{"@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/1362825895467289088.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1016/s0273-1177(99)01087-x"}},{"identifier":{"@type":"URI","@value":"https://api.elsevier.com/content/article/PII:S027311779901087X?httpAccept=text/xml"}},{"identifier":{"@type":"URI","@value":"https://api.elsevier.com/content/article/PII:S027311779901087X?httpAccept=text/plain"}}],"dc:title":[{"@value":"Comparative study of flares and substorms"}],"description":[{"notation":[{"@value":"Abstract   Comparative studies of solar flares and substorms are useful in obtaining comprehensive understanding of magnetic reconnection processes, since flare studies give us better information on macroscopic processes such as global changes of magnetic field configuration while substorm studies give us more detailed knowledge on microscopic processes. Recent spacecraft observations both for magnetospheric substorms and solar flares have dramatically enriched our understanding for physical processes occurring during these interesting phenomena. We first summarize keys of these new observations from the magnetotail studies, and try to compare them with those from the solar flare studies on a common physical basis."}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1380004230555398277","@type":"Researcher","foaf:name":[{"@value":"T. Terasawa"}]},{"@id":"https://cir.nii.ac.jp/crid/1382825895467289088","@type":"Researcher","foaf:name":[{"@value":"K. Shibata"}]},{"@id":"https://cir.nii.ac.jp/crid/1382825895467288960","@type":"Researcher","foaf:name":[{"@value":"M. Scholer"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"02731177"}],"prism:publicationName":[{"@value":"Advances in Space Research"}],"dc:publisher":[{"@value":"Elsevier BV"}],"prism:publicationDate":"2000","prism:volume":"26","prism:number":"3","prism:startingPage":"573","prism:endingPage":"583"},"reviewed":"false","dc:rights":["https://www.elsevier.com/tdm/userlicense/1.0/","https://www.elsevier.com/legal/tdmrep-license"],"url":[{"@id":"https://api.elsevier.com/content/article/PII:S027311779901087X?httpAccept=text/xml"},{"@id":"https://api.elsevier.com/content/article/PII:S027311779901087X?httpAccept=text/plain"}],"createdAt":"2002-07-25","modifiedAt":"2025-10-03","relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1360004230555398528","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Fractal Reconnection in Solar and Stellar Environments"}]},{"@id":"https://cir.nii.ac.jp/crid/1360004230881420032","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Thermal Non-equilibrium Plasma Observed by Hinode"}]},{"@id":"https://cir.nii.ac.jp/crid/1360005520008962688","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Disturbance of the Front Region of Magnetic Reconnection Outflow Jets due to the Lower-Hybrid Drift Instability"}]},{"@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/1360857593757132800","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Comparative Study of Electric Currents and Energetic Particle Fluxes in a Solar Flare and Earth Magnetospheric Substorm"}]},{"@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/s0273-1177(99)01087-x"},{"@type":"OPENAIRE","@value":"doi_dedup___::25e41dc16d6166d828c667b11819405e"},{"@type":"CROSSREF","@value":"10.1007/978-3-319-26432-5_10_references_DOI_ABEmHnRPfR4HaQWtldUrKJTgr7K"},{"@type":"CROSSREF","@value":"10.1007/978-981-10-7742-5_20_references_DOI_ABEmHnRPfR4HaQWtldUrKJTgr7K"},{"@type":"CROSSREF","@value":"10.1103/physrevlett.123.235101_references_DOI_ABEmHnRPfR4HaQWtldUrKJTgr7K"},{"@type":"CROSSREF","@value":"10.1186/s40623-015-0372-2_references_DOI_ABEmHnRPfR4HaQWtldUrKJTgr7K"},{"@type":"CROSSREF","@value":"10.1007/s11214-018-0515-4_references_DOI_ABEmHnRPfR4HaQWtldUrKJTgr7K"},{"@type":"CROSSREF","@value":"10.3847/1538-4357/ac2dfc_references_DOI_ABEmHnRPfR4HaQWtldUrKJTgr7K"}]}