Gamma-ray burst high time-resolution spectral observations made with the Solar Maximum Mission

Details Gamma-ray burst high time-resolution spectral observations made with the Solar Maximum Mission Gamma-ray burst high time-resolution spectral observations made with the Solar Maximum Mission

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc....1...43d&link_type=abstract

IN: International Cosmic Ray Conference, 18th, Bangalore, India, August 22-September 3, 1983, Conference Papers. Volume 1 (A85-2

Physics

Energy Spectra, Gamma Ray Bursts, Solar Maximum Mission, Absorption Spectra, Bremsstrahlung, Spectral Resolution, Temporal Resolution

Scientific paper

The gamma-ray bursts of April 19 and 21, 1980, and March 1, 1981, are characterized on the basis of observations obtained at 25-500 keV and time resolution 128 msec using the hard-X-ray-burst spectrometer of the SMM satellite. The data are presented graphically, and the parameters determined by fitting three theoretical models to the data for each phase (rising phase, decay phase, and valleys between pulses) are given in tables. Models used are thin thermal bremsstrahlung with or without absorption lines, thermal synchrotron with or without absorption lines, and power law with exponential cutoff.

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