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dc.contributor.authorKolstø, Håkon Midthun
dc.contributor.authorHesse, Michael
dc.contributor.authorNorgren, Astrid Elisabet Cecilia
dc.contributor.authorTenfjord, Paul
dc.contributor.authorSpinnangr, Susanne Flø
dc.contributor.authorKwagala, Norah Kaggwa
dc.date.accessioned2021-05-28T08:23:27Z
dc.date.available2021-05-28T08:23:27Z
dc.date.created2021-01-19T11:57:46Z
dc.date.issued2020
dc.identifier.issn0094-8276
dc.identifier.urihttps://hdl.handle.net/11250/2756794
dc.description.abstractCombined with the magnetic field, the distribution of charged particles in the inflow region is expected to control the rate of magnetic reconnection. This paper investigates how the reconnection process is altered by a cold, asymmetrically distributed, oxygen population, which is initially located away from the current layer in the inflow regions. A particle-in-cell simulation is used to gain further insight into the dynamics of the system. The time evolution of the reconnection process proceeds rapidly compared to the cyclotron period of O urn:x-wiley:grl:media:grl59941:grl59941-math-0001. Therefore, the oxygen remains, to a good approximation, demagnetized. Thus, Alfvén scaling is not an adequate description of the reconnection rate. A scaling relation for the reconnection rate for an asymmetrically distributed, demagnetized species has been developed. Additionally, we find that an asymmetric density configuration leads to a distinct motion of the reconnection site and generates an asymmetry of the diffusion region and the Hall electric field.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.titleCollisionless Magnetic Reconnection in an Asymmetric Oxygen Density Configurationen_US
dc.typeJournal articleen_US
dc.typePeer revieweden_US
dc.description.versionpublishedVersionen_US
dc.rights.holderCopyright 2020 The Authorsen_US
dc.source.articlenumbere2019GL085359en_US
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode2
dc.identifier.doi10.1029/2019GL085359
dc.identifier.cristin1874200
dc.source.journalGeophysical Research Lettersen_US
dc.source.4047
dc.source.141
dc.identifier.citationGeophysical Research Letters. 2020, 47(1), e2019GL085359en_US
dc.source.volume47en_US
dc.source.issue1en_US


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