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Carbon-poor solar flare eventsEnergetic particle flux enhancements over the period October 1973 - December 1977 were surveyed using ULET sensor on the IMP-8 spacecraft. During the four year period the most extreme periods of Fe enrichment compared to oxygen were during solar flare events in February 1974 and May 1974. In these same events, the carbon abundance with respect to oxygen was significantly depleted when compared with a value C:0 is approximately 0.45:1 for typical solar flares. These observations, taken together with previously reported He-3 enrichment in these events, give strong evidence for the importance of a wave-particle interaction in the pre-injection heating of the ambient matter.
Document ID
19790013810
Acquisition Source
Legacy CDMS
Document Type
Contractor Report (CR)
Authors
Mason, G. M.
(Maryland Univ. College Park, MD, United States)
Gloeckler, G.
(Maryland Univ. College Park, MD, United States)
Hovestadt, D.
(Max-Planck-Inst. fuer Physik und Astrophysik Munich, Germany)
Date Acquired
September 3, 2013
Publication Date
February 20, 1979
Subject Category
Solar Physics
Report/Patent Number
NASA-CR-158470
TR-79-065
PP-79-143
Report Number: NASA-CR-158470
Report Number: TR-79-065
Report Number: PP-79-143
Accession Number
79N21981
Funding Number(s)
CONTRACT_GRANT: NGL-21-002-224
CONTRACT_GRANT: NAS5-11063
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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