Solution of the transfer equation in a scattering atmosphere with spherical symmetry

Details Solution of the transfer equation in a scattering atmosphere with spherical symmetry Solution of the transfer equation in a scattering atmosphere with spherical symmetry

Mar 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975ap%26ss..33..245m&link_type=abstract

Astrophysics and Space Science, vol. 33, Mar. 1975, p. 245-251.

Computer Science

Numerical Analysis

4

Atmospheric Scattering, Chromosphere, Compton Effect, Radiative Transfer, Solar Atmosphere, Approximation, Atmospheric Density, Atmospheric Models, Boundary Value Problems, Computer Techniques, Integral Equations, Numerical Analysis, Partial Differential Equations

Scientific paper

An exact formal solution of the n-approximation radiative transfer
equations is obtained for Compton scattering in a spherically symmetric
atmosphere. The simple case of a single chromospheric layer where the
density is inversely proportional to the radius is analyzed, and
solutions for 20 approximations equations are obtained with a computer.

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