, Abteilung-186/1 From: Werner Purgathofer Subject: Questionnaire (forwarded) Message-Id: X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Date: Thu, 26 Jan 1995 08:54:26 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit >X-POP3-Rcpt: wp@stellaris >To: wp@eigsg1.tuwien.ac.at >From: in%vezza%public.iunet.it%eigvs4@auniw >Subject: Questionnaire >Date: Wed, 25 Jan 1995 23:50:25 +0100 > >Received: from HOSTESS.GRAPHICS.CS.CMU.EDU by Pap.UniVie.AC.AT (PMDF #12401) id > <01HMA5OGXIDC9YDY5E@Pap.UniVie.AC.AT>; Wed, 25 Jan 1995 23:49 GMT+0100 >Received: from EDRC.CMU.EDU by HOSTESS.GRAPHICS.CS.CMU.EDU id aa01567; 25 Jan > 95 17:34:39 EST >Received: from [192.106.6.15] by EDRC.CMU.EDU id aa13658; 25 Jan 95 17:33:25 EST >Received: (from vezza@localhost) by public.iunet.it (8.6.9/8.6.9) id XAA15125 > for globillum@cs.cmu.edu; Wed, 25 Jan 1995 23:13:06 +0100 >Date: Wed, 25 Jan 1995 23:13:04 +0100 (MET) >From: Luca Vezzadini >Subject: Questionnaire >To: globillum@cs.cmu.edu >Message-id: <199501252213.XAA15125@public.iunet.it> >Content-type: text >X-Mailer: ELM [version 2.4 PL23] >Content-Length: 430 > >Hi ! >I am working in Italy on a book on 3D graphics; I am preparing a kind of >questionnaire, a general interview on this field, that will help me in >my project. Is there anybody out there who would like to take a look at it? >(Some of you probably already have it...) >I would like to get in touch with scientists and artists dealing with >3D graphics. >Thanks for your attention ! > >- Luca Vezzadini > E-mail: vezza@mailbox.iunet.it > From X-POP3-Rcpt: wp@stellaris Received: from mr.tuwien.ac.at by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for wp id AA05877; Tue, 31 Jan 95 14:50:43 +0100 Message-Id: <9501311350.AA05877@stellaris.cg.tuwien.ac.at> Received: from EIGVS4 by mr.tuwien.ac.at with DECNET-IN (PP) id <16071-0@mr.tuwien.ac.at>; Tue, 31 Jan 1995 14:47:22 +0100 X-Vms-To: IN%"globillum@cs.cmu.edu" To: wp@eigsg1.tuwien.ac.at From: in%hwj%hwj.gk.dtu.dk%eigvs4@auniw Date: Tue, 31 Jan 1995 14:47:22 +0100 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Received: from HOSTESS.GRAPHICS.CS.CMU.EDU by Pap.UniVie.AC.AT (PMDF #12401) id <01HMI0HCXY749YEBID@Pap.UniVie.AC.AT>; Tue, 31 Jan 1995 14:46 GMT+0100 Received: from RI.CMU.EDU by HOSTESS.GRAPHICS.CS.CMU.EDU id aa07463; 31 Jan 95 8:37:36 EST Received: from [130.225.91.126] by RI.CMU.EDU id aa12395; 31 Jan 95 8:37:17 EST Received: (from hwj@localhost) by hwj.gk.dtu.dk (8.6.9/8.6.9) id RAA04054 for globillum@cs.cmu.edu; Tue, 31 Jan 1995 17:25:53 +0100 Date: Tue, 31 Jan 1995 17:25:53 +0100 From: Henrik Wann Jensen To: globillum@cs.cmu.edu Message-id: <199501311625.RAA04054@hwj.gk.dtu.dk> Hi All, For some time I have been using a brute force Path Tracing method to validate the results from other global illumination methods. The results are images in which the pixel values are represented as either pure float (one per. wavelength) or as Greg Wards real pixels. My question is: How can I compare these images? I have primarily been using a squared sum of pixel differences. This means that the two images being compared are subtracted giving a difference image. The pixel values in the difference image are squared and added together giving some number (=error) indicating the "distance" between the two images. This method is relatively good but it gives pour ratings to images which have just a few pixels with a large distance (these images could perhaps be corrected using a noise reduction filter). Furthermore the method doesn't say much about the visual quality of the image being validated -- sometimes a little noise does look good... The error (number) also depends on the brightness of the image and images which has problems in dark areas (like shadows) gets a smaller error than images with problems in bright areas. It has no meaning (or very little meaning) comparing the error resulting from the computation of different images. etc.... Alternative methods could be: Maximum pixel difference, Average pixel difference etc. I would like some kind of normalized squared sum of pixel differences. It should, however, not "go berserk" in very dark areas with relatively large (but still invisible errors). And even better if the method gave the error 42 using the same global illumination method on two different images then the "looks of the error" would be the same on the two images (is this impossible?). That was my first two cents :-) - Henrik Wann Jensen From X-POP3-Rcpt: wp@stellaris Received: from mr.tuwien.ac.at by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for wp id AA07313; Tue, 31 Jan 95 18:00:27 +0100 Message-Id: <9501311700.AA07313@stellaris.cg.tuwien.ac.at> Received: from EIGVS4 by mr.tuwien.ac.at with DECNET-IN (PP) id <24898-0@mr.tuwien.ac.at>; Tue, 31 Jan 1995 17:57:06 +0100 X-Vms-To: IN%"hwj@hwj.gk.dtu.dk" "Henrik Wann Jensen", IN%"globillum@cs.cmu.edu" To: wp@eigsg1.tuwien.ac.at From: in%holly%cam.nist.gov%eigvs4@auniw Subject: image comparisons Date: Tue, 31 Jan 1995 17:57:06 +0100 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Received: from HOSTESS.GRAPHICS.CS.CMU.EDU by Pap.UniVie.AC.AT (PMDF #12401) id <01HMI73GGBKG9YEBHO@Pap.UniVie.AC.AT>; Tue, 31 Jan 1995 17:56 GMT+0100 Received: from CS.CMU.EDU by HOSTESS.GRAPHICS.CS.CMU.EDU id aa08124; 31 Jan 95 11:42:30 EST Received: from fs1.cam.nist.gov by CS.CMU.EDU id aa06265; 31 Jan 95 11:41:06 EST Received: from plum (plum.cam.nist.gov) by fs1.cam.nist.gov (4.1/SMI-DDN) id AA12639; Tue, 31 Jan 95 11:41:03 EST Received: by plum (940406.SGI/SMI-3.2) id AA17150; Tue, 31 Jan 95 11:41:01 -0500 Date: Tue, 31 Jan 1995 11:41:01 -0500 From: Holly E Rushmeier Subject: image comparisons In-reply-to: Henrik Wann Jensen "" (Jan 31, 5:25pm) To: Henrik Wann Jensen , globillum@cs.cmu.edu Message-id: <9501311141.ZM17148@plum.cam.nist.gov> Content-type: text/plain; charset=us-ascii X-Mailer: Z-Mail (3.1.0 22feb94 MediaMail) Mime-Version: 1.0 References: <199501311625.RAA04054@hwj.gk.dtu.dk> Hi -- We have also been looking at the image comparison problem. I don't have any good suggestions right now, but our approach is to try to build on the work on image metrics for evaluating the effects of lossy compression. Here are some references. I'm not familiar with these papers in any depth, so you have to make your own assessments of their usefulness: Mannos & Sakrison, "The Effects of a Vision Fidelity Criterion on the Encoding of Images", IEEE Trans. on Information Theory, vol. it-20, July 1974, pp. 525-536. Saghri, Cheatham, & Habbi "Image quality measure based on a human visual system model", Optical Engineering, July 1989, vol 28, no. 7, pp. 813-818. Nill, " A Visual Model Weighted Cosine Transform for Image Compression and Quality Assessment", IEEE Transactions on Communications, vol. com-33, no. 6, June 1985, pp. 551-557 Even if you can't find these particular papers, you can probably draw some inspiration for methods to test out by rifling through the literature on evaluating lossy compression methods. I think incorporating even simple-minded human visual models would give useful results, and keep the metric from going beserk in dark areas, etc. -- Holly From X-POP3-Rcpt: wp@stellaris Received: from mr.tuwien.ac.at by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for wp id AA07489; Tue, 31 Jan 95 19:32:11 +0100 Message-Id: <9501311832.AA07489@stellaris.cg.tuwien.ac.at> Received: from EIGVS4 by mr.tuwien.ac.at with DECNET-IN (PP) id <28452-0@mr.tuwien.ac.at>; Tue, 31 Jan 1995 19:28:51 +0100 X-Vms-To: IN%"globillum@cs.cmu.edu" To: wp@eigsg1.tuwien.ac.at From: in%donm%microsoft.com%eigvs4@auniw Subject: image quality metrics Date: Tue, 31 Jan 1995 19:28:51 +0100 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Received: from HOSTESS.GRAPHICS.CS.CMU.EDU by Pap.UniVie.AC.AT (PMDF #12401) id <01HMIAB84HGG9YEBVI@Pap.UniVie.AC.AT>; Tue, 31 Jan 1995 19:28 GMT+0100 Received: from EDRC.CMU.EDU by HOSTESS.GRAPHICS.CS.CMU.EDU id aa00442; 31 Jan 95 13:20:51 EST Received: from netmail2.microsoft.com by EDRC.CMU.EDU id aa15785; 31 Jan 95 13:18:57 EST Received: by netmail2.microsoft.com (5.65/25-eef) id AA26339; Tue, 31 Jan 95 10:19:28 -0800 Received: by netmail2 using fxenixd 1.0 Tue, 31 Jan 95 10:19:28 PST Date: Tue, 31 Jan 95 10:09:41 TZ From: Don Mitchell Subject: image quality metrics To: globillum@cs.cmu.edu Message-id: <9501311819.AA26339@netmail2.microsoft.com> X-Msmail-Message-Id: 4291C4D3 X-Msmail-Conversation-Id: 4291C4D3 I've played with Mannos and Sakrison's method. The wisdom at Bell Labs seemed to be that numerical image-quality metrics were a sort of holy grail that has never been completely achieved. Be careful. There is so much going on in our subjective response! Methods like M&S can take into account the logarithmic response to contrast and the basic color and spatial frequency dependance. Oh wait, the color response stuff is in another paper by Werner Frei (I'll try to find that reference). But there are other things like visual masking that are hard to model -- the visibility of noise depends a lot on the context. Don't be afraid to do subjective testing. Well, be a little afraid, because its a pain in the neck to organize it, but I think letting expert observers make judgements means more than assigning a mysterious number (which ultimate is based on some fit to some set of subjective-testing data anyway!). From X-POP3-Rcpt: wp@stellaris Received: from mr.tuwien.ac.at by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for wp id AA07560; Tue, 31 Jan 95 20:00:41 +0100 Message-Id: <9501311900.AA07560@stellaris.cg.tuwien.ac.at> Received: from EIGVS4 by mr.tuwien.ac.at with DECNET-IN (PP) id <29327-0@mr.tuwien.ac.at>; Tue, 31 Jan 1995 19:57:33 +0100 X-Vms-To: IN%"globillum@cs.cmu.edu" To: wp@eigsg1.tuwien.ac.at From: in%greg%taligent.com%eigvs4@auniw Subject: RE: image quality metrics Date: Tue, 31 Jan 1995 19:57:33 +0100 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Received: from HOSTESS.GRAPHICS.CS.CMU.EDU by Pap.UniVie.AC.AT (PMDF #12401) id <01HMIBAZ1HSG9YECEB@Pap.UniVie.AC.AT>; Tue, 31 Jan 1995 19:57 GMT+0100 Received: from CS.CMU.EDU by HOSTESS.GRAPHICS.CS.CMU.EDU id aa00578; 31 Jan 95 13:48:49 EST Received: from mailserv.taligent.com by CS.CMU.EDU id aa07687; 31 Jan 95 13:46:24 EST Received: from yahoo.taligent.com by mailserv.taligent.com (AIX 3.2/UCB 5.64/4.03) id AA204633; Tue, 31 Jan 1995 10:46:50 -0800 Received: by yahoo.taligent.com (AIX 4.1/UCB 5.64/4.03) id AA26620; Tue, 31 Jan 1995 10:46:49 -0800 Date: Tue, 31 Jan 1995 10:46:49 -0800 From: greg@taligent.com Subject: RE: image quality metrics In-reply-to: <9501311819.AA26339@netmail2.microsoft.com> To: globillum@cs.cmu.edu Message-id: <9501311846.AA26620@yahoo.taligent.com> References: <9501311819.AA26339@netmail2.microsoft.com> >>>>> "DM" == Don Mitchell writes: DM> I've played with Mannos and Sakrison's method. The wisdom at Bell DM> Labs seemed to be that numerical image-quality metrics were a sort DM> of holy grail that has never been completely achieved. DM> ... DM> Don't be afraid to do subjective testing. Well, be a little DM> afraid, because its a pain in the neck to organize it, but I think DM> letting expert observers make judgements means more than assigning DM> a mysterious number (which ultimate is based on some fit to some DM> set of subjective-testing data anyway!). I would agree completely. I did a lot of work on the perceptual brightness of light sources for my thesis, and perceptual testing seems to be the only reliable (well, pretty reliable anyhow) way to test image quality. It is a pain to design a good test, though. The up side is that you don't usually need too many subjects. -Greg. From X-POP3-Rcpt: wp@stellaris Received: from mr.tuwien.ac.at by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for wp id AA07588; Tue, 31 Jan 95 20:22:30 +0100 Message-Id: <9501311922.AA07588@stellaris.cg.tuwien.ac.at> Received: from EIGVS4 by mr.tuwien.ac.at with DECNET-IN (PP) id <29910-0@mr.tuwien.ac.at>; Tue, 31 Jan 1995 20:19:00 +0100 X-Vms-To: IN%"donm@microsoft.com" "Don Mitchell", IN%"globillum@cs.cmu.edu" To: wp@eigsg1.tuwien.ac.at From: in%holly%cam.nist.gov%eigvs4@auniw Subject: RE: image quality metrics Date: Tue, 31 Jan 1995 20:19:00 +0100 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Received: from HOSTESS.GRAPHICS.CS.CMU.EDU by Pap.UniVie.AC.AT (PMDF #12401) id <01HMIC2DHL9C9YEBAW@Pap.UniVie.AC.AT>; Tue, 31 Jan 1995 20:18 GMT+0100 Received: from CS.CMU.EDU by HOSTESS.GRAPHICS.CS.CMU.EDU id aa00613; 31 Jan 95 14:00:02 EST Received: from fs1.cam.nist.gov by CS.CMU.EDU id aa07857; 31 Jan 95 13:59:16 EST Received: from plum (plum.cam.nist.gov) by fs1.cam.nist.gov (4.1/SMI-DDN) id AA14000; Tue, 31 Jan 95 13:59:11 EST Received: by plum (940406.SGI/SMI-3.2) id AA17371; Tue, 31 Jan 95 13:59:08 -0500 Date: Tue, 31 Jan 1995 13:59:08 -0500 From: Holly E Rushmeier Subject: RE: image quality metrics In-reply-to: Don Mitchell "image quality metrics" (Jan 31, 10:09am) To: Don Mitchell , globillum@cs.cmu.edu Message-id: <9501311359.ZM17369@plum.cam.nist.gov> Content-type: text/plain; charset=us-ascii X-Mailer: Z-Mail (3.1.0 22feb94 MediaMail) Mime-Version: 1.0 References: <9501311819.AA26339@netmail2.microsoft.com> Don and Greg have a good point about image quality metrics. However, sitting here at "Metrics R Us", I feel like have to respond. Clearly, there isn't ever going to be one metric that everyone agrees on, but we I think we can develop a set of metrics that are more useful than root-mean-square error. I also know that there will never be a universally accepted model of subjective response. On the other hand, we use displays that rely on a lot of models of human vision (like metamerism) that are imperfect, but do a decent job for a lot of tasks. Compression methods, like jpeg, aren't perfect, but by exploiting some simple models of vision they do a decent job for some classes of images. No one wants to compute an image by following every photon, because everyone knows you can't see a difference beyond some point. The more precise a definition you can give "beyond some point", the more efficiently you can compute the results. Ultimately, we want to generate synthetic images that we can rely on, even without the "truth" image to compare to. The ultimate purpose for a metric I think is to incorporated it into our computing techniques. As we compute our image, we can use the metric to know if we're done yet. Subjective testing is useful, but what do you have as results? How well a method A did relative to method B for a particular problem? The original "Cornell Box" experiment showed that "traditional" radiosity did a good job for that box, but obviously didn't prove that radiosity is the way to go for any arbitrary environment. Unless you can abstract the results into a mathematical model you can't apply the results to anything else. My attitude is lets look at the models people have abstracted so far for other applications. Then we can develop our own metrics to use to develop error bounds for image synthesis techniques, where, as in compression some of the bounds will be restricted to certain classes of images. From X-POP3-Rcpt: wp@stellaris Received: from mr.tuwien.ac.at by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for wp id AA07680; Tue, 31 Jan 95 22:09:45 +0100 Message-Id: <9501312109.AA07680@stellaris.cg.tuwien.ac.at> Received: from EIGVS4 by mr.tuwien.ac.at with DECNET-IN (PP) id <02621-0@mr.tuwien.ac.at>; Tue, 31 Jan 1995 22:06:31 +0100 X-Vms-To: IN%"globillum@cs.cmu.edu" To: wp@eigsg1.tuwien.ac.at From: in%ruffb%rpi.edu%eigvs4@auniw Subject: Image comparison/quality Date: Tue, 31 Jan 1995 22:06:31 +0100 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Received: from HOSTESS.GRAPHICS.CS.CMU.EDU by Pap.UniVie.AC.AT (PMDF #12401) id <01HMIFSDIUFK9YECVL@Pap.UniVie.AC.AT>; Tue, 31 Jan 1995 22:05 GMT+0100 Received: from RI.CMU.EDU by HOSTESS.GRAPHICS.CS.CMU.EDU id aa01053; 31 Jan 95 15:52:25 EST Received: from mail1.its.rpi.edu by RI.CMU.EDU id aa13950; 31 Jan 95 15:51:40 EST Received: from goya.its.rpi.edu (ruffb@goya.its.rpi.edu [128.113.100.15]) by mail1.its.rpi.edu (8.6.9/8.6.4) with ESMTP id PAA00796 for ; Tue, 31 Jan 1995 15:51:11 -0500 Received: (ruffb@localhost) by goya.its.rpi.edu (8.6.9/8.6.4) id PAA00367 for globillum@cs.cmu.edu; Tue, 31 Jan 1995 15:50:56 -0500 Date: Tue, 31 Jan 1995 15:50:56 -0500 From: Barry Carlton Ruff Subject: Image comparison/quality To: globillum@cs.cmu.edu Message-id: <199501312050.PAA00367@goya.its.rpi.edu> More image comparison/quality thoughts... The textbook "Flat-Panel Displays and CRTs" has an excellent chapter entitled "Image Quality: Measures and Visual Performance" by Harry Snyder. He characterizes a number of pixel error measures of image quality ( primarily based on mean square error, some weighted by properties of the human visual system ). The real strength of the chapter though is it's coverage of techniques that use the Modulation Transfer Function of display systems to obtain spatial information that can be compared with characteristics of our visual capabilities. I agree with Holly there is a lot of info in the compression literature on this topic. I recommend also scanning the the displays literature and television journals specifically, the Society for Information Display and the Society for Motion Picture and Television Engineers ( SID and SMPTE ) both hold a high stake in developing metrics for measuring image quality. Here are a few more references: Glenn, William. Digital Image Compression Based on Visual Perception and Scene Properties. SMPTE Journal May 1993: p.392-397 Hall, Charles; Hall, Ernest. A Nonlinear Model for the Spatial Characteristics of the Human Visual System. IEEE Transactions on Systems, Man, and Cybernetics. March 1977 vSMC-7(no. 3): p.161-170 Poynton, Charles. "Gamma" and It's Disguises: The Nonlinear Mappings of Intensity in Perception, CRTs, Film and Video. SMPTE Journal. December, 1993 p.1099-1108 Statistical comparison of image data is useful but to obtain measures of image quality perceptual models will have to be incorporated. As mentioned subjective ratings may be an alternative presently but herein lies some pitfalls as well. Experimental design must be controlled to assure subjects are rating actual quality as opposed to simply preference. ( there's no accounting for taste ) I have used a pair-wise comparison where subjects are presented both a reference image and a test image and are then asked to rank their impression of the test against the reference this works out well. Perception Based Rendering, coming soon to a machine near you... Barry Ruff Lighting Research Center Rensselaer Polytechnic Institute From X-POP3-Rcpt: wp@stellaris Received: from mr.tuwien.ac.at by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for wp id AA07793; Wed, 1 Feb 95 00:27:47 +0100 Message-Id: <9501312327.AA07793@stellaris.cg.tuwien.ac.at> Received: from EIGVS4 by mr.tuwien.ac.at with DECNET-IN (PP) id <06386-0@mr.tuwien.ac.at>; Wed, 1 Feb 1995 00:24:26 +0100 X-Vms-To: IN%"globillum@cs.cmu.edu" To: wp@eigsg1.tuwien.ac.at From: in%spworley%netcom.com%eigvs4@auniw Subject: More image comparison thoughts Date: Wed, 1 Feb 1995 00:24:26 +0100 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Received: from HOSTESS.GRAPHICS.CS.CMU.EDU by Pap.UniVie.AC.AT (PMDF #12401) id <01HMIKMG47QO9YECZI@Pap.UniVie.AC.AT>; Wed, 1 Feb 1995 00:23 GMT+0100 Received: from CS.CMU.EDU by HOSTESS.GRAPHICS.CS.CMU.EDU id aa01457; 31 Jan 95 18:16:12 EST Received: from netcom13.netcom.com by CS.CMU.EDU id aa11019; 31 Jan 95 18:15:36 EST Received: by netcom13.netcom.com (8.6.9/Netcom) id PAA28690; Tue, 31 Jan 1995 15:14:21 -0800 Date: Tue, 31 Jan 1995 15:14:21 -0800 From: Steve Worley Subject: More image comparison thoughts To: globillum@cs.cmu.edu Message-id: <199501312314.PAA28690@netcom13.netcom.com> I think that a single universal image "error" metric doesn't exist, simply because one type of image deviation may be trivial for one application but horrible for another. The diversity of uses for an error metric make a universal measure impossible. Consider two images which are identical except one image has been shifted over one pixel to the right. If these images were a before and after version of a test of a compression method, you'd want to use a human perception metric of difference. Put the images side by side and any viewer would probably say "Fantastic!". But if the images were comparisons of one radiosity method with a "truth" image from extreme oversampled Monte Carlo, you'd probably look for mean squared and maximum pixel differences of some sort. Here the offset registration causes very large errors in the two images, especially at sharp horizontal intensity changes. So error metrics should be tailored to the application. I would feel that a new global illumination method would best be measured against a "known" image by simple mean squared pixel intensity differences, probably independently at each wavelength. These differneces should be in actual intensity differences if possible, not cruddy quantized 0-255 RGB values. This is a more physical, direct measurement, showing any differences at a very low level. When testing a new algorithmic method for light transport, these importances are probably the most important. A visual metric might be better for determining speedups for a specific renderer. Say I'm trying to add Greg Ward's cool method of estimating shadow coverages of hundreds of light sources to a current commerical renderer. The users of the renderer are logo pilots and general animators. If the image doesn't LOOK different, and rendering is much faster, I'm likely to have happy customers. Even if the accuracy of rendering has decreased considerably (maybe the shadow boundaries are a lot noisier, with changes of +- 10% in the correct RGB values) it doesn't matter as long as peopele viewing the image don't notice or at least notice much. Unlike pixel by pixel mean-squared differences, trying to come up with a metric for human vision is a lot trickier. One group that probably put the most work into this topic were the nameless engineers who crafted NTSC in the 50's. They had an insanely small bandwidth to pack as much image quality as they could into. They exploited our vision's weak points by allocating their bandwidth carefully. I would think that a better VISUAL metric would come from pixel by pixel differences in YUV space rather than RGB space, and weighting Y errors much more than U and U more than V, as NTSC does. This doesn't solve some problems, though: think about the case where you increase each pixel's intensity 5% uniformly. Visually the image doesn't change much, but the pixel by pixel differences all have a 5% absolute error in them. Oops. Maybe some global gamma/contrast/brightness tweaking should attempt to "match" the two images first, THEN use pixel by pixel differences. But what about nonlinear spacial intensity changes, like the ones Rushmier, Ward, and Shirley have played with? Arggh.. there's an awful lot to account for! So forming a quantitative VISUAL difference metric is, simply, a pain. I will buy dinner for anyone who can come up with a good model or two and actually compare these to human experimentation where people rate image "differences" by eye. But luckily, the more sterile question of validating an algorithm can use less subjective measures. Simple pixel by pixel mean, mean squared, and maximum errors, are enough to quickly tell wether the two algorithms agree or disagree. Especially in radiation transport, we do know how to use the right units for measurements of light flux though a solid angle, and that's all we're trying to compute accurately. Anyway, just some thoughts to keep this thread going. I'm glad I discovered this list... -Steve Worley spworley@netcom.com From X-POP3-Rcpt: wp@stellaris Received: from mr.tuwien.ac.at by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for wp id AA11244; Wed, 1 Feb 95 17:14:34 +0100 Message-Id: <9502011614.AA11244@stellaris.cg.tuwien.ac.at> Received: from EIGVS4 by mr.tuwien.ac.at with DECNET-IN (PP) id <08614-0@mr.tuwien.ac.at>; Wed, 1 Feb 1995 17:11:04 +0100 X-Vms-To: IN%"globillum@cs.cmu.edu" To: wp@eigsg1.tuwien.ac.at From: in%hwj%hwj.gk.dtu.dk%eigvs4@auniw Subject: Image comparison Date: Wed, 1 Feb 1995 17:11:04 +0100 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Received: from HOSTESS.GRAPHICS.CS.CMU.EDU by Pap.UniVie.AC.AT (PMDF #12401) id <01HMJJRWMV5C9YECW1@Pap.UniVie.AC.AT>; Wed, 1 Feb 1995 17:10 GMT+0100 Received: from CS.CMU.EDU by HOSTESS.GRAPHICS.CS.CMU.EDU id aa02466; 1 Feb 95 10:56:37 EST Received: from hwj.gk.dtu.dk by CS.CMU.EDU id aa17543; 1 Feb 95 10:55:42 EST Received: (from hwj@localhost) by hwj.gk.dtu.dk (8.6.9/8.6.9) id TAA04681 for globillum@cs.cmu.edu; Wed, 1 Feb 1995 19:44:50 +0100 Date: Wed, 1 Feb 1995 19:44:50 +0100 From: Henrik Wann Jensen Subject: Image comparison To: globillum@cs.cmu.edu Message-id: <199502011844.TAA04681@hwj.gk.dtu.dk> Hi everyone, Thanks for all the replies and an interesting discussion... I can see that it is difficult to compute just one number/error related to the 'perceptual difference' between two images. Subjective testing avoids this difficulty, but I agree with Holly that subjective testing cannot replace an error metric. Firstly, subjective testing is, well, subjective. I am used to looking at and seeing errors in a computer generated image therefore I will probably catch more errors than a person who is not working with computer graphics. I also find it quite unsatisfactory to write in a paper: ".. as we can see it looks good..". Furthermore I like to examine the effects of different parameters in my software by plotting a graph showing the convergence/error (currently the RMS-error) as a function of one of these parameters -- this is not possible with subjective testing. When comparing two images A and B we could extract a number of features from the difference image C=A-B. For instance we could examine whether C contains edges that aren't in the reference image A. We could also test whether C is noisy in areas where A is smooth etc. These features could be weighted and added together to give an error metric. I guess someone has tried this before... A good error metric could initially be used to speed up current global illumination algorithms. Perhaps improve methods featuring progressive refinement. Later on we might be able to incorporate the error metric in our algorithms in order to automatically determine when we are finished. Currently the most common stop-criteria within Monte Carlo ray tracing is the variance - which is directly related to the RMS-error. This criteria is unfortunate since we often use more samples than necessary. An example is procedural textures based on Perlins noise function. Since noise is a property of the texture and therefore not disturbing the use of variance as a stop-criteria results in unnecessary oversampling of these textures. If we had an error metric capable of saying whether the noise is disturbing or not then we could do a lot better... - Henrik From X-POP3-Rcpt: wp@stellaris Received: from mr.tuwien.ac.at by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for wp id AA12002; Wed, 1 Feb 95 21:23:42 +0100 Message-Id: <9502012023.AA12002@stellaris.cg.tuwien.ac.at> Received: from EIGVS4 by mr.tuwien.ac.at with DECNET-IN (PP) id <17647-0@mr.tuwien.ac.at>; Wed, 1 Feb 1995 21:20:33 +0100 X-Vms-To: IN%"globillum@cs.cmu.edu" To: wp@eigsg1.tuwien.ac.at From: in%donm%microsoft.com%eigvs4@auniw Subject: error metrics, color Date: Wed, 1 Feb 1995 21:20:33 +0100 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Received: from HOSTESS.GRAPHICS.CS.CMU.EDU by Pap.UniVie.AC.AT (PMDF #12401) id <01HMJSHWGESG9YEFMY@Pap.UniVie.AC.AT>; Wed, 1 Feb 1995 21:19 GMT+0100 Received: from RI.CMU.EDU by HOSTESS.GRAPHICS.CS.CMU.EDU id aa03031; 1 Feb 95 13:01:13 EST Received: from netmail2.microsoft.com by RI.CMU.EDU id aa18104; 1 Feb 95 13:00:29 EST Received: by netmail2.microsoft.com (5.65/25-eef) id AA10544; Wed, 1 Feb 95 10:00:59 -0800 Received: by netmail2 using fxenixd 1.0 Wed, 01 Feb 95 10:00:59 PST Date: Wed, 1 Feb 95 09:50:08 TZ From: Don Mitchell Subject: error metrics, color To: globillum@cs.cmu.edu Message-id: <9502011800.AA10544@netmail2.microsoft.com> X-Msmail-Message-Id: D880BBAE X-Msmail-Conversation-Id: D880BBAE Naturally, you want to have some number to minimize when you are trying various image synthesis methods. RMS error is an obvious one. But I caution against equating that number with "image quality". Variance and RMS error are actually quite poor measure of subjective image quality -- logarithmic weight or cube-root weight would even be a better measure of visible error than summing the square of the error. The spatial frequency effects the visibility of noise, with the maximum response being around 12 cycles per degree. The dependance on color is especially tricky. A common mistake in color quantization is to us Luv or Lab coordinates -- if you look at the SMTPE literature, you'll find they recommend almost the opposite metric, with a strong emphasis on reducing noise in the green channel. This is because there are really two kinds of error being talked about: color-matching error, and visibility of spatial patterns of noise. Luv is about color matching, the eye is quite insensitive to variations in shades of green, for example. But if you are worried about grain noise or dither patterns, the eye is most sensitive to green colored patterns. Getting back to metrics. Simple measures like variance or log-error might be fine for measuring the error in a pixel. But you certainly need more complex metrics if you are looking at global noise characteristics. RMS error was not at all useful in the work I reported in my SIGGRAPH 91 paper on spectrally optimal sampling, but I think the images clearly demonstrated the value of forcing noise into high frequencies. I used the Mannos Sakrison metric at that time and found the results to be poorly correlated with subjective image quality. For me, seeing is believing, and I did not use the M&S numbers. From X-POP3-Rcpt: wp@stellaris Received: from mr.tuwien.ac.at by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for wp id AA16372; Fri, 3 Feb 95 01:48:39 +0100 Message-Id: <9502030048.AA16372@stellaris.cg.tuwien.ac.at> Received: from EIGVS4 by mr.tuwien.ac.at with DECNET-IN (PP) id <04697-0@mr.tuwien.ac.at>; Fri, 3 Feb 1995 01:45:22 +0100 X-Vms-To: IN%"globillum@cs.cmu.edu" To: wp@eigsg1.tuwien.ac.at From: in%t-jackt%microsoft.com%eigvs4@auniw Subject: A perceptual image metric (monochrome) Date: Fri, 3 Feb 1995 01:45:22 +0100 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Received: from HOSTESS.GRAPHICS.CS.CMU.EDU by Pap.UniVie.AC.AT (PMDF #12401) id <01HMLG1TAZZK9YEJHN@Pap.UniVie.AC.AT>; Fri, 3 Feb 1995 01:44 GMT+0100 Received: by HOSTESS.GRAPHICS.CS.CMU.EDU id aa11302; 2 Feb 95 19:43:49 EST Received: from EDRC.CMU.EDU by HOSTESS.GRAPHICS.CS.CMU.EDU id aa11266; 2 Feb 95 19:26:20 EST Received: from netmail2.microsoft.com by EDRC.CMU.EDU id aa00800; 2 Feb 95 19:25:53 EST Received: by netmail2.microsoft.com (5.65/25-eef) id AA24865; Thu, 2 Feb 95 16:26:26 -0800 Received: by netmail2 using fxenixd 1.0 Thu, 02 Feb 95 16:26:25 PST Date: Thu, 2 Feb 95 16:21:14 TZ From: Jack Tumblin Subject: A perceptual image metric (monochrome) To: globillum@cs.cmu.edu Message-id: <9502030026.AA24865@netmail2.microsoft.com> X-Msmail-Message-Id: 40CF4B1B X-Msmail-Conversation-Id: 40CF4B1B P. Teo & D. Heeger at Stanford have a promising perceptual image metric. They try to model the response of directionally- selective cells in the striate cortex using modified image pyramids and steerable filters, so that noise patterns that are aligned with nearby image features contribute much less error than misaligned noise. It is rather elaborate, but built on solid results from psychophysics and physiology. Their example pictures are impressive. See: "Perceptual Image Distortion", Teo, Patrick C., and Heeger, David J., pp.982-986 Proceedings of First International Conference on Image Processing, Austin TX, Nov. 1994. It's monochrome, though, and assumes moderate, CRT-like luminances-- not intended for high-dynamic range images. Regards, -Jack Tumblin From X-POP3-Rcpt: wp@stellaris Received: from mr.tuwien.ac.at by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for wp id AA07565; Tue, 7 Feb 95 18:19:47 +0100 Message-Id: <9502071719.AA07565@stellaris.cg.tuwien.ac.at> Received: from EIGVS4 by mr.tuwien.ac.at with DECNET-IN (PP) id <10656-0@mr.tuwien.ac.at>; Tue, 7 Feb 1995 18:15:22 +0100 X-Vms-To: IN%"globillum@imag.fr" To: wp@eigsg1.tuwien.ac.at From: in%francois.sillion%imag.fr%eigvs4@auniw Subject: IMPORTANT: address change for globillum Date: Tue, 7 Feb 1995 18:15:22 +0100 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Received: from isis.imag.fr by Pap.UniVie.AC.AT (PMDF #12401) id <01HMRZRERHB49YERWB@Pap.UniVie.AC.AT>; Tue, 7 Feb 1995 18:14 GMT+0100 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.9/8.6.9) with ESMTP id QAA04717 for ; Tue, 7 Feb 1995 16:01:22 +0100 Received: from safran (safran.imag.fr [129.88.29.1]) by imag.imag.fr (8.6.9/8.6.9) with ESMTP id PAA28345 for ; Tue, 7 Feb 1995 15:36:25 +0100 Received: from localhost (sillion@localhost) by safran (8.6.4/8.6.4) id PAA23698 for globillum@imag.fr; Tue, 7 Feb 1995 15:36:10 +0200 Date: Tue, 7 Feb 1995 15:36:10 +0200 (MET) From: Francois Sillion Subject: IMPORTANT: address change for globillum To: globillum@imag.fr (Global Illumination List) Reply-to: Francois.Sillion@imag.fr Message-id: <199502071336.PAA23698@safran> Content-type: text/plain; charset=ISO-8859-1 Content-transfer-encoding: 8bit X-Mailer: ELM [version 2.4 PL23] MIME-Version: 1.0 Content-Length: 20423 Dear fellow globillumers, The 'globillum' mailing list has been in existence for almost five years! Paul Heckbert has offered a great service to our community by setting up and maintaining the list for all this time. He deserves a rest and I will be taking over the maintenance of the list. Before I go on to explain what it means for you, I suggest we all thank Paul for his efforts: (one, two, three...) THANKS A LOT, PAUL ! OK, here's the technical information. The address used to send mail to the entire group has changed: it is now globillum@imag.fr The address used to contact me for matters pertaining to this list (such as adding new members, mail address problems, etc..) is now globillum-request@imag.fr I am appending below a copy of the mailing list in the form of a mailrc file. Please take the time to modify your globillum alias NOW, to avoid unnecessary traffic at the old address. You do not need to include all the aliases in the list in your .mailrc if you only want to contact the group. The prefered way to contact the entire group is always to use the globillum address, to ensure that the most up-to-date list is used. For thos of you using ELM to read/send mail, an elm alias database is also available by ftp (see below). Previous discussions among us (over 800k bytes of it) and a current copy of the mailing list are available via ftp at any time: ftp safran.imag.fr NAME: anonymous PASSWORD: yourlogin cd /pub/sillion/globillum ls prompt mget * quit and if the name server doesn't know the machine number, use ftp 129.88.29.1 Or if you can't ftp, tell me and I'll mail them to you. I hope the transition will be smooth, please let me know if there are any problems. +------------------+---------------------------+--------------------------+ | | iMAGIS / IMAG | Tel: (+33) 76 51 43 54 | | Francois SILLION | B.P. 53 | Fax: (+33) 76 44 66 75 | | ' | F-38041 Grenoble Cedex 09 | Francois.Sillion@imag.fr | +------------------+---------------------------+--------------------------+ The current members list follows in the form of a .mailrc file. # GLOBAL ILLUMINATION MAILING LIST, 2 Feb 95 # append the following to your .mailrc file # # send corrections/additions to globillum-request@imag.fr # (which is forwarded to Francois Sillion) # The preferred way to send mail to everyone on the list is to mail to # globillum (aliased below), where a master copy of list is being maintained. alias globillum globillum@imag.fr alias globillum-request globillum-request@imag.fr # lines beginning with "# #" are people who are not on the list as # individuals, but are members of a group that subscribes alias globillum_explicit \ allison almagro amanatides arvo ashdown baum bhate borel \ bouatouch buckalew cabrero campbell carlton casasayas achalmers \ chen nchristensen pchristensen christou mcohen compagnon \ cornell_students costa jdave delft desousa dilaura dorsey \ drettakis fiume forsyth fournier fussell gatenby george gifford \ glassner goel grant greenberg guenther guibas haines \ hanrahan heal heckbert hedley ivanov jensen jessel gjones kaneda kirk \ kolb kopp kouhia lalonde languenou levoy blewis plewis lightwork \ marini max metge dmitchell newhall anewton nishita patmore \ pattanaik paulin pela pharr poulin puech pueyo purgathofer rekola \ ruff rushmeier salesin schlick pschroeder \ scopigno seron shinya shirley gimagis sillion \ slusallek speer spencer stolfi stollnitz stuerzlinger ksubramanian \ sung tampieri teller tellier townsend \ troutman tumblin turner uselton vanliere \ vanwyk veach vilaplana jwallace cwang ward westin wexler \ winget worley worrall zhang zisserman zumtobel # Mike Allison alias allison mike@documentum.com # Carlos Urena Almagro; ETS Ingenieria Informatica; # Universidad de Granada; 18071 Granada; Spain alias almagro almagro@ugr.es # John Amanatides, York U, Toronto alias amanatides amana@cs.yorku.ca # Jim Arvo, Apollo / Yale alias arvo arvo@graphics.cornell.edu # Ian Ashdown; Ledalite Architectural Products Inc.; Langley, B.C.; Canada alias ashdown 72060.2420@CompuServe.COM alias ashdown2 Ledalite@mindlink.bc.ca # Dan Baum, Silicon Graphics alias baum drb@sgi.com # Neeta Bhate; University of South Florida; Tampa, Florida alias bhate bhate@sol.csee.usf.edu # Chris Borel; SST-8, MS D438; Los Alamos National Lab; Los Alamos, NM 87545 # interests: simulation of lighting under vegetative canopies alias borel cborel@lanl.gov # Kadi Bouatouch; IRISA; Campus de Beaulieu; 35042 Rennes Cedex; France # interests: ray tracing, sampling, realism, physics & perception alias bouatouch kadi@irisa.fr alias bouatouch2 bouatouch@irisa.fr # # Wim F. Bronsvoort; Faculty of Technical Mathematics and Informatics; # Delft University of Technology; Julianalaan 132; 2628 BL Delft; Netherlands alias bronsvoort wim@duticg.twi.tudelft.nl # Chris Buckalew, Cal Poly alias buckalew buckalew@polyslo.calpoly.edu # Alan Cabrero; 514 Computer Center; East Lansing MI 48824 alias cabrero adc@tardis.cl.msu.edu # Alvin T. Campbell III; Applied Research Laboratories; U. of Texas at Austin; # P. O. Box 8029; Austin, TX 78713-8029 # interests: global illumination, heat transfer, animation, scientific vis. alias campbell atc@arlut.utexas.edu # Eloise Carlton, Fujitsu America alias carlton eloisec@ossi.com # Mateu Sbert Casasayas # interests: doing thesis on Monte Carlo radiosity alias casasayas sbert@lsi.upc.es # Alan Chalmers; Dept. of Computer Science; University of Bristol; # University Walk; Bristol; BS8 1TR; United Kingdom # interests: large parallel MIMD computers for radiosity and ray tracing alias achalmers alan@compsci.bristol.ac.uk alias achalmers2 alan@cs.bris.ac.uk # Eric Chen, Apple alias chen chense@apple.com # Niels J. Christensen; Technical U. Denmark; B. 116, DK-2800 Lyngby; Denmark alias nchristensen iftnjc83@vm.uni-c.dk # Per H. Christensen; U. of Washington # interests: light reflection models, image analysis & synthesis alias pchristensen per@cs.washington.edu # Chris Christou, Oxford U. alias christou cgc@physiology.oxford.ac.uk # Michael Cohen, Princeton U. alias mcohen mfc@cs.princeton.edu # Raphael Compagnon, EPFL Switzerland alias compagnon compagnon@eldp.epfl.ch # Antonio Costa; Comp. Graphics & CAD; INESC; # Largo Mompilher 22; 4100 Porto Portugal alias costa acosta@porto.inescn.pt # alias costa acc@asterix.inescn.pt (this address failing 1/95) # Cornell Students, includes Himlan & others; but not Greenberg or Arvo alias cornell_students gi-students@graphics.cornell.edu # Jubin P. Dave; U. of New Hampshire alias jdave jd@kepler.unh.edu # Delft University of Technology graphics group # an alias for Jansen, Bronsvoort, Kok, Post # interests: VLSI for radiosity; ray tracing, texture mapping, CSG alias delft globillum@duticg.twi.tudelft.nl # A. Augusto de Sousa; INESC; Largo Mompilher, 22; 4000 Porto; Portugal alias desousa aa_sousa@inescn.pt # David L. DiLaura; Senior Instructor, Civil and Architectural Engineering; # University of Colorado; Boulder, CO 80309 alias dilaura dilaura@bechtel.colorado.edu # Julie Dorsey; Assistant Professor, Architecture, MIT alias dorsey dorsey@mit.edu # George Drettakis, iMAGIS/IMAG, BP 53 F-38041 Grenoble Cedex 09 France # interests: sampling and filtering techniques for GI, quality & error metrics alias drettakis George.Drettakis@imag.fr # Eugene Fiume, U. of Toronto alias fiume elf@dgp.utoronto.ca # David Forsyth alias forsyth daf@CS.Berkeley.EDU # Alain Fournier, U. of British Columbia, Vancouver BC, Canada alias fournier fournier@cs.ubc.ca # Don Fussell, U. of Texas, Austin alias fussell fussell@cs.utexas.edu # Neil Gatenby, Manchester Computing Centre, Manchester, England # interests: alternatives to hemicube, accurate numerical form factors alias gatenby gatenby@vax3.graphics.manchester-computing-centre.ac.uk # David George, Gain Technology, Palo Alto alias george george@gain.com # Stephen Gifford, Electrical and Computer Engineering Dept, Carnegie Mellon # interests: implemented radiosity/ray tracing hybrid on Connection Machine alias gifford Stephen.Gifford@maps.cs.cmu.edu # Andrew Glassner, Microsoft alias glassner glassner@microsoft.com # Narendra Goel, Wayne State U. alias goel ngoel@pandora.cs.wayne.edu # Chuck Grant, Lawrence Livermore Lab alias grant grant1@llnl.gov alias grant2 grant%delvalle.llnl.gov@lll-lcc.llnl.gov # Don Greenberg c/o Fran Brown, Cornell U. alias greenberg fmb@graphics.cornell.edu # Nico Guenther; Universitaet Rostock; Fachbereich Informatik; # Rostock 18059; Germany # interests: animation of radiosity, physically based approaches, perception alias guenther nic@informatik.uni-rostock.de # Leo Guibas; CS Dept, Stanford U. / DEC Systems Research Center, Palo Alto alias guibas guibas@cs.stanford.edu # Eric Haines, 3D/Eye alias haines erich@eye.com # Pat Hanrahan, Stanford U. alias hanrahan hanrahan@cs.stanford.edu # Brian W. Heal; School of Information Science; Portsmouth Polytechnic; # Mercantile House; Hampshire Terrace; Portsmouth, PO1 2EG; United Kingdom # interests: rendering octree models, post-hidden-surface-removal rendering alias heal healb@csovax.portsmouth.ac.uk # Paul Heckbert; Computer Science Dept.; Carnegie Mellon University; # 5000 Forbes Ave; Pittsburgh PA 15213-3891; USA # interests: finite element & integral equation methods for global illumination alias heckbert ph@cs.cmu.edu # David Hedley alias hedley hedley@cs.bris.ac.uk # # Ted H. Himlan, Cornell # interests: empirical measurements of materials and lights, validation alias himlan thh@graphics.cornell.edu # Alexander Ivanov alias ivanov Alexander.Ivanov@comlab.ox.ac.uk # # Frederik W. Jansen (Erik); Faculty of Technical Mathematics and Informatics; # Delft University of Technology; Julianalaan 132; 2628 BL Delft; Netherlands alias jansen fwj@duticg.twi.tudelft.nl # Henrik Wann Jensen; Institute of Graphical Communication # Technical University of Denmark; Building 116; 2800 Lyngby; Denmark alias jensen igkhwj@unidhp.uni-c.dk # J. P. Jessel; Institut de Recherche en Informatique de Toulouse; # Universite Paul Sabatier; 31062 Toulouse; France # interests: parallel radiosity and ray tracing algorithms on Transputers alias jessel jessel@irit.fr # Graham Jones; Oxford U. alias gjones graham@robots.oxford.ac.uk # Kazufumi Kaneda; Electric Machinery Lab, Hiroshima U. alias kaneda kin@eml.hiroshima-u.ac.jp # Dave Kirk, Caltech alias kirk dk@egg.gg.caltech.edu # # Arjan Kok; Delft U. of Technology; Netherlands # interests: radiosity effects using ray tracing alias kok arjan@duticg.twi.tudelft.nl # Craig Kolb, Stanford (but email address is Princeton) alias kolb cek@cs.princeton.edu # Manfred Kopp; Inst. of Computer Graphics, Technical University of Vienna # Karlsplatz 13/186-2; A-1040 Wien; Austria alias kopp kopp@stellaris.cg.tuwien.ac.at alias kopp2 m.kopp@ieee.org alias kopp3 kopp@eigvs4.una.ac.at # alias kopp kopp@eigvs4.tuwien.ac.at # Juhana Kouhia alias kouhia jk87377@cs.tut.fi # Paul Lalonde, U. of British Columbia alias lalonde lalonde@cs.ubc.ca # Eric Languenou; IRISA; Projet Siames; Campus de Beaulieu; # 35042 Rennes Cedex France # interests: participating media, adaptive radiosity; doing PhD with Bouatouch alias languenou langueno@irisa.fr # Marc Levoy, CS Dept, Stanford U. alias levoy levoy@cs.stanford.edu # Bob Lewis; CS Dept; U. of British Columbia; # 6356 Agricultural Road; Vancouver, BC V6T 1W5; Canada # interests: 3-D texture, ray tracing, radiosity, parallelism alias blewis bobl@cs.ubc.ca # Lewis; Dept. Geography; University College London # 26 Bedford Way; London WC1H 0AP; UK # I don't use a first name, "I'm known just as Lewis" # interests: modeling canopy reflectance, remote sensing alias plewis plewis@ps.ucl.ac.uk # people at LightWork Design; Cooper Bldgs.; Arundel Street; # Sheffield, S1 2NS; UK alias lightwork radios@lightwork.co.uk # Daniele Marini; Eidomatics Lab, Computer Science Dept, Univ. of Milan; Italy # interests: radiosity, ray tracing, parallel processing (Meiko) alias marini marini@imiucca.csi.unimi.it # Nelson Max, Lawrence Livermore Lab alias max max2@llnl.gov alias max2 nelson@ramius.ocf.llnl.gov # Christian Metge; Institut de Recherche en Informatique de Toulouse; # Universite Paul Sabatier; 31062 Toulouse; France # interests: parallel discrete radiosity and ray tracing algorithms # (Transputers, workstation networks) alias metge metge@irit.fr # Don Mitchell, Microsoft alias dmitchell donm@microsoft.com # # Eihachiro Nakamae; Electric Machinery Lab, Hiroshima U. alias nakamae naka@eml.hiroshima-u.ac.jp # William Parsons Newhall, Jr., The American University alias newhall newhall@auvm.american.edu # Andy Newton; Remote Sensing Research, University College London alias anewton anewton@ps.ucl.ac.uk # Tomoyuki Nishita; Electric Machinery Lab, Hiroshima U. alias nishita nis@eml.hiroshima-u.ac.jp # Christopher Patmore; Programming Research Group; Oxford U. # interests: skylight radiosity alias patmore cjp@prg.oxford.ac.uk # Sumant Narayan Pattanaik; IRISA; Rennes; France alias pattanaik sumant.pattanaik@irisa.fr # Mathias Paulin; Institut de Recherche en Informatique de Toulouse; # Universite Paul Sabatier; 31062 Toulouse; France # interests: parallel radiosity and ray tracing algorithms (Transputers, PVM) # shadow accuracy, transfer simulations in dense foliage alias paulin paulin@irit.fr # Barbara Pela, Joint Research Centre, Commission of the European Communities, # Ispra, Italy alias pela barbara.pela@cen.jrc.it # Matt Pharr alias pharr mmp@lux.Stanford.EDU # # Frits Post; Faculty of Technical Mathematics and Informatics; # Delft University of Technology; Julianalaan 132; 2628 BL Delft; Netherlands alias post frits@duticg.twi.tudelft.nl # Pierre Poulin; Dept. IRO, Universite de Montreal, # C.P. 6128, succ. Centre-Ville, Montreal, Quebec, Canada H3C 3J7 # interests: illumination, rendering, realism alias poulin poulin@iro.umontreal.ca # Claude Puech; LIENS; 45, rue d'Ulm; 75230 Paris Cedex 05; France alias puech Claude.Puech@imag.fr # Xavier Pueyo; Dept. Llenguatges i Sistemes Informatics; # Universitat Politecnica de Catalunya; Av. Diagonal, 647 planta 8; # 08028-Barcelona; Spain; # interests: diffuse environments alias pueyo xavier@ima.udg.es alias pueyo2 xavier@lsi.upc.es alias pueyo3 eapueyo@ebrupc51.bitnet # Werner Purgathofer; Institute for Computer Graphics; Techn. Univ. Vienna; # Karlsplatz 13 / 186; A-1040 Wien / Austria # interests: parallel ray tracing and radiosity, BSP, color, animation # [I've had trouble with most of Werner's email addresses! -Paul H.] alias purgathofer purgathofer@eigvs4.una.ac.at alias purgathofer2 purgathofer@eigvs4.tuwien.ac.at alias purgathofer3 wp@eigcl1.una.ac.at # Panu Rekola; Computer Science Dept, Helsinki U. of Tech.; Finland alias rekola pre@cs.hut.fi # Barry Carlton Ruff alias ruff ruffb@rpi.edu # Holly Rushmeier, Computing and Applied Math Lab; # National Institute for Standards and Technology; Gaithersburg, Maryland alias rushmeier holly@cam.nist.gov # David Salesin; U. of Washington alias salesin salesin@cs.washington.edu # # Jodok Schaeffler, Zumtobel, Austria alias schaeffler js@cophos.co.at # Christophe Schlick; LaBRI; U. of Bordeaux; 351 Cours de la Liberation # 33400 Talence; France # interests: ray tracing, radiosity, antialiasing, general reflectance functions alias schlick schlick@labri.u-bordeaux.fr alias schlick2 schlick@geocub.greco-prog.fr # Peter Schroeder alias pschroeder ps@math.scarolina.edu # Roberto Scopigno; CNUCE; Consiglio Nazionale delle Richerche; # Via S.Maria, 36; 56100 Pisa; Italy # interests: volume rendering, user interfaces, parallel processing, geography alias scopigno R.Scopigno@cnuce.cnr.it # Francisco Seron; Dpto. Ingenieria Electrica e Informatica; # Centro Politecnico Superior de Ingenieros; Universidad de Zaragoza; # C/ Maria Luna s/n; E-50015 Zaragoza; Spain alias seron pseron@mcps.unizar.es # Mikio Shinya, pencil tracing alias shinya shinya@nttarm.ntt.jp # alias shinya shinya@nttcvg.ntt.jp # Pete Shirley, Indiana U., on leave at Cornell as of 7/94 alias shirley shirley@graphics.cornell.edu alias shirley2 shirley@iuvax.cs.indiana.edu # Global Illumination group at iMAGIS/IMAG alias gimagis gimagis@safran.imag.fr # Francois Sillion; IMAG; Grenoble; France alias sillion Francois.Sillion@imag.fr # Philipp Slusallek; Universitaet Erlangen; # IMMD IX - Graphische Datenverarbeitung; Am Weichselgarten 9; # W-8520 Erlangen, Germany # interests: CAD, surfaces, doing PhD on physical basis of glob. illum. alias slusallek slusallek@informatik.uni-erlangen.de # Rick Speer alias speer speer@crl.com alias speer2 speer@cs.colorado.edu # Stephen Spencer alias spencer spencer@cgrg.ohio-state.edu # Jorge Stolfi alias stolfi stolfi@dcc.unicamp.br # Eric Stollnitz alias stollnitz stoll@amath.washington.edu # Wolfgang Stuerzlinger, Department of Graphics and Parallel Processing, # Johannes Kepler University, Linz, Austria alias stuerzlinger wrzl@gup.uni-linz.ac.at # K. R. Subramanian; AT&T Bell Labs; Murray Hill, NJ alias ksubramanian krs@allegra.att.com # Kelvin Sung; Dept. of Information Systems and Computer Science; # National University of Singapore; Kent Ridge, Singapore 0511 # Republic of Singapore # interests: fast ray tracing, modular global illumination software alias sung ksung@iscs.nus.sg # Filippo Tampieri; Lightscape Technologies, Inc; San Jose, CA alias tampieri fxt@lightscape.com # Seth Teller; MIT alias teller seth@lcs.mit.edu # Pierre Tellier # LSIIT (Laboratoire des Sciences de l'Image, d'Informatique et de # Teledetection); Departement d'Informatique de l'Universite Louis Pasteur; # 7, rue R. Descartes; 67084 Strasbourg; France alias tellier tellier@dpt-info.u-strasbg.fr # J. Eric Townsend; General Magic # interests: massively parallel based visualization codes, mostly ray tracing alias townsend jet@genmagic.com # Roy Troutman, Lawrence Livermore Lab alias troutman roy@ninja.nersc.gov alias troutman2 roy@ninja.llnl.gov # Jack Tumblin, Georgia Tech alias tumblin ccsupjt@cc.gatech.edu # Doug Turner, Apple alias turner turner@apple.com # Sam Uselton; CSC, NASA Ames, Mountain View, CA alias uselton uselton@nas.nasa.gov # Robert van Liere; Department of Interactive Systems; # Center for Mathematics and Computer Science (CWI); # Kruislaan 413, 1098 SJ Amsterdam, The Netherlands # interests: generalizing radiosity method, parallel methods for radiosity alias vanliere robertl@cwi.nl # Cornelius Skip Van Wyk, Jr; Carnegie Mellon U; Dept of Architecture alias vanwyk vanwyk@cad.cs.cmu.edu # Eric Veach; Stanford U. # interests: hierarchical global illumination, clustering objects, # global illumination methods for "black box" scene representations alias veach ericv@cs.stanford.edu # Josep Vilaplana; Universitat Politecnica de Catalunya; # Departament de Llenguatges i Sistemes Informatics; # Av. Diagonal 647 planta 8; 08028 Barcelona; Spain # interests: hardware and parallel algs for speeding radiosity & ray tracing alias vilaplana vilaplana@lsi.upc.es # John Wallace, 3D/Eye alias jwallace johnw@eye.com # Changyaw Wang; U. of Indiana # interests: rendering and modeling of complex outdoor environments alias cwang wangc@iuvax.cs.indiana.edu # Greg Ward; Lighting Systems Research Group; Lawrence Berkeley Lab; California alias ward gjward@lbl.gov # Stephen H. Westin alias westin westin@dsg42.nad.ford.com # Dan Wexler; Berkeley alias wexler wex@miro.berkeley.edu # Jim Winget, Silicon Graphics alias winget jmw@sgi.com # Steve Worley alias worley spworley@netcom.com # Adam Worrall, University of Bristol Graphics Group # Computer Science Department, The University, Bristol, UK alias worrall Adam.Worrall@bristol.ac.uk # Ning Zhang # interests: radiosity, ray tracing, physically-based illumination models alias zhang zhang@vti.com # Andrew Zisserman; Robotics Research Group; Oxford University; UK # interests: computer vision, radiosity alias zisserman az@robots.oxford.ac.uk # Zumtobel Licht GmbH; Schweizerstr. 30; A-6850 Dornbirn; Austria # interests: lighting design visualization, radiosity # (an alias for global illumination folks at the Zumtobel company) alias zumtobel glbi@cophos.co.at # END OF GLOBAL ILLUMINATION MAILING LIST From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for kopp id AA15316; Fri, 24 Feb 95 11:09:20 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.10/8.6.9) with ESMTP id KAA15325 for ; Fri, 24 Feb 1995 10:39:41 +0100 Received: from sesame.imag.fr (sesame.imag.fr [129.88.29.83]) by imag.imag.fr (8.6.10/8.6.9) with ESMTP id KAA15574 for ; Fri, 24 Feb 1995 10:39:40 +0100 Received: from localhost (sillion@localhost) by sesame.imag.fr (8.6.4/8.6.4) id KAA21073 for globillum@imag.fr; Fri, 24 Feb 1995 10:35:58 +0200 From: Francois Sillion Message-Id: <199502240835.KAA21073@sesame.imag.fr> Subject: looking for 3D data of human head To: Global Illumination List Date: Fri, 24 Feb 1995 10:35:55 +0200 (MET) Reply-To: Francois.Sillion@imag.fr X-Mailer: ELM [version 2.4 PL23] Mime-Version: 1.0 Content-Type: text/plain; charset=windows-1252; format=flowed Content-Transfer-Encoding: 8bit X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Dear all, this is not really a globillum question, but I am sure many of you probably can help me with this request. I am trying to locate a 3D dataset of a human head. I am in fact only interested in the skull at the moment, but I figured I could extract it easily from any of the medical datasets that have been floating around. Unfortunately I haven't been able to do so with the head dataset from the UNC ftp site. More precisely I haven't been able to extract the skull from the data with simple classification tools. Maybe I am doing something wrong, or maybe the MRI data is not well suited to the particular classification I need ? can somebody confirm or deny this? Anyway, my questions are o would somebody have a pre-classified volume dataset of a skull? o would somebody have a volume dataset of a head that seems easy enough to classify so that the skull can be separated? maybe CT data would be better than MRI? Thanks in advance +------------------+---------------------------+--------------------------+ | | iMAGIS / IMAG | Tel: (+33) 76 51 43 54 | | Francois SILLION | B.P. 53 | Fax: (+33) 76 44 66 75 | | ' | F-38041 Grenoble Cedex 09 | Francois.Sillion@imag.fr | +------------------+---------------------------+--------------------------+ From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for kopp id AA16788; Fri, 24 Feb 95 15:31:54 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.10/8.6.9) with ESMTP id OAA26627 for ; Fri, 24 Feb 1995 14:14:40 +0100 Received: from dns004.ford.com (dns004.ford.com [198.111.80.22]) by imag.imag.fr (8.6.10/8.6.9) with ESMTP id OAA20876; Fri, 24 Feb 1995 14:14:37 +0100 Received: from dsg145.nad.ford.com (dsg145.nad.ford.com [19.4.96.29]) by dns004.ford.com (8.6.7/8.6.6) with SMTP id IAA08625; Fri, 24 Feb 1995 08:14:21 -0500 Received: by dsg145.nad.ford.com (931110.SGI/930416.SGI.AUTO) for globillum@imag.fr id AA24203; Fri, 24 Feb 95 08:14:22 -0500 Date: Fri, 24 Feb 95 08:14:22 -0500 From: "Stephen H. Westin" Message-Id: <9502241314.AA24203@dsg145.nad.ford.com> To: Francois.Sillion@imag.fr Cc: globillum@imag.fr In-Reply-To: <199502240835.KAA21073@sesame.imag.fr> (message from Francois Sillion on Fri, 24 Feb 1995 10:35:55 +0200 (MET)) Subject: Re: looking for 3D data of human head Reply-To: westin@dsg145.nad.ford.com X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit > Unfortunately I haven't been able to do so with the head dataset > from the UNC ftp site. More precisely I haven't been able > to extract the skull from the data with simple classification tools. > Maybe I am doing something wrong, or maybe the MRI data is not well > suited to the particular classification I need ? can somebody confirm > or deny this? > > Anyway, my questions are > > o would somebody have a pre-classified volume dataset of a skull? > o would somebody have a volume dataset of a head that seems easy > enough to classify so that the skull can be separated? > maybe CT data would be better than MRI? I think that's exactly correct: CT is best at distinguishing bone, and MRI was developed to look at soft tissue. I have an old friend who used to be involved with nuclear medicine sorts of things, and I'll ask him if he has any skulls lying around. -Steve From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for kopp id AA17542; Fri, 24 Feb 95 19:43:59 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.10/8.6.9) with ESMTP id TAA16691 for ; Fri, 24 Feb 1995 19:18:30 +0100 Received: from mail.uncc.edu (mail.uncc.edu [152.15.10.135]) by imag.imag.fr (8.6.10/8.6.9) with ESMTP id TAA29929; Fri, 24 Feb 1995 19:18:28 +0100 Received: from uncc.edu (bach.uncc.edu [152.15.30.15]) by mail.uncc.edu (8.6.4/8.6.4) with SMTP id NAA27681; Fri, 24 Feb 1995 13:18:04 -0500 Received: from strauss.uncc.edu (strauss.cs.uncc.edu) by uncc.edu (5.0/mail.byaddr) id AA05678 for westin@dsg145.nad.ford.com; Fri, 24 Feb 1995 13:13:05 +0500 Received: by strauss.uncc.edu (5.0/) id AA09154 for globillum@imag.fr; Fri, 24 Feb 1995 13:18:35 +0500 Message-Id: <9502241818.AA09154@strauss.uncc.edu> From: "K. R. Subramanian" Date: Fri, 24 Feb 1995 13:18:34 GMT+447 X-Mailer: Mail User's Shell (7.1.1 5/02/90) To: westin@dsg145.nad.ford.com, Francois.Sillion@imag.fr Subject: Re: looking for 3D data of human head Cc: globillum@imag.fr X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit On Feb 24, 8:14am, globillum-request@imag.fr wrote: > I think that's exactly correct: CT is best at distinguishing bone, and > MRI was developed to look at soft tissue. > > I have an old friend who used to be involved with nuclear medicine > sorts of things, and I'll ask him if he has any skulls lying around. ^^^^^^^^^^ What kind of a lab is this with a bunch of skulls lying around?? Anyway, that was pretty funny.. -- krs > > -Steve > > >-- End of excerpt from globillum-request@imag.fr -- K.R.Subramanian Phone: (704) 547-4872 Computer Science Department FAX: (704) 547-3516 The University of N.Carolina at Charlotte email : krs@strauss.uncc.edu Charlotte, NC 28223 From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for kopp id AA26591; Mon, 27 Feb 95 15:52:28 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.10/8.6.9) with ESMTP id PAA04597 for ; Mon, 27 Feb 1995 15:14:01 +0100 Received: from eye.com (eye.com [149.54.1.2]) by imag.imag.fr (8.6.10/8.6.9) with SMTP id PAA16471 for ; Mon, 27 Feb 1995 15:13:54 +0100 Received: from hemlock.eye.com by eye.com with SMTP (1.36.108.4/16.2) id AA18135; Mon, 27 Feb 1995 09:13:41 -0500 Received: by hemlock (1.37.109.8/15.6) id AA22176; Mon, 27 Feb 1995 09:13:41 -0500 Date: Mon, 27 Feb 1995 09:13:41 -0500 From: Eric Haines Message-Id: <9502271413.AA22176@hemlock> To: globillum@imag.fr Subject: new theses X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Globillumer, Here are the abstracts of two new articles on radiosity which may be of interest. These were sent to me automagically by the Elib server at Stanford, which I highly recommend for keeping you informed about various keywords - it's simple to set up and non-intrusive. Send "help" to the address at the bottom of the message if you're interested (there's also a Usenet news searcher that Stanford runs which scans netnews for articles with your keyword and sends you the first 20 lines of each article - handy if you don't have time to read netnews but still would like to track a few special topics. The address for it is netnews@db.stanford.edu). Eric Haines Score : 100 BIB-VERSION:: CS-TR-v2.0 ID:: PRINCETONCS//TR-473-94 ENTRY:: February 21, 1995 ORGANIZATION:: Princeton University, Computer Science Department LANGUAGE:: English TITLE:: Wavelet Methods for Computer Graphics (Thesis) AUTHOR:: Gortler, Steven J. DATE:: January 1995 PAGES:: 183 ABSTRACT:: This thesis discusses how a wavelet basis can be used in the context of two computer graphics applications, realistic rendering and geometric modeling, to produced more efficient and flexible algorithms. The goal of realistic rendering is to simulate the interreflection of light in some geometric environment in order to produce realistic images. Radiosity is a commonly used solution method for this problem. Recently Hanrahan et al. have introduced a hierarchical method that can solve radiosity problems in $O(n)$ time instead of $O(n^2)$. This thesis explores how the hierarchical radiosity algorithm can be formally understood from the context of wavelet theory. When the radiosity problem is expressed with respect to a wavelet basis, the resulting linear system is sparse, with only $O(n)$ significant terms. By casting the hierarchical method in this framework, a variety of wavelet basis functions can be used, resulting in more efficient radiosity methods. This thesis also discusses how wavelets can be used in the context of geometric modeling. Geometric modeling is the study of how geometric shapes can be represented and manipulated by a designer. This thesis explores the use of wavelets to represent parametric curves and surfaces within the context of geometric modeling interfaces. One intuitive modeling interface commonly used in geometric modeling allows the user to directly manipulate curves and surfaces. This manipulation defines some set of constraints that the curve or surface must satisfy (such as interpolation and tangent constraints). Direct manipulation, however, usually leads to an underconstrained problem since there are, in general, many possible surfaces meeting some set of constraints. Therefore an optimization problem must be solved. This thesis discusses how geometric modeling optimization problems can be solved more efficiently by using a wavelet basis. Because the wavelet basis is hierarchical, iterative optimization methods converge rapidly. And because the wavelet coefficients indicate the degree of detail in the solution, they can be used to determine the number of basis functions needed to express the variational minimum, thus avoiding unnecessary computation. An implementation is discussed and experimental results are reported. END:: PRINCETONCS//TR-473-94 Score : 90 BIB-VERSION:: CS-TR-v2.0 ID:: PRINCETONCS//TR-485-95 ENTRY:: February 21, 1995 ORGANIZATION:: Princeton University, Computer Science Department LANGUAGE:: English TITLE:: An Adaptive Gauss Method for Computing Irradiance Coefficients of Galerkin Radiosity System s AUTHOR:: Gershbein, Reid DATE:: February 1995 PAGES:: 10 ABSTRACT:: Computing energy transfer between objects is the most expensive operation in radiosity systems. This energy transfer operation, known as the irradiance operator, is an integral that, in general, must be calculated numerically. We wish to increase the speed of this computation without severely compromising fidelity and perform a study of numerical integration techniques, $Quadrature$ $Methods$. The results of our study show the strengths of $Gauss$ $Quadrature$ $Rules$ and give us insights into greatly reducing the cost of the irradiance operator while maintaining accuracy. An adaptive method for choosing Gauss quadrature rules is presented, and our performance analysis of the new adaptive algorithm shows that it can be up to 10 times faster than previous methods. END:: PRINCETONCS//TR-485-95 =-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-= Electronically available reports can be retrieved via ftp (as described in records.) For other reports, local users can access them in the Math/CS Library. Non-Stanford users should either contact the publish- Electronic Library ing institution or arrange with their local library elib@db.stanford.edu for an interlibrary loan from Stanford Green Library. =-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-= From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for kopp id AA00097; Tue, 28 Feb 95 01:49:44 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.10/8.6.9) with ESMTP id BAA04245 for ; Tue, 28 Feb 1995 01:36:37 +0100 Received: from fs1.cam.nist.gov (fs1.cam.nist.gov [129.6.80.33]) by imag.imag.fr (8.6.10/8.6.9) with SMTP id BAA01717; Tue, 28 Feb 1995 01:36:35 +0100 Received: from plum (plum.cam.nist.gov) by fs1.cam.nist.gov (4.1/SMI-DDN) id AA05621; Mon, 27 Feb 95 19:36:37 EST Received: by plum (950215.SGI.8.6.10/SMI-3.2) id TAA20860; Mon, 27 Feb 1995 19:36:31 -0500 From: "Holly E Rushmeier" Message-Id: <9502271936.ZM20858@plum.cam.nist.gov> Date: Mon, 27 Feb 1995 19:36:31 -0500 In-Reply-To: Francois Sillion "looking for 3D data of human head" (Feb 24, 10:35am) References: <199502240835.KAA21073@sesame.imag.fr> X-Mailer: Z-Mail (3.1.0 22feb94 MediaMail) To: Francois.Sillion@imag.fr, Global Illumination List Subject: Re: looking for 3D data of human head Content-Type: text/plain; charset=us-ascii; format=flowed Mime-Version: 1.0 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hi This is more data than you probably wanted, but I thought I would mention that the complete data for the male "Visible Human" (as seen at Vol. Vis. '94) is now available -- this includes CAT, MRI and cryosections at 1 millimeter intervals. The URL http://www.nlm.nih.gov/extramural_research.dir/visible_human.html has a complete description of the data and how to get it. You need to fill out forms about what you are going to do with the data -- for example whether you are going to develop a commercial product. I don't think you have to pay anything unless you want them to send you data on tape. They also have a few sample images. -- Holly From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for kopp id AA06311; Wed, 1 Mar 95 01:52:45 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.10/8.6.9) with ESMTP id BAA15708 for ; Wed, 1 Mar 1995 01:17:19 +0100 Received: from fs1.cam.nist.gov (fs1.cam.nist.gov [129.6.80.33]) by imag.imag.fr (8.6.10/8.6.9) with SMTP id BAA04750 for ; Wed, 1 Mar 1995 01:17:17 +0100 Received: from plum (plum.cam.nist.gov) by fs1.cam.nist.gov (4.1/SMI-DDN) id AA24075; Tue, 28 Feb 95 19:17:14 EST Received: by plum (950215.SGI.8.6.10/SMI-3.2) id TAA22987; Tue, 28 Feb 1995 19:17:09 -0500 From: "Holly E Rushmeier" Message-Id: <9502281917.ZM22985@plum.cam.nist.gov> Date: Tue, 28 Feb 1995 19:17:08 -0500 X-Mailer: Z-Mail (3.1.0 22feb94 MediaMail) To: globillum@imag.fr Subject: Radiative Heat Transfer Workshop Results Content-Type: text/plain; charset=us-ascii; format=flowed Mime-Version: 1.0 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hi globillumers, For those of you interested in rendering participating media, you might want to check out http://www.sandia.gov/html/frame/NSFFinal_with_graphics_1.html which is "The Use of High-Performance Computing to Solve Participating Media Radiative Heat Transfer Problems - Results of an NSF Workshop" Of particular interest is that the "Volume Rendering Problem" is identified as a "Major Research Thrust". -- Holly From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for kopp id AA08373; Wed, 1 Mar 95 11:47:41 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.10/8.6.9) with ESMTP id LAA12686 for ; Wed, 1 Mar 1995 11:24:39 +0100 Received: from fhg.de (fhg.de [153.96.1.1]) by imag.imag.fr (8.6.10/8.6.9) with SMTP id LAA14879 for ; Wed, 1 Mar 1995 11:24:26 +0100 From: gatenby@igd.fhg.de Received: by fhg.de (mail-gw.fhg.de) with PRESMTP; Wed, 1 Mar 95 11:24:15 +0100 from FHG-GATEWAY Received: by fhg.de (mail-gw.fhg.de) with SMTP; Wed, 1 Mar 95 11:24:06 +0100 from igd.igd.fhg.de Received: by igd.igd.fhg.de; Wed, 1 Mar 95 11:27:04 +0100 Received: by pluto.igd.fhg.de (940816.SGI.8.6.9/SMI-4.0) id LAA13886; Wed, 1 Mar 1995 11:20:48 +0100 Date: Wed, 1 Mar 1995 11:20:48 +0100 Message-Id: <199503011020.LAA13886@pluto.igd.fhg.de> To: globillum@imag.fr Subject: polyhedra from polygons X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Hi, I wonder if anyone could help? ... I'm interested in generating a polyhedral scene from a set of input polygons which are completely free of connectivity/adjacency information. I would like to process these polygons to produce a collection of polyhedra. Does anyone have any pointers to papers on this topic? Does anyone have any experience of doing this - any advice on a nice compact representation for the polyhedra (I want to identify silhouette edges for disc. meshing radiosity) - i.e. which data structure would you advise - do people REALLY use things as wieldy as the winged edge? Any help much appreciated. Thanks in advance, Neil Gatenby Fraunhofer-Institut fuer Graphische Datenverarbeitung (Fraunhofer Institute for Computer Graphics) Neil Gatenby e-mail: gatenby@igd.fhg.de Fraunhofer-IGD, Wilhelminenstr. 7, 64283 Darmstadt, Germany. From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for kopp id AA11058; Wed, 1 Mar 95 19:57:05 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.10/8.6.9) with ESMTP id TAA21200 for ; Wed, 1 Mar 1995 19:19:53 +0100 Received: from lbl.gov (lbl.gov [128.3.254.23]) by imag.imag.fr (8.6.10/8.6.9) with SMTP id TAA02332 for ; Wed, 1 Mar 1995 19:19:46 +0100 Received: from hobbes.lbl.gov by lbl.gov (4.1/1.39) id AA24258; Wed, 1 Mar 95 10:19:40 PST Received: by hobbes.lbl.gov (3.2/SMI-3.2) id AA26871; Wed, 1 Mar 95 10:16:34 PST Date: Wed, 1 Mar 95 10:16:34 PST From: "Gregory J. Ward" Message-Id: <9503011816.AA26871@hobbes.lbl.gov> To: gatenby@igd.fhg.de, globillum@imag.fr Subject: Re: polyhedra from polygons X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Coalescing vertices from disjoint polygons is not particularly difficult, so long as your scenes are reasonably well-behaved. I wrote a translator from Radiance format (http://radsite.lbl.gov/radiance/HOME.html) to MGF (http://radsite.lbl.gov/mgf/HOME.html) which coalesced vertices using a simple hashing scheme. You are welcome to the source code for this -- it is on the above-mentioned servers. As far as connectivity information goes, I know nothing. It's a meshy problem! -Greg From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for kopp id AA12314; Thu, 2 Mar 95 06:29:10 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.10/8.6.9) with ESMTP id GAA00378 for ; Thu, 2 Mar 1995 06:16:08 +0100 Received: from postoffice.mail.cornell.edu (POSTOFFICE.MAIL.CORNELL.EDU [132.236.56.7]) by imag.imag.fr (8.6.10/8.6.9) with ESMTP id GAA11360 for ; Thu, 2 Mar 1995 06:16:05 +0100 Received: from [132.236.236.96] (CU-DIALUP-0322.CIT.CORNELL.EDU [132.236.236.96]) by postoffice.mail.cornell.edu (8.6.9/8.6.9) with SMTP id AAA04690; Thu, 2 Mar 1995 00:15:46 -0500 X-Sender: bwade@max.graphics.cornell.edu Message-Id: Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed Date: Thu, 2 Mar 1995 00:15:59 -0500 To: gatenby@igd.fhg.de, globillum@imag.fr From: Bretton Wade Subject: Re: polyhedra from polygons X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit At 5:20 AM 3/1/95, gatenby@igd.fhg.de wrote: > Does anyone have any experience of doing this - any advice on a nice > compact representation for the polyhedra (I want to identify silhouette > edges for disc. meshing radiosity) - i.e. which data structure would > you advise - do people REALLY use things as wieldy as the winged edge? Dani Lischinski and Fillipo Tampieri used BSP trees to track discontinuities through space. BSP trees are fairly compact geometry representations that do not require explicit connectivity information, and so might be good for you. They would not be very useful for extracting polyhedra, however. I don't have the references right in front of me, so I hesitate to specify them; but I have them on my desk at work if needed. If you are not familiar with BSP trees, you might want to look at the BSP tree FAQ, which is still under construction: http://www.graphics.cornell.edu/bspfaq/ -- Bretton Wade (bwade@graphics.cornell.edu) http://www.graphics.cornell.edu/~bwade/ From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for kopp id AA17568; Thu, 2 Mar 95 14:34:01 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.10/8.6.9) with ESMTP id LAA24140 for ; Thu, 2 Mar 1995 11:53:06 +0100 Received: from hwj.gk.dtu.dk (root@hwj.gk.dtu.dk [130.225.91.126]) by imag.imag.fr (8.6.10/8.6.9) with ESMTP id LAA19799 for ; Thu, 2 Mar 1995 11:53:04 +0100 Received: (from hwj@localhost) by hwj.gk.dtu.dk (8.6.9/8.6.9) id LAA12054 for globillum@imag.fr; Thu, 2 Mar 1995 11:54:39 +0100 Date: Thu, 2 Mar 1995 11:54:39 +0100 From: Henrik Wann Jensen Message-Id: <199503021054.LAA12054@hwj.gk.dtu.dk> To: globillum@imag.fr Subject: Rendering Complex Scenes X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Dear GlobIllumers, A few years ago a comparison between Radiance and a radiosity implementation on a moderately complex scene lead to the conclusion that Radiance was faster. I have wondered whether it in general is safe to assume that Monte Carlo based ray tracing methods are faster in highly complex scenes (ie. scenes with billions of objects) considering newer radiosity techniques like hierarchical radiosity and radiosity using clustering? I know it depends on the contents of the scene, but if we omit the irradiance gradient method and use path tracing or bidirectional path tracing and continue to increase the number of objects in the scene then I think we would see that the Monte Carlo techniques would render the scene in constant time, while radiosity somehow depends on the number of objects. - Henrik Wann Jensen From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for kopp id AA20689; Thu, 2 Mar 95 22:47:58 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.10/8.6.9) with ESMTP id WAA02345 for ; Thu, 2 Mar 1995 22:23:43 +0100 Received: from netmail2.microsoft.com (netmail2.microsoft.com [131.107.1.13]) by imag.imag.fr (8.6.10/8.6.9) with SMTP id WAA08866 for ; Thu, 2 Mar 1995 22:23:41 +0100 Received: by netmail2.microsoft.com (5.65/25-eef) id AA16163; Thu, 2 Mar 95 13:24:30 -0800 Message-Id: <9503022124.AA16163@netmail2.microsoft.com> Received: by netmail2 using fxenixd 1.0 Thu, 02 Mar 95 13:24:30 PST X-Msmail-Message-Id: 6E95E378 X-Msmail-Conversation-Id: 6E95E378 From: Don Mitchell To: globillum@imag.fr, ziv@argus.asd.sgi.com Date: Thu, 2 Mar 95 12:21:04 TZ Subject: Re: O(n^2) bps trees X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit I don't think Seth was being rude. It's important to understand the computational complexity of the algorithms we use, and visibility is a very tricky game in this regard. BSP-trees seem to gather a lot of passionate evangelism and detraction. I believe Apollo built a CAD system with BSP trees which did go O(n^2) -- pretty much in their customers' faces. I've heard other people say they never saw more than O(n) growth. Ziv Gigus has a masters thesis that gives details of experiments and results, and there clearly needs to be more of that in the literature. I seem to recall Ziv reported typical O(N logN) growth in 3D. Ziv, want to comment? What is really needed is an ongoing contest between inputs and algorithms. Something like this happens in the ray-tracing community, with Eric Haines input test scenes. The visibility problem (not just BSP approaches) would benefit from this. Revolutionary new approaches to visibility are being taken in games and PC graphics libraries. I can't divulge proprietary algorithms, so I'll just taunt you a bit. Look forward to some interesting revelations on visiblity in the coming years. :-) John Carmack, at id Software, deserves some special credit for the visibility algorithm used in DOOM. The bspfaq says he is using bps trees, but I believe he has made some novel advances beyond the standard usage. His first insight was that typical building interiors can be treated as a 2D problem instead of 3D. Paterson and Yao point out that the worst-case space complexity of BSP trees is only O(N logN) in 2D. Secondly, Carmack deals with occlusion culling in two interesting ways -- by drawing front to back with an efficient algorithm for knowing when the screen is completely drawn, and by augmenting the BSP-tree with bounding boxes for rapid culling of occluded subtrees. We've been using the term "DOOM trees" to refer to Carmack's work. I think he deserves that honor. :-) -- Don From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for kopp id AA17897; Thu, 2 Mar 95 14:45:35 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.10/8.6.9) with ESMTP id NAA00931 for ; Thu, 2 Mar 1995 13:44:28 +0100 Received: from theory.lcs.mit.edu (theory.lcs.mit.edu [18.52.0.92]) by imag.imag.fr (8.6.10/8.6.9) with SMTP id NAA23330 for ; Thu, 2 Mar 1995 13:43:51 +0100 Received: from jabiru.lcs.mit.edu by theory.lcs.mit.edu (5.65c/TOC-1.2S) id AA23288; Thu, 02 Mar 95 07:41:13 EST Received: by jabiru.lcs.mit.edu (931110.SGI/TOC-1.2C) id AA05669; Thu, 2 Mar 95 07:43:51 -0500 From: "Seth Teller" Message-Id: <9503020743.ZM5667@jabiru.lcs.mit.edu> Date: Thu, 2 Mar 1995 07:43:50 -0500 In-Reply-To: bwade@graphics.cornell.edu (Bretton Wade) "Re: polyhedra from polygons" (Mar 2, 12:15am) References: Reply-To: seth@theory.lcs.mit.edu X-Mailer: Z-Mail (3.1.0 22feb94 MediaMail) To: Bretton Wade , gatenby@igd.fhg.de, globillum@imag.fr Subject: Re: polyhedra from polygons, O(n^2) BSP Content-Type: text/plain; charset=us-ascii; format=flowed Mime-Version: 1.0 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit > discontinuities through space. BSP trees are fairly compact geometry > representations that do not require explicit connectivity information, and > so might be good for you. They would not be very useful for extracting > polyhedra, however.... Bretton, with all due respect I must ask you to be more careful about dispensing incorrect and/or misleading information in your replies, in your BSP faq, and elsewhere. A.) BSP trees are arguably not "compact," as they require Omega(n^2) storage and O(n^3) construction time for some 3D inputs. The storage lower bound is tight, see p. 500 of @article{Paterson90, author = "Michael S. Paterson and F. Frances Yao", title = "Efficient Binary Space Partitions for Hidden-Surface Removal and Solid Modeling", journal = "Discrete and Computational Geometry", volume = 5, number = 5, year = 1990, pages = "485--503", comments = "also Xerox PARC tech report CSL 89-6"} Stated differently, this means that there inputs of n polygons in 3d for which *every* BSP tree has size at least O(n^2). Apparently you have not yet corrected your FAQ http://www.graphics.cornell.edu/cgi-bin/bsp?18.txt in this regard. Your statement there that BSP's have a "provable lower bound [of] O(n)" doesn't make any sense. B) A BSP tree, if available, would be an ideal preprocessed data structure from which to abstract a winged-edge, facet-edge, or other adjacency data structure. You don't need a reference to see how; you simply walk the (necessarily convex) leaves of the tree, inducing shared edge pointers wherever two cutting planes of the BSP tree meet two faces of the input polyhedron along a common line in 3-space. Regards, Seth. -- Asst. Prof of EE & CS Synthetic 0 ~ ~ seth@lcs.mit.edu MIT Lab for CS NE43-208 Imagery <\> ~ tel: 617 258 7885 545 Technology Square Group / \ fax: 617 253 6652 Cambridge MA 02139 _______________ web: http://theory.lcs.mit.edu/~seth/ From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for kopp id AA21926; Fri, 3 Mar 95 08:52:48 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.10/8.6.9) with ESMTP id PAA13113 for ; Thu, 2 Mar 1995 15:44:57 +0100 Received: from explorer.dgp.toronto.edu (explorer.dgp.toronto.edu [128.100.1.129]) by imag.imag.fr (8.6.10/8.6.9) with SMTP id PAA27877 for ; Thu, 2 Mar 1995 15:44:52 +0100 Received: by explorer-en.dgp.toronto.edu id <144285>; Thu, 2 Mar 1995 09:41:44 -0500 In-Reply-To: "Seth Teller"'s message as of Mar 2, 8:11am X-Mailer: Mail User's Shell (7.2.3 5/22/91) From: Eugene Fiume To: globillum@imag.fr Subject: Re: polyhedra from polygons, O(n^2) BSP Message-Id: <95Mar2.094144est.144285@explorer-en.dgp.toronto.edu> Date: Thu, 2 Mar 1995 09:41:32 -0500 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit On Mar 2, 8:11am, "Seth Teller" wrote: and then he wrote: } A.) BSP trees are arguably not "compact," as they require } Omega(n^2) storage and O(n^3) construction time for some } 3D inputs. The storage lower bound is tight, see p. 500 of The existence of such results, and indeed the ease of constructing such worst cases does not mean that these configurations are "common". Worst-case upper bound arguments are nice intellectual exercises and are sometimes even informative. Now, if you attach an argument that this situation readily arises, then you'll have my attention and you'll have properly made your point. Eugene. From To: Abteilung-186/2, CG-Gruppe From: Werner Purgathofer Subject: from Globillum: references Message-Id: X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Date: Fri, 3 Mar 1995 07:17:55 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit >X-POP3-Rcpt: wp@stellaris >Date: Thu, 2 Mar 1995 13:06:49 -0500 >From: Eric Haines >To: globillum@imag.fr >Subject: references >Cc: bloom@cs.cornell.edu, erich@hemlock.eye.com > >I've run across a truly amazing site on the WWW (i.e. it's actually useful): > > http://www.ira.uka.de/ftp/ira/bibliography/index.html > >which has a collection of all sorts of computer science bibliographies. The >nice part is that you can do on-line searches - it just turned up a reference >I didn't know about on a topic, so I'm happy with it. You can search all the >bibliographies (whew!) for a topic or just some specific ones. Fantastic, >and free. > >Eric Haines From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for kopp id AA01080; Fri, 3 Mar 95 20:17:50 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.10/8.6.9) with ESMTP id TAA28588 for ; Fri, 3 Mar 1995 19:27:41 +0100 Received: from relay.cdnnet.ca (relay.cdnnet.ca [192.73.5.1]) by imag.imag.fr (8.6.10/8.6.9) with ESMTP id SAA08971 for ; Fri, 3 Mar 1995 18:55:46 +0100 Received: (from ean@localhost) by relay.cdnnet.ca (8.6.9/8.6.9) id JAA07032; Fri, 3 Mar 1995 09:55:22 -0800 X400-Received: by /PRMD=CA/ADMD=CDNnet/C=CA/; Relayed; Fri, 3 Mar 1995 9:55:21 UTC-0800 X400-Received: by /PRMD=ca/ADMD=telecom.canada/C=ca/; Relayed; Fri, 3 Mar 1995 9:55:17 UTC-0800 Date: Fri, 3 Mar 1995 9:55:17 UTC-0800 X400-Originator: fournier@cs.ubc.ca X400-Recipients: non-disclosure:; X400-Content-Type: P2-1984 (2) X400-Mts-Identifier: [/PRMD=ca/ADMD=telecom.canada/C=ca/;950303095517] Content-Identifier: 4003 From: Alain Fournier To: "Henrik Wann Jensen (return)" Cc: return In-Reply-To: <199503031601.RAA16321@hwj.gk.dtu.dk> Message-Id: <"4003*fournier@cs.ubc.ca"@MHS> Subject: Re: Rendering Complex Scenes Mime-Version: 1.0 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed Content-transfer-encoding: 8bit "In deserto clamavi" (Latin from memory, pardon the potential barbarisms). Loosely translated, it means "I get no respect". I have long claimed that a good solution for global illumination of complex scenes is to use a "light driven" approach, namely where the light is transported explicitly between cells (sections of the environment), and not between surfaces (as in "radiosity" or path following schemes). The obvious advantage is that you control the process exactly where it should be controlled, as a function of the amount of light transported, not as the level of where it comes from or where it's going (even though you still have some control about that). The other big one is that "clustering", or simplification of the light flux, becomes a simple issue. I claim (somewhat facetiously, but with a basis in truth) that it is the only approach that has asymptotically the complexity of the "Utah approximation" (as Jim Kajiya calls it) with depth-buffer visibility, namely O(N), where N is the number of primitives in the scene. I won't go on about this, but details can be obtained on request. For many reasons (some fair, some not), the community has been unwilling to accept presentation of work in this direction, even in forums (fora) dedicated to works in progress. I think it's our collective loss, since even if one does not believe in a particular approach, one should realize that some of the concepts and techniques used can be relevant to other problems (not necessarily actively considered at the time). To quote Sonny Terry & Brownie McGhee: "We might be fighting a losing battle, but we had fun trying to win". From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for kopp id AA01279; Fri, 3 Mar 95 21:23:18 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.10/8.6.9) with ESMTP id UAA29885 for ; Fri, 3 Mar 1995 20:29:52 +0100 Received: from milo.math.scarolina.edu (milo.math.scarolina.edu [129.252.12.2]) by imag.imag.fr (8.6.10/8.6.9) with SMTP id UAA01373 for ; Fri, 3 Mar 1995 20:29:50 +0100 Received: by milo.math.scarolina.edu (4.1/6.0s-FWP); id AA10858; Fri, 3 Mar 95 14:29:38 EST Date: Fri, 3 Mar 95 14:29:38 EST From: Peter Schroder Message-Id: <9503031929.AA10858@milo.math.scarolina.edu> To: fournier@cs.ubc.ca Cc: hwj@hwj.gk.dtu.dk, globillum@imag.fr In-Reply-To: Alain Fournier's message of Fri, 3 Mar 1995 9:55:17 UTC-0800 <"4003*fournier@cs.ubc.ca"@MHS> Subject: Rendering Complex Scenes X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Date: Fri, 3 Mar 1995 9:55:17 UTC-0800 From: Alain Fournier I have long claimed that a good solution for global illumination of complex scenes is to use a "light driven" approach, namely where the light is transported explicitly between cells (sections of the environment), and not between surfaces (as in "radiosity" or path following schemes). The obvious advantage is that you control the process exactly where it should be controlled, as a function of the amount of light transported, not as the level of where it comes from or where it's going (even though you still have some control about that). The other big one is that "clustering", or simplification of the light flux, becomes a simple issue. I couldn't agree more. Once you include clustering into radiosity/radiance algorithms you get exactly this situation. See some of the recent work in this direction from GI and Siggraph. However, even if we get this to work there is still that pesky little problem of visibility. In fact we may have made enough progress on hierarchical numerical schemes at this point that fast and approximate(!) visibility is the most important aspect to attack. Peter From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for kopp id AA01290; Fri, 3 Mar 95 21:29:51 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.10/8.6.9) with ESMTP id UAA29938 for ; Fri, 3 Mar 1995 20:37:04 +0100 Received: from wk309.nas.nasa.gov (wk309.nas.nasa.gov [129.99.64.29]) by imag.imag.fr (8.6.10/8.6.9) with ESMTP id UAA01429 for ; Fri, 3 Mar 1995 20:37:00 +0100 Received: (from uselton@localhost) by wk309.nas.nasa.gov (8.6.8.2/NAS.6.1) id LAA23106; Fri, 3 Mar 1995 11:36:43 -0800 Date: Fri, 3 Mar 1995 11:36:43 -0800 From: "Samuel P. Uselton" Message-Id: <199503031936.LAA23106@wk309.nas.nasa.gov> To: fournier@cs.ubc.ca Cc: hwj@hwj.gk.dtu.dk, globillum@imag.fr In-Reply-To: Alain Fournier's message of Fri, 3 Mar 1995 9:55:17 UTC-0800 <"4003*fournier@cs.ubc.ca"@MHS> Subject: Rendering Complex Scenes Reply-To: uselton@nas.nasa.gov X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Yo Alain! If we can have adaptive gridding of the environment, then I'm with you. Of course adaptive gridding is hard in its own right. (There are folks here at Ames working on exactly that kind of problem!) And it handles the participating media issues properly as well. I'm really surprised to hear you are having trouble finding a venue for this stuff. I'm interested in hearing about some of this "work-in-progress". I'll follow up with private mail. Later, Sam U. uselton@nas.nasa.gov From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for kopp id AA01330; Fri, 3 Mar 95 21:50:43 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.10/8.6.9) with ESMTP id VAA00941 for ; Fri, 3 Mar 1995 21:07:30 +0100 Received: from lbl.gov (lbl.gov [128.3.254.23]) by imag.imag.fr (8.6.10/8.6.9) with SMTP id VAA01837 for ; Fri, 3 Mar 1995 21:07:20 +0100 Received: from hobbes.lbl.gov by lbl.gov (4.1/1.39) id AA05084; Fri, 3 Mar 95 12:06:58 PST Received: by hobbes.lbl.gov (3.2/SMI-3.2) id AA02145; Fri, 3 Mar 95 12:03:24 PST Date: Fri, 3 Mar 95 12:03:24 PST From: "Gregory J. Ward" Message-Id: <9503032003.AA02145@hobbes.lbl.gov> To: fournier@cs.ubc.ca, hwj@hwj.gk.dtu.dk Subject: Re: Rendering Complex Scenes Cc: globillum@imag.fr X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit I think Alain is onto something -- and maybe it has been used after all. As near as I can figure, the Integra system (sold by Arris in the US) uses a cell-transfer or at least cell-collected transport mechanism similar to the one described. Is Karol out there listening? Care to comment? As to the complexity of radiosity and path tracing approaches, I think in the end everything will be the same. After all, they are solving the same problem. Recent assertions as to the storage and computation required for advanced hierarchical and clustering radiosity methods are similar to those one would compute for a Monte Carlo solution to the same problem. The key difference currently is the problem definition itself -- most radiosity algorithms solve for the irradiance on objects, whereas most Monte Carlo algorithms solve for the pixels in an image. Given this difference, radiosity is bound to win when the number of pixels grows relative to the number of objects, and Monte Carlo will win as the number of objects grows relative to the number of pixels. I cite the additional evidence that most radiosity optimizations these days focus on geometric simplification (i.e. clustering and hierarchy) where current Monte Carlo optimizations focus on improved image sampling and filtering. A system such as the one Dr. Fournier proposes would no doubt concentrate on optimal subdivision and sampling of volumes instead. Looking at how Nature solves this problem, I would have to bet on pure Monte Carlo for the ultimate solution. However, given the finite resources of the computing world, we have to go with whatever bag of tricks gets us closest to what we want in the least amount of time. This, it seems, depends a good deal on the particular problem at hand. Monte Carlo for a forest, radiosity for three boxes. -Greg From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for kopp id AA01426; Fri, 3 Mar 95 22:31:01 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.10/8.6.9) with ESMTP id VAA08932 for ; Fri, 3 Mar 1995 21:48:02 +0100 Received: from merckx.graphics.cornell.edu (MERCKX.GRAPHICS.CORNELL.EDU [128.84.247.147]) by imag.imag.fr (8.6.10/8.6.9) with SMTP id VAA02269 for ; Fri, 3 Mar 1995 21:48:00 +0100 Received: by merckx.graphics.cornell.edu (5.65/DEC-Ultrix/4.3) id AA07889; Fri, 3 Mar 1995 15:48:16 -0500 Message-Id: <9503032048.AA07889@merckx.graphics.cornell.edu> Received: by gaia.graphics.cornell.edu (1.37.109.8/16.2) id AA08347; Fri, 3 Mar 1995 15:47:53 -0500 From: Peter Shirley Subject: Re: Rendering Complex Scenes To: Henrik Wann Jensen Date: Fri, 3 Mar 95 15:47:53 EST Cc: globillum@imag.fr In-Reply-To: <199503021054.LAA12054@hwj.gk.dtu.dk>; from "Henrik Wann Jensen" at Mar 2, 95 11:54 am Mailer: Elm [revision: 70.85] X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Kajiya addressed this topic many years ago in a course note that I really liked: Article{kaji88, Author = "James T. Kajiya", Title = {An Overview and Comparison of Rendering Methods}, Journal = {A Consumer's and Developer's Guide to Image Synthesis}, Year = 1988, Pages = {259-263}, Note = {ACM Siggraph '88 Course 12 Notes} } He basically said that path tracing is faster than z-buffer approaches once there are thousands of primitives per pixel (note-- he said z-buffer-- we aren't even talking radiosity here). I think this assumes a static environment where you plan to make many frames in an animation-- this way you don't have to count the O(N) (I assume a uniform grid) setup time for ray tracing. I think AF's method sounds pretty neat. Please don't only share with SU! One thing I wonder about is how to ray trace procedural environments that are too big to be stored. Here I think you must use something other than straight radiosity (the light transport might have less detail than the geometry, so the AF volume idea might still work). Can we encode a spatial subdivision structure in the procedural model so that rays are log(N), where N is the number of "fully expanded" primitive polygons (or whatever the atomic primitive is)? How expressive are the set of primitve objects that can have such friendly properties? As an analogy, Perlin-style solid textures are friendly, while reaction-diffusion textures are not. I think making friendly procedural objects that coexist peacefully with hand-modeled objects is a neat (and hard) area to look at. A start can be found in: Article{ambu86, Author = "Phil Amburn and Eric Grant and Turner Whitted", Title = {Managing Geometric Complexity with Enhanced Procedural Models}, Journal = {Computer Graphics}, Year = 1986, Pages = {189-195}, Volume = 20, Number = 4, Month = {August}, Note = {ACM Siggraph '86 Conference Proceedings} } Does anyone have a bibliography on procedural modeling? From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for kopp id AA01570; Sat, 4 Mar 95 00:22:54 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.10/8.6.9) with ESMTP id XAA10116 for ; Fri, 3 Mar 1995 23:24:50 +0100 Received: from june.cs.washington.edu (june.cs.washington.edu [128.95.1.4]) by imag.imag.fr (8.6.10/8.6.9) with ESMTP id XAA03338 for ; Fri, 3 Mar 1995 23:24:48 +0100 Received: (per@localhost) by june.cs.washington.edu (8.6.10/7.2ju) id OAA18414; Fri, 3 Mar 1995 14:24:29 -0800 Date: Fri, 3 Mar 1995 14:24:28 -0800 (PST) From: "Per H. Christensen" To: Peter Schroder Cc: hwj@hwj.gk.dtu.dk, globillum@imag.fr Subject: Re: Rendering Complex Scenes In-Reply-To: <9503031929.AA10858@milo.math.scarolina.edu> Message-Id: Mime-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII; format=flowed X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit On Fri, 3 Mar 1995, Peter Schroder wrote: [...] > there is still that pesky little problem of visibility. In fact we may have > made enough progress on hierarchical numerical schemes at this point that > fast and approximate(!) visibility is the most important aspect to attack. > > Peter Yes, approximate visibility is perhaps the most important and difficult problem now (both for Monte Carlo or finite element methods)! We tried for a while to do some work on this, but got stuck on what we call the "coherence problem": If you divide the environment into cells, approximate visibility information can be computed for each cell. This can be done to a wide range of spatial and directional accuracy. So far so good. But -- when this approximate occlusion information is to be combined from the different cells that are between the "sender" and "receiver", the "coherence problem" arises: Using the approximate occlusion information, we no longer have information whether the patches in each cell are coherent or incoherent with the patches in the other cells. For example, if a beam of light is passing through two cells, with each cell having 50% occlusion within that beam (and in that direction), the total occlusion could be anything from 50% (if all the patches in one cluster are aligned with the patches in the other cluster) to 100% (if the patches in one cluster overlap the "holes" through the other cluster). In the end, we had to go back to the "good old" technique of shooting some number of sample rays and check each ray for intersection along the path. The accuracy can be controlled by the number of rays shot. Even with a hierarchy of cells, this sampling method is very time consuming -- it is easily the most time consuming part of global illumination. There is plenty of room for improvement here! -- Per From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for kopp id AA03113; Sat, 4 Mar 95 13:54:07 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.10/8.6.9) with ESMTP id MAA22160 for ; Sat, 4 Mar 1995 12:53:26 +0100 Received: from tiete.dcc.unicamp.br (dcc.unicamp.br [143.106.1.11]) by imag.imag.fr (8.6.10/8.6.9) with SMTP id MAA09475 for ; Sat, 4 Mar 1995 12:53:19 +0100 Received: from stack (stack.dcc.unicamp.br) by tiete.dcc.unicamp.br (4.1/SMI-4.1) id AA00587; Sat, 4 Mar 95 08:51:31 EST Date: Sat, 4 Mar 95 08:51:31 EST From: Jorge Stolfi Message-Id: <9503041151.AA00587@tiete.dcc.unicamp.br> Received: by stack (4.1/SMI-4.1) id AA01008; Sat, 4 Mar 95 08:51:25 EST To: Alain Fournier Cc: globillum@imag.fr Subject: Re: Rendering Complex Scenes In-Reply-To: <"4003*fournier@cs.ubc.ca"@MHS> References: <199503031601.RAA16321@hwj.gk.dtu.dk> <"4003*fournier@cs.ubc.ca"@MHS> Reply-To: stolfi@dcc.unicamp.br X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit > "In deserto clamavi" (Latin from memory, pardon the potential > barbarisms). Loosely translated, it means "I get no respect". > > I have long claimed that a good solution for global illumination > of complex scenes is to use a "light driven" approach, namely > where the light is transported explicitly between cells > (sections of the environment), and not between surfaces (as in > "radiosity" or path following schemes). The obvious advantage > is that you control the process exactly where it should be > controlled, as a function of the amount of light transported, > not as the level of where it comes from or where it's going > (even though you still have some control about that). The other > big one is that "clustering", or simplification of the light > flux, becomes a simple issue. One problem of using volume cells instead of surface patches is that a non-planar assemblage of Lambertian diffusers is in general not a Lambertian diffuser; that is, the amount of light scattered towards a given direction may depend strongly on the incoming direction. In fact, the scattering function can be much more complicated than typical models for non-Lambertian but flat surfaces. For instance, consider a cylindrical tin can, open at one end, painted black on the outside and white on the inside. Depending on where the incident light is coming from, the percentage scattered may vary from 0 to 100% of the incident light; and the outgoing distribution will probably have several peaks, in funny directions. So, I would think that a global illumination model that handles clustering must be a "second-order" model, where the unknowns are flows between pairs of cells, and the coefficient matrix has three-way form factors --- "how much of the light flowing from cell i to cell j is diverted to cell k". Are we ready to tackle this? I believe Leo Guibas and Eric Veach (Stanford) were looking into this approach a couple of years ago. Perhaps you should get in touch with them? --stolfi ------------------------------------------------------------------------ Jorge Stolfi | http://www.dcc.unicamp.br/~stolfi | stolfi@dcc.unicamp.br Computer Science Dept. (DCC-IMECC) | Tel +55 (192) 39-8442 Universidade Estadual de Campinas (UNICAMP) | +55 (192) 39-3115 Campinas, SP -- Brazil | Fax +55 (192) 39-7470 ------------------------------------------------------------------------ Please do not copy this .signature virus into your .signature file! From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for kopp id AA04042; Sat, 4 Mar 95 22:13:02 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.10/8.6.9) with ESMTP id VAA00873 for ; Sat, 4 Mar 1995 21:12:34 +0100 Received: from postoffice.mail.cornell.edu (POSTOFFICE.MAIL.CORNELL.EDU [132.236.56.7]) by imag.imag.fr (8.6.10/8.6.9) with ESMTP id VAA12773 for ; Sat, 4 Mar 1995 21:12:33 +0100 Received: from [132.236.236.187] (CU-DIALUP-0617.CIT.CORNELL.EDU [132.236.236.187]) by postoffice.mail.cornell.edu (8.6.9/8.6.9) with SMTP id PAA25749 for ; Sat, 4 Mar 1995 15:12:27 -0500 X-Sender: bwade@max.graphics.cornell.edu Message-Id: Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed Date: Sat, 4 Mar 1995 15:12:37 -0500 To: globillum@imag.fr From: Bretton Wade Subject: BSP Trees X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Bruce Naylor asked me to forward some of his comments on BSP Tree complexity to this mailing list. His first response to my and Seth's post: >First, Partitionings Trees are a representation of polytopes, >so the phrase "extract a polyhedra from bsp trees" needs to >be restated as "generate a boundary representation from a partitioning >tree". This I do all the time. > >Secondly, with regard to the O(n^2) result of Paterson and Yao, >this is not such an interesting result as it may seem. First, >in terms of worst case complexity, I showed in my thesis (1981) >that there were b-reps for which any tree using only planes of polygons >would be O(n^2). The result of Paterson and Yao is stronger in that >it gives an example for which any tree, including one using planes >not containing polygons, is O(n^2). However, this result is superceded >by a result in Benard Chazelle's thesis (1981), which proves that there >are polyhedra for which any convex decomposition is O(n^2). Since >partitioning trees are a convex decomposition, the fact that trees >can be O(n^2) follows immediately. > >Now in terms of expected case, all empirical evidence indicates >that tree size is O(n) for objects of interest (see my tutorial >in siggraph 94 course notes). And that the "compressed" versions >of trees are typically smaller than the "compressed" version of b-reps. > >The reason for the discrepency between worst and expected case is >the following. All worst case examples violate what I call the >Principal of Locality, that is, that geometric features of >real-world objects are local, i.e. they do not span the space. >The best example of geometry that violates the Locality Principal >is arrangements of hyperplanes, since hyperplanes are infinite. >And in fact, the upperbound for trees containing n hyperplanes >is exactly the bound on the size of arrangements of hyperplane, >which is O(n^d). > >Partitioning Trees capture locality through the ordering of the >hyperplanes. As one descends the tree, the size of the convex regions of >space represented by each tree-node decreases monontonically. >This can be used to create a multi-resolution representation >such that details are added as one descends into the tree. > >One last comment, the best published work on using Partitioning >Trees for radiosity is the paper of Campbell and Fussell in >Sigraph '90. A much fuller exposition is given in Campbell's >Ph.D. thesis, obtained at UT Austin. A different statement of why the O(n ^ 2) figure is not so useful: >In general, spatial search structures are only useful if what >you are "selecting" is a reasonably small subset of the geometry >present. So with non-local features, it is typically not possible >to select a significantly reduced subset, precisely because the >features are effectively global. So returning to the worst case >examples, every search structure using planes by which to partition >space, and so including regular grids and octrees, will also be >of size O(n^2) if one want no more than a constant number of >pieices in each cell of the search structure. What's more, if the >pieces of the b-reps are pushed together slightly so that they touch each >other, and one removes the coincident pieces of the b-rep, then >the number of b-rep polygons will also be O(n^2). > >So I think the O(n^2) result is not nearly as interesting as >some have thought it might be. A statement of the conditions which produce the worst case: >The case that produces O(n^2) is constructed from lines on >a hyperboloid of one sheet. This is a ruled surface with >two pencils of lines that, in essence, cross each other. >There is no way around this case. -- Bretton Wade (bwade@graphics.cornell.edu) http://www.graphics.cornell.edu/~bwade/ From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for kopp id AA04269; Sun, 5 Mar 95 01:04:44 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.10/8.6.9) with ESMTP id AAA02404 for ; Sun, 5 Mar 1995 00:44:22 +0100 Received: from theory.lcs.mit.edu (theory.lcs.mit.edu [18.52.0.92]) by imag.imag.fr (8.6.10/8.6.9) with SMTP id AAA14327 for ; Sun, 5 Mar 1995 00:44:20 +0100 Received: from jabiru.lcs.mit.edu by theory.lcs.mit.edu (5.65c/TOC-1.2S) id AA07307; Sat, 04 Mar 95 18:42:51 EST Received: by jabiru.lcs.mit.edu (931110.SGI/TOC-1.2C) id AA07866; Sat, 4 Mar 95 18:46:29 -0500 From: "Seth Teller" Message-Id: <9503041846.ZM7864@jabiru.lcs.mit.edu> Date: Sat, 4 Mar 1995 18:46:27 -0500 Reply-To: seth@theory.lcs.mit.edu X-Mailer: Z-Mail (3.1.0 22feb94 MediaMail) To: globillum@imag.fr Subject: BSP Tree [observed] complexity Content-Type: text/plain; charset=us-ascii; format=flowed Mime-Version: 1.0 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Bruce Naylor writes, via Bretton Wade: > the phrase "extract a polyhedra from bsp trees" needs to be > restated as "generate a [b-rep] from a partitioning tree".... i don't know what "needs to be restated" means. nor am i sure from where bruce took the phrase "extract a polyhedr[on] from bsp trees". my globillum post stated: A BSP tree, if available, would be an ideal preprocessed data structure from which to [ex]tract a winged-edge, facet-edge, or other adjacency data structure. my point was that generating robust connectivity information from an unorganized set of polygons seems hard, starting from scratch; but if someone hands you a BSP tree for the input, it becomes straightforward. > .... the O(n^2) result of Paterson and Yao ... is not [as] > interesting as it may seem.... in terms of expected case, > all empirical evidence indicates that tree size is O(n) for > objects of interest (see my tutorial in siggraph 94 course notes). this statement may be true, but it is unsupported by the scant body of empirical evidence in the literature, and seems to be refuted by many anecdotal reports. this is not the way to draw worthwhile conclusions about anything. i add my voice to don mitchell's: a thorough, objective empirical examination of the average case (not worst case) behavior of BSP trees is needed: a joint effort, perhaps using bruce's public-domain code as an agreeable "standard" testbed. i propose that we tabulate: construction time; total BSP complexity; and perhaps minimum achievable BSP complexity, without regard to construction time as a function of: varying model type (desk, plane, building, person, etc.), and increasing complexity (or level of detail) within each type. who will join in this effort? seth. -- Asst. Prof of EE & CS Synthetic 0 ~ ~ seth@lcs.mit.edu MIT Lab for CS NE43-208 Imagery <\> ~ tel: 617 258 7885 545 Technology Square Group / \ fax: 617 253 6652 Cambridge MA 02139 _______________ web: http://theory.lcs.mit.edu/~seth/ From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for kopp id AA07027; Mon, 6 Mar 95 08:42:37 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.10/8.6.9) with ESMTP id IAA21117 for ; Mon, 6 Mar 1995 08:16:09 +0100 Received: from relay.cdnnet.ca (relay.cdnnet.ca [192.73.5.1]) by imag.imag.fr (8.6.10/8.6.9) with ESMTP id IAA29405 for ; Mon, 6 Mar 1995 08:16:04 +0100 Received: (from ean@localhost) by relay.cdnnet.ca (8.6.9/8.6.9) id XAA28228 for globillum@imag.fr; Sun, 5 Mar 1995 23:16:01 -0800 X400-Received: by /PRMD=CA/ADMD=CDNnet/C=CA/; Relayed; Sun, 5 Mar 1995 23:16:00 UTC-0800 X400-Received: by /PRMD=ca/ADMD=telecom.canada/C=ca/; Relayed; Sun, 5 Mar 1995 23:15:57 UTC-0800 Date: Sun, 5 Mar 1995 23:15:57 UTC-0800 X400-Originator: fournier@cs.ubc.ca X400-Recipients: non-disclosure:; X400-Content-Type: P2-1984 (2) X400-Mts-Identifier: [/PRMD=ca/ADMD=telecom.canada/C=ca/;950305231557] Content-Identifier: 4011 From: Alain Fournier To: return Message-Id: <"4011*fournier@cs.ubc.ca"@MHS> Subject: Re: Rendering Complex Scenes Mime-Version: 1.0 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed Content-transfer-encoding: 8bit It is gratifying to have so many thoughtful answers to my global rumination. It shows, though, the power of a paradigm (I must use this word because it's convenient in the context, and "model" is overloaded in computer graphics), in this case the rendering-equation/radiosity/form-factor/diffuse-reflector one. The following is not to say that the relevant posts are wrong (I have respect for most of the posters), but that some interpolations or extrapolations were too influenced by what is (and not helped by my tersity). When we talk about clustering, it should be clear that what we really want to achieve is cluster the light (the illumination), not the objects. In other words we are not (usually) interested in the cause but in the result. This is basic. If I am given a complete description of the light falling on an area (or a volume, generally speaking on a subset of the universe), I do not really care about where it comes from. Of course if my paradigm is to consider exchange of light energy between objects, it is difficult to deal with that, and form factors, or equivalent concepts, are hard to avoid. Essentially I have no model to express the light outside of objects, which is quite paradoxical when you think about it, since "free flight" light is a lot easier to deal with than light at interfaces with matter. Light clustering is handled easily in the light-driven approach, since you have an explicit representation of it. Spatial hierarchy is also handled because a reasonable implementation of the paradigm is to subdivide the scene hierarchically and adaptively as a function of the light transported. We use an octree, as the easiest structure to deal with, and because it fits beautifully with the dyadic subdivisions of our wavelet-based representation of the light flux. There seems to be a "miracle" happening, because we seem to solve an integral equation (the rendering equation) by non-standard ways. But it should be realised that the rendering equation has to be solved in its standard form only if we want to know for each surface element (or volume element) not only its radiance, but in some way where it is getting it from, which is gross overkill. To make the point more clearly, assume that I install a wall in the middle of my environment which collects every photon it receives and reemits it instantly or a some later date with the same wavelength and the same direction on the other side. Each half space is now totally independent by considering the wall to be an emitter with a fairly complex distribution, and a total absorber for incident light. Of course if there are only few objects on both sides of the wall, it is much worse than to compute directly the light exchanged between objects, but if there are huge numbers of objects with complex emitting and reflecting behaviour, it will always reach a point where the description of the light received (and consequently emitted on the other side) by the wall is simpler than the description of the exchange of light between the two sides. This is first because photons do not interact with each other, and because I assume that I can represent the light flux in a compact yet precise way (guess what I will use?). Now of course the problem is that some of the light reaching one side will bounce back to illuminate the other side, and so on.. If we assume that the light effects are linear (not always true in the vast physical world, but if we cannot assume this, "radiosity" and "ray-tracing" are also dead in the water), all we have to do is repeat the process. How many times? Well first we can wait until each side has settled down and only then sent the result to the other side. But then (especially after the emitters on each side have been taken care of) the amount of energy (actually power in a steady state) can only decrease, guaranteeing convergence. How fast? Well, consider a situation where 20% (quite generous) of the light received from one side is sent back to the other side. The fraction left after N trips across is of course 5^-N, which is a respectable convergence rate. Can you say "divide and conquer"? I knew you could. In practice we do not create a single wall, but subdivide adaptively the world according to the amount of undistributed power it has and the complexity of the scene it contains (that's where the octree comes in). Peter Schroeder mentions visibility, and indeed it is a pesky problem. But note that we have only local visibility problems here. We don't care to know if objects not in the same cell can see each other or not. If they can't their light ain't there, but we do not know that explicitly. Note that if we have a closet full of junk that does not receive any light, we do not even look at them (I exaggerate slightly, it depends on where the cells' boundaries fall). Note also that it looks like the old Warnock algorithm for visibility (in spirit, not in practice). Jorge Stolfi mentioned the fact that the light coming from groups of Lambertian diffusers is not distributed like from a single planar Lambertian diffuser. Indeed, but we are not restricted in any way to Lambertian diffusers (which is good, since they are so rare in captivity). In fact the less diffuse the light is the better it is for this approach in some sense (I must point out the Lazlo Neumann (& Neumann) has a wonderful study of various situations for the distribution of reflected light in the standard approaches to global illumination and what to do about it, to appear in TOG soon, I hope). Jorge's last point about 3-way form factors is precisely the reason the light- driven approach is attractive, since we do not have to consider explicitly the exchanges between cells, let alone between objects. Per Christensen's point about "approximate" visibility is well taken. No matter how well you represent the light flux at the cell boundary, an adversary can set up scenes where you are very wrong (the adversary just has to know if there is a band-limit to the representation, and set up two parallel venetian blinds above the limit frequency, which can either block all the light or let about half of it pass). But any method based on finite representations is vulnerable to such tricks. That does not mean that we should not be careful, though. Let me reiterate that in our model the cells do not represent groups of objects, but only provide boundaries at which to represent the light flux. Thank you also to people like Nelson Max and Greg Ward who pointed at the Integra system and Fujimoto as a possible source for a similar approach; Jorge Stolfi also pointed at work by Leo Guibas and Veach. I will follow these leads. I am gathering some old stuff we wrote about this, together with more current stuff. The history is that Eugene Fiume and I started to work on this around 1988 in Toronto (with Marc Ouellette and Chuan Chee), submitted a paper to Siggraph '89, got rejected, resubmitted in 1990, same fate. Paradoxically a paper on a parallel implementation of the scheme (with George Drettakis and Eugene Fiume) was accepted and published at Eurographics '90. At UBC we shifted to a wavelet representation for light flux (with Bob Lewis), submitted a paper to the Eurographics workshop on rendering, again to no avail. We will post a decent draft on the web asap. Note that we have not submitted anything about this to sigwaf this year, so there is no danger of interfering with the blind review process. Last point for now: much to my dismay it makes global illumination amenable to an Object-Oriented approach. From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for kopp id AA06355; Mon, 6 Mar 95 02:20:10 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.10/8.6.9) with ESMTP id BAA16427 for ; Mon, 6 Mar 1995 01:44:43 +0100 Received: from merckx.graphics.cornell.edu (MERCKX.GRAPHICS.CORNELL.EDU [128.84.247.147]) by imag.imag.fr (8.6.10/8.6.9) with SMTP id BAA26352 for ; Mon, 6 Mar 1995 01:44:41 +0100 Received: by merckx.graphics.cornell.edu (5.65/DEC-Ultrix/4.3) id AA22559; Sun, 5 Mar 1995 19:45:02 -0500 Message-Id: <9503060045.AA22559@merckx.graphics.cornell.edu> Received: by zap.graphics.cornell.edu (1.37.109.8/16.2) id AA18791; Sun, 5 Mar 1995 19:44:40 -0500 From: Peter Shirley Subject: Re: BSP Tree [observed] complexity To: seth@theory.lcs.mit.edu Date: Sun, 5 Mar 1995 19:44:40 -0500 (EST) Cc: globillum@imag.fr In-Reply-To: <9503041846.ZM7864@jabiru.lcs.mit.edu> from "Seth Teller" at Mar 4, 95 06:46:27 pm X-Mailer: ELM [version 2.4 PL24] Mime-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 seth@lcs.mit.edu writes: > > i add my voice to don mitchell's: a thorough, objective empirical > examination of the average case (not worst case) behavior of BSP trees > is needed: a joint effort, perhaps using bruce's public-domain code > as an agreeable "standard" testbed. i propose that we tabulate: > > construction time; > total BSP complexity; > > and perhaps > > minimum achievable BSP complexity, > without regard to construction time > > as a function of: > > varying model type (desk, plane, building, person, etc.), and > increasing complexity (or level of detail) within each type. This is a great idea. Eric Haines started such a database for ray tracing that certainly made comparisons MUCH easier, and I think it is time to pick some models that are more representative of real scenes. Seth, could we use some or all of the Berkeley CS building? Classifying scene properties will be fun-- I like Seth's classifications from the 94 Siggraph paper, but a more extensive categorization is needed. I think BSP trees and ray tracing algorithms would both be good to test on such a database... Pete From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for kopp id AA07728; Mon, 6 Mar 95 09:50:40 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.10/8.6.9) with ESMTP id JAA24472 for ; Mon, 6 Mar 1995 09:18:41 +0100 Received: from mr.tuwien.ac.at (mr.tuwien.ac.at [128.130.2.10]) by imag.imag.fr (8.6.10/8.6.9) with SMTP id JAA00762 for ; Mon, 6 Mar 1995 09:18:25 +0100 Received: from stellaris.cg.tuwien.ac.at by mr.tuwien.ac.at with SMTP (PP); Mon, 6 Mar 1995 09:18:03 +0100 Received: from eigmq2.tuwien.ac.at by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for @EMAIL.TUWIEN.AC.AT:globillum@imag.fr id AA07418; Mon, 6 Mar 95 09:21:16 +0100 X-Sender: wp@stellaris.cg.tuwien.ac.at Message-Id: Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed Date: Mon, 6 Mar 1995 09:19:33 +0100 To: globillum@imag.fr From: Werner Purgathofer Subject: Re: Rendering Complex Scenes X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hello Alain, As you have not cited this in your Eurographics'90 paper, you might have overseen a very related approach by Xu, Peng, and Liang: "Accelerated Radiosity Method for Complex Environments", Eurographics'89 (North Holland). from the abstract: ... An () algorithm (), based on environment localization and the directional form-factor concept, is presented (). First we subdivide the object space into many regions. (). The radiant light energy transfer between different regions is evaluated at their common boundaries. ... Good luck! Werner ------------------------------------------------------------------- Werner Purgathofer Tel. +43(1)58801 4548 Institute of Computer Graphics ( secretary: 4549 ) Technical University of Vienna Fax. +43(1)5874932 Karlsplatz 13 / 186 email: wp@cg.tuwien.ac.at A-1040 Wien / Austria WWW: http://www.cg.tuwien.ac.at ------------------------------------------------------------------- From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for kopp id AA03612; Thu, 9 Mar 95 15:47:15 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.10/8.6.9) with ESMTP id OAA09517 for ; Thu, 9 Mar 1995 14:38:04 +0100 Received: from mr.tuwien.ac.at (pop.tuwien.ac.at [128.130.2.10]) by imag.imag.fr (8.6.10/8.6.9) with SMTP id OAA07088 for ; Thu, 9 Mar 1995 14:38:02 +0100 Received: from stellaris.cg.tuwien.ac.at by mr.tuwien.ac.at with SMTP (PP); Thu, 9 Mar 1995 14:27:31 +0100 Received: from eigpc5.tuwien.ac.at by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for @EMAIL.TUWIEN.AC.AT:globillum@imag.fr id AA03005; Thu, 9 Mar 95 14:30:43 +0100 Date: Thu, 9 Mar 95 14:30:43 +0100 Message-Id: <9503091330.AA03005@stellaris.cg.tuwien.ac.at> X-Sender: kopp@stellaris.cg.tuwien.ac.at Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed To: globillum@imag.fr From: Manfred Kopp Subject: CFP: 6th Eurographics Workshop on Rendering X-Mailer: X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit ================================================== 6th Eurographics Workshop on Rendering Dublin, Ireland 12-14 June 1995 ================================================== CALL FOR CONTRIBUTIONS ================================================== Aims and Scope: Following five successful workshops (Rennes-1990, Barcelona-1991, Bristol-1992, Paris-1993, Darmstadt-1994) we announce the sixth Workshop on Rendering Techniques. The workshop is now well established as a major international forum in exchanging experience and knowledge between people from universities, research, and industry, interested in the different aspects of rendering techniques. Main topics include (but are not restricted to): - Radiosity - Ray Tracing - Illumination Models - Color, Texture - Sampling, Filtering, Anti-aliasing - Parallel Algorithms for Rendering This workshop also encourages to submit "unfinished" work, "incomplete" ideas, and "only partially" implemented new techniques and perspectives. This year the discussion parts will be extended even more than in previous years, enabling the participants to actively query all uncertainties after the paper presentations. Additionally, internationally well-known speakers will give invited lectures. Participation will be limited to approximately 80 people. Call for Contributions: Authors are requested to send five copies of a full paper including figures and images (max. 10 pages) or a complete e-mail version (LaTeX or PostScript) to one of the program chairs. Please include a separate sheet containing the title and the author(s) of the paper, indicating which author shall be contacted, including your telephone, fax and e-mail address. Submissions missing the deadline can only be considered in exceptional cases and with reduced priority. A copied version of all papers will be distributed to all workshop participants, a complete proceedings book will appear shortly after the workshop (by Springer-Verlag). Schedule: 4 April, 1995 Submission deadline 4 May, 1995 Notification of acceptance 29 May, 1995 Full-paper deadline for proceedings 12-14 June, 1995 Workshop Organization: The workshop will take place in Dublin, Ireland, and is organized by the Trinity College Dublin in association with Eurographics. The fee of about 250 SFr for EG members (350 SFr for non-members) includes lunch, coffee in the breaks, workshop handouts and the final proceedings book (will be mailed after the workshop). A social event is also planned and will be charged separately. Organizing Chair: Steven Collins (IRL) Program Chairs: Pat Hanrahan (USA), Werner Purgathofer (A) Program Committee: K. Anjyo (J), K. Bouatouch (F), A. Chalmers (UK), M. Cohen (USA), M. Feda (A), A. Glassner (USA), S. Green (UK), P. Heckbert (USA), F. Jansen (NL), E. Nakamae (J), L. Neumann (H), S. Pattanaik (IND), C. Puech (F), X. Pueyo (E), H. Rushmeier (USA), G. Sakas (D), D. Salesin (USA), Ch. Schlick (F), P. Shirley (USA), Ph. Slusallek (D), F. Sillion (F), A. de Sousa (P), G. Ward (USA) Organization office: Steven Collins, Comp. Science, Trinity College, Dublin 2, Ireland Tel.: +353-1-7021436 Fax: +353-1-6772204 e-mail: rw6@cs.tcd.ie Send papers to either: Pat Hanrahan, Stanford University, 217 Center for Integrated Systems, Stanford, CA 94305-4070, USA, Tel. +1-415-723-8530 e-mail: hanrahan@cs.stanford.edu or to Werner Purgathofer, TU Wien, Karlsplatz 13/186, A-1040 Vienna/Austria Tel. +43-1-58801-4548 Fax: +43-1-5874932 e-mail: wp@cg.tuwien.ac.at ================================================== From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for kopp id AA14724; Fri, 21 Apr 95 20:43:33 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id UAA14319 for ; Fri, 21 Apr 1995 20:14:19 +0200 Received: from netmail2.microsoft.com (netmail2.microsoft.com [131.107.1.13]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id UAA12393; Fri, 21 Apr 1995 20:14:16 +0200 Received: by netmail2.microsoft.com (5.65/25-eef) id AA10516; Fri, 21 Apr 95 11:16:25 -0700 Message-Id: <9504211816.AA10516@netmail2.microsoft.com> Received: by netmail2 using fxenixd 1.0 Fri, 21 Apr 95 11:16:25 PDT X-Msmail-Message-Id: F6055F1D X-Msmail-Conversation-Id: F6055F1D From: Andrew Glassner To: globillum@imag.fr, globillum-request@imag.fr Date: Fri, 21 Apr 95 11:08:11 TZ Subject: RE: Definition of "Radiosity method"? X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit | | 1. A FE method for lambertian scenes. | | 2. A solution that somehow uses linear equations to represent light | transport in a lambertain scene. | | 3. A FE method for global illumination (would include Sillion et a. '91). | | 4. An algorithm that computes view-independent illumination information. | I tempted to agree with Francois in liking #4 the best, but it's too general. It can contain things that we don't want to call radiosity, like systems that decimate the world into cubes and do physical optics, propagating wavefronts from cube to cube. That's so far in spirit from the original use of radiosity that the term becomes so vague as to be useless. I'd reserve "radiosity" for FE methods like #3 (though Francois is right that it's not even such a good word for that). The problem is that as different things are added to the basic ideas of classical radiosity, the term seems to need to grow to accomodate them all. Maybe we can take a cue from the filter folks (with IIR and FIR filters) and refer to view-dependent illumination and view-independent illumination as VDI and VII algorithms; then classical radiosity algorithms are a subclass of the VII algorithms. So Radiance implements a VII method, but it's not radiosity. -Andrew From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for kopp id AA15057; Sat, 22 Apr 95 00:21:11 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id XAA16326 for ; Fri, 21 Apr 1995 23:54:18 +0200 Received: from netmail2.microsoft.com (netmail2.microsoft.com [131.107.1.13]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id XAA14487; Fri, 21 Apr 1995 23:54:13 +0200 Received: by netmail2.microsoft.com (5.65/25-eef) id AA26415; Fri, 21 Apr 95 14:56:22 -0700 Message-Id: <9504212156.AA26415@netmail2.microsoft.com> Received: by netmail2 using fxenixd 1.0 Fri, 21 Apr 95 14:56:22 PDT X-Msmail-Message-Id: 3DA7EB16 X-Msmail-Conversation-Id: 3DA7EB16 From: Andrew Glassner To: globillum@imag.fr, globillum-request@imag.fr Date: Fri, 21 Apr 95 14:48:30 TZ Subject: RE: Definition of "Radiosity method"? X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit I wrote (and I quote): | Maybe we can take a cue from the filter folks (with IIR and FIR filters) | and refer to view-dependent illumination and view-independent | illumination as VDI and VII algorithms; then classical radiosity algorithms are | a subclass of the VII algorithms. So Radiance implements a VII method, | but it's not radiosity. As Seth pointed out, new acronyms are tricky. When I said that Radiance is VII, I meant the part that deposits little diffuse packets on surfaces. This is driven, in part, by a VDI algorithm. Another reason, perhaps, why we ought not to let one term grow to encompass everything. From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for kopp id AA13949; Fri, 21 Apr 95 17:49:40 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id RAA07441 for ; Fri, 21 Apr 1995 17:06:22 +0200 Received: from merckx.graphics.cornell.edu (MERCKX.GRAPHICS.CORNELL.EDU [128.84.247.147]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id RAA08344 for ; Fri, 21 Apr 1995 17:06:18 +0200 Received: by merckx.graphics.cornell.edu (5.65/DEC-Ultrix/4.3) id AA10681; Fri, 21 Apr 1995 11:06:42 -0400 Message-Id: <9504211506.AA10681@merckx.graphics.cornell.edu> Received: by zap.graphics.cornell.edu (1.37.109.8/16.2) id AA27183; Fri, 21 Apr 1995 11:06:12 -0400 From: Peter Shirley Subject: Definition of "Radiosity method"? To: globillum@imag.fr Date: Fri, 21 Apr 1995 11:06:12 -0400 (EDT) X-Mailer: ELM [version 2.4 PL24] Mime-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 < summary-- I want feedback on a proposed definition for "radiosity method"> Because of some comments in some siggraph reviews I have been researching the definition of "radiosity method". There are four obvious candidates given the usage I have seen: 1. A FE method for lambertian scenes. 2. A solution that somehow uses linear equations to represent light transport in a lambertain scene. 3. A FE method for global illumination (would include Sillion et a. '91). 4. An algorithm that computes view-independent illumination information. I have problems with all of these definitions. For example, if I use definition 1, is Pattanaik's thesis code a radiosity method in an all diffuse scene? Probably not, but I think most of us would want to call it a radiosity method. And how about Sillion and Puech '89? There are mirrors in their work-- is it radiosity? Jim Arvo has proposed a definition I want to float: A radiosity method computes radiosity (or irradiance) for at least some surfaces in the scene. This definition will encompass both FE and MC methods that compute quantities for the diffuse surfaces in a scene. It would not include Sillion et al. '91 (which could be a "radiance" method I suppose). Reactions? Pete From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for kopp id AA14026; Fri, 21 Apr 95 18:17:44 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id RAA09490 for ; Fri, 21 Apr 1995 17:43:30 +0200 Received: from safran-28.imag.fr (safran.imag.fr [129.88.29.1]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id RAA09598; Fri, 21 Apr 1995 17:43:29 +0200 Received: (sillion@localhost) by safran-28.imag.fr (8.6.10/8.6.4) id PAA18716; Fri, 21 Apr 1995 15:43:16 GMT From: Francois Sillion Message-Id: <199504211543.PAA18716@safran-28.imag.fr> Subject: Re: Definition of "Radiosity method"? To: Peter Shirley Date: Fri, 21 Apr 1995 17:43:15 +0200 (MDT) Cc: Global Illumination List In-Reply-To: <9504211506.AA10681@merckx.graphics.cornell.edu> from "Peter Shirley" at Apr 21, 95 11:06:12 am Reply-To: Francois.Sillion@imag.fr X-Mailer: ELM [version 2.4 PL23] Mime-Version: 1.0 Content-Type: text/plain; charset=windows-1252; format=flowed Content-Transfer-Encoding: 8bit X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 < summary-- feedback on a proposed definition for "radiosity method"> I tend to think of a "radiosity method" whenever information is computed and attached to the surfaces, thus it includes illumination maps and 'light path tracing', as well as techniques where lambertian or directional radiant information is exchanged with form factors. In fact, I realize that any method that stores *some* radiant information is for me *a* radiosity method. *The* radiosity method, on the other hand, should be reserved for Lambertian surfaces with form factors etc... I think it is a pity to have inherited such a name (radiosity is not a method, but a radiant quantity), and I personally oppose the use of the similar 'radiance' method. I vote for item # 4 in your list: > Because of some comments in some siggraph reviews I have been > researching the definition of "radiosity method". There are > four obvious candidates given the usage I have seen: > > 1. A FE method for lambertian scenes. > > 2. A solution that somehow uses linear equations to represent light > transport in a lambertain scene. > > 3. A FE method for global illumination (would include Sillion et a. '91). > > 4. An algorithm that computes view-independent illumination information. > +------------------+---------------------------+--------------------------+ | | iMAGIS / IMAG | Tel: (+33) 76 51 43 54 | | Francois SILLION | B.P. 53 | Fax: (+33) 76 44 66 75 | | ' | F-38041 Grenoble Cedex 09 | Francois.Sillion@imag.fr | +------------------+---------------------------+--------------------------+ From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for kopp id AA16043; Sat, 22 Apr 95 08:35:55 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id IAA21089 for ; Sat, 22 Apr 1995 08:21:02 +0200 Received: from grolsch.cs.ubc.ca (grolsch-2.cs.ubc.ca [142.103.5.5]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id IAA18746 for ; Sat, 22 Apr 1995 08:21:00 +0200 Received: (from ean@localhost) by grolsch.cs.ubc.ca (8.6.10/8.6.9) id XAA06038; Fri, 21 Apr 1995 23:16:36 -0700 X400-Received: by /PRMD=ca/ADMD=telecom.canada/C=ca/; Relayed; Fri, 21 Apr 1995 23:16:32 UTC-0700 Date: Fri, 21 Apr 1995 23:16:32 UTC-0700 X400-Originator: fournier@cs.ubc.ca X400-Recipients: non-disclosure:; X400-Content-Type: P2-1984 (2) X400-Mts-Identifier: [/PRMD=ca/ADMD=telecom.canada/C=ca/;950421231632] Content-Identifier: 4103 From: Alain Fournier To: "Ian Ashdown (return)" <72060.2420@CompuServe.COM> Cc: "Global Illumination (return)" In-Reply-To: <950422045648_72060.2420_FHG18-1@CompuServe.COM> Message-Id: <"4103*fournier@cs.ubc.ca"@MHS> Subject: RE: Definition of "Radiosity method"? Mime-Version: 1.0 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed Content-transfer-encoding: 8bit Ah, the thrill of lexicography! We all realize that there will not be any definition that satisfies our understanding of an expression like "radiosity method", or any expression that covers exactly what we mean by any definition that would satisfy our understanding of it, if it were to exist. I hope I made myself clear. But seriously, folks... Things only mean what we say they mean. Take "finite element" for example. There is no way you would know what that means just looking at it, and even after hearing a definition (try one that does not take two pages and/or does not include just about everything that is computed) you still are not too sure what it starts and where it ends. The safest for us is that whenever we use an expression like "radiosity" we briefly say what we mean by it --in the particular context where it is used--. I had to do this recently because I wrote about using "arbitrary" BRDFs within the "classic" radiosity approach. In this context I called the classic radiosity approach "linear radiosity", thus approaching very closely definition 2. of Peter, except that surfaces are not necessarily Lambertian. Obviously "linear" here refers to the system of equations obtained. I actually like the use of the synecdoche for "radiosity", as long as we don't forget that anything that computes illumination in a useful way will have to be able to compute radiosity --the radiometric quantity. Few more things. I agree with Ian that we owe it to the other communities not to change arbitrarily the meaning of expressions they have been using for a while. I disagree with him about needing a taxonomy. To paraphrase Sam Goldwyn ("verbal agreements are not worth the paper they are written on"), taxonomies are usually not worth the theory they are not based on (I have indulged in the past, but I don't have to be consistent). Recently at a "PhD Thesis Proposal" (one of the events we cherish here in our department), the "candidate" was attacked because he used the word "illumination" in his title. The objection was that illumination is a quantity, not a topic or an area of research. Of course it used to be a quantity, but it never was only that, and it is now "deprecated", as they say, as a quantity. The candidate replied too politely. There are times when a graduate student should be able to tell a full prof that he is full of it (OK, maybe that was NOT the time...). In conclusion: we have to be as clear as possible, but not clearer. From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for kopp id AA16165; Sat, 22 Apr 95 09:29:44 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id JAA21384 for ; Sat, 22 Apr 1995 09:11:20 +0200 Received: from netmail2.microsoft.com (netmail2.microsoft.com [131.107.1.13]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id JAA19200 for ; Sat, 22 Apr 1995 09:11:18 +0200 Received: by netmail2.microsoft.com (5.65/25-eef) id AA26783; Sat, 22 Apr 95 00:13:40 -0700 Message-Id: <9504220713.AA26783@netmail2.microsoft.com> Received: by netmail2 using fxenixd 1.0 Sat, 22 Apr 95 00:13:39 PDT X-Msmail-Message-Id: D37CFA1E X-Msmail-Conversation-Id: D37CFA1E From: Don Mitchell To: globillum@imag.fr Date: Fri, 21 Apr 95 23:58:08 TZ Subject: radiosity X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit I think a totalizing definition of radiosity would be easily deconstructed by the inherent contradictions in the binary opposition of radiosity and ray tracing. Wouldn't you agree, Alain? From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for kopp id AA15933; Sat, 22 Apr 95 07:19:09 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id HAA20619 for ; Sat, 22 Apr 1995 07:01:36 +0200 Received: from dub-img-3.compuserve.com (dub-img-3.compuserve.com [198.4.9.3]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id HAA18400 for ; Sat, 22 Apr 1995 07:01:34 +0200 Received: by dub-img-3.compuserve.com (8.6.10/5.941228sam) id BAA17245; Sat, 22 Apr 1995 01:00:11 -0400 Date: 22 Apr 95 00:56:48 EDT From: Ian Ashdown <72060.2420@CompuServe.COM> To: Global Illumination Subject: RE: Definition of "Radiosity method"? Message-Id: <950422045648_72060.2420_FHG18-1@CompuServe.COM> X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Call me a traditionalist, but I prefer to think of radiosity methods (plural) as finite element methods. They were in use as such for over 50 years before they were appropriated for computer graphics applications, and were called "radiosity methods" by Sparrow way back in 1963. It seems rather presumptuous to be fiddling with the basic definition some thirty years later to suit our particular needs. I see no particular problem with incorporating nondiffuse surfaces within the definition of radiosity methods. This allows for Pete's third definition, "an FE method for global illumination." However, adding Monte Carlo ray tracing to the definition (via Jim Arvo's proposal) may not be a good idea. One objection is that this would conflict with the similar definition of "radiative flux transfer" in the illumination engineering community. We lighting nerds clearly (and sometimes passionately) distinguish radiative transfer methods from Monte Carlo ray tracing techniques. The variety of global illumination algorithms we now have clearly calls for some sort of reasoned taxonomy to describe and classify them. Whatever this may be, however, I would argue that we should not attempt to redefine "radiosity methods" beyond that commonly understood within the computer graphics, thermal engineering, illumination engineering, and acoustic engineering communities. - Ian Ashdown From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for kopp id AA17577; Sat, 22 Apr 95 14:07:08 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id NAA02428 for ; Sat, 22 Apr 1995 13:55:03 +0200 Received: from merckx.graphics.cornell.edu (MERCKX.GRAPHICS.CORNELL.EDU [128.84.247.147]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id NAA20701 for ; Sat, 22 Apr 1995 13:55:02 +0200 Received: by merckx.graphics.cornell.edu (5.65/DEC-Ultrix/4.3) id AA20346; Sat, 22 Apr 1995 07:55:30 -0400 Message-Id: <9504221155.AA20346@merckx.graphics.cornell.edu> Received: by gaia.graphics.cornell.edu (1.37.109.8/16.2) id AA14552; Sat, 22 Apr 1995 07:54:59 -0400 From: Peter Shirley Subject: Clarification on question To: globillum@imag.fr Date: Sat, 22 Apr 95 7:54:59 EDT Mailer: Elm [revision: 70.85] X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Thanks for the interesting responses so far! Here are three methods that estimate "radiosity" in a view-ind. manner: 1. Wallace: uses explicit patch-to-patch ray tracing and solves linear system. 2. Airey: uses Malley-style form factor computation using random directional ray shooting. 3. Pattanaik: uses photon-like particle walks and counts collisions with "zones" on the surfaces. I think 1 and 2 are FE methods. Number 3 is probably not under most definitions (e.g. Cohen and Wallace's book). But 2 and 3 are SO close conceptually and in code. The biggest difference is that in 2 a particle can leave the patch from a slightly different location than it hits. I am very uncomfortable with a definition of "radiosity method" that includes only one of 2 or 3. I also think we will confuse heat transer and illumination engineering people if we include methods such as Sillion et al. '91 which might never compute a "radiosity" anywhere. Pete PS-- one thing I AM sure of now-- the is NOT an accepted definition. This is something we should take care of culturally (rather than "officially") or we are doing a great disservice to future graphics people. From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via SMTP (931110.SGI/910805.SGI) for kopp id AA18621; Sat, 22 Apr 95 17:33:52 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id RAA08163 for ; Sat, 22 Apr 1995 17:23:11 +0200 Received: from merckx.graphics.cornell.edu (MERCKX.GRAPHICS.CORNELL.EDU [128.84.247.147]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id RAA22172 for ; Sat, 22 Apr 1995 17:23:09 +0200 Received: by merckx.graphics.cornell.edu (5.65/DEC-Ultrix/4.3) id AA27291; Sat, 22 Apr 1995 11:23:37 -0400 Message-Id: <9504221523.AA27291@merckx.graphics.cornell.edu> Received: by zap.graphics.cornell.edu (1.37.109.8/16.2) id AA05999; Sat, 22 Apr 1995 11:23:07 -0400 From: Jim Arvo Subject: the meaning of radiosity To: globillum@imag.fr Date: Sat, 22 Apr 1995 11:23:07 -0400 (EDT) X-Mailer: ELM [version 2.4 PL24] Mime-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 I'd like to offer a few thoughts on the use of the term "radiosity". The gist of my argument is that the simplest definition of the term seems to be most useful; making it more general or more specific causes problems. I advocate the following definition (which Pete Shirley already tossed out): A "radiosity algorithm" is an algorithm that generates radiosity-like quantities associated with surfaces (i.e. power per unit area, or the photometric equivalent) based on radiative transfer. Note that there is no reference to how this is done, whether all the surfaces are Lambertian, or whether there is any dependence on the view. The latter distinctions can be made by context or by attaching modifiers. As a very crude analogy, consider sorting algorithms. Any algorithm that generates a sorted list of things is a sorting algorithm, regardless of how it is done. If the "how" is important, then we may specify "quick sort", "heap sort", etc. Before getting into the real argument, I'd like to propose some rationale for why we invent terminology in the first place. It seems to me that a bit of terminology will catch on (and improve our lives) if it is 1) unambiguous (makes a clear distinction) 2) convenient (concise and makes a useful distinction) 3) self evident (agrees with intuition and/or common usage) Clearly these will often conflict, so it's not always possible to satisfy them all. In general, we try to satisfy these criteria by using short pithy terms for large classes of things (or extremely fundamental things), and attaching modifiers to call out specific sub-categories. I believe that the above definition of a radiosity algorithm is a good one with respect to these criteria. If the term "radiosity" is made more specific, such as by limiting it to finite element methods, then we shall need to 1) agree upon what a finite element method is, and 2) refrain from calling anything a radiosity method if it is not a finite element method. I believe there are problems on both counts. Consider the method developed by both Pattanaik and Shirley, which estimates radiosities on discrete elements via random walks. Is this a Monte Carlo method or a finite element method? If you focus on the path tracing, it is Monte Carlo. If you focus on (the expected values of) the estimated quantities, it is a Galerkin finite element method. Whether it is classified as a "radiosity" method should not (in my opinion) depend on which aspect you deem most relevant. As a second example, consider Hanrahan's original hierarchical radiosity method -- a Galerkin approach with constant elements. I believe there is universal agreement that this should be called a "radiosity" method. However, the form factors are computed using Monte Carlo, so one could argue that it is actually a Monte Carlo method (after all, it makes calls to "rand", right?). Is it therefore NOT a radiosity method? As a third example, consider an algorithm based on the Nystrom method: that is, a method that replaces the integral operator with a quadrature rule based on point-to-point transfers (i.e. no form factors). This is a deterministic method that is not a finite element method. However, it is very much like a finite element method. I would really like to call it "Nystrom radiosity" if what it computes is radiosity. Does this not seem very appropriate? As a final example, consider a hypothetical algorithm that can transform a simple scene (such as the "Cornell box") into an equivalent problem with an analytic solution. I know of no such algorithm, but I would not hesitate to call it a radiosity algorithm since it solves the same type of problem (albeit, without any type of projection onto an approximating subspace, which is inherent in finite element methods). In view of the above, I feel that including "finite element" in the definition of a radiosity method fails on two counts: 1) it is ambiguous, since it depends on which aspect of the problem you deem most important (sometimes we choose to ignore the Monte Carlo aspect, and sometimes we don't), and 2) it fails to make a useful distinction. Because of an historical accident (finite element methods came along first) it separates methods that seem to belong together because of their *function*. If it's important to distinguish the "how", it's easy to do so by adding a modifier like "finite element", "stochastic", "Nystrom", "analytic", etc. On the other hand, if the term is made more general by including methods that solve for surface radiance functions, then just about everything becomes a radiosity algorithm. I feel that we then lose a very useful distinction. I believe that one of the most fundamental distinctions among global illumination algorithms is whether they generate functions with directional dependence or not. Since the word "radiosity" taken by itself implies that there is no such dependence, the term is self evident only if we preserve that connotation; moreover, doing so agrees with most prior usage. Whether an algorithm is based on Monte Carlo or a finite element method, is view-dependent or view-independent, can be cleared up nicely by attaching the appropriate modifier when context alone is inadequate. Here are a few examples, which I'm sure will cause some controversy. I apologize in advance for leaving out so many references and for using such terse abbreviations -- I've listed just a few obvious examples in order to illustrate. (I hope I got most of these right.) Radiosity: Any method that produces radiosity (or irradiance, or luminosity) as its output. Examples: [Goral 84] [Cohen 85] [Sillion 89] [Rushmeier 90] [Shirley 90] [Pattanaik 90] [Hanrahan 91] [Zatz 93] [Troutman 93] [Gortler 93] [Smits 94] View-dependent radiosity: Solves for radiosities of visible surfaces, or some closely related set of surfaces. Example: [Smits 92], if importance is driven by the view, and not some other criteria. Also includes view-dependent path tracing, such as [Ward 88]. Radiosity with non-diffuse surfaces: ("non-diffuse radiosity" sounds like an oxymoron) One that takes non-diffuse transfers into account, but still produces only radiosities (or irradiances, or luminosities). Examples: [Sillion 89], [Rushmeier 90] Radiosity with participating media: One that solves for both surface radiosities [watts/m^2] and energy densities [watts/m^3] (the natural analogue of radiosity in a volume). Example [Rushmeier 87] Radiance method: An algorithm that produces surface radiance functions (I believe that all are currently view-dependent). Examples: Ward's RADIANCE system, [Kajiya 86] [Wallace 87] [Sillion 91] [Aupperle 93] (Note that this may involve a "radiosity" first-pass with a view-dependent path tracing second-pass). Radiance with participating media: One that solves for radiance functions at surfaces and/or in space, with at least one of them having directional variation. Example: [Max 94] Global illumination method: Any of the above. Now, even if everyone were to agree with the above argument (which is HIGHLY unlikely, I realize :-), we would still not be out of the woods. Should the definition also be more specific about the underlying physics (this was Andrew's point, I believe). What about direct illumination only? What about classical ray tracing (direct illumination plus pure specular chains)? My feeling is that we want to rule these out, but I'm wary of making the definition too specific, so I've not addressed this point (which seems to be a non-problem anyway). -- Jim Arvo From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id XAA00802; Sun, 23 Apr 1995 23:29:11 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id XAA24878 for ; Sun, 23 Apr 1995 23:14:01 +0200 Received: from june.cs.washington.edu (june.cs.washington.edu [128.95.1.4]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id XAA06529 for ; Sun, 23 Apr 1995 23:13:57 +0200 Received: (per@localhost) by june.cs.washington.edu (8.6.12/7.2ju) id OAA07899; Sun, 23 Apr 1995 14:13:55 -0700 Date: Sun, 23 Apr 1995 14:13:54 -0700 (PDT) From: "Per H. Christensen" To: globillum@imag.fr Subject: Re: Definition of "Radiosity method"? Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII; format=flowed X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit In my opinion, the term "radiosity method" should only be used for a method that *computes radiosity*. Why extend the term "radiosity method" to mean something not computing radiosity? If we want to describe global illumination methods, why not be more specific and describe them as: 1) what they compute (diffuse, glossy, specular, general), 2) the solution method (for example finite elements or Monte Carlo). For example, a more precise term for the classic radiosity method would be "a finite element method for diffuse global illumination". Jim Arvo proposed: > A radiosity method computes radiosity (or irradiance) for > at least some surfaces in the scene. I would favor a definition even more restrictive than this: a method that computes only radiosity, that is, no directional radiance information at all. With this definition of the term "radiosity method", the following classifications result: Pattanaik's thesis code working in a purely diffuse scene would be a radiosity method, I would call it "Monte Carlo solution of diffuse global illumination". If the scene had some non-diffuse reflection, it would not be a radiosity method, since the solution could not be described in terms of just radiosity (but requires radiance). Sillion et al '91 would not be a "radiosity method" since it computes directional radiance. I would describe it as a "finite element method for (general) global illumination". This avoids the term "radiance method" which several people dislike. Sillion and Puech '89 computes radiosity, but intermediate specular reflections are taken into account, I would call it something like "a finite element method for diffuse and specular global illumination". The computation method has nothing to do with whether the result is radiosity or not. Furthermore, whether the solution is view-dependent has nothing to do with whether the method computes radiosity or not. For example, Smits' et al '92 compute view-dependent radiosity solutions (at least the accuracy is view-dependent). Regards, -- Per From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id MAA01380; Tue, 25 Apr 1995 12:50:20 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id RAA18582 for ; Mon, 24 Apr 1995 17:46:08 +0200 Received: from fs1.cam.nist.gov (fs1.cam.nist.gov [129.6.80.33]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id RAA12347 for ; Mon, 24 Apr 1995 17:46:03 +0200 Received: from plum (plum.cam.nist.gov) by fs1.cam.nist.gov (4.1/SMI-DDN) id AA11712; Mon, 24 Apr 95 11:45:33 EDT Received: by plum (950215.SGI.8.6.10/SMI-3.2) id LAA12665; Mon, 24 Apr 1995 11:45:32 -0400 From: "Holly E Rushmeier" Message-Id: <9504241145.ZM12663@plum.cam.nist.gov> Date: Mon, 24 Apr 1995 11:45:31 -0400 X-Mailer: Z-Mail (3.1.0 22feb94 MediaMail) To: globillum@imag.fr Subject: terminology, taxonomy, was defn of "Radioisty" Content-Type: text/plain; charset=us-ascii; format=flowed Mime-Version: 1.0 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hi I am glad this topic came up. I think taxonomies are really useful. They are a useful guide for people who want to use an existing method for their application. I'm prejudiced, but I think a useful taxonomy has been developed in the NIST Guide to Available Mathematical software (http://gams.nist.gov/). It helps people sift through all the various software repositories and find code that will solve their problem. People in the lighting community have recognized the problem in terminology and classifying methods. Michael Smith from Lighting Technologies is heading a CIE technical committee on computer procedures for lighting metrics and visualization. A major problem they hope to address is that users have no idea how to choose a lighting software package based on how it does calculations, because there is no standard vocabularly to talk about how the calculations are done. The committee is supposed to present a report that introduces a standard terminology for describing lighting calculations, gives a survey of algorithms and description of each, prepates a set of guidelines for what method should be used for what application, and produces an extensive set of references. Anyway, the point of all this is that standards for terminology and taxonomies are in the works so it is really worthwhile keeping up the discussion. -- Holly From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id TAA07840; Sun, 30 Apr 1995 19:20:25 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id TAA20887 for ; Sun, 30 Apr 1995 19:10:18 +0200 Received: from merckx.graphics.cornell.edu (MERCKX.GRAPHICS.CORNELL.EDU [128.84.247.147]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id TAA27468 for ; Sun, 30 Apr 1995 19:10:15 +0200 Received: by merckx.graphics.cornell.edu (5.65/DEC-Ultrix/4.3) id AA28199; Sun, 30 Apr 1995 13:09:43 -0400 Message-Id: <9504301709.AA28199@merckx.graphics.cornell.edu> Received: by zap.graphics.cornell.edu (1.37.109.8/16.2) id AA25369; Sun, 30 Apr 1995 11:09:13 -0600 From: Peter Shirley Subject: Another unscientific survey To: globillum@imag.fr Date: Sun, 30 Apr 95 11:09:13 MDT Mailer: Elm [revision: 70.85] X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit After our most recent discussions, it is clear to me that there is no accepted def'n for a "radiosity method" (in the rendering communit anyway)y. I have no feel for whether there is approximate aggreement however. I would like to get at this by having people on the list answer three questions from which a definition becomes implicit. Question 1: A radiosity method must be a finite element method (agree/disagree). Question 2: A radiosity method must estimate radiosity (radiant exitance), irradiance, or an analogous photometric quantity (agree/disagree). (as opposed to estimating radiance, etc.). Question 3: A radiosity method must compute a view-independent solution (agree/disagree). (for the sake of simplicity, meshing can be based on importance or viewpoint and still be view-independent). Please send responses to shirley@graphics.cornell.edu From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id UAA09004; Sun, 30 Apr 1995 20:52:51 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id UAA21650 for ; Sun, 30 Apr 1995 20:43:13 +0200 Received: from merckx.graphics.cornell.edu (MERCKX.GRAPHICS.CORNELL.EDU [128.84.247.147]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id UAA29122 for ; Sun, 30 Apr 1995 20:43:11 +0200 Received: by merckx.graphics.cornell.edu (5.65/DEC-Ultrix/4.3) id AA01644; Sun, 30 Apr 1995 14:43:40 -0400 Message-Id: <9504301843.AA01644@merckx.graphics.cornell.edu> Received: by zap.graphics.cornell.edu (1.37.109.8/16.2) id AA25799; Sun, 30 Apr 1995 12:43:10 -0600 From: Peter Shirley Subject: READ THIS FIRST-- survey To: globillum@imag.fr Date: Sun, 30 Apr 95 12:43:10 MDT Mailer: Elm [revision: 70.85] X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Peter S, Jim A, and Dani L all gave me some valuable debugging on the previous version of the survey. Please answer these FOUR questions instead. After our most recent discussions, it is clear to me that there is no accepted def'n for a "radiosity method" (in the rendering communit anyway)y. I have no feel for whether there is approximate aggreement however. I would like to get at this by having people on the list answer four questions from which a definition becomes implicit. Question 1: A radiosity method must be a finite element method (agree/disagree). Question 2: A radiosity method must estimates a radiometric quantity for Lambertian surfaces only (agree/disagree). Question 3: A radiosity method may account for diffuse-specular-diffuse transfer. Question 4: A radiosity method must compute a radiometric quantity for (at least) every Lambertian surface in the environment (agree/disagree). Please send responses to shirley@graphics.cornell.edu Notes: Question 1 is asking whether Malley '88 MS thesis is a radiosity method (this may be an FE method-- so also is asking whether Pattanaik's particle tracing is a radiosity method). Question 2 is asking whether methods such as Sillion et al. 91 is a radioisty method. Question 3 is really asking whether Sillion and Puech is a radiosity method. Question 4 is really asking whether a diffuse-only Kajiya style path tracer is a radiosity method. -- From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id SAA14824; Mon, 1 May 1995 18:44:44 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id SAA10837 for ; Mon, 1 May 1995 18:29:41 +0200 Received: from fs.CS.Princeton.EDU (fs.CS.Princeton.EDU [128.112.152.7]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id SAA22672 for ; Mon, 1 May 1995 18:29:40 +0200 Received: from cs (mfc@stilb.CS.Princeton.EDU [128.112.92.14]) by fs.CS.Princeton.EDU (8.6.10/8.6.9) with ESMTP id MAA19797 for ; Mon, 1 May 1995 12:29:38 -0400 From: Michael Cohen Received: by cs (940816.SGI.8.6.9/CS-Client) id MAA07328; Mon, 1 May 1995 12:29:36 -0400 Date: Mon, 1 May 1995 12:29:36 -0400 Message-Id: <199505011629.MAA07328@cs> To: globillum@imag.fr Subject: Radiosity X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit 1. Agree (but of course this begs the question to define FEM) 2. Disagree - it doesn't bother me to have people to use the title of Radiosity Methods with appropriate adjectives for non-diffuse environments. 3. Agree - as I think this is part of the definition of (1) I think about the problem like this. We can (in general) distinguish between two sets of methods. Those that compute coefficients for basis functions that are not defines with reference to the view (although the computation of the coefficients might be). The result would be view independent (although the accuracy might not). I'm happy to have all these called radiosity methods (although I would prefer they were all just called Finite Element Methods). The second set of methods computes coefficients to basis functions that are view dependent, i.e., for the light arriving at some region of the image. These methods I would refer to as Ray Tracing type methods. I realize this also is not a clean line, for example, where does this place Greg's Radiance system. I'd call it Ray Tracing based as although there is some diffuse information deposited in object space, the final computation of a solution is always in image space. -Michael From To: Peter Shirley From: Werner Purgathofer Subject: Re: Another unscientific survey Message-Id: X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Date: Tue, 2 May 1995 08:03:43 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Hi Peter, here are my votes: >Question 1: > A radiosity method must be a finite element method (agree/disagree). DISAGREE >Question 2: > A radiosity method must estimate radiosity (radiant exitance), > irradiance, or an analogous photometric quantity (agree/disagree). > (as opposed to estimating radiance, etc.). DISAGREE >Question 3: > A radiosity method must compute a view-independent > solution (agree/disagree). (for the sake of simplicity, > meshing can be based on importance or viewpoint and still > be view-independent). AGREE Sincerely, Werner From X-POP3-Rcpt: wp@stellaris Received: from merckx.graphics.cornell.edu by stellaris.cg.tuwien.ac.at via SMTP (940816.SGI.8.6.9/910805.SGI) for id NAA19578; Tue, 2 May 1995 13:59:07 +0200 Received: by merckx.graphics.cornell.edu (5.65/DEC-Ultrix/4.3) id AA24729; Tue, 2 May 1995 07:59:36 -0400 Message-Id: <9505021159.AA24729@merckx.graphics.cornell.edu> Received: by zap.graphics.cornell.edu (1.37.109.8/16.2) id AA11758; Tue, 2 May 1995 05:59:05 -0600 From: Peter Shirley Subject: Re: Another unscientific survey To: Werner Purgathofer Werner Purgathofer Date: Tue, 2 May 95 5:59:05 MDT In-Reply-To: ; from "Werner Purgathofer" at May 2, 95 8:03 am Mailer: Elm [revision: 70.85] X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Thanks Werner-- sorry-- did you see the next note with the modified questions? pete -- > > Hi Peter, here are my votes: > > Sincerely, > Werner > From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id SAA18575; Tue, 9 May 1995 18:44:58 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id SAA18368 for ; Tue, 9 May 1995 18:01:58 +0200 Received: from mr.tuwien.ac.at (pop.tuwien.ac.at [128.130.2.10]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id SAA09159 for ; Tue, 9 May 1995 18:01:53 +0200 Received: from stellaris.cg.tuwien.ac.at by mr.tuwien.ac.at with SMTP (PP); Tue, 9 May 1995 18:01:38 +0200 Received: from [128.130.166.50] by stellaris.cg.tuwien.ac.at via SMTP (940816.SGI.8.6.9/910805.SGI) for id SAA18269; Tue, 9 May 1995 18:01:35 +0200 X-Sender: wp@stellaris.cg.tuwien.ac.at Message-Id: Mime-Version: 1.0 Content-Type: text/plain; charset=windows-1252; format=flowed Date: Tue, 9 May 1995 18:02:22 +0100 To: globillum@imag.fr From: Werner Purgathofer Subject: Eurographics Rendering Workshop Advance Program X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit ----------------------------------------------------------- Advance Program of the Eurographics Rendering Workshop 1995 June 12-14, Dublin, Ireland for registration information please contact Steven.Collins@cs.tcd.ie or see the web at the url http://vangogh.cs.tcd.ie/rw6 ----------------------------------------------------------- Monday, 12 June 9:00-9:15 Opening 9:15-10:15 Keynote Speaker Jim Arvo + discussion "The Role of Functional Analysis in Global Illumination" 10:15-10:45 Coffee Break 10:45-12:00 Ray Tracing * Maurice van der Zwaan, Erik Reinhard, Frederik W. Jansen "Pyramid Clipping for Efficient Ray Traversal" * Eric P. Lafortune and, Yves D. Willems "A 5D Tree to Reduce the Variance of Monte Carlo Ray Tracing" * Yair Kurzion and Roni Yagel "Space Deformation using Ray Deflectors" ( each [ 15 min + 10 min discussion ]) 12:00-13:00 Reconstruction Techniques * Raghu Machiraju, Edward Swan, and Roni Yagel "Spatial Domain Characterization and Control of Reconstruction Errors" * N. Max and K. Ohsaki "Rendering trees from precomputed Z-buffer views" ( each [ 20 min + 10 min discussion ]) 13:00-14:30 Lunch 14:30-16:00 Volume Rendering * Tsukasa Noma "Bridging Between Surface Rendering and Volume Rendering for Multi-Resolution Display" * J. Stam "Multiple scattering as a diffusion process" * Georgios Sakas, Marcus Grimm, Alexandros Savopoulos "Optimized Maximum Intensity Projection (MIP)" ( [ 15 + 20 + 15 min ] + 25 min discussion) 15:45-16:15 Coffee Break 16:15-17:30 Illumination * Stefan MŸller, Wolfram Kresse, Frank Schšffel "A Radiosity Approach For The Simulation Of Daylight" * P.M. Deville and J.C. Paul "Modeling the Spatial Energy Distribution of Complex Light Sources for Lighting Engineering" * Pierre Poulin and Alain Fournier "Painting Surface Characteristics" ( each [ 15 min + 10 min discussion ]) Tuesday, 13 June 9:00-10:30 Hierarchical Radiosity * Sumanta N. Pattanaik and Kadi Bouatouch "Linear Radiosity with Error Estimation" * Nicolas Holzschuch and Francois Sillion "Isolating Discretisation Error: an Accurate Refinement Strategy for Hierarchical Radiosity with Linear Functions" * F. Sillion, G. Drettakis, C. Soler "A clustering algorithm for radiance calculation in general environments" ( each [ 20 min ] + 30 min discussion) 10:30-11:00 Coffee Break 11:00-12:30 Monte Carlo Radiosity * L.Neumann, W. Purgathofer, R.F. Tobler, A. Neumann, P. Elias, M. Feda, X. Pueyo "The Stochastic Ray Method for Radiosity" * Peter Shirley, Bretton Wade, Philip Hubbard, David Zareski, Bruce Walter, Donald P. Greenberg "Global Illumination via Density Estimation" * Mateu Sbert, Frederic Perez, Xavier Pueyo "Global Monte Carlo. A Progressive Solution" ( each [ 20 min ] + 30 min discussion) 12:30-14:00 Lunch 14:00-15:30 User Interface Aspects * H. Rushmeier, G. Ward, C. Piatko, P. Sanders, B. Rust "Comparing real and synthetic images: Some ideas about metrics" * J. Nimeroff, J. Dorsey, H. Rushmeier "A framework for global illumination in animated environments" * G. Ward "Making global illumination user friendly" ( each [ 15 min ] + 45 min discussion) 15:30-16:00 Coffee Break 16:00-17:30 "Can realistic rendering be applied to real problems?" (invited panel discussion, G. Sakas, G. Ward, J.C. Paul) Wednesday, 14 June 9:00-10:00 Wavelet Radiosity * Philipp Slusallek, Michael Schršder, Marc Stamminger, Hans-Peter Seidel "Smart Links and Efficient Reconstruction for Wavelet Radiosity" * P. Schršder, W. Sweldens "Spherical wavelets: texture processing" * R. Gershbein "A study of integration methods for couplings of Galerkin radiosity systems" ( each [ 15 min ] + 15 min discussion) 10:00-10:30 Coffee Break 10:30-11:30 Nondiffuse Radiosity * Steven Collins "Reconstruction of Indirect Illumination from Area Luminaires" * Kurt Zimmerman and Peter Shirley "A Two-Pass Realistic Image Synthesis Method for Complex Scenes" * A. Fournier "Separating reflection functions for linear radiosity" ( each [ 15 min ] + 15 min discussion) 11:30-12:30 "Radiosity Notations" (panel discussion, Peter Shirley) 12:30-14:00 Lunch 14:00-14:45 Radiosity Performance Improvements * L. Neumann, R.F. Tobler, P. Elias "The Constant Radiosity Step" * Gladimir Baranoski, Randall Bramley, and Peter Shirley "Fast Radiosity Solutions for High Average Reflectance Environments" ( each [ 15 min ] + 15 min discussion) 14:45-15:15 Coffee Break 15:15-16:30 Importance Sampling * Ph. DutrŽ, Y.D.Willems "Potential-driven Monte Carlo Particle Tracing for Diffuse Environments with Adaptive Probability Density Functions" * Philippe Bekaert and Yves D. Willems "Importance-Driven Progressive Refinement Radiosity" * Henrik Wann Jensen "Importance Driven Path Tracing using the Photon Map" ( each [ 15 min ] + 30 min discussion) 16:30-17:30 Keynote Speaker Alain Fournier + discussion "From Local to Global Illumination and Back" ------------------------------------------------------------------- Werner Purgathofer Tel. +43(1)58801 4548 Institute of Computer Graphics ( secretary: 4549 ) Technical University of Vienna Fax. +43(1)5874932 Karlsplatz 13 / 186 email: wp@cg.tuwien.ac.at A-1040 Wien / Austria WWW: http://www.cg.tuwien.ac.at ------------------------------------------------------------------- From To: Globillum From: Werner Purgathofer Subject: Eurographics Rendering Workshop Advance Program Message-Id: X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Date: Tue, 9 May 1995 18:02:18 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit ----------------------------------------------------------- Advance Program of the Eurographics Rendering Workshop 1995 June 12-14, Dublin, Ireland for registration information please contact Steven.Collins@cs.tcd.ie or see the web at the url http://vangogh.cs.tcd.ie/rw6 ----------------------------------------------------------- Monday, 12 June 9:00-9:15 Opening 9:15-10:15 Keynote Speaker Jim Arvo + discussion "The Role of Functional Analysis in Global Illumination" 10:15-10:45 Coffee Break 10:45-12:00 Ray Tracing * Maurice van der Zwaan, Erik Reinhard, Frederik W. Jansen "Pyramid Clipping for Efficient Ray Traversal" * Eric P. Lafortune and, Yves D. Willems "A 5D Tree to Reduce the Variance of Monte Carlo Ray Tracing" * Yair Kurzion and Roni Yagel "Space Deformation using Ray Deflectors" ( each [ 15 min + 10 min discussion ]) 12:00-13:00 Reconstruction Techniques * Raghu Machiraju, Edward Swan, and Roni Yagel "Spatial Domain Characterization and Control of Reconstruction Errors" * N. Max and K. Ohsaki "Rendering trees from precomputed Z-buffer views" ( each [ 20 min + 10 min discussion ]) 13:00-14:30 Lunch 14:30-16:00 Volume Rendering * Tsukasa Noma "Bridging Between Surface Rendering and Volume Rendering for Multi-Resolution Display" * J. Stam "Multiple scattering as a diffusion process" * Georgios Sakas, Marcus Grimm, Alexandros Savopoulos "Optimized Maximum Intensity Projection (MIP)" ( [ 15 + 20 + 15 min ] + 25 min discussion) 15:45-16:15 Coffee Break 16:15-17:30 Illumination * Stefan MŸller, Wolfram Kresse, Frank Schšffel "A Radiosity Approach For The Simulation Of Daylight" * P.M. Deville and J.C. Paul "Modeling the Spatial Energy Distribution of Complex Light Sources for Lighting Engineering" * Pierre Poulin and Alain Fournier "Painting Surface Characteristics" ( each [ 15 min + 10 min discussion ]) Tuesday, 13 June 9:00-10:30 Hierarchical Radiosity * Sumanta N. Pattanaik and Kadi Bouatouch "Linear Radiosity with Error Estimation" * Nicolas Holzschuch and Francois Sillion "Isolating Discretisation Error: an Accurate Refinement Strategy for Hierarchical Radiosity with Linear Functions" * F. Sillion, G. Drettakis, C. Soler "A clustering algorithm for radiance calculation in general environments" ( each [ 20 min ] + 30 min discussion) 10:30-11:00 Coffee Break 11:00-12:30 Monte Carlo Radiosity * L.Neumann, W. Purgathofer, R.F. Tobler, A. Neumann, P. Elias, M. Feda, X. Pueyo "The Stochastic Ray Method for Radiosity" * Peter Shirley, Bretton Wade, Philip Hubbard, David Zareski, Bruce Walter, Donald P. Greenberg "Global Illumination via Density Estimation" * Mateu Sbert, Frederic Perez, Xavier Pueyo "Global Monte Carlo. A Progressive Solution" ( each [ 20 min ] + 30 min discussion) 12:30-14:00 Lunch 14:00-15:30 User Interface Aspects * H. Rushmeier, G. Ward, C. Piatko, P. Sanders, B. Rust "Comparing real and synthetic images: Some ideas about metrics" * J. Nimeroff, J. Dorsey, H. Rushmeier "A framework for global illumination in animated environments" * G. Ward "Making global illumination user friendly" ( each [ 15 min ] + 45 min discussion) 15:30-16:00 Coffee Break 16:00-17:30 "Can realistic rendering be applied to real problems?" (invited panel discussion, G. Sakas, G. Ward, J.C. Paul) Wednesday, 14 June 9:00-10:00 Wavelet Radiosity * Philipp Slusallek, Michael Schršder, Marc Stamminger, Hans-Peter Seidel "Smart Links and Efficient Reconstruction for Wavelet Radiosity" * P. Schršder, W. Sweldens "Spherical wavelets: texture processing" * R. Gershbein "A study of integration methods for couplings of Galerkin radiosity systems" ( each [ 15 min ] + 15 min discussion) 10:00-10:30 Coffee Break 10:30-11:30 Nondiffuse Radiosity * Steven Collins "Reconstruction of Indirect Illumination from Area Luminaires" * Kurt Zimmerman and Peter Shirley "A Two-Pass Realistic Image Synthesis Method for Complex Scenes" * A. Fournier "Separating reflection functions for linear radiosity" ( each [ 15 min ] + 15 min discussion) 11:30-12:30 "Radiosity Notations" (panel discussion, Peter Shirley) 12:30-14:00 Lunch 14:00-14:45 Radiosity Performance Improvements * L. Neumann, R.F. Tobler, P. Elias "The Constant Radiosity Step" * Gladimir Baranoski, Randall Bramley, and Peter Shirley "Fast Radiosity Solutions for High Average Reflectance Environments" ( each [ 15 min ] + 15 min discussion) 14:45-15:15 Coffee Break 15:15-16:30 Importance Sampling * Ph. DutrŽ, Y.D.Willems "Potential-driven Monte Carlo Particle Tracing for Diffuse Environments with Adaptive Probability Density Functions" * Philippe Bekaert and Yves D. Willems "Importance-Driven Progressive Refinement Radiosity" * Henrik Wann Jensen "Importance Driven Path Tracing using the Photon Map" ( each [ 15 min ] + 30 min discussion) 16:30-17:30 Keynote Speaker Alain Fournier + discussion "From Local to Global Illumination and Back" From To: Peter Shirley From: Werner Purgathofer Subject: Re: READ THIS FIRST-- survey Message-Id: X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Date: Wed, 17 May 1995 13:59:02 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit A little late, but here they are, my answers: > >Question 1: > A radiosity method must be a finite element method (agree/disagree). DISAGREE >Question 2: > A radiosity method must estimates a radiometric quantity > for Lambertian surfaces only (agree/disagree). DISAGREE >Question 3: > A radiosity method may account for diffuse-specular-diffuse > transfer. AGREE >Question 4: > A radiosity method must compute a radiometric quantity > for (at least) every Lambertian surface in the > environment (agree/disagree). DISAGREE with the word "every", because I believe that importance sampling techniques, which leave away many invisible, irrelevant surfaces, are allowed. See you in Dublin, Werner From To: Peter Shirley From: Werner Purgathofer Subject: Re: READ THIS FIRST-- survey Cc: Hanrahan Message-Id: X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Date: Wed, 17 May 1995 16:45:57 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit >Perhaps instead of a proposal I could summarize current usage (I should >say "usages"-- that is why we need this). And I think a discussion >of the auditorium would be great. I will try to have the summary >done soon enough to send out by email to make sure people have time >to digest it before the workshop. I can bring copies to the workshop >as well. Very good! >Also, I think it would be productive to discuss BRDF terminology >as well (e.g. diffuse, directional-diffuse, lambertian, specular, etc). >ok? o.k.! Werner From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id OAA05784; Thu, 18 May 1995 14:34:54 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id NAA05869 for ; Thu, 18 May 1995 13:42:50 +0200 Received: from hwj.gk.dtu.dk (hwj.gk.dtu.dk [130.225.91.126]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id NAA25204 for ; Thu, 18 May 1995 13:42:49 +0200 Received: (from hwj@localhost) by hwj.gk.dtu.dk (8.6.11/8.6.9) id NAA13386 for globillum@imag.fr; Thu, 18 May 1995 13:44:10 +0100 Date: Thu, 18 May 1995 13:44:10 +0100 From: Henrik Wann Jensen Message-Id: <199505181244.NAA13386@hwj.gk.dtu.dk> To: globillum@imag.fr Subject: BSDF symbol? X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Dear Global Illuminators, The 1986 ANSI standard "Nomenclature and Definitions for Illuminating Engineering" containes symbol definitions for the BRDF (f_r) and the BTDF (f_t). However, it does not mention something like the BSDF (bidirectional scattering distribution function) f_s where f_s = f_r + f_t Is f_s a valid symbol or is p_bds or p_bd the preferred standard? - Henrik From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id WAA14890; Thu, 18 May 1995 22:20:17 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id WAA10354 for ; Thu, 18 May 1995 22:00:20 +0200 Received: from merckx.graphics.cornell.edu (MERCKX.GRAPHICS.CORNELL.EDU [128.84.247.147]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id WAA18888 for ; Thu, 18 May 1995 22:00:18 +0200 Received: by merckx.graphics.cornell.edu (5.65/DEC-Ultrix/4.3) id AA07713; Thu, 18 May 1995 16:00:33 -0400 Received: by gaia.graphics.cornell.edu (1.37.109.8/16.2) id AA01939; Thu, 18 May 1995 15:59:59 -0400 Date: Thu, 18 May 1995 15:59:59 -0400 (EDT) From: Dave Zareski Subject: Hierarchical or Monte Carlo Radiosity in Parallel? To: globillum@imag.fr Message-Id: Mime-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII; format=flowed X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Can anyone point me to a research paper or two which discusses parallelizing either Hierarchical or Monte Carlo radiosity? The only paper I've been able to find so far is Singh '93 (from Stanford). From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id CAA15409; Fri, 19 May 1995 02:51:57 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id CAA00623 for ; Fri, 19 May 1995 02:35:01 +0200 Received: from arl-img-4.compuserve.com (arl-img-4.compuserve.com [198.4.7.4]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id CAA23566 for ; Fri, 19 May 1995 02:34:59 +0200 Received: by arl-img-4.compuserve.com (8.6.10/5.950515) id UAA16483; Thu, 18 May 1995 20:34:27 -0400 Date: 18 May 95 20:31:58 EDT From: Ian Ashdown <72060.2420@CompuServe.COM> To: Global Illumination Subject: Hierarchical or Monte Carlo Radiosity in Parallel? Message-ID: <950519003158_72060.2420_FHG117-2@CompuServe.COM> X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Dave Zareski (zareski@graphics.cornell.edu) writes: > Can anyone point me to a research paper or two which discusses > parallelizing either Hierarchical or Monte Carlo radiosity? > > The only paper I've been able to find so far is Singh '93 (from > Stanford). The following references were extracted from RadBib95, a comprehensive radiosity bibliography that is available as /pub/doc/RadBib95.Z from hobbes.lbl.gov. There are numerous other references to radiosity on parallel processors that may or may not discuss hierarchical or Monte Carlo radiosity -- search for anything with the keyword "parallel." Also, the source code for a parallel hierarchical radiosity renderer (from Stanford) is available on-line. I found copies on ftp.ibp.fr and ftp.jussieu.fr under: /pub/parallel/environments/splash/codes/apps/radiosity Hope this helps! Ian Ashdown, President byHeart Software Limited 620 Ballantree Road West Vancouver, B.C. Canada V7S 1W3 ----------------------------------------------------------------------- %A Christian-A. Bohn %A Robert Garmann %T A Parallel Approach to Hierarchical Radiosity %J Proceedings of the Winter School of Computer Graphics and CAD Systems '95 %E V. Skala %I University of West Bohemia %C Plzen, Czech Republic %D February 1995 %P 26-35 %A Michael Brannon Carter %T Parallel Hierarchical Radiosity Rendering %R PhD thesis %I Iowa State University %D 1993 %A Martin Feda %A Werner Purgathofer %T Efficient Realistic Image Synthesis by Parallel Monte Carlo Radiosity on Transputers %J Transputer and Occam Engineering (Proceedings of the World Transputer Congress '94) %I IOS Press %V Series 41 %P 54-?? %C Cernobbio, Italy %D September 1994 %Z Monte Carlo radiosity, parallelism, transputers %A Shirley A. Hermitage %A Terrance L. Huntsberger %A Beverly A. Huntsberger %T Hypercube Algorithm for Radiosity in a Ray Tracing Environment %J Proceedings of the 5th Distributed Memory Computing Conference %I IEEE Society Press %D 1990 %P 206-211 %K parallelism %A Stefan Muller %T Radiosity und Ray Tracing: Integration und Parallelisierung %R Master's thesis (in German) %I Technische Tocheschule Darmstadt %D 1991 %K parallel algorithms %A Jaswinder P. Singh %A C. Holt %A T. Totsuka %A A. Gupta %A J. L. Hennessy %T Load Balancing and Data Locality in Hierarchical N-body Methods %R Technical Report CSL-TR-92-505 %I Computer Systems Laboratory, Stanford University %C Stanford, CA %D 1992 %K parallelism, hierarchical N-body %A Jaswinder P. Singh %T Parallel Hierarchical N-Body Methods and their Implications for Multiprocessors %R Technical Report CSL-TR-93-563 %I Computer Systems Laboratory, Stanford University %C Stanford, CA %D February 1993 %K parallel processors, hierarchical radiosity, N-body %A Jaswinder P. Singh %A Annop Gupta %A Marc Levoy %T Parallel Visualization Algorithms: Performance and Architectural Implications %J IEEE Computer %V 27 %N 7 %D July 1994 %P 45-55 %K hierarchical radiosity, multiprocessor, parallel processing, ray tracing From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id UAA01742; Mon, 22 May 1995 20:16:36 +0200 Received: from faure.Colorado.EDU (faure.Colorado.EDU [128.138.228.84]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id TAA28729 for ; Mon, 22 May 1995 19:35:18 +0200 Received: (from dilaura@localhost) by faure.Colorado.EDU (8.6.12/8.6.11/Unixops/Hesiod/(SDM)) id LAA03116 for globillum@imag.fr; Mon, 22 May 1995 11:37:57 -0600 Date: Mon, 22 May 1995 11:37:57 -0600 From: DILAURA DAVID L Message-Id: <199505221737.LAA03116@faure.Colorado.EDU> To: globillum@imag.fr Subject: non-diff contour integration X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Colleagues: A few months back I wrote that I had been working on developing the double contour integration formulation for non-diffuse radiative transfer between areas. That work has been completed and my paper has been accepted by the Illuminating Engineering Society. I am able to make preprints available. I have made a postscript file available. The ftp address is: civil.colrado.edu once you're connected, cd to pub/Illumination (Notice the upper case I). The file name is non_diff_contour_2.ps The results are interesting in that they generalize the work of Fock done for the case of diffuse emitters. Naturally, your comments would be helpful. David L. DiLaura Civil & Architectural Engineering College of Engineering University of Colorado at Boulder dilaura@bechtel.colorado.edu From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id EAA02609; Tue, 23 May 1995 04:30:03 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id EAA16778 for ; Tue, 23 May 1995 04:19:28 +0200 Received: from theory.lcs.mit.edu (theory.lcs.mit.edu [18.52.0.92]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id EAA03796 for ; Tue, 23 May 1995 04:19:26 +0200 Received: from jabiru.lcs.mit.edu by theory.lcs.mit.edu (5.65c/TOC-1.2S) id AA03062; Mon, 22 May 95 22:19:22 EDT From: Seth Teller Received: by jabiru.lcs.mit.edu (940816.SGI.8.6.9/TOC-1.2C) id WAA03915; Mon, 22 May 1995 22:21:13 -0400 Date: Mon, 22 May 1995 22:21:13 -0400 Message-Id: <9505222221.ZM3913@jabiru.lcs.mit.edu> Reply-To: seth@theory.lcs.mit.edu X-Mailer: Z-Mail (3.2.0 26oct94 MediaMail) To: globillum@imag.fr Subject: (Fwd) non-diff contour integration Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit or, for the impatient: ftp://civil.colorado.edu:/pub/Illumination/non_diff_contour_2.ps --- Forwarded mail from DILAURA DAVID L Date: Mon, 22 May 1995 11:37:57 -0600 From: DILAURA DAVID L Subject: non-diff contour integration ... ftp address is: civil.colrado.edu cd pub/Illumination [get] non_diff_contour_2.ps ---End of forwarded mail from DILAURA DAVID L From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id TAA04880; Tue, 23 May 1995 19:29:18 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id SAA17391 for ; Tue, 23 May 1995 18:34:18 +0200 Received: from bechtel.Colorado.EDU (bechtel.Colorado.EDU [128.138.238.217]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id SAA09070 for ; Tue, 23 May 1995 18:34:11 +0200 From: dilaura@bechtel.colorado.edu Received: from localhost (dilaura@localhost [127.0.0.1]) by bechtel.Colorado.EDU (8.6.12/8.6.11/Unixops/Hesiod/(SDM)) with SMTP id KAA26834 for ; Tue, 23 May 1995 10:34:05 -0600 Message-Id: <199505231634.KAA26834@bechtel.Colorado.EDU> X-Authentication-Warning: bechtel.Colorado.EDU: Host localhost didn't use HELO protocol To: globillum@imag.fr Subject: ftp address Date: Tue, 23 May 95 10:34:05 -0600 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Colleagues: It what can only be called an act of ingenious carelessness, I misspelled the ftp address I gave yesterday. It should read: civil.colorado.edu D.L. DiLaura From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id VAA05203; Tue, 23 May 1995 21:06:20 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id UAA20762 for ; Tue, 23 May 1995 20:34:10 +0200 Received: from lbl.gov (lbl.gov [128.3.254.23]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id UAA13292 for ; Tue, 23 May 1995 20:34:03 +0200 Received: from hobbes.lbl.gov by lbl.gov (4.1/1.39) id AA11045; Tue, 23 May 95 11:33:52 PDT Received: by hobbes.lbl.gov (3.2/SMI-3.2) id AA05605; Tue, 23 May 95 11:33:23 PDT Date: Tue, 23 May 95 11:33:23 PDT From: "Gregory J. Ward" Message-Id: <9505231833.AA05605@hobbes.lbl.gov> To: globillum@imag.fr Subject: Dave DiLaura's paper X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Just a warning to people who are grabbing David DiLaura's paper on non-diffuse contour integration. There seems to be an errant character at the beginning of the file that causes it not to be recognized as PostScript, at least on my printer. It printed out instead in uninterpreted form, about 200 pages before I stopped it. I suggest that everyone wait until Dr. DiLaura fixes the problem before printing it out and making the same mistake I did! -Greg From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id WAA05481; Tue, 23 May 1995 22:16:34 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id VAA21102 for ; Tue, 23 May 1995 21:01:59 +0200 Received: from explorer.dgp.toronto.edu (explorer.dgp.toronto.edu [128.100.1.129]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id VAA14068 for ; Tue, 23 May 1995 21:01:57 +0200 Received: by explorer.dgp.toronto.edu id <144031>; Tue, 23 May 1995 15:01:31 -0400 In-Reply-To: Gregory J. Ward's message as of May 23, 2:44pm X-Mailer: Mail User's Shell (7.2.3 5/22/91) From: Eugene Fiume To: "Gregory J. Ward" , globillum@imag.fr Subject: Re: Dave DiLaura's paper Message-Id: <95May23.150131edt.144031@explorer.dgp.toronto.edu> Date: Tue, 23 May 1995 15:01:27 -0400 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit I was pretty eager to see the paper, but I had the same problem as reported by Greg. There's a CNTL-D at the beginning and end of the paper that must be removed (actually, only the first). AFter that it prints fine. Cheers all, Eugene. From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id WAA05388; Tue, 23 May 1995 22:01:02 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id VAA21406 for ; Tue, 23 May 1995 21:18:23 +0200 Received: from mane.cgrg.ohio-state.edu (mane.cgrg.ohio-state.edu [128.146.18.78]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id VAA14681 for ; Tue, 23 May 1995 21:18:19 +0200 Received: from emily.cgrg.ohio-state.edu (spencer@cgrg.ohio-state.edu) by mane.cgrg.ohio-state.edu (8.6.12/941010.52) with ESMTP id PAA12618 for ; Tue, 23 May 1995 15:18:10 -0400 Received: (from spencer) by emily.cgrg.ohio-state.edu (8.6.12/941010) id PAA15934; Tue, 23 May 1995 15:18:10 -0400 Date: Tue, 23 May 1995 15:18:10 -0400 From: "Stephen N. Spencer" Message-Id: <199505231918.PAA15934@emily.cgrg.ohio-state.edu> To: globillum@imag.fr Subject: re: Dave DiLaura's paper In-Reply-To: <9505231833.AA05605@hobbes.lbl.gov> References: <9505231833.AA05605@hobbes.lbl.gov> X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Gregory J. Ward writes: > Just a warning to people who are grabbing David DiLaura's paper on > non-diffuse contour integration. There seems to be an errant character > at the beginning of the file that causes it not to be recognized as > PostScript, at least on my printer. It's a -D character -- 'xpsview' on my SGI had no problem skipping over it and correctly displaying the file, but I had the same problem when I went to print it -- I then edited the one character out of the file and reprinted successfully. Stephen From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id QAA10487; Wed, 24 May 1995 16:01:31 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id VAA21478 for ; Tue, 23 May 1995 21:22:06 +0200 Received: from hwj.gk.dtu.dk (hwj.gk.dtu.dk [130.225.91.126]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id VAA14781 for ; Tue, 23 May 1995 21:22:04 +0200 Received: (from hwj@localhost) by hwj.gk.dtu.dk (8.6.11/8.6.9) id VAA29410; Tue, 23 May 1995 21:23:25 +0100 Date: Tue, 23 May 1995 21:23:24 +0100 (GMT+0100) From: Henrik Wann Jensen To: "Gregory J. Ward" cc: globillum@imag.fr Subject: Re: Dave DiLaura's paper In-Reply-To: <9505231833.AA05605@hobbes.lbl.gov> Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII; format=flowed X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit This problem is caused by a CTRL-D code in the file. This often happens when dos/windows is used to create the postscript file. Just pipe the file through the following program. ------------------ CUT HERE ---------------------- /* psfix.c (remove ctrl-d codes from postscript-files) * Henrik Wann Jensen 070394 */ #include /*******/ main() { /*******/ int ch; while ( (ch = getchar()) != EOF ) { switch (ch) { case 04 : break; default : putchar(ch); } } } -------------------------------------------- Usage: psfix Just a warning to people who are grabbing David DiLaura's paper on > non-diffuse contour integration. There seems to be an errant character > at the beginning of the file that causes it not to be recognized as > PostScript, at least on my printer. It printed out instead in uninterpreted > form, about 200 pages before I stopped it. > > I suggest that everyone wait until Dr. DiLaura fixes the problem before > printing it out and making the same mistake I did! > > -Greg > From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id XAA05692; Tue, 23 May 1995 23:22:20 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id XAA23759 for ; Tue, 23 May 1995 23:10:23 +0200 Received: from victor.labri.u-bordeaux.fr (victor.labri.u-bordeaux.fr [147.210.8.168]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id XAA17533 for ; Tue, 23 May 1995 23:10:22 +0200 Received: from galadriel.labri (galadriel.labri.u-bordeaux.fr) by victor.labri.u-bordeaux.fr (4.1/SM-mailhost-BORDEAUX-1.0) id AA00371; Tue, 23 May 95 23:14:34 +0200 Date: Tue, 23 May 95 23:14:34 +0200 From: Christophe SCHLICK Message-Id: <9505232114.AA00371@victor.labri.u-bordeaux.fr> To: globillum@imag.fr Subject: Re: Dave DiLaura's paper X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Well, another DOS/UNIX translation caveat which arises quite often since there are more and more files put on Internet by PC users. Anyway, a good reflex is to test each unknown PostScript file as follows: cat -v file.ps | head -1 Note also that some PostScript files created under DOS or Windows contain an additional ^M (LineFeed) character at the end of each line. As far as I know, these extra characters do not disturb the printing process. CS From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id XAA05764; Tue, 23 May 1995 23:41:38 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id XAA23895 for ; Tue, 23 May 1995 23:23:34 +0200 Received: from faure.Colorado.EDU (faure.Colorado.EDU [128.138.228.84]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id XAA17769 for ; Tue, 23 May 1995 23:20:28 +0200 From: dilaura@faure.Colorado.EDU Received: from localhost (dilaura@localhost [127.0.0.1]) by faure.Colorado.EDU (8.6.12/8.6.11/Unixops/Hesiod/(SDM)) with SMTP id PAA05233 for ; Tue, 23 May 1995 15:23:44 -0600 Message-Id: <199505232123.PAA05233@faure.Colorado.EDU> X-Authentication-Warning: faure.Colorado.EDU: Host localhost didn't use HELO protocol To: globillum@imag.fr Subject: ps file Date: Tue, 23 May 95 15:23:41 -0600 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Colleagues: The offending character has been removed from the file. I`m certainly sorry for this inconvenience. (I just hope the damn paper is worth it!) David DiLaura From X-POP3-Rcpt: wp@stellaris Received: from radawana.cg.tuwien.ac.at by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) for id RAA10958; Wed, 24 May 1995 17:12:56 +0200 Received: (from pst@localhost) by radawana.cg.tuwien.ac.at (8.6.10/8.6.9) id RAA05915 for wp@stellaris.cg.tuwien.ac.at; Wed, 24 May 1995 17:09:23 +0200 From: Peter Stieglecker Message-Id: <199505241509.RAA05915@radawana.cg.tuwien.ac.at> Subject: Re: from Globillum: Re: Dave DiLaura's paper To: Werner Purgathofer Date: Wed, 24 May 1995 17:09:21 +0200 (MET DST) In-Reply-To: from "Werner Purgathofer" at May 24, 95 04:16:08 pm X-Mailer: ELM [version 2.4 PL23] Content-Type: text; charset=windows-1252 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 MIME-Version: 1.0 Content-transfer-encoding: 8bit > >------------------ CUT HERE ---------------------- > > > >/* psfix.c (remove ctrl-d codes from postscript-files) > > * Henrik Wann Jensen 070394 > >*/ > > > >#include > > > >/*******/ > >main() { > >/*******/ > >int ch; > > > >while ( (ch = getchar()) != EOF ) { > > switch (ch) { > > case 04 : break; > > default : putchar(ch); > > } > > } > >} pfui gack, das schreit ja fast nach einem flame war! :) sowas von ineffizient und unkommentiert... hardwired den char code eingetragen. ausserdem handelt es sich bei diesem proggie um eine abgespeckte version des unix 'tr' kommandos... also wirklich - leute kennst du *kopfschuettel* mfg pst :) From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id RAA04683; Mon, 12 Jun 1995 17:47:46 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id QAA00713 for ; Mon, 12 Jun 1995 16:30:46 +0200 Received: from eye.eye.com (eye.eye.com [149.54.1.2]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id QAA28304 for ; Mon, 12 Jun 1995 16:30:35 +0200 Received: from hemlock (hemlock.eye.com) by eye.eye.com with SMTP ($Revision: 1.36.108.11 $/16.2) id AA050817409; Mon, 12 Jun 1995 10:30:10 -0400 Received: by hemlock (1.37.109.8/15.6) id AA14120; Mon, 12 Jun 1995 10:30:04 -0400 Date: Mon, 12 Jun 1995 10:30:04 -0400 From: Eric Haines Message-Id: <9506121430.AA14120@hemlock> To: globillum@imag.fr Subject: total internal reflection X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Subject: Total internal reflection and ray trees I've run into an interesting implementation problem (again) which I've found annoying. Imagine you've got something with a big index of refraction, like a diamond, and you shoot a ray at it. A refraction ray is spawned and passes through the diamond. Due to total internal reflection (TIR) (i.e. the ray's past the critical angle) no refraction ray exits when this refracted ray (the one passing through the diamond) now intersects the surface, only a reflection ray is generated which bounces back through the diamond. The normal correction for TIR is to simply boost the reflection ray's contribution if the refraction ray is not generated. However, what happens if this reflection ray again hits, TIR occurs, and again only a reflection ray is spawned? Say this happens again and again until the maximum level of computation is reached and we call it quits. What happens at this point? That is, how do you shade this bottommost ray? Very little color has been picked up along the way, as it is expected that the reflection ray eventually hits something mostly diffuse and takes up that color. Really, this is just a special case of the general problem of what should happen when the maximum ray level is hit. Currently my kludgy fix is to say when the maximum level is hit we simply don't shoot the reflection ray but return the background color times the reflectivity and call it a day. I've also tried just taking the bottommost ray's surface and boost the diffuse component, but this is scary. I am interested to hear how other ray tracer coders have handled this problem. (Perhaps I can glue up the answers into an article for the Ray Tracing News). Eric Haines erich@eye.com 3D/Eye Inc. From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id PAA12407; Fri, 16 Jun 1995 15:08:51 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id NAA21009 for ; Fri, 16 Jun 1995 13:32:20 +0200 Received: from merckx.graphics.cornell.edu (MERCKX.GRAPHICS.CORNELL.EDU [128.84.247.147]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id NAA14411 for ; Fri, 16 Jun 1995 13:32:14 +0200 Received: by merckx.graphics.cornell.edu (5.65/DEC-Ultrix/4.3) id AA12477; Fri, 16 Jun 1995 07:32:27 -0400 Message-Id: <9506161132.AA12477@merckx.graphics.cornell.edu> Received: by barn.graphics.cornell.edu (1.37.109.8/16.2) id AA23824; Fri, 16 Jun 1995 07:31:47 -0400 From: Peter Shirley Subject: Re: total internal reflection To: Eric Haines Date: Fri, 16 Jun 95 7:31:47 EDT Cc: globillum@imag.fr In-Reply-To: <9506121430.AA14120@hemlock>; from "Eric Haines" at Jun 12, 95 10:30 am Mailer: Elm [revision: 70.85] X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit I find that it is worth it to let the ray go for at least dozens of bounces before terminating it-- especially for glass panes (like tabletops). This way the sides of panes can take on that colored "look" that makes a big difference in realism. But what happens when it goes further (as Eric asks?). I make it black-- that HAS to be bad. Should we let these rays go for hundreds of bounces? Maybe... From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id UAA01194; Fri, 16 Jun 1995 20:29:01 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id PAA27026 for ; Fri, 16 Jun 1995 15:06:32 +0200 Received: from idefix.cs.kuleuven.ac.be (idefix.cs.kuleuven.ac.be [134.58.40.4]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id PAA19153 for ; Fri, 16 Jun 1995 15:06:27 +0200 Received: from krasser.cs.kuleuven.ac.be (philipd@krasser.cs.kuleuven.ac.be [134.58.45.36]) by idefix.cs.kuleuven.ac.be (8.6.12/8.6.12) with ESMTP id PAA29455 for ; Fri, 16 Jun 1995 15:06:23 +0200 Received: (from philipd@localhost) by krasser.cs.kuleuven.ac.be (8.6.12/8.6.12) id PAA03749 for globillum@imag.fr; Fri, 16 Jun 1995 15:06:20 +0200 Date: Fri, 16 Jun 1995 15:06:20 +0200 From: Phil Dutre Message-Id: <199506161306.PAA03749@krasser.cs.kuleuven.ac.be> To: globillum@imag.fr Subject: Re: total internal reflection X-Sun-Charset: US-ASCII X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit It's a known problem in the diamond-cutting world, that a bad cut diamond can cause black spots to be visible, due to infinite total internal reflection. So, it's hard to be sure whether a ray will leave a diamond again. Theoretically, this could happen after a few thousand internal bounces. This is also a problem when you want to render an endoscope, used by doctors to look at your intestines. If you model a glass fiber endoscope, and put the eyepoint of the ray tracer in front of it, you may want to go for a large number of bounces to see the things at the other side. So, basically, there is no way to do it correct, unless you let ray bounce an infinite number of times. Philip +---------------------------------------------------------------------------+ | Philip.Dutre@cs.kuleuven.ac.be Department of Computer Science | | http://www.cs.kuleuven.ac.be/~philipd/ Computer Graphics Research Group | | Phone: ++32 16 327094 Katholieke Universiteit Leuven | | Fax: ++32 16 327996 Celestijnenlaan 200A | | Office: C200, K.00.10 B-3001 Heverlee, BELGIUM | +---------------------------------------------------------------------------+ From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id CAA01872; Sat, 17 Jun 1995 02:44:46 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id CAA18355 for ; Sat, 17 Jun 1995 02:32:07 +0200 Received: from merckx.graphics.cornell.edu (MERCKX.GRAPHICS.CORNELL.EDU [128.84.247.147]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id CAA13154; Sat, 17 Jun 1995 02:32:04 +0200 Received: by merckx.graphics.cornell.edu (5.65/DEC-Ultrix/4.3) id AA11029; Fri, 16 Jun 1995 20:32:36 -0400 Message-Id: <9506170032.AA11029@merckx.graphics.cornell.edu> Received: by barn.graphics.cornell.edu (1.37.109.8/16.2) id AA04137; Fri, 16 Jun 1995 20:31:54 -0400 From: Peter Shirley Subject: Re: total internal reflection To: Eugene Fiume Eugene Fiume Date: Fri, 16 Jun 95 20:31:54 EDT Cc: shirley@graphics.cornell.edu, erich@eye.com, globillum@imag.fr In-Reply-To: <199506162310.BAA29843@safran-28>; from "Eugene Fiume" at Jun 17, 95 1:10 am Mailer: Elm [revision: 70.85] X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit > > of this phenomenon. But let's go even further back and recall the > immortal words in Turner Whitted's paper: > > For the case of surfaces aligned in such a way that a branch of > a tree [of ray tracings] has infinite depth, the branch is > truncated at the point where it exceeds the allotted storage. > > I always have loved the chutzpah of that line. > I recently re-read the Whitted paper and was shocked to see that it suggested randomly perturbing reflection vectors on glossy surfaces. Cook indeed credited him with the idea in the 84 Siggraph paper. That paper was full of gems. P From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id BAA01713; Sat, 17 Jun 1995 01:23:56 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id BAA17577 for ; Sat, 17 Jun 1995 01:10:57 +0200 Received: from safran-28 (safran.imag.fr [129.88.29.1]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id BAA11811; Sat, 17 Jun 1995 01:10:56 +0200 Received: from localhost (elf@localhost) by safran-28 (8.6.4/8.6.4) id BAA29843; Sat, 17 Jun 1995 01:10:55 +0200 Message-Id: <199506162310.BAA29843@safran-28> From: Eugene Fiume Date: Sat, 17 Jun 1995 01:10:55 -0600 In-Reply-To: Peter Shirley's message as of Jun 16, 2:55pm X-Mailer: Mail User's Shell (7.2.5 10/14/92) To: Peter Shirley , Eric Haines Subject: Re: total internal reflection Cc: globillum@imag.fr X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Peter remarks } But what happens when it goes further (as Eric asks?). I make } it black-- that HAS to be bad. Should we let these rays go for } hundreds of bounces? Maybe... Back (way back!) when I was interested in proving formal lower bounds for ray tracing I recall sketching something out that took advantage of this phenomenon. But let's go even further back and recall the immortal words in Turner Whitted's paper: For the case of surfaces aligned in such a way that a branch of a tree [of ray tracings] has infinite depth, the branch is truncated at the point where it exceeds the allotted storage. I always have loved the chutzpah of that line. [If Alain Fournier can quote Joyce, I'm allowed to quote Whitted, especially on Bloomsday.] Eugene. From X-POP3-Rcpt: wp@stellaris Received: from eigpc5.tuwien.ac.at by stellaris.cg.tuwien.ac.at via SMTP (940816.SGI.8.6.9/910805.SGI) for id MAA20513; Tue, 27 Jun 1995 12:56:52 +0200 Message-Id: Date: Tue, 27 Jun 95 12:26:57 0200 Sender: manfred@ieee.org From: Manfred Kopp Organization: Institute of Computer Graphics, TU-Vienna X-Mailer: Mozilla 1.1N (X11; I; Linux 1.1.95 i486) MIME-Version: 1.0 To: wp Subject: E-Mail addresses of Globillumers X-URL: ftp://safran.imag.fr/pub/sillion/globillum/glob.elmaliases Content-Transfer-Encoding: 8bit Content-Type: text/plain; charset=us-ascii; format=flowed X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 > imartin = Ignacio Martin Campos = imartin@turing.upc.es > # Nelson Max, Lawrence Livermore Lab > max = Nelson Max = max2@llnl.gov > # Christian Metge; Institut de Recherche en Informatique de Toulouse; > # Universite Paul Sabatier; 31062 Toulouse; France > # interests: parallel discrete radiosity and ray tracing algorithms > # (Transputers, workstation networks) > metge = Christian Metge = metge@irit.fr > # Don Mitchell, Microsoft > dmitchell = Don Mitchell = donm@microsoft.com > # William Parsons Newhall, Jr., The American University > newhall = William Parsons Newhall = newhall@auvm.american.edu > # Andy Newton; Remote Sensing Research, University College London > anewton = Andy Newton = anewton@ps.ucl.ac.uk > # Fabrice Neyret; I.N.R.I.A. Rocquencourt, Projet Syntim > neyret = Fabrice Neyret = Fabrice.Neyret@inria.fr > # Jeffry Nimeroff; Penn University > nimeroff = Jeffry Nimeroff = jnimerof@graphics.cis.upenn.edu > # Tomoyuki Nishita; Electric Machinery Lab, Hiroshima U. > nishita = Tomoyuki Nishita = nis@eml.hiroshima-u.ac.jp > # Christopher Patmore; Programming Research Group; Oxford U. > # interests: skylight radiosity > patmore = Christopher Patmore = cjp@prg.oxford.ac.uk > # Sumant Narayan Pattanaik; IRISA; Rennes; France > pattanaik = Sumant Narayan Pattanaik = sumant.pattanaik@irisa.fr > # Mathias Paulin; Institut de Recherche en Informatique de Toulouse; > # Universite Paul Sabatier; 31062 Toulouse; France > # interests: parallel radiosity and ray tracing algorithms (Transputers, PVM) > # shadow accuracy, transfer simulations in dense foliage > paulin = Mathias Paulin = paulin@irit.fr > # Barbara Pela, Joint Research Centre, Commission of the European Communities, > # Ispra, Italy > pela = Barbara Pela = barbara.pela@cen.jrc.it > # Frederic Perez Cazorla; University of Girona > perez = Frederic Perez Cazorla = frederic@ima.udg.es > # Matt Pharr > pharr = Matt Pharr = mmp@lux.Stanford.EDU > # Brad Pillow > pillow = Brad Pillow = bpillow@pillowsoft.com > # Pierre Poulin; Dept. IRO, Universite de Montreal, > # C.P. 6128, succ. Centre-Ville, Montreal, Quebec, Canada H3C 3J7 > # interests: illumination, rendering, realism > poulin = Pierre Poulin = poulin@iro.umontreal.ca > # Claude Puech; iMAGIS/IMAG, BP 53, F-38041 Grenoble Cedex 9. France > puech = Claude Puech = Claude.Puech@imag.fr > # Xavier Pueyo; Dept. Llenguatges i Sistemes Informatics; > # Universitat Politecnica de Catalunya; Av. Diagonal, 647 planta 8; > # 08028-Barcelona; Spain; > # interests: diffuse environments > pueyo = Xavier Pueyo = xavier@ima.udg.es > # Werner Purgathofer; Institute of Computer Graphics; Techn. Univ. Vienna; > # Karlsplatz 13 / 186; A-1040 Wien / Austria > # interests: radiosity, ray tracing, color, virtual reality, > # dithering and quantization > purgathofer = Werner Purgathofer = wp@cg.tuwien.ac.at > # Jordi Regincos > regincos = Jordi Regincos = jordir@upisun4.uab.es > # Panu Rekola; Computer Science Dept, Helsinki U. of Tech.; Finland > rekola = Panu Rekola = pre@cs.hut.fi > # Barry Carlton Ruff > ruff = Barry Carlton Ruff = ruffb@rpi.edu > # Holly Rushmeier, Computing and Applied Math Lab; > # National Institute for Standards and Technology; Gaithersburg, Maryland > rushmeier = Holly Rushmeier = holly@cam.nist.gov > # David Salesin; U. of Washington > salesin = David Salesin = salesin@cs.washington.edu > # Stefan Schaefer; University of Bonn > schaefer = Stefan Schaefer = schaefer@graphics.cs.uni-bonn.de > # Christophe Schlick; LaBRI; U. of Bordeaux; 351 Cours de la Liberation > # 33400 Talence; France > # interests: ray tracing, radiosity, antialiasing, general reflectance functions > schlick = Christophe Schlick = schlick@labri.u-bordeaux.fr > # Michael Schroeder; University of Erlangen > # Hierarchical Radiosity, Monte-Carlo methods > mschroeder = Michael Schroeder = Michael.Schroeder@informatik.uni-erlangen.de > # Peter Schroeder > pschroeder = Peter Schroeder = ps@math.scarolina.edu > # Roberto Scopigno; CNUCE; Consiglio Nazionale delle Richerche; > # Via S.Maria, 36; 56100 Pisa; Italy > # interests: volume rendering, user interfaces, parallel processing, geography > scopigno = Roberto Scopigno = R.Scopigno@cnuce.cnr.it > # Francisco Seron; Dpto. Ingenieria Electrica e Informatica; > # Centro Politecnico Superior de Ingenieros; Universidad de Zaragoza; > # C/ Maria Luna s/n; E-50015 Zaragoza; Spain > seron = Francisco Seron = pseron@mcps.unizar.es > # Mikio Shinya, pencil tracing > shinya = Mikio Shinya = shinya@nttarm.ntt.jp > # Pete Shirley, Indiana U., on leave at Cornell as of 7/94 > shirley = Pete Shirley = shirley@graphics.cornell.edu > # Global Illumination group at iMAGIS/IMAG > gimagis = Global Illumination group at iMAGIS/IMAG = gimagis@safran.imag.fr > # Reetinder Sidhu; Supercomp Edu & Research Centre > # Indian Institute of Science, Banglore 560012, INDIA > sidhu = Reetinder Sidhu = sidhu@cadl.iisc.ernet.in > # Francois Sillion; IMAG; Grenoble; France > sillion = Francois Sillion = Francois.Sillion@imag.fr > # Simon Sleight; Postgraduate student, Bristol Univerity > # currently working with 'Radiance', aiming to produce photo realistic > # graphics displaying shop windows. > sleight = Simon Sleight = sleight@cs.bris.ac.uk > # Philipp Slusallek; Universitaet Erlangen; > # IMMD IX - Graphische Datenverarbeitung; Am Weichselgarten 9; > # W-8520 Erlangen, Germany > # interests: CAD, surfaces, doing PhD on physical basis of glob. illum. > slusallek = Philipp Slusallek = slusallek@informatik.uni-erlangen.de > # Rick Speer > speer = Rick Speer = speer@crl.com > # Greg Spencer > gspencer = Greg Spencer = greg_spencer@Taligent.com > # Stephen Spencer > spencer = Stephen Spencer = spencer@cgrg.ohio-state.edu > # Marc Stamminger; University of Erlangen > # Wavelet Radiosity/Radiance, > # in future: Clustering, Parallelization of Radiosity/Radiance algorithms > stamminger = Marc Stamminger = Marc.Stamminger@informatik.uni-erlangen.de > # Jorge Stolfi > stolfi = Jorge Stolfi = stolfi@dcc.unicamp.br > # Eric Stollnitz > stollnitz = Eric Stollnitz = stoll@amath.washington.edu > # Wolfgang Stuerzlinger, Department of Graphics and Parallel Processing, > # Johannes Kepler University, Linz, Austria > stuerzlinger = Wolfgang Stuerzlinger = wrzl@gup.uni-linz.ac.at > # K. R. Subramanian; AT&T Bell Labs; Murray Hill, NJ > ksubramanian = K. R. Subramanian = krs@allegra.att.com > # Kelvin Sung; Dept. of Information Systems and Computer Science; > # National University of Singapore; Kent Ridge, Singapore 0511 > # Republic of Singapore > # interests: fast ray tracing, modular global illumination software > sung = Kelvin Sung = ksung@iscs.nus.sg > # Filippo Tampieri; Lightscape Technologies, Inc; San Jose, CA > tampieri = Filippo Tampieri = fxt@lightscape.com > # Seth Teller; MIT > teller = Seth Teller = seth@lcs.mit.edu > # Pierre Tellier > # LSIIT (Laboratoire des Sciences de l'Image, d'Informatique et de > # Teledetection); Departement d'Informatique de l'Universite Louis Pasteur; > # 7, rue R. Descartes; 67084 Strasbourg; France > tellier = Pierre Tellier = tellier@dpt-info.u-strasbg.fr > # Kim Beng Teo; Berkeley; interests: Radiosity and Modelling > kbteo = Kim Beng Teo = kbteo@cs.berkeley.edu > # Chris Thornborrow; Edinburgh Parallel Computing Centre, > # moving to Silicon Graphics (Manchester) > # interests: Photon tracing, particularly solving the noise problem. > thornborrow = Chris Thornborrow = ct@epcc.ed.ac.uk > # J. Eric Townsend; General Magic > # interests: massively parallel based visualization codes, mostly ray tracing > townsend = J. Eric Townsend = jet@genmagic.com > # Roy Troutman, Lawrence Livermore Lab > troutman = Roy Troutman = roy@ninja.nersc.gov > # Jack Tumblin, Georgia Tech > tumblin = Jack Tumblin = ccsupjt@cc.gatech.edu > # Doug Turner, Apple > turner = Doug Turner = turner@apple.com > # Sam Uselton; CSC, NASA Ames, Mountain View, CA > uselton = Sam Uselton = uselton@nas.nasa.gov > # Robert van Liere; Department of Interactive Systems; > # Center for Mathematics and Computer Science (CWI); > # Kruislaan 413, 1098 SJ Amsterdam, The Netherlands > # interests: generalizing radiosity method, parallel methods for radiosity > vanliere = Robert van Liere = robertl@cwi.nl > # Cornelius Skip Van Wyk, Jr; Carnegie Mellon U; Dept of Architecture > vanwyk = Cornelius Skip Van Wyk = vanwyk@cad.cs.cmu.edu > # Eric Veach; Stanford U. > # interests: hierarchical global illumination, clustering objects, > # global illumination methods for "black box" scene representations > veach = Eric Veach = ericv@cs.stanford.edu > # Josep Vilaplana; Universitat Politecnica de Catalunya; > # Departament de Llenguatges i Sistemes Informatics; > # Av. Diagonal 647 planta 8; 08028 Barcelona; Spain > # interests: hardware and parallel algs for speeding radiosity & ray tracing > vilaplana = Josep Vilaplana = vilaplana@lsi.upc.es > # John Wallace, 3D/Eye > jwallace = John Wallace = johnw@eye.com > # Changyaw Wang; U. of Indiana > # interests: rendering and modeling of complex outdoor environments > cwang = Changyaw Wang = wangc@iuvax.cs.indiana.edu > # Greg Ward; Lighting Systems Research Group; Lawrence Berkeley Lab; California > ward = Greg Ward = gjward@lbl.gov > # Daniel E. Wexler; R&D Staff; Pacific Data Images > wexler2 = Daniel E. Wexler = wex@pdi.com > # Chuck Wiley; Applied Research Laboritories; U. of Texas at Austin > #interests: scientific vis., adaptive rendering, digital terrain, > cwiley = Chuck Wiley = cawiley@arlut.utexas.edu > # Andrew J. Willmott; CMU > willmott = Andrew J. Willmott = Andrew.Willmott@cs.cmu.edu > # Jason R. Wilson; U. North Carolina > # Interests: Radiosity for large models and curved surfaces. > wilson = Jason R. Wilson = wilson@cs.unc.edu > # Jim Winget, Silicon Graphics > winget = Jim Winget = jmw@sgi.com > # Steve Worley > worley = Steve Worley = spworley@netcom.com > # Adam Worrall, University of Bristol Graphics Group > # Computer Science Department, The University, Bristol, UK > worrall = Adam Worrall = Adam.Worrall@bristol.ac.uk > # Chien Kok Yang; UC Berkeley > # My research interests are realistic image synthesis and modeling > yang = Chien Kok Yang = ckyang@bach.eecs.berkeley.edu > # Ning Zhang > # interests: radiosity, ray tracing, physically-based illumination models > zhang = Ning Zhang = zhang@vti.com > # Kurt Zimmerman > zimmerman = Kurt Zimmerman = kuzimmer@cs.indiana.edu > # Andrew Zisserman; Robotics Research Group; Oxford University; UK > # interests: computer vision, radiosity > zisserman = Andrew Zisserman = az@robots.oxford.ac.uk > # Zumtobel Licht GmbH; Schweizerstr. 30; A-6850 Dornbirn; Austria > # interests: lighting design visualization, radiosity > # (an alias for global illumination folks at the Zumtobel company) > zumtobel = Zumtobel Licht GmbH = glbi@cophos.co.at > > ### Explicit globillum alias (use of globillum strongly advised instead) > > globillum_explicit = globillum explicit list = > mallison, almagro, amanatides, arvo, ashdown, bastos, baum, bekaert, > besuievsky, borel, bouatouch, buckalew, cabrero, campbell, carlton, > casasayas, achalmers, chelle, chen, nchristensen, pchristensen, christou, > cignoni, mcohen, compagnon, costa, cornell_students, curless, dadalto, wkdai, > jdave, delft, desousa, dilaura, donaldson, dorsey, drettakis, dutre, elias, > ferwerda, fiume, forsyth, fournier, fussell, gatenby, dgeorge, gibson, > gifford, glassner, goel, grabenstein, grant, greenberg, guenther, guibas, > haines, hanrahan, heal, heckbert, hedley, ivanov, jensen, jessel, gjones, > kalinowski, kaneda, karner, keller, kesteloot, kirk, kolb, kopp, kouhia, > kumar, lafortune, lalonde, languenou, levoy, blewis, plewis, lightwork, > lischinski, loofbour, maierhofer, manocha, marini, imartin, max, metge, > dmitchell, newhall, anewton, neyret, nimeroff, nishita, patmore, pattanaik, > paulin, pela, perez, pharr, pillow, poulin, puech, pueyo, purgathofer, > regincos, rekola, ruff, rushmeier, salesin, schaefer, schlick, mschroeder, > pschroeder, scopigno, seron, shinya, shirley, gimagis, sidhu, sillion, > sleight, slusallek, speer, gspencer, spencer, stamminger, stolfi, stollnitz, > stuerzlinger, ksubramanian, sung, tampieri, teller, tellier, kbteo, > thornborrow, townsend, troutman, tumblin, turner, uselton, vanliere, vanwyk, > veach, vilaplana, jwallace, cwang, ward, wexler2, cwiley, willmott, wilson, > winget, worley, worrall, yang, zhang, zimmerman, zisserman, zumtobel > > ### Current number of globillum members: 162 > ### END OF GLOBAL ILLUMINATION MAILING LIST -- -manfred ---------------------------------------------------------------------------- Manfred causes nothing but trouble and desire. "Simple Mic" ---------------------------------------------------------------------------- Manfred Kopp | Institute of Computer Graphics | email: m.kopp@ieee.org Technical University of Vienna | kopp@stellaris.cg.tuwien.ac.at Karlsplatz 13-186/2 | phone: +43 (1) 588 01 / 41 02 A-1040 Wien, Austria, Europe | WWW: http://www.cg.tuwien.ac.at/~kopp/ ---------------------------------------------------------------------------- From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id SAA29554; Tue, 27 Jun 1995 18:59:36 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.32.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id SAA26298 for ; Tue, 27 Jun 1995 18:37:30 +0200 Received: from merckx.graphics.cornell.edu (MERCKX.GRAPHICS.CORNELL.EDU [128.84.247.147]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id SAA24533 for ; Tue, 27 Jun 1995 18:37:24 +0200 Received: by merckx.graphics.cornell.edu (5.65/DEC-Ultrix/4.3) id AA15729; Tue, 27 Jun 1995 12:38:00 -0400 Received: from [132.236.155.40] (CU-DIALUP-0726.CIT.CORNELL.EDU) by MAX-F.GRAPHICS.CORNELL.EDU with SMTP (1.37.109.16/16.2) id AA083191076; Tue, 27 Jun 1995 12:37:56 -0400 X-Sender: bwade@max.graphics.cornell.edu Message-Id: Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed Date: Tue, 27 Jun 1995 12:37:20 -0400 To: globillum@imag.fr From: Bretton Wade Subject: finite element meshing technology X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit http://www-users.informatik.rwth-aachen.de/~roberts/meshgeneration.html It seems to me that a web page like this one could be very useful to us, especially given the recent interests in decimation and meshing of functions. If you know of any other online resources, please send them to me. I'll either forward them to the owner of the page above, or organize them myself. Thanks, Bretton -- Bretton Wade (bwade@graphics.cornell.edu) http://www.graphics.cornell.edu/~bwade/ From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id TAA12358; Wed, 5 Jul 1995 19:30:58 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id SAA02270 for ; Wed, 5 Jul 1995 18:00:07 +0200 Received: from haven.uniserve.com (haven.uniserve.com [198.53.215.121]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id RAA23074 for ; Wed, 5 Jul 1995 17:59:55 +0200 Received: from pm2-1.TVS.NET ([204.191.197.11]) by haven.uniserve.com with SMTP id <30816>; Wed, 5 Jul 1995 08:59:59 +0100 X-Sender: iashdown@ledalite.com (Unverified) X-Mailer: Windows Eudora Version 2.0.3 Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed To: globillum@imag.fr From: Ian Ashdown Subject: Mesh generation Message-Id: <95Jul5.085959+0100_pdt.30816+3472@haven.uniserve.com> Date: Wed, 5 Jul 1995 08:59:58 +0100 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Radiosity, anyone? If you are looking for a 2D mesh generator that offers constrained Delaunay triangulation with user-specified constraints on the minimum angle and maximum area of the triangles, check out: http://www.cs.cmu.edu/~quake/triangle.html Jonathan Shewchuk has made available the documentation and full C source code for his mesh generator, Triangle. The code is extremely well-written and fully commented. It's an excellent piece of work. Ian Ashdown, P. Eng. READ THE BOOK! Research & Development Manager Radiosity: A Programmer's Perspective Ledalite Architectural Products Inc. by Ian Ashdown 9087A - 198th Street John Wiley & Sons, 1994 Langley, British Columbia Canada V3A 4P8 (Sneaky Internet Advertising) From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id BAA10740; Fri, 7 Jul 1995 01:32:48 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id BAA01238 for ; Fri, 7 Jul 1995 01:19:25 +0200 Received: from haven.uniserve.com (haven.uniserve.com [198.53.215.121]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id BAA12995 for ; Fri, 7 Jul 1995 01:19:15 +0200 Received: from pm2-29.TVS.NET ([204.191.197.39]) by haven.uniserve.com with SMTP id <30747>; Thu, 6 Jul 1995 16:20:34 +0100 X-Sender: iashdown@ledalite.com (Unverified) X-Mailer: Windows Eudora Version 2.0.3 Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed To: globillum@imag.fr From: Ian Ashdown Subject: Non-Diffuse Radiative Transfer Message-Id: <95Jul6.162034+0100_pdt.30747+1278@haven.uniserve.com> Date: Thu, 6 Jul 1995 16:20:34 +0100 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Several weeks ago, David DiLaura posted a message saying that he had written a paper called "Non-Diffuse Radiative Transfer 2: Planar Area Sources and Receivers." He indicated where a Postscript copy could be downloaded from for review. If you downloaded and read (and understood!) the paper, the Illuminating Engineering Society of North America has a favor to ask of you. David will be presenting his paper at the 1995 IESNA Annual Conference in New York at the end of this month. Following each presentation is an audience discussion in which the paper is dissected and commented on. In the case of David's paper, there may not be anyone at the conference who will be qualified to discuss his work. If so, this will be unfortunate, because (a) the discussions become part of a presented paper when (and if) it is published in the Journal of the IES; and (b) I feel that this is an important piece of work. If anyone has any comments on the paper, ranging from errors in the text or mathematics to general comments on the usefulness of this approach in global illumination applications, the IESNA would very much like to hear from you. Any comments will be presented to the audience, and so they should be 400 words or less in length. Submissions that David will need to respond to are required by July 12th; otherwise, they will be accepted if received before July 25th. If you can e-mail or fax your comments to me at: e-mail: iashdown@ledalite.com Fax: (604) 888-0566 (Attn: Ian Ashdown) I will ensure that they are presented at the conference (with full credit to the authors, of course). On behalf of the IESNA, thanks! Ian Ashdown, P. Eng. READ THE BOOK! Research & Development Manager Radiosity: A Programmer's Perspective Ledalite Architectural Products Inc. by Ian Ashdown 9087A - 198th Street New York, NY: John Wiley & Sons, 1994 Langley, British Columbia Canada V3A 4P8 (Sneaky Internet Advertising) From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id CAA10812; Fri, 7 Jul 1995 02:24:15 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id CAA02070 for ; Fri, 7 Jul 1995 02:11:40 +0200 Received: from haven.uniserve.com (haven.uniserve.com [198.53.215.121]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id CAA13567 for ; Fri, 7 Jul 1995 02:11:14 +0200 Received: from pm2-29.TVS.NET ([204.191.197.39]) by haven.uniserve.com with SMTP id <30751>; Thu, 6 Jul 1995 17:12:21 +0100 X-Sender: iashdown@ledalite.com X-Mailer: Windows Eudora Version 2.0.3 Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed To: globillum@imag.fr From: Ian Ashdown Subject: Shortest radiosity code? Message-Id: <95Jul6.171221+0100_pdt.30751+1317@haven.uniserve.com> Date: Thu, 6 Jul 1995 17:12:19 +0100 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit I couldn't resist this one. Chris Borel from the Los Alamos National Laboratory (cborel@lanl.gov) asked me: >In 1993 or so I spent a day to rewrite [my] radiosity code in IDL making use >of IDL's powerful 3-D manipulation and Z-buffer capabilities and came up >with a code of 153 lines doing the same task as the viewfactor FORTRAN code >at about the same speed! The code is not quite finished yet but I wonder >if there is any radiosity code that is shorter than that. I know a ray tracer can be written in one line of C source code, but a radiosity renderer!?! Ian Ashdown, P. Eng. READ THE BOOK! Research & Development Manager Radiosity: A Programmer's Perspective Ledalite Architectural Products Inc. by Ian Ashdown 9087A - 198th Street New York, NY: John Wiley & Sons, 1994 Langley, British Columbia Canada V3A 4P8 (Sneaky Internet Advertising) From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id DAA10908; Fri, 7 Jul 1995 03:36:22 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id DAA02806 for ; Fri, 7 Jul 1995 03:27:45 +0200 Received: from fred.interval.com (fred.interval.com [192.203.6.36]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id DAA14364 for ; Fri, 7 Jul 1995 03:27:42 +0200 Received: from interval.interval.com (interval.interval.com [199.170.106.10]) by fred.interval.com with ESMTP id SAA19207 for ; Thu, 6 Jul 1995 18:27:40 -0700 Received: by interval.interval.com id SAA11674; Thu, 6 Jul 1995 18:27:40 -0700 Date: Thu, 6 Jul 1995 18:27:40 -0700 From: Peter Schroeder Message-Id: <199507070127.SAA11674@interval.interval.com> To: globillum@imag.fr In-reply-to: <95Jul6.171221+0100_pdt.30751+1317@haven.uniserve.com> (iashdown@ledalite.com) Subject: Re: Shortest radiosity code? X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit From: iashdown@ledalite.com (Ian Ashdown) Date: Thu, 6 Jul 1995 17:12:19 +0100 I know a ray tracer can be written in one line of C source code, but a radiosity renderer!?! Don't be shy folks, make it run in postscript on that idle printer down the hall! Peter From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id MAA13908; Fri, 7 Jul 1995 12:37:01 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id MAA19832 for ; Fri, 7 Jul 1995 12:05:00 +0200 Received: from safran-28 (safran.imag.fr [129.88.29.1]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id MAA28143; Fri, 7 Jul 1995 12:04:59 +0200 Received: (fournier@localhost) by safran-28 (940816.SGI.8.6.9/8.6.4) id MAA10483; Fri, 7 Jul 1995 12:04:58 +0200 Message-Id: <199507071004.MAA10483@safran-28> From: Alain Fournier Date: Fri, 7 Jul 1995 12:04:57 -0600 In-Reply-To: Peter Schroeder "Re: Shortest radiosity code?" (Jul 6, 6:36pm) X-Mailer: Mail User's Shell (7.2.5 10/14/92) To: Peter Schroeder , globillum@imag.fr Subject: Re: Shortest radiosity code? X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Considering that there is an inverse relationship between length of code and running time, I am afraid that "idle printer down the hall" won't be idle any more in this millenium. Remind me not to send any printing job to Peter's place (by the way, can you "nice" a postscript job?). From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id RAA00038; Wed, 12 Jul 1995 17:28:53 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id QAA25588 for ; Wed, 12 Jul 1995 16:45:06 +0200 Received: from profs0.prosolvia.se ([193.13.245.193]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id QAA29809 for ; Wed, 12 Jul 1995 16:44:55 +0200 Received: (from tompa@localhost) by profs0.prosolvia.se (940816.SGI.8.6.9/8.6.11) id QAA01324; Wed, 12 Jul 1995 16:44:22 +0200 Date: Wed, 12 Jul 1995 16:44:22 +0200 From: Tomas Moller Message-Id: <199507121444.QAA01324@profs0.prosolvia.se> Apparently-To: globillum@imag.fr Apparently-To: Radiosity@prosolvia.se Apparently-To: sampling@prosolvia.se Apparently-To: &@prosolvia.se Apparently-To: reconstruction@prosolvia.se X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Hello GlobIlluminers! I have just joined this mailing list (thanks Francois Sillion) and yesterday I read all previous discussions here. Interesting! I am working on a radiosityprogram for use within VR-applications. I hope to finish my master thesis at the end of this summer. The surfaces that are imported to my program are all NURBS. I have found three references for curved surfaces within radiosity: %T A Progressive Radiosity Algorithm for Scenes Containing Curved Surfaces %J Computer Graphics Forum (Eurographics '93) %D Sept. 1993 %T A New Radiosity Apporach Using Area Sampling for Parametric Patches %J Computer Graphics Forum (Eurographics '93) %D Sept. 1993 %T A Two-Pass Radiosity Method for Bezier Patches %E K. Bouatouch %E C. Bouville %B Photorealism in Computer Graphics (Proceedings Eurographics Workshop on Photosimulation, Realism and Physics in Computer Graphics, 1990) %D 1992 But I have not got hold of these articles. Can anyone help? Anyway, I am sampling (using ray-casting to compute form-factors) uniformly in uv-space on the NURBS, and then I subdivide adaptively if needed. Now I was wondering if there is some other technique for sampling curved surfaces. Has anyone tried sampling uniformly in 3D instead, that is letting the 3D-distance between a pair of neighbour-points be constant all over the surface? Or positioning more sample points in regions of high curvature (although this seems often to be the case when sampling uniformly in the parametric uv-space for my NURBS) ? Or any other? I am using my radiosity solutions for VR-applications which means that I want fast reconstruction of the radiosity functions over the surfaces. Is everyone using Gouraud-shading for fast radiosity- reconstruction? Sampling uniformly in the uv-space implies a texture map, so I am generating a texture map containing the radiosities of each surface. Then I am texture mapping this bitmap onto the surface in order to reconstruct the radiosity function fast. My machine has no performance penalty for texture mapping, so it is fast. Also, another advantage is that you could use the radiosity texture map with any triangulation of the surface. This is not the case when using Gouraud shading. Anyone has any comments, faster methods, better methods? Are these just old ideas? A last question: do most people use discontinuity meshing nowadays or are you still using the traditional methods? Sincerely, Tomas Lund Institute of Technology Sweden From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id FAA06936; Sat, 22 Jul 1995 05:46:13 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id FAA10608 for ; Sat, 22 Jul 1995 05:28:31 +0200 Received: from june.cs.washington.edu (june.cs.washington.edu [128.95.1.4]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id FAA18839 for ; Sat, 22 Jul 1995 05:28:29 +0200 Received: (per@localhost) by june.cs.washington.edu (8.6.12/7.2ju) id UAA18894; Fri, 21 Jul 1995 20:28:28 -0700 Date: Fri, 21 Jul 1995 20:28:27 -0700 (PDT) From: "Per H. Christensen" To: globillum@imag.fr cc: "Per H. Christensen" Subject: Thesis Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII; format=flowed X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hi Globillumers! I've just finished my dissertation. It's entitled "Hierarchical Techniques for Glossy Global Illumination" -------------------------------------------------------------------- Abstract: This dissertation concerns efficient computation of realistic images. To compute realistic synthetic images, the effect of global illumination is essential. Ray tracing algorithms solve the global illumination problem for specular interreflections, and radiosity algorithms solve it for diffuse interreflections. But computing a solution is more complicated when the surfaces have glossy reflection. This dissertation describes hierarchical techniques for efficient solution of the glossy global illumination problem. Two types of hierarchy are utilized: wavelets to accurately represent radiance distributions on surface patches, and clusters to approximately represent radiant intensity from groups of surface patches. Without hierarchical techniques, the solution time would be quadratic in the number of patches and $O(b^{1.5})$ in the number of basis functions~$b$. The hierarchical techniques make solution time linear in both the number of patches and in the number of basis functions. This reduction is significant since the numbers of patches and basis functions are large for accurate solutions in realistic environments. Furthermore, directional importance is used to focus refinement of the solution on parts that contribute significantly to a particular view of the scene. Our method is the first finite-element method capable of handling complex glossy scenes. ----------------------------------------------------------------- If you would like to read more than the abstract, go to http://www.cs.washington.edu/homes/per/publication.html and click on "dissertation" or "smaller version". The smaller version is much faster to transfer, but has no color images. -- Per From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id QAA22490; Tue, 25 Jul 1995 16:31:41 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id PAA28496 for ; Tue, 25 Jul 1995 15:53:47 +0200 Received: from m1.cs.man.ac.uk (m1.cs.man.ac.uk [130.88.13.4]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id PAA29474 for ; Tue, 25 Jul 1995 15:53:44 +0200 Received: from r9.cs.man.ac.uk by m1.cs.man.ac.uk (4.1/SMI-4.1:AL5l) id AA03765; Tue, 25 Jul 95 14:53:30 BST Date: Tue, 25 Jul 95 14:53:28 BST From: Simon Gibson Message-Id: <9507251353.AA11586@r9.cs.man.ac.uk> To: globillum@imag.fr Subject: Units of Radiance X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Dear all, Could somebody please tell me how to convert from luminance (cd/m(-2)) to radiance (W/m(-2)/sr). E.g. a surface has a radiance value of 3183 cd/m(-2). What is that in W/m(-2)/sr?? Any help much appreciated. Simon. From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id TAA21488; Wed, 26 Jul 1995 19:15:59 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id PAA04327 for ; Wed, 26 Jul 1995 15:52:13 +0200 Received: from inra.inra.fr (inra.inra.fr [138.102.88.1]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id PAA04254 for ; Wed, 26 Jul 1995 15:52:12 +0200 Received: from bcgn.grignon.inra.fr (bcgn.grignon.inra.fr [192.93.95.1]) by inra.inra.fr (8.6.12/8.6.12) with SMTP id PAA19044 for ; Wed, 26 Jul 1995 15:50:33 +0200 Received: from tld213.GRIGNON.INRA.FR by bcgn.grignon.inra.fr, Wed, 26 Jul 95 15:45:15 +0200 Received: by tld213.GRIGNON.INRA.FR (5.x/SMI-SVR4) id AA00710; Wed, 26 Jul 1995 14:48:24 +0100 Date: Wed, 26 Jul 1995 14:48:24 +0100 From: Michael Chelle Message-Id: <9507261348.AA00710@tld213.GRIGNON.INRA.FR> To: globillum@imag.fr Subject: 6th Eurographic Workshop on rendering X-Sun-Charset: US-ASCII X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Hi Globillumers! Is there exist a bib file (BibTeX format), with the references of the last Eurographic Workshop on Rendering (6th, Dublin, June 95)? Michael _________________________________________________________________________ / Michael CHELLE \ | | | INRA | email : chelle@bcgn.grignon.inra.fr | | Station de Bioclimatologie | phone : +33 1 30 81 55 31 | | 78850 THIVERVAL-GRIGNON (France) | fax : +33 1 30 81 55 63 | \_________________________________________________________________________/ From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id EAA24737; Thu, 27 Jul 1995 04:27:09 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id EAA18250 for ; Thu, 27 Jul 1995 04:17:01 +0200 Received: from arl-img-4.compuserve.com (arl-img-4.compuserve.com [198.4.7.4]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id EAA21064 for ; Thu, 27 Jul 1995 04:17:00 +0200 Received: by arl-img-4.compuserve.com (8.6.10/5.950515) id WAA01415; Wed, 26 Jul 1995 22:16:28 -0400 Date: 26 Jul 95 22:14:12 EDT From: Ian Ashdown <72060.2420@CompuServe.COM> To: Global Illumination Subject: Re: 6th Eurographics Workshop on Rendering Message-ID: <950727021412_72060.2420_FHG132-1@CompuServe.COM> X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Michael Chelle wrote: > Is there exist a bib file (BibTeX format), with the references of > the last Eurographic Workshop on Rendering (6th, Dublin, June 95)? The following is from the forthcoming (August 15th) release of RadBib95.Z, the one and only radiosity bibliography that is available from hobbes.lbl.gov and other fine ftp sites. I understand that Springer Verlag will be publishing the workshop proceedings Real Soon Now, at which point I will add the publisher reference and page numbers. (If Springer Verlag wants to send me a prepublication review copy, I will not object ... :+) P.S. - the next release of RadBib95 will have an additional 65 radiosity and global illumination references, for a total of 711. It's been a good year! P.P.S. - I cannot vouch for the accuracy of the following, since all I had to go on was the Advance Announcement for the workshop. %A Gladimir Baranoski %A Randall Bramley %A Peter Shirley %T Fast Radiosity Solutions for High Average Reflectance Environments %J Sixth Eurographics Workshop on Rendering %C Dublin, Ireland %D June 1995 %Z (to appear) %A Philippe Bekaert %A Yves D. Willems %T Improtance-Driven Progressive Refinement Radiosity %J Sixth Eurographics Workshop on Rendering %C Dublin, Ireland %D June 1995 %Z (to appear) %A Steven Collins %T Reconstruction of Indirect Illumination from Area Luminaires %J Sixth Eurographics Workshop on Rendering %C Dublin, Ireland %D June 1995 %Z (to appear) %A P. M. Deville %A J. C. Paul %T Modelling the Spatial Energy Distribution of Complex Light Sources for Lighting Engineering %J Sixth Eurographics Workshop on Rendering %C Dublin, Ireland %D June 1995 %Z (to appear) %A P. Dutre %A Y. D. Willems %T Potential-Driven Monte Carlo Particle Tracing for Diffuse Environments with Adaptive Probability Density Functions %J Sixth Eurographics Workshop on Rendering %C Dublin, Ireland %D June 1995 %Z (to appear) %A A. Fournier %T Separating Reflection Functions for Linear Radiosity %J Sixth Eurographics Workshop on Rendering %C Dublin, Ireland %D June 1995 %Z (to appear) %A R. Gershbein %T A Study of Integration Methods for Coupling of Galerkin Radiosity Systems %J Sixth Eurographics Workshop on Rendering %C Dublin, Ireland %D June 1995 %Z (to appear) %A Nicolas Holzschuch %A Francois Sillion %T Isolating Discretization Error: An Accurate Refinement Strategy for Hierarchical Radiosity with Linear Functions %J Sixth Eurographics Workshop on Rendering %C Dublin, Ireland %D June 1995 %Z (to appear) %A Henrik Wann Jensen %T Importance Driven Path Tracing Using the Photon Map %J Sixth Eurographics Workshop on Rendering %C Dublin, Ireland %D June 1995 %Z (to appear) %A Stefan Muller %A Wolfram Kresse %A Frank Schoffel %T A Radiosity Approach for the Simulation of Daylight %J Sixth Eurographics Workshop on Rendering %C Dublin, Ireland %D June 1995 %Z (to appear) %A L. Neumann %A W. Purgathofer %A R. F. Tobler %A A. Neumann %A P. Elias %A M. Feda %A X. Pueyo %A The Stochastic Ray Method for Radiosity %J Sixth Eurographics Workshop on Rendering %C Dublin, Ireland %D June 1995 %Z (to appear) %A L. Neumann %A R. F. Tobler %A P. Elias %T The Constant Radiosity Step %J Sixth Eurographics Workshop on Rendering %C Dublin, Ireland %D June 1995 %Z (to appear) %A J. Nimeroff %A J. Dorsey %A H. Rushmeier %T A Framework for Global Illumination in Animated Environments %J Sixth Eurographics Workshop on Rendering %C Dublin, Ireland %D June 1995 %Z (to appear) %A Sumanta N. Pattanaik %A Kadi Bouatouch %T Linear Radiosity with Estimation Error %J Sixth Eurographics Workshop on Rendering %C Dublin, Ireland %D June 1995 %Z (to appear) %A Mateu Sbert %A Frederic Perez %A Xavier Pueyo %T Global Monte Carlo: A Progressive Solution %J Sixth Eurographics Workshop on Rendering %C Dublin, Ireland %D June 1995 %Z (to appear) %A P. Schroder %A W. Sweldens %T Spherical Wavelets: Texture Processing %J Sixth Eurographics Workshop on Rendering %C Dublin, Ireland %D June 1995 %Z (to appear) %A Peter Shirley %A Bretton Wade %A Philip Hubbard %A David Zareski %A Bruce Walter %A Donald P. Greenberg %T Global Illumination via Density Estimation %J Sixth Eurographics Workshop on Rendering %C Dublin, Ireland %D June 1995 %Z (to appear) %A F. Sillion %A G. Drettakis %A C. Soler %T A Clustering Algorithm for Radiance Calculation in General Environments %J Sixth Eurographics Workshop on Rendering %C Dublin, Ireland %D June 1995 %Z (to appear) %A Philipp Slusallek %A Michael Schroder %A Marc Stamminger %A Hans-Peter Seidel %T Smart Links and Efficient Reconstruction for Wavelet Radiosity %J Sixth Eurographics Workshop on Rendering %C Dublin, Ireland %D June 1995 %Z (to appear) %A G. Ward %T Making Global Illumination User Friendly %J Sixth Eurographics Workshop on Rendering %C Dublin, Ireland %D June 1995 %Z (to appear) %A Kurt Zimmerman %A Peter Shirley %T A Two-Pass Realistic Image Synthesis Method for Complex Scenes %J Sixth Eurographics Workshop on Rendering %C Dublin, Ireland %D June 1995 %Z (to appear) From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id BAA12000; Fri, 28 Jul 1995 01:13:31 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id BAA18017 for ; Fri, 28 Jul 1995 01:02:04 +0200 Received: from june.cs.washington.edu (june.cs.washington.edu [128.95.1.4]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id BAA21317 for ; Fri, 28 Jul 1995 01:02:01 +0200 Received: (danix@localhost) by june.cs.washington.edu (8.6.12/7.2ju) id QAA29067 for globillum@imag.fr; Thu, 27 Jul 1995 16:01:59 -0700 From: Dani Lischinski Message-Id: <199507272301.QAA29067@june.cs.washington.edu> Subject: glossy clustering To: globillum@imag.fr Date: Thu, 27 Jul 1995 16:01:58 -0700 (PDT) X-Mailer: ELM [version 2.4 PL23] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Dear globillumers, As some of you may know, Per Christensen, Eric Stollnitz, David Salesin and I have been doing some research on extending clustering to glossy global illumination. Last month we submitted a paper "Clustering for Glossy Global Illumination" summarizing our research to ACM TOG. The paper is available online via anonymous ftp from espresso.cs.washinton.edu under pub/danix/clustering (ftp://espresso.cs.washinton.edu/pub/danix/clustering on the WWW). An earlier version of this paper was submitted to Siggraph 95 (and was rejected). Fortunately, the comments of the anonymous reviewers challenged us to substantially improve both the paper and the implementation. The highlights of the results section are: a comparison with RADIANCE on a glossy "sphereflake" model and nice global illumination solutions for an architectural environment with ~8000 initial surfaces, most of which are glossy. If you happen to read the paper and have any comments, please e-mail them to me, or we could discuss them at Siggraph. Thanks, Dani ------------------------------------------------------- Dani Lischinski Department of Computer Science and Engineering University of Washington Box 352350 Seattle, WA 98195-2350 e-mail: danix@cs.washington.edu, phone: 206 543-3368 ------------------------------------------------------- From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id TAA26864; Fri, 28 Jul 1995 19:02:17 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id SAA14499 for ; Fri, 28 Jul 1995 18:38:51 +0200 Received: from june.cs.washington.edu (june.cs.washington.edu [128.95.1.4]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id SAA15051 for ; Fri, 28 Jul 1995 18:38:50 +0200 Received: (danix@localhost) by june.cs.washington.edu (8.6.12/7.2ju) id JAA18413 for globillum@imag.fr; Fri, 28 Jul 1995 09:38:46 -0700 From: Dani Lischinski Message-Id: <199507281638.JAA18413@june.cs.washington.edu> Subject: Re: glossy clustering - Oops! To: globillum@imag.fr Date: Fri, 28 Jul 1995 09:38:46 -0700 (PDT) In-Reply-To: <199507272301.QAA29067@june.cs.washington.edu> from "Dani Lischinski" at Jul 27, 95 04:01:58 pm X-Mailer: ELM [version 2.4 PL23] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Naturally, I had to have a typo in the most important line of my message. To make matters worse, I replicated the typo by cutting and pasting, instead of retyping. The correct address for the ftp site is, of course: ftp from espresso.cs.washington.edu under pub/danix/clustering (ftp://espresso.cs.washington.edu/pub/danix/clustering on the WWW). (in my original message I omitted the 'g' in "washington") Thanks to those of you who pointed this out to me. Dani ------------------------------------------------------- Dani Lischinski Department of Computer Science and Engineering University of Washington Box 352350 Seattle, WA 98195-2350 e-mail: danix@cs.washington.edu, phone: 206 543-3368 ------------------------------------------------------- From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id AAA01655; Fri, 11 Aug 1995 00:17:55 +0200 Received: from lbl.gov (lbl.gov [128.3.254.23]) by isis.imag.fr (8.6.11/8.6.9) with SMTP id AAA00458 for ; Fri, 11 Aug 1995 00:03:22 +0200 Received: from theo.lbl.gov by lbl.gov (4.1/1.39) id AA04369; Thu, 10 Aug 95 15:00:47 PDT Received: by theo.lbl.gov (4.1/1.39) id AA07415; Thu, 10 Aug 95 15:00:36 PDT Date: Thu, 10 Aug 95 15:00:36 PDT From: Greg Ward Message-Id: <9508102200.AA07415@theo.lbl.gov> To: globillum@imag.fr Subject: Siggraph meeting X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Hello Globillumers, Well, we just got out of our annual Siggraph lunch meeting, so I thought I would jot some notes about it while it was still fresh in my overcrowded brain. There were about 20 of us attending, and I won't embarrass myself by mispelling (or forgetting) everyone's name, but instead I'll just mention some of the topics we covered and what was said about them. 1. Sharing models and data To address need for shared models that are usable and useful for global illumination, a new format has been developed called MGF (for Materials and Geometry Format) and models and libraries are now available from: http://radsite.lbl.gov/mgf/HOME.html Or, if you only have ftp access, try: anonymous@hobbes.lbl.gov /www/mgf/ This format supports a reasonable reflectance model, CIE XYZ and spectral colors, and the IES luminaire data format for light sources. A number of models from Radiance and other sources have been collected, and we encourage people with big hearts to add their own models to our collection. Write to me if you have any questions or want to get on the mailing list for how to improve this format to meet our long-term needs. 2. Setting up light sources Dan Wexler pointed out that one of the biggest time sinks in animation and rendering for film is the setting up of light sources, and that methods for making this more interactive were critical to this application. Specifically, he felt that a "deep raster" approach (similar to that developed by Sequin et al and presented at Siggraph 4 years or so ago) was a good way to go. In general, he felt there needed to be more of an emphasis on animation and interaction than there was in our current focus on static environments and generating one really nice image. 3. Image-based rendering Pete Shirley addressed a general question to the group about the relative importance and promise of image-based rendering (ala Quicktime VR) versus polygon-based methods. The overall response seemed to indicate that indeed image interpolation was a significant direction to head in the future, though polygon rendering will continue to be important when object manipulatin is required and for nearby objects. It seemed that at least five people there were actively pursuing such techniques. (Check out this year's Siggraph proceedings on Plenoptic Modeling and Quicktime VR, also Nimeroff et al in Eurographics Rendering Workshop '95.) 4. Visibility processing Several people talked about the difficulty of geometric simplification and other statistical or computational geometry methods for detecting visibility changes or approximating visibility. Christine Piatko of NIST reminded folks that tracking visibility is an O(N^6) problem and not something you want to do explicitly, and there was an interesting paper by Francois Sillion and George Drettakis (similar in some respects to the one Francois presented at EGRW this June) on approximating shadows. Jeff Nimeroff of UPenn also mentioned the work he had done with Julie Dorsey and Holly Rushmeier and presented at EGRW on statistical measures of object visibility for looking at this problem. It was agreed by most that statistical measures or simplification were necessary in large environments, though there is still much work to be done in this area. 5. Calibrated input and output Holly Rushmeier (who by the way is next year's Siggraph papers chair) talked a little about the difficulty of obtaining accurate physical data from real-world scenes, and a number of people lamented about the undetermined nature of image-to-output mappings for computer monitors, printers and film recorders. It was suggested that these devices be measured, which is certainly possible, and that this data be shared with the larger community. (Hear, hear, let's all do it, etc.) Holly and I also reminded people to look at the conference room image measurements and model we have made available on the web site: http://radsite.lbl.gov/mgf/compare.html >>From there, you can also pick up an online copy of our EGRW '95 paper on image metrics if you haven't purchased the Springer-Verlag proceedings yet. 6. Getting papers into Siggraph Henrik Wann Jensen of Denmark asked about the lack of papers covering global illumination this year at Siggraph, and if this was a trend or what? Holly answered that there's a bias against incremental work in any field, and that Siggraph tends to accept papers that are new directions rather than the logical next step in a technique previously published. Ian Ashdown of Ledalite said that he had submitted something that reviewers liked except that it didn't have any pretty pictures and was therefore rejected. (No one had anything to say to console him on this.) I made the unsubstantiated claim that it can help to provide evidence of a real-life application along with an incremental improvement in one or more existing algorithms, and Holly agreed that there must be a balance between application and innovation. There is a lot of useful information by the way on next year's Siggraph in New Orleans, and even an early opportunity to suggest new ideas by October 4th. Look for the "new" icons on the web site: http://www.s95.siggraph.org/conferences/siggraph96/siggraph96.html In particular, you should be aware of the new electronic abstract requirement for technical papers. 7. Oracle-assisted rendering Another trend that people discussed (me for one) was the use of oracles to decide when and where to apply which alogrithms (a.k.a. "hacks") to improve the speed and quality of renderings. Some information may be derived from the scene itself, but other assistance will always require the user to help the program to guide the calculation. This is not as bad as it sounds, since users are after all necessary to rendering, so they may as well guide it. I directed people to my EGRW '95 paper on the subject, which I can make available online if people are interested. Although I don't plan to pursue this too much myself, I think it continues to be an interesting and promising direction for investigation. 8. Rendering code available Philipp Slusallek of Erlangen Univ. mentioned to the group that they have a renderer that extends Renderman input to include global illumination calculations (physically-based) and that code is available from him. His address is if you're interested. (He's going to hate me when he gets back.) Remember also about the Blue Moon Ray Tracer, written by Larry Gritz and available at: http://www.seas.gwu.edu/student/gritz/bmrt.html It also does some global illumination calculations, though I'm not in a position to compare the two. As long as I'm plugging other people's code, must mention my own for those of you who have been asleep or locked up for some time: http://radsite.lbl.gov/radiance/HOME.html Well, that's about it I guess. Anyone else who was there and remembers stuff I forgot or points I left out, please pipe in. I tend to do a really bad job at these sorts of summaries, and I neglected to take notes during the meeting, so I'm relying here on my less-than-adequate memory. -Greg From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id EAA19042; Wed, 16 Aug 1995 04:46:52 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id EAA12477 for ; Wed, 16 Aug 1995 04:40:58 +0200 Received: from haven.uniserve.com (haven.uniserve.com [198.53.215.121]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id EAA17159 for ; Wed, 16 Aug 1995 04:40:46 +0200 Received: from pm2-39.TVS.NET ([204.191.197.49]) by haven.uniserve.com with SMTP id <30813>; Tue, 15 Aug 1995 19:42:20 +0100 X-Sender: iashdown@ledalite.com (Unverified) X-Mailer: Windows Eudora Version 2.0.3 Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed To: globillum@imag.fr From: Ian Ashdown Subject: Radiosity bibliography updated Message-Id: <95Aug15.194220+0100_pdt.30813+719@haven.uniserve.com> Date: Tue, 15 Aug 1995 19:40:26 +0100 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit The latest release (August 15th) of my radiosity bibliography is now available as /pub/doc/RadBib95.Z from hobbes.lbl.gov. Since the last release (April 2nd), I managed to find another 99 papers and theses on radiosity and global illumination, bringing the total number of references to 745. You folks have been very busy this year! If I happened to miss anything or made any errors, *please* send me e-mail with the details. (I strongly suspect that I am missing numerous European references, particularly theses.) ... and as always, my thanks to Greg Ward at Lawrence Berkeley Laboratory for providing the disk space and the decidedly animated handshake. Ian Ashdown, P. Eng. READ THE BOOK! Research & Development Manager Radiosity: A Programmer's Perspective Ledalite Architectural Products Inc. by Ian Ashdown 9087A - 198th Street John Wiley & Sons, 1994 Langley, British Columbia Canada V3A 4P8 (Sneaky Internet Advertising) From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id GAA19159; Wed, 16 Aug 1995 06:00:41 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id FAA12808 for ; Wed, 16 Aug 1995 05:53:20 +0200 Received: from sgi.sgi.com (SGI.COM [192.48.153.1]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id FAA18394 for ; Wed, 16 Aug 1995 05:53:18 +0200 Received: from pdi.com by sgi.sgi.com via UUCP (950405.SGI.8.6.12/910110.SGI) for globillum@imag.fr id UAA17742; Tue, 15 Aug 1995 20:53:12 -0700 Received: from lilbuddy.pdi.com by pdi.pdi.com via SMTP (920330.SGI/(911001.SGI)1.4-PDI.RELAY) for globillum@imag.fr id AA13409; Tue, 15 Aug 95 20:46:42 -0700 Received: by lilbuddy.pdi.com (940816.SGI.8.6.9/(911001.SGI)1.2-PDI) for globillum@imag.fr id UAA25398; Tue, 15 Aug 1995 20:46:41 -0700 From: Dan Wexler Message-Id: <199508160346.UAA25398@lilbuddy.pdi.com> Subject: Cinematography references To: globillum@imag.fr Date: Tue, 15 Aug 1995 20:46:41 -0700 (PDT) X-Mailer: ELM [version 2.4 PL23] Mime-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Last week at SigGraph I mentioned that the Cinematography literature is replete with information concerning real-time global illumination. Here are a couple of my favorite references: American Cinematographer Manual Published by the American Society of Cinematographers (ASC), this is the Foley, vanDam (F&H) of all cameramen and lighting experts. Complete descriptions of all types of cameras, lights, lenses, filters and supports are given along with comparason tables. Techniques for special visual effects (background plates, compositing, miniatures, travelling mattes, optical printers), and special techniques (arial, underwater, arctic, tropical, day for night, stereo 3D, sound, television) are briefly discusses. There's even a section on Computer Graphics. This is a small book that can be found in many good book stores and sells for about $70. ISBN 0-935578-11-0 Millerson, Gerald; "Lighting for Television and Film"; 3rd Ed.; Focal Press; This is a very good introduction on how to light for film and video. Excellent discussions of the aesthetic qualities of light and perception. The basic principals of lighting (key, fill, shadows, balance, direction, continuity) are summarized. Detailed chapters on lighting people, the production process, atmospheric lighting, light sources and equipment, color temperature, picture control, scenery, and visual effects. A great book to learn how to light a scene to achieve a specific mood. First published in '72, third edition revised in '91. ISBN 0-240-51299-5 Malkiewicz, Kris; "Cinematography"; Simon & Schuster; '73 & '89 A shorter, but thorough treatment of the basic techniques. Chapters include Cameras, Films and Sensitometry, Filters and Light, Picture Quality Control, Sound Recording, Cutting and Lab Work, The Basics of Optical Printing, Vehicle and Underwater Cinematography, Production, and Video Transfer. ISBN 0-671-76220-6 Other excellent texts include: Lowell, Ross; "Matters of Light & Depth"; Broad Street Books; '92 ISBN 1-879174-03-0 Brown, Braun & Grondin; "Lighting Secrets for the Professional Photographer"; Writers Digest Books; '90; ISBN 0-89879-412-9 Hart, John; "Lighting for Action"; AMPHOTO; '92; ISBN 0-8174-4225-1 These contain other references, and I will happily send you more if you send me mail. I think I might like the third one because the author makes special mention of Haskell Wexler, who is, of course, not related to me in any way I know of. I am indebted to Jean Cunningham, one of our local lighting experts for most of these references. I cannot emphasize enough how much there is to learn from this body of knowledge. Good lighting with a bad renderer always looks better than bad lighting with a good renderer, IMHO. Daniel Wexler R&D Staff, Pacific Data Images From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id GAA01409; Thu, 17 Aug 1995 06:59:07 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id GAA06101 for ; Thu, 17 Aug 1995 06:49:54 +0200 Received: from merckx.graphics.cornell.edu (MERCKX.GRAPHICS.CORNELL.EDU [128.84.247.147]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id GAA20838 for ; Thu, 17 Aug 1995 06:49:53 +0200 Received: by merckx.graphics.cornell.edu (5.65/DEC-Ultrix/4.3) id AA17786; Thu, 17 Aug 1995 00:50:33 -0400 Message-Id: <9508170450.AA17786@merckx.graphics.cornell.edu> Received: by gaia.graphics.cornell.edu (1.37.109.8/16.2) id AA09361; Thu, 17 Aug 1995 00:49:47 -0400 From: Sing-Choong Foo Subject: Re: Cinematography references To: Dan Wexler Date: Thu, 17 Aug 1995 00:49:47 -0400 (EDT) Cc: globillum@imag.fr In-Reply-To: <199508160346.UAA25398@lilbuddy.pdi.com> from "Dan Wexler" at Aug 15, 95 08:46:41 pm X-Mailer: ELM [version 2.4 PL24] Mime-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 > American Cinematographer Manual > Published by the American Society of Cinematographers (ASC), this > is the Foley, vanDam (F&H) of all cameramen and lighting experts. > Complete descriptions of all types of cameras, lights, lenses, > filters and supports are given along with comparason tables. > Techniques for special visual effects (background plates, compositing, > miniatures, travelling mattes, optical printers), and special > techniques (arial, underwater, arctic, tropical, day for night, > stereo 3D, sound, television) are briefly discusses. There's even > a section on Computer Graphics. This is a small book that can be > found in many good book stores and sells for about $70. > ISBN 0-935578-11-0 > The price is only $49.95. You can order it from ASC (American Society of Cinematographers) (213)969-4333. -Sing From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id PAA12753; Thu, 17 Aug 1995 15:35:47 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id PAA15338 for ; Thu, 17 Aug 1995 15:19:42 +0200 Received: from fs1.cam.nist.gov (fs1.cam.nist.gov [129.6.80.33]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id PAA02878 for ; Thu, 17 Aug 1995 15:19:38 +0200 Received: from plum (plum.cam.nist.gov) by fs1.cam.nist.gov (4.1/SMI-DDN) id AA03794; Thu, 17 Aug 95 09:19:07 EDT Received: by plum (950215.SGI.8.6.10/SMI-3.2) id JAA28878; Thu, 17 Aug 1995 09:19:05 -0400 From: "Holly E Rushmeier" Message-Id: <9508170919.ZM28876@plum.cam.nist.gov> Date: Thu, 17 Aug 1995 09:19:05 -0400 X-Face: eO|V;3{XkGh^/1hW"\R$2ajo-]{6b+iSL&s}264L"[Qr(@>+$'c"p(xid20x|DKhrQ-OZw#!/6;*ny_NU>tEA4Z#p5~.hbz)nL990=A^Z/88}i]; Mon, 21 Aug 1995 15:38:59 +0200 Received: from mr.tuwien.ac.at (mr.tuwien.ac.at [128.130.2.10]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id PAA22454 for ; Mon, 21 Aug 1995 15:38:58 +0200 Received: from stellaris.cg.tuwien.ac.at by mr.tuwien.ac.at with SMTP (PP); Mon, 21 Aug 1995 15:38:57 +0200 Received: from [128.130.166.50] by stellaris.cg.tuwien.ac.at via SMTP (940816.SGI.8.6.9/910805.SGI) for id PAA02070; Mon, 21 Aug 1995 15:38:54 +0200 X-Sender: wp@stellaris.cg.tuwien.ac.at Message-Id: Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed Date: Mon, 21 Aug 1995 15:41:01 +0100 To: globillum@imag.fr From: Werner Purgathofer Subject: Rendering Workshop proceedings X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit The Proceedings of the Rendering Workshops 5 and 6 are available now! ------------------------------------------------------------------ 5th Rendering Workshop 1994: Photorealistic Rendering Techniques (ed. Sakas, Shirley, Mueller) ISBN 3-540-58475-7 410 pages, DM 198,- order from: Springer-Verlag Postfach 31 13 40 D-10643 Berlin, Germany URL: http://www.springer.de/ ------------------------------------------------------------------ 6th Rendering Workshop 1995: Rendering Techniques'95 (ed. Hanrahan, Purgathofer) ISBN 3-211-82733-1 384 pages, DM 118,- order from: Springer-Verlag P.O.Box 89 A-1201 Vienna, Austria email: springer@springer.co.at Participants of the 1995-workshop will receive a copy of the book within the next weeks, it was included in the workshop fee. ------------------------------------------------------------------ for your information: 7th Rendering Workshop 1996: will take place in Porto, Portugal, in June 1996. Program chairs: Peter Schroeder, Xavier Pueyo. Submission deadline will be the 5th April, 96. ------------------------------------------------------------------- Werner Purgathofer Tel. +43(1)58801 4548 Institute of Computer Graphics ( secretary: 4549 ) Technical University of Vienna Fax. +43(1)5874932 Karlsplatz 13 / 186 email: wp@cg.tuwien.ac.at A-1040 Wien / Austria WWW: http://www.cg.tuwien.ac.at ------------------------------------------------------------------- From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id WAA21742; Thu, 31 Aug 1995 22:18:52 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id VAA20822 for ; Thu, 31 Aug 1995 21:51:17 +0200 Received: from haven.uniserve.com (haven.uniserve.com [198.53.215.121]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id VAA23123 for ; Thu, 31 Aug 1995 21:50:56 +0200 Received: from pm2-32.TVS.NET ([204.191.197.42]) by haven.uniserve.com with SMTP id <31178>; Thu, 31 Aug 1995 12:52:23 +0100 X-Sender: iashdown@ledalite.com (Unverified) X-Mailer: Windows Eudora Version 2.0.3 Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed To: globillum@imag.fr From: Ian Ashdown Subject: Photometric data now available Cc: lighting@garnet.nist.gov Message-Id: <95Aug31.125223+0100_pdt.31178+783@haven.uniserve.com> Date: Thu, 31 Aug 1995 12:46:47 +0100 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit *** NOW AVAILABLE (FREE!) *** * 200+ photometric data files for fluorescent light fixtures * Documentation and ANSI C source code for an IESNA LM-63 photometric data file parser (public domain) * Demonstration radiosity renderer for MS-Windows 3.1 and Windows '95 * Radiosity bibliography * Color quantization bibliography * ... and more Ledalite Architectural Products Inc. (Vancouver, BC) is a leading North American designer and manufacturer of linear architectural lighting systems. Our R&D efforts include a strong and active interest in advanced photometric measurement techniques, global illumination algorithms (especially radiosity), and photorealistic rendering for architectural applications. Ledalite's Home Page -------------------- As part of this effort, we have recently established our presence on the World Wide Web: http://www.ledalite.com The primary purpose of this home page is to provide product information and technical support for our customers. However, we are also making the following resources available as a service to the computer graphics and illumination engineering research communities: Photometric Data Files ---------------------- Ledalite manufactures linear fluorescent lighting systems for commercial, educational, and institutional projects. We have over two hundred IESNA LM-63 photometric data files for these products available for downloading. At this time, these files are catalogued by product code only. However, we are currently working to place our product catalog (including AutoCAD drawings) online. If you are associated with an educational institution and would like a copy of Ledalite's product catalog, please contact iashdown@ledalite.com. The files are available in a PKZIP file for MS-DOS platforms. A GZIP version for UNIX platforms will be added in the near future. IESNA LM-63 Photometric Data File Parser ---------------------------------------- IESNA LM-63 is the North American standard for photometric data files provided by lighting fixture manufacturers. The file format specification is documented in the Illuminating Engineering Society of North America's LM-63-1991 publication. (A revised version, LM-63-1995, will be published later this year.) Implementing a parser for LM-63 photometric data files is not an easy task, particularly if you are not familiar with illumination engineering terminology. If you need such a parser but do not want to reinvent the wheel, you are welcome to download and use our public domain file parser. It is provided as ANSI C source code and accompanying documentation. The code compiles and executes on both MS-DOS and UNIX platforms with no modifications necessary. The files are available in a PKZIP file for MS-DOS platforms. A GZIP version for UNIX platforms will be added in the near future. In the meantime, the files are available as /pub/programs/iesparser.tar.Z from hobbes.lbl.gov and http://radsite.lbl.gov/mgf/HOME.html. Demonstration Radiosity Renderer -------------------------------- READ THE BOOK! and all that jazz. One of the byproducts of our R&D efforts was a book on radiosity ("Radiosity: A Programmer's Perspective," by Ian Ashdown). It includes C++ source code for HELIOS, a fully- functional radiosity renderer for MS-Windows 3.1 and Windows NT. You can download a demonstration version of this program (sorry, source code not included) for MS-Windows 3.1 and Windows '95. There is only one scene description file provided (the ubiquitous Cornell Room), but the input file formats are documented in the online help. This program is also available as HELIOS2B.ZIP from Compuserve (GO GRAPHDEV, Raytrace Sources library) and as /pub/misc/helios2b.zip from ftp.avalon1.viewpoint.com. Radiosity Bibliography ---------------------- What Eric Haines of 3D/Eye began, Ledalite carries on as a public service. The radiosity bibliography now has 745 references, and continues to grow. This is another PKZIP file (BIBLIO.ZIP) for MS-DOS platforms. A GZIP version for UNIX platforms will be added in the near future. In the meantime, the file is available as /pub/doc/RadBib95.Z from hobbes.lbl.gov and http://radsite.lbl.gov. Color Quantization Bibliography ------------------------------- This bibliography of 60+ papers, articles, and books about color quantization algorithms is another public service from Ledalite. You can only answer the same question on comp.graphics.algorithms so many times! CQUANT95.TXT is included in the PKZIP file BIBLIO.ZIP for MS-DOS platforms. A GZIP version for UNIX platforms will be added in the near future. In the meantime, the file is available as /pub/doc/cquant95.Z from hobbes.lbl.gov and http://radsite.lbl.gov. Coming Soon ----------- Near-field photometry Nonimaging optics design using genetic algorithms Photometry and radiometry tutorials Lighting simulation software validation techniques Our home page is (as always) very much "Under Construction." We will be updating it and adding features as we gain experience with our customers' needs. In the meantime, we hope it offers you a useful resource. Acknowledgements ---------------- Our thanks to Greg Ward of Lawrence Berkeley Laboratory for providing space on hobbes.lbl.gov for our radiosity and color quantization bibliographies, and for leading 100-odd people into the fountain to get soaking wet at SIGGRAPH '95. Ian Ashdown, P. Eng. READ THE BOOK! Research & Development Manager Radiosity: A Programmer's Perspective Ledalite Architectural Products Inc. by Ian Ashdown 9087A - 198th Street New York, NY: John Wiley & Sons, 1994 Langley, British Columbia Canada V3A 4P8 (Sneaky Internet Advertising) From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id VAA27534; Fri, 8 Sep 1995 21:37:17 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id VAA20952 for ; Fri, 8 Sep 1995 21:13:37 +0200 Received: from kama.cse.ucsc.edu (kama.cse.ucsc.edu [128.114.24.49]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id VAA06561 for ; Fri, 8 Sep 1995 21:13:35 +0200 Received: (from raptor@localhost) by kama.cse.ucsc.edu (8.6.10/8.6.9) id MAA07022 for globillum@imag.fr; Fri, 8 Sep 1995 12:15:24 -0800 Date: Fri, 8 Sep 1995 12:15:24 -0800 From: "Adam G. Freeman" Message-Id: <199509082015.MAA07022@kama.cse.ucsc.edu> To: globillum@imag.fr Subject: code X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Hello, I'm looking for any pointers to hierarchical, importance-driven and/or discontinuity meshing radiosity code. Thanks, Adam Freeman /| / | / | /| _______________/ |__ / | __/ ------------ | / {@} | /.. | . VVvvvvvvv\ )) | ___///_ / | ___ | o< /o \// AAA^^^^^^/ ___-------- \ | o< )____ __/\\ \_____________\ \------- \| o< \\ \ \__\ From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id SAA00866; Fri, 15 Sep 1995 18:35:24 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id RAA15844 for ; Fri, 15 Sep 1995 17:48:43 +0200 Received: from sesame (sesame.imag.fr [129.88.29.83]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id RAA04985 for ; Fri, 15 Sep 1995 17:48:42 +0200 Received: from localhost (sillion@localhost) by sesame (8.6.4/8.6.4) id RAA03770 for globillum@imag.fr; Fri, 15 Sep 1995 17:48:41 +0200 From: Francois Sillion Message-Id: <199509151548.RAA03770@sesame> Subject: WWW home page for globillum To: Global Illumination List Date: Fri, 15 Sep 1995 17:48:41 +0200 (MDT) Reply-To: Francois.Sillion@imag.fr X-Mailer: ELM [version 2.4 PL23] MIME-Version: 1.0 Content-Type: text/plain; charset=windows-1252; format=flowed Content-Transfer-Encoding: 8bit X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Please note the change of http address for the globillum list's home page: the new address is http://safran.imag.fr/Membres/Francois.Sillion/GlobillumList.html The reason for the change is that there is now a 'public' page for access to the world, with the old name (since it had been diffused through graphics-related archives already). The difference between the two is mainly access to the main mail alias and discussion archives. The new setup should prevent glitches such as uninformed people sending requests to the entire list.. +------------------+------------------------------------------------------+ | Francois SILLION | iMAGIS/IMAG, B.P. 53, 38041 Grenoble Cedex 9. France | | ' | Tel: (+33) 76 51 43 54 -- Fax: (+33) 76 44 66 75 | +------------------+----------+-------------------------------------------+ | Francois.Sillion@imag.fr | http://safran.imag.fr/~Francois.Sillion | +-----------------------------+-------------------------------------------+ From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id OAA15357; Mon, 16 Oct 1995 14:05:29 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id KAA03013 for ; Mon, 16 Oct 1995 10:24:28 +0100 Received: from lorraine.loria.fr (lorraine.loria.fr [152.81.1.17]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id KAA11000 for ; Mon, 16 Oct 1995 10:24:27 +0100 Received: from oudinot.loria.fr (oudinot.loria.fr [152.81.8.13]) by lorraine.loria.fr (8.6.12/8.6.12) with ESMTP id KAA17255 for ; Mon, 16 Oct 1995 10:24:25 +0100 From: Sylvain Petitjean Received: (petitjea@localhost) by oudinot.loria.fr (8.6.12/8.6.12) id KAA28292; Mon, 16 Oct 1995 10:24:25 +0100 Date: Mon, 16 Oct 1995 10:24:25 +0100 Message-Id: <199510160924.KAA28292@oudinot.loria.fr> To: globillum@imag.fr Subject: reference X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Dear Globillumers, I have been looking for the following reference (taken from the radiosity bib of Ian Ashdown) for some time but to no avail. Can anyone help locate it? %A F. Bresciani %A P. P. Rinaldi %A F. Tapparo %T Applications and Comparisons of Different Mathematical Methods to Compute Form Factors for Radiosity Images %B Workstations for Experiments %I Springer-Verlag %C Berlin, Germany %D 1989 %K form factors Thanks in advance, - Sylvain From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id SAA11931; Fri, 20 Oct 1995 18:57:37 +0100 Received: from idefix.cs.kuleuven.ac.be (idefix.cs.kuleuven.ac.be [134.58.40.4]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id SAA18553 for ; Fri, 20 Oct 1995 18:03:54 +0100 Received: from flater.cs.kuleuven.ac.be (philippe@flater.cs.kuleuven.ac.be [134.58.45.35]) by idefix.cs.kuleuven.ac.be (8.6.12/8.6.12) with ESMTP id SAA22061 for ; Fri, 20 Oct 1995 18:03:32 +0100 Received: (from philippe@localhost) by flater.cs.kuleuven.ac.be (8.6.12/8.6.12) id SAA10468; Fri, 20 Oct 1995 18:03:28 +0100 From: Philippe Bekaert Message-Id: <199510201703.SAA10468@flater.cs.kuleuven.ac.be> Subject: initial release of our radiosity code available To: globillum@imag.fr Date: Fri, 20 Oct 1995 18:03:27 +0100 (MET) Cc: Philippe Bekaert MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Dear Globillumers, I'd like to announce the initial release of the radiosity code developed in our research group (see http://www.cs.kuleuven.ac.be/cwis/research/graphics/graphics-E.shtml). Features: --------- - It does both shooting (progressive refinement radiosity) and gathering. - Hierarchical refinement if you like (for both shooting or gathering) - Importance-driven if you like (for both shooting or gathering) - Formfactor computation by numerical integration. The ray-casting for visibility determination is accelerated by using hierarchical bounding boxes, shadow caching and shaftculling. - handles both triangles and (convex) quadrilaterals. - T-vertex elimination and many other rendering options. - reads Greg Wards MGF scene description files (see http://radsite.lbl.gov/mgf/HOME.html) - a more or less nice user interface and interactive view manipulation. - ... It requires - Motif, - Silicon Graphics' Iris GL (or a clone) or PEX - an ANSI-C compiler (gcc 2.7.0 was used to develop it) and GNU make (or another make which offers the .include feature, unless you change the Makefiles a bit) to compile it. You can obtain this code for free on URL: http://www.cs.kuleuven.ac.be/~philippe/rad.html +----------------------------------+------------------------------------------+ | Philippe Bekaert | Pracu koname presne, rychlo a dobre, ale | | Computer Graphics Research Group | potrebujeme nove stroje (We do the work | | Department of Computer Science | precisely, quick and well, but we need | | K. U. Leuven - Leuven (Belgium) | new machines) - J. Mistrik, Basic Slovak | +----------------------------------+------------------------------------------+ Philippe.Bekaert@cs.kuleuven.ac.be From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id TAA13777; Thu, 2 Nov 1995 19:44:01 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id RAA12791 for ; Thu, 2 Nov 1995 17:24:56 +0100 Received: from irz401.inf.tu-dresden.de (irz401.inf.tu-dresden.de [141.76.1.12]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id RAA24230 for ; Thu, 2 Nov 1995 17:24:36 +0100 Received: by irz401.inf.tu-dresden.de (8.6.12/8.6.12-s1) id SAA06974 for globillum@imag.fr; Thu, 2 Nov 1995 18:24:04 +0200 From: "Nguyen, D.C.(JuHu)" Message-Id: <199511021624.SAA06974@irz401.inf.tu-dresden.de> Subject: [Q] approximation for NFF-materials ? To: globillum@imag.fr Date: Thu, 2 Nov 1995 18:24:04 +0200 (MESZ) X-Mailer: ELM [version 2.4 PL23] MIME-Version: 1.0 Content-Type: text/plain; charset=windows-1252; format=flowed Content-Transfer-Encoding: 8bit X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hi, Im writing a .3DS -> .NFF converter for GX/GENERIC and got a problem w/ the NFF-coefficients for materials : A correct conversion of material coefficients from .3DS -> NFF is not possible, because the diffuse and specular component of object-material in NFF are *uniformly* scaled to Red,Green,Blue. e.g.: ## in 3DS: MatProperies { RGB Ambient; RGB Diffuse; RGB Specular; ... } ## in NFF: MatProperties { RGB Color; float kDiffuse; float kSpecular; ... } Thus, for NFF, Ambient = 0 , Diffuse = Color * kDiffuse, Specular = Color * kSpecular My question is: which approximation should be used to convert the 3 vectors Ambient, Diffuse and Specular in 3DS to the 1 vector Color and the 2 coefficients kDiffuse and kSpecular in NFF ???? Thanks in advance, JuHu -- /\__ Nguyen Duc Cuong (aka JuHu) - CG-student \ "This theory is based /__\ \ EMail : cn1@irz.inf.tu-dresden.de \ on arithmetic overflow!" \__/ WWW : http://www.inf.tu-dresden.de/~cn1/ \ [..VIDEA'95 story..] From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id CAA14454; Fri, 3 Nov 1995 02:56:32 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id CAA04006 for ; Fri, 3 Nov 1995 02:36:30 +0100 Received: from haven.uniserve.com (haven.uniserve.com [198.53.215.121]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id CAA05200 for ; Fri, 3 Nov 1995 02:35:59 +0100 Received: from pm3-46.TVS.NET ([204.191.197.56]) by haven.uniserve.com with SMTP id <30742-4>; Thu, 2 Nov 1995 17:37:28 -0000 X-Sender: iashdown@ledalite.com X-Mailer: Windows Eudora Version 2.0.3 Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed To: globillum@imag.fr From: Ian Ashdown Subject: Re: [Q] approximation for NFF-materials ? Message-Id: <95Nov2.173728-0000_pst.30742-4+200@haven.uniserve.com> Date: Thu, 2 Nov 1995 17:37:18 -0000 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Greg Ward wrote earlier today: > >The common approximation used converts color to scaled luminance, and is: > > grey = 0.3*red + 0.59*green + 0.11*blue > >This is based on a sort of generic definition of RGB, since there is no >accepted standard for it. > Oops! Sorry to disagree here, Greg, but this approximation is out of date. I made this same boo-boo in my book, and got firmly (and rightfully) slapped for it by someone from the University of Manchester. It happens to be that the < 0.30, 0.59, 0.11 > coefficients were established in the early days of NTSC color television. As noted by Charles Poynton in his excellent color FAQ (http://www.inforamp.net/~poynton): The coefficients 0.299, 0.587 and 0.114 properly computed luminance for monitors having phosphors that were contemporary at the introduction of NTSC television in 1953. They are still appropriate for computing video *luma* to be discussed below in Section 11 [i.e., Poynton's FAQ]. However, these coefficients do not accurately compute luminance for contemporary monitors. Backing up a few paragraphs: Contemporary CRT phosphors are standardardized in ITU-R Recommendation BT.709, "Basic Parameter Values for the HDTV Standard for the Studio and for the International Programme Exchange (1990) [formerly CCIR Rec. 709], to be described in Section 17 (ibid). The weights to compute true CIE luminance from *linear* red, green and blue (indicated without prime symbols), for the Rec. 709, are these: y709 = 0.2125 R + 0.7154 G + 0.0721 B So, there you have it. These coefficients are roughly the same as the old NTSC coefficients. However, the differences are quite evident in the resultant gray-scale images, particularly for saturated colors. Ian Ashdown, P. Eng. | READ THE BOOK! Research & Development Manager | Radiosity: A Programmer's Perspective Ledalite Architectural Products Inc. | by Ian Ashdown | John Wiley & Sons, 1994 | Visit http://www.ledalite.com | (Sneaky Internet Advertising) From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id VAA13952; Thu, 2 Nov 1995 21:14:11 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id UAA19754 for ; Thu, 2 Nov 1995 20:45:26 +0100 Received: from lbl.gov (lbl.gov [128.3.254.23]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id UAA00261 for ; Thu, 2 Nov 1995 20:45:23 +0100 Received: from hobbes.lbl.gov by lbl.gov (4.1/1.39) id AA07144; Thu, 2 Nov 95 11:45:12 PST Received: by hobbes.lbl.gov (3.2/SMI-3.2) id AA08360; Thu, 2 Nov 95 11:44:46 PST Date: Thu, 2 Nov 95 11:44:46 PST From: "Gregory J. Ward" Message-Id: <9511021944.AA08360@hobbes.lbl.gov> To: globillum@imag.fr Subject: Re: [Q] approximation for NFF-materials ? X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Hello Everyone, I forgot to cc this to the rest of the group, so JuHu doesn't get a million similar answers. (If you have a different answer, by all means...) ------------ Hi JuHu, The common approximation used converts color to scaled luminance, and is: grey = 0.3*red + 0.59*green + 0.11*blue This is based on a sort of generic definition of RGB, since there is no accepted standard for it. -Greg ------------ By the way, it seems like an appropriate time to make another plug for the Materials and Geometry Format, which I developed with a little help from my friends for representing and sharing physically-based scene descriptions for Monte Carlo rendering, radiosity and similar abuses. The web site is: http://radsite.lbl.gov/mgf/HOME.html While you are there, be sure to check out the conference room model done by Holly Rushmeier and others at NIST, who also took photometric images of the actual space for the ultimate comparison. We also have many cool and useful scenes and objects, culled from the Radiance distribution and even a few hand-built examples, including a complete office space with ugly Dilbert-style cubicle workstations. Parsing MGF is easy, thanks to the generic ANSI-C parser included, with more documentation than you can shake a stick at. All here, all now, all free. (Now, you just need some free time to go with it.) -Greg From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id WAA14030; Thu, 2 Nov 1995 22:20:39 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id WAA00958 for ; Thu, 2 Nov 1995 22:01:41 +0100 Received: from irz101.inf.tu-dresden.de (irz101.inf.tu-dresden.de [141.76.1.9]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id WAA01781 for ; Thu, 2 Nov 1995 22:01:31 +0100 Received: by irz101.inf.tu-dresden.de (8.6.12/8.6.12-s1) id XAA10571; Thu, 2 Nov 1995 23:00:52 +0200 From: "Nguyen, D.C.(JuHu)" Message-Id: <199511022100.XAA10571@irz101.inf.tu-dresden.de> Subject: Re: [Q] approximation for NFF-materials ? To: "Gregory J. Ward" Date: Thu, 2 Nov 1995 23:00:51 +0200 (MESZ) Cc: globillum@imag.fr In-Reply-To: <9511021944.AA08360@hobbes.lbl.gov> from "Gregory J. Ward" at Nov 2, 95 11:44:46 am X-Mailer: ELM [version 2.4 PL23] MIME-Version: 1.0 Content-Type: text/plain; charset=windows-1252; format=flowed Content-Transfer-Encoding: 8bit X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 > > Hello Everyone, > > I forgot to cc this to the rest of the group, so JuHu doesn't get a million > similar answers. (If you have a different answer, by all means...) > > ------------ > Hi JuHu, > > The common approximation used converts color to scaled luminance, and is: > > grey = 0.3*red + 0.59*green + 0.11*blue > > This is based on a sort of generic definition of RGB, since there is no > accepted standard for it. > > -Greg > ------------ Cool! I never hear about this mind-opened formular. Thanx! As far as i undertand, this formula can be used to get kDiffuse and kSpecular. But how to do i get Color ? Eric's idea is : > >My educated guess would be use the Diffuse color in 3DS, set kD to 1.0, and >also set kS to be something like > max_component(Specular) / max_component(Diffuse) >(avoiding division by 0). > I have tested his idea and got better results than my first approximation. -JuHu From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id VAA11210; Wed, 8 Nov 1995 21:01:29 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id TAA17657 for ; Wed, 8 Nov 1995 19:28:50 +0100 Received: from irz101.inf.tu-dresden.de (irz101.inf.tu-dresden.de [141.76.1.9]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id TAA05601 for ; Wed, 8 Nov 1995 19:28:42 +0100 Received: by irz101.inf.tu-dresden.de (8.6.12/8.6.12-s1) id TAA21390 for globillum@imag.fr; Wed, 8 Nov 1995 19:36:38 +0200 From: "Nguyen, D.C.(JuHu)" Message-Id: <199511081736.TAA21390@irz101.inf.tu-dresden.de> Subject: GENERIC To: Global Illumination List Date: Wed, 8 Nov 1995 19:36:37 +0200 (MESZ) X-Mailer: ELM [version 2.4 PL23] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hi, This message was posted to comp.graphics.algorithm, but i'm sure that not all persons on this list have time to read NEWS :). If you are interrested in OO-graphics, then this's the right one for you. -JuHu -- /\__ Nguyen Duc Cuong (aka JuHu) - CG-student \ "This theory is based /__\ \ EMail : cn1@irz.inf.tu-dresden.de \ on arithmetic overflow!" \__/ WWW : http://www.inf.tu-dresden.de/~cn1/ \ [..VIDEA'95 story..] ======================================================================= [ANNOUNCE] A Generic 3D Graphics Kernel V1.3 Current graphic systems (traditional or object-oriented) offer a certain amount of functionality but also prescribe a lot of impli- cations, constraints and may not fit a given task. The result is that in many cases people start from scratch, implement the basic graphics stuff again and again. The objective of the announced project is to develop a generic 3D graphics kernel that may be used to implement an own system by derivating the generic one. By aggregation and inheritance the interfaces and implementation of the generic kernel may be used. The generic kernel shall offer a huge functionality consisting of uncoupled classes that may adaptively be integrated into a specialized system without any run-time and memory overhead. The principal functionality of the system will be [is]: - basic parametric aggregates and related operators [parametric fix-sized vector, dl list, dynamic list, for-each iterators] - elementary graphical data types: vector (2D, 3D, generic), matrices, colors, vertex, etc. and related operators [2D, 3D, nD Vector, 4x4, nxn Matrix, "Phong" Surface, RGB color, different vertex types] - essential scene collections (DAG, tree, binary tree, linear list) [based on above-mentioned aggregates] - basic graphical design patterns such as PHIGS' CSS, or a CGRM environment with its components - basic topological classes w/ covariant extensibility [1D-, 2D-, Polyhedron topology, parametric curve and surface] - abstract and concrete rendering classes (rendering interfaces, camera models, specific rendering primitives, i.e., Quadric for ray-tracing) [ray-tracing and shading interface, perspectivic and orthographic camera model, shader, ray-tracer, quadric, polygon, shading and ray-tracing iterators to be used for cameras and composites, to be platform-independent, the specific shading stuff is encapsulated in a "device driver" with following realizations until now: * OpenGL and X11 * OpenGL and Tk 3.6/4.0 * OpenGL and Windows/NT * OpenGL and Windows/NT and Tk3.6 * OpenGL and Windows/NT and MFC 2.0 NOTE: OpenGL compatible public domain library Mesa has been tested successfully as replacement for OpenGL] - pixel-based output devices [Pixmap, ImageFile] - rendering-independent mathematical stuff, e.g., Splines and free form surfaces [solid textures, bump mappings, interpolated spline curves and surfaces] - basic interaction classes (abstract and concrete, e.g., low-level event types) [2D mouse and spaceball events, socket encapsulation, pixmap update event, callbacks, abstract input device featuring feedback access and hierarchical organization, input server, timer and file input devices] - utility classes (identification, file formats, user interface integration) [string, SGI-, Targa-, RGBA-file format, Tcl language binding (optional), interpretative class system, generic DeltaBlue constraint solver] For papers discussing the need for a generic graphics kernel see ftp://metallica.prakinf.tu-ilmenau.de/pub/PROJECTS/GENERIC/dublin.ps.gz ftp://metallica.prakinf.tu-ilmenau.de/pub/PROJECTS/GENERIC/springer95.ps.gz The generic kernel itself is available by ftp://metallica.prakinf.tu-ilmenau.de/pub/PROJECTS/GENERIC/generic1.3.tar.gz The generic kernel is provided with all sources and may be used for both commercial and non-commercial projects without restrictions. Comments, discussion and extensions are greatly welcome. Derived kernels until now: GX - an extended ray-tracing kernel by Nguyen Duc Cuong GT - an NFF compatible ray-tracing kernel for test purposes basing on GX (GX and GT are parts of the distribution) EGR GF - an object-oriented commercial semantic kernel for European furniture industry (headers included for demonstration purposes) EGR MAF - a distributed Multimedia application framework EGR TIGER - an interpretative OpenGL environment including Motif-like GUI functionality and hi-level OpenGL-based kernel for education Kernels in work: GY - reimplementation of former 3D graphics kernel YART GP - sample implementation of ISO PREMO There is a mailing List: generic@prakinf.tu-ilmenau.de [send mail with subject "subscribe GENERIC mailing list" to ekki@prakinf.tu-ilmenau.de ] Ekki. Special thx goes to Frank Wicht (TU Ilmenau, Germany), Nguyen Duc Cuong (TU Dresden, Germany), Heiko Fischer (EasternGraphics, Ger- many), Pavol Michalik (TU Ilmenau, Germany) and EasternGraphics GmbH, Arnstadt, Germany. **************************************************************** * Ekkehard 'Ekki' Beier * * email: ekki@prakinf.tu-ilmenau.de * * phone: ++49-3677-692775 fax: ++49-3677-694540 * * talk : ekki@metallica.prakinf.tu-ilmenau.de [141.24.11.247] * * www : http://metallica.prakinf.tu-ilmenau.de/ekki.html * * yart/vr: institute@speedy.prakinf.tu-ilmenau.de * * Technical University of Ilmenau * * Department of Computer Graphics * * Am Ehrenberg, PSF 327, D-98684 Ilmenau, GERMANY * **************************************************************** From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id UAA06284; Mon, 13 Nov 1995 20:40:12 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id TAA09763 for ; Mon, 13 Nov 1995 19:35:35 +0100 Received: from haven.uniserve.com ([198.53.215.121]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id TAA04644 for ; Mon, 13 Nov 1995 19:33:55 +0100 Received: from pm3-15.TVS.NET ([204.191.197.55]) by haven.uniserve.com with SMTP id <31369-3>; Mon, 13 Nov 1995 10:35:23 -0000 X-Sender: iashdown@ledalite.com (Unverified) X-Mailer: Windows Eudora Version 2.0.3 Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed To: globillum@imag.fr From: Ian Ashdown Subject: Radiosity Bibliography, Take Six Message-Id: <95Nov13.103523-0000_pst.31369-3+706@haven.uniserve.com> Date: Mon, 13 Nov 1995 10:35:14 -0000 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit The sixth installment of RADBIB95, the definitive radiosity and global illumination bibliography, is now available from: ftp://hobbes.lbl.gov/pub/doc/ and (please wait until Wednesday, Nov. 15): http://www.ledalite.com/library/rrt.html The number of references has grown to (yoicks!) 781. The color quantization bibliography (CQUANT95) has also been updated, and now has 87 references. It is available from hobbes.lbl.gov and (again, please wait until next Wednesaday): http://www.ledalite.com/library/cgis.html Incidentally, has anyone seen this paper? %A R. L. Perry %A E. P. Speck %T Geometric Factors for Thermal Radiation Exchange between Cows and their Surroundings %R Technical Report 59-323 %I Journal of the American Society of Agricultural Engineering %D 1959 %K form factors %Z a seminal paper in computing cow form factors Moo! Ian Ashdown, P. Eng. | READ THE BOOK! Research & Development Manager | Radiosity: A Programmer's Perspective Ledalite Architectural Products Inc. | by Ian Ashdown | John Wiley & Sons, 1994 | Visit http://www.ledalite.com | (Sneaky Internet Advertising) From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id WAA06501; Mon, 13 Nov 1995 22:33:01 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id VAA12337 for ; Mon, 13 Nov 1995 21:55:41 +0100 Received: from fs1.cam.nist.gov (fs1.cam.nist.gov [129.6.80.33]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id VAA08379 for ; Mon, 13 Nov 1995 21:55:39 +0100 Received: from plum (plum.cam.nist.gov) by fs1.cam.nist.gov (4.1/SMI-DDN) id AA22679; Mon, 13 Nov 95 15:55:32 EST Received: by plum (950911.SGI.8.6.12.PATCH825/SMI-3.2) id PAA24103; Mon, 13 Nov 1995 15:55:28 -0500 From: "Holly E Rushmeier" Message-Id: <9511131555.ZM24101@plum.cam.nist.gov> Date: Mon, 13 Nov 1995 15:55:28 -0500 In-Reply-To: iashdown@ledalite.com (Ian Ashdown) "Radiosity Bibliography, Take Six" (Nov 13, 10:35am) References: <95Nov13.103523-0000_pst.31369-3+706@haven.uniserve.com> Reply-To: holly.rushmeier@nist.gov X-Face: eO|V;3{XkGh^/1hW"\R$2ajo-]{6b+iSL&s}264L"[Qr(@>+$'c"p(xid20x|DKhrQ-OZw#!/6;*ny_NU>tEA4Z#p5~.hbz)nL990=A^Z/88}i], globillum@imag.fr Subject: Re: Radiosity Bibliography, Take Six Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hi everyone - I did look up the cow paper once, and it is for real. The motivation was designing heating systems for the care of livestock. Here is a summary: "Uses mechanical integrator to measure factors from various wall elements to a cow, and presents some results for size of equivalent sphere that gives same factor as cow. It is found that the sphere origin should be place at one-fourth of the withers-to-pin-bone length back of the withers, at a height above the floor of two-thirds the height of the withers, and the equivalent sphere radius should be 1.8, 2.08 or 1.78 times the heart girth for exchange with the floor and ceiling, sidewalls, or front and back walls respectively. Also discusses exchange between cows and entire bounding walls, floor and ceiling and between parallel cows." I don't think I kept a copy of the paper, so please don't ask me for it. As I recall, the authors were from California, and the paper was initially read at an agricultural meeting held at Cornell. I looked it up in the library at Ga. Tech., but I expect it could be found at other places, such as Cornell (in Mann library if Carpenter doesn't have it) which has a degree program in Agricultural Engineering. Pastorally, Holly On Nov 13, 10:35am, Ian Ashdown wrote: > > Incidentally, has anyone seen this paper? > > %A R. L. Perry > %A E. P. Speck > %T Geometric Factors for Thermal Radiation Exchange between Cows and > their Surroundings > %R Technical Report 59-323 > %I Journal of the American Society of Agricultural Engineering > %D 1959 > %K form factors > %Z a seminal paper in computing cow form factors > > Moo! > Ian Ashdown, P. Eng. | READ THE BOOK! > Research & Development Manager | Radiosity: A Programmer's Perspective > Ledalite Architectural Products Inc. | by Ian Ashdown > | John Wiley & Sons, 1994 > | > Visit http://www.ledalite.com | (Sneaky Internet Advertising) > >-- End of excerpt from Ian Ashdown From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id UAA14666; Tue, 21 Nov 1995 20:28:55 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id TAA26728 for ; Tue, 21 Nov 1995 19:49:12 +0100 Received: from merckx.graphics.cornell.edu (MERCKX.GRAPHICS.CORNELL.EDU [128.84.247.147]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id TAA26675 for ; Tue, 21 Nov 1995 19:49:06 +0100 Received: by merckx.graphics.cornell.edu (5.65/DEC-Ultrix/4.3) id AA21688; Tue, 21 Nov 1995 13:48:54 -0500 Message-Id: <9511211848.AA21688@merckx.graphics.cornell.edu> Received: by barn.graphics.cornell.edu (1.37.109.8/16.2) id AA10158; Tue, 21 Nov 1995 13:48:33 -0500 From: Peter Shirley Subject: graphics pages To: globillum@imag.fr Date: Tue, 21 Nov 95 13:48:32 EST Mailer: Elm [revision: 70.85] X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit I am updating my list of graphics pages at: http://www.graphics.cornell.edu/~shirley/graphics.html If you know of any I should add, please let me know. Also, if you have online Monte Carlo code or papers, please let me know and I will add you to: http://www.graphics.cornell.edu/~shirley/mc.html Thanks Pete Shirley shirley@graphics.cornell.edu From To: Peter Shirley From: Werner Purgathofer Subject: Re: graphics pages Message-Id: X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Date: Wed, 22 Nov 1995 08:47:13 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit >I am updating my list of graphics pages at: > >http://www.graphics.cornell.edu/~shirley/graphics.html > >If you know of any I should add, please let me know. Dear Pete, here are some additional CG labs: http://www.fsz.bme.hu/~szirmay http://www.sys.uea.ac.uk/Research/ResGroups/CGP/ http://korsika.informatik.uni-rostock.de:8080/ http://sgi.felk.cvut.cz/index.html http://www.inf.ethz.ch/department/IS/cg/ http://www.cs.uml.edu/~haim/ivpr.html http://www.igd.fhg.de/ http://www9.informatik.uni-erlangen.de/ http://greco.gris.informatik.uni-tuebingen.de/ http://www.susx.ac.uk/engg/research/vlsi/vlsi.htm http://www.comp.brad.ac.uk/research/GIP/graphme1.html http://cuisg13.unige.ch:8100/HomePage.html http://ligsg2.epfl.ch/ http://ls7-www.informatik.uni-dortmund.de/ at: http://www.dgp.toronto.edu/OtherLabs.html gopher://ftp.inria.fr:71/11/Labs http://ls7-www.informatik.uni-dortmund.de/html/englisch/servers.html there are other lists of CG labs The correct address for Leuwen is: http://www.cs.kuleuven.ac.be/cwis/research/graphics/graphics-E.shtml sincerely, Werner From X-POP3-Rcpt: wp@stellaris Received: from merckx.graphics.cornell.edu by stellaris.cg.tuwien.ac.at via SMTP (940816.SGI.8.6.9/910805.SGI) for id NAA17077; Wed, 22 Nov 1995 13:38:57 +0100 Received: by merckx.graphics.cornell.edu (5.65/DEC-Ultrix/4.3) id AA03325; Wed, 22 Nov 1995 07:38:53 -0500 Message-Id: <9511221238.AA03325@merckx.graphics.cornell.edu> Received: by barn.graphics.cornell.edu (1.37.109.8/16.2) id AA11989; Wed, 22 Nov 1995 07:38:49 -0500 From: Peter Shirley Subject: Re: graphics pages To: Werner Purgathofer Werner Purgathofer Date: Wed, 22 Nov 95 7:38:49 EST In-Reply-To: ; from "Werner Purgathofer" at Nov 22, 95 8:47 am Mailer: Elm [revision: 70.85] X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Wow! Thanks-- I will add these. Pete > > >I am updating my list of graphics pages at: > > > >http://www.graphics.cornell.edu/~shirley/graphics.html > > > >If you know of any I should add, please let me know. > > Dear Pete, > > here are some additional CG labs: > > http://www.fsz.bme.hu/~szirmay > http://www.sys.uea.ac.uk/Research/ResGroups/CGP/ > http://korsika.informatik.uni-rostock.de:8080/ > http://sgi.felk.cvut.cz/index.html > http://www.inf.ethz.ch/department/IS/cg/ > http://www.cs.uml.edu/~haim/ivpr.html > http://www.igd.fhg.de/ > http://www9.informatik.uni-erlangen.de/ > http://greco.gris.informatik.uni-tuebingen.de/ > http://www.susx.ac.uk/engg/research/vlsi/vlsi.htm > http://www.comp.brad.ac.uk/research/GIP/graphme1.html > http://cuisg13.unige.ch:8100/HomePage.html > http://ligsg2.epfl.ch/ > http://ls7-www.informatik.uni-dortmund.de/ > > at: > http://www.dgp.toronto.edu/OtherLabs.html > gopher://ftp.inria.fr:71/11/Labs > http://ls7-www.informatik.uni-dortmund.de/html/englisch/servers.html > there are other lists of CG labs > > The correct address for Leuwen is: > http://www.cs.kuleuven.ac.be/cwis/research/graphics/graphics-E.shtml > > sincerely, > Werner > > > > -- > |""""""""""""""""""""""""""""""""|"""""""""""""""""""""""""""""""""| > | Werner Purgathofer | Tel. +43(1)58801 4548 | > | Institute of Computer Graphics | ( secretary: 4549 ) | > | Technical University of Vienna | Fax. +43(1)5874932 | > | Karlsplatz 13 / 186 | email: wp@cg.tuwien.ac.at | > | A-1040 Wien / Austria | WWW: http://www.cg.tuwien.ac.at | > """""""""""""""""""""""""""""""""""""""""""""""""""""""""""""""""""" > > > From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id SAA04443; Tue, 5 Dec 1995 18:43:19 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id QAA08880 for ; Tue, 5 Dec 1995 16:02:57 +0100 Received: from dira.bris.ac.uk (dira.bris.ac.uk [137.222.10.41]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id QAA12304 for ; Tue, 5 Dec 1995 16:02:47 +0100 Received: from kukini.cs.bris.ac.uk by dira.bris.ac.uk with SMTP (PP); Tue, 5 Dec 1995 15:02:05 +0000 Received: from danno by kukini.compsci.bristol.ac.uk id aa09807; 5 Dec 95 15:04 GMT To: globillum@imag.fr Subject: participating media Cc: blacksha@cs.bris.ac.uk Date: Tue, 5 Dec 95 14:59:16 GMT From: blacksha@cs.bris.ac.uk Sender: blacksha@cs.bris.ac.uk Message-ID: <9512051459.aa26006@uk.ac.bristol.compsci.danno> X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Dear all, I am a final year student investigating the visualisation of participating media using the particle tracing method. I would be most grateful if anyone could point me in the right direction as to where i might find a description of the properties, and how they might be modelled, of media such as fog & rain, smoke and dust. many thanks, Julian Blackshaw. Email: blacksha@compsci.bristol.ac.uk From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id UAA04711; Tue, 5 Dec 1995 20:55:02 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id UAA25958 for ; Tue, 5 Dec 1995 20:39:01 +0100 Received: from irz101.inf.tu-dresden.de (irz101.inf.tu-dresden.de [141.76.1.9]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id UAA22835 for ; Tue, 5 Dec 1995 20:38:57 +0100 Received: by irz101.inf.tu-dresden.de (8.6.12/8.6.12-s1) id VAA00521 for globillum@imag.fr; Tue, 5 Dec 1995 21:38:51 +0200 From: "Nguyen, D.C." Message-Id: <199512051938.VAA00521@irz101.inf.tu-dresden.de> Subject: GX/GENERIC page To: Global Illumination List Date: Tue, 5 Dec 1995 21:38:51 +0200 (MESZ) X-Mailer: ELM [version 2.4 PL23] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hi, I've uploaded the GX/GENERIC WWW-page w/ some demos picts and performance-reports. The URLs are: http://www.inf.tu-dresden.de/~cn1/gx.html or http://www.rz.tu-ilmenau.de/~juhu/gx.html -JuHu /\__ Nguyen Duc Cuong (aka JuHu) - CG-student \ "Computers in the future may /__\ \ EMail : cn1@irz.inf.tu-dresden.de \ weigh no more than 1.5 tons" \__/ WWW : http://www.inf.tu-dresden.de/~cn1/ \[ Popular Mechanics 1949 ] From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id TAA04384; Tue, 12 Dec 1995 19:03:38 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id NAA18936 for ; Tue, 12 Dec 1995 13:35:35 +0100 Received: from alf2.tcd.ie (alf2.tcd.ie [134.226.1.26]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id NAA04078 for ; Tue, 12 Dec 1995 13:35:28 +0100 Received: (from vtcodd@localhost) by alf2.tcd.ie (8.6.10/8.6.10) id MAA21590 for globillum@imag.fr; Tue, 12 Dec 1995 12:35:15 GMT From: Vinnie Codd Message-Id: <199512121235.MAA21590@alf2.tcd.ie> Subject: RE:Radiosity To: globillum@imag.fr Date: Tue, 12 Dec 1995 12:35:14 +0000 (GMT) X-Mailer: ELM [version 2.4 PL23] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hello there, I wonder could anyone give me information on Radiosity. I would like information on where to get code to implement the radiosity algorithm eg ftp sites.My project entails solving the radiosity equation for a cubical room with a light source at the centre of the roof and a cube at the centre of the floor.I am using ray-tracing for form factor evaluation and for the final viewing phase.I am using progresive refinement to solve the equation itself.I wonder could anyone give me some information as to where to find code or anything else helpfull for this problem. Vincent Codd(vtcodd@alf2.tcd.ie) From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id TAA04430; Tue, 12 Dec 1995 19:13:03 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id PAA24380 for ; Tue, 12 Dec 1995 15:12:13 +0100 Received: from sbox.tu-graz.ac.at (dialup6.tu-graz.ac.at [129.27.250.7]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id PAA08491 for ; Tue, 12 Dec 1995 15:12:07 +0100 Received: (from sw@localhost) by sbox.tu-graz.ac.at (8.6.12/8.6.9) id PAA00504; Tue, 12 Dec 1995 15:48:12 +0100 Date: Tue, 12 Dec 1995 15:48:08 +0100 (MET) From: Siegfried Wiesenhofer To: globillum@imag.fr Subject: nomenclature recommendation ? Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII; format=flowed X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit hi, i' m currently working on my diploma thesis on "numerical simulation of radiation heat transfer". having finished the implementation part i recently started committing the work to paper. now my question: which nomenclature should i use ? heat transfer or global illumination (proposed standard, or ANSI/IES RP-16-1986) ? i am torn between using nomenclature from siegel's & howell's book "thermal radiation heat transfer" (which i think is a standard work on radiative heat transfer), global illumination literature, and the proposed standard for global illumination. any recommendations ? many thanx in advance, siegi <<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<< v siegfried wiesenhofer ^ v graz university of technology / austria - europe ^ v keywords: siegi, radiosity, jazz, funk, paragliding... ^ v email: sw@sbox.tu-graz.ac.at ^ >>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>> From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id UAA04860; Tue, 12 Dec 1995 20:42:23 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id UAA11378 for ; Tue, 12 Dec 1995 20:14:44 +0100 Received: from lbl.gov (lbl.gov [128.3.254.23]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id UAA24418 for ; Tue, 12 Dec 1995 20:14:10 +0100 Received: from hobbes.lbl.gov by lbl.gov (4.1/1.39) id AA10568; Tue, 12 Dec 95 11:13:41 PST Received: by hobbes.lbl.gov (3.2/SMI-3.2) id AA11547; Tue, 12 Dec 95 11:12:59 PST Date: Tue, 12 Dec 95 11:12:59 PST From: "Gregory J. Ward" Message-Id: <9512121912.AA11547@hobbes.lbl.gov> To: globillum@imag.fr, vtcodd@tcd.ie Subject: RE:Radiosity X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Sounds like you want Ian Ashdown's book: Ashdown, I. 1994. Radiosity: A Programmer's Perspective. New York, NY: John Wiley & Sons, Inc. Softcover, 498 pages, 12 color plates. ISBN 0-471-30444-1 (without diskette) $44.95 US ISBN 0-471-30488-3 (with 3.5-inch MS-DOS diskette) $59.95 US A demo version of his radiosity implementation, called HELIOS, is available from the Ledalite web site: http://www.ledalite.com/ He has also written a nice IES luminaire file parser, which I recommend to anyone who is serious about realistic rendering, available from the same site. If you want some good, physically-based models and solutions to compare to, also check out the following site, which I manage: http://radsite.lbl.gov/mgf/HOME.html Good luck! -Greg From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id UAA04878; Tue, 12 Dec 1995 20:48:20 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id UAA11493 for ; Tue, 12 Dec 1995 20:25:25 +0100 Received: from lbl.gov (lbl.gov [128.3.254.23]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id UAA24930 for ; Tue, 12 Dec 1995 20:25:23 +0100 Received: from hobbes.lbl.gov by lbl.gov (4.1/1.39) id AA10884; Tue, 12 Dec 95 11:24:25 PST Received: by hobbes.lbl.gov (3.2/SMI-3.2) id AA11599; Tue, 12 Dec 95 11:23:43 PST Date: Tue, 12 Dec 95 11:23:43 PST From: "Gregory J. Ward" Message-Id: <9512121923.AA11599@hobbes.lbl.gov> To: globillum@imag.fr, sw@sbox.tu-graz.ac.at Subject: Re: nomenclature recommendation ? X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit I recommend that you pick up the following files by Holly Rushmeier from the anonymous ftp account on tiber.nist.gov: pub/holly/symb.tex - LaTeX document pub/holly/symb.ps - printable PostScript of above This summarizes recommended notation from ANSI/IES RP-16-1986, which is the preferred standard for global illumination. Even if you are working within the field of radiative heat transfer, this is a more consistent notation for a broader audience. (Someone, correct me if I'm mistaken.) -Greg P.S. A group of us are still hoping to come up with some standard terminology and put it on the globillum web page, but we're a bit slow. From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id KAA18022; Fri, 15 Dec 1995 10:58:25 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id KAA06430 for ; Fri, 15 Dec 1995 10:10:38 +0100 Received: from relay7.UU.NET (relay7.UU.NET [192.48.96.17]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id KAA20728 for ; Fri, 15 Dec 1995 10:10:29 +0100 Received: from iisc.ernet.in by relay7.UU.NET with SMTP id QQzueu27049; Fri, 15 Dec 1995 04:09:35 -0500 (EST) Received: from serc.serc.iisc.ernet.in (dhruva.serc.iisc.ernet.in) by iisc.ernet.in (ERNET-IISc/SMI-4.1) id AA19904; Fri, 15 Dec 95 14:44:49+0530 Received: by serc.serc.iisc.ernet.in (AIX 3.2/UCB 5.64/4.03) id AA11191; Fri, 15 Dec 1995 14:43:38 GMT Date: Fri, 15 Dec 1995 14:43:38 GMT From: Reetinder Singh Sidhu Message-Id: <9512151443.AA11191@serc.serc.iisc.ernet.in> To: globillum@imag.fr Subject: Analytical Form Factors X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Would anyone know the analytic form factor from a differential area to a triangle? I need the formulae for the two cases when the diff. area and the triangle are (1) parallel (2) perpendicular. My aplogies for bothering about such a trivial matter but time is too short for me to work it out and verify it. Reetinder Sidhu From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id RAA25772; Thu, 4 Jan 1996 17:14:58 +0100 Received: from haven.uniserve.com (haven.uniserve.com [198.53.215.121]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id PAA05326 for ; Thu, 4 Jan 1996 15:30:17 +0100 Received: from van0118.TVS.NET ([204.191.197.28]) by haven.uniserve.com with SMTP id <30746-4>; Thu, 4 Jan 1996 06:28:01 -0000 X-Sender: iashdown@ledalite.com (Unverified) X-Mailer: Windows Eudora Version 2.0.3 Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed To: globillum@imag.fr From: Ian Ashdown Subject: Radiosity & Color Quantization bibliographies Message-Id: <96Jan4.062801pst.30746-4+426@haven.uniserve.com> Date: Thu, 4 Jan 1996 06:27:56 -0000 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Revised and new bibliography releases for: * radiosity and global illumination * color quantization algorithms * edge-based (e.g., winged-edge) boundary representations 1. RADBIB96.TXT This is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. A total of 49 new references have been added since its last release as RADBIB95.TXT on November 11, 1995, bringing the total to 832 references. Available as RADBIB96.ZIP or RADBIB96.TXT.Z from http://www.ledalite.com/library/rrt.html (courtesy of Ledalite Architectural Products Inc.) Also available as /pub/doc/RadBib96.Z from hobbes.lbl.gov (courtesy of Greg Ward and Lawrence Berkeley Laboratory). This bibliography is in refer format. However, some anonymous but kind soul converted the previous release to bib format, which is available as: ftp.cs.columbia.edu/archives/bibliographies/Graphics/rad.html A refer-format file containing only the new references for RADBIB96.TXT is also available. Send your e-mail request to iashdown@ledalite.com. 2. CQUANT96.TXT This is a comprehensive bibliography of color quantization algorithms. A total of 6 new references have been added since its last release as CQUANT95.TXT on November 11, 1995, bringing the total to 91 references. Available as CQUANT96.ZIP or CQUANT96.TXT.Z from http://www.ledalite.com/library/cgis.html (courtesy of Ledalite Architectural Products Inc.) Also available as /pub/doc/cquant96.Z from hobbes.lbl.gov (courtesy of Greg Ward and Lawrence Berkeley Laboratory). 3. B-REP96.TXT This is a bibliography of edge-based boundary representation papers, theses, articles, and books, and includes 39 references. If you are having trouble locating information on Baumgart's winged-edge data structure for radiosity-based rendering and other finite element method applications, start here. Available as B-REP96.ZIP or B-REP96.TXT.Z from http://www.ledalite.com/library/cgis.html (courtesy of Ledalite Architectural Products Inc.) Also available as /pub/doc/brep96.Z from hobbes.lbl.gov (courtesy of Greg Ward and Lawrence Berkeley Laboratory). My thanks to all of you who have made your conference proceedings, publication lists, and especially papers available online through your Web pages. It has made my self-appointed task of tracking down your contributions to the global illumination literature much easier. Ian Ashdown, P. Eng. | READ THE BOOK! Research & Development Manager | Radiosity: A Programmer's Perspective Ledalite Architectural Products Inc. | by Ian Ashdown | John Wiley & Sons, 1994 Visit http://www.ledalite.com | (Sneaky Internet Advertising) From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id AAA27792; Thu, 8 Feb 1996 00:25:15 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id AAA12422 for ; Thu, 8 Feb 1996 00:03:44 +0100 Received: from augustea.it (jupiter.augustea.it [194.20.105.1]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id AAA18410 for ; Thu, 8 Feb 1996 00:03:39 +0100 Received: from ppp-7.augustea.it (ppp-5.augustea.it) by augustea.it with SMTP id AA05841 (5.67b/IDA-1.5 for ); Thu, 8 Feb 1996 00:02:54 +0100 Message-Id: <30F0D822.4965@jupiter.augustea.it> Date: Mon, 08 Jan 1996 00:38:58 -0800 From: Paolo Bernardelli Organization: Poliedra X-Mailer: Mozilla 2.0b6a (Win16; I) Mime-Version: 1.0 To: globillum@imag.fr Subject: Materials definition for esterior lighting simulation Content-Type: text/plain; charset=windows-1252; format=flowed Content-Transfer-Encoding: 8bit X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 For radiosity people ..... Im studing about illumination conditions of monuments and building in exterior and thier visual effect. For this we use Radiance and we need to define some quantity of materials like especially: >plaster >smooth marble ( like white marble called Travertino - All Rome is built with this ) >ashlar marble >wood for windows >nude reinforced concrete >pavement street Where is it possible find this informations with a physical definition ( Like BRDF materials and MGF standard )? As your gruop ingaged this problems? How measure you materials color and unknown elements of materials? Thanks for your attention. Paolo Bernarderlli From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id VAA19719; Tue, 6 Feb 1996 21:48:54 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id VAA14488 for ; Tue, 6 Feb 1996 21:28:24 +0100 Received: from akbar.psc.edu (akbar.psc.edu [128.182.61.69]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id VAA29240 for ; Tue, 6 Feb 1996 21:28:19 +0100 Received: by akbar.psc.edu (950911.SGI.8.6.12.PATCH825/930416.SGI.AUTO) id KAA20392; Tue, 6 Feb 1996 10:00:28 -0500 Date: Tue, 6 Feb 1996 10:00:28 -0500 From: Joe Geigel Message-Id: <199602061500.KAA20392@akbar.psc.edu> To: radiance-discuss@hobbes.lbl.gov, globillum@imag.fr Subject: Looking for accurate illumination/BRDFs Reply-to: geigel@psc.edu X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Hello... I am conducting an experiment, in the spirit of the studies with the Cornell box, where I will be comparing a computer rendered scene (rendered with RADIANCE) with an equivalent scene in the real world. As such, I will need to find luminarires and materials in the real world whose physical data is accurately recorded and generally available. I was wondering if anyone can recommend any particular luminaires whose illumination data is available (and considered accurate) and/or materials whose BRDF data is available (and also accurate) and where I might obtain such data. Any help or pointers would be greatly appreciated. Thanks in advance, -- joe geigel pittsburgh supercomputing center geigel@psc.edu From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id WAA28594; Tue, 13 Feb 1996 22:28:12 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id VAA10931 for ; Tue, 13 Feb 1996 21:56:25 +0100 Received: from irz201.inf.tu-dresden.de (irz201.inf.tu-dresden.de [141.76.1.10]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id VAA17438 for ; Tue, 13 Feb 1996 21:56:04 +0100 Received: by irz201.inf.tu-dresden.de (8.6.12/8.6.12-s1) id WAA07103 for globillum@imag.fr; Tue, 13 Feb 1996 22:54:15 +0200 From: "Nguyen, D.C." Message-Id: <199602132054.WAA07103@irz201.inf.tu-dresden.de> Subject: shadow boundaries for ext. lights To: Global Illumination List Date: Tue, 13 Feb 1996 22:54:14 +0200 (MESZ) X-Mailer: ELM [version 2.4 PL24 ME8b] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hi, Is there any general (not only polygonal) approach to compute the shadow boundaries for volume-lightsoures ? I use Monte-Carlo-technique to compute softshadows and got many problems w/ it. Even with importance sampling, the raytracer requires a lot of shadow-rays to fire to produce an acceptable image. There are too much noises, and some small occluding patches are missed. An analytical solution would be nice, but i only found papers where special solutions for polygonal objects are described. Is it possible to contruct the discontinuity mesh for all types of objects ? Thanks for any help. --JuHu /\__ Nguyen Duc Cuong (aka JuHu) - CG-student \ "Computers in the future may /__\ \ EMail : cn1@irz.inf.tu-dresden.de \ weigh no more than 1.5 tons" \__/ WWW : http://www.inf.tu-dresden.de/~cn1/ \[ Popular Mechanics 1949 ] From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id TAA20374; Sat, 17 Feb 1996 19:45:02 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id TAA02590 for ; Sat, 17 Feb 1996 19:26:38 +0100 Received: from haven.uniserve.com (haven.uniserve.com [198.53.215.121]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id TAA11391 for ; Sat, 17 Feb 1996 19:25:13 +0100 Received: from van0102.TVS.NET ([204.191.197.12]) by haven.uniserve.com with SMTP id <30821-24133>; Sat, 17 Feb 1996 10:27:55 -0800 X-Sender: iashdown@ledalite.com X-Mailer: Windows Eudora Version 2.0.3 Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed To: globillum@imag.fr From: Ian Ashdown Subject: ANNOUNCE: Free Radiosity Renderer (inc. C++ source code) Message-Id: <96Feb17.102755pst.30821-24133+279@haven.uniserve.com> Date: Sat, 17 Feb 1996 10:27:55 -0800 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hi, folks. My apologies for cluttering up your mailbox, but rumour has it that some of you (or, more likely, your undergrad students) are actually using the HELIOS radiosity renderer from my book. The following is a self-serving blurb announcing that the complete (and guaranteed 100% free) C++ development package for HELIOS V1.02C is now available for downloading from our Web server. - Ian Ashdown ---------------------------------------------------------------- The C++ source code for HELIOS, a fully-functional radiosity renderer for MS-Windows 3.1, is now available for downloading on the 'net ... "Radiosity" is a computer graphics technique that enables you to synthesize photorealistic images. Whereas ray tracing techniques excel in the rendition of point light sources, specular reflections, and refraction effects, radiosity methods accurately model area light sources, diffuse reflections, color bleeding between surfaces, and detailed shading within shadows. They are in a sense complementary approaches to photorealistic rendering. Folklore had it that you needed a graphics workstation with gigabytes of RAM or even a supercomputer to do radiosity rendering. This is no longer true: You can use your personal desktop computer -- a '386 IBM-PC with a math coprocessor, 4 MB of RAM, and a 256-color SVGA display will do nicely -- to experiment with radiosity methods. A 66-MHz '486DX machine will render a simple scene (540 polygons) in less than three minutes. A more complex scene with 2,700 polygons can be rendered in a little over six minutes. Commercial radiosity renderers are slowly making their way into the marketplace. Take a look, for example, at the incomparable Lightscape Visualization system (http://www.lightscape.com) to see what is available now for Windows NT. (Other interesting sites on the Web for commercial radiosity renderers are http://www.bentley.com/products/masterpiece.html -- download the Microstation MasterPiece Technical Profile -- and the Italian http://www.atma.it/english/rlight.html.) In the meantime, you can download HELIOS to experiment with the possibilities of radiosity rendering using MS-Windows 3.1 or Windows 95. The Web site is: http://www.ledalite.com/lighthouse.html where you will find a demonstration version of HELIOS Version 1.02C (106 KB) and the complete C++ development package (806 KB), including four different executable versions of HELIOS, fully- commented C++ source code (over 12,700 lines), make files for Microsoft Visual C++ 1.5 and Borland C++ 4.5, online help files, two demonstration environments, demo images, and more. (While you are perusing our Web site, you might want to look at http://www.ledalite.com/library/ledapub.html -- we have an eclectic variety of academic papers and articles on computer graphics and related topics available online for downloading.) The HELIOS development package is *not* in the public domain. It is copyrighted material that may be freely copied, redistributed, and/or modified for personal, non-commercial use ONLY, provided the copyright notice is included with all source code files. HELIOS was first developed in: Ashdown, I. 1994. Radiosity: A Programmer's Perspective. New York, NY: John Wiley & Sons, Inc. Softcover, 498 pages, 12 color plates. ISBN 0-471-30444-1 (without diskette) $39.95 US ISBN 0-471-30488-3 (with 3.5-inch MS-DOS diskette) $54.95 US This book provides a detailed explanation of radiosity theory and its associated algorithms (no knowledge of higher mathematics required!) More important, it also includes complete, fully documented, and compiler-independent C++ source code (over 7,500 lines) for HELIOS Version 1.00A, a fully-functional radiosity- based rendering program for MS-Windows 3.1, Windows 95, and Windows NT. The radiosity-related code presented in the book is identical to that now offered online. If you want to fully understand how HELIOS (and radiosity) works, you more or less need to buy the book. You can order "Radiosity: A Programmer's Perspective" from your local bookseller or (in the United States) directly from John Wiley & Sons by calling 1-800-CALL-WILEY. You can also order the book online from http://www.wiley.com. Ian Ashdown, P. Eng. | READ THE BOOK! Research & Development Manager | Radiosity: A Programmer's Perspective Ledalite Architectural Products Inc. | by Ian Ashdown | John Wiley & Sons, 1994 Visit http://www.ledalite.com | (Sneaky Internet Advertising) From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id EAA21635; Sun, 18 Feb 1996 04:13:21 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id EAA06659 for ; Sun, 18 Feb 1996 04:03:50 +0100 Received: from haven.uniserve.com (haven.uniserve.com [198.53.215.121]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id EAA17560 for ; Sun, 18 Feb 1996 04:03:48 +0100 Received: from van0105.TVS.NET ([204.191.197.15]) by haven.uniserve.com with SMTP id <30977-24130>; Sat, 17 Feb 1996 19:06:43 -0800 X-Sender: iashdown@ledalite.com X-Mailer: Windows Eudora Version 2.0.3 Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed To: globillum@imag.fr From: Ian Ashdown Subject: ANNOUNCE corrigendum Message-Id: <96Feb17.190643pst.30977-24130+549@haven.uniserve.com> Date: Sat, 17 Feb 1996 19:06:38 -0800 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Corrigendum to earlier message: >In the meantime, you can download HELIOS to experiment with the >possibilities of radiosity rendering using MS-Windows 3.1 or >Windows 95. The Web site is: > > http://www.ledalite.com/lighthouse.html > Oops ... make that http://www/ledalite.com/lighthse.html Ian Ashdown, P. Eng. | READ THE BOOK! Research & Development Manager | Radiosity: A Programmer's Perspective Ledalite Architectural Products Inc. | by Ian Ashdown | John Wiley & Sons, 1994 Visit http://www.ledalite.com | (Sneaky Internet Advertising) From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id WAA12477; Wed, 21 Feb 1996 22:00:34 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id VAA28605 for ; Wed, 21 Feb 1996 21:24:01 +0100 Received: from gateway.lightscape.com (gate-gateway.lightscape.com [206.139.79.2]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id VAA16678 for ; Wed, 21 Feb 1996 21:23:40 +0100 Received: from junior.lightscape.com by gateway.lightscape.com via ESMTP (950511.SGI.8.6.12.PATCH526/940406.SGI.AUTO) for <@gateway.lightscape.com:globillum@imag.fr> id MAA00578; Wed, 21 Feb 1996 12:23:04 -0800 Received: from basil.lightscape.com by junior.lightscape.com via ESMTP (950511.SGI.8.6.12.PATCH526/940406.SGI.AUTO) for <@junior.lightscape.com:globillum@imag.fr> id MAA15774; Wed, 21 Feb 1996 12:23:04 -0800 Received: from basil by basil.lightscape.com via SMTP (940816.SGI.8.6.9/940406.SGI.AUTO) for id MAA17837; Wed, 21 Feb 1996 12:23:02 -0800 Sender: greg@lightscape.com Message-ID: <312B7F26.6956@lightscape.com> Date: Wed, 21 Feb 1996 12:23:02 -0800 From: Greg Spencer Organization: Lightscape Technologies, Inc. X-Mailer: Mozilla 2.0b6a (X11; I; IRIX 5.3 IP22) MIME-Version: 1.0 To: globillum@imag.fr Subject: Caught in the Act X-URL: http://www.3d-design.com/bruno/bruno.html Content-Type: text/plain; charset=windows-1252; format=flowed X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit I just thought I would provide a bit of appropriate humor to this list. If you would like a good laugh, read the following article on lighting from 3D Design magazine -- it's a wonderful example of how to sound technical without actually having to know anything about the subject you are writing about (or even much about writing). http://www.3d-design.com/bruno/bruno.html -Greg. -- Greg Spencer, Software Engineer Lightscape Technologies., Inc. Caught in the Shadows

