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The direct solution of the radiative transfer equation for optically thick atmospheres
Authors:José Canosa  Alan Wray
Institution:IBM Scientific Center, Palo Alto, CA 94304, U.S.A.
Abstract: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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