An ionospheric scintillation index derived from dual-frequency Doppler measurements released by geodetic GNSS receivers operating at 1 Hz

Bibliographic Details
Main Author: Luo, Xiaomin
Publication Date: 2023
Other Authors: Xie, Zichun, Monico, João Francisco Galera [UNESP], Zhang, Baocheng, Pereira, Vinícius Amadeu Stuani, Lou, Yidong
Format: Article
Language: eng
Source: Repositório Institucional da UNESP
Download full: http://dx.doi.org/10.1007/s00190-023-01760-y
https://hdl.handle.net/11449/303986
Summary: Doppler measurements are immune to cycle slips, which offers great potential for constructing the ionospheric scintillation indexes. This study proposes a new scintillation index referred to as Doppler Index (DI) derived from dual-frequency Doppler measurements released by geodetic receivers operating at 1 Hz. The reliability of DI is compared with the dedicated scintillation indexes S4 and σφ outputted by the ionospheric scintillation monitoring receivers (ISMRs) as well as the indexes ROTI and S4c derived from geodetic GNSS receivers. Experimental results suggest that there is strong correlation between DI and the common scintillation indexes S4 , σφ , and ROTI . The statistics indicate that the mean values of correlation coefficients between DI and S4 / σφ are around 0.6–0.8 based on three ISMR stations data located at low, middle, and high latitudes. Using different types of geodetic GNSS receivers (Septentrio, Javad, Leica, and Trimble) data, the mean values of correlation coefficients between DI and ROTI can reach around 0.9. In addition, due to the different tracking technologies and locations for the different receiver types, the features of scintillation occurrence thresholds based on DI are also analyzed in this study. Statistical results suggest that for the Septentrio, Javad, Leica, and Trimble receivers, the μ+ 3 σ can be used as the threshold of DI in ionospheric scintillation monitoring.
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spelling An ionospheric scintillation index derived from dual-frequency Doppler measurements released by geodetic GNSS receivers operating at 1 HzDoppler indexGeodetic GNSS receiversIonospheric scintillation indexesIonospheric scintillation monitoring receiver (ISMR)Doppler measurements are immune to cycle slips, which offers great potential for constructing the ionospheric scintillation indexes. This study proposes a new scintillation index referred to as Doppler Index (DI) derived from dual-frequency Doppler measurements released by geodetic receivers operating at 1 Hz. The reliability of DI is compared with the dedicated scintillation indexes S4 and σφ outputted by the ionospheric scintillation monitoring receivers (ISMRs) as well as the indexes ROTI and S4c derived from geodetic GNSS receivers. Experimental results suggest that there is strong correlation between DI and the common scintillation indexes S4 , σφ , and ROTI . The statistics indicate that the mean values of correlation coefficients between DI and S4 / σφ are around 0.6–0.8 based on three ISMR stations data located at low, middle, and high latitudes. Using different types of geodetic GNSS receivers (Septentrio, Javad, Leica, and Trimble) data, the mean values of correlation coefficients between DI and ROTI can reach around 0.9. In addition, due to the different tracking technologies and locations for the different receiver types, the features of scintillation occurrence thresholds based on DI are also analyzed in this study. Statistical results suggest that for the Septentrio, Javad, Leica, and Trimble receivers, the μ+ 3 σ can be used as the threshold of DI in ionospheric scintillation monitoring.National Natural Science Foundation of ChinaSchool of Geography and Information Engineering China University of Geosciences (Wuhan), Lumo Road 388Faculty of Science and Technology Sao Paulo State University, Roberto Simonsen, 305, SPInnovation Academy for Precision Measurement Science and Technology Chinese Academy of SciencesGNSS Research Center Wuhan University, Luoyu Road 129Federal University of Technology -Parana, Cerejeira Street, PRFaculty of Science and Technology Sao Paulo State University, Roberto Simonsen, 305, SPNational Natural Science Foundation of China: 42104029China University of Geosciences (Wuhan)Universidade Estadual Paulista (UNESP)Chinese Academy of SciencesWuhan UniversityFederal University of Technology -ParanaLuo, XiaominXie, ZichunMonico, João Francisco Galera [UNESP]Zhang, BaochengPereira, Vinícius Amadeu StuaniLou, Yidong2025-04-29T19:33:33Z2023-07-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articlehttp://dx.doi.org/10.1007/s00190-023-01760-yJournal of Geodesy, v. 97, n. 7, 2023.1432-13940949-7714https://hdl.handle.net/11449/30398610.1007/s00190-023-01760-y2-s2.0-85165251919Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengJournal of Geodesyinfo:eu-repo/semantics/openAccess2025-04-30T14:24:23Zoai:repositorio.unesp.br:11449/303986Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestrepositoriounesp@unesp.bropendoar:29462025-04-30T14:24:23Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv An ionospheric scintillation index derived from dual-frequency Doppler measurements released by geodetic GNSS receivers operating at 1 Hz