Caught in the Shadows

by Joey Bruno

Even the most stunning 3D models are useless without light sources. Put these tips, tricks, and hands-on techniques to the test to get the most from your light sources.

The notion of lighting a 3D scene seems rather simplistic, but it's not. Consider the many ways that shadows are created in 3D programs -- from a simple, single light source to special effect shots with uplighting, whirling spotlights, and laser bolts flying freely. And these effects are not limited to the higher-end workstations or software -- 3D packages selling for as little as $500 offer the ability to create lighting and shadow effects.

So what's the big deal? Why all the fuss about lighting a scene and simulating shadows? Sure you can build some geometry, throw a shadow-casting light source or two in and render away. But if you think that's all there is to it, think again. If your goal is to add realism to your design but you neglect to spend the time setting up the lights within it, you're all but asking for trouble. When it gets down to the final scene, it won't matter that your geometry is perfect or that you've included more special effects than a sci-fi movie. If your lighting and shadows are sloppy, people will notice.

Understand the shadows

A shadow is not a hard, razor-edged entity, nor is it an absolute absence of light. Shadows are created by blocking the in-line flow of light from an object, which can be caused by refraction, diffusion, or complete blockage. Consider for a moment how light itself works. Light does not cast a perfectly straight beam -- it projects in all directions from its source. This scattering effect is referred to as "propagation." Rays of light run three-dimensionally in a radial fashion from their sources. Close to the source, the rays are densely packed. As they move out, they disperse. That's why the effect of light gets weaker the further it moves from its source.

Consider how propagation affects an object. What do these radial light waves do when they strike an object? How about when light waves strike light waves or light waves interact with atmospheric diffusion? The physics get complicated, but in a nutshell, it produces scatter. When light strikes an object, especially the face of an object perpendicular to its source, it "kicks" the light back in the same direction as its source, causing reflections in an object. The greater an object's ability to return this light without interference from its surface characteristics (i.e., less returned diffusion), the shinier it is.

Light rays reach a breaking point at the edge of an object. Edges that are jutting out in space tend to "slice" the beam; part of the beam will strike the object and other parts of the beam will scatter. This scattering light must go somewhere. The energy of the light will tend to make it continue in the direction it was originally traveling. However, it may be a bit off-course because of a diffusion material (probably atmosphere).

The important thing to remember is the energy factor involved. The more energy the photon of light has, the more it will tend to stay on course after diffusion. Remember also that light waves are more dense and compact near their source.

Imagine that you have a crate sitting in a large room and a single light source at the far end of that room. The room should be fairly well lit near the light and the crate should cast somewhat of a shadow. However, this shadow will probably be more of a negative highlight effect with a roughly definable outline of the crate on the floor. Now move the crate closer to the light. The shadow edge will become more defined as you approach the light. because the photons of light are stronger, they tend to travel more closely toward their original path in a straight line. Also, depending on the amount of scattered light in the room, the shadow will have more depth and contrast to the rest of the scene as it approaches the light source.

Prepare yourself

Now, let's talk about 3D models and how to apply some of these techniques to them. First of all, it is a great temptation to make shadows razor-edged with 3D software -- besides, it's a neat effect. 3D lighting and objects tend to be "perfect" in their interaction, which means lights can be absolute, without diffusion or drop off, and have pure color saturation.

Some software packages can help to minimize this temptation by offering raytraced shadows. Raytracing allows the shadowing effects to behave in a more natural (light bouncing) fashion. As long as you don't go crazy with lights and wash everything out, you'll be okay. The problem with creating raytraced shadows on a PC is that the renderings take so long to produce. For a still shot it's not a big deal, but incorporating raytrace rendering into an animation (even a small one) can become a nightmare. Therefore, it's wise to use regular shadows for animation and reserve raytracing for stills. Besides, animation tends to minimize any "goofs" you make in setting up your lights and shadows.

Whether your software has the ability to create raytraced shadows or not, the following can help minimize the effects of improperly used lights and shadows:

ï Plan your shots and decide where lights and (especially) shadows are going to play a role. Don't worry about the shadows on "the other side of that mountain" or "building" unless you're going to be visiting it at some point.

ï Use a variety of lights. Don't make the mistake of using a single, pinpoint light source as the sun or broad daylight. Use a nice, even, ambient lighting set-up and place spotlights for shadows on objects that need them. The exception to this is architectural renderings. These renderings have traditionally been done a certain way, with hard-edged, single-source lighting. It's a matter of tradition over accuracy. However, do offer your clients the choice of both. They might surprise you and break tradition a bit if you can show them good reason.

ï Don't forget about diffusion and remember that light scatters. Go ahead and let your scene have razor sharp edges in its shadows. Now, go to the opposite end of the scene and add a contrasting fill light. Bring the level of the fill light up until you get a nice "washing" effect in the shadows. This is a very realistic effect if done properly and will give you results almost identical to raytracing.

If your software has the ability to project images with a light source (a movie projector of sorts) and you can make matte objects (objects that don't render, yet still affect the scene), try this. Set up all of your lights, then matte out all the objects in the scene. Render from the top and record all the shadows where they strike the ground. Take this image into a paint program and apply some effects to it over time, using the same number of frames that your animation will have. Now take all the lights out of your scene except for one big fill light (an omni light works great for this since it creates good highlights), bring all the objects back so they will render, project your shadow effect from above and move your fill light around. Depending on what you did in the paint program and how you move your fill light, you can make shadows "fall" backwards, which makes all the shadows dissolve into a whirlpool or simply transform into flowers. It's strange, but can be a very neat effect.

And, finally...

Read up on how lighting works. Check out some good books on theatrical lighting from the library or go to a good modeling/hobby shop and pick up a book or two on photographing model railroads. Some of the techniques in these books are pure genius and are easily applied to computer generated graphics.

Or turn to film for inspiration. Watch some old black and white movies or look at some old photos or stills. Movie makers of the past didn't have the luxury of color to give their scenes depth or definition. Take another look at cinema classics like Citizen Kane or Gaslight to see how shadows become a part of the storyline. Make note of the contrasts created using lights and shadows and take the techniques of yesteryear to work with you today.

Joey Bruno has been doing multimedia consulting for more than five years and is the founder of Image One, a multimedia consulting group based in Birmingham, AL. Joey also teaches 3D Studio and multimedia at Virginia College in Birmingham. He can be reached electronically at 102712.107@compuserve.com via the Internet.

