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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/631
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dc.contributor.authorPant, P-
dc.date.accessioned2005-12-07T03:49:58Z-
dc.date.available2005-12-07T03:49:58Z-
dc.date.issued1984-09-
dc.identifier.citationBASI, Vol. 12, No. 3, pp. 252-257en
dc.identifier.urihttp://hdl.handle.net/2248/631-
dc.description.abstractWe describe time-lapse H-alpha observations of a peculiar type of prominence activation of 1981 October 7 and and its morphological behaviour. The prominence material seems to have originated from the photosphere as a huge twisted rope-like structure. It reached a height of ~ 10/sup5/ km, and later on split into braided closed loop-like features, which remained stable for a few minutes before breaking up at the top of the loop and finally fading out. The splitting of the twisted rope-like structure is explained on the basis of screw-type instability in current-carrying plasma column.en
dc.format.extent432146 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherAstronomical Society of Indiaen
dc.subjectProminence activationen
dc.subjectScrew-type instabilityen
dc.subjectTwisted ropeen
dc.subjectPlasmaen
dc.subjectFlux tubeen
dc.titleOn a peculiar type of prominence activationen
dc.typeArticleen
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