The direct solution of the radiative transfer equation for optically thick atmospheres

Details The direct solution of the radiative transfer equation for optically thick atmospheres The direct solution of the radiative transfer equation for optically thick atmospheres

Apr 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977jqsrt..17..445c&link_type=abstract

Journal of Quantitative Spectroscopy and Radiative Transfer, vol. 17, Apr. 1977, p. 445-448.

Mathematics

Atmospheric Scattering, Optical Thickness, Radiative Transfer, Spherical Harmonics, Atmospheric Models, Linear Equations, Matrices (Mathematics), Mie Scattering, Rayleigh Scattering

Scientific paper

A simple improvement of a previous direct method of solution of the
spherical harmonics approximation to the radiative transfer equation
results in higher computational efficiencies by factors of 2-4; these
higher efficiencies are particularly important to shorten the lengthy
computations required in optically thick nonhomogeneous atmospheres.

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