1154 |
|
<p> |
1155 |
|
|
1156 |
|
<dt> |
1157 |
+ |
<a NAME="aBSDF"> |
1158 |
+ |
<b>aBSDF</b> |
1159 |
+ |
</a> |
1160 |
+ |
|
1161 |
+ |
<dd> |
1162 |
+ |
The aBSDF material is identical to the BSDF type with two |
1163 |
+ |
important differences. First, proxy geometry is not |
1164 |
+ |
supported, so there is no thickness parameter. Second, an |
1165 |
+ |
aBSDF is assumed to have some specular through component |
1166 |
+ |
(the ’a’ stands for "aperture"), |
1167 |
+ |
which is treated specially during the direct calculation |
1168 |
+ |
and when viewing the material. Based on the BSDF data, the |
1169 |
+ |
coefficient of specular transmission is determined and used |
1170 |
+ |
for modifying unscattered shadow and view rays. |
1171 |
+ |
|
1172 |
+ |
<pre> |
1173 |
+ |
mod aBSDF id |
1174 |
+ |
5+ BSDFfile ux uy uz funcfile transform |
1175 |
+ |
0 |
1176 |
+ |
0|3|6|9 |
1177 |
+ |
rfdif gfdif bfdif |
1178 |
+ |
rbdif gbdif bbdif |
1179 |
+ |
rtdif gtdif btdif |
1180 |
+ |
</pre> |
1181 |
+ |
|
1182 |
+ |
<p> |
1183 |
+ |
If a material has no specular transmitted component, it is |
1184 |
+ |
much better to use the BSDF type with a zero thickness |
1185 |
+ |
than to use aBSDF. |
1186 |
+ |
<p> |
1187 |
+ |
|
1188 |
+ |
<dt> |
1189 |
|
<a NAME="Antimatter"> |
1190 |
|
<b>Antimatter</b> |
1191 |
|
</a> |