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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3488
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dc.contributor.authorUddin, W-
dc.contributor.authorVerma, V. K-
dc.date.accessioned2008-09-08T16:42:59Z-
dc.date.available2008-09-08T16:42:59Z-
dc.date.issued1998-
dc.identifier.citationBASI, Vol. 26, pp. 200 - 202en
dc.identifier.urihttp://hdl.handle.net/2248/3488-
dc.description.abstractIn this paper we present CCD observations between 14th to 20th Feb. 1994 and analysis of the giant twisted filament evolved in the active region NOAA 7671. The dynamic eruption of the filament accompanied by major flare (3B/M4), CME long duration type II, type IV radio bursts, great microwave bursts, long duration soft X-ray burst, SIFs, strong geomagnetic storms and most energetic proton flare. We analysed and estimated the twist, length, volume, mass and energy associated with filament system between 14th to 20th Feb. 1994. We also give the explantion of the event in the light of existing theories.en
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/1998BASI...26..200Uen
dc.subjectTwisted filamenten
dc.subjectEnergy storageen
dc.subjectSolar flareen
dc.subjectFilament eruptionen
dc.titleEruption of twisted filament, associated flare and transient phenomenaen
dc.typeArticleen
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