Towards forecasting and mitigating ionospheric scintillation effects on GNSS

Detalhes bibliográficos
Autor(a) principal: Aquino, M.
Data de Publicação: 2007
Outros Autores: Dodson, A., DeFranceschi, G., Alfonsi, L., Romano, V., Monico, J. F G [UNESP], Marques, H. [UNESP], Mitchell, C.
Tipo de documento: Artigo de conferência
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1109/ELMAR.2007.4418801
http://hdl.handle.net/11449/70014
Resumo: The effect of the ionosphere on the signals of Global Navigation Satellite Systems (GNSS), such as the Global Positionig System (GPS) and the proposed European Galileo, is dependent on the ionospheric electron density, given by its Total Electron Content (TEC). Ionospheric time-varying density irregularities may cause scintillations, which are fluctuations in phase and amplitude of the signals. Scintillations occur more often at equatorial and high latitudes. They can degrade navigation and positioning accuracy and may cause loss of signal tracking, disrupting safety-critical applications, such as marine navigation and civil aviation. This paper addresses the results of initial research carried out on two fronts that are relevant to GNSS users if they are to counter ionospheric scintillations, i.e. forecasting and mitigating their effects. On the forecasting front, the dynamics of scintillation occurrence were analysed during the severe ionospheric storm that took place on the evening of 30 October 2003, using data from a network of GPS Ionospheric Scintillation and TEC Monitor (GISTM) receivers set up in Northern Europe. Previous results [1] indicated that GPS scintillations in that region can originate from ionospheric plasma structures from the American sector. In this paper we describe experiments that enabled confirmation of those findings. On the mitigation front we used the variance of the output error of the GPS receiver DLL (Delay Locked Loop) to modify the least squares stochastic model applied by an ordinary receiver to compute position. This error was modelled according to [2], as a function of the S4 amplitude scintillation index measured by the GISTM receivers. An improvement of up to 21% in relative positioning accuracy was achieved with this technnique.
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spelling Towards forecasting and mitigating ionospheric scintillation effects on GNSSGalileoGNSSGPSIonosphereIonospheric scintillationTotal Electron Content (TEC)Atmospheric electricityCurve fittingError analysisForecastingGlobal positioning systemIonospheric measurementLeast squares approximationsLight emissionLuminescenceMarine applicationsMathematical modelsNavigationResearchSatellite navigation aidsStochastic modelsAmplitude scintillation indexDelay-locked loop (DLL)Density irregularitiesEuropeanGalileo (CO)Global navigation satellite systems (GLONASS)GPS receiversHigh LatitudesIn phase (IP)International symposiumIonospheric electronIonospheric plasmasIonospheric scintillationsIonospheric stormLeast squares (LS)Loss of signalMarine navigationMobile multimediaMonitor (CO)Navigation and positioningOutput error (OE)Paper addressesRelative positioningSafety critical applicationsTime-varyingTotal electron content (TEC)ScintillationThe effect of the ionosphere on the signals of Global Navigation Satellite Systems (GNSS), such as the Global Positionig System (GPS) and the proposed European Galileo, is dependent on the ionospheric electron density, given by its Total Electron Content (TEC). Ionospheric time-varying density irregularities may cause scintillations, which are fluctuations in phase and amplitude of the signals. Scintillations occur more often at equatorial and high latitudes. They can degrade navigation and positioning accuracy and may cause loss of signal tracking, disrupting safety-critical applications, such as marine navigation and civil aviation. This paper addresses the results of initial research carried out on two fronts that are relevant to GNSS users if they are to counter ionospheric scintillations, i.e. forecasting and mitigating their effects. On the forecasting front, the dynamics of scintillation occurrence were analysed during the severe ionospheric storm that took place on the evening of 30 October 2003, using data from a network of GPS Ionospheric Scintillation and TEC Monitor (GISTM) receivers