Longitudinal distribution of the hard X-ray bursts on the sun

Details Longitudinal distribution of the hard X-ray bursts on the sun Longitudinal distribution of the hard X-ray bursts on the sun

Sep 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985soph...99..285v&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 99, Sept. 1985, p. 285-289.

Astronomy and Astrophysics

Astronomy

4

Radiation Distribution, Solar Activity, Solar X-Rays, X Ray Astronomy, Japanese Spacecraft, Longitude, Photons, Solar Flares, Spaceborne Astronomy

Scientific paper

The analysis of 315 hard X-ray bursts (HXR) producing solar flares
observed by Hinotori satellite shows that the HXR bursts occur most
prominently at 110°, 140°, 290°, and 320° longitude,
respectively. These longitudes are not only prolific in producing flares
in number but also in producing flares with large photon counts.

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