Exact solution of the incompressible Hall magnetohydrodynamics

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DC Field	Value	Language
dc.contributor.author	Mahajan, S. M	-
dc.contributor.author	Krishan, V	-
dc.date.accessioned	2008-09-10T12:12:10Z	-
dc.date.available	2008-09-10T12:12:10Z	-
dc.date.issued	2005-05	-
dc.identifier.citation	Monthly Notices of the Royal Astronomical Society, Vol. 359, No. 1, pp. L27 - L29	en
dc.identifier.issn	0035-8711	-
dc.identifier.uri	http://hdl.handle.net/2248/3524	-
dc.description	Restricted Access	en
dc.description.abstract	The Alfvén wave is known to be an exact solution of the ideal magnetohydrodynamics (MHD), and this has found use in modelling astrophysical turbulence. In this paper we show that the Hall MHD also submits itself to an exact solution in the incompressible limit. We compare the linear and the non-linear modes of the Hall MHD and comment on their probable role in describing turbulent fluctuations in different astrophysical situations.	en
dc.language.iso	en	en
dc.publisher	Royal Astronomical Society	en
dc.relation.uri	http://dx.doi.org/10.1111/j.1745-3933.2005.00028.x	en
dc.subject	MHD	en
dc.subject	Turbulence	en
dc.subject	Waves	en
dc.title	Exact solution of the incompressible Hall magnetohydrodynamics	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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