Inversion Methods in Atmospheric Remote Sounding by Adarsh Deepak

By Adarsh Deepak

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Barkstrom: These methods are connected with problems, such as finite clouds. Lenoble: But for spherical problems you mentioned the problem of stellar atmospheres. It is quite different because you don't have the solar illumination so you have really a spherical symmetry. Barkstrom: It doesn't matter; the procedure is the same. Unidentified Speaker: What are the publication plans for the report you are preparing for the Radiation Commission? Well, the first draft of the report has been published.

Therefore, the result is wrong in the forward direction (μ = - 1) for small 29 REVIEW OF RADIATIVE TRANSFER METHODS TABLE 3 Error τ. 4 are smaller than the values expected for primary scattering only. Elsewhere, it is expected that the truncature procedure gives an accuracy better than 1%. The Monte Carlo method has no problem with the forward peak and the results at μ = -1 and small optical thickness are better than those of the Spherical Harmonics. But the computation time becomes very large for such large optical thickness and only one group of authors has run the Monte Carlo program for the cloud case.

Irvine Δ Modified Two-Stream (Drs. Kerschgens, Raschke and Pilz) © Exponential Kernel (Dr. Brogniez) 0 Fig. 1. 1 (Dr. Shettle) Shettle) (Dr. Wiscombe) (Dr. 9, μ = -1. (See Ref. 2) JACQUELINE LENOBLE 32 larger than 100 or even the use of a computer can be avoided. Moreover they give simple analytical expressions of the flux. Between them we have classified the similarity relations which reduce the anisotropic problem to an isotropic one, the Eddington, Two-Stream, and Exponential Kernel methods.

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