Erosion of the plasmasphere during a storm

dc.citation.firstpage9320en_US
dc.citation.issueNumber9en_US
dc.citation.journalTitleJournal of Geophysical Research: Space Physicsen_US
dc.citation.lastpage9328en_US
dc.citation.volumeNumber122en_US
dc.contributor.authorKrall, J.en_US
dc.contributor.authorHuba, J.D.en_US
dc.contributor.authorSazykin, S.en_US
dc.date.accessioned2018-06-29T16:54:54Zen_US
dc.date.available2018-06-29T16:54:54Zen_US
dc.date.issued2017en_US
dc.description.abstractThe erosion of the plasmasphere during a storm is analyzed using the Naval Research Laboratory Sami3 is Also a Model of the Ionosphere ionosphere/plasmasphere code, coupled to the Rice Convection Model of the inner magnetosphere and ring current. We reproduce the commonly observed poststorm plasmasphere profile, with strong erosion outside of a sharp, poststorm plasmapause, and weak erosion inside the plasmapause. We find that inclusion of the ring current E field sharpens the poststorm plasmapause. In the case of a weak storm, erosion inside the poststorm plasmapause might not occur. In all cases, plasma flows are dominated by E × B drifts. For strong storms, we find that erosion, both inside and outside of the poststorm plasmapause, is caused by outward E × B drifts.en_US
dc.identifier.citationKrall, J., Huba, J.D. and Sazykin, S.. "Erosion of the plasmasphere during a storm." <i>Journal of Geophysical Research: Space Physics,</i> 122, no. 9 (2017) Wiley: 9320-9328. https://doi.org/10.1002/2017JA024450.en_US
dc.identifier.doihttps://doi.org/10.1002/2017JA024450en_US
dc.identifier.urihttps://hdl.handle.net/1911/102323en_US
dc.language.isoengen_US
dc.publisherWileyen_US
dc.rightsArticle is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.en_US
dc.titleErosion of the plasmasphere during a stormen_US
dc.typeJournal articleen_US
dc.type.dcmiTexten_US
dc.type.publicationpublisher versionen_US
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