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NASA NTRS · 19750003478

Solving multiple scattering problems in planetary atmospheres

Abstract

Multiple scattering problems, radiative transfer problems in planetary atmospheres within extended visible portion of the spectrum, are examined. The direct and inverse problems and the extinction coefficient are defined, along with other scattering characteristics. Albedos in semi-infinite and finite atmospheres are considered, as well as surface illumination, energy deposition, and polarization. The Eddington approximation figures prominently in the calculations. Precise numerical methods and analytical solutions are included.

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BibTeXRIS

Irvine, W. M., Lenoble, J.. 1974-01-01. Solving multiple scattering problems in planetary atmospheres. https://ntrs.nasa.gov/citations/19750003478

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