Optical conditions in a homogeneous spherical envelope

Details Optical conditions in a homogeneous spherical envelope Optical conditions in a homogeneous spherical envelope

Apr 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985velen....q..73k&link_type=abstract

Leningradskii Universitet, Vestnik, Matematika, Mekhanika, Astronomiia (ISSN 0024-0850), April 1985, p. 73-80. In Russian.

Statistics

Computation

Computational Astrophysics, Optical Paths, Radiant Flux Density, Radiative Transfer, Stellar Envelopes, Stellar Luminosity, Green'S Functions, Integral Equations, Light Scattering, Planetary Nebulae, Point Sources, Reflectance, Transmittance

Scientific paper

A method for calculating radiation fields in a homogeneous anisotropically scattering spherical stellar envelope with spherically symmetric distribution of sources is proposed. The method is based on integral relations between Green functions for radiative transfer in a spherical envelope and an infinite medium. An algorithm for calculating radiation intensities in an envelope with a central point source is considered as an example.

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