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Enrichment of heavy nuclei in He-3-rich flaresIMP-7 observations of five solar-flare particle events characterized by He-3 enrichment are reported which show that such events are also enriched in nuclei with charges (Z) of at least 6. The ratio of these nuclei to H-1 at approximately 3 MeV/nucleon was found to be enriched by about 10 to 100 times, while the ratio with respect to He-4 was enriched by about 3 to 30 times. It is suggested that the simultaneous enhancement of He-3 and the heavier nuclei as well as the absence of H-2 and H-3 during the observed events may be partly due to a preferential acceleration process which depends on the ratio of the square of the charge to the atomic weight of the nuclei.
Document ID
19760029786
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Hurford, G. J.
(California Inst. of Tech. Pasadena, CA, United States)
Mewaldt, R. A.
(California Inst. of Tech. Pasadena, CA, United States)
Stone, E. C.
(California Inst. of Tech. Pasadena, CA, United States)
Vogt, R. E.
(California Institute of Technology Pasadena, Calif., United States)
Date Acquired
August 8, 2013
Publication Date
October 15, 1975
Publication Information
Publication: Astrophysical Journal
Volume: 201
Subject Category
Solar Physics
Accession Number
76A12752
Funding Number(s)
CONTRACT_GRANT: NSF GA-43200
CONTRACT_GRANT: NGR-05-002-160
CONTRACT_GRANT: NAS5-11066
Distribution Limits
Public
Copyright
Other

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