1. Identificação | |
Tipo de Referência | Capítulo de Livro (Book Section) |
Site | mtc-m16.sid.inpe.br |
Código do Detentor | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identificador | 8JMKD3MGPDW/3PBE42P |
Repositório | sid.inpe.br/mtc-m16/2017/07.25.17.23 (acesso restrito) |
Última Atualização | 2017:07.25.17.23.09 (UTC) simone |
Repositório de Metadados | sid.inpe.br/mtc-m16/2017/07.25.17.23.09 |
Última Atualização dos Metadados | 2023:12.29.17.44.37 (UTC) simone |
Chave Secundária | INPE--/ |
ISBN | 978-0-87590-432-0 |
Chave de Citação | TsurutaniMcGoLuGoGu:2006:MaStCa |
Título | Magnetic storms caused by corotating solar wind streams |
Ano | 2006 |
Data de Acesso | 27 abr. 2024 |
Tipo Secundário | PRE LI |
Número de Arquivos | 1 |
Tamanho | 1798 KiB |
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2. Contextualização | |
Autor | 1 Tsurutani, B. T. 2 McPherron, Robert L. 3 Gonzalez Alarcon, Walter Demétrio 4 Lu, Gang 5 Gopalswamy, Nat 6 Guarnieri, Fernando Luis |
Grupo | 1 2 University of California 3 DGE-INPE-MCT-BR 4 5 6 DGE-INPE-MCT-BR |
Afiliação | 1 Jet Propulsion Laboratory 2 3 Instituto Nacional de Pesquisas Espaciais (INPE) 4 High Altitude Observatory 5 Goddard Space Flight Center 6 Instituto Nacional de Pesquisas Espaciais (INPE) |
Editor | Tsurutani, B. T. McPherron, R. Gonzalez Alarcon, W. D. Lu, G. Sobral, J. H. A. Gopalswamy, N. |
Título do Livro | Recurrente magnetic storms: corotating solar wind streams |
Editora (Publisher) | AGU |
Cidade | Washington |
Páginas | 1-17 |
Título da Série | Geophysical monograph 167 |
Histórico (UTC) | 2017-07-25 17:23:09 :: simone -> administrator :: 2023-12-29 17:43:44 :: administrator -> simone :: 2006 |
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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 | magnetic storms corotating solar wind streams |
Resumo | Geomagnetic activity at Earth due to corotating high speed solar wind streams are reviewed. High density plasma regions in the vicinity of the heliospheric current sheet in the slow solar wind impinge upon the magnetosphere and create magnetic storm intial phases. Dst increases can be higher than those associated with shocks in front of interplanetary coronal mass ejections. High speed streams following the high density interplanetary plasma interact with the upstream slow speed streams and create magnetic field compression regions called corotating interaction regions (CIRs). The southward components of the typically rapid Bz fluctuations within the CIRs, through sporadic magnetic reconnection with the Earths magnetic fields, lead to weak to moderate intensity magnetic storm main phases, typically Dst >−100 nT. Some CIRs (without southward component Bz fields) cause no perceptible Dst changes at all. The recovery phases of CIR-induced magnetic storms can last for a few days up to 27 days. The cause of these particularly long duration storm recoveries is near-continuous shallow plasma injections into the magnetosphere. Magnetic reconnection associated with the southward component of the Alfvén waves within the high speed streams with magnetopause fields is the cause of these injections. The auroras during these intervals are continuous and global auroral zone features. The AE/AL maxima are not substorms or convection bays. Relativistic electrons are accelerated/observed during these high speed stream intervals. The electrons first appear in the beginning of the lengthy storm recovery phases. Geomagnetic quiet is due to weak interplanetary magnetic fields with a lack of Alfvénic fluctuations. These interplanetary regions generally occur in the decay portion of high speed streams. |
Área | CEA |
Arranjo | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Magnetic storms caused... |
Conteúdo da Pasta doc | acessar |
Conteúdo da Pasta source | não têm arquivos |
Conteúdo da Pasta agreement | |
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4. Condições de acesso e uso | |
Idioma | en |
Arquivo Alvo | tsurutani_et al.pdf |
Grupo de Usuários | administrator simone |
Grupo de Leitores | administrator simone |
Visibilidade | shown |
Permissão de Leitura | deny from all and allow from 150.163 |
Permissão de Atualização | não transferida |
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5. Fontes relacionadas | |
Unidades Imediatamente Superiores | 8JMKD3MGPCW/3EU29DP |
Lista de Itens Citando | sid.inpe.br/bibdigital/2013/10.01.22.11 1 |
Divulgação | NTRSNASA; BNDEPOSITOLEGAL. |
Acervo Hospedeiro | sid.inpe.br/banon/2003/08.15.17.40 |
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6. Notas | |
Campos Vazios | archivingpolicy archivist callnumber copyholder copyright creatorhistory descriptionlevel doi e-mailaddress edition electronicmailaddress format issn label lineage mark mirrorrepository nextedition notes numberofvolumes orcid parameterlist parentrepositories previousedition previouslowerunit progress project resumeid rightsholder schedulinginformation secondarydate secondarymark serieseditor session shorttitle sponsor subject tertiarymark tertiarytype translator url volume |
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7. Controle da descrição | |
e-Mail (login) | simone |
atualizar | |
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