The structure of the Venus atmosphere according to optical measurements carried out on Venera 11, 13, and 14

Details The structure of the Venus atmosphere according to optical measurements carried out on Venera 11, 13, and 14 The structure of the Venus atmosphere according to optical measurements carried out on Venera 11, 13, and 14

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988avest..22..262d&link_type=abstract

Astronomicheskii Vestnik (ISSN 0320-930X), vol. 22, July-Sept. 1988, p. 262-271. In Russian.

Physics

Optics

1

Atmospheric Optics, Optical Measurement, Venera Satellites, Venus Atmosphere, Atmospheric Stratification, Infrared Astronomy, Radiative Transfer, Visible Spectrum

Scientific paper

A strict theory of the radiation transfer in the multilayer atmosphere is used for the interpretation of Venera 11, 13 and 14 published measurements of radiation field in the Venus atmosphere. For the spectral interval 0.45 - 1.01 μm the optical parameters of the atmosphere are determined. A comparison with previous results obtained mainly by means of approximate methods is given.

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