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dc.contributor.authorHaaland, Stein
dc.contributor.authorRunov, Andrei
dc.contributor.authorArtemyev, Anton
dc.contributor.authorAngelopoulos, Vassillis
dc.date.accessioned2020-06-08T13:43:14Z
dc.date.available2020-06-08T13:43:14Z
dc.date.issued2019-05-30
dc.PublishedHaaland SE, Runov A, Artemyev A, Angelopoulos V. Characteristics of the Flank Magnetopause: THEMIS Observations. Journal of Geophysical Research (JGR): Space Physics. 2019;124(5)eng
dc.identifier.issn2169-9402en_US
dc.identifier.issn2169-9380en_US
dc.identifier.urihttps://hdl.handle.net/1956/22494
dc.description.abstractThe terrestrial magnetopause is the boundary that shields the Earth's magnetosphere on one side from the shocked solar wind and its embedded interplanetary magnetic field on the other side. In this paper, we show observations from two of the Time History of Events and Macroscales Interactions during Substorms (THEMIS) satellites, comparing dayside magnetopause crossings with flank crossings near the terminator. Macroscopic properties such as current sheet thickness, motion, and current density are examined for a large number of magnetopause crossings. The results show that the flank magnetopause is typically thicker than the dayside magnetopause and has a lower current density. Consistent with earlier results from Cluster observations, we also find a persistent dawn‐dusk asymmetry with a thicker and more dynamic magnetopause at dawn than at dusk.en_US
dc.language.isoengeng
dc.publisherAGUen_US
dc.rightsAttribution CC BY-NC-NDeng
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/4.0/eng
dc.titleCharacteristics of the Flank Magnetopause: THEMIS Observationsen_US
dc.typePeer reviewed
dc.typeJournal article
dc.date.updated2019-11-22T09:36:09Z
dc.description.versionpublishedVersionen_US
dc.rights.holderCopyright 2019 The Authorsen_US
dc.identifier.doihttps://doi.org/10.1029/2019ja026459
dc.identifier.cristin1704729
dc.source.journalJournal of Geophysical Research (JGR): Space Physics


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