Please use this identifier to cite or link to this item: http://hdl.handle.net/10397/100719
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dc.contributorDepartment of Land Surveying and Geo-Informaticsen_US
dc.creatorLiu, Zen_US
dc.creatorYang, Zen_US
dc.creatorXu, Den_US
dc.creatorMorton, YJen_US
dc.date.accessioned2023-08-11T03:12:54Z-
dc.date.available2023-08-11T03:12:54Z-
dc.identifier.issn0048-6604en_US
dc.identifier.urihttp://hdl.handle.net/10397/100719-
dc.language.isoenen_US
dc.publisherWiley-Blackwellen_US
dc.rights©2019. American Geophysical Union. All Rights Reserved.en_US
dc.titleOn inconsistent ROTI derived from multiconstellation GNSS measurements of globally distributed GNSS receivers for ionospheric irregularities characterizationen_US
dc.typeJournal/Magazine Articleen_US
dc.description.otherinformationTitle on author’s file: On Ionospheric Irregularities Characterized by nconsistent ROTI Derived from Multi-Constellation GNSS Measurements Based on Globally Distributed GNSS Receiversen_US
dc.identifier.spage215en_US
dc.identifier.epage232en_US
dc.identifier.volume54en_US
dc.identifier.issue3en_US
dc.identifier.doi10.1029/2018RS006596en_US
dcterms.abstractThis study for the first time presents an investigation into the exploitation of multi-Global Navigation Satellite System (GNSS) observations (Global Positioning System, Globalnaya Navigazionnaya Sputnikovaya Sistema, Galileo, and BeiDou) to characterize ionospheric plasma irregularities, based on the rate of change of total electron content index (ROTI) sampled at 1 s. It is demonstrated that the multi-GNSS ROTIs can represent temporal evolutions of ionospheric plasma irregularities during a large geomagnetic storm. However, an inconsistency in the magnitudes of multi-GNSS ROTIs is found among a variety of GNSS receivers (i.e., Javad, Leica, Trimble, and Septentrio). Through cross comparisons between GNSS receivers installed at zero/short baselines and validations by receivers distributed separately, it is observed that the magnitude of ROTI corresponding to each system differs between closely installed and even collocated receivers of different models, as well as between the GNSS signals on the same frequency. From 1-year (i.e., 2015) data analysis, it is found that the magnitudes of multi-GNSS ROTIs exhibit the dependence on the receiver type. Among the four GNSS receiver types, the largest discrepancy in the multi-GNSS ROTIs is observed from Septentrio receivers, while the smallest one is shown by Trimble receivers. A one-to-one comparison indicates that the ROTI difference is noticeable and can increase to 4–6 TECu/min under ionospheric irregularities conditions, that is, in the postsunset period of 18–02 local time. To investigate the inconsistency, the effect of adopting different equivalent noise bandwidths in the tracking loop design is discussed, via cross comparisons between a GNSS software-defined receiver and a collocated Septentrio receiver. The result shows that adopting 15- and 2-Hz noise bandwidths in the tracking loop can cause 0.2- to 0.5-TECu/min differences in the magnitude of ROTI, suggesting that the diverse tracking techniques deployed by various receivers are very likely a major contributor to the inconsistency of multi-GNSS ROTIs.en_US
dcterms.accessRightsopen accessen_US
dcterms.bibliographicCitationRadio science, Mar. 2019, v. 54, no. 3, p. 215-232en_US
dcterms.isPartOfRadio scienceen_US
dcterms.issued2019-03-
dc.identifier.scopus2-s2.0-85062496783-
dc.identifier.eissn1944-799xen_US
dc.description.validate202305 bckwen_US
dc.description.oaVersion of Recorden_US
dc.identifier.FolderNumberLSGI-0222-
dc.description.fundingSourceRGCen_US
dc.description.fundingSourceOthersen_US
dc.description.fundingTextPolyU; Key Program of National Natural Science Foundation of Chinaen_US
dc.description.pubStatusPublisheden_US
dc.identifier.OPUS29138110-
dc.description.oaCategoryVoR alloweden_US
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