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Evidence for delayed second phase acceleration in solar flaresData gathered on solar gamma-ray events by the gamma-ray spectrometer on board the HEAO-3 satellite are discussed. Measurements were made of both hard X-ray and gamma-ray events. A total of 37 flare-like incidences were detected from October 1979 to July 1980. Power law spectra were fitted to the flux energies exceeding 420 keV. The appearance of two events with a 30 sec interval between radiation peaks, a slow rise and quick decay of the high energy component, and the softening of the low energy component are taken for evidence of two acceleration processes, one boosting electrons to hundreds of keV for the X ray bursts, the other producing gamma rays through ions accelerated to tens of MeV.
Document ID
19830038815
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Willett, J. B.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Ling, J. C.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Mahoney, W. A.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Riegler, G. R.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Jacobson, A. S.
(California Institute of Technology, Jet Propulsion Laboratory, Pasadena CA, United States)
Date Acquired
August 11, 2013
Publication Date
January 1, 1982
Subject Category
Solar Physics
Meeting Information
Meeting: Gamma ray transients and related astrophysical phenomena; Workshop
Location: La Jolla, CA
Start Date: August 5, 1981
End Date: August 8, 1981
Sponsors: U. S. Department of Energy
Accession Number
83A20033
Distribution Limits
Public
Copyright
Other

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