Solar response of the BATSE instrument on the gamma-ray observatory

Details Solar response of the BATSE instrument on the gamma-ray observatory Solar response of the BATSE instrument on the gamma-ray observatory

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988fnsm.work..204f&link_type=abstract

In NASA, Goddard Space Flight Center, Max 1991: Flare Research at the Next Solar Maximum. Workshop 1: Scientific Objectives p 20

Computer Science

Equipment Specifications, Gamma Ray Bursts, Gamma Ray Observatory, Solar Flares, Spectrum Analysis, X Rays, Data Acquisition, Emission Spectra, Gamma Ray Spectra, High Resolution, Monte Carlo Method, X Ray Spectra

Scientific paper

The Burst and Transient Source Experiment (BATSE) on board the gamma ray observatory (GRO) aims at comprehensive observations of time profiles, spectra, and locations of high-energy transient sources. The mysterious cosmic gamma ray bursts provided the main motivation for the observations, but BATSE will make excellent observations of many classes of sources, and in particular solar flares. The solar response of BATSE, as inferred from its design parameters, is analyzed for two purposes: the optimization of the solar observations themselves, and the characterization of the solar effects on ordinary nonsolar observations.

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