Numerical simulations to assess ART and MART performance for ionospheric tomography of chapman profiles

Detalhes bibliográficos
Autor(a) principal: Prol, Fabricio dos Santos [UNESP]
Data de Publicação: 2017
Outros Autores: Camargo, Paulo O. [UNESP], Muella, Marcio T. A. H.
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1590/0001-3765201720170116
http://hdl.handle.net/11449/175259
Resumo: The incomplete geometrical coverage of the Global Navigation Satellite System (GNSS) makes the ionospheric tomographic system an ill-conditioned problem for ionospheric imaging. In order to detect the principal limitations of the ill-conditioned tomographic solutions, numerical simulations of the ionosphere are under constant investigation. In this paper, we show an investigation of the accuracy of Algebraic Reconstruction Technique (ART) and Multiplicative ART (MART) for performing tomographic reconstruction of Chapman profiles using a simulated optimum scenario of GNSS signals tracked by ground-based receivers. Chapman functions were used to represent the ionospheric morphology and a set of analyses was conducted to assess ART and MART performance for estimating the Total Electron Content (TEC) and parameters that describes the Chapman function. The results showed that MART performed better in the reconstruction of the electron density peak and ART gave a better representation for estimating TEC and the shape of the ionosphere. Since we used an optimum scenario of the GNSS signals, the analyses indicate the intrinsic problems that may occur with ART and MART to recover valuable information for many applications of Telecommunication, Spatial Geodesy and Space Weather.
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spelling Numerical simulations to assess ART and MART performance for ionospheric tomography of chapman profilesChapman functionElectron densityGNSSGrid-based tomographyIonospheric profileTECThe incomplete geometrical coverage of the Global Navigation Satellite System (GNSS) makes the ionospheric tomographic system an ill-conditioned problem for ionospheric imaging. In order to detect the principal limitations of the ill-conditioned tomographic solutions, numerical simulations of the ionosphere are under constant investigation. In this paper, we show an investigation of the accuracy of Algebraic Reconstruction Technique (ART) and Multiplicative ART (MART) for performing tomographic reconstruction of Chapman profiles using a simulated optimum scenario of GNSS signals tracked by ground-based receivers. Chapman functions were used to represent the ionospheric morphology and a set of analyses was conducted to assess ART and MART performance for estimating the Total Electron Content (TEC) and parameters that describes the Chapman function. The results showed that MART performed better in the reconstruction of the electron density peak and ART gave a better representation for estimating TEC and the shape of the ionosphere. Since we used an optimum scenario of the GNSS signals, the analyses indicate the intrinsic problems that may occur with ART and MART to recover valuable information for many applications of Telecommunication, Spatial Geodesy and Space Weather.Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)Universidade Estadual Paulista/UNESP Departamento de Cartografia, Rua Roberto Simonsen, 305Universidade do Vale do Paraíba/UNIVAP Laboratório de Física e Astronomia - IP&D, Rua Shishima Hifumi, 2911Universidade Estadual Paulista/UNESP Departamento de Cartografia, Rua Roberto Simonsen, 305CNPq: 2014/09240-7FAPESP: 2015/15027-7Universidade Estadual Paulista (Unesp)Laboratório de Física e Astronomia - IP&DProl, Fabricio dos Santos [UNESP]Camargo, Paulo O. [UNESP]Muella, Marcio T. A. H.2018-12-11T17:15:02Z2018-12-11T17:15:02Z2017-07-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article1531-1542application/pdfhttp://dx.doi.org/10.1590/0001-3765201720170116Anais da Academia Brasileira de Ciencias, v. 89, n. 3, p. 1531-1542, 2017.1678-26900001-3765http://hdl.handle.net/11449/17525910.1590/0001-3765201720170116S0001-376520170004015312-s2.0-85029922175S0001-37652017000401531.pdfScopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengAnais da Academia Brasileira de Ciencias0,4180,418info:eu-repo/semantics/openAccess2023-12-28T06:14:27Zoai:repositorio.unesp.br:11449/175259Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462023-12-28T06:14:27Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Numerical simulations to assess ART and MART performance for ionospheric tomography of chapman profiles
