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The production of He-3 and heavy ion enrichment in He-3-rich flares by electromagnetic hydrogen cyclotron wavesA new model is presented for the production of He-3 and heavy ion enrichments in He-3-rich flares using a direct single-stage mechanism. In analogy with the production of electromagnetic hydrogen cyclotron waves in earth's aurora by electron beams, it is suggested that such waves should exist in the electron acceleration region of impulsive solar flares. Both analytic and test-particle models of the effect of such waves in a nonuniform magnetic field show that these waves can selectively accelerate He-3 and heavy ions to MeV energies in a single-stage process, in contrast to other models which require a two-stage mechanism.
Document ID
19920057179
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Temerin, M.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Roth, I.
(California, University Berkeley, United States)
Date Acquired
August 15, 2013
Publication Date
June 1, 1992
Publication Information
Publication: Astrophysical Journal, Part 2 - Letters
Volume: 391
Issue: 2 Ju
ISSN: 0004-637X
Subject Category
Solar Physics
Accession Number
92A39803
Funding Number(s)
CONTRACT_GRANT: NSF ATM-89-18774
CONTRACT_GRANT: NAG5-1098
CONTRACT_GRANT: NAGW-1626
Distribution Limits
Public
Copyright
Other

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