Abstract
The inverse problem in the form of Fredholm integral equation of the first kind for determining the distribution density of the number of specular points of 3-D Gaussian sea surface is formulated and solved. The kernel of this equation is determined by the characteristic function of the distribution of radii of curvature at the specular points. On the basis of numerical experiments, and also by using images of the Sun glitters it is shown that on the known distribution density of the intensity of reflected light it is possible to define the distribution densities of both the number of specular points and the radii of curvature at the specular points.
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