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dc.contributor.authorMcKay, Derek
dc.contributor.authorPaavilainen, Tuula
dc.contributor.authorGustavsson, Björn Johan
dc.contributor.authorKvammen, Andreas
dc.contributor.authorPartamies, Noora
dc.date.accessioned2020-03-30T13:38:39Z
dc.date.available2020-03-30T13:38:39Z
dc.date.created2019-08-13T14:35:02Z
dc.date.issued2019
dc.identifier.citationGeophysical Research Letters. 2019, 46 (13), 7214-7221.
dc.identifier.issn0094-8276
dc.identifier.urihttps://hdl.handle.net/11250/2649443
dc.description.abstractThe development of a magnetospheric substorm may be classified into three phases: growth, expansion, and recovery. The growth phase is important as it includes processes that lead to the expansion. In a recent growth-phase study, a type of fast discrete auroral transient phenomena -- referred to as Lumikot -- were observed. The Lumikot are several kilometers across and move in the high-energy precipitation region, parallel to the main growth-phase arc, with both east-west and west-east directions of travel during the same event. Their apparent transverse movement and quasi-stable intensity make them distinct from co-occurring optical pulsating aurorae. Comparison to other studies show that they occur in the cosmic noise absorption region and it is likely that the Lumikot are co-located with high-energy particle populations on the boundary between the outer radiation belt and the plasmasheet.
dc.language.isoeng
dc.titleLumikot: Fast auroral transients during the growth phase of substorms
dc.typePeer reviewed
dc.typeJournal article
dc.description.versionpublishedVersion
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode2
dc.identifier.doi10.1029/2019GL082985
dc.identifier.cristin1715636
dc.source.journalGeophysical Research Letters
dc.source.volume46
dc.source.issue13
dc.source.pagenumber7214-7221
dc.relation.projectNorges forskningsråd: 223252


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