{"@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/1361699995936049792.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1029/2006gl027578"}},{"identifier":{"@type":"URI","@value":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1029%2F2006GL027578"}},{"identifier":{"@type":"URI","@value":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/2006GL027578"}}],"dc:title":[{"@value":"Correlation between energetic ion enhancements and heliospheric current sheet crossings in the outer heliosphere"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:p>Voyagers 1 and 2 observed highly‐variable beams of energetic ions in the foreshock region upstream of the termination shock (TS). At Voyager 2 (V2), the ion intensities are generally not related to the plasma properties. At Voyager 1 (V1), the beams are often coincident with crossings of the heliospheric current sheet (HCS). The V1 intensity peaks occur when the HCS is crossed from negative to positive magnetic polarities and V1 is within a few AU of the TS. Two mechanisms are considered: current sheet drift and streaming of ions from the TS along magnetic field lines which are parallel to the HCS. The current sheet drift hypothesis predicts that enhancements observed at V2 will occur when the HCS is crossed in the opposite direction, from positive to negative magnetic polarity, since V2 is at southern heliolatitudes.</jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1380290617391261447","@type":"Researcher","foaf:name":[{"@value":"J. D. Richardson"}],"jpcoar:affiliationName":[{"@value":"Center for Space Research Massachusetts Institute of Technology  Cambridge Massachusetts USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1381699995936049796","@type":"Researcher","foaf:name":[{"@value":"E. C. Stone"}],"jpcoar:affiliationName":[{"@value":"Division of Physics, Mathematics, and Astronomy California Institute of Technology  Pasadena California USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1381699995936049794","@type":"Researcher","foaf:name":[{"@value":"A. C. Cummings"}],"jpcoar:affiliationName":[{"@value":"Division of Physics, Mathematics, and Astronomy California Institute of Technology  Pasadena California USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1381699995936049797","@type":"Researcher","foaf:name":[{"@value":"J. C. Kasper"}],"jpcoar:affiliationName":[{"@value":"Center for Space Research Massachusetts Institute of Technology  Cambridge Massachusetts USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1381699995936049792","@type":"Researcher","foaf:name":[{"@value":"M. Zhang"}],"jpcoar:affiliationName":[{"@value":"Department of Physics and Space Sciences Florida Institute of Technology  Melbourne Florida USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1381699995936049799","@type":"Researcher","foaf:name":[{"@value":"L. F. Burlaga"}],"jpcoar:affiliationName":[{"@value":"Laboratory for Solar and Space Physics NASA Goddard Space Flight Center  Greenbelt Maryland USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1381699995936049793","@type":"Researcher","foaf:name":[{"@value":"N. F. Ness"}],"jpcoar:affiliationName":[{"@value":"Bartol Research Institute University of Delaware  Newark Delaware USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1381699995936049798","@type":"Researcher","foaf:name":[{"@value":"Y. Liu"}],"jpcoar:affiliationName":[{"@value":"Center for Space Research Massachusetts Institute of Technology  Cambridge Massachusetts USA"}]}],"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":"2006-11","prism:volume":"33","prism:number":"21","prism:startingPage":"1"},"reviewed":"false","dc:rights":["http://onlinelibrary.wiley.com/termsAndConditions#vor"],"url":[{"@id":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1029%2F2006GL027578"},{"@id":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/2006GL027578"}],"createdAt":"2006-11-13","modifiedAt":"2023-10-31","relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/2050307417125237632","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Unusual enhancement of ~ 30 MeV proton flux in an ICME sheath region"}]}],"dataSourceIdentifier":[{"@type":"CROSSREF","@value":"10.1029/2006gl027578"},{"@type":"CROSSREF","@value":"10.1186/s40623-021-01362-y_references_DOI_Rr4Yrpuv2ENhPtgUELucFdPRrPW"}]}