From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id XAA24871; Wed, 28 Feb 1996 23:49:21 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id XAA29827 for ; Wed, 28 Feb 1996 23:16:46 +0100 Received: from fs1.cam.nist.gov (fs1.cam.nist.gov [129.6.80.33]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id XAA23726 for ; Wed, 28 Feb 1996 23:16:44 +0100 Received: from plum (plum.cam.nist.gov) by fs1.cam.nist.gov (4.1/SMI-DDN) id AA16176; Wed, 28 Feb 96 17:16:40 EST Received: by plum (950911.SGI.8.6.12.PATCH825/SMI-3.2) id RAA15220; Wed, 28 Feb 1996 17:16:35 -0500 From: "Holly E Rushmeier" Message-Id: <9602281716.ZM15218@plum.cam.nist.gov> Date: Wed, 28 Feb 1996 17:16:34 -0500 Reply-To: holly.rushmeier@nist.gov X-Face: eO|V;3{XkGh^/1hW"\R$2ajo-]{6b+iSL&s}264L"[Qr(@>+$'c"p(xid20x|DKhrQ-OZw#!/6;*ny_NU>tEA4Z#p5~.hbz)nL990=A^Z/88}i]; Thu, 14 Mar 1996 22:59:14 +0100 Received: from UX3.SP.CS.CMU.EDU (UX3.SP.CS.CMU.EDU [128.2.198.103]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id WAA20046 for ; Thu, 14 Mar 1996 22:59:12 +0100 Received: from GS190.SP.CS.CMU.EDU by UX3.SP.CS.CMU.EDU id aa04306; 14 Mar 96 16:58 EST X-Sender: ajw@a.gp.cs.cmu.edu Message-Id: Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed Date: Thu, 14 Mar 1996 16:58:28 -0500 To: globillum@imag.fr From: "Andrew J. Willmott" Subject: Triangular surface elements for wavelet radiosity X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Has anyone else out there implemented wavelet radiosity using triangular patches? Specifically, Flatlets and Multiwavelets. There seem to be a number of different ways to approach the various parts of the problem, and it would be interesting to compare our approach with any others that exist. Cheers, Andrew --- mailto:a.willmott@cs.cmu.edu ------- http://www.cs.cmu.edu/~ajw --- From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id TAA09206; Sun, 17 Mar 1996 19:18:17 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id SAA11408 for ; Sun, 17 Mar 1996 18:55:15 +0100 Received: from merckx.graphics.cornell.edu (MERCKX.GRAPHICS.CORNELL.EDU [128.84.247.147]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id SAA17054 for ; Sun, 17 Mar 1996 18:55:13 +0100 Received: by merckx.graphics.cornell.edu (5.65/DEC-Ultrix/4.3) id AA22776; Sun, 17 Mar 1996 12:55:10 -0500 Message-Id: <9603171755.AA22776@merckx.graphics.cornell.edu> Received: by barn.graphics.cornell.edu (1.37.109.8/16.2) id AA23202; Sun, 17 Mar 1996 12:54:38 -0500 From: Peter Shirley Subject: Will anyone send me this paper? To: globillum@imag.fr Date: Sun, 17 Mar 96 12:54:38 EST Mailer: Elm [revision: 70.85] X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Lately my students and I have been working on approximating light flow in volumes. Reviewers have said that we should reference the Toronto work of the late 80s: Drettakis, et. al, "Titghly coupled multiprocessing for a Global Illumination Algroithm", pp. 387-398, Eurographics '90. And Fournier, et. al, "FIAT LUX: Light Driven Global Illumination", DGP Technical Memo DGP89-1, 1989. I would love to, but I have not read them. AF has given me a high-level idea of the work, but I would love to get hold of the real papers. If anyone is willing to help me, please send copies to: Pete Shirley Program of Computer Graphics 580 Rhodes Hall Cornell University Ithaca, NY 14853 USA Thanks! Pete PS-- are old Eurographics proceedings (pre 1991) available? From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id XAA09864; Sun, 17 Mar 1996 23:51:43 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id XAA13452 for ; Sun, 17 Mar 1996 23:40:03 +0100 Received: from explorer.dgp.toronto.edu (explorer.dgp.toronto.edu [128.100.1.129]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id XAA21686 for ; Sun, 17 Mar 1996 23:39:56 +0100 Received: by explorer-en.dgp.toronto.edu id <144010>; Sun, 17 Mar 1996 17:38:44 -0500 In-Reply-To: Peter Shirley's message as of Mar 17, 1:17pm X-Mailer: Mail User's Shell (7.2.3 5/22/91) From: Eugene Fiume To: Peter Shirley , globillum@imag.fr Subject: Re: Will anyone send me this paper? Message-Id: <96Mar17.173844est.144010@explorer-en.dgp.toronto.edu> Date: Sun, 17 Mar 1996 17:38:36 -0500 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit On Mar 17, 1:17pm, Peter Shirley wrote: } Subject: Will anyone send me this paper? } } Drettakis, et. al, "Titghly coupled multiprocessing } for a Global Illumination Algroithm", pp. 387-398, } Eurographics '90. } } And Fournier, et. al, "FIAT LUX: Light Driven Global } Illumination", DGP Technical Memo DGP89-1, 1989. } } I would love to, but I have not read them. AF has given } me a high-level idea of the work, but I would love to get } hold of the real papers. If anyone is willing to } help me, please send copies to: You can get a postscript copy of the first off my web page or George's. Start from, for example, http://www.dgp.toronto.edu/people/elf/elf.html and poke around in my "papers" page. I think it goes out to George's node in France to get the paper. As for the second, I can't seem to find the troff source for it. Hmmm. Maybe Alain has it. I know a real paper copy is sitting in a pile somewhere in the bowels of my office. I'll look for it when next I have a chance. Regards, Eugene. From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id NAA21096; Tue, 19 Mar 1996 13:48:22 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id NAA24867 for ; Tue, 19 Mar 1996 13:22:37 +0100 Received: from merckx.graphics.cornell.edu (MERCKX.GRAPHICS.CORNELL.EDU [128.84.247.147]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id NAA26211 for ; Tue, 19 Mar 1996 13:22:35 +0100 Received: by merckx.graphics.cornell.edu (5.65/DEC-Ultrix/4.3) id AA04424; Tue, 19 Mar 1996 07:22:30 -0500 Message-Id: <9603191222.AA04424@merckx.graphics.cornell.edu> Received: by barn.graphics.cornell.edu (1.37.109.8/16.2) id AA00238; Tue, 19 Mar 1996 07:21:58 -0500 From: Peter Shirley Subject: papers-- thanks To: globillum@imag.fr Date: Tue, 19 Mar 96 7:21:58 EST Mailer: Elm [revision: 70.85] X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Thanks for the many offers to send papers. I have online copies that I got from Alain, Eugene, and George (ask the authors first-- duh!). I will summarize where these are available once I make sure everything prints, etc. Pete From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id WAA08993; Fri, 22 Mar 1996 22:46:20 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id WAA09209 for ; Fri, 22 Mar 1996 22:21:00 +0100 Received: from merckx.graphics.cornell.edu (MERCKX.GRAPHICS.CORNELL.EDU [128.84.247.147]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id WAA24672 for ; Fri, 22 Mar 1996 22:20:59 +0100 Received: by merckx.graphics.cornell.edu (5.65/DEC-Ultrix/4.3) id AA09366; Fri, 22 Mar 1996 16:20:58 -0500 Message-Id: <9603222120.AA09366@merckx.graphics.cornell.edu> Received: by barn.graphics.cornell.edu (1.37.109.8/16.2) id AA15808; Fri, 22 Mar 1996 16:20:24 -0500 From: Peter Shirley Subject: Fiat/Lucifer To: globillum@imag.fr Date: Fri, 22 Mar 96 16:20:23 EST Mailer: Elm [revision: 70.85] X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Thanks again to those who offered to send me papers, and to Alain F, Eugene F, Philip H, and George D for sending me online info. Here is the story as I now understand it. Fiat was a program developed at Toronto in the late 80s, and has been revamped into a program called Lucifer under development at U of British Columbia. The basic idea that these programs draw from is that you want a cheap approximation to incoming light ("field radiance" in Priesendorfer (sp?) borrowed by Arvo) terminology. Unlike Rushhmeier's group, who simplified geometry to simplify field radiance, the Lucifer code attempts to simplify the light coming through virtual surfaces in space. This turns out to be exactly what Zimmerman, Chiu, and I have been trying to do in a Monte Carlo setting (several years late :^} ). So several anonymous reviewers of a rejected SIGGRAPH paper made a good call on saying our work was related to Fiat (thanks to the ones reading this). I may have misunderstood things because I have not read any of this work carefully yet. But being a natural academic I was vague enough that I am sure I seemed knowledgable. I think this basic idea has a lot of promise, and I certainly want to keep pursuing it (but with many more calls to rand() than Alain would have, of course!). For those that want to learn more about Fiat and Lucifer: The Eurographics 90 paper and George's MS thesis which has a discussion of Fiat. http://w3imagis.imag.fr/~George.Drettakis/pub.hmtl Several tech reports that relate to Lucifer http://www.cs.ubc.ca/nest/imager/contributions/healey/imager-tr/imager-tr.html See TR-95-28 : A work-in-progress on Lucifer and wavelets. TR-95-26 : Alain's rendering workshop paper that discusses Lucifer at a high level Alain also sent me a copy of a paper describing Fiat, but I am not sure if it is online (Alain?). Pete PS-- If you are not on my Monte Carlo graphics page and should be, let me know. See: http://www.graphics.cornell.edu/~shirley/mc.html If you have online noisy papers, code, or images, you should be on there. From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id FAA13446; Sun, 24 Mar 1996 05:24:06 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id FAA22869 for ; Sun, 24 Mar 1996 05:10:32 +0100 Received: from haven.uniserve.com (haven.uniserve.com [198.53.215.121]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id FAA28013 for ; Sun, 24 Mar 1996 05:10:27 +0100 Received: from van0101.TVS.NET ([204.191.197.11]) by haven.uniserve.com with SMTP id <34892-137>; Sat, 23 Mar 1996 20:13:22 -0800 X-Sender: iashdown@ledalite.com X-Mailer: Windows Eudora Version 2.0.3 Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed To: globillum@imag.fr From: Ian Ashdown Subject: Radiosity bibliography update Message-Id: <96Mar23.201322pst.34892-137+823@haven.uniserve.com> Date: Sat, 23 Mar 1996 20:13:21 -0800 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Here we go again: it's time for another quarterly update to the global illumination (and radiosity) bibliography, RadBib96. RadBib96 now has 850 references, including 21 new entries that I found over the past three months. The latest version will be posted to our Web site (http://www.ledalite.com/library/rrt.html) on April 1st. In the meantime, here are the new entries. (If you have any corrections or additions, please e-mail them to me before April 1st.) %A D. Arques %A S. Michelin %T Improving the Zonal Method Through the Use of Series Developments to Approximate Volume/Volume Form Factors %J Proceedings of the Fourth International Conference in Central Europe on Computer Graphics and Visualization '96 %E V. Skala %I University of West Bohemia %C Plzen, Czech Republic %D February 1996 %A G. Baciu %A R. K. W. Tsang %T Advancing Front Meshing for Radiosity Solutions %B Lecture Notes in Computer Science %E R. T. Chin %I Springer-Verlag %C Berlin, Germany %V 1024 %P 283-291 %D 1995 %A Martin Feda %T Parallel Radiosity on Transputer with Low Communication Overhead %J Hungarian Academy of Sciences Central Research Institute for Physics %I Hungarian Academy of Sciences %V 2 %N M,N %P 62-70 %D 1995 %O Second Austrian-Hungarian Workshop on Transputer Applications (Budapest, September 1994) %A T. A. Funkhouser %T Database Management for Interactive Display of Large Radiosity Models %J Graphics Interface '96 %C Toronto, Ontario %D May 1996 %P (to appear) %A S. Ghali %A A. J. Stewart %T A Complete Treatment of D1 Discontinuities in a Discontinuity Mesh %J Graphics Interface '96 %C Toronto, Ontario %D May 1996 %P (to appear) %A Jonathan Goldman %T Parallel Progressive Refinement and Projection-based Discontinuity Meshing for Radiosity %R Master's thesis %I University of Illinois at Chicago %C Chicago, IL %D 1995 %A Henrik Wann Jensen %A Niels J. Christensen %T Efficiently Rendering Shadows Using the Photon Map %J Edugraphics + Compugraphics Proceedings %E Harold P. Santo %I GRASP- Graphic Science Promotions & Publications, P.O. Box 4076, Massama, 2745 Queluz, Portugal %C Alvor, Portugal '95 %D December 12, 1995 %P 285-291 %O ISBN 972-8342-00-4 %A Henrik Wann Jensen %T Rendering Caustics on Non-Lambertian Surfaces %J Graphics Interface '96 %C Toronto, Ontario %D May 1996 %P (to appear) %A A. Keller %T A Quasi-Monte Carlo Algorithm for the Global Illumination Problem in the Radiosity Setting %B Lecture Notes in Statistics %I Springer-Verlag %C New York, NY %V 106 %P 239-251 %D 1995 %A S. Z. Li %T Adaptive Sampling and Mesh Generation %J Computer-Aided Design %V 27 %N 3 %D March 1995 %P 235-240 %A A. A. Maierhofer %A M. Gervautz %A K. F. Karner %T Meshing for Discontinuity Driven Hierarchical Radiosity %J Proceedings of the Fourth International Conference in Central Europe on Computer Graphics and Visualization '96 %E V. Skala %I University of West Bohemia %C Plzen, Czech Republic %D February 1996 %A T. Moeller %T Radiosity Techniques for Virtual Reality - Faster Reconstruction and Support for Levels of Details %J Proceedings of the Fourth International Conference in Central Europe on Computer Graphics and Visualization '96 %E V. Skala %I University of West Bohemia %C Plzen, Czech Republic %D February 1996 %A K. Myszkowski %A T. L. Kunii %T An Efficient Cluster-Based Hierarchical Progressive Radiosity Algorithm %B Lecture Notes in Computer Science %E R. T. Chin %I Springer-Verlag %C Berlin, Germany %V 1024 %P 292-303 %D 1995 %A K. Nechvile %A J. Sochor %T Form-factor Evaluation with Regional BSP Trees %J Proceedings of the Fourth International Conference in Central Europe on Computer Graphics and Visualization '96 %E V. Skala %I University of West Bohemia %C Plzen, Czech Republic %D February 1996 %A Adelene Whye-Leng Ng %T Assessment of Five Radiosity Acceleration Techniques %J Computers & Graphics %V 19 %N 5 %P 727-??? %D 1995 %A Thomas Kenji Otake %T Saccade-based Progressive Refinement Radiosity for Virtual Reality Displays %R Master's thesis %I Department of Computer Science, University of Alabama %D 1995 %A M. Sbert %A X. Pueyo %A L. Neumann %A W. Purgathofer %T Global Multipath Monte Carlo Algorithms for Radiosity %J The Visual Computer %V 12 %N 2 %P 47-?? %D 1996 %A Gernot Schaufler %A Wolfgang Stuerzlinger-Protoy %T Exact and Error Bounded Approximation of Local Illumination %J Edugraphics + Compugraphics Proceedings %E Harold P. Santo %I GRASP- Graphic Science Promotions & Publications, P.O. Box 4076, Massama, 2745 Queluz, Portugal %C Alvor, Portugal '95 %D December 12, 1995 %P 327-366 %O ISBN 972-8342-00-4 %A L. Sindlar %A J. Pelikan %T Parallel Radiosity on a Cluster of Workstations %J Proceedings of the Fourth International Conference in Central Europe on Computer Graphics and Visualization '96 %E V. Skala %I University of West Bohemia %C Plzen, Czech Republic %D February 1996 %A Chegu Vinod %T Parallel Hierarchical Radiosity Algorithms %R Master's thesis %I Wayne State University %D 1995 %A Adam Worrall %A Claire Willis %A Derek Paddon %T Dynamic Discontinuities for Radiosity %J Edugraphics + Compugraphics Proceedings %E Harold P. Santo %I GRASP- Graphic Science Promotions & Publications, P.O. Box 4076, Massama, 2745 Queluz, Portugal %C Alvor, Portugal '95 %D December 12, 1995 %P 367 - 375 %K discontinuity meshing, dynamic environments %O ISBN 972-8342-00-4 %Z available as http://aloha.cs.bris.ac.uk/~worrall/scope/port95.html Ian Ashdown, P. Eng. | READ THE BOOK! Research & Development Manager | Radiosity: A Programmer's Perspective Ledalite Architectural Products Inc. | by Ian Ashdown | John Wiley & Sons, 1994 Visit http://www.ledalite.com | (Sneaky Internet Advertising) From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id RAA21640; Mon, 25 Mar 1996 17:42:38 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id QAA09124 for ; Mon, 25 Mar 1996 16:46:35 +0100 Received: from idefix.cs.kuleuven.ac.be (idefix.cs.kuleuven.ac.be [134.58.40.4]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id QAA15731 for ; Mon, 25 Mar 1996 16:46:31 +0100 Received: from pixel.cs.kuleuven.ac.be (ericl@pixel.cs.kuleuven.ac.be [134.58.45.34]) by idefix.cs.kuleuven.ac.be (8.7.5/8.7.3) with ESMTP id QAA26952 for ; Mon, 25 Mar 1996 16:45:57 +0100 (MET) Received: (from ericl@localhost) by pixel.cs.kuleuven.ac.be (8.7.5/8.7.3) id QAA03307; Mon, 25 Mar 1996 16:45:54 +0100 (MET) Date: Mon, 25 Mar 1996 16:45:54 +0100 (MET) From: Eric Lafortune Message-Id: <199603251545.QAA03307@pixel.cs.kuleuven.ac.be> To: globillum@imag.fr Subject: PhD dissertation X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Dear Globillumers, It is my pleasure to announce that my PhD dissertation is now available on the net. The dissertation is entitled: Mathematical Models and Monte Carlo Algorithms for Physically Based Rendering It's all about global illumination models, Monte Carlo methods, variance reduction techniques, path tracing, light tracing and bidirectional path tracing. You can find the abstract, an overview of the chapters, the table of contents, the colour images and the dissertation itself at: http://www.cs.kuleuven.ac.be/~ericl/thesis/ Even if you're not interested in the text you can just have a look at the pretty pictures. Enjoy! Kind regards, Eric Lafortune Computer Graphics Research Group Department of Computer Science Katholieke Universiteit Leuven Belgium From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id VAA22565; Mon, 25 Mar 1996 21:49:39 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id VAA19346 for ; Mon, 25 Mar 1996 21:21:30 +0100 Received: from enzo.qualia.com (enzo.qualia.com [205.161.13.2]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id VAA26620 for ; Mon, 25 Mar 1996 21:21:29 +0100 Received: from [205.161.13.133] by enzo.qualia.com via SMTP (940816.SGI.8.6.9/940406.SGI.AUTO) for id PAA28621; Mon, 25 Mar 1996 15:18:58 -0500 X-Sender: bwade@enzo.qualia.com Message-Id: Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed Date: Mon, 25 Mar 1996 15:26:09 -0500 To: globillum@imag.fr From: Bretton Wade Subject: BSP Trees X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit %A K. Nechvile %A J. Sochor %T Form-factor Evaluation with Regional BSP Trees %J Proceedings of the Fourth International Conference in Central Europe on Computer Graphics and Visualization '96 %E V. Skala %I University of West Bohemia %C Plzen, Czech Republic %D February 1996 Does this paper exist in electronic form anywhere? I would very much like a copy. -- bwade@qualia.com http://www.qualia.com/~bwade/ From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id WAA22625; Mon, 25 Mar 1996 22:05:56 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id VAA19666 for ; Mon, 25 Mar 1996 21:47:57 +0100 Received: from uu6.psi.com (uu6.psi.com [38.145.155.3]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id VAA27116 for ; Mon, 25 Mar 1996 21:47:50 +0100 Received: from iceman.eaglesoft.com by uu6.psi.com (5.65b/4.0.071791-PSI/PSINet) via SMTP; id AA07771 for globillum@imag.fr; Mon, 25 Mar 96 15:47:27 -0500 Received: from ghostjam by iceman (5.4R3.10) id AA02142; Mon, 25 Mar 1996 14:48:23 -0600 Received: by ghostjam (5.x) id AA04787; Mon, 25 Mar 1996 14:49:45 -0600 Date: Mon, 25 Mar 1996 14:49:43 -0600 (CST) From: Alexander Ivanov To: Bretton Wade Cc: globillum@imag.fr Subject: Re: BSP Trees In-Reply-To: Message-Id: Mime-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII; format=flowed X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Check out:
University of West Bohemia Home Page
The Third International Conference in Central Europe on Computer Graphics and Visualization '95 Hope this helps. Alex. On Mon, 25 Mar 1996, Bretton Wade wrote: > %A K. Nechvile > %A J. Sochor > %T Form-factor Evaluation with Regional BSP Trees > %J Proceedings of the Fourth International Conference in Central > Europe on Computer Graphics and Visualization '96 > %E V. Skala > %I University of West Bohemia > %C Plzen, Czech Republic > %D February 1996 > > Does this paper exist in electronic form anywhere? I would very much like a > copy. > > -- > bwade@qualia.com > http://www.qualia.com/~bwade/ > > > From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id EAA02173; Fri, 29 Mar 1996 04:40:53 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id DAA08816 for ; Fri, 29 Mar 1996 03:26:50 +0100 Received: from merckx.graphics.cornell.edu (MERCKX.GRAPHICS.CORNELL.EDU [128.84.247.147]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id DAA18566 for ; Fri, 29 Mar 1996 03:26:49 +0100 Received: by merckx.graphics.cornell.edu (5.65/DEC-Ultrix/4.3) id AA01371; Thu, 28 Mar 1996 21:26:48 -0500 Message-Id: <9603290226.AA01371@merckx.graphics.cornell.edu> Received: by barn.graphics.cornell.edu (1.37.109.8/16.2) id AA13834; Thu, 28 Mar 1996 21:26:13 -0500 From: Peter Shirley Subject: Ugly terminology question To: globillum@imag.fr Date: Thu, 28 Mar 96 21:26:12 EST Mailer: Elm [revision: 70.85] X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Ok, we often pretend that we are solving for radiance, or spectral radiance at each pixel. But chances are we are calculatining luminance Y = 683 lm/cd INT y(lambda) L(lambda) dlamba as well as X and Z. In a "radiosity" program (no flames please) we calculate luminous exitance plus some X and Z that are like luminous exitance but with x and z for weighting functions. Here is the question, if Y is called luminance, what are X and Z called? And what is (X,Y,Z) called? And if V is scotopic luminance, what is (V,X,Y,Z) called? The IES handbook and W&S do not seem to have an answer (but one can miss a 20 page article in either of those volumes!). Does anyone? Thanks, Pete PS-- Bruce Walter suggested "tristimulance" for (X,Y,Z), and this also implies "tristimulous exitance". I am not sure what (V,X,Y,Z) is in this system. From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id WAA07446; Mon, 1 Apr 1996 22:21:41 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id VAA15822 for ; Mon, 1 Apr 1996 21:53:49 +0200 Received: from alf2.tcd.ie (alf2.tcd.ie [134.226.1.26]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id VAA00762 for ; Mon, 1 Apr 1996 21:53:48 +0200 Received: (from lhopkins@localhost) by alf2.tcd.ie (8.7.1/8.6.10) id UAA11145 for globillum@imag.fr; Mon, 1 Apr 1996 20:53:46 +0100 (BST) From: Brother Louis Message-Id: <199604011953.UAA11145@alf2.tcd.ie> Subject: Radiosity vs ray tracing To: globillum@imag.fr Date: Mon, 1 Apr 1996 20:53:45 +0000 (BST) X-Mailer: ELM [version 2.4 PL23] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 I wonder could anyone tell me where I could get information on Ray Tracing versus Radiosity in the context of solving a scene......ie which models shadows better etc,etc. Or any recomended books on the subject. Any information would be gratefully appreciated From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id NAA13748; Sat, 6 Apr 1996 13:35:48 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id NAA24982 for ; Sat, 6 Apr 1996 13:14:50 +0200 Received: from idefix.cs.kuleuven.ac.be (idefix.cs.kuleuven.ac.be [134.58.40.4]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id NAA00182 for ; Sat, 6 Apr 1996 13:14:49 +0200 Received: from pixel.cs.kuleuven.ac.be (ericl@pixel.cs.kuleuven.ac.be [134.58.45.34]) by idefix.cs.kuleuven.ac.be (8.7.5/8.7.3) with ESMTP id NAA18910 for ; Sat, 6 Apr 1996 13:14:46 +0200 (MET DST) Received: (from ericl@localhost) by pixel.cs.kuleuven.ac.be (8.7.5/8.7.3) id NAA15591; Sat, 6 Apr 1996 13:14:44 +0200 (MET DST) Date: Sat, 6 Apr 1996 13:14:44 +0200 (MET DST) From: Eric Lafortune Message-Id: <199604061114.NAA15591@pixel.cs.kuleuven.ac.be> To: globillum@imag.fr Subject: Re: PhD dissertation X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Dear Globillumers, Those of you who have tried downloading my PhD dissertation on Monte Carlo rendering may have experienced problems getting the entire files, due to the connections stalling and timing out. I'm sorry for the inconvenience. Both the b/w and grey-scale versions are now mirrored at ftp.funet.fi and at www.graphics.cornell.edu. You can reach them through my web page at: http://www.cs.kuleuven.ac.be/~ericl/thesis/ or directly at: ftp://ftp.funet.fi/pub/sci/papers/graphics/Lafortune/ or: http://www.graphics.cornell.edu/~eric/ Thanks to Juhana and to Sumant. So, does this dissertation present the ultimate solution to the global illumination problem? Does its bibliography do justice to your work? Will Clive realise that Bill is actually his long-lost half-brother? Tune in and find out... Kind regards, Eric Lafortune. From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id RAA01340; Mon, 15 Apr 1996 17:50:30 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id QAA00370 for ; Mon, 15 Apr 1996 16:37:28 +0200 Received: from cs.uct.ac.za (cs.uct.ac.za [137.158.128.249]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id QAA24784 for ; Mon, 15 Apr 1996 16:34:07 +0200 Received: from maguro.cs.uct.ac.za by cs.uct.ac.za with smtp (Smail3.1.29.1 #11) id m0u8p71-000983C; Mon, 15 Apr 96 16:18 SAT (+0200) From: Nicholas Holzschuch Received: by maguro.cs.uct.ac.za (950911.SGI.8.6.12.PATCH825/maguro.02) id QAA07359; Mon, 15 Apr 1996 16:18:38 +0200 Date: Mon, 15 Apr 1996 16:18:38 +0200 Message-Id: <199604151418.QAA07359@maguro.cs.uct.ac.za> To: globillum@imag.fr Subject: PhD Thesis available X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Hi Globillumers ! My PhD thesis is now available. It deals with hierarchical radiosity, radiosity derivatives, namely first derivatives (Jacobian or gradient) and second derivatives (Hessian), and how to compute them (especially the Hessian). It also explores ways to use these derivatives to compute reliable error-bounds on any interaction, using concavity properties of the radiosity. Finally, it presents a refinement strategy based on these error bounds. The thesis is on A4 paper, takes 176 pages: ftp://ftp.imag.fr/pub/Mediatheque.IMAG/theses/96-Holzschuch.Nicolas/these.ps.gz (3.4 Mo) If you wish, there is a version with 2 pages on one, takes only 88 pages: ftp://ftp.imag.fr/pub/Mediatheque.IMAG/theses/96-Holzschuch.Nicolas/these.a5.ps.gz (3.4 Mo anyway) I'm afraid it is written in french. There should be a paper in english dealing with the same problems, coming real soon :-) Abstract ======= We introduce several improvements to the hierarchical radiosity method. First, a complete analysis of a specific implementation of the hierarchical radiosity method allows to point out its bottlenecks. Based on this analysis, we suggest two simple improvements: a lazy evaluation of top-level interactions, and a new refinement criterion, that greatly reduces the number of interactions, without loss of precision. A brief introduction to the properties of functions of several variables and their derivatives follows, which allows a rewriting of the expression of radiosity, and hence a better numerical approximation. Methods for the estimation of the error produced during the radiosity computations are analysed. We then introduce the concavity properties of the radiosity function that, combined with an exact computation of the radiosity derivatives, allow a complete control of the error on the interactions between patches, and hence a precise minoration and majoration of the radiosity on all the patches. We introduce a new refinement criterion based on this modelling of interactions, and a complete hierarchical radiosity algorithm using this refinement criterion. The last part of the thesis is devoted to practical computations of the radiosity derivatives (gradient and Hessian), first for a constant emitter with total visibility, then for a constant emitter with partial visibility and for an emitter with linear radiosity. -- +-----------------------------+---------------------+ | Nicolas Holzschuch -- Équipe iMAGIS/IMAG | | 385, avenue de la Bibliothèque | | B.P. 53 -- 38041 Grenoble cedex 9 -- France | +---------------------------------------------------+ | Currently at the University of Cape Town, | | Dept. of Computer Science -- 7700 Rondebosch | | South Africa | +---------------------------------------------------+ From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id TAA24732; Tue, 23 Apr 1996 19:15:30 +0200 Received: from graphics.lcs.mit.edu (graphics.lcs.mit.edu [18.24.0.46]) by isis.imag.fr (8.6.11/8.6.9) with SMTP id RAA13536 for ; Tue, 23 Apr 1996 17:15:12 +0200 Received: from pastel.lcs.mit.edu by graphics.lcs.mit.edu (AIX 4.1/UCB 5.64/4.03) id AA17104; Tue, 23 Apr 1996 10:24:16 -0400 From: Seth Teller Received: by pastel.lcs.mit.edu (940816.SGI.8.6.9/TOC-1.2C) id KAA00870; Tue, 23 Apr 1996 10:25:04 -0400 Date: Tue, 23 Apr 1996 10:25:04 -0400 Message-Id: <9604231025.ZM866@pastel.lcs.mit.edu> Reply-To: seth@graphics.lcs.mit.edu X-Mailer: Z-Mail (3.2.2 10apr95 MediaMail) To: globillum@imag.fr Subject: Comp. Geom. Impact Task Force Report (Application Challenges to CG) Cc: sequin@CS.Berkeley.EDU, arir@cs.huji.ac.il, chazelle@cs.princeton.edu, edelman@lcs.mit.edu, gjs@ai.mit.edu, graphics@graphics.lcs.mit.edu, nmp@deslab.mit.edu, olivier.faugeras@sophia.inria.fr, tlp@ai.mit.edu, wisdom@mit.edu Mime-Version: 1.0 Content-Type: text/plain; charset=windows-1252; format=flowed X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit dear global illumination researchers and others, charged by, and under the leadership of, bernard chazelle, the CG Impact Task Force has completed its report entitled "Application Challenges to Computational Geometry." it's an exhortation to comp. geometers to get more involved in identi- fying and attacking problems faced by practitioners in many areas of geometric computing, including computer graphics, imaging, shape reconstruction, machine vision, GIS, mesh generation, robotics, manufacturing, robustness, computa- tional and molecular biology, and astrophysics. i hope that many in our community will find it an interesting, provocative read as well. three versions (dvi, postscript, and compressed postscript) of the full report are available at http://graphics.lcs.mit.edu/~seth/pubs/acmtaskforce.dvi 1/4Mb http://graphics.lcs.mit.edu/~seth/pubs/acmtaskforce.ps 1/2Mb http://graphics.lcs.mit.edu/~seth/pubs/acmtaskforce.ps.Z 1/4Mb (postscript is also available off bernard's page at princeton, but for some reason it's a 2Mb file there.) i've attached to this message postscript for the title page. finally, a paper version of the report is available as TR-521-96 from the princeton cs dept, 35 olden st., princeton nj 08544 usa. comments, criticism, discussion are of course encouraged. best regards, seth teller. -- Asst. Prof of CS and Eng. Synthetic O ~ ~ seth@lcs.mit.edu MIT Lab for CS NE43-208 Imagery <=> ~ tel: 617 258 7885 545 Technology Square Group / \ fax: 617 253 6652 Cambridge MA 02139 / ____________ / http://graphics.lcs.mit.edu/~seth/ X-Zm-Content-Name: acmtaskforce1.ps Content-Description: Postscript Content-Type: application/postscript ; name="acmtaskforce1.ps" X-Zm-Decoding-Hint: mimencode -b -u Attachment converted: WP«s Duo:acmtaskforce1.ps (TEXT/mlpr) (00002B20) From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id SAA03871; Wed, 24 Apr 1996 18:28:23 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id RAA03093 for ; Wed, 24 Apr 1996 17:59:52 +0200 Received: from faure.Colorado.EDU (faure.Colorado.EDU [128.138.228.84]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id RAA26764 for ; Wed, 24 Apr 1996 17:59:45 +0200 Received: (from dilaura@localhost) by faure.Colorado.EDU (8.6.13/8.6.11/Unixops/Hesiod/(SDM)) id KAA03772 for globillum@imag.fr; Wed, 24 Apr 1996 10:07:28 -0600 Date: Wed, 24 Apr 1996 10:07:28 -0600 From: DILAURA DAVID L Message-Id: <199604241607.KAA03772@faure.Colorado.EDU> To: globillum@imag.fr Subject: Form Factor Calculations X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Colleagues: We have found (more) new equations for the calculation of radiative transfer form factors. A result of this work is a new method for determining the effect of blocking objects. I will be presenting a paper on this at the Annual Conference of the Illuminating Engineering Society in August. I have placed a postscript pre-print of it in anonymous ftp at: civil.colorado.edu The file name is: non_diff_contour_4.ps and it is in the directory: pub/Illumination Notice the uppercase I. ___ David L. DiLaura Department of Civil and Architectural Engineering University of Colorado at Boulder From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id FAA05750; Thu, 25 Apr 1996 05:07:09 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id EAA11930 for ; Thu, 25 Apr 1996 04:57:59 +0200 Received: from graphics.lcs.mit.edu (graphics.lcs.mit.edu [18.24.0.46]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id EAA08781 for ; Thu, 25 Apr 1996 04:57:34 +0200 Received: from pastel.lcs.mit.edu by graphics.lcs.mit.edu (AIX 4.1/UCB 5.64/4.03) id AA19446; Wed, 24 Apr 1996 22:55:43 -0400 From: Seth Teller Received: by pastel.lcs.mit.edu (940816.SGI.8.6.9/TOC-1.2C) id WAA01901; Wed, 24 Apr 1996 22:56:32 -0400 Date: Wed, 24 Apr 1996 22:56:32 -0400 Message-Id: <9604242256.ZM1899@pastel.lcs.mit.edu> Reply-To: seth@graphics.lcs.mit.edu X-Mailer: Z-Mail (3.2.2 10apr95 MediaMail) To: globillum@imag.fr Subject: CG Impact Task Force Report now in html, ps, dvi... Cc: arir@cs.huji.ac.il, chazelle@cs.princeton.edu, edelman@lcs.mit.edu, gjs@ai.mit.edu, graphics@graphics.lcs.mit.edu, karlin@cs.washington.edu, nmp@deslab.mit.edu, olivier.faugeras@sophia.inria.fr, sequin@CS.Berkeley.EDU, tlp@ai.mit.edu, wisdom@mit.edu Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit hi everyone, the taskforce report is now available in html as http://graphics.lcs.mit.edu/~seth/pubs/taskforce/techrep.html as well as in postscript http://graphics.lcs.mit.edu/~seth/pubs/taskforce.ps compressed postscript http://graphics.lcs.mit.edu/~seth/pubs/taskforce.ps.Z and dvi http://graphics.lcs.mit.edu/~seth/pubs/taskforce.dvi please forgive my cluttering your mailbox with this second message. best regards, seth teller. From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id UAA05459; Wed, 1 May 1996 20:29:18 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id UAA01447 for ; Wed, 1 May 1996 20:10:40 +0200 Received: from igw2.watson.ibm.com ([129.34.139.6]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id UAA05198 for ; Wed, 1 May 1996 20:10:39 +0200 Received: from vertex.watson.ibm.com (vertex.watson.ibm.com [9.2.2.72]) by igw2.watson.ibm.com (8.7.4/8.7.1) with SMTP id OAA28047 for ; Wed, 1 May 1996 14:10:10 -0400 Received: by vertex.watson.ibm.com (AIX 3.2/UCB 5.64/4/8/96) id AA16814; Wed, 1 May 1996 14:09:54 -0400 Date: Wed, 1 May 1996 14:09:54 -0400 From: Holly Rushmeier Message-Id: <9605011809.AA16814@vertex.watson.ibm.com> To: globillum@imag.fr Subject: appearance workshop X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit For those of you interested in reflectance modelling/measurement, my ex-coworkers at NIST are organizing a workshop to generate industry interest in research in the appearance of coatings. The workshop and the project they are trying to get started are described at: http://titan.cbt.nist.gov/~mikeg/workshop.html -- Holly Rushmeier holly@watson.ibm.com From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id BAA04861; Sat, 25 May 1996 01:28:27 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id BAA09768 for ; Sat, 25 May 1996 01:14:18 +0200 Received: from netcomsv.netcom.com (uucp6.netcom.com [163.179.3.6]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id BAA15862 for ; Sat, 25 May 1996 01:14:16 +0200 Received: from pdi.com by netcomsv.netcom.com with UUCP (8.6.12/SMI-4.1) id QAA25081; Fri, 24 May 1996 16:02:24 -0700 Received: from lilbuddy.pdi.com by pdi.pdi.com via SMTP (920330.SGI/(911001.SGI)1.4-PDI.RELAY) for globillum@imag.fr id AA17540; Fri, 24 May 96 16:03:42 -0700 Received: by lilbuddy.pdi.com (940816.SGI.8.6.9/(911001.SGI)1.2-PDI) id QAA25421; Fri, 24 May 1996 16:03:42 -0700 From: Dan Wexler Message-Id: <199605242303.QAA25421@lilbuddy.pdi.com> Subject: Illuminated by black light To: globillum@imag.fr, thad@hammerhead.com Date: Fri, 24 May 1996 16:03:41 -0700 (PDT) X-Mailer: ELM [version 2.4 PL23] Mime-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Here's a great little anecdote that illustrates just how far rendering is from reality: One of our animators was trying to simulate a shadow using a projection light. He created a texture that was white where he wanted light, and black where he wanted shadow. Then he used a special material shader we have called a 'shadow-only' shader that renders the inverse shadow (ie. white/gray wherever there are shadows and black everywhere else). As you might guess, the "shadows" from the projection light did not show up in the image generated by the shadow-only shader. When I explained the situation to him I caught myself saying: "Well, those points are not in shadow. They are illuminated with black light." He looked at me with a completely blank expression, so I went on: "If you were in a completely closed room without a light, would the room be completely shadowed, or not illuminated?" The boundary between science and philosophy is a blurry one. Daniel Wexler R&D Staff, Pacific Data Images From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id CAA04971; Sat, 25 May 1996 02:22:54 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id CAA10108 for ; Sat, 25 May 1996 02:10:52 +0200 Received: from wk309.nas.nasa.gov (wk309.nas.nasa.gov [129.99.64.29]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id CAA16178 for ; Sat, 25 May 1996 02:10:42 +0200 Received: (from uselton@localhost) by wk309.nas.nasa.gov (8.6.12/NAS.6.1) id RAA19501; Fri, 24 May 1996 17:10:36 -0700 Date: Fri, 24 May 1996 17:10:36 -0700 Message-Id: <199605250010.RAA19501@wk309.nas.nasa.gov> From: "Samuel P. Uselton" To: globillum@imag.fr Subject: [wexler@pdi.com: Illuminated by black light] Reply-to: uselton@nas.nasa.gov X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit From: wexler@pdi.com (Dan Wexler) > >Here's a great little anecdote that illustrates just how far >rendering is from reality: > >One of our animators was trying to simulate a shadow using {trimmed for brevity} > >When I explained the situation to him I caught myself saying: > >"Well, those points are not in shadow. They are illuminated >with black light." > >He looked at me with a completely blank expression, so I went on: > >"If you were in a completely closed room without a light, >would the room be completely shadowed, or not illuminated?" > >The boundary between science and philosophy is a blurry one. Of course we aren't always trying to duplicate reality. Sometimes, especially in scientific visualization, we want to make realistic *seeming* images of things that one can not see. My anecdote on the communication break down between disciplines goes like this... A petroleum engineer (old, gruff and crotchety) was attending the annual project review for the Visualization group at an oil company research lab. The company and the engineer shall remain nameless, but one of the people making the presentation was my friend, collaborator and one time student, Mark Lee. The main uses of visualization in the oil company were in the analysis of seismic data and the display of petroleum reservoir simulation results. Mark was explaining about adding capabilities to use a variety of shading models, and what the input to the vis package needed to be for some of the nicer shaders. In particular, he described the benefits of being able to specify the position of the light source, and change it interactively, in enhancing visibility of certain things in the visualization. The petroleum engineer interrupts and rather rudely proclaims to all that the software can't POSSIBLY work like that 'cause everybody knows there's no light underground. Mark tried to explain, but his critic couldn't pry his mind open enough to understand the explanation. Sam Uselton uselton@nas.nasa.gov From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id VAA20023; Tue, 28 May 1996 21:39:15 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id VAA29194 for ; Tue, 28 May 1996 21:24:39 +0200 Received: from irz201.inf.tu-dresden.de (irz201.inf.tu-dresden.de [141.76.1.10]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id VAA12203 for ; Tue, 28 May 1996 21:24:35 +0200 Received: by irz201.inf.tu-dresden.de (8.6.12/8.6.12-s1) id VAA25396 for globillum@imag.fr; Tue, 28 May 1996 21:24:19 +0200 From: "Nguyen, D.C." Message-Id: <199605281924.VAA25396@irz201.inf.tu-dresden.de> Subject: Procedural bloby objects avialable. To: Global Illumination List Date: Tue, 28 May 1996 21:24:19 +0200 (MESZ) X-Mailer: ELM [version 2.4 PL25 ME8b] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 For infos about RTEvol(RayTraced Evolution:), a free package for procedural- modelling, using Lindenmeyer-grammars and interpreted C-like macros/function, look at this URL: http://www.rz.tu-ilmenau.de/~juhu/GX/RTEvol/ Primarly i use this package to test some raytracing-acceleration techniques, but now it expands to a fully programmable system. It is an ideal tool for quickly generation of test-scenes . Have fun, --JuHu From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id VAA02473; Thu, 30 May 1996 21:49:38 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id VAA13835 for ; Thu, 30 May 1996 21:27:05 +0200 Received: from haven.uniserve.com (haven.uniserve.com [198.53.215.121]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id VAA13197 for ; Thu, 30 May 1996 21:26:36 +0200 Received: from van0217.tvs.net ([204.191.197.57]) by haven.uniserve.com with SMTP id <30778-28269>; Thu, 30 May 1996 12:28:36 -0800 Date: Thu, 30 May 96 12:21:51 -0700 From: Ian Ashdown Organization: Ledalite Architectural Products X-Mailer: Mozilla 1.1N (Windows; I; 16bit) MIME-Version: 1.0 Newsgroups: comp.graphics.algorithms,comp.graphics.rendering.misc,comp.graphics.rendering.raytracing,comp.graphics.visualization,alt.3d To: globillum@imag.fr Subject: ANNOUNCE: Radiosity Bibliography Update Content-Transfer-Encoding: 8bit Content-Type: text/plain; charset=us-ascii; format=flowed Message-Id: <96May30.122836pdt.30778-28269+3646@haven.uniserve.com> X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 ANNOUNCE: 96/06/01 Release of RADBIB96 -------------------------------------- RADBIB96 is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. A total of 51 new references have been added since its last release on April 1, 1996, bringing the total to 904 references. This bibliography is available in refer format (ASCII text) as RADBIB96.TXT (with a release date of June 1, 1996) from: http://www.ledalite.com/library/rrt.html and as gzip-compressed RadBib96.Z from: ftp://hobbes.lbl.gov/pub/doc A gzip-compressed BibTex-format version is available from: ftp.cs.columbia.edu/archives/bibliographies/Graphics/rad.html but it may be a previous release. An interim release dated May 15, 1996 will be included as part of Course 7, "Global Illumination in Architecture and Entertainment," on the ACM SIGGRAPH 96 Course Notes CD-ROM. A refer-format file containing only the new references is also available -- send your e-mail request to iashdown@ledalite.com. As always, it is time-consuming and sometimes difficult to track down conference papers and theses on radiosity and global illumination. If you know of a relevant reference that is not included in the bibliography, please let me know so that I can include it in the next release. From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id HAA01983; Thu, 20 Jun 1996 07:08:23 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id GAA25413 for ; Thu, 20 Jun 1996 06:52:05 +0200 Received: from haven.uniserve.com (haven.uniserve.com [198.53.215.121]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id GAA21289 for ; Thu, 20 Jun 1996 06:52:03 +0200 Received: from van0127.TVS.NET ([204.191.197.37]) by haven.uniserve.com with SMTP id <31569-6551>; Wed, 19 Jun 1996 21:55:32 -0800 X-Sender: iashdown@ledalite.com X-Mailer: Windows Eudora Version 2.0.3 Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed To: globillum@imag.fr From: Ian Ashdown Subject: Interesting literature Message-Id: <96Jun19.215532pdt.31569-6551+1234@haven.uniserve.com> Date: Wed, 19 Jun 1996 21:55:25 -0800 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Here are three papers scheduled to be presented at the 1996 Illuminating Engineering Society Annual Conference in Cleveland, Ohio (August 5-7) that may be of interest: 1. DiLaura, David L. 1996. "Non-Diffuse Radiative Transfer III: Inhomogeneous Planar Area Sources and Point Receivers." 2. DiLaura, David L., and Scott Santoro. 1996. "Non-Diffuse Radiative Transfer IV: General Procedure for Planar Area Sources and Area Receivers." 3. Nievergelt, Y. 1996. "Making Any Radiosity Matrix Symmetrix Positive Definite." You can obtain preprints of David's papers as pub/Illumination/ non_diff_contour_3.ps and pub/Illumination/non_diff_contour_4.ps from civil.colorado.edu. As for Nievergelt's paper, I am not aware of it being available online. If it isn't, you might want to obtain a copy of the 1996 IESNA Annual Conference Technical Papers that are supposed to be available in mid-June. Check http://www.iesna.org for details -- they are generally not available after the conference is over. (If it's anything like the past few years, the publication will be over 1,000 pages and cost about $125 US.) Ian Ashdown, P. Eng. | READ THE BOOK! Research & Development Manager | Radiosity: A Programmer's Perspective Ledalite Architectural Products Inc. | by Ian Ashdown | John Wiley & Sons, 1994 Visit http://www.ledalite.com | (Sneaky Internet Advertising) From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id QAA09908; Thu, 27 Jun 1996 16:37:49 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id PAA00776 for ; Thu, 27 Jun 1996 15:49:57 +0200 Received: from uni-kl.de (stepsun.uni-kl.de [131.246.136.50]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id PAA24510 for ; Thu, 27 Jun 1996 15:49:05 +0200 Received: from uklirb.informatik.uni-kl.de by stepsun.uni-kl.de id af03629; 27 Jun 96 15:48 MET DST Received: from irz1.informatik.uni-kl.de by uklirb.informatik.uni-kl.de id aa09152; 27 Jun 96 15:45 MET DST Received: by irz1.informatik.uni-kl.de (SMI-8.6/SMI-SVR4) id PAA14659; Thu, 27 Jun 1996 15:45:23 +0200 From: Alexander Keller AG Heinrich Message-Id: <199606271345.PAA14659@irz1.informatik.uni-kl.de> Subject: Quasi-Monte Carlo Radiosity To: globillum@imag.fr Date: Thu, 27 Jun 1996 15:45:22 +0200 (MET DST) X-Mailer: ELM [version 2.4 PL24] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hi ! The extended version of my Eurographics Workshop on Rendering contribution is now available on the net via: http://www.uni-kl.de/AG-Heinrich/Alex.html and then clicking the "publications and reports" link. Besides the 18-pages version (instead of 10), you will find related work from the field of quasi-Monte Carlo methods. Any comments or discussions about the work are welcome. Best regards, Alex -- Alexander Keller, Tel.: +49-631-205-3345, Fax.: +49-631-205-3270 Dept. of Computer Science, University of Kaiserslautern Postfach 3049, D-67653 Kaiserslautern, Germany e-mail: keller@informatik.uni-kl.de, URL: http://www.uni-kl.de/AG-Heinrich/ From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id BAA09739; Thu, 4 Jul 1996 01:25:59 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id BAA04048 for ; Thu, 4 Jul 1996 01:14:43 +0200 Received: from usc.edu (usc.edu [128.125.253.136]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id BAA12400 for ; Thu, 4 Jul 1996 01:14:41 +0200 Received: from halcyon.usc.edu (sidhu@halcyon.usc.edu [128.125.72.33]) by usc.edu (8.7.2/8.7.2/usc) with ESMTP id QAA27403 for ; Wed, 3 Jul 1996 16:14:35 -0700 (PDT) Received: (from sidhu@localhost) by halcyon.usc.edu (8.7.2/8.7.2/usc) id QAA24994; Wed, 3 Jul 1996 16:14:34 -0700 (PDT) Date: Wed, 3 Jul 1996 16:14:34 -0700 (PDT) Message-Id: <199607032314.QAA24994@halcyon.usc.edu> From: Reetinder Pal Sidhu To: globillum@imag.fr Subject: Graphics Gems X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Does anyone know if another book in the Graphics Gems series is in the works? Please let me know if you have any idea who should be contacted for submitting contributions to it. Thank you. Reetinder Sidhu From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id BAA09823; Thu, 4 Jul 1996 01:57:56 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id BAA04164 for ; Thu, 4 Jul 1996 01:47:51 +0200 Received: from wk309.nas.nasa.gov (wk309.nas.nasa.gov [129.99.64.29]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id BAA12618 for ; Thu, 4 Jul 1996 01:47:49 +0200 Received: (from uselton@localhost) by wk309.nas.nasa.gov (8.6.12/NAS.6.1) id QAA13057; Wed, 3 Jul 1996 16:47:42 -0700 Date: Wed, 3 Jul 1996 16:47:42 -0700 Message-Id: <199607032347.QAA13057@wk309.nas.nasa.gov> From: "Samuel P. Uselton" To: sidhu@halcyon.usc.edu CC: globillum@imag.fr In-reply-to: <199607032314.QAA24994@halcyon.usc.edu> (message from Reetinder Pal Sidhu on Wed, 3 Jul 1996 16:14:34 -0700 (PDT)) Subject: Re: Graphics Gems Reply-to: uselton@nas.nasa.gov X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit The word is that rather than continuing the Graphics Gems book series, a periodical called Journal of Graphics Tools (JGT) is starting, which will carry such things. For more info see http://www.acm.org/jgt/ I don't know how recent this info is, but it is a good starting point. Sam Uselton uselton@nas.nasa.gov From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id HAA10670; Thu, 4 Jul 1996 07:17:58 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id HAA05137 for ; Thu, 4 Jul 1996 07:05:32 +0200 Received: from abash1.microsoft.com (abash1.microsoft.com [131.107.3.23]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id HAA17689 for ; Thu, 4 Jul 1996 07:05:30 +0200 Received: by abash1.microsoft.com with SMTP (Microsoft Exchange Server Internet Mail Connector Version 4.0.985.1) id <01BB6926.E1EE1190@abash1.microsoft.com>; Wed, 3 Jul 1996 21:30:40 -0700 Message-ID: From: Andrew Glassner To: "'globillum@imag.fr'" , "'Reetinder Pal Sidhu'" Subject: RE: Graphics Gems Date: Wed, 3 Jul 1996 21:30:25 -0700 X-Mailer: Microsoft Exchange Server Internet Mail Connector Version 4.0.985.1 Encoding: 22 TEXT X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit I believe that there will not be any more volumes in the Gems series. You may wish to instead consider the Journal of Graphics Tools, which is a new quarterly journal for small and practical graphics methods. The first issue or two will be available at Siggraph. Check out http://www.acm.org/jgt/ -Andrew Glassner http://www.research.microsoft.com/research/graphics/glassner/ >---------- >From: Reetinder Pal Sidhu[SMTP:sidhu@halcyon.usc.edu] >Sent: Wednesday, July 03, 1996 4:14 PM >To: globillum@imag.fr >Subject: Graphics Gems > >Does anyone know if another book in the Graphics Gems series is in the >works? Please let me know if you have any idea who should be contacted >for submitting contributions to it. Thank you. > > Reetinder Sidhu > From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id NAA12658; Thu, 4 Jul 1996 13:42:17 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id NAA13184 for ; Thu, 4 Jul 1996 13:11:46 +0200 Received: from ibis.doc.ic.ac.uk (ibis.doc.ic.ac.uk [146.169.12.90]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id NAA28776 for ; Thu, 4 Jul 1996 13:11:41 +0200 Received: from ibis.doc.ic.ac.uk by ibis.doc.ic.ac.uk with smtp (Smail3.1.28.1 #8) id m0ubl57-0002nbC; Thu, 4 Jul 96 10:52 BST Sender: ajc@imag.fr Message-ID: <31DB9450.41C67EA6@doc.ic.ac.uk> Date: Thu, 04 Jul 1996 10:52:16 +0100 From: "Adrian J. Chung" Organization: Dept. of Computing, Imperial College X-Mailer: Mozilla 2.02 (X11; I; SunOS 4.1.3 sun4c) MIME-Version: 1.0 To: globillum@imag.fr Subject: Book Reviews Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 8bit X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 (Warning: I'm new to this list...) I'm surveying a cross section of research publications in global illumination and have come across a few candidates for what I'd consider to be "the bible" for this field (in the same sense that the Foley & Van Dam book is for CG in general). I'd like to hear your opinions on the matter. I've skimmed through the past archived communications for globillum in case this was already discussed, but it doesn't seem to have been recently. So... Andrew S. Glassner: Priciples of Digital Image Synthesis Is it well worth the US$90? How much does it cost in the UK? I'm considering diverting a portion of my student grant toward acquiring the two volume set. (Fewer beers on weekends, looks like...) How does it compare to the less expensive alternatives: Franois X. Sillion & Claude Puech: Radiosity and Global Illumination Michael F. Cohen & John R. Wallace: Radiosity and Realistic Image Synthesis ...any others I should know about? Adrian -- If you think in seasons, plant crops. If you think in decades, plant trees. If you think in centuries, educate your children. Confucious From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id GAA16109; Thu, 11 Jul 1996 06:58:00 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id GAA11785 for ; Thu, 11 Jul 1996 06:49:27 +0200 Received: from haven.uniserve.com (haven.uniserve.com [198.53.215.121]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id GAA22500 for ; Thu, 11 Jul 1996 06:49:25 +0200 Received: from van0210.tvs.net ([204.191.197.50]) by haven.uniserve.com with SMTP id <32355-14394>; Wed, 10 Jul 1996 21:53:07 -0800 X-Sender: iashdown@ledalite.com X-Mailer: Windows Eudora Version 2.0.3 Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed To: globillum@imag.fr From: Ian Ashdown Subject: Re: Book Reviews Message-Id: <96Jul10.215307pdt.32355-14394+1615@haven.uniserve.com> Date: Wed, 10 Jul 1996 21:53:04 -0800 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit On Thu, 04 Jul 1996 10:52:16, Adrian J. Chung wrote: >I'm surveying a cross section of research publications in global illumination >and have come across a few candidates for what I'd consider to be "the bible" >for this field (in the same sense that the Foley & Van Dam book is for CG in >general). I'd like to hear your opinions on the matter. I've skimmed through the >past archived communications for globillum in case this was already discussed, >but it doesn't seem to have been recently. So... > In my very humble opinion, the definitive bible on global illumination has yet to be written. One good reason for this is that global illumination research is still a very active topic. There have been close to 100 global illumination papers and theses released in the past six months alone. Given that it takes 12 to 18 months to get a book written and published, any "bible" will be at least a year out of date as soon as it is released. >Andrew S. Glassner: Principles of Digital Image Synthesis > >Is it well worth the US$90? How much does it cost in the UK? >I'm considering diverting a portion of my student grant toward acquiring the two >volume set. (Fewer beers on weekends, looks like...) > Knowing how much one publisher in particular marks up its books for the UK market, I shudder to think how much the two-volume set will cost you. You may have to give up beer for the remainder of your academic career :+) For what it's worth, I much prefer Glassner to Foley et alia as my primary CG reference. However, I can appreciate that many undergraduate students may be intimidated by the mathematical depth of the former. Different strokes ... >How does it compare to the less expensive alternatives: > >Francois X. Sillion & Claude Puech: Radiosity and Global Illumination > >Michael F. Cohen & John R. Wallace: Radiosity and Realistic Image Synthesis > It all depends on your needs and interests, and also on whether you are interested in (and enjoy) the mathematical details. I have all three, and I can recommend any of them. >...any others I should know about? > I haven't had the opportunity to read this book, but you might try: Kok, Arjan J. F. 1994. "Ray Tracing and Radiosity Algorithms for Photorealistic Image Synthesis," Delft University Press, Stevinweg 1, 2628 CN Delft, The Netherlands, ISBN 90-6275-981-5. (Also available from Coronet Books, Philadelphia.) This was Arjan's PhD thesis at the Delft University of Technology. There have been at least two other books written on radiosity, but neither qualify as global illumination "bibles." Actually, the best sources of up-to-date and comprehensive information on global illumination techniques are the most recent MSc and PhD theses, many of which are available online. PhD theses in particular are great -- the poor students are required to demonstrate their in-depth knowledge of the field, which generally means a 50-page prologue to their actual research topic, and a bibliography with at least 50 references. For a complete listing ... ah heck, you know where to find my bibliography ;+> Ian Ashdown, P. Eng. | READ THE BOOK! Research & Development Manager | Radiosity: A Programmer's Perspective Ledalite Architectural Products Inc. | by Ian Ashdown | John Wiley & Sons, 1994 Visit http://www.ledalite.com | (Sneaky Internet Advertising) From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id WAA19894; Thu, 11 Jul 1996 22:22:55 +0200 Received: from anduin.ocf.llnl.gov (anduin.ocf.llnl.gov [134.9.49.1]) by isis.imag.fr (8.6.11/8.6.9) with SMTP id VAA11021 for ; Thu, 11 Jul 1996 21:02:03 +0200 Received: from max.ocf.llnl.gov by anduin.ocf.llnl.gov (4.1/SMI-4.0) id AA28397; Thu, 11 Jul 96 11:36:24 PDT Received: by max.ocf.llnl.gov (951211.SGI.8.6.12.PATCH1042/951211.SGI.AUTO) for globillum@imag.fr id LAA11557; Thu, 11 Jul 1996 11:36:24 -0700 From: "Nelson L. Max" Message-Id: <9607111136.ZM11555@max.ocf.llnl.gov> Date: Thu, 11 Jul 1996 11:36:17 -0700 X-Mailer: Z-Mail (3.2.0 26oct94 MediaMail) To: globillum@imag.fr Subject: Report on Dagstuhl and Porto rendering conferences. Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit The following is a report on three conferences I attended. I am broadcasting it because it contains summaries of several papers that may not appear for a while in more widely read venues. I appologize if your paper was not mentioned. Only the first two conferences were on rendering, so you might want to skip the stuff about the last one, though my summaries for it are mostly restricted to rendering-related talks. My first stop was the University of Kaiserslautern, where I visited the research laboratory of Hans Hagen. Hans arranged for a schedule of demonstrations and discussions with his graduate students, and arranged for them to take me out to lunch and dinner in town (I paid for my food, but they provided the transportation and the company, which was a nice form of hospitality.) I was impressed with Hans' personal research in the design of plastic reflector and lens shapes for car headlights, to give a desired distribution of illumination intensity on the road. I also had a long discussion with Alexander Keller, who explained to me in detail the Quasi-Monte-Carlo method he was using for global illumination, which he presented at both of the next two meetings. He gave me the longer"uncut" version of his paper, so I was able to appreciate well the fact that certain non-random sequences of test points give estimates that converge much faster than for random test points. A final memorable project was a method where potential purchasers could design and view semi-custom prefabricated homes over the Internet. The meeting in Schloss Dagstuhl was one of a series of week-long seminars in aspects of Computer Science partially supported by the governments of Germany and the state of Saarbrucken. The topic of this seminar was rendering, and it was scheduled to just precede the Eurographics workshop the following week. The hope was that attendees from outside Europe would gain efficiency in their long distance travel plans, which was the case for me, but many Europeans could not afford more than a week away from their institutions, especially if they were teaching, so the attendance at the Eurographics Workshop was actually down from last year. A summary of the some of talks follows. Xavier Pueyo proposed methods for generating random densities of infinite lines in space, and intersecting each line with all objects in the scene to get form factor contributions from each segment in the space between two object surfaces. He chose his lines by connecting two random points on the surface of a sphere enclosing all the objects, and I later pointed out that this will not give the correct density because it is missing a cosine term. Dani Tost discussed her work on visualizing blood vessels, involving both maximum intensity projection and shading, with voxel splats. Henrick Wann Jensen's talk on "Global Illumination using Photon Maps" generated the most excitement and discussion of the seminar, because of the impressive performance of his method, which is based on saving in a spatial data structure (a KD tree) both position and direction of all hits by photon paths traced from light sources through multiple random bounces. During viewpoint dependent rendering, these are used for the intensity at the second bounce in a local pass from the eye, by expanding a sphere about the hit point until the n closest photon hits are found in the KD tree. At the first bounce from the eye, the same distribution is used for importance sampling of the bounced rays. Finally, the initial rays from the light source are continued past their first surface intersection to create shadow maps at subsequent intersections, which are used to decide when shadow feelers are necessary to determine direct illumination. Since the incoming directions are available, non diffuse reflections can be rendered. A separate caustic map, with many more photons directed at only the shiny surfaces, is used similarly at the first bounce in rendering. Dani Lischinski gave a preview of a Siggraph paper on "Hierarchical Image Caching for Accelerated Walkthroughs of Complex Environments." Robert Garmann talked on the computational complexity of hierarchical radiosity, and gave a careful analysis of the number of links required in a simple scene with two parallel plane patches, in which the subdivision oracle is based on the total form factor of a link. He showed that the total number of links, as the allowed error approaches zero, is of order O(N^2), where N is the number of leaf nodes in the hierarchical subdivision. This seems to contradict previous beliefs that it would be O(N log N), or even O(N). Dieter Fellner, working with Stefan Müller's group at Darmstadt, showed how real time rendering of radiosity scenes could be accomplished on environments with the order of a million polygons, and presented an impressive video of additions to the Frankfort airport. Wolfgang Stürzlinger talked about using hierarchical radiosity links in the local pass (final one bounce gather to the viewpoint) by doing a Weiler-Atherton type subdivision of the unit hemisphere, using 3D coordinates of the unit vectors, in order to determine the links involved at a pixel. Mark Summinger from Erlangen University talked about decoupling the reflection and transport operators in a progressive radiosity framework for non diffuse surfaces. The shot and transported energy is saved in a data structure which is indexed by both receiving position and angle bins. The advantage is that when it is time to shoot for a patch, all the energy in an incoming angle bin can be reflected at once, which requires fewer evaluations or accesses to the BDRF. The abstracts to these talks were handwritten into a Dagstuhl record book, and are being transcribed to be sent to the participants and saved at Dagstuhl. The proceedings of the next conference I attended, the 7th Eurographics Workshop on Rendering, at Porto, Portugal, will be published rapidly by Springer. At Porto, (and also at Dagstuhl) I spoke on "Hierarchical Rendering of Trees from Precomputed Multi-Layer Z-Buffers". This is based on reprojecting images of trees and their subparts, prerendered from different viewpoints (image based rendering). Fabrice Neyret gave a related paper which had an impressive video of a flight over a forest, produced by ray tracing hierarchical (mip mapped) volume textures with an ellipsoidally approximated surface normal distribution at each voxel. Fredo Durand, George Drettakis, and Claude Puesch gave a speculative talk on an unimplemented method of dividing the 4D space of all lines in 3D up into regions where the visibility along the ray is constant. To deal with rays which have multiple segments in the free volume between objects, they use and extra discrete dimension to index the segments, but the space of such segments still has only 4 real parameters for a fixed scene. They discuss the various lower dimensional manifolds of visibility change events that divide this space into regions of homogeneous visibility, and show why the resulting data structure is of size O(n^4), where n is the number of polygon edges, and can be constructed by a sort and sweep algorithm in time O(n^4 log n). This is considerably better than the aspect graph, of size O(n^6), because the aspect graph computes for each viewing direction (or viewpoint) the intersection of the 2D pencil of lines making up the image, with this subdivision of the 4D space of all lines.Eric Veach pointed out that in the case of caustic maps under water, and the case of bump mapped shading normals differing from the normals of the surfaces which intercept the light transport rays, non symmetric scattering functions (BDRFs or BDTFs) must be used, which do not satisfy reciprocity, and therefore act differently when light energy or importance are being transported, or equivalently, act differently for the two directions in bidirectional path tracing (photon paths and viewing paths). Stephen Hardt and Seth Teller from MIT showed how the rendering pipeline and texture mapping hardware with perspective correction of a high end workstation could be cleverly used to produce accurate radiosity rendering at interactive rates by fitting the radiosity off-line (ahead of time) by quadratic triangular patches, and then using the hardware polygon renderer to deposit at each pixel the polygon ID and two barycentric coordinates in the triangle. They use the perspective correction in the texture mapper to get the barycentric coordinates accurately. With Michael Allison, I showed in Graphic Gems III how the barycentric coordinates could be stored in color fields, using only the Gouraud shading interpolation hardware, if perspective corrections are not needed. The radiosity is then computed in software as a quadratic polynomial in the two barycentric coordinates, with coefficients indexed by the polygon ID. Jos Stam and Eric Languénou spoke about ray tracing in non-constant media (mirages). Eric Lafortune and Yves Willems extended bidirectional path tracing to the case of 3D volumes with participating media (smoke, steam, or clouds). George Dretakis and Francois Sillion spoke on incorporating discontinuity meshing into hierarchical quadtree meshes, which allows large quadtree cells on homogeneous unoccluded regions; previous discontinuity meshes based on BSP trees had unnecessarily long edges crossing into regions beyond the discontinuities that defined them. I spent the 6 days between the Porto and Chamonix conferences on vacation in Portugal, cycling with my wife Mika from Coimbra to Alcobaca, on bicycles kindly loaned by the local conference organizer, Augusto de Sousa, because there were no bicycle rental shops in northern Portugal. The final day before the Curves and Surfaces conference began was spent travelling from Porto to Chamonix. The topics of the Chamonix conference were less familiar to me, being weighted towards approximation theory based on functional analysis on Sobelov spaces (I still haven't figured out what theses are) and wavelets. I attended because Greg Nielson invited me to give a talk at a Mini-symposium he organized an Scientific Visualization. I spoke on "Applications of Texture Mapping to Volume and Flow Visualization," giving in 25 minutes almost all the content of the version I also earlier presented at the University of Kaiserslautern in 65 minutes. In the same session, Marcus Gross gave a talk on "Finite Element Modelling and Visualization for Facial Surgery," in which the soft tissues between the bone and skin are modelled by finite elements, whose deformation is simulated as bones are cut and displaced, so that the final appearance of the face can be displayed before the operation is carried out. There were 6 days of mostly 3 parallel sessions of 25 minute talks form 8:30 AM until 6:30 PM (with a 2 hour break for lunch, and two half hour coffee breaks) for 6 conference days, which made for a pretty grueling schedule. I attended most of the time, but admit to "playing hooky" for two mornings in order to enjoy the mountain scenery. I probably absorbed some approximation theory by osmosis, especially from an excellent Mini-symposium on non-linear and adaptive wavelet approximation, including talks by Yves Meyer on the bump algebra, by S. Mallet on Image Compression, emphasizing the quantization and coding of the wavelet or basis coefficients, and the coding of the position indices of the non-zero coefficients, as well as just which coefficients can be set to zero, and by Ron DeVore on adaptive numerical methods for partial differential equations. There was also an interesting talk by A. Pinkus on approximating by ridge functions, the set of finite linear combinations of ridges, which are "long crested waves" of one linear parameter in 2 or 3 dimensions. There were many talks on extending the ideas of wavelets from the plane to arbitrary 2-manifolds, and in particular, to the 2-sphere. Beyond these approximation theory talks, the talks I understood best were on surface shape. There were a couple of talks on developable surfaces, which are important in manufacturing because they can be formed from sheet metal without stretching. An invited talk by Joseph Hoschek on interpolation and approximation with developable surfaces gave an example of designing the blank holder in a sheet metal forming process. This is the part of the mold which should first clamp the sheet, without stretching it, and hold it while the part of the deformation involving more severe stretching deformations takes place. Another talk by Y. L. Kergosian analyzed the folds and cusps where a developable surface can have singularities, and simulated them for the case of a bent tin can, generating impressively realistic images. There was also a Mini-symposium on Multiresolution Methods in Computer Graphics, including the following talks. Richard Bartels talked on hierarchical splines. Peter Scrhöder spoke on spherical wavelets, and showed his Siggraph '95 images. After hearing it for the nth time, I finally understood the idea behind lifting. R. Westerman described his wavelet-based volume rendering, in which the wavelets are used only for determining the appropriate adaptive sampling frequency along a ray and for reconstructing the samples, for a traditional opacity accumulation algorithm. Thus full opacity effects are possible, in contrast to faster algorithms which try to precompute the splats of each wavelet, and therefore cannot account for interwavelet opacity effects. David Salesin presented three multiresolution techniques from his past and future Siggraph papers: image editing, image querying, and multiresolution video "clip art". -- Nelson Max http://www.llnl.gov/graphics max2@llnl.gov Lawrence Livermore National Laboratory (510) 422-4074 7000 East Avenue fax (510) 423-8704 Livermore, CA 94550, USA From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id NAA24500; Fri, 12 Jul 1996 13:24:23 +0200 Received: from cosmos.imag.fr (cosmos.imag.fr [147.171.130.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id MAA20929 for ; Fri, 12 Jul 1996 12:46:22 +0200 Received: from goliat.ugr.es (goliat.ugr.es [150.214.20.3]) by cosmos.imag.fr (8.6.13-durand/8.6.9) with ESMTP id MAA25769 for ; Fri, 12 Jul 1996 12:46:20 +0200 Received: (from almagro@localhost) by goliat.ugr.es (8.6.10/8.6.12) id MAA23089; Fri, 12 Jul 1996 12:44:25 +0100 Date: Fri, 12 Jul 1996 12:44:16 +0100 (WET DST) From: Carlos Urena Almagro X-Sender: almagro@goliat To: "Nelson L. Max" cc: globillum@imag.fr Subject: Re: Report on Dagstuhl and Porto rendering conferences. In-Reply-To: <9607111136.ZM11555@max.ocf.llnl.gov> Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII; format=flowed X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit On Thu, 11 Jul 1996, Nelson L. Max wrote: > Xavier Pueyo proposed methods for generating random densities of infinite > lines in space, and intersecting each line with all objects in the scene to get > form factor contributions from each segment in the space between two object > surfaces. He chose his lines by connecting two random points on the surface of > a sphere enclosing all the objects, and I later pointed out that this will not > give the correct density because it is missing a cosine term. Some years ago, when Sbert & Pueyo showed me their method, I though about this objection, because it seems counter-intuitive that this selection of points on the sphere induces the correct density. But later I was convinced of it's correctnes, both by estimating that way form-factors whose value was analiticaly known a priori, and by formal derivations from results in Integral Geometry theory. There is a formula on Santalo's book about Integral Geomtery which gives the density of the points of intersection of a convex object with lines of constant density in 3D. When instancing the convex object to a sphere, the density for intersections points becomes uniform. This is so because the formula involves the diferential poin-to-point form factor between the two intersection points of each line, an this value, in the case of a sphere, is a constant which only depends on sphere's radius. You can check this by seeing the internal angles of a triangle whose vertexs are these two points and the center of the sphere. The refered formula is at the bottom of page 230 of: Integral Geometry and Geometric Probability. Luis A. Santalo. Addison-Wesley, 1976. Sincerely yours, Carlos Urena. _____________________________________________________________________________ Carlos Urena Almagro e-mail : almagro@goliat.ugr.es Dpto. de Lenguajes y Sistemas Informaticos voice : +34 58 243178 ETS Ingenieria Informatica Universidad de Granada From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id TAA01886; Mon, 15 Jul 1996 19:11:08 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id SAA27574 for ; Mon, 15 Jul 1996 18:53:18 +0200 Received: from anduin.ocf.llnl.gov (anduin.ocf.llnl.gov [134.9.49.1]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id SAA01799 for ; Mon, 15 Jul 1996 18:53:16 +0200 Received: from max.ocf.llnl.gov by anduin.ocf.llnl.gov (4.1/SMI-4.0) id AA21369; Mon, 15 Jul 96 09:53:14 PDT Received: by max.ocf.llnl.gov (951211.SGI.8.6.12.PATCH1042/951211.SGI.AUTO) id JAA15039; Mon, 15 Jul 1996 09:20:36 -0700 From: "Nelson L. Max" Message-Id: <9607150920.ZM15037@max.ocf.llnl.gov> Date: Mon, 15 Jul 1996 09:20:30 -0700 X-Mailer: Z-Mail (3.2.0 26oct94 MediaMail) To: globillum@imag.fr Subject: Correction to Report on Dagstuhl and Porto rendering conferences Cc: almagro@goliat.ugr.es, xavier@ima.udg.es Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit I had claimed that the method used by Xavier Pueyo to generate uniformly distributed lines inside a sphere, by joining pairs of points randomly distributed on the sphere's surface, was incorrect, but Carlos Urena Almagro has pointed out that it is I who was mistaken. My reasoning was as follows. If uniformly distributed lines in a certain fixed direction w intersect the unit sphere, they will not be uniformly distributed on the surface area. Instead, lines making an angle of t with the surface normal at their point of intersection will be less dense by a factor of cos t, as in the geometrical reasoning behind Lambert's law. However, I neglected to consider the solid angle effect. It turns out that the chord length of the ray segment between sphere surface intersection points A and B, is twice cos t. Therefore, the solid angle intercepted by a surface area ds at A, as measured at B, is (ds cos t)/(2 cos t)^2 = ds/(4 cos t). The cos t in the denominator here cancels the cos t for the Lambert area distribution factor at B, so that the number of rays within an element ds dw, of differential area ds normal to the beam and differential solid angle dw, is constant. (The cos t for the Lambert factor at A is already present in the numerator at the left side of the above equation.) -- Nelson Max http://www.llnl.gov/graphics max2@llnl.gov Lawrence Livermore National Laboratory (510) 422-4074 7000 East Avenue fax (510) 423-8704 Livermore, CA 94550, USA From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id TAA10616; Tue, 16 Jul 1996 19:39:20 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.11/8.6.9) with ESMTP id SAA28311 for ; Tue, 16 Jul 1996 18:49:58 +0200 Received: from anduin.ocf.llnl.gov (anduin.ocf.llnl.gov [134.9.49.1]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id SAA06893 for ; Tue, 16 Jul 1996 18:49:56 +0200 Received: from max.ocf.llnl.gov by anduin.ocf.llnl.gov (4.1/SMI-4.0) id AA21822; Tue, 16 Jul 96 09:49:54 PDT Received: by max.ocf.llnl.gov (951211.SGI.8.6.12.PATCH1042/951211.SGI.AUTO) for globillum@imag.fr id JAA16546; Tue, 16 Jul 1996 09:49:53 -0700 From: "Nelson L. Max" Message-Id: <9607160949.ZM16542@max.ocf.llnl.gov> Date: Tue, 16 Jul 1996 09:49:45 -0700 X-Mailer: Z-Mail (3.2.0 26oct94 MediaMail) To: globillum@imag.fr Subject: Another Correction to Report on Dagstuhl Mime-Version: 1.0 Content-Type: text/plain; charset=windows-1252; format=flowed X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Content-Description: Text Content-Type: text/plain X-Zm-Decoding-Hint: mimencode -q -u My first attempt at a broadcast message to globillum has certainly generated a lot of comment. Dieter Fellner writes that I have attributed too much to his group at Darmstadt. Here is the text of his meaasge. Dear Nelson, May I suggest a minor change to your report on the Dagstuhl workshop? You write > Dieter Fellner, working with Stefan MŸller's group at Darmstadt, > showed how real time rendering of radiosity scenes could be accomplished > on environments with the order of a million polygons, and presented an > impressive video of additions to the Frankfort airport. Well, I don't know how the two presentations could be linked so closely. And of course, it's quite flattering for my group. But truth is, that our two groups have not cooperated in this activity. My group has been working on a graphics architecture called MRT and as one of the more interesting applications I talked about the simulation of radio wave propagation in urban environments used in the planing of micro cells for mobile phone networks as well as on the consistent handling of approximative rendering and radiosity, both based of a clever use of a data structure derived from the windged edge data structure. As I don't want to take credit for things we haven't done and your mail reached a large number of people I would like to ask you to consider a revised version of your report. Best regards, Dieter ____________________________________________________________________________ -- Nelson Max http://www.llnl.gov/graphics max2@llnl.gov Lawrence Livermore National Laboratory (510) 422-4074 7000 East Avenue fax (510) 423-8704 Livermore, CA 94550, USA From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id WAA05150; Thu, 18 Jul 1996 22:02:21 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.13-durand/8.6.9) with ESMTP id VAA06331 for ; Thu, 18 Jul 1996 21:24:02 +0200 Received: from igw2.watson.ibm.com (igw2.watson.ibm.com [129.34.139.6]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id VAA24174 for ; Thu, 18 Jul 1996 21:24:01 +0200 Received: from mailhub1.watson.ibm.com (mailhub1.watson.ibm.com [9.2.249.31]) by igw2.watson.ibm.com (8.7.4/8.7.1) with ESMTP id PAA20324 for ; Thu, 18 Jul 1996 15:24:27 -0400 Received: from watngi01.watson.ibm.com (watngi01.watson.ibm.com [9.2.235.20]) by mailhub1.watson.ibm.com (8.7.1/07-17-96) with SMTP id PAA18831 for ; Thu, 18 Jul 1996 15:23:59 -0400 Received: by watngi01.watson.ibm.com (IBM OS/2 SENDMAIL VERSION 1.3.17/07-11-96 ) id AA1959; Thu, 18 Jul 96 15:23:58 -0400 Message-Id: <9607181923.AA1959@watngi01.watson.ibm.com> Received: from IBM Research with "Lotus Notes Mail Gateway for SMTP" id D7FA55E00701DE978525636B006912B1; Thu, 18 Jul 96 15:23:57 To: globillum From: Holly Rushmeier/Watson/IBM Research Date: 18 Jul 96 15:22:09 Subject: Globillum at SIGGRAPH? Mime-Version: 1.0 Content-Type: Text/Plain; charset=windows-1252; format=flowed X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Unless I missed something, nobody has said anything about a globillum get together at SIGGRAPH. Last years was the best discussion we have had, people were actually willing to bring up questions instead of staring at each other. I enjoyed hearing Nelson's comments on the conferences he went to. Perhaps some more people could summarize interesting papers from the Rendering workshop and other meetings. Also, the first session of papers is on Image-Based modelling and rendering. I would like to hear what people think of the image-based trend as far as how we compute illumination, and which of the proposed techniques looks the most promising. There is a papers "break-out" room, Rm 55 in the convention center, that we could meet at noon on Wednesday, right after the first session. Alright, I have something of an outside motivation for this. Every year they have one of these rooms reserved to discuss papers that are generally vacant, and I want to make this the first year people really use them to discuss papers. -- Holly From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id UAA26001; Fri, 26 Jul 1996 20:26:38 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.13-durand/8.6.9) with ESMTP id UAA23665 for ; Fri, 26 Jul 1996 20:04:33 +0200 Received: from irz201.inf.tu-dresden.de (irz201.inf.tu-dresden.de [141.76.1.10]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id UAA00623 for ; Fri, 26 Jul 1996 20:04:16 +0200 Received: by irz201.inf.tu-dresden.de (8.6.12/8.6.12-s1) id UAA20940 for globillum@imag.fr; Fri, 26 Jul 1996 20:03:40 +0200 From: "Nguyen, D.C." Message-Id: <199607261803.UAA20940@irz201.inf.tu-dresden.de> Subject: Comments for Diplom-Thesis To: Global Illumination List Date: Fri, 26 Jul 1996 20:03:39 +0200 (MESZ) X-Mailer: ELM [version 2.4 PL25 ME8b] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hi, The prereleased version of my diplom (in german!) could be found at: http://www.rz.tu-ilmenau.de/~juhu/Diplom/juhudip.ps.gz Be warned!(I've spend 1 year for hacking, but only 1 week for writing..:) Below are some highlights of this work: -Improvements for classical speedup-methodes, i.a: - the use of coherence for speedup-methodes (1D,2D,3D,5D) - projected area weighted, object intersection cost weighted ABVH - balanced BSP (to avoid the "Teapot in a football stadium" problem) - adaptive, "on the fly" subdivided Vista/Light-Buffer, applicable for volume-lightsources and extended cameras (There is a methode to avoid the "exhaustive classification/reclassification" effects, caused by Monte-Carlo-rays bundles near a big lightsource) - 5D Ray Classification for groups of pointlightsources or for a volume-lightsource w/ complicated shape -Comparisons: - Heuristics for efficiencies/defficienies of classical methodes - How to determine the complexity of a scene ? - What methode is best (hehe) ? -Hybrid-speeedup: - When to use, and how ? - Implemention of some hybrid shemes, such as hybrid-subdivision, local optimizaion for shadow/eye-rays (adaptive Vista/Light-Buffer for eye/shadow rays balaced BSP for secondary rays), generalized Polymorph-Caching etc.. - Some speculations on hybrid-methodes, not much infomative... I would like to hear your comments on this work....Thanks in advance, --JuHu /\__ Nguyen Duc Cuong (aka JuHu) - CG-student +- / -> Home /__\ \ EMail : juhu@rz.tu-ilmenau.de +- /GX -> GX/GENERIC \__/ WWW : http://www.rz.tu-ilmenau.de/~juhu -+- /GX/RTEvol -> RTEvol From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id RAA13173; Thu, 1 Aug 1996 17:29:19 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.13-durand/8.6.9) with ESMTP id QAA09737 for ; Thu, 1 Aug 1996 16:21:26 +0200 Received: from central.cis.upenn.edu (CENTRAL.CIS.UPENN.EDU [158.130.12.2]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id QAA04053 for ; Thu, 1 Aug 1996 16:21:24 +0200 Received: from graphics.cis.upenn.edu (GRAPHICS.CIS.UPENN.EDU [158.130.2.10]) by central.cis.upenn.edu (8.6.12/UPenn 1.4) with ESMTP id KAA23710 for ; Thu, 1 Aug 1996 10:21:22 -0400 Received: from LOCALHOST by graphics.cis.upenn.edu id KAA10463; Thu, 1 Aug 1996 10:21:21 -0400 Posted-Date: Thu, 1 Aug 1996 10:21:21 -0400 Message-Id: <199608011421.KAA10463@graphics.cis.upenn.edu> X-Mailer: exmh version 1.6.7 5/3/96 To: globillum@imag.fr cc: jnimerof@graphics.cis.upenn.edu Subject: Siggraph Date: Thu, 01 Aug 96 10:21:21 -0400 From: "Jeffry S. Nimeroff" X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Hello all, I'm dropping this mail message to all the globillumers going to Siggraph. Please drop me a line if you are interested in 'touring' New Orleans. I have been there about 10 times, and know the city reasonably well :-). We can hit the garden district, voodoo museum, or just stay on Bourbon street for a Lucky Dog (when you get there you'll understand. To show I'm a sport, this offer includes those people who I owe a drink (Porto). You guys know who you are. See you in New Orleans. I am staying at the Holiday Inn Chateau LeMoyne from Tuesday through Sunday. -Jeff From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id RAA20849; Sat, 3 Aug 1996 17:51:03 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.13-durand/8.6.9) with ESMTP id RAA25401 for ; Sat, 3 Aug 1996 17:27:08 +0200 Received: from central.cis.upenn.edu (CENTRAL.CIS.UPENN.EDU [158.130.12.2]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id RAA29839 for ; Sat, 3 Aug 1996 17:27:07 +0200 Received: from graphics.cis.upenn.edu (GRAPHICS.CIS.UPENN.EDU [158.130.2.10]) by central.cis.upenn.edu (8.6.12/UPenn 1.4) with ESMTP id LAA16925 for ; Sat, 3 Aug 1996 11:27:06 -0400 Received: from LOCALHOST by graphics.cis.upenn.edu id LAA29615; Sat, 3 Aug 1996 11:27:05 -0400 Posted-Date: Sat, 3 Aug 1996 11:27:05 -0400 Message-Id: <199608031527.LAA29615@graphics.cis.upenn.edu> X-Mailer: exmh version 1.6.7 5/3/96 To: globillum@imag.fr cc: jnimerof@graphics.cis.upenn.edu Subject: New Orleans Date: Sat, 03 Aug 96 11:27:05 -0400 From: "Jeffry S. Nimeroff" X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Hello all, So far I have received mail from a handfull of people about touring NO. In order to save bandwidth, I will be posting a message on the message board under the name "globillum". Please don't take the message (so everyone who wants to can read it). I will place some suggestions about when we might meet, etc. I will try to coordinate everything from there. I am staying at the Holiday Inn Chateau LeMoyne. You can always get me there. See you in NO. -Jeff p.s. I am taking the hotel information for everyone who responded, so I can also try to track you down. From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id AAA01003; Sat, 31 Aug 1996 00:33:51 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.13-durand/8.6.9) with ESMTP id AAA09221 for ; Sat, 31 Aug 1996 00:13:35 +0200 Received: from june.cs.washington.edu (june.cs.washington.edu [128.95.1.4]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id AAA16588 for ; Sat, 31 Aug 1996 00:13:34 +0200 Received: (danix@localhost) by june.cs.washington.edu (8.7.5/7.2ju) id PAA08139 for globillum@imag.fr; Fri, 30 Aug 1996 15:13:32 -0700 From: Dani Lischinski Message-Id: <199608302213.PAA08139@june.cs.washington.edu> Subject: terminology question To: globillum@imag.fr Date: Fri, 30 Aug 1996 15:13:31 -0700 (PDT) X-Mailer: ELM [version 2.4 PL23] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hi globillumers, Is there a name for incoming flux per unit PROJECTED area? Note that this is different from irradiance (incoming flux per unit area). If there's a name, is there also a symbol or letter commonly used to represent this quantity? Thanks a bunch, Dani From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id BAA01085; Sat, 31 Aug 1996 01:38:54 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.13-durand/8.6.9) with ESMTP id BAA09287 for ; Sat, 31 Aug 1996 01:27:03 +0200 Received: from mercury.uniserve.com (mercury.uniserve.com [204.191.197.248]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id BAA17432 for ; Sat, 31 Aug 1996 01:27:00 +0200 Received: from van0227.tvs.net (van0227.tvs.net [204.191.197.67]) by mercury.uniserve.com (8.7.5/8.7.3) with SMTP id QAA06338 for ; Fri, 30 Aug 1996 16:20:35 -0700 (PDT) Date: Fri, 30 Aug 1996 16:20:35 -0700 (PDT) Message-Id: <199608302320.QAA06338@mercury.uniserve.com> X-Sender: iashdown@pop.uniserve.com X-Mailer: Windows Eudora Version 2.0.3 Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed To: globillum@imag.fr From: Ian Ashdown Subject: Re: terminology question X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit >Hi globillumers, > >Is there a name for incoming flux per unit PROJECTED area? >Note that this is different from irradiance (incoming flux >per unit area). If there's a name, is there also a symbol >or letter commonly used to represent this quantity? > >Thanks a bunch, > The lighting community's bible, ANSI/IES RP-16, "Nomenclature and Definitions for Illuminating Engineering," neatly sidesteps this issue by saying in Clause 3.3 (which admittedly refers to illuminance rather than irradiance) that the surface "need not be a physical surface; it may also be a mathematical plane." In other words, their definition of irradiance/illuminance applies both to physical surfaces and imaginary surfaces (which can include those normal to the direction of the incident flux). You might find what you are looking for in Moon and Spencer's "The Photic Field" (MIT Press, 1981), where I think they called it "pharosage." However, adopting any of Parry Moon's terminology (apart from his "radiosity") is an open invitation to be ignored by the old guard in the IESNA :+) Ian Ashdown, P. Eng. | READ THE BOOK! Research & Development Manager | Radiosity: A Programmer's Perspective Ledalite Architectural Products Inc. | by Ian Ashdown | John Wiley & Sons, 1994 Visit http://www.ledalite.com | (Sneaky Internet Advertising) From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id TAA07302; Mon, 2 Sep 1996 19:45:55 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.13-durand/8.6.9) with ESMTP id TAA11331 for ; Mon, 2 Sep 1996 19:04:46 +0200 Received: from sys4.cambridge.uk.psi.net (sys4.cambridge.uk.psi.net [154.32.106.14]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id TAA21357 for ; Mon, 2 Sep 1996 19:03:56 +0200 Received: from lightwk.uucp by sys4.cambridge.uk.psi.net (8.7.5/SMI-5.5-UKPSINet) id RAA08434; Mon, 2 Sep 1996 17:15:40 +0100 (BST) From: Neil Gatenby Date: Mon, 2 Sep 96 16:57:55 BST Message-Id: <28453.9609021557@lightwork.co.uk> To: globillum@imag.fr Subject: goniometric file formats X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Hi globillum folk; I have a question regarding file formats used to store luminaire goniometric data; any help would be much appreciated. Which file formats are in common useage in Japan and Germany? I know the UK is keen on CIBSE. I know the US is keen on IESNA. I know a little about the CIE format (what I've read in Glassner's "Principles ...") But, I don't know what's popular in these two large market areas. Thanks in advance Neil Neil Gatenby, | LightWork Design, Senior Graphics Programmer, | 60 Clarkehouse Road, email: neil@lightwork.co.uk | Sheffield, S10 2LH, England. voice: (+44) (0)114 266 8404 ..... fax: (+44) (0)114 266 1383 From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id XAA01079; Tue, 3 Sep 1996 23:03:35 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.13-durand/8.6.9) with ESMTP id WAA02806 for ; Tue, 3 Sep 1996 22:36:06 +0200 Received: from mercury.uniserve.com (mercury.uniserve.com [204.191.197.248]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id WAA18869 for ; Tue, 3 Sep 1996 22:36:05 +0200 Received: from van0125.TVS.NET (van0125.TVS.NET [204.191.197.35]) by mercury.uniserve.com (8.7.5/8.7.3) with SMTP id NAA05863 for ; Tue, 3 Sep 1996 13:29:10 -0700 (PDT) Date: Tue, 3 Sep 1996 13:29:10 -0700 (PDT) Message-Id: <199609032029.NAA05863@mercury.uniserve.com> X-Sender: iashdown@pop.uniserve.com (Unverified) X-Mailer: Windows Eudora Version 1.4.4 Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed To: globillum@imag.fr From: Ian Ashdown Subject: Global illumination bibliography update X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit ANNOUNCE: 96/09/01 Release of RADBIB96 -------------------------------------- RADBIB96 is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. A total of 41 new references have been added since its last release on July 1, 1996, bringing the total to 975 references. This bibliography is available in refer format (ASCII text) as RADBIB96.TXT (with a release date of September 1, 1996) from: http://www.ledalite.com/library-/rrt.htm and as compressed RadBib96.Z from: ftp://hobbes.lbl.gov/pub/doc A gzip-compressed BibTex-format version is available from: ftp.cs.columbia.edu/archives/bibliographies/Graphics/rad.html but it may be a previous release. As always, it is time-consuming and sometimes difficult to track down conference papers and theses on radiosity and global illumination. If you know of a relevant reference that is not included in the bibliography, please let me know so that I can include it in the next release. From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id PAA02001; Fri, 6 Sep 1996 15:53:06 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.13-durand/8.6.9) with ESMTP id PAA10390 for ; Fri, 6 Sep 1996 15:25:24 +0200 Received: from btcgate.btc.uwe.ac.uk (btcgate.btc.uwe.ac.uk [164.11.100.1]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id PAA28497 for ; Fri, 6 Sep 1996 15:25:16 +0200 From: jpt@btc.uwe.ac.uk Received: by btcgate.btc.uwe.ac.uk (4.1/SMI-4.1) id AA06636; Fri, 6 Sep 96 14:24:10 BST Received: from hal-9000.btc.uwe.ac.uk(164.11.0.3) by sparky via smap (V1.3mjr) id sma006627; Fri Sep 6 14:23:10 1996 Received: from marvin.uwe.ac.uk by btc.uwe.ac.uk (4.1/SMI-4.1-BTC-06) for jpt@hal/globillum@imag.fr id AA08225; Fri, 6 Sep 96 14:23:06 BST Date: Fri, 6 Sep 96 14:23:06 BST Message-Id: <9609061323.AA08225@btc.uwe.ac.uk> To: globillum@imag.fr Subject: Voxel neighbours in octrees X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Hello colleagues I have a problem relating to finding neighbouring voxels in octrees and feel sure this must have been addressed previously. I want to be able to find all the neighbouring (adjacent in space) voxels from a given voxel stored in an octree. It seems feasible that an operation based on traversal of the octree will allow neighbouring voxels to be discovered. Thanks in advance for any assistance john -------------------------------------------------------------------------- Jonathan Tidmus jpt@ics.uwe.ac.uk Researcher Intelligent Computer Systems Centre phone: +44 (0)117 9656261 ext 3357 University of the West of England fax: +44 (0)117 9750416 Bristol BS16 1QY From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id RAA02732; Fri, 6 Sep 1996 17:18:36 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.13-durand/8.6.9) with ESMTP id QAA12333 for ; Fri, 6 Sep 1996 16:43:27 +0200 Received: from safran.imag.fr (safran.imag.fr [129.88.31.3]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id QAA03480; Fri, 6 Sep 1996 16:43:26 +0200 Received: (sillion@localhost) by safran.imag.fr (8.6.10/8.6.4) id QAA03893; Fri, 6 Sep 1996 16:45:18 +0200 From: Francois Sillion Message-Id: <199609061445.QAA03893@safran.imag.fr> Subject: Re: Voxel neighbours in octrees To: jpt@btc.uwe.ac.uk Date: Fri, 6 Sep 1996 16:45:18 +0200 (MDT) Cc: globillum@imag.fr In-Reply-To: <9609061323.AA08225@btc.uwe.ac.uk> from "jpt@btc.uwe.ac.uk" at Sep 6, 96 02:23:06 pm Reply-To: Francois.Sillion@imag.fr X-Mailer: ELM [version 2.4 PL23] MIME-Version: 1.0 Content-Type: text/plain; charset=windows-1252; format=flowed Content-Transfer-Encoding: 8bit X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 > Hello colleagues > > I have a problem relating to finding neighbouring voxels in octrees and > feel sure this must have been addressed previously. > > I want to be able to find all the neighbouring (adjacent in space) voxels > from a given voxel stored in an octree. It seems feasible that an > operation based on traversal of the octree will allow neighbouring > voxels to be discovered. > I have only done it with quadtrees, but I believe that you will find simple code that does precisely that in one of H. Samet's book on hierarchical data structures. @book{Samet90, author = {Hanan Samet}, title = {The Design and Analysis of Spatial Data Structures}, publisher = {Addison-Wesley}, address = {Reading, Massachusetts}, year = {1990} } @book{Samet, author = {Hanan Samet}, title = {Applications of Spatial Data Structures}, publisher = {Addison-Wesley}, address = {Reading, Massachusetts}, year = {1990} } +------------------+------------------------------------------------------+ | Francois SILLION | iMAGIS - GRAVIR/IMAG, B.P. 53, 38041 Grenoble Cedex 9| | ' | France. Tel:(+33) 76 51 43 54 - Fax:(+33) 76 44 66 75| +------------------+----------+-------------------------------------------+ | Francois.Sillion@imag.fr | http://w3imagis.imag.fr/~Francois.Sillion | +-----------------------------+-------------------------------------------+ From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id UAA03364; Fri, 6 Sep 1996 20:31:56 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.13-durand/8.6.9) with ESMTP id UAA15163 for ; Fri, 6 Sep 1996 20:06:24 +0200 Received: from mail2.microsoft.com (mail2.microsoft.com [131.107.3.42]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id UAA12219; Fri, 6 Sep 1996 20:06:20 +0200 Received: by mail2.microsoft.com with SMTP (Microsoft Exchange Server Internet Mail Connector Version 4.0.994.24) id <01BB9BE2.E8CC06E0@mail2.microsoft.com>; Fri, 6 Sep 1996 11:02:35 -0700 Message-ID: From: Andrew Glassner To: "'jpt@btc.uwe.ac.uk'" , "'Francois.Sillion@imag.fr'" Cc: "'globillum@imag.fr'" Subject: RE: Voxel neighbours in octrees Date: Fri, 6 Sep 1996 11:02:32 -0700 X-Mailer: Microsoft Exchange Server Internet Mail Connector Version 4.0.994.24 Encoding: 48 TEXT X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit I believe they're called "Neighbor Pointers" - that might be a good place to start looking in the index. >---------- >From: Francois Sillion[SMTP:Francois.Sillion@imag.fr] >Sent: Friday, September 06, 1996 7:45 AM >To: jpt@btc.uwe.ac.uk >Cc: globillum@imag.fr >Subject: Re: Voxel neighbours in octrees > >> Hello colleagues >> >> I have a problem relating to finding neighbouring voxels in octrees and >> feel sure this must have been addressed previously. >> >> I want to be able to find all the neighbouring (adjacent in space) voxels >> from a given voxel stored in an octree. It seems feasible that an >> operation based on traversal of the octree will allow neighbouring >> voxels to be discovered. >> > >I have only done it with quadtrees, but I believe that you will find >simple code that does precisely that in one of H. Samet's book on >hierarchical data structures. > >@book{Samet90, > author = {Hanan Samet}, > title = {The Design and Analysis of Spatial Data Structures}, > publisher = {Addison-Wesley}, > address = {Reading, Massachusetts}, > year = {1990} >} > >@book{Samet, > author = {Hanan Samet}, > title = {Applications of Spatial Data Structures}, > publisher = {Addison-Wesley}, > address = {Reading, Massachusetts}, > year = {1990} >} > >+------------------+------------------------------------------------------+ >| Francois SILLION | iMAGIS - GRAVIR/IMAG, B.P. 53, 38041 Grenoble Cedex 9| >| ' | France. Tel:(+33) 76 51 43 54 - Fax:(+33) 76 44 66 75| >+------------------+----------+-------------------------------------------+ >| Francois.Sillion@imag.fr | http://w3imagis.imag.fr/~Francois.Sillion | >+-----------------------------+-------------------------------------------+ > From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id XAA03617; Fri, 6 Sep 1996 23:31:47 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.13-durand/8.6.9) with ESMTP id XAA15596 for ; Fri, 6 Sep 1996 23:14:53 +0200 Received: from HOSTESS.GRAPHICS.CS.CMU.EDU (HOSTESS.GRAPHICS.CS.CMU.EDU [128.2.206.188]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id XAA18022; Fri, 6 Sep 1996 23:14:52 +0200 From: Paul.Heckbert@HOSTESS.GRAPHICS.CS.CMU.EDU Message-Id: <199609062114.XAA18022@imag.imag.fr> Date: Fri, 6 Sep 96 17:03:59 EDT To: Francois.Sillion@imag.fr, glassner@microsoft.com, jpt@btc.uwe.ac.uk Subject: RE: Voxel neighbours in octrees Cc: globillum@imag.fr X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit One of the methods that Samet describes does not require neighbor pointers (although that is certainly one way to do it), but instead you ascend the tree until you can step in the direction you want, then you descend the tree, staying as close spatially to the previous point as possible, until you hit a leaf, or get to the level of the tree that you desire. With this method, you don't need neighbor pointers, just 8 child pointers and 1 parent pointer. Samet shows, as I recall, that you go up and down 2 times, on average, i.e. that the average cost to find a neighbor is O(1). If you found neighbors by starting at the root every time, it would cost O(depth). >> jpt@btc.uwe.ac.uk >> >> I have a problem relating to finding neighbouring voxels in octrees and >> feel sure this must have been addressed previously. Paul Heckbert Computer Science Dept., Carnegie Mellon University 5000 Forbes Ave, Pittsburgh PA 15213-3891, USA ph@cs.cmu.edu http://www.cs.cmu.edu/~ph From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id OAA04616; Sat, 7 Sep 1996 14:31:23 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.13-durand/8.6.9) with ESMTP id OAA17429 for ; Sat, 7 Sep 1996 14:03:23 +0200 Received: from silter.silesia.ternet.pl ([194.204.187.254]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id OAA12670 for ; Sat, 7 Sep 1996 14:03:20 +0200 Received: from miki.wro.ternet.pl (root@ppp-cen66.wroclaw.tpnet.pl [194.204.169.66]) by silter.silesia.ternet.pl (8.7.4/8.6.9) with ESMTP id OAA16268 for ; Sat, 7 Sep 1996 14:03:09 +0200 (MET DST) Received: from loc1.wro.ternet.pl (loc1 [10.0.0.11]) by miki.wro.ternet.pl (8.6.12/8.6.12) with SMTP id OAA11855 for ; Sat, 7 Sep 1996 14:03:05 +0200 Received: by loc1.wro.ternet.pl with Microsoft Mail id <01BB9CC6.143FBE00@loc1.wro.ternet.pl>; Sat, 7 Sep 1996 14:08:44 +-200 Message-ID: <01BB9CC6.143FBE00@loc1.wro.ternet.pl> From: Slawomir Kilanowski To: "'globillum list'" Date: Sat, 7 Sep 1996 14:07:21 +-200 MIME-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 8bit X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Dear Collegues, I am working on speed-up of global illumination calculations and ray tracing for scenes containing huge number of lights. Except some visibility pre-processing I would like to limit number of considered lights for given space points doing some "light importance" pre-processing. The tempting idea is to partition scene space into regions tied with ordered lists of lights that can influence them, then, during calculation, process only those "significant" lights in order of their importance. I have browsed RadBIB and ACM Siggraph bibliographies but I have not found any related papers. Have I missed something important ? Does anybody know about some previous work on such or similar concepts ? Thanks in advance, Slawek ================================================================ Slawomir Kilanowski metagram@wro.ternet.pl METAGRAM, Swieradowska 73/23, 50-559 Wroclaw, Poland Phone/Fax : +48-(71)-731519 ================================================================ From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id WAA05198; Sat, 7 Sep 1996 22:34:57 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.13-durand/8.6.9) with ESMTP id WAA18339 for ; Sat, 7 Sep 1996 22:19:21 +0200 Received: from freenet.hut.fi (freenet.hut.fi [130.233.208.40]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id WAA26484 for ; Sat, 7 Sep 1996 22:19:20 +0200 Received: from frodo.leader.es (pippin.leader.es [194.179.72.212]) by freenet.hut.fi (8.7.5/8.7.3) with SMTP id XAA22192 for ; Sat, 7 Sep 1996 23:19:16 +0300 (EET DST) Received: by frodo.leader.es with Microsoft Mail id <01BB9D0B.20434060@frodo.leader.es>; Sat, 7 Sep 1996 22:22:59 +-200 Message-ID: <01BB9D0B.20434060@frodo.leader.es> From: Marcos Fajardo Orellana To: "'globillum@imag.fr'" Subject: RE: Date: Sat, 7 Sep 1996 21:02:51 +-200 MIME-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 8bit X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Slawomir Kilanowski wrote: >Dear Collegues, > > I am working on speed-up of global illumination calculations and ray tracing for scenes >containing huge number of lights. Except some visibility pre-processing I would like to >limit number of considered lights for given space points doing some "light importance" >pre-processing. The tempting idea is to partition scene space into regions tied with >ordered lists of lights that can influence them, then, during calculation, process only >those "significant" lights in order of their importance. > > I have browsed RadBIB and ACM Siggraph bibliographies but I have not found any >related papers. Have I missed something important ? Does anybody know about some >previous work on such or similar concepts ? > >Thanks in advance, > >Slawek I think these two papers could be of interest to you, Ward, Gregory, "The RADIANCE Lighting Simulation and Rendering System," Computer Graphics, pp. 459-472, July 1994 Ward, Gregory, "Adaptive Shadow Testing for Ray Tracing," Second EUROGRAPHICS Workshop on Rendering, Barcelona, Spain, April 1991 Peter Shirley has some excellent work on sampling light sources as well. This one is on-line (check out his homepage at http://www.cs.utah.edu/~shirley ), Shirley, Peter, "Direct Lighting Calculation by Monte Carlo Integration," Second EUROGRAPHICS Workshop on Rendering, June 1991 (?) Hope this helps Marcos http://www.geocities.com/TimesSquare/2143 From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id MAA08995; Mon, 9 Sep 1996 12:57:39 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.13-durand/8.6.9) with ESMTP id MAA26396 for ; Mon, 9 Sep 1996 12:34:21 +0200 Received: from m1.cs.man.ac.uk (m1.cs.man.ac.uk [130.88.13.4]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id MAA04606 for ; Mon, 9 Sep 1996 12:34:18 +0200 Received: from r9.cs.man.ac.uk by m1.cs.man.ac.uk (4.1/SMI-4.1:AL6) id AA09212; Mon, 9 Sep 96 11:34:12 BST Date: Mon, 9 Sep 96 11:34:09 BST From: Simon Gibson Message-Id: <9609091034.AA02666@r9.cs.man.ac.uk> To: globillum@imag.fr Subject: Re: X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Slawomir Kilanowski wrote: >Dear Collegues, > > I am working on speed-up of global illumination calculations and ray tracing for scenes >containing huge number of lights. Except some visibility pre-processing I would like to >limit number of considered lights for given space points doing some "light importance" >pre-processing. The tempting idea is to partition scene space into regions tied with >ordered lists of lights that can influence them, then, during calculation, process only >those "significant" lights in order of their importance. > > I have browsed RadBIB and ACM Siggraph bibliographies but I have not found any >related papers. Have I missed something important ? Does anybody know about some >previous work on such or similar concepts ? > >Thanks in advance, > >Slawek You might want to check out: %A Kurt Zimmerman %A Peter Shirley %T A Two-Pass Realistic Image Synthesis Method for Complex Scenes %E P. M. Hanrahan %E W. Purgathofer %B Rendering Techniques '95 (Proceedings of the Sixth Eurographics Workshop on Rendering) %I Springer-Verlag %C New York, NY %D 1995 %P 284-295 %O ISBN 3-211-82733-1 available as an Indiana University Technical Report - ftp://ftp.cs.indiana.edu/pub/techreports/TR434.ps.Z Simon - From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id UAA10905; Mon, 9 Sep 1996 20:32:24 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.13-durand/8.6.9) with ESMTP id TAA03094 for ; Mon, 9 Sep 1996 19:52:09 +0200 Received: from zfr200.ZUMtOBEL.co.at (zfr200.ZUMtOBEL.co.at [146.108.200.200]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id TAA26385 for ; Mon, 9 Sep 1996 19:52:07 +0200 Received: from localhost by zfr200.ZUMtOBEL.co.at; (5.65v3.2/1.1.8.2/20Jun96-0712PM) id AA06732; Mon, 9 Sep 1996 19:59:47 +0200 Received: by oedo1a.zumtobel.co.at (UCX V4.0-10B, OpenVMS V5.5-2H4 VAX); Mon, 9 Sep 1996 19:51:34 +0200 Received: by bug.cophos.co.at (940816.SGI.8.6.9/940406.SGI.AUTO) for globillum@imag.fr id TAA11640; Mon, 9 Sep 1996 19:51:29 +0200 From: Martin Lob Message-Id: <199609091751.TAA11640@bug.cophos.co.at> Subject: Re: goniometric file formats To: globillum@imag.fr Date: Mon, 9 Sep 1996 19:51:29 +0200 (CETDST) In-Reply-To: <28453.9609021557@lightwork.co.uk> from "Neil Gatenby" at Sep 2, 96 04:57:55 pm Reply-To: ml@cophos.co.at Organization: Cophos Development Team, Zumtobel Licht, Dornbirn, Austria Phone: +43-5572-390-1383 Fax: +43-5572-390-246 X-Mailer: ELM [version 2.4 PL24 PGP3 *ALPHA*] Mime-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Neil Gatenby wrote ... | From: Neil Gatenby | Date: Mon, 2 Sep 96 16:57:55 BST | Message-Id: <28453.9609021557@lightwork.co.uk> | To: globillum@imag.fr | Subject: goniometric file formats | | | Hi globillum folk; | | I have a question regarding file formats used to store luminaire | goniometric data; any help would be much appreciated. | | Which file formats are in common useage in Japan and Germany? In Germany the EULUMDAT format is used. It was introduced by Axel Stockmar. A copy of the format description aswell as files in EULUMDAT are available from ZUMTOBEL. | | I know the UK is keen on CIBSE. | I know the US is keen on IESNA. | I know a little about the CIE format (what I've read in Glassner's | "Principles ...") | | But, I don't know what's popular in these two large market areas. | | Thanks in advance | Neil | | Neil Gatenby, | LightWork Design, | Senior Graphics Programmer, | 60 Clarkehouse Road, | email: neil@lightwork.co.uk | Sheffield, S10 2LH, England. | voice: (+44) (0)114 266 8404 ..... fax: (+44) (0)114 266 1383 | -- \|/ ml@cophos.co.at http://www.cophos.co.at/~ml --O-- /|\ l Tel.: +43/5572/390-1383 ___ ___ m mmm mmm l Fax : +43/5572/390-650 / __\ /__ \ mm m m l ZUMTOBEL Licht GmbH / / \ / \ mm m m l Schweizerstr. 30 / / \ / \ m m m l A-6850 DORNBIRN | | \ m m martin . lob . Austria | | :-Q | | Prediction is very difficult, especially of the future! | | n_u__n___ From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id WAA11068; Mon, 9 Sep 1996 22:54:06 +0200 Received: from cosmos.imag.fr (cosmos.imag.fr [147.171.130.1]) by isis.imag.fr (8.6.13-durand/8.6.9) with ESMTP id WAA03475 for ; Mon, 9 Sep 1996 22:26:21 +0200 Received: from lsi.lsil.com (lsi.lsil.com [147.145.40.2]) by cosmos.imag.fr (8.6.13-durand/8.6.9) with ESMTP id WAA16936 for ; Mon, 9 Sep 1996 22:26:17 +0200 Received: from mhost.lsil.com (mhost.lsil.com [147.145.69.84]) by lsi.lsil.com with SMTP id NAA16618 (8.6.12/IDA-1.6 for ); Mon, 9 Sep 1996 13:16:10 -0700 Received: from sjs1 by mhost.lsil.com id AA12440 (4.1/SMI-4.1 for globillum@imag.fr); Mon, 9 Sep 96 13:15:51 PDT Received: from sj80.lsil.com by sjs1 (4.1/SMI-4.1) id AA26156; Mon, 9 Sep 96 13:15:51 PDT Date: Mon, 9 Sep 96 13:15:51 PDT From: Al Zimmerman Message-Id: <9609092015.AA26156@sjs1> To: globillum@imag.fr Subject: spatial subdivision X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit I've been researching spatial subdivision. Yes, I am aware of bounding boxes, octrees, and uniform spatial subdivision. I've seen references in the past of non-uniform grids for spatial subdivision. (not talking about octrees) in ray-tracing news somewhere from 1990-92 The only paper that seems to mention anything formal about this is "Accelerated ray tracing using non-uniform grids" by M. Gigante. After weeks of trying to contact the author, I have given up the pursuit. (He must not like my name) So, does anybody out there have any familiarity with non-uniform grids for spatial subdivision. For your info, I have my own ideas on how to construct non-uniform grids but have not seen any formal documentation on the subject. Anything from anybody would greatly appreciated, Anything ?????? Thanks in advance, Al Z From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id AAA11199; Tue, 10 Sep 1996 00:10:26 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.13-durand/8.6.9) with ESMTP id XAA03635 for ; Mon, 9 Sep 1996 23:46:41 +0200 Received: from grolsch.cs.ubc.ca (grolsch.cs.ubc.ca [142.103.6.9]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id XAA04330 for ; Mon, 9 Sep 1996 23:46:39 +0200 Received: from chaplin.cs.ubc.ca (fournier@chaplin.cs.ubc.ca [142.103.9.32]) by grolsch.cs.ubc.ca (8.6.12/8.6.9) with SMTP id OAA18322; Mon, 9 Sep 1996 14:46:14 -0700 Date: Mon, 9 Sep 1996 14:46:14 -0700 From: Alain Fournier Message-Id: <199609092146.OAA18322@grolsch.cs.ubc.ca> To: alz@lsil.com, globillum@imag.fr Subject: Re: spatial subdivision X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit You might find useful a look at Fournier, A., and Poulin, P., ``A Ray Tracing Accelerator Based on a Hierarchy of 1D Sorted Lists'', Proceedings of GI '93, Toronto, May 1993, pp. 53-61. We used a hierarchy of bounding boxes aligned with the axes. This of course determines an irregular grid on the scene, which is traversed by listing events (entering and exiting a box) in 1D lists (one per coordinates). Many interesting conclusions, but the first one: "it's hard to beat regular grid subdivision". From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id AAA11231; Tue, 10 Sep 1996 00:25:37 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.13-durand/8.6.9) with ESMTP id AAA03699 for ; Tue, 10 Sep 1996 00:07:13 +0200 Received: from wk309.nas.nasa.gov (wk309.nas.nasa.gov [129.99.64.29]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id AAA04970 for ; Tue, 10 Sep 1996 00:07:11 +0200 Received: (from uselton@localhost) by wk309.nas.nasa.gov (8.6.12/NAS.6.1) id PAA12723; Mon, 9 Sep 1996 15:07:07 -0700 Date: Mon, 9 Sep 1996 15:07:07 -0700 Message-Id: <199609092207.PAA12723@wk309.nas.nasa.gov> From: "Samuel P. Uselton" To: alz@lsil.com CC: globillum@imag.fr In-reply-to: <9609092015.AA26156@sjs1> (alz@lsil.com) Subject: Re: spatial subdivision Reply-to: uselton@nas.nasa.gov X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit I had an MS student who did a thesis on the topic many (7? 8?) years ago. The main paper got turned down for SIGGRAPH. The student took a job and I left academia, so we never got the "improved" version completed and accepted anywhere. However, a description of a hardware accelerator for it was accepted in a small conference. The student who did this work was Scott Senften (this year's SIGGRAPH Tutorial's chair); you should be able to reach him at scott@lgc.com or senften@siggraph.org. I know k-d trees and space partitioning trees (BSP-trees) have also been considered for this purpose, but I don't know if the work has been published. I hope that helps. Sam Uselton uselton@nas.nasa.gov From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id FAA11654; Tue, 10 Sep 1996 05:06:42 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.13-durand/8.6.9) with ESMTP id EAA04534 for ; Tue, 10 Sep 1996 04:53:39 +0200 Received: from zappa.cs.uncc.edu (zappa.cs.uncc.edu [152.15.35.2]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id EAA09895 for ; Tue, 10 Sep 1996 04:53:38 +0200 Received: from strauss.cs.uncc.edu by zappa.cs.uncc.edu (5.x/SMI-SVR4) id AA07466; Mon, 9 Sep 1996 22:40:37 -0400 Received: by strauss.cs.uncc.edu (5.x/SMI-SVR4) id AA01341; Mon, 9 Sep 1996 22:53:25 -0400 Message-Id: <9609100253.AA01341@strauss.cs.uncc.edu> From: "K. R." Date: Mon, 9 Sep 1996 22:53:25 GMT+447 X-Mailer: Mail User's Shell (7.1.1 5/02/90) To: globillum@imag.fr Subject: k-d trees in ray tracing.. X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit On Sep 9, 9:08pm, "Eric A. Haines" wrote: > Subject: Re: spatial subdivision > As far as non-uniform grids go, I come up empty beyond Gigante's work. > > > >K-d trees for ray-tracing are described in K.R.Subramanian's PhD > >thesis: > > An easier to obtain paper is: > > %A K.R. Subramanian > %A Donald S. Fussell > %T Automatic Termination Criteria for Ray Tracing Hierarchies > %J Proceedings of Graphics Interface '91 > %I Canadian Information Processing Society > %C Calgary, Alberta > %D June 1991 > %P 93-100 > %K octree Or, a postscript version of the above is available from my web page: http://www.cs.uncc.edu/~krs/publ.html I also have a postscript file of my thesis. Always willing to spread the word! > > Morgan-Kaufmann sells GI Proceedings (which I recommend; I've never been, but > the proceedings have some interesting and useful papers in these). > K.R. Subramanian is currently at krs@mail.cs.uncc.edu, UNC Charlotte. > > > >As for BSP-trees, I don't know of any paper describing their appli- > >cation to ray-tracing, but the following paper discusses ways of > >constructing good BSP-trees for ray-tracing: There is a tech report on it: B. Naylor, W. Thibault, "Application of BSP Trees to Ray Tracing and CSG Evaluation", TR GIT-CS 86/03, School of Inf. and Comp.Sc. Georgia Tech., 1986. Naylor can be reached at naylor@spatial-labs.com > There are six ray tracing papers with BSP in the title (and many other related > papers using octrees, a relative of BSP), and there are some other > papers by K.R. Subramanian on k-d trees (tech. reports, etc), check: > > http://wuarchive.wustl.edu/graphics/graphics/bib/ > or > ftp://wuarchive.wustl.edu/graphics/graphics/bib/ > > and get rtabs.shar.Z (which is Tom Wilson's collection of abstracts of hundreds > of ray tracing articles) and rtbib95.zip/tar.Z, which is Paul Heckbert's and > my collection of ray tracing references (somewhat dated, I've been too busy - > please do send me new references, I hope to get an update out before year's > end). > > Eric Haines > erich@eye.com >-- End of excerpt from "Eric A. Haines" -- krs -- K.R.Subramanian Phone: (704) 547-4872 Department of Computer Science FAX: (704) 547-3516 UNC Charlotte email: krs@zappa.cs.uncc.edu Charlotte, NC 28223-0001 WWW: http://www.cs.uncc.edu/~krs From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id CAA11401; Tue, 10 Sep 1996 02:47:56 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.13-durand/8.6.9) with ESMTP id CAA03973 for ; Tue, 10 Sep 1996 02:16:24 +0200 Received: from mail.cs.utexas.edu (mail.cs.utexas.edu [128.83.139.10]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id CAA06347 for ; Tue, 10 Sep 1996 02:16:23 +0200 Received: from mr-skullhead.cs.utexas.edu (ecamahor@mr-skullhead.cs.utexas.edu [128.83.138.79]) by mail.cs.utexas.edu (8.7.1/8.7.1) with ESMTP id TAA01577; Mon, 9 Sep 1996 19:12:00 -0500 (CDT) Received: by mr-skullhead.cs.utexas.edu (8.7.1/Client-1.4) id TAA07231; Mon, 9 Sep 1996 19:11:59 -0500 (CDT) Message-Id: <199609100011.TAA07231@mr-skullhead.cs.utexas.edu> From: Emilio Camahort Date: Mon, 9 Sep 1996 19:11:58 -0500 In-Reply-To: Message from "Samuel P. Uselton", date: Mon Sep 9 96, 15:07 X-Mailer: Mail User's Shell (7.2.5 10/14/92) To: globillum@imag.fr Subject: Re: spatial subdivision Cc: alz@lsil.com X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit >I know k-d trees and space partitioning trees (BSP-trees) have also >been considered for this purpose, but I don't know if the work has >been published. K-d trees for ray-tracing are described in K.R.Subramanian's PhD thesis: K.R.Subramanian "Adapting Search Structures to Scene Characteristics for Ray Tracing" Department of Computer Sciences, The University of Texas at Austin, Austin, TX 78712, December 1990 You may be able to obtain a copy from: trcenter@cs.utexas.edu As for BSP-trees, I don't know of any paper describing their appli- cation to ray-tracing, but the following paper discusses ways of constructing good BSP-trees for ray-tracing: B.Naylor "Constructing Good Partitioning Trees" Proceedings of Graphics Interface'93, 1993 Good luck!! Emilio ecamahor@cs.utexas.edu From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id DAA11462; Tue, 10 Sep 1996 03:16:27 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.13-durand/8.6.9) with ESMTP id DAA04236 for ; Tue, 10 Sep 1996 03:08:19 +0200 Received: from eye.eye.com (eye.eye.com [149.54.1.2]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id DAA06729 for ; Tue, 10 Sep 1996 03:08:17 +0200 Received: from hemlock (hemlock.eye.com) by eye.eye.com with SMTP ($Revision: 1.36.108.11 $/16.2) id AA127257694; Mon, 9 Sep 1996 21:08:14 -0400 Received: by hemlock (1.37.109.8/15.6) id AA05715; Mon, 9 Sep 1996 21:08:14 -0400 From: "Eric A. Haines" Message-Id: <9609100108.AA05715@hemlock> Subject: Re: spatial subdivision To: ecamahor@cs.utexas.edu Date: Mon, 9 Sep 96 21:08:13 EDT Cc: globillum@imag.fr In-Reply-To: <199609100011.TAA07231@mr-skullhead.cs.utexas.edu>; from "Emilio Camahort" at Sep 9, 96 7:11 pm Mailer: Elm [revision: 70.85] X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit As far as non-uniform grids go, I come up empty beyond Gigante's work. >K-d trees for ray-tracing are described in K.R.Subramanian's PhD >thesis: An easier to obtain paper is: %A K.R. Subramanian %A Donald S. Fussell %T Automatic Termination Criteria for Ray Tracing Hierarchies %J Proceedings of Graphics Interface '91 %I Canadian Information Processing Society %C Calgary, Alberta %D June 1991 %P 93-100 %K octree Morgan-Kaufmann sells GI Proceedings (which I recommend; I've never been, but the proceedings have some interesting and useful papers in these). K.R. Subramanian is currently at krs@mail.cs.uncc.edu, UNC Charlotte. >As for BSP-trees, I don't know of any paper describing their appli- >cation to ray-tracing, but the following paper discusses ways of >constructing good BSP-trees for ray-tracing: There are six ray tracing papers with BSP in the title (and many other related papers using octrees, a relative of BSP), and there are some other papers by K.R. Subramanian on k-d trees (tech. reports, etc), check: http://wuarchive.wustl.edu/graphics/graphics/bib/ or ftp://wuarchive.wustl.edu/graphics/graphics/bib/ and get rtabs.shar.Z (which is Tom Wilson's collection of abstracts of hundreds of ray tracing articles) and rtbib95.zip/tar.Z, which is Paul Heckbert's and my collection of ray tracing references (somewhat dated, I've been too busy - please do send me new references, I hope to get an update out before year's end). Eric Haines erich@eye.com From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id PAA14527; Tue, 10 Sep 1996 15:14:42 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.13-durand/8.6.9) with ESMTP id OAA13191 for ; Tue, 10 Sep 1996 14:42:43 +0200 Received: from irz201.inf.tu-dresden.de (irz201.inf.tu-dresden.de [141.76.1.10]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id OAA08872 for ; Tue, 10 Sep 1996 14:42:36 +0200 Received: (from cn1@localhost) by irz201.inf.tu-dresden.de (8.6.12/8.6.12-s1) id OAA23411; Tue, 10 Sep 1996 14:41:40 +0200 From: "Nguyen, D.C." Message-Id: <199609101241.OAA23411@irz201.inf.tu-dresden.de> Subject: Re: spatial subdivision To: Al Zimmerman Date: Tue, 10 Sep 1996 14:41:39 +0200 (MESZ) Cc: globillum@imag.fr In-Reply-To: <9609092015.AA26156@sjs1> from "Al Zimmerman" at Sep 9, 96 01:15:51 pm X-Mailer: ELM [version 2.4 PL25 ME8b] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 > > So, does anybody out there have any familiarity with non-uniform grids > for spatial subdivision. I never used grids for RT-speedup (memories!), but it should be possible to construct a near-optimal BSP-tree and then convert it back to your grids. I dont think that grids are much faster than BSP, except you implement this alg. in hardware. Another fact is that pure-spatial subdivision algorithms are almost always static and they all are based on some more or less efficient "heuristics", so it is very hard to obtain a really optimal subdivision. A good idea is to bring some "intelligence" into your subdivision sheme, alias hybrid-shemes. Especially for raytracing, i've some good results while implementing some hybrid-shemes in GX: The speedup is about 300-500% comparing to balanced BSP(!) --JuHu /\__ Nguyen Duc Cuong (aka JuHu) - CG-student +- / -> Home /__\ \ EMail : juhu@rz.tu-ilmenau.de +- /GX -> GX/GENERIC \__/ WWW : http://www.rz.tu-ilmenau.de/~juhu -+- /GX/RTEvol -> RTEvol From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id RAA01560; Wed, 11 Sep 1996 17:28:31 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.13-durand/8.6.9) with ESMTP id PAA01355 for ; Wed, 11 Sep 1996 15:52:48 +0200 Received: from safran.imag.fr (safran.imag.fr [129.88.31.3]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id PAA12747; Wed, 11 Sep 1996 15:52:46 +0200 Received: (cazals@localhost) by safran.imag.fr (8.6.10/8.6.4) id PAA00310; Wed, 11 Sep 1996 15:54:39 +0200 From: Frederic Cazals Message-Id: <199609111354.PAA00310@safran.imag.fr> Subject: Re: spatial subdivision To: erich@eye.com Date: Wed, 11 Sep 1996 15:54:38 +0200 (MDT) Cc: globillum@imag.fr X-Mailer: ELM [version 2.4 PL23] MIME-Version: 1.0 Content-Type: text/plain; charset=windows-1252; format=flowed Content-Transfer-Encoding: 8bit X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hello, here are my $0.02 about speeding up ray-tracing with spatial subdivisions. the following elements are based upon a paper presented at Eurographics 95 (so see the proceedings or plug into http://flamingo.stanford.edu/~cazals/xfc_research.html and get the first paper) called 'Filtering, clustering and hierarchy construction: a new solution for ray tracing complex scenes' -so far, it seems that the fastest data structures are the recursive grids roughly built as follows: subdivide the bounding box of n objects into \sqrt[3]{n} subdivisions along the x,y and z axis, and iterate in each voxel containing more than MAX items --where MAX is some constant, say 50. of course, getting the right value for MAX in order to have a good tradeoff speed/memory requirements is the tricky point and that's one of the reasons why we came up with the Hierarchy of Uniform Grids (hug :)) -it is not obvious that non uniform subdivision implies 'heuristic that will fail in some particular case'. see the intuition provided by what is known about the asymptotic complexity of bucket sort vs. quick sort in our paper and how this should help in capturing the statistical properties of complex scenes frederic Cazals. -- ------------------------------------ ---------------- -------- ---- -- - -- iMAGIS Projet - Bat. B, 3 eme etage -- 385 rue de la Bibliotheque - Domaine Universitaire - StMartin d'Heres -- BP 53 - 38041 Grenoble cedex 09 - FRANCE -- Tel: 76-63-57-95 - Fax: 76-44-66-75 -- Frederic.Cazals@imag.fr From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id RAA01570; Wed, 11 Sep 1996 17:34:42 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.13-durand/8.6.9) with ESMTP id QAA02096 for ; Wed, 11 Sep 1996 16:15:50 +0200 Received: from eye.eye.com (eye.eye.com [149.54.1.2]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id QAA14338; Wed, 11 Sep 1996 16:15:44 +0200 Received: from hemlock (hemlock.eye.com) by eye.eye.com with SMTP ($Revision: 1.36.108.11 $/16.2) id AA161961334; Wed, 11 Sep 1996 10:15:35 -0400 Received: by hemlock (1.37.109.8/15.6) id AA06553; Wed, 11 Sep 1996 10:15:34 -0400 From: "Eric A. Haines" Message-Id: <9609111415.AA06553@hemlock> Subject: Re: spatial subdivision To: Frederic.Cazals@imag.fr Date: Wed, 11 Sep 96 10:15:33 EDT Cc: erich@eye.eye.com, globillum@imag.fr In-Reply-To: <199609111354.PAA00310@safran.imag.fr>; from "Frederic Cazals" at Sep 11, 96 3:54 pm Mailer: Elm [revision: 70.85] X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Frederic Cazals writes: >-so far, it seems that the fastest data structures are the recursive >grids roughly built as follows: subdivide the bounding box of n >objects into \sqrt[3]{n} subdivisions along the x,y and z axis, and >iterate in each voxel containing more than MAX items --where MAX is >some constant, say 50. of course, getting the right value for MAX in I agree entirely, nested grids looks like a big win: you get the walking efficiency of grids and so get to walk large empty spaces quickly with the adaptive advantages of speed and robustness (rendering a teapot in a stadium brings a single grid structure to its knees). For similar work, see: %A David Jevans %A Brian Wyvill %T Adaptive Voxel Subdivision for Ray Tracing %J Proceedings of Graphics Interface '89 %I Canadian Information Processing Society %C Toronto, Ontario %D June 1989 %P 164-72 %Z nested grid subdivision structures %K grid subdivision, hierarchical subdivision %A David Jevans %T Adaptive Voxel Subdivision for Ray Tracing %R Master's Thesis %I Dept. of Computer Science, Univ. of Calgary %D 1990 %Z long version of paper %K grid subdivision, hierarchical subdivision Frederic, if you've seen these, how does your work compare with their technique? Personally, I use a variant of having the global grid store just object IDs, then each object itself has a bounding volume and grid if needed. The advantage to me is ease of coding and tight bounds - the same generic grid code is used for both, and the object's bounding box defines its grid size. Also, this method has the advantage of an intermediate bounding volume test before going into the nested grid, as a global grid cell may have a tiny object or a small part of some object in it, in which case you would normally spend (with just nested grids) a fair bit of time traversing the nested grid for no intersection. I need the bounding box test anyway to get a ray starting point for the object's grid. Eric Haines erich@eye.com From X-POP3-Rcpt: wp@stellaris Received: from isis.imag.fr by stellaris.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/910805.SGI) id OAA02650; Thu, 12 Sep 1996 14:01:08 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.13-durand/8.6.9) with ESMTP id NAA15888 for ; Thu, 12 Sep 1996 13:41:16 +0200 Received: from safran.imag.fr (safran.imag.fr [129.88.31.3]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id NAA00674; Thu, 12 Sep 1996 13:41:15 +0200 Received: (cazals@localhost) by safran.imag.fr (8.6.10/8.6.4) id NAA11313; Thu, 12 Sep 1996 13:43:09 +0200 From: Frederic Cazals Message-Id: <199609121143.NAA11313@safran.imag.fr> Subject: Re: spatial subdivision To: "Eric A. Haines" Date: Thu, 12 Sep 1996 13:43:09 +0200 (MDT) Cc: globillum@imag.fr In-Reply-To: <9609111415.AA06553@hemlock> from "Eric A. Haines" at Sep 11, 96 10:15:33 am X-Mailer: ELM [version 2.4 PL23] MIME-Version: 1.0 Content-Type: text/plain; charset=windows-1252; format=flowed Content-Transfer-Encoding: 8bit X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 > %A David Jevans > %T Adaptive Voxel Subdivision for Ray Tracing > %R Master's Thesis > %I Dept. of Computer Science, Univ. of Calgary > %D 1990 > %Z long version of paper > %K grid subdivision, hierarchical subdivision > > Frederic, if you've seen these, how does your work compare with their technique? there are three major differences: -while D. Jevans's data structure is built top-down, ours is built bottom-up -we do not have any hand tuned parameter while he has two of them: the max number of items per voxel and the max hierarchy depth -he assumes that he has an efficient dynamic hashing algorithm to store the non-empty voxels since he does not know beforehand how many such voxels he is going to end up with, while the only data structures we are using are arrays and lists (allocated once for all and thus not causing any memory fragmentation problem). frederic Cazals. -- ------------------------------------ ---------------- -------- ---- -- - -- iMAGIS Projet - Bat. B, 3 eme etage -- 385 rue de la Bibliotheque - Domaine Universitaire - StMartin d'Heres -- BP 53 - 38041 Grenoble cedex 09 - FRANCE -- Tel: 76-63-57-95 - Fax: 76-44-66-75 -- Frederic.Cazals@imag.fr From Received: from isis.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id LAA14542; Mon, 16 Sep 1996 11:59:32 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.6.13-durand/8.6.9) with ESMTP id LAA21219 for ; Mon, 16 Sep 1996 11:27:27 +0200 Received: from mr.tuwien.ac.at (mr.tuwien.ac.at [128.130.2.10]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id LAA28595 for ; Mon, 16 Sep 1996 11:27:21 +0200 Received: from titus.cg.tuwien.ac.at by mr.tuwien.ac.at with SMTP (PP); Mon, 16 Sep 1996 11:26:10 +0200 Received: from [128.130.166.56] by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) for id LAA14332; Mon, 16 Sep 1996 11:26:08 +0200 X-Sender: wp@128.130.166.14 Message-Id: Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed Date: Mon, 16 Sep 1996 11:25:57 +0200 To: globillum@imag.fr From: Werner Purgathofer Subject: radiosity research position X-UIDL: 923e170c1572fba91c8d1cd18017a287 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit ************************************************************* There is a granted research position in the field of radiosity available for a period of two years at the Technical University of Vienna, Institute of Computer Graphics (see http://www.cg.tuwien.ac.at/envisage for further information) The title of the project is "Radiosity Methods for Highly Complex Scenes by Perceptual Importance". The primary goal of this project is to develop an efficient stochastic radiosity method. Using importance driven view-dependent methods, perceptually based error metrics shall be investigated in order to increase the visual quality of the images. All algorithms shall be designed in an object oriented way with respect to parallel computation. The starting date is as soon as possible, i.e. immediately! The conditions are: You get: - about 25.000,- US$ gross income per year (that is about 18.500,- US$ net income) *) - the working environment (desk in our department, access to SGI-computers, access to a good computer graphics library ...) - wonderful colleagues You don't get (neither money for nor organisation of): - travelling to or from Vienna - place to live (apartment or room or tent or whatever) - breakfast, lunch, dinner We expect: - you have completed a graduate study in computer science (or similar) - you are familiar with radiosity and related computer graphics techniques - you are an extremely motivated researcher - you want to write a PhD **) - you speak and write very good English - you are prepared to help a little bit with teaching We do *not* expect: - you speak German - you wear ties every day *) Some living costs: You don't need a car in Vienna, public transport is very good, at about 47$ per month. You can eat in a normal restaurant for about 10-12$, beer (half liter) costs about 3$ (60-70c in the supermarket), the University provides lunch for about 4-5$. You should be able to find a room for less than 300$ per month, an apartment costs at least 500$ per month. A cinema ticket costs about 10-12$, black bread 2$/kg, 1l milk 1$, chocolate from 50c/100g, meat 5-20$/kg, drinking water from the pipe is free. **) two years is probably not enough for a complete PhD, but the kernel of the work should be done. However, the project should be the basis for a continuing cooperation, enabling you to obtain a PhD from our University thereafter. There might also be the possibility to extend the project by a third year. If you are interested, please apply *by email* before 25th September 1996 to Werner Purgathofer (mailto:wp@cg.tuwien.ac.at) Please send at least: - your curriculum vitae - your list of publications (if any) - the topic of your diploma thesis (masters thesis) - a short essay why you are interested in this position - two or three references, i.e. people who know you professionally - an email address to answer you You may include an internet-URL of your WWW home pages, if this makes it easier for us to evaluate you and your previous work. Notice 1: In case of equal qualification women will be preferred. Notice 2: Smoking is prohibitted in our offices (as in all public rooms in Austria) ************************************************************* From Received: from isis.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id QAA20511; Tue, 24 Sep 1996 16:02:39 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.8.Beta.5/8.6.9) with ESMTP id OAA23029 for ; Tue, 24 Sep 1996 14:26:43 +0200 (MET DST) Received: from idefix.cs.kuleuven.ac.be (idefix.cs.kuleuven.ac.be [134.58.40.4]) by imag.imag.fr (8.6.11/8.6.9) with ESMTP id OAA11961 for ; Tue, 24 Sep 1996 14:26:31 +0200 Received: from krasser.cs.kuleuven.ac.be (philipd@krasser.cs.kuleuven.ac.be [134.58.45.36]) by idefix.cs.kuleuven.ac.be (8.7.6/8.7.3) with ESMTP id OAA23913 for ; Tue, 24 Sep 1996 14:26:10 +0200 (MET DST) Received: (from philipd@localhost) by krasser.cs.kuleuven.ac.be (8.7.6/8.7.3) id OAA24569 for globillum@imag.fr; Tue, 24 Sep 1996 14:26:07 +0200 (MET DST) Date: Tue, 24 Sep 1996 14:26:07 +0200 (MET DST) From: Phil Dutre Message-Id: <199609241226.OAA24569@krasser.cs.kuleuven.ac.be> To: globillum@imag.fr Subject: Ph.D. Thesis available X-Sun-Charset: US-ASCII X-UIDL: 40582e8ddc215d4982df76bf712843a4 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Dear collegues, My Ph.D Thesis (which I defended succesfully last week) is available on the WWW: http://www.cs.kuleuven.ac.be/cwis/research/graphics/CGRG.PUBLICATIONS/PHDPHD/ (nice alliteration there ... ) The files are available as gzipped postscript. If you have any problems in downloading the text, please do not hesitate to contact me. Philip Dutre +-----------------------------------------------------------------------+ |Philip.Dutre@cs.kuleuven.ac.be Department of Computer Science | |http://www.cs.kuleuven.ac.be/~philipd/ Computer Graphics Research Group| |Phone: ++32 16 327667 (NEW!) Katholieke Universiteit Leuven | |Fax: ++32 16 327996 Celestijnenlaan 200A | |Office: C200, A.01.44 B-3001 Heverlee, BELGIUM | +-----------------------------------------------------------------------+ Title: Mathematical Frameworks and Monte Carlo Algorithms for Global Illumination in Computer Graphics Abstract: The title of this thesis `Mathematical Frameworks and Monte Carlo Algorithms for Global Illumination in Computer Graphics' refers to a domain in the field of computer graphics known as photo-realistic image rendering or global illumination. The goal of this domain is to compute realistic pictures of a three-dimensional scene, as could have been observed by a human observer or more precisely, a camera. The first part of this work describes the physical and mathematical foundations which are needed in order to describe the global illumination problem. The fundamental physical measure needed to describe the distribution of light in an environment is radiance. The equation describing the transport of radiance is a recursive integral equation. The dual problem introduces potential as a basic measure, and the potential equation as the corresponding transport equation. Both dual formulations can be used in order to solve the global illumination problem. Once the mathematical framework has been developed, the equations describing the transport of light or potential can be solved. Due to the high number of integrals and the complexity and unknown behaviour of the functions to be integrated, Monte Carlo integration provides a viable method of computing the global illumination in a three-dimensional scene. Depending on the choice of what transport equation to use, the radiance transport equation leads to distributed ray tracing or path tracing, and the potential transport equation leads to light tracing or particle tracing. The latter method generates particles at the light sources, which each carry a small amount of power. They carry out a random walk in the three-dimensional scene, and possibly contribute their power to the flux of a pixel on the screen. Mathematically, this algorithm can be considered as the dual algorithm of ray tracing. The sampling functions used for the generation of the random walks can be based on reflective properties of the surfaces encountered. However, in diffuse environments, better results can be expected when they are based on the (unknown) potential distribution. Since the optimal sampling function is not known in advance, one solution is to use adaptive probability density functions. As more particles are being generated, the potential distribution can be approximated more accurately, and thus a better sampling function can be constructed. This technique requires a substantial amount of memory, but produces better results. The used sampling algorithms can also be extended to other Monte Carlo rendering algorithms, such as bidirectional path tracing. From Received: from isis.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id WAA21487; Tue, 24 Sep 1996 22:24:12 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.8.Beta.5/8.6.9) with ESMTP id VAA05825 for ; Tue, 24 Sep 1996 21:57:46 +0200 (MET DST) Received: from buffer.lsu.edu (buffer.csc.lsu.edu [130.39.130.30]) by imag.imag.fr (8.6.11/8.6.9) with SMTP id VAA03334 for ; Tue, 24 Sep 1996 21:57:44 +0200 From: oleg@buffer.lsu.edu Received: by buffer.lsu.edu (5.65/DEC-Ultrix/4.3) id AA00925; Tue, 24 Sep 1996 14:58:42 -0500 Message-Id: <9609241958.AA00925@buffer.lsu.edu> To: globillum@imag.fr Subject: analytic solutions Date: Tue, 24 Sep 96 14:58:31 -0500 X-Mts: smtp X-UIDL: ae52bdf192ac82101e4b7be86def5f10 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Salut ! I was doing my radiosity project when I realized that the approximate "differential area - to - disk" form factor formula FF = cos(a)*cos(b)*R^2 / (R^2 + h^2) given in so many books for numerical form factor integration gives in most cases 100%-200% numerical errors (!) . I had to derive the exact general analytic solution for this case, which was possibly known before ( do you have any references ?), but apparently was never recommended for practical use (to my knowledge). This exact formula is not very complicated compared to its widely used approximation, but it produces much more accurate results. It is also computationally simpler than the exact formulas known for other geometries (such as point-to-polygon); I think it makes this solution very useful. If it sounds interesting or if you faced any form factor computing problems before, please give me some feedback. I am also interested in any related open research problems. Oleg Pianykh Ph.D. student Louisiana State University oleg@bit.csc.lsu.edu P.S. Vous pouvez repondre en francais... From Received: from isis.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id SAA08750; Thu, 3 Oct 1996 18:38:55 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.8.Beta.5/8.6.9) with ESMTP id RAA18595 for ; Thu, 3 Oct 1996 17:54:55 +0200 (MET DST) Received: from cs.utah.edu (cs.utah.edu [128.110.4.21]) by imag.imag.fr (8.8.Beta.5/8.6.9) with SMTP id RAA25894 for ; Thu, 3 Oct 1996 17:54:52 +0200 (MET DST) From: shirley@facility.cs.utah.edu Received: from wingate.cs.utah.edu by cs.utah.edu (8.6.12/utah-2.21-cs) id JAA04480; Thu, 3 Oct 1996 09:54:50 -0600 Received: by wingate.cs.utah.edu (8.6.12/utah-2.15sun-leaf) id JAA14832; Thu, 3 Oct 1996 09:54:49 -0600 Message-Id: <199610031554.JAA14832@wingate.cs.utah.edu> Subject: Help with conference/journal links To: globillum@imag.fr Date: Thu, 3 Oct 1996 09:54:48 -0600 (MDT) X-Mailer: ELM [version 2.4 PL25] Content-Type: text; charset=windows-1252 X-UIDL: 65f7fde0003df454be138bea66875368 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 MIME-Version: 1.0 Content-transfer-encoding: 8bit Hi-- on my new home page: http://www.cs.utah.edu/~shirley/ I have added links to graphics journals and conferences with home pages. Please send me additions/corrections (I know I am missing GI and C&G-- where are they?) Thanks Pete Shirley shirley@cs.utah.edu From Received: from isis.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id JAA11999; Fri, 4 Oct 1996 09:36:02 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.8.Beta.5/8.6.9) with ESMTP id JAA24816 for ; Fri, 4 Oct 1996 09:08:51 +0200 (MET DST) Received: from safran.imag.fr (safran.imag.fr [129.88.31.3]) by imag.imag.fr (8.8.Beta.5/8.6.9) with ESMTP id JAA23653 for ; Fri, 4 Oct 1996 09:08:50 +0200 (MET DST) Received: (from sillion@localhost) by safran.imag.fr (8.6.10/8.6.9) id JAA01413 for globillum@imag.fr; Fri, 4 Oct 1996 09:08:49 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by safran.imag.fr (8.6.10/8.6.9) with ESMTP id SAA23072 for ; Thu, 3 Oct 1996 18:42:01 GMT Received: from nala.ctima.uma.es (nala.ctima.uma.es [150.214.57.7]) by imag.imag.fr (8.8.Beta.5/8.6.9) with SMTP id UAA03174 for ; Thu, 3 Oct 1996 20:41:41 +0200 (MET DST) Received: from sol10.lcc.uma.es (sol10.lcc.uma.es [150.214.108.1]) by nala.ctima.uma.es (8.6.9/8.6.9) with SMTP id TAA10914 for ; Thu, 3 Oct 1996 19:39:38 GMT Received: from frvm.lcc.uma.es ([150.214.58.68]) by sol10.lcc.uma.es (5.x/SMI-SVR4) id AA13932; Thu, 3 Oct 1996 20:40:57 GMT Date: Thu, 3 Oct 1996 20:40:55 GMT Message-Id: <1.5.4.16.19961003203114.0b3f7372@sol10.lcc.uma.es> X-Sender: villa@sol10.lcc.uma.es X-Mailer: Windows Eudora Light Version 1.5.4 (16) Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed To: owner-globillum@imag.fr From: Francisco Villatoro Subject: Re: analytic solutions Sender: Francois.Sillion@imag.fr X-UIDL: cc815d2c7061ba07dc6792e4d65cd2d6 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit >Date: Thu, 03 Oct 1996 17:58:23 >To: oleg@buffer.lsu.edu >From: Francisco Villatoro >Subject: Re: analytic solutions >>>>>>>>> Returned mail: Host unknown (Name server: buffer.lsu.edu: host not found) So I send it again, but now to all globillum's people. > > Hi ! >>>>>>>>>> From >> Oleg Pianykh >> Ph.D. student >> Louisiana State University >> oleg@bit.csc.lsu.edu >> >> I was doing my radiosity project when I realized that the approximate >>"differential area - to - disk" form factor formula >> >> FF = cos(a)*cos(b)*R^2 / (R^2 + h^2) >> >>given in so many books for numerical form factor integration gives in most cases >>100%-200% numerical errors (!) . I had to derive the exact general analytic solution for >>this case, which was possibly known before ( do you have any references ?), > > The general analytic solution for the view (or form) factor from > a differential area to a disk, when the disk is fully visible and > when it is partially visible (the contour is a line (chord) and a partial > circle), has been previously published by > > M. H. N. Naraghi, "Radiation View Factors from Differential Plane > Sources to Disks--A General Formulation" > AIAA Journal of ThermoPhysics & Heat Transfer > Vol. 2, No. 3, pp. 271-274, 1988. > >> but >>apparently was never recommended for practical use (to my knowledge). This exact formula >>is not very complicated compared to its widely used approximation, but it produces much >>more accurate results. > > > To my knowledge, the approximate "differential area - to - disk" > form factor formula you presented above, is the Juul formula, which is valid > only when the diff. area is in front of the disk and passing through its > center, although the orientation of the diff. area is arbitrary. > > N. H. Juul, "Diffuse Radiative View Factors from Differential Plane > Sources to Spheres" > Trans. of ASME, Journal of Heat Transfer > Vol. 101, No. 3, pp. 558-560, 1979. > > > And so, this approximation is expected to produce large errors when > the disk is oriented arbitrary on space or is not exactly in front of the > diff. area. > >>It is also computationally simpler than the exact formulas known >>for other geometries (such as point-to-polygon); I think it makes this solution very >>useful. > >> If it sounds interesting or if you faced any form factor computing problems >>before, please give me some feedback. > > One of my students is involved in a "graduation work" (similar to > a Master Thesis in Engineering) on a comparison of different techniques > for form-factor evaluation. The student has started recently, and today, > we have no new results. > > I am also interested in any related problem on form factors. > > >PS: Thanks to J.I. Ramos (University of Malaga) and N. Winowich (University >of Tennessee) for their help and suggestions. > > ------------------------------------------------------- Francisco R. Villatoro Machuca Dpto. Lenguajes y Ciencias de la Computacion Universidad de Malaga e-mail: villa@lcc.uma.es http://www.lcc.uma.es/personal/villa/villa.html Telf.: +34-5-213.20.96 FAX : +34-5-213.28.16 From Received: from isis.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id QAA23575; Tue, 8 Oct 1996 16:47:48 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.8.Beta.5/8.6.9) with ESMTP id QAA15152 for ; Tue, 8 Oct 1996 16:07:11 +0200 (MET DST) Received: from miki.wro.ternet.pl (root@ppp-cen66.wroclaw.tpnet.pl [194.204.169.66]) by imag.imag.fr (8.8.Beta.5/8.6.9) with SMTP id QAA01684 for ; Tue, 8 Oct 1996 16:07:04 +0200 (MET DST) Received: from ppp (loc1 [10.0.0.11]) by miki.wro.ternet.pl (8.6.12/8.6.12) with SMTP id QAA05311 for ; Tue, 8 Oct 1996 16:06:32 +0200 Message-ID: <325A585C.3B10@wro.ternet.pl> Date: Tue, 08 Oct 1996 14:34:20 +0100 From: Slawomir Kilanowski Organization: Metagram X-Mailer: Mozilla 3.0 (Win95; I) MIME-Version: 1.0 To: Global Illumination Mailing List Subject: Shadow analysis acceleration Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: 85c3c4d215f54fbe45d66f8e499ca64c X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Dear Collegues, A month ago (September 7th) I asked for help in finding papers related to the project I was involved in - speed up of shadows analysis. I would like to thank once again all those who answered my query. Below you'll find the small bibliography I have completed. I hope it may be of some use for someone who will encounter the same problem. For those who are interested in "quick fix" of performance of a ray tracer with shadows calculated by ray casting I may honestly devise the Greg Ward's method described in "Adaptive Shadow Testing for Ray Tracing". It gave average speed-up factor varying from 1.5 - 5.0 calculated on models build of 10,000 - 40,000 polygons, with 50 - 400 lights. The differences in resultant images were not noticeable. In absolute terms (number of differing pixels and magnitude of differences) the differences were smaller than introduced by standard JPEG compression. Andrew Woo and Pierre Poulin and Alain Fournier, "A Survey of Shadow Algorithms", IEEE Computer Graphics and Applications, Vol 10, No 6, November 1990 Andrew Woo and John Amanatides, "Voxel Occlusion Testing: {A} Shadow Determination Accelerator for Ray Tracing", Proceedings of Graphics Interface '90, held in Halifax, Nova Scotia; 14-18 May 1990", Andrew Pearce and David Jevans "Exploiting Shadow Coherence in Ray Tracing", Proceedings of Graphics Interface '91", held in Calgary, Alberta; 3-7 June 1991, Frederic Asensio, "A Hierarchical Ray-Casting Algorithm for Radiosity Shadows" Third Eurographics Workshop on Rendering, 1991, Bristol, UK H. K. Choi and C. M. Kyung Pysha: a Shadow-Testing Acceleration Scheme for Ray Tracing, Computer-aided design, Vol 24, No 2, February 1992 A. James Stewart and Sherif Ghali, "An Output Sensitive Algorithm for the Computation of Shadow Boundaries", Canadian Conference on Computational Geometry, August 1993 Arjan J. F. Kok and Frederik W. Jansen and C.Woodward, "Efficient, Complete Radiosity Ray Tracing Using a Shadow-Coherence Method", The Visual Computer, Vol 10, 1994 A. James Stewart and Sherif Ghali, "Fast Computation of Shadow Boundaries Using Spatial Coherence and Backprojections", Proceedings of SIGGRAPH '94 (Orlando, Florida, July 24--29, 1994) Yiorgos Chrysanthou and Mel Slater, Shadow Volume {BSP} Trees for Computation of Shadows in Dynamic Scenes, 1995 Symposium on Interactive {3D} Graphics, Seth Teller and Pat Hanrahan, "Global Visibility Algorithms for Illumination Computations", Computer Graphics Proceedings, Annual Conference Series, 1993, A.J.F. Kok and F.W. Jansen Source Selection of the Direct Lighting Computation in Global Illumination Proceedings Second Rendering Workshop, 1991, Barcelona. In: Photorealistic Rendering in Computer Graphics, Springer Verlag, 75-82. Kurt Zimmerman, Peter Shirley "A Two-Pass Realistic Image Synthesis Method for Complex Scenes" Rendering Techniques '95 (Proceedings of the Sixth Eurographics Workshop on Rendering), Springer-Verlag, New York, NY 1995, pp 284-295 George Dretakkis and Eugene Fiume, "A Fast Shadow Algorithm for Area Light Sources Using Backprojection" Proceedings of SIGGRAPH '94 (Orlando, Florida, July 24--29, 1994), Seth J. Teller and Carlo H. Sequin, "Visibility preprocessing for interactive walkthroughs", Computer Graphics (SIGGRAPH '91 Proceedings), held in Las Vegas, Nevada; 28 July - 2 August 1991, Ward, Gregory, "Adaptive Shadow Testing for Ray Tracing," Second EUROGRAPHICS Workshop on Rendering, Barcelona, Spain, April 1991 Shirley, Peter, "Direct Lighting Calculation by Monte Carlo Integration," Second EUROGRAPHICS Workshop on Rendering, June 1991 (?) George Drettakis, Francois Sillion "Accurate Visibility and Meshing Calculations for Hierarchical Radiosity" Seth Teller, Pat Hanrahan "Global Visibility Algorithms for Illumination Computations", Computer Graphics, SIGGRAPH '94 proceedings. Kurt Zimmerman, Peter Shirley "A Two-Pass Realistic Image Synthesis Method for Complex Scenes", Indiana Univeristy, Technical Report No 434 -- ================================================================ Slawomir Kilanowski metagram@wro.ternet.pl METAGRAM, Swieradowska 73/23, 50-559 Wroclaw, Poland Phone/Fax : +48-(71)-731519 ================================================================ From Received: from isis.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id TAA24840; Tue, 8 Oct 1996 19:52:31 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.8.Beta.5/8.6.9) with ESMTP id TAA19136 for ; Tue, 8 Oct 1996 19:31:07 +0200 (MET DST) Received: from HOSTESS.GRAPHICS.CS.CMU.EDU (HOSTESS.GRAPHICS.CS.CMU.EDU [128.2.206.188]) by imag.imag.fr (8.8.Beta.5/8.6.9) with SMTP id TAA13643 for ; Tue, 8 Oct 1996 19:31:05 +0200 (MET DST) From: Paul.Heckbert@HOSTESS.GRAPHICS.CS.CMU.EDU Message-Id: <199610081731.TAA13643@imag.imag.fr> Date: Tue, 8 Oct 96 13:23:43 EDT To: globillum@imag.fr Subject: mesh generation info on web X-UIDL: 384f85f7094efb6fdf04b7d7ca8aee94 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit I've created an index to mesh generation info on the world wide web. This might be of interest to radiosity researchers. http://www.cs.cmu.edu/~ph/mesh.html Here's a preview of what you'll find there: ----------------------------------------------------------- Paul Heckbert's Collection of Mesh Generation Links This is a collection of World Wide Web links to information on mesh generation. There are also some links not specifically focused on mesh generation, relating to computational fluid dynamics (CFD), finite element methods (FEM), multigrid, triangulation, and computational geometry. The bias of these links is toward anisotropic unstructured triangular mesh generation (and consequently toward viscous flow applications). Too much jargon? Try the [mini-glossary of mesh generation]. table of contents: Collections of Links (this section includes links to several more comprehensive collections by Robert Schneiders and Steve Owen) Bibliographies Online Conferences/Journals/Newsletters & Big Paper Collections Offline Conferences & Journals People and Their Papers Software ----------------------------------------------------------- Paul Heckbert Computer Science Dept., Carnegie Mellon University 5000 Forbes Ave, Pittsburgh PA 15213-3891, USA ph@cs.cmu.edu http://www.cs.cmu.edu/~ph From Received: from isis.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id KAA26979; Wed, 9 Oct 1996 10:24:44 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.8.Beta.5/8.6.9) with ESMTP id KAA24610 for ; Wed, 9 Oct 1996 10:01:04 +0200 (MET DST) Received: from TUDRNV.TUDELFT.NL (tudrnv.tudelft.nl [130.161.180.88]) by imag.imag.fr (8.8.Beta.5/8.6.9) with ESMTP id KAA09305 for ; Wed, 9 Oct 1996 10:01:01 +0200 (MET DST) Received: from mailsrv.twi.tudelft.nl (mailsrv.twi.tudelft.nl) by TUDRNV.TUDelft.NL (PMDF V5.0-6 #15266) id <01IAFNUPVB7K003B64@TUDRNV.TUDelft.NL>; Wed, 09 Oct 1996 09:48:41 +0200 Received: from duticg.twi.tudelft.nl by mailsrv.twi.tudelft.nl with ESMTP ($Revision: 1.37.109.23 $/15.6) id AA069027484; Wed, 09 Oct 1996 08:51:26 +0100 Received: by duticg.twi.tudelft.nl ($Revision: 1.37.109.23 $/16.2) id AA207217298; Wed, 09 Oct 1996 09:48:18 +0200 Date: Wed, 9 Oct 96 9:48:15 METDST From: Erik Jansen Subject: Re: Shadow analysis acceleration In-reply-to: <325A585C.3B10@wro.ternet.pl>; from "Slawomir Kilanowski" at Oct 08, 96 2:34 pm To: Slawomir Kilanowski Cc: globillum@imag.fr Message-id: <199610090748.AA207217298@duticg.twi.tudelft.nl> Content-transfer-encoding: 8bit Mailer: Elm [revision: 70.85.1.76] X-UIDL: ac6e4d071277da016b74c8100dd8b153 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Slawomir Kilanowski wrote: > > A month ago (September 7th) I asked for help in finding papers > related to the project I was involved in - speed up of shadows > analysis. I would like to thank once again all those who answered > my query. Below you'll find the small bibliography I have completed. > I hope it may be of some use for someone who will encounter the > same problem. Excellent to give this overview of your experiences and results. To complement your list of references I can provide the following information: > > Ward, Gregory, "Adaptive Shadow Testing for Ray Tracing," Second > EUROGRAPHICS Workshop on Rendering, Barcelona, Spain, April 1991 > > Shirley, Peter, "Direct Lighting Calculation by Monte Carlo > Integration," Second EUROGRAPHICS Workshop on Rendering, June 1991 (?) > The second EG Workshop on Rendering was held in May(!) 1991. And the proceedings are published as P. Brunet, F.W. Jansen (eds) Photorealistic Rendering in Computer Graphics, Springer Verlag, 1994 (!) ISBN 3-540-56449-7 or 0-387-56449-7 The papers mentioned appear at the following pages: Ward, "Adaptive Shadow Testing for Ray Tracing," p. 11 - 20. Shirley, "Direct Lighting Calculation ...", p. 54 - 59. Kok and Jansen, "Source Selection for ....", p. 75 - 82. I would like to suggest that the papers are referenced as dating from 1991 instead of 1994 the year the Springer proceedings were published. The latest RW proceedings (Rendering Techniques'9x) are now fortunately published within the same year as the workshop has been held. Erik Jansen From Received: from isis.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id WAA13629; Sat, 12 Oct 1996 22:15:00 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.8.Beta.5/8.6.9) with ESMTP id WAA24487 for ; Sat, 12 Oct 1996 22:00:03 +0200 (MET DST) Received: from mercury.uniserve.com (mercury.uniserve.com [204.191.197.248]) by imag.imag.fr (8.8.Beta.5/8.6.9) with ESMTP id VAA16873 for ; Sat, 12 Oct 1996 21:59:57 +0200 (MET DST) Received: from van0102.TVS.NET (van0102.TVS.NET [204.191.197.12]) by mercury.uniserve.com (8.7.5/8.7.3) with SMTP id MAA29091 for ; Sat, 12 Oct 1996 12:56:02 -0700 (PDT) Date: Sat, 12 Oct 1996 12:56:02 -0700 (PDT) Message-Id: <199610121956.MAA29091@mercury.uniserve.com> X-Sender: iashdown@pop.uniserve.com X-Mailer: Windows Eudora Version 2.0.3 Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed To: globillum@imag.fr From: Ian Ashdown Subject: Radiosity bibliography update X-UIDL: cff89b43ba9109fa7f72fdf1587395ca X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit It's me again, cluttering up your "in" basket with yet another update to the radiosity and global illumination bibliography, RADBIB96.TXT. There were a fair number of editing changes made to the last release. To To save you the trouble of determining what's new, here are the additional references: RADBIB96.TXT - Radiosity and Global Illumination Bibliography ------------------------------------------------------------- ORIGINAL FILE: RADBIB96.TXT 96/09/01 NEW FILE: RADBIB96.TXT 96/10/15 The following 26 new references were added to RADBIB96.TXT since its last release on September 1, 1996. Corrections to the original file are not included. RADBIB96.TXT can be downloaded via anonymous ftp as: /pub/docs/RadBib96.Z from hobbes.lbl.gov, and as: RADBIB96.TXT from http://www.ledalite.com/library-/rrt.html A BibTex version of this bibliography is available from: ftp.cs.columbia.edu/archives/bibliographies/Graphics/rad.html ------------------------------------------------------------------------- %A Rui Bastos %A Michael Goslin %A Hansong Zhang %T Efficient Rendering of Radiosity Usinig Textures and Bicubic Reconstruction %R Technical Report TR95-026 %I Department of Computer Science, University of North Carolina at Chapel Hill %C Chapel Hill, NC %D 1995 %A Paul J. Diefenbach %A Norman I. Badler %T Pipeline Rendering: Interactive Refractions, Reflections, and Shadows %J Displays (Special Issue on Interactive Computer Graphics) %V 15 %N 3 %P 173-180 %D 1994 %A Paul J. Diefenbach %T Pipeline Rendering: Interaction and Realism through Hardware-Based Multi-Pass Rendering %R PhD thesis %I University of Pennsylvania %D 1996 %A Yoshinori Dobashi %A Kazufumi Kaneda %A Hideki Nakatani %A Hideo Yamashita %T A Quick Rendering Method for Outdoor Scenes Using Sky Light Luminance Function Expressed with Basis Functions %J Journal of the Institute of Image Electronics Engineers of Japan %V 24 %N 3 %P 196-205 %D 1995 %Z in Japanese %A Alexander Keller %T A Quasi-Monte Carlo Algorithm for the Global Illumination Problem in the Radiosity Setting %B Monte Carlo and Quasi-Monte Carlo Methods in Scientific Computing %E H. Niederreiter %E P. Shiue %I Springer-Verlag %C New York, NY %P 239-251 %D 1995 %A Alexander Keller %T Quasi-Monte Carlo Methods in Computer Graphics: The Global Illumination Problem %J Proceedings of the SIAM Conference in Park City %P ??? %D 1996 %A Alexander Keller %T The Fast Calculation of Form Factors Using Low Discrepancy Sequences %J Proceedings of the Twelfth Spring Conference on Computer Graphics (SCCG '96) %I Comenius University Press %C Bratislava, Slovakia %P ??? %D June 1996 %A A. Kersch %A W. Morokoff %A A. Schuster %T Radiative Heat Transfer with Quasi-Monte Carlo Methods %J Transport Theory and Statistical Physics %V 7 %N 23 %P 1001-1021 %D 1994 %A Hiroaki Kobayashi %A Hitoshi Yamauchi %A Yuichiro Toh %A Tadao Nakamura %T M PI-Squared: A Hierarchical Parallel Processing System for a Global Illumination Model %J Proceedings of ISPAN '94 %P 157-164 %D 1994 %A K. Kuo %A R. C. Weger %A R. M. Cox %T The Picard Iterative Approximation to the Solution of the Integral Equation of Radiative Transfer - Part II. Three-Dimensional Geometry %J Journal of Quantitative Spectroscopy and Radiative Transfer %V 55 %N 2 %P 195-212 %D 1996 %A Eric Languenou %A Kadi Bouatouch %A Pierre Tellier %T Une Nouvelle Approche Realiste de Simulation d'Eclairage dans un Environnement Diffus %R Research Report 1553 %I INRIA %C Rennes, France %D November 1991 %A Robert R. Lewis %T Wavelet Radiance Transport and Surface Interaction %J Proceedings of the Seventh Western Computer Graphics Symposium %E John C. Hart %P 73-83 %D March 1996 %A W. M. G. Malalasekera %A E. H. James %T Calculation of Radiative Heat Transfer Three-Dimensional Complex Geometries %J 1995 ASME National Heat Transfer Conference Proceedings %V 315 %P 53-61 %D 1995 %K discrete transfer method %A W. M. G. Malalasekera %A E. H. James %T Radiative Heat Transfer Calculations in Three-Dimensional Complex Geometries %J Journal of Heat Transfer %V 118 %P 225-227 %D February 1996 %K discrete transfer method %A G. I. Marchuk %A V. I. Agoshkov %T Reflection Operators and Contemporary Applications to Radiative Transfer %J Applied Mathematics and Computation %V 69 %N 1 %P 3-?? %D 1995 %A M. H. N. Naraghi %T Radiation View Factors from Differential Plane Sources to Disks - A General Formulation %J AIAA Journal of Thermophysics and Heat Transfer %V 2 %N 3 %P 271-274 %D 1988 %A D. M. O'Brien %T Accelerated Quasi Monte Carlo Integration of the Radiative Transfer Equation %J Journal of Quantitative Spectroscopy and Radiative Transfer %V 48 %N 1 %P 41-?? %D July 1992 %K quasi Monte Carlo integration, radiative transfer equation %A Rachel Orti %A Stephane Riviere %A Fredo Durand %A Claude Puech %T Using the Visibility Complex for Radiosity Computation %J Proceedings of the ACM Workshop on Applied Computational Geometry %P ? %D May 1996 %A Sumanta N. Pattanaik %A Kadi Bouatouch %T Interactive Walk-Through Using Particle Tracing %R Technical Report PI-903 %I IRISA %C Rennes, France %Z available from http://www.irisa.fr/EXTERNE/bibli/pi (in French) %A Edward Saxe %A ? %T Higher-Order Color Interpolation for Real-time Radiosity Display %R Technical Report TR96-023 %I Department of Computer Science, University of North Carolina at Chapel Hill %C Chapel Hill, NC %D 1996 %A Christophe Schlick %T Elements pour une Synthese d'Images Realistes %R PhD thesis %I Universite Bordeaux 1, France %D November 1992 %A Frank Schoffel %T Radiosity in Dynamischen Szenen %R Master's thesis %I Technische Hochschule Darmstadt %C Darmstadt, Germany %D 1994 %K dynamic environments, shadow-form-factor-list, scene coherence, radiosity repropagation, progressive refinement %A E. S. Shaw %T Hierarchical Radiosity for Dynamic Environments %R Master's thesis %I Program of Computer Graphics, Cornell University %C Ithaca, NY %D August 1994 %A J. Spanier %T Quasi-Monte Carlo Methods for Particle Transport Problems %B Monte Carlo and Quasi-Monte Carlo Methods in Scientific Computing %E H. Niederreiter %E P. Shiue %I Springer-Verlag %C New York, NY %P 121-148 %D 1995 %A Laszlo Szirmay-Kalos %T Application of Variational Calculus in Radiosity Method %J Periodica Polytechnica %P ? %D ? %Z to appear %A Pierre Tellier %T Synthese d'Image Realiste: Simulation d'Eclairage Interieur et Exterieur Mixte (Naturel et Artificiel) %R PhD thesis %I Universite de Rennes %C Rennes, France %D April 1993 %A Bruce Walter %A Peter Shirley %T Cost Analysis of a Monte Carlo Radiosity Algorithm %R Technical Report PCG-95-3 %I Program of Computer Graphics, Cornell University %C Cornell, NY %D May 1995 END OF FILE Ian Ashdown, P. Eng. | READ THE BOOK! Research & Development Manager | Radiosity: A Programmer's Perspective Ledalite Architectural Products Inc. | by Ian Ashdown | John Wiley & Sons, 1994 Visit http://www.ledalite.com | (Sneaky Internet Advertising) From Received: from isis.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id AAA17136; Wed, 23 Oct 1996 00:20:23 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.8.1/8.6.9) with ESMTP id AAA04853 for ; Wed, 23 Oct 1996 00:06:48 +0200 (MET DST) Received: from mercury.uniserve.com (mercury.uniserve.com [204.191.197.248]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id AAA10568 for ; Wed, 23 Oct 1996 00:06:46 +0200 (MET DST) Received: from van0129.TVS.NET (van0129.TVS.NET [204.191.197.39]) by mercury.uniserve.com (8.7.5/8.7.3) with SMTP id PAA11570; Tue, 22 Oct 1996 15:03:59 -0700 (PDT) Date: Tue, 22 Oct 1996 15:03:59 -0700 (PDT) Message-Id: <199610222203.PAA11570@mercury.uniserve.com> X-Sender: iashdown@pop.uniserve.com X-Mailer: Windows Eudora Version 2.0.3 Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed To: globillum@imag.fr From: Ian Ashdown Subject: Radiosity bibliography in BibTex X-UIDL: 5de979eff5606b1f47a2dc114bfee0d9 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit In response to intense public pressure (well, two people did complain), I have finally converted the RADBIB96 radiosity and global illumination bibliography from refer to BibTex format. I also converted the color quantization (CQUANT96) and winged edge / boundary representation (B-REP96) bibliographies. They are now available as: ftp://ftp.ledalite.com/pub/radbib96.bib ftp://ftp.ledalite.com/pub/cquant96.bib ftp://ftp.ledalite.com/pub/b-rep96.bib and also from our Web site: http://www.ledalite.com/library-/rrt.htm http://www.ledalite.com/library-/cgis.htm These files are mirrored by Greg Ward's ftp server: ftp://hobbes.lbl.gov/pub/doc while the old refer-format files are still available at: ftp://hobbes.lbl.gov/pub/doc/refer However, these files will not be updated with new releases. Thanks to Christine Piatko at NIST for providing the conversion software. Ian Ashdown, P. Eng. | READ THE BOOK! Research & Development Manager | Radiosity: A Programmer's Perspective Ledalite Architectural Products Inc. | by Ian Ashdown | John Wiley & Sons, 1994 Visit http://www.ledalite.com | (Sneaky Internet Advertising) From Received: from isis.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id UAA05441; Fri, 25 Oct 1996 20:20:51 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by isis.imag.fr (8.8.1/8.6.9) with ESMTP id TAA29913 for ; Fri, 25 Oct 1996 19:33:39 +0200 (MET DST) Received: from mercury.uniserve.com (mercury.uniserve.com [204.191.197.248]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id TAA14365 for ; Fri, 25 Oct 1996 19:33:37 +0200 (MET DST) Received: from van0416.tvs.net (van0416.tvs.net [204.191.197.116]) by mercury.uniserve.com (8.7.5/8.7.3) with SMTP id KAA21406 for ; Fri, 25 Oct 1996 10:30:48 -0700 (PDT) Date: Fri, 25 Oct 1996 10:30:48 -0700 (PDT) Message-Id: <199610251730.KAA21406@mercury.uniserve.com> X-Sender: iashdown@pop.uniserve.com (Unverified) X-Mailer: Windows Eudora Version 1.4.4 Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed To: globillum@imag.fr From: Ian Ashdown Subject: RADBIB96.BIB -- oops! X-UIDL: 9d76997cc32d07f87121445ef9694860 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Anyone who downloaded RADBIB96.BIB since it was made available earlier this week is advised to do so again. The file was inadvertently truncated at the reference {Eric P. Lafortune and Yves D. Willems}. (We exceeded our 50 MB space allocation). Our apologies for the inconvenience. For those who missed the earlier announcement, RADBIB96.BIB is available from: ftp://ftp.ledalite.com/pub/radbib96.bib and: http://www.ledalite.com/library-/rrt.htm It's also available as ftp://hobbes.lbl.gov/pub/doc/RADBIB96.Z, but please allow Greg Ward a day or so to update his copy of the file. From Received: from horus.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id PAA14864; Mon, 28 Oct 1996 15:58:27 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by horus.imag.fr (8.8.1/8.6.9) with ESMTP id PAA06105 for ; Mon, 28 Oct 1996 15:25:53 +0100 (MET) Received: from irz201.inf.tu-dresden.de (irz201.inf.tu-dresden.de [141.76.1.10]) by imag.imag.fr (8.8.1/8.6.9) with SMTP id PAA21744 for ; Mon, 28 Oct 1996 15:25:45 +0100 (MET) Received: (from cn1@localhost) by irz201.inf.tu-dresden.de (8.6.12/8.6.12-s1) id PAA26785 for globillum@imag.fr; Mon, 28 Oct 1996 15:50:36 +0200 From: "Nguyen, D.C." Message-Id: <199610281350.PAA26785@irz201.inf.tu-dresden.de> Subject: What's wrong w/ Monte-Carlo methods? To: Global Illumination List Date: Mon, 28 Oct 1996 15:50:34 +0200 (MESZ) X-Mailer: ELM [version 2.4 PL25 ME8b] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: 0507ca91c9c495845c66026ec20816b9 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 I often ask myself : Monte-Carlo ray-tracing, is this the way to do globillum in the future? After reading a lot of papers aboud MC-methods, i still get confused w/ their terminologies. I can't see any advantage of these methods over traditional methods (radiosity), except the fact that meshing is not needed, and that you can do reference-images for RMS-benchmark(!) For me, the most important feature of a rendering method is not its physical-correctness, but its efficiency and visual-asthetic-possibilty. With MC-rendering, i must spend lot of works to develope specific sampling shemes and reasonable 'good' estimators. Even w/ that, i still get useless images (too noisy!), or i must increase the sampling rate and wait forever... It is not always true that most people find noises less obsevable than aliasing.( i.e white pixels in a dark-corner vesus aliased dark-lines) . Especially for the direct lighting computation, MC-methods are definitely *NOT* the way to go. : The most regions of an image are not in shadow, so why should we cast so many shadow-rays to the light-source ? In fact, we dont need to cast any shadow-rays, if the visibilities are known a priory ( w/ shaftculling) and the radiance comming from the light can be easly computed (analytically). Only for the case, that complex-shadow occurs, MC-sampling would be helpfull. Also for this case, the soft-shadow generated w/ them can be much better without increasing the sampling rate ( We simple smooth the shadow-regions, visual-aesthetic, not physical-correct!). Of course, i could be wrong:) --JuHu From Received: from horus.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id RAA15222; Mon, 28 Oct 1996 17:16:26 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by horus.imag.fr (8.8.1/8.6.9) with ESMTP id QAA07404 for ; Mon, 28 Oct 1996 16:31:54 +0100 (MET) Received: from cs.utah.edu (cs.utah.edu [128.110.4.21]) by imag.imag.fr (8.8.1/8.6.9) with SMTP id QAA25872 for ; Mon, 28 Oct 1996 16:31:48 +0100 (MET) From: shirley@facility.cs.utah.edu Received: from wingate.cs.utah.edu by cs.utah.edu (8.6.12/utah-2.21-cs) id IAA16752; Mon, 28 Oct 1996 08:31:31 -0700 Received: by wingate.cs.utah.edu (8.6.12/utah-2.15sun-leaf) id IAA10756; Mon, 28 Oct 1996 08:31:23 -0700 Message-Id: <199610281531.IAA10756@wingate.cs.utah.edu> Subject: Re: What's wrong w/ Monte-Carlo methods? To: "Nguyen D.C." Date: Mon, 28 Oct 1996 08:31:22 -0700 (MST) Cc: globillum@imag.fr, Peter Shirley In-Reply-To: <199610281350.PAA26785@irz201.inf.tu-dresden.de> from "Nguyen, D.C." at Oct 28, 96 03:50:34 pm X-Mailer: ELM [version 2.4 PL25] Content-Type: text; charset=windows-1252 X-UIDL: 835b313c5ca97a8698ae25781d510f5c X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 MIME-Version: 1.0 Content-transfer-encoding: 8bit Wow-- we may actually get a discussion going! Is this allowed? :^) > I often ask myself : Monte-Carlo ray-tracing, is this the way to do > globillum in the future? After reading a lot of papers aboud MC-methods, i still get > confused w/ their terminologies. I can't see any advantage of these methods > over traditional methods (radiosity), except the fact that meshing is not > needed, and that you can do reference-images for RMS-benchmark(!) There is a lot of confusion on this because we all over-hype our methods in papers (me included) and as reviewers and authors we are sloppy about making people carefully characterize their methods. Here-- I will make up four scenes: 1. Lambertian Cornell box 2. Lambertian Cornell box w/smooth metal box 3. Lambertian Cornell box w/glass sphere instead of short block 4. Semi-matte (direction diffuse) Cornell box 5. Semi-matte (direction diffuse) Cornell box with "real object (10^6 patches) 1. Traditional world-space FE will work easily and we can do a walkthrough. RADIANCE will also work easily, but will not in practice allow a walkthrough-- the view-independent info is there, but it is not easily accessible. MCPT (Monte Carlo path tracing) will take all day, but will give an unbiased image (so what?). 2. Now radiosity has problems. We can add a virtual world, or use particle-tracing based radiosity with a density estimation post-process, but then doing the walktrhough is a problem. RADIANCE does fine for a given viewpoint, and we can re-use the irradiance map. MCPT will have LOTS of noise on the ceiling unless very good importance sampling is used. 3. Uh-oh-- particle tracing based radiosity works. RADIANCE and MCPT will have a very noisy caustic under the ball (although RADIANCE will not have this problem for the important glass case-- windows!). 4. Ouch. Sillion-style FE works, as does Jensen's photon map. MCPT is so dumb, it doesn't realize that this case is harder than Lambertian. RADIANCE will not work because it caches irradiance, so it will degenerate to MCPT (really, you can treat secondary bounces as Lambertian-- I believe this is a good move in almost all scenes, but it is hard to quantitatively justify). 5. Ouch^2. FE runs out of memory FAST. MCPT works no worse than 4. Jensen's photon map also works, but will be storage-intensive if the object is not very smooth. Radiance will perform as in 4. In summary, pure MCPT has only two advantages-- it is so dumb that it doesn't get hit by big scenes, and it is easy to implement. If you want an interactive walkthrough, then you are currently limited to radiosity (I use that term for all world space irradiance calculating alg's), and that limits you to a relatively small scene (100k initial polygons will kill almost all radiosity implementations). > For me, the most important feature of a rendering method is not its > physical-correctness, but its efficiency and visual-asthetic-possibilty. > With MC-rendering, i must spend lot of works to develope specific sampling > shemes and reasonable 'good' estimators. Even w/ that, i still get useless > images (too noisy!), or i must increase the sampling rate and wait forever... > It is not always true that most people find noises less obsevable than aliasing.( > i.e white pixels in a dark-corner vesus aliased dark-lines) . I agree with the above, and I think the solution is hybrid methods-- add bias! (This is blasphemy in MC circles :^) ). I do want to keep the good parts of MC methods-- they are damned robust and are possible to implement correctly-- my MC code does not bomb on wierd untweaked inputs-- tell me with a straight face that is true of most non-MC implementations. However, you are right that the results are too noisy!!! We can keep these benefits and reduce noise if we add bias the right way (not that I know what that right way is). > Especially for the direct lighting computation, MC-methods are definitely > *NOT* the way to go. : The most regions of an image are not in shadow, so why > should we cast so many shadow-rays to the light-source ? In fact, we dont > need to cast any > shadow-rays, if the visibilities are known a priory ( w/ shaftculling) and > the radiance comming from the light can be easly computed (analytically). > Only for the case, that complex-shadow occurs, MC-sampling would be > helpfull. Also for this case, the soft-shadow generated w/ them can be much > better without increasing the sampling rate ( We simple smooth the > shadow-regions, visual-aesthetic, not physical-correct!). I welcome you to implement shaft-culling on scene 5 above. Slower than MC, and will usually core-dump even with a year of implementation I'll bet. Now shaft culling on simplified geometries (which it sounds like you might be suggesting) sounds like a very good idea. Only use MC when needed-- yes, definitely smart. Overall, this has got me to again reflect on the state of our field. It is VERY hard to get a rendering paper into SIGGRAPH, even with good reviews. It is easy to get toys based on low-handing fruit into SIGGRAPH. Clearly we are doing something very wrong (you could rightly argue SIGGRAPH is doing something wrong, but that wont change anything-- we have to figure out where our share of the blame is). I think this is partially because most graphics people think TOY STORY graphics is good enough. I, however, want virtual reality that looks REAL and is predictive-- I don't want a virtual cartoon world. We are very far from getting things to look real, and from understanding our algorithms' behaviors. No working program gives useful error estimates. We have totally inadequate local reflection models. Most algorithms are memory hogs and don't parallelize. Most algorithms do a very poor job with dielectrics (water, glass). I think we need to make our own "grand challenge" models, and publicize that they can't currently be done (e.g, a human at a desk illuminated through a skylight), so that our field wont dry up and blow away. Pete From Received: from horus.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id RAA15507; Mon, 28 Oct 1996 17:43:45 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by horus.imag.fr (8.8.1/8.6.9) with ESMTP id RAA08278 for ; Mon, 28 Oct 1996 17:10:00 +0100 (MET) Received: from internet-mail2.ford.com (internet-mail2.ford.com [198.111.80.24]) by imag.imag.fr (8.8.1/8.6.9) with SMTP id RAA28377 for ; Mon, 28 Oct 1996 17:09:57 +0100 (MET) Received: by internet-mail2.ford.com id AA29410 (InterLock SMTP Gateway 3.0 for globillum@imag.fr); Mon, 28 Oct 1996 11:09:49 -0500 Message-Id: <199610281609.AA29410@internet-mail2.ford.com> Received: by internet-mail2.ford.com (Protected-side Proxy Mail Agent-1); Mon, 28 Oct 1996 11:09:49 -0500 Date: Mon, 28 Oct 96 11:09:48 -0500 From: Stephen Westin To: globillum@imag.fr In-Reply-To: <199610281350.PAA26785@irz201.inf.tu-dresden.de> (cn1@irz301.inf.tu-dresden.de) Subject: Re: What's wrong w/ Monte-Carlo methods? X-UIDL: e1fe0662411d4a1a22e42a696215def7 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Why do folks bother at all with Monte Carlo methods for global illumination? Complexity. Think of the problem of computing the irradiance at a given point. Do you want to go around the whole environment, calculating the irradiance from every object, regardless of occlusion or distance from the point? Or do you want to probe the environment, spending similar effort for every incident direction? This is the basic choice between mesh-based methods and Monte Carlo calculations. For simple environments, the mesh-based methods are excellent; they give no noise artifacts, and computation is tractable. For extremely complex environments, mesh-based algorithms tend to get inefficient. Actually, the mesh-based world and Monte Carlo are working toward each other. Hierarchical meshing is basically a way to make a mesh-based algorithm behave more like Monte Carlo, spending effort for irradiance contributions rather than for geometric complexity. And any well-designed Monte Carlo calculation uses deterministic methods wherever practical, and attempts to take advantage of spatial coherence. The ultimate global illumination method will probably be a hybrid of Monte Carlo and mesh-based methods. -Stephen H. Westin swestin@ford.com The information and opinions in this message are mine, not Ford's. From Received: from horus.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id RAA15596; Mon, 28 Oct 1996 17:47:35 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by horus.imag.fr (8.8.1/8.6.9) with ESMTP id RAA08633 for ; Mon, 28 Oct 1996 17:24:00 +0100 (MET) Received: from irz201.inf.tu-dresden.de (irz201.inf.tu-dresden.de [141.76.1.10]) by imag.imag.fr (8.8.1/8.6.9) with SMTP id RAA29205 for ; Mon, 28 Oct 1996 17:23:51 +0100 (MET) Received: (from cn1@localhost) by irz201.inf.tu-dresden.de (8.6.12/8.6.12-s1) id SAA04797; Mon, 28 Oct 1996 18:23:20 +0200 From: "Nguyen, D.C." Message-Id: <199610281623.SAA04797@irz201.inf.tu-dresden.de> Subject: Re: What's wrong w/ Monte-Carlo methods? To: shirley@facility.cs.utah.edu Date: Mon, 28 Oct 1996 18:23:19 +0200 (MESZ) Cc: cn1@irz301.inf.tu-dresden.de, globillum@imag.fr In-Reply-To: <199610281531.IAA10756@wingate.cs.utah.edu> from "shirley@facility.cs.utah.edu" at Oct 28, 96 08:31:22 am X-Mailer: ELM [version 2.4 PL25 ME8b] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: 685cca1d61fc0fe9ea8264099989012e X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 > > > Especially for the direct lighting computation, MC-methods are definitely > > *NOT* the way to go. : The most regions of an image are not in shadow, so why > > should we cast so many shadow-rays to the light-source ? In fact, we dont > > need to cast any > > shadow-rays, if the visibilities are known a priory ( w/ shaftculling) and > > the radiance comming from the light can be easly computed (analytically). > > Only for the case, that complex-shadow occurs, MC-sampling would be > > helpfull. Also for this case, the soft-shadow generated w/ them can be much > > better without increasing the sampling rate ( We simple smooth the > > shadow-regions, visual-aesthetic, not physical-correct!). > > I welcome you to implement shaft-culling on scene 5 above. Slower > than MC, and will usually core-dump even with a year > of implementation I'll bet. I've actually implemented shaft-culling for complex-scenes in GX/GENERIC. Not really shaft-culling, but a combined version of Arvo's hyperoctree and Haines's light-buffer. It's definitely faster than pur MC, because the cost for collision-test between a beam and a bbox is quite the same between a ray and a bbox. --JuHu From Received: from horus.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id TAA15993; Mon, 28 Oct 1996 19:14:42 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by horus.imag.fr (8.8.1/8.6.9) with ESMTP id SAA10101 for ; Mon, 28 Oct 1996 18:26:23 +0100 (MET) Received: from gateway.lightscape.com (gate-gateway.lightscape.com [206.139.79.2]) by imag.imag.fr (8.8.1/8.6.9) with SMTP id SAA03175 for ; Mon, 28 Oct 1996 18:26:16 +0100 (MET) Received: from topo.lightscape.com by gateway.lightscape.com via ESMTP (950511.SGI.8.6.12.PATCH526/940406.SGI.AUTO) for <@gateway.lightscape.com:globillum@imag.fr> id JAA09196; Mon, 28 Oct 1996 09:24:25 -0800 Received: from basil.lightscape.com by topo.lightscape.com via ESMTP (940816.SGI.8.6.9/940406.SGI.AUTO) for <@topo.lightscape.com:globillum@imag.fr> id JAA08894; Mon, 28 Oct 1996 09:24:25 -0800 Received: from basil by basil.lightscape.com via SMTP (940816.SGI.8.6.9/940406.SGI.AUTO) for id JAA25333; Mon, 28 Oct 1996 09:24:23 -0800 Sender: greg@lightscape.com Message-ID: <3274EC47.41C6@lightscape.com> Date: Mon, 28 Oct 1996 09:24:23 -0800 From: Greg Spencer Organization: Lightscape Technologies, Inc. http://www.lightscape.com X-Mailer: Mozilla 3.0Gold (X11; U; IRIX 5.3 IP22) MIME-Version: 1.0 To: globillum@imag.fr Subject: Lens measurement? Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: 845fedcea2fdc5e031cb4fb00c455742 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 This isn't directly related to global illumination, but does relate to physically-based rendering. Does anyone know where one might get a real camera lens measured in order to calibrate it -- i.e., the distortion, chromatic abberations, intensity falloff, etc? I'd like to plug the results into a rendering system to get good approximations of a physical lens, but I have no data... It doesn't have to be a free service, but those are (of course) preferred. I've heard several rumors about a "European" company that does this sort of thing (for a large fee), but that's the entire rumor. Please respond to me directly, since I don't want to fill your mailboxes with non-related junk. I'll post a summary of responses in a week. I've researched using the Tsai method for calibration, but that uses video cameras and iteration... I would like to be able to measure lenses used for film cameras. Thanks! -Greg. -- Greg Spencer, Software Engineer greg@lightscape.com Lightscape Technologies., Inc. (408) 342-1900 http://www.lightscape.com (PGP key available upon request) From Received: from horus.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id VAA16366; Mon, 28 Oct 1996 21:47:29 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by horus.imag.fr (8.8.1/8.6.9) with ESMTP id VAA11457 for ; Mon, 28 Oct 1996 21:25:17 +0100 (MET) Received: from lsi.lsil.com (lsi.lsil.com [147.145.40.2]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id VAA10883 for ; Mon, 28 Oct 1996 21:25:15 +0100 (MET) Received: from mhost.lsil.com (mhost.lsil.com [147.145.69.84]) by lsi.lsil.com with SMTP id MAA06905 (8.6.12/IDA-1.6 for ); Mon, 28 Oct 1996 12:25:09 -0800 Received: from sjs1 by mhost.lsil.com id AA04540 (4.1/SMI-4.1 for globillum@imag.fr); Mon, 28 Oct 96 12:25:03 PST Received: from sj80.lsil.com by sjs1 (4.1/SMI-4.1) id AA21784; Mon, 28 Oct 96 12:25:02 PST Date: Mon, 28 Oct 96 12:25:02 PST From: Al Zimmerman Message-Id: <9610282025.AA21784@sjs1> To: globillum@imag.fr Subject: quadratic intersection Cc: alz@lsil.com X-UIDL: 1a57d64e89a8bae3bdaa88d9801b1924 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit I was reading up on ray intersection with a quadratic and I always see mention of the Q matrix, but I can't find any material describing how to construct the Q matrix. The Q matrix is mentioned in just about every piece of documentation that deals with intersecting a ray with a quadratic, but none of the documentation states how to construct the matrix. The only documentation I can find deals with the Q matrix when the quadratic is in homogeneous coordinates where most of the variables in the Q matrix go to zero. To work around this problem, I've seen solutions to translate the quadratic back to the origin, scale , and then rotate to lie on the axis. Now use the homogeneous Q matrix for intersection. Does anyone know how to construct the Q matrix when the quadratic is not in homogeneous unit coordinates ? Thanks in advance, Al Z From Received: from horus.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id WAA16381; Mon, 28 Oct 1996 22:00:38 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by horus.imag.fr (8.8.1/8.6.9) with ESMTP id VAA11465 for ; Mon, 28 Oct 1996 21:36:33 +0100 (MET) Received: from Xenon.Stanford.EDU (Xenon.Stanford.EDU [171.64.64.24]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id VAA11226 for ; Mon, 28 Oct 1996 21:36:22 +0100 (MET) Received: (from ericv@localhost) by Xenon.Stanford.EDU (8.7.6/8.7.1) id MAA17462 for globillum@imag.fr; Mon, 28 Oct 1996 12:36:15 -0800 (PST) From: Eric Veach Message-Id: <199610282036.MAA17462@Xenon.Stanford.EDU> Subject: Re: What's wrong w/ Monte-Carlo methods? To: globillum@imag.fr Date: Mon, 28 Oct 1996 12:36:11 -0800 (PST) In-Reply-To: <199610281350.PAA26785@irz201.inf.tu-dresden.de> from "Nguyen, D.C." at Oct 28, 96 03:50:34 pm X-Mailer: ELM [version 2.4 PL25] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: 59ca2e39e0192639e77d0360bd041f33 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 One of the big advantages of MC algorithms is that they let you model the scene you actually want to use. Sure, radiosity algorithms can be efficient --- if we limit ourselves to diffuse surfaces, with maybe a few mirrors or whatever that are handled in a ray-tracing pass. But flat polygons and diffuse reflectors do not go very far in modeling the real world, and finite-element algorithms don't seem to be practical for much more than this. (Memory usage blows up for complex scenes, or when there are lots of glossy surfaces.) This is an important issue in graphics, since often the biggest source of error is the scene model itself. What good is an accurate solution to the wrong scene model? At least MC algorithms start with the desired input. Even if you aren't interested in physically correct results, diffuse surfaces lead to that wonderful "computer graphics look" we all know and love. It's no wonder that radiosity algorithms tend to be faster, since they are solving a much simpler problem: the solution is only a two-dimensional function rather than a four-dimensional one. To me, the amazing thing is that radiosity algorithms need to be so *complicated* to be efficient. By the time you implement discontinuity meshing, hierarchical basis functions, clustering, shaft culling, etc., how many lines of code are we talking about? And can you actually trust it not to core-dump, and to compute a reasonable result in a reasonable amount of time? And let's not kid ourselves that an algorithm is "general" just because it can handle a few mirrors or glossy surfaces. The real test of generality is how an algorithm performs when there are *no* diffuse surfaces, since that's how it is in the real world. Another reason to use MC algorithms is scene complexity. Finite element algorithms work with explicit representations of the scene and its properties. They are strongly affected by the size and complexity of the scene representation. On the other hand, Monte Carlo algorithms are based on sampling, which means that the scene model is accessed through a small set of queries (e.g. what is the first surface point intersected by this ray?) This hides the scene complexity behind a layer of abstraction, and can mean that rendering times are only loosely coupled to the scene representation (e.g. it may affect the time required to cast a ray). In effect, Monte Carlo algorithms can sample the scene to determine the information they actually need, while deterministic algorithms examine every detail, whether it is relevant or not. That's not to say that MC algorithms need to sample *everything*. It's perfectly reasonable to embed deterministic calculations within a Monte Carlo framework, especially for low-dimensional integration problems (e.g.\ direct lighting from a small number of uniform, diffuse, polygonal luminaires). Sometimes this introduces bias, but often this is okay, especially when we can bound the errors or at least characterize them. Ideally, rendering algorithms should not depend on the details of the scene representation, but only on the underlying mathematical model. For example, a square area light source can be simulated fairly well with a ten by ten array of point sources, but many rendering algorithms would have a much worse performance in the second case. Similarly, if we replace the square light source by two flourescent bulbs covered by a diffusely transmitting panel, why should it make a huge difference to our algorithms? The same comments apply to geometric complexity: if we represent an indoor plant as a thousand polygons or a million Bezier patches, how much should the rendering time go up? I can't say that MC algorithms have achieved this level of isolation from the scene representation, but at least it seems that the opportunity is there. There has been a lot of emphasis on rendering algorithms that exploit special properties of the input scene, e.g. that lighting is direct rather than through a diffusing panel or bouncing off the ceiling. It would be nice to see more work on algorithms whose performance does not go down the tubes when these conditions are not met, i.e. algorithms that are more *robust*. It seems that this should be possible without resorting to the level of "dumbness" found in MCPT (as Pete Shirley put it). I guess the last major issue for MC algorithms is the correctness of the results. Here it is important to distinguish between unbiased, biased, and consistent estimators. Intuitively, an unbiased estimator computes the right answer, on average. A biased estimator computes the wrong answer, on average. A consistent estimator also computes the wrong answer, on average, but the error can be made arbitrarily small by increasing the number of samples. Most of the "biased" algorithms in graphics are in fact consistent, otherwise we wouldn't have any confidence at all in their results. The main advantage of unbiased algorithms is that they make it far easier to estimate the error in a solution. For unbiased algorithms, this error can be estimated by the sample variance, since any error is guaranteed to show up as random variation among the samples. Thus, if an unbiased image is not noisy, we can be reasonably sure that it is correct. For scene of realistic complexity, this seems to be the only practical way to generate correct images. For algorithms which are merely consistent, however, we must also bound the bias. In general this is difficult to do; we cannot estimate bias by simply drawing a few more samples. Bias shows up as results that are not noisy, but in fact are incorrect. In graphics algorithms, this error is often noticeable visually, in the form of discontinuities, excessive blurring, or surface shading that just looks wrong. Other things being equal, it is clear that we should prefer an unbiased algorithm. If these algorithms were also robust and efficient, then why would we want to use anything else? However, conventional wisdom says that unbiased methods are "too expensive", and that we can achieve an acceptable image in less time by making approximations. But where is the research to support this claim? There has been a huge amount of effort on approximate methods in graphics, while there has been hardly any work on unbiased algorithms. Some people seem to think that "unbiased" is a synonym for "pure Monte Carlo path tracing". Until we have thoroughly explored this type of algorithm, we can hardly make judgements on their capabilities. I would like to see more results on what can and cannot be achieved by unbiased methods, so that we can make better decisions on these issues. (Can you tell that I'm writing a thesis? :-) Eric From Received: from horus.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id PAA20500; Tue, 29 Oct 1996 15:09:02 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by horus.imag.fr (8.8.1/8.6.9) with ESMTP id OAA20974 for ; Tue, 29 Oct 1996 14:14:01 +0100 (MET) Received: from igw3.watson.ibm.com (igw3.watson.ibm.com [129.34.139.18]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id OAA29971 for ; Tue, 29 Oct 1996 14:13:58 +0100 (MET) Received: from mailhub1.watson.ibm.com (mailhub1.watson.ibm.com [9.2.249.31]) by igw3.watson.ibm.com (8.7.6/8.7.1) with ESMTP id IAA10720; Tue, 29 Oct 1996 08:13:59 -0500 Received: from watngi01.watson.ibm.com (watngi01.watson.ibm.com [9.2.235.20]) by mailhub1.watson.ibm.com (8.7.1/10-26-96) with SMTP id IAA724477; Tue, 29 Oct 1996 08:13:46 -0500 Received: by watngi01.watson.ibm.com(Lotus SMTP MTA Release 1.0.1) id 852563D2.0048A25C ; Tue, 29 Oct 1996 08:13:21 -0400 X-Lotus-FromDomain: IBM RESEARCH From: "Holly Rushmeier" To: shirley@facility.cs.utah.edu cc: cn1@irz301.inf.tu-dresden.de, globillum@imag.fr Message-ID: <852563D2:0047B6D7.00@watngi01.watson.ibm.com> Date: Tue, 29 Oct 1996 08:11:58 -0400 Subject: Re: What's wrong w/ Monte-Carlo methods? Mime-Version: 1.0 Content-type: text/plain; charset=us-ascii; format=flowed X-UIDL: 3df6dd4f3c62c4bdb0be46fae764c082 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit I would take issue with one of Pete's statements: >In summary, pure MCPT has only two advantages-- it is so dumb >that it doesn't get hit by big scenes, and it is easy to implement. >If you want an interactive walkthrough, then you are currently >limited to radiosity (I use that term for all world space >irradiance calculating alg's), and that limits you to >a relatively small scene (100k initial polygons will kill >almost all radiosity implementations). The big deal about image-based rendering, i.e. QuickTimeVR (or PanoramIX :) ), or the more advanced Light Field Rendering or Lumigraph is that we can interactively walkthrough scenes precomputed with Monte Carlo -- the same way you can walk through a scene precomputed with radiosity. -- Holly From Received: from horus.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id PAA20511; Tue, 29 Oct 1996 15:10:05 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by horus.imag.fr (8.8.1/8.6.9) with ESMTP id OAA21136 for ; Tue, 29 Oct 1996 14:24:09 +0100 (MET) Received: from cs.utah.edu (cs.utah.edu [128.110.4.21]) by imag.imag.fr (8.8.1/8.6.9) with SMTP id OAA00572 for ; Tue, 29 Oct 1996 14:23:58 +0100 (MET) From: shirley@facility.cs.utah.edu Received: from wingate.cs.utah.edu by cs.utah.edu (8.6.12/utah-2.21-cs) id GAA12076; Tue, 29 Oct 1996 06:23:46 -0700 Received: by wingate.cs.utah.edu (8.6.12/utah-2.15sun-leaf) id GAA11490; Tue, 29 Oct 1996 06:23:45 -0700 Message-Id: <199610291323.GAA11490@wingate.cs.utah.edu> Subject: Re: What's wrong w/ Monte-Carlo methods? To: Holly Rushmeier Date: Tue, 29 Oct 1996 06:23:45 -0700 (MST) Cc: shirley@facility.cs.utah.edu, cn1@irz301.inf.tu-dresden.de, globillum@imag.fr In-Reply-To: <852563D2:0047B6D7.00@watngi01.watson.ibm.com> from "Holly Rushmeier" at Oct 29, 96 08:11:58 am X-Mailer: ELM [version 2.4 PL25] Content-Type: text; charset=windows-1252 X-UIDL: 5752f261e1d7004c2fa7b0afbf18841e X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 MIME-Version: 1.0 Content-transfer-encoding: 8bit Holly is of course right! As a MCPT fan (maybe you couldn't tell that from my note-- it is my favorite rendering alg, because although it is flawed, I think its flaws are easier to fix than other alg's flaws-- see Eric Veach's note), I was very happy to see that image-based stuff get big-- where will those images come from? :^) Also, my comments really apply to "naive" MCPT-- if you add bias or good importance sampling, it may end up being practical even without Image-based stuff. Pete > > I would take issue with one of Pete's statements: > > >In summary, pure MCPT has only two advantages-- it is so dumb > >that it doesn't get hit by big scenes, and it is easy to implement. > >If you want an interactive walkthrough, then you are currently > >limited to radiosity (I use that term for all world space > >irradiance calculating alg's), and that limits you to > >a relatively small scene (100k initial polygons will kill > >almost all radiosity implementations). > > The big deal about image-based rendering, i.e. QuickTimeVR > (or PanoramIX :) ), or the more advanced Light Field Rendering or > Lumigraph is that we can interactively walkthrough scenes > precomputed with Monte Carlo -- the same way you can walk > through a scene precomputed with radiosity. > > -- Holly > > > > > > From Received: from horus.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id SAA21406; Tue, 29 Oct 1996 18:05:57 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by horus.imag.fr (8.8.1/8.6.9) with ESMTP id RAA26547 for ; Tue, 29 Oct 1996 17:23:50 +0100 (MET) Received: from central.cis.upenn.edu (CENTRAL.CIS.UPENN.EDU [158.130.12.2]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id RAA11133 for ; Tue, 29 Oct 1996 17:23:48 +0100 (MET) Received: from graphics.cis.upenn.edu (GRAPHICS.CIS.UPENN.EDU [158.130.2.10]) by central.cis.upenn.edu (8.6.12/UPenn 1.4) with ESMTP id LAA18919; Tue, 29 Oct 1996 11:23:40 -0500 Received: from GRAPHICS.CIS.UPENN.EDU by graphics.cis.upenn.edu id QAA04113; Tue, 29 Oct 1996 16:23:39 GMT Posted-Date: Tue, 29 Oct 1996 16:23:38 GMT Message-Id: <199610291623.QAA04113@graphics.cis.upenn.edu> X-Mailer: exmh version 1.6.7 5/3/96 To: "Holly Rushmeier" cc: shirley@facility.cs.utah.edu, cn1@irz301.inf.tu-dresden.de, globillum@imag.fr, jnimerof@graphics.cis.upenn.edu Subject: Re: What's wrong w/ Monte-Carlo methods? In-reply-to: Your message of "Tue, 29 Oct 1996 08:11:58 -0400." <852563D2:0047B6D7.00@watngi01.watson.ibm.com> Date: Tue, 29 Oct 1996 11:23:38 -0500 From: "Jeffry S. Nimeroff" X-UIDL: 7909b7161a0bea1f6f510ff168235a3d X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit > > The big deal about image-based rendering, i.e. QuickTimeVR > (or PanoramIX :) ), or the more advanced Light Field Rendering or > Lumigraph is that we can interactively walkthrough scenes > precomputed with Monte Carlo -- the same way you can walk > through a scene precomputed with radiosity. > > -- Holly > Well, I have to take exception with this statement, at least for now (sorry Holly :-)). The lumigraph and light fields are for the space around convex regions of the environment (inside the "slabs") or for a free space region inside an interior scene. Freedom of movement (quick indexing of the data structure) can be done using hardware texturing which is nice, but the method is not applicable for any environments I would consider outstanding. Being able to orbit around or pan near a small cluster of objects is not much more novel than the capabilities supplied in Quicktime VR and I don't know of many interior scenes that have lots of free space (pathways without occlusions like columns, or furniture). There is a simple modification of light-fields that allows full range of motion within computer-rendered scenes that is equally as efficient as the original implementation, but you'll have to wait for my newest work to be done :-). And if you want moving objects in your scene (a sense of time)... -Jeff From Received: from horus.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id TAA21702; Tue, 29 Oct 1996 19:03:03 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by horus.imag.fr (8.8.1/8.6.9) with ESMTP id SAA28221 for ; Tue, 29 Oct 1996 18:36:25 +0100 (MET) Received: from grolsch.cs.ubc.ca (grolsch.cs.ubc.ca [142.103.6.9]) by imag.imag.fr (8.8.1/8.6.9) with SMTP id SAA15221 for ; Tue, 29 Oct 1996 18:36:23 +0100 (MET) Received: from chaplin.cs.ubc.ca (fournier@chaplin.cs.ubc.ca [142.103.9.32]) by grolsch.cs.ubc.ca (8.6.12/8.6.9) with SMTP id JAA18989; Tue, 29 Oct 1996 09:35:57 -0800 Date: Tue, 29 Oct 1996 09:35:57 -0800 From: Alain Fournier Message-Id: <199610291735.JAA18989@grolsch.cs.ubc.ca> To: HOLLY@watson.ibm.com, jnimerof@graphics.cis.upenn.edu Subject: Re: What's wrong w/ Monte-Carlo methods? Cc: cn1@irz301.inf.tu-dresden.de, globillum@imag.fr, shirley@facility.cs.utah.edu X-UIDL: 52fa7bf2be49a9c1c085588c56f1fba2 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Quick remark (and boy, have I been wrong before): I think the light field techniques are very interesting and valuable, but not as primary rendering techniques (if they were ever intended that way). They will be especially useful when merged with CG scenes rendered from models (with global illum, natch, also merging with real scenes won't hurt). Paper at 11:00. From Received: from horus.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id WAA22304; Tue, 29 Oct 1996 22:11:50 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by horus.imag.fr (8.8.1/8.6.9) with ESMTP id VAA03126 for ; Tue, 29 Oct 1996 21:36:55 +0100 (MET) Received: from gate.mental.com (GATE.MENTAL.COM [192.31.14.2]) by imag.imag.fr (8.8.1/8.6.9) with SMTP id VAA21990 for ; Tue, 29 Oct 1996 21:36:53 +0100 (MET) Received: (from smap@localhost) by gate.mental.com (8.6.12/Lobo-960523) id VAA19469; Tue, 29 Oct 1996 21:36:49 +0100 Received: from twen(172.16.0.5) by gate via smap (V1.3) id sma019466; Tue Oct 29 21:36:27 1996 Received: (from henrik@localhost) by mental.com (8.6.12/Lobo-960725) id VAA05219; Tue, 29 Oct 1996 21:38:44 +0100 From: Henrik Wann Jensen Message-Id: <199610292038.VAA05219@mental.com> Subject: Re: What's wrong w/ Monte-Carlo methods? To: Eric Veach Date: Tue, 29 Oct 1996 21:38:43 +0100 (MET) Cc: globillum@imag.fr In-Reply-To: <199610282036.MAA17462@Xenon.Stanford.EDU> from "Eric Veach" at Oct 28, 96 12:36:11 pm X-Mailer: ELM [version 2.4 PL22] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: 776f3fc538ff5f4c31cd68513a423fd0 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Eric Veach wrote: > MC is better than FE... I agree :-) > Other things being equal, it is clear that we should prefer an > unbiased algorithm. I vote for consistent MC-methods since they really are significantly faster than the unbiased methods we have seen so far. Just take the irradiance gradient caching scheme by Greg Ward and the photon map :) > The main advantage of unbiased algorithms is that they make it > far easier to estimate the error in a solution. It's true that the error can be estimated for unbiased methods but this estimate is probabilistic which in my opinion makes it less useful since you cannot really trust your result but only be "reasonably sure" that it is correct. > I would like to see more results on what can and > cannot be achieved by unbiased methods, so that we can make > better decisions on these issues. You can solve all rendering problems using unbiased techniques such as path tracing and bidirectional path tracing. But for certain problems these methods are *very* inefficient. Path tracing is not practical for rendering caustics. Bidirectional path tracing is much better at visualizing caustics but it fails when it comes to rendering the mirror reflection of caustics (created by a small light source). Consider for example a glass of cognac on a procedural surface :) Even bidirectional path tracing would have a hard time computing the illumination of the surface just below the glass and it would be very costly (and time-consuming) computing billions of intersection points with a complex procedural surface. This problem is much easier to solve if you allow storing illumination information in the model (=bias). - Henrik From Received: from horus.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id DAA22869; Wed, 30 Oct 1996 03:10:57 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by horus.imag.fr (8.8.1/8.6.9) with ESMTP id CAA03955 for ; Wed, 30 Oct 1996 02:58:26 +0100 (MET) Received: from Xenon.Stanford.EDU (Xenon.Stanford.EDU [171.64.64.24]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id CAA28255 for ; Wed, 30 Oct 1996 02:58:21 +0100 (MET) Received: (from ericv@localhost) by Xenon.Stanford.EDU (8.7.6/8.7.1) id RAA21466; Tue, 29 Oct 1996 17:58:01 -0800 (PST) From: Eric Veach Message-Id: <199610300158.RAA21466@Xenon.Stanford.EDU> Subject: Re: What's wrong w/ Monte-Carlo methods? To: Henrik Wann Jensen Date: Tue, 29 Oct 1996 17:58:01 -0800 (PST) Cc: ericv@cs.stanford.edu, globillum@imag.fr In-Reply-To: <199610292038.VAA05219@mental.com> from "Henrik Wann Jensen" at Oct 29, 96 09:38:43 pm X-Mailer: ELM [version 2.4 PL25] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: 6c86fef92a10fed4a89dee176f4e968e X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Henrik Wann Jensen writes: | > MC is better than FE... Hey, I didn't say that. Finite element methods also have advantages, I just didn't mention them. | > Other things being equal, it is clear that we should prefer an ^^^^^^^^^^^^^^^^^^^^^^^^ | > unbiased algorithm. | | I vote for consistent MC-methods since they really are significantly faster | than the unbiased methods we have seen so far. Just take the irradiance | gradient caching scheme by Greg Ward and the photon map :) The point is that you can't judge the whole class of unbiased algorithms based on a couple of examples. If you had an unbiased algorithm that was just as fast, wouldn't you use it? Such an algorithm doesn't exist yet, but we haven't seen any solid evidence that this goal is impossible. It's going to take more research before we know what can be achieved. | It's true that the error can be estimated for unbiased methods but | this estimate is probabilistic which in my opinion makes it less useful | since you cannot really trust your result but only be "reasonably sure" | that it is correct. Well, that's still better than no error estimates at all, which is what you get with biased or consistent algorithms. For example, let's consider your photon map. I like this algorithm, and I think it's a great practical tool. But like many consistent algorithms, it can make large errors that are difficult to characterize (as I'm sure you are aware). Let's look at some of the situations where this happens. For some scenes, the results can be wrong by an arbitrary amount. The cognac glass sitting on a fractal surface is a perfect example. Given some point "x" to be shaded, you find the smallest sphere centered at "x" that encloses N photon hits. Then you estimate irradiance by assuming that the scene is locally planar, i.e. its intersection with the interior of the sphere is approximately a flat *disc*. Thus to get irradiance, the power carried by each photon is divided by (Pi * r^2). This obviously doesn't make any sense for a fractal surface. The area of the surface within a sphere of radius "r" is much larger than Pi * r^2 (for a true fractal, the area would be infinite, but even for the reasonably fine subdivisions you are using, it would be significantly higher). So, the caustics in your images are probably much brighter than they should be. Similarly, the disc estimate will be substantially wrong near corners, or for narrow objects (dangling power cords, wire cages, blades of grass), or for parallel surfaces that are close together (e.g. a slide tray, or vertical blinds). The errors are not small -- we're talking about factors of two, or ten, or even a hundred. The error depends on the ratio of the true surface area over which the photons are distributed, vs. the area of the approximating disc. Now, the photon map is a consistent estimator, so these errors will get smaller as the number of photons is increased. But for these examples, it would take incredible numbers of photons to get a reasonable error. Let's consider the handle on my coffee mug. It has a diameter of about 1cm. For the disc estimate to be reasonable (say within 20%), the diameter of the corresponding sphere must be a couple of millimeters at most. This sphere is supposed to enclose N=50 or so photons, according to your rules of thumb, so this implies a density of about ten million photon hits per square meter. Since all of these photons are stored in a search tree, the memory requirements would be ridiculous for typical scenes. These kinds of errors are typical of many rendering algorithms that are only claim consistency. I have just been using the photon map as an example. In fact, it would be my first choice for some applications. Let's face it, we are stuck with consistent algorithms for many problems (until something better comes along). However, I don't think it's fair to compare the photon map with an unbiased algorithm like bidirectional path tracing. Sure, there are situations where bidirectional path tracing does not work well either, but at least the errors can be detected and estimated by means of the sample variance. Eric From Received: from horus.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id KAA00845; Wed, 30 Oct 1996 10:36:10 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by horus.imag.fr (8.8.1/8.6.9) with ESMTP id KAA07171 for ; Wed, 30 Oct 1996 10:10:53 +0100 (MET) Received: from gate.mental.com (GATE.MENTAL.COM [192.31.14.2]) by imag.imag.fr (8.8.1/8.6.9) with SMTP id KAA17835 for ; Wed, 30 Oct 1996 10:10:49 +0100 (MET) Received: (from smap@localhost) by gate.mental.com (8.6.12/Lobo-960523) id KAA19845; Wed, 30 Oct 1996 10:10:07 +0100 Received: from twen(172.16.0.5) by gate via smap (V1.3) id sma019843; Wed Oct 30 10:10:03 1996 Received: (from henrik@localhost) by mental.com (8.6.12/Lobo-960725) id KAA13846; Wed, 30 Oct 1996 10:12:19 +0100 From: Henrik Wann Jensen Message-Id: <199610300912.KAA13846@mental.com> Subject: Re: What's wrong w/ Monte-Carlo methods? To: Eric Veach Date: Wed, 30 Oct 1996 10:12:19 +0100 (MET) Cc: globillum@imag.fr In-Reply-To: <199610300158.RAA21466@Xenon.Stanford.EDU> from "Eric Veach" at Oct 29, 96 05:58:01 pm X-Mailer: ELM [version 2.4 PL22] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: 798a4e3b924b6e637a6e514bc5c04683 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Thus spoke Eric Veach: > > Henrik Wann Jensen writes: > | > MC is better than FE... > > Hey, I didn't say that. Finite element methods also have > advantages, I just didn't mention them. I were just abbreviating your intro ;-) > If you had an unbiased algorithm that was just as fast, wouldn't you use it? I sure would. In my examples I was simply refering to the two wellknown examples of unbiased path tracing based algorithms and they are very slow. > For the disc estimate to > be reasonable (say within 20%), the diameter of the corresponding > sphere must be a couple of millimeters at most. This sphere is > supposed to enclose N=50 or so photons, according to your rules > of thumb, so this implies a density of about ten million photon > hits per square meter. Since all of these photons are stored in > a search tree, the memory requirements would be ridiculous for > typical scenes. I agree that the basic photon map implementation can give large errors. These errors can be reduced by using different filtering techniques but still, I agree, if you want absolute confidence in your result you may need a large number of photons. The same does, however, apply to path tracing. A student of mine recently investigated the error estimates for unbiased path tracing. His results indicate that just having a confidence of 15% (five percent) that you are within 1% of the correct result required for most pixels thousands of sample rays and for some pixels (such as the edges of light sources) the number of rays exploded. But I must admit that I really like the unbiased path tracing algorithms and they would be my choice if I wanted to have absolute confidence in the result. They are, however, not very practical for everyday rendering. - Henrik From Received: from horus.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id QAA02483; Wed, 30 Oct 1996 16:19:40 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by horus.imag.fr (8.8.1/8.6.9) with ESMTP id PAA13125 for ; Wed, 30 Oct 1996 15:43:50 +0100 (MET) Received: from gate.mental.com (GATE.MENTAL.COM [192.31.14.2]) by imag.imag.fr (8.8.1/8.6.9) with SMTP id PAA06946 for ; Wed, 30 Oct 1996 15:43:48 +0100 (MET) Received: (from smap@localhost) by gate.mental.com (8.6.12/Lobo-960523) for id PAA20120; Wed, 30 Oct 1996 15:43:46 +0100 Received: from twen(172.16.0.5) by gate via smap (V1.3) id sma020118; Wed Oct 30 15:43:38 1996 Received: (from henrik@localhost) by mental.com (8.6.12/Lobo-960725) for globillum@imag.fr id PAA20618; Wed, 30 Oct 1996 15:45:49 +0100 From: Henrik Wann Jensen Message-Id: <199610301445.PAA20618@mental.com> Subject: Re: What's wrong w/ Monte-Carlo methods? To: globillum@imag.fr Date: Wed, 30 Oct 1996 15:45:49 +0100 (MET) X-Mailer: ELM [version 2.4 PL22] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: c06c984de06043a135e9b72982acb349 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Henrik Wann Jensen wrote: > His results indicate that just having a confidence of 15% (five percent).. This should be 15% and not 5% and btw. the scene was a simple Cornell box model. - Henrik From Received: from horus.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id RAA02925; Wed, 30 Oct 1996 17:45:22 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by horus.imag.fr (8.8.1/8.6.9) with ESMTP id RAA15480 for ; Wed, 30 Oct 1996 17:13:19 +0100 (MET) Received: from igw3.watson.ibm.com (igw3.watson.ibm.com [129.34.139.18]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id RAA13090 for ; Wed, 30 Oct 1996 17:13:16 +0100 (MET) Received: from mailhub1.watson.ibm.com (mailhub1.watson.ibm.com [9.2.249.31]) by igw3.watson.ibm.com (8.7.6/8.7.1) with ESMTP id LAA14028; Wed, 30 Oct 1996 11:13:18 -0500 Received: from watngi01.watson.ibm.com (watngi01.watson.ibm.com [9.2.235.20]) by mailhub1.watson.ibm.com (8.7.1/10-26-96) with SMTP id LAA548968; Wed, 30 Oct 1996 11:13:06 -0500 Received: by watngi01.watson.ibm.com(Lotus SMTP MTA Release 1.0.1) id 052563D3.00590FC4 ; Wed, 30 Oct 1996 11:12:47 -0400 X-Lotus-FromDomain: IBM RESEARCH From: "Holly Rushmeier" To: henrik@mental.com cc: ericv@cs.stanford.edu, globillum@imag.fr Message-ID: <852563D3:0057ED7B.00@watngi01.watson.ibm.com> Date: Wed, 30 Oct 1996 11:11:38 -0400 Subject: Re: What's wrong w/ Monte-Carlo methods? Mime-Version: 1.0 Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: 0f6434031d9373848027654a85dd767e X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit To: ericv @ CS.Stanford.EDU cc: globillum @ imag.fr (bcc: Holly Rushmeier/Watson/IBM Research) From: henrik @ mental.com Date: 10/30/96 10:12:19 AM Z-1 Subject: Re: What's wrong w/ Monte-Carlo methods? Henrik wrote: >The same does, however, apply to path tracing. A student of mine recently investigated the >error estimates for unbiased path tracing. His results >indicate that just having a confidence of 15% (five percent) that you >are within 1% of the correct result required for most pixels thousands >of sample rays and for some pixels (such as the edges of light sources) >the number of rays exploded. Werner Purgathofer did a nice analysis of the number of samples needed for anti-aliasing in "A Statistical Method for Adaptive Sampling" in Computers and Graphics, 1987, pp. 157-162. Using his methodology, and taking into account the dynamic range of the global illumination problem, assuming simple minded tone mapping, allowing an error of +/- 10 in final pixel value (out of 0-255) and a requiring an 80% confidence level gives a minimum sampling rate of 16094 (see Rushmeier & Ward, "Energy Preserving Non-Linear Filters", Siggraph 94, pp 131 - 138) The above paper also brings up the notion, that rather than use a biased algorithm, you can compute a result with an unbiased algorithm, and then filter the results for consistency based on the values and error estimates that you get. -- Holly From Received: from horus.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id UAA03374; Wed, 30 Oct 1996 20:33:06 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by horus.imag.fr (8.8.1/8.6.9) with ESMTP id SAA19087 for ; Wed, 30 Oct 1996 18:38:47 +0100 (MET) Received: from central.cis.upenn.edu (CENTRAL.CIS.UPENN.EDU [158.130.12.2]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id SAA17963 for ; Wed, 30 Oct 1996 18:38:45 +0100 (MET) Received: from graphics.cis.upenn.edu (GRAPHICS.CIS.UPENN.EDU [158.130.2.10]) by central.cis.upenn.edu (8.6.12/UPenn 1.4) with ESMTP id MAA28301; Wed, 30 Oct 1996 12:38:43 -0500 Received: from GRAPHICS.CIS.UPENN.EDU by graphics.cis.upenn.edu id RAA00607; Wed, 30 Oct 1996 17:38:40 GMT Posted-Date: Wed, 30 Oct 1996 17:38:40 GMT Message-Id: <199610301738.RAA00607@graphics.cis.upenn.edu> X-Mailer: exmh version 1.6.7 5/3/96 To: "Holly Rushmeier" cc: henrik@mental.com, ericv@cs.stanford.edu, globillum@imag.fr, jnimerof@graphics.cis.upenn.edu Subject: Re: What's wrong w/ Monte-Carlo methods? In-reply-to: Your message of "Wed, 30 Oct 1996 11:11:38 -0400." <852563D3:0057ED7B.00@watngi01.watson.ibm.com> Date: Wed, 30 Oct 1996 12:38:40 -0500 From: "Jeffry S. Nimeroff" X-UIDL: 78b17c51f2cb1c169cff14574f6e80eb X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit > > Werner Purgathofer did a nice analysis of the number of samples > needed for anti-aliasing in "A Statistical Method for Adaptive > Sampling" in Computers and Graphics, 1987, pp. 157-162. > > Using his methodology, and taking into account the dynamic range > of the global illumination problem, assuming simple minded > tone mapping, allowing an error of +/- 10 in > final pixel value (out of 0-255) and a requiring an 80% confidence > level gives a minimum sampling rate of 16094 (see Rushmeier & Ward, > "Energy Preserving Non-Linear Filters", Siggraph 94, pp 131 - 138) > > The above paper also brings up the notion, that rather than use a > biased algorithm, you can compute a result with an unbiased algorithm, and > then filter the results for consistency based on the values and error > estimates that you get. > > -- Holly > I think this brings up the best motivation of all. Unbiased algorithm, then filtering for results. Not being a MC person myself, has work been done in this manner. It always seems that the algorithms themselves are either unbiased (with proponents talking about error bounds and validation), or biased (with proponents talking about consistency and/or promoting the "look" of the results). It seems like efficiency increases with error bounds (even if they are conservative) can best be accomplished by meeting in the middle. -Jeff From Received: from horus.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id XAA03752; Wed, 30 Oct 1996 23:26:27 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by horus.imag.fr (8.8.1/8.6.9) with ESMTP id XAA20640 for ; Wed, 30 Oct 1996 23:13:04 +0100 (MET) Received: from franklin.seas.gwu.edu (franklin.seas.gwu.edu [128.164.9.2]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id XAA28323 for ; Wed, 30 Oct 1996 23:13:02 +0100 (MET) Received: from seas.gwu.edu (musgrave@felix.seas.gwu.edu [128.164.9.3]) by franklin.seas.gwu.edu (8.7.1/8.7.1) with ESMTP id RAA10591 for ; Wed, 30 Oct 1996 17:13:01 -0500 (EST) Received: (from musgrave@localhost) by seas.gwu.edu (8.7.1/8.7.1) id RAA10053 for globillum@imag.fr; Wed, 30 Oct 1996 17:12:57 -0500 (EST) Date: Wed, 30 Oct 1996 17:12:57 -0500 (EST) From: Ken Musgrave Message-Id: <199610302212.RAA10053@seas.gwu.edu> To: globillum@imag.fr Subject: Re: What's wrong w/ Monte-Carlo methods? X-UIDL: 3bc40ca3c57639f2a3173665dc70f9ae X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit My two cent's worth on Monte Carlo vs. radiosity: The former stands up to a shave with Occam's razor substantially better. It took years for Mandelbrot to pound a full appreciation of elegance into my thick head. -Ken From Received: from horus.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id NAA06149; Thu, 31 Oct 1996 13:51:48 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by horus.imag.fr (8.8.1/8.6.9) with ESMTP id NAA29859 for ; Thu, 31 Oct 1996 13:05:38 +0100 (MET) Received: from gate.mental.com (GATE.MENTAL.COM [192.31.14.2]) by imag.imag.fr (8.8.1/8.6.9) with SMTP id NAA00385 for ; Thu, 31 Oct 1996 13:05:34 +0100 (MET) Received: (from smap@localhost) by gate.mental.com (8.6.12/Lobo-960523) id NAA21095; Thu, 31 Oct 1996 13:05:22 +0100 Received: from twen(172.16.0.5) by gate via smap (V1.3) id sma021093; Thu Oct 31 13:05:15 1996 Received: (from henrik@localhost) by mental.com (8.6.12/Lobo-960725) id NAA09763; Thu, 31 Oct 1996 13:07:25 +0100 From: Henrik Wann Jensen Message-Id: <199610311207.NAA09763@mental.com> Subject: Re: What's wrong w/ Monte-Carlo methods? To: Holly Rushmeier Date: Thu, 31 Oct 1996 13:07:24 +0100 (MET) Cc: globillum@imag.fr In-Reply-To: <852563D3:0057ED7B.00@watngi01.watson.ibm.com> from "Holly Rushmeier" at Oct 30, 96 11:11:38 am X-Mailer: ELM [version 2.4 PL22] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: 0fc8230e0b792ebf4b9743a6ae77e25b X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Thus spoke Holly Rushmeier: > Using his methodology, and taking into account the dynamic range > of the global illumination problem, assuming simple minded > tone mapping, allowing an error of +/- 10 in > final pixel value (out of 0-255) and a requiring an 80% confidence > level gives a minimum sampling rate of 16094 (see Rushmeier & Ward, > "Energy Preserving Non-Linear Filters", Siggraph 94, pp 131 - 138) > > The above paper also brings up the notion, that rather than use a > biased algorithm, you can compute a result with an unbiased algorithm, and > then filter the results for consistency based on the values and error > estimates that you get. You can also filter an image generated by a consistent Monte Carlo renderer and obtain "good quality" much faster. I seem to remember that the "Energy Preserving Non-Linear Filters" paper also presented a technique for filtering images generated by Radiance (= a consistent but biased MC renderer). - Henrik From Received: from horus.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id XAA08212; Thu, 31 Oct 1996 23:10:56 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by horus.imag.fr (8.8.1/8.6.9) with ESMTP id WAA06400 for ; Thu, 31 Oct 1996 22:58:29 +0100 (MET) Received: from franklin.seas.gwu.edu (franklin.seas.gwu.edu [128.164.9.2]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id WAA28763 for ; Thu, 31 Oct 1996 22:58:27 +0100 (MET) Received: from seas.gwu.edu (musgrave@felix.seas.gwu.edu [128.164.9.3]) by franklin.seas.gwu.edu (8.7.1/8.7.1) with ESMTP id QAA04706 for ; Thu, 31 Oct 1996 16:58:26 -0500 (EST) Received: (from musgrave@localhost) by seas.gwu.edu (8.7.1/8.7.1) id QAA04839 for globillum@imag.fr; Thu, 31 Oct 1996 16:58:21 -0500 (EST) Date: Thu, 31 Oct 1996 16:58:21 -0500 (EST) From: Ken Musgrave Message-Id: <199610312158.QAA04839@seas.gwu.edu> To: globillum@imag.fr Subject: Re: What's wrong w/ Monte-Carlo methods? X-UIDL: e7bebe82f037ab4cece462cc28ba8df8 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit |From: Eric Veach |Date: Tue, 29 Oct 1996 17:58:01 -0800 (PST) | |This obviously doesn't make any sense for a fractal surface. The |area of the surface within a sphere of radius "r" is much larger |than Pi * r^2 (for a true fractal, the area would be infinite, Not to mention the fact that there would exist no surface normal anywhere for such a fractal, and that therefore light can only be propagated via diffraction. ;-) Mo Fractal From Received: from horus.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id LAA09432; Fri, 1 Nov 1996 11:57:42 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by horus.imag.fr (8.8.1/8.6.9) with ESMTP id LAA08159 for ; Fri, 1 Nov 1996 11:44:16 +0100 (MET) Received: from gate.mental.com (GATE.MENTAL.COM [192.31.14.2]) by imag.imag.fr (8.8.1/8.6.9) with SMTP id LAA23111 for ; Fri, 1 Nov 1996 11:44:14 +0100 (MET) Received: (from smap@localhost) by gate.mental.com (8.6.12/Lobo-960523) id LAA22379; Fri, 1 Nov 1996 11:44:02 +0100 Received: from twen(172.16.0.5) by gate via smap (V1.3) id sma022377; Fri Nov 1 11:43:53 1996 Received: (from henrik@localhost) by mental.com (8.6.12/Lobo-960725) id LAA03380; Fri, 1 Nov 1996 11:46:08 +0100 From: Henrik Wann Jensen Message-Id: <199611011046.LAA03380@mental.com> Subject: Re: What's wrong w/ Monte-Carlo methods? To: ericv@cs.stanford.edu Date: Fri, 1 Nov 1996 11:46:08 +0100 (MET) Cc: globillum@imag.fr X-Mailer: ELM [version 2.4 PL22] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: 5db65a6ce82ac03e934e992b746ebac5 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Thus spoke Eric Veach > This obviously doesn't make any sense for a fractal surface. The > area of the surface within a sphere of radius "r" is much larger > than Pi * r^2 (for a true fractal, the area would be infinite, The formula actually uses the *projected area* which is well-defined even for a fractal surface. And we do not need the normal if the reflection model for the fractal is Lambertian :) - Henrik From Received: from horus.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id AAA23820; Tue, 12 Nov 1996 00:37:44 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by horus.imag.fr (8.8.1/8.6.9) with ESMTP id AAA02244 for ; Tue, 12 Nov 1996 00:14:15 +0100 (MET) Received: from zappa.cs.uncc.edu (zappa.cs.uncc.edu [152.15.35.2]) by imag.imag.fr (8.8.1/8.6.9) with SMTP id AAA17338 for ; Tue, 12 Nov 1996 00:14:14 +0100 (MET) Received: from strauss.cs.uncc.edu by zappa.cs.uncc.edu (5.x/SMI-SVR4) id AA02337; Mon, 11 Nov 1996 18:12:51 -0500 Received: by strauss.cs.uncc.edu (5.x/SMI-SVR4) id AA04108; Mon, 11 Nov 1996 18:13:57 -0500 Message-Id: <9611112313.AA04108@strauss.cs.uncc.edu> From: "K. R." Date: Mon, 11 Nov 1996 18:13:57 GMT+447 X-Mailer: Mail User's Shell (7.1.1 5/02/90) To: globillum@imag.fr Subject: Foley,Van Dam - diffuse reflection.. X-UIDL: f3231111052ebf52d0084600ef6d4c09 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit I wonder if any of you have read carefully through Foley Van Dam's explanation of diffuse reflection. The explanation is either misleading or incorrect. Lambert's law is claimed to be related to the viewer location/angle.. I quote, "...Second, we must consider the amount of light seen by the viewer. Lambertian surfaces have the property, often known as Lambert's law, that the amount of light reflected from a unit differential area dA towards the viewer is directly proportional to the cosine of the angle between the direction of viewer and N..." They go on to use this to explain how the intensity is constant in all directions. However, on the one hand the angle theta is between the normal and the light vector, while the second angle is between the viewer and N. These are certainly not the same. -- krs -- K.R.Subramanian Phone: (704) 547-4872 Department of Computer Science FAX: (704) 547-3516 UNC Charlotte email: krs@zappa.cs.uncc.edu Charlotte, NC 28223-0001 WWW: http://www.cs.uncc.edu/~krs From Received: from horus.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id RAA28537; Tue, 12 Nov 1996 17:39:55 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by horus.imag.fr (8.8.1/8.6.9) with ESMTP id OAA10793 for ; Tue, 12 Nov 1996 14:57:20 +0100 (MET) Received: from ibis.doc.ic.ac.uk (ibis.doc.ic.ac.uk [146.169.12.90]) by imag.imag.fr (8.8.1/8.6.9) with SMTP id OAA21906 for ; Tue, 12 Nov 1996 14:56:39 +0100 (MET) Received: by ibis.doc.ic.ac.uk (Smail3.1.28.1 #8) id m0vNJF9-0002ndC; Tue, 12 Nov 96 13:51 GMT Message-Id: Date: Tue, 12 Nov 96 13:51 GMT From: Adrian James Chung To: globillum@imag.fr Subject: The case for FEM X-UIDL: f618bbfa94cfe33d15e42b2c1a9d6b4a X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit I guess the "What's wrong w/ Monte-Carlo methods?" thread has died. Pity. I was quite enjoying it as it reflected the "state of the art" in Global Illum more than any paper would have IMHO. I'd like to give my 2p if it's not too late: ** On scene complexity: Pete Shirley: > In summary, pure MCPT has only two advantages-- it is so dumb > that it doesn't get hit by big scenes, and it is easy to implement. [...] > radiosity (I use that term for all world space > irradiance calculating alg's), and that limits you to > a relatively small scene (100k initial polygons will kill > almost all radiosity implementations) This just illustrates the time/space trade-off in global illumination. Naive MCPT is so "dumb" it keeps throwing away intermediate results that could come in handy when the next path gets traced. I know there are some intersection acceleration techniques to exploit path coherency but very few exploit coherency in the radiance function (for instance, irradiance caching in RADIANCE). Stephen Westin: > Why do folks bother at all with Monte Carlo methods for global > illumination? Complexity. [...] > Do you want to go around the whole environment, calculating the > irradiance from every object, regardless of occlusion or distance from > the point? Which is the motivation for importance (or Pattanaik's potential) based FE techniques. > Hierarchical meshing is basically a way to make a mesh-based algorithm > behave more like Monte Carlo, spending effort for irradiance > contributions rather than for geometric complexity. (...) > The ultimate global illumination method will probably be a > hybrid of Monte Carlo and mesh-based methods It's a pity that intrisically MCPT is not really hierarchical. It may use a hierarchical data structure for every intersection but it is essentially a point sampling method. In Fast Multipole Methods the physical characteristics stored at each interior node serves as a course representation of that stored by the descendant nodes in the heirarchy thus interactions can be computed without descending all the way to the leaves. As all point samples in MCPT are independent they must all descend to the leaves of the data structure to determine on an individual basis how each gets reflected. Unanswered questions: Should we, and how do we, make MCPT more like FMM? Or should Hierarchical FE be made more like MCPT? In short, what form should this hybrid take? Eric Veach: > But flat polygons and diffuse reflectors do not go very far in > modeling the real world, and finite-element algorithms don't seem to > be practical for much more than this. And in a later email: > The point is that you can't judge the whole class of unbiased > algorithms based on a couple of examples. Same applies to finite element methods. This thread has been judging the relative merits of MCPT and FE on the basis of what can currently be done practically. I say we also need to look at their potential for future improvements. We criticise FE's inability to deal with gloss based upon methods that apply meshing to 2D surfaces. But the global plenoptic function is 5-dimensional and have there been any attempts at discretizing this space? (Drettakis et al.'s visibility complex is a start...) > I would like to see more results on what can and > cannot be achieved by unbiased methods, so that we can make > better decisions on these issues. ...as well as for FE and true hierarchical methods. IMO visibilty has been handled poorly in FE radiosity, often reducing to a MonteCarlo approach of casting rays between patches and/or clusters. Is there a robust algorithm that reliably implements the triage concept (i.e. doesn't say two patches are fully occluded simply because the 16 rays cast between them so happened to hit the cloud of intervening occluders). > To me, the amazing thing is that radiosity algorithms need to be so > *complicated* to be efficient. I get this same feeling for MCPT. We now have irradiance caching, a variety of intersection acceleration methods, special cases for direct illumination, luminaire classification schemes based on significance, caustic and photon-mapping pre-passes, special closed form analytical BRDFs, "imposter" substitution for indirect luminaires (or whatever the correct term for it is...), etc. Of course, once you've implemented all these you'd be able to handle a much wider domain of problems than current FE methods, but I bet you'll still miss your deadline. ** On memory management and parallelism Pete: > Most algorithms are memory hogs and don't parallelize. This enters into the field of operating systems. My opinion is that most OS designs have been based on applications of the 70's and before. Back then there was little use of dynamic data structures. It would be a mistake to design a globillum application to fit into this framework. Things are improving with new research into microkernels which can allow one to specify user defined virtual memory systems specially taylored for the demands of particular algorithms. On the parallelism front computational scientists are increasingly moving toward adaptive irregular computations (a behaviour so common in MCPT and HR) necessitating runtime support for multi-threading and asynchronous control. My belief is that most MCPT and FE radiosity methods can be expressed in a multithreaded asynchronous style to make use of these innovations. ** Grand Challenge models Pete: > I think we need to make our own "grand challenge" models, and publicize > that they can't currently be done (e.g, a human at a desk illuminated > through a skylight), so that our field wont dry up and blow away. A Great Idea! Eric Veach: > The real test of generality is how an algorithm performs when there are > *no* diffuse surfaces, since that's how it is in the real world. Additionally: (i) when 90% of the scene is outside the viewing frustum but may still influence the illumination of the visible geometry. How would the photon map perform on a 5 story architecture where the janitor has left the light on inside a closed closet? How does MCPT perform on the nested labyrinth models used by Smits (SigGraph 1992)? This and Eric Veach's comment below makes the case for importance estimation which can be done by FE also: > In effect, Monte Carlo algorithms can sample the scene to > determine the information they actually need, while deterministic > algorithms examine every detail, whether it is relevant or not. (ii) when feature sizes vary over several orders of magnitude (such as fractals). A pathological case would be to render a scene of a pile of sand where part of the view is through a powerful magnifying glass. Contrived though it is, it illustrates where a sort of multi-resolution BRDF would come in handy so that samples passing through the magnifying glass make use of the detailed BRDF of the sand particles, whereas indirect illumination reflecting off the entire pile uses the courser BRDF representation. Has there been any research into generating a multi-resolution BRDF like this automatically? The current technique is to use imposters but this requires user intervention. This would help handle this model: Eric: > Ideally, rendering algorithms should not depend on the details of > the scene representation, but only on the underlying mathematical > model. For example, a square area light source can be simulated > fairly well with a ten by ten array of point sources (...) > Similarly, if we replace the square light source by two flourescent > bulbs covered by a diffusely transmitting panel, (...) The same > comments apply to geometric complexity: if we represent an indoor > plant as a thousand polygons or a million Bezier patches, how much > should the rendering time go up? These will make great Grand Challenge problems! Someone should catalogue pathological cases with explanations why each of the currently available techniques perform poorly. Henrik Wann Jensen: > Consider for example a glass of cognac on a procedural surface :) Eric Veach: > Let's consider the handle on my coffee > mug. (...) this implies a density of about ten million photon > hits per square meter. We can make this another Grand Challenge problem. Picture a messy kitchen with daylight incident on a sink full of turbid water reflecting caustics onto Eric's mug. (Do you have a NURBS description of that?) Henrik on the photon map & fractal surfaces: > The formula actually uses the *projected area* which is well-defined > even for a fractal surface. And we do not need the normal if the > reflection model for the fractal is Lambertian :) I'm confused. Does the formula apply if the fractal surface self occludes? What about fractally defined aggregate surfaces (e.g. a ball of cotton) ** On bias vs. variance (noise) > For algorithms which are merely consistent, however, we must also > bound the bias. (...) Bias shows up as results that are not noisy, > but in fact are incorrect. In graphics algorithms, this error is > often noticeable visually, in the form of discontinuities, excessive > blurring, or surface shading that just looks wrong. Not necessarily bound it but *blend* it between visually coherent regions such that the bias is not noticeable. I know the scientifically correct way would be to bound bias, but if the end product is an aesthetic image rather than actual luminance statistics, you can probably produce something acceptable by removing unnecessary variation via judicious use of interpolation. This amounts to filtering over the finite elements of course. > Finite element methods also have advantages, I just didn't mention > them. I didn't mean to write this much... Just that no one else was speaking up for FE. Please feel free to rebut since I'm about to invest a massive amount of time implementing a hairy hierarchical global illumination multigridded FE method with importance sampling etc. :-) Adrian -- Oh and since no one has answered this at time of writing... K. R. wrote: > I wonder if any of you have read carefully through Foley > Van Dam's explanation of diffuse reflection. The explanation is > either misleading or incorrect. Lambert's law is claimed to be > related to the viewer location/angle.. I quote, > > "... that the amount of light reflected from a unit differential > area dA towards the viewer is directly proportional to the cosine of > the angle between the direction of viewer and N..." Depends on what is meant by "amount of light". If referring to energy or power directed towards the viewer then this is correct. Since radiance is constant over the hemisphere the "amount of light" will depend on area projected by the unit differential area towards the viewer which will indeed be proportional to the cosine of the angle between N and view direction.(A simple check: if N is at right angles to your view, the differential area is a silhouette, projects zero area on the image, hence cannot be seen) In practice this calculation is taken care of by the perspective/orthographic projection or by sampling in the image domain. Most implementations take the cosine of the angle between N and a light source direction in order to estimate how much light energy was being intercepted by the surface in the first place to determine what constant value the radiance will take. It is misleading in that the terminology isn't quite clear. (Did that make any sense or did I just make a fool of myself?) From Received: from horus.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id UAA29491; Tue, 12 Nov 1996 20:37:56 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by horus.imag.fr (8.8.1/8.6.9) with ESMTP id TAA16534 for ; Tue, 12 Nov 1996 19:54:19 +0100 (MET) Received: from gateway.lightscape.com (gate-gateway.lightscape.com [206.139.79.2]) by imag.imag.fr (8.8.1/8.6.9) with SMTP id TAA10229 for ; Tue, 12 Nov 1996 19:54:15 +0100 (MET) Received: from topo.lightscape.com by gateway.lightscape.com via ESMTP (950511.SGI.8.6.12.PATCH526/940406.SGI.AUTO) for <@gateway.lightscape.com:globillum@imag.fr> id KAA14119; Tue, 12 Nov 1996 10:53:42 -0800 Received: from basil.lightscape.com by topo.lightscape.com via ESMTP (940816.SGI.8.6.9/940406.SGI.AUTO) for <@topo.lightscape.com:globillum@imag.fr> id KAA09119; Tue, 12 Nov 1996 10:53:41 -0800 Received: from basil by basil.lightscape.com via SMTP (940816.SGI.8.6.9/940406.SGI.AUTO) for id KAA02833; Tue, 12 Nov 1996 10:53:39 -0800 Sender: greg@lightscape.com Message-ID: <3288C7B2.1CFB@lightscape.com> Date: Tue, 12 Nov 1996 10:53:38 -0800 From: Greg Spencer Organization: Lightscape Technologies, Inc. http://www.lightscape.com X-Mailer: Mozilla 3.0Gold (X11; U; IRIX 5.3 IP22) MIME-Version: 1.0 To: globillum@imag.fr Subject: Lens Calibration summary Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: 93a892bf3202c5296ae8d742f6d9c1f9 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 I got so caught up in the FE vs. MCPT thread, I forgot to post the summary of lens calibration responses that I got. I got several possibilities, and even found that elusive "company" in europe that I had heard abnout. It turns out that the "company" is actually a photogrammetry department at University College London, and they will measure lenses for a fee of 522.50 pounds (see attached message for address, etc.). Michael Cohen reports that Tsai's method is satisfactory for most uses as long as you can get the images scanned in reliably. The drawbacks I see are that Tsai's method only models radial distortion, and doesn't handle any chromatic or intensity issues. I also found a piece of Macintosh photogrammetry software that will take an image which contains their calibration target and provide you with radial distortion and other information about the camera system. It is designed for CCDs, but reportedly could be used for any camera system where the scanning of the image was consistent. The name of the software is "Opti-CAL", and the contact for information is gchow@kinetic.bc.ca. If anyone is interested, I have a technical summary that they sent me on the product. Ken Musgrave's friend (who is a lens designer) suggested that if one wishes to model the optics directly to determine a mapping (as in Craig Kolb's SIGGRAPH paper), lens patent descriptions may be used to find out information on the configurations of the lenses. -Greg. -- Greg Spencer, Software Engineer greg@lightscape.com Lightscape Technologies., Inc. (408) 342-1900 http://www.lightscape.com (PGP key available upon request) ---------------------------------snip-------------------------------- Subject: Re: Lens measurement? From: Leoni Blank We do have a service for calibrating cameras in our dept. (Department of Photogrammetry and Surveying, UCL). We normally deal with photogrammetric metric cameras, but can also measure semi and non metric cameras. We calibrate for lens distortion, principle distance, and principle point position. However we do not consider chromatic abberation or intensity falloff. We do charge for this service, if you send the camera to us then we will carry out the calibration and issue a certificate for 522.50 pounds. If you want any details then please email me, and let me know what kind of camera you have. Leoni Blank Department of Photogrammetry and Surveying UCL Gower Street London WC1E 6BT From Received: from horus.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id XAA29959; Tue, 12 Nov 1996 23:14:36 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by horus.imag.fr (8.8.1/8.6.9) with ESMTP id WAA17465 for ; Tue, 12 Nov 1996 22:54:59 +0100 (MET) Received: from HOSTESS.GRAPHICS.CS.CMU.EDU (HOSTESS.GRAPHICS.CS.CMU.EDU [128.2.206.188]) by imag.imag.fr (8.8.1/8.6.9) with SMTP id WAA17301 for ; Tue, 12 Nov 1996 22:54:56 +0100 (MET) From: Paul.Heckbert@HOSTESS.GRAPHICS.CS.CMU.EDU Message-Id: <199611122154.WAA17301@imag.imag.fr> Date: Tue, 12 Nov 96 16:46:37 EST To: globillum@imag.fr Subject: Re: Foley,Van Dam - diffuse reflection.. X-UIDL: 475573b170f2188c2b141a6acbe32ac1 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit I hadn't noticed that one, but if we're collecting weaknesses of that book, I've been quite disappointed by their discussion of gamma correction. In my undergrad graphics class (see my web page), I always tell my students to skip the gamma correction section of Foley et al's book and to read Blinn's column on that topic instead: James F. Blinn Dirty Pixels IEEE Computer Graphics & Applications July 1989 pp. 100-105 By the way, somebody should collect up these comments on Foley's book and forward them to Foley et al. Paul Heckbert Computer Science Dept., Carnegie Mellon University 5000 Forbes Ave, Pittsburgh PA 15213-3891, USA ph@cs.cmu.edu http://www.cs.cmu.edu/~ph From Received: from horus.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id AAA05813; Thu, 14 Nov 1996 00:53:07 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by horus.imag.fr (8.8.1/8.6.9) with ESMTP id AAA05569 for ; Thu, 14 Nov 1996 00:27:56 +0100 (MET) Received: from june.cs.washington.edu (june.cs.washington.edu [128.95.1.4]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id AAA27769 for ; Thu, 14 Nov 1996 00:27:54 +0100 (MET) Received: (jfh@localhost) by june.cs.washington.edu (8.7.6/7.2ju) id PAA03722; Wed, 13 Nov 1996 15:27:46 -0800 From: John Hughes Message-Id: <199611132327.PAA03722@june.cs.washington.edu> Subject: [krs@strauss.cs.uncc.edu: Foley,Van Dam - diffuse reflection..] (fwd) To: globillum@imag.fr Date: Wed, 13 Nov 1996 15:27:45 -0800 (PST) Cc: avd@cs.brown.edu, foley@merl.com, feiner@cs.columbia.edu X-Mailer: ELM [version 2.4 PL23] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: e042444d6a4a0e8e8535a36d22e9d08f X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 David Salesin was kind enough to forward the following message to me, and I figured that I'd try to address it. First of all, let me admit that our book has many errors, all of which we try to track in our "Bug List," which is available by sending mail to graphtext@cs.brown.edu. But I believe that the "error" below is one of the (many?) places where we actually got it right. > "...Second, we must consider the amount of light seen by the viewer. Lambertian > surfaces have the property, often known as Lambert's law, that the amount > of light reflected from a unit differential area dA towards the viewer is > directly proportional to the cosine of the angle between the direction of > viewer and N..." I believe that the statement above is correct; but you need to note that it says that the amount reflected *from a unit differential area* is proportional to the cosine of the *view-to-normal* angle. But a single bit of your eye (one receptor, for example) will actually see more or less surface depending on the viewing angle. That's what the next sentence says: "...Since the amount of surface area seen is inversely proportional to the cosine of this angle, these two factors cancel out." The phrase "this angle" has antecedent "the angle between the direction to the viewer and N", and "two factors" has antecedents "directly proportional to the cosine of ..." and "inversely proportional to the cosine of...". > They go on to use this to explain how the intensity is constant in all > directions. However, on the one hand the angle theta is between the > normal and the light vector, while the second angle is between the viewer > and N. These are certainly not the same. The symbol theta is only used to denote the angle between the direction to the light source and the normal. The direction-to-viewer/normal angle is not given a symbol anywhere in the discussion, but is simply described as it is used, two times (which happen to cancel out). * * * Paul Heckbert also commented on Gamma Correction. There, too, I think that the explanation is correct, although I personally am not in love with the presentation of the material -- if we were to do it over again, and I had a chance to rewrite *that* bit, I'd be inclined to do it differently. Anyhow, I feel sure that I speak for my coauthors as well when I say that we really *are* sorry about the errors in the text, and hope that the stuff that's right makes up for it. Some of the errors come directly from the source material (I won't say here whose papers had incorrect descriptions of the work which was only fixed in subsequent papers, but such errors do abound), others are our fault alone. It's also interesting to see one's own errors propagated to other texts, whose authors apparently didn't bother to read the original papers themselves. It's annoying, however, to see whole chunks of one's (correct) prose copied verbatim to other texts without attribution :-(. -John Hughes From Received: from horus.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id XAA13831; Thu, 14 Nov 1996 23:28:20 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by horus.imag.fr (8.8.1/8.6.9) with ESMTP id WAA18910 for ; Thu, 14 Nov 1996 22:57:23 +0100 (MET) Received: from igw3.watson.ibm.com (igw3.watson.ibm.com [129.34.139.18]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id WAA27431 for ; Thu, 14 Nov 1996 22:57:21 +0100 (MET) Received: from mailhub1.watson.ibm.com (mailhub1.watson.ibm.com [9.2.249.31]) by igw3.watson.ibm.com (8.7.6/8.7.1) with ESMTP id QAA14060 for ; Thu, 14 Nov 1996 16:57:37 -0500 Received: from watngi01.watson.ibm.com (watngi01.watson.ibm.com [9.2.235.20]) by mailhub1.watson.ibm.com (8.8.2/11-10-96) with SMTP id QAA644769 for ; Thu, 14 Nov 1996 16:57:19 -0500 Received: by watngi01.watson.ibm.com(Lotus SMTP MTA Release 1.0.1) id 852563E2.0078988E ; Thu, 14 Nov 1996 16:57:13 -0400 X-Lotus-FromDomain: IBM RESEARCH From: "Holly Rushmeier" To: globillum@imag.fr Message-ID: <852563E2:0077FFC6.00@watngi01.watson.ibm.com> Date: Thu, 14 Nov 1996 16:56:33 -0400 Subject: ACM TOG Mime-Version: 1.0 Content-type: text/plain; charset=us-ascii; format=flowed X-UIDL: 98ddf4b82dcecb4fac13074bde53af57 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hi -- I don't know if you have noticed, but over the past year TOG (Transactions on Graphics) has had a number of papers of interest to globillumers, e.g. in the Jan. 1996 issue there were: " Monte Carlo Techniques for Direct Lighting Calculations" , by Peter Shirley, Chang Yaw Wang, and Kurt Zimmerman and "Global Illumination of Glossy Environments Using Wavelets and Importance" by Per H. Christensen, Eric J. Stollnitz, David H. Salesin, and Tony D. DeRose The Oct. 1996 issue also has some papers you may be interested in, such as: "Image Shading Taking into Account Relativistic Effects" "Quadrature Prefiltering for High Quality Antialiasing" "Computing the Discrepancy with Applications to Supersampling Patterns", and for a limited time you can download the **full text** of these articles in PDF format from the TOG web page at: http://www.acm.org/tog/Current.html -- Holly From Received: from horus.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id RAA09862; Mon, 18 Nov 1996 17:38:48 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by horus.imag.fr (8.8.1/8.6.9) with ESMTP id QAA22314 for ; Mon, 18 Nov 1996 16:52:12 +0100 (MET) Received: from franklin.seas.gwu.edu (franklin.seas.gwu.edu [128.164.9.2]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id QAA07445 for ; Mon, 18 Nov 1996 16:52:08 +0100 (MET) Received: from seas.gwu.edu (musgrave@felix.seas.gwu.edu [128.164.9.3]) by franklin.seas.gwu.edu (8.7.1/8.7.1) with ESMTP id KAA21809 for ; Mon, 18 Nov 1996 10:52:05 -0500 (EST) Received: (from musgrave@localhost) by seas.gwu.edu (8.7.1/8.7.1) id KAA23115 for globillum@imag.fr; Mon, 18 Nov 1996 10:52:01 -0500 (EST) Date: Mon, 18 Nov 1996 10:52:01 -0500 (EST) From: Ken Musgrave Message-Id: <199611181552.KAA23115@seas.gwu.edu> To: globillum@imag.fr Subject: Can anyone help this person? X-UIDL: 03250da8b00d7cf890d33e97fbfbd8bf X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit This is an interesting and tough problem. I recall speaking to some researchers at Sandia and/or Los Alamos who were working on exactly this, But fo r the life of me, I can't remember whom. Any inputs? -Ken >>From raja4@iris1.cz3.nus.sg Mon Nov 18 06:40 EST 1996 From: Raja s/o Vengadasalam To: musgrave@seas.gwu.edu Subject: Re: Computation of Scattering Point Spread Functions due to Atmospheric Aerosols in Optical Satellite Remote Sensing of Earth Surface Dear Sir, a good day to you . Under my course in Computational physics, i have been assigned the above. I have been asked to compute the scattering PSF assuming a certain aerosol model characterised by i) scattering albedo ii) scattering extinction coefficient iii) scattering phase function using radiative transfer methods or Monte Carlo methods or radiosity methods. I am also to investigate how PSF is dependent on the particular aerosel and geometry of image acquisition. Deconvolution of a SPOT satellite image is also to be attempted from the computed PSF. I am baffled as to how to derive a single scattering PSF and generate successive orders of scattering PSF to account for multiple scattering. 1. I have a pattern on the ground defining my spatially varied reflectance R(x,y) 2. I have a line from my sensor to the ground. 3. I have choose a point on this line 4. I draw a line from some point (x',y') to the point chosen on the line from the sensor to the ground. 5. I calculate the phase angle of radiation traveling from (x',y') to the point chosen on the line from the sensor to the ground, and being scattered into the sensor. 6. Integrate over all (x',y') 7. Integrate over all possible points on the line from the sensor to the ground. 8. My result should look like a convolution. I would think the approach to take would be to use a Monte Carlo code. Create a model atmosphere which contains an aerosol layer at some altitude above the surface. Draw an optical ray into the aerosol layer and let it randomly scatter one time, according to statistics determined by the aerosol phase function, and extend the scattered ray to the earth's surface. You do this many times and you have a blurry spot on the ground which is the aerosol point spread function for single scattering. Take a single point on the ground and trace a ray back up through the aerosol layer, I think I will get the same pattern (as a function of angle). A round-trip through the aerosol layer is probably equivalent to a convolution of the single-scatter PSF. We could approximate the effect of multiple scattering by successive convolutions, but it is not too difficult to allow multiple scatterings of the rays within the aerosol layer. We might also consider double-bounce reflections between the aerosol layer and the surface. I have difficulty finding suitable programs compatible in Unix platforms for any of the above methods. I would be obliged if you can mail me any computational codes that can generate PSF's using any of the above methods, if you know of any. Thanks raja e-mail address: sci30380@leonis.nus.sg raja4@cz3.nus.sg ---1987817213-15594127-844913622=:17493-- From Received: from horus.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id TAA10289; Mon, 18 Nov 1996 19:38:27 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by horus.imag.fr (8.8.1/8.6.9) with ESMTP id TAA24623 for ; Mon, 18 Nov 1996 19:04:47 +0100 (MET) Received: from igw3.watson.ibm.com (igw3.watson.ibm.com [129.34.139.18]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id TAA16012 for ; Mon, 18 Nov 1996 19:04:44 +0100 (MET) Received: from mailhub1.watson.ibm.com (mailhub1.watson.ibm.com [9.2.249.31]) by igw3.watson.ibm.com (8.7.6/8.7.1) with ESMTP id NAA15144; Mon, 18 Nov 1996 13:04:59 -0500 Received: from watngi01.watson.ibm.com (watngi01.watson.ibm.com [9.2.235.20]) by mailhub1.watson.ibm.com (8.8.2/11-10-96) with SMTP id NAA587622; Mon, 18 Nov 1996 13:04:39 -0500 Received: by watngi01.watson.ibm.com(Lotus SMTP MTA Release 1.0.1) id 852563E6.00634BCD ; Mon, 18 Nov 1996 13:04:34 -0400 X-Lotus-FromDomain: IBM RESEARCH From: "Holly Rushmeier" To: musgrave@seas.gwu.edu cc: globillum@imag.fr Message-ID: <852563E6:00630451.00@watngi01.watson.ibm.com> Date: Mon, 18 Nov 1996 13:03:43 -0400 Subject: Re: Can anyone help this person? Mime-Version: 1.0 Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: 00eab3f4b73666ccbe41e5e90e1a4058 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit I have received two such messages from this person **after** providing what information I could. -- Holly To: globillum @ imag.fr cc: (bcc: Holly Rushmeier/Watson/IBM Research) From: musgrave @ seas.gwu.edu Date: 11/18/96 10:52:01 AM Subject: Can anyone help this person? This is an interesting and tough problem. I recall speaking to some researchers at Sandia and/or Los Alamos who were working on exactly this, But fo r the life of me, I can't remember whom. Any inputs? -Ken From raja4@iris1.cz3.nus.sg Mon Nov 18 06:40 EST 1996 From: Raja s/o Vengadasalam To: musgrave@seas.gwu.edu Subject: Re: Computation of Scattering Point Spread Functions due to Atmospheric Aerosols in Optical Satellite Remote Sensing of Earth Surface Dear Sir, .. (.... body of message deleted ...) Thanks raja e-mail address: sci30380@leonis.nus.sg raja4@cz3.nus.sg ---1987817213-15594127-844913622=:17493-- From Received: from horus.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id SAA28299; Thu, 21 Nov 1996 18:37:09 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by horus.imag.fr (8.8.1/8.6.9) with ESMTP id RAA10172 for ; Thu, 21 Nov 1996 17:25:43 +0100 (MET) Received: from phong.cs.utah.edu (phong.cs.utah.edu [128.110.4.52]) by imag.imag.fr (8.8.1/8.6.9) with SMTP id RAA21546 for ; Thu, 21 Nov 1996 17:25:32 +0100 (MET) Received: (from shirley@localhost) by phong.cs.utah.edu (950413.SGI.8.6.12/950213.SGI.AUTOCF) id JAA05978 for globillum@imag.fr; Thu, 21 Nov 1996 09:23:07 -0700 From: Peter Shirley Message-Id: <199611211623.JAA05978@phong.cs.utah.edu> Subject: reflection questions To: globillum@imag.fr Date: Thu, 21 Nov 1996 09:23:07 -0700 (MST) X-Mailer: ELM [version 2.4 PL23] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: c3bcda0396254538b0f1199630623f04 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hi all. I was recently pointed to the web page: http://www.erim.org/on-line-docs/GUIDE/guide.frm.html Which has a discussion of several BRDF models. It has several small errors, but also some very good information. I have two questions that arise from it I hope somebody can answer: 1. In Equation 8, the "glossy coating BRDF", there is a specular reflectance (surface term) and a subsurface term: rho0 [ 1-R(thetai) ] [ 1-R(thetar) ] / (PI n^2) where rho0 is the diffuse refectance of the substrate, thetai and thetar are angles to the normal, R is the surface (Fresnel) term, and n is the refractive index. This is very similar to a model I arrived at independently, so I want to track the source down. Anybody know where it is from? 2. A paper by [Rushmeier and Tynor, 90] is alluded to, with no title or bibliography entry. What is it (I have a feeling our friend HR can answer this one). Thanks Pete From Received: from horus.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id UAA28713; Thu, 21 Nov 1996 20:06:33 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by horus.imag.fr (8.8.1/8.6.9) with ESMTP id TAA12396 for ; Thu, 21 Nov 1996 19:42:42 +0100 (MET) Received: from mane.cgrg.ohio-state.edu (mane.cgrg.ohio-state.edu [128.146.18.78]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id TAA29245 for ; Thu, 21 Nov 1996 19:42:35 +0100 (MET) Received: from emily.cgrg.ohio-state.edu (spencer@emily.cgrg.ohio-state.edu) by mane.cgrg.ohio-state.edu (8.8.2/941010.52) with SMTP id NAA12316 for ; Thu, 21 Nov 1996 13:42:20 -0500 (EST) Date: Thu, 21 Nov 1996 13:42:19 -0500 (EST) From: "Stephen N. Spencer" To: globillum@imag.fr Subject: Re: reflection questions In-Reply-To: <199611211623.JAA05978@phong.cs.utah.edu> Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII; format=flowed X-UIDL: 521b2ddc9ff42a1be9822f055e3e173d X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit On Thu, 21 Nov 1996, Peter Shirley wrote: > 2. A paper by [Rushmeier and Tynor, 90] is alluded to, with > no title or bibliography entry. What is it (I have a feeling > our friend HR can answer this one). >>From the SIGGRAPH Computer Graphics Bibliography Database comes: @InProceedings{Rushmeier:1990:IBI, author = "Holly E. Rushmeier and Stephen D. Tynor", title = "Incorporating the {BRDF} Into an Infrared Scene Generation System", year = "1990", month = apr, volume = "1311", booktitle = "Conference on Characterization, Propagation and Simulation of Infrared Scenes, SPIE Proceedings", address = "Orlando, Florida", } Is this information correct, Holly, or does it need adjustment? Stephen N. Spencer 614.292.3416 (v) Graphics Research Specialist spencer@siggraph.org 614.292.7776 (f) ACCAD - The Ohio State University spencer@cgrg.ohio-state.edu SIGGRAPH Director for Publications spencer@acm.org "After ecstasy, laundry." - Zen writing From Received: from horus.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id AAA29294; Fri, 22 Nov 1996 00:24:53 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by horus.imag.fr (8.8.1/8.6.9) with ESMTP id AAA13337 for ; Fri, 22 Nov 1996 00:09:07 +0100 (MET) Received: from igw3.watson.ibm.com (igw3.watson.ibm.com [129.34.139.18]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id AAA08788 for ; Fri, 22 Nov 1996 00:09:05 +0100 (MET) Received: from mailhub1.watson.ibm.com (mailhub1.watson.ibm.com [9.2.249.31]) by igw3.watson.ibm.com (8.7.6/8.7.1) with ESMTP id SAA16198; Thu, 21 Nov 1996 18:09:13 -0500 Received: from watngi01.watson.ibm.com (watngi01.watson.ibm.com [9.2.235.20]) by mailhub1.watson.ibm.com (8.8.2/11-10-96) with SMTP id SAA642208; Thu, 21 Nov 1996 18:08:52 -0500 Received: by watngi01.watson.ibm.com(Lotus SMTP MTA Release 1.0.1) id 052563E9.007F24C9 ; Thu, 21 Nov 1996 18:08:44 -0400 X-Lotus-FromDomain: IBM RESEARCH From: "Holly Rushmeier" To: spencer@emily.cgrg.ohio-state.edu cc: globillum@imag.fr Message-ID: <852563E9:007DF50B.00@watngi01.watson.ibm.com> Date: Thu, 21 Nov 1996 18:07:47 -0400 Subject: Re: reflection questions Mime-Version: 1.0 Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: fe464cdd597ee838430d9d27c474d850 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit The bibliographic reference is correct, and what the paper describes is the implementation of the Sanford-Robertson model to one reflection from a surface for infrared signature generation (since the bulk of the signature is emission, one bounce is a fairly small percentage of the signature, and multiple bounces don't add much.) Anyway, the ERIM page Pete referred to http://www.erim.org/on-line-docs/GUIDE/guide.frm.html was prepared by Ken Ellis, who can probably answer questions about the source of the various equations. If the email on web page doesn't work, try ellis@aaec.com. I believe he works for Atlantic Aerospace. He has a recent paper on first principle reflectance modeling you might find interesting: "First-Principles Coatings Reflectance Model Validation" Ellis, Jones, Chu, and Lynn Sixth Annual Ground Target Modeling and Validation Conference, Houghton,MI, 22-24 Aug. 1995 If you have trouble finding the paper, you could email to one of the information addresses on the ERIM home page at http://www.erim.org/ -- Holly To: globillum @ imag.fr cc: (bcc: Holly Rushmeier/Watson/IBM Research) From: spencer @ emily.cgrg.ohio-state.edu Date: 11/21/96 01:42:19 PM Subject: Re: reflection questions On Thu, 21 Nov 1996, Peter Shirley wrote: > 2. A paper by [Rushmeier and Tynor, 90] is alluded to, with > no title or bibliography entry. What is it (I have a feeling > our friend HR can answer this one). From the SIGGRAPH Computer Graphics Bibliography Database comes: @InProceedings{Rushmeier:1990:IBI, author = "Holly E. Rushmeier and Stephen D. Tynor", title = "Incorporating the {BRDF} Into an Infrared Scene Generation System", year = "1990", month = apr, volume = "1311", booktitle = "Conference on Characterization, Propagation and Simulation of Infrared Scenes, SPIE Proceedings", address = "Orlando, Florida", } Is this information correct, Holly, or does it need adjustment? Stephen N. Spencer 614.292.3416 (v) Graphics Research Specialist spencer@siggraph.org 614.292.7776 (f) ACCAD - The Ohio State University spencer@cgrg.ohio-state.edu SIGGRAPH Director for Publications spencer@acm.org "After ecstasy, laundry." - Zen writing From Received: from horus.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id VAA04361; Fri, 22 Nov 1996 21:24:44 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by horus.imag.fr (8.8.1/8.6.9) with ESMTP id UAA01635 for ; Fri, 22 Nov 1996 20:53:30 +0100 (MET) Received: from anduin.ocf.llnl.gov (anduin.ocf.llnl.gov [134.9.49.1]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id UAA10424 for ; Fri, 22 Nov 1996 20:53:28 +0100 (MET) Received: from teapot.llnl.gov (nelson@teapot.llnl.gov [128.115.101.121]) by anduin.ocf.llnl.gov (8.7.5/8.7.3/LLNL-Jun96) with SMTP id LAA08933 for <@anduin.ocf.llnl.gov:globillum@imag.fr>; Fri, 22 Nov 1996 11:53:24 -0800 (PST) Received: by teapot.llnl.gov (951211.SGI.8.6.12.PATCH1042/951211.SGI.AUTO) for globillum@imag.fr id LAA29699; Fri, 22 Nov 1996 11:53:41 -0800 From: "Nelson L. Max" Message-Id: <9611221153.ZM29697@teapot.llnl.gov> Date: Fri, 22 Nov 1996 11:53:37 -0800 Reply-to: max2@llnl.gov X-Mailer: Z-Mail (3.2.0 26oct94 MediaMail) To: globillum@imag.fr Subject: Cloud shading Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed X-UIDL: 88c82a632d11afe33ee0baf8361014ac X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit I was just looking out my window at some beautiful clouds, and I think I have finally figured out why their edges are dark! The clouds were lit by the sun from the upper right, at 90 degrees to my viewing direction, but their right hand and upper edges still looked dark when viewed against more distant clouds of the same white color. If each water droplet scattered or absorbed the same amount of light in all directions, the color would depend only on the integrated density of droplets along a viewing ray (column density), and not on their density distribution along the ray. If anything, one would expect the sunlit droplets at the edge of a cloud to scatter more light than those inside. The answer is that they probably do, but at the tenuous edge of the cloud, the probability of multiple scattering is lower, so that the highly forward scattering in the water droplets does not undergo enough multiple scattering for its direction to be randomized. Looking from the side, I saw less than my share of this forward scattered light, although the extinction (absorption) of these edge droplets still attenuated the light from behind according to their column density. When the sun is directly behind a cloud, the edges look much brighter, due to the forward scattering, so everything balances out. -- Nelson Max http://www.llnl.gov/graphics max2@llnl.gov Lawrence Livermore National Laboratory (510) 422-4074 7000 East Avenue fax (510) 423-8704 Livermore, CA 94550, USA From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id RAA25218; Wed, 27 Nov 1996 17:31:11 +0100 Received: from cs.brown.edu (cs.brown.edu [128.148.128.2]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id QAA16512 for ; Wed, 27 Nov 1996 16:33:56 +0100 (MET) Received: from power.cs.brown.edu (power.cs.brown.edu [128.148.38.29]) by cs.brown.edu (8.8.3/8.7.1) with ESMTP id KAA19545; Wed, 27 Nov 1996 10:33:02 -0500 (EST) Received: from power (localhost [127.0.0.1]) by power.cs.brown.edu (8.8.3/BrownCS1.0) with SMTP id KAA15725; Wed, 27 Nov 1996 10:33:03 -0500 (EST) Sender: avd@cs.brown.edu Message-ID: <329C5F2F.51E6@cs.brown.edu> Date: Wed, 27 Nov 1996 10:33:03 -0500 From: Andy van Dam Organization: Brown University X-Mailer: Mozilla 3.0 (X11; I; SunOS 5.5 sun4m) MIME-Version: 1.0 To: globillum@imag.fr CC: Jonathan Corson-Rikert , Jim Arvo , Peter Shirley Subject: Looking for interactive demos Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: 86f62affc69974da656a9c06e300de38 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 such as Java applets illustrating basic radiosity, e.g., shooting versus gathering... or videotapes of same... (i'd like to use them in my intro graphics course and don't have time to develop them this semester.) tx, -andy From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id XAA26014; Wed, 27 Nov 1996 23:01:33 +0100 Received: from phong.cs.utah.edu (phong.cs.utah.edu [128.110.4.52]) by imag.imag.fr (8.8.1/8.6.9) with SMTP id WAA05765 for ; Wed, 27 Nov 1996 22:30:48 +0100 (MET) Received: (from shirley@localhost) by phong.cs.utah.edu (950413.SGI.8.6.12/950213.SGI.AUTOCF) id OAA06323 for globillum@imag.fr; Wed, 27 Nov 1996 14:28:09 -0700 From: Peter Shirley Message-Id: <199611272128.OAA06323@phong.cs.utah.edu> Subject: International Conference on ISST To: globillum@imag.fr Date: Wed, 27 Nov 1996 14:28:09 -0700 (MST) X-Mailer: ELM [version 2.4 PL23] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: 44f46fdc587847c5347f5be1dbb73bb6 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 I have not been to this conference, but will probably go since it is driving distance from me. More importantly, it is my karma to go. Excerpts from the announcement at http://www.lcc.uma.es/personal/mana/CISST2.html Title of session: Monte Carlo Methods for Physically Based Rendering and.... The conference will be held in the Monte Carlo Resort and Casino hotel, Las Vegas, Nevada, USA. If anybody has any comments on this conference, please share them. Pete From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id VAA01993; Thu, 28 Nov 1996 21:28:44 +0100 Received: from horus.imag.fr (horus.imag.fr [129.88.38.2]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id NAA14450 for ; Thu, 28 Nov 1996 13:59:16 +0100 (MET) Received: from nala.ctima.uma.es (nala.ctima.uma.es [150.214.57.7]) by horus.imag.fr (8.8.1/8.6.9) with SMTP id NAA03291 for ; Thu, 28 Nov 1996 13:54:12 +0100 (MET) Received: from sol10.lcc.uma.es (sol10.lcc.uma.es [150.214.108.1]) by nala.ctima.uma.es (8.6.9/8.6.9) with SMTP id NAA05688 for ; Thu, 28 Nov 1996 13:52:13 GMT Received: from frvm.lcc.uma.es ([150.214.58.68]) by sol10.lcc.uma.es (5.x/SMI-SVR4) id AA14205; Thu, 28 Nov 1996 13:54:31 GMT Date: Thu, 28 Nov 1996 13:54:31 GMT Message-Id: <1.5.4.16.19961128134948.0a37972e@sol10.lcc.uma.es> X-Sender: villa@sol10.lcc.uma.es X-Mailer: Windows Eudora Light Version 1.5.4 (16) Mime-Version: 1.0 Content-Type: text/plain; charset=windows-1252; format=flowed To: globillum@imag.fr From: Francisco Villatoro Subject: Call for Papers: Monte Carlo Methods at CISST'97 X-UIDL: afdf413fb684b4383a8ca786e307595c X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit I think that the following Technical Session to be held at the CISST'97 can be of interest to all globillum people, specially since the recent "What's wrong w/ Monte-Carlo methods?" discussion: ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ Title of session: Monte Carlo Methods for Physically Based Rendering ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ Chair: Mr. Francisco R. Villatoro-Machuca E-mail: villa@lcc.uma.es www: http://www.lcc.uma.es/personal/villa/MonteCarlo.html Description: Physically based rendering is based on the numerical solution of the rendering equation. Two main techniques can be used: Monte Carlo path tracing (image-space stochastic sampling methods) and finite elements (world-space radiosity like mesh-based methods). Monte Carlo methods are very versatile, and if unbiased, convergence is assured, but slow. Mesh-based methods can be used as a bias for Monte Carlo methods in order to improve efficacy. Bias shows up as results that are not noisy, but in fact are incorrect. However, if the bias is adecuately bounded, the image is visually coherent and it is not noticeable. In the future hybrid of Monte Carlo and mesh-based methods are the point. This sesion deals with an analysis of the relative merits of Monte Carlo Path Tracing (MCPT) and Finite Elements (FE) on the basis of their potential for future improvements. Questions as: Should we, and how do we, make MCPT more like Hierarchical FE? Or should Hierarchical FE be made more like MCPT? In short, what form should this hybrid take? ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ THE CALL FOR PAPERS OF THE MAIN CISST'97 EVENT (with the TECHNICAL SESSIONS locally SCHUDULED here in MALAGA appended) follows: --------------- 11/25/1996 Dear Colleagues: I would appreciate your assistance in distributing the appended conference announcement to your colleagues. Any help in publicizing the conference would be most appreciated. Please send any questions about the conference to Professor Hamid R. Arabnia The University of Georgia Tel: (706) 542-3480 Fax: (706) 542-2966 E-mail: hra@cs.uga.edu or to Mr. Antonio Ma–a-G—mez University of Malaga Tel: (+34) 5 213 2754 Fax: (+34) 5 213 1397 E-mail: amg@lcc.uma.es www: http://www.lcc.uma.es/personal/mana/mana.html or to Mr. Francisco R. Villatoro-Machuca University of Malaga Tel: (+34) 5 213 20 96 FAX: (+34) 5 213 28 16 E-mail: villa@lcc.uma.es www: http://www.lcc.uma.es/personal/villa/villa.html Send any questions about technical sessions to their respective Chairs. Kindest regards, Antonio Ma–a-G—mez and Francisco R. Villatoro-Machuca. International Conference on Imaging Science, ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ Systems, and Technology ~~~~~~~~~~~~~~~~~~~~~~~~~ CISST'97 June 30 - July 2, 1997 Las Vegas, Nevada, USA The International Conference on Imaging Science, Systems, and Technology (CISST'97) will be celebrated together with the 1997 International Conference on Parallel and Distributed Processing Techniques and Applications (PDPTA'97) We believe that the parallel/distribute processing researchers and the imaging community can both benefit from each other's expertise. Therefore, we have scheduled both conferences at the same time and location (Las Vegas, June 30 - July 2, 1997) for the benefit of those who would like to exchange research ideas with the other research community. CALL FOR PAPERS The first International Conference on Imaging Science, Systems, and Technology (CISST'97) will be held in Las Vegas, Nevada, June 30 - July 2, 1997. All aspects of computer graphics, image processing, and pattern recognition are included in CISST. You are invited to submit a draft paper of about 5 pages and/or a proposal to organize a technical session (see below for submission information). All accepted papers will be published in the conference proceedings. THE NAMES OF TECHNICAL SESSION CHAIRS WILL APPEAR AS ASSOCIATE EDITORS ON THE COVER OF CONFERENCE PROCEEDINGS. SCOPE Topics of interest include, but are not limited to, the following: O Image generation, acquisition, and processing. O Image display techniques. O Image data structures and databases. O Convergence of imaging media (video and computer). O Virtual reality. O Image compression, coding, and encryption. O Tools for multimedia production and services. O Digital imaging for film and television. O Visualization. O Scene and object modeling. O Knowledge acquisition. O Visual inspection. O Document image understanding. O Image algebra. O Mathematical morphology. O Architecture of imaging and vision systems (including parallel architectures and algorithms). O Neural network techniques and fuzzy logic. O Performance analysis and evaluation. O Software tools and environments for imaging. O Applications including: medicine, robotic, GIS, remote sensing, ... O Other aspects and applications relating to imaging science. SUBMISSION OF PAPERS: Prospective authors are invited to submit three copies of their draft paper (about 5 pages) to H. R. Arabnia (address is given below) by the due date. Submissions for the technical sessions must be send to the Session Chair. E-mail and Fax submissions are also acceptable. The length of the Camera-Ready papers (if accepted) will be limited to 10 pages. Papers must not have been previously published or currently submitted for publication elsewhere. The first page of the draft paper should include: title of the paper, name, affiliation, postal address, E-mail address, telephone number, and Fax number for each author. The first page should also include the name of the author who will be presenting the paper (if accepted) and a maximum of 5 keywords. PROPOSAL FOR ORGANIZING TECHNICAL SESSIONS: Each technical session will have 5/6 paper presentations. The session chairs will be responsible in selecting the papers for their own sessions. The names of session chairs will appear as Associate Editors in the conference proceedings. Proposals to organize technical sessions should include the following information: name and address (+ E-mail) of proposer, title of session, a 100-word description of the topic of the session, and how you plan to advertise the session and select papers for the proposed session. Mail your proposal to H. R. Arabnia (address is given below); E-mail submissions are preferred. Currently Scheduled Technical Sessions: ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ Title of session: Internet Image Security ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ Chair: Mr. Antonio Mana-Gomez E-mail: amg@lcc.uma.es www: http://www.lcc.uma.es/personal/mana/ImageSecurity.html Description: Image transmission over the Internet is one the keys for its popularity. However, one of the great drawbacks of the Internet is the free access to and broadcasting of these images. It is possible to view the transmission of images from two different standpoints: firstly, it is a due to allow the users to transmit with privacy and efficacy the images, so there has to be a tool to supply those items; secondly, the frequent news in the media on child pornography and other illegal topics, shows that Internet can become a crime paradise. From this second approach it is clear that the development of tools to control the broadcasting of these images is a need. Balance between the user's right to privacy and the community need of instruments to avoid misuse of the Internet has to be achieved by any solution to this problem. This technical session deals with new techniques and protocols that can make possible this balance whithout compromising efficiency. ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ Title of session: Monte Carlo Methods for Physically Based Rendering ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ Chair: Mr. Francisco R. Villatoro-Machuca E-mail: villa@lcc.uma.es www: http://www.lcc.uma.es/personal/villa/MonteCarlo.html Description: Physically based rendering is based on the numerical solution of the rendering equation. Two main techniques can be used: Monte Carlo path tracing (image-space stochastic sampling methods) and finite elements (world-space radiosity like mesh-based methods). Monte Carlo methods are very versatile, and if unbiased, convergence is assured, but slow. Mesh-based methods can be used as a bias for Monte Carlo methods in order to improve efficacy. Bias shows up as results that are not noisy, but in fact are incorrect. However, if the bias is adecuately bounded, the image is visually coherent and it is not noticeable. In the future hybrid of Monte Carlo and mesh-based methods are the point. This sesion deals with an analysis of the relative merits of Monte Carlo Path Tracing (MCPT) and Finite Elements (FE) on the basis of their potential for future improvements. Questions as: Should we, and how do we, make MCPT more like Hierarchical FE? Or should Hierarchical FE be made more like MCPT? In short, what form should this hybrid take? ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ Title of session: Progressive Transmission and Rendering of 3D Scenes for the Internet ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ Chair: Mr. Francisco R. Villatoro-Machuca E-mail: villa@lcc.uma.es www: http://www.lcc.uma.es/personal/villa/ProgTrans.html Description: New extensions of the World Wide Web (WWW) interface (the Virtual Reality Modeling Language (VRML),JAVA Scripts) has been addressed the ability to visualize three dimensional (3D) object oriented scenarios and allowed the interactive manipulation with their basic elements. Unfortunately, most realistic scenes require a large amount of storage and, consequently, their transmission is very slow. Existing viewers must deal with this problem. Multiresolution video, wavelet multiresolution meshes, progressive transmission, mesh compression and dynamic display are proposed solutions. This technical session is about theses new techniques which can make possible virtual worlds on the cyberspace. ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ EVALUATION OF PAPERS: Papers will be evaluated for originality, significance, clarity, and soundness. Each paper will be refereed by two researchers in the topical area. The Camera-Ready papers will be reviewed by one person. Please refer to the technical sessions pages for details on the evaluation of the papers for those sessions. PUBLICATION: The conference proceedings will be published by CSREA Press. The proceedings will be available at the conference. Please note that all color pictures/diagrams will be published in gray-scale. ORGANIZERS/SPONSORS: A number of university faculty members in cooperation with the Monte Carlo Hotel (conference division) will be organizing the conference. The conference is sponsored by the Computer Science Research, Education, and Applications Tech. (CSREA) in cooperation with the Computer Vision Research and Applications Tech. (CVRA), The National Supercomputing Center for Energy and the Environment (USA), developers of high-performance machines and systems (pending) and related computer associations (pending.) LOCATION OF CONFERENCE: The conference will be held in the Monte Carlo Resort and Casino hotel, Las Vegas, Nevada, USA. This is a new hotel with excellent conference facilities and over 3000 rooms. The hotel is minutes from the Las Vegas airport with free shuttles to and from the airport. The hotel has many vacation and recreational attractions, including: casino, waterfalls, spa, kiddie pools, sunning decks, Easy River water ride, wave pool with cascades, lighted tennis courts, health spa (with workout equipment, whirlpool, sauna, ...), arcade virtual reality game rooms, nightly shows, snack bars, a number of restaurants, shopping area, ... Many of these attractions are open 24 hours a day and most are suitable for families and children. The hotel's room rate is very reasonable ($79 + 8% tax) per night for the duration of the conference. The hotel is minutes from other Las Vegas attractions (major shopping areas, recreational destinations, fine dining and night clubs, free street shows, ...). For the benefit of our international colleagues: the state of Nevada neighbors with the states of California, Oregon, Idaho, Utah, and Arizona. Las Vegas is only a few driving hours away from other major cities, including: Los Angeles, San Diego, Phoenix, ... EXHIBITION: An exhibition is planned during the conference. We have reserved 20+ exhibit spaces. Interested parties should contact H. R. Arabnia (address is given below). All exhibitors will be considered to be the co-sponsors of the conference. Each exhibitor will have the opportunity to include a two-page description of their latest products in the conference proceedings (if submitted by May 19, 1997). IMPORTANT DATES: February 12, 1997 (Wednesday): Draft papers (5-page) due April 8, 1997 (Tuesday): Notification of acceptance May 19, 1997 (Monday): Camera-Ready papers & Preregistration due June 30, July 1, July 2: CISST'97 Conference Proposals to organize technical sessions should be submitted as soon as possible (well ahead of the February 12 deadline). All accepted papers are expected to be presented at the conference. PROGRAM COMMITTEE: (as of Nov. 25, 1996) I. Ahmad, Hong Kong University of Science & Technology, Hong Kong; H. R. Arabnia, University of Georgia, Athens, GA, USA; C. Colin, Ecole des Mines de Nantes, France; J. Farison, University of Toledo, Toledo, OH, USA; M. E. Fayad, University of Nevada, Reno, NV, USA; O. Frieder, George Mason University & Florida Tech., USA; F. Golshani, Arizona State University, Tempe, AZ, USA; V. Gudivada, University of Missouri at Rolla, MO, USA; M. Halem, Space Data & Comp. Div., Goddard Space Flight Center, NASA, USA; G. Hu, Central Michigan University, MI, USA; K-C. Hui, Chinese University of Hong Kong, Shatin, Hong Kong; O. H. Ibarra, University of California, Santa Barbara, CA, USA; X. Jia, City University of Hong Kong, Hong Kong; J. Jin, University of New South Wales, Sydney, Australia; D. Kazakos, University of Southwestern Louisiana, LA, USA; A. Law, Ohio State University, Columbus, OH, USA; D. Luzeaux, Etca/Crea/Sp, France; K. Makki, University of Nevada Las Vegas, NV, USA; S. A. M. Makki, University of Queensland, Australia; A. Mana-Gomez, E.T.S.I.Informatica, Malaga, Spain; N. Memon, Northern Illinois University, DeKalb, IL, USA; B. Nassersharif, National Supercomputing Center For Energy and the Environment, Las Vegas, Nevada, USA; M. S. Obaidat, Monmouth University, NJ, USA; Y. Pan, University of Dayton, Dayton, OH, USA; E. K. Park, University of Missouri-Kansas City, USA; W. Peng, Southwest Texas State University, San Marcos, TX, USA; N. Pissinou, University of Southwestern Louisiana, Lafayette, LA, USA; Rajkumar, Centre for Development of Advanced Computing, Bangalore, India; S. Sahni, University of Florida, Gainesville, FL, USA; H. Sharif, University of Nebraska Lincoln, USA; H. Shi, University of Missouri-Columbia, MO, USA; M. Singhal, Ohio State University, Columbus, OH, USA; S. Y. W. Su, University of Florida, Gainesville, FL, USA; A. Tentov, University "Sv. Kiril i Metodij", Republic of Macedonia; E. Torng, Michigan State University, MI, USA; N-F. Tzeng, University of Southwestern Louisiana, Lafayette, LA, USA; F. R. Villatoro-Machuca, Universidad de Malaga, Malaga, Spain; Y. Xu, Oak Ridge National Laboratory, Oak Ridge, TN, USA; S. You, State University of New York at Stony Brook, NY, USA; H. Zhang, Aptronix, Inc., Santa Clara, CA, USA; D. Zhu, Aptronix, Inc., Santa Clara, CA, USA; A. Y. Zomaya, University of Western Australia, Australia. CONFERENCE CONTACT: Professor Hamid R. Arabnia (CISST General Chair) The University of Georgia Department of Computer Science 415 Graduate Studies Research Center Athens, Georgia 30602-7404, U.S.A. Tel: (706) 542-3480 Fax: (706) 542-2966 E-Mail : hra@cs.uga.edu LOCAL ARRANGEMENT CHAIRS: Professor Kia Makki Department of Computer Science University of Nevada Las Vegas Las Vegas, Nevada 89154-4019, USA E-Mail : kia@koko.cs.unlv.edu Professor Niki Pissinou Center For Advanced Computer Studies University of Southwestern Louisiana Lafayette, LA 70508, USA E-Mail : pissinou@cacs.usl.edu PUBLICITY CHAIR: Professor Yi Pan Department of Computer Science University of Dayton Dayton, OH 45469-2160, USA Tel: (513) 229-3807 Fax: (513) 229-4000 E-Mail : pan@cps.udayton.edu WWW PAGES: http://www.lcc.uma.es/congresos/CISST.html (CISST'97 Home Page) http://www.cps.udayton.edu/~pan/pdpta (PDPTA'97 Home Page) OTHER INFORMATION: ~~~~~ ( o o ) +----------------o000-----U------000o--------------------+ ! _ , ! ! Antonio Mana Gomez eMail: amg@lcc.uma.es ! ! ! ! Departamento de Lenguajes y Ciencias de la Computacion ! ! E.T.S.I.Informatica. Desp. 1.2.B.19 ! ! Universidad de Malaga ! ! Campus de Teatinos. ! ! 29071 MALAGA (SPAIN) ! ! ! ! Phone: (+34) 5 213 27 54 Fax: (+34) 5 213 13 97 ! +--------------------------------------------------------+ OR OTHERWISE FROM: +---------------------------------------------------------+ ! ! ! Francisco R. Villatoro Machuca EMAIL: villa@lcc.uma.es ! ! ! ! Departamento de Lenguajes y Ciencias de la Computacion ! ! E.T.S.Ing. Industriales Desp. I-323-D ! ! Universidad de Malaga ! ! Campus de El Ejido. ! ! 29013 MALAGA (SPAIN) ! ! ! ! Phone: (+34) 5 213 20 96 Fax: (+34) 5 213 28 16 ! ! ! ! http://www.lcc.uma.es/personal/villa/villa.html ! +---------------------------------------------------------+ From Received: from launzatte.cg.tuwien.ac.at by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) for id JAA25804; Mon, 2 Dec 1996 09:45:10 +0100 Received: (from prikryl@localhost) by launzatte.cg.tuwien.ac.at (8.6.12/8.6.9) id JAA02613; Mon, 2 Dec 1996 09:39:13 +0100 From: Jan Prikryl Message-Id: <199612020839.JAA02613@launzatte.cg.tuwien.ac.at> Subject: Re: reflection questions In-Reply-To: from by way of Werner Purgathofer at "Dec 2, 96 08:48:05 am" To: by way of Werner Purgathofer Date: Mon, 2 Dec 1996 09:39:12 +0100 (CET) Cc: Werner Purgathofer X-Mailer: ELM [version 2.4ME+ PL28 (25)] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: 9c1ee991c493b25dda9eed21ac246226 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 > Date: Mon, 2 Dec 1996 08:48:05 +0100 > To: globillum, gervautz, tobler, wilkie, prikryl@sgi.felk.cvut.cz, matkovic, > maria > From: shirley@phong.cs.utah.edu (Peter Shirley) (by way of Werner Purgathofer) > Subject: reflection questions > 2. A paper by [Rushmeier and Tynor, 90] is alluded to, with > no title or bibliography entry. What is it (I have a feeling > our friend HR can answer this one). @InProceedings{Rushmeier90b, author = "Holly E. Rushmeier and Stephen D. Tynor", title = "Incorporating the {BRDF} into an Infrared Scene Generation System", booktitle = "Conference on Characterization, Propagation and Simulation of Infrared Scenes, SPIE Proceedings", volume = "1311", address = "Orlando, Florida", month = apr, year = "1990", note = "also as Technical Report \#90-17, Laboratoire Bordelais de Recherche en Informatique, Universite de Bordeaux.", } http://sgi.felk.cvut.cz/~biblio/ http://liinwww.ira.uka.de/bibliography/ -- JP ------------------------------------------------------------------------- Jan Prikryl http://www.cg.tuwien.ac.at/staff/JanPrikryl.html Institute of Computer Graphics and Visualisation Vienna Institue of Technology, Austria ------------------------------------------------------------------------- From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id SAA07988; Tue, 3 Dec 1996 18:26:59 +0100 Received: from HOSTESS.GRAPHICS.CS.CMU.EDU (HOSTESS.GRAPHICS.CS.CMU.EDU [128.2.206.188]) by imag.imag.fr (8.8.1/8.6.9) with SMTP id RAA18025 for ; Tue, 3 Dec 1996 17:24:02 +0100 (MET) From: Paul.Heckbert@HOSTESS.GRAPHICS.CS.CMU.EDU Message-Id: <199612031624.RAA18025@imag.imag.fr> Date: Tue, 3 Dec 96 11:08:20 EST To: shirley@PHONG.CS.UTAH.EDU Subject: Re: International Conference on ISST Cc: globillum@imag.fr X-UIDL: f2ffe7c11d0d14ba45e5fb8156059ab7 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Re: Peter Shirley's email about the conference: International Conference on Imaging Science, Systems, and Technology CISST'97 June 30 - July 2, 1997 Las Vegas, Nevada, USA http://www.lcc.uma.es/personal/mana/CISST2.html Hmmm, the web page says there will be a self-appointed program committee / session chairs / associate editors. Sounds quite suspicious, frankly. I wouldn't be surprised if their acceptance rate is near 100%. I would predict highly variable paper quality. There is an excellent water slide in Las Vegas, however! :-) I just participated in a workshop where only 3 out of 28 papers submitted were rejected, but it was still worthwhile, however. Are you familiar with the VIDEA story? Beware of VIDEA!, an amusing and troubling account of a bogus conference, reported by Purgathofer, Groeller, and Feda of the U of Vienna. From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id EAA14959; Wed, 11 Dec 1996 04:28:16 +0100 Received: from mercury.uniserve.com (mercury.uniserve.com [204.191.197.248]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id EAA03509 for ; Wed, 11 Dec 1996 04:04:19 +0100 (MET) Received: from helios (van0202.tvs.net [204.191.197.42]) by mercury.uniserve.com (8.8.2/8.8.2) with ESMTP id SAA12854 for ; Tue, 10 Dec 1996 18:56:16 -0800 (PST) Message-Id: <199612110256.SAA12854@mercury.uniserve.com> From: "Ian Ashdown" To: globillum@imag.fr Subject: Radiosity bibliography update Date: Tue, 10 Dec 1996 19:02:16 -0800 X-MSMail-Priority: Normal X-Priority: 3 X-Mailer: Microsoft Internet Mail 4.70.1155 MIME-Version: 1.0 Content-Type: text/plain; charset=windows-1252; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: 2f1597796ff7a36c321fa979124c98c0 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 ANNOUNCE: 96/12/15 Release of RADBIB96 -------------------------------------- RADBIB96 is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. The total number of references is now 1,008 (including four U.S. patents on radiosity techniques). This bibliography is available in BibTex format as RADBIB96.BIB (with a release date of December 15, 1996) from: http://www.ledalite.com/library-/rrt.htm and as compressed RadBib96.Z from: ftp://hobbes.lbl.gov/pub/doc As always, it is time-consuming and sometimes difficult to track down conference papers and theses on radiosity and global illumination. If you know of a relevant reference that is not included in the bibliography, please let me know so that I can include it in the next release. --- Ian Ashdown, P. Eng. Research & Development Manager Ledalite Architectural Products Inc. http://www.ledalite.com From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id WAA03682; Fri, 20 Dec 1996 22:49:27 +0100 Received: from eye.eye.com (eye.eye.com [149.54.1.2]) by imag.imag.fr (8.8.1/8.6.9) with SMTP id SAA19457 for ; Fri, 20 Dec 1996 18:52:35 +0100 (MET) Received: from hemlock.eye.com by eye.eye.com with SMTP (1.37.109.8/16.2) id AA10404; Fri, 20 Dec 1996 12:51:54 -0500 Received: by hemlock (1.37.109.8/15.6) id AA20852; Fri, 20 Dec 1996 12:52:21 -0500 Date: Fri, 20 Dec 1996 12:52:21 -0500 From: Eric Haines Message-Id: <9612201752.AA20852@hemlock> To: globillum@imag.fr Subject: new ray tracing bibliography available Cc: erich@hemlock.eye.com X-UIDL: 06f6903bd9e767eb73ae7defecfc29f9 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit I have made the latest version of the ray tracing bibliography which Paul Heckbert and I compiled (with help from many others) available at: http://www.acm.org/tog/resources/bib/ Let me know of any errors or missing references. I've tried to limit new entries to those directly dealing with ray tracing itself as a rendering algorithm or that talk about monte carlo sampling or volume visualization using ray tracing (as opposed to references which mention ray tracing simply as another tool, which for the most part it has become). Eric Haines erich@acm.org From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id VAA08619; Sat, 28 Dec 1996 21:44:28 +0100 Received: from mercury.uniserve.com (mercury.uniserve.com [204.191.197.248]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id VAA04618 for ; Sat, 28 Dec 1996 21:33:35 +0100 (MET) Received: from helios (van0405.tvs.net [204.191.197.105]) by mercury.uniserve.com (8.8.2/8.8.2) with ESMTP id MAA27534 for ; Sat, 28 Dec 1996 12:23:27 -0800 (PST) Message-Id: <199612282023.MAA27534@mercury.uniserve.com> From: "Ian Ashdown" To: globillum@imag.fr Subject: Global illumination validation studies Date: Sat, 28 Dec 1996 12:31:32 -0800 X-MSMail-Priority: Normal X-Priority: 3 X-Mailer: Microsoft Internet Mail 4.70.1155 MIME-Version: 1.0 Content-Type: text/plain; charset=windows-1252; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: f7e94f36ccf72ca43ef90b0dc76bba69 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Chas Ehrlich at Lawrence Berkeley National Lab uncovered these two Web pages: "Physically Accurate Lighting Simulation in Computer Graphics Software" URL: http://rmp.kiam1.rssi.ru/articles/pals/pals.htm "Comparison of Two Methods of Global Illumination Analysis" URL: http:://rmp.kiam1.rssi.ru/articles/cmgia/cmgia.htm I bring them to the attention of this mailing list because: (a) Very few papers have been written on the physical validation of radiosity and global illumination algorithms; (b) The information presented in these Web pages constitute complete technical reports, yet do not appear to have been otherwise published; and (c) The authors compare Lightscape, Radiance, and Specter (Integra Inc.) with some interesting conclusions. Ian Ashdown, P. Eng. Research & Development Manager Ledalite Architectural Products Inc. From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id GAA09745; Sun, 29 Dec 1996 06:18:36 +0100 Received: from relay6.UU.NET (relay6.UU.NET [192.48.96.16]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id GAA18425 for ; Sun, 29 Dec 1996 06:10:17 +0100 (MET) Received: from audrey by relay6.UU.NET with SMTP (peer crosschecked as: Cust115.Max16.San-Francisco2.CA.MS.UU.NET [153.34.189.243]) id QQbwdg05815; Sun, 29 Dec 1996 00:10:06 -0500 (EST) Sender: crs@uunet.uu.net Message-ID: <32C5FB86.167E@pop.net> Date: Sat, 28 Dec 1996 21:03:02 -0800 From: Chris Schoeneman X-Mailer: Mozilla 2.0S (X11; I; IRIX 6.2 IP22) MIME-Version: 1.0 To: Ian Ashdown CC: globillum@imag.fr Subject: Re: Global illumination validation studies References: <199612282023.MAA27534@mercury.uniserve.com> Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: 55cb2736695d3b6a1b7c6d3f733926c3 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Ian Ashdown wrote: > > Chas Ehrlich at Lawrence Berkeley National Lab uncovered these two Web > pages: > > "Physically Accurate Lighting Simulation in Computer Graphics Software" > URL: http://rmp.kiam1.rssi.ru/articles/pals/pals.htm > > "Comparison of Two Methods of Global Illumination Analysis" > URL: http://rmp.kiam1.rssi.ru/articles/cmgia/cmgia.htm This was very interesting reading. From what I know of LVS, most conclusions sounded pretty reasonable. I noted that they used LVS version 1.2.4. My guess is that version 1.3 (available for well over a year) would have given more accurate results, at least for the CUBE test. Version 2.0 would be better still. Both of these versions accurately solve an environment with an analytical solution (the inside of a cube where each face is a perfect diffuse emitter), while 1.2.4 (if I recall correctly) failed this test. In any case, I did find some unexpected conclusions. 1. In APART2 they're surprised by the specular reflection model used by LVS. They assume it's incorrect but it is in fact demonstrating the angular dependence of reflectivity. Whether the model is accurate could be the subject of a similar analysis. 2. In the DREAM0 evaluation they state that LVS doesn't have `cone' lights. Well of course LVS does have them (it calls them spot lights). 3. Also in DREAM0 they note bleeding of light from the red carpet on a corner in the cove with the blue carpet. It shouldn't be there and they say they can't explain the effect. It looks like a light leak, which they should recognize. I'd be more comfortable with their conclusions if they clearly stated that it wasn't a light leak and that the models were constructed to avoid light and shadow leaks. Still, since the ROOM model is from Lightscape it's safe to assume that it is so constructed. And since it fails to match Specter and Radiance, it's pretty clear that LVS 1.2.4 isn't as accurate as either. Perhaps it's my bias from having worked at Lightscape, but at a visceral level I generally find the Lightscape images much more realistic looking than either the Specter or Radiance images. Too bad they're not as accurate. Many thanks to Chas and the authors for making this known. Cheers, -chris From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id XAA15056; Mon, 30 Dec 1996 23:53:55 +0100 Received: from lbl.gov (lbl.gov [128.3.254.23]) by imag.imag.fr (8.8.1/8.6.9) with SMTP id XAA25091 for ; Mon, 30 Dec 1996 23:21:51 +0100 (MET) Received: from hobbes.lbl.gov by lbl.gov (SMI-8.6/SMI-SVR4) id OAA28251; Mon, 30 Dec 1996 14:21:25 -0800 Received: by hobbes.lbl.gov (3.2/SMI-3.2) id AA08533; Mon, 30 Dec 96 14:20:07 PST Date: Mon, 30 Dec 96 14:20:07 PST From: "Gregory J. Ward" Message-Id: <9612302220.AA08533@hobbes.lbl.gov> To: Oek@int.keldysh.ru Subject: lighting simulation comparisons Cc: chas@hobbes.lbl.gov, globillum@imag.fr, iashdown@ledalite.com X-UIDL: a68bfb384bfb109f8d297500f5b94de0 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit This is very good work (referring to the comparison between Lightscape, Spectre and Radiance at http://rmp.kiam1.rssi.ru/articles/pals/pals.htm). Is this going to be a technical report somewhere? I would like to learn more about Spectre also. I have followed this program through its various name changes, but never actually spoken to someone with a copy of it. It sounds like it has come a long way, and is worth a closer look. Can you send us a working web address for this product (the link on your report seems to be broken)? I was a bit disappointed at the quality of the Radiance renderings you showed, and I wonder if you used the new "rad" interface to generate them? This is an executive script that makes the control of calculation parameters and image filtering much more automatic and natural, and would reduce or eliminate many of the artifacts you are seeing, which are the result of poor parameter choices or (in the case of the aliasing artifacts) missing the final image filtering pass. This same program also has a GUI, called trad, which makes running and controlling the rendering process much easier. I was very pleased to see the in-depth analysis of the three calculation methods. I was particularly intrigued by Spectre's apparent ability to control the overall simulation accuracy. Since this quantity is intricately tied to the geometric modeling and the resolution of the illumination map, however, I am not sure exactly what is being controlled here. I notice in the comparison of absolute error, that Spectre did not seem to have as good a handle on its calculation as implied by this accuracy parameter. In my own research on global illumination, I have found such absolute error bounds to be extremely elusive. The work on this by Arvo and others has shown some promise for error limits at radiosity mesh points, but of course this says nothing about what's going on between mesh points, and this is for diffuse-only environments besides. Monte Carlo methods can offer statistical error estimates for arbitrary environments, but achieving specific accuracy tolerances at some pixels is next to impossible using conventional methods. (I won't scoop Eric Veach, who seems to have found a very promising new MC technique which I hope will appear in the literature sooner rather than later.) There were some other, very minor, errors in your exposition, which I would be happy to correct if you like. The main problem in my view was the way Radiance was used, which had a large effect on the results. I admit that it is not at all clear for the new user how to best apply this software, even if they have an excellent understanding of the underlying algorithms. I am hoping to remedy this situation with the publication of a book from Wiley, which will hopefully be available by this Summer. Please forward this also to Andrei, as I did not find his e-mail address. Thanks! -Greg Ward From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id AAA15100; Tue, 31 Dec 1996 00:14:38 +0100 Received: from lbl.gov (lbl.gov [128.3.254.23]) by imag.imag.fr (8.8.1/8.6.9) with SMTP id XAA26115 for ; Mon, 30 Dec 1996 23:49:37 +0100 (MET) Received: from hobbes.lbl.gov by lbl.gov (SMI-8.6/SMI-SVR4) id OAA28566; Mon, 30 Dec 1996 14:49:13 -0800 Received: by hobbes.lbl.gov (3.2/SMI-3.2) id AA08597; Mon, 30 Dec 96 14:47:56 PST Date: Mon, 30 Dec 96 14:47:56 PST From: "Gregory J. Ward" Message-Id: <9612302247.AA08597@hobbes.lbl.gov> To: Oek@int.keldysh.ru Subject: P.S. to last message Cc: chas@hobbes.lbl.gov, globillum@imag.fr, iashdown@ledalite.com X-UIDL: 42ea3d5cd68b16c7f76b9ab46f26eedf X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit If you want to see some other examples of how close Radiance can come to reality (I always do), check out the following web page: http://sap.mit.edu/projects/studioimages.html This is work done independently by Philip Thompson and Jack DeValpine at MIT. -Greg From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id SAA00143; Mon, 6 Jan 1997 18:27:05 +0100 Received: from gin.keldysh.ru (root@[194.226.56.162]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id QAA11675 for ; Mon, 6 Jan 1997 16:45:08 +0100 (MET) Received: from oak.keldysh.ru (oak.keldysh.ru [194.226.56.183]) by gin.keldysh.ru (8.7.6/8.7.3) with SMTP id SAA13496; Mon, 6 Jan 1997 18:44:33 +0300 Message-ID: <32D11D7F.3E94@gin.keldysh.ru> Date: Mon, 06 Jan 1997 18:42:57 +0300 From: Andrei Khodulev Reply-To: abkhod@gin.keldysh.ru Organization: Integra X-Mailer: Mozilla 3.0 (Win95; I) MIME-Version: 1.0 To: globillum@imag.fr CC: greg@hobbes.lbl.gov, crs@pop.net Subject: Re: lighting simulation comparisons Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: 8f02d859ed55d97febb9b2a005760dc7 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Some year and half ago we requested providers of physically accurate lighting simulation software to deliver their software for the purpose of evaluation. We did our best to perform as unbiased benchmarks as possible. The results has been published in Graphicon 96 and posted on our (KI) home page http://rmp.kiam1.rssi.ru/articles/pals since May 1996. As people behind Radiance (Greg Ward) and LVS (Chris Shoeneman) are not necessarily satisfied with the way their software has been used in comparisons we are ready to repeat the benchmarks following the additional information. We also welcome others who are willing to deliver their software for benchmarking. Andrei Khodulev, abkhod@gin.keldysh.ru Edward Kopylov, oek@gin.keldysh.ru P.S. There is also a paper "Comparison of two Methods of Global Illumination Analysis" devoted to comparison of Deterministic and Monte Carlo algorithms of global illumination analysis. http://rmp.kiam1.rssi.ru/articles/cmgia/ Andrei Khodulev. From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id UAA00404; Mon, 6 Jan 1997 20:22:25 +0100 Received: from gin.keldysh.ru (root@[194.226.56.162]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id TAA22481 for ; Mon, 6 Jan 1997 19:57:14 +0100 (MET) Received: from oak.keldysh.ru (oak.keldysh.ru [194.226.56.183]) by gin.keldysh.ru (8.7.6/8.7.3) with SMTP id VAA14116; Mon, 6 Jan 1997 21:56:11 +0300 Message-ID: <32D14A69.5E4C@gin.keldysh.ru> Date: Mon, 06 Jan 1997 21:54:35 +0300 From: Andrei Khodulev Reply-To: abkhod@gin.keldysh.ru Organization: Keldysh Inst. of Appl. Math. X-Mailer: Mozilla 3.0 (Win95; I) MIME-Version: 1.0 To: greg@hobbes.lbl.gov CC: globillum@imag.fr, chas@hobbes.lbl.gov, iashdown@ledalite.com Subject: Re: lighting simulation comparisons Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: 0ece291858c5d28fb8e1042e14dbe066 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Dear Greg, Hello from Andrei Khodulev, with whom You exchanged some letters in 1992. >I would like to learn more about Spectre also. I have followed >this program through its various name changes, but never actually >spoken to someone with a copy of it. >It sounds like it has come a long way, and is worth a closer >look. Can you send us a working web address for this product >(the link on your report seems to be broken)? Integra Inc. is in the process of establishing official page in English. For this reasons links are not available. At this point only Japanese page exist: http://www.kt.rim.or.jp/~integra/ Mr. A. Fujimoto, the president of Integra Inc., was asked about preparation of non-commercial version of SPECTER that can be used by others for comparison study analogous to our one. Please wait for answer from him. COMPARISON As You (and apparently LVS) are not satisfied with the way RADIANCE (LIGHTSCAPE) has been used we are going to repeat the comparison following your advises and with new software version(3.0 ?). Today we sent a message to globillum at this topic and welcome others who are willing to deliver their software for benchmarking. I think it will take finite time until all information is completed and conditions are agreed among the interested parties. >I was a bit disappointed at the quality of the Radiance renderings you >showed, and I wonder if you used the new "rad" interface to generate >them? > This is an executive script that makes the control of calculation >parameters and image filtering much more automatic and natural, and would >reduce or eliminate many of the artifacts you are seeing, which are the >result of poor parameter choices or (in the case of the aliasing artifacts) >missing the final image filtering pass. > > >This same program also has a GUI, called trad, which makes running and >controlling the rendering process much easier. > You pointed our serious mistake: we refer to RADIANCE 2.5 (and we actually used it for benchmarks!) while obsolete Reference Manual (for previous 2.4 version) was used. So, we knew nothing about 'trad'. What concerns to 'rad' we found it more convenient to call the batch programs ('oconv', 'rpict', 'ximage') directly as we need sometimes rather long calculations. Maybe we missed some possibilities offered by 'rad'. Filtering was not used at all. Apparently we met some problems with its usage. >I was particularly intrigued by Spectre's apparent ability to >control the overall simulation accuracy. Since this quantity is intricately >tied to the geometric modeling and the resolution of the illumination map, >however, I am not sure exactly what is being controlled here. > Have you seen the paper "Comparison of two Methods of Global Illumination Analysis" at http://rmp.kiam1.rssi.ru/articles/cmgia/monte_carlo.htm ? Section 3.1 of this paper contains detailed explanation of how accuracy is controlled in Specter. We'll be very grateful to You for any remarks. The reason for this request is that some readers find this part unclear. >I notice in the comparison of absolute error, that Spectre did >not seem to have as good a handle on its calculation as implied >by this accuracy parameter. In my own research on global >illumination, I have found such absolute error bounds to be >extremely elusive. > Yes, we also found that the accuracy control Specter provides is not always natural for user. Actually, the Specter's accuracy measure is frequently used in relative manner: we don't know how the value reported relates to perceptual quality, but we can rely that decreasing of this value twice will lead to twice as good image. >There were some other, very minor, errors in your exposition, >which I would be happy to correct if you like. > > >The main problem in my view was the way Radiance was used, which >had a large effect on the results. > Any remarks are welcome. > I admit that >it is not at all clear for the new user how to best apply this software, >even if they have an excellent understanding of the underlying algorithms. >I am hoping to remedy this situation with the publication of a book from >Wiley, which will hopefully be available by this Summer. > Is there any possibility to get draft of this book in electronic from? Thank you in advance. >If you want to see some other examples of how close Radiance can come to >reality (I always do), check out the following web page: > >http://sap.mit.edu/projects/studioimages.html > >This is work done independently by Philip Thompson and Jack DeValpine at >MIT. > Can we get scenes used to generate these images? We could use them in our comparison. With best regards, Edward Kopylov, Andrei Khodulev. From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id XAA16047; Tue, 7 Jan 1997 23:13:04 +0100 Received: from internet-mail2.ford.com (internet-mail2.ford.com [198.111.80.24]) by imag.imag.fr (8.8.1/8.6.9) with SMTP id WAA03594 for ; Tue, 7 Jan 1997 22:51:10 +0100 (MET) Received: by internet-mail2.ford.com id AA18258 (InterLock SMTP Gateway 3.0 for globillum@imag.fr); Tue, 7 Jan 1997 16:50:28 -0500 Message-Id: <199701072150.AA18258@internet-mail2.ford.com> Received: by internet-mail2.ford.com (Protected-side Proxy Mail Agent-1); Tue, 7 Jan 1997 16:50:28 -0500 Date: Tue, 7 Jan 1997 16:50:27 -0500 From: Stephen Westin To: globillum@imag.fr In-Reply-To: <32D24D96.2781E494@doc.ic.ac.uk> (ajc@doc.ic.ac.uk) Subject: Kajiya path tracing X-UIDL: 01ef6eef483f2e210a1252f753e90e07 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit > PS. Under what conditions would 40 samples per pixel in MCPT be enough to > visualise a double-refracted caustic? This is in reference to J. T. Kajiya's > landmark SIGGraph '86 paper the "The Rendering Equation". The caustics cast in > his tetrahedron of glass balls image seem so noise free. I wonder how they did > it. Extremely large light sources, I understand. -Stephen H. Westin swestin@ford.com The information and opinions in this message are mine, not Ford's. From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id IAA18132; Wed, 8 Jan 1997 08:24:09 +0100 Received: from safran.imag.fr (safran.imag.fr [129.88.32.200]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id IAA17322 for ; Wed, 8 Jan 1997 08:09:42 +0100 (MET) Received: (from sillion@localhost) by safran.imag.fr (8.6.10/8.6.9) id IAA05020 for globillum@imag.fr; Wed, 8 Jan 1997 08:09:41 +0100 From: Francois Sillion Message-Id: <199701080709.IAA05020@safran.imag.fr> Subject: Teamcad problem resolved To: Global Illumination List Date: Wed, 8 Jan 1997 08:09:40 +0100 (MET) Reply-To: Francois.Sillion@imag.fr X-Mailer: ELM [version 2.4 PL23] MIME-Version: 1.0 Content-Type: text/plain; charset=windows-1252; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: fef84b86def1b8bc8c34b14b4016ea16 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Dear globillumers, first of all, a happy new year to all ! Most of you have noticed a very annoying problem with the teamcad and teamcad2 mailing lists. These lists included the globillum alias, without having asked the globillum recipients or myself for approval. This was a simple mishap and the people at Georgia Tech are very sorry. Now I understand that globillum should have been removed from these lists. The confusion only grew because so many people responded to the first teamcad messages and copied their answers to the list! The second message I want to send to globillumers is that we are undergoing some technical changes here as globillum has been moved to a list server. Apparently everything works fine but it means that some people who have requested to be on the list have not been added yet. If you know anybody in this situation... tell them I'll work on it as soon as possible ! +------------------+------------------------------------------------------+ | Francois SILLION | iMAGIS - GRAVIR/IMAG, B.P. 53, 38041 Grenoble Cedex 9| | ' | France. Tel:+33 4 76 51 43 54 - Fax:+33 4 76 44 66 75| +------------------+----------+-------------------------------------------+ | Francois.Sillion@imag.fr | http://w3imagis.imag.fr/~Francois.Sillion | +-----------------------------+-------------------------------------------+ From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id QAA01209; Thu, 9 Jan 1997 16:36:30 +0100 Received: from igw3.watson.ibm.com (igw3.watson.ibm.com [129.34.139.18]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id PAA14088 for ; Thu, 9 Jan 1997 15:57:02 +0100 (MET) Received: from mailhub1.watson.ibm.com (mailhub1.watson.ibm.com [9.2.249.31]) by igw3.watson.ibm.com (8.7.6/8.7.1) with ESMTP id JAA13986 for ; Thu, 9 Jan 1997 09:57:23 -0500 Received: from watngi01.watson.ibm.com (watngi01.watson.ibm.com [9.2.235.20]) by mailhub1.watson.ibm.com (8.8.2/11-26-96) with SMTP id JAA54332 for ; Thu, 9 Jan 1997 09:56:44 -0500 Received: by watngi01.watson.ibm.com(Lotus SMTP MTA Release 1.0.1) id 8525641A.00521663 ; Thu, 9 Jan 1997 09:56:36 -0400 X-Lotus-FromDomain: IBM RESEARCH From: "Holly Rushmeier" To: globillum@imag.fr Message-ID: <8525641A:0051795D.00@watngi01.watson.ibm.com> Date: Thu, 9 Jan 1997 09:55:51 -0400 Subject: Need refs. about need Mime-Version: 1.0 Content-type: text/plain; charset=us-ascii; format=flowed X-UIDL: 2d48493319f989e335d4b611834f12cb X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hi -- One of the people working on the appearance project at NIST asked me for "some references that talk about the need for measurements of appearance properties of materials." A lot of people ask about where to find catalogs of measurements etc., but I am having a hard time finding "citable" references for the need for measurements. If you have written anything, either technical paper or more informal "position" paper that could be cited about the need for measurements to support realistic rendering please let me know. Or, if you haven't written anything, but would be willing to be quoted about how your work would benefit by the availability of measurements, or measurement techniques, let me know. Thanks, Holly From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id CAA21734; Thu, 16 Jan 1997 02:29:59 +0100 Received: from ftp20.jet.es (root@[194.179.100.193]) by imag.imag.fr (8.8.1/8.6.9) with SMTP id CAA11623 for ; Thu, 16 Jan 1997 02:14:10 +0100 (MET) Received: from 007 (info636.jet.es [194.224.182.126]) by ftp20.jet.es (8.6.12/8.6.9) with SMTP id DAA12836 for ; Thu, 16 Jan 1997 03:12:10 +0100 Message-ID: <32DD8061.77A0@jet.es> Date: Thu, 16 Jan 1997 02:12:01 +0100 From: Eduardo Bustillo Iceta X-Mailer: Mozilla 3.0 (WinNT; I) MIME-Version: 1.0 To: globillum@imag.fr Subject: kd-tree Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: e1c38e4a2486743f9d1286a476a702c2 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hi globillumers :) I am preparing a paper on a new globillum rendering technique and I am trying to implement several other methods in my rendering architecture for comparison and benchmarking. One of these methods is the photon map. Reading H.W. Jensen's "Global illumination using photon maps" paper there is a reference to Bentley's kd-tree M nearest point searching algorithm. Jensen explains that this algorithm can find the M nearest (euclidean distance) photons to any given point in a N point set in O(M log2 N) time. Due to the shortage of CS books in my school I have been unable to find Bentley's paper :( I have worked out another method creating 3 sorted lists (one for each coord.) and doing the following: -For the first coord. I search for the M closest 1D photons right and left from the nearest. -For the other coords. I also search right and left from the closest 1D point in the list and within a constantly updated range given by the longest euclidean distance of the M photons found to that point to update the M nearest photons list. The longest distance bounds the 1D range so that photons outside it must be farther away. This method is much worse than O(M log2 N) making it almost worthless. I have been thinking about how it could be performed using a kd-tree but it seems much more prepared to handle hypercubes than hyperspheres... I am sorry to put this question on the list as it might sound quite naive but if any of you could be kind enough to point me the right way (as in Bentley's), I would be really grateful as I have been thinking of changing to an octree structure or hanging myself :) Thanks a lot, Eduardo. --- Eduardo Bustillo Iceta Particular de Basterra 1 48990 Getxo (Vizcaya) SPAIN e-mail: ebic@jet.es ebic@acm.org From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id WAA18966; Tue, 21 Jan 1997 22:03:06 +0100 Received: from ebene.inrialpes.fr (ebene.inrialpes.fr [194.199.18.70]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id VAA02387 for ; Tue, 21 Jan 1997 21:33:12 +0100 (MET) Received: from lbl.gov ([128.3.254.23]) by ebene.inrialpes.fr (8.6.13-durand/8.6.9) with ESMTP id VAA27452 for ; Tue, 21 Jan 1997 21:33:10 +0100 Received: from hobbes.lbl.gov by lbl.gov (SMI-8.6/SMI-SVR4) id MAA28357; Tue, 21 Jan 1997 12:19:23 -0800 Received: by hobbes.lbl.gov (3.2/SMI-3.2) id AA15537; Tue, 21 Jan 97 12:17:56 PST Date: Tue, 21 Jan 97 12:17:56 PST From: "Gregory J. Ward" Message-Id: <9701212017.AA15537@hobbes.lbl.gov> To: abkhod@gin.keldysh.ru Subject: Re: lighting simulation comparisons Cc: chas@hobbes.lbl.gov, globillum@imag.fr, iashdown@ledalite.com X-UIDL: a06b16f28ecc3ec2caf1006192a30008 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Hi Andrei, I am just getting to comment on your web pages, and I'll just write about what I notice as I go through it (the comparison and validation pages): In http://rmp.kiam1.rssi.ru/articles/pals/radiance.htm, Section 3.1: Note that Radiance has not possibility to specify point or cone light sources at all, i.e. when the light starts from abstract point. As an approximation to point light in Radiance a small lighting sphere can be used. If by "cone light sources" you mean spotlights, there is a spotlight material type that can be used to produce light in cones, not that any such ideal exists in the real world. As for point sources, the spheres may be arbitrarily small. Radiance has not intelligent sampling of light sources. The only case that is handled properly is parallelograms. Light sources in form of sphere are not sampled at all in Radiance. Other sources are approximately rectangular (ref. to Radiance Digest, v2n5.2, 537 line). This is not entirely accurate. It is true that parallelograms are the only sources that are sampled exactly correctly, but the sampling of most other source shapes is approximately correct. Spheres are sampled over a cubic area, which though inaccurate in some sense, does not result in great inaccuracies in the result, and it is considerably faster than doing it exactly as a sphere. I hope you read all of the Radiance Digest section you reference, as Peter did find out that he had been making a mistake in his integration, and that Radiance was actually converging to the correct result. You mention that the conversion from IES luminaire files is "not correct." Again, it is an approximation, as is EVERYTHING in lighting simulation! It doesn't help matters to make inflammatory remarks, especially when you fail to make them for the other packages. None of the packages can model the arbitrarily strange shapes included in the IES specification, and Radiance simply chooses the closest approximating geometry, which is what the other packages must do, also. Section 3.2: Radiance does not "subdivide surfaces into patches." The algorithm employed never makes use of any explicit geometric subdivision of any kind, but relies instead on unorganized point value interpolation. The octree is used for point lookup, but does not decimate the scene. This way, values may be shared between surfaces and subsurfaces on an arbitrary topology, which is a unique feature of the system. You say that Radiance does not handle semispecular surfaces efficiently, when in fact it does, at least as efficiently as Specter. Except for the user-specified BRDF types, all light interactions are accounted for in Radiance, and the process proceeds efficiently from the point of measurement (i.e., the viewpoint) backwards to the light sources. Ideal specular surfaces are treated with the special material types you mention in order to avoid the source-finding problem of light-backwards ray tracing, and the corresponding shadow accuracy (i-map resolution) problem of light-forwards ray tracing. The efficiency enhancements you mention for limiting the cost of the virtual light source calculation are OPTIONAL. For people who insist on accuracy guarantees (which by the way are completely bogus, because light propogation is a probabilistic process), can change these parameters to guarantee results. The runaway creation of virtual sources is still avoided by geometry checks that are 100% reliable. Again, I would like to see a change in the summary, since Radiance does in fact model diffuse-specular interactions fully and correctly. Section 3.3: I agree that setting parameters is non-trivial, which is why I wrote the "rad" program, described in a paper at the 1995 Eurographics Workshop on Rendering. In general, direct accuracy controls are unreliable, but even so, Radiance parameters are tied to accuracy whenever it is possible or reasonable to do so. Section 3.4: You are rightly critical of Radiance 2.5's display mapping function. The next version of Radiance (3.1) includes a new program called "pcond," which contains a comprehensive tone mapping operator with strong ties to human vision. http://rmp.kiam1.rssi.ru/articles/pals/results.htm, Section 5.1.4: I thought this section demonstrated very well my point about the absolute control of accuracy, or lack thereof. That is to say, even though you have so-called "accuracy" settings in Specter, they do not in fact correspond to any kind of accuracy you can measure. Although absolute accuracy is a laudable goal, it is not a practical one when it comes to lighting simulation. All you can do is trade time for accuracy and peform convergence tests such as this on specific scenes. There is no technique that can guarantee lighting simulation accuracy in arbitrary environments. The best we can hope for is a statistical estimate based on Monte Carlo convergence tests, and such a criterion offers no guarantee that the process will EVER finish! Section 5.2: The Radiance rendering exhibits significant aliasing because the final (pfilt) pass was not made. This is an error in the way the rendering was performed that affects the appearance, but not the accuracy of the pixel values. The accuracy of the shadows is a function of the -dj as well as the -ds parameter, which should be controlled by the "rad" program I mentioned before. Section 5.3: Again, the complaint about Radiance images showing jaggies is the result of failing to filter the result properly with pfilt. This can be remedied by applying the "rad" program, which runs it automatically. For some reason, you did not include the time for Radiance rendering of the flower scene. In the bathroom (CG) scene, you say that Specter computed the image an "order of magnitude" (10 times) faster than Radiance, when your table shows times of 4.1 and 3 hours for the two systems, with Radiance being the faster. Something is wrong, here. In the final office scene (very nice, by the way), the rendering parameters obviously require adjustment. Once again, the "rad" program makes this process very intuitive, and I strongly suggest you use it. It also has a single "accuracy" control called "QUALITY", but does not attempt to tie this to numerical accuracy, which cannot be guaranteed, as we have witnessed from the Specter results. http://rmp.kiam1.rssi.ru/articles/pals/conclusion.htm, Section 6: In general, I agreed with your conclusions, despite my earlier remarks. Overall, I think you have provided the global illumination community a tremendous service, and we owe you a debt of gratitude. I hope that your analysis has a great influence on any future validation and comparison work, as a standard of excellence for others to match! -Greg From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id VAA18948; Tue, 21 Jan 1997 21:52:50 +0100 Received: from horus.imag.fr (horus.imag.fr [129.88.38.2]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id VAA02409 for ; Tue, 21 Jan 1997 21:33:42 +0100 (MET) Received: from lbl.gov (lbl.gov [128.3.254.23]) by horus.imag.fr (8.8.1/8.6.9) with SMTP id VAA24066 for ; Tue, 21 Jan 1997 21:33:41 +0100 (MET) Received: from hobbes.lbl.gov by lbl.gov (SMI-8.6/SMI-SVR4) id MAA28841; Tue, 21 Jan 1997 12:29:58 -0800 Received: by hobbes.lbl.gov (3.2/SMI-3.2) id AA15569; Tue, 21 Jan 97 12:28:31 PST Date: Tue, 21 Jan 97 12:28:31 PST From: "Gregory J. Ward" Message-Id: <9701212028.AA15569@hobbes.lbl.gov> To: abkhod@gin.keldysh.ru Subject: Re: lighting simulation comparisons Cc: chas@hobbes.lbl.gov, globillum@imag.fr, iashdown@ledalite.com X-UIDL: 5593d4c2a3d12074a2012ad9440e42fa X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit P.S. to my previous comments. I forgot to mention that the latest version of Radiance (3.0) also has participating media, and can therefore simulate the same effects that Specter seems to. I do not know enough about Specter to comment on the accuracy of its model, but Radiance does apply a fairly rigorous PM model, with typical optimizations to minimize rendering time. These optimizations do require a degree of user control, however. From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id UAA24817; Wed, 22 Jan 1997 20:22:39 +0100 Received: from gin.keldysh.ru (root@[194.226.56.162]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id QAA17088 for ; Wed, 22 Jan 1997 16:11:57 +0100 (MET) Received: from oak.keldysh.ru (oak.keldysh.ru [194.226.56.183]) by gin.keldysh.ru (8.7.6/8.7.3) with SMTP id SAA17189; Wed, 22 Jan 1997 18:10:11 +0300 Message-ID: <32E62DA0.2325@gin.keldysh.ru> Date: Wed, 22 Jan 1997 18:09:21 +0300 From: Andrei Khodulev Reply-To: abkhod@gin.keldysh.ru Organization: Keldysh Inst. of Appl. Math. X-Mailer: Mozilla 3.0 (Win95; I) MIME-Version: 1.0 To: "Gregory J. Ward" CC: chas@hobbes.lbl.gov, globillum@imag.fr, iashdown@ledalite.com Subject: Re: lighting simulation comparisons References: <9701212017.AA15537@hobbes.lbl.gov> Content-Type: text/plain; charset=koi8-r; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: 1c840f07829da8defc45faed5e0e4e1e X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hello, Greg, Thank you for detailed analysis of our comparison study. It seems that we really failed to use some important features of Radiance. Here I comment on one trivial error, I'll answer in more details later. Anyhow we'll undertake new comparison with account for your remarks and suggestions. > For some reason, you did not include the time for Radiance rendering of > the flower scene. In the bathroom (CG) scene, you say that Specter > computed the image an "order of magnitude" (10 times) faster than > Radiance, when your table shows times of 4.1 and 3 hours for the two > systems, with Radiance being the faster. Something is wrong, here. There is a technical error in our text: one column was lost in the timing table. The correct table is: --------------------------------------------- Scene | Simulation + rendering time (hours) name |------------------------------------- | LVS | Specter | Radiance --------------------------------------------- APART2 | 86 | 0.3 | 3.7 DREAM0 | 5.4 | 2.3 | 4.3 FLOWER | 34 | 1.3 | 0.7 CG | 27 | 4.1 | 31 HONSHA | --- | 29 | 38 And one question to you. We downloaded the document http://radsite.lbl.gov:80/mgf/mgfdoc.ps.Z and can not read it. When seen via Ghostscript on IBM PC the document seems to be incorrectly formatted (too tight interline spacing). Can you suggest anything? With best regards, -Andrei. From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id QAA16143; Wed, 29 Jan 1997 16:44:59 +0100 Received: from sys2.london2.uk.psi.net (sys2.london2.uk.psi.net [154.32.110.6]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id PAA17612 for ; Wed, 29 Jan 1997 15:44:50 +0100 (MET) Received: from lightwk.uucp by sys2.london2.uk.psi.net (8.8.4/SMI-5.5-UKPSINet) id NAA27029; Wed, 29 Jan 1997 13:39:30 GMT Received: from bianca by lightwork.co.uk; Wed, 29 Jan 97 13:33:51 GMT Message-Id: <32EF5239.7120@lightwork.co.uk> Date: Wed, 29 Jan 1997 13:35:53 +0000 From: Lindsey Shackleton Organization: LightWork Design X-Mailer: Mozilla 3.0 (WinNT; I) Mime-Version: 1.0 To: globillum@imag.fr Subject: Diffuse/Specular Reflection: Schlick's approximation Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: 455563e85c730bf78f1c33beb4a3c8ca X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hi, Re: "An Inexpensive BRDF Model for Physically Based Rendering" C. Schlick EuroGraphics 94 VVol 13 number 3 I've been working my way through the above paper, and have come unstuck in several places. Any suggestions will be much appreciated. ________________________________________________________________________ Eqn 30. First imagine the terms without the normalisation factor, 4Pi, so it becomes: D(t,v,v',w) = G(v) G(v') Z(t) A(w) + ( 1 - G(v) G(v') ) __________ ______________ v v' v v' First I think this should actually be: D(t,v,v',w) = G(v) G(v') Z(t) A(w) + ( 1 - G(v) G(v') ) __________ __________ v v' v v' Surely this means that ALL the directional diffuse would be reemitted along v'. Shouldn't the ( 1 - G(v)G(v')/vv') be divided by 2Pi so that it is equally distributed over the hemisphere? ________________________________________________________________________ ________________________________________________________________________ - Eqn 32 D(t,v,v',w) = a + b B(t,v,v',w) + c Dirac-delta __ ______________ ______________ Pi 4 Pi v v' v' dV' a,b,c are weighting coefficients. Shouldn't this be D(t,v,v',w) = a Diffuse_refl + b B(t,v,v',w) + c Fresnel Dirac-delta ______________ ______________ ______________________ Pi Pi v' dV' B(t,v,v',w) is the previous D(t,v,v',w). First put the reflectance coefficients in, remove the unecessary vv'. Why was there a factor of 4 on the denominator, if Int[Z(t)A(w)] = Pi over the hemisphere for perfectly smooth isotropic reflectors? ________________________________________________________________________ I would be very grateful for any explanations, Lindsey Shackleton Software Engineer LightWork Design Ltd. From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id SAA19469; Mon, 3 Feb 1997 18:57:09 +0100 Received: from mercury.uniserve.com (mercury.uniserve.com [204.191.197.248]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id QAA13682 for ; Mon, 3 Feb 1997 16:59:25 +0100 (MET) Received: from van0208.tvs.net (van0208.tvs.net [204.191.197.48]) by mercury.uniserve.com (8.8.2/8.8.2) with SMTP id HAA28060 for ; Mon, 3 Feb 1997 07:44:38 -0800 (PST) Date: Mon, 3 Feb 1997 07:44:38 -0800 (PST) Message-Id: <199702031544.HAA28060@mercury.uniserve.com> X-Sender: iashdown@pop.uniserve.com X-Mailer: Windows Eudora Version 1.4.4 Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed To: globillum@imag.fr From: Ian Ashdown Subject: Global illumination bibliography X-UIDL: 7ec7e951c44fd6cabf3a871ef5c06e12 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit ANNOUNCE: 97/02/01 Release of RADBIB97 -------------------------------------- RADBIB97 is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. It currently includes 1,031 references, with some 15 new references being added per month. This bibliography is available in BibTex format as RADBIB97.BIB (with a release date of February 1, 1997) from: http://www.ledalite.com/library-/rrt.htm and as compressed RadBib97.bib.Z from: ftp://hobbes.lbl.gov/pub/doc As always, it is time-consuming and sometimes difficult to track down conference papers and theses on radiosity and global illumination. If you know of a relevant reference that is not included in the bibliography, please let me know so that I can include it in the next release. From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id TAA04407; Thu, 20 Feb 1997 19:10:53 +0100 Received: from sun630.uco.es (el1segag@sun630.uco.es [150.214.110.160]) by imag.imag.fr (8.8.1/8.6.9) with SMTP id SAA18285 for ; Thu, 20 Feb 1997 18:28:04 +0100 (MET) X-quien: el1segag@localhost Received: (from el1segag@localhost) by sun630.uco.es (8.6.12/8.6.12) id SAA14614 for globillum@imag.fr; Thu, 20 Feb 1997 18:25:37 +0100 Date: Thu, 20 Feb 1997 18:25:37 +0100 From: Gonzalo Senuela Garcia Message-Id: <199702201725.SAA14614@sun630.uco.es> To: globillum@imag.fr Subject: Two Pass (Radiosity and raytracing) programs vs Radiance X-UIDL: 03d951bd72d5d358c429f141d9a71471 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Hello Everyone know a paper about a comparative analysis between Two Pass programs (Radiosity-raytracing) and Radiance (Greg Wards) programs - Gonzalo From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id WAA04774; Thu, 20 Feb 1997 22:08:34 +0100 Received: from faui45.informatik.uni-erlangen.de (root@faui45.informatik.uni-erlangen.de [131.188.2.45]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id VAA26928 for ; Thu, 20 Feb 1997 21:45:23 +0100 (MET) Received: from immd9.informatik.uni-erlangen.de (faui90.informatik.uni-erlangen.de [131.188.39.4]) by uni-erlangen.de with SMTP id VAA25356 (8.7.6/7.5c-FAU); for ; Thu, 20 Feb 1997 21:45:12 +0100 (MET) Received: (from slusalle@localhost) by immd9.informatik.uni-erlangen.de id VAA08482 (950413.SGI.8.6.12/7.5b-FAU); for globillum@imag.fr; Thu, 20 Feb 1997 21:45:10 +0100 From: "slusalle@immd9.informatik.uni-erlangen.de" Message-Id: <199702202045.VAA08482@immd9.informatik.uni-erlangen.de> Subject: Eurographics Mailing lists To: globillum@imag.fr Date: Thu, 20 Feb 1997 21:45:10 +0100 (MEZ) X-Mailer: ELM [version 2.4 PL25] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: 6b085daccb2cd345196cc57d716bfb0a X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Dear all, Ivan Herrman from Eurographics asked me to forward the following announcement to this mailinglist: > Dear collegues, > > lately, two mailing lists have been set up by the Eurographics Association > for various announcements. The mailing list called 'members@eg.org' is > reserverd for members of the Association, and will be used for strictly > Association matters (e.g., elections, etc.) The other, larger list, called > 'non-members@eg.org' will be used to announce workshop, conferences, other EG > events. > > Both lists are 'closed', in the sense that only the members of the EG > Executive Committee have the right to post a message onto it. We tried to > avoid an invasion of junk-mails on the mailing list by doing so. > > We would like you to join this mailing lists, thereby making it sure that you > will always receive all announcements in a timely manner in the future. All you > have to do (whether you are a member of EG or not) is to go to the page > > http://www.eg.org/register > > and fill the form there. All the rest will be done automatically. > > Sincerely > > > -- > Ivan Herman > > CWI/IS Kruislaan 413, 1098 SJ Amsterdam, The Netherlands. > Email: Ivan.Herman@cwi.nl Tel: +31-20-592.4163, Fax: +31-20-592 4199 > URL: http://www.cwi.nl/~ivan/ -- Philipp Slusallek Universitaet Erlangen, IMMD IX - Graphische Datenverarbeitung Email: slusallek@informatik.uni-erlangen.de URL: http://www9.informatik.uni-erlangen.de/Persons/Slusallek From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id XAA09769; Fri, 21 Feb 1997 23:32:12 +0100 Received: from internet-mail2.ford.com (internet-mail2.ford.com [198.111.80.24]) by imag.imag.fr (8.8.1/8.6.9) with SMTP id XAA26004 for ; Fri, 21 Feb 1997 23:06:48 +0100 (MET) Received: by internet-mail2.ford.com id AA14559 (InterLock SMTP Gateway 3.0 for globillum@imag.fr); Fri, 21 Feb 1997 17:06:25 -0500 Message-Id: <199702212206.AA14559@internet-mail2.ford.com> Received: by internet-mail2.ford.com (Protected-side Proxy Mail Agent-1); Fri, 21 Feb 1997 17:06:25 -0500 Date: Fri, 21 Feb 1997 17:06:21 -0500 From: Stephen Westin To: holly@watson.ibm.com Cc: globillum@imag.fr In-Reply-To: <8525641A:0051795D.00@watngi01.watson.ibm.com> (holly@watson.ibm.com) Subject: Re: Need refs. about need X-UIDL: 5350ecdfdef7652c62b6f02fa4bed8d5 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit > Hi -- > > One of the people working on the appearance project at NIST asked > me for "some references that talk about the need for measurements > of appearance properties of materials." A lot of people ask about where > to find catalogs of measurements etc., but I am having a hard time > finding "citable" references for the need for measurements. If you > have written anything, either technical paper or more informal > "position" paper that could be cited about the need for measurements > to support realistic rendering please let me know. Or, if you haven't > written anything, but would be willing to be quoted about how your > work would benefit by the availability of measurements, or measurement > techniques, let me know. > > Thanks, > Holly > > Found this dusty message just now; I didn't answer because, frankly, I've never convinced anyone here that better visual simulations, reflectance functions, reflectance measurements, etc, are needed. Sorry. Actually, you might contact someone in the Advanced Lighting Technology Group about this; they have at least played with optical simulations of the down-the-road view at night, and hired ERIM for a while to code something up for them. When I visited (a year ago? two years ago?), they said, "there's this parameter called 'gamma' in the program, and you can make the picture look bright or dark with it. Any idea what it does?" Sigh. I talked to Mahendra Dassanayake (mdassana@ford.com) and Balvant Patel (bpatel6@ford.com). You probably have run into the tendency of numerical simulation analysts to be from India :). -Steve P.S. I'm working on that SIGGRAPH review... From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id MAA06858; Fri, 28 Feb 1997 12:58:16 +0100 Received: from concorde.inria.fr (concorde.inria.fr [192.93.2.39]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id MAA18959 for ; Fri, 28 Feb 1997 12:12:16 +0100 (MET) From: Samuel.Boivin@inria.fr Received: from delhi.inria.fr (delhi.inria.fr [128.93.24.1]) by concorde.inria.fr (8.7.6/8.7.3) with ESMTP id MAA23140; Fri, 28 Feb 1997 12:12:10 +0100 (MET) Received: (from boivin@localhost) by delhi.inria.fr (8.7.6/8.7.3) id MAA02464; Fri, 28 Feb 1997 12:12:09 +0100 (MET) Message-Id: <199702281112.MAA02464@delhi.inria.fr> To: globillum@imag.fr cc: boivin@bora.inria.fr Subject: FORM FACTORS COMPUTATION THROUGH SGI HARDWARE X-Mailer: exmh version 1.5gamma 8/15/94 Date: Fri, 28 Feb 97 12:12:08 +0100 X-UIDL: df6d6ecd9da3fe2714a37c24c03c764a X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Hello everybody, I have some questions that concern Hardware Acceleration for Form Factor Computation. So I tried all what is possible to compute off-screen(and 'on-screen') form factors using OpenGL. The problem is that the computation time I obtained is really BAD ! So does anybody have any information about programming off-screen rendering to EFFECTIVELY accelerate the computation time for form factors using the SGI hardware? You can find next all the solutions I tried: - OpenInventor SoOffScreenRender Class: computation time is incredibly slow: it is unusable. - GLXPixmaps with X11 Pixmaps: the computation time is DRAMATICALLY slow, therefore it is unusable too. 99.99 % computation time is in the GLReadPixels() OpenGL Command (?!?!?) - PBuffers on a Maximum Impact R10000 (195Mhz). The computation time is the following: 15.6sec to compute 300x300 resolution 2000 Z-Buffers with a 70 patches scene (then 140000 projections). For me, it is really unacceptable: MaxImpact has at least a 1.5Million polygons/second rendering capacity with Gouraud shading(there is probably no glReadPixels() call). In any case, I am only using Flat Shading and one light source, and this gives us a 10000 polygon/sec rendering capacity (!?!!): we had better computation time using Mesa Library(14.89 sec) to render this small scene on the same machine ! In my opinion, there are several problem levels: - Does PBuffers really use Hardware ? It doesn't seem to be the case since, using osview, we can see that Hardware lines(gfxc, gfxf...) gives 0.00% (?!?). So, if it doesn't use Hardware, why computation time is faster than using X Pixmaps(as PBuffers are Pixmaps Hardware) ? - There is a SGI paper on using hardware for radiosity: "Real Time Radiosity Through Parallel Processing and Hardware Acceleration", by D.R. Baum and J.M. Winget, Computer Graphics 1990(Symposium on Interactive 3D graphics) p67-75. Page 69: "Once the five hemi-cube are generated(top of hemi-cube and four sides), they are read back from frame buffer memory to host shared memory for processing". This paper is 7 years old and - in spite of the fact they were using multi-processing - they obtained results that I consider impossible to have today on a Maximum Impact R10k 195mhz ! I suspect that it is due to the fact that this technique was performed using GL Library, and we moved to OpenGL that is really slower. To finish with this very long mail: HOW TO USE HARDWARE WITH OFF-SCREEN RENDERING ?!?!? I don't want to open any window ! I just want to use Hardware, compute Z-Buffers(FLAT) and get the result images in real time: is it possible for a Max Impact to compute a 300x300 Z-Buffer of a 400000 patches scene and to get the result image in less than 1 sec ? Samuel. ||======================================|| || Samuel Boivin || ||======================================|| || I.N.R.I.A || || Batiment 24, Projet SYNTIM || || Domaine de Voluceau || || 78153 LE CHESNAY Cedex || || Tel: 01-39-63-51-86 || || Fax: 01-39-63-57-71 || || E-mail: Samuel.Boivin@inria.fr || ||======================================|| From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id PAA07634; Fri, 28 Feb 1997 15:30:46 +0100 Received: from internet-mail2.ford.com (internet-mail2.ford.com [198.111.80.24]) by imag.imag.fr (8.8.1/8.6.9) with SMTP id PAA26359 for ; Fri, 28 Feb 1997 15:00:04 +0100 (MET) Received: by internet-mail2.ford.com id AA00045 (InterLock SMTP Gateway 3.0 for globillum@imag.fr); Fri, 28 Feb 1997 08:59:46 -0500 Message-Id: <199702281359.AA00045@internet-mail2.ford.com> Received: by internet-mail2.ford.com (Protected-side Proxy Mail Agent-1); Fri, 28 Feb 1997 08:59:46 -0500 Date: Fri, 28 Feb 1997 08:59:45 -0500 From: Stephen Westin To: Samuel.Boivin@inria.fr Cc: globillum@imag.fr In-Reply-To: <199702281112.MAA02464@delhi.inria.fr> (Samuel.Boivin@inria.fr) Subject: Re: FORM FACTORS COMPUTATION THROUGH SGI HARDWARE X-UIDL: d7d5127caf1b0dbebf28b86a59ae2c69 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit > - There is a SGI paper on using hardware for radiosity: "Real Time Radiosity > Through Parallel Processing and Hardware Acceleration", by D.R. Baum and J.M. > Winget, Computer Graphics 1990(Symposium on Interactive 3D graphics) p67-75. > Page 69: "Once the five hemi-cube are generated(top of hemi-cube and four > sides), they are read back from frame buffer memory to host shared memory for ^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^ > processing". This paper is 7 years old and - in spite of the fact they were > using multi-processing - they obtained results that I consider impossible to > have today on a Maximum Impact R10k 195mhz ! I suspect that it is due to the > fact that this technique was performed using GL Library, and we moved to > OpenGL that is really slower. No, I suspect that the phrase I highlighted above is the key; SGI machines are generally highly optimized to render to the screen. I would not be at all surprised if off-screen rendering were much slower on most SGI machines. Maybe you are stuck with using the screen, then reading back the frame buffer. I would suggest a post to USENET group comp.sys.sgi.graphics; there are several SGI engineers who hang out there and give you the *real* answer. -Stephen H. Westin swestin@ford.com The information and opinions in this message are mine, not Ford's. From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id QAA07754; Fri, 28 Feb 1997 16:06:03 +0100 Received: from concorde.inria.fr (concorde.inria.fr [192.93.2.39]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id PAA27159 for ; Fri, 28 Feb 1997 15:18:23 +0100 (MET) From: Samuel.Boivin@inria.fr Received: from delhi.inria.fr (delhi.inria.fr [128.93.24.1]) by concorde.inria.fr (8.7.6/8.7.3) with ESMTP id PAA27008 for ; Fri, 28 Feb 1997 15:18:23 +0100 (MET) Received: (from boivin@localhost) by delhi.inria.fr (8.7.6/8.7.3) id PAA02896; Fri, 28 Feb 1997 15:18:20 +0100 (MET) Message-Id: <199702281418.PAA02896@delhi.inria.fr> To: globillum@imag.fr Subject: FORM FACTORS COMPUTATION THROUGH SGI HARDWARE X-Mailer: exmh version 1.5gamma 8/15/94 Date: Fri, 28 Feb 97 15:18:20 +0100 X-UIDL: cda90de9cbc64847d63cdb659a1799a3 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit > No, I suspect that the phrase I highlighted above is the key; SGI > machines are generally highly optimized to render to the screen. I > would not be at all surprised if off-screen rendering were much slower > on most SGI machines. You are right: off-screen rendering is generally slower than "on-screen" rendering(but it depends on the technique you chose). But if you use the glReadPixels() function in your "render to screen" program, then you have quite similar computation time to these obtained with off-screen rendering. > Maybe you are stuck with using the screen, then reading back the frame > buffer. > > I would suggest a post to USENET group comp.sys.sgi.graphics; there > are several SGI engineers who hang out there and give you the *real* > answer. I already sent a message in the OpenGL usenet, and nobody answered me, or just with "did you read the faqs ?" ... So, I will send a message to comp.sys.sgi.graphics too. But I already sent several mails to SGI HOT-LINE in France and USA. They didn't arrive to resolve my problem. In France and in USA, there is still an opened phone-line on my problem(ref FR62888). I am still waiting about a solution. -Samuel From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id QAA07791; Fri, 28 Feb 1997 16:19:48 +0100 Received: from mercury.uniserve.com (mercury.uniserve.com [204.191.197.248]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id PAA27540 for ; Fri, 28 Feb 1997 15:24:45 +0100 (MET) Received: from helios (van0200.tvs.net [204.191.197.40]) by mercury.uniserve.com (8.8.2/8.8.2) with ESMTP id GAA02371; Fri, 28 Feb 1997 06:23:32 -0800 (PST) Message-Id: <199702281423.GAA02371@mercury.uniserve.com> From: "Ian Ashdown" To: Samuel.Boivin@inria.fr Cc: globillum@imag.fr Subject: Re: FORM FACTORS COMPUTATION THROUGH SGI HARDWARE Date: Fri, 28 Feb 1997 06:21:24 -0800 X-MSMail-Priority: Normal X-Priority: 3 X-Mailer: Microsoft Internet Mail 4.70.1155 MIME-Version: 1.0 Content-Type: text/plain; charset=windows-1252; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: f3044fc0104e5fa4ce21bbc16419dcbe X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Samuel Boivin wrote: > I have some questions that concern Hardware Acceleration for Form Factor > Computation. So I tried all what is possible to compute off-screen(and > 'on-screen') form factors using OpenGL. The problem is that the computation > time I obtained is really BAD ! > So does anybody have any information about programming off-screen rendering to > EFFECTIVELY accelerate the computation time for form factors using the SGI > hardware? If you can find a copy of: Rushmeier, H. E., D. R. Baum, and D. E. Hall. 1991. "Aceelerating the Hemi-Cube Algorithm for Calculating Radiation Form Factors," Transactions of the ASME Vol. 113 (November), pp. 1044-1047. you can read about how they achieved speedup factors of up to 6.7 (for a hemicube resolution of 300) on an SGI Personal Iris W-4D20G. Ian Ashdown, P. Eng. Research & Development Manager Ledalite Architectural Products Inc. From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id RAA08080; Fri, 28 Feb 1997 17:20:28 +0100 Received: from ns1.arlut.utexas.edu (ns1.arlut.utexas.edu [129.116.212.1]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id QAA00888 for ; Fri, 28 Feb 1997 16:32:30 +0100 (MET) Received: from mail-firewall.arlut.utexas.edu (ns1.arlut.utexas.edu [129.116.212.1]) by ns1.arlut.utexas.edu (8.7.5/8.7.3) with ESMTP id JAA28242; Fri, 28 Feb 1997 09:30:12 -0600 (CST) Received: from sting.arlut.utexas.edu (sting.arlut.utexas.edu [129.116.128.90]) by mail-firewall.arlut.utexas.edu (8.7.5/8.7.3) with ESMTP id JAA28236; Fri, 28 Feb 1997 09:30:11 -0600 (CST) Received: from sting (localhost [127.0.0.1]) by sting.arlut.utexas.edu (8.8.5/8.7.3) with SMTP id JAA07791; Fri, 28 Feb 1997 09:28:39 -0600 (CST) Sender: atc@arlut.utexas.edu Message-ID: <3316F9A6.2E2C@arlut.utexas.edu> Date: Fri, 28 Feb 1997 09:28:39 -0600 From: "A. T. Campbell" X-Mailer: Mozilla 3.01 (X11; I; HP-UX A.09.07 9000/770) MIME-Version: 1.0 To: Samuel.Boivin@inria.fr CC: globillum@imag.fr Subject: Re: FORM FACTORS COMPUTATION THROUGH SGI HARDWARE References: <199702281423.GAA02371@mercury.uniserve.com> Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: 90453cb58233668aa46b46c304d5bf08 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Another good reference for hardware form factor calculation is the following: Nelson Max and Michael J. Allison, "Linear Radiosity Approximation Using Vertex-to-Vertex Form Factors", Graphics Gems III, edited by David Kirk, Academic Press, 1992. -- A. T. Campbell, III atc@arlut.utexas.edu http://www.arlut.utexas.edu/~atc Applied Research Labs, University of Texas, PO Box 8029, Austin,TX 78713 From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id SAA08350; Fri, 28 Feb 1997 18:38:45 +0100 Received: from relay6.UU.NET (relay6.UU.NET [192.48.96.16]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id SAA05321 for ; Fri, 28 Feb 1997 18:03:54 +0100 (MET) Received: from audrey by relay6.UU.NET with SMTP (peer crosschecked as: Cust111.Max17.San-Francisco.CA.MS.UU.NET [153.35.241.239]) id QQcewi22948; Fri, 28 Feb 1997 12:03:16 -0500 (EST) Sender: crs@uunet.uu.net Message-ID: <33170F00.41C6@nospam.pop.net> Date: Fri, 28 Feb 1997 08:59:44 -0800 From: Chris Schoeneman X-Mailer: Mozilla 2.0S (X11; I; IRIX 6.2 IP22) MIME-Version: 1.0 To: globillum@imag.fr CC: boivin@bora.inria.fr Subject: Re: FORM FACTORS COMPUTATION THROUGH SGI HARDWARE References: <199702281112.MAA02464@delhi.inria.fr> Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: 5bbc8792f8ad90fd6280cbd682be5e2c X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Samuel.Boivin@inria.fr wrote: > > I have some questions that concern Hardware Acceleration for Form Factor > Computation. So I tried all what is possible to compute off-screen(and > 'on-screen') form factors using OpenGL. The problem is that the computation > time I obtained is really BAD ! > > - OpenInventor SoOffScreenRender Class: computation time is incredibly slow: > it is unusable. > > - GLXPixmaps with X11 Pixmaps: the computation time is DRAMATICALLY slow, > therefore it is unusable too. 99.99 % computation time is in the > GLReadPixels() OpenGL Command (?!?!?) Both of these do the same thing (render to pixmaps). They make an indirect rendering context, which sends all OpenGL commands through the X server. As you've discovered, that's slow. But read on to see the real problem. > - PBuffers on a Maximum Impact R10000 (195Mhz). The computation time is > the following: 15.6sec to compute 300x300 resolution 2000 Z-Buffers with a 70 > patches scene (then 140000 projections). For me, it is really unacceptable: > MaxImpact has at least a 1.5Million polygons/second rendering capacity with > Gouraud shading(there is probably no glReadPixels() call). In any case, I > am only using Flat Shading and one light source, and this gives us a 10000 > polygon/sec rendering capacity (!?!!): we had better computation time using > Mesa Library(14.89 sec) to render this small scene on the same machine ! You're not going to get anywhere near the top polygon rendering performance of the Max Impact with a 70 polygon scene. Think about it. You clear the 300x300 buffer, render 70 polygons, then read the pixels. The time it takes to render 70 polygons is miniscule compared to the time it takes to clear and read 90000 pixels. Try rendering 7000 polygons and see what happens to your `polygon' performance. The problem here was your measurement of performance. When you read 1.5M polygons/sec from the marketing brochures it means 1.5M polygons per second, not 1.5M polygons per second including reading and clearing the screen every 70 polygons. Are the marketing numbers misleading? No, they say exactly what they mean. Some suggestions for increasing performance. Use as large a buffer as you can make that's a multiple of 300x300. Clear the entire buffer, render your scene into each 300x300 subregion, then read the entire buffer in one call. That'll amortize the overhead of each clear and pixel read. If you're in a closed environment then every pixel in each 300x300 region will be written to. See the first issue of the Journal of Graphics Tools for a simple technique to avoid the screen clear completely. Make sure you're using a direct rendering context (the last parameter to glXCreateContext should be True). What's the light source for? Turn it off if you don't really need it. In any case, the pixel read will remain the bottleneck. > In my opinion, there are several problem levels: > - Does PBuffers really use Hardware ? Yes, if you use a direct rendering context. > - There is a SGI paper on using hardware for radiosity: "Real Time Radiosity > Through Parallel Processing and Hardware Acceleration", by D.R. Baum and J.M. > Winget, Computer Graphics 1990(Symposium on Interactive 3D graphics) p67-75. > ... I suspect that it is due to the > fact that this technique was performed using GL Library, and we moved to > OpenGL that is really slower. Definitely not. That'd be a brilliant move for SGI, ``with OpenGL get the graphics performance of 5 years ago, TODAY!'' It might well be due to the author's in-depth knowledge of the platform and the bottlenecks in rendering. Cheers, -chris From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id TAA08596; Fri, 28 Feb 1997 19:45:02 +0100 Received: from vivarin.res.cmu.edu (VIVARIN.RES.CMU.EDU [128.2.92.43]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id TAA08330 for ; Fri, 28 Feb 1997 19:16:23 +0100 (MET) Received: from vivarin.res.cmu.edu (localhost [127.0.0.1]) by vivarin.res.cmu.edu (8.8.2/8.6.9) with ESMTP id NAA02000 for ; Fri, 28 Feb 1997 13:14:50 -0500 Message-Id: <199702281814.NAA02000@vivarin.res.cmu.edu> Reply-To: Michael Herf To: globillum@imag.fr Subject: Re: FORM FACTORS COMPUTATION THROUGH SGI HARDWARE In-reply-to: Your message of Fri, 28 Feb 1997 06:21:24 PST. Date: Fri, 28 Feb 1997 13:14:50 -0500 From: Michael Herf X-UIDL: 1a716b621ce17c703d05a854e3fa99b3 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Pixmap rendering is all done in software, so it should be slow. I imagine the Inventor class uses Pixmaps. pBuffers are the way to go on a RE, but on an Impact I wouldn't be surprised if they were in software. I don't think the framebuffer on the Impact has many spare bits. The backbuffer should be a good option in double-buffered mode on any SGI hardware, though some machines will draw in dithered 16-bit mode, so be careful about how much you trust that. glReadPixels always goes through host memory, so you're bound by the memory bandwidth there. I think the Impact gives you a generous 200 MB/sec, but even so it's not pretty. For an Impact, drawing 70 polygons is trivial, so you can consider your test a benchmark of glReadPixels. In answer to your question: you can certainly create a 300x300 image of a 400,000-patch scene in a backbuffer in < 1 second on this hardware. At this point you won't be depending on host memory for your throughput, and the hardware will be able to scream through rendering polygons. Again, maybe pbuffers will work in single-buffered mode on the Impact, but I don't know about this. In the broader scope, I think that hemicube radiosity really presents some architectural problems for all but the latest of graphics hardware. There's a huge overhead for using the bus between the hardware and the host CPU, but the constant "ping-ponging" back and forth means that efficient systems are hard to build. The newer SGI machines (O2 and Onyx2) have UMA (unified memory architecture), so the bus is not nearly as much of a bottleneck. As a point of reference, can someone post some empirical speed results from ray-casting (using appropriate subdivision) into "typical" scenes of a variety of sizes? I imagine that at the 70-patch level, software would be faster, and at the 400,000-patch level, hardware would win. But an approximate intersection point would be nice to have. mike From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id AAA09376; Sat, 1 Mar 1997 00:27:55 +0100 Received: from sgi.sgi.com (SGI.COM [192.48.153.1]) by imag.imag.fr (8.8.1/8.6.9) with SMTP id AAA18451 for ; Sat, 1 Mar 1997 00:16:44 +0100 (MET) Received: from odin.corp.sgi.com (odin.corp.sgi.com [192.26.51.194]) by sgi.sgi.com (950413.SGI.8.6.12/950213.SGI.AUTOCF) via ESMTP id PAA07656; Fri, 28 Feb 1997 15:16:10 -0800 Received: from palladium.corp.sgi.com by odin.corp.sgi.com via ESMTP (951211.SGI.8.6.12.PATCH1502/951211.SGI) id PAA18619; Fri, 28 Feb 1997 15:16:09 -0800 Received: from giraffe.asd.sgi.com by palladium.corp.sgi.com via ESMTP (951211.SGI.8.6.12.PATCH1502/911001.SGI) id LAA08013; Fri, 28 Feb 1997 11:53:55 -0800 Received: from studmuffin.asd.sgi.com by giraffe.asd.sgi.com via ESMTP (951211.SGI.8.6.12.PATCH1502/951211.SGI) id LAA20990; Fri, 28 Feb 1997 11:53:41 -0800 Received: by studmuffin.asd.sgi.com (950413.SGI.8.6.12/940406.SGI.AUTO) id LAA06166; Fri, 28 Feb 1997 11:53:41 -0800 From: "Dan Baum" Message-Id: <9702281153.ZM6164@studmuffin.asd.sgi.com> Date: Fri, 28 Feb 1997 11:53:41 -0800 In-Reply-To: Samuel.Boivin@inria.fr "FORM FACTORS COMPUTATION THROUGH SGI HARDWARE" (Feb 28, 3:18pm) References: <199702281418.PAA02896@delhi.inria.fr> X-Mailer: Z-Mail (3.2.3 08feb96 MediaMail) To: Samuel.Boivin@inria.fr, globillum@imag.fr Subject: Re: FORM FACTORS COMPUTATION THROUGH SGI HARDWARE Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed X-UIDL: 023fe17784fcca449b485c0f7b2070b4 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit FYI, I've sent email to Samuel saying that I would help him out. I did the original work on hardware FF acceleration about 8 years ago. He actually had sent me email about a month ago, but I had mistakenly deleted it before responding. On Feb 28, 3:18pm, Samuel.Boivin@inria.fr wrote: > Subject: FORM FACTORS COMPUTATION THROUGH SGI HARDWARE > > No, I suspect that the phrase I highlighted above is the key; SGI > > machines are generally highly optimized to render to the screen. I > > would not be at all surprised if off-screen rendering were much slower > > on most SGI machines. > You are right: off-screen rendering is generally slower than "on-screen" > rendering(but it depends on the technique you chose). > But if you use the glReadPixels() function in your "render to screen" program, > then you have quite similar computation time to these obtained with off-screen > rendering. > > > > Maybe you are stuck with using the screen, then reading back the frame > > buffer. > > > > I would suggest a post to USENET group comp.sys.sgi.graphics; there > > are several SGI engineers who hang out there and give you the *real* > > answer. > > I already sent a message in the OpenGL usenet, and nobody answered me, or just > with "did you read the faqs ?" ... > So, I will send a message to comp.sys.sgi.graphics too. But I already sent > several mails to SGI HOT-LINE in France and USA. They didn't arrive to resolve > my problem. In France and in USA, there is still an opened phone-line on my > problem(ref FR62888). I am still waiting about a solution. > > -Samuel > >-- End of excerpt from Samuel.Boivin@inria.fr From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id VAA08866; Fri, 28 Feb 1997 21:17:45 +0100 Received: from deliverator.sgi.com (deliverator.sgi.com [204.94.214.10]) by imag.imag.fr (8.8.1/8.6.9) with SMTP id UAA12034 for ; Fri, 28 Feb 1997 20:58:01 +0100 (MET) Received: from odin.corp.sgi.com by deliverator.sgi.com via ESMTP (950413.SGI.8.6.12/951211.SGI.AUTO) id LAA08640; Fri, 28 Feb 1997 11:57:47 -0800 Received: from giraffe.asd.sgi.com by odin.corp.sgi.com via ESMTP (951211.SGI.8.6.12.PATCH1502/951211.SGI) id LAA07069; Fri, 28 Feb 1997 11:57:47 -0800 Received: from studmuffin.asd.sgi.com by giraffe.asd.sgi.com via ESMTP (951211.SGI.8.6.12.PATCH1502/951211.SGI) id LAA21221; Fri, 28 Feb 1997 11:57:31 -0800 Received: by studmuffin.asd.sgi.com (950413.SGI.8.6.12/940406.SGI.AUTO) id LAA06171; Fri, 28 Feb 1997 11:57:31 -0800 From: "Dan Baum" Message-Id: <9702281157.ZM6169@studmuffin.asd.sgi.com> Date: Fri, 28 Feb 1997 11:57:31 -0800 In-Reply-To: Chris Schoeneman "Re: FORM FACTORS COMPUTATION THROUGH SGI HARDWARE" (Feb 28, 8:59am) References: <199702281112.MAA02464@delhi.inria.fr> <33170F00.41C6@nospam.pop.net> X-Mailer: Z-Mail (3.2.3 08feb96 MediaMail) To: Chris Schoeneman , globillum@imag.fr Subject: Re: FORM FACTORS COMPUTATION THROUGH SGI HARDWARE Cc: boivin@bora.inria.fr Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed X-UIDL: 8ca9809afc336363eaef55b16add1920 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Chris has made some excellent suggestions below. Additionally, if you overlap the remainder of the host based form-factor computation with the hemicube visiblity calculations you are performing on the hardware you will see additional time savings. On Feb 28, 8:59am, Chris Schoeneman wrote: > Subject: Re: FORM FACTORS COMPUTATION THROUGH SGI HARDWARE > Samuel.Boivin@inria.fr wrote: > > > > I have some questions that concern Hardware Acceleration for Form Factor > > Computation. So I tried all what is possible to compute off-screen(and > > 'on-screen') form factors using OpenGL. The problem is that the computation > > time I obtained is really BAD ! > > > > - OpenInventor SoOffScreenRender Class: computation time is incredibly slow: > > it is unusable. > > > > - GLXPixmaps with X11 Pixmaps: the computation time is DRAMATICALLY slow, > > therefore it is unusable too. 99.99 % computation time is in the > > GLReadPixels() OpenGL Command (?!?!?) > > Both of these do the same thing (render to pixmaps). They make an indirect > rendering context, which sends all OpenGL commands through the X server. > As you've discovered, that's slow. But read on to see the real problem. > > > - PBuffers on a Maximum Impact R10000 (195Mhz). The computation time is > > the following: 15.6sec to compute 300x300 resolution 2000 Z-Buffers with a 70 > > patches scene (then 140000 projections). For me, it is really unacceptable: > > MaxImpact has at least a 1.5Million polygons/second rendering capacity with > > Gouraud shading(there is probably no glReadPixels() call). In any case, I > > am only using Flat Shading and one light source, and this gives us a 10000 > > polygon/sec rendering capacity (!?!!): we had better computation time using > > Mesa Library(14.89 sec) to render this small scene on the same machine ! > > You're not going to get anywhere near the top polygon rendering > performance of the Max Impact with a 70 polygon scene. Think about it. > You clear the 300x300 buffer, render 70 polygons, then read the pixels. > The time it takes to render 70 polygons is miniscule compared to the time > it takes to clear and read 90000 pixels. Try rendering 7000 polygons and > see what happens to your `polygon' performance. > > The problem here was your measurement of performance. When you read 1.5M > polygons/sec from the marketing brochures it means 1.5M polygons per > second, not 1.5M polygons per second including reading and clearing the > screen every 70 polygons. Are the marketing numbers misleading? No, > they say exactly what they mean. > > Some suggestions for increasing performance. Use as large a buffer as > you can make that's a multiple of 300x300. Clear the entire buffer, > render your scene into each 300x300 subregion, then read the entire buffer > in one call. That'll amortize the overhead of each clear and pixel read. > > If you're in a closed environment then every pixel in each 300x300 region > will be written to. See the first issue of the Journal of Graphics Tools > for a simple technique to avoid the screen clear completely. > > Make sure you're using a direct rendering context (the last parameter to > glXCreateContext should be True). > > What's the light source for? Turn it off if you don't really need it. > > In any case, the pixel read will remain the bottleneck. > > > > In my opinion, there are several problem levels: > > - Does PBuffers really use Hardware ? > > Yes, if you use a direct rendering context. > > > > - There is a SGI paper on using hardware for radiosity: "Real Time Radiosity > > Through Parallel Processing and Hardware Acceleration", by D.R. Baum and J.M. > > Winget, Computer Graphics 1990(Symposium on Interactive 3D graphics) p67-75. > > ... I suspect that it is due to the > > fact that this technique was performed using GL Library, and we moved to > > OpenGL that is really slower. > > Definitely not. That'd be a brilliant move for SGI, ``with OpenGL get the > graphics performance of 5 years ago, TODAY!'' It might well be due to the > author's in-depth knowledge of the platform and the bottlenecks in rendering. > > Cheers, > -chris > >-- End of excerpt from Chris Schoeneman From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id VAA08906; Fri, 28 Feb 1997 21:29:10 +0100 Received: from sgi.sgi.com (SGI.COM [192.48.153.1]) by imag.imag.fr (8.8.1/8.6.9) with SMTP id VAA12634 for ; Fri, 28 Feb 1997 21:16:14 +0100 (MET) Received: from odin.corp.sgi.com (odin.corp.sgi.com [192.26.51.194]) by sgi.sgi.com (950413.SGI.8.6.12/950213.SGI.AUTOCF) via ESMTP id MAA17408; Fri, 28 Feb 1997 12:15:20 -0800 Received: from giraffe.asd.sgi.com by odin.corp.sgi.com via ESMTP (951211.SGI.8.6.12.PATCH1502/951211.SGI) id MAA10148; Fri, 28 Feb 1997 12:15:14 -0800 Received: from studmuffin.asd.sgi.com by giraffe.asd.sgi.com via ESMTP (951211.SGI.8.6.12.PATCH1502/951211.SGI) id MAA22250; Fri, 28 Feb 1997 12:15:00 -0800 Received: by studmuffin.asd.sgi.com (950413.SGI.8.6.12/940406.SGI.AUTO) id MAA06226; Fri, 28 Feb 1997 12:15:00 -0800 From: "Dan Baum" Message-Id: <9702281214.ZM6224@studmuffin.asd.sgi.com> Date: Fri, 28 Feb 1997 12:14:59 -0800 In-Reply-To: Michael Herf "Re: FORM FACTORS COMPUTATION THROUGH SGI HARDWARE" (Feb 28, 1:14pm) References: <199702281814.NAA02000@vivarin.res.cmu.edu> X-Mailer: Z-Mail (3.2.3 08feb96 MediaMail) To: Michael Herf , globillum@imag.fr Subject: Re: FORM FACTORS COMPUTATION THROUGH SGI HARDWARE Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed X-UIDL: 3683cc8522fed50dbfc3137f20715ebd X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit > > In the broader scope, I think that hemicube radiosity really presents some > architectural problems for all but the latest of graphics hardware. > There's a huge overhead for using the bus between the hardware and the > host CPU, but the constant "ping-ponging" back and forth means that > efficient systems are hard to build. The newer SGI machines (O2 and > Onyx2) have UMA (unified memory architecture), so the bus is not > nearly as much of a bottleneck. A couple of comments on the above. First, with a scene of interesting complexity (minimum of several thousand polys rendered 5 times for each face of the cube), read back overhead shouldn't be that bad. Again,if you've got an MP machine think about overlapping your computations. Also, the Onyx2 is not what I would call a UMA architecture. We officially term is as SSMP, but you might want to think of it as NUMA (non-uniform memory access) in that there isn't a common system bus inbetween CPU and main memory. Main memory is distributed throughout the system with different access times depending on the location of memory. Obviously, the system tries to be intelligent to keep your data as close to the processor that operating on it. > > As a point of reference, can someone post some empirical speed results > from ray-casting (using appropriate subdivision) into "typical" scenes of > a variety of sizes? I imagine that at the 70-patch level, software would > be faster, and at the 400,000-patch level, hardware would win. But an > approximate intersection point would be nice to have. > > mike >-- End of excerpt from Michael Herf From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id UAA23235; Mon, 3 Mar 1997 20:19:12 +0100 Received: from concorde.inria.fr (concorde.inria.fr [192.93.2.39]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id MAA26967 for ; Mon, 3 Mar 1997 12:00:20 +0100 (MET) From: Samuel.Boivin@inria.fr Received: from delhi.inria.fr (delhi.inria.fr [128.93.24.1]) by concorde.inria.fr (8.7.6/8.7.3) with ESMTP id MAA24126; Mon, 3 Mar 1997 12:00:18 +0100 (MET) Received: (from boivin@localhost) by delhi.inria.fr (8.7.6/8.7.3) id MAA06576; Mon, 3 Mar 1997 12:00:16 +0100 (MET) Message-Id: <199703031100.MAA06576@delhi.inria.fr> To: globillum@imag.fr cc: boivin@bora.inria.fr Subject: Re: FORM FACTORS COMPUTATION THROUGH SGI HARDWARE In-reply-to: Your message of "Fri, 28 Feb 97 08:59:44 PST." <33170F00.41C6@nospam.pop.net> X-Mailer: exmh version 1.5gamma 8/15/94 Date: Mon, 03 Mar 97 12:00:16 +0100 X-UIDL: df9123e1fe3f713294166c8ff150f8aa X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Chris Schoeneman wrote: > Both of these do the same thing (render to pixmaps). They make an indirect > rendering context, which sends all OpenGL commands through the X server. > As you've discovered, that's slow. But read on to see the real problem. You are right, but I knew that. So, it's my fault, I fear that I haven't been clear about my real problem. In fact, I spent several weeks to try each method about off-screen rendering and I spent several hours with SGI Hot-Line to understand the reasons of the bad performances I obtained. In fact, in my opinion, for GLXPixmaps, there is nothing to do, because of the same reasons you invoked. For Pbuffers(the last solution ?), I have the sensation it could be a good solution if you have a Infinite Reality or a Reality Monster. On a Maximum Impact, it is too slow. Maybe there is another idea: isn't it possible to put a (ubyte *) pointer to the memory area where pixels are stored ? I think It would be really faster than using glReadPixels() function, no ? > You're not going to get anywhere near the top polygon rendering > performance of the Max Impact with a 70 polygon scene. Think about it. > You clear the 300x300 buffer, render 70 polygons, then read the pixels. > The time it takes to render 70 polygons is miniscule compared to the time > it takes to clear and read 90000 pixels. Try rendering 7000 polygons and > see what happens to your `polygon' performance. Again, you are right. But if I have a 7000 polygon scene, I will approximately read 35000 buffers to compute form factors, then I think it will be really slow, since it takes a lot of time to do a single "glReadPixels()" call. > The problem here was your measurement of performance. When you read 1.5M > polygons/sec from the marketing brochures it means 1.5M polygons per > second, not 1.5M polygons per second including reading and clearing the > screen every 70 polygons. Are the marketing numbers misleading? No, > they say exactly what they mean. You are right again and that's what I said in my previous mail: ther is no read buffer in their performance measurements. But, 1.5 Million polygon per second doesn't mean anything for me. Indeed, when we read their performance announcements, you can't find: Buffer resolution(50x50 or 1000x1000 ?), percentage of bitmap occupation(10% or 90% ?), and -and it is really important- polygons configuration (I mean if they project the scene in a special order(sorted polygons), they can really accelerate the computation time). But that is not the real problem here. So if the numbers are not really exact, I don't think they are completely false. What I really would like to know is: what is done in glReadPixels() ? If you read the OpenGL Faqs, you can see that disabling fog, texture... accelerate the reading command execution ! WHY ?!?! For me reading the frame buffer is only a problem of getting memory address ! It has been stored somewhere, and I only what to get a pointer on this memory area ! There is nothing to compute ! > Some suggestions for increasing performance. Use as large a buffer as > you can make that's a multiple of 300x300. Clear the entire buffer, > render your scene into each 300x300 subregion, then read the entire buffer > in one call. That'll amortize the overhead of each clear and pixel read. > If you're in a closed environment then every pixel in each 300x300 region > will be written to. See the first issue of the Journal of Graphics Tools > for a simple technique to avoid the screen clear completely. OK, thank you for the information. I will apply this idea. > Make sure you're using a direct rendering context (the last parameter to > glXCreateContext should be True). Sure it is ! Otherwise, I can't use Hardware. > What's the light source for? Turn it off if you don't really need it. Sorry, I made a mistake. I didn't define any light source. And they are disabled before reading the buffer because it seems to accelerate the reading command !?!?! > Yes, if you use a direct rendering context. Sorry, I can't be agree. It is not the case on a Maximum Impact: I made a lot of tests, and each time the graphics card is not sollicited. And if you ask to SGI, they say you that Pbuffers uses Hardware on high/max Impact, RE2, IR and O2. So, I sent my code to SGI, and they try it on Maximum Impact and O2, and they saw that there is no Hardware use ! So they open a phone-line(FR-62888) about that problem... I am still waiting for an answer. > Definitely not. That'd be a brilliant move for SGI, ``with OpenGL get the > graphics performance of 5 years ago, TODAY!'' It might well be due to the > author's in-depth knowledge of the platform and the bottlenecks in rendering. Maybe. But, if you make some tests with pure GL read command and if you compare it to the same OpenGL command, you obtain very big differences ! The GL read command is several times faster than the OpenGL one !! -Samuel From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id VAA23498; Mon, 3 Mar 1997 21:43:19 +0100 Received: from vivarin.res.cmu.edu (VIVARIN.RES.CMU.EDU [128.2.92.43]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id VAA00038 for ; Mon, 3 Mar 1997 21:22:41 +0100 (MET) Received: from vivarin.res.cmu.edu (localhost [127.0.0.1]) by vivarin.res.cmu.edu (8.8.2/8.6.9) with ESMTP id PAA19842 for ; Mon, 3 Mar 1997 15:20:47 -0500 Message-Id: <199703032020.PAA19842@vivarin.res.cmu.edu> To: globillum@imag.fr Subject: Re: FORM FACTORS COMPUTATION THROUGH SGI HARDWARE Reply-To: Michael Herf Date: Mon, 03 Mar 1997 15:20:47 -0500 From: Michael Herf X-UIDL: af8d3da656fdf019d88f12ec073ffa1a X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit First, there is no such thing as a memory-mapped framebuffer on an SGI. This is part of the design spec. Everything is done through library calls, so when you call glReadPixels() the framebuffer is copied into a buffer in your program's address space. So you can't just assign a pointer and read. However, you should be able to get better rates on glReadPixels. I think that on the machines you're using GL_RGB (GL_ABGR_EXT on older machines) with GL_UNSIGNED_BYTE is a fast path. If, instead of bytes, you're reading into floats, the conversion is likely done in software, and you'll pay very dearly for it. Using these parameters, you should get speed equivalent to the IRIS-GL command. Try doing repeated glReadPixels from an on-screen region, using the same call you are using now. Measure the throughput in MB/sec. On the worst of SGI machines, I think you should get better than ~30 MB/sec. It's probably much better on the machines you're talking about. I would guess that your system profile isn't indicating the drawing time, since it's so little work for the hardware. As I remember, glReadPixels will show up as "user time" in gr_osview. mike From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id VAA23529; Mon, 3 Mar 1997 21:53:13 +0100 Received: from internet-mail2.ford.com (internet-mail2.ford.com [198.111.80.24]) by imag.imag.fr (8.8.1/8.6.9) with SMTP id VAA00069 for ; Mon, 3 Mar 1997 21:24:41 +0100 (MET) Received: by internet-mail2.ford.com id AA27240 (InterLock SMTP Gateway 3.0 for globillum@imag.fr); Mon, 3 Mar 1997 15:24:27 -0500 Message-Id: <199703032024.AA27240@internet-mail2.ford.com> Received: by internet-mail2.ford.com (Protected-side Proxy Mail Agent-1); Mon, 3 Mar 1997 15:24:27 -0500 Date: Mon, 3 Mar 1997 15:24:26 -0500 From: Stephen Westin To: Samuel.Boivin@inria.fr Cc: globillum@imag.fr In-Reply-To: <199703031100.MAA06576@delhi.inria.fr> (Samuel.Boivin@inria.fr) Subject: Re: FORM FACTORS COMPUTATION THROUGH SGI HARDWARE X-UIDL: efe69ebde3ed0c8c9ff7522e2413b87a X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Samuel Boivin wrote: > Chris Schoeneman wrote: > > Definitely not. That'd be a brilliant move for SGI, ``with OpenGL get the > > graphics performance of 5 years ago, TODAY!'' It might well be due to the > > author's in-depth knowledge of the platform and the bottlenecks in rendering. > > Maybe. But, if you make some tests with pure GL read command and if you > compare it to the same OpenGL command, you obtain very big differences ! The > GL read command is several times faster than the OpenGL one !! Just a minute here. What pixel format are you using in the readback? If you're reading pixels that must be repacked after reading from the frame buffer, there will be sicgnificant overhead. I suspect that defaults may well be different from IRIS/GL and OpenGL. I also would expect that the optimum pixel format would vary with hardware type. Generally, OpenGL should run faster than IRIS/GL on the Impact series, as that's its native mode. Older graphics adapters, like IMPACT, would probably be faster with IRIS/GL. I think posting the kernel of your readback code would be useful; I bet Chris can help speed it up. -Stephen H. Westin swestin@ford.com The information and opinions in this message are mine, not Ford's. From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id XAA23845; Mon, 3 Mar 1997 23:44:18 +0100 Received: from sgi.sgi.com (SGI.COM [192.48.153.1]) by imag.imag.fr (8.8.1/8.6.9) with SMTP id XAA04243 for ; Mon, 3 Mar 1997 23:17:15 +0100 (MET) Received: from odin.corp.sgi.com (odin.corp.sgi.com [192.26.51.194]) by sgi.sgi.com (950413.SGI.8.6.12/950213.SGI.AUTOCF) via ESMTP id OAA27927; Mon, 3 Mar 1997 14:16:41 -0800 Received: from giraffe.asd.sgi.com by odin.corp.sgi.com via ESMTP (951211.SGI.8.6.12.PATCH1502/951211.SGI) id OAA07645; Mon, 3 Mar 1997 14:16:38 -0800 Received: from studmuffin.asd.sgi.com by giraffe.asd.sgi.com via ESMTP (951211.SGI.8.6.12.PATCH1502/951211.SGI) id OAA00819; Mon, 3 Mar 1997 14:15:30 -0800 Received: by studmuffin.asd.sgi.com (950413.SGI.8.6.12/940406.SGI.AUTO) id OAA09641; Mon, 3 Mar 1997 14:15:29 -0800 From: "Dan Baum" Message-Id: <9703031415.ZM9639@studmuffin.asd.sgi.com> Date: Mon, 3 Mar 1997 14:15:29 -0800 In-Reply-To: Samuel.Boivin@inria.fr "Re: FORM FACTORS COMPUTATION THROUGH SGI HARDWARE" (Mar 3, 12:00pm) References: <199703031100.MAA06576@delhi.inria.fr> X-Mailer: Z-Mail (3.2.3 08feb96 MediaMail) To: Samuel.Boivin@inria.fr, globillum@imag.fr Subject: Re: FORM FACTORS COMPUTATION THROUGH SGI HARDWARE Cc: boivin@bora.inria.fr Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed X-UIDL: 8300dd2080e2f35820bbc188c4e3c2d2 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hi Samuel: As has been pointed out by others, there is no way to access the framebuffer directly. It must be copied back using glReadPixels. Now the performance for glReadPixels depends on the machine you are running on and the amount of data you are reading back. There is overhead to setup the read transfer regardless of the number of pixels you are going to read back. So, to get maximum performance you have to treat this as a systems problem and tune to get maximum performance for your system. For example, try rendering several hemi-cubes into the framebuffer and then read them all back with a single glReadPixels(). On a Max Impact, glReadPixels() should be just as fast as IrisGL based pixel read unless you are using some odd conversion (I would assume you are reading the hemi-cube pixels back as unsigned integers). BTW, I'm not nearly as familiar with the Impact architecture and performance characteristics as I am with our high end machines. From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id SAA29753; Tue, 4 Mar 1997 18:04:39 +0100 Received: from sgi.sgi.com (SGI.COM [192.48.153.1]) by imag.imag.fr (8.8.1/8.6.9) with SMTP id RAA19822 for ; Tue, 4 Mar 1997 17:06:44 +0100 (MET) Received: from avalon.manchester.sgi.com ([144.253.96.20]) by sgi.sgi.com (950413.SGI.8.6.12/950213.SGI.AUTOCF) via ESMTP id IAA13026; Tue, 4 Mar 1997 08:06:05 -0800 Received: by avalon.manchester.sgi.com (950413.SGI.8.6.12/911001.SGI) id PAA08044; Tue, 4 Mar 1997 15:54:52 GMT From: "Chris Thornborrow" Message-Id: <9703041554.ZM8042@avalon.manchester.sgi.com> Date: Tue, 4 Mar 1997 15:54:52 +0000 In-Reply-To: Michael Herf "Re: FORM FACTORS COMPUTATION THROUGH SGI HARDWARE" (Mar 3, 3:20pm) References: <199703032020.PAA19842@vivarin.res.cmu.edu> X-Mailer: Z-Mail (3.2.3 08feb96 MediaMail) To: Michael Herf , globillum@imag.fr Subject: Re: FORM FACTORS COMPUTATION THROUGH SGI HARDWARE Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed X-UIDL: 7bcdfc3bd7c6a8640b4fc38bf9d5d601 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit On Mar 3, 3:20pm, Michael Herf wrote: > Subject: Re: FORM FACTORS COMPUTATION THROUGH SGI HARDWARE > First, there is no such thing as a memory-mapped framebuffer on an SGI. > This is part of the design spec. Everything is done through library > calls, so when you call glReadPixels() the framebuffer is copied into a > buffer in your program's address space. So you can't just assign a > pointer and read. Well yes and no. The O2 does have a memory mapped frame buffer in one sense - the obvious sense :-). So technically it is possible to look into memory and see whats on the screen using a pointer and some jiggery pokery. Its the second part that worries me. I believe the exact way in which the frame buffer is organised in memory is documented *but* the documentation says that SGI reserve the right to alter it at any time. Therefore the only safe way to code is to do as suggested above and access through digital media libraries or opengl. You could peek and poke memory, I wouldn't advise it. However, this is irrelevant as the speed of reading the framebuffer is very fast through opengl as all that is really going on is a memcopy. Chris. -- ------------------------------------------------------------------------------- |Chris Thornborrow email : chris@manchester.sgi.com | |Silicon Graphics tel : +44 161 877 8801 ext 1309 | | | |Home Page URL : http://reality.sgi.com/chris_manchester/ | |Arthurian URL : http://reality.sgi.com/chris_manchester/arthur.html | ------------------------------------------------------------------------------- From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id SAA29767; Tue, 4 Mar 1997 18:07:10 +0100 Received: from sgi.sgi.com (SGI.COM [192.48.153.1]) by imag.imag.fr (8.8.1/8.6.9) with SMTP id RAA20421 for ; Tue, 4 Mar 1997 17:14:19 +0100 (MET) Received: from avalon.manchester.sgi.com ([144.253.96.20]) by sgi.sgi.com (950413.SGI.8.6.12/950213.SGI.AUTOCF) via ESMTP id IAA15099 for <@sgi.com:globillum@imag.fr>; Tue, 4 Mar 1997 08:13:55 -0800 Received: by avalon.manchester.sgi.com (950413.SGI.8.6.12/911001.SGI) for globillum@imag.fr id QAA08055; Tue, 4 Mar 1997 16:02:46 GMT From: "Chris Thornborrow" Message-Id: <9703041602.ZM8053@avalon.manchester.sgi.com> Date: Tue, 4 Mar 1997 16:02:45 +0000 In-Reply-To: swestin@ford.com (Stephen Westin ) "Re: FORM FACTORS COMPUTATION THROUGH SGI HARDWARE" (Mar 3, 3:24pm) References: <199703032024.AA27240@internet-mail2.ford.com> X-Mailer: Z-Mail (3.2.3 08feb96 MediaMail) To: globillum@imag.fr Subject: Re: FORM FACTORS COMPUTATION THROUGH SGI HARDWARE Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed X-UIDL: 1148c357a98fdaa74691bb0f87e0517b X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit > > Maybe. But, if you make some tests with pure GL read command and if you > > compare it to the same OpenGL command, you obtain very big differences ! The > > GL read command is several times faster than the OpenGL one !! This is one of the commonest complaints (usually its a complaint about the speed of writing pixels) when moving from GL to OpenGL. It is also a misconception. OpenGL has far more state information relating to pixel data and formats than GL had. The problem is that most people don't set the correct values for the operation they wish to perform. In OpenGL this will result in poor performance. I just looked for my piece of code to demonstrate this but its mysteriously vanished :-(. The one caveat is if you are running on old hardware some commands are faster in GL than OpenGL. Chris. -- ------------------------------------------------------------------------------- |Chris Thornborrow email : chris@manchester.sgi.com | |Silicon Graphics tel : +44 161 877 8801 ext 1309 | | | |Home Page URL : http://reality.sgi.com/chris_manchester/ | |Arthurian URL : http://reality.sgi.com/chris_manchester/arthur.html | ------------------------------------------------------------------------------- From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id WAA07773; Sat, 15 Mar 1997 22:48:54 +0100 Received: from merckx.graphics.cornell.edu (MERCKX.GRAPHICS.CORNELL.EDU [128.84.247.147]) by imag.imag.fr (8.8.1/8.6.9) with SMTP id WAA18260 for ; Sat, 15 Mar 1997 22:33:42 +0100 (MET) Received: by merckx.graphics.cornell.edu (5.65/DEC-Ultrix/4.3) id AA16577; Sat, 15 Mar 1997 16:33:41 -0500 Message-Id: <9703152133.AA16577@merckx.graphics.cornell.edu> Received: by phoenix.graphics.cornell.edu (1.37.109.8/16.2) id AA11022; Sat, 15 Mar 1997 16:33:41 -0500 From: Bruce Walter Subject: Terminology question To: globillum@imag.fr Date: Sat, 15 Mar 1997 16:33:40 -0500 (EST) X-Mailer: ELM [version 2.4 PL25] Mime-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: f2424c33af6cac578a33740fa633ab87 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Dear Globillum'ers, I've recently run into a seemingly difficult terminology question about what to call the quantities that we actually compute or attempt to compute in global illumination. We often refer to our results as radiance or radiant exitance, but what we actually compute and store does not correspond the definitions of these terms as given the IES/ANSI standard for illuminating engineering terminology. That terminology seems to fall into three categories: spectral radiometry, radiometry, and photometry. Spectral radiometric functions (e.g. spectral radiance) give the amount of light as a function of wavelength. They contain the most information and the others are derived from them by various wavelength weighting functions. Radiometric functions (e.g. radiance) weight power at all wavelengths equally and thus measure total power. Photometric functions (e.g. luminance) weight the light power by the human luminance response curve and measure human grayscale response. Radiometric functions are fine for heat transfer applications that are concerned about the flow of heat energy. Photometric functions are fine for grayscale image making. However as far as I can tell, there doesn't seem to be any standard terminology for the quantities needed to make color images. The usual standard for color response is the CIE 1931 Standard Colormetric Observer which defines colors by three values, XYZ which can be found by using three standard wavelength weighting functions. We compute a color image by weighting the spectral radiance by these three response functions. The Y response curve is the luminous response curve and thus is luminance. However there doesn't seem to be a name for X and Z channel results. Together the XYZ values are sometimes refered to as the tristimulus values, so it would seem correct to call our results the "tristimulus values of the spectral radiance". However that seems rather cumbersome, and it would be nicer to have a name for quantities which we actually compute and store. I'd like to propose a new set of terminology for "color photometry". Analogous to radiometry and photometry, it would give names for the spectral radiometric functions when weighted by the CIE XYZ response curves. The proposed corresponding terms are: Radiometry Photometry Color Photometry --------------------------------------------------------- radiance luminance tristimulance irradiance illuminance intristimulance radiant exitance luminous exitance tristimulus exitance I'd like to hear people's reactions. Do names for these quantities already exist? Are there better names? Do we need names for these quantities? It seems a little sloppy to keep refering to our results as the radiance when at best we really mean the spectral radiance and in practice we really mean what I'm calling the tristimulance. Bruce Walter Cornell Program of Computer Graphics p.s. Tristimulus values do not necessarily refer to the CIE 1931 XYZ values. It is also used in the literature to refer to values generated by other three channel color models. So we would need to be careful to specify which color model we are using when we want to be precise. p.p.s. I wanted to call it the chrominance, but this term is already in use and often means the portion of the color which is "orthogonal" to the luminance. Using tristimulance instead avoids this confusion. From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id UAA04869; Wed, 19 Mar 1997 20:02:33 +0100 Received: from irz201.inf.tu-dresden.de (irz201.inf.tu-dresden.de [141.76.1.10]) by imag.imag.fr (8.8.1/8.6.9) with SMTP id SAA29464 for ; Wed, 19 Mar 1997 18:23:59 +0100 (MET) Received: (from cn1@localhost) by irz201.inf.tu-dresden.de (8.6.12/8.6.12-s1) id TAA02485 for globillum@imag.fr; Wed, 19 Mar 1997 19:23:58 +0200 From: "Nguyen, D.C." Message-Id: <199703191723.TAA02485@irz201.inf.tu-dresden.de> Subject: paper for coherence-based RT-accel. methods To: Global Illumination List Date: Wed, 19 Mar 1997 19:23:57 +0200 (MESZ) X-Mailer: ELM [version 2.4 PL25 ME8b] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: 4a8acb183b621acecb27bf6e92478642 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hi, Here is my first attempt writing a paper in english :) "An exploration of coherence-based acceleration methodes using the ray tracing kernel G/GX " located at: http://www.rz.tu-ilmenau.de/~juhu/Papers/IWK.ps.gz It handles some problems of coherence-based accel. methods, comparison results, possibilities & limitations of hybrid methods etc. It also proposes an algorithm making BSP-trees balanced. As an alternative to the shadow-volume method for softshadows, a new approach using the ext. Light-Buffer and Clipping beams to avoid unecessary Monte-Carlo rays for direct-lighting is also described. Could someone please proofread it ? (My english is really *bad*!) Thanks, --JuHu From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id UAA01762; Mon, 24 Mar 1997 20:13:11 +0100 Received: from merckx.graphics.cornell.edu (MERCKX.GRAPHICS.CORNELL.EDU [128.84.247.147]) by imag.imag.fr (8.8.1/8.6.9) with SMTP id TAA15323 for ; Mon, 24 Mar 1997 19:40:00 +0100 (MET) Received: by merckx.graphics.cornell.edu (5.65/DEC-Ultrix/4.3) id AA29561; Mon, 24 Mar 1997 13:39:58 -0500 Message-Id: <9703241839.AA29561@merckx.graphics.cornell.edu> Received: by phoenix.graphics.cornell.edu (1.37.109.8/16.2) id AA17898; Mon, 24 Mar 1997 13:39:58 -0500 From: Bruce Walter Subject: Re: Terminology question To: globillum@imag.fr Date: Mon, 24 Mar 1997 13:39:58 -0500 (EST) X-Mailer: ELM [version 2.4 PL25] Mime-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: 27a2e8682db94b4b7b9712327cccce02 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 At the risk of beating a dead horse, I'll post a update to my terminology posting of a week ago. I've received a few replies but all off list. So far my terminology proposal has been greeted with a collective yawn. This is not surprising as terminology issues are like credit card bills. Not very exciting but you will end up in big trouble if you don't deal with them. Even I am not all that thrilled by my proposed "tristimulance" terminology, and I'd be happy to endorse a better suggestion if one is put forward. But I think that there is something unsatisfactory about our current use of terminology and specifically the term "radiance". If we accept the ANSI/IES illuminating engineering terminology standard, then the term radiance has a precise definition, and it precisely describes a quantity which is useless for computer graphics. It measures radiated power regardless of its wavelength. If I'm warming my feet by a roaring fire, radiance is useful for telling me how close I can get before my socks are in danger of catching on fire, but it does not describe what I will actually see with my eyes. The current usage often seems be (and I too am guilty of this): "I'll say 'radiance' (since I'm used to the term and others use it too) because its obvious that I don't actually mean 'radiance' (as defined in the ANSI/IES standard) and therefore my audience will figure out what I actually mean (even if I'm not sure myself)". If we want to continue using the term radiance we should really decide what we mean by it. It is fine for describing monochromatic light, but that's only useful for some pedagogical purposes. We could claim that it is a shorthand for the spectral radiance, but we should recognize that that is an implicit redefinition of the term radiance. Also we aren't really after spectral radiance. I don't know anyone who actually stores a spectra at each of their pixels (at least not in computer graphics). And we don't bother to compute the spectral radiance outside of the visible band, not because its not significant, but because it doesn't affect what really are interested in. So what is it that we are really interested in computing and what should we call it? This may all seem like hair splitting, but what is the point of having precisely defined terms unless we use them precisely? So I would challenge people to either specify what it is they actually mean when they say radiance, or to find some alternate terminology to use instead. Let me quickly respond to a few comments that I received: - CIE and IES standards committees are very slow moving bodies, do not coordinate with each other, and are not necessarily receptive to outside suggestions. Thus the chance of affecting the official standards is slim. > I believe the graphics community should follow standards where they exist and are applicable, but we also have the right to define our own terminology where no appropiate standard exists. - Is the "tri" in tristimulance really necessary, what if you are using a different number of weighting functions. How about stimulance instead? > The tristimulance terminology is specifically intended for color vision in the phototopic range where the three color channel approximation is nearly universal. It is also intended to be derivative the somewhat standard terminology "tristimulus values". Other quantities might be termed stimulance, though there would be some objections if these quantities did not correspond to actual stimuli. - Why not just call it the "color of the radiance"? > Radiance by definition does not contain the color information. It would be at least as correct (and I would argue probably more correct) to call it the "color of the luminance". In my opinion, neither one is really satisfactory or terribly precise. Bruce Walter From Received: from eye.eye.com by titus.cg.tuwien.ac.at via SMTP (940816.SGI.8.6.9/940406.SGI) for id SAA03656; Mon, 31 Mar 1997 18:42:34 +0200 Received: from [149.54.2.22] by eye.eye.com with SMTP (1.37.109.8/16.2) id AA06990; Mon, 31 Mar 1997 11:42:33 -0500 Received: by hemlock (1.37.109.8/15.6) id AA06437; Mon, 31 Mar 1997 11:42:33 -0500 Date: Mon, 31 Mar 1997 11:42:33 -0500 From: Eric Haines Message-Id: <9703311642.AA06437@hemlock> To: purgathofer X-UIDL: e0753515513d283547167ad1e2095824 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Doh! I should *definitely* have mentioned that you should put Autodesk in my regular mail address. It should get there without it, but just in case use: Eric Haines Autodesk Inc. 1050 Craft Road Ithaca, NY 14850 erich@acm.org (in case of bounce, more direct is: Eric.Haines@autodesk.com) 607-266-7000 fax 607-266-7100 Thanks, Eric From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id TAA03802; Mon, 31 Mar 1997 19:58:56 +0200 Received: from mercury.uniserve.com (mercury.uniserve.com [204.191.197.248]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id TAA01991 for ; Mon, 31 Mar 1997 19:36:11 +0200 (MET DST) Received: from helios (van0102.TVS.NET [204.191.197.12]) by mercury.uniserve.com (8.8.2/8.8.2) with ESMTP id JAA04922; Mon, 31 Mar 1997 09:32:10 -0800 (PST) Message-Id: <199703311732.JAA04922@mercury.uniserve.com> From: "Ian Ashdown" To: globillum@imag.fr Cc: mscytsy@scs.leeds.ac.uk Subject: New global illumination bibliography Date: Mon, 31 Mar 1997 09:33:34 -0800 X-MSMail-Priority: Normal X-Priority: 3 X-Mailer: Microsoft Internet Mail 4.70.1155 MIME-Version: 1.0 Content-Type: text/plain; charset=windows-1252; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: 1c7850e8980314e5bd2e7aeb783f8e59 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 There is a wonderful *annotated* global illumination bibliography that has been put together by Travlex Yeap. You can access it at: http://www.scs.leeds.ac.uk/mscytsy/md/abs-mnu.htm Ian Ashdown, P. Eng. Research & Development Manager Ledalite Architectural Products Inc. From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id WAA16068; Wed, 2 Apr 1997 22:35:13 +0200 Received: from mercury.uniserve.com (mercury.uniserve.com [204.191.197.248]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id RAA07549 for ; Wed, 2 Apr 1997 17:29:32 +0200 (MET DST) Received: from van0114.TVS.NET (van0114.TVS.NET [204.191.197.24]) by mercury.uniserve.com (8.8.2/8.8.2) with SMTP id HAA09000 for ; Wed, 2 Apr 1997 07:25:01 -0800 (PST) Date: Wed, 2 Apr 1997 07:25:01 -0800 (PST) Message-Id: <199704021525.HAA09000@mercury.uniserve.com> X-Sender: iashdown@pop.uniserve.com X-Mailer: Windows Eudora Version 1.4.4 Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed To: globillum@imag.fr From: Ian Ashdown Subject: ANNOUNCE: Radiosity Bibliography Update X-UIDL: 03e949598a2a41d7fb0f20ef8416a19a X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit ANNOUNCE: 97/04/01 Release of RADBIB97.BIB ------------------------------------------ RADBIB97 is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. It currently includes 1,106 references. This bibliography is available in BibTex format as RADBIB97.BIB (with a release date of April 1, 1997) from: http://www.ledalite.com/library-/rrt.htm and as compressed RadBib97.Z from: ftp://hobbes.lbl.gov/pub/doc As always, it is time-consuming and sometimes difficult to track down conference papers and theses on radiosity and global illumination. If you know of a relevant reference that is not included in the bibliography, please let me know so that I can include it in the next release. From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id VAA07544; Thu, 17 Apr 1997 21:37:08 +0200 Received: from ux2.sp.cs.cmu.edu (UX2.SP.CS.CMU.EDU [128.2.198.102]) by imag.imag.fr (8.8.1/8.6.9) with SMTP id VAA10664 for ; Thu, 17 Apr 1997 21:18:30 +0200 (MET DST) Received: from GS190.SP.CS.CMU.EDU by ux2.sp.cs.cmu.edu id aa07856; 17 Apr 97 15:17 EDT X-Sender: ajw@ux1.sp.cs.cmu.edu Message-Id: Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed Date: Thu, 17 Apr 1997 15:21:20 -0400 To: globillum@imag.fr From: "Andrew J. Willmott" Subject: Tech report on radiosity methods X-UIDL: 4c79f77043cab7606d7c45a7a47dd943 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit I just wanted to announce that a technical report on our investigation of the various radiosity algorithms out there is available on the web at: http://www.cs.cmu.edu/~radiosity/emprad-tr.html The abstract is reproduced below: --- An Empirical Comparison of Radiosity Algorithms Andrew J. Willmott and Paul S. Heckbert This report presents an extensive empirical comparison of matrix, progressive, and wavelet radiosity algorithms for simulating diffuse interreflection in three-dimensional scenes. The algorithms are tested in their basic forms, without advanced variations such as clustering, discontinuity meshing, or Monte Carlo techniques. The three algorithms were implemented in a common code base to facilitate direct empirical comparison. A number of parameterized scenes were designed to test the basic methods' ability to deal with such issues as singularities, occlusion, high reflectance, and scene complexity. Each algorithm was run on the set of scenes at several parameter settings, and results were examined in terms of their error, speed, and memory consumption. For the basic algorithms as we implemented them, our results show: Progressive radiosity with substructuring is best for simple scenes, but for moderately complex scenes it is outperformed by wavelet radiosity using the Haar basis. Wavelet methods use an immense amount of memory; without clustering they become totally impractical for complex scenes. The problem is particularly severe for higher order bases, less so for Haar. Visibility handling was also found to be a critical problem with higher order wavelets. This study also provides a general framework for comparisons of global illumination techniques. --- Cheers, Andrew --- mailto:a.willmott@cs.cmu.edu ------- http://www.cs.cmu.edu/~ajw --- From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id XAA09899; Wed, 14 May 1997 23:08:33 +0200 Received: from graphics.lcs.mit.edu (graphics.lcs.mit.edu [18.24.2.30]) by imag.imag.fr (8.8.1/8.6.9) with SMTP id WAA08815 for ; Wed, 14 May 1997 22:38:40 +0200 (MET DST) Received: from easel.lcs.mit.edu by graphics.lcs.mit.edu (AIX 4.1/UCB 5.64/4.03) id AA49972; Wed, 14 May 1997 16:35:08 -0400 Received: by easel.lcs.mit.edu (950413.SGI.8.6.12/TOC-1.2C) id QAA21393; Wed, 14 May 1997 16:37:59 -0400 From: "Julie Dorsey" Message-Id: <9705141637.ZM21391@easel.lcs.mit.edu> Date: Wed, 14 May 1997 16:37:58 -0400 X-Mailer: Z-Mail (3.2.3 08feb96 MediaMail) To: globillum@imag.fr Subject: (Fwd) NIST postdoc in GI Cc: hunt@cam.nist.gov Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed X-UIDL: 6e843ff049e0c96515b819a5daeec5aa X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit --- Forwarded mail from hunt@cam.nist.gov (Fern Hunt) Date: Wed, 14 May 97 16:29:51 EDT From: hunt@cam.nist.gov (Fern Hunt) To: dorsey@graphics.lcs.mit.edu Postdoctoral position at NIST in Global Illumination Modeling An interdiscplinary group at NIST is involved in research on the scientific basis of appearance of painted and coated surfaces with a view towards developing rational manufacturing and design strategies based on the coupling of goniophotometric and material measurements with computer graphics models. Our reserach interests lie in the application and development of physically based global illumination models of the interatction of light with coated surfaces. We will use the results of textural, spectral and reflectance measurements as well as mathematical modeling efforts here at NIST and elsewhere, modifying where necessary to meet the needs of our application. Opportunities exist in realistic rendering from measured and computed BRDS, wavelet and other database techniques for compactly storing and representing BRDF, development of metrics for evaluating fidelity of simulated images and realistic 2D and 3D images, and techniques for converting physical simulations of coated surfaces to visually realistic displays on a monitor. Those interested in applying for the postdoc should write to: Dr. Jack Hsia Office of Academic Affairs National Institute of Standards and Technology Gaithersburg, MD. 20899 An official announcement will appear in July with the deadline for applications January 15, 1998. Positions will begin in the Fall 1998. ---End of forwarded mail from hunt@cam.nist.gov (Fern Hunt) From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id SAA19788; Sun, 18 May 1997 18:36:48 +0200 Received: from mercury.uniserve.com (mercury.uniserve.com [204.191.197.248]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id SAA24857 for ; Sun, 18 May 1997 18:20:08 +0200 (MET DST) Received: from helios (van0120.TVS.NET [204.191.197.30]) by mercury.uniserve.com with ESMTP id JAA28909 for ; Sun, 18 May 1997 09:20:03 -0700 (PDT) Message-Id: <199705181620.JAA28909@mercury.uniserve.com> From: "Ian Ashdown" To: globillum@imag.fr Subject: Software patents Date: Sun, 18 May 1997 09:20:42 -0700 X-MSMail-Priority: Normal X-Priority: 3 X-Mailer: Microsoft Internet Mail 4.70.1155 MIME-Version: 1.0 Content-Type: text/plain; charset=windows-1252; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: 48fd666dce7a63e56eff71d423a5c912 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 You may be interested to know that on May 28, 1996, the United States Patent Office awarded the following two patents: US Patent Number: 5,521,852 5,521,853 (continuation) Title: Method and System for Designing Lighting Installations Inventors: John D. Hibbs Douglas J. Stang Assignee: Holophane Lighting, Inc. Newark, Ohio There are no less than 42 claims between these two patents, and they are very broad in scope. They pertain to any computer graphics program that attempts to model physically realistic lighting. Ian Ashdown, P. Eng. | READ THE BOOK! | Research & Development Manager | Radiosity: A Programmer's Perspective | Ledalite Architectural Products | Wiley & Sons 1994 | Visit http://www.ledalite.com | (Sneaky Internet Advertising) | From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id SAA21129; Mon, 19 May 1997 18:29:45 +0200 Received: from sgi.sgi.com (SGI.COM [192.48.153.1]) by imag.imag.fr (8.8.1/8.6.9) with SMTP id SAA06323 for ; Mon, 19 May 1997 18:09:42 +0200 (MET DST) Received: from cthulhu.engr.sgi.com (cthulhu.engr.sgi.com [192.26.80.2]) by sgi.sgi.com (950413.SGI.8.6.12/970507) via ESMTP id JAA01266 for <@sgi.engr.sgi.com:globillum@imag.fr>; Mon, 19 May 1997 09:09:40 -0700 env-from (bwade@cthulhu.engr.sgi.com) Received: from amie.engr.sgi.com (amie.engr.sgi.com [198.29.108.214]) by cthulhu.engr.sgi.com (950413.SGI.8.6.12/960327.SGI.AUTOCF) via ESMTP id JAA07565 for <@cthulhu.engr.sgi.com:globillum@imag.fr>; Mon, 19 May 1997 09:09:39 -0700 Received: from pc-amie (pc-amie.engr.sgi.com [198.29.108.199]) by amie.engr.sgi.com (950413.SGI.8.6.12/960327.SGI.AUTOCF) via SMTP id JAA12589 for ; Mon, 19 May 1997 09:09:38 -0700 Message-Id: <3.0.1.32.19970519090938.00a93260@amie.engr.sgi.com> X-Sender: bwade@amie.engr.sgi.com X-Mailer: Windows Eudora Pro Version 3.0.1 (32) Date: Mon, 19 May 1997 09:09:38 -0700 To: globillum@imag.fr From: Bretton Wade Subject: Re: Software patents In-Reply-To: <199705181620.JAA28909@mercury.uniserve.com> Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed X-UIDL: cca99e43a53c639f7fd9546cd20ad71e X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit And was everyone on this list presented as a co-creator? Seriously, can you give any more details? Thanks, Bretton At 09:20 AM 5/18/97 -0700, Ian Ashdown wrote: >You may be interested to know that on May 28, 1996, the United States >Patent Office awarded the following two patents: > > US Patent Number: 5,521,852 > 5,521,853 (continuation) > Title: Method and System for Designing Lighting > Installations > Inventors: John D. Hibbs > Douglas J. Stang > Assignee: Holophane Lighting, Inc. > Newark, Ohio > >There are no less than 42 claims between these two patents, and they are >very broad in scope. They pertain to any computer graphics program that >attempts to model physically realistic lighting. > >Ian Ashdown, P. Eng. | READ THE BOOK! | >Research & Development Manager | Radiosity: A Programmer's Perspective | >Ledalite Architectural Products | Wiley & Sons 1994 | >Visit http://www.ledalite.com | (Sneaky Internet Advertising) | > > -- Bretton Wade (bwade@engr.sgi.com) From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id VAA21312; Mon, 19 May 1997 21:31:14 +0200 Received: from relay2.mail.uk.psi.net (sys1.london.uk.psi.net [154.32.108.2]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id UAA08338 for ; Mon, 19 May 1997 20:51:42 +0200 (MET DST) Received: from lightwork.co.uk (lightwork.co.uk [195.152.206.2]) by relay2.mail.uk.psi.net (8.8.4/) with SMTP id TAA10863; Mon, 19 May 1997 19:41:18 +0100 (BST) Received: by lightwork.co.uk (SMI-8.6/SMI-SVR4) id TAA10823; Mon, 19 May 1997 19:40:43 +0100 Received: from owl(192.9.200.2) by roo via smap (V1.3) id sma010821; Mon May 19 19:40:21 1997 Received: from hermia by owl.lightwork.co.uk (SMI-8.6/SMI-SVR4) id TAA22723; Mon, 19 May 1997 19:40:10 +0100 Message-ID: <33809D23.56AF@lightwork.co.uk> Date: Mon, 19 May 1997 19:34:11 +0100 From: Neil Gatenby Reply-To: neil@lightwork.co.uk Organization: LightWork Design Ltd X-Mailer: Mozilla 3.0 (WinNT; I) MIME-Version: 1.0 To: Bretton Wade CC: globillum@imag.fr Subject: Re: Software patents References: <3.0.1.32.19970519090938.00a93260@amie.engr.sgi.com> Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: 606f5f2a537842a8b952a8b6723403f7 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Bretton Wade wrote: > > And was everyone on this list presented as a co-creator? > > Seriously, can you give any more details? > > Thanks, > Bretton > > At 09:20 AM 5/18/97 -0700, Ian Ashdown wrote: > >You may be interested to know that on May 28, 1996, the United States > >Patent Office awarded the following two patents: > > > > US Patent Number: 5,521,852 > > 5,521,853 (continuation) > > Title: Method and System for Designing Lighting > > Installations > > Inventors: John D. Hibbs > > Douglas J. Stang > > Assignee: Holophane Lighting, Inc. > > Newark, Ohio > > > >There are no less than 42 claims between these two patents, and they are > >very broad in scope. They pertain to any computer graphics program that > >attempts to model physically realistic lighting. The two attached files were collated from http://www.uspto.gov/ the first details the patents, the second is the list of patents referenced by these patents Neil From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id BAA21501; Tue, 20 May 1997 01:22:20 +0200 Received: from igw3.watson.ibm.com (igw3.watson.ibm.com [129.34.139.18]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id AAA11191 for ; Tue, 20 May 1997 00:57:41 +0200 (MET DST) Received: from mailhub1.watson.ibm.com (mailhub1.watson.ibm.com [9.2.249.31]) by igw3.watson.ibm.com (8.7.6/8.7.1) with ESMTP id SAA03508; Mon, 19 May 1997 18:56:16 -0400 Received: from watngi01.watson.ibm.com (watngi01.watson.ibm.com [9.2.235.20]) by mailhub1.watson.ibm.com (8.8.2/01-15-97) with SMTP id SAA32164; Mon, 19 May 1997 18:56:42 -0400 Received: by watngi01.watson.ibm.com(Lotus SMTP MTA v1.05 (305.3 1-15-1997)) id 8525649C.007E0610 ; Mon, 19 May 1997 18:56:30 -0400 X-Lotus-FromDomain: IBM RESEARCH From: "Holly Rushmeier" To: neil@lightwork.co.uk cc: bwade@relay.engr.SGI.COM, globillum@imag.fr Message-ID: <8525649C.0075B959.00@watngi01.watson.ibm.com> Date: Mon, 19 May 1997 18:55:27 -0400 Subject: Re: Software patents Mime-Version: 1.0 Content-type: text/plain; charset=us-ascii; format=flowed X-UIDL: ab4cc66ea7123046d0f46134708b0b5d X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit I find patents very hard to read and I probably misinterpret them. There are a lot of alarming sounding patents. Since IBM is big on patenting, there is a patent search web page from IBM for searching on text etc. if you want to find more. http://patent.womplex.ibm.com/ Besides locating the patent, you can read the full text from gif images of the actual patent, or just get ascii text of all the claims. The patent Ian mentioned seems from my naive point of view to be impossible to defend -- they describe a lot of well-known stuff like a simple adaptive subdivision scheme for meshing. Another odd example is, 5590062 "Simulator for producing various living environments mainly for visual perception" seems to patent VR for looking at realistic 3D environments. I like the part on page 41 that says "The 3-D space is not limited to the internal space ... a plain in the Mesozoic era where dinosaurs exist can be simulated just for fun." I suppose there is a good legal reason for saying something like this. I also suppose there is a reason they reference Chernoff's paper on multivariate visualization with faces. Then there is 4928250 "System for deriving radiation images" (aka the hemicube patent) and the 16 patents that reference it including the hierarchical z-buffer and something called "Image Processing Apparatus" that has to do with ray casting in radiosity calculations. Three patents reference the patent on ray casting for view factors including 5546327 "Apparatus for calculating geometrical view factor", just issued last August which seems to patent using a hemisphere instead of the hemicube. Following various links also leads to 5619627 "Multiple-level occulting using a mask buffer" that describes an "Occulting apparatus" which just seems to be a method for finding hidden surfaces fast, not as mysterious an apparatus as you might think. I was surprised to find 5363477 "Method for displaying an image of an object surface using a luminance transformationin accordance with a non-linear characteristic" that sounds like a patent on the notion of tone mapping for synthetic images. You can also search by assignee, for example to see all of Pixar's patents, e.g. 5239624 "Pseudo-random point sampling techniques in computer graphics". Anyway, if you get depressed over this , try the "Gallery of Obscure Patents" at http://patent.womplex.ibm.com/gallery.html which includes "Wacky Patent of the Month." On the other hand, the fact that some one was able to patent a hat that looks like a fried egg might depress you even more. -- Holly From Received: from imag.imag.fr by titus.cg.tuwien.ac.at via ESMTP (940816.SGI.8.6.9/940406.SGI) id SAA23827; Tue, 20 May 1997 18:03:47 +0200 Received: from ibis.doc.ic.ac.uk (ibis.doc.ic.ac.uk [146.169.12.90]) by imag.imag.fr (8.8.1/8.6.9) with SMTP id OAA29782 for ; Tue, 20 May 1997 14:41:25 +0200 (MET DST) Received: by ibis.doc.ic.ac.uk (Smail3.1.28.1 #8) id m0wTnlY-0002ndC; Tue, 20 May 97 13:11 BST Message-Id: Date: Tue, 20 May 97 13:11 BST To: globillum@imag.fr From: "Adrian J. Chung" References: <8525649C.0075B959.00@watngi01.watson.ibm.com> X-Mailer: vmail-0.06alpha Subject: Re: Software patents X-UIDL: ce4348d9fa055455585d89da13a20fd9 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit "Holly Rushmeier" wrote: > I find patents very hard to read and I probably misinterpret > them. There are a lot of alarming sounding patents. IANAL. Any lawyers on this list? > Since IBM is big on patenting, there is a patent search web page from IBM > for searching on text etc. if you want to find more. > > http://patent.womplex.ibm.com/ Thank's for the URL. Bookmarked. I'm sure many of you are familiar with the Electronic Frontier Foundation page on intellectual property: http://www.eff.org/pub/Intellectual_property/ Useful for some legal insight on software law. Not sure how biased it is though. > The patent Ian mentioned seems from my naive point of view to be > impossible to defend -- they describe a lot of well-known stuff like > a simple adaptive subdivision scheme for meshing. Maybe they're hoping to capitalise on it in the same way E-Data has been with patent 4528643, which claims rights to all methods of electronic multimedia distribution. In this case the patent predates the now "well known" nature of WWW. ( See http://www.lpf.org/Patents/edata.html for the anti-software-patent point of view of the case) If worse comes to worse perhaps the Net will treat enforced software patents as damage and route around them. (to misquote John Gillmore) This was certainly a major motivating factor behind the PNG standard as a GIF replacement. I can see it now. Huge Monte Carlo rendering farms being set up in the Caribbean (or other legal havens) servicing contracts from US based companies. Adrian "your milage may vary" -- DISCLAIMER: URLs quoted in the above message should not in anyway imply that the author, the department, or indeed the institution from which the email is sent are in any sense libertarian. Copyright 1997 by Adrian J. Chung. It may be quoted in part for strictly non-commercial use only. From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by mail.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id TAA04388; Wed, 28 May 1997 19:49:46 +0200 Received: from sys3.cambridge.uk.psi.net (sys3.cambridge.uk.psi.net [154.32.106.10]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id TAA05629 for ; Wed, 28 May 1997 19:25:23 +0200 (MET DST) Received: from lightwork.co.uk (lightwork.co.uk [195.152.206.2]) by sys3.cambridge.uk.psi.net (8.8.4/) with SMTP id SAA19108 for ; Wed, 28 May 1997 18:25:18 +0100 (BST) Received: by lightwork.co.uk (SMI-8.6/SMI-SVR4) id SAA20124; Wed, 28 May 1997 18:24:47 +0100 Received: from owl(192.9.200.2) by roo via smap (V1.3) id sma020122; Wed May 28 18:24:33 1997 Received: from hermia by owl.lightwork.co.uk (SMI-8.6/SMI-SVR4) id SAA08832; Wed, 28 May 1997 18:24:32 +0100 Message-ID: <338C68CD.4C30@lightwork.co.uk> Date: Wed, 28 May 1997 18:18:05 +0100 From: Neil Gatenby Reply-To: neil@lightwork.co.uk Organization: LightWork Design Ltd X-Mailer: Mozilla 3.0 (WinNT; I) MIME-Version: 1.0 To: globillum@imag.fr Subject: jobs Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: 7c403569db32fb64f35e11169bd518d6 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 For jobs in global illumination, and other areas of 3D graphics, see http://www.lightwork.com/vacancies/ For global illumination, follow the "Software Engineer - Lighting Simulation and Radiosity" thread. Neil -- Neil Gatenby, Software lead, LightWork Design Limited. mailto:neil@lightwork.co.uk http://www.lightwork.com Tel: +44 114 266 8404 ext 118 FAX: +44 114 266 1383 From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by mail.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id VAA32578; Fri, 6 Jun 1997 21:53:47 +0200 Received: from redemption.uniserve.com (redemption.uniserve.com [204.191.197.254]) by imag.imag.fr (8.8.1/8.6.9) with SMTP id VAA03266 for ; Fri, 6 Jun 1997 21:38:01 +0200 (MET DST) Received: from ian [204.191.197.127] by redemption.uniserve.com with smtp (Exim 1.62 #1) id 0wa4pi-0004bb-00; Fri, 6 Jun 1997 12:37:58 -0700 X-Sender: iashdown@pop.uniserve.com X-Mailer: Windows Eudora Version 1.4.4 Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed To: globillum@imag.fr From: Ian Ashdown Subject: 97/06/01 Release of RADBIB97.BIB Message-Id: Date: Fri, 6 Jun 1997 12:37:58 -0700 X-UIDL: e34627c507c40c6ea549989001ec8306 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit ANNOUNCE: 97/06/01 Release of RADBIB97.BIB ------------------------------------------ RADBIB97 is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. It currently includes 1,152 references. This bibliography is available in BibTex format as RADBIB97.BIB (with a release date of June 1, 1997) from: http://www.ledalite.com/library-/rrt.htm ftp://ftp.ledalite.com/pub/radbib97.bib - Ian Ashdown From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by mail.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id TAA30319; Mon, 9 Jun 1997 19:58:36 +0200 Received: from HOSTESS.GRAPHICS.CS.CMU.EDU (HOSTESS.GRAPHICS.CS.CMU.EDU [128.2.206.188]) by imag.imag.fr (8.8.1/8.6.9) with SMTP id TAA13181 for ; Mon, 9 Jun 1997 19:39:15 +0200 (MET DST) From: Paul.Heckbert@HOSTESS.GRAPHICS.CS.CMU.EDU Message-Id: <199706091739.TAA13181@imag.imag.fr> Date: Mon, 9 Jun 97 13:18:21 EDT To: globillum@imag.fr Subject: read comparison before St Etienne? X-UIDL: 815fd91825b8c053663a6074374e6911 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit If you are coming to the Eurographics Workshop on Rendering in St Etienne, France next week (see http://www.emse.fr/RENDERING97/) then I would like to suggest that you read a tech report "An Empirical Comparison of Radiosity Algorithms" http://www.cs.cmu.edu/~radiosity/emprad-tr.html as my co-author and I would enjoy getting feedback on this work at the workshop, and we feel it could be an interesting topic of discussion there. Some of our conclusions: * Wavelet radiosity without clustering and matrix radiosity are memory hogs. (esp. matrix radiosity and higher order wavelets; HR not so bad) This was previously known; our results show how bad they are. * Visibility handling in wavelet radiosity algorithms is poor, consequently higher order wavelets are not currently practical. * Progressive radiosity with substructuring is often a better choice than wavelet radiosity. Paul Heckbert Computer Science Dept., Carnegie Mellon University 5000 Forbes Ave, Pittsburgh PA 15213-3891, USA ph@cs.cmu.edu http://www.cs.cmu.edu/~ph From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by mail.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id UAA13100; Wed, 11 Jun 1997 20:33:12 +0200 Received: from redemption.uniserve.com (redemption.uniserve.com [204.191.197.254]) by imag.imag.fr (8.8.1/8.6.9) with SMTP id UAA06911 for ; Wed, 11 Jun 1997 20:18:22 +0200 (MET DST) Received: from ian [204.191.197.53] by redemption.uniserve.com with smtp (Exim 1.62 #1) id 0wbryJ-0006mc-00; Wed, 11 Jun 1997 11:18:16 -0700 X-Sender: iashdown@pop.uniserve.com X-Mailer: Windows Eudora Version 1.4.4 Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed To: globillum@imag.fr From: Ian Ashdown Subject: Spectroradiometric data Message-Id: Date: Wed, 11 Jun 1997 11:18:16 -0700 X-UIDL: 523f31c3da35a6a2460d7b370ed3626d X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit One of our most common excuses for using the simplistic RGB color model in global illumination-based rendering is that "there are no spectroradiometric data for commonly available materials." This has undoubtably been true in the past, but this excuse is beginning to wear thin. If you are looking for such data, try: http://www.lut.fi/ltkk/tite/research/color/lutcs_readme.html - Ian Ashdown P.S. - I'm sure they are many more sites out there with equally useful data. I only found this particular one because I was (am still am) looking for an algorithm to convert DIN RAL codes to their equivalent Munsell values. Any suggestions on where to look for this information (short of actually the DIN standards ;+) would be much appreciated. From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by mail.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id LAA04239; Thu, 12 Jun 1997 11:14:20 +0200 Received: from mail3.microsoft.com (mail3.microsoft.com [131.107.3.23]) by imag.imag.fr (8.8.1/8.6.9) with ESMTP id KAA28823 for ; Thu, 12 Jun 1997 10:41:52 +0200 (MET DST) Received: by mail3.microsoft.com with Internet Mail Service (5.0.1458.30) id ; Thu, 12 Jun 1997 01:44:16 -0700 Message-ID: <011290D45A8ACF119B8B00805FD471D60321993B@RED-24-MSG.dns.microsoft.com> From: Andrew Glassner To: globillum@imag.fr, "'iashdown@ledalite.com'" Subject: RE: Spectroradiometric data Date: Thu, 12 Jun 1997 01:41:25 -0700 X-Priority: 3 X-Mailer: Internet Mail Service (5.0.1458.30) X-UIDL: 2985d0d035da6d47e9a3993e0e986936 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit This has long been a pet peeve of mine as well. You can find a bunch of public-domain standard curves and some standard and unusual reflectance data at http://www.research.microsoft.com/research/graphics/glassner/work/projec ts/pdis/pdis.htm Gregory Ward Larson has also made this available in MGF style at http://radsite.lbl.gov/mgf/HOME.html -Andrew > ---------- > From: iashdown@ledalite.com[SMTP:iashdown@ledalite.com] > Sent: Wednesday, June 11, 1997 11:18 AM > To: globillum@imag.fr > Subject: Spectroradiometric data > > One of our most common excuses for using the simplistic RGB > color model in global illumination-based rendering is that > "there are no spectroradiometric data for commonly available > materials." > > This has undoubtably been true in the past, but this excuse > is beginning to wear thin. If you are looking for such data, > try: > > http://www.lut.fi/ltkk/tite/research/color/lutcs_readme.html > > - Ian Ashdown > > P.S. - I'm sure they are many more sites out there with > equally useful data. I only found this particular one because > I was (am still am) looking for an algorithm to convert DIN > RAL codes to their equivalent Munsell values. Any suggestions > on where to look for this information (short of actually > the DIN standards ;+) would be much appreciated. > From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by mail.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id PAA22519; Fri, 13 Jun 1997 15:14:46 +0200 Received: from inf.ethz.ch (root@neptune.ethz.ch [129.132.10.10]) by imag.imag.fr (8.8.1/8.8.5) with SMTP id OAA05884 for ; Fri, 13 Jun 1997 14:39:37 +0200 (MET DST) Received: from barks (barks.inf.ethz.ch [129.132.10.212]) by inf.ethz.ch (8.6.10/8.6.10) with ESMTP id OAA25807 for ; Fri, 13 Jun 1997 14:39:36 +0200 Received: (lippert@localhost) by barks (950413.SGI.8.6.12/8.6.9) id OAA15558 for globillum@imag.fr; Fri, 13 Jun 1997 14:39:35 +0200 From: "Lars Lippert" Message-Id: <9706131439.ZM15556@barks.inf.ethz.ch> Date: Fri, 13 Jun 1997 14:39:34 -0600 X-Mailer: Z-Mail (3.2.3 08feb96 MediaMail) To: globillum@imag.fr Subject: Volume Rendering in Java Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed X-UIDL: 1aea486363374f0cbccc8b479b5cd9ee X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hi, I just wanted to announce that an interactive web-based volume renderer can now be tested. The program is written as an applet, that runs inside Web pages. The concept behind this software is a hierarchical (wavelet-based) representation of the volume data-set. The data is rendered directly from wavelet-space and thus requires a minumum of memory. The applet presents a novel way of presenting volumetric data on the Internet. The user can manipulate an inferior quality version of 3-D volume interactively in order to set up the viewing parameters, and when they are correct the image refines progressively. The rendering perfomance depends on the network bandwidth and the available hardware platform. Simply point your internet browser to: http://www.inf.ethz.ch/personal/lippert/EVOLVE/ Please feel free to contact me with comments, suggestions, or bug-reports. I only ran the program on my Indy and PC , but one of the nice feature of Java is that it runs on all architectures. If this is not the case, please let me know. Lars -- _________________________________________________________________________ Lars Lippert Computer Graphics Research Group Institute for Information Systems Swiss Federal Institute of Technology Zuerich Tel.: +41-1-632 71 21 Email: lippert@inf.ethz.ch Fax : +41-1-632 11 72 Office: IFW E45.2 http://www.inf.ethz.ch/personal/lippert _________________________________________________________________________ From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by mail.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id SAA11910; Wed, 18 Jun 1997 18:42:41 +0200 Received: from adeskgate.autodesk.com (adeskgate.autodesk.com [198.93.152.11]) by imag.imag.fr (8.8.1/8.8.5) with ESMTP id SAA14615 for ; Wed, 18 Jun 1997 18:04:58 +0200 (MET DST) Received: from autodesk.autodesk.com by adeskgate.autodesk.com (8.6.12/SMI-5.3) with ESMTP id JAA19403; Wed, 18 Jun 1997 09:04:07 -0700 Received: from hqhubmu1.autodesk.com by autodesk.autodesk.com (8.6.12/4.4BSD) with ESMTP id JAA05628; Wed, 18 Jun 1997 09:03:54 -0700 Received: from ccinternet.autodesk.com (ccinternet [144.111.240.144]) by hqhubmu1.autodesk.com (8.7.5/8.7.3) with SMTP id JAA21836 for ; Wed, 18 Jun 1997 09:03:52 -0700 (PDT) Received: from ccMail by ccinternet.autodesk.com (IMA Internet Exchange 2.11 (Pre-release) Enterprise) id 0002051F; Wed, 18 Jun 1997 09:03:11 -0700 Mime-Version: 1.0 Date: Wed, 18 Jun 1997 11:59:38 -0700 Message-ID: <0002051F.4149@autodesk.com> From: Eric Haines Subject: Ray tracing bibliography updated To: globillum Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit Content-Description: cc:Mail note part X-UIDL: b8b7dcc924586d4eaf75ae8cd18b30e7 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Globillumers, I've updated the free ray tracing bibliography with a number of new references (many thanks to Steve Warren at Sandia). The bibliography is available at: http://www.acm.org/tog/resources/bib/ Please do let me know of any additions/corrections you know of, Eric Haines erich@acm.org From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by mail.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id UAA13443; Mon, 23 Jun 1997 20:45:54 +0200 Received: from ns1.arlut.utexas.edu (ns1.arlut.utexas.edu [129.116.212.1]) by imag.imag.fr (8.8.1/8.8.5) with ESMTP id RAA16375 for ; Mon, 23 Jun 1997 17:52:10 +0200 (MET DST) Received: from mail-firewall.arlut.utexas.edu (ns1.arlut.utexas.edu [129.116.212.1]) by ns1.arlut.utexas.edu (8.8.5/8.8.5) with ESMTP id KAA12978; Mon, 23 Jun 1997 10:48:38 -0500 (CDT) Received: from sting.arlut.utexas.edu (sting.arlut.utexas.edu [129.116.128.90]) by mail-firewall.arlut.utexas.edu (8.8.5/8.8.5) with ESMTP id KAA12971; Mon, 23 Jun 1997 10:48:37 -0500 (CDT) Received: from sting (localhost [127.0.0.1]) by sting.arlut.utexas.edu (8.8.5/8.7.3) with SMTP id KAA24180; Mon, 23 Jun 1997 10:48:35 -0500 (CDT) Sender: atc@arlut.utexas.edu Message-ID: <33AE9AD3.6263@arlut.utexas.edu> Date: Mon, 23 Jun 1997 10:48:35 -0500 From: "A. T. Campbell" X-Mailer: Mozilla 3.01 (X11; I; HP-UX A.09.07 9000/770) MIME-Version: 1.0 To: Neil Gatenby CC: "'globillum@imag.fr'" Subject: Re: Proceedings of Graphics Interface 97 References: <01BC7FBC.CC783360@hermia.lightwork> Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: a8fb08abb75c9a39a1daad7f69338eaf X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Neil Gatenby wrote: > > Hi; > > Could anyone tell me how I can get hold of a copy of the proceedings of Graphics Interface 97? I have tried searching on the web, but to no avail. > > Thanks in advance, > > Neil Electronic copies of all the papers from GI '97 are available from the conference's web page: http://www.dgp.toronto.edu/gi/gi97/home.html Hardcopies of the proceedings may be purchased from Morgan Kaufmann Publishers. Their web page's URL is the following: http://www.mkp.com/ -- A. T. Campbell, III atc@arlut.utexas.edu http://www.arlut.utexas.edu/~atc Applied Research Labs, University of Texas, PO Box 8029, Austin,TX 78713 From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by mail.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id XAA16050; Mon, 23 Jun 1997 23:48:34 +0200 Received: from HOSTESS.GRAPHICS.CS.CMU.EDU (HOSTESS.GRAPHICS.CS.CMU.EDU [128.2.206.188]) by imag.imag.fr (8.8.1/8.8.5) with SMTP id XAA26345 for ; Mon, 23 Jun 1997 23:17:13 +0200 (MET DST) From: Paul.Heckbert@HOSTESS.GRAPHICS.CS.CMU.EDU Message-Id: <199706232117.XAA26345@imag.imag.fr> Date: Mon, 23 Jun 97 17:06:54 EDT To: globillum@imag.fr Subject: reflectance model visualizer X-UIDL: a0f0e5f1e01f1cc3f98d8b948f4af22e X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit A reflectance model visualizer is available in SGI executable form and C++ source code form at http://www.cs.cmu.edu/~ph/src/illum/ The program should be portable to other machines that support the Xforms user interface library and X windows without too much difficulty. This program is a fairly general viewer for bidirectional reflectance distribution functions (BRDF's). It was written by some students and myself in a graduate course in global illumination that I taught in Fall 1996. The program implements the following reflectance models: Phong Cook-Torrance Oren-Nayar He et al. I demonstrated the program at the Eurographics Workshop on Rendering in St. Etienne, France last week, and there was enough interest that I decided to release it more generally. enjoy! Paul Heckbert Computer Science Dept., Carnegie Mellon University 5000 Forbes Ave, Pittsburgh PA 15213-3891, USA ph@cs.cmu.edu http://www.cs.cmu.edu/~ph From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by mail.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id WAA00300; Wed, 25 Jun 1997 22:19:40 +0200 Received: from horus.imag.fr (horus.imag.fr [129.88.38.2]) by imag.imag.fr (8.8.1/8.8.5) with ESMTP id OAA16211 for ; Wed, 25 Jun 1997 14:45:25 +0200 (MET DST) Received: from dirc.bris.ac.uk (dirc.bris.ac.uk [137.222.10.51]) by horus.imag.fr (8.8.1/8.6.9) with SMTP id OAA02857 for ; Wed, 25 Jun 1997 14:45:23 +0200 (MET DST) Received: from luna.cs.bris.ac.uk by dirc.bris.ac.uk with SMTP (XT-PP) with ESMTP; Wed, 25 Jun 1997 13:43:11 +0100 Received: from danno.cs.bris.ac.uk (danno.cs.bris.ac.uk [137.222.102.2]) by luna.cs.bris.ac.uk (8.8.6/8.8.5) with SMTP id NAA04949 for ; Wed, 25 Jun 1997 13:40:14 +0100 (BST) Received: from localhost by danno.cs.bris.ac.uk (SMI-8.6/SMI-SVR4) id NAA13131; Wed, 25 Jun 1997 13:40:28 +0100 Date: Wed, 25 Jun 1997 13:40:27 +0100 (BST) From: "P. Larsen" X-Sender: larsen@danno To: globillum@imag.fr Subject: URGENT - Freeware/Shareware Radiosity package Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII; format=flowed X-UIDL: ba936cb17a53d7335602119e564a8b71 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hello, my name is Phillip Larsen and I am a MSc student at the University of Bristol, England. I am writing my dissertation on radiosity and need to get hold of a radiosity package which I can build on for my dissertation. The system configuration I will be running the program on is a Sun workstation with the Solaris operating system. If anyon knows where I can get hold of a freeware/shareware radiosity package with accompanying sourcecode I would really appreciate it if you would send me a line saying how and where I could find it. Thankyou for taking the time to read this message. Yours sincerely Phillip Andre' Larsen From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by mail.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id CAA25514; Fri, 27 Jun 1997 02:07:36 +0200 Received: from droopy.cs.kuleuven.ac.be (root@droopy.cs.kuleuven.ac.be [134.58.41.10]) by imag.imag.fr (8.8.1/8.8.5) with ESMTP id WAA21052 for ; Thu, 26 Jun 1997 22:55:00 +0200 (MET DST) Received: from flater.cs.kuleuven.ac.be (philippe@flater.cs.kuleuven.ac.be [134.58.45.35]) by droopy.cs.kuleuven.ac.be (8.8.5/8.8.5) with ESMTP id VAA14573; Thu, 26 Jun 1997 21:29:26 +0200 (MET DST) Received: (from philippe@localhost) by flater.cs.kuleuven.ac.be (8.8.6/8.8.6) id VAA04735; Thu, 26 Jun 1997 21:29:14 +0200 (MET DST) From: Philippe Bekaert Message-Id: <199706261929.VAA04735@flater.cs.kuleuven.ac.be> Subject: Radiosity Software Available for Free In-Reply-To: from "P. Larsen" at "Jun 25, 97 01:40:27 pm" To: globillum@imag.fr Date: Thu, 26 Jun 1997 21:29:13 +0200 (MET DST) Cc: "P. Larsen" , stuerzl@cs.unc.edu, kadi@irisa.fr, Paul.Heckbert@HOSTESS.GRAPHICS.CS.CMU.EDU X-Mailer: ELM [version 2.4ME+ PL32 (25)] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: 8b18d1c979022180f5c3469447bbf48e X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Last week at the Eurographics Rendering Workshop in St-Stienne, France, I gave a demo of the photorealistic renderer called "RenderPark", we are developping in the context of our research here in Leuven (Belgium). The renderer currently offers: - Galerkin radiosity (both gathering and shooting) with (or without) hierarchical refinement, higher order approximations, clustering, view-importance, ... - stochastic ray radiosity - ray-casting, classic and stochastic ray-tracing It is known to compile and run fine on a SUN Sparcstation (with LEO graphics hardware and the Nth Protable GL), under Linux (with Mesa, a free OpenGL like graphics library) and on a number of SGI machines (with OpenGL). You can retrieve the source code and example scene files (MGF format) from the URL: http://www.cs.kuleuven.ac.be/cwis/research/graphics/RENDERPARK/ You can build on it for your research too if you like (hooks are provided already for your ultimate rendering algorithm). Best regards, Philippe. -- /~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~|~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~\ \ Philippe Bekaert | If anything can go wrong, it will, but / / Computer Graphics Research Group | ... we're prepared for it (Switzerland) \ \ Department of Computer Science | ... we don't care (Greece) / / K.U.Leuven - Belgium | ... what the heck, it's been going \ \ | wrong for centuries already (Portugal) / / http://www.cs.kuleuven.ac.be/ | ... it's the fault of the Walloons \ \ ~philippe/ | (Flanders) / /__________________________________| ... we deserve it (Wallonie) \ \ | ... as long as there's vodka we don't / / Not everything that is written | care (Russia) \ \ here is my employers opinion, | ... how much money do I loose? / / sometimes not even mine. | (The Netherlands) \ \__________________________________|_________________________________________/ From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by mail.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id TAA03674; Tue, 1 Jul 1997 19:39:23 +0200 Received: from deliverator.sgi.com (deliverator.sgi.com [204.94.214.10]) by imag.imag.fr (8.8.1/8.8.5) with SMTP id TAA09290 for ; Tue, 1 Jul 1997 19:13:23 +0200 (MET DST) Received: from odin.corp.sgi.com (odin.corp.sgi.com [192.26.51.194]) by deliverator.sgi.com (950413.SGI.8.6.12/951211.SGI.AUTO) via ESMTP id KAA22091; Tue, 1 Jul 1997 10:13:12 -0700 env-from (gregl@radiate.asd.sgi.com) Received: from giraffe.asd.sgi.com by odin.corp.sgi.com via ESMTP (951211.SGI.8.6.12.PATCH1502/951211.SGI) id KAA26500; Tue, 1 Jul 1997 10:13:04 -0700 Received: from radiate.asd.sgi.com by giraffe.asd.sgi.com via ESMTP (951211.SGI.8.6.12.PATCH1502/951211.SGI) id KAA20174; Tue, 1 Jul 1997 10:12:57 -0700 Received: by radiate.asd.sgi.com (950413.SGI.8.6.12/940406.SGI.AUTO) id KAA05298; Tue, 1 Jul 1997 10:12:49 -0700 Date: Tue, 1 Jul 1997 10:12:49 -0700 From: Greg Larson Message-Id: <199707011712.KAA05298@radiate.asd.sgi.com> To: globillum@imag.fr Subject: Siggraph gathering X-UIDL: f5b2b08e2c0334b9d37d39afa889862a X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Dear Siggraph-bound Globillumers: Each year at Siggraph, we try to get together to discuss common issues and share ideas. This year, I'd like to suggest we plan in advance so that we have the best chance of squeezing a meeting into what is always an overcrowded week. I would therefore like to suggest the following time for our get together: Thursday, August 7th, 1-2pm, location TBA We'll probably end up in one of the Birds-of-a-Feather rooms like we did the last two years, and there is always a board near the registration or merchandise pick-up areas where BOF gatherings are posted. This is where we will post the final meeting location and verify the time. If anyone has a compelling reason why this is a poor choice of time (e.g., it conflicts with Microsoft's announcement that they will be purchasing Sony and relocating Japan next to Puget Sound), please let me know. To get the ball rolling, we will have a special guest from the National Institute of Standards and Technology (formerly NBS), Dr. Fern Hunt, who will give an informal overview of a NIST project to standardize reflectance measurements and models for use in computer graphics and paint manufacturing. Of particular interest is a new database called NEF, recently declassified by the CIA, which contains a wealth of data on the reflectance properties (including spectral and directional BRDFs) for common exterior materials. NIST is coordinating the dissemination of this information, with help from a number of people in the industry. For more information on the NIST appearance project, look up: http://math.nist.gov/mcsd/Staff/RLipman/appearance/ Hope to see you there! -Greg _____________________________________________________________________ Gregory Ward Larson (the computer artist formerly known as Greg Ward) Silicon Graphics, Inc. Computer Science Department 2011 N. Shoreline Blvd., M/S 07U-553 537 Soda Hall, UC Berkeley Mountain View, CA 94043-1389 Berkeley, CA 94720-1776 (415) 933-4878, -2663 fax (510) 642-3631, -5775 fax gregl@sgi.com on Tues., Thurs. and Fri. ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by mail.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id QAA07175; Thu, 3 Jul 1997 16:16:38 +0200 Received: from safran.imag.fr (safran.imag.fr [129.88.42.9]) by imag.imag.fr (8.8.1/8.8.5) with ESMTP id PAA03040 for ; Thu, 3 Jul 1997 15:47:05 +0200 (MET DST) Received: (from sillion@localhost) by safran.imag.fr (8.6.10/8.6.9) id PAA13824 for globillum@imag.fr; Thu, 3 Jul 1997 15:47:04 +0200 From: Francois Sillion Message-Id: <199707031347.PAA13824@safran.imag.fr> Subject: POSTDOCTORAL / Research Associate position available To: Global Illumination List Date: Thu, 3 Jul 1997 15:47:04 +0200 (MDT) Reply-To: Francois.Sillion@imag.fr X-Mailer: ELM [version 2.4 PL24] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: af12274e35ce8c3c5ea1a9a26e708db0 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 POSTDOCTORAL/RESEARCH ASSOCIATE POSITIONS AVAILABLE FOR PROJECTS ON LIGHTING SIMULATION at iMAGIS, Grenoble, FRANCE The iMAGIS research group is part of the French national research organisations CNRS and INRIA, and of Grenoble Universities UJF and INPG. iMAGIS researchers have had a strong presence in the international computer graphics community, regularly publishing at the SIGGRAPH and Eurographics conferences and workshops, as well as in the major scientific journals of the domain. (for more information see http://www-imagis.imag.fr) The iMAGIS research group will be participating in two European Union funded Long Term Research (LTR) projects. These projects are related to radiosity and lighting algorithms, with special focus on making radiosity usable (data acquisition, complex scenes, automatic simulation control and interactive updates) and on developing practical algorithms for extended lighting effects (glossy reflection, participating media). We are searching for two motivated young researchers for a postdoctoral or research associate position. Candidates should hold a Ph.D. or M.Sc. (or equivalents depending on country of origin), specialised in the domain of lighting simulation (radiosity, stochastic methods etc.). Candidates with equivalent experience in the development of lighting simulation software will also be considered. Good spoken and written English skills are a necessity. The duration of this employment will be 2-3 years; the starting date is autumn 1997. The second position could have a later starting date (summer 1998 latest). The timing details are still somewhat flexible at this stage. The persons appointed will be primarily responsible for the production of the LTR deliverables (software, demos, reports and scientific publications), and participating in meetings with partners (in Spain, Germany and the UK). This work will be performed in the context of the research software development effort of iMAGIS, and thus will include an important research-oriented component. The work will be performed in close collaboration with the principal investigators of these projects, Francois Sillion, George Drettakis and Claude Puech. For holders of Ph.D.'s part of their time will be available for personal research in the context of the iMAGIS research group. The distribution of time and responsibilities is negociable and will be adapted individually. Salary will be commensurate with experience; for a postdoctoral position they will be in the standard range of French research organisations postdoc salaries. Candidates interested in these positions should contact either Francois Sillion (Francois.Sillion@imag.fr) or George Drettakis (George.Drettakis@imag.fr). We are also reacheable by FAX at +33 4 76 63 55 80. It will be possible to meet with promising applicants at the SIGGRAPH and Eurographics conferences. Potential candidates are thus encouraged to express interest as soon as possible. -- George Drettakis, Chercheur INRIA Researcher, iMAGIS/GRAVIR/IMAG-INRIA NOTE CHANGE !! C-123 Bat. C, 1er, 220 rue de la chimie, Domaine Universitaire BP 53 F-38041 Grenoble Cedex 09 FRANCE (all info for courier, BP only for post) (en France) tel: 04 76 63 56 46 fax 04 76 63 55 80 tel: (+33) 4 76 63 56 46 fax (+33) 4 76 63 55 80 email: George.Drettakis@imag.fr http://www-imagis.imag.fr/~George.Drettakis +------------------+------------------------------------------------------+ | Francois SILLION | iMAGIS - GRAVIR/IMAG, B.P. 53, 38041 Grenoble Cedex 9| | ' | France. Tel:+33 4 76 51 43 54 - Fax:+33 4 76 63 55 80| +------------------+----------+-------------------------------------------+ | Francois.Sillion@imag.fr | http://w3imagis.imag.fr/~Francois.Sillion | +-----------------------------+-------------------------------------------+ From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id XAA01519; Mon, 7 Jul 1997 23:59:21 +0200 Received: from deliverator.sgi.com (deliverator.sgi.com [204.94.214.10]) by imag.imag.fr (8.8.1/8.8.5) with SMTP id XAA06985 for ; Mon, 7 Jul 1997 23:44:28 +0200 (MET DST) Received: from odin.corp.sgi.com (odin.corp.sgi.com [192.26.51.194]) by deliverator.sgi.com (950413.SGI.8.6.12/951211.SGI.AUTO) via ESMTP id OAA16528; Mon, 7 Jul 1997 14:43:58 -0700 env-from (gregl@radiate.asd.sgi.com) Received: from giraffe.asd.sgi.com by odin.corp.sgi.com via ESMTP (951211.SGI.8.6.12.PATCH1502/951211.SGI) id OAA00745; Mon, 7 Jul 1997 14:43:53 -0700 Received: from radiate.asd.sgi.com by giraffe.asd.sgi.com via ESMTP (951211.SGI.8.6.12.PATCH1502/951211.SGI) id OAA24798; Mon, 7 Jul 1997 14:43:29 -0700 Received: by radiate.asd.sgi.com (950413.SGI.8.6.12/940406.SGI.AUTO) id OAA11921; Mon, 7 Jul 1997 14:43:28 -0700 Date: Mon, 7 Jul 1997 14:43:28 -0700 From: Greg Larson Message-Id: <199707072143.OAA11921@radiate.asd.sgi.com> To: globillum@imag.fr Subject: Re: Siggraph gathering X-UIDL: 291f7f88a45e5db06f7081926c1a3187 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Regarding the earlier proposal to hold the Siggraph '97 Globillum meeting on Thursday at 1pm, Paul Heckbert wrote suggesting that we move up the time so he doesn't have to miss his student's presentation at the 2 o'clock session. Therefore, I'm recommending that those who can convene at: Thursday, August 7th, at 12:30pm, location TBA We'll reserve one of the birds-of-a-feather rooms and mark the time and place on the BOF board that is usually situated near the materials pick-up. Feel free to grab a bite to eat and bring it with you. In years past, we've tried to pick up food for everyone, but usually that's a fiasco, so you're on your own this year. We probably won't get serious until 1 o'clock still, so if you can't make it at 12:30, just come when you can. Hope to see you there! -Greg _____________________________________________________________________ Gregory Ward Larson (the computer artist formerly known as Greg Ward) Silicon Graphics, Inc. Computer Science Department 2011 N. Shoreline Blvd., M/S 07U-553 537 Soda Hall, UC Berkeley Mountain View, CA 94043-1389 Berkeley, CA 94720-1776 (415) 933-4878, -2663 fax (510) 642-3631, -5775 fax gregl@sgi.com on Tues., Thurs. and Fri. ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id UAA17584; Tue, 8 Jul 1997 20:52:33 +0200 Received: from mail1.microsoft.com (mail1.microsoft.com [131.107.3.41]) by imag.imag.fr (8.8.1/8.8.5) with ESMTP id UAA27289 for ; Tue, 8 Jul 1997 20:32:21 +0200 (MET DST) Received: by INET-01-IMC with Internet Mail Service (5.0.1458.49) id <32KF2X21>; Tue, 8 Jul 1997 11:32:19 -0700 Message-ID: <011290D45A8ACF119B8B00805FD471D60349C93C@RED-24-MSG.dns.microsoft.com> From: Andrew Glassner To: "'globillum@imag.fr'" Subject: New errata for PoDIS Date: Tue, 8 Jul 1997 11:32:14 -0700 X-Priority: 3 X-Mailer: Internet Mail Service (5.0.1458.49) X-UIDL: 7513d7674640576b16456d38d5bd2ded X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit I've just updated the errata for Principles of Digital Image Synthesis. You can find the complete list at: http://www.research.microsoft.com/research/graphics/glassner/work/projec ts/pdis/errata.htm --- Andrew Glassner | glassner@microsoft.com | +1(206)703-0120 http://www.research.microsoft.com/research/graphics/glassner/ From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id XAA08879; Wed, 9 Jul 1997 23:37:01 +0200 Received: from redemption.uniserve.com (redemption.uniserve.com [204.191.197.254]) by imag.imag.fr (8.8.1/8.8.5) with SMTP id XAA18106 for ; Wed, 9 Jul 1997 23:20:15 +0200 (MET DST) Received: from ian [204.191.197.48] by redemption.uniserve.com with smtp (Exim 1.62 #1) id 0wm49O-00036j-00; Wed, 9 Jul 1997 14:19:51 -0700 X-Sender: iashdown@pop.uniserve.com X-Mailer: Windows Eudora Version 1.4.4 Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed To: globillum@imag.fr From: Ian Ashdown Subject: More book errata Message-Id: Date: Wed, 9 Jul 1997 14:19:51 -0700 X-UIDL: df9c86837c74538611156c3ae0a880e2 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit For those who might be interested, the errata to "Radiosity: A Programmer's Perspective" (Wiley 1994) is now available from: http://www.ledalite.com/library-/rrt.htm Ian Ashdown, P. Eng. | READ THE BOOK! | Research & Development Manager | Radiosity: A Programmer's Perspective | Ledalite Architectural Products | Wiley & Sons 1994 | Visit http://www.ledalite.com | (Sneaky Internet Advertising) | Book Review: http://www.ercb.com/ddj/1996/ddj.9605.html Book Order: https://www.wiley.com/compbooks/catalog/30444-1.htm Free Software: http://www.ledalite.com/software/software.htm From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id GAA12765; Thu, 10 Jul 1997 06:30:16 +0200 Received: from mercury.uniserve.com (mercury.uniserve.com [204.191.197.248]) by imag.imag.fr (8.8.1/8.8.5) with ESMTP id GAA28711 for ; Thu, 10 Jul 1997 06:27:33 +0200 (MET DST) Received: from helios (van0404.tvs.net [204.191.197.104]) by mercury.uniserve.com with ESMTP id VAA07361 for ; Wed, 9 Jul 1997 21:27:22 -0700 (PDT) Message-Id: <199707100427.VAA07361@mercury.uniserve.com> Reply-To: byheart@acm.org From: "Ian Ashdown" To: globillum@imag.fr Subject: Interesting radiosity papers Date: Wed, 9 Jul 1997 21:28:17 -0700 X-MSMail-Priority: Normal X-Priority: 3 X-Mailer: Microsoft Internet Mail 4.70.1155 MIME-Version: 1.0 Content-Type: text/plain; charset=windows-1252; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: 5aa4970ed62166bb3877f0567ccba0e7 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Papers on global illumination are beginning to appear in some decidedly non-traditional journals. The following two papers (one accepted for publication, the other submitted) may be of interest to some of you: Atkinson, K., and D. Chen. 1997. "A Fast Matrix-Vector Multiplication Method for Solving the Radiosity Equation." Submitted for publication. Atkinson, K., and G. Chandler. 1997. "The Collocation Method for Solving the Radiosity Equation for Unoccluded Surfaces." To appear in Journal of Integral Equations & Applications." Both papers are available in Postscript format from Kendall Atkinson's home page at: http://www.math.uiowa.edu/~atkinson/papers.html For those of you who have thoroughly researched the literature, you may recognize Dr. Kendall as the author of the 1976 book, "A Survey of Numerical Methods for the Solution of Fredholm Intergral Equations of the Second Kind." The above two papers are no less rigorous in their treatment of the subject. - Ian Ashdown From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id XAA20784; Sat, 12 Jul 1997 23:56:28 +0200 Received: from mercury.uniserve.com (mercury.uniserve.com [204.191.197.248]) by imag.imag.fr (8.8.1/8.8.5) with ESMTP id XAA20704 for ; Sat, 12 Jul 1997 23:49:26 +0200 (MET DST) Received: from helios (dy1-41.van.tvs.net [204.244.156.50]) by mercury.uniserve.com with ESMTP id OAA19687 for ; Sat, 12 Jul 1997 14:49:20 -0700 (PDT) Message-Id: <199707122149.OAA19687@mercury.uniserve.com> Reply-To: byheart@acm.org From: "Ian Ashdown" To: globillum@imag.fr Subject: Global illumination bibliography update Date: Sat, 12 Jul 1997 14:50:12 -0700 X-MSMail-Priority: Normal X-Priority: 3 X-Mailer: Microsoft Internet Mail 4.70.1155 MIME-Version: 1.0 Content-Type: text/plain; charset=windows-1252; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: a5a816c3c051e9e44278fc113d1da5ac X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 ANNOUNCE: 97/07/15 Release of RADBIB97.BIB ------------------------------------------ RADBIB97 is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. It currently includes 1,164 references. This bibliography is available in BibTex format as RADBIB97.BIB (with a release date of July 15, 1997) from: http://www.ledalite.com/library-/rrt.htm ftp://ftp.ledalite.com/pub/radbib97.bib As always, it is time-consuming and sometimes difficult to track down conference papers and theses on radiosity and global illumination. If you know of a relevant reference that is not included in the bibliography, please let me know so that I can include it in the next release. Ian Ashdown, P. Eng. | READ THE BOOK! | Research & Development Manager | Radiosity: A Programmer's Perspective | Ledalite Architectural Products | Wiley & Sons 1994 | Visit http://www.ledalite.com | (Sneaky Internet Advertising) | From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id JAA07746; Wed, 16 Jul 1997 09:10:27 +0200 Received: from ux3.sp.cs.cmu.edu (UX3.SP.CS.CMU.EDU [128.2.198.103]) by imag.imag.fr (8.8.1/8.8.5) with SMTP id IAA00561 for ; Wed, 16 Jul 1997 08:47:26 +0200 (MET DST) Received: from GS190.SP.CS.CMU.EDU by ux3.sp.cs.cmu.edu id aa25424; 16 Jul 97 2:46 EDT X-Sender: ajw@ux1.sp.cs.cmu.edu Message-Id: Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed Date: Wed, 16 Jul 1997 02:46:32 -0400 To: globillum@imag.fr From: "Andrew J. Willmott" Subject: More radiosity software... X-UIDL: a27266506749d51c41bd22ca894b4561 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Just a reminder that the radiosity software and experimental system used in our comparison of radiosity methods is available from http://www.cs.cmu.edu/~radiosity/dist. (The comparison was presented at the recent Eurographics Workshop on Rendering.) The software supports matrix, progressive, and wavelet radiosity (bases: M2/M3/F2/F3), T-vertex elimination, and more. The code is set up to compile under Irix, but it should be easily portable to anything with a C++ compiler and an OpenGL library. Cheers, Andrew --- mailto:a.willmott@cs.cmu.edu ------- http://www.cs.cmu.edu/~ajw --- From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id TAA06692; Tue, 22 Jul 1997 19:29:37 +0200 Received: from m1.cs.man.ac.uk (0@m1.cs.man.ac.uk [130.88.13.4]) by imag.imag.fr (8.8.1/8.8.5) with SMTP id PAA06657 for ; Tue, 22 Jul 1997 15:25:17 +0200 (MET DST) Received: from rdf010.cs.man.ac.uk by m1.cs.man.ac.uk (4.1/SMI-4.1:AL6) id AA28172; Tue, 22 Jul 97 14:25:16 BST Date: Tue, 22 Jul 97 14:25:14 BST From: Simon Gibson Message-Id: <9707221325.AA08828@rdf010.cs.man.ac.uk> To: globillum@imag.fr Subject: notations and terminology document X-UIDL: 5edecdd92c49033bc15caed7c0909ed2 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Hello all, I am trying to track down the .ps or .tex file on notations and terminology used for global illumination research that is linked from the Eurographics working group on rendering home page. The ftp link to tiber.nist.gov/pub/holly/symb.tex is dead. Does anybody know if the documents are available from anywhere else? Thanks Simon From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id VAA07575; Tue, 22 Jul 1997 21:43:03 +0200 Received: from igw2.watson.ibm.com (igw2.watson.ibm.com [198.81.209.6]) by imag.imag.fr (8.8.1/8.8.5) with ESMTP id VAA18996 for ; Tue, 22 Jul 1997 21:25:22 +0200 (MET DST) Received: from mailhub1.watson.ibm.com (mailhub1.watson.ibm.com [9.2.249.31]) by igw2.watson.ibm.com (8.8.5/07-11-97) with ESMTP id PAA04906; Tue, 22 Jul 1997 15:24:16 -0400 Received: from watngi01.watson.ibm.com (watngi01.watson.ibm.com [9.2.235.20]) by mailhub1.watson.ibm.com (8.8.2/07-14-97) with SMTP id PAA39819; Tue, 22 Jul 1997 15:25:19 -0400 Received: by watngi01.watson.ibm.com(Lotus SMTP MTA v1.06 (346.4 3-18-1997)) id 852564DC.006AADA5 ; Tue, 22 Jul 1997 15:25:12 -0400 X-Lotus-FromDomain: IBM RESEARCH From: "Holly Rushmeier" To: gibsons@cs.man.ac.uk cc: globillum@imag.fr Message-ID: <852564DC.00697E94.00@watngi01.watson.ibm.com> Date: Tue, 22 Jul 1997 15:23:49 -0400 Subject: Re: notations and terminology document Mime-Version: 1.0 Content-type: text/plain; charset=us-ascii; format=flowed X-UIDL: ea14235904f96ff19f3a31626cfddfd1 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hi -- The files on tiber.nist.gov/pub/holly left NIST when I did. I still have the files, but I can't make them available via ftp because of the fire wall here. I'm emailing symb.tex to Simon. If anyone has a site where they can keep the documents I will be happy to email them to you, and the Eurographics links can be updated. -- Holly From: gibsons @ cs.man.ac.uk Date: 07/22/97 02:25:14 PM CET Subject: notations and terminology document Hello all, I am trying to track down the .ps or .tex file on notations and terminology used for global illumination research that is linked from the Eurographics working group on rendering home page. The ftp link to tiber.nist.gov/pub/holly/symb.tex is dead. Does anybody know if the documents are available from anywhere else? Thanks Simon From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id XAA09152; Tue, 22 Jul 1997 23:32:13 +0200 Received: from safran.imag.fr (safran.imag.fr [129.88.42.9]) by imag.imag.fr (8.8.1/8.8.5) with ESMTP id XAA22021; Tue, 22 Jul 1997 23:20:47 +0200 (MET DST) Received: (from sillion@localhost) by safran.imag.fr (8.6.10/8.6.9) id XAA14356; Tue, 22 Jul 1997 23:20:46 +0200 From: Francois Sillion Message-Id: <199707222120.XAA14356@safran.imag.fr> Subject: Re: notations and terminology document To: Holly Rushmeier Date: Tue, 22 Jul 1997 23:20:46 +0200 (MDT) Cc: gibsons@cs.man.ac.uk, globillum@imag.fr In-Reply-To: <852564DC.00697E94.00@watngi01.watson.ibm.com> from "Holly Rushmeier" at Jul 22, 97 03:23:49 pm Reply-To: Francois.Sillion@imag.fr X-Mailer: ELM [version 2.4 PL24] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: d8469b15cbd3c97a3794c52a86597142 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Sorry about this, I do have the files and putting them on our ftp server is on my todo list... I will do that tomorrow! > > Hi -- > The files on tiber.nist.gov/pub/holly left NIST when I did. > I still have the files, but I can't make them available via ftp because > of the fire wall here. I'm emailing symb.tex to Simon. If anyone has > a site where they can keep the documents I will be happy to email > them to you, and the Eurographics links can be updated. > > -- Holly > > +------------------+------------------------------------------------------+ | Francois SILLION | iMAGIS - GRAVIR/IMAG, B.P. 53, 38041 Grenoble Cedex 9| | ' | France. Tel:+33 4 76 51 43 54 - Fax:+33 4 76 63 55 80| +------------------+----------+-------------------------------------------+ | Francois.Sillion@imag.fr | http://w3imagis.imag.fr/~Francois.Sillion | +-----------------------------+-------------------------------------------+ From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id LAA15486; Fri, 25 Jul 1997 11:41:01 +0200 Received: from safran.imag.fr (safran.imag.fr [129.88.42.9]) by imag.imag.fr (8.8.1/8.8.5) with ESMTP id KAA02024 for ; Fri, 25 Jul 1997 10:49:19 +0200 (MET DST) Received: (from sillion@localhost) by safran.imag.fr (8.6.10/8.6.9) id KAA10215 for globillum@imag.fr; Fri, 25 Jul 1997 10:49:18 +0200 From: Francois Sillion Message-Id: <199707250849.KAA10215@safran.imag.fr> Subject: Think about it... To: Global Illumination List Date: Fri, 25 Jul 1997 10:49:18 +0200 (MDT) Reply-To: Francois.Sillion@imag.fr X-Mailer: ELM [version 2.4 PL24] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: c9eb77c3880421a577f16dc7e78866fb X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hi globillumers, We are still looking for post-docs, in the next three years. I will be at SIGGRAPH and could talk to interested people. So if you are finishing a PhD soon, or if you want some change in your life, and if you like the beautiful mountains of the french alps, think about it... > POSTDOCTORAL/RESEARCH ASSOCIATE POSITIONS > AVAILABLE FOR PROJECTS ON LIGHTING SIMULATION > at iMAGIS, Grenoble, FRANCE > > The iMAGIS research group is part of the French national research > organisations CNRS and INRIA, and of Grenoble Universities UJF and > INPG. iMAGIS researchers have had a strong presence in the > international computer graphics community, regularly publishing at the > SIGGRAPH and Eurographics conferences and workshops, as well as in the > major scientific journals of the domain. > (for more information see http://www-imagis.imag.fr) > > The iMAGIS research group will be participating in two European Union > funded Long Term Research (LTR) projects. These projects are related > to radiosity and lighting algorithms, with special focus on making > radiosity usable (data acquisition, complex scenes, automatic > simulation control and interactive updates) and on developing practical > algorithms for extended lighting effects (glossy reflection, > participating media). > > We are searching for two motivated young researchers for a postdoctoral > or research associate position. Candidates should hold a Ph.D. or > M.Sc. (or equivalents depending on country of origin), specialised in > the domain of lighting simulation (radiosity, stochastic methods > etc.). Candidates with equivalent experience in the development of > lighting simulation software will also be considered. Good spoken and > written English skills are a necessity. > > The duration of this employment will be 2-3 years; the starting date is > autumn 1997. The second position could have a later starting date > (summer 1998 latest). The timing details are still somewhat flexible > at this stage. > > The persons appointed will be primarily responsible for the production > of the LTR deliverables (software, demos, reports and scientific > publications), and participating in meetings with partners (in Spain, > Germany and the UK). This work will be performed in the context of the > research software development effort of iMAGIS, and thus will include > an important research-oriented component. The work will be performed > in close collaboration with the principal investigators of these > projects, Francois Sillion, George Drettakis and Claude Puech. > > For holders of Ph.D.'s part of their time will be available for > personal research in the context of the iMAGIS research group. The > distribution of time and responsibilities is negociable and will be > adapted individually. > > Salary will be commensurate with experience; for a postdoctoral > position they will be in the standard range of French research > organisations postdoc salaries. > > Candidates interested in these positions should contact either Francois > Sillion (Francois.Sillion@imag.fr) or George Drettakis > (George.Drettakis@imag.fr). We are also reacheable by > FAX at +33 4 76 63 55 80. > > It will be possible to meet with promising applicants at the SIGGRAPH > and Eurographics conferences. Potential candidates are thus encouraged > to express interest as soon as possible. > +------------------+------------------------------------------------------+ | Francois SILLION | iMAGIS - GRAVIR/IMAG, B.P. 53, 38041 Grenoble Cedex 9| | ' | France. Tel:+33 4 76 51 43 54 - Fax:+33 4 76 63 55 80| +------------------+--------+---------------------------------------------+ | Francois.Sillion@imag.fr | http://www-imagis.imag.fr/~Francois.Sillion | +---------------------------+---------------------------------------------+ From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id QAA18741; Fri, 25 Jul 1997 16:44:02 +0200 Received: from safran.imag.fr (safran.imag.fr [129.88.42.9]) by imag.imag.fr (8.8.1/8.8.5) with ESMTP id QAA15050; Fri, 25 Jul 1997 16:13:48 +0200 (MET DST) Received: (from sillion@localhost) by safran.imag.fr (8.6.10/8.6.9) id QAA17064; Fri, 25 Jul 1997 16:13:47 +0200 From: Francois Sillion Message-Id: <199707251413.QAA17064@safran.imag.fr> Subject: Re: notations and terminology document To: Roland Schregle Date: Fri, 25 Jul 1997 16:13:47 +0200 (MDT) Cc: Global Illumination List In-Reply-To: <9707251441.ZM15061@jupiter.informatik.uni-bonn.de> from "Roland Schregle" at Jul 25, 97 12:41:27 pm Reply-To: Francois.Sillion@imag.fr X-Mailer: ELM [version 2.4 PL24] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: 9828cf1d4ec766ce07ec0f0617b221ca X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hi, I placed links to the documents on the EG working group on rendering's page. (http://www-imagis.imag.fr/Membres/Francois.Sillion/egwkgr.html). the links point to the following ftp area: ftp://www-imagis.imag.fr/pub/sillion/EGwkgr/... > Hi Francois, > > I checked the /doc directory of your ftp site (ftp.imag.fr) but didn't find the > documents pertaining to radiometric terms. Where can I find them? > > > Roland Schregle > +------------------+------------------------------------------------------+ | Francois SILLION | iMAGIS - GRAVIR/IMAG, B.P. 53, 38041 Grenoble Cedex 9| | ' | France. Tel:+33 4 76 51 43 54 - Fax:+33 4 76 63 55 80| +------------------+--------+---------------------------------------------+ | Francois.Sillion@imag.fr | http://www-imagis.imag.fr/~Francois.Sillion | +---------------------------+---------------------------------------------+ From To: Francois.Sillion@imag.fr From: Werner Purgathofer Subject: Re: notations and terminology document Message-Id: In-Reply-To: <199707251413.QAA17064@safran.imag.fr> References: <9707251441.ZM15061@jupiter.informatik.uni-bonn.de> from "Roland Schregle" at Jul 25, 97 12:41:27 pm X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Date: Mon, 28 Jul 1997 14:37:22 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Dear Francois, following your email to globillum I have browsed the Rendering Group page and want to propose to you to add the following links: http://www.springer.co.at/books/book.phtml?id_cat=3&id=15 http://www.springer.co.at/books/book.phtml?id_cat=3&id=155 http://www.springer.co.at/books/book.phtml?id_cat=3&id=337 which are information on the Rendering Workshop Proceedings 95, 96, 97 from Springer-Verlag. See you soon! Werner >Hi, > >I placed links to the documents on the EG working group on rendering's page. >(http://www-imagis.imag.fr/Membres/Francois.Sillion/egwkgr.html). > >the links point to the following ftp area: > > ftp://www-imagis.imag.fr/pub/sillion/EGwkgr/... > >> Hi Francois, >> >> I checked the /doc directory of your ftp site (ftp.imag.fr) but didn't find the >> documents pertaining to radiometric terms. Where can I find them? >> >> >> Roland Schregle >> > >+------------------+------------------------------------------------------+ >| Francois SILLION | iMAGIS - GRAVIR/IMAG, B.P. 53, 38041 Grenoble Cedex 9| >| ' | France. Tel:+33 4 76 51 43 54 - Fax:+33 4 76 63 55 80| >+------------------+--------+---------------------------------------------+ >| Francois.Sillion@imag.fr | http://www-imagis.imag.fr/~Francois.Sillion | >+---------------------------+---------------------------------------------+ From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id HAA16739; Fri, 1 Aug 1997 07:18:45 +0200 Received: from mercury.uniserve.com (mercury.uniserve.com [204.191.197.248]) by imag.imag.fr (8.8.1/8.8.5) with ESMTP id HAA27883 for ; Fri, 1 Aug 1997 07:12:09 +0200 (MET DST) Received: from helios (p2-31.van.tvs.net [204.244.158.158]) by mercury.uniserve.com with ESMTP id WAA03598; Thu, 31 Jul 1997 22:11:48 -0700 (PDT) Message-Id: <199708010511.WAA03598@mercury.uniserve.com> Reply-To: byheart@acm.org From: "Ian Ashdown" To: globillum@imag.fr Cc: judy-brown@uiowa.edu Subject: ANNOUNCE - Global Illumination Bibliography Project Date: Thu, 31 Jul 1997 22:12:38 -0700 X-MSMail-Priority: Normal X-Priority: 3 X-Mailer: Microsoft Internet Mail 4.70.1155 MIME-Version: 1.0 Content-Type: text/plain; charset=windows-1252; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: e8f7af382e30fe5cb27b21d48fa75600 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 ANNOUNCE - Global Illumination Bibliography Project --------------------------------------------------- The SIGGRAPH Special Projects Committee has awarded a grant of $1,500 in support of the Global Illumination Bibliography project. This funding will go towards the purchase of academic journals, subscriptions, and conference proceedings for two years, plus photocopying and mailing charges. The Global Illumination Bibliography project is perhaps better known as Eric Haines' original RADBIB radiosity bibliography, now called RADBIB97 and maintained as a public service for the computer graphics community by Ian Ashdown (byHeart Consultants Limited). It currently contains 1,165 references to global illumination papers, articles, books, and theses. (Oops, make that 1,187 -- another 22 references from 1927 through 1974 appeared on my desk today.) RADBIB97 is available from http://www.ledalite.com and other Web and ftp sites worldwide (including SIGGRAPH). What I have not previously announced in public is that I have an extensive collection of the publications referenced in RADBIB97. I have not counted the holdings recently, but they currently fill 25 two-inch ring binders. This is an offer to all globillum subscribers: if you see anything of interest in RADBIB97 that you cannot obtain through your interlibrary loan services, please send me an e-mail request. The chances are good that I will have it in my collection or know where you can obtain an electronic copy. For out-of-print material from hard-to-find journals and conference proceedings, I can likely send you a scanned copy by e-mail or ftp, or (worst-case scenario) a photocopy via the Canadian Postal Disservice. (Books and full-length theses are an exception, of course.) And with this, I would like to thank the SIGGRAPH Special Projects Committee on behalf of the globillum mailing subscribers for their generous support of the Global Illumination Bibliography project. Ian Ashdown, P. Eng. | READ THE BOOK! | Research & Development Manager | Radiosity: A Programmer's Perspective | Ledalite Architectural Products | Wiley & Sons 1994 | Visit http://www.ledalite.com | (Sneaky Internet Advertising) | Book Review: http://www.ercb.com/ddj/1996/ddj.9605.html Book Order: https://www.wiley.com/compbooks/catalog/30444-1.htm Free Software: http://www.ledalite.com/software/software.htm From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id LAA01359; Tue, 12 Aug 1997 11:19:41 +0200 Received: from sgi.sgi.com (SGI.COM [192.48.153.1]) by imag.imag.fr (8.8.1/8.8.5) with SMTP id UAA10346 for ; Mon, 11 Aug 1997 20:52:47 +0200 (MET DST) Received: from cthulhu.engr.sgi.com (cthulhu.engr.sgi.com [192.26.80.2]) by sgi.sgi.com (950413.SGI.8.6.12/970507) via ESMTP id LAA06259; Mon, 11 Aug 1997 11:52:44 -0700 env-from (gregl@radiate.engr.sgi.com) Received: from radiate.engr.sgi.com (radiate.engr.sgi.com [192.26.72.11]) by cthulhu.engr.sgi.com (950413.SGI.8.6.12/960327.SGI.AUTOCF) via ESMTP id LAA23445; Mon, 11 Aug 1997 11:52:43 -0700 Received: (from gregl@localhost) by radiate.engr.sgi.com (950413.SGI.8.6.12/960327.SGI.AUTOCF) id LAA27541; Mon, 11 Aug 1997 11:52:42 -0700 Date: Mon, 11 Aug 1997 11:52:42 -0700 From: Greg Larson Message-Id: <199708111852.LAA27541@radiate.engr.sgi.com> To: globillum@imag.fr Subject: Siggraph Globillum Meeting Cc: drb@sgi.com X-UIDL: e7971cf67a588fad6d16f4d11687ca7a X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Well, since no one volunteered to take notes at the Globillum meeting on Thursday at Siggraph, you're stuck with my ratty minutes again this year. There was some confusion on the time for the meeting -- some thought it was to start at 12:30, and some thought 1:00. Since the judges of the all-important Siggraph T-shirt contest had the room until 1:00, the few of us who showed up at 12:30 went around and (re)introduced ourselves outside while we waited for the room and for the others to arrive. By the time 1pm rolled around, there were quite a few of us who had been introduced, and folks were still trickling into the room, so I apologize that not everyone got a proper chance to hear the early birds' names. We had quite a turnout this year, and I attempted to get everyone's names down, but I'm sure I missed a few (and misspelled a few more). Nevertheless, I've included this list of names at the bottom, in case you find a friend there who can tell you about the meeting first-hand. After the aforementioned haphazard introductions, Fern Hunt of the National Institute of Standards and Technology gave a scheduled presentation of the work she is doing on BRDF measurement and characterization with Mary McKnight and others at NIST, in cooperation with industry. Dr. Hunt is one of a few mathematicians at NIST who are attempting to predict BRDFs (bidirectional reflection distribution functions) from paint compositions and application techniques. Specifically, they are asking the question, "If you have some material, and you know its physical characteristics and topography, what else do you need to know to recreate its appearance; what accuracy levels are needed?" NIST of course has some of the most (if not THE most) sophisticated equipment for measuring surface reflectance and topography, and they are very interested in working with industry and research institutions to make this information more useful and available. Bob Lipman (also of NIST) then talked about a newly available database of BRDFs for various common materials, collected by the CIA for use in analyzing satellite images. Recently declassified (and simultaneously defunded), the NEF database (obviously stands for "Nonconventional Exploitation Factors") contains hundreds(?) of exterior finishes and natural materials, characterized by full spectral reflectance models and measurements. It was meticulously created by the National Imaging and Mapping Agency, and represents a huge effort. I strongly recommend to anyone interested in material reflectance data that they go check it out. For more information, see the following web sites: http://math.nist.gov/mcsd/Staff/RLipman/appearance/ http://math.nist.gov/mcsd/Staff/RLipman/brdf/nefhome.html The interface to the database currently runs only under Solaris, and Bob is looking to create a simpler interface to access the data under other systems, as well as seeing if the current interface can be ported. (His initial attempts to do so failed for unknown reasons.) Fern Hunt can be reached at , (301) 975-3887. Bob Lipman is at , (301) 975-3829. Fern also reminded the group that they are still looking for someone for a post-doc position in realistic image synthesis funded by the National Research Council, for which they are taking applications until Jan. 15, 1998. They promised to have an announcement soon at the following URL: http://rap.nas.edu/lab/NIST/ (Bear in mind that there is a U.S. citizenship requirement for this position.) Next, I brought up a subject that has been popular at past globillum meetings, which is lighting and level of realism in the entertainment (i.e., film animation) industry. Specifically, I was wondering why global illumination is not more widely used for producing digital effects, which to my eye still look pretty fake due to poor lighting and color. Larry Gritz (of Pixar) had quite a bit to say on this topic, since he has spent some time on both sides of the fence. As the author of the Blue Moon Rendering Tools, Larry knows that global illumination techniques can be quite effective at improving the realism of rendered environments, even within the Renderman specification. However, he has seen expert "lighters," as they're called, do a much better job producing convincing effects for movies like "Toy Story" without any kind of global calculations going on. In fact, Larry said that global effects can often be exactly what you DON'T want when lighting a scene, since the addition of a light in one corner can screw up the lighting you just tweaked to perfection in the other corner. Alain Fournier of the University of British Columbia and Mayur Patel of Disney Engineering also participated in the conversation (among others), and in the end there seemed to be some agreement that there is a lot of room for improvement in existing animation systems. Specifically, there must be some way to ease the burden lighting places on scene design with better global illumination that still does not diminish creative control. Anything they can do to keep the computer graphics from jumping off the screen and saying "Hey, I was done with computer graphics!" would be great by me. Finally, Paul Heckbert (of Carnegie Mellon University) brought up the issue of code sharing, and suggested that we post announcements to the group if we have some code or results we want to share via the internet. No one seemed to object to this, given how light traffic on globillum usually is. Anyway, to get the ball rolling, here are a few links that people volunteered: Wavelet Radiosity Testbed (Andrew Wilmott): http://www.cs.cmu.edu/~radiosity/dist/ Interactive BRDF editor (Paul Heckbert and students): http://www.cs.cmu.edu/~ph/src/illum/ BRDF comparison (Szymon Rusinkiewicz): http://www-graphics.stanford.edu/~smr/cs348c/paper.html Blue Moon Rendering Tools (Larry Gritz): http://www.seas.gwu.edu/student/gritz/bmrt.html Instant Radiosity (Alex Keller -- see Siggraph '97 paper): http://www.uni-kl.de/AG-Heinrich/Alex.html (Actually, I couldn't find the link, but Alex said he had one.) Validation studies (Karol Myszkowski): http://www.u-aizu.ac.jp/~k-myszk/valid Radiance (how could I miss the opportunity for a plug?): http://radsite.lbl.gov/radiance/HOME.html Materials and Geometry Format (ditto): http://radsite.lbl.gov/mgf/HOME.html Also, I plan to announce a high dynamic-range format within TIFF for images using a logL (u',v') color system in 32-bits/pixel, which is even better than the one used in Radiance since it is not gamut-limited. This will be released as part of Sam Leffler's TIFF library. I hope to have it ready (with an X11 viewer) by the end of this month. And now, the list of attendees in alfabetickal order: Ashdown, Ian (ByHeart Software) Bala, Kavita (MIT) Baranoski, Gladimir Christensen, Per (Mental Ray) Fajardo, Marco Foo, Sing (Blue Sky Studios) Fournier, Alain (Univ. of British Columbia) Gatenby, Niel (LightWorks) Gritz, Larry (Pixar) Haines, Eric (Autodesk) Hanrahan, Pat (Stanford Univ.) Heckbert, Paul (Carnegie Mellon Univ.) Heidrich, Wolfgang (University of Erlangen) Herf, Michael (Carnegie Mellon Univ.) Hunt, Fern (NIST) Keller, Alex (Universitat Kaiserslautern) Kolb, Craig (Stanford) LaFortune, Eric (Cornell Univ.) Larson, Greg (SGI) Lipman, Bob (NIST) Marshner, Steve Max, Nelson (LLL and UC Davis) Meyer, Gary (Univ. of Oregon) Myszkowski, Karol (Univ. of Aizu) Patel, Mayur (Disney Engineering) Patow, Glastvo Pattanaik, Sumant (Cornell Univ.) Phar, Matt (Stanford Univ.) Ruff, Barry (RIT?) Rushmeier, Holly (IBM T.J. Watson Research) Rushwold, Andrew Rusinkiewicz, Szymon (Stanford Univ.) Shirley, Pete (Univ. of Utah) Sillion, Francois (IMAGIS, University of Grenoble) Slusallek, Phillipp (University of Erlangen) Stuerzling, Wolfgang (Austria) Tamstorf, Rasmus Uselton, Sam (NASA) Van Wensen, Henrik (Mental Ray) Van Wyk, Skip (Univ. of New Mexico) Veach, Eric (Stanford Univ.) Wade, Bretton (SGI) Waltner, Bruce (Cornell Univ.) Westin, Steve (Cornell University) Wilmott, Andrew (Carnegie Mellon Univ.) Worley, Steve Zimmerman, Kurt (Indiana Univ.) Forgive me if I munged your name or forgot your affiliation, or missed you altogether! Take it as an excuse to send mail to globillum with a correction and a little information on your interests and background.... All the best, -Greg _____________________________________________________________________ Gregory Ward Larson (the computer artist formerly known as Greg Ward) Silicon Graphics, Inc. Computer Science Department 2011 N. Shoreline Blvd., M/S 07U-553 537 Soda Hall, UC Berkeley Mountain View, CA 94043-1389 Berkeley, CA 94720-1776 (415) 933-4878, -2663 fax (510) 642-3631, -5775 fax gregl@sgi.com on Tues., Thurs. and Fri. ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id UAA08126; Tue, 12 Aug 1997 20:35:00 +0200 Received: from bcgn.grignon.inra.fr (bcgn.grignon.inra.fr [192.93.95.1]) by imag.imag.fr (8.8.1/8.8.5) with ESMTP id MAA29436 for ; Tue, 12 Aug 1997 12:09:22 +0200 (MET DST) Received: from ultra2 (ultra2 [192.93.95.4]) by bcgn.grignon.inra.fr (8.8.4/8.8.4) with SMTP id MAA03214 for ; Tue, 12 Aug 1997 12:09:15 +0200 (MET DST) Sender: chelle@bcgn.grignon.inra.fr Message-ID: <33F035D0.76BD@bcgn.grignon.inra.fr> Date: Tue, 12 Aug 1997 11:07:12 +0100 From: Michael Chelle X-Mailer: Mozilla 3.0 (X11; I; SunOS 5.5.1 sun4u) MIME-Version: 1.0 To: globillum@imag.fr Subject: Distance point-triangle Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: 0d23f6005bcf58a1a46900efa7b95a0e X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Is there a formula or an efficient algorithm to compute the distance between a point and a triangle (ie the minimum distance)? Thanks in advance Michael -- Michael CHELLE INRA | email : chelle@bcgn.grignon.inra.fr Station de Bioclimatologie | phone : +33 1 30 81 55 31 78850 THIVERVAL-GRIGNON (France) | fax : +33 1 30 81 55 63 From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id KAA15114; Wed, 13 Aug 1997 10:55:47 +0200 Received: from uni-kl.de (mmdf@news.uni-kl.de [131.246.136.51]) by imag.imag.fr (8.8.1/8.8.5) with SMTP id KAA03160 for ; Wed, 13 Aug 1997 10:07:13 +0200 (MET DST) Received: from uklirb.informatik.uni-kl.de by news.uni-kl.de id af06589; 13 Aug 97 10:07 MET DST Received: from irz1.informatik.uni-kl.de by uklirb.informatik.uni-kl.de id aa16784; 13 Aug 97 10:01 MET DST Received: by irz1.informatik.uni-kl.de (SMI-8.6/SMI-SVR4) id KAA17572; Wed, 13 Aug 1997 10:01:33 +0200 From: Alexander Keller AG Heinrich Message-Id: <199708130801.KAA17572@irz1.informatik.uni-kl.de> Subject: Re: SIGGRAPH GlobIllum Meeting To: globillum@imag.fr Date: Wed, 13 Aug 1997 10:01:33 +0200 (MET DST) X-Mailer: ELM [version 2.4 PL24] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: 7cdd43aeeb2700f712fb432b7d9a34a2 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hi! Since I returned from SIGGRAPH yesterday, I was not able to supply the link to my CAL-content on Instant Radiosity earlier. On my page on reports and software you can download the CAL-content as presented on SIGGRAPH 97. The software will run on any system larger or equal to an SGI O2. Note that the speed of the demo software could be improved even more if shadow maps, display lists, etc. were applied. The file cal.tar.gz is installed by creating a directory and un-tar-ing the file in that directory. Then netscape is started, where a bried explanation of the algorithm and how to run it is supplied. The link to the software page is http://www.uni-kl.de/AG-Heinrich/Software.html Have fun testing Instant Radiosity... Best regards, Alex -- Alexander Keller | FB Informatik, Geb. 36/212 | Tel.: +49-631-205-3345 Universitaet Kaiserslautern | Fax.: +49-631-205-3270 Postfach 3049 | keller@informatik.uni-kl.de D-67653 Kaiserslautern, GERMANY | http://www.uni-kl.de/AG-Heinrich/Alex.html From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id OAA17302; Wed, 13 Aug 1997 14:00:58 +0200 Received: from mtigwc03.worldnet.att.net (mtigwc03.worldnet.att.net [204.127.131.34]) by imag.imag.fr (8.8.1/8.8.5) with ESMTP id NAA10820 for ; Wed, 13 Aug 1997 13:43:08 +0200 (MET DST) Received: from espresso ([207.147.208.138]) by mtigwc03.worldnet.att.net (post.office MTA v2.0 0613 ) with SMTP id AAA8025; Wed, 13 Aug 1997 11:42:06 +0000 Received: by localhost with Microsoft MAPI; Wed, 13 Aug 1997 16:40:29 -0700 Message-ID: <01BCA807.9BCD6D20@mherf@worldnet.att.net> From: Michael Herf Reply-To: "herf@cmu.edu" To: "'Alexander Keller AG Heinrich'" , "'globillum@imag.fr'" Subject: RE: SIGGRAPH GlobIllum Meeting Date: Wed, 13 Aug 1997 16:39:54 -0700 X-Mailer: Microsoft Internet E-mail/MAPI - 8.0.0.4008 MIME-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: d9e1e5fd7c8fcab67b78aa739757133d X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hi Alex. I was at your demo directly after the papers session at SIGGRAPH. My first question: Is the reason that an O2 is required the stencil planes or the accumulation buffer speed? With regards to the accumulation buffer, I just wrote a special-case version at work that runs on PCs. The accumulation buffer in OpenGL handles arbitrary combinations of images, and each time glAccum is called it converts the pixels to floating-point format and then does a multiply per pixel to add them -- not too efficient! (Some implementations may optimize this in integer, but the multiply remains.) If you instead assume that you just want to "average" a number of images equally -- the most common case for the accumulation buffer -- you can implement the same thing in software (using glReadPixels to read into a local buffer) with very good performance. My implementation is doing better than 30 accumulation buffer operations per second (a special case of glAccum) at 640x480 in 24-bit RGB, which is more than enough for decent results with your algorithm. The basic idea is to restrict yourself to one or two adds per pixel, and then make the return step do an optimized scale to average the output. (This requires a 16-16-16 bit intermediate image. All this work doesn't buy you anything on a RealityEngine, but it might be cool to see a port to lower-end machines. I think that performance wouldn't hinder you, since $400 cards on the PC can double the O2's polygon performance in many cases. thanks, mike On Wednesday, August 13, 1997 1:02 AM, Alexander Keller AG Heinrich [SMTP:keller@informatik.uni-kl.de] wrote: > Hi! > > Since I returned from SIGGRAPH yesterday, I was not able to > supply the link to my CAL-content on Instant Radiosity > earlier. On my page on reports and software you can download > the CAL-content as presented on SIGGRAPH 97. The software > will run on any system larger or equal to an SGI O2. Note > that the speed of the demo software could be improved even > more if shadow maps, display lists, etc. were applied. > The file cal.tar.gz is installed by creating a directory > and un-tar-ing the file in that directory. Then netscape > is started, where a bried explanation of the algorithm > and how to run it is supplied. > > The link to the software page is > > http://www.uni-kl.de/AG-Heinrich/Software.html > > > Have fun testing Instant Radiosity... > > Best regards, > Alex > -- > Alexander Keller | > FB Informatik, Geb. 36/212 | Tel.: +49-631-205-3345 > Universitaet Kaiserslautern | Fax.: +49-631-205-3270 > Postfach 3049 | keller@informatik.uni-kl.de > D-67653 Kaiserslautern, GERMANY | http://www.uni-kl.de/AG-Heinrich/Alex.html From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id UAA00517; Tue, 19 Aug 1997 20:56:40 +0200 Received: from austin.cs.unc.edu (austin.cs.unc.edu [152.2.128.87]) by imag.imag.fr (8.8.1/8.8.5) with SMTP id UAA05949 for ; Tue, 19 Aug 1997 20:42:08 +0200 (MET DST) Received: from catfish.cs.unc.edu by austin.cs.unc.edu (8.6.10/UNC_10_05_96) id OAA25751; Tue, 19 Aug 1997 14:42:06 -0400 Received: from localhost (localhost [127.0.0.1]) by catfish.cs.unc.edu (8.8.6/8.8.6) with SMTP id OAA17005 for ; Tue, 19 Aug 1997 14:42:05 -0400 (EDT) Date: Tue, 19 Aug 1997 14:42:03 -0400 (EDT) From: Wolfgang Stuerzlinger To: globillum@imag.fr Subject: Software announcement (+small correction) Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII; format=flowed X-UIDL: f849a35992bfdb106ed0a5e93e0af1f0 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit My (correct) name is Wolfgang Stuerzlinger and I am currently a visiting post-graduate researcher at UNC Chapel Hill (originally from Univ. Linz, Austria, so Greg's entry is almost correct :-). My WWW-page is at: http://www.cs.unc.edu/~stuerzl. Parts of my globillum code (e.g. hemispherical projection, discontinuity meshing) and almost all my publications are available there. Wolfgang P.S.: My current entry on reseach interests in globillum reads: In the area of globillum I am doing research on hardware accelerated methods for displaying results of diffuse+glossy+mirror globillum simulations. Also I am interested in hardware accelerated methods for solving the rendering equation. -- Wolfgang Stuerzlinger Dept. of Computer Science, UNC, Chapel Hill, NC 27599-3175 stuerzl@cs.unc.edu http://www.cs.unc.edu/~stuerzl From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id TAA28205; Thu, 28 Aug 1997 19:30:19 +0200 Received: from pink.lbl.gov (pink.lbl.gov [128.3.12.112]) by imag.imag.fr (8.8.1/8.8.5) with SMTP id TAA00871 for ; Thu, 28 Aug 1997 19:10:31 +0200 (MET DST) Received: (from greg@localhost) by pink.lbl.gov (950413.SGI.8.6.12/950213.SGI.AUTOCF) id KAA05425 for globillum@imag.fr; Thu, 28 Aug 1997 10:12:15 -0700 Date: Thu, 28 Aug 1997 10:12:15 -0700 From: "Gregory W. Larson" Message-Id: <199708281712.KAA05425@pink.lbl.gov> To: globillum@imag.fr Subject: Radiosity for Virtual Reality Systems X-UIDL: d90adb7d5b93b6dd93355d3a9b36f2fb X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit This would seem to be of general interest: >>From tralvex@computer.org Thu Aug 28 04:22:17 1997 Received: from sgi.sgi.com (SGI.COM [192.48.153.1]) by pink.lbl.gov (950413.SGI.8.6.12/950213.SGI.AUTOCF) via ESMTP id EAA05170 for ; Thu, 28 Aug 1997 04:22:06 -0700 Received: from cthulhu.engr.sgi.com (cthulhu.engr.sgi.com [192.26.80.2]) by sgi.sgi.com (950413.SGI.8.6.12/970507) via ESMTP id EAA13785 for <@sgi.engr.sgi.com:greg@pink.lbl.gov>; Thu, 28 Aug 1997 04:20:07 -0700 env-from (tralvex@computer.org) Received: from radiate.engr.sgi.com (radiate.engr.sgi.com [192.26.72.11]) by cthulhu.engr.sgi.com (950413.SGI.8.6.12/960327.SGI.AUTOCF) via ESMTP id EAA05245 for <@cthulhu.engr.sgi.com:greg@pink.lbl.gov>; Thu, 28 Aug 1997 04:20:00 -0700 Received: from giraffe.asd.sgi.com (giraffe.asd.sgi.com [192.26.72.158]) by radiate.engr.sgi.com (950413.SGI.8.6.12/960327.SGI.AUTOCF) via ESMTP id EAA15911 for ; Thu, 28 Aug 1997 04:19:50 -0700 Received: from sgi.sgi.com by giraffe.asd.sgi.com via ESMTP (951211.SGI.8.6.12.PATCH1502/951211.SGI) for id EAA23105; Thu, 28 Aug 1997 04:19:45 -0700 Received: from csunb0.leeds.ac.uk (csunb0.leeds.ac.uk [129.11.144.2]) by sgi.sgi.com (950413.SGI.8.6.12/970507) via ESMTP id EAA13739 for ; Thu, 28 Aug 1997 04:19:43 -0700 env-from (tralvex@computer.org) Received: from cspcx20 (cspcx20.leeds.ac.uk [129.11.147.20]) by csunb0.leeds.ac.uk (8.6.12/8.6.12) with SMTP id MAA11559; Thu, 28 Aug 1997 12:00:10 +0100 Message-Id: <2.2.32.19970828095907.0060e4dc@csirisa> X-Sender: mscytsy@csirisa X-Mailer: Windows Eudora Pro Version 2.2 (32) Mime-Version: 1.0 Content-Type: text/plain; charset="us-ascii" Date: Thu, 28 Aug 1997 10:59:07 +0100 To: iashdown@ledalite.com, renambot@irisa.fr, fiction@pressroom.com, alz@lanminds.com, ali@eel.ufl.edu, pawel@assari.cc.tut.fi, vlad@hops.cs.jhu.edu, accmdq@mail.telepac.pt, gregl@sgi.com, abraham@sp.ac.sg, neil@lightwork.co.uk, ttwong@unixg.ubc.ca, Wim.Dumon@cs.kuleuven.ac.be, mart@dcre.leeds.ac.uk, rcl@scs.leeds.ac.uk, wbt@graphics.cornell.edu, bes@phoenix.cs.utah.edu, dpg@graphics.cornell.edu, eric@graphics.cornell.edu, pmh@monk.cs.wustl.edu, gibsons@cs.man.ac.uk From: "Tralvex Yeap (T.Rex)" Subject: Radiosity for Virtual Reality Systems and Huge links Status: R Hi guys, I have finish my MSc thesis and have setup a permanant website for that over at University of Leeds - http://dream.leeds.ac.uk/cuddles/rover The site contains the thesis itself, images, hyperlink abstracts and biblio., huge collection of links on radiosity papers on the Web, free radiosity software on the web, and many others. Thanks for everything and I hope you'll find the resources compiled there useful for your work. Best Regards, - t - tralvex@computer.org * http://www.singnet.com.sg/~tyeap "Give to the world the best you have and the best will come back to you" From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id UAA10173; Fri, 29 Aug 1997 20:50:30 +0200 Received: from adeskgate.autodesk.com (adeskgate.autodesk.com [198.93.152.11]) by imag.imag.fr (8.8.1/8.8.5) with ESMTP id UAA14005 for ; Fri, 29 Aug 1997 20:41:05 +0200 (MET DST) Received: from autodesk.autodesk.com by adeskgate.autodesk.com (8.6.12/SMI-5.3) with ESMTP id LAA11450; Fri, 29 Aug 1997 11:40:23 -0700 Received: from hqhubmu1.autodesk.com by autodesk.autodesk.com (8.6.12/4.4BSD) with ESMTP id LAA02084; Fri, 29 Aug 1997 11:40:13 -0700 Received: from ccinternet.autodesk.com (ccinternet [144.111.240.144]) by hqhubmu1.autodesk.com (8.7.5/8.7.3) with SMTP id LAA17655 for ; Fri, 29 Aug 1997 11:40:11 -0700 (PDT) Received: from ccMail by ccinternet.autodesk.com (IMA Internet Exchange 2.11 (Pre-release) Enterprise) id 00099F68; Fri, 13 Jun 1997 11:41:19 -0700 Mime-Version: 1.0 Date: Fri, 29 Aug 1997 14:38:29 -0700 Message-ID: <00099F68.4149@autodesk.com> From: Eric Haines Subject: ACM TOG article(s) of interest To: globillum Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit Content-Description: cc:Mail note part X-UIDL: e60dc4f41d6ade313855d1969bc080d7 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 The latest issue of ACM TOG is out. The first article in particular should be of interest to globillumers. Here's the table of contents: Volume 16, Number 3 (July 1997) Global illumination using local linear density estimation, Bruce Walter, Philip M. Hubbard, Peter Shirley and Donald P. Greenberg Color image quantization by minimizing the maximum intercluster distance, Zhigang Xiang Smooth invariant interpolation of rotations, F. C. Park and Bahram Ravani Some characterizations of families of surfaces using functional equations, Enrique Castillo and Andres Iglesias The symmetric analogue of the polynomial power basis, J. Sanchez-Reyes Abstracts and index terms for these articles are available at http://www.acm.org/pubs/contents/journals/tog/1997-16/ The ACM TOG site, http://www.acm.org/tog/, also has pointers to various online resources for computer graphics researchers and educators. Eric Haines erich@acm.org From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id SAA09399; Fri, 5 Sep 1997 18:06:22 +0200 Received: from lms02.us1.ibm.com (lms02.ny.us.ibm.com [198.133.22.25]) by imag.imag.fr (8.8.1/8.8.5) with SMTP id RAA11135 for ; Fri, 5 Sep 1997 17:07:28 +0200 (MET DST) Received: from d01lms03.pok.ibm.com by lms02.us1.ibm.com (AIX 4.1/UCB 5.64/4.03) id AA16746; Fri, 5 Sep 1997 15:07:02 GMT Received: by US.IBM.COM (Soft-Switch LMS 2.0) with snapi via D01AU041 id 5010300008757645; Fri, 5 Sep 1997 11:03:15 -0400 From: Holly Rushmeier To: globillum@imag.fr, Program.s96@siggraph.org Cc: bartram@siggraph.org Subject: COMPUTING REVIEWS Category Editor Duties Message-Id: <5010300008757645000002L052*@MHS> Date: Fri, 5 Sep 1997 11:03:15 -0400 Mime-Version: 1.0 Content-Type: text/plain; charset=windows-1252; format=flowed X-UIDL: d566c946de21803a162e462f5052a183 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hi -- Appended is a note from the editor of Computing Reviews, who is looking for a Category Editor for computer graphics. This job is an important service to the computing community. I've mentioned the position to several people, but apparently no one has come forward yet. If you are interested, please contact Neal directly. Also, please distribute this to anyone you know who you think is qualified and might be interested. Thanks, Holly ---------------------- Forwarded by Holly Rushmeier/Watson/IBM on 09/05/97 10:51 AM --------------------------- neal @ cse.fau.edu 07/29/97 08:44 AM To: holly @ watson.ibm.com cc: neal @ cse.fau.edu (bcc: Holly Rushmeier/Watson/IBM Research) Subject: COMPUTING REVIEWS Category Editor Duties Holly, as promised yesterday, attached is a description of the functions of a COMPUTING REVIEWS Category Editor. We are searching for someone to fill the I.3--Computer Graphics position. Please see the January 1997 edition of COMPUTING REVIEWS for a listing of the complete Computing Classification System taxonomy, or see http://www.acm.org/class/1991 or the ACM home page for links to COMPUTING REVIEWS and its charter, editorial board, etc. Please contact me with any questions you have. Neal --------------------------------------------------------- Neal Coulter Computer Science and Engineering Department Florida Atlantic University Boca Raton, FL 33431 561-367-3983 561-367-2800 (fax) neal@cse.fau.edu FUNCTIONS OF CATEGORY EDITORS These guidelines were drafted by Jean E. Sammet in 1985 and updated in 1994. The basic functions of each Category Editor (CE) are to improve the quality and to increase the quantity of reviews for Computing Reviews (CR). ACM Headquarters is responsible for producing CR. The separate responsibilities of HQ and the category editors follow. ACM Headquarters Basic Responsibilities 1. acquiring material (with input from CEs for unusual material) 2. maintaining reviewer database (additions, deletions, and changes) 3. assigning priorities for reviewing 4. assigning material to specific reviewers 5. receiving, processing, and editing the reviews and scheduling them for publication Category Editor's Responsibilities 1. Provide advice and aid to HQ and Editor-in-Chief (EIC) for special projects (as requested by HQ or EIC) 2. Specify items that deserve quickly published reviews. Guidelines for priority identification: a. Do this even for journals that already receive high coverage. b. Do not do this for ACM journals, because HQ sometimes works from page proofs of these. c. For journals or proceedings that HQ does not normally receive, the CE must send a copy of the paper to HQ, or the coverage will be delayed while HQ obtains the document. d. Specify articles in ACM SIG newsletters that should be reviewed. 3. Examine reviews after they are sent to Headquarters (normally sent to CEs within 5 working days after it arrives at HQ). Guidelines for review examination: a. Notify ACM HQ within one week of receipt of changes needed for categories and/or General Terms, and your evaluation of each review. Rate the review on a scale from 1--5 for technical content (TE), completeness (CO), and clarity (CL). Electronic mail should be used if possible. Mail to reviews@cr.acm.org. If using regular mail, send to: ACM Computing Reviews, 1515 Broadway, 17th Floor, New York, NY 10036. b. Notify ACM HQ within one week of reviews that are not acceptable to publish or require substantial revision. Particular attention should be paid to the length of reviews. Reviews of books should be between 250 and 800 words, depending on the length and/or importance of the book. Reviews of papers or book chapters should be between 100 and 250 words. There is no length limit for Comparative, Feature, and Scholarly reviews. The Managing Editor, Associate Editor, and Assignment Editor work closely with reviewers to keep these special reviews to an appropriate length. c. Make suggestions to help reviewer improve future reviews. Do this in any time period you feel is appropriate and use any format you are comfortable with. 4. Collaborate with ACM HQ (Assignment Editor) to suggest Comparative book reviews. In special cases, the CE and assignment editor may also get involved in single book review problems. Suggest reviewers for Comparative reviews. 5. Notify HQ of "obscure" documents not normally reviewed---but needing review---and suggest reviewers, if possible. This includes proceedings, journals not normally received at HQ, university press publications, videotapes, and books from obscure publishers. Provide HQ with full source information, author, and title. 6. Notify HQ of new journals along with recommendation of level of coverage (full, moderate, or occasional). 7. Suggest specific reviewers to HQ for specific documents whenever appropriate. Timing is critical and notification by CE to HQ must be rapid, or this won't work. 8. Recruit reviewers for your area. If possible, use specific approaches unique to your area. Rate reviewers. 9. Recruit outstanding and well-known experts to review special items, under the condition that this does not interfere with normal HQ operations. This will only be effective if based on personal contact and special arrangements. 10. Write reviews yourself at least twice a year. 11. Review your portion of the category tree and make recommendations for changes as requested by the EIC. 12. Prepare index terms for items not in the category tree as requested by the EIC. 13. Recommend important conference papers for review. Solicit Scholarly and Feature reviews. General note: Because no single CE is likely to be equally familiar with all the topics under the category, it is permissible (and encouraged) for each Category Editor to find one or more assistants to carry out many of the above tasks for a subcategory, or to provide advice. This should be done on an informal basis. The CE retains authority and responsibility. From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id UAA24510; Mon, 8 Sep 1997 20:08:09 +0200 Received: from cs.uct.ac.za (root@cs.uct.ac.za [137.158.128.249]) by imag.imag.fr (8.8.1/8.8.5) with SMTP id SAA25114 for ; Mon, 8 Sep 1997 18:56:35 +0200 (MET DST) Received: from tai.cs.uct.ac.za by cs.uct.ac.za with smtp (Smail3.1.29.1 #11) id m0x86re-00098RC; Mon, 8 Sep 97 18:40 SAT (+0200) Received: by tai.cs.uct.ac.za (951211.SGI.8.6.12.PATCH1042/ika.02) id SAA19984; Mon, 8 Sep 1997 18:40:38 +0200 From: "Wolfram Kresse" Message-Id: <9709081840.ZM19982@tai> Date: Mon, 8 Sep 1997 18:40:37 +0000 X-Face: .4|Jp[=9'pK#xl6x&l>D4xycaCh FF=0.5 - if A is at a vertex of the emitter, I've got a problem... By naive empirical analysis, I managed to find a solution for the following cases (A at an emitter vertex): /|E / |____ | / /R | / / |/___/ (side view) - if emitter and receiver are rectangular, the FF at the vertex is 0.25*(1+cos(alpha)). (alpha= angle between emitter and receiver) _______ \ |E \ b2 | \ | \ | \ | b1 \ | ______\| / \ / \ /____________\R (front view) - if alpha is a right angle, and the angle of the emitter is beta2 (b2), and the angle between the receiver edge in the emitter plane and the emitter is beta1 (b1), and beta=b1+b2 (are you still with me? :) ), then the FF is 0.25*(cos(beta1)-cos(beta)). ...well, that's as far as I got. It seems already that the combination of these two cases (varying alpha *and* beta1/beta) isn't that simple that it can be figured out just by writing down some values and trying. My hope is that there is a (or several) formula for the general case (e.g. the result seems also to depend on how I approach the receiver vertex - and thus on the angle of the receiver). One simple way to 'solve' it, is just to move the receiver vertex away from the emitter plane, but this looks more like a workaround and it might even lead to other problems. - is this how everybody does it ;-) or are there other ways to get a correct FF value for these cases? Any suggestions/help appreciated. Thanks! Cheers, Wolfram -- +-------+-----Wolfram Kresse---------------------------------------------+ | _ _ | wkresse@igd.fhg.de http://www.igd.fhg.de/~wkresse | | +-------------------------+-----------------+--------------------+ | -O-O- |"Meeneemeeneemeenee" | CU l8r, LE g8r! | | > |"Yes,that's right,Twiki."+-----------------+ | _____ +-----+-----+-------------+ | U | 8^) | :u) | +-------+-----+-----+ From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id VAA25119; Mon, 8 Sep 1997 21:32:44 +0200 Received: from mail.uniserve.com (dns1-van.uniserve.com [204.244.163.48]) by imag.imag.fr (8.8.1/8.8.5) with SMTP id VAA28869 for ; Mon, 8 Sep 1997 21:22:05 +0200 (MET DST) Received: from ian [204.244.158.195] by mail.uniserve.com with smtp (Exim 1.70 #1) id 0x89Qn-0004un-00; Mon, 8 Sep 1997 12:25:06 -0700 X-Sender: iashdown@pop.uniserve.com X-Mailer: Windows Eudora Version 1.4.4 Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed To: globillum@imag.fr From: Ian Ashdown Subject: RADBIB97 - September 1st release Message-Id: Date: Mon, 8 Sep 1997 12:25:06 -0700 X-UIDL: 6a6e7accde943870905a729c3aa3fd84 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit ANNOUNCE: 97/09/01 Release of RADBIB97.BIB and GITHESIS.BIB ----------------------------------------------------------- RADBIB97 is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. It currently includes 1,219 references -- 55 new additions since the 97/07/15 release! This bibliography is available in BibTex format as RADBIB97.BIB (with a release date of September 1, 1997) from: http://www.ledalite.com/library-/rrt.htm ftp://ftp.ledalite.com/pub/radbib97.bib Also available from this site is an abridged version of RADBIB97.BIB called GITHESIS.BIB. This bibliography includes 138 references to radiosity and global illumination theses. As always, it is time-consuming and sometimes difficult to track down conference papers and theses on radiosity and global illumination. If you know of a relevant reference that is not included in these bibliographies, please let us know so that we can include it in the next release. Partial financial support for the maintenance of these bibliographies has been provided by the ACM SIGGRAPH Special Projects. Ian Ashdown, P. Eng. | READ THE BOOK! | Research & Development Manager | Radiosity: A Programmer's Perspective | Ledalite Architectural Products | Wiley & Sons 1994 | Visit http://www.ledalite.com | (Sneaky Internet Advertising) | Book Review: http://www.ercb.com/ddj/1996/ddj.9605.html Book Order: https://www.wiley.com/compbooks/catalog/30444-1.htm Free Software: http://www.ledalite.com/software/software.htm From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id VAA12050; Tue, 9 Sep 1997 21:15:46 +0200 Received: from pink.lbl.gov (pink.lbl.gov [128.3.12.112]) by imag.imag.fr (8.8.1/8.8.5) with SMTP id UAA15800 for ; Tue, 9 Sep 1997 20:06:48 +0200 (MET DST) Received: (from greg@localhost) by pink.lbl.gov (950413.SGI.8.6.12/950213.SGI.AUTOCF) id LAA25029; Tue, 9 Sep 1997 11:08:41 -0700 Date: Tue, 9 Sep 1997 11:08:41 -0700 From: "Gregory W. Larson" Message-Id: <199709091808.LAA25029@pink.lbl.gov> To: globillum@imag.fr Subject: new extended-range TIFF library Cc: drb@sgi.com, malik@CS.Berkeley.EDU, debevec@CS.Berkeley.EDU X-UIDL: 4dbcb0734dc85b2017176491c6ab6515 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Hi All, As promised, I have put together some web pages describing a new addition to Sam Leffler's TIFF library, with facilities for reading and writing high dynamic-range images. See: http://www.sgi.com/Technology/pixformat/ The format is based on a 16-bit log encoding of luminance, plus a 16-bit encoding of color in CIE (u',v') coordinates. This allows the format to cover the full range of human vision in imperceptible steps. In fact, the encoding covers over 38 orders of magnitude, which means that you don't have to worry about exposure when storing your global illumination calculations. I have included over 100 example images, mostly Radiance renderings but some scanned images from Debevec and Malik's '97 Siggraph paper and my own experiments. I'm hoping this will encourage people to download and compile the library and viewer and start playing around with tone-mapping algorithms and the like. For those of you who want to experiment with image-based rendering algorithms, I have also included 5 cylindrical (360 degree) panoramas. Let me know if you have any problems, questions or suggestions. -Greg _____________________________________________________________________ Gregory Ward Larson (the computer artist formerly known as Greg Ward) Silicon Graphics, Inc. Computer Science Department 2011 N. Shoreline Blvd., M/S 07U-553 537 Soda Hall, UC Berkeley Mountain View, CA 94043-1389 Berkeley, CA 94720-1776 (650) 933-4878, -2663 fax (510) 642-3631, -5775 fax gregl@sgi.com on Tues., Thurs. and Fri. ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id VAA12890; Fri, 3 Oct 1997 21:03:05 +0200 Received: from mail.uniserve.com (dns1-van.uniserve.com [204.244.163.48]) by imag.imag.fr (8.8.5/8.8.5) with SMTP id SAA18727 for ; Fri, 3 Oct 1997 18:59:52 +0200 (MET DST) Received: from p1-10.van.tvs.net [204.244.158.89] by mail.uniserve.com with smtp (Exim 1.70 #1) id 0xHB4h-0003lA-00; Fri, 3 Oct 1997 09:59:35 -0700 X-Sender: iashdown@pop.uniserve.com (Unverified) X-Mailer: Windows Eudora Version 1.4.4 Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed To: globillum@imag.fr From: Ian Ashdown Message-Id: Date: Fri, 3 Oct 1997 09:59:35 -0700 X-UIDL: c07169b9c69233a8edede96d5936b4ab X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit ANNOUNCE: 97/10/01 Release of RADBIB97.BIB and GITHESIS.BIB ----------------------------------------------------------- RADBIB97 is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. It currently includes 1,237 references -- 18 new additions since the 97/09/01 release. This bibliography is available in BibTex format as RADBIB97.BIB (with a release date of October 1, 1997) from: http://www.ledalite.com/library-/rrt.htm ftp://ftp.ledalite.com/pub/radbib97.bib Also available from this site is an abridged version of RADBIB97.BIB called GITHESIS.BIB. This bibliography includes 145 references to radiosity and global illumination theses -- 7 new additions since the 97/09/01 release. As always, it is time-consuming and sometimes difficult to track down conference papers and theses on radiosity and global illumination. If you know of a relevant reference that is not included in these bibliographies, please let us know so that we can include it in the next release. Partial financial support for the maintenance of these bibliographies has been provided by the ACM SIGGRAPH Special Projects. Ian Ashdown, P. Eng. | READ THE BOOK! Research & Development Manager | Radiosity: A Programmer's Perspective Ledalite Architectural Products | Wiley & Sons 1994 Visit http://www.ledalite.com | (http://www.amazon.com) From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id VAA00217; Tue, 7 Oct 1997 21:50:51 +0200 Received: from ladybug.seas.gwu.edu (ladybug.seas.gwu.edu [128.164.9.8]) by imag.imag.fr (8.8.5/8.8.5) with ESMTP id PAA18931 for ; Tue, 7 Oct 1997 15:20:28 +0200 (MET DST) Received: from seas.gwu.edu (felix.seas.gwu.edu [128.164.9.3]) by ladybug.seas.gwu.edu (v8) with ESMTP id JAA00173 for ; Tue, 7 Oct 1997 09:20:14 -0400 (EDT) Received: (from musgrave@localhost) by seas.gwu.edu (8.8.7/8.7.1) id JAA21547; Tue, 7 Oct 1997 09:20:06 -0400 (EDT) Date: Tue, 7 Oct 1997 09:20:06 -0400 (EDT) From: Ken Musgrave Message-Id: <199710071320.JAA21547@seas.gwu.edu> To: globillum@imag.fr Subject: Clouds, imaged nicely Cc: sylee@seas.gwu.edu X-UIDL: f0be69bb59915a0ea4384a1b638fc449 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit One of my students at GWU, Sang Yoon Lee, has implemented Nelson Max's high-albedo anisotropic multiple scattering model in my cloud models with adaptive level of detail. The resulting images are worth a look (I've wanted to see such results for years!): www.seas.gwu.edu/student/sylee Enjoy! -Ken From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id UAA14238; Fri, 10 Oct 1997 20:47:36 +0200 Received: from pink.lbl.gov (pink.lbl.gov [128.3.12.112]) by imag.imag.fr (8.8.5/8.8.5) with SMTP id UAA02276 for ; Fri, 10 Oct 1997 20:28:30 +0200 (MET DST) Received: (from greg@localhost) by pink.lbl.gov (950413.SGI.8.6.12/950213.SGI.AUTOCF) id LAA06568; Fri, 10 Oct 1997 11:30:31 -0700 Date: Fri, 10 Oct 1997 11:30:31 -0700 From: "Gregory W. Larson" Message-Id: <199710101830.LAA06568@pink.lbl.gov> To: globillum@imag.fr Subject: webmover program X-UIDL: 4bda7cae70fed830bc5fffed2e51dddb X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Hi Everyone, I just wrote a program that has nothing to do with global illumination, but I don't belong to any appropriate groups so I thought I'd announce it here, anyway. It's a little utility for checking and moving web pages. It's especially useful for translating web pages you want to publish on a CD-ROM in ISO-9660 format. I am faced with this task myself, translating the Radiance web pages for a CD-ROM to accompany the book Rob Shakespeare and I wrote on Radiance for Morgan Kaufmann. (Plug: the book should be out early next year.) If you've ever had to go through a large web site, renaming files and fixing links, you know what a pain it can be. This program does it for you, and it's fast and it's free (with no warranty!). Here's the help screen: Usage: webmover [-u|-i|-d][-v] base_URL orig_dir/[html] [new_dir/[html]] Or: webmover -h[elp] Arguments to webmover and their interpretation: base_URL The starting point for this website (beginning with "http://") orig_dir/[html] The original directory [and front page] relative to base_URL If [html] is left off, then we assume "index.html" newdir/[html] The destination directory [and front page] relative to base_URL This new directory must not exist. If this argument is left off, webmover just checks pages. Options to webmover and their meanings: -u Convert to UNIX file naming conventions and newline -i Convert to ISO-9660 file naming conventions -d Convert to DOS file naming conventions and newline -v Verbose reporting of progress to stdout Assumptions made by webmover: o Only move what front page references, directly and indirectly o Overhead references (above front page directory) are not moved o No non-printing, non-white characters are desired in pages o Symbolic links are followed and not treated specially o Hard links are made to destination whenever possible o Hard links are preserved among files The following file suffixes are recognized: ____UNIX____ISO____ html htm jpeg jpg tiff tif tar.Z trz ps.Z psz tar.gz tgz ps.gz pgz text txt jfif jff ------------------------------- To pick it up, just follow the URL below: file://radsite.lbl.gov/rad/pub/translators/webmover.c Feel free to share this with whomever you like. It's public domain. -Greg _____________________________________________________________________ Gregory Ward Larson (the computer artist formerly known as Greg Ward) Silicon Graphics, Inc. Computer Science Department 2011 N. Shoreline Blvd., M/S 07U-553 537 Soda Hall, UC Berkeley Mountain View, CA 94043-1389 Berkeley, CA 94720-1776 (650) 933-4878, -2663 fax (510) 642-3631, -5775 fax gregl@sgi.com on Tues., Thurs. and Fri. ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id TAA17682; Wed, 22 Oct 1997 19:29:42 +0200 Received: from phong.cs.utah.edu (phong.cs.utah.edu [128.110.4.52]) by imag.imag.fr (8.8.5/8.8.5) with SMTP id SAA05530 for ; Wed, 22 Oct 1997 18:56:18 +0200 (MET DST) Received: (from shirley@localhost) by phong.cs.utah.edu (950413.SGI.8.6.12/950213.SGI.AUTOCF) id KAA08066 for globillum@imag.fr; Wed, 22 Oct 1997 10:46:33 -0600 From: Peter Shirley Message-Id: <199710221646.KAA08066@phong.cs.utah.edu> Subject: Grad recruiting at Utah To: globillum@imag.fr Date: Wed, 22 Oct 1997 10:46:33 -0600 (MDT) X-Mailer: ELM [version 2.4 PL23] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: be0ae5ac60a0a85c859a024fa6c940f0 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 I apologize for this potential misuse of the list-- I would like to spread the word that we are trying to increase our grad population size at Utah, and if possible please pass on the following tidbits to your seniors considering grad school (in graphics or not): 1) Almost all students get assitantships 2) Cohen/Johnson/Shirley/Riesenfeld/Hansen/Smits here as either profs or postdocs-- that is two modeling, two rendering, and two viz people. 3) Much equipemnt including Origin2000 with RealityMonster 4) Free online application-- see www.cs.utah.edu As for lifestyle, this is the best place I know of for outdoorsy types that still want to be able to see an art-film or get an expresso or microbrew. It is probably not a good place for true urbanites or people that want a small town. Thanks, Pete Shirley shirley@cs.utah.edu PS-- obligatory globillum material-- I just returned from Pacific Graphics 97 and Parallel Rendering 97. I saw three different talks that had radiosity solutions on models with more than 0.5 million initial patches. Also, it was mentioned that the next version of doom has full radiosity solutions! From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id SAA16090; Fri, 24 Oct 1997 18:50:25 +0200 Received: from adeskgate.autodesk.com (adeskgate.autodesk.com [198.93.152.11]) by imag.imag.fr (8.8.5/8.8.5) with ESMTP id RAA26415 for ; Fri, 24 Oct 1997 17:48:23 +0200 (MET DST) Received: from autodesk.autodesk.com by adeskgate.autodesk.com (8.6.12/SMI-5.3) with ESMTP id IAA16556; Fri, 24 Oct 1997 08:47:07 -0700 (PDT) Received: from hqhubmu1.autodesk.com by autodesk.autodesk.com (8.6.12/4.4BSD) with ESMTP id IAA19892; Fri, 24 Oct 1997 08:46:55 -0700 Received: from ccinternet.autodesk.com (ccinternet [144.111.240.144]) by hqhubmu1.autodesk.com (8.7.5/8.7.3) with SMTP id IAA15681 for ; Fri, 24 Oct 1997 08:46:53 -0700 (PDT) Received: from ccMail by ccinternet.autodesk.com (IMA Internet Exchange 2.11 Enterprise) id 001748AC; Fri, 24 Oct 1997 08:47:05 -0700 Mime-Version: 1.0 Date: Fri, 24 Oct 1997 11:45:08 -0700 Message-ID: <001748AC.4149@autodesk.com> From: Eric Haines Subject: ACM Digital Library open to all To: globillum Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit Content-Description: cc:Mail note part X-UIDL: d9935ecb3206aa7595fb77239377556e X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 I'd like to mention a resource here that is worth knowing about: ACM Transactions on Graphics and all other ACM journals are now searchable online via ACM's Digital Library. Also, many articles are becoming available in digital form to subscribers. Until the end of the year the search engine is available to anyone for free. The Digital Library is located at: http://www.acm.org/dl/ As an example, here are the publications found when searching on radiosity or global illumination as keywords (excuse the margins): 1) 30 Radiosity and hybrid methods; La'szlo' Neumann ; ACM Trans. Graph. 14, 3 (Jul. 1995), Pages 233 - 265 2) 20 Global illumination of glossy environments using wavelets and importance; Per H.Christensen ; ACM Trans. Graph. 15, 1 (Jan. 1996), Pages 37 - 71 3) 10 Extending the radiosity method to include specularly reflecting and translucent materials; Holly E.Rushmeier ; ACM Trans. Graph. 9, 1 (Jan. 1990), Pages 1 - 27 4) 10 Global illumination using local linear density estimation; Bruce Walter ; ACM Trans. Graph. 16, 3 (Jul. 1997), Pages 217 - 259 5) 10 Global illumination using local linear density estimation; Bruce Walter ; ACM Trans. Graph. 16, 3 (Jul. 1997), Pages 217 - 259 6) 10 Multiresolution analysis for surfaces of arbitrary topological type; Michael Lounsbery ; ACM Trans. Graph. 16, 1 (Jan. 1997), Pages 34 - 73 7) 10 Clustering for glossy global illumination; Per H.Christensen ; ACM Trans. Graph. 16, 1 (Jan. 1997), Pages 3 - 33 8) 10 Smooth B-spline illumination maps for bidirectional ray tracing; Richard A.Redner ; ACM Trans. Graph. 14, 4 (Oct. 1995), Pages 337 - 362 9) 10 Adjoint equations and random walks for illumination computation; S. N.Pattanaik ; ACM Trans. Graph. 14, 1 (Jan. 1995), Pages 77 - 102 I've noticed that unfortunately the older years of some journals are not yet part of the Digital Library, which seems to go back to about 1985. Eric Haines erich@acm.org From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id WAA27894; Thu, 30 Oct 1997 22:18:56 +0100 Received: from lorraine.loria.fr (lorraine.loria.fr [152.81.1.17]) by imag.imag.fr (8.8.5/8.8.5) with ESMTP id PAA01132 for ; Thu, 30 Oct 1997 15:15:28 +0100 (MET) Received: from cloe.loria.fr (cloe.loria.fr [152.81.3.123]) by lorraine.loria.fr (8.8.7/8.8.7/8.8.7/JCG) with ESMTP id PAA24560 for ; Thu, 30 Oct 1997 15:15:26 +0100 (MET) From: Nicolas Holzschuch Received: (from holzschu@localhost) by cloe.loria.fr (8.7.4/8.7.3) id PAA06361 for globillum@imag.fr; Thu, 30 Oct 1997 15:15:25 +0100 (MET) Message-Id: <199710301415.PAA06361@cloe.loria.fr> Subject: Test scenes To: globillum@imag.fr Date: Thu, 30 Oct 1997 15:15:25 +0100 (MET) X-Mailer: ELM [version 2.4 PL25] MIME-Version: 1.0 Content-Type: text/plain; charset=windows-1252; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: ad7c247a92d5de8667146e41337c1fba X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hello globillumers, I just had a message from a student, asking for some test scenes to check his radiosity program. I immediately thought of this nice set of 10 test scenes that was released for the fifth Eurographics Workshop on Rendering (by Peter Shirley, if my memory serves me well). However, I couldn't remember where to find them. Can anyone help me? Nicolas Holzschuch From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id XAA28253; Thu, 30 Oct 1997 23:19:37 +0100 Received: from pink.lbl.gov (pink.lbl.gov [128.3.12.112]) by imag.imag.fr (8.8.5/8.8.5) with SMTP id XAA24723 for ; Thu, 30 Oct 1997 23:07:44 +0100 (MET) Received: (from greg@localhost) by pink.lbl.gov (950413.SGI.8.6.12/950213.SGI.AUTOCF) id OAA02716; Thu, 30 Oct 1997 14:09:48 -0800 Date: Thu, 30 Oct 1997 14:09:48 -0800 From: "Gregory W. Larson" Message-Id: <199710302209.OAA02716@pink.lbl.gov> To: Nicolas Holzschuch Subject: Re: Test scenes Cc: globillum@imag.fr X-UIDL: 198c90e92b139748647caf7ae2d2f381 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit > Hello globillumers, > I just had a message from a student, asking > for some test scenes to check his radiosity > program. I immediately thought of this nice > set of 10 test scenes that was released for > the fifth Eurographics Workshop on Rendering > (by Peter Shirley, if my memory serves me > well). However, I couldn't remember where > to find them. > > Can anyone help me? > > Nicolas Holzschuch Peter Shirley's test scenes are together with a bunch of scenes taken from Radiance at the MGF web site: http://radsite.lbl.gov/mgf/ There is also a free parser library for reading the data, documentation, etc. -Greg _____________________________________________________________________ Gregory Ward Larson (the computer artist formerly known as Greg Ward) Silicon Graphics, Inc. Computer Science Department 2011 N. Shoreline Blvd., M/S 07U-553 537 Soda Hall, UC Berkeley Mountain View, CA 94043-1389 Berkeley, CA 94720-1776 (650) 933-4878, -2663 fax (510) 642-3631, -5775 fax gregl@sgi.com on Tues., Thurs. and Fri. ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id LAA04601; Fri, 31 Oct 1997 11:51:07 +0100 Received: from idefix.cs.kuleuven.ac.be (root@idefix.cs.kuleuven.ac.be [134.58.41.7]) by imag.imag.fr (8.8.5/8.8.5) with ESMTP id LAA21501 for ; Fri, 31 Oct 1997 11:07:44 +0100 (MET) Received: from flater.cs.kuleuven.ac.be (philippe@flater.cs.kuleuven.ac.be [134.58.45.35]) by idefix.cs.kuleuven.ac.be (8.8.6/8.8.6) with ESMTP id LAA05495; Fri, 31 Oct 1997 11:07:34 +0100 (MET) Received: (from philippe@localhost) by flater.cs.kuleuven.ac.be (8.8.6/8.8.6) id LAA00725; Fri, 31 Oct 1997 11:07:27 +0100 (MET) From: Philippe Bekaert Message-Id: <199710311007.LAA00725@flater.cs.kuleuven.ac.be> Subject: Re: Test scenes In-Reply-To: <199710301415.PAA06361@cloe.loria.fr> from Nicolas Holzschuch at "Oct 30, 97 03:15:25 pm" To: Nicolas Holzschuch Date: Fri, 31 Oct 1997 11:07:27 +0100 (MET) Cc: globillum@imag.fr X-Mailer: ELM [version 2.4ME+ PL32 (25)] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: 63a189da0e9b64dd633966a181615ac6 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 > I just had a message from a student, asking > for some test scenes to check his radiosity > program. I immediately thought of this nice Here's one of my favourites: Everyone knows that if all surfaces in a scene have relfectance and emittance equal to 0.5, the total radiance will be 1 everywhere. It's one of the few cases where you have an analytical solution, regardless of the scene geometry. Actually, this is true as long as the sum of the reflectance and emittance is everywhere equal to one. This doesn't mean that the reflectances have to be equal everywhere: Take e.g. a labyrinth scene with a few patches that are almost perfect emittors (emittance 0.99 and reflectance 0.01) while all others are almost perfect reflectors (emittance 0.01 and reflectance 0.99). Also in this case, the total radiance will be equal to one everywhere, but it's a very nice experiment to test out what your radiosity implementation does with it. It was suggested to me by Laszlo and Attila Neumann. Regards, Philippe. -- /~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~|~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~\ \ Philippe Bekaert | If anything can go wrong, it will, but / / Computer Graphics Research Group | ... we're prepared for it (Switzerland) \ \ Department of Computer Science | ... we don't care (Greece) / / K.U.Leuven - Belgium | ... what the heck, it's been going \ \ | wrong for centuries already (Portugal) / / http://www.cs.kuleuven.ac.be/ | ... it's the fault of the Walloons \ \ ~philippe/ | (Flanders) / /__________________________________| ... we deserve it (Wallonie) \ \ | ... as long as there's vodka we don't / / Not everything that is written | care (Russia) \ \ here is my employers opinion, | ... how much money do I loose? / / sometimes not even mine. | (The Netherlands) \ \__________________________________|_________________________________________/ From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id RAA11717; Fri, 31 Oct 1997 17:12:16 +0100 Received: from idefix.cs.kuleuven.ac.be (root@idefix.cs.kuleuven.ac.be [134.58.41.7]) by imag.imag.fr (8.8.5/8.8.5) with ESMTP id QAA10790 for ; Fri, 31 Oct 1997 16:28:17 +0100 (MET) Received: from flater.cs.kuleuven.ac.be (philippe@flater.cs.kuleuven.ac.be [134.58.45.35]) by idefix.cs.kuleuven.ac.be (8.8.6/8.8.6) with ESMTP id QAA14592 for ; Fri, 31 Oct 1997 16:28:08 +0100 (MET) Received: (from philippe@localhost) by flater.cs.kuleuven.ac.be (8.8.6/8.8.6) id QAA02163; Fri, 31 Oct 1997 16:28:06 +0100 (MET) From: Philippe Bekaert Message-Id: <199710311528.QAA02163@flater.cs.kuleuven.ac.be> Subject: test scenes To: globillum@imag.fr Date: Fri, 31 Oct 1997 16:28:06 +0100 (MET) X-Mailer: ELM [version 2.4ME+ PL32 (25)] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: 645f462677774c9b6a3dae9c98b99b2e X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Some people doubt whether it is true that the total radiance in a diffuse scene will be everywhere equal to one if the sum of emittance and reflectance is everyhwere equal to one. Well ... they are right: it's not always true. I forgot to mention that the scenes should be closed. But the proof (for closed scenes) is as follows: Consider first the "radiosity case": L_i = E_i + rho_i sum_j F_ij L_j My claim is that if E_i + rho_i = 1 for all patches i, then also L_i = 1 for all patches. Proof: fill L_i = 1 for all patches in the radiance equation: 1 = E_i + rho_i sum_j F_ij 1 sum_j F_ij = 1 in a closed environment, so this would imply: 1 = E_i + rho_i and that's exactly what I supposed. It *is* a proof because the solution of the radiance equation is unique. The proof without discretising is very similar. And the result can be generalized to non diffuse environments: the radiance leaving any point in any direction will be equal to one if the sum of selfemitted radiance L_e(x, theta_out) + albedo rho(x, theta_out) equals 1 for all points x and directions theta_out, with rho(x, theta_out) = integral over hemisphere at x of brdf f_r(x, theta_in, theta_out) times cos(angle between theta_in and normal at x) times differential solid angle around theta_in Sorry for wasting your time if you already knew this. Best regards, Philippe. -- /~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~|~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~\ \ Philippe Bekaert | If anything can go wrong, it will, but / / Computer Graphics Research Group | ... we're prepared for it (Switzerland) \ \ Department of Computer Science | ... we don't care (Greece) / / K.U.Leuven - Belgium | ... what the heck, it's been going \ \ | wrong for centuries already (Portugal) / / http://www.cs.kuleuven.ac.be/ | ... it's the fault of the Walloons \ \ ~philippe/ | (Flanders) / /__________________________________| ... we deserve it (Wallonie) \ \ | ... as long as there's vodka we don't / / Not everything that is written | care (Russia) \ \ here is my employers opinion, | ... how much money do I loose? / / sometimes not even mine. | (The Netherlands) \ \__________________________________|_________________________________________/ From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id LAA09578; Tue, 4 Nov 1997 11:47:26 +0100 Received: from santos.doc.ic.ac.uk (d2EarJ8xK+E1+7X6yyqe2wjqw/k40ilg@santos.doc.ic.ac.uk [146.169.2.42]) by imag.imag.fr (8.8.5/8.8.5) with SMTP id LAA27017 for ; Tue, 4 Nov 1997 11:24:23 +0100 (MET) Received: from peaberry.doc.ic.ac.uk [146.169.12.8] ([KzpNU4iLe92V+XjmCR2zgInuMJSgIo5N]) by santos.doc.ic.ac.uk with smtp (Exim 1.62 #2) id 0xSgAI-0006zD-00; Tue, 4 Nov 1997 10:24:54 +0000 Received: from ajc by peaberry.doc.ic.ac.uk with local (Exim 1.62 #2) id 0xSgAC-0000ZF-00; Tue, 4 Nov 1997 10:24:48 +0000 From: Adrian James Chung To: globillum@imag.fr Subject: Global illumination mailing list has been spammed Message-Id: Date: Tue, 4 Nov 1997 10:24:48 +0000 X-UIDL: 97ebd950894db31cf4f9913c6d240aa1 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Sorry to have to bring up something that has little to do with computer graphics, but the serious problem of spam has finally reached the globillum listserver. You no doubt would have received (perhaps twice) unsolicited commercial email (UCE) with the following headers: Return-path: Envelope-to: ajc@doc.ic.ac.uk Delivery-date: Mon, 3 Nov 1997 22:34:51 +0000 Received: from pigeon.doc.ic.ac.uk [146.169.5.10] ([vdpgkE0wQyuWqrqL+lUNOKRqmUZux2eI]) by santos.doc.ic.ac.uk with smtp (Exim 1.62 #2) id 0xSV57-0006Ja-00; Mon, 3 Nov 1997 22:34:49 +0000 Received: from imag.imag.fr [129.88.30.1] by pigeon.doc.ic.ac.uk with esmtp (Exim 0.55 #3) id E0xSV4b-0001PG-00; Mon, 3 Nov 1997 22:34:17 +0000 Received: from baghdad.savoynet.com (root@baghdad.savoynet.com [204.157.255.21]) by imag.imag.fr (8.8.5/8.8.5) with ESMTP id XAA25613 for ; Mon, 3 Nov 1997 23:22:54 +0100 (MET) From: twilling@swain.savoynet.com Message-Id: <199711032222.XAA25613@imag.imag.fr> Date: Mon, 3 Nov 1997 18:21:56 -0500 X-Sender: twilling@swain.savoynet.com X-Advertisement: Click here to be removed. To: twilling@swain.savoynet.com Subject: United Circuits I have taken great pains to fit a personalised and highly tuned spam filter on my college email box in order to make this channel of communication usable again. Naturally I have implemented an unconditional bypass for all the mailing lists that I have subscribed to. I consider the information posted to this forum very valuable and would hate to have to apply anti-spam filtering to messages posted here, lest I lose an article of considerable importance. In this context, I ask what actions will the list maintainers be taking to prevent more UCE from flooding this list, making unfair usage of resources (list server, disk quota), and if left unchecked rendering this mailing list unusable? Will someone be reporting this to news:news.admin.net-abuse.email and news:news.admin.net-abuse.sightings ? Any comments welcome. (Perhaps better if discussed off this forum. Make sure it doesn't resemble spam.) Adrian -- For details http://spam.abuse.net/spam/ PS. Okay, I finally thought of an on-topic question. What modelling software do you professionals use to construct your test scenes? Is it commercial? Is there something I can download off the Net for any UNIX box running X, (with source) ? And handles parametric curved surfaces? I find that text editing a scripted modelling language falls far short of a real GUI-interface modeller. From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id XAA21747; Tue, 4 Nov 1997 23:52:45 +0100 Received: from mail.uniserve.com ([204.244.163.48]) by imag.imag.fr (8.8.5/8.8.5) with SMTP id RAA22463 for ; Tue, 4 Nov 1997 17:23:26 +0100 (MET) Received: from p1-24.van.tvs.net [204.244.158.103] by mail.uniserve.com with smtp (Exim 1.70 #1) id 0xSlk0-0005xx-00; Tue, 4 Nov 1997 08:22:08 -0800 X-Sender: iashdown@pop.uniserve.com X-Mailer: Windows Eudora Version 1.4.4 Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed To: globillum@imag.fr From: Ian Ashdown Subject: Interesting radiosity paper Message-Id: Date: Tue, 4 Nov 1997 08:22:08 -0800 X-UIDL: 2307d4dc9a455c9a40b3f4d278f4bc03 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit For those of you who teach global illumination, there is a just- published survey paper that may be of interest: Nievergelt, Yves. 1997. "Radiosity in Illumination Engineering," UMAP Journal 18(2):167-178 (Summer). The paper provides an overview of the radiosity equation and its application to the engineering design of lighting systems, with topic headings such as "Lambertian Surfaces," "Luminous Flux," "Form Factors for Lambertian Surfaces," "Setting Up Radiosity Systems," "Solving Large Radiosity Systems," "How Southwell's Method is Used," and "Inverse Problems." As you may have surmised, it is entirely concerned with applied mathematics. I like this paper because it offers a fresh perspective from a mathematician's point of view. More important, it poses four open questions in the mathematics of global illumination that should interest motivated graduate students. (Even better, what is the relationship between radiosity systems and Ansel Adam's 1941 photograph "Moonrise, Hernandez, New Mexico?") UMAP is the Journal of Undergraduate Mathematics and its Applications. If radiosity in illumination engineering doesn't garner your attention, you might consider some of the other articles, including "Communication Games and the Canadian Constitution," "The Mathematics of Scuba Diving," and "How Does the NFL Rate Passers?" It's an interesting publication. Ian Ashdown, P. Eng. | READ THE BOOK! Research & Development Manager | Radiosity: A Programmer's Perspective Ledalite Architectural Products | Wiley & Sons 1994 Visit http://www.ledalite.com | (http://www.amazon.com) From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id BAA00557; Fri, 7 Nov 1997 01:12:29 +0100 Received: from safran.imag.fr (safran.imag.fr [129.88.42.9]) by imag.imag.fr (8.8.5/8.8.5) with ESMTP id RAA28404; Thu, 6 Nov 1997 17:08:27 +0100 (MET) Received: (from sillion@localhost) by safran.imag.fr (8.6.10/8.6.9) id RAA29644; Thu, 6 Nov 1997 17:08:18 +0100 From: Francois Sillion Message-Id: <199711061608.RAA29644@safran.imag.fr> Subject: Globillum SPAMMING fix (only read if you care) To: Adrian James Chung Date: Thu, 6 Nov 1997 17:08:17 +0100 (MET) Cc: Global Illumination List In-Reply-To: from "Adrian James Chung" at Nov 4, 97 10:24:48 am Reply-To: Francois.Sillion@imag.fr X-Mailer: ELM [version 2.4 PL24] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: eb8f0ba06aac9a06a602332fd35fa539 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hi all, Sorry to bother you, but I wanted to re-assure you all that whenever a SPAM-like message is sent to globillum, I protest in all the ways I am aware of. In the latest case, I had the sender domain added to our local black list, and also manually removed the globillum address from the marketer's web site. I will not send such a message every time a problem happens, but be sure I do everything I can to avoid such problems. > Any comments welcome. (Perhaps better if discussed off this > forum. Make sure it doesn't resemble spam.) > > For details http://spam.abuse.net/spam/ +------------------+------------------------------------------------------+ | Francois SILLION | iMAGIS - GRAVIR/IMAG, B.P. 53, 38041 Grenoble Cedex 9| | ' | France. Tel:+33 4 76 51 43 54 - Fax:+33 4 76 63 55 80| +------------------+--------+---------------------------------------------+ | Francois.Sillion@imag.fr | http://www-imagis.imag.fr/~Francois.Sillion | +---------------------------+---------------------------------------------+ From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id IAA28649; Sat, 29 Nov 1997 08:50:35 +0100 Received: from netcomsv. (uu2news.netcom.com [163.179.3.15]) by imag.imag.fr (8.8.5/8.8.5) with SMTP id IAA05218 for ; Sat, 29 Nov 1997 08:44:56 +0100 (MET) Received: by netcomsv. (SMI-8.6/SMI-SVR4) id XAA08802; Fri, 28 Nov 1997 23:44:38 -0800 >Received: from ponfar.pdi.com by pdi.pdi.com via ESMTP (951211.SGI.8.6.12.PATCH1502/(911001.SGI)1.4-PDI.RELAY) for <@pdi.pdi.com:globillum@imag.fr> id PAA10539; Wed, 26 Nov 1997 15:43:42 -0800 Received: from pdi.com by netcomsv.netcom.com; Fri, 28 Nov 1997 23:44 PST Received: from ponfar.pdi.com by pdi.pdi.com via ESMTP (951211.SGI.8.6.12.PATCH1502/(911001.SGI)1.4-PDI.RELAY) for <@pdi.pdi.com:globillum@imag.fr> id PAA10539; Wed, 26 Nov 1997 15:43:42 -0800 Received: by ponfar.pdi.com (940816.SGI.8.6.9/(911001.SGI)1.2-PDI) for globillum@imag.fr id PAA23986; Wed, 26 Nov 1997 15:43:42 -0800 From: Dan Wexler Message-Id: <199711262343.PAA23986@ponfar.pdi.com> Subject: Quantization To: globillum@imag.fr Date: Wed, 26 Nov 1997 15:43:42 -0800 (PST) MIME-Version: 1.0 Content-Transfer-Encoding: 8bit Content-Type: text/plain; charset=US-ASCII; format=flowed X-UIDL: 80d5fcc38a55eb7db4e4a3eb6022d894 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 What is the best way to quantize floating point RGB colors (0 to 1) into 8-bit integers? Is the answer different for different output devices? Daniel Wexler R&D Staff, Pacific Data Images From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id RAA31649; Sat, 29 Nov 1997 17:25:21 +0100 Received: from merckx.graphics.cornell.edu (MERCKX.GRAPHICS.CORNELL.EDU [128.84.247.147]) by imag.imag.fr (8.8.5/8.8.5) with SMTP id RAA24662 for ; Sat, 29 Nov 1997 17:20:09 +0100 (MET) Received: by merckx.graphics.cornell.edu (5.65/DEC-Ultrix/4.3) id AA00495; Sat, 29 Nov 1997 11:19:59 -0500 Message-Id: <9711291619.AA00495@merckx.graphics.cornell.edu> Received: by beauty.graphics.cornell.edu (1.37.109.8/16.2) id AA02933; Sat, 29 Nov 1997 11:19:57 -0500 Date: Sat, 29 Nov 1997 11:19:57 -0500 From: "Stephen H. Westin" To: wexler@pdi.com Cc: globillum@imag.fr In-Reply-To: <199711262343.PAA23986@ponfar.pdi.com> (wexler@pdi.com) Subject: Re: Quantization Reply-To: westin@graphics.cornell.edu X-UIDL: 9e2dd83da17cf72430049bfde5bc935b X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit > What is the best way to quantize floating point RGB colors (0 to 1) > into 8-bit integers? Is the answer different for different output > devices? Well, the quantization should probably be non-linear, as the eye is more sensitive to quantization in dark areas of the image. I prefer using a gamma correction of 2.2, which then can be re-corrected for a particular output device. I would also add random dither before quantization to reduce visible quantization artifacts further. How about pixel_val = (int) ( 255.0 * pow ( float_val, 0.45 ) * drand48() ); for a start? This will o correct for a gamma of 2.2222... o scale to the range 0:255 o add 0.5 for correct rounding o add random noise in the range -0.5:0.5 There's a bit of inconsistency here, as we're assuming nonlinearity in the output device, but adding noise that's uniformly distributed. But I think it will work pretty well. From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id GAA18432; Mon, 1 Dec 1997 06:44:35 +0100 Received: from phong.cs.utah.edu (phong.cs.utah.edu [128.110.4.52]) by imag.imag.fr (8.8.5/8.8.5) with SMTP id GAA14802 for ; Mon, 1 Dec 1997 06:31:29 +0100 (MET) Received: (from shirley@localhost) by phong.cs.utah.edu (950413.SGI.8.6.12/950213.SGI.AUTOCF) id WAA12371 for globillum@imag.fr; Sun, 30 Nov 1997 22:30:45 -0700 From: Peter Shirley Message-Id: <199712010530.WAA12371@phong.cs.utah.edu> Subject: conference data? To: globillum@imag.fr Date: Sun, 30 Nov 1997 22:30:45 -0700 (MST) X-Mailer: ELM [version 2.4 PL23] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: 4aed71356ecbc94579bef80240027c39 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hi gang. I have updated the conference announcements on my web-page: http://www.cs.utah.edu/~shirley/ This includes the rendering workshop page (which I had a little trouble finding-- please add links to this on your own pages!). I know I am missing several workshops-- updates appreciated. Thanks, Pete /***********************************************************************/ /* */ /* Free online forms grad application */ /* http://www.cs.utah.edu/admissions-webform.html */ /* */ /* Faculty job ad */ /* http://www.cs.utah.edu/ad-faculty.html */ /* */ /***********************************************************************/ From To: Robert F Tobler From: Werner Purgathofer Subject: Re: Globillum Message-Id: In-Reply-To: <9712010957.AA15599@raven.cg.tuwien.ac.at> X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Date: Mon, 1 Dec 1997 11:17:25 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Problem: ich forwarde das an die Rendering-Group.... Kannst du nicht auch alle anderen (evtl. nach Ruecksprache) in die Globillum-Liste aufnehmen lassen? + Mic, dann kann ich mir das Forwarden ganz sparen! Danke Werner >Werner -- > >Ich bin jetzt direkt im Globillum Verteiler. Kannst Du mich bitte aus Deinem >herausnehmen? > >Danke, > >-- Robert From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id UAA00372; Mon, 1 Dec 1997 20:18:15 +0100 Received: from pop.uniserve.com (pop.uniserve.com [204.244.156.3]) by imag.imag.fr (8.8.5/8.8.5) with SMTP id TAA08295 for ; Mon, 1 Dec 1997 19:59:42 +0100 (MET) Received: from p3-06.van.tvs.net [204.244.158.181] by pop.uniserve.com with smtp (Exim 1.73 #1) id 0xcb49-0004dG-00; Mon, 1 Dec 1997 10:59:33 -0800 X-Sender: iashdown@pop.uniserve.com X-Mailer: Windows Eudora Version 1.4.4 Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed To: globillum@imag.fr From: Ian Ashdown Subject: Re: Radiosity research peaks in 1994? Message-Id: Date: Mon, 1 Dec 1997 10:59:33 -0800 X-UIDL: fa10ea9709a3a86ce6ee54977ca14ec3 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit > I just ran across an interesting resource. See the graph at: > > http://liinwww.ira.uka.de/bibliography/Graphics/rad.html > > near the bottom. It shows the raw number of references in the > radiosity bibliography peaked in 1994 (for comparison, ray tracing > peaks in 1990). It's also interesting to look at SIGGRAPH's > comprehensive bibliography graphed in this way: 1983 has the most > articles published, with other peaks (though decreasing) in 1991 and > 1995 (4 year cycle? ;-> ). > > Eric Haines > erich@acm.org > Ah, but it's the *quality* of the papers that really matters. There are still many open questions in radiative transfer/radiosity theory, and from what I have seen of the publications over the past few years, 1994 was the beginning of a trend towards investigating the deeper problems. For whatever reason, most the really interesting work is now being done in Europe, Asia and the Far East. Cornell's legacy unfortunately appears to be on the wane in North America. P.S. - the latest RADBIB97.BIB and GITHESIS.BIB bibliographies are being released later today. I managed to find only nine new references for global illumination in the past two months instead of the usual fifteen to thirty. Hmm ... Ian Ashdown, P. Eng. | READ THE BOOK! Research & Development Manager | Radiosity: A Programmer's Perspective Ledalite Architectural Products | Wiley & Sons 1994 Visit http://www.ledalite.com | (http://www.amazon.com) From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id TAA11909; Mon, 1 Dec 1997 19:19:01 +0100 Received: from adeskgate.autodesk.com (adeskgate.autodesk.com [198.93.152.11]) by imag.imag.fr (8.8.5/8.8.5) with ESMTP id SAA03425 for ; Mon, 1 Dec 1997 18:42:08 +0100 (MET) Received: from autodesk.autodesk.com by adeskgate.autodesk.com (8.6.12/SMI-5.3) with ESMTP id JAA28737; Mon, 1 Dec 1997 09:40:58 -0800 (PST) Received: from hqhubmu1.autodesk.com by autodesk.autodesk.com (8.6.12/4.4BSD) with ESMTP id JAA21676; Mon, 1 Dec 1997 09:40:53 -0800 Received: from ccinternet.autodesk.com (ccinternet [144.111.240.144]) by hqhubmu1.autodesk.com (8.7.5/8.7.3) with SMTP id JAA13471 for ; Mon, 1 Dec 1997 09:40:51 -0800 (PST) Received: from ccMail by ccinternet.autodesk.com (IMA Internet Exchange 2.12 Enterprise) id 002408C3; Mon, 1 Dec 1997 09:40:33 -0800 Mime-Version: 1.0 Date: Mon, 1 Dec 1997 12:37:56 -0800 Message-ID: <002408C3.4149@autodesk.com> From: Eric Haines Subject: Radiosity research peaks in 1994? To: globillum Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit Content-Description: cc:Mail note part X-UIDL: 1712245010b2612e564f9a2001885123 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 I just ran across an interesting resource. See the graph at: http://liinwww.ira.uka.de/bibliography/Graphics/rad.html near the bottom. It shows the raw number of references in the radiosity bibliography peaked in 1994 (for comparison, ray tracing peaks in 1990). It's also interesting to look at SIGGRAPH's comprehensive bibliography graphed in this way: 1983 has the most articles published, with other peaks (though decreasing) in 1991 and 1995 (4 year cycle? ;-> ). Eric Haines erich@acm.org From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id PAA17048; Tue, 2 Dec 1997 15:43:08 +0100 Received: from pop.uniserve.com (pop.uniserve.com [204.244.156.3]) by imag.imag.fr (8.8.5/8.8.5) with SMTP id OAA04974 for ; Tue, 2 Dec 1997 14:55:47 +0100 (MET) Received: from p1-37.van.tvs.net [204.244.158.116] by pop.uniserve.com with smtp (Exim 1.73 #1) id 0xcsmi-0006TR-00; Tue, 2 Dec 1997 05:54:45 -0800 Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: Radiosity Bibliography Update (December 1997) Date: Tue, 2 Dec 1997 05:55:16 -0800 Message-ID: <01bcff29$eb452310$749ef4cc@helios> MIME-Version: 1.0 Content-Type: text/plain; charset=windows-1252; format=flowed Content-Transfer-Encoding: 8bit X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 4.71.1712.3 X-MimeOLE: Produced By Microsoft MimeOLE V4.71.1712.3 X-UIDL: 3fdab8e655705f89d9a5f15467ab9d98 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 ANNOUNCE: 97/12/01 Release of RADBIB97.BIB and GITHESIS.BIB ----------------------------------------------------------- RADBIB97 is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. It currently includes 1,246 references -- 9 new additions since the 97/10/01 release. This bibliography is available in BibTex format as RADBIB97.BIB (with a release date of December 1, 1997) from: http://www.ledalite.com/library-/rrt.htm ftp://ftp.ledalite.com/pub/radbib97.bib Also available from this site is an abridged version of RADBIB97.BIB called GITHESIS.BIB. This bibliography includes 149 references to radiosity and global illumination theses -- 4 new additions since the 97/10/01 release. As always, it is time-consuming and sometimes difficult to track down conference papers and theses on radiosity and global illumination. If you know of a relevant reference that is not included in these bibliographies, please let us know so that we can include it in the next release. Partial financial support for the maintenance of these bibliographies has been provided by the ACM SIGGRAPH Special Projects. -- Ian Ashdown, P. Eng. | READ THE BOOK! Research & Development Manager | Radiosity: A Programmer's Perspective Ledalite Architectural Products | Wiley & Sons 1994 http://www.ledalite.com | http://www.amazon.com From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id VAA25194; Tue, 2 Dec 1997 21:13:04 +0100 Received: from relay2.mail.uk.psi.net (relay1.mail.uk.psi.net [154.32.105.6]) by imag.imag.fr (8.8.5/8.8.5) with ESMTP id RAA17914 for ; Tue, 2 Dec 1997 17:40:10 +0100 (MET) Received: from elvis.lightwork (lightwork.co.uk [195.152.206.2]) by relay2.mail.uk.psi.net (8.8.5/) with ESMTP id QAA05377 for ; Tue, 2 Dec 1997 16:40:08 GMT Received: by elvis.lightwork with Internet Mail Service (5.0.1457.3) id ; Tue, 2 Dec 1997 16:39:20 -0000 Message-ID: <8815647C7041D111A3010060B06BE1C00B064E@elvis.lightwork> From: Tim Hammond To: globillum@imag.fr Cc: self Subject: Query regarding probability sampling Date: Tue, 2 Dec 1997 16:39:19 -0000 X-Priority: 3 MIME-Version: 1.0 X-Mailer: Internet Mail Service (5.0.1457.3) Content-Type: text/plain; charset=windows-1252; format=flowed X-UIDL: e5679731df08a4f1d4864cd4e32e1366 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hi, I would be grateful if anyone on the list could provide me with any useful suggestions on the following: I'm currently working on code designed to shoot photons at random into a scene from a variety of light sources. This will involve a considerable amount of random sampling. For example, given a set of lights we need to determine at random which light to shoot a photon from. Then if the light source is made up of multiple polygons, which polygon do we shoot from and whereabouts on the polygon. Finally what will the initial direction of the photon be? The solution we intend to implement involves a certain amount of preprocessing for each test so that we end up with a probability distribution that can be quickly sampled to return a random selection (a light say) during shooting of photons. The goal is a generic process which, when given a set of N outcomes and N weights generates a data structure. This data structure will then need to be interrogated by a function which takes a random float in the range [0,1) and as quickly as possible returns one of the outcomes. The probability of returning any given outcome is proportional to the weight assigned to that outcome (for example for lights we would assign weights according to the output power of each light). Currently I am thinking about implementing the data structure produced by pre-processing as either a lookup table or a binary tree. The lookup table approach is very fast, but more memory intensive, whilst the binary tree approach would use less memory, but be slower. To clarify the problem, here is a very simple example. Take a scene with 5 light sources with respective powers of 50W 10W 5W 20W and 15W. In our current binary tree approach we would divide the region [0,1) as follows: Values in the range [0, 0.5) represent choosing the first light, values in the range [0.5, 0.6) the second, values in the range [0.6, 0.65) the third, values in the range [0.65, 0.85) the fourth and values in the range [0.85, 1) the fifth To then actually convert from a random number in the range [0,1) to a light, the lights could be arranged in a binary tree something like the following: [P<0.65] 0 [P>=0.65] / \ [P<0.6] O O [P>=0.85] / \ / \ O 3 4 5 / \ 1 2 At the first level of the tree, testing of whether the random value P is < or >= 0.65 (chosen so that roughly the same numbers of lights fall on each side) takes us down either the left or right branch. Further tests then occur at each level, for example P is < or >= 0.6 for the left-hand branch, until we arrive at a light. In a lookup table approach we have to subdivide the range [0,1) into a set of bins, the size of which is determined by the relative size of the smallest weight in the list of possible outcomes. Given the number of bins we can immediately convert a random float in the range [0,1) into an array index which points at one of the outcomes. As I said before this approach is very fast, but uses more memory, especially in cases where there is a large relative difference in weights between the most likely and least likely outcomes (we are forced to use a lot of small bins in order to include every possible outcome). I am keen to hear from anyone who has experience in this area or anyone who can suggest improvements to the solutions I have outlined above, or indeed any better solutions. Many thanks, Tim. Tim Hammond, Software Engineer, LightWork Design Ltd. tim.hammond@lightwork.co.uk http://www.lightwork.com Tel:+44 (0)114 266 8404 ext 242 Fax:+44 (0)114 266 1383 From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id WAA25765; Tue, 2 Dec 1997 22:29:39 +0100 Received: from teapot.llnl.gov (nelson@teapot.llnl.gov [128.115.19.100]) by imag.imag.fr (8.8.5/8.8.5) with SMTP id WAA03999 for ; Tue, 2 Dec 1997 22:20:27 +0100 (MET) Received: by teapot.llnl.gov (951211.SGI.8.6.12.PATCH1502/951211.SGI.AUTO) id NAA13829; Tue, 2 Dec 1997 13:17:47 -0800 From: "Nelson L. Max" Message-Id: <9712021317.ZM13827@teapot.llnl.gov> Date: Tue, 2 Dec 1997 13:17:45 -0800 In-Reply-To: Tim Hammond "Query regarding probability sampling" (Dec 2, 4:39pm) References: <8815647C7041D111A3010060B06BE1C00B064E@elvis.lightwork> Reply-to: max2@llnl.gov X-Mailer: Z-Mail (3.2.0 26oct94 MediaMail) To: Tim Hammond , globillum@imag.fr Subject: Re: Query regarding probability sampling Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed X-UIDL: ba792a6661ccb61641a229ddd3cd0ebb X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit If you want complete accuracy in the lookup table, you need to make all the weights be rational numbers, and make the size of the table the common denominator (the least common multiple of all the denominators when each fraction is in "reduced" form, with no common factors in the numerator and denominator). I think this is worse than you indicated. How about a compromise between the two methods: let a smaller table point to a (possibly internal) node of the tree, at which to begin the search. -- email: max2@llnl.gov Nelson Max, Mail Stop L-307 http://www.llnl.gov/graphics Lawrence Livermore National Laboratory phone (510) 422-4074 7000 East Avenue fax (510) 423-4139 Livermore, CA 94550, USA From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id AAA26820; Wed, 3 Dec 1997 00:09:58 +0100 Received: from sgi.sgi.com (SGI.COM [192.48.153.1]) by imag.imag.fr (8.8.5/8.8.5) with SMTP id XAA07116 for ; Tue, 2 Dec 1997 23:31:40 +0100 (MET) Received: from cthulhu.engr.sgi.com (cthulhu.engr.sgi.com [192.26.80.2]) by sgi.sgi.com (950413.SGI.8.6.12/970507) via ESMTP id OAA17266 for <@sgi.engr.sgi.com:globillum@imag.fr>; Tue, 2 Dec 1997 14:31:37 -0800 env-from (bwade@sgi.com) Received: from amie.engr.sgi.com (amie.engr.sgi.com [150.166.55.164]) by cthulhu.engr.sgi.com (950413.SGI.8.6.12/960327.SGI.AUTOCF) via ESMTP id OAA11546 for <@cthulhu.engr.sgi.com:globillum@imag.fr>; Tue, 2 Dec 1997 14:31:37 -0800 Received: from pc-amie (pc-amie.engr.sgi.com [150.166.55.165]) by amie.engr.sgi.com (950413.SGI.8.6.12/960327.SGI.AUTOCF) via SMTP id OAA03092 for ; Tue, 2 Dec 1997 14:31:33 -0800 Message-Id: <3.0.5.32.19971202143133.00a4a480@amie.engr.sgi.com> X-Sender: bwade@amie.engr.sgi.com X-Mailer: QUALCOMM Windows Eudora Pro Version 3.0.5 (32) Date: Tue, 02 Dec 1997 14:31:33 -0800 To: globillum@imag.fr From: Bretton Wade Subject: Re: Query regarding probability sampling In-Reply-To: <8815647C7041D111A3010060B06BE1C00B064E@elvis.lightwork> Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed X-UIDL: 3a4b48cbf7d0ba8ac70060916c0bf4cf X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit >an array index which points at one of the outcomes. As I said before >this approach is very fast, but uses more memory, especially in cases >where there is a large relative difference in weights between the most >likely and least likely outcomes (we are forced to use a lot of small >bins in order to include every possible outcome). I would go with the table approach. This is grossly simplified, but the table grows linearly with the number of lights if the light source power values are all approximately the same order of magnitude (This statement is clearly subject to verification). Can you characterize the typical scene? If you were going to have lots of scenes with 1000 suns and 1 flashlight, the table might not be a reasonable approach. If you had 100 light sources at 100W and one light source at 1W, you would be using approximately 40Kb (assuming the table stored a 4 byte pointer). In a commercial, high end rendering product, I would consider even 100 times this requirement to be modest if the gain is significant, especially if the model is already so complex as to include 101 distinct light sources. >If you want complete accuracy in the lookup table, you need to make all the >weights be rational numbers, and make the size of the table the common >denominator (the least common multiple of all the denominators when each >fraction is in "reduced" form, with no common factors in the numerator and >denominator). I think this is worse than you indicated. Would it be reasonable to simply reject sources which are extremely unlikely to contribute? In the example above, eliminating the 1W light source (with an occurrence probability of 1e-4) reduces a 40Kb table to 400 bytes. Doing this clearly helps to reduce the table size, but it is easy to imagine a scene with a sun and a flashlight where the point of interest is illuminated only by the flashlight. Perhaps a very coarse pre-process which propogates importance from the viewpoint(s) would be useful. -- Bretton Wade (bwade@sgi.com) Cosmo Software - A Silicon Graphics Company From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id DAA29101; Wed, 3 Dec 1997 03:00:14 +0100 Received: from grande.dcc.unicamp.br (dcc.unicamp.br [143.106.1.11]) by imag.imag.fr (8.8.5/8.8.5) with ESMTP id CAA14437 for ; Wed, 3 Dec 1997 02:55:58 +0100 (MET) Received: from amazonas.dcc.unicamp.br (amazonas3 [143.106.7.11]) by grande.dcc.unicamp.br (8.8.5/8.8.5) with ESMTP id XAA10596; Tue, 2 Dec 1997 23:47:16 -0200 (EDT) Received: from coruja.dcc.unicamp.br (coruja [143.106.24.80]) by amazonas.dcc.unicamp.br (8.8.5/8.8.5) with ESMTP id XAA06695; Tue, 2 Dec 1997 23:47:13 -0200 (EDT) Received: (from stolfi@localhost) by coruja.dcc.unicamp.br (8.8.5/8.8.5) id XAA07543; Tue, 2 Dec 1997 23:47:13 -0200 (EDT) Date: Tue, 2 Dec 1997 23:47:13 -0200 (EDT) Message-Id: <199712030147.XAA07543@coruja.dcc.unicamp.br> From: Jorge Stolfi To: Tim Hammond Cc: globillum@imag.fr Subject: Re: Query regarding probability sampling MIME-Version: 1.0 Content-Transfer-Encoding: 8bit Content-Type: text/plain; charset=windows-1252; format=flowed In-Reply-To: <8815647C7041D111A3010060B06BE1C00B064E@elvis.lightwork> References: <8815647C7041D111A3010060B06BE1C00B064E@elvis.lightwork> Reply-To: stolfi@dcc.unicamp.br X-UIDL: 9330830ee25d2a26c0873f9d0eebda1c X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 > To then actually convert from a random number in the range [0,1) to a > light, the lights could be arranged in a binary tree something like the > following: > > > [P<0.65] 0 [P>=0.65] > / \ > [P<0.6] O O [P>=0.85] > / \ / \ > O 3 4 5 > / \ > 1 2 > > At the first level of the tree, testing of whether the random value P is > < or >= 0.65 (chosen so that roughly the same numbers of lights fall on > each side) takes us down either the left or right branch. Further tests > then occur at each level, for example P is < or >= 0.6 for the left-hand > branch, until we arrive at a light. > > In a lookup table approach we have to subdivide the range [0,1) into a > set of bins, the size of which is determined by the relative size of the > smallest weight in the list of possible outcomes. Given the number of > bins we can immediately convert a random float in the range [0,1) into > an array index which points at one of the outcomes. You can also precompute a vector s[i] = sum{ p[j] : j < i }, where p[j] is the desired probability of chosing item j. Then you generate a random P in [0 _ 1], and use binary search on s to locate an i such that s[i] < P < s[i+i]. This is simpler than building a binary tree, and at least as fast if coded with care. Moreover, if you expect a large number of items with similar probabilities, you can use linear interpolation (i.e. round(P*n) \pm K) to guess an initial range for the binary search. --stolfi From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id EAA00203; Tue, 6 Jan 1998 04:24:20 +0100 Received: from cottage.direct.ca (cottage.direct.ca [199.60.229.12]) by imag.imag.fr (8.8.5/8.8.5) with SMTP id EAA22429 for ; Tue, 6 Jan 1998 04:12:23 +0100 (MET) Received: from van-52-2014.direct.ca (helios) [204.174.243.206] by cottage.direct.ca with smtp (Exim 1.82 #1) id 0xpPR5-0005J8-00; Mon, 5 Jan 1998 19:12:11 -0800 Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: 98/01/01 Releases of RADBIB98 and GITHESIS Date: Mon, 5 Jan 1998 19:12:37 -0800 Message-ID: <01bd1a50$f0920850$cef3aecc@helios> MIME-Version: 1.0 Content-Type: text/plain; charset=windows-1252; format=flowed Content-Transfer-Encoding: 8bit X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 4.71.1712.3 X-MimeOLE: Produced By Microsoft MimeOLE V4.71.1712.3 X-UIDL: 6c5aedec807af71d043ea8230e6c4c54 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 ANNOUNCE: 98/01/01 Release of RADBIB98.BIB and GITHESIS.BIB ----------------------------------------------------------- RADBIB98 is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. It currently includes 1,275 references -- 29 new additions since the 97/12/01 release. This bibliography is available in BibTex format as RADBIB98.BIB (with a release date of January 1, 1998) from: http://www.ledalite.com/library-/rrt.htm ftp://ftp.ledalite.com/pub/radbib98.bib Also available from this site is an abridged version of RADBIB98.BIB called GITHESIS.BIB. This bibliography includes 153 references to radiosity and global illumination theses -- 4 new additions since the 97/12/01 release. As always, it is time-consuming and sometimes difficult to track down conference papers and theses on radiosity and global illumination. If you know of a relevant reference that is not included in these bibliographies, please let us know so that we can include it in the next release. Partial financial support for the maintenance of these bibliographies has been provided by the ACM SIGGRAPH Special Projects. Ian Ashdown, P. Eng. | READ THE BOOK! Vice President, R & D | Radiosity: A Programmer's Perspective byHeart Consultants Limited | Wiley & Sons 1994 West Vancouver, BC (Canada) | http://www.amazon.com From To: Robert F Tobler From: Werner Purgathofer Subject: Re: Travel to rendering workshop? Cc: Globillum Mailing List Message-Id: In-Reply-To: <9801191038.AA14486@raven.cg.tuwien.ac.at> X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Date: Mon, 19 Jan 1998 14:06:29 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Peter: I see two more alternatives. The first is Lauda-Air http://www.laudaair.com/twol.htm they often have very attractive offers. The second is to fly to Budapest (Hungary), and take a train to Wien (=Vienna) from there. This train takes about 3 hours. See you soon! Werner At 11:38 Uhr +0100 19.01.1998, Robert F Tobler wrote: >Peter Shirley wrote: > >> I'm having a lot of trouble finding a reasonable fare >> to make it to the rendering workshop: >> >> http://www.cg.tuwien.ac.at/conferences/EGRWS98/ > >Delta Air Lines and Austrian Airlines have a joint operation on flights to >Vienna from New York, Atlanta, Washingon D.C, and Chicago: > http://www.wizard.net/aua_usa/transatl.htm > >This might be your best bet in terms of prices, although I have not checked >them yet. In general you should try to include a weekend in your stay in >Vienna. Air fares will be substantially cheaper that way. > >If you travel to other cities in Europe, probably the only good train >connection to Vienna will be from Munich, Germany. A train leaves from Munich >to Vienna nearly every hour, and the trip takes between 5 and 6 hours. > >In the hope that you find a cheap and good connection and make it to >the Rendering Workshop, > >Robert F. Tobler >Organising Chairman >http://www.cg.tuwien.ac.at/conferences/EGRWS98/ > >------------------------------------------------------------------------ > Robert F. Tobler - tel:+43(1)58801-4575,fax:5874932 > Institute of Computer Graphics - mailto:rft@cg.tuwien.ac.at > Vienna University of Technology - http://www.cg.tuwien.ac.at/~rft/ From To: Nicolas Holzschuch From: Werner Purgathofer Subject: Re: Travel to rendering workshop? Cc: globillum@imag.fr Message-Id: In-Reply-To: <199801191605.RAA11037@venus.loria.fr> References: from "Werner Purgathofer" at Jan 19, 98 02:06:29 pm X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Date: Tue, 20 Jan 1998 11:23:24 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit To all: as a European, I would normally *fly* from Amsterdam, Frankfurt, Paris, Roma, Geneva and other cities in that distance to Wien. So, unless you are fond of a long train ride and/or you have a really exorbitantly cheaper flight to somewhere else in Europe, I recommmend that you fly to Wien (or maybe Budapest). There is also an airport in Bratislava (capitol of Slovakia) which is less than 50 miles from Wien. Hope too see you all in Wien! Werner At 17:05 Uhr +0100 19.01.1998, Nicolas Holzschuch wrote: > To all: >Assuming your airline company does not fly to Vienna, >you also have the possibility to do some travel by train. > ... there are the following links between >Wien and other major european cities with airports: > >- from Amsterdam: ... >- from Frankfurt: ... >- from Paris: ... >- from Roma: ... >- from Geneva: ... >- from Budapest: ... From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id HAA13271; Tue, 27 Jan 1998 07:03:48 +0100 Received: from nit.Stanford.EDU (nit.Stanford.EDU [171.64.77.197]) by imag.imag.fr (8.8.5/8.8.5) with ESMTP id GAA16673 for ; Tue, 27 Jan 1998 06:46:15 +0100 (MET) Received: (from ericv@localhost) by nit.Stanford.EDU (8.7.5/8.7.1) id VAA23168 for globillum@imag.fr; Mon, 26 Jan 1998 21:46:15 -0800 (PST) From: Eric Veach Message-Id: <199801270546.VAA23168@nit.Stanford.EDU> Subject: Thesis available online To: globillum@imag.fr Date: Mon, 26 Jan 1998 21:46:15 -0800 (PST) X-Mailer: ELM [version 2.4ME+ PL28 (25)] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: ada25cecee6f0a0dfdb13f2a9a457aef X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hello everyone, For those who are interested, my thesis is now available online: Robust Monte Carlo Methods for Light Transport Simulation Eric Veach Ph.D. dissertation Stanford University December 1997 http://graphics.stanford.edu/papers/veach_thesis/ It describes techniques such as Metropolis light transport, multiple importance sampling, and bidirectional path tracing in more detail than in the corresponding papers. It also includes quite a bit of new material, including studies of: - the inherent limitations of unbiased Monte Carlo methods - new variance reduction techniques - the history of reciprocity principles and important exceptions to them - the derivation of a new reciprocity principle that applies to materials that transmit as well as reflect light [i.e. BTDF's as well as BRDF's] You can find the abstract and table of contents on the web page, as well as Postscript and PDF versions of the thesis. Best regards, Eric From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id PAA07485; Sat, 31 Jan 1998 15:19:40 +0100 Received: from phoenix.cs.utah.edu (phoenix.cs.utah.edu [155.99.209.77]) by imag.imag.fr (8.8.5/8.8.5) with SMTP id PAA23098 for ; Sat, 31 Jan 1998 15:12:09 +0100 (MET) Received: (from shirley@localhost) by phoenix.cs.utah.edu (950413.SGI.8.6.12/950213.SGI.AUTOCF) id HAA00557 for globillum@imag.fr; Sat, 31 Jan 1998 07:12:06 -0700 From: Peter Shirley Message-Id: <199801311412.HAA00557@phoenix.cs.utah.edu> Subject: Sky luminance models To: globillum@imag.fr Date: Sat, 31 Jan 1998 07:12:06 -0700 (MST) X-Mailer: ELM [version 2.4 PL23] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: 9cf90e0784b8508ccd03826550ead6b1 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hi all. I have a student working on creating sky dome radiance functions. A couple of questions: 1) Are any of you aware of newer models than the classic CIE models? I seem to remember Nishita discussing a recent one and I can't find it in his papers. 2) Does the CIE luminance function include the sun or not? Its description in Wyszecki&Stiles implies it does not, but its actual form has a sun-like spike in it that does not look like forward scattering. Thanks, Pete From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id PAA07610; Sat, 31 Jan 1998 15:45:02 +0100 Received: from kiultra.eml.hiroshima-u.ac.jp (kiultra.eml.hiroshima-u.ac.jp [133.41.51.161]) by imag.imag.fr (8.8.5/8.8.5) with ESMTP id PAA23974 for ; Sat, 31 Jan 1998 15:40:33 +0100 (MET) Received: from vaio.nisken.fuee.fukuyama-u.ac.jp (vaio.nisken.fuee.fukuyama-u.ac.jp [163.145.94.29]) by kiultra.eml.hiroshima-u.ac.jp (8.8.5+2.7Wbeta5/3.6Wbeta5) with SMTP id XAA11833; Sat, 31 Jan 1998 23:37:12 +0900 (JST) Message-ID: <34D33526.2A2C@eml.hiroshima-u.ac.jp> Date: Sat, 31 Jan 1998 23:28:54 +0900 From: Tomoyuki Nishita Reply-To: nis@eml.hiroshima-u.ac.jp Organization: Fukuyama University X-Mailer: Mozilla 3.03Gold (Win95; I) MIME-Version: 1.0 To: Peter Shirley CC: globillum@imag.fr Subject: Re: Sky luminance models References: <199801311412.HAA00557@phoenix.cs.utah.edu> Content-Type: text/plain; charset=iso-2022-jp Content-Transfer-Encoding: 7bit X-UIDL: 491addefb7ffa5d38dd8e2f5a0604094 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hi Dr. Peter Shirley; > Nishita discussing a recent one and I can't find it > in his papers. I use the classic CIE model. >2) Does the CIE luminance function include the sun or not? I believe that it does not include the sun. > but its actual form has a sun-like spike in it that does > not look like forward scattering. I think that it due to strong forward scattering from aerosols particles. Tomoyuki Nishita Professor Dept. of Electronic and Electrical Engineering Faculty of Engineering Fukuyama University Higashimura-cho, Fukuyama, 729-02 Japan Work phone: +81-849-36-2111(ext.4731) Fax number: +81-849-36-2023 nis@eml.hiroshima-u.ac.jp http://www.eml.hiroshima-u.ac.jp/~nis From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id LAA00109; Mon, 2 Feb 1998 11:33:58 +0100 Received: from relay1.mail.uk.psi.net (relay1.mail.uk.psi.net [154.32.105.6]) by imag.imag.fr (8.8.5/8.8.5) with ESMTP id LAA06155 for ; Mon, 2 Feb 1998 11:07:35 +0100 (MET) Received: from elvis.lightwork (lightwork.co.uk [195.152.206.2]) by relay1.mail.uk.psi.net (8.8.5/) with ESMTP id KAA02958 for ; Mon, 2 Feb 1998 10:07:20 GMT Received: by elvis.lightwork with Internet Mail Service (5.0.1457.3) id <11VZA0C1>; Mon, 2 Feb 1998 10:06:46 -0000 Message-ID: <8815647C7041D111A3010060B06BE1C0149375@elvis.lightwork> From: Neil Gatenby To: shirley@phoenix.cs.utah.edu, globillum@imag.fr Subject: RE: Sky luminance models Date: Mon, 2 Feb 1998 10:06:44 -0000 X-Priority: 3 MIME-Version: 1.0 X-Mailer: Internet Mail Service (5.0.1457.3) Content-Type: text/plain; charset=windows-1252; format=flowed X-UIDL: 874db5d98a9232e402bf9f567a453004 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Pete; when you say "the classic CIE models" do you mean CIE 1973? I think CIE 1994 has one more sky ... an intermediate sky, but maybe that was there in 73, too ... dunno. Anyway, quoting from CIE Technical Report CIE 110-1994 "Spatial Distribution of Daylight - Luminance Distributions of Various Reference Skies" ISBN 3 900 734 52 6 They say on pg 1 ... "The skies treated in this report do not include direct sunlight" I think the spike you are seeing is to be expected ... the sky dome being illuminated most markedly where the sun is. best wishes Neil On Saturday, January 31, 1998 2:12 PM, shirley@phoenix.cs.utah.edu [SMTP:shirley@phoenix.cs.utah.edu] wrote: > > Hi all. I have a student working on creating sky dome > radiance functions. A couple of questions: > > 1) Are any of you aware of newer models than the > classic CIE models? I seem to remember > Nishita discussing a recent one and I can't find it > in his papers. > > 2) Does the CIE luminance function include the sun or not? > Its description in Wyszecki&Stiles implies it does not, > but its actual form has a sun-like spike in it that does > not look like forward scattering. > > Thanks, > > Pete From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id RAA07619; Mon, 2 Feb 1998 17:12:49 +0100 Received: from monster.igd.fhg.de (monster.igd.fhg.de [153.97.128.43]) by imag.imag.fr (8.8.5/8.8.5) with SMTP id QAA28616 for ; Mon, 2 Feb 1998 16:09:00 +0100 (MET) From: wkresse@igd.fhg.de Received: from michelangelo.igd.fhg.de by monster.igd.fhg.de (5.x/SMI-4.1) id AA27061; Mon, 2 Feb 1998 16:07:42 +0100 Received: by michelangelo.igd.fhg.de (950413.SGI.8.6.12/SMI-4.0) id QAA21078; Mon, 2 Feb 1998 16:07:41 +0100 Date: Mon, 2 Feb 1998 16:07:41 +0100 Message-Id: <9802021607.ZM21077@michelangelo> In-Reply-To: shirley@phoenix.cs.utah.edu (Peter Shirley) "Sky luminance models" (Jan 31, 7:12) References: <199801311412.HAA00557@phoenix.cs.utah.edu> X-Face: .4|Jp[=9'pK#xl6x&l>D4xycaCh Hi all. I have a student working on creating sky dome > radiance functions. A couple of questions: > > 1) Are any of you aware of newer models than the > classic CIE models? I seem to remember > Nishita discussing a recent one and I can't find it > in his papers. > Perez et al. (1993) are introducing a sky model which is a generalization of the CIE standard clear sky formula and includes 5 parameters that can be adjusted to account for any luminance distribution ranging from totally overcast to very clear. The parameters describe the darkening of the horizon region in respect to the zenith, the luminance gradient near the horizon, the relative intensity as well as the width of the circumsolar region, and the relative intensity of the backscattered light received at the earth's surface. The CIE clear sky can also be expressed by appropriate settings of these parameters. These parameters can be simplified to 'sky clearness' and 'sky brightness', which can also be derived from actually measured sky data with horizontal diffuse and normal incident direct irradiance. Perez R., Seals R., Michalsky J., "All-Weather Model for Sky Luminance Distribution - Preliminary Configuration and Validation", Solar Energy, Vol. 50, No. 3, 1993, pp.235-245 Perez R., Ineichen P., Seals R., Michalsky J., Stewart R., "Modelling Daylight Availability and Irradiance Components from Direct and Global Irradiance", Solar Energy, Vol. 44, No. 5, 1990, pp.271-289 > 2) Does the CIE luminance function include the sun or not? > Its description in Wyszecki&Stiles implies it does not, > but its actual form has a sun-like spike in it that does > not look like forward scattering. > No, the direct sunlight has to be accounted for explicitely since it is described by a narrow angle several levels of magnitude brighter than the diffuse skylight of the hemisphere. The higher intensity near the circumsolar region represented in the models is probably caused by some kind of scattering effect. The same is true for the Perez model. Cheers, Wolfram -- +-------+-----Wolfram Kresse---------------------------------------------+ | _ _ | wkresse@igd.fhg.de http://www.igd.fhg.de/~wkresse | | +-------------------------+-----------------+--------------------+ | -O-O- |"Meeneemeeneemeenee" | CU l8r, LE g8r! | | > |"Yes,that's right,Twiki."+-----------------+ | _____ +-----+-----+-------------+ | U | 8^) | :u) | +-------+-----+-----+ "Life is complex. It has real and imaginary components." From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id WAA15989; Fri, 13 Feb 1998 22:35:42 +0100 Received: from adeskgate.autodesk.com (adeskgate.autodesk.com [198.93.152.11]) by imag.imag.fr (8.8.5/8.8.5) with ESMTP id WAA23517 for ; Fri, 13 Feb 1998 22:24:05 +0100 (MET) Received: from autodesk.autodesk.com by adeskgate.autodesk.com (8.6.12/SMI-5.3) with ESMTP id NAA22690; Fri, 13 Feb 1998 13:23:31 -0800 (PST) Received: from hqhubmu1.autodesk.com by autodesk.autodesk.com (8.6.12/4.4BSD) with ESMTP id NAA28667; Fri, 13 Feb 1998 13:21:46 -0800 (PST) Received: from ccinternet.autodesk.com (ccinternet [144.111.240.144]) by hqhubmu1.autodesk.com (8.7.5/8.7.3) with SMTP id NAA00274; Fri, 13 Feb 1998 13:21:45 -0800 (PST) Received: from ccMail by ccinternet.autodesk.com (IMA Internet Exchange 2.12 Enterprise) id 0037C07C; Fri, 13 Feb 1998 13:24:38 -0800 Mime-Version: 1.0 Date: Fri, 13 Feb 1998 16:21:09 -0800 Message-ID: <0037C07C.4149@autodesk.com> From: Eric Haines Subject: rendering comparisons available on web To: globillum Cc: scott owen Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit Content-Description: cc:Mail note part X-UIDL: ed645afa0023cfcf72b6146c60312556 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Due to an email request, I've put some old (7 years old or older) rendering comparison images on the web. They're at my homepage: http://www.acm.org/tog/editors/erich/index.html About 2/3rds of the way down you'll see thumbnails of sets of images showing some rendering techniques compared. Techniques include z-buffering, traditional ray tracing, stochastic ray tracing, meshed radiosity, and a ray tracing/radiosity blend (tres funky). Feel free to use them for educational purposes as you wish. Eric Haines erich@acm.org From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id VAA09621; Mon, 16 Feb 1998 21:11:34 +0100 Received: from adeskgate.autodesk.com (adeskgate.autodesk.com [198.93.152.11]) by imag.imag.fr (8.8.5/8.8.5) with ESMTP id TAA27516 for ; Mon, 16 Feb 1998 19:14:44 +0100 (MET) Received: from autodesk.autodesk.com by adeskgate.autodesk.com (8.6.12/SMI-5.3) with ESMTP id KAA20248; Mon, 16 Feb 1998 10:14:11 -0800 (PST) Received: from hqhubmu1.autodesk.com by autodesk.autodesk.com (8.6.12/4.4BSD) with ESMTP id KAA13791; Mon, 16 Feb 1998 10:12:21 -0800 Received: from ccinternet.autodesk.com (ccinternet [144.111.240.144]) by hqhubmu1.autodesk.com (8.7.5/8.7.3) with SMTP id KAA08661 for ; Mon, 16 Feb 1998 10:12:20 -0800 (PST) Received: from ccMail by ccinternet.autodesk.com (IMA Internet Exchange 2.12 Enterprise) id 00384465; Mon, 16 Feb 1998 10:16:16 -0800 Mime-Version: 1.0 Date: Mon, 16 Feb 1998 13:12:01 -0800 Message-ID: <00384465.4149@autodesk.com> From: Eric Haines Subject: articles of possible interest To: globillum Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Description: cc:Mail note part Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from quoted-printable to 8bit by www.cg.tuwien.ac.at id VAA09621 X-UIDL: c60414f16cc3c9a6d2868e08fac42050 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 The _journal of graphics tools_ has just published some articles which are likely to be of interest to globillumers. Attached is Ronen Barzel's announcement. Note that the abstracts and some additional information are available online. Eric ----------- Contents of volume 2 number 2: "The Close Objects Buffer: A Sharp Shadow Detection Technique for Radiosity Methods" A. C. Telea and C. W. A. M. van Overveld (abstract, images at http://www.acm.org/jgt/papers/TeleaVanOverveld97) "Sampling with Hammersley and Halton Points" Tien-Tsin Wong, Wai-Shing Luk, and Pheng-Ann Heng. (abstract, demo, source, images at http://www.acm.org/jgt/papers/WongLukHeng97) "A Fast Triangle-Triangle Intersection Test" Tomas Möller (abstract, source at http://www.acm.org/jgt/papers/Moller97) "Rendering Radiosity Solutions by Adaptive Gathering" A. J. Chung and A. J. Field. (abstract, images at http://www.acm.org/jgt/papers/ChungField97) For further information, see http://www.acm.org/jgt, or contact the publisher: A K Peters, Ltd. 289 Linden Street, Wellesley, MA 02181 Phone (781) 235-2210 Fax (781) 235-2204 editorial@akpeters.com Or, if you have any questions, feel free to contact me. Thanks. -Ronen Barzel Editor-in-Chief, Journal of Graphics Tools ronen@pixar.com From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id RAA12790; Fri, 13 Mar 1998 17:41:48 +0100 Received: (from daemon@localhost) by imag.imag.fr (8.8.5/8.8.5) id OAA26619 for globillum-imag-outgoing; Fri, 13 Mar 1998 14:48:24 +0100 (MET) From: Francois Sillion Message-Id: <199803131347.OAA02649@safran.imag.fr> Subject: Globillum list -- actions taken to avoid spamming To: Global Illumination List Date: Fri, 13 Mar 1998 14:47:45 +0100 (MET) Reply-To: Francois.Sillion@imag.fr X-Mailer: ELM [version 2.4 PL24] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 28f00d0b56ceaa6935a88cc921a7e758 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hello globillumers, As you know the 'globillum list' has been a target of several spam messages in the past. Our institution decided to apply a general policy with mailing lists, in order to avoid such inconvenience. Namely, postings to the list will be restricted to registered list members. I think this is compatible with our list, since most messages are coming from members anyway. But I needed to inform you because it means that you can only post from the e-mail address that is know to the list. It may be a slight problem for those with multiple e-mail addresses. More importantly, some sites are using a single email alias in the list, to serve all users locally that are interested in global illumination. These aliases must be replaced by the complete list of email addresses of individual people. Please contact me if you are in this situation, otherwise your local members will not be able to post. at least the following groups should correct the problem: > gi-students@graphics.cornell.edu (Cornell Students) > globillum@duticg.twi.tudelft.nl (Delft University of Technology graphics group) > globillum@loria.fr (LORIA Laboratory) > gimagis@safran.imag.fr (Global Illumination group at iMAGIS/IMAG) > az@robots.oxford.ac.uk (Andrew Zisserman) > glbi@cophos.co.at (Zumtobel Licht GmbH) +------------------+------------------------------------------------------+ | Francois SILLION | iMAGIS - GRAVIR/IMAG, B.P. 53, 38041 Grenoble Cedex 9| | ' | France. Tel:+33 4 76 51 43 54 - Fax:+33 4 76 63 55 80| +------------------+--------+---------------------------------------------+ | Francois.Sillion@imag.fr | http://www-imagis.imag.fr/~Francois.Sillion | +---------------------------+---------------------------------------------+ From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id TAA11316; Wed, 15 Apr 1998 19:08:43 +0200 Received: (from daemon@localhost) by imag.imag.fr (8.8.5/8.8.5) id SAA15038 for globillum-imag-outgoing; Wed, 15 Apr 1998 18:35:37 +0200 (MET DST) Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: 98/04/15 Release of RADBIB98.BIB Date: Wed, 15 Apr 1998 09:30:24 -0700 Message-ID: <01bd688b$ca5edf80$2d2aa8c0@ledalite045.ledalite.com> MIME-Version: 1.0 Content-Type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 4.71.1712.3 X-MimeOLE: Produced By Microsoft MimeOLE V4.71.1712.3 Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: d6161da70f3414ed329254eb6121c55b X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit
ANNOUNCE: 98/04/15 Release of RADBIB98.BIB
------------------------------------------
RADBIB98 is a comprehensive bibliography of radiosity and
related global illumination papers, theses, articles, and
books. It currently includes 1,340 references -- 38 new
additions since the 98/02/10 release. 
 
