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Comparison of plasma wave measurements in the bow shocks at Earth, Jupiter, Saturn, Uranus and NeptunePlasma wave measurements from the Voyager 2 crossing of Neptune's bow shock are presented and compared with measurements from the bow shocks of Earth, Jupiter, Saturn, and Uranus. The wave amplitudes above 0.01fp, when normalized to the solar wind ion thermal energy density at each planet, are significantly higher at the outer planets than at Earth. Despite the differences in amplitude, the shock spectra of all the planets can be fitted to curves of similar form in this frequency range. The total normalized electric field energy densities exhibit an exponential dependence on ion thermal Mach number, Magnetosheath wave energies are comparable at all of the planets when normalized to the downstream plasma pressure.
Document ID
19900065476
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Moses, S. L.
(TRW, Inc. Redondo Beach, CA, United States)
Coroniti, F. V.
(TRW, Inc. Redondo Beach, CA, United States)
Kennel, C. F.
(TRW Space and Technology Group Redondo Beach, CA, United States)
Kurth, W. S.
(TRW, Inc. Redondo Beach, CA, United States)
Gurnett, D. A.
(Iowa, University Iowa City, 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
Accession Number
90A52531
Funding Number(s)
CONTRACT_GRANT: JPL-957723
CONTRACT_GRANT: JPL-957805
Distribution Limits
Public
Copyright
Other

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