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

dc.contributor.authorMoraes, Alison de O.
dc.contributor.authorVani, Bruno C. [UNESP]
dc.contributor.authorCosta, Emanoel
dc.contributor.authorSousasantos, Jonas
dc.contributor.authorAbdu, Mangalathayil A.
dc.contributor.authorRodrigues, Fabiano
dc.contributor.authorGladek, Yuri C.
dc.contributor.authorOliveira, Cesar B. A. de
dc.contributor.authorGalera Monico, Joao F. [UNESP]
dc.contributor.institutionInst Tecnol Aeronaut
dc.contributor.institutionInst Fed Educ Ciencia & Tecnol Sao Paulo Campus P
dc.contributor.institutionUniversidade Estadual Paulista (Unesp)
dc.contributor.institutionPontificia Univ Catolica Rio de Janeiro
dc.contributor.institutionInst Nacl Pesquisas Espaciais
dc.contributor.institutionUniv Texas Dallas
dc.contributor.institutionEMBRAER
dc.date.accessioned2019-10-04T12:31:31Z
dc.date.available2019-10-04T12:31:31Z
dc.date.issued2018-09-01
dc.description.abstractThe 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.en
dc.description.affiliationInst Tecnol Aeronaut, Inst Aeronaut & Espaco, Sao Jose Dos Campos, Brazil
dc.description.affiliationInst Fed Educ Ciencia & Tecnol Sao Paulo Campus P, Dept Informat, Presidente Epitacio, Brazil
dc.description.affiliationUniv Estadual Paulista, Dept Cartog, Presidente Epitacio, Brazil
dc.description.affiliationPontificia Univ Catolica Rio de Janeiro, Ctr Estudos Telecomunicacoes, Rio De Janeiro, Brazil
dc.description.affiliationInst Tecnol Aeronaut, Sao Jose Dos Campos, Brazil
dc.description.affiliationInst Nacl Pesquisas Espaciais, Inst Tecnol Aeronaut, Sao Jose Dos Campos, Brazil
dc.description.affiliationUniv Texas Dallas, William B Hanson Ctr Space Sci, Richardson, TX 75083 USA
dc.description.affiliationEMBRAER, Sao Jose Dos Campos, Brazil
dc.description.affiliationUnespUniv Estadual Paulista, Dept Cartog, Presidente Epitacio, Brazil
dc.description.sponsorshipConselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)
dc.description.sponsorshipFundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)
dc.description.sponsorshipCoordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)
dc.description.sponsorshipNSF
dc.description.sponsorshipEuropean Commission (EC)
dc.description.sponsorshipIdCNPq: 465648/2014-2
dc.description.sponsorshipIdFAPESP: 2017/50115-0
dc.description.sponsorshipIdFAPESP: 06/04008-2
dc.description.sponsorshipIdCNPq: 309013/2016-0
dc.description.sponsorshipIdNSF: AST-1547048
dc.description.sponsorshipIdEuropean Commission (EC): FP7-GALILEO-2009-GSA
dc.description.sponsorshipIdEuropean Commission (EC): FP7-GALILEO-2011-GSA-1a
dc.format.extent1165-1174
dc.identifierhttp://dx.doi.org/10.1029/2018RS006653
dc.identifier.citationRadio Science. Washington: Amer Geophysical Union, v. 53, n. 9, p. 1165-1174, 2018.
dc.identifier.doi10.1029/2018RS006653
dc.identifier.issn0048-6604
dc.identifier.urihttp://hdl.handle.net/11449/184969
dc.identifier.wosWOS:000447804600013
dc.language.isoeng
dc.publisherAmer Geophysical Union
dc.relation.ispartofRadio Science
dc.rights.accessRightsAcesso aberto
dc.sourceWeb of Science
dc.subjectionospheric scintillation
dc.subjectfading coefficients
dc.subjectGNSS availability
dc.titleIonospheric Scintillation Fading Coefficients for the GPS L1, L2, and L5 Frequenciesen
dc.typeArtigo
dcterms.rightsHolderAmer Geophysical Union
dspace.entity.typePublication
unesp.departmentCartografia - FCTpt

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