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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2246
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dc.contributor.authorUddin, W-
dc.contributor.authorLalan, P-
dc.date.accessioned2008-04-22T07:34:14Z-
dc.date.available2008-04-22T07:34:14Z-
dc.date.issued2001-
dc.identifier.citationBASI, Vol. 29, No. 3, pp. 241 - 243en
dc.identifier.urihttp://hdl.handle.net/2248/2246-
dc.description.abstractWe observed a post-flare loop system in Hα on the west limb on 27 November 1996 which started earlier than 05:07:20 UT in NOAA active region 7997 (N04, W89). The post-flare loops were associated with long duration x-ray flare of important class B9.0. We study the evolution of post-flare loop system which display complex, fan like structure with multi bright loop tops in Hα as well as in x-ray/Yohkoh and SOHO observations. This event shows the characteristics of long duration event (LDE). The main aim of this paper is to study the morphological changes of post-flare loops to understand the prolonged post eruption energy release process in decay phase in Hα, x-ray, radio wave and in microwave regions. The results of our investigation has been discussed in the light of existing models.en
dc.format.extent359073 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2001BASI...29..241Uen
dc.subjectPost-flare loopsen
dc.subjectEnergy releaseen
dc.titleDynamical properties of flare Loops of 27 November 1996en
dc.typeArticleen
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