Exact solution of the equation of transfer with planetary phase function

Details Exact solution of the equation of transfer with planetary phase function Exact solution of the equation of transfer with planetary phase function

Oct 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992em%26p...59....1k&link_type=abstract

Earth, Moon, and Planets (ISSN 0167-9295), vol. 59, no. 1, p. 1-10.

Physics

1

Atmospheric Models, Atmospheric Radiation, Atmospheric Scattering, Radiative Transfer, Laplace Transformation, Optical Thickness, Wiener Hopf Equations

Scientific paper

The transport equation for radiative transfer in semiinfinite atmosphere with no incident radiation and scattering was solved exactly by a method based on the use of the Laplace transform and the Wiener-Hopf technique. The solution was used to determine the emergent radiation intensity and the intensity at any optical depth. The emergent radiation intensity obtained was found to agree with that of Chandrasekhar (1990).

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