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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/42NRR6L
Repositóriosid.inpe.br/mtc-m21c/2020/06.26.12.30
Última Atualização2020:06.26.12.30.09 (UTC) administrator
Repositório de Metadadossid.inpe.br/mtc-m21c/2020/06.26.12.30.09
Última Atualização dos Metadados2022:03.18.22.11.33 (UTC) administrator
DOI10.1029/2019JA027519
ISSN2169-9402
Chave de CitaçãoResendeSDBNAAMSCBWL:2020:InDiDy
TítuloThe influence of disturbance dynamo electric field in the formation of strong sporadic E layers over Boa Vista, a low‐latitude station in the American sector
Ano2020
Data de Acesso13 maio 2024
Tipo de Trabalhojournal article
Tipo SecundárioPRE PI
Número de Arquivos1
Tamanho6015 KiB
2. Contextualização
Autor 1 Resende, Laysa Cristina Araújo
 2 Shi, Jiankui K.
 3 Denardini, Clezio Marcos
 4 Batista, Inez Staciarini
 5 Nogueira, Paulo A. B.
 6 Arras, C.
 7 Andrioli, Vânia Fátima
 8 Moro, Juliano
 9 Silva, Ligia Alves da
10 Carrasco, A. J.
11 Barbosa Neto, Paulo França
12 Wang, Chi
13 Liu, Z.
Identificador de Curriculo 1
 2
 3
 4 8JMKD3MGP5W/3C9JHDA
ORCID 1 0000-0001-6968-6184
 2 0000-0002-8008-0527
 3 0000-0002-3624-2461
 4 0000-0001-5385-4112
 5 0000-0003-0810-1044
 6
 7 0000-0001-9065-2122
 8 0000-0003-4078-2222
 9
10
11
12 0000-0001-6991-9398
Grupo 1 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
 2
 3 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
 4 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
 5
 6
 7 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
 8 CRCRS-COCRE-INPE-MCTIC-GOV-BR
 9 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
10
11 GESAST-CEA-SESPG-INPE-MCTIC-GOV-BR
Afiliação 1 Instituto Nacional de Pesquisas Espaciais (INPE)
 2 State Key Laboratory of Space Weather, NSSC/CAS
 3 Instituto Nacional de Pesquisas Espaciais (INPE)
 4 Instituto Nacional de Pesquisas Espaciais (INPE)
 5 Instituto Federal de Educação, Ciência e Tecnologia de São Paulo (IFSP)
 6 Helmholtz Centre Potsdam
 7 Instituto Nacional de Pesquisas Espaciais (INPE)
 8 Instituto Nacional de Pesquisas Espaciais (INPE)
 9 Instituto Nacional de Pesquisas Espaciais (INPE)
10 Universidad de Los Andes
11 Instituto Nacional de Pesquisas Espaciais (INPE)
12 State Key Laboratory of Space Weather, NSSC/CAS
13 State Key Laboratory of Space Weather, NSSC/CAS
Endereço de e-Mail do Autor 1 laysa.resende@inpe.br
 2
 3 clezio.denardin@inpe.br
 4 inez.batista@inpe.br
 5
 6
 7 vania.andrioli@inpe.br
 8
 9
10
11 paulo.barbosa@inpe.br
RevistaJournal of Geophysical Research: Space Physics
Volume102
Número9
Histórico (UTC)2020-06-26 12:30:09 :: simone -> administrator ::
2020-06-26 12:30:10 :: administrator -> simone :: 2020
2020-06-26 12:34:06 :: simone -> administrator :: 2020
2020-06-26 13:35:31 :: administrator -> simone :: 2020
2020-06-26 13:47:34 :: simone -> administrator :: 2020
2020-06-27 12:29:46 :: administrator -> simone :: 2020
2020-12-14 13:58:32 :: simone -> administrator :: 2020
2022-03-18 22:11:33 :: administrator -> simone :: 2020
3. Conteúdo e estrutura
É a matriz ou uma cópia?é a matriz
Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
Tipo de Versãopublisher
ResumoThis study analyzes strong sporadic E layer (Es) formation in Boa Vista (BV, 2.8°N, 60.7°W, dip: 18°), a low‐latitude region in the Brazilian sector, which occurred far after the onset of a magnetic storm recovery phase. Such occurrences were observed during seven magnetic storms with available data for BV. Thus, the ionospheric behavior on days around the magnetic storm that occurred on 20 January 2016 was investigated to search for possible explanations. This analysis indicated that the probable mechanism acting during the Es layer strengthening is the zonal westward electric field caused by a disturbance dynamo. The same evidence was also observed in two other magnetic storms at the same location. Hence, a numerical model of the E region dynamics, called MIRE (Portuguese acronym for E Region Ionospheric Model), was used to confirm whether the disturbance dynamo could cause the Es layer intensification. The inputs for the model were the electric field deduced from the vertical drift and the wind components provided by GSWM‐00 model. The simulations indicate that the Es layer density is significantly enhanced when the zonal electric field is present compared to the reference scenario with only the winds. Therefore, it is concluded that the disturbance dynamo electric field is the likely cause of the strong Es layers in the analyzed cases. Finally, the combined results from the model and observational data seem to contribute significantly to advance our understanding of the role of the electric fields in the Es layer formation at low latitudes.
ÁreaCEA
Conteúdo da Pasta docacessar
Conteúdo da Pasta sourcenão têm arquivos
Conteúdo da Pasta agreement
agreement.html 26/06/2020 09:30 1.0 KiB 
4. Condições de acesso e uso
URL dos dadoshttp://urlib.net/ibi/8JMKD3MGP3W34R/42NRR6L
URL dos dados zipadoshttp://urlib.net/zip/8JMKD3MGP3W34R/42NRR6L
Idiomaen
Arquivo AlvoResende_influence.pdf
Grupo de Usuáriossimone
Visibilidadeshown
Política de Arquivamentodenypublisher6 allowfinaldraft
Permissão de Leituraallow from all
Permissão de Atualizaçãonão transferida
5. Fontes relacionadas
Unidades Imediatamente Superiores8JMKD3MGPCW/3ETL868
8JMKD3MGPCW/3EUFCFP
8JMKD3MGPCW/3F2PBEE
Lista de Itens Citandosid.inpe.br/bibdigital/2013/10.12.21.02 1
sid.inpe.br/mtc-m21/2012/07.13.14.50.14 1
sid.inpe.br/bibdigital/2013/09.29.20.43 1
DivulgaçãoWEBSCI; AGU; MGA; COMPENDEX.
Acervo Hospedeirourlib.net/www/2017/11.22.19.04
6. Notas
Campos Vaziosalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn keywords label lineage mark mirrorrepository month nextedition notes pages parameterlist parentrepositories previousedition previouslowerunit progress project readergroup rightsholder schedulinginformation secondarydate secondarykey secondarymark session shorttitle sponsor subject tertiarymark tertiarytype url
7. Controle da descrição
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