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Observation of gamma-ray bursts with the SMM gamma-ray spectrometerThe gamma-ray spectrometer on SMM is sensitive to bursts within its field of view with intensities greater than 0.000005 erg/sq cm above 100 keV. It has detected 17 events between February 1980 and March 1981 with the characteristics of cosmic gamma-ray bursts. The most intense burst, on 19 April 1980, had a photon spectrum consistent with a power law with spectral index - 2.5 from 300 keV to approximately 7 MeV. It is not possible at present to exclude the sun as the source of this burst. Spectra of 11 of the bursts have been studied for line features with no clear evidence for line emission greater than 300 keV. The continuum radiation from about half of these events have hard emission extending to approximately equal to or greater than 2 MeV.
Document ID
19820046850
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Share, G. H.
(Hulburt (E. O.) Center for Space Research Washington, DC, United States)
Strickman, M. S.
(Hulburt (E. O.) Center for Space Research Washington, DC, United States)
Kinzer, R. L.
(U.S. Navy, E. O. Hulburt Center for Space Research, Washington DC, United States)
Chupp, E. L.
(Hulburt (E. O.) Center for Space Research Washington, DC, United States)
Forrest, D. J.
(Hulburt (E. O.) Center for Space Research Washington, DC, United States)
Ryan, J. M.
(New Hampshire, University Durham, NH, United States)
Rieger, E.
(Hulburt (E. O.) Center for Space Research Washington, DC, United States)
Reppin, C.
(Hulburt (E. O.) Center for Space Research Washington, DC, United States)
Kanbach, G.
(Max-Planck-Institut fur Physik und Astrophysik Garching, Germany)
Date Acquired
August 10, 2013
Publication Date
January 1, 1982
Subject Category
Space Radiation
Meeting Information
Meeting: International Cosmic Ray Conference
Location: Paris
Country: France
Start Date: July 13, 1981
End Date: July 25, 1981
Accession Number
82A30385
Funding Number(s)
CONTRACT_GRANT: NASA ORDER S-70926-A
Distribution Limits
Public
Copyright
Other

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