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The Hard X-ray Imaging Spectrometer (HXIS)
Authors:H Frank Van Beek  Peter Hoyng  Bill Lafleur  George M Simnett
Institution:(1) Space Research Laboratory, The Astronomical Institute at Utrecht, Utrecht, The Netherlands;(2) Department of Space Research, University of Birmingham, Birmingham, England
Abstract:The HXIS, a joint instrument of the Space Research Laboratory at Utrecht, The Netherlands, and the Department of Space Research of the University of Birmingham, U.K., images the Sun in hard X-rays: Six energy bands in energy range 3.5–30 keV, spatial resolution 8Prime over Ø 2prime40Prime and 32Prime over Ø 6prime24Prime field of view, and time resolution of 0.5–7 s depending on the mode of operation. By means of a lsquoflare flagrsquo it alerts all the other SMM instruments when a flare sets in and informs them about the location of the X-ray emission. The experiment should yield information about the position, extension and spectrum of the hard X-ray bursts in flares, their relation to the magnetic field structure and to the quasi-thermal soft X-rays, and about the characteristics and development of lsquotype IVrsquo electron clouds above flare regions.
Keywords:
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