{"@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/1361137046352741632.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.5194/angeo-28-2059-2010"}},{"identifier":{"@type":"URI","@value":"https://angeo.copernicus.org/articles/28/2059/2010/angeo-28-2059-2010.pdf"}}],"dc:title":[{"@value":"Equatorial spread &lt;I&gt;F&lt;/I&gt; fossil plumes"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:p>Abstract. Behaviour of equatorial spread F (ESF) fossil plumes, i.e., ESF plumes that have stopped rising, is examined using the NRL SAMI3/ESF three-dimensional simulation code. We find that fossil bubbles, plasma density depletions associated with fossil plumes, can persist as high-altitude equatorial depletions even while being \"blown\" by zonal winds. Corresponding airglow-proxy images of fossil plumes, plots of electron density versus longitude and latitude at a constant altitude of 288 km, are shown to partially \"fill in\" in most cases, beginning with the highest altitude field lines within the plume. Specifically, field lines upon which the E field has fallen entirely to zero are affected and only the low altitude (≤600 km) portion if each field line fills in. This suggests that it should be possible to observe a bubble at high altitude on a field line for which the corresponding airglow image no longer shows a depletion. In all cases ESF plumes stop rising when the flux-tube-integrated ion mass density inside the upper edge of the bubble is equal to that of the nearby background, further supporting the result of Krall et al. (2010b).\n                    </jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1381137046352741635","@type":"Researcher","foaf:name":[{"@value":"J. Krall"}]},{"@id":"https://cir.nii.ac.jp/crid/1380285711830766475","@type":"Researcher","foaf:name":[{"@value":"J. D. Huba"}]},{"@id":"https://cir.nii.ac.jp/crid/1381137046352741632","@type":"Researcher","foaf:name":[{"@value":"S. L. Ossakow"}]},{"@id":"https://cir.nii.ac.jp/crid/1381137046352741633","@type":"Researcher","foaf:name":[{"@value":"G. Joyce"}]}],"publication":{"publicationIdentifier":[{"@type":"EISSN","@value":"14320576"}],"prism:publicationName":[{"@value":"Annales Geophysicae"}],"dc:publisher":[{"@value":"Copernicus GmbH"}],"prism:publicationDate":"2010-11-09","prism:volume":"28","prism:number":"11","prism:startingPage":"2059","prism:endingPage":"2069"},"reviewed":"false","dc:rights":["https://creativecommons.org/licenses/by/3.0/"],"url":[{"@id":"https://angeo.copernicus.org/articles/28/2059/2010/angeo-28-2059-2010.pdf"}],"createdAt":"2010-11-09","modifiedAt":"2021-01-23","relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1360004229806106496","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Shrinking equatorial plasma bubbles"}]},{"@id":"https://cir.nii.ac.jp/crid/1360567179757649408","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Predawn plasma bubble cluster observed in Southeast Asia"}]},{"@id":"https://cir.nii.ac.jp/crid/1360865815483929600","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Ionosphere-thermosphere interaction"}]},{"@id":"https://cir.nii.ac.jp/crid/2051433317007350400","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"A review on the numerical simulation of equatorial plasma bubbles toward scintillation evaluation and forecasting"}]}],"dataSourceIdentifier":[{"@type":"CROSSREF","@value":"10.5194/angeo-28-2059-2010"},{"@type":"CROSSREF","@value":"10.1002/2016ja022633_references_DOI_Qnrsu9aFUD4WCXs3YcIz04oxKRL"},{"@type":"CROSSREF","@value":"10.1186/s40645-017-0153-6_references_DOI_Qnrsu9aFUD4WCXs3YcIz04oxKRL"},{"@type":"CROSSREF","@value":"10.1002/2015ja022069_references_DOI_Qnrsu9aFUD4WCXs3YcIz04oxKRL"},{"@type":"CROSSREF","@value":"10.1016/b978-0-12-821366-7.00003-2_references_DOI_Qnrsu9aFUD4WCXs3YcIz04oxKRL"}]}