{"@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/1363388843365296000.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1016/0032-0633(76)90076-3"}},{"identifier":{"@type":"URI","@value":"https://api.elsevier.com/content/article/PII:0032063376900763?httpAccept=text/xml"}},{"identifier":{"@type":"URI","@value":"https://api.elsevier.com/content/article/PII:0032063376900763?httpAccept=text/plain"}},{"identifier":{"@type":"NAID","@value":"80013561962"}}],"dc:title":[{"@value":"Simultaneous observations of relativistic electron bursts and neutral-line signatures in the magnetotail"}],"description":[{"notation":[{"@value":"Abstract   The relationship between the relativistic electron bursts (0.3 ∼ 1.0 MeV) observed in the magnetotail at  X  = −20 ∼ −30  R   e   and the evolution of the structure of the magnetotail during substorms is investigated. It is found that the majority of the relativistic electron bursts are associated with the substorm activity and occurs inside the plasma sheet at the time of the local  BZ -southward turning. It is suggested that these electrons are accelerated at the neutral line and trapped in the magnetic loop structure."}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1583668926254644864","@type":"Researcher","foaf:name":[{"@value":"T. Terasawa"}]},{"@id":"https://cir.nii.ac.jp/crid/1383388843365296000","@type":"Researcher","foaf:name":[{"@value":"A. Nishida"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"00320633"}],"prism:publicationName":[{"@value":"Planetary and Space Science"}],"dc:publisher":[{"@value":"Elsevier BV"}],"prism:publicationDate":"1976-09","prism:volume":"24","prism:number":"9","prism:startingPage":"855","prism:endingPage":"866"},"reviewed":"false","dc:rights":["https://www.elsevier.com/tdm/userlicense/1.0/"],"url":[{"@id":"https://api.elsevier.com/content/article/PII:0032063376900763?httpAccept=text/xml"},{"@id":"https://api.elsevier.com/content/article/PII:0032063376900763?httpAccept=text/plain"}],"createdAt":"2002-11-12","modifiedAt":"2019-04-02","relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1360282589004799744","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Favorable conditions for energetic electron acceleration during magnetic reconnection in the Earth's magnetotail"}]},{"@id":"https://cir.nii.ac.jp/crid/1360306905642872448","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Maximum Energy of Particles in Plasmas"}]},{"@id":"https://cir.nii.ac.jp/crid/1360565165385710592","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Particle Acceleration in the Magnetotail and Aurora"}]},{"@id":"https://cir.nii.ac.jp/crid/1360848656365857280","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Electron Power-Law Spectra in Solar and Space Plasmas"}]},{"@id":"https://cir.nii.ac.jp/crid/1390001206510960128","@type":"Article","relationType":["isReferencedBy","isCitedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"MHD wave characteristics inferred from correlations between X-rays, VLF, and ULFs at Syowa Station, Antarctica and Tjörnes, Iceland (L - 6)"},{"@value":"MHD wave characteristics inferred from correlations between X-rays, VLF, and ULFs at Syowa Station, Antarctica and Tjornes, Iceland (L～6)"},{"@value":"MHD wave characteristics inferred from correlations between X-rays, VLF, and ULFs at Syowa Station, Antarctica and Tjörnes, Iceland (L∼6)"}]},{"@id":"https://cir.nii.ac.jp/crid/1390282681490449408","@type":"Article","relationType":["isReferencedBy","isCitedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Strong electron heating and non-Maxwellian behavior in magnetic reconnection"}]},{"@id":"https://cir.nii.ac.jp/crid/2050870367122245632","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Energetic ion acceleration during magnetic reconnection in the Earth's magnetotail"}]}],"dataSourceIdentifier":[{"@type":"CROSSREF","@value":"10.1016/0032-0633(76)90076-3"},{"@type":"CIA","@value":"80013561962"},{"@type":"OPENAIRE","@value":"doi_dedup___::fd4779104bc281452c4f09581882ea75"},{"@type":"CROSSREF","@value":"10.1029/2011ja016576_references_DOI_Mp1Td5iGC7jELPnNC3SrMAFsS5J"},{"@type":"CROSSREF","@value":"10.1186/s40623-015-0372-2_references_DOI_Mp1Td5iGC7jELPnNC3SrMAFsS5J"},{"@type":"CROSSREF","@value":"10.3847/1538-4357/ad9916_references_DOI_Mp1Td5iGC7jELPnNC3SrMAFsS5J"},{"@type":"CROSSREF","@value":"10.1007/s11214-012-9874-4_references_DOI_Mp1Td5iGC7jELPnNC3SrMAFsS5J"},{"@type":"CROSSREF","@value":"10.1186/bf03353282_references_DOI_Mp1Td5iGC7jELPnNC3SrMAFsS5J"},{"@type":"CROSSREF","@value":"10.1186/bf03352207_references_DOI_Mp1Td5iGC7jELPnNC3SrMAFsS5J"},{"@type":"CROSSREF","@value":"10.1007/s11214-018-0515-4_references_DOI_Mp1Td5iGC7jELPnNC3SrMAFsS5J"}]}