The peculiar solar flare of 1981 May 13

dc.contributor.author	Bondal, K. R.
dc.contributor.author	Pant, P.
dc.contributor.author	Pande, M. C.
dc.contributor.author	Ballabh, G. M.
dc.date.accessioned	2010-04-13T08:11:42Z
dc.date.available	2010-04-13T08:11:42Z
dc.date.issued	1982
dc.identifier.uri	http://hdl.handle.net/123456789/652
dc.description.abstract	Time-lapse photographic observations with 0.7 Å passband H-alpha filter and the morphological-cum-temporal behaviour of a large double solar flare which occurred on 1981 May 13 have been described. The two strands, constituting the flare, which initially appeared to cross each other, with a bright region at the location of crossing, later separated out, ultimately becoming roughly parallel. The mean separation between the two strands at various intervals of time have been measured. It is concluded that apart from the oscillating behaviour of the stands, there is shearing in them probably due to rotation of the footprints.	en_US
dc.language.iso	en	en_US
dc.relation.ispartofseries	basi10-137
dc.subject	Solar Flare, Helical Structure, Magnetic Shearing, Ionospheric Effects	en_US
dc.title	The peculiar solar flare of 1981 May 13	en_US
dc.type	Article	en_US