This bibliography is available in BibTex format as
RADBIB98.BIB (with a release date of April 15, 1998)
from: 
 
 
Also available from this site is an abridged version of
RADBIB98.BIB called GITHESIS.BIB. This bibliography
includes 154 references to radiosity and global
illumination theses -- no new additions since the 98/02/10
release. 
 
As always, it is time-consuming and sometimes difficult to
track down conference papers and theses on radiosity and
global illumination. If you know of a relevant reference
that is not included in these bibliographies, please let us
know so that we can include it in the next release. 
 
Partial financial support for the maintenance of these
bibliographies has been provided by the ACM SIGGRAPH
Special Projects.
 
Ian Ashdown, P. Eng, LC
Head of Research
Ledalite Architectural Products Inc.
http://www.ledalite.com
 
From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id XAA25171; Mon, 11 May 1998 23:18:26 +0200 Received: (from daemon@localhost) by imag.imag.fr (8.8.5/8.8.5) id XAA20146 for globillum-imag-outgoing; Mon, 11 May 1998 23:00:23 +0200 (MET DST) Message-Id: <3.0.5.32.19980511140144.00b97190@amie.engr.sgi.com> X-Sender: bwade@amie.engr.sgi.com X-Mailer: QUALCOMM Windows Eudora Pro Version 3.0.5 (32) Date: Mon, 11 May 1998 14:01:44 -0700 To: globillum@imag.fr From: Bretton Wade Subject: attenuation in water Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 65ec1eee9d78e82e173e6709e8ab280b X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hi globillumers, I'm seeking information about attenuation of light in seawater. Does anybody have any pointers? I'm not really interested in scattering due to particles in suspension, only clean, clear water. TIA, Bretton -- Bretton Wade (bwade@sgi.com) Cosmo Software - A Silicon Graphics Company From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id XAA27352; Mon, 11 May 1998 23:46:34 +0200 Received: (from daemon@localhost) by imag.imag.fr (8.8.5/8.8.5) id XAA21225 for globillum-imag-outgoing; Mon, 11 May 1998 23:28:41 +0200 (MET DST) Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: "Bretton Wade" Cc: globillum@imag.fr Subject: Re: attenuation in water Date: Mon, 11 May 1998 14:30:28 -0700 Message-ID: <01bd7d24$04c73260$2d2aa8c0@ledalite045.ledalite.com> MIME-Version: 1.0 Content-Type: text/plain; charset=windows-1252; format=flowed Content-Transfer-Encoding: 8bit X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 4.71.1712.3 X-MimeOLE: Produced By Microsoft MimeOLE V4.71.1712.3 Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: f08d7ad3ec94af4ab9b7049bdc46d5f3 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 >Hi globillumers, > >I'm seeking information about attenuation of light in seawater. Does >anybody have any pointers? I'm not really interested in scattering due to >particles in suspension, only clean, clear water. > Hi, Bretton. There is some basic information in Chapter 28, "Underwater Lighting" of the IES Lighting Handbook, Eighth Edition. It includes a discussion of the absorption coefficient (which is wavelength-dependent) , plus scattering information. The chapter includes 17 references, although these should be sufficient: Lankes, L. R. 1970. "Optics and the Physical Parameters of the Sea," Opt. Spectra 4(5):42-49. Smith, R. C., and K. S. Baker. 1981. "Optical Properties of the Clearest Natural Waters (200-800 nm)," Applied Optics 20(2):177-184. Duntley, S. Q. 1963. "Light in the Sea," J. Optical Society of America 53(2):214-233. Austin, R. W. 1970. "Assessing Underwater Visibility," Opt. Spectra 4(5):34-39. Kinney, J. A., S. M. Luria and D. O. Weitzman. 1967. "Visibility of Colors Underwater," J. Optical Society of America 57(6):802-809. Ian Ashdown, P. Eng, LC Head of Research Ledalite Architectural Products Inc. http://www.ledalite.com From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id RAA29411; Thu, 14 May 1998 17:55:43 +0200 Received: (from daemon@localhost) by imag.imag.fr (8.8.5/8.8.5) id RAA25024 for globillum-imag-outgoing; Thu, 14 May 1998 17:17:26 +0200 (MET DST) Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: globillum@imag.fr Subject: IES Lighting Handbook Date: Thu, 14 May 1998 08:18:35 -0700 Message-ID: <01bd7f4b$902d3b00$2d2aa8c0@ledalite045.ledalite.com> MIME-Version: 1.0 Content-Type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 4.71.1712.3 X-MimeOLE: Produced By Microsoft MimeOLE V4.71.1712.3 Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 516be35410d74ebc48423588f442e6f4 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit
Several people has asked me about the availability of the Illuminating Engineering Society of North America's "IES Lighting Handbook" that I referenced in an earlier message.
 
It appears that Amazon Books (www.amazon.com) is selling the 1987 IES Lighting Handbook Applications Volume. I have no idea where they are obtaining copies of this book, as it was superceded by the IES Lighting Handbook, Eighth Edition in 1993. (Even so, all the good stuff is in the companion 1987 IES Lighting Handbook Reference Volume. The two volume were combined to form a 990-page "handbook" for the 1993 edition.)
 
The IES Lighting Handbook, Eighth Edition, is available directly from the Illuminating Engineering Society of North America:
 
Tel: (212) 248-5000
Fax: (212) 248-5017
 
The cost of the book is $389.00 US for non-members and $225.00 US for members.
 
Please note that the handbook does *not* include the IESNA Lighting Library. Of particular interest may be IES LM-63, "Standard File Format for Electronic Transfer of Photometric Data" ($10.00 members, $18.00 non-members) and ANSI/IES RP-16, "Nomenclature and Definitions for Illuminating Engineering" ($10.00 members, $15.00 non-members).
 
The entire IESNA Lighting Library is available for $999.00 For members and $1,800.00 for non-members. (If you think this is expensive, check out the cost of the Commission Internationale de l'Eclairage [http://www.cie.co.at/cie/] publications.)
 
Ian Ashdown, P. Eng, LC
Head of Research
Ledalite Architectural Products Inc.
http://www.ledalite.com
 
From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id TAA11404; Fri, 22 May 1998 19:03:42 +0200 Received: (from daemon@localhost) by imag.imag.fr (8.8.5/8.8.5) id SAA22880 for globillum-imag-outgoing; Fri, 22 May 1998 18:20:01 +0200 (MET DST) Message-ID: From: "Michael Cohen (Research)" To: "'globillum@imag.fr'" Subject: FW: wavelet radiosity with triangular mesh Date: Fri, 22 May 1998 09:19:57 -0700 X-Mailer: Internet Mail Service (5.5.1960.3) Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 638abbae79279e0306129101a9deb9d8 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Someone want to take this? -Michael > -----Original Message----- > From: Berruyer [SMTP:berruyer@AVO.fr] > Sent: Friday, May 22, 1998 1:25 AM > To: Michael Cohen (Research) > Subject: wavelet radiosity with triangular mesh > > Hello, > I'm currently working on a radiosity project consisting in > comparing different algorithms. I'm now facing the wavelet > problem. As a matter of fact, all the radiosity litterature that i've read > only considers quadrilateral polygons. > Would you mind telling me if there have been researches > about wavelet radiosity with a triangular mesh ? > In this case, do you know where i could get any information ? >   > Thanks in anticipation. >   > Benoît BERRUYER > berruyer@avo.fr From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id RAA30553; Mon, 25 May 1998 17:54:51 +0200 Received: (from daemon@localhost) by imag.imag.fr (8.8.5/8.8.5) id QAA20934 for globillum-imag-outgoing; Mon, 25 May 1998 16:58:23 +0200 (MET DST) From: Nicolas Holzschuch Message-Id: <199805251456.QAA14725@yutz.loria.fr> Subject: Something is nagging me... To: globillum@imag.fr Date: Mon, 25 May 1998 16:56:12 +0200 (MDT) X-Mailer: ELM [version 2.4 PL25] MIME-Version: 1.0 Content-Type: text/plain; charset=windows-1252; format=flowed Content-Transfer-Encoding: 8bit Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 8cb4bb857573eb9d021c89e2d70ac889 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hello fellow globillumers, there is an idea that has been nagging me for some time, and I thought I would share it with the list. I couldn't help noticing there is a Workshop on Rendering for our research results, there is Siggraph for our outstanding research results. However, there is nothing to discuss the specific problems occuring in implementations of large rendering systems. I'm thinking of large, polyvalent rendering systems, with several global illumination algorithms, that deal with 500 K input polygons on a daily basis. I'm thinking about softwares like Vision, Genesis, etc. So here is the question: are there people out there interested in discussing problems specific to these issues? Expose how you deal with 500 K input polygons and 1 Gb of memory? How long does it take you to do the Soda Hall (with furnitures)? Nicolas Holzschuch Researcher, ISA Research Team, INRIA, Nancy, France. From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id RAA13310; Wed, 3 Jun 1998 17:31:59 +0200 Received: (from daemon@localhost) by imag.imag.fr (8.8.5/8.8.5) id NAA29265 for globillum-imag-outgoing; Wed, 3 Jun 1998 13:03:20 +0200 (MET DST) Message-ID: <8815647C7041D111A3010060B06BE1C0288D1D@elvis.lightwork> From: Neil Gatenby To: globillum@imag.fr Subject: gonio-photometry Date: Wed, 3 Jun 1998 12:02:07 +0100 MIME-Version: 1.0 X-Mailer: Internet Mail Service (5.0.1460.8) Content-Type: text/plain; charset=windows-1252; format=flowed Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: eacdb003eaf4ef09821fb0415f184bb0 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hi all; Does anyone know of any companies or academic institutions that can provide a gonio-photometer service for measuring the BRDFs of everyday materials? Does anyone have any experiences with such services? Does anyone know where any such data is available, to download? I know about the NIST site, with lots of data that you can't see! And I know of a European site that has some fascinating watercress BRDF data (all I need is the BRDF data for lettuce I can render a really nice salad!) any help much appreciated Neil From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id WAA18840; Wed, 3 Jun 1998 22:00:33 +0200 Received: (from daemon@localhost) by imag.imag.fr (8.8.5/8.8.5) id VAA29548 for globillum-imag-outgoing; Wed, 3 Jun 1998 21:56:16 +0200 (MET DST) Date: Wed, 3 Jun 1998 11:03:55 -0700 (PDT) From: Alain Fournier Message-Id: <199806031803.LAA14704@pedigree.cs.ubc.ca> To: Neil@lightwork.co.uk, globillum@imag.fr Subject: Re: gonio-photometry Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: faa38d2c8efd626761b829e739919c0d X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit We will soon here at UBC be able to allow people to design, simulate and conduct their own experiments (including measuring BRDF) across the web on our facility (called ACME, for ACtive MEasurement facility). It will be at leat a few weeks before we are ready, but stay tuned. "(all I need is the BRDF data for lettuce I can render a really nice salad!)" Yes, but what about the vinaigrette (dressing is the most important part of salad, without it it's just grass). From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id BAA09808; Mon, 8 Jun 1998 01:24:58 +0200 Received: (from daemon@localhost) by imag.imag.fr (8.8.5/8.8.5) id BAA03905 for globillum-imag-outgoing; Mon, 8 Jun 1998 01:20:44 +0200 (MET DST) Message-Id: <9806072320.AA10011@merckx.graphics.cornell.edu> Date: Sun, 7 Jun 1998 19:20:04 -0400 From: Eric Lafortune To: Neil@lightwork.co.uk Cc: globillum@imag.fr Subject: Re: gonio-photometry Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 97daabb0dcbcf51d138c85950b8f9e43 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Neil Gatenby wrote: > Does anyone know of any companies or academic institutions that can provide > a gonio-photometer service for measuring the BRDFs of everyday materials? > > Does anyone have any experiences with such services? Does anyone know where > any such data is available, to download? Should you be happy with just an example, we have full hemispherical BRDF data for blue latex paint available at our web site: http://www.graphics.cornell.edu/online/measurements/ The data were measured by Sing Foo, and we used them in our Siggraph'97 paper "Non-Linear Approximation of Reflectance Functions". I've just added some graphs of the function in the plane of incidence, to give a first impression of its shape. It's an interesting start for experiments. With Steve Westin (westin@graphics.cornell.edu) in charge of the measurement lab, we are doing more measurements, which may become available in the future. However, it is unlikely that we will ever be a service bureau. Kind regards, Eric Lafortune. From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id TAA24791; Thu, 11 Jun 1998 19:59:32 +0200 Received: (from daemon@localhost) by imag.imag.fr (8.8.5/8.8.5) id TAA25635 for globillum-imag-outgoing; Thu, 11 Jun 1998 19:49:36 +0200 (MET DST) Message-ID: <35801555.86656AD9@iro.umontreal.ca> Date: Thu, 11 Jun 1998 13:35:17 -0400 From: Martin Blais Organization: DIRO-UdeM X-Mailer: Mozilla 4.05 [en] (X11; I; IRIX64 6.2 IP28) MIME-Version: 1.0 To: Global Illumination List , IBR List Subject: Wanted: EGWR proceedings (your conference copies). Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 8bit Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: f5cec6a6dbc87b27f8c308aa294267df X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hi global and image-based illuminationerers. I know some of you who attend the EGWR actually buy the "published" proceedings after the conference (the nice, very expensive ones). Unfortunately, a masters student like me cannot afford those (yet :-). I know this is probably a shot in the dark, but I'm very interested in buying your conference version (the cheaper, photocopies-like version you receive at EGWR itself). So if you want to get rid of them, I'll give you a few bucks for them, and we can meet at SIGGRAPH'98 to do the exchange. If you're interested, you can contact me at blais@iro.umontreal.ca Best regards to all, M. P.S. Apologies to those people both on the globillum and IBR lists, you'll receive this post twice. -- \-----------------------------------------------------------/ \ Martin Blais Universite de Montreal / / mailto:blais@iro.umontreal.ca Computer graphics lab. \ / http://www.iro.umontreal.ca/~blais \ "Lui parler de tout, de rien; de rien surtout, c'est ce qui nous tracasse le plus." ---Nor, "Des nouvelles du Bon Dieu" From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id LAA07052; Wed, 17 Jun 1998 11:56:04 +0200 Received: (from daemon@localhost) by imag.imag.fr (8.8.5/8.8.5) id LAA06682 for globillum-imag-outgoing; Wed, 17 Jun 1998 11:39:27 +0200 (MET DST) Date: Wed, 17 Jun 1998 11:36:49 +0200 (MDT) Message-Id: <199806170936.LAA08522@yutz.loria.fr> From: Nicolas Holzschuch To: globillum@imag.fr Subject: PhD thesis bursary Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 48713258a922eec2a5193e578543b1e7 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Hello fellow globillumers, We are looking for a PhD student, starting september 1998. The PhD would be funded by a CIFRE convention. The student would be working with the ISA research team, following our research on global illumination algorithms and hierarchical radiosity. Since the bursary is a CIFRE, there will be some part of interaction with industries. Applications and requests for further information should be directed to Jean-Claude Paul (Jean-Claude.Paul@inria.fr). Nicolas Holzschuch ISA research team, INRIA-Lorraine. From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id MAA08677; Wed, 17 Jun 1998 12:58:45 +0200 Received: (from daemon@localhost) by imag.imag.fr (8.8.5/8.8.5) id MAA10391 for globillum-imag-outgoing; Wed, 17 Jun 1998 12:46:28 +0200 (MET DST) From: Nicolas Holzschuch Message-Id: <199806171043.MAA08700@yutz.loria.fr> Subject: Re: PhD thesis bursary To: Nicolas Holzschuch Date: Wed, 17 Jun 1998 12:43:46 +0200 (MDT) Cc: globillum@imag.fr In-Reply-To: <199806170936.LAA08522@yutz.loria.fr> from "Nicolas Holzschuch" at Jun 17, 98 11:36:49 am X-Mailer: ELM [version 2.4 PL25] MIME-Version: 1.0 Content-Type: text/plain; charset=windows-1252; format=flowed Content-Transfer-Encoding: 8bit Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: de462a27bd11dceb340777d5771d71ee X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 > Hello fellow globillumers, Sorry for the double posting. I forgot to mention that if you want to know more about the ISA research team, you can take a look at our web page, http://www.loria.fr/equipes/isa/ Nicolas Holzschuch ISA research team, INRIA Lorraine http://www.loria.fr/~holzschu/ > We are looking for a PhD student, starting september 1998. The PhD > would be funded by a CIFRE convention. The student would be working > with the ISA research team, following our research on global > illumination algorithms and hierarchical radiosity. > > Since the bursary is a CIFRE, there will be some part of interaction > with industries. > > Applications and requests for further information should be directed > to Jean-Claude Paul (Jean-Claude.Paul@inria.fr). > > Nicolas Holzschuch > ISA research team, INRIA-Lorraine. > From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id QAA03960; Tue, 23 Jun 1998 16:44:18 +0200 Received: (from daemon@localhost) by imag.imag.fr (8.8.5/8.8.5) id QAA26166 for globillum-imag-outgoing; Tue, 23 Jun 1998 16:09:25 +0200 (MET DST) From: Francois Sillion Message-Id: <199806231408.QAA04576@safran.imag.fr> Subject: no subject (file transmission) To: Global Illumination List Date: Tue, 23 Jun 1998 16:08:47 +0200 (MDT) Reply-To: Francois.Sillion@imag.fr X-Mailer: ELM [version 2.4 PL24] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: a120d53dc84ae83fd59f3bdc5cd54941 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Dear Globillumers, I feel terrible for taking so long to come back to the issue of email address filtering on globillum. Some of you might be wondering why their messages took so long to appear on the list. As I said, our administrators here decided to prevent posting to mailing lists from non-members. Since the filter is based on the email address used to register you in the list, any email sent from another address will be blocked. I am appending in the next message the current list of addresses I have. Please take a minute to check that your address is correct, and is the one used when you *send* messages. Some people certainly have a problem, if they use a different email address for receiving and sending messages. I don't have a real answer for them, the only workaround I can see is to add both of their addresses (they may then receive two copies of each and every message). When the duplication is due to an anti-spam scheme, one might hope that one of the two copies will be blocked as "spam" :-) Anyway, you should ALWAYS be careful when sending email to the list and check that you are sending from the "authorized" address. I am also appending a number of messages which were blocked by our system. Again, please excuse the delay. The authors of all these messages should definitely contact me to solve the problem. Please contact me if you have any questions or want your address changed. +------------------+------------------------------------------------------+ | Francois SILLION | iMAGIS - GRAVIR/IMAG, B.P. 53, 38041 Grenoble Cedex 9| | ' | France. Tel:+33 4 76 51 43 54 - Fax:+33 4 76 63 55 80| +------------------+--------+---------------------------------------------+ | Francois.Sillion@imag.fr | http://www-imagis.imag.fr/~Francois.Sillion | +---------------------------+---------------------------------------------+ ------------------------------------------------------------------------ Messages that got blocked: please read and make sure they did not come from you! ------------------------------------------------------------------------ Subject: BOUNCE globillum@imag.imag.fr: Non-member submission from ["Stephen H. Westin" ] Subject: Re: IES Lighting Handbook Reply-To: westin@graphics.cornell.edu References: <01bd7f4b$902d3b00$2d2aa8c0@ledalite045.ledalite.com> Ian Ashdown wrote: > The IES Lighting Handbook, Eighth Edition, is available directly from = > the Illuminating Engineering Society of North America: > > Tel: (212) 248-5000 > Fax: (212) 248-5017 > URL: www.iesna.org > > The cost of the book is $389.00 US for non-members and $225.00 US for = > members. And note that membership dues are less than the difference; it's worth joining just to save money on the handbook. -Stephen H. Westin Any information or opinions in this message are mine: they do not represent the position of Cornell University or any of its sponsors. ------------------------------------------------------------------------ Subject: BOUNCE globillum@imag.imag.fr: Non-member submission from [Fredo Durand ] Date: Tue, 19 May 1998 10:40:53 +0200 From: Fredo Durand Organization: iMAGIS Subject: siggraph 98 papers on the net Hi, with the help of Tim Rowley, I've gathered a lot of links on the electronic versions of the papers that will be presented at siggraph this year. They are available at http://www-imagis.imag.fr/Membres/Fredo.Durand/Book/sig98.html Not all papers are available at the moment, if you know a link I have forgotten or missed, please let me know. By the way, these are part of my collection of computer graphics links where you can find web pages of researchers, labs, conferences, image galleries, code, etc. http://www-imagis.imag.fr/~Fredo.Durand/book.html Fredo Durand iMAGIS Grenoble, France http://www-imagis.imag.fr/~Fredo.Durand ------------------------------------------------------------------------ Subject: BOUNCE globillum@imag.imag.fr: Non-member submission from ["Ian Ashdown" ] From: "Ian Ashdown" To: Cc: Subject: UNIX-based radiosity renderer available Date: Thu, 21 May 1998 09:37:31 -0700 Dr. Ugur Gudukbay (gudukbay@CS.Bilkent.Edu.TR) and his students at the Department of Computer Engineering and Information Science, Bilkent University (Ankara, Turkey) have kindly ported my hopelessly Windows-centric Helios Radiosity Renderer to the UNIX operating environment. If anyone is looking for C++ source code for a basic but effective progressive radiosity renderer, you can download helios_tar.tar from http://www.cs.bilkent.edu.tr/~gudukbay/home.html. Ian Ashdown, P. Eng. | READ THE BOOK! Vice President, R & D | Radiosity: A Programmer's Perspective byHeart Consultants Limited | John Wiley & Sons 1994 West Vancouver, BC (Canada) | http://mypage.direct.ca/b/byheart ------------------------------------------------------------------------ Subject: BOUNCE globillum@imag.imag.fr: Non-member submission from ["A. T. Campbell, III" ] Date: Fri, 22 May 1998 14:35:49 -0500 From: "A. T. Campbell, III" Subject: new job/address Friends/Colleagues/etc., I have recently started a job at Schlumberger. My new contact information, effective immediately, is below: e-mail: atcampbell@slb.com address: Schlumberger Austin Product Center 8311 North FM 620 Austin, Texas 78726 USA phone: (512)331-3382 My home address has not changed Thanks for your time. -- A. T. Campbell, III (atcampbell@slb.com) Phone:(512)331-3382 Fax:(512)331-3387 Schlumberger Austin Product Center, 8311 N. FM 620, Austin, TX 78726 ------------------------------------------------------------------------ Subject: BOUNCE globillum@imag.imag.fr: Non-member submission from ["Andrew J. Willmott" ] Date: Fri, 22 May 1998 21:34:55 -0400 To: berruyer@AVO.fr From: "Andrew J. Willmott" Subject: Re: FW: wavelet radiosity with triangular mesh Cc: globillum@imag.fr >> Hello, >> I'm currently working on a radiosity project consisting in >> comparing different algorithms. I'm now facing the wavelet >> problem. As a matter of fact, all the radiosity litterature that i've read >> only considers quadrilateral polygons. >> Would you mind telling me if there have been researches >> about wavelet radiosity with a triangular mesh ? >> In this case, do you know where i could get any information ? >> >> Thanks in anticipation. >> >> Benot BERRUYER >> berruyer@avo.fr I know that at least Philippe Bekaert and I have adapted wavelet radiosity to triangular meshes. (I think there are also some triangular coefficients listed in Peter Schroeder's thesis.) I have a technical note online at http://www.cs.cmu.edu/~radiosity/notes/note-coeffs.[ps|pdf] which discusses wavelet radiosity operations in a matrix-oriented setting, lists the necessary coefficients for these operations, and gives some examples of how to use them. It includes coefficients for the M[2-3], F[2-3] bases for both quadrilaterals and triangles. You may also want to download Philippe et. al's RenderPark and/or my 'rad' radiosity program and try looking at the code. They can be found at: http://www.cs.kuleuven.ac.be/cwis/research/graphics/RENDERPARK http://www.cs.cmu.edu/~radiosity/dist Cheers, Andrew --- mailto:a.willmott@cs.cmu.edu ------- http://www.cs.cmu.edu/~ajw --- ------------------------------------------------------------------------ Subject: BOUNCE globillum@imag.imag.fr: Non-member submission from ["Stephen H. Westin" ] Date: Tue, 2 Jun 1998 11:46:40 -0400 From: "Stephen H. Westin" To: globillum@imag.fr Subject: Thesis on-line My old Master's thesis (from 1992) has made it to the Web: Also available are: o '92 SIGGRAPH paper (full text and images) o Images from the paper, thesis, and SIGGRAPH talk o Microgeometry for a Gaussian rough surface, used in the paper and the thesis ------------------------------------------------------------------------ Subject: BOUNCE globillum@imag.imag.fr: Non-member submission from ["Stephen H. Westin" ] Subject: Re: gonio-photometry > Hi all; > > Does anyone know of any companies or academic institutions that can provide > a gonio-photometer service for measuring the BRDFs of everyday materials? > > Does anyone have any experiences with such services? Does anyone know where > any such data is available, to download? We have a gonioreflectometer that I think of as being on the verge of operational. While we have no plans to offer a measurement service, we have posted one measured BRDF, with hopes for more in the future. See ------------------------------------------------------------------------ Subject: BOUNCE globillum@imag.imag.fr: Non-member submission from [hertjwr@us.ibm.com] From: hertjwr@us.ibm.com To: globillum@imag.fr cc: pellelgrini@imc.pi.cnr.it Date: Sun, 21 Jun 1998 12:54:03 -0400 Subject: form factors on line Hi Globillumers -- I don't remember anyone else bringing this up, but I have been a little out of touch so maybe I missed it. Anyway, I just found that Jack Howell's "Catalog of Radiation Heat Transfer Configuration Factors" is now on line (it used to be only in a book that you could only find in some Engineering libraries). It's at: http://sage.me.utexas.edu/~howell/ Section C is not completely filled in, so perhaps it is still a work in progress. At least now everyone can have access to infamous cow factors: http://sage.me.utexas.edu/~howell/sectionb/b-63.html -- Holly Rushmeier holly@watson.ibm.com From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id QAA03928; Tue, 23 Jun 1998 16:42:42 +0200 Received: (from daemon@localhost) by imag.imag.fr (8.8.5/8.8.5) id QAA26233 for globillum-imag-outgoing; Tue, 23 Jun 1998 16:09:57 +0200 (MET DST) From: Francois Sillion Message-Id: <199806231409.QAA04591@safran.imag.fr> Subject: GLOBILLUM: new messages and important email-address issue To: Global Illumination List Date: Tue, 23 Jun 1998 16:09:18 +0200 (MDT) Reply-To: Francois.Sillion@imag.fr X-Mailer: ELM [version 2.4 PL24] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: e4dc56d2b93a666b7f231ca2e4f4b113 X-Mozilla-Status: 9001 X-Mozilla-Status2: 00000000 ------------------------------------------------------------------------ ### Global Illumination mailing list # # # append the following to your .mailrc file # # send corrections/additions to globillum-request@imag.fr # (which is forwarded to Francois Sillion) # The preferred way to send mail to everyone on the list is to mail to # globillum (aliased below), where a master copy of list is being maintained. # Maneesh Agrawala; PhD Student, Stanford University alias agrawala maneesh@uni.Stanford.EDU # Farah Al-Agha; University of Bristol, England. # I am interested in the following areas: Hierarchical Radiosity, # Discontinuity meshing, virual studio, Augmented reality and virtual reality. alias alagha alagha@cs.bris.ac.uk # Mike Allison alias mallison mike@documentum.com # Carlos Urena Almagro; ETS Ingenieria Informatica; # Universidad de Granada; 18071 Granada; Spain alias almagro almagro@goliat.ugr.es # John Amanatides, York U, Toronto alias amanatides amana@cs.yorku.ca # Jason Andreas; illipse Inc # CG interests; natural-phenomena, more specifically, realistic # lightning simulation, plants/trees, and clouds to go with the lightning alias andreas jandreas@ultranet.com # Jean-Christophe Arnu; IUP Ingenierie de Systemes Informatiques de Toulouse alias arnu isi2g7@cict.fr # Jim Arvo; California institute of technology alias arvo arvo@cs.caltech.edu # Ian Ashdown; Ledalite Architectural Products Inc.; Langley, B.C.; Canada alias ashdown iashdown@ledalite.com # Godavarthy Sreenadha Babu ; University of South Carolina # I am looking at single pass algorithms for accurate solutions to global # illumination problem. My major focus right now is on wavelets, sparse # representation of the integral operators and error analysis of the # integral solution. alias babu godavart@cs.sc.edu # Sanjay Bakshi; SGI alias bakshi sbakshi@aw.sgi.com # Kavita Bala; MIT graphics group alias bala kaybee@graphics.lcs.mit.edu # Gladimir V.G. Baranoski; University of Calgary alias baranoski gbaranos@cpsc.ucalgary.ca # Rui Bastos; Graduate Student, University of North Carolina at Chapel Hill alias bastos bastos@cs.unc.edu # Dan Baum, Silicon Graphics alias baum drb@sgi.com # Philippe Bekaert; K. U. Leuven (Belgium) alias bekaert philippe@idefix.cs.kuleuven.ac.be # Sergio Gonzalo Besuievsky; Universitat de Girona alias besuievsky gonzalo@baloo.udg.es # Christian-A. Bohn; Dept. Visualization and Media Systems Design (VisWiz,VMSD) # Institute for Media Communication (IMK), GMD. alias bohn bohn@gmd.de # Samuel Boivin ; INRIA alias boivin Samuel.Boivin@inria.fr # Chris Borel; SST-8, MS D438; Los Alamos National Lab; Los Alamos, NM 87545 # interests: simulation of lighting under vegetative canopies alias cborel cborel@lanl.gov # Kadi Bouatouch; IRISA; Campus de Beaulieu; 35042 Rennes Cedex; France # interests: ray tracing, sampling, realism, physics & perception alias bouatouch Kadi.Bouatouch@irisa.fr # Chris Buckalew, Cal Poly alias buckalew buckalew@polyslo.calpoly.edu # Eduardo Bustillo Iceta; # My main interests are Monte Carlo radiosity, meshing techniques, # BDRF modelization and artificial intelligence alias bustillo epabuice@bicc00.bi.ehu.es # Emilio Camahort; University of TExas Austin alias camahort ecamahor@cs.utexas.edu # Alvin T. Campbell III; Schlumberger Austin Product Center 8311 North FM 620 # Austin, Texas 78726 USA phone: (512)331-3382 # interests: global illumination, heat transfer, animation, scientific vis. alias campbell atcampbell@slb.com # Pedro Cano Olivares; Universidad de Granada, Spain alias canoolivares pcano@goliat.ugr.es # Marcos C. C. Carrard; University of Ijuí (Brazil) alias carrard carrard@sede.unijui.tche.br # Mateu Sbert Casasayas # interests: doing thesis on Monte Carlo radiosity alias casasayas sbert@lsi.upc.es # Alan Chalmers; Dept. of Computer Science; University of Bristol; # University Walk; Bristol; BS8 1TR; United Kingdom # interests: large parallel MIMD computers for radiosity and ray tracing alias achalmers alan@compsci.bristol.ac.uk # Michael Chelle alias chelle chelle@bcgn.grignon.inra.fr # Eric Chen, Apple alias chen chense@rlspace.com # Niels J. Christensen; Technical U. Denmark; B. 116, DK-2800 Lyngby; Denmark alias nchristensen iftnjc83@vm.uni-c.dk # Per H. Christensen; mental images, Fasanenstrasse 81, D-10623 Berlin, Germany # interests: global illumination, photorealistic rendering, shape from shading alias pchristensen per@mental.com # Adrian J. Chung; Imperial College of Science, Technology and Medicine, London #Computationally intensive applications like those found in global illumination #pose are typically developed with the implicit assumption of a high-end #uniprocessor with practically infinite RAM. My research focuses on the porting #issue, particularly when making use of parallelism. alias chung ajc@doc.ic.ac.uk # Michael Cohen, Microsoft alias mcohen mcohen@microsoft.com # Steven Collins; Image Synthesis Group, Trinity college, Dublin # Interests: light ray tracing, illumination from transparent objects, # distribution ray tracing, wavefront tracking. alias collins Steven.Collins@cs.tcd.ie # Antonio Costa; Comp. Graphics & CAD; INESC; # Largo Mompilher 22; 4100 Porto Portugal alias costa acc@asterix.inescn.pt # Cornell Students, includes Himlan & others; but not Greenberg or Arvo alias cornell_students gi-students@graphics.cornell.edu # Andre Mauricio CUNHA CAMPOS; ISIMA, Clermon-Ferrand, France alias cunha andre@sp.isima.fr # Brian Curless; Stanford # interests: zonal radiosity methods alias curless curless@candor.Stanford.EDU # Jubin P. Dave; U. of New Hampshire alias jdave jd@kepler.unh.edu # DENIEL Jean-Marc; CSTB, 11 rue Henri Picherit,B.P. 82341,44323 Nantes Cedex 3 alias deniel deniel@cstb.fr # David L. DiLaura; Senior Instructor, Civil and Architectural Engineering; # University of Colorado; Boulder, CO 80309 alias dilaura dilaura@bechtel.colorado.edu # Akio Doi; SUNY Stony brook. # My interest fields are a global illumination model, radiosity, volume # rendering, volume graphics, and so on. alias doi doi@sbcs.cs.sunysb.edu # Gavin Donaldson-Selby; Technikon Natal, Durban, South Africa. # application of global illumination techniques (and software) in stage # lighting design. alias donaldson artlite@iaccess.za # Julie Dorsey; Assistant Professor, Architecture, MIT alias dorsey dorsey@graphics.lcs.mit.edu # George Drettakis, iMAGIS/IMAG, BP 53 F-38041 Grenoble Cedex 09 France # interests: sampling and filtering techniques for GI, quality & error metrics alias drettakis George.Drettakis@imag.fr # Emmanuel Dumont; Universite de Montreal # rendering of natural phenomena alias dumont dumont@iro.umontreal.ca # Fredo Durand; iMAGIS, Grenoble, France alias fdurand Fredo.Durand@imag.fr # Philip Dutre; Computer Graphics Research Group, Katholieke Universiteit Leuven # Interests: Monte Carlo solutions for global illumination, adaptive # probability density functions, potential-driven algorithms alias dutre Philip.Dutre@cs.kuleuven.ac.be # Pavol Elias; Technical University Vienna alias elias elias@cg.tuwien.ac.at # Dieter Fellner; Bonn University, Germany alias fellner fellner@cs.uni-bonn.de # James A Ferwerda; Cornell University alias ferwerda jaf@graphics.cornell.edu # Eugene Fiume, U. of Toronto alias fiume elf@dgp.utoronto.ca # David Forsyth alias forsyth daf@CS.Berkeley.EDU # Alain Fournier, U. of British Columbia, Vancouver BC, Canada alias fournier fournier@cs.ubc.ca # Don Fussell, U. of Texas, Austin alias fussell fussell@cs.utexas.edu # Gonzalo Cerruela Garcia; # I am doctoral student in Computer Science . I interesting in Radiosity # method for global illumination . alias garcia el1segag@sun630.uco.es # Robert Garmann; University of Dortmund # rendering, hierarchical methods, monte-carlo-methods, parallel computing alias garmann garmann@ls7.informatik.uni-dortmund.de # Neil Gatenby, Manchester Computing Centre, Manchester, England # interests: alternatives to hemicube, accurate numerical form factors alias gatenby neil@lightwork.co.uk # Joe Geigel; Pittsburgh Supercomputing Center alias geigel geigel@psc.edu # Reid Gershbein; Stanford University alias gershbein rsg@uni.stanford.edu # Simon Gibson # Interests: Hierarchical Radiosity: Error-Estimates/Mesh Optimisation/Parallel # Implementations/Dynamic Environments and use in Virtual Reality. alias gibson gibsons@cs.man.ac.uk # Stephen Gifford, Electrical and Computer Engineering Dept, Carnegie Mellon # interests: implemented radiosity/ray tracing hybrid on Connection Machine alias gifford Stephen.Gifford@maps.cs.cmu.edu # Andrew Glassner, Microsoft alias glassner glassner@microsoft.com # Narendra Goel, Wayne State U. alias goel ngoel@cs.wayne.edu # Martin Grabenstein; Mental Images alias grabenstein martin@mental.de # Chuck Grant, Lawrence Livermore Lab alias grant grant1@llnl.gov # Don Greenberg c/o Fran Brown, Cornell U. alias greenberg dpg@graphics.cornell.edu # Larry Gritz ; Pixar alias gritz lg@pixar.com # Leo Guibas; CS Dept, Stanford U. / DEC Systems Research Center, Palo Alto alias guibas guibas@cs.stanford.edu # Eric Haines, 3D/Eye alias haines erich@acm.org # Pat Hanrahan, Stanford U. alias hanrahan hanrahan@cs.stanford.edu # Brian W. Heal; School of Information Science; Portsmouth Polytechnic; # Mercantile House; Hampshire Terrace; Portsmouth, PO1 2EG; United Kingdom # interests: rendering octree models, post-hidden-surface-removal rendering alias heal healb@csovax.portsmouth.ac.uk # Paul Heckbert; Computer Science Dept.; Carnegie Mellon University; # 5000 Forbes Ave; Pittsburgh PA 15213-3891; USA # interests: finite element & integral equation methods for global illumination alias heckbert ph@cs.cmu.edu # David Hedley alias hedley hedley@cs.bris.ac.uk # Wolfgang Heidrich; University of Erlangen # I am a PhD student at the University of Erlangen with research interests in # both global illumination and hardware accellerated rendering alias heidrich heidrich@informatik.uni-erlangen.de # Steve Hollasch; Microsoft alias hollasch stevehol@MICROSOFT.com # Nicolas Holzschuch. INRIA Lorraine. alias holzschuch Nicolas.Holzschuch@loria.fr # Helen H. Hu; Univ. of Utah alias helenhu hhh@facility.cs.utah.edu # Philip Hubbard; Washington University # My research interests include global illumination and time-critical # algorithms for the real-time display of global-illumination solutions. alias hubbard pmh@cs.wustl.edu # Alexander Ivanov alias ivanov Alexander.Ivanov@comlab.ox.ac.uk # A. M. Jelle Post; TU Delft # physically correct lighting studies in the architects designing stage. alias jelle zeno@euronet.nl # Henrik Wann Jensen; Institute of Graphical Communication # Technical University of Denmark; Building 116; 2800 Lyngby; Denmark alias jensen henrik@mental.com # J. P. Jessel; Institut de Recherche en Informatique de Toulouse; # Universite Paul Sabatier; 31062 Toulouse; France # interests: parallel radiosity and ray tracing algorithms on Transputers alias jessel jessel@irit.fr # Graham Jones; Oxford U. alias gjones graham@robots.oxford.ac.uk # Fern Hunt; NIST alias hunt fern.hunt@nist.gov # Vincent Jolivet; Faculte des Sciences de LIMOGES alias jolivet jolivet@unilim.fr # Kazufumi Kaneda; Electric Machinery Lab, Hiroshima U. alias kaneda kin@eml.hiroshima-u.ac.jp # Konrad F. KARNER; Institute for Computer Graphics; # Graz University of Technology alias karner karner@icg.tu-graz.ac.at # Alexander Keller ; Universitaet Kaiserslautern. Fachbereich Informatik # D-67653 Kaiserslautern. Postfach 3049. alias keller keller@informatik.uni-kl.de # Lawrence Kesteloot; # I'm a graduate student at the University of North Carolina. My interests # are global illumination through path tracing and other monte carlo methods. alias kesteloot kesteloo@cs.unc.edu # Slawomir Kilanowski; Software engineer developing 3D graphics applications. # Owner of one-man software company rendering development services. # Specific interests in global illumination: Fast, robust methods for # calculation of interreflected light in architectual visualization. alias kilanowski metagram@pwr.wroc.pl # Dave Kirk alias kirk davidk@nvidia.com # Arjan Kok; TNO-FEL, P.O.Box 96864, 2509 JG 's-Gravenhage, The Netherlands alias kok kok@fel.tno.nl # Craig Kolb, Stanford (but email address is Princeton) alias kolb cek@cs.princeton.edu # Juhana Kouhia; # I'm mathematics student (with studies in physics) and just interested # in the theory of global illumination. alias kouhia kouhia@nic.funet.fi # Wolfram Kresse ; Fraunhofer IGD, Darmstadt # Our group is developing a tool for Raytracing, Radiosity and # VR model preparation. alias kresse wkresse@igd.fhg.de # Subodh Kumar; Computer Science, UNC, Chapel Hill NC 27599 alias kumar kumar@cs.unc.edu # Eric Lafortune; Cornell University Progra of COmputer Graphics # interests: mathematical models and Monte Carlo techniques alias lafortune eric@graphics.cornell.edu # Paul Lalonde, U. of British Columbia alias lalonde lalonde@cs.ubc.ca # Mathias Lang; DACOS Software GmbH. Software engeneer at SAP alias lang mathias.lang@sap-ag.de # Michael Langer; NEC Research Institute. # I am computer vision researcher interested in how material and shape # properties of surfaces can be automatically recovered from images. alias langer langer@research.nj.nec.com # George Leaver; University of Manchester, England # currently undertaking an M.Sc in the Computer Graphics Unit of the university. # Interests: Higher Order Radiosity and NURBS alias leaver leaverg@cs.man.ac.uk # Justin Legakis; MIT alias legakis legakis@graphics.lcs.mit.edu # Marc Levoy, CS Dept, Stanford U. alias levoy levoy@cs.stanford.edu # Bob Lewis; CS Dept; U. of British Columbia; # 6356 Agricultural Road; Vancouver, BC V6T 1W5; Canada # interests: 3-D texture, ray tracing, radiosity, parallelism alias blewis bobl@cs.ubc.ca # Lewis; Dept. Geography; University College London # 26 Bedford Way; London WC1H 0AP; UK # I don't use a first name, "I'm known just as Lewis" # interests: modeling canopy reflectance, remote sensing alias plewis plewis@ps.ucl.ac.uk # Robert Lipman, NIST # I work on a project related to the reflectance (appearance) of materials alias lipman robert.lipman@nist.gov # Lars Lippert; Swiss Federal Institute of Technology Zuerich # I am a research assistant and I am working on my PhD-Thesis. I am generally # interested in global illumination and multiresolution approaches. alias lippert lippert@inf.ethz.ch # Dani Lischinski; Hebrew University of Jerusalem alias lischinski danix@cs.huji.ac.il # LORIA laboratory; (Nancy, France) INRIA-lorraine, CRIN alias loria globillum@loria.fr # Celine Loscos; iMAGIS, Grenoble, France alias loscos Celine.Loscos@imag.fr # Hugh McCabe; University College Dublin, Ireland alias mccabe hugh.mccabe@ucd.ie # Ann Mc Namara; Univ. of Bristol, Vision & Graphics Lab. alias mcnamara mcnamara@cs.bris.ac.uk # Alois Maierhofer ; TU Graz (Austria) alias maierhofer ali@icg.tu-graz.ac.at # Eric Maisel; IRISA, Rennes, France alias maisel maisel@irisa.fr # Dinesh Manocha; UNC # interested in problems related to modeling and rendering. # recent work on problems in display large datasets ( polygons or NURBS) # and eventually radiositizing them. alias manocha manocha@cs.unc.edu # Mathieu Marache ; LORIA #marache = Mathieu Marache = Mathieu.Marache@loria.fr # John Mardaljevic; De Montfort University alias mardaljevic jm@dmu.ac.uk # Daniele Marini; Eidomatics Lab, Computer Science Dept, Univ. of Milan; Italy # interests: radiosity, ray tracing, parallel processing (Meiko) alias marini marini@imiucca.csi.unimi.it # Ignacio Martin Campos # Universitat Politecnica de Catalunya # interests: radiosity and dynamic environments alias imartin imartin@ima.udg.es # Nelson Max, Lawrence Livermore Lab alias max max2@llnl.gov # Daniel Meneveaux; IRISA, Rennes, France alias meneveaux dmenevea@irisa.fr # Christian Metge; Institut de Recherche en Informatique de Toulouse; # Universite Paul Sabatier; 31062 Toulouse; France # interests: parallel discrete radiosity and ray tracing algorithms # (Transputers, workstation networks) alias metge metge@irit.fr # Don Mitchell, Microsoft alias dmitchell donm@microsoft.com # Tomas Moller; Lund Institute of Technology # developping a radiosity program for use with Virtual Reality applications. alias moller tompa@clarus.se # Hassan Moubaraki; MIC (Media Integration and Communications) # ATR Research Labs in Kyoto, Japan # My research topics include computer animation and graphics (facial # animation) and I am interested in some research issues in global illumination. alias moubaraki moubarak@mic.atr.co.jp # Gordon Mueller; Univ. Bonn # My research interests are widespread: # efficient raytracing and radiosity in general; alias gmueller mueller@graphics.cs.uni-bonn.de # Ken Musgrave; The George Washington University # Interests: natural phenomena, e.g., light propagation in nature. alias musgrave musgrave@seas.gwu.edu # Karol Myszkowski; The University of Aizu # My interest in global illumination are focused on practical lighting # simulation algorithms handling complex environments, experimental validation # of such algorithms, psyhophysiological aspects of image display. alias myszkowski k-myszk@u-aizu.ac.jp # Fabrice Neyret; I.N.R.I.A. Rocquencourt, Projet Syntim alias neyret Fabrice.Neyret@imag.fr # Nguyen Duc Cuong; TU Dresden alias nguyen cn1@irz.inf.tu-dresden.de # Jeffry Nimeroff; Penn University alias nimeroff jnimerof@graphics.cis.upenn.edu # Tomoyuki Nishita; Electric Machinery Lab, Hiroshima U. alias nishita nis@eml.hiroshima-u.ac.jp # Eric Paquette; Universite' de Montre'al # Student, Master's degree at Universite de Montreal (Canada) # Interested in radiosity, monte-carlo and ray-tracing techniques used for # global illumination. alias paquette bs527@freenet.carleton.ca # Christopher Patmore; Programming Research Group; Oxford U. # interests: skylight radiosity alias patmore cjp@prg.oxford.ac.uk # Gustavo Patow; University of Girona # My main interest is finding faster ways to compute photorrealistic # images, specially solving the global illumination problem (or parts of # it! :-) ) in a fast and more or less accurate way alias patow dagush@sol.info.unlp.edu.ar # Sumant Narayan Pattanaik; IRISA; Rennes; France alias pattanaik sumant@graphics.cornell.edu # Charles Patterson; Georgia Tech # I'm a Ph.D. at Georgia Tech and I work on radiosity clustering. # My formal advisor is Dr. Holly Rushmeier. alias patterson charliep@cc.gatech.edu # Mathias Paulin; Institut de Recherche en Informatique de Toulouse; # Universite Paul Sabatier; 31062 Toulouse; France # interests: parallel radiosity and ray tracing algorithms (Transputers, PVM) # shadow accuracy, transfer simulations in dense foliage alias paulin paulin@irit.fr # Hans K. Pedersen; Stanford University alias pedersen hkp@aperture.stanford.edu # Frederic Perez Cazorla; University of Girona alias perez frederic@ima.udg.es # Bernard Peroche; Ecole des Mines de Saint Etienne # domains of interest : ray tracing, color reproduction, BRDF models alias peroche peroche@emse.fr # Ingmar Peter; University of Dortmund # I am student of computer science at the University of Dortmund and currently # writing my master theses, an object-oriented Monte-Carlo Ray-Tracer. alias ipeter peter@ls7.informatik.uni-dortmund.de # Sylvain Petitjean; ISA project, CRIN, Nancy (France) alias petitjean Sylvain.Petitjean@loria.fr # Fabrizio Pezzola; eyeTech Graphix; I am a computer engineering student and # I'm writing a Ray-tracer which use global illumination algorithms. alias pezzola mc4242@mclink.it # Matt Pharr alias pharr mmp@lux.Stanford.EDU # Georg Pietrek; Universitaet Dortmund. # radiosity, combination radiosity/ray tracing, OO design for rendering programs alias pietrek pietrek@ls7.informatik.uni-dortmund.de # Pierre Poulin; Dept. IRO, Universite de Montreal, # C.P. 6128, succ. Centre-Ville, Montreal, Quebec, Canada H3C 3J7 # interests: illumination, rendering, realism alias poulin poulin@iro.umontreal.ca # Bob Powell ; Rhythm and Hues. http://www.rhythm.com/~bpowell/index.html alias powell bpowell@rhythm.com # Jan Prikryl; T.U. Vienna, Institute of Computer Graphics and Visualisation alias prikryl prikryl@cg.tuwien.ac.at # Claude Puech; iMAGIS/IMAG, BP 53, F-38041 Grenoble Cedex 9. France alias puech Claude.Puech@imag.fr # Xavier Pueyo; Dept. Llenguatges i Sistemes Informatics; # Universitat Politecnica de Catalunya; Av. Diagonal, 647 planta 8; # 08028-Barcelona; Spain; # interests: diffuse environments alias pueyo xavier@ima.udg.es # Werner Purgathofer; Institute of Computer Graphics; Techn. Univ. Vienna; # Karlsplatz 13 / 186; A-1040 Wien / Austria # interests: radiosity, ray tracing, color, virtual reality, # dithering and quantization alias purgathofer wp@cg.tuwien.ac.at # Szymon Rusinkiewicz ; stanford # I am currently working in BRDF measurement and representation, and am also # interested in the relation between spatially varying BRDFs and light fields. alias rusinkiewicz smr@cs.stanford.edu # Ari Rappoport alias rappoport arir@cs.huji.ac.il # Jordi Regincos alias regincos jordir@upisun4.uab.es # Panu Rekola; Computer Science Dept, Helsinki U. of Tech.; Finland alias rekola pre@cs.hut.fi # Luc Renambot; IRISA # I began a PhD at IRISA in Rennes about the parallelization # of global illumination and radiosity methods. alias renambot renambot@irisa.fr # Erik Robson: interested in Global illumination's advantages in architectural # situations, as a sculptor/writer/photographer turned digital artist alias robson fiction@pressroom.com # Barry Carlton Ruff alias ruff bruff@wsicorp.com # Holly Rushmeier, Computing and Applied Math Lab; # National Institute for Standards and Technology; Gaithersburg, Maryland alias rushmeier holly@watson.ibm.com # David Salesin; U. of Washington alias salesin salesin@cs.washington.edu # Stefan Schaefer; University of Bonn alias schaefer schaefer@graphics.cs.uni-bonn.de # Christophe Schlick; LaBRI; U. of Bordeaux; 351 Cours de la Liberation # 33400 Talence; France # interests: ray tracing, radiosity, antialiasing, general reflectance functions alias schlick schlick@labri.u-bordeaux.fr # Karl Johann Schmidt; Mental Images alias kjschmidt kjs@mental.de # Olaf Schmidt; University of Paderborn # PARAGRAPH-Project, parallel simulation of global illumination alias oschmidt merlin@uni-paderborn.de # Frank Schoeffel; Fraunhofer IGD in Darmstadt, Germany alias schoeffel schoeffe@igd.fhg.de # Roland Schregle; ??? alias schregle schregle@uran.informatik.uni-bonn.de # My interest in global illumination pertains to the photon map. I'm currently # implementing it as part of my master's degree in the computer graphics dept. # at Bonn university. # Michael Schroeder; University of Erlangen # Hierarchical Radiosity, Monte-Carlo methods alias mschroeder Michael.Schroeder@informatik.uni-erlangen.de # Peter Schroeder alias pschroeder ps@cs.caltech.edu # Roberto Scopigno; CNUCE; Consiglio Nazionale delle Richerche; # Via S.Maria, 36; 56100 Pisa; Italy # interests: volume rendering, user interfaces, parallel processing, geography alias scopigno R.Scopigno@cnuce.cnr.it # Peter Segal; # development of commercial applications of global illumination alias psegal Peter.Segal@Bentley.Com # Francisco Seron; Dpto. Ingenieria Electrica e Informatica; # Centro Politecnico Superior de Ingenieros; Universidad de Zaragoza; # C/ Maria Luna s/n; E-50015 Zaragoza; Spain alias seron pseron@mcps.unizar.es # Pete Shirley, Indiana U., on leave at Cornell as of 7/94 alias shirley shirley@cs.utah.edu # Francois Sillion; IMAG; Grenoble; France alias sillion Francois.Sillion@imag.fr # Philipp Slusallek; Universitaet Erlangen; # IMMD IX - Graphische Datenverarbeitung; Am Weichselgarten 9; # W-8520 Erlangen, Germany # interests: CAD, surfaces, doing PhD on physical basis of glob. illum. alias slusallek slusallek@informatik.uni-erlangen.de # Brian Smits; University of Utah alias smits bes@cs.utah.edu # Cyril Soler; iMAGIS, Grenoble, France alias csoler Cyril.Soler@imag.fr # Rick Speer alias speer speer@crl.com # Stephen Spencer alias spencer spencer@cgrg.ohio-state.edu # Marc Stamminger; University of Erlangen # Wavelet Radiosity/Radiance, # in future: Clustering, Parallelization of Radiosity/Radiance algorithms alias stamminger Marc.Stamminger@informatik.uni-erlangen.de # Jorge Stolfi alias stolfi stolfi@dcc.unicamp.br # Eric Stollnitz alias stollnitz stoll@amath.washington.edu # Wolfgang Stuerzlinger, Department of Graphics and Parallel Processing, # Johannes Kepler University, Linz, Austria alias stuerzlinger wrzl@gup.uni-linz.ac.at # K. R. Subramanian; AT&T Bell Labs; Murray Hill, NJ alias ksubramanian krs@allegra.att.com # Kelvin Sung; Alias Research Inc. #110 Richmond Street East # Toronto, Canada, M5C 1P1 # interests: fast ray tracing, modular global illumination software alias sung ksung@aw.sgi.com # Frank Suykens; Computer Graphics Research Group, K.U.Leuven alias suykens Frank.Suykens@cs.kuleuven.ac.be # Filippo Tampieri; Lightscape Technologies, Inc; San Jose, CA alias tampieri fxt@discreet.com # Rasmus Tamstorf; Technical University of Denmark # Monte Carlo based rendering, image processing and computer vision. alias tamstorf tamstorf@fa.disney.com # Seth Teller; MIT alias teller seth@lcs.mit.edu # Pierre Tellier # LSIIT (Laboratoire des Sciences de l'Image, d'Informatique et de # Teledetection); Departement d'Informatique de l'Universite Louis Pasteur; # 7, rue R. Descartes; 67084 Strasbourg; France alias tellier tellier@dpt-info.u-strasbg.fr # J Tidmus; University of the West of England in Bristol alias tidmus jpt@btc.uwe.ac.uk # Robert Tobler. T.U. Vienna, Institute of Computer Graphics and Visualisation alias tobler rft@cg.tuwien.ac.at # Jack Tumblin, Georgia Tech alias tumblin ccsupjt@cc.gatech.edu # Sam Uselton; CSC, NASA Ames, Mountain View, CA alias uselton uselton@nas.nasa.gov # Robert van Liere; Department of Interactive Systems; # Center for Mathematics and Computer Science (CWI); # Kruislaan 413, 1098 SJ Amsterdam, The Netherlands # interests: generalizing radiosity method, parallel methods for radiosity alias vanliere robertl@cwi.nl # Cornelius Skip Van Wyk, Jr; ?? alias vanwyk vanwyk@unm.edu # Eric Veach; Stanford U. # interests: hierarchical global illumination, clustering objects, # global illumination methods for "black box" scene representations alias veach ericv@cs.stanford.edu # Francisco Villatoro; Universidad de Malaga (SPAIN) alias villatoro villa@lcc.uma.es # Gianluca Vezzadini; Alias | Wavefront (Paris, France) # My main interests are in lighting design; I am also very interested in any # debate concerning standardization: of terminology, of file format for data #exchange, etc. alias vezzadini gvezzadini@aw.sgi.com # Bretton Wade; alias bwade bwade@sgi.com # Changyaw Wang; Alias Wavefront # interests: rendering and modeling of complex outdoor environments alias cwang wang@aw.sgi.com # Greg Ward Larson; SGI alias ward gwlarson@positron.CS.Berkeley.EDU # Stephen H. Westin; Cornell Program of Computer Graphics alias westin westin@graphics.cornell.edu # Daniel E. Wexler; R&D Staff; Pacific Data Images alias wexler2 wexler@pdi.com # Alexander Wilkie; T.U. Vienna alias wilkie wilkie@cg.tuwien.ac.at # Peter L. Williams; Vassar College; NASA Ames Research Center alias plwilliams williams@cs.vassar.edu # Andrew J. Willmott; CMU alias willmott Andrew.Willmott@cs.cmu.edu # Jim Winget, Silicon Graphics alias winget jmw@sgi.com # Stephen Wittkopf; Dept of Architecture, Technical University Darmstadt,Germany alias wittkopf wittkopf@hp01.cad.architektur.th-darmstadt.de # Adam Worrall, University of Bristol Graphics Group # Computer Science Department, The University, Bristol, UK alias worrall Adam.Worrall@bristol.ac.uk # Chien Kok Yang; UC Berkeley # My research interests are realistic image synthesis and modeling alias yang ckyang@bach.eecs.berkeley.edu # J. Zanizetti; Ecole des Mines de Saint-Etienne, France. alias zanizetti jzaninet@emse.fr # Dave Zareski ; # development of commercial applications of global illuminatio alias zareski David.Zareski@Bentley.Com # Hansong Zhang; University of North Carolina at Chapel Hill. # My interest include radiosity, interactive 3D graphics, simplification.. alias hzhang zhangh@cs.unc.edu # Sunday Safran Zidonis; I am a student at Columbus State Community College # and am pursuing my second degree in Technical Communications. alias zidonis sundayz@ix.netcom.com # Al Zimmerman; # I am interested in acceleration of global illumination alias azimmerman alz@LanMinds.com # Kurt Zimmerman alias zimmerman kuzimmer@cs.indiana.edu # Andrew Zisserman; Robotics Research Group; Oxford University; UK # interests: computer vision, radiosity alias zisserman az@robots.oxford.ac.uk # Zumtobel Licht GmbH; Schweizerstr. 30; A-6850 Dornbirn; Austria # interests: lighting design visualization, radiosity # (an alias for global illumination folks at the Zumtobel company) alias zumtobel glbi@cophos.co.at # alias globillum_explicit \ agrawala alagha mallison almagro amanatides andreas arnu arvo ashdown babu\ bakshi bala baranoski bastos baum bekaert besuievsky bohn boivin cborel\ bouatouch buckalew bustillo camahort campbell canoolivares carrard\ casasayas achalmers chelle chen nchristensen pchristensen chung mcohen\ collins costa cornell_students cunha curless jdave deniel dilaura doi\ donaldson dorsey drettakis dumont fdurand dutre elias fellner ferwerda\ fiume forsyth fournier fussell garcia garmann gatenby geigel gershbein\ gibson gifford glassner goel grabenstein grant greenberg gritz guibas\ haines hanrahan heal heckbert hedley heidrich hollasch holzschuch helenhu\ hubbard ivanov jelle jensen jessel gjones hunt jolivet kaneda karner keller\ kesteloot kilanowski kirk kok kolb kouhia kresse kumar lafortune lalonde\ lang langer leaver legakis levoy blewis plewis lipman lippert lischinski\ loria loscos mccabe mcnamara maierhofer maisel manocha mardaljevic marini\ imartin max meneveaux metge dmitchell moller moubaraki gmueller musgrave\ myszkowski neyret nguyen nimeroff nishita paquette patmore patow pattanaik\ patterson paulin pedersen perez peroche ipeter petitjean pezzola pharr\ pietrek poulin powell prikryl puech pueyo purgathofer rusinkiewicz\ rappoport regincos rekola renambot robson ruff rushmeier salesin schaefer\ schlick kjschmidt oschmidt schoeffel schregle mschroeder pschroeder\ scopigno psegal seron shirley sillion slusallek smits csoler speer spencer\ stamminger stolfi stollnitz stuerzlinger ksubramanian sung suykens tampieri\ tamstorf teller tellier tidmus tobler tumblin uselton vanliere vanwyk veach\ villatoro vezzadini bwade cwang ward westin wexler2 wilkie plwilliams\ willmott winget wittkopf worrall yang zanizetti zareski hzhang zidonis\ azimmerman zimmerman zisserman zumtobel ### Current number of globillum members: 221 ### END OF GLOBAL ILLUMINATION MAILING LIST +------------------+------------------------------------------------------+ | Francois SILLION | iMAGIS - GRAVIR/IMAG, B.P. 53, 38041 Grenoble Cedex 9| | ' | France. Tel:+33 4 76 51 43 54 - Fax:+33 4 76 63 55 80| +------------------+--------+---------------------------------------------+ | Francois.Sillion@imag.fr | http://www-imagis.imag.fr/~Francois.Sillion | +---------------------------+---------------------------------------------+ From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id XAA06123; Thu, 2 Jul 1998 23:17:47 +0200 Received: (from daemon@localhost) by imag.imag.fr (8.8.5/8.8.5) id WAA26633 for globillum-imag-outgoing; Thu, 2 Jul 1998 22:50:48 +0200 (MET DST) Message-ID: <004201bda5fa$e4f7e420$2d2aa8c0@ian-ashdown> From: "Ian Ashdown" To: globillum@imag.fr Subject: New paper of interest Date: Thu, 2 Jul 1998 13:49:22 -0700 MIME-Version: 1.0 Content-Type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 4.72.3110.1 X-MimeOLE: Produced By Microsoft MimeOLE V4.72.3110.3 Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: ff64735ed06f989f8af02fb145081434 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit
This mailing list has been awfully quiet of late ...
 
Some of you may know Kendall Jackson as the author of "The Numerical Solution of Integral Equations of the Second Kind" (Cambridge University Press - http://www.cup.org/Titles/58/0521583918.html) or as editor of the Journal of Integral Equations and Applications (http://www.math.uiowa.edu/~atkinson/jieapage.html).
 
Ken has coauthored several very interesting papers on the radiosity equation lately. His most recent paper (26 pages!), "The Planar Radiosity Equation and its Numerical Solution," is now available as rdsty-planar.ps.Z and rdsty-planar.pdf.Z from http://www.math.uiowa.edu/ftp/atkinson/.
 
I have just begun reading this challenging paper, and so I cannot offer any comments on it. However, it appears to be an important contribution to global illumination research. Given that it will not be published in the usual roundup of computer graphics journals, I thought it best to bring the paper to the attention of this group.
 
Ian Ashdown, P. Eng., LC
Head of Research
Ledalite Architectural Products
 
From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id EAA12382; Wed, 8 Jul 1998 04:29:04 +0200 Received: (from daemon@localhost) by imag.imag.fr (8.8.5/8.8.5) id EAA10798 for globillum-imag-outgoing; Wed, 8 Jul 1998 04:22:38 +0200 (MET DST) Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: globillum@imag.fr Subject: Global Illumination Bibliography update Date: Tue, 7 Jul 1998 19:21:59 -0700 Message-ID: <01bdaa17$2fcff710$6af9aecc@helios> MIME-Version: 1.0 Content-Type: text/plain; charset=windows-1252; format=flowed Content-Transfer-Encoding: 8bit X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 4.71.1712.3 X-MimeOLE: Produced By Microsoft MimeOLE V4.71.1712.3 Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 5ece1f0c4a7ee164d755bdb3bebf5120 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 ANNOUNCE: 98/07/01 Release of RADBIB98.BIB ------------------------------------------ RADBIB98 is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. It currently includes 1,399 references -- 59 new additions since the 98/04/15 release. This bibliography is available in BibTex format as RADBIB98.BIB (with a release date of July 1, 1998) from: http://www.ledalite.com/library-/rrt.htm ftp://ftp.ledalite.com/pub/radbib98.bib Also available from this site is an abridged version of RADBIB98.BIB called GITHESIS.BIB. This bibliography includes 161 references to radiosity and global illumination theses -- 7 new additions since the 98/02/10 release. As always, it is time-consuming and sometimes difficult to track down conference papers and theses on radiosity and global illumination. If you know of a relevant reference that is not included in these bibliographies, please let us know so that we can include it in the next release. Partial financial support for the maintenance of these bibliographies has been provided by the ACM SIGGRAPH Special Projects. Ian Ashdown, P. Eng., LC | READ THE BOOK! Vice President, R & D | Radiosity: A Programmer's Perspective byHeart Consultants Limited | John Wiley & Sons 1994 West Vancouver, BC (Canada) | http://mypage.direct.ca/b/byheart From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id RAA32035; Wed, 8 Jul 1998 17:39:10 +0200 Received: (from daemon@localhost) by imag.imag.fr (8.8.5/8.8.5) id RAA15563 for globillum-imag-outgoing; Wed, 8 Jul 1998 17:30:53 +0200 (MET DST) Message-ID: <35A39084.E4FF654@irisa.fr> Date: Wed, 08 Jul 1998 17:30:14 +0200 From: Kadi Bouatouch Organization: IRISA Campus de Beaulieu Rennes FRANCE X-Mailer: Mozilla 4.03 [fr] (WinNT; I) MIME-Version: 1.0 To: globillum@imag.fr, forum_afig@irisa.fr Subject: A new Journal Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 8bit Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 6ad49aeaae61899bccc1ba0ee0dc854f X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Find attached the announcement of a new journal. Kadi ************************************************************************** Announcement of New Journal and Call for Papers for Volume 1, Number 1, late 1998 ************************************************************************** International Journal of High Performance Computer Graphics, Multimedia and Visualisation http://www.bath.ac.uk/~maxhpcg/ This Journal is a high quality fully refereed Journal that brings together papers under one heading that relate to high performance computing in Computer Graphics, Multimedia and Visualisation. The term high performance will not be restricted to parallelism but instead will include any form of computing that can be regarded as extending the performance capability of the work to a level that merits reporting to the research and practitioner community. The Journal's scope includes, but is not restricted to: * Fundamentals of higher performance computing. * Systems for high performance. * Architectures and technologies for high performance computing. * New algorithms that accelerate performance. * High performance applications. * Performance modelling, analysis and measurement. * Theoretical analysis of high performance algorithms. * Virtual environments, distributed virtual environments. * Real-time dynamic environments. * Computer animation. * Time varying data * Volume and information visualisation. * Video and media processing. * Real-time interaction. * High performance photo-realism in computer graphics. * Algorithmic impact on high performance architectures. * Architectural impact on high performance algorithms. Other topics will be considered by the editors for publication if the work is in keeping with the general aims and objectives of the Journal. Joint Editors-in-Chief Derek Paddon and Claire Willis Editorial Board: Ken-ichi Anjyo - Japan Kadi Bouatouch - France Tom Crockett - USA Don Fussell - USA Pat Hanrahan - USA Chuck Hansen - USA Alan Heirich - USA Horst Holstein - UK Roger Hubbold - UK Paul Mackerras - Australia Ulrich Neumann - USA Bulent Ozguc - Turkey Derek Paddon - UK Sumanta Pattanaik - India/USA Antonio Sousa Pereira - Portugal Jan Prins - USA Thierry Priol - France Werner Purgathofer - Austria Georgios Sakas Germany Sam Uselton - USA Scott Whitman - USA Claire Willis - UK Craig Wittenbrink - USA Format of the Journal The initial circulation would be 4 issues per year of approximately 100 pages per issue. The use of coloured illustrations will be encouraged where it adds to the value of the papers. The length of papers is open, therefore each issue is expected to contain major papers as well as work of a shorter length. Technical notes are encouraged with a special section being devoted to these items. Authors can report major discoveries or innovation as a short technical note in advance of the ideas being fully implemented. These notes will receive very rapid refereeing in order to bring the work to the notice of the community and also to mark the achievement of the authors. As well as publishing previously unseen original work, the journal provides a focus for selected high quality conference papers that are currently appearing in special interest conferences related to high performance issues. These papers will always be re-refereed and as a result can be expected to be extended or reworked in some way. Full details on submission procedures for papers and other information related to the Journal can be found at the following www site: http://www.bath.ac.uk/~maxhpcg/ The Editors-in-Chief can be contacted by email as follows: Derek Paddon hpcg@cs.bris.ac.uk Claire Willis H.P.C.Journal@bath.ac.uk -- ------------------------------------------------------------------ Kadi Bouatouch | Tel: (33) 2-99-84-72-58 | IRISA | Fax: (33) 2-99-84-71-71 | University of Rennes 1 | | Campus de Beaulieu | E-mail: kadi@irisa.fr | F35042 RENNES CEDEX | | FRANCE | | http://www.irisa.fr/siames/SIAMES97 | ------------------------------------------------------------------ From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id RAA31994; Wed, 8 Jul 1998 17:36:09 +0200 Received: (from daemon@localhost) by imag.imag.fr (8.8.5/8.8.5) id RAA15300 for globillum-imag-outgoing; Wed, 8 Jul 1998 17:25:32 +0200 (MET DST) Mime-Version: 1.0 Date: Wed, 8 Jul 1998 11:19:02 -0700 Message-ID: <0061B799.4149@autodesk.com> From: Eric Haines Subject: Ray tracing roundtable & bibliography To: globillum@imag.fr Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit Content-Description: cc:Mail note part Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: b4cd01939d56ccd1c45441be79c9a500 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Ian's note reminded me of two things worth mentioning here. First, the Nth annual Ray Tracing Roundtable will be meeting at SIGGRAPH on Thursday, July 23rd, from 6:15 to 7:45 pm at the Peabody Hotel (across the street from the convention center) in Bayhill Rooms I & II. At this event we quickly introduce ourselves, then break up to talk with each other about what we've been doing in the field. It fits in nicely in the dead time between papers and the reception. Second, I've updated the free ray tracing bibliography at http://www.acm.org/tog/resources/bib/, and added a link to search the bibliography online (as part of the collection of computer science bibliographies, a wonderful free service). Not too many new references, but a few - let me know if I've missed your work. I've also made Tom Wilson's collection of ray tracing article abstracts available at this site. Eric Haines erich@acm.org http://www.acm.org/tog/editors/erich/ From Return-Path: Received: from adeskgate.autodesk.com (adeskgate.autodesk.com [198.93.152.11]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id RAA32094 for ; Wed, 8 Jul 1998 17:44:35 +0200 Received: from autodesk.autodesk.com by adeskgate.autodesk.com (8.8.8/SMI-5.3) with ESMTP id IAA20368; Wed, 8 Jul 1998 08:29:58 -0700 (PDT) Received: from hqhubmu1.autodesk.com by autodesk.autodesk.com (8.8.8/4.4BSD) with ESMTP id IAA24847; Wed, 8 Jul 1998 08:29:53 -0700 (PDT) Received: from ccinternet.autodesk.com (ccinternet [144.111.240.144]) by hqhubmu1.autodesk.com (8.7.5/8.7.3) with SMTP id IAA11320; Wed, 8 Jul 1998 08:29:45 -0700 (PDT) Received: from ccMail by ccinternet.autodesk.com (IMA Internet Exchange 2.12 Enterprise) id 0061B816; Wed, 8 Jul 1998 08:26:51 -0700 Mime-Version: 1.0 Date: Wed, 8 Jul 1998 11:24:18 -0700 Message-ID: <0061B816.4149@autodesk.com> From: Eric Haines Subject: Ray Tracing Roundtable announcement Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit Content-Description: cc:Mail note part X-UIDL: 7d08aacf11c76d3f62975cbdec255871 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 The Nth annual Ray Tracing Roundtable will be meeting at SIGGRAPH on Thursday, July 23rd, from 6:15 to 7:45 pm at the Peabody Hotel (across the street from the convention center) in Bayhill Rooms I & II. At this event we quickly introduce ourselves, then break up to talk with each other about what we've been doing in the field. It fits in nicely in the dead time between papers and the reception. Eric Haines erich@acm.org http://www.acm.org/tog/editors/erich/ p.s. a too-long issue of the RT News will be out real soon now. From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id TAA23405; Tue, 14 Jul 1998 19:04:39 +0200 Received: (from daemon@localhost) by imag.imag.fr (8.8.5/8.8.5) id SAA28742 for globillum-imag-outgoing; Tue, 14 Jul 1998 18:47:20 +0200 (MET DST) Date: Tue, 14 Jul 1998 09:46:02 -0700 (PDT) From: Gregory Ward Larson Message-Id: <199807141646.JAA32211@positron.CS.Berkeley.EDU> To: globillum@imag.fr Subject: color printer advice Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 64883d6e6222b7ddca050565e8ef1955 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Does anyone have any advice to offer on buying a cheap, full-color printer? I've heard there are units available for less than $1000, but I haven't heard any testimonials from unbiased sources. We were looking at a Codonics printer to connect to our Unix network, which I've heard is a good solution, though it costs about $10,000, which is a little bit much for our budget. If you have any experiences to offer, positive or negative, please share, because I'd like to check these printers out while I'm at Siggraph next week. Thanks in advance, -Greg _____________________________________________________________________ Gregory Ward Larson (the computer artist formerly known as Greg Ward) Silicon Graphics, Inc. Computer Science Department 2011 N. Shoreline Blvd., M/S 40U-553 537 Soda Hall, UC Berkeley Mountain View, CA 94043-1389 Berkeley, CA 94720-1776 (650) 933-4878, 932-4878 fax (510) 642-3631, -5775 fax gregl@sgi.com on Tues., Thurs. and Fri. ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id AAA29161; Wed, 15 Jul 1998 00:19:04 +0200 Received: (from daemon@localhost) by imag.imag.fr (8.8.5/8.8.5) id AAA07026 for globillum-imag-outgoing; Wed, 15 Jul 1998 00:11:05 +0200 (MET DST) Date: Tue, 14 Jul 1998 15:10:12 -0700 (PDT) Message-Id: <199807142210.PAA26155@wk312.nas.nasa.gov> From: "Samuel P. Uselton" To: gwlarson@positron.CS.Berkeley.EDU CC: globillum@imag.fr In-reply-to: <199807141646.JAA32211@positron.CS.Berkeley.EDU> (gwlarson@positron.CS.Berkeley.EDU) Subject: Re: color printer advice Reply-to: uselton@nas.nasa.gov Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: c53c7dbacf54b54a7a50bf7f5f96392c X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit The NAS Division bought two Codonics printers to replace our ancient Kodak color printers. Ordinarily I'd say they are better - in particular they seem to stay reasonably close to the settings selected (the Kodak by my office "drifted" fairly quickly). However, I'm on deadline for the Viz conference so of course the "critical need circuits" in all the printers are doing their best to make life hard. I wasn't involved in the purchase so I don't have price or feature details. Sam U. uselton@nas.nasa.gov From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id XAA00809; Thu, 16 Jul 1998 23:56:04 +0200 Received: (from daemon@localhost) by imag.imag.fr (8.8.5/8.8.5) id XAA14386 for globillum-imag-outgoing; Thu, 16 Jul 1998 23:44:07 +0200 (MET DST) From: Peter Shirley Message-Id: <199807162143.PAA19239@lal.cs.utah.edu> Subject: links and atmospheric persp. To: globillum@imag.fr Date: Thu, 16 Jul 1998 15:43:28 -0600 (MDT) X-Mailer: ELM [version 2.4 PL25] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: bebeac1f8149b42e17bb01a4442de5e1 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hi Globillumers. Two things: 1. Anybody know any good computer graphics references which have implemented atmospheric perspective in a physically-based way? 2. I am setting up a page of links on global illumination-- http://www.cs.utah.edu/~shirley/gi/ it is barely started. Additions appreciated. See many of you soon. Pete From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id AAA29510; Tue, 28 Jul 1998 00:16:58 +0200 Received: (from daemon@localhost) by imag.imag.fr (8.8.5/8.8.5) id AAA25826 for globillum-imag-outgoing; Tue, 28 Jul 1998 00:07:03 +0200 (MET DST) Mime-Version: 1.0 Date: Mon, 27 Jul 1998 18:02:07 -0700 Message-ID: <00667C4C.4149@autodesk.com> From: Eric Haines Subject: ray tracing bibliography updated To: globillum Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit Content-Description: cc:Mail note part Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 20419817d67034a07fb0abcfc4e2902d X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 The free ray tracing bibliography at: http://www.acm.org/pubs/tog/resources/bib/ has been updated with recent papers in SIGGRAPH '98 proceedings and course notes. Eric  From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id TAA31219; Fri, 11 Sep 1998 19:42:53 +0200 Received: (from daemon@localhost) by imag.imag.fr (8.8.5/8.8.5) id TAA05782 for globillum-imag-outgoing; Fri, 11 Sep 1998 19:34:53 +0200 (MET DST) Mime-Version: 1.0 Date: Fri, 11 Sep 1998 13:29:15 -0700 Message-ID: <0074A561.4149@autodesk.com> From: Eric Haines Subject: article in new issue of "journal of graphics tools" To: globillum Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit Content-Description: cc:Mail note part Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: ae7816cbac30e484879f4e7e1dcb2284 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Globillumers, "A Low Distortion Map Between Disk and Square", by Peter Shirley and Kenneth Chu, has just been published in the _journal of graphics tools_, v.2 n.3, p.45-52. See http://www.acm.org/jgt/papers/ShirleyChiu97/ for the abstract and code for the technique. It should be noted that this technique is extended in the paper to mapping between a hemisphere and square. It has obvious application within the field of global illumination. Eric From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id MAA18695; Mon, 21 Sep 1998 12:19:18 +0200 Received: (from daemon@localhost) by imag.imag.fr (8.8.5/8.8.5) id MAA17382 for globillum-imag-outgoing; Mon, 21 Sep 1998 12:02:30 +0200 (MET DST) Message-ID: <8815647C7041D111A3010060B06BE1C039C202@elvis.lightwork> From: Neil Gatenby To: globillum@imag.fr Subject: near field stuff Date: Mon, 21 Sep 1998 11:01:07 +0100 MIME-Version: 1.0 X-Mailer: Internet Mail Service (5.0.1460.8) Content-Type: text/plain; charset=windows-1252; format=flowed Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 6127de4bbe22f445c1198e2fc1406514 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Following on from a recent chit-chat that began at the (Wien/Vienna) Eurographics Workshop on Rendering, some of you may find the following site of interest. (relates to "canned light sources"/"near field photometric data") http://www.radimg.com/products_radiantsources.htm Neil From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id QAA18865; Tue, 6 Oct 1998 16:14:43 +0200 Received: (from daemon@localhost) by imag.imag.fr (8.8.5/8.8.5) id PAA03740 for globillum-imag-outgoing; Tue, 6 Oct 1998 15:53:08 +0200 (MET DST) Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: globillum@imag.fr Subject: More global illumination patents Date: Tue, 6 Oct 1998 06:52:21 -0700 Message-ID: <01bdf130$8a83ce60$bf8442d8@helios> MIME-Version: 1.0 Content-Type: text/plain; charset=iso-8859-1; format=flowed Content-Transfer-Encoding: 8bit X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 4.71.1712.3 X-MimeOLE: Produced By Microsoft MimeOLE V4.71.1712.3 Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 412146d92d8b29df9d8e8c354eeae446 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Two more global illumination patents to consider: US Patent 5,734,385, Drawing Method and Apparatus Using Radiosity Algorithm Issue Date: March 31, 1998 US Patent 5,742,292, System and Method for Realistically Displaying Images Indicating the Effects of Lighting on an Object in Three Dimensional Space Issue Date: April 21, 1998 and one which, if I read it correctly, apparently patents the WHILE loop construct: US Patent 5,561,752, Multipass Graphics Rendering Method and Apparatus with Re-Traverse Flag Issue Date: October 1, 1996 Assignee: Apple Computer, Inc. Ian Ashdown, P. Eng., LC | READ THE BOOK! (300 copies remaining) Vice President, R & D | Radiosity: A Programmer's Perspective byHeart Consultants Limited | John Wiley & Sons 1994 West Vancouver, BC (Canada) | http://mypage.direct.ca/b/byheart From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id QAA20613; Tue, 6 Oct 1998 16:48:11 +0200 Received: (from daemon@localhost) by imag.imag.fr (8.8.5/8.8.5) id QAA06883 for globillum-imag-outgoing; Tue, 6 Oct 1998 16:35:07 +0200 (MET DST) From: Peter Shirley Message-Id: <199810061434.IAA02720@phong.cs.utah.edu> Subject: Clearcoat? To: globillum@imag.fr Date: Tue, 6 Oct 1998 08:34:16 -0600 (MDT) X-Mailer: ELM [version 2.4 PL25] Content-Type: text; charset=windows-1252 Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 3900b02dd62f70a5681a581b4a5e2554 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 MIME-Version: 1.0 Content-transfer-encoding: 8bit Anyone have the scoop on what this technology is: http://www.sgi.com/newsroom/press_releases/1998/september/clearcoat.html ?? As far as I can guess it is just environment mapping with variable reflectance. But it is hard to tell if there is more (the above release is all marketing content-free verbiage). I couldn't find a whitepaper at the SGI web site either. Thanks Pete Shirley From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id TAA26618; Tue, 6 Oct 1998 19:34:18 +0200 Received: (from daemon@localhost) by imag.imag.fr (8.8.5/8.8.5) id SAA17367 for globillum-imag-outgoing; Tue, 6 Oct 1998 18:38:51 +0200 (MET DST) Date: Tue, 6 Oct 1998 09:37:57 -0700 (PDT) From: Alain Fournier Message-Id: <199810061637.JAA20592@pedigree.cs.ubc.ca> To: byheart@Direct.CA, globillum@imag.fr Subject: Re: More global illumination patents Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 2bdf65366b47f51146f16def76fa1c7c X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit As Ian says "one which, if I read it correctly, apparently patents the WHILE loop". That is great, if that means the REPEAT UNTIL loop remains available to patent. From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id TAA27201; Tue, 6 Oct 1998 19:54:39 +0200 Received: (from daemon@localhost) by imag.imag.fr (8.8.5/8.8.5) id TAA21136 for globillum-imag-outgoing; Tue, 6 Oct 1998 19:48:18 +0200 (MET DST) Message-ID: From: Don Mitchell To: Ian Ashdown , globillum@imag.fr Subject: RE: More global illumination patents Date: Tue, 6 Oct 1998 10:47:39 -0700 X-Mailer: Internet Mail Service (5.5.2232.9) Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 7c11457e1324499e680daf6df5f68cb9 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Patents have cooties. If you're writing and selling graphics software, talk to your attorney and he will explain what that means and why you should not look at these documents. :-) > -----Original Message----- > From: Ian Ashdown [SMTP:byheart@direct.ca] > Sent: Tuesday, October 06, 1998 6:52 AM > To: globillum@imag.fr > Subject: More global illumination patents > > Two more global illumination patents to consider: > > US Patent 5,734,385, Drawing Method and Apparatus Using Radiosity > Algorithm > Issue Date: March 31, 1998 > > US Patent 5,742,292, System and Method for Realistically Displaying Images > Indicating the Effects of Lighting on an Object in Three Dimensional Space > Issue Date: April 21, 1998 > > and one which, if I read it correctly, apparently patents the WHILE loop > construct: > > US Patent 5,561,752, Multipass Graphics Rendering Method and Apparatus > with > Re-Traverse Flag > Issue Date: October 1, 1996 > Assignee: Apple Computer, Inc. > > Ian Ashdown, P. Eng., LC | READ THE BOOK! (300 copies remaining) > Vice President, R & D | Radiosity: A Programmer's Perspective > byHeart Consultants Limited | John Wiley & Sons 1994 > West Vancouver, BC (Canada) | http://mypage.direct.ca/b/byheart > From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id JAA03623; Wed, 7 Oct 1998 09:00:30 +0200 Received: (from daemon@localhost) by imag.imag.fr (8.8.5/8.8.5) id IAA05536 for globillum-imag-outgoing; Wed, 7 Oct 1998 08:46:50 +0200 (MET DST) From: Francois Sillion Message-Id: <199810070646.IAA09595@safran> Subject: Re: Clearcoat? To: Global Illumination List Date: Wed, 7 Oct 1998 08:46:13 +0200 (MDT) Cc: reiners@igd.fhg.de Reply-To: Francois.Sillion@imag.fr X-Mailer: ELM [version 2.4 PL24] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: d36db2e75a59e3a975c62a20a3efe567 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 I am forwarding this message since it is clearly of interest to all of us. The original message bounced because of the problem I explained earlier, namely that our list server only accepts contributions from the listed e-mail addresses... Again, if the adress listed in globillum is not the one you send e-mail from, please send me the new one. --Francois. owner-globillum@imag.imag.fr wrote: > From owner-globillum@imag.fr Tue Oct 6 20:47:42 1998 > Date: Tue, 6 Oct 1998 20:47:41 +0200 (MET DST) > Message-Id: <199810061847.UAA24587@imag.imag.fr> > To: owner-globillum@imag.imag.fr > From: owner-globillum@imag.imag.fr > Subject: BOUNCE globillum@imag.imag.fr: Non-member submission from [reiners@igd.fhg.de] > > > > Hi folks, > > if you want to see it and you're an SGI developer, try > > https://toolbox.sgi.com/toolbox/src/demos/Onyx2/ > > they have a demo to download for Irix 6.4. It doesn't say a lot about > the technology, it only says that it's a single pass reflection map > technique to handle surfaces whose reflecitivty varies with incident > angle. Andreas Fischer of Daimler Benz sent me a mail saying that the > Fresnel Index and the intensity of the map are included in the > calculation. The demo is general enough so that you can load your own > models and the above webpage has some documentation on the parameters. > Maybe somebody more knowledgeable can take a look at it and guess how > it does what it does. > > My feeling is that it's just a name for calculating envmaps for the > material characteristics you want, but maybe I get some more info > later. > > Hope it helps > > Dirk > > -- > -- > -- Dirk Reiners reiners@igd.fhg.de > -- IGD - A4 http://www.igd.fhg.de/~reiners > -- Rundeturmstrasse 6 > -- D-64283 Darmstadt All standard disclaimers apply. > -- Truth is stranger than fiction because fiction has to make sense. > +------------------+------------------------------------------------------+ | Francois SILLION | iMAGIS - GRAVIR/IMAG, B.P. 53, 38041 Grenoble Cedex 9| | ' | France. Tel:+33 4 76 51 43 54 - Fax:+33 4 76 63 55 80| +------------------+--------+---------------------------------------------+ | Francois.Sillion@imag.fr | http://www-imagis.imag.fr/~Francois.Sillion | +---------------------------+---------------------------------------------+ From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id JAA03702; Wed, 7 Oct 1998 09:01:12 +0200 Received: (from daemon@localhost) by imag.imag.fr (8.8.5/8.8.5) id IAA05735 for globillum-imag-outgoing; Wed, 7 Oct 1998 08:48:33 +0200 (MET DST) From: Francois Sillion Message-Id: <199810070647.IAA09618@safran> Subject: Re: Clearcoat? To: Global Illumination List Date: Wed, 7 Oct 1998 08:47:54 +0200 (MDT) Cc: "Stephen H. Westin" Reply-To: Francois.Sillion@imag.fr X-Mailer: ELM [version 2.4 PL24] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 1383e05b2eb6af4a3e60b9f3ebb46beb X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Same deal... owner-globillum@imag.imag.fr wrote: > From owner-globillum@imag.fr Tue Oct 6 22:38:30 1998 > Date: Tue, 6 Oct 1998 22:38:29 +0200 (MET DST) > Message-Id: <199810062038.WAA04796@imag.imag.fr> > To: owner-globillum@imag.imag.fr > From: owner-globillum@imag.imag.fr > Subject: BOUNCE globillum@imag.imag.fr: Non-member submission from ["Stephen H. Westin" ] > > Subject: Re: Clearcoat? > Reply-To: westin@graphics.cornell.edu > > > > Anyone have the scoop on what this technology is: > > > > http://www.sgi.com/newsroom/press_releases/1998/september/clearcoat.html > > > As far as I can guess it is just environment mapping with variable reflectance. > > But it is hard to tell if there is more (the above release is all > > marketing content-free verbiage). I couldn't find a whitepaper at the > > SGI web site either. > > A couple of speculations: > > - Separating the lighting calculation from the reflection map. > I believe OpenGL actually multiplies the reflection map by > the result of the lighting calculation, which is a bit silly. > > - Cube-based environment maps. Hitherto, the spherical map used > in OpenGL is camera-centric: you could rotate the car, but > not walk around it. A paper some years ago from SGI showed > how to do this not too painfully with existing hardware. > > Anyway, it's quite possible that they are just fixing something that's > broken :). > > Another possibility is that they are doing Fresnel reflectance (or > some approximation) at a low level. But if everything has to be baked > into a precomputed map (e.g. lighting), why not include Fresnel in > that? > > My spies at Ford haven't responded yet... > +------------------+------------------------------------------------------+ | Francois SILLION | iMAGIS - GRAVIR/IMAG, B.P. 53, 38041 Grenoble Cedex 9| | ' | France. Tel:+33 4 76 51 43 54 - Fax:+33 4 76 63 55 80| +------------------+--------+---------------------------------------------+ | Francois.Sillion@imag.fr | http://www-imagis.imag.fr/~Francois.Sillion | +---------------------------+---------------------------------------------+ From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id SAA08420; Thu, 8 Oct 1998 18:07:13 +0200 Received: (from daemon@localhost) by imag.imag.fr (8.8.5/8.8.5) id RAA02810 for globillum-imag-outgoing; Thu, 8 Oct 1998 17:50:25 +0200 (MET DST) Mime-Version: 1.0 Date: Thu, 8 Oct 1998 11:46:20 -0700 Message-ID: <007B71EF.4149@autodesk.com> From: Eric Haines To: globillum Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit Content-Description: cc:Mail note part Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 68c819286e4df0feddfa515b8245599c X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Globillumers, I've just improved and added a number of things to the Ray Tracing News site at: http://www.acm.org/tog/resources/RTNews/html/index.html There's now a fairly powerful searcher, so you can easily poke through the 11 years of back issues. Next, the issue index has been updated and expanded (for example, it now includes pointers to all book reviews which have appeared in the News). I have also added a note to the site page saying that you can send me a note if you want to be notified when a new issue comes out (or just write me direct). The searcher, index, and other information is at the top of the main page. Enjoy, Eric Haines erich@acm.org p.s. The free Xavatoria web site searcher at http://www.xav.com/scripts/search/ is the one I decided to go with - it was surprisingly easy to set up and run. I recommend it (so far). From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id TAA30673; Tue, 13 Oct 1998 19:53:09 +0200 Received: (from daemon@localhost) by imag.imag.fr (8.8.5/8.8.5) id TAA08481 for globillum-imag-outgoing; Tue, 13 Oct 1998 19:43:41 +0200 (MET DST) Message-ID: <36239117.711833EA@cs.yorku.ca> Date: Tue, 13 Oct 1998 13:42:47 -0400 From: Wolfgang Stuerzlinger Organization: Dept. of Computer Science, York University X-Mailer: Mozilla 4.5b2 [en] (Win95; I) X-Accept-Language: en MIME-Version: 1.0 To: globillum@imag.fr Subject: CFP: WSCG99 Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 8bit Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 4c3832aad86ea6cea772d964a835f0f2 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 >>>>> CHANGE <<<<< October 15, 1998 if not registered October 29, 1998 if registered via http://wscg.zcu.cz select WSCG99 and send correctly by FTP in the proper format You have the very last opportunity to present your paper before the year 2000 ----------------------------------------------------------- W S C G'99 The 7-th International Conference in Central Europe on Computer Graphics, Visualization and Digital Interactive Media 99 in cooperation with EUROGRAPHICS and IFIP working group 5.10 on Computer Graphics and Virtual Worlds will be held in February 8 - 12, 1999 in Plzen at the University of West Bohemia close to PRAGUE, the capital of the Czech Republic ----------------------------------------------------------------------- >> If you are willing to help us as a REVIEWER, please, << >> fill in the form at the http://wscg.zcu.cz/reviewer.htm << ----------------------------------------------------------------------- >>Spare WSCG'98 proceedings are still available - ask your librarian << >>to order one - form is available from http://wscg.zcu.cz & WSCG99 << ----------------------------------------------------------------------- Conference Chairs ================= Nadia Magnenat Thalmann, MIRALab-CUI, Univ. of Geneva, Switzerland Vaclav Skala, Univ. of West Bohemia, Czech Republic International Programme Committee ================================= Bergougnoux,P.(F) Chalmers,A.(UK) Chen,J.(USA) Fellner,D.(D) Ferko,A.(SK) Groeller,E.(A) Hubbold,R.(UK) Iones,A.(RU) Jensen,W.H.(D) Klein,R.(D) Mockrzycki,V.(PL) Peroche,B.(F) Pratt,M.(USA) Rossignac,J.(USA) Sbert, M.(ES) Seidel,H.-P.(D) Sillion,F.(F) Slavik,P.(CR) Slusalek,P.(D) Sochor, J.(CR) Strasser,W.(D) Stuerzlinger,W.(CA) Szirmay-Kalos,L.(H) Tokuta,A.(USA) Willis, P.(UK) Wuetrich,C.(D) Yagel, R.(USA) Yukita,S.(J) Zara, J.(CR) Sponsors and supporting organizations ===================================== Digital Equipment, Hewlett Packard, IBM, Silicon Graphics, Intergraph, Bentley Systems, Microsoft Information for authors ======================== Deadline for contributions: October 15, 1998 if not registered October 29, 1998 if registered via http://wscg.zcu.cz select WSCG99 and send correctly by FTP in the proper format original(full affiliation) +3 copies(non-affiliated) +electronic form in CORRECT Postscript to be compressed to gz format format A4 (strictly NOT B4, properly formated), 8 pages including figures, tables etc. Posters: same format, length restricted to 2 pages including pictures, tables etc. If presented by an author will be printed in separate volume. For details, please, see http://wscg.zcu.cz select WSCG'99 Topics included --------------- Fundamental algorithms, rendering and visualization, virtual reality, animation and multimedia, medical imaging, geometric modelling and fractals, graphical interaction, object-oriented graphics, WWW technologies, standards, computer vision, parallel and distributed graphics, computational geometry, computer aided geometric design, CAD/CAM, DTP and GIS systems, educational aspects of related fields, usage of graphics within mathematical software (Maple, Mathematica, MathCAD etc.) in education The program includes international books exhibition and video show, too. --------------------------------------------- W S C G '99 International Exhibition ------------------------------------ Information for exhibitors: Please contact the organiser as soon as possible -------------------------- for detailed information and conditions. The WSCG98 Exhibition will be held in parallel. Top leading European and Czech companies active in computer graphics, visualization and computer vision, CAD/CAM and GIS systems, virtual reality, multimedia systems and others will be presenting their latest products. Special programme will be available, too. ----------------- Accepted papers will be published in the Conference proceedings with ISBN. They are reviewed by INSPEC, Cambridge Scientific Abstracts, InfoStore, IEEE , ISI , AIMS , INIST and others for citations index and other purposes. The best papers will be considered for possible publication in the Journal of Visualisation and Computer Animation, Computers&Graphics, The Visual Computer, Machine Graphics & Vision and others journals. Organizer and conference secretariat ------------------------------------ Vaclav Skala c/o Computer Science Dept., Univ.of West Bohemia Univerzitni 8, Box 314, 306 14 Plzen, Czech Republic e-mail: skala@kiv.zcu.cz Subject: INFO WSCG99 tel.:+420-19-7491-188 fax:+420-19-7491-188 fax:+420-19-7822-578 The latest information is available at: http://wscg.zcu.cz select WSCG'99 Information on all WSCG conferences: http://wscg.zcu.cz In case of any problems: http://147.228.63.9 From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id JAA05580; Wed, 14 Oct 1998 09:38:11 +0200 Received: (from daemon@localhost) by imag.imag.fr (8.8.5/8.8.5) id JAA16206 for globillum-imag-outgoing; Wed, 14 Oct 1998 09:26:49 +0200 (MET DST) Message-ID: <36245214.1211C043@irisa.fr> Date: Wed, 14 Oct 1998 09:26:13 +0200 From: Kadi Bouatouch Organization: IRISA Campus de Beaulieu Rennes FRANCE X-Mailer: Mozilla 4.03 [fr] (WinNT; I) MIME-Version: 1.0 To: globillum@imag.fr, kadi@irisa.fr, arnaldi@irisa.fr, cozot@irisa.fr Subject: Postdoctoral jobs Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 8bit Content-Transfer-Encoding: 8bit Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: f1d6696fe67a71e73c985cf9388bdf17 X-Mozilla-Status: 9001 X-Mozilla-Status2: 00000000 Our group can offer postdoctoral grants (for one or two years) for researchers who are not french citizens. If you are interested, please let me know. If you want to know further information please connect to the page web : http://www.irisa.fr/siames/pub/pavr.html Sincerely kadi -- ------------------------------------------------------------------ Kadi Bouatouch | Tel: (33) 2-99-84-72-58 | IRISA | Fax: (33) 2-99-84-71-71 | University of Rennes 1 | | Campus de Beaulieu | E-mail: kadi@irisa.fr | F35042 RENNES CEDEX | | FRANCE | | http://www.irisa.fr/siames/SIAMES97 | ------------------------------------------------------------------ From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id XAA01559; Sat, 17 Oct 1998 23:56:42 +0200 Received: (from daemon@localhost) by imag.imag.fr (8.8.5/8.8.5) id XAA10717 for globillum-imag-outgoing; Sat, 17 Oct 1998 23:48:58 +0200 (MET DST) Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: globillum@imag.fr Subject: Stochastic global illumination and RADBIB98 Date: Sat, 17 Oct 1998 14:47:32 -0700 Message-ID: <01bdfa17$bea46ac0$0100007f@helios> MIME-Version: 1.0 Content-Type: text/plain; charset=iso-8859-1; format=flowed Content-Transfer-Encoding: 8bit X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 4.71.1712.3 X-MimeOLE: Produced By Microsoft MimeOLE V4.71.1712.3 Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 18d0623389b1555c264979fcc44a7b9a X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 I normally refrain from commenting on the papers that I add to the RADBIB98 global illumination bibliography, but in this case I will make an exception. Dr. Laszlo Szirmay-Kalos of the Department of Control Engineering and Information Technology, Technical University of Budapest (szirmay@fsz.bme.hu) and various co-authors have been prolific in the number of high-quality papers and technical reports they have written on global illumination over the past few years. I have listed these publications in RADBIB98 (see below), but I want to draw your attention to one in particular: "Stochastic Methods in Global Illumination - State of the Art Report" (Technical Report TR-186-2-98-23). This 29-page report (in English) presents "a state-of-the-art report of those global illumination algorithms which involve Monte Carlo or quasi-Monte Carlo algorithms." If you are a grad student involved in this area, this is likely a must-read paper. It offers an excellent overview and 84 references to follow up on. To download this paper or the many others that Dr. Szimay-Kalos and co-authors have written, go to http://www.fsz.bme.hu/~szirmay/puba.html. Speaking of RADBIB98, it and GITHESIS are still very much alive. Unfortunately, the Webmeister of their host Web site (www.ledalite.com) has been inundated with work and has so far been unable to upload the September 30th releases for me. RADBIB98 now has 1,440 entries (34 additions since its July 15th release) and GITHESIS (a subset of RADBIB98 featuring MSc and PhD theses) has 168 entries (7 additions), with more to come. I do not know when Ledalite will be able to upload the latest versions. If it doesn't happen by the end of the month, I may set up a new Web site for global illumination research and host them myself. In the meantime, if you would like copies, please send me an e-mail request at iashdown@cs.ubc.ca. (Yes, I am now a full-time computer science graduate student.) - Ian Ashdown From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id EAA30659; Fri, 6 Nov 1998 04:39:02 +0100 Received: (from daemon@localhost) by imag.imag.fr (8.8.5/8.8.5) id EAA02582 for globillum-imag-outgoing; Fri, 6 Nov 1998 04:30:57 +0100 (MET) Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: 98/11/15 Release of RADBIB98.BIB and GITHESIS.BIB Date: Thu, 5 Nov 1998 19:29:50 -0800 Message-ID: <01be0935$b62f6a70$4f8742d8@helios> MIME-Version: 1.0 Content-Type: text/plain; charset=iso-8859-1; format=flowed Content-Transfer-Encoding: 8bit X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 4.71.1712.3 X-MimeOLE: Produced By Microsoft MimeOLE V4.71.1712.3 Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 0d6ce2e0415f29de9001e643a63e3cf1 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 ANNOUNCE: 98/11/15 Release of RADBIB98.BIB and GITHESIS.BIB ----------------------------------------------------------- RADBIB98 is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. It currently includes 1,466 references -- 60 new additions since the 98/07/15 release. This bibliography is available in BibTex format as RADBIB98.BIB (with a release date of November 15, 1998) from: http://www.ledalite.com/library-/rrt.htm ftp://ftp.ledalite.com/pub/radbib98.bib Also available from this site is an abridged version of RADBIB98.BIB called GITHESIS.BIB. This bibliography includes 171 references to radiosity and global illumination theses -- 10 new additions since the 98/07/15 release. As always, it is time-consuming and sometimes difficult to track down conference papers and theses on radiosity and global illumination. If you know of a relevant reference that is not included in these bibliographies, please let us know so that we can include it in the next release. Partial financial support for the maintenance of these bibliographies has been provided by the ACM SIGGRAPH Special Projects. Ian Ashdown Head of Research Ledalite Architrctural Products Inc. http://www.ledalite.com From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id SAA09503; Wed, 18 Nov 1998 18:54:34 +0100 Received: (from daemon@localhost) by imag.imag.fr (8.8.5/8.8.5) id SAA03688 for globillum-imag-outgoing; Wed, 18 Nov 1998 18:41:17 +0100 (MET) Message-Id: <9811181740.AA03053@merckx.graphics.cornell.edu> Date: Wed, 18 Nov 1998 12:40:39 -0500 From: "Stephen H. Westin" To: globillum@imag.fr Subject: Translation of Kubelka-Munk Paper Reply-To: westin@graphics.cornell.edu Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 264fd2830c796cc806c3209b3f2028f6 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit I have translated the 1931 paper, "Ein Beitrag zur Optik der Farbanstriche", by Paul Kubelka and Franz Munk, into English. This is the fundamental paper on reflectance of pigment-bearing layers. I would appreciate any corrections or improvements to my amateur translation. The translation is available in gzipped PostScript at . -Stephen H. Westin Any information or opinions in this message are mine: they do not represent the position of Cornell University or any of its sponsors. From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id TAA14394; Wed, 13 Jan 1999 19:12:49 +0100 Received: (from daemon@localhost) by imag.imag.fr (8.8.5/8.8.5) id SAA17944 for globillum-imag-outgoing; Wed, 13 Jan 1999 18:52:50 +0100 (MET) From: Adrian James Chung To: globillum@imag.fr Subject: Thesis downloadable Message-Id: Date: Wed, 13 Jan 1999 17:52:13 +0000 Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 1d5ac53766accc7db5bb98ad300230ee X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/html; charset=windows-1252 MIME-Version: 1.0 Content-transfer-encoding: 8bit Dear researcher,

I've finally completed my Ph.D. duties and have placed the resulting thesis
online:

http://www.doc.ic.ac.uk/~ajc/Papers/thesis.ps.bz2  (2.0 MB)

While this body of work does not concentrate purely on Global
Illumination some interesting ideas are proposed, implemented and
studied that may be of interest to researchers in this field:

1. Ray space partitions for ray casting acceleration

2. Detecting total occlusion of ray shafts in non-polygonal environments

3. Constructing smooth shading functions over arbitrary topologies

4. Robust classification of shadow regions -- umbra, penumbra and full
   illumination.

Bye.
Adrian.
 From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id JAA32528; Fri, 15 Jan 1999 09:53:41 +0100 Received: (from daemon@localhost) by imag.imag.fr (8.8.5/8.8.5) id IAA06951 for globillum-imag-outgoing; Fri, 15 Jan 1999 08:58:33 +0100 (MET) Reply-To: byheart@direct.ca From: "Ian Ashdown" To: globillum@imag.fr Subject: RADBIB99 and GITHESIS - new releases Date: Fri, 15 Jan 1999 00:00:58 -0800 Message-ID: <000001be405d$33db5160$2b8742d8@byheart> MIME-Version: 1.0 Content-Type: text/plain; charset=iso-8859-1; format=flowed Content-Transfer-Encoding: 8bit X-Priority: 3 (Normal) X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook 8.5, Build 4.71.2173.0 Importance: Normal X-MimeOLE: Produced By Microsoft MimeOLE V4.72.3110.3 Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 84bedd6faefa144ce74d3773d1668219 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 ANNOUNCE: 99/01/01 Release of RADBIB99.BIB ------------------------------------------ RADBIB99 is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. It currently includes 1,550 references -- 84 new additions since the 98/11/15 release. This bibliography is available in BibTex format as RADBIB99.BIB (with a release date of January 1, 1999) from: http://www.ledalite.com/library-/rrt.htm ftp://ftp.ledalite.com/pub/radbib99.bib Also available from this site is an abridged version of RADBIB99.BIB called GITHESIS.BIB. This bibliography includes 186 references to radiosity and global illumination theses -- 15 new additions since the 98/11/15 release. As always, it is time-consuming and sometimes difficult to track down conference papers and theses on radiosity and global illumination. If you know of a relevant reference that is not included in these bibliographies, please let us know so that we can include it in the next release. Partial financial support for the maintenance of these bibliographies has been provided by the ACM SIGGRAPH Special Projects. Ian Ashdown, P. Eng, LC READ THE BOOK! Vice President Radiosity: A Programmer's Perspective byHeart Consultants Limited John Wiley & Sons 1994 http://persweb.direct.ca/byheart/Ashdown.html From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id PAA14555; Tue, 16 Feb 1999 15:29:23 +0100 Received: (from daemon@localhost) by imag.imag.fr (8.8.5/8.8.5) id PAA10445 for globillum-imag-outgoing; Tue, 16 Feb 1999 15:22:02 +0100 (MET) Message-ID: <003801be59b8$1c58f8c0$7e8442d8@byheart> From: "Ian Ashdown" To: globillum@imag.fr Subject: Fw: fast hemispherical scatterometer - commercial partner wanted Date: Tue, 16 Feb 1999 06:24:48 -0800 MIME-Version: 1.0 Content-Type: text/plain; charset=iso-8859-1; format=flowed Content-Transfer-Encoding: 8bit X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 4.72.3155.0 X-MimeOLE: Produced By Microsoft MimeOLE V4.72.3155.0 Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: c3645bef71f20e69955317dd5c985f70 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Interesting item from sci.optics -- anyone have any details on this (presumably European) patent? (If the device really is patented rather than patent pending, the details should be in the public domain.) - Ian Ashdown -----Original Message----- From: Sipke Wadman Newsgroups: sci.optics Date: February 16, 1999 2:35 AM Subject: fast hemispherical scatterometer - commercial partner wanted >Title: Fast hemispherical scatterometer - commercial partner wanted > >We have a new, patented scatterometer capable of measuring a full >hemispherical scatterogram of a surface for light from +90 to -90 degrees >(reflected and transmitted) incidence in seconds. Probed surface approx. 1 - >10 mm, multiple wavelength. Its purpose is fast quantitative >characterisation of textures, visual appearance etc. for use as a quality >monitoring tool for industrial production processes and as an input for >computer graphics. The scatterometer is under further development and will >be equipped with appropriate software for data processing. > >Building scatterometers is not our core business and we seek co-operation >with a commercial instrumentation manufacturer to design, build and sell a >commercial version under licence, so we (and others) can simply buy it on >the market. > >Potential partners are invited to respond by E-mail (s.wadman@philips.com) >or by fax (+31 40 2737012); technical details will be given under prior >legal non-disclosure agreement. > >Sipke Wadman, >Centre for Manufacturing Technology of Royal Philips Electronics, >Netherlands From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id FAA07212; Sat, 6 Mar 1999 05:44:41 +0100 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id FAA08951 for globillum-imag-outgoing; Sat, 6 Mar 1999 05:37:47 +0100 (MET) X-Authentication-Warning: imag.imag.fr: majordom set sender to owner-globillum@imag.imag.fr using -f Message-ID: <006401be678b$ab66aae0$608642d8@byheart> From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: Updated RADBIB99 and GITHESIS Date: Fri, 5 Mar 1999 20:41:55 -0800 MIME-Version: 1.0 Content-Type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 4.72.3155.0 X-MimeOLE: Produced By Microsoft MimeOLE V4.72.3155.0 Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 67838601e2e1fb5bfc0e4e112934bf23 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit
ANNOUNCE: 99/03/01 Release of RADBIB99.BIB
------------------------------------------
RADBIB99 is a comprehensive bibliography of radiosity and
related global illumination papers, theses, articles, and
books. It currently includes 1,558 references -- 8 new
additions since the 99/01/01 release.
 
This bibliography is available in BibTex format as
RADBIB99.BIB (with a release date of March 1, 1999) from:
 
 
Also available from this site is an abridged version of
RADBIB99.BIB called GITHESIS.BIB. This bibliography
includes 190 references to radiosity and global
illumination theses -- 4 new additions since the 99/01/01
release.
 
