Computed magnetic field structure of the flares observed by HINOTORI hard X-ray telescope

Details Computed magnetic field structure of the flares observed by HINOTORI hard X-ray telescope Computed magnetic field structure of the flares observed by HINOTORI hard X-ray telescope

Jul 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983soph...86..339s&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

Physics

13

Solar Flares, Solar Magnetic Field, Solar X-Rays, X Ray Telescopes, Coronal Loops

Scientific paper

Potential field computations have been carried out to study the location of hard X-ray sources observed by the Hinotori hard X-ray imaging instrument, SXT. Of the two flares studied, the X-ray source of the 1981 May 13 event, a very unusual gradual flare, appears to lie at the top of an arcade of field lines. In the other event, the 1981 October 15 flare, the observed double source structure is not explained in the present computation, implying the existence of non-negligible electric currents in the flare region.

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