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dc.contributor.authorHaaland, S.
dc.contributor.authorLybekk, B.
dc.contributor.authorMaes, L.
dc.contributor.authorLaundal, K.
dc.contributor.authorPedersen, A.
dc.contributor.authorTenfjord, P.
dc.contributor.authorOhma, A.
dc.contributor.authorØstgaard, N.
dc.contributor.authorReistad, J.
dc.contributor.authorSnekvik, K.
dc.date2017
dc.date.accessioned2017-02-27T11:57:20Z
dc.date.available2017-02-27T11:57:20Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/4792
dc.descriptionIn this paper, we present observations of cold (0–70 eV) plasma density in the magnetotail lobes. The observations and results are based on 16 years of Cluster observation of spacecraft potential measurements converted into local plasma densities. Measurements from all four Cluster spacecraft have been used, and the survey indicates a persistent asymmetry in lobe density, with consistently higher cold plasma densities in the northern lobe. External influences, such as daily and seasonal variations in the Earth's tilt angle, can introduce temporary north-south asymmetries through asymmetric ionization of the two hemispheres. Likewise, external drivers, such as the orientation of the interplanetary magnetic field can set up additional spatial asymmetries in outflow and lobe filling. The persistent asymmetry reported in this paper is also influenced by these external factors but is mainly caused by differences in magnetic field configuration in the Northern and Southern Hemisphere ionospheres.
dc.languageeng
dc.titleNorth-south asymmetries in cold plasma density in the magnetotail lobes: Cluster observations
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.source.titleJournal of Geophysical Research: Space Physics
dc.source.volume122
dc.source.issue1
dc.source.page136-149
Orfeo.peerreviewedYes
dc.identifier.doi10.1002/2016JA023404
dc.identifier.scopus2-s2.0-85010693284


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