Performance of the L2C civil GPS signal under various ionospheric scintillation effects
Main Author: | |
---|---|
Publication Date: | 2016 |
Other Authors: | , |
Format: | Article |
Language: | eng |
Source: | Repositório Institucional da UNESP |
Download full: | http://dx.doi.org/10.1007/s10291-015-0472-2 http://hdl.handle.net/11449/168485 |
Summary: | 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. |
id |
UNSP_91f3e8a11f7a8fa23f9e194f9076db21 |
---|---|
oai_identifier_str |
oai:repositorio.unesp.br:11449/168485 |
network_acronym_str |
UNSP |
network_name_str |
Repositório Institucional da UNESP |
repository_id_str |
2946 |
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 |
_version_ |
1834482438762397696 |