Relationship between spherical albedo and the observed characteristics of a planetary atmosphere

Details Relationship between spherical albedo and the observed characteristics of a planetary atmosphere Relationship between spherical albedo and the observed characteristics of a planetary atmosphere

Mar 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986avest..20....5f&link_type=abstract

Astronomicheskii Vestnik (ISSN 0320-930X), vol. 20, Jan.-Mar. 1986, p. 5-14. In Russian.

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Albedo, Atmospheric Optics, Optical Reflection, Planetary Atmospheres, Absorption Spectra, Approximation, Computational Astrophysics, Jupiter Atmosphere, Molecular Absorption, Optical Properties, Radiative Transfer, Saturn Atmosphere

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Semiempirical dependences of the geometrical albedo and the reflection coefficient at the center of the planetary disk on the spherical albedo are found. Approximate formulas are used to study nonstationary analogs of these quantities. It is noted that these quantities can be used to examine radiative transfer in molecular absorption bands. The results are particularly applicable to Jupiter and Saturn.

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