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dc.contributor.authorWalsh, Andrew P.eng
dc.contributor.authorHaaland, Steineng
dc.contributor.authorForsyth, Colineng
dc.contributor.authorKeesee, Amy M.eng
dc.contributor.authorKissinger, Jennifereng
dc.contributor.authorLi, Kuneng
dc.contributor.authorRunov, Andreieng
dc.contributor.authorSoucek, Josefeng
dc.contributor.authorWalsh, Brian M.eng
dc.contributor.authorWing, Simoneng
dc.contributor.authorTaylor, Matthew G.G.T.eng
dc.PublishedAnnales Geophysicae 2014, 32(7):705-737eng
dc.description.abstractDawn–dusk asymmetries are ubiquitous features of the coupled solar-wind–magnetosphere–ionosphere system. During the last decades, increasing availability of satellite and ground-based measurements has made it possible to study these phenomena in more detail. Numerous publications have documented the existence of persistent asymmetries in processes, properties and topology of plasma structures in various regions of geospace. In this paper, we present a review of our present knowledge of some of the most pronounced dawn–dusk asymmetries. We focus on four key aspects: (1) the role of external influences such as the solar wind and its interaction with the Earth's magnetosphere; (2) properties of the magnetosphere itself; (3) the role of the ionosphere and (4) feedback and coupling between regions. We have also identified potential inconsistencies and gaps in our understanding of dawn–dusk asymmetries in the Earth's magnetosphere and ionosphere.en_US
dc.publisherCopernicus Publicationsen_US
dc.rightsAttribution CC BYeng
dc.titleDawn-dusk asymmetries in the coupled solar wind-magnetosphere-ionosphere system: a reviewen_US
dc.typePeer reviewed
dc.typeJournal article
dc.rights.holderCopyright 2014 The Authorsen_US
dc.subject.nsiVDP::Matematikk og naturvitenskap: 400::Fysikk: 430::Rom- og plasmafysikk: 437
dc.subject.nsiVDP::Mathematics and natural scienses: 400::Physics: 430::Space and plasma physics: 437

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