{"@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/1362262944704638720.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1016/0032-0633(92)90089-7"}},{"identifier":{"@type":"URI","@value":"https://api.elsevier.com/content/article/PII:0032063392900897?httpAccept=text/xml"}},{"identifier":{"@type":"URI","@value":"https://api.elsevier.com/content/article/PII:0032063392900897?httpAccept=text/plain"}}],"dc:title":[{"@value":"Mid-latitude and plasmaspheric hiss: A review"}],"description":[{"notation":[{"@value":"Abstract   A review of mid-latitude and plasmaspheric hiss-type emissions observed on ground-based stations and in the Earth's magnetosphere is presented. Different approaches to modelling of these emissions are discussed. It is pointed out that mid-latitude hiss emissions are most likely to be generated in the equatorial magnetosphere where the energy of electrons is transferred to wave energy via the electron cyclotron instability. Some quantitative characteristics of these emissions are explained in terms of a quasilinear model of this instability. Many properties of plasmaspheric hiss emissions are likely to be related to the same electron cyclotron instability, although the contribution of other mechanisms cannot be excluded."}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1380017282197315976","@type":"Researcher","foaf:name":[{"@value":"M. Hayakawa"}]},{"@id":"https://cir.nii.ac.jp/crid/1382262944704638721","@type":"Researcher","foaf:name":[{"@value":"S.S. Sazhin"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"00320633"}],"prism:publicationName":[{"@value":"Planetary and Space Science"}],"dc:publisher":[{"@value":"Elsevier BV"}],"prism:publicationDate":"1992-10","prism:volume":"40","prism:number":"10","prism:startingPage":"1325","prism:endingPage":"1338"},"reviewed":"false","dc:rights":["https://www.elsevier.com/tdm/userlicense/1.0/"],"url":[{"@id":"https://api.elsevier.com/content/article/PII:0032063392900897?httpAccept=text/xml"},{"@id":"https://api.elsevier.com/content/article/PII:0032063392900897?httpAccept=text/plain"}],"createdAt":"2003-01-17","modifiedAt":"2024-01-07","relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1360009142739828992","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Investigation of Small‐Scale Electron Density Irregularities Observed by the Arase and Van Allen Probes Satellites Inside and Outside the Plasmasphere"}]},{"@id":"https://cir.nii.ac.jp/crid/1360580230583935616","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Statistics of Unusual Naturally Occurring VLF Radio Emissions Termed Bursty‐Patches Observed at Kannuslehto, Finland"}]},{"@id":"https://cir.nii.ac.jp/crid/1360848654732391680","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Fine structure of plasmaspheric hiss"}]},{"@id":"https://cir.nii.ac.jp/crid/1390566775130621568","@type":"Article","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Effect of geomagnetic storms on VLF waves at low latitudes based on the analysis of whistlers and VLF emissions observed at Indian ground stations: A Review"}]},{"@id":"https://cir.nii.ac.jp/crid/2050588892106657280","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"A review of unusual VLF bursty-patches observed in Northern Finland for Earth, Planets and Space"}]}],"dataSourceIdentifier":[{"@type":"CROSSREF","@value":"10.1016/0032-0633(92)90089-7"},{"@type":"OPENAIRE","@value":"doi_dedup___::c958346c91971bc702841895071aac14"},{"@type":"CROSSREF","@value":"10.1029/2020ja027917_references_DOI_VHIWIN8KvnteVlfkUhZk7GV5d7d"},{"@type":"CROSSREF","@value":"10.1186/s40623-021-01516-y_references_DOI_VHIWIN8KvnteVlfkUhZk7GV5d7d"},{"@type":"CROSSREF","@value":"10.1029/2022ja030792_references_DOI_VHIWIN8KvnteVlfkUhZk7GV5d7d"},{"@type":"CROSSREF","@value":"10.1002/2014ja020437_references_DOI_VHIWIN8KvnteVlfkUhZk7GV5d7d"},{"@type":"CROSSREF","@value":"10.1541/jae.38.67_references_DOI_VHIWIN8KvnteVlfkUhZk7GV5d7d"}]}