Exact solution of a radiative transfer problem by the Laplace transform and Wiener-Hopf technique

Details Exact solution of a radiative transfer problem by the Laplace transform and Wiener-Hopf technique Exact solution of a radiative transfer problem by the Laplace transform and Wiener-Hopf technique

Oct 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ap%26ss.208..113k&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 208, no. 1, p. 113-123

Astronomy and Astrophysics

Astrophysics

Energy Distribution, Laplace Transformation, Radiative Transfer, Rayleigh Scattering, Reference Atmospheres, Boundary Conditions, Flux Density, Optical Thickness, Problem Solving

Scientific paper

The transfer equation for the case of grey scattering according to
Rayleigh's phase function in a semi-infinite axially symmetric
atmosphere is considered. The emergent intensity and the intensity at
any optical depth have been determined by the Laplace Transform and
Wiener-Hopf Technique.

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