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Comparison of the open‐closed separatrix in a global magnetospheric simulation with observations: The role of the ring current

dc.contributor.authorRae, I. J.en_US
dc.contributor.authorKabin, K.en_US
dc.contributor.authorLu, J. Y.en_US
dc.contributor.authorRankin, R.en_US
dc.contributor.authorMilan, S. E.en_US
dc.contributor.authorFenrich, F. R.en_US
dc.contributor.authorWatt, C. E. J.en_US
dc.contributor.authorZhang, J.‐c.en_US
dc.contributor.authorRidley, A. J.en_US
dc.contributor.authorGombosi, T. I.en_US
dc.contributor.authorClauer, C. R.en_US
dc.contributor.authorTóth, G.en_US
dc.contributor.authorDeZeeuw, D. L.en_US
dc.date.accessioned2013-01-03T19:42:55Z
dc.date.available2013-01-03T19:42:55Z
dc.date.issued2010-08en_US
dc.identifier.citationRae, I. J.; Kabin, K.; Lu, J. Y.; Rankin, R.; Milan, S. E.; Fenrich, F. R.; Watt, C. E. J.; Zhang, J.‐c. ; Ridley, A. J.; Gombosi, T. I.; Clauer, C. R.; Tóth, G. ; DeZeeuw, D. L. (2010). "Comparison of the openâ closed separatrix in a global magnetospheric simulation with observations: The role of the ring current." Journal of Geophysical Research: Space Physics 115(A8): n/a-n/a. <http://hdl.handle.net/2027.42/95344>en_US
dc.identifier.issn0148-0227en_US
dc.identifier.issn2156-2202en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/95344
dc.publisherWiley Periodicals, Inc.en_US
dc.subject.otherReconnectionen_US
dc.subject.otherGlobal Convectionen_US
dc.subject.otherRing Currenten_US
dc.titleComparison of the open‐closed separatrix in a global magnetospheric simulation with observations: The role of the ring currenten_US
dc.typeArticleen_US
dc.rights.robotsIndexNoFollowen_US
dc.subject.hlbsecondlevelAstronomy and Astrophysicsen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/95344/1/jgra20421.pdf
dc.identifier.doi10.1029/2009JA015068en_US
dc.identifier.sourceJournal of Geophysical Research: Space Physicsen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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