set up in Northern Europe. Previous results [1] indicated that GPS scintillations in that region can originate from ionospheric plasma structures from the American sector. In this paper we describe experiments that enabled confirmation of those findings. On the mitigation front we used the variance of the output error of the GPS receiver DLL (Delay Locked Loop) to modify the least squares stochastic model applied by an ordinary receiver to compute position. This error was modelled according to [2], as a function of the S4 amplitude scintillation index measured by the GISTM receivers. An improvement of up to 21% in relative positioning accuracy was achieved with this technnique.Institute of Engineering Surveying and Space Geodesy University of Nottingham, University Park, Nottingham, NG7 2RDNational Institute for Geophysics and Volcanology (INGV), Via di Vigna Murata 605, Rome, 00143Department of Cartography Sao Paulo State University (UNESP) at Presidente Prudente, 19060-900, Sao PauloDepartment of Electronic and Electrical Engineering University of Bath, Bath, BA2 7AYDepartment of Cartography Sao Paulo State University (UNESP) at Presidente Prudente, 19060-900, Sao PauloUniversity of NottinghamNational Institute for Geophysics and Volcanology (INGV)Universidade Estadual Paulista (Unesp)University of BathAquino, M.Dodson, A.DeFranceschi, G.Alfonsi, L.Romano, V.Monico, J. F G [UNESP]Marques, H. [UNESP]Mitchell, C.2014-05-27T11:22:39Z2014-05-27T11:22:39Z2007-12-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/conferenceObject63-67http://dx.doi.org/10.1109/ELMAR.2007.4418801Proceedings Elmar - International Symposium Electronics in Marine, p. 63-67.1334-2630http://hdl.handle.net/11449/7001410.1109/ELMAR.2007.44188012-s2.0-473490893897180879644760038Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengProceedings Elmar - International Symposium Electronics in Marine0,187info:eu-repo/semantics/openAccess2021-10-23T21:44:11Zoai:repositorio.unesp.br:11449/70014Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462021-10-23T21:44:11Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Towards forecasting and mitigating ionospheric scintillation effects on GNSS
title Towards forecasting and mitigating ionospheric scintillation effects on GNSS
spellingShingle Towards forecasting and mitigating ionospheric scintillation effects on GNSS
Aquino, M.
Galileo
GNSS
GPS
Ionosphere
Ionospheric scintillation
Total Electron Content (TEC)
Atmospheric electricity
Curve fitting
Error analysis
Forecasting
Global positioning system
Ionospheric measurement
Least squares approximations
Light emission
Luminescence
Marine applications
Mathematical models
Navigation
Research
Satellite navigation aids
Stochastic models
Amplitude scintillation index
Delay-locked loop (DLL)
Density irregularities
European
Galileo (CO)
Global navigation satellite systems (GLONASS)
GPS receivers
High Latitudes
In phase (IP)
International symposium
Ionospheric electron
Ionospheric plasmas
Ionospheric scintillations
Ionospheric storm
Least squares (LS)
Loss of signal
Marine navigation
Mobile multimedia
Monitor (CO)
Navigation and positioning
Output error (OE)
Paper addresses
Relative positioning
Safety critical applications
Time-varying
Total electron content (TEC)
Scintillation
title_short Towards forecasting and mitigating ionospheric scintillation effects on GNSS
title_full Towards forecasting and mitigating ionospheric scintillation effects on GNSS
title_fullStr Towards forecasting and mitigating ionospheric scintillation effects on GNSS
title_full_unstemmed Towards forecasting and mitigating ionospheric scintillation effects on GNSS
title_sort Towards forecasting and mitigating ionospheric scintillation effects on GNSS
author Aquino, M.
author_facet Aquino, M.
Dodson, A.
DeFranceschi, G.
Alfonsi, L.
Romano, V.
Monico, J. F G [UNESP]
Marques, H. [UNESP]
Mitchell, C.
author_role author
author2 Dodson, A.
DeFranceschi, G.
Alfonsi, L.
Romano, V.
Monico, J. F G [UNESP]
Marques, H. [UNESP]
Mitchell, C.
author2_role author
author
author
author
author
author
author
dc.contributor.none.fl_str_mv University of Nottingham
National Institute for Geophysics and Volcanology (INGV)
Universidade Estadual Paulista (Unesp)
University of Bath
dc.contributor.author.fl_str_mv Aquino, M.
Dodson, A.
DeFranceschi, G.
Alfonsi, L.
Romano, V.
