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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4226
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dc.contributor.authorHasan, S. S-
dc.date.accessioned2009-01-02T11:10:09Z-
dc.date.available2009-01-02T11:10:09Z-
dc.date.issued1983-
dc.identifier.citationDordrecht, D. ed., Solar and stellar magnetic fields: Origins and coronal effects; Proceedings of the Symposium, Zurich, Switzerland, August 2 - 6, 1982, pp. 73 - 77en
dc.identifier.urihttp://hdl.handle.net/2248/4226-
dc.description.abstractThe time-dependent collapse of a slender flux tube extending vertically in the convection zone of the sun is modelled. Starting from an initial state in which the flux tube is in hydrostatic equilibrium, the non-linear MHD equations are used to examine its temporal evolution. A detailed study of the flow variables and magnetic field within the tube is presented. It is seen that asymptotically in time a unique state of dynamic equilibrium is established, irrespective of the value of beta-O (the ratio of the thermal to magnetic pressure at the initial epoch).en
dc.language.isoenen
dc.publisherD. Reidel Publishing Coen
dc.relation.ispartofseriesIAU Symposium No. 102-
dc.relation.urihttp://adsabs.harvard.edu/abs/1983IAUS..102...73Hen
dc.subjectConvective Flowen
dc.subjectPlasma Dynamicsen
dc.subjectSolar Fluxen
dc.subjectStellar Modelsen
dc.subjectCollapseen
dc.subjectField Strengthen
dc.subjectFlow Velocityen
dc.subjectSolar Magnetic Fielden
dc.subjectTime Dependenceen
dc.subjectTubesen
dc.titleTime-dependent convective collapse of flux tubesen
dc.typeArticleen
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