Axisymmetric MHD equilibrium of a self-gravitating incompressible fluid

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2970

Full metadata record

DC Field	Value	Language
dc.contributor.author	Satya Narayanan, A	-
dc.date.accessioned	2008-08-01T06:00:37Z	-
dc.date.available	2008-08-01T06:00:37Z	-
dc.date.issued	1996-05	-
dc.identifier.citation	Physical Scripta, Vol. 53, No. 5, pp. 638 - 640	en
dc.identifier.issn	0281-1847	-
dc.identifier.uri	http://hdl.handle.net/2248/2970	-
dc.description	Restricted Access	-
dc.description.abstract	The equilibrium of a self-gravitating incompressible fluid with a magnetic field and large electrical conductivity is studied. The magnetic fields and fluid motions are assumed to have a symmetry about an axis. The basic magnetic field is assumed to consist of two parts, namely, poloidal and toroidal while the fluid motion is assumed to be purely rotational. An exact solution of the MHD equations for the above configuration is presented. This study presents a more general form for the poloidal magnetic field than that studied by Gokhale and Hiremath for their modelling of the steady part of the Sun's internal magnetic field.	en
dc.format.extent	3894 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Royal Swedish Academy of Sciences	en
dc.subject	MHD equilibrium	en
dc.subject	self-gravitating incompressible fluid	en
dc.title	Axisymmetric MHD equilibrium of a self-gravitating incompressible fluid	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

Files in This Item:

File	Description	Size	Format
Axisymmetric MHD equilibrium Restricted Access	Restricted Access	245.23 kB	Adobe PDF	View/Open Request a copy

DSpace JSPUI