Performance of the L2C civil GPS signal under various ionospheric scintillation effects

Detalhes bibliográficos
Autor(a) principal: Marques, H. A.S. [UNESP]
Data de Publicação: 2016
Outros Autores: Monico, J. F.G. [UNESP], Marques, H. A.
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1007/s10291-015-0472-2
http://hdl.handle.net/11449/168485
Resumo: As GPS is modernizing, there are currently fourteen satellites transmitting L2C civil code and seven satellites transmitting L5 signal. While the GPS observables are subject to several sources of errors, the ionosphere is one of the largest error sources affecting GPS signals. Small irregularities in the electrons density along the GPS radio signal propagation path cause ionospheric scintillation that is characterized by rapid fluctuations in the signal amplitude and phase. The ionospheric scintillation effects are stronger in equatorial and high-latitude geomagnetic latitude regions and occur mainly due to equatorial anomaly and solar storms. Several researchers have analyzed the L2C signal quality since becoming available in December, 2005. We analyze the performance of L2C using GPS data from stations in the equatorial region of Brazil, which is subject of weak, moderate and strong ionospheric scintillation conditions. The GPS data were collected by Septentrio PolaRxS–PRO receivers as part of the CIGALA/CALIBRA network. The analysis was performed as a function of scintillations indexes S4 and Phi60, lock time (time interval in seconds that the carrier phase is tracked continuously without cycle slips), multipath RMS and position variation of precise point positioning solutions. The analysis shows that L2C code solutions are less affected by multipath effects than that of P2 when data are collected under weak ionospheric scintillation effects. In terms of analysis of positions, the kinematic PPP results using L2C instead P2 codes show accuracy improvements up to 33 % in periods of weak or strong ionospheric scintillation. When combining phase and code collected under weak scintillation effects, the results by applying L2C against P2 provide improvement in accuracy up to 59 %. However, for data under strong scintillation effects, the use of L2C for PPP with code and phase does not provide improvements in the positioning accuracy.
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spelling Performance of the L2C civil GPS signal under various ionospheric scintillation effectsGPS modernizationGPS positioningIonospheric scintillationL2CAs GPS is modernizing, there are currently fourteen satellites transmitting L2C civil code and seven satellites transmitting L5 signal. While the GPS observables are subject to several sources of errors, the ionosphere is one of the largest error sources affecting GPS signals. Small irregularities in the electrons density along the GPS radio signal propagation path cause ionospheric scintillation that is characterized by rapid fluctuations in the signal amplitude and phase. The ionospheric scintillation effects are stronger in equatorial and high-latitude geomagnetic latitude regions and occur mainly due to equatorial anomaly and solar storms. Several researchers have analyzed the L2C signal quality since becoming available in December, 2005. We analyze the performance of L2C using GPS data from stations in the equatorial region of Brazil, which is subject of weak, moderate and strong ionospheric scintillation conditions. The GPS data were collected by Septentrio PolaRxS–PRO receivers as part of the CIGALA/CALIBRA network. The analysis was performed as a function of scintillations indexes S4 and Phi60, lock time (time interval in seconds that the carrier phase is tracked continuously without cycle slips), multipath RMS and position variation of precise point positioning solutions. The analysis shows that L2C code solutions are less affected by multipath effects than that of P2 when data are collected under weak ionospheric scintillation effects. In terms of analysis of positions, the kinematic PPP results using L2C instead P2 codes show accuracy improvements up to 33 % in periods of weak or strong ionospheric scintillation. When combining phase and code collected under weak scintillation effects, the results by applying L2C against P2 provide improvement in accuracy up to 59 %. However, for data under strong scintillation effects, the use of L2C for PPP with code and phase does not provide improvements in the positioning accuracy.Sao Paulo State University (UNESP), Roberto Simonsen, 305Federal University of Pernambuco (UFPE), Prof. Moraes Rego, 1235Sao Paulo State University (UNESP), Roberto Simonsen, 305Universidade Estadual Paulista (Unesp)Universidade Federal de Pernambuco (UFPE)Marques, H. A.S. [UNESP]Monico, J. F.G. [UNESP]Marques, H. A.2018-12-11T16:41:28Z2018-12-11T16:41:28Z2016-04-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article139-149application/pdfhttp://dx.doi.org/10.1007/s10291-015-0472-2GPS Solutions, v. 20, n. 2, p. 139-149, 2016.1521-18861080-5370http://hdl.handle.net/11449/16848510.1007/s10291-015-0472-22-s2.0-84961157437Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengGPS Solutions1,674info:eu-repo/semantics/openAccess2025-04-11T19:38:54Zoai:repositorio.unesp.br:11449/168485Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestrepositoriounesp@unesp.bropendoar:29462025-04-11T19:38:54Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Performance of the L2C civil GPS signal under various ionospheric scintillation effects
