1. IIA Institutional Repository
  2. Publications of Astronomical Society of India
  3. BASI Publications
Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/652
Full metadata record
DC FieldValueLanguage
dc.contributor.authorVerma, V. K-
dc.contributor.authorPande, M. C-
dc.date.accessioned2005-12-07T09:16:48Z-
dc.date.available2005-12-07T09:16:48Z-
dc.date.issued1985-06-
dc.identifier.citationBASI, Vol. 13, No. 2, pp. 148-152en
dc.identifier.urihttp://hdl.handle.net/2248/652-
dc.description.abstractA 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.extent445672 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherAstronomical Society of Indiaen
dc.subjectH-alphaen
dc.subjectSoft x-raysen
dc.subjectSolar flaresen
dc.titleTime delay between H-alpha and soft x-ray emissions during solar flaresen
dc.typeArticleen
Appears in Collections:BASI Publications

Files in This Item:
File Description SizeFormat 
Verma.pdf435.23 kBAdobe PDFThumbnail
View/Open
Show simple item record


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.