{"@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/1360855567866914432.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1002/2016gl069096"}},{"identifier":{"@type":"URI","@value":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1002%2F2016GL069096"}},{"identifier":{"@type":"URI","@value":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1002/2016GL069096"}}],"dc:title":[{"@value":"Cluster observations of reflected EMIC‐triggered emission"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:title>Abstract</jats:title><jats:p>On 19 March 2001, the Cluster fleet recorded an electromagnetic rising tone on the nightside of the plasmasphere. The emission was found to propagate toward the Earth and toward the magnetic equator at a group velocity of about 200 km/s. The Poynting vector is mainly oblique to the background magnetic field and directed toward the Earth. The propagation angle \n<jats:inline-graphic xmlns:xlink=\"http://www.w3.org/1999/xlink\" xlink:href=\"graphic/grl54384-math-0001.png\" xlink:title=\"urn:x-wiley:grl:media:grl54384:grl54384-math-0001\"/> becomes more oblique with increasing magnetic latitude. Inside each rising tone \n<jats:inline-graphic xmlns:xlink=\"http://www.w3.org/1999/xlink\" xlink:href=\"graphic/grl54384-math-0002.png\" xlink:title=\"urn:x-wiley:grl:media:grl54384:grl54384-math-0002\"/> is more field aligned for higher frequencies. Comparing our results to previous ray tracing analysis we conclude that this emission is a triggered electromagnetic ion cyclotron (EMIC) wave generated at the nightside plasmapause. We detect the wave just after its reflection in the plasmasphere. The reflection makes the tone slope shallower. This process can contribute to the formation of pearl pulsations.</jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1380848661783125633","@type":"Researcher","foaf:name":[{"@value":"B. Grison"}],"jpcoar:affiliationName":[{"@value":"Department of Space Physics, Institute of Atmospheric Physics CAS  Prague Czech Republic"}]},{"@id":"https://cir.nii.ac.jp/crid/1380855567866914436","@type":"Researcher","foaf:name":[{"@value":"F. Darrouzet"}],"jpcoar:affiliationName":[{"@value":"Royal Belgian Institute for Space Aeronomy (BIRA‐IASB)  Brussels Belgium"}]},{"@id":"https://cir.nii.ac.jp/crid/1380855567866914432","@type":"Researcher","foaf:name":[{"@value":"O. Santolík"}],"jpcoar:affiliationName":[{"@value":"Department of Space Physics, Institute of Atmospheric Physics CAS  Prague Czech Republic"},{"@value":"Faculty of Mathematics and Physics Charles University  Prague Czech Republic"}]},{"@id":"https://cir.nii.ac.jp/crid/1380579816633469312","@type":"Researcher","foaf:name":[{"@value":"N. Cornilleau‐Wehrlin"}],"jpcoar:affiliationName":[{"@value":"Laboratoire de Physique des Plasmas CNRS/Ecole Polytechnique/Obs. de Paris/UPMC/Univ. Paris‐Sud  Palaiseau France"}]},{"@id":"https://cir.nii.ac.jp/crid/1380855567866914433","@type":"Researcher","foaf:name":[{"@value":"A. Masson"}],"jpcoar:affiliationName":[{"@value":"Science Operations Department, ESAC European Space Agency  Madrid Spain"}]}],"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":"2016-05-14","prism:volume":"43","prism:number":"9","prism:startingPage":"4164","prism:endingPage":"4171"},"reviewed":"false","dc:rights":["http://onlinelibrary.wiley.com/termsAndConditions#vor"],"url":[{"@id":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1002%2F2016GL069096"},{"@id":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1002/2016GL069096"}],"createdAt":"2016-05-02","modifiedAt":"2023-09-09","relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1050845763137853440","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Onboard software of Plasma Wave Experiment aboard Arase: instrument management and signal processing of Waveform Capture/Onboard Frequency Analyzer"}]},{"@id":"https://cir.nii.ac.jp/crid/1360294643716454144","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Multipoint Analysis of Source Regions of EMIC Waves and Rapid Growth of Subpackets"}]}],"dataSourceIdentifier":[{"@type":"CROSSREF","@value":"10.1002/2016gl069096"},{"@type":"CROSSREF","@value":"10.1029/2021ja029514_references_DOI_EYeVNaUsAqFuON000PgvmSMSnEv"},{"@type":"CROSSREF","@value":"10.1186/s40623-018-0838-0_references_DOI_3CiN5uHKQgpEyEQulv61n3YpRBU"}]}