Calculation of the thermal state of the Martian atmosphere

Details Calculation of the thermal state of the Martian atmosphere Calculation of the thermal state of the Martian atmosphere

Mar 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976kosis..14..265v&link_type=abstract

Kosmicheskie Issledovaniia, vol. 14, Mar.-Apr. 1976, p. 265-271. In Russian.

Physics

Atmospheric Temperature, Carbon Dioxide, Infrared Spectra, Mars Atmosphere, Atmospheric Attenuation, Atmospheric Stratification, Long Wave Radiation, Molecular Absorption, Near Infrared Radiation, Spectral Bands, Temperature Distribution, Vertical Distribution

Scientific paper

The transmission function of CO2 is calculated for a range of temperatures, pressures, and absorbing masses corresponding to physical conditions in the Martian atmosphere. Integral absorption in the near-IR bands of CO2 (2.7 and 4.3 microns) and in the 15-micron band is computed as a function of pressure and absorbing mass for temperatures of 200, 250, and 300 K. The transmission function obtained and temperature profiles observed in the Martian atmosphere are used to determine the ascending and descending longwave-radiation fluxes in that atmosphere.

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