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Voyager 2 plasma ion observations in the magnetosphere of UranusPositive ion measurements in the magnetosphere of Uranus have been made by the Voyager 2 plasma science experiment. The paper presents an overview of the entire data set and a detailed analysis of the observations from the inner magnetosphere which complements and extends results reported elsewhere. Densities and temperatures are obtained from an analysis which incorporates details of the instrumental response. These results are then used to calculate flux tube particle and energy content to support the hypothesis that the plasma transport is controlled by a solar wind-driven magnetospheric convection system. Variations in the flux tube content suggest both a local source of plasma, produced from the neutral hydrogen corona of Uranus, and a nonlocal source, convected inwared and heated by adiabatic compression. In each case a proton composition is inferred. Sharp boundaries in the high-energy (approximately 1 keV) plasma population are interpreted in terms of the spatial extent of the magnetospheric convection, with significant shielding of the convection electric field. The convection theory is also used in a simulation of the low-energy (approximately 10 eV) ion component using the neutral hydrogen source, resulting in distribution functions which qualitatively agree with the observations.
Document ID
19880039609
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Selesnick, Richard S.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Mcnutt, Ralph L., Jr.
(MIT Cambridge, MA, United States)
Date Acquired
August 13, 2013
Publication Date
December 30, 1987
Publication Information
Publication: Journal of Geophysical Research
Volume: 92
ISSN: 0148-0227
Subject Category
Lunar And Planetary Exploration
Accession Number
88A26836
Funding Number(s)
CONTRACT_GRANT: JPL-953733
Distribution Limits
Public
Copyright
Other

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