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1. Identificação
Tipo de ReferênciaArtigo em Revista Científica (Journal Article)
Sitemarte3.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador6qtX3pFwXQZ3r59YCT/GSsAp
Repositóriosid.inpe.br/iris@1905/2005/07.25.22.35.28
Última Atualização2017:05.10.18.50.40 (UTC) marciana
Repositório de Metadadossid.inpe.br/iris@1905/2005/07.25.22.35.38
Última Atualização dos Metadados2018:06.06.04.40.14 (UTC) administrator
Chave SecundáriaINPE-8865-PRE/4575
ISSN0148-0227
2156-2202
Rótulo3146
Chave de CitaçãoMozerGinBogKelSch:1974:HiLaEl
TítuloHigh latitude electric-field and 3-dimensional interaction between interplanetary and terrestrial magnetic-fields
ProjetoASTRO
Ano1974
Data de Acesso30 jun. 2024
Tipo SecundárioPRE PI
Número de Arquivos1
Tamanho2462 KiB
2. Contextualização
Autor1 Mozer, F. S.
2 Ginzalez-Alarcan, Walter Demetrio
3 Bogott, F.
4 Kelley, M. C.
5 Schutz, S.
Grupo1 DGE-INPE-BR
Afiliação1 Instituto Nacional de Pesquisas Espaciais (INPE)
RevistaJournal of Geophysical Research
Volume79
Número1
Páginas56-63
Histórico (UTC)2014-09-29 15:30:54 :: administrator -> marciana :: 1974
2017-05-10 18:50:40 :: marciana -> administrator :: 1974
2018-06-06 04:40:14 :: administrator -> marciana :: 1974
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-ChaveGEOFÍSICA ESPACIAL
ResumoMore than 200 hours of ionospheric electric field measurements taken on balloons flown from three polar cap sites have been analyzed to determine average properties of the largescale polar cap electric field and its dependencies on the interplanetary magnetic field. The major component of this electric field was directed from dawn to dusk and produced an average polar cap potential drop of about 55 kV. The magnitude of this potential provides an upper limit of about 700 RE for the length of the magnetospheric tail and implies an energy input from the solar wind to the magnetosphere of about 5 X 1019 ergs/see, The dawn to dusk component of the high4atitude polar cap electric field responds to BZ, the northward component of the interplanetary magnetic field, on a time scale <1 hour and with an average increase of about 3 mV/m for each 1 ? decrease of BZ. The hourly averages of the electric field data at each of the three sites are well described by a two-cell convection pattern whose location depends on the y component of the interplanetary magnetic field. When BY is positive (negative), the two-cell convection pattern shifts toward dawn (dusk)in the northern hemisphere with the following consequences: the maximum intensity of the northern polar cap: dawn to dusk electric field component occurs at local morning (evening), and the auroral zone return flow reaches higher latitudes in the evening (morning). Evidence of the vector nature of the interaction between interplanetary and terrestrial magnetic fields is provided by the observation that the above BY dependent signatures are most evident when BZ is most negative.
ÁreaCEA
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4. Condições de acesso e uso
URL dos dadoshttp://urlib.net/ibi/6qtX3pFwXQZ3r59YCT/GSsAp
URL dos dados zipadoshttp://urlib.net/zip/6qtX3pFwXQZ3r59YCT/GSsAp
Arquivo Alvo8865.pdf
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Permissão de Atualizaçãonão transferida
5. Fontes relacionadas
Unidades Imediatamente Superiores8JMKD3MGPCW/3EU29DP
Lista de Itens Citando
DivulgaçãoWEBSCI; AGU; MGA; COMPENDEX.
Acervo Hospedeirosid.inpe.br/banon/2001/04.03.15.36
6. Notas
Campos Vaziosalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel doi e-mailaddress electronicmailaddress format isbn language lineage mark mirrorrepository month nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress readpermission resumeid rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url
7. Controle da descrição
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