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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2439
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dc.contributor.authorRausaria, R. R-
dc.contributor.authorAleem, S. M-
dc.contributor.authorSundararaman, K-
dc.date.accessioned2008-06-17T05:19:20Z-
dc.date.available2008-06-17T05:19:20Z-
dc.date.issued1992-11-
dc.identifier.citationSolar Physics, Vol. 142, No. 1, pp. 131 - 141en
dc.identifier.urihttp://hdl.handle.net/2248/2439-
dc.description.abstractWe have studied the evolution of the double-ribbon, spotless flare of 21 February, 1992, using Kodaikanal Hagr and Kf1 observations. The analysis of the data shows that the Hagr filament underwent a large change in shear prior to the day of the onset of the flare. We find considerable rotation of the plage region before the emergence of a small magnetic pore. It is concluded that shear plays an important role in the triggering of a spotless flareen
dc.format.extent1132292 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherSpringer Netherlandsen
dc.relation.urihttp://www.springerlink.com/content/u86h518468928123/en
dc.relation.urihttp://adsabs.harvard.edu/abs/1992SoPh..142..131Ren
dc.subjectFACULAEen
dc.subjectSOLAR FLARESen
dc.subjectSOLAR MAGNETIC FIELDen
dc.subjectH ALPHA LINEen
dc.subjectPHOTOSPHEREen
dc.titleOn the triggering of a spotless double-ribbon flareen
dc.typeArticleen
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