{"@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/1361981471373855104.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1002/2014gl060953"}},{"identifier":{"@type":"URI","@value":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1002%2F2014GL060953"}},{"identifier":{"@type":"URI","@value":"https://onlinelibrary.wiley.com/doi/pdf/10.1002/2014GL060953"}},{"identifier":{"@type":"URI","@value":"https://onlinelibrary.wiley.com/doi/full-xml/10.1002/2014GL060953"}},{"identifier":{"@type":"URI","@value":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1002/2014GL060953"}}],"dc:title":[{"@value":"Geomagnetic control of equatorial plasma bubble activity modeled by the TIEGCM with <i>Kp</i>"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:title>Abstract</jats:title><jats:p>Describing the day‐to‐day variability of Equatorial Plasma Bubble (EPB) occurrence remains a significant challenge. In this study we use the Thermosphere‐Ionosphere Electrodynamics General Circulation Model (TIEGCM), driven by solar (<jats:italic>F</jats:italic><jats:sub>10.7</jats:sub>) and geomagnetic (<jats:italic>K</jats:italic><jats:italic>p</jats:italic>) activity indices, to study daily variations of the linear Rayleigh‐Taylor (R‐T) instability growth rate in relation to the measured scintillation strength at five longitudinally distributed stations. For locations characterized by generally favorable conditions for EPB growth (i.e., within the scintillation season for that location), we find that the TIEGCM is capable of identifying days when EPB development, determined from the calculated R‐T growth rate, is suppressed as a result of geomagnetic activity. Both observed and modeled upward plasma drifts indicate that the prereversal enhancement scales linearly with <jats:italic>K</jats:italic><jats:italic>p</jats:italic> from several hours prior, from which it is concluded that even small <jats:italic>K</jats:italic><jats:italic>p</jats:italic> changes cause significant variations in daily EPB growth.</jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1380004057903080068","@type":"Researcher","foaf:name":[{"@value":"B. A. Carter"}],"jpcoar:affiliationName":[{"@value":"Institute for Scientific Research Boston College  Newton Massachusetts USA"},{"@value":"SPACE Research Centre RMIT University  Melbourne Victoria Australia"}]},{"@id":"https://cir.nii.ac.jp/crid/1381981471373855112","@type":"Researcher","foaf:name":[{"@value":"J. M. Retterer"}],"jpcoar:affiliationName":[{"@value":"Institute for Scientific Research Boston College  Newton Massachusetts USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1381981471373855114","@type":"Researcher","foaf:name":[{"@value":"E. Yizengaw"}],"jpcoar:affiliationName":[{"@value":"Institute for Scientific Research Boston College  Newton Massachusetts USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1381981471373855106","@type":"Researcher","foaf:name":[{"@value":"K. Groves"}],"jpcoar:affiliationName":[{"@value":"Institute for Scientific Research Boston College  Newton Massachusetts USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1381981471373855113","@type":"Researcher","foaf:name":[{"@value":"R. Caton"}],"jpcoar:affiliationName":[{"@value":"Air Force Research Laboratory Kirkland AFB  Albuquerque New Mexico USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1381981471373855108","@type":"Researcher","foaf:name":[{"@value":"L. McNamara"}],"jpcoar:affiliationName":[{"@value":"Air Force Research Laboratory Kirkland AFB  Albuquerque New Mexico USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1381981471373855104","@type":"Researcher","foaf:name":[{"@value":"C. Bridgwood"}],"jpcoar:affiliationName":[{"@value":"Institute for Scientific Research Boston College  Newton Massachusetts USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1381981471373855105","@type":"Researcher","foaf:name":[{"@value":"M. Francis"}],"jpcoar:affiliationName":[{"@value":"IPS Radio and Space Services Bureau of Meteorology  Sydney New South Wales Australia"}]},{"@id":"https://cir.nii.ac.jp/crid/1381981471373855107","@type":"Researcher","foaf:name":[{"@value":"M. Terkildsen"}],"jpcoar:affiliationName":[{"@value":"IPS Radio and Space Services Bureau of Meteorology  Sydney New South Wales Australia"}]},{"@id":"https://cir.nii.ac.jp/crid/1381981471373855111","@type":"Researcher","foaf:name":[{"@value":"R. Norman"}],"jpcoar:affiliationName":[{"@value":"SPACE