Partial financial support for the maintenance of these
bibliographies has been provided by the ACM SIGGRAPH
Special Projects.
- Ian Ashdown
 
From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id SAA20029; Tue, 30 Mar 1999 18:11:04 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id SAA25428 for globillum-imag-outgoing; Tue, 30 Mar 1999 18:00:46 +0200 (MET DST) Message-ID: <97B07886CAF8D111AE400008C7F4E17D8966D7@HQ_EXCHANGE> From: Ian Ashdown To: "'globillum@imag.fr'" Subject: news48_1 (http://www.ping.at/cie/publ/news/news48.html) Date: Tue, 30 Mar 1999 08:00:44 -0800 MIME-Version: 1.0 X-Mailer: Internet Mail Service (5.5.2232.9) Content-Type: text/plain; charset=windows-1252; format=flowed Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 570f979c592e7136211ca521c74d8e61 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit The International Lighting Commission has recently established CIE Division 8, "Image Technology." Technical committees of possible interest to globillum subscribers include: TC 8-02: Colour Difference Evaluation in Images Terms of Reference: To study, develop and standardise methods to derive colour differences for images. TC 8-03: Gamut Mapping Terms of Reference: To study, develop and recommend an optimal solution for cross-device and cross-media image reproduction. This solution will provide a standard procedure to calculate the colour gamut of an image, an imaging system, or its components, and either one algorithm, or a set of algorithms and rules for use in specific applications. TC 8-04: Adaptation Under Mixed Illumination Conditions Terms of Reference: To investigate the state of adaptation of the visual system when comparing soft-copy images on self-luminous displays and hard copy images viewed under various ambient lighting conditions. Details are available at: http://www.ping.at/cie/publ/news/news48.html Ian Ashdown, P. Eng., LC Head of Research Ledalite Architectural Products Inc. http://www.ledalite.com <> Attachment Converted: "D:\Program Files\Eudora\Attach-ab Mrz 99\news48_1.url" From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id SAA20711; Tue, 30 Mar 1999 18:39:32 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id SAA27844 for globillum-imag-outgoing; Tue, 30 Mar 1999 18:36:25 +0200 (MET DST) Message-ID: <8815647C7041D111A3010060B06BE1C06930C8@elvis.lightwork> From: Neil Gatenby To: "'globillum@imag.fr'" Subject: RE: news48_1 (http://www.ping.at/cie/publ/news/news48.html) Date: Tue, 30 Mar 1999 17:35:54 +0100 MIME-Version: 1.0 X-Mailer: Internet Mail Service (5.5.2232.9) Content-Type: text/plain; charset=iso-8859-1; format=flowed Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 47c2a5e4c7c4eee8127b188248dd2506 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit > -----Original Message----- > From: Ian Ashdown [mailto:iashdown@ledalite.com] > Sent: Tuesday, March 30, 1999 5:01 PM > To: 'globillum@imag.fr' > Subject: news48_1 (http://www.ping.at/cie/publ/news/news48.html) > Also of possible interest to globillumers, and found at the same URL, are details of the following CIE publication, which is new to me ... Neil --- Practical Methods for the Measurement of Reflectance and Transmittance CIE 130-1998 ISBN 3 900 734 88 7 The characteristics of materials related to their reflection and transmission properties are defined in accordance with the International Lighting Vocabulary and other relevant CIE publications. The parameters affecting these characteristics and the principles of measurement involved, which are the same whether the measurement is made in terms of spectral or weighted (e.g. luminous) characteristics, are specified. Methods, using an integrating sphere, are recommended for the measurement of - reflectance for directional r , r (e ) and hemispherical rdif incidence of radiation, - diffuse reflectance r d, - transmittance for directional t , t (e ) and hemispherical tdif incidence of radiation, - diffuse transmittance t d. Specific methods are also recommended for the measurement of - regular reflectance r r, - regular transmittance t r, - radiance/luminance factor b (radiance/luminance coefficient q). The absorptance a can either be measured directly or calculated from the measured values of reflectance and transmittance. Both procedures are described. The principal measurement errors are examined and, where possible, methods for their elimination indicated. The publication contains 66 pages, 28 figures and 1 table. From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id VAA26384; Tue, 30 Mar 1999 21:08:10 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id VAA04722 for globillum-imag-outgoing; Tue, 30 Mar 1999 21:03:44 +0200 (MET DST) From: hertjwr@us.ibm.com X-Lotus-FromDomain: IBMUS To: Ian Ashdown cc: "'globillum@imag.fr'" Message-ID: <85256744.0068AA4B.00@D51MTA03.pok.ibm.com> Date: Tue, 30 Mar 1999 14:03:22 -0500 Subject: Re: news48_1 (http://www.ping.at/cie/publ/news/news48.html) Mime-Version: 1.0 Content-type: text/plain; charset=us-ascii; format=flowed Content-Disposition: inline Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 5a697a8030d7f5040e28d11f498de523 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Speaking of cross media image comparisons, do many people do their work on flat panels rather than CRTs? If so, have you found a transformation that you feel is compatible with CRT appearance? Not only are the chromaticities and gamma different, chromaticity of the primaries varies with luminance on the flat panels, and a simple gamma may not be as good a fit for characterizing performance. You can't measure the chromaticities in the standard way because pressing on the screen changes its color. All if this is in addition to the color change with view angle issue. ( I can deal with this generally by putting my head in the right place, but it does make the standard gamma tests useless -- by the time I get far enough back from the screen for to see a smooth shade instead of white and black pixels the patches have all changed color.) I found a report on the characterization of an Apple Flat panel display by Fairchiled and Wyble who recommend a look up table in place of gamma. http://www.cis.rit.edu/research/mcsl/pubs/PDFs/LCD.pdf There is also research report from our flat panel people here at (IBM) (RC21397 "On the Color Calibration of Liquid Crystal Displays" by Cazes et a., abstract only online, order by email to reports@us.ibm.com) that recommend corrections for leakage and the high "black" level to account for the variation of chromaticity of the primaries. I know there are more reports on measuring LCD's, but I am wondering if anyone has come across any other models for correctly converting images so that they display correctly. __________________________ Holly Rushmeier , holly@watson.ibm.com, (914)784-7252 IBM TJ Watson Research Center, 30 Saw Mill River Road, Hawthorne, NY 10532, USA From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id VAA28250; Fri, 16 Apr 1999 21:36:10 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id VAA00091 for globillum-imag-outgoing; Fri, 16 Apr 1999 21:32:03 +0200 (MET DST) Date: Fri, 16 Apr 1999 15:31:52 -0400 (EDT) From: Henrik Wann Jensen To: globillum@imag.fr Subject: Interesting display technology Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII; format=flowed Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: eb9ed18b06e6de8259ce3698f028613d X-Mozilla-Status: 9001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Check out http://www.hitl.washington.edu/research/vrd/project.html It describes a new display technique that illuminates the retina directly. It promises: - Very small and lightweight, glasses mountable - Large field of view, greater than 120 degrees - High resolution, approaching that of human vision - Full color with better color resolution than standard displays - Brightness sufficient for outdoor use - Very low power consumption - True stereo display with depth modulation - Capable of fully inclusive or see through display modes Now if this is true. It seems seems like the perfect device for displaying our global illumination renderings. -- Henrik From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id WAA28691; Fri, 16 Apr 1999 22:10:05 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id WAA01690 for globillum-imag-outgoing; Fri, 16 Apr 1999 22:07:50 +0200 (MET DST) Date: Fri, 16 Apr 1999 16:07:43 -0400 (EDT) Message-Id: <199904162007.QAA20278@bach.Graphics.Cornell.EDU> From: "Stephen H. Westin" To: globillum@imag.fr In-reply-to: (message from Henrik Wann Jensen on Fri, 16 Apr 1999 15:31:52 -0400 (EDT)) Subject: Re: Interesting display technology Reply-to: westin@graphics.cornell.edu References: Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: deb10e23aade704e4dac15ceb9fecebf X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit > Check out > > http://www.hitl.washington.edu/research/vrd/project.html > Now if this is true. It seems seems like the perfect device > for displaying our global illumination renderings. Well, it seemed promising whe I tried it five or so years ago. At that point it was monochrome (red) and only 512x512 or so. But it seemed like a simple optical system that could be developed into a practical product. -Stephen H. Westin Any information or opinions in this message are mine: they do not represent the position of Cornell University or any of its sponsors. From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id WAA28854; Fri, 16 Apr 1999 22:24:31 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id WAA02171 for globillum-imag-outgoing; Fri, 16 Apr 1999 22:21:12 +0200 (MET DST) Date: Fri, 16 Apr 99 13:21 PDT From: Larry Gritz Message-Id: <9904161321.ZM1020573@apu> In-Reply-To: "Stephen H. Westin" "Re: Interesting display technology" (Apr 16, 4:07pm) References: <199904162007.QAA20278@bach.Graphics.Cornell.EDU> Organization: Pixar Reply-To: lg@pixar.com X-Mailer: Z-Mail (3.2.3 08feb96 MediaMail) To: westin@graphics.cornell.edu Subject: Re: Interesting display technology Cc: globillum@imag.fr Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: b69d13f6e3d5e32e9819c25f82a5f52e X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit On Apr 16, 4:07pm, Stephen H. Westin wrote: > Well, it seemed promising whe I tried it five or so years ago. At that ^^^^^^^^^ You let them zap your retina? Are you already on the waiting list for the cerebral cortex implants also? :-) -- lg -- Larry Gritz Pixar Animation Studios lg@pixar.com Richmond, CA From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id WAA29078; Fri, 16 Apr 1999 22:45:46 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id WAA02986 for globillum-imag-outgoing; Fri, 16 Apr 1999 22:39:50 +0200 (MET DST) From: hertjwr@us.ibm.com X-Lotus-FromDomain: IBMUS To: globillum@imag.fr Message-ID: <85256755.007165F8.00@D51MTA03.pok.ibm.com> Date: Fri, 16 Apr 1999 16:38:44 -0400 Subject: rubin papers - references Mime-Version: 1.0 Content-type: text/plain; charset=us-ascii; format=flowed Content-Disposition: inline Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 3dc48f811acb604ea7310c08423f4393 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Here is some other information that came up as result of the recent rendering workshop (besides the retina display thing.). Anyway, some time ago I saw a presentation from a guy at DuPont who did some simulations of carpet fibers -- the pictures he showed was fascinating but I didn't get his name or any citation information. I saw Mary McKnight from NIST at the workshop, and she dug out the references for me. I think this a very interesting application for rendering and specifically for simulating appearance (and it doesn't involve games or the movies -- the major rendering applications that came up in the group discussions in the workshop.) -- Holly Holly, Here are a couple of references to papers by Barry Rubin from DuPont. Mary ----- Prediction and verification of an iridescent synthetic fiber Rubin B, Kobsa H, Shearer SM APPLIED OPTICS 36: (25) 6388-6392 SEP 1 1997 Document type: Article Language: English Cited References: 9 Times Cited: 1 Abstract: An optical model that predicts the reflection of light by a synthetic fiber of arbitrary cross-sectional shape is described. The model uses a Monte Carlo simulation of an exact ray trace of light for incident rays directed at a selected angle to the fiber axis. The model revealed an optical effect in round fibers that led to the prediction of a new mechanism for iridescence (change-of color with angle of illumination or view) in a fabric by means of round, concentric, sheath-core fibers, with core size less than or equal to 40% by volume and with the sheath and core dyed different colors. The prediction has been verified in actual fabrics. (C) 1997 Optical Society of America. Author Keywords: ray trace, Monte Carlo, iridescence, appearance, synthetic fiber, fabric, carpet KeyWords Plus: REFLECTANCE Addresses: Rubin B, DUPONT CO INC, CENT SCI & ENGN, WILMINGTON, DE 19880. Publisher: OPTICAL SOC AMER, WASHINGTON IDS Number: XT925 ISSN: 0003-6935 Tailored fiber cross sections Rubin B ADVANCED MATERIALS 10: (15) 1225-+ OCT 20 1998 Document type: Article Language: English Cited References: 10 Times Cited: 0 Abstract: Research News: The cross-sectional shape and size of individual fibers have a major impact on the appearance of carpets or fabrics. A mathematical model for the interaction of light with fiber cross-sectional geometry has been developed and applied for the development of new products. The Figure represents the cross section of a new nylon carpet. The selection of this shape was based in part on model predictions. KeyWords Plus: REFLECTANCE Addresses: Rubin B, Dupont Co, Cent Res & Dev, Expt Stn, POB 80357, Wilmington, DE 19880 USA. Dupont Co, Cent Res & Dev, Expt Stn, Wilmington, DE 19880 USA. Publisher: WILEY-V C H VERLAG GMBH, BERLIN IDS Number: 133UT ISSN: 0935-9648 ------------------------------------- Name: Mary McKnight E-mail: mary.mcknight@nist.gov phone: 301-975-6714 fax: 301-990-6891 National Inst. of Standards and Technology 100 Bureau Drive Stop 8621 Gaithersburg, MD 20899-8621 Date: 4/16/99 Time: 4:24:51 PM From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id XAA29329; Fri, 16 Apr 1999 23:03:00 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id XAA03714 for globillum-imag-outgoing; Fri, 16 Apr 1999 23:00:27 +0200 (MET DST) Date: Fri, 16 Apr 1999 14:00:06 -0700 (PDT) From: Gregory Ward Larson Message-Id: <199904162100.OAA95767@positron.CS.Berkeley.EDU> To: lg@pixar.com Subject: Re: Interesting display technology Cc: globillum@imag.fr References: <199904162007.QAA20278@bach.Graphics.Cornell.EDU> Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 9c81165e256962a7b3a54df1c84f082a X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit This is very interesting. I would prefer this myself to a brain implant, though I don't want the modulator to lose power before the laser, although the following paper claims it's perfectly safe: Viirre, E., Johnston, R., Pryor, H. and Nagata, S. (1997). Laser Safety Analysis of a Retinal Scanning Display System. Journal of Laser Applications, 9(4), 253-260. (http://www.hitl.washington.edu/publications/r-97-31/) I was wondering how they would manage to track eye movements, and I guess they're still working on the problem, or at least they were still thinking about it in 1995: Tidwell, M., Johnston, R.S., Melville, D. and Furness, T.A. (1995). The Virtual Retinal Display - A Retinal Scanning Imaging System. In Proceedings of Virtual Reality World '95, pp. 325-333. (http://www.hitl.washington.edu/publications/p-95-1/) Quote: 4.6.2 Exit Pupil The exit pupil in the current prototypes is still quite small. The exit pupil for Prototype #2, for example, is approximately 1.5 millimeters. Thus, the eye must be aligned with the exit pupil to view the image. This will not present an issue in a hand held unit but is not optimal for a head mounted unit. Methods of enlarging the exit pupil are therefore being developed. I noticed that many of their proposed applications had to do with "low vision," i.e., people with poor eyesight. This also corresponds to the time when implants start to make some kind of sense, though not to me, personally. -Greg ______________________________________________________________________________ Gregory Ward Larson (the computer artist formerly known as Greg Ward) Silicon Graphics, Inc. Computer Science Department 2011 N. Shoreline Blvd., 40U-553 537 Soda Hall, UC Berkeley Mountain View, CA 94043-1389 Berkeley, CA 94720-1776 (650) 933-4878, 932-4878 fax (510) 642-3631, -5775 fax gregl@sgi.com http://positron.cs.berkeley.edu/gwlarson ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id XAA29368; Fri, 16 Apr 1999 23:05:50 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id XAA03834 for globillum-imag-outgoing; Fri, 16 Apr 1999 23:04:03 +0200 (MET DST) Date: Fri, 16 Apr 1999 17:03:56 -0400 (EDT) From: Jack Tumblin Reply-To: Jack Tumblin To: "Global Illum. Mail List" Subject: Hi Contrasts, implants, ... Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII; format=flowed Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 0bc8f9b39d2290d61244c78964fcfbca X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit This may be drifting off the subject, but scary-sounding implants are getting serious attention to help replace dead photoreceptors in the retinas of macular degeneration patients. Take a look at: [ http://www.ims-chips.de/products.html ] and click on '3.BMBF Project "Subretinal Microphotodiodes" This same group has had good, working high-dynamic range camera (uses logarithmic responding pixels, 120dB range = 1:10^6 contrast range) for several years now that may be useful for verifying global illumination solutions: [ http://www.ims-chips.de/products.html ] and click on 1. Vision Chips & Digital Cameras Regards, -Jack Tumblin (ccsupjt@cc.gatech.edu) Gradual Student, College of Computing Use all letters: "Jackdaws love my big sphinx of quartz!"-`Says You', NPR From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id FAA32687; Sat, 17 Apr 1999 05:28:15 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id FAA16933 for globillum-imag-outgoing; Sat, 17 Apr 1999 05:26:23 +0200 (MET DST) Message-ID: <009101be8881$ffeeee80$1f8742d8@helios> Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: globillum@imag.fr Subject: High dynamic range cameras Date: Fri, 16 Apr 1999 20:25:52 -0700 MIME-Version: 1.0 Content-Type: text/plain; charset=iso-8859-1; format=flowed Content-Transfer-Encoding: 8bit X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 4.72.3110.5 X-MimeOLE: Produced By Microsoft MimeOLE V4.72.3110.3 Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: fb8b691f7ea0f8e44f01c3c3057ffcca X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Jack Tumblin wrote: > >This same group has had good, working high-dynamic range camera (uses >logarithmic responding pixels, 120dB range = 1:10^6 contrast range) for >several years now that may be useful for verifying global illumination >solutions: > >[ http://www.ims-chips.de/products.html ] and click on > 1. Vision Chips & Digital Cameras > I haven't looked at this Web site, but you can purchase high dynamic range cameras in the US at very reasonable prices. I don't have their catalog handy, but I believe that the C-Cam digital cameras from The Imaging Source (see http://www.theimagingsource.com/catalog/index.htm) cost on the order of $500 or so. The good news is that they have a 120 dB dynamic range; the bad news is that they have an 8-bit output. I'll leave it as an exercise to figure out the dynamic range of each step. (Actually, it isn't as bad as this. You can program the camera to digitize within a four-decade window in the dynamic range, or you can use an external 10-bit digitizer.) The C-Cam cameras are very useful for imaging inherently high dynamic range scenes such as bare lamps (at the expense of everything else in the field of view, of course), but they are a looong way from offering serious competition to our biological imaging systems. - Ian Ashdown From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id JAA08632; Mon, 19 Apr 1999 09:37:24 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id JAA26816 for globillum-imag-outgoing; Mon, 19 Apr 1999 09:25:35 +0200 (MET DST) Message-ID: <371ADA6D.21DCBDC4@imag.fr> Date: Mon, 19 Apr 1999 09:25:33 +0200 From: Francois Sillion Organization: iMAGIS - GRAVIR/IMAG INRIA X-Mailer: Mozilla 4.5C-SGI [en] (X11; I; IRIX 6.5 IP32) X-Accept-Language: en MIME-Version: 1.0 To: globillum@imag.fr Subject: More on display technologies References: <199904162007.QAA20278@bach.Graphics.Cornell.EDU> Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 8bit Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: c422401aa7f4c23b3304f8878c7d348a X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Dear Globillum members, Please let me remind you that our anti-spam filters will only allow your contributions from the e-mail address listed on our server. Several messages bounced back in the last few days, so I am including them below. I realise this is not the most convenient system, but that's how it works... please try to remember to post from your designated account/email address. ----------------------------------------------------------------------------- Daniel Kartch wrote: Am I the only person leery of the idea of intentionally shining a laser diode into my eye. I can just imagine some virus infecting the device driver files and before I can yank the thing off I've got "Kilroy was here" permanently burned into my retina. ----------------------------------------------------------------------------- Marc Levoy wrote: I recall trying a similar retinal display system years ago, head-mounted, manufactured by Reflection Technologies. One problem with it was that visual saccades and blinking caused disturbing tearing of the perceived image. -Marc Levoy +------------------+--------------------------------------------------------+ | Francois SILLION | iMAGIS-GRAVIR/IMAG/INRIA, BP 53, 38041 Grenoble Cedex 9| | ' | France. Tel: +33 4 76 51 43 54 - Fax: +33 4 76 63 55 80| +------------------+--------+-----------------------------------------------+ | Francois.Sillion@imag.fr | http://www-imagis.imag.fr/~Francois.Sillion | +---------------------------+-----------------------------------------------+ From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id TAA23905; Mon, 19 Apr 1999 19:02:40 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id SAA15703 for globillum-imag-outgoing; Mon, 19 Apr 1999 18:56:26 +0200 (MET DST) Date: Mon, 19 Apr 1999 09:55:59 -0700 (PDT) From: Alain Fournier Message-Id: <199904191655.JAA17587@pedigree.cs.ubc.ca> To: Francois.Sillion@imag.fr, globillum@imag.fr Subject: Re: More on display technologies Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 1e951ccf6a4312b001bea073da1dd895 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Marc Levoy's point about saccade and blinking is interesting. Even though I've heard before of the HIT lab device (some of the Imager people here I think had a demo of it on the visit to Seattle a couple of years ago) I did not think about this (serious) kind of potential problems (I'd rather wear glasses than contacts, so you can imagine how I feel about shining light under computer control directly on my retina). From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id UAA24954; Mon, 19 Apr 1999 20:22:25 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id UAA20174 for globillum-imag-outgoing; Mon, 19 Apr 1999 20:18:22 +0200 (MET DST) Message-ID: <4FD6422BE942D111908D00805F3158DF13ABC213@RED-MSG-52> From: Steve Hollasch To: globillum@imag.fr Subject: RE: Virtual Retinal Display (was: More on display technologies) Date: Mon, 19 Apr 1999 11:17:40 -0700 X-Mailer: Internet Mail Service (5.5.2524.0) Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: fc8fe9b4cfb379fcc200774be1e0f0a1 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Hello; I chair the SIGGRAPH Seattle chapter, and hosted a talk on the Virtual Retinal Display two years ago at the University of Washington. I thought I'd share some of my experiences with the VRD since it's come up here. First off, a picture of the color VRD prototype (with Dr. Furness viewing) can be found at the hit lab home page: . The corresponding color image is on the CRT in the background. Several viewers have expressed a reticence about having a computer-controlled laser projected directly onto your retina. Let me assure you, the burning sensation is minimal, and the image fades within a week or so. =^) Truthfully, the laser (or diode) is extremely low power. Dr. Furness stated that leaving the beam targeted to a single region on the retina for eight hours straight would still be well (*well*) within industry guidelines for illumination intensity. This is probably the most common concern (and one of the first questions) about this device, probably because we're so used to high-energy lasers. In fact, the energy needed to excite our rods or cones is extremely low. From the rod's or cone's point of view, it really doesn't matter if the photons are coming from a coherent beam or as part of a larger bundle of light rays focused on the retina (say, from a CRT light source focused via the eye's natural lens). Beyond that, what is particularly interesting about this device is that the focal point of the projected image is *inside the eye's lens*. In normal vision, the focal point is inside the eyeball, and the entire lens is used to focus the resulting image. With the VRD, the light rays pivot about the lens-centered focal point, using very little of the lens refractive properties, and effectively bypassing the normal optical system. The result of this is that the image is well-focused regardless of the viewer's optical vision, and corrective eyewear (the image above notwithstanding) is unnecessary. And better than that. Dr. Furness related a time that he was giving a demonstration and a fellow viewed the device with one eye, and then for grins with the other eye. In a very quiet voice he asked what was going on, since he saw a crystal-clear image in the eye in which he was legally blind. Specifically, his eye was injured in an auto accident, and corneal scarring had eventually rendered that eye useless. Nevertheless, there was a tiny unscarred region of the cornea through which the VRD beams could pass, and then bloom out to the full image directly on his retina. What I find particularly compelling about this technology is that it does for displays what Graffiti (and variants) did for user input. Imagine having an effective large high-resolution display included in your Palm Pilot or cell-phone, for example. =^) All in all, I was quite impressed with the prototypes I played with. From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id RAA21305; Fri, 30 Apr 1999 17:08:39 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id RAA08951 for globillum-imag-outgoing; Fri, 30 Apr 1999 17:03:41 +0200 (MET DST) Message-ID: <001301be931b$66c15960$448442d8@byheart> From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: New Release of RADBIB99 Date: Fri, 30 Apr 1999 08:09:10 -0700 MIME-Version: 1.0 Content-Type: text/plain; charset=iso-8859-1; format=flowed Content-Transfer-Encoding: 8bit X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 5.00.2014.211 X-MimeOLE: Produced By Microsoft MimeOLE V5.00.2014.211 Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: bb2d859902e9eb9ac8ee74f212e3354f X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 ANNOUNCE: 99/05/01 Release of RADBIB99.BIB RADBIB99 is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. It currently includes 1,577 references -- 19 new additions since the 99/03/01 release. This bibliography is available in BibTex format as RADBIB99.BIB (with a release date of May 1, 1999) from: http://persweb.direct.ca/byheart/Ashdown.html Also available from this site is an abridged version of RADBIB99.BIB called GITHESIS.BIB. This bibliography includes 191 references to radiosity and global illumination theses -- 1 new addition since the 99/03/01 release. Partial financial support for the maintenance of these bibliographies has been provided by the ACM SIGGRAPH Special Projects. Ian Ashdown, P. Eng., LC Vice President, R & D byHeart Consultants Limited http://persweb.direct.ca/byheart/Ashdown.html From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id PAA29490; Fri, 7 May 1999 15:30:09 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id PAA07539 for globillum-imag-outgoing; Fri, 7 May 1999 15:25:18 +0200 (MET DST) Message-ID: <3732E99E.CE934F6E@imag.fr> Date: Fri, 07 May 1999 15:24:46 +0200 From: Fredo Durand Organization: iMAGIS X-Mailer: Mozilla 4.07C-SGI [en] (X11; I; IRIX 6.5 IP32) MIME-Version: 1.0 To: globillum@imag.fr, image-based-rendering@cs.unc.edu Subject: siggraph papers on the wen Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 8bit Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 153da016d293a5a0cef00351cb05af94 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hi, I've started to gather links to electronic versions of this year's Siggraph papers. They are available at http://www-imagis.imag.fr/~Fredo.Durand/sig99.html If you know the address of some missing items, please e-mail me. These links are part of my collection of computer graphics bookmarks. http://www-imagis.imag.fr/~Fredo.Durand/book.html Fredo Durand iMAGIS-GRAVIR http://www-imagis.imag.fr/~Fredo.Durand From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id IAA24875; Fri, 18 Jun 1999 08:16:23 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id HAA06786 for globillum-imag-outgoing; Fri, 18 Jun 1999 07:50:11 +0200 (MET DST) From: "Bretton Wade" To: "Globillum" Subject: Birds of a feather? Date: Thu, 17 Jun 1999 22:50:33 -0700 Message-ID: <000101beb94e$7b432c20$cc94aace@pacbell.net> MIME-Version: 1.0 Content-Type: text/plain; charset=iso-8859-1; format=flowed Content-Transfer-Encoding: 8bit X-Priority: 3 (Normal) X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook 8.5, Build 4.71.2232.26 X-MimeOLE: Produced By Microsoft MimeOLE V5.00.2014.211 Importance: Normal Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: da8f3dca684699835aa7e215888291a8 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 What are the plans for birds of a feather and other gatherings of the graphics research communities at SIGGRAPH this year? -- Bretton Wade bretton_wade@acm.org Microsoft Research brettonw@microsoft.com From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id PAA02240; Fri, 18 Jun 1999 15:36:33 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id PAA14715 for globillum-imag-outgoing; Fri, 18 Jun 1999 15:30:10 +0200 (MET DST) From: eric.haines@autodesk.com Message-ID: <19879C753611D3119DAB0008C7A4C0C10B74E3@hqmsgsrf04.autodesk.com> To: bretton_wade@acm.org, globillum@imag.fr Subject: RE: Birds of a feather? Date: Fri, 18 Jun 1999 06:29:51 -0700 MIME-Version: 1.0 X-Mailer: Internet Mail Service (5.5.2448.0) Content-Type: text/plain; charset=iso-8859-1; format=flowed Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 852315342ed12c6351e3d1c3e848e8dc X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit >What are the plans for birds of a feather and other gatherings of the >graphics research communities at SIGGRAPH this year? The Ray Tracing Roundtable SIG will happen, as usual, on Thursday evening around 6:30 to 8. The meeting will be at the HQ hotel. I'll put something on this list once I have a precise location & time. Last year's meeting was unexpectedly meaty, I'm happy to report (more than just a schmooze-fest), and with the rising interest in real-time ray tracing I expect this year's to offer some chewy discussions. Eric From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id RAA21743; Thu, 24 Jun 1999 17:02:30 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id QAA21847 for globillum-imag-outgoing; Thu, 24 Jun 1999 16:58:40 +0200 (MET DST) Date: Thu, 24 Jun 1999 10:58:32 -0400 (EDT) Message-Id: <199906241458.KAA14110@bach.Graphics.Cornell.EDU> From: "Stephen H. Westin" To: globillum@imag.fr Subject: Paper on line: image-based BRDF acquisition Reply-to: westin@graphics.cornell.edu Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 29fd996219eac7a469b23a2dedb1b7f6 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit The paper Image-Based BRDF Acquisition Including Human Skin, by Steve Marschner, myself, Eric Lafortune, Ken Torrance, and Don Greenberg, presented this week at the 10th Eurographics Workshop on Rendering, is now available online at . It describes how we measured the BRDF of various surfaces, including living human skin, using only a digital camera, an electronic flash, and a Cyberware scanner. The measurements have been verified against measurements on our gonioreflectometer; in the best case, they appear to be accurate to within the limits of the gonioreflectometer. Stephen H. Westin Research Project Leader Program of Computer Graphics Cornell University westin@graphics.cornell.edu 607 255 9080 (VOX) 607 255 0806 (FAX) From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id VAA28337; Thu, 24 Jun 1999 21:43:49 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id VAA08991 for globillum-imag-outgoing; Thu, 24 Jun 1999 21:41:23 +0200 (MET DST) Date: Thu, 24 Jun 1999 15:41:14 -0400 (EDT) Message-Id: <199906241941.PAA15683@bach.Graphics.Cornell.EDU> From: "Stephen H. Westin" To: globillum@imag.fr Subject: Slides from April Ithaca workshop on line Reply-to: westin@graphics.cornell.edu Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 13e9e7e6413abe7f735fbec7422950c8 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Through the good graces of our speakers, we are able to make the slides (and some animations and VRML files) from the recent Workshop on Rendering, Perception, and Measurement available on the Web. point your browser to A few photos from the workshop are available here; more are on line at Greg Larson's Web site: Stephen H. Westin Research Project Leader Program of Computer Graphics Cornell University westin@graphics.cornell.edu 607 255 9080 (VOX) 607 255 0806 (FAX) From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id UAA28938; Mon, 19 Jul 1999 20:14:30 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id UAA05872 for globillum-imag-outgoing; Mon, 19 Jul 1999 20:09:06 +0200 (MET DST) Message-Id: <199907191809.OAA12648@bach.Graphics.Cornell.EDU> From: "Stephen H. Westin" Date: Mon, 19 Jul 1999 13:54:11 -0400 (EDT) To: globillum@imag.fr Subject: Paper online has moved: technical reports added Reply-to: westin@graphics.cornell.edu Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: e47e5598737bf11ebbc8a862369870b9 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit For those who may be interested in the following paper Stephen R. Marschner, Stephen H. Westin, Eric P. F. Lafortune, Kenneth E. Torrance, and Donald P. Greenberg. Image-based brdf measurement including human skin. In Eurographics Workshop on Rendering, 1999. we now have a permanent URL: Also online are two more detailed technical reports on the research: see . Stephen H. Westin Research Project Leader Program of Computer Graphics Cornell University westin@graphics.cornell.edu 607 255 9080 (VOX) 607 255 0806 (FAX) From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id TAA06690; Mon, 26 Jul 1999 19:09:51 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id TAA17526 for globillum-imag-outgoing; Mon, 26 Jul 1999 19:02:52 +0200 (MET DST) From: eric.haines@autodesk.com Message-ID: <19879C753611D3119DAB0008C7A4C0C10122717D@hqmsgsrf04.autodesk.com> To: globillum@imag.fr Subject: Ray Tracing Roundtable Date: Mon, 26 Jul 1999 10:02:37 -0700 MIME-Version: 1.0 X-Mailer: Internet Mail Service (5.5.2448.0) Content-Type: text/plain; charset=iso-8859-1; format=flowed Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 245ad9041f19d1782bfb3c84e0ec7978 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit At SIGGRAPH the Ray Tracing Roundtable SIG will meet: Thursday, August 12th 6:30-7:45 pm Garden East, Wilshire Grand Hotel (HQ hotel) This SIG is a way for ray tracing researchers and developers to informally gather and discuss topics of interest. Personally, I'm looking forward to it. With real-time ray tracing becoming more possible as specialized and general hardware develops, last year's roundtable was the most interesting one in years, as people presented different viewpoints and schemes. One question I'm interested in is what is the future(s) of real-time rendering and hardware for it. With developments like the Playstation 2 we're seeing 20 million polys/sec sustained in a consumer-level box. Admittedly, this gets chopped down as multiple passes are used for more elaborate illumination models, environment maps, reflection passes, etc. Diefenbach http://www.openworlds.com/employees/paul/index.html has done interesting work on using polygon hardware for global illumination, and Heidrich and others http://www.cgl.uwaterloo.ca/Projects/rendering/Papers/index.html#sepbrdfT have worked with multipass rendering and environment mapping to perform BRDF approximations. That said, the crossover point where there are more polygons per frame than pixels is within sight. As this point is passed, what happens? Current real-time polygon engines assume an average polygon covers, say, 50 pixels, so triangle setup time (figuring out edge locations and differentials) could be amortized over this filled area. If you're filling a single pixel or less, are something like REYES micropolygons more appropriate? Or subdivision surfaces in hardware, as well as other LOD techniques? Or voxels and splats? Or a hybrid of polygons for close-ups and image based impostors for distant objects? Or does ray tracing become a method whose flexibility and simplicity makes up for its overall processing cost? Given ray tracing's ability to avoid having to access every single polygon in the scene (if something is not visible, it can avoid being queried at all by a ray tracer), if and when does this ability outperform various view and occlusion culling schemes used for polygon renderers? Or can well-placed impostors and LOD models almost always win out? Seeing things like the incredible rates Utah had for its 60 CPU machine (around 525 million spheres a second), there are certainly scenes where pure ray tracing can win today, and where these other techniques cannot be easily applied. Each technique mentioned above has its areas of strength, scenes and animation paths where it excels. What interests me is the long-term trends in the field and what functionality moves to hardware. Textured, filtered (via mipmapping or even anisotropic filters) and alpha-blended polygons are now a basic primitive in consumer hardware, making traditional polygon rendering as well as some image-based and voxel rendering techniques possible. What's next? Will anything win hands down in the very long term? Even if hybrid schemes are supported, what are the basic building blocks? What the fast "atomic" operations are strongly influences what algorithms will be used, of course; when the set of basic operations changes, the field shifts. Opinions or datapoints, anyone? Anywell, I hope to see you at the Roundtable, Eric From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id TAA12069; Tue, 27 Jul 1999 19:08:06 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id TAA28244 for globillum-imag-outgoing; Tue, 27 Jul 1999 19:04:15 +0200 (MET DST) From: eric.haines@autodesk.com Message-ID: <19879C753611D3119DAB0008C7A4C0C10122790C@hqmsgsrf04.autodesk.com> To: globillum@imag.fr Subject: Future of real-time rendering Date: Tue, 27 Jul 1999 10:03:55 -0700 MIME-Version: 1.0 X-Mailer: Internet Mail Service (5.5.2448.0) Content-Type: text/plain; charset=iso-8859-1; format=flowed Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 2e7888e3fcad7dd1694649192f71c88a X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit [Ken did not have the globillum email address handy, so asked me to post his reply. - EAH] -----Original Message----- From: Ken Musgrave [mailto:musgrave@metacreations.com] Sent: Tuesday, July 27, 1999 10:19 AM To: eric.haines@autodesk.com Subject: Re: Ray Tracing Roundtable >Opinions or datapoints, anyone? It is my considered view that eventually the machines will become fast enough that we, the human programmers, will not have to devise Rube Goldberg schemes--like scanline rendering--to accomodate their limited capabilities. The machines will eventually accomodate more anthropocentric models. Then, the elegance of the model will come to the fore as its primary measure of merit. (The long-awaited entrance of Occam's Razor to computer science.) At that time, ray tracing will rule. Other methods will become historical footnotes; monstrosities akin to bleeding the sick to heal them. Until we can accomodate rendering models including the wave nature of light. Fortunately, that will take a while longer. >;^) -Mo Soapbox AKA Ray Tracing Prejudiced -------------------------------------------------------------------------- Ken Musgrave MetaCreations http://www.metacreations.com/people/musgrave (805) 689-9222 (c) (805) 684-6774 (h) (805) 566-6331 (w) Arbitrary mayhem at the interstices. -------------------------------------------------------------------------- From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id VAA16069; Tue, 27 Jul 1999 21:32:35 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id VAA04831 for globillum-imag-outgoing; Tue, 27 Jul 1999 21:30:27 +0200 (MET DST) Message-ID: <379E08CC.67CB3F71@llnl.gov> Date: Tue, 27 Jul 1999 12:30:20 -0700 From: "Nelson L. Max" X-Mailer: Mozilla 4.51C-SGI [en] (X11; I; IRIX64 6.5 IP30) X-Accept-Language: en MIME-Version: 1.0 To: globillum@imag.fr Subject: EGWR99 Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 8bit Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 4164b82af8ef620966f65316dd1395b7 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Holly Rushmeier wanted to know what went on at EGWR99. Here is my trip report, biased toward what I needed to tell LLNL and the DOE. The purpose of the trip was to attend the 10th Eurographics Workshop on Rendering, which took place on June 21 to 23, at the Congress Hall in Granada, Spain. This annual workshop has become the main forum for new research results in rendering (second only to the Siggraph conference, which has space for only a few papers on this topic). Although it is traditionally held in Europe, participants come from all over the world. As in past years, many of the papers concerned local and global illumination. For local illumination, these included papers on mathematically modelling, measuring, representing and approximating local reflection functions (for example, of paint, human skin, wet materials, and surfaces covered by thin films). For global illumination these included stochastic methods, computing soft shadows and approximating their discontinuities, face clustering, interreflection in thick surface geometries, accelerated matrix solution techniques, and efficiently updating global illumination for scenes with moving objects. A new area that is rapidly becoming important is image-based rendering, and papers on this subject included model acquisition and display, visibility ordering for reprojected triangles, use of images in measuring local reflection functions, and uses of hardware in image based rendering. My presented paper in this field "Hierarchical Image-Based Rendering using Texture Mapping Hardware" combined my hierarchical modelling, presented in this workshop in 1996, the hardware-based reprojection techniques I learned from Gernot Schaufler's talk at last year's workshop, and the hardware shading techniques I learned from Rudiger Westermann when I visited him at Erlangen last year. (This proves the utility of my DOE supported trip to Europe last summer.) The paper that I was co-author on was "Shadow Penumbras for Complex Objects by Depth Dependent Filtering of Multi-Layer Images", presented by my Ph.D. student Brett Keating, and the shadow algorithm described is also applicable to image-based models. There were also talks on optimized lighting design, filtering motion sequences using human spatio-temporal perception effects (and in related different paper, producing motion sequences by reprojecting cached surface points from previous frames), adding snow and trees to terrain images, and compressing precomputed intersurface visibility data. The vacation days in Spain were spent looking at churches and palaces, including the Alhambra, and the vacation days in Russia were spent touring with Slavyanka, a male slavic chorus, giving three formal concerts, and singing informally in churches, monasteries, and at the Hermitage museum in St. Petersburg. -- email: max2@llnl.gov Nelson Max, Mail Stop L-560 http://www.llnl.gov/graphics Lawrence Livermore National Laboratory phone (925) 422-4074 7000 East Avenue fax (925) 422-6287 Livermore, CA 94550, USA From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id WAA17587; Tue, 27 Jul 1999 22:45:35 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id WAA08115 for globillum-imag-outgoing; Tue, 27 Jul 1999 22:43:26 +0200 (MET DST) From: eric.haines@autodesk.com Message-ID: <19879C753611D3119DAB0008C7A4C0C101227B3A@hqmsgsrf04.autodesk.com> To: globillum@imag.fr Subject: FW: Ray Tracing Roundtable Date: Tue, 27 Jul 1999 13:43:18 -0700 MIME-Version: 1.0 X-Mailer: Internet Mail Service (5.5.2448.0) Content-Type: text/plain; charset=iso-8859-1; format=flowed Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 4ffca291e1036aba5395b470afde06a1 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit [another person who wanted to have his note forwarded to globillum. Since I'm forwarding it, I've responded at the end. -EAH] -----Original Message----- From: Fabrice Neyret [mailto:Fabrice.Neyret@imag.fr] Sent: Tuesday, July 27, 1999 3:27 PM To: eric.haines@autodesk.com Cc: Fabrice.Neyret@imag.fr Subject: Re: Ray Tracing Roundtable There is a big issue about image quality (and not only data quantity). For instance, there is a big deal concerning aliasing. I don't believe ray-tracing can win soon, because of its very bad properties on this topic. Just have a look on the non-realtime side: does video-production companies massively use raytracing ? the answer is no, and it is very far from being ( indeed, it is a minority ). Instead, high quality renderers used in video production are using algorithms that are members of the projective rendering familly, with much extensions that allows nice quality (antialiasing, reflects, shaders, procedural textures, etc). Typically, this is the A-buffer algorithm and various variations about it (possibly mixed with other algorithms, at pixels needing special features). Thus, I feel reasonable to guess than the same path can be followed for hardware graphic accelerators: More than one color+z per pixel, per-pixel computations, coverage masks are features already or soon available on SGIs. Basic limitations such as the number of textures tend to vanish on Playstation2. Less limitations and per-pixel shaders may help decreasing the number of passes. >>From this, one may reach soon an A-buffer configuration, per-pixel shaders and so on. A-buffer allows easy anti-aliasing computation, clear separation of geometry and shading (allowing material editing ala IPR), and the obstacle about turning it into hardware 10 years ago was mainly memory... I guess all these are properties that makes the method electable ! Fabrice NEYRET -------------------------------------------- equipe iMAGIS ( GRAVIR (CNRS,INPG,UJF) & INRIA ) http://www-imagis.imag.fr/Membres/Fabrice.Neyret/index.html fax: +33 (0)4 76 63 55 80 secretariat: +33 (0)4 76 51 46 90 -------------------------------------------- Eric here: I'd like to respond by agreeing a fair bit. Beyond Blue Sky Studios (who did win an Academy Award last year for "Bunny", http://www.blueskystudios.com/), most production software uses A-buffers or use RenderMan, i.e. micropolygons, with ray tracing an occasional "nothing else will do (or at least not easily)" effect. A-buffering gives a lot of samples per pixel cheaply, and so often looks better than adaptive subdivision ray tracing (it catches the spokes of a wheel more consistently, for example). Is this approach the future, or does the simplicity of ray tracing have the same effect as the simplicity of the Z-buffer vs. the 10 hidden-surface algorithms compared by Sutherland et al. 25 years ago? The Z-buffer won out as of today because it had fixed memory costs, memory got cheaper, and "dumbest wins" when programming hardware chips since it saves on dedicated transistors. That said, Winner et al. in SIGGRAPH '97 talk about how A-buffers can reuse much of the Z-buffer pipeline, so are low cost to add to existing designs. Or is the future dictated more by memory size than processor speed, i.e. A Bug's Life scenes have a gigabyte of geometry (not including textures), and a RenderMan architecture allows dealing with it a small chunk at a time vs. the whole caboodle at once as needed in global solutions [but then there's Matt Pharr's ray tracing approach...]. BTW, to wow your friends and confound your enemies, try out some of the real-time ray tracing demos at http://www.acm.org/tog/resources/RTNews/demos/overview.htm That a 4K program like chrome.zip can do anything at all I consider miraculous. From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id AAA19152; Wed, 28 Jul 1999 00:20:02 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id AAA12481 for globillum-imag-outgoing; Wed, 28 Jul 1999 00:18:05 +0200 (MET DST) Message-ID: From: Francois Sillion To: "'globillum@imag.fr'" Subject: Ray tracing roundtable. BOUNCE globillum@imag.imag.fr: Non-me mber submission from [Dan Wexler ] Date: Tue, 27 Jul 1999 15:15:13 -0700 X-Mailer: Internet Mail Service (5.5.2524.0) Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 5ca03696d5f5a89d9f361420240409aa X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Here's another contribution (from Dan Wexler) to the thread. Let me remind everyone that our anti-spam filter will only accept contributions from the actuale-mail address registered in the list. If you want to change your e-mail address, drop me a note! +-----------------+--------------------------------------------------------+ |Francois SILLION | iMAGIS-GRAVIR/IMAG/INRIA, BP 53, 38041 Grenoble Cedex 9| |Senior Researcher| France. Tel: +33 4 76 51 43 54 - Fax: +33 4 76 63 55 80| +-----------------+--------------------------------------------------------| |Microsoft Research 31/1145, 1 Microsoft Way Redmond WA 9898052-6399 USA | |Tel: (425) 703 8412, Fax: (425) 936 7329. < mailto:sillion@microsoft.com> | +--------------------------+-----------------------------------------------+ |Francois.Sillion@imag.fr | http://www-imagis.imag.fr/~Francois.Sillion | +--------------------------+-----------------------------------------------+ > -----Original Message----- > Date: Tue, 27 Jul 1999 14:57:13 -0700 > From: Dan Wexler > To: globillum@imag.fr > Subject: Re: FW: Ray Tracing Roundtable > > > Instead, high quality renderers used in video production are using > > algorithms that are members of the projective rendering familly, > > with much extensions that allows nice quality > (antialiasing, reflects, > > shaders, procedural textures, etc). > > Typically, this is the A-buffer algorithm and various > variations about it > > (possibly mixed with other algorithms, at pixels needing > special features). > > Really? Here at PDI we use a variant of the A-buffer algorithm, > but I don't believe this is the norm. I don't think I'd qualify > PRMan as an abuffer algorithm, nor is Mental Ray, nor the > renderer used at Rhythm and Hues (from what I've gathered at least) > nor the scanline renderers found in many of the commercial packages. > > I don't think we're going to stick with the abuffer method either > for too much longer. The abuffer algorithm does not have very > good antialiasing qualities. The abuffer representation of a > subpixel fragment just isn't accurate enough for really high quality > antialiasing. It tries to represent a area (as opposed to a point > sample) and does so rather poorly, IMHO. > > Another major issue is handling motion blur and depth of field. > These don't work too well in a traditional abuffer renderer. > > Then Eric added: > > > A-buffering gives a lot of samples per pixel > > cheaply, and so often looks better than adaptive > subdivision ray tracing (it > > catches the spokes of a wheel more consistently, for example). > > Multiple samples per pixel? Really? I spent a bunch of time > modifying our abuffer to actually shade multiple samples for > a single abuffer fragment, and I could never really get it to > work correctly. Consider the problem of representing the range > of surface normals over a given abuffer fragment. It is not > an easy task to modify your scan converter to generate these data. > I suppose you could just shade each of the subpixels in the > abuffer mask using the interpolated scanline values, but I don't > think that is the norm, and it assumes that you generate an abuffer > mask using a sort of zbuffer scan conversion. Also, in that case > it would still probably be using a regular sampling pattern. > > Sure, you get coverage information that represents portions of > the pixel, but it tends to be regularly sampled. Again, modifying > the abuffer algorithm to handle some form of stochastic sampling > is non-trivial. > > Regarding memory usage, the average shot on Antz had upwards of > 1-2 GB of data in the form of geometry, textures, and scene > description -- and much of the geometry was generated procedurally. > We had an *average* of 12 polygons per pixel and we sampled > well over 100 points in shadow maps for each shaded sample. > We also must render all our frames in under 8 hours. > > > > Wex > From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id BAA19992; Wed, 28 Jul 1999 01:46:15 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id BAA15713 for globillum-imag-outgoing; Wed, 28 Jul 1999 01:41:51 +0200 (MET DST) Date: Tue, 27 Jul 99 16:41 PDT From: Larry Gritz Message-Id: <990727164145.ZM27730@apu> In-Reply-To: Francois Sillion "Ray tracing roundtable. BOUNCE globillum@imag.imag.fr: Non-me mber submission from [Dan Wexler ]" (Jul 27, 3:15pm) References: Organization: Pixar Reply-To: lg@pixar.com X-Mailer: Z-Mail (5.0.0 30July97) To: "'globillum@imag.fr'" Subject: Re: Ray tracing roundtable. BOUNCE globillum@imag.imag.fr: Non-me mber submission from [Dan Wexler ] MIME-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 60a54acdb1b253ca3f723faf2a4ed26d X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit > > -----Original Message----- > > Date: Tue, 27 Jul 1999 14:57:13 -0700 > > From: Dan Wexler > > To: globillum@imag.fr > > Subject: Re: FW: Ray Tracing Roundtable > > > > Really? Here at PDI we use a variant of the A-buffer algorithm, > > but I don't believe this is the norm. I don't think I'd qualify > > PRMan as an abuffer algorithm, nor is Mental Ray, nor the > > renderer used at Rhythm and Hues (from what I've gathered at least) > > nor the scanline renderers found in many of the commercial packages. PRMan is REYES, not A-Buffer. -- lg -- Larry Gritz Pixar Animation Studios lg@pixar.com Richmond, CA From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id CAA20129; Wed, 28 Jul 1999 02:00:14 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id BAA16290 for globillum-imag-outgoing; Wed, 28 Jul 1999 01:58:54 +0200 (MET DST) Date: Tue, 27 Jul 1999 19:58:49 -0400 From: Hansong Zhang To: globillum@imag.fr Subject: [Fwd: Ray tracing in everyone's future?] Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII; format=flowed Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: f3e24840f50c8b1fac98f72f65e92769 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit A comment from Michael Jones... -------- Original Message -------- Subject: Ray tracing in everyone's future? Date: Tue, 27 Jul 1999 15:28:40 -0700 From: "Michael T. Jones" To: hansong@intrinsic.com Hansong, I have a comment on Eric's comment. Pass it along to him if you wish... When Eric writes "...The Z-buffer won out as of today because it had fixed memory costs, memory got cheaper, and "dumbest wins" when programming hardware chips since it saves on dedicated transistors." I would restate this--essentially challenging it. What wins is the nice combination of "true" parallelism without cross-communication, or at least with tremendously reduced cross-communication bandwidth compared to action at the parallel stage. Machines like the SGI G, GT, VGX, RE, and IR have this characteristic: LOW: one polygon in, HIGH fanned-out to hundreds of non-cross-connected mini-framebuffer / rasterization engines (multiple of these on a chip), and then LOW fan-in to a single coherent raster-order byte stream for video display. Such structures are well suited to the current interconnect technology. Packaging technology reinforces this too, since the number of gates grows much faster than the number of pins, and the frequency of those gates grows much faster than the frequency of those pins. As a result, the "next gen killer architecture" for the next while will be designed as the answer to "how can I best exploit locality?" With interesting answers like "in this core, in this cache, in this chip, on this board, etc." This is where the "it will all be ray-tracing" line of thinking hits the brick wall of VLSI truth. If you can think of a structured way to ray cast, then may be it's ok. If not, then no. It's easier to render something coherent five times than to jump around once and I expect it to stay that way until busses become somewhat like crossbars (i.e., multifrequency fiber with an open channel per link-pair). Michael Jones ---------- Michael T. Jones - mtj@intrinsic.com From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id RAA32012; Wed, 28 Jul 1999 17:13:14 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id OAA23175 for globillum-imag-outgoing; Wed, 28 Jul 1999 14:53:19 +0200 (MET DST) From: hertjwr@us.ibm.com X-Lotus-FromDomain: IBMUS To: globillum@imag.fr Message-ID: <852567BC.0046C23B.00@D51MTA03.pok.ibm.com> Date: Wed, 28 Jul 1999 08:53:03 -0400 Subject: Re: [Fwd: Ray tracing in everyone's future?] Mime-Version: 1.0 Content-type: text/plain; charset=us-ascii; format=flowed Content-Disposition: inline Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 463719209f217126756275424b67b48e X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit I realize that I always make the same points, but I can't help bringing this up again. As far as ray tracing for real time rendering, doesn't it matter what the goal of the rendering is? Exploiting geometric coherence as Michael describes wins if you can settle for a non-global lighting solution (which is the right thing to do for a lot of applications) , or if you can cope with a temporally fixed lighting solution that carries around a lot of directional information. If you want to have on-the-fly accurate lighting, ray tracing wins I think over other schemes to make use of zbuffers for secondary lighting etc. The rendering used for motion picture production is a really different problem from a person interacting with building design on their computer. As difficult as the motion picture problem is, they can define the lighting rules they want, and they don't have to cope with changes on the fly. On the other hand, they can't allow random artifacts to crop up -- the method they used has to be robust. On the other hand if I were to be designing something, I want to be able to move things around whenever I want to, and if there is an occasion glitch or aliasing it isn't going to bother me that much. __________________________ Holly Rushmeier , holly@watson.ibm.com, (914)784-7252 IBM TJ Watson Research Center, 30 Saw Mill River Road, Hawthorne, NY 10532, USA From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id QAA13183; Fri, 30 Jul 1999 16:26:14 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id QAA25770 for globillum-imag-outgoing; Fri, 30 Jul 1999 16:23:34 +0200 (MET DST) Message-Id: <199907301423.QAA25763@imag.imag.fr> Subject: Re: Ray tracing roundtable. To: globillum@imag.fr Date: Fri, 30 Jul 1999 10:23:08 -0400 (EDT) From: Andrew Willmott Reply-To: ajw+@cs.cmu.edu X-Mailer: ELM [version 2.4 PL25-40] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 3ab87e4319963b32a7ebfe47551caa1a X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Dan Wexler wrote: > > Really? Here at PDI we use a variant of the A-buffer algorithm, > > but I don't believe this is the norm. I don't think I'd qualify > > PRMan as an abuffer algorithm, nor is Mental Ray, nor the > > renderer used at Rhythm and Hues (from what I've gathered at least) > > nor the scanline renderers found in many of the commercial packages. I had some experience with hacking on the R&H renderer some years ago. It was a reasonably standard scanline renderer. If I recall correctly, in the default mode 3x3 subsampling was used for antialiasing, but by default only one shading sample was used for each polygon that fell within a pixel. (Though that polygon might cover a number of subsamples.) The assumption being that typically shading varied more slowly than geometry. (Shading every subsample could be forced when this wasn't the case.) I've always thought that the big win for REYES-type architectures is that motion blur was pretty much for free. With the traditional scanline renderers you have to render a number of slices and composite, so your rendering cost goes up as motion blur increases. With REYES, you're just perturbing a fixed number of fragments differently, so the cost stays pretty much the same. As a trivial data point, I was running some timing tests on a new PC we got in the graphics lab yesterday, on a 100,000 triangle whale model, in a 400x400 pixel window; definitely more than one polygon per pixel. On an SGI O2 the update rate for hardware rendering, one light source, was 0.59s per frame. On the new PC box, with a 450Mhz PIII, I was getting 0.50s per frame rendered with a nested grid raytracer for the same settings. Of course, for animation, handling things like texture map sizzle, shading, shadows, motion blur, and the sheer size of those scenes in a robust manner is often more important than getting the last ounce of speed out of your renderer. Andrew From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id UAA18872; Fri, 30 Jul 1999 20:46:18 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id UAA09080 for globillum-imag-outgoing; Fri, 30 Jul 1999 20:44:30 +0200 (MET DST) From: eric.haines@autodesk.com Message-ID: <19879C753611D3119DAB0008C7A4C0C101414467@hqmsgsrf04.autodesk.com> To: globillum@imag.fr Subject: RE: Ray tracing roundtable Date: Fri, 30 Jul 1999 11:44:22 -0700 MIME-Version: 1.0 X-Mailer: Internet Mail Service (5.5.2448.0) Content-Type: text/plain; charset=iso-8859-1; format=flowed Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: f0944cad81fef9fffb0d1e212045ea6a X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Dan Wexler wrote: > I don't think we're going to stick with the abuffer method either > for too much longer. The abuffer algorithm does not have very > good antialiasing qualities. The abuffer representation of a > subpixel fragment just isn't accurate enough for really high quality > antialiasing. It tries to represent a area (as opposed to a point > sample) and does so rather poorly, IMHO. I agree, it's poor for some cases. Near horizontal or vertical edges, for example, will tend to have only five levels of antialiasing with a 4x4 A-buffer, i.e. edge covers nothing, edge covers 1/4th, edge covers 2/4ths, edge covers 3/4ths, edge covers whole thing. It's pretty visible. Stochastic sampling or other non-uniform sampling schemes are really the way to go. But you have to walk before you run, so I suspect multisampling will (will? already is, on high-end SGIs) be the next step. One thing that would help multisampling further is actually doing half-decent filtering on it, not treating a pixel like a little square. Harder in hardware, since a sample then affects a few pixels. Eric From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id DAA31030; Wed, 4 Aug 1999 03:27:02 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id DAA13655 for globillum-imag-outgoing; Wed, 4 Aug 1999 03:24:43 +0200 (MET DST) Message-ID: <003901bede18$1b22cf00$989c42d8@byheart> Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: 99/08/01 Release of RADBIB99.BIB Date: Tue, 3 Aug 1999 18:24:30 -0700 Organization: byHeartConsultants Limited MIME-Version: 1.0 Content-Type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 5.00.2314.1300 X-MimeOLE: Produced By Microsoft MimeOLE V5.00.2314.1300 Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 8c9bc4e5a5ebdad01162b6fef3b9715f X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit ANNOUNCE: 99/08/01 Release of RADBIB99.BIB
------------------------------------------
RADBIB99 is a comprehensive bibliography of radiosity and
related global illumination papers, theses, articles, and
books. It currently includes 1,621 references -- 17 new
additions since the 99/07/15 release.

This bibliography is available in BibTex format as
RADBIB99.BIB (with a release date of August 1, 1999) from:

  http://www.helios32.com/resources.htm

Also available from this site is an abridged version of
RADBIB99.BIB called GITHESIS.BIB. This bibliography
includes 195 references to radiosity and global illumination
theses -- one new addition since the 99/07/15 release.

Financial support for the maintenance of these
bibliographies has been provided by ACM SIGGRAPH Special
Projects and byHeart Consultants Limited.
--
Ian Ashdown, P. Eng., LC
Vice President
byHeart Consultants Limited
http://www.helios32.com
 From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id HAA13502; Tue, 17 Aug 1999 07:03:18 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id HAA08841 for globillum-imag-outgoing; Tue, 17 Aug 1999 07:00:00 +0200 (MET DST) From: "Bretton Wade" To: "Globillum" Subject: Web pages, and conversations Date: Mon, 16 Aug 1999 21:58:54 -0700 Message-ID: MIME-Version: 1.0 Content-Type: text/plain; charset=iso-8859-1; format=flowed Content-Transfer-Encoding: 8bit X-Priority: 3 (Normal) X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook IMO, Build 9.0.2416 (9.0.2910.0) X-MimeOLE: Produced By Microsoft MimeOLE V5.00.2919.4200 Importance: Normal Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 97add151ae5c395ec8345fbac4965110 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hi folks, I enjoyed seeing, and in some cases meeting you all at SIGGRAPH. Some interesting points of discussion came up at different times. The one that I'm intrigued by was touched on somewhat at the BOF, but also at the ray-tracing roundtable, and that is the role of global illumination in the entertainment industry, or the lack thereof. I realize that this could be a divisive topic, so I'll take the low road and be provocative. Listening to the second (third?) annual panel on "(global illumination in production)" echoed several sentiments I heard from people at PDI and Pixar: 1. Global illumination is too expensive in terms of compute time, 2. Artists can get as good or better with the tools they have, and 3. Even if they had instant global illumination algorithms at hand, artists don't want the effect of realism. In fact, they want everything but realism. Blue Sky engineers confirmed what I inferred from the panel, that the use of globillum techniques, even for a lame scene in which most of the reflected energy would bounce into space, comes up almost even with the artists manually placing extra lights to achieve the desired results, at least in terms of time. The artist's time costs more, though. I'll make the additional observation that SIGGRAPH this year had a lot of algorithms presented that were strictly approximations useful to the entertainment industry. This is a fair deviation from past years, but I think it reflects one of the major consumers of the technology usually presented at SIGGRAPH. So what this comes down to is the question, "what computational tools for illumination would artists use, that the research community could actually delve into?" That could perhaps be worded more precisely, but I think it gets at the heart of the matter I'm thinking about, which is that the global illumination community hasn't really been developing what it's primary customer wants. If "we" were a company, we'd be going out of business. Now I realize that there are lots of important applications of true photorealistic image development, and physically accurate simulation. Perhaps it is just a side effect of the glamour of the entertainment industry overshadowing other professions, but I perceive that the bulk of our community not in academia is in entertainment (games, movies, television). One suggestion that Dani mentioned was an extended "Painting with Light", referring to the technique presented by Chris Schoeneman, et al. in 1993, for using least squares minimization to determine the needed intensity and color for a set of fixed position light sources. The next step in that direction sounds intimidating, placing light sources to accomodate a desired result. Bruce Walter et al. touched on this again in 1997 using ordinary Phong sources to capture highlights on specular surfaces in a hardware rendered walkthrough, again using least squares minimization. I'm sure there are other examples, but how much harder is the real problem? So, what thoughts does anybody have? On another note, could somebody *please* send me the URL for the globillum archive web page? -- Bretton Wade http://redirect.to/bretton_wade From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id SAA22442; Thu, 19 Aug 1999 18:28:42 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id SAA18604 for globillum-imag-outgoing; Thu, 19 Aug 1999 18:25:14 +0200 (MET DST) Message-ID: From: Francois Sillion To: "'globillum@imag.fr'" Subject: good old ones (from P. Dutre and M. Blais) Date: Thu, 19 Aug 1999 09:24:57 -0700 X-Mailer: Internet Mail Service (5.5.2448.0) Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 8e7a95209639e28274c5b0f8090fbcc4 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit [Remember, to prevent spamming you can only post to globillum from your currently listed address] > from [Phil > Dutre ] > Date: Mon, 16 Aug 1999 15:32:20 -0400 > From: Phil Dutre > Organization: Program of Computer Graphics > Subject: Re: good old ones > > Fabrice Neyret wrote: > > > -> do you know any way (group, news-group, store) to get them ? > > Sometimes they are being sold by an individual in one of the > comp.graphics.* newsgroups. > > You can also track them down through 2nd hand booksellers > (check www.barnesandnoble.com) > > These two approaches worked for me in the past. Nevertheless, > I'm still missing 1984, 1988 and 1990. > > > > On a totally unrelated note, I've started to compile a > 'Global Illumination Compendium', being a collection > of formulas useful in global illumination. I was getting tired > of trying to remember in what book or paper a certain equation > or formula was given, so I decided to collect them all in a single > document. So far, the information is limited (21 pages), but more > information is added on an 'as we need it' basis. > http://www.graphics.cornell.edu/~phil/GI/ > Any input, remarks, etc. are appreciated. > > > Phil Dutre > > > > -- > ============================================================== > ========= > Philip Dutre Program of Computer Graphics Cornell > University > phil@graphics.cornell.edu > http://www.graphics.cornell.edu/~phil/ > ============================================================== > ========= ---------------------------------------------------------------------------- ----------------------------- > Date: Mon, 16 Aug 1999 13:56:30 -0400 > From: Martin Blais > Organization: Discreet Logic > Subject: Re: old good ones > > Fabrice Neyret wrote: > > > > I really would like to found and buy very old Siggraph proceedings, > > my favorite epoch being 1983-1989. > > > > Siggraph and ACM have nothing that old > > ( I was so happy, 2 years ago, to get > > the last 1989, with a dammaged back cover ! > > ) > > ( hey, where our memory is going ? ) > > > > -> do you know any way (group, news-group, store) to get them ? > > ( Excepted by parsing every Library College Annual Big Sell, > > where some very lucky people I know could find somes at > 2$ each :^) > > ) > > > > Fabrice NEYRET > > I was looking for the same thing some time ago, but to no > avail. Someone who > wants to give up on their proceedings is pretty hard to > find... perhaps by > tracking down fatalities amongst some of us you could get > your hands on a big > collection ;-) > > More seriously, wouldn't it be really nice if ACM / SIGGRAPH > scan/converted the > old proceedings into pdf files and sold CD reprints of these > old proceedings? > > Also, maybe they are already available thru the ACM Digital Library? > > > > > -- > M. From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id UAA25160; Thu, 19 Aug 1999 20:26:45 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id UAA23162 for globillum-imag-outgoing; Thu, 19 Aug 1999 20:21:14 +0200 (MET DST) X-Gnus-Agent-Meta-Information: mail nil Original-Sender: mmp@nurbs.stanford.edu To: "'globillum@imag.fr'" Subject: Re: good old ones (from P. Dutre and M. Blais) References: X-Face: C!.oGaE]n@p)VF9Ss3]f'|<)kRrtpG)^^b^X-3_zhUHp\jBj29jaoTItqWR>mHa+v-{/!jx7OA@!cV0>Fm-b:zEL<`oOXG[BFQ\ Date: 19 Aug 1999 10:26:11 -0700 In-Reply-To: Francois Sillion's message of "Thu, 19 Aug 1999 09:24:57 -0700" Message-ID: User-Agent: Gnus/5.070095 (Pterodactyl Gnus v0.95) XEmacs/20.4 (Emerald) Content-Type: text/plain; charset=us-ascii; format=flowed X-Face: C!.oGaE]n@p)VF9Ss3]f'|<)kRrtpG)^^b^X-3_zhUHp\jBj29jaoTItqWR>mHa+v-{/!jx7OA@!cV0>Fm-b:zEL<`oOXG[BFQ\ writes: > > From: Martin Blais > > Organization: Discreet Logic > > Subject: Re: old good ones > > > > More seriously, wouldn't it be really nice if ACM / SIGGRAPH > > scan/converted the old proceedings into pdf files and sold CD reprints > > of these old proceedings? This question comes up on the comp.graphics newsgroups periodically. At some point, Stephen Spencer posted a reply to the effect that SIGGRAPH is aware of the issue and that remedies along the lines of CD reprints are in the works. -matt -- Matt Pharr mmp@graphics.stanford.edu From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id XAA29301; Thu, 19 Aug 1999 23:25:41 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id XAA28354 for globillum-imag-outgoing; Thu, 19 Aug 1999 23:19:42 +0200 (MET DST) From: eric.haines@autodesk.com Message-ID: <19879C753611D3119DAB0008C7A4C0C1019507DD@hqmsgsrf04.autodesk.com> To: globillum@imag.fr Subject: RE: good old ones (from P. Dutre and M. Blais) Date: Thu, 19 Aug 1999 14:19:31 -0700 MIME-Version: 1.0 X-Mailer: Internet Mail Service (5.5.2448.0) Content-Type: text/plain; charset=iso-8859-1; format=flowed Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: a5ac6364a5888af8159d45d1116a544b X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit > Fabrice Neyret wrote: > > > > I really would like to found and buy very old Siggraph proceedings, > > my favorite epoch being 1983-1989. Matt Pharr's comment is right, the ACM is eventually going to have everything ever published by them from 1947 on, journals & proceedings & etc, scanned in and available in the ACM Digital Library (http://www.acm.org/dl). From what I can tell, it's mostly just a matter of funding and time to scan and archive all the material. Right now the Digital Library dates back to about 1991-92 for everything, but even that's pretty useful - there are some hard-to-get proceedings out there that have solid information. If you use it, a nice deal at $87/year. Other resources on the web (though not of much help for pre 1992 papers, though...): http://www2.iro.umontreal.ca/~ratib/code/ (go to Applications/Computer Graphics/Publications) - a great resource, but only a few links to pre 1992 SIGGRAPH papers. http://w3imagis.imag.fr/Membres/Fredo.Durand/Book/publi.html - Siggraph 99 and other papers on the web, links to other wonderful resources. An actual repository exists at http://grafix3d.tzo.com/main/index.html (click on "quick list" at the bottom of the column), but this site is somewhat underpowered and a little clunky to access - nonetheless, it's quite a large graphics paper repository. Eric From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id PAA32342; Thu, 26 Aug 1999 15:54:18 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id PAA22419 for globillum-imag-outgoing; Thu, 26 Aug 1999 15:17:59 +0200 (MET DST) Message-ID: <37C53E89.5DAE696B@gmd.de> Date: Thu, 26 Aug 1999 15:18:02 +0200 From: Christian Bohn X-Mailer: Mozilla 4.51 [en] (X11; U; IRIX 6.3 IP32) X-Accept-Language: en MIME-Version: 1.0 To: globillum@imag.fr Subject: new rendering group at GMD / job offer Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 8bit Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 24d8f6394929fe2e02536918ad21409e X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 In July '99, GMD founded the 'research island' "Rendering Techniques and Application". Now, we are looking for people who want to take part in the early phase of defining research directions and the character of the group. Task of the island is doing fundamental research in rendering techniques and connected fields with focus on interactivity and on using rendering hardware. The size of the group is aimed at 5-7 people at the beginning of 2000. Positions offered are postdoctoral (full position), postgraduate (half-time), students, and trainees. For questions or more information contact me or have a look at http://viswiz.gmd.de/reta/ Thanks, feel free to distribute this offer. Christian Bohn -- Christian Bohn, Institute for Media Communication, GMD +49-2241-142230, http://viswiz.gmd.de/bohn, bohn@gmd.de From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id PAA31566; Thu, 26 Aug 1999 15:31:58 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id PAA23036 for globillum-imag-outgoing; Thu, 26 Aug 1999 15:25:44 +0200 (MET DST) Message-ID: <37C54061.3896D715@gmd.de> Date: Thu, 26 Aug 1999 15:25:54 +0200 From: Christian Bohn X-Mailer: Mozilla 4.51 [en] (X11; U; IRIX 6.3 IP32) X-Accept-Language: en MIME-Version: 1.0 To: globillum@imag.fr Subject: new rendering group at GMD / job offer / CORRECTION Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 8bit Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: b4415b3876450fbe0d0cdf6e94c362a1 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 It is http://imk.gmd.de/reta Sorry Christian -- Christian Bohn, Institute for Media Communication, GMD +49-2241-142230, http://viswiz.gmd.de/bohn, bohn@gmd.de From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.8.4/8.8.4) with ESMTP id HAA12879; Sun, 29 Aug 1999 07:23:17 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id HAA06086 for globillum-imag-outgoing; Sun, 29 Aug 1999 07:19:13 +0200 (MET DST) From: Peter Shirley Message-Id: <199908290518.XAA19578@lal.cs.utah.edu> Subject: BRDF links? To: globillum@imag.fr Date: Sat, 28 Aug 1999 23:18:33 -0600 (MDT) X-Mailer: ELM [version 2.4 PL25] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: db7c7c37f249b62a79983943de16ca44 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hi-- I am teaching a seminar on BRDFs this term: http://www2.cs.utah.edu/~shirley/classes/brdf/ If you have any other links please send them to me. Also, I used to have a list of journals etc on my page. If you used this they have moved to: http://www2.cs.utah.edu/vissim/resources/ Thanks Pete From Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id TAA08361; Tue, 31 Aug 1999 19:51:25 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id TAA25923 for globillum-imag-outgoing; Tue, 31 Aug 1999 19:44:13 +0200 (MET DST) Date: Tue, 31 Aug 1999 13:44:05 -0400 From: "Stephen N. Spencer" To: globillum@imag.fr Subject: Re: good old ones (from P. Dutre and M. Blais) In-Reply-To: Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII; format=flowed Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 7e2727f8e7b6064d2bc123ada2b07148 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit > More seriously, wouldn't it be really nice if ACM / SIGGRAPH > scan/converted the old proceedings into pdf files and sold CD reprints of > these old proceedings? Funny you should say that -- it's exactly what we're doing right now, with the help of Xerox Business Services. Hopefully they'll be available by year's end. > Also, maybe they are already available thru the ACM Digital Library? They'll be available through the ACM Digital Library, too, though probably not as quickly as they'll be available on CD. Stephen N. Spencer 614.292.1067 (v) Graphics Research Specialist spencer@siggraph.org 614.292.7776 (f) ACCAD - The Ohio State University spencer@cgrg.ohio-state.edu 614.520.5799 (p) SIGGRAPH Director for Publications spencer@acm.org "After ecstasy, laundry." -- Zen writing "The truth is that progress is usually small and sneaky." -- Anne Lamott From Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id RAA07138; Thu, 2 Sep 1999 17:44:13 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id RAA23908 for globillum-imag-outgoing; Thu, 2 Sep 1999 17:41:02 +0200 (MET DST) From: hertjwr@us.ibm.com X-Lotus-FromDomain: IBMUS To: Peter Shirley cc: globillum@imag.fr Message-ID: <852567E0.00561BB7.00@D51MTA03.pok.ibm.com> Date: Thu, 2 Sep 1999 11:40:29 -0400 Subject: Re: BRDF links? Mime-Version: 1.0 Content-type: text/plain; charset=us-ascii; format=flowed Content-Disposition: inline Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 6e6e2686ab98ff3ba2951a3ae8fa7522 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hi -- -- My own BRDF interests are in the capture end of things, and there are a fair number of papers in the Computer Vision literature. I can't find free on-line copies of many (i.e. if you have access to the IEEE or ACM digital libraries there are on-line copies), but at least one I think to note is: Object Shape and reflectance Modeling from Color Image Sequence Y. Sato http://www.ri.cmu.edu/pubs/pub_1438.html ____ My uncle asked me about an interesting problem involving BRDF. He had read once that we get 1/9 the light from a half moon than we get from a full moon. If you work it out for a Lambertian surface, we would get 1/pi the light. I couldn't come up with 1/9 right of the bat, but I think it has to do with the moon being retroreflective. Siegel and Howell points out since a full moon looks equally bright all the way across, the peak of retroreflectance must increase with view angle to compensate for the reduced projected area. If the 1/9 figure is correct, I think you can also estimate the width of the lobe around the direction of retroreflection ( or you could use the data from Siegel and Howell to approximate the BRDF and check if 1/9 is about right.) -- Holly __________________________ Holly Rushmeier , holly@watson.ibm.com, (914)784-7252 IBM TJ Watson Research Center, 30 Saw Mill River Road, Hawthorne, NY 10532, USA From Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id SAA09082; Thu, 2 Sep 1999 18:35:19 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id SAA26629 for globillum-imag-outgoing; Thu, 2 Sep 1999 18:32:36 +0200 (MET DST) Date: Thu, 2 Sep 1999 12:32:23 -0400 (EDT) Message-Id: <199909021632.MAA06058@bach.Graphics.Cornell.EDU> From: "Stephen H. Westin" To: globillum@imag.fr In-reply-to: <852567E0.00561BB7.00@D51MTA03.pok.ibm.com> (hertjwr@us.ibm.com) Subject: Re: BRDF links? Reply-to: westin@graphics.cornell.edu References: <852567E0.00561BB7.00@D51MTA03.pok.ibm.com> Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 589fb05786cf54bc96cb96136a930e96 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Holly wrote: > My uncle asked me about an interesting problem involving BRDF. He > had read once that we get 1/9 the light from a half moon than we get > from a full moon. If you work it out for a Lambertian surface, we > would get 1/pi the light. I couldn't come up with 1/9 right of the > bat, but I think it has to do with the moon being retroreflective. > Siegel and Howell points out since a full moon looks equally bright > all the way across, the peak of retroreflectance must increase with > view angle to compensate for the reduced projected area. If the 1/9 > figure is correct, I think you can also estimate the width of the > lobe around the direction of retroreflection ( or you could use the > data from Siegel and Howell to approximate the BRDF and check if 1/9 > is about right.) Actually, this is quite well studied in planetary science. A model originated by Hapke and enhanced over the last two or three decades is generally used; it includes a term for the "opposition surge", which is their term for retroreflection. I think there is still debate about the actual physical mechanism involved, and how best to model it. The enhanced Hapke model looks pretty ugly to me, but then what do I know about planetary science? Anyway, it's interesting to talk to these folks, as they have the opposite problem to rendering: they know something about the radiance, and want to deduce composition, surface structure, and even geometry from their images. The Moon has been studied particularly well, as it's the only extraterrestrial body from which we have actual samples. The hope is that a model that deduces the correct characteristics for the Moon will probably give you the right answer on Mars or an asteroid. -Stephen H. Westin Any information or opinions in this message are mine: they do not represent the position of Cornell University or any of its sponsors. From Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id XAA18738; Thu, 2 Sep 1999 23:45:25 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id XAA07105 for globillum-imag-outgoing; Thu, 2 Sep 1999 23:42:46 +0200 (MET DST) Date: Thu, 2 Sep 1999 14:21:11 -0700 (PDT) From: Alain Fournier Message-Id: <199909022121.OAA06588@pedigree.cs.ubc.ca> To: hertjwr@us.ibm.com, shirley@cs.utah.edu Subject: Re: BRDF links? Cc: globillum@imag.fr Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: c9d55f2cdafeca16a5506af4187b1c49 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit I remember that a simple formula to "explain" the uniform brightness of the full moon is that it raflects as cos(theta)^0.5, where theta of course is the angle between surface normal and light source (sun) direction, which is the same as the viewing direction when the moon is full. I would have to figure out if it gives the 1/9 ratio for the half moon. I also have to find the relevant references (Bob Woodham in our department has been involved with that very subject in the not too distant past). From Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id PAA01222; Mon, 6 Sep 1999 15:35:32 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id PAA08007 for globillum-imag-outgoing; Mon, 6 Sep 1999 15:29:46 +0200 (MET DST) From: eric.haines@autodesk.com Message-ID: <19879C753611D3119DAB0008C7A4C0C101C446F0@hqmsgsrf04.autodesk.com> To: globillum@imag.fr Subject: New ray tracing bibliography Date: Fri, 3 Sep 1999 08:13:30 -0700 MIME-Version: 1.0 X-Mailer: Internet Mail Service (5.5.2448.0) Content-Type: text/plain; charset=iso-8859-1; format=flowed Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 5d7c7e52e8892394f928c82a81ba5b2b X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit The free ray tracing bibliography has been updated, it's at http://www.acm.org/pubs/tog/resources/bib/ While it's continuing to get hazy as to what a ray tracing paper is (e.g. do Monte Carlo sampling papers count? No, I try to list papers specifically about how to do ray tracing, not about using ray tracing as a tool), I still think it's worth maintaining. As usual, let me know of any missing papers, Eric From Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id SAA04683; Mon, 6 Sep 1999 18:15:01 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id SAA12020 for globillum-imag-outgoing; Mon, 6 Sep 1999 18:07:49 +0200 (MET DST) Message-ID: <001501bef881$b4b0ae20$9f9c42d8@byheart> Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: globillum@imag.fr References: <19879C753611D3119DAB0008C7A4C0C101C446F0@hqmsgsrf04.autodesk.com> Subject: Re: New ray tracing bibliography Date: Mon, 6 Sep 1999 09:05:56 -0700 Organization: byHeartConsultants Limited MIME-Version: 1.0 Content-Type: text/plain; charset=iso-8859-1; format=flowed Content-Transfer-Encoding: 8bit X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 5.00.2314.1300 X-MimeOLE: Produced By Microsoft MimeOLE V5.00.2314.1300 Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: b4017c4b952f125dc6165bdeaa98c1cd X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 > The free ray tracing bibliography has been updated, it's at > http://www.acm.org/pubs/tog/resources/bib/ While it's continuing to get hazy > as to what a ray tracing paper is (e.g. do Monte Carlo sampling papers > count? No, I try to list papers specifically about how to do ray tracing, > not about using ray tracing as a tool), I still think it's worth > maintaining. > Given that the RADBIB global illumination bibliography gets over 100 hits a month from my Web site alone, I would say that Eric's maintaining his ray tracing bibliography is well worth the effort. If nothing else, consider the poor grad student who has to jump from Foley et al.'s Computer Graphics to researching a quarter-century of obscure publications. Keep up the good work, Eric -- it is appreciated! Ian Ashdown, P. Eng., LC Vice President byHeart Consultants Limited http://www.helios32.com From Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id WAA25882; Mon, 13 Sep 1999 22:42:50 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id WAA13543 for globillum-imag-outgoing; Mon, 13 Sep 1999 22:38:52 +0200 (MET DST) From: "A Gallardo" To: "Peter Shirley" , globillum@imag.fr Subject: RE: BRDF links? Date: Mon, 13 Sep 1999 16:30:20 -0400 Message-ID: <000801befe26$cc3106d0$e3d81a26@dellxps> MIME-Version: 1.0 Content-Type: text/plain; charset=iso-8859-1; format=flowed Content-Transfer-Encoding: 8bit X-Priority: 3 (Normal) X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook 8.5, Build 4.71.2377.0 In-Reply-To: <199908290518.XAA19578@lal.cs.utah.edu> X-MimeOLE: Produced By Microsoft MimeOLE V5.00.2014.211 Importance: Normal Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 7ef1f7b7f44c2f28172bcb588b91a0f1 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hi, Sorry for the delayed post. I am just catching up on my e-mail. Here are a few liks I have found. http://www.cgl.uwaterloo.ca/Projects/rendering/refl.html http://www.cs.columbia.edu/CAVE/curet/ Regards, Arnold Gallardo Visual Content Creator > -----Original Message----- > From: owner-globillum@imag.imag.fr > [mailto:owner-globillum@imag.imag.fr]On Behalf Of Peter Shirley > Sent: Sunday, August 29, 1999 1:19 AM > To: globillum@imag.fr > Subject: BRDF links? > > > > Hi-- I am teaching a seminar on BRDFs this term: > http://www2.cs.utah.edu/~shirley/classes/brdf/ > > If you have any other links please send them to me. > > Also, I used to have a list of journals etc on my page. > If you used this they have moved to: > http://www2.cs.utah.edu/vissim/resources/ > > Thanks > > Pete > From Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id XAA26270; Mon, 13 Sep 1999 23:18:48 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id XAA14935 for globillum-imag-outgoing; Mon, 13 Sep 1999 23:16:45 +0200 (MET DST) From: "A Gallardo" To: "Globillum" Subject: RE: Web pages, and conversations Date: Mon, 13 Sep 1999 17:16:26 -0400 Message-ID: <000901befe2d$3d4b48c0$e3d81a26@dellxps> MIME-Version: 1.0 Content-Type: text/plain; charset=iso-8859-1; format=flowed Content-Transfer-Encoding: 8bit X-Priority: 3 (Normal) X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook 8.5, Build 4.71.2377.0 In-Reply-To: X-MimeOLE: Produced By Microsoft MimeOLE V5.00.2014.211 Importance: Normal Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 6fb4a773ebabc2515d0aad9ac7fe9cc4 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hi, I am just catching up so sorry if this seemed old to you. I am not a global illum researcher per se but rather got into researching because of the radiosity images that I have seen as well as in using a commercially available progressive refinement program. My comments are below. > Listening to the second (third?) annual panel on "(global illumination in > production)" echoed several sentiments I heard from people at PDI > and Pixar: > > 1. Global illumination is too expensive in terms of compute time, > 2. Artists can get as good or better with the tools they have, and > 3. Even if they had instant global illumination algorithms > at hand, artists > don't want > the effect of realism. In fact, they want everything but realism. The third comment is true. Most users after being exposed to a commercial progressive refinement program says it too much work. Too many things to setup and it is easier to achieve by simulating radiosity using local none-shadow casting omnidirectional lights to simulate indirect illumination. It also requires a trememdous amount of processing power and RAM for complex scenes. Most people resent that fact that they have to redo the solutions again if they want to change the geometry. They expect the ease of moving geometry with ttheir scanline or raytracer program, none of them have heard about discontinuity meshing much less dynamic discontinuity meshing. On the other end of the spectrum, beginners using a relatively easy program with minimal parameters are baffled by terms like 'convergeance','iterations' and 'tonemapping'. They generally assume that radiosity is as easy as a raytracer which only requires light placement, color and intensity to work. They expect radiosity to have no 'user intervention issues' at all. Lastly most are not aware of the quadrilateral polygonal geometry requirement which speeds things up and avoid artifacts and they also expect NURBS-based geometry to work well with radiosity. I think that most end users are more likely to adapt to the monte-carlo based radiosity rather than with the deterministic ones. So the issue today is that radiosity even with its gorgeous renderings are no longer persuasive once the end user experience the amount of knowledge needed as well as the amount of intervention needed to produce realistic renderings. It is just so much easier to 'fake' radiosity. It remains to be seen if monte-carlo based radiosity would change the tide. Regards, Arnold Gallardo Visual Content Creator > So, what thoughts does anybody have? > > On another note, could somebody *please* send me the URL for the globillum > archive web page? > > -- > Bretton Wade > http://redirect.to/bretton_wade > From Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id XAA12892; Wed, 15 Sep 1999 23:08:36 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id XAA03907 for globillum-imag-outgoing; Wed, 15 Sep 1999 23:03:49 +0200 (MET DST) From: hertjwr@us.ibm.com X-Lotus-FromDomain: IBMUS To: globillum@imag.fr Message-ID: <852567ED.0073A7AE.00@D51MTA03.pok.ibm.com> Date: Wed, 15 Sep 1999 17:03:26 -0400 Subject: job openings Mime-Version: 1.0 Content-type: text/plain; charset=us-ascii; format=flowed Content-Disposition: inline Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 01bbfc3ab4010e507b24f0f65b33ff22 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Please note that you should contact Gabriel (contact coordinates at the end) with any questions about these openings (rather than using "Reply " to this note) -- Holly Rushmeier ========================================================================= Dear friends, I have two job openings in my department. Job #1 is at the programmer level. It requires a M.Sc. or B.Sc. in computer science, experience with graphics/geometric algorithms, and software development. The successful candidate will help other members of the group develop and implement new ideas, as well as transfer our technology to other IBM divisions, such as the Internet Division. Job #2 is post-doctoral position. The successful candidate will interact with other members of the group to invent and implement new geometric/graphics algorithms/technologies. In the Visual and Geometric Computing group, we are interested in issues related to 3D Graphics in a networked environment, including 3D scanning, surface reconstruction, surface simplification, geometry compression, progressive transmission, and rendering. We are also interested in new image-based representation and rendering schemes. The two most recent projects we have worked on are: 1) the Pieta project, where we reconstructed a 3D model of Michaelangelo's Florentine Pieta, to support art historian Jack Wasserman's study of the statue. 2) the Geometry Compression project, where the technology we developed during the last four years is now part of the MPEG-4 standard. In the 3D scanning front, and based on the experience acquired scanning the Pieta, we are now interested in developing new inexpensive and easy to use 3D scanning systems, including both hardware and software. In the Geometry Compression front, we are now working closely with the IBM Internet Media group to incorporate our MPEG-4 technology to their HotMedia product. We are also developing new schemes/algorithms. If any one of your students/associates is interested in any one of these two positions, please tell her/him to get in touch with me. IBM is an equal opportunity employer. Best regards. -------------------------------------------------------------------------- Gabriel Taubin Manager, Visual and Geometric Computing email: taubin@us.ibm.com IBM T. J. Watson Research Center phone: (914)-784-7095 P.O.Box 704, Yorktown Heights, NY 10598 fax : (914)-784-7667 -------------------------------------------------------------------------- From Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id WAA00228; Thu, 16 Sep 1999 22:11:00 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id VAA15088 for globillum-imag-outgoing; Thu, 16 Sep 1999 21:50:32 +0200 (MET DST) From: Paul.Heckbert@HOSTESS.GRAPHICS.CS.CMU.EDU Message-Id: <199909161950.VAA15084@imag.imag.fr> Date: Thu, 16 Sep 99 15:27:43 EDT To: globillum@imag.fr Subject: Re: global illumination in production Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 84fae8b009d073fe1fb680d803966fd8 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Arnold Gallardo says: | From: "A Gallardo" | Subject: RE: Web pages, and conversations | Date: Mon, 13 Sep 1999 17:16:26 -0400 | | ... sentiments I heard from people at PDI and Pixar: | > 1. Global illumination is too expensive in terms of compute time, | > 2. Artists can get as good or better with the tools they have, and | > 3. Even if they had instant global illumination algorithms | > at hand, artists don't want the effect of realism. | > In fact, they want everything but realism. This reminds me of attitudes regarding animation techniques from about ten or fifteen years ago. Back then, almost everybody doing animation was using keyframe or procedural methods, and there were only a few academic graphics people and finite element-oriented engineers doing dynamics, and only in specialized situations. The realism of dynamics was attractive, but nobody wanted to give up the control of keyframing systems and turn animation into an initial value problem (users' control limited to initial positions, velocities, masses, and positions), since it would be extremely tedious to get things to move where you wanted. Dynamics is still not easy to use, in general, but with faster hardware, improved algorithms, spacetime techniques, combinations of dynamics for realism and keyframing for control, and better user interfaces, dynamics is much more usable today than it was back then. It's no longer just a "research topic", but is used in production on a regular basis. Global illumination is probably a few years behind dynamics, but it has many of the same high level strengths and weaknesses: * it's good at achieving realism * achieving realism with "manual" techniques is tedious * if you use it whole hog, you give up control * it appears too slow * current methods are too specialized If we keep chipping away at the tough research problems, pay more attention to what users want (control, ease of use, ...) then global illumination will become very commonly used some day soon. -Paul Paul Heckbert, Associate Professor Computer Science Dept., Carnegie Mellon University 5000 Forbes Ave, Pittsburgh PA 15213-3891, USA ph@cs.cmu.edu http://www.cs.cmu.edu/~ph From Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id SAA21183; Fri, 17 Sep 1999 18:12:18 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id QAA09893 for globillum-imag-outgoing; Fri, 17 Sep 1999 16:02:31 +0200 (MET DST) Message-ID: <37E249F2.DAA98529@gmd.de> Date: Fri, 17 Sep 1999 16:02:26 +0200 From: Christian Bohn X-Mailer: Mozilla 4.51 [en] (X11; U; IRIX 6.3 IP32) X-Accept-Language: en MIME-Version: 1.0 To: globillum@imag.fr Subject: CG and wave theory ? Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 8bit Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: c3ef4dacca96d1212deae17bdcc6a2c6 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Hi all, Does anybody know about recent activities concerning '3D-CG and wave theory'? It seems that actually there's not much interest in that field?! What I only found is Moravec's paper from siggraph'81, and I am wondering if anybody else did some work during the past two decades. Thanks for any links, references, etc. Christian -- Christian Bohn, Institute for Media Communication, GMD +49-2241-142230, http://viswiz.gmd.de/bohn, bohn@gmd.de From Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id SAA21478; Fri, 17 Sep 1999 18:39:55 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id SAA19055 for globillum-imag-outgoing; Fri, 17 Sep 1999 18:23:41 +0200 (MET DST) Message-ID: From: "Michael Cohen (Research)" To: "'globillum@imag.fr'" Subject: RE: CG and wave theory ? Date: Fri, 17 Sep 1999 09:23:33 -0700 X-Mailer: Internet Mail Service (5.5.2524.0) Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 42c5ac5725b0b3f3edad21be3facfce2 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit I think Gershon Elber had a related paper in SIGGRAPH in '97 or '98 ??? - Michael > -----Original Message----- > From: Christian Bohn [SMTP:bohn@gmd.de] > Sent: Friday, September 17, 1999 7:02 AM > To: globillum@imag.fr > Subject: CG and wave theory ? > > Hi all, > Does anybody know about recent activities concerning > '3D-CG and wave theory'? > > It seems that actually there's not much interest in that field?! > What I only found is Moravec's paper from siggraph'81, and I am > wondering if anybody else did some work during the past two decades. > > Thanks for any links, references, etc. > > Christian > > > > -- > Christian Bohn, Institute for Media Communication, GMD > +49-2241-142230, http://viswiz.gmd.de/bohn, bohn@gmd.de > > From Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id TAA22483; Fri, 17 Sep 1999 19:13:11 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id TAA20966 for globillum-imag-outgoing; Fri, 17 Sep 1999 19:02:58 +0200 (MET DST) Date: Fri, 17 Sep 1999 13:02:53 -0400 (EDT) Message-Id: <199909171702.NAA08236@bach.Graphics.Cornell.EDU> From: "Stephen H. Westin" To: globillum@imag.fr In-reply-to: <37E249F2.DAA98529@gmd.de> (message from Christian Bohn on Fri, 17 Sep 1999 16:02:26 +0200) Subject: Re: CG and wave theory ? Reply-to: westin@graphics.cornell.edu References: <37E249F2.DAA98529@gmd.de> Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 802230c0f01bd30608c80eb1f33a29d6 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit > Date: Fri, 17 Sep 1999 16:02:26 +0200 > From: Christian Bohn > X-Accept-Language: en > Content-Type: text/plain; charset=us-ascii > Sender: owner-globillum@imag.imag.fr > Precedence: bulk > > Hi all, > Does anybody know about recent activities concerning > '3D-CG and wave theory'? > > It seems that actually there's not much interest in that field?! > What I only found is Moravec's paper from siggraph'81, and I am > wondering if anybody else did some work during the past two decades. Well, modeling light as waves at a macro level doesn't really make a lot of sense: you need incredible resolution (Moravec's paper really basically did visualization of radio wave propagation) and it's hard to find a situation where it makes a visible difference. More useful is modeling wave optics where it really does matter: in interaction with surfaces and such. Several papers deal with that: the SIGGRAPH '91 paper from He et al. comes to mind. That solved for wave optics of a class of rough surfaces. Gondek and Meyer did simulations of reflectance, including interference effects within the surface microstructure; that was presented at SIGGRAPH '94, as I recall. And it followed on a Eurographics '90 (I think) paper by Smits and Meyer. Most recently, Jos Stam presented a paper last month at SIGGRAPH on an anisotropic wave-optics model. On the original point, Peter Kochevar did his dissertation here at Cornell in 1989 on a cell-based rendering method designed for massive parallelism. While it wasn't explicitly wave-based, it exhibited some similar characteristics, such as diffraction around corners. From Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id UAA24012; Fri, 17 Sep 1999 20:53:08 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id UAA24589 for globillum-imag-outgoing; Fri, 17 Sep 1999 20:14:16 +0200 (MET DST) Date: Fri, 17 Sep 1999 14:14:10 -0400 From: "Stephen N. Spencer" To: globillum@imag.fr cc: globillum@imag.fr Subject: Re: CG and wave theory ? In-Reply-To: <37E249F2.DAA98529@gmd.de> Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII; format=flowed Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 4dfeacb08e36d892a3a64caeee610645 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit On Fri, 17 Sep 1999, Christian Bohn wrote: > Does anybody know about recent activities concerning > '3D-CG and wave theory'? How 'bout Jos Stam's SIGGRAPH 99 paper on diffraction shaders? Stephen N. Spencer 614.292.1067 (v) Graphics Research Specialist spencer@siggraph.org 614.292.7776 (f) ACCAD - The Ohio State University spencer@cgrg.ohio-state.edu 614.520.5799 (p) SIGGRAPH Director for Publications spencer@acm.org "After ecstasy, laundry." -- Zen writing "The truth is that progress is usually small and sneaky." -- Anne Lamott From Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id VAA24347; Fri, 17 Sep 1999 21:13:34 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id UAA26357 for globillum-imag-outgoing; Fri, 17 Sep 1999 20:56:34 +0200 (MET DST) From: hertjwr@us.ibm.com X-Lotus-FromDomain: IBMUS To: "Michael Cohen (Research)" cc: "'globillum@imag.fr'" Message-ID: <852567EF.0067FEC5.00@D51MTA03.pok.ibm.com> Date: Fri, 17 Sep 1999 14:56:10 -0400 Subject: RE: CG and wave theory ? Mime-Version: 1.0 Content-type: text/plain; charset=us-ascii; format=flowed Content-Disposition: inline Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: ebb380db0ebd419f9aee63d3e9cfa22c X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Maybe you are thinking of: Gershon Elber. ``Low Cost Illumination Computation using an Approximation of Light Wavefronts.'' Computer Graphics, pp 335-342, July 1994, (Siggraph 1994) ? I think the above paper is about a geometric solution to following sets of waves by following a "wavefront" coming from a spherical source. It doesn't treat the wave nature of light. __________________________ Holly Rushmeier , holly@watson.ibm.com, (914)784-7252 IBM TJ Watson Research Center, 30 Saw Mill River Road, Hawthorne, NY 10532, USA From Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id KAA27507; Wed, 22 Sep 1999 10:28:09 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id KAA03145 for globillum-imag-outgoing; Wed, 22 Sep 1999 10:25:13 +0200 (MET DST) From: Fredo Durand Message-Id: <199909220825.EAA22969@hue.lcs.mit.edu> Subject: Re: wavefront To: globillum@imag.fr Date: Wed, 22 Sep 1999 04:25:04 -0400 (EDT) X-Mailer: ELM [version 2.4 PL25] MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: fce2315dc85233028627c26505566fe8 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 You can also have a look at: http://www.lems.brown.edu/~leymarie/WaveRender/NotesDec98.html for a research project related to wave propagation I'm sure there are also lots of references in sound simulation Fredo From Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id PAA04456; Wed, 22 Sep 1999 15:10:48 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id OAA00701 for globillum-imag-outgoing; Wed, 22 Sep 1999 14:54:57 +0200 (MET DST) From: hertjwr@us.ibm.com X-Lotus-FromDomain: IBMUS To: Fredo Durand cc: globillum@imag.fr Message-ID: <852567F4.0046E87B.00@D51MTA03.pok.ibm.com> Date: Wed, 22 Sep 1999 08:54:27 -0400 Subject: Re: wavefront Mime-Version: 1.0 Content-type: text/plain; charset=us-ascii; format=flowed Content-Disposition: inline Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 30d44aec63895bf31e494fafe151c314 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit The approach described in the page Fredo cited seems to me in some ways similar to the Gelber SIGGRAPH 94 paper. They are all using **geometric optics**. The geometrical wavefront being modelled is the surface that is perpendicular to the light rays passing through it. I think Mitchell and Hanrahan's SIGGRAPH 92 was the first to describe these geometric wavefronts and their use in an illumination solution in graphics. Leymarie and Kimia discuss the use of BRDF's in the solution, and BRDF's are the encapsulation of the wave effects of light near a surface when you have to take into account geometric features comparable in size to the wavelength of light. They take an approach for tracking this waves using cellular automata -- which sounds very similar to Peter Kochevar's work that Steve Westin referred to. You can't capture diffraction, interference effects with this voxel approach, unless you have voxels smaller than the wavelength of the radiation. For visible light, this means chopping up the environment pretty finely!! For other types of radiation with substantionally longer wavelengths this is not so bad. Anyway, -- computing geometric wavefronts is not the same as computing effects due to the wave nature of light (i.e. diffraction, interference), but they are both interesting topics -- for the complexity of solving for effects of the wave nature of light we are stuck with dealing with discretizations on the order of (wavelength of light/ our size) or approx.10-7, which makes it much more demanding computationally that some other types of radiation. __________ -- Holly __________________________ Holly Rushmeier , holly@watson.ibm.com, (914)784-7252 IBM TJ Watson Research Center, 30 Saw Mill River Road, Hawthorne, NY 10532, USA Fredo Durand @imag.imag.fr on 09/22/99 04:25:04 AM Sent by: owner-globillum@imag.imag.fr To: globillum@imag.fr cc: Subject: Re: wavefront You can also have a look at: http://www.lems.brown.edu/~leymarie/WaveRender/NotesDec98.html for a research project related to wave propagation I'm sure there are also lots of references in sound simulation Fredo From Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id RAA03334; Wed, 22 Sep 1999 17:14:29 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id RAA11265 for globillum-imag-outgoing; Wed, 22 Sep 1999 17:09:21 +0200 (MET DST) Date: Wed, 22 Sep 1999 11:09:14 -0400 (EDT) From: Jack Tumblin To: hertjwr@us.ibm.com cc: Fredo Durand , globillum@imag.fr Subject: Re: wavefront In-Reply-To: <852567F4.0046E87B.00@D51MTA03.pok.ibm.com> Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII; format=flowed Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: f9e974ce4262bca8bf558d3806be8d25 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Gulp, I'm not very familiar with these papers on wave optics in computer graphics, so maybe I should keep my mouth shut here, but sampling volumes at wavelength resolution seems an especially unfortunate choice for modeling wave propagation in the free space between objects. Instead, I'd suggest looking at the Fourier optics formulation for free-space propagation of coherent and monochromatic incoherent light. It is a wave-optics technique that describes light as a continuous-domain complex scalar field: each point (x,y,z) has just amplitude and phase. The math for propagation through free space (or any ordinary uniform medium) from a point source uses a quadratic approximation that looks ALMOST like a Fourier transform, and has proved very accurate for lenses, holography, diffraction and interference through arbitrary apertures, and lots of work in optical computing (military folks used Fourier-optics-based equipment as much as 35-45 years ago for broadband radio surveillance/spying). Would Fourier optics permit us to compute some sort of `complex form factor' to describe the aggregate phase and amplitude relationship between surface patches alone, so that we can forget about the empty volume inbetween? Perhaps a complex integration across source and the receiver patches chosen according to display image resolution? Of course this patch-to-patch integral might be even tougher to solve than Shroder&Hanrahan's precise form factor integral of SIGGRAPH'93, but who knows--it might be simpler. Is it REALLY necessary to have wave-sized patches, even on surfaces, if 1) their results are merged to screen resolution for display, and 2) their free-space interactions are a weighted sum of many sinusoids? I think only the DISTANCES between surface points matter for the wave effects of interest to computer graphics; there's no need to sample those distances to find the phase of a sinusoid spanning it! The classic text for Fourier Optics is: "Introduction to Fourier Optics" J.W.Goodman(1968), and the library website shows 16 other promising looking tutorials & textbooks. It's course material in the optics track in Electrical Engineering here at Tech, (William Rhoades taught / teaches it and later wrote a textbook for the course I took long ago). Regards, -Jack Tumblin (ccsupjt@cc.gatech.edu) Gradual Student, College of Computing (leaving for Cornell Univ. post-doc Sept 23) "Black care rarely sits behind a rider who is fast enough" T. Roosevelt On Wed, 22 Sep 1999 hertjwr@us.ibm.com wrote: > The approach described in the page Fredo cited seems to me in some ways similar > to the Gelber SIGGRAPH 94 paper. They are all using **geometric > optics**. The geometrical ... > > Leymarie and Kimia discuss the use of BRDF's in the solution, > and BRDF's are the encapsulation of the wave effects of light near a surface > when you have to take into account geometric features comparable in size > to the wavelength of light. They take an approach for tracking this > waves using cellular automata -- which sounds very similar to Peter > Kochevar's work that Steve Westin referred to. You can't capture > diffraction, interference effects with this voxel approach, unless you > have voxels smaller than the wavelength of the radiation. For visible > light, this means chopping up the environment pretty finely!! For other > types of radiation with substantionally longer wavelengths this is not > so bad. > >for the complexity of solving for effects of the wave nature of light we are !!!!> stuck with dealing with discretizations on the order of (wavelength !!!!> of light/ our size) or approx.10-7, which makes it much more !!!!> demanding computationally that some other types of radiation. > __________ > Holly Rushmeier , holly@watson.ibm.com, (914)784-7252 > IBM TJ Watson Research Center, 30 Saw Mill River Road, Hawthorne, NY 10532, USA > > > Fredo Durand @imag.imag.fr on 09/22/99 04:25:04 AM > You can also have a look at: > http://www.lems.brown.edu/~leymarie/WaveRender/NotesDec98.html > for a research project related to wave propagation > > I'm sure there are also lots of references in sound simulation > > Fredo From Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id VAA00655; Wed, 22 Sep 1999 21:48:55 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id VAA28573 for globillum-imag-outgoing; Wed, 22 Sep 1999 21:45:32 +0200 (MET DST) Message-ID: From: Don Mitchell To: globillum@imag.fr Subject: RE: wavefront Date: Wed, 22 Sep 1999 12:35:12 -0700 X-Mailer: Internet Mail Service (5.5.2650.21) Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: ffb453c98c3b812223a4e0d191353a1d X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Shinya's pencil-tracing paper is also based on geometrical optics, described with a somewhat different formalism. Wavefront tracing buys you the ability to get an irradiance value along the ray, so you can almost do backward ray tracing with interpolation instead of density estimation. However, because the wavefront can fold, generating caustics, that interpolation is not simple. There was an elegant paper from Manchester (and I'm blanking on the reference now...) where they did backward wavefront tracing, and used the curvature to control the kernel size in a density estimation. -----Original Message----- From: hertjwr@us.ibm.com [mailto:hertjwr@us.ibm.com] Sent: Wednesday, September 22, 1999 5:54 AM To: Fredo Durand Cc: globillum@imag.fr Subject: Re: wavefront The approach described in the page Fredo cited seems to me in some ways similar to the Gelber SIGGRAPH 94 paper. They are all using **geometric optics**. The geometrical wavefront being modelled is the surface that is perpendicular to the light rays passing through it. I think Mitchell and Hanrahan's SIGGRAPH 92 was the first to describe these geometric wavefronts and their use in an illumination solution in graphics. Leymarie and Kimia discuss the use of BRDF's in the solution, and BRDF's are the encapsulation of the wave effects of light near a surface when you have to take into account geometric features comparable in size to the wavelength of light. They take an approach for tracking this waves using cellular automata -- which sounds very similar to Peter Kochevar's work that Steve Westin referred to. You can't capture diffraction, interference effects with this voxel approach, unless you have voxels smaller than the wavelength of the radiation. For visible light, this means chopping up the environment pretty finely!! For other types of radiation with substantionally longer wavelengths this is not so bad. Anyway, -- computing geometric wavefronts is not the same as computing effects due to the wave nature of light (i.e. diffraction, interference), but they are both interesting topics -- for the complexity of solving for effects of the wave nature of light we are stuck with dealing with discretizations on the order of (wavelength of light/ our size) or approx.10-7, which makes it much more demanding computationally that some other types of radiation. __________ -- Holly __________________________ Holly Rushmeier , holly@watson.ibm.com, (914)784-7252 IBM TJ Watson Research Center, 30 Saw Mill River Road, Hawthorne, NY 10532, USA Fredo Durand @imag.imag.fr on 09/22/99 04:25:04 AM Sent by: owner-globillum@imag.imag.fr To: globillum@imag.fr cc: Subject: Re: wavefront You can also have a look at: http://www.lems.brown.edu/~leymarie/WaveRender/NotesDec98.html for a research project related to wave propagation I'm sure there are also lots of references in sound simulation Fredo From Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id WAA01143; Wed, 22 Sep 1999 22:33:12 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id WAA00566 for globillum-imag-outgoing; Wed, 22 Sep 1999 22:30:48 +0200 (MET DST) Message-ID: <000401bf0610$7b801c20$0c0200c0@langzaam.toren.com> From: "tallind" To: hertjwr@us.ibm.com, "Fredo Durand" Cc: globillum@imag.fr Subject: Re: wavefront Date: Fri, 24 Sep 1999 00:10:43 +0200 MIME-Version: 1.0 Content-Type: text/plain; charset=iso-8859-1; format=flowed Content-Transfer-Encoding: 8bit X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 4.72.3110.5 X-MimeOLE: Produced By Microsoft MimeOLE V4.72.3110.3 Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 0276850bcfe320b125e7b1a417e5c06a X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Hi, I`m Jolly. I joined the global illumiation newsletter not so long ago. What I want to ask is what program you people think is the best for architectural visualisation. ( and would be able to be used in a production enviroment ) Regards, Jolly From Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id SAA21631; Fri, 8 Oct 1999 18:03:31 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id RAA05783 for globillum-imag-outgoing; Fri, 8 Oct 1999 17:55:11 +0200 (MET DST) Date: Fri, 8 Oct 1999 11:55:06 -0400 From: "Stephen N. Spencer" To: globillum@imag.fr Subject: [globillum] SIGGRAPH paper template in Word? In-Reply-To: <000901befe2d$3d4b48c0$e3d81a26@dellxps> Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII; format=flowed Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 50f23550990aa9d56ba73ba8ce938529 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit All -- sorry for the off-topic item, but I'm curious to find out if anyone hsa a Microsoft Word template for SIGGRAPH papers that they'd be willing to donate for others to use. If you've got one, e-mail it my way, please. Thanks! Stephen N. Spencer 614.292.1067 (v) Graphics Research Specialist spencer@siggraph.org 614.292.7776 (f) ACCAD - The Ohio State University spencer@cgrg.ohio-state.edu 614.520.5799 (p) SIGGRAPH Director for Publications spencer@acm.org "After ecstasy, laundry." -- Zen writing "The truth is that progress is usually small and sneaky." -- Anne Lamott "What is maddening is the terrible notion that a person's value depends on how important and financially successful they are, and that this is measured in terms of money." -- Tim Berners-Lee From Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id EAA11822; Mon, 11 Oct 1999 04:57:50 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id EAA02374 for globillum-imag-outgoing; Mon, 11 Oct 1999 04:55:18 +0200 (MET DST) Message-ID: <001a01bf1393$9ca766c0$669c42d8@byheart> Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: 99/10/09 Release of RADBIB99.BIB Date: Sun, 10 Oct 1999 19:52:08 -0700 Organization: byHeartConsultants Limited MIME-Version: 1.0 Content-Type: text/plain; charset=iso-8859-1; format=flowed Content-Transfer-Encoding: 8bit X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 5.00.2314.1300 X-MimeOLE: Produced By Microsoft MimeOLE V5.00.2314.1300 Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 83b6630c721f12efab65b90554796eda X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 ANNOUNCE: 99/10/09 Release of RADBIB99.BIB ------------------------------------------ RADBIB99 is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. It currently includes 1,661 references -- 40 new additions since the 99/08/01 release. This bibliography is available in BibTex format as RADBIB99.BIB (with a release date of October 9, 1999) from: http://www.helios32.com/resources.htm Also available from this site is an abridged version of RADBIB99.BIB called GITHESIS.BIB. This bibliography includes 195 references to radiosity and global illumination theses -- no new additions since the 99/07/15 release. Financial support for the maintenance of these bibliographies has been provided by ACM SIGGRAPH Special Projects and byHeart Consultants Limited. Ian Ashdown, P. Eng., LC Vice President byHeart Consultants Limited http://www.helios32.com From Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id AAA26295; Mon, 18 Oct 1999 00:33:46 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id AAA16233 for globillum-imag-outgoing; Mon, 18 Oct 1999 00:23:21 +0200 (MET DST) Date: Mon, 18 Oct 1999 00:23:15 +0200 From: Jan Prikryl To: globillum@imag.fr Subject: Best efficiency scheme project proposal Message-ID: <19991018002315.A31375@launzatte.cg.tuwien.ac.at> Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed X-Mailer: Mutt 0.95.4i Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: bd06813c549cb323714bb70057424630 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Dear everyone, inspired by the debate in RTNews about which space-subdivision scheme actually performs best for ray-shooting, we put together a proposal for a project that aims to statistically evaluate the performance of different space-subdivision schemes for scenes of different complexity and for several slightly different ray-shooting tasks. The preliminary version of the project proposal can be found at http://www.cgg.cvut.cz/GOLEM/proposal1.html If any reader of this list would like to comment on the proposal, all the comments are welcome on e-mail addresses listed in the header of the project proposal. We are currently in the stage of collecting test scenes for the project. We are going through several scene collections that are available on Internet, but this won't be probably enough. Therefore I wanted to ask: Does anyone of you know a source of good moderately-to-highly complex scene geometries that we could use? Does anyone have an idea if there are any companies that we could ask for support? Is any reader of this list willing to support us with the scenes that they use? And all this with restriction that the scenes are made publicly available after finishing the project so that other people can cross-check our results without too much hassle? Thanks in advance for any response. Vlastimil Havran/Jiri Bittner/Jan Prikryl -- ------------------------------------------------------------------------- Jan Prikryl http://www.cg.tuwien.ac.at/staff/JanPrikryl.html Institute of Computer Graphics and Visualisation Vienna University of Technology, Austria ------------------------------------------------------------------------- From Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id SAA07499; Mon, 8 Nov 1999 18:38:48 +0100 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id SAA11526 for globillum-imag-outgoing; Mon, 8 Nov 1999 18:30:52 +0100 (MET) From: Kavita Bala Message-Id: <199911081730.MAA40801@fresco.lcs.mit.edu> Subject: PhD thesis available online To: globillum@imag.fr Date: Mon, 8 Nov 1999 12:30:37 -0500 (EST) Cc: Kavita Bala X-Mailer: ELM [version 2.4 PL25] MIME-Version: 1.0 Content-Type: text/plain; charset=ISO-8859-1; format=flowed Content-Transfer-Encoding: 8bit Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: e08694e12652718a164630c28993ac14 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 FYI, I recently completed my PhD at the MIT Graphics Group under the supervision of Profs. Julie Dorsey and Seth Teller. The title of my thesis is: "Radiance Interpolants for Interactive Scene Editing and Ray Tracing" The abstract is included below. The thesis is now available at: http://www.graphics.cornell.edu/~kb/publications.html Kavita Bala WWW : http://www.graphics.cornell.edu/~kb email: kb@graphics.cornell.edu Abstract: Ray tracers are usually regarded as off-line rendering algorithms that are too slow for interactive use. This thesis introduces techniques to accelerate ray tracing and to support interactive editing of ray-traced scenes. These techniques should be useful in many applications, such as architectural walk-throughs, modeling, and games, and will enhance both interactive and batch rendering. This thesis introduces {\em radiance interpolants}: radiance samples that can be used to rapidly approximate radiance with bounded approximation error. Radiance interpolants capture object-space, ray-space, image-space and temporal coherence in the radiance function. New algorithms are presented that efficiently, accurately and conservatively bound approximation error. The {\em interpolant ray tracer} is a novel renderer that uses radiance interpolants to accelerate both primary operations of a ray tracer: shading and visibility determination. Shading is accelerated by quadrilinearly interpolating the radiance samples associated with a radiance interpolant. Determination of the visible object at each pixel is accelerated by {\em reprojecting} interpolants as the user's viewpoint changes. A fast scan-line algorithm then achieves high performance without sacrificing image quality. For a smoothly varying viewpoint, the combination of lazily sampled interpolants and reprojection substantially accelerates the ray tracer. Additionally, an efficient cache management algorithm keeps the memory footprint of the system small with negligible overhead. The interpolant ray tracer is the first accelerated ray tracer that reconstructs radiance from sparse samples while bounding error conservatively. The system controls error by adaptively sampling at discontinuities and radiance non-linearities. Because the error introduced by interpolation does not exceed a user-specified bound, the user can trade performance for quality. The interpolant ray tracer also supports interactive scene editing with {\em incremental} rendering; it is the first incremental ray tracer to support both object manipulation and changes to the viewpoint. A new hierarchical data structure, called the {\em ray segment tree}, tracks the dependencies of radiance interpolants on regions of world space. When the scene is edited, affected interpolants are rapidly identified and updated by traversing these ray segment trees. From Received: from acm.org (IDENT:prikryl@launzatte.cg.tuwien.ac.at [128.130.166.38]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id UAA08613 for ; Tue, 9 Nov 1999 20:45:08 +0100 Sender: prikryl Message-ID: <382879C4.AFCA30B9@acm.org> Date: Tue, 09 Nov 1999 20:45:08 +0100 From: Jan Prikryl X-Mailer: Mozilla 4.7 [en] (X11; I; Linux 2.2.10 i686) X-Accept-Language: Czech, en, de-AT, de-CH, de-DE, de MIME-Version: 1.0 To: rendering-group@cg.tuwien.ac.at Subject: GMTC Survey Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 8bit X-UIDL: 69e76ef1227977871a4da5b16b595335 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 http://www.colour.org/tc8-03/survey/survey_index.html From Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id QAA10708; Tue, 16 Nov 1999 16:13:03 +0100 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id PAA04117 for globillum-imag-outgoing; Tue, 16 Nov 1999 15:35:22 +0100 (MET) From: eric.haines@autodesk.com Message-ID: <19879C753611D3119DAB0008C7A4C0C102A44B70@hqmsgsrf04.autodesk.com> To: globillum@imag.fr Subject: Standard Procedural Databases version 3.13 out Date: Tue, 16 Nov 1999 06:34:50 -0800 MIME-Version: 1.0 X-Mailer: Internet Mail Service (5.5.2448.0) Content-Type: text/plain; charset=iso-8859-1; format=flowed Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 97b3d603320410954949ea79d040e493 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit An updated version of the Standard Procedural Databases (SPD) is now available at: http://www.acm.org/tog/resources/SPD/overview.html Though the SPD output is not meant to be a serious shading language, nonetheless I felt it worth making the visual results using VRML, Rayshade, and POV-Ray be as close as (easily) possible. There were some bugs in the previous version of the SPD, including the problem of determining whether a renderer uses Phong's specular highlighting or Blinn's formula (see "R.E versus N.H Specular Highlights" in Graphics Gems IV). OpenGL/VRML uses Blinn's N.H, Rayshade uses Phong's original R.E, and POV-Ray uses both. I've put updated images of the databases on the site, at full resolution and color (in PNG format, click the thumbnails). The SPD are a set of programs which generate models procedurally. They're meant for testing ray tracing efficiency schemes [rayshade with tweaked grids seems to still be a fair bit faster than POV-Ray, by the way], but can be adapted to experiments in real-time display systems (multiple levels of detail, for example), and tessellation of all primitives is built in as an output option. For example, the famous teapot is stored in its original spline surface form and can be generated at any level of complexity. NFF (Neutral File Format, the default output of the SPD programs) is a stupid little language which is relatively easy to edit by hand. It's much easier than VRML, for example; no human alive can set a non-trivial VRML camera by hand. That said, NFF's not particularly efficient (no polygon meshes, for example). Using the "readnff" program, NFF models can be converted to about 16 different file formats (some ancient), including POV-Ray, RIB, DXF, VRML, and Rayshade (these are also directly supported by the generating programs). One interesting new project to extend the NFF language is at http://www.ce.chalmers.se/staff/tomasm/benchmark/index.html - the idea is to make the data generated also have animation information, so that time-related ray-tracing efficiency scheme research can be done on a shared set of benchmarks. Enjoy, Eric Haines erich@acm.org http://www.acm.org/tog/editors/erich/ From Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id TAA01759; Thu, 18 Nov 1999 19:28:41 +0100 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id TAA08759 for globillum-imag-outgoing; Thu, 18 Nov 1999 19:24:09 +0100 (MET) Date: Thu, 18 Nov 1999 13:23:48 -0500 (EST) Message-Id: <199911181823.NAA21762@bach.Graphics.Cornell.EDU> From: "Stephen H. Westin" To: globillum@imag.fr cc: jstam@aw.sgi.com, mmccool@mud.cgl.uwaterloo.ca, okk@gin.keldysh.ru Subject: Skin BRDF data now available Reply-to: westin@graphics.cornell.edu References: <38281B7A.CBBCA44A@cs.kuleuven.ac.be> Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 480db70e8216a51ae930c33c991af9c9 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit In response to several requests, we have made available measured skin BRDF data from the 1999 EGWR paper, "Image-Based BRDF Measurement Including Human Skin", by Steve Marschner, myself, Eric Lafortune, Ken Torrance, and Don Greenberg. Data are in gzipped tar archives, each with a lot of binary data files containing raw BRDF samples in red, green, and blue channels. Data on the spectral response of the camera and the spectral balance of the source are included, and two of the three data sets include coefficients for rendering with the multi-lobe representation of Lafortune et al. (SIGGRAPH 97). The URL is . Have fun. Stephen H. Westin Research Project Leader Program of Computer Graphics Cornell University westin@graphics.cornell.edu 607 255 9080 (VOX) 607 255 0806 (FAX) From Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id VAA06158; Thu, 18 Nov 1999 21:38:23 +0100 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id VAA15480 for globillum-imag-outgoing; Thu, 18 Nov 1999 21:36:10 +0100 (MET) Date: Thu, 18 Nov 1999 15:36:06 -0500 (EST) Message-Id: <199911182036.PAA23395@bach.Graphics.Cornell.EDU> From: "Stephen H. Westin" To: musgrave@metacreations.com CC: globillum@imag.fr In-reply-to: (message from Ken Musgrave on Thu, 18 Nov 1999 12:19:21 -0800) Subject: Re: Skin BRDF data now available Reply-to: westin@graphics.cornell.edu References: <38281B7A.CBBCA44A@cs.kuleuven.ac.be> Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 81482b5b4ea0105d68a71bf2f2bc8576 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit > Did you measure it in a variety of places? It varies locally and, I > think, the variations over the human face are critical to realism. Cheeks > have peach fuzz, noses and bald pates can be shiny, lips are krinkly, > eyelids are...different again, at least on many Caucasian heads and faces. Frankly, we were tickled just to get any data at all: as far as I can find out, these are the first full directional measurements of the reflectance of living human skin, with the exception of some ultraviolet measurements by some dermatologists at Lodz, Poland a few years back. Data on cadaver skin is easier to come by, but obviously suffers changes in reflectance during the preparation process, and grad students just don't seem as dedicated as they used to be... We measured the forehead, because: o We figured it was pretty constant over its area, which we need for our technique. o Its curvature covers more than a 90-degree range of angles, which we also need. o It's strictly convex, which avoids the problem of secondary reflections. o It's relatively easy to attach geometric calibration targets rigidly, by means of a modified hat. o It is pretty non-deformable, so we could take a series of images and be confident that its geometry remains constant. o It didn't involve removing any clothing. > This is part of why I view synthesis of human faces to be the hardest > problem in CG--mostly because humans are so exquisitely sensitive to the > nuances in human faces. Not like terrains and other natural phenomena > where we're amazingly undiscriminating... Yup, I agree. But we decided to tackle the directional characteristics of reflectance first, as no one had done that. And even when you account for the color variations via a painted or scanned texture map, it doesn't look like skin. We thought that even a constant directionality would get us a bit closer to reality, if it is valid for at least part of the face . Stephen H. Westin Research Project Leader Program of Computer Graphics Cornell University westin@graphics.cornell.edu 607 255 9080 (VOX) 607 255 0806 (FAX) From Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id RAA12075; Tue, 30 Nov 1999 17:38:01 +0100 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id RAA03510 for globillum-imag-outgoing; Tue, 30 Nov 1999 17:29:06 +0100 (MET) From: eric.haines@autodesk.com Message-ID: <19879C753611D3119DAB0008C7A4C0C102C0B2D4@hqmsgsrf04.autodesk.com> To: globillum@imag.fr Subject: Fantasy Graphics League Date: Tue, 30 Nov 1999 08:28:30 -0800 MIME-Version: 1.0 X-Mailer: Internet Mail Service (5.5.2448.0) Content-Type: text/plain; charset=iso-8859-1; format=flowed Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 4bf98aacffe6fd3da5b479a27c0acbd8 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit It being just a month and a half until the SIGGRAPH 2000 (S2K) paper deadline, we've decided to create a little contest to while away a few spare moments. For your bemusement, the Fantasy Graphics League website is up and running at: http://www.realtimerendering.com/fgl/ Enjoy, Eric p.s. be patient after you hit the "Enter The Contest" link, the costframe.htm page sometimes takes awhile to load (blame the imminent collapse of the Internet). From Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id SAA20236; Mon, 6 Dec 1999 18:06:05 +0100 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id RAA04535 for globillum-imag-outgoing; Mon, 6 Dec 1999 17:57:34 +0100 (MET) Date: Mon, 6 Dec 1999 11:57:15 -0500 (EST) Message-Id: <199912061657.LAA04509@bach.Graphics.Cornell.EDU> From: "Stephen H. Westin" To: globillum@imag.fr Subject: Re: Skin BRDF data now available Reply-to: westin@graphics.cornell.edu Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 9626517d5c60af00b3ea5f012a7c900a X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit I have corrected the following errors in the Web posting of these data: o Both links to "coefficients" files pointed to the same file o The color correction matrix given had an incorrect scale factor of approximately 1/338 applied. This was corrected both in the directly- accessible files of coefficients, and in the files contained in the tar archives. Thanks again to Kevin Bjorke for pointing out the errors. -- -Stephen H. Westin Any information or opinions in this message are mine: they do not represent the position of Cornell University or any of its sponsors. From Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id RAA26628; Mon, 20 Dec 1999 17:42:28 +0100 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id RAA05263 for globillum-imag-outgoing; Mon, 20 Dec 1999 17:37:27 +0100 (MET) Message-ID: <385E5B3E.941D9456@cs.kuleuven.ac.be> Date: Mon, 20 Dec 1999 17:37:18 +0100 From: Philippe Bekaert Organization: K.U.Leuven - department of computer science X-Mailer: Mozilla 4.61C-SGI [en] (X11; I; IRIX 6.5 IP32) X-Accept-Language: en MIME-Version: 1.0 To: "globillum@imag.fr" Subject: dissertation online Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 8bit Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: da4c96807a7d265100d5fcbef7b502db X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Dear all, Last tuesday, I succesfully defended my PhD dissertation on "hierarchical and stochastic algorithms for radiosity". The dissertation text is available online on the following locations: http://www.cs.kuleuven.ac.be/cwis/research/graphics/CGRG.PUBLICATIONS/PHBPHD/ ftp://ftp.cs.kuleuven.ac.be/pub/graphics/thesis/bekaert/ The abstract is included below. Philippe Bekaert. Computer Graphics Research Group Department of Computer Science - K.U.Leuven Celestijnenlaan, 200A - B3001 Heverlee - Belgium Tel: ++32 16 32 76 67 Fax: ++32 16 32 79 96 http://www.cs.kuleuven.ac.be/cwis/research/graphics/graphics-E.shtml -------------------------------------------------------------------- Hierarchical and Stochastic Algorithms for Radiosity The radiosity method is a physically based method to compute the illumination in a virtual environment with diffuse (matte) surfaces. It allows to generate very realistic images of such environments by computer, and it is suitable for quantitative predictions of the illumination. In the radiosity method, a number of simplifying assumptions are made that can however lead to certain image artifacts. In this dissertation, the numerical error introduced by these assumptions is analysed. The analysis allows to propose new algorithms in which this error, the discretisation error, is efficiently controlled during the computations by means of hierarchical refinement. The radiosity method also requires the solution of very large non-sparse systems of linear equations (about 100,000 equations is common). Moreover, the coefficients of these systems are non-trivial four-dimensional integrals. The main part of this dissertation is devoted to an in-depth study of how the Monte Carlo method can be applied in this context. The Monte Carlo method is suitable for reliable computation of the coefficients of the systems of equations. It also leads to algorithms that do not require explicit computation and storage of these coefficients. A systematic overview of such algorithms is presented. Previously proposed algorithms of this type are compared and some new algorithms are developed. Next, the application of several variance-reduction techniques is described, and the use of low-discrepancy sampling in this context is discussed. Finally, new ways to incorporate higher-order radiosity approximations and hierarchical refinement are proposed. The resulting Monte Carlo radiosity algorithms do not only appear to be more reliable, but also often lead more rapidly to usable images than their deterministic counterparts. They require significantly less computer storage, and they are more user friendly. It is expected that these algorithms will stimulate the use of the radiosity method in a wide spectrum of applications. Keywords: computer graphics, physically based image synthesis, illumination simulations, radiosity method, Galerkin method, hierarchical refinement, Monte Carlo method, quasi-Monte Carlo, form factor computation, systems of linear algebraic equations. From Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id WAA30113; Thu, 23 Dec 1999 22:55:54 +0100 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id WAA07468 for globillum-imag-outgoing; Thu, 23 Dec 1999 22:51:25 +0100 (MET) Date: Thu, 23 Dec 1999 16:49:49 -0500 (EST) Message-Id: <199912232149.QAA24430@bach.Graphics.Cornell.EDU> From: "Stephen H. Westin" To: globillum@imag.fr cc: jstam@aw.sgi.com, mmccool@mud.cgl.uwaterloo.ca, okk@gin.keldysh.ru Subject: Skin BRDF data now corrected Reply-to: westin@graphics.cornell.edu Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 23ac363178038f46de616073f5a403cb X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit I have found out (partly through the feedback of a user) that the color correction matrices supplied with our BRDF data are wrong. Here is the correct matrix: 1.0633 0.3820 -0.4453 -0.2981 1.6677 -0.3695 -1.3223 -0.4463 2.7686 You may: 1. Use this matrix in place of the one supplied in the "coefficients" file, 2. Download a new copy of the relevant files (steve-face-981211-coefficients and mahesh-981228-coefficients) from , or 3. Download the whole dataset again from the URL above. Sorry for the mistake. Stephen H. Westin Research Project Leader Program of Computer Graphics Cornell University westin@graphics.cornell.edu 607 255 9080 (VOX) 607 255 0806 (FAX) From Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id SAA31728; Wed, 12 Jan 2000 18:43:04 +0100 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id SAA10588 for globillum-imag-outgoing; Wed, 12 Jan 2000 18:37:58 +0100 (MET) Message-ID: <000f01bf5d23$2c3e9280$b29c42d8@byheart> Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: 00/01/15 Release of RADBIB and GITHESIS Date: Wed, 12 Jan 2000 09:33:16 -0800 Organization: byHeartConsultants Limited MIME-Version: 1.0 Content-Type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 5.00.2919.6600 X-MimeOLE: Produced By Microsoft MimeOLE V5.00.2919.6600 Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 337e66c12c9e898587ce9c883cc0d824 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit
ANNOUNCE: 00/01/15 Release of RADBIB.BIB
----------------------------------------
RADBIB is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. It currently includes 1,673 references -- 2 new additions since its 99/11/26 release as RADBIB99.
 
This bibliography is available in BibTex format as RADBIB.BIB (with a release date of January 15, 2000) from:
 
 
in the Resources section.
 
Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 199 references to radiosity and global illumination theses -- 1 new addition since the 99/08/01 release.
 
Financial support for the maintenance of these bibliographies has been provided by ACM SIGGRAPH Special Projects and byHeart Consultants Limited.
 
Ian Ashdown, P. Eng., LC
Vice President
byHeart Consultants Limited
http://www.helios32.com
PS - yes, it is only January 12th. I put new batteries in my calendar and it is running a bit fast!
 
From Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id DAA31657; Wed, 19 Jan 2000 03:54:38 +0100 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id DAA06923 for globillum-imag-outgoing; Wed, 19 Jan 2000 03:48:24 +0100 (MET) Message-ID: <388525F3.51A943D6@graphics.lcs.mit.edu> Date: Tue, 18 Jan 2000 21:48:19 -0500 From: Fredo Durand X-Mailer: Mozilla 4.7C-SGI [en] (X11; I; IRIX 6.5 IP32) X-Accept-Language: fr, en MIME-Version: 1.0 To: globillum@imag.fr Subject: thesis and survey on visibility Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 8bit Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 141bf90c8baeb31d9ffe7f0accce948c X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hi, My thesis is available on the web: http://graphics.lcs.mit.edu/~fredo/THESE/ It deals with 3D visibility, and also contains a huge survey of visibility techniques in different fields such as graphics, vision or robotics. Abstract: Visibility problems are central to many computer graphics applications. The most common examples include hidden-part removal for view computation, shadow boundaries, mutual visibility of pairs of points, etc. In this document, we first present a theoretical study of 3D visibility properties in the space of light rays. We group rays that see the same object; this defines the 3D visibility complex. The boundaries of these groups of rays correspond to the visual events of the scene (limits of shadows, disappearance of an object when the viewpoint is moved, etc.). We simplify this structure into a graph in line-space which we call the visibility skeleton. Visual events are the arcs of this graph, and our construction algorithm avoids the intricate treatment of the corresponding 1D sets of lines. We simply compute the extremities (lines with 0 degrees of freedom) of these sets, and we topologically deduce the visual events using a catalogue of adjacencies. Our implementation shows that the skeleton is more general, more efficient and more robust than previous techniques. Applied to lighting simulation, the visibility skeleton permits more accurate and more rapid simulations. We have also developed an occlusion culling preprocess for the display of very complex scenes. We compute the set of potentially visible objects with respect to a volumetric region. In this context, our method is the first which handles the cumulative occlusion due to multiple blockers. Our occlusion tests are performed in planes using extended projections, which makes them simple, efficient and robust. In the second part of the document, we present a vast survey of work related to visibility in various domains. From Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id RAA27009; Thu, 27 Jan 2000 17:29:38 +0100 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id RAA03254 for globillum-imag-outgoing; Thu, 27 Jan 2000 17:20:25 +0100 (MET) Message-ID: <38907034.881D35F9@graphics.lcs.mit.edu> Date: Thu, 27 Jan 2000 11:20:04 -0500 From: Fredo Durand X-Mailer: Mozilla 4.7C-SGI [en] (X11; I; IRIX 6.5 IP32) X-Accept-Language: fr, en MIME-Version: 1.0 To: globillum@imag.fr Subject: page of links and new graphics search engine Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 8bit Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 1714b76ffdc4c58a0ac31f4ac7d357b0 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hi everybody, To fight the post siggraph deadline blues, I have updated my page of web links to graphics related pages : http://www.graphics.lcs.mit.edu/~fredo/Book/index.html In particular the researcher and lab sections have been checked and updated. I also installed a search engine which recursively digs the web starting from my pages of links. Since I allow only 2 hops, this means that it is more likely to index pages really related to graphics (but of course some unrelated pages are indexed as well). Enjoy! I'm now in the process of cleaning up my "other index", "code" and "data" pages. Unfortunately I cannot maintain the "compagny", "gallery" and thematic pages, it just takes too much time. I'd be happy to receive feedback, any idea of improvement (if it doesn't take me too long!), missing or wrong links (What? You're such an important researcher in graphics and I have no link on you! I'm so ashamed, I'll be happy to oblige and reference you!), etc. cheers Fredo http://www.graphics.lcs.mit.edu/~fredo From Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id QAA03027; Tue, 1 Feb 2000 16:06:18 +0100 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id PAA29180 for globillum-imag-outgoing; Tue, 1 Feb 2000 15:55:42 +0100 (MET) Message-ID: From: DENIEL Jean Marc To: globillum@imag.fr Subject: Spectral imaging sensors Date: Tue, 1 Feb 2000 15:51:52 +0100 MIME-Version: 1.0 X-Mailer: Internet Mail Service (5.5.2448.0) Content-Type: text/plain; charset=iso-8859-1; format=flowed Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from quoted-printable to 8bit by imag.imag.fr id PAA29173 Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 9cd86c4e7313c83d9ae661725c162876 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 We're looking for some informations about imaging sensors like cameras that could deliver some spectral information instead of RGB or B/W levels. Has someone heard baout this ? Thank you in advance. JM Jean-Marc Deniel CSTB - division Eclairage et Colorimétrie 11, rue Henri Picherit BP 82341 44323 NANTES Cedex 3 Tel: 02.40.37.20.15 Fax: 02.40.37.20.40 From Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id RAA08984; Tue, 1 Feb 2000 17:46:32 +0100 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id RAA09357 for globillum-imag-outgoing; Tue, 1 Feb 2000 17:41:04 +0100 (MET) Date: Tue, 1 Feb 2000 11:40:45 -0500 (EST) Message-Id: <200002011640.LAA02820@bach.Graphics.Cornell.EDU> From: "Stephen H. Westin" To: globillum@imag.fr In-reply-to: (message from DENIEL Jean Marc on Tue, 1 Feb 2000 15:51:52 +0100) Subject: Re: Spectral imaging sensors Reply-to: westin@graphics.cornell.edu References: Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 5c17030b40b15bf85229a1bafde1056e X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit > From: DENIEL Jean Marc > Date: Tue, 1 Feb 2000 15:51:52 +0100 > We're looking for some informations about imaging sensors like cameras that > could deliver > some spectral information instead of RGB or B/W levels. > Has someone heard baout this ? > Thank you in advance. There are two basic approaches to this. Either you take repeated images with a series of narrowband filters, or you use a diffraction grating in the camera to turn a full 2D image sensor into a line-scan spectrometer. The series-of-filters approach is much easier if you use a tunable narrow-band filter, such as that from Cambridge Research, Inc. (CRI). David Brainard at UCSB has done this; see for details. A company called "Spectral Imaging Systems" seems to have a vaguely similar system that works with some sort of interferometric techique that I suspect is equivalent. There are a number of companies that turned up on an AllTheWeb search on spectral imaging. The diffraction-grating approach has been implemented by a company named Wintriss . I suspect others have done the same. The disadvantage to both these techniques is that they are not instantaneous: your subject must remain completely stationary for some significant period of time (seconds to minutes). Stephen H. Westin Research Project Leader Program of Computer Graphics Cornell University westin@graphics.cornell.edu 607 255 9080 (VOX) 607 255 0806 (FAX) From Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id TAA14221; Tue, 1 Feb 2000 19:10:09 +0100 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id TAA16200 for globillum-imag-outgoing; Tue, 1 Feb 2000 19:05:28 +0100 (MET) From: hertjwr@us.ibm.com X-Lotus-FromDomain: IBMUS To: DENIEL Jean Marc cc: globillum@imag.fr Message-ID: <85256878.00635384.00@D51MTA03.pok.ibm.com> Date: Tue, 1 Feb 2000 13:05:02 -0500 Subject: Re: Spectral imaging sensors Mime-Version: 1.0 Content-type: text/plain; charset=iso-8859-1; format=flowed Content-Disposition: inline Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from quoted-printable to 8bit by imag.imag.fr id TAA16197 Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 09db7b38890caa8717c849e022d38336 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Miyake's lab in at Chiba University has done a lot of work in multispectral sensing. At least one of their papers is on line Goniospectral imaging of 3D objects Color Imaging Conference , Scottsdale, AZ (1998.11) http://www.icsd6.tj.chiba-u.ac.jp/~haneishi/color.html -- Holly __________________________ Holly Rushmeier , holly@watson.ibm.com, (914)784-7252 IBM TJ Watson Research Center, 30 Saw Mill River Road, Hawthorne, NY 10532, USA DENIEL Jean Marc @imag.imag.fr on 02/01/2000 09:51:52 AM Sent by: owner-globillum@imag.imag.fr To: globillum@imag.fr cc: Subject: Spectral imaging sensors We're looking for some informations about imaging sensors like cameras that could deliver some spectral information instead of RGB or B/W levels. Has someone heard baout this ? Thank you in advance. JM Jean-Marc Deniel CSTB - division Eclairage et Colorimétrie 11, rue Henri Picherit BP 82341 44323 NANTES Cedex 3 Tel: 02.40.37.20.15 Fax: 02.40.37.20.40 From Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id DAA02956; Wed, 2 Feb 2000 03:58:51 +0100 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id DAA22237 for globillum-imag-outgoing; Wed, 2 Feb 2000 03:55:05 +0100 (MET) Message-ID: <002501bf6d27$fa0ef6a0$879c42d8@byheart> Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: deniel@cstb.fr Cc: globillum@imag.fr Subject: Re: Spectral imaging sensors Date: Tue, 1 Feb 2000 18:48:20 -0800 Organization: byHeartConsultants Limited MIME-Version: 1.0 Content-Type: text/plain; charset=iso-8859-1; format=flowed Content-Transfer-Encoding: 8bit X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 5.00.2919.6600 X-MimeOLE: Produced By Microsoft MimeOLE V5.00.2919.6600 Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: e3679aa15d9d682c2856eb05bbd9c80e X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 > We're looking for some informations about imaging sensors like cameras that > could deliver some spectral information instead of RGB or B/W levels. > Has someone heard baout this ? > Thank you in advance. > Searching the Web for the keyword "hyperspectral" should give you at least 5,000 useful hits. It's a common technique for remote sensing and satellite surveillance. Ian Ashdown, P. Eng., LC Vice President byHeart Consultants Limited http://www.helios32.com From Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id IAA08009; Wed, 2 Feb 2000 08:32:18 +0100 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id IAA03430 for globillum-imag-outgoing; Wed, 2 Feb 2000 08:31:02 +0100 (MET) Message-ID: From: DENIEL Jean Marc To: "'globillum@imag.fr'" Subject: High luminance displays Date: Wed, 2 Feb 2000 08:27:56 +0100 MIME-Version: 1.0 X-Mailer: Internet Mail Service (5.5.2448.0) Content-Type: text/plain; charset=iso-8859-1; format=flowed Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from quoted-printable to 8bit by imag.imag.fr id IAA03424 Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 361e0e86797aa5d014869acae0db0403 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Thank you for your numerous answers about spectral sensors. These will help us a lot. We're interested too in hight luminance displays. Does anyone have infos about such peripherals ? JM Jean-Marc Deniel CSTB - division Eclairage et Colorimétrie 11, rue Henri Picherit BP 82341 44323 NANTES Cedex 3 Tel: 02.40.37.20.15 Fax: 02.40.37.20.40 From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id OAA25134; Tue, 29 Feb 2000 14:12:21 +0100 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id OAA10337 for globillum-imag-outgoing; Tue, 29 Feb 2000 14:00:04 +0100 (MET) Message-ID: <001101bf82b4$6a229a40$961dc2a5@nm.cau.ac.kr> From: "Sungye Kim" To: globillum@imag.fr Subject: Tone reproduction Date: Tue, 29 Feb 2000 21:56:37 +0900 MIME-Version: 1.0 Content-Type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 5.00.2919.6600 X-MimeOLE: Produced By Microsoft MimeOLE V5.00.2919.6600 Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 1454364c80391b31971c80409beb7697 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit
Hello..
I'm.. a student at Chung-Ang Univ. in Seoul, Korea.
My major is Computer Graphics, and
during my master period, I have interested in Global Illumination and Radiosity.

Recently, I have made a study of the Tone reproduction.
And then, I am implementing the method that was proposed in 1991 and publicated in 1993 by Tumblin and Rushmeier.
In theier paper, I don't know how I can calculate the factor, expected value, E{log10(L_in)}.
If you are OK, I want to get your help.
 
From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id PAA28972; Tue, 29 Feb 2000 15:42:18 +0100 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id PAA20703 for globillum-imag-outgoing; Tue, 29 Feb 2000 15:35:47 +0100 (MET) Message-ID: <38BBD919.E84EBB28@graphics.lcs.mit.edu> Date: Tue, 29 Feb 2000 09:35:05 -0500 From: Fredo Durand X-Mailer: Mozilla 4.7C-SGI [en] (X11; I; IRIX 6.5 IP32) X-Accept-Language: fr, en MIME-Version: 1.0 To: Sungye Kim CC: globillum@imag.fr Subject: Re: Tone reproduction References: <001101bf82b4$6a229a40$961dc2a5@nm.cau.ac.kr> Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 8bit Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: a32c2ca6ed0bdc2518f2e066891ddf20 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 I suggest you look in the appendix of Jack Tumblin's thesis, where he presents a version of the operator which is easier to understand (and which removes a couple of artefacts): http://www.cc.gatech.edu/gvu/people/jack.tumblin/ Fredo -- Fredo Durand, MIT-LCS Graphics Group NE43-255, Cambridge, MA 02139 phone : (617) 253 7223 fax : (617) 253 4640 http://graphics.lcs.mit.edu/~fredo/ From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id RAA01927; Tue, 29 Feb 2000 17:30:32 +0100 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id RAA02578 for globillum-imag-outgoing; Tue, 29 Feb 2000 17:25:11 +0100 (MET) Message-ID: <38BBF2C3.7073BB24@graphics.cornell.edu> Date: Tue, 29 Feb 2000 11:24:35 -0500 From: Jack John Erwin Tumblin X-Mailer: Mozilla 4.7 [en] (WinNT; U) X-Accept-Language: en MIME-Version: 1.0 To: Fredo Durand , Sungye Kim , "globillum@imag.fr" Subject: Re: Tone reproduction References: <001101bf82b4$6a229a40$961dc2a5@nm.cau.ac.kr> <38BBD919.E84EBB28@graphics.lcs.mit.edu> Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 8bit Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: c16275e479dbb974b9baaafbd16de81a X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hello Sungye Kim and Fredo Durand! To answer the original question from Sungye Kim, the term E{log10(L_in)} is just the 'expected value', also known as the mean or the average, of the logarithm of each pixel. To compute it, find the logarithm of each pixel's luminance, add all of them together, then divide the total by the number of pixels. Fredo Durand is correct; an improved, less awkward version of this tone reproduction operator appears in an appendix to my dissertation, but it was first published in a paper last year. This paper includes a survey of other tone reproduction operators you might find useful: @Article{THG:1999:hicont, author = "Tumblin, J. and Hodgins, J. and Guenter, B.", title = "Two Methods for Display of High Contrast Images", journal = "ACM Transactions On Graphics", year = "1999", volume = "18", number = "1", pages = "56--94", month = jan, } I'm sorry to say that my website at Ga Tech still contains only a draft of my dissertation. The appendix is probably correct, but the main text is missing some corrections and improvements I made later. I hope to get the final version on-line soon. Thank you both for your interest in my work! Regards, -Jack Tumblin Fredo Durand wrote: > I suggest you look in the appendix of Jack Tumblin's thesis, where he > presents a version of the operator which is easier to understand (and > which removes a couple of artefacts): > http://www.cc.gatech.edu/gvu/people/jack.tumblin/ > > Fredo > > -- > Fredo Durand, MIT-LCS Graphics Group > NE43-255, Cambridge, MA 02139 > phone : (617) 253 7223 fax : (617) 253 4640 > http://graphics.lcs.mit.edu/~fredo/ From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id MAA11425; Wed, 15 Mar 2000 12:55:58 +0100 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id MAA17039 for globillum-imag-outgoing; Wed, 15 Mar 2000 12:39:58 +0100 (MET) Message-ID: <8815647C7041D111A3010060B06BE1C0C4DF03@elvis.lightwork> From: Neil Gatenby To: globillum@imag.fr Subject: FW: CCD v. Cell Photometry Date: Wed, 15 Mar 2000 10:03:18 -0000 MIME-Version: 1.0 X-Mailer: Internet Mail Service (5.5.2650.21) Content-Type: text/plain; charset=windows-1252; format=flowed Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 25cd3ce71c309776e9daf47524a24565 X-Mozilla-Status: 9001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit This thread, starting on sci.engr.lighting, may be of interest to some in this group Neil <> Message-ID: From: Martin Moore To: Subject: Re: CCD v. Cell Photometry Date: Wed, 15 Mar 2000 03:06:10 -0000 MIME-Version: 1.0 X-Mailer: Internet Mail Service (5.5.2650.21) Content-Type: text/plain; charset="iso-8859-1" How do CCD and cell photometry compare? The otherwise excellent recently (1998) published *Handbook of Applied Photometry* gives CCD photometry rather short shrift - a couple of paragraphs in the penultimate section 11.4.3 of the book, including:- **Two dimensional charge-coupled device (CCD) cameras have already high enough dynamic range and low enough cross-talk to be used for photometric purposes. Due to non-uniform spatial sensitivity and local differences in the spectral sensitivity the filter correction of such a photometer is still somewhat poorer than that of a traditional illuminance or luminance meter. ** CCD photometry seems excellent for relative photometric measurements in a lab environment. How good (accurate) is CCD for absolute photometric measurements? Are CCD photometrics endorsed/sanctioned by IESNA, ANSI, etc.? In practice, can you do reliable CCD photometry in the field? Martin Moore From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id QAA06148; Fri, 17 Mar 2000 16:44:10 +0100 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id QAA12751 for globillum-imag-outgoing; Fri, 17 Mar 2000 16:30:52 +0100 (MET) Date: Fri, 17 Mar 2000 16:30:41 +0100 From: Nicolas Holzschuch To: globillum@imag.fr Subject: Higher order wavelets Message-ID: <20000317163041.A3239@yutz.loria.fr> Mime-Version: 1.0 Content-Type: text/plain; charset=iso-8859-1; format=flowed Content-Transfer-Encoding: 8bit X-Mailer: Mutt 1.0i Organisation: LORIA/INRIA Lorraine Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 23e54fe87f4cc7816d20aa9933f9642f X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hello fellow globillumers, I would like to advertise our paper "A novel approach makes higher order wavelets really efficient for radiosity", by François Cuny, Laurent Alonso and Nicolas Holzschuch. It will be at the Eurographics 2000 conference. In the meantime, it can also be downloaded at http://www.loria.fr/~holzschu/Publications/paper20.pdf Greetings, Nicolas Holzschuch ISA research team, INRIA Lorraine From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id SAA20177; Sat, 29 Apr 2000 18:04:54 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id RAA28871 for globillum-imag-outgoing; Sat, 29 Apr 2000 17:43:32 +0200 (MET DST) Message-ID: <000901bfb1f1$b4bbbb60$8f9c42d8@byheart> Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: May 1, 2000 Release of RADBIB Global Illumination Bibliography Date: Sat, 29 Apr 2000 08:43:44 -0700 Organization: byHeartConsultants Limited MIME-Version: 1.0 Content-Type: text/plain; charset=iso-8859-1; format=flowed Content-Transfer-Encoding: 8bit X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 5.00.2919.6600 X-MimeOLE: Produced By Microsoft MimeOLE V5.00.2919.6600 Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 621f6c186112094a2fb3bd80f1966aae X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 ANNOUNCE: 00/05/01 Release of RADBIB.BIB ---------------------------------------- RADBIB is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. It currently includes 1,723 references -- 11 new additions since its 00/04/01 release. This bibliography is available in BibTex format as RADBIB.BIB (with a release date of May 1, 2000) from: http://www.helios32.com Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 203 references to radiosity and global illumination theses -- no new additions since the 00/04/01 release. Financial support for the maintenance of these bibliographies has been provided by ACM SIGGRAPH Special Projects and byHeart Consultants Limited. Ian Ashdown, P. Eng., LC Vice President byHeart Consultants Limited http://www.helios32.com From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id DAA27496; Thu, 4 May 2000 03:46:30 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id DAA02901 for globillum-imag-outgoing; Thu, 4 May 2000 03:44:19 +0200 (MET DST) Message-ID: <002901bfb56a$46daf9e0$961dc2a5@nm.cau.ac.kr> From: "Sungye Kim" To: "globillum" Subject: Fluid Spattering simulation Date: Thu, 4 May 2000 10:44:24 +0900 MIME-Version: 1.0 Content-Type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 5.00.2919.6600 X-MIMEOLE: Produced By Microsoft MimeOLE V5.00.2919.6600 Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 0d59e439819790f367758b1da0b0201d X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit
Hello fellow globillumers,
We're looking for some informations about water(fluid) spattering or splashing simulation.
 
Has someone heard about this?
 
Thank you in advance.
 
 
Kim
 
=====================================================================
 
Sungye Kim
 
221 Huksuk-Dong, DongJak-Ku, Seoul, Korea 
Dept. of Computer Science & Engineering Chung Ang Univ.
Computer Graphics Lab.
 
Tel: +82-2-820-5411
Fax : +82-2-820-5301
From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id PAA13712; Thu, 4 May 2000 15:51:25 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id OAA17631 for globillum-imag-outgoing; Thu, 4 May 2000 14:59:02 +0200 (MET DST) From: hertjwr@us.ibm.com X-Lotus-FromDomain: IBMUS To: "Sungye Kim" cc: "globillum" Message-ID: <852568D5.004733C1.00@D51MTA03.pok.ibm.com> Date: Thu, 4 May 2000 08:57:42 -0400 Subject: Re: Fluid Spattering simulation Mime-Version: 1.0 Content-type: text/plain; charset=us-ascii; format=flowed Content-Disposition: inline Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 71af7a828825beec34d640339a369c99 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit For the dynamics of the water motion on example is the work at Georgia Tech: http://www.cc.gatech.edu/gvu/animation/Areas/secondary/water.html -- Holly __________________________ Holly Rushmeier , holly@watson.ibm.com, http://www.research.ibm.com/people/h/holly, (914)784-7252 IBM TJ Watson Research Center, 30 Saw Mill River Road, Hawthorne, NY 10532, USA "Sungye Kim" @imag.imag.fr on 05/03/2000 09:44:24 PM Sent by: owner-globillum@imag.imag.fr To: "globillum" cc: Subject: Fluid Spattering simulation Hello fellow globillumers, We're looking for some informations about water(fluid) spattering or splashing simulation. Has someone heard about this? Thank you in advance. Kim ===================================================================== Sungye Kim 221 Huksuk-Dong, DongJak-Ku, Seoul, Korea Dept. of Computer Science & Engineering Chung Ang Univ. Computer Graphics Lab. Tel: +82-2-820-5411 Fax : +82-2-820-5301 From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id RAA18326; Thu, 4 May 2000 17:34:56 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id RAA17968 for globillum-imag-outgoing; Thu, 4 May 2000 17:11:52 +0200 (MET DST) From: Brian Curless MIME-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 8bit Message-ID: <14609.37628.23130.334837@breve.cs.washington.edu> Date: Thu, 4 May 2000 08:10:52 -0700 (PDT) To: hertjwr@us.ibm.com Cc: "Sungye Kim" , "globillum" Subject: Re: Fluid Spattering simulation In-Reply-To: <852568D5.004733C1.00@D51MTA03.pok.ibm.com> References: <852568D5.004733C1.00@D51MTA03.pok.ibm.com> X-Mailer: VM 6.75 under Emacs 19.34.1 Reply-To: curless@cs.washington.edu Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: b5c101b7f2a62d99ebc1ac9a911c16cb X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 A company called Arete' Image Software has some amazing fluid simulations: http://www.areteis.com In particular: http://www.areteis.com/fillbox.mov Brian ---- Brian Curless Assistant Professor Graphics and Imaging Laboratory Dept. of Computer Science & Engineering Office: (206) 685-3796 University of Washington Fax: (206) 543-2969 Sieg Hall, Box 352350 Email: curless@cs.washington.edu Seattle, Washington 98195-2350 http://www.cs.washington.edu/homes/curless -----Original message----- From: hertjwr@us.ibm.com To: "Sungye Kim" Subject: Re: Fluid Spattering simulation Date: Thu, 4 May 2000 08:57:42 -0400 cc: "globillum" For the dynamics of the water motion on example is the work at Georgia Tech: http://www.cc.gatech.edu/gvu/animation/Areas/secondary/water.html -- Holly __________________________ Holly Rushmeier , holly@watson.ibm.com, http://www.research.ibm.com/people/h/holly, (914)784-7252 IBM TJ Watson Research Center, 30 Saw Mill River Road, Hawthorne, NY 10532, USA "Sungye Kim" @imag.imag.fr on 05/03/2000 09:44:24 PM Sent by: owner-globillum@imag.imag.fr To: "globillum" cc: Subject: Fluid Spattering simulation Hello fellow globillumers, We're looking for some informations about water(fluid) spattering or splashing simulation. Has someone heard about this? Thank you in advance. Kim ===================================================================== Sungye Kim 221 Huksuk-Dong, DongJak-Ku, Seoul, Korea Dept. of Computer Science & Engineering Chung Ang Univ. Computer Graphics Lab. Tel: +82-2-820-5411 Fax : +82-2-820-5301 From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id UAA28354; Thu, 4 May 2000 20:47:09 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id UAA06802 for globillum-imag-outgoing; Thu, 4 May 2000 20:40:04 +0200 (MET DST) Date: Thu, 4 May 2000 08:42:27 -0700 From: Rasmus Tamstorf X-Sender: tamstorf@bacon.fas.fa.disney.com To: Sungye Kim cc: globillum Subject: Re: Fluid Spattering simulation In-Reply-To: <002901bfb56a$46daf9e0$961dc2a5@nm.cau.ac.kr> Message-Id: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII; format=flowed Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: 8e0dd89558248f69609f92163b178daa X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit On Thu, 4 May 2000, Sungye Kim wrote: > Hello fellow globillumers, > > We're looking for some informations about water(fluid) spattering or splashing simulation. > > Has someone heard about this? There was a technical sketch last year at Siggraph about this : "Multifluid Finite Volume Navier-Stokes Solutions for Realistic Fluid Animation" by John A. Turner and Andre C. Mazzone @ Blue Sky Studios The simulation software was based on a system developed at Los Alamos and it definitely wasn't for the faint at heart, but it looked great :) Rasmus ----------------------------------------------------------------------------- Rasmus.Tamstorf@disney.com "A problem worthy of attack, Walt Disney Feature Animation proves its worth by hitting back" Kumbel ----------------------------------------------------------------------------- From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by www.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id VAA29215; Thu, 4 May 2000 21:19:13 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id VAA11040 for globillum-imag-outgoing; Thu, 4 May 2000 21:17:51 +0200 (MET DST) From: "A Gallardo" To: globillum@imag.fr Subject: RE: Fluid Spattering simulation Date: Thu, 4 May 2000 15:16:18 -0400 Message-ID: <000201bfb5fd$3953cd90$a5051a26@dellxps> MIME-Version: 1.0 Content-Type: text/plain; charset=iso-8859-1; format=flowed Content-Transfer-Encoding: 8bit X-Priority: 3 (Normal) X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook 8.5, Build 4.71.2377.0 X-MimeOLE: Produced By Microsoft MimeOLE V5.00.2919.6600 In-Reply-To: <002901bfb56a$46daf9e0$961dc2a5@nm.cau.ac.kr> Importance: Normal Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: ad103626f3f31f5377d862de1233a36b X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hi, Well I am not sure if you are after simulation or actual fluid dynamics. But there are several plugins that does this for commercial 3d applications. Realflow: http://www.realflow.com/ Splash! http://www.digimation.com/asp/products_stills.asp?product_id=88 Technical: http://www.ma.adfa.oz.au/Teaching/Subjects/VFD/VFD.html http://www.cs.indiana.edu/scicomp/cfd.html http://www.gbhap.com/journals/722/ http://vortex.mae.cornell.edu/ http://www.damtp.cam.ac.uk/user/fdl/ http://raphael.mit.edu/casl.html http://www.princeton.edu/~gasdyn/ Hope this helps. Also do use a search engine for more links. Regards, Arnold Gallardo Visual Content Creator http://members.toast.net/zeroneg1/Web/index.html > Hello fellow globillumers, > > We're looking for some informations about water(fluid) spattering or = > splashing simulation. > > Has someone heard about this? > > Thank you in advance. > > > Kim > > Sungye Kim > > 221 Huksuk-Dong, DongJak-Ku, Seoul, Korea=20 > Dept. of Computer Science & Engineering Chung Ang Univ. > Computer Graphics Lab. > > Tel: +82-2-820-5411 > Fax : +82-2-820-5301 From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by christl.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id RAA32299; Thu, 1 Jun 2000 17:40:42 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id RAA18773 for globillum-imag-outgoing; Thu, 1 Jun 2000 17:38:23 +0200 (MET DST) Message-ID: <001501bfcbdf$41dcd400$9f9c42d8@byheart> Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: Updated Radiosity and Global Illuminaion Bibliographies Date: Thu, 1 Jun 2000 08:37:10 -0700 Organization: byHeartConsultants Limited MIME-Version: 1.0 Content-Type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 5.00.2919.6600 X-MimeOLE: Produced By Microsoft MimeOLE V5.00.2919.6600 Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: ac4f003e94036b69108f2b4f997aa70c X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit
ANNOUNCE: 00/06/01 Release of RADBIB.BIB
----------------------------------------
RADBIB is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. It currently includes 1,734 references -- 11 new additions since its 00/05/01 release.
 
This bibliography is available in BibTex format as RADBIB.BIB (with a release date of June 1, 2000) from:
 
 
Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 203 references to radiosity and global illumination theses -- no new additions since the 00/04/01 release.
 
Financial support for the maintenance of these bibliographies has been provided by ACM SIGGRAPH Special Projects and byHeart Consultants Limited.
----
Ian Ashdown, P. Eng., LC
Vice President
byHeart Consultants Limited
http://www.helios32.com
From X-POP3-Rcpt: wp@christl Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by christl.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id RAA08680; Tue, 13 Jun 2000 17:19:02 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id RAA18697 for globillum-imag-outgoing; Tue, 13 Jun 2000 17:13:55 +0200 (MET DST) From: Brian Smits Message-Id: <200006131513.JAA169249@phoenix.cs.utah.edu> Subject: Test Scenes for Energy Transport To: globillum@imag.fr Date: Tue, 13 Jun 2000 09:13:41 -0600 (MDT) Cc: henrik@graphics.stanford.edu X-Mailer: ELM [version 2.5 PL2] MIME-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 8bit Sender: owner-globillum@imag.imag.fr Precedence: bulk X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hello, Henrik Wann Jensen and I have designed a set of scenes for testing energy transport. Our main goal was simplicity, both for the scenes, and for the type of transport tested by each scene. We wanted a set of very simple scenes that would exercise different aspects of rendering algorithms and make it fairly obvious when something wasn't working correctly. They range from the fairly simple (direct illumination without occluders) to the fairly challenging (reflection of a caustic from a secondary luminaire). We would appreciate any feedback you have. Global Illumination Test Scenes Brian Smits Henrik Wann Jensen University of Utah Stanford University University of Utah Technical Report UUCS-00-013 http://www.cs.utah.edu/~bes/papers/scenes Abstract: The global illumination community has discussed having a database of scenes that could be used to compare and validate different global illumination algorithms. We present a set of test scenes for global illumination algorithms and propose that they be the beginning of such a database. These scenes are designed to be as simple as possible and still test a particular aspect of energy transport. The scenes are available on a web site in a variety of formats, along with images and pixel radiance data. We feel that the simplicity and availability of the models will make it easier for the community to use them, and that the field will benefit from a standard set of scenes. Additionally, we discuss classes of models with analytic solutions. Tech Report: http://www.cs.utah.edu/~bes/papers/scenes/ Scene Repository: http://www.cs.utah.edu/~bes/graphics/scenes/ Thank you, Brian Smits bes@cs.utah.edu Henrik Wann Jensen henrik@graphics.stanford.edu From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by christl.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id EAA09831; Mon, 26 Jun 2000 04:15:47 +0200 Received: (from majordom@localhost) by imag.imag.fr (8.9.3/8.8.5) id EAA11349 for globillum-imag-outgoing; Mon, 26 Jun 2000 04:02:53 +0200 (MET DST) Message-ID: <000a01bfdf12$29bb2840$999c42d8@byheart> Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: globillum@imag.fr Subject: July 1st Release of RADBIB and GITHESIS Date: Sun, 25 Jun 2000 18:59:27 -0700 Organization: byHeartConsultants Limited MIME-Version: 1.0 Content-Type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 5.00.2919.6600 X-MimeOLE: Produced By Microsoft MimeOLE V5.00.2919.6600 Sender: owner-globillum@imag.imag.fr Precedence: bulk X-UIDL: k/]"!TeK!!0pV"!b%##! X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit
Yeah, I know -- July 1st is still a few days away. Consider this announcement a sneak preview!
 
- Ian Ashdown
 
ANNOUNCE: 00/07/01 Release of RADBIB.BIB
----------------------------------------
RADBIB is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. It currently includes 1,775 references -- 41 new additions since its 00/06/01 release.
 
This bibliography is available in BibTex format as RADBIB.BIB (with a release date of July 1, 2000) from:
 
  http://www.helios32.com (Resources section)
 
Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 224 references to radiosity and global illumination theses -- 21 new additions since the 00/06/01 release.
 
Financial support for the maintenance of these bibliographies has been provided by ACM SIGGRAPH Special Projects and byHeart Consultants Limited.
 
Ian Ashdown, P. Eng., LC, FIES
Vice President
byHeart Consultants Limited
http://www.helios32.com
From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id LAA30297; Tue, 4 Jul 2000 11:00:49 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id LAA06821; Tue, 4 Jul 2000 11:00:50 +0200 Received: from ebene.inrialpes.fr (ebene.inrialpes.fr [194.199.18.70]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id LAA06816 for ; Tue, 4 Jul 2000 11:00:45 +0200 Received: from safran.inrialpes.fr (safran.inrialpes.fr [194.199.26.1]) by ebene.inrialpes.fr (8.9.3/8.8.5) with ESMTP id LAA10713 for ; Tue, 4 Jul 2000 11:00:45 +0200 (MET DST) Received: from imag.fr (sesame [194.199.26.83]) by safran.inrialpes.fr (980427.SGI.8.8.8/8.8.5) with ESMTP id LAA28716 for ; Tue, 4 Jul 2000 11:00:45 +0200 (MDT) Sender: Francois.Sillion@imag.fr Message-Id: <3961A7BD.1837F1AF@imag.fr> Date: Tue, 04 Jul 2000 11:00:45 +0200 From: Francois Sillion Organization: iMAGIS - GRAVIR/IMAG INRIA X-Mailer: Mozilla 4.7C-SGI [en] (X11; I; IRIX 6.5 IP32) X-Accept-Language: en Mime-Version: 1.0 To: globillum@imag.fr Subject: globillum list: minor changes Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 8bit X-Loop: globillum@imag.fr X-Sequence: 1 Precedence: list X-UIDL: 2;c"!,d"#!KDL"!]B"#! X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hello all, This quick note is to inform you that we have changed our list manager here at IMAG. The address for the mailing list remains the same (mailto:globillum@imag.fr), but the robot now takes instructions at the following address: listes@imag.fr (try a message with 'help' as subject'. More interestingly, future messages will be archived and can be accessed through the www interface at http://listes.imag.fr. On that site you can customize your options and, for instance, request messages in "digest" mode. On the scientific side, last week saw the 11th EG workshop on rendering in Brno, Czeck republic. Unfortunately I spent most of the time in my bed fighting a bad virus, but from what little I saw it was a great success. Hopefully someone on this list will feel inspired to report on the workshop? -- >>>>> PLEASE NOTE OUR NEW ADDRESS ! EFFECTIVE October 4th, 1999 +------------------+--------------------------------------------------------+ | Francois SILLION | iMAGIS, Laboratoire GRAVIR/IMAG (CNRS,INRIA,INPG,UJF) | | ' | INRIA Rhone-Alpes, 655 Av de l'Europe, 38330 Montbonnot| | Senior researcher| France. Tel: +33 4 76 61 54 23 - Fax: +33 4 76 61 54 40| +------------------+--------+-----------------------------------------------+ | Francois.Sillion@imag.fr | http://www-imagis.imag.fr/~Francois.Sillion | +---------------------------+-----------------------------------------------+ From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id PAA12600; Wed, 5 Jul 2000 15:40:56 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id PAA10233; Wed, 5 Jul 2000 15:40:57 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id PAA10228 for ; Wed, 5 Jul 2000 15:40:52 +0200 Received: from mut.autodesk.com ([198.102.112.26]) by imag.imag.fr (8.9.3/8.8.5) with ESMTP id PAA05144 for ; Wed, 5 Jul 2000 15:40:52 +0200 (MET DST) Received: from autodesk.autodesk.com (autodesk.autodesk.com [144.111.216.101]) by mut.autodesk.com (8.9.3/8.9.3) with ESMTP id GAA03042 for ; Wed, 5 Jul 2000 06:40:43 -0700 (PDT) Received: from hqmsgsrf00.autodesk.com by autodesk.autodesk.com (8.8.8/4.4BSD) with ESMTP id GAA17990; Wed, 5 Jul 2000 06:40:30 -0700 (PDT) Received: by hqmsgsrf00.autodesk.com with Internet Mail Service (5.5.2448.0) id ; Wed, 5 Jul 2000 06:40:33 -0700 Message-Id: <19879C753611D3119DAB0008C7A4C0C10B7563@hqmsgsrf04.autodesk.com> From: eric.haines@autodesk.com To: globillum@imag.fr Subject: Object intersection, Gems repository update Date: Wed, 5 Jul 2000 06:40:40 -0700 Mime-Version: 1.0 X-Mailer: Internet Mail Service (5.5.2448.0) X-Loop: globillum@imag.fr X-Sequence: 2 Precedence: list Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: Rb6"!e]U!!~"J!!*cg!! X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit I have two bits of info for this list: A few of us have put together a page about references and resources for 3D object intersection tests. See http://www.realtimerendering.com/int/ I (finally) updated the Graphics Gems repository so that all code is linked directly from the HTML pages (vs. having to download the whole archive and search for it). The new pages are: http://www.acm.org/tog/GraphicsGems/category.html - by category http://www.acm.org/tog/GraphicsGems/authors.html - by author http://www.acm.org/tog/GraphicsGems/gems.html - by order of appearance Eric ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id QAA05392; Tue, 11 Jul 2000 16:43:37 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id QAA22046; Tue, 11 Jul 2000 16:43:35 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id QAA22041 for ; Tue, 11 Jul 2000 16:43:32 +0200 Received: from bach.Graphics.Cornell.EDU (bach.graphics.cornell.edu [128.84.247.50]) by imag.imag.fr (8.9.3/8.8.5) with ESMTP id QAA26741 for ; Tue, 11 Jul 2000 16:43:34 +0200 (MET DST) Received: from graphics.cornell.edu (bray.graphics.cornell.edu [128.84.247.212]) by bach.Graphics.Cornell.EDU (8.9.1/8.9.1) with ESMTP id KAA08221; Tue, 11 Jul 2000 10:43:27 -0400 (EDT) (envelope-from phil@graphics.cornell.edu) Message-Id: <396B3127.4CD2663A@graphics.cornell.edu> Date: Tue, 11 Jul 2000 10:37:27 -0400 From: Phil Dutre Organization: Program of Computer Graphics X-Mailer: Mozilla 4.73 [en] (WinNT; U) X-Accept-Language: en Mime-Version: 1.0 To: globillum@imag.fr Cc: graphics@Graphics.Cornell.EDU Subject: global illumination compendium X-Loop: globillum@imag.fr X-Sequence: 3 Precedence: list Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: ]j Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id QAA21899; Wed, 2 Aug 2000 16:26:40 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id QAA19555; Wed, 2 Aug 2000 16:26:39 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id QAA19550 for ; Wed, 2 Aug 2000 16:26:28 +0200 Received: from nut.autodesk.com (nut.autodesk.com [198.102.112.27]) by imag.imag.fr (8.9.3/8.8.5) with ESMTP id QAA28061 for ; Wed, 2 Aug 2000 16:26:33 +0200 (MET DST) From: eric.haines@autodesk.com Received: from autodesk.autodesk.com (autodesk.autodesk.com [144.111.216.101]) by nut.autodesk.com (8.9.3/8.9.3) with ESMTP id HAA13831 for ; Wed, 2 Aug 2000 07:26:13 -0700 (PDT) Received: from hqmsgsrf00.autodesk.com by autodesk.autodesk.com (8.8.8/4.4BSD) with ESMTP id HAA07343; Wed, 2 Aug 2000 07:26:10 -0700 (PDT) Received: by hqmsgsrf00.autodesk.com with Internet Mail Service (5.5.2448.0) id ; Wed, 2 Aug 2000 07:26:09 -0700 Message-Id: <19879C753611D3119DAB0008C7A4C0C10B7577@hqmsgsrf04.autodesk.com> To: globillum@imag.fr Subject: Nelson Max's European graphics tour Date: Wed, 2 Aug 2000 07:26:15 -0700 Mime-Version: 1.0 X-Mailer: Internet Mail Service (5.5.2448.0) X-Loop: globillum@imag.fr X-Sequence: 8 Precedence: list Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: AMA!!?@Q!!g;T"!7-g!! X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit [Nelson is having problems posting to globillum, and Francois is on vacation, so I'm posting this for Nelson; direct your comments to him. - Eric] From: "Nelson L. Max" In May and June, I attended five European conferences, including the Eurographics Workshop on Rendering (EGRW). I was required to submit a trip report to justify my salary at the conferences, and wrote an expanded description of the EGRW for the benefit of globillum. The complete report appears below, with the EGRW portion enclosed between two lines marked ******************. The papers I mentioned specifically represent my own personal interests, so please do not take offense if other important papers were not mentioned. The original purpose of the trip was to attend the two Eurographics workshops and the two Dagstuhl seminars. Since I could not afford multiple trips to Europe, I also arranged a U. C. Davis sabbatical at INRIA in Grenoble France, where I did research on Image-Based Rendering (IBR). Then, after I submitted the DOE trip proposal, I learned of the Non-Photorealistic Animation and Rendering Symposium, held in conjunction with the International Animated Film Festival, in Annecy, France, and got permission form INRIA to attend them also, although I received no DOE salary during these two events. I will describe these conferences briefly in consecutive order below, and then my research at INRIA. Dagstuhl Seminar 00211 on Scientific Visualization was organized by G.-P. Bonneau (IMAG, Grenoble), G. Nielson (Tempe), and F. Post (Delft). The main announced topics were Volume Modeling, Information Visualization, Flow Visualization, and Volume Visualization. Most participants gave 20-25 minute talks on their current research. The talk I remember best was by Robert van Liere on a citation analysis of the last ten years of the annual IEEE Visualization conferences. The most cited paper was "Texture Splats for 3D Vector and Scalar Fields Visualization", because it was in the intersection of the texture, volume visualization, and animation areas. The reason I remember it well is because I was a co-author of this paper, whose first author, Roger Crawfis, was a student of mine. My own talk was: Volume Rendering for Curvilinear and Unstructured Grids by Hardware-assisted Polyhedron Projection coauthored by myself, Peter Williams, Lawrence Livermore National Laboratory and Claudio Silva, AT&T Laboratory-Research Abstract: Hardware polygon rendering pipelines can be used together with hardware compositing to volume-render grids composed of convex polyhedral cells. This technique is described, together with the global sorting necessary for back-to-front compositing, and the modifications that must be made to handle curvilinear grids, whose faces may not be planar. Immediately following this seminar was the Eurographics/IEEE Symposium on Visualization, in Amsterdam, Holland. The topics included Large Datasets and Multi Resolution, Information Visualization, and Visualization Systems. I chaired the session on Volume and Flow Visualization. There was an interesting talk on "Fast Visualization of Special Relativistic Effects on Geometry and Illumination" by Daniel Weiskopf, in which he took advantage of hardware texture mapping and color matrices to generate the effects in real time, and one by David J. Holliday and Gregory M. Nielson "Progressive Volume Models for Rectilinear Data using Tetrahedral Coons Volumes, in which they solved the cracking problem between levels of a multi-resolution description by using piecewise rational Coons patches defined only in terms of the values of the function on the boundary of the triangle or tetrahedron. The next conference was the Non-Photorealistic Animation and Rendering Symposium, in Annecy, France. The talks centered mainly on the two fundamental problems in this area: (1) how to determine line detail for features like intersections, profiles, hatching, selectively inserted detail, or lines of curvature for shading, or stroke detail for "painterly rendering" of known color raster images, and (2) how to make these line or stroke features move smoothly and appropriately during animation. Though the problems were old ones, significant new progress was reported. The conference ended with a session of talks on animation, capped by a long, interesting, and entertaining talk by John Lasseter on the production of computer animation at Pixar. This conference was a part of the International Animated Film Festival, also in Annecy, and I spent the rest of the week, as well as some gaps between Symposium events, looking at animation. There were some interesting full length features from Japan, most of which were too violent or too difficult to understand for me or even my Japanese wife to follow. She explained that often an animated film will cap a year long series of Manga (adult comics) installments, and most of the audience is already familiar with the plot, so the compressed story does not bother them. An exception to this was the enjoyable "My neighbors, the Yamadas", which was about the humorous struggles of a Japanese family with young children, taken from a newspaper comic strip. The most memorable film of the festival, was with hand animated oil paintings, (slightly changed per frame while still wet), of Hemmingway's "The Old Man and the Sea", produced at the National Film Board of Canada. An educational part of the festival was a carefully selected historical series of 84 classic animated short films. Dagstuhl Seminar 00251, organized by M. Cohen (Microsoft Redmond), H. Müller (Dortmund), C. Puech (Grenoble), and H.-P. Seidel (Erlangen), was on Image Synthesis and Interactive 3D Graphics. There were several talks on improving the performance of Monte Carlo type radiosity or radiance calculations. In previews of Siggraph 2000 papers, Oliver Deussen showed artistic line drawings of trees, and Brian Curless described approximating and compressing as a surface texture the light reflected in all directions from a non-lambertian surface, as determined from multiple photographs. Karol Myszkowski showed a system for using human visible difference perception models to allocate computing resources in a global illumination calculation. My own talk was Illumination and Hierarchical Image-Based Rendering for Trees Abstract: I describe hierarchical Image-Based Rendering methods for trees, first done in software, and more recently in hardware. The idea is to prepare precomputed orthogonal views from the six + and - axis directions, including colors, normals, and depth at several layers, and then reproject them into a new viewing situation. These images are precomputed for all the different-sized objects in the hierarchical model of the tree, which are selected adaptively to give sufficient resolution for the current view. The visible surfaces are shaded using the color and (rotated) normal information in the reprojected view. By use of OpenGL features like texture mapping, alpha test, and color matrix transforms, the reprojection and shading can now be accomplished in hardware. I also compute multiple scattering of the light by reflection and transmission through the leaves, by treating the leaves as a volume distribution of infinitessimal planar fragments, whose areas and normals follow a distribution depending spatially only on the height above the ground. By discretizing the light flow directions into bins, the radiance transport equations turn into a system of ordinary differential equations in the height, which are solved by the method of invariant embedding. ************************ The last meeting I attended was the Eurographics Workshop on Rendering, for which I was on the Paper Committee, and also chaired a session. This annual workshop has become the main forum for new research results in rendering (second only to the Siggraph conference, which has space for only a few papers on this topic). Although it is traditionally held in Europe, participants come from all over the world. As in past years, many of the papers concerned global illumination. Mark Pauley, Thomas Kollig, and Alexander Keller showed how to extend Metropolis light transport to participating media. Frank Suykens and Yves Willems decreased the storage needed for photon maps by determining the required density in an importance prepass. If this density is already achieved in a region, the energy of excess photons reaching it is redistributed to nearby photons already in the map. Xavier Granier, George Drettakis, and Bruce Walter showed how to supplement finite element diffuse radiosity with particle tracing for glossy and specular effects like caustics, in a clustered hierarchical radiosity framework. Mark Stamminger, Jorg Haber, Hartmut Schirmacher, and Hans-Peter Seidel achieved a similar goal for interactive walkthroughs by supplementing a precomputed diffuse radiosity solution by view-dependent corrective textures, computed in parallel by tracing rays from the viewpoint in areas where specular effects are deemed necessary. For real-time performance, the texels in the texture are retained for a number of frames, determined by the predicted rate of change in the specular effects. Cyril Soler and Francois Sillion described a hierarchical clustered radiosity system based on repeatedly instantiating geometrical identical (or reasonably similar) structures for which transmittance and the bidirectional scattering phase function are precomputed using hardware rendering. For the primary application, to plant geometry where hierarchical instantiation is very appropriate, the phase function is the product of a radiance, depending only on the lighting direction, times a projected area depending only on the viewing direction. The philosophy is to use these precomputed functions for energy transfer across links, in a top down manner, going down into the hierarchy to the leaf polygons only for the purposes of producing a shaded image, and then deleting the detailed descriptions to save memory. For computing the form factor from a polygon to a vertex, Michael Stark and Richard Riesenfeld gave a formula which involved a sum over the vertices of the visible portion of the polygon. In contrast to the familiar sum over the edges, this formulation involves isolated visibility events, rather than maintaining the edge structure of the polygon though multiple clipping computations. Min Chen and James Arvo gave a closed form solution for the irradiance from polygonal sources on which the radiance varies linearly, in terms of elementary functions and Clausen's integral, a special function of one variable for which a numerical approximation was supplied. The paper was heavily mathematical, with more details promised in a tech report, which also contains generalizations to polynomially varying luminaires. There were two papers on occlusion culling per view cell, as a preprocess for interactive walkthroughs. These dealt with the problem of many small occluders, which jointly but not individually can hide objects from any viewpoint in the view cell. The first, by Vladlan Koltun, Yiorgos Chrysanthou, and Daniel Cohen-Or, was a 2D method, based on growing the virtual occluders by intersecting objects with active separating and supporting lines. The method was extended to 2.5D by using multiple 2D slicing planes, and is then applicable to architectural environments built from vertically extruded volumes. The second, by Peter Wonka, Michael Wimmer, and Dieter Schmalsteig, computes the objects occluded from all of a collection of regularly spaced viewpoints on the boundary of the view cell by occluders appropriately shrunk to account for the spacing of the viewpoints. A related paper by Luc Leblanc and Pierre Poulin applied occlusion in the context of cluster hierarchical radiosity. They tried to determine whether the shaft between a source and receiver was either completely occluded, or completely unoccluded, using hierarchical bounding volumes for the potential occluders. Although they did not perform the general occluder fusion discussed above, they did attempt to join occluding elements lying on the same plane into large rectangles. There were also two papers on shadows. Peter-Pike Sloan and Michael Cohen showed how to accomplish my Horizon Mapping technique in real-time, taking advantage of the register combining features of the NVidia hardware to combine weighted versions of the horizon textures precomputed for several discrete directions. Also, Wolfgang Heidrich, Stefan Brabeck, and Hans-Peter Seidel showed how to use hardware for approximating shadow penumbras for linear light sources, by computing shadow maps for the two extremities, doing edge detection for the depth discontinuities, and then generating "skin" polygons warped from one depth map to the other, to approximate linearly the variation in the illumination across the penumbra. Brian Smits, Peter Shirley, and Michael Stark showed how to efficiently ray trace a topologically regular "hexagonal" mesh of displacement mapped triangles, by traversing the approximately prismatic bounding cells over each mesh triangle, bounded by segments of the normals erected at the mesh vertices. The decision about which face a ray exits such a prism depends on testing to which side of the normal opposite the entering face the ray passes, and the topological regularity then allows the next cell to be easily indexed. There were two papers on local reflection. Yinlong Sun, David Fracchia, Mark Drew, and Thomas Calvert rendered the diffraction-related iridescent colors of optical disks, taking into account the geometry of the pits, the random change of the phase of the pits between successive turns of the spiral track, and the non-diffractive contribution to the reflectivity. Their approach differs from the methods used in the three earlier publications by Beckmann, He et al., and Stam in that it is applicable to dielectric as well as conducting surfaces, and seems to better correspond to photographs of real optical disks. Isabel Icart and Didier Arques computed the BRDF for multilayer coated materials with uncorrelated rough boundaries, using the Helmholtz-Kirchoff integral, and the Abeles matrix formulation, assuming the slopes of the surface layer interfaces are so small that they can be neglected, and only the variations in layer thickness effect the calculation. **************************** Of the remaining time in my sabbatical, not occupied by attending these conferences, I spent about half reviewing papers for conferences and journals, chiefly for the Eurographics Workshop on Rendering. I spent the other half working with Sylvain Paris and Francois Sillion on an IBR approach to utilize 40 simultaneous photographs of a city scene, containing foreground characters, a fountain, and background buildings, in order to generate renderings from new viewpoints. Sylvain started by using the MatchMover software from RealVis to do a combined fit for all the optical and viewing parameters of the cameras, based on correspondences between image points, partly entered by hand and partly propagated automatically by image correlation. Next he used voxel coloring, and was able to segment the foreground character from the objects behind it. I then attempted to model it with a texture/displacement map, by using the texture from the central image, and displacements along viewing rays in the central image. I used these displacements, plus x and y misregistration variables, as parameters in a Conjugate Gradient minimization of the RMS differences between the input images and the ones produced by rendering the displaced textured mesh. I added a surface bending term to these RMS differences, in order to suppress wild folds in the surface. This is a similar approach to that of Fua and Leclerc, who in addition added a shape-from-shading error term, but differs in that I used hardware rendering rather than software. Unfortunately, I did not have time to finish debugging this approach, so I hope for time to continue to work on it. In conjunction with my research on IBR, I visited Sophia-Antipolis, where I spoke to several graduate students at INRIA, and to Luc Robert, the CTO at RealVis. In addition to demonstrating and discussing the MatchMover program I described above, he also showed me ReTimer, which can change the length of a filmed sequence using optical flow to interpolate between frames, and a system for modelling textured objects from multiple views, using computed epipolar lines to guide a user in selecting corresponding points in the images. The object is then modeled with the aid of a surface patch modelling system like Maya or SoftImage. These three products are designed for the film industry, which is accustomed to using human mouse click input, so the goal was not to automate the whole process. The RealVis IBR systems are being increasingly used for special effects in the film and TV commercial industry. Luc Robert suggested that he could employ a student intern from U C Davis for a period of time, so this contact may prove useful. At INRIA in Grenoble, I also spoke to the other graphics researchers and got demonstrations of their graphics software. I was particularly impressed by the work of Eric Ferley on sculptural modelling with metaballs and meta-ellipsoids, done interactively in a three-projector immersive cylindrical screen theater with liquid crystal shutter stereo glasses. I also was inspired by conversations with Fabrice Neyret to invent a new algorithm for rendering clouds, combining the diffusion approximation on the interior with multiple scattering near the surface. This is an elaboration of the message I sent to globillum 2 or 3 years ago about the dark edges on cloud profiles, and I hope to eventually implement and it. -- email: max2@llnl.gov Nelson Max, Mail Stop L-560 http://www.llnl.gov/graphics Lawrence Livermore National Laboratory phone (925) 422-4074 7000 East Avenue fax (925) 422-6287 Livermore, CA 94550, USA ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id WAA20152; Sun, 13 Aug 2000 22:32:25 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id WAA17426; Sun, 13 Aug 2000 22:32:29 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id WAA17421 for ; Sun, 13 Aug 2000 22:32:21 +0200 Received: from mail.easyhosting.com (smartmail1.easyhosting.com [207.136.80.71]) by imag.imag.fr (8.9.3/8.8.5) with ESMTP id WAA22495 for ; Sun, 13 Aug 2000 22:32:22 +0200 (MET DST) Received: from byheart (bc-van-wvn-a53-01-29.look.ca [216.66.156.125]) by mail.easyhosting.com (8.9.3/8.9.3) with SMTP id QAA16933 for ; Sun, 13 Aug 2000 16:33:43 -0400 (EDT) Message-Id: <000c01c00564$7dc4eca0$7d9c42d8@byheart> Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: 00/08/15 Release of RADBIB.BIB Global Illumination Bibliography Date: Sun, 13 Aug 2000 13:24:31 -0700 Organization: byHeartConsultants Limited Mime-Version: 1.0 Content-Type: text/html; charset=windows-1252 X-Priority: 3 X-Msmail-Priority: Normal X-Mailer: Microsoft Outlook Express 5.50.4133.2400 X-Mimeole: Produced By Microsoft MimeOLE V5.50.4133.2400 X-Loop: globillum@imag.fr X-Sequence: 9 Precedence: list X-UIDL: T_k!!&
ANNOUNCE: 00/08/15 Release of RADBIB.BIB
----------------------------------------
RADBIB is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. It currently includes 1,783 references -- 8 new additions since its 00/07/01 release.
 
This bibliography is available in BibTex format as RADBIB.BIB (with a release date of August 15, 2000) from:
 
  http://www.helios32.com (Resources section)
 
Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 224 references to radiosity and global illumination theses -- no new additions since the 00/07/01 release.
 
Financial support for the maintenance of these bibliographies has been provided by ACM SIGGRAPH Special Projects and byHeart Consultants Limited.
 
PS - For those interested in photometric data files, a freeware EULUMDAT to IES LM-63-1995 file conversion utility is now also available from http://www.helios32.com (Resources section).
 
Ian Ashdown, P. Eng., LC, FIES
Vice President
byHeart Consultants Limited
http://www.helios32.com
From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id WAA15971; Wed, 16 Aug 2000 22:34:02 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id WAA22152; Wed, 16 Aug 2000 22:33:34 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id WAA22147 for ; Wed, 16 Aug 2000 22:33:32 +0200 Received: from bach.Graphics.Cornell.EDU (bach.graphics.cornell.edu [128.84.247.50]) by imag.imag.fr (8.9.3/8.8.5) with ESMTP id WAA15065 for ; Wed, 16 Aug 2000 22:33:34 +0200 (MET DST) Received: from kerub (kerub.graphics.cornell.edu [128.84.247.84]) by bach.Graphics.Cornell.EDU (8.9.1/8.9.1) with ESMTP id QAA22177 for ; Wed, 16 Aug 2000 16:33:30 -0400 (EDT) (envelope-from hector@graphics.cornell.edu) Message-Id: <4.2.0.58.20000816163133.00abedf0@hpmail.graphics.cornell.edu> X-Sender: hector@hpmail.graphics.cornell.edu X-Mailer: QUALCOMM Windows Eudora Pro Version 4.2.0.58 Date: Wed, 16 Aug 2000 16:33:46 -0400 To: globillum@imag.fr From: Hector Yee Subject: Globillum/Perception Thesis Mime-Version: 1.0 X-Loop: globillum@imag.fr X-Sequence: 10 Precedence: list Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: QMp!!JWM!!kf##!QN>!! X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit http://www.graphics.cornell.edu/~hector/yee2000.pdf Abstract: We present a method to accelerate global illumination computation in dynamic environments by taking advantage of limitations of the human visual system. A model of visual attention is used to locate regions of interest in a scene and to modulate spatiotemporal sensitivity. The method is applied in the form of a spatiotemporal error tolerance map. Perceptual acceleration combined with good sampling protocols provide a global illumination solution feasible for use in animation. Results indicate an order of magnitude improvement in computational speed. The method is adaptable and can also be used in image-based rendering, geometry level of detail selection, realistic image synthesis, video telephony and video compression. ---------- { Yangli | Hector } Yee Program of Computer Graphics, Cornell University Work: http://www.graphics.cornell.edu/~hector Fun: http://www.people.cornell.edu/pages/yhy1 Hinei, mah-tov u-mah-naim shbayt achim gam yachad! Behold, how good and how pleasant [it is] for brethren to dwell together in unity! ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id AAA26826; Fri, 18 Aug 2000 00:04:24 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id AAA23981; Fri, 18 Aug 2000 00:04:19 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id AAA23976 for ; Fri, 18 Aug 2000 00:04:16 +0200 Received: from positron.cs.berkeley.edu (positron.CS.Berkeley.EDU [128.32.37.42]) by imag.imag.fr (8.9.3/8.8.5) with ESMTP id AAA19945 for ; Fri, 18 Aug 2000 00:04:17 +0200 (MET DST) Received: (from gwlarson@localhost) by positron.cs.berkeley.edu (980427.SGI.8.8.8/980728.SGI.AUTOCF) id PAA08618; Thu, 17 Aug 2000 15:05:29 -0700 (PDT) Date: Thu, 17 Aug 2000 15:05:29 -0700 (PDT) From: Gregory Ward Larson Message-Id: <200008172205.PAA08618@positron.cs.berkeley.edu> To: globillum@imag.fr Subject: Alain Fournier passed away X-Loop: globillum@imag.fr X-Sequence: 11 Precedence: list Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: +Dp"!U(h!!9Dp"!]`_!! X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 MIME-Version: 1.0 Content-transfer-encoding: 8bit This is a multi-part message in MIME format... ------------=_966549858-22368-1 Paul Heckbert asked me to forward this to globillum, since his new e-mail doesn't seem to be on the approved list. Very sad news for all of us. We'll miss him. -Greg -------------------- The following is a message from Kelly Booth: Monday, August 14, 2000 (from Eugene Fiume, former PhD student and colleague of Alain's): > Alain Fournier died this morning at about 2:30PDT in Vancouver, ending a > 10 year battle with lymphoma. > > There were no two ways about Alain. Either you loved him, or you loved > him more. Anyone who ever met him knew in an instant that he was an > extraordinary person. He was a poet and a scientist. He was utterly > genuine, completely unique. He leaves behind his wife Adrienne, his > 13-year-old daughter Ariel, and a huge cohort of friends and admirers. > In time we will work out a good way to commemorate his contributions to > our department and to his field. A number of people have sent e-mail expressing their sadness at Alain's passing, and their best wishes for his family. At this time, there are no firm plans for how we might remember Alain in a formal way, although I know that many people are already thinking of the most fitting way to honour his memory. The following message came from the Department of Computer Science at the University of British Columbia. I'm including it in case anyone is able to attend. There is also some information about a possible memorial to be established, but please note that this is tentative until there has been an opportunity to consult more widely among his many friends and his family. > The flag will be lowered today, August 14, 2000 in memory of Dr. Alain > Fournier who passed away today. He was a professor in Computer > Sciences. A memorial service will be held at the the Leon and Thea > Koerner University Centre (formerly the old Faculty Club) at 2:00 pm on > August 19th, 2000. > > The family have requested no flowers at the present time. > > A memorial fund in Alain's name is being set up to support > Ph.D. students at Canadian universities, tentatively. Further > details will announced. We are all saddened by Alain's death. Kelly Booth ------------=_966549858-22368-1 Content-Type: text/plain; name="message.footer" Content-Disposition: inline; filename="message.footer" Content-Transfer-Encoding: 8bit ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- ------------=_966549858-22368-1-- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id TAA32064; Mon, 28 Aug 2000 19:30:40 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id TAA11318; Mon, 28 Aug 2000 19:30:38 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id TAA11313 for ; Mon, 28 Aug 2000 19:30:35 +0200 Received: from postoffice.srv.cs.cmu.edu (POSTOFFICE.SRV.CS.CMU.EDU [128.2.181.62]) by imag.imag.fr (8.9.3/8.8.6) with SMTP id TAA21836 for ; Mon, 28 Aug 2000 19:30:39 +0200 (MET DST) Received: from KRUNCH.GRAPHICS.CS.CMU.EDU by postoffice.srv.cs.cmu.edu id aa13849; 28 Aug 2000 13:30 EDT Sender: ph@postoffice.srv.cs.cmu.edu Message-Id: <39AAA1A2.6EC7D5AF@cs.cmu.edu> Date: Mon, 28 Aug 2000 13:30:10 -0400 From: Paul Heckbert Organization: Computer Science Dept., Carnegie Mellon University X-Mailer: Mozilla 4.08 [en] (X11; U; IRIX 6.2 IP22) Mime-Version: 1.0 To: Mailing List for Global Illumination , Joe Cychosz , Computer Graphics Group Subject: contest: ray tracer in functional language X-Loop: globillum@imag.fr X-Sequence: 12 Precedence: list Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: e;2"!K?7!!91X!!7PQ!! X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit There is a programming contest happening right now to write a ray tracer. The contest is being put on by people affiliated with the International Conference on Functional Programming (specifically Greg Morrisett and John Reppy at Cornell). This community is fond of ML, O'Caml, and related functional programming languages, but apparently any language can be used in the contest. Entries are judged on speed, quality, and other criteria. The contest started Saturday at 5pm EDT and ends Tuesday at 5pm EDT (so get busy!) I just learned about the contest a few minutes ago. See http://www.cs.cornell.edu/icfp/ ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id RAA04078; Mon, 4 Sep 2000 17:39:59 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id RAA29619; Mon, 4 Sep 2000 17:39:30 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id RAA29614 for ; Mon, 4 Sep 2000 17:39:27 +0200 Received: from mail.easyhosting.com (smartmail1.easyhosting.com [207.136.80.71]) by imag.imag.fr (8.9.3/8.8.6) with ESMTP id RAA21734 for ; Mon, 4 Sep 2000 17:39:28 +0200 (MET DST) Received: from byheart (bc-van-wvn-a53-01-03.look.ca [216.66.156.99]) by mail.easyhosting.com (8.9.3/8.9.3) with SMTP id LAA20148 for ; Mon, 4 Sep 2000 11:39:19 -0400 (EDT) Message-Id: <004001c01686$62f620a0$639c42d8@byheart> Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: 00/09/01 Release of RADBIB.BIB Date: Mon, 4 Sep 2000 08:39:58 -0700 Organization: byHeartConsultants Limited Mime-Version: 1.0 Content-Type: text/html; charset=windows-1252 X-Priority: 3 X-Msmail-Priority: Normal X-Mailer: Microsoft Outlook Express 5.50.4133.2400 X-Mimeole: Produced By Microsoft MimeOLE V5.50.4133.2400 X-Loop: globillum@imag.fr X-Sequence: 16 Precedence: list X-UIDL: 6Ef!!YL\!!n_'!!bO]"! X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit
ANNOUNCE: 00/09/01 Release of RADBIB.BIB
----------------------------------------
RADBIB is a comprehensive bibliography of radiosity and related global
illumination papers, theses, articles, and books. It currently includes
1,795 references -- 12 new additions since its 00/08/15 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a
release date of September 01, 2000) from:

  http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called
GITHESIS.BIB. This bibliography includes 224 references to radiosity and
global illumination theses -- no new additions since the 00/07/01 release.
----
Ian Ashdown, P. Eng., LC, FIES
Vice President
byHeart Consultants Limited
http://www.helios32.com
From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id RAA16693; Tue, 5 Sep 2000 17:22:07 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id RAA31252; Tue, 5 Sep 2000 17:22:10 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id RAA31247 for ; Tue, 5 Sep 2000 17:22:08 +0200 Received: from mut.autodesk.com (mut.autodesk.com [198.102.112.26]) by imag.imag.fr (8.9.3/8.8.6) with ESMTP id RAA19270 for ; Tue, 5 Sep 2000 17:22:07 +0200 (MET DST) From: eric.haines@autodesk.com Received: from autodesk.autodesk.com (autodesk.autodesk.com [144.111.216.101]) by mut.autodesk.com (8.9.3/8.9.3) with ESMTP id IAA10148 for ; Tue, 5 Sep 2000 08:21:49 -0700 (PDT) Received: from hqmsgsrf00.autodesk.com by autodesk.autodesk.com (8.8.8/4.4BSD) with ESMTP id IAA02654; Tue, 5 Sep 2000 08:21:08 -0700 (PDT) Received: by hqmsgsrf00.autodesk.com with Internet Mail Service (5.5.2448.0) id ; Tue, 5 Sep 2000 08:20:52 -0700 Message-Id: <19879C753611D3119DAB0008C7A4C0C1057F8F2A@hqmsgsrf04.autodesk.com> To: globillum@imag.fr Subject: Graphics Gems and Ray Tracing News URLs Date: Tue, 5 Sep 2000 08:21:12 -0700 Mime-Version: 1.0 X-Mailer: Internet Mail Service (5.5.2448.0) X-Loop: globillum@imag.fr X-Sequence: 17 Precedence: list Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: I$?!!$*G"!YX\!!!Jn"! X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit I decided to buy a forwarding URL for two resources I maintain and edit, to make it easy for people to remember how to find them. http://www.graphicsgems.org is the Graphics Gems repository address (sorry, the .com version was grabbed by someone else). http://www.raytracingnews.com is the Ray Tracing News archive. Enjoy, Eric ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id KAA09237; Fri, 15 Sep 2000 10:15:20 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id KAA13251; Fri, 15 Sep 2000 10:15:11 +0200 Received: from ebene.inrialpes.fr (ebene.inrialpes.fr [194.199.18.70]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id KAA13246 for ; Fri, 15 Sep 2000 10:15:06 +0200 Received: from safran.inrialpes.fr (safran.inrialpes.fr [194.199.26.1]) by ebene.inrialpes.fr (8.9.3/8.8.6) with ESMTP id KAA06341 for ; Fri, 15 Sep 2000 10:15:06 +0200 (MET DST) Received: from imag.fr (sesame [194.199.26.83]) by safran.inrialpes.fr (980427.SGI.8.8.8/8.8.5) with ESMTP id KAA02017 for ; Fri, 15 Sep 2000 10:15:06 +0200 (MDT) Sender: Francois.Sillion@imag.fr Message-ID: <39C1DA8A.F3148C2D@imag.fr> Date: Fri, 15 Sep 2000 10:15:06 +0200 From: Francois Sillion Organization: iMAGIS - GRAVIR/IMAG INRIA X-Mailer: Mozilla 4.7C-SGI [en] (X11; I; IRIX 6.5 IP32) X-Accept-Language: en MIME-Version: 1.0 To: globillum@imag.fr Subject: [Fwd: FW: radioptimization] X-MIME-Autoconverted: from quoted-printable to 8bit by chopinette.imag.fr id KAA13246 X-Loop: globillum@imag.fr X-Sequence: 20 Precedence: list List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: 8M6!!0Zg"!^`8"!bi)"! X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit I am forwarding this mesage from Michael since he had trouble posting. by the way, we have tried to fix all problems that were introduced by our migration to a new list server. All should be in order now, let me know if you experience any problemes and sorry about the glitches. -------- Original Message -------- Subject: FW: radioptimization Date: Tue, 29 Aug 2000 08:53:47 -0700 From: "Michael Cohen (RESEARCH)" To: "'globillum@imag.fr'" CC: "'sillion@imag.fr'" As I haven't thought about this in a while, anyone else want to help Maria out?- Michael -----Original Message----- From: Maria Juliana Gambini [mailto:mjgambini@movi.com.ar] Sent: Monday, August 28, 2000 1:17 PM To: Michael Cohen (RESEARCH) Subject: radioptimization Dear Mr. Cohen,I´m a theacher of Computer Graphics in The Buenos Aires University (UBA) and a pupil of post graduate course in Computer Science. For this reason I´m looking for information about ¨radioptimization¨. I´m interesting in this for my research work.I finded a paper publicated in SIGGRAPH´93 and I would like to know more about this.Please, can you send me some information? May be new papers, or new works or people adresses.Thank you very much, and I´m sorry by interrupt you. Great regards, M. Juliana Gambini ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id UAA12512; Sat, 23 Sep 2000 20:09:45 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id TAA00791; Sat, 23 Sep 2000 19:09:47 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id TAA00786 for ; Sat, 23 Sep 2000 19:09:28 +0200 Received: from mail.easyhosting.com (smartmail1.easyhosting.com [207.136.80.71]) by imag.imag.fr (8.9.3/8.8.6) with ESMTP id UAA10311 for ; Sat, 23 Sep 2000 20:09:28 +0200 (MET DST) Received: from byheart (bc-van-wvn-a53-01-09.look.ca [216.66.156.105]) by mail.easyhosting.com (8.9.3/8.9.3) with SMTP id OAA28393 for ; Sat, 23 Sep 2000 14:09:20 -0400 (EDT) Message-ID: <003701c02589$620adc00$699c42d8@byheart> Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: 00/09/23 Release of RADBIB and GITHESIS Date: Sat, 23 Sep 2000 11:09:13 -0700 Organization: byHeartConsultants Limited MIME-Version: 1.0 Content-Type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 5.50.4133.2400 X-MimeOLE: Produced By Microsoft MimeOLE V5.50.4133.2400 X-Loop: globillum@imag.fr X-Sequence: 21 Precedence: list List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-UIDL: [W9!!be1!!W2b"!#Qd!! X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit
ANNOUNCE: 00/09/23 Release of RADBIB and GITHESIS
-------------------------------------------------
RADBIB is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. It currently includes 1,805 references -- 10 new additions since its 00/09/01 release.
 
This bibliography is available in BibTex format as RADBIB.BIB (with a release date of September 23, 2000) from:
 
  http://www.helios32.com (Resources section)
 
Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 232 references to radiosity and global illumination theses -- 7 new additions since the 00/07/01 release.
 
Financial support for the maintenance of these bibliographies has been provided by ACM SIGGRAPH Special Projects and byHeart Consultants Limited.
 
Ian Ashdown, P. Eng., LC, FIES
Vice President
byHeart Consultants Limited
http://www.helios32.com
From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id BAA08134; Tue, 26 Sep 2000 01:07:16 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id BAA03138; Tue, 26 Sep 2000 01:07:15 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id BAA03133 for ; Tue, 26 Sep 2000 01:07:14 +0200 Received: from postoffice.srv.cs.cmu.edu (POSTOFFICE.SRV.CS.CMU.EDU [128.2.181.62]) by imag.imag.fr (8.9.3/8.8.6) with SMTP id BAA12804 for ; Tue, 26 Sep 2000 01:07:14 +0200 (MET DST) Received: from KRUNCH.GRAPHICS.CS.CMU.EDU by postoffice.srv.cs.cmu.edu id aa12850; 25 Sep 2000 19:06 EDT Sender: ph@postoffice.srv.cs.cmu.edu Message-ID: <39CFDA87.C805B0FB@cs.cmu.edu> Date: Mon, 25 Sep 2000 19:06:47 -0400 From: Paul Heckbert Organization: Computer Science Dept., Carnegie Mellon University X-Mailer: Mozilla 4.08 [en] (X11; U; IRIX 6.2 IP22) MIME-Version: 1.0 To: Mailing List for Global Illumination Subject: Alain Fournier Scholarhip Memorial Fund X-Loop: globillum@imag.fr X-Sequence: 23 Precedence: list List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: Z5G!!Pb"! X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Kellogg Booth wrote: > > An endowment fund has been set up to honour the memory of Dr Alain > Fournier and his contributions to the field of computer graphics in > Canada. The endowment will fund a scholarship to a PhD student in > computer graphics at a Canadian university. > > Alain's influence as a scientist, a teacher, a mentor and a friend went > far beyond the boundaries of UBC. He is remembered with respect, > gratitude and abiding affection. The scope of his research profoundly > affected the field of computer graphics at the local, provincial, > national and international levels. It is therefore fitting that the > scholarship should be national in character, and that it should be > adjudicated by Alain's former doctoral students, in conjunction with > the Department of Computer Science at UBC. > > We hereby invite friends, colleagues, alumni/ae, indeed, anyone who > felt Alain's influence, to contribute to the Alain Fournier Scholarship. > It is our hope and expectation that Alain's memory will live on for > generations to come through the generous funding of this endowment and > the provision of a scholarship to a doctoral student in computer graphics. > > Please send your contributions to: > > The Alain Fournier Memorial Fund > Department of Computer Science > University of British Columbia > 201-2366 Main Mall > Vanouver, BC > Canada V6T 1Z4 > > *** Please forward this message to those who you think would appreciate > *** receiving it. ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id VAA11934; Wed, 25 Oct 2000 21:53:21 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id VAA15468; Wed, 25 Oct 2000 21:53:16 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id VAA15463 for ; Wed, 25 Oct 2000 21:53:13 +0200 Received: from bach.Graphics.Cornell.EDU (bach.graphics.cornell.edu [128.84.247.50]) by imag.imag.fr (8.9.3/8.8.6) with ESMTP id VAA00622 for ; Wed, 25 Oct 2000 21:53:12 +0200 (MET DST) Received: from DIESEL (diesel.graphics.cornell.edu [128.84.247.211]) by bach.Graphics.Cornell.EDU (8.9.1/8.9.1) with ESMTP id PAA25564 for ; Wed, 25 Oct 2000 15:53:11 -0400 (EDT) (envelope-from westin@graphics.cornell.edu) Date: Wed, 25 Oct 2000 15:53:11 -0400 (EDT) Message-Id: <200010251953.PAA25564@bach.Graphics.Cornell.EDU> From: "Stephen H. Westin" To: globillum@imag.fr Subject: Revised RenderMan implementation of Lafortune model Reply-to: westin@Graphics.Cornell.EDU X-Loop: globillum@imag.fr X-Sequence: 24 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: )]0"!8R`!!/'2"!*"b!! X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 MIME-Version: 1.0 Content-transfer-encoding: 8bit This is a multi-part message in MIME format... ------------=_972503595-12166-0 I have corrected my RenderMan shader implementation of the Lafortune BRDF representation; Sing-Choong Foo pointed out that I failed to multiply the lobes by the incident cosine. The revised shader eliminates some hard-edge artifacts at grazing incidence. Get it at . -Stephen H. Westin Any information or opinions in this message are mine: they do not represent the position of Cornell University or any of its sponsors. ------------=_972503595-12166-0 Content-Type: text/plain; name="message.footer" Content-Disposition: inline; filename="message.footer" Content-Transfer-Encoding: 8bit ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- ------------=_972503595-12166-0-- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id SAA06683; Fri, 27 Oct 2000 18:19:18 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id SAA20626; Fri, 27 Oct 2000 18:19:22 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id SAA20620 for ; Fri, 27 Oct 2000 18:19:20 +0200 Received: from bach.Graphics.Cornell.EDU (bach.graphics.cornell.edu [128.84.247.50]) by imag.imag.fr (8.9.3/8.8.6) with ESMTP id SAA07334 for ; Fri, 27 Oct 2000 18:19:19 +0200 (MET DST) Received: from DIESEL (diesel.graphics.cornell.edu [128.84.247.211]) by bach.Graphics.Cornell.EDU (8.9.1/8.9.1) with ESMTP id MAA28730 for ; Fri, 27 Oct 2000 12:19:10 -0400 (EDT) (envelope-from westin@graphics.cornell.edu) Date: Fri, 27 Oct 2000 12:19:09 -0400 (EDT) Message-Id: <200010271619.MAA28730@bach.Graphics.Cornell.EDU> From: "Stephen H. Westin" To: globillum@imag.fr Subject: Revised revised Lafortune shader: face gets redder Reply-to: westin@Graphics.Cornell.EDU References: <39CE5834.A96B4D58@cs.yorku.ca> X-Loop: globillum@imag.fr X-Sequence: 25 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: gXB"!SNd!!l6i!!fI^!! X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 MIME-Version: 1.0 Content-transfer-encoding: 8bit This is a multi-part message in MIME format... ------------=_972663561-17889-0 I revised the Lafortune RenderMan shader, posted it to the Web, and another error was pointed out to me. Please pick up the latest version at . As always, coefficients for using this shader to approximate human skin are available at . Two sets of coefficients are available; only one has been reformatted for RenderMan, but it can serve as a guide for formatting the other. Stephen H. Westin Research Project Leader Program of Computer Graphics Cornell University westin@graphics.cornell.edu 607 255 9080 (VOX) 607 255 0806 (FAX) ------------=_972663561-17889-0 Content-Type: text/plain; name="message.footer" Content-Disposition: inline; filename="message.footer" Content-Transfer-Encoding: 8bit ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- ------------=_972663561-17889-0-- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id QAA13695; Mon, 30 Oct 2000 16:12:25 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id QAA26915; Mon, 30 Oct 2000 16:12:21 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id QAA26910 for ; Mon, 30 Oct 2000 16:12:18 +0100 Received: from mail.easyhosting.com (smartmail1.easyhosting.com [207.136.80.71]) by imag.imag.fr (8.9.3/8.8.6) with ESMTP id QAA01012 for ; Mon, 30 Oct 2000 16:12:16 +0100 (MET) Received: from byheart (bc-van-wvn-a53-01-01.look.ca [216.66.156.97]) by mail.easyhosting.com (8.9.3/8.9.3) with SMTP id KAA10016 for ; Mon, 30 Oct 2000 10:12:03 -0500 (EST) Message-ID: <001c01c04283$88fced00$619c42d8@byheart> Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: November 1st Release of RADBIB Date: Mon, 30 Oct 2000 07:01:54 -0800 Organization: byHeartConsultants Limited MIME-Version: 1.0 X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 5.50.4133.2400 X-MimeOLE: Produced By Microsoft MimeOLE V5.50.4133.2400 X-Loop: globillum@imag.fr X-Sequence: 26 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: a6b"!SE-!!,)Q"!](>!! X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit ANNOUNCE: 00/11/01 Release of RADBIB and GITHESIS ------------------------------------------------- RADBIB is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. It currently includes 1,825 references -- 20 new additions since its 00/09/23 release. This bibliography is available in BibTex format as RADBIB.BIB (with a release date of November 1, 2000) from: http://www.helios32.com (Resources section) Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 232 references to radiosity and global illumination theses -- no new additions since the 00/09/23 release. Financial support for the maintenance of these bibliographies has been provided by byHeart Consultants Limited. Ian Ashdown, P. Eng., LC, FIES Chief Technology Officer byHeart Consultants Limited http://www.helios32.com ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id SAA23507; Mon, 6 Nov 2000 18:50:30 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id SAA10216; Mon, 6 Nov 2000 18:50:29 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id SAA10211 for ; Mon, 6 Nov 2000 18:50:26 +0100 Received: from scan1.fhg.de (scan1.fhg.de [153.96.1.35]) by imag.imag.fr (8.9.3/8.8.6) with ESMTP id SAA18550 for ; Mon, 6 Nov 2000 18:50:21 +0100 (MET) Received: from scan1.fhg.de (localhost [127.0.0.1]) by scan1.fhg.de (8.9.3/8.9.3) with ESMTP id SAA29496 for ; Mon, 6 Nov 2000 18:50:17 +0100 (MET) Received: from ise.fhg.de (ise.fhg.de [153.96.32.2]) by scan1.fhg.de (8.9.3/8.9.3) with SMTP id SAA29492 for ; Mon, 6 Nov 2000 18:50:16 +0100 (MET) Received: from server0.ise.fhg.de by ise.fhg.de (SMI-8.6/SMI-SVR4) id SAA24809; Mon, 6 Nov 2000 18:49:59 +0100 Received: from ise.fhg.de by server0.ise.fhg.de; Mon, 6 Nov 2000 17:48:02 +0100 (MEZ) Sender: schregle@ise.fhg.de Message-ID: <3A06E0C1.A739C40D@ise.fhg.de> Date: Mon, 06 Nov 2000 17:48:01 +0100 From: Roland Schregle Reply-To: schregle@ise.fhg.de Organization: Fraunhofer ISE X-Mailer: Mozilla 4.7 [en] (X11; I; Linux 2.2.10 i686) X-Accept-Language: en MIME-Version: 1.0 To: Globillum List Subject: Diploma thesis at FhG ISE X-Loop: globillum@imag.fr X-Sequence: 27 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: 5Gk!!l"o!!*NI!!1pA!! X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit The Fraunhofer Institute for Solar Energy Systems in Freiburg, Germany has a position for a diploma thesis in the daylighting research group (TOS). Scope of the work is the validation of a forward raytracing module embedded in the RADIANCE rendering system and its application in daylighting simulation. Requirements are a background in physics and programming skills in C. Contact Roland Schregle (schregle@ise.fhg.de) or Peter Apian-Bennewitz (apian@ise.fhg.de). -- Roland Schregle Fraunhofer Institute for Solar Energy Systems Oltmannsstr. 5, D-79100 Freiburg, Germany Phone: +49-761-4588-153 ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by christl.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id WAA25271; Fri, 10 Nov 2000 22:48:08 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id WAA29256; Fri, 10 Nov 2000 22:48:59 +0100 (MET) Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id WAA19101; Fri, 10 Nov 2000 22:48:12 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id WAA19096 for ; Fri, 10 Nov 2000 22:48:11 +0100 Received: from bach.Graphics.Cornell.EDU (bach.graphics.cornell.edu [128.84.247.50]) by imag.imag.fr (8.9.3/8.8.6) with ESMTP id WAA06371 for ; Fri, 10 Nov 2000 22:48:09 +0100 (MET) Received: from akila.graphics.cornell.edu (akila.graphics.cornell.edu [128.84.247.237]) by bach.Graphics.Cornell.EDU (8.9.1/8.9.1) with ESMTP id QAA17926 for ; Fri, 10 Nov 2000 16:48:08 -0500 (EST) (envelope-from parag@graphics.cornell.edu) Message-Id: <4.3.2.7.2.20001110164756.00c2c8c0@pop.graphics.cornell.edu> X-Sender: parag@pop.graphics.cornell.edu X-Mailer: QUALCOMM Windows Eudora Version 4.3.2 Date: Fri, 10 Nov 2000 16:49:11 -0500 To: globillum@imag.fr From: Parag Tole Subject: form factor to disc. Mime-Version: 1.0 X-Loop: globillum@imag.fr X-Sequence: 28 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: Qi6!!GNc!!7:f!!VSV"! X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hello, Is anyone aware of a formula for the form factor from a differential element to a (circular) disc? What about disc to disc? Thanks. ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by christl.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id WAA25314; Fri, 10 Nov 2000 22:54:22 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id WAA29450; Fri, 10 Nov 2000 22:55:02 +0100 (MET) Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id WAA19166; Fri, 10 Nov 2000 22:54:16 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id WAA19161 for ; Fri, 10 Nov 2000 22:54:14 +0100 Received: from nut.autodesk.com (nut.autodesk.com [198.102.112.27]) by imag.imag.fr (8.9.3/8.8.6) with ESMTP id WAA06557 for ; Fri, 10 Nov 2000 22:54:13 +0100 (MET) From: eric.haines@autodesk.com Received: from hqmsgsrf00.autodesk.com (hqmsgsrf00.autodesk.com [144.111.216.79]) by nut.autodesk.com (8.9.3/8.9.3) with ESMTP id NAA11784 for ; Fri, 10 Nov 2000 13:54:11 -0800 (PST) Received: by hqmsgsrf00.autodesk.com with Internet Mail Service (5.5.2448.0) id ; Fri, 10 Nov 2000 13:54:10 -0800 Message-ID: <19879C753611D3119DAB0008C7A4C0C1063AF0ED@hqmsgsrf04.autodesk.com> To: globillum@imag.fr Subject: Fantasy Graphics League - 2001 season has begun Date: Fri, 10 Nov 2000 13:54:09 -0800 MIME-Version: 1.0 X-Mailer: Internet Mail Service (5.5.2448.0) X-Loop: globillum@imag.fr X-Sequence: 29 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: FM]!!e_J"!l09!!4`$!! X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit The Fantasy Graphics League's second recruiting season has begun, and you're invited to form a laboratory. Go do it at: http://www.realtimerendering.com/fgl/ Eric ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by christl.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id XAA25430; Fri, 10 Nov 2000 23:06:17 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id XAA29898; Fri, 10 Nov 2000 23:07:04 +0100 (MET) Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id XAA19227; Fri, 10 Nov 2000 23:06:17 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id XAA19222 for ; Fri, 10 Nov 2000 23:06:16 +0100 Received: from e3.ny.us.ibm.com (e3.ny.us.ibm.com [32.97.182.103]) by imag.imag.fr (8.9.3/8.8.6) with ESMTP id XAA06882 for ; Fri, 10 Nov 2000 23:06:15 +0100 (MET) Received: from northrelay02.pok.ibm.com (northrelay02.pok.ibm.com [9.117.200.22]) by e3.ny.us.ibm.com (8.9.3/8.9.3) with ESMTP id RAA86274; Fri, 10 Nov 2000 17:05:30 -0500 Received: from d01ml244.pok.ibm.com (d01ml244.pok.ibm.com [9.117.200.44]) by northrelay02.pok.ibm.com (8.8.8m3/NCO v4.95) with ESMTP id RAA11876; Fri, 10 Nov 2000 17:04:58 -0500 Importance: Normal Subject: form factors To: globillum@imag.fr Cc: parag@graphics.cornell.edu X-Mailer: Lotus Notes Release 5.0.3 (Intl) 21 March 2000 Message-ID: From: "Holly Rushmeier/Watson/IBM" Date: Fri, 10 Nov 2000 17:06:00 -0500 X-MIMETrack: Serialize by Router on D01ML244/01/M/IBM(Release 5.0.5 |September 22, 2000) at 11/10/2000 05:06:01 PM MIME-Version: 1.0 X-Loop: globillum@imag.fr X-Sequence: 30 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: AZ$!!jSN"!L"`!!J\f"! X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit You could check the on-line catalog of A CATALOG OF RADIATION HEAT TRANSFER CONFIGURATION FACTORS by John R. Howell , University of Texas at Austin at http://www.me.utexas.edu/~howell/ Parag Tole on 11/10/2000 04:49:11 PM To: globillum@imag.fr cc: Subject: form factor to disc. Hello, Is anyone aware of a formula for the form factor from a differential element to a (circular) disc? What about disc to disc? Thanks. __________________________ Holly Rushmeier , holly@watson.ibm.com, http://www.research.ibm.com/people/h/holly, (914)784-7252 IBM TJ Watson Research Center, 30 Saw Mill River Road, Hawthorne, NY 10532, USA ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by christl.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id EAA30165; Sat, 11 Nov 2000 04:08:14 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id EAA07963; Sat, 11 Nov 2000 04:09:00 +0100 (MET) Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id EAA19570; Sat, 11 Nov 2000 04:08:14 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id EAA19565 for ; Sat, 11 Nov 2000 04:08:10 +0100 Received: from smartmail2.idirecthosting.com (smartmail2.easyhosting.com [207.136.80.73]) by imag.imag.fr (8.9.3/8.8.6) with ESMTP id EAA12141 for ; Sat, 11 Nov 2000 04:08:09 +0100 (MET) Received: from byheart (bc-van-wvn-a53-01-30.look.ca [216.66.156.126]) by smartmail2.idirecthosting.com (8.11.1/8.9.3) with SMTP id eAB381A93012; Fri, 10 Nov 2000 22:08:02 -0500 (EST) Message-ID: <007201c04b8c$dca242e0$7e9c42d8@byheart> Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: globillum@imag.fr, "Holly Rushmeier/Watson/IBM" Cc: parag@graphics.cornell.edu References: Subject: Re: form factors Date: Fri, 10 Nov 2000 19:09:51 -0800 Organization: byHeartConsultants Limited MIME-Version: 1.0 X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 5.50.4133.2400 X-MimeOLE: Produced By Microsoft MimeOLE V5.50.4133.2400 X-Loop: globillum@imag.fr X-Sequence: 31 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: #g="!Za>"!5J`"!3'c"! X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit > You could check the on-line catalog of > A CATALOG OF RADIATION HEAT TRANSFER > CONFIGURATION FACTORS > by John R. Howell , University of Texas at Austin > at > > http://www.me.utexas.edu/~howell/ > Does this include the classic "spherical cow" form factor equation? (Incidentally, I found a paper that may trump this one: an analytic expression for the form factor of a chicken embryo that includes interreflections from the interior of its shell.) Ian Ashdown, P. Eng., LC, FIES Chief Technology Officer byHeart Consultants Limited http://www.helios32.com ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by christl.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id UAA06880; Wed, 29 Nov 2000 20:35:56 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.11.1/8.11.1) with ESMTP id eATJak401502; Wed, 29 Nov 2000 20:36:47 +0100 (MET) Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id UAA24943; Wed, 29 Nov 2000 20:35:58 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id UAA24938 for ; Wed, 29 Nov 2000 20:35:57 +0100 Received: from ux1.sp.cs.cmu.edu (UX1.SP.CS.CMU.EDU [128.2.198.101]) by imag.imag.fr (8.9.3/8.8.6) with SMTP id UAA24399 for ; Wed, 29 Nov 2000 20:35:56 +0100 (MET) Message-Id: <200011291935.UAA24399@imag.imag.fr> Subject: Dissertation online To: globillum@imag.fr Date: Wed, 29 Nov 2000 14:35:51 -0500 (EST) From: Andrew Willmott Reply-To: ajw+@cs.cmu.edu X-Mailer: ELM [version 2.4 PL25-40] MIME-Version: 1.0 X-Loop: globillum@imag.fr X-Sequence: 32 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: +Q<"!=9C"!8H"#!(Z~!! X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hi everyone. My PhD dissertation, "Hierarchical Radiosity with Multiresolution Meshes", is finally online at: http://www.cs.cmu.edu/~ajw/thesis/ The abstract is included below. Cheers, Andrew --- The hierarchical radiosity algorithm solves for the global transfer of diffuse illumination in a scene. While its potential algorithmic complexity is superior to both previous radiosity methods and distributed ray tracing, for scenes containing detailed polygonal models, or highly tessellated curved surfaces, its time performance and memory consumption are less than ideal. My thesis is that by using hierarchies similar to those of multiresolution models, the performance of the hierarchical radiosity algorithm can be made sub-linear in the number of input polygons, and thus make radiosity on scenes containing detailed models tractable. The underlying goal of my thesis work has been to make high-speed radiosity solutions possible with such scenes. To achieve this goal, a new face clustering technique for automatically partitioning polygonal models has been developed. The face clusters produced group adjacent triangles with similar normal vectors. They are used during radiosity solution to represent the light reflected by a complex object at multiple levels of detail. Also, the radiosity method is reformulated in terms of vector irradiance. Together, face clustering and the vector formulation of radiosity permit large savings. Excessively fine levels of detail are not accessed by the algorithm during the bulk of the solution phase, greatly reducing its memory requirements relative to previous methods. Consequently, the costliest steps in the simulation can be made sub-linear in scene complexity. I have developed a radiosity system incorporating these ideas, and shown that its performance is far superior to existing hierarchical radiosity algorithms, in the domain of scenes containing complex models. ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by christl.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id VAA07155; Wed, 29 Nov 2000 21:04:13 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.11.1/8.11.1) with ESMTP id eATK54402775; Wed, 29 Nov 2000 21:05:04 +0100 (MET) Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id VAA25021; Wed, 29 Nov 2000 21:04:18 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id VAA25016 for ; Wed, 29 Nov 2000 21:04:15 +0100 Received: from postoffice.srv.cs.cmu.edu (POSTOFFICE.SRV.CS.CMU.EDU [128.2.181.62]) by imag.imag.fr (8.9.3/8.8.6) with SMTP id VAA25567 for ; Wed, 29 Nov 2000 21:04:14 +0100 (MET) Received: from KRUNCH.GRAPHICS.CS.CMU.EDU by postoffice.srv.cs.cmu.edu id aa14859; 29 Nov 2000 15:03 EST Sender: ph@postoffice.srv.cs.cmu.edu Message-ID: <3A25612D.25B2C764@cs.cmu.edu> Date: Wed, 29 Nov 2000 15:03:57 -0500 From: Paul Heckbert Organization: Computer Science Dept., Carnegie Mellon University X-Mailer: Mozilla 4.08 [en] (X11; U; IRIX 6.2 IP22) MIME-Version: 1.0 To: globillum@imag.fr CC: Michael Garland Subject: Re: Dissertation online References: <200011291935.UAA24399@imag.imag.fr> X-Loop: globillum@imag.fr X-Sequence: 33 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: [jd"!om_!!5F5"!FpB!! X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit I would add that Andrew's algorithm can do the view-independent solution phase of a radiosity simulation in under 4 minutes on a 3 million polygon scene, using only 41 megabytes of memory! That is not counting the cluster creation and view-dependent display phases. The use of multiresolution face clusters is what permits his algorithm to have such low memory use and to be so fast. (but I was Andrew's advisor so perhaps I'm biased) -Paul Paul Heckbert Associate Professor of Computer Science Carnegie Mellon University http://www.cs.cmu.edu/~ph Andrew Willmott wrote: > > Hi everyone. My PhD dissertation, "Hierarchical Radiosity with > Multiresolution Meshes", is finally online at: > > http://www.cs.cmu.edu/~ajw/thesis/ > > The abstract is included below. > > Cheers, > > Andrew > > --- > > The hierarchical radiosity algorithm solves for the global transfer of > diffuse illumination in a scene. While its potential algorithmic > complexity is superior to both previous radiosity methods and > distributed ray tracing, for scenes containing detailed polygonal > models, or highly tessellated curved surfaces, its time performance and > memory consumption are less than ideal. > > My thesis is that by using hierarchies similar to those of > multiresolution models, the performance of the hierarchical radiosity > algorithm can be made sub-linear in the number of input polygons, and > thus make radiosity on scenes containing detailed models tractable. The > underlying goal of my thesis work has been to make high-speed radiosity > solutions possible with such scenes. > > To achieve this goal, a new face clustering technique for automatically > partitioning polygonal models has been developed. The face clusters > produced group adjacent triangles with similar normal vectors. They are > used during radiosity solution to represent the light reflected by a > complex object at multiple levels of detail. Also, the radiosity method > is reformulated in terms of vector irradiance. Together, face clustering > and the vector formulation of radiosity permit large savings. > Excessively fine levels of detail are not accessed by the algorithm > during the bulk of the solution phase, greatly reducing its memory > requirements relative to previous methods. Consequently, the costliest > steps in the simulation can be made sub-linear in scene complexity. > > I have developed a radiosity system incorporating these ideas, and shown > that its performance is far superior to existing hierarchical radiosity > algorithms, in the domain of scenes containing complex models. --------------------------------------------------------------------- ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by christl.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id XAA08142; Wed, 29 Nov 2000 23:28:23 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.11.1/8.11.1) with ESMTP id eATMTF409575; Wed, 29 Nov 2000 23:29:15 +0100 (MET) Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id XAA25178; Wed, 29 Nov 2000 23:28:28 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id XAA25173 for ; Wed, 29 Nov 2000 23:28:20 +0100 Received: from smartmail2.idirecthosting.com (smartmail2.easyhosting.com [207.136.80.73]) by imag.imag.fr (8.9.3/8.8.6) with ESMTP id XAA00508 for ; Wed, 29 Nov 2000 23:28:19 +0100 (MET) Received: from byheart (bc-van-wvn-a53-01-32.look.ca [216.66.156.128]) by smartmail2.idirecthosting.com (8.11.1/8.9.3) with SMTP id eATMS4C94099 for ; Wed, 29 Nov 2000 17:28:05 -0500 (EST) Message-ID: <000e01c05a53$a7285e80$809c42d8@byheart> Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: RADBIB and GITHESIS (00/12/01) Date: Wed, 29 Nov 2000 14:28:07 -0800 Organization: byHeartConsultants Limited MIME-Version: 1.0 Content-Type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 5.50.4133.2400 X-MimeOLE: Produced By Microsoft MimeOLE V5.50.4133.2400 X-Loop: globillum@imag.fr X-Sequence: 34 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: X-UIDL: #:!"!=>K!!Q8
ANNOUNCE: 00/12/01 Release of RADBIB and GITHESIS
-------------------------------------------------
RADBIB is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. It currently includes 1,840 references -- 15 new additions since its 00/11/01 release.
 
This bibliography is available in BibTex format as RADBIB.BIB (with a release date of December 1, 2000) from:
 
  http://www.helios32.com (Resources section)
 
Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 233 references to radiosity and global illumination theses -- one new addition since the 00/09/23 release.
 
Financial support for the maintenance of these bibliographies has been provided by byHeart Consultants Limited.
 
Ian Ashdown, P. Eng., LC, FIES
Chief Technology Officer
byHeart Consultants Limited
http://www.helios32.com
From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by christl.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id CAA07351; Tue, 5 Dec 2000 02:35:06 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.11.1/8.11.1) with ESMTP id eB51ZMf11957; Tue, 5 Dec 2000 02:35:22 +0100 (MET) Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id CAA07191; Tue, 5 Dec 2000 02:34:31 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id CAA07186 for ; Tue, 5 Dec 2000 02:34:05 +0100 Received: from dirty.research.bell-labs.com (dirty.research.bell-labs.com [204.178.16.6]) by imag.imag.fr (8.9.3/8.8.6) with SMTP id CAA20872 for ; Tue, 5 Dec 2000 02:34:04 +0100 (MET) Received: from mcs.research.bell-labs.com ([135.104.32.15]) by dirty; Mon Dec 4 20:33:48 EST 2000 Received: from research.bell-labs.com (tsingos.lra.lucent.com [135.255.40.190]) by mcs.research.bell-labs.com (8.8.8/8.8.8) with ESMTP id UAA2098320; Mon, 4 Dec 2000 20:33:17 -0500 (EST) Message-ID: <3A2C45D6.92165EA@research.bell-labs.com> Date: Mon, 04 Dec 2000 20:33:10 -0500 From: Nicolas Tsingos Organization: Bell Laboratories X-Mailer: Mozilla 4.73 [en] (Win98; U) X-Accept-Language: en MIME-Version: 1.0 To: adrian@cnmat.berkeley.edu, globillum@imag.fr, db@eos.arc.nasa.gov, dg@lexicon.com, bwenzel@mail.arc.nasa.gov, polack@ccr.jussieu.fr, len@lake.com.au, warren.dale@eng.sun.com, Tapio.Lokki@hut.fi, Matti.Karjalainen@hut.fi, Ville.Pulki@hut.fi, jmjot@emu.com, jyri.huopaniemi@research.nokia.com, jos@ccrma.stanford.edu, andrew.rimell@bt.com, mab@dtstech.com, rinus@akst.tn.tudelft.nl, pope@cs.bris.ac.uk, alan@cs.bris.ac.uk, tsingos@research.bell-labs.com, cwendt@research.bell-labs.com, funk@cs.princeton.edu, marc.emerit@cnet.francetelecom.fr, eckel@gmd.de, Nick.Sacharov@research.nokia.com, info@catt.se, odeon@dat.dtu.dk, George.Drettakis@sophia.inria.fr, jc.lombardo@cstb.fr, j.martin@cstb.fr, billg@media.mit.edu, mcm@mit.edu, dorsey@lcs.mit.edu, carlbom@research.bell-labs.com, hodgson@mech.ubc.ca, central@aea.ruhr-uni-bochum.de, farina@pcfarina.eng.unipr.it, jmt@atc.creative.com, Jean-Dominique.Gascuel@imag.fr, tta@cs.hut.fi, titakala@helsinki.fi, hahn@seas.gwu.edu, emb@dolby.com, nsincaglia@usa.net, srebaud@usa.net, Olivier.Warusfel@ircam.fr, gabillet@cstb.fr, gwe@research.bell-labs.com Subject: ACM SIGGRAPH/EUROGRAPHICS CAMPFIRE ON ACOUSTICS RENDERING X-Loop: globillum@imag.fr X-Sequence: 35 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: dL0"!^1S!!;`2"!cgR!! X-Mozilla-Status: 9001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit -------------------------------------------- ACM Special Interest Group on Computer Graphics and Interactive Techniques. European Computer Graphics Association. CALL FOR INTEREST Joint ACM SIGGRAPH/EUROGRAPHICS Campfire on ACOUSTICS RENDERING FOR VIRTUAL ENVIRONMENTS -------------------------------------------- Organizers: Nicolas Tsingos (Bell Labs) Alan Chalmers (Bristol University) -------------------------------------------- We have been invited to submit a proposal for an ACM SIGGRAPH/EUROGRAPHICS campfire, which is a small focused workshop which facilitates detailed discussion about interdisciplinary themes: http://www.siggraph.org/special-projects/campfires/index.html The theme of our proposed campfire is : "Acoustics rendering for virtual environments" It will be held in Snowbird, Utah (minutes from Salt Lake City) circa May 12th-15th 2001. We propose to divide the campfire into the following panels/sessions during 3 days: - Interactive simulation: Real-time acoustic simulation techniques, efficient geometrical techniques for acoustics - Perception: Audio/visual interaction in virtual worlds and combined audio/visual perception. Psycho-acoustics of sound reverberation, diffraction, etc. - Hardware and programming: Audio processing hardware and virtual acoustics API's. - DSP and audio technology: Real-time Digital Signal Processing techniques and audio reproduction techniques (surround sound, etc.) - Systems and applications: Virtual reality audio/visual system integration and applications. This is the first call for expressions of interest in such an event. If you think you would like to attend, please reply to this email as soon as possible. If you would like to suggest themes or organise some sessions, let us know. We hope to include a diverse group of participants whose interests span a wide range of disciplines, so please feel free to pass this on to any interested parties. We are looking forward to your reply, Best Regards, Nicolas Tsingos and Alan Chalmers -- ------------------------------------------------------------------- Nicolas Tsingos Visual Communications Research Bell Laboratories, Room 2D-509 Tel. : (908) 582 2638 600-700 Mountain Avenue Fax : (908) 582 7308 Murray Hill NJ 07974 USA tsingos@research.bell-labs.com http://www.bell-labs.com/~tsingos ------------------------------------------------------------------- ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by christl.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id PAA31345; Mon, 18 Dec 2000 15:48:22 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.11.1/8.11.1) with ESMTP id eBIEnDf16033; Mon, 18 Dec 2000 15:49:13 +0100 (MET) Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id PAA03679; Mon, 18 Dec 2000 15:48:24 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id PAA03674 for ; Mon, 18 Dec 2000 15:48:20 +0100 Received: from nut.autodesk.com ([198.102.112.27]) by imag.imag.fr (8.9.3/8.8.6) with ESMTP id PAA23993 for ; Mon, 18 Dec 2000 15:48:18 +0100 (MET) From: eric.haines@autodesk.com Received: from hqmsgsrf00.autodesk.com (hqmsgsrf00.autodesk.com [144.111.216.79]) by nut.autodesk.com (8.9.3/8.9.3) with ESMTP id GAA14632 for ; Mon, 18 Dec 2000 06:48:17 -0800 (PST) Received: by hqmsgsrf00.autodesk.com with Internet Mail Service (5.5.2448.0) id ; Mon, 18 Dec 2000 06:48:16 -0800 Message-ID: <19879C753611D3119DAB0008C7A4C0C106A1DCA3@hqmsgsrf04.autodesk.com> To: globillum@imag.fr Subject: Fantasy Graphics League - LOST ENTRIES Date: Mon, 18 Dec 2000 06:48:15 -0800 MIME-Version: 1.0 X-Mailer: Internet Mail Service (5.5.2448.0) X-Loop: globillum@imag.fr X-Sequence: 37 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: Po~"!%!W"!7?D!!7M)#! X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit No hanging chads, but rather a hanging /usr/lib/sendmail due to a server switch by the ISP (I guess that's to be expected when they charge only $2.99/month), has caused the Fantasy Graphics League to lose all entries dating from December 6th to December 16th. Foo. So, if you entered during this time, please re-enter. You can tell if your entry did not get registered by either just asking me (erich@acm.org), or by checking if you received a confirmation note from me entitled "FGL submission" - if you didn't, your entry's in the /dev/null bit bucket and you should re-enter. The Fantasy Graphics League is at: http://www.realtimerendering.com/fgl and is a free contest to choose a laboratory of computer graphics researchers. You have a budget, limited office space, and your goal is to choose the best team of real researchers to create an imaginary lab. The lab is then judged by what papers the real researchers have accepted for SIGGRAPH 2001. Deadline's the same as SIGGRAPH: January 10, 2001. We made this contest for the fun of it - we're not building up a spam list, or trying to sell you love pills or laserjet ink, we're just a bunch of guys with a silly idea and some time to follow through on it. Have fun, or else you won't, Eric ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by christl.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id VAA18264; Tue, 19 Dec 2000 21:02:31 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.11.1/8.11.1) with ESMTP id eBJK3Of03528; Tue, 19 Dec 2000 21:03:24 +0100 (MET) Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id VAA07761; Tue, 19 Dec 2000 21:02:35 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id VAA07756 for ; Tue, 19 Dec 2000 21:02:31 +0100 Received: from nut.autodesk.com (nut.autodesk.com [198.102.112.27]) by imag.imag.fr (8.9.3/8.8.6) with ESMTP id VAA20761 for ; Tue, 19 Dec 2000 21:02:30 +0100 (MET) From: eric.haines@autodesk.com Received: from hqmsgsrf00.autodesk.com (hqmsgsrf00.autodesk.com [144.111.216.79]) by nut.autodesk.com (8.9.3/8.9.3) with ESMTP id MAA19732 for ; Tue, 19 Dec 2000 12:02:29 -0800 (PST) Received: by hqmsgsrf00.autodesk.com with Internet Mail Service (5.5.2448.0) id ; Tue, 19 Dec 2000 12:02:28 -0800 Message-ID: <19879C753611D3119DAB0008C7A4C0C106A1E360@hqmsgsrf04.autodesk.com> To: globillum@imag.fr Subject: Lighting design glossary Date: Tue, 19 Dec 2000 12:02:23 -0800 MIME-Version: 1.0 X-Mailer: Internet Mail Service (5.5.2448.0) X-Loop: globillum@imag.fr X-Sequence: 38 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: b[k"!6k$"!PdW!!$X:!! X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit I just ran across this, and thought I'd pass it along: http://www.schorsch.com/kbase/glossary/index.html a glossary of the various terms used in the area of lighting and related fields. Reasonably done, though nothing deep. There are certainly a few I've never heard of before (e.g. "etendue"). The resources page: http://www.schorsch.com/kbase/resources/index.html also looks useful. The site is maintained by a one-person company making a platform independent GUI for Radiance (called Rayfront). Eric ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by christl.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id QAA04909; Sun, 31 Dec 2000 16:54:47 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.11.1/8.11.1) with ESMTP id eBVFtff24891; Sun, 31 Dec 2000 16:55:41 +0100 (MET) Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id QAA08196; Sun, 31 Dec 2000 16:54:50 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id QAA08191 for ; Sun, 31 Dec 2000 16:54:39 +0100 Received: from smartmail2.idirecthosting.com (smartmail2.easyhosting.com [207.136.80.73]) by imag.imag.fr (8.9.3/8.8.6) with ESMTP id QAA23334 for ; Sun, 31 Dec 2000 16:54:38 +0100 (MET) Received: from byheart (bc-van-wvn-a53-01-64.look.ca [216.66.156.160]) by smartmail2.idirecthosting.com (8.11.1/8.9.3) with SMTP id eBVFsQe65400 for ; Sun, 31 Dec 2000 10:54:30 -0500 (EST) Message-ID: <000c01c07341$ac4bef60$a09c42d8@byheart> Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: 01/01/01 Release of RADBIB and GITHESIS Date: Sun, 31 Dec 2000 07:52:19 -0800 Organization: byHeartConsultants Limited MIME-Version: 1.0 Content-Type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 5.50.4522.1200 X-MimeOLE: Produced By Microsoft MimeOLE V5.50.4522.1200 X-Loop: globillum@imag.fr X-Sequence: 39 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: X-UIDL: n(K!!7"o!!38I!!\AH!! X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit
ANNOUNCE: 01/01/01 Release of RADBIB and GITHESIS
-------------------------------------------------
RADBIB is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. It currently includes 1,847 references -- 7 new additions since its 00/12/01 release.
 
This bibliography is available in BibTex format as RADBIB.BIB (with a release date of January 1, 2001) from:
 
  http://www.helios32.com (Resources section)
 
Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 237 references to radiosity and global illumination theses -- four new additions since the 00/12/01 release.
 
Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.
 
PS - Happy New Millenium!
Ian Ashdown, P. Eng., LC, FIES
Chief Technology Officer
byHeart Consultants Limited
http://www.helios32.com
From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by christl.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id XAA08267; Wed, 3 Jan 2001 23:38:00 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.11.1/8.11.1) with ESMTP id f03Mctf14645; Wed, 3 Jan 2001 23:38:55 +0100 (MET) Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id XAA13030; Wed, 3 Jan 2001 23:38:03 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id XAA13025 for ; Wed, 3 Jan 2001 23:37:59 +0100 Received: from bach.Graphics.Cornell.EDU (bach.graphics.cornell.edu [128.84.247.50]) by imag.imag.fr (8.9.3/8.8.6) with ESMTP id XAA15609 for ; Wed, 3 Jan 2001 23:37:58 +0100 (MET) Received: from DIESEL (diesel.graphics.cornell.edu [128.84.247.211]) by bach.Graphics.Cornell.EDU (8.9.1/8.9.1) with ESMTP id RAA16928; Wed, 3 Jan 2001 17:37:55 -0500 (EST) (envelope-from westin@graphics.cornell.edu) Date: Wed, 3 Jan 2001 17:37:54 -0500 (EST) Message-Id: <200101032237.RAA16928@bach.Graphics.Cornell.EDU> From: "Stephen H. Westin" To: globillum@imag.fr cc: ket1@cornell.edu, dpg@Graphics.Cornell.EDU, jcr@Graphics.Cornell.EDU Subject: BRDF data now available in text format Reply-to: westin@Graphics.Cornell.EDU X-Loop: globillum@imag.fr X-Sequence: 40 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: 6O2!!NM;"!7E<"!~,M!! X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 MIME-Version: 1.0 Content-transfer-encoding: 8bit This is a multi-part message in MIME format... ------------=_978561483-10469-1 I have just added a few new files to Cornell's online collection of BRDF data. No new datasets have been added, but most datasets are now in a text format for easier decoding (previously only MATLAB workspace files were available). In addition, I have converted these datasets from a wavelength-resolved format (with 31 wavelengths) to CIE XYZ tristimulus values as well as RGB values for a Sony Trinitron monitor. The text format is based on Appendix X3 of ASTM Standard E1392-96, "Standard Practice for Angle Resolved Optical Scatter Measurements on Specular or Diffuse Surface". I have no way to test my compliance with this standard, as I have not been able to find any sample data files in this format, nor any software that reads it. I welcome any corrections as to the format of these files. The files are available at ; the new files are for the datasets acryl_blue, garnet_red, krylon_blue, mystique, and cayman. Stephen H. Westin Research Project Leader Program of Computer Graphics Cornell University westin@graphics.cornell.edu 607 255 9080 (VOX) 607 255 0806 (FAX) ------------=_978561483-10469-1 Content-Type: text/plain; name="message.footer" Content-Disposition: inline; filename="message.footer" Content-Transfer-Encoding: 8bit ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- ------------=_978561483-10469-1-- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by christl.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id TAA03490; Fri, 5 Jan 2001 19:08:13 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.11.1/8.11.1) with ESMTP id f05I98c22657; Fri, 5 Jan 2001 19:09:09 +0100 (MET) Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id TAA19313; Fri, 5 Jan 2001 19:08:11 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id TAA19308 for ; Fri, 5 Jan 2001 19:08:08 +0100 Received: from bach.Graphics.Cornell.EDU (bach.graphics.cornell.edu [128.84.247.50]) by imag.imag.fr (8.9.3/8.8.6) with ESMTP id TAA05904 for ; Fri, 5 Jan 2001 19:08:06 +0100 (MET) Received: from DIESEL (diesel.graphics.cornell.edu [128.84.247.211]) by bach.Graphics.Cornell.EDU (8.9.1/8.9.1) with ESMTP id NAA08235 for ; Fri, 5 Jan 2001 13:08:04 -0500 (EST) (envelope-from westin@graphics.cornell.edu) Date: Fri, 5 Jan 2001 13:08:03 -0500 (EST) Message-Id: <200101051808.NAA08235@bach.Graphics.Cornell.EDU> From: "Stephen H. Westin" To: globillum@imag.fr Subject: Corrected BRDF text-format data Reply-to: westin@Graphics.Cornell.EDU X-Loop: globillum@imag.fr X-Sequence: 41 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: *NJ!!B<;!!L%Q!!gK?"! X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 MIME-Version: 1.0 Content-transfer-encoding: 8bit This is a multi-part message in MIME format... ------------=_978718090-16594-0 Well, Michael McCool graciously pointed out that all my files were truncated; I believe that's fixed now. If you downloaded any of the ASTM-format BRDF files (compressed or not) before about 1:00PM EST (about 18:00 UTC), you need to get them again. As before, the page is at . Stephen H. Westin Research Project Leader Program of Computer Graphics Cornell University westin@graphics.cornell.edu 607 255 9080 (VOX) 607 255 0806 (FAX) ------------=_978718090-16594-0 Content-Type: text/plain; name="message.footer" Content-Disposition: inline; filename="message.footer" Content-Transfer-Encoding: 8bit ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- ------------=_978718090-16594-0-- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by christl.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id PAA25769; Tue, 9 Jan 2001 15:14:59 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.11.1/8.11.1) with ESMTP id f09EFpc07418; Tue, 9 Jan 2001 15:15:51 +0100 (MET) Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id PAA26995; Tue, 9 Jan 2001 15:14:58 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id PAA26990 for ; Tue, 9 Jan 2001 15:14:53 +0100 Received: from nut.autodesk.com ([198.102.112.27]) by imag.imag.fr (8.9.3/8.8.6) with ESMTP id PAA09317 for ; Tue, 9 Jan 2001 15:14:51 +0100 (MET) From: eric.haines@autodesk.com Received: from hqmsgsrf00.autodesk.com (hqmsgsrf00.autodesk.com [144.111.216.79]) by nut.autodesk.com (8.9.3/8.9.3) with ESMTP id GAA22894 for ; Tue, 9 Jan 2001 06:14:46 -0800 (PST) Received: by hqmsgsrf00.autodesk.com with Internet Mail Service (5.5.2448.0) id ; Tue, 9 Jan 2001 06:14:45 -0800 Message-ID: <19879C753611D3119DAB0008C7A4C0C106D18316@hqmsgsrf04.autodesk.com> To: globillum@imag.fr Subject: Fantasy Graphics League - last chance Date: Tue, 9 Jan 2001 06:14:45 -0800 MIME-Version: 1.0 X-Mailer: Internet Mail Service (5.5.2448.0) X-Loop: globillum@imag.fr X-Sequence: 42 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: W/,!!\4&"!SG,!!&VO!! X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit It's your last chance to enter the Fantasy Graphics League; the SIGGRAPH paper deadline is January 10th, as is the League's. Choose a team of researchers within budget and space limitations, trying to be the most productive graphics lab in the virtual world. Win great prizes (somewhere else), and attain unheard of fame in your own lifetime (we promise you won't be heard of, at least not from us). It's free, pointless, and fun, and we won't even spam you later: http://www.realtimerendering.com/fgl/ Have fun, or else you won't, Eric ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by christl.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id XAA14953; Wed, 10 Jan 2001 23:48:39 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.11.1/8.11.1) with ESMTP id f0AMnac18093; Wed, 10 Jan 2001 23:49:36 +0100 (MET) Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id XAA32749; Wed, 10 Jan 2001 23:48:43 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id XAA32744 for ; Wed, 10 Jan 2001 23:48:38 +0100 Received: from bach.Graphics.Cornell.EDU (bach.graphics.cornell.edu [128.84.247.50]) by imag.imag.fr (8.9.3/8.8.6) with ESMTP id XAA26071 for ; Wed, 10 Jan 2001 23:48:37 +0100 (MET) Received: from graphics.cornell.edu (bray.graphics.cornell.edu [128.84.247.212]) by bach.Graphics.Cornell.EDU (8.9.1/8.9.1) with ESMTP id RAA02335; Wed, 10 Jan 2001 17:48:33 -0500 (EST) (envelope-from phil@graphics.cornell.edu) Message-ID: <3A5CE5D4.FD688FE7@graphics.cornell.edu> Date: Wed, 10 Jan 2001 17:44:36 -0500 From: Phil Dutre Organization: Program of Computer Graphics X-Mailer: Mozilla 4.73 [en] (WinNT; U) X-Accept-Language: en MIME-Version: 1.0 Newsgroups: comp.graphics.rendering.misc,comp.graphics.algorithms To: globillum@imag.fr CC: graphics@Graphics.Cornell.EDU Subject: Global Illumination Compendium X-Loop: globillum@imag.fr X-Sequence: 43 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: NJ\"!^_)!!Z)2!!')Q!! X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit A slightly updated version of the global illumination compendium is available at http://www.graphics.cornell.edu/~phil/GI/ Philip Dutre ======================================================================= This page contains the Global Illumination Compendium, an effort to bring together most of the useful formulas and equations for global illumination algorithms in computer graphics. This collection of formulas and equations is supposed to be useful for anyone who is active in the field of global illumination in computer graphics. The specific selection is made on an ‘as we go’ basis, adding more items if necessary. This compendium does not claim to be complete. Any further input and suggestions for more useful content are therefore strongly appreciated. If possible, adequate references are given to look up some of the equations in more detail, or to look up the derivations. ======================================================================= -- ======================================================================= Philip Dutre Program of Computer Graphics Cornell University phil@graphics.cornell.edu http://www.graphics.cornell.edu/~phil/ ======================================================================= ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by christl.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id UAA01473; Tue, 16 Jan 2001 20:49:46 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.11.1/8.11.1) with ESMTP id f0GJohc29843; Tue, 16 Jan 2001 20:50:43 +0100 (MET) Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id UAA17552; Tue, 16 Jan 2001 20:49:49 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id UAA17547 for ; Tue, 16 Jan 2001 20:49:46 +0100 Received: from bach.Graphics.Cornell.EDU (bach.graphics.cornell.edu [128.84.247.50]) by imag.imag.fr (8.9.3/8.8.6) with ESMTP id UAA16679 for ; Tue, 16 Jan 2001 20:49:45 +0100 (MET) Received: from DIESEL (diesel.graphics.cornell.edu [128.84.247.211]) by bach.Graphics.Cornell.EDU (8.9.1/8.9.1) with ESMTP id OAA04284; Tue, 16 Jan 2001 14:49:42 -0500 (EST) (envelope-from westin@graphics.cornell.edu) Date: Tue, 16 Jan 2001 14:49:41 -0500 (EST) Message-Id: <200101161949.OAA04284@bach.Graphics.Cornell.EDU> From: "Stephen H. Westin" To: globillum@imag.fr cc: ket1@cornell.edu, dpg@Graphics.Cornell.EDU, jcr@Graphics.Cornell.EDU Subject: More BRDF data available online Reply-to: westin@Graphics.Cornell.EDU X-Loop: globillum@imag.fr X-Sequence: 44 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: Fo*!!ZUM"!`h`!!;. The following data sets have been added. Gonioreflectometer data (31 wavelengths, ~1500 samples): o 5 new samples of wall paint, ranging from black through gray to white Image-based data (RGB, >300K samples), captured for the paper Image-based brdf measurement including human skin. Stephen R. Marschner, Stephen H. Westin, Eric P. F. Lafortune, Kenneth E. Torrance, and Donald P. Greenberg. Presented at Eurographics Workshop on Rendering, 1999. o A clay pot depicted in Plate 1 of the 1999 SIGGRAPH paper o Gray Krylon primer, used for the floor plane in Plate 1 o Black felt, used for the hat in Plate 1 These datasets also are represented as coefficients for the Lafortune BRDF representation (SIGGRAPH 97). More datasets will be added as time allows. Stephen H. Westin Research Project Leader Program of Computer Graphics Cornell University westin@graphics.cornell.edu 607 255 9080 (VOX) 607 255 0806 (FAX) ------------=_979674588-12540-0 Content-Type: text/plain; name="message.footer" Content-Disposition: inline; filename="message.footer" Content-Transfer-Encoding: 8bit ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- ------------=_979674588-12540-0-- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by christl.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id UAA29763; Sat, 27 Jan 2001 20:41:28 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.11.1/8.11.1) with ESMTP id f0RJgP226561; Sat, 27 Jan 2001 20:42:25 +0100 (MET) Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id UAA16286; Sat, 27 Jan 2001 20:41:31 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id UAA16281 for ; Sat, 27 Jan 2001 20:41:14 +0100 Received: from rabacal.direct.ca (rabacal.direct.ca [199.60.229.8]) by imag.imag.fr (8.9.3/8.8.6) with ESMTP id UAA01985 for ; Sat, 27 Jan 2001 20:41:12 +0100 (MET) Received: from bc-van-wvn-a53-01-54.look.ca ([216.66.156.150] helo=byheart) by rabacal.direct.ca with smtp (Exim 2.12 #7) id 14MbDh-0002ag-00 for globillum@imag.fr; Sat, 27 Jan 2001 11:41:09 -0800 Message-ID: <001501c08898$62c29620$969c42d8@byheart> Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: 01/02/01 Release of RADBIB and GITHESIS Date: Sat, 27 Jan 2001 11:36:02 -0800 Organization: byHeartConsultants Limited MIME-Version: 1.0 Content-Type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 5.50.4522.1200 X-MimeOLE: Produced By Microsoft MimeOLE V5.50.4522.1200 X-Loop: globillum@imag.fr X-Sequence: 45 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: X-UIDL: Mm;"!U^,#!Na=!!-6k"! X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit
ANNOUNCE: 01/02/01 Release of RADBIB and GITHESIS
-------------------------------------------------
RADBIB is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. It currently includes 1,870 references -- 23 new additions since its 01/01/01 release.
 
This bibliography is available in BibTex format as RADBIB.BIB (with a release date of February 1, 2001) from:
 
  http://www.helios32.com (Resources section)
 
Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 237 references to radiosity and global illumination theses -- no new additions since the 01/01/01 release.
 
Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.
 
