H-alpha flare of 14 March, 1984 -- Evidence for reconnection?

Details H-alpha flare of 14 March, 1984 -- Evidence for reconnection? H-alpha flare of 14 March, 1984 -- Evidence for reconnection?

Jan 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994soph..149..119s&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 149, no. 1, p. 119-127

Physics

2

H Alpha Line, Magnetic Field Configurations, Magnetic Field Reconnection, Solar Flares, Solar Magnetic Field, Solar Prominences, Sunspots, Chromosphere, Faculae, Magnetic Energy Storage, Photosphere, Polarity, Spectrograms

Scientific paper

Kodaikanal H-alpha monochromatic and white-light observations are used to study the circular flare of 14 March, 1984. We report here the dynamic activity of the H-alpha filament, which attained a severe twist before erupting as a 4B flare. We feel that the relative motion between the emerging spot field and its neighboring field is responsible for the field line reconnection, which triggered the flare.

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