{"@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/1362262946097438464.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1029/2001gl014416"}},{"identifier":{"@type":"URI","@value":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1029%2F2001GL014416"}},{"identifier":{"@type":"URI","@value":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/2001GL014416"}}],"dc:title":[{"@value":"Interchange instability in the inner magnetosphere associated with geosynchronous particle flux decreases"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:p>We simulate the inner magnetosphere during the magnetic storm of September 25, 1998 using the Rice Convection Model with boundary fluxes estimated from geosynchronous data. Model results indicate development of an interchange‐like instability in the dusk‐to‐midnight sector, producing ripple structures in the plasma density, swirls in the subauroral ionospheric electric field pattern, and undulations near the equatorward edge of the diffuse aurora. We suggest that these disturbances might be observable whenever a strong main‐phase ring‐current injection is followed by a major, sustained decrease in the plasma energy density at geosynchronous orbit, a circumstance that will also produce rapid decay of the storm‐time ring current.</jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1382262946097438341","@type":"Researcher","foaf:name":[{"@value":"S. Sazykin"}],"jpcoar:affiliationName":[{"@value":"Physics and Astronomy Department Rice University  Houston Texas USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1382262946097438338","@type":"Researcher","foaf:name":[{"@value":"R. A. Wolf"}],"jpcoar:affiliationName":[{"@value":"Physics and Astronomy Department Rice University  Houston Texas USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1382262946097438340","@type":"Researcher","foaf:name":[{"@value":"R. W. Spiro"}],"jpcoar:affiliationName":[{"@value":"Physics and Astronomy Department Rice University  Houston Texas USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1382262946097438336","@type":"Researcher","foaf:name":[{"@value":"T. I. Gombosi"}],"jpcoar:affiliationName":[{"@value":"Department of Atmospheric, Oceanic, and Space Sciences University of Michigan  Ann Arbor Michigan USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1382262946097438337","@type":"Researcher","foaf:name":[{"@value":"D. L. De Zeeuw"}],"jpcoar:affiliationName":[{"@value":"Department of Atmospheric, Oceanic, and Space Sciences University of Michigan  Ann Arbor Michigan USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1382262946097438339","@type":"Researcher","foaf:name":[{"@value":"M. F. Thomsen"}],"jpcoar:affiliationName":[{"@value":"Space and Atmospheric Sciences Los Alamos National Laboratory  Los Alamos New Mexico 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":"2002-05-15","prism:volume":"29","prism:number":"10"},"reviewed":"false","dc:rights":["http://onlinelibrary.wiley.com/termsAndConditions#vor"],"url":[{"@id":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1029%2F2001GL014416"},{"@id":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/2001GL014416"}],"createdAt":"2002-10-27","modifiedAt":"2023-10-31","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/1050282813186026624","@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: 1. magnetic storms"}]},{"@id":"https://cir.nii.ac.jp/crid/1360021389801934976","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Long Lifetime Hiss Rays in the Disturbed Plasmasphere"}]},{"@id":"https://cir.nii.ac.jp/crid/1360848658215961216","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Reimei observation of highly structured auroras caused by nonaccelerated electrons"}]}],"dataSourceIdentifier":[{"@type":"CROSSREF","@value":"10.1029/2001gl014416"},{"@type":"CROSSREF","@value":"10.1029/2023gl107825_references_DOI_7iIsHq6iQyU8olXE9HoXfO1Vbyw"},{"@type":"CROSSREF","@value":"10.1002/2015ja021831_references_DOI_7iIsHq6iQyU8olXE9HoXfO1Vbyw"},{"@type":"CROSSREF","@value":"10.1029/2009ja015009_references_DOI_7iIsHq6iQyU8olXE9HoXfO1Vbyw"},{"@type":"CROSSREF","@value":"10.1186/s40645-019-0264-3_references_DOI_7iIsHq6iQyU8olXE9HoXfO1Vbyw"}]}