Ionospheric TEC Weather Map Over South America

Detalhes bibliográficos
Autor(a) principal: Takahashi, H.
Data de Publicação: 2016
Outros Autores: Wrasse, C. M., Denardini, C. M., Padua, M. B., Paula, E. R. de, Costa, S. M. A., Otsuka, Y., Shiokawa, K., Galera Monico, J. F. [UNESP], Ivo, A., Sant'Anna, N.
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1002/2016SW001474
http://hdl.handle.net/11449/162284
Resumo: Ionospheric weather maps using the total electron content (TEC) monitored by ground-based Global Navigation Satellite Systems (GNSS) receivers over South American continent, TECMAP, have been operationally produced by Instituto Nacional de Pesquisas Espaciais's Space Weather Study and Monitoring Program (Estudo e Monitoramento Brasileiro de Clima Especial) since 2013. In order to cover the whole continent, four GNSS receiver networks, (Rede Brasileiro de Monitoramento Continuo) RBMC/Brazilian Institute for Geography and Statistics, Low-latitude Ionospheric Sensor Network, International GNSS Service, and Red Argentina de Monitoreo Satelital Continuo, in total similar to 140 sites, have been used. TECMAPs with a time resolution of 10min are produced in 12h time delay. Spatial resolution of the map is rather low, varying between 50 and 500km depending on the density of the observation points. Large day-to-day variabilities of the equatorial ionization anomaly have been observed. Spatial gradient of TEC from the anomaly trough (total electron content unit, 1TECU=10(16)elm(-2) (TECU) <10) to the crest region (TECU>80) causes a large ionospheric range delay in the GNSS positioning system. Ionospheric plasma bubbles, their seeding and development, could be monitored. This plasma density (spatial and temporal) variability causes not only the GNSS-based positioning error but also radio wave scintillations. Monitoring of these phenomena by TEC mapping becomes an important issue for space weather concern for high-technology positioning system and telecommunication.
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spelling Ionospheric TEC Weather Map Over South Americaionospheric weatherTEC mappingplasma bubblesGNSS positioningIonospheric weather maps using the total electron content (TEC) monitored by ground-based Global Navigation Satellite Systems (GNSS) receivers over South American continent, TECMAP, have been operationally produced by Instituto Nacional de Pesquisas Espaciais's Space Weather Study and Monitoring Program (Estudo e Monitoramento Brasileiro de Clima Especial) since 2013. In order to cover the whole continent, four GNSS receiver networks, (Rede Brasileiro de Monitoramento Continuo) RBMC/Brazilian Institute for Geography and Statistics, Low-latitude Ionospheric Sensor Network, International GNSS Service, and Red Argentina de Monitoreo Satelital Continuo, in total similar to 140 sites, have been used. TECMAPs with a time resolution of 10min are produced in 12h time delay. Spatial resolution of the map is rather low, varying between 50 and 500km depending on the density of the observation points. Large day-to-day variabilities of the equatorial ionization anomaly have been observed. Spatial gradient of TEC from the anomaly trough (total electron content unit, 1TECU=10(16)elm(-2) (TECU) <10) to the crest region (TECU>80) causes a large ionospheric range delay in the GNSS positioning system. Ionospheric plasma bubbles, their seeding and development, could be monitored. This plasma density (spatial and temporal) variability causes not only the GNSS-based positioning error but also radio wave scintillations. Monitoring of these phenomena by TEC mapping becomes an important issue for space weather concern for high-technology positioning system and telecommunication.Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)JSPS KAKENHIInst Nacl Pesquisas Espaciais, EMBRACE, Sao Jose Dos Campos, BrazilInst Brasileiro Geog & Estat, GRRP CGED, Rio De Janeiro, BrazilNagoya Univ, Inst Space Earth Environm Res, Nagoya, Aichi, JapanUniv Estadual Paulista, Dept Cartog, Presidente Prudente, BrazilUniv Estadual Paulista, Dept Cartog, Presidente Prudente, BrazilCNPq: 30.5461/2015-0CNPq: 310802/2015-6CNPq: 303121/2014-9FAPESP: 2012/08445-9JSPS KAKENHI: 15H05815Amer Geophysical UnionInst Nacl Pesquisas EspaciaisInst Brasileiro Geog & EstatNagoya UnivUniversidade Estadual Paulista (Unesp)Takahashi, H.Wrasse, C. M.Denardini, C. M.Padua, M. B.Paula, E. R. deCosta, S. M. A.Otsuka, Y.Shiokawa, K.Galera Monico, J. F. [UNESP]Ivo, A.Sant'Anna, N.2018-11-26T17:15:28Z2018-11-26T17:15:28Z2016-11-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article937-949application/pdfhttp://dx.doi.org/10.1002/2016SW001474Space Weather-the International Journal Of Research And Applications. Washington: Amer Geophysical Union, v. 14, n. 11, p. 937-949, 2016.1542-7390http://hdl.handle.net/11449/16228410.1002/2016SW001474WOS:000390647400004WOS000390647400004.pdfWeb of Sciencereponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengSpace Weather-the International Journal Of Research And Applicationsinfo:eu-repo/semantics/openAccess2024-06-18T15:01:38Zoai:repositorio.unesp.br:11449/162284Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T18:46:45.724400Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Ionospheric TEC Weather Map Over South America
title Ionospheric TEC Weather Map Over South America
spellingShingle Ionospheric TEC Weather Map Over South America
Takahashi, H.
