Computer Science
Scientific paper
Mar 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983kosis..21..211k&link_type=abstract
Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 21, Mar.-Apr. 1983, p. 211-217. In Russian.
Computer Science
2
Doppler Radar, Venera Satellites, Venus Atmosphere, Wind Profiles, Wind Velocity Measurement, Atmospheric Turbulence, Equatorial Atmosphere, Landing Modules, Radial Velocity, Radio Telemetry, Venus Clouds, Vertical Distribution, Wind Variations
Scientific paper
Vertical profiles of wind velocity in the Venus atmosphere were obtained through Doppler measurements of the velocities of the Venera-13 and Venera-14 probes. The vertical distribution of the zonal component of wind velocity is presented, and variations of the radial component of the velocity of the descent module near the lower boundary of the cloud layer are examined. The general character of velocity variations is shown to be associated with atmospheric turbulence: appreciable variations having a characteristic time of 20 sec and greater and amplitudes greater than 0.7-1 m/sec were observed in the cloud layer; below 45 km, velocity variations did not exceed 0.3-0.5 m/sec.
Antsibor N. M.
Kariagin V. P.
Kerzhanovich Viktor V.
Kustodiev V. D.
Makarov Iu. F.
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