| 1. Identificação | |
| Tipo de Referência | Artigo em Revista Científica (Journal Article) |
| Site | marte3.sid.inpe.br |
| Código do Detentor | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
| Identificador | 6qtX3pFwXQZ3r59YCT/H37G9 |
| Repositório | sid.inpe.br/iris@1905/2005/08.02.21.50.36 (acesso restrito) |
| Última Atualização | 2013:06.06.16.39.44 (UTC) banon |
| Repositório de Metadados | sid.inpe.br/iris@1905/2005/08.02.21.50.39 |
| Última Atualização dos Metadados | 2021:07.18.04.00.42 (UTC) administrator |
| Chave Secundária | INPE-8677-PRE/4413 |
| ISSN | 1364-6826 |
| Rótulo | 9636 |
| Chave de Citação | TsurutaniZAGLVPAYRHLB:2001:AuZoDa |
| Título | Auroral zone dayside precipitation during magentic storm initial phases  |
| Ano | 2001 |
| Mês | Mar. |
| Data de Acesso | 25 jun. 2024 |
| Tipo Secundário | PRE PI |
| Número de Arquivos | 1 |
| Tamanho | 875 KiB |
| 2. Contextualização | |
| Autor | 1 Tsurutani, Bruce T. 2 Zhou, X. Y. 3 Arballo, John. K. 4 Gonzalez, Walter Demétrio 5 Lakhina, G. S. 6 Vasyliunas, V. 7 Pickett, J. S. 8 Araki, T. 9 Yang, H. 10 Rostoker, G. 11 Hughes, T. J. 12 Lepping, R. P. 13 Berdichevsky, D. |
| Grupo | 1 2 3 4 DGE-INPE-MCT-BR |
| Afiliação | 1 Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA 2 Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA 3 Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA 4 Instituto Nacional de Pesquisas Espaciais (INPE) 5 Indian Institute of Geomagnetism, Mumbai, India 6 Max-Planck-Institut für Aeronomie, Lindau, Germany 7 Department of Physics & Astronomy, University of Iowa, USA 8 Department of Geophysics, Kyoto University, Japan 9 National Institute of Polar Research, Tokyo, Japan 10 Technical Communication and Services, Ottawa, Canada 11 Technical Communication and Services, Ottawa, Canada 12 Goddard Space Flight Center, Code 696, Greenbelt, MD, USA 13 Goddard Space Flight Center, Code 696, Greenbelt, MD, USA |
| Endereço de e-Mail do Autor | 1 btsurutani@jplsp.jpl.nasa.gov 2 3 4 gonzalez@dge.inpe.br |
| Endereço de e-Mail | marcelo.pazos@inpe.br |
| Revista | Journal of Atmospheric and Solar-Terrestrial Physics |
| Volume | 63 |
| Número | 5 |
| Páginas | 513-522 |
| Histórico (UTC) | 2013-06-06 16:19:32 :: administrator -> jefferson :: 2001 2013-06-06 16:39:44 :: jefferson -> marcelo.pazos@sid.inpe.br :: 2001 2013-06-06 16:43:49 :: marcelo.pazos@sid.inpe.br -> administrator :: 2001 2021-02-27 13:25:41 :: administrator -> banon :: 2001 2021-02-27 13:26:59 :: banon -> administrator :: 2001 2021-07-18 04:00:42 :: administrator -> marcelo.pazos@sid.inpe.br :: 2001 |
| 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 | zonas aurorais tempestades magnéticas magnetosferas auroral zones magnetic storms magnetospheres |
| Resumo | Significant charged-particle precipitation occurs in the dayside auroral zone during and after interplanetary shock impingements on the Earth's magnetosphere. The precipitation intensities and spatial and temporal evolution are discussed. Although the post-shock energy flux (1020 erg cm-2 s-1) is lower than that of substorms, the total energy deposition rate may be considerably greater (similar to an order of magnitude) than nightside energy rates due to the greater area of the dayside portion of the auroral oval (defined as extending from 03 MLT through noon to 21 MLT). This dayside precipitation represents direct solar wind energy input into the magnetosphere, ionosphere system. The exact mechanisms for particle energization and precipitation into the ionosphere are not known at this time. Different mechanisms are probably occurring during different portions of the storm initial phase. Immediately after shock compression of the magnetosphere possible precipitation-related mechanisms are: (1) betatron compression of preexisting outer zone magnetospheric particles. The anisotropic plasma is unstable to loss-cone instabilities, leading to plasma wave growth, resonant particle pitch-angle scattering and electron and proton losses into the upper ionosphere. (2) The compression of the magnetosphere can also lead to enhanced field-aligned currents and the formation of dayside double-layers. Finally (3) in the latter stages of the storm initial phase. there is efidence for a long-lasting viscous-like interaction occurring on the Ranks of the magnetopause. Ground-based observations identifying the types of dayside auroral forms would be extremely useful in identifying the specific solar wind energy transfer mechanisms. |
| Área | CEA |
| Arranjo | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Auroral zone dayside... |
| 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-S1364682600001619-main.pdf |
| Grupo de Usuários | administrator marcelo.pazos@inpe.br |
| Grupo de Leitores | administrator banon 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 | |
| Unidades Imediatamente Superiores | 8JMKD3MGPCW/3EU29DP |
| Lista de Itens Citando | 1 |
| Divulgação | WEBSCI; PORTALCAPES; AGU; MGA; COMPENDEX. |
| Acervo Hospedeiro | sid.inpe.br/banon/2001/04.03.15.36 |
| 6. Notas | |
| Campos Vazios | alternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel doi format isbn lineage mark mirrorrepository nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project resumeid rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url |
| 7. Controle da descrição | |
| e-Mail (login) | marcelo.pazos@sid.inpe.br |
| atualizar | |