Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2664
Title: H-alpha flare of 14 March, 1984 -- Evidence for reconnection?
Authors: Sundararaman, K
Aleem, S. M
Singh, J
Selvendran, R
Thiagarajan, R
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
Issue Date: Jan-1994
Publisher: Springer
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.
URI: http://hdl.handle.net/2248/2664
ISSN: 0038-0938
???metadata.dc.relation.uri???: http://adsabs.harvard.edu/abs/1994SoPh..149..119S
http://www.springerlink.com/content/v4617167g2524n66/
Appears in Collections:IIAP Publications

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