Ravi Ramamoorthi  Computer Graphics Laboratory , 
Pat Hanrahan  Stanford University 
AbstractWe present a theoretical analysis of the relationship between incoming radiance and irradiance. Specifically, we address the question of whether it is possible to compute the incident radiance from knowledge of the irradiance at all surface orientations. This is a fundamental question in computer vision and inverse radiative transfer. We show that the irradiance can be viewed as a simple convolution of the incident illumination, i.e.\ radiance and a clamped cosine transfer function. Estimating the radiance can then be seen as a deconvolution operation. We derive a simple closedform formula for the irradiance in terms of sphericalharmonic coefficients of the incident illumination and demonstrate that the oddorder modes of the lighting with order greater than one are completely annihilated. Therefore, these components cannot be estimated from the irradiance, contradicting a theorem due to Preisendorfer.
A practical realization of the radiancefromirradiance problem is the
estimation of the lighting from images of a homogeneous convex curved
Lambertian surface of known geometry under distant illumination, since
a Lambertian object reflects light equally in all directions
proportional to the irradiance. We briefly discuss practical and
physical considerations, and describe a simple experimental test to
verify our theoretical results. SummaryThis paper derives an analytic formula for the irradiance in terms of the radiance. The formula is in terms of spherical harmonics which can be thought of in some sense as the eigenfunctions of the Lambertian BRDF. It is shown that the oddorder modes of the illumination (greater than one) are completely annihilated, so irradiance cannot be estimated from radiance. There is also a deeper analysis of how positivity of the lighting affects the results, and how this can allow for a solution in certain special cases. Finally, we present empirical and theoretical evidence showing that in practice, the irradiance depends only on the first 2 orders of spherical harmonic modes of the illumination, and can be represented as a quadratic polynomial of the cartesian components of the surface normal. In fact, 99% of the energy of the Lambertian BRDF filter is contained by orders 0,1, and 2. In particular, we care only about the first 2 orders of the illumination, that is 9 parameters. These first 9 coefficients are also all that can be determined regarding the lighting. This 9 parameter model is likely to have wide impact in computer graphics and vision, as we have already demonstrated for forward and inverse rendering. ResultsThe figures on the right summarize some of the main results from the paper. Figures 1,2: Our analytic irradiance formula in terms of spherical harmonic coefficients, and the analytic values for the coefficients of the Lambertian BRDF filter. These are the key results of the paper. The coefficients of the Lambertian BRDF fall off as l^(5/2) for even terms and vanish for odd terms > 1. This makes radiancefromirradiance formally illposed as well as illconditioned for frequencies l > 2. Figure 3: A plot of the spherical harmonic coefficients (from the equations in figure 2) versus frequency (l). We see the rapid decay of coefficients and the zeros for odd modes greater than one. Figure 4: Showing that we can indeed get the first 2 orders (9 terms) of the lighting from the irradiance but that this fails miserably for higher orders. Relevant Links


 
 
