Time delay between H-alpha and soft x-ray emissions during solar flares

dc.contributor.author	Verma, V. K.
dc.contributor.author	Pande, M. C.
dc.date.accessioned	2010-03-03T10:45:05Z
dc.date.available	2010-03-03T10:45:05Z
dc.date.issued	1985
dc.identifier.citation	This article is downloaded from ADS	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/603
dc.description.abstract	A statistical analysis of time delay between H-alpha and soft x-ray (SXR) emissions at onset and peak respectively during solar flares is presented. We find that at the onset of flares SXR emission starts simultaneously or upto two min earlier than H-alpha emissions. At peak flux the SXR emission is found to be peaked between 2 min before to 3 min after the H-alpha emissions.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	basi13-148
dc.subject	H-alpha, Soft x-rays, Solar flares	en_US
dc.title	Time delay between H-alpha and soft x-ray emissions during solar flares	en_US
dc.type	Article	en_US