Please use this identifier to cite or link to this item: http://hdl.handle.net/10397/112889
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dc.contributorDepartment of Land Surveying and Geo-Informaticsen_US
dc.creatorZhang, Ben_US
dc.creatorLiu, Ten_US
dc.creatorFeng, Xen_US
dc.creatorXu, Gen_US
dc.date.accessioned2025-05-09T06:14:44Z-
dc.date.available2025-05-09T06:14:44Z-
dc.identifier.issn1539-4956en_US
dc.identifier.urihttp://hdl.handle.net/10397/112889-
dc.language.isoenen_US
dc.publisherWiley-Blackwell Publishing, Inc.en_US
dc.rights© 2025 The Author(s). This is an open access article under the terms of the Creative Commons Attribution‐NonCommercial (http://creativecommons.org/licenses/by-nc/4.0/) License, which permits use, distribution and reproduction in any medium, provided the original work is properly cited and is not used for commercial purposes.en_US
dc.rightsThe following publication Zhang, B., Liu, T., Feng, X., & Xu, G. (2025). Successively equatorward propagating ionospheric acoustic waves and possible mechanisms following the Mw 7.5 earthquake in Noto, Japan, on 1 January 2024. Space Weather, 23(4), e2024SW003957 is available at https://doi.org/10.1029/2024SW003957.en_US
dc.titleSuccessively equatorward propagating ionospheric acoustic waves and possible mechanisms following the Mw 7.5 earthquake in Noto, Japan, on 1 January 2024en_US
dc.typeJournal/Magazine Articleen_US
dc.identifier.volume23en_US
dc.identifier.issue4en_US
dc.identifier.doi10.1029/2024SW003957en_US
dcterms.abstractOn 1 January 2024, the Mw 7.5 Noto Peninsula earthquake in Japan generated ionospheric disturbances detected via dense GNSS networks. Significant coseismic acoustic waves emerged ∼8 min post-event, exhibiting 0.3 TECU amplitudes, 2–8 min periods, and ∼1 km/s propagation speeds. These disturbances propagated exclusively southward as arc-shaped fronts. The observed anisotropy aligns closely with the local geomagnetic field orientation (declination 8.7°), suggesting magnetic channeling as a key factor. Secondary factors likely include northward thermospheric winds suppressing northward wave propagation and land-ocean coupling efficiency differences, which enhanced vertical displacements over southern continental regions. Notably, weak disturbances linked to the Mw 6.2 aftershock were detected, challenging conventional magnitude thresholds for ionospheric detection. While the mainshock's CID dynamics reflect known magnetic guidance mechanisms, the southward preference highlights site-specific interactions between seismic forcing and geophysical filters. This study provides new observational evidence of earthquake-ionosphere coupling, emphasizing the detectability of moderate-magnitude events under favorable conditions, with implications for space weather monitoring and multi-scale seismic hazard assessment.en_US
dcterms.accessRightsopen accessen_US
dcterms.bibliographicCitationSpace weather, Apr. 2025, v. 23, no. 4, e2024SW003957en_US
dcterms.isPartOfSpace weatheren_US
dcterms.issued2025-04-
dc.identifier.scopus2-s2.0-105002304825-
dc.identifier.eissn1542-7390en_US
dc.identifier.artne2024SW003957en_US
dc.description.validate202505 bcfcen_US
dc.description.oaVersion of Recorden_US
dc.identifier.FolderNumberOA_TA, a3752-
dc.identifier.SubFormID50938-
dc.description.fundingSourceOthersen_US
dc.description.fundingTextNational Key R&D Program of China (2022YFC3003800)en_US
dc.description.pubStatusPublisheden_US
dc.description.TAWiley (2025)en_US
dc.description.oaCategoryTAen_US
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