{"@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/1361137044827267072.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1086/167211"}},{"identifier":{"@type":"NAID","@value":"30017582936"}}],"dc:title":[{"@value":"Effects of toroidal forces in current loops embedded in a background plasma"}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1381137044827267072","@type":"Researcher","foaf:name":[{"@value":"James Chen"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"0004637X"},{"@type":"EISSN","@value":"15384357"}],"prism:publicationName":[{"@value":"The Astrophysical Journal"}],"dc:publisher":[{"@value":"American Astronomical Society"}],"prism:publicationDate":"1989-03","prism:volume":"338","prism:startingPage":"453"},"reviewed":"false","createdAt":"2002-07-26","modifiedAt":"2020-11-06","relatedProduct":[{"@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/1360004234382031104","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"A STUDY OF THE HELIOCENTRIC DEPENDENCE OF SHOCK STANDOFF DISTANCE AND GEOMETRY USING 2.5D MAGNETOHYDRODYNAMIC SIMULATIONS OF CORONAL MASS EJECTION DRIVEN SHOCKS"}]},{"@id":"https://cir.nii.ac.jp/crid/1360025430205829632","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"A fast-filament eruption observed in the H<i>α</i> spectral line"}]},{"@id":"https://cir.nii.ac.jp/crid/1390001206512735616","@type":"Article","relationType":["isReferencedBy","isCitedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Spheromaks, solar prominences, and Alfvén instability of current sheets"},{"@value":"Spheromaks, solar prominences, and Alfven instability of current sheets"}]},{"@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":"10.1086/167211"},{"@type":"CIA","@value":"30017582936"},{"@type":"CROSSREF","@value":"10.1038/s41467-017-02616-8_references_DOI_NijmkKLZgTtcolHHU9LAQZ7yOd1"},{"@type":"CROSSREF","@value":"10.1186/bf03353261_references_DOI_NijmkKLZgTtcolHHU9LAQZ7yOd1"},{"@type":"CROSSREF","@value":"10.1088/0004-637x/759/2/103_references_DOI_NijmkKLZgTtcolHHU9LAQZ7yOd1"},{"@type":"CROSSREF","@value":"10.1051/0004-6361/202450099_references_DOI_NijmkKLZgTtcolHHU9LAQZ7yOd1"},{"@type":"CROSSREF","@value":"10.1186/s40645-016-0084-7_references_DOI_NijmkKLZgTtcolHHU9LAQZ7yOd1"}]}