--- ray/doc/notes/ReleaseNotes 2005/01/18 00:33:16 1.62 +++ ray/doc/notes/ReleaseNotes 2005/04/19 01:15:06 1.71 @@ -1393,3 +1393,49 @@ Added -pd option to handle depth-of-field blur in rpic that the view directon (-vd option) include focal distance information, which is now preserved by the various view file routines, and reported by the vwright command. + +Added DBLUR variable to ranimate and pmdblur script to handle simultaneous +motion and depth-of-field blurring. Thanks to Visarc for funding this work. + +Added setting of focus distance in rvu ("focus" command) and rholo +('f'/"frame" command). + +Changed default remote shell in ranimate to "ssh" rather than "rsh", +which has been abandoned on most Unix systems due to security issues. + +Fixed behavior of source primitive using illum with no alternate +material. These now become transparent so one can see the sky or +light-probe background for use in image-based lighting. Previously, +the user needed to specify the background glow as the alternate +material for a distant illum source to behave properly. (This still +works.) + +Fixed some minor problems and inconsistencies with 16-bit/channel +TIFF i/o in ra_tiff. + +Created mksource program to generate distant sources for improved +image-based lighting with light probes. + +Changed ambient calculation so that -ad will not limit recursion +depth, and a minimum of 27 samples will be sent out for each stored +ambient value, or 3 samples if -aa is 0 (caching off). + +Added -oM option to rtrace to report material (rather than modifier) +for cases where actual material is aliased or further up modifier chain. + +Rearranged the way ray contributions are computed so that it might be +possible to use rtrace to derive daylight coefficients and optical +transfer functions. The new -oTW option of rtrace produces color +contribution weights for each ray, which combined with the -ti (or -tI) +option permits the contribution of selected surfaces or sources to +be determined. Using the -oTW option, one should also specify +options "-dt 0 -aa 0 -as 0" for optimal results. In particular, +one cannot expect reasonable tallies with -ab >= 1 and irradiance +caching on (-aa > 0). + +The same code modifications included a change to the indirect computation +with caching switched off (-aa 0). Whereas before, the number of secondary +rays after the first bounce were half of the previous generation, they are +now determined by the surface reflectance, making for a better and faster +calculation. It should now be possible to compute many bounces with -aa 0, +which used to be prohibitively expensive.