{"@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/1050845760765770752.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"HDL","@value":"http://hdl.handle.net/2433/215839"}},{"identifier":{"@type":"NDL_BIB_ID","@value":"10193165"}},{"identifier":{"@type":"DOI","@value":"10.1186/s40623-016-0444-y"}},{"identifier":{"@type":"URI","@value":"http://id.ndl.go.jp/digimeta/10193165"}},{"identifier":{"@type":"URI","@value":"https://dl.ndl.go.jp/pid/10193165"}},{"identifier":{"@type":"URI","@value":"http://link.springer.com/content/pdf/10.1186/s40623-016-0444-y.pdf"}},{"identifier":{"@type":"URI","@value":"http://link.springer.com/article/10.1186/s40623-016-0444-y/fulltext.html"}},{"identifier":{"@type":"URI","@value":"http://link.springer.com/content/pdf/10.1186/s40623-016-0444-y"}},{"identifier":{"@type":"HANDLE","@value":"2433/215839"}},{"identifier":{"@type":"NAID","@value":"120005774660"}}],"resourceType":"学術雑誌論文(journal article)","dc:title":[{"@language":"en","@value":"Relationship between solar wind dynamic pressure and amplitude of geomagnetic sudden commencement (SC)"}],"dc:language":"en","description":[{"type":"Abstract","notation":[{"@language":"en","@value":"The local time variation of geomagnetic sudden commencements (SCs) has not been taken into account in the Siscoe's linear relationship which connects the SC amplitude with the corresponding dynamic pressure variation of the solar wind. By considering the physical background of SC, we studied which local time is best to extract the information of the solar wind dynamic pressure and concluded that the SC amplitude at 4-5 h local time of middle- and low-latitude stations most directly reflects the dynamic pressure effect. This result is used to re-check the order of magnitude of the largest 3 SCs observed since 1868."}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1420282801209009664","@type":"Researcher","personIdentifier":[{"@type":"KAKEN_RESEARCHERS","@value":"50025433"},{"@type":"NRID","@value":"1000050025433"},{"@type":"NRID","@value":"9000253255991"},{"@type":"NRID","@value":"9000253257821"},{"@type":"NRID","@value":"9000253258739"},{"@type":"NRID","@value":"9000000073420"},{"@type":"NRID","@value":"9000239868165"},{"@type":"NRID","@value":"9000254262375"},{"@type":"NRID","@value":"9000338691012"},{"@type":"NRID","@value":"9000327104774"},{"@type":"NRID","@value":"9000253253752"},{"@type":"NRID","@value":"9000239868187"},{"@type":"NRID","@value":"9000239868268"},{"@type":"NRID","@value":"9000253256037"},{"@type":"NRID","@value":"9000338691171"},{"@type":"NRID","@value":"9000253256020"},{"@type":"RESEARCHMAP","@value":"https://researchmap.jp/tohru.araki"}],"foaf:name":[{"@language":"en","@value":"Araki, Tohru"}]},{"@id":"https://cir.nii.ac.jp/crid/1070845760765770753","@type":"Researcher","personIdentifier":[{"@type":"NRID","@value":"9000327104774"}],"foaf:name":[{"@language":"en","@value":"Shinbori, Atsuki"},{"@language":"ja","@value":"新堀, 淳樹"}]}],"contributor":[{"@id":"https://cir.nii.ac.jp/crid/1893962440621305984","@type":"Researcher","foaf:name":[{"@value":"新堀, 淳樹"}]}],"publication":{"publicationIdentifier":[{"@type":"EISSN","@value":"18805981"},{"@type":"ISSN","@value":"18805981"},{"@type":"LISSN","@value":"13438832"}],"prism:publicationName":[{"@language":"en","@value":"Earth, Planets and Space"}],"dc:publisher":[{"@value":"SpringerOpen"}],"prism:publicationDate":"2016-05-28","prism:volume":"68"},"reviewed":"false","dcterms:accessRights":"http://purl.org/coar/access_right/c_abf2","dc:rights":["© 2016 Araki and Shinbori. This article is distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution, and reproduction in any medium, provided you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made."],"url":[{"@id":"http://id.ndl.go.jp/digimeta/10193165"},{"@id":"https://dl.ndl.go.jp/pid/10193165"},{"@id":"http://link.springer.com/content/pdf/10.1186/s40623-016-0444-y.pdf"},{"@id":"http://link.springer.com/article/10.1186/s40623-016-0444-y/fulltext.html"},{"@id":"http://link.springer.com/content/pdf/10.1186/s40623-016-0444-y"},{"@id":"http://hdl.handle.net/2433/215839"}],"foaf:topic":[{"@id":"https://cir.nii.ac.jp/all?q=Geomagnetic%20sudden%20commencement","dc:title":"Geomagnetic sudden commencement"},{"@id":"https://cir.nii.ac.jp/all?q=Solar%20wind%20dynamic%20pressure","dc:title":"Solar wind dynamic pressure"},{"@id":"https://cir.nii.ac.jp/all?q=Local%20time%20variation","dc:title":"Local time variation"},{"@id":"https://cir.nii.ac.jp/all?q=Siscoe's%20relationship","dc:title":"Siscoe's relationship"},{"@id":"https://cir.nii.ac.jp/all?q=Largest%20sudden%20commencement","dc:title":"Largest sudden commencement"}],"dcterms:subject":[{"subjectScheme":"Other","notation":[{"@language":"en","@value":"Geomagnetic sudden commencement"}]},{"subjectScheme":"Other","notation":[{"@language":"en","@value":"Solar wind dynamic pressure"}]},{"subjectScheme":"Other","notation":[{"@language":"en","@value":"Local time variation"}]},{"subjectScheme":"Other","notation":[{"@language":"en","@value":"Siscoe's relationship"}]},{"subjectScheme":"Other","notation":[{"@language":"en","@value":"Largest sudden commencement"}]}],"project":[{"@id":"https://cir.nii.ac.jp/crid/1040000782297899520","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"26400478"},{"@type":"JGN","@value":"JP26400478"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-26400478/"}],"notation":[{"@language":"ja","@value":"地磁気擾乱時における電離圏電場分布の変動と電離圏擾乱ダイナモとの関係"},{"@language":"en","@value":"Temporal and spatial variations of ionospheric electric fields during geomagnetic storms and the relation to ionospheric disturbance dynamo"}]}],"relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1360011143589078016","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Night-time sudden commencements observed by CHAMP and ground-based magnetometers and their relationship to solar wind parameters"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011144003619200","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The solar diurnal variation in the amplitude of sudden commencements of magnetic storms at the geomagnetic equator"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011144346243072","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A numerical simulation of the geomagnetic sudden commencement: 2. 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