BATSE Solar Flare Spectroscopy

Details BATSE Solar Flare Spectroscopy BATSE Solar Flare Spectroscopy

Mar 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998nasa.reptt....s&link_type=abstract

Technical Report, NASA/CR-1998-206868; NAS 1.26:206868; Rept-98-REP-0187

Astronomy and Astrophysics

Astronomy

Solar Flares, Spectroscopy, Gamma Ray Bursts, Goes Satellites, Spaceborne Astronomy, Gamma Ray Observatory, Data Bases, Sunspots, Spaceborne Telescopes

Scientific paper

This final report describes the progress originally proposed: (1) the continued improvement of a software and database environment capable of supporting all users of BATSE solar data as well as providing scientific expertise and effort to the BATSE solar community; (2) the continued participation with the PI team and other guest investigators in the detailed analysis of the BATSE detectors' response at low energies; (3) using spectroscopic techniques to fully exploit the potential of electron time-of-flight studies; and, (4) a full search for flare gamma-ray line emission at 2.2 MeV from all GOES X-class flares observed with BATSE.

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