Physics
Scientific paper
Aug 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008soph..250..431k&link_type=abstract
Solar Physics, Volume 250, Issue 2, pp.431-441
Physics
X-Ray Detector, Spectrometer, Cdte, Hard X-Ray
Scientific paper
Spectroscopic observation of solar flares in the hard X-ray energy range, particularly the 20 ˜ 100 keV region, is an invaluable tool for investigating the flare mechanism. This paper describes the design and performance of a balloon-borne hard X-ray spectrometer using CdTe detectors developed for solar flare observation. The instrument is a small balloon payload (gondola weight 70 kg) with sixteen 10×10×0.5 mm CdTe detectors, designed for a 1-day flight at 41 km altitude. It observes in an energy range of 20-120 keV and has an energy resolution of 3 keV at 60 keV. The second flight on 24 May 2002 succeeded in observing a class M1.1 flare.
Katsukawa Yukio
Kobayashi Koji
Kohara Naoki
Kubo Masahito
Kumagai Kazuyoshi
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