Infrared emission of Venus - Approximate methods for calculating spectra in the absorption bands of atmospheric gases

Details Infrared emission of Venus - Approximate methods for calculating spectra in the absorption bands of atmospheric gases Infrared emission of Venus - Approximate methods for calculating spectra in the absorption bands of atmospheric gases

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985kosis..23..259m&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 23, Mar.-Apr. 1985, p. 259-267. In Russian.

Physics

1

Absorption Spectra, Gas Spectroscopy, Infrared Spectra, Planetary Radiation, Venus Atmosphere, Carbon Dioxide, Spectral Bands, Sulfur Dioxides, Water

Scientific paper

Approximate methods for calculating synthetic spectra in the H2O, CO2, and SO2 absorption bands are described which are used for a quantitative interpretation (chemical analysis and determination of cloud-layer parameters) of results of the Venera 15 and 16 infrared experiment. A simplified version of the line-by-line method is used for H2O; an equidistant-line method is used for CO2; and the overlapping-line method is used for SO2.

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