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dc.contributor.authorMatthaeus, William H.
dc.contributor.authorDmitruk, Pablo
dc.contributor.authorSmith, D.
dc.contributor.authorGhosh, S.
dc.contributor.authorOughton, Sean
dc.date.accessioned2009-01-06T21:18:49Z
dc.date.available2009-01-06T21:18:49Z
dc.date.issued2003
dc.identifier.citationMatthaeus, W.H., Dmitruk, P., Smith, D., Ghosh, S. & Oughton, S. (2003). Impact of Hall effect on energy dacay in magnetohydrodynamic turbulence. Geophysical Research Letters, 30(21), 2104.en
dc.identifier.urihttps://hdl.handle.net/10289/1742
dc.description.abstractWe examine numerically the influence of Hall effect corrections to Ohm's law upon the decay of homogeneous compressible magnetohydrodynamic turbulence and conclude that there are no significant differences in global decay rate associated with the Hall effect. This affirms expectations that energy decay is controlled by the large-scale eddies.en
dc.format.mimetypeapplication/pdf
dc.language.isoen
dc.publisherAmerican Geophysical Unionen_NZ
dc.relation.urihttp://www.agu.org/journals/gl/gl0321/2003GL017949/en
dc.subjectmathematicsen
dc.subjectinterplanetary Physicsen
dc.subjectMHD waves and turbulenceen
dc.subjectmagnetospheric Physicsen
dc.subjectMHD waves and instabilitiesen
dc.subjectspace Plasma Physicsen
dc.subjectkinetic and MHD theoryen
dc.subjectturbulenceen
dc.subjectWave/particle interactionsen
dc.titleImpact of Hall effect on energy decay in magnetohydrodynamic turbulenceen
dc.typeJournal Articleen
dc.identifier.doi10.1029/2003GL017949en
dc.relation.isPartOfGeophysical Research Lettersen_NZ
pubs.begin-page1en_NZ
pubs.elements-id29595
pubs.end-page5en_NZ
pubs.issue21en_NZ
pubs.volume30en_NZ
uow.identifier.article-noARTN 2104en_NZ


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