Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5195
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dc.contributor.authorHasan, S. S-
dc.contributor.authorSobouti, Y-
dc.date.accessioned2010-07-15T15:10:57Z-
dc.date.available2010-07-15T15:10:57Z-
dc.date.issued1987-09-
dc.identifier.citationMNRAS, Vol. 228, pp. 427-451en
dc.identifier.urihttp://hdl.handle.net/2248/5195-
dc.description.abstractThe authors examine the structure of motions that can occur in a vertical magnetic flux tube with a rectangular cross-section. A polytropic stratification is assumed in the vertical direction. The authors use a gauged version of Helmholtz's theorem, the decompose the perturbations into an irrotational component and a solenoidal component, which they further split into the sum of poloidal and toroidal components. These components are identified with p, g and toroidal modes of a fluid. The normal modes of the tube are determined using a Rayleigh-Ritz variational technique. The authors' technique efficiently isolates all the modes to high orders. They first consider some special cases, in order to highlight some interesting properties of the modes. Then, they choose a parameter range to study the properties of oscillations in intense flux tubes on the Sun.en
dc.language.isoenen
dc.publisherBlackwellen
dc.relation.urihttp://adsabs.harvard.edu/abs/1987MNRAS.228..427Hen
dc.subjectMagnetic fluxen
dc.subjectPropagation modesen
dc.subjectSolar magnetic fielden
dc.subjectWave propagationen
dc.subjectPolytropic processesen
dc.subjectStellar oscillationsen
dc.subjectVertical distributionen
dc.titleMode classification and wave propagation in a magnetically structured mediumen
dc.typeArticleen
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