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Anomalous abundances of solar energetic particles and coronal gas: Coulomb effects and First Ionization Potential (FIP) orderingThe first ionization potential (FIP) ordering of elemental abundances in solar energetic particles and in the corona which can both be explained Coulomb effects is discussed. Solar energetic particles (SEP) and coronal gas have anomalous abundances relative to the photosphere. The anomalies are similar in both cases: which led to the conclusion that SEP acceleration is not selective, but merely preserves the source abundances. It is argued that SEP acceleration can be selective, because identical selectivity operates to determine the coronal abundances. The abundance anomalies are ordered by first ionization potential (FIP).
Document ID
19850026478
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Mullan, D. J.
(Franklin Inst. Newark, DE, United States)
Date Acquired
August 12, 2013
Publication Date
August 1, 1985
Publication Information
Publication: 19th Intern. Cosmic Ray Conf - Vol. 4
Subject Category
Solar Physics
Report/Patent Number
SH-2.1-10
Report Number: SH-2.1-10
Accession Number
85N34791
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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