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The Vega balloon experimentsThe goals of the Vega-1 and -2 experiments were to trace the large- and small-scale motions, measure the turbulent heat and momentum flow in the cloud layer, and determine the physical parameters of the Venus atmosphere. The arrangement of the balloon-probe payload, the balloon-deployment sequence, and the balloon flight paths are described. The balloons drifted latitudinally in the Venus atmosphere about one-third the way around the planet at a height of 53-54 km and speeds close to 67 m/sec. The balloon-probe signals, recorded on earth by radio telescopes of ten countries, are being processed.
Document ID
19870032278
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Sagdeev, R. Z.
(Academy of Sciences (USSR) Moscow, Ussr)
Linkin, V. M.
(AN SSSR, Institut Kosmicheskikh Issledovanii, Moscow, USSR)
Kremnev, R. S.
(AN SSSR, Sovet Interkosmos, Moscow, USSR)
Blamont, J. E.
(CNES, Paris, France)
Preston, R. A.
(California Institute of Technology, Jet Propulsion Laboratory, Pasadena)
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
87A19552
Distribution Limits
Public
Copyright
Other

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