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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3078
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dc.contributor.authorMangalam, A-
dc.contributor.authorKrishan, V-
dc.date.accessioned2008-08-12T09:00:55Z-
dc.date.available2008-08-12T09:00:55Z-
dc.date.issued2000-12-
dc.identifier.citationJournal of Astrophysics and Astronomy, Vol. 21, No. 3 – 4, pp. 299 - 302en
dc.identifier.issn0250-6335-
dc.identifier.urihttp://hdl.handle.net/2248/3078-
dc.description.abstractWe study the relaxation of a compressible plasma to an equilibrium with flow. The constraints of conservation of mass, energy, angular momentum, cross-helicity and relative magnetic helicity are imposed. Equilibria corresponding to the energy extrema while conserving these invariants for parallel flows yield three classes of solutions and one of them with an increasing radial density profile, relevant to solar flux tubes is presented.en
dc.format.extent85891 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherIndian Academy of Sciencesen
dc.relation.urihttp://adsabs.harvard.edu/abs/2000JApA...21..299Men
dc.subjectHydromagneticsen
dc.subjectSun: atmosphereen
dc.subjectMagnetic fieldsen
dc.titleModels of Flux Tubes from Constrained Relaxationen
dc.typeArticleen
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