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dc.contributor.authorWatthanasangmechai, Kornyanaten
dc.contributor.authorYamamoto, Mamoruen
dc.contributor.authorSaito, Akinorien
dc.contributor.authorMaruyama, Takashien
dc.contributor.authorYokoyama, Tatsuhiroen
dc.contributor.authorNishioka, Michien
dc.contributor.authorIshii, Mamoruen
dc.date.accessioned2015-11-06T04:57:36Z-
dc.date.available2015-11-06T04:57:36Z-
dc.date.issued2015-05-27-
dc.identifier.issn1343-8832-
dc.identifier.urihttp://hdl.handle.net/2433/201377-
dc.description.abstractTo reveal the temporal change of the equatorial ionization anomaly (EIA) asymmetry, a multipoint satellite-ground beacon experiment was conducted along the meridional plane of the Thailand–Indonesia sector. The observation includes one station near the magnetic equator and four stations at off-equator latitudes. This is the first EIA asymmetry study with high spatial resolution using GNU Radio Beacon Receiver (GRBR) observations in Southeast Asia. GRBR-total electron contents (TECs) from 97 polar-orbit satellite passes in March 2012 were analyzed in this study. Successive passes captured rapid evolution of EIA asymmetry, especially during geomagnetic disturbances. The penetrating electric fields that occur during geomagnetic disturbed days are not the cause of the asymmetry. Instead, high background TEC associated with an intense electric field empowers the neutral wind to produce severe asymmetry of the EIA. Such rapid evolution of EIA asymmetry was not seen during nighttime, when meridional wind mainly controlled the asymmetric structures. Additional data are necessary to identify the source of the variations, i.e., atmospheric waves. Precisely capturing the locations of the crests and the evolution of the asymmetry enhances understanding of the temporal change of EIA asymmetry at the local scale and leads to a future local modeling for TEC prediction in Southeast Asia.en
dc.format.mimetypeapplication/pdf-
dc.language.isoeng-
dc.publisherSpringerOpenen
dc.rights© 2015 Watthanasangmechai et al.; licensee Springer. This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly credited.en
dc.subjectEIA asymmetryen
dc.subjectGRBRen
dc.subjectBeacon receiver networken
dc.subjectSoutheast Asiaen
dc.subjectEquatorial ionosphereen
dc.subjectThermospheric meridional winden
dc.subjectGeomagnetic disturbancesen
dc.titleTemporal change of EIA asymmetry revealed by a beacon receiver network in Southeast Asiaen
dc.typejournal article-
dc.type.niitypeJournal Article-
dc.identifier.jtitleEarth, Planets and Spaceen
dc.identifier.volume67-
dc.identifier.issue1-
dc.relation.doi10.1186/s40623-015-0252-9-
dc.textversionpublisher-
dc.identifier.artnum623-
dcterms.accessRightsopen access-
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