Transport of cross helicity and radial evolution of alfvenicity in the solar wind

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dc.contributor.authorMatthaeus, William H.
dc.contributor.authorMinnie, J.
dc.contributor.authorBreech, Ben
dc.contributor.authorParhi, S.
dc.contributor.authorBieber, J.W.
dc.contributor.authorOughton, Sean
dc.date.accessioned2009-01-06T21:05:18Z
dc.date.available2009-01-06T21:05:18Z
dc.date.issued2004
dc.description.abstractA transport theory including cross helicity, magnetohydrodynamic(MHD) turbulence, and driving by shear and pickup ions, is applied to the radial evolution of the solar wind. The radial decrease of cross helicity observed in the solar wind can be accounted for when sufficient driving is included to overcome the inherent tendency for MHD turbulence to produce Alfvenic states.en
dc.format.mimetypeapplication/pdf
dc.identifier.citationMatthaeus, W.H., Minnie, J., Breech, B., Parhi, S., Bieber, J.W. & Oughton, S. (2004). Transport of cross helicity and radial evolution of alfvenicity in the solar wind. Geophysical Research Letters, 31(12).en
dc.identifier.doi10.1029/2004GL019465en
dc.identifier.urihttps://hdl.handle.net/10289/1741
dc.language.isoen
dc.publisherAmerican Geophysical Unionen_NZ
dc.relation.isPartOfGeophysical Research Lettersen_NZ
dc.relation.urihttp://www.agu.org/journals/gl/gl0412/2004GL019645/2004GL019645.pdfen
dc.rights© 2004 American Geophysical Union.
dc.subjectmathematicsen
dc.subjectinterplanetary Physicsen
dc.subjectMHD waves and turbulenceen
dc.subjectsolar wind plasmaen
dc.subjectspace plasma physicsen
dc.subjectnonlinear phenomenaen
dc.subjecttransport processesen
dc.titleTransport of cross helicity and radial evolution of alfvenicity in the solar winden
dc.typeJournal Articleen
dspace.entity.typePublication
pubs.begin-page1en_NZ
pubs.editionJuneen_NZ
pubs.end-page4en_NZ
pubs.issue12en_NZ
pubs.volume31en_NZ
uow.identifier.article-noARTN L12803en_NZ
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