Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2540
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dc.contributor.authorSivaraman, K. R-
dc.contributor.authorRausaria, R. R-
dc.contributor.authorAleem, S. M-
dc.date.accessioned2008-06-30T06:18:08Z-
dc.date.available2008-06-30T06:18:08Z-
dc.date.issued1992-04-
dc.identifier.citationSolar Physics, Vol. 138, No. 2, pp. 353 - 360en
dc.identifier.issn0038-0938 (Print) 1573-093X (Online)-
dc.identifier.urihttp://hdl.handle.net/2248/2540-
dc.description.abstractWe have evaluated the shear angle of the neutral line of the non-potential magnetic field for one or two days prior to and after the flare event for 10 cases. We have used the Hagr filament positions to evaluate the shear in the neutral line. We find from the samples we have studied that it is the change in the shear that occurs a day prior to the flare that can lead to the event. This change can be in either direction, i.e., it can be a large increase from a small value or a decrease from a large initial value. Thus it is the change in the shear angle that seems to be a deciding criterion for a flare to occur and not a large value for the shear angle itself. We have one instance where there was no significant change in the shear angle over a period of a few days and this region, although similar to other active regions studied, did not produce any flare activityen
dc.format.extent572572 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherSpringer Netherlandsen
dc.relation.urihttp://adsabs.harvard.edu/abs/1992SoPh..138..353Sen
dc.relation.urihttp://www.springerlink.com/content/x3531m5574k46110/en
dc.subjectH alpha lineen
dc.subjectSolar flaresen
dc.subjectSolar magnetic fielden
dc.subjectSolar prominencesen
dc.subjectEnergy sourcesen
dc.subjectFree energyen
dc.subjectMagnetic energy storageen
dc.subjectSolar activity effectsen
dc.titleMagnetic shear in flaring regions. I - Quantitative evaluation of the change in shearen
dc.typeArticleen
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