Mathematics
Scientific paper
May 1976
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976kosis..14..417g&link_type=abstract
Kosmicheskie Issledovaniia, vol. 14, May-June 1976, p. 417-427. In Russian.
Mathematics
Absorption Spectra, Atmospheric Attenuation, Infrared Radiation, Lower Atmosphere, Venus Atmosphere, Atmospheric Windows, Attenuation Coefficients, Carbon Dioxide, Error Analysis, Fine Structure, Mathematical Models, Optimization, Spectral Line Width, Water Vapor
Scientific paper
The method of calculating the rotational structure of absorption bands, a minimization method for determining the line shapes of CO2, a quasi-statistical model taking account of spectral line width variations and a method for calculating the absorption of water vapor are described and applied to the calculation of absorption coefficients for the subcloud atmosphere of Venus in the wavelength range 0.8-100 microns. It is noted that further theoretical and experimental studies of the absorption spectra of CO2 and H2O, especially in the infrared transparence windows of the Venus atmosphere, are necessary.
Galtsev A. P.
Osipov Vladimir M.
Shari V. P.
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