Computer Science
Scientific paper
Sep 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989kosis..27..761k&link_type=abstract
Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 27, Sept.-Oct. 1989, p. 761-764. In Russian.
Computer Science
Balloon Flight, Orography, Vega Project, Venus Atmosphere, Wave Interaction, Atmospheric Temperature, Mountains, Vertical Distribution, Wind Velocity, Zonal Flow (Meteorology)
Scientific paper
A preliminary analysis of data from the Vega balloon experiment pointed to a complex nature of the balloon movements in the Venus atmosphere: relatively quiet motion alternated with sharp changes in the vertical wind-velocity component with an amplitude of a few meters per second. Numerical simulation results indicate that variations of the planetary relief have an influence on the formation of spatial wave structures of the field of the vertical velocity component formed above a mass if at a height of 54 km.
Kerzhanovich Viktor V.
Kurganskii M. V.
Linkin V. M.
Ozorovich Iu. R.
Pertsev Nikolay
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