Mathematics
Scientific paper
Mar 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981kosis..19..249g&link_type=abstract
Kosmicheskie Issledovaniia, vol. 19, Mar.-Apr. 1981, p. 249-260. In Russian.
Mathematics
3
Atmospheric Composition, Atmospheric Models, Atmospheric Temperature, Mathematical Models, Thermosphere, Atmospheric Chemistry, Carbon Dioxide Concentration, Gas Density, Infrared Radiation, Molecular Spectra, Temperature Distribution
Scientific paper
A numerical model of the thermal state of the thermosphere is presented, taking into account infrared radiation in the 1.27-63 micron range (including the vibration-rotation bands of NO, CO2, OH, and O3). The vertical profiles of gas density and temperature determined by the present model agree well with corresponding profiles from the CIRA-72 and Jacchia-77 models. A numerical experiment was used to determine the CO2 (01/0/0) deactivation rate constant in collisions with O at 180-400 K. It is shown that the main energy sink from the thermosphere in the 90-180 km region is determined by infrared radiation in the 15-micron band of CO2 and the 5.3-micron band of NO.
Gordiets B. F.
Kulikov Iu. N.
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