Ian Ashdown, P. Eng., LC, FIES
Chief Technology Officer
byHeart Consultants Limited
http://www.helios32.com
From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by christl.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id RAA29348; Tue, 6 Feb 2001 17:52:10 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.11.1/8.11.1) with ESMTP id f16Gr8j13692; Tue, 6 Feb 2001 17:53:08 +0100 (MET) Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id RAA19599; Tue, 6 Feb 2001 17:52:10 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id RAA19594 for ; Tue, 6 Feb 2001 17:52:01 +0100 Received: from crufty.research.bell-labs.com (crufty.research.bell-labs.com [204.178.16.49]) by imag.imag.fr (8.9.3/8.8.6) with SMTP id RAA09673; Tue, 6 Feb 2001 17:51:35 +0100 (MET) Received: from mcs.research.bell-labs.com ([135.104.32.15]) by crufty; Tue Feb 6 11:48:28 EST 2001 Received: from research.bell-labs.com (solar.research.bell-labs.com [135.104.34.67]) by mcs.research.bell-labs.com (8.8.8/8.8.8) with ESMTP id LAA09407; Tue, 6 Feb 2001 11:48:31 -0500 (EST) Sender: tsingos@research.bell-labs.com Message-ID: <3A802ADC.811A36A6@research.bell-labs.com> Date: Tue, 06 Feb 2001 11:48:28 -0500 From: Nicolas Tsingos X-Mailer: Mozilla 4.7C-SGI [en] (X11; I; IRIX64 6.5 IP30) X-Accept-Language: en MIME-Version: 1.0 To: Ingrid Carlbom , Thomas Funkhouser , Jean-Dominique Gascuel , globillum , db , dg , bwenzel , polack , len , "warren.dale" , "Tapio.Lokki" , "Matti.Karjalainen" , "Ville.Pulki" , jmjot , "jyri.huopaniemi" , jos , "andrew.rimell" , mab , rinus , pope , alan , tsingos , cwendt , "marc.emerit" , eckel , "Nick.Sacharov" , info , odeon , "George.Drettakis" , "jc.lombardo" , jmartin , billg , mcm , dorsey , hodgson , central , farina , jmt , tta , titakala , hahn , emb , nsincaglia , srebaud , "Olivier.Warusfel" , shinn , "w.davies" , sullivan , "d.murphy" , dlubman , "D.McGrath" , pai , "marc.emerit" , dombois , "Francois.Sillion" , fyluo_99 , fouads , ian_ashdown , Day_J , jmj , adrian , jm-t , kadi , mgriffin , mk , "P.Flanagan" , rendell , petersen , rstorms , "s.a.rizzi" , ktlokki , "robert.s.wall" , wlm , "y.zhang1" , "noel.chateau" , lcerveau , jaron , dev , dan , cruz , tom , jiashuchen , kurt , "Veronique.Larcher" , "J.G.Beerends" , kahrs , jeanl Subject: AUDIO RENDERING CAMPFIRE - CALL FOR PARTICIPATION X-Loop: globillum@imag.fr X-Sequence: 46 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: #)Y"!1Kk!!/pN!!7:!"! X-Mozilla-Status: 9001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit --------------------------------------------------------------------------- ACM Special Interest Group on Computer Graphics and Interactive Techniques. European Computer Graphics Association. *** CALL FOR PARTICIPATION *** Joint ACM SIGGRAPH/EUROGRAPHICS Campfire on ACOUSTIC RENDERING FOR VIRTUAL ENVIRONMENTS http://www.bell-labs.com/topic/conferences/campfire/ May 26th-29th, Snowbird, Utah, USA ** Registration deadline is March 9, 2001. ** --------------------------------------------------------------------------- Co-Chairs: Nicolas Tsingos (Bell Labs) Alan Chalmers (Bristol University) --------------------------------------------------------------------------- ACM SIGGRAPH and EUROGRAPHICS are sponsoring a small workshop (campfire) on "Acoustic rendering for virtual environments". The main aims of the Campfire are: sharing information and forging new research directions. Because of the interesting mix of disciplines, there will be both introductory information-sharing sessions and more focused panels and presentations which will concentrate on the challenges of this interdisciplinary domain. The event will be held in Snowbird, Utah (minutes from Salt Lake City) on May 26th-29th 2001 (Memorial weekend). PROPOSED TOPICS --------------- We suggest the following topics as a basis for submission/discussion: - Simulation: real-time acoustic simulation techniques, efficient geometrical techniques for acoustics, validation - Perception: audio/visual interaction in virtual worlds and combined audio/visual perception. Psycho-acoustics of sound reverberation, diffraction, etc. - Hardware and programming: audio processing hardware and virtual acoustics APIs. - DSP and audio technology: real-time digital signal processing techniques and audio reproduction techniques (surround sound, etc.) - Systems and applications: virtual reality audio/visual system integration and applications. SUBMISSION & REGISTRATION ------------------------- All attendees are required to compose a short position paper (1-5 pages), indicating their area of expertise, what they would like to learn from the Campfire, and issues they wish to discuss. Please feel free to suggest additional topics to the proposed list. Places on the campfire are restricted, and will be allocated on a first-come, first-served basis. A place will be reserved for you upon receipt of your position paper. This will be confirmed once you have registered and paid the appropriate fee. Additional information regarding the campfire can be found at: http://www.bell-labs.com/topic/conferences/campfire/ You can submit your position paper online or email it to: tsingos@lucent.com ******************************************************************** * Deadline for submission of position papers is March 9, 2001. * ******************************************************************** Feel free to forward this call for participation to any interested party. We look forward to your participation and hope to see you soon in Utah, Best Regards, Nicolas Tsingos and Alan Chalmers -- ------------------------------------------------------------------- Nicolas TSINGOS Visual Communications Research Bell Laboratories, Room 2D-509 Tel. : (908) 582 2638 600-700 Mountain Avenue Fax : (908) 582 7308 Murray Hill NJ 07974 USA tsingos@research.bell-labs.com http://www.bell-labs.com/~tsingos ------------------------------------------------------------------- ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by christl.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id VAA31324; Tue, 13 Feb 2001 21:46:49 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.11.1/8.11.1) with ESMTP id f1DKllj25817; Tue, 13 Feb 2001 21:47:48 +0100 (MET) Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id VAA05380; Tue, 13 Feb 2001 21:46:41 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id VAA05375 for ; Tue, 13 Feb 2001 21:46:37 +0100 Received: from castor.host4u.net (castor.host4u.net [216.71.64.37]) by imag.imag.fr (8.9.3/8.8.6) with ESMTP id VAA18820 for ; Tue, 13 Feb 2001 21:46:36 +0100 (MET) Received: from djshivan ([212.166.211.72]) by castor.host4u.net (8.8.5/8.8.5) with ESMTP id OAA13846 for ; Tue, 13 Feb 2001 14:38:12 -0600 Date: Tue, 13 Feb 2001 21:48:04 +0100 From: =?windows-1252?Q?Juan_Carlos_Jim=E9nez?= To: globillum@imag.fr Subject: Help with my book (author from Spain) Message-Id: <20010213214623.1146.JCJIMENEZ@beneito.com> MIME-Version: 1.0 X-Mailer: Becky! ver. 2.00 (beta 34rc) X-MIME-Autoconverted: from quoted-printable to 8bit by chopinette.imag.fr id VAA05375 X-Loop: globillum@imag.fr X-Sequence: 48 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: `]_"!+ec!!_i Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id TAA13897; Tue, 17 Apr 2001 19:39:05 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id TAA32729; Tue, 17 Apr 2001 19:39:05 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id TAA32724 for ; Tue, 17 Apr 2001 19:39:01 +0200 Received: from mut.autodesk.com (mut.autodesk.com [198.102.112.26]) by imag.imag.fr (8.9.3/8.8.6) with ESMTP id TAA08325 for ; Tue, 17 Apr 2001 19:38:59 +0200 (MET DST) From: eric.haines@autodesk.com Received: from hqmsgsrf00.autodesk.com (hqmsgsrf00.autodesk.com [144.111.32.210]) by mut.autodesk.com (8.9.3/8.9.3) with ESMTP id KAA16006 for ; Tue, 17 Apr 2001 10:38:57 -0700 (PDT) Received: by hqmsgsrf00.autodesk.com with Internet Mail Service (5.5.2653.19) id <2JFTF7M6>; Tue, 17 Apr 2001 10:38:56 -0700 Message-ID: <19879C753611D3119DAB0008C7A4C0C10822B741@hqmsgsrf04.autodesk.com> To: globillum@imag.fr Subject: Fantasy Graphics League semi-results; and a question Date: Tue, 17 Apr 2001 10:38:54 -0700 MIME-Version: 1.0 X-Mailer: Internet Mail Service (5.5.2653.19) X-Loop: globillum@imag.fr X-Sequence: 50 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: G_^!!/&O"!:nV"!j=@"! X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Globillumers, Pharr's not far ahead, others are moving in on his crown. The initial, partial results for the 2nd Annual Fantasy Graphics League are up at http://www.realtimerendering.com/fgl/. A real thing: We talk about 72 FPS being a reasonably smooth refresh rate, though 85 FPS is better yet for large, bright screens. There is also experimental data for perception happening as fast as 1/220th of a second (see the end of the article at http://www.penstarsys.com/editor/30v60/30v60p1.htm). What I'm missing here is primary sources: does anyone have references to solid literature on what an acceptable/perceptible FPS rate is for computer monitors? There's obviously no hard and fast number, and it depends on what's being displayed, etc, but if there some good overview/summary of this area, some discussion of tradeoffs and limits, I would be happy to know of it. Eric ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id UAA13055; Sat, 28 Apr 2001 20:24:10 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id UAA28255; Sat, 28 Apr 2001 20:23:49 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id UAA28250 for ; Sat, 28 Apr 2001 20:23:46 +0200 Received: from rabacal.direct.ca (rabacal.direct.ca [199.60.229.8]) by imag.imag.fr (8.9.3/8.8.6) with ESMTP id UAA00982 for ; Sat, 28 Apr 2001 20:23:44 +0200 (MET DST) Received: from bc-van-wvn-a53-01-88.look.ca ([216.66.156.184] helo=chocolate) by rabacal.direct.ca with smtp (Exim 2.12 #7) id 14tZNZ-00026H-00 for globillum@imag.fr; Sat, 28 Apr 2001 11:23:40 -0700 Message-ID: <000a01c0d00f$b3d8f180$6000a8c0@chocolate> Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: 01/05/01 Release of RADBIB and GITHESIS Date: Sat, 28 Apr 2001 11:19:01 -0700 Organization: byHeartConsultants Limited MIME-Version: 1.0 X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 5.50.4522.1200 X-MimeOLE: Produced By Microsoft MimeOLE V5.50.4522.1200 X-Loop: globillum@imag.fr X-Sequence: 51 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: WMY!!9Ea"!npg!![_Q!! X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Prologue: It has been three months since the last (monthly) release of RADBIB and GITHESIS. My excuse is that I had to complete my MSc thesis ("Eigenvector Radiosity") before the end of this month. (I made the submission deadline with four hours to spare, thanks to the generous assistance of Drs. Wolfgang Heidrich and Paul Lalonde.) ANNOUNCE: 01/05/01 Release of RADBIB and GITHESIS ------------------------------------------------- RADBIB is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. It currently includes 1,899 references -- 29 new additions since its 00/02/01 release. This bibliography is available in BibTex format as RADBIB.BIB (with a release date of May 1, 2001) from: http://www.helios32.com (Resources section) Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 243 references to radiosity and global illumination theses -- 6 new additions since the 00/02/01 release. Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited. Ian Ashdown, P. Eng., LC, FIES Chief Technology Officer byHeart Consultants Limited http://www.helios32.com ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id RAA14152; Fri, 11 May 2001 17:35:14 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id RAA24747; Fri, 11 May 2001 17:35:08 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id RAA24742 for ; Fri, 11 May 2001 17:35:01 +0200 Received: from ns.felk.cvut.cz (ns.felk.cvut.cz [147.32.80.9]) by imag.imag.fr (8.9.3/8.8.6) with ESMTP id RAA20375 for ; Fri, 11 May 2001 17:34:58 +0200 (MET DST) Received: from mira1.felk.cvut.cz (IDENT:havran@mira1.felk.cvut.cz [147.32.80.171]) by ns.felk.cvut.cz (8.11.3/8.9.3) with ESMTP id f4BFYvW45357 for ; Fri, 11 May 2001 17:34:57 +0200 (MET DST) (envelope-from havran@fel.cvut.cz) Date: Fri, 11 May 2001 17:37:46 +0200 (CEST) From: havran X-Sender: To: globillum@imag.fr Subject: Dissertation: Heuristic Ray Shooting Algorithms Message-ID: MIME-Version: 1.0 X-Loop: globillum@imag.fr X-Sequence: 54 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: dH8!!cjQ"!T>?!!Bk7!! X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hi everyone, my Ph.D. Thesis, "Heuristic Ray Shooting Algorithms", defended on 20 April 2001, can be downloaded at: http://www.cgg.cvut.cz/~havran/phdthesis.html Any comments are welcome by e-mail to VHavran@seznam.cz. Sincerely, Vlastimil Havran http://www.cgg.cvut.cz/~havran -------------------------------------------------------------------------- Abstract: Global illumination research aiming at the photo-realistic image synthesis pushes forward research in computer graphics as a whole. The computation of visually plausible images is time-consuming and far from being realtime at present. A significant part of computation in global illumination algorithms involves repetitive computing of visibility queries. In the thesis, we describe our results in ray shooting, which is a well-known problem in the field of visibility. The problem is difficult in spite of its simple definition: For a given oriented half-line and a set of objects, find out the first object intersected by the half-line if such an object exists. A naive algorithm has the time complexity $O(N)$, where $N$ is the number of objects. The naive algorithm is practically inapplicable in global illumination applications for a scene with a high number of objects, due its huge time requirements. In this thesis we deal with heuristic ray shooting algorithms that use additional spatial data structures. We put stress on average-case complexity and we particularly investigate the ray shooting algorithms based on spatial hierarchies. In the thesis we deal with two major topics. In the first part of the thesis, we introduce a ray shooting computation model and performance model. Based on these two models we develop a methodology for comparing various ray shooting algorithms for a set of experiments performed on a set of scenes. Consecutively, we compare common heuristic ray shooting algorithms based on BSP trees, kd-trees, octrees, bounding volume hierarchies, uniform grids, and three types of hierarchical grids using a set of 30 scenes from Standard Procedural Database. We show that for this set of scenes the ray shooting algorithm based on the kd-tree is the winning candidate among all tested ray shooting algorithms. The second and major part of the thesis presents several techniques for decreasing the time and space complexity for ray shooting algorithms based on kd-tree. We deal with both kd-tree construction and ray traversal algorithms. In the context of kd-tree construction, we present new methods for adaptive construction of the kd-tree using empty spatial regions in the scene, termination criteria, general cost model for the kd-tree, and modified surface area heuristics for a restricted set of rays. Further, we describe a new version of the recursive ray traversal algorithm. In context of the recursive ray traversal algorithm based on the kd-tree, we develop the concept of the largest common traversal sequence. This reduces the number of hierarchical traversal steps in the kd-tree for certain ray sets. We also describe one technique closely related to computer architecture, namely mapping kd-tree nodes to memory to increase the cache hit ratio for processors with a large cache line. Most of the techniques proposed in the thesis can be used in combination. In practice, the average time complexity of the ray shooting algorithms based on the kd-tree, as presented in this thesis, is about $O(log N)$, where the hidden multiplicative factor depends on the input data. However, at present it is not known to have been proved theoretically for scenes with general distribution of objects. For these reasons our findings are supported by a set of experiments for the above-mentioned set of 30 scenes. ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id BAA21187; Wed, 16 May 2001 01:07:16 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id BAA02355; Wed, 16 May 2001 01:07:11 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id BAA02350 for ; Wed, 16 May 2001 01:07:04 +0200 Received: from edam.direct.ca (edam.direct.ca [199.60.229.6]) by imag.imag.fr (8.9.3/8.8.6) with ESMTP id BAA04003 for ; Wed, 16 May 2001 01:07:02 +0200 (MEST) Received: from bc-van-wvn-a53-01-86.look.ca ([216.66.156.182] helo=chocolate) by edam.direct.ca with smtp (Exim 2.12 #7) id 14znu7-0006QL-00; Tue, 15 May 2001 16:06:59 -0700 Message-ID: <002e01c0dd93$c7daa520$6000a8c0@chocolate> Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: globillum@imag.fr Subject: REQUEST FOR INFORMATION - Lighting & Luminaire Design Software Date: Tue, 15 May 2001 16:07:13 -0700 Organization: byHeartConsultants Limited MIME-Version: 1.0 X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 5.50.4522.1200 X-MimeOLE: Produced By Microsoft MimeOLE V5.50.4522.1200 X-Loop: globillum@imag.fr X-Sequence: 55 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: "F%#!bD8!!=64!!]f$#! X-Mozilla-Status: 8003 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit I know -- this message is a bit off-topic for our mailing list. (I posted it earlier today to sci.engr.lighting and sci.optics.) On the other hand, you may know of European or Far East companies (especially startups) that I somehow missed while doing my Web searches. Any assistance would be much appreciated. - Ian Ashdown REQUEST FOR INFORMATION - Lighting & Luminaire Design Software The IESNA Computer Committee (Illuminating Engineering Society of North America) is compiling its annual IESNA Software Survey for publication in a forthcoming issue of Lighting Design+Application magazine (www.iesna.org). This software survey will enumerate the features of lighting and luminaire design and analysis software products for architectural and roadway lighting applications. The Committee wishes to include information on products from as many software developers and manufacturers as possible. In particular, we are looking for companies worldwide --lighting and luminaire design software addresses a global market. The following list of companies, products and Web URLs is what the Committee has compiled to date from Web searches and previous surveys. WE ARE LOOKING FOR COMPANIES WE HAVE MISSED. If you are aware of a software developer or manufacturer that is not on this list, please contact: Ian Ashdown byHeart Consultants Limited ian_ashdown@helios32.com with the following information: 1. Product name 2. Company name. 3. Company Web URL. We will then contact the company and request that they complete a product survey. Thanking you on behalf of the IESNA Computer Committee, Ian Ashdown, P. Eng., LC, FIES Chief Technology Officer byHeart Consultants Limited http://www.helios32.com --------------- Lighting Design --------------- Lightscape - Autodesk (www.lightscape.com) LitePro - Columbia Lighting (www.columbia-ltg.com) Luxicon - Cooper Lighting (www.cooperltg.com) AccuRender, Flamingo - Robert McNeel & Associates (www.accurender.com) Genesys II -Canlyte (www.canlyte.com), Lightolier (www.lightolier.com) OptiWin - Glamox AS (www.glamox.com) RayFront - www.schorsch.com (www.schorsch.com) LIGHTPAD, BEEM - Electric Power Research Institute (www.epri.com) LightCalc- Enviro-Systems (www.lightcalc.com) Aladan - GE Lighting Systems (www.ge-lightingsystems.com) AUTOLUX - Independent Testing Laboratories (itl@boulder.net) Desktop Radiance - Lawrence Berkeley National Laboratory (http://radsite.lbl.gov/deskrad) Perfect Lite - Trevor Caswell Software (http://www.powerup.com.au/~trevorc/index.htm) FOTOCAT - Wellmade Products (www.wlmd.com) Olivia, Fiona - Ray Forge Services (www.ozemail.com.au/~rayforge) AGI32, Photometric Toolbox - Lighting Analysts Inc. (www.lightinganalysts.com) Lumen Micro 2000, Simply Economics, Simply Lighting, Simply Roadway - Lighting Technologies, Inc. (www.lightingtechnologies.com) Lightworks - Lightwork Design Ltd. (www.lightwork.com) Visual, Photometric Viewer, TEMPLIT - Lithonia Lighting (www.lithonia.com) Speos - Optis (www.optis.fr) Martin ShoweDesigner - Martin Professional (www.martinpro.com) Worldlyte - Worldlyte (www.worldlyte.com) Relux, LumEdit -Relux Informatik AG (www.relux.ch) DIALux - Dial GmbH (www.dial.de) Pytha - Pytha (www.pytha.com) Ecolumen - Tata Infotech (www.tatainfotech.com) LiteStar, Lite, PhotoWin - OxyTech Srl (www.oxytech.it) Luminaire Design ---------------- ASAP, ReflectorCAD - Breault Research (www.breault.com) OSLO, TracePro - Lambda Research Corp. (www.lambdares.com) RayMaster - Lighting Sciences Inc. (www.lightingsciences.com) LightTools - Optical Research Associates (www.opticalres.com) Photopia - Lighting Technologies, Inc. (www.lightingtechnologies.com) Solstis, Speos, Light, OptiCalc - Optis (www.optis.fr) Zelum - Focus Software (www.focus-software.com) RoadRunner - Acme Optics (www.acmeoptics.com) ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Message-Id: To: "Ian Ashdown" From: Werner Purgathofer Subject: Re: REQUEST FOR INFORMATION - Lighting & Luminaire Design Software In-Reply-To: <002e01c0dd93$c7daa520$6000a8c0@chocolate> X-Eudora-Signature: X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Date: Wed, 16 May 2001 08:20:40 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Dear Ian, I am not sure if this company (Zumtobel) is completely in your scope, but I guess it is close enough. See: http://www.zumtobel.at/display.asp?s=2&m=3&p=1&language=en Best regards, Werner At 04:07 PM 5/15/01 -0700, you wrote: >I know -- this message is a bit off-topic for our mailing list. (I posted it >earlier today to sci.engr.lighting and sci.optics.) On the other hand, you >may know of European or Far East companies (especially startups) that I >somehow missed while doing my Web searches. Any assistance would be much >appreciated. > >- Ian Ashdown > >REQUEST FOR INFORMATION - Lighting & Luminaire Design Software > >The IESNA Computer Committee (Illuminating Engineering Society of North >America) is compiling its annual IESNA Software Survey for publication in a >forthcoming issue of Lighting Design+Application magazine (www.iesna.org). > >This software survey will enumerate the features of lighting and luminaire >design and analysis software products for architectural and roadway lighting >applications. > >The Committee wishes to include information on products from as many >software developers and manufacturers as possible. In particular, we are >looking for companies worldwide --lighting and luminaire design software >addresses a global market. > >The following list of companies, products and Web URLs is what the Committee >has compiled to date from Web searches and previous surveys. > >WE ARE LOOKING FOR COMPANIES WE HAVE MISSED. If you are aware of a software >developer or manufacturer that is not on this list, please contact: > >Ian Ashdown >byHeart Consultants Limited >ian_ashdown@helios32.com > >with the following information: > >1. Product name >2. Company name. >3. Company Web URL. > >We will then contact the company and request that they complete a product >survey. > >Thanking you on behalf of the IESNA Computer Committee, > >Ian Ashdown, P. Eng., LC, FIES >Chief Technology Officer >byHeart Consultants Limited >http://www.helios32.com > >--------------- >Lighting Design >--------------- >Lightscape - Autodesk (www.lightscape.com) >LitePro - Columbia Lighting (www.columbia-ltg.com) >Luxicon - Cooper Lighting (www.cooperltg.com) >AccuRender, Flamingo - Robert McNeel & Associates (www.accurender.com) >Genesys II -Canlyte (www.canlyte.com), Lightolier (www.lightolier.com) >OptiWin - Glamox AS (www.glamox.com) >RayFront - www.schorsch.com (www.schorsch.com) >LIGHTPAD, BEEM - Electric Power Research Institute (www.epri.com) >LightCalc- Enviro-Systems (www.lightcalc.com) >Aladan - GE Lighting Systems (www.ge-lightingsystems.com) >AUTOLUX - Independent Testing Laboratories (itl@boulder.net) >Desktop Radiance - Lawrence Berkeley National Laboratory >(http://radsite.lbl.gov/deskrad) >Perfect Lite - Trevor Caswell Software >(http://www.powerup.com.au/~trevorc/index.htm) >FOTOCAT - Wellmade Products (www.wlmd.com) >Olivia, Fiona - Ray Forge Services (www.ozemail.com.au/~rayforge) >AGI32, Photometric Toolbox - Lighting Analysts Inc. >(www.lightinganalysts.com) >Lumen Micro 2000, Simply Economics, Simply Lighting, Simply Roadway - >Lighting Technologies, Inc. (www.lightingtechnologies.com) >Lightworks - Lightwork Design Ltd. (www.lightwork.com) >Visual, Photometric Viewer, TEMPLIT - Lithonia Lighting (www.lithonia.com) >Speos - Optis (www.optis.fr) >Martin ShoweDesigner - Martin Professional (www.martinpro.com) >Worldlyte - Worldlyte (www.worldlyte.com) >Relux, LumEdit -Relux Informatik AG (www.relux.ch) >DIALux - Dial GmbH (www.dial.de) >Pytha - Pytha (www.pytha.com) >Ecolumen - Tata Infotech (www.tatainfotech.com) >LiteStar, Lite, PhotoWin - OxyTech Srl (www.oxytech.it) > >Luminaire Design >---------------- >ASAP, ReflectorCAD - Breault Research (www.breault.com) >OSLO, TracePro - Lambda Research Corp. (www.lambdares.com) >RayMaster - Lighting Sciences Inc. (www.lightingsciences.com) >LightTools - Optical Research Associates (www.opticalres.com) >Photopia - Lighting Technologies, Inc. (www.lightingtechnologies.com) >Solstis, Speos, Light, OptiCalc - Optis (www.optis.fr) >Zelum - Focus Software (www.focus-software.com) >RoadRunner - Acme Optics (www.acmeoptics.com) > > >------------------------------------------------------------------------- >globillum@imag.fr -- mailing list devoted to global illumination research >For list archives or to configure your options, see http://listes.imag.fr >------------------------------------------------------------------------- From Return-Path: Received: from rabacal.direct.ca (rabacal.direct.ca [199.60.229.8]) by christl.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id JAA29727 for ; Wed, 16 May 2001 09:17:00 +0200 Received: from bc-van-wvn-a53-01-86.look.ca ([216.66.156.182] helo=VANILLA) by rabacal.direct.ca with smtp (Exim 2.12 #7) id 14zvYI-0003LW-00 for wp@cg.tuwien.ac.at; Wed, 16 May 2001 00:16:59 -0700 Message-ID: <001901c0ddd8$37f06630$0100a8c0@VANILLA> Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: "Werner Purgathofer" References: <200105160617.IAA28520@christl.cg.tuwien.ac.at> Subject: Re: REQUEST FOR INFORMATION - Lighting & Luminaire Design Software Date: Wed, 16 May 2001 00:17:07 -0700 Organization: byHeart Consultants Limited MIME-Version: 1.0 Content-Type: text/plain; charset=iso-8859-1; format=flowed Content-Transfer-Encoding: 8bit X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 5.50.4133.2400 X-MimeOLE: Produced By Microsoft MimeOLE V5.50.4133.2400 X-UIDL: 0c2!!aKa!!`'F!!J9B!! X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Ooh, but I am embarrassed -- how on earth did I overlook Cophos? I was also unaware of Thorn's Vision. Thanks for the informaqtion, Werner. Ian Ashdown, P. Eng., LC, FIES Chief Technology Officer byHeart Consultants Limited http://www.helios32.com ----- Original Message ----- From: "Werner Purgathofer" To: "Ian Ashdown" Sent: Tuesday, May 15, 2001 11:20 PM Subject: Re: REQUEST FOR INFORMATION - Lighting & Luminaire Design Software > Dear Ian, > I am not sure if this company (Zumtobel) is completely in your scope, but I > guess it is close enough. See: > > http://www.zumtobel.at/display.asp?s=2&m=3&p=1&language=en > Best regards, > Werner > > > At 04:07 PM 5/15/01 -0700, you wrote: > >I know -- this message is a bit off-topic for our mailing list. (I posted it > >earlier today to sci.engr.lighting and sci.optics.) On the other hand, you > >may know of European or Far East companies (especially startups) that I > >somehow missed while doing my Web searches. Any assistance would be much > >appreciated. > > > >- Ian Ashdown > > > >REQUEST FOR INFORMATION - Lighting & Luminaire Design Software > > > >The IESNA Computer Committee (Illuminating Engineering Society of North > >America) is compiling its annual IESNA Software Survey for publication in a > >forthcoming issue of Lighting Design+Application magazine (www.iesna.org). > > > >This software survey will enumerate the features of lighting and luminaire > >design and analysis software products for architectural and roadway lighting > >applications. > > > >The Committee wishes to include information on products from as many > >software developers and manufacturers as possible. In particular, we are > >looking for companies worldwide --lighting and luminaire design software > >addresses a global market. > > > >The following list of companies, products and Web URLs is what the Committee > >has compiled to date from Web searches and previous surveys. > > > >WE ARE LOOKING FOR COMPANIES WE HAVE MISSED. If you are aware of a software > >developer or manufacturer that is not on this list, please contact: > > > >Ian Ashdown > >byHeart Consultants Limited > >ian_ashdown@helios32.com > > > >with the following information: > > > >1. Product name > >2. Company name. > >3. Company Web URL. > > > >We will then contact the company and request that they complete a product > >survey. > > > >Thanking you on behalf of the IESNA Computer Committee, > > > >Ian Ashdown, P. Eng., LC, FIES > >Chief Technology Officer > >byHeart Consultants Limited > >http://www.helios32.com > > > >--------------- > >Lighting Design > >--------------- > >Lightscape - Autodesk (www.lightscape.com) > >LitePro - Columbia Lighting (www.columbia-ltg.com) > >Luxicon - Cooper Lighting (www.cooperltg.com) > >AccuRender, Flamingo - Robert McNeel & Associates (www.accurender.com) > >Genesys II -Canlyte (www.canlyte.com), Lightolier (www.lightolier.com) > >OptiWin - Glamox AS (www.glamox.com) > >RayFront - www.schorsch.com (www.schorsch.com) > >LIGHTPAD, BEEM - Electric Power Research Institute (www.epri.com) > >LightCalc- Enviro-Systems (www.lightcalc.com) > >Aladan - GE Lighting Systems (www.ge-lightingsystems.com) > >AUTOLUX - Independent Testing Laboratories (itl@boulder.net) > >Desktop Radiance - Lawrence Berkeley National Laboratory > >(http://radsite.lbl.gov/deskrad) > >Perfect Lite - Trevor Caswell Software > >(http://www.powerup.com.au/~trevorc/index.htm) > >FOTOCAT - Wellmade Products (www.wlmd.com) > >Olivia, Fiona - Ray Forge Services (www.ozemail.com.au/~rayforge) > >AGI32, Photometric Toolbox - Lighting Analysts Inc. > >(www.lightinganalysts.com) > >Lumen Micro 2000, Simply Economics, Simply Lighting, Simply Roadway - > >Lighting Technologies, Inc. (www.lightingtechnologies.com) > >Lightworks - Lightwork Design Ltd. (www.lightwork.com) > >Visual, Photometric Viewer, TEMPLIT - Lithonia Lighting (www.lithonia.com) > > >Speos - Optis (www.optis.fr) > >Martin ShoweDesigner - Martin Professional (www.martinpro.com) > >Worldlyte - Worldlyte (www.worldlyte.com) > >Relux, LumEdit -Relux Informatik AG (www.relux.ch) > >DIALux - Dial GmbH (www.dial.de) > >Pytha - Pytha (www.pytha.com) > >Ecolumen - Tata Infotech (www.tatainfotech.com) > >LiteStar, Lite, PhotoWin - OxyTech Srl (www.oxytech.it) > > > >Luminaire Design > >---------------- > >ASAP, ReflectorCAD - Breault Research (www.breault.com) > >OSLO, TracePro - Lambda Research Corp. (www.lambdares.com) > >RayMaster - Lighting Sciences Inc. (www.lightingsciences.com) > >LightTools - Optical Research Associates (www.opticalres.com) > >Photopia - Lighting Technologies, Inc. (www.lightingtechnologies.com) > >Solstis, Speos, Light, OptiCalc - Optis (www.optis.fr) > >Zelum - Focus Software (www.focus-software.com) > >RoadRunner - Acme Optics (www.acmeoptics.com) > > > > > >------------------------------------------------------------------------- > >globillum@imag.fr -- mailing list devoted to global illumination research > >For list archives or to configure your options, see http://listes.imag.fr > >------------------------------------------------------------------------- > -- > Werner Purgathofer | Tel. +43(1)58801 18648 > Technische Universitaet Wien | http://www.cg.tuwien.ac.at > > *** Are you a member of Eurographics?: http://www.eg.org > From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id XAA23608; Fri, 1 Jun 2001 23:35:48 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id XAA22525; Fri, 1 Jun 2001 23:35:45 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id XAA22520 for ; Fri, 1 Jun 2001 23:35:35 +0200 Received: from edam.direct.ca (edam.direct.ca [199.60.229.6]) by imag.imag.fr (8.9.3/8.8.6) with ESMTP id XAA12909 for ; Fri, 1 Jun 2001 23:35:34 +0200 (MEST) Received: from bc-van-wvn-a53-01-45.look.ca ([216.66.156.141] helo=VANILLA) by edam.direct.ca with smtp (Exim 2.12 #7) id 155wZv-0005wR-00 for globillum@imag.fr; Fri, 1 Jun 2001 14:35:31 -0700 Message-ID: <00c901c0eae2$e2041240$0100a8c0@VANILLA> Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: globillum@imag.fr Subject: Eigenvector Radiosity Date: Fri, 1 Jun 2001 14:36:12 -0700 Organization: byHeart Consultants Limited MIME-Version: 1.0 Content-Type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 5.50.4133.2400 X-MimeOLE: Produced By Microsoft MimeOLE V5.50.4133.2400 X-Loop: globillum@imag.fr X-Sequence: 56 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: X-UIDL: p&h"!S[X!!,@Z!!gpR!! X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit
From the pen of your faithful RADBIB / GITHESIS bibliographer:
 
Ashdown, I. 2001. Eigenvector Radiosity. MSc thesis. Department of Computer Science, University of British Columbia. Vancouver, BC.
 
Abstract:
 
Radiative flux transfer between Lambertian surfaces can be described in terms of linear resistive networks with voltage sources. This thesis examines how these "radiative transfer networks" provide a physical interpretation for the eigenvalues and eigenvectors of form factor matrices. This leads to a novel approach to photorealistic image synthesis and radiative flux transfer analysis called eigenvector radiosity.
 
Available from:
 
 
Ian Ashdown, P. Eng., LC, FIES
Chief Technology Officer
byHeart Consultants Limited
http://www.helios32.com
 
From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.9.3/8.9.3) with ESMTP id TAA29355; Thu, 14 Jun 2001 19:17:10 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id TAA23705; Thu, 14 Jun 2001 19:17:08 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id TAA23700 for ; Thu, 14 Jun 2001 19:17:04 +0200 Received: from mut.autodesk.com (mut.autodesk.com [198.102.112.26]) by imag.imag.fr (8.11.3/8.11.3) with ESMTP id f5EHH2B16385 for ; Thu, 14 Jun 2001 19:17:03 +0200 (MEST) Received: from hqmsgsrf00.autodesk.com (hqmsgsrf00.autodesk.com [144.111.32.210]) by mut.autodesk.com (8.9.3/8.9.3) with ESMTP id KAA08125 for ; Thu, 14 Jun 2001 10:16:56 -0700 (PDT) From: eric.haines@autodesk.com Received: by hqmsgsrf00.autodesk.com with Internet Mail Service (5.5.2653.19) id ; Thu, 14 Jun 2001 10:16:45 -0700 Message-ID: <19879C753611D3119DAB0008C7A4C0C10948F0DC@hqmsgsrf04.autodesk.com> To: globillum@imag.fr Subject: Fantasy Graphics League 2001 Final Results Date: Thu, 14 Jun 2001 10:16:45 -0700 MIME-Version: 1.0 X-Mailer: Internet Mail Service (5.5.2653.19) X-Loop: globillum@imag.fr X-Sequence: 58 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: ^Z#"!QXA!!^Gd"!oJ:"! X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit The results of the Fantasy Graphics League for 2001 are now final and official: http://www.realtimerendering.com/fgl. Thanks to all those who participated; your involvement made this the best (can I say "best" if there is no competition?) fantasy sports league based on SIGGRAPH papers. You can now tell your grandchildren about how you participated in the FGL before it became a premier Las Vegas betting game. Shares in the IPO for the FGL can be purchased from the organizers for one drink ticket each at SIGGRAPH. Individual results will be mailed out shortly, Eric ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.4/8.11.4) with ESMTP id f6C86c101169; Thu, 12 Jul 2001 10:06:38 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id KAA13554; Thu, 12 Jul 2001 10:05:16 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id KAA13549 for ; Thu, 12 Jul 2001 10:05:11 +0200 Received: from dire.bris.ac.uk (dire.bris.ac.uk [137.222.10.60]) by imag.imag.fr (8.11.3/8.11.3) with ESMTP id f6C85Bj14388 for ; Thu, 12 Jul 2001 10:05:11 +0200 (MEST) Received: from cs.bris.ac.uk (actually host lunaleka.cs.bris.ac.uk) by dire.bris.ac.uk with SMTP-PRIV with ESMTP; Thu, 12 Jul 2001 09:05:05 +0100 Received: from voodoo.cs.bris.ac.uk (voodoo [137.222.102.33]) by cs.bris.ac.uk (8.9.3/8.9.3) with ESMTP id JAA11066 for ; Thu, 12 Jul 2001 09:04:55 +0100 (BST) Received: from localhost by voodoo.cs.bris.ac.uk (8.9.3) id JAA23790; Thu, 12 Jul 2001 09:04:55 +0100 (BST) Date: Thu, 12 Jul 2001 09:04:55 +0100 (BST) From: Alan Chalmers X-Sender: alan@voodoo To: globillum@imag.fr Subject: Thesis on line ... Message-ID: MIME-Version: 1.0 X-Loop: globillum@imag.fr X-Sequence: 60 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: '^j"!PYU!!JC("!V;O"! X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Ann McNamara's PhD thesis: "Comparing Real and Synthetic Scenes using Human Judgements of Lightness". PhD. thesis. Department of Computer Science, University of Bristol, UK is now available on-line from: http://www.cs.tcd.ie/people/Ann.McNamara/ Abstract: Current rendering systems are now capable of accurately simulating the physical distribution of light in an environment. However, this physical accuracy does not ensure that the displayed images faithfully represent reality. The problem is how to measure how close to reality these images are? Existing measures of image fidelity take account of certain characteristics such as the fourier content of an image, but this may not reveal specific errors in the portrayal of lighting and shadows; furthermore it could be argued that one needs a measure of fidelity which involves assessment of performance on a specific visual task, performance on that task in a real scene can be compared with performance on that task in a graphical scene to give a measure of fidelity. By conducting such a set of experiments, based on psychophysics, we can estimate how close a rendered image is to its original counterpart. Is this experimental framework using human observers better than using existing image comparison methods? In order to demonstrate the differences between using algorithmic metrics and human evaluation we generated a series of images using different lighting simulation programs. Resulting images were then compared to the real scene they represent, first using metrics (comparing to a captured image of the real scene), then using psychophysics (comparing to the actual real scene). In this thesis, we present the results of these comparisons. ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.4/8.11.4) with ESMTP id f6ELph101492; Sat, 14 Jul 2001 23:51:44 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id XAA20316; Sat, 14 Jul 2001 23:50:13 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id XAA20309 for ; Sat, 14 Jul 2001 23:50:00 +0200 Received: from cheddar.direct.ca (cheddar.direct.ca [199.60.229.16]) by imag.imag.fr (8.11.3/8.11.3) with ESMTP id f6ELnxH21294 for ; Sat, 14 Jul 2001 23:49:59 +0200 (MEST) Received: from bc-van-wvn-a53-01-53.look.ca ([216.66.156.149] helo=VANILLA) by cheddar.direct.ca with smtp (Exim 2.12 #6) id 15LX4e-0002Ak-00 for globillum@imag.fr; Sat, 14 Jul 2001 14:35:41 -0700 Message-ID: <001f01c10caf$36f105e0$0100a8c0@VANILLA> Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: globillum@imag.fr Subject: ANN: Radiosity and Global Illumination bibliographies updated Date: Sat, 14 Jul 2001 14:52:01 -0700 Organization: byHeart Consultants Limited MIME-Version: 1.0 Content-Type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 5.50.4522.1200 X-MimeOLE: Produced By Microsoft MimeOLE V5.50.4522.1200 X-Loop: globillum@imag.fr X-Sequence: 61 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: X-UIDL: !fX!!S)B"!Meg!!K#Z!! 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ANNOUNCE: 01/07/15 Release of RADBIB and GITHESIS
-------------------------------------------------
RADBIB is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. It currently includes 1,934 references -- 20 new additions since its 01/06/15 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of July 15, 2001) from:

http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 247 references to radiosity and global illumination theses -- 2 new additions since the 01/06/15 release.

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

Ian Ashdown, P. Eng., LC, FIES
Chief Technology Officer
byHeart Consultants Limited
http://www.helios32.com

From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.4/8.11.4) with ESMTP id f6ICJiK03437; Wed, 18 Jul 2001 14:19:44 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id OAA27613; Wed, 18 Jul 2001 14:19:31 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id OAA27608 for ; Wed, 18 Jul 2001 14:19:26 +0200 Received: from relay2.mail.uk.psi.net (relay2.mail.uk.psi.net [154.32.107.6]) by imag.imag.fr (8.11.3/8.11.3) with ESMTP id f6ICJP219766 for ; Wed, 18 Jul 2001 14:19:26 +0200 (MEST) Received: from lightwork.co.uk ([195.152.206.2] helo=elvis.lightwork) by relay2.mail.uk.psi.net with esmtp (Exim 2.12 #2) id 15MqIU-0002XA-00 for globillum@imag.fr; Wed, 18 Jul 2001 13:19:22 +0100 Received: by elvis.lightwork with Internet Mail Service (5.5.2650.21) id ; Wed, 18 Jul 2001 13:19:06 +0100 Message-ID: <8815647C7041D111A3010060B06BE1C0015EE89E@elvis.lightwork> From: Neil Gatenby To: globillum@imag.fr Subject: adaptation luminance Date: Wed, 18 Jul 2001 13:18:58 +0100 MIME-Version: 1.0 X-Mailer: Internet Mail Service (5.5.2650.21) X-Loop: globillum@imag.fr X-Sequence: 63 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: $g0!!j@E!!B:G!!#U4"! X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hi all Does anyone have a definition for "adaptation luminance" ? I see the term used a lot, in tone mapping papers, but I can't seem to find a concise/clear definition. TIA Neil ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.4/8.11.4) with ESMTP id f6IFFHK05728; Wed, 18 Jul 2001 17:15:17 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id RAA28153; Wed, 18 Jul 2001 17:15:17 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id RAA28148 for ; Wed, 18 Jul 2001 17:15:15 +0200 Received: from cheddar.direct.ca (cheddar.direct.ca [199.60.229.16]) by imag.imag.fr (8.11.3/8.11.3) with ESMTP id f6IFFE200738 for ; Wed, 18 Jul 2001 17:15:14 +0200 (MEST) Received: from bc-van-wvn-a53-01-46.look.ca ([216.66.156.142] helo=VANILLA) by cheddar.direct.ca with smtp (Exim 2.12 #6) id 15Msol-0007gm-00; Wed, 18 Jul 2001 08:00:51 -0700 Message-ID: <001701c10f9c$bfbb6a10$0100a8c0@VANILLA> Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: "Neil Gatenby" , globillum@imag.fr References: <8815647C7041D111A3010060B06BE1C0015EE89E@elvis.lightwork> Subject: Re: adaptation luminance Date: Wed, 18 Jul 2001 08:17:23 -0700 Organization: byHeart Consultants Limited MIME-Version: 1.0 X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 5.50.4522.1200 X-MimeOLE: Produced By Microsoft MimeOLE V5.50.4522.1200 X-Loop: globillum@imag.fr X-Sequence: 64 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: fDO"!a=c"![aY!!:`W"! X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit "Adaptation luminance" is not officially recognized by the Illuminating Engineering Society in its ANSI / IESNA RP-16-1996, "Nomenclature and Definitions for Illuminating Engineering." However, it does appear in The IESNA Lighting Handbook, Ninth Edition. RP-16 adds this note under "adaptation": "Adaptation is also used to refer to the final state of the [adaptation] process, such as reaching a condition of adaptation to a specific luminance level." There is no explanation of what "a specific luminance level" means, but presumably it refers to the average background lluminance. This is a dangerous approximation in that adaptation is due largely to what is in the foveal field of view. Anything outside of this narrow 2-degree cone has little effect on adaptation. Ian Ashdown, P. Eng., LC, FIES Chief Technology Officer byHeart Consultants Limited http://www.helios32.com ----- Original Message ----- From: "Neil Gatenby" To: Sent: Wednesday, July 18, 2001 5:18 AM Subject: adaptation luminance > > Hi all > > Does anyone have a definition for "adaptation luminance" ? I see the term > used a lot, in tone mapping papers, but I can't seem to find a concise/clear > definition. ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.4/8.11.4) with ESMTP id f6IFLHK05806; Wed, 18 Jul 2001 17:21:17 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id RAA28239; Wed, 18 Jul 2001 17:21:18 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id RAA28234 for ; Wed, 18 Jul 2001 17:21:15 +0200 Received: from graphics.lcs.mit.edu (graphics.lcs.mit.edu [18.24.2.30]) by imag.imag.fr (8.11.3/8.11.3) with ESMTP id f6IFLE201161 for ; Wed, 18 Jul 2001 17:21:14 +0200 (MEST) Received: from graphics.lcs.mit.edu (pigment.lcs.mit.edu [18.24.2.83]) by graphics.lcs.mit.edu (8.11.4/8.11.4) with ESMTP id f6IFJon63387; Wed, 18 Jul 2001 11:19:50 -0400 (EDT) Sender: fredo@graphics.lcs.mit.edu Message-ID: <3B55A916.8D89FB1A@graphics.lcs.mit.edu> Date: Wed, 18 Jul 2001 11:19:50 -0400 From: Fredo Durand X-Mailer: Mozilla 4.76C-SGI [en] (X11; I; IRIX 6.5 IP32) X-Accept-Language: en, fr MIME-Version: 1.0 To: Neil Gatenby CC: globillum@imag.fr, Ian Ashdown Subject: Re: adaptation luminance References: <8815647C7041D111A3010060B06BE1C0015EE89E@elvis.lightwork> X-Loop: globillum@imag.fr X-Sequence: 65 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: kPk"!^9A"!a2&#!d$X!! X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Very good question indeed, since this is one of the fuzzy points of most tone-mapping work (including mine). Unfortunately, there is no "good" answer. In fact, tone mapping methods deal with two definitions of adaptation luminance. The main and first one comes from perception litterature. It is the input axis of many psychophysics curves describing simple characteristics of the visual system depending on luminance. It is fairly well defined for simple conditions (see below). The other definition is basically an exposure metering and corresponds to a reasonable sort of average of the image intensity. As you can read, it is more fuzzy. The main assumption is that you can plug these two notions together and obtain a nice pecreptually-based tone mapping. This is true in practice (aren't Tumblin, Ferwerda et al.'s results nice?), but the fact that we mix those two notions is not always clear enough. The sensitivity of the visual system and other properties (subjective estimation of brightness, contrast sensitivity, pupil size, etc.) vary with luminance. These interactions are very complex. The adaptation luminance can be rigorously defined only in simple experimental setups, where the subject is first adapted to a steady and uniform background of a given luminance (called, guess what, the adaptation luminance). Then numerous properties can be tested using a variety of stimuli, and very nice curves are deduced (like what is the smallest intensity visible depending on the adaptation background). Note that adaptation luminance is defined mainly with respect to an experimental setup, not as an intrinsic input of the visual system. Tone mapping techniques use these data and aim at matching a property (say sensitivity)in the display and virtual conditions. This means that you need to compute an adaptation luminance for both conditions. Unfortunately, our images are usually not uniform adapting field, and our monitors are not in these conditions either. This raises two problems: - How do you compute such an average intensity ? In practice, everyone uses a little recipe to come up with a reasonable adaptation luminance. Like using the average luminosity when light sources are excluded. - Bigger concern: It assumes that there is a single global adaptation state for the whole visual system. This is true for example for the pupil size (obviously), but this is unfortunately not true for e.g. sensitivity. Adaptation mechanisms are very local, which means that you would need an adaptation luminance for every single cone, and moreover that you should handle the dynamic aspects of it (including gaze movements and variations of the luminance of the scene). This is why the notion of a global adaptation luminance is a bit ill-defined in tone mapping, and why no magical formula can be found. But using whatever average luminosity of the image is not unreasonable. By doing so, we are in fact addressing the question: what is the adaptation luminance in a simple setup that would the most closely match my complex real or virtual conditions. However it does not mean that tone mapping techniques are pointless and useless. It just means that they are not 100% phsychophysically based, because the problem itself cannot be solved by psychophysics at this point. However, it means that one should be careful of not confusing tone mapping and accurate adaptation predictions. If you want to display images that look perceptually plausible, perceptually-based tone mapping is great. If you have safety decisions to make, such as visibility in tunnels, maybe check with specialists before blindly (no pun intended) trusting a tone mapping model. Fredo Neil Gatenby wrote: > > Hi all > > Does anyone have a definition for "adaptation luminance" ? I see the term > used a lot, in tone mapping papers, but I can't seem to find a concise/clear > definition. > > TIA > > Neil > > ------------------------------------------------------------------------ > ------------------------------------------------------------------------- > globillum@imag.fr -- mailing list devoted to global illumination research > For list archives or to configure your options, see http://listes.imag.fr > ------------------------------------------------------------------------- -- Fredo Durand, MIT-LCS Graphics Group 200 technology sq. NE43-255, Cambridge, MA 02139 phone : (617) 253 7223 fax : (617) 253 4640 http://graphics.lcs.mit.edu/~fredo/ ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.4/8.11.4) with ESMTP id f6IGbjK06678; Wed, 18 Jul 2001 18:37:45 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id SAA28438; Wed, 18 Jul 2001 18:37:47 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id SAA28433 for ; Wed, 18 Jul 2001 18:37:41 +0200 Received: from bach.Graphics.Cornell.EDU (bach.graphics.cornell.edu [128.84.247.50]) by imag.imag.fr (8.11.3/8.11.3) with ESMTP id f6IGbe205777 for ; Wed, 18 Jul 2001 18:37:40 +0200 (MEST) Received: from graphics.cornell.edu (everest.graphics.cornell.edu [128.84.247.224]) by bach.Graphics.Cornell.EDU (8.9.1/8.9.1) with ESMTP id MAA27332; Wed, 18 Jul 2001 12:34:58 -0400 (EDT) (envelope-from jet@graphics.cornell.edu) Message-ID: <3B55B8D7.827C3B62@graphics.cornell.edu> Date: Wed, 18 Jul 2001 12:27:03 -0400 From: Jack John Erwin Tumblin X-Mailer: Mozilla 4.75 [en] (Windows NT 5.0; U) X-Accept-Language: en MIME-Version: 1.0 To: Neil Gatenby , "Global Illum. Mail List" Subject: Re: adaptation luminance References: <8815647C7041D111A3010060B06BE1C0015EE89E@elvis.lightwork> X-Loop: globillum@imag.fr X-Sequence: 66 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: \K=!!:-9!!_"b"!DWJ"! X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hi Neil Gatenby & Globillumers: I wrote some of those papers, so the confusion on this term is partly my fault. Let me add another note to the detailed responses already sent by Ian Ashdown and Fredo Durand : `Adaptation luminance' is a simple approximation, an single scalar value that intended to describe the current amount of sensitivity adjustment our eyes have made to look at a given scene. As Fredo Durand said, the term came from psychophysics papers (some as much as 100 years old) in which experimenters tried to measure the smallest changes that our eyes could detect. Test subjects were asked to report the presence or absence of an almost-invisible test stimulus shown against a broad featureless background of utterly uniform intensity. Before beginning the test, test subjects would stare at this uniform background long enough to let their eyes completely finish adjusting to it, so eye responses won't vary during the test and corrupt the data. The intensity of this uniform background is usually called the 'adaptation luminance'. Now suppose you are one of those test subjects, and also suppose you could somehow magically look inside your head at the biological machinery that adjusts your vision system to the available light; imagine that you have gears and wheels that turn left or right as we adapt to look at dark or bright scenes. With the help of the experimenter's equipment, suppose you look at a uniform field of 0.1 cd/m^2 for a long time. After the gears and wheels in your head stop turning, you reach in and make a fine scratch mark at the top of one of those wheels. Next, get the experimenter to adjust the intensity of the uniform field to, say, 1.0cd/m^2, and once again stare at it long enough for the wheels in your head to settle down, and make a second mark on the wheel. Continue this for a wide range of background intensities until you build up a calibration scale marked on that wheel. 'Adaptation luminance' is then the reading on the calibrated scale you marked on that wheel--it isn't the measurable amounts of light that you're actually looking at, but rather how much your visual system has _adjusted_ to available light. Now suppose we scrub off the calibration scratches you make on the wheel and close up your head again so you can't see the gears inside. How do you find the adaptation value? When you look at a uniform field for a long time, the answer is obvious; but what if you look at a more complicated scene, with a wide range of intensities? Or what if you want to know the transient readings on that wheel when you suddenly change what you're looking at? If you stick with this simple gear-filled approximation of the visual system, then the adaptation luminance is some nominal mid-range value, somewhere in the span of scene intensities we've recently viewed. Just about every paper on global tone-mapping methods give a simple formula to compute such a value of 'adaptation luminance' from the scene luminances we're looking at. My personal favorite is mean log luminance: L_adapt = exp(mean(log(L_scene))); your mileage may vary. But make no mistake; even though adaptation luminance is computed from measurable light intensities, it is just a prediction of the gear-and-wheel positions in your head; it isn't a physically measurable quantity. As Ian Ashdown and Fredo Durand have pointed out, our eyes are actually far more complicated in their adaptation response to light than 'adaptation luminance' would suggest. We adapt differently at different areas of the retina, and the foveal region dominates the visual appearance of the scene. Also, there are at least three adaptation mechanisms at work in the retina alone, each with its own adjustment rates and effects on visual appearance, and there are also very different adjustment rates for rods and cone receptors (see the book "The Retina: An Approachable Part of the Brain", John Dowling, for a beautiful, authoritative introduction). Darn--*WAY* too long-winded again. Hope this helps! Regards, -Jack Tumblin Neil Gatenby wrote: > Hi all > > Does anyone have a definition for "adaptation luminance" ? I see the term > used a lot, in tone mapping papers, but I can't seem to find a concise/clear > definition. > > TIA > > Neil > > ------------------------------------------------------------------------ > ------------------------------------------------------------------------- > globillum@imag.fr -- mailing list devoted to global illumination research > For list archives or to configure your options, see http://listes.imag.fr > ------------------------------------------------------------------------- ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.4/8.11.4) with ESMTP id f6IHoHK07317; Wed, 18 Jul 2001 19:50:17 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id TAA28623; Wed, 18 Jul 2001 19:48:44 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id TAA28618 for ; Wed, 18 Jul 2001 19:48:41 +0200 Received: from pimout2-int.prodigy.net (pimout2-ext.prodigy.net [207.115.63.101]) by imag.imag.fr (8.11.3/8.11.3) with ESMTP id f6IHmd209185 for ; Wed, 18 Jul 2001 19:48:39 +0200 (MEST) Received: from pb-s600-p233 (A020-0036.DNVR.splitrock.net [63.253.54.36]) by pimout2-int.prodigy.net (8.11.0/8.11.0) with SMTP id f6IHmZQ25836 for ; Wed, 18 Jul 2001 13:48:36 -0400 Message-Id: <3.0.5.32.20010718114022.00a89330@bechtel.colorado.edu> X-Sender: dilaura@bechtel.colorado.edu X-Mailer: QUALCOMM Windows Eudora Light Version 3.0.5 (32) Date: Wed, 18 Jul 2001 11:40:22 -0600 To: globillum@imag.fr From: "David L. DiLaura" Subject: Occluded configuration factors Mime-Version: 1.0 X-Loop: globillum@imag.fr X-Sequence: 67 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: D:T"!0mI"!]a?"!#91!! X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Colleagues: I have found a new way to account for occlusion in radiative transfer calculations. I will be presenting this paper at the upcoming conference of the Illuminating Engineering Society: ftp://bechtel.colorado.edu/pub/Illumination/OccludedConfigurationFactors.pdf Ian Ashdown has kindly provided one review, and I have been asked to find at least one more. If you are interested please let me know. Regards David L. DiLaura ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.4/8.11.4) with ESMTP id f6J5xrK15581; Thu, 19 Jul 2001 07:59:53 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id HAA29264; Thu, 19 Jul 2001 07:59:34 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id HAA29259 for ; Thu, 19 Jul 2001 07:59:21 +0200 Received: from ultra.cs.nchu.edu.tw (ultra.cs.nchu.edu.tw [140.120.14.28]) by imag.imag.fr (8.11.3/8.11.3) with ESMTP id f6J5wr227130 for ; Thu, 19 Jul 2001 07:59:17 +0200 (MEST) Received: from daboo (daboo.cs.nchu.edu.tw [140.120.13.244]) by ultra.cs.nchu.edu.tw (8.9.3/8.9.3) with SMTP id NAA26472 for ; Thu, 19 Jul 2001 13:58:39 +0800 (CST) Message-ID: <014b01c11017$eadb0900$f40d788c@cs.nchu.edu.tw> Reply-To: "Hsien" From: "Hsien" To: globillum@imag.fr Subject: Please give me some opinions Date: Thu, 19 Jul 2001 13:59:03 +0800 Organization: ACM MIME-Version: 1.0 Content-Type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 5.00.2615.200 X-MimeOLE: Produced By Microsoft MimeOLE V5.00.2615.200 X-Loop: globillum@imag.fr X-Sequence: 68 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: X-UIDL: &HR!!+gY"!LB["!n/2!! 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Dear all,
 
    I proposed a method for  approximating a solid angle subtended by a luminaire by a set of spherical
triagles.  This method is used to calculate the direct lighting radiance. Some reviewers suggested me to
consider tessellating the surface of the luminaire, rather than bounding it.  It will  increase the sampling
efficiency ratio.  But I think that tessellation is a biased mehtod.  Efficiency and unbiase, which is important
for photorealistic rendering? Please give me some opinions. Thanks a lot.
 
                                                                                                                                    Best regards,
                                                                                                                                               Hsien
From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.4/8.11.4) with ESMTP id f6JKu5K25869; Thu, 19 Jul 2001 22:56:06 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id WAA31472; Thu, 19 Jul 2001 22:56:02 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id WAA31467 for ; Thu, 19 Jul 2001 22:55:51 +0200 Received: from bach.Graphics.Cornell.EDU (bach.graphics.cornell.edu [128.84.247.50]) by imag.imag.fr (8.11.3/8.11.3) with ESMTP id f6JKtmT15735 for ; Thu, 19 Jul 2001 22:55:48 +0200 (MEST) Received: from graphics.cornell.edu (bray.graphics.cornell.edu [128.84.247.212]) by bach.Graphics.Cornell.EDU (8.9.1/8.9.1) with ESMTP id QAA29630; Thu, 19 Jul 2001 16:55:43 -0400 (EDT) (envelope-from phil@graphics.cornell.edu) Message-ID: <3B57476A.54C7FD33@graphics.cornell.edu> Date: Thu, 19 Jul 2001 16:47:38 -0400 From: Phil Dutre Organization: Program of Computer Graphics X-Mailer: Mozilla 4.77 [en] (WinNT; U) X-Accept-Language: en MIME-Version: 1.0 To: Hsien CC: globillum@imag.fr Subject: Re: Please give me some opinions References: <014b01c11017$eadb0900$f40d788c@cs.nchu.edu.tw> X-Loop: globillum@imag.fr X-Sequence: 69 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: >D7"!U\T!!&hP"!dEC"! X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit > Hsien wrote: > > Dear all, > > I proposed a method for approximating a solid angle subtended by > a luminaire by a set of spherical > triagles. This method is used to calculate the direct lighting > radiance. Some reviewers suggested me to > consider tessellating the surface of the luminaire, rather than > bounding it. It will increase the sampling > efficiency ratio. But I think that tessellation is a biased mehtod. > Efficiency and unbiase, which is important > for photorealistic rendering? Please give me some opinions. Thanks a > lot. > > > Best regards, > Hsien Hi, I'm not sure I understand everything you refer to, but basically, when you sample a light source, it all comes down to: generate points on or in the neighborhoud of the source, and evaluate the self-emmision (which might be zero). So, one can have: - sample the area of the source - sample the visible area - sample the solid angle - sample the visible solid angle - etc ... However, it might be impractical to sample an irregular shape, so, yes, one can put an bounding shape around the light source, sample that, and then evaluate Le (which might be zero). Arvo95 has described a way of sampling the solid angle of a spherical triangle. So, a triangular light source can now be sampled based on its solid angle EXACTLY. If we have a polygonal light source, all one has to do is to tesselate it in triangles, and sample each of them seperately, or pick one of these at random for each sample, or according to any other weighting function. This tessealation is UNBIASED, if the underlying sampling is unbiased. The only thing we have done is subdivide the domain in smaller and easier chunks such that we can come up with a way to sample it. We haven't changed the domain or the function itself, nor have we introduced anything else that changes the underlying integral to be evaluated. More info can be found in the Global Illumination Compendium: http://www.graphics.cornell.edu/~phil/GI/ Hope this helps, Phil -- ======================================================================= Philip Dutre Program of Computer Graphics Cornell University phil@graphics.cornell.edu http://www.graphics.cornell.edu/~phil/ ======================================================================= ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.4/8.11.4) with ESMTP id f6K5OMK31927; Fri, 20 Jul 2001 07:24:22 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id HAA31949; Fri, 20 Jul 2001 07:24:17 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id HAA31944 for ; Fri, 20 Jul 2001 07:24:01 +0200 Received: from ultra.cs.nchu.edu.tw (ultra.cs.nchu.edu.tw [140.120.14.28]) by imag.imag.fr (8.11.3/8.11.3) with ESMTP id f6K5NRT27687 for ; Fri, 20 Jul 2001 07:23:33 +0200 (MEST) Received: from daboo (daboo.cs.nchu.edu.tw [140.120.13.244]) by ultra.cs.nchu.edu.tw (8.9.3/8.9.3) with SMTP id NAA07152; Fri, 20 Jul 2001 13:23:06 +0800 (CST) Message-ID: <002a01c110dc$152ced80$f40d788c@cs.nchu.edu.tw> Reply-To: "Hsien" From: "Hsien" To: "Phil Dutre" Cc: globillum@imag.fr References: <014b01c11017$eadb0900$f40d788c@cs.nchu.edu.tw> <3B57476A.54C7FD33@graphics.cornell.edu> Subject: Re: Please give me some opinions Date: Fri, 20 Jul 2001 13:23:13 +0800 Organization: ACM MIME-Version: 1.0 X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 5.00.2615.200 X-MimeOLE: Produced By Microsoft MimeOLE V5.00.2615.200 X-Loop: globillum@imag.fr X-Sequence: 70 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: EfI!!5P\"!bC\"!T8a!! X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hi, Thanks for your reply. :) The Global Illumination Compendium helps me a lot. But I still have some question. Our method is constructing a bounding box (bigger then the luminaire) for the luminaire and project those vertices of the bounding box onto the unit hemisphere. Thus we can easily trianglise the solid angle subtended by the bounding box into a set of spherical triangles. The luminaires used in our method are represented in its geometric properties. (e.g. the sphere is represented by its center and radius.) It is not constructed by polygons. If we tesselate the luminaire , some parts of the luminaire will not be sampled. That is why I thought it is a biased method. Isn't it? Hsien > > Hi, > > I'm not sure I understand everything you refer to, but basically, > when you sample a light source, it all comes down to: generate > points on or in the neighborhoud of the source, and evaluate the > self-emmision (which might be zero). > > So, one can have: > - sample the area of the source > - sample the visible area > - sample the solid angle > - sample the visible solid angle > - etc ... > > However, it might be impractical to sample an irregular shape, > so, yes, one can put an bounding shape around the light source, > sample that, and then evaluate Le (which might be zero). > > Arvo95 has described a way of sampling the solid angle of a spherical > triangle. So, a triangular light source can now be sampled > based on its solid angle EXACTLY. > If we have a polygonal light source, all one has to do is to > tesselate it in triangles, and sample each of them seperately, > or pick one of these at random for each sample, or according to > any other weighting function. > > This tessealation is UNBIASED, if the underlying sampling is unbiased. > The only thing we have done is subdivide the domain in smaller > and easier chunks such that we can come up with a way to sample it. > We haven't changed the domain or the function itself, nor have > we introduced anything else that changes the underlying integral > to be evaluated. > > More info can be found in the Global Illumination Compendium: > http://www.graphics.cornell.edu/~phil/GI/ > > Hope this helps, > > Phil > > > -- > ======================================================================= > Philip Dutre Program of Computer Graphics Cornell University > phil@graphics.cornell.edu http://www.graphics.cornell.edu/~phil/ > ======================================================================= > ---------------------------------------------------------------------------- ---- > ------------------------------------------------------------------------- > globillum@imag.fr -- mailing list devoted to global illumination research > For list archives or to configure your options, see http://listes.imag.fr > ------------------------------------------------------------------------- ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.4/8.11.4) with ESMTP id f6PEw7K11077; Wed, 25 Jul 2001 16:58:07 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id QAA10835; Wed, 25 Jul 2001 16:58:08 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id QAA10830 for ; Wed, 25 Jul 2001 16:58:06 +0200 Received: from nut.autodesk.com (nut.autodesk.com [198.102.112.27]) by imag.imag.fr (8.11.3/8.11.3) with ESMTP id f6PEw4v26517 for ; Wed, 25 Jul 2001 16:58:04 +0200 (MEST) Received: from hqmsgsrf00.autodesk.com (hqmsgsrf00.autodesk.com [144.111.32.210]) by nut.autodesk.com (8.9.3/8.9.3) with ESMTP id HAA24955 for ; Wed, 25 Jul 2001 07:57:58 -0700 (PDT) From: eric.haines@autodesk.com Received: by hqmsgsrf00.autodesk.com with Internet Mail Service (5.5.2653.19) id ; Wed, 25 Jul 2001 07:57:57 -0700 Message-ID: <19879C753611D3119DAB0008C7A4C0C109ACDFF1@hqmsgsrf04.autodesk.com> To: globillum@imag.fr Subject: Some recent Irisa papers Date: Wed, 25 Jul 2001 07:57:56 -0700 MIME-Version: 1.0 X-Mailer: Internet Mail Service (5.5.2653.19) X-Loop: globillum@imag.fr X-Sequence: 72 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: K;K!!+`'#!P*+!!WR$!! X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Posting this for Kadi Bouatouch (kadi@irisa.fr). Please reply to him. Eric =================== For those who are interested in some of our recently published papers, they can get them at : 1- E Guillou, D. Meneveaux, E. Maisel, K. Bouatouch: Using vanishing points for camera calibration and coarse 3D reconstruction from a single image Visual Comp 16 (2000) 7, 396-410 URL: http://link.springer.de/link/service/journals/00371/bibs/0016007/00160396.htm or http://link.springer-ny.com/link/service/journals/00371/bibs/0016007/00160396.htm or http://www.irisa.fr/prive/kadi/Reconstruction/ 2- D. Meneveaux, K. Bouatouch, E. Maisel and R. Delmont: A New partitioning method for architectural environments The journal of Visualization and Computer Animation 9 (1998) , 195-213 http://www.irisa.fr/prive/kadi/Partitioning/ 3- R. Dumont and K. Bouatouch Combining Hierarchical Radiosity and LODs http://www.irisa.fr/prive/kadi/Level_Of_Detail/ You can also get other papers from : http://www.irisa.fr/prive/kadi/ Kadi ----------------------------------------------------------------------------------- ----------------------------------------------------------------------------------- Kadi Bouatouch | Tel: (33) 2-99-84-72-58 | IRISA | Fax: (33) 2-99-84-71-71 | University of Rennes 1 | | Campus de Beaulieu | E-mail: kadi@irisa.fr | F35042 RENNES CEDEX | | FRANCE | | http://www.irisa.fr/siames/Kadi.Bouatouch | | http://www.irisa.fr/prive/kadi | Download some of my papers | ----------------------------------------------------------------------- ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.4/8.11.4) with ESMTP id f7BGAIW21348; Sat, 11 Aug 2001 18:10:18 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id SAA13990; Sat, 11 Aug 2001 18:10:18 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id SAA13985 for ; Sat, 11 Aug 2001 18:10:11 +0200 Received: from edam.direct.ca (edam.direct.ca [199.60.229.6]) by imag.imag.fr (8.11.3/8.11.3) with ESMTP id f7BGAA711484 for ; Sat, 11 Aug 2001 18:10:10 +0200 (MEST) Received: from bc-van-wvn-a53-01-19.look.ca ([216.66.156.115] helo=VANILLA) by edam.direct.ca with smtp (Exim 2.12 #7) id 15VbKw-0007MD-00 for globillum@imag.fr; Sat, 11 Aug 2001 09:10:06 -0700 Message-ID: <004401c12280$816c6f10$0100a8c0@VANILLA> Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: globillum@imag.fr Subject: Photometria Date: Sat, 11 Aug 2001 09:13:05 -0700 Organization: byHeart Consultants Limited MIME-Version: 1.0 Content-Type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 5.50.4522.1200 X-MimeOLE: Produced By Microsoft MimeOLE V5.50.4522.1200 X-Loop: globillum@imag.fr X-Sequence: 76 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: X-UIDL: S/5!!#2*!!"da"!V+d!! X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit
Dear Colleagues:

While many of us have referenced (or seen referenced) Johann Heinrich
Lambert's 1760 classic text "Photometria" in our papers, it is likely that
few of us have read the original Latin text or the abridged 1892 German
translation by Anding.

This is unfortunate, as Lambert had much to say on photometry and
radiometry, including form factor calculations. For example, Lambert was the
first to develop a closed form expression for the form factor between a
differential surface element and a polygon. (See for example Cohen and
Wallace's book "Radiosity and Realistic Image Synthesis," p. 70, quoting
Schroeder and Hanrahan).

I am therefore pleased and honoured to announce on behalf of my friend and
colleague David DiLaura of the University of Colorado at Boulder that his
English translation of Photometria from the original Latin is now available
as a 680-page bound hardcover book from the Illuminating Engineering Society
of North America (www.iesna.org). The following is from their Publications
page:
----------
Photometria
DD-1-01 List Price: $79.00
Member Price: $63.20
Johann Heinrich Lambert's celebrated "Photometria" is unique in the history
of applied optics and what has come to be called Illumnination Engineering.
Written in 1760, it was the first systematic attempt to formulate, prove,
and demonstrate the processes and principles to be used in the
quantification of light, its effects, and the photometric properties of
materials. Though his interest had its roots in atmospheric and astronomic
phenomena, Lambert's intent was a quantification of all matters dealing with
light, including vision.
----------
This translation was a three-year labour of love by David DiLaura, who
included a 200-page introduction. I have no hestitation in labelling it one
of the most significant contributions to the fields of illumination
engineering and global illumination in the past one hundred years. It brings
us not only a historical text that has been all but lost to the scientific
literature, but many unique perspectives on topics of interest to all of us.

Our work is not a linear progression of mathematical development, but a
breadth-first search of ideas garnered from many disciplines. As we
collectively learn, we gather information that allows us to re-evaluate the
results and hypotheses of previously abandoned investigations. On this basis
alone, Photometria is highly recommended reading for any global illumination
researcher .

Ian Ashdown, P. Eng., LC, FIES
Chief Technology Officer
byHeart Consultants Limited
http://www.helios32.com

From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.4/8.11.4) with ESMTP id f7CGj0W30893; Sun, 12 Aug 2001 18:45:00 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id SAA15180; Sun, 12 Aug 2001 18:44:53 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id SAA15175 for ; Sun, 12 Aug 2001 18:44:41 +0200 Received: from rabacal.direct.ca (rabacal.direct.ca [199.60.229.8]) by imag.imag.fr (8.11.3/8.11.3) with ESMTP id f7CGid721087 for ; Sun, 12 Aug 2001 18:44:40 +0200 (MEST) Received: from bc-van-wvn-a53-01-85.look.ca ([216.66.156.181] helo=VANILLA) by rabacal.direct.ca with smtp (Exim 2.12 #7) id 15VyLs-0006mg-00 for globillum@imag.fr; Sun, 12 Aug 2001 09:44:37 -0700 Message-ID: <001401c1234e$7f1924a0$0100a8c0@VANILLA> Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: 01/08/15 Release of RADBIB and GITHESIS Date: Sun, 12 Aug 2001 09:47:37 -0700 Organization: byHeart Consultants Limited MIME-Version: 1.0 Content-Type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 5.50.4522.1200 X-MimeOLE: Produced By Microsoft MimeOLE V5.50.4522.1200 X-Loop: globillum@imag.fr X-Sequence: 77 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: X-UIDL: ;O;"!Sj^!!)B+#!oI1!! X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

ANNOUNCE: 01/08/15 Release of RADBIB and GITHESIS
-------------------------------------------------
RADBIB is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. It currently includes 1,972 references -- 37 new additions since its 01/07/15 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of August 15, 2001) from:

http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 248 references to radiosity and global illumination theses -- 1 new addition since the 01/07/15 release.

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

Ian Ashdown, P. Eng., LC, FIES
Chief Technology Officer
byHeart Consultants Limited
http://www.helios32.com


 

From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.4/8.11.4) with ESMTP id f8MFtov16125; Sat, 22 Sep 2001 17:55:50 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id RAA23854; Sat, 22 Sep 2001 17:55:38 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id RAA23849 for ; Sat, 22 Sep 2001 17:55:31 +0200 Received: from cheddar.direct.ca (cheddar.direct.ca [199.60.229.16]) by imag.imag.fr (8.11.6/8.11.3) with ESMTP id f8MFtUB13501 for ; Sat, 22 Sep 2001 17:55:30 +0200 (MEST) Received: from bc-van-wvn-a53-01-26.look.ca ([216.66.156.122] helo=VANILLA) by cheddar.direct.ca with smtp (Exim 2.12 #6) id 15kosx-0000YI-00 for globillum@imag.fr; Sat, 22 Sep 2001 08:40:08 -0700 Message-ID: <002701c1437f$98cf3af0$0100a8c0@VANILLA> Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: 01/09/21 Release of RADBIB and GITHESIS Date: Sat, 22 Sep 2001 08:59:43 -0700 Organization: byHeart Consultants Limited MIME-Version: 1.0 Content-Type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 6.00.2600.0000 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2600.0000 X-Loop: globillum@imag.fr X-Sequence: 81 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: X-UIDL: \0'"!D:l"!VIA!!Te]!! X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit
ANNOUNCE: 01/09/21 Release of RADBIB and GITHESIS
-------------------------------------------------
RADBIB is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. It currently includes 1,979 references -- 7 new additions since its 01/08/15 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of September 21, 2001) from:

http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 248 references to radiosity and global illumination theses -- no new additions since the 01/08/15 release.

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

PS - byHeart Consultants Limited has moved. Visit the panoramic views from our office at http://www.helios32.com/office.html. (Bill Gates should be so lucky!)

Ian Ashdown, P. Eng., LC, FIES
Chief Technology Officer
byHeart Consultants Limited
http://www.helios32.com
 
From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.4/8.11.4) with ESMTP id f8MGj3v16403; Sat, 22 Sep 2001 18:45:03 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id SAA24004; Sat, 22 Sep 2001 18:45:05 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id SAA23999 for ; Sat, 22 Sep 2001 18:45:01 +0200 Received: from edam.direct.ca (edam.direct.ca [199.60.229.6]) by imag.imag.fr (8.11.6/8.11.3) with ESMTP id f8MGj0B14150 for ; Sat, 22 Sep 2001 18:45:00 +0200 (MEST) Received: from bc-van-wvn-a53-01-33.look.ca ([216.66.156.129] helo=VANILLA) by edam.direct.ca with smtp (Exim 2.12 #7) id 15kptZ-0005RC-00 for globillum@imag.fr; Sat, 22 Sep 2001 09:44:50 -0700 Message-ID: <001e01c14386$80e6c2d0$0100a8c0@VANILLA> Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: globillum@imag.fr References: <002701c1437f$98cf3af0$0100a8c0@VANILLA> Subject: Re: ANNOUNCE: 01/09/21 Release of RADBIB and GITHESIS Date: Sat, 22 Sep 2001 09:49:09 -0700 Organization: byHeart Consultants Limited MIME-Version: 1.0 Content-Type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 6.00.2600.0000 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2600.0000 X-Loop: globillum@imag.fr X-Sequence: 82 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: X-UIDL: L-c"!3g-!!)TJ"!Tp^!! X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit
Oops! Make that http://www.helios32.com/office.htm. (A moment of levity ...)
 
Ian Ashdown, P. Eng., LC, FIES
Chief Technology Officer
byHeart Consultants Limited
http://www.helios32.com
 
From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.4/8.11.4) with ESMTP id f8OHxmv08232; Mon, 24 Sep 2001 19:59:48 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id TAA31843; Mon, 24 Sep 2001 19:59:46 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id TAA31838 for ; Mon, 24 Sep 2001 19:59:45 +0200 Received: from mut.autodesk.com (mut.autodesk.com [198.102.112.26]) by imag.imag.fr (8.11.6/8.11.3) with ESMTP id f8OHxim19241 for ; Mon, 24 Sep 2001 19:59:44 +0200 (MEST) Received: from hqmsgsrf00.autodesk.com (hqmsgsrf00.autodesk.com [144.111.32.210]) by mut.autodesk.com (8.9.3/8.9.3) with ESMTP id KAA00791 for ; Mon, 24 Sep 2001 10:59:36 -0700 (PDT) From: eric.haines@autodesk.com Received: by hqmsgsrf00.autodesk.com with Internet Mail Service (5.5.2653.19) id ; Mon, 24 Sep 2001 10:59:35 -0700 Message-ID: <19879C753611D3119DAB0008C7A4C0C10A71B5DE@hqmsgsrf04.autodesk.com> To: globillum@imag.fr Subject: Fantasy Graphics League's 2001-2002 season now open Date: Mon, 24 Sep 2001 10:58:46 -0700 MIME-Version: 1.0 X-Mailer: Internet Mail Service (5.5.2653.19) X-Loop: globillum@imag.fr X-Sequence: 84 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: 5NW"!TnE"!Q/M"!E#^!! X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Yes, you've been champing at the bit to try again, to strive to out-do your past accomplishments, to pick a really good Fantasy Graphics League team this time around. Here's your chance to hire the best lab of computer graphics researchers you can, from past SIGGRAPH authors, and pit yourself against thousands, well, tens of other labs from around the world: http://www.realtimerendering.com/fgl It's free, it is considered fun in some sense by a few, and it's free. Enjoy, or else you won't, Eric ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.4/8.11.4) with ESMTP id f9BDfM115277; Thu, 11 Oct 2001 15:41:22 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id PAA15472; Thu, 11 Oct 2001 15:41:23 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id PAA15467 for ; Thu, 11 Oct 2001 15:41:21 +0200 Received: from e1.ny.us.ibm.com (e1.ny.us.ibm.com [32.97.182.101]) by imag.imag.fr (8.11.6/8.11.6) with ESMTP id f9BDfJx15277 for ; Thu, 11 Oct 2001 15:41:20 +0200 (MEST) Received: from northrelay02.pok.ibm.com (northrelay02.pok.ibm.com [9.117.200.22]) by e1.ny.us.ibm.com (8.9.3/8.9.3) with ESMTP id JAA226120 for ; Thu, 11 Oct 2001 09:38:44 -0400 Received: from d01ml244.pok.ibm.com (d01ml244.pok.ibm.com [9.117.127.106]) by northrelay02.pok.ibm.com (8.11.1m3/NCO v4.97.1) with ESMTP id f9BDf8l137162 for ; Thu, 11 Oct 2001 09:41:08 -0400 Importance: Normal Subject: eg2001 presentation etc. To: globillum@imag.fr X-Mailer: Lotus Notes Release 5.0.3 (Intl) 21 March 2000 Message-ID: From: "Holly Rushmeier" Date: Thu, 11 Oct 2001 09:40:52 -0400 X-MIMETrack: Serialize by Router on D01ML244/01/M/IBM(Release 5.0.8 |June 18, 2001) at 10/11/2001 09:41:08 AM MIME-Version: 1.0 X-Loop: globillum@imag.fr X-Sequence: 87 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: \Q\"!/)K!!!?-"!UgT"! X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hi globillumers! A couple of people suggested that I put my Eurographics talk on "Rendering:Input/Output" online, so it is now available at: http://www.research.ibm.com/people/h/holly/pres.html its in pdf, and with all the images still pretty bulky, so I divided it into 2 to 6 Mb pieces. I also put a couple other presentations, including my attempt to be controversial for the "Newton's Nightmare" panel at SIGGRAPH. Since we finally got a template that allows us to put our own papers online with company approval, the ICCV shadow carving paper I mentioned and the SPIE perception related papers can be downloaded from: http://www.research.ibm.com/people/h/holly/pubs.html -- Holly __________________________ Holly Rushmeier , holly@watson.ibm.com, http://www.research.ibm.com/people/h/holly, (914)784-7252 IBM TJ Watson Research Center, 30 Saw Mill River Road, Hawthorne, NY 10532, USA ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.4/8.11.4) with ESMTP id fA6Hel917551; Tue, 6 Nov 2001 18:40:48 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id SAA09206; Tue, 6 Nov 2001 18:40:49 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id SAA09197 for ; Tue, 6 Nov 2001 18:40:30 +0100 Received: from rabacal.direct.ca (rabacal.direct.ca [199.60.229.8]) by imag.imag.fr (8.11.6/8.11.6) with ESMTP id fA6HeS514167 for ; Tue, 6 Nov 2001 18:40:29 +0100 (MET) Received: from bc-van-wvn-a53-01-94.look.ca ([216.66.156.190] helo=VANILLA) by rabacal.direct.ca with smtp (Exim 2.12 #7) id 161AD0-0003s2-00 for globillum@imag.fr; Tue, 6 Nov 2001 09:40:23 -0800 Message-ID: <002601c166ea$e9675bd0$0100a8c0@VANILLA> Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: 01/11/07 Release of RADBIB and GITHESIS Date: Tue, 6 Nov 2001 09:46:05 -0800 Organization: byHeart Consultants Limited MIME-Version: 1.0 Content-Type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 6.00.2600.0000 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2600.0000 X-Loop: globillum@imag.fr X-Sequence: 88 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: X-UIDL: dG\"!6V:!!^fV"!Ih5"! X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit
ANNOUNCE: 01/11/07 Release of RADBIB and GITHESIS
-------------------------------------------------
RADBIB is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. It currently includes 1,987 references -- 8 new additions since its 01/09/21 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of November 7, 2001) from:

http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 251 references to radiosity and global illumination theses -- 3 new additions since the 01/09/21 release.

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

Ian Ashdown, P. Eng., LC, FIES
Chief Technology Officer
byHeart Consultants Limited
http://www.helios32.com
 
From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.4/8.11.4) with ESMTP id fAGK0p910733; Fri, 16 Nov 2001 21:00:52 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id VAA04652; Fri, 16 Nov 2001 21:00:53 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id VAA04647 for ; Fri, 16 Nov 2001 21:00:50 +0100 Received: from mut.autodesk.com (mut.autodesk.com [198.102.112.26]) by imag.imag.fr (8.11.6/8.11.6) with ESMTP id fAGK0nY29146 for ; Fri, 16 Nov 2001 21:00:49 +0100 (MET) Received: from hqmsgsrf00.autodesk.com (hqmsgsrf00.autodesk.com [144.111.32.210]) by mut.autodesk.com (8.9.3/8.9.3) with ESMTP id MAA28782 for ; Fri, 16 Nov 2001 12:00:43 -0800 (PST) From: eric.haines@autodesk.com Received: by hqmsgsrf00.autodesk.com with Internet Mail Service (5.5.2653.19) id ; Fri, 16 Nov 2001 12:00:42 -0800 Message-ID: <19879C753611D3119DAB0008C7A4C0C10B16BB10@hqmsgsrf04.autodesk.com> To: globillum@imag.fr Subject: 1/r^2 lighting for interactive rendering Date: Fri, 16 Nov 2001 12:00:17 -0800 MIME-Version: 1.0 X-Mailer: Internet Mail Service (5.5.2653.19) X-Loop: globillum@imag.fr X-Sequence: 90 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: Z\:!!9\1"!4n4!!I_E"! X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit I've got a global illumination question about normal 1/(r^2) lighting. This form of lighting is supported in APIs such as OpenGL, but it's not all that usable. The problem is that the effect of the light dies off too quickly. I think there are two causes for this: 1) Gamma correction not done. Everything gets dimmed down too quickly if you ignore gamma, as is commonly done in interactive applications on the PC. Jonathan Blow pointed this problem out to me, and noted some examples by Brian Hook: http://www.pyrogon.com/shots/. If you don't correct for gamma, forget the rest of the question, as this factor is pretty major. 2) Light reflected from nearby objects is not accounted for. Say you have a single light in an environment, dropping off at 1/(r^2). If it's an outdoor scene like a large flat desert, then interreflectivity is nil (the light hits the desert and reflects upwards to infinity), so 1/(r^2) is fine. What I'm wondering about is the effect when inside an enclosed room. The light bouncing around obviously does have an effect, and what I'm wondering is whether there's any rule of thumb as to a way to account for this in the drop-off equation. Could you simply add in some 1/r term to get some reasonable approximation on the average? I'm guessing such add-ins would just be ad hoc (as is usually done), twiddle with the 1/r and 1/r^2 light components on a scene by scene basis until it looks good. Also, such twiddling assumes light comes only from the light's direction, patently false. More generally, it seems like this sort of thing could be analyzed fairly cleanly for various types of scenes - has anyone done anything like this, getting some reasonable approximation of the radiance distribution and overall irradiance given a single overhead light? It might be useful to have irradiance maps computed for various places in the room and interpolate among these as you move through the room (subtracting out the 1/r^2 light itself, so you could add that in on the fly, since it's so important). Any thoughts appreciated, Eric ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.4/8.11.4) with ESMTP id fAGM2s911417; Fri, 16 Nov 2001 23:02:57 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id XAA04961; Fri, 16 Nov 2001 23:03:00 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id XAA04956 for ; Fri, 16 Nov 2001 23:02:55 +0100 Received: from mut.autodesk.com (mut.autodesk.com [198.102.112.26]) by imag.imag.fr (8.11.6/8.11.6) with ESMTP id fAGM2sY01800 for ; Fri, 16 Nov 2001 23:02:54 +0100 (MET) Received: from hqmsgsrf00.autodesk.com (hqmsgsrf00.autodesk.com [144.111.32.210]) by mut.autodesk.com (8.9.3/8.9.3) with ESMTP id OAA22603 for ; Fri, 16 Nov 2001 14:02:48 -0800 (PST) From: eric.haines@autodesk.com Received: by hqmsgsrf00.autodesk.com with Internet Mail Service (5.5.2653.19) id ; Fri, 16 Nov 2001 14:02:47 -0800 Message-ID: <19879C753611D3119DAB0008C7A4C0C10B24A651@hqmsgsrf04.autodesk.com> To: globillum@imag.fr Subject: Fresnel term Date: Fri, 16 Nov 2001 14:02:19 -0800 MIME-Version: 1.0 X-Mailer: Internet Mail Service (5.5.2653.19) X-Loop: globillum@imag.fr X-Sequence: 91 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: @_*#!+i:!!JZJ!!:QX"! X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit There's been a fair amount of interest in simulating the Fresnel term for real-time rendering. Another thing that's been on my mind: Grab a CD jewel case. Look at a light reflected off of it (not at a grazing angle, since a grazing angle causes full reflection). According to the Fresnel effect, the light coming off the surface is around 1/25th as bright as the light itself (true for dielectrics, depends on the index of refraction). Personally, to me the reflection looks dimmer, sure, but not 1/25th as bright. (With incandescents I definitely notice the difference in luminance [it's painful to look at the bulb itself], but not much with fluorescent lights). Is there some good explanation here, beyond "the eye is an amazing thing" and tone reproduction problems? I usually think of tone reproduction as something that comes into play in places where there are radically different lighting situations in the same view (looking out of the tunnel, etc). Using a high dynamic range figures in to computing such reflectance terms correctly, but that does little to explain the perceptual effect. If anything, I think this example shows how far we are from having a good model of the eye for rendering a scene well - if you don't agree, please let me know what I'm missing. If anyone has any further insights or ideas on this one, pass them on, Eric ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.4/8.11.4) with ESMTP id fAH03B914369; Sat, 17 Nov 2001 01:03:12 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id BAA05117; Sat, 17 Nov 2001 01:03:10 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id BAA05112 for ; Sat, 17 Nov 2001 01:03:07 +0100 Received: from darkwing.uoregon.edu (daemon@darkwing.uoregon.edu [128.223.142.13]) by imag.imag.fr (8.11.6/8.11.6) with ESMTP id fAH036Y03749 for ; Sat, 17 Nov 2001 01:03:06 +0100 (MET) Received: (from randolph@localhost) by darkwing.uoregon.edu (8.11.6/8.11.6) id fAH030801320 for globillum@imag.fr; Fri, 16 Nov 2001 16:03:00 -0800 (PST) Date: Fri, 16 Nov 2001 16:03:00 -0800 From: Randolph Fritz To: globillum@imag.fr Subject: Re: Fresnel term Message-ID: <20011116160300.A26791@darkwing.uoregon.edu> Mail-Followup-To: Randolph Fritz , globillum@imag.fr References: <19879C753611D3119DAB0008C7A4C0C10B24A651@hqmsgsrf04.autodesk.com> Mime-Version: 1.0 User-Agent: Mutt/1.2.5i In-Reply-To: <19879C753611D3119DAB0008C7A4C0C10B24A651@hqmsgsrf04.autodesk.com>; from eric.haines@autodesk.com on Fri, Nov 16, 2001 at 02:02:19PM -0800 X-Loop: globillum@imag.fr X-Sequence: 92 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: 8Qf!!/\m!!o1U!!#K)#! X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit On Fri, Nov 16, 2001 at 02:02:19PM -0800, eric.haines@autodesk.com wrote: > > [...]According to the Fresnel effect, the light coming off > the surface is around 1/25th as bright as the light itself (true for > dielectrics, depends on the index of refraction). Personally, to me > the reflection looks dimmer, sure, but not 1/25th as bright. [...] > > Is there some good explanation here, beyond "the eye is an amazing > thing" and tone reproduction problems? At this risk of asking a naive question, did you account for logarithmic compression in visual processing in your 1/25th? If it's just 1/25th of the energy, I'd expect it to seem maybe four or five times dimmer. (log2(25)) Randolph ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.4/8.11.4) with ESMTP id fAH0NU915280; Sat, 17 Nov 2001 01:23:31 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id BAA05247; Sat, 17 Nov 2001 01:23:29 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id BAA05242 for ; Sat, 17 Nov 2001 01:23:28 +0100 Received: from graphics.lcs.mit.edu (graphics.lcs.mit.edu [18.24.2.30]) by imag.imag.fr (8.11.6/8.11.6) with ESMTP id fAH0NRY04104 for ; Sat, 17 Nov 2001 01:23:27 +0100 (MET) Received: from graphics.lcs.mit.edu (pigment.lcs.mit.edu [18.24.2.83]) by graphics.lcs.mit.edu (8.11.4/8.11.4) with ESMTP id fAH0N3S854221; Fri, 16 Nov 2001 19:23:03 -0500 (EST) Sender: fredo@graphics.lcs.mit.edu Message-ID: <3BF5ADE6.80A3AB98@graphics.lcs.mit.edu> Date: Fri, 16 Nov 2001 19:23:02 -0500 From: Fredo Durand X-Mailer: Mozilla 4.77C-SGI [en] (X11; I; IRIX 6.5 IP32) X-Accept-Language: en, fr MIME-Version: 1.0 To: Randolph Fritz CC: globillum@imag.fr Subject: Re: Fresnel term References: <19879C753611D3119DAB0008C7A4C0C10B24A651@hqmsgsrf04.autodesk.com> <20011116160300.A26791@darkwing.uoregon.edu> X-Loop: globillum@imag.fr X-Sequence: 93 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: \,W!!>^!#![aK!!&fX"! X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit There is no logarithmic compression in visual processing. However, (subjective) brightness tends to be estimated as the cubic root of the luminance (Stevens and Stevens, in the sixties). So in your case the subjective factor should be around 3. And yes, tone reproduction problems, the initial paper by Tumblin uses some data by Stevens. And anyway, the human visual system is extremely bad at estimating absolute luminosity. See e.g. the very cool illusion by Adelson http://www-bcs.mit.edu/persci/high/gallery/checkershadow_illusion.html And yes, the eye is an amazing thing. Fredo Randolph Fritz wrote: > > On Fri, Nov 16, 2001 at 02:02:19PM -0800, eric.haines@autodesk.com wrote: > > > > [...]According to the Fresnel effect, the light coming off > > the surface is around 1/25th as bright as the light itself (true for > > dielectrics, depends on the index of refraction). Personally, to me > > the reflection looks dimmer, sure, but not 1/25th as bright. [...] > > > > Is there some good explanation here, beyond "the eye is an amazing > > thing" and tone reproduction problems? > > At this risk of asking a naive question, did you account for > logarithmic compression in visual processing in your 1/25th? If it's > just 1/25th of the energy, I'd expect it to seem maybe four or five > times dimmer. (log2(25)) > > Randolph > > ------------------------------------------------------------------------ > ------------------------------------------------------------------------- > globillum@imag.fr -- mailing list devoted to global illumination research > For list archives or to configure your options, see http://listes.imag.fr > ------------------------------------------------------------------------- -- Fredo Durand, MIT-LCS Graphics Group 200 technology sq. NE43-242, Cambridge, MA 02139 phone : (617) 253 7223 fax : (617) 253 4640 http://graphics.lcs.mit.edu/~fredo/ ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.4/8.11.4) with ESMTP id fAH3tA916128; Sat, 17 Nov 2001 04:55:11 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id EAA05627; Sat, 17 Nov 2001 04:54:55 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id EAA05622 for ; Sat, 17 Nov 2001 04:54:53 +0100 Received: from wrath.cs.utah.edu (wrath.cs.utah.edu [155.99.198.100]) by imag.imag.fr (8.11.6/8.11.6) with ESMTP id fAH3spY06438 for ; Sat, 17 Nov 2001 04:54:51 +0100 (MET) Received: from faith.cs.utah.edu (faith.cs.utah.edu [155.99.198.108]) by wrath.cs.utah.edu (8.11.6/8.11.6) with ESMTP id fAH3sj505414; Fri, 16 Nov 2001 20:54:45 -0700 (MST) From: Peter Shirley Received: (from shirley@localhost) by faith.cs.utah.edu (8.11.1/8.11.1) id fAH3siW23906; Fri, 16 Nov 2001 20:54:44 -0700 (MST) Message-Id: <200111170354.fAH3siW23906@faith.cs.utah.edu> Subject: Re: Fresnel term To: Fredo Durand Date: Fri, 16 Nov 2001 20:54:44 -0700 (MST) Cc: Randolph Fritz , globillum@imag.fr In-Reply-To: <3BF5ADE6.80A3AB98@graphics.lcs.mit.edu> from "Fredo Durand" at Nov 16, 2001 07:23:02 PM X-Mailer: ELM [version 2.5 PL2] MIME-Version: 1.0 X-Loop: globillum@imag.fr X-Sequence: 94 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.4/8.11.4) with ESMTP id fAHBWA917820; Sat, 17 Nov 2001 12:32:11 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id MAA05961; Sat, 17 Nov 2001 12:32:08 +0100 Received: from ebene.inrialpes.fr (ebene.inrialpes.fr [194.199.18.70]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id MAA05956 for ; Sat, 17 Nov 2001 12:32:04 +0100 Received: from safran.inrialpes.fr (safran.inrialpes.fr [194.199.26.1]) by ebene.inrialpes.fr (8.11.6/8.11.6) with ESMTP id fAHBSHr07926; Sat, 17 Nov 2001 12:28:17 +0100 (MET) Received: from localhost (fneyret@localhost) by safran.inrialpes.fr (980427.SGI.8.8.8/8.8.5) with SMTP id MAA18298; Sat, 17 Nov 2001 12:31:59 +0100 (MET) Message-Id: <200111171131.MAA18298@safran.inrialpes.fr> X-Authentication-Warning: safran.inrialpes.fr: fneyret@localhost didn't use HELO protocol To: eric.haines@autodesk.com Cc: globillum@imag.fr, Fabrice.Neyret@imag.fr Subject: Re: 1/r^2 lighting for interactive rendering In-reply-to: Your message of "Fri, 16 Nov 2001 12:00:17 PST." <19879C753611D3119DAB0008C7A4C0C10B16BB10@hqmsgsrf04.autodesk.com> Date: Sat, 17 Nov 2001 12:31:59 +0100 From: Fabrice Neyret X-Loop: globillum@imag.fr X-Sequence: 95 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: 7C:!!1XM"![lA"!6 I've got a global illumination question about normal 1/(r^2) lighting. > This form of lighting is supported in APIs such as OpenGL, but it's not all that usable. > The problem is that the effect of the light dies off too quickly. I think there are two > causes for this: > 2) Light reflected from nearby objects is not accounted for. > [] What I'm wondering about is the effect when inside an > enclosed room. The light bouncing around obviously does have an effect, and what I'm > wondering is whether there's any rule of thumb as to a way to account for this in the > drop-off equation. Could you simply add in some 1/r term to get some reasonable > approximation on the average? I'm guessing such add-ins would just be ad hoc > (as is usually done), twiddle with the 1/r and 1/r^2 light components on a scene by scene > basis until it looks good. A remark that OpenGL provides for a constant, a *linear*, and a quadratic attenuations, and it indeed allows a combination of the three; see man glLight: " If the light is positional [], its intensity is attenuated by the reciprocal of the sum of the constant factor, the linear factor times the distance between the light and the vertex being lighted, and the quadratic factor times the square of the same distance. The initial attenuation factors are (1, 0, 0), resulting in no attenuation." Togather with the effect of inter-reflections, I remember an other argument for not using the 1/r2 drop-off in interior scenes (was it simply in the Foley & van Dam ?), that was the fact that light sources are generally not points. However, I don't remember any rules of the thumb to set the coefficients ( same for the estimation of the varying 'ambient term' to be used at different locations, apart for some specialized pieces of work by Max and Fournier on horizon maps, or by Reeves and Max on light attenuation through areas congested with leaves. ) PS: please tells your mailer to wrap the lines !!! Fabrice NEYRET -------------------------------------------- equipe iMAGIS ( GRAVIR (CNRS,INPG,UJF) & INRIA ) http://www-imagis.imag.fr/Membres/Fabrice.Neyret/index.html fax: +33 (0)4 76 61 54 40 secretariat: +33 (0)4 76 61 54 26 -------------------------------------------- ------------=_1005996724-5543-1 Content-Type: text/plain; name="message.footer" Content-Disposition: inline; filename="message.footer" Content-Transfer-Encoding: 8bit ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- ------------=_1005996724-5543-1-- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.4/8.11.4) with ESMTP id fAHGdl919086; Sat, 17 Nov 2001 17:39:48 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id RAA06256; Sat, 17 Nov 2001 17:39:49 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id RAA06251 for ; Sat, 17 Nov 2001 17:39:44 +0100 Received: from rabacal.direct.ca (rabacal.direct.ca [199.60.229.8]) by imag.imag.fr (8.11.6/8.11.6) with ESMTP id fAHGdgY17069 for ; Sat, 17 Nov 2001 17:39:43 +0100 (MET) Received: from bc-van-wvn-a53-01-57.look.ca ([216.66.156.153] helo=VANILLA) by rabacal.direct.ca with smtp (Exim 2.12 #7) id 1658VF-0004hh-00 for globillum@imag.fr; Sat, 17 Nov 2001 08:39:37 -0800 Message-ID: <001901c16f86$b94b5fb0$999c42d8@VANILLA> Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: globillum@imag.fr References: <200111171131.MAA18298@safran.inrialpes.fr> Subject: Re: 1/r^2 lighting for interactive rendering Date: Sat, 17 Nov 2001 08:41:35 -0800 Organization: byHeart Consultants Limited MIME-Version: 1.0 X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 6.00.2600.0000 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2600.0000 X-Loop: globillum@imag.fr X-Sequence: 96 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: (1I!!,S~!!G#)#!2LN!! X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Regarding Eric Haines' question regarding ad hoc techniques for improving the appearance of inverse square law lighting in OpenGL and Fabrice Neyret's response: 1. As Eric noted, gamma correction is absolutely essential. Without it, the inverse square law lighting of OpenGL will not result in the physically correct appearance of direct illuminance due to point light sources. 2. Adding a 1/r term to model indirect illumination due to interreflections is the wrong approach, even as an ad hoc technique. Any representation of indirect illumination must be based on the geometry and material properties (in particular diffuse spectral reflectance) of the environment. The following paper addresses these issues: Castro, F., L. Neumann, and M. Sbert. 2000. "Extended Ambient Term," Journal of Graphics Tools 5(4):1-7. 3. Regarding the applicability of the inverse square law to area light sources, we can turn to Johann Lambert (Photometria, 1760) and his recommendation of the "five-times" rule. Namely, the inverse square law applies if the distance from the source to the illuminated surface is greater than five times the projected width of the light source as seen from the surface. In other words, the area light source should subtend a maximum angle of less than 0.2 radians as seen from the illuminated point. This rule of thumb has been used by illumination engineers for the past century. A comprehensive analysis of the errors involved (typically less than 2 percent) is given in: Murdoch, J. B. 1981. "Inverse Square Law Approximation of Illuminance," Journal of the Illuminating Engineering Society 11(2):96-106. Ian Ashdown, P. Eng., LC, FIES Chief Technology Officer byHeart Consultants Limited http://www.helios32.com ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.4/8.11.4) with ESMTP id fAJEZT909877; Mon, 19 Nov 2001 15:35:30 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id PAA10412; Mon, 19 Nov 2001 15:35:32 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id PAA10407 for ; Mon, 19 Nov 2001 15:35:29 +0100 Received: from bach.graphics.cornell.edu (bach.graphics.cornell.edu [128.84.247.50]) by imag.imag.fr (8.11.6/8.11.6) with ESMTP id fAJEZSE18704 for ; Mon, 19 Nov 2001 15:35:28 +0100 (MET) Received: from RALPH (ralph.graphics.cornell.edu [128.84.247.95]) by bach.graphics.cornell.edu (8.12.1/8.12.1) with ESMTP id fAJEZMo6010763; Mon, 19 Nov 2001 09:35:22 -0500 (EST) Date: Mon, 19 Nov 2001 09:35:22 -0500 (EST) Message-Id: <200111191435.fAJEZMo6010763@bach.graphics.cornell.edu> From: "Stephen H. Westin" To: eric.haines@autodesk.com CC: globillum@imag.fr In-reply-to: <19879C753611D3119DAB0008C7A4C0C10B16BB10@hqmsgsrf04.autodesk.com> (eric.haines@autodesk.com) Subject: Re: 1/r^2 lighting for interactive rendering Reply-to: westin@graphics.cornell.edu References: <19879C753611D3119DAB0008C7A4C0C10B16BB10@hqmsgsrf04.autodesk.com> X-Loop: globillum@imag.fr X-Sequence: 97 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: 6X3!!bG8!!j'Z"!2F["! X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 MIME-Version: 1.0 Content-transfer-encoding: 8bit This is a multi-part message in MIME format... ------------=_1006180531-8112-0 > I've got a global illumination question about normal 1/(r^2) > lighting. This form of lighting is supported in APIs such as OpenGL, > but it's not all that usable. The problem is that the effect of the > light dies off too quickly. I think there are two causes for this: > > 1) Gamma correction not done. > 2) Light reflected from nearby objects is not accounted for. And 3) Dynamic range problems. To keep the bright areas of the scene from saturating hopelessly, the lighting must be cranked down to the point where most of the scene goes nearly black, to within the limitations of the display. In a real scene, the visual system would deal in a spatially-dependent way with the brightness range, making both the very bright and the dim areas visible. -Stephen H. Westin Any information or opinions in this message are mine: they do not represent the position of Cornell University or any of its sponsors. ------------=_1006180531-8112-0 Content-Type: text/plain; name="message.footer" Content-Disposition: inline; filename="message.footer" Content-Transfer-Encoding: 8bit ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- ------------=_1006180531-8112-0-- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.4/8.11.4) with ESMTP id fALKK4920731; Wed, 21 Nov 2001 21:20:05 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id VAA04271; Wed, 21 Nov 2001 21:20:05 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id VAA04264 for ; Wed, 21 Nov 2001 21:19:54 +0100 Received: from graphics.lcs.mit.edu (graphics.lcs.mit.edu [18.24.2.30]) by imag.imag.fr (8.11.6/8.11.6) with ESMTP id fALKJra16313 for ; Wed, 21 Nov 2001 21:19:53 +0100 (MET) Received: from graphics.lcs.mit.edu (pigment.lcs.mit.edu [18.24.2.83]) by graphics.lcs.mit.edu (8.11.4/8.11.4) with ESMTP id fALKIxS1013523; Wed, 21 Nov 2001 15:18:59 -0500 (EST) Sender: fredo@graphics.lcs.mit.edu Message-ID: <3BFC0C33.D2D19B18@graphics.lcs.mit.edu> Date: Wed, 21 Nov 2001 15:18:59 -0500 From: Fredo Durand X-Mailer: Mozilla 4.77C-SGI [en] (X11; I; IRIX 6.5 IP32) X-Accept-Language: en, fr MIME-Version: 1.0 To: eric.haines@autodesk.com CC: "globillum@imag.fr" Subject: Re: Fresnel term References: <19879C753611D3119DAB0008C7A4C0C10B24A992@hqmsgsrf04.autodesk.com> X-Loop: globillum@imag.fr X-Sequence: 98 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: ]3U"!;)F"!'2X!!1$["! X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit > Hmmm, this is very interesting! I'm not sure what to make of all this. Traditional computer graphics, done with Science(tm), is: > > 1) compute radiance in a given direction > 2) gamma correct for system. > 3) store that value in the pixel. > > which seems wrong if there is this subjective factor that should be accounted for. Or should it? Do you think that even for scenes with a low dynamic range (say it all fits nicely in a 1-255 range) that some other adjustment has to be done? I do not understand what this subjective brightness idea means to image synthesis, if anything. Well, almost the same nonlinearity is applied when you look at the scene and when you look at the picture. So it is mostly OK. (Similarly the image is optically inversed in your eye, but it is OK because both the scene and the image are inversed the same way !) However, this nonlinearity varies with background luminance. Since we typically watch pictures in darker environmnet than the corresponding scenes, we need to compensate. This is why gamma correction is needed. The fact that CRTs happen to need an additional non-linearity is secondary. Gamma correction was first developed for film photography, where no CRT gun is involved! See e.g. the book by Hunt on color reproduction. The fact that CRTs have a non-linearity causes a lot of confusion about gamma correction And this is essentially what Tumblin and Rushmeier's operator does : vary the exponent of the non-linearity according to the scene average luminance. So what you want to do in realistic lighting simulation is 1/ compute radiance 2/ store this linear radiance value in floating point 3/ apply relevant tone mapping algorithm (including some gamma correction) 4/ maybe store that image as well (but it is now an image, not the result of a radiometric simulation) In theory, you would want to re-apply the tone mapping differently for each new viewing condition. For example, if you have a much better display than I have, with far better contrast, and maybe your office has more light than mine, you could want to use different tone mapping parameters. Another example is Tumblin foveated tone mapping operator: the transfer function depends on the part of the image you're looking at. Fredo -- Fredo Durand, MIT-LCS Graphics Group 200 technology sq. NE43-242, Cambridge, MA 02139 phone : (617) 253 7223 fax : (617) 253 4640 http://graphics.lcs.mit.edu/~fredo/ ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.4/8.11.4) with ESMTP id fB22qX930413; Sun, 2 Dec 2001 03:52:34 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id DAA17324; Sun, 2 Dec 2001 03:52:31 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id DAA17319 for ; Sun, 2 Dec 2001 03:52:23 +0100 Received: from rabacal.direct.ca (rabacal.direct.ca [199.60.229.8]) by imag.imag.fr (8.11.6/8.11.6) with ESMTP id fB22qLA07759 for ; Sun, 2 Dec 2001 03:52:22 +0100 (MET) Received: from bc-van-wvn-a53-01-26.look.ca ([216.66.156.122] helo=VANILLA) by rabacal.direct.ca with smtp (Exim 2.12 #7) id 16AMjq-0004AX-00 for globillum@imag.fr; Sat, 1 Dec 2001 18:52:19 -0800 Message-ID: <000c01c17adc$b1b94f30$7a9c42d8@VANILLA> Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: 01/12/01 Update of RADBIB and GITHESIS Date: Sat, 1 Dec 2001 18:54:41 -0800 Organization: byHeart Consultants Limited MIME-Version: 1.0 Content-Type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 6.00.2600.0000 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2600.0000 X-Loop: globillum@imag.fr X-Sequence: 101 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: X-UIDL: W=M!!5)!#!)\!"!7O*"! X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

ANNOUNCE: 01/12/01 Release of RADBIB and GITHESIS
-------------------------------------------------
RADBIB is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. It currently includes 2,003 references -- 16 new additions since its 01/11/07 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of December 1, 2001) from:

http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 252 references to radiosity and global illumination theses -- 1 new addition since the 01/11/07 release.

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

Ian Ashdown, P. Eng., LC, FIES
Chief Technology Officer
byHeart Consultants Limited
http://www.helios32.com

 

From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.4/8.11.4) with ESMTP id fBBJn5920283; Tue, 11 Dec 2001 20:49:06 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id UAA25607; Tue, 11 Dec 2001 20:49:09 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id UAA25602 for ; Tue, 11 Dec 2001 20:49:07 +0100 Received: from mut.autodesk.com (mut.autodesk.com [198.102.112.26]) by imag.imag.fr (8.11.6/8.11.6) with ESMTP id fBBJn6f18270 for ; Tue, 11 Dec 2001 20:49:06 +0100 (MET) Received: from hqmsgsrf00.autodesk.com (hqmsgsrf00.autodesk.com [144.111.32.210]) by mut.autodesk.com (8.9.3/8.9.3) with ESMTP id LAA22643 for ; Tue, 11 Dec 2001 11:48:59 -0800 (PST) From: eric.haines@autodesk.com Received: by hqmsgsrf00.autodesk.com with Internet Mail Service (5.5.2653.19) id ; Tue, 11 Dec 2001 11:48:58 -0800 Message-ID: <19879C753611D3119DAB0008C7A4C0C10B67775A@hqmsgsrf04.autodesk.com> To: globillum@imag.fr Subject: fake or foto and FGL reminder Date: Tue, 11 Dec 2001 11:48:49 -0800 MIME-Version: 1.0 X-Mailer: Internet Mail Service (5.5.2653.19) X-Loop: globillum@imag.fr X-Sequence: 103 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: E7$#!"SJ!!mVG"!=c)"! X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Two things for your bemusement: http://www.fakeorfoto.com/quiz.html - somewhat contrived and abstract scenes, but worth a minute of time (thanks to Randy Fernando for passing me this link). http://www.realtimerendering.com/fgl - there's less than a month left to get your virtual research lab hired, so get going. Back to work, Eric ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id g1Q4Lkf14791; Tue, 26 Feb 2002 05:21:46 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id FAA30359; Tue, 26 Feb 2002 05:24:07 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id FAA30354 for ; Tue, 26 Feb 2002 05:24:02 +0100 Received: from photon.look.ca (photon.look.ca [207.136.80.123]) by imag.imag.fr (8.11.6/8.11.6) with ESMTP id g1Q4O1000938 for ; Tue, 26 Feb 2002 05:24:01 +0100 (MET) Received: from bc-van-wvn-a53-01-38.look.ca ([216.66.156.134] helo=VANILLA) by photon.look.ca with smtp (Exim 3.12 #9) id 16fZ9j-0005He-00 for globillum@imag.fr; Tue, 26 Feb 2002 04:24:00 +0000 Message-ID: <004c01c1be7e$1d07c610$979c42d8@VANILLA> Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: 02/02/25 Release of RADBIB and GITHESIS Date: Mon, 25 Feb 2002 20:28:30 -0800 Organization: byHeart Consultants Limited MIME-Version: 1.0 Content-Type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 6.00.2600.0000 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2600.0000 X-Loop: globillum@imag.fr X-Sequence: 108 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: X-UIDL: BbB!!$:o"!*gl!!?Y-!! X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

ANNOUNCE: 02/02/25 Release of RADBIB and GITHESIS
-------------------------------------------------
RADBIB is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. It currently includes 2,019 references -- 9 new additions since its 02/01/01 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of February 25, 2002) from:

http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 255 references to radiosity and global illumination theses -- 1 new addition since the 02/01/01 release.

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

Ian Ashdown, P. Eng., LC, FIES
Chief Technology Officer
byHeart Consultants Limited
http://www.helios32.com

 

From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id g2H2tLX22147; Sun, 17 Mar 2002 03:59:22 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.9.3/8.8.5) id DAA10967; Sun, 17 Mar 2002 03:56:17 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.9.3/8.8.5) with ESMTP id DAA10962 for ; Sun, 17 Mar 2002 03:56:16 +0100 Received: from photon.look.ca (photon.look.ca [207.136.80.123]) by imag.imag.fr (8.11.6/8.11.6) with ESMTP id g2H2uFg13609 for ; Sun, 17 Mar 2002 03:56:16 +0100 (MET) Received: from bc-van-wvn-a53-01-10.look.ca ([216.66.156.106] helo=VANILLA) by photon.look.ca with smtp (Exim 3.12 #9) id 16mQqD-0006nI-00 for globillum@imag.fr; Sun, 17 Mar 2002 02:56:14 +0000 Message-ID: <000a01c1cd60$1468ede0$6a9c42d8@VANILLA> Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: 02/03/16 Release of RADBIB and GITHESIS Date: Sat, 16 Mar 2002 19:01:46 -0800 Organization: byHeart Consultants Limited MIME-Version: 1.0 Content-Type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 6.00.2600.0000 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2600.0000 X-Loop: globillum@imag.fr X-Sequence: 111 Precedence: list List-Help: List-Unsubscribe: List-Post: List-Owner: X-UIDL: *i@!!';C"!CX*!!+8h"! X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

ANNOUNCE: 02/03/16 Release of RADBIB and GITHESIS
-------------------------------------------------
RADBIB is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. It currently includes 2,033 references -- 14 new additions since its 02/02/25 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of March 16, 2002) from:

http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 260 references to radiosity and global illumination theses -- 4 new additions since the 02/02/25 release.

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

Ian Ashdown, P. Eng., LC, FIES
Chief Technology Officer
byHeart Consultants Limited
http://www.helios32.com

From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id g3U4s5X24025; Tue, 30 Apr 2002 06:54:06 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id g3U4xS121422; Tue, 30 Apr 2002 06:59:28 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id g3U4wWQ21385 for ; Tue, 30 Apr 2002 06:58:32 +0200 Received: from photon.look.ca (photon.look.ca [207.136.80.123]) by imag.imag.fr (8.11.6/8.11.6) with ESMTP id g3U4wWS22701 for ; Tue, 30 Apr 2002 06:58:32 +0200 (MEST) Received: from bc-van-wvn-a53-01-67.look.ca ([216.66.156.163] helo=VANILLA) by photon.look.ca with smtp (Exim 3.12 #9) id 172Pig-0006uZ-00 for globillum@imag.fr; Tue, 30 Apr 2002 04:58:30 +0000 Message-ID: <000a01c1f004$34c314a0$a39c42d8@VANILLA> Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: globillum@imag.fr Subject: Updated RADBIB and GITHESIS Date: Mon, 29 Apr 2002 22:02:16 -0700 Organization: byHeart Consultants Limited MIME-Version: 1.0 Content-Type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 6.00.2600.0000 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2600.0000 X-Loop: globillum@imag.fr X-Sequence: 119 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-UIDL: PoF"!;n["!_=n!!~(G"! X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

ANNOUNCE: 02/05/01 Release of RADBIB and GITHESIS
-------------------------------------------------
RADBIB is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. It currently includes 2,061 references -- 28 new additions since its 02/03/16 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of May 1, 2002) from:

http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 264 references to radiosity and global illumination theses -- 4 new additions since the 02/03/16 release.

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

Ian Ashdown, P. Eng., LC, FIES
Chief Technology Officer
byHeart Consultants Limited
http://www.helios32.com

PS - Due to threatened legal action from our ISP regarding spam messages, this announcement will no longer be posted to the comp.graphics and related newsgroups.

 

From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id g5FDxgX04642; Sat, 15 Jun 2002 15:59:43 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id g5FEA7m30846; Sat, 15 Jun 2002 16:10:07 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id g5FEA1Q30826 for ; Sat, 15 Jun 2002 16:10:01 +0200 Received: from parsec.look.ca (parsec.look.ca [207.136.80.122]) by imag.imag.fr (8.11.6/8.11.6) with ESMTP id g5FE9xQ16833 for ; Sat, 15 Jun 2002 16:10:00 +0200 (MEST) Received: from bc-van-wvn-a53-01-13.look.ca ([216.66.156.109] helo=VANILLA) by parsec.look.ca with smtp (Exim 3.32 #10) id 17JEFZ-00046y-00 for globillum@imag.fr; Sat, 15 Jun 2002 14:09:57 +0000 Message-ID: <004301c21476$5b340ef0$0100a8c0@VANILLA> Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: globillum@imag.fr Subject: RADBIB & GITHESIS updateANNOUNCE: 02/05/01 Release of RADBIB and GITHESIS Date: Sat, 15 Jun 2002 07:10:06 -0700 Organization: byHeart Consultants Limited MIME-Version: 1.0 X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 6.00.2600.0000 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2600.0000 X-Loop: globillum@imag.fr X-Sequence: 122 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: :U="!WXF"!&Z>"!^j&"! X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit ANNOUNCE: 02/05/01 Release of RADBIB and GITHESIS --------------------------------------------------------------- RADBIB is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. It currently includes 2,073 references -- 12 new additions since its 02/05/01 release. This bibliography is available in BibTex format as RADBIB.BIB (with a release date of June 13 2002) from: http://www.helios32.com (Resources section) Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 264 references to radiosity and global illumination theses -- no new additions since the 02/05/01 release. Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited. Ian Ashdown, P. Eng., LC, FIES Chief Technology Officer byHeart Consultants Limited http://www.helios32.com ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id g6FNghj20742; Tue, 16 Jul 2002 01:42:44 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id g6FNuGr25551; Tue, 16 Jul 2002 01:56:16 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id g6FNtkc25519 for ; Tue, 16 Jul 2002 01:55:46 +0200 Received: from smtp-2.llnl.gov (smtp-2.llnl.gov [128.115.250.82]) by imag.imag.fr (8.11.6/8.11.6) with ESMTP id g6FNtiS03630 for ; Tue, 16 Jul 2002 01:55:45 +0200 (MEST) Received: from cliff.llnl.gov (localhost [127.0.0.1]) by smtp-2.llnl.gov (8.9.3/8.9.3/LLNL-gateway-1.0) with ESMTP id QAA05948 for ; Mon, 15 Jul 2002 16:55:28 -0700 (PDT) Received: from llnl.gov ([134.9.13.35]) by cliff.llnl.gov (Netscape Messaging Server 4.15) with ESMTP id GZBEGM00.BTM for ; Mon, 15 Jul 2002 16:55:34 -0700 Sender: nelson@smtp-2.llnl.gov Message-ID: <3D3360F6.DDC1FF28@llnl.gov> Date: Mon, 15 Jul 2002 16:55:34 -0700 From: "Nelson L. Max" X-Mailer: Mozilla 4.79C-SGI [en] (X11; U; IRIX64 6.5 IP30) X-Accept-Language: en MIME-Version: 1.0 To: globillum@imag.fr Subject: 3DPVT and EGWR02 reports X-Loop: globillum@imag.fr X-Sequence: 125 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: ??0"!Qk7"!=1<"!S^4!! X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit On this year's trip I attended two conferences in Italy in consecutive weeks. Here are my reports. On the 3DPVT conference, I only summarized the papers that interested me, but on the EGWR conference I summarized all those presented. (One of the published papers was not persented due to travel connection problems). As usual, I apologize if I skipped or misrepresented your paper. 3D Data Processing Visualization and Transmission The 3D Data Processing Visualization and Transmission conference in Padova, Italy, June 19 - 21, had a large component of image based model acquisition and rendering papers. Silvio Savarese, Holly Rushmeier, Fausto Bernandini, and Pietro Perona described the "Implementation of a Shadow Carving System for Shape Capture" where volumes are carved away if they are inconsistent with the observed shadows, in images with multiple lighting directions and viewpoints. Li Zhang, Brian Curless, and Steven Seitz described a method of shape acquisition using stripes of colored light, in a sequence of colors chosen to avoid ambiguities in phase. The matching correspondences are found by multi-pass dynamic programming. Mark Levoy gave a keynote talk "Why is 3D scanning hard" in which he listed many difficulties, and showed examples of statues which he believes are not scannable, because of glossy surfaces, wide light diffusion, or geometries with inaccessible regions. Carlos Hernandez Esteban and Francis Schmitt described a multi-camera stereo system starting from a visual hull approximation using the silhouette images, then carving along an average viewing direction up to the point of best image correlation, and finally filtering the resulting carving depths to reduce noise. Takashi Matsuyama and Takeshi Takai "Generation, Visualization, and Editing of 3D Video" used texture mapping on the visual hull from silhouettes, as was done by Matusik et al. at Siggraph 2000. However they used a voxel-based method for the visual hull instead of a computational geometry one, and created the textures by interpolating carefully weighted average colors at each vertex of the marching cubes contour surface of their binary voxel volume. Their video results seemed superior to those of Matusik et al.. Carlo Colombo, Alberto Del Bimbo, and Federico Pernici showed that it is possible to do "Uncalibrated 3D metric reconstruction and flattened texture acquisition from a single view of a surface of revolution", since in this case there is enough information in a single view to determine the camera calibration and the shape of the curve being revolved. In "Texture at the Terminator" Jan Koenderink and Sylvia Pont discussed several ways of plotting the maximum, minimum, and median radiance of a region of a surface, and a ratio they call the "contrast", as functions of each other and of the angle of incident illumination. The plots for concrete duplicate those from a simple diffuse microfacet model, but those from plastic and crumpled aluminum are more complex due to specular reflection and multiple scattering. The graphs can be used to estimate the angle range of microfacet normals, and the effects of cast shadows on the bumps projecting out beyond the terminator can be used to estimate the maximum bump heights. James Davis, Stephen Marschner, Matt Garr, and Marc Levoy "Filling Holes in Complex Surfaces using Volumetric Diffusion" construct a signed distance function in the vicinity of the surface and then apply a diffusion process to extend this function through the volume until it bridges whatever holes may be present. Takeshi Masuda "Object Shape Modelling from Multiple Range Images by Matching Signed Distance Fields" iteratively applies rigid body motions to each distance field to minimize the deviation from the appropriately weighted average of the rest. Thomas Bulow "Spherical Diffusion for 3D Surface Smoothing" shows how star shaped objects can be smoothed by diffusing the height function on a sphere, and analyze the process using the spherical harmonic transform as an analog of the Fourier transform. John Isidoro and Stan Sclaroff "Stochastic Mesh-Based Multi-View Reconstruction" build the visual hull from simplified silhouettes, simplify and subdivide it, and then move the vertices according to a free-form deformation to match optimal deformation vectors along randomly chosen specific viewing rays, concentrated in areas of reprojection error. The deformation vectors are chosen to minimize the reprojection error (taking visibility into account). Greg Slabaugh, Ron Schafer, and Mat Hans, "Image-Based Photo Hulls" have an output-view-dependent color consistency algorithm. They determine the intersection of each viewing ray with the visual hull by the intersecting of the 2D intersections of its projection with the segmented foreground object in each input view. Then starting from the closest point on the visual hull, they step along the ray until color consistency is achieved. Christian Fruh and Avideh Zakhor, "Data Processing Algorithms for Generating Textured 3D Building Facade Meshes from Laser Scans and Camera Images", drove a truck equipped with side looking laser scanner and color cameras for about 7 km through downtown Berkeley. They segmented the foreground occluders away from the background facades, filled in the holes using hypotheses about the structure of the ground plane and facade geometry, and then applied the color texture from the non-occluded photograph most normal to the facade. There were also invited sessions on matching protein structure geometry to homologous evolutionarily related structures, ond on 3D geometry compression, plus numerous poster sessions. For the first meeting of this kind, the papers were of very good quality. The conference took place at the historic campus of the University of Padova, the second oldest in Italy, established in about 1225. The conference week was an unusually hot one for northern Italy, and on three successive mornings the electric power failed due to the overload from air conditioning. The posters were outside in the courtyard, so we switched to them when the power failed. However, the courtyard was also the scene of numerous individual congratulation and hazing ceremonies, at which graduating students's friends and family shouted out a particularly obscene graduation song. Eurographics Workshop on Rendering The Eurographics Workshop on Rendering is an established conference, and the 13th annual session was held in Pisa, Italy, on June 26 - 28. Here are summaries of all the papers presented. Fernandez, Bala, and Greenberg computed "Local Illumination Environments" which store in octree cells the fully and partially visible light sources and potential occluders for the cell, accelerating direct lighting computations. Wald, Kollig, Benthin, Keller, and Slusallek do parallel global illumination by tracing coherent ray groups with quasi-Monte Carlo integration sampling. Dimitriev, Brabek, Myszkowski, and Seidel do selective photon tracing for moving scenes, first tracing "pilot photons" to detect regions of change, and then tracing "corrective photons" for more accurate integration there. Coconu and Hege have an octree-based point rendering system, which composits in hardware RGBA splats, using the recursive back to front sort for the octree cells, and the LDI occlusion compatible ordering for the points in an octree node. Botsch, Wiratanaya, and Kobbelt replace the points by the octree cells themselves, splatting the cell centers. Since most cells will be empty for surfaces, they suggest an efficient encoding taking about 2 bits per full cell. They also encode the normals and colors, and shade the normal codes, rather than the individual points. Yang, Everett, Buehler, and McMillan described a system of 64 unsynchronized cheap firewire video cameras connected to 6 PCs, which warp on graphics cards only the parts of their input images that will be needed in the final novel image, composited by a seventh PC. With no use of geometry to enhance the light field reconstruction, multiple exposures are visible outside of the plane of focus. Sander, Gortler, Snyder, and Hoppe construct a metric tensor representing the detail in a color or normal texture, and reparametrize the texture coordinate charts to minimize the stretch in this metric, putting the texture detail where it is needed most. Zelinka and Garland do very fast texture synthesis from examples using a jump map, which lists for each input pixel a set of matching input pixels. A new texture pixel is usually synthesized by extending the input patch of one of its neighbors, but occasionally a jump to a new patch is taken using the jump map. Lefebvre and Neyret generate either color or bump-map tree bark textures by an approximate simulation of the cracking process of the inelastic bark layers as the tree grows in diameter beneath them. Ward and Eydelberg-Vileshin render color accurately by defining the surface colors in CIE XYZ space using spectral integration with the spectrum of the dominant illuminant (good for direct illumination from a single kind of source, but not for multiple bounces or spectrally different sources) and then correct for white-point balancing in the "Sharp color space", which is based on super-saturated RGB primaries. Beckaert, Sbert, and Halton speed up path tracing by reusing all but the first leg of the ray paths at nearby pixels. Cammarano and Wann Jensen do time dependent photon mapping for correct motion blur of caustics by storing time as well as color, energy, and direction at each photon hit, and then averaging photons that are near in time as well as in space when rendering with a distributed ray caster. Ashikhman maps high dynamic range input images to a limited output range by determining a local adaptation level (the average over the largest neighborhood without high contrast), tone mapping this adaptation level using linear compression, and then putting back the detailed contrast by multiplying by the ratio of the input pixel value to the local adaptation level. Sawhney, Arpa, Kumar, Samarasekera, Aggarwal, Hsu, Nister, and Hanna map multiple real-time video surveillance images as textures onto a navigable urban geometric environment model. Yamazaki, Sagawa, Kawasaki, Ikeuchi, and Sakauchi extract RGBZ microfacets from a laser-scanner / color-camera input images by clipping the color/range data to small cubical volumes, and projecting it onto small quadrilaterals perpendicular to the output viewing directions. The projection and depth clipping is done in hardware by converting the depth to an opacity, and using register combiners and alpha clipping. Jeshke and Wimmer simplify a complex model into textured polygonal meshes suitable for a specific view cell by scan converting the model into a voxel representation using depth-clipped hardware rendering into layers. The layer spacing is chosen so that parallax from a moving viewpoint within the view cell is no more than one pixel. The layers are processed in front-to-back order, in order to delete all occluded voxels, with special treatment for the one-pixel-wide border between filled and empty pixels in each layer. An initial complex polygonal mesh is constructed and then simplified, with the constraint that the simplified mesh must cover exactly all the non-occluded voxels. Nirenstein, Blake, and Gain do exact polygon-to-polygon visibility by representing all stabbing lines connecting the two polygons in a 5D euclidean space using Plucker coordinates (with one of the six coordinates normalized to 1). By computational geometry in this space, volumes are subtracted for stabbing lines hitting each occluder, leaving the non-occluded stabbing lines. This is applied to give exact visibility culling for a polyhedral viewpoint volume. Baxter, Sud, Govindaraju, and Manocha achieve interactive walkthroughs for huge complex environments, with a parallel pipelined system using two graphics pipelines and three CPU processes, based on an axis aligned bounding box scene hierarchy, hierarchical Z buffer occlusion culling, and level of detail decisions.The first process drives one pipeline renders an Item/Z buffer from the culled geometry for the previous frame, which is read back for the hierarchical Z buffer occlusion cull. Another process performs the view frustum and occlusion culls and level of detail decisions in software, and the third process drives the final rendering in the second graphics pipeline. Secord, Heidrich, and Striet place point or stroke primitives for illustration-style rendering of a grey scale image, by redistributing a predefined Poisson-disc or Halton sequence 2D point distribution. The marginal y cumulative distribution of intensity in the input image (found by integration in x along scan lines) is used to redistribute the y coordinates, and then the cumulative distribution in x on the scan lines is used to redistribute the x coordinates. Corrections are made to account for the probability that multiple stokes are assigned to the same pixel. Stroke direction can be determined from image gradients, colors, or information from a 3D model, if available. Freudenberg, Masuch, and Strothotte use blending operations on graphics hardware to emulate the halftone screening process traditionally used in the printing industry. Hertzmann, Oliver, Curless, and Seitz create line drawing line styles from examples, by adapting ideas from texture synthesis from examples. Masselus, Dutre, and Anrys capture the reflectance field of an object by determining the position of a hand-moved light source from its effects on four small diffusely reflecting spheres. Furukawa, Kawasaki, Ikeuchi, and Sakauchi compress a 4D bi-directional texture function measured from images of an object under varying illumination, using a tensor product expansion. Matusik, Pfister, Ziegler, Ngan, and McMillan acquire low resolution reflectance information for a reflecting and refracting object using a traditional set-up of multiple rotating lights, a fixed set of cameras, and a rotating turntable for the object. But they add two large plasma panel monitors, a horizontal one below the turntable, and a vertical one behind the object, to obtain high resolution reflection and refraction information, each represented by a gaussian weight distribution about a reflection or refraction direction, as determined by fitting the response to 1D sinusoidal wave patterns in three orientations on the monitors. These monitor views are also used for detecting an alpha-matted visual hull. The parameters of the gaussians are determined for a new view using unstructured lumigraph interpolation, and used to convolve with a new environment map. Wexler, Fitzgibbon, and Zisserman solve a similar problem by using a sequence of images of a transparent object, moving in front of a fixed planar background image, but use a weighted combination of a few nearby pixels instead of a gaussian, and consider only refraction. Kautz, Sloan, and Snyder convolve a BRDF with an environment map by representing both with spherical harmonics. The necessary rotations of the spherical harmonic coefficients for the environment into the local frame for the surface are done per vertex in software. The rotation of the viewing vector, the look-up of the spherical harmonic coefficients for expansion in the lighting direction from a texture function of the viewing vector, and the dot product of the two aligned spherical harmonic coefficients to do the convolution in frequency space, are done per pixel in hardware. Akenine-Moller and Assarsson generalize Frank Crow's shadow volume method to penumbras by following along profile contour polylines creating a shadow wedge for each edge, bounded by the umbra plane, the penumbra plane, and two side planes separating the wedge for the current edge from those from the preceding and following edges on the contour. If a surface point is found to lie inside a wedge, a light intensity is found by bilinear interpolation within the quadrilateral where the plane through the viewing ray parallel to the profile edge intersects the wedge. -- email: max2@llnl.gov Nelson Max, Mail Stop L-560 http://www.llnl.gov/graphics Lawrence Livermore National Laboratory phone (925) 422-4074 7000 East Avenue fax (925) 422-6287 Livermore, CA 94550, USA ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id g6TEtdj04002 for ; Mon, 29 Jul 2002 16:55:39 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id g6TFAmJ28361 for wp@cg.tuwien.ac.at; Mon, 29 Jul 2002 17:10:48 +0200 Date: Mon, 29 Jul 2002 17:10:48 +0200 Message-Id: <200207291510.g6TFAmJ28361@chopinette.imag.fr> To: wp@cg.tuwien.ac.at From: listes@imag.fr Subject: Removed from globillum X-UIDL: CPX!!hT@"!i_k!!LXS"! X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit Your address (wp@cg.tuwien.ac.at) has been removed from list globillum@imag.fr, probably because we received non-delivery reports for your address. You can subscribe again : mailto:listes@imag.fr?subject=sub%20globillum From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id g6U89Xj14732; Tue, 30 Jul 2002 10:09:34 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id g6U8OfS02830; Tue, 30 Jul 2002 10:24:41 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id g6U8OWc02811 for ; Tue, 30 Jul 2002 10:24:32 +0200 Received: from nic.funet.fi (nic.funet.fi [193.166.3.1]) by imag.imag.fr (8.11.6/8.11.6) with ESMTP id g6U8OUh04259 for ; Tue, 30 Jul 2002 10:24:31 +0200 (MEST) Received: (from localhost user: 'kouhia' uid#241 fake: STDIN (kouhia@nic.funet.fi)) by nic.funet.fi id ; Tue, 30 Jul 2002 11:24:29 +0300 Sender: Juhana Sadeharju From: Juhana Sadeharju To: globillum@imag.fr Subject: no html please Message-Id: <20020730082429Z13885-12376+9182@nic.funet.fi> Date: Tue, 30 Jul 2002 11:24:29 +0300 X-Loop: globillum@imag.fr X-Sequence: 126 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: km1!!*K0!!X=="!BF)#! X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 MIME-Version: 1.0 Content-transfer-encoding: 8bit This is a multi-part message in MIME format... ------------=_1028017476-1394-0 Hello. Please don't post html mails to globillum. Our server bounces them, and globillum list kicks me out of the list. Can list maintainer do something because I do want to receive at least non-html mails? Best regards, Juhana ------------=_1028017476-1394-0 Content-Type: text/plain; name="message.footer" Content-Disposition: inline; filename="message.footer" Content-Transfer-Encoding: 8bit ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- ------------=_1028017476-1394-0-- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id g6UFckj19749; Tue, 30 Jul 2002 17:38:47 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id g6UFriw06189; Tue, 30 Jul 2002 17:53:44 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id g6UFrcc06170 for ; Tue, 30 Jul 2002 17:53:38 +0200 Received: from lmi.net (lanfill.lmi.net [208.25.68.10]) by imag.imag.fr (8.11.6/8.11.6) with ESMTP id g6UFrbh00022 for ; Tue, 30 Jul 2002 17:53:37 +0200 (MEST) Received: from photon.exponent.com (hat38.ppp.lmi.net [208.25.88.106]) by lmi.net (8.8.8/8.8.7) with ESMTP id IAA17323 for ; Tue, 30 Jul 2002 08:53:35 -0700 (PDT) Date: Tue, 30 Jul 2002 08:51:22 -0700 Mime-Version: 1.0 Subject: Radiance workshop reminder From: Greg Ward To: globillum@imag.fr Message-Id: <325FDEEE-A3D4-11D6-B80F-00306540F848@lmi.net> X-Mailer: Apple Mail (2.482) X-Loop: globillum@imag.fr X-Sequence: 129 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: iQ1"!@lD!!5Nj!!Z Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id g7II8Pu31352; Sun, 18 Aug 2002 20:08:26 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id g7IJ8YH02084; Sun, 18 Aug 2002 21:08:34 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id g7IJ6p901980 for ; Sun, 18 Aug 2002 21:06:51 +0200 Received: from parsec.look.ca (parsec.look.ca [207.136.80.122]) by imag.imag.fr (8.11.6/8.11.6) with ESMTP id g7IJ6mT16443 for ; Sun, 18 Aug 2002 21:06:49 +0200 (MEST) Received: from bc-van-wvn-a53-01-39.look.ca ([216.66.156.135] helo=VANILLA) by parsec.look.ca with smtp (Exim 4.05) id 17gVNs-0003H6-00 for globillum@imag.fr; Sun, 18 Aug 2002 19:06:45 +0000 Message-ID: <000d01c246ea$b430bde0$0100a8c0@VANILLA> Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: 02/08/17 Release of RADBIB and GITHESIS Date: Sun, 18 Aug 2002 12:08:55 -0700 Organization: byHeart Consultants Limited MIME-Version: 1.0 Content-Type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 6.00.2600.0000 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2600.0000 X-Loop: globillum@imag.fr X-Sequence: 130 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-UIDL: GJK"!Wm_!!Bbd!!IJ-"! X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

ANNOUNCE: 02/08/17 Release of RADBIB and GITHESIS
-------------------------------------------------
RADBIB is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. It currently includes 2,078 references -- 5 new additions since its 02/06/13 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of August 17, 2002) from:

http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 265 references to radiosity and global illumination theses -- one new addition since the 02/06/13 release. (Congratulations, Ravi!)

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

Ian Ashdown, P. Eng., LC, FIES
Chief Technology Officer
byHeart Consultants Limited
http://www.helios32.com

 

From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id g8SGsL809956; Sat, 28 Sep 2002 18:54:22 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id g8SGrew27722; Sat, 28 Sep 2002 18:53:40 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id g8SGr2u27667 for ; Sat, 28 Sep 2002 18:53:02 +0200 Received: from twiddle.look.ca (twiddle.look.ca [207.136.80.125]) by imag.imag.fr (8.11.6/8.11.6) with ESMTP id g8SGr1310030 for ; Sat, 28 Sep 2002 18:53:02 +0200 (MEST) Received: from bc-van-wvn-a53-01-81.look.ca ([216.66.156.177] helo=VANILLA) by twiddle.look.ca with smtp (Exim 4.05) id 17vKpp-0001Eh-00 for globillum@imag.fr; Sat, 28 Sep 2002 12:52:55 -0400 Message-ID: <000c01c2670f$fc346de0$0100a8c0@VANILLA> Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: 02/09/30 Release of RADBIB and GITHESIS Date: Sat, 28 Sep 2002 09:56:18 -0700 Organization: byHeart Consultants Limited MIME-Version: 1.0 Content-Type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 6.00.2800.1106 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1106 X-Loop: globillum@imag.fr X-Sequence: 135 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-UIDL: j/^"!*K("!!:e!!T8:"! X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit ANNOUNCE: 02/09/30 Release of RADBIB and GITHESIS
-------------------------------------------------
RADBIB is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. It currently includes 2,095 references -- 17 new additions since its 02/08/17 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of September 30, 2002) from:

http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 271 references to radiosity and global illumination theses -- 6 new additions since the 02/08/17 release.

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

Ian Ashdown, P. Eng., LC, FIES
Chief Technology Officer
byHeart Consultants Limited
http://www.helios32.com From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id g9L8mKh27015; Mon, 21 Oct 2002 10:48:21 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id g9L8lvK24219; Mon, 21 Oct 2002 10:47:57 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id g9L8lqu24200 for ; Mon, 21 Oct 2002 10:47:52 +0200 Received: from hermes.cs.kuleuven.ac.be (hermes.cs.kuleuven.ac.be [134.58.40.3]) by imag.imag.fr (8.11.6/8.11.6) with ESMTP id g9L8loJ12085 for ; Mon, 21 Oct 2002 10:47:51 +0200 (MEST) Received: from cs.kuleuven.ac.be (dr-zook.cs.kuleuven.ac.be [134.58.41.20]) by hermes.cs.kuleuven.ac.be (A_Good_MTA/0.6.11) with SMTP id g9L8lfl26499 for ; Mon, 21 Oct 2002 10:47:41 +0200 (MEST) Received: by cs.kuleuven.ac.be; id KAA15219; Mon, 21 Oct 2002 10:47:36 +0200 Received: from nodnsquery(134.58.41.11) by dr-zook.cs.kuleuven.ac.be via csmap (V4.1) id srcAAA0nwc83; Mon, 21 Oct 02 10:47:34 +0200 Received: from cs.kuleuven.ac.be (luxo.cs.kuleuven.ac.be [134.58.39.227]) by iris.cs.kuleuven.ac.be (A_Good_MTA/0.6.11) with ESMTP id g9L8lX815248 for ; Mon, 21 Oct 2002 10:47:33 +0200 (MEST) Sender: Frank.Suykens@cs.kuleuven.ac.be Message-ID: <3DB3BF62.BB6CFB1B@cs.kuleuven.ac.be> Date: Mon, 21 Oct 2002 10:48:34 +0200 From: Frank Suykens Organization: K.U.Leuven X-Mailer: Mozilla 4.77 [en] (X11; U; Linux 2.4.4-4GB i686) X-Accept-Language: en MIME-Version: 1.0 To: globillum@imag.fr Subject: PhD. Thesis online X-Loop: globillum@imag.fr X-Sequence: 136 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: iLd"!L0##!^;$#!^OW"! X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hi, I just want to announce that my Ph.D. thesis, entitled "On robust Monte Carlo algorithms for multi-pass global illumination", is online at: http://www.cs.kuleuven.ac.be/~graphics/CGRG.PUBLICATIONS/FRANKPHD/ Abstract, table of contents, and downloads in various formats can be found there. Best regards, Frank Suykens. -- -==========================================================- Frank Suykens (Frank.Suykens@cs.kuleuven.ac.be, ++32 16 327833) Graphics, K.U. Leuven http://www.cs.kuleuven.ac.be/~graphics/ -==========================================================- "I believe that global illumination will become the norm. Direct illumination renderers like prman have reached the limit of the realism they can produce in terms of lighting." Kaveh Kardan, Square USA, in an Ars Technica interview ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id g9M45Mh13430; Tue, 22 Oct 2002 06:05:24 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id g9M3woe31539; Tue, 22 Oct 2002 05:58:50 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id g9M3wiu31520 for ; Tue, 22 Oct 2002 05:58:44 +0200 Received: from gpo.stanford.edu (gpo.Stanford.EDU [171.64.77.203]) by imag.imag.fr (8.11.6/8.11.6) with ESMTP id g9M3wh301906 for ; Tue, 22 Oct 2002 05:58:43 +0200 (MEST) Received: (qmail 26310 invoked from network); 22 Oct 2002 03:58:40 -0000 Received: from dda.stanford.edu (HELO dda.Stanford.EDU.stanford.edu) (171.64.77.104) by electrolux.Stanford.EDU with SMTP; 22 Oct 2002 03:58:40 -0000 From: Marc Levoy MIME-Version: 1.0 Message-ID: <15796.52464.603154.982427@dda.Stanford.EDU> Date: Mon, 21 Oct 2002 20:58:40 -0700 To: globillum@imag.fr CC: glab@graphics CC: glab@graphics Subject: Nicodemus online X-Mailer: VM 7.07 under Emacs 21.2.1 X-Loop: globillum@imag.fr X-Sequence: 137 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: \)h"!]1:!!(Q##!J3a!! X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Fellow researchers in computer graphics, Jack Hsia, one of the authors of the classic 1977 paper on BRDF nomenclature, by Nicodemus et al., has kindly agreed to have the paper optically scanned and placed online. You can find it at: http://physics.nist.gov/spectrophotometry -Marc Levoy Stanford University ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id gABG0Oh06895; Mon, 11 Nov 2002 17:00:25 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id gABG0BX02300; Mon, 11 Nov 2002 17:00:11 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id gABG03u02281 for ; Mon, 11 Nov 2002 17:00:03 +0100 Received: from nut.autodesk.com (nut.autodesk.com [198.102.112.27]) by imag.imag.fr (8.11.6/8.11.6) with ESMTP id gABG01I21773 for ; Mon, 11 Nov 2002 17:00:02 +0100 (MET) Received: from hqmsgsrf00.autodesk.com (hqmsgsrf00.autodesk.com [144.111.32.210]) by nut.autodesk.com (8.12.5/8.12.5) with ESMTP id gABFxvV0020633; Mon, 11 Nov 2002 07:59:57 -0800 (PST) Received: by hqmsgsrf00.autodesk.com with Internet Mail Service (5.5.2653.19) id ; Mon, 11 Nov 2002 07:59:57 -0800 Message-ID: From: eric.haines@autodesk.com To: globillum@imag.fr Cc: henrik@graphics.stanford.edu Subject: Another photon mapping book Date: Mon, 11 Nov 2002 07:59:24 -0800 MIME-Version: 1.0 X-Mailer: Internet Mail Service (5.5.2653.19) Content-Type: text/html; charset=windows-1252 X-Loop: globillum@imag.fr X-Sequence: 140 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-UIDL:

I ran across this book recently: http://www.premierpressbooks.com/catalog/product.cfm?category=Game%20Development&isbn=1592000088 - a surprising thing, a book about photon mapping made as a paperback in their "Game Developer" series.

 

Eric

From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id gABMlPh10259; Mon, 11 Nov 2002 23:47:26 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id gABMl4U03536; Mon, 11 Nov 2002 23:47:04 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id gABMklu03503 for ; Mon, 11 Nov 2002 23:46:47 +0100 Received: from quark.look.ca (quark.look.ca [207.136.80.22]) by imag.imag.fr (8.11.6/8.11.6) with ESMTP id gABMkkI06432 for ; Mon, 11 Nov 2002 23:46:46 +0100 (MET) Received: from bc-van-wvn-a53-01-74.look.ca ([216.66.156.170] helo=VANILLA) by quark.look.ca with smtp (Exim 4.05) id 18BNK4-0001V7-00 for globillum@imag.fr; Mon, 11 Nov 2002 22:46:25 +0000 Message-ID: <001601c289d4$d88b8710$0100a8c0@VANILLA> Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: globillum@imag.fr Date: Mon, 11 Nov 2002 14:51:15 -0800 Organization: byHeart Consultants Limited MIME-Version: 1.0 X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 6.00.2800.1106 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1106 Subject: ANNOUNCE: 02/11/11 Release of RADBIB and GITHESIS Content-Type: text/html; charset=windows-1252 X-Spam-Status: No, hits=0.8 required=6.0 tests=NOSPAM_INC,SPAM_PHRASE_00_01,SUPERLONG_LINE,USER_AGENT_OE version=2.43 X-Loop: globillum@imag.fr X-Sequence: 141 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-UIDL: =l4!!%2P"!PLa"!'8M!! X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

ANNOUNCE: 02/11/11 Release of RADBIB and GITHESIS
-------------------------------------------------
RADBIB is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. It currently includes 2,136 references -- 41 new additions since its 02/09/30 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of November 11, 2002) from:

http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 273 references to radiosity and global illumination theses -- 2 new additions since the 02/09/30 release.

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id gAGJjDh21078; Sat, 16 Nov 2002 20:45:14 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id gAGJipH07877; Sat, 16 Nov 2002 20:44:51 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id gAGJifM07858 for ; Sat, 16 Nov 2002 20:44:41 +0100 Received: from e35.co.us.ibm.com (e35.co.us.ibm.com [32.97.110.133]) by imag.imag.fr (8.11.6/8.11.6) with ESMTP id gAGJid622505 for ; Sat, 16 Nov 2002 20:44:40 +0100 (MET) Received: from westrelay02.boulder.ibm.com (westrelay02.boulder.ibm.com [9.17.194.23]) by e35.co.us.ibm.com (8.12.2/8.12.2) with ESMTP id gAGJiWsr037398 for ; Sat, 16 Nov 2002 14:44:32 -0500 Received: from d01ml244.pok.ibm.com (d01av02.pok.ibm.com [9.56.224.216]) by westrelay02.boulder.ibm.com (8.12.3/NCO/VER6.4) with ESMTP id gAGJiVUP132520 for ; Sat, 16 Nov 2002 12:44:32 -0700 Importance: Normal Subject: tone reproduction/image metrics code To: globillum@imag.fr X-Mailer: Lotus Notes Release 5.0.7 March 21, 2001 Message-ID: From: Holly Rushmeier Date: Sat, 16 Nov 2002 14:44:29 -0500 X-MIMETrack: Serialize by Router on D01ML244/01/M/IBM(Release 6.0 [IBM]|November 8, 2002) at 11/16/2002 14:44:31 MIME-Version: 1.0 X-Loop: globillum@imag.fr X-Sequence: 143 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: )lh"!U[k"!acW!!~Sl"! X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hi -- I have recently gotten various requests for code for tone reproduction operators and better-than-pixel-rms image comparisons. I don't have code on hand to make available to people, and quick Google checks didn't turn up any obvious repositories for this type of code. Is any one maintaining sites for freely available code for either of these problems? As we near the paper deadlines I forsee more people looking for this stuff, as we are always asking people to compare their results with previous methods. -- Holly __________________________ Holly Rushmeier ,hertjwr@us.ibm.com, http://www.research.ibm.com/people/h/holly (914)784-7252 IBM TJ Watson Research Center, 19 Skyline Drive, Hawthorne, NY 10532, USA ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id gAIFkUh14041; Mon, 18 Nov 2002 16:46:31 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id gAIFk5802187; Mon, 18 Nov 2002 16:46:05 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id gAIFjvo02168 for ; Mon, 18 Nov 2002 16:45:57 +0100 Received: from e5.ny.us.ibm.com (e5.ny.us.ibm.com [32.97.182.105]) by imag.imag.fr (8.11.6/8.11.6) with ESMTP id gAIFjup20156 for ; Mon, 18 Nov 2002 16:45:56 +0100 (MET) Received: from northrelay02.pok.ibm.com (northrelay02.pok.ibm.com [9.56.224.150]) by e5.ny.us.ibm.com (8.12.2/8.12.2) with ESMTP id gAIFjn4s075146 for ; Mon, 18 Nov 2002 10:45:49 -0500 Received: from d01ml244.pok.ibm.com (d01av02.pok.ibm.com [9.56.224.216]) by northrelay02.pok.ibm.com (8.12.3/NCO/VER6.4) with ESMTP id gAIFjg8p045762 for ; Mon, 18 Nov 2002 10:45:43 -0500 Importance: Normal Subject: Re: tone reproduction/image metrics code To: globillum@imag.fr X-Mailer: Lotus Notes Release 5.0.7 March 21, 2001 Message-ID: From: Holly Rushmeier Date: Mon, 18 Nov 2002 10:45:41 -0500 X-MIMETrack: Serialize by Router on D01ML244/01/M/IBM(Release 6.0 [IBM]|November 8, 2002) at 11/18/2002 10:45:44 MIME-Version: 1.0 X-Loop: globillum@imag.fr X-Sequence: 144 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: @0J!!f0M!!j8'"!n9+"! X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit >>From Erik: __________________________ Holly Rushmeier ,hertjwr@us.ibm.com, http://www.research.ibm.com/people/h/holly (914)784-7252 IBM TJ Watson Research Center, 19 Skyline Drive, Hawthorne, NY 10532, USA ---------------------- Forwarded by Holly Rushmeier/Watson/IBM on 11/18/2002 10:40 AM --------------------------- Erik Reinhard on 11/17/2002 11:45:26 AM To: Holly Rushmeier/Watson/IBM@IBMUS Subject: Re: tone reproduction/image metrics code Hi, Regarding tone reproduction operators, here's what I know/have: the Radiance package implements Greg Ward's histogram adjustment technique. Source code for our photographic tone reproduction operator (Siggraph '02) is freely available online (it implements a newer version which automates two parameters that used to be manual): http://www.cs.ucf.edu/~reinhard/Reinhard02/ I have research code for a number of other operators, but this code is not cleaned up, messy and comes with no guarantees, and is for those reasons not online. If any one has a need for that code, I'd be happy to share - please send e-mail. Cheers, Erik ____________________________________ Erik Reinhard reinhard@cs.ucf.edu ____________________________________ ------------------------------------------------- This mail sent through IMP: http://horde.org/imp/ ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From To: "Georg Zotti" , "Alessandro Artusi" , "Attila Neumann" , "Michael Wimmer" , "Alexander Wilkie" , "Christiane Ulbricht" , "Jiri Bittner" , bittner@cg.tuwien.ac.at From: Werner Purgathofer Subject: globillum mailing list Message-Id: <5.1.1.6.0.20021121121502.01fe7968@mail.cg.tuwien.ac.at> X-Eudora-Signature: X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Date: Thu, 21 Nov 2002 12:18:52 Content-type: text/html; charset=windows-1252 MIME-Version: 1.0 Content-transfer-encoding: 8bit Dear all,
I assume that you are all registered for the "Globillum" mailing list. If not, you should do this as soon as possible. Ask Alex how to do that, he should no.
Werner


--
 Werner Purgathofer             | Tel. +43(1)58801 18648     
 Technische Universitaet Wien   | http://www.cg.tuwien.ac.at
From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id gANIHuh13204; Sat, 23 Nov 2002 19:17:57 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id gANIHiK23094; Sat, 23 Nov 2002 19:17:44 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id gANIGjo23041 for ; Sat, 23 Nov 2002 19:16:45 +0100 Received: from twiddle.look.ca (twiddle.look.ca [207.136.80.125]) by imag.imag.fr (8.11.6/8.11.6) with ESMTP id gANIGiU14215 for ; Sat, 23 Nov 2002 19:16:44 +0100 (MET) Received: from bc-van-wvn-a53-01-90.look.ca ([216.66.156.186] helo=VANILLA) by twiddle.look.ca with smtp (Exim 4.05) id 18Fepb-0006eO-00 for globillum@imag.fr; Sat, 23 Nov 2002 13:16:40 -0500 Message-ID: <001601c2931d$3169d7f0$0100a8c0@VANILLA> Reply-To: "Ian Ashdown" From: "Ian Ashdown" To: globillum@imag.fr Date: Sat, 23 Nov 2002 10:21:49 -0800 Organization: byHeart Consultants Limited MIME-Version: 1.0 X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 6.00.2800.1106 X-MIMEOLE: Produced By Microsoft MimeOLE V6.00.2800.1106 Subject: RADBIB and GITHESIS ... yet another update Content-Type: text/html; charset=windows-1252 X-Spam-Status: No, hits=0.8 required=6.0 tests=NOSPAM_INC,SPAM_PHRASE_00_01,SUPERLONG_LINE,USER_AGENT_OE version=2.43 X-Loop: globillum@imag.fr X-Sequence: 146 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-UIDL:

ANNOUNCE: 02/11/23 Release of RADBIB and GITHESIS
RADBIB is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. It currently includes 2,161 references -- 25 new additions since its 02/11/23 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of November 23, 2002) from:

http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 273 references to radiosity and global illumination theses -- no new additions since the 02/11/11 release.

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.
Ian Ashdown, P. Eng., LC, FIES
President
byHeart Consultants Limited
http://www.helios32.com
From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id gB5LA3h05055; Thu, 5 Dec 2002 22:10:04 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id gB5L9rY06411; Thu, 5 Dec 2002 22:09:53 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id gB5L7aK06346 for ; Thu, 5 Dec 2002 22:07:36 +0100 Received: from MAIL03.toast.net (mail.toast.net [206.244.185.10]) by imag.imag.fr (8.11.6/8.11.6) with ESMTP id gB5L7Z308697 for ; Thu, 5 Dec 2002 22:07:35 +0100 (MET) Received: from delldaextn (unverified [66.19.11.113]) by MAIL03.toast.net (Vircom SMTPRS 1.4.232) with ESMTP id ; Thu, 5 Dec 2002 16:05:50 -0500 From: "A Gallardo" To: "Holly Rushmeier" , globillum@imag.fr Subject: RE: Shockwave/modeling package Date: Thu, 5 Dec 2002 04:07:42 -0500 Message-ID: <000201c29c3d$c4786d80$710b1342@delldaextn> MIME-Version: 1.0 X-Priority: 3 (Normal) X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook 8.5, Build 4.71.2173.0 In-Reply-To: Importance: Normal X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1106 X-Loop: globillum@imag.fr X-Sequence: 149 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: [9$"!''E!!NYg"!9M#!! X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hi, I have not posted here for awhile but I have something to contribute. :) Most Shockwave 3D outputs I have seen are either from 3DS MAX or LW and others with built-in modules/ plugins for 3D shockwave output. I have no clue though if SW3D is capable of handling interpolated vertex shading info and 'storage' but surely raster-based texture maps derived from GI/Radiosity solutions should work. As for cheap modelers under 100 there are a lot but there free ones online that are very good although most only runs on Win32's environment: Hamapatch: spline-based http://www.hamapatch.t2u.com/ Metasequoia: LW toolset inspired polygon modeler: http://www1.sphere.ne.jp/mizno/main_e.html Softy3D: organic metaballs modeler: http://www.softy3d.com/en/index.htm SoftCAd Lite: CAD modeler lite version http://www.softcad.com/index.asp?page=product/do_fS3D.asp SPATCH: Spline organic modeler http://www.eatonhand.com/images/spatch.htm OpenFX: 3D modeler,animation program with source code http://www.openfx.org/news/index.php Photomodeler lite:3d models from photos http://www.photomodeler.com/Lite/ Loq Ariou: 3d sketch modeler: http://www.quelsolaar.com/loqairou/index.html WINGS 3D: Polygon modeler based on NENDO http://www.wings3d.com/ STRATA 3D: free 3d modeler http://www.computerarts.co.uk/downloads/3d/apps.asp?page=1 turboCAD LE: http://nct.digitalriver.com/fulfill/0002.16 Good Luck! Sincerely, Arnold Gallardo Visual Content Creator Technical Writer > -----Original Message----- > From: Holly Rushmeier [mailto:hertjwr@us.ibm.com] > Sent: Thursday, December 05, 2002 3:06 PM > To: globillum@imag.fr > Subject: Shockwave/modeling package > > > > > > > I would like to know what experience people have had with a couple of > things: > > -- Has anybody experimented with advanced rendering techniques withing > Shockwave 3D? > Before getting into learning a new package, I would like to know if there > are some major > problems/limitations with doing things like operating on multiple textures > or using > specific types of hardware. So far everything I have seen refers to > exporting things defined > in Studiomax or similar package, has anybody tried writing their > own custom > rendering > in Shockwave? > They have a nice demo accessible from > http://www.macromedia.com/support/director/ts/documents/render_test.htm > but it has an unsettling warning about possible blue screen results. > > -- Does anybody know of really cheap 3D modeling packages (less than $100) > that are > useful for defining basic scenes? > > ____________ > Holly > > > __________________________ > Holly Rushmeier ,hertjwr@us.ibm.com, > http://www.research.ibm.com/people/h/holly (914)784-7252 > IBM TJ Watson Research Center, 19 Skyline Drive, Hawthorne, NY 10532, USA > > ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id gB5K72h04569; Thu, 5 Dec 2002 21:07:02 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id gB5K6n202638; Thu, 5 Dec 2002 21:06:49 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id gB5K6eK02353 for ; Thu, 5 Dec 2002 21:06:40 +0100 Received: from e33.co.us.ibm.com (e33.co.us.ibm.com [32.97.110.131]) by imag.imag.fr (8.11.6/8.11.6) with ESMTP id gB5K6d306026 for ; Thu, 5 Dec 2002 21:06:39 +0100 (MET) Received: from westrelay04.boulder.ibm.com (westrelay04.boulder.ibm.com [9.17.193.32]) by e33.co.us.ibm.com (8.12.2/8.12.2) with ESMTP id gB5K6aae008854 for ; Thu, 5 Dec 2002 15:06:37 -0500 Received: from d01ml244.pok.ibm.com (d01av02.pok.ibm.com [9.56.224.216]) by westrelay04.boulder.ibm.com (8.12.3/NCO/VER6.4) with ESMTP id gB5K9V4Y025848 for ; Thu, 5 Dec 2002 13:09:32 -0700 Importance: Normal Subject: Shockwave/modeling package To: globillum@imag.fr X-Mailer: Lotus Notes Release 5.0.7 March 21, 2001 Message-ID: From: Holly Rushmeier Date: Thu, 5 Dec 2002 15:06:28 -0500 X-MIMETrack: Serialize by Router on D01ML244/01/M/IBM(Release 6.0 [IBM]|November 8, 2002) at 12/05/2002 15:06:32 MIME-Version: 1.0 X-Loop: globillum@imag.fr X-Sequence: 147 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: $K]"!BlG!!I~o!!^Yg!! X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit I would like to know what experience people have had with a couple of things: -- Has anybody experimented with advanced rendering techniques withing Shockwave 3D? Before getting into learning a new package, I would like to know if there are some major problems/limitations with doing things like operating on multiple textures or using specific types of hardware. So far everything I have seen refers to exporting things defined in Studiomax or similar package, has anybody tried writing their own custom rendering in Shockwave? They have a nice demo accessible from http://www.macromedia.com/support/director/ts/documents/render_test.htm but it has an unsettling warning about possible blue screen results. -- Does anybody know of really cheap 3D modeling packages (less than $100) that are useful for defining basic scenes? ____________ Holly __________________________ Holly Rushmeier ,hertjwr@us.ibm.com, http://www.research.ibm.com/people/h/holly (914)784-7252 IBM TJ Watson Research Center, 19 Skyline Drive, Hawthorne, NY 10532, USA ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id gB5KGnh04688; Thu, 5 Dec 2002 21:16:50 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id gB5KGe103133; Thu, 5 Dec 2002 21:16:40 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id gB5KGVK03113 for ; Thu, 5 Dec 2002 21:16:31 +0100 Received: from mail-imagis (mail-imagis.inrialpes.fr [194.199.26.22]) by imag.imag.fr (8.11.6/8.11.6) with ESMTP id gB5KGS306600; Thu, 5 Dec 2002 21:16:28 +0100 (MET) Received: from imag.fr (cormier [194.199.26.158]) by mail-imagis (Postfix) with ESMTP id 23FB240168; Thu, 5 Dec 2002 21:16:23 +0100 (CET) Sender: David.Bourguignon@imag.fr Message-ID: <3DEFB417.60F6A8F6@imag.fr> Date: Thu, 05 Dec 2002 21:16:23 +0100 From: David Bourguignon Organization: iMAGIS X-Mailer: Mozilla 4.78 [en] (X11; U; Linux 2.4.8-34.1mdksmp i686) X-Accept-Language: en MIME-Version: 1.0 To: Holly Rushmeier Cc: globillum@imag.fr Subject: Re: Shockwave/modeling package References: X-Loop: globillum@imag.fr X-Sequence: 148 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: 8-_"!B*f"!3SX!!,L0!! X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Holly Rushmeier wrote: > > -- Does anybody know of really cheap 3D modeling packages (less than $100) > that are > useful for defining basic scenes? > Hi Holly, You can try blender (http://www.blender.org/). It's free software (in all meanings of the words) and it works great. David. -- iMAGIS project, GRAVIR lab INRIA Rhône-Alpes, 655 avenue de l'Europe 38330 Montbonnot Saint Martin, France http://www-imagis.imag.fr/Membres/David.Bourguignon/index.gb.html ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id gB5LFgh05124; Thu, 5 Dec 2002 22:15:43 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id gB5LFVK06882; Thu, 5 Dec 2002 22:15:31 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id gB5LDVK06815 for ; Thu, 5 Dec 2002 22:13:31 +0100 Received: from mail.slb.com (nammta01.sugar-land.nam.slb.com [163.188.150.130]) by imag.imag.fr (8.11.6/8.11.6) with ESMTP id gB5LDL309009; Thu, 5 Dec 2002 22:13:21 +0100 (MET) Received: from conversion-daemon.nammta01.sugar-land.nam.slb.com by nammta01.sugar-land.nam.slb.com (iPlanet Messaging Server 5.2 HotFix 1.06 (built Nov 15 2002)) id <0H6N00K01ZNUJB@nammta01.sugar-land.nam.slb.com>; Thu, 05 Dec 2002 21:01:51 +0000 (GMT) Received: from baja-clear.austin.apc.slb.com (baja-clear.austin.apc.slb.com [163.185.74.6]) by nammta01.sugar-land.nam.slb.com (iPlanet Messaging Server 5.2 HotFix 1.06 (built Nov 15 2002)) with ESMTP id <0H6N00B3PZQZLW@nammta01.sugar-land.nam.slb.com>; Thu, 05 Dec 2002 21:01:47 +0000 (GMT) Received: from slb.com ([163.185.73.61]) by baja-clear.austin.apc.slb.com (8.9.3/8.9.3) with ESMTP id PAA10878; Thu, 05 Dec 2002 15:01:40 -0600 (CST) Date: Thu, 05 Dec 2002 15:01:42 -0600 From: "A. T. Campbell, III" Subject: Re: Shockwave/modeling package To: David Bourguignon Cc: Holly Rushmeier , globillum@imag.fr Message-id: <3DEFBEB6.8020700@slb.com> MIME-version: 1.0 X-Accept-Language: en-us, en User-Agent: Mozilla/5.0 (Windows; U; Windows NT 5.0; en-US; rv:1.0.1) Gecko/20020823 Netscape/7.0 References: <3DEFB417.60F6A8F6@imag.fr> X-Loop: globillum@imag.fr X-Sequence: 150 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: "AE"!&?&!!l)m!!NT0!! X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Holly (and Globillumers), Blender is indeed a good free program, but its user interface is so unusual that you'll probably need to buy its $50 manual to use it effectively. You might also look into Amapi3D from Eovia. The latest version costs a few hundred dollars, but a release from a couple of years ago is available for free download from a game development website: http://amapi.idevgames.com/ Adobe has a new 3D modeling product called Atmosphere that's current being distributed in beta as a free download: http://www.adobe.com/products/atmosphere/ There are several decent free and inexpensive modelers primarily intended for creating scenes for the POV-Ray raytracer. Many of them also export VRML, DXF, and other 3D file formats. From this group, I've tried and liked Breeze Designer and Ayam. Here's a set of links: http://www.povray.org/resources/links/3D_Programs/POV-Ray_Modelling_Programs/ Also, you might try some modelers aimed at the computer game community. A recent and powerful one is gmax from Discreet. It's basically a scaled-down version of 3D Studio Max. To use the editor you'll need to have a copy of a recent game it supports (Microsoft Flight Simulator 2002,Unreal Tournament 2003, etc.). Here's the link: http://www.discreet.com/products/gmax/ I hope this helps! -- A. T. Campbell, III (atcampbell@slb.com) Phone:(512)331-3382 Fax:(512)331-3387 Schlumberger Austin Product Center, 8311 N. FM 620, Austin, TX 78726 =============================== David Bourguignon wrote: > Holly Rushmeier wrote: > >>-- Does anybody know of really cheap 3D modeling packages (less than $100) >>that are >>useful for defining basic scenes? >> > > Hi Holly, > > You can try blender (http://www.blender.org/). > It's free software (in all meanings of the words) and it works great. > > David. ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id gB5Lcih05244; Thu, 5 Dec 2002 22:38:45 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id gB5LcaK08482; Thu, 5 Dec 2002 22:38:36 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id gB5LcTK08463 for ; Thu, 5 Dec 2002 22:38:29 +0100 Received: from pd5mo2so.prod.shaw.ca (shawidc-mo1.cg.shawcable.net [24.71.223.10]) by imag.imag.fr (8.11.6/8.11.6) with ESMTP id gB5LcR310110; Thu, 5 Dec 2002 22:38:28 +0100 (MET) Received: from pd2mr2so.prod.shaw.ca (pd2mr2so-ser.prod.shaw.ca [10.0.141.109]) by l-daemon (iPlanet Messaging Server 5.1 HotFix 0.8 (built May 12 2002)) with ESMTP id <0H6O0089A1CK5L@l-daemon>; Thu, 05 Dec 2002 14:36:20 -0700 (MST) Received: from pn2ml7so.prod.shaw.ca (pn2ml7so-qfe0.prod.shaw.ca [10.0.121.151]) by l-daemon (iPlanet Messaging Server 5.1 HotFix 0.8 (built May 12 2002)) with ESMTP id <0H6O00GQG1CJY5@l-daemon>; Thu, 05 Dec 2002 14:36:19 -0700 (MST) Received: from VANILLA (h24-87-171-127.vn.shawcable.net [24.87.171.127]) by l-daemon (iPlanet Messaging Server 5.1 HotFix 0.8 (built May 12 2002)) with SMTP id <0H6O007YG1CHZL@l-daemon>; Thu, 05 Dec 2002 14:36:19 -0700 (MST) Date: Thu, 05 Dec 2002 13:35:43 -0800 From: Ian Ashdown Subject: Re: Shockwave/modeling package To: "A. T. Campbell, III" , David Bourguignon Cc: Holly Rushmeier , globillum@imag.fr Reply-to: Ian Ashdown Message-id: <018101c29ca6$441c3a40$7fab5718@VANILLA> Organization: byHeart Consultants Limited MIME-version: 1.0 X-MIMEOLE: Produced By Microsoft MimeOLE V6.00.2800.1106 X-Mailer: Microsoft Outlook Express 6.00.2800.1106 X-Priority: 3 X-MSMail-priority: Normal References: <3DEFB417.60F6A8F6@imag.fr> <3DEFBEB6.8020700@slb.com> X-Loop: globillum@imag.fr X-Sequence: 151 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: E_^"!C4S!!@HH"!M6~"! X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Speaking of Blender, I understood from comp.graphics.rendering.raytracing that the company (NAN?) went under several months ago, and that their Web site was taken off-line. Does anyone know the latest news on this? Ian Ashdown, P. Eng., LC, FIES President byHeart Consultants Limited http://www.helios32.com ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id gB5Ljch05312; Thu, 5 Dec 2002 22:45:39 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id gB5LjUC08965; Thu, 5 Dec 2002 22:45:30 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id gB5LjMK08946 for ; Thu, 5 Dec 2002 22:45:22 +0100 Received: from mail-imagis (mail-imagis.inrialpes.fr [194.199.26.22]) by imag.imag.fr (8.11.6/8.11.6) with ESMTP id gB5Lj6310456; Thu, 5 Dec 2002 22:45:06 +0100 (MET) Received: from imag.fr (cormier [194.199.26.158]) by mail-imagis (Postfix) with ESMTP id 4DC4C40168; Thu, 5 Dec 2002 22:45:01 +0100 (CET) Sender: David.Bourguignon@imag.fr Message-ID: <3DEFC8DD.440ADD76@imag.fr> Date: Thu, 05 Dec 2002 22:45:01 +0100 From: David Bourguignon Organization: iMAGIS X-Mailer: Mozilla 4.78 [en] (X11; U; Linux 2.4.8-34.1mdksmp i686) X-Accept-Language: en MIME-Version: 1.0 To: Ian Ashdown Cc: "A. T. Campbell, III" , Holly Rushmeier , globillum@imag.fr Subject: Re: Shockwave/modeling package References: <3DEFB417.60F6A8F6@imag.fr> <3DEFBEB6.8020700@slb.com> <018101c29ca6$441c3a40$7fab5718@VANILLA> X-Loop: globillum@imag.fr X-Sequence: 152 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: 585"!DH@"!46+!!+o@"! X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Ian Ashdown wrote: > > Speaking of Blender, I understood from comp.graphics.rendering.raytracing > that the company (NAN?) went under several months ago, and that their Web > site was taken off-line. Does anyone know the latest news on this? > > Ian Ashdown, P. Eng., LC, FIES > President > byHeart Consultants Limited > http://www.helios32.com Hi Ian, According to the author of one of the posts on the blender site: ""For the first time (as far as i know) in the Internet history, and maybe in the "real world" history too, a community of wideworld based people, only tied by the same "passion", bought a commercial product and decided to make it available gatuitously for all the people in the world (well, at least, for those who have a computer access). Yes, the so called "BLENDER Community", have paid the amount of money (100,000 EURO) that NAN, the proprietary company of the "software" was demanding, and then, released it FREE, under the GPL License."" David. -- iMAGIS project, GRAVIR lab INRIA Rhône-Alpes, 655 avenue de l'Europe 38330 Montbonnot Saint Martin, France http://www-imagis.imag.fr/Membres/David.Bourguignon/index.gb.html ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id h057JEh13871; Sun, 5 Jan 2003 08:19:17 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h057Ipe06750; Sun, 5 Jan 2003 08:18:51 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h057GHK06435 for ; Sun, 5 Jan 2003 08:16:17 +0100 Received: from pd6mo1so.prod.shaw.ca (shawidc-mo1.cg.shawcable.net [24.71.223.10]) by imag.imag.fr (8.11.6/8.11.6) with ESMTP id h057GF723848 for ; Sun, 5 Jan 2003 08:16:16 +0100 (MET) Received: from pd3mr3so.prod.shaw.ca (pd3mr3so-ser.prod.shaw.ca [10.0.141.179]) by l-daemon (iPlanet Messaging Server 5.1 HotFix 0.8 (built May 12 2002)) with ESMTP id <0H88002NMC72N8@l-daemon> for globillum@imag.fr; Sun, 05 Jan 2003 00:16:14 -0700 (MST) Received: from pn2ml6so.prod.shaw.ca (pn2ml6so-qfe0.prod.shaw.ca [10.0.121.150]) by l-daemon (iPlanet Messaging Server 5.1 HotFix 0.8 (built May 12 2002)) with ESMTP id <0H88000DNC7244@l-daemon> for globillum@imag.fr; Sun, 05 Jan 2003 00:16:14 -0700 (MST) Received: from VANILLA (h24-87-171-127.vn.shawcable.net [24.87.171.127]) by l-daemon (iPlanet Messaging Server 5.1 HotFix 0.8 (built May 12 2002)) with SMTP id <0H8800175C70CU@l-daemon> for globillum@imag.fr; Sun, 05 Jan 2003 00:16:14 -0700 (MST) Date: Sat, 04 Jan 2003 23:16:36 -0800 From: Ian Ashdown Subject: ANNOUNCE: January 5th, 2003 release of RADBIB and GITHESIS To: globillum@imag.fr Reply-to: Ian Ashdown Message-id: <007301c2b48a$6218bc70$7fab5718@VANILLA> Organization: byHeart Consultants Limited MIME-version: 1.0 X-MIMEOLE: Produced By Microsoft MimeOLE V6.00.2800.1106 X-Mailer: Microsoft Outlook Express 6.00.2800.1106 Content-type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-priority: Normal X-Loop: globillum@imag.fr X-Sequence: 154 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-UIDL: $I9"!J03"!@c7!![$2!! X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

ANNOUNCE: 03/01/05 Release of RADBIB and GITHESIS
-------------------------------------------------
RADBIB is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. It currently includes 2,185 references -- 24 new additions since its 02/11/23 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of January 5, 2003) from:

http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 282 references to radiosity and global illumination theses -- 9 new additions since the 02/11/23 release.

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

Ian Ashdown, P. Eng., LC, FIES
President
byHeart Consultants Limited
http://www.helios32.com

 

From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id h0GGRkh06892; Thu, 16 Jan 2003 17:27:48 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h0GGOki12427; Thu, 16 Jan 2003 17:24:46 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h0GGNo512353 for ; Thu, 16 Jan 2003 17:23:50 +0100 Received: from nut.autodesk.com (nut.autodesk.com [198.102.112.27]) by imag.imag.fr (8.11.6/8.11.6) with ESMTP id h0GGNnp17117 for ; Thu, 16 Jan 2003 17:23:49 +0100 (MET) Received: from hqmsgsrf00.autodesk.com (hqmsgsrf00.autodesk.com [144.111.32.210]) by nut.autodesk.com (8.12.6/8.12.5) with ESMTP id h0GGNax0004919; Thu, 16 Jan 2003 08:23:36 -0800 (PST) Received: by hqmsgsrf00.autodesk.com with Internet Mail Service (5.5.2653.19) id ; Thu, 16 Jan 2003 08:23:36 -0800 Message-ID: From: eric.haines@autodesk.com To: globillum@imag.fr Subject: Less than a week left! Date: Thu, 16 Jan 2003 08:23:32 -0800 MIME-Version: 1.0 X-Mailer: Internet Mail Service (5.5.2653.19) Content-Type: text/html; charset=windows-1252 X-Loop: globillum@imag.fr X-Sequence: 156 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-UIDL: i8G!!<[""!Ao@!!E>2"! X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

Yes, it's less than a week left until that all-important date, the Fantasy Graphics League entry deadline: http://www.realtimerendering.com/fgl/

 

After you meet this deadline, you can then finish your SIGGRAPH paper submissions.

 

Enjoy,

 

Eric

From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id h0LEUTh17164; Tue, 21 Jan 2003 15:30:32 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h0LEU4T15789; Tue, 21 Jan 2003 15:30:04 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h0LETI515714 for ; Tue, 21 Jan 2003 15:29:18 +0100 Received: from nut.autodesk.com (nut.autodesk.com [198.102.112.27]) by imag.imag.fr (8.11.6/8.11.6) with ESMTP id h0LETHX12008 for ; Tue, 21 Jan 2003 15:29:17 +0100 (MET) Received: from hqmsgsrf00.autodesk.com (hqmsgsrf00.autodesk.com [144.111.32.210]) by nut.autodesk.com (8.12.6/8.12.5) with ESMTP id h0LESLx0029071 for ; Tue, 21 Jan 2003 06:29:11 -0800 (PST) Received: by hqmsgsrf00.autodesk.com with Internet Mail Service (5.5.2653.19) id ; Tue, 21 Jan 2003 06:28:21 -0800 Message-ID: From: eric.haines@autodesk.com To: globillum@imag.fr Subject: Ugh, foo, and bah Date: Tue, 21 Jan 2003 06:28:14 -0800 MIME-Version: 1.0 X-Mailer: Internet Mail Service (5.5.2653.19) Content-Type: text/html; charset=windows-1252 X-Loop: globillum@imag.fr X-Sequence: 157 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-UIDL: S@

If you've been waiting until the last minute to submit your Fantasy Graphics League team, http://www.realtimerendering.com/fgl, please keep waiting. It turns out that somebody diddled with server permissions and whatnot, and my CGI script is no longer working (and hasn't been since about Dec. 12th!). Anyway, I'll let you know when it's working again, and I'll extend the deadline; just thought I'd warn you now to not waste the time now (waste it later).

 

I do have a question for you all, as I've been exchanging correspondence on this topic: when was the first use of computing ray intersections and paths for optics? Also, when was the first use of the idea of rays as a way of determining shadows? If you've run across anything interesting on these two subjects, please pass them on, as I'd like to collect them all for the Ray Tracing News.

 

Eric

From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id h0LKLvh21103; Tue, 21 Jan 2003 21:21:58 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h0LKLcs03491; Tue, 21 Jan 2003 21:21:38 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h0LKLK503457 for ; Tue, 21 Jan 2003 21:21:20 +0100 Received: from nut.autodesk.com (nut.autodesk.com [198.102.112.27]) by imag.imag.fr (8.11.6/8.11.6) with ESMTP id h0LKLJO23346 for ; Tue, 21 Jan 2003 21:21:19 +0100 (MET) Received: from hqmsgsrf00.autodesk.com (hqmsgsrf00.autodesk.com [144.111.32.210]) by nut.autodesk.com (8.12.6/8.12.5) with ESMTP id h0LKL7x0013179 for ; Tue, 21 Jan 2003 12:21:12 -0800 (PST) Received: by hqmsgsrf00.autodesk.com with Internet Mail Service (5.5.2653.19) id ; Tue, 21 Jan 2003 12:21:06 -0800 Message-ID: From: eric.haines@autodesk.com To: globillum@imag.fr Subject: RE: Ugh, foo, and bah Date: Tue, 21 Jan 2003 12:21:03 -0800 MIME-Version: 1.0 X-Mailer: Internet Mail Service (5.5.2653.19) Content-Type: text/html; charset=windows-1252 X-Loop: globillum@imag.fr X-Sequence: 158 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-UIDL: c&W!!V`6!!<-d!!l/2!! X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

Given that two people have responded "Appel?" in the past few hours, I guess I should explain further. I agree that Appel was, to my knowledge, the first to use computers to trace rays, at least in the field of computer graphics research (I can imagine other fields using computers to compute occlusion for non-graphical reasons earlier than Appel). I was more interested in earlier uses of rays and their computation (not on computers) to evaluate lens designs, for creating silhouettes, etc. I've seen a figure from DaVinci's workshop showing the use of rays in how a silhouette is formed, for example. If anyone had any facts they'd run across in their travels about the use of rays throughout history, I'd like to know. I'm just compiling a light article for the Ray Tracing News, nothing deep; I find the historical roots interesting. Also, maybe people in other disciplines like Optics won't laugh at us so much, since we then won't say things like, "computer graphics people invented the idea of tracing rays to create shadows and through refractive objects."

 

Eric

From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id h0MK2nh05727; Wed, 22 Jan 2003 21:02:50 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h0MK2aa15146; Wed, 22 Jan 2003 21:02:36 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h0MK2Q515126 for ; Wed, 22 Jan 2003 21:02:26 +0100 Received: from nut.autodesk.com (nut.autodesk.com [198.102.112.27]) by imag.imag.fr (8.12.7/8.12.7) with ESMTP id h0MK2P8H019493 for ; Wed, 22 Jan 2003 21:02:26 +0100 (CET) Received: from hqmsgsrf00.autodesk.com (hqmsgsrf00.autodesk.com [144.111.32.210]) by nut.autodesk.com (8.12.6/8.12.5) with ESMTP id h0MK1Px0013621 for ; Wed, 22 Jan 2003 12:02:14 -0800 (PST) Received: by hqmsgsrf00.autodesk.com with Internet Mail Service (5.5.2653.19) id ; Wed, 22 Jan 2003 12:01:24 -0800 Message-ID: From: eric.haines@autodesk.com To: globillum@imag.fr Subject: This time for sure... Date: Wed, 22 Jan 2003 12:01:20 -0800 MIME-Version: 1.0 X-Mailer: Internet Mail Service (5.5.2653.19) Content-Type: text/html; charset=windows-1252 X-Loop: globillum@imag.fr X-Sequence: 159 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-UIDL: I5("!(8a!!oS?"!Mkm"! X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

The Fantasy Graphics League site is now working for real: http://www.realtimerendering.com/fgl. The deadline's been extended to February 2nd, since the program's been flaked out for awhile.

 

Eric

From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id h0NAOmh15645; Thu, 23 Jan 2003 11:24:49 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h0NAOE429749; Thu, 23 Jan 2003 11:24:14 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h0NAO8529729 for ; Thu, 23 Jan 2003 11:24:08 +0100 Received: from relay2.mail.uk.psi.net (relay2.mail.uk.psi.net [154.32.107.6]) by imag.imag.fr (8.12.7/8.12.7) with ESMTP id h0NAO78H016307 for ; Thu, 23 Jan 2003 11:24:08 +0100 (CET) Received: from lightwork.co.uk ([195.152.206.2] helo=elvis.lightwork) by relay2.mail.uk.psi.net with esmtp (Exim 2.12 #2) id 18beWl-0006Ad-00 for globillum@imag.fr; Thu, 23 Jan 2003 10:24:07 +0000 Received: by elvis.lightwork with Internet Mail Service (5.5.2650.21) id ; Thu, 23 Jan 2003 10:24:06 -0000 Message-ID: <8815647C7041D111A3010060B06BE1C001DA0237@elvis.lightwork> From: Neil Gatenby To: globillum@imag.fr Subject: HDR image format Date: Thu, 23 Jan 2003 10:24:05 -0000 MIME-Version: 1.0 X-Mailer: Internet Mail Service (5.5.2650.21) X-Loop: globillum@imag.fr X-Sequence: 160 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: lT,"!E8I"!]'j!!R='"! X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hi The following will be of interest to some here: http://www.openexr.com/ "OpenEXR is a high dynamic-range (HDR) image file format developed by Industrial Light & Magic for use in computer imaging applications. ILM has released OpenEXR as free software." Would someone on this group, who knows more about HDR than me, care to comment on the differences between this format and the Debevec format (http://www.debevec.org/HDRShop/) ??? If I wanted to illuminate 3D scenes with HDR images, which format do I go for? Best wishes Neil ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id h0NCubh17416; Thu, 23 Jan 2003 13:56:38 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h0NCuQh06622; Thu, 23 Jan 2003 13:56:26 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h0NCt5506338 for ; Thu, 23 Jan 2003 13:55:05 +0100 Received: from cmailm2.svr.pol.co.uk (cmailm2.svr.pol.co.uk [195.92.193.210]) by imag.imag.fr (8.12.7/8.12.7) with ESMTP id h0NCt48H024950 for ; Thu, 23 Jan 2003 13:55:05 +0100 (CET) Received: from user-2012.bbd11tcl.dsl.pol.co.uk ([81.77.151.220] helo=simon) by cmailm2.svr.pol.co.uk with smtp (Exim 3.35 #1) id 18bgsp-0001vK-00; Thu, 23 Jan 2003 12:55:03 +0000 Message-ID: <005601c2c2df$2b55bd10$0101a8c0@simon> From: "Simon Bunker" To: "Neil Gatenby" , globillum@imag.fr References: <8815647C7041D111A3010060B06BE1C001DA0237@elvis.lightwork> Subject: Re: HDR image format Date: Thu, 23 Jan 2003 12:58:47 -0000 MIME-Version: 1.0 X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 6.00.2800.1106 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1106 X-Loop: globillum@imag.fr X-Sequence: 161 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: g'6"!Cg$"!0\7!!?\\"! X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit >>From a really quick look they look very similar. Except ILM's one has more dynamic range information as it uses 16 bits per channel instead of the 8 (I think) the .hdr/.pic format uses (which Greg Ward-Larson created for Radiance). Both use a mantissa for basic colour information, and an exponent - just OpenEXR has more of them! .pic uses 8bits /colour channel to save space. The fourth channel is the common exponent instead of an alpha. OpenEXR can have different exponents for each channel, plus you can mix data types between channels. Radiance file format information can be found here http://radsite.lbl.gov/radiance/framer.html .pic has the advantage that it is already supported in several applications - eg. HDRshop, Radiance and Lightwave. OpenEXR has the advantage it comes from ILM and has a cool geek factor ;o) I just hope we see some more projects emerge from ILM as Open source - this is a nice start. And the second part of your question - if you want to store radiance maps in a high dynamic range format and use it in commercial software anytime soon then you'll have to use .pic. You could use OpenEXR if you a) write your own renderer b) are very good friends with someone who writes a renderer or c) are willing to wait for the tools to catch up (OpenEXR was only released yesturday!) Simon http://www.rendermania.com/ > > Hi > > The following will be of interest to some here: > > http://www.openexr.com/ > > "OpenEXR is a high dynamic-range (HDR) image file format developed by > Industrial Light & Magic for use in computer imaging applications. > ILM has released OpenEXR as free software." > > Would someone on this group, who knows more about HDR than me, care to > comment on the differences between this format and the Debevec format > (http://www.debevec.org/HDRShop/) ??? > > If I wanted to illuminate 3D scenes with HDR images, which format do I go > for? > > Best wishes > > Neil > ---------------------------------------------------------------------------- ---- > ------------------------------------------------------------------------- > globillum@imag.fr -- mailing list devoted to global illumination research > For list archives or to configure your options, see http://listes.imag.fr > ------------------------------------------------------------------------- ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id h0NGMeh19741; Thu, 23 Jan 2003 17:22:41 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h0NGMA318318; Thu, 23 Jan 2003 17:22:10 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h0NGM4518298 for ; Thu, 23 Jan 2003 17:22:04 +0100 Received: from bach.graphics.cornell.edu (bach.graphics.cornell.edu [128.84.247.50]) by imag.imag.fr (8.12.7/8.12.7) with ESMTP id h0NGM27S009122 for ; Thu, 23 Jan 2003 17:22:03 +0100 (CET) Received: from diesel.graphics.cornell.edu (diesel.graphics.cornell.edu [128.84.247.211]) by bach.graphics.cornell.edu (8.12.1/8.12.1) with ESMTP id h0NGLtqT008528 for ; Thu, 23 Jan 2003 11:21:56 -0500 (EST) Date: Thu, 23 Jan 2003 11:21:55 -0500 (EST) Message-Id: <200301231621.h0NGLtqT008528@bach.graphics.cornell.edu> From: "Stephen H. Westin" To: globillum@imag.fr In-reply-to: <8815647C7041D111A3010060B06BE1C001DA0237@elvis.lightwork> (message from Neil Gatenby on Thu, 23 Jan 2003 10:24:05 -0000) Subject: Re: HDR image format Reply-to: westin@graphics.cornell.edu References: <8815647C7041D111A3010060B06BE1C001DA0237@elvis.lightwork> X-Loop: globillum@imag.fr X-Sequence: 162 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: %K8"!mJ[!!: From: Neil Gatenby > Date: Thu, 23 Jan 2003 10:24:05 -0000 > > > Hi > > The following will be of interest to some here: > > http://www.openexr.com/ > > "OpenEXR is a high dynamic-range (HDR) image file format developed by > Industrial Light & Magic for use in computer imaging applications. > ILM has released OpenEXR as free software." > > Would someone on this group, who knows more about HDR than me, care to > comment on the differences between this format and the Debevec format > (http://www.debevec.org/HDRShop/) ??? You mean, of course, the Ward/Larson format that Greg Ward (and sometimes Larson) created for Radiance. There's code on our Web site to read and write it. > If I wanted to illuminate 3D scenes with HDR images, which format do I go > for? First choice for compatibility: RADIANCE .pic/.hdr/.rgbe format. For more precision, TIFF either in floating-point format (compatible in the RenderMan world as texture map input, I think) or in LOGLUV format which Greg invented as a more universal sequel to pic/hdr/rgbe. Both are supported by libtiff (the Sam Leffler publicly-available library), but not by Photoshop. -Stephen H. Westin Any information or opinions in this message are mine: they do not represent the position of Cornell University or any of its sponsors. ------------=_1043338926-9207-2 Content-Type: text/plain; name="message.footer" Content-Disposition: inline; filename="message.footer" Content-Transfer-Encoding: 8bit ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- ------------=_1043338926-9207-2-- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id h0NGroh20101; Thu, 23 Jan 2003 17:53:50 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h0NGraT20150; Thu, 23 Jan 2003 17:53:36 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h0NGrO520130 for ; Thu, 23 Jan 2003 17:53:24 +0100 Received: from pimout2-ext.prodigy.net (pimout2-ext.prodigy.net [207.115.63.101]) by imag.imag.fr (8.12.7/8.12.7) with ESMTP id h0NGrM7S011265 for ; Thu, 23 Jan 2003 17:53:23 +0100 (CET) Received: from lmi.net (adsl-64-163-213-187.dsl.snfc21.pacbell.net [64.163.213.187]) by pimout2-ext.prodigy.net (8.12.3 da nor stuldap/8.12.3) with ESMTP id h0NGr6wU340590; Thu, 23 Jan 2003 11:53:12 -0500 Date: Thu, 23 Jan 2003 08:52:15 -0800 Subject: Re: HDR image format Content-Type: text/plain; charset=windows-1252; format=flowed Mime-Version: 1.0 Cc: "Neil Gatenby" , globillum@imag.fr To: "Simon Bunker" From: Greg Ward In-Reply-To: <005601c2c2df$2b55bd10$0101a8c0@simon> Message-Id: <06D7F276-2EF3-11D7-9A22-00306540F848@lmi.net> X-Mailer: Apple Mail (2.551) X-Loop: globillum@imag.fr X-Sequence: 163 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-UIDL: jpF!!Vi3!!I0=!!5hR"! X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit I just wanted to add my two cents to this discussion, provided I haven't been deleted from the globillum list again... I have been working with Drew Hess of ILM to get OpenEXR to compile under Mac OS X, and I have the following comments. The 16-bit/primary EXR "half" float format uses what's called an "s-e5-10" bit arrangement, for "sign plus 5 exponent plus 10 mantissa." This arrangement allows for correct sorting by bit pattern, and is the same format designed at SGI for their never-happened-generation of high-end graphics, which eventually became NVidia's cg system. It covers values of 6e-5 to 6.5e4, positive and negative, where the bottom part of the range "denormalized" to a linear form. This follows IEEE float conventions very closely, including a zero bit pattern that corresponds to 0.0 and representations for infinity and NaN, I believe. Heck, let me just make a table showing the different representations I know. Regrettably, the text of this table is unreadable because I put in too many columns, so I'm attaching a PDF version. (How annoying.) The summary though is that OpenEXR compares favorably with Radiance format, offering 9 orders of magnitude in dynamic range at much better precision (0.1% rather than the 0.8% of Radiance). The down side is that it takes up slightly more space, and the i/o library is C++ and a LOT more complicated. (It's quite nice, though.) If what you care about is color accuracy, the LogLuv TIFF format is what I recommend. It uses a perceptual color space to get the most relevant information into the fewest bits. There's a 24-bit and a 32-bit/pixel format to choose from (plus a 16-bit/pixel luminance variant). A lot of programmers balk at the CIE XYZ color interface, but it's the best way to be sure of the color you're getting. Most of the other formats just assume you know, without making the color space explicit. Radiance supports an additional tag (as does floating-point TIFF) saying what the primaries are, but since Radiance doesn't allow for negative primary values, your gamut is restricted to the colors within this space. (Not so for EXR or floating-point TIFF.) Also, LogLuv TIFF is supported for reading by such common viewers as ACDSee, because it was incorporated into Sam Leffler's library to convert automatically to 8-bit RGBA. The main advantage I find, though, is that the separation of luminance and chrominance channels allows for very fast global tone-mapping using look-ups. I can load and tone-map a LogLuv TIFF in less time than it takes to decompress a JPEG of the same size! Speaking of which, anyone who wants to play around with HDR images on the Mac should pick up and try out the Photosphere application I've been working on. It's available from the URL below for a limited time only to beta testers, and catalogs regular TIFFs and JPEGs as well as the various HDRI formats. It also has facilities for building HDRI's from multiple, hand-held exposures. It's the only program that can as far as I know. I also have a command-line tool that works on Linux and under Windows, but I need to recompile it for those platforms. -Greg Photosphere at: http://viz.cs.berkeley.edu/gwlarson/pickup/ Attachment Converted: "D:\meine Daten\eudora\Attach ab 2002.09.17\HDRformats.pdf" ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id h0OIVth03391; Fri, 24 Jan 2003 19:31:56 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h0OIVgs13538; Fri, 24 Jan 2003 19:31:42 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h0OIVY513518 for ; Fri, 24 Jan 2003 19:31:34 +0100 Received: from pimout2-ext.prodigy.net (pimout2-ext.prodigy.net [207.115.63.101]) by imag.imag.fr (8.12.7/8.12.7) with ESMTP id h0OIVW7S012549 for ; Fri, 24 Jan 2003 19:31:33 +0100 (CET) Received: from lmi.net (adsl-64-163-212-245.dsl.snfc21.pacbell.net [64.163.212.245]) by pimout2-ext.prodigy.net (8.12.3 da nor stuldap/8.12.3) with ESMTP id h0OIVUwU241388; Fri, 24 Jan 2003 13:31:30 -0500 Date: Fri, 24 Jan 2003 10:30:37 -0800 Subject: Re: HDR image format Mime-Version: 1.0 Cc: globillum@imag.fr To: "Bretton Wade" From: Greg Ward In-Reply-To: <54972B5E70821540A22B9CFBDA062FE5A70BE8@RED-MSG-02.redmond.corp.microsoft.com> Message-Id: X-Mailer: Apple Mail (2.551) X-Loop: globillum@imag.fr X-Sequence: 164 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: U3[!!Dj_!!\"T!!!,!"! X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit > From: "Bretton Wade" > Date: Thu Jan 23, 2003 10:57:08 AM US/Pacific > To: "Greg Ward" > Subject: RE: HDR image format > > Hi Greg, > > Thanks for your very precise commentary here, it's very helpful. Could > you also speak to how you see these file formats playing into next > generation graphics hardware from nVidia and ATI, and their support for > floating point buffers? > > Regards, > Bretton > -- > Bretton Wade (aka Noz Moe King) in Bellevue, WA Well, I'm not much of a graphics hardware expert, but the fact that the OpenEXR "half" data type matches that used by nVidia in their new card has to be a plus. (I don't know anything about ATI's format, but I can't imagine it's too different.) Taking an EXR image, you should be able to go straight into a texture map on these cards. Both cards will have the problem of mapping their output to a display, since you presumably put your hardware between your software and your display, not between your software and more software. The study of how to map high dynamic-range imagery to low dynamic-range displays has garnered a lot of attention, recently. There were three papers in last year's Siggraph, and one at the Eurographics Workshop on Rendering. -Greg ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id h15Lsuh18235; Wed, 5 Feb 2003 22:54:57 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h15Lsc123412; Wed, 5 Feb 2003 22:54:38 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h15LsV523395 for ; Wed, 5 Feb 2003 22:54:31 +0100 Received: from e1.ny.us.ibm.com (e1.ny.us.ibm.com [32.97.182.101]) by imag.imag.fr (8.12.7/8.12.7) with ESMTP id h15LsUJt011971 (version=TLSv1/SSLv3 cipher=EDH-RSA-DES-CBC3-SHA bits=168 verify=FAIL) for ; Wed, 5 Feb 2003 22:54:31 +0100 (CET) Received: from northrelay02.pok.ibm.com (northrelay02.pok.ibm.com [9.56.224.150]) by e1.ny.us.ibm.com (8.12.2/8.12.2) with ESMTP id h15LsNs5067558 for ; Wed, 5 Feb 2003 16:54:24 -0500 Received: from d01ml244.pok.ibm.com (d01av02.pok.ibm.com [9.56.224.216]) by northrelay02.pok.ibm.com (8.12.3/NCO/VER6.5) with ESMTP id h15LsKaW049028 for ; Wed, 5 Feb 2003 16:54:21 -0500 Importance: Normal Subject: Volunteer needed To: globillum@imag.fr X-Mailer: Lotus Notes Release 5.0.7 March 21, 2001 Message-ID: From: Holly Rushmeier Date: Wed, 5 Feb 2003 16:54:20 -0500 X-MIMETrack: Serialize by Router on D01ML244/01/M/IBM(Build V601_01232003|January 23, 2003) at 02/05/2003 16:54:21 MIME-Version: 1.0 X-Loop: globillum@imag.fr X-Sequence: 166 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: (Y]"!o35"!pL:"!,\E!! X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Computing Reviews, the 40-year-old review publication of the ACM, is seeking a volunteer area expert in Computer Graphics (encompassing algorithms, computational geometry, modeling, methodology) who can serve on its Editorial Board. The qualified candidate will be prepared to check written reviews for quality and the classification terms from ACM's Computing Classification System (CCS) for accuracy, as well as use a Web-based editing system to make any suggested changes to the CCS terms or to the review itself. This is an opportunity for an enthusiast about the discipline to stay on the cutting edge of the field, while making a significant contribution to the computing community along with 16 other area editors. Please contact Carol Hutchins, Editor-in-Chief of Computing Reviews, at carol.hutchins@nyu.edu __________________________ Holly Rushmeier ,hertjwr@us.ibm.com, http://www.research.ibm.com/people/h/holly (914)784-7252 IBM TJ Watson Research Center, 19 Skyline Drive, Hawthorne, NY 10532, USA ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id h17HBfh14263; Fri, 7 Feb 2003 18:11:41 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h17H7wT09911; Fri, 7 Feb 2003 18:07:58 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h17H7q509894 for ; Fri, 7 Feb 2003 18:07:52 +0100 Received: from mail.itc.utm.my (dns.itc.utm.my [161.139.194.149]) by imag.imag.fr (8.12.7/8.12.7) with ESMTP id h17H7mYH026078 for ; Fri, 7 Feb 2003 18:07:51 +0100 (CET) Received: from starfire.itc.utm.my ([161.139.194.150]) by itc.utm.my ([161.139.194.146]) with SMTP (MDaemon.PRO.v6.5.2.R) for ; Sat, 08 Feb 2003 01:04:43 +0800 Message-Id: <5.1.0.14.2.20030208005821.00b1bc10@mail.itc.utm.my> X-Sender: aukauk@mail.itc.utm.my X-Mailer: QUALCOMM Windows Eudora Version 5.1 Date: Sat, 08 Feb 2003 01:07:38 +0800 To: globillum@imag.fr From: Sarudin Kari Subject: Synthetic Scene Simulation Mime-Version: 1.0 X-MDRemoteIP: 161.139.194.150 X-Return-Path: aukauk@itc.utm.my X-MDaemon-Deliver-To: globillum@imag.fr X-Loop: globillum@imag.fr X-Sequence: 167 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: A=+"!Y6J"!W:#"!:=%"! X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hi, I am doing synthetic scene simulation for remote sensing image chain process (scene capture, atmospheric transfer, sensor models etc). Any pointers (papers, books, codes etc) ? I have studied only Vermote (6S) and Salvaggio Phd Thesis (DIRSIG). Thank you very much. Sarudin Kari FSKSM-UTM ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id h17HYMh14495; Fri, 7 Feb 2003 18:34:23 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h17HXr811366; Fri, 7 Feb 2003 18:33:53 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h17HXg511349 for ; Fri, 7 Feb 2003 18:33:42 +0100 Received: from e1.ny.us.ibm.com (e1.ny.us.ibm.com [32.97.182.101]) by imag.imag.fr (8.12.7/8.12.7) with ESMTP id h17HXeYI027414 (version=TLSv1/SSLv3 cipher=EDH-RSA-DES-CBC3-SHA bits=168 verify=FAIL) for ; Fri, 7 Feb 2003 18:33:42 +0100 (CET) Received: from northrelay02.pok.ibm.com (northrelay02.pok.ibm.com [9.56.224.150]) by e1.ny.us.ibm.com (8.12.7/8.12.2) with ESMTP id h17HXYEs011130; Fri, 7 Feb 2003 12:33:34 -0500 Received: from d01ml244.pok.ibm.com (d01av02.pok.ibm.com [9.56.224.216]) by northrelay02.pok.ibm.com (8.12.3/NCO/VER6.5) with ESMTP id h17HXVxo035596; Fri, 7 Feb 2003 12:33:31 -0500 Importance: Normal Subject: Re: Synthetic Scene Simulation To: Sarudin Kari Cc: globillum@imag.fr X-Mailer: Lotus Notes Release 5.0.7 March 21, 2001 Message-ID: From: Holly Rushmeier Date: Fri, 7 Feb 2003 12:33:31 -0500 X-MIMETrack: Serialize by Router on D01ML244/01/M/IBM(Build V601_02022003|February 02, 2003) at 02/07/2003 12:33:32 MIME-Version: 1.0 X-Loop: globillum@imag.fr X-Sequence: 168 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: R`/!!]h9!!jFU"!U~@"! X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit For a lot of remote sensing related work check Chris Borel's page at LANL: http://nis-www.lanl.gov/~borel/ As far as atmospheric transfer, check Shree Nayar's work: http://www.cs.columbia.edu/CAVE/research/publications/vision_weather.html __________________________ Holly Rushmeier ,hertjwr@us.ibm.com, http://www.research.ibm.com/people/h/holly (914)784-7252 IBM TJ Watson Research Center, 19 Skyline Drive, Hawthorne, NY 10532, USA Sarudin Kari on 02/07/2003 12:07:38 PM To: globillum@imag.fr cc: Subject: Synthetic Scene Simulation Hi, I am doing synthetic scene simulation for remote sensing image chain process (scene capture, atmospheric transfer, sensor models etc). Any pointers (papers, books, codes etc) ? I have studied only Vermote (6S) and Salvaggio Phd Thesis (DIRSIG). Thank you very much. Sarudin Kari FSKSM-UTM ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id h17HnBh14638; Fri, 7 Feb 2003 18:49:12 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h17Hjig12065; Fri, 7 Feb 2003 18:45:44 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h17HiN511989 for ; Fri, 7 Feb 2003 18:44:23 +0100 Received: from pd6mo2so.prod.shaw.ca (shawidc-mo1.cg.shawcable.net [24.71.223.10]) by imag.imag.fr (8.12.7/8.12.7) with ESMTP id h17HiLG3027956 for ; Fri, 7 Feb 2003 18:44:23 +0100 (CET) Received: from pd3mr3so.prod.shaw.ca (pd3mr3so-ser.prod.shaw.ca [10.0.141.179]) by l-daemon (iPlanet Messaging Server 5.1 HotFix 0.8 (built May 12 2002)) with ESMTP id <0H9Y00FCV99W6J@l-daemon> for globillum@imag.fr; Fri, 07 Feb 2003 10:44:20 -0700 (MST) Received: from pn2ml9so.prod.shaw.ca (pn2ml9so-qfe0.prod.shaw.ca [10.0.121.7]) by l-daemon (iPlanet Messaging Server 5.1 HotFix 0.8 (built May 12 2002)) with ESMTP id <0H9Y00HEP99WD8@l-daemon> for globillum@imag.fr; Fri, 07 Feb 2003 10:44:20 -0700 (MST) Received: from VANILLA (h24-87-171-230.vn.shawcable.net [24.87.171.230]) by l-daemon (iPlanet Messaging Server 5.1 HotFix 0.8 (built May 12 2002)) with SMTP id <0H9Y00DE999VC1@l-daemon> for globillum@imag.fr; Fri, 07 Feb 2003 10:44:20 -0700 (MST) Date: Fri, 07 Feb 2003 09:45:48 -0800 From: Ian Ashdown Subject: Re: Synthetic Scene Simulation To: globillum@imag.fr, Sarudin Kari Reply-to: Ian Ashdown Message-id: <00dd01c2ced0$c021b870$6401a8c0@VANILLA> Organization: byHeart Consultants Limited MIME-version: 1.0 X-MIMEOLE: Produced By Microsoft MimeOLE V6.00.2800.1106 X-Mailer: Microsoft Outlook Express 6.00.2800.1106 X-Priority: 3 X-MSMail-priority: Normal References: <5.1.0.14.2.20030208005821.00b1bc10@mail.itc.utm.my> X-Loop: globillum@imag.fr X-Sequence: 169 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: a;;"![3_!!^#B!!!\B!! X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit The RADBIB and GITHESIS global illumination bibliographies (in the Resources section of www.helios32.com) include over 2,100 references that may be of interest to you. (They do not however delve too deeply into the atmospheric attenuation literature.) Ian Ashdown, P. Eng., LC, FIES President byHeart Consultants Limited http://www.helios32.com ----- Original Message ----- From: "Sarudin Kari" To: Sent: Friday, February 07, 2003 9:07 AM Subject: Synthetic Scene Simulation > Hi, > > I am doing synthetic scene simulation for remote sensing image chain > process (scene capture, atmospheric transfer, sensor models etc). Any > pointers (papers, books, codes etc) ? I have studied only Vermote (6S) and > Salvaggio Phd Thesis (DIRSIG). > > Thank you very much. > > Sarudin Kari > FSKSM-UTM > > ---------------------------------------------------------------------------- ---- > ------------------------------------------------------------------------- > globillum@imag.fr -- mailing list devoted to global illumination research > For list archives or to configure your options, see http://listes.imag.fr > ------------------------------------------------------------------------- ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id h1G3tVh06409; Sun, 16 Feb 2003 04:55:33 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h1G3pqE12661; Sun, 16 Feb 2003 04:51:52 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h1G3oQ512362 for ; Sun, 16 Feb 2003 04:50:26 +0100 Received: from MAIL03.toast.net (mail.toast.net [206.244.185.10]) by imag.imag.fr (8.12.7/8.12.7) with ESMTP id h1G3oP52023389 for ; Sun, 16 Feb 2003 04:50:26 +0100 (CET) Received: from delldaextn (unverified [64.24.69.155]) by MAIL03.toast.net (Vircom SMTPRS 1.4.232) with ESMTP id for ; Sat, 15 Feb 2003 22:45:23 -0500 From: "A Gallardo" To: globillum@imag.fr Subject: standardized GI/rad test scenes? Date: Sat, 15 Feb 2003 22:51:40 -0500 Message-ID: <000a01c2d56e$b68d2f20$9b451840@delldaextn> MIME-Version: 1.0 Content-Type: text/html; charset=windows-1252 X-Priority: 3 (Normal) X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook 8.5, Build 4.71.2173.0 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1106 Importance: Normal In-Reply-To: X-Loop: globillum@imag.fr X-Sequence: 172 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-UIDL: e%X"!4,c"!RhP"!bb7!! X-Mozilla-Status: 9001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit
Hi all,
 
    This is my second or third post on this forum but have been a member for sometime.
 
    I am going to be doing an exhaustive evaluation of mostly commercial render engines used for architectural visualization for an web article (cgarchitect.com). I am going to be doing this on my own accord so there is no bias involved however I am interested in knowing if there are standardized scenes being used other than the classic occluder scenes (chair,flat occluders etc),Cornell boxes as well as the standard ones done by Brian Smits and Henrik Wann Jensen paper.  I do intend to use most comonly used scenes such as bathrooms, fireplaces, conference rooms and other challenging scens that will expose light transfer issues such as having curve surfaces with interesting material properties.  I also would be testing for 'specular to diffuse transfers' as well as caustics if possible as well as photometric issues (mainly near field photometry issues) if the renderer can handle it. I would also be doing clean room scenes with windows with patterns and shapes (discontinuity tests) to test for shadow boundary issues and area light tests shiing on subjects that are near and far with curve and planar surfaces.  'Daylight' and night processing will also be involved for both interior and exterior scenes as much as possible.
 
    Are there more tests I should be considering? IS there a standard test scene I should test?   I do intend to evaluate the renderers based on aesthetics, speed, accuracy,fidelity and workflow issues such as polygon load handling and material properties flexibility. 
 
    I know that there are no identical test scenes but I am interested in knowing if there are common approaches done and which are those as well as any potential pitfalls for a project such as this.  BTW if you are interested here are some old test scenes I used for progressive radiosity (lightscape) tests:
 
 
 
 
 
 
 
 
    I intend to use some of these but mostly updated scenes with optimized quadrilateral surfaces only with minimal triangulation. Thank you.
 
Sincerely,
 
Arnold Gallardo
Visual Content Creator
Technical Writer/Author
 
 
 
 
From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id h1G5gBh06925; Sun, 16 Feb 2003 06:42:12 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h1G4cqQ15194; Sun, 16 Feb 2003 05:38:52 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h1G4cj515176 for ; Sun, 16 Feb 2003 05:38:45 +0100 Received: from wrath.cs.utah.edu (wrath.cs.utah.edu [155.99.198.100]) by imag.imag.fr (8.12.7/8.12.7) with ESMTP id h1G4ci52024036 for ; Sun, 16 Feb 2003 05:38:44 +0100 (CET) Received: from eiger.cs.utah.edu (eiger.cs.utah.edu [155.99.195.28]) by wrath.cs.utah.edu (8.11.6/8.11.6) with ESMTP id h1G4caD05842; Sat, 15 Feb 2003 21:38:37 -0700 (MST) Received: from premoze (helo=localhost) by eiger.cs.utah.edu with local-esmtp (Exim 3.35 #1 (Debian)) id 18kGZY-00062e-00; Sat, 15 Feb 2003 21:38:36 -0700 Date: Sat, 15 Feb 2003 21:38:36 -0700 (MST) From: Simon PREMOZE To: A Gallardo cc: globillum@imag.fr Subject: Re: standardized GI/rad test scenes? In-Reply-To: <000a01c2d56e$b68d2f20$9b451840@delldaextn> Message-ID: MIME-Version: 1.0 X-Loop: globillum@imag.fr X-Sequence: 173 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: Gml"!AO_"!8K8"!if=!! X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hi, There have been some attempts to standardize test scenes for global illumination. Brian Smits and Henrik Wann Jensen describe GI test scenes and provide geometry for tests: http://www.cs.utah.edu/~bes/papers/scenes/ Simon Premoze ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id h1GImBh11361; Sun, 16 Feb 2003 19:48:12 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h1GIioi26638; Sun, 16 Feb 2003 19:44:50 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h1GIhL526601 for ; Sun, 16 Feb 2003 19:43:21 +0100 Received: from ls405.hinet.hr (ls405.hinet.hr [195.29.150.97]) by imag.imag.fr (8.12.7/8.12.7) with ESMTP id h1GIhK52007671 for ; Sun, 16 Feb 2003 19:43:20 +0100 (CET) Received: from ls401.hinet.hr (ls401.hinet.hr [195.29.150.2]) by ls405.hinet.hr (0.0.0/8.11.6) with ESMTP id h1GIhGx20544; Sun, 16 Feb 2003 19:43:16 +0100 Received: from EVON800V (ad15-m180.net.hinet.hr [195.29.50.180]) by ls401.hinet.hr (0.0.0/8.11.6) with SMTP id h1GIhEu12647; Sun, 16 Feb 2003 19:43:14 +0100 Message-ID: <001f01c2d5eb$349e84f0$b4321dc3@EVON800V> From: "Marko Dabrovic" To: "A Gallardo" , globillum@imag.fr References: <000a01c2d56e$b68d2f20$9b451840@delldaextn> Subject: Re: standardized GI/rad test scenes? Date: Sun, 16 Feb 2003 19:41:51 +0100 MIME-Version: 1.0 Content-Type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 6.00.2720.3000 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2600.0000 X-Loop: globillum@imag.fr X-Sequence: 174 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-UIDL: k8B"!mb[!!Gm4!!>eL"! X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit
Hi Arnold,
 
I have prepared two interesting (real lifes) scenes for testing GI, Cathetdral in Sibenik and Atrium of Sponza pallace in Dubrovnik. Another scene, Postsparkasse was prepared by Christian Bauer (mother of CGtechnique).
You can download all three models in majority of 3d formats at http://hdri.cgtechniques.com/~sibenik2/
I think these three scenes show how complex is way to measure abilities of software. some people have acheived better looking images since they knew software shortcuts better than others...
I would recomend you not to use textures, since they cover most of errors.
 
Regards,
Marko Dabrovic
RNA studio
From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id h1GJFjh11555; Sun, 16 Feb 2003 20:15:46 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h1GJCVl28552; Sun, 16 Feb 2003 20:12:31 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h1GJB4528317 for ; Sun, 16 Feb 2003 20:11:04 +0100 Received: from MAIL03.toast.net (mail.toast.net [206.244.185.10]) by imag.imag.fr (8.12.7/8.12.7) with ESMTP id h1GJB352008274 for ; Sun, 16 Feb 2003 20:11:03 +0100 (CET) Received: from delldaextn (unverified [64.24.68.161]) by MAIL03.toast.net (Vircom SMTPRS 1.4.232) with ESMTP id for ; Sun, 16 Feb 2003 14:05:59 -0500 From: "A Gallardo" To: globillum@imag.fr Subject: RE: standardized GI/rad test scenes? Date: Sun, 16 Feb 2003 14:12:20 -0500 Message-ID: <000901c2d5ef$544e68c0$a1441840@delldaextn> MIME-Version: 1.0 Content-Type: text/html; charset=windows-1252 X-Priority: 3 (Normal) X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook 8.5, Build 4.71.2173.0 Importance: Normal X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1106 In-Reply-To: <001f01c2d5eb$349e84f0$b4321dc3@EVON800V> X-Loop: globillum@imag.fr X-Sequence: 175 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-UIDL: Gd2!!KNJ"!P#o"!'aS!! X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit
Hi all,
 
    Thanks for these and thanks to those who privately e-mailed.  Actually I am not looking for actual geometry to use but just approaches, meaning images will do if they show a spcific test for a specific algorithm.  I am sorry if I gave the wrong impression on here asking for actual geometry or mesh to use, I am not.  I am not asking for those but rather situations and if I do need to watch for certain things when testing GI/radiosity renderers specifically if I do need to have different scenes for photon mapping and another for other types since I realized that some scenes would be easy for one algorithm but not the others so the test is not balanced.
 
    I would look at these though Mark and I am familiar already with your Cathedral challenge project but not the others. 
 
Sincerely,
 
Arnold
 
 
-----Original Message-----
From: Marko Dabrovic [mailto:mdabrov@rna.hr]
Sent: Sunday, February 16, 2003 1:42 PM
To: A Gallardo; globillum@imag.fr
Subject: Re: standardized GI/rad test scenes?

Hi Arnold,
 
I have prepared two interesting (real lifes) scenes for testing GI, Cathetdral in Sibenik and Atrium of Sponza pallace in Dubrovnik. Another scene, Postsparkasse was prepared by Christian Bauer (mother of CGtechnique).
You can download all three models in majority of 3d formats at http://hdri.cgtechniques.com/~sibenik2/
I think these three scenes show how complex is way to measure abilities of software. some people have acheived better looking images since they knew software shortcuts better than others...
I would recomend you not to use textures, since they cover most of errors.
 
Regards,
Marko Dabrovic
RNA studio
From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id h1H0KUh16754; Mon, 17 Feb 2003 01:20:31 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h1H0KCs12342; Mon, 17 Feb 2003 01:20:12 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h1H0Ij512305 for ; Mon, 17 Feb 2003 01:18:45 +0100 Received: from pd4mo2so.prod.shaw.ca (shawidc-mo1.cg.shawcable.net [24.71.223.10]) by imag.imag.fr (8.12.7/8.12.7) with ESMTP id h1H0Ii52015470 for ; Mon, 17 Feb 2003 01:18:45 +0100 (CET) Received: from pd4mr2so.prod.shaw.ca (pd4mr2so-qfe3.prod.shaw.ca [10.0.141.213]) by l-daemon (iPlanet Messaging Server 5.1 HotFix 0.8 (built May 12 2002)) with ESMTP id <0HAF00DFGF957A@l-daemon> for globillum@imag.fr; Sun, 16 Feb 2003 17:12:41 -0700 (MST) Received: from pn2ml10so.prod.shaw.ca (pn2ml10so-qfe0.prod.shaw.ca [10.0.121.80]) by l-daemon (iPlanet Messaging Server 5.1 HotFix 0.8 (built May 12 2002)) with ESMTP id <0HAF00173F95SG@l-daemon> for globillum@imag.fr; Sun, 16 Feb 2003 17:12:41 -0700 (MST) Received: from VANILLA (h24-87-171-230.vn.shawcable.net [24.87.171.230]) by l-daemon (iPlanet Messaging Server 5.1 HotFix 0.8 (built May 12 2002)) with SMTP id <0HAF006FMF93E9@l-daemon> for globillum@imag.fr; Sun, 16 Feb 2003 17:12:41 -0700 (MST) Date: Sun, 16 Feb 2003 16:14:27 -0800 From: Ian Ashdown Subject: ANNOUNCE - 03/02/16 Release of RADBIB and GITHESIS To: globillum@imag.fr Reply-to: Ian Ashdown Message-id: <002101c2d619$88ea5420$6401a8c0@VANILLA> Organization: byHeart Consultants Limited MIME-version: 1.0 X-MIMEOLE: Produced By Microsoft MimeOLE V6.00.2800.1106 X-Mailer: Microsoft Outlook Express 6.00.2800.1106 Content-type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-priority: Normal X-Loop: globillum@imag.fr X-Sequence: 176 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-UIDL: G1$#!45)!!K";!!?1_"! X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

ANNOUNCE: 03/02/16 Release of RADBIB and GITHESIS

RADBIB is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. It currently includes 2,195 references -- 10 new additions since its 03/01/05 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of February 16, 2003) from:

http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 284 references to radiosity and global illumination theses -- two new additions since the 03/01/05 release.

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

Ian Ashdown, P. Eng., LC, FIES
President
byHeart Consultants Limited
http://www.helios32.com

From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id h2SAl8e04242; Fri, 28 Mar 2003 11:47:09 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h2SAjxH29136; Fri, 28 Mar 2003 11:45:59 +0100 Received: from ebene.inrialpes.fr (ebene.inrialpes.fr [194.199.18.70]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h2SAgib29097 for ; Fri, 28 Mar 2003 11:42:44 +0100 Received: from safran.inrialpes.fr (safran.inrialpes.fr [194.199.26.1]) by ebene.inrialpes.fr (8.11.6/8.11.6) with ESMTP id h2SAghA15329 for ; Fri, 28 Mar 2003 11:42:43 +0100 (MET) Received: from imag.fr (ache [194.199.26.136]) by safran.inrialpes.fr (980427.SGI.8.8.8/8.8.5) with ESMTP id MAA15791 for ; Fri, 28 Mar 2003 12:42:44 +0200 (MDT) Date: Fri, 28 Mar 2003 11:42:43 +0100 Mime-Version: 1.0 Content-Type: multipart/mixed; boundary="------------080101070208090204070808" Subject: Visibility estimates From: Nicolas Holzschuch To: globillum@imag.fr Message-Id: <019078F5-610A-11D7-8ADF-00039310B9C2@imag.fr> X-Mailer: Apple Mail (2.551) X-Loop: globillum@imag.fr X-Sequence: 180 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-UIDL: 37[!!lp*#!S7f"!N9["! X-Mozilla-Status: 0001 X-Mozilla-Status2: 10000000 This is a multi-part message in MIME format. --------------080101070208090204070808 Content-Type: text/plain; charset=windows-1252; format=flowed Content-Transfer-Encoding: 8bit Hello fellow globillumers, sorry to put some traffic on an otherwise very quiet list :-), but I have a question, and I think other globillumers can have the answer. I have to compute a visibility estimate between a point and an area light source. That is to say, I am computing what percentage of the light source is visible from the point, taking into account occlusion. Something very classical, isnt't it? I have computed this value using two methods: - send a bunch of rays. Very easy to implement. Not very fast, but supposed to be accurate. I used 100 regularly spaced rays (10x10) - backprojection (see Drettakis 94). Projecting the occluders onto the plane of the emitter, and computing the area of the emitter that is not included in the projection. Very hard to implement, but accurate. Very accurate. I ran a series of test, and I plotted the two values against each other. x is for the backprojection method, y is for ray-casting. Here is the plot: Attachment Converted: "C:\meine Daten\eudora\Attach ab 2003.03.13\visibility.png" Roughly, the two methods are giving the same values. However, the ray-casting method can be quite far away from the exact value. Much more than I anticipated. We have errors of about 0.1 in the visibility estimate, even using 100 rays. Worse, we can have an error of 0.1 for a visibility value of 0.01, giving a relative error of 90 %. Anyone have an explanation for this difference? A way to reduce it, maybe? The points that are the most far away from the line are the points for whom the occluders are cutting the emitter in more than two parts (e.g. three parts, two parts that are hidden and one part that is visible) This is not just theory (although I would like to have an explanation on the reason for this difference). The difference in visibility estimates has a visible result on refinement for radiosity computations. -- Greetings, Nicolas Holzschuch ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- --------------080101070208090204070808 Content-Type: image/png; name="visibility.png" Content-Transfer-Encoding: base64 Content-Disposition: attachment; filename="visibility.png" iVBORw0KGgoAAAANSUhEUgAAAoAAAAHgBAMAAADH/8HXAAAAA3NCSVQCAgLMTMuiAAAAMFBM VEX//////1X/Vf//VVVV//9V/1VVVf9VVVWqqqqqqgCqAKqqAAAAqqoAqgAAAKoAAABJ/07M AAAAL3RFWHRTb2Z0d2FyZQBnbnVwbG90IExpbnV4IHZlcnNpb24gMy43IHBhdGNobGV2ZWwg MV0EBjsAABamSURBVHic7V1rquM8DDWI/r5bMZjsoxC6/y1cmAXciSW/kzSO87ITHfiYR2/b zPmOJVmWJSEYDAaDwWAwGAwG42L8XP0ArePv6gdoAyDnXmEFZkGpuVeIwD/GV/xT/ZwEicDf 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Xkj2ncXfecwS/itbwtGY9pJ3/q22ve4716u++J2Io2ygH9Ne8M4CU+a+s8julr0T8f1Jy72w H9Ne8M5CL6zfWeb5C98pihliMBgMBoPBYNwH/wEhlupxSxIXjwAAAABJRU5ErkJggg== --------------080101070208090204070808-- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id h2THKSe21905; Sat, 29 Mar 2003 18:20:29 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h2THH6n02314; Sat, 29 Mar 2003 18:17:06 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h2THCTb01988 for ; Sat, 29 Mar 2003 18:12:29 +0100 Received: from pd2mo2so.prod.shaw.ca (shawidc-mo1.cg.shawcable.net [24.71.223.10]) by imag.imag.fr (8.12.8/8.12.8) with ESMTP id h2THCSUT001361 for ; Sat, 29 Mar 2003 18:12:29 +0100 (CET) Received: from pd3mr2so.prod.shaw.ca (pd3mr2so-ser.prod.shaw.ca [10.0.141.178]) by l-daemon (iPlanet Messaging Server 5.1 HotFix 0.8 (built May 12 2002)) with ESMTP id <0HCI00J24T4RPY@l-daemon> for globillum@imag.fr; Sat, 29 Mar 2003 10:12:27 -0700 (MST) Received: from pn2ml5so.prod.shaw.ca (pn2ml5so-qfe0.prod.shaw.ca [10.0.121.149]) by l-daemon (iPlanet Messaging Server 5.1 HotFix 0.8 (built May 12 2002)) with ESMTP id <0HCI00F3KT4R9B@l-daemon> for globillum@imag.fr; Sat, 29 Mar 2003 10:12:27 -0700 (MST) Received: from VANILLA ([24.87.171.230]) by l-daemon (iPlanet Messaging Server 5.1 HotFix 0.8 (built May 12 2002)) with SMTP id <0HCI00FPXT4PET@l-daemon> for globillum@imag.fr; Sat, 29 Mar 2003 10:12:27 -0700 (MST) Date: Sat, 29 Mar 2003 09:15:29 -0800 From: Ian Ashdown Subject: Learning from the Cornell box To: globillum@imag.fr Reply-to: Ian Ashdown Message-id: <008201c2f616$cc794c10$6401a8c0@VANILLA> Organization: byHeart Consultants Limited MIME-version: 1.0 X-MIMEOLE: Produced By Microsoft MimeOLE V6.00.2800.1106 X-Mailer: Microsoft Outlook Express 6.00.2800.1106 Content-type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-priority: Normal X-Loop: globillum@imag.fr X-Sequence: 181 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-UIDL: 3ME!!?IV!!U'U!!#pf"! X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit
If you are interested in an artistic view of global illumination with specific reference to the "Cornell Box," you might be interested in reading:
 
Niedenthal, Simon. 2002. "Learning from the Cornell Box," Leonardo 35(3):249-254.
 
which is available online as:
 
 
Ian Ashdown, P. Eng., LC, FIES
President
byHeart Consultants Limited
http://www.helios32.com
 
From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id h2VAiSe14803; Mon, 31 Mar 2003 12:44:29 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h2VAeO410141; Mon, 31 Mar 2003 12:40:24 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h2VAbrb10066 for ; Mon, 31 Mar 2003 12:37:53 +0200 Received: from relay2.mail.uk.psi.net (relay2.mail.uk.psi.net [154.32.107.6]) by imag.imag.fr (8.12.8/8.12.8) with ESMTP id h2VAbq7H005925; Mon, 31 Mar 2003 12:37:52 +0200 (CEST) Received: from lightwork.co.uk ([195.152.206.2] helo=elvis.lightwork) by relay2.mail.uk.psi.net with esmtp (Exim 2.12 #2) id 18zwfj-0006ff-01; Mon, 31 Mar 2003 11:37:47 +0100 Received: by elvis.lightwork with Internet Mail Service (5.5.2650.21) id <18QQ1MBM>; Mon, 31 Mar 2003 11:37:46 +0100 Message-ID: <8815647C7041D111A3010060B06BE1C001E61B21@elvis.lightwork> From: Neil Gatenby To: Nicolas Holzschuch , globillum@imag.fr Subject: RE: Visibility estimates Date: Mon, 31 Mar 2003 11:37:37 +0100 MIME-Version: 1.0 X-Mailer: Internet Mail Service (5.5.2650.21) X-Loop: globillum@imag.fr X-Sequence: 182 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: a>k"!Hhn"!I=A!!`P@"! X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Nicolas Holzschuch wrote: > I have to compute a visibility estimate between a point and an area > light source. > > I have computed this value using two methods: > - send a bunch of rays. > - backprojection (see Drettakis 94). > Roughly, the two methods are giving the same values. However, the > ray-casting method can be quite far away from the exact value. Much > more than I anticipated. We have errors of about 0.1 in the visibility > estimate, even using 100 rays. Worse, we can have an error of 0.1 for a > visibility value of 0.01, giving a relative error of 90 %. Anyone have > an explanation for this difference? A way to reduce it, maybe? > > The points that are the most far away from the line are the points for > whom the occluders are cutting the emitter in more than two parts (e.g. > three parts, two parts that are hidden and one part that is visible) > > This is not just theory (although I would like to have an explanation > on the reason for this difference). The difference in visibility > estimates has a visible result on refinement for radiosity computations. Hiya Nicolas Surely the ray casting can be arbitrarily inaccurate, for appropriately unpleasant occluders? With thin occluders cutting across the source (as viewed from the point being lit) maybe all the rays miss? It is easy to picture a case where 10 very thin strips cover every single sample point, but the true visibility is actually only 0.000001 I have no great ideas for how to reduce the error. But maybe several tests consisting of 10 or 20 rays each would be a better place to start? If you carry out 5 tests, with 10 random rays each, and they each agree that the visibility is the same (probably 0 or 1) then probably you are OK. If they disagree, then probably you have a case where you should cast more rays. I know Pergathofer did some work on ray tracing which looked at the variance of the expected value of the pixel value; maybe you could keep sampling until the variance of the expected value of the visibility estimate goes small? Maybe Turbet's approach, where he uses different tools in different scenarios is the way to go? If you find that 5x10 rays give 5 very different answers, then go for back face culling? Or other oracles (see JeT) to decide when to be expensive and when to be cheap? Who is this Drettakis guy, anyway? ;-) Neil P.S. In architectural scenes, you find that lots of occluders are axis-aligned; in this case, a uniform sampling grid is probably not a good idea ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id h2VChue16222; Mon, 31 Mar 2003 14:43:58 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h2VCh8Z17774; Mon, 31 Mar 2003 14:43:08 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h2VCemb17463 for ; Mon, 31 Mar 2003 14:40:48 +0200 Received: from mwinf0301.wanadoo.fr (smtp4.wanadoo.fr [193.252.22.28]) by imag.imag.fr (8.12.8/8.12.8) with ESMTP id h2VCelFx014156 for ; Mon, 31 Mar 2003 14:40:47 +0200 (CEST) Received: from jedi.simteam.com (APh-Aug-103-1-3-85.abo.wanadoo.fr [80.11.153.85]) by mwinf0301.wanadoo.fr (Postfix) with SMTP id 0A750400749 for ; Mon, 31 Mar 2003 14:40:47 +0200 (CEST) Received: from simteam.com ([192.168.0.40]) by jedi.simteam.com (MERAK 3.00.140) with ESMTP id 048E177C for ; Mon, 31 Mar 2003 14:49:44 +0200 Message-ID: <3E8835C6.1FE52844@simteam.com> Date: Mon, 31 Mar 2003 14:34:14 +0200 From: Alan Savary X-Mailer: Mozilla 4.79 [en] (Windows NT 5.0; U) X-Accept-Language: en MIME-Version: 1.0 To: globillum@imag.fr Subject: Re: Visibility estimates References: <8815647C7041D111A3010060B06BE1C001E61B21@elvis.lightwork> X-Loop: globillum@imag.fr X-Sequence: 183 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: J7*"!'$9"!#=d!!@1U"! X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Its a quick thought but perhaps it can help you speeding up your visibility computation. I don't know the backprojection algo from Drettakis but what I'm thinking is that you should backproject your light geometry, then can cast a ray and if this ray intersect a primitive you backproject into the same structure the light was backprojected. Next you will cast ray by choosing a point outside the currently occluded regions of your backprojection structure. If this new ray intersect a new primitive (it should be a new one), do same process, and so on. At the end (when maximum cast, or full research space is occluded [no ray can be cast]), you should have a good estimate. Perhaps other optimization such as : - Use of a pixel-based occlusion buffer (for fast backprojection). If your projected primitive is convex, then is projection is convex too. So you know that each pixel inside the 2D convex shape (except border) fully occlude the light, for pixel border you could have a sampling approach. But the best thing is to avoid to cast ray that intersect border because if you cast a ray outside this border (in non-currently occluded area) you could perhaps project a new primitive that will cover border pixel. At the end when only border pixel remain, you could cast ray to refine your estimation at those boundaries. -If your the next point to evaluate is near the previous one, you could directly project previous projected primitive,... Hope this is not stupide, and is usefull. Alan Savary Neil Gatenby wrote: > Nicolas Holzschuch wrote: > > I have to compute a visibility estimate between a point and an area > > light source. > > > > I have computed this value using two methods: > > - send a bunch of rays. > > - backprojection (see Drettakis 94). > > > Roughly, the two methods are giving the same values. However, the > > ray-casting method can be quite far away from the exact value. Much > > more than I anticipated. We have errors of about 0.1 in the visibility > > estimate, even using 100 rays. Worse, we can have an error of 0.1 for a > > visibility value of 0.01, giving a relative error of 90 %. Anyone have > > an explanation for this difference? A way to reduce it, maybe? > > > > The points that are the most far away from the line are the points for > > whom the occluders are cutting the emitter in more than two parts (e.g. > > three parts, two parts that are hidden and one part that is visible) > > > > This is not just theory (although I would like to have an explanation > > on the reason for this difference). The difference in visibility > > estimates has a visible result on refinement for radiosity computations. > > Hiya Nicolas > > Surely the ray casting can be arbitrarily inaccurate, for appropriately > unpleasant occluders? With thin occluders cutting across the source (as > viewed from the point being lit) maybe all the rays miss? It is easy to > picture a case where 10 very thin strips cover every single sample point, > but the true visibility is actually only 0.000001 > > I have no great ideas for how to reduce the error. But maybe several tests > consisting of 10 or 20 rays each would be a better place to start? If you > carry out 5 tests, with 10 random rays each, and they each agree that the > visibility is the same (probably 0 or 1) then probably you are OK. If they > disagree, then probably you have a case where you should cast more rays. I > know Pergathofer did some work on ray tracing which looked at the variance > of the expected value of the pixel value; maybe you could keep sampling > until the variance of the expected value of the visibility estimate goes > small? > > Maybe Turbet's approach, where he uses different tools in different > scenarios is the way to go? If you find that 5x10 rays give 5 very > different answers, then go for back face culling? Or other oracles (see > JeT) to decide when to be expensive and when to be cheap? > > Who is this Drettakis guy, anyway? > > ;-) > > Neil > > P.S. In architectural scenes, you find that lots of occluders are > axis-aligned; in this case, a uniform sampling grid is probably not a good > idea > > ------------------------------------------------------------------------ > ------------------------------------------------------------------------- > globillum@imag.fr -- mailing list devoted to global illumination research > For list archives or to configure your options, see http://listes.imag.fr > ------------------------------------------------------------------------- -- ============================================ "Savoir c'est vivre, et maintenir dans l'ignorance c'est presque un homicide" ============================================ Alan Savary Technical Director - R&D Engineer SimTeam Tel: +33 (0)1 53 27 37 77 Fax: +33 (0)1 53 27 37 78 Web: http://www.simteam.com email: alan@simteam.com ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id h32EJxe18765; Wed, 2 Apr 2003 16:20:00 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h32EGHi08088; Wed, 2 Apr 2003 16:16:17 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h32EGBj08071 for ; Wed, 2 Apr 2003 16:16:11 +0200 Received: from nut.autodesk.com (nut.autodesk.com [198.102.112.27]) by imag.imag.fr (8.12.9/8.12.8) with ESMTP id h32EGAhm010482 for ; Wed, 2 Apr 2003 16:16:11 +0200 (CEST) Received: from msgpetfe1.amer.ads.autodesk.com ([144.111.32.12]) by nut.autodesk.com (8.12.8/8.12.6) with ESMTP id h32EG3Wf001741 for ; Wed, 2 Apr 2003 06:16:09 -0800 (PST) Received: from msgpetmb1.amer.ads.autodesk.com ([144.111.33.142]) by msgpetfe1.amer.ads.autodesk.com with Microsoft SMTPSVC(5.0.2195.5329); Wed, 2 Apr 2003 06:16:08 -0800 x-mimeole: Produced By Microsoft Exchange V6.0.6249.0 content-class: urn:content-classes:message MIME-Version: 1.0 Content-Type: text/html; charset=windows-1252 Subject: SIGGRAPH 2003 papers web page Date: Wed, 2 Apr 2003 06:16:08 -0800 Message-ID: Thread-Topic: SIGGRAPH 2003 papers web page Thread-Index: AcL5Imbis3ljEQUgSpC/87Hm7O1q4g== From: "Eric Haines (Autodesk, NY)" To: globillum@imag.fr X-OriginalArrivalTime: 02 Apr 2003 14:16:08.0094 (UTC) FILETIME=[67879BE0:01C2F922] X-Loop: globillum@imag.fr X-Sequence: 184 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-UIDL: W?-!!,\E!!`>_"!$]&"! 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In case you hadn’t heard, Tim Rowley does it again: http://www.cs.brown.edu/people/tor/sig2003.html

 

From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id h38FIIe21349; Tue, 8 Apr 2003 17:18:22 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h38FELD05083; Tue, 8 Apr 2003 17:14:21 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h38FBim05042 for ; Tue, 8 Apr 2003 17:11:44 +0200 Received: from pd6mo3so.prod.shaw.ca (shawidc-mo1.cg.shawcable.net [24.71.223.10]) by imag.imag.fr (8.12.9/8.12.8) with ESMTP id h38FBhOw015674 for ; Tue, 8 Apr 2003 17:11:44 +0200 (CEST) Received: from pd6mr4so.prod.shaw.ca (pd6mr4so-qfe3.prod.shaw.ca [10.0.141.219]) by l-daemon (iPlanet Messaging Server 5.1 HotFix 0.8 (built May 12 2002)) with ESMTP id <0HD1009A767HMO@l-daemon> for globillum@imag.fr; Tue, 08 Apr 2003 09:11:41 -0600 (MDT) Received: from pn2ml10so.prod.shaw.ca (pn2ml10so-qfe0.prod.shaw.ca [10.0.121.80]) by l-daemon (iPlanet Messaging Server 5.1 HotFix 0.8 (built May 12 2002)) with ESMTP id <0HD10092U67H0L@l-daemon> for globillum@imag.fr; Tue, 08 Apr 2003 09:11:41 -0600 (MDT) Received: from VANILLA (h24-87-171-230.vn.shawcable.net [24.87.171.230]) by l-daemon (iPlanet Messaging Server 5.1 HotFix 0.8 (built May 12 2002)) with SMTP id <0HD10077R67FNL@l-daemon> for globillum@imag.fr; Tue, 08 Apr 2003 09:11:41 -0600 (MDT) Date: Tue, 08 Apr 2003 08:15:03 -0700 From: Ian Ashdown Subject: Unifying equation useful for CG? To: globillum@imag.fr Reply-to: Ian Ashdown Message-id: <004701c2fde1$a1814df0$6401a8c0@VANILLA> Organization: byHeart Consultants Limited MIME-version: 1.0 X-MIMEOLE: Produced By Microsoft MimeOLE V6.00.2800.1106 X-Mailer: Microsoft Outlook Express 6.00.2800.1106 Content-type: multipart/related; boundary="------------010506020409030509020209" X-Priority: 3 X-MSMail-priority: Normal X-Loop: globillum@imag.fr X-Sequence: 186 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-UIDL: AA>!!3GV!!>IH!!am'#! X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 This is a multi-part message in MIME format. --------------010506020409030509020209 Content-Type: text/html; charset=windows-1252 Content-Transfer-Encoding: 8bit

While I would not normally post off-topic information to our mailing list, this news item from www.nature.com&nbsp;caught my interest. While I have not yet read the American Journal of Botany paper it references (and normally I would never look at this journal), the existence of a unifying equation for many geometric shapes would clearly have implications for computer graphics applications.

- Ian Ashdown

Maths gets into shape

Is it a starfish? Is it an orchid? No, it's Superformula.
2 April 2003

JOHN WHITFIELD

For centuries scientists have sought to express natural forms in mathematical terms.
© alamy.com

One simple equation can generate a vast diversity of natural shapes, a Belgian biologist has discovered. The Superformula, as its creator Johan Gielis has christened it, produces everything from simple triangles and pentagons, to stars, spirals and petals.

"When I found the formula, all these beautiful shapes came rolling out of my computer," says Gielis, at University of Nijmegen, Holland. "It seemed too good to be true - I spent two years thinking 'What did I do wrong?' and 'How come no one else has discovered it?'" Having spoken to mathematicians, he reckons that he's found something new.

The Superformula is a modified version of the equation for a circle1. Changing one term in the formula varies the proportions of the shape - moving from a round circle to a long and skinny ellipse. Changing another varies the axes of symmetry - shifting from a circle to triangle, square, pentagon and so on.

Varying both proportion and symmetry together produces shapes with any number of sides, regular and irregular. It can also produce three-dimensional structures, and non-biological shapes such as snowflakes and crystals. "It's a new way of describing nature," says Gielis.

For centuries, scientists have sought to express natural forms - such as the spiral of a sheep's horn, the branching of a tree, or a bee's honeycomb - in mathematical terms.

"Describing form is one of the more intractable problems in biology," says botanist Karl Niklas of Cornell University in Ithaca, New York. Researchers have come up with many ways to describe leaves and shells, for example, but there is little unity: "Things have become cumbersome and idiosyncratic," he says.

The Superformula might provide a single, simple framework for analysing and comparing the shapes of life, believes Niklas. "This is an exciting development."

The Superformula produces regular and irregular shapes with any number of sides.
© J. Gielis

Gielis has patented his discovery, and is developing computer software based on it. Using one formula to produce shapes will make graphics programs much more efficient, he says. It might also be useful in pattern recognition.

What's less clear is whether nature uses the formula to generate different shapes. "I'm not convinced this is significant, but it might turn out to be profound if it could be related to how things grow," says mathematician Ian Stewart of the University of Warwick, UK.

Other, more complicated, single equations can produce a similar diversity of shapes, says Stewart. He believes that the Superformula is more likely to provide a useful tool than an insight into how life actually works.

Gielis acknowledges that the formula describes nature's end product, not how it got there, but he hopes that time might prove the Superformula's profundity. "Description always precedes ideas about the real connection between maths and nature," he says.

References
  1. Gielis, J. A generic geometric transformation that unifies a wide range of natural and abstract shapes. American Journal of Botany, 90, 333 - 338, (2003). |Article|


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(host6924.igd.fhg.de [146.140.28.12] (may be forged)) by imag.imag.fr (8.12.9/8.12.8) with ESMTP id h38FsiOw019102 for ; Tue, 8 Apr 2003 17:54:44 +0200 (CEST) Received: from duerer.igd.fhg.de (duerer.igd.fhg.de [146.140.4.203]) by heinrichschiff.igd.fhg.de (8.9.3+Sun/8.9.3) with ESMTP id RAA15248 for ; Tue, 8 Apr 2003 17:48:13 +0200 (MEST) From: Wolfram Kresse Received: (from wkresse@localhost) by duerer.igd.fhg.de (SGI-8.9.3/8.9.3) id RAA02836 for globillum@imag.fr; Tue, 8 Apr 2003 17:54:44 +0200 (CEST) Date: Tue, 8 Apr 2003 17:54:44 +0200 (CEST) Message-Id: <1030408175444.ZM28341064@duerer.igd.fhg.de> In-Reply-To: Ian Ashdown "Unifying equation useful for CG?" (Apr 8, 8:15) References: <004701c2fde1$a1814df0$6401a8c0@VANILLA> X-Face: 'Sr;3%AL1_h0kt\C+>MJ`;@c\l#+Nm/{W2Jt#x^CqV-EPD-6Oa[(>Marf,0v:#BRzP}Myyd]6$Gg+hfmjp&N7n*\xiDN;j!i&. List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: L$[!!$a~!!CNI!!01l!! X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Here is some more information (.pdf and source) http://astronomy.swin.edu.au/~pbourke/curves/supershape/ Cheers, Wolfram -- +-----+-----Wolfram Kresse------------------------------------------------+ | 8-P | wkresse@igd.fhg.de http://www.igd.fhg.de/~wkresse 06151/155-276 | +-----+-------------------------+-----------------+-----------------------+ Worf: 70 Romulan ships are attacking Starbase 420. We are supposed to meet at coordinates 29.9 mark 310. Picard: Ummmh...tell them our...our... Geordi: ...spatial hyperscanner? Picard: ...is broken, and we need to wait for a... Number One: Channeled automnemonic tetrion processor? Picard: Yeah, that's a good one! ...to replace it. ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id h38JbLe24255; Tue, 8 Apr 2003 21:37:22 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h38JbAm20864; Tue, 8 Apr 2003 21:37:10 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h38JYWm20559 for ; Tue, 8 Apr 2003 21:34:32 +0200 Received: from wren.cs.unc.edu (wren.cs.unc.edu [152.2.128.86]) by imag.imag.fr (8.12.9/8.12.8) with ESMTP id h38JYUIf014455 for ; Tue, 8 Apr 2003 21:34:31 +0200 (CEST) Received: from HARRISMCS (harrism-cs.cs.unc.edu [152.2.132.112]) by wren.cs.unc.edu (8.12.8/8.12.5) with ESMTP id h38JYME2022078; Tue, 8 Apr 2003 15:34:23 -0400 (EDT) Reply-To: harrism@cs.unc.edu From: "Mark Harris" To: "'Ian Ashdown'" , globillum@imag.fr Subject: RE: Unifying equation useful for CG? Date: Tue, 8 Apr 2003 15:34:22 -0400 Message-ID: <002701c2fe05$dbfe4180$70840298@cs.unc.edu> MIME-Version: 1.0 Content-Type: multipart/mixed; boundary="------------030406060700070704000905" X-Priority: 3 (Normal) X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook, Build 10.0.2627 In-Reply-To: <004701c2fde1$a1814df0$6401a8c0@VANILLA> Importance: Normal X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1106 X-Loop: globillum@imag.fr X-Sequence: 188 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-UIDL: T8X"!~Z"!!*!R"!-eX"! X-Mozilla-Status: 0011 X-Mozilla-Status2: 10000000 This is a multi-part message in MIME format. --------------030406060700070704000905 Content-Type: multipart/related; boundary="------------050405050406060503000106" --------------050405050406060503000106 Content-Type: text/html; charset=windows-1252 Content-Transfer-Encoding: 7bit Message
Hi all,
&nbsp;
I don't know if there are big&nbsp;implications for computer graphics applications, but it sure is easy to code up (10 minutes)!&nbsp; Here is a simple Cg program that generates a SuperShape (as a height field).&nbsp; I used the result to create a bumpmap and generate the image attached.&nbsp; I'll put a demo on my website when I get time to clean it up.&nbsp; What a neat formula!
&nbsp;
fragout main(vf30 IN,
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; uniform float2&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; resolution,
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; uniform float&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; heightScale,
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; uniform float4&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; params) // m, n1-n3
{
&nbsp; fragout OUT;
&nbsp;
&nbsp; float2 pos = 0.5 - IN.WPOS.xy / resolution.xy;
&nbsp; float R&nbsp;&nbsp;&nbsp; = length(pos);
&nbsp; float phi&nbsp; = acos(pos.x / R);
&nbsp;
&nbsp; float t1&nbsp;&nbsp; = pow(abs(cos(params.x * phi / 4)), params.z);
&nbsp; float t2&nbsp;&nbsp; = pow(abs(sin(params.x * phi / 4)), params.w);
&nbsp;
&nbsp; float r&nbsp;&nbsp;&nbsp; = 1 / pow(t1 + t2, 1 / params.y);
&nbsp;
&nbsp; OUT.col&nbsp;&nbsp; = heightScale * ((R < 0.5 * r) ? 2 * R / r : 1);
&nbsp;
&nbsp; return OUT;
}
&nbsp;
Mark
-----Original Message-----
From: Ian Ashdown [mailto:ian_ashdown@helios32.com]
Sent: Tuesday, April 08, 2003 11:15 AM
To: globillum@imag.fr
Subject: Unifying equation useful for CG?

While I would not normally post off-topic information to our mailing list, this news item from www.nature.com&nbsp;caught my interest. While I have not yet read the American Journal of Botany paper it references (and normally I would never look at this journal), the existence of a unifying equation for many geometric shapes would clearly have implications for computer graphics applications.

- Ian Ashdown

Maths gets into shape

Is it a starfish? Is it an orchid? No, it's Superformula.
2 April 2003

JOHN WHITFIELD

For centuries scientists have sought to express natural forms in mathematical terms.
&copy; alamy.com

One simple equation can generate a vast diversity of natural shapes, a Belgian biologist has discovered. The Superformula, as its creator Johan Gielis has christened it, produces everything from simple triangles and pentagons, to stars, spirals and petals.

"When I found the formula, all these beautiful shapes came rolling out of my computer," says Gielis, at University of Nijmegen, Holland. "It seemed too good to be true - I spent two years thinking 'What did I do wrong?' and 'How come no one else has discovered it?'" Having spoken to mathematicians, he reckons that he's found something new.

The Superformula is a modified version of the equation for a circle1. Changing one term in the formula varies the proportions of the shape - moving from a round circle to a long and skinny ellipse. Changing another varies the axes of symmetry - shifting from a circle to triangle, square, pentagon and so on.

Varying both proportion and symmetry together produces shapes with any number of sides, regular and irregular. It can also produce three-dimensional structures, and non-biological shapes such as snowflakes and crystals. "It's a new way of describing nature," says Gielis.

For centuries, scientists have sought to express natural forms - such as the spiral of a sheep's horn, the branching of a tree, or a bee's honeycomb - in mathematical terms.

"Describing form is one of the more intractable problems in biology," says botanist Karl Niklas of Cornell University in Ithaca, New York. Researchers have come up with many ways to describe leaves and shells, for example, but there is little unity: "Things have become cumbersome and idiosyncratic," he says.

The Superformula might provide a single, simple framework for analysing and comparing the shapes of life, believes Niklas. "This is an exciting development."

The Superformula produces regular and irregular shapes with any number of sides.
&copy; J. Gielis

Gielis has patented his discovery, and is developing computer software based on it. Using one formula to produce shapes will make graphics programs much more efficient, he says. It might also be useful in pattern recognition.

What's less clear is whether nature uses the formula to generate different shapes. "I'm not convinced this is significant, but it might turn out to be profound if it could be related to how things grow," says mathematician Ian Stewart of the University of Warwick, UK.

Other, more complicated, single equations can produce a similar diversity of shapes, says Stewart. He believes that the Superformula is more likely to provide a useful tool than an insight into how life actually works.

Gielis acknowledges that the formula describes nature's end product, not how it got there, but he hopes that time might prove the Superformula's profundity. "Description always precedes ideas about the real connection between maths and nature," he says.

References
  1. Gielis, J. A generic geometric transformation that unifies a wide range of natural and abstract shapes. American Journal of Botany, 90, 333 - 338, (2003). |Article|


&copy; Nature News Service / Macmillan Magazines Ltd 2003

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4hB4if8ARPf+ZbI//nmY/wDEQOEf+hv/AOWGZ/8AzEf1RiQ9iD7Hr/Q08Se2PcH/AD/Ov5W/ +Ilo9/2LP/Njcf8AvCDSj/g5bI6fsWH/AMSO/wDxD0f8Qg8RP+ie/wDMtkf/AM8w/wCIgcI/ 9Df/AMsMz/8AmI/qnEv+1j64/mf8aeJD6A/T/Jr+Vcf8HLp7/sVg/wDdxv8A+If+lL/xEvf9 WV/+bHf/AIh6X/EH/EP/AKJ37s2yNefTM/If/EQeEv8Aob+WuAzN/ngvI/u98EHPgvwifXwv oB/8pVpRXlX7KXxM/wCF0/sufs2/GP8AsX/hGv8AhbPwD+DvxM/4Rz+0v7Z/sD/hPPh54d8U /wBi/wBr/YNK/tX+yv7V+w/2l/Zem/bvI+1fYLPzfs8ZX9V5fRqYfAYHD1o8lWhg8NRqwvGX LUpUYQnHmi5Rlyyi1eMnF2um1Zn4Ri6kK2KxNWnLmp1cRWqU5Wa5oTqSlGVpJSV4tO0kmtmk 9D/LL/4KQ/8AKRD9vX/s9D9qT/1ePjqvi+iivsaf8On/AII/+ko8CW79X+YUUUVYgooooAKK KKACiiigAooooAKKKKACiiigAooooAKKKKACiiigAooooAKKKKACiiigAooooAKKKKAP9bD/ AIJvf8o7/wBgr/sy/wDZb/8AVHeBaKKK+Zn8cv8AFL82etD4I/4Y/kj/2Q== --------------030406060700070704000905-- From Return-Path: Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id h39MIte09459; Thu, 10 Apr 2003 00:18:56 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h39MIb316568; Thu, 10 Apr 2003 00:18:37 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h39MIUe16551 for ; Thu, 10 Apr 2003 00:18:30 +0200 Received: from mail.tricity.wsu.edu (oberon.tricity.wsu.edu [192.220.200.27]) by imag.imag.fr (8.12.9/8.12.8) with ESMTP id h39MIRcQ003919 for ; Thu, 10 Apr 2003 00:18:29 +0200 (CEST) Received: (from bobl@localhost) by mail.tricity.wsu.edu (8.11.6/8.9.3) id h39MKVq04154 for globillum@imag.fr; Wed, 9 Apr 2003 15:20:31 -0700 Date: Wed, 9 Apr 2003 15:20:31 -0700 From: Bob Lewis To: globillum@imag.fr Subject: Re: Unifying equation useful for CG? Message-ID: <20030409152031.A3474@peacock.tricity.wsu.edu> References: <004701c2fde1$a1814df0$6401a8c0@VANILLA> <002701c2fe05$dbfe4180$70840298@cs.unc.edu> Mime-Version: 1.0 User-Agent: Mutt/1.2.5.1i In-Reply-To: <002701c2fe05$dbfe4180$70840298@cs.unc.edu>; from harrism@cs.unc.edu on Tue, Apr 08, 2003 at 03:34:22PM -0400 X-Loop: globillum@imag.fr X-Sequence: 189 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: >Q6!!9S0!!JI[!!`!3!! X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit On Tue, Apr 08, 2003 at 03:34:22PM -0400, Mark Harris wrote: > I don't know if there are big implications for computer graphics > applications, but it sure is easy to code up (10 minutes)! Here is a > simple Cg program that generates a SuperShape (as a height field). I > used the result to create a bumpmap and generate the image attached. > I'll put a demo on my website when I get time to clean it up. What a > neat formula! > > fragout main(vf30 IN, > uniform float2 resolution, > uniform float heightScale, > uniform float4 params) // m, n1-n3 > { ... > } Very nice images! The code, however, assumes that 0 <= phi <= 2pi (as it must for an image or height field). The formula is weirder than that, however. Larger values of phi can produce Spirograph(TM)-like patterns, especially for non-integer "m" values. I've thrown together a little ~100-line interactive Python program that visualizes the function. You can download it from http://www.tricity.wsu.edu/~bobl/superb-0.1.tar. The README (included in the tar file) is: This is the modestly-named "superb", a quick-and-dirty interactive browser for the supershape function. To run it, you need Python (probably 2.1 or later) and the Tkinter user interface package. There's a GIF image "supershape1.gif" (courtesy of Paul Bourke) that, ideally, needs to be in your local directory when you run it. It's only known deficiency is that it is missing an optimal formula for the maximum phi value to produce a closed figure for non-integer m. (See the code for more details.) I welcome suggestions. If you find it useful, let me know. In any case, no warranty is expressed or implied. - Bob Lewis bobl@tricity.wsu.edu ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id h44KO8e28305; Sun, 4 May 2003 22:24:09 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by tuvok.kom.tuwien.ac.at (8.12.8/8.12.8) with ESMTP id h44KOBsA013389; Sun, 4 May 2003 22:24:11 +0200 (MEST) X-Connecting-Host: imag.imag.fr [129.88.30.1] X-Connecting-Addr: 129.88.30.1 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by imag.imag.fr (8.12.9/8.12.9) with ESMTP id h44KNxnr022739; Sun, 4 May 2003 22:24:01 +0200 (CEST) Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h44KNwi02716; Sun, 4 May 2003 22:23:58 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h44KM3J02442 for ; Sun, 4 May 2003 22:22:03 +0200 Received: from pd6mo1so.prod.shaw.ca (shawidc-mo1.cg.shawcable.net [24.71.223.10]) by imag.imag.fr (8.12.9/8.12.9) with ESMTP id h44KM2nr022637 for ; Sun, 4 May 2003 22:22:02 +0200 (CEST) Received: from pd6mr4so.prod.shaw.ca (pd6mr4so-qfe3.prod.shaw.ca [10.0.141.219]) by l-daemon (iPlanet Messaging Server 5.1 HotFix 0.8 (built May 12 2002)) with ESMTP id <0HED00IE5PWP6K@l-daemon> for globillum@imag.fr; Sun, 04 May 2003 14:22:01 -0600 (MDT) Received: from pn2ml8so.prod.shaw.ca (pn2ml8so-qfe0.prod.shaw.ca [10.0.121.152]) by l-daemon (iPlanet Messaging Server 5.1 HotFix 0.8 (built May 12 2002)) with ESMTP id <0HED00IAWPWPLV@l-daemon> for globillum@imag.fr; Sun, 04 May 2003 14:22:01 -0600 (MDT) Received: from VANILLA (h24-87-171-230.vn.shawcable.net [24.87.171.230]) by l-daemon (iPlanet Messaging Server 5.1 HotFix 0.8 (built May 12 2002)) with SMTP id <0HED00LCVPWOT8@l-daemon> for globillum@imag.fr; Sun, 04 May 2003 14:22:01 -0600 (MDT) Date: Sun, 04 May 2003 13:26:16 -0700 From: Ian Ashdown Subject: ANNOUNCE: RADBIB and GITHESIS updated To: globillum@imag.fr Reply-to: Ian Ashdown Message-id: <009d01c3127b$6a24cd60$6401a8c0@VANILLA> Organization: byHeart Consultants Limited MIME-version: 1.0 X-MIMEOLE: Produced By Microsoft MimeOLE V6.00.2800.1165 X-Mailer: Microsoft Outlook Express 6.00.2800.1158 Content-type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-priority: Normal X-Loop: globillum@imag.fr X-Sequence: 192 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -21 X-Spam-TU-Processing-Host: tuvok X-UIDL: B5]!!TG8!!%Rm"!MnP"! X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

ANNOUNCE: 03/05/04 Release of RADBIB and GITHESIS
-------------------------------------------------
RADBIB is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. It currently includes 2,218 references -- 23 new additions since its 03/02/16 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of May 4, 2003) from:

http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 288 references to radiosity and global illumination theses -- 4 new additions since the 03/02/16 release.

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

Ian Ashdown, P. Eng., LC, FIES
President
byHeart Consultants Limited
http://www.helios32.com

From Return-Path: Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id h4HIHbe14911; Sat, 17 May 2003 20:17:40 +0200 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by imag.imag.fr (8.12.9/8.12.9) with ESMTP id h4HIHJiV013626; Sat, 17 May 2003 20:17:21 +0200 (CEST) Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h4HIHHc13189; Sat, 17 May 2003 20:17:17 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h4HIHAY13172 for ; Sat, 17 May 2003 20:17:10 +0200 Received: from pd3mo3so.prod.shaw.ca ([24.71.223.10]) by imag.imag.fr (8.12.9/8.12.9) with ESMTP id h4HIGpiV013600 for ; Sat, 17 May 2003 20:17:10 +0200 (CEST) Received: from pd3mr3so.prod.shaw.ca (pd3mr3so-ser.prod.shaw.ca [10.0.141.179]) by l-daemon (iPlanet Messaging Server 5.2 HotFix 1.14 (built Mar 18 2003)) with ESMTP id <0HF100CMHMRQJ0@l-daemon> for globillum@imag.fr; Sat, 17 May 2003 12:16:38 -0600 (MDT) Received: from pn2ml7so.prod.shaw.ca (pn2ml7so-qfe0.prod.shaw.ca [10.0.121.151]) by l-daemon (iPlanet Messaging Server 5.2 HotFix 1.14 (built Mar 18 2003)) with ESMTP id <0HF10046PMRQMZ@l-daemon> for globillum@imag.fr; Sat, 17 May 2003 12:16:38 -0600 (MDT) Received: from VANILLA (h24-87-171-230.vn.shawcable.net [24.87.171.230]) by l-daemon (iPlanet Messaging Server 5.2 HotFix 1.14 (built Mar 18 2003)) with SMTP id <0HF1004P8MRPT5@l-daemon> for globillum@imag.fr; Sat, 17 May 2003 12:16:38 -0600 (MDT) Date: Sat, 17 May 2003 11:21:18 -0700 From: Ian Ashdown Subject: ANNOUNCE: RADBIB and GITHESIS updated (May 17, 2003) To: globillum@imag.fr Reply-to: Ian Ashdown Message-id: <001901c31ca1$1cb28600$6401a8c0@VANILLA> Organization: byHeart Consultants Limited MIME-version: 1.0 X-MIMEOLE: Produced By Microsoft MimeOLE V6.00.2800.1165 X-Mailer: Microsoft Outlook Express 6.00.2800.1158 X-Priority: 3 X-MSMail-priority: Normal X-Loop: globillum@imag.fr X-Sequence: 195 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-UIDL: ?6n!!f0["!/bo!!biI!! X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit ANNOUNCE: 03/05/17 Release of RADBIB and GITHESIS --------------------------------------------------------------- RADBIB is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. It currently includes 2,246 references -- 28 new additions since its 03/05/04 release. This bibliography is available in BibTex format as RADBIB.BIB (with a release date of May 17, 2003) from: http://www.helios32.com (Resources section) Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 294 references to radiosity and global illumination theses -- 6 new additions since the 03/05/04 release. Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited. Ian Ashdown, P. Eng., LC, FIES President byHeart Consultants Limited http://www.helios32.com ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id h4PFc5X11052; Sun, 25 May 2003 17:38:06 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by tuvok.kom.tuwien.ac.at (8.12.8/8.12.8) with ESMTP id h4PFc6kZ019458; Sun, 25 May 2003 17:38:06 +0200 (MEST) X-Connecting-Host: imag.imag.fr [129.88.30.1] X-Connecting-Addr: 129.88.30.1 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by imag.imag.fr (8.12.9/8.12.9) with ESMTP id h4PFbwLM023316; Sun, 25 May 2003 17:38:01 +0200 (CEST) Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h4PFbpx03371; Sun, 25 May 2003 17:37:51 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h4PFZsY03050 for ; Sun, 25 May 2003 17:35:54 +0200 Received: from pd5mo1so.prod.shaw.ca (shawidc-mo1.cg.shawcable.net [24.71.223.10]) by imag.imag.fr (8.12.9/8.12.9) with ESMTP id h4PFZoLM023059 for ; Sun, 25 May 2003 17:35:51 +0200 (CEST) Received: from pd4mr1so.prod.shaw.ca (pd4mr1so-qfe3.prod.shaw.ca [10.0.141.212]) by l-daemon (iPlanet Messaging Server 5.2 HotFix 1.14 (built Mar 18 2003)) with ESMTP id <0HFG00JPQ8NP14@l-daemon> for globillum@imag.fr; Sun, 25 May 2003 09:35:49 -0600 (MDT) Received: from pn2ml10so.prod.shaw.ca (pn2ml10so-qfe0.prod.shaw.ca [10.0.121.80]) by l-daemon (iPlanet Messaging Server 5.2 HotFix 1.14 (built Mar 18 2003)) with ESMTP id <0HFG009K08NPDR@l-daemon> for globillum@imag.fr; Sun, 25 May 2003 09:35:49 -0600 (MDT) Received: from VANILLA (h24-87-171-230.vn.shawcable.net [24.87.171.230]) by l-daemon (iPlanet Messaging Server 5.2 HotFix 1.14 (built Mar 18 2003)) with SMTP id <0HFG00DPJ8NO2T@l-daemon> for globillum@imag.fr; Sun, 25 May 2003 09:35:49 -0600 (MDT) Date: Sun, 25 May 2003 08:40:45 -0700 From: Ian Ashdown Subject: ANNOUNCE: RADBIB and GITHESIS updated (again) To: globillum@imag.fr Reply-to: Ian Ashdown Message-id: <007001c322d4$02462b30$6401a8c0@VANILLA> Organization: byHeart Consultants Limited MIME-version: 1.0 X-MIMEOLE: Produced By Microsoft MimeOLE V6.00.2800.1165 X-Mailer: Microsoft Outlook Express 6.00.2800.1158 Content-type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-priority: Normal X-MailScanner: Found to be clean, Found to be clean X-Loop: globillum@imag.fr X-Sequence: 196 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-MailScanner-Information: Please contact the ISP for more information X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -36 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok X-UIDL: EBk!!n#K"!6+V"!ofX!! X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

ANNOUNCE: 03/05/25 Release of RADBIB and GITHESIS
RADBIB is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. It currently includes 2,260 references -- 14 new additions since its 03/05/17 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of May 25, 2003) from:

http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 294 references to radiosity and global illumination theses -- no new additions since the 03/05/17 release.

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

Ian Ashdown, P. Eng., LC, FIES
President
byHeart Consultants Limited
http://www.helios32.com

From Return-Path: Received: from neelix.kom.tuwien.ac.at (neelix.kom.tuwien.ac.at [192.35.241.67]) by christl.cg.tuwien.ac.at (8.11.6/8.11.6) with ESMTP id h5UFvSX21903; Mon, 30 Jun 2003 17:57:29 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by neelix.kom.tuwien.ac.at (8.12.8/8.12.8) with ESMTP id h5UFvRsP019902; Mon, 30 Jun 2003 17:57:27 +0200 (MEST) X-Connecting-Host: imag.imag.fr [129.88.30.1] X-Connecting-Addr: 129.88.30.1 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by imag.imag.fr (8.12.9/8.12.9) with ESMTP id h5TGUQgn020921; Sun, 29 Jun 2003 18:30:26 +0200 (CEST) Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h5TGUPY18386; Sun, 29 Jun 2003 18:30:25 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h5TGSNs18315 for ; Sun, 29 Jun 2003 18:28:23 +0200 Received: from pd5mo2so.prod.shaw.ca ([24.71.223.10]) by imag.imag.fr (8.12.9/8.12.9) with ESMTP id h5TGSLgn020645 for ; Sun, 29 Jun 2003 18:28:22 +0200 (CEST) Received: from pd4mr1so.prod.shaw.ca (pd4mr1so-qfe3.prod.shaw.ca [10.0.141.212]) by l-daemon (iPlanet Messaging Server 5.2 HotFix 1.16 (built May 14 2003)) with ESMTP id <0HH900DFU4EYEG@l-daemon> for globillum@imag.fr; Sun, 29 Jun 2003 10:28:10 -0600 (MDT) Received: from pn2ml4so.prod.shaw.ca (pn2ml4so-qfe0.prod.shaw.ca [10.0.121.148]) by l-daemon (iPlanet Messaging Server 5.2 HotFix 1.16 (built May 14 2003)) with ESMTP id <0HH900GPD4EY1P@l-daemon> for globillum@imag.fr; Sun, 29 Jun 2003 10:28:10 -0600 (MDT) Received: from VANILLA (h24-87-171-230.vn.shawcable.net [24.87.171.230]) by l-daemon (iPlanet Messaging Server 5.2 HotFix 1.16 (built May 14 2003)) with SMTP id <0HH9004ON4EWVF@l-daemon> for globillum@imag.fr; Sun, 29 Jun 2003 10:28:10 -0600 (MDT) Date: Sun, 29 Jun 2003 09:28:05 -0700 From: Ian Ashdown Subject: ANNUNCE: 03/06/29 Release of RADBIB and GITHESIS To: globillum@imag.fr Reply-to: Ian Ashdown Message-id: <002401c33e5b$6b028860$6401a8c0@VANILLA> Organization: byHeart Consultants Limited MIME-version: 1.0 X-MIMEOLE: Produced By Microsoft MimeOLE V6.00.2800.1165 X-Mailer: Microsoft Outlook Express 6.00.2800.1158 Content-type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-priority: Normal X-MailScanner: Found to be clean, Found to be clean X-Loop: globillum@imag.fr X-Sequence: 197 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-MailScanner-Information: Please contact the ISP for more information X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -6 X-Spam-Level: - X-Spam-TU-Processing-Host: neelix X-UIDL: MbO"!Xd0!!pgh!!cm="! X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

ANNOUNCE: 03/06/29 Release of RADBIB and GITHESIS

RADBIB is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. It currently includes 2,276 references -- 16 new additions since its 03/05/25 release.

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http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 295 references to radiosity and global illumination theses -- one new addition since the 03/05/25 release.

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

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From Return-Path: Received: from neelix.kom.tuwien.ac.at (neelix.kom.tuwien.ac.at [192.35.241.67]) by mail.cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.4) with ESMTP id h7P6Ww3Z020621; Mon, 25 Aug 2003 08:32:58 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by neelix.kom.tuwien.ac.at (8.12.8/8.12.8) with ESMTP id h7P6dUaM008904; Mon, 25 Aug 2003 08:39:30 +0200 (MEST) X-Connecting-Host: imag.imag.fr [129.88.30.1] X-Connecting-Addr: 129.88.30.1 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by imag.imag.fr (8.12.9/8.12.9) with ESMTP id h7P6VPRb018227; Mon, 25 Aug 2003 08:31:25 +0200 (CEST) Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h7P6UsW19779; Mon, 25 Aug 2003 08:30:54 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h7P6J6H18112 for ; Mon, 25 Aug 2003 08:19:06 +0200 Received: from pd6mo3so.prod.shaw.ca (shawidc-mo1.cg.shawcable.net [24.71.223.10]) by imag.imag.fr (8.12.9/8.12.9) with ESMTP id h7P6IwRb016216 for ; Mon, 25 Aug 2003 08:18:58 +0200 (CEST) Received: from pd3mr3so.prod.shaw.ca (pd3mr3so-ser.prod.shaw.ca [10.0.141.179]) by l-daemon (iPlanet Messaging Server 5.2 HotFix 1.16 (built May 14 2003)) with ESMTP id <0HK500K73W7LHQ@l-daemon> for globillum@imag.fr; Mon, 25 Aug 2003 00:18:57 -0600 (MDT) Received: from pn2ml3so.prod.shaw.ca (pn2ml3so-qfe0.prod.shaw.ca [10.0.121.147]) by l-daemon (iPlanet Messaging Server 5.2 HotFix 1.16 (built May 14 2003)) with ESMTP id <0HK5006DMW7L94@l-daemon> for globillum@imag.fr; Mon, 25 Aug 2003 00:18:57 -0600 (MDT) Received: from FEBRUARY (h24-87-171-230.vn.shawcable.net [24.87.171.230]) by l-daemon (iPlanet Messaging Server 5.2 HotFix 1.16 (built May 14 2003)) with SMTP id <0HK500IBVW7JC5@l-daemon> for globillum@imag.fr; Mon, 25 Aug 2003 00:18:57 -0600 (MDT) Date: Sun, 24 Aug 2003 23:20:41 -0700 From: Ian Ashdown Subject: ANNOUNCE: 03/08/24 Release of RADBIB and GITHESIS To: globillum@imag.fr Reply-to: Ian Ashdown Message-id: <000a01c36ad1$02a1e7a0$6401a8c0@FEBRUARY> Organization: byHeart Consultants Limited MIME-version: 1.0 X-MIMEOLE: Produced By Microsoft MimeOLE V6.00.2800.1165 X-Mailer: Microsoft Outlook Express 6.00.2800.1158 Content-type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-priority: Normal X-MailScanner: Found to be clean, Found to be clean X-Loop: globillum@imag.fr X-Sequence: 198 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-MailScanner-Information: Please contact the ISP for more information X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; 2 X-Spam-Level: ++ X-Spam-TU-Processing-Host: neelix X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

ANNOUNCE: 03/08/24 Release of RADBIB and GITHESIS

RADBIB is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. It currently includes 2,289 references -- 13 new additions since its 03/06/29 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of August 24, 2003) from:

    http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 295 references to radiosity and global illumination theses -- no new additions since the 03/05/25 release.

