{"@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/1362825893955040384.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1029/2010ja016017"}},{"identifier":{"@type":"URI","@value":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1029%2F2010JA016017"}},{"identifier":{"@type":"URI","@value":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/2010JA016017"}}],"dc:title":[{"@value":"A dynamical model of high‐latitude convection derived from SuperDARN plasma drift measurements"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:p>A discrete set of climatological patterns of high‐latitude ionospheric convection are derived using line‐of‐sight plasma drift data from the Super Dual Auroral Radar Network (SuperDARN). The patterns are derived independently for the Northern Hemisphere and Southern Hemisphere and for varying solar wind, interplanetary magnetic field (IMF), and dipole tilt angle conditions. By interpolating between discrete patterns, a dynamical model of convection is obtained, which can uniquely specify the high‐latitude electrostatic potential distribution for a wide range of solar wind, IMF, and dipole tilt parameter values. Accounting for solar wind velocity dependencies in convection leads to better resolving the large‐scale convection pattern, as compared to previous statistical models based on SuperDARN data. It is shown that the mesoscale features of the climatological model compare favorably to the features seen in instantaneous patterns of convection observed with SuperDARN. Comparison of the model to other statistical or empirical models derived from ground‐ and space‐based measurements shows good agreement with most models.</jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1380848661784570766","@type":"Researcher","foaf:name":[{"@value":"E. D. P. Cousins"}],"jpcoar:affiliationName":[{"@value":"Thayer School of Engineering Dartmouth College  Hanover New Hampshire USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1382825893955040384","@type":"Researcher","foaf:name":[{"@value":"S. G. Shepherd"}],"jpcoar:affiliationName":[{"@value":"Thayer School of Engineering Dartmouth College  Hanover New Hampshire USA"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"01480227"}],"prism:publicationName":[{"@value":"Journal of Geophysical Research: Space Physics"}],"dc:publisher":[{"@value":"American Geophysical Union (AGU)"}],"prism:publicationDate":"2010-12","prism:volume":"115","prism:number":"A12","prism:startingPage":"A12329"},"reviewed":"false","dc:rights":["http://onlinelibrary.wiley.com/termsAndConditions#vor"],"url":[{"@id":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1029%2F2010JA016017"},{"@id":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/2010JA016017"}],"createdAt":"2010-12-20","modifiedAt":"2023-11-02","relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1360004229808121344","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Average field‐aligned ion velocity over the EISCAT radars"}]},{"@id":"https://cir.nii.ac.jp/crid/1360004240189481472","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Local time extent of magnetopause reconnection using space–ground coordination"}]},{"@id":"https://cir.nii.ac.jp/crid/1360294643748518144","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Cusp Dynamics and Polar Cap Patch Formation Associated With a Small IMF Southward Turning"}]},{"@id":"https://cir.nii.ac.jp/crid/2051151842044692096","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Review of the accomplishments of midlatitude Super Dual Auroral Radar Network (SuperDARN) HF radars"}]}],"dataSourceIdentifier":[{"@type":"CROSSREF","@value":"10.1029/2010ja016017"},{"@type":"CROSSREF","@value":"10.1002/2017ja023974_references_DOI_2KaLb58MoYpylVsF7jzDNu0ILcd"},{"@type":"CROSSREF","@value":"10.5194/angeo-37-215-2019_references_DOI_2KaLb58MoYpylVsF7jzDNu0ILcd"},{"@type":"CROSSREF","@value":"10.1029/2020ja029090_references_DOI_2KaLb58MoYpylVsF7jzDNu0ILcd"},{"@type":"CROSSREF","@value":"10.1186/s40645-019-0270-5_references_DOI_2KaLb58MoYpylVsF7jzDNu0ILcd"}]}