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dc.contributor.authorChunhua Jiangen_US
dc.contributor.authorGuobin Yangen_US
dc.contributor.authorJing Liuen_US
dc.contributor.authorTatsuhiro Yokoyamaen_US
dc.contributor.authorTongxin Liuen_US
dc.contributor.authorTing Lanen_US
dc.contributor.authorChen Zhouen_US
dc.contributor.authorYuannong Zhangen_US
dc.contributor.authorZhengyu Zhaoen_US
dc.contributor.authorTharadol Komolmisen_US
dc.contributor.authorPornchai Supnithien_US
dc.contributor.authorClara Y. Yatinien_US
dc.date.accessioned2018-09-05T03:27:13Z-
dc.date.available2018-09-05T03:27:13Z-
dc.date.issued2017-05-01en_US
dc.identifier.issn21699402en_US
dc.identifier.issn21699380en_US
dc.identifier.other2-s2.0-85019950142en_US
dc.identifier.other10.1002/2017JA024134en_US
dc.identifier.urihttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85019950142&origin=inwarden_US
dc.identifier.urihttp://cmuir.cmu.ac.th/jspui/handle/6653943832/56525-
dc.description.abstract©2017. American Geophysical Union. All Rights Reserved. This study mainly investigates equatorial and low-latitude ionospheric response to a great geomagnetic storm that occurred on 17 March 2015. We found that there were some interesting ionospheric phenomena, e.g., short-term ionospheric positive effect, daytime spread F, and morning Equatorial Ionization Anomaly (EIA) in the topside ionosphere, emerged at equatorial and low-latitude region along the longitude of about 100°E. Ground-based ionosondes and in situ satellite (Swarm) were utilized to study the possible mechanisms for these ionospheric phenomena. We found that vertical downward transport of plasma or neutral induced by traveling ionospheric disturbances (TIDs) or traveling atmospheric disturbances (TADs) might make a contribution to the short-term ionospheric positive effect at the main stage of this great storm. Additionally, results suggested that the occurrence of daytime spread F at low latitudes might be due to the diffusion of equatorial ionospheric irregularities in the topside ionosphere along geomagnetic field lines. Moreover, observational evidence shows that TIDs also might be the main driver for morning EIA-like feature recorded by Swarm B satellite in the topside ionosphere. These ionospheric phenomena mentioned above could make us gain a better understanding of ionospheric storm effects at equatorial and low-latitude region.en_US
dc.subjectAgricultural and Biological Sciencesen_US
dc.subjectEarth and Planetary Sciencesen_US
dc.subjectEnvironmental Scienceen_US
dc.titleEquatorial and low-latitude ionospheric response to the 17–18 March 2015 great storm over Southeast Asia longitude sectoren_US
dc.typeJournalen_US
article.title.sourcetitleJournal of Geophysical Research: Space Physicsen_US
article.volume122en_US
article.stream.affiliationsWuhan Universityen_US
article.stream.affiliationsChina Earthquake Administrationen_US
article.stream.affiliationsJapan National Institute of Information and Communications Technologyen_US
article.stream.affiliationsChiang Mai Universityen_US
article.stream.affiliationsKing Mongkuts University of Technologyen_US
article.stream.affiliationsIndonesian National Institute of Aeronautics and Spaceen_US
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