The transfer of radiation by an emitting atmosphere. VI

Details The transfer of radiation by an emitting atmosphere. VI The transfer of radiation by an emitting atmosphere. VI

Jun 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...238.1047h&link_type=abstract

Astrophysical Journal, Part 1, vol. 238, June 15, 1980, p. 1047-1053.

Astronomy and Astrophysics

Astrophysics

Atmospheric Radiation, Radiation Distribution, Radiative Transfer, Stellar Atmospheres, Stellar Radiation, Light Scattering, Optical Thickness, Polynomials, Transfer Functions

Scientific paper

The transfer of radiation by a plane-parallel atmosphere containing a polynomial distribution of emission sources is solved using the method of doubling, combined with symmetry principles. Calculational results are presented for linear and quadratic source distributions embedded in a medium that scatters light in accordance with the spherical phase function with albedo.

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