Study of ionospheric irregularities during intense magnetic storms

Detalhes bibliográficos
Autor(a) principal: Rezende,Luiz Felipe Campos de
Data de Publicação: 2007
Outros Autores: Paula,Eurico Rodrigues de, Batista,Inez Staciarini, Kantor,Ivan Jelinek, Muella,Marcio Tadeu de Assis Honorato
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Revista Brasileira de Geofísica (Online)
Texto Completo: http://old.scielo.br/scielo.php?script=sci_arttext&pid=S0102-261X2007000600017
Resumo: The effects of two intense magnetic storms over ionospheric irregularities were analyzed using GPS signal scintillation data from the stations of São Luís (2.57ºS, 44.21ºW, dip latitude 1.73ºS) in the equatorial region, São José dos Campos (23.07ºS, 45.86ºW, dip latitude 18.01ºS) and Cachoeira Paulista (22.57ºS, 45.07ºW, dip latitude 18.12ºS) both under the Equatorial Ionization Anomaly (EIA), and São Martinho da Serra (29.28ºS, 53.82ºW, dip latitude 18.57ºS), located in the South of Brazil. Total Electron Content (TEC) data for São Luís and São José dos Campos, were also analyzed. The analyzed storms occurred on October 28-31, 2003 and on November 7-11, 2004. Both storm periods presented two main phases. In the nights of 29/30 and 30/31 of October, during the two storm main phase, it was observed that TEC over São José dos Campos reached higher values than the TEC for the magnetically quiet day of October 10, due to the effect of eastward electric field prompt penetration to magnetic equator that intensified the EIA. Compared to a quiet day (Oct 10), scintillation in the GPS signal amplitude due to ionospheric irregularity, quantified by the scintillation index S4, was stronger for Cachoeira Paulista (under EIA) during the night of 30/31but not for the night of 29/30 and for São Martinho da Serra was stronger during the nights of 29/30 and 30/31. Scintillation for the nights of 29/30 and 30/31 at these two stations lasted longer than on October 10, reaching the post midnight time sector. During the November 7-11 storm, TEC kept the behavior of a quiet day except during days 10 and 11 (up to 9 UT), when a large TEC decrease was observed. The GPS scintillation, compared to the quiet day November 19, was larger at the equatorial station of São Luís during the nights of 7/8 and 8/9 and it was completely inhibited for the São Luís and São José dos Campos stations during the nights of 9/10 and 10/11, probably due to action of westward disturbance dynamo electric field penetration to equator.
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spelling Study of ionospheric irregularities during intense magnetic stormsGPSionospheric scintillationmagnetic stormTEC (Total Electron Content)The effects of two intense magnetic storms over ionospheric irregularities were analyzed using GPS signal scintillation data from the stations of São Luís (2.57ºS, 44.21ºW, dip latitude 1.73ºS) in the equatorial region, São José dos Campos (23.07ºS, 45.86ºW, dip latitude 18.01ºS) and Cachoeira Paulista (22.57ºS, 45.07ºW, dip latitude 18.12ºS) both under the Equatorial Ionization Anomaly (EIA), and São Martinho da Serra (29.28ºS, 53.82ºW, dip latitude 18.57ºS), located in the South of Brazil. Total Electron Content (TEC) data for São Luís and São José dos Campos, were also analyzed. The analyzed storms occurred on October 28-31, 2003 and on November 7-11, 2004. Both storm periods presented two main phases. In the nights of 29/30 and 30/31 of October, during the two storm main phase, it was observed that TEC over São José dos Campos reached higher values than the TEC for the magnetically quiet day of October 10, due to the effect of eastward electric field prompt penetration to magnetic equator that intensified the EIA. Compared to a quiet day (Oct 10), scintillation in the GPS signal amplitude due to ionospheric irregularity, quantified by the scintillation index S4, was stronger for Cachoeira Paulista (under EIA) during the night of 30/31but not for the night of 29/30 and for São Martinho da Serra was stronger during the nights of 29/30 and 30/31. Scintillation for the nights of 29/30 and 30/31 at these two stations lasted longer than on October 10, reaching the post midnight time sector. During the November 7-11 storm, TEC kept the behavior of a quiet day except during days 10 and 11 (up to 9 UT), when a large TEC decrease was observed. The GPS scintillation, compared to the quiet day November 19, was larger at the equatorial station of São Luís during the nights of 7/8 and 8/9 and it was completely inhibited for the São Luís and São José dos Campos stations during the nights of 9/10 and 10/11, probably due to action of westward disturbance dynamo electric field penetration to equator.Sociedade Brasileira de Geofísica2007-01-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersiontext/htmlhttp://old.scielo.br/scielo.php?script=sci_arttext&pid=S0102-261X2007000600017Revista Brasileira de Geofísica v.25 suppl.2 2007reponame:Revista Brasileira de Geofísica (Online)instname:Sociedade Brasileira de Geofísica (SBG)instacron:SBG10.1590/S0102-261X2007000600017info:eu-repo/semantics/openAccessRezende,Luiz Felipe Campos dePaula,Eurico Rodrigues deBatista,Inez StaciariniKantor,Ivan JelinekMuella,Marcio Tadeu de Assis Honoratoeng2007-11-22T00:00:00Zoai:scielo:S0102-261X2007000600017Revistahttp://www.scielo.br/rbgONGhttps://old.scielo.br/oai/scielo-oai.php||sbgf@sbgf.org.br1809-45110102-261Xopendoar:2007-11-22T00:00Revista Brasileira de Geofísica (Online) - Sociedade Brasileira de Geofísica (SBG)false
