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dc.contributor.authorJimenez, Judit Perez-Coll
dc.contributor.authorTenfjord, Paul Arne Riksheim
dc.contributor.authorHesse, Michael
dc.contributor.authorNorgren, Astrid Elisabet Cecilia
dc.contributor.authorKwagala, Norah Kaggwa
dc.contributor.authorKolstø, Håkon Midthun
dc.contributor.authorSpinnangr, Susanne Flø
dc.date.accessioned2023-03-31T10:29:37Z
dc.date.available2023-03-31T10:29:37Z
dc.date.created2022-09-26T08:49:35Z
dc.date.issued2022
dc.identifier.issn2169-9380
dc.identifier.urihttps://hdl.handle.net/11250/3061379
dc.description.abstractUsing a resistive MagnetoHydroDynamic (MHD) simulation, we study how the magnitude and shape of diffusion influence magnetic reconnection. Specifically, we investigate how and why the reconnection rate is influenced by variations in the diffusion distribution and magnitude. By running multiple MHD simulations where we vary the localized resistivity, we find that the properties of the diffusion region greatly influence the rate of reconnection. Increasing the magnitude of the imposed resistivity results in a higher reconnection rate, but the rate saturates at approximately 0.2. We show how a redistribution of the current density, leading to a bifurcated current sheet, play a major role in this limitation. In addition, we investigate the impact of different shapes of resistive region. The shape of the diffusion region also plays a major role in how efficient the reconnection energy conversion can operate. The highest reconnection rate, approximately 0.25, is achieved for an optimal opening angle. Our results imply that reconnection has a speed limit that may depend on properties outside the diffusion region.en_US
dc.language.isoengen_US
dc.publisherWileyen_US
dc.rightsNavngivelse 4.0 Internasjonal*
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/deed.no*
dc.titleThe Role of Resistivity on the Efficiency of Magnetic Reconnection in MHDen_US
dc.typeJournal articleen_US
dc.typePeer revieweden_US
dc.description.versionpublishedVersionen_US
dc.rights.holderCopyright 2022. The Authorsen_US
dc.source.articlenumbere2021JA030134en_US
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode2
dc.identifier.doi10.1029/2021JA030134
dc.identifier.cristin2055209
dc.source.journalJournal of Geophysical Research (JGR): Space Physicsen_US
dc.identifier.citationJournal of Geophysical Research: Space Physics. 2022, 127 (6), e2021JA030134.en_US
dc.source.volume127en_US
dc.source.issue6en_US


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