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Hot plasma parameters in Neptune's magnetosphereThis paper presents values of particle spectral parameters and estimates of plasma densities, temperatures, and beta parameters, obtained with the Low Energy Charged Particle instrument during the Voyager 2 encounter with Neptune on August 24-25, 1989. In addition, trapped electron intensities are compared with the whistler mode stably trapped limits. The results revealed a very good inbound-outbound symmetry for both the proton and the electron profiles, suggesting that there was little dynamical activity in Neptune's magnetosphere during the Voyager encounter. The similarities and differences observed between Neptune and Uranus in the values of plasma density, pressure, and beta are discussed.
Document ID
19900065484
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Krimigis, S. M.
(Johns Hopkins Univ. Laurel, MD, United States)
Mauk, B. H.
(Johns Hopkins Univ. Laurel, MD, United States)
Cheng, A. F.
(Johns Hopkins Univ. Laurel, MD, United States)
Keath, E. P.
(Johns Hopkins Univ. Laurel, MD, United States)
Kane, M.
(Johns Hopkins University Laurel, MD, United States)
Date Acquired
August 14, 2013
Publication Date
September 1, 1990
Publication Information
Publication: Geophysical Research Letters
Volume: 17
ISSN: 0094-8276
Subject Category
Lunar And Planetary Exploration
Report/Patent Number
ISSN: 0094-8276
Accession Number
90A52539
Funding Number(s)
CONTRACT_GRANT: N00039-89-C-0001
CONTRACT_GRANT: N00039-89-C-5301
Distribution Limits
Public
Copyright
Other

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