Hard X-ray dynamic spectrum of flares observed by HINOTORI

Details Hard X-ray dynamic spectrum of flares observed by HINOTORI Hard X-ray dynamic spectrum of flares observed by HINOTORI

Jul 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983soph...86..241n&link_type=abstract

(Japan Society for the Promotion of Science and National Science Foundation, U.S.-Japan Seminar on the Recent Advances in the Un

Astronomy and Astrophysics

Astronomy

9

Solar Flares, Solar X-Rays, Spaceborne Astronomy, X Ray Spectra, Bursts, Gamma Ray Spectrometers, Temporal Distribution

Scientific paper

Time variations of the hard X-ray spectrum in solar flares are observed by the hard X-ray spectrometer aboard the Hinotori satellite. With a new presentation of the dynamic spectrum the authors have studied the differences between impulsive and gradual hard X-ray bursts. In the impulsive events a "bent" spectrum up to some hundred keV persists at least until the main peak. In the gradual events, on the other hand, a power-law spectrum augmented by a low-energy excess is dominant.

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