Localization of the Solar Flare SF900610 in X-rays with the WATCH Instrument of the GRANAT Observatory

Details Localization of the Solar Flare SF900610 in X-rays with the WATCH Instrument of the GRANAT Observatory Localization of the Solar Flare SF900610 in X-rays with the WATCH Instrument of the GRANAT Observatory

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002astl...28..853t&link_type=abstract

Astronomy Letters, Volume 28, Issue 12, pp.853-856

Astronomy and Astrophysics

Astronomy

The Sun, X-Ray And Gamma-Ray Sources

Scientific paper

During the solar flare of June 10, 1990, the WATCH instrument of the GRANAT space observatory obtained 110 localizations of the X-ray source in the X-ray range 8-20 keV. Its coordinates were measured with an accuracy of ˜2 arcmin at a 3 σ confidence level. The coordinates of the X-ray source do not coincide with the coordinates of the Hα-line flare. The X-ray source moved over the solar disk during the flare. This probably implies that, as the X-ray emission was generated, different parts of one loop or a system of magnetic loops dominated at different flare times.

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