Polarization of radiation in the case of multiple scattering in a plane layer

Details Polarization of radiation in the case of multiple scattering in a plane layer Polarization of radiation in the case of multiple scattering in a plane layer

Jul 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981afz....17..535l&link_type=abstract

(Astrofizika, vol. 17, July-Sept. 1981, p. 535-546.) Astrophysics, vol. 17, no. 3, Jan. 1982, p. 299-306. Translation.

Astronomy and Astrophysics

Astrophysics

7

Atmospheric Radiation, Planetary Atmospheres, Polarized Radiation, Radiative Transfer, Rayleigh Scattering, Stellar Atmospheres, Energy Distribution, Linear Equations, Optical Thickness, Scattering Coefficients

Scientific paper

A method by Sobolev (1949), which consists of obtaining linear integral equations that determine directly the intensity of radiation emerging from the atmosphere, is used to determine the degree of polarization of radiation emerging from an atmosphere of finite optical thickness. Radiation transfer in a plane layer of finite optical thickness is considered for the case of the Rayleigh scattering law and for true absorption. The linear integral equations determine the intensities of the radiation that emerges from the layer, and these equations are solved for the case of a uniform distribution of the energy source within the layer.

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