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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1833
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dc.contributor.authorMaity, S-
dc.contributor.authorPaul, S. N-
dc.contributor.authorBondyopadhaya, R-
dc.date.accessioned2007-09-27T09:27:17Z-
dc.date.available2007-09-27T09:27:17Z-
dc.date.issued1996-
dc.identifier.citationBASI, Vol.24 No. 4 pp. 659-662en
dc.identifier.urihttp://hdl.handle.net/2248/1833-
dc.description.abstractThe dispersion relation for the MHD waves in a homogeneous medium having differential rotaion has been derived by using spherical polar coordinates. It is found that, for equatorial flow the instability of waves is influenced by the differential rotation. The waves with frequency ω >> VA/r in the direction of increasing differential rotation will undergo damping. At the end a very brief discussion about the wave instability inside the sun has been made.en
dc.format.extent250543 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/1996BASI...24..659Men
dc.subjectWave propagationen
dc.subjectDispersion relationen
dc.subjectSpherical-MHD systemen
dc.titleInfluence of differential rotation on the wave propagation in a spherical MHD system with an application to sunen
dc.typeArticleen
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