Monte Carlo calculations of resonance-line formation in a plane layer

Details Monte Carlo calculations of resonance-line formation in a plane layer Monte Carlo calculations of resonance-line formation in a plane layer

Oct 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982pazh....8..566v&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 8, Sept. 1982, p. 566-572) Soviet Astronomy Letters (ISSN 0360-0327), vol. 8, Sept.-Oct

Astronomy and Astrophysics

Astronomy

Electromagnetic Scattering, Monte Carlo Method, Photon Beams, Planetary Atmospheres, Radiative Transfer, Resonance Lines, Optical Thickness, Particle Collisions, Particle Trajectories, Radiation Distribution, Reflected Waves

Scientific paper

Spectra are calculated for the radiation emerging from a plane layer in which a parallel beam of incident photons are scattered, for two cases: complete and incomplete frequency redistribution. If the incident photons are limited to the central frequency of a line, the reflected radiation will have different spectra in these two cases. The dependence of the source function (distribution of secondary sources within the layer) on the angle of incidence of the external photon beam is determined. The transmissivity and number of collisions are calculated as functions for the optical thickness of the layer.

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