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Global simulations of magnetorotational turbulence - I. Convergence and the quasi-steady state

Parkin, Elliott; Bicknell, Geoffrey

Description

Magnetorotational turbulence provides a viable mechanism for angular momentum transport in accretion discs. We present global, three-dimensional (3D), magnetohydrodynamic accretion disc simulations that investigate the dependence of the turbulent stresses

dc.contributor.authorParkin, Elliott
dc.contributor.authorBicknell, Geoffrey
dc.date.accessioned2015-12-13T22:31:20Z
dc.identifier.issn0035-8711
dc.identifier.urihttp://hdl.handle.net/1885/75204
dc.description.abstractMagnetorotational turbulence provides a viable mechanism for angular momentum transport in accretion discs. We present global, three-dimensional (3D), magnetohydrodynamic accretion disc simulations that investigate the dependence of the turbulent stresses
dc.publisherBlackwell Publishing Ltd
dc.rightsAuthor/s retain copyright
dc.sourceMonthly Notices of the Royal Astronomical Society
dc.subjectKeywords: Accretion; Accretion discs; Instabilities; MHD; Turbulence.
dc.titleGlobal simulations of magnetorotational turbulence - I. Convergence and the quasi-steady state
dc.typeJournal article
local.description.notesImported from ARIES
local.identifier.citationvolume435
dc.date.issued2013
local.identifier.absfor020100 - ASTRONOMICAL AND SPACE SCIENCES
local.identifier.ariespublicationf5625xPUB4514
local.type.statusPublished Version
local.contributor.affiliationParkin, Elliott, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationBicknell, Geoffrey, College of Physical and Mathematical Sciences, ANU
local.bibliographicCitation.issue3
local.bibliographicCitation.startpage2281
local.bibliographicCitation.lastpage2298
local.identifier.doi10.1093/mnras/stt1450
dc.date.updated2016-02-24T09:25:59Z
local.identifier.scopusID2-s2.0-84885743886
local.identifier.thomsonID000325773000036
dcterms.accessRightsOpen Access
CollectionsANU Research Publications

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