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

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