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dc.contributor.authorBreech, Ben
dc.contributor.authorMatthaeus, William H.
dc.contributor.authorMinnie, J.
dc.contributor.authorOughton, Sean
dc.contributor.authorOarhi, S.
dc.contributor.authorBieber, J.W.
dc.contributor.authorBavassano, B.
dc.date.accessioned2014-03-28T02:48:30Z
dc.date.available2014-03-28T02:48:30Z
dc.date.copyright2005
dc.date.issued2005
dc.identifier.citationBreech, B., Matthaeus, W. H., Minnie, J., Oughton, S., Oarhi, S., Bieber, J. W., & Bavassano, B. (2005). Radial evolution of cross helicity in high-latitude solar wind. Geophysical Research Letters, 32(6), L06103.en_NZ
dc.identifier.urihttps://hdl.handle.net/10289/8578
dc.description.abstractWe employ a turbulence transport theory to explain the high-latitude radial evolution of cross helicity, or Alfvénicity, observed by the Ulysses spacecraft. Evolution is slower than at low latitudes due to weakened shear driving.en_NZ
dc.format.mimetypeapplication/pdf
dc.language.isoenen_NZ
dc.publisherAmerican Geophysical Unionen_NZ
dc.relation.ispartofGeophysical Research Letters
dc.relation.urihttp://onlinelibrary.wiley.com/doi/10.1029/2004GL022321/abstracten_NZ
dc.rights© 2005 the American Geophysical Unionen_NZ
dc.subjectsolar winden_NZ
dc.titleRadial evolution of cross helicity in high-latitude solar winden_NZ
dc.typeJournal Articleen_NZ
dc.identifier.doi10.1029/2004gl022321en_NZ
dc.relation.isPartOfGeophysical Research Lettersen_NZ
pubs.begin-page1en_NZ
pubs.elements-id31930
pubs.end-page4en_NZ
pubs.issue6en_NZ
pubs.volume32en_NZ
uow.identifier.article-noARTN L06103en_NZ


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