| 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/3E9B7N4 |
| Repositório | sid.inpe.br/mtc-m19/2013/06.09.02.13.14 (acesso restrito) |
| Última Atualização | 2013:07.17.14.23.23 (UTC) administrator |
| Repositório de Metadados | sid.inpe.br/mtc-m19/2013/06.09.02.13.15 |
| Última Atualização dos Metadados | 2021:07.18.04.02.25 (UTC) administrator |
| DOI | 10.1016/j.jastp.2013.04.003 |
| ISSN | 1364-6826 |
| Rótulo | scopus |
| Chave de Citação | MenesesKlKlKhMuXuHa:2013:ElTeEn |
| Título | Electron temperature enhancements in nighttime equatorial ionosphere under the occurrence of plasma bubbles  |
| Ano | 2013 |
| Mês | Apr. |
| Data de Acesso | 02 maio 2024 |
| Tipo Secundário | PRE PI |
| Número de Arquivos | 1 |
| Tamanho | 3016 KiB |
| 2. Contextualização | |
| Autor | 1 Meneses, F. C. de 2 Klimenko, M. V. 3 Klimenko, V. V. 4 Kherani, Esfhan Alam 5 Muralikrishna, Polinaya 6 Xu, J. 7 Hasbi, A. M. |
| Identificador de Curriculo | 1 2 3 4 5 8JMKD3MGP5W/3C9JJ4G |
| Grupo | 1 2 3 4 DAE-CEA-INPE-MCTI-GOV-BR 5 DAE-CEA-INPE-MCTI-GOV-BR |
| Afiliação | 1 State Key Laboratory of Space Weather, Center for Space Science and Applied Research (CSSAR), Chinese Academy of Sciences, P.O. Box 8701, Beijing 100080, PR China 2 West Department of Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation RAS, Kaliningrad 236017, Russia 3 West Department of Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation RAS, Kaliningrad 236017, Russia 4 National Institute for Space Research (INPE), Av. dos Astronautas, 1758, C.P. 515, 12201-970 São José dos Campos, SP, Brazil; Institut de Physique du Globe de Paris, CNRS, Paris, France 5 National Institute for Space Research (INPE), Av. dos Astronautas, 1758, C.P. 515, 12201-970 São José dos Campos, SP, Brazil 6 State Key Laboratory of Space Weather, Center for Space Science and Applied Research (CSSAR), Chinese Academy of Sciences, P.O. Box 8701, Beijing 100080, PR China 7 Department of Electrical, Electronic and Systems Engineering, Universiti Kebangsaan Malaysia (UKM), Malaysia; Institute of Space Science, Universiti Kebangsaan Malaysia (UKM), Malaysia |
| Endereço de e-Mail do Autor | 1 2 3 4 alam@dae.inpe.br 5 murali@dae.inpe.br |
| Endereço de e-Mail | marcelo.pazos@inpe.br |
| Revista | Journal of Atmospheric and Solar-Terrestrial Physics |
| Volume | 103 |
| Nota Secundária | A1 B1 B1 B1 B1 B2 C |
| Histórico (UTC) | 2021-07-18 04:02:25 :: administrator -> marcelo.pazos@inpe.br :: 2013 |
| 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 | Electron temperature Plasma bubbles Equatorial ionosphere Rocket measurements |
| Resumo | Simultaneous in-situ measurements of electron density and temperature in the nighttime equatorial region were performed by a rocket experiment launched under solar minimum and geomagnetic quiet conditions from the station of Alcântara (2.24°S; 44.24°W), Brazil, on Dec. 18, 1995, 21:17 LT. These measurements detected during the upleg flight a large overheated area around the base of density profile. The presence of plasma bubbles was revealed during the downleg phase, as well as temperature enhancements detected preferentially at altitudes where plasma depletions are found. It was assumed that the region traversed by the rocket during the downleg was preceded before the bubble's onset by a large overheating as observed during the upleg flight. Analyzing this framework under the light of the Global Self-Consistent Model of the Thermosphere, Ionosphere and Protonosphere (GSM TIP), as well as a 2D numerical code that simulate the growth of an instability and the evolution of thermal energy inside a bubble, we found that despite an overheated area in the F-region bottomside can disturb the electron density profile around the altitude interval where such heat is deposited, it seems not have a direct influence over parameters responsible for the bubble onset. Additionally, the phenomenon of the intra-bubble thermal enhancement could be formed due to the convection of hot-electron fluid transported from the overheated region surrounding the base of the F-region to upper altitudes by the underlying mechanism of bubble generation. |
| Área | CEA |
| Arranjo | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAE > Electron temperature enhancements... |
| 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 | 1-s2.0-S1364682613001168-main.pdf |
| Grupo de Usuários | administrator marcelo.pazos@inpe.br |
| Grupo de Leitores | administrator marcelo.pazos@inpe.br |
| 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 | iconet.com.br/banon/2006/11.26.21.31 |
| Unidades Imediatamente Superiores | 8JMKD3MGPCW/3ETL868 |
| Lista de Itens Citando | sid.inpe.br/bibdigital/2013/09.29.20.43 1 |
| URL (dados não confiáveis) | http://dx.doi.org/10.1016/j.jastp.2013.04.003 |
| Divulgação | WEBSCI; PORTALCAPES; AGU; MGA; COMPENDEX; SCOPUS. |
| Acervo Hospedeiro | sid.inpe.br/mtc-m19@80/2009/08.21.17.02 |
| 6. Notas | |
| Notas | In Press, Corrected Proof |
| Campos Vazios | alternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel format isbn lineage mark nextedition number orcid pages parameterlist parentrepositories previousedition previouslowerunit progress project rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject tertiarymark tertiarytype typeofwork |
| 7. Controle da descrição | |
| e-Mail (login) | marcelo.pazos@inpe.br |
| atualizar | |