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Pion-decay radiation and two-phase acceleration in the June 3, 1982 solar flareThe June 3, 1982 flare is unique in the wealth of observed neutron, gamma-ray and energetic-particle emission that it produced. Using calculations of high-energy emissions to fit the various time-dependent gamma-ray fluxes, a self-consistent interaction model for the June 3 flare is constructed in which the observed fluxes are produced by two distinct particle populations with different acceleration and interaction time histories as well as different but time-independent energy spectra. The two populations are associated with first- and second-phase particle acceleration, respectively.
Document ID
19870052725
Document Type
Reprint (Version printed in journal)
Authors
Ramaty, R. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Dermer, C. D. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Murphy, R. J. (Maryland, University College Park, United States)
Date Acquired
August 13, 2013
Publication Date
January 1, 1986
Publication Information
Publication: Advances in Space Research
Volume: 6
Issue: 6, 19
ISSN: 0273-1177
Subject Category
SOLAR PHYSICS
Distribution Limits
Public
Copyright
Other