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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1752
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dc.contributor.authorGokhale, M. H-
dc.contributor.authorHiremath, K. M-
dc.date.accessioned2007-07-27T07:23:49Z-
dc.date.available2007-07-27T07:23:49Z-
dc.date.issued1986-
dc.identifier.citationAdvances in Space Research, Vol. 6, No. 8, pp. 47 - 50en
dc.identifier.issn0273-1177-
dc.identifier.urihttp://hdl.handle.net/2248/1752-
dc.descriptionRestricted Access-
dc.description.abstractIt is shown that if a thin, isolated and untwisted magnetic flux tube, consisting of a current-free core bounded by a thin current sheath, is in an ‘overall’ equilibrium in a stratified atmosphere, then there is, in general, a net upward force on the current sheath and a net downward force on the core or vice-versa. It is suggested that this effect may be used to model the Evershed flows in sunspots and other longitudinal flows in solar and stellar magnetic flux tubes.en
dc.format.extent3812096 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherElsevieren
dc.relation.urihttp://dx.doi.org/10.1016/0273-1177(86)90407-2en
dc.subjectMagnetohydrodynamic Flowen
dc.subjectSolar Fluxen
dc.subjectSolar Magnetic Field-
dc.subjectStellar Magnetic Fields-
dc.subjectSunspots-
dc.subjectPlasma Equilibrium-
dc.subjectPlasma Sheaths-
dc.subjectStellar Cores-
dc.titleLongitudinal flows in stellar magnetic flux tubesen
dc.typeArticleen
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