Ionospheric Scintillation Fading Coefficients for the GPS L1, L2, and L5 Frequencies

Detalhes bibliográficos
Autor(a) principal: Moraes, Alison de O.
Data de Publicação: 2018
Outros Autores: Vani, Bruno C. [UNESP], Costa, Emanoel, Sousasantos, Jonas, Abdu, Mangalathayil A., Rodrigues, Fabiano, Gladek, Yuri C., Oliveira, Cesar B. A. de, Galera Monico, Joao F. [UNESP]
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1029/2018RS006653
http://hdl.handle.net/11449/184969
Resumo: The terrestrial ionosphere over low-latitude regions presents the unique phenomena of the equatorial ionization anomaly (characterized by global maximum in plasma concentration) and plasma-depleted regions known as equatorial plasma bubbles and associated smaller-scale plasma irregularities. Transionospheric radio signals such as those from Global Navigation Satellite Systems constellations, traveling across this ambient, may suffer severe scintillation in amplitude and phase due to these plasma structures. Presently, three civilian signals available for GPS users, at L1 (1575.42MHz), L2C (1227.60MHz), and L5 (1176.45MHz) are used to investigate the propagation effects due to these irregularities. The purpose of the present work is to evaluate statistically the distribution of severe fade events for each of these carrier frequencies based on the nonlinear ionospheric propagation effects as represented by the fading coefficients of - distribution. The results from the analyses of data sets recorded by stations at different geomagnetic latitude locations in Brazil show that regions closer to the equatorial ionization anomaly crest present higher probability of severe fade events. Additionally, the L5 signals, dedicated for safety-of-life applications, revealed more unfavorable results when compared to the L1 and L2C frequencies. The results further showed that for 0.8S(4)1.0 the probabilities of fades deeper than -10dB were between 8.0% and 6.5% depending on the station position. Considering the case of fades deeper than -20dB, the results reach values near 1%, which is quite concerning. These results show empirically the fading environment that users of the new civilian signals may experience in low-latitude region. Additionally, the fading coefficients may help in the comprehension of the distribution of amplitude scintillation and its relation with the frequency used, aiding in the future the development of signal processing algorithms capable to mitigate errors for navigation users. This work shows differences in the statistics of GPS signals at different frequencies. The results warn that new signals will be more affected by the ionosphere in regions of low latitudes.
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spelling Ionospheric Scintillation Fading Coefficients for the GPS L1, L2, and L5 Frequenciesionospheric scintillationfading coefficientsGNSS availabilityThe terrestrial ionosphere over low-latitude regions presents the unique phenomena of the equatorial ionization anomaly (characterized by global maximum in plasma concentration) and plasma-depleted regions known as equatorial plasma bubbles and associated smaller-scale plasma irregularities. Transionospheric radio signals such as those from Global Navigation Satellite Systems constellations, traveling across this ambient, may suffer severe scintillation in amplitude and phase due to these plasma structures. Presently, three civilian signals available for GPS users, at L1 (1575.42MHz), L2C (1227.60MHz), and L5 (1176.45MHz) are used to investigate the propagation effects due to these irregularities. The purpose of the present work is to evaluate statistically the distribution of severe fade events for each of these carrier frequencies based on the nonlinear ionospheric propagation effects as represented by the fading coefficients of - distribution. The results from the analyses of data sets recorded by stations at different geomagnetic latitude locations in Brazil show that regions closer to the equatorial ionization