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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1794
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dc.contributor.authorGokhale, M. H-
dc.date.accessioned2007-09-17T07:56:10Z-
dc.date.available2007-09-17T07:56:10Z-
dc.date.issued1996-
dc.identifier.citationBASI, Vol. 24, No. 2, pp. 121-124en
dc.identifier.urihttp://hdl.handle.net/2248/1794-
dc.description.abstractOur recent studies of rotation and magnetic field near the Sun's surface have indicated that the solar activity may be originating in interference of global torsional MHD oscillations in the Sun. Using theory of dynamics and solar system ephemerides we have shown that these oscillations may be caused by a latitude-dependent inertial torque which couples the Sun's internal MHD to the solar system dynamics.en
dc.format.extent290101 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/1996BASI...24..121Gen
dc.subjectsunen
dc.subjectinterior - sunen
dc.subjectactivity - sunen
dc.subjectmagnetic field - solar system dynamicsen
dc.titleMHD window on the sunen
dc.typeArticleen
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