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Pick-up ions at PlutoMethane molecules escaping from Pluto's atmosphere are ionized, and the resulting ions are picked up by the solar wind. The mass loading associated with this ion pick-up can produce a cometlike interaction of the solar wind with Pluto. Heavy ion gyroradii are as large as a half million km in the weak interplanetary magnetic field that exists at 30 AU, which is about an order of magnitude larger than the size of the 'interaction region'. We have calculated velocity space distributions of pick-up ions using numerically determined ion trajectories. The predicted pick-up ion fluxes are high enough to be detectable by standard charged particle detectors as far upstream of Pluto as 10 exp 6 km.
Document ID
19930051821
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Kecskemety, K.
(NASA Headquarters Washington, DC United States)
Cravens, T. E.
(Kansas Univ. Lawrence, United States)
Date Acquired
August 16, 2013
Publication Date
April 9, 1993
Publication Information
Publication: Geophysical Research Letters
Volume: 20
Issue: 7
ISSN: 0094-8276
Subject Category
Lunar And Planetary Exploration
Accession Number
93A35818
Funding Number(s)
CONTRACT_GRANT: NAGW-2162
CONTRACT_GRANT: NSF ATM-89-96116
CONTRACT_GRANT: NAGW-1588
Distribution Limits
Public
Copyright
Other

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