Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4226
Title: Time-dependent convective collapse of flux tubes
Authors: Hasan, S. S
Keywords: Convective Flow;Plasma Dynamics;Solar Flux;Stellar Models;Collapse;Field Strength;Flow Velocity;Solar Magnetic Field;Time Dependence;Tubes
Issue Date: 1983
Publisher: D. Reidel Publishing Co
Citation: Dordrecht, D. ed., Solar and stellar magnetic fields: Origins and coronal effects; Proceedings of the Symposium, Zurich, Switzerland, August 2 - 6, 1982, pp. 73 - 77
Series/Report no.: IAU Symposium No. 102
Abstract: The 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).
URI: http://hdl.handle.net/2248/4226
???metadata.dc.relation.uri???: http://adsabs.harvard.edu/abs/1983IAUS..102...73H
Appears in Collections:IIAP Publications

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