Physics
Scientific paper
Sep 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980kosis..18..775t&link_type=abstract
Kosmicheskie Issledovaniia, vol. 18, Sept.-Oct. 1980, p. 775-782. In Russian.
Physics
1
Atmospheric Turbulence, Radio Occultation, Turbulence Effects, Venera Satellites, Venus Atmosphere, Amplitude Distribution Analysis, Decametric Waves, Equatorial Regions, Height, Polar Regions, Solar Position, Temperate Regions, Venera 10 Satellite, Venera 9 Satellite
Scientific paper
Experiments involving the radio occultation of the Venus atmosphere are described. Height profiles of amplitude fluctuation intensity are obtained for the polar, equatorial, and midlatitude regions of the planet. These data are used to determine the height profiles of atmospheric turbulence. In the upper turbulence region (56-70 km), the sturcture characteristic of turbulence varies from day to day in the range (1.6-2.6) x 10 to the -8th/cm to the 1/3.
Efimov Alexander I.
Iakovlev O. I.
Timofeeva T. S.
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