The X-, Y-, and H-matrices for molecular scattering

Details The X-, Y-, and H-matrices for molecular scattering The X-, Y-, and H-matrices for molecular scattering

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ap%26ss.178..133v&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 178, no. 1, April 1991, p. 133-145.

Astronomy and Astrophysics

Astrophysics

6

Atmospheric Scattering, Molecular Excitation, Planetary Atmospheres, Diffuse Radiation, Matrices, Rayleigh Scattering

Scientific paper

The three matrices for conservative or nonconservative planetary atmospheres with molecular scattering can be found by means of a method based on Chandresekhar (1989) in which both the internal and external fields are calculated. By utilizing the intensity vector of the emergent radiation, the scattering and transmission matrices can be found, which are then transformed into the X-, Y-, and H-matrices. A sample of results is given, and the method is found to be useful for determining the relevant characteristics of molecular scattering.

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