| 1419 | 
  | 
Changed ambient calculation so that -ad will not limit recursion | 
| 1420 | 
  | 
depth, and a minimum of 27 samples will be sent out for each stored | 
| 1421 | 
  | 
ambient value, or 3 samples if -aa is 0 (caching off). | 
| 1422 | 
+ | 
 | 
| 1423 | 
+ | 
Added -oM option to rtrace to report material (rather than modifier) | 
| 1424 | 
+ | 
for cases where actual material is aliased or further up modifier chain. | 
| 1425 | 
+ | 
 | 
| 1426 | 
+ | 
Rearranged the way ray contributions are computed so that it might be | 
| 1427 | 
+ | 
possible to use rtrace to derive daylight coefficients and optical | 
| 1428 | 
+ | 
transfer functions.  The new -oTW option of rtrace produces color | 
| 1429 | 
+ | 
contribution weights for each ray, which combined with the -ti (or -tI) | 
| 1430 | 
+ | 
option permits the contribution of selected surfaces or sources to | 
| 1431 | 
+ | 
be determined.  Using the -oTW option, one should also specify | 
| 1432 | 
+ | 
options "-dt 0 -aa 0 -as 0" for optimal results.  In particular, | 
| 1433 | 
+ | 
one cannot expect reasonable tallies with -ab >= 1 and irradiance | 
| 1434 | 
+ | 
caching on (-aa > 0). | 
| 1435 | 
+ | 
 | 
| 1436 | 
+ | 
The same code modifications included a change to the indirect computation | 
| 1437 | 
+ | 
with caching switched off (-aa 0).  Whereas before, the number of secondary | 
| 1438 | 
+ | 
rays after the first bounce were half of the previous generation, they are | 
| 1439 | 
+ | 
now determined by the surface reflectance, making for a better and faster | 
| 1440 | 
+ | 
calculation.  It should now be possible to compute many bounces with -aa 0, | 
| 1441 | 
+ | 
which used to be prohibitively expensive. | 
| 1442 | 
+ | 
 | 
| 1443 | 
+ | 
Added -T option to xshowtrace to trace rays to light sources. | 
| 1444 | 
+ | 
 | 
| 1445 | 
+ | 
Added meta2bmp program to produce BMP files from metafile graphics. | 
| 1446 | 
+ | 
 | 
| 1447 | 
+ | 
Added cct_x(t) and cct_y(t) to src/cal/cal/blackbody.cal to interpolate | 
| 1448 | 
+ | 
CIE chromaticities for particular black-body temperatures. |