{"@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/1360004229805921152.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1002/2016gl070706"}},{"identifier":{"@type":"URI","@value":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1002%2F2016GL070706"}},{"identifier":{"@type":"URI","@value":"https://onlinelibrary.wiley.com/doi/pdf/10.1002/2016GL070706"}},{"identifier":{"@type":"URI","@value":"https://onlinelibrary.wiley.com/doi/full-xml/10.1002/2016GL070706"}},{"identifier":{"@type":"URI","@value":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1002/2016GL070706"}}],"resourceType":"学術雑誌論文(journal article)","dc:title":[{"@value":"Properties of hot electrons in the Jovian inner magnetosphere deduced from extended observations of the Io Plasma Torus"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:title>Abstract</jats:title><jats:p>One of the focal points of interest in Jovian magnetospheric physics is the transport of energy and particles into the inner region. While an explosive energy release event in the midmagnetosphere is manifested as an aurora transient, its connection to the inner part has not been investigated due to sparsity of observations. Here we take the advantage of long‐term and quasi‐continuous simultaneous monitoring of the polar aurora and the Io Plasma Torus (IPT) located in the inner magnetosphere by Extreme Ultraviolet Spectroscope for Exospheric Dynamics/Hisaki. Studies on temporal characteristics over hours enable us to see slow (~10 h) coupling between the middle and inner magnetosphere as well as to quantify the temperature of hot electrons in the IPT. We derive parameters that characterize the strong particle acceleration process.</jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1380004229805921158","@type":"Researcher","foaf:name":[{"@value":"Ichiro Yoshikawa"}],"jpcoar:affiliationName":[{"@value":"Department of Complexity Science and Engineering University of Tokyo  Kashiwa Japan"},{"@value":"Department of Earth and Planetary Science University of Tokyo  Tokyo 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Kasaba"}],"jpcoar:affiliationName":[{"@value":"Department of Geophysics Tohoku University  Sendai Japan"}]},{"@id":"https://cir.nii.ac.jp/crid/1420564276183697408","@type":"Researcher","personIdentifier":[{"@type":"KAKEN_RESEARCHERS","@value":"30242811"},{"@type":"NRID","@value":"1000030242811"}],"foaf:name":[{"@value":"Masaki Fujimoto"}],"jpcoar:affiliationName":[{"@value":"Institute of Space and Astronautical Science Japan Aerospace Exploration Agency  Sagamihara Japan"}]}],"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":"2016-11-23","prism:volume":"43","prism:number":"22","prism:startingPage":"11552"},"reviewed":"false","dc:rights":["http://onlinelibrary.wiley.com/termsAndConditions#vor"],"url":[{"@id":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1002%2F2016GL070706"},{"@id":"https://onlinelibrary.wiley.com/doi/pdf/10.1002/2016GL070706"},{"@id":"https://onlinelibrary.wiley.com/doi/full-xml/10.1002/2016GL070706"},{"@id":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1002/2016GL070706"}],"createdAt":"2016-11-09","modifiedAt":"2023-09-06","project":[{"@id":"https://cir.nii.ac.jp/crid/1040000781862677632","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"15K17769"},{"@type":"JGN","@value":"JP15K17769"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-15K17769/"}],"notation":[{"@language":"ja","@value":"オーロラ紫外スペクトルのオーロラ加速域情報から探る木星・土星電磁圏ダイナミクス"},{"@language":"en","@value":"Jupiter and Saturn magnetospheric dynamics explored using auroral electron accelerations derived from ultraviolet auroral emissions"}]},{"@id":"https://cir.nii.ac.jp/crid/1040000782297892992","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"26400476"},{"@type":"JGN","@value":"JP26400476"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-26400476/"}],"notation":[{"@language":"ja","@value":"木星内部磁気圏におけるプラズマ輸送過程の実証的研究"},{"@language":"en","@value":"Transport of plasma mass and energy in the Jovian inner magnetosphere"}]},{"@id":"https://cir.nii.ac.jp/crid/1040282256809620480","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"15H05209"},{"@type":"JGN","@value":"JP15H05209"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-15H05209/"}],"notation":[{"@language":"ja","@value":"ハワイ・ハレアカラ小中口径鏡による太陽系惑星の可視・赤外高分散分光研究"},{"@language":"en","@value":"Investigation of solar panels system planets by visible and infrared high-dispersion spectroscopy on small/medium-sized telescopes at Haleakala, Hawaii"}]},{"@id":"https://cir.nii.ac.jp/crid/1040282257263195776","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"26287118"},{"@type":"JGN","@value":"JP26287118"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-26287118/"}],"notation":[{"@language":"ja","@value":"地上・宇宙光学望遠鏡ならびに電波望遠鏡による木星大気圏－電磁圏結合過程の解明"},{"@language":"en","@value":"Understanding of Jovian atmosphere-ionosphere-magnetosphere coupling process based on optical and radio telescopes from ground and space"}]},{"@id":"https://cir.nii.ac.jp/crid/1040282257263205248","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"26287122"},{"@type":"JGN","@value":"JP26287122"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-26287122/"}],"notation":[{"@language":"ja","@value":"太陽系の外惑星領域における磁気圏ダイナミクス"},{"@language":"en","@value":"Magnetospheric dynamics of outer planets"}]}],"relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1050001202716094592","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Response of Jupiter's Aurora to Plasma Mass Loading Rate Monitored by the Hisaki Satellite During Volcanic Eruptions at Io"}]},{"@id":"https://cir.nii.ac.jp/crid/1050282810790115968","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@language":"en","@value":"First spaceborne observation of the entire concentric airglow structure caused by tropospheric disturbance"},{"@value":"Evidence for global electron transportation into the jovian inner magnetosphere"}]},{"@id":"https://cir.nii.ac.jp/crid/1360002215432335872","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Extreme Ultraviolet Radiation Measurement for Planetary 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