Ionospheric Scintillation Fading Coefficients for the GPS L1, L2, and L5 Frequencies
Autor(a) principal: | |
---|---|
Data de Publicação: | 2018 |
Outros Autores: | , , , , , , , |
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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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 |
|
_version_ |
1808128336165076992 |