Initial results from the solar flare X-ray observations with ulysses

Details Initial results from the solar flare X-ray observations with ulysses Initial results from the solar flare X-ray observations with ulysses

Sep 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993adspr..13..241k&link_type=abstract

Advances in Space Research, Volume 13, Issue 9, p. 241-243.

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6

Scientific paper

The Solar X-Ray/Cosmic Gamma-Ray Burst Experiment aboard the Ulysses spacecraft measures hard X-ray spectra in the nominal energy range 15-150 keV, which can be changed by ground command. Since the experiment turn-on on 11 November 1990, it has recorded hard X-ray emission from ~100 solar flares of GOES soft X-ray class > M and several hundred smaller flares. Some of these flares were also observed by comparable instruments aboard other interplanetary and near-Earth spacecraft such as Pioneer Venus Orbiter (PVO), Yohkoh and Compton Observatory (formerly GRO), thus providing a stereoscopic view of the hard X-ray sources in those flares. This paper presents a brief description of the Ulysses instrument and some early observational results.

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