Radiosity and Occlusion

CS 481/681 2007 Lecture, Dr. Lawlor

Try all of these techniques out with the 481_radiosity2 example program, linked off the front page.

Global illumination image fixed_angle

We begin with a classic OpenGL fixed-direction, infinite-distance light source.

Global illumination image local_angle

If we compute the vector pointing to the light source from each pixel, we immediately gain realism. The ground gets darker farther away simply because the vector to the light source is pointing farther away from the normal, not because of any distance-related falloff.

Global illumination image solid_angle

If we compute the solid angle to the actual polygon light source, using the classic loop around the vertices (angle-weighted cross products), we get far nbetter local effects, as well as properly handling light sources of varying sizes.

Global illumination image hard_shadow

Occluding objects cast shadows by reducing the solid angle of the light source. The easiest way to handle this is to shoot a ray from the receiver to the light source's center--if the ray hits something, the object is "in shadow". This binary shadowing choice gives clean but unnaturally sharp shadows.

Global illumination image two_shadow

One method to approximate soft shadows is to shoot several "shadow rays", and average the results. This is equivalent to approximating the area light source with several point light sources.

Global illumination image three_shadow

Shooting more shadow rays (in this case, three) gives a better approximation of soft shadows, but it still isn't really very good.

Global illumination image random_shadow

Using the same three shadow rays, but shooting toward random points on the light source, gives far better results. Random numbers aren't very easy to generate in a pixel shader, so this version repeats a short series, resulting in a rectangular dithering-type pattern. A better approach would probably be to generate a low-correlation random number texture, and look up the random numbers from that.

Global illumination image conetraced_shadow

For spherical light sources and occluders, you can use "Conetracing" to estimate the fraction of the light source covered by the occluder. The big advantage to this is you can get analytically-accurate, smooth results while taking only one sample. The disadvantage is it only works nicely for spheres! I once wrote a raytracer using conetracing for everything. Amanatides wrote an article "Ray Tracing with Cones" in SIGGRAPH 1984 expanding how to do this correctly, and Jon Genetti has a paper on "Pyramidal" raytracing as well.


Unfortunately, the Achilles heel of all these techniques is scalability--they work fine for one or two occluders, but the raytracing process slows down as you add occluders.  A more promising approach for even moderately large models is to somehow use fragments to approximate solid angle and radiosity simultaniously, which we'll look at next class.