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

Ian Ashdown, P. Eng., LC, FIES
President
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http://www.helios32.com

 

From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by mail.cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.4) with ESMTP id h8IE02EI031253; Thu, 18 Sep 2003 16:00:03 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by tuvok.kom.tuwien.ac.at (8.12.8/8.12.8) with ESMTP id h8IDxSma017302; Thu, 18 Sep 2003 15:59:28 +0200 (MEST) X-Connecting-Host: imag.imag.fr [129.88.30.1] X-Connecting-Addr: 129.88.30.1 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by imag.imag.fr (8.12.9/8.12.9) with ESMTP id h8IDxGii014679; Thu, 18 Sep 2003 15:59:16 +0200 (CEST) Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h8IDxFx30987; Thu, 18 Sep 2003 15:59:15 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h8IDthn30378 for ; Thu, 18 Sep 2003 15:55:43 +0200 Received: from nut.autodesk.com (nut.autodesk.com [198.102.112.27]) by imag.imag.fr (8.12.9/8.12.9) with ESMTP id h8IDteii013689 for ; Thu, 18 Sep 2003 15:55:40 +0200 (CEST) Received: from msgusawfe02.ads.autodesk.com ([144.111.33.211]) by nut.autodesk.com (8.12.9/8.12.6) with ESMTP id h8IDtbU8027363; Thu, 18 Sep 2003 06:55:38 -0700 (PDT) Received: from msgusaemb01.ads.autodesk.com ([144.111.72.50]) by msgusawfe02.ads.autodesk.com with Microsoft SMTPSVC(5.0.2195.5329); Thu, 18 Sep 2003 06:55:37 -0700 X-MimeOLE: Produced By Microsoft Exchange V6.0.6375.0 content-class: urn:content-classes:message MIME-Version: 1.0 Content-Type: text/html; charset=windows-1252 Subject: Random ray? Date: Thu, 18 Sep 2003 09:55:58 -0400 Message-ID: Thread-Topic: Random ray? Thread-Index: AcN97JYqTtStDQjWTqOOYx0OzrfxHA== From: "Eric Haines (Autodesk, NY)" To: globillum@imag.fr X-OriginalArrivalTime: 18 Sep 2003 13:55:37.0658 (UTC) FILETIME=[89F1B9A0:01C37DEC] X-IMAG-MailScanner: Found to be clean, Found to be clean X-Loop: globillum@imag.fr X-Sequence: 199 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; 7 X-Spam-Level: +++++++ X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

Globillumers,

 

What’s an efficient way to generate a random ray to hit an axis-aligned bounding box? I’m sure this has been done before, someone wrote it down somewhere, but I don’t know where…

 

Certainly, for a random ray direction I can use the method in:

 

    Arvo, James, Fast Random Rotation Matrices, Graphics Gems III, p. 117-120

 

The best method I can think of for generating the ray origin is to bound the box with a bounding sphere, generate a random direction and have this ray pass through the center of the sphere, then randomly move the origin to somewhere on the circle (of the sphere’s radius) perpendicular to this ray direction, finally moving this point along the ray back to the surface of the bounding sphere. Then test if this ray hits the bounding box; if not, start from scratch and generate a new direction & origin. I think this is unbiased: you’re always picking from a random direction, then choosing in an unbiased manner an origin from the circle that must enclose the projection of the box along the ray direction.

 

Is this reasonable? Is there something cleverer or more efficient? This looks fairly efficient for “squarish” boxes, but is pretty bad for, say, 10x1x1 dimension boxes.

 

Eric

From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by mail.cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.4) with ESMTP id h8IG76EI032391; Thu, 18 Sep 2003 18:07:06 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by tuvok.kom.tuwien.ac.at (8.12.8/8.12.8) with ESMTP id h8IG6xma025481; Thu, 18 Sep 2003 18:06:59 +0200 (MEST) X-Connecting-Host: imag.imag.fr [129.88.30.1] X-Connecting-Addr: 129.88.30.1 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by imag.imag.fr (8.12.9/8.12.9) with ESMTP id h8IG6uJI018172; Thu, 18 Sep 2003 18:06:56 +0200 (CEST) Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h8IG6u812393; Thu, 18 Sep 2003 18:06:56 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h8IG52n12340 for ; Thu, 18 Sep 2003 18:05:02 +0200 Received: from smtp803.mail.sc5.yahoo.com (smtp803.mail.sc5.yahoo.com [66.163.168.182]) by imag.imag.fr (8.12.9/8.12.9) with SMTP id h8IG4xJI017520 for ; Thu, 18 Sep 2003 18:05:00 +0200 (CEST) Received: from adsl-64-163-212-26.dsl.snfc21.pacbell.net (HELO lmi.net) (gregoryjward@64.163.212.26 with plain) by smtp-sbc-v1.mail.vip.sc5.yahoo.com with SMTP; 18 Sep 2003 16:04:58 -0000 Date: Thu, 18 Sep 2003 09:07:01 -0700 Subject: Re: Random ray? Mime-Version: 1.0 Cc: globillum@imag.fr To: "Eric Haines (Autodesk, NY)" From: Greg Ward In-Reply-To: Message-Id: <23683912-E9F2-11D7-AC35-000A956D40C8@lmi.net> X-Mailer: Apple Mail (2.552) X-IMAG-MailScanner: Found to be clean, Found to be clean X-MIME-Autoconverted: from quoted-printable to 8bit by chopinette.imag.fr id h8IG52n12340 X-Loop: globillum@imag.fr X-Sequence: 200 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -34 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hi Eric, As long as the object is reasonably distant from the ray origin, you can get close to an unbiased sampling by first picking which face to sample based on its projected area over the total projected area of the block, where the projected area of each face facing the ray is just the corresponding ray direction component times the normal face area. Once you have chosen a face, randomly distributing the ray destination within it should get you a good sample. I don't know how to solve the more general problem of completely unbiased sampling for an axis-aligned block at any distance, since nearby blocks become elongated in a projected view from the ray origin. The above will still work of course, but I think it will be slightly biased in its distribution. I take an even worse shortcut in Radiance, which is to randomly set the ray destination in the volume, which definitely biases the sample towards the object center. -Greg > From: "Eric Haines (Autodesk, NY)" > Date: Thu Sep 18, 2003 6:55:58 AM US/Pacific > > Globillumers, > > What’s an efficient way to generate a random ray to hit an > axis-aligned bounding box? I’m sure this has been done before, someone > wrote it down somewhere, but I don’t know where… > > Certainly, for a random ray direction I can use the method in: > >     Arvo, James, Fast Random Rotation Matrices, Graphics Gems III, p. > 117-120 > > The best method I can think of for generating the ray origin is to > bound the box with a bounding sphere, generate a random direction and > have this ray pass through the center of the sphere, then randomly > move the origin to somewhere on the circle (of the sphere’s radius) > perpendicular to this ray direction, finally moving this point along > the ray back to the surface of the bounding sphere. Then test if this > ray hits the bounding box; if not, start from scratch and generate a > new direction & origin. I think this is unbiased: you’re always > picking from a random direction, then choosing in an unbiased manner > an origin from the circle that must enclose the projection of the box > along the ray direction. > > Is this reasonable? Is there something cleverer or more efficient? > This looks fairly efficient for “squarish” boxes, but is pretty bad > for, say, 10x1x1 dimension boxes. ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by mail.cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.4) with ESMTP id h8J3IGEI007344; Fri, 19 Sep 2003 05:18:16 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by tuvok.kom.tuwien.ac.at (8.12.8/8.12.8) with ESMTP id h8J3IAma002096; Fri, 19 Sep 2003 05:18:11 +0200 (MEST) X-Connecting-Host: imag.imag.fr [129.88.30.1] X-Connecting-Addr: 129.88.30.1 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by imag.imag.fr (8.12.9/8.12.9) with ESMTP id h8J3HiJI006716; Fri, 19 Sep 2003 05:17:44 +0200 (CEST) Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h8J3HhJ17635; Fri, 19 Sep 2003 05:17:43 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h8IGsan17822 for ; Thu, 18 Sep 2003 18:54:36 +0200 Received: from mail-svr1.cs.utah.edu (mail-svr1.cs.utah.edu [155.99.198.200]) by imag.imag.fr (8.12.9/8.12.9) with ESMTP id h8IGsXJI028123 for ; Thu, 18 Sep 2003 18:54:34 +0200 (CEST) Received: from faith.cs.utah.edu (faith.cs.utah.edu [155.99.198.108]) by mail-svr1.cs.utah.edu (Postfix) with ESMTP id E6364346EE; Thu, 18 Sep 2003 10:54:30 -0600 (MDT) Received: by faith.cs.utah.edu (Postfix, from userid 2179) id E9EFB2EC1F; Thu, 18 Sep 2003 10:54:29 -0600 (MDT) Received: from localhost (localhost [127.0.0.1]) by faith.cs.utah.edu (Postfix) with ESMTP id 87CE434423; Thu, 18 Sep 2003 10:54:29 -0600 (MDT) Date: Thu, 18 Sep 2003 10:54:29 -0600 (MDT) From: Peter Shirley To: "Eric Haines (Autodesk, NY)" Cc: globillum@imag.fr Subject: Re: Random ray? In-Reply-To: Message-ID: References: MIME-Version: 1.0 X-IMAG-MailScanner: Found to be clean, Found to be clean X-Loop: globillum@imag.fr X-Sequence: 201 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -30 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hi Eric. I am pretty sure the following observations are true using geometric probability for justification (i.e., I read this once but don't have a strong argument, but I think there is one using measure theory that I don't remember!) * all points on the surface of a convex solid are equally likely to be hit by a random line * the angle of incidence of random lines near a point follow a cosine distribution with respect to the normal at that point. So I think the pseudocode is much as Greg suggests: 1. Choose a random face based on area 2. Choose a random point uniformly on that face 3. Choose a random direction with respect to normal N 3 is most easily done by constructing a UVW basis with W = N, and then choosing (u,v,w) as follows: phi = 2*pi*ra() // ra is random on [0,1), e.g., drand48() r = sqrt(ra()) u = r*cos(phi) v = r*sin(phi) w = sqrt(1-u*u-v*v) direction = u*U + v*V + w*W You could stratify in 4D for all this, but I think that would only start to pay off for billions of samples. Pete ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from neelix.kom.tuwien.ac.at (neelix.kom.tuwien.ac.at [192.35.241.67]) by mail.cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.4) with ESMTP id h8J3JZEI007354; Fri, 19 Sep 2003 05:19:35 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by neelix.kom.tuwien.ac.at (8.12.8/8.12.8) with ESMTP id h8J3JQtN011874; Fri, 19 Sep 2003 05:19:27 +0200 (MEST) X-Connecting-Host: imag.imag.fr [129.88.30.1] X-Connecting-Addr: 129.88.30.1 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by imag.imag.fr (8.12.9/8.12.9) with ESMTP id h8J3JNJI007295; Fri, 19 Sep 2003 05:19:23 +0200 (CEST) Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h8J3JNG18264; Fri, 19 Sep 2003 05:19:23 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h8IHBDn19397 for ; Thu, 18 Sep 2003 19:11:13 +0200 Received: from mut.autodesk.com (mut.autodesk.com [198.102.112.26]) by imag.imag.fr (8.12.9/8.12.9) with ESMTP id h8IHBBJI001142 for ; Thu, 18 Sep 2003 19:11:11 +0200 (CEST) Received: from msgusawfe01.ads.autodesk.com ([144.111.33.210]) by mut.autodesk.com (8.12.9/8.12.6) with ESMTP id h8IHB66R018886 for ; Thu, 18 Sep 2003 10:11:10 -0700 (PDT) Received: from msgusaemb01.ads.autodesk.com ([144.111.72.50]) by msgusawfe01.ads.autodesk.com with Microsoft SMTPSVC(5.0.2195.5329); Thu, 18 Sep 2003 10:11:29 -0700 X-MimeOLE: Produced By Microsoft Exchange V6.0.6375.0 content-class: urn:content-classes:message MIME-Version: 1.0 Content-Type: text/html; charset=windows-1252 Subject: FW: Random ray? Date: Thu, 18 Sep 2003 13:11:28 -0400 Message-ID: Thread-Topic: Random ray? Thread-Index: AcN99HzvFrWcJJIgS22kSEfoUnOGPQAEylkw From: "Eric Haines (Autodesk, NY)" To: globillum@imag.fr X-OriginalArrivalTime: 18 Sep 2003 17:11:29.0025 (UTC) FILETIME=[E64E0710:01C37E07] X-IMAG-MailScanner: Found to be clean, Found to be clean X-Loop: globillum@imag.fr X-Sequence: 202 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; 2 X-Spam-Level: ++ X-Spam-TU-Processing-Host: neelix X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

Thanks for all your responses, and I think we have consensus on the method Jim Arvo describes below (Pete Shirley and Bruce Walter also describe it, but Jim’s was the first I received and it’s a good presentation). I don’t think Jim’s response showed up on globillum for some reason, so I’m attaching it below.

 

Eric

 

-----Original Message-----
From: Jim Arvo [mailto:arvo@uci.edu]
Sent: September 18, 2003 10:52 AM
To: Eric Haines (Autodesk, NY); globillum@imag.fr
Cc: Jim Arvo
Subject: Re: Random ray?

 

Hi Eric,

 

    Here's what I would do.  If I'm understanding your question correctly,

this should be about the most efficient (and, I believe, unbiased) approach:

 

    1)  Randomly select a face F, with probability proportional to its area.

 

    2)  Uniformly sample F to obtain the ray origin P.

 

    3)  Sample the hemisphere above P (i.e. oriented using to F) according

         to a cosine distribution.  Equivalently, uniformly sample the unit disk

         about P and in the plane of F, and project up to the incoming

         hemisphere to get the point Q.  Set the ray direction to P - Q.

 

The resulting rays are guaranteed to hit the box (by construction), and are

uniformly distributed within that class of rays (I think).  The only part that may

seem counter-intuitive is the use of a cosine-weighted distribution for the

incoming hemisphere rather than a uniform distribution.  The reason for this

lies in the conditional probability of a ray's direction, given that it has hit a

specific face.  The direction will be biased toward normal incidence if the

rays were uniformly distributed (i.e. "fewer" rays hit the face with glancing

incidence).

 

Step #1 follows from the fact that the face should be chosen with a probability

proportional to its average projected area; but average projected area is

proportional to area (with a constant of proportionality of 1/2).

 

I've not checked this out formally, but I'm reasonably sure that it's correct.

 

-- Jim

 

----- Original Message -----

Sent: Thursday, September 18, 2003 6:55 AM

Subject: Random ray?

 

Globillumers,

 

What’s an efficient way to generate a random ray to hit an axis-aligned bounding box? I’m sure this has been done before, someone wrote it down somewhere, but I don’t know where…

 

Certainly, for a random ray direction I can use the method in:

 

    Arvo, James, Fast Random Rotation Matrices, Graphics Gems III, p. 117-120

 

The best method I can think of for generating the ray origin is to bound the box with a bounding sphere, generate a random direction and have this ray pass through the center of the sphere, then randomly move the origin to somewhere on the circle (of the sphere’s radius) perpendicular to this ray direction, finally moving this point along the ray back to the surface of the bounding sphere. Then test if this ray hits the bounding box; if not, start from scratch and generate a new direction & origin. I think this is unbiased: you’re always picking from a random direction, then choosing in an unbiased manner an origin from the circle that must enclose the projection of the box along the ray direction.

 

Is this reasonable? Is there something cleverer or more efficient? This looks fairly efficient for “squarish” boxes, but is pretty bad for, say, 10x1x1 dimension boxes.

 

Eric

From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by mail.cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.4) with ESMTP id h8J3j9EI007506; Fri, 19 Sep 2003 05:45:09 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by tuvok.kom.tuwien.ac.at (8.12.8/8.12.8) with ESMTP id h8J3j1ma008891; Fri, 19 Sep 2003 05:45:01 +0200 (MEST) X-Connecting-Host: imag.imag.fr [129.88.30.1] X-Connecting-Addr: 129.88.30.1 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by imag.imag.fr (8.12.9/8.12.9) with ESMTP id h8J3KmJI007728; Fri, 19 Sep 2003 05:20:48 +0200 (CEST) Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h8J3Kmu18390; Fri, 19 Sep 2003 05:20:48 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h8ILRRn13185 for ; Thu, 18 Sep 2003 23:27:27 +0200 Received: from orb.pobox.com (orb.pobox.com [216.65.124.72]) by imag.imag.fr (8.12.9/8.12.9) with ESMTP id h8ILRPJI013034 for ; Thu, 18 Sep 2003 23:27:25 +0200 (CEST) Received: from texas.pobox.com (texas.pobox.com[64.49.223.111]) by orb.pobox.com (Postfix) with ESMTP id 69D05156000; Thu, 18 Sep 2003 17:27:19 -0400 (EDT) Received: from BltMobile (dsl081-039-223.lax1.dsl.speakeasy.net [64.81.39.223]) by texas.pobox.com (Postfix) with ESMTP id 068FB45416; Thu, 18 Sep 2003 17:27:19 -0400 (EDT) Message-ID: <034801c37e2b$a3180620$7001a8c0@BltMobile> From: "Michael Herf" To: "Eric Haines (Autodesk, NY)" , "Greg Ward" Cc: globillum@imag.fr References: <23683912-E9F2-11D7-AC35-000A956D40C8@lmi.net> Subject: Re: Random ray? Date: Thu, 18 Sep 2003 14:27:17 -0700 MIME-Version: 1.0 X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 6.00.2800.1106 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1106 X-IMAG-MailScanner: Found to be clean, Found to be clean X-Loop: globillum@imag.fr X-Sequence: 203 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -18 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit I think you have to limit distance in the problem definition to make perspective matter at all -- if the ray origin is uniform over R^3 then it does just become an ortho projection in the average case (because the average ray tends towards infinity). If you're doing enclosed scenes, perspective matters, and if you're doing something like atmospheric lighting it probably doesn't. It seems like you care about it for this problem though. I like the parameterization of direction that Eric suggests, but it doesn't account for perspective as you move away from the bounding sphere (i.e. the perspective changes the distribution with distance to the center). If you simply choose a random distance, you've done it in a biased way, so I think you can inversely weight the distance by r^2 to account for this. So before you construct the circle you could just randomly move the ray origin away from the sphere origin by a random value inversely weighted by r^2. (And if you let r be unbounded, you just end up with all rays at infinity when you uniformly distribute, so you should pick a range first.) mike ----- Original Message ----- From: "Greg Ward" To: "Eric Haines (Autodesk, NY)" Cc: Sent: Thursday, September 18, 2003 9:07 AM Subject: Re: Random ray? > Hi Eric, > > As long as the object is reasonably distant from the ray origin, you > can get close to an unbiased sampling by first picking which face to > sample based on its projected area over the total projected area of the > block, where the projected area of each face facing the ray is just the > corresponding ray direction component times the normal face area. Once > you have chosen a face, randomly distributing the ray destination > within it should get you a good sample. > > I don't know how to solve the more general problem of completely > unbiased sampling for an axis-aligned block at any distance, since > nearby blocks become elongated in a projected view from the ray origin. > The above will still work of course, but I think it will be slightly > biased in its distribution. I take an even worse shortcut in Radiance, > which is to randomly set the ray destination in the volume, which > definitely biases the sample towards the object center. > > -Greg > > > From: "Eric Haines (Autodesk, NY)" > > Date: Thu Sep 18, 2003 6:55:58 AM US/Pacific > > > > Globillumers, > > > > What’s an efficient way to generate a random ray to hit an > > axis-aligned bounding box? I’m sure this has been done before, someone > > wrote it down somewhere, but I don’t know where… > > > > Certainly, for a random ray direction I can use the method in: > > > > Arvo, James, Fast Random Rotation Matrices, Graphics Gems III, p. > > 117-120 > > > > The best method I can think of for generating the ray origin is to > > bound the box with a bounding sphere, generate a random direction and > > have this ray pass through the center of the sphere, then randomly > > move the origin to somewhere on the circle (of the sphere’s radius) > > perpendicular to this ray direction, finally moving this point along > > the ray back to the surface of the bounding sphere. Then test if this > > ray hits the bounding box; if not, start from scratch and generate a > > new direction & origin. I think this is unbiased: you’re always > > picking from a random direction, then choosing in an unbiased manner > > an origin from the circle that must enclose the projection of the box > > along the ray direction. > > > > Is this reasonable? Is there something cleverer or more efficient? > > This looks fairly efficient for “squarish” boxes, but is pretty bad > > for, say, 10x1x1 dimension boxes. > > ---------------------------------------------------------------------------- ---- > ------------------------------------------------------------------------- > globillum@imag.fr -- mailing list devoted to global illumination research > For list archives or to configure your options, see http://listes.imag.fr > ------------------------------------------------------------------------- ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from neelix.kom.tuwien.ac.at (neelix.kom.tuwien.ac.at [192.35.241.67]) by mail.cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.4) with ESMTP id h8K3S0EI020947; Sat, 20 Sep 2003 05:28:00 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by neelix.kom.tuwien.ac.at (8.12.8/8.12.8) with ESMTP id h8K3RqtN014044; Sat, 20 Sep 2003 05:27:52 +0200 (MEST) X-Connecting-Host: imag.imag.fr [129.88.30.1] X-Connecting-Addr: 129.88.30.1 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id h8K3KCC3023244; Sat, 20 Sep 2003 05:20:12 +0200 (CEST) Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h8K3KBW06553; Sat, 20 Sep 2003 05:20:11 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h8JGhPn05259 for ; Fri, 19 Sep 2003 18:43:25 +0200 Received: from nut.autodesk.com (nut.autodesk.com [198.102.112.27]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id h8JGhIC3005831 for ; Fri, 19 Sep 2003 18:43:20 +0200 (CEST) Received: from msgusawfe01.ads.autodesk.com ([144.111.33.210]) by nut.autodesk.com (8.12.10/8.12.6) with ESMTP id h8JGhHNC012401 for ; Fri, 19 Sep 2003 09:43:17 -0700 (PDT) Received: from msgusaemb01.ads.autodesk.com ([144.111.72.50]) by msgusawfe01.ads.autodesk.com with Microsoft SMTPSVC(5.0.2195.5329); Fri, 19 Sep 2003 09:43:40 -0700 X-MimeOLE: Produced By Microsoft Exchange V6.0.6375.0 MIME-Version: 1.0 Subject: RE: Random ray? Date: Fri, 19 Sep 2003 12:43:39 -0400 Message-ID: Thread-Topic: Random ray? Thread-Index: AcN+OYwygp3CXnLBQXCjQ5nn5zt3xwAju/TQ From: "Eric Haines (Autodesk, NY)" To: globillum@imag.fr X-OriginalArrivalTime: 19 Sep 2003 16:43:40.0125 (UTC) FILETIME=[2DF9D8D0:01C37ECD] X-IMAG-MailScanner: Found to be clean, Found to be clean X-MIME-Autoconverted: from quoted-printable to 8bit by chopinette.imag.fr id h8JGhPn05259 X-Loop: globillum@imag.fr X-Sequence: 204 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; 0 X-Spam-TU-Processing-Host: neelix X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit content-class: urn:content-classes:message Content-Type: text/plain; charset="us-ascii" Content-Transfer-Encoding: 8bit Nelson, Michael, and Greg, Yes, I guess I wasn't entirely clear. I was looking for an unbiased and efficient method for getting random rays that hit a box, but without a fixed ray origin. Think "background radiation" instead of eye rays. Jim Arvo (and Pete Shirley and Bruce Walter) sent on an efficient way to solve this, so I'm happy. The "from a fixed view" question is an interesting one, though - you do have to correct for perspective distortion on the view plane, etc. I've received some great and educational responses, thanks everyone. However, I'm wondering if there's some anti-spam feature/bug with the globillum list. Did you all receive globillum emails from Michael Herf, Nelson Max, Peter Shirley, Fredo Durand, and Bruce Walter? If not, I'm guessing that if "cc:" is used to write to globillum, or perhaps if there are multiple "to:" addresses, it is not redistributed, at least from the way people are talking. True? Eric ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from neelix.kom.tuwien.ac.at (neelix.kom.tuwien.ac.at [192.35.241.67]) by mail.cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.4) with ESMTP id h8NMsCEI000629; Wed, 24 Sep 2003 00:54:13 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by neelix.kom.tuwien.ac.at (8.12.10/8.12.8) with ESMTP id h8NMroDJ011117; Wed, 24 Sep 2003 00:53:50 +0200 (MEST) X-Connecting-Host: imag.imag.fr [129.88.30.1] X-Connecting-Addr: 129.88.30.1 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id h8MH7MMX012731; Mon, 22 Sep 2003 19:07:23 +0200 (CEST) Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h8MH7M414615; Mon, 22 Sep 2003 19:07:22 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h8MH7Dn14598 for ; Mon, 22 Sep 2003 19:07:13 +0200 Received: from bach.graphics.cornell.edu (bach.graphics.cornell.edu [128.84.247.50]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id h8MH77MX012570 for ; Mon, 22 Sep 2003 19:07:07 +0200 (CEST) Received: from diesel.graphics.cornell.edu (diesel.graphics.cornell.edu [128.84.247.211]) by bach.graphics.cornell.edu (8.12.8p1/8.12.8) with ESMTP id h8MH74uX037262; Mon, 22 Sep 2003 13:07:05 -0400 (EDT) Date: Mon, 22 Sep 2003 13:07:04 -0400 (EDT) Message-Id: <200309221707.h8MH74uX037262@bach.graphics.cornell.edu> From: "Stephen H. Westin" To: eric.haines@autodesk.com CC: globillum@imag.fr In-reply-to: (eric.haines@autodesk.com) Subject: Re: Random ray? Reply-to: westin@graphics.cornell.edu References: X-IMAG-MailScanner: Found to be clean, Found to be clean X-Loop: globillum@imag.fr X-Sequence: 205 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; 4 X-Spam-Level: ++++ X-Spam-TU-Processing-Host: neelix X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 MIME-Version: 1.0 Content-transfer-encoding: 8bit This is a multi-part message in MIME format... ------------=_1064250438-13459-1 > Date: Thu, 18 Sep 2003 09:55:58 -0400 > From: "Eric Haines (Autodesk, NY)" > Globillumers, > > > > What's an efficient way to generate a random ray to hit an axis-aligned > bounding box? I'm sure this has been done before, someone wrote it down > somewhere, but I don't know where... > > > > Certainly, for a random ray direction I can use the method in: > > > > Arvo, James, Fast Random Rotation Matrices, Graphics Gems III, p. > 117-120 > > > > The best method I can think of for generating the ray origin is to bound > the box with a bounding sphere, generate a random direction and have > this ray pass through the center of the sphere, then randomly move the > origin to somewhere on the circle (of the sphere's radius) perpendicular > to this ray direction, finally moving this point along the ray back to > the surface of the bounding sphere. Then test if this ray hits the > bounding box; if not, start from scratch and generate a new direction & > origin. I think this is unbiased: you're always picking from a random > direction, then choosing in an unbiased manner an origin from the circle > that must enclose the projection of the box along the ray direction. Ugh. I wound up finding the (up to) three sides of the box that face toward the ray origin. I tesselate these with triangles, project them onto the unit sphere around the ray origin, and use Jim Arvo's method for randomly sampling spherical triangles (see his Web site) to get a random direction. As I recall, I computed the area of each spherical triangle to get the probability with which to select one. -Stephen H. Westin Any information or opinions in this message are mine: they do not represent the position of Cornell University or any of its sponsors. ------------=_1064250438-13459-1 Content-Type: text/plain; name="message.footer" Content-Disposition: inline; filename="message.footer" Content-Transfer-Encoding: 8bit ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- ------------=_1064250438-13459-1-- From Return-Path: Received: from neelix.kom.tuwien.ac.at (neelix.kom.tuwien.ac.at [192.35.241.67]) by mail.cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.4) with ESMTP id h8P3TMEI018978; Thu, 25 Sep 2003 05:29:22 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by neelix.kom.tuwien.ac.at (8.12.10/8.12.8) with ESMTP id h8P3TGDJ019915; Thu, 25 Sep 2003 05:29:17 +0200 (MEST) X-Connecting-Host: imag.imag.fr [129.88.30.1] X-Connecting-Addr: 129.88.30.1 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id h8P3JtVC005007; Thu, 25 Sep 2003 05:19:56 +0200 (CEST) Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h8P3JsV27450; Thu, 25 Sep 2003 05:19:54 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h8ONkCn04249 for ; Thu, 25 Sep 2003 01:46:12 +0200 Received: from graphics.csail.mit.edu (graphics.csail.mit.edu [18.24.2.30]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id h8ONk8VD004208 (version=TLSv1/SSLv3 cipher=EDH-RSA-DES-CBC3-SHA bits=168 verify=NO) for ; Thu, 25 Sep 2003 01:46:09 +0200 (CEST) Received: from graphics.lcs.mit.edu (etching.csail.mit.edu [18.24.2.47]) by graphics.csail.mit.edu (8.12.10/8.12.10) with ESMTP id h8ONk8CF031284 for ; Wed, 24 Sep 2003 19:46:08 -0400 Message-ID: <3F722CBF.1060408@graphics.lcs.mit.edu> Date: Wed, 24 Sep 2003 19:46:07 -0400 From: Fredo Durand User-Agent: Mozilla/5.0 (Windows; U; Windows NT 5.1; en-US; rv:1.4) Gecko/20030624 Netscape/7.1 (ax) X-Accept-Language: en-us, en MIME-Version: 1.0 To: "globillum@imag.fr" Subject: BRDF models in the real world X-IMAG-MailScanner: Found to be clean, Found to be clean X-Loop: globillum@imag.fr X-Sequence: 206 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; 2 X-Spam-Level: ++ X-Spam-TU-Processing-Host: neelix X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit A student and I are wondering about the BRDF models used in "real-world" applications. My usual claim is that everybody uses Phong. How true is that? In architecture lighting simulation? In production rendering? In games? It is probably not entirely true because Radiance like the Ward model a lot (I wonder why?-), and Maya proposes a weird anisotropic model. Thanks Fredo -- -- Fredo Durand, MIT-CSAIL Graphics Group 200 technology sq. NE43-254, Cambridge, MA 02139, USA phone : (617) 253 7223 fax : (617) 253 4640 http://graphics.lcs.mit.edu/~fredo/ ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from neelix.kom.tuwien.ac.at (neelix.kom.tuwien.ac.at [192.35.241.67]) by mail.cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.4) with ESMTP id h8SDdcEI025989; Sun, 28 Sep 2003 15:39:38 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by neelix.kom.tuwien.ac.at (8.12.10/8.12.8) with ESMTP id h8SDdUfC016159; Sun, 28 Sep 2003 15:39:31 +0200 (MEST) X-Connecting-Host: imag.imag.fr [129.88.30.1] X-Connecting-Addr: 129.88.30.1 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id h8SDdR42005061; Sun, 28 Sep 2003 15:39:27 +0200 (CEST) Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h8SDdQ423124; Sun, 28 Sep 2003 15:39:26 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h8SDdJn23107 for ; Sun, 28 Sep 2003 15:39:19 +0200 Received: from moutng.kundenserver.de (moutng.kundenserver.de [212.227.126.184]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id h8SDdG42005013 for ; Sun, 28 Sep 2003 15:39:16 +0200 (CEST) Received: from [212.227.126.162] (helo=mrelayng.kundenserver.de) by moutng.kundenserver.de with esmtp (Exim 3.35 #1) id 1A3bla-0006Lo-00; Sun, 28 Sep 2003 15:39:14 +0200 Received: from [217.80.183.214] (helo=cs.uni-sb.de) by mrelayng.kundenserver.de with asmtp (TLSv1:RC4-MD5:128) (Exim 3.35 #1) id 1A3bla-0000nX-00; Sun, 28 Sep 2003 15:39:14 +0200 Message-ID: <3F76E527.8030808@cs.uni-sb.de> Date: Sun, 28 Sep 2003 15:41:59 +0200 From: "Prof. Philipp Slusallek" Reply-To: slusallek@cs.uni-sb.de Organization: Saarland University, Computer Graphics Lab User-Agent: Mozilla/5.0 (X11; U; Linux i686; en-US; rv:1.4) Gecko/20030827 Debian/1.4-3 X-Accept-Language: en, de MIME-Version: 1.0 To: Fredo Durand CC: globillum@imag.fr Subject: Re: BRDF models in the real world References: <3F722CBF.1060408@graphics.lcs.mit.edu> In-Reply-To: <3F722CBF.1060408@graphics.lcs.mit.edu> X-IMAG-MailScanner: Found to be clean, Found to be clean X-Loop: globillum@imag.fr X-Sequence: 207 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; 7 X-Spam-Level: +++++++ X-Spam-TU-Processing-Host: neelix X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Dear Fredo, Fredo Durand wrote: > A student and I are wondering about the BRDF models used in "real-world" > applications. My usual claim is that everybody uses Phong. How true is > that? In architecture lighting simulation? In production rendering? In > games? > > It is probably not entirely true because Radiance like the Ward model a > lot (I wonder why?-), and Maya proposes a weird anisotropic model. We just started using measured BRDFs (from Bonn University, R. Klein) in our realtime ray tracer and presented it to Volkswagen last week. Real materials are a very hot topic in the automotive industry in order to be able use rendering as the basis for decisions instead of just as a source of (more or less) nice images. One simple example is car paint, which just looks awful and nothing like the real thing if you are using Phong. Philipp -- Prof. Dr.-Ing Philipp Slusallek, Computer Graphics Lab Universität des Saarlandes, FR 6.2 - Informatik, Im Stadtwald, Geb 36.1; 66123 Saarbrücken, Germany Tel: +49 681 302 3830, Fax: +49 681 302 3843, Email: slusallek@cs.uni-sb.de URL: http://graphics.cs.uni-sb.de ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by mail.cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.4) with ESMTP id h8SHEbEI026988; Sun, 28 Sep 2003 19:14:37 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by tuvok.kom.tuwien.ac.at (8.12.10/8.12.8) with ESMTP id h8SHEXuV022427; Sun, 28 Sep 2003 19:14:34 +0200 (MEST) X-Connecting-Host: imag.imag.fr [129.88.30.1] X-Connecting-Addr: 129.88.30.1 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id h8SHER42029090; Sun, 28 Sep 2003 19:14:27 +0200 (CEST) Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h8SHERK14601; Sun, 28 Sep 2003 19:14:27 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h8SHCwn14019 for ; Sun, 28 Sep 2003 19:12:58 +0200 Received: from mail.gmx.net (mail.gmx.de [213.165.64.20]) by imag.imag.fr (8.12.10/8.12.10) with SMTP id h8SHCv42028791 for ; Sun, 28 Sep 2003 19:12:57 +0200 (CEST) Received: (qmail 893 invoked by uid 65534); 28 Sep 2003 17:12:56 -0000 Received: from p5085665E.dip0.t-ipconnect.de (EHLO gmx.net) (80.133.102.94) by mail.gmx.net (mp001) with SMTP; 28 Sep 2003 19:12:56 +0200 X-Authenticated: #8703357 Message-ID: <3F771685.1060108@gmx.net> Date: Sun, 28 Sep 2003 19:12:37 +0200 From: Roland Schregle Organization: *Out Of Order* User-Agent: Mozilla/5.0 (X11; U; Linux i686; en-US; rv:1.3) Gecko/20030313 X-Accept-Language: en-us, en MIME-Version: 1.0 To: globillum@imag.fr Subject: Re: BRDF models in the real world References: <3F722CBF.1060408@graphics.lcs.mit.edu> <3F76E527.8030808@cs.uni-sb.de> In-Reply-To: <3F76E527.8030808@cs.uni-sb.de> X-IMAG-MailScanner: Found to be clean, Found to be clean X-Loop: globillum@imag.fr X-Sequence: 208 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -45 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Prof. Philipp Slusallek wrote: > Dear Fredo, > > Fredo Durand wrote: > >> A student and I are wondering about the BRDF models used in >> "real-world" applications. My usual claim is that everybody uses >> Phong. How true is that? In architecture lighting simulation? In >> production rendering? In games? As far as RealLife[tm] architectural applications are concerned, the Ward model implemented in the RADIANCE suite sees fairly widespread use, at least if lighting studies are involved rather than just pretty pictures which approximate what the finished building *might* will look like. >> It is probably not entirely true because Radiance like the Ward model >> a lot (I wonder why?-), and Maya proposes a weird anisotropic model. > > > We just started using measured BRDFs (from Bonn University, R. Klein) in > our realtime ray tracer and presented it to Volkswagen last week. Real > materials are a very hot topic in the automotive industry in order to be > able use rendering as the basis for decisions instead of just as a > source of (more or less) nice images. > > One simple example is car paint, which just looks awful and nothing like > the real thing if you are using Phong. Good point -- the Lafortune model comes to mind here. It's general enough to handle off-specularity and retroreflection, both of which are encountered when dealing with paints in general, particularly those used in automotive applications. It can also be fitted to measured data as Lafortune showed in his paper. Getting back to the original question, however, I'm not sure how widespread its use is in RealLife[tm] applications as opposed to research, where it tends to pop up more often. --Roland -- END OF LINE. (MCP) ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by mail.cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id h9CFUAl1012684; Sun, 12 Oct 2003 17:30:10 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by tuvok.kom.tuwien.ac.at (8.12.10/8.12.8) with ESMTP id h9CFTtxC003768; Sun, 12 Oct 2003 17:29:58 +0200 (MEST) X-Connecting-Host: imag.imag.fr [129.88.30.1] X-Connecting-Addr: 129.88.30.1 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id h9CFLfbR028650; Sun, 12 Oct 2003 17:21:41 +0200 (CEST) Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h9CFLe404601; Sun, 12 Oct 2003 17:21:40 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h9C6dvJ15302 for ; Sun, 12 Oct 2003 08:39:57 +0200 Received: from pd6mo1so.prod.shaw.ca (shawidc-mo1.cg.shawcable.net [24.71.223.10]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id h9C6dtbR000581 for ; Sun, 12 Oct 2003 08:39:55 +0200 (CEST) Received: from pd2mr1so.prod.shaw.ca (pd2mr1so-ser.prod.shaw.ca [10.0.141.110]) by l-daemon (iPlanet Messaging Server 5.2 HotFix 1.16 (built May 14 2003)) with ESMTP id <0HMM00BKCT6A6A@l-daemon> for globillum@imag.fr; Sun, 12 Oct 2003 00:39:46 -0600 (MDT) Received: from pn2ml6so.prod.shaw.ca (pn2ml6so-qfe0.prod.shaw.ca [10.0.121.150]) by l-daemon (iPlanet Messaging Server 5.2 HotFix 1.16 (built May 14 2003)) with ESMTP id <0HMM00GDAT6AQV@l-daemon> for globillum@imag.fr; Sun, 12 Oct 2003 00:39:46 -0600 (MDT) Received: from FEBRUARY (h24-87-171-230.vn.shawcable.net [24.87.171.230]) by l-daemon (iPlanet Messaging Server 5.2 HotFix 1.16 (built May 14 2003)) with SMTP id <0HMM00LPFT68VN@l-daemon> for globillum@imag.fr; Sun, 12 Oct 2003 00:39:46 -0600 (MDT) Date: Sat, 11 Oct 2003 23:37:55 -0700 From: Ian Ashdown Subject: ANNOUNCE: 03/10/11 Release of RADBIB and GITHESIS To: globillum@imag.fr Reply-to: Ian Ashdown Message-id: <001901c3908b$5e95df00$6401a8c0@FEBRUARY> Organization: byHeart Consultants Limited MIME-version: 1.0 X-MIMEOLE: Produced By Microsoft MimeOLE V6.00.2800.1165 X-Mailer: Microsoft Outlook Express 6.00.2800.1158 Content-type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-priority: Normal X-IMAG-MailScanner: Found to be clean, Found to be clean X-Loop: globillum@imag.fr X-Sequence: 210 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; 15 X-Spam-Level: *+++++ X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

ANNOUNCE: 03/10/11 Release of RADBIB and GITHESIS

RADBIB is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. It currently includes 2,322 references -- 33 new additions since its 03/08/24 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of October 11, 2003) from:

    http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 303 references to radiosity and global illumination theses -- 8 new additions since the 03/08/24 release.

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

Ian Ashdown, P. Eng., LC, FIES
President
byHeart Consultants Limited
http://www.helios32.com

From Return-Path: Received: from neelix.kom.tuwien.ac.at (neelix.kom.tuwien.ac.at [192.35.241.67]) by mail.cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id h9G3tIl1030206; Thu, 16 Oct 2003 05:55:18 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by neelix.kom.tuwien.ac.at (8.12.10/8.12.8) with ESMTP id h9G3t3G8018148; Thu, 16 Oct 2003 05:55:06 +0200 (MEST) X-Connecting-Host: imag.imag.fr [129.88.30.1] X-Connecting-Addr: 129.88.30.1 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id h9G3qckn005578; Thu, 16 Oct 2003 05:52:38 +0200 (CEST) Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h9G3qcB18029; Thu, 16 Oct 2003 05:52:38 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h9G3qWJ18010 for ; Thu, 16 Oct 2003 05:52:32 +0200 Received: from ns.csis.hku.hk (ns.csis.hku.hk [147.8.178.10]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id h9G3qTkn005510 for ; Thu, 16 Oct 2003 05:52:30 +0200 (CEST) Received: from study.csis.hku.hk (study [147.8.178.15]) by ns.csis.hku.hk (8.12.10+Sun/8.12.9) with ESMTP id h9G3qPcJ022421; Thu, 16 Oct 2003 11:52:25 +0800 (HKT) Received: from csis.hku.hk (jcfhopc [147.8.177.161]) by study.csis.hku.hk (8.11.7p1+Sun/8.11.6) with ESMTP id h9G3qOY21873; Thu, 16 Oct 2003 11:52:24 +0800 (CST) Message-ID: <3F8E15FA.5090003@csis.hku.hk> Date: Thu, 16 Oct 2003 11:52:26 +0800 From: "Jeffrey C. F. Ho" User-Agent: Mozilla/5.0 (Windows; U; Windows NT 5.1; en-US; rv:1.0.1) Gecko/20020823 Netscape/7.0 X-Accept-Language: en-us, en MIME-Version: 1.0 To: globillum@imag.fr Subject: How to test a graphics program? X-IMAG-MailScanner: Found to be clean, Found to be clean X-Loop: globillum@imag.fr X-Sequence: 212 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -26 X-Spam-Level: - X-Spam-TU-Processing-Host: neelix X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hi all, I am a MPhil student in Hong Kong. My research work is about software testing on graphics software. Can anyone give me idea about currently how people do software testing on graphics software? namely, how to verify that a graphics program is implmenting the mathematical model that simulates the realworld lighting phenomena?? by human vision? any systematic ways? Cheers, Jeffrey ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by mail.cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id h9GCTZl1001843; Thu, 16 Oct 2003 14:29:35 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by tuvok.kom.tuwien.ac.at (8.12.10/8.12.8) with ESMTP id h9GCTPxC019989; Thu, 16 Oct 2003 14:29:25 +0200 (MEST) X-Connecting-Host: imag.imag.fr [129.88.30.1] X-Connecting-Addr: 129.88.30.1 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id h9GCLZEk024409; Thu, 16 Oct 2003 14:21:36 +0200 (CEST) Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h9GCLZj11545; Thu, 16 Oct 2003 14:21:35 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h9GCLRJ11527 for ; Thu, 16 Oct 2003 14:21:27 +0200 Received: from mail.gmx.net (pop.gmx.de [213.165.64.20]) by imag.imag.fr (8.12.10/8.12.10) with SMTP id h9GCLOEk024330 for ; Thu, 16 Oct 2003 14:21:25 +0200 (CEST) Received: (qmail 20991 invoked by uid 65534); 16 Oct 2003 12:21:24 -0000 Received: from p5085696B.dip0.t-ipconnect.de (EHLO gmx.net) (80.133.105.107) by mail.gmx.net (mp009) with SMTP; 16 Oct 2003 14:21:24 +0200 X-Authenticated: #8703357 Message-ID: <3F8E8D04.6020005@gmx.net> Date: Thu, 16 Oct 2003 14:20:20 +0200 From: Roland Schregle Organization: *Out Of Order* User-Agent: Mozilla/5.0 (X11; U; Linux i686; en-US; rv:1.3) Gecko/20030313 X-Accept-Language: en-us, en MIME-Version: 1.0 CC: globillum@imag.fr Subject: Re: How to test a graphics program? References: <3F8E15FA.5090003@csis.hku.hk> In-Reply-To: <3F8E15FA.5090003@csis.hku.hk> X-IMAG-MailScanner: Found to be clean, Found to be clean X-Loop: globillum@imag.fr X-Sequence: 214 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -24 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Jeffrey C. F. Ho wrote: > Hi all, > > I am a MPhil student in Hong Kong. My research work is about software > testing on graphics software. > Can anyone give me idea about currently how people do software testing > on graphics software? > namely, how to verify that a graphics program is implmenting the > mathematical model that simulates the realworld lighting phenomena?? by > human vision? any systematic ways? Hi Jeff, I guess your options for validating a CG algorithm depend on whether your application requires quantitative or qualitative analysis. In the former case you can compare radiometric or photometric reference quantities with your simulation. In the latter, you can probably do with vision-based comparisons, although these can of course be subjective. I did a photon map validation as part of my PhD thesis based on quantitative analysis. The references for comparison can be either from analytic solutions (using very simple geometries and therefore limited in scope), or measurements from a physical model. My thesis covers both, and the physical validation was no fun. These can be highly complex and a systematic methodology is essential, even for the simple model we used. In particular, you must account for error margins inherent in the measurements; the material BRDFs are a major contributor here (we used goniometric measurements of material samples). Alas, the thesis is still in the works... :^) Regards, --Roland -- END OF LINE. (MCP) ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by mail.cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id h9GE9Nl1002776; Thu, 16 Oct 2003 16:09:23 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by tuvok.kom.tuwien.ac.at (8.12.10/8.12.8) with ESMTP id h9GE93xC017897; Thu, 16 Oct 2003 16:09:06 +0200 (MEST) X-Connecting-Host: imag.imag.fr [129.88.30.1] X-Connecting-Addr: 129.88.30.1 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id h9GE12HT022423; Thu, 16 Oct 2003 16:01:02 +0200 (CEST) Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h9GE11423036; Thu, 16 Oct 2003 16:01:01 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h9GE0tJ23017 for ; Thu, 16 Oct 2003 16:00:55 +0200 Received: from dire.bris.ac.uk (dire.bris.ac.uk [137.222.10.60]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id h9GE0pHT022320 for ; Thu, 16 Oct 2003 16:00:51 +0200 (CEST) Received: from cs.bris.ac.uk (actually host lunaleka.cs.bris.ac.uk) by dire.bris.ac.uk with SMTP-PRIV with ESMTP; Thu, 16 Oct 2003 15:00:05 +0100 Received: from voodoo.cs.bris.ac.uk (voodoo [137.222.102.33]) by cs.bris.ac.uk (8.9.3/8.9.3) with ESMTP id OAA26967; Thu, 16 Oct 2003 14:58:20 +0100 (BST) Received: from localhost by voodoo.cs.bris.ac.uk (8.9.3p2) id OAA16101; Thu, 16 Oct 2003 14:58:19 +0100 (BST) Date: Thu, 16 Oct 2003 14:58:18 +0100 (BST) From: Alan Chalmers X-Sender: alan@voodoo To: "Jeffrey C. F. Ho" cc: globillum@imag.fr Subject: Re: How to test a graphics program? In-Reply-To: <3F8E15FA.5090003@csis.hku.hk> Message-ID: MIME-Version: 1.0 X-IMAG-MailScanner: Found to be clean, Found to be clean X-Loop: globillum@imag.fr X-Sequence: 215 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -39 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hi Jeffrey We had two courses at SIGGRAPH looking at Image Quality Metrics including computational measures using computer models of the human visual system (eg VDP) and psychophysical methods - such as lightness - where users did the comparisons between the real and virtual scene. Chalmers A.G., McNamara A., Daly S., Myszkowski K., Rushmeier H., Troscianko T. "Seeing is Believing: Reality Perception in Modeling, Rendering and Animation", SIGGRAPH 2001 Course, 21, 180 pages, ACM SIGGRAPH, August 2001. Chalmers A.G., McNamara A., Daly S., Myszkowski K., Troscianko T. "Image Quality Metrics", SIGGRAPH 2000 Course, 44, 117 pages, ACM SIGGRAPH, July 2000. These courses will be available on the appropriate SIGGRAPH course CDs. I hope this helps! Best wishes Alan On Thu, 16 Oct 2003, Jeffrey C. F. Ho wrote: > Hi all, > > I am a MPhil student in Hong Kong. My research work is about software > testing on graphics software. > Can anyone give me idea about currently how people do software testing > on graphics software? > namely, how to verify that a graphics program is implmenting the > mathematical model that simulates the realworld lighting phenomena?? by > human vision? any systematic ways? > > Cheers, > Jeffrey > > ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from neelix.kom.tuwien.ac.at (neelix.kom.tuwien.ac.at [192.35.241.67]) by mail.cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id h9GGd7l1004013; Thu, 16 Oct 2003 18:39:07 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by neelix.kom.tuwien.ac.at (8.12.10/8.12.8) with ESMTP id h9GGcnG8020520; Thu, 16 Oct 2003 18:38:52 +0200 (MEST) X-Connecting-Host: imag.imag.fr [129.88.30.1] X-Connecting-Addr: 129.88.30.1 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id h9GGDwJ4028183; Thu, 16 Oct 2003 18:13:58 +0200 (CEST) Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h9GGDvF06765; Thu, 16 Oct 2003 18:13:57 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h9GGDmJ06748 for ; Thu, 16 Oct 2003 18:13:48 +0200 Received: from ns.csis.hku.hk (ns.csis.hku.hk [147.8.178.10]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id h9GGDiJ4028083 for ; Thu, 16 Oct 2003 18:13:45 +0200 (CEST) Received: from intranet.csis.hku.hk (intranet.csis.hku.hk [147.8.175.20]) by ns.csis.hku.hk (8.12.10+Sun/8.12.9) with ESMTP id h9GGDgcJ029418 for ; Fri, 17 Oct 2003 00:13:43 +0800 (HKT) Received: from intranet.csis.hku.hk (localhost [127.0.0.1]) by intranet.csis.hku.hk (8.12.9+Sun/8.12.9) with ESMTP id h9GGDg4t027029 for ; Fri, 17 Oct 2003 00:13:42 +0800 (HKT) Received: (from info@localhost) by intranet.csis.hku.hk (8.12.9+Sun/8.12.2/Submit) id h9GGDfaa027028 for globillum@imag.fr; Fri, 17 Oct 2003 00:13:41 +0800 (HKT) X-Authentication-Warning: intranet.csis.hku.hk: info set sender to jcfho@csis.hku.hk using -f Received: from 218.254.69.232 ( [218.254.69.232]) as user jcfho@study.csis.hku.hk by intranet.csis.hku.hk with HTTP; Fri, 17 Oct 2003 00:13:41 +0800 Message-ID: <1066320821.3f8ec3b56ff5d@intranet.csis.hku.hk> Date: Fri, 17 Oct 2003 00:13:41 +0800 From: jcfho@csis.hku.hk To: globillum@imag.fr Subject: How to test a graphics program? (2) MIME-Version: 1.0 User-Agent: Internet Messaging Program (IMP) 3.1 X-Originating-IP: 218.254.69.232 X-IMAG-MailScanner: Found to be clean, Found to be clean X-Loop: globillum@imag.fr X-Sequence: 216 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -6 X-Spam-Level: - X-Spam-TU-Processing-Host: neelix X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hi everybody, Thank you very much! What you guys gave are very interesting. One question, how people know that there is defect/bug in a graphics program? People checks the output image with human vision? That would require much experience to find non-trival problems. How do currently people do? any systematic ways or even automatic ways? Regards, Jeff ------------------------------------------------- This mail sent through IMP: http://horde.org/imp/ ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from neelix.kom.tuwien.ac.at (neelix.kom.tuwien.ac.at [192.35.241.67]) by mail.cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id h9GGQil1003916; Thu, 16 Oct 2003 18:26:44 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by neelix.kom.tuwien.ac.at (8.12.10/8.12.8) with ESMTP id h9GGQUG8016901; Thu, 16 Oct 2003 18:26:32 +0200 (MEST) X-Connecting-Host: imag.imag.fr [129.88.30.1] X-Connecting-Addr: 129.88.30.1 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id h9GGMIJ4000570; Thu, 16 Oct 2003 18:22:18 +0200 (CEST) Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h9GGMIq07994; Thu, 16 Oct 2003 18:22:18 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h9GGMDJ07977 for ; Thu, 16 Oct 2003 18:22:13 +0200 Received: from dire.bris.ac.uk (dire.bris.ac.uk [137.222.10.60]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id h9GGM9J4000497 for ; Thu, 16 Oct 2003 18:22:09 +0200 (CEST) Received: from cs.bris.ac.uk (actually host lunaleka.cs.bris.ac.uk) by dire.bris.ac.uk with SMTP-PRIV with ESMTP; Thu, 16 Oct 2003 17:22:02 +0100 Received: from voodoo.cs.bris.ac.uk (voodoo [137.222.102.33]) by cs.bris.ac.uk (8.9.3/8.9.3) with ESMTP id RAA05025; Thu, 16 Oct 2003 17:20:53 +0100 (BST) Received: from localhost by voodoo.cs.bris.ac.uk (8.9.3p2) id RAA27666; Thu, 16 Oct 2003 17:20:52 +0100 (BST) Date: Thu, 16 Oct 2003 17:20:52 +0100 (BST) From: Alan Chalmers X-Sender: alan@voodoo To: jcfho@csis.hku.hk cc: globillum@imag.fr Subject: Re: How to test a graphics program? (2) In-Reply-To: <1066320821.3f8ec3b56ff5d@intranet.csis.hku.hk> Message-ID: MIME-Version: 1.0 X-IMAG-MailScanner: Found to be clean, Found to be clean X-Loop: globillum@imag.fr X-Sequence: 217 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -60 X-Spam-Level: - X-Spam-TU-Processing-Host: neelix X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hi Jeff I guess it all depends on just how perceptually important the bug is ... if the human visual system can't see it then ... for some applications ... who cares! Another way of comparison would be detailed physical measurements with, eg a chromameter. Cheers Alan On Fri, 17 Oct 2003 jcfho@csis.hku.hk wrote: > Hi everybody, > > Thank you very much! What you guys gave are very interesting. > > One question, how people know that there is defect/bug in a graphics program? > People checks the output image with human vision? That would require much > experience to find non-trival problems. How do currently people do? any > systematic ways or even automatic ways? > > Regards, > Jeff > > > > ------------------------------------------------- > This mail sent through IMP: http://horde.org/imp/ > ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from neelix.kom.tuwien.ac.at (neelix.kom.tuwien.ac.at [192.35.241.67]) by mail.cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id h9GGZWl1003990; Thu, 16 Oct 2003 18:35:32 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by neelix.kom.tuwien.ac.at (8.12.10/8.12.8) with ESMTP id h9GGZKG8019334; Thu, 16 Oct 2003 18:35:20 +0200 (MEST) X-Connecting-Host: imag.imag.fr [129.88.30.1] X-Connecting-Addr: 129.88.30.1 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id h9GGYQJ4003671; Thu, 16 Oct 2003 18:34:26 +0200 (CEST) Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h9GGYPA09328; Thu, 16 Oct 2003 18:34:25 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h9GGWwJ09291 for ; Thu, 16 Oct 2003 18:32:58 +0200 Received: from pd3mo2so.prod.shaw.ca (shawidc-mo1.cg.shawcable.net [24.71.223.10]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id h9GGWuJ4003215 for ; Thu, 16 Oct 2003 18:32:57 +0200 (CEST) Received: from pd3mr3so.prod.shaw.ca (pd3mr3so-ser.prod.shaw.ca [10.0.141.179]) by l-daemon (iPlanet Messaging Server 5.2 HotFix 1.16 (built May 14 2003)) with ESMTP id <0HMU0025RZAVXG@l-daemon> for globillum@imag.fr; Thu, 16 Oct 2003 10:32:55 -0600 (MDT) Received: from pn2ml4so.prod.shaw.ca (pn2ml4so-qfe0.prod.shaw.ca [10.0.121.148]) by l-daemon (iPlanet Messaging Server 5.2 HotFix 1.16 (built May 14 2003)) with ESMTP id <0HMU006HLZAVGB@l-daemon> for globillum@imag.fr; Thu, 16 Oct 2003 10:32:55 -0600 (MDT) Received: from FEBRUARY (h24-87-171-230.vn.shawcable.net [24.87.171.230]) by l-daemon (iPlanet Messaging Server 5.2 HotFix 1.16 (built May 14 2003)) with SMTP id <0HMU00CS9ZATN1@l-daemon> for globillum@imag.fr; Thu, 16 Oct 2003 10:32:55 -0600 (MDT) Date: Thu, 16 Oct 2003 09:31:14 -0700 From: Ian Ashdown Subject: Re: How to test a graphics program? (2) To: jcfho@csis.hku.hk, globillum@imag.fr Reply-to: Ian Ashdown Message-id: <004e01c39402$eafcfe40$6401a8c0@FEBRUARY> Organization: byHeart Consultants Limited MIME-version: 1.0 X-MIMEOLE: Produced By Microsoft MimeOLE V6.00.2800.1165 X-Mailer: Microsoft Outlook Express 6.00.2800.1158 X-Priority: 3 X-MSMail-priority: Normal References: <1066320821.3f8ec3b56ff5d@intranet.csis.hku.hk> X-IMAG-MailScanner: Found to be clean, Found to be clean X-Loop: globillum@imag.fr X-Sequence: 218 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -13 X-Spam-Level: - X-Spam-TU-Processing-Host: neelix X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit > Thank you very much! What you guys gave are very interesting. > > One question, how people know that there is defect/bug in a graphics program? > People checks the output image with human vision? That would require much > experience to find non-trival problems. How do currently people do? any > systematic ways or even automatic ways? > > Regards, > Jeff > It is not a question of whether a computer graphics program is provably correct. Whether you are interested in physical (i.e., spectroradiometric) qunatities or photometric (i.e., photometric and colorimetric) quantities, ALL computer graphics programs necessarily provide gross approximations of the "real world." The computer graphics research community has been addressing these issues for the past twenty years, and similar work has been done by the illumination engineering / lighting design and vision research communities. There is a large body of academic literature scattered over many journals, conference proceedings, and theses. A good introduction to this literature is the SIGGRAPH 2001 course suggested by Alan Chalmers. This will help you refine your question in terms of what is possible rather than what approaches global illumination researchers are currently taking. Ian Ashdown, P. Eng., LC, FIES President byHeart Consultants Limited http://www.helios32.com ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from neelix.kom.tuwien.ac.at (neelix.kom.tuwien.ac.at [192.35.241.67]) by mail.cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id h9GH3tl1004183; Thu, 16 Oct 2003 19:03:55 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by neelix.kom.tuwien.ac.at (8.12.10/8.12.8) with ESMTP id h9GH3cG8027298; Thu, 16 Oct 2003 19:03:41 +0200 (MEST) X-Connecting-Host: imag.imag.fr [129.88.30.1] X-Connecting-Addr: 129.88.30.1 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id h9GGq3J4007895; Thu, 16 Oct 2003 18:52:03 +0200 (CEST) Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h9GGq3k11690; Thu, 16 Oct 2003 18:52:03 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h9GGoWJ11094 for ; Thu, 16 Oct 2003 18:50:32 +0200 Received: from ns.csis.hku.hk (ns.csis.hku.hk [147.8.178.10]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id h9GGoTJ4007448 for ; Thu, 16 Oct 2003 18:50:30 +0200 (CEST) Received: from intranet.csis.hku.hk (intranet.csis.hku.hk [147.8.175.20]) by ns.csis.hku.hk (8.12.10+Sun/8.12.9) with ESMTP id h9GGoNcJ000948; Fri, 17 Oct 2003 00:50:23 +0800 (HKT) Received: from intranet.csis.hku.hk (localhost [127.0.0.1]) by intranet.csis.hku.hk (8.12.9+Sun/8.12.9) with ESMTP id h9GGoN4t002964; Fri, 17 Oct 2003 00:50:23 +0800 (HKT) Received: (from info@localhost) by intranet.csis.hku.hk (8.12.9+Sun/8.12.2/Submit) id h9GGoNVJ002963; Fri, 17 Oct 2003 00:50:23 +0800 (HKT) X-Authentication-Warning: intranet.csis.hku.hk: info set sender to jcfho@csis.hku.hk using -f Received: from 218.254.69.232 ( [218.254.69.232]) as user jcfho@study.csis.hku.hk by intranet.csis.hku.hk with HTTP; Fri, 17 Oct 2003 00:50:22 +0800 Message-ID: <1066323022.3f8ecc4ed96fe@intranet.csis.hku.hk> Date: Fri, 17 Oct 2003 00:50:22 +0800 From: jcfho@csis.hku.hk To: Ian Ashdown Cc: globillum@imag.fr Subject: Re: How to test a graphics program? (2) References: <1066320821.3f8ec3b56ff5d@intranet.csis.hku.hk> <004e01c39402$eafcfe40$6401a8c0@FEBRUARY> In-Reply-To: <004e01c39402$eafcfe40$6401a8c0@FEBRUARY> MIME-Version: 1.0 User-Agent: Internet Messaging Program (IMP) 3.1 X-Originating-IP: 218.254.69.232 X-IMAG-MailScanner: Found to be clean, Found to be clean X-Loop: globillum@imag.fr X-Sequence: 219 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -31 X-Spam-Level: - X-Spam-TU-Processing-Host: neelix X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hi, 1. "Mathematical model approximates the real world." 2. "Graphics Program implments the mathematical model." What I am trying to focus is checking no. 2. The graphics program gives output with many values, say a matrix of 640x480 (the image). How the developer verify that every pixel is correctly rendered according to the mathematical model? Regards, Jeff Quoting Ian Ashdown : > > Thank you very much! What you guys gave are very interesting. > > > > One question, how people know that there is defect/bug in a graphics > program? > > People checks the output image with human vision? That would require much > > experience to find non-trival problems. How do currently people do? any > > systematic ways or even automatic ways? > > > > Regards, > > Jeff > > > It is not a question of whether a computer graphics program is provably > correct. Whether you are interested in physical (i.e., spectroradiometric) > qunatities or photometric (i.e., photometric and colorimetric) quantities, > ALL computer graphics programs necessarily provide gross approximations of > the "real world." > > The computer graphics research community has been addressing these issues > for the past twenty years, and similar work has been done by the > illumination engineering / lighting design and vision research communities. > There is a large body of academic literature scattered over many journals, > conference proceedings, and theses. > > A good introduction to this literature is the SIGGRAPH 2001 course suggested > by Alan Chalmers. This will help you refine your question in terms of what > is possible rather than what approaches global illumination researchers are > currently taking. > > Ian Ashdown, P. Eng., LC, FIES > President > byHeart Consultants Limited > http://www.helios32.com > > > ------------------------------------------------- This mail sent through IMP: http://horde.org/imp/ ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from neelix.kom.tuwien.ac.at (neelix.kom.tuwien.ac.at [192.35.241.67]) by mail.cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id h9GHkMl1004500; Thu, 16 Oct 2003 19:46:22 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by neelix.kom.tuwien.ac.at (8.12.10/8.12.8) with ESMTP id h9GHk7G8008514; Thu, 16 Oct 2003 19:46:10 +0200 (MEST) X-Connecting-Host: imag.imag.fr [129.88.30.1] X-Connecting-Addr: 129.88.30.1 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id h9GHZjJ4017165; Thu, 16 Oct 2003 19:35:45 +0200 (CEST) Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h9GHZjv16375; Thu, 16 Oct 2003 19:35:45 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h9GHYGJ16324 for ; Thu, 16 Oct 2003 19:34:16 +0200 Received: from pd3mo2so.prod.shaw.ca (shawidc-mo1.cg.shawcable.net [24.71.223.10]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id h9GHYBJ4016821 for ; Thu, 16 Oct 2003 19:34:12 +0200 (CEST) Received: from pd5mr3so.prod.shaw.ca (pd5mr3so-qfe3.prod.shaw.ca [10.0.141.144]) by l-daemon (iPlanet Messaging Server 5.2 HotFix 1.16 (built May 14 2003)) with ESMTP id <0HMV00I3S24MIA@l-daemon> for globillum@imag.fr; Thu, 16 Oct 2003 11:33:58 -0600 (MDT) Received: from pn2ml8so.prod.shaw.ca (pn2ml8so-qfe0.prod.shaw.ca [10.0.121.152]) by l-daemon (iPlanet Messaging Server 5.2 HotFix 1.16 (built May 14 2003)) with ESMTP id <0HMV00MMG24MV2@l-daemon> for globillum@imag.fr; Thu, 16 Oct 2003 11:33:58 -0600 (MDT) Received: from FEBRUARY (h24-87-171-230.vn.shawcable.net [24.87.171.230]) by l-daemon (iPlanet Messaging Server 5.2 HotFix 1.16 (built May 14 2003)) with SMTP id <0HMV0026124J38@l-daemon> for globillum@imag.fr; Thu, 16 Oct 2003 11:33:58 -0600 (MDT) Date: Thu, 16 Oct 2003 10:32:16 -0700 From: Ian Ashdown Subject: Re: How to test a graphics program? (2) To: jcfho@csis.hku.hk Cc: globillum@imag.fr Reply-to: Ian Ashdown Message-id: <00a101c3940b$7188fce0$6401a8c0@FEBRUARY> Organization: byHeart Consultants Limited MIME-version: 1.0 X-MIMEOLE: Produced By Microsoft MimeOLE V6.00.2800.1165 X-Mailer: Microsoft Outlook Express 6.00.2800.1158 Content-type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-priority: Normal References: <1066320821.3f8ec3b56ff5d@intranet.csis.hku.hk> <004e01c39402$eafcfe40$6401a8c0@FEBRUARY> <1066323022.3f8ecc4ed96fe@intranet.csis.hku.hk> X-IMAG-MailScanner: Found to be clean, Found to be clean X-Loop: globillum@imag.fr X-Sequence: 220 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; 6 X-Spam-Level: ++++++ X-Spam-TU-Processing-Host: neelix X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit
> Hi,
>
> 1. "Mathematical model approximates the real world."
> 2. "Graphics Program implments the mathematical model."
>
> What I am trying to focus is checking no. 2. The graphics program gives output
> with many values, say a matrix of 640x480 (the image). How the developer verify
> that every pixel is correctly rendered according to the mathematical model?
>
> Regards,
> Jeff
>
This question is currently being addressed by CIE Technical Committee TC 3.33. To quote from http://www.cie.co.at:
 
TC 3-33 Test Cases for Assessment of Accuracy of Interior Lighting Computer Programs. To develop a set of validation benchmarks to assess the accuracy of lighting computer programs. The benchmarks consist of a set of test cases produced using analytical solutions and measurements with scale models, including 1:1 scale. Sensitivity studies will be carried out and software examples produced. Chair: F. Maamari (France).
 
The basic (brute force) approach is to develop a series of analytical models for simple environments (mostly empty rooms) with both electric and natural lighting. A set of expected values is then calculated for a grid of points on each surface (i.e., in object space).
 
All surfaces are assumed to be diffuse, so that this is a validation of the radiosity equation rather than the rendering equation (with the exception of Fresnel reflection from glazed windows).
 
There are currently ten test cases:
  • Description of Luminaires with Intensity Distribution Files
  • Direct Illuminance with Glazed Wall Openings under CIE General Sky Type 16
  • Direct Illuminance with Roof Openings under CIE General Sky Type 5 (Uniform Sky)
  • Direct Illuminance with Unglazed Wall Openings under CIE General Sky Type 5
  • Directional Transmittance of Clear Glass
  • Luminous Flux Penetration through Aperture
  • Shape Factor
  • Sky Component with Glazed Roof Openings under the CIE General Sky Type 16 (CIE Overcast Sky)
  • Sky Component with Unglazed Openings under the CIE General Sky Type 16 (CIE Overcast Sky)
  • Surface Reflectance
This does not fully answer your question in that you indicated that you are interested in validating a view-dependent solution in image space. However, unless the object space solution is at least approximately correct, the question of program correctness becomes rather ill-defined.
 
Ian Ashdown, P. Eng., LC, FIES
President
byHeart Consultants Limited
http://www.helios32.com
 
From Return-Path: Received: from neelix.kom.tuwien.ac.at (neelix.kom.tuwien.ac.at [192.35.241.67]) by mail.cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id h9H21Kl1010252; Fri, 17 Oct 2003 04:01:20 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by neelix.kom.tuwien.ac.at (8.12.10/8.12.8) with ESMTP id h9H215Jo007900; Fri, 17 Oct 2003 04:01:09 +0200 (MEST) X-Connecting-Host: imag.imag.fr [129.88.30.1] X-Connecting-Addr: 129.88.30.1 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id h9H208J4017168; Fri, 17 Oct 2003 04:00:08 +0200 (CEST) Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h9H208c08231; Fri, 17 Oct 2003 04:00:08 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h9H201J08214 for ; Fri, 17 Oct 2003 04:00:01 +0200 Received: from pd5mo3so.prod.shaw.ca (shawidc-mo1.cg.shawcable.net [24.71.223.10]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id h9H1xuJ4017090 for ; Fri, 17 Oct 2003 03:59:56 +0200 (CEST) Received: from pd5mr3so.prod.shaw.ca (pd5mr3so-qfe3.prod.shaw.ca [10.0.141.144]) by l-daemon (iPlanet Messaging Server 5.2 HotFix 1.16 (built May 14 2003)) with ESMTP id <0HMV0007QPJVIF@l-daemon> for globillum@imag.fr; Thu, 16 Oct 2003 19:59:55 -0600 (MDT) Received: from pn2ml3so.prod.shaw.ca (pn2ml3so-qfe0.prod.shaw.ca [10.0.121.147]) by l-daemon (iPlanet Messaging Server 5.2 HotFix 1.16 (built May 14 2003)) with ESMTP id <0HMV00FMVPJVYS@l-daemon> for globillum@imag.fr; Thu, 16 Oct 2003 19:59:55 -0600 (MDT) Received: from FEBRUARY (h24-87-171-230.vn.shawcable.net [24.87.171.230]) by l-daemon (iPlanet Messaging Server 5.2 HotFix 1.16 (built May 14 2003)) with SMTP id <0HMV004ATPJTYW@l-daemon> for globillum@imag.fr; Thu, 16 Oct 2003 19:59:55 -0600 (MDT) Date: Thu, 16 Oct 2003 18:58:15 -0700 From: Ian Ashdown Subject: CIE TC 3.33 To: globillum@imag.fr Reply-to: Ian Ashdown Message-id: <003a01c39452$21299bf0$6401a8c0@FEBRUARY> Organization: byHeart Consultants Limited MIME-version: 1.0 X-MIMEOLE: Produced By Microsoft MimeOLE V6.00.2800.1165 X-Mailer: Microsoft Outlook Express 6.00.2800.1158 X-Priority: 3 X-MSMail-priority: Normal References: <1066320821.3f8ec3b56ff5d@intranet.csis.hku.hk> <004e01c39402$eafcfe40$6401a8c0@FEBRUARY> <1066323022.3f8ecc4ed96fe@intranet.csis.hku.hk> <00a101c3940b$7188fce0$6401a8c0@FEBRUARY> X-IMAG-MailScanner: Found to be clean, Found to be clean X-Loop: globillum@imag.fr X-Sequence: 221 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -4 X-Spam-Level: - X-Spam-TU-Processing-Host: neelix X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit I mentioned in an earlier message that CIE Technical Committee TC 3.33 was addressing global illumination validation issues from the perspective of architectural lighting design. For those who are interested, this on-going work is summarized in: Maamari F., and M. Fontoynont. 2003. "Analytical Tests for Investigating the Accuracy of Lighting Programs," Lighting Research and Technology 35(3):225-242. Ian Ashdown, P. Eng., LC, FIES President byHeart Consultants Limited http://www.helios32.com ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by mail.cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id h9N28Sl1022329; Thu, 23 Oct 2003 04:08:28 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by tuvok.kom.tuwien.ac.at (8.12.10/8.12.8) with ESMTP id h9N27aw9008433; Thu, 23 Oct 2003 04:07:39 +0200 (MEST) X-Connecting-Host: imag.imag.fr [129.88.30.1] X-Connecting-Addr: 129.88.30.1 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id h9N25dgM002901; Thu, 23 Oct 2003 04:05:39 +0200 (CEST) Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h9N25c413734; Thu, 23 Oct 2003 04:05:38 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h9N23ZJ13676 for ; Thu, 23 Oct 2003 04:03:35 +0200 Received: from ns.csis.hku.hk (ns.csis.hku.hk [147.8.178.10]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id h9N23VgM002467 for ; Thu, 23 Oct 2003 04:03:32 +0200 (CEST) Received: from study.csis.hku.hk (study [147.8.178.15]) by ns.csis.hku.hk (8.12.10+Sun/8.12.9) with ESMTP id h9N23DcJ013865; Thu, 23 Oct 2003 10:03:14 +0800 (HKT) Received: from csis.hku.hk (jcfhopc [147.8.177.161]) by study.csis.hku.hk (8.11.7p1+Sun/8.11.6) with ESMTP id h9N23BY04035; Thu, 23 Oct 2003 10:03:12 +0800 (CST) Message-ID: <3F9736E5.4010909@csis.hku.hk> Date: Thu, 23 Oct 2003 10:03:17 +0800 From: "Jeffrey C. F. Ho" User-Agent: Mozilla/5.0 (Windows; U; Windows NT 5.1; en-US; rv:1.0.1) Gecko/20020823 Netscape/7.0 X-Accept-Language: en-us, en MIME-Version: 1.0 To: Ingo Wald CC: globillum@imag.fr Subject: Re: How to test a graphics program? (2) References: <1066320821.3f8ec3b56ff5d@intranet.csis.hku.hk> <004e01c39402$eafcfe40$6401a8c0@FEBRUARY> <1066323022.3f8ecc4ed96fe@intranet.csis.hku.hk> <3F927A73.1010205@graphics.cs.uni-sb.de> X-IMAG-MailScanner: Found to be clean, Found to be clean X-Loop: globillum@imag.fr X-Sequence: 222 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -56 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hi, Thanks for your information. So is this method satisfactory for the time being? Does the "simplest renderer" that renders the master reference image very difficult ensure correctness? Jeff Ingo Wald wrote: > jcfho@csis.hku.hk wrote: > >> Hi, >> 1. "Mathematical model approximates the real world." >> 2. "Graphics Program implments the mathematical model." >> >> What I am trying to focus is checking no. 2. The graphics program >> gives output with many values, say a matrix of 640x480 (the image). >> How the developer verify that every pixel is correctly rendered >> according to the mathematical model? >> >> Regards, >> Jeff >> >> > if you're only referring to the correctness of the *implementation* of > an algorithm, then probably the most common way is to cross-compare > images generated with various different algorithms. there is a large > variety of global illumination algorithms out there, and several vary > mostly in their efficiency but otherwise implement the same > 'mathematical model'. > > in order to "validate" a new implementation of a more complex algorithm, > it is then > common to first render a "master image" with a slow renderer of which > one assumes that > it is correct. > for example, one renders an image with a the most simple global > illumination algorithm -- i.e. a slow path tracer, which is kept as > simple and unoptimized as possible to make as sure as possible that it > is correct -- then uses a huge number of samples (65,000 samples per > pixel minimum), and compares wether the new renderer converges to the > same image. > > to strengthen this approach in a more systemic way (as a single master > image might just not contain a certain effect on which the algorithm > might be buggy) some people (i think it was brian smits and some others, > though i'm not sure - brian, you should be on this list ;-) ) have even > proposed a set of "global illumination test scenes" (i think, this was > actually the title of the paper). these test scenes stress various > special cases, and are provided in several file formats, and even with > pre-rendered master images against which one can compare. > > obviously, this is just 'systematic testing', not a real 'validation'. > however, in my experience it's the most common approach... > > Ciao > > Ingo > > ps: sorry i can't currently provide the reference to the paper i > mentioned. i'm sure somebody on this list will follow up with it... > > > ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by mail.cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id h9N3pMl1022691; Thu, 23 Oct 2003 05:51:22 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by tuvok.kom.tuwien.ac.at (8.12.10/8.12.8) with ESMTP id h9N3p5w9009266; Thu, 23 Oct 2003 05:51:08 +0200 (MEST) X-Connecting-Host: imag.imag.fr [129.88.30.1] X-Connecting-Addr: 129.88.30.1 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id h9N3UegM012763; Thu, 23 Oct 2003 05:30:40 +0200 (CEST) Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h9N3Udp23340; Thu, 23 Oct 2003 05:30:39 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h9N3UWJ23321 for ; Thu, 23 Oct 2003 05:30:32 +0200 Received: from pd5mo3so.prod.shaw.ca (shawidc-mo1.cg.shawcable.net [24.71.223.10]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id h9N3UTgM012715 for ; Thu, 23 Oct 2003 05:30:30 +0200 (CEST) Received: from pd5mr4so.prod.shaw.ca (pd5mr4so-qfe3.prod.shaw.ca [10.0.141.168]) by l-daemon (iPlanet Messaging Server 5.2 HotFix 1.16 (built May 14 2003)) with ESMTP id <0HN6009EOUTUFF@l-daemon> for globillum@imag.fr; Wed, 22 Oct 2003 20:27:30 -0600 (MDT) Received: from pn2ml3so.prod.shaw.ca (pn2ml3so-qfe0.prod.shaw.ca [10.0.121.147]) by l-daemon (iPlanet Messaging Server 5.2 HotFix 1.16 (built May 14 2003)) with ESMTP id <0HN6007DKUTU4C@l-daemon> for globillum@imag.fr; Wed, 22 Oct 2003 20:27:30 -0600 (MDT) Received: from FEBRUARY (h24-87-171-230.vn.shawcable.net [24.87.171.230]) by l-daemon (iPlanet Messaging Server 5.2 HotFix 1.16 (built May 14 2003)) with SMTP id <0HN600G4UUTSTB@l-daemon> for globillum@imag.fr; Wed, 22 Oct 2003 20:27:30 -0600 (MDT) Date: Wed, 22 Oct 2003 19:25:54 -0700 From: Ian Ashdown Subject: Re: How to test a graphics program? (2) To: globillum@imag.fr Reply-to: Ian Ashdown Message-id: <011a01c3990c$ffe71f20$6401a8c0@FEBRUARY> Organization: byHeart Consultants Limited MIME-version: 1.0 X-MIMEOLE: Produced By Microsoft MimeOLE V6.00.2800.1165 X-Mailer: Microsoft Outlook Express 6.00.2800.1158 X-Priority: 3 X-MSMail-priority: Normal References: <1066320821.3f8ec3b56ff5d@intranet.csis.hku.hk> <004e01c39402$eafcfe40$6401a8c0@FEBRUARY> <1066323022.3f8ecc4ed96fe@intranet.csis.hku.hk> <3F927A73.1010205@graphics.cs.uni-sb.de> <3F9736E5.4010909@csis.hku.hk> X-IMAG-MailScanner: Found to be clean, Found to be clean X-Loop: globillum@imag.fr X-Sequence: 223 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -13 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit > to strengthen this approach in a more systemic way (as a single master > image might just not contain a certain effect on which the algorithm > might be buggy) some people (i think it was brian smits and some others, > though i'm not sure - brian, you should be on this list ;-) ) have even > proposed a set of "global illumination test scenes" (i think, this was > actually the title of the paper). these test scenes stress various > special cases, and are provided in several file formats, and even with > pre-rendered master images against which one can compare. > That would be: Smits, B., and H. W. Jensen. 2000. "Global Illumination Test Scenes." Technical Report UUCS-00-13. Department of Computer Science, University of Utah. It is no longer available from http://www.cs.utah.edu/bes/papers/scenes, so I will ask Pete Shirley for an update. Pete? - Ian Ashdown ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from neelix.kom.tuwien.ac.at (neelix.kom.tuwien.ac.at [192.35.241.67]) by mail.cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id h9NDpol1027455; Thu, 23 Oct 2003 15:51:50 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by neelix.kom.tuwien.ac.at (8.12.10/8.12.8) with ESMTP id h9NDpfpf006336; Thu, 23 Oct 2003 15:51:43 +0200 (MEST) X-Connecting-Host: imag.imag.fr [129.88.30.1] X-Connecting-Addr: 129.88.30.1 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id h9ND6SLF016852; Thu, 23 Oct 2003 15:06:28 +0200 (CEST) Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h9ND6Rc22984; Thu, 23 Oct 2003 15:06:27 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h9ND6IJ22965 for ; Thu, 23 Oct 2003 15:06:18 +0200 Received: from mail.gmx.net (mail.gmx.de [213.165.64.20]) by imag.imag.fr (8.12.10/8.12.10) with SMTP id h9ND6GLF016782 for ; Thu, 23 Oct 2003 15:06:16 +0200 (CEST) Received: (qmail 31599 invoked by uid 65534); 23 Oct 2003 13:06:16 -0000 Received: from p50856170.dip0.t-ipconnect.de (EHLO gmx.net) (80.133.97.112) by mail.gmx.net (mp014) with SMTP; 23 Oct 2003 15:06:16 +0200 X-Authenticated: #8703357 Message-ID: <3F97D1EB.2030708@gmx.net> Date: Thu, 23 Oct 2003 15:04:43 +0200 From: Roland Schregle Organization: *Out Of Order* User-Agent: Mozilla/5.0 (X11; U; Linux i686; en-US; rv:1.3) Gecko/20030313 X-Accept-Language: en-us, en MIME-Version: 1.0 To: globillum@imag.fr Subject: Re: How to test a graphics program? (2) References: <1066320821.3f8ec3b56ff5d@intranet.csis.hku.hk> <004e01c39402$eafcfe40$6401a8c0@FEBRUARY> <1066323022.3f8ecc4ed96fe@intranet.csis.hku.hk> <3F927A73.1010205@graphics.cs.uni-sb.de> <3F9736E5.4010909@csis.hku.hk> <011a01c3990c$ffe71f20$6401a8c0@FEBRUARY> In-Reply-To: <011a01c3990c$ffe71f20$6401a8c0@FEBRUARY> X-IMAG-MailScanner: Found to be clean, Found to be clean X-Loop: globillum@imag.fr X-Sequence: 224 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -40 X-Spam-Level: - X-Spam-TU-Processing-Host: neelix X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Ian Ashdown wrote: >>to strengthen this approach in a more systemic way (as a single master >>image might just not contain a certain effect on which the algorithm >>might be buggy) some people (i think it was brian smits and some others, >>though i'm not sure - brian, you should be on this list ;-) ) have even >>proposed a set of "global illumination test scenes" (i think, this was >>actually the title of the paper). these test scenes stress various >>special cases, and are provided in several file formats, and even with >>pre-rendered master images against which one can compare. >> > > That would be: > > Smits, B., and H. W. Jensen. 2000. "Global Illumination Test Scenes." > Technical Report UUCS-00-13. Department of Computer Science, University of > Utah. > > It is no longer available from http://www.cs.utah.edu/bes/papers/scenes, so > I will ask Pete Shirley for an update. Pete? I have a PDF of this paper if you can't find it. Let me know! --Roland -- Roland Schregle PhD candidate, Fraunhofer Institute for Solar Energy Systems RADIANCE Photon Map page: www.ise.fhg.de/radiance/photon-map END OF LINE. (MCP) ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from neelix.kom.tuwien.ac.at (neelix.kom.tuwien.ac.at [192.35.241.67]) by mail.cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id h9NGE1l1028765; Thu, 23 Oct 2003 18:14:01 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by neelix.kom.tuwien.ac.at (8.12.10/8.12.8) with ESMTP id h9NGDRpf015616; Thu, 23 Oct 2003 18:13:33 +0200 (MEST) X-Connecting-Host: imag.imag.fr [129.88.30.1] X-Connecting-Addr: 129.88.30.1 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id h9NG4b8J005805; Thu, 23 Oct 2003 18:04:37 +0200 (CEST) Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id h9NG4b511857; Thu, 23 Oct 2003 18:04:37 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id h9NG4UJ11840 for ; Thu, 23 Oct 2003 18:04:30 +0200 Received: from bjork.pharr.org (adsl-66-125-65-154.dsl.sntc01.pacbell.net [66.125.65.154]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id h9NG4R8J005694 for ; Thu, 23 Oct 2003 18:04:28 +0200 (CEST) Received: by bjork.pharr.org (Postfix, from userid 501) id 3FF4B11E741; Thu, 23 Oct 2003 09:04:23 -0700 (PDT) To: globillum@imag.fr Subject: Re: How to test a graphics program? (2) References: <1066320821.3f8ec3b56ff5d@intranet.csis.hku.hk> <004e01c39402$eafcfe40$6401a8c0@FEBRUARY> <1066323022.3f8ecc4ed96fe@intranet.csis.hku.hk> <3F927A73.1010205@graphics.cs.uni-sb.de> <3F9736E5.4010909@csis.hku.hk> <011a01c3990c$ffe71f20$6401a8c0@FEBRUARY> <3F97D1EB.2030708@gmx.net> From: Matt Pharr X-Face: C!.oGaE]n@p)VF9Ss3]f'|<)kRrtpG)^^b^X-3_zhUHp\jBj29jaoTItqWR>mHa+v-{/!jx7OA@!cV0>Fm-b:zEL<`oOXG[BFQ\ (Roland Schregle's message of "Thu, 23 Oct 2003 15:04:43 +0200") Message-ID: User-Agent: Gnus/5.1003 (Gnus v5.10.3) XEmacs/21.4 (Military Intelligence, linux) MIME-Version: 1.0 X-IMAG-MailScanner: Found to be clean, Found to be clean X-Loop: globillum@imag.fr X-Sequence: 225 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -65 X-Spam-Level: - X-Spam-TU-Processing-Host: neelix X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit > Ian Ashdown wrote: >> That would be: >> Smits, B., and H. W. Jensen. 2000. "Global Illumination Test Scenes." >> Technical Report UUCS-00-13. Department of Computer Science, University of >> Utah. >> It is no longer available from http://www.cs.utah.edu/bes/papers/scenes, >> so >> I will ask Pete Shirley for an update. Pete? It's actually still there; you're just missing a tilde: http://www.cs.utah.edu/~bes/papers/scenes -matt -- Matt Pharr matt@pharr.org ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from neelix.kom.tuwien.ac.at (neelix.kom.tuwien.ac.at [192.35.241.67]) by mail.cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id hAH4fvl1004407; Mon, 17 Nov 2003 05:41:57 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by neelix.kom.tuwien.ac.at (8.12.10/8.12.8) with ESMTP id hAH4fnoX000447; Mon, 17 Nov 2003 05:41:49 +0100 (MET) X-Connecting-Host: imag.imag.fr [129.88.30.1] X-Connecting-Addr: 129.88.30.1 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id hAH4fiEA022864; Mon, 17 Nov 2003 05:41:44 +0100 (CET) Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id hAH4fdA27242; Mon, 17 Nov 2003 05:41:39 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id hAH4dpJ27202 for ; Mon, 17 Nov 2003 05:39:51 +0100 Received: from pd3mo2so.prod.shaw.ca (shawidc-mo1.cg.shawcable.net [24.71.223.10]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id hAH4dnEA022527 for ; Mon, 17 Nov 2003 05:39:49 +0100 (CET) Received: from pd2mr2so.prod.shaw.ca (pd2mr2so-ser.prod.shaw.ca [10.0.141.109]) by l-daemon (iPlanet Messaging Server 5.2 HotFix 1.18 (built Jul 28 2003)) with ESMTP id <0HOH00LCZBM4PL@l-daemon> for globillum@imag.fr; Sun, 16 Nov 2003 21:39:40 -0700 (MST) Received: from pn2ml5so.prod.shaw.ca (pn2ml5so-qfe0.prod.shaw.ca [10.0.121.149]) by l-daemon (iPlanet Messaging Server 5.2 HotFix 1.18 (built Jul 28 2003)) with ESMTP id <0HOH001GXBM4S8@l-daemon> for globillum@imag.fr; Sun, 16 Nov 2003 21:39:40 -0700 (MST) Received: from FEBRUARY (h24-87-171-230.vn.shawcable.net [24.87.171.230]) by l-daemon (iPlanet Messaging Server 5.2 HotFix 1.18 (built Jul 28 2003)) with SMTP id <0HOH00F3KBM2JZ@l-daemon> for globillum@imag.fr; Sun, 16 Nov 2003 21:39:40 -0700 (MST) Date: Sun, 16 Nov 2003 20:38:59 -0800 From: Ian Ashdown Subject: ANNOUNCE: 03/11/16 Release of RADBIB and GITHESIS To: globillum@imag.fr Reply-to: Ian Ashdown Message-id: <000a01c3acc4$b8761620$6401a8c0@FEBRUARY> Organization: byHeart Consultants Limited MIME-version: 1.0 X-MIMEOLE: Produced By Microsoft MimeOLE V6.00.2800.1165 X-Mailer: Microsoft Outlook Express 6.00.2800.1158 Content-type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-priority: Normal X-IMAG-MailScanner: Found to be clean, Found to be clean X-Loop: globillum@imag.fr X-Sequence: 227 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; 15 X-Spam-Level: *+++++ X-Spam-TU-Processing-Host: neelix X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

ANNOUNCE: 03/11/16 Release of RADBIB and GITHESIS

RADBIB is a comprehensive bibliography of radiosity and related global illumination papers, theses, articles, and books. It currently includes 2,338 references -- 16 new additions since its 03/10/11 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of October 11, 2003) from:

http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 305 references to radiosity and global illumination theses -- 2 new additions since the 03/10/11 release.

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

Ian Ashdown, P. Eng., LC, FIES
President
byHeart Consultants Limited
http://www.helios32.com

From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by mail.cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id hBIHcQl1014994; Thu, 18 Dec 2003 18:38:26 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by tuvok.kom.tuwien.ac.at (8.12.10/8.12.8) with ESMTP id hBIHcI6G025774; Thu, 18 Dec 2003 18:38:18 +0100 (MET) X-Connecting-Host: imag.imag.fr [129.88.30.1] X-Connecting-Addr: 129.88.30.1 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id hBIHc7Nt027937; Thu, 18 Dec 2003 18:38:07 +0100 (CET) Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id hBIHc6C09183; Thu, 18 Dec 2003 18:38:06 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id hBIHc0f09161 for ; Thu, 18 Dec 2003 18:38:00 +0100 Received: from tut.autodesk.com (tut.eur.autodesk.com [132.188.62.7]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id hBIHbvNt027874 for ; Thu, 18 Dec 2003 18:37:58 +0100 (CET) Received: from msgusawfe02.ads.autodesk.com ([144.111.33.211]) by tut.autodesk.com (8.12.10/8.12.6) with ESMTP id hBIHbtew013689 for ; Thu, 18 Dec 2003 18:37:56 +0100 (CET) Received: from msgusaepf01.ads.autodesk.com ([144.111.72.51]) by msgusawfe02.ads.autodesk.com with Microsoft SMTPSVC(5.0.2195.6713); Thu, 18 Dec 2003 09:39:22 -0800 Received: from msgusaemb01.ads.autodesk.com ([144.111.72.50]) by msgusaepf01.ads.autodesk.com with Microsoft SMTPSVC(5.0.2195.6713); Thu, 18 Dec 2003 12:39:21 -0500 X-MimeOLE: Produced By Microsoft Exchange V6.0.6487.1 MIME-Version: 1.0 Subject: Fantasy Graphics League season begins Date: Thu, 18 Dec 2003 12:39:13 -0500 Message-ID: Thread-Topic: Fantasy Graphics League season begins Thread-Index: AcPFbgd8+ZcLwGaNSzitbi/ArEwNVQAHph5A From: "Eric Haines (Autodesk, NY)" To: globillum@imag.fr X-OriginalArrivalTime: 18 Dec 2003 17:39:22.0059 (UTC) FILETIME=[DF1A01B0:01C3C58D] X-IMAG-MailScanner: Found to be clean, Found to be clean X-MIME-Autoconverted: from quoted-printable to 8bit by chopinette.imag.fr id hBIHc0f09161 X-Loop: globillum@imag.fr X-Sequence: 232 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; 0 X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit content-class: urn:content-classes:message Content-Type: text/plain; charset="us-ascii" Content-Transfer-Encoding: 8bit The next season of the Fantasy Graphics League has begun: http://www.realtimerendering.com/fgl/siggraph2004/ Oh, while I'm here, Matt Pharr & Greg Humphreys' upcoming book on realistic image synthesis (out in a few months), from MKP, looks very promising. It covers the topic from soup to nuts (includes things like filtering, tone mapping, etc). It's aimed towards making a good design and implementation (and there's fully working code; in fact, it's in Literate Programming style), with lots of theory and code bits supporting this goal. What I like best is that it actually makes design decisions and says what the tradeoffs are, instead of the standard textbook style of, "there are ten ways to perform this process and I'm going to describe all ten because I don't quite know enough to rule any out." Eric ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by mail.cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id i04GJWl1006438; Sun, 4 Jan 2004 17:19:32 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by tuvok.kom.tuwien.ac.at (8.12.10/8.12.8) with ESMTP id i04GJKJU005690; Sun, 4 Jan 2004 17:19:21 +0100 (MET) X-Connecting-Host: imag.imag.fr [129.88.30.1] X-Connecting-Addr: 129.88.30.1 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id i04G5An8015493; Sun, 4 Jan 2004 17:05:10 +0100 (CET) Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id i04G55l07699; Sun, 4 Jan 2004 17:05:05 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id i04G4uf07681 for ; Sun, 4 Jan 2004 17:04:56 +0100 Received: from mail-imagis (mail-imagis.inrialpes.fr [194.199.26.22]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id i04G4tn8015407 for ; Sun, 4 Jan 2004 17:04:55 +0100 (CET) Received: from graphics.csail.mit.edu (pourpier [194.199.26.183]) by mail-imagis (Postfix) with ESMTP id 0C6E31C85B for ; Sun, 4 Jan 2004 17:04:55 +0100 (CET) Message-ID: <3FF839A6.7000207@graphics.csail.mit.edu> Date: Sun, 04 Jan 2004 17:04:54 +0100 From: Fredo Durand User-Agent: Mozilla/5.0 (Windows; U; Windows NT 5.1; en-US; rv:1.4) Gecko/20030624 Netscape/7.1 (ax) X-Accept-Language: en-us, en MIME-Version: 1.0 To: "globillum@imag.fr" Subject: BRDF previsualization X-IMAG-MailScanner: Found to be clean, Found to be clean X-Loop: globillum@imag.fr X-Sequence: 233 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -1 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hi everyone Happy New Year! I have a question about the previsualization of complex analytical models such as Cook Torrance using simpler models such as Blinn/Phong. Say, for a production software, you can set more advanced analytical models but have interactive preview using OpenGL. I gues sthat now people start using pixel shaders, but in teh good old days, was there a formula to get Phong parameters from Cook-Torrance or Ward? Thanks Fredo -- -- Fredo Durand, MIT-CSAIL Graphics Group 200 technology sq. NE43-254, Cambridge, MA 02139, USA phone : (617) 253 7223 fax : (617) 253 4640 http://graphics.lcs.mit.edu/~fredo/ ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by mail.cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id i04N79L0006197; Mon, 5 Jan 2004 00:07:09 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by tuvok.kom.tuwien.ac.at (8.12.10/8.12.8) with ESMTP id i04N6vJU002959; Mon, 5 Jan 2004 00:06:57 +0100 (MET) X-Connecting-Host: imag.imag.fr [129.88.30.1] X-Connecting-Addr: 129.88.30.1 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id i04MvFn8009580; Sun, 4 Jan 2004 23:57:15 +0100 (CET) Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id i04MvEx19791; Sun, 4 Jan 2004 23:57:14 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id i04Mv6f19773 for ; Sun, 4 Jan 2004 23:57:06 +0100 Received: from smtp812.mail.sc5.yahoo.com (smtp812.mail.sc5.yahoo.com [66.163.170.82]) by imag.imag.fr (8.12.10/8.12.10) with SMTP id i04Mv0n8009522 for ; Sun, 4 Jan 2004 23:57:01 +0100 (CET) Received: from unknown (HELO ?64.163.213.209?) (gregoryjward@64.163.213.209 with plain) by smtp812.mail.sc5.yahoo.com with SMTP; 4 Jan 2004 22:56:59 -0000 In-Reply-To: <3FF839A6.7000207@graphics.csail.mit.edu> References: <3FF839A6.7000207@graphics.csail.mit.edu> Mime-Version: 1.0 Message-Id: <442BD856-3F09-11D8-A4BD-000A95BB392A@lmi.net> Cc: globillum@imag.fr From: Greg Ward Subject: Re: BRDF previsualization Date: Sun, 4 Jan 2004 14:56:43 -0800 To: Fredo Durand X-Mailer: Apple Mail (2.609) X-IMAG-MailScanner: Found to be clean, Found to be clean X-Loop: globillum@imag.fr X-Sequence: 234 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -20 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hi Fredo, The very rough approximation to get specular roughness (i.e., gaussian surface height std. dev. over correlation distance) from Phong specular power is: roughness = sqrt(2/specular_power) There may be a better correlation out there, however. (See for more info.) -Greg > From: Fredo Durand > Date: January 4, 2004 8:04:54 AM PST > > Hi everyone > > Happy New Year! > > I have a question about the previsualization of complex analytical > models such as Cook Torrance using simpler models such as Blinn/Phong. > Say, for a production software, you can set more advanced analytical > models but have interactive preview using OpenGL. > I gues sthat now people start using pixel shaders, but in teh good old > days, was there a formula to get Phong parameters from Cook-Torrance > or Ward? > > Thanks > > Fredo ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from neelix.kom.tuwien.ac.at (neelix.kom.tuwien.ac.at [192.35.241.67]) by mail.cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id i04NLBL0006337; Mon, 5 Jan 2004 00:21:11 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by neelix.kom.tuwien.ac.at (8.12.10/8.12.8) with ESMTP id i04NKveX012201; Mon, 5 Jan 2004 00:20:58 +0100 (MET) X-Connecting-Host: imag.imag.fr [129.88.30.1] X-Connecting-Addr: 129.88.30.1 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id i04N8Yn8012217; Mon, 5 Jan 2004 00:08:34 +0100 (CET) Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id i04N8YT20991; Mon, 5 Jan 2004 00:08:34 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id i04N6hf20940 for ; Mon, 5 Jan 2004 00:06:43 +0100 Received: from vivarin.mherf.com (h-67-100-249-210.LSANCA54.covad.net [67.100.249.210]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id i04N6en8011780 for ; Mon, 5 Jan 2004 00:06:41 +0100 (CET) Received: from capsaicin (guarana [192.168.1.12]) by vivarin.mherf.com (Postfix) with SMTP id 671694353D; Sun, 4 Jan 2004 15:06:34 -0800 (PST) Message-ID: <444501c3d317$a29be4a0$0c01a8c0@capsaicin> From: "Michael Herf" To: "Fredo Durand" Cc: globillum@imag.fr References: <3FF839A6.7000207@graphics.csail.mit.edu> <442BD856-3F09-11D8-A4BD-000A95BB392A@lmi.net> Subject: Re: BRDF previsualization Date: Sun, 4 Jan 2004 15:08:16 -0800 MIME-Version: 1.0 X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 6.00.2800.1158 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1165 X-IMAG-MailScanner: Found to be clean, Found to be clean X-Loop: globillum@imag.fr X-Sequence: 235 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -10 X-Spam-Level: - X-Spam-TU-Processing-Host: neelix X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit There's a paper from SIGGRAPH 97 that might be of interest: http://www.graphics.cornell.edu/~bjw/virtlite.html For object lighting (as opposed to scene lighting), you might be able to just put the reflectance you want in an environment map and use it -- depends on your application, of course. miek ----- Original Message ----- From: "Greg Ward" To: "Fredo Durand" Cc: Sent: Sunday, January 04, 2004 2:56 PM Subject: Re: BRDF previsualization > Hi Fredo, > > The very rough approximation to get specular roughness (i.e., gaussian > surface height std. dev. over correlation distance) from Phong specular > power is: > > roughness = sqrt(2/specular_power) > > There may be a better correlation out there, however. > > (See for more > info.) > > -Greg > > > From: Fredo Durand > > Date: January 4, 2004 8:04:54 AM PST > > > > Hi everyone > > > > Happy New Year! > > > > I have a question about the previsualization of complex analytical > > models such as Cook Torrance using simpler models such as Blinn/Phong. > > Say, for a production software, you can set more advanced analytical > > models but have interactive preview using OpenGL. > > I gues sthat now people start using pixel shaders, but in teh good old > > days, was there a formula to get Phong parameters from Cook-Torrance > > or Ward? > > > > Thanks > > > > Fredo > > ---------------------------------------------------------------------- ---------- > -------------------------------------------------------------------- ----- > globillum@imag.fr -- mailing list devoted to global illumination research > For list archives or to configure your options, see http://listes.imag.fr > -------------------------------------------------------------------- ----- ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id i173vExX007099; Sat, 7 Feb 2004 04:57:14 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.12.10/8.12.8) with ESMTP id i173v4Rr000373; Sat, 7 Feb 2004 04:57:04 +0100 (MET) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id i173ucM14200; Sat, 7 Feb 2004 04:56:38 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id i173siv13630 for ; Sat, 7 Feb 2004 04:54:44 +0100 Received: from pd3mo2so.prod.shaw.ca (shawidc-mo1.cg.shawcable.net [24.71.223.10]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id i173sexF022885 for ; Sat, 7 Feb 2004 04:54:40 +0100 (CET) Received: from pd2mr4so.prod.shaw.ca (pd2mr4so-ser.prod.shaw.ca [10.0.141.107]) by l-daemon (iPlanet Messaging Server 5.2 HotFix 1.18 (built Jul 28 2003)) with ESMTP id <0HSP00NOL3ZS35@l-daemon> for globillum@imag.fr; Fri, 06 Feb 2004 20:50:16 -0700 (MST) Received: from pn2ml3so.prod.shaw.ca (pn2ml3so-qfe0.prod.shaw.ca [10.0.121.147]) by l-daemon (iPlanet Messaging Server 5.2 HotFix 1.18 (built Jul 28 2003)) with ESMTP id <0HSP00K263ZT7N@l-daemon> for globillum@imag.fr; Fri, 06 Feb 2004 20:50:17 -0700 (MST) Received: from FEBRUARY ([24.87.171.230]) by l-daemon (iPlanet Messaging Server 5.2 HotFix 1.18 (built Jul 28 2003)) with SMTP id <0HSP006303ZRCD@l-daemon> for globillum@imag.fr; Fri, 06 Feb 2004 20:50:16 -0700 (MST) Date: Fri, 06 Feb 2004 19:52:17 -0800 From: Ian Ashdown Subject: ANNOUNCE: 04/02/06 Release of RADBIB and GITHESIS To: globillum@imag.fr Reply-to: Ian Ashdown Message-id: <004801c3ed2d$c7b7ab40$6401a8c0@FEBRUARY> Organization: byHeart Consultants Limited MIME-version: 1.0 X-MIMEOLE: Produced By Microsoft MimeOLE V6.00.2800.1165 X-Mailer: Microsoft Outlook Express 6.00.2800.1158 Content-type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-priority: Normal X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Loop: globillum@imag.fr X-Sequence: 238 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; 13 X-Spam-Level: *+++ X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

ANNOUNCE: 04/02/06 Release of RADBIB and GITHESIS

RADBIB is a comprehensive bibliography of radiosity, photon mapping, and related global illumination papers, theses, articles, and books. It currently includes 2,355 references -- 17 new additions since its 03/11/16 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of February 6, 2004) from:

    http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 314 references to radiosity, photon mapping, and related global illumination theses -- 9 new additions since the 03/11/16 release.

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

Ian Ashdown, P. Eng., LC, FIES
President
byHeart Consultants Limited
http://www.helios32.com


 

 From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id i25GFHCC013737; Fri, 5 Mar 2004 17:15:18 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.12.10/8.12.8) with ESMTP id i25GEoGk023223; Fri, 5 Mar 2004 17:14:51 +0100 (MET) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id i25G81n21674; Fri, 5 Mar 2004 17:08:01 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id i25G5fk21612 for ; Fri, 5 Mar 2004 17:05:41 +0100 Received: from hqemgate00.nvidia.com (hqemgate00.nvidia.com [216.228.112.144]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id i25G5asr015968 for ; Fri, 5 Mar 2004 17:05:37 +0100 (CET) Received: from mail-sc-0.nvidia.com (Not Verified[172.16.217.105]) id ; Fri, 05 Mar 2004 08:07:04 -0800 Received: by mail-sc-0.nvidia.com with Internet Mail Service (5.5.2657.72) id ; Fri, 5 Mar 2004 08:05:30 -0800 Received: from PHECKBERTDT3 (PHECKBERT-DT3 [172.16.226.43]) by mail-sc-0.nvidia.com with SMTP (Microsoft Exchange Internet Mail Service Version 5.5.2657.72) id FV375QAD; Fri, 5 Mar 2004 08:05:27 -0800 From: Paul Heckbert To: "Global Illumination, Mailing List for" X-Mailer: Microsoft Outlook Express 6.00.2800.1158 X-MimeOLE: Microsoft Outlook Express 6.00.2800.1158 Message-ID: <005201c402cb$ad2a1750$2be210ac@nvidia.com> Subject: NY Times article on digital walkthroughs Date: Fri, 5 Mar 2004 11:05:27 -0500 MIME-Version: 1.0 Content-Type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 6.00.2800.1158 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1165 X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Loop: globillum@imag.fr X-Sequence: 241 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; 15 X-Spam-Level: *+++++ X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit
It's not exactly global illumination, but it is a sign that digital walkthroughs and electronic architectural simulation are coming of age:
 
See the article "For New Buildings, Digital Models Offer an Advance Walk-Through" in today's New York Times. http://www.nytimes.com/2004/03/04/technology/circuits/04desi.html
 
If the NY Times website asks you to register, don't worry, go ahead and do that, it's quick, free, and you'll get no spam.
 
excerpt:
 
AEI Digital, a division of EwingCole, one of the architectural firms that designed the [Philadelphia Phillies ballpark], meticulously constructed it in more than four million polygons. This was accomplished long before the last real brick, last cubic yard of real concrete and last piece of real structural steel were laid, poured and bolted into place - even before the place was named Citizens Bank Park.
From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id i2609JCC021243; Sat, 6 Mar 2004 01:09:20 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.12.10/8.12.8) with ESMTP id i26096Gk020389; Sat, 6 Mar 2004 01:09:07 +0100 (MET) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id i2602VO09753; Sat, 6 Mar 2004 01:02:31 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id i2602Mk09730 for ; Sat, 6 Mar 2004 01:02:22 +0100 Received: from busybox.pixar.com (busybox.pixar.com [138.72.18.213]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id i2602BZI029505 (version=TLSv1/SSLv3 cipher=EDH-RSA-DES-CBC3-SHA bits=168 verify=NO) for ; Sat, 6 Mar 2004 01:02:19 +0100 (CET) Received: from pixar.com (slush [192.168.50.17]) by busybox.pixar.com (8.12.8/8.12.8) with ESMTP id i26027Hw022544; Fri, 5 Mar 2004 16:02:08 -0800 Message-ID: <404914FF.7090600@pixar.com> Date: Fri, 05 Mar 2004 16:02:07 -0800 From: Per Christensen User-Agent: Mozilla/5.0 (X11; U; Linux i686; en-US; rv:1.2.1) Gecko/20030225 X-Accept-Language: en-us, en MIME-Version: 1.0 To: globillum@imag.fr CC: per.christensen@acm.org Subject: Importance bibliographies X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Loop: globillum@imag.fr X-Sequence: 243 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -1 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Dear fellow globillum'ers, In the hope that this might be useful for somebody, I've put two bibliographies for adjoints and importance up on the following web page: http://www.seanet.com/~myandper/importance.htm "importance_background.bib" contains references to mathematics texts on adjoints in general and articles and books about the use of importance in nuclear physics (where it is an adjoint of neutron density). "importance_graphics.bib" contains references to articles, dissertations, and books about the use of importance (defined as an adjoint of light) in global illumination and ray tracing. The entries are divided into five categories: 1) theoretical results in rendering, 2) "classic" ray tracing and distribution ray tracing, 3) finite element methods, 4) Monte Carlo methods, 5) volume ray tracing and participating media. The entries are sorted chronologically within each category. The bibliographies are in BibTeX format and are intended to supplement Ian Ashdown's excellent radbib bibliography. Many thanks to Philippe Bekaert who pointed out some of these references. If you know of any references that should be added, please send me an e-mail. Enjoy! -- Per ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id i2HFUYCC004492; Wed, 17 Mar 2004 16:30:34 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.12.11/8.12.11) with ESMTP id i2HFUSXN015930; Wed, 17 Mar 2004 16:30:28 +0100 (MET) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id i2HFO0O24510; Wed, 17 Mar 2004 16:24:00 +0100 Received: from harmonie.imag.fr (harmonie.imag.fr [147.171.130.40]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id i2HFNok24493 for ; Wed, 17 Mar 2004 16:23:50 +0100 Received: from ns.csis.hku.hk (ns.csis.hku.hk [147.8.178.10]) by harmonie.imag.fr (8.12.10/8.12.7) with ESMTP id i2HFNib6027382 for ; Wed, 17 Mar 2004 16:23:46 +0100 (CET) Received: from genius.csis.hku.hk (genius-nat [147.8.177.11]) by ns.csis.hku.hk (8.12.10+Sun/8.12.10) with ESMTP id i2HFMgN7018490; Wed, 17 Mar 2004 23:22:59 +0800 (HKT) Received: from genius.csis.hku.hk (localhost [127.0.0.1]) by genius.csis.hku.hk (8.12.9+Sun/8.12.9) with ESMTP id i2HFMgNx010334; Wed, 17 Mar 2004 23:22:42 +0800 (HKT) Received: from localhost (jcfho@localhost) by genius.csis.hku.hk (8.12.9+Sun/8.12.2/Submit) with ESMTP id i2HFMORb010331; Wed, 17 Mar 2004 23:22:42 +0800 (HKT) X-Authentication-Warning: genius.csis.hku.hk: jcfho owned process doing -bs Date: Wed, 17 Mar 2004 23:22:24 +0800 (HKT) From: "Ho Jeffrey Chun Fai [PG]" To: globillum@imag.fr cc: jcfho@csis.hku.hk Subject: Papers on Error estimate of Radiosity Message-ID: MIME-Version: 1.0 X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Loop: globillum@imag.fr X-Sequence: 245 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -49 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Dear all, I am trying to find papers on error estimate of radiosity. I found the following two. Can anyone tell me other important or more recent papers related to this? What I found: - A Framework for the Analysis of Error in Global Illumination Algorithms, James Arvo, Kenneth Torrance, Brian Smits. - Bounds and Error Estimates for Radiosity, Dani Lischinshi, Brian Smits, Donald P. Greenberg. Thanks! Jeffrey Ho ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from neelix.kom.tuwien.ac.at (neelix.kom.tuwien.ac.at [192.35.241.67]) by cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id i2HFn5CC005307; Wed, 17 Mar 2004 16:49:06 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by neelix.kom.tuwien.ac.at (8.12.10/8.12.8) with ESMTP id i2HFmob1020522; Wed, 17 Mar 2004 16:48:52 +0100 (MET) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id i2HFgNW26830; Wed, 17 Mar 2004 16:42:23 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id i2HFgIk26813 for ; Wed, 17 Mar 2004 16:42:18 +0100 Received: from imag.fr (ache.inrialpes.fr [194.199.26.136]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id i2HFgBgl002157; Wed, 17 Mar 2004 16:42:11 +0100 (CET) Date: Wed, 17 Mar 2004 16:43:56 +0100 Subject: Re: Papers on Error estimate of Radiosity Mime-Version: 1.0 Cc: globillum@imag.fr To: "Ho Jeffrey Chun Fai [PG]" From: Nicolas Holzschuch In-Reply-To: Message-Id: X-Mailer: Apple Mail (2.553) X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-Information: Please contact the ISP for more information X-MIME-Autoconverted: from quoted-printable to 8bit by chopinette.imag.fr id i2HFgIk26813 X-Loop: globillum@imag.fr X-Sequence: 246 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -10 X-Spam-Level: - X-Spam-TU-Processing-Host: neelix X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hello, Le mercredi, 17 mars 2004, à 16:22 Europe/Zurich, Ho Jeffrey Chun Fai [PG] a écrit : > Dear all, > > I am trying to find papers on error estimate of radiosity. I found the > following two. Can anyone tell me other important or more recent papers > related to this? I can strongly recommand my own paper: An Exhaustive Error-Bounding Algorithm for Hierarchical Radiosity, N. Holzschuch and F. Sillion, Computer Graphics Forum, vol. 17, number 4 http://artis.imag.fr/Publications/1998/HS98/ But I think the most interesting view on the subject is inside: Ph. Bekaert, Y.D. Willems, Error Control for Radiosity, Rendering Techniques '96, X. Pueyo, P. Schröder (eds.), Springer-Verlag 1996, ISBN 3-211-82883-4 Also in: Proceedings of the 7th Eurographics Workshop on Rendering, O Porto, Portugal (June 1996). http://www.cs.kuleuven.ac.be/cwis/research/graphics/CGRG.PUBLICATIONS/ RadError/ Philippe's refinement oracle is actually implemented into every industrial application of hierarchical radiosity that I know of. :-) It works especially well with higher-order basis functions, such as quadric wavelets (see A novel approach makes higher order wavelets really efficient for radiosity, F Cuny et al., Computer Graphics Forum - Sep 2000, http://artis.imag.fr/Publications/2000/CAH00/) > What I found: > - A Framework for the Analysis of Error in Global Illumination > Algorithms, > James Arvo, Kenneth Torrance, Brian Smits. > > - Bounds and Error Estimates for Radiosity, Dani Lischinshi, Brian > Smits, > Donald P. Greenberg. -- Greetings, Nicolas Holzschuch ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from neelix.kom.tuwien.ac.at (neelix.kom.tuwien.ac.at [192.35.241.67]) by cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id i2HFuaCC005719; Wed, 17 Mar 2004 16:56:36 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by neelix.kom.tuwien.ac.at (8.12.10/8.12.8) with ESMTP id i2HFuBb1024625; Wed, 17 Mar 2004 16:56:16 +0100 (MET) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id i2HFqn728147; Wed, 17 Mar 2004 16:52:49 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id i2HFojk28083 for ; Wed, 17 Mar 2004 16:50:45 +0100 Received: from hqemgate00.nvidia.com (hqemgate00.nvidia.com [216.228.112.144]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id i2HFodgl005515; Wed, 17 Mar 2004 16:50:40 +0100 (CET) Received: from mail-sc-0.nvidia.com (Not Verified[172.16.217.105]) id ; Wed, 17 Mar 2004 07:50:18 -0800 Received: by mail-sc-0.nvidia.com with Internet Mail Service (5.5.2657.72) id ; Wed, 17 Mar 2004 07:50:18 -0800 Received: from PHECKBERTDT3 (PHECKBERT-DT3 [172.16.226.112]) by mail-sc-0.nvidia.com with SMTP (Microsoft Exchange Internet Mail Service Version 5.5.2657.72) id G0SRN1B0; Wed, 17 Mar 2004 07:50:11 -0800 From: Paul Heckbert To: "Ho Jeffrey Chun Fai [PG]" , Nicolas Holzschuch Cc: globillum@imag.fr, "Willmott, Andrew" X-Mailer: Microsoft Outlook Express 6.00.2800.1158 X-MimeOLE: Microsoft Outlook Express 6.00.2800.1158 Message-ID: <04d201c40c37$869e6a80$1de210ac@nvidia.com> References: Subject: Re: Papers on Error estimate of Radiosity Date: Wed, 17 Mar 2004 10:50:08 -0500 MIME-Version: 1.0 X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 6.00.2800.1158 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1165 X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Loop: globillum@imag.fr X-Sequence: 247 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -10 X-Spam-Level: - X-Spam-TU-Processing-Host: neelix X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Also see @PHDTHESIS{Willmott00phd, author={Andrew J. Willmott}, title={Hierarchical Radiosity with Multiresolution Meshes}, school={School of Computer Science, Carnegie Mellon University}, month=nov, year=2000, keywords={global illumination, visibility, face cluster, error analysis, hierarchical radiosity, clustering}, note={\URL{http://www.cs.cmu.edu/~ajw}}, } and the shorter and earlier paper @InProceedings{Willmott99fcr, author = "Andrew J. Willmott and Paul S. Heckbert and Michael Garland", title = "Face Cluster Radiosity", booktitle = "Eurographics Workshop on Rendering", month = jun, year = 1999, note = "\URL{http://www.cs.cmu.edu/~ajw/paper/fcr-eg99/}" } ----- Original Message ----- From: "Nicolas Holzschuch" To: "Ho Jeffrey Chun Fai [PG]" Cc: Sent: Wednesday, March 17, 2004 10:43 AM Subject: Re: Papers on Error estimate of Radiosity Hello, Le mercredi, 17 mars 2004, à 16:22 Europe/Zurich, Ho Jeffrey Chun Fai [PG] a écrit : > Dear all, > > I am trying to find papers on error estimate of radiosity. I found the > following two. Can anyone tell me other important or more recent papers > related to this? I can strongly recommand my own paper: An Exhaustive Error-Bounding Algorithm for Hierarchical Radiosity, N. Holzschuch and F. Sillion, Computer Graphics Forum, vol. 17, number 4 http://artis.imag.fr/Publications/1998/HS98/ But I think the most interesting view on the subject is inside: Ph. Bekaert, Y.D. Willems, Error Control for Radiosity, Rendering Techniques '96, X. Pueyo, P. Schröder (eds.), Springer-Verlag 1996, ISBN 3-211-82883-4 Also in: Proceedings of the 7th Eurographics Workshop on Rendering, O Porto, Portugal (June 1996). http://www.cs.kuleuven.ac.be/cwis/research/graphics/CGRG.PUBLICATIONS/ RadError/ Philippe's refinement oracle is actually implemented into every industrial application of hierarchical radiosity that I know of. :-) It works especially well with higher-order basis functions, such as quadric wavelets (see A novel approach makes higher order wavelets really efficient for radiosity, F Cuny et al., Computer Graphics Forum - Sep 2000, http://artis.imag.fr/Publications/2000/CAH00/) > What I found: > - A Framework for the Analysis of Error in Global Illumination > Algorithms, > James Arvo, Kenneth Torrance, Brian Smits. > > - Bounds and Error Estimates for Radiosity, Dani Lischinshi, Brian > Smits, > Donald P. Greenberg. -- Greetings, Nicolas Holzschuch ---------------------------------------------------------------------------- ---- > ------------------------------------------------------------------------- > globillum@imag.fr -- mailing list devoted to global illumination research > For list archives or to configure your options, see http://listes.imag.fr > ------------------------------------------------------------------------- ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id i2JNCACC007512; Sat, 20 Mar 2004 00:12:11 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.12.11/8.12.11) with ESMTP id i2JNC0Km004039; Sat, 20 Mar 2004 00:12:01 +0100 (MET) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id i2JN8TT04303; Sat, 20 Mar 2004 00:08:29 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id i2JN8Nk04286 for ; Sat, 20 Mar 2004 00:08:23 +0100 Received: from serv01.divms.uiowa.edu (serv01.divms.uiowa.edu [128.255.44.134]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id i2JN8KpT018543 (version=TLSv1/SSLv3 cipher=EDH-RSA-DES-CBC3-SHA bits=168 verify=FAIL) for ; Sat, 20 Mar 2004 00:08:21 +0100 (CET) Received: from mlh1B ([128.255.45.228]) by serv01.divms.uiowa.edu with id i2JN8Hc2024588 for ; Fri, 19 Mar 2004 17:08:17 -0600 (CST) Message-ID: <001301c40e07$108ca830$e42dff80@mlh1B> From: "Kendall Atkinson" To: globillum@imag.fr Subject: Re: Papers on Error estimate of Radiosity Date: Fri, 19 Mar 2004 17:08:12 -0600 MIME-Version: 1.0 Content-Type: text/plain; charset=windows-1252; format=flowed X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 6.00.2800.1158 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1165 X-Spam-Score: -4.801 () BAYES_00,HTML_MESSAGE X-Scanned-By: MIMEDefang 2.37 X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Loop: globillum@imag.fr X-Sequence: 248 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -49 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit In reply to the request for references on the error analysis for the numerical analysis of the radiosity equation, I would like to note the work of Olaf Hansen. He recently completed his habilitation thesis at the University of Mainz. He is now in the Mathematics Dept of California State University at San Marcos. Below are his papers on the radiosity equation. * O. Hansen, The local behavior of the solution of the radiosity equation on polyhedral domains in R^3 , SIAM Journal on Mathematical Analysis, Vol. 33, No. 3, 718-750, 2001. * O. Hansen, On the Stability of the Collocation Method for the Radiosity Equation on Polyhedral Domains , IMA Journal of Numerical Analysis, Vol. 22, 463-479, 2002. * O. Hansen, The Mapping Properties of the Radiosity Operator along an Edge, Mathematical Methods in the Applied Sciences, Vol. 25, 1075-1090, 2002. * O. Hansen, The Radiosity Equation on certain Spaces of Continuous Functions and its Numerical Solution, Journal of Integral Equations and Applications, Vol. 15, 2, 153-202, 2003. * O. Hansen, A fast collocation method for the radiosity equation, based on the hierarchical algorithm of P. Hanrahan and D. Salzman: The 1d case, accepted in Advances in Computational Mathematics. * O. Hansen, The asymptotic behavior of the spectrum of the reflection operator on conical surfaces, accepted in Integral Equations and Operator Theory. Kendall Atkinson Depts of Mathematics and Computer Science University of Iowa From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id i2K2Y2CC014673; Sat, 20 Mar 2004 03:34:02 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.12.11/8.12.11) with ESMTP id i2K2XtOG024325; Sat, 20 Mar 2004 03:33:56 +0100 (MET) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id i2K2UUB26293; Sat, 20 Mar 2004 03:30:30 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id i2K2SVk25715 for ; Sat, 20 Mar 2004 03:28:31 +0100 Received: from pd3mo3so.prod.shaw.ca (shawidc-mo1.cg.shawcable.net [24.71.223.10]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id i2K2SPpS003798 for ; Sat, 20 Mar 2004 03:28:26 +0100 (CET) Received: from pd5mr6so.prod.shaw.ca (pd5mr6so-qfe3.prod.shaw.ca [10.0.141.182]) by l-daemon (iPlanet Messaging Server 5.2 HotFix 1.18 (built Jul 28 2003)) with ESMTP id <0HUU00GDXS7DUC@l-daemon> for globillum@imag.fr; Fri, 19 Mar 2004 19:28:25 -0700 (MST) Received: from pn2ml4so.prod.shaw.ca ([10.0.121.148]) by pd5mr6so.prod.shaw.ca (Sun ONE Messaging Server 6.0 Patch 1 (built Jan 13 2004)) with ESMTP id <0HUU00CPMS780870@pd5mr6so.prod.shaw.ca> for globillum@imag.fr; Fri, 19 Mar 2004 19:28:20 -0700 (MST) Received: from FEBRUARY (h24-87-171-230.vn.shawcable.net [24.87.171.230]) by l-daemon (iPlanet Messaging Server 5.2 HotFix 1.18 (built Jul 28 2003)) with SMTP id <0HUU0010HS7BY1@l-daemon> for globillum@imag.fr; Fri, 19 Mar 2004 19:28:24 -0700 (MST) Date: Fri, 19 Mar 2004 18:31:45 -0800 From: Ian Ashdown Subject: RADBIB and GITHESIS - March 19th Release To: globillum@imag.fr Reply-to: Ian Ashdown Message-id: <002a01c40e23$7d8292d0$6401a8c0@FEBRUARY> Organization: byHeart Consultants Limited MIME-version: 1.0 X-MIMEOLE: Produced By Microsoft MimeOLE V6.00.2800.1165 X-Mailer: Microsoft Outlook Express 6.00.2800.1158 Content-type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-priority: Normal X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Loop: globillum@imag.fr X-Sequence: 249 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; 14 X-Spam-Level: *++++ X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

ANNOUNCE: 04/03/19 Release of RADBIB and GITHESIS

RADBIB is a comprehensive bibliography of radiosity, photon mapping, and related global illumination papers, theses, articles, and books. It currently includes 2,359 references -- 4 new additions since its 04/02/06 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of March 19, 2004) from:

    http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 314 references to radiosity, photon mapping, and related global illumination theses -- no new additions since the 04/02/06 release.

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

Ian Ashdown, P. Eng., LC, FIES
President
byHeart Consultants Limited
http://www.helios32.com

From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id i3E6URCC013125; Wed, 14 Apr 2004 08:30:27 +0200 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.12.11/8.12.11) with ESMTP id i3E6TXA0018110; Wed, 14 Apr 2004 08:29:36 +0200 (MEST) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id i3E6N0u18331; Wed, 14 Apr 2004 08:23:00 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id i3E6IxZ17704 for ; Wed, 14 Apr 2004 08:18:59 +0200 Received: from pd3mo1so.prod.shaw.ca (shawidc-mo1.cg.shawcable.net [24.71.223.10]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id i3E6IpQi013670 for ; Wed, 14 Apr 2004 08:18:52 +0200 (CEST) Received: from pd5mr7so.prod.shaw.ca (pd5mr7so-qfe3.prod.shaw.ca [10.0.141.183]) by l-daemon (iPlanet Messaging Server 5.2 HotFix 1.18 (built Jul 28 2003)) with ESMTP id <0HW500MO9CWAB5@l-daemon> for globillum@imag.fr; Wed, 14 Apr 2004 00:04:58 -0600 (MDT) Received: from pn2ml4so.prod.shaw.ca ([10.0.121.148]) by pd5mr7so.prod.shaw.ca (Sun ONE Messaging Server 6.0 HotFix 1.01 (built Mar 15 2004)) with ESMTP id <0HW500K1VCXEDP20@pd5mr7so.prod.shaw.ca> for globillum@imag.fr; Wed, 14 Apr 2004 00:05:38 -0600 (MDT) Received: from FEBRUARY (S01060006257abbc2.vn.shawcable.net [24.87.171.230]) by l-daemon (iPlanet Messaging Server 5.2 HotFix 1.18 (built Jul 28 2003)) with SMTP id <0HW50032ECW6YN@l-daemon> for globillum@imag.fr; Wed, 14 Apr 2004 00:04:55 -0600 (MDT) Date: Tue, 13 Apr 2004 23:09:07 -0700 From: Ian Ashdown Subject: ANNOUNCE: 04/04/14 Release of RADBIB and GITHESIS To: globillum@imag.fr Reply-to: Ian Ashdown Message-id: <001401c421e6$fec785e0$6401a8c0@FEBRUARY> Organization: byHeart Consultants Limited MIME-version: 1.0 X-MIMEOLE: Produced By Microsoft MimeOLE V6.00.2800.1165 X-Mailer: Microsoft Outlook Express 6.00.2800.1158 Content-type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-priority: Normal X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Loop: globillum@imag.fr X-Sequence: 252 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; 39 X-Spam-Level: ***+++++++++ X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

ANNOUNCE: 04/04/14 Release of RADBIB and GITHESIS

RADBIB is a comprehensive bibliography of radiosity, photon mapping, and related global illumination papers, theses, articles, and books. It currently includes 2,365 references -- 6 new additions since its 04/03/19 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of April 14, 2004) from:

    http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 314 references to radiosity, photon mapping, and related global illumination theses -- no new additions since the 04/03/19 release.

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

Ian Ashdown, P. Eng., LC, FIES
President
byHeart Consultants Limited
http://www.helios32.com

 

From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id i3EDDpCC028030; Wed, 14 Apr 2004 15:13:51 +0200 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.12.11/8.12.11) with ESMTP id i3EDDkbv018800; Wed, 14 Apr 2004 15:13:46 +0200 (MEST) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id i3ED71900572; Wed, 14 Apr 2004 15:07:01 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id i3ED4ZZ32447 for ; Wed, 14 Apr 2004 15:04:35 +0200 Received: from graphics.csail.mit.edu (graphics.csail.mit.edu [18.24.2.30]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id i3ED4Rd1020739 (version=TLSv1/SSLv3 cipher=EDH-RSA-DES-CBC3-SHA bits=168 verify=NO) for ; Wed, 14 Apr 2004 15:04:28 +0200 (CEST) Received: from graphics.csail.mit.edu (pool-68-163-219-210.bos.east.verizon.net [68.163.219.210]) by graphics.csail.mit.edu (8.12.10/8.12.10) with ESMTP id i3ED4Qd9002835; Wed, 14 Apr 2004 09:04:27 -0400 Message-ID: <407D36DC.7030803@graphics.csail.mit.edu> Date: Wed, 14 Apr 2004 09:04:28 -0400 From: Fredo Durand User-Agent: Mozilla/5.0 (Windows; U; Windows NT 5.1; en-US; rv:1.4) Gecko/20030624 Netscape/7.1 (ax) X-Accept-Language: en-us, en MIME-Version: 1.0 To: globillum@imag.fr CC: Maneesh Agrawala Subject: CFP: Smart Depiction, CG&A special issue X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Loop: globillum@imag.fr X-Sequence: 254 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -22 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Call for Papers: SMART DEPICTION FOR VISUAL COMMUNICATION Special Issue of IEEE CG&A, May/June 2005 Guest Editors Maneesh Agrawala and Frédo Durand http://www.computer.org/cga/CFPMay05.htm Submissions due: September 1, 2004 Author notification: December 1, 2004 Final versions due: February 1, 2005 As computers become faster, smaller, ubiquitous, and interconnected, their primary function is shifting from computation to communication. Visual media in the form of photographs, photorealistic renderings, diagrams, sketches, animations, and film are increasingly generated, manipulated, and transmitted by computers. Yet even with the aid of a computer, producing effective and expressive visual content can take hours or days and consume considerable artistic skills. The challenge is to develop new algorithms and user interfaces that facilitate visual communication by making it fast and easy to generate compelling graphical visual content. The most effective graphics combine principles and techniques from graphic design, visual art, perceptual psychology, and cognitive science. Smart depiction systems are computer algorithms and interfaces that embody these principles and techniques. Such systems hold the potential for significantly reducing the time and effort required to generate rich and effective visual content. The purpose of this special issue is to attract novel research results on smart depiction for visual communication. We seek work that identifies and algorithmically instantiates the principles and techniques for creating effective visual content. Potential topics for articles include, but are not limited to: * Visual abstraction techniques * Dealing with visual density and clutter * Creating effective explanatory animations * Material perception, depiction, and stylization * Improving comprehensibility of photorealistic images * Automated lighting and viewpoint control * Design principles for layout and composition * Shape and space perception and visualization Articles should be fewer than 10 magazine pages, where a page is 800 words and a quarter page image counts as 200 words. Cite only the 12 most critical references, and consider providing background in sidebars for nonexpert readers. Color images can be interspersed through the article and should be limited to a total of 10. Visit CG&A style and length guidelines here. Please submit your paper using our online manuscript submission service. When uploading your paper, please select the appropriate special issue title under the category “Manuscript Type.” If you have any questions about submitting your article, please contact Alkenia Winston. Please direct any correspondence prior to submission to both guest editors at: Maneesh Agrawala One Microsoft Way Redmond, WA 98052-6399 Email: maneesh@graphics.stanford.edu Phone: +1 425 705-5718 Fax: +1 425 936-7329 and Frédo Durand MIT CSAIL The Stata Center 32-D426 32 Vassar Street Cambridge, MA 02139, USA Email: fredo@graphics.csail.mit.edu Phone : +1 617 253 7223 Fax : +1 617 253 4640 -- -- Fredo Durand, MIT-CSAIL Graphics Group Stata Center, 32-D426, Cambridge, MA 02139, USA phone : (617) 253 7223 fax : (617) 253 4640 http://graphics.lcs.mit.edu/~fredo/ ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id i3KEmuq3031258; Tue, 20 Apr 2004 16:48:57 +0200 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.12.11/8.12.11) with ESMTP id i3KEmj11004506; Tue, 20 Apr 2004 16:48:45 +0200 (MEST) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id i3KEhq406509; Tue, 20 Apr 2004 16:43:52 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id i3KEfpr05945 for ; Tue, 20 Apr 2004 16:41:51 +0200 Received: from cut.autodesk.com (cut.autodesk.com [198.102.112.47]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id i3KEfkwH023088 for ; Tue, 20 Apr 2004 16:41:47 +0200 (CEST) Received: from msgusawfe02.ads.autodesk.com ([144.111.33.211]) by cut.autodesk.com (8.12.10/8.12.6) with ESMTP id i3KEfh8j000166; Tue, 20 Apr 2004 07:41:43 -0700 (PDT) Received: from msgusawpf01.ads.autodesk.com ([144.111.33.212]) by msgusawfe02.ads.autodesk.com with Microsoft SMTPSVC(5.0.2195.6713); Tue, 20 Apr 2004 07:41:43 -0700 Received: from msgusaefe01.ads.autodesk.com ([144.111.72.49]) by msgusawpf01.ads.autodesk.com with Microsoft SMTPSVC(5.0.2195.6713); Tue, 20 Apr 2004 07:41:42 -0700 Received: from msgusaemb01.ads.autodesk.com ([144.111.72.50]) by msgusaefe01.ads.autodesk.com with Microsoft SMTPSVC(5.0.2195.6713); Tue, 20 Apr 2004 10:41:41 -0400 x-mimeole: Produced By Microsoft Exchange V6.0.6487.1 content-class: urn:content-classes:message MIME-Version: 1.0 Content-Type: text/html; charset=windows-1252 Subject: Gelato Date: Tue, 20 Apr 2004 10:41:41 -0400 Message-ID: Thread-Topic: Gelato Thread-Index: AcQm5ZgUx0us+LQrTgeQE8f7RegmUw== From: "Eric Haines (Autodesk, NY)" To: globillum@imag.fr X-OriginalArrivalTime: 20 Apr 2004 14:41:41.0578 (UTC) FILETIME=[982EB2A0:01C426E5] X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Loop: globillum@imag.fr X-Sequence: 256 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -22 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

Just noticed this on Slashdot, so I thought I’d pass it on: http://film.nvidia.com/page/gelato.html - has the magic words ray-tracing and global illumination in it. This is the stuff Larry Gritz, Matt Pharr, and others have been working on.

 

Eric

From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id i46F7mEl005279; Thu, 6 May 2004 17:07:48 +0200 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.12.11/8.12.11) with ESMTP id i46F7gvp011012; Thu, 6 May 2004 17:07:42 +0200 (MEST) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id i46ExFU02373; Thu, 6 May 2004 16:59:15 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id i46EuuA01786 for ; Thu, 6 May 2004 16:56:56 +0200 Received: from nut.autodesk.com (nut.autodesk.com [198.102.112.27]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id i46Euem0028574 for ; Thu, 6 May 2004 16:56:41 +0200 (CEST) Received: from msgusawfe02.ads.autodesk.com ([144.111.33.211]) by nut.autodesk.com (8.12.10/8.12.6) with ESMTP id i46EubY5005644 for ; Thu, 6 May 2004 07:56:40 -0700 (PDT) Received: from msgusawpf01.ads.autodesk.com ([144.111.33.212]) by msgusawfe02.ads.autodesk.com with Microsoft SMTPSVC(5.0.2195.6713); Thu, 6 May 2004 07:56:37 -0700 Received: from msgusaepf01.ads.autodesk.com ([144.111.72.51]) by msgusawpf01.ads.autodesk.com with Microsoft SMTPSVC(5.0.2195.6713); Thu, 6 May 2004 07:56:37 -0700 Received: from msgusaemb01.ads.autodesk.com ([144.111.72.50]) by msgusaepf01.ads.autodesk.com with Microsoft SMTPSVC(5.0.2195.6713); Thu, 6 May 2004 10:56:36 -0400 X-MimeOLE: Produced By Microsoft Exchange V6.0.6487.1 content-class: urn:content-classes:message MIME-Version: 1.0 Content-Type: text/html; charset=windows-1252 Subject: Viewgraph Giveaway Date: Thu, 6 May 2004 10:56:36 -0400 Message-ID: Thread-Topic: Viewgraph Giveaway Thread-Index: AcQzelO/YFILk4ZzRlyvrKuQmE44Lg== From: "Eric Haines (Autodesk, NY)" To: globillum@imag.fr X-OriginalArrivalTime: 06 May 2004 14:56:36.0604 (UTC) FILETIME=[5444D3C0:01C4337A] X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Loop: globillum@imag.fr X-Sequence: 257 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -47 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

[posting for Andrew; please reply to him, not me.]

 

Dear Globillumers:

 

While cleaning up my office, I uncovered a collection of viewgraphs that I’ve prepared over the years for several classes on rendering (viewgraphs are the transparent sheets that you write on with colored markers and display on an overhead projector).  There are two main topics: the theory and practice of ray tracing, and using Unix, along with a miscellany of brief presentations on other graphics-related topics (e.g., human vision and texturing, as well as some research talks).  I don’t need these any more, and would be happy to donate them to a good home.  The stack, which is about 9” (23 cm) high, contains several hundred lecture-ready viewgraphs, as well as a box of about 70 blanks.  The only catch is that you’ll have to pay shipping: I estimate that shipping this 30 pound box domestically inside the US would cost between $15 and $40 depending on destination, and shipping to Europe would be about US $45 (I can get the exact numbers when I ship).  First come, first served.  Please contact me directly if you’re interested.  I’ll hang onto these until May 15.  

 

-Andrew Glassner ( andrew@glassner.com | www.glassner.com )

 

From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id i4AH65El021616; Mon, 10 May 2004 19:06:05 +0200 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.12.11/8.12.11) with ESMTP id i4AH5s84020447; Mon, 10 May 2004 19:05:57 +0200 (MEST) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id i4AGu5902227; Mon, 10 May 2004 18:56:05 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id i4AGtxC02210 for ; Mon, 10 May 2004 18:55:59 +0200 Received: from bells.cs.ucl.ac.uk (bells.cs.ucl.ac.uk [128.16.5.31]) by imag.imag.fr (8.12.10/8.12.10) with SMTP id i4AGtukQ006891 for ; Mon, 10 May 2004 18:55:56 +0200 (CEST) Received: from raylight.cs.ucl.ac.uk by bells.cs.ucl.ac.uk with local SMTP id ; Mon, 10 May 2004 17:55:33 +0100 Message-Id: <6.0.1.1.2.20040510175916.03374d30@pop.cs.ucl.ac.uk> X-Sender: ucacmsl@pop.cs.ucl.ac.uk X-Mailer: QUALCOMM Windows Eudora Version 6.0.1.1 Date: Mon, 10 May 2004 18:00:28 +0100 To: globillum@imag.fr From: Mel Slater Subject: One Day Seminar on Virtual Light Field Mime-Version: 1.0 X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Loop: globillum@imag.fr X-Sequence: 259 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -49 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit There will be a one day seminar on The Virtual Light Field: Global Illumination - Propagation and Rendering at University College London 4th June, 2004 Full details on http://www.cs.ucl.ac.uk/research/vr/Projects/VLF/Seminar/ regards Mel Slater Department of Computer Science University College London Gower Street London WC1E 6BT http://www.cs.ucl.ac.uk/staff/m.slater ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from neelix.kom.tuwien.ac.at (neelix.kom.tuwien.ac.at [192.35.241.67]) by cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id i4JEVUEl022669; Wed, 19 May 2004 16:31:30 +0200 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by neelix.kom.tuwien.ac.at (8.12.10/8.12.11) with ESMTP id i4JEVFTB016736; Wed, 19 May 2004 16:31:15 +0200 (MEST) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id i4JEOfQ09379; Wed, 19 May 2004 16:24:41 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id i4JELa608829 for ; Wed, 19 May 2004 16:21:36 +0200 Received: from rinka.central.susx.ac.uk (rinka.central.susx.ac.uk [139.184.14.19]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id i4JELXa3029562 for ; Wed, 19 May 2004 16:21:33 +0200 (CEST) Received: from engg100-149.engg.susx.ac.uk ([139.184.100.149] helo=sussex.ac.uk) by rinka.central.susx.ac.uk with esmtp (Exim 4.10) id 1BQRwr-0005X7-00 for globillum@imag.fr; Wed, 19 May 2004 15:21:33 +0100 Message-ID: <40AB6D3C.5050707@sussex.ac.uk> Date: Wed, 19 May 2004 15:20:44 +0100 Organization: University of Sussex User-Agent: Mozilla/5.0 (Windows; U; Windows NT 5.0; en-US; rv:1.4) Gecko/20030624 Netscape/7.1 (ax) X-Accept-Language: en-us, en MIME-Version: 1.0 To: globillum@imag.fr Subject: research post Content-Type: text/html; charset=windows-1252 X-Sussex: true From: Katerina Mania X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Loop: globillum@imag.fr X-Sequence: 265 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; 12 X-Spam-Level: *++ X-Spam-TU-Processing-Host: neelix X-Mozilla-Status: 9001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit
Dear all,

Please distribute as you wish. Closing date for applications is the 4th of June 2004. Apologies for cross-postings.

Best regards
Katerina Mania

---------------------------------------------------------------------------------------------
Advertisement for a Research Fellow:
Quantifying Fidelity for Virtual Environment Simulations employing Schema Assumptions
Department Of Informatics, University of Sussex, UK

Fixed term for 23 months – appointment available immediately

The Department of Informatics, University of Sussex, UK wishes to invite applications for the full-time post of Research fellow working on a project entitled “Quantifying Fidelity for Virtual Environment Simulations employing Schema Assumptions”. This is a joint, 2-year collaboration between the Department of Informatics University of Sussex (Dr Katerina Mania), the Department of Experimental Psychology University of Bristol (Prof. Tom Troscianko), collaborating with Hewlett Packard Laboratories Bristol (Dr Rycharde Hawkes). This post is based at the University of Sussex in Brighton, in close collaboration with the University of Bristol and communication with Hewlett Packard Laboratories in Bristol.

The objectives of the project are:
Conducting experimental studies that will test specific hypothesis related to schema activation (memory research) in computer graphics worlds of varied rendering photorealism. Schemata are knowledge structures based on past experience. When participants are exposed to a large amount of information in a scene, cognitive psychologists have suggested that schemata are used to guide the search for information in memory. For example, if a quick visual scan of a room indicates that there is a clock on the wall, hands may be assigned to it at a memory test, even though this particular clock does not have hands. The results obtained in these experiments will be used to target graphics resources in a demonstrably efficient manner – an object-based rendering engine or a simulation of an engine is going to be implemented which will incorporate more rendering detail according to the degree of association of an object with the schema in context.

This rendering system is going to be validated psychophysically, in comparison to a fully-fledged rendering solution. The major deliverable on this work is a technique which assesses functional realism in an entirely novel way, and can lead to an efficient use of graphics resources by rendering only those objects to a high level which require detailed inspection, and vice versa.

The Department of Informatics is a multidisciplinary, dynamic, and creative department within the School of Science and Technology in the University of Sussex, UK. The Department of Informatics was recently formed from a subset based on the former School of Engineering and IT together with a subset of the former School of Cognitive and Computing Sciences (COGS). Both Schools were awarded a grade 5 in the 2001 Research Assessment Exercise, confirming their world-class reputation in research. The researcher of this post will be a member of the Centre for VLSI and Computer Graphics, a designated EU Marie Curie training centre. The group currently consists of five academic staff and at least 12 research staff and doctoral students. You should have a PhD in a relevant subject area ranging from computer graphics, virtual environments, human computer interaction, human factors or have equivalent experience.

£18,893 – £28,279 p/a

Starting salary will be no higher than £21,852

Closing date for receipt of applications is 4th June 2004.

Interviews are due to take place on the 21st June 2004.

Informal enquiries about this post may be directed to Dr Katerina Mania at k.mania@sussex.ac.uk.

Application details (Ref 614) are available from and should be returned to the Human Resources Division, Sussex House, University of Sussex, Falmer, Brighton, BN1 9RH. Tel 01273 678706, Fax 01273 877401, email recruitment@sussex.ac.uk. Details of all posts can be found via the University website: http://www.susx.ac.uk/Units/staffing

An Equal Opportunity Employer 
-- 
-----------------------------------------------
Dr Katerina Mania
Department of Informatics
University of Sussex, UK
Falmer, BN1 9QT Brighton, UK

T: +44 1273 678964
URL: http://www.sussex.ac.uk/Users/km3
-----------------------------------------------
From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id i4T1JYEl017617; Sat, 29 May 2004 03:19:35 +0200 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.12.11/8.12.11) with ESMTP id i4T1JPWd021366; Sat, 29 May 2004 03:19:28 +0200 (MEST) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id i4T1Cmn18913; Sat, 29 May 2004 03:12:48 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id i4T1CgV18895 for ; Sat, 29 May 2004 03:12:42 +0200 Received: from nut.autodesk.com (nut.autodesk.com [198.102.112.27]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id i4T1CbwG006290 for ; Sat, 29 May 2004 03:12:37 +0200 (CEST) Received: from msgusawfe01.ads.autodesk.com ([144.111.33.210]) by nut.autodesk.com (8.12.10/8.12.6) with ESMTP id i4T1CXjt013871 for ; Fri, 28 May 2004 18:12:34 -0700 (PDT) Received: from msgusawpf01.ads.autodesk.com ([144.111.33.212]) by msgusawfe01.ads.autodesk.com with Microsoft SMTPSVC(5.0.2195.6713); Fri, 28 May 2004 18:12:33 -0700 Received: from msgusaepf01.ads.autodesk.com ([144.111.72.51]) by msgusawpf01.ads.autodesk.com with Microsoft SMTPSVC(5.0.2195.6713); Fri, 28 May 2004 18:12:33 -0700 Received: from msgusaemb01.ads.autodesk.com ([144.111.72.50]) by msgusaepf01.ads.autodesk.com with Microsoft SMTPSVC(5.0.2195.6713); Fri, 28 May 2004 21:12:32 -0400 X-MimeOLE: Produced By Microsoft Exchange V6.0.6487.1 Content-Class: urn:content-classes:message MIME-Version: 1.0 Content-Type: text/html; charset=windows-1252 Subject: And the winner of the Fantasy Graphics League is... Date: Fri, 28 May 2004 21:12:32 -0400 Message-ID: Thread-Topic: And the winner of the Fantasy Graphics League is... Thread-Index: AcRFGgSi7DmUqkW0SQ2IIkTgzkdBRg== From: "Eric Haines (Autodesk, NY)" To: globillum@imag.fr X-OriginalArrivalTime: 29 May 2004 01:12:32.0533 (UTC) FILETIME=[04CE9450:01C4451A] X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Loop: globillum@imag.fr X-Sequence: 268 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -7 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit
 
Enjoy,
 
Eric
Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id i5136HEl011636; Tue, 1 Jun 2004 05:06:17 +0200 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.12.11/8.12.11) with ESMTP id i51367MI022011; Tue, 1 Jun 2004 05:06:09 +0200 (MEST) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id i5132gZ17706; Tue, 1 Jun 2004 05:02:42 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id i512xuU17613 for ; Tue, 1 Jun 2004 04:59:56 +0200 Received: from pd2mo3so.prod.shaw.ca (shawidc-mo1.cg.shawcable.net [24.71.223.10]) by imag.imag.fr (8.12.10/8.12.10) with ESMTP id i512xrwG028154 for ; Tue, 1 Jun 2004 04:59:54 +0200 (CEST) Received: from pd4mr3so.prod.shaw.ca (pd4mr3so-qfe3.prod.shaw.ca [10.0.141.214]) by l-daemon (iPlanet Messaging Server 5.2 HotFix 1.18 (built Jul 28 2003)) with ESMTP id <0HYM00EHM01QST@l-daemon> for globillum@imag.fr; Mon, 31 May 2004 20:53:50 -0600 (MDT) Received: from pn2ml2so.prod.shaw.ca ([10.0.121.146]) by pd4mr3so.prod.shaw.ca (Sun ONE Messaging Server 6.0 HotFix 1.01 (built Mar 15 2004)) with ESMTP id <0HYM00GMC01QDMF0@pd4mr3so.prod.shaw.ca> for globillum@imag.fr; Mon, 31 May 2004 20:53:50 -0600 (MDT) Received: from BLUEBERRY (S01060006257abbc2.vn.shawcable.net [24.87.171.230]) by l-daemon (iPlanet Messaging Server 5.2 HotFix 1.18 (built Jul 28 2003)) with SMTP id <0HYM0012S01O1I@l-daemon> for globillum@imag.fr; Mon, 31 May 2004 20:53:50 -0600 (MDT) Date: Mon, 31 May 2004 19:59:30 -0700 From: Ian Ashdown Subject: ANNOUNCE: 04/06/01 Release of RADBIB and GITHESIS To: globillum@imag.fr Reply-to: Ian Ashdown Message-id: <00b401c44784$767dfd40$6401a8c0@BLUEBERRY> Organization: byHeart Consultants Limited MIME-version: 1.0 X-MIMEOLE: Produced By Microsoft MimeOLE V6.00.2800.1409 X-Mailer: Microsoft Outlook Express 6.00.2800.1409 Content-type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-priority: Normal X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Loop: globillum@imag.fr X-Sequence: 270 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; 14 X-Spam-Level: *++++ X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

ANNOUNCE: 04/06/01 Release of RADBIB and GITHESIS

RADBIB is a comprehensive bibliography of radiosity, photon mapping, and related global illumination papers, theses, articles, and books. It currently includes 2,372 references -- 7 new additions since its 04/04/16 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of June 1, 2004) from:

    http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 314 references to radiosity, photon mapping, and related global illumination theses -- no new additions since the 04/04/16 release.

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

Ian Ashdown, P. Eng., LC, FIES
President
byHeart Consultants Limited
http://www.helios32.com

From Return-Path: Received: from neelix.kom.tuwien.ac.at (neelix.kom.tuwien.ac.at [192.35.241.67]) by cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id i6L42dIx003632; Wed, 21 Jul 2004 06:02:41 +0200 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by neelix.kom.tuwien.ac.at (8.12.11/8.12.11) with ESMTP id i6L42Tk3018552; Wed, 21 Jul 2004 06:02:32 +0200 (MEST) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id i6L3x0F01913; Wed, 21 Jul 2004 05:59:00 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id i6L3st201320 for ; Wed, 21 Jul 2004 05:54:55 +0200 Received: from pd3mo1so.prod.shaw.ca (shawidc-mo1.cg.shawcable.net [24.71.223.10]) by imag.imag.fr (8.13.0/8.13.0) with ESMTP id i6L3sqWL014914 for ; Wed, 21 Jul 2004 05:54:53 +0200 (CEST) Received: from pd3mr4so.prod.shaw.ca (pd3mr4so-ser.prod.shaw.ca [10.0.141.180]) by l-daemon (iPlanet Messaging Server 5.2 HotFix 1.18 (built Jul 28 2003)) with ESMTP id <0I16008YGNSVSB@l-daemon> for globillum@imag.fr; Tue, 20 Jul 2004 21:46:07 -0600 (MDT) Received: from pn2ml10so.prod.shaw.ca ([10.0.121.80]) by pd3mr4so.prod.shaw.ca (Sun ONE Messaging Server 6.0 HotFix 1.01 (built Mar 15 2004)) with ESMTP id <0I16007D4NSVXB30@pd3mr4so.prod.shaw.ca> for globillum@imag.fr; Tue, 20 Jul 2004 21:46:07 -0600 (MDT) Received: from BLUEBERRY (S01060006257abbc2.vn.shawcable.net [24.87.171.230]) by l-daemon (iPlanet Messaging Server 5.2 HotFix 1.18 (built Jul 28 2003)) with SMTP id <0I160056ZNSUXG@l-daemon> for globillum@imag.fr; Tue, 20 Jul 2004 21:46:07 -0600 (MDT) Date: Tue, 20 Jul 2004 20:48:24 -0700 From: Ian Ashdown Subject: ANNOUNCE: 04/07/19 Release of RADBIB and GITHESIS To: globillum@imag.fr Reply-to: Ian Ashdown Message-id: <004c01c46ed5$933c0490$6401a8c0@BLUEBERRY> Organization: byHeart Consultants Limited MIME-version: 1.0 X-MIMEOLE: Produced By Microsoft MimeOLE V6.00.2800.1441 X-Mailer: Microsoft Outlook Express 6.00.2800.1437 Content-type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-priority: Normal X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Loop: globillum@imag.fr X-Sequence: 274 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; 14 X-Spam-Level: *++++ X-Spam-TU-Processing-Host: neelix X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

ANNOUNCE: 04/07/19 Release of RADBIB and GITHESIS

RADBIB is a comprehensive bibliography of radiosity, photon mapping, and related global illumination papers, theses, articles, and books. It currently includes 2,390 references -- 18 new additions since its 04/06/01 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of July 19, 2004) from:

http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 315 references to radiosity, photon mapping, and related global illumination theses -- one new addition since the 04/06/01 release.

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

Ian Ashdown, P. Eng., LC, FIES
President
byHeart Consultants Limited
http://www.helios32.com

From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id i85MAw1B002831; Mon, 6 Sep 2004 00:10:58 +0200 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.12.11/8.12.11) with ESMTP id i85MAkiu021728; Mon, 6 Sep 2004 00:10:48 +0200 (MEST) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id i85M4JS20615; Mon, 6 Sep 2004 00:04:19 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id i85M1fa20549 for ; Mon, 6 Sep 2004 00:01:41 +0200 Received: from pd5mo3so.prod.shaw.ca (shawidc-mo1.cg.shawcable.net [24.71.223.10]) by imag.imag.fr (8.13.0/8.13.0) with ESMTP id i85M1cEJ009876 for ; Mon, 6 Sep 2004 00:01:39 +0200 (CEST) Received: from pd4mr6so.prod.shaw.ca (pd4mr6so-qfe3.prod.shaw.ca [10.0.141.69]) by l-daemon (iPlanet Messaging Server 5.2 HotFix 1.18 (built Jul 28 2003)) with ESMTP id <0I3L007U85VI2Z@l-daemon> for globillum@imag.fr; Sun, 05 Sep 2004 14:50:06 -0600 (MDT) Received: from pn2ml5so.prod.shaw.ca ([10.0.121.149]) by pd4mr6so.prod.shaw.ca (Sun ONE Messaging Server 6.0 HotFix 1.01 (built Mar 15 2004)) with ESMTP id <0I3L00CKM5VI4TC0@pd4mr6so.prod.shaw.ca> for globillum@imag.fr; Sun, 05 Sep 2004 14:50:06 -0600 (MDT) Received: from BLUEBERRY (S01060006257abbc2.vn.shawcable.net [24.87.171.230]) by l-daemon (iPlanet Messaging Server 5.2 HotFix 1.18 (built Jul 28 2003)) with SMTP id <0I3L00C2A5VG01@l-daemon> for globillum@imag.fr; Sun, 05 Sep 2004 14:50:05 -0600 (MDT) Date: Sun, 05 Sep 2004 13:53:56 -0700 From: Ian Ashdown Subject: ANNOUNCE - 04/09/05 Release of RADBIB and GITHESIS To: globillum@imag.fr Reply-to: Ian Ashdown Message-id: <000a01c4938a$7631c680$6501a8c0@BLUEBERRY> Organization: byHeart Consultants Limited MIME-version: 1.0 X-MIMEOLE: Produced By Microsoft MimeOLE V6.00.2800.1441 X-Mailer: Microsoft Outlook Express 6.00.2800.1437 Content-type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-priority: Normal X-Greylist: Delayed for 01:05:39 by milter-greylist-1.4 (imag.imag.fr [129.88.30.1]); Mon, 06 Sep 2004 00:01:39 +0200 (CEST) X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Loop: globillum@imag.fr X-Sequence: 277 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -6 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

ANNOUNCE: 04/09/05 Release of RADBIB and GITHESIS

RADBIB is a comprehensive bibliography of radiosity, photon mapping, and related global illumination papers, theses, articles, and books. It currently includes 2,397 references -- 7 new additions since its 04/07/19 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of September 5, 2004) from:

http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 316 references to radiosity, photon mapping, and related global illumination theses -- one new addition since the 04/07/19 release.

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

Ian Ashdown, P. Eng., LC, FIES
President
byHeart Consultants Limited
http://www.helios32.com

From Return-Path: Received: from neelix.kom.tuwien.ac.at (neelix.kom.tuwien.ac.at [192.35.241.67]) by cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id i88Irf1B009248; Wed, 8 Sep 2004 20:53:42 +0200 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by neelix.kom.tuwien.ac.at (8.12.11/8.12.11) with ESMTP id i88IrWWE008083; Wed, 8 Sep 2004 20:53:35 +0200 (MEST) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id i88Il3707027; Wed, 8 Sep 2004 20:47:03 +0200 Received: from mx-serv.inrialpes.fr (mx-serv.inrialpes.fr [194.199.18.100]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id i88IkvA07009 for ; Wed, 8 Sep 2004 20:46:57 +0200 Received: from smtp.unc.edu (smtpsrv10.isis.unc.edu [152.2.1.241]) by mx-serv.inrialpes.fr (8.12.10/8.12.10) with ESMTP id i88Ikq6m023116 for ; Wed, 8 Sep 2004 20:46:52 +0200 (MEST) Received: from LT40CS (lt40-cs.cs.unc.edu [152.2.131.82]) (authenticated bits=0) by smtp.unc.edu (8.12.9/8.12.9) with ESMTP id i88IkXhX024638 for ; Wed, 8 Sep 2004 14:46:34 -0400 (EDT) Reply-To: lastra@cs.unc.edu From: "Anselmo Lastra" To: globillum@imag.fr Subject: The SBRDF Site Date: Wed, 8 Sep 2004 14:46:34 -0400 Organization: Anselmo Lastra Message-ID: <001801c495d4$2a39c150$52830298@cs.unc.edu> MIME-Version: 1.0 X-Priority: 3 (Normal) X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook, Build 10.0.2627 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1441 Importance: Normal X-SMAUG-MailScanner-Information: Please contact postmaster@inrialpes.fr for more information X-SMAUG-MailScanner: McAfee uvscan 4241 RBL+ ORBS Found to be clean X-SMAUG-MailScanner-SpamCheck: RBL+ ORBS n'est pas un polluriel, SpamAssassin (score=0, requis 4.9) X-Loop: globillum@imag.fr X-Sequence: 278 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -49 X-Spam-Level: - X-Spam-TU-Processing-Host: neelix X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit I'm sending this for Dave McAllister. ====== We would like to announce the SBRDF web site. Spatial Bi-directional Reflectance Distribution Functions are reflectance functions that vary over both the incident and exitant hemispheres and spatially over the surface. Acquiring, compressing and rendering SBRDFs was the topic of my dissertation two years ago. I'm finally making my data sets available publicly. We (Dave McAllister and Anselmo Lastra) have acquired data sets with up to 8000 poses over an anisotropic BRDF domain, with avg. 0.15 mm per pixel over the surface. The data are available in raw CCD pixels; rectified, registered reflectance values in RGBE; or final compressed SBRDF texture maps. Also, check out the result images and videos, and the list of relevant papers that we're aware of. Also, this site can be a clearing house for sharing information on all aspects of acquiring and rendering with spatially-varying reflectance. Let us know if you'd like us to link to your site or papers, or if you have any news items or data sets to add. http://www.cs.unc.edu/sbrdf DaveMc ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id i91527uJ009368; Fri, 1 Oct 2004 07:02:07 +0200 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.12.11/8.12.11) with ESMTP id i9151xZk003958; Fri, 1 Oct 2004 07:02:02 +0200 (MEST) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id i914tPp16737; Fri, 1 Oct 2004 06:55:25 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id i914pPO16394 for ; Fri, 1 Oct 2004 06:51:25 +0200 Received: from pd3mo3so.prod.shaw.ca (shawidc-mo1.cg.shawcable.net [24.71.223.10]) by imag.imag.fr (8.13.0/8.13.0) with ESMTP id i914pKPA007478 for ; Fri, 1 Oct 2004 06:51:22 +0200 (CEST) Received: from pd4mr2so.prod.shaw.ca (pd4mr2so-qfe3.prod.shaw.ca [10.0.141.213]) by l-daemon (Sun ONE Messaging Server 6.0 HotFix 1.01 (built Mar 15 2004)) with ESMTP id <0I4W0076901HOND0@l-daemon> for globillum@imag.fr; Thu, 30 Sep 2004 21:51:17 -0600 (MDT) Received: from pn2ml10so.prod.shaw.ca ([10.0.121.80]) by pd4mr2so.prod.shaw.ca (Sun ONE Messaging Server 6.0 HotFix 1.01 (built Mar 15 2004)) with ESMTP id <0I4W00HCT01HY0K0@pd4mr2so.prod.shaw.ca> for globillum@imag.fr; Thu, 30 Sep 2004 21:51:17 -0600 (MDT) Received: from BLUEBERRY (S01060006257abbc2.vn.shawcable.net [24.87.171.230]) by l-daemon (iPlanet Messaging Server 5.2 HotFix 1.18 (built Jul 28 2003)) with SMTP id <0I4W004CS01FZU@l-daemon> for globillum@imag.fr; Thu, 30 Sep 2004 21:51:17 -0600 (MDT) Date: Thu, 30 Sep 2004 20:55:56 -0700 From: Ian Ashdown Subject: ANNOUNCE: 04/10/01 Release of RADBIB and GITHESIS To: globillum@imag.fr Reply-to: Ian Ashdown Message-id: <000f01c4a76a$8e500f80$6501a8c0@BLUEBERRY> Organization: byHeart Consultants Limited MIME-version: 1.0 X-MIMEOLE: Produced By Microsoft MimeOLE V6.00.2800.1441 X-Mailer: Microsoft Outlook Express 6.00.2800.1437 Content-type: text/html; charset=windows-1252 X-Priority: 3 X-MSMail-priority: Normal X-Greylist: Delayed for 01:00:02 by milter-greylist-1.4 (imag.imag.fr [129.88.30.1]); Fri, 01 Oct 2004 06:51:22 +0200 (CEST) X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Loop: globillum@imag.fr X-Sequence: 279 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; 9 X-Spam-Level: +++++++++ X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

ANNOUNCE: 04/10/01 Release of RADBIB and GITHESIS
RADBIB is a comprehensive bibliography of radiosity, photon mapping, and related global illumination papers, theses, articles, and books. It currently includes 2,405 references -- 7 new additions since its 04/09/05 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of October 1, 2004) from:

http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 316 references to radiosity, photon mapping, and related global illumination theses -- no new additions since the 04/09/05 release.

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

Ian Ashdown, P. Eng., LC, FIES
President
byHeart Consultants Limited
http://www.helios32.com

From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id iB2JN3BF005184; Thu, 2 Dec 2004 20:23:05 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.13.1/8.13.1) with ESMTP id iB2JMrih020409; Thu, 2 Dec 2004 20:22:56 +0100 (MET) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id iB2JGK412056; Thu, 2 Dec 2004 20:16:20 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id iB2JDOm11476 for ; Thu, 2 Dec 2004 20:13:24 +0100 Received: from cut.autodesk.com (cut.autodesk.com [198.102.112.47]) by imag.imag.fr (8.13.0/8.13.0) with ESMTP id iB2JDLJM026086 for ; Thu, 2 Dec 2004 20:13:23 +0100 (CET) Received: from msgusawfe01.ads.autodesk.com ([144.111.33.210]) by cut.autodesk.com (8.13.0/8.12.6) with ESMTP id iB2H3dtD004979 for ; Thu, 2 Dec 2004 09:04:27 -0800 (PST) Received: from msgusawpf01.ads.autodesk.com ([144.111.33.212]) by msgusawfe01.ads.autodesk.com with Microsoft SMTPSVC(5.0.2195.6713); Thu, 2 Dec 2004 09:04:20 -0800 Received: from msgusaepf01.ads.autodesk.com ([144.111.72.51]) by msgusawpf01.ads.autodesk.com with Microsoft SMTPSVC(5.0.2195.6713); Thu, 2 Dec 2004 09:04:20 -0800 Received: from msgusaemb01.ads.autodesk.com ([144.111.72.50]) by msgusaepf01.ads.autodesk.com with Microsoft SMTPSVC(5.0.2195.6713); Thu, 2 Dec 2004 12:04:17 -0500 X-MimeOLE: Produced By Microsoft Exchange V6.0.6603.0 Content-Class: urn:content-classes:message MIME-Version: 1.0 Content-Type: text/html; charset=windows-1252 Subject: The Fantasy Graphics League 2005 season has begun Date: Thu, 2 Dec 2004 12:04:16 -0500 Message-ID: Thread-Topic: The Fantasy Graphics League 2005 season has begun Thread-Index: AcTYkPP/uW1rdLsJRtS4mqrGV1gbeQ== From: "Eric Haines" To: globillum@imag.fr X-OriginalArrivalTime: 02 Dec 2004 17:04:17.0069 (UTC) FILETIME=[F50285D0:01C4D890] X-Greylist: Delayed for 02:08:48 by milter-greylist-1.4 (imag.imag.fr [129.88.30.1]); Thu, 02 Dec 2004 20:13:23 +0100 (CET) X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Loop: globillum@imag.fr X-Sequence: 284 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -47 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

http://www.realtimerendering.com/fgl/siggraph2005/index.htm

 

I was going to quit running this thing, but Mark Harris talked me into doing it again, and kindly is hosting the Perl scripts.

 

Have fun,

 

Eric

From Return-Path: Received: from neelix.kom.tuwien.ac.at (neelix.kom.tuwien.ac.at [192.35.241.67]) by cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id iBDGUNBF018001; Mon, 13 Dec 2004 17:30:23 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by neelix.kom.tuwien.ac.at (8.13.1/8.13.1) with ESMTP id iBDGU9SV028356; Mon, 13 Dec 2004 17:30:12 +0100 (MET) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id iBDGNRL13417; Mon, 13 Dec 2004 17:23:27 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id iBDGNGx13399 for ; Mon, 13 Dec 2004 17:23:16 +0100 Received: from mail.officeworks-uk.com (mail.officeworks-uk.com [195.152.206.150] (may be forged)) by imag.imag.fr (8.13.0/8.13.0) with ESMTP id iBDGNAMG008303 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO) for ; Mon, 13 Dec 2004 17:23:12 +0100 (CET) Received: from elvis.lightwork (elvis.lightwork [192.9.200.30]) by mail.officeworks-uk.com (8.12.8/8.12.8) with ESMTP id iBDFDaos029805 for ; Mon, 13 Dec 2004 15:13:36 GMT Received: by ELVIS with Internet Mail Service (5.5.2650.21) id ; Mon, 13 Dec 2004 15:13:37 -0000 Message-ID: <8815647C7041D111A3010060B06BE1C002A7DBF8@ELVIS> From: Neil Gatenby To: globillum@imag.fr Subject: Rendering Magazine Date: Mon, 13 Dec 2004 15:13:32 -0000 MIME-Version: 1.0 X-Mailer: Internet Mail Service (5.5.2650.21) X-Greylist: Delayed for 01:09:33 by milter-greylist-1.4 (imag.imag.fr [129.88.30.1]); Mon, 13 Dec 2004 17:23:12 +0100 (CET) X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Loop: globillum@imag.fr X-Sequence: 285 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -49 X-Spam-Level: - X-Spam-TU-Processing-Host: neelix X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Well, I thought that Google had found a new CGI magazine for our delectation, but it seems I was wrong! http://www.rendermagazine.com/ ;-) Neil Neil Gatenby Senior Software Specialist LightWork Design, Rutledge House, 78 Clarkehouse Road, Sheffield, S10 2LJ, UK Tel: +44 114 266 8404, Fax: +44 114 266 1383 neil.gatenby@lightworkdesign.com, http://www.lightworkdesign.com/ ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from neelix.kom.tuwien.ac.at (neelix.kom.tuwien.ac.at [192.35.241.67]) by cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id iBQLBHBF026171; Sun, 26 Dec 2004 22:11:20 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by neelix.kom.tuwien.ac.at (8.13.1/8.13.1) with ESMTP id iBQLB8Rf004120; Sun, 26 Dec 2004 22:11:11 +0100 (MET) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id iBQL4Wm20515; Sun, 26 Dec 2004 22:04:33 +0100 Received: from mx-serv.inrialpes.fr (mx-serv.inrialpes.fr [194.199.18.100]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id iBQL3Lx20468 for ; Sun, 26 Dec 2004 22:03:21 +0100 Received: from mail59.megamailservers.com (mail59.megamailservers.com [216.251.36.59]) by mx-serv.inrialpes.fr (8.13.0/8.13.0) with SMTP id iBQL39mX025379 for ; Sun, 26 Dec 2004 22:03:11 +0100 (MET) X-POP-User: sales.helios32.com Received: from FEBRUARY (S01060006257abbc2.vn.shawcable.net [24.87.171.230]) by mail59.megamailservers.com (8.13.1/8.13.1) with ESMTP id iBQL2jL0011006 for ; Sun, 26 Dec 2004 16:02:50 -0500 Message-Id: <200412262102.iBQL2jL0011006@mail59.megamailservers.com> From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: 04/12/26 Release of RADBIB and GITHESIS Date: Sun, 26 Dec 2004 13:02:49 -0800 Organization: byHeart Consultants Limited MIME-Version: 1.0 Content-Type: text/html; charset=windows-1252 X-Mailer: Microsoft Office Outlook, Build 11.0.6353 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2900.2180 Thread-Index: AcTrjkIAL3KtpNIjRiiUORKGL8jaGQ== X-SMAUG-MailScanner: Found to be clean Envelope-From: ian_ashdown@helios32.com Envelope-To: globillum@imag.fr X-Loop: globillum@imag.fr X-Sequence: 287 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; 2 X-Spam-Level: ++ X-Spam-TU-Processing-Host: neelix X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit ANNOUNCE: 04/12/26 Release of RADBIB and GITHESIS

ANNOUNCE: 04/12/26 Release of RADBIB and GITHESIS

RADBIB is a comprehensive bibliography of radiosity, photon mapping, and related global illumination papers, theses, articles, and books. It currently includes 2,431 references -- 26 new additions since its 04/10/01 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of December 26, 2004) from:

  http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 318 references to radiosity, photon mapping, and related global illumination theses -- two new additions since the 04/10/01 release.

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

Ian Ashdown, P. Eng., LC, FIES

President

byHeart Consultants Limited

http://www.helios32.com

From Return-Path: Received: from neelix.kom.tuwien.ac.at (neelix.kom.tuwien.ac.at [192.35.241.67]) by cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id j0PJPqMX001593; Tue, 25 Jan 2005 20:25:52 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by neelix.kom.tuwien.ac.at (8.13.1/8.13.1) with ESMTP id j0PJPhb9021434; Tue, 25 Jan 2005 20:25:45 +0100 (MET) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: (from sympa@localhost) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) id j0PJJBv00598; Tue, 25 Jan 2005 20:19:11 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.11.6/8.11.6/ImagV2) with ESMTP id j0PJIZ500579 for ; Tue, 25 Jan 2005 20:18:35 +0100 Received: from nut.autodesk.com (nut.autodesk.com [198.102.112.27]) by imag.imag.fr (8.13.0/8.13.0) with ESMTP id j0PJIVo9023745 for ; Tue, 25 Jan 2005 20:18:33 +0100 (CET) Received: from msgusawfe02.ads.autodesk.com ([144.111.33.211]) by nut.autodesk.com (8.13.0/8.12.6) with ESMTP id j0PEhn0A002903 for ; Tue, 25 Jan 2005 06:43:51 -0800 (PST) Received: from msgusawmb01.ads.autodesk.com ([144.111.33.217]) by msgusawfe02.ads.autodesk.com with Microsoft SMTPSVC(5.0.2195.6713); Tue, 25 Jan 2005 06:43:49 -0800 Received: from msgusaefe01.ads.autodesk.com ([144.111.72.49]) by msgusawmb01.ads.autodesk.com with Microsoft SMTPSVC(5.0.2195.6713); Tue, 25 Jan 2005 06:43:49 -0800 Received: from msgusaemb01.ads.autodesk.com ([144.111.72.50]) by msgusaefe01.ads.autodesk.com with Microsoft SMTPSVC(5.0.2195.6713); Tue, 25 Jan 2005 09:43:47 -0500 X-MimeOLE: Produced By Microsoft Exchange V6.0.6603.0 Content-Class: urn:content-classes:message MIME-Version: 1.0 Content-Type: text/html; charset=windows-1252 Subject: Last chance for your FGL entry Date: Tue, 25 Jan 2005 09:43:47 -0500 Message-ID: Thread-Topic: Last chance for your FGL entry Thread-Index: AcUC7EeJ/mXZf7kaQbmvOTokhO14Hw== From: "Eric Haines" To: globillum@imag.fr X-OriginalArrivalTime: 25 Jan 2005 14:43:47.0949 (UTC) FILETIME=[472B61D0:01C502EC] X-Greylist: Delayed for 04:34:37 by milter-greylist-1.4 (imag.imag.fr [129.88.30.1]); Tue, 25 Jan 2005 20:18:33 +0100 (CET) X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Loop: globillum@imag.fr X-Sequence: 288 Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -47 X-Spam-Level: - X-Spam-TU-Processing-Host: neelix X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

January 26th. To some, the SIGGRAPH deadline. As important, if you're insane, it's also the Fantasy Graphics League (FGL) deadline.

 

A SIGGRAPH paper can gain you the respect of your peers, help you get tenure, perhaps land you a dream job. Winning the FGL just shows you're a geek. But, the FGL takes about 10 minutes to choose a lame-o team, while a lame SIGGRAPH paper can take hours, if not days, to write. Meet one deadline. Meet both. Your choice:

 

http://www.realtimerendering.com/fgl/siggraph2005/index.htm

 

Have fun,

 

Eric

From Return-Path: Received: from neelix.kom.tuwien.ac.at (neelix.kom.tuwien.ac.at [192.35.241.67]) by cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id j13HdeAv020471; Thu, 3 Feb 2005 18:39:40 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by neelix.kom.tuwien.ac.at (8.13.1/8.13.1) with ESMTP id j13HdXZT011860; Thu, 3 Feb 2005 18:39:33 +0100 (MET) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11/8.12.11/ImagV2.1) with ESMTP id j13He2GN005145; Thu, 3 Feb 2005 18:40:02 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11/8.12.11/Submit) id j13He1b6005140; Thu, 3 Feb 2005 18:40:01 +0100 X-Authentication-Warning: chopinette.imag.fr: sympa set sender to globillum-owner@imag.fr using -f Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.12.11/8.12.11/ImagV2.1) with ESMTP id j13HcFcC004130 for ; Thu, 3 Feb 2005 18:38:15 +0100 Received: from cut.autodesk.com (cut.autodesk.com [198.102.112.47]) by imag.imag.fr (8.13.0/8.13.0) with ESMTP id j13HbZZ0012076 for ; Thu, 3 Feb 2005 18:37:37 +0100 (CET) Received: from msgusawfe02.ads.autodesk.com ([144.111.33.211]) by cut.autodesk.com (8.13.0/8.12.6) with ESMTP id j13Fen6D003026 for ; Thu, 3 Feb 2005 07:40:51 -0800 (PST) Received: from msgusawpf01.ads.autodesk.com ([144.111.33.212]) by msgusawfe02.ads.autodesk.com with Microsoft SMTPSVC(5.0.2195.6713); Thu, 3 Feb 2005 07:40:49 -0800 Received: from msgusaefe01.ads.autodesk.com ([144.111.72.49]) by msgusawpf01.ads.autodesk.com with Microsoft SMTPSVC(5.0.2195.6713); Thu, 3 Feb 2005 07:40:48 -0800 Received: from msgusaemb01.ads.autodesk.com ([144.111.72.50]) by msgusaefe01.ads.autodesk.com with Microsoft SMTPSVC(5.0.2195.6713); Thu, 3 Feb 2005 10:40:47 -0500 X-MimeOLE: Produced By Microsoft Exchange V6.0.6603.0 MIME-Version: 1.0 Subject: GPU open source ray tracer Date: Thu, 3 Feb 2005 10:40:47 -0500 Message-ID: Thread-Topic: GPU open source ray tracer Thread-Index: AcUKBrkiEg/INLqwRfS2Y0M/uw6Paw== From: "Eric Haines" To: globillum@imag.fr X-OriginalArrivalTime: 03 Feb 2005 15:40:47.0796 (UTC) FILETIME=[BB465F40:01C50A06] X-Greylist: Delayed for 01:56:42 by milter-greylist-1.4 (imag.imag.fr [129.88.30.1]); Thu, 03 Feb 2005 18:37:37 +0100 (CET) X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Loop: globillum@imag.fr X-Sequence: 290 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/html; charset=windows-1252 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -48 X-Spam-Level: - X-Spam-TU-Processing-Host: neelix X-Mozilla-Status: 9001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Content-Class: urn:content-classes:message Content-Type: multipart/alternative; boundary="----_=_NextPart_001_01C50A06.BB188D90"

In case Ulf doesn’t know about this list (I haven’t seen any posting from him), I thought I’d pass this on. I had been wondering when someone would make an open-source ray tracer for GPUs; now I know. Cool, there are two!

 

Eric

 

 

Ulf Assarsson ulf.assarsson@illuminatelabs.com writes:

 

In case it interests you, I just wanted to inform that we (Filip Karlsson, Carl Johan Ljungstedt and Ulf Assarsson) submitted an open source GPU ray tracer to GPGPU. It is part of a master thesis project - I'm having the supervisor role nowadays, but I've been deeply involved in this project...

 

The practical contribution is that we actually got it working under OpenGL and Cg, which has been very messy with all driver bugs, Cg-compiler bugs, and unwritten "features" of the PixelShader 3.0-support of the NV 6800. Theoretically, it is not very hard to write a GPU-ray tracer, but in practice it was a totally different story, and we have spent at least 3 months more or less full time. Our hope is that people will use it as a startup for continued research/development or whatever to boost evolution of GPU-ray tracing. As a small research contribution, we also test standard grids vs. grids and proximity clouds. The largest model we tested was the classic Buddha of 1M triangles.

 

Home page with thesis report and open source here: http://www.ce.chalmers.se/edu/proj/raygpu/

 

There is also a very nice "competitor" work :-), by Martin Christen, published the same day at GPGPU, here: http://www.clockworkcoders.com/oglsl/rt/

 

His version is also open source and uses Direct3D and HLSL. He also has a version running with NVEmulateTool under OpenGL and GLSL, but unfortunately that version does not yet work on the real hardware (6800) due to driver bugs. I've been testing his Direct3D-ray tracer some and it works fine. He has an own implemented CPU ray tracer that he compares performance against, while we use Mental Ray.

 

Both Christen's and our version can import 3DS-files, although the shading of course is much more limited than in 3DStudio.

 

Ulf

 

 

------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id j18CYPAv022806; Tue, 8 Feb 2005 13:34:25 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.13.1/8.13.1) with ESMTP id j18CYIvZ003631; Tue, 8 Feb 2005 13:34:21 +0100 (MET) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11/8.12.11/ImagV2.1) with ESMTP id j18CYFCN015285; Tue, 8 Feb 2005 13:34:15 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11/8.12.11/Submit) id j18CYBr6015274; Tue, 8 Feb 2005 13:34:11 +0100 X-Authentication-Warning: chopinette.imag.fr: sympa set sender to globillum-owner@imag.fr using -f Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.12.11/8.12.11/ImagV2.1) with ESMTP id j18CX4fp014267 for ; Tue, 8 Feb 2005 13:33:04 +0100 Received: from cg.tuwien.ac.at (mail.cg.tuwien.ac.at [128.131.166.76]) by imag.imag.fr (8.13.0/8.13.0) with ESMTP id j18CWseW020776 (version=TLSv1/SSLv3 cipher=EDH-RSA-DES-CBC3-SHA bits=168 verify=NO) for ; Tue, 8 Feb 2005 13:32:58 +0100 (CET) Received: from Beinhart.cg.tuwien.ac.at (beinhart.cg.tuwien.ac.at [128.131.166.14]) by cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id j18CLnB0021699; Tue, 8 Feb 2005 13:21:51 +0100 Message-Id: <6.0.0.22.2.20050208131837.0343f900@christl.cg.tuwien.ac.at> X-Sender: wp@christl.cg.tuwien.ac.at (Unverified) X-Mailer: QUALCOMM Windows Eudora Version 6.0.0.22 Date: Tue, 08 Feb 2005 13:20:51 +0100 To: globillum@imag.fr From: Werner Purgathofer Subject: Second Call for EG Workshop on Computational Aesthetics Mime-Version: 1.0 X-Greylist: Delayed for 00:10:34 by milter-greylist-1.4 (imag.imag.fr [129.88.30.1]); Tue, 08 Feb 2005 13:32:58 +0100 (CET) X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-Information: Please contact the ISP for more information X-MIME-Autoconverted: from quoted-printable to 8bit by chopinette.imag.fr id j18CX4fp014267 X-Loop: globillum@imag.fr X-Sequence: 291 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -49 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Dear Colleagues, The submission deadline of the one-page abstract for the First EG Workshop on Computational Aesthetics in Graphics, Visualization and Imaging is 15 March 2005. The aim of the workshop is to set a starting sign for this new, emerging discipline. For further details please visit our web-site at www.computational-aesthetics.org Location: the sunny Girona near to Barcelona, SPAIN Dates: 18 - 20 May, 2005 Invited speakers: - Oliver Deussen - Antal Nemcsics - David Salesin Organizers: Laszlo Neumann (E), Mateu Sbert (E), Bruce Gooch (US), Werner Purgathofer (A) ----------------- more information: ----------------- EUROGRAPHICS WORKSHOP on Computational Aesthetics in Graphics, Visualization, and Imaging 18 - 20 May, 2005 in Girona, Spain Call for Participation This will be the first EG workshop on Computational Aesthetics in Graphics, Visualization and Imaging, to take place in sunny Spain, in Girona which is near to Barcelona. The goal of this event is to enable experts of computer graphics, visualization, coloristic and imaging to meet and discuss various aspects of this emerging interdisciplinary area. The new discipline of Computational Aesthetics is an experimentally based scientific field and not a philosophically based modern version of art. The goals, methods, and scholarly endeavor of interest to the respective communities are different. Accordingly this workshop will deal with the applied rather than the philosophical nature of aesthetics. Computational Aesthetics provides tools for the graphics and visualization communities to increase the value of displayed imagery and to avoid classical artifacts. Beginning work in the area demonstrates examples of effective techniques and provides a methodology that will generalize to a broader class of problems. This iterative two-part process consists of using artistic computer graphics techniques to enhance the presentation of important data features, then conducting perceptual studies to evaluate the effectiveness of the resulting imagery. The strength of this approach lies in the synergy achieved in the tight coupling of these research areas. The workshop shall ensure further possibilities for researchers dealing with partly overlapping areas like non-photorealistic rendering or applied perception. Workshop topics include but are not restricted to - Optimal view point selection (artistic and/or representative visualization) - Automatic Lighting Design, Image Relighting Techniques - Non-Photorealistic Rendering, Painting-like rendering, Drawing - Artistic Textures, Patterns, Ornaments, Tiling - Sketching, Simplification techniques, Technical and Medical Illustration - Computational Color Harmony, Color Dynamics, Color Environmental Design - Color Preferences / Effects and Roles of Colors - Colorization of gray-scale images, Pseudo-Coloring techniques - Color Style Transfer Techniques between Images - Image Analogies - Applied Visual Perception (Color Appearance, Spatial Vision and other aspects) - Perceptual / Cognitive High Dynamic Range Imaging - Artistic Image Transformation Techniques - Generalized Image Synthesis (nonlinear mappings, spaces, rays, camera models) - Image Style Analysis (paintings, photographs, others) - Composition, Visual Balance, Layout - Design of Geometrical and Fractal Scenes - Image and Scene Complexity, Image Appearance, Image Quality - Empirically based Metrics of Aesthetical Attributes Participation can be with or without an oral presentation. To apply for a talk, please send a one-page abstract of your intended topic by 15 March, 2005. Topics do not have to be unpublished research, but should either highlight the aesthetic aspects or contain new ideas in this direction. Talks will be 20 minutes plus 20 minutes discussion. A selection of submitted abstracts will be done on a pure thematic judgment, notification will happen before 31 March, 2005. During the workshop the organizers together with the participants will define those papers which shall be included in a full color proceedings volume published by Eurographics. Organizers: László Neumann (E), Mateu Sbert (E), Bruce Gooch (US), Werner Purgathofer (A) For further details please visit our web-site at www.computational-aesthetics.org -- Werner Purgathofer | Tel. +43(1)58801 18648 Technische Universitaet Wien | http://www.cg.tuwien.ac.at ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from neelix.kom.tuwien.ac.at (neelix.kom.tuwien.ac.at [192.35.241.67]) by cg.tuwien.ac.at (8.12.3/8.12.3/Debian-6.6) with ESMTP id j1FCT5Av022368; Tue, 15 Feb 2005 13:29:09 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by neelix.kom.tuwien.ac.at (8.13.1/8.13.1) with ESMTP id j1FCSwJ5017481; Tue, 15 Feb 2005 13:28:58 +0100 (MET) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11/8.12.11/ImagV2.1) with ESMTP id j1FCSo2k024737; Tue, 15 Feb 2005 13:28:50 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11/8.12.11/Submit) id j1FCSjBE024706; Tue, 15 Feb 2005 13:28:45 +0100 X-Authentication-Warning: chopinette.imag.fr: sympa set sender to globillum-owner@imag.fr using -f Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.12.11/8.12.11/ImagV2.1) with ESMTP id j1FCSQ4s023737 for ; Tue, 15 Feb 2005 13:28:26 +0100 Received: from mail.officeworks-uk.com (mail.officeworks-uk.com [195.152.206.150]) by imag.imag.fr (8.13.0/8.13.0) with ESMTP id j1FCSO3X019529 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO) for ; Tue, 15 Feb 2005 13:28:25 +0100 (CET) Received: from elvis.lightwork (elvis.lightwork [192.9.200.30]) by mail.officeworks-uk.com (8.12.8/8.12.8) with ESMTP id j1FBZE7c000310 for ; Tue, 15 Feb 2005 11:35:20 GMT Received: by ELVIS with Internet Mail Service (5.5.2650.21) id ; Tue, 15 Feb 2005 11:37:59 -0000 Message-ID: <8815647C7041D111A3010060B06BE1C002B9789E@ELVIS> From: Neil Gatenby To: globillum@imag.fr Subject: GI benchmark Date: Tue, 15 Feb 2005 11:37:55 -0000 MIME-Version: 1.0 X-Mailer: Internet Mail Service (5.5.2650.21) X-Greylist: Delayed for 00:50:03 by milter-greylist-1.4 (imag.imag.fr [129.88.30.1]); Tue, 15 Feb 2005 13:28:25 +0100 (CET) X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Loop: globillum@imag.fr X-Sequence: 292 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -49 X-Spam-Level: - X-Spam-TU-Processing-Host: neelix X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hi I have a contact that is referring to the "teapots on wall" benchmark scene, for photon tracing. Anybody here know which model that is? TIA Neil Neil Gatenby Senior Software Specialist LightWork Design, Rutledge House, 78 Clarkehouse Road, Sheffield, S10 2LJ, UK Tel: +44 114 266 8404, Fax: +44 114 266 1383 neil.gatenby@lightworkdesign.com, http://www.lightworkdesign.com/ ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by cg.tuwien.ac.at (8.12.3/8.12.3/Debian-7.1) with ESMTP id j22DaLCP032138; Wed, 2 Mar 2005 14:36:21 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.13.1/8.13.1) with ESMTP id j22DaB3P014504; Wed, 2 Mar 2005 14:36:16 +0100 (MET) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11/8.12.11/ImagV2.1) with ESMTP id j22DZuHG025248; Wed, 2 Mar 2005 14:35:56 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11/8.12.11/Submit) id j22DZu0Z025243; Wed, 2 Mar 2005 14:35:56 +0100 X-Authentication-Warning: chopinette.imag.fr: sympa set sender to globillum-owner@imag.fr using -f Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.12.11/8.12.11/ImagV2.1) with ESMTP id j22DZhwx024129 for ; Wed, 2 Mar 2005 14:35:43 +0100 Received: from cg.tuwien.ac.at (mail.cg.tuwien.ac.at [128.131.166.76]) by imag.imag.fr (8.13.0/8.13.0) with ESMTP id j22DZrNb024402 (version=TLSv1/SSLv3 cipher=EDH-RSA-DES-CBC3-SHA bits=168 verify=NO) for ; Wed, 2 Mar 2005 14:35:54 +0100 (CET) Received: from Beinhart.cg.tuwien.ac.at (beinhart.cg.tuwien.ac.at [128.131.166.14]) by cg.tuwien.ac.at (8.12.3/8.12.3/Debian-7.1) with ESMTP id j22DMUCS030996 for ; Wed, 2 Mar 2005 14:22:35 +0100 Message-Id: <6.0.0.22.2.20050302133000.01d28880@christl.cg.tuwien.ac.at> X-Sender: wp@christl.cg.tuwien.ac.at (Unverified) X-Mailer: QUALCOMM Windows Eudora Version 6.0.0.22 Date: Wed, 02 Mar 2005 13:34:54 +0100 To: globillum@imag.fr From: Werner Purgathofer Subject: Open Position in Vienna Mime-Version: 1.0 X-Greylist: Delayed for 00:13:17 by milter-greylist-1.4 (imag.imag.fr [129.88.30.1]); Wed, 02 Mar 2005 14:35:54 +0100 (CET) X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Loop: globillum@imag.fr X-Sequence: 294 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -49 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Dear globillum members, I'm looking for a PhD student for a research project on real-time illumination of trees. Details can be found here: http://www.cg.tuwien.ac.at/jobs/treelumination_opening.html If you know a good candidate, please contact me. If possible, please also forward this to other interested parties. Thanks, Michael Wimmer -- -- Dr. Michael Wimmer-------------------------------------------------------- Institute of Computer Graphics and Algorithms tel: +43 (1) 58801 18687 Vienna University of Technology fax: +43 (1) 58801 18698 Favoritenstr. 9-11/5/E186 http://www.cg.tuwien.ac.at A-1040 Vienna, Austria mailto:wimmer@cg.tuwien.ac.at ----------------------------------------------------------------------------- -- Werner Purgathofer | Tel. +43(1)58801 18648 Technische Universitaet Wien | http://www.cg.tuwien.ac.at ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by cg.tuwien.ac.at (8.12.3/8.12.3/Debian-7.1) with ESMTP id j22HfJCP020954; Wed, 2 Mar 2005 18:41:19 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.13.1/8.13.1) with ESMTP id j22HfBjA021699; Wed, 2 Mar 2005 18:41:16 +0100 (MET) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11/8.12.11/ImagV2.1) with ESMTP id j22HeoFD026924; Wed, 2 Mar 2005 18:40:50 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11/8.12.11/Submit) id j22HenBW026918; Wed, 2 Mar 2005 18:40:49 +0100 X-Authentication-Warning: chopinette.imag.fr: sympa set sender to globillum-owner@imag.fr using -f Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.12.11/8.12.11/ImagV2.1) with ESMTP id j22HebbM025940 for ; Wed, 2 Mar 2005 18:40:37 +0100 Received: from nic.funet.fi (nic.funet.fi [193.166.3.1]) by imag.imag.fr (8.13.0/8.13.0) with ESMTP id j22HXF8G007176 (version=TLSv1/SSLv3 cipher=EDH-RSA-DES-CBC3-SHA bits=168 verify=FAIL) for ; Wed, 2 Mar 2005 18:33:17 +0100 (CET) Received: (from localhost user: 'kouhia' uid#241 fake: STDIN (kouhia@nic.funet.fi)) by nic.funet.fi id S9593AbVCBQmv for ; Wed, 2 Mar 2005 18:42:51 +0200 Sender: Juhana Sadeharju From: Juhana Sadeharju To: globillum@imag.fr Subject: PRT / Ambient Occlusion? Message-Id: Date: Wed, 2 Mar 2005 18:42:51 +0200 X-Greylist: Delayed for 00:50:19 by milter-greylist-1.4 (imag.imag.fr [129.88.30.1]); Wed, 02 Mar 2005 18:33:17 +0100 (CET) X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Loop: globillum@imag.fr X-Sequence: 295 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; 8 X-Spam-Level: ++++++++ X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 MIME-Version: 1.0 Content-transfer-encoding: 8bit This is a multi-part message in MIME format... ------------=_1109785245-13911-18 Hello. Would anyone have a GPL (or equivalent) source code for generating Precomputed Radiance Transfer values? Crystal Space game engine (crystal.sourceforge.net) would need such code. Sad to hear that Ambient Occlusion has been patented. I myself invented the same basic idea several years ago. I also had an another idea for computing the same effect: negative light sources. Numerous negative light sources are placed to positions which would yield the same effect. Because the negative light sources would be local, the algorithm is suitable for parallel processing in similar manner than the AO algorithm. Are there other non-patented alternative algorithms for generating the "Ambient Occlusion" effect? Juhana -- http://music.columbia.edu/mailman/listinfo/linux-graphics-dev for developers of open source graphics software ------------=_1109785245-13911-18 Content-Type: text/plain; name="message-footer.txt" Content-Disposition: inline; filename="message-footer.txt" Content-Transfer-Encoding: 8bit ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- ------------=_1109785245-13911-18-- From Return-Path: Received: from neelix.kom.tuwien.ac.at (neelix.kom.tuwien.ac.at [192.35.241.67]) by cg.tuwien.ac.at (8.12.3/8.12.3/Debian-7.1) with ESMTP id j22JkVCP030328; Wed, 2 Mar 2005 20:46:31 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by neelix.kom.tuwien.ac.at (8.13.1/8.13.1) with ESMTP id j22JkLT6026984; Wed, 2 Mar 2005 20:46:28 +0100 (MET) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11/8.12.11/ImagV2.1) with ESMTP id j22Jk1rO011846; Wed, 2 Mar 2005 20:46:01 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11/8.12.11/Submit) id j22Jk1GJ011841; Wed, 2 Mar 2005 20:46:01 +0100 X-Authentication-Warning: chopinette.imag.fr: sympa set sender to globillum-owner@imag.fr using -f Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.12.11/8.12.11/ImagV2.1) with ESMTP id j22JjlqW010863 for ; Wed, 2 Mar 2005 20:45:47 +0100 Received: from warhol.graphics.cornell.edu (warhol.graphics.cornell.edu [128.84.247.228]) by imag.imag.fr (8.13.0/8.13.0) with ESMTP id j22JjuAl007599 for ; Wed, 2 Mar 2005 20:45:57 +0100 (CET) Received: from diesel.graphics.cornell.edu (diesel.graphics.cornell.edu [128.84.247.211]) by warhol.graphics.cornell.edu (Postfix) with ESMTP id D9B8A30177 for ; Wed, 2 Mar 2005 14:24:49 -0500 (EST) Sender: westin@graphics.cornell.edu To: globillum@imag.fr Subject: Re: PRT / Ambient Occlusion? References: Reply-To: westin@graphics.cornell.edu From: westin@graphics.cornell.edu X-Home-Page: http://www.graphics.cornell.edu/~westin Date: 02 Mar 2005 14:24:49 -0500 In-Reply-To: Message-ID: Lines: 15 User-Agent: Gnus/5.09 (Gnus v5.9.0) Emacs/21.3.50 MIME-Version: 1.0 X-PCG-MailScanner-Information: For more info see http://www.graphics.cornell.edu/spam X-PCG-MailScanner: Found to be clean X-PCG-MailScanner-SpamCheck: not spam (whitelisted), SpamAssassin (score=-4.717, required 5, AWL 0.02, BAYES_00 -4.90, NO_REAL_NAME 0.16) X-Greylist: Delayed for 00:20:59 by milter-greylist-1.4 (imag.imag.fr [129.88.30.1]); Wed, 02 Mar 2005 20:45:57 +0100 (CET) X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Loop: globillum@imag.fr X-Sequence: 296 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -12 X-Spam-Level: - X-Spam-TU-Processing-Host: neelix X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Juhana Sadeharju writes: > Sad to hear that Ambient Occlusion has been patented. By whom? It would be nice to have a patent number. -- -Stephen H. Westin Any information or opinions in this message are mine: they do not represent the position of Cornell University or any of its sponsors. ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from neelix.kom.tuwien.ac.at (neelix.kom.tuwien.ac.at [192.35.241.67]) by cg.tuwien.ac.at (8.12.3/8.12.3/Debian-7.1) with ESMTP id j2KKAiVZ004203; Sun, 20 Mar 2005 21:10:44 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by neelix.kom.tuwien.ac.at (8.13.1/8.13.1) with ESMTP id j2KKAYsx019039; Sun, 20 Mar 2005 21:10:41 +0100 (MET) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11/8.12.11/ImagV2.1) with ESMTP id j2KKA4gj012657; Sun, 20 Mar 2005 21:10:05 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11/8.12.11/Submit) id j2KKA05e012649; Sun, 20 Mar 2005 21:10:00 +0100 X-Authentication-Warning: chopinette.imag.fr: sympa set sender to globillum-owner@imag.fr using -f Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.12.11/8.12.11/ImagV2.1) with ESMTP id j2KK76ma012343 for ; Sun, 20 Mar 2005 21:07:06 +0100 Received: from mail96.megamailservers.com (mail96.megamailservers.com [216.251.36.96]) by imag.imag.fr (8.13.0/8.13.0) with ESMTP id j2KK7QaY005736 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO) for ; Sun, 20 Mar 2005 21:07:28 +0100 (CET) X-POP-User: sales.helios32.com Received: from FEBRUARY (S01060006257abbc2.vn.shawcable.net [24.87.171.230]) by mail96.megamailservers.com (8.13.1/8.13.1) with ESMTP id j2KHavah018135 for ; Sun, 20 Mar 2005 12:37:02 -0500 Message-Id: <200503201737.j2KHavah018135@mail96.megamailservers.com> From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: 05/03/20 Release of RADBIB and GITHESIS Date: Sun, 20 Mar 2005 09:37:01 -0800 Organization: byHeart Consultants Limited MIME-Version: 1.0 X-Mailer: Microsoft Office Outlook, Build 11.0.6353 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2900.2527 Thread-Index: AcUtc2xRz/Jlh087RqaGQ+2S9wewcA== X-Greylist: Delayed for 02:30:16 by milter-greylist-1.6 (imag.imag.fr [129.88.30.1]); Sun, 20 Mar 2005 21:07:28 +0100 (CET) X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Loop: globillum@imag.fr X-Sequence: 299 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/html; charset=windows-1252 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -32 X-Spam-Level: - X-Spam-TU-Processing-Host: neelix X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

ANNOUNCE: 05/03/20 Release of RADBIB and GITHESIS

RADBIB is a comprehensive bibliography of radiosity, photon mapping, and related global illumination papers, theses, articles, and books. It currently includes 2,436 references -- 5 new additions since its 04/12/26 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of March 20, 2005) from:

  http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 319 references to radiosity, photon mapping, and related global illumination theses -- one new addition since the 04/12/26 release.

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

 

Ian Ashdown, P. Eng., LC, FIES

President

byHeart Consultants Limited

http://www.helios32.com

 

------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from neelix.kom.tuwien.ac.at (neelix.kom.tuwien.ac.at [192.35.241.67]) by cg.tuwien.ac.at (8.12.3/8.12.3/Debian-7.1) with ESMTP id j3BC8NVZ015213; Mon, 11 Apr 2005 14:08:23 +0200 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by neelix.kom.tuwien.ac.at (8.13.1/8.13.1) with ESMTP id j3BC8DYL014333; Mon, 11 Apr 2005 14:08:20 +0200 (MEST) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11/8.12.11/ImagV2.1) with ESMTP id j3BC7XEB004094; Mon, 11 Apr 2005 14:07:33 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11/8.12.11/Submit) id j3BC7OCa004048; Mon, 11 Apr 2005 14:07:24 +0200 X-Authentication-Warning: chopinette.imag.fr: sympa set sender to globillum-owner@imag.fr using -f Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.12.11/8.12.11/ImagV2.1) with ESMTP id j3BC7Bu3004026 for ; Mon, 11 Apr 2005 14:07:11 +0200 Received: from mail.officeworks-uk.com (mail.officeworks-uk.com [195.152.206.150]) by imag.imag.fr (8.13.0/8.13.0) with ESMTP id j3BC7jdp015963 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO) for ; Mon, 11 Apr 2005 14:07:47 +0200 (CEST) Received: from elvis.lightwork (elvis.lightwork [192.9.200.30]) by mail.officeworks-uk.com (8.12.8/8.12.8) with ESMTP id j3BBST5b019494; Mon, 11 Apr 2005 12:28:30 +0100 Received: by ELVIS with Internet Mail Service (5.5.2650.21) id ; Mon, 11 Apr 2005 12:28:26 +0100 Message-ID: <8815647C7041D111A3010060B06BE1C002C3B2AA@ELVIS> From: Neil Gatenby To: globillum@imag.fr Cc: eric.haines@autodesk.com Subject: RE: GI benchmark Date: Mon, 11 Apr 2005 12:28:25 +0100 MIME-Version: 1.0 X-Mailer: Internet Mail Service (5.5.2650.21) X-Greylist: Delayed for 00:39:06 by milter-greylist-1.6 (imag.imag.fr [129.88.30.1]); Mon, 11 Apr 2005 14:07:47 +0200 (CEST) X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Loop: globillum@imag.fr X-Sequence: 300 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -49 X-Spam-Level: - X-Spam-TU-Processing-Host: neelix X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hi Eric Hi all Neil wrote: > I have a contact that is referring to the "teapots on wall" benchmark > scene, for photon tracing. > > Anybody here know which model that is? Eric Haines replied: > I hadn't heard of that one, really, though I vaguely recall a scene like > that somewhere. If you *do* figure it out, please let me (us all) know, > as I'd like to mention it in the Ray Tracing News. Look what I found ... http://www.ixor.gr/maxwelltest/maxwell.htm points us at http://ixor.gr/maxwelltest/teapottest.zip ;-) http://www.ixor.gr/maxwelltest/tea.htm contains many images from different renderers All the best Neil Neil Gatenby Senior Software Specialist LightWork Design, Rutledge House, 78 Clarkehouse Road, Sheffield, S10 2LJ, UK Tel: +44 114 266 8404, Fax: +44 114 266 1383 neil.gatenby@lightworkdesign.com, http://www.lightworkdesign.com/ ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by cg.tuwien.ac.at (8.12.3/8.12.3/Debian-7.1) with ESMTP id j4B70TVZ032530; Wed, 11 May 2005 09:00:29 +0200 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.13.1/8.13.1) with ESMTP id j4B70FEI007798; Wed, 11 May 2005 09:00:22 +0200 (MEST) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11/8.12.11/ImagV2.1) with ESMTP id j4B6xILS030486; Wed, 11 May 2005 08:59:18 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11/8.12.11/Submit) id j4B6xBPe030473; Wed, 11 May 2005 08:59:11 +0200 X-Authentication-Warning: chopinette.imag.fr: sympa set sender to globillum-owner@imag.fr using -f Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.12.11/8.12.11/ImagV2.1) with ESMTP id j4B6ttKI029470 for ; Wed, 11 May 2005 08:55:55 +0200 Received: from mail113.megamailservers.com (mail113.megamailservers.com [216.251.36.113]) by imag.imag.fr (8.13.0/8.13.0) with ESMTP id j4B6ukDf015079 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO) for ; Wed, 11 May 2005 08:56:49 +0200 (CEST) X-POP-User: sales.helios32.com Received: from FEBRUARY (S01060006257abbc2.vn.shawcable.net [24.87.171.230]) by mail113.megamailservers.com (8.13.1/8.13.1) with ESMTP id j4B332ij004592 for ; Tue, 10 May 2005 23:03:07 -0400 Message-Id: <200505110303.j4B332ij004592@mail113.megamailservers.com> From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: 05/05/10 Release of RADBIB and GITHESIS Date: Tue, 10 May 2005 20:03:01 -0700 Organization: byHeart Consultants Limited MIME-Version: 1.0 X-Mailer: Microsoft Office Outlook, Build 11.0.6353 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2900.2527 Thread-Index: AcVV1fD+9veiDXnpTQ+6B7jACZi6mQ== X-Greylist: Delayed for 03:53:34 by milter-greylist-1.6 (imag.imag.fr [129.88.30.1]); Wed, 11 May 2005 08:56:49 +0200 (CEST) X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Loop: globillum@imag.fr X-Sequence: 302 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/html; charset=windows-1252 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -32 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

ANNOUNCE: 05/05/10 Release of RADBIB and GITHESIS

RADBIB is a comprehensive bibliography of radiosity, photon mapping, and related global illumination papers, theses, articles, and books. It currently includes 2,448 references -- 12 new additions since its 05/03/20 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of May 10, 2005) from:

  http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 319 references to radiosity, photon mapping, and related global illumination theses -- no new additions since the 05/03/20 release.

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

Ian Ashdown, P. Eng., LC, FIES

President

byHeart Consultants Limited

http://www.helios32.com

 

 

------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by cg.tuwien.ac.at (8.12.3/8.12.3/Debian-7.1) with ESMTP id j4CG1rVZ001855; Thu, 12 May 2005 18:01:53 +0200 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.13.1/8.13.1) with ESMTP id j4CG1kbk025890; Thu, 12 May 2005 18:01:51 +0200 (MEST) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11/8.12.11/ImagV2.1) with ESMTP id j4CG0kMH001706; Thu, 12 May 2005 18:00:46 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11/8.12.11/Submit) id j4CG0iSb001700; Thu, 12 May 2005 18:00:44 +0200 X-Authentication-Warning: chopinette.imag.fr: sympa set sender to globillum-owner@imag.fr using -f Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.12.11/8.12.11/ImagV2.1) with ESMTP id j4CFwhjp000443 for ; Thu, 12 May 2005 17:58:43 +0200 Received: from nut.autodesk.com (nut.autodesk.com [198.102.112.27]) by imag.imag.fr (8.13.0/8.13.0) with ESMTP id j4CFxWAA029706 for ; Thu, 12 May 2005 17:59:34 +0200 (CEST) Received: from msgusawfe01.ads.autodesk.com ([144.111.33.210]) by nut.autodesk.com (8.13.0/8.12.6) with ESMTP id j4CEr71Z020735 for ; Thu, 12 May 2005 07:53:09 -0700 (PDT) Received: from msgusawpf01.ads.autodesk.com ([144.111.33.212]) by msgusawfe01.ads.autodesk.com with Microsoft SMTPSVC(5.0.2195.6713); Thu, 12 May 2005 07:53:07 -0700 Received: from msgusaemb01.ads.autodesk.com ([144.111.72.50]) by msgusawpf01.ads.autodesk.com with Microsoft SMTPSVC(5.0.2195.6713); Thu, 12 May 2005 07:53:07 -0700 X-MimeOLE: Produced By Microsoft Exchange V6.0.6603.0 MIME-Version: 1.0 Subject: FGL results Date: Thu, 12 May 2005 10:53:05 -0400 Message-ID: Thread-Topic: FGL results Thread-Index: AcVXAk2qaGnwYmIRQgi41+dVb5bhLw== From: "Eric Haines" To: globillum@imag.fr X-OriginalArrivalTime: 12 May 2005 14:53:07.0199 (UTC) FILETIME=[4EB568F0:01C55702] X-Greylist: Delayed for 01:06:17 by milter-greylist-1.6 (imag.imag.fr [129.88.30.1]); Thu, 12 May 2005 17:59:35 +0200 (CEST) X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Loop: globillum@imag.fr X-Sequence: 303 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/html; charset=windows-1252 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -47 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit content-class: urn:content-classes:message Content-Type: multipart/alternative; boundary="----_=_NextPart_001_01C55702.4DF66668"

Are the monkeys or the humans ahead? The Fantasy Graphics League preliminary (pre-sketches) results are up at: http://www.realtimerendering.com/fgl/siggraph2005/index.htm

 

Enjoy,

 

Eric

 

 

------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by cg.tuwien.ac.at (8.13.4/8.13.4/Debian-3) with ESMTP id j5M4ZDXq003941; Wed, 22 Jun 2005 06:35:13 +0200 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.13.1/8.13.1) with ESMTP id j5M4YvF9026619; Wed, 22 Jun 2005 06:35:02 +0200 (MEST) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11/8.12.11/ImagV2.1) with ESMTP id j5M4XSH5015489; Wed, 22 Jun 2005 06:33:28 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11/8.12.11/Submit) id j5M4XFXU015476; Wed, 22 Jun 2005 06:33:15 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.12.11/8.12.11/ImagV2.1) with ESMTP id j5M4UHDL014465 for ; Wed, 22 Jun 2005 06:30:17 +0200 Received: from cut.autodesk.com (cut.autodesk.com [198.102.112.47]) by imag.imag.fr (8.13.0/8.13.0) with ESMTP id j5M4VZqM010169 for ; Wed, 22 Jun 2005 06:31:37 +0200 (CEST) Received: from msgusawfe01.ads.autodesk.com ([144.111.33.210]) by cut.autodesk.com (8.13.0/8.12.6) with ESMTP id j5M3tGT0019680 for ; Tue, 21 Jun 2005 20:55:23 -0700 (PDT) Received: from msgusawmb01.ads.autodesk.com ([144.111.33.217]) by msgusawfe01.ads.autodesk.com with Microsoft SMTPSVC(5.0.2195.6713); Tue, 21 Jun 2005 20:55:19 -0700 Received: from msgusaemb01.ads.autodesk.com ([144.111.72.50]) by msgusawmb01.ads.autodesk.com with Microsoft SMTPSVC(5.0.2195.6713); Tue, 21 Jun 2005 20:55:19 -0700 X-MimeOLE: Produced By Microsoft Exchange V6.0.6603.0 MIME-Version: 1.0 Subject: Fantasy Graphics League results are in Date: Tue, 21 Jun 2005 23:55:18 -0400 Message-ID: Thread-Topic: Fantasy Graphics League results are in thread-index: AcV23WONIDfQjkcsTrGiEwa62O/6yQ== From: "Eric Haines" To: globillum@imag.fr X-OriginalArrivalTime: 22 Jun 2005 03:55:19.0428 (UTC) FILETIME=[35053C40:01C576DE] X-Greylist: Delayed for 00:36:09 by milter-greylist-1.6 (imag.imag.fr [129.88.30.1]); Wed, 22 Jun 2005 06:31:38 +0200 (CEST) X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Loop: globillum@imag.fr X-Sequence: 305 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/html; charset=windows-1252 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -47 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Content-class: urn:content-classes:message Content-Type: multipart/alternative; boundary="----_=_NextPart_001_01C576DE.343D9AC8"

And waiting for you to soak in their hand-crafted pixels: http://www.realtimerendering.com/fgl/siggraph2005/index.htm

 

Enjoy,

 

Eric

------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by cg.tuwien.ac.at (8.13.4/8.13.4/Debian-3) with ESMTP id j63JcrWI023676; Sun, 3 Jul 2005 21:38:53 +0200 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.13.1/8.13.1) with ESMTP id j63JcK8R024262; Sun, 3 Jul 2005 21:38:26 +0200 (MEST) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11/8.12.11/ImagV2.1) with ESMTP id j63Ibdo2010054; Sun, 3 Jul 2005 20:37:39 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11/8.12.11/Submit) id j63IbXgR010046; Sun, 3 Jul 2005 20:37:33 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.12.11/8.12.11/ImagV2.1) with ESMTP id j63IYnIG009030 for ; Sun, 3 Jul 2005 20:34:49 +0200 Received: from mail191.megamailservers.com (mail191.megamailservers.com [216.251.36.191]) by imag.imag.fr (8.13.0/8.13.0) with ESMTP id j63JZKIV025956 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO) for ; Sun, 3 Jul 2005 21:35:22 +0200 (CEST) X-POP-User: sales.helios32.com Received: from FEBRUARY (S01060006257abbc2.vn.shawcable.net [24.87.171.230]) by mail191.megamailservers.com (8.13.1/8.13.1) with ESMTP id j63Gn8YS022552 for ; Sun, 3 Jul 2005 12:49:14 -0400 Message-Id: <200507031649.j63Gn8YS022552@mail191.megamailservers.com> From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: 05/07/03 Release of RADBIB and GITHESIS Date: Sun, 3 Jul 2005 09:49:11 -0700 Organization: byHeart Consultants Limited MIME-Version: 1.0 X-Mailer: Microsoft Office Outlook, Build 11.0.6353 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2900.2527 Thread-Index: AcV/7yMwO8zqpRR6TMKvLT/zUmK/8Q== X-Greylist: Delayed for 02:46:04 by milter-greylist-1.6 (imag.imag.fr [129.88.30.1]); Sun, 03 Jul 2005 21:35:23 +0200 (CEST) X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Loop: globillum@imag.fr X-Sequence: 307 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/html; charset=windows-1252 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -32 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

ANNOUNCE: 05/07/03 Release of RADBIB and GITHESIS

RADBIB is a comprehensive bibliography of radiosity, photon mapping, and related global illumination papers, theses, articles, and books. It currently includes 2,459 references -- 11 new additions since its 05/05/10 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of July 3, 2005) from:

  http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 319 references to radiosity, photon mapping, and related global illumination theses -- no new additions since the 05/05/10 release.

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

Ian Ashdown, P. Eng., LC, FIES

President

byHeart Consultants Limited

http://www.helios32.com

 

------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by cg.tuwien.ac.at (8.13.4/8.13.4/Debian-3) with ESMTP id j7KM5PQp004889; Sun, 21 Aug 2005 00:05:25 +0200 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.13.1/8.13.1) with ESMTP id j7KM3jGP006779; Sun, 21 Aug 2005 00:03:52 +0200 (MEST) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11/8.12.11/ImagV2.1) with ESMTP id j7KL2fnO010007; Sat, 20 Aug 2005 23:02:41 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11/8.12.11/Submit) id j7KL2TVY009993; Sat, 20 Aug 2005 23:02:29 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.12.11/8.12.11/ImagV2.1) with ESMTP id j7KKwd2p008754 for ; Sat, 20 Aug 2005 22:58:39 +0200 Received: from mail181.megamailservers.com (mail181.megamailservers.com [216.251.36.181]) by imag.imag.fr (8.13.0/8.13.0) with ESMTP id j7KLxaM7015151 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO) for ; Sat, 20 Aug 2005 23:59:38 +0200 (CEST) X-POP-User: sales.helios32.com Received: from FEBRUARY (S01060006257abbc2.vn.shawcable.net [24.87.171.230]) by mail181.megamailservers.com (8.13.1/8.13.1) with ESMTP id j7KHXloS005802 for ; Sat, 20 Aug 2005 13:33:52 -0400 Message-Id: <200508201733.j7KHXloS005802@mail181.megamailservers.com> From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: 05/08/20 Release of RADBIB and GITHESIS Date: Sat, 20 Aug 2005 10:33:44 -0700 Organization: byHeart Consultants Limited MIME-Version: 1.0 X-Mailer: Microsoft Office Outlook, Build 11.0.6353 Thread-Index: AcWlrVBDb/2TIczmQbetPzl0s61kZg== X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2900.2527 X-Greylist: Delayed for 04:25:38 by milter-greylist-1.6 (imag.imag.fr [129.88.30.1]); Sat, 20 Aug 2005 23:59:38 +0200 (CEST) X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Loop: globillum@imag.fr X-Sequence: 308 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/html; charset=windows-1252 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -32 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

ANNOUNCE: 05/08/20 Release of RADBIB and GITHESIS

RADBIB is a comprehensive bibliography of radiosity, photon mapping, and related global illumination papers, theses, articles, and books. It currently includes 2,480 references -- 21 new additions since its 05/07/03 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of August 20, 2005) from:

  http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 319 references to radiosity, photon mapping, and related global illumination theses -- no new additions since the 05/07/03 release.

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

 

NOTE: All references marked with an asterisk in the title (e.g., Abe97-TDISR*) are in our corporate library in either electronic or printed format. If you have exhausted all other avenues for obtaining a copy of an obscure paper or thesis, please contact Ian Ashdown at ian_ashdown@helios32.com for assistance.

 

Ian Ashdown, P. Eng., LC, FIES

President

byHeart Consultants Limited

http://www.helios32.com

 

------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from neelix.kom.tuwien.ac.at (neelix.kom.tuwien.ac.at [192.35.241.67]) by cg.tuwien.ac.at (8.13.4/8.13.4/Debian-3) with ESMTP id jA5KprtS002251; Sat, 5 Nov 2005 21:51:53 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by neelix.kom.tuwien.ac.at (8.13.1/8.13.1) with ESMTP id jA5KpdND016187; Sat, 5 Nov 2005 21:51:46 +0100 (MET) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11/8.12.11/ImagV2.1) with ESMTP id jA5KoxP4001779; Sat, 5 Nov 2005 21:50:59 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11/8.12.11/Submit) id jA5KosKf001774; Sat, 5 Nov 2005 21:50:54 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.12.11/8.12.11/ImagV2.1) with ESMTP id jA5KmvjT032278 for ; Sat, 5 Nov 2005 21:48:57 +0100 Received: from mail97.megamailservers.com (mail97.megamailservers.com [216.251.36.97]) by imag.imag.fr (8.13.0/8.13.0) with ESMTP id jA5KnWur010847 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO) for ; Sat, 5 Nov 2005 21:49:34 +0100 (CET) X-POP-User: sales.helios32.com Received: from IAN (S01060006257abbc2.vn.shawcable.net [24.87.171.230]) by mail97.megamailservers.com (8.13.1/8.13.1) with ESMTP id jA5IrVGu017015 for ; Sat, 5 Nov 2005 13:53:38 -0500 From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: 05/11/05 Release of RADBIB and GITHESIS Date: Sat, 5 Nov 2005 10:53:43 -0800 Organization: byHeart Consultants Limited Message-ID: <002401c5e23a$41feb800$6401a8c0@IAN> MIME-Version: 1.0 X-Mailer: Microsoft Office Outlook 11 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2900.2527 Thread-Index: AcXiOj6TcPO0+YuYTIWBrHFn/mt4lw== X-Greylist: Delayed for 01:55:46 by milter-greylist-1.6 (imag.imag.fr [129.88.30.1]); Sat, 05 Nov 2005 21:49:34 +0100 (CET) X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Loop: globillum@imag.fr X-Sequence: 309 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/html; charset=windows-1252 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -31 X-Spam-Level: - X-Spam-TU-Processing-Host: neelix X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

ANNOUNCE: 05/11/05 Release of RADBIB and GITHESIS

 

RADBIB is a comprehensive bibliography of radiosity, photon mapping, and related global illumination papers, theses, articles, and books. It currently includes 2,499 references -- 19 new additions since its 05/08/20 release.

 

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of November 5, 2005) from:

 

  http://www.helios32.com (Resources section)

 

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 319 references to radiosity, photon mapping, and related global illumination theses -- no new additions since the 05/08/20 release.

 

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

 

NOTE: All papers marked with an asterisk in the title (e.g., Abe97-TDISR*) are in our corporate library in either electronic or printed format. If you have exhausted all other avenues for obtaining a copy of an obscure paper, please contact Ian Ashdown at ian_ashdown@helios32.com.

 

Ian Ashdown, P. Eng., LC, FIES

President

byHeart Consultants Limited

http://www.helios32.com

 

------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by cg.tuwien.ac.at (8.13.4/8.13.4/Debian-3) with ESMTP id jA8GiXBu025234; Tue, 8 Nov 2005 17:44:33 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.13.1/8.13.1) with ESMTP id jA8GiKXi007615; Tue, 8 Nov 2005 17:44:26 +0100 (MET) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11/8.12.11/ImagV2.1) with ESMTP id jA8GhcFB019791; Tue, 8 Nov 2005 17:43:38 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11/8.12.11/Submit) id jA8Ghbo6019787; Tue, 8 Nov 2005 17:43:37 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.12.11/8.12.11/ImagV2.1) with ESMTP id jA8GhIUO018821 for ; Tue, 8 Nov 2005 17:43:19 +0100 Received: from smtp102.sbc.mail.mud.yahoo.com (smtp102.sbc.mail.mud.yahoo.com [68.142.198.201]) by imag.imag.fr (8.13.0/8.13.0) with SMTP id jA8Ghupm012526 for ; Tue, 8 Nov 2005 17:43:57 +0100 (CET) Received: (qmail 21001 invoked from network); 8 Nov 2005 16:17:16 -0000 Received: from unknown (HELO ?65.74.199.104?) (gregoryjward@65.74.199.104 with plain) by smtp102.sbc.mail.mud.yahoo.com with SMTP; 8 Nov 2005 16:17:16 -0000 Mime-Version: 1.0 References: <200511081224.jA8COIUZ021090@gmoblfmail3.net.vodafone.it> Message-Id: Cc: Stefania Nardelli From: Greg Ward Subject: Fwd: Tone Reproduction Operators Date: Tue, 8 Nov 2005 09:17:26 -0700 To: globillum@imag.fr X-Mailer: Apple Mail (2.746.2) X-Greylist: Delayed for 00:26:38 by milter-greylist-1.6 (imag.imag.fr [129.88.30.1]); Tue, 08 Nov 2005 17:43:58 +0100 (CET) X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Loop: globillum@imag.fr X-Sequence: 310 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -34 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Dear All, Does anyone have or know of a selection of Matlab tone-mapping operators? The following person asked me about it, and all the implementations I know of are in C. Many of these were done by Erik Reinhard, and are included on the DVD-ROM of his (our) new HDR Imaging book. I think he may even put them on the website at some point , but he's probably waiting for the book to hit the shelves, first. -Greg Begin forwarded message: > From: "Stefania Nardelli" > Date: November 8, 2005 5:24:18 AM MST > > Hi, > > I'm looking for Tone Mapping Operators > for High Dynamic Range Imaging implemented in Matlab. > > I found iCam operator in Munsell Color Lab's website, > can you help me about other tone mapping operators in Matlab > or can you tell me if someone can help me, please? > > Best regards, > Stefania Nardelli ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from neelix.kom.tuwien.ac.at (neelix.kom.tuwien.ac.at [192.35.241.67]) by cg.tuwien.ac.at (8.13.4/8.13.4/Debian-3) with ESMTP id jAR0Z9Hn028464; Sun, 27 Nov 2005 01:35:09 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by neelix.kom.tuwien.ac.at (8.13.1/8.13.1) with ESMTP id jAR0Z0th008527; Sun, 27 Nov 2005 01:35:06 +0100 (MET) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11/8.12.11/ImagV2.1) with ESMTP id jAR0XxlQ003193; Sun, 27 Nov 2005 01:33:59 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11/8.12.11/Submit) id jAR0XnBO003185; Sun, 27 Nov 2005 01:33:49 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.12.11/8.12.11/ImagV2.1) with ESMTP id jAR0U9en002172 for ; Sun, 27 Nov 2005 01:30:09 +0100 Received: from mail98.megamailservers.com (mail98.megamailservers.com [216.251.36.98]) by imag.imag.fr (8.13.0/8.13.0) with ESMTP id jAR0UwPr022582 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO) for ; Sun, 27 Nov 2005 01:31:00 +0100 (CET) X-POP-User: sales.helios32.com Received: from IAN (S01060006257abbc2.vn.shawcable.net [24.87.171.230]) by mail98.megamailservers.com (8.13.1/8.13.1) with ESMTP id jAQNEL5q004769 for ; Sat, 26 Nov 2005 18:14:27 -0500 From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE - 05/11/26 Release of RADBIB and GITHESIS Date: Sat, 26 Nov 2005 15:14:25 -0800 Organization: byHeart Consultants Limited Message-ID: <000f01c5f2df$25f85e30$6501a8c0@IAN> MIME-Version: 1.0 X-Mailer: Microsoft Office Outlook 11 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2900.2527 Thread-Index: AcXy3yRzbAjICjrOQx+U6HDCHn4wIA== X-Greylist: Delayed for 01:16:28 by milter-greylist-1.6 (imag.imag.fr [129.88.30.1]); Sun, 27 Nov 2005 01:31:00 +0100 (CET) X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Loop: globillum@imag.fr X-Sequence: 311 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/html; charset=windows-1252 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -32 X-Spam-Level: - X-Spam-TU-Processing-Host: neelix X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

ANNOUNCE: 05/11/26 Release of RADBIB and GITHESIS

RADBIB is a comprehensive bibliography of radiosity, photon mapping, and related global illumination papers, theses, articles, and books. It currently includes 2,524 references -- 25 new additions since its 05/11/05 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of November 26, 2005) from:

  http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 320 references to radiosity, photon mapping, and related global illumination theses -- one new addition since the 05/11/05 release.

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

NOTE: All papers marked with an asterisk in the title (e.g., Abe97-TDISR*) are in our corporate library in either electronic or printed format. If you have exhausted all other avenues for obtaining a copy of an obscure paper, please contact Ian Ashdown at ian_ashdown@helios32.com.

Ian Ashdown, P. Eng., LC, FIES
President
byHeart Consultants Limited
http://www.helios32.com

 

------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from neelix.kom.tuwien.ac.at (neelix.kom.tuwien.ac.at [192.35.241.67]) by cg.tuwien.ac.at (8.13.4/8.13.4/Debian-3) with ESMTP id jB5BWTe1026447; Mon, 5 Dec 2005 12:32:30 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by neelix.kom.tuwien.ac.at (8.13.1/8.13.1) with ESMTP id jB5BWEOx026961; Mon, 5 Dec 2005 12:32:20 +0100 (MET) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11/8.12.11/ImagV2.1) with ESMTP id jB5BVBjN011889; Mon, 5 Dec 2005 12:31:11 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11/8.12.11/Submit) id jB5BV6oY011884; Mon, 5 Dec 2005 12:31:06 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.12.11/8.12.11/ImagV2.1) with ESMTP id jB5BS6SQ010630 for ; Mon, 5 Dec 2005 12:28:06 +0100 Received: from cg.tuwien.ac.at (mail.cg.tuwien.ac.at [128.131.166.76]) by imag.imag.fr (8.13.0/8.13.0) with ESMTP id jB5BSsj2012937 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO) for ; Mon, 5 Dec 2005 12:29:00 +0100 (CET) Received: from Beinhart-05.cg.tuwien.ac.at (beinhart-05.cg.tuwien.ac.at [128.131.166.9]) by cg.tuwien.ac.at (8.13.4/8.13.4/Debian-3) with ESMTP id jB5BI6Jo025021 for ; Mon, 5 Dec 2005 12:18:07 +0100 Message-Id: <6.2.0.14.2.20051205121842.03a50258@mail.cg.tuwien.ac.at> X-Mailer: QUALCOMM Windows Eudora Version 6.2.0.14 Date: Mon, 05 Dec 2005 12:18:53 +0100 To: globillum@imag.fr From: Werner Purgathofer Subject: EG2006 Call for Contributions Mime-Version: 1.0 X-Greylist: Delayed for 00:10:51 by milter-greylist-1.6 (imag.imag.fr [129.88.30.1]); Mon, 05 Dec 2005 12:29:00 +0100 (CET) X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Loop: globillum@imag.fr X-Sequence: 312 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -49 X-Spam-Level: - X-Spam-TU-Processing-Host: neelix X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Please forward to interested colleagues, and please excuse multiple postings. Thank you! ******************************************************************* EUROGRAPHICS'2006, Vienna, Austria September 4 - 8, 2006 C A L L F O R C O N T R I B U T I O N S Conference Website: www.eg.org/eg2006 Email: eg2006@eg.org ******************************************************************* From Monday, September 4th to Friday, September 8th, 2006, the Austrian Academy of Sciences in Vienna, Austria, will play host to Eurographics'2006, the 27th annual conference of the European Association for Computer Graphics. The conference program will include keynote talks from Herbert Edelsbrunner (Duke University) Reinhard Klein (University of Bonn) Jos Stam (Alias-Wavefront) Conference Co-Chairs: Werner Purgathofer (A), Sabine Coquillart (F) Program Co-Chairs: Laszlo Szirmay-Kalos (H), Eduard Groeller (A) ******************************************************************* CALL FOR PAPERS * deadline Febr. 6, 2006 ******************************************************************* CALL FOR STATE OF THE ART REPORTS * deadline Febr. 15, 2006 ******************************************************************* CALL FOR TUTORIALS * deadline Febr. 15, 2006 ******************************************************************* CALL FOR SHORT PAPERS * deadline April 28, 2006 ******************************************************************* CALL FOR ANIMATIONS & MULTIMEDIA * deadline April 28, 2006 ******************************************************************* CALL FOR RESEARCH CENTRE PRESENTATIONS * deadline April 28, 2006 ******************************************************************* CALL FOR EDUCATION PAPERS * deadline April 28, 2006 ******************************************************************* CALL FOR GAME DEMOS * deadline April 28, 2006 ******************************************************************* Co-located with Eurographics'2006 the following 5 events will take place in Vienna: * Symposium on Computer Animation (2-4 September) * Workshop on Sketch Based Interfaces and Modeling (3-4 September) * Workshop on Graphics Hardware (3-5 September) * Workshop on Natural Phenomena (5 September) * Workshop on Graphics Education (9 September) For all details about Eurographics'2006 in Vienna including links to the 5 other events see www.eg.org/eg2006 ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by cg.tuwien.ac.at (8.13.4/8.13.4/Debian-3) with ESMTP id jBDHFbQI004839; Tue, 13 Dec 2005 18:15:39 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.13.1/8.13.1) with ESMTP id jBDHFMwr022216; Tue, 13 Dec 2005 18:15:32 +0100 (MET) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11/8.12.11/ImagV2.1) with ESMTP id jBDHEDcQ019532; Tue, 13 Dec 2005 18:14:13 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11/8.12.11/Submit) id jBDHEC4R019527; Tue, 13 Dec 2005 18:14:12 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.12.11/8.12.11/ImagV2.1) with ESMTP id jBDHCJfN018508 for ; Tue, 13 Dec 2005 18:12:19 +0100 Received: from paste.autodesk.com (paste.autodesk.com [198.102.112.48]) by imag.imag.fr (8.13.0/8.13.0) with ESMTP id jBDHDBBv005453 for ; Tue, 13 Dec 2005 18:13:13 +0100 (CET) Received: from msgusawfe01.ads.autodesk.com ([144.111.33.210]) by paste.autodesk.com (8.13.0/8.12.6) with ESMTP id jBDFRUjD021285 for ; Tue, 13 Dec 2005 07:27:32 -0800 (PST) Received: from msgusawpf01.ads.autodesk.com ([144.111.33.212]) by msgusawfe01.ads.autodesk.com with Microsoft SMTPSVC(5.0.2195.6713); Tue, 13 Dec 2005 07:27:30 -0800 Received: from msgusaepf01.ads.autodesk.com ([144.111.72.51]) by msgusawpf01.ads.autodesk.com with Microsoft SMTPSVC(5.0.2195.6713); Tue, 13 Dec 2005 07:27:30 -0800 Received: from msgusaemb02.ads.autodesk.com ([144.111.72.54]) by msgusaepf01.ads.autodesk.com with Microsoft SMTPSVC(5.0.2195.6713); Tue, 13 Dec 2005 10:30:08 -0500 X-MimeOLE: Produced By Microsoft Exchange V6.0.6603.0 MIME-Version: 1.0 Subject: Ray Tracing News vol.18 no.1 is out Date: Tue, 13 Dec 2005 10:30:08 -0500 Message-ID: Thread-Topic: Ray Tracing News vol.18 no.1 is out thread-index: AcX/+hkedNzv8H4lRKuw0ZKxbR0K5A== From: "Eric Haines" To: globillum@imag.fr X-OriginalArrivalTime: 13 Dec 2005 15:30:08.0438 (UTC) FILETIME=[197BD560:01C5FFFA] X-Greylist: Delayed for 01:45:36 by milter-greylist-1.6 (imag.imag.fr [129.88.30.1]); Tue, 13 Dec 2005 18:13:18 +0100 (CET) X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Loop: globillum@imag.fr X-Sequence: 313 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/html; charset=windows-1252 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -47 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Content-Class: urn:content-classes:message Content-Type: multipart/alternative; boundary="----_=_NextPart_001_01C5FFFA.19725614"

Come and get it:

 

http://www.acm.org/tog/resources/RTNews/html/rtnv18n1.html

 

If nothing else, check out the Ray Tracing Roundup section; lots of interesting links to resources and whatnot there.

 

Enjoy,

 

Eric

------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by cg.tuwien.ac.at (8.13.4/8.13.4/Debian-3) with ESMTP id k2NMesO9029898; Thu, 23 Mar 2006 23:40:54 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.13.6/8.13.6) with ESMTP id k2NMeiIo012784; Thu, 23 Mar 2006 23:40:52 +0100 (MET) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11/8.12.11/ImagV2.1) with ESMTP id k2NMeddU015359; Thu, 23 Mar 2006 23:40:39 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11/8.12.11/Submit) id k2NMebXO015349; Thu, 23 Mar 2006 23:40:37 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.12.11/8.12.11/ImagV2.1) with ESMTP id k2NMeJ3q014377 for ; Thu, 23 Mar 2006 23:40:19 +0100 Received: from smtp108.sbc.mail.mud.yahoo.com (smtp108.sbc.mail.mud.yahoo.com [68.142.198.207]) by imag.imag.fr (8.13.0/8.13.0) with SMTP id k2NMeEEx028781 for ; Thu, 23 Mar 2006 23:40:15 +0100 (CET) Received: (qmail 57662 invoked from network); 23 Mar 2006 22:13:34 -0000 Received: from unknown (HELO ?192.168.1.65?) (gregoryjward@63.200.48.103 with plain) by smtp108.sbc.mail.mud.yahoo.com with SMTP; 23 Mar 2006 22:13:33 -0000 Mime-Version: 1.0 Message-Id: To: globillum@imag.fr From: Greg Ward Subject: HDR animation contest Date: Thu, 23 Mar 2006 14:14:10 -0800 X-Mailer: Apple Mail (2.746.3) X-Greylist: Delayed for 00:26:39 by milter-greylist-1.6 (imag.imag.fr [129.88.30.1]); Thu, 23 Mar 2006 23:40:16 +0100 (CET) X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Loop: globillum@imag.fr X-Sequence: 316 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -48 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Apologies for the cross-posting, but there isn't 100% overlap on these lists... BrightSide Technologies is having an HDR animation contest for all those who are interested in participating: http://www.brightsidetech.com/HDRContest/HDRContest.php The field is wide open as near as I can tell. -Greg ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from neelix.kom.tuwien.ac.at (neelix.kom.tuwien.ac.at [192.35.241.67]) by cg.tuwien.ac.at (8.13.4/8.13.4/Debian-3) with ESMTP id k2O5ef9K021867; Fri, 24 Mar 2006 06:40:41 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by neelix.kom.tuwien.ac.at (8.13.6/8.13.6) with ESMTP id k2O5eW8d026595; Fri, 24 Mar 2006 06:40:40 +0100 (MET) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11/8.12.11/ImagV2.1) with ESMTP id k2O5ePs2029763; Fri, 24 Mar 2006 06:40:25 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11/8.12.11/Submit) id k2O5eIfi029758; Fri, 24 Mar 2006 06:40:18 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.12.11/8.12.11/ImagV2.1) with ESMTP id k2O5d3p6028478 for ; Fri, 24 Mar 2006 06:39:03 +0100 Received: from mail117.megamailservers.com (mail117.megamailservers.com [216.251.36.117]) by imag.imag.fr (8.13.0/8.13.0) with ESMTP id k2O5cxuU001918 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO) for ; Fri, 24 Mar 2006 06:39:01 +0100 (CET) X-POP-User: janet_ashdown.helios32.com Received: from IAN (S01060006257abbc2.vn.shawcable.net [24.82.124.200]) by mail117.megamailservers.com (8.13.1/8.13.1) with ESMTP id k2O4P0Lb026885 for ; Thu, 23 Mar 2006 23:25:07 -0500 From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE - 06/03/23 Release of Updated RADBIB and GITHESIS bibliographies Date: Thu, 23 Mar 2006 20:25:06 -0800 Organization: byHeart Consultants Limited Message-ID: <004901c64efa$ef6d3520$6501a8c0@IAN> MIME-Version: 1.0 X-Mailer: Microsoft Office Outlook 11 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2900.2527 Thread-Index: AcZO+u2LZT9xPaj7R7mSXUpIIps6Sg== X-Greylist: Delayed for 01:13:48 by milter-greylist-1.6 (imag.imag.fr [129.88.30.1]); Fri, 24 Mar 2006 06:39:01 +0100 (CET) X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-Information: Please contact the ISP for more information X-Loop: globillum@imag.fr X-Sequence: 317 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/html; charset=windows-1252 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -32 X-Spam-Level: - X-Spam-TU-Processing-Host: neelix X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

ANNOUNCE: 06/03/23 Release of RADBIB and GITHESIS

RADBIB is a comprehensive bibliography of radiosity, photon mapping, and related global illumination papers, theses, articles, and books. It currently includes 2,535 references -- 11 new additions since its 05/11/26 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of March 23, 2006) from:

    http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 320 references to radiosity, photon mapping, and related global illumination theses -- no new additions since the 05/11/26 release.

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

Ian Ashdown, P. Eng., LC, FIES
President
byHeart Consultants Limited
http://www.helios32.com



 

------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by cg.tuwien.ac.at (8.13.4/8.13.4/Debian-3sarge1) with ESMTP id k3R50rSh017387; Thu, 27 Apr 2006 07:00:53 +0200 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.13.6/8.13.6) with ESMTP id k3R50nCN001334; Thu, 27 Apr 2006 07:00:54 +0200 (MEST) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id k3R50ngW026159; Thu, 27 Apr 2006 07:00:49 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id k3R50mpr026154; Thu, 27 Apr 2006 07:00:48 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id k3R50Xkt025165 for ; Thu, 27 Apr 2006 07:00:33 +0200 Received: from mail110.megamailservers.com (mail110.megamailservers.com [216.251.36.110]) by imag.imag.fr (8.13.6/8.13.6) with ESMTP id k3R50Tfo020492 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO) for ; Thu, 27 Apr 2006 07:00:31 +0200 (CEST) X-POP-User: book.helios32.com Received: from IAN (S01060006257abbc2.vn.shawcable.net [24.82.124.200]) by mail110.megamailservers.com (8.13.6/8.13.1) with ESMTP id k3R3fQPS029801 for ; Wed, 26 Apr 2006 23:41:32 -0400 From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: "Radiosity: A Programmer's Perspective" now available for free Date: Wed, 26 Apr 2006 20:41:32 -0700 Organization: byHeart Consultants Limited Message-ID: <007701c669ac$7b016c20$6401a8c0@IAN> MIME-Version: 1.0 X-Mailer: Microsoft Office Outlook 11 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2900.2869 Thread-Index: AcZprHmGefSITGiNTH+Cji/YzpzD/Q== X-Greylist: Delayed for 01:18:55 by milter-greylist-1.6 (imag.imag.fr [129.88.30.1]); Thu, 27 Apr 2006 07:00:31 +0200 (CEST) X-IMAG-MailScanner-Information: Please contact IMAG DMI for more information X-IMAG-MailScanner: Found to be clean X-MailScanner-From: ian_ashdown@helios32.com X-Loop: globillum@imag.fr X-Sequence: 321 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/html; charset=windows-1252 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -31 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

I may regret this, but …

 

"Radiosity: A Programmer's Perspective" by Ian Ashdown (1994) is a 500-page undergraduate-level textbook on the mathematics of synthesizing photorealistic images using radiosity methods. It includes C++ source code for a fully-functional radiosity renderer that runs under MS-Windows. Out of print since 1998, the book is now available free (as in beer).

 

Please contact Book[at]Helios32.com to request a copy (PDF file, approximately 8 MB) to be delivered by e-mail.

 

Ian Ashdown, P. Eng., LC, FIES

President

byHeart Consultants Limited

http://www.helios32.com

 

------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by cg.tuwien.ac.at (8.13.4/8.13.4/Debian-3sarge1) with ESMTP id k3R4O7HY012637; Thu, 27 Apr 2006 06:24:07 +0200 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.13.6/8.13.6) with ESMTP id k3R4NvjM014563; Thu, 27 Apr 2006 06:24:05 +0200 (MEST) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id k3R4Nn3Y020959; Thu, 27 Apr 2006 06:23:49 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id k3R4NkIB020954; Thu, 27 Apr 2006 06:23:46 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id k3R4Lg24019953 for ; Thu, 27 Apr 2006 06:21:42 +0200 Received: from mail60.megamailservers.com (mail60.megamailservers.com [216.251.36.60]) by imag.imag.fr (8.13.6/8.13.6) with ESMTP id k3R4LcUQ016672 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO) for ; Thu, 27 Apr 2006 06:21:40 +0200 (CEST) X-POP-User: ian_ashdown.helios32.com Received: from IAN (S01060006257abbc2.vn.shawcable.net [24.82.124.200]) by mail60.megamailservers.com (8.13.6/8.13.1) with ESMTP id k3R3hNZL011921 for ; Wed, 26 Apr 2006 23:43:29 -0400 From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: 06/04/26 Release of RADBIB and GITHESIS Date: Wed, 26 Apr 2006 20:43:29 -0700 Organization: byHeart Consultants Limited Message-ID: <007c01c669ac$c0c56090$6401a8c0@IAN> MIME-Version: 1.0 X-Mailer: Microsoft Office Outlook 11 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2900.2869 Thread-Index: AcZprL+PZ4G1ZrGPTl6Mk9seHuv4Eg== X-Greylist: Delayed for 00:38:08 by milter-greylist-1.6 (imag.imag.fr [129.88.30.1]); Thu, 27 Apr 2006 06:21:40 +0200 (CEST) X-IMAG-MailScanner-Information: Please contact IMAG DMI for more information X-IMAG-MailScanner: Found to be clean X-MailScanner-From: ian_ashdown@helios32.com X-Loop: globillum@imag.fr X-Sequence: 320 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/html; charset=windows-1252 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -32 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

ANNOUNCE: 06/04/26 Release of RADBIB and GITHESIS

RADBIB is a comprehensive bibliography of radiosity, photon mapping, and related global illumination papers, theses, articles, and books. It currently includes 2,547 references -- 12 new additions since its 06/03/23 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of April 26, 2006) from:

  http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 320 references to radiosity, photon mapping, and related global illumination theses -- no new additions since the 06/03/23 release.

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

Ian Ashdown, P. Eng., LC, FIES
President
byHeart Consultants Limited
http://www.helios32.com

------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by cg.tuwien.ac.at (8.13.4/8.13.4/Debian-3sarge1) with ESMTP id k3UHiiBr017803; Sun, 30 Apr 2006 19:44:44 +0200 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.13.6/8.13.6) with ESMTP id k3UHiagn016055; Sun, 30 Apr 2006 19:44:42 +0200 (MEST) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id k3UHiT0h006907; Sun, 30 Apr 2006 19:44:29 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id k3UHiIjK006899; Sun, 30 Apr 2006 19:44:18 +0200 Received: from harmonie.imag.fr (harmonie.imag.fr [147.171.130.40]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id k3UHfjGv005580 for ; Sun, 30 Apr 2006 19:41:45 +0200 Received: from mail77.megamailservers.com (mail77.megamailservers.com [216.251.36.77]) by harmonie.imag.fr (8.13.6/8.13.6) with ESMTP id k3UHfbTS022335 for ; Sun, 30 Apr 2006 19:41:43 +0200 (CEST) X-POP-User: book.helios32.com Received: from IAN (S01060006257abbc2.vn.shawcable.net [24.82.124.200]) by mail77.megamailservers.com (8.13.6/8.13.1) with ESMTP id k3UHfCv6031805; Sun, 30 Apr 2006 13:41:23 -0400 From: "Ian Ashdown" To: globillum@imag.fr Cc: wout.van.bommrl@philips.com Subject: ANNOUNCE: New CIE publication Date: Sun, 30 Apr 2006 10:41:20 -0700 Organization: byHeart Consultants Limited Message-ID: <000401c66c7d$4e7cc770$6401a8c0@IAN> MIME-Version: 1.0 X-Mailer: Microsoft Office Outlook 11 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2900.2869 Thread-Index: AcZsfUpm1LNk3SyQSp+KSo5+QdnP2w== X-Greylist: Delayed for 85:59:56 by milter-greylist-1.6 (harmonie.imag.fr [147.171.130.40]); Sun, 30 Apr 2006 19:41:44 +0200 (CEST) X-IMAG-MailScanner-Information: Please contact IMAG DMI for more information X-IMAG-MailScanner: Found to be clean X-MailScanner-From: ian_ashdown@helios32.com X-Loop: globillum@imag.fr X-Sequence: 322 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/html; charset=windows-1252 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -32 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 9001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

Globillum members with an interest in the validation of global illumination algorithms and software products utilizing global illumination may be interested in the following International Lighting Commission (CIE) publication:

 

 

Test Cases to Assess the Accuracy of Lighting Computer Programs

 

CIE 171:2006

ISBN 3 901 906 47 9

 

The objective of this report is to help lighting program users and developers assess the accuracy of lighting computer programs and to identify their weaknesses. A validation approach is therefore presented based on the concept of separately testing the different aspects of light propagation. To apply this approach, a suite of test cases has been designed where each test case highlights a given aspect of the lighting simulation domain and is associated with the related reference data.

 

Two types of reference data are used: data based on analytic calculation and data based on experimental measurements. The first is associated with theoretical scenarios that avoid uncertainties in the reference values. The second type is obtained through experimental measurements, where the scenario and the protocol are defined in a manner that minimizes the uncertainties associated with the measurements.

 

A set of recommendations is also presented in order to achieve reliable experimental data for validation purposes. These recommendations address the choice and description of the scenarios, to the experimental protocol precautions, to the estimation of the error sources and to the presentation of the reference data.

 

The report consists of 97 pages with 27 figures and 65 tables.

 

The price of the publication is 72 EU. See http://www.cie.co.at for ordering information.

 

 

Ian Ashdown, P. Eng., LC, FIES

President

byHeart Consultants Limited

http://www.helios32.com

 

------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from neelix.kom.tuwien.ac.at (neelix.kom.tuwien.ac.at [192.35.241.67]) by cg.tuwien.ac.at (8.13.4/8.13.4/Debian-3sarge1) with ESMTP id k5OHwcx7023027; Sat, 24 Jun 2006 19:58:39 +0200 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by neelix.kom.tuwien.ac.at (8.13.7/8.13.7) with ESMTP id k5OHwUuS008711; Sat, 24 Jun 2006 19:58:35 +0200 (MEST) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id k5OHwTaa025585; Sat, 24 Jun 2006 19:58:29 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id k5OHwGN9025297; Sat, 24 Jun 2006 19:58:16 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id k5OHuXQD024296 for ; Sat, 24 Jun 2006 19:56:33 +0200 Received: from mail76.megamailservers.com (mail76.megamailservers.com [216.251.36.76]) by imag.imag.fr (8.13.6/8.13.6) with ESMTP id k5OHuSv5015067 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO) for ; Sat, 24 Jun 2006 19:56:31 +0200 (CEST) Received: from IAN (S01060006257abbc2.vn.shawcable.net [24.81.109.204]) by mail76.megamailservers.com (8.13.6/8.13.1) with ESMTP id k5OGsKd6000661 for ; Sat, 24 Jun 2006 12:54:26 -0400 From: "Ian Ashdown" To: globillum@imag.fr Subject: Radiometry and photometry definitions Date: Sat, 24 Jun 2006 09:54:19 -0700 Organization: byHeart Consultants Limited Message-ID: <000401c697ae$d7806f20$6401a8c0@IAN> MIME-Version: 1.0 X-Mailer: Microsoft Office Outlook 11 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2900.2869 Thread-Index: AcaXrtYKUoTxSaU9SLuuvJmkkPp7mg== X-Greylist: Delayed for 01:01:57 by milter-greylist-1.6 (imag.imag.fr [129.88.30.1]); Sat, 24 Jun 2006 19:56:31 +0200 (CEST) X-IMAG-MailScanner-Information: Please contact IMAG DMI for more information X-IMAG-MailScanner: Found to be clean X-MailScanner-From: ian_ashdown@helios32.com X-Loop: globillum@imag.fr X-Sequence: 326 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/html; charset=windows-1252 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -31 X-Spam-Level: - X-Spam-TU-Processing-Host: neelix X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

Dear colleagues:

 

The Illuminating Engineering Society of North America (www.iesna.org) has recently published:

 

ANSI/IESNA RP-16-05

Nomenclature and Definitions for Illuminating Engineering

120 pages softcover, $50 US

 

This publication includes definitions of the photometric and radiometric terms used in global illumination. (It even defines radiosity as an “old” term for radiant exitance, now used mostly by the computer graphics community.)

 

The IESNA has a five-year reaffirmation cycle for its technical publications, although RP-16 was last revised in 1996. However, the latest release is subject to the IESNA’s “continuous maintenance program,” whereby the public is encouraged to submit proposed changes to the document. Approved changes will apparently be issued electronically on an annual basis.

 

An authorized excerpt from the 1986 release of RP-16 in included in Appendix A of my book, “Radiosity: A Programmer’s Perspective.” The entire book is available for free download (free as in beer) from:

 

      http://www.helios32.com/Ashdown Radiosity.zip

 

You may need to use:

 

      http://www.helios32.com/Ashdown%20Radiosity.zip

 

with some browsers, notably (I am told) Netscape.

 

Cheers,

 

Ian Ashdown, P. Eng., LC, FIES

President

byHeart Consultants Limited

http://www.helios32.com

 

------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by cg.tuwien.ac.at (8.13.4/8.13.4/Debian-3sarge1) with ESMTP id k72ATfcc001675; Wed, 2 Aug 2006 12:29:41 +0200 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.13.7/8.13.7) with ESMTP id k72ATM25002402; Wed, 2 Aug 2006 12:29:30 +0200 (MEST) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id k72ATK7l012457; Wed, 2 Aug 2006 12:29:20 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id k72ATBw3012446; Wed, 2 Aug 2006 12:29:11 +0200 Received: from mx-serv.inrialpes.fr (mx-serv.inrialpes.fr [194.199.18.100]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id k72ARikM011087 for ; Wed, 2 Aug 2006 12:27:44 +0200 Received: from mail.vsiltd.co.uk (mail.vsiltd.co.uk [195.152.206.150]) by mx-serv.inrialpes.fr (8.13.6/8.13.0) with ESMTP id k72ARa8q025654 for ; Wed, 2 Aug 2006 12:27:38 +0200 (MEST) Received: from elvis.lightwork (slade.owshared [195.152.206.70]) by mail.vsiltd.co.uk (8.12.8/8.12.8) with ESMTP id k72AMsGP017910 for ; Wed, 2 Aug 2006 11:22:54 +0100 Received: by ELVIS with Internet Mail Service (5.5.2653.19) id <36CP28KV>; Wed, 2 Aug 2006 11:27:17 +0100 Message-ID: <8815647C7041D111A3010060B06BE1C0034FCF4F@ELVIS> From: Neil Gatenby To: globillum@imag.fr Subject: HDRI content Date: Wed, 2 Aug 2006 11:27:09 +0100 MIME-Version: 1.0 X-Mailer: Internet Mail Service (5.5.2653.19) X-Greylist: Sender is SPF-compliant, not delayed by milter-greylist-2.0.2 (mx-serv.inrialpes.fr [194.199.18.100]); Wed, 02 Aug 2006 12:27:38 +0200 (MEST) X-mx-serv-inrialpes-fr-MailScanner-Information: Please contact postmaster@inrialpes.fr for more information X-mx-serv-inrialpes-fr-MailScanner: Found to be clean X-mx-serv-inrialpes-fr-MailScanner-SpamCheck: n'est pas un polluriel, SpamAssassin (score=0, requis 6) X-mx-serv-inrialpes-fr-MailScanner-From: neil.gatenby@lightworkdesign.com X-Spam-Status: LOW ; -49 X-Spam-Status: No X-Loop: globillum@imag.fr X-Sequence: 327 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hi all Seems strange writing to a .fr email address, when the whole of France is still on holiday, but hopefully the rest of the world is reading! I've a question about HDR images, and the relation between the colours I find in the file, and the real-world values that a light meter might have captured, had it been there at the time of image capture. What is the relationship? I'm finding that loads of the content I'm getting my hands on is not "deep" at all. I'll have a "sun in sky" image where the sun is only 100x brighter than the darkest parts of the image - this seems to be really common - I have lots of data, and very little is truly HDR I can see that there must be a camera response curve in there somewhere, and that the combination of different exposures in one HDRI will further complicate the issue. Does anyone know of any published work in this field? Any mappings from so-called HDRIs to truly HDRIs? (e.g., the user says they want 6 log units in their result) I'm importance-sampling HDRIs in a prerender step, and then using those "N distant lights" during rendering, but I don't get a sharp shadow from the sun cos the sample(s) that are sat on the sun are not THAT much brighter than the other samples out there. Any input much appreciated Cheers Neil P.S. Anyone got any precis reports on what was cool at the Rendering Symposium, or SIGGRAPH? Neil Gatenby Senior Software Specialist Lightwork Design, Rutledge House, 78 Clarkehouse Road, Sheffield, S10 2LJ, UK Tel: +44 114 266 8404, Fax: +44 114 1383 neil.gatenby@lightworkdesign.com, http://www.lightworkdesign.com/ ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by cg.tuwien.ac.at (8.13.4/8.13.4/Debian-3sarge1) with ESMTP id k734AnLK002399; Thu, 3 Aug 2006 06:10:49 +0200 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.13.7/8.13.7) with ESMTP id k734AdVR007548; Thu, 3 Aug 2006 06:10:46 +0200 (MEST) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id k734AYI5016475; Thu, 3 Aug 2006 06:10:34 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id k734AS6G016468; Thu, 3 Aug 2006 06:10:28 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id k7348tx3013266 for ; Thu, 3 Aug 2006 06:09:00 +0200 Received: from imeil.udg.es (imeil.udg.es [130.206.45.97]) by imag.imag.fr (8.13.6/8.13.6) with ESMTP id k733KkVA005704 for ; Thu, 3 Aug 2006 05:20:47 +0200 (CEST) Received: from imeil.udg.es (avirimeil.udg.es [130.206.45.95]) by imeil.udg.es (8.11.6/out/otb) with ESMTP id k72IA9r15247 for ; Wed, 2 Aug 2006 20:10:09 +0200 Received: from morisca.udg.es (correu.udg.es [130.206.127.29]) by imeil.udg.es (8.11.6/in/otb) with ESMTP id k72IA4D15202; Wed, 2 Aug 2006 20:10:09 +0200 Received: from mailima.udg.es (mailima.udg.es [84.88.162.217]) by morisca.udg.es (Postfix) with ESMTP id 1DB0583E09; Wed, 2 Aug 2006 20:10:01 +0200 (CEST) Received: from mailima.udg.es (localhost [127.0.0.1]) by localhost (Postfix) with ESMTP id 23DAA10FB8C; Wed, 2 Aug 2006 20:10:02 +0200 (CEST) Received: by mailima.udg.es (Postfix, from userid 30) id 04ACA10FB8B; Wed, 2 Aug 2006 20:10:01 +0200 (CEST) Received: from 216.Red-80-38-74.staticIP.rima-tde.net (216.Red-80-38-74.staticIP.rima-tde.net [80.38.74.216]) by mailima.udg.es (IMP) with HTTP for ; Wed, 2 Aug 2006 20:10:01 +0200 Message-ID: <1154542201.44d0ea799fcd2@mailima.udg.es> Date: Wed, 2 Aug 2006 20:10:01 +0200 From: Frederic Perez Reply-To: fredericpcx@terra.es To: Neil Gatenby Cc: globillum@imag.fr Subject: Re: HDRI content References: <8815647C7041D111A3010060B06BE1C0034FCF4F@ELVIS> In-Reply-To: <8815647C7041D111A3010060B06BE1C0034FCF4F@ELVIS> MIME-Version: 1.0 User-Agent: Internet Messaging Program (IMP) 3.2.1 X-Originating-IP: 80.38.74.216 X-Greylist: Delayed for 09:10:36 by milter-greylist-1.6 (imag.imag.fr [129.88.30.1]); Thu, 03 Aug 2006 05:20:47 +0200 (CEST) X-IMAG-MailScanner-Information: Please contact IMAG DMI for more information X-IMAG-MailScanner: Found to be clean X-MailScanner-From: frederic@ima.udg.es X-Loop: globillum@imag.fr X-Sequence: 328 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -49 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hi Neil, my only two cents on this is that Blender has recently added support for HDR images---there seems to be a variety of formats (http://www.blender.org/cms/High_Dynamic_Range_Gra.765.0.html), and thus I'm not surprised to learn what you describe. Perhaps you can find interesting links under http://en.wikibooks.org/wiki/Blender_3D:_Noob_to_Pro/HDRi (as an example, I found out that a course entitled "High-Dynamic-Range Imaging: Theory and Applications" took place at SIGGRAPH 2006: http://www.siggraph.org/s2006/main.php?f=conference&p=courses&s=5 Cool enough?) Best regards, Frederic Quoting Neil Gatenby : > > Hi all > > Seems strange writing to a .fr email address, when the whole of France is > still on holiday, but hopefully the rest of the world is reading! > > I've a question about HDR images, and the relation between the colours I > find in the file, and the real-world values that a light meter might have > captured, had it been there at the time of image capture. What is the > relationship? > > I'm finding that loads of the content I'm getting my hands on is not "deep" > at all. I'll have a "sun in sky" image where the sun is only 100x brighter > than the darkest parts of the image - this seems to be really common - I > have lots of data, and very little is truly HDR > > I can see that there must be a camera response curve in there somewhere, and > that the combination of different exposures in one HDRI will further > complicate the issue. > > Does anyone know of any published work in this field? > > Any mappings from so-called HDRIs to truly HDRIs? (e.g., the user says they > want 6 log units in their result) > > I'm importance-sampling HDRIs in a prerender step, and then using those "N > distant lights" during rendering, but I don't get a sharp shadow from the > sun cos the sample(s) that are sat on the sun are not THAT much brighter > than the other samples out there. > > Any input much appreciated > > Cheers > Neil > > P.S. Anyone got any precis reports on what was cool at the Rendering > Symposium, or SIGGRAPH? ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by cg.tuwien.ac.at (8.13.4/8.13.4/Debian-3sarge1) with ESMTP id k735WHRb015349; Thu, 3 Aug 2006 07:32:19 +0200 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.13.7/8.13.7) with ESMTP id k735W3cO015167; Thu, 3 Aug 2006 07:32:08 +0200 (MEST) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id k735W32j026912; Thu, 3 Aug 2006 07:32:03 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id k735W2Mv026907; Thu, 3 Aug 2006 07:32:02 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id k735V7vQ025902 for ; Thu, 3 Aug 2006 07:31:07 +0200 Received: from vms042pub.verizon.net (vms042pub.verizon.net [206.46.252.42]) by imag.imag.fr (8.13.6/8.13.6) with ESMTP id k735V3Lb019214 for ; Thu, 3 Aug 2006 07:31:05 +0200 (CEST) Received: from ATHLON1 ([70.23.142.105]) by vms042.mailsrvcs.net (Sun Java System Messaging Server 6.2-4.02 (built Sep 9 2005)) with ESMTPA id <0J3E00HKGN6ADOZ7@vms042.mailsrvcs.net> for globillum@imag.fr; Wed, 02 Aug 2006 23:30:11 -0500 (CDT) Date: Thu, 03 Aug 2006 00:30:11 -0400 From: "Arnold Gallardo" Subject: RE: HDRI content In-reply-to: <8815647C7041D111A3010060B06BE1C0034FCF4F@ELVIS> To: globillum@imag.fr Message-id: MIME-version: 1.0 X-MIMEOLE: Produced By Microsoft MimeOLE V6.00.2900.2869 X-Mailer: Microsoft Outlook IMO, Build 9.0.6604 (9.0.2911.0) Importance: Normal X-Priority: 3 (Normal) X-MSMail-priority: Normal X-Greylist: Delayed for 01:00:21 by milter-greylist-1.6 (imag.imag.fr [129.88.30.1]); Thu, 03 Aug 2006 07:31:05 +0200 (CEST) X-IMAG-MailScanner-Information: Please contact IMAG DMI for more information X-IMAG-MailScanner: Found to be clean X-MailScanner-From: zeroneg1@toast.net X-Loop: globillum@imag.fr X-Sequence: 329 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -49 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hi, HDR was started if not popularized by Paul Debevec: http://www.debevec.org/Research/HDR/ http://gl.ict.usc.edu/skyprobes/ http://www.hdrshop.com/ You might want to directly contact Paul. You might want to contact him directly at his website. I had the privelege of meeting him at one of Siggraph's private parties and he was a very nice guy. As for your questions that's fairly complicated although we do have direct access to luminance data via the RAW file storage. I however have not verified through incident light metering if the luminance values in the RAW files that I have corresponded well with the actual presnet values in the environment. Another issue though that is often not discussed it tonemapping. Could this be an issue in your application if you are using mean value? Regards, Arnold Gallardo -----Original Message----- From: Neil Gatenby [mailto:neil.gatenby@lightworkdesign.com] Sent: Wednesday, August 02, 2006 6:27 AM To: globillum@imag.fr Subject: HDRI content Hi all Seems strange writing to a .fr email address, when the whole of France is still on holiday, but hopefully the rest of the world is reading! I've a question about HDR images, and the relation between the colours I find in the file, and the real-world values that a light meter might have captured, had it been there at the time of image capture. What is the relationship? I'm finding that loads of the content I'm getting my hands on is not "deep" at all. I'll have a "sun in sky" image where the sun is only 100x brighter than the darkest parts of the image - this seems to be really common - I have lots of data, and very little is truly HDR I can see that there must be a camera response curve in there somewhere, and that the combination of different exposures in one HDRI will further complicate the issue. Does anyone know of any published work in this field? Any mappings from so-called HDRIs to truly HDRIs? (e.g., the user says they want 6 log units in their result) I'm importance-sampling HDRIs in a prerender step, and then using those "N distant lights" during rendering, but I don't get a sharp shadow from the sun cos the sample(s) that are sat on the sun are not THAT much brighter than the other samples out there. Any input much appreciated Cheers Neil P.S. Anyone got any precis reports on what was cool at the Rendering Symposium, or SIGGRAPH? Neil Gatenby Senior Software Specialist Lightwork Design, Rutledge House, 78 Clarkehouse Road, Sheffield, S10 2LJ, UK Tel: +44 114 266 8404, Fax: +44 114 1383 neil.gatenby@lightworkdesign.com, http://www.lightworkdesign.com/ ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from neelix.kom.tuwien.ac.at (neelix.kom.tuwien.ac.at [192.35.241.67]) by cg.tuwien.ac.at (8.13.4/8.13.4/Debian-3sarge1) with ESMTP id k7QEv4lk003978; Sat, 26 Aug 2006 16:57:04 +0200 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by neelix.kom.tuwien.ac.at (8.13.7/8.13.7) with ESMTP id k7QEusd5024040; Sat, 26 Aug 2006 16:57:01 +0200 (MEST) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id k7QEuq4v032148; Sat, 26 Aug 2006 16:56:52 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id k7QEupsr032144; Sat, 26 Aug 2006 16:56:51 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id k7QEuaEe031148 for ; Sat, 26 Aug 2006 16:56:36 +0200 Received: from sophia.inria.fr (sophia.inria.fr [138.96.64.20]) by imag.imag.fr (8.13.6/8.13.6) with ESMTP id k7QEuWnE006302 (version=TLSv1/SSLv3 cipher=EDH-RSA-DES-CBC3-SHA bits=168 verify=NO) for ; Sat, 26 Aug 2006 16:56:33 +0200 (CEST) Received: from localhost (localhost [127.0.0.1]) by sophia.inria.fr (8.13.8/8.13.4) with ESMTP id k7QEuV16023752 for ; Sat, 26 Aug 2006 16:56:31 +0200 Received: from sophia.inria.fr (ANice-151-1-21-22.w83-113.abo.wanadoo.fr [83.113.221.22]) (authenticated bits=0) by sophia.inria.fr (8.13.8/8.13.4) with ESMTP id k7QEiIRL011039 (version=TLSv1/SSLv3 cipher=RC4-MD5 bits=128 verify=NO) for ; Sat, 26 Aug 2006 16:44:18 +0200 Message-ID: <44F05E41.3060106@sophia.inria.fr> Date: Sat, 26 Aug 2006 16:44:17 +0200 From: George Drettakis User-Agent: Mozilla/5.0 (Windows; U; Windows NT 5.1; fr-FR; rv:1.4) Gecko/20030624 Netscape/7.1 (ax) X-Accept-Language: fr-fr, fr MIME-Version: 1.0 To: globillum@imag.fr Subject: RenderCache code available (Post for Bruce Walter) X-Greylist: Sender IP whitelisted, not delayed by milter-greylist-1.6 (imag.imag.fr [129.88.30.1]); Sat, 26 Aug 2006 16:56:34 +0200 (CEST) X-Greylist: Sender succeeded SMTP AUTH authentication, not delayed by milter-greylist-2.0.2 (sophia.inria.fr [138.96.64.20]); Sat, 26 Aug 2006 16:44:19 +0200 (MEST) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-IMAG-MailScanner-Information: Please contact IMAG DMI for more information X-IMAG-MailScanner: Found to be clean X-MailScanner-From: george.drettakis@sophia.inria.fr X-Loop: globillum@imag.fr X-Sequence: 330 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-Spam-Status: LOW ; -49 X-Spam-Level: - X-Spam-TU-Processing-Host: neelix X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hello all Here is a note from Bruce Walter who had problems with the list server: ----------------- Just a quick note to announce that the complete C++ source code for the Render Cache is now available under GPL license at: http://www.graphics.cornell.edu/research/interactive/rendercache/ The Render Cache is an interactive display adapter/system for use with ray-based renderers published in EGSR 99 and 02 (see page for more details). I've had requests for code, but hadn't been able to release it until now. thanks, Bruce Walter ---------- Cheers -g -- George Drettakis, Group Leader, REVES -- INRIA Sophia-Antipolis, 2004 route des Lucioles, BP 93 F-06902 Sophia Antipolis, France; email: George.Drettakis@sophia.inria.fr tel: +33 4 92 38 50 32 fax: +33 4 92 38 50 30 (dial 04 92 38 ... in France) http://www-sop.inria.fr/reves/George.Drettakis "Le luxe, c'est le temps" -- Jean-Jacques Goldman ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by cg.tuwien.ac.at (8.13.4/8.13.4/Debian-3sarge1) with ESMTP id k8CDi53J015307; Tue, 12 Sep 2006 15:44:07 +0200 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.13.7/8.13.7) with ESMTP id k8CEhuv7006931; Tue, 12 Sep 2006 16:44:02 +0200 (MEST) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id k8CEhuFp005775; Tue, 12 Sep 2006 16:43:56 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id k8CEhtKb005770; Tue, 12 Sep 2006 16:43:55 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id k8CEeaZ4004486 for ; Tue, 12 Sep 2006 16:40:36 +0200 Received: from mail20c0.megamailservers.com (mail20c0.megamailservers.com [216.251.36.230]) by imag.imag.fr (8.13.6/8.13.6) with ESMTP id k8CEeV51027609 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO) for ; Tue, 12 Sep 2006 16:40:34 +0200 (CEST) X-POP-User: book.helios32.com Received: from IAN (S01060006257abbc2.vn.shawcable.net [24.81.109.189]) by mail20c0.megamailservers.com (8.13.6/8.13.1) with ESMTP id k8CEHXk9003457 for ; Tue, 12 Sep 2006 10:17:38 -0400 From: "Ian Ashdown" To: globillum@imag.fr Subject: Radiosity: A Programmer's Perspective - Now Free! Date: Tue, 12 Sep 2006 07:17:31 -0700 Organization: byHeart Consultants Limited Message-ID: <000e01c6d676$311da830$6401a8c0@IAN> MIME-Version: 1.0 X-Mailer: Microsoft Office Outlook 11 Thread-Index: AcbWdi93UjI2ol7cRe6QJpK/M14WcA== X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2900.2962 X-Greylist: Delayed for 00:22:52 by milter-greylist-1.6 (imag.imag.fr [129.88.30.1]); Tue, 12 Sep 2006 16:40:34 +0200 (CEST) X-IMAG-MailScanner-Information: Please contact IMAG DMI for more information X-IMAG-MailScanner: Found to be clean X-MailScanner-From: ian_ashdown@helios32.com X-Loop: globillum@imag.fr X-Sequence: 331 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/html; charset=windows-1252 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -22 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

From www.cgarchitect.com:

 

Radiosity: A Programmer’s Perspective - Now Free!
September 12, 2006

Radiosity: A Programmer’s Perspective (Wiley 1994), is now available for free from Lighting Analysts. The downloadable ZIP file includes C++ source code for HELIOS, a fully-functional radiosity renderer.

