| 1. Identificação | |
| Tipo de Referência | Artigo em Revista Científica (Journal Article) |
| Site | mtc-m16d.sid.inpe.br |
| Código do Detentor | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
| Identificador | 8JMKD3MGP7W/37UBHES |
| Repositório | sid.inpe.br/mtc-m19@80/2010/07.29.12.22 (acesso restrito) |
| Última Atualização | 2011:09.15.11.39.19 (UTC) administrator |
| Repositório de Metadados | sid.inpe.br/mtc-m19@80/2010/07.29.12.22.49 |
| Última Atualização dos Metadados | 2018:06.05.04.36.51 (UTC) administrator |
| Chave Secundária | INPE--PRE/ |
| DOI | 10.1029/2009JA014788 |
| ISSN | 0926-9851 |
| Chave de Citação | MuellaKPCKKMBA:2010:ScFrIr |
| Título | Scintillation-producing Fresnel-scale irregularities associated with the regions of steepest TEC gradients adjacent to the equatorial ionization anomaly  |
| Ano | 2010 |
| Mês | Mar. |
| Data de Acesso | 05 maio 2024 |
| Tipo Secundário | PRE PI |
| Número de Arquivos | 1 |
| Tamanho | 3669 KiB |
| 2. Contextualização | |
| Autor | 1 Muella, M. T. A. H 2 Kherani, E. A. 3 Paula, E. R 4 Cerruti, A. P 5 Kintner, P. M 6 Kantor, I. J. 7 Mitchell, C. N. 8 Batista, I. S 9 Abdu, M. A. |
| Grupo | 1 2 DAE-CEA-INPE-MCT-BR 3 DAE-CEA-INPE-MCT-BR 4 5 6 DAE-CEA-INPE-MCT-BR 7 8 DAE-CEA-INPE-MCT-BR 9 DAE-CEA-INPE-MCT-BR |
| Afiliação | 1 Cornell Univ, Sch Elect & Comp Engn, Ithaca, NY 14853 USA. 2 Instituto Nacional de Pesquisas Espaciais (INPE) 3 Instituto Nacional de Pesquisas Espaciais (INPE) 4 Cornell Univ, Sch Elect & Comp Engn, Ithaca, NY 14853 USA. 5 6 Instituto Nacional de Pesquisas Espaciais (INPE) 7 Univ Bath, Dept Elect & Elect Engn, Bath BA2 7AY, Avon, England. 8 Instituto Nacional de Pesquisas Espaciais (INPE) 9 Instituto Nacional de Pesquisas Espaciais (INPE) |
| Revista | Journal of Applied Geophysics |
| Volume | 115 |
| Número | A03301 |
| Páginas | 19 |
| Histórico (UTC) | 2011-03-21 20:01:23 :: marciana -> lise@dpi.inpe.br :: 2010 2011-09-13 12:40:32 :: lise@dpi.inpe.br -> marciana :: 2010 2011-09-15 11:39:19 :: marciana -> administrator :: 2010 2011-09-15 12:47:45 :: administrator -> marciana :: 2010 2012-01-26 11:05:13 :: marciana -> administrator :: 2010 2012-07-15 03:42:24 :: administrator -> banon :: 2010 2012-09-26 15:28:39 :: banon -> administrator :: 2010 2018-06-05 04:36:51 :: administrator -> marciana :: 2010 |
| 3. Conteúdo e estrutura | |
| É a matriz ou uma cópia? | é a matriz |
| Estágio do Conteúdo | concluido |
| Transferível | 1 |
| Tipo do Conteúdo | External Contribution |
| Tipo de Versão | publisher |
| Palavras-Chave | total electron-content l-band scintillations 20 november 2003 spread-f low-latitude ionospheric scintillation horizontal gradients density gradients neutral wind zonal drifts |
| Resumo | Using ground-based GPS and digital ionosonde instruments, we have built up at latitudes of the equatorial ionization anomaly (EIA), in the Brazilian sector, a time-evolving picture of total electron content (TEC), L-band amplitude scintillations, and F region heights, and we have investigated likely reasons for the occurrence or suppression of equatorial scintillations during the disturbed period of 18-23 November 2003. During the prestorm quiet nights, scintillations are occurring postsunset, as expected; however, during the storm time period, their spatial-temporal characteristics and intensity modify significantly owing to the dramatic changes in the ionospheric plasma density distribution and in the temporal evolution of TEC. The two-dimensional maps showing both TEC and amplitude scintillations revealed strong evidence of turbulences at the Fresnel length (causing scintillations) concurrent with those regions of steepest TEC gradients adjacent to the crests of the EIA. The largest density gradients have been found to occur in an environment of increased background electron density, and their spatial distribution and location during the disturbed period may differ significantly from the magnetic quiet night pattern. However, in terms of magnitude the gradients at equatorial and low latitudes appear to not change during both magnetic quiet and disturbed conditions. The scenarios for the formation or suppression of scintillation-producing Fresnel-scale irregularities during the prestorm quiet nights and disturbed nights are discussed in view of different competing effects computed from numerical simulation techniques. |
| Área | CEA |
| Arranjo | urlib.net > DIDAE > Scintillation-producing Fresnel-scale irregularities... |
| Conteúdo da Pasta doc | acessar |
| Conteúdo da Pasta source | não têm arquivos |
| Conteúdo da Pasta agreement | não têm arquivos |
| 4. Condições de acesso e uso | |
| Idioma | en |
| Arquivo Alvo | 2009JA014788.pdf |
| Grupo de Usuários | administrator banon marciana |
| Visibilidade | shown |
| Política de Arquivamento | denypublisher denyfinaldraft24 |
| Permissão de Leitura | deny from all and allow from 150.163 |
| Permissão de Atualização | não transferida |
| 5. Fontes relacionadas | |
| Repositório Espelho | sid.inpe.br/mtc-m19@80/2009/08.21.17.02.53 |
| Unidades Imediatamente Superiores | 8JMKD3MGPCW/3ETL868 |
| Divulgação | WEBSCI; AGU; MGA; COMPENDEX. |
| Acervo Hospedeiro | sid.inpe.br/mtc-m19@80/2009/08.21.17.02 |
| 6. Notas | |
| Campos Vazios | alternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress electronicmailaddress format isbn label lineage mark nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup resumeid rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url |
| 7. Controle da descrição | |
| e-Mail (login) | marciana |
| atualizar | |