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On the origin of the pion-decay radiation in the 1982 June 3 solar flareThe June 3, 1982 flare produced a wealth of observed gamma-ray, energetic particle, and neutron emissions. It is shown that the predictions of an interaction model developed for the June 3 flare by Murphy, Dermer, and Ramaty (1987) compare favorably with new data on the time-dependent flux on pion-decay emission from this flare. It is concluded that the particles which produced the bulk of the pions could have the same origin as the particle observed in interplanetary space from the June 3 flare.
Document ID
19870052052
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/184888
Authors
Ramaty, R. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Murphy, R. J. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Dermer, C. D. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 13, 2013
Publication Date
May 1, 1987
Publication Information
Publication: Astrophysical Journal, Part 2 - Letters to the Editor
Volume: 316
ISSN: 0004-637X
Subject Category
Solar Physics
Accession Number
87A39326
Funding Number(s)
CONTRACT_GRANT: NAG5-723
CONTRACT_GRANT: NGR-21-002-316
Distribution Limits
Public
Copyright
Other

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