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dc.contributor.authorOhtani, S.
dc.contributor.authorGjerløv, Jesper
dc.contributor.authorMcWilliams, Kathryn A.
dc.contributor.authorRuohoniemi, J. M.
dc.contributor.authorFrey, Harald U.
dc.date.accessioned2022-03-16T13:33:38Z
dc.date.available2022-03-16T13:33:38Z
dc.date.created2022-01-25T12:52:44Z
dc.date.issued2021
dc.identifier.issn2169-9380
dc.identifier.urihttps://hdl.handle.net/11250/2985595
dc.description.abstractThe expansion phase of auroral substorms is characterized by the formation of an auroral bulge, and it is generally considered that a single bulge forms following each substorm onset. However, we find that occasionally two auroral intensifications takes place close in time but apart in space leading to the formation of double auroral bulges, which later merge into one large bulge. We report three such events. In those events the westward auroral electrojet intensified in each auroral bulge, and geosynchronous magnetic field dipolarized in the same sector. It appears that two substorms took place simultaneously, and each substorm was accompanied by the formation of its own substorm current wedge system. This finding strongly suggests that the initiation of auroral substorms is a local process, and there is no global reference frame for their development. For example, ideas such as (i) the auroralbreakup takes place in the vicinity of the Harang reversal and (ii) the westward traveling surge maps to the interface between the plasma sheet and low-latitude boundary layer, do not necessarily hold for every substorm. Even if those ideas may be suggestive of causal magnetospheric processes, the reference structures themselves are probably not essential. It is also found that despite the formation of two distinct auroral bulges, the overall magnetosphere-ionosphere current system is represented by one globally coherent system, and we suggest that its structure is determined by the relative intensities and locations of the two substorm current wedges that correspond to the individual auroral bulges.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.titleSimultaneous Development of Multiple Auroral Substorms: Double Auroral Bulge Formationen_US
dc.typeJournal articleen_US
dc.typePeer revieweden_US
dc.description.versionpublishedVersionen_US
dc.rights.holderCopyright 2021. The Authorsen_US
dc.source.articlenumbere2020JA028883en_US
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode2
dc.identifier.doi10.1029/2020JA028883
dc.identifier.cristin1989458
dc.source.journalJournal of Geophysical Research (JGR): Space Physicsen_US
dc.identifier.citationJournal of Geophysical Research: Space Physics. 2021, 126 (5), e2020JA028883.en_US
dc.source.volume126en_US
dc.source.issue5en_US


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