Numerical simulations to assess ART and MART performance for ionospheric tomography of chapman profiles
Autor(a) principal: | |
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Data de Publicação: | 2017 |
Outros Autores: | , |
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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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/openAccess2024-06-18T15:01:52Zoai:repositorio.unesp.br:11449/175259Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T21:29:10.333674Repositório 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 |
|
_version_ |
1808129325610827776 |