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Small-scale turbulence in the Venus middle cloud layerMeasurements of the Doppler-velocity fluctuations indicated by the radio signals from the Vega balloons testify to strong turbulence in the nightside as well as the dayside Venus cloud layer. Wind speeds vary by up to 2 m/sec on time scales of 30-100 sec.
Document ID
19870032285
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Kerzhanovich, V. V. (Academy of Sciences (USSR) Moscow, Ussr)
Pichkhadze, K. M. (AN SSSR, Institut Kosmicheskikh Issledovanii, Moscow, USSR Moscow, Ussr)
Andreev, R. A. (AN SSSR, Institut Kosmicheskikh Issledovanii and Institut Radiotekhniki i Elektroniki, Moscow, USSR Moscow, Ussr)
Aleksandrov, Iu. N. (Academy of Sciences (USSR) Moscow, Ussr)
Armand, N. A. (AN SSSR, Institut Radiotekhniki i Elektroniki, Moscow, USSR Moscow, Ussr)
Hildebrand, C. E. (Academy of Sciences (USSR))
Preston, R. A. (California Institute of Technology, Jet Propulsion Laboratory, Pasadena)
Vorontsov, V. A. (Academy of Sciences (USSR))
Vyshlov, A. S. (Academy of Sciences (USSR))
Young, R. E. (NASA Ames Research Center, Moffett Field, CA)
Date Acquired
August 13, 2013
Publication Date
February 1, 1986
Publication Information
Publication: Soviet Astronomy Letters
Volume: 12
ISSN: 0360-0327
Subject Category
Lunar And Planetary Exploration
Report/Patent Number
ISSN: 0360-0327
Accession Number
87A19559
Distribution Limits
Public
Copyright
Other

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