Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/3793
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dc.contributor.authorSridhar, S.-
dc.contributor.authorSubramanian, Kandaswamy-
dc.date.accessioned2009-07-15T06:48:00Z-
dc.date.available2009-07-15T06:48:00Z-
dc.date.issued2009-04-
dc.identifier.citationPhysical Review E, 2009, Vol.79, p045305en
dc.identifier.issnE-ISSN: 1550-2376-
dc.identifier.issnP-ISSN: 1539-3755-
dc.identifier.urihttp://hdl.handle.net/2289/3793-
dc.descriptionOpen Accessen
dc.description.abstractLarge-scale dynamo action due to turbulence in the presence of a linear shear flow is studied. Our treatment is quasilinear and kinematic but is nonperturbative in the shear strength. We derive the integrodifferential equation for the evolution of the mean magnetic field by systematic use of the shearing coordinate transformation and the Galilean invariance of the linear shear flow. For nonhelical turbulence the time evolution of the cross-shear components of the mean field does not depend on any other components excepting themselves. This is valid for any Galilean-invariant velocity field, independent of its dynamics. Hence the shear-current assisted dynamo is essentially absent, although large-scale nonhelical dynamo action is not ruled out.en
dc.language.isoenen
dc.publisherAmerican Physical Societyen
dc.relation.urihttp://dx.doi.org/ 10.1103/PhysRevE.79.045305en
dc.relation.urihttp://arxiv.org/abs/0812.3269en
dc.rights2009 The American Physical Societyen
dc.subjectcomputational fluid dynamicsen
dc.subjectintegro-differential equationsen
dc.subjectinvarianceen
dc.subjectmagnetohydrodynamicsen
dc.subjectshear turbulenceen
dc.titleShear dynamo problem: quasilinear kinematic theoryen
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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