Monico, J. F G [UNESP]
Marques, H. [UNESP]
Mitchell, C.
dc.subject.por.fl_str_mv Galileo
GNSS
GPS
Ionosphere
Ionospheric scintillation
Total Electron Content (TEC)
Atmospheric electricity
Curve fitting
Error analysis
Forecasting
Global positioning system
Ionospheric measurement
Least squares approximations
Light emission
Luminescence
Marine applications
Mathematical models
Navigation
Research
Satellite navigation aids
Stochastic models
Amplitude scintillation index
Delay-locked loop (DLL)
Density irregularities
European
Galileo (CO)
Global navigation satellite systems (GLONASS)
GPS receivers
High Latitudes
In phase (IP)
International symposium
Ionospheric electron
Ionospheric plasmas
Ionospheric scintillations
Ionospheric storm
Least squares (LS)
Loss of signal
Marine navigation
Mobile multimedia
Monitor (CO)
Navigation and positioning
Output error (OE)
Paper addresses
Relative positioning
Safety critical applications
Time-varying
Total electron content (TEC)
Scintillation
topic Galileo
GNSS
GPS
Ionosphere
Ionospheric scintillation
Total Electron Content (TEC)
Atmospheric electricity
Curve fitting
Error analysis
Forecasting
Global positioning system
Ionospheric measurement
Least squares approximations
Light emission
Luminescence
Marine applications
Mathematical models
Navigation
Research
Satellite navigation aids
Stochastic models
Amplitude scintillation index
Delay-locked loop (DLL)
Density irregularities
European
Galileo (CO)
Global navigation satellite systems (GLONASS)
GPS receivers
High Latitudes
In phase (IP)
International symposium
Ionospheric electron
Ionospheric plasmas
Ionospheric scintillations
Ionospheric storm
Least squares (LS)
Loss of signal
Marine navigation
Mobile multimedia
Monitor (CO)
Navigation and positioning
Output error (OE)
Paper addresses
Relative positioning
Safety critical applications
Time-varying
Total electron content (TEC)
Scintillation
description The effect of the ionosphere on the signals of Global Navigation Satellite Systems (GNSS), such as the Global Positionig System (GPS) and the proposed European Galileo, is dependent on the ionospheric electron density, given by its Total Electron Content (TEC). Ionospheric time-varying density irregularities may cause scintillations, which are fluctuations in phase and amplitude of the signals. Scintillations occur more often at equatorial and high latitudes. They can degrade navigation and positioning accuracy and may cause loss of signal tracking, disrupting safety-critical applications, such as marine navigation and civil aviation. This paper addresses the results of initial research carried out on two fronts that are relevant to GNSS users if they are to counter ionospheric scintillations, i.e. forecasting and mitigating their effects. On the forecasting front, the dynamics of scintillation occurrence were analysed during the severe ionospheric storm that took place on the evening of 30 October 2003, using data from a network of GPS Ionospheric Scintillation and TEC Monitor (GISTM) receivers set up in Northern Europe. Previous results [1] indicated that GPS scintillations in that region can originate from ionospheric plasma structures from the American sector. In this paper we describe experiments that enabled confirmation of those findings. On the mitigation front we used the variance of the output error of the GPS receiver DLL (Delay Locked Loop) to modify the least squares stochastic model applied by an ordinary receiver to compute position. This error was modelled according to [2], as a function of the S4 amplitude scintillation index measured by the GISTM receivers. An improvement of up to 21% in relative positioning accuracy was achieved with this technnique.
publishDate 2007
dc.date.none.fl_str_mv 2007-12-01
2014-05-27T11:22:39Z
2014-05-27T11:22:39Z
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/conferenceObject
format conferenceObject
status_str publishedVersion
dc.identifier.uri.fl_str_mv http://dx.doi.org/10.1109/ELMAR.2007.4418801
Proceedings Elmar - International Symposium Electronics in Marine, p. 63-67.
1334-2630
http://hdl.handle.net/11449/70014
10.1109/ELMAR.2007.4418801
2-s2.0-47349089389
7180879644760038
url http://dx.doi.org/10.1109/ELMAR.2007.4418801
http://hdl.handle.net/11449/70014
identifier_str_mv Proceedings Elmar - International Symposium Electronics in Marine, p. 63-67.
1334-2630
10.1109/ELMAR.2007.4418801
2-s2.0-47349089389
7180879644760038
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Proceedings Elmar - International Symposium Electronics in Marine
0,187
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv 63-67
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
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