Research Centre RMIT University  Melbourne Victoria Australia"}]},{"@id":"https://cir.nii.ac.jp/crid/1381981471373855109","@type":"Researcher","foaf:name":[{"@value":"K. Zhang"}],"jpcoar:affiliationName":[{"@value":"SPACE Research Centre RMIT University  Melbourne Victoria Australia"}]}],"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":"2014-08","prism:volume":"41","prism:number":"15","prism:startingPage":"5331","prism:endingPage":"5339"},"reviewed":"false","dc:rights":["http://onlinelibrary.wiley.com/termsAndConditions#vor"],"url":[{"@id":"https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1002%2F2014GL060953"},{"@id":"https://onlinelibrary.wiley.com/doi/pdf/10.1002/2014GL060953"},{"@id":"https://onlinelibrary.wiley.com/doi/full-xml/10.1002/2014GL060953"},{"@id":"https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1002/2014GL060953"}],"createdAt":"2014-07-21","modifiedAt":"2023-10-04","relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1050282813185827968","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Observation of equatorial plasma bubbles by the airglow imager on ISS-IMAP"}]},{"@id":"https://cir.nii.ac.jp/crid/1050282813782632832","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Equinoctial asymmetry in the zonal distribution of scintillation as observed by GPS receivers in Indonesia"}]},{"@id":"https://cir.nii.ac.jp/crid/1360298757412383488","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Challenges to Equatorial Plasma Bubble and Ionospheric Scintillation Short-Term Forecasting and Future Aspects in East and Southeast Asia"}]},{"@id":"https://cir.nii.ac.jp/crid/1360848654738430080","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"First Study on the Occurrence Frequency of Equatorial Plasma Bubbles over West Africa Using an All‐Sky Airglow Imager and GNSS Receivers"}]},{"@id":"https://cir.nii.ac.jp/crid/1360865815677714176","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Monitoring of equatorial plasma bubbles using aeronautical navigation system: a feasibility study"}]},{"@id":"https://cir.nii.ac.jp/crid/2050025942124959104","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Daily and seasonal variations in the linear growth rate of the Rayleigh-Taylor instability in the ionosphere obtained with GAIA"}]},{"@id":"https://cir.nii.ac.jp/crid/2050025942135631488","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Unseasonal development of post-sunset F-region irregularities over Southeast Asia on 28 July 2014 : 2. Forcing from below？"}]},{"@id":"https://cir.nii.ac.jp/crid/2050307417119864704","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Observations of equatorial plasma bubbles using a low-cost 630.0-nm all-sky imager in Ishigaki Island, Japan"}]},{"@id":"https://cir.nii.ac.jp/crid/2050870367078673408","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"A review of the SCOSTEP’s 5-year scientific program VarSITI—Variability of the Sun and Its Terrestrial Impact"}]},{"@id":"https://cir.nii.ac.jp/crid/2051151842031800576","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Unseasonal development of post-sunset F-region irregularities over Southeast Asia on 28 July 2014 : 1. Forcing from above？"}]}],"dataSourceIdentifier":[{"@type":"CROSSREF","@value":"10.1002/2014gl060953"},{"@type":"CROSSREF","@value":"10.1186/s40645-018-0175-8_references_DOI_7tznmFcPk5V3IDAZEOl7dxnRtYr"},{"@type":"CROSSREF","@value":"10.1186/s40645-018-0218-1_references_DOI_7tznmFcPk5V3IDAZEOl7dxnRtYr"},{"@type":"CROSSREF","@value":"10.1186/s40645-018-0227-0_references_DOI_7tznmFcPk5V3IDAZEOl7dxnRtYr"},{"@type":"CROSSREF","@value":"10.1186/s40645-021-00410-1_references_DOI_7tznmFcPk5V3IDAZEOl7dxnRtYr"},{"@type":"CROSSREF","@value":"10.1002/2017ja024146_references_DOI_7tznmFcPk5V3IDAZEOl7dxnRtYr"},{"@type":"CROSSREF","@value":"10.1007/s10712-020-09613-5_references_DOI_7tznmFcPk5V3IDAZEOl7dxnRtYr"},{"@type":"CROSSREF","@value":"10.1186/s40623-020-01187-1_references_DOI_7tznmFcPk5V3IDAZEOl7dxnRtYr"},{"@type":"CROSSREF","@value":"10.1186/s40645-018-0164-y_references_DOI_7tznmFcPk5V3IDAZEOl7dxnRtYr"},{"@type":"CROSSREF","@value":"10.1002/2017ja024602_references_DOI_7tznmFcPk5V3IDAZEOl7dxnRtYr"},{"@type":"CROSSREF","@value":"10.1186/s40623-023-01911-7_references_DOI_7tznmFcPk5V3IDAZEOl7dxnRtYr"}]}