 

See http://www.agi32.com/Extra/TechnicalDocs/technicalDocuments.htm for details.

 

Ian Ashdown, P. Eng., LC, FIES

President

byHeart Consultants Limited

http://www.helios32.com

 

------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from neelix.kom.tuwien.ac.at (neelix.kom.tuwien.ac.at [192.35.241.67]) by cg.tuwien.ac.at (8.13.4/8.13.4/Debian-3sarge3) with ESMTP id k8JEYFE2022721; Tue, 19 Sep 2006 16:34:15 +0200 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by neelix.kom.tuwien.ac.at (8.13.7/8.13.7) with ESMTP id k8JFXrie025412; Tue, 19 Sep 2006 17:33:59 +0200 (MEST) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id k8JFXq0S004175; Tue, 19 Sep 2006 17:33:52 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id k8JFXkdn004165; Tue, 19 Sep 2006 17:33:46 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id k8JFWRYn003144 for ; Tue, 19 Sep 2006 17:32:27 +0200 Received: from mail76.megamailservers.com (mail76.megamailservers.com [216.251.36.76]) by imag.imag.fr (8.13.6/8.13.6) with ESMTP id k8JFW9R1002036 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO) for ; Tue, 19 Sep 2006 17:32:12 +0200 (CEST) X-POP-User: book.helios32.com Received: from IAN (S01060006257abbc2.vn.shawcable.net [24.81.109.189]) by mail76.megamailservers.com (8.13.6/8.13.1) with ESMTP id k8JF6kf2021669 for ; Tue, 19 Sep 2006 11:06:52 -0400 From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: 06/09/19 Release of RADBIB and GITHESIS Date: Tue, 19 Sep 2006 08:06:46 -0700 Organization: byHeart Consultants Limited Message-ID: <000501c6dbfd$3b617790$6401a8c0@IAN> MIME-Version: 1.0 X-Mailer: Microsoft Office Outlook 11 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2900.2962 Thread-Index: Acbb/TmJzvID4+c6TYOQPC/H/U+d2g== X-Greylist: Delayed for 00:25:13 by milter-greylist-1.6 (imag.imag.fr [129.88.30.1]); Tue, 19 Sep 2006 17:32:12 +0200 (CEST) X-IMAG-MailScanner-Information: Please contact IMAG DMI for more information X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-From: ian_ashdown@helios32.com X-Loop: globillum@imag.fr X-Sequence: 332 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/html; charset=windows-1252 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -32 X-Spam-Level: - X-Spam-TU-Processing-Host: neelix X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

ANNOUNCE: 06/09/19 Release of RADBIB and GITHESIS

RADBIB is a comprehensive bibliography of radiosity, photon mapping, and related global illumination papers, theses, articles, and books. It currently includes 2,572 references -- 25 new additions since its 06/04/26 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of September 19, 2006) from:

  http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 323 references to radiosity, photon mapping, and related global illumination theses -- 3 new additions since the 06/04/26 release.

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

Ian Ashdown, P. Eng., LC, FIES
President
byHeart Consultants Limited
http://www.helios32.com

 

------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from neelix.kom.tuwien.ac.at (neelix.kom.tuwien.ac.at [192.35.241.67]) by cg.tuwien.ac.at (8.13.4/8.13.4/Debian-3sarge3) with ESMTP id k8UGdFna024190; Sat, 30 Sep 2006 18:39:15 +0200 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by neelix.kom.tuwien.ac.at (8.13.7/8.13.7) with ESMTP id k8UGd23a008704; Sat, 30 Sep 2006 18:39:09 +0200 (MEST) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id k8UGctvY020306; Sat, 30 Sep 2006 18:38:55 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id k8UGcimc020296; Sat, 30 Sep 2006 18:38:44 +0200 Received: from mx-serv.inrialpes.fr (mx-serv.inrialpes.fr [194.199.18.100]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id k8UGbE7J019281 for ; Sat, 30 Sep 2006 18:37:14 +0200 Received: from paste.autodesk.com (paste.autodesk.com [198.102.112.48]) by mx-serv.inrialpes.fr (8.13.6/8.13.0) with ESMTP id k8UGb8x2001319 for ; Sat, 30 Sep 2006 18:37:09 +0200 (MEST) Received: from msgusawfe01.ads.autodesk.com ([144.111.33.210]) by paste.autodesk.com (8.13.0/8.12.6) with ESMTP id k8UGaZ9t013676 for ; Sat, 30 Sep 2006 09:36:45 -0700 (PDT) Received: from msgusawpf02.ads.autodesk.com ([144.111.33.213]) by msgusawfe01.ads.autodesk.com with Microsoft SMTPSVC(5.0.2195.6713); Sat, 30 Sep 2006 09:36:35 -0700 Received: from msgusaepf01.ads.autodesk.com ([144.111.72.51]) by msgusawpf02.ads.autodesk.com with Microsoft SMTPSVC(5.0.2195.6713); Sat, 30 Sep 2006 09:36:35 -0700 Received: from msgusaemb02.ads.autodesk.com ([144.111.72.54]) by msgusaepf01.ads.autodesk.com with Microsoft SMTPSVC(5.0.2195.6713); Sat, 30 Sep 2006 12:36:34 -0400 x-mimeole: Produced By Microsoft Exchange V6.0.6603.0 MIME-Version: 1.0 Subject: Ray Tracing News v. 19 no. 1 is out Date: Sat, 30 Sep 2006 12:36:34 -0400 Message-ID: Thread-Topic: Ray Tracing News v. 19 no. 1 is out Thread-Index: Acbkrpcbn9/vJH5xR1K3T88nh28iNQ== From: "Eric Haines" To: globillum@imag.fr X-OriginalArrivalTime: 30 Sep 2006 16:36:34.0456 (UTC) FILETIME=[978B2980:01C6E4AE] X-Greylist: Sender is SPF-compliant, not delayed by milter-greylist-2.0.2 (mx-serv.inrialpes.fr [194.199.18.100]); Sat, 30 Sep 2006 18:37:10 +0200 (MEST) X-mx-serv-inrialpes-fr-MailScanner-Information: Please contact postmaster@inrialpes.fr for more information X-mx-serv-inrialpes-fr-MailScanner: Found to be clean X-mx-serv-inrialpes-fr-MailScanner-SpamCheck: n'est pas un polluriel, SpamAssassin (score=0.001, requis 6, HTML_MESSAGE 0.00) X-mx-serv-inrialpes-fr-MailScanner-From: eric.haines@autodesk.com X-Spam-Status: LOW ; -47 X-Spam-Status: No X-Loop: globillum@imag.fr X-Sequence: 335 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/html; charset=windows-1252 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Level: - X-Spam-TU-Processing-Host: neelix X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit content-class: urn:content-classes:message Content-Type: multipart/alternative; boundary="----_=_NextPart_001_01C6E4AE.9781D73F"

The Ray Tracing News v. 19 no. 1 is now available at http://www.raytracingnews.org/rtnv19n1.html

 

Contents:

    * Introduction

    * Ray Tracing Roundup

    * Notes on Efficient Ray Tracing, by Solomon Boulos and Eric Haines

    * Ray-Box Sorting, by Solomon Boulos and Eric Haines

    * BVHs and Memory Coherence, notes by Christer Ericson and Sung-Eui Yoon

    * "So long and thanks for all the fish...", from Michael Ashikhmin, comments by Eric Haines

    * Ray/Box Intersection Optimization, by Eric Haines, Solomon Boulos, and Pete Shirley

    * SIGGRAPH 2006 Report, by Eric Haines

 

Enjoy,

 

Eric

------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by cg.tuwien.ac.at (8.13.4/8.13.4/Debian-3sarge3) with ESMTP id k969YNfg010417; Fri, 6 Oct 2006 11:34:23 +0200 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.13.7/8.13.7) with ESMTP id k969XksT014348; Fri, 6 Oct 2006 11:33:56 +0200 (MEST) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id k969XkXu004015; Fri, 6 Oct 2006 11:33:46 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id k969XUIl004009; Fri, 6 Oct 2006 11:33:30 +0200 Received: from mx-serv.inrialpes.fr (mx-serv.inrialpes.fr [194.199.18.100]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id k969VDdD003885 for ; Fri, 6 Oct 2006 11:31:14 +0200 Received: from mail.vsiltd.co.uk (mail.vsiltd.co.uk [195.152.206.150] (may be forged)) by mx-serv.inrialpes.fr (8.13.6/8.13.0) with ESMTP id k968xQnm004499 for ; Fri, 6 Oct 2006 10:59:43 +0200 (MEST) Received: from elvis.lightwork (slade.owshared [195.152.206.70]) by mail.vsiltd.co.uk (8.12.8/8.12.8) with ESMTP id k968wZcn003966 for ; Fri, 6 Oct 2006 09:58:36 +0100 Received: by ELVIS with Internet Mail Service (5.5.2653.19) id ; Fri, 6 Oct 2006 09:58:35 +0100 Message-ID: <8815647C7041D111A3010060B06BE1C003B18BBF@ELVIS> From: Neil Gatenby To: globillum@imag.fr Subject: The great unbiased renderer debate Date: Fri, 6 Oct 2006 09:58:34 +0100 MIME-Version: 1.0 X-Mailer: Internet Mail Service (5.5.2653.19) X-Greylist: Sender is SPF-compliant, not delayed by milter-greylist-2.0.2 (mx-serv.inrialpes.fr [194.199.18.100]); Fri, 06 Oct 2006 10:59:44 +0200 (MEST) X-mx-serv-inrialpes-fr-MailScanner-Information: Please contact postmaster@inrialpes.fr for more information X-mx-serv-inrialpes-fr-MailScanner: Found to be clean X-mx-serv-inrialpes-fr-MailScanner-SpamCheck: n'est pas un polluriel, SpamAssassin (score=0, requis 6) X-mx-serv-inrialpes-fr-MailScanner-From: neil.gatenby@lightworkdesign.com X-Spam-Status: LOW ; -49 X-Spam-Status: No X-Loop: globillum@imag.fr X-Sequence: 336 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hiya It's Friday, so I thought I'd start this ... I'm noticing lots of unbiased renderers popping up in the market: http://www.maxwellrender.com/ http://www.fryrender.com/ http://www.indigorenderer.com/ If you sample a PDF which represents the distribution of their offices across the surface of the world, you will probably find yourself in Madrid. No bad thing, I'm sure. (Unless you're a Barca fan!) Anyone here have strong thoughts on whether they are a good thing, or a bad thing? It surely depends on what you are trying to do. So I'm assuming this use case: somebody sat in front of a 3DSMax-like piece of software, trying to do several (3? 6? 10?) photorealistic renders of a building. Interior, exterior (both, either), night, day (both, either), realistic lighting, materials and geometry. Feel free to invent different use cases to support your PoV Surely unbiased means noisy and slow, whereas bias means applying intelligent smoothing to unbiased numbers so as to achieve the same (or _very nearly the same) image in less time? Or a fast image with nowhere near so much noise? I'd be interested to read your views Have a good w/e, all Cheers Neil Neil Gatenby Senior Software Specialist Lightwork Design, Rutledge House, 78 Clarkehouse Road, Sheffield, S10 2LJ, UK Tel: +44 114 266 8404, Fax: +44 114 1383 neil.gatenby@lightworkdesign.com, http://www.lightworkdesign.com/ ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by cg.tuwien.ac.at (8.13.4/8.13.4/Debian-3sarge3) with ESMTP id k9C0FOXl019769; Thu, 12 Oct 2006 02:15:24 +0200 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.13.7/8.13.7) with ESMTP id k9C0EYtj023172; Thu, 12 Oct 2006 02:14:42 +0200 (MEST) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id k9C0ESws029257; Thu, 12 Oct 2006 02:14:28 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id k9C0ELVp029252; Thu, 12 Oct 2006 02:14:21 +0200 Received: from mx-serv.inrialpes.fr (mx-serv.inrialpes.fr [194.199.18.100]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id k9C0BtQQ027961 for ; Thu, 12 Oct 2006 02:11:55 +0200 Received: from mail.vsiltd.co.uk (mail.vsiltd.co.uk [195.152.206.150]) by mx-serv.inrialpes.fr (8.13.6/8.13.0) with ESMTP id k9C0Blg8014810 for ; Thu, 12 Oct 2006 02:11:51 +0200 (MEST) Received: from elvis.lightwork (slade.owshared [195.152.206.70]) by mail.vsiltd.co.uk (8.12.8/8.12.8) with ESMTP id k9C0BYco017980 for ; Thu, 12 Oct 2006 01:11:35 +0100 Received: by ELVIS with Internet Mail Service (5.5.2653.19) id ; Thu, 12 Oct 2006 01:11:36 +0100 Message-ID: <8815647C7041D111A3010060B06BE1C003B18BF5@ELVIS> From: Neil Gatenby To: globillum@imag.fr Subject: FW: unbiased vs biased Date: Thu, 12 Oct 2006 01:11:27 +0100 MIME-Version: 1.0 X-Mailer: Internet Mail Service (5.5.2653.19) Content-Type: text/plain; charset=windows-1252; format=flowed X-Greylist: Sender is SPF-compliant, not delayed by milter-greylist-2.0.2 (mx-serv.inrialpes.fr [194.199.18.100]); Thu, 12 Oct 2006 02:11:51 +0200 (MEST) X-mx-serv-inrialpes-fr-MailScanner-Information: Please contact postmaster@inrialpes.fr for more information X-mx-serv-inrialpes-fr-MailScanner: Found to be clean X-mx-serv-inrialpes-fr-MailScanner-SpamCheck: n'est pas un polluriel, SpamAssassin (score=0, requis 6) X-mx-serv-inrialpes-fr-MailScanner-From: neil.gatenby@lightworkdesign.com X-Spam-Status: LOW ; -49 X-Spam-Status: No X-Loop: globillum@imag.fr X-Sequence: 337 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hi again Brian has had trouble getting an email onto the list, so I'm forwarding his email here, since I feel it adds to the debate, and he has given me the OK to do so Brian mentions Instant Radiosity, which is also available commercially (http://www.artlantis.com/products/artlantisR/) although presumably its biased, so as to avoid the artefacts described in the attached Cheers Neil Message-ID: <5b7094580610110628s22f27387uf6ecdecec072fbd4@mail.gmail.com> From: Brian Budge To: Neil Gatenby Subject: re: unbiased vs biased Date: Wed, 11 Oct 2006 14:28:22 +0100 MIME-Version: 1.0 X-Mailer: Internet Mail Service (5.5.2653.19) Content-Type: text/plain HI Neil - I've been trying for a couple of days to get on the globillum@imag.fr mailing list, but somehow have failed... anyhow, here's my view: I agree that it depends on the use of the software. There are surely cases where bias is unimportant, but there are others where it is potentially important. Also, my view is that you can introduce so many different kinds of bias leading to different levels of artifacts. One that we are all familiar with is when a photon map is directly visualized as in Jensen's original paper. When I wrote my first photon mapping renderer, I thought I'd made a mistake... what were all these "splats"? Add a level of indirection, and the splats go away, and the image is more reasonable (and also takes much longer to compute). Another case would be instant radiosity. The algorithm is in general unbiased for most paths (LD*SDE can't be represented at all) when no bounding is done on the lighting, but it looks terrible with all the blooming, and it really would take infinitely many samples using infinite precision software for the blooming to go away. When you add a bounding term though, the algorithm converges quite nicely and quickly (although now biased and noticeably too dark). I think that unbiased algorithms bring something important to the table, though, which may or may not be important depending on your application. Sure, photon mapping will give you a reasonable image most of the time, but there is no guarantee of that, even if you run as many samples as you want. Path tracing on the other hand should eventually guarantee the correct image, albeit more slowly. I think unbiased renderers and their underlying algorithms are important. You can add biased versions if you want them, but unbiased software will work in general, and usually with less "tweaking" (gee, how many times have I rendered an image with photon mapping and decided that I actually needed to shoot more photons?) Brian ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by cg.tuwien.ac.at (8.13.4/8.13.4/Debian-3sarge3) with ESMTP id kA68irFv029543; Mon, 6 Nov 2006 09:44:53 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.13.7/8.13.7) with ESMTP id kA68iLdA020337; Mon, 6 Nov 2006 09:44:27 +0100 (MET) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id kA68iL0l005022; Mon, 6 Nov 2006 09:44:21 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id kA68iCO0004943; Mon, 6 Nov 2006 09:44:12 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id kA68ZGOX002656 for ; Mon, 6 Nov 2006 09:35:36 +0100 Received: from pantheon-po12.its.yale.edu (pantheon-po12.its.yale.edu [130.132.50.70]) by imag.imag.fr (8.13.6/8.13.6) with ESMTP id kA5KJUsB010566 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=FAIL) for ; Sun, 5 Nov 2006 21:19:33 +0100 (CET) Received: from Edith (vpn130132044043.its.yale.edu [130.132.44.43]) by pantheon-po12.its.yale.edu (8.12.11.20060308/8.12.11) with ESMTP id kA5JuUBl011674 for ; Sun, 5 Nov 2006 14:56:33 -0500 From: "Holly Rushmeier" To: globillum@imag.fr Subject: Data Sets Available Date: Sun, 5 Nov 2006 14:56:30 -0500 Message-ID: <002901c70114$7cdc6220$6501a8c0@cs.yale.edu> MIME-Version: 1.0 X-Mailer: Microsoft Office Outlook 11 Thread-Index: AccBE//Fyg2gjQEDQKG1VStaV5DH8QAAGfSw X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2900.2962 X-YaleITSMailFilter: Version 1.2c (attachment(s) not renamed) X-Greylist: Delayed for 00:22:56 by milter-greylist-1.6 (imag.imag.fr [129.88.30.1]); Sun, 05 Nov 2006 21:19:33 +0100 (CET) X-IMAG-MailScanner-Information: Please contact IMAG DMI for more information X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-From: holly@acm.org X-Loop: globillum@imag.fr X-Sequence: 339 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -26 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 9001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hi, We have just made several data sets available for testing algorithms for synthesizing material aging effects, and for extracting consistent texture maps from sets of digital images: 1. Directions for obtaining both source and target data from our paper "Context Aware Textures" http://graphics.cs.yale.edu/CAT/ are available from http://graphics.cs.yale.edu/CAT/CAT_data.htm The data sets include spatially and temporally varying appearances due to weathering effects, with these variations correlated to geometric and environmental factors. 2. Directions for obtaining both high dynamic range images and Cyra scans from our paper "A System for Reconstructing Integrated Texture Maps for Large Structures" http://graphics.cs.yale.edu/publications/finalsubmission073.pdf are available from http://graphics.cs.yale.edu/data/readme_data_vc.html -- Holly _______________ Holly Rushmeier, Dept. of CS, Yale University, PO Box 208285, New Haven,CT 06520-8285,Phone: (203)432-4091, holly@acm.org ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by cg.tuwien.ac.at (8.13.4/8.13.4/Debian-3sarge3) with ESMTP id kAN023G6016099; Thu, 23 Nov 2006 01:02:03 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.13.7/8.13.7) with ESMTP id kAN01uHR014786; Thu, 23 Nov 2006 01:01:56 +0100 (MET) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id kAN01r0B004167; Thu, 23 Nov 2006 01:01:53 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id kAN01rmC004158; Thu, 23 Nov 2006 01:01:53 +0100 Received: from mx-serv.inrialpes.fr (mx-serv.inrialpes.fr [194.199.18.100]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id kAN01c2e003184 for ; Thu, 23 Nov 2006 01:01:38 +0100 Received: from shell.lmi.net (shell.lmi.net [66.117.140.246]) by mx-serv.inrialpes.fr (8.13.6/8.13.0) with ESMTP id kAN01KnU010823; Thu, 23 Nov 2006 01:01:32 +0100 (MET) Received: from localhost (shell.lmi.net [66.117.140.246]) by shell.lmi.net (8.13.6/8.13.6) with ESMTP id kAN014sM039464; Wed, 22 Nov 2006 16:01:05 -0800 (PST) Subject: Re: Blinn's law From: Larry Gritz To: Nicolas Holzschuch Cc: globillum@imag.fr In-Reply-To: References: Date: Wed, 22 Nov 2006 16:02:16 -0800 Message-Id: <1164240136.12957.3.camel@dhcp-10> Mime-Version: 1.0 X-Mailer: Evolution 2.4.0 X-Scanned-By: MIMEDefang 2.37 X-mx-serv-inrialpes-fr-MailScanner-Information: Please contact postmaster@inrialpes.fr for more information X-mx-serv-inrialpes-fr-MailScanner: Found to be clean X-mx-serv-inrialpes-fr-MailScanner-SpamCheck: n'est pas un polluriel, SpamAssassin (score=0, requis 5) X-mx-serv-inrialpes-fr-MailScanner-From: lg@larrygritz.com X-Spam-Status: LOW ; -2 X-Spam-Status: No X-Loop: globillum@imag.fr X-Sequence: 341 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-Virus-Scanned: by amavisd-new X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 9001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Jim Blinn said or wrote this quite a while back. At one point a couple years ago, I asked him directly for the original citation and he said he'd long since forgotten exactly when he said it. The "original" form, near as Jim told me he could remember it, was "all frames take 15 minutes to render, regardless of improvements to technology." I've found that the time limit varies from person to person and company to company (some think 1 minute is long enough, others will tolerate 8 hour renders), but the principle holds remarkably well -- faster machines or better algorithms always result (for film rendering, anyway) in the artists increasing complexity until they're back at the original time limit. -- lg On Wed, 2006-11-22 at 22:10 +0100, Nicolas Holzschuch wrote: > Hello fellow globillumers, > If I remember well, at EGWR in Vienna (1998), A. Apodaca mentionned a > "Blinn's law" (the appetite of users for "cool features" will double > every twelve months) that trumps Moore's law. > > I've been doing some research, but I can't find a definitive source > on "Blinn's law". Can anyone help? -- Larry Gritz lg@larrygritz.com (for work *ONLY*, lgritz@nvidia.com) ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by cg.tuwien.ac.at (8.13.4/8.13.4/Debian-3sarge3) with ESMTP id kBDDMmUN010617; Wed, 13 Dec 2006 14:22:48 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.13.7/8.13.7) with ESMTP id kBDDMcac000518; Wed, 13 Dec 2006 14:22:41 +0100 (MET) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id kBDDMZTe000332; Wed, 13 Dec 2006 14:22:35 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id kBDDMUHg000300; Wed, 13 Dec 2006 14:22:30 +0100 Received: from mx-serv.inrialpes.fr (mx-serv.inrialpes.fr [194.199.18.100]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id kBDDMF4t031804 for ; Wed, 13 Dec 2006 14:22:15 +0100 Received: from rozz.csail.mit.edu (rozz.csail.mit.edu [128.30.2.16]) by mx-serv.inrialpes.fr (8.13.6/8.13.0) with ESMTP id kBDDM8uc015458 for ; Wed, 13 Dec 2006 14:22:10 +0100 (MET) Received: from etching.csail.mit.edu ([128.30.96.89]) by rozz.csail.mit.edu with esmtps (TLSv1:AES256-SHA:256) (Exim 4.63) (envelope-from ) id 1GuU3Z-0001Nb-Qj for globillum@imag.fr; Wed, 13 Dec 2006 08:21:57 -0500 Message-ID: <457FFE77.4050000@csail.mit.edu> Date: Wed, 13 Dec 2006 08:21:59 -0500 From: Fredo Durand Reply-To: fredo@csail.mit.edu User-Agent: Thunderbird 1.5.0.8 (Windows/20061025) MIME-Version: 1.0 To: globillum@imag.fr Subject: 3D meshes with textures X-Greylist: Sender is SPF-compliant, not delayed by milter-greylist-2.0.2 (mx-serv.inrialpes.fr [194.199.18.100]); Wed, 13 Dec 2006 14:22:10 +0100 (MET) X-mx-serv-inrialpes-fr-MailScanner-Information: Please contact postmaster@inrialpes.fr for more information X-mx-serv-inrialpes-fr-MailScanner: Found to be clean X-mx-serv-inrialpes-fr-MailScanner-SpamCheck: n'est pas un polluriel, SpamAssassin (score=0, requis 5) X-mx-serv-inrialpes-fr-MailScanner-From: fredo@csail.mit.edu X-Spam-Status: LOW ; -11 X-Spam-Status: No X-Loop: globillum@imag.fr X-Sequence: 342 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-Virus-Scanned: by amavisd-new X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 9001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit We have just put online some pretty high-quality 3D meshes with parameterization and texture atlases http://people.csail.mit.edu/tmertens/textransfer/data/index.html (corresponding to our EGSR paper http://people.csail.mit.edu/tmertens/textransfer/index.html Enjoy. Fredo -- Fredo Durand, MIT CSAIL The Stata Center 32-D426, 32 Vassar Street, Cambridge, MA 02139, USA phone : 617 253 7223 fax : 617 253 4640 http://graphics.csail.mit.edu/~fredo/ ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by cg.tuwien.ac.at (8.13.4/8.13.4/Debian-3sarge3) with ESMTP id l47FCH8V031775; Mon, 7 May 2007 17:12:18 +0200 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.13.7/8.13.7) with ESMTP id l47FCAVQ009491; Mon, 7 May 2007 17:12:10 +0200 (MEST) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id l47FC9Vq018774; Mon, 7 May 2007 17:12:09 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id l47FC6cL018769; Mon, 7 May 2007 17:12:06 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id l47F9ic3017762 for ; Mon, 7 May 2007 17:09:44 +0200 Received: from mail113.megamailservers.com (mail113.megamailservers.com [216.251.36.113]) by imag.imag.fr (8.13.8/8.13.8) with ESMTP id l47F9Vo8016826 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO) for ; Mon, 7 May 2007 17:09:34 +0200 (CEST) X-POP-User: ian_ashdown.helios32.com Received: from Ian (S01060006257abbc2.vn.shawcable.net [24.85.220.50]) by mail113.megamailservers.com (8.13.6.20060614/8.13.1) with ESMTP id l47DH3HE021470 for ; Mon, 7 May 2007 09:17:08 -0400 From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: 07/04/03 Release of RADBIB and GITHESIS Date: Mon, 7 May 2007 06:16:44 -0700 Organization: byHeart Consultants Limited Message-ID: <000301c790a9$f6ad6520$6401a8c0@Ian> MIME-Version: 1.0 X-Mailer: Microsoft Office Outlook 11 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2900.3028 Thread-Index: AceQqfWUM+sQiNHASMG1plM4P0xw9g== X-Greylist: Sender is SPF-compliant, not delayed by milter-greylist-3.0 (tuvok.kom.tuwien.ac.at [192.35.241.66]); Mon, 07 May 2007 17:12:13 +0200 (MEST) X-Greylist: Delayed for 01:52:20 by milter-greylist-3.0 (imag.imag.fr [129.88.30.1]); Mon, 07 May 2007 17:09:34 +0200 (CEST) X-IMAG-MailScanner-Information: Please contact IMAG DMI for more information X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-From: ian_ashdown@helios32.com X-Loop: globillum@imag.fr X-Sequence: 349 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/html; charset=windows-1252 X-Virus-Scanned: by amavisd-new X-Spam-Status: LOW ; -11 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

ANNOUNCE: 07/04/03 Release of RADBIB and GITHESIS

RADBIB is a comprehensive bibliography of radiosity, photon mapping, and related global illumination papers, theses, articles, and books. It currently includes 2,583 references -- 11 new additions since its 06/09/19 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of May 3, 2007) from:

  http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 324 references to radiosity, photon mapping, and related global illumination theses -- 1 new addition since the 06/09/19 release.

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

Ian Ashdown, P. Eng., LC, FIES
President
byHeart Consultants Limited
http://www.helios32.com

 

------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from neelix.kom.tuwien.ac.at (neelix.kom.tuwien.ac.at [192.35.241.67]) by cg.tuwien.ac.at (8.13.4/8.13.4/Debian-3sarge3) with ESMTP id l4LEVcm2028987; Mon, 21 May 2007 16:31:38 +0200 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by neelix.kom.tuwien.ac.at (8.13.7/8.13.7) with ESMTP id l4LEV9X1008004; Mon, 21 May 2007 16:31:13 +0200 (MEST) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id l4LEV9Bt015520; Mon, 21 May 2007 16:31:09 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id l4LEV87T015515; Mon, 21 May 2007 16:31:08 +0200 Received: from mx-serv.inrialpes.fr (mx-serv.inrialpes.fr [194.199.18.100]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id l4LETPWm014508 for ; Mon, 21 May 2007 16:29:25 +0200 Received: from mut.autodesk.com (mut.autodesk.com [198.102.112.26]) by mx-serv.inrialpes.fr (8.13.6/8.13.0) with ESMTP id l4LETIF4006596 for ; Mon, 21 May 2007 16:29:19 +0200 (MEST) Received: from msgusawfe02.ads.autodesk.com ([144.111.33.211]) by mut.autodesk.com (8.13.0/8.12.6) with ESMTP id l4LESnnZ003224 for ; Mon, 21 May 2007 07:29:08 -0700 (PDT) Received: from MSGUSAWBH01.ads.autodesk.com ([144.111.33.207]) by msgusawfe02.ads.autodesk.com with Microsoft SMTPSVC(5.0.2195.6713); Mon, 21 May 2007 07:29:03 -0700 Received: from msgusaebh01.ads.autodesk.com ([144.111.72.71]) by MSGUSAWBH01.ads.autodesk.com with Microsoft SMTPSVC(5.0.2195.6713); Mon, 21 May 2007 07:29:02 -0700 Received: from msgusaemb02.ads.autodesk.com ([144.111.72.54]) by msgusaebh01.ads.autodesk.com with Microsoft SMTPSVC(5.0.2195.6713); Mon, 21 May 2007 10:29:01 -0400 X-MimeOLE: Produced By Microsoft Exchange V6.0.6603.0 Content-class: urn:content-classes:message MIME-Version: 1.0 Content-Type: multipart/mixed; boundary="------------090700090804030907010204" Subject: New Ray Tracing News is out Date: Mon, 21 May 2007 10:29:01 -0400 Message-ID: X-MS-TNEF-Correlator: Thread-Topic: New Ray Tracing News is out Thread-Index: AcebtGAFqQCH/K7MRwOl3agXXRZbYg== From: "Eric Haines" To: "globillum" X-OriginalArrivalTime: 21 May 2007 14:29:01.0248 (UTC) FILETIME=[60200C00:01C79BB4] X-Greylist: Sender is SPF-compliant, not delayed by milter-greylist-3.0 (neelix.kom.tuwien.ac.at [192.35.241.67]); Mon, 21 May 2007 16:31:34 +0200 (MEST) X-Greylist: Sender is SPF-compliant, not delayed by milter-greylist-2.0.2 (mx-serv.inrialpes.fr [194.199.18.100]); Mon, 21 May 2007 16:29:20 +0200 (MEST) X-mx-serv-inrialpes-fr-MailScanner-Information: Please contact postmaster@inrialpes.fr for more information X-mx-serv-inrialpes-fr-MailScanner: Found to be clean X-mx-serv-inrialpes-fr-MailScanner-SpamCheck: n'est pas un polluriel, SpamAssassin (score=0, requis 5) X-mx-serv-inrialpes-fr-MailScanner-From: eric.haines@autodesk.com X-Spam-Status: LOW ; 0 X-Spam-Status: No X-Loop: globillum@imag.fr X-Sequence: 350 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-Virus-Scanned: by amavisd-new X-Spam-TU-Processing-Host: neelix X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 This is a multi-part message in MIME format. --------------090700090804030907010204 Content-Type: text/plain; charset=windows-1252; format=flowed Content-Transfer-Encoding: 8bit Ray Tracing News v20 n1 (wow, 20 years?) is out at http://raytracingnews.org/rtnv20n1.html Please do give the puzzle a try, I'd love to see an intuitive answer for this one, Eric Attachment Converted: "C:\meine daten\eudora\Attach ab 2007.02.16\msg-25689-5051.txt" ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- --------------090700090804030907010204 Content-Type: text/plain; charset=windows-1252; name="msg-25689-5051.txt" Content-Transfer-Encoding: 7bit Content-Disposition: attachment; filename="msg-25689-5051.txt" Ray Tracing News v20 n1 (wow, 20 years?) is out at http://raytracingnews.org/rtnv20n1.html Please do give the puzzle a try, I'd love to see an intuitive answer for this one, Eric --------------090700090804030907010204-- From Return-Path: Received: from neelix.kom.tuwien.ac.at (neelix.kom.tuwien.ac.at [192.35.241.67]) by cg.tuwien.ac.at (8.13.4/8.13.4/Debian-3sarge3) with ESMTP id l545vpfr023010; Mon, 4 Jun 2007 07:57:52 +0200 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by neelix.kom.tuwien.ac.at (8.13.7/8.13.7) with ESMTP id l545vg8M010894; Mon, 4 Jun 2007 07:57:42 +0200 (MEST) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id l545vfHT005070; Mon, 4 Jun 2007 07:57:41 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id l545vWSp005059; Mon, 4 Jun 2007 07:57:32 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id l545s5pr003977 for ; Mon, 4 Jun 2007 07:54:05 +0200 Received: from mail99.megamailservers.com (mail99.megamailservers.com [216.251.36.99]) by imag.imag.fr (8.13.8/8.13.8) with ESMTP id l545rYfR003315 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO) for ; Mon, 4 Jun 2007 07:53:54 +0200 (CEST) X-POP-User: ian_ashdown.helios32.com Received: from Ian (S01060006257abbc2.vn.shawcable.net [24.81.109.183]) by mail99.megamailservers.com (8.13.6.20060614/8.13.1) with ESMTP id l544ECSa009712 for ; Mon, 4 Jun 2007 00:14:20 -0400 From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: 07/06/03 Release of RADBIB and GITHESIS Date: Sun, 3 Jun 2007 21:13:04 -0700 Organization: byHeart Consultants Limited Message-ID: <000301c7a65e$a8700a00$6401a8c0@Ian> MIME-Version: 1.0 X-Mailer: Microsoft Office Outlook 11 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2900.3028 Thread-Index: AcemXqYX0Yowmy5iQuedwKQXsFhLeg== X-Greylist: Delayed for 01:39:28 by milter-greylist-3.0 (imag.imag.fr [129.88.30.1]); Mon, 04 Jun 2007 07:53:54 +0200 (CEST) X-IMAG-MailScanner-Information: Please contact IMAG DMI for more information X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-From: ian_ashdown@helios32.com X-Loop: globillum@imag.fr X-Sequence: 351 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/html; charset=windows-1252 X-Virus-Scanned: by amavisd-new X-Spam-Status: LOW ; 0 X-Spam-TU-Processing-Host: neelix X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

ANNOUNCE: 07/04/03 Release of RADBIB and GITHESIS

RADBIB is a comprehensive bibliography of radiosity, photon mapping, and related global illumination papers, theses, articles, and books. It currently includes 2,597 references -- 14 new additions since its 07/05/03 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of June 3, 2007) from:

  http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 323 references to radiosity, photon mapping, and related global illumination theses -- no new additions since the 07/05/03 release.

NOTE: There is also an unpublished two-page manuscript in the Resources section called "Simplifying Eigenvector Radiosity." If you have ever wanted to solve the radiosity equation directly rather than iteratively …

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

Ian Ashdown, P. Eng., LC, FIES
President
byHeart Consultants Limited
http://www.helios32.com

 

------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by cg.tuwien.ac.at (8.13.4/8.13.4/Debian-3sarge3) with ESMTP id l6J81AOO024866; Thu, 19 Jul 2007 10:01:10 +0200 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.13.7/8.13.7) with ESMTP id l6J7vJqW015823; Thu, 19 Jul 2007 09:57:20 +0200 (MEST) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id l6J7vJSA021834; Thu, 19 Jul 2007 09:57:19 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id l6J7vEWB021828; Thu, 19 Jul 2007 09:57:14 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id l6J7rqIG019764 for ; Thu, 19 Jul 2007 09:53:52 +0200 Received: from mail97.megamailservers.com (mail97.megamailservers.com [216.251.36.97]) by imag.imag.fr (8.13.8/8.13.8) with ESMTP id l6J7rciD012084 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO) for ; Thu, 19 Jul 2007 09:53:40 +0200 (CEST) X-POP-User: ian_ashdown.helios32.com Received: from Ian (S01060006257abbc2.vn.shawcable.net [24.81.109.239]) by mail97.megamailservers.com (8.13.6.20060614/8.13.1) with ESMTP id l6J5fQ0u011905 for ; Thu, 19 Jul 2007 01:41:31 -0400 From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: 07/07/18 Release of RADBIB and GITHESIS Date: Wed, 18 Jul 2007 22:38:58 -0700 Organization: byHeart Consultants Limited Message-ID: <005a01c7c9c7$1bba2f50$6b01a8c0@Ian> MIME-Version: 1.0 X-Mailer: Microsoft Office Outlook 11 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2900.3138 Thread-Index: AcfJxxqZvkEJ6zDMQ++UvTkw0gm2ew== X-Greylist: Sender is SPF-compliant, not delayed by milter-greylist-3.0 (tuvok.kom.tuwien.ac.at [192.35.241.66]); Thu, 19 Jul 2007 10:01:10 +0200 (MEST) X-Greylist: Delayed for 02:12:05 by milter-greylist-3.0 (imag.imag.fr [129.88.30.1]); Thu, 19 Jul 2007 09:53:40 +0200 (CEST) X-IMAG-MailScanner-Information: Please contact IMAG DMI for more information X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-From: ian_ashdown@helios32.com X-Loop: globillum@imag.fr X-Sequence: 354 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/html; charset=windows-1252 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit ANNOUNCE: 07/07/18 Release of RADBIB and GITHESIS

ANNOUNCE: 07/07/18 Release of RADBIB and GITHESIS

RADBIB is a comprehensive bibliography of radiosity, photon mapping, and related global illumination papers, theses, articles, and books. It currently includes 2,610 references -- 13 new additions since its 07/06/03 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of July 18, 2007) from:

  http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 323 references to radiosity, photon mapping, and related global illumination theses -- no new additions since the 07/05/03 release.

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

Ian Ashdown, P. Eng., LC, FIES
President
byHeart Consultants Limited
http://www.helios32.com

------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by cg.tuwien.ac.at (8.13.4/8.13.4/Debian-3sarge3) with ESMTP id l7IHfC8Z001185; Sat, 18 Aug 2007 19:41:12 +0200 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.13.7/8.13.7) with ESMTP id l7IHf75N004662; Sat, 18 Aug 2007 19:41:08 +0200 (MEST) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id l7IHf7s0000698; Sat, 18 Aug 2007 19:41:07 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id l7IHevQK000690; Sat, 18 Aug 2007 19:40:57 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id l7IHbeO3032086 for ; Sat, 18 Aug 2007 19:37:40 +0200 Received: from mail57.megamailservers.com (mail57.megamailservers.com [216.251.36.57]) by imag.imag.fr (8.13.8/8.13.8) with ESMTP id l7IHatT9006818 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO) for ; Sat, 18 Aug 2007 19:36:57 +0200 (CEST) X-POP-User: janet_ashdown.helios32.com Received: from Ian (S01060006257abbc2.vn.shawcable.net [24.81.109.239]) by mail57.megamailservers.com (8.13.6.20060614/8.13.1) with ESMTP id l7IGueUx005905 for ; Sat, 18 Aug 2007 12:56:45 -0400 From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: 07/08/18 Release of RADBIB and GITHESIS Date: Sat, 18 Aug 2007 09:53:17 -0700 Organization: byHeart Consultants Limited Message-ID: <001401c7e1b8$475bd060$7801a8c0@Ian> MIME-Version: 1.0 X-Mailer: Microsoft Office Outlook 11 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2900.3138 Thread-Index: AcfhuEZVFJuh6za8T4K8R3BNID/hPQ== X-Greylist: Sender is SPF-compliant, not delayed by milter-greylist-3.0 (tuvok.kom.tuwien.ac.at [192.35.241.66]); Sat, 18 Aug 2007 19:41:11 +0200 (MEST) X-Greylist: Delayed for 00:40:08 by milter-greylist-3.0 (imag.imag.fr [129.88.30.1]); Sat, 18 Aug 2007 19:36:58 +0200 (CEST) X-IMAG-MailScanner-Information: Please contact IMAG DMI for more information X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-From: ian_ashdown@helios32.com X-Loop: globillum@imag.fr X-Sequence: 355 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/html; charset=windows-1252 X-Virus-Scanned: by amavisd-new X-Spam-Status: LOW ; -7 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

ANNOUNCE: 07/08/18 Release of RADBIB and GITHESIS

RADBIB is a comprehensive bibliography of radiosity, photon mapping, and related global illumination papers, theses, articles, and books. It currently includes 2,616 references -- 6 new additions since its 07/07/18 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of August 18, 2007) from:

  http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 323 references to radiosity, photon mapping, and related global illumination theses -- no new additions since the 07/07/18 release.

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

Ian Ashdown, P. Eng., LC, FIES
President
byHeart Consultants Limited
http://www.helios32.com



 

------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from tuvok.kom.tuwien.ac.at (tuvok.kom.tuwien.ac.at [192.35.241.66]) by cg.tuwien.ac.at (8.13.8/8.13.8/Debian-3) with ESMTP id l9J663gr014346; Fri, 19 Oct 2007 08:06:03 +0200 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.13.7/8.13.7) with ESMTP id l9J65t9S004410; Fri, 19 Oct 2007 08:05:56 +0200 (MEST) X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id l9J65toi025310; Fri, 19 Oct 2007 08:05:55 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id l9J65o0i025302; Fri, 19 Oct 2007 08:05:50 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id l9J62dSj023284 for ; Fri, 19 Oct 2007 08:02:39 +0200 Received: from server.agi32.com (unknown.ord.scnet.net [66.225.254.249] (may be forged)) by imag.imag.fr (8.13.8/8.13.8) with ESMTP id l9J62Fpr027684 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO) for ; Fri, 19 Oct 2007 08:02:17 +0200 (CEST) Received: from [24.81.109.239] (helo=Ian) by server.agi32.com with esmtpa (Exim 4.68) (envelope-from ) id 1IikUe-00011z-MO for globillum@imag.fr; Thu, 18 Oct 2007 23:33:57 -0600 From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: 07/10/18 Release of RADBIB and GITHESIS Date: Thu, 18 Oct 2007 22:33:51 -0700 Organization: byHeart Consultants Limited Message-ID: <000301c81211$a3b45e70$6901a8c0@Ian> MIME-Version: 1.0 X-Mailer: Microsoft Office Outlook 11 Thread-Index: AcgSEaHcokaRFdCdSlKul0tGYxhLLA== X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2900.3198 X-AntiAbuse: This header was added to track abuse, please include it with any abuse report X-AntiAbuse: Primary Hostname - server.agi32.com X-AntiAbuse: Original Domain - imag.fr X-AntiAbuse: Originator/Caller UID/GID - [47 12] / [47 12] X-AntiAbuse: Sender Address Domain - helios32.com X-Greylist: Sender is SPF-compliant, not delayed by milter-greylist-3.0 (tuvok.kom.tuwien.ac.at [192.35.241.66]); Fri, 19 Oct 2007 08:06:03 +0200 (MEST) X-Greylist: Delayed for 00:28:16 by milter-greylist-3.0 (imag.imag.fr [129.88.30.1]); Fri, 19 Oct 2007 08:02:18 +0200 (CEST) X-IMAG-MailScanner-Information: Please contact IMAG DMI for more information X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-From: ian_ashdown@helios32.com X-Loop: globillum@imag.fr X-Sequence: 357 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/html; charset=windows-1252 X-Virus-Scanned: by amavisd-new X-Spam-Status: LOW ; -25 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

ANNOUNCE: 07/10/18 Release of RADBIB and GITHESIS

RADBIB is a comprehensive bibliography of radiosity, photon mapping, and related global illumination papers, theses, articles, and books. It currently includes 2,646 references -- 30 new additions since its 07/08/18 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of October 18, 2007) from:

  http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 324 references to radiosity, photon mapping, and related global illumination theses -- one new addition since the 07/08/18 release.

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

Ian Ashdown, P. Eng., LC, FIES
President
byHeart Consultants Limited
http://www.helios32.com



 

------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-Path: Received: from neelix.kom.tuwien.ac.at (neelix.kom.tuwien.ac.at [192.35.241.67]) by cg.tuwien.ac.at (8.13.8/8.13.8/Debian-3) with ESMTP id l9RKVRkI009744; Sat, 27 Oct 2007 22:31:27 +0200 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by neelix.kom.tuwien.ac.at (8.13.8/8.13.8) with ESMTP id l9RKVM4j028051; Sat, 27 Oct 2007 22:31:22 +0200 X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id l9RKVLtD002858; Sat, 27 Oct 2007 22:31:21 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id l9RKVKUK002853; Sat, 27 Oct 2007 22:31:20 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id l9RKUKfp001827 for ; Sat, 27 Oct 2007 22:30:20 +0200 Received: from server.agi32.com (unknown.ord.scnet.net [66.225.254.249] (may be forged)) by imag.imag.fr (8.13.8/8.13.8) with ESMTP id l9RKU74A027446 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO) for ; Sat, 27 Oct 2007 22:30:09 +0200 (CEST) Received: from s01060006257abbc2.vn.shawcable.net ([24.81.109.239] helo=Ian) by server.agi32.com with esmtpa (Exim 4.68) (envelope-from ) id 1IlsIG-0002lZ-Sq for globillum@imag.fr; Sat, 27 Oct 2007 14:30:05 -0600 From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: 07/10/27 Release of RADBIB and GITHESIS Date: Sat, 27 Oct 2007 13:29:49 -0700 Organization: byHeart Consultants Limited Message-ID: <000401c818d8$1f1372f0$7301a8c0@Ian> MIME-Version: 1.0 X-Mailer: Microsoft Office Outlook 11 Thread-Index: AcgY16dfPP3NZNyiQxOq47HsiC5aLQ== X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2900.3198 X-AntiAbuse: This header was added to track abuse, please include it with any abuse report X-AntiAbuse: Primary Hostname - server.agi32.com X-AntiAbuse: Original Domain - imag.fr X-AntiAbuse: Originator/Caller UID/GID - [47 12] / [47 12] X-AntiAbuse: Sender Address Domain - helios32.com X-Greylist: Sender is SPF-compliant, not delayed by milter-greylist-4.0rc1 (neelix.kom.tuwien.ac.at [192.35.241.67]); Sat, 27 Oct 2007 22:31:27 +0200 (CEST) X-Greylist: IP, sender and recipient auto-whitelisted, not delayed by milter-greylist-3.0 (imag.imag.fr [129.88.30.1]); Sat, 27 Oct 2007 22:30:10 +0200 (CEST) X-IMAG-MailScanner-Information: Please contact IMAG DMI for more information X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-From: ian_ashdown@helios32.com X-Loop: globillum@imag.fr X-Sequence: 358 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/html; charset=windows-1252 X-Virus-Scanned: by amavisd-new X-Spam-Status: LOW ; 0 X-Spam-TU-Processing-Host: neelix X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

ANNOUNCE: 07/10/27 Release of RADBIB and GITHESIS

RADBIB is a comprehensive bibliography of radiosity, photon mapping, and related global illumination papers, theses, articles, and books. It currently includes 2,657 references -- 11 new additions since its 07/10/18 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of October 27, 2007) from:

  http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 324 references to radiosity, photon mapping, and related global illumination theses -- no new additions since the 07/10/18 release.

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

Ian Ashdown, P. Eng., LC, FIES
President
byHeart Consultants Limited
http://www.helios32.com

 

------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-path: Envelope-to: wp@cg.tuwien.ac.at Delivery-date: Thu, 13 Mar 2008 07:09:17 +0100 Received: from tuvok.kom.tuwien.ac.at ([192.35.241.66]:45430) by christl.cg.tuwien.ac.at with esmtp (Exim 4.63) (envelope-from ) id 1JZgcv-0007kz-9G; Thu, 13 Mar 2008 07:09:17 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.14.1/8.14.1) with ESMTP id m2D695gV013695; Thu, 13 Mar 2008 07:09:05 +0100 X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id m2D695hj015331; Thu, 13 Mar 2008 07:09:05 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id m2D694i9015324; Thu, 13 Mar 2008 07:09:04 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id m2D63E74023662 for ; Thu, 13 Mar 2008 07:03:28 +0100 Received: from server.agi32.com (unknown.ord.scnet.net [66.225.254.249] (may be forged)) by imag.imag.fr (8.13.8/8.13.8) with ESMTP id m2D55OHC007967 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO) for ; Thu, 13 Mar 2008 06:05:26 +0100 (CET) Received: from s01060006257abbc2.vn.shawcable.net ([24.84.242.155] helo=Ian) by server.agi32.com with esmtpa (Exim 4.68) (envelope-from ) id 1JZeYY-0001ER-In for globillum@imag.fr; Wed, 12 Mar 2008 21:56:39 -0600 From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: 08/03/12 Release of RADBIB and GITHESIS Date: Wed, 12 Mar 2008 20:56:26 -0700 Organization: byHeart Consultants Limited Message-ID: <000601c884be$38056730$6401a8c0@Ian> MIME-Version: 1.0 X-Mailer: Microsoft Office Outlook 11 Thread-Index: AciEvjYhdmcwgvY7SVKwck1mD2V4hw== X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2900.3198 X-AntiAbuse: This header was added to track abuse, please include it with any abuse report X-AntiAbuse: Primary Hostname - server.agi32.com X-AntiAbuse: Original Domain - imag.fr X-AntiAbuse: Originator/Caller UID/GID - [47 12] / [47 12] X-AntiAbuse: Sender Address Domain - helios32.com X-Greylist: Sender is SPF-compliant, not delayed by milter-greylist-4.0rc1 (tuvok.kom.tuwien.ac.at [192.35.241.66]); Thu, 13 Mar 2008 07:09:17 +0100 (CET) X-Greylist: Delayed for 01:08:43 by milter-greylist-3.0 (imag.imag.fr [129.88.30.1]); Thu, 13 Mar 2008 06:05:26 +0100 (CET) X-IMAG-MailScanner-Information: Please contact MI2S MIM for more information X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-From: ian_ashdown@helios32.com X-Loop: globillum@imag.fr X-Sequence: 362 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/html; charset=windows-1252 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; 0 X-Spam-TU-Processing-Host: tuvok.kom.tuwien.ac.at X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

ANNOUNCE: 08/03/12 Release of RADBIB and GITHESIS

RADBIB is a comprehensive bibliography of radiosity, photon mapping, and related global illumination papers, theses, articles, and books. It currently includes 2,671 references -- 14 new additions since its 08/03/12 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of March 12, 2008) from:

  http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 328 references to radiosity, photon mapping, and related global illumination theses -- two new additions since the 07/10/27 release.

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

Ian Ashdown, P. Eng., LC, FIES
President
byHeart Consultants Limited
http://www.helios32.com

 

------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-path: Envelope-to: wp@cg.tuwien.ac.at Delivery-date: Fri, 14 Mar 2008 11:46:38 +0100 Received: from neelix.kom.tuwien.ac.at ([192.35.241.67]:57200) by christl.cg.tuwien.ac.at with esmtp (Exim 4.63) (envelope-from ) id 1Ja7Qr-0001Fv-SL; Fri, 14 Mar 2008 11:46:37 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by neelix.kom.tuwien.ac.at (8.14.1/8.14.1) with ESMTP id m2EAkVIh032093; Fri, 14 Mar 2008 11:46:32 +0100 X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id m2EAkVID002749; Fri, 14 Mar 2008 11:46:31 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id m2EAkUZ8002743; Fri, 14 Mar 2008 11:46:30 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id m2EAkEL5001753 for ; Fri, 14 Mar 2008 11:46:14 +0100 Received: from mail.vsiltd.co.uk (mail.vsiltd.co.uk [195.152.206.150]) by imag.imag.fr (8.13.8/8.13.8) with ESMTP id m2EAiwiI024481 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO) for ; Fri, 14 Mar 2008 11:44:59 +0100 (CET) Received: from macy.ows.local ([195.152.206.70]) by mail.vsiltd.co.uk (8.13.8/8.13.8) with ESMTP id m2EANLZL031179 for ; Fri, 14 Mar 2008 10:23:21 GMT MIME-Version: 1.0 X-MimeOLE: Produced By Microsoft Exchange V6.5 Subject: ray tracing for games engines Date: Fri, 14 Mar 2008 10:23:18 -0000 Message-ID: Thread-Topic: ray tracing for games engines Thread-Index: AciFvWubOY080hkCRreWJHTP2aO9bA== From: "Neil Gatenby" To: globillum@imag.fr X-VSI-MailScanner-Information: Please contact ITS for more information X-VSI-MailScanner: Found to be clean X-VSI-MailScanner-SpamCheck: not spam, SpamAssassin (not cached, score=-2.413, required 6, AWL 0.09, BAYES_00 -2.60, RDNS_NONE 0.10) X-VSI-MailScanner-From: neil.gatenby@lightworkdesign.com X-VSI-MailScanner-To: globillum@imag.fr X-Spam-Status: LOW ; 0 X-Spam-Status: No X-Greylist: Sender is SPF-compliant, not delayed by milter-greylist-4.0rc1 (neelix.kom.tuwien.ac.at [192.35.241.67]); Fri, 14 Mar 2008 11:46:37 +0100 (CET) X-Greylist: Delayed for 00:21:22 by milter-greylist-3.0 (imag.imag.fr [129.88.30.1]); Fri, 14 Mar 2008 11:45:00 +0100 (CET) X-IMAG-MailScanner-Information: Please contact MI2S MIM for more information X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-From: neil.gatenby@lightworkdesign.com X-MIME-Autoconverted: from quoted-printable to 8bit by chopinette.imag.fr id m2EAkEL5001753 X-Loop: globillum@imag.fr X-Sequence: 363 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-Virus-Scanned: by amavisd-new X-Spam-TU-Processing-Host: neelix.kom.tuwien.ac.at X-Mozilla-Status: 9001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Content-class: urn:content-classes:message Content-Type: text/plain; charset="us-ascii" Content-Transfer-Encoding: 8bit Hi Not really my thing, but possibly of interest to some receiving this http://games.slashdot.org/games/08/03/12/1918250.shtml Neil Neil Gatenby Senior Software Specialist Lightwork Design, Rutledge House, 78 Clarkehouse Road, Sheffield, S10 2LJ, UK Tel: +44 114 266 8404, Fax: +44 114 1383 neil.gatenby@lightworkdesign.com, http://www.lightworkdesign.com/ ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-path: Envelope-to: wp@cg.tuwien.ac.at Delivery-date: Mon, 07 Jul 2008 16:08:00 +0200 Received: from tuvok.kom.tuwien.ac.at ([192.35.241.66]:42561) by christl.cg.tuwien.ac.at with esmtp (Exim 4.63) (envelope-from ) id 1KFrNo-0000cC-DK; Mon, 07 Jul 2008 16:08:00 +0200 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.14.1/8.14.1) with ESMTP id m67E7YAZ017720; Mon, 7 Jul 2008 16:07:35 +0200 X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id m67E7Y8I019489; Mon, 7 Jul 2008 16:07:34 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id m67E7Vto019484; Mon, 7 Jul 2008 16:07:31 +0200 Received: from harmonie.imag.fr (harmonie.imag.fr [147.171.130.40]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id m67E6JRh016663 for ; Mon, 7 Jul 2008 16:06:19 +0200 Received: from server.agi32.com (unknown.ord.scnet.net [66.225.254.249] (may be forged)) by harmonie.imag.fr (8.13.8/8.13.8) with ESMTP id m67E5QQu003537 for ; Mon, 7 Jul 2008 16:05:28 +0200 (CEST) Received: from s01060006257abbc2.vn.shawcable.net ([24.84.242.22] helo=Ian) by server.agi32.com with esmtpa (Exim 4.69) (envelope-from ) id 1KFqVf-0007wa-CK for globillum@imag.fr; Mon, 07 Jul 2008 07:12:04 -0600 From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: 08/07/06 Release of RADBIB and GITHESIS Date: Mon, 7 Jul 2008 06:11:54 -0700 Organization: byHeart Consultants Limited Message-ID: <000001c8e033$0b015610$6501a8c0@Ian> MIME-Version: 1.0 X-Mailer: Microsoft Office Outlook 11 Thread-Index: AcjgMwXKiAkkjDn+TiurQNveS46MjQ== X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2900.3198 X-AntiAbuse: This header was added to track abuse, please include it with any abuse report X-AntiAbuse: Primary Hostname - server.agi32.com X-AntiAbuse: Original Domain - imag.fr X-AntiAbuse: Originator/Caller UID/GID - [47 12] / [47 12] X-AntiAbuse: Sender Address Domain - helios32.com X-Greylist: Sender passed SPF test, not delayed by milter-greylist-4.1.1 (tuvok.kom.tuwien.ac.at [192.35.241.66]); Mon, 07 Jul 2008 16:08:00 +0200 (CEST) X-Greylist: Delayed for 00:51:34 by milter-greylist-3.0 (harmonie.imag.fr [147.171.130.40]); Mon, 07 Jul 2008 16:05:28 +0200 (CEST) X-IMAG-MailScanner-Information: Please contact MI2S MIM for more information X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-From: ian_ashdown@helios32.com X-Loop: globillum@imag.fr X-Sequence: 370 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/html; charset=windows-1252 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; -6 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok.kom.tuwien.ac.at X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

ANNOUNCE: 08/07/06 Release of RADBIB and GITHESIS

RADBIB is a comprehensive bibliography of radiosity, photon mapping, and related global illumination papers, theses, articles, and books. It currently includes 2,683 references -- 12 new additions since its 08/03/12 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of July 6, 2008) from:

  http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 331 references to radiosity, photon mapping, and related global illumination theses -- three new additions since the 08/03/12 release.

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

Ian Ashdown, P. Eng., LC, FIES
President
byHeart Consultants Limited
http://www.helios32.com

 

------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-path: Envelope-to: wp@cg.tuwien.ac.at Delivery-date: Fri, 18 Jul 2008 15:34:38 +0200 Received: from tuvok.kom.tuwien.ac.at ([192.35.241.66]:45858) by christl.cg.tuwien.ac.at with esmtp (Exim 4.63) (envelope-from ) id 1KJq6Y-0003Vk-7I; Fri, 18 Jul 2008 15:34:38 +0200 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.14.1/8.14.1) with ESMTP id m6IDYW95004515; Fri, 18 Jul 2008 15:34:32 +0200 X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id m6IDYVS6001105; Fri, 18 Jul 2008 15:34:31 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id m6IDYUgg001101; Fri, 18 Jul 2008 15:34:30 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id m6IDY1dh030984 for ; Fri, 18 Jul 2008 15:34:01 +0200 Received: from pantheon-po11.its.yale.edu (pantheon-po11.its.yale.edu [130.132.50.69]) by imag.imag.fr (8.13.8/8.13.8) with ESMTP id m6IDWiss021341 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=FAIL) for ; Fri, 18 Jul 2008 15:32:46 +0200 (CEST) Received: from Edith (vpn147.its.yale.edu [130.132.120.147]) by pantheon-po11.its.yale.edu (8.12.11.20060308/8.12.11) with ESMTP id m6IDKfPY010017 for ; Fri, 18 Jul 2008 09:20:45 -0400 From: "Holly Rushmeier" To: globillum@imag.fr Subject: Search for new EiC of ACM TAP Date: Fri, 18 Jul 2008 09:20:36 -0400 Message-ID: <000c01c8e8d9$120e6660$6501a8c0@cs.yale.edu> MIME-Version: 1.0 X-Mailer: Microsoft Office Outlook 11 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2900.3198 Thread-Index: Acjo2RAvG27gnOZLTgS1LXNz3+WehQ== X-YaleITSMailFilter: Version 1.2c (attachment(s) not renamed) X-Greylist: Sender passed SPF test, not delayed by milter-greylist-4.1.1 (tuvok.kom.tuwien.ac.at [192.35.241.66]); Fri, 18 Jul 2008 15:34:38 +0200 (CEST) X-Greylist: Delayed for 00:11:50 by milter-greylist-3.0 (imag.imag.fr [129.88.30.1]); Fri, 18 Jul 2008 15:32:46 +0200 (CEST) X-IMAG-MailScanner-Information: Please contact MI2S MIM for more information X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-From: holly@acm.org X-Loop: globillum@imag.fr X-Sequence: 371 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-Virus-Scanned: by amavisd-new X-Spam-Status: LOW ; 0 X-Spam-TU-Processing-Host: tuvok.kom.tuwien.ac.at X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit A search is currently being conducted for the next Editor-in-Chief of ACM Transactions on Applied Perception. Please see the announcement at: http://tap.acm.org/EditorInChief.html to apply for the position yourself, or to submit a nomination. -- Holly Rushmeier _______________ Holly Rushmeier, Dept. of CS, Yale University, PO Box 208285, New Haven,CT 06520-8285,Phone: (203)432-4091, holly@acm.org ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-path: Envelope-to: wp@cg.tuwien.ac.at Delivery-date: Tue, 05 Aug 2008 15:58:16 +0200 Received: from neelix.kom.tuwien.ac.at ([192.35.241.67]:41288) by christl.cg.tuwien.ac.at with esmtp (Exim 4.63) (envelope-from ) id 1KQN3I-0004dn-Ae; Tue, 05 Aug 2008 15:58:16 +0200 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by neelix.kom.tuwien.ac.at (8.14.1/8.14.1) with ESMTP id m75Dw94i013465; Tue, 5 Aug 2008 15:58:09 +0200 X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id m75Dw8Ru014056; Tue, 5 Aug 2008 15:58:08 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id m75Dw7Ql014045; Tue, 5 Aug 2008 15:58:07 +0200 Received: from ebene.inrialpes.fr (ebene.inrialpes.fr [194.199.18.70]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id m75DvkD8013069 for ; Tue, 5 Aug 2008 15:57:46 +0200 Received: from pantheon-po06.its.yale.edu (pantheon-po06.its.yale.edu [130.132.50.36]) by ebene.inrialpes.fr (8.13.6/8.13.8) with ESMTP id m75Dvd28019339 for ; Tue, 5 Aug 2008 15:57:40 +0200 (MEST) Received: from Edith (dhcp128036161188.central.yale.edu [128.36.161.188]) by pantheon-po06.its.yale.edu (8.12.11.20060308/8.12.11) with ESMTP id m75DdqYx025316 for ; Tue, 5 Aug 2008 09:39:56 -0400 From: "Holly Rushmeier" To: globillum@imag.fr Subject: ACM TOG EiC Search Date: Tue, 5 Aug 2008 09:39:52 -0400 Message-ID: <000001c8f700$bd77b9e0$bca12480@cs.yale.edu> MIME-Version: 1.0 X-Mailer: Microsoft Office Outlook 11 Thread-Index: Acj3ALtOLJT5xU9OR/uxndmB8EhqMw== X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2900.3198 X-YaleITSMailFilter: Version 1.2c (attachment(s) not renamed) X-Greylist: Sender passed SPF test, not delayed by milter-greylist-4.1.1 (neelix.kom.tuwien.ac.at [192.35.241.67]); Tue, 05 Aug 2008 15:58:16 +0200 (CEST) X-Greylist: Delayed for 00:11:21 by milter-greylist-3.0 (ebene.inrialpes.fr [194.199.18.70]); Tue, 05 Aug 2008 15:57:41 +0200 (MEST) X-IMAG-MailScanner-Information: Please contact MI2S MIM for more information X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-From: holly@acm.org X-Spam-Status: LOW ; 0 X-Spam-Status: No X-Loop: globillum@imag.fr X-Sequence: 373 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-Virus-Scanned: by amavisd-new X-Spam-TU-Processing-Host: neelix.kom.tuwien.ac.at X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Recently I wrote that a search was being conducted for a new Editor-in-Chief for ACM Transactions on Applied Perception. There is now also a search ongoing for a new Editor-in-Chief for ACM Transactions on Graphics. See the call at: http://tog.acm.org/ Finding excellent people for these two positions is vital for the continuing health of our research community. Please consider applying, or nominating someone. -- Holly _______________ Holly Rushmeier, Dept. of CS, Yale University, PO Box 208285, New Haven,CT 06520-8285,Phone: (203)432-4091, holly@acm.org ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-path: Envelope-to: wp@cg.tuwien.ac.at Delivery-date: Fri, 05 Sep 2008 08:07:52 +0200 Received: from tuvok.kom.tuwien.ac.at ([192.35.241.66]:35414) by christl.cg.tuwien.ac.at with esmtp (Exim 4.63) (envelope-from ) id 1KbUU4-000184-CO; Fri, 05 Sep 2008 08:07:52 +0200 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.14.1/8.14.1) with ESMTP id m8567h6S009723; Fri, 5 Sep 2008 08:07:43 +0200 X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id m8567hWW028305; Fri, 5 Sep 2008 08:07:43 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id m8567fNr028300; Fri, 5 Sep 2008 08:07:41 +0200 Received: from harmonie.imag.fr (harmonie.imag.fr [147.171.130.40]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id m8566kdM027302 for ; Fri, 5 Sep 2008 08:06:46 +0200 Received: from server.agi32.com (unknown.ord.scnet.net [66.225.254.249] (may be forged)) by harmonie.imag.fr (8.13.8/8.13.8) with ESMTP id m8565Qdf015219 for ; Fri, 5 Sep 2008 08:05:27 +0200 (CEST) Received: from s01060006257abbc2.vn.shawcable.net ([24.80.79.8] helo=Ian) by server.agi32.com with esmtpa (Exim 4.69) (envelope-from ) id 1KbTLb-0002mX-My for globillum@imag.fr; Thu, 04 Sep 2008 22:55:03 -0600 From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: 08/09/04 Release of RADBIB and GITHESIS Date: Thu, 4 Sep 2008 21:54:55 -0700 Organization: byHeart Consultants Limited Message-ID: <001501c90f13$8bf8bf60$6501a8c0@Ian> MIME-Version: 1.0 X-Mailer: Microsoft Office Outlook 11 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2900.3350 Thread-Index: AckPE4o9r/PWekbBRDSll2vIcBKQdw== X-AntiAbuse: This header was added to track abuse, please include it with any abuse report X-AntiAbuse: Primary Hostname - server.agi32.com X-AntiAbuse: Original Domain - imag.fr X-AntiAbuse: Originator/Caller UID/GID - [47 12] / [47 12] X-AntiAbuse: Sender Address Domain - helios32.com X-Greylist: Sender passed SPF test, not delayed by milter-greylist-4.1.1 (tuvok.kom.tuwien.ac.at [192.35.241.66]); Fri, 05 Sep 2008 08:07:52 +0200 (CEST) X-Greylist: Delayed for 01:10:12 by milter-greylist-3.0 (harmonie.imag.fr [147.171.130.40]); Fri, 05 Sep 2008 08:05:27 +0200 (CEST) X-IMAG-MailScanner-Information: Please contact MI2S MIM for more information X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-From: ian_ashdown@helios32.com X-Loop: globillum@imag.fr X-Sequence: 375 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/html; charset=windows-1252 X-Virus-Scanned: by amavisd-new X-Spam-Status: LOW ; 1 X-Spam-Level: + X-Spam-TU-Processing-Host: tuvok.kom.tuwien.ac.at X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

ANNOUNCE: 08/09/04 Release of RADBIB and GITHESIS

RADBIB is a comprehensive bibliography of radiosity, photon mapping, and related global illumination papers, theses, articles, and books. It currently includes 2,703 references -- 20 new additions since its 08/07/06 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of September 4, 2008) from:

  http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 334 references to radiosity, photon mapping, and related global illumination theses -- three new additions since the 08/07/06 release.

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

Ian Ashdown, P. Eng., LC, FIES
Cum Grano Salis
byHeart Consultants Limited
http://www.helios32.com



 

------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-path: Envelope-to: wp@cg.tuwien.ac.at Delivery-date: Fri, 05 Sep 2008 20:07:01 +0200 Received: from neelix.kom.tuwien.ac.at ([192.35.241.67]:54520) by christl.cg.tuwien.ac.at with esmtp (Exim 4.63) (envelope-from ) id 1Kbfi1-00035q-7m; Fri, 05 Sep 2008 20:07:01 +0200 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by neelix.kom.tuwien.ac.at (8.14.1/8.14.1) with ESMTP id m85I6nsB011222; Fri, 5 Sep 2008 20:06:49 +0200 X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id m85I6ndW006907; Fri, 5 Sep 2008 20:06:49 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id m85I6mkR006901; Fri, 5 Sep 2008 20:06:48 +0200 Received: from harmonie.imag.fr (harmonie.imag.fr [147.171.130.40]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id m85I5wnA005906 for ; Fri, 5 Sep 2008 20:05:58 +0200 Received: from server.agi32.com (unknown.ord.scnet.net [66.225.254.249] (may be forged)) by harmonie.imag.fr (8.13.8/8.13.8) with ESMTP id m85I4anX026469 for ; Fri, 5 Sep 2008 20:04:37 +0200 (CEST) Received: from s01060006257abbc2.vn.shawcable.net ([24.80.79.8] helo=Ian) by server.agi32.com with esmtpa (Exim 4.69) (envelope-from ) id 1Kbfbn-0006mU-4L for globillum@imag.fr; Fri, 05 Sep 2008 12:00:35 -0600 From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: (Another) Release ofRADBIB and GITHESIS Date: Fri, 5 Sep 2008 11:00:26 -0700 Organization: byHeart Consultants Limited Message-ID: <001e01c90f81$4888ea20$6501a8c0@Ian> MIME-Version: 1.0 X-Mailer: Microsoft Office Outlook 11 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2900.3350 Thread-Index: AckPgUagQqMXO5aVSlCAiGGN4LY10w== X-AntiAbuse: This header was added to track abuse, please include it with any abuse report X-AntiAbuse: Primary Hostname - server.agi32.com X-AntiAbuse: Original Domain - imag.fr X-AntiAbuse: Originator/Caller UID/GID - [47 12] / [47 12] X-AntiAbuse: Sender Address Domain - helios32.com X-Greylist: Sender passed SPF test, not delayed by milter-greylist-4.1.1 (neelix.kom.tuwien.ac.at [192.35.241.67]); Fri, 05 Sep 2008 20:07:01 +0200 (CEST) X-Greylist: IP, sender and recipient auto-whitelisted, not delayed by milter-greylist-3.0 (harmonie.imag.fr [147.171.130.40]); Fri, 05 Sep 2008 20:04:38 +0200 (CEST) X-IMAG-MailScanner-Information: Please contact MI2S MIM for more information X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-From: ian_ashdown@helios32.com X-Loop: globillum@imag.fr X-Sequence: 376 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/html; charset=windows-1252 X-Virus-Scanned: by amavisd-new X-Spam-Status: LOW ; 0 X-Spam-TU-Processing-Host: neelix.kom.tuwien.ac.at X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

Thanks to Per Christensen for pointing me to another 8 papers that I missed in yesterday’s release.

 

ANNOUNCE: 08/09/05 Release of RADBIB and GITHESIS

RADBIB is a comprehensive bibliography of radiosity, photon mapping, and related global illumination papers, theses, articles, and books. It currently includes 2,711 references -- 28 new additions since its 08/07/06 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of September 5, 2008) from:

  http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 334 references to radiosity, photon mapping, and related global illumination theses -- three new additions since the 08/07/06 release.

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

Ian Ashdown, P. Eng., LC, FIES
President
byHeart Consultants Limited
http://www.helios32.com

 

------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-path: Envelope-to: wp@cg.tuwien.ac.at Delivery-date: Mon, 29 Dec 2008 13:18:31 +0100 Received: from tuvok.kom.tuwien.ac.at ([192.35.241.66]:48350) by christl.cg.tuwien.ac.at with esmtp (Exim 4.63) (envelope-from ) id 1LHH4p-0004m1-47; Mon, 29 Dec 2008 13:18:31 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.14.1/8.14.1) with ESMTP id mBTCHwI0023434; Mon, 29 Dec 2008 13:17:58 +0100 X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id mBTCHvnW001236; Mon, 29 Dec 2008 13:17:57 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id mBTCHuA5001231; Mon, 29 Dec 2008 13:17:56 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id mBTCHAMv032697 for ; Mon, 29 Dec 2008 13:17:10 +0100 Received: from uni-sb.de (mail.uni-sb.de [134.96.252.33]) by imag.imag.fr (8.13.8/8.13.8) with ESMTP id mBTCCVh6029045 for ; Mon, 29 Dec 2008 13:12:42 +0100 (CET) Received: from mail.cs.uni-sb.de (mail.cs.uni-sb.de [134.96.254.200]) by uni-sb.de (8.14.3/2008091900) with ESMTP id mBTCCUP7029788 for ; Mon, 29 Dec 2008 13:12:30 +0100 (CET) Received: from scihparg.cs.uni-sb.de (scihparg.cs.uni-sb.de [134.96.249.75]) by mail.cs.uni-sb.de (8.14.3/2008120800) with ESMTP id mBTCCUsH007482 for ; Mon, 29 Dec 2008 13:12:30 +0100 (CET) Received: from 62-47-252-14.adsl.highway.telekom.at ([62.47.252.14] helo=[192.168.1.34]) by scihparg.cs.uni-sb.de with esmtpsa (TLS-1.0:DHE_RSA_AES_256_CBC_SHA:32) (Exim 4.50) id 1LHGyw-0002bW-QJ for globillum@imag.fr; Mon, 29 Dec 2008 13:12:30 +0100 Message-ID: <4958BEA8.2000102@cs.uni-sb.de> Date: Mon, 29 Dec 2008 13:12:24 +0100 From: Philipp Slusallek Organization: DFKI Saarbrücken & Saarland Universit y User-Agent: Thunderbird 2.0.0.18 (Windows/20081105) MIME-Version: 1.0 To: "Illumination List, Global" Content-Type: multipart/mixed; boundary="------------030200040809090102040104" X-SA-Exim-Connect-IP: 62.47.252.14 X-SA-Exim-Mail-From: slusallek@cs.uni-sb.de Subject: Saarland University is looking for several Junior Research Group Leaders in the Cluster of Excellence on Multimodal Computing and Interaction X-Spam-Checker-Version: SpamAssassin 3.0.3 (2005-04-27) on scihparg.cs.uni-sb.de X-Spam-Level: *+++++++ X-Spam-Status: LOW ; 17 X-Spam-Status: No, score=-2.7 required=5.0 tests=ALL_TRUSTED,AWL autolearn=disabled version=3.0.3 X-SA-Exim-Version: 4.2 (built Thu, 03 Mar 2005 10:44:12 +0100) X-SA-Exim-Scanned: Yes (on scihparg.cs.uni-sb.de) X-DCC-URT-Metrics: mail.cs.uni-sb.de; whitelist X-IMAG-MailScanner-Information: Please contact MI2S MIM for more information X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-From: slusallek@cs.uni-sb.de X-Loop: globillum@imag.fr X-Sequence: 382 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-TU-Processing-Host: tuvok.kom.tuwien.ac.at X-Greylist: Sender passed SPF test, not delayed by milter-greylist-4.1.1 (tuvok.kom.tuwien.ac.at [192.35.241.66]); Mon, 29 Dec 2008 13:18:31 +0100 (CET) X-Mozilla-Status: 9001 X-Mozilla-Status2: 00000000 This is a multi-part message in MIME format. --------------030200040809090102040104 Content-Type: text/plain; charset=windows-1252; format=flowed Content-Transfer-Encoding: 8bit Content-Type: text/plain; charset=UTF-8; format=flowed X-MIME-Autoconverted: from 8bit to quoted-printable by tuvok.kom.tuwien.ac.at id mBTCHwI0023434 Hi, This might be interesting to a few people on the list. All the best, Philipp -------- Saarland University is seeking to establish several Junior Research Groups (W1/W2) within the recently established Cluster of Excellence “œMultimodal Computing and Interactionâ€Â which was established by tthe German Research Foundation (DFG) within the framework of the German Excellence Initiative. The term “multimodalâ€Â describes tes the different types of digital information such as text, speech, images, video, graphics, and high-dimensional data, and the way it is perceived and communicated, particularly through vision, hearing, and human expression. The challenge is now to organize, understand, and search this multimodal information in a robust, efficient and intelligent way, and to create dependable systems that allow natural and intuitive multimodal interaction. We are looking for highly motivated young researchers with a background in the research areas of the cluster, including algorithmic foundations, secure and autonomous networked systems, open science web, information processing in the life sciences, visual computing, large-scale virtual environments, synthetic virtual characters, text and speech processing and multimodal dialog systems. Additional information on the Cluster of Excellence is available on http://www.mmci.uni-saarland.de. Group leaders will receive junior faculty status at Saarland University, including the right to supervise Bachelor, Master and PhD students. Positions are limited to five years. Applicants for W1 positions (phase I of the program) must have completed an outstanding PhD. Upon successful evaluation after two years, W1 group leaders are eligible for promotion to W2. Direct applicants for W2 positions (phase II of the program) must have completed a postdoc stay and must have demonstrated outstanding research potential and the ability to successfully lead their own research group. Junior research groups are equipped with a budget of 80k to 100k Euros per year to cover research personnel and other costs. Saarland University has leading departments in computer science and computational linguistics, with more than 200 PhD students working on topics related to the cluster (see http://www.informatik-saarland.de for additional information). The German Excellence Initiative recently awarded multi-million grants to the Cluster of Excellence ‬œMultimodal Computing and Interactionâ€Â as well as to the â“Saarbrücken Graduate School of Computer Scienceâ€Â. An important factor to tthis success were the close ties to the Max Planck Institute for Computer Science, the German Research Center for Artificial Intelligence (DFKI), and the Max Planck Institute for Software Systems which are co-located on the same campus. Candidates should submit their application (curriculum vitae, photograph, list of publications, short research plan, copies of degree certificates, copies of the five most important publications, list of five references) to the coordinator of the cluster, Prof. Hans-Peter Seidel, MPI for Computer Science, Campus E1 4, 66123 Saarbrücken, Germany. Please, also send your application as a single PDF file to applications@mmci.uni-saarland.de. The review of applications will begin on January 15, 2009, and applicants are strongly encouraged to submit applications by that date; however, applications will continue to be accepted until January 31, 2009. Final decisions will be made following a candidate symposium that will be held during March 9 â€â€œ 13, 2009. Saarland University is an equal opportunity employer. In accordance with its policy of increasing the proportion of women in this type of employment, the University actively encourages applications from women. For candidates with equal qualification, preference will be given to people with physical disabilities. Attachment Converted: "C:\meine daten\eudora\Attach ab 2008.11.04\slusallek1.vcf" ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- --------------030200040809090102040104 Content-Type: text/x-vcard; charset=windows-1252; name="slusallek1.vcf" Content-Transfer-Encoding: 7bit Content-Disposition: attachment; filename="slusallek1.vcf" begin:vcard fn:Philipp Slusallek n:Slusallek;Philipp org;quoted-printable:DFKI Saarbr=C3=BCcken & Saarland University;Agents and Simulated Reality adr;quoted-printable:;;Stuhlsatzenhausweg 3;Saarbr=C3=BCcken;;66123;Germany email;internet:slusallek@cs.uni-sb.de title:Scientific Director & Prof. Dr.-Ing. tel;work:+49 681 302 5377 tel;fax:+49 681 302 2235 tel;home:+49 6826 188 7132 tel;cell:+49 173 659 2518 x-mozilla-html:FALSE url:http://graphics.cs.uni-sb.de version:2.1 end:vcard --------------030200040809090102040104-- From Return-path: Envelope-to: wp@cg.tuwien.ac.at Delivery-date: Fri, 16 Jan 2009 07:35:38 +0100 Received: from neelix.kom.tuwien.ac.at ([192.35.241.67]:56718) by christl.cg.tuwien.ac.at with esmtp (Exim 4.63) (envelope-from ) id 1LNiIr-0005ic-KD; Fri, 16 Jan 2009 07:35:37 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by neelix.kom.tuwien.ac.at (8.14.1/8.14.1) with ESMTP id n0G6Z7KP006440; Fri, 16 Jan 2009 07:35:08 +0100 X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id n0G6Z7hs005301; Fri, 16 Jan 2009 07:35:07 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id n0G6Z4Sd005296; Fri, 16 Jan 2009 07:35:04 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id n0G6MtMH026990 for ; Fri, 16 Jan 2009 07:22:55 +0100 Received: from server.agi32.com (unknown.ord.scnet.net [66.225.254.249] (may be forged)) by imag.imag.fr (8.13.8/8.13.8) with ESMTP id n0G6JOeK012957 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO) for ; Fri, 16 Jan 2009 07:19:26 +0100 (CET) Received: from s01060006257abbc2.vn.shawcable.net ([24.87.90.99] helo=Ian) by server.agi32.com with esmtpa (Exim 4.69) (envelope-from ) id 1LNguJ-0006KT-MO; Thu, 15 Jan 2009 22:06:12 -0700 From: "Ian Ashdown" To: globillum@imag.fr Subject: BRDF data for tunnel materials? Date: Thu, 15 Jan 2009 21:05:42 -0800 Organization: byHeart Consultants Limited Message-ID: <41CFC639DB7748E4A45DDD9DCA9A7798@Ian> MIME-Version: 1.0 X-Mailer: Microsoft Office Outlook 11 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2900.5579 Thread-Index: Acl3PGOgD4ar9HprR1WCUPGi8m9stAAU6UvQ X-AntiAbuse: This header was added to track abuse, please include it with any abuse report X-AntiAbuse: Primary Hostname - server.agi32.com X-AntiAbuse: Original Domain - imag.fr X-AntiAbuse: Originator/Caller UID/GID - [47 12] / [47 12] X-AntiAbuse: Sender Address Domain - helios32.com X-Greylist: Sender passed SPF test, not delayed by milter-greylist-4.1.1 (neelix.kom.tuwien.ac.at [192.35.241.67]); Fri, 16 Jan 2009 07:35:37 +0100 (CET) X-Greylist: Delayed for 01:13:10 by milter-greylist-3.0 (imag.imag.fr [129.88.30.1]); Fri, 16 Jan 2009 07:19:27 +0100 (CET) X-IMAG-MailScanner-Information: Please contact MI2S MIM for more information X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-From: ian_ashdown@helios32.com X-Loop: globillum@imag.fr X-Sequence: 383 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/html; charset=windows-1252 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; 0 X-Spam-TU-Processing-Host: neelix.kom.tuwien.ac.at X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

This message is in part a test – I have no idea how many people still subscribe to the globillum mailing list, so it will be interesting to see how many responses I get.

 

This is also a chance for the global illumination community to contribute its collective expertise to a real-world problem.

 

The Illuminating Engineering Society of North America publishes RP-22, Tunnel Lighting. This is an ANSI / IESNA publication with the description:

 

“This standard practice has the goal of providing information that will assist in determining lighting needs, provide solutions, and evaluate resulting visibility within vehicular roadway tunnels. Pedestrian and other non-vehicular tunnels are not addressed. This practice is intended for use by engineers, consultants, technicians, and administrators charged with the responsibility of providing a safe environment within a tunnel - day and night.”

 

An important component of this publication concerns BRDFs for tunnel materials (and more generally for roadway surfaces). The IESNA Roadway Lighting Committee (RLC) is currently working on the next edition, and wants to incorporate BRDFs, either as published material data or (more likely) as recommended procedures for measuring and manipulating the data.

 

LTI Optics (www.ltioptics.com) has the hardware and expertise to perform BRDF measurements, but the IESNA Roadway Lighting Committee is wondering what measurement angles are needed and how coarse the angular increments can be.

 

Most of the materials to be tested are tiles with glossy coatings and concrete materials.

 

The viewing angles are limited to the standard observer (standard height moving across lanes, but multiple reflection angles to other surfaces may need to be considered.

 

For calculation purposes, one of the goals is to predict disability glare from the surfaces for the standard observer, using for example Radiance.

 

I realize that this is an open-ended set of questions that will likely require more information. However, at this point, I am more interested in seeing whether there are enough people from the old globillum gang available to conduct a mailing list discussion. I could probably research and answer these questions myself for the Roadway Lighting Committee, but I would much prefer to rely on the collective wisdom of the global illumination community.

 

The podium is open …

 

Ian Ashdown, P. Eng., LC, FIES

President

byHeart Consultants Limited

http://www.helios32.com

------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-path: Envelope-to: wp@cg.tuwien.ac.at Delivery-date: Fri, 16 Jan 2009 11:17:55 +0100 Received: from neelix.kom.tuwien.ac.at ([192.35.241.67]:39358) by christl.cg.tuwien.ac.at with esmtp (Exim 4.63) (envelope-from ) id 1LNllz-0007mX-Kl; Fri, 16 Jan 2009 11:17:55 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by neelix.kom.tuwien.ac.at (8.14.1/8.14.1) with ESMTP id n0GAHe0H026003; Fri, 16 Jan 2009 11:17:40 +0100 X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id n0GAHepV031777; Fri, 16 Jan 2009 11:17:40 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id n0GAHcHZ031772; Fri, 16 Jan 2009 11:17:38 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id n0GAH2k3030766 for ; Fri, 16 Jan 2009 11:17:02 +0100 Received: from rodin.limsi.fr (rodin.limsi.fr [129.175.152.156]) by imag.imag.fr (8.13.8/8.13.8) with ESMTP id n0GAApfD020604 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=OK) for ; Fri, 16 Jan 2009 11:10:52 +0100 (CET) Received: from [129.175.152.81] (kingdom-of-heaven.limsi.fr [129.175.152.81]) by rodin.limsi.fr (8.13.4/8.13.4/Debian-3sarge3) with ESMTP id n0GA9JSE021024 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NOT); Fri, 16 Jan 2009 11:09:19 +0100 Message-ID: <49705CD4.4070906@inria.fr> Date: Fri, 16 Jan 2009 11:09:24 +0100 From: Samuel Boivin User-Agent: Thunderbird 2.0.0.19 (Windows/20081209) MIME-Version: 1.0 To: Ian Ashdown CC: globillum@imag.fr Subject: Re: BRDF data for tunnel materials? References: <41CFC639DB7748E4A45DDD9DCA9A7798@Ian> In-Reply-To: <41CFC639DB7748E4A45DDD9DCA9A7798@Ian> X-LIMSI-rodin-MailScanner: Found to be clean X-LIMSI-rodin-MailScanner-SpamCheck: not spam (whitelisted), SpamAssassin (score=0, requis 5) X-MailScanner-Auteur: samuel.boivin@inria.fr X-MailScanner-Dest: globillum@imag.fr, ian_ashdown@helios32.com X-Greylist: Sender passed SPF test, not delayed by milter-greylist-4.1.1 (neelix.kom.tuwien.ac.at [192.35.241.67]); Fri, 16 Jan 2009 11:17:55 +0100 (CET) X-Greylist: Sender succeeded STARTTLS authentication, not delayed by milter-greylist-3.0 (imag.imag.fr [129.88.30.1]); Fri, 16 Jan 2009 11:10:52 +0100 (CET) X-IMAG-MailScanner-Information: Please contact MI2S MIM for more information X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-From: samuel.boivin@inria.fr X-Loop: globillum@imag.fr X-Sequence: 384 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-Virus-Scanned: by amavisd-new X-Spam-Status: LOW ; 0 X-Spam-TU-Processing-Host: neelix.kom.tuwien.ac.at X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hello Ian, As you already said it, this kind of problems opens a wide range a sub-problems. > (...) > > LTI Optics (www.ltioptics.com ) has the > hardware and expertise to perform BRDF measurements, but the IESNA > Roadway Lighting Committee is wondering what measurement angles are > needed and how coarse the angular increments can be. > > > > Most of the materials to be tested are tiles with glossy coatings and > concrete materials. > From my experience, it is always hard to have an opinion about a material's BRDF without having a look at a real sample of this material first. However, considering what you're describing here, I doubt that you really need a lot of measurement angles to get a good approximation of the BRDF. For regular tiles, the roughness parameters are in general pretty "small" and more important the material's roughness itself has an almost uniform distribution all around the surface (i.e. if you look closer at the surface you won't huge valleys). But, reading again your email and since "ltioptics has the hardware and expertise to perform BRDF measurements", I don't get why they just don't do the job themselves by trying several sets of measurements and thus getting the corresponding error ? Other questions are: are all the tiles made of the same material ? Are they highly specular (is it "glossy" more like an orange or more like a metal ?) ? > > The viewing angles are limited to the standard observer (standard > height moving across lanes, but multiple reflection angles to other > surfaces may need to be considered. > > For calculation purposes, one of the goals is to predict disability > glare from the surfaces for the standard observer, using for example > Radiance. > I'm not sure to understand what you exaclty want to simulate here. Is the goal for example to observe undesirable visual effects due to the tiles' BRDF and/or to determine what kind of lighting to use ? If so and if these materials are highly specular, I think that simulating a complete real scene could be useful, just because multiple specular reflections always produce surprising and unexpected effects. The problem of using a measurement device on a complete scene is the required time that the people would need for getting all object BRDFs... . Personally, for simulating real world, detecting multiple reflection issues (for example) and getting an accurate evaluation of the error introduced by the chosen BRDF or the numbers of measurements samples, I would go with something like inverse/image-based rendering methods and comparing real materials with materials rendered using Radiance and the appropriate BRDF. A mixed method with the ltioptics measurement system would also probably make sense and increase accuracy. I'm actually not sure that my comments really help here, I'm just giving you some of my experience about measuring data (including BRDFs) from real world. All the best, Sam. ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-path: Envelope-to: wp@cg.tuwien.ac.at Delivery-date: Fri, 16 Jan 2009 15:55:25 +0100 Received: from tuvok.kom.tuwien.ac.at ([192.35.241.66]:42824) by christl.cg.tuwien.ac.at with esmtp (Exim 4.63) (envelope-from ) id 1LNq6X-0003xZ-7F; Fri, 16 Jan 2009 15:55:25 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.14.1/8.14.1) with ESMTP id n0GEtE85014403; Fri, 16 Jan 2009 15:55:14 +0100 X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id n0GEtEnI013438; Fri, 16 Jan 2009 15:55:14 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id n0GEtDn1013433; Fri, 16 Jan 2009 15:55:13 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id n0GEsMPo011479 for ; Fri, 16 Jan 2009 15:54:22 +0100 Received: from server.agi32.com (unknown.ord.scnet.net [66.225.254.249] (may be forged)) by imag.imag.fr (8.13.8/8.13.8) with ESMTP id n0GEoLUe005255 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO) for ; Fri, 16 Jan 2009 15:50:25 +0100 (CET) Received: from s01060006257abbc2.vn.shawcable.net ([24.87.90.99] helo=Ian) by server.agi32.com with esmtpa (Exim 4.69) (envelope-from ) id 1LNq1Z-0000fK-19 for globillum@imag.fr; Fri, 16 Jan 2009 07:50:17 -0700 From: "Ian Ashdown" To: globillum@imag.fr Subject: FW: BRDF data for tunnel materials? Date: Fri, 16 Jan 2009 06:49:48 -0800 Organization: byHeart Consultants Limited Message-ID: <598DFD413BAF4BA2ABDA51D8CA7370F9@Ian> MIME-Version: 1.0 X-Mailer: Microsoft Office Outlook 11 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2900.5579 Thread-Index: Acl3pchEOZK31IWYQnWqOFUMM4JfnAAQIGiw X-AntiAbuse: This header was added to track abuse, please include it with any abuse report X-AntiAbuse: Primary Hostname - server.agi32.com X-AntiAbuse: Original Domain - imag.fr X-AntiAbuse: Originator/Caller UID/GID - [47 12] / [47 12] X-AntiAbuse: Sender Address Domain - helios32.com X-Greylist: Sender passed SPF test, not delayed by milter-greylist-4.1.1 (tuvok.kom.tuwien.ac.at [192.35.241.66]); Fri, 16 Jan 2009 15:55:25 +0100 (CET) X-Greylist: IP, sender and recipient auto-whitelisted, not delayed by milter-greylist-3.0 (imag.imag.fr [129.88.30.1]); Fri, 16 Jan 2009 15:50:25 +0100 (CET) X-IMAG-MailScanner-Information: Please contact MI2S MIM for more information X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-From: ian_ashdown@helios32.com X-Loop: globillum@imag.fr X-Sequence: 385 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-Virus-Scanned: by amavisd-new X-Spam-Status: LOW ; 0 X-Spam-TU-Processing-Host: tuvok.kom.tuwien.ac.at X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Quoting from Henrik Wann Jensen reply below: > we were all interested in finding a standard for representing > BRDFs (perhaps you are already aware of one?) > The only BRDF standard that I am aware of is ASTM E1392-96 (see http://www.graphics.cornell.edu/online/measurements/reflectance/index.html). On the downside, the only use of this standard that I am aware of is the above Cornell study from 2001. > Btw. I am currently involved in performing a verification of a >lighting program according to the CIE report that you made a few > years ago. It seems that the cases 5.7 and 5.14 have some errors? > Are you aware of these issues? > Yes indeed. These issues are documented in: CIE 171:2006, "Test Cases to Assess the Accuracy of Lighting Computer Programs: Results for AGi32 V1.94. which can be downloaded from http://agi32.com/Extra/TechnicalDocs/technicalDocuments.htm. The appendix has a full and rigorous analysis of cases 5.7 and 5.8, as well as analytic solutions. There is also a tabular error in case 5.13, but I am not aware of any problems with 5.14. > Are you aware of these issues? And are you involved in making > any updated testcases? > I have reported these errors to the CIE executive, but unfortunately the technical committee chair is no longer involved with the CIE, and there has been no response from the CIE executive to address the errors with an addendum. I had plans to summarize the above report in a paper for the IESNA Leukos publication, but that project has been on hold for over a year. In lieu of this, the aforementioned report is the only source of information that I am aware of. > It seems the ones in the report are tuned towards finite element > radiosity having only flat diffuse surfaces. > This is correct. There were some general comments in Section 6 regarding non-diffuse surfaces, but like every paper with a "future work" section, nothing has or likely ever will be done to address these issues, at least within the context of CIE 171. - Ian -----Original Message----- From: Henrik Wann Jensen [mailto:henrik@cs.ucsd.edu] Sent: January 15, 2009 10:44 PM To: Ian Ashdown Subject: Re: BRDF data for tunnel materials? Hi Ian, I am interested in hearing more about this. We have a new gantry at UC San Diego, which we use for BRDF measurements. I also had a long discussion at SIGGRAPH Asia with a group of people including Don Greenberg, and we were all interested in finding a standard for representing BRDFs (perhaps you are already aware of one?) Btw. I am currently involved in performing a verification of a lighting program according to the CIE report that you made a few years ago. It seems that the cases 5.7 and 5.14 have some errors? Are you aware of these issues? And are you involved in making any updated testcases? It seems the ones in the report are tuned towards finite element radiosity having only flat diffuse surfaces. Cheers, Henrik On Thu, 15 Jan 2009, Ian Ashdown wrote: > This message is in part a test - I have no idea how many people still > subscribe to the globillum mailing list, so it will be interesting to see > how many responses I get. > > > > This is also a chance for the global illumination community to contribute > its collective expertise to a real-world problem. > > > > The Illuminating Engineering Society of North America publishes RP-22, > Tunnel Lighting. This is an ANSI / IESNA publication with the description: > > > > "This standard practice has the goal of providing information that will > assist in determining lighting needs, provide solutions, and evaluate > resulting visibility within vehicular roadway tunnels. Pedestrian and other > non-vehicular tunnels are not addressed. This practice is intended for use > by engineers, consultants, technicians, and administrators charged with the > responsibility of providing a safe environment within a tunnel - day and > night." > > > > An important component of this publication concerns BRDFs for tunnel > materials (and more generally for roadway surfaces). The IESNA Roadway > Lighting Committee (RLC) is currently working on the next edition, and wants > to incorporate BRDFs, either as published material data or (more likely) as > recommended procedures for measuring and manipulating the data. > > > > LTI Optics (www.ltioptics.com ) has the hardware > and expertise to perform BRDF measurements, but the IESNA Roadway Lighting > Committee is wondering what measurement angles are needed and how coarse the > angular increments can be. > > > > Most of the materials to be tested are tiles with glossy coatings and > concrete materials. > > > > The viewing angles are limited to the standard observer (standard height > moving across lanes, but multiple reflection angles to other surfaces may > need to be considered. > > > > For calculation purposes, one of the goals is to predict disability glare > from the surfaces for the standard observer, using for example Radiance. > > > > I realize that this is an open-ended set of questions that will likely > require more information. However, at this point, I am more interested in > seeing whether there are enough people from the old globillum gang available > to conduct a mailing list discussion. I could probably research and answer > these questions myself for the Roadway Lighting Committee, but I would much > prefer to rely on the collective wisdom of the global illumination > community. > > > > The podium is open . > > > > Ian Ashdown, P. Eng., LC, FIES > > President > > byHeart Consultants Limited > > http://www.helios32.com > > ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-path: Envelope-to: wp@cg.tuwien.ac.at Delivery-date: Sat, 17 Jan 2009 19:40:10 +0100 Received: from tuvok.kom.tuwien.ac.at ([192.35.241.66]:54443) by christl.cg.tuwien.ac.at with esmtp (Exim 4.63) (envelope-from ) id 1LOG5a-0008Ln-GY; Sat, 17 Jan 2009 19:40:10 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.14.1/8.14.1) with ESMTP id n0HIdwPh022606; Sat, 17 Jan 2009 19:39:59 +0100 X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id n0HIdwko031565; Sat, 17 Jan 2009 19:39:58 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id n0HIdwQ6031560; Sat, 17 Jan 2009 19:39:58 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id n0HIdD3u030563 for ; Sat, 17 Jan 2009 19:39:13 +0100 Received: from server.agi32.com (unknown.ord.scnet.net [66.225.254.249] (may be forged)) by imag.imag.fr (8.13.8/8.13.8) with ESMTP id n0HIaPje021332 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO) for ; Sat, 17 Jan 2009 19:36:28 +0100 (CET) Received: from s01060006257abbc2.vn.shawcable.net ([24.87.90.99] helo=Ian) by server.agi32.com with esmtpa (Exim 4.69) (envelope-from ) id 1LOG1v-0004kV-LM; Sat, 17 Jan 2009 11:36:23 -0700 From: "Ian Ashdown" To: "'Samuel Boivin'" Cc: globillum@imag.fr References: <41CFC639DB7748E4A45DDD9DCA9A7798@Ian> <49705CD4.4070906@inria.fr> Subject: RE: BRDF data for tunnel materials? Date: Sat, 17 Jan 2009 10:35:52 -0800 Organization: byHeart Consultants Limited Message-ID: <6636001A84924C0B848A886EDBF2BD95@Ian> MIME-Version: 1.0 X-Mailer: Microsoft Office Outlook 11 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2900.5579 Thread-Index: Acl3w6eK7S6taCWYThqlBSgOtPjxzABCAhjA In-Reply-To: <49705CD4.4070906@inria.fr> X-AntiAbuse: This header was added to track abuse, please include it with any abuse report X-AntiAbuse: Primary Hostname - server.agi32.com X-AntiAbuse: Original Domain - imag.fr X-AntiAbuse: Originator/Caller UID/GID - [47 12] / [47 12] X-AntiAbuse: Sender Address Domain - helios32.com X-Greylist: Sender passed SPF test, not delayed by milter-greylist-4.1.1 (tuvok.kom.tuwien.ac.at [192.35.241.66]); Sat, 17 Jan 2009 19:40:10 +0100 (CET) X-Greylist: IP, sender and recipient auto-whitelisted, not delayed by milter-greylist-3.0 (imag.imag.fr [129.88.30.1]); Sat, 17 Jan 2009 19:36:28 +0100 (CET) X-IMAG-MailScanner-Information: Please contact MI2S MIM for more information X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-From: ian_ashdown@helios32.com X-Loop: globillum@imag.fr X-Sequence: 386 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-Virus-Scanned: by amavisd-new X-Spam-Status: LOW ; 6 X-Spam-Level: ++++++ X-Spam-TU-Processing-Host: tuvok.kom.tuwien.ac.at X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit > But, reading again your email and since "ltioptics has the > hardware and expertise to perform BRDF measurements", I don't > get why they just don't do the job themselves by trying several > sets of measurements and thus getting the corresponding error ? > My understanding is that LTI Optics has offered to do the work, but the details have not yet been worked out as to what is to be measured. > Other questions are: are all the tiles made of the same > material ? Are they highly specular (is it "glossy" more like > an orange or more like a metal ?) ? > I do not have much experience with tunnel lighting, but from what I have seen, most tunnel walls and ceilings are either concrete or lined with white ceramic tiles to improve the diffuse reflectance and provide a washable surface. For "glossy" then, think of ceramic floor tiles. Photographs of a typical tiled tunnel installation are available here: http://www.tirsys.com/data/content/files/file/pdf/resources/brochures/BCP-42 0-001%20Tunnel%20Lighting%20Guide%20Document.pdf > I'm not sure to understand what you exaclty want to simulate > here. Is the goal for example to observe undesirable visual > effects due to the tiles' BRDF and/or to determine what kind of > lighting to use ? > The state of the art in roadway and tunnel lighting calculations is nicely explained in this document: http://www.iar.unicamp.br/lab/luz/ld/Arquitetural/Ilumina%E7%E3o%20P%FAblica /Rodovias/ROADWAY%20LIGHTING%20DESIGN%20METHODOLOGY%20AND%20EVALUATION.pdf where Section 6 describes the CIE r-tables (BRDF measurements) and subsequent roadway material classification. The CIE measurements were obtained in 1967. At present, tunnel lighting is calculated using programs such as Lighting Analysts' AGi32 (www.agi32.com), which is based on radiosity methods and so limited to ideal diffuse reflections. If the IESNA provides BRDF measurements for common tunnel materials however, these programs can be modified to calculate glossy reflections for estimating disability glare. It is also possible of course to generate real-time walkthroughs and ray-traced renderings with glossy reflections, but this is eye candy for roadway lighting design. (Even for architectural lighting design, it is estimated that fewer than one percent of professional lighting designers bother to create ray-traced images for their clients.) > Personally, for simulating real world, detecting multiple reflection > issues (for example) and getting an accurate evaluation of the error > introduced by the chosen BRDF or the numbers of measurements samples, > I would go with something like inverse/image-based rendering methods > and comparing real materials with materials rendered using Radiance > and the appropriate BRDF. > I agree that this is the preferred approach for photorealistic renderings. However, for the purposes of tunnel lighting calculations and in consideration of the low gloss of most ceramic tiles, I think a first bounce approximation will be sufficient. - Ian -----Original Message----- From: Samuel Boivin [mailto:Samuel.Boivin@inria.fr] Sent: January 16, 2009 2:09 AM To: Ian Ashdown Cc: globillum@imag.fr Subject: Re: BRDF data for tunnel materials? Hello Ian, As you already said it, this kind of problems opens a wide range a sub-problems. > (...) > > LTI Optics (www.ltioptics.com ) has the > hardware and expertise to perform BRDF measurements, but the IESNA > Roadway Lighting Committee is wondering what measurement angles are > needed and how coarse the angular increments can be. > > > > Most of the materials to be tested are tiles with glossy coatings and > concrete materials. > From my experience, it is always hard to have an opinion about a material's BRDF without having a look at a real sample of this material first. However, considering what you're describing here, I doubt that you really need a lot of measurement angles to get a good approximation of the BRDF. For regular tiles, the roughness parameters are in general pretty "small" and more important the material's roughness itself has an almost uniform distribution all around the surface (i.e. if you look closer at the surface you won't huge valleys). But, reading again your email and since "ltioptics has the hardware and expertise to perform BRDF measurements", I don't get why they just don't do the job themselves by trying several sets of measurements and thus getting the corresponding error ? Other questions are: are all the tiles made of the same material ? Are they highly specular (is it "glossy" more like an orange or more like a metal ?) ? > > The viewing angles are limited to the standard observer (standard > height moving across lanes, but multiple reflection angles to other > surfaces may need to be considered. > > For calculation purposes, one of the goals is to predict disability > glare from the surfaces for the standard observer, using for example > Radiance. > I'm not sure to understand what you exaclty want to simulate here. Is the goal for example to observe undesirable visual effects due to the tiles' BRDF and/or to determine what kind of lighting to use ? If so and if these materials are highly specular, I think that simulating a complete real scene could be useful, just because multiple specular reflections always produce surprising and unexpected effects. The problem of using a measurement device on a complete scene is the required time that the people would need for getting all object BRDFs... . Personally, for simulating real world, detecting multiple reflection issues (for example) and getting an accurate evaluation of the error introduced by the chosen BRDF or the numbers of measurements samples, I would go with something like inverse/image-based rendering methods and comparing real materials with materials rendered using Radiance and the appropriate BRDF. A mixed method with the ltioptics measurement system would also probably make sense and increase accuracy. I'm actually not sure that my comments really help here, I'm just giving you some of my experience about measuring data (including BRDFs) from real world. All the best, Sam. ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-path: Envelope-to: wp@cg.tuwien.ac.at Delivery-date: Sat, 17 Jan 2009 19:48:06 +0100 Received: from tuvok.kom.tuwien.ac.at ([192.35.241.66]:33806) by christl.cg.tuwien.ac.at with esmtp (Exim 4.63) (envelope-from ) id 1LOGDG-0008Pt-0G; Sat, 17 Jan 2009 19:48:06 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by tuvok.kom.tuwien.ac.at (8.14.1/8.14.1) with ESMTP id n0HIlttG031019; Sat, 17 Jan 2009 19:47:55 +0100 X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id n0HIlswA002314; Sat, 17 Jan 2009 19:47:54 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id n0HIlswv002309; Sat, 17 Jan 2009 19:47:54 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id n0HIlHbR032757 for ; Sat, 17 Jan 2009 19:47:17 +0100 Received: from server.agi32.com (unknown.ord.scnet.net [66.225.254.249] (may be forged)) by imag.imag.fr (8.13.8/8.13.8) with ESMTP id n0HIhwnj022241 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO) for ; Sat, 17 Jan 2009 19:44:00 +0100 (CET) Received: from s01060006257abbc2.vn.shawcable.net ([24.87.90.99] helo=Ian) by server.agi32.com with esmtpa (Exim 4.69) (envelope-from ) id 1LOG9F-0003tq-1S; Sat, 17 Jan 2009 11:43:57 -0700 From: "Ian Ashdown" To: "'Steve Marschner'" Cc: globillum@imag.fr References: <41CFC639DB7748E4A45DDD9DCA9A7798@Ian> <80066FA7-0246-4395-A03B-7C2C1048E2F2@cs.cornell.edu> Subject: RE: BRDF data for tunnel materials? 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Thank you for your comments, Steve.

 

I agree that the entire BRDFs should be measured, rather than be limited to a narrow range of viewing angles. While the IESNA Roadway Lighting Committee is likely thinking of BRDFs in the context of disability glare from reflections, the commercial lighting design programs (such as AGi32) used for tunnel lighting design and analysis should really be extended to support first-bounce glossy reflections. (Being the software developer of AGi32’s calculation and visualization engines, I get to stare at myself in the mirror when I say this ;+)

 

To answer your question regarding the tiles, a picture is worth a thousand words: http://www.tirsys.com/data/content/files/file/pdf/resources/brochures/BCP-420-001%20Tunnel%20Lighting%20Guide%20Document.pdf.

 

- Ian

 

From: Steve Marschner [mailto:srm@cs.cornell.edu]
Sent: January 16, 2009 7:09 AM
To: Ian Ashdown
Subject: Re: BRDF data for tunnel materials?

 

Hi Ian,

 

I'm on this list, and interested in this problem.

 

My quick reaction is that one should really measure entire BRDFs rather than just particular viewing angles, since inevitably they'll want to consider multiple reflections, at which point the required angles will depend entirely on the particular geometry.

 

I think fairly coarse sampling would be sufficient, with appropriate separation of the specular component from the glossy tiles.  Is the material for the tiles really the aggregate reflection from a wall covered with tiles (including typical tolerances on flatness, etc.) rather than the BRDF of an individual tile?

 

Steve

 

On Jan 16, 2009, at 12:05 AM, Ian Ashdown wrote:



This message is in part a test – I have no idea how many people still subscribe to the globillum mailing list, so it will be interesting to see how many responses I get.

 

This is also a chance for the global illumination community to contribute its collective expertise to a real-world problem.

 

The Illuminating Engineering Society of North America publishes RP-22, Tunnel Lighting. This is an ANSI / IESNA publication with the description:

 

“This standard practice has the goal of providing information that will assist in determining lighting needs, provide solutions, and evaluate resulting visibility within vehicular roadway tunnels. Pedestrian and other non-vehicular tunnels are not addressed. This practice is intended for use by engineers, consultants, technicians, and administrators charged with the responsibility of providing a safe environment within a tunnel - day and night.”

 

An important component of this publication concerns BRDFs for tunnel materials (and more generally for roadway surfaces). The IESNA Roadway Lighting Committee (RLC) is currently working on the next edition, and wants to incorporate BRDFs, either as published material data or (more likely) as recommended procedures for measuring and manipulating the data.

 

LTI Optics (www.ltioptics.com) has the hardware and expertise to perform BRDF measurements, but the IESNA Roadway Lighting Committee is wondering what measurement angles are needed and how coarse the angular increments can be.

 

Most of the materials to be tested are tiles with glossy coatings and concrete materials.

 

The viewing angles are limited to the standard observer (standard height moving across lanes, but multiple reflection angles to other surfaces may need to be considered.

 

For calculation purposes, one of the goals is to predict disability glare from the surfaces for the standard observer, using for example Radiance.

 

I realize that this is an open-ended set of questions that will likely require more information. However, at this point, I am more interested in seeing whether there are enough people from the old globillum gang available to conduct a mailing list discussion. I could probably research and answer these questions myself for the Roadway Lighting Committee, but I would much prefer to rely on the collective wisdom of the global illumination community.

 

The podium is open …

 

Ian Ashdown, P. Eng., LC, FIES

President

byHeart Consultants Limited

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------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-path: Envelope-to: wp@cg.tuwien.ac.at Delivery-date: Sat, 17 Jan 2009 20:14:41 +0100 Received: from neelix.kom.tuwien.ac.at ([192.35.241.67]:51495) by christl.cg.tuwien.ac.at with esmtp (Exim 4.63) (envelope-from ) id 1LOGcz-0000A1-BE; Sat, 17 Jan 2009 20:14:41 +0100 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by neelix.kom.tuwien.ac.at (8.14.1/8.14.1) with ESMTP id n0HJEBPJ032370; Sat, 17 Jan 2009 20:14:11 +0100 X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id n0HJEBot011558; Sat, 17 Jan 2009 20:14:11 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id n0HJEBGQ011553; Sat, 17 Jan 2009 20:14:11 +0100 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id n0HJDXaj009605 for ; Sat, 17 Jan 2009 20:13:33 +0100 Received: from server.agi32.com (unknown.ord.scnet.net [66.225.254.249] (may be forged)) by imag.imag.fr (8.13.8/8.13.8) with ESMTP id n0HJ9MwK025154 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO) for ; Sat, 17 Jan 2009 20:09:24 +0100 (CET) Received: from s01060006257abbc2.vn.shawcable.net ([24.87.90.99] helo=Ian) by server.agi32.com with esmtpa (Exim 4.69) (envelope-from ) id 1LOGXo-0006NB-SW; Sat, 17 Jan 2009 12:09:21 -0700 From: "Ian Ashdown" To: "'Leora Radetsky'" Cc: globillum@imag.fr References: <2342C75498954107A98E1B5A2A690955@Ian> <74b5f8fa0901160923s4561658ch282bf659323900b5@mail.gmail.com> Subject: RE: FW: BRDF data for tunnel materials? Date: Sat, 17 Jan 2009 11:08:50 -0800 Organization: byHeart Consultants Limited Message-ID: MIME-Version: 1.0 X-Mailer: Microsoft Office Outlook 11 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2900.5579 Thread-Index: Acl3/yzfq66cfPfXTfK5EVAOSbzmcAA1lChw In-Reply-To: <74b5f8fa0901160923s4561658ch282bf659323900b5@mail.gmail.com> X-AntiAbuse: This header was added to track abuse, please include it with any abuse report X-AntiAbuse: Primary Hostname - server.agi32.com X-AntiAbuse: Original Domain - imag.fr X-AntiAbuse: Originator/Caller UID/GID - [47 12] / [47 12] X-AntiAbuse: Sender Address Domain - helios32.com X-Greylist: Sender passed SPF test, not delayed by milter-greylist-4.1.1 (neelix.kom.tuwien.ac.at [192.35.241.67]); Sat, 17 Jan 2009 20:14:41 +0100 (CET) X-Greylist: IP, sender and recipient auto-whitelisted, not delayed by milter-greylist-3.0 (imag.imag.fr [129.88.30.1]); Sat, 17 Jan 2009 20:09:25 +0100 (CET) X-IMAG-MailScanner-Information: Please contact MI2S MIM for more information X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-From: ian_ashdown@helios32.com X-Loop: globillum@imag.fr X-Sequence: 388 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/html; charset=windows-1252 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Spam-Status: LOW ; 0 X-Spam-TU-Processing-Host: neelix.kom.tuwien.ac.at X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

Sam got it right – do the measurements and then determine what is the best angular resolution within a given error limit. Ignore the R-tables, as they may be revised at some point in the future (especially for wet concrete and asphalt).

 

Also, be sure to archive the original BRDF measurements and make them available through a Web site or on DVD-ROM. The revised RP-22 or RP-8 may publish lower resolution data in print for illustration purposes, but lighting design programs should be encouraged to use the actual data. (They can always downscale the resolution internally if required.)

 

Another reason for doing this is that the specular component becomes significant at acute viewing angles – see the TIR brochure photos of the reflected car headlights for a good example. For AGi32, I would likely separate the raw BRDF data into a diffuse component and a separate semispecular component for calculation purposes. However, this sort of implementation detail should be left up to the software developer; the role of the IESNA is to provide the raw data.

 

- Ian

 

From: Leora Radetsky [mailto:r.leora@gmail.com]
Sent: January 16, 2009 9:24 AM
To: Ian Ashdown
Subject: Re: FW: BRDF data for tunnel materials?

 

cool. Just wanted to mention another complication (perhaps its just a limiting factor) - one I am sure you thought of already. Should the coarseness of the tile BRDF be related to the coarseness of R-tables? I do not expect our current pavement standards to change because of economics (no one is going to spend the money necessary to update and reclassify our existing r-tables). So - if we have very coarse pavement data, how meaningful will having more "dense" wall data be. Yes it will be more meaningful for its own sake (disability and possibly discomfort glare from the wall, specular reflections visible etc) but when it bounces from the wall to the pavement much of that detail is lost in terms of re reflection from the pavement. Do we only need to be "as good" as the r-table or should we be better?

 

I think we should be better, but will it matter?

 

Lee

-----Original Message-----
From: Samuel Boivin [mailto:Samuel.Boivin@inria.fr]
Sent: January 16, 2009 2:09 AM
To: Ian Ashdown
Cc: globillum@imag.fr
Subject: Re: BRDF data for tunnel materials?

Hello Ian,

As you already said it, this kind of problems opens a wide range a
sub-problems.
> (...)

>
> LTI Optics (www.ltioptics.com <http://www.ltioptics.com/>) has the
> hardware and expertise to perform BRDF measurements, but the IESNA
> Roadway Lighting Committee is wondering what measurement angles are
> needed and how coarse the angular increments can be.
>
>
>
> Most of the materials to be tested are tiles with glossy coatings and
> concrete materials.
>

 From my experience, it is always hard to have an opinion about a
material's BRDF without having a look at a real sample of this material
first.
However, considering what you're describing here, I doubt that you
really need a lot of measurement angles to get a good approximation of
the BRDF. For regular tiles, the roughness parameters are in general
pretty "small" and more important the material's roughness itself has an
almost uniform distribution all around the surface (i.e. if you look
closer at the surface you won't huge valleys).
But, reading again your email and since "ltioptics has the hardware and
expertise to perform BRDF measurements", I don't get why they just don't
do the job themselves by trying several sets of measurements and thus
getting the corresponding error ?
Other questions are: are all the tiles made of the same material ? Are
they highly specular (is it "glossy" more like an orange or more like a
metal ?) ?

>
> The viewing angles are limited to the standard observer (standard
> height moving across lanes, but multiple reflection angles to other
> surfaces may need to be considered.
>
> For calculation purposes, one of the goals is to predict disability
> glare from the surfaces for the standard observer, using for example
> Radiance.
>

I'm not sure to understand what you exaclty want to simulate here. Is
the goal for example to observe undesirable visual effects due to the
tiles' BRDF and/or to determine what kind of lighting to use ?
If so and if these materials are highly specular, I think that
simulating a complete real scene could be useful, just because multiple
specular reflections always produce surprising and unexpected effects.
The problem of using a measurement device on a complete scene is the
required time that the people would need for getting all object BRDFs...
. Personally, for simulating real world, detecting multiple reflection
issues (for example) and getting an accurate evaluation of the error
introduced by the chosen BRDF or the numbers of measurements samples, I
would go with something like inverse/image-based rendering methods and
comparing real materials with materials rendered using Radiance and the
appropriate BRDF. A mixed method with the ltioptics measurement system
would also probably make sense and increase accuracy.

I'm actually not sure that my comments really help here, I'm just giving
you some of my experience about measuring data (including BRDFs) from
real world.

All the best,

Sam.

 

------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-path: Envelope-to: wp@cg.tuwien.ac.at Delivery-date: Tue, 05 May 2009 11:48:56 +0200 Received: from neelix.kom.tuwien.ac.at ([192.35.241.67]:48119) by christl.cg.tuwien.ac.at with esmtp (Exim 4.63) (envelope-from ) id 1M1HGi-0000rm-BN; Tue, 05 May 2009 11:48:56 +0200 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by neelix.kom.tuwien.ac.at (8.14.1/8.14.1) with ESMTP id n459mnqP023128; Tue, 5 May 2009 11:48:49 +0200 X-Connecting-Host: chopinette.imag.fr [129.88.34.204] X-Connecting-Addr: 129.88.34.204 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id n459mmYk024736; Tue, 5 May 2009 11:48:48 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id n459mmdc024731; Tue, 5 May 2009 11:48:48 +0200 Received: from harmonie.imag.fr (harmonie.imag.fr [147.171.130.40]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id n459loCp022849 for ; Tue, 5 May 2009 11:47:50 +0200 Received: from christl.cg.tuwien.ac.at (mail.cg.tuwien.ac.at [128.131.166.76]) by harmonie.imag.fr (8.13.8/8.13.8) with ESMTP id n459jOZG001467 for ; Tue, 5 May 2009 11:45:25 +0200 (CEST) Received: from beinhart-09.cg.tuwien.ac.at ([128.131.166.9]:49895) by christl.cg.tuwien.ac.at with esmtpsa (TLS-1.0:DHE_RSA_AES_256_CBC_SHA1:32) (Exim 4.63) (envelope-from ) id 1M1Gdm-0000Cn-Lz; Tue, 05 May 2009 11:08:42 +0200 X-Mailer: QUALCOMM Windows Eudora Version 7.1.0.9 Date: Tue, 05 May 2009 09:58:30 +0200 To: globillum@imag.fr From: Werner Purgathofer Subject: CFP: International Journal of Creative Interfaces & Computer Graphics -- NEW in 2010! Mime-Version: 1.0 Message-Id: X-Greylist: Sender passed SPF test, not delayed by milter-greylist-4.1.1 (neelix.kom.tuwien.ac.at [192.35.241.67]); Tue, 05 May 2009 11:48:50 +0200 (CEST) X-Greylist: Delayed for 00:36:37 by milter-greylist-3.0 (harmonie.imag.fr [147.171.130.40]); Tue, 05 May 2009 11:45:25 +0200 (CEST) X-IMAG-MailScanner-Information: Please contact MI2S MIM for more information X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-From: wp@cg.tuwien.ac.at X-Loop: globillum@imag.fr X-Sequence: 389 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-Spam-Status: LOW ; -2 X-Spam-Level: - X-Spam-TU-Processing-Host: neelix.kom.tuwien.ac.at X-Virus-Scanned: by amavisd-new X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Dear Colleagues, I was asked to forward this information to the globillum mailing list. Best regards, Werner Purgathofer International Journal of Creative Interfaces & Computer Graphics ** New in 2010 ** http://www.igi-global.com/IJCICG An Official Publication of the Information Resources Management Association Editor-in-Chief: Ben Falchuk, Telcordia Technologies Inc., USA Published: Semi-Annually Call for Papers: The Editor-in-Chief of the International Journal of Creative Interfaces and Computer Graphics (IJCICG) would like to invite you to consider submitting a manuscript for inclusion in this scholarly journal. The following describes the mission, coverage, and guidelines for submission to IJCICG. Mission The primary objective of International Journal of Creative Interfaces and Computer Graphics (IJCICG) is to bring together research, pragmatic work, and results revolving around the most innovative, fascinating, and technically advanced computer graphic applications and their human- computer interfaces. This journal's key themes include design rationale and approach, software underpinnings, deployment, and interaction, with an emphasis on creative, cutting-edge, aesthetic, and innovative uses of graphics in applications and human-computer interfaces. Articles in this journal are presented in a systematic but accessible style and emphasize their impact, extraordinary nature, and their positioning in this exciting field. Targeting researchers, developers, designers, user-experience engineers, artists, and planners, IJCICG supplies readers with a better understanding of the design and deployment of novel graphical applications and technologies on the desktop, the Web, mobile devices, and public spaces. Coverage Topics to be discussed in this journal include (but are not limited to) the following: o Advances in interfaces to support creativity, productivity, and expression o Aesthetic computing, visual explanations, and data visualization o Bleeding-edge Web, RIA, and mobile interfaces o Cutting-edge interfaces and applications in practical creative fields such as engineering and design, digital art, entertainment, video gaming and computer animation, museums, performance, and other creative endeavors o Design of new styles of interaction-rich applications and services o Novel visual metaphors used for visualization or practical data mining o Societal impact and evaluation of graphical applications and interfaces o State of the art mobile applications with unique visual characteristics o Technologies and underpinnings that enable or support visually compelling interfaces o Trends in innovative and future interfaces o Use of visual elegance and simplicity Submission To view the full guidelines for submission: http://www.igi-global.com/development/author_info/guide.asp All submissions and inquiries should be directed to the attention of: Ben Falchuk, PhD Editor-in-Chief International Journal of Creative Interfaces and Computer Graphics E-mail: bfalchuk AT research.telcordia.com HTML version of this Call: http://www.igi-global.com/journals/details.asp?ID=34400&v=callForPapers -- Werner Purgathofer | Tel. +43(1)58801 18655 Technische Universitaet Wien | http://www.cg.tuwien.ac.at ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-path: Envelope-to: wp@cg.tuwien.ac.at Delivery-date: Mon, 10 Aug 2009 10:24:07 +0200 Received: from tuvok.kom.tuwien.ac.at ([192.35.241.66]:51968) by christl.cg.tuwien.ac.at with esmtp (Exim 4.63) (envelope-from ) id 1MaQAo-0001GV-90; Mon, 10 Aug 2009 10:24:06 +0200 Received: from shiva.imag.fr (mx1.imag.fr [129.88.30.5]) by tuvok.kom.tuwien.ac.at (8.14.1/8.14.1) with ESMTP id n79I3Eik015788; Sun, 9 Aug 2009 20:03:15 +0200 X-Connecting-Host: mx1.imag.fr [129.88.30.5] X-Connecting-Addr: 129.88.30.5 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by shiva.imag.fr (8.13.8/8.13.8) with ESMTP id n79I0qHr023945 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO); Sun, 9 Aug 2009 20:00:52 +0200 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id n79I3ATq030525; Sun, 9 Aug 2009 20:03:10 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id n79I356D030511; Sun, 9 Aug 2009 20:03:05 +0200 Received: from shiva.imag.fr (mx1.imag.fr [129.88.30.5]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id n79I2J74029500 for ; Sun, 9 Aug 2009 20:02:19 +0200 Received: from server.agi32.com (unknown.ord.scnet.net [66.225.254.249] (may be forged)) by shiva.imag.fr (8.13.8/8.13.8) with ESMTP id n79Hxs82023425 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO) for ; Sun, 9 Aug 2009 19:59:56 +0200 Received: from s01060006257abbc2.vn.shawcable.net ([24.87.90.99] helo=Ian) by server.agi32.com with esmtpa (Exim 4.69) (envelope-from ) id 1MaCG1-0001Fk-F2 for globillum@imag.fr; Sun, 09 Aug 2009 11:32:33 -0600 From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: 09/08/09 Release of RADBIB and GITHESIS Date: Sun, 9 Aug 2009 10:32:26 -0700 Organization: byHeart Consultants Limited Message-ID: MIME-Version: 1.0 X-Mailer: Microsoft Office Outlook 11 X-MIMEOLE: Produced By Microsoft MimeOLE V6.00.2900.5579 Thread-Index: AcoZF1x9EwCW1X2gQE63vBQkEXt95Q== X-AntiAbuse: This header was added to track abuse, please include it with any abuse report X-AntiAbuse: Primary Hostname - server.agi32.com X-AntiAbuse: Original Domain - imag.fr X-AntiAbuse: Originator/Caller UID/GID - [47 12] / [47 12] X-AntiAbuse: Sender Address Domain - helios32.com X-Greylist: Sender passed SPF test, not delayed by milter-greylist-4.1.1 (tuvok.kom.tuwien.ac.at [192.35.241.66]); Sun, 09 Aug 2009 20:03:15 +0200 (CEST) X-Greylist: Sender IP whitelisted, not delayed by milter-greylist-4.0.1 (shiva.imag.fr [129.88.30.5]); Sun, 09 Aug 2009 20:00:53 +0200 (CEST) X-Greylist: Delayed for 00:29:34 by milter-greylist-4.0.1 (shiva.imag.fr [129.88.30.5]); Sun, 09 Aug 2009 19:59:56 +0200 (CEST) X-IMAG-MailScanner: Found to be clean, Found to be clean X-IMAG-MailScanner-SpamCheck: , X-Loop: globillum@imag.fr X-Sequence: 394 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/html; charset=windows-1252 X-IMAG-MailScanner-Information: Please contact MI2S MIM for more information X-MailScanner-ID: n79I0qHr023945 X-IMAG-MailScanner-From: globillum-owner@imag.fr MailScanner-NULL-Check: 1250445653.74544@ys9zEAB3slVJ4FD0uAZ0RA X-Spam-Status: LOW ; -26 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok.kom.tuwien.ac.at X-Virus-Scanned: by amavisd-new X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

ANNOUNCE: 09/08/09 Release of RADBIB and GITHESIS

RADBIB is a comprehensive bibliography of radiosity, photon mapping, and related global illumination papers, theses, articles, and books. It currently includes 2,732 references -- 13 new additions since its 09/05/18 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of August 9, 2009) from:

  http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 336 references to radiosity, photon mapping, and related global illumination theses -- no new additions since the 09/05/18 release.

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

Ian Ashdown, P. Eng., LC, FIES

President

byHeart Consultants Limited

http://www.helios32.com

 

------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-path: Envelope-to: wp@cg.tuwien.ac.at Delivery-date: Tue, 15 Sep 2009 19:22:02 +0200 Received: from tuvok.kom.tuwien.ac.at ([192.35.241.66]:54362) by christl.cg.tuwien.ac.at with esmtp (Exim 4.63) (envelope-from ) id 1Mnbj7-0006K9-W0; Tue, 15 Sep 2009 19:22:02 +0200 Received: from shiva.imag.fr (mx1.imag.fr [129.88.30.5]) by tuvok.kom.tuwien.ac.at (8.14.1/8.14.1) with ESMTP id n8FHLj3v031000; Tue, 15 Sep 2009 19:21:46 +0200 X-Connecting-Host: mx1.imag.fr [129.88.30.5] X-Connecting-Addr: 129.88.30.5 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by shiva.imag.fr (8.13.8/8.13.8) with ESMTP id n8FHHYCv030945 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO); Tue, 15 Sep 2009 19:17:34 +0200 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id n8FHLeli019753; Tue, 15 Sep 2009 19:21:40 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id n8FHLbeG019748; Tue, 15 Sep 2009 19:21:37 +0200 Received: from imag.imag.fr (imag.imag.fr [129.88.30.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id n8FHKHeh018703 for ; Tue, 15 Sep 2009 19:20:17 +0200 Received: from server.agi32.com (unknown.ord.scnet.net [66.225.254.249] (may be forged)) by imag.imag.fr (8.13.8/8.13.8) with ESMTP id n8FHGGeF025587 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO) for ; Tue, 15 Sep 2009 19:16:28 +0200 (CEST) Received: from s01060006257abbc2.vn.shawcable.net ([24.87.85.53] helo=Ian) by server.agi32.com with esmtpa (Exim 4.69) (envelope-from ) id 1MnbdQ-00078F-PM for globillum@imag.fr; Tue, 15 Sep 2009 11:16:08 -0600 From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: 09/09/14 Release of RADBIB and GITHESIS Date: Tue, 15 Sep 2009 10:15:55 -0700 Organization: byHeart Consultants Limited Message-ID: <51F7010711CE411BB10680EB0EC56AEC@Ian> MIME-Version: 1.0 X-Mailer: Microsoft Office Outlook 11 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2900.5579 Thread-Index: Aco2KC7EQzzKVQr3R2OstkauK5NnwA== X-AntiAbuse: This header was added to track abuse, please include it with any abuse report X-AntiAbuse: Primary Hostname - server.agi32.com X-AntiAbuse: Original Domain - imag.fr X-AntiAbuse: Originator/Caller UID/GID - [47 12] / [47 12] X-AntiAbuse: Sender Address Domain - helios32.com X-IMAG-MailScanner: Found to be clean, Found to be clean X-IMAG-MailScanner-SpamCheck: , X-Loop: globillum@imag.fr X-Sequence: 397 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/html; charset=windows-1252 X-Greylist: Sender passed SPF test, not delayed by milter-greylist-4.1.1 (tuvok.kom.tuwien.ac.at [192.35.241.66]); Tue, 15 Sep 2009 19:21:46 +0200 (CEST) X-Greylist: Sender IP whitelisted, not delayed by milter-greylist-4.0.1 (shiva.imag.fr [129.88.30.5]); Tue, 15 Sep 2009 19:17:34 +0200 (CEST) X-IMAG-MailScanner-Information: Please contact MI2S MIM for more information X-MailScanner-ID: n8FHHYCv030945 X-IMAG-MailScanner-From: globillum-owner@imag.fr MailScanner-NULL-Check: 1253639855.26629@95pon1tjyK2H/x6z7HbHyw X-Spam-Status: LOW ; 0 X-Spam-TU-Processing-Host: tuvok.kom.tuwien.ac.at X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit

ANNOUNCE: 09/09/14 Release of RADBIB and GITHESIS

RADBIB is a comprehensive bibliography of radiosity, photon mapping, and related global illumination papers, theses, articles, and books. It currently includes 2,745 references -- 13 new additions since its 09/08/09 release.

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of September 14, 2009) from:

  http://www.helios32.com (Resources section)

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 336 references to radiosity, photon mapping, and related global illumination theses -- no new additions since the 09/08/09 release.

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

Ian Ashdown, P. Eng., LC, FIES
President
byHeart Consultants Limited
http://www.helios32.com

------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From To: globillum@imag.fr From: Werner Purgathofer Subject: CFP: c&g Special Issue on Procedural Methods in CG Bcc: Michael Wimmer , Peter Wonka Message-Id: <7.1.0.9.2.20091009081748.05379808@cg.tuwien.ac.at> X-Eudora-Signature: X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Date: Fri, 9 Oct 2009 08:18:52 Content-type: text/plain; charset=windows-1252; format=flowed MIME-Version: 1.0 Content-transfer-encoding: 8bit [Apologies if you receive this CFP more than once] CALL FOR PAPERS Procedural Methods in Computer Graphics Special Issue of Computers & Graphics, August 2010 http://www.cg.tuwien.ac.at/cagproceduralissue/ Submission deadline: January 7, 2010 Guest Editors: Michael Wimmer Peter Wonka AIMS AND SCOPE: --------------- The purpose of this special issue is to attract and showcase novel research results on procedural methods in computer graphics. We thus solicit articles that report innovative results in related research. Potential topics for articles include, but are not limited to, the following: Rendering and visualization of procedural models Procedural modeling of textures and texture synthesis Procedural surface modeling Image-guided procedural modeling Procedural methods for animation Procedural methods to model plants and landscapes Procedural methods in computational photography and image processing Procedural methods in virtual heritage User interfaces for procedural modeling Procedural modeling of urban structures and architecture Procedural sound modeling DEADLINES: ---------- Submissions due: January 7, 2010 First notification: April 5, 2010 Revised version due: May 5, 2010 Final notification: May 12, 2010 Camera ready copies: May 27, 2010 To expedite the review process we would appreciate it if authors intending to submit a paper could send a title, author list, and abstract to wimmer@cg.tuwien.ac.at by January 2, 2009. SUBMISSION INFORMATION: ----------------------- Please prepare your article in Latex, using the instructions and style provided here: http://www.elsevier.com/latex. Use the following line in your manuscript: \documentclass[5p,times]{elsarticle} Articles should be as long as their content requires, but not longer. If your article exceeds 14 pages including all references and images when formatted in the above style, please contact the guest editors before submitting. Please submit your article using our online manuscript submission service located here: http://ees.elsevier.com/cag/. Be sure to read the "Guide for Authors" before uploading, and follow the instructions carefully. When uploading your article, select the appropriate special issue title under the Article Type. Also include complete contact information for all authors and coauthors in the submission. The review process for this special issue will be double blind, so please select "manuscript without author details" as submission category, and remove any identifying items from your submission. If you have any questions about submitting your article, please contact authorsupport@elsevier.com. Please direct any correspondence prior to submission to the guest editors: Michael Wimmer Email: wimmer@cg.tuwien.ac.at Peter Wonka Email: peter.wonka@asu.edu This call is also available from the special issue webpage at: http://www.cg.tuwien.ac.at/cagproceduralissue/ From Return-path: Envelope-to: wp@cg.tuwien.ac.at Delivery-date: Mon, 08 Feb 2010 14:13:19 +0100 Received: from tuvok.kom.tuwien.ac.at ([192.35.241.66]:46774) by christl.cg.tuwien.ac.at with esmtp (Exim 4.63) (envelope-from ) id 1NeTQV-00014F-1e; Mon, 08 Feb 2010 14:13:19 +0100 Received: from shiva.imag.fr (mx1.imag.fr [129.88.30.5]) by tuvok.kom.tuwien.ac.at (8.14.1/8.14.1) with ESMTP id o18DD1Qh003574; Mon, 8 Feb 2010 14:13:01 +0100 X-Connecting-Host: mx1.imag.fr [129.88.30.5] X-Connecting-Addr: 129.88.30.5 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by shiva.imag.fr (8.13.8/8.13.8) with ESMTP id o18DB8Ib021528 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO); Mon, 8 Feb 2010 14:11:08 +0100 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id o18DClXw024438; Mon, 8 Feb 2010 14:12:47 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id o18DCfPj024406; Mon, 8 Feb 2010 14:12:41 +0100 Received: from rominette.imag.fr (mx2.imag.fr [129.88.30.17]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id o18DCC69022482 for ; Mon, 8 Feb 2010 14:12:12 +0100 Received: from mini003.webpack.hosteurope.de (mini003.webpack.hosteurope.de [80.237.130.132]) by rominette.imag.fr (8.13.8/8.13.8) with ESMTP id o18DAUdX021583 for ; Mon, 8 Feb 2010 14:10:31 +0100 Received: from ip-94-79-177-17.unitymediagroup.de ([94.79.177.17] helo=touchlab-pc4.cpe.ish); authenticated by mini003.webpack.hosteurope.de running ExIM with esmtpsa (TLSv1:RC4-SHA:128) id 1NeT69-0008If-44; Mon, 08 Feb 2010 13:52:17 +0100 To: globillum@imag.fr Date: Mon, 08 Feb 2010 13:52:16 +0100 Subject: stunningly realistic architecture/nature/lighting CGI MIME-Version: 1.0 From: "Wolfram Kresse" Organization: WekaDev Message-ID: User-Agent: Opera Mail/10.10 (Win32) X-bounce-key: webpack.hosteurope.de;wk@wkresse.de;1265634728;59f54f06; X-Greylist: Sender passed SPF test, not delayed by milter-greylist-4.1.1 (tuvok.kom.tuwien.ac.at [192.35.241.66]); Mon, 08 Feb 2010 14:13:02 +0100 (CET) X-Greylist: Sender IP whitelisted, not delayed by milter-greylist-4.0.1 (shiva.imag.fr [129.88.30.5]); Mon, 08 Feb 2010 14:11:09 +0100 (CET) X-Greylist: Delayed for 00:19:50 by milter-greylist-4.2.2 (rominette.imag.fr [129.88.30.17]); Mon, 08 Feb 2010 14:10:31 +0100 (CET) X-IMAG-MailScanner: Found to be clean, Found to be clean X-IMAG-MailScanner-SpamCheck: , X-Loop: globillum@imag.fr X-Sequence: 400 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-IMAG-MailScanner-Information: Please contact MI2S MIM for more information X-MailScanner-ID: o18DB8Ib021528 X-IMAG-MailScanner-From: globillum-owner@imag.fr MailScanner-NULL-Check: 1266239469.70749@qhAxjy5UFF3pHprHSxJtRA X-Spam-Status: LOW ; 0 X-Spam-TU-Processing-Host: tuvok.kom.tuwien.ac.at X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Hello fellow globilluminati ;-) Are you familiar with the work of Alex Roman? A friend just showed me this CGI film, which might yield to some jaw-dropping - at least it did for me: until I saw the making-of, I was highly sceptical that this actually *was* entirely CGI... While I'm not sure whether he actually used some form of global illumination, it is still a must-see for people striving to achieve absolute realism in CGI imagery - he combined many techniques into an artistical and convincing performance. Until I saw the making-of, I was highly sceptical that this actually *was* entirely CGI - except for the occasionally visible texture repeating pattern (sometimes intentional), the effort put into getting the details right make this a pretty impressive piece of work, IMHO. http://vimeo.com/7809605 Have fun watching this in fullscreen, Best regards, Wolfram -- +-----+-------------------------------------------------------------------+ | 8-P | Wolfram Kresse wk@wkresse.de http://www.wkresse.de | +-----+-------------------------------------------------------------------+ Data: Turbolift 7 is jammed. Picard: ALL HANDS, ABANDON SHIP! Computer! Set auto-destruct to 30 seconds! Number One: Uh...Captain? Picard: ...er...sorry, I got carried away. ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-path: Envelope-to: wp@cg.tuwien.ac.at Delivery-date: Mon, 08 Feb 2010 14:30:45 +0100 Received: from tuvok.kom.tuwien.ac.at ([192.35.241.66]:45855) by christl.cg.tuwien.ac.at with esmtp (Exim 4.63) (envelope-from ) id 1NeThN-0001MO-D6; Mon, 08 Feb 2010 14:30:45 +0100 Received: from shiva.imag.fr (mx1.imag.fr [129.88.30.5]) by tuvok.kom.tuwien.ac.at (8.14.1/8.14.1) with ESMTP id o18DUbO7006280; Mon, 8 Feb 2010 14:30:37 +0100 X-Connecting-Host: mx1.imag.fr [129.88.30.5] X-Connecting-Addr: 129.88.30.5 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by shiva.imag.fr (8.13.8/8.13.8) with ESMTP id o18DSYVM028565 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO); Mon, 8 Feb 2010 14:28:34 +0100 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id o18DUCZO009590; Mon, 8 Feb 2010 14:30:12 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id o18DUCRr009588; Mon, 8 Feb 2010 14:30:12 +0100 Received: from rominette.imag.fr (mx2.imag.fr [129.88.30.17]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id o18DThEf007637 for ; Mon, 8 Feb 2010 14:29:43 +0100 Received: from mini003.webpack.hosteurope.de (mini003.webpack.hosteurope.de [80.237.130.132]) by rominette.imag.fr (8.13.8/8.13.8) with ESMTP id o18DS1nU026935 for ; Mon, 8 Feb 2010 14:28:02 +0100 Received: from ip-94-79-177-17.unitymediagroup.de ([94.79.177.17] helo=touchlab-pc4.cpe.ish); authenticated by mini003.webpack.hosteurope.de running ExIM with esmtpsa (TLSv1:RC4-SHA:128) id 1NeTgI-0003Dy-9k; Mon, 08 Feb 2010 14:29:38 +0100 To: globillum@imag.fr Subject: Re: stunningly realistic architecture/nature/lighting CGI References: Date: Mon, 08 Feb 2010 14:29:39 +0100 MIME-Version: 1.0 From: "Wolfram Kresse" Organization: WekaDev Message-ID: In-Reply-To: User-Agent: Opera Mail/10.10 (Win32) X-bounce-key: webpack.hosteurope.de;wk@wkresse.de;1265635779;848375ed; X-Greylist: Sender passed SPF test, not delayed by milter-greylist-4.1.1 (tuvok.kom.tuwien.ac.at [192.35.241.66]); Mon, 08 Feb 2010 14:30:38 +0100 (CET) X-Greylist: Sender IP whitelisted, not delayed by milter-greylist-4.0.1 (shiva.imag.fr [129.88.30.5]); Mon, 08 Feb 2010 14:28:34 +0100 (CET) X-Greylist: IP, sender and recipient auto-whitelisted, not delayed by milter-greylist-4.2.2 (rominette.imag.fr [129.88.30.17]); Mon, 08 Feb 2010 14:28:02 +0100 (CET) X-IMAG-MailScanner: Found to be clean, Found to be clean X-IMAG-MailScanner-SpamCheck: , X-Loop: globillum@imag.fr X-Sequence: 401 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-IMAG-MailScanner-Information: Please contact MI2S MIM for more information X-MailScanner-ID: o18DSYVM028565 X-IMAG-MailScanner-From: globillum-owner@imag.fr MailScanner-NULL-Check: 1266240516.5636@fxAP9Xit4+H09DycHodtZA X-Spam-Status: LOW ; 0 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok.kom.tuwien.ac.at X-Virus-Scanned: by amavisd-new X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit On Mon, 08 Feb 2010 13:52:16 +0100, Wolfram Kresse wrote: > While I'm not sure whether he actually used some form of global illumination, Hm, watching the film again, and paying more attention, I saw the obvious global illumination effects. It *is*, after all, an essential part of realistic imagery - that's why we're doing this ;-) In fact, he mentions he uses V-Ray. Cheers, Wolfram -- +-----+-------------------------------------------------------------------+ | 8-P | Wolfram Kresse wk@wkresse.de http://www.wkresse.de | +-----+-------------------------------------------------------------------+ Geordi: I'd like to enhance the annular static particle controller by using our ventral interdimensional flux module to access the tertiary converging pulse node! Data: I do not recommend doing this before matching the enhanced diverging storage discriminator to our confocal energetic shield sensor, otherwise the inverse cataclysmic quantum charger will destabilize. Geordi: Smart-ass. ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-path: Envelope-to: wp@cg.tuwien.ac.at Delivery-date: Fri, 12 Feb 2010 23:46:29 +0100 Received: from neelix.kom.tuwien.ac.at ([192.35.241.67]:37818) by christl.cg.tuwien.ac.at with esmtp (Exim 4.63) (envelope-from ) id 1Ng4HM-0005c6-T5; Fri, 12 Feb 2010 23:46:29 +0100 Received: from shiva.imag.fr (mx1.imag.fr [129.88.30.5]) by neelix.kom.tuwien.ac.at (8.14.1/8.14.1) with ESMTP id o1CMkLI9025691; Fri, 12 Feb 2010 23:46:21 +0100 X-Connecting-Host: mx1.imag.fr [129.88.30.5] X-Connecting-Addr: 129.88.30.5 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by shiva.imag.fr (8.13.8/8.13.8) with ESMTP id o1CMiNna029510 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO); Fri, 12 Feb 2010 23:44:23 +0100 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id o1CMkFN8018591; Fri, 12 Feb 2010 23:46:15 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id o1CMkAsV018579; Fri, 12 Feb 2010 23:46:10 +0100 Received: from shiva.imag.fr (mx1.imag.fr [129.88.30.5]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id o1CMjJMd017576 for ; Fri, 12 Feb 2010 23:45:19 +0100 Received: from mail.vsiltd.co.uk (mail.vsiltd.co.uk [195.152.206.150]) by shiva.imag.fr (8.13.8/8.13.8) with ESMTP id o1CMhMiC029203 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO) for ; Fri, 12 Feb 2010 23:43:24 +0100 Received: from macy.ows.local ([195.152.206.70]) by mail.vsiltd.co.uk (8.13.8/8.13.8) with ESMTP id o1CMRUhi015679 for ; Fri, 12 Feb 2010 22:27:31 GMT Subject: importance sampling direct lighting MIME-Version: 1.0 Date: Fri, 12 Feb 2010 22:27:30 -0000 X-MimeOLE: Produced By Microsoft Exchange V6.5 Message-ID: Thread-Topic: importance sampling direct lighting Thread-Index: AcqsMpCHTcq9dIASSWqsnfAWryz0vQ== From: "Neil Gatenby" To: globillum@imag.fr X-VSI-MailScanner-Information: Please contact ITS for more information X-VSI-MailScanner: Found to be clean X-VSI-MailScanner-SpamCheck: not spam, SpamAssassin (not cached, score=-2.301, required 6, AWL 0.20, BAYES_00 -2.60, HTML_MESSAGE 0.00, RDNS_NONE 0.10) X-VSI-MailScanner-From: neil.gatenby@lightworkdesign.com X-VSI-MailScanner-To: globillum@imag.fr X-Spam-Status: LOW ; -11 X-Spam-Status: No X-Greylist: Sender passed SPF test, not delayed by milter-greylist-4.1.1 (neelix.kom.tuwien.ac.at [192.35.241.67]); Fri, 12 Feb 2010 23:46:22 +0100 (CET) X-Greylist: Sender IP whitelisted, not delayed by milter-greylist-4.0.1 (shiva.imag.fr [129.88.30.5]); Fri, 12 Feb 2010 23:44:25 +0100 (CET) X-Greylist: Delayed for 00:17:04 by milter-greylist-4.0.1 (shiva.imag.fr [129.88.30.5]); Fri, 12 Feb 2010 23:43:24 +0100 (CET) X-IMAG-MailScanner: Found to be clean, Found to be clean X-IMAG-MailScanner-SpamCheck: , X-Loop: globillum@imag.fr X-Sequence: 403 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/html; charset=windows-1252 X-IMAG-MailScanner-Information: Please contact MI2S MIM for more information X-MailScanner-ID: o1CMiNna029510 X-IMAG-MailScanner-From: globillum-owner@imag.fr MailScanner-NULL-Check: 1266619466.17236@vxhcXgjM+QkbFnWOxiZTAQ X-Spam-Level: - X-Spam-TU-Processing-Host: neelix.kom.tuwien.ac.at X-Virus-Scanned: by amavisd-new X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Content-Type: multipart/alternative; boundary="----_=_NextPart_001_01CAAC32.907A1634" Content-class: urn:content-classes:message
 
Hi
 
When I was younger and less wise I listened to a paper (probably at a Eurographics Workshop on Rendering) and now I can't find the paper ...
 
Part (all?) of the talk was on a lighting situation where you have hundreds (N) of small point/spot lights and you calculated their contribution using m<<N shadow rays  
 
   for each light L
     find unoccluded contribution at point of interest, due to L
     accumulate unccluded data ... build a PDF
 
   for i = 1 to m
     pick a light by importance sampling the PDF
     cast shadow ray - get a visibility - increment irrad at point of interest
 
   add in the contribution of the N-m-1 other lights using the mean visibility got from sampling the m
 
They were lighting a theatre with lots of little lights illuminating the many steps in the auditorium
 
Ring any bells?
 
I can find quite a few modern papers that take the approach and advance upon it, but can't find the original paper - even digging around in bibliographies
 
I have a feeling it might have been Paul Heckbert or Greg Ward - but they presented lots of papers (and often each others!) so maybe that is not the case.  Pete Shirley?
 
Any pointers much appreciated
 
Have a good w/e all
 
TIA
Neil
 
 
 
 
------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-path: Envelope-to: wp@cg.tuwien.ac.at Delivery-date: Sat, 13 Feb 2010 02:35:27 +0100 Received: from neelix.kom.tuwien.ac.at ([192.35.241.67]:35253) by christl.cg.tuwien.ac.at with esmtp (Exim 4.63) (envelope-from ) id 1Ng6ut-0006mv-2x; Sat, 13 Feb 2010 02:35:27 +0100 Received: from shiva.imag.fr (mx1.imag.fr [129.88.30.5]) by neelix.kom.tuwien.ac.at (8.14.1/8.14.1) with ESMTP id o1D1ZHmK026898; Sat, 13 Feb 2010 02:35:18 +0100 X-Connecting-Host: mx1.imag.fr [129.88.30.5] X-Connecting-Addr: 129.88.30.5 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by shiva.imag.fr (8.13.8/8.13.8) with ESMTP id o1D1Wp75003894 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO); Sat, 13 Feb 2010 02:32:51 +0100 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id o1D1YhKr013769; Sat, 13 Feb 2010 02:34:43 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id o1D1YgWh013762; Sat, 13 Feb 2010 02:34:42 +0100 Received: from rominette.imag.fr (mx2.imag.fr [129.88.30.17]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id o1D1XsGq012754 for ; Sat, 13 Feb 2010 02:33:54 +0100 Received: from mail.vsiltd.co.uk (mail.vsiltd.co.uk [195.152.206.150]) by rominette.imag.fr (8.13.8/8.13.8) with ESMTP id o1D1Vt9s013930 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO) for ; Sat, 13 Feb 2010 02:31:58 +0100 Received: from macy.ows.local ([195.152.206.70]) by mail.vsiltd.co.uk (8.13.8/8.13.8) with ESMTP id o1D1XH0P032159; Sat, 13 Feb 2010 01:33:18 GMT MIME-Version: 1.0 Subject: RE: importance sampling direct lighting X-MimeOLE: Produced By Microsoft Exchange V6.5 Date: Sat, 13 Feb 2010 01:32:49 -0000 Message-ID: Thread-Topic: importance sampling direct lighting Thread-Index: AcqsNwk/Uqq3nuXOQZ+tLxSH4YJTIAAFT3yA References: <4B21426F-E457-4DBE-A6A2-7B672BD1458C@lmi.net> From: "Neil Gatenby" To: "Greg Ward" Cc: globillum@imag.fr X-VSI-MailScanner-Information: Please contact ITS for more information X-VSI-MailScanner: Found to be clean X-VSI-MailScanner-SpamCheck: not spam, SpamAssassin (not cached, score=-2.302, required 6, AWL 0.20, BAYES_00 -2.60, RDNS_NONE 0.10) X-VSI-MailScanner-From: neil.gatenby@lightworkdesign.com X-VSI-MailScanner-To: globillum@imag.fr, gregoryjward@gmail.com X-Spam-Status: LOW ; -26 X-Spam-Status: No X-Greylist: Sender passed SPF test, not delayed by milter-greylist-4.1.1 (neelix.kom.tuwien.ac.at [192.35.241.67]); Sat, 13 Feb 2010 02:35:20 +0100 (CET) X-Greylist: Sender IP whitelisted, not delayed by milter-greylist-4.0.1 (shiva.imag.fr [129.88.30.5]); Sat, 13 Feb 2010 02:32:55 +0100 (CET) X-Greylist: Delayed for 03:05:38 by milter-greylist-4.2.2 (rominette.imag.fr [129.88.30.17]); Sat, 13 Feb 2010 02:31:59 +0100 (CET) X-IMAG-MailScanner: Found to be clean, Found to be clean X-IMAG-MailScanner-SpamCheck: , X-MIME-Autoconverted: from quoted-printable to 8bit by chopinette.imag.fr id o1D1XsGq012754 X-Loop: globillum@imag.fr X-Sequence: 404 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/plain; charset=windows-1252; format=flowed X-IMAG-MailScanner-Information: Please contact MI2S MIM for more information X-MailScanner-ID: o1D1Wp75003894 X-IMAG-MailScanner-From: globillum-owner@imag.fr MailScanner-NULL-Check: 1266629575.58234@XrsrDh9xYdd+5sR9nD4wmQ X-Spam-Level: - X-Spam-TU-Processing-Host: neelix.kom.tuwien.ac.at X-Virus-Scanned: by amavisd-new X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Content-class: urn:content-classes:message Content-Type: text/plain; charset="us-ascii" Content-Transfer-Encoding: 8bit Brilliant Thanks Greg, and to all the others that responded directly Am hoping to get to Saarbruecken this year, but childcare duties may keep me away Cheers N > -----Original Message----- > From: Greg Ward [mailto:gregoryjward@gmail.com] > Sent: 12 February 2010 22:59 > To: Neil Gatenby > Cc: globillum@imag.fr > Subject: Re: importance sampling direct lighting > > Hi Neil, > > I think you're referring to my "Adaptive Shadow Testing for Ray > Tracing" paper, which I gave at the 1991 EG workshop on rendering -- > good memory! The Candlestick Theater model (created by Charles > Ehrlich) was given as an example during my talk, but doesn't > appear in > the paper. This technique was also mentioned in the 1994 Siggraph > paper on Radiance. Peter Shirley gave a paper on a different shadow > testing technique from the same workshop, where he treated > the set of > all light sources as a single (discontinuous) source and applied MC > sampling. A link to my papers can be found towards the bottom of my > pubs page at: > > http://www.anyhere.com/gward/papers.html > > Pete's '91 EGWR paper, "Direct Lighting Calculation by Monte Carlo > Integration", is reference number 6 on his pubs page: > > http://www.cs.utah.edu/~shirley/papers/ > > Cheers, > -Greg > > > From: "Neil Gatenby" > > Date: February 12, 2010 2:27:30 PM PST > > > > Hi > > > > When I was younger and less wise I listened to a paper > (probably at > > a Eurographics Workshop on Rendering) and now I can't find the > > paper ... > > > > Part (all?) of the talk was on a lighting situation where you have > > hundreds (N) of small point/spot lights and you calculated their > > contribution using m< > > > for each light L > > find unoccluded contribution at point of interest, due to L > > accumulate unccluded data ... build a PDF > > > > for i = 1 to m > > pick a light by importance sampling the PDF > > cast shadow ray - get a visibility - increment irrad at point > > of interest > > > > add in the contribution of the N-m-1 other lights using > the mean > > visibility got from sampling the m > > > > They were lighting a theatre with lots of little lights > illuminating > > the many steps in the auditorium > > > > Ring any bells? > > > > I can find quite a few modern papers that take the approach and > > advance upon it, but can't find the original paper - even digging > > around in bibliographies > > > > I have a feeling it might have been Paul Heckbert or Greg > Ward - but > > they presented lots of papers (and often each others!) so > maybe that > > is not the case. Pete Shirley? > > > > Any pointers much appreciated > > > > Have a good w/e all > > > > TIA > > Neil > ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-path: Envelope-to: wp@cg.tuwien.ac.at Delivery-date: Mon, 21 Jun 2010 21:03:39 +0200 Received: from tuvok.kom.tuwien.ac.at ([192.35.241.66]:49732) by christl.cg.tuwien.ac.at with esmtp (Exim 4.63) (envelope-from ) id 1OQmHI-0004V7-AC; Mon, 21 Jun 2010 21:03:29 +0200 Received: from shiva.imag.fr (mx1.imag.fr [129.88.30.5]) by tuvok.kom.tuwien.ac.at (8.14.1/8.14.1) with ESMTP id o5LJ3Id7020999; Mon, 21 Jun 2010 21:03:19 +0200 X-Connecting-Host: mx1.imag.fr [129.88.30.5] X-Connecting-Addr: 129.88.30.5 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by shiva.imag.fr (8.13.8/8.13.8) with ESMTP id o5LIss5c028049 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO); Mon, 21 Jun 2010 20:54:54 +0200 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id o5LJ3DIE025600; Mon, 21 Jun 2010 21:03:13 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id o5LJ3CM8025595; Mon, 21 Jun 2010 21:03:12 +0200 Received: from shiva.imag.fr (mx1.imag.fr [129.88.30.5]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id o5LJ2IYM024577 for ; Mon, 21 Jun 2010 21:02:18 +0200 Received: from server.agi32.com (unknown.hostforweb.net [66.225.254.249] (may be forged)) by shiva.imag.fr (8.13.8/8.13.8) with ESMTP id o5LIrsNI027751 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO) for ; Mon, 21 Jun 2010 20:53:56 +0200 Received: from s0106001e5802cdcd.vn.shawcable.net ([174.7.99.121] helo=Evergreen) by server.agi32.com with esmtp (Exim 4.69) (envelope-from ) id 1OQlgB-0003Ok-6H for globillum@imag.fr; Mon, 21 Jun 2010 12:25:07 -0600 From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: 10/06/21 Release of RADBIB and GITHESIS Date: Mon, 21 Jun 2010 11:25:03 -0700 Message-ID: <005a01cb116f$12d8a0e0$3889e2a0$@com> MIME-Version: 1.0 X-Mailer: Microsoft Office Outlook 12.0 Thread-Index: AcsRbxFGwSPSWI6lRWivSvCUUYHhWA== X-AntiAbuse: This header was added to track abuse, please include it with any abuse report X-AntiAbuse: Primary Hostname - server.agi32.com X-AntiAbuse: Original Domain - imag.fr X-AntiAbuse: Originator/Caller UID/GID - [47 12] / [47 12] X-AntiAbuse: Sender Address Domain - helios32.com X-Greylist: Sender passed SPF test, not delayed by milter-greylist-4.1.1 (tuvok.kom.tuwien.ac.at [192.35.241.66]); Mon, 21 Jun 2010 21:03:19 +0200 (CEST) X-Greylist: Sender IP whitelisted, not delayed by milter-greylist-4.0.1 (shiva.imag.fr [129.88.30.5]); Mon, 21 Jun 2010 20:54:54 +0200 (CEST) X-Greylist: Delayed for 00:37:05 by milter-greylist-4.0.1 (shiva.imag.fr [129.88.30.5]); Mon, 21 Jun 2010 20:53:57 +0200 (CEST) X-IMAG-MailScanner: Found to be clean, Found to be clean X-IMAG-MailScanner-SpamCheck: , X-Loop: globillum@imag.fr X-Sequence: 410 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/html; charset=windows-1252 X-IMAG-MailScanner-Information: Please contact MI2S MIM for more information X-MailScanner-ID: o5LIss5c028049 X-IMAG-MailScanner-From: globillum-owner@imag.fr MailScanner-NULL-Check: 1277751298.93795@f9+MfrGX8V1zIGYmk1f9uQ X-Spam-Status: LOW ; 0 X-Spam-TU-Processing-Host: tuvok.kom.tuwien.ac.at X-Virus-Scanned: by amavisd-new on vc7.kom.tuwien.ac.at X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Content-Type: multipart/alternative; boundary="----=_NextPart_000_005B_01CB1134.6679C8E0" Content-Language: en-ca

ANNOUNCE: 10/06/21 Release of RADBIB and GITHESIS

 

RADBIB is a comprehensive bibliography of radiosity, photon mapping, and related global illumination papers, theses, articles, and books. It currently includes 2,803 references -- 5813 new additions since its 09/09/14 release.

 

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of June 21, 2010) from:

 

  http://www.helios32.com (Resources section)

 

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 337 references to radiosity, photon mapping, and related global illumination theses -- one new addition since the 09/09/14 release.

 

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

 

Ian Ashdown, P. Eng., LC, FIES

President

byHeart Consultants Limited

http://www.helios32.com

 

------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From Return-path: Envelope-to: wp@cg.tuwien.ac.at Delivery-date: Fri, 11 Feb 2011 07:31:39 +0100 Received: from tuvok.kom.tuwien.ac.at ([192.35.241.66]) by mail.cg.tuwien.ac.at with esmtp (Exim 4.71) (envelope-from ) id 1PnmXa-0005RV-B6; Fri, 11 Feb 2011 07:31:38 +0100 Received: from shiva.imag.fr (mx1.imag.fr [129.88.30.5]) by tuvok.kom.tuwien.ac.at (8.14.1/8.14.1) with ESMTP id p1B6VS6p027957; Fri, 11 Feb 2011 07:31:28 +0100 X-Connecting-Host: mx1.imag.fr [129.88.30.5] X-Connecting-Addr: 129.88.30.5 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by shiva.imag.fr (8.13.8/8.13.8) with ESMTP id p1B6VQGq010477 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO); Fri, 11 Feb 2011 07:31:26 +0100 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id p1B6VRup031259; Fri, 11 Feb 2011 07:31:27 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id p1B6VQRQ031254; Fri, 11 Feb 2011 07:31:26 +0100 Received: from rominette.imag.fr (mx2.imag.fr [129.88.30.17]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id p1B6Umrw030961 for ; Fri, 11 Feb 2011 07:30:49 +0100 Received: from server.agi32.com (server.agi32.com [65.60.14.58]) by rominette.imag.fr (8.13.8/8.13.8) with ESMTP id p1B62F3F011057 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO) for ; Fri, 11 Feb 2011 07:02:17 +0100 Received: from s0106001cc0f76225.vn.shawcable.net ([174.7.111.91] helo=Evergreen) by server.agi32.com with esmtp (Exim 4.69) (envelope-from ) id 1PnlDI-000384-8Z for globillum@imag.fr; Thu, 10 Feb 2011 22:06:36 -0700 From: "Ian Ashdown" To: globillum@imag.fr Subject: ANNOUNCE: 11/02/10 Release of RADBIB and GITHESIS Date: Thu, 10 Feb 2011 21:06:01 -0800 Message-ID: <000001cbc9a9$62297050$267c50f0$@com> MIME-Version: 1.0 X-Mailer: Microsoft Office Outlook 12.0 Thread-Index: AcvJqWBaXKgoWlhLSsuivLhBBcJDFg== X-AntiAbuse: This header was added to track abuse, please include it with any abuse report X-AntiAbuse: Primary Hostname - server.agi32.com X-AntiAbuse: Original Domain - imag.fr X-AntiAbuse: Originator/Caller UID/GID - [47 12] / [47 12] X-AntiAbuse: Sender Address Domain - helios32.com X-Greylist: Sender passed SPF test, not delayed by milter-greylist-4.1.1 (tuvok.kom.tuwien.ac.at [192.35.241.66]); Fri, 11 Feb 2011 07:31:29 +0100 (CET) X-Greylist: Sender IP whitelisted, not delayed by milter-greylist-4.0.1 (shiva.imag.fr [129.88.30.5]); Fri, 11 Feb 2011 07:31:27 +0100 (CET) X-Greylist: Delayed for 00:55:35 by milter-greylist-4.2.2 (rominette.imag.fr [129.88.30.17]); Fri, 11 Feb 2011 07:02:17 +0100 (CET) X-IMAG-MailScanner: Found to be clean, Found to be clean X-IMAG-MailScanner-SpamCheck: , X-Loop: globillum@imag.fr X-Sequence: 411 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: text/html; charset=windows-1252 X-IMAG-MailScanner-Information: Please contact MI2S MIM for more information X-MailScanner-ID: p1B6VQGq010477 X-IMAG-MailScanner-From: globillum-owner@imag.fr MailScanner-NULL-Check: 1298010687.08845@wQw/lWe3HMvBB+XDvOxyrw X-Spam-Status: LOW ; -26 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok.kom.tuwien.ac.at X-Virus-Scanned: by amavisd-new on vc9.kom.tuwien.ac.at X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Content-transfer-encoding: 8bit Content-Type: multipart/alternative; boundary="----=_NextPart_000_0001_01CBC966.54063050" Content-Language: en-ca

ANNOUNCE: 11/02/10 Release of RADBIB and GITHESIS

 

RADBIB is a comprehensive bibliography of radiosity, photon mapping, and related global illumination papers, theses, articles, and books. It currently includes 2,840 references -- 37 new additions since its 10/06/21 release.

 

This bibliography is available in BibTex format as RADBIB.BIB (with a release date of February 10, 2011) from:

 

  http://www.helios32.com (Resources section)

 

Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 338 references to radiosity, photon mapping, and related global illumination theses -- one new addition since the 10/06/21 release.

 

Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited.

 

Ian Ashdown, P. Eng., FIES

President

byHeart Consultants Limited

http://www.helios32.com

 

CONFIDENTIALITY NOTICE: This entire communication, including without limitation any attachments, is intended for the use of ther recipient to which or whom it is addressed, and may contain confidential, personal, and or privileged informatio n. Please contact us immediately if you are not the intended recipient of this commumication, and do not copy, distribute, or take action relying on it. Any communication received in error, or subsequent reply, should be deleted or destroyed.

 

------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- From X-Account-Key: account1 X-UIDL: 0000c1934778b2c7 X-Mozilla-Status: 0001 X-Mozilla-Status2: 10000000 X-Mozilla-Keys: Return-path: Envelope-to: wp@cg.tuwien.ac.at Delivery-date: Fri, 15 Apr 2011 21:13:25 +0200 Received: from tuvok.kom.tuwien.ac.at ([192.35.241.66]) by mail.cg.tuwien.ac.at with esmtp (Exim 4.71) (envelope-from ) id 1QAoSK-0006A2-Pj; Fri, 15 Apr 2011 21:13:25 +0200 Received: from shiva.imag.fr (mx1.imag.fr [129.88.30.5]) by tuvok.kom.tuwien.ac.at (8.14.1/8.14.1) with ESMTP id p3FJDDOT002369; Fri, 15 Apr 2011 21:13:13 +0200 X-Connecting-Host: mx1.imag.fr [129.88.30.5] X-Connecting-Addr: 129.88.30.5 Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by shiva.imag.fr (8.13.8/8.13.8) with ESMTP id p3FJ2kMt010492 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO); Fri, 15 Apr 2011 21:02:46 +0200 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id p3FJ2mKM014408; Fri, 15 Apr 2011 21:02:48 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id p3FJ2lwa014401; Fri, 15 Apr 2011 21:02:47 +0200 Received: from shiva.imag.fr (mx1.imag.fr [129.88.30.5]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id p3FJ2RE2014362 for ; Fri, 15 Apr 2011 21:02:27 +0200 Received: from server.agi32.com (server.agi32.com [65.60.14.58]) by shiva.imag.fr (8.13.8/8.13.8) with ESMTP id p3FJ2L9A010411 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO) for ; Fri, 15 Apr 2011 21:02:23 +0200 Received: from s0106001cc0f76225.vn.shawcable.net ([174.7.123.54] helo=Evergreen) by server.agi32.com with esmtp (Exim 4.69) (envelope-from ) id 1QAnXN-0004xL-LU for globillum@imag.fr; Fri, 15 Apr 2011 12:14:34 -0600 From: "Ian Ashdown" To: Subject: ANNOUNCE: 11/04/15 Release of RADBIB and GITHESIS Date: Fri, 15 Apr 2011 11:14:24 -0700 Message-ID: <003401cbfb98$f48c5770$dda50650$@com> MIME-Version: 1.0 X-Mailer: Microsoft Office Outlook 12.0 Thread-Index: Acv7mPLu5O+IjGQOTMCOVLWH8/1gtA== X-AntiAbuse: This header was added to track abuse, please include it with any abuse report X-AntiAbuse: Primary Hostname - server.agi32.com X-AntiAbuse: Original Domain - imag.fr X-AntiAbuse: Originator/Caller UID/GID - [47 12] / [47 12] X-AntiAbuse: Sender Address Domain - helios32.com X-Source: X-Source-Args: X-Source-Dir: X-Greylist: Sender passed SPF test, not delayed by milter-greylist-4.1.1 (tuvok.kom.tuwien.ac.at [192.35.241.66]); Fri, 15 Apr 2011 21:13:14 +0200 (CEST) X-Greylist: Sender IP whitelisted, not delayed by milter-greylist-4.0.1 (shiva.imag.fr [129.88.30.5]); Fri, 15 Apr 2011 21:02:46 +0200 (CEST) X-Greylist: Delayed for 00:47:45 by milter-greylist-4.0.1 (shiva.imag.fr [129.88.30.5]); Fri, 15 Apr 2011 21:02:23 +0200 (CEST) X-IMAG-MailScanner: Found to be clean, Found to be clean X-IMAG-MailScanner-SpamCheck: , X-Loop: globillum@imag.fr X-Sequence: 414 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: multipart/mixed; boundary="----------=_1302894151-31352-14" X-IMAG-MailScanner-Information: Please contact MI2S MIM for more information X-MailScanner-ID: p3FJ2kMt010492 X-IMAG-MailScanner-From: globillum-owner@imag.fr MailScanner-NULL-Check: 1303498970.65234@mDCR8b8CkZhLuvXaH8exOA X-Spam-Status: LOW ; -26 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok.kom.tuwien.ac.at X-Virus-Scanned: by amavisd-new on vc7.kom.tuwien.ac.at This is a multi-part message in MIME format... ------------=_1302894151-31352-14 Content-Type: multipart/alternative; boundary="----=_NextPart_000_0035_01CBFB5E.482D7F70" Content-Language: en-ca This is a multi-part message in MIME format. ------=_NextPart_000_0035_01CBFB5E.482D7F70 Content-Type: text/plain; charset="us-ascii" Content-Transfer-Encoding: 7bit ANNOUNCE: 11/04/15 Release of RADBIB and GITHESIS RADBIB is a comprehensive bibliography of radiosity, photon mapping, and related global illumination papers, theses, articles, and books. It currently includes 2,855 references -- 15 new additions since its 11/02/10 release. This bibliography is available in BibTex format as RADBIB.BIB (with a release date of April 15, 2011) from: http://www.helios32.com (Resources section) ************************************************************************ NOTE: RADBIB does NOT include the following paper: Authors: Qiong Zhang School of International Business Tianjin Foreign Studies University Tianjin, China Zhichao Li Department of Information Management China Central Party School Beijing, China Riwei Wang Tianjin Key Laboratory of Intelligence Computing and Novel Software Technology Tianjin University of Technology Tianjin, China Month: October Year: 2010 Title: A Parallel Radiosity Algorithm for Virtual Reality Booktitle: 2010 Third International Congress on Image and Signal Processing (CISP 2010)) Volume: 5 Pages: 2469 -- 2472 Publisher: IEEE Xplore Digital Library DOI: 10.1109/CISP.2010.5647841 The authors are invited to contact the author of "Eigenvector Radiosity" (2001 MSc thesis, University of British Columbia) to explain why their "original technique" (funded by a grant from the Tianjin Natural Science Foundation) is simply an extract from the author's thesis (which they neglected to reference in their paper). ************************************************************************ Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 339 references to radiosity, photon mapping, and related global illumination theses -- one new addition since the 11/02/10 release. Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited. Ian Ashdown, P. Eng., FIES President byHeart Consultants Limited http://www.helios32.com ------=_NextPart_000_0035_01CBFB5E.482D7F70 Content-Type: text/html; charset="us-ascii" Content-Transfer-Encoding: quoted-printable

ANNOUNCE: 11/04/15 Release of RADBIB and GITHESIS=

 

RADBIB is a comprehensive bibliography of radiosi= ty, photon mapping, and

related global illumination papers, theses= , articles, and books. It

currently includes 2,855 references -- 1= 5 new additions since its

11/02/10 release.

<= p class=3DMsoNormal> 

release date of April 15, 2011) from:

 

&nbs= p; http://www.helios32.com (Resources section)

 

***= *********************************************************************<= /o:p>

NOTE: RADBIB does NOT include the following paper:

 =

Authors:     Qiong Zhang

  &nbs= p;          School of Internat= ional Business

        &nb= sp;       Tianjin Foreign Studies University=

           = ;     Tianjin, China

    =               <= o:p>

           =   Zhichao Li

       &= nbsp;     Department of Information

 &nbs= p;           Management C= hina Central Party School

      &nbs= p;      Beijing, China

   =           

&nbs= p;            R= iwei Wang

         &n= bsp;   Tianjin Key Laboratory of Intelligence Computing and Novel=

           = ;  Software Technology

      &n= bsp;      Tianjin University of Technology

 

Month:     = ; October    

Year:    &n= bsp;  2010

 

<= span style=3D'font-family:"Courier New"'>Title:    &nbs= p; A Parallel Radiosity Algorithm for Virtual Reality

=

Booktitle:&n= bsp; 2010 Third International Congress on Image and Signal

 &= nbsp;          Processing (CIS= P 2010))

Volume:     5

Pages: &n= bsp;    2469 -- 2472

 

Publisher:&nbs= p; IEEE Xplore Digital Library

DOI:     &= nbsp;  10.1109/CISP.2010.5647841

 

=

The authors = are invited to contact the author of "Eigenvector Radiosity"=

(2001 MSc thesis, University of British Columbia) to explain why their=

"original technique" (funded by a grant from the Tianji= n Natural Science

Foundation) is simply an extract from the author= 's thesis (which they

neglected to reference in their paper). = ;

    

*****************************= *******************************************

 

Also= available from this site is an abridged version of RADBIB.BIB called<= /o:p>

GITHESIS.BIB. This bibliography includes 339 references to radiosity,

photon mapping, and related global illumination theses -- one new

addition since the 11/02/10 release.

 

Fina= ncial support for the maintenance of these bibliographies is provided<= /o:p>

by byHeart Consultants Limited.

 

Ian Ashdown, P= . Eng., FIES

President

<= span style=3D'font-family:"Courier New"'>byHeart Consultants Limited

http://www.helios32.com

 

= ------=_NextPart_000_0035_01CBFB5E.482D7F70-- ------------=_1302894151-31352-14 Content-Type: text/plain; name="message-footer.txt" Content-Disposition: inline; filename="message-footer.txt" Content-Transfer-Encoding: 8bit ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- ------------=_1302894151-31352-14-- From X-Account-Key: account1 X-UIDL: 000156bd4778b2c7 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: Return-path: Envelope-to: wp@cg.tuwien.ac.at Delivery-date: Mon, 02 Dec 2013 22:02:46 +0100 Received: from tuvok.kom.tuwien.ac.at ([192.35.241.66]) by mail.cg.tuwien.ac.at with esmtp (Exim 4.76) (envelope-from ) id 1Vnadh-0005NE-Rs; Mon, 02 Dec 2013 22:02:45 +0100 Received: from shiva.imag.fr (mx1.imag.fr [IPv6:2001:660:5301:6::5]) by tuvok.kom.tuwien.ac.at (8.14.5/8.14.5) with ESMTP id rB2L2TmR016801 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=FAIL); Mon, 2 Dec 2013 22:02:29 +0100 X-Connecting-Host: mx1.imag.fr [IPv6:2001:660:5301:6::5] X-Connecting-Addr: IPv6:2001:660:5301:6::5 X-Sent-From: globillum-owner@imag.fr Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by shiva.imag.fr (8.13.8/8.13.8) with ESMTP id rB2L2OtP022412 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO); Mon, 2 Dec 2013 22:02:24 +0100 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id rB2L2Qkt017329; Mon, 2 Dec 2013 22:02:26 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id rB2L2O0L017321; Mon, 2 Dec 2013 22:02:24 +0100 Received: from shiva.imag.fr (mx1.imag.fr [129.88.30.5]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id rB2L28Li017283 for ; Mon, 2 Dec 2013 22:02:08 +0100 Received: from server.agi32.com (server.agi32.com [96.127.164.26]) by shiva.imag.fr (8.13.8/8.13.8) with ESMTP id rB2L23DQ022295 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO) for ; Mon, 2 Dec 2013 22:02:05 +0100 Received: from s0106001cc0f76225.vn.shawcable.net ([174.7.220.16]:56612 helo=Earth) by server.agi32.com with esmtpa (Exim 4.80.1) (envelope-from ) id 1VnZov-0001l9-VU for globillum@imag.fr; Mon, 02 Dec 2013 14:10:18 -0600 From: "Ian Ashdown" To: Subject: ANNOUNCE: 13/12/02 Release of RADBIB and GITHESIS Date: Mon, 2 Dec 2013 12:10:19 -0800 Message-ID: <008601ceef9a$868fdbe0$93af93a0$@helios32.com> MIME-Version: 1.0 X-Mailer: Microsoft Outlook 14.0 Thread-index: Ac7vmZuO7YuN3ZSDSkSu2WE3dakWWw== X-AntiAbuse: This header was added to track abuse, please include it with any abuse report X-AntiAbuse: Primary Hostname - server.agi32.com X-AntiAbuse: Original Domain - imag.fr X-AntiAbuse: Originator/Caller UID/GID - [47 12] / [47 12] X-AntiAbuse: Sender Address Domain - helios32.com X-Get-Message-Sender-Via: server.agi32.com: authenticated_id: ian_ashdown@helios32.com X-Greylist: Sender passed SPF test, not delayed by milter-greylist-4.2.7 (tuvok.kom.tuwien.ac.at [IPv6:2001:629:1004:11::25]); Mon, 02 Dec 2013 22:02:30 +0100 (CET) X-Greylist: Sender IP whitelisted, not delayed by milter-greylist-4.0.1 (shiva.imag.fr [129.88.30.5]); Mon, 02 Dec 2013 22:02:24 +0100 (CET) X-Greylist: Delayed for 00:51:43 by milter-greylist-4.0.1 (shiva.imag.fr [129.88.30.5]); Mon, 02 Dec 2013 22:02:05 +0100 (CET) X-IMAG-MailScanner: Found to be clean, Found to be clean X-IMAG-MailScanner-SpamCheck: , X-Loop: globillum@imag.fr X-Sequence: 425 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: multipart/mixed; boundary="----------=_1386018132-32000-6" X-IMAG-MailScanner-Information: Please contact MI2S MIM for more information X-MailScanner-ID: rB2L2OtP022412 X-IMAG-MailScanner-From: globillum-owner@imag.fr MailScanner-NULL-Check: 1386622946.6267@rpqzxJQGp2r7TdPKzNDMsA X-Spam-Status: LOW ; -43 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok.kom.tuwien.ac.at X-Virus-Scanned: by amavisd-new on vc7.kom.tuwien.ac.at This is a multi-part message in MIME format... ------------=_1386018132-32000-6 Content-Type: multipart/alternative; boundary="----=_NextPart_000_0087_01CEEF57.786F0CE0" Content-Language: en-ca This is a multipart message in MIME format. ------=_NextPart_000_0087_01CEEF57.786F0CE0 Content-Type: text/plain; charset="us-ascii" Content-Transfer-Encoding: 7bit ANNOUNCE: 13/12/02 Release of RADBIB and GITHESIS Twenty years of RADBIB and GITHESIS !!! RADBIB is a comprehensive bibliography of radiosity, photon mapping, and related global illumination papers, theses, articles, and books. It currently includes 3,125 references -- 70 new additions since its 13/02/18 release. NOTE: the scope has been expanded to include acoustic radiosity and related topics. This bibliography is available in BibTex format as RADBIB.BIB from: http://www.helios32.com (Resources section) Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 356 references to radiosity, photon mapping, and related global illumination theses -- two new additions since the 13/02/18 release. Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited. Ian Ashdown, P. Eng., FIES President byHeart Consultants Limited http://www.helios32.com CONFIDENTIALITY NOTICE: This entire communication, including without limitation any attachments, is intended for the use of the recipient to which or whom it is addressed, and may contain confidential, personal, and/or privileged information. Please contact us immediately if you are not the intended recipient of this communication, and do not copy, distribute, or take action relying on it. Any communication received in error, or subsequent reply, should be deleted or destroyed. ------=_NextPart_000_0087_01CEEF57.786F0CE0 Content-Type: text/html; charset="us-ascii" Content-Transfer-Encoding: quoted-printable

ANNOUNCE: 13/= 12/02 Release of RADBIB and GITHESIS

 

Twenty years of RADBIB and GITHE= SIS !!!

 

RADBIB is a comprehensive bibliography of radiosity, photon mappi= ng, and related global illumination papers, theses, articles, and books. It= currently includes 3,125 references -- 70 new additions since its 13/02/18= release.

 

NOTE: the scope has been expanded to include acoustic radiosit= y and related topics.

 <= /p>

This bibliography is available in BibTex format as = RADBIB.BIB from:

 

  http://www.helios32.com (Resources section)<= /o:p>

 

Als= o available from this site is an abridged version of RADBIB.BIB called GITH= ESIS.BIB. This bibliography includes 356 references to radiosity, photon ma= pping, and related global illumination theses -- two new additions since th= e 13/02/18 release.

 

Financial support for the maintenance of these biblio= graphies is provided by byHeart Consultants Limited.

 

Ian Ashdown, P. Eng.= , FIES

President

byHeart Consultants Limited

http://www.helios32.com

 

C= ONFIDENTIALITY NOTICE: This entire communication, including without limitat= ion any attachments, is intended for the use of the recipient to which or w= hom it is addressed, and may contain confidential, personal, and/or privile= ged information. Please contact us immediately if you are not the intended = recipient of this communication, and do not copy, distribute, or take actio= n relying on it. Any communication received in error, or subsequent reply, = should be deleted or destroyed.

<= o:p> 

= ------=_NextPart_000_0087_01CEEF57.786F0CE0-- ------------=_1386018132-32000-6 Content-Type: text/plain; name="message-footer.txt" Content-Disposition: inline; filename="message-footer.txt" Content-Transfer-Encoding: 8bit ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- ------------=_1386018132-32000-6-- From X-Account-Key: account1 X-UIDL: 0001699e4778b2c7 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: Return-path: Envelope-to: wp@cg.tuwien.ac.at Delivery-date: Sun, 02 Mar 2014 20:02:52 +0100 Received: from tuvok.kom.tuwien.ac.at ([192.35.241.66]) by mail.cg.tuwien.ac.at with esmtp (Exim 4.76) (envelope-from ) id 1WKBf1-0000sS-St; Sun, 02 Mar 2014 20:02:51 +0100 Received: from rominette.imag.fr (mx2.imag.fr [IPv6:2001:660:5301:59::17]) by tuvok.kom.tuwien.ac.at (8.14.5/8.14.5) with ESMTP id s22J2bQr011927 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=FAIL); Sun, 2 Mar 2014 20:02:37 +0100 X-Connecting-Host: mx2.imag.fr [IPv6:2001:660:5301:59::17] X-Connecting-Addr: IPv6:2001:660:5301:59::17 X-Sent-From: globillum-owner@imag.fr Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by rominette.imag.fr (8.13.8/8.13.8) with ESMTP id s22J2Sdq012766 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO); Sun, 2 Mar 2014 20:02:29 +0100 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id s22J2Vtk009540; Sun, 2 Mar 2014 20:02:31 +0100 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id s22J2V1l009535; Sun, 2 Mar 2014 20:02:31 +0100 Received: from shiva.imag.fr (mx1.imag.fr [129.88.30.5]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id s22J2Dge009493 for ; Sun, 2 Mar 2014 20:02:13 +0100 Received: from server.agi32.com (server.agi32.com [96.127.164.26]) by shiva.imag.fr (8.13.8/8.13.8) with ESMTP id s22J26GI010334 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO) for ; Sun, 2 Mar 2014 20:02:08 +0100 Received: from s0106001cc0f76225.vn.shawcable.net ([174.7.112.119]:50785 helo=Earth) by server.agi32.com with esmtpa (Exim 4.80.1) (envelope-from ) id 1WKB4k-0001Zt-8W for globillum@imag.fr; Sun, 02 Mar 2014 12:25:22 -0600 From: "Ian Ashdown" To: Subject: ANNOUNCE - 14/03/02 Release of RADBIB and GITHESIS Date: Sun, 2 Mar 2014 10:25:26 -0800 Message-ID: <003601cf3644$c97c0d20$5c742760$@helios32.com> MIME-Version: 1.0 X-Mailer: Microsoft Outlook 14.0 Thread-Index: Ac82RFAK8kUCO8GWTxCBRKQbwqQd9Q== X-AntiAbuse: This header was added to track abuse, please include it with any abuse report X-AntiAbuse: Primary Hostname - server.agi32.com X-AntiAbuse: Original Domain - imag.fr X-AntiAbuse: Originator/Caller UID/GID - [47 12] / [47 12] X-AntiAbuse: Sender Address Domain - helios32.com X-Get-Message-Sender-Via: server.agi32.com: authenticated_id: ian_ashdown@helios32.com X-Greylist: Sender passed SPF test, not delayed by milter-greylist-4.2.7 (tuvok.kom.tuwien.ac.at [IPv6:2001:629:1004:11::25]); Sun, 02 Mar 2014 20:02:38 +0100 (CET) X-Greylist: Sender IP whitelisted, not delayed by milter-greylist-4.2.2 (rominette.imag.fr [129.88.30.17]); Sun, 02 Mar 2014 20:02:30 +0100 (CET) X-Greylist: Delayed for 00:36:42 by milter-greylist-4.0.1 (shiva.imag.fr [129.88.30.5]); Sun, 02 Mar 2014 20:02:09 +0100 (CET) X-IMAG-MailScanner: Found to be clean, Found to be clean X-IMAG-MailScanner-SpamCheck: , X-Loop: globillum@imag.fr X-Sequence: 426 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: multipart/mixed; boundary="----------=_1393786936-28184-0" X-IMAG-MailScanner-Information: Please contact MI2S MIM for more information X-MailScanner-ID: s22J2Sdq012766 X-IMAG-MailScanner-From: globillum-owner@imag.fr MailScanner-NULL-Check: 1394391754.09341@7UTud52Xo+e8Ydu6fcg05Q X-Spam-Status: LOW ; -43 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok.kom.tuwien.ac.at X-Virus-Scanned: by amavisd-new on vc9.kom.tuwien.ac.at This is a multi-part message in MIME format... ------------=_1393786936-28184-0 Content-Type: multipart/alternative; boundary="----=_NextPart_000_0037_01CF3601.BB594250" Content-Language: en-ca This is a multipart message in MIME format. ------=_NextPart_000_0037_01CF3601.BB594250 Content-Type: text/plain; charset="us-ascii" Content-Transfer-Encoding: 7bit ANNOUNCE: 14/03/02 Release of RADBIB and GITHESIS Celebrating twenty years . RADBIB is a comprehensive bibliography of radiosity, photon mapping, and related global illumination papers, theses, articles, and books. It currently includes 3,152 references -- 27 new additions since its 13/12/02 release. This bibliography is available in BibTex format as RADBIB.BIB from: http://www.helios32.com (Resources section) Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 360 references to radiosity, photon mapping, and related global illumination theses -- four new additions since the 13/12/02 release. Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited. Ian Ashdown, P. Eng., FIES President byHeart Consultants Limited http://www.helios32.com CONFIDENTIALITY NOTICE: This entire communication, including without limitation any attachments, is intended for the use of the recipient to which or whom it is addressed, and may contain confidential, personal, and/or privileged information. Please contact us immediately if you are not the intended recipient of this communication, and do not copy, distribute, or take action relying on it. Any communication received in error, or subsequent reply, should be deleted or destroyed. ------=_NextPart_000_0037_01CF3601.BB594250 Content-Type: text/html; charset="us-ascii" Content-Transfer-Encoding: quoted-printable

ANNOUNCE: 14/= 03/02 Release of RADBIB and GITHESIS

 

Celebrating twenty years …=

 

RADBIB is a comprehensive bibliography of radiosity, photon mapping, and= related global illumination papers, theses, articles, and books. It curren= tly includes 3,152 references -- 27 new additions since its 13/12/02 releas= e.

 

This bibliography is available in BibTex format as RADBIB.BIB from:

 

=   http://www.helios32.com (Res= ources section)

 

Also available from this site is an abridged version of R= ADBIB.BIB called GITHESIS.BIB. This bibliography includes 360 references to= radiosity, photon mapping, and related global illumination theses -- four = new additions since the 13/12/02 release.

 

Financial support for the maint= enance of these bibliographies is provided by byHeart Consultants Limited.<= o:p>

 

Ian Ashdown, P. Eng., FIES

President

byHeart Consultants Limited

http://www.helio= s32.com

 

CONFIDENTIALITY NOTICE: This entire communication, incl= uding without limitation any attachments, is intended for the use of the re= cipient to which or whom it is addressed, and may contain confidential, per= sonal, and/or privileged information. Please contact us immediately if you = are not the intended recipient of this communication, and do not copy, dist= ribute, or take action relying on it. Any communication received in error, = or subsequent reply, should be deleted or destroyed.

<= p class=3DMsoNormal> 

= ------=_NextPart_000_0037_01CF3601.BB594250-- ------------=_1393786936-28184-0 Content-Type: text/plain; name="message-footer.txt" Content-Disposition: inline; filename="message-footer.txt" Content-Transfer-Encoding: 8bit ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- ------------=_1393786936-28184-0-- From X-Account-Key: account1 X-UIDL: 000189b14778b2c7 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: Return-path: Envelope-to: wp@cg.tuwien.ac.at Delivery-date: Mon, 28 Jul 2014 17:05:26 +0200 Received: from tuvok.kom.tuwien.ac.at ([192.35.241.66]) by mail.cg.tuwien.ac.at with esmtp (Exim 4.76) (envelope-from ) id 1XBmUP-0002J2-7f; Mon, 28 Jul 2014 17:05:25 +0200 Received: from shiva.imag.fr (mx1.imag.fr [IPv6:2001:660:5301:6::5]) by tuvok.kom.tuwien.ac.at (8.14.5/8.14.5) with ESMTP id s6SF5Crc024350 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=OK); Mon, 28 Jul 2014 17:05:13 +0200 X-Connecting-Host: mx1.imag.fr [IPv6:2001:660:5301:6::5] X-Connecting-Addr: IPv6:2001:660:5301:6::5 X-Sent-From: globillum-owner@imag.fr Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by shiva.imag.fr (8.13.8/8.13.8) with ESMTP id s6SF51bc005943 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO); Mon, 28 Jul 2014 17:05:03 +0200 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id s6SF53Dp018245; Mon, 28 Jul 2014 17:05:03 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id s6SF5304018240; Mon, 28 Jul 2014 17:05:03 +0200 Received: from shiva.imag.fr (mx1.imag.fr [129.88.30.5]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id s6SF4Bfs018189 for ; Mon, 28 Jul 2014 17:04:11 +0200 Received: from server.agi32.com (server.agi32.com [96.127.164.26]) by shiva.imag.fr (8.13.8/8.13.8) with ESMTP id s6SF43Zd005515 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO) for ; Mon, 28 Jul 2014 17:04:05 +0200 Received: from s01060018e7f1256d.vn.shawcable.net ([174.7.125.60]:52359 helo=Earth) by server.agi32.com with esmtpa (Exim 4.80.1) (envelope-from ) id 1XBm47-0005eQ-Pd for globillum@imag.fr; Mon, 28 Jul 2014 09:38:16 -0500 From: "Ian Ashdown" To: Subject: ANNOUNCE: 14/07/28 Release of RADBIB and GITHESIS Date: Mon, 28 Jul 2014 07:38:16 -0700 Message-ID: <006801cfaa71$91e2f3f0$b5a8dbd0$@helios32.com> MIME-Version: 1.0 X-Mailer: Microsoft Outlook 14.0 Thread-Index: Ac+qcX21NYkm8ra/QWi6zbkcK88KmA== X-AntiAbuse: This header was added to track abuse, please include it with any abuse report X-AntiAbuse: Primary Hostname - server.agi32.com X-AntiAbuse: Original Domain - imag.fr X-AntiAbuse: Originator/Caller UID/GID - [47 12] / [47 12] X-AntiAbuse: Sender Address Domain - helios32.com X-Get-Message-Sender-Via: server.agi32.com: authenticated_id: ian_ashdown@helios32.com X-Greylist: Sender succeeded STARTTLS authentication, not delayed by milter-greylist-4.2.7 (tuvok.kom.tuwien.ac.at [IPv6:2001:629:1004:11::25]); Mon, 28 Jul 2014 17:05:13 +0200 (CEST) X-Greylist: Sender IP whitelisted, not delayed by milter-greylist-4.0.1 (shiva.imag.fr [129.88.30.5]); Mon, 28 Jul 2014 17:05:06 +0200 (CEST) X-Greylist: Delayed for 00:25:46 by milter-greylist-4.0.1 (shiva.imag.fr [129.88.30.5]); Mon, 28 Jul 2014 17:04:05 +0200 (CEST) X-IMAG-MailScanner: Found to be clean, Found to be clean X-IMAG-MailScanner-SpamCheck: , X-Loop: globillum@imag.fr X-Sequence: 429 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: multipart/mixed; boundary="----------=_1406559854-9913-0" X-IMAG-MailScanner-Information: Please contact MI2S MIM for more information X-MailScanner-ID: s6SF51bc005943 X-IMAG-MailScanner-From: globillum-owner@imag.fr MailScanner-NULL-Check: 1407164710.19418@MnAs2XkACOFkeQZdhLRo+w X-Spam-Status: LOW ; -24 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok.kom.tuwien.ac.at X-Virus-Scanned: by amavisd-new on vc7.kom.tuwien.ac.at This is a multi-part message in MIME format... ------------=_1406559854-9913-0 Content-Type: multipart/alternative; boundary="----=_NextPart_000_0069_01CFAA36.E5855470" Content-Language: en-ca This is a multipart message in MIME format. ------=_NextPart_000_0069_01CFAA36.E5855470 Content-Type: text/plain; charset="us-ascii" Content-Transfer-Encoding: 7bit ANNOUNCE: 14/07/28 Release of RADBIB and GITHESIS RADBIB is a comprehensive bibliography of radiosity, photon mapping, and related global illumination papers, theses, articles, and books. It currently includes 3,183 references -- 18 new additions since its 14/05/21 release. This bibliography is available in BibTex format as RADBIB.BIB from: http://www.helios32.com (Resources section) Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 365 references to radiosity, photon mapping, and related global illumination theses -- two new additions since the 14/05/21 release. Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited. Ian Ashdown, P. Eng., FIES President byHeart Consultants Limited http://www.helios32.com CONFIDENTIALITY NOTICE: This entire communication, including without limitation any attachments, is intended for the use of the recipient to which or whom it is addressed, and may contain confidential, personal, and/or privileged information. Please contact us immediately if you are not the intended recipient of this communication, and do not copy, distribute, or take action relying on it. Any communication received in error, or subsequent reply, should be deleted or destroyed. ------=_NextPart_000_0069_01CFAA36.E5855470 Content-Type: text/html; charset="us-ascii" Content-Transfer-Encoding: quoted-printable

ANNOUNCE: 14/= 07/28 Release of RADBIB and GITHESIS

 

RADBIB is a comprehensive biblio= graphy of radiosity, photon mapping, and related global illumination papers= , theses, articles, and books. It currently includes 3,183 references -- 18= new additions since its 14/05/21 release.

 

This bibliography is available= in BibTex format as RADBIB.BIB from:

 

  http://www.helios32.com (Res= ources section)

 

Also available from this site is an abridged version of R= ADBIB.BIB called GITHESIS.BIB. This bibliography includes 365 references to= radiosity, photon mapping, and related global illumination theses -- two n= ew additions since the 14/05/21 release.

 

Financial support for the mainte= nance of these bibliographies is provided by byHeart Consultants Limited.

 

Ian Ashdown, P. Eng., FIES

President

byHeart Consultants Limited

=

http://www.helios= 32.com

 

CONFIDENTIALITY NOTICE: This entire communication, inclu= ding without limitation any attachments, is intended for the use of the rec= ipient to which or whom it is addressed, and may contain confidential, pers= onal, and/or privileged information. Please contact us immediately if you a= re not the intended recipient of this communication, and do not copy, distr= ibute, or take action relying on it. Any communication received in error, o= r subsequent reply, should be deleted or destroyed.

 

= ------=_NextPart_000_0069_01CFAA36.E5855470-- ------------=_1406559854-9913-0 Content-Type: text/plain; name="message-footer.txt" Content-Disposition: inline; filename="message-footer.txt" Content-Transfer-Encoding: 8bit ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- ------------=_1406559854-9913-0-- From X-Account-Key: account1 X-UIDL: 000190454778b2c7 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: Return-path: Envelope-to: wp@cg.tuwien.ac.at Delivery-date: Tue, 09 Sep 2014 11:36:51 +0200 Received: from tuvok.kom.tuwien.ac.at ([192.35.241.66]) by mail.cg.tuwien.ac.at with esmtp (Exim 4.76) (envelope-from ) id 1XRHr0-00066E-Uq; Tue, 09 Sep 2014 11:36:51 +0200 Received: from rominette.imag.fr (mx2.imag.fr [IPv6:2001:660:5301:59::17]) by tuvok.kom.tuwien.ac.at (8.14.5/8.14.5) with ESMTP id s899aanh011776 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=OK); Tue, 9 Sep 2014 11:36:37 +0200 X-Connecting-Host: mx2.imag.fr [IPv6:2001:660:5301:59::17] X-Connecting-Addr: IPv6:2001:660:5301:59::17 X-Sent-From: globillum-owner@imag.fr Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by rominette.imag.fr (8.13.8/8.13.8) with ESMTP id s899aAU0016949 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO); Tue, 9 Sep 2014 11:36:10 +0200 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id s899aBaj020416; Tue, 9 Sep 2014 11:36:11 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id s899aB9h020411; Tue, 9 Sep 2014 11:36:11 +0200 Received: from rominette.imag.fr (mx2.imag.fr [129.88.30.17]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id s899ZIIg020368 for ; Tue, 9 Sep 2014 11:35:18 +0200 Received: from mail.cg.tuwien.ac.at (mail.cg.tuwien.ac.at [128.131.166.76]) by rominette.imag.fr (8.13.8/8.13.8) with ESMTP id s899ZBoX016535 (version=TLSv1/SSLv3 cipher=AES256-SHA bits=256 verify=NO) for ; Tue, 9 Sep 2014 11:35:13 +0200 Received: from e221-059.eduroam.tuwien.ac.at ([128.131.221.59]) by mail.cg.tuwien.ac.at with esmtpsa (TLS1.0:DHE_RSA_AES_128_CBC_SHA1:16) (Exim 4.76) (envelope-from ) id 1XRHJI-0004uE-I2; Tue, 09 Sep 2014 11:02:00 +0200 Message-ID: <540EC203.3070706@cg.tuwien.ac.at> Date: Tue, 09 Sep 2014 11:01:55 +0200 From: Werner Purgathofer User-Agent: Mozilla/5.0 (Windows NT 6.1; WOW64; rv:24.0) Gecko/20100101 Thunderbird/24.6.0 MIME-Version: 1.0 To: Globillum CC: Michael Wimmer Subject: EG 2015: Call for Full Papers References: <004601cfb134$016cb170$04461450$@eg.org> In-Reply-To: <004601cfb134$016cb170$04461450$@eg.org> X-Greylist: Sender succeeded STARTTLS authentication, not delayed by milter-greylist-4.2.7 (tuvok.kom.tuwien.ac.at [IPv6:2001:629:1004:11::25]); Tue, 09 Sep 2014 11:36:38 +0200 (CEST) X-Greylist: Sender IP whitelisted, not delayed by milter-greylist-4.2.2 (rominette.imag.fr [129.88.30.17]); Tue, 09 Sep 2014 11:36:11 +0200 (CEST) X-Greylist: Delayed for 00:33:11 by milter-greylist-4.2.2 (rominette.imag.fr [129.88.30.17]); Tue, 09 Sep 2014 11:35:13 +0200 (CEST) X-IMAG-MailScanner: Found to be clean, Found to be clean X-IMAG-MailScanner-SpamCheck: , X-Loop: globillum@imag.fr X-Sequence: 430 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: multipart/mixed; boundary="----------=_1410255322-13996-2" X-IMAG-MailScanner-Information: Please contact MI2S MIM for more information X-MailScanner-ID: s899aAU0016949 X-IMAG-MailScanner-From: globillum-owner@imag.fr MailScanner-NULL-Check: 1410860172.70176@DtL7SUw3ipQeZwAtvHsk+A X-Spam-Status: LOW ; -15 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok.kom.tuwien.ac.at X-Virus-Scanned: by amavisd-new on vc8.kom.tuwien.ac.at This is a multi-part message in MIME format... ------------=_1410255322-13996-2 Content-Type: multipart/alternative; boundary="------------050407080602010505070400" This is a multi-part message in MIME format. --------------050407080602010505070400 Content-Type: text/plain; charset=ISO-8859-1; format=flowed Content-Transfer-Encoding: quoted-printable X-MIME-Autoconverted: from 8bit to quoted-printable by tuvok.kom.tuwien.ac.at id s899aanh011776 =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D Apologies if you receive multiple copies of this Call for Papers Please forward this mail to anyone interested =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D Eurographics 2015:Call for Full Papers ( http://www.eurographics2015.ch/ ) The Eurographics 2015 Technical Papers programme will showcase=20 innovative research in Computer Graphics and related areas. We invite=20 submissions of new ideas, and encourage all forms of research creativity=20 and originality. We are interested in practice, experience, novel=20 applications, technological or theoretical papers, with the ambition of=20 setting the standard in the field and stimulating future trends.=AD=AD=AD Accepted papers will be presented at *Eurographics 2015* and published=20 in a special issue of the Eurographics journal *Computer Graphics Forum*=20 .=20 Therefore, submissions will undergo a two-step review process. We=20 encourage submissions from all areas related to computer graphics such=20 as rendering, modeling, animation, visualization, virtual reality,=20 computer vision, imaging, computer-aided fabrication, human-computer=20 interaction, and related disciplines. Submission Dates A preliminary abstract is due by 23:59 GMT, Friday, *September 19,=20 2014*, and the full paper deadline is 23:59 GMT, Friday, *September 26,=20 2014*. Note that a full paper can only be submitted if an abstract has=20 been submitted by the abstract deadline. ------------------------------------------------------------------------ Submission Electronic submission of all papers is mandatory and will be conducted=20 using the Submission and Review Management=20 (SRMv2) system. Papers=20 must be written in English, they must be anonymized, and must be=20 formatted according to the Eurographics Computer Graphics Forum=20 publication guidelines. The publication guidelines and LaTeX templates=20 are available on SRMv2=20 . Accepted=20 papers must be presented in English at Eurographics 2015. This event=20 uses a double-blind reviewing approach, so please remove all personal=20 data (such as authors, affiliations, etc.) from your submission.=20 Reviewers are asked to keep confidential all materials sent to them for=20 evaluation. Note that this year, there is no arbitrary maximum length imposed on=20 papers. Papers should be as long as they need to be, but not longer. If=20 a submission is perceived as repetitive or unnecessarily long, it might=20 be ranked lower by reviewers than a concisely written submission. Double Submission Policy Authors are required to include a declaration that they have not=20 previously published the scientific contribution claimed in their paper,=20 nor has it been submitted to or is currently under review in any other=20 conference or journal before or during the Eurographics 2015 Technical=20 Papers review period. Any paper that does not adhere to these=20 requirements will be rejected without review. Re-Submitted Material For papers that have previously been reviewed for other venues and have=20 been rejected or withdrawn, the authors are encouraged to provide a=20 cover letter to describe the history of the paper (however, this does=20 not imply reviewer continuity). This cover letter can also answer the=20 comments made in the previous reviews, by either listing the changes=20 that were made to comply with them, or discussing/rebutting/clarifying=20 some elements if need be. Though not mandatory, this procedure is=20 strongly recommended. The cover letter has to be submitted through the=20 SRM as an 'Additional Attachment' (last section of the SRM upload form). Rebuttal, Notification, Publication & Prizes * The reviews will be made available to the authors on *November 13, 2014*. A rebuttal period from *November 13 to November 18, 2014* will allow authors to submit a brief document to address any factual errors or clarify other issues raised in the reviews. * The date for notification of the results of the first round of the review process is *December 5, 2014*. * Revised versions of the papers conditionally accepted in the first round must be submitted by *December 31, 2014*. The final notification of the outcome of the second reviewing round will be made on *January 14, 2015*. The camera-ready version of accepted papers will be due on *January 28, 2015*. * From all accepted and presented papers, an international jury will select the best papers. The best paper will receive the *G=FCnter Enderle Award, *including a cash prize of 1000 Euros, presented at Eurographics 2015. For any question concerning full paper submissions please contact the=20 papers program co-chairs: chairs-eg2015@eg.org Full Papers Chairs Olga Sorkine-Hornung , ETH Zurich, Switzerla= nd Michael Wimmer , Vienna University of=20 Technology, Austria --------------050407080602010505070400 Content-Type: text/html; charset=ISO-8859-1 Content-Transfer-Encoding: 7bit
=======================================================================
Apologies if you receive multiple copies of this Call for Papers
Please forward this mail to anyone interested
=======================================================================

Eurographics 2015: Call for Full Papers

( http://www.eurographics2015.ch/ )

The Eurographics 2015 Technical Papers programme will showcase innovative research in Computer Graphics and related areas. We invite submissions of new ideas, and encourage all forms of research creativity and originality. We are interested in practice, experience, novel applications, technological or theoretical papers, with the ambition of setting the standard in the field and stimulating future trends.­­­

Accepted papers will be presented at Eurographics 2015 and published in a special issue of the Eurographics journal Computer Graphics Forum. Therefore, submissions will undergo a two-step review process. We encourage submissions from all areas related to computer graphics such as rendering, modeling, animation, visualization, virtual reality, computer vision, imaging, computer-aided fabrication, human-computer interaction, and related disciplines. 

Submission Dates

A preliminary abstract is due by 23:59 GMT, Friday, September 19, 2014, and the full paper deadline is 23:59 GMT, Friday, September 26, 2014. Note that a full paper can only be submitted if an abstract has been submitted by the abstract deadline.

Submission

Electronic submission of all papers is mandatory and will be conducted using the Submission and Review Management (SRMv2) system. Papers must be written in English, they must be anonymized, and must be formatted according to the Eurographics Computer Graphics Forum publication guidelines. The publication guidelines and LaTeX templates are available on SRMv2. Accepted papers must be presented in English at Eurographics 2015. This event uses a double-blind reviewing approach, so please remove all personal data (such as authors, affiliations, etc.) from your submission. Reviewers are asked to keep confidential all materials sent to them for evaluation.

Note that this year, there is no arbitrary maximum length imposed on papers. Papers should be as long as they need to be, but not longer. If a submission is perceived as repetitive or unnecessarily long, it might be ranked lower by reviewers than a concisely written submission. 

Double Submission Policy

Authors are required to include a declaration that they have not previously published the scientific contribution claimed in their paper, nor has it been submitted to or is currently under review in any other conference or journal before or during the Eurographics 2015 Technical Papers review period. Any paper that does not adhere to these requirements will be rejected without review. 

Re-Submitted Material

For papers that have previously been reviewed for other venues and have been rejected or withdrawn, the authors are encouraged to provide a cover letter to describe the history of the paper (however, this does not imply reviewer continuity). This cover letter can also answer the comments made in the previous reviews, by either listing the changes that were made to comply with them, or discussing/rebutting/clarifying some elements if need be. Though not mandatory, this procedure is strongly recommended. The cover letter has to be submitted through the SRM as an ‘Additional Attachment’ (last section of the SRM upload form). 

Rebuttal, Notification, Publication & Prizes

  • The reviews will be made available to the authors on November 13, 2014. A rebuttal period from November 13 to November 18, 2014 will allow authors to submit a brief document to address any factual errors or clarify other issues raised in the reviews.
  • The date for notification of the results of the first round of the review process is December 5, 2014.
  • Revised versions of the papers conditionally accepted in the first round must be submitted by December 31, 2014. The final notification of the outcome of the second reviewing round will be made on January 14, 2015. The camera-ready version of accepted papers will be due on January 28, 2015.
  • From all accepted and presented papers, an international jury will select the best papers. The best paper will receive the Günter Enderle Award, including a cash prize of 1000 Euros, presented at Eurographics 2015.

For any question concerning full paper submissions please contact the papers program co-chairs:
chairs-eg2015@eg.org

Full Papers Chairs

Olga Sorkine-Hornung, ETH Zurich, Switzerland
Michael Wimmer, Vienna University of Technology, Austria  

 

--------------050407080602010505070400-- ------------=_1410255322-13996-2 Content-Type: text/plain; name="message-footer.txt" Content-Disposition: inline; filename="message-footer.txt" Content-Transfer-Encoding: 8bit ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- ------------=_1410255322-13996-2-- From X-Account-Key: account1 X-UIDL: 0001dfee4778b2c7 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: Return-path: Envelope-to: wp@cg.tuwien.ac.at Delivery-date: Wed, 16 Sep 2015 02:32:25 +0200 Received: from tuvok.kom.tuwien.ac.at ([192.35.241.66]) by mail.cg.tuwien.ac.at with esmtp (Exim 4.76) (envelope-from ) id 1Zc0e9-0002Jq-6V; Wed, 16 Sep 2015 02:32:25 +0200 Received: from rominette.imag.fr (mx2.imag.fr [IPv6:2001:660:5301:59::17]) by tuvok.kom.tuwien.ac.at (8.14.5/8.14.5) with ESMTP id t8G0WB6o027210 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES128-SHA bits=128 verify=OK); Wed, 16 Sep 2015 02:32:12 +0200 X-Connecting-Host: mx2.imag.fr [IPv6:2001:660:5301:59::17] X-Connecting-Addr: IPv6:2001:660:5301:59::17 X-Sent-From: globillum-owner@imag.fr Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by rominette.imag.fr (8.13.8/8.13.8) with ESMTP id t8G0Vuum003488 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES128-SHA bits=128 verify=NO); Wed, 16 Sep 2015 02:31:57 +0200 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id t8G0W00W009747; Wed, 16 Sep 2015 02:32:00 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id t8G0Vxje009742; Wed, 16 Sep 2015 02:31:59 +0200 Received: from shiva.imag.fr (mx1.imag.fr [129.88.30.5]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id t8G0Vdkm009700 for ; Wed, 16 Sep 2015 02:31:39 +0200 Received: from mxb1-1.relay.renater.fr (mxb1-1.relay.renater.fr [194.214.201.8]) by shiva.imag.fr (8.13.8/8.13.8) with ESMTP id t8G0VZ9a030046 for ; Wed, 16 Sep 2015 02:31:36 +0200 Received: from server.agi32.com (server.agi32.com [96.127.164.26]) by mxb1-1.relay.renater.fr (asm) with ESMTP id 8582060000D for ; Wed, 16 Sep 2015 02:31:37 +0200 (CEST) Received: from s010600224d80691f.vn.shawcable.net ([174.7.100.71]:54549 helo=Earth) by server.agi32.com with esmtpa (Exim 4.85) (envelope-from ) id 1Zc0dK-0006qR-Ig for globillum@imag.fr; Tue, 15 Sep 2015 19:31:34 -0500 From: "Ian Ashdown" To: Subject: ANNOUNCE: 15/09/15 Release of RADBIB and GITHESIS Date: Tue, 15 Sep 2015 17:31:37 -0700 Message-ID: <051c01d0f017$0d0e4f20$272aed60$@helios32.com> MIME-Version: 1.0 X-Mailer: Microsoft Outlook 14.0 Thread-Index: AdDwFuzS6fgWQxEsTiGcxc55qEotKQ== X-AntiAbuse: This header was added to track abuse, please include it with any abuse report X-AntiAbuse: Primary Hostname - server.agi32.com X-AntiAbuse: Original Domain - imag.fr X-AntiAbuse: Originator/Caller UID/GID - [47 12] / [47 12] X-AntiAbuse: Sender Address Domain - helios32.com X-Get-Message-Sender-Via: server.agi32.com: authenticated_id: ian_ashdown@helios32.com X-Original-Source-IP: 96.127.164.26 X-Bizanga: IMP - mxb1-1.relay.renater.fr X-Renater-SpamState: 0 X-Renater-SpamScore: 0 X-Renater-SpamCause: gggruggvucftvghtrhhoucdtuddrfeekgedrvdekgdegtdcutefuodetggdotefrucfrrhhofhhilhgvmecutffgpfetvffgtfdpggftfghnshhusghstghrihgsvgenuceurghilhhouhhtmecufedttdenucenucfjughrpefhvffufffkgggtofhtsegrtdhgpedvtddvnecuhfhrohhmpedfkfgrnhcutehshhguohifnhdfuceoihgrnhgprghshhguohifnheshhgvlhhiohhsfedvrdgtohhmqeenucffohhmrghinhephhgvlhhiohhsfedvrdgtohhm X-Renater-ServerName: mxb1-1.relay.renater.fr X-Greylist: Sender succeeded STARTTLS authentication, not delayed by milter-greylist-4.2.7 (tuvok.kom.tuwien.ac.at [IPv6:2001:629:1004:11::25]); Wed, 16 Sep 2015 02:32:14 +0200 (CEST) X-Greylist: Sender IP whitelisted, not delayed by milter-greylist-4.2.2 (rominette.imag.fr [129.88.30.17]); Wed, 16 Sep 2015 02:31:57 +0200 (CEST) X-Greylist: Sender IP whitelisted, not delayed by milter-greylist-4.0.1 (shiva.imag.fr [129.88.30.5]); Wed, 16 Sep 2015 02:31:36 +0200 (CEST) X-Loop: globillum@imag.fr X-Sequence: 434 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: multipart/mixed; boundary="----------=_1442363503-1849-3" X-IMAG-MailScanner-Information: Please contact MI2S MIM for more information X-MailScanner-ID: t8G0Vuum003488 X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-SpamCheck: X-IMAG-MailScanner-From: globillum-owner@imag.fr MailScanner-NULL-Check: 1442968317.57999@GW5g1PDCx8orS39A83FZEw X-Spam-Status: LOW ; -8 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok.kom.tuwien.ac.at X-Virus-Scanned: by amavisd-new on vc9.kom.tuwien.ac.at This is a multi-part message in MIME format... ------------=_1442363503-1849-3 Content-Type: multipart/alternative; boundary="----=_NextPart_000_051D_01D0EFDC.60B08890" Content-Language: en-ca This is a multipart message in MIME format. ------=_NextPart_000_051D_01D0EFDC.60B08890 Content-Type: text/plain; charset="us-ascii" Content-Transfer-Encoding: 7bit ANNOUNCE: 15/09/15 Release of RADBIB and GITHESIS RADBIB is a comprehensive bibliography of radiosity, photon mapping, and related global illumination papers, theses, articles, and books. It currently includes 3,290 references -- 70 new additions since its 14/12/27 release. This bibliography is available in BibTex format as RADBIB.BIB from: http://www.helios32.com (Resources section) Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 375 references to radiosity, photon mapping, and related global illumination theses -- six new additions since the 14/12/27 release. Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited. Ian Ashdown, P. Eng., FIES President byHeart Consultants Limited http://www.helios32.com Ian Ashdown, P. Eng., FIES President byHeart Consultants Limited http://www.helios32.com CONFIDENTIALITY NOTICE: This entire communication, including without limitation any attachments, is intended for the use of the recipient to which or whom it is addressed, and may contain confidential, personal, and/or privileged information. Please contact us immediately if you are not the intended recipient of this communication, and do not copy, distribute, or take action relying on it. Any communication received in error, or subsequent reply, should be deleted or destroyed. ------=_NextPart_000_051D_01D0EFDC.60B08890 Content-Type: text/html; charset="us-ascii" Content-Transfer-Encoding: quoted-printable

ANNOUNCE: 15/= 09/15 Release of RADBIB and GITHESIS

 

RADBIB is a comprehensive biblio= graphy of radiosity, photon mapping, and related global illumination papers= , theses, articles, and books. It currently includes 3,290 references -- 70= new additions since its 14/12/27 release.

 

This bibliography is available= in BibTex format as RADBIB.BIB from:

 

  http://www.helios32.com (Res= ources section)

 

Also available from this site is an abridged version of R= ADBIB.BIB called GITHESIS.BIB. This bibliography includes 375 references to= radiosity, photon mapping, and related global illumination theses -- six n= ew additions since the 14/12/27 release.

 

Financial support for the mainte= nance of these bibliographies is provided by byHeart Consultants Limited.

 

Ian Ashdown, P. Eng., FIES

President

byHeart Consultants Limited

=

http://www.helios32.com

 

Ian Ashdown, P. Eng., FIES

President

byHeart Consultants Limited

http://www.helios32.com

 

CONFIDENT= IALITY NOTICE: This entire communication, including without limitation any = attachments, is intended for the use of the recipient to which or whom it i= s addressed, and may contain confidential, personal, and/or privileged info= rmation. Please contact us immediately if you are not the intended recipien= t of this communication, and do not copy, distribute, or take action relyin= g on it. Any communication received in error, or subsequent reply, should b= e deleted or destroyed.

&nbs= p;

= ------=_NextPart_000_051D_01D0EFDC.60B08890-- ------------=_1442363503-1849-3 Content-Type: text/plain; name="message-footer.txt" Content-Disposition: inline; filename="message-footer.txt" Content-Transfer-Encoding: 8bit ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- ------------=_1442363503-1849-3-- From X-Account-Key: account1 X-UIDL: 0001e7594778b2c7 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: Return-path: Envelope-to: wp@cg.tuwien.ac.at Delivery-date: Mon, 19 Oct 2015 12:43:37 +0200 Received: from neelix.kom.tuwien.ac.at ([192.35.241.67]) by mail.cg.tuwien.ac.at with esmtp (Exim 4.76) (envelope-from ) id 1Zo7uj-0002MM-CT; Mon, 19 Oct 2015 12:43:37 +0200 Received: from shiva.imag.fr (mx1.imag.fr [IPv6:2001:660:5301:6::5]) by neelix.kom.tuwien.ac.at (8.14.5/8.14.5) with ESMTP id t9JAhUYY029841 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES128-SHA bits=128 verify=OK); Mon, 19 Oct 2015 12:43:30 +0200 X-Connecting-Host: mx1.imag.fr [IPv6:2001:660:5301:6::5] X-Connecting-Addr: IPv6:2001:660:5301:6::5 X-Sent-From: globillum-owner@imag.fr Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by shiva.imag.fr (8.13.8/8.13.8) with ESMTP id t9JAhMrM028361 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES128-SHA bits=128 verify=NO); Mon, 19 Oct 2015 12:43:23 +0200 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id t9JAhNXh022524; Mon, 19 Oct 2015 12:43:24 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id t9JAhNrh022519; Mon, 19 Oct 2015 12:43:23 +0200 Received: from shiva.imag.fr (mx1.imag.fr [129.88.30.5]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id t9JAh4xG022477 for ; Mon, 19 Oct 2015 12:43:04 +0200 Received: from mxb1-1.relay.renater.fr (mxb1-1.relay.renater.fr [194.214.201.8]) by shiva.imag.fr (8.13.8/8.13.8) with ESMTP id t9JAh1UE028262 for ; Mon, 19 Oct 2015 12:43:02 +0200 Received: from mail.cg.tuwien.ac.at (mail.cg.tuwien.ac.at [128.131.166.76]) by mxb1-1.relay.renater.fr (asm) with ESMTP id 0F594600230 for ; Mon, 19 Oct 2015 12:43:02 +0200 (CEST) Received: from pool119.cg.tuwien.ac.at ([128.131.166.119]) by mail.cg.tuwien.ac.at with esmtpsa (TLS1.0:DHE_RSA_AES_128_CBC_SHA1:16) (Exim 4.76) (envelope-from ) id 1Zo7u8-0002Lw-UU; Mon, 19 Oct 2015 12:43:01 +0200 From: Werner Purgathofer Subject: 10 PhD positions at the Center for Geometry and Computational Design, TU Wien To: Globillum References: <561E2FB7.7020006@gmail.com> Cc: Michael Wimmer Message-ID: <5624C946.3060200@cg.tuwien.ac.at> Date: Mon, 19 Oct 2015 12:43:18 +0200 User-Agent: Mozilla/5.0 (Windows NT 6.3; WOW64; rv:38.0) Gecko/20100101 Thunderbird/38.3.0 MIME-Version: 1.0 In-Reply-To: <561E2FB7.7020006@gmail.com> X-Original-Source-IP: 128.131.166.76 X-Bizanga: IMP - mxb1-1.relay.renater.fr X-Renater-SpamState: 0 X-Renater-SpamScore: -100 X-Renater-SpamCause: gggruggvucftvghtrhhoucdtuddrfeekgedrleeigdeffecutefuodetggdotefrucfrrhhofhhilhgvmecutffgpfetvffgtfdpggftfghnshhusghstghrihgsvgenuceurghilhhouhhtmecufedttdenucesvcftvggtihhpihgvnhhtshculddquddttddmnecujfgurhephffuvfhfkffffgggjggtgfesthekrgdttdefjeenucfhrhhomhephggvrhhnvghrucfruhhrghgrthhhohhfvghruceofihpsegtghdrthhufihivghnrdgrtgdrrghtqeenucffohhmrghinhepthhufihivghnrdgrtgdrrghtnecurfgrrhgrmhepmhhouggvpehsmhhtphdphhgvlhhopehmrghilhdrtghgrdhtuhifihgvnhdrrggtrdgrthdpihhnvghtpeduvdekrddufedurdduieeirdejiedpmhgrihhlfhhrohhmpeifphestghgrdhtuhifihgvnhdrrggtrdgrthdprhgtphhtthhopehglhhosghilhhluhhmsehimhgrghdrfhhr X-Renater-ServerName: mxb1-1.relay.renater.fr X-Greylist: Sender succeeded STARTTLS authentication, not delayed by milter-greylist-4.2.7 (neelix.kom.tuwien.ac.at [IPv6:2001:629:1004:11::1:25]); Mon, 19 Oct 2015 12:43:33 +0200 (CEST) X-Greylist: Sender IP whitelisted, not delayed by milter-greylist-4.0.1 (shiva.imag.fr [129.88.30.5]); Mon, 19 Oct 2015 12:43:25 +0200 (CEST) X-Greylist: Sender IP whitelisted, not delayed by milter-greylist-4.0.1 (shiva.imag.fr [129.88.30.5]); Mon, 19 Oct 2015 12:43:02 +0200 (CEST) X-Loop: globillum@imag.fr X-Sequence: 436 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Content-type: multipart/mixed; boundary="----------=_1445251385-19989-2" X-IMAG-MailScanner-Information: Please contact MI2S MIM for more information X-MailScanner-ID: t9JAhMrM028361 X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-SpamCheck: X-IMAG-MailScanner-From: globillum-owner@imag.fr MailScanner-NULL-Check: 1445856208.38398@5B7oht8BZVy0L2zNnJLPYA X-Spam-Status: LOW ; -36 X-Spam-Level: - X-Spam-TU-Processing-Host: neelix.kom.tuwien.ac.at X-Virus-Scanned: by amavisd-new on vc9.kom.tuwien.ac.at This is a multi-part message in MIME format... ------------=_1445251385-19989-2 Content-Type: text/plain; charset=utf-8; format=flowed Content-Transfer-Encoding: quoted-printable X-MIME-Autoconverted: from 8bit to quoted-printable by neelix.kom.tuwien.ac.at id t9JAhUYY029841 Dear colleagues, The Center for Geometry and Computational Design, TU Wien, invites=20 applications for 10 PhD positions in the Doctoral College 'Computational Design'. Several of these positions have strong components of computer graphics. Application deadline is November 15, 2015. The Doctoral College starts in January 2016. For further details see the announcement below and the following link: http://gcd.tuwien.ac.at I would appreciate if you could forward this announcement to qualified candidates. Best regards, Michael Wimmer --=20 -- Dr. Michael=20 Wimmer-------------------------------------------------------- Institut fuer Computergraphik und Algorithmen tel: +43 (1) 58801=20 18687 Technische Universitaet Wien fax: +43 (1) 58801=20 18698 Favoritenstr. 9-11/5/E186=20 http://www.cg.tuwien.ac.at A-1040 Wien, Oesterreich=20 mailto:wimmer@cg.tuwien.ac.at -------------------------------------------------------------------------= ---- -------------------------------------------------- The Doctoral College Computational Design (DC:{CD}) at TU Wien, embedded in the Center for Geometry and Computational Design, is the first PhD program in Austria that is situated at the interface of several areas of excellence in research: Computer Graphics and Algorithms, Software Technology and Interactive Systems, Computer Aided Automation, Discrete Mathematics and Geometry, Architectural Sciences, Art and Design, History of Art, Building Archaeology and Restoration, Interdisciplinary Construction Process Management and Mechanics of Materials and Structures. The prerequisite for becoming a PhD student in the DC is a completed master degree or equivalent (e.g., Dipl.-Ing., Dipl.-Inf.), preferably with distinction, in the following fields: =E2=80=A2 Architecture =E2=80=A2 Civil engineering/structural engineering =E2=80=A2 Computer science/informatics =E2=80=A2 Mathematics =E2=80=A2 Mechanical or industrial engineering =E2=80=A2 Physics For more details on PhD topics and how to apply see: http://gcd.tuwien.ac.at ------------=_1445251385-19989-2 Content-Type: text/plain; name="message-footer.txt" Content-Disposition: inline; filename="message-footer.txt" Content-Transfer-Encoding: 8bit ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- ------------=_1445251385-19989-2-- From X-Account-Key: account1 X-UIDL: 0001f96f4778b2c7 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: Return-path: Envelope-to: wp@cg.tuwien.ac.at Delivery-date: Tue, 12 Jan 2016 05:35:13 +0100 Received: from neelix.kom.tuwien.ac.at ([192.35.241.67]) by mail.cg.tuwien.ac.at with esmtp (Exim 4.76) (envelope-from ) id 1aIqfp-0003tf-3h; 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Tue, 12 Jan 2016 05:31:24 +0100 Received: from mxb2-2.relay.renater.fr (mxb2-2.relay.renater.fr [194.214.200.9]) by rominette.imag.fr (8.13.8/8.13.8) with ESMTP id u0C4A730009590 for ; Tue, 12 Jan 2016 05:10:08 +0100 Received: from server.agi32.com (server.agi32.com [96.127.164.26]) by mxb2-2.relay.renater.fr (asm) with ESMTP id 95C1D6000F5 for ; Tue, 12 Jan 2016 05:10:07 +0100 (CET) Received: from s010600224d80691f.vn.shawcable.net ([174.7.100.71]:52497 helo=Earth) by server.agi32.com with esmtpa (Exim 4.86) (envelope-from ) id 1aIqHU-0001Qg-LO for globillum@imag.fr; Mon, 11 Jan 2016 22:10:04 -0600 From: "Ian Ashdown" To: Subject: ANNOUNCE: 16/01/11 Release of RADBIB and GITHESIS Date: Mon, 11 Jan 2016 20:10:11 -0800 Message-ID: <000f01d14cef$220f5560$662e0020$@helios32.com> MIME-Version: 1.0 X-Mailer: Microsoft Outlook 14.0 Thread-Index: AdFM7xs1tHWMXMsRRkqn4bCZHR1OVw== X-AntiAbuse: This header was added to track abuse, please include it with any abuse report X-AntiAbuse: Primary Hostname - server.agi32.com X-AntiAbuse: Original Domain - imag.fr X-AntiAbuse: Originator/Caller UID/GID - [47 12] / [47 12] X-AntiAbuse: Sender Address Domain - helios32.com X-Get-Message-Sender-Via: server.agi32.com: authenticated_id: ian_ashdown@helios32.com X-Authenticated-Sender: server.agi32.com: ian_ashdown@helios32.com X-Original-Source-IP: 96.127.164.26 X-Bizanga: IMP - mxb2-2.relay.renater.fr X-Renater-SpamState: 0 X-Renater-SpamScore: 0 X-Renater-SpamCause: gggruggvucftvghtrhhoucdtuddrfeekiedrkedvgddvlecutefuodetggdotefrodftvfcurfhrohhfihhlvgemucftgffptefvgfftpdggtfgfnhhsuhgsshgtrhhisggvnecuuegrihhlohhuthemuceftddtnecunecujfgurhephffvufffkfggtgfothesrgdtghepvddtvdenucfhrhhomhepfdfkrghnucetshhhughofihnfdcuoehirghnpggrshhhughofihnsehhvghlihhoshefvddrtghomheqnecuffhomhgrihhnpehhvghlihhoshefvddrtghomhenucfrrghrrghmpehmohguvgepshhmthhppdhhvghlohepshgvrhhvvghrrdgrghhifedvrdgtohhmpdhinhgvthepleeirdduvdejrdduieegrddviedpmhgrihhlfhhrohhmpehirghnpggrshhhughofihnsehhvghlihhoshefvddrtghomhdprhgtphhtthhopehglhhosghilhhluhhmsehimhgrghdrfhhr X-Renater-ServerName: mxb2-2.relay.renater.fr X-Greylist: Sender succeeded STARTTLS authentication, not delayed by milter-greylist-4.2.7 (neelix.kom.tuwien.ac.at [192.35.241.67]); 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boundary="----=_NextPart_000_0010_01D14CAC.13ED26D0" Content-Language: en-ca This is a multipart message in MIME format. ------=_NextPart_000_0010_01D14CAC.13ED26D0 Content-Type: text/plain; charset="us-ascii" Content-Transfer-Encoding: 7bit ANNOUNCE: 16/01/11 Release of RADBIB and GITHESIS RADBIB is a comprehensive bibliography of radiosity, photon mapping, and related global illumination papers, theses, articles, and books. It currently includes 3,320 references -- 30 new additions since its 15/09/15 release. This bibliography is available in BibTex format as RADBIB.BIB from: http://www.helios32.com (Resources section) Also available from this site is an abridged version of RADBIB.BIB called GITHESIS.BIB. This bibliography includes 375 references to radiosity, photon mapping, and related global illumination theses -- no new additions since the 15/09/15 release. Financial support for the maintenance of these bibliographies is provided by byHeart Consultants Limited. Ian Ashdown, P. Eng., FIES President byHeart Consultants Limited http://www.helios32.com CONFIDENTIALITY NOTICE: This entire communication, including without limitation any attachments, is intended for the use of the recipient to which or whom it is addressed, and may contain confidential, personal, and/or privileged information. 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ANNOUNCE: 16/= 01/11 Release of RADBIB and GITHESIS

 

RADBIB is a comprehensive biblio= graphy of radiosity, photon mapping, and related global illumination papers= , theses, articles, and books. It currently includes 3,320 references -- 30= new additions since its 15/09/15 release.

 

This bibliography is available= in BibTex format as RADBIB.BIB from:

 

  http://www.helios32.com (Res= ources section)

 

Also available from this site is an abridged version of R= ADBIB.BIB called GITHESIS.BIB. This bibliography includes 375 references to= radiosity, photon mapping, and related global illumination theses -- no ne= w additions since the 15/09/15 release.

=  

Financial support for the mainten= ance of these bibliographies is provided by byHeart Consultants Limited.

 

= Ian Ashdown, P. Eng., FIES

President

byHeart Consultants Limited

<= p class=3DMsoNormal>http://www.helios3= 2.com

 

CONFIDENTIALITY NOTICE: This entire communication, inclu= ding without limitation any attachments, is intended for the use of the rec= ipient to which or whom it is addressed, and may contain confidential, pers= onal, and/or privileged information. Please contact us immediately if you a= re not the intended recipient of this communication, and do not copy, distr= ibute, or take action relying on it. Any communication received in error, o= r subsequent reply, should be deleted or destroyed.

 

= ------=_NextPart_000_0010_01D14CAC.13ED26D0-- ------------=_1452573089-4438-0 Content-Type: text/plain; name="message-footer.txt" Content-Disposition: inline; filename="message-footer.txt" Content-Transfer-Encoding: 8bit ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- ------------=_1452573089-4438-0-- From X-Account-Key: account1 X-UIDL: 00020e0e4778b2c7 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: Return-path: Envelope-to: wp@cg.tuwien.ac.at Delivery-date: Tue, 05 Apr 2016 16:10:13 +0200 Received: from neelix.kom.tuwien.ac.at ([192.35.241.67]) by mail.cg.tuwien.ac.at with esmtp (Exim 4.76) (envelope-from ) id 1anRgL-0002Gf-8W; Tue, 05 Apr 2016 16:10:13 +0200 Received: from mx1.imag.fr (mx1.imag.fr [IPv6:2001:660:5301:6::5]) by neelix.kom.tuwien.ac.at (8.14.5/8.14.5) with ESMTP id u35EA6SJ007055 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES128-SHA bits=128 verify=OK); Tue, 5 Apr 2016 16:10:07 +0200 X-Connecting-Host: mx1.imag.fr [IPv6:2001:660:5301:6::5] X-Connecting-Addr: IPv6:2001:660:5301:6::5 X-Sent-From: globillum-owner@imag.fr Received: from chopinette.imag.fr (chopinette.imag.fr [129.88.34.204]) by mx1.imag.fr (8.13.8/8.13.8) with ESMTP id u35EA1ui016883 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES128-SHA bits=128 verify=NO); Tue, 5 Apr 2016 16:10:02 +0200 Received: from chopinette.imag.fr (localhost.localdomain [127.0.0.1]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id u35EA3OD000328; Tue, 5 Apr 2016 16:10:03 +0200 Received: (from sympa@localhost) by chopinette.imag.fr (8.12.11.20060308/8.12.11/Submit) id u35EA3km000323; Tue, 5 Apr 2016 16:10:03 +0200 Received: from mx2.imag.fr (mx2.imag.fr [129.88.30.17]) by chopinette.imag.fr (8.12.11.20060308/8.12.11/ImagV2.1) with ESMTP id u35E9jrl032742 for ; Tue, 5 Apr 2016 16:09:45 +0200 Received: from mxb2-1.relay.renater.fr (mxb2-1.relay.renater.fr [194.214.200.8]) by mx2.imag.fr (8.13.8/8.13.8) with ESMTP id u35E9f5A031347 for ; Tue, 5 Apr 2016 16:09:42 +0200 Received: from mail.cg.tuwien.ac.at (mail.cg.tuwien.ac.at [128.131.166.76]) by mxb2-1.relay.renater.fr (asm) with ESMTP id 6544E6001CE for ; Tue, 5 Apr 2016 16:09:42 +0200 (CEST) Received: from beinhart.cg.tuwien.ac.at ([128.131.166.32]) by mail.cg.tuwien.ac.at with esmtpsa (TLS1.0:DHE_RSA_AES_128_CBC_SHA1:16) (Exim 4.76) (envelope-from ) id 1anRfp-00027c-MO for globillum@imag.fr; Tue, 05 Apr 2016 16:09:41 +0200 To: Globillum From: Werner Purgathofer Subject: Robert Tobler passed away... Message-ID: <5703C7B6.4040506@cg.tuwien.ac.at> Date: Tue, 5 Apr 2016 16:12:06 +0200 User-Agent: Mozilla/5.0 (Windows NT 6.3; WOW64; rv:38.0) Gecko/20100101 Thunderbird/38.7.1 MIME-Version: 1.0 Content-Type: multipart/mixed; boundary="------------010000060907050002090004" X-Original-Source-IP: 128.131.166.76 X-Bizanga: IMP - mxb2-1.relay.renater.fr X-Renater-SpamState: 0 X-Renater-SpamScore: 0 X-Renater-SpamCause: gggruggvucftvghtrhhoucdtuddrfeekkedrfeelgdejhecutefuodetggdotefrodftvfcurfhrohhfihhlvgemucftgffptefvgfftpdggtfgfnhhsuhgsshgtrhhisggvnecuuegrihhlohhuthemuceftddtnecunecujfgurhepvffhuffkffgfgggtsehmtdgrrgdtfeejnecuhfhrohhmpeghvghrnhgvrhcurfhurhhgrghthhhofhgvrhcuoeifphestghgrdhtuhifihgvnhdrrggtrdgrtheqnecuffhomhgrihhnpehtuhifihgvnhdrrggtrdgrthenucfkphepuddvkedrudefuddrudeiiedrjeeipdduvdekrddufedurdduieeirdefvdenucfrrghrrghmpehmohguvgepshhmthhppdhhvghlohepmhgrihhlrdgtghdrthhufihivghnrdgrtgdrrghtpdhinhgvthepuddvkedrudefuddrudeiiedrjeeipdhmrghilhhfrhhomhepfihpsegtghdrthhufihivghnrdgrtgdrrghtpdhrtghpthhtohepghhlohgsihhllhhumhesihhmrghgrdhfrh X-Renater-ServerName: mxb2-1.relay.renater.fr X-Greylist: Sender succeeded STARTTLS authentication, not delayed by milter-greylist-4.2.7 (neelix.kom.tuwien.ac.at [IPv6:2001:629:1004:11::1:25]); Tue, 05 Apr 2016 16:10:10 +0200 (CEST) X-Greylist: Sender IP whitelisted, not delayed by milter-greylist-4.0.1 (mx1.imag.fr [129.88.30.5]); Tue, 05 Apr 2016 16:10:02 +0200 (CEST) X-Greylist: Sender IP whitelisted, not delayed by milter-greylist-4.2.2 (mx2.imag.fr [129.88.30.17]); Tue, 05 Apr 2016 16:09:42 +0200 (CEST) X-Loop: globillum@imag.fr X-Sequence: 439 Errors-to: globillum-owner@imag.fr Precedence: list X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: X-IMAG-MailScanner-Information: Please contact MI2S MIM for more information X-MailScanner-ID: u35EA1ui016883 X-IMAG-MailScanner: Found to be clean X-IMAG-MailScanner-SpamCheck: X-IMAG-MailScanner-From: globillum-owner@imag.fr MailScanner-NULL-Check: 1460470204.40112@RbVW40zU4AeUiE0dqUaGtw X-Spam-Status: LOW ; -15 X-Spam-Level: - X-Spam-TU-Processing-Host: neelix.kom.tuwien.ac.at X-Virus-Scanned: by amavisd-new on vc9.kom.tuwien.ac.at This is a multi-part message in MIME format. --------------010000060907050002090004 Content-Type: text/plain; charset=utf-8; format=flowed Content-Transfer-Encoding: 7bit Dear colleagues, in deep shock I have to inform you that Robert Tobler died in a sailplane crash last weekend. Attached you find a short obituary. Werner -- Werner Purgathofer TU Wien Favoritenstrasse 9 / 186 A-1040 Vienna / Austria Tel. +43-1-58801-18655 Email wp@cg.tuwien.ac.at Web www.cg.tuwien.ac.at --------------010000060907050002090004 Content-Type: application/pdf; name="Tobler Nachruf - engl.pdf" Content-Transfer-Encoding: base64 Content-Disposition: attachment; filename="Tobler Nachruf - engl.pdf" JVBERi0xLjUNJeLjz9MNCjI1IDAgb2JqDTw8L0xpbmVhcml6ZWQgMS9MIDEw NjYxOS9PIDI3L0UgMTAxMjMwL04gMS9UIDEwNjMxNC9IIFsgNDk1IDE4M10+ Pg1lbmRvYmoNICAgICAgICAgICAgICAgDQo0NCAwIG9iag08PC9EZWNvZGVQ YXJtczw8L0NvbHVtbnMgNC9QcmVkaWN0b3IgMTI+Pi9GaWx0ZXIvRmxhdGVE ZWNvZGUvSURbPEMzMjUyMzlFMzVBREZENEVCQzIwMEI2Njg0NDQzRjE0PjxC OTJBOUEzNkI1MDk2RTQwQTE5NjJBNTg2NkI5QkY5Qj5dL0luZGV4WzI1IDI4 XS9JbmZvIDI0IDAgUi9MZW5ndGggOTIvUHJldiAxMDYzMTUvUm9vdCAyNiAw IFIvU2l6ZSA1My9UeXBlL1hSZWYvV1sxIDIgMV0+PnN0cmVhbQ0KaN5iYmQQ YGBiYJoGJBgbQYQfkGA+DyRY7oFY00Gs1SDiL4jbD2JFg1gRIFYpSIcSkOCK BBJe/0BGgcTyrUAsayAh8pOBiZFhBZDFwMCIm/jPePkXQIABABa4DyoNCmVu 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purgathofer@cg.tuwien.ac.at Delivery-date: Thu, 14 Jun 2018 18:44:23 +0200 Received: from tuvok.kom.tuwien.ac.at ([192.35.241.66]) by mail.cg.tuwien.ac.at with esmtps (TLS1.0:DHE_RSA_AES_256_CBC_SHA1:256) (Exim 4.86_2) (envelope-from ) id 1fTVME-0002aK-UW for purgathofer@cg.tuwien.ac.at; Thu, 14 Jun 2018 18:44:23 +0200 X-Virus-Scanned: amavisd-new-r at vc6.kom.tuwien.ac.at Received: from mail-lf0-x241.google.com (mail-lf0-x241.google.com [IPv6:2a00:1450:4010:c07::241]) by tuvok.kom.tuwien.ac.at (8.14.5/8.14.5) with ESMTP id w5EGi5w5020990 (version=TLSv1/SSLv3 cipher=AES128-SHA bits=128 verify=OK) for ; Thu, 14 Jun 2018 18:44:06 +0200 X-Connecting-Host: mail-lf0-x241.google.com [IPv6:2a00:1450:4010:c07::241] X-Connecting-Addr: IPv6:2a00:1450:4010:c07::241 X-Sent-To: X-Sent-From: eric.haines@gmail.com Received: by mail-lf0-x241.google.com with SMTP id y20-v6so10469533lfy.0 for ; Thu, 14 Jun 2018 09:44:06 -0700 (PDT) DKIM-Signature: v=1; a=rsa-sha256; c=relaxed/relaxed; d=gmail.com; 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Ph/Kxd1TuykjcX8pNDsVPPafODCFiL8yiCFpZt/dCRNjVp4FGsdcT3Gg616HfcGpYlnU 4P4g== X-Gm-Message-State: APt69E12M3XA4FwvF5x589yyJF5BBvV7+4T8bgKrACUrAGPccq9znWVh zp+sBEg//oWONDTigdPRrcf9/qpPfeI+6H6LtRY= X-Google-Smtp-Source: ADUXVKKvzu9X5NF3qZ69iUUYEWO4x69EBVcFTkkGfCfRRa7Nttur78LjSFkwoauQB3jx8VTchyagvOuDnhoG6XYcCTs= X-Received: by 2002:a19:3bc5:: with SMTP id d66-v6mr5734089lfl.113.1528994641194; Thu, 14 Jun 2018 09:44:01 -0700 (PDT) MIME-Version: 1.0 From: Eric Haines Date: Thu, 14 Jun 2018 12:43:22 -0400 Message-ID: Subject: (Optional) abstracts for "Ray Tracing Gems" due June 21 To: Eric Haines Cc: =?UTF-8?Q?Tomas_Akenine=2DM=C3=B6ller?= Content-Type: multipart/related; boundary="0000000000007476b3056e9ccea1" X-Greylist: Sender succeeded STARTTLS authentication, not delayed by milter-greylist-4.2.7 (tuvok.kom.tuwien.ac.at [IPv6:2001:629:1004:11::25]); Thu, 14 Jun 2018 18:44:07 +0200 (CEST) X-Spam-Status: LOW ; 32 X-Spam-Level: ***++ X-Spam-TU-Processing-Host: tuvok.kom.tuwien.ac.at --0000000000007476b3056e9ccea1 Content-Type: multipart/alternative; boundary="0000000000007476b1056e9ccea0" --0000000000007476b1056e9ccea0 Content-Type: text/plain; charset="UTF-8" This morning I started to write people involved in ray tracing and ray casting, past and present, fully or tangentially, asking to consider submitting something to the book I'm co-editing, *Ray Tracing Gems* . It finally dawned on me that writing each of you individually would take a week, at which point the deadline for the additional incentive offered by NVIDIA (free wicked fast GPUs (I now live near Boston, so have to say "wicked fast")) would be over. So, I wrote a blog post, tweeted it, and even posted on Facebook (I should have put a cute cat photo with it, to get likes. Hmmm, I'll add one here instead). However, I wanted to make sure you, yes, you, definitely received word. Here's the (short) post: *http://www.realtimerendering.com/blog/one-week-to-go-submit/* If you are inspired, I hope you'll consider submitting a proposal or three (if nothing else, the photo at the bottom of that post is worthwhile). Thanks for your consideration, and please do pass this email on to anyone you think may be interested, Eric And, our family's cat-almost-in-bounding-box Ezra says "Submit!" (expressed purely through the eyes) [image: image.png] --0000000000007476b1056e9ccea0 Content-Type: text/html; charset="UTF-8" Content-Transfer-Encoding: quoted-printable
This morning I started to write people involved in ra= y tracing and ray casting, past and present, fully or tangentially, asking = to consider submitting something to the book I'm co-editing, Ray Tracing Gems. = It finally dawned on me that writing each of you individually would take a = week, at which point the deadline for the additional incentive offered by NVI= DIA (free wicked fast GPUs (I now live near Boston, so have to say &quo= t;wicked fast")) would be over.

So, = I wrote a blog post, tweeted it, and even posted on Facebook (I should have= put a cute cat photo with it, to get likes. Hmmm, I'll add one here in= stead). However, I wanted to make sure you, yes, you, definitely received w= ord. Here's the (short) post:


If you are inspire= d, I hope you'll consider submitting a proposal or three (if nothing el= se, the photo at the bottom of that post is worthwhile).

<= /div>
Thanks for your consideration, and please do pass this email on= to anyone you think may be interested,

Eri= c

And, our family's cat-almost-in-bounding-box= Ezra says "Submit!" (expressed purely through the eyes)

3D"image.png"



<= /div>
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2019 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Return-path: Envelope-to: wp@cg.tuwien.ac.at Delivery-date: Thu, 12 Dec 2019 12:12:58 +0100 Received: from tuvok.kom.tuwien.ac.at ([192.35.241.66]) by mail.cg.tuwien.ac.at with esmtps (TLS1.0:DHE_RSA_AES_256_CBC_SHA1:256) (Exim 4.90_1) (envelope-from ) id 1ifMOw-0001kr-1s for wp@cg.tuwien.ac.at; Thu, 12 Dec 2019 12:12:58 +0100 X-Virus-Scanned: amavisd-new-r at vc3.kom.tuwien.ac.at Received: from amazone.ujf-grenoble.fr (mailmx.ujf-grenoble.fr [193.54.238.254]) by tuvok.kom.tuwien.ac.at (8.14.5/8.14.5) with ESMTP id xBCBCkvH016630 for ; Thu, 12 Dec 2019 12:12:52 +0100 X-Connecting-Host: mailmx.ujf-grenoble.fr [193.54.238.254] X-Connecting-Addr: 193.54.238.254 X-Sent-To: X-Sent-From: globillum-owner@univ-grenoble-alpes.fr Received: from danube.u-ga.fr (danube.u-ga.fr [195.83.24.186]) by amazone.ujf-grenoble.fr (Postfix) with ESMTP id 47YWNt33ndz1yYf; Thu, 12 Dec 2019 12:12:46 +0100 (CET) Received: by danube.u-ga.fr (Postfix, from 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mail2-relais-roc.national.inria.fr with ESMTP/TLS/DHE-RSA-AES256-GCM-SHA384; 12 Dec 2019 12:12:43 +0100 From: Nicolas Holzschuch Mime-Version: 1.0 (Mac OS X Mail 13.0 \(3601.0.10\)) Subject: Reconstructing the globillum archives Message-Id: Date: Thu, 12 Dec 2019 12:12:43 +0100 To: globillum@univ-grenoble-alpes.fr X-Mailer: Apple Mail (2.3601.0.10) X-Original-Source-IP: 192.134.164.83 X-Renater-SpamState: 0 X-Renater-SpamScore: 0 X-Renater-SpamCause: gggruggvucftvghtrhhoucdtuddrgedufedrudeljedgvdejucetufdoteggodetrfdotffvucfrrhhofhhilhgvmecutffgpfetvffgtfdpggftfghnshhusghstghrihgsvgenuceurghilhhouhhtmecufedtudenucenucfjughrpefhtgfgggfukfffvffosehtqhhmtdhhtddvnecuhfhrohhmpefpihgtohhlrghsucfjohhliihstghhuhgthhcuoefpihgtohhlrghsrdfjohhliihstghhuhgthhesihhnrhhirgdrfhhrqeenucfkphepudelvddrudefgedrudeigedrkeefpddufedtrdduledtrddutdeirddvhedvnecurfgrrhgrmhepmhhouggvpehsmhhtphdphhgvlhhopehmrghilhdvqdhrvghlrghishdqrhhotgdrnhgrthhiohhnrghlrdhinhhrihgrrdhfrhdpihhnvghtpeduledvrddufeegrdduieegrdekfedpmhgrihhlfhhrohhmpefpihgtohhlrghsrdfjohhliihstghhuhgthhesihhnrhhirgdrfhhrpdhrtghpthhtohepghhlohgsihhllhhumhesuhhnihhvqdhgrhgvnhhosghlvgdqrghlphgvshdrfhhrnecuvehluhhsthgvrhfuihiivgeptd X-Renater-ServerName: mxb1-1.relay.renater.fr X-Bizanga: IMP - mxb1-1.relay.renater.fr Reply-To: Nicolas Holzschuch X-Loop: globillum@univ-grenoble-alpes.fr X-Sequence: 440 Errors-To: globillum-owner@univ-grenoble-alpes.fr Precedence: list Precedence: bulk Sender: globillum-request@univ-grenoble-alpes.fr X-no-archive: yes List-Id: List-Help: List-Subscribe: List-Unsubscribe: List-Post: List-Owner: List-Archive: Archived-At: Content-type: multipart/mixed; boundary="----------=_1576149165-3988-7" X-Greylist: Sender passed SPF test, not delayed by milter-greylist-4.2.7 (tuvok.kom.tuwien.ac.at [192.35.241.66]); Thu, 12 Dec 2019 12:12:52 +0100 (CET) X-Spam-Status: LOW ; -34 X-Spam-Level: - X-Spam-TU-Processing-Host: tuvok.kom.tuwien.ac.at This is a multi-part message in MIME format... ------------=_1576149165-3988-7 Content-Type: text/plain; charset=us-ascii Content-Transfer-Encoding: quoted-printable Hello fellow globillumers,=20 this e-mail has two purposes: 1) to check that the mailing list still works after the change of server an= d address (we are now globillum@univ-grenoble-alpes.fr instead of globillum= @imag.fr) 2) in the process of moving servers, we appear to have lost the globillum a= rchives. Some of these could be interesting, if only for historical purpose= s. I'm sure some of you have archived e-mails from globillum, and we could = use that to reconstruct the entire archive (or most of it). Best regards, Nicolas Holzschuch ------------=_1576149165-3988-7 Content-Type: text/plain; charset="UTF-8" Content-Disposition: inline Content-Transfer-Encoding: 8bit ------------------------------------------------------------------------- globillum@imag.fr -- mailing list devoted to global illumination research For list archives or to configure your options, see http://listes.imag.fr ------------------------------------------------------------------------- ------------=_1576149165-3988-7--