{"@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/1363670319282807424.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1029/97ja03995"}},{"identifier":{"@type":"URI","@value":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1029%2F97JA03995"}},{"identifier":{"@type":"URI","@value":"https://onlinelibrary.wiley.com/doi/pdf/10.1029/97JA03995"}},{"identifier":{"@type":"URI","@value":"https://onlinelibrary.wiley.com/doi/full-xml/10.1029/97JA03995"}},{"identifier":{"@type":"URI","@value":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/97JA03995"}},{"identifier":{"@type":"NAID","@value":"30013334960"}}],"dc:title":[{"@value":"Simulations of radiation belt formation during storm sudden commencements"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:p>MHD fields from a global three‐dimensional simulation of the great March 24, 1991, storm sudden commencement (SSC) are used to follow the trajectories of particles in a guiding center test particle simulation of radiation belt formation during this event. Modeling of less intense events during the lifetime of the CRRES satellite, with similar morphology but less radial transport and energization, is also presented. In all cases analyzed, a solar proton event was followed by an SSC, leading to the formation of a new proton belt earthward of solar proton penetration. The effect on particle energization of varying solar wind and model pulse parameters is investigated. Both a seed population of solar protons and the SSC shock‐induced compression of the magnetosphere are necessary conditions for the formation of a new proton belt. The outer boundary of the inner zone protons can be affected by an SSC and a newly formed belt can be affected by the ensuing or a subsequent storm, which may occur in rapid succession, as was the case in June and July 1991. The acceleration process is effective for both northward and southward IMF, with more energization and inward radial transport for the southward case for otherwise comparable solar wind parameters, because of the initially more compressed magnetopause in the southward case. The inner boundary and stability of the newly formed belt depends on the magnitude of radial transport at the time of formation and subsequent ring current perturbation of adiabatic trapping.</jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1580572701433187200","@type":"Researcher","foaf:name":[{"@value":"M. K. Hudson"}]},{"@id":"https://cir.nii.ac.jp/crid/1383670319282807432","@type":"Researcher","foaf:name":[{"@value":"S. R. Elkington"}]},{"@id":"https://cir.nii.ac.jp/crid/1383670319282807424","@type":"Researcher","foaf:name":[{"@value":"J. G. Lyon"}]},{"@id":"https://cir.nii.ac.jp/crid/1383670319282807430","@type":"Researcher","foaf:name":[{"@value":"V. A. Marchenko"}]},{"@id":"https://cir.nii.ac.jp/crid/1383670319282807425","@type":"Researcher","foaf:name":[{"@value":"I. Roth"}]},{"@id":"https://cir.nii.ac.jp/crid/1383670319282807426","@type":"Researcher","foaf:name":[{"@value":"M. Temerin"}]},{"@id":"https://cir.nii.ac.jp/crid/1383670319282807431","@type":"Researcher","foaf:name":[{"@value":"J. B. Blake"}]},{"@id":"https://cir.nii.ac.jp/crid/1383670319282807427","@type":"Researcher","foaf:name":[{"@value":"M. S. Gussenhoven"}]},{"@id":"https://cir.nii.ac.jp/crid/1383670319282807428","@type":"Researcher","foaf:name":[{"@value":"J. R. Wygant"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"01480227"}],"prism:publicationName":[{"@value":"Journal of Geophysical Research: Space Physics"}],"dc:publisher":[{"@value":"American Geophysical Union (AGU)"}],"prism:publicationDate":"1997-01","prism:volume":"102","prism:number":"A7","prism:startingPage":"14087","prism:endingPage":"14102"},"reviewed":"false","dc:rights":["http://onlinelibrary.wiley.com/termsAndConditions#vor"],"url":[{"@id":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1029%2F97JA03995"},{"@id":"https://onlinelibrary.wiley.com/doi/pdf/10.1029/97JA03995"},{"@id":"https://onlinelibrary.wiley.com/doi/full-xml/10.1029/97JA03995"},{"@id":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/97JA03995"}],"createdAt":"2004-02-03","modifiedAt":"2024-01-24","relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1360004229806287488","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Formation of multiple energy dispersion of H<sup>+</sup>, He<sup>+</sup>, and O<sup>+</sup> ions in the inner magnetosphere in response to interplanetary shock"}]},{"@id":"https://cir.nii.ac.jp/crid/1360576118775716736","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Seasonal variation and geomagnetic storm index effects on the proton flux response in the South Atlantic Anomaly by test particle simulations"}]},{"@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/1360584341823587968","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Geomagnetic Storm Effects on the LEO Proton Flux During Solar Energetic Particle Events"}]},{"@id":"https://cir.nii.ac.jp/crid/1390845713060727552","@type":"Article","relationType":["isCitedBy"],"jpcoar:relatedTitle":[{"@language":"ja","@value":"放射線帯粒子環境"},{"@value":"宇宙機と宇宙プラズマ環境(1)放射線帯粒子環境"},{"@language":"ja-Kana","@value":"ウチュウキ ト ウチュウ プラズマ カンキョウ 1 ホウシャセンタイ リュウシ カンキョウ"}]},{"@id":"https://cir.nii.ac.jp/crid/2051433317035013760","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Dynamics of the terrestrial radiation belts : a review of recent results during the VarSITI (Variability of the Sun and Its Terrestrial Impact) era, 2014–2018"}]}],"dataSourceIdentifier":[{"@type":"CROSSREF","@value":"10.1029/97ja03995"},{"@type":"CIA","@value":"30013334960"},{"@type":"CROSSREF","@value":"10.1002/2016ja023704_references_DOI_APYqpsZbvsRXI2cOjdD4sqkOjO0"},{"@type":"CROSSREF","@value":"10.1186/s40645-021-00413-y_references_DOI_APYqpsZbvsRXI2cOjdD4sqkOjO0"},{"@type":"CROSSREF","@value":"10.1016/j.jastp.2021.105808_references_DOI_APYqpsZbvsRXI2cOjdD4sqkOjO0"},{"@type":"CROSSREF","@value":"10.1109/tps.2022.3208906_references_DOI_APYqpsZbvsRXI2cOjdD4sqkOjO0"},{"@type":"CROSSREF","@value":"10.1029/2023sw003664_references_DOI_S78aQfmYn2tB1C2DoFYeLmmDn6F"}]}