Towards linearization of atmospheric radiative transfer in spherical geometry

We present a general approach for the linearization of radiative transfer in a spherical planetary atmosphere. The approach is based on the forward-adjoint perturbation theory. In the first part we develop the theoretical background for a linearization of radiative transfer in spherical geometry. Us...

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Published inJournal of quantitative spectroscopy & radiative transfer Vol. 95; no. 2; pp. 175 - 200
Main Authors Walter, Holger H., Landgraf, Jochen
Format Journal Article
LanguageEnglish
Published Elsevier Ltd 01.10.2005
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Summary:We present a general approach for the linearization of radiative transfer in a spherical planetary atmosphere. The approach is based on the forward-adjoint perturbation theory. In the first part we develop the theoretical background for a linearization of radiative transfer in spherical geometry. Using an operator formulation of radiative transfer allows one to derive the linearization principles in a universally valid notation. The application of the derived principles is demonstrated for a radiative transfer problem in simplified spherical geometry in the second part of this paper. Here, we calculate the derivatives of the radiance at the top of the atmosphere with respect to the absorption properties of a trace gas species in the case of a nadir-viewing satellite instrument.
Bibliography:ObjectType-Article-1
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content type line 23
ISSN:0022-4073
1879-1352
DOI:10.1016/j.jqsrt.2004.08.043