title Performance of the L2C civil GPS signal under various ionospheric scintillation effects
spellingShingle Performance of the L2C civil GPS signal under various ionospheric scintillation effects
Marques, H. A.S. [UNESP]
GPS modernization
GPS positioning
Ionospheric scintillation
L2C
title_short Performance of the L2C civil GPS signal under various ionospheric scintillation effects
title_full Performance of the L2C civil GPS signal under various ionospheric scintillation effects
title_fullStr Performance of the L2C civil GPS signal under various ionospheric scintillation effects
title_full_unstemmed Performance of the L2C civil GPS signal under various ionospheric scintillation effects
title_sort Performance of the L2C civil GPS signal under various ionospheric scintillation effects
author Marques, H. A.S. [UNESP]
author_facet Marques, H. A.S. [UNESP]
Monico, J. F.G. [UNESP]
Marques, H. A.
author_role author
author2 Monico, J. F.G. [UNESP]
Marques, H. A.
author2_role author
author
dc.contributor.none.fl_str_mv Universidade Estadual Paulista (Unesp)
Universidade Federal de Pernambuco (UFPE)
dc.contributor.author.fl_str_mv Marques, H. A.S. [UNESP]
Monico, J. F.G. [UNESP]
Marques, H. A.
dc.subject.por.fl_str_mv GPS modernization
GPS positioning
Ionospheric scintillation
L2C
topic GPS modernization
GPS positioning
Ionospheric scintillation
L2C
description As GPS is modernizing, there are currently fourteen satellites transmitting L2C civil code and seven satellites transmitting L5 signal. While the GPS observables are subject to several sources of errors, the ionosphere is one of the largest error sources affecting GPS signals. Small irregularities in the electrons density along the GPS radio signal propagation path cause ionospheric scintillation that is characterized by rapid fluctuations in the signal amplitude and phase. The ionospheric scintillation effects are stronger in equatorial and high-latitude geomagnetic latitude regions and occur mainly due to equatorial anomaly and solar storms. Several researchers have analyzed the L2C signal quality since becoming available in December, 2005. We analyze the performance of L2C using GPS data from stations in the equatorial region of Brazil, which is subject of weak, moderate and strong ionospheric scintillation conditions. The GPS data were collected by Septentrio PolaRxS–PRO receivers as part of the CIGALA/CALIBRA network. The analysis was performed as a function of scintillations indexes S4 and Phi60, lock time (time interval in seconds that the carrier phase is tracked continuously without cycle slips), multipath RMS and position variation of precise point positioning solutions. The analysis shows that L2C code solutions are less affected by multipath effects than that of P2 when data are collected under weak ionospheric scintillation effects. In terms of analysis of positions, the kinematic PPP results using L2C instead P2 codes show accuracy improvements up to 33 % in periods of weak or strong ionospheric scintillation. When combining phase and code collected under weak scintillation effects, the results by applying L2C against P2 provide improvement in accuracy up to 59 %. However, for data under strong scintillation effects, the use of L2C for PPP with code and phase does not provide improvements in the positioning accuracy.
publishDate 2016
dc.date.none.fl_str_mv 2016-04-01
2018-12-11T16:41:28Z
2018-12-11T16:41:28Z
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/s10291-015-0472-2
GPS Solutions, v. 20, n. 2, p. 139-149, 2016.
1521-1886
1080-5370
http://hdl.handle.net/11449/168485
10.1007/s10291-015-0472-2
2-s2.0-84961157437
url http://dx.doi.org/10.1007/s10291-015-0472-2
http://hdl.handle.net/11449/168485
identifier_str_mv GPS Solutions, v. 20, n. 2, p. 139-149, 2016.
1521-1886
1080-5370
10.1007/s10291-015-0472-2
2-s2.0-84961157437
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv GPS Solutions
1,674
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv 139-149
application/pdf
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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