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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1785
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dc.contributor.authorUddin, W-
dc.contributor.authorGaur, V. P-
dc.contributor.authorPande, M. C-
dc.date.accessioned2007-09-14T06:42:28Z-
dc.date.available2007-09-14T06:42:28Z-
dc.date.issued1995-
dc.identifier.citationBASI, Vol. 23, No. 2, pp. 159-164en
dc.identifier.urihttp://hdl.handle.net/2248/1785-
dc.description.abstractFollowing Vrsnak (1990), the observations of an eruptive prominence are analysed. Time evolution of height and velocity of the ascending prominence are measured. The prominence manifested helical structure and many knots. Large loop of the prominence prior to eruption has been seemingly formed by reconnections. The evolutions of the average pitch angles in the legs of the prominence and near the summit, from pre-eruptive phase to eruptive phase, are measured. The decrease of pitch angle in legs and near the summit of the prominence sugget 'detwisting'. Velocities of five selected knots are also given.en
dc.format.extent384895 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/1995BASI...23..159Uen
dc.subjectprominenceen
dc.subjectpitch angleen
dc.subjectpitch lengthen
dc.titleEvolution of the helical prominence of December 15, 1992en
dc.typeArticleen
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