{"@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/1362825893900313472.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1029/2019ja027694"}},{"identifier":{"@type":"URI","@value":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1029%2F2019JA027694"}},{"identifier":{"@type":"URI","@value":"https://onlinelibrary.wiley.com/doi/pdf/10.1029/2019JA027694"}},{"identifier":{"@type":"URI","@value":"https://onlinelibrary.wiley.com/doi/full-xml/10.1029/2019JA027694"}},{"identifier":{"@type":"URI","@value":"https://agupubs.onlinelibrary.wiley.com/doi/am-pdf/10.1029/2019JA027694"}},{"identifier":{"@type":"URI","@value":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/2019JA027694"}}],"dc:title":[{"@value":"Latitude Dependence of Interhemispheric Field‐Aligned Currents (IHFACs) as Observed by the Swarm Constellation"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:title>Key Points</jats:title><jats:p>\n<jats:list list-type=\"bullet\">\n<jats:list-item><jats:p>Two clearly different systems of IHFACs exist at low and middle latitudes, respectively, with a boundary near ±35° in magnetic latitudes</jats:p></jats:list-item>\n<jats:list-item><jats:p>The latitudinal and longitudinal structures of IHFACs depend strongly on wave forcing from the lower atmosphere, below 30 km</jats:p></jats:list-item>\n<jats:list-item><jats:p>Midlatitude IHFACs have similar climatology in equinoxes/June solstice, while those of December solstice exhibit different behavior</jats:p></jats:list-item>\n</jats:list></jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1382825893900313472","@type":"Researcher","foaf:name":[{"@value":"Jaeheung Park"}],"jpcoar:affiliationName":[{"@value":"Space Science Division Korea Astronomy and Space Science Institute  Daejeon South Korea"},{"@value":"Department of Astronomy and Space Science Korea University of Science and Technology  Daejeon South Korea"}]},{"@id":"https://cir.nii.ac.jp/crid/1382825893900313473","@type":"Researcher","foaf:name":[{"@value":"Yosuke Yamazaki"}],"jpcoar:affiliationName":[{"@value":"GFZ‐German Research Centre for Geosciences, Sect. 2.3, Geomagnetism  Potsdam Germany"}]},{"@id":"https://cir.nii.ac.jp/crid/1382825893900313474","@type":"Researcher","foaf:name":[{"@value":"Hermann Lühr"}],"jpcoar:affiliationName":[{"@value":"GFZ‐German Research Centre for Geosciences, Sect. 2.3, Geomagnetism  Potsdam Germany"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"21699380"},{"@type":"EISSN","@value":"21699402"}],"prism:publicationName":[{"@value":"Journal of Geophysical Research: Space Physics"}],"dc:publisher":[{"@value":"American Geophysical Union (AGU)"}],"prism:publicationDate":"2020-02","prism:volume":"125","prism:number":"2"},"reviewed":"false","dc:rights":["http://onlinelibrary.wiley.com/termsAndConditions#am","http://onlinelibrary.wiley.com/termsAndConditions#vor"],"url":[{"@id":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1029%2F2019JA027694"},{"@id":"https://onlinelibrary.wiley.com/doi/pdf/10.1029/2019JA027694"},{"@id":"https://onlinelibrary.wiley.com/doi/full-xml/10.1029/2019JA027694"},{"@id":"https://agupubs.onlinelibrary.wiley.com/doi/am-pdf/10.1029/2019JA027694"},{"@id":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/2019JA027694"}],"createdAt":"2020-02-03","modifiedAt":"2023-09-02","relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1050295027686608000","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Seasonal variation of inter-hemispheric field-aligned currents deduced from time-series analysis of the equatorial 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