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Statics of the nightside Jovian plasma sheetData are analyzed from the low energy charged particle (LECP) and magnetic field (MAG) experiments on the Voyager 2 spacecraft that demonstrate that the configuration of the Jovian plasma sheet at distances of about .80 to about 120 Jupiter radii is determined by ions (protons and heavier nuclei) of energies greater than approximately 30 keV. The energy densities of these ions are sufficient to provide the diamagnetic depressions in the magnetic field strengths observed as the spacecraft crossed the Jovian plasma sheet. The particle bulk direction of motion is predominantly across the local magnetic field, consistent with that expected from corotation of the planetary magnetic field.
Document ID
19810025890
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Lanzerotti, L. J.
(Bell Telephone Labs., Inc. Murray Hill, NJ, United States)
Maclennan, C. G.
(Bell Telephone Laboratories, Inc. Murray Hill, N.J., United States)
Krimigis, S. M.
(Johns Hopkins University Applied Physics Laboratory, Laurel, Md., United States)
Armstrong, T. P.
(Kansas, University Lawrence, Kan., United States)
Behannon, K.
(Bell Telephone Labs., Inc. Murray Hill, NJ, United States)
Ness, N. F.
(NASA Goddard Space Flight Center Greenbelt, Md., United States)
Date Acquired
August 11, 2013
Publication Date
October 1, 1980
Publication Information
Publication: Geophysical Research Letters
Volume: 7
Subject Category
Lunar And Planetary Exploration
Accession Number
81A10294
Funding Number(s)
CONTRACT_GRANT: NASA TASK I
CONTRACT_GRANT: N00024-78-C-5384
Distribution Limits
Public
Copyright
Other

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