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	2005-12-07T09:16:48Z
dc.date.available	2005-12-07T09:16:48Z
dc.date.issued	1985-06
dc.identifier.citation	BASI, Vol. 13, No. 2, pp. 148-152	en
dc.identifier.uri	http://hdl.handle.net/2248/652
dc.description.abstract	A statistical analysis of time delays 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
dc.format.extent	445672 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en
dc.publisher	Astronomical Society of India	en
dc.subject	H-alpha	en
dc.subject	Soft x-rays	en
dc.subject	Solar flares	en
dc.title	Time delay between H-alpha and soft x-ray emissions during solar flares	en
dc.type	Article	en