The relation between H-alpha and SXR emission of the flares

Details The relation between H-alpha and SXR emission of the flares The relation between H-alpha and SXR emission of the flares

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.285..145a&link_type=abstract

In ESA, Proceedings of an International School and Workshop on Reconnection in Space Plasma, Volume 2 p 145-148 (SEE N89-24974 1

Physics

H Alpha Line, Solar Flares, Solar Magnetic Field, Solar X-Rays, Coronal Loops, Magnetic Induction, Magnetic Signatures

Scientific paper

The evolutionary coincidence between the occurrence of the LDE flares and the formation of the evolving delta configuration, in the solar active region, was found. Fifty-one cases of LDE flares were analyzed from the viewpoint of the precise location of their flare loop arcade (located above delta configuration). The quasi-delta configurations (i.e., kinematical joining of the two stable spots of the opposite magnetic induction) are not LDE flare productive.

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