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The VEGA Venus balloon experimentIn June 1985, two instrumented balloons were placed in the atmosphere of Venus as part of the VEGA mission. Each balloon traveled about 30 percent of the way around the planet at a float altitude near 54 kilometers. In situ sensors measured pressure, temperature, vertical wind velocity, cloud particle backscatter, ambient light level, and frequency of lightning. A ground-based network of 20 radio antennas tracked the balloons by very long baseline interferometry (VLBI) techniques to monitor the Venus winds. The history, organization, and principal characteristics of this international balloon experiment are described.
Document ID
19860046078
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Sagdeev, R. Z.
(Institute of Space Research Moscow, Ussr)
Linkin, V. M.
(AN SSSR Institut Kosmicheskikh Issledovanii, Moscow, Ussr)
Blamont, J. E.
(CNES Paris, France)
Preston, R. A.
(California Institute of Technology Jet Propulsion Laboratory, Pasadena, United States)
Date Acquired
August 12, 2013
Publication Date
March 21, 1986
Publication Information
Publication: Science
Volume: 231
ISSN: 0036-8075
Subject Category
Astronautics (General)
Report/Patent Number
ISSN: 0036-8075
Accession Number
86A30816
Distribution Limits
Public
Copyright
Other

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