anomaly crest present higher probability of severe fade events. Additionally, the L5 signals, dedicated for safety-of-life applications, revealed more unfavorable results when compared to the L1 and L2C frequencies. The results further showed that for 0.8S(4)1.0 the probabilities of fades deeper than -10dB were between 8.0% and 6.5% depending on the station position. Considering the case of fades deeper than -20dB, the results reach values near 1%, which is quite concerning. These results show empirically the fading environment that users of the new civilian signals may experience in low-latitude region. Additionally, the fading coefficients may help in the comprehension of the distribution of amplitude scintillation and its relation with the frequency used, aiding in the future the development of signal processing algorithms capable to mitigate errors for navigation users. This work shows differences in the statistics of GPS signals at different frequencies. The results warn that new signals will be more affected by the ionosphere in regions of low latitudes.Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)NSFEuropean Commission (EC)Inst Tecnol Aeronaut, Inst Aeronaut & Espaco, Sao Jose Dos Campos, BrazilInst Fed Educ Ciencia & Tecnol Sao Paulo Campus P, Dept Informat, Presidente Epitacio, BrazilUniv Estadual Paulista, Dept Cartog, Presidente Epitacio, BrazilPontificia Univ Catolica Rio de Janeiro, Ctr Estudos Telecomunicacoes, Rio De Janeiro, BrazilInst Tecnol Aeronaut, Sao Jose Dos Campos, BrazilInst Nacl Pesquisas Espaciais, Inst Tecnol Aeronaut, Sao Jose Dos Campos, BrazilUniv Texas Dallas, William B Hanson Ctr Space Sci, Richardson, TX 75083 USAEMBRAER, Sao Jose Dos Campos, BrazilUniv Estadual Paulista, Dept Cartog, Presidente Epitacio, BrazilCNPq: 465648/2014-2FAPESP: 2017/50115-0FAPESP: 06/04008-2CNPq: 309013/2016-0NSF: AST-1547048European Commission (EC): FP7-GALILEO-2009-GSAEuropean Commission (EC): FP7-GALILEO-2011-GSA-1aAmer Geophysical UnionInst Tecnol AeronautInst Fed Educ Ciencia & Tecnol Sao Paulo Campus PUniversidade Estadual Paulista (Unesp)Pontificia Univ Catolica Rio de JaneiroInst Nacl Pesquisas EspaciaisUniv Texas DallasEMBRAERMoraes, Alison de O.Vani, Bruno C. [UNESP]Costa, EmanoelSousasantos, JonasAbdu, Mangalathayil A.Rodrigues, FabianoGladek, Yuri C.Oliveira, Cesar B. A. deGalera Monico, Joao F. [UNESP]2019-10-04T12:31:31Z2019-10-04T12:31:31Z2018-09-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article1165-1174http://dx.doi.org/10.1029/2018RS006653Radio Science. Washington: Amer Geophysical Union, v. 53, n. 9, p. 1165-1174, 2018.0048-6604http://hdl.handle.net/11449/18496910.1029/2018RS006653WOS:000447804600013Web of Sciencereponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengRadio Scienceinfo:eu-repo/semantics/openAccess2024-06-18T15:01:04Zoai:repositorio.unesp.br:11449/184969Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T14:14:53.557288Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Ionospheric Scintillation Fading Coefficients for the GPS L1, L2, and L5 Frequencies
title Ionospheric Scintillation Fading Coefficients for the GPS L1, L2, and L5 Frequencies
spellingShingle Ionospheric Scintillation Fading Coefficients for the GPS L1, L2, and L5 Frequencies
Moraes, Alison de O.
ionospheric scintillation
fading coefficients
GNSS availability
title_short Ionospheric Scintillation Fading Coefficients for the GPS L1, L2, and L5 Frequencies
title_full Ionospheric Scintillation Fading Coefficients for the GPS L1, L2, and L5 Frequencies
title_fullStr Ionospheric Scintillation Fading Coefficients for the GPS L1, L2, and L5 Frequencies
title_full_unstemmed Ionospheric Scintillation Fading Coefficients for the GPS L1, L2, and L5 Frequencies
title_sort Ionospheric Scintillation Fading Coefficients for the GPS L1, L2, and L5 Frequencies
author Moraes, Alison de O.
author_facet Moraes, Alison de O.
Vani, Bruno C. [UNESP]
Costa, Emanoel
Sousasantos, Jonas
Abdu, Mangalathayil A.
Rodrigues, Fabiano
Gladek, Yuri C.
