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1. Identificação
Tipo de ReferênciaArtigo em Revista Científica (Journal Article)
Sitemtc-m16.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador6qtX3pFwXQZsFDuKxG/APQnp
Repositóriosid.inpe.br/marciana/2004/01.20.12.42
Última Atualização2014:05.13.12.39.28 (UTC) administrator
Repositório de Metadadossid.inpe.br/marciana/2004/01.20.12.42.42
Última Atualização dos Metadados2018:06.05.01.20.51 (UTC) administrator
Chave SecundáriaINPE--PRE/
DOI10.1029/2002JA009721
ISSN0148-0227
2156-2202
Chave de CitaçãoAbduBaTaMaSoMeTr:2003:CaStBr
TítuloMagnetospheric disturbance induced equatorial plasma bubble development and dynamics: A case study in Brazilian Sector
ProjetoFAPESP (99/00437-0); CNPq [520185/ 95-1 (SU)].
Ano2003
MêsDec.
Data de Acesso17 maio 2024
Tipo de Trabalhojournal article
Tipo SecundárioPRE PI
Número de Arquivos1
Tamanho1725 KiB
2. Contextualização
Autor1 Abdu, Mangalathayil Ali
2 Batista, Inez Staciarini
3 Takahashi, Hisao
4 MacDougall, J. W.
5 Sobral, José Humberto Andrade
6 Medeiros, Amauri Fragoso de
7 Trivedi, Nalin Babulal
Grupo1 DAE-INPE-MCT-BR
2 DAE-INPE-MCT-BR
3 DAE-INPE-MCT-BR
4
5 DAE-INPE-MCT-BR
Afiliação1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 University of Western Ontario
5 Instituto Nacional de Pesquisas Espaciais (INPE)
6 Universidade Federal da Paraiba
7 Instituto Nacional de Pesquisas Espaciais (INPE)
Endereço de e-Mail do Autor1 abdu@dae.inpe.br
2 inez@dae.inpe.br
3 hisaotak@laser.inpe.br
4 jamacdoug@uwo.ca
5 sobral@dae.inpe.br
6 afragoso@df.ufpb.br
7 hisao@laser.inpe.br
RevistaJournal of Geophysical Research
Volume108
NúmeroA12
Páginas1449 (13pp)
Histórico (UTC)2013-09-29 20:50:58 :: administrator -> marciana :: 2003
2014-05-13 12:39:31 :: marciana -> administrator :: 2003
2018-06-05 01:20:51 :: administrator -> :: 2003
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-Chaveelectric fields
equatorial ionosphere
ionospheric disturbances
ionospheric irregularities
particle precipitation
ionosphere/atmosphere interaction
ResumoEquatorial ionospheric plasma bubble irregularity development and dynamics during the major magnetospheric storm of 26 August 1998 are investigated using the data collected by a multistation and multi-instrument diagnostic network operated at equatorial and low latitude sites in Brazil, and auroral electrojet activity (AU/AL), IMF, and Dst indices. A magnetospheric disturbance onset in the morning of 26 August 1998 was initiated by a solar wind shock and associated IMF Bz polarity reversals and ssc that were soon followed by a succession of substorm-like auroral electrojet (AE) intensifications and Dst development. An IMF Bz southward turning and associated AE intensifications in the Brazilian dusk sector produced intense prompt penetration eastward electric field that caused large F region vertical drift and consequently the developments of intense postsunset equatorial anomaly and a series of intense plasma bubbles, the latter event lasting the entire night, as observed by digital ionosondes at São Luís (2.33S, 315.8E, dip angle: - .5) and Fortaleza (3.9S, 321.55W, dip angle: - 9) and an all-sky imager, two scanning photometers, and a Digisonde at the lowlatitude site Cachoeira Paulista (22.6S, 315E; dip angle: - 28). A notable aspect of the dynamics of the bubbles was their initially very low eastward drift velocity which turned into steadily increasing westward velocity that lasted till early morning hours. The results show for the first time a relationship between the zonal drift velocities of optically observed large-scale bubbles (tens to hundreds of kilometers) and that of the smaller scale (kilometer sizes) structures as observed by a digital ionosonde. The results point to the dominant role of a disturbance dynamo associated westward thermospheric wind to maintain the plasma irregularity drift increasingly westward going into postmidnight hours. As an important finding, the results further show that significant contribution to the westward plasma bubble irregularity drift, normally attributed to disturbance dynamo effect, could arise from prompt penetration disturbance zonal electric field, in the course of a disturbance sequence lasting several hours. Such effect is attributed to Hall electric field arising from the primary disturbance zonal electric field, under enhanced nighttime ionospheric conductivities produced possibly by storm associated particle precipitation, in the Brazilian longitude sector in agreement with recent evidences [Abdu et al., 1998b].
ÁreaCEA
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Conteúdo da Pasta docacessar
Conteúdo da Pasta sourcenão têm arquivos
Conteúdo da Pasta agreementnão têm arquivos
4. Condições de acesso e uso
URL dos dadoshttp://urlib.net/ibi/6qtX3pFwXQZsFDuKxG/APQnp
URL dos dados zipadoshttp://urlib.net/zip/6qtX3pFwXQZsFDuKxG/APQnp
Idiomaen
Arquivo Alvojgra16862.pdf
Grupo de Usuáriosadministrator
Grupo de Leitoresadministrator
marciana
Visibilidadeshown
Política de Arquivamentodenypublisher6 allowfinaldraft
Permissão de Atualizaçãonão transferida
5. Fontes relacionadas
Unidades Imediatamente Superiores8JMKD3MGPCW/3ETL868
Lista de Itens Citandosid.inpe.br/bibdigital/2013/09.29.20.43 2
DivulgaçãoWEBSCI; AGU; MGA; COMPENDEX.
Acervo Hospedeirosid.inpe.br/banon/2003/08.15.17.40
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 readpermission resumeid rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject tertiarymark tertiarytype url


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