Multiple Laser Guide Stars can be used to retrieve the three-dimensional di
stribution of the perturbing layers on the coming wavefront in Adaptive Opt
ics system and to derive corrections for conical anisoplanatism. We outline
the basic analytical details of a modal approach to this problem. The adva
ntages of this approach with respect to the traditional zonal one are point
ed out along with a preliminary discussion of the way the involved matrices
are to be treated in order to minimize noise propagation problems.