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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5713
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dc.contributor.authorFurukawa, M-
dc.contributor.authorKrishan, V-
dc.contributor.authorHirota, M-
dc.contributor.authorYoshida, Z-
dc.date.accessioned2012-03-01T10:03:14Z-
dc.date.available2012-03-01T10:03:14Z-
dc.date.issued2006-
dc.identifier.citationPlasma and Fusion Research, Vol. 1, pp. 001-1 - 001-2en
dc.identifier.urihttp://hdl.handle.net/2248/5713-
dc.description.abstractThe temporal behavior of axisymmetric magneto-rotational instability in a thin accretion disk is analyzed via the Wentzel-Kramars-Brillouin (WKB) method. The height of the thin disk is used as a small parameter. It is found that the oscillation of the envelope of the mode accelerates with time because of the density distribution in the direction of the disk height.en
dc.language.isoenen
dc.publisherThe Japan Society of Plasma Science and Nuclear Fusion Researchen
dc.relation.urihttp://dx.doi.org/10.1585/pfr.1.001en
dc.rights© The Japan Society of Plasma Science and Nuclear Fusion Researchen
dc.subjectMagneto-rotational instabilityen
dc.subjectAccretion disken
dc.subjectWKB analysisen
dc.titleWKB Analysis of Axisymmetric Magneto-Rotational Instability in a Thin Accretion Disken
dc.typeArticleen
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