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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2664
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dc.contributor.authorSundararaman, K-
dc.contributor.authorAleem, S. M-
dc.contributor.authorSingh, J-
dc.contributor.authorSelvendran, R-
dc.contributor.authorThiagarajan, R-
dc.date.accessioned2008-07-14T06:23:54Z-
dc.date.available2008-07-14T06:23:54Z-
dc.date.issued1994-01-
dc.identifier.citationSolar Physics, Vol. 149, No. 1, pp. 119 - 127en
dc.identifier.issn0038-0938-
dc.identifier.urihttp://hdl.handle.net/2248/2664-
dc.description.abstractKodaikanal H-alpha monochromatic and white-light observations are used to study the circular flare of 14 March, 1984. We report here the dynamic activity of the H-alpha filament, which attained a severe twist before erupting as a 4B flare. We feel that the relative motion between the emerging spot field and its neighboring field is responsible for the field line reconnection, which triggered the flare.en
dc.format.extent617395 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherSpringeren
dc.relation.urihttp://adsabs.harvard.edu/abs/1994SoPh..149..119Sen
dc.relation.urihttp://www.springerlink.com/content/v4617167g2524n66/en
dc.subjectH Alpha Lineen
dc.subjectMagnetic Field Configurationsen
dc.subjectMagnetic Field Reconnectionen
dc.subjectSolar Flaresen
dc.subjectSolar Magnetic Fielden
dc.subjectSolar Prominencesen
dc.subjectSunspotsen
dc.subjectChromosphereen
dc.subjectFaculaeen
dc.subjectMagnetic Energy Storageen
dc.subjectPhotosphereen
dc.subjectPolarityen
dc.subjectSpectrogramsen
dc.titleH-alpha flare of 14 March, 1984 -- Evidence for reconnection?en
dc.typeArticleen
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