ionospheric weather
TEC mapping
plasma bubbles
GNSS positioning
title_short Ionospheric TEC Weather Map Over South America
title_full Ionospheric TEC Weather Map Over South America
title_fullStr Ionospheric TEC Weather Map Over South America
title_full_unstemmed Ionospheric TEC Weather Map Over South America
title_sort Ionospheric TEC Weather Map Over South America
author Takahashi, H.
author_facet Takahashi, H.
Wrasse, C. M.
Denardini, C. M.
Padua, M. B.
Paula, E. R. de
Costa, S. M. A.
Otsuka, Y.
Shiokawa, K.
Galera Monico, J. F. [UNESP]
Ivo, A.
Sant'Anna, N.
author_role author
author2 Wrasse, C. M.
Denardini, C. M.
Padua, M. B.
Paula, E. R. de
Costa, S. M. A.
Otsuka, Y.
Shiokawa, K.
Galera Monico, J. F. [UNESP]
Ivo, A.
Sant'Anna, N.
author2_role author
author
author
author
author
author
author
author
author
author
dc.contributor.none.fl_str_mv Inst Nacl Pesquisas Espaciais
Inst Brasileiro Geog & Estat
Nagoya Univ
Universidade Estadual Paulista (Unesp)
dc.contributor.author.fl_str_mv Takahashi, H.
Wrasse, C. M.
Denardini, C. M.
Padua, M. B.
Paula, E. R. de
Costa, S. M. A.
Otsuka, Y.
Shiokawa, K.
Galera Monico, J. F. [UNESP]
Ivo, A.
Sant'Anna, N.
dc.subject.por.fl_str_mv ionospheric weather
TEC mapping
plasma bubbles
GNSS positioning
topic ionospheric weather
TEC mapping
plasma bubbles
GNSS positioning
description Ionospheric weather maps using the total electron content (TEC) monitored by ground-based Global Navigation Satellite Systems (GNSS) receivers over South American continent, TECMAP, have been operationally produced by Instituto Nacional de Pesquisas Espaciais's Space Weather Study and Monitoring Program (Estudo e Monitoramento Brasileiro de Clima Especial) since 2013. In order to cover the whole continent, four GNSS receiver networks, (Rede Brasileiro de Monitoramento Continuo) RBMC/Brazilian Institute for Geography and Statistics, Low-latitude Ionospheric Sensor Network, International GNSS Service, and Red Argentina de Monitoreo Satelital Continuo, in total similar to 140 sites, have been used. TECMAPs with a time resolution of 10min are produced in 12h time delay. Spatial resolution of the map is rather low, varying between 50 and 500km depending on the density of the observation points. Large day-to-day variabilities of the equatorial ionization anomaly have been observed. Spatial gradient of TEC from the anomaly trough (total electron content unit, 1TECU=10(16)elm(-2) (TECU) <10) to the crest region (TECU>80) causes a large ionospheric range delay in the GNSS positioning system. Ionospheric plasma bubbles, their seeding and development, could be monitored. This plasma density (spatial and temporal) variability causes not only the GNSS-based positioning error but also radio wave scintillations. Monitoring of these phenomena by TEC mapping becomes an important issue for space weather concern for high-technology positioning system and telecommunication.
publishDate 2016
dc.date.none.fl_str_mv 2016-11-01
2018-11-26T17:15:28Z
2018-11-26T17:15:28Z
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/10.1002/2016SW001474
Space Weather-the International Journal Of Research And Applications. Washington: Amer Geophysical Union, v. 14, n. 11, p. 937-949, 2016.
1542-7390
http://hdl.handle.net/11449/162284
10.1002/2016SW001474
WOS:000390647400004
WOS000390647400004.pdf
url http://dx.doi.org/10.1002/2016SW001474
http://hdl.handle.net/11449/162284
identifier_str_mv Space Weather-the International Journal Of Research And Applications. Washington: Amer Geophysical Union, v. 14, n. 11, p. 937-949, 2016.
1542-7390
10.1002/2016SW001474
WOS:000390647400004
WOS000390647400004.pdf
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Space Weather-the International Journal Of Research And Applications
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv 937-949
application/pdf
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
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