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dc.contributor.authorMoretto, T
dc.contributor.authorHesse, Michael
dc.contributor.authorVennerstrøm, Susanne
dc.contributor.authorTenfjord, Paul
dc.date.accessioned2019-05-28T08:24:14Z
dc.date.available2019-05-28T08:24:14Z
dc.date.issued2018-12
dc.PublishedMoretto T, Hesse M, Vennerstrøm S, Tenfjord PAR. Estimating the Rate of Cessation of Magnetospheric Activity in AMPERE Field‐Aligned Currents. Geophysical Research Letters. 2018;45(23):12713-12719eng
dc.identifier.issn1944-8007en_US
dc.identifier.issn0094-8276en_US
dc.identifier.urihttps://hdl.handle.net/1956/19751
dc.description.abstractThe decay of magnetospheric activity when driving is turned off (to a minimum) was measured in total field‐aligned current estimates from the Active Magnetosphere and Planetary Electrodynamics Response Experiment (AMPERE) project. Events of distinct northward turnings of the interplanetary magnetic field were identified, with prolonged periods of stable southward driving conditions followed by northward interplanetary magnetic field conditions. All but 4 of 43 identified events exhibit a well‐defined exponential decay in the total hemispheric field‐aligned current following the northward turning. A superposed epoch analysis yields a generic decay constant of 0.9, corresponding to an e‐folding time of 1.1 hr. A statistical analysis of the ensemble of events also reveals a seasonal variation in the decay parameter with faster decay observed in the winter than in the summer hemisphere. This result can be understood in terms of stronger/weaker line tying of the ionospheric foot points of magnetospheric field lines for higher/lower conductivity.en_US
dc.language.isoengeng
dc.publisherWileyen_US
dc.rightsAttribution CC BY-NC-NDeng
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/4.0/eng
dc.titleEstimating the Rate of Cessation of Magnetospheric Activity in AMPERE Field‐Aligned Currentsen_US
dc.typePeer reviewed
dc.typeJournal article
dc.date.updated2019-01-04T13:38:31Z
dc.description.versionpublishedVersionen_US
dc.rights.holderCopyright 2018 The Author(s)en_US
dc.identifier.doihttps://doi.org/10.1029/2018gl080631
dc.identifier.cristin1650563
dc.source.journalGeophysical Research Letters
dc.relation.projectNorges forskningsråd: 223252


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