
Topographic correction 199
5.5.3 Camera models and RFM approximations
Equations (5.54) are very simple because they assume that the world
and
image coordinates coincide. But in order to apply them, one has first to
transform the world coordinate system to the satellite coordinate system.
This can be do ne in a straightforward way w ith the rotation and translation
transformatio ns intr oduced above. However, it requires accurate knowledge of
the altitude, orientation and detailed properties of the satellite imaging sys tem
at the time of the image acquisition (or, more precisely, during the acquisition,
since the la tter is never instantaneous). The