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The new heliospheric magnetic field: Observational implications

dc.contributor.authorZurbuchen, Thomas H.en_US
dc.contributor.authorFisk, Lennard A.en_US
dc.contributor.authorHefti, S.en_US
dc.contributor.authorSchwadron, Nathan A.en_US
dc.date.accessioned2011-11-15T16:07:19Z
dc.date.available2011-11-15T16:07:19Z
dc.date.issued1999-06-16en_US
dc.identifier.citationZurbuchen, T. H.; Fisk, L. A.; Hefti, S.; Schwadron, N. A. (1999). "The new heliospheric magnetic field: Observational implications." AIP Conference Proceedings 471(1): 87-92. <http://hdl.handle.net/2027.42/87723>en_US
dc.identifier.otherAPCPCS-471-1en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/87723
dc.description.abstractA summary of the new model of the heliospheric magnetic field and its observational implications is presented. We first introduce a global model for the steady-state configuration in the low corona and discuss solar and heliospheric implications of the resulting field configuration. Finally, we compare the effects of this model with random transport of field-lines due to reconnection on the solar surface and to the dynamic turbulent transport of magnetic field-lines. © 1999 American Institute of Physics.en_US
dc.publisherThe American Institute of Physicsen_US
dc.rights© The American Institute of Physicsen_US
dc.titleThe new heliospheric magnetic field: Observational implicationsen_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelPhysicsen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumDepartment of Atmospheric, Oceanic and Space Sciences, University of Michigan, Ann Arboren_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/87723/2/87_1.pdf
dc.identifier.doi10.1063/1.58737en_US
dc.identifier.sourceThe solar wind nine conferenceen_US
dc.owningcollnamePhysics, Department of


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