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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2863
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dc.contributor.authorVenkatakrishnan, P-
dc.contributor.authorNarayanan, R. S-
dc.contributor.authorPrasad, N. D. N-
dc.date.accessioned2008-07-23T11:35:10Z-
dc.date.available2008-07-23T11:35:10Z-
dc.date.issued1993-04-
dc.identifier.citationSolar physics, Vol. 144, No. 2, pp. 315 - 322en
dc.identifier.issn0038-0938-
dc.identifier.urihttp://hdl.handle.net/2248/2863-
dc.description.abstractThe difference between the magnetic tension and magnetic shear was calculated for four vector magnetograms of NOAA AR 4474. It was seen that this difference between the two independent angular measures of magnetic stress is less than 18 deg for more than 50 percent of the pixels. Magnetic tension is thus found to be fairly well correlated with magnetic shear for AR 4474.en
dc.format.extent585795 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherKluwer Academic Publishersen
dc.relation.urihttp://adsabs.harvard.edu/abs/1993SoPh..144..315Ven
dc.subjectSolar flaresen
dc.subjectSolar magnetic fielden
dc.subjectSolar physicsen
dc.subjectMagnetic signaturesen
dc.subjectSolar coronaen
dc.titleCorrelation between magnetic shear and magnetic tension in a solar active regionen
dc.typeArticleen
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