{"@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/1362825895246710912.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1029/98gl00662"}},{"identifier":{"@type":"URI","@value":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1029%2F98GL00662"}},{"identifier":{"@type":"URI","@value":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/98GL00662"}}],"dc:title":[{"@value":"Simulation of the March 9, 1995, substorm: Auroral brightening and the onset of lobe reconnection"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:p>A global MHD simulation of an isolated substorm that occurred on March 9, 1995 is presented. The simulation, driven with solar wind data provided by the Wind satellite, reproduced to a surprising degree the evolution of substorm activity. The onset of the expansion phase was coincident with the penetration of an electric field spike into the near‐Earth region. This impulse launched a tailward propagating signal (rarefaction wave) that enhanced reconnection in the mid tail. Substorm intensification was correlated with the enhancement of the reconnection rate at the preexisting reconnection region located at 30 <jats:italic>R<jats:sub>E</jats:sub></jats:italic>. The importance of the electric field spike in correlating ionospheric and magnetospheric aspects of the substorm is emphasized.</jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1380021390577578119","@type":"Researcher","foaf:name":[{"@value":"J. G. Lyon"}]},{"@id":"https://cir.nii.ac.jp/crid/1382825895246710914","@type":"Researcher","foaf:name":[{"@value":"R. E. Lopez"}]},{"@id":"https://cir.nii.ac.jp/crid/1382825895246710915","@type":"Researcher","foaf:name":[{"@value":"C. C. Goodrich"}]},{"@id":"https://cir.nii.ac.jp/crid/1382825895246710913","@type":"Researcher","foaf:name":[{"@value":"M. Wiltberger"}]},{"@id":"https://cir.nii.ac.jp/crid/1382825895246710916","@type":"Researcher","foaf:name":[{"@value":"K. Papadopoulos"}]}],"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":"1998-08","prism:volume":"25","prism:number":"15","prism:startingPage":"3039","prism:endingPage":"3042"},"reviewed":"false","dc:rights":["http://onlinelibrary.wiley.com/termsAndConditions#vor"],"url":[{"@id":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1029%2F98GL00662"},{"@id":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/98GL00662"}],"createdAt":"2004-02-04","modifiedAt":"2023-11-22","relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1050001338210505600","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Substorm simulation: Quiet and N-S arcs preceding auroral breakup"},{"@value":"Substorm simulation: Quiet and N‐S arcs preceding auroral breakup"}]},{"@id":"https://cir.nii.ac.jp/crid/1050564288163925760","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Simulation study of near-Earth space disturbances: 2. Auroral substorms"}]},{"@id":"https://cir.nii.ac.jp/crid/1050572512051726464","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Evolution of auroral substorm as viewed from MHD simulations: dynamics, energy transfer and energy conversion"}]},{"@id":"https://cir.nii.ac.jp/crid/1050865265017810816","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Generation mechanism of Region 1 field-aligned current and energy transfer from solar wind to polar ionosphere"}]}],"dataSourceIdentifier":[{"@type":"CROSSREF","@value":"10.1029/98gl00662"},{"@type":"CROSSREF","@value":"10.1007/s41614-024-00154-7_references_DOI_3zbh5jQXEbs1fOWk9lVRt8Sp5Vy"},{"@type":"CROSSREF","@value":"10.1002/2015ja021831_references_DOI_3zbh5jQXEbs1fOWk9lVRt8Sp5Vy"},{"@type":"CROSSREF","@value":"10.1186/s40645-019-0273-2_references_DOI_3zbh5jQXEbs1fOWk9lVRt8Sp5Vy"},{"@type":"CROSSREF","@value":"10.1007/s41614-019-0037-x_references_DOI_3zbh5jQXEbs1fOWk9lVRt8Sp5Vy"}]}