1. Identificação | |
Tipo de Referência | Artigo em Revista Científica (Journal Article) |
Site | mtc-m16.sid.inpe.br |
Código do Detentor | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identificador | 6qtX3pFwXQZsFDuKxG/AR5za |
Repositório | sid.inpe.br/marciana/2004/01.22.13.15 (acesso restrito) |
Última Atualização | 2004:07.05.03.00.00 (UTC) administrator |
Repositório de Metadados | sid.inpe.br/marciana/2004/01.22.13.15.15 |
Última Atualização dos Metadados | 2021:07.18.04.01.22 (UTC) administrator |
Chave Secundária | INPE-10797-PRE/6253 |
ISSN | 1364-6826 |
Chave de Citação | TsurutaniGonZhoLepBot:2004:PrSlMa |
Título | Properties of slow magnetic clouds |
Ano | 2004 |
Mês | Jan. |
Data de Acesso | 06 maio 2024 |
Tipo Secundário | PRE PI |
Número de Arquivos | 1 |
Tamanho | 435 KiB |
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2. Contextualização | |
Autor | 1 Tsurutani, Bruce T. 2 González-Alarcon, Walter Demétrio 3 Zhoua, Xian. Yan 4 Leppingc, R. P. 5 Bothmerd, V. |
Grupo | 1 DGE-INPE-MCT-BR |
Afiliação | 1 Jet Propulsion Laboratory, California Institute of Technology, MS 169-506, 4800 Oak Grove Drive 2 Pasadena, CA 91109, USA 3 Instituto Nacional de Pesquisas Espaciais, Sao Jose dos Campos, 12201-970, Sao Paulo, Brazil 4 Goddard Space Flight Center, Greenbelt, MD 20771, USA 5 Max-Planck-Institut für Aeronomie, Katlenburg-Lindau, D-37191, Germany |
Revista | Journal of Atmospheric and Solar-Terrestrial Physics |
Volume | 66 |
Número | 2 |
Páginas | 147-151 |
Histórico (UTC) | 2021-07-18 04:01:22 :: administrator -> marciana :: 2004 |
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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 |
Palavras-Chave | Slow magnetic clouds Geoeffectiveness Interplanetary magnetic fields |
Resumo | Slow (VSW<400 km s-1) magnetic clouds have been analyzed to determine their characteristics and geoeffectiveness. It is found that slow clouds have mean magnetic field strengths of ~13 nT, peak BS~9 nT, and dawn–dusk electric fields of ESW~2.5 mV m-1. The clouds are small in spatial size, typically ~0.18 AU. The slowest events may have been accelerated to their speeds by interaction with the slow solar wind. Slow clouds are surprisingly geoeffective. Five out of 27 events caused major (DST-100 nT) magnetic storms. Likewise, these geoeffective clouds may have been decelerated to VSW<400 km s-1. The issue of interplanetary acceleration/deceleration will be examined with SOHO coronal mass ejection data in the near future. Author Keywords: Slow (VSW<400 km s-1) magnetic clouds have been analyzed to determine their characteristics and geoeffectiveness. It is found that slow clouds have mean magnetic field strengths of ~13 nT, peak BS~9 nT, and dawn–dusk electric fields of ESW~2.5 mV m-1. The clouds are small in spatial size, typically ~0.18 AU. The slowest events may have been accelerated to their speeds by interaction with the slow solar wind. Slow clouds are surprisingly geoeffective. Five out of 27 events caused major (DST-100 nT) magnetic storms. Likewise, these geoeffective clouds may have been decelerated to VSW<400 km s-1. The issue of interplanetary acceleration/deceleration will be examined with SOHO coronal mass ejection data in the near future. |
Área | CEA |
Arranjo | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Properties of slow... |
Conteúdo da Pasta doc | acessar |
Conteúdo da Pasta source | não têm arquivos |
Conteúdo da Pasta agreement | não têm arquivos |
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4. Condições de acesso e uso | |
Idioma | en |
Arquivo Alvo | science.pdf |
Grupo de Usuários | administrator |
Visibilidade | shown |
Detentor da Cópia | SID/SCD |
Política de Arquivamento | denypublisher denyfinaldraft24 |
Permissão de Leitura | deny from all and allow from 150.163 |
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5. Fontes relacionadas | |
Unidades Imediatamente Superiores | 8JMKD3MGPCW/3EU29DP |
Divulgação | WEBSCI; PORTALCAPES; AGU; MGA; COMPENDEX. |
Acervo Hospedeiro | sid.inpe.br/banon/2003/08.15.17.40 |
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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 |
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7. Controle da descrição | |
e-Mail (login) | marciana |
atualizar | |
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