{"@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/1361699994178128256.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1029/2000ja000005"}},{"identifier":{"@type":"URI","@value":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1029%2F2000JA000005"}},{"identifier":{"@type":"URI","@value":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/2000JA000005"}}],"dc:title":[{"@value":"A review on the genesis of coronal mass ejections"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:p>This paper provides a short review of some of the basic concepts related to the origin of coronal mass ejections (CMEs). The various ideas which have been put forward to explain the initiation of CMEs are categorized in terms of whether they are force‐free or non‐force‐free and ideal or nonideal. A few representative models of each category are examined to illustrate the principles involved. At the present time there is no model which is sufficiently developed to aid forecasters in their efforts to predict CMEs, but given the current pace of research, this situation could improve dramatically in the near future.</jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1380004057902981377","@type":"Researcher","foaf:name":[{"@value":"T. G. Forbes"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"01480227"}],"prism:publicationName":[{"@value":"Journal of Geophysical Research: Space Physics"}],"dc:publisher":[{"@value":"American Geophysical Union (AGU)"}],"prism:publicationDate":"2000-10","prism:volume":"105","prism:number":"A10","prism:startingPage":"23153","prism:endingPage":"23165"},"reviewed":"false","dc:rights":["http://onlinelibrary.wiley.com/termsAndConditions#vor"],"url":[{"@id":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1029%2F2000JA000005"},{"@id":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/2000JA000005"}],"createdAt":"2004-02-03","modifiedAt":"2023-09-23","relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1050290384124567424","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Eruptivity in Solar Flares: The Challenges of Magnetic Flux Ropes"}]},{"@id":"https://cir.nii.ac.jp/crid/1360002216823143168","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Formation and dynamics of a solar eruptive flux tube"}]},{"@id":"https://cir.nii.ac.jp/crid/1360002217424462976","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"MAGNETIC FIELD STRUCTURES TRIGGERING SOLAR FLARES AND CORONAL MASS EJECTIONS"}]},{"@id":"https://cir.nii.ac.jp/crid/1360002220785152896","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Plasma Evolution within an Erupting Coronal Cavity"}]},{"@id":"https://cir.nii.ac.jp/crid/1360025430644951936","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Magnetic Reconnection in Solar Flares and the Near-Sun Solar Wind"}]},{"@id":"https://cir.nii.ac.jp/crid/1360285714652453760","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Formation of an Active Region Filament Driven By a Series of Jets"}]},{"@id":"https://cir.nii.ac.jp/crid/1360285714652730496","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Magnetohydrodynamic Modeling of a Solar Eruption Associated with an X9.3 Flare Observed in the Active Region 12673"}]},{"@id":"https://cir.nii.ac.jp/crid/1360298345008304256","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Extreme solar events"}]},{"@id":"https://cir.nii.ac.jp/crid/1360584340522017280","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Space Plasma Physics: A Review"}]},{"@id":"https://cir.nii.ac.jp/crid/1360861707130157440","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Nonequilibrium Flux Rope Formation by Confined Flares Preceding a Solar Coronal Mass Ejection"}]},{"@id":"https://cir.nii.ac.jp/crid/1364227869147384192","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Localized Microwave and EUV Bright Structures in an Eruptive Prominence"}]},{"@id":"https://cir.nii.ac.jp/crid/2050307416982588672","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Magnetohydrodynamics modeling of coronal magnetic field and solar eruptions based on the photospheric magnetic field"}]}],"dataSourceIdentifier":[{"@type":"CROSSREF","@value":"10.1029/2000ja000005"},{"@type":"CROSSREF","@value":"10.1038/s41467-017-02616-8_references_DOI_OxzMtli18qNyNFwC3Cgrn7fIe3R"},{"@type":"CROSSREF","@value":"10.1088/0004-637x/760/1/31_references_DOI_OxzMtli18qNyNFwC3Cgrn7fIe3R"},{"@type":"CROSSREF","@value":"10.3847/1538-4357/aaad68_references_DOI_OxzMtli18qNyNFwC3Cgrn7fIe3R"},{"@type":"CROSSREF","@value":"10.1007/s11214-025-01153-x_references_DOI_OxzMtli18qNyNFwC3Cgrn7fIe3R"},{"@type":"CROSSREF","@value":"10.1186/s40645-016-0084-7_references_DOI_OxzMtli18qNyNFwC3Cgrn7fIe3R"},{"@type":"CROSSREF","@value":"10.3847/1538-4357/aad187_references_DOI_OxzMtli18qNyNFwC3Cgrn7fIe3R"},{"@type":"CROSSREF","@value":"10.3847/1538-4357/aae079_references_DOI_OxzMtli18qNyNFwC3Cgrn7fIe3R"},{"@type":"CROSSREF","@value":"10.1007/s41116-022-00033-8_references_DOI_OxzMtli18qNyNFwC3Cgrn7fIe3R"},{"@type":"CROSSREF","@value":"10.1109/tps.2022.3208906_references_DOI_OxzMtli18qNyNFwC3Cgrn7fIe3R"},{"@type":"CROSSREF","@value":"10.3847/1538-4357/abf3c1_references_DOI_OxzMtli18qNyNFwC3Cgrn7fIe3R"},{"@type":"CROSSREF","@value":"10.3847/1538-4357/abda37_references_DOI_OxzMtli18qNyNFwC3Cgrn7fIe3R"},{"@type":"CROSSREF","@value":"10.3847/1538-4357/ab0e80_references_DOI_OxzMtli18qNyNFwC3Cgrn7fIe3R"}]}