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Io-accelerated electrons - Predictions for Pioneer 10 and Pioneer 11Based on a model in which electrons are accelerated to energies of 100 kiloelectron volts through sheaths associated with Io, predictions are made about energetic electrons to be observed by Pioneer 10 and Pioneer 11 in the Jovian magnetosphere. This energetic electron source may be distinguishable from the solar wind diffusion source by the radial flux profile and by the characteristic electron energies.
Document ID
19740033038
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Shawhan, S. D.
Gurnett, D. A.
Hubbard, R. F.
Joyce, G.
(Iowa, University Iowa City, Iowa, United States)
Date Acquired
August 7, 2013
Publication Date
December 28, 1973
Publication Information
Publication: Science
Volume: 182
Subject Category
Space Sciences
Accession Number
74A15788
Funding Number(s)
CONTRACT_GRANT: NGL-16-001-043
CONTRACT_GRANT: NGL-16-001-002
CONTRACT_GRANT: NSF GA-31676
Distribution Limits
Public
Copyright
Other

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