Viscous damping of Alfven surface waves in the solar atmosphere

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4946

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DC Field	Value	Language
dc.contributor.author	Rathinavelu, G. D	-
dc.contributor.author	Sivaraman, M	-
dc.contributor.author	Narayanan, A. S	-
dc.date.accessioned	2009-12-21T11:44:15Z	-
dc.date.available	2009-12-21T11:44:15Z	-
dc.date.issued	2009-12	-
dc.identifier.citation	Plasma Physics Reports, Vol. 35, No. 11, pp. 976 - 979	en
dc.identifier.issn	1063-780X	-
dc.identifier.uri	http://hdl.handle.net/2248/4946	-
dc.description	The original publication is available at springerlink.com	en
dc.description	Restricted Access	-
dc.description.abstract	The dispersion relation for the propagation of viscous Alfven surface waves along viscous plasma plasma interface has been derived. Two modes of Alfven surface waves are found to propagate with their characteristics depend on the interface parameters like magnetic field, density ratio, viscosity, etc. The viscous damping of Alfven surface waves has been studied in the astrophysical point of view. The damping length of Alfven surface waves due to viscosity in the solar atmosphere has been estimated.	en
dc.language.iso	en	en
dc.publisher	MAIK Nauka	en
dc.relation.uri	http://dx.doi.org/10.1134/S1063780X09110075	en
dc.rights	© Springer	en
dc.subject	Magnetohydrodynamic Waves	en
dc.subject	Interface	en
dc.subject	Plasmas	en
dc.title	Viscous damping of Alfven surface waves in the solar atmosphere	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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