| 1. Identificação | |
| Tipo de Referência | Artigo em Evento (Conference Proceedings) |
| Site | mtc-m16.sid.inpe.br |
| Código do Detentor | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
| Identificador | 6qtX3pFwXQZsFDuKxG/EJqEk |
| Repositório | sid.inpe.br/marciana/2005/01.10.10.39 |
| Repositório de Metadados | sid.inpe.br/marciana/2005/01.10.10.39.59 |
| Última Atualização dos Metadados | 2019:03.25.18.00.22 (UTC) simone |
| Chave Secundária | INPE--PRE/ |
| Rótulo | self-archiving-INPE-MCTIC-GOV-BR |
| Chave de Citação | SilvaVDEAMKS:2004:DeBeAv |
| Título | Determination of best avarage time interval of the interplanetary magnetic field for application in space weather forecasting  |
| Ano | 2004 |
| Data de Acesso | 20 maio 2024 |
| Tipo Secundário | PRE CI |
| 2. Contextualização | |
| Autor | 1 Silva, M. R. da 2 Vieira, Luiz Eduardo Antunes 3 Dal Lago, Alisson 4 Echer, Ezequiel 5 Alarcon, Walter Demetrio Gonzalez 6 Munakata, Kazuoki 7 Kuwabara, T. 8 Schuch, Nelson Jorge |
| Grupo | 1 DGE-INPE-MCT-BR 2 RSU-INPE-MCT-BR |
| Nome do Evento | Scientific Assembly of COSPAR, (37Th). |
| Localização do Evento | Paris, France |
| Data | 18-25 july |
| Editora (Publisher) | INPE |
| Título do Livro | Anais |
| Histórico (UTC) | 2005-01-10 12:40:00 :: jefferson -> administrator :: 2018-06-05 01:21:25 :: administrator -> marciana :: 2004 2019-03-25 18:00:02 :: marciana -> simone :: 2004 |
| 3. Conteúdo e estrutura | |
| É a matriz ou uma cópia? | é a matriz |
| Estágio do Conteúdo | concluido |
| Transferível | 1 |
| Resumo | The solar activity drives a large number of phenomena that occur in the near-earth interplanetary space and in the earth's magnetosphere, the so-called Space Weather. Among the most important phenomena of Space Weather we have the Geomagnetic Storms. In these phenomena, a great transfer of energy from the Sun and the Interplanetary Medium to the earth's magnetosphere takes place. It is well known that the galactic cosmic ray particles are also affected by the solar activity. One of the most important solar ejected structures, the Coronal Mass Ejection (CME), is the main cause of intense Geomagnetic Storms, and it is known to modulate cosmic ray intensity observed with ground detectors as they approach and pass the earth (Munakata et al., 2000). Thus ground cosmic ray observations may be used for forecasting this kind of interplanetary structures. By analyzing the cosmic ray intensities measured in various directions in space by the International Muon Detector Network, together with the Interplanetary Magnetic Field (IMF) data observed by the Advanced Composition Explorer Satellite (ACE), the Loss Cone precursor can be seen some 6 to 9 hours prior to an interplanetary disturbance reaching the Earth Magnetosphere and then causing a geomagnetic storm. As the direction of the IMF is an important parameter in this forecasting scheme, this work has the objective of determining the best average time interval of the interplanetary magnetic field to be used together with the high-energy cosmic ray observations. We use ACE IMF observations from 1998 to 2001. |
| Área | CEA |
| Arranjo 1 | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Determination of best... |
| Arranjo 2 | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > CRCRS > Determination of best... |
| Conteúdo da Pasta doc | não têm arquivos |
| Conteúdo da Pasta source | não têm arquivos |
| Conteúdo da Pasta agreement | não têm arquivos |
| 4. Condições de acesso e uso | |
| Idioma | en |
| Grupo de Usuários | administrator jefferson simone |
| Grupo de Leitores | administrator simone |
| Visibilidade | shown |
| Permissão de Atualização | não transferida |
| 5. Fontes relacionadas | |
| Unidades Imediatamente Superiores | 8JMKD3MGPCW/3EU29DP 8JMKD3MGPCW/3EUFCFP |
| Acervo Hospedeiro | sid.inpe.br/banon/2003/08.15.17.40 |
| 6. Notas | |
| Campos Vazios | affiliation archivingpolicy archivist callnumber contenttype copyholder copyright creatorhistory descriptionlevel dissemination doi e-mailaddress edition editor electronicmailaddress format isbn issn keywords lineage mark mirrorrepository nextedition notes numberoffiles numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisheraddress readpermission resumeid rightsholder schedulinginformation secondarydate secondarymark serieseditor session shorttitle size sponsor subject targetfile tertiarymark tertiarytype type url versiontype volume |
| 7. Controle da descrição | |
| e-Mail (login) | simone |
| atualizar | |