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Influence of differential rotation on the wave propagation in a spherical MHD system with an application to sun

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dc.contributor.author Maity, S
dc.contributor.author Paul, S. N
dc.contributor.author Bondyopadhaya, R
dc.date.accessioned 2007-09-27T09:27:17Z
dc.date.available 2007-09-27T09:27:17Z
dc.date.issued 1996
dc.identifier.citation BASI, Vol.24 No. 4 pp. 659-662 en
dc.identifier.uri http://hdl.handle.net/2248/1833
dc.description.abstract The 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.extent 250543 bytes
dc.format.mimetype application/pdf
dc.language.iso en en
dc.publisher Astronomical Society of India en
dc.relation.uri http://adsabs.harvard.edu/abs/1996BASI...24..659M en
dc.subject Wave propagation en
dc.subject Dispersion relation en
dc.subject Spherical-MHD system en
dc.title Influence of differential rotation on the wave propagation in a spherical MHD system with an application to sun en
dc.type Article en


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