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dc.contributor.authorElhawary, Reham Zakaria Ahmed Mohamed
dc.contributor.authorLaundal, Karl Magnus
dc.contributor.authorReistad, Jone Peter
dc.contributor.authorMadelaire, Michael
dc.date.accessioned2024-08-30T06:57:46Z
dc.date.available2024-08-30T06:57:46Z
dc.date.created2024-08-29T13:37:02Z
dc.date.issued2024
dc.identifier.issn2169-9380
dc.identifier.urihttps://hdl.handle.net/11250/3149196
dc.description.abstractIonospheric dynamics exhibits a distinct hemispheric asymmetry, influenced primarily by the Interplanetary Magnetic Field (IMF) By component, dipole tilt, or a combination of both. Previous studies have indicated a reduction in these asymmetries during substorms. In this study, we conduct a superposed epoch analysis using ground magnetometer data from the northern hemisphere to examine the impact of substorms on ionospheric current asymmetry. This analysis uses the assumption of mirror symmetry between the northern and southern hemispheres when IMF By and dipole tilt are reversed. We observe a significant reduction in nightside equivalent current asymmetry indicating the IMF By and dipole tilt have minimal influence on the substorm current. On the other hand, we find that substorms exert minimal or negligible effects on dayside currents. This difference in response between nightside and dayside currents emphasizes the need to incorporate nightside dynamics into existing climatological models, which presently rely mainly on upstream parameters due to a lack of robust parameters effectively representing them. Our findings provide important insights for future modeling efforts, highlighting the distinct interactions between substorms and ionospheric currents across different hemispheric regions.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.titleHow Do Substorms Influence Hemispheric Asymmetries in Equivalent Currents?en_US
dc.typeJournal articleen_US
dc.typePeer revieweden_US
dc.description.versionpublishedVersionen_US
dc.rights.holderCopyright 2024 The Author(s)en_US
dc.source.articlenumbere2024JA032507en_US
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode2
dc.identifier.doihttps://doi.org/10.1029/2024JA032507
dc.identifier.cristin2290490
dc.source.journalJournal of Geophysical Research (JGR): Space Physicsen_US
dc.identifier.citationJournal of Geophysical Research (JGR): Space Physics. 2024, 129 (8), e2024JA032507.en_US
dc.source.volume129en_US
dc.source.issue8en_US


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