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On the anticorrelation between the He-3/He-4 ratio and proton intensity in He-3 rich flaresA model is presented which can explain the observed anticorrelation between the size of the 3He/4He abundance ratio at greater than or approximately 10 MeV/nuc and the peak intensity of approximately 10 MeV protons in 3He rich events. If 3He is preaccelerated with respect to 4He prior to the main ion acceleration phase, and if the main ion acceleration phase has an effective injection cutoff which varies from flare to flare, the observed anticorrelation follows naturally.
Document ID
19810016490
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Pesses, M. E.
(Maryland Univ. College Park, MD, United States)
Date Acquired
August 11, 2013
Publication Date
January 1, 1981
Publication Information
Publication: Contrib. to the 17th Inter. Conf. on Cosmic Rays
Subject Category
Solar Physics
Accession Number
81N25025
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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