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Multiply reflected standing Alfven waves in the Io torus - Pioneer 10 observationsObservations from the Voyager 1 pass by the Io flux tube strongly suggest that large amplitude standing Alfven waves are generated as Jovian plasma flows past Io. It has recently been proposed by Gurnett and Goertz (1981) that this Io generated standing Alfven wave system extends an appreciable way around the Io L-shell. Observations are presented here of magnetic perturbations found in the Pioneer 10 record as it crossed the Io L-shell. The field perturbations are found to be qualitatively consistent with the passage of the spacecraft through a standing Alfven wave pattern. The observations suggest an Alfven Mach number of 0.03, which is 1/5 the value inferred from Voyager 1 observations. This implies a lower plasma density at the time of the flyby of Pioneer 10.
Document ID
19820033454
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Walker, R.
(California Univ. Los Angeles, CA, United States)
Kivelson, M.
(California, University Los Angeles, CA, United States)
Date Acquired
August 10, 2013
Publication Date
December 1, 1981
Publication Information
Publication: Geophysical Research Letters
Volume: 8
Subject Category
Lunar And Planetary Exploration
Accession Number
82A16989
Funding Number(s)
CONTRACT_GRANT: NSG-7295
CONTRACT_GRANT: NSF ATM-79-23586
Distribution Limits
Public
Copyright
Other

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