Adiabatic plasma rotations in orthogonal coordinate systems

Please use this identifier to cite or link to this item: http://dspace.mediu.edu.my:8181/xmlui/handle/123456789/3146

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DC Field	Value	Language
dc.creator	Viana Ricardo L.	-
dc.date	2001	-
dc.date.accessioned	2013-05-30T00:40:41Z	-
dc.date.available	2013-05-30T00:40:41Z	-
dc.date.issued	2013-05-30	-
dc.identifier	http://www.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332001000100011	-
dc.identifier	http://www.doaj.org/doaj?func=openurl&genre=article&issn=01039733&date=2001&volume=31&issue=1&spage=58	-
dc.identifier.uri	http://koha.mediu.edu.my:8181/jspui/handle/123456789/3146	-
dc.description	An equation for MHD stationary equilibrium of rotating plasmas in the azimuthal direction is derived in the case of an orthogonal curvilinear coordinate system. The basic assumptions we made are: (i) there is an ignorable coordinate so that surface quantities are independent of it; (ii) the entropy is a surface quantity.	-
dc.publisher	Sociedade Brasileira de Física	-
dc.source	Brazilian Journal of Physics	-
dc.title	Adiabatic plasma rotations in orthogonal coordinate systems	-
Appears in Collections:	Physics and Astronomy

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