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1. Identificação
Tipo de ReferênciaArtigo em Revista Científica (Journal Article)
Sitemtc-m21c.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador8JMKD3MGP3W34R/3RHS9FB
Repositóriosid.inpe.br/mtc-m21c/2018/08.01.13.27
Última Atualização2018:08.01.13.27.21 (UTC) simone
Repositório de Metadadossid.inpe.br/mtc-m21c/2018/08.01.13.27.21
Última Atualização dos Metadados2021:07.28.22.48.29 (UTC) administrator
DOI10.1186/s40623-018-0875-8
ISSN1880-5981
Chave de CitaçãoCandidoBKNBPSC:2018:ReToEl
TítuloResponse of the total electron content at Brazilian low latitudes to corotating interaction region and high-speed streams during solar minimum 2008
Ano2018
MêsJune
Data de Acesso28 abr. 2024
Tipo de Trabalhojournal article
Tipo SecundárioPRE PI
Número de Arquivos1
Tamanho10086 KiB
2. Contextualização
Autor1 Candido, Cláudia Maria Nicoli
2 Batista, Inez Staciarini
3 Klausner, Virginia
4 Negreti, Patrícia Mara de Siqueira
5 Becker Guedes, Fábio
6 Paula, Eurico Rodrigues de
7 Shi, Jiankui
8 Correia, Emília
Identificador de Curriculo1
2 8JMKD3MGP5W/3C9JHDA
3
4
5
6 8JMKD3MGP5W/3C9JH2U
7
8 8JMKD3MGP5W/3C9JH2C
Grupo1 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
2 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
3
4 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
5 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
6 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
7 DIDAS-CGCEA-INPE-MCTIC-GOV-BR
8 DIDAS-CGCEA-INPE-MCTIC-GOV-BR
Afiliação1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3
4 Instituto Nacional de Pesquisas Espaciais (INPE)
5 Instituto Nacional de Pesquisas Espaciais (INPE)
6 Instituto Nacional de Pesquisas Espaciais (INPE)
7 Instituto Nacional de Pesquisas Espaciais (INPE)
8 Instituto Nacional de Pesquisas Espaciais (INPE)
Endereço de e-Mail do Autor1 claudia.candido@inpe.br
2 inez.batista@inpe.br
3
4 patricia.negreti@inpe.br
5 fabio.guedes@inpe.br
6 eurico.paula@inpe.br
7 emilia.correia@inpe.br
RevistaEarth, Planets and Space
Volume70
Páginase104
Histórico (UTC)2018-08-01 13:27:21 :: simone -> administrator ::
2018-08-01 13:27:24 :: administrator -> simone :: 2018
2018-08-01 13:28:31 :: simone -> administrator :: 2018
2019-01-04 16:57:07 :: administrator -> simone :: 2018
2019-01-07 12:34:27 :: simone -> administrator :: 2018
2021-07-28 22:48:29 :: administrator -> simone :: 2018
3. Conteúdo e estrutura
É a matriz ou uma cópia?é a matriz
Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
Tipo de Versãopublisher
Palavras-ChaveSolar minimum
High-speed streams
Corotating interaction region
High-intensity long-duration continuous auroral activity
Equatorial ionization anomaly
Total electron content
ResumoIn this work, we investigate the Brazilian low-latitude ionospheric response to two corotating interaction regions (CIRs) and high-speed streams (HSSs) events during the solar minimum of solar cycle 23, in 2008. The studied intervals are enclosed in the whole heliospheric interval, studied by other authors, for distinct longitudinal sectors. CIRs/HSSs are structures commonly observed during the descending and low solar activity, and they are related to the occurrence of coronal holes. These events cause weak-to-moderate recurrent geomagnetic storms characterized by negative excursions of the interplanetary magnetic field, IMF_Bz, as well as long-duration auroral activity, considered as a favorable scenario for continuous prompt penetration interplanetary electric field (PPEF). In this study, we used the vertical total electron content (VTEC) calculated from GPS receivers database from the Brazilian Continuous Monitoring Network managed by the Brazilian Institute of Geography and Statistics. Moreover, we analyzed the F-layer peak height, hmF2 and the critical plasma frequency, foF2, taken from a Digisonde installed at the southern crest of the equatorial ionization anomaly, in Cachoeira Paulista, CP. It was observed that during the CIRs/HSSs-driven geomagnetic disturbances VTEC increased more than 120% over the quiet times averaged values, which is comparable to intense geomagnetic storms. On the other hand, VTEC decreases were also observed during the recovery phase of the storm. Spectral analysis using gapped wavelet technique (GWT) revealed periodicities of 7, 9, 13.5 days, which are sub-harmonics of the solar rotation period, similar to 27 days. These periods in VTEC are closely associated with those observed in solar and geomagnetic indices such as Vsw, IMF_Bz and AE during CIRs/HSSs intervals. We discuss PPEF associated to IMF_ Bz reconnection processes and the auroral activity as the most probable causes for the VTEC variations. These results can be of interest for studies related to space weather monitoring, modeling and forecasting, especially during low solar activity.
ÁreaCEA
Arranjo 1urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAE > Response of the...
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4. Condições de acesso e uso
URL dos dadoshttp://urlib.net/ibi/8JMKD3MGP3W34R/3RHS9FB
URL dos dados zipadoshttp://urlib.net/zip/8JMKD3MGP3W34R/3RHS9FB
Idiomaen
Arquivo Alvocandido_response.pdf
Grupo de Usuáriossimone
Grupo de Leitoresadministrator
simone
Visibilidadeshown
Política de Arquivamentoallowpublisher allowfinaldraft
Permissão de Atualizaçãonão transferida
5. Fontes relacionadas
Unidades Imediatamente Superiores8JMKD3MGPCW/3ETL868
8JMKD3MGPCW/3ETR8EH
Lista de Itens Citandosid.inpe.br/mtc-m21/2012/07.13.14.45.35 4
sid.inpe.br/mtc-m21/2012/07.13.14.50.14 3
sid.inpe.br/bibdigital/2013/09.29.20.43 1
DivulgaçãoWEBSCI; PORTALCAPES; SCOPUS.
Acervo Hospedeirourlib.net/www/2017/11.22.19.04
6. Notas
Campos Vaziosalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn label lineage mark mirrorrepository nextedition notes number orcid parameterlist parentrepositories previousedition previouslowerunit progress project readpermission rightsholder schedulinginformation secondarydate secondarykey secondarymark session shorttitle sponsor subject tertiarymark tertiarytype url
7. Controle da descrição
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