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<!-- RCSid $Id$ --> |
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<head> |
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<title> |
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The RADIANCE 5.1 Synthetic Imaging System |
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The RADIANCE 5.2 Synthetic Imaging System |
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</title> |
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</head> |
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<body> |
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<p> |
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<h1> |
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The RADIANCE 5.1 Synthetic Imaging System |
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The RADIANCE 5.2 Synthetic Imaging System |
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</h1> |
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<p> |
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the surface will be invisible from behind. Unlike other |
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data-driven material types, the BSDF type is fully supported |
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and all parts of the distribution are properly sampled. |
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<dt> |
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<a NAME="aBSDF"> |
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<b>aBSDF</b> |
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</a> |
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<dd> |
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The aBSDF material is identical to the BSDF type with two |
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important differences. First, proxy geometry is not |
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supported, so there is no thickness parameter. Second, an |
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aBSDF is assumed to have some specular through component |
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(the ’a’ stands for "aperture"), |
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which is treated specially during the direct calculation |
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and when viewing the material. Based on the BSDF data, the |
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coefficient of specular transmission is determined and used |
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for modifying unscattered shadow and view rays. |
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<pre> |
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mod aBSDF id |
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5+ BSDFfile ux uy uz funcfile transform |
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0 |
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0|3|6|9 |
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rfdif gfdif bfdif |
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rbdif gbdif bbdif |
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rtdif gtdif btdif |
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</pre> |
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<p> |
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If a material has no specular transmitted component, it is |
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much better to use the BSDF type with a zero thickness |
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than to use aBSDF. |
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<p> |
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<dt> |