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1. Identificação
Tipo de ReferênciaArtigo em Revista Científica (Journal Article)
Sitemtc-m21c.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador8JMKD3MGP3W34R/44E938S
Repositóriosid.inpe.br/mtc-m21c/2021/04.01.15.13   (acesso restrito)
Última Atualização2021:04.01.15.13.25 (UTC) simone
Repositório de Metadadossid.inpe.br/mtc-m21c/2021/04.01.15.13.25
Última Atualização dos Metadados2022:04.03.23.14.29 (UTC) administrator
DOI10.1029/2020EA001314
ISSN2333-5084
Chave de CitaçãoPaulaMMCCDGVCARAWBS:2021:Pe6Di
TítuloPerformance of 6 Different Global Navigation Satellite System Receivers at Low Latitude Under Moderate and Strong Scintillation
Ano2021
MêsFeb.
Data de Acesso07 fev. 2023
Tipo de Trabalhojournal article
Tipo SecundárioPRE PI
Número de Arquivos1
Tamanho7617 KiB
2. Contextualização
Autor 1 Paula, Eurico Rodrigues de
 2 Martinon, André Ricardo Fazanaro
 3 Moraes, A. O.
 4 Carrano, C.
 5 Cunha Neto, Acacio
 6 Doherty, P.
 7 Groves, K.
 8 Valladares, C. E.
 9 Crowley, G.
10 Azeem, I.
11 Reynolds, A.
12 Akos, D. M.
13 Walter, T.
14 Beach, T. L.
15 Slewaegen, J. M.
Identificador de Curriculo 1 8JMKD3MGP5W/3C9JH2U
ORCID 1 0000-0003-2756-3826
 2 0000-0002-6578-0170
 3 0000-0002-6493-1694
 4 0000-0003-1317-2453
 5
 6 0000-0002-3040-4511
 7 0000-0002-2067-1579
 8
 9
10 0000-0002-8928-9837
11 0000-0002-9259-0890
12
13 0000-0002-3257-3175
Grupo 1 DIHPA-CGCE-INPE-MCTI-GOV-BR
 2 COPDT-CGIP-INPE-MCTI-GOV-BR
 3
 4
 5 DIHPA-CGCE-INPE-MCTI-GOV-BR
Afiliação 1 Instituto Nacional de Pesquisas Espaciais (INPE)
 2 Instituto Nacional de Pesquisas Espaciais (INPE)
 3 Instituto de Aeronáutica e Espaço (IAE)
 4 Boston College
 5 Instituto Nacional de Pesquisas Espaciais (INPE)
 6 Boston College
 7 Boston College
 8 Univerity of Texas at Dallas
 9 Atmospheric & Space Technology Research Associates (ASTRA)
10 Atmospheric & Space Technology Research Associates (ASTRA)
11 Atmospheric & Space Technology Research Associates (ASTRA)
12 Stanford University
13 Stanford University
14 Creare L. L. C.
15 Septentrio
Endereço de e-Mail do Autor 1 eurico.paula@inpe.br
 2 andre.martinon@inpe.br
 3
 4
 5 acacio.cunha@inpe.br
RevistaEarth and Space Science
Volume8
Número2
Páginase2020EA001314
Histórico (UTC)2021-04-01 15:15:45 :: simone -> administrator :: 2021
2022-04-03 23:14:29 :: administrator -> simone :: 2021
3. Conteúdo e estrutura
É a matriz ou uma cópia?é a matriz
Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
Tipo de Versãopublisher
Palavras-Chaveamplitude and phase scintillation indexes
GNSS receiver performance
ionospheric irregularities
ionospheric scintillation
scintillation monitor
ResumoAfter sunset, in the equatorial regions ionospheric plasma irregularities are generated due to the generalized Rayleigh-Taylor instability. Under favorable conditions these irregularities develop in the equatorial region while mapping along the magnetic field lines giving rise to large plasma depletion structures called Equatorial Plasma Bubbles with embedded smaller structures on their walls. The global navigation satellite system (GNSS) L1 band frequency is sensitive to irregularities of the size of 300-400 m in the first Fresnel zone, which cause scattering and diffraction of the signal and produce amplitude and/or phase scintillation. Severe scintillation of GNSS signals can in turn cause loss of lock of the receiver code and/or carrier loops. As a result, GNSS navigation and positioning solution can be adversely affected by the ionospheric scintillation. There are multiple GNSS receivers designed to monitor scintillations. These receivers are based on different hardware designs and use different methodologies to process the raw data. When using simultaneous data from different GNSS scintillation monitors it is important to evaluate and compare their performances under similar scintillation conditions. The scintillation monitoring techniques may be useful for many applications that use GNSS signal. The aim of this work is to evaluate the performance of six different GNSS receivers located at Sao Jose dos Campos (23.1 degrees S, 45.8 degrees W, dip latitude 17.3 degrees S) during moderate and strong scintillation activity. The amplitude (S-4) and phase (sigma(phi)) scintillation indexes from these receivers were analyzed and compared for the nights February 20-21 and November 27-28, 2013.
ÁreaCEA
Arranjo 1urlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > Performance of 6...
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Conteúdo da Pasta docacessar
Conteúdo da Pasta sourcenão têm arquivos
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4. Condições de acesso e uso
Idiomaen
Arquivo Alvopaula_performance.pdf
Grupo de Usuáriossimone
Grupo de Leitoresadministrator
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Visibilidadeshown
Permissão de Leituradeny from all and allow from 150.163
Permissão de Atualizaçãonão transferida
5. Fontes relacionadas
Unidades Imediatamente Superiores8JMKD3MGPCW/46KTFK8
8JMKD3MGPCW/46KUES5
DivulgaçãoWEBSCI; PORTALCAPES; SCOPUS.
Acervo Hospedeirourlib.net/www/2017/11.22.19.04
6. Notas
Campos Vaziosalternatejournal archivingpolicy archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn label lineage mark mirrorrepository nextedition notes parameterlist parentrepositories previousedition previouslowerunit progress project rightsholder secondarydate secondarykey secondarymark session shorttitle sponsor subject tertiarymark tertiarytype url
7. Controle da descrição
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