{"@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/1361137044885115264.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1029/94gl00375"}},{"identifier":{"@type":"URI","@value":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1029%2F94GL00375"}},{"identifier":{"@type":"URI","@value":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/94GL00375"}}],"dc:title":[{"@value":"Large amplitude electric and magnetic field signatures in the inner magnetosphere during injection of 15 MeV electron drift echoes"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:p>Electric and magnetic fields were measured by the CRRES spacecraft at an L‐value of 2.2 to 2.6 near 0300 magnetic local time during a strong storm sudden commencement (SSC) on March 24, 1991. The electric field signature at the spacecraft at the time of the SSC was characterized by a large amplitude oscillation (80 mV/m peak to peak) with a period corresponding to the 150 second drift echo period of the simultaneously observed 15 MeV electrons. Considerations of previous statistical studies of the magnitude of SSC electric and magnetic fields versus local time and analysis of the energization and cross‐L transport of the particles imply the existence of 200 to 300 mV/m electric fields over much of the dayside magnetosphere. These observations also suggest that the 15 MeV drift echo electrons were selectively energized because their gradient drift velocity allowed them to reside in the region of strong electric fields for the duration of the accelerating phase of the electric field.</jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1380004236852388613","@type":"Researcher","foaf:name":[{"@value":"J. Wygant"}]},{"@id":"https://cir.nii.ac.jp/crid/1381137044885115265","@type":"Researcher","foaf:name":[{"@value":"F. Mozer"}]},{"@id":"https://cir.nii.ac.jp/crid/1381137044885115264","@type":"Researcher","foaf:name":[{"@value":"M. Temerin"}]},{"@id":"https://cir.nii.ac.jp/crid/1381137044885115138","@type":"Researcher","foaf:name":[{"@value":"J. Blake"}]},{"@id":"https://cir.nii.ac.jp/crid/1381137044885115136","@type":"Researcher","foaf:name":[{"@value":"N. Maynard"}]},{"@id":"https://cir.nii.ac.jp/crid/1381137044885115266","@type":"Researcher","foaf:name":[{"@value":"H. Singer"}]},{"@id":"https://cir.nii.ac.jp/crid/1381137044885115139","@type":"Researcher","foaf:name":[{"@value":"M. Smiddy"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"00948276"},{"@type":"EISSN","@value":"19448007"}],"prism:publicationName":[{"@value":"Geophysical Research Letters"}],"dc:publisher":[{"@value":"American Geophysical Union (AGU)"}],"prism:publicationDate":"1994-08","prism:volume":"21","prism:number":"16","prism:startingPage":"1739","prism:endingPage":"1742"},"reviewed":"false","dc:rights":["http://onlinelibrary.wiley.com/termsAndConditions#vor"],"url":[{"@id":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1029%2F94GL00375"},{"@id":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/94GL00375"}],"createdAt":"2004-02-04","modifiedAt":"2023-09-22","relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1050845760765770752","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Relationship between solar wind dynamic pressure and amplitude of geomagnetic sudden commencement (SC)"}]},{"@id":"https://cir.nii.ac.jp/crid/1360567179761549184","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Propagation and evolution of electric fields associated with solar wind pressure pulses based on spacecraft and ground‐based observations"}]},{"@id":"https://cir.nii.ac.jp/crid/1390001206511826176","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Electrodynamics in the duskside inner magnetosphere and plasmasphere during a super magnetic storm on March 13-15, 1989"}]},{"@id":"https://cir.nii.ac.jp/crid/1390001206513307392","@type":"Article","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"SC related electric and magnetic field phenomena observed by the Akebono satellite inside the plasmasphere"}]},{"@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":"10.1029/94gl00375"},{"@type":"CROSSREF","@value":"10.1186/bf03353409_references_DOI_3hCDdfegcqXbfYveCbk8YCVbxOD"},{"@type":"CROSSREF","@value":"10.1186/s40623-016-0444-y_references_DOI_3hCDdfegcqXbfYveCbk8YCVbxOD"},{"@type":"CROSSREF","@value":"10.1186/s40645-021-00413-y_references_DOI_3hCDdfegcqXbfYveCbk8YCVbxOD"},{"@type":"CROSSREF","@value":"10.1186/bf03351843_references_DOI_3hCDdfegcqXbfYveCbk8YCVbxOD"},{"@type":"CROSSREF","@value":"10.1002/2017ja023990_references_DOI_3hCDdfegcqXbfYveCbk8YCVbxOD"}]}