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Preacceleration in collapsing magnetic neutral sheets and anomalous abundances of solar flare particlesLevine's (1974) concept of a collapsing magnetic neutral sheet which can accelerate ambient protons to several times the mean thermal speed, provided that the collapse time scale is shorter than the proton Coulomb loss time, is applied to heavier elements in an investigation of the composition of the particles which can be accelerated by such a sheet. Tables of ionization equilibrium are combined with the thermal structure of a constant pressure loop in order to calculate phi sub x (the fraction of an element x which is accelerated) of 18 heavy elements, from carbon to nickel which satisfy a maximum-ionization criterion. Normalizing phi sub x to oxygen, it is found that relative to the composition of the ambient materials, C and N can be depleted by factors of up to 2-10, while other heavy elements, along with hydrogen, are enhanced. The numerical results obtained are qualitatively similar to anomalous abundances reported among solar flare particles.
Document ID
19820031832
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Mullan, D. J.
(Franklin Institute, Bartol Research Foundation, Newark DE, United States)
Levine, R. H.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Date Acquired
August 10, 2013
Publication Date
October 1, 1981
Publication Information
Publication: Astrophysical Journal Supplement Series
Volume: 47
Subject Category
Solar Physics
Accession Number
82A15367
Funding Number(s)
CONTRACT_GRANT: NSF ATM-78-20936-01
CONTRACT_GRANT: NAS5-3949
CONTRACT_GRANT: NSG-5315
Distribution Limits
Public
Copyright
Other

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