danielkaijzer/CV_Photometric_Stereo
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Author: Daniel A. Kaijzer CSCI 49369 - Computational Vision HW 4 FORMULA FOR S2: Given the brightest point (x,y) on sphere's projected image, centroid (xbar, ybar) and radius r: light source direction = normal vector = (dx/length, dy/length, z/length) light source vector = normal vector * I where: # dx and dy are vectors from center to point x,y dx = x - xbar dy = y - ybar # z is calculated by rearranging sphere equation # since we're doing orthographic projection we can treat z as constant z = root(r^2 - dx^2 - dy^2) # use length to normalize to unit length length = root(dx^2 + dy^2 + z^2) I is intensity of brightest pixel