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2 Notation and basics

Following [ 4 ], we consider a stereo pair composed of two pinhole cameras, each modelled by its optical center and its retinal plane (or image plane ) . In each camera, a point in 3-D space is projected into an image point , which is the intersection of the line with . The transformation from to is modelled by the linear transformation in projective (or homogeneous) coordinate:

 

where

The points for which S =0 define the focal plane and are projected to infinity. The projection matrix can be decomposed into the product . maps from world to camera coordinates and depends on the extrinsic parameters of the stereo rig only; , which maps from camera to pixel coordinates and depends on the intrinsic parameters only, has the following form:

 

where f is the focal length in millimeters, are the scale factors along the u and v axes respectively (the number of pixels per millimiter), and , and are the focal lengths in horizontal and vertical pixels, respectively. If we write the projection matrix as

we see that the plane ( S =0) is the focal plane, and the two planes and intersect the retinal plane in the vertical ( U =0) and horizontal ( V =0) axis of the retinal coordinates, respectively.

The optical center , , is the intersection of the three planes introduced in the previous paragraph; therefore , and . The optical ray associated to an image point is the line , i.e. the set of points . The equation of this ray can be written in parametric form as .



Next: 3 The rectification transformation Up: Rectification with unconstrained stereo Previous: 1 Introduction and motivations

Adrian F Clark
Wed Jul 23 16:48:44 BST 1997