{"@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/1361699995166562304.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1029/ja095ia04p04303"}},{"identifier":{"@type":"URI","@value":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1029%2FJA095iA04p04303"}},{"identifier":{"@type":"URI","@value":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/JA095iA04p04303"}}],"dc:title":[{"@value":"Solar cycle variations in <i>F</i> region electrodynamic drifts at Arecibo"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:p>Plasma drift measurements for the <jats:italic>F</jats:italic> region of the ionosphere have been made by the Arecibo incoherent scatter radar over the course of more than one solar cycle. The analysis of the data indicates that there are significant differences in the nighttime drifts between solar minimum and solar maximum. In general, these results agree qualitatively with results obtained through previous studies which have been done for incoherent scatter measurements from Jicamarca, Peru, as well as with some characteristics of model simulations.</jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1380004236852103170","@type":"Researcher","foaf:name":[{"@value":"JE Berkey"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"01480227"}],"prism:publicationName":[{"@value":"Journal of Geophysical Research: Space Physics"}],"dc:publisher":[{"@value":"American Geophysical Union (AGU)"}],"prism:publicationDate":"1990-04","prism:volume":"95","prism:number":"A4","prism:startingPage":"4303","prism:endingPage":"4306"},"reviewed":"false","dc:rights":["http://onlinelibrary.wiley.com/termsAndConditions#vor"],"url":[{"@id":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1029%2FJA095iA04p04303"},{"@id":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/JA095iA04p04303"}],"createdAt":"2008-02-06","modifiedAt":"2023-11-22","relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1050001335802470528","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Long-term variation in the upper atmosphere as seen in the geomagnetic solar quiet daily variation"}]}],"dataSourceIdentifier":[{"@type":"CROSSREF","@value":"10.1029/ja095ia04p04303"},{"@type":"CROSSREF","@value":"10.1186/s40623-014-0155-1_references_DOI_SCM8vcpb9ZXTEBSS02GVZQtVozO"}]}