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Plasma convection in Neptune's magnetosphereThe magnetosphere of Neptune changes its magnetic configuration continuously as the planet rotates, leading to a strong modulation of the convection electric field. Even though the corotation speed is considerably larger, the modulation causes the small convection speed to have a cumulative effect, much like the acceleration of particles in a cyclotron. A model calculation shows that plasma on one side of the planet convects out of the magnetosphere in a few planetary rotations, while on the other side it convects slowly planetward. The observation of nitrogen ions from a Triton plasma torus may provide a critical test of the model.
Document ID
19900065483
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Selesnick, R. S.
(California Institute of Technology Pasadena, 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
90A52538
Funding Number(s)
CONTRACT_GRANT: NAS7-918
CONTRACT_GRANT: NGR-05-002-160
Distribution Limits
Public
Copyright
Other

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