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Abstract

Based 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.

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Published In

Science
Volume 182 | Issue 4119
28 December 1973

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Published in print: 28 December 1973

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Stanley D. Shawhan
Department of Physics and Astronomy, University of Iowa, Iowa City 52242
Donald A. Gurnett
Department of Physics and Astronomy, University of Iowa, Iowa City 52242
Richard F. Hubbard
Department of Physics and Astronomy, University of Iowa, Iowa City 52242
Glenn Joyce
Department of Physics and Astronomy, University of Iowa, Iowa City 52242

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  1. Radiation Belts of Jupiter: A Second Look, Science, 188, 4187, (465-467), (1975)./doi/10.1126/science.188.4187.465
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