Resonance Line Transfer Calculations by Doubling Thin Layers. II. The Use of the R II Redistribution Function

Details Resonance Line Transfer Calculations by Doubling Thin Layers. II. The Use of the R II Redistribution Function Resonance Line Transfer Calculations by Doubling Thin Layers. II. The Use of the R II Redistribution Function

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...346..489w&link_type=abstract

Astrophysical Journal v.346, p.489

Astronomy and Astrophysics

Astronomy

10

Analytical Methods, Line Formation, Planets: Atmospheres, Radiative Transfer

Scientific paper

The doubling technique for the solution of resonance line scattering problems, which was developed by Yelle and Wallace, has been applied to the problem where the RII redistribution function is appropriate, both neglecting and including polarization. With the constraint that the atmosphere is illuminated from the zenith, the only difficulty of consequence was that of performing precise frequency integrations over the line profiles. With that problem solved, it is apparent that it is no longer necessary to use the Monte Carlo method to solve this class of problem.

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