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dc.contributor.authorBurch, James L.
dc.contributor.authorWebster, James M.
dc.contributor.authorHesse, Michael
dc.contributor.authorGenestreti, Kevin J.
dc.contributor.authorDenton, Richard E.
dc.contributor.authorPhan, Tai D.
dc.contributor.authorHasegawa, Hiroshi
dc.contributor.authorCassak, Paul A.
dc.contributor.authorTorbert, Roy B.
dc.contributor.authorGiles, Barbara L.
dc.contributor.authorGershman, Daniel J.
dc.contributor.authorErgun, Robert E.
dc.contributor.authorRussell, Christopher T.
dc.contributor.authorStrangeway, Robert J.
dc.contributor.authorLe Contel, Olivier
dc.contributor.authorPritchard, Kris R.
dc.contributor.authorMarshall, Andrew T.
dc.contributor.authorHwang, Kyoung-Joo
dc.contributor.authorDokgo, Kyunghwan
dc.contributor.authorFuselier, Stephen A.
dc.contributor.authorChen, Li-Jen
dc.contributor.authorWang, Shan
dc.contributor.authorSwisdak, Marc
dc.contributor.authorDrake, James F.
dc.contributor.authorArgall, Matthew R.
dc.contributor.authorTrattner, Karlheinz J.
dc.contributor.authorYamada, Masaaki
dc.contributor.authorPaschmann, Götz
dc.date.accessioned2021-08-02T11:00:38Z
dc.date.available2021-08-02T11:00:38Z
dc.date.created2020-09-26T13:18:09Z
dc.date.issued2020
dc.identifier.issn0094-8276
dc.identifier.urihttps://hdl.handle.net/11250/2765825
dc.description.abstractElectron inflow and outflow velocities during magnetic reconnection at and near the dayside magnetopause are measured using satellites from NASA's Magnetospheric Multiscale (MMS) mission. A case study is examined in detail, and three other events with similar behavior are shown, with one of them being a recently published electron-only reconnection event in the magnetosheath. The measured inflow speeds of 200–400 km/s imply dimensionless reconnection rates of 0.05–0.25 when normalized to the relevant electron Alfvén speed, which are within the range of expectations. The outflow speeds are about 1.5–3 times the inflow speeds, which is consistent with theoretical predictions of the aspect ratio of the inner electron diffusion region. A reconnection rate of 0.04 ± 25% was obtained for the case study event using the reconnection electric field as compared to the 0.12 ± 20% rate determined from the inflow velocity.en_US
dc.language.isoengen_US
dc.publisherAGUen_US
dc.rightsNavngivelse 4.0 Internasjonal*
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/deed.no*
dc.titleElectron inflow velocities and reconnection rates at earth's magnetopause and magnetosheathen_US
dc.typeJournal articleen_US
dc.typePeer revieweden_US
dc.description.versionpublishedVersionen_US
dc.rights.holderCopyright 2020 The Authorsen_US
dc.source.articlenumbere2020GL089082en_US
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode2
dc.identifier.doi10.1029/2020GL089082
dc.identifier.cristin1833753
dc.source.journalGeophysical Research Lettersen_US
dc.identifier.citationGeophysical Research Letters. 2020, 47(17):e2020GL089082en_US
dc.source.volume47en_US
dc.source.issue17en_US


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Navngivelse 4.0 Internasjonal
Except where otherwise noted, this item's license is described as Navngivelse 4.0 Internasjonal