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Plasma effects on the interaction of a comet with JupiterI consider some plasma effects to be expected when the fragments of Comet Shoemaker-Levy 9 crash into Jupiter. Emphasis is put on pre-impact effects, and on the possibility of significant radio emission. It is shown than an ionizing shock will develop at altitudes below about 600 km, and that significant ionization will exist above that altitude. The incoming comet and its surroundings will then represent a rapidly moving conductor in a strong magnetic field and will induce large currents in Jupiter's magnetosphere, similar both qualitatively and quantitatively to a way in which Io interacts with Jupiter's magnetic field and with the plasma of the torus. This process is thought to be involved in the generation of decametric radiation, so that the impact of the comet may also produce such radiation. The power involved in this interaction is estimated to be at least 1/15th of the power due to Io, and its duration to be for 10-20 s before the comet's impact with the surface of Jupiter.
Document ID
19950043542
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Kellogg, Paul J.
(University of Minnesota, Minneapolis, MN United States)
Date Acquired
August 16, 2013
Publication Date
June 1, 1994
Publication Information
Publication: Geophysical Research Letters
Volume: 21
Issue: 11
ISSN: 0094-8276
Subject Category
Astrophysics
Accession Number
95A75141
Funding Number(s)
CONTRACT_GRANT: NAS5-31219
Distribution Limits
Public
Copyright
Other

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