{"@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/1363670319305251968.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1002/2015gl063187"}},{"identifier":{"@type":"URI","@value":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1002%2F2015GL063187"}},{"identifier":{"@type":"URI","@value":"https://onlinelibrary.wiley.com/doi/pdf/10.1002/2015GL063187"}},{"identifier":{"@type":"URI","@value":"https://onlinelibrary.wiley.com/doi/full-xml/10.1002/2015GL063187"}},{"identifier":{"@type":"URI","@value":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1002/2015GL063187"}}],"dc:title":[{"@value":"Electrostatic reconnection in the ionosphere"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:title>Abstract</jats:title><jats:p>Postsunset equatorial plasma bubble merging is examined using the National Research Laboratory code SAMI3/equatorial spread <jats:italic>F</jats:italic>. It is found that bubbles merge through an “electrostatic reconnection” process. As multiple bubbles develop, the electrostatic potential associated with one bubble can connect with that of a neighboring bubble: this provides a pathway for the low‐density plasma in one bubble to flow into the adjoining bubble and merge with it. Additionally, high‐speed plasma channels (approximately greater than hundreds of meters per second) can develop during the merging process. Optical data is presented of equatorial plasma bubble evolution that suggests bubble merging occurs in the nighttime equatorial ionosphere.</jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1380285711830766477","@type":"Researcher","foaf:name":[{"@value":"J. D. Huba"}],"jpcoar:affiliationName":[{"@value":"Plasma Physics Division Naval Research Laboratory  Washington District of Columbia USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1383670319305251970","@type":"Researcher","foaf:name":[{"@value":"T.‐W. Wu"}],"jpcoar:affiliationName":[{"@value":"Plasma Physics Division Naval Research Laboratory  Washington District of Columbia USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1383670319305251969","@type":"Researcher","foaf:name":[{"@value":"J. J. Makela"}],"jpcoar:affiliationName":[{"@value":"Department of Electrical and Computer Engineering University of Illinois at Urbana‐Champaign  Urbana Illinois USA"}]}],"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":"2015-03-27","prism:volume":"42","prism:number":"6","prism:startingPage":"1626","prism:endingPage":"1631"},"reviewed":"false","dc:rights":["http://onlinelibrary.wiley.com/termsAndConditions#vor"],"url":[{"@id":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1002%2F2015GL063187"},{"@id":"https://onlinelibrary.wiley.com/doi/pdf/10.1002/2015GL063187"},{"@id":"https://onlinelibrary.wiley.com/doi/full-xml/10.1002/2015GL063187"},{"@id":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1002/2015GL063187"}],"createdAt":"2015-02-24","modifiedAt":"2023-09-03","relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1360004229804174208","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"West wall structuring of equatorial plasma bubbles simulated by three‐dimensional HIRB model"}]},{"@id":"https://cir.nii.ac.jp/crid/1360021390558288768","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Modeling of Multi‐Ion Plasma Bubbles in the Equatorial Ionosphere"}]},{"@id":"https://cir.nii.ac.jp/crid/1360848654734306816","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"West wall structuring of equatorial plasma bubbles simulated by three-dimensional HIRB model"}]},{"@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":"10.1002/2015gl063187"},{"@type":"CROSSREF","@value":"10.1002/2015ja021799_references_DOI_LMfPts9Y94Go7UyJSoP6HMEw2zg"},{"@type":"CROSSREF","@value":"10.1029/2023ja031753_references_DOI_LMfPts9Y94Go7UyJSoP6HMEw2zg"},{"@type":"CROSSREF","@value":"10.1186/s40645-017-0153-6_references_DOI_LMfPts9Y94Go7UyJSoP6HMEw2zg"},{"@type":"CROSSREF","@value":"10.1002/2015ja021799-t_references_DOI_LMfPts9Y94Go7UyJSoP6HMEw2zg"}]}