About a Surface Planet Remote Sensing Problem by Way of its Atmosphere

The problem is considered of the surface remote sensing by way of the planet atmosphere. The efficient method of the space-data atmosphere correction has been developed. The model of the atmosphere transfer characteristics is represented as the linear functional - the superposition integral, underlying the classic linearly-system approach. The optical transfer operator stated mathematically rigorous and physically corrective by the influence functions and spatial-frequence characteristics method. The influence functions and spatial-frequency characteristics of the 'atmosphere - planet surface' system are the functional kernels and the objective characteristics which are invariant about the specific structures of the remote sensing objects, the illumination and observation conditions. The spatial-frequency characteristics are introduced as the Fourier-images of the influence functions over the horizontal coordinates. The basics of the spatial filtration theory, having the wide field of application are described for the remote-sensing problem. The fundamental problems of the three-dimensional radiation transfer are noted.