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

Sundararaman, K; Aleem, S. M; Singh, J; Selvendran, R; Thiagarajan, R

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dc.contributor.author	Sundararaman, K
dc.contributor.author	Aleem, S. M
dc.contributor.author	Singh, J
dc.contributor.author	Selvendran, R
dc.contributor.author	Thiagarajan, R
dc.date.accessioned	2008-07-14T06:23:54Z
dc.date.available	2008-07-14T06:23:54Z
dc.date.issued	1994-01
dc.identifier.citation	Solar Physics, Vol. 149, No. 1, pp. 119 - 127	en
dc.identifier.issn	0038-0938
dc.identifier.uri	http://hdl.handle.net/2248/2664
dc.description.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.	en
dc.format.extent	617395 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Springer	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1994SoPh..149..119S	en
dc.relation.uri	http://www.springerlink.com/content/v4617167g2524n66/	en
dc.subject	H Alpha Line	en
dc.subject	Magnetic Field Configurations	en
dc.subject	Magnetic Field Reconnection	en
dc.subject	Solar Flares	en
dc.subject	Solar Magnetic Field	en
dc.subject	Solar Prominences	en
dc.subject	Sunspots	en
dc.subject	Chromosphere	en
dc.subject	Faculae	en
dc.subject	Magnetic Energy Storage	en
dc.subject	Photosphere	en
dc.subject	Polarity	en
dc.subject	Spectrograms	en
dc.title	H-alpha flare of 14 March, 1984 -- Evidence for reconnection?	en
dc.type	Article	en