title Numerical simulations to assess ART and MART performance for ionospheric tomography of chapman profiles
spellingShingle Numerical simulations to assess ART and MART performance for ionospheric tomography of chapman profiles
Prol, Fabricio dos Santos [UNESP]
Chapman function
Electron density
GNSS
Grid-based tomography
Ionospheric profile
TEC
title_short Numerical simulations to assess ART and MART performance for ionospheric tomography of chapman profiles
title_full Numerical simulations to assess ART and MART performance for ionospheric tomography of chapman profiles
title_fullStr Numerical simulations to assess ART and MART performance for ionospheric tomography of chapman profiles
title_full_unstemmed Numerical simulations to assess ART and MART performance for ionospheric tomography of chapman profiles
title_sort Numerical simulations to assess ART and MART performance for ionospheric tomography of chapman profiles
author Prol, Fabricio dos Santos [UNESP]
author_facet Prol, Fabricio dos Santos [UNESP]
Camargo, Paulo O. [UNESP]
Muella, Marcio T. A. H.
author_role author
author2 Camargo, Paulo O. [UNESP]
Muella, Marcio T. A. H.
author2_role author
author
dc.contributor.none.fl_str_mv Universidade Estadual Paulista (Unesp)
Laboratório de Física e Astronomia - IP&D
dc.contributor.author.fl_str_mv Prol, Fabricio dos Santos [UNESP]
Camargo, Paulo O. [UNESP]
Muella, Marcio T. A. H.
dc.subject.por.fl_str_mv Chapman function
Electron density
GNSS
Grid-based tomography
Ionospheric profile
TEC
topic Chapman function
Electron density
GNSS
Grid-based tomography
Ionospheric profile
TEC
description The incomplete geometrical coverage of the Global Navigation Satellite System (GNSS) makes the ionospheric tomographic system an ill-conditioned problem for ionospheric imaging. In order to detect the principal limitations of the ill-conditioned tomographic solutions, numerical simulations of the ionosphere are under constant investigation. In this paper, we show an investigation of the accuracy of Algebraic Reconstruction Technique (ART) and Multiplicative ART (MART) for performing tomographic reconstruction of Chapman profiles using a simulated optimum scenario of GNSS signals tracked by ground-based receivers. Chapman functions were used to represent the ionospheric morphology and a set of analyses was conducted to assess ART and MART performance for estimating the Total Electron Content (TEC) and parameters that describes the Chapman function. The results showed that MART performed better in the reconstruction of the electron density peak and ART gave a better representation for estimating TEC and the shape of the ionosphere. Since we used an optimum scenario of the GNSS signals, the analyses indicate the intrinsic problems that may occur with ART and MART to recover valuable information for many applications of Telecommunication, Spatial Geodesy and Space Weather.
publishDate 2017
dc.date.none.fl_str_mv 2017-07-01
2018-12-11T17:15:02Z
2018-12-11T17:15:02Z
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/10.1590/0001-3765201720170116
Anais da Academia Brasileira de Ciencias, v. 89, n. 3, p. 1531-1542, 2017.
1678-2690
0001-3765
http://hdl.handle.net/11449/175259
10.1590/0001-3765201720170116
S0001-37652017000401531
2-s2.0-85029922175
S0001-37652017000401531.pdf
url http://dx.doi.org/10.1590/0001-3765201720170116
http://hdl.handle.net/11449/175259
identifier_str_mv Anais da Academia Brasileira de Ciencias, v. 89, n. 3, p. 1531-1542, 2017.
1678-2690
0001-3765
10.1590/0001-3765201720170116
S0001-37652017000401531
2-s2.0-85029922175
S0001-37652017000401531.pdf
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Anais da Academia Brasileira de Ciencias
0,418
0,418
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv 1531-1542
application/pdf
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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