On the existence of interfacial waves with inclined magnetic fields

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3243

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DC Field	Value	Language
dc.contributor.author	Satya Narayanan, A	-
dc.date.accessioned	2008-08-22T10:12:46Z	-
dc.date.available	2008-08-22T10:12:46Z	-
dc.date.issued	1997-08	-
dc.identifier.citation	Astronomy and Astrophysics , Vol. 324, No. 3, pp. 977 - 980	en
dc.identifier.issn	0004-6361	-
dc.identifier.uri	http://hdl.handle.net/2248/3243	-
dc.description.abstract	The dispersive characteristics of interfacial waves in low β plasma is studied. The condition for the existence of these waves is derived. It is assumed that the magnetic field and the propagation vector are inclined at different angles to the density discontinuity which is horizontal.The dispersion relation for such a configuration is solved for the interfacial (surface) waves as a function of the propagation angle for a given inclination of the magnetic field. The normalized phase speed of these waves are studied for different values of α=ρ_02_/ρ_01_ , γ_1_ and γ_2_.	en
dc.format.extent	138124 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	European Southern Observatory	en
dc.relation.uri	http://aa.springer.de/bibs/7324003/2300977/small.htm	en
dc.subject	Interfacial Waves	en
dc.subject	Low {Beta} Plasma	en
dc.subject	Inclined Magnetic Fields	en
dc.title	On the existence of interfacial waves with inclined magnetic fields	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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