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|Title:||H-alpha flare of 14 March, 1984 -- Evidence for reconnection?|
Aleem, S. M
|Keywords:||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|
|Citation:||Solar Physics, Vol. 149, No. 1, pp. 119 - 127|
|Abstract:||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.|
|Appears in Collections:||IIAP Publications|
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