Please use this identifier to cite or link to this item: http://hdl.handle.net/10397/109289
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dc.contributorDepartment of Land Surveying and Geo-Informatics-
dc.creatorGao, HY-
dc.creatorZhang, DH-
dc.creatorLiu, ZZ-
dc.creatorSun, SJ-
dc.creatorHao, YQ-
dc.creatorXiao, Z-
dc.date.accessioned2024-10-03T08:17:42Z-
dc.date.available2024-10-03T08:17:42Z-
dc.identifier.issn1539-4956-
dc.identifier.urihttp://hdl.handle.net/10397/109289-
dc.language.isoenen_US
dc.publisherWiley-Blackwell Publishing, Inc.en_US
dc.rights© 2023. The Authors. This is an open access article under the terms of the Creative Commons Attribution-NonCommercial-NoDerivs License (http://creativecommons.org/licenses/by-nc-nd/4.0/), which permits use and distribution in any medium, provided the original work is properly cited, the use is non-commercial and no modifications or adaptations are made.en_US
dc.rightsThe following publication Gao, H. Y., Zhang, D. H., Liu, Z. Z., Sun, S. J., Hao, Y. Q., & Xiao, Z. (2023). Revisiting the variation of the ionospheric irregularities in the low latitude region of China based on small regional geodetic GNSS station network. Space Weather, 21, e2023SW003452 is available at https://doi.org/10.1029/2023SW003452.en_US
dc.titleRevisiting the variation of the ionospheric irregularities in the low latitude region of China based on small regional geodetic GNSS station networken_US
dc.typeJournal/Magazine Articleen_US
dc.identifier.volume21-
dc.identifier.issue8-
dc.identifier.doi10.1029/2023SW003452-
dcterms.abstractThe rate of total electron content index (ROTI) and loss of lock (LoL) from global navigation satellite system (GNSS) observations are an important data source for ionospheric scintillation study. However, there are certain limitations of these data in ionospheric scintillation study, and clearing these limitations is important to understand the results from these data. In this paper, the variation of the ionospheric scintillation is revisited based on LoL and ROTI from a spatial dense GNSS network in the low latitude region of China. Via a priori knowledge of scintillation morphology, the method to determine the baseline ROTI for discriminating quiet and disturbed conditions is provided, and the abnormal data of ROTI and LoL unrelated to ionosphere are found and eliminated. Results show that the data examination is necessary. Using the qualified ROTI and LoL, the morphological variations of ionospheric irregularities are revisited. The temporal variation of ROTI and LoL are generally consistent, but there are some discrepancies. The maximum LoL occurrence is at about 21:00 LT, it is between 20:00 and 23:00 LT for ROTI. For spatial distribution, both parameters reach maximum occurrence in the southwest direction, but LoL is more concentrated. The azimuth range of maximum occurrence is 180–190° for LoL and 210–220° for ROTI. Statistically, the correlation between LoL occurrence and ROTI value from observation of single GNSS station is relatively good when ROTI <5 TECU/min, but it becomes worse when ROTI >5 TECU/min. However, their correlation can be greatly improved when data are averaged among all the stations.-
dcterms.accessRightsopen accessen_US
dcterms.bibliographicCitationSpace weather, Aug. 2023, v. 21, no. 8, e2023SW003452-
dcterms.isPartOfSpace weather-
dcterms.issued2023-08-
dc.identifier.scopus2-s2.0-85166663535-
dc.identifier.eissn1542-7390-
dc.identifier.artne2023SW003452-
dc.description.validate202410 bcch-
dc.description.oaVersion of Recorden_US
dc.identifier.FolderNumberOA_Scopus/WOSen_US
dc.description.fundingSourceOthersen_US
dc.description.fundingTextNational Natural Science Foundation of China; Stable-Support Scientific Project of China Research Institute of Radio-wave Propagation; Chinese Meridian Projecten_US
dc.description.pubStatusPublisheden_US
dc.description.oaCategoryCCen_US
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