Correlation between X-ray Temporal Variability and Magnetic Environment in Solar Flares

Details Correlation between X-ray Temporal Variability and Magnetic Environment in Solar Flares Correlation between X-ray Temporal Variability and Magnetic Environment in Solar Flares

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992aas...181.5503n&link_type=abstract

American Astronomical Society, 181st AAS Meeting, #55.03; Bulletin of the American Astronomical Society, Vol. 24, p.1211

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Scientific paper

The X-ray time history of a solar flare can reflect basic processes of heating and/or acceleration, which in turn may depend on the magnetic environment of the site. Some flares show a simple rise and fall temporal behavior, whereas others show more than one peak. Comparisons of images taken by the Soft X-ray Telescope (SXT) aboard the Yohkoh spacecraft with ground-based magnetic data (Hawaii, Kitt Peak and Mitaka) reveal that, at least for a flare-productive active region (NOAA 7260), flares with double-peaked and single-peaked time profiles occurred at systematically different locations within the region. We discuss this result in terms of theoretical models, especially those of coalescence of two current loops.

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