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Observation of gamma-ray bursts with the SMM gamma-ray spectrometer

Authors :
Share, G. H
Strickman, M. S
Kinzer, R. L
Chupp, E. L
Forrest, D. J
Ryan, J. M
Rieger, E
Reppin, C
Kanbach, G
Publication Year :
1982
Publisher :
United States: NASA Center for Aerospace Information (CASI), 1982.

Abstract

The 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.

Subjects

Subjects :
Space Radiation

Details

Language :
English
Database :
NASA Technical Reports
Notes :
NASA ORDER S-70926-A
Publication Type :
Report
Accession number :
edsnas.19820046850
Document Type :
Report