Exact Solution of the Transport Equation for Radiative Transfer with Scattering Albedo ω0 < 1 using the Laplace Transform and the Wiener-Hopf Technique and an Expression of H-Function

Details Exact Solution of the Transport Equation for Radiative Transfer with Scattering Albedo ω0 < 1 using the Laplace Transform and the Wiener-Hopf Technique and an Expression of H-Function Exact Solution of the Transport Equation for Radiative Transfer with Scattering Albedo ω0 < 1 using the Laplace Transform and the Wiener-Hopf Technique and an Expression of H-Function

Jan 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979ap%26ss..60...49d&link_type=abstract

Astrophysics and Space Science, Volume 60, Issue 1, pp.49-58

Astronomy and Astrophysics

Astrophysics

3

Scientific paper

We have considered the transport equation for radiative transfer to a problem in semi-infinite non-conservative atmosphere with no incident radiation and scattering albedo ω0 < 1. Usint the Laplace transform and the Wiener-Hopf technique, we have determined the emergent intensity and the intensity at any optical depth. We have obtained theH-function of Dasgupta (1977) by equating the emergent intensity with the intensity at zero optical depth.

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