title An ionospheric scintillation index derived from dual-frequency Doppler measurements released by geodetic GNSS receivers operating at 1 Hz
spellingShingle An ionospheric scintillation index derived from dual-frequency Doppler measurements released by geodetic GNSS receivers operating at 1 Hz
Luo, Xiaomin
Doppler index
Geodetic GNSS receivers
Ionospheric scintillation indexes
Ionospheric scintillation monitoring receiver (ISMR)
title_short An ionospheric scintillation index derived from dual-frequency Doppler measurements released by geodetic GNSS receivers operating at 1 Hz
title_full An ionospheric scintillation index derived from dual-frequency Doppler measurements released by geodetic GNSS receivers operating at 1 Hz
title_fullStr An ionospheric scintillation index derived from dual-frequency Doppler measurements released by geodetic GNSS receivers operating at 1 Hz
title_full_unstemmed An ionospheric scintillation index derived from dual-frequency Doppler measurements released by geodetic GNSS receivers operating at 1 Hz
title_sort An ionospheric scintillation index derived from dual-frequency Doppler measurements released by geodetic GNSS receivers operating at 1 Hz
author Luo, Xiaomin
author_facet Luo, Xiaomin
Xie, Zichun
Monico, João Francisco Galera [UNESP]
Zhang, Baocheng
Pereira, Vinícius Amadeu Stuani
Lou, Yidong
author_role author
author2 Xie, Zichun
Monico, João Francisco Galera [UNESP]
Zhang, Baocheng
Pereira, Vinícius Amadeu Stuani
Lou, Yidong
author2_role author
author
author
author
author
dc.contributor.none.fl_str_mv China University of Geosciences (Wuhan)
Universidade Estadual Paulista (UNESP)
Chinese Academy of Sciences
Wuhan University
Federal University of Technology -Parana
dc.contributor.author.fl_str_mv Luo, Xiaomin
Xie, Zichun
Monico, João Francisco Galera [UNESP]
Zhang, Baocheng
Pereira, Vinícius Amadeu Stuani
Lou, Yidong
dc.subject.por.fl_str_mv Doppler index
Geodetic GNSS receivers
Ionospheric scintillation indexes
Ionospheric scintillation monitoring receiver (ISMR)
topic Doppler index
Geodetic GNSS receivers
Ionospheric scintillation indexes
Ionospheric scintillation monitoring receiver (ISMR)
description Doppler measurements are immune to cycle slips, which offers great potential for constructing the ionospheric scintillation indexes. This study proposes a new scintillation index referred to as Doppler Index (DI) derived from dual-frequency Doppler measurements released by geodetic receivers operating at 1 Hz. The reliability of DI is compared with the dedicated scintillation indexes S4 and σφ outputted by the ionospheric scintillation monitoring receivers (ISMRs) as well as the indexes ROTI and S4c derived from geodetic GNSS receivers. Experimental results suggest that there is strong correlation between DI and the common scintillation indexes S4 , σφ , and ROTI . The statistics indicate that the mean values of correlation coefficients between DI and S4 / σφ are around 0.6–0.8 based on three ISMR stations data located at low, middle, and high latitudes. Using different types of geodetic GNSS receivers (Septentrio, Javad, Leica, and Trimble) data, the mean values of correlation coefficients between DI and ROTI can reach around 0.9. In addition, due to the different tracking technologies and locations for the different receiver types, the features of scintillation occurrence thresholds based on DI are also analyzed in this study. Statistical results suggest that for the Septentrio, Javad, Leica, and Trimble receivers, the μ+ 3 σ can be used as the threshold of DI in ionospheric scintillation monitoring.
publishDate 2023
dc.date.none.fl_str_mv 2023-07-01
2025-04-29T19:33:33Z
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/article
format article
status_str publishedVersion
dc.identifier.uri.fl_str_mv http://dx.doi.org/10.1007/s00190-023-01760-y
Journal of Geodesy, v. 97, n. 7, 2023.
1432-1394
0949-7714
https://hdl.handle.net/11449/303986
10.1007/s00190-023-01760-y
2-s2.0-85165251919
url http://dx.doi.org/10.1007/s00190-023-01760-y
https://hdl.handle.net/11449/303986
identifier_str_mv Journal of Geodesy, v. 97, n. 7, 2023.
1432-1394
0949-7714
10.1007/s00190-023-01760-y
2-s2.0-85165251919
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Journal of Geodesy
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.source.none.fl_str_mv Scopus
reponame:Repositório Institucional da UNESP
instname:Universidade Estadual Paulista (UNESP)
instacron:UNESP
instname_str Universidade Estadual Paulista (UNESP)
instacron_str UNESP
institution UNESP
reponame_str Repositório Institucional da UNESP
collection Repositório Institucional da UNESP
repository.name.fl_str_mv Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)
repository.mail.fl_str_mv repositoriounesp@unesp.br
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