| 1. Identificação | |
| Tipo de Referência | Artigo em Revista Científica (Journal Article) |
| Site | mtc-m16b.sid.inpe.br |
| Código do Detentor | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
| Identificador | 6qtX3pFwXQZGivnK2Y/NqLfa |
| Repositório | sid.inpe.br/mtc-m17@80/2006/12.11.15.55 (acesso restrito) |
| Última Atualização | 2007:06.26.18.30.37 (UTC) administrator |
| Repositório de Metadados | sid.inpe.br/mtc-m17@80/2006/12.11.15.55.28 |
| Última Atualização dos Metadados | 2018:06.05.03.33.57 (UTC) administrator |
| Chave Secundária | INPE-14472-PRE/9713 |
| ISSN | 0032-0633 |
| Chave de Citação | DaglisTGKOCKHV:2007:CoStSo |
| Título | Key features of intense geospace storms: A comparative study of a solar maximum and a solar minimum storm  |
| Ano | 2007 |
| Mês | Jan. |
| Data de Acesso | 19 maio 2024 |
| Tipo Secundário | PRE PI |
| Número de Arquivos | 1 |
| Tamanho | 2517 KiB |
| 2. Contextualização | |
| Autor | 1 Daglis, I. A. 2 Tsurutani, Bruce T. 3 Gonzalez-Alarcon, Walter Demétrio 4 Kozyra, J. U. 5 Orsini, S. 6 Cladis, J. 7 Kamide, Y. 8 Henderson, M. G. 9 Vassiliadis, D. |
| Grupo | 1 2 3 DGE-INPE-MCT-BR |
| Afiliação | 1 Institute for Space Applications and Remote Sensing, National Observatory of Athens 2 Jet Propulsion Laboratory, California Institute of Technology 3 Instituto Nacional de Pesquisas Espaciais (INPE) 4 Space Physics Research Laboratory 5 Istituto di Fisica dello Spazio Interplanetario 6 Consultant to Lockheed Martin Space Physics Laboratory 7 Solar-Terrestrial Environment Laboratory 8 Los Alamos National Laboratory 9 USRA at NASA/Goddard Space Flight Center |
| Revista | Planetary and Space Science |
| Volume | 55 |
| Número | 1/2 |
| Páginas | 32-52 |
| Histórico (UTC) | 2007-06-26 18:30:38 :: simone -> administrator :: 2008-06-29 02:33:04 :: administrator -> simone :: 2011-05-29 09:26:45 :: simone -> administrator :: 2012-11-24 01:39:45 :: administrator -> simone :: 2007 2013-02-20 15:19:55 :: simone -> administrator :: 2007 2018-06-05 03:33:57 :: administrator -> marciana :: 2007 |
| 3. Conteúdo e estrutura | |
| É a matriz ou uma cópia? | é a matriz |
| Estágio do Conteúdo | concluido |
| Transferível | 1 |
| Tipo do Conteúdo | External Contribution |
| Palavras-Chave | Storms and substorms Solar wind-magnetosphere interactions Magnetosphere-ionosphere interactions Magnetospheric configuration and dynamics Energetic particles Trapped Current systems Particle acceleration |
| Resumo | This paper addresses the question of particular causes and dynamical characteristics of intense geospace storms through the comparative study of two specific examples: a solar maximum storm (46 June 1991) and a solar minimum storm (2426 September 1998). We concentrate on issues pertaining to the origin, development, dynamical evolution and recovery of intense storms. The comparative study addresses the solar and interplanetary drivers, the ring current composition and its implications, the stormsubstorm relationship, and the ring current decay. Our aim has been to identify features assumed common or repeatable and to elaborate on similarities or differences between two intense storms that are separated by 7 years and which occurred in different phases of the solar cycle. In view of planetary exploration, which is becoming the focus of space science both in the US and in Europe, classifying the drivers and parameters of solar-planetary connection is of particular interest. Solar system exploration will undoubtedly benefit from detailed knowledge of the conditions leading to intense geospace storms. The main conclusions of this paper can be listed as follows. More intense solar events do not necessarily result in more intense geospace storms. Storm development is driven by the appropriate interplanetary conditions; however, storm evolution is not defined by interplanetary conditions alone, but also by internal magnetospheric conditionsnamely plasma sheet density and ion composition. Storm dynamics may also be modified by solar wind pressure. Magnetosphereionosphere coupling in the form of ionospheric outflow during storms presumably is the key to substorm influence on storm dynamics; i.e., substorms influence storm development substantially, whenever they drive intense outflow of ionospheric-origin O+ ions into the magnetosphere. In particular, substorm-driven O+ outflow is one of the main features of intense storms. |
| Área | CEA |
| Arranjo | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Key features of... |
| 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 | key features.pdf |
| Grupo de Usuários | administrator simone |
| Visibilidade | shown |
| Detentor da Cópia | SID/SCD |
| Política de Arquivamento | denypublisher denyfinaldraft24 |
| Permissão de Leitura | deny from all and allow from 150.163 |
| 5. Fontes relacionadas | |
| Unidades Imediatamente Superiores | 8JMKD3MGPCW/3EU29DP |
| Divulgação | WEBSCI; PORTALCAPES; COMPENDEX. |
| Acervo Hospedeiro | lcp.inpe.br/ignes/2004/02.12.18.39 cptec.inpe.br/walmeida/2003/04.25.17.12 |
| 6. Notas | |
| Campos Vazios | alternatejournal archivist callnumber copyright creatorhistory descriptionlevel documentstage doi e-mailaddress electronicmailaddress format isbn label lineage mark mirrorrepository nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup resumeid rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url versiontype |
| 7. Controle da descrição | |
| e-Mail (login) | marciana |
| atualizar | |