An ionospheric scintillation index derived from dual-frequency Doppler measurements released by geodetic GNSS receivers operating at 1 Hz
Main Author: | |
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Publication Date: | 2023 |
Other Authors: | , , , , |
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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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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1834482492649766912 |