{"@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/1363670320918347008.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1029/2005gl022647"}},{"identifier":{"@type":"URI","@value":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1029%2F2005GL022647"}},{"identifier":{"@type":"URI","@value":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/2005GL022647"}}],"dc:title":[{"@value":"Energetic ion acceleration in Saturn's magnetotail: Substorms at Saturn?"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:p>The Magnetospheric Imaging Instrument (MIMI) Ion and Neutral Camera (INCA) on the Cassini spacecraft has recorded abrupt increases in energetic neutral atom flux coming from the general direction of Saturn's magnetotail. These bursts of ion activity in the tail are well correlated with enhancements in the Saturn kilometric radiation. Given the similarities between these events and substorm activity on Earth, including their dependence on interplanetary conditions, we conclude that Earth‐like substorms occur within Saturn's magnetosphere.</jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1380004054097470225","@type":"Researcher","foaf:name":[{"@value":"D. G. Mitchell"}],"jpcoar:affiliationName":[{"@value":"Applied Physics Laboratory Johns Hopkins University  Laurel Maryland USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1380861294532352387","@type":"Researcher","foaf:name":[{"@value":"P. C. Brandt"}],"jpcoar:affiliationName":[{"@value":"Applied Physics Laboratory Johns Hopkins University  Laurel Maryland USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1380861294532352384","@type":"Researcher","foaf:name":[{"@value":"E. C. Roelof"}],"jpcoar:affiliationName":[{"@value":"Applied Physics Laboratory Johns Hopkins University  Laurel Maryland USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1380861294532352395","@type":"Researcher","foaf:name":[{"@value":"J. Dandouras"}],"jpcoar:affiliationName":[{"@value":"Centre D'Etude Spatiale Des Rayonnements  Toulouse France"}]},{"@id":"https://cir.nii.ac.jp/crid/1380861294532352386","@type":"Researcher","foaf:name":[{"@value":"S. M. Krimigis"}],"jpcoar:affiliationName":[{"@value":"Applied Physics Laboratory Johns Hopkins University  Laurel Maryland USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1380861294532352385","@type":"Researcher","foaf:name":[{"@value":"B. H. Mauk"}],"jpcoar:affiliationName":[{"@value":"Applied Physics Laboratory Johns Hopkins University  Laurel Maryland USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1380861294532352391","@type":"Researcher","foaf:name":[{"@value":"C. P. Paranicas"}],"jpcoar:affiliationName":[{"@value":"Applied Physics Laboratory Johns Hopkins University  Laurel Maryland USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1380861294532352388","@type":"Researcher","foaf:name":[{"@value":"N. Krupp"}],"jpcoar:affiliationName":[{"@value":"Max‐Planck‐Institut für Sonnensystemforschung  Lindau Germany"}]},{"@id":"https://cir.nii.ac.jp/crid/1380861294532352392","@type":"Researcher","foaf:name":[{"@value":"D. C. Hamilton"}],"jpcoar:affiliationName":[{"@value":"University of Maryland  College Park Maryland USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1380861294532352389","@type":"Researcher","foaf:name":[{"@value":"W. S. Kurth"}],"jpcoar:affiliationName":[{"@value":"Department of Physics and Astronomy University of Iowa  Iowa City Iowa USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1380861294532352393","@type":"Researcher","foaf:name":[{"@value":"P. Zarka"}],"jpcoar:affiliationName":[{"@value":"Observatory of Paris  Meudon France"}]},{"@id":"https://cir.nii.ac.jp/crid/1380861294532352396","@type":"Researcher","foaf:name":[{"@value":"M. K. Dougherty"}],"jpcoar:affiliationName":[{"@value":"Space and Atmospheric Physics Imperial College  London U.K"}]},{"@id":"https://cir.nii.ac.jp/crid/1380861294532352394","@type":"Researcher","foaf:name":[{"@value":"E. J. Bunce"}],"jpcoar:affiliationName":[{"@value":"Department of Physics & Astronomy University of Leicester  Leicester U.K"}]},{"@id":"https://cir.nii.ac.jp/crid/1380861294532352390","@type":"Researcher","foaf:name":[{"@value":"D. E. Shemansky"}],"jpcoar:affiliationName":[{"@value":"Department of Aerospace Engineering University of Southern California Los Angeles  California 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":"2005-06-25","prism:volume":"32","prism:number":"20","prism:startingPage":"L12S03"},"reviewed":"false","dc:rights":["http://onlinelibrary.wiley.com/termsAndConditions#vor"],"url":[{"@id":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1029%2F2005GL022647"},{"@id":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/2005GL022647"}],"createdAt":"2005-06-24","modifiedAt":"2023-10-31","relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1360002215432335872","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Extreme Ultraviolet Radiation Measurement for Planetary Atmospheres/Magnetospheres from the Earth-Orbiting Spacecraft (Extreme Ultraviolet Spectroscope for Exospheric Dynamics: EXCEED)"}]},{"@id":"https://cir.nii.ac.jp/crid/1360306904383751040","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Magnetosphere and Plasma Science with the Jupiter Icy Moons Explorer"}]},{"@id":"https://cir.nii.ac.jp/crid/2050307417166183168","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"The science case for the EISCAT_3D radar"}]}],"dataSourceIdentifier":[{"@type":"CROSSREF","@value":"10.1029/2005gl022647"},{"@type":"CROSSREF","@value":"10.1007/s11214-014-0077-z_references_DOI_5722g6nBq5hTIFxlxqikHkahdg8"},{"@type":"CROSSREF","@value":"10.1186/s40645-015-0051-8_references_DOI_5722g6nBq5hTIFxlxqikHkahdg8"},{"@type":"CROSSREF","@value":"10.1007/s11214-025-01148-8_references_DOI_5722g6nBq5hTIFxlxqikHkahdg8"}]}