| 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 | 6qtX3pFwXQZGivnJVY/LB7it |
| Repositório | sid.inpe.br/mtc-m16@80/2006/06.29.17.37 (acesso restrito) |
| Última Atualização | 2014:04.16.18.45.58 (UTC) administrator |
| Repositório de Metadados | sid.inpe.br/mtc-m16@80/2006/06.29.17.37.11 |
| Última Atualização dos Metadados | 2021:07.18.04.01.22 (UTC) administrator |
| Chave Secundária | INPE-14130--PRE/9264 |
| DOI | 10.1016/j.jastp.2006.04.001 |
| ISSN | 1364-6826 |
| Chave de Citação | Kane:2006:SoStFe |
| Título | Modulation of cosmic rays in cycle 23: Some striking features  |
| Projeto | FINEP-537/CT. |
| Ano | 2006 |
| Mês | Aug. |
| Data de Acesso | 05 maio 2024 |
| Tipo de Trabalho | journal article |
| Tipo Secundário | PRE PI |
| Número de Arquivos | 1 |
| Tamanho | 472 KiB |
| 2. Contextualização | |
| Autor | Kane, Rajaram Purushottam |
| Identificador de Curriculo | 8JMKD3MGP5W/3C9JJ4U |
| Grupo | DGE-INPE-MCT-BR |
| Afiliação | Instituto Nacional de Pesquisas Espaciais, Divisão de Geofísica Espacial (INPE.DGE) |
| Endereço de e-Mail do Autor | kane@dge.inpe.br |
| Endereço de e-Mail | marcelo.pazos@inpe.br |
| Revista | Journal of Atmospheric and Solar-Terrestrial Physics |
| Volume | 68 |
| Número | 12 |
| Páginas | 1291-1310 |
| Histórico (UTC) | 2006-09-05 17:38:12 :: simone -> administrator :: 2014-02-20 18:36:50 :: administrator -> marciana :: 2006 2014-04-16 18:43:30 :: marciana -> administrator :: 2006 2014-04-16 18:44:59 :: administrator -> marcelo.pazos@sid.inpe.br :: 2006 2014-04-16 18:46:43 :: marcelo.pazos@sid.inpe.br -> administrator :: 2006 2021-07-18 04:01:22 :: administrator -> :: 2006 |
| 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 | modulation cosmic rays cycle 23 |
| Resumo | The evolutions of the mid-latitude cosmic ray (CR) neutron monitor intensities and interplanetary and solar indices for 19962003 (rising phase of solar cycle 23) showed the following: (1) Monthly values: Most of the solar indices started increasing by July 1997 and reached a first peak near July 2000, a second peak near October 2001, and a third minor peak near September 2002. However, CR remained at an almost steady level up to March 1998, suffered a sharp decline during MarchMay 1998, remained almost steady up to July 1999, decreased thereafter almost smoothly up to July 2000 (first trough), and fluctuated thereafter to have a second trough in September 2002. The solar open magnetic flux (<45° solar latitude) and IMF B component did not change fully parallel to the solar indices. (2) Daily values: CR depressions mostly coincided well with geomagnetic Dst, but sometimes, the two were dissimilar. Also, CR and many other parameters showed oscillations with peak spacings of 727 days. (3) Hourly values: cosmic rays showed (Forbush) decreases evolving in a very similar way to geomagnetic Dst, particularly when the IMF B was large. We do not think that the idea that the long-term modulation in step-like form is caused by the propagating diffusive barriers Global MIRs (GMIRs) (e.g., Burlaga, L.F., McDonald, F.B., Ness, N.F., 1993. CR modulation and the distant heliospheric magnetic field: Voyager 1 and 2 observations from 1986 to 1989, near 11 AU. J. Geophys. Res. 98, 111) and the alternative suggestion (e. g., Cane, H.V., Wibberenz, G., Richardson, I.G., von Rosenvinge, T.T., 1999. CR modulation and the solar magnetic field. Geophys. Res. Lett. 26, 565568) that the step-like changes (medium-term events, lasting about an year) were related to a fundamental process at the Sun, are mutually exclusive. Both the processes are operative simultaneously, only that the relationship with near-Earth IMF is more spectacular as it occurs with considerable CR changes in a short time (hours to few days). During the absence of near-Earth events, the effects of GMIRs are seen clearly as slow CR decreases lasting for several days. |
| Área | CEA |
| Arranjo | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Modulation of cosmic... |
| 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 | 1-s2.0-S1364682606000964-main.pdf |
| Grupo de Usuários | administrator marcelo.pazos@inpe.br simone |
| Grupo de Leitores | administrator marcelo.pazos@inpe.br marciana |
| Visibilidade | shown |
| Detentor da Cópia | SID/SCD |
| Política de Arquivamento | denypublisher denyfinaldraft24 |
| Permissão de Leitura | deny from all and allow from 150.163 |
| Permissão de Atualização | não transferida |
| 5. Fontes relacionadas | |
| Unidades Imediatamente Superiores | 8JMKD3MGPCW/3EU29DP |
| Lista de Itens Citando | sid.inpe.br/bibdigital/2013/10.01.22.11 4 sid.inpe.br/mtc-m21/2012/07.13.14.58.38 1 |
| Divulgação | WEBSCI; PORTALCAPES; AGU; MGA; COMPENDEX. |
| Acervo Hospedeiro | sid.inpe.br/banon/2003/08.15.17.40 |
| 6. Notas | |
| Campos Vazios | alternatejournal archivist callnumber copyright creatorhistory descriptionlevel format isbn label lineage mark mirrorrepository nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject tertiarymark tertiarytype url |