Oliveira, Cesar B. A. de
Galera Monico, Joao F. [UNESP]
author_role author
author2 Vani, Bruno C. [UNESP]
Costa, Emanoel
Sousasantos, Jonas
Abdu, Mangalathayil A.
Rodrigues, Fabiano
Gladek, Yuri C.
Oliveira, Cesar B. A. de
Galera Monico, Joao F. [UNESP]
author2_role author
author
author
author
author
author
author
author
dc.contributor.none.fl_str_mv Inst Tecnol Aeronaut
Inst Fed Educ Ciencia & Tecnol Sao Paulo Campus P
Universidade Estadual Paulista (Unesp)
Pontificia Univ Catolica Rio de Janeiro
Inst Nacl Pesquisas Espaciais
Univ Texas Dallas
EMBRAER
dc.contributor.author.fl_str_mv Moraes, Alison de O.
Vani, Bruno C. [UNESP]
Costa, Emanoel
Sousasantos, Jonas
Abdu, Mangalathayil A.
Rodrigues, Fabiano
Gladek, Yuri C.
Oliveira, Cesar B. A. de
Galera Monico, Joao F. [UNESP]
dc.subject.por.fl_str_mv ionospheric scintillation
fading coefficients
GNSS availability
topic ionospheric scintillation
fading coefficients
GNSS availability
description The terrestrial ionosphere over low-latitude regions presents the unique phenomena of the equatorial ionization anomaly (characterized by global maximum in plasma concentration) and plasma-depleted regions known as equatorial plasma bubbles and associated smaller-scale plasma irregularities. Transionospheric radio signals such as those from Global Navigation Satellite Systems constellations, traveling across this ambient, may suffer severe scintillation in amplitude and phase due to these plasma structures. Presently, three civilian signals available for GPS users, at L1 (1575.42MHz), L2C (1227.60MHz), and L5 (1176.45MHz) are used to investigate the propagation effects due to these irregularities. The purpose of the present work is to evaluate statistically the distribution of severe fade events for each of these carrier frequencies based on the nonlinear ionospheric propagation effects as represented by the fading coefficients of - distribution. The results from the analyses of data sets recorded by stations at different geomagnetic latitude locations in Brazil show that regions closer to the equatorial ionization anomaly crest present higher probability of severe fade events. Additionally, the L5 signals, dedicated for safety-of-life applications, revealed more unfavorable results when compared to the L1 and L2C frequencies. The results further showed that for 0.8S(4)1.0 the probabilities of fades deeper than -10dB were between 8.0% and 6.5% depending on the station position. Considering the case of fades deeper than -20dB, the results reach values near 1%, which is quite concerning. These results show empirically the fading environment that users of the new civilian signals may experience in low-latitude region. Additionally, the fading coefficients may help in the comprehension of the distribution of amplitude scintillation and its relation with the frequency used, aiding in the future the development of signal processing algorithms capable to mitigate errors for navigation users. This work shows differences in the statistics of GPS signals at different frequencies. The results warn that new signals will be more affected by the ionosphere in regions of low latitudes.
publishDate 2018
dc.date.none.fl_str_mv 2018-09-01
2019-10-04T12:31:31Z
2019-10-04T12:31:31Z
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/10.1029/2018RS006653
Radio Science. Washington: Amer Geophysical Union, v. 53, n. 9, p. 1165-1174, 2018.
0048-6604
http://hdl.handle.net/11449/184969
10.1029/2018RS006653
WOS:000447804600013
url http://dx.doi.org/10.1029/2018RS006653
http://hdl.handle.net/11449/184969
identifier_str_mv Radio Science. Washington: Amer Geophysical Union, v. 53, n. 9, p. 1165-1174, 2018.
0048-6604
10.1029/2018RS006653
WOS:000447804600013
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Radio Science
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv 1165-1174
dc.publisher.none.fl_str_mv Amer Geophysical Union
publisher.none.fl_str_mv Amer Geophysical Union
dc.source.none.fl_str_mv Web of Science
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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