The Hard X-ray Imaging Spectrometer (HXIS) |
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Authors: | H. Frank Van Beek Peter Hoyng Bill Lafleur George M. Simnett |
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Affiliation: | (1) Space Research Laboratory, The Astronomical Institute at Utrecht, Utrecht, The Netherlands;(2) Department of Space Research, University of Birmingham, Birmingham, England |
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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 8 over Ø 240 and 32 over Ø 624 field of view, and time resolution of 0.5–7 s depending on the mode of operation. By means of a flare flag 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 type IV electron clouds above flare regions. |
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