{"@context":{"@vocab":"https://cir.nii.ac.jp/schema/1.0/","rdfs":"http://www.w3.org/2000/01/rdf-schema#","dc":"http://purl.org/dc/elements/1.1/","dcterms":"http://purl.org/dc/terms/","foaf":"http://xmlns.com/foaf/0.1/","prism":"http://prismstandard.org/namespaces/basic/2.0/","cinii":"http://ci.nii.ac.jp/ns/1.0/","datacite":"https://schema.datacite.org/meta/kernel-4/","ndl":"http://ndl.go.jp/dcndl/terms/","jpcoar":"https://github.com/JPCOAR/schema/blob/master/2.0/"},"@id":"https://cir.nii.ac.jp/crid/1363388844926425728.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1029/2004gl019838"}},{"identifier":{"@type":"URI","@value":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1029%2F2004GL019838"}},{"identifier":{"@type":"URI","@value":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/2004GL019838"}}],"dc:title":[{"@value":"High‐resolution observations of the small‐scale flow pattern associated with a poleward moving auroral form in the cusp"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:p>In this paper we present high‐resolution observations by the EISCAT Svalbard Radar of the localized ionospheric flow response due to one single flux transfer event and the relative location of a poleward moving auroral form. In a fast scan mode the radar was tracking a 50–60 km wide channel of westward flow in the cusp region. This flow channel was surrounded by flow running in the opposite direction. At the poleward edge of the narrow flow channel a poleward moving auroral form was situated, consistent with the auroral form being the signature of an upward Birkeland current filament. Our observations can be interpreted in terms of the <jats:ext-link xmlns:xlink=\"http://www.w3.org/1999/xlink\" xlink:href=\"#grl18257-bib-0018\"><jats:italic>Southwood</jats:italic> [1985</jats:ext-link>, <jats:ext-link xmlns:xlink=\"http://www.w3.org/1999/xlink\" xlink:href=\"#grl18257-bib-0019\">1987]</jats:ext-link> flux transfer model, and the FTE twin‐cell flow pattern appears to be a ripple onto the larger‐scale background convection.</jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1380286991027116034","@type":"Researcher","foaf:name":[{"@value":"K. Oksavik"}],"jpcoar:affiliationName":[{"@value":"Department of Physics University of Oslo  Oslo Norway"}]},{"@id":"https://cir.nii.ac.jp/crid/1383388844926425729","@type":"Researcher","foaf:name":[{"@value":"J. Moen"}],"jpcoar:affiliationName":[{"@value":"Department of Physics University of Oslo  Oslo Norway"}]},{"@id":"https://cir.nii.ac.jp/crid/1383388844926425730","@type":"Researcher","foaf:name":[{"@value":"H. C. Carlson"}],"jpcoar:affiliationName":[{"@value":"Air Force Office of Scientific Research  Arlington Virginia USA"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"00948276"},{"@type":"EISSN","@value":"19448007"}],"prism:publicationName":[{"@value":"Geophysical Research Letters"}],"dc:publisher":[{"@value":"American Geophysical Union (AGU)"}],"prism:publicationDate":"2004-06","prism:volume":"31","prism:number":"11","prism:startingPage":"L11807"},"reviewed":"false","dc:rights":["http://onlinelibrary.wiley.com/termsAndConditions#vor"],"url":[{"@id":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1029%2F2004GL019838"},{"@id":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/2004GL019838"}],"createdAt":"2004-06-09","modifiedAt":"2023-10-31","relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1050282810828710400","@type":"Article","resourceType":"学術雑誌論文(journal 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