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/UuLwP |
Repositório | sid.inpe.br/mtc-m17@80/2008/06.18.12.23 (acesso restrito) |
Última Atualização | 2008:06.18.12.23.11 (UTC) administrator |
Repositório de Metadados | sid.inpe.br/mtc-m17@80/2008/06.18.12.23.13 |
Última Atualização dos Metadados | 2018:06.05.03.30.52 (UTC) administrator |
Chave Secundária | INPE--PRE/ |
DOI | 10.1007/s11207-008-9185-9 |
ISSN | 0038-0938 1573-093X |
Chave de Citação | Kane:2008:GnPeGa |
Título | Gnevyshev Peaks and Gaps for Coronal Mass Ejections of Different Widths Originating in Different Solar Position Angles |
Ano | 2008 |
Mês | June |
Data de Acesso | 07 maio 2024 |
Tipo Secundário | PRE PI |
Número de Arquivos | 1 |
Tamanho | 511 KiB |
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2. Contextualização | |
Autor | Kane, Rajaram Purushotam |
Grupo | DGE-CEA-INPE-MCT-BR |
Afiliação | Instituto Nacional de Pesquisas Espaciais (INPE) |
Revista | Solar Physics |
Volume | 249 |
Número | 2 |
Páginas | 369-380 |
Histórico (UTC) | 2008-06-18 12:23:13 :: simone -> administrator :: 2012-07-13 22:33:07 :: administrator -> simone :: 2013-02-20 15:20:20 :: simone -> administrator :: 2008 2018-06-05 03:30:52 :: administrator -> marciana :: 2008 |
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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 |
Resumo | The sunspot number series at the peak of sunspot activity often has two or three peaks (Gnevyshev peaks; Gnevyshev, Solar Phys. 1, 107, 1967; Solar Phys. 51, 175, 1977). The sunspot group number (SGN) data were examined for 1997 2003 (part of cycle 23) and compared with data for coronal mass ejection (CME) events. It was noticed that they exhibited mostly two Gnevyshev peaks in each of the four latitude belts 0° 10°, 10° 20°, 20 ° 30°, and > 30°, in both N (northern) and S (southern) solar hemispheres. The SGN were confined to within latitudes ± 50° around the Equator, mostly around ± 35°, and seemed to occur later in lower latitudes, indicating possible latitudinal migration as in the Maunder butterfly diagrams. In CMEs, less energetic CMEs (of widths < 71°) showed prominent Gnevyshev peaks during sunspot maximum years in almost all latitude belts, including near the poles. The CME activity lasted longer than the SGN activity. However, the CME peaks did not match the SGN peaks and were almost simultaneous at different latitudes, indicating no latitudinal migration. In energetic CMEs including halo CMEs, the Gnevyshev peaks were obscure and ill-defined. The solar polar magnetic fields show polarity reversal during sunspot maximum years, first at the North Pole and, a few months later, at the South Pole. However, the CME peaks and gaps did not match with the magnetic field reversal times, preceding them by several months, rendering any cause effect relationship doubtful. |
Área | CEA |
Arranjo | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Gnevyshev Peaks and... |
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 | gnevyshev.pdf |
Grupo de Usuários | administrator simone |
Visibilidade | shown |
Política de Arquivamento | denypublisher denyfinaldraft12 |
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. |
Acervo Hospedeiro | lcp.inpe.br/ignes/2004/02.12.18.39 cptec.inpe.br/walmeida/2003/04.25.17.12 |
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6. Notas | |
Campos Vazios | alternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel documentstage e-mailaddress electronicmailaddress format isbn keywords 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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