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Acceleration of heavy ions in the solar windThe preferential acceleration and heating of solar wind heavy ions by the resonant cyclotron interaction were studied. It is concluded that this interaction is incapable of producing the observed differential speeds for reasonable solar wind parameters.
Document ID
19840005050
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Isenberg, P. A. (New Hampshire Univ. Durham, NH, United States)
Date Acquired
August 12, 2013
Publication Date
November 1, 1983
Publication Information
Publication: JPL Solar Wind Five
Subject Category
Solar Physics
Accession Number
84N13118
Funding Number(s)
CONTRACT_GRANT: NAG5-130
CONTRACT_GRANT: NAGW-76
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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