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dc.contributor.authorRietveld, Michael T.
dc.contributor.authorTereshchenko, E.D.
dc.contributor.authorBrekke, Asgeir
dc.contributor.authorKhudukon, B.Z.
dc.contributor.authorKozlova, M.O.
dc.contributor.authorEvstafiev, O.V.
dc.contributor.authorNygren, T.
dc.date.accessioned2007-01-24T10:00:45Z
dc.date.available2007-01-24T10:00:45Z
dc.date.issued2000
dc.description.abstractResults are shown from an experimental campaign where satellite scintillation was observed at three sites at high latitudes and, simultaneously, the F region plasma flow was measured by the nearby EISCAT incoherent scatter radar. The anisotropy parameters of field-aligned irregularities are determined from amplitude scintillation using a method based on the variance of the relative logarithmic amplitude. The orientation of the anisotropy in a plane perpendicular to the geomagnetic field is compared with the direction of F region plasma flow. The results indicate that in most cases a good agreement between the two directions is obtained.en
dc.format.extent198715 bytes
dc.format.mimetypeapplication/pdf
dc.identifier.issn1432-0576 (elektronisk)
dc.identifier.urihttps://hdl.handle.net/10037/559
dc.identifier.urnURN:NBN:no-uit_munin_386
dc.language.isoengen
dc.publisherEuropean Geophysical Societyen
dc.relation.ispartofseriesAnnales Geophysicae 18(2000), pp 918-926en
dc.rights.accessRightsopenAccess
dc.subjectionosphereen
dc.subjectauroral ionosphereen
dc.subjectionospheric irregularitiesen
dc.subjectVDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Rom- og plasmafysikk: 437en
dc.titleComparison of the orientation of small-scale electron density irregularities and F region plasma flow direction.en
dc.typeJournal articleen
dc.typeTidsskriftartikkelno
dc.typePeer reviewed


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