dc.title.none.fl_str_mv Study of ionospheric irregularities during intense magnetic storms
title Study of ionospheric irregularities during intense magnetic storms
spellingShingle Study of ionospheric irregularities during intense magnetic storms
Rezende,Luiz Felipe Campos de
GPS
ionospheric scintillation
magnetic storm
TEC (Total Electron Content)
title_short Study of ionospheric irregularities during intense magnetic storms
title_full Study of ionospheric irregularities during intense magnetic storms
title_fullStr Study of ionospheric irregularities during intense magnetic storms
title_full_unstemmed Study of ionospheric irregularities during intense magnetic storms
title_sort Study of ionospheric irregularities during intense magnetic storms
author Rezende,Luiz Felipe Campos de
author_facet Rezende,Luiz Felipe Campos de
Paula,Eurico Rodrigues de
Batista,Inez Staciarini
Kantor,Ivan Jelinek
Muella,Marcio Tadeu de Assis Honorato
author_role author
author2 Paula,Eurico Rodrigues de
Batista,Inez Staciarini
Kantor,Ivan Jelinek
Muella,Marcio Tadeu de Assis Honorato
author2_role author
author
author
author
dc.contributor.author.fl_str_mv Rezende,Luiz Felipe Campos de
Paula,Eurico Rodrigues de
Batista,Inez Staciarini
Kantor,Ivan Jelinek
Muella,Marcio Tadeu de Assis Honorato
dc.subject.por.fl_str_mv GPS
ionospheric scintillation
magnetic storm
TEC (Total Electron Content)
topic GPS
ionospheric scintillation
magnetic storm
TEC (Total Electron Content)
description The effects of two intense magnetic storms over ionospheric irregularities were analyzed using GPS signal scintillation data from the stations of São Luís (2.57ºS, 44.21ºW, dip latitude 1.73ºS) in the equatorial region, São José dos Campos (23.07ºS, 45.86ºW, dip latitude 18.01ºS) and Cachoeira Paulista (22.57ºS, 45.07ºW, dip latitude 18.12ºS) both under the Equatorial Ionization Anomaly (EIA), and São Martinho da Serra (29.28ºS, 53.82ºW, dip latitude 18.57ºS), located in the South of Brazil. Total Electron Content (TEC) data for São Luís and São José dos Campos, were also analyzed. The analyzed storms occurred on October 28-31, 2003 and on November 7-11, 2004. Both storm periods presented two main phases. In the nights of 29/30 and 30/31 of October, during the two storm main phase, it was observed that TEC over São José dos Campos reached higher values than the TEC for the magnetically quiet day of October 10, due to the effect of eastward electric field prompt penetration to magnetic equator that intensified the EIA. Compared to a quiet day (Oct 10), scintillation in the GPS signal amplitude due to ionospheric irregularity, quantified by the scintillation index S4, was stronger for Cachoeira Paulista (under EIA) during the night of 30/31but not for the night of 29/30 and for São Martinho da Serra was stronger during the nights of 29/30 and 30/31. Scintillation for the nights of 29/30 and 30/31 at these two stations lasted longer than on October 10, reaching the post midnight time sector. During the November 7-11 storm, TEC kept the behavior of a quiet day except during days 10 and 11 (up to 9 UT), when a large TEC decrease was observed. The GPS scintillation, compared to the quiet day November 19, was larger at the equatorial station of São Luís during the nights of 7/8 and 8/9 and it was completely inhibited for the São Luís and São José dos Campos stations during the nights of 9/10 and 10/11, probably due to action of westward disturbance dynamo electric field penetration to equator.
publishDate 2007
dc.date.none.fl_str_mv 2007-01-01
dc.type.driver.fl_str_mv info:eu-repo/semantics/article
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
format article
status_str publishedVersion
dc.identifier.uri.fl_str_mv http://old.scielo.br/scielo.php?script=sci_arttext&pid=S0102-261X2007000600017
url http://old.scielo.br/scielo.php?script=sci_arttext&pid=S0102-261X2007000600017
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv 10.1590/S0102-261X2007000600017
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv text/html
dc.publisher.none.fl_str_mv Sociedade Brasileira de Geofísica
publisher.none.fl_str_mv Sociedade Brasileira de Geofísica
dc.source.none.fl_str_mv Revista Brasileira de Geofísica v.25 suppl.2 2007
reponame:Revista Brasileira de Geofísica (Online)
instname:Sociedade Brasileira de Geofísica (SBG)
instacron:SBG
instname_str Sociedade Brasileira de Geofísica (SBG)
instacron_str SBG
institution SBG
reponame_str Revista Brasileira de Geofísica (Online)
collection Revista Brasileira de Geofísica (Online)
repository.name.fl_str_mv Revista Brasileira de Geofísica (Online) - Sociedade Brasileira de Geofísica (SBG)
repository.mail.fl_str_mv ||sbgf@sbgf.org.br
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