The Venera 15 and 16 infrared experiment. II - Preliminary results on the determination of temperature profiles

Details The Venera 15 and 16 infrared experiment. II - Preliminary results on the determination of temperature profiles The Venera 15 and 16 infrared experiment. II - Preliminary results on the determination of temperature profiles

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985kosis..23..206s&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 23, Mar.-Apr. 1985, p. 206-220. In Russian.

Astronomy and Astrophysics

Astronomy

3

Atmospheric Temperature, Infrared Astronomy, Planetary Temperature, Spaceborne Experiments, Venera Satellites, Emission Spectra, Latitude, Spectral Bands, Vertical Distribution, Weighting Functions

Scientific paper

Thermal-emission spectra of Venus obtained by Venera 15 and 16 were used to determine the temperature profile in the Venus atmosphere at heights of 60-95 km. The obtained profiles show that the temperature decreases monotonically with increasing height inside the latitude zone of +, - 60 deg. At higher latitudes the atmosphere is warmer, and inversion or isothermal conditions are observed at a level of 10-100 mbar. Diurnal variations of temperature were not observed.

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