GPS positioning in the Brazilian region during intense magnetic storm of the October, 29 2003
Autor(a) principal: | |
---|---|
Data de Publicação: | 2008 |
Outros Autores: | , |
Tipo de documento: | Artigo |
Idioma: | por |
Título da fonte: | Repositório Institucional da UNESP |
Texto Completo: | http://dx.doi.org/10.22456/1807-9806.17891 http://hdl.handle.net/11449/249104 |
Resumo: | The error due to the ionosphere in the GPS observables depends on the Total Electron Content (TEC) in the ionospheric layer. The TEC varies regularly in time and space in relation to the sunspot number, the season, the local time, the geographic position, and others. However, the TEC can suffer abrupt modifications in its behavior due to the occurrence of intense magnetic storm. On 28 October 2003, at 1110 UT, a major solar flare took place from a sunspot directly in line with the Earth. A coronal mass ejection was observed to leave the Sun in the direction of the Earth, causing an intense magnetic storm that started at 0611 UT of the following day. In this paper, GPS data from RBMC and IGS network and Digisonde data were used, to analyze the influence of the intense magnetic storm that occurred on October 29, 2003 in the behavior of TEC and in the performance of the point positioning in the Brazilian region. |
id |
UNSP_64addce84d73ee5b687d70a99d284f94 |
---|---|
oai_identifier_str |
oai:repositorio.unesp.br:11449/249104 |
network_acronym_str |
UNSP |
network_name_str |
Repositório Institucional da UNESP |
repository_id_str |
2946 |
spelling |
GPS positioning in the Brazilian region during intense magnetic storm of the October, 29 2003Posicionamento por GPS na Região Brasileira Durante a Intensa Tempestade Geomagnética de 29 de Outubro de 2003Geomagnetic StormGlobal Positioning SystemTECThe error due to the ionosphere in the GPS observables depends on the Total Electron Content (TEC) in the ionospheric layer. The TEC varies regularly in time and space in relation to the sunspot number, the season, the local time, the geographic position, and others. However, the TEC can suffer abrupt modifications in its behavior due to the occurrence of intense magnetic storm. On 28 October 2003, at 1110 UT, a major solar flare took place from a sunspot directly in line with the Earth. A coronal mass ejection was observed to leave the Sun in the direction of the Earth, causing an intense magnetic storm that started at 0611 UT of the following day. In this paper, GPS data from RBMC and IGS network and Digisonde data were used, to analyze the influence of the intense magnetic storm that occurred on October 29, 2003 in the behavior of TEC and in the performance of the point positioning in the Brazilian region.Instituto de Geociências Universidade Federal do Rio Grande do Sul, Cx. Postal 15001, RSUniversidade Estadual Paulista, SPInstituto Nacional de Pesquisas Espaciais, SPUniversidade Estadual Paulista, SPUniversidade Federal do Rio Grande do SulUniversidade Estadual Paulista (UNESP)Instituto Nacional de Pesquisas EspaciaisMatsuoka, Marcelo TomioCamargo, PAULO DE OLIVEIRA [UNESP]Batista, Inez Staciarini2023-07-29T14:02:35Z2023-07-29T14:02:35Z2008-07-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article3-19http://dx.doi.org/10.22456/1807-9806.17891Pesquisas em Geociencias, v. 35, n. 1, p. 3-19, 2008.1807-98061518-2398http://hdl.handle.net/11449/24910410.22456/1807-9806.178912-s2.0-70350028822Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPporPesquisas em Geocienciasinfo:eu-repo/semantics/openAccess2024-06-18T15:01:53Zoai:repositorio.unesp.br:11449/249104Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T22:19:47.023557Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false |
dc.title.none.fl_str_mv |
GPS positioning in the Brazilian region during intense magnetic storm of the October, 29 2003 Posicionamento por GPS na Região Brasileira Durante a Intensa Tempestade Geomagnética de 29 de Outubro de 2003 |
title |
GPS positioning in the Brazilian region during intense magnetic storm of the October, 29 2003 |
spellingShingle |
GPS positioning in the Brazilian region during intense magnetic storm of the October, 29 2003 Matsuoka, Marcelo Tomio Geomagnetic Storm Global Positioning System TEC |
title_short |
GPS positioning in the Brazilian region during intense magnetic storm of the October, 29 2003 |
title_full |
GPS positioning in the Brazilian region during intense magnetic storm of the October, 29 2003 |
title_fullStr |
GPS positioning in the Brazilian region during intense magnetic storm of the October, 29 2003 |
title_full_unstemmed |
GPS positioning in the Brazilian region during intense magnetic storm of the October, 29 2003 |
title_sort |
GPS positioning in the Brazilian region during intense magnetic storm of the October, 29 2003 |
author |
Matsuoka, Marcelo Tomio |
author_facet |
Matsuoka, Marcelo Tomio Camargo, PAULO DE OLIVEIRA [UNESP] Batista, Inez Staciarini |
author_role |
author |
author2 |
Camargo, PAULO DE OLIVEIRA [UNESP] Batista, Inez Staciarini |
author2_role |
author author |
dc.contributor.none.fl_str_mv |
Universidade Federal do Rio Grande do Sul Universidade Estadual Paulista (UNESP) Instituto Nacional de Pesquisas Espaciais |
dc.contributor.author.fl_str_mv |
Matsuoka, Marcelo Tomio Camargo, PAULO DE OLIVEIRA [UNESP] Batista, Inez Staciarini |
dc.subject.por.fl_str_mv |
Geomagnetic Storm Global Positioning System TEC |
topic |
Geomagnetic Storm Global Positioning System TEC |
description |
The error due to the ionosphere in the GPS observables depends on the Total Electron Content (TEC) in the ionospheric layer. The TEC varies regularly in time and space in relation to the sunspot number, the season, the local time, the geographic position, and others. However, the TEC can suffer abrupt modifications in its behavior due to the occurrence of intense magnetic storm. On 28 October 2003, at 1110 UT, a major solar flare took place from a sunspot directly in line with the Earth. A coronal mass ejection was observed to leave the Sun in the direction of the Earth, causing an intense magnetic storm that started at 0611 UT of the following day. In this paper, GPS data from RBMC and IGS network and Digisonde data were used, to analyze the influence of the intense magnetic storm that occurred on October 29, 2003 in the behavior of TEC and in the performance of the point positioning in the Brazilian region. |
publishDate |
2008 |
dc.date.none.fl_str_mv |
2008-07-01 2023-07-29T14:02:35Z 2023-07-29T14:02:35Z |
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/10.22456/1807-9806.17891 Pesquisas em Geociencias, v. 35, n. 1, p. 3-19, 2008. 1807-9806 1518-2398 http://hdl.handle.net/11449/249104 10.22456/1807-9806.17891 2-s2.0-70350028822 |
url |
http://dx.doi.org/10.22456/1807-9806.17891 http://hdl.handle.net/11449/249104 |
identifier_str_mv |
Pesquisas em Geociencias, v. 35, n. 1, p. 3-19, 2008. 1807-9806 1518-2398 10.22456/1807-9806.17891 2-s2.0-70350028822 |
dc.language.iso.fl_str_mv |
por |
language |
por |
dc.relation.none.fl_str_mv |
Pesquisas em Geociencias |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.format.none.fl_str_mv |
3-19 |
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_ |
1808129415667777536 |