Filament activity in a quiet region flare

dc.contributor.author	Sundararaman, K
dc.contributor.author	Gupta, S. S
dc.contributor.author	Selvendran, R
dc.date.accessioned	2008-07-23T11:34:10Z
dc.date.available	2008-07-23T11:34:10Z
dc.date.issued	1993-03
dc.identifier.citation	Journal of Astrophysics and Astronomy, Vol. 14, No. 1, pp. 45 - 52.	en
dc.identifier.issn	0250-6335
dc.identifier.uri	http://hdl.handle.net/2248/2861
dc.description.abstract	We have taken the case of a circular H-alpha filament observed on May 9, 1979 erupting into a double-ribbon flare associated with a nonspot region. The plage motions are responsible for the filament reorientation and, here as a special case, wherein the filament attains a clear circular shape before the onset of a flare. We conclude that the change in the orientation of the H-alpha filament marks the instability giving rise to the flare.	en
dc.format.extent	1145754 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Indian Academy of Sciences	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1993JApA...14...45S	en
dc.subject	Solar flares	en
dc.subject	Solar prominences	en
dc.subject	Coronal loops	en
dc.subject	H alpha line	en
dc.subject	Sunspots	en
dc.title	Filament activity in a quiet region flare	en
dc.type	Article	en