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Earth-Based Radio Tracking of the Galileo Probe for Jupiter Wind EstimationAlthough the Galileo probe was designed to communicate only to the orbiter, the probe radio signal was detected at two Earth-based radio observatories where the signal was a billion times weaker. The measured signal frequency was used to derive a vertical profile of the jovian zonal wind speed. Due to the mission geometry, the Earth-based wind estimates are less sensitive to descent trajectory errors than estimates based on probe-orbiter Doppler measurements. The two estimates of wind profiles agree qualitatively; both show high wind speeds at all depths sampled.
Document ID
19990014559
Acquisition Source
Jet Propulsion Laboratory
Document Type
Reprint (Version printed in journal)
Authors
Folkner, W. M.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Preston, R. A.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Border, J. S.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Navarro, J.
(National Radio Astronomy Observatory Socorro, NM United States)
Wilson, W. E.
(Australia Telescope National Facility Epping, Australia)
Oestreich, M.
(Australia Telescope National Facility Epping, Australia)
Date Acquired
August 19, 2013
Publication Date
January 31, 1997
Publication Information
Publication: Science
Volume: 275
ISSN: 0036-8423
Subject Category
Communications And Radar
Distribution Limits
Public
Copyright
Other

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