Titlebook: Radiative Transfer; An Introduction to E Hélène Frisch Book 2022 The Editor(s) (if applicable) and The Author(s), under exclusive license t

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Polarized Radiative Transfer Equationsolev. In this chapter, we present a few linearly polarized radiative transfer equations describing monochromatic Rayleigh scattering, resonance polarization, and the Hanle effect, and then show how to construct vector and matrix convolution integral equations. They are used, in the following chapter

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Scattering Problems with No Exact Solution I: The Auxiliary Matricesresonance polarization, and the Hanle effect. For these processes, there is no explicit solution for radiative transfer problems in semi-infinite plane parallel media. They have to be solved numerically, directly from the radiative transfer equations, or by means of a nonlinear .-equation. The funda

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Radiative Transfer Equations presented in Appendix J of Chap. . and some asymptotic results on the large scale behavior of the radiation field in Chap. .. Otherwise, we consider only spectral lines formed with complete frequency redistribution (also known as .) for which exact results can be obtained.

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