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Meteorological data along the Vega 1, 2 float pathsThe Vega balloons transmitted in situ measurements of pressure, temperature, vertical wind velocity relative to the balloon craft, cloud-particle backscatter coefficient, and ambient light level in the Venus middle cloud layer. Doppler tracking has yielded estimates for the velocities of atmospheric motion.
Document ID
19870032282
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Sagdeev, R. Z. (Academy of Sciences (USSR) Moscow, Ussr)
Linkin, V. M. (Academy of Sciences (USSR) Moscow, Ussr)
Kerzhanovich, V. V. (Academy of Sciences (USSR) Moscow, Ussr)
Lipatov, A. N. (Academy of Sciences (USSR) Moscow, Ussr)
Shurupov, A. A. (Academy of Sciences (USSR) Moscow, Ussr)
Terterashvili, A. V. (AN SSSR, Institut Kosmicheskikh Issledovanii, Moscow, USSR Moscow, Ussr)
Blamont, J. E. (CNES, Paris, France)
Preston, R. A. (Academy of Sciences (USSR))
Elson, L. S. (California Institute of Technology, Jet Propulsion Laboratory, Pasadena)
Ragent, B. (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
87A19556
Distribution Limits
Public
Copyright
Other

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