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/ShrBk |
Repositório | sid.inpe.br/mtc-m17@80/2007/11.27.13.46 |
Última Atualização | 2010:09.24.19.42.28 (UTC) administrator |
Repositório de Metadados | sid.inpe.br/mtc-m17@80/2007/11.27.13.46.16 |
Última Atualização dos Metadados | 2018:06.05.03.35.32 (UTC) administrator |
Chave Secundária | INPE-14992-PRE/9903 |
ISSN | 0992-7689 |
Chave de Citação | Kane:2007:HyLoCo |
Título | Hysteresis loops of Cosmic Ray intensity decreases versus solar and interplanetary parameters ![](http://mtc-m16b.sid.inpe.br/col/dpi.inpe.br/banon/2000/01.23.20.24/doc/externalLink.gif) |
Ano | 2007 |
Data de Acesso | 25 jun. 2024 |
Tipo Secundário | PRE PI |
Número de Arquivos | 1 |
Tamanho | 8260 KiB |
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2. Contextualização | |
Autor | Kane, Rajaram Purushottam |
Identificador de Curriculo | 8JMKD3MGP5W/3C9JJ4U |
Grupo | DGE-INPE-MCT-BR |
Afiliação | Instituto Nacional de Pesquisas Espaciais (INPE) |
Revista | Annales Geophysicae |
Volume | 25 |
Número | 9 |
Páginas | 2087-2097 |
Histórico (UTC) | 2007-12-19 14:18:21 :: simone -> administrator :: 2008-06-29 02:37:37 :: administrator -> banon :: 2010-05-11 15:21:19 :: banon -> simone :: 2010-09-24 19:42:29 :: simone -> administrator :: 2012-10-24 00:03:42 :: administrator -> simone :: 2007 2013-02-20 15:20:08 :: simone -> marciana :: 2007 2013-03-07 13:47:37 :: marciana -> administrator :: 2007 2018-06-05 03:35:32 :: administrator -> marciana :: 2007 |
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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 | Interplanetary physics (Cosmic rays Heliopause and solar wind termination Interplanetary magnetic fields) |
Resumo | The purpose of this study was to examine the correlation between CR (Cosmic Ray) intensity and solar, interplanetary and terrestrial parameters. The hysteresis loops of (CR) versus those of several solar parameters showed narrow loops in even cycles 20, 22 and broad loops in odd cycles 19, 21, as also in the recent odd cycle 23. Hysteresis plots for CR versus interplanetary number density N and speed V were erratic and uncertain (broad and narrow, all mixed up). Plots of CR versus Interplanetary magnetic field (IMF) B seemed to be narrow for even as well as odd cycles. Hysteresis loops between CR and other interplanetary parameters were not clear-cut. The same was true for terrestrial parameters. During sunspot maximum years 20002003 of cycle 23, there is a double peak structure in all parameters. Whereas CR have a peak spacing of 30 months, sunspots and Tilt angle have a spacing of only 20 months. The solar open magnetic flux and the Voyager 1 magnetic field have a spacing of 25 months. The solar polar magnetic field reverses later than the first peak of all parameters and hence, could not be a direct cause (as if effect started before the cause and lasted for several months more after the cause disappeared). It seems that CR modulation is mainly guided by magnetic configurations deep in the heliosphere, which may not have a simple relationship with parameters near Earth or near Sun. |
Área | CEA |
Arranjo | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Hysteresis loops of... |
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 | |
URL dos dados | http://urlib.net/ibi/6qtX3pFwXQZGivnK2Y/ShrBk |
URL dos dados zipados | http://urlib.net/zip/6qtX3pFwXQZGivnK2Y/ShrBk |
Idioma | en |
Arquivo Alvo | Dr.kane-1.pdf |
Grupo de Usuários | administrator banon marciana simone |
Visibilidade | shown |
Detentor da Cópia | SID/SCD |
Política de Arquivamento | allowpublisher allowfinaldraft |
Permissão de Leitura | allow from all |
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 sid.inpe.br/mtc-m21/2012/07.13.14.58.38 1 |
Divulgação | WEBSCI; PORTALCAPES; MGA; COMPENDEX. |
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 copyright creatorhistory descriptionlevel doi e-mailaddress electronicmailaddress format isbn label lineage mark mirrorrepository month nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url |
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7. Controle da descrição | |
e-Mail (login) | marciana |
atualizar | |
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