H-function for three-term scattering indicatrix

Details H-function for three-term scattering indicatrix H-function for three-term scattering indicatrix

Jul 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.113..119k&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 113, no. 1, July 1985, p. 119-123.

Astronomy and Astrophysics

Astrophysics

1

Atmospheric Scattering, Eigenvectors, Scattering Functions, Integral Equations, Nonlinear Equations

Scientific paper

In solving the equation of transfer for a semiinfinite, plane-parallel atmosphere, the emergent intensity is largely obtained in terms of Chandrasekhar's H-function; in cases where the H-function is within an integral sign, a good approximate form is needed to minimize computational effort. The Karanjai and Sen (1971) H-function approximation for isotropic scattering is presently extended to the case of the three-term scattering indicatrix.

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