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Gamma-ray, neutron, and hard X-ray studies and requirements for a high-energy solar physics facilityThe requirements for future high-resolution spatial, spectral, and temporal observation of hard X-rays, gamma rays and neutrons from solar flares are discussed in the context of current high-energy flare observations. There is much promise from these observations for achieving a deep understanding of processes of energy release, particle acceleration and particle transport in a complicated environment such as the turbulent and highly magnetized atmosphere of the active sun.
Document ID
19890040740
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Ramaty, R.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Dennis, B. R.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Emslie, A. G.
(Alabama, University Huntsville, United States)
Date Acquired
August 14, 2013
Publication Date
January 1, 1988
Publication Information
Publication: Solar Physics
Volume: 118
Issue: 1-2
ISSN: 0038-0938
Subject Category
Solar Physics
Accession Number
89A28111
Funding Number(s)
CONTRACT_GRANT: NAG5-500
CONTRACT_GRANT: NSF ATM-87-15195
CONTRACT_GRANT: NSF AST-83-51058
CONTRACT_GRANT: NAGW-294
Distribution Limits
Public
Copyright
Other

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