Evidence Supporting Quadruple Magnetic Source Model of Arcade Flarings, and Implications

Details Evidence Supporting Quadruple Magnetic Source Model of Arcade Flarings, and Implications Evidence Supporting Quadruple Magnetic Source Model of Arcade Flarings, and Implications

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999spro.proc..397u&link_type=abstract

Solar Physics with Radio Observations, Proceedings of the Nobeyama Symposium, held in Kiyosato, Japan, Oct. 27-30, 1998, Edited

Physics

1

Scientific paper

Taking advantage of high sensitivity, wide dynamic range observations by Yohkoh, we have investigated the structures and their changes in the still faint pre-event coronal region around a dark filament which is going to be involved in arcade flarings (arcade flares or high latitude arcade formations). It becomes clear that what we find from the observations is quite different from what we expect from the classical ``Re-closing of Once Opened-up Simple Magnetic Aracde Model'' for arcade flarings. The observations, instead, indicate that the quadruple magnetic source model advocated by Uchida (1980), for which definitive support from observations was not possible at that time, turns out to be a likely model that explains the observations.

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