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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1819
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dc.contributor.authorGangadhara, R. T-
dc.contributor.authorHasan, S. S-
dc.date.accessioned2007-09-21T12:10:32Z-
dc.date.available2007-09-21T12:10:32Z-
dc.date.issued1996-
dc.identifier.citationBASI, Vol.24 No. 2 pp. 341-344en
dc.identifier.urihttp://hdl.handle.net/2248/1819-
dc.description.abstractWe numerically simulate the dynamical relaxation to equilibrium of a sunspot. Treating the sunspot as a thick axisymmetric flux tube in cylindrical geometry, we solve the time dependent MHD equation to examine the evolution of a sunspot towards equilibrium, starting from an arbitrary initial state.en
dc.format.extent305141 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/1996BASI...24..341Gen
dc.subjectMagnetohydrodynamics-Sunen
dc.subjectMagnetic fields-Sunen
dc.subjectSunspotsen
dc.titleModelling sunspot equilibrium through a solution of the time dependent MHD equationsen
dc.typeArticleen
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