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Field dipolarization in Saturn's magnetotail with planetward ion flows and energetic particle flow bursts: Evidence of quasi‐steady reconnection

dc.contributor.authorJackman, C. M.en_US
dc.contributor.authorThomsen, M. F.en_US
dc.contributor.authorMitchell, D. G.en_US
dc.contributor.authorSergis, N.en_US
dc.contributor.authorArridge, C. S.en_US
dc.contributor.authorFelici, M.en_US
dc.contributor.authorBadman, S. V.en_US
dc.contributor.authorParanicas, C.en_US
dc.contributor.authorJia, X.en_US
dc.contributor.authorHospodarksy, G. B.en_US
dc.contributor.authorAndriopoulou, M.en_US
dc.contributor.authorKhurana, K. K.en_US
dc.contributor.authorSmith, A. W.en_US
dc.contributor.authorDougherty, M. K.en_US
dc.date.accessioned2015-07-01T20:56:46Z
dc.date.available2016-07-05T17:27:58Zen
dc.date.issued2015-05en_US
dc.identifier.citationJackman, C. M.; Thomsen, M. F.; Mitchell, D. G.; Sergis, N.; Arridge, C. S.; Felici, M.; Badman, S. V.; Paranicas, C.; Jia, X.; Hospodarksy, G. B.; Andriopoulou, M.; Khurana, K. K.; Smith, A. W.; Dougherty, M. K. (2015). "Field dipolarization in Saturn's magnetotail with planetward ion flows and energetic particle flow bursts: Evidence of quasi‐steady reconnection." Journal of Geophysical Research: Space Physics 120(5): 3603-3617.en_US
dc.identifier.issn2169-9380en_US
dc.identifier.issn2169-9402en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/111992
dc.description.abstractWe present a case study of an event from 20 August (day 232) of 2006, when the Cassini spacecraft was sampling the region near 32 RS and 22 h LT in Saturn's magnetotail. Cassini observed a strong northward‐to‐southward turning of the magnetic field, which is interpreted as the signature of dipolarization of the field as seen by the spacecraft planetward of the reconnection X line. This event was accompanied by very rapid (up to ~1500 km s−1) thermal plasma flow toward the planet. At energies above 28 keV, energetic hydrogen and oxygen ion flow bursts were observed to stream planetward from a reconnection site downtail of the spacecraft. Meanwhile, a strong field‐aligned beam of energetic hydrogen was also observed to stream tailward, likely from an ionospheric source. Saturn kilometric radiation emissions were stimulated shortly after the observation of the dipolarization. We discuss the field, plasma, energetic particle, and radio observations in the context of the impact this reconnection event had on global magnetospheric dynamics.Key PointsRare observation of strong planetward flow following Saturn tail reconnectionIon flows at speeds of up to 1500 km/s observed, indicating energetic eventData imply quasi‐steady Vasyliunas‐type reconnection beyond 32 RSen_US
dc.publisherAGUen_US
dc.publisherWiley Periodicals, Inc.en_US
dc.subject.otherSaturnen_US
dc.subject.otherreconnectionen_US
dc.subject.otherbeamsen_US
dc.subject.othermagnetotailen_US
dc.titleField dipolarization in Saturn's magnetotail with planetward ion flows and energetic particle flow bursts: Evidence of quasi‐steady reconnectionen_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/2027.42/111992/1/jgra51764.pdf
dc.identifier.doi10.1002/2015JA020995en_US
dc.identifier.sourceJournal of Geophysical Research: Space Physicsen_US
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