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Numerical Modelling of the Reflection Spectrum of Venus in the Visual and Near Infrared Ranges

Published online by Cambridge University Press:  14 August 2015

E. M. Feigelson ,
N. L. Lukashevich ,
G. M. Krekov  and
G. A. Tytov
E. M. Feigelson
Affiliation:
Institute of Optics of the Atmosphere, Tomsk, U.S.S.R.
N. L. Lukashevich
Affiliation:
Institute of Applied Mathematics, Moscow, U.S.S.R.
G. M. Krekov
Affiliation:
Institute of Optics of the Atmosphere, Tomsk, U.S.S.R.
G. A. Tytov
Affiliation:
Institute of Optics of the Atmosphere, Tomsk, U.S.S.R.

Abstract

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The influence of a dense molecular atmosphere under a cloud layer on spectral albedo of a planet is investigated. The lengths of paths of protons in the clouds are calculated. Experimental spectral transmission functions were used to calculate gas absorption. The results are compared with experimental data.

Type
Part II Terrestrial Planets
Information
Symposium - International Astronomical Union , Volume 65: Exploration of the Planetary System , 1974 , pp. 185 - 189
Copyright
Copyright © Reidel 1974