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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2861
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dc.contributor.authorSundararaman, K-
dc.contributor.authorGupta, S. S-
dc.contributor.authorSelvendran, R-
dc.date.accessioned2008-07-23T11:34:10Z-
dc.date.available2008-07-23T11:34:10Z-
dc.date.issued1993-03-
dc.identifier.citationJournal of Astrophysics and Astronomy, Vol. 14, No. 1, pp. 45 - 52.en
dc.identifier.issn0250-6335-
dc.identifier.urihttp://hdl.handle.net/2248/2861-
dc.description.abstractWe have taken the case of a circular H-alpha filament observed on May 9, 1979 erupting into a double-ribbon flare associated with a nonspot region. The plage motions are responsible for the filament reorientation and, here as a special case, wherein the filament attains a clear circular shape before the onset of a flare. We conclude that the change in the orientation of the H-alpha filament marks the instability giving rise to the flare.en
dc.format.extent1145754 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherIndian Academy of Sciencesen
dc.relation.urihttp://adsabs.harvard.edu/abs/1993JApA...14...45Sen
dc.subjectSolar flaresen
dc.subjectSolar prominencesen
dc.subjectCoronal loopsen
dc.subjectH alpha lineen
dc.subjectSunspotsen
dc.titleFilament activity in a quiet region flareen
dc.typeArticleen
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