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Metadados

1. Identificação
Tipo de ReferênciaArtigo em Revista Científica (Journal Article)
Sitemtc-m21c.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador8JMKD3MGP3W34R/3TUJDKS
Repositóriosid.inpe.br/mtc-m21c/2019/09.03.14.01   (acesso restrito)
Última Atualização2019:09.03.14.01.34 (UTC) simone
Repositório de Metadadossid.inpe.br/mtc-m21c/2019/09.03.14.01.34
Última Atualização dos Metadados2022:03.18.22.15.07 (UTC) administrator
DOI10.1016/j.asr.2019.06.041
ISSN0273-1177
1879-1948
Chave de CitaçãoAgyei-YeboahPMBPELTW:2019:SeVaPl
TítuloSeasonal variation of plasma bubbles during solar cycle 23–24 over the Brazilian equatorial region
Ano2019
MêsOct.
Data de Acesso06 maio 2024
Tipo de Trabalhojournal article
Tipo SecundárioPRE PI
Número de Arquivos1
Tamanho1836 KiB
2. Contextualização
Autor1 Agyei-Yeboah, Ebenezer
2 Paulino, Igo
3 Medeiros, Amauri Fragaso
4 Buriti, Ricardo Arlen
5 Paulino, Ana Roberta
6 Essien, Patrick
7 Lomotey, Solomon Otoo
8 Takahashi, Hisao
9 Wrasse, Cristiano Max
Identificador de Curriculo1
2
3
4
5
6
7
8 8JMKD3MGP5W/3C9JHCM
Grupo1
2
3
4
5
6 GESATM-CEA-SESPG-INPE-MCTIC-GOV-BR
7 GESATM-CEA-SESPG-INPE-MCTIC-GOV-BR
8 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
9 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
Afiliação1 Universidade do Vale do Paraíba (UNIVAP)
2 Universidade Federal de Campina Grande (UFCG)
3 Universidade Federal de Campina Grande (UFCG)
4 Universidade Federal de Campina Grande (UFCG)
5 Universidade Federal de Campina Grande (UFCG)
6 Instituto Nacional de Pesquisas Espaciais (INPE)
7 Instituto Nacional de Pesquisas Espaciais (INPE)
8 Instituto Nacional de Pesquisas Espaciais (INPE)
9 Instituto Nacional de Pesquisas Espaciais (INPE)
Endereço de e-Mail do Autor1 agyeiyeboah.e@univap.br
2 igo.paulino@df.ufcg.edu.br
3
4
5
6 patrick.essien21@inpe.br
7 lomoteys@gmail.com
8 hisao.takahashi@inpe.br
9 cristiano.wrasse@inpe.br
RevistaAdvances in Space Research
Volume64
Número7
Páginas1365-1374
Nota SecundáriaB1_INTERDISCIPLINAR B1_GEOCIÊNCIAS B1_ENGENHARIAS_IV B1_ENGENHARIAS_III B1_BIODIVERSIDADE B3_CIÊNCIA_DA_COMPUTAÇÃO B4_ASTRONOMIA_/_FÍSICA C_CIÊNCIAS_BIOLÓGICAS_I
Histórico (UTC)2019-09-03 14:01:34 :: simone -> administrator ::
2019-09-03 14:01:34 :: administrator -> simone :: 2019
2019-09-03 14:02:44 :: simone -> administrator :: 2019
2022-03-18 22:15:07 :: administrator -> simone :: 2019
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 cycle
Plasma bubbles
All-sky imaging
Equatorial ionosphere
ResumoIn this study, OI 630.0 nm nightglow image data obtained from an all-sky imaging station located at Sao Joao do Cariri (7.4S, 36.5 W), have been used to study the occurrence of equatorial plasma bubbles (EPBs) over the Brazilian equatorial region. The observations, which took place from September 2000 to December 2010 (almost eleven years), covered a significant part of solar cycle 23 (descending phase of SC23) and the very beginning of solar cycle 24 (ascending phase of SC24). There were 1337 nights of observations with 666 nights with EPB events, which translates to an occurrence rate of 49.8%. Of these nights, 1290 were considered quiet (Dst - 50 nT) with 50% plasma bubbles occurrence rate. The occurrence of EPBs was studied under three solar activity phases high solar activity phase (HSA, September 2000 March 2004), moderate solar activity phase (MSA or descending phase, March 2004 October 2006) and low solar activity phase (LSA, October 2006 December 2010). The low solar activity phase is part of the peculiar solar cycle 24, considered the weakest in over a century with most sunspotless days (20082009). The maximum occurrence of bubbles, equal to 54.2%, was found during the HSA phase, with percentages characterizing MSA and LSA being respectively 52.4% and 45.8%. The analysis also showed clear seasonal variation in the EPB occurrence with maximum rates in summer, spring, autumn, and the minimum rates in winter for all solar activity phases. Overall, there was observed solar cycle variation in each season with maximum occurrence in HSA followed by MSA and then LSA except in autumn where higher occurrence rate was observed in LSA phase than in MSA phase.
ÁreaCEA
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4. Condições de acesso e uso
Idiomaen
Arquivo Alvoagyei_sesonal.pdf
Grupo de Usuáriossimone
Grupo de Leitoresadministrator
simone
Visibilidadeshown
Política de Arquivamentodenypublisher denyfinaldraft24
Permissão de Leituradeny from all and allow from 150.163
Permissão de Atualizaçãonão transferida
5. Fontes relacionadas
Unidades Imediatamente Superiores8JMKD3MGPCW/3ETL868
8JMKD3MGPCW/3F2PBEE
Lista de Itens Citandosid.inpe.br/bibdigital/2013/09.29.20.43 2
sid.inpe.br/mtc-m21/2012/07.13.14.49.58 1
DivulgaçãoWEBSCI; PORTALCAPES; COMPENDEX; 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 orcid parameterlist parentrepositories previousedition previouslowerunit progress project rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject tertiarymark tertiarytype url
7. Controle da descrição
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