Lommel-Seeliger diffuse model
- article : http://www.shlyaev.com/rnd/37-cpp-category/60-diffuseshaders
- Arnold API Reference : https://trac.solidangle.com/arnoldpedia/chrome/site/Arnold-4.0.14.0/doc/api/group__ai__shader__brdf.html#ga57496c0b8e0e8efff54ed2f233c0d241
// Quoted from http://www.shlyaev.com/rnd/37-cpp-category/60-diffuseshaders The Lommel-Seeliger volumetric scattering BRDF is a simple BRDF predicting scattering from a dusty surface. Dusty surfaces scatter the reflected light in all directions toward grazing angles to the surface. The BRDF is: brdf(wi,wo) = 1 / (N.wi)+(N.wo) The Lommel-Seeliger function is essentially a "distillation" of the Hapke function that does not contain more complicated terms. It relies on the incidence and emergence angles alone. It ignores masking and shadowing. The Lambert and Lommel-Seeliger functions represent end-members on a scale that ranges from an "icy-type" surface (Lambert) to a "lunar-type" surface (Lommel-Seeliger).
- Links for Lommel-Seeliger diffuse model
- http://www.iriacenter.org/tutorial/guide.frm.html#hapke
- http://graphics.stanford.edu/~smr/cs348c/paper.html
- http://www.hinjang.com/articles/03.html
- http://isis.astrogeology.usgs.gov/Isis2/isis-bin/pdfs2.cgi?chardip
- http://articles.adsabs.harvard.edu//full/2005JRASC..99...92F/0000092.000.html
- http://orca.phys.uvic.ca/~tatum/plphot/plphot03.pdf