Inverse problem of photometric observation of solar radiation reflected by an optically dense planetary atmosphere. Mathematical methods and weighting functions of linearized inverse problem.

Details Inverse problem of photometric observation of solar radiation reflected by an optically dense planetary atmosphere. Mathematical methods and weighting functions of linearized inverse problem. Inverse problem of photometric observation of solar radiation reflected by an optically dense planetary atmosphere. Mathematical methods and weighting functions of linearized inverse problem.

Jan 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992cosre..29..519u&link_type=abstract

Cosmic Res., Vol. 29, No. 4, p. 519 - 532

Computer Science

6

Scientific paper

A general approach to the solution of the inverse radiative transfer problem based on the investigation of solutions of the corresponding direct and inverses radiative transfer problems is considered. The approach is applied to the case of an optimally dense planetary atmosphere. The adjoint transfer equation and corresponding boundary conditions are derived. Numerical solutions are obtained using spherical harmonics. Weighting functions of the vertical profiles of the coefficients of the expansion of the atmospheric scattering phase function in Legendre polynomials are computed for a simulated Rayleigh atmosphere.

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