Time delay between Hα and hard X-ray emissions during implusive solar flares

dc.contributor.author	Verma, V. K.
dc.contributor.author	Pande, M. C.
dc.date.accessioned	2010-03-03T09:26:24Z
dc.date.available	2010-03-03T09:26:24Z
dc.date.issued	1985
dc.identifier.citation	This article is downloaded for ADS	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/599
dc.description.abstract	This investigation shows that statistically there are significant time delay between Hα and hard X-ray (HXR) emissions during solar flares; most impulsive flares produce HXR emissions up to ~1 min before and up to 2 min after the onset of Hα emission. HXR emissions are also found to be peaked up to 2 min before the Hα emissions.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	sp97-107
dc.subject	Hα emissions, Hard X-ray	en_US
dc.title	Time delay between Hα and hard X-ray emissions during implusive solar flares	en_US
dc.type	Article	en_US