In 1996, Faugeras and Robert [3] completely solved the problem about what could be predicted about a third view of an object, given two other views. This problem is central to stereo, motion, and object recognition. They describe the geometry of three cameras, illustrated in figure 5, as follows:
The prediction of points is very simple. We assume that we have two corresponding pixels m1 and m2 in images 1 and 2. Them m3 must belong to the epipolar line of m1 in the third image, given by , and to the epipolar line of pixel m2 in the third image, given by .Therefore, m3 belongs to the intersection of these two lines, and we can write
The prediction of lines is also simple. We assume now that we are given two corresponding lines l1 and l2 in images 1 and 2. The problem is to determine the position of l3 in image 3. Let m1, m'1 be two points of l1. They define two points m2, m'2 of l2 as the intersections of the epipolar line of m1 represented by and of m'1 represented by with l2. Therefore we can write
and Therefore, the line l3 is defined by the two points m3 and m'3, intersections of the epipolar lines of m1 and m'1 and m2 and m'2 in the third image. Therefore we can writeThe prediction of curvatures is slightly more complicated and will not be covered in these lectures.