Please use this identifier to cite or link to this item: http://hdl.handle.net/10397/113196
DC FieldValueLanguage
dc.contributorDepartment of Land Surveying and Geo-Informatics-
dc.creatorNie, W-
dc.creatorWang, F-
dc.creatorQiao, Z-
dc.creatorXu, T-
dc.creatorWang, Y-
dc.creatorYe, M-
dc.creatorHu, L-
dc.creatorLiu, T-
dc.date.accessioned2025-05-29T07:59:16Z-
dc.date.available2025-05-29T07:59:16Z-
dc.identifier.issn2169-9380-
dc.identifier.urihttp://hdl.handle.net/10397/113196-
dc.language.isoenen_US
dc.publisherWiley-Blackwell Publishing, Inc.en_US
dc.titleIonospheric irregularities coinciding with the 2023 Typhoon Saola : a multi-instrument studyen_US
dc.typeJournal/Magazine Articleen_US
dc.identifier.volume129-
dc.identifier.issue12-
dc.identifier.doi10.1029/2024JA033043-
dcterms.abstractTyphoons exert significant influences on the ionosphere through atmospheric waves, ultimately affecting radio signals in the L-band of the Global Navigation Satellite System (GNSS). Due to the limitations of ground observations, the mechanisms and full impacts of typhoon-induced ionospheric variation remain to be explored. To address this gap, we embarked on a challenging expedition, employing a shipborne ionospheric scintillation monitoring receiver (ISMR) to gather data near the trajectory of Typhoon Saola during August and September 2023. The results revealed prominent amplitude scintillation and total electron content fluctuations in GNSS satellite detections, particularly during sunset from 29 to 31 August 2023. The findings are cross-validated with ground GNSS stations, high-frequency radar and the Swarm satellite, confirming the presence of equatorial plasma bubbles (EPBs). These EPBs have demonstrable effects on GNSS signals, ultimately influencing the precision of positioning performance. By examining the influence of the neutral wind field on atmospheric gravity waves triggered by typhoons, we elucidated how these waves impact the ionosphere, ultimately leading to the formation of plasma bubbles.-
dcterms.accessRightsembargoed accessen_US
dcterms.bibliographicCitationJournal of geophysical research : space physics, Dec. 2024, v. 129, no. 12, e2024JA033043-
dcterms.isPartOfJournal of geophysical research : space physics-
dcterms.issued2024-12-
dc.identifier.scopus2-s2.0-85212692904-
dc.identifier.eissn2169-9402-
dc.identifier.artne2024JA033043-
dc.description.validate202505 bcch-
dc.identifier.FolderNumberOA_Othersen_US
dc.description.fundingSourceOthersen_US
dc.description.fundingTextNational Natural Science Foundation of China (42004012); Natural Science Foundation of Shandong Province, China (ZR2024MD094, ZR2022MD034); the Young Scholars Program of Shandong University, Weihai and Youth Innovation Team Development Project of Higher School in Shandong Province (2023KJ143); the International Partnership Program of Chinese Academy of Sciences (183311KYSB20200003); Xiaomi Young Talents Program, the Chinese Meridian Project, and the National Key Laboratory of Electromagnetic Environment (JCKY2022210C614240301); the National Natural Science Foundation of China (42020104002); the Solar-Terrestrial Environment Research Network (STERN) of Chinese Academy of Sciencesen_US
dc.description.pubStatusPublisheden_US
dc.date.embargo30/6/2025en_US
dc.description.oaCategoryVoR alloweden_US
Appears in Collections:Journal/Magazine Article
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Embargo End Date 30/6/2025
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