| 1. Identificação | |
| Tipo de Referência | Artigo em Evento (Conference Proceedings) |
| Site | plutao.sid.inpe.br |
| Código do Detentor | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
| Identificador | J8LNKAN8RW/3AFLGR5 |
| Repositório | dpi.inpe.br/plutao/2011/09.22.19.46.42 |
| Última Atualização | 2012:06.14.12.54.01 (UTC) ana.silveira |
| Repositório de Metadados | dpi.inpe.br/plutao/2011/09.22.19.46.43 |
| Última Atualização dos Metadados | 2018:06.05.00.01.30 (UTC) administrator |
| Rótulo | lattes: 3638070053255922 7 SchuchMBDSLPSBVSHL:2011:SpWeAn |
| Chave de Citação | SchuchMBDSLPSBVSHL:2011:SpWeGl |
| Título | Space Weather and the Global Muon Detector Network - GMDN  |
| Ano | 2011 |
| Data de Acesso | 25 maio 2024 |
| Tipo Secundário | PRE CN |
| Número de Arquivos | 1 |
| Tamanho | 1139 KiB |
| 2. Contextualização | |
| Autor | 1 Schuch, Nelson Jorge 2 Munakata, Kazuoki 3 Bieber, John W. 4 Duldig, Marcus L. 5 Sabbah, Ismail 6 Lago, Alisson Dal 7 Petry, Adriano 8 rigozo, nivaor rodolfo 9 Silva, Marlos Rockenbach da 10 Braga, Carlos Roberto 11 Vieira, Lucas Ramos 12 Stekel, Tardelli Ronan Coelho 13 souza, mauricio rosa 14 Hammerschmitt, Bruno Knevitz 15 Lima, Roger Hatwig de |
| Grupo | 1 CRS-CCR-INPE-MCT-BR 2 3 4 5 6 DGE-CEA-INPE-MCT-BR 7 CRS-CCR-INPE-MCT-BR 8 CRS-CCR-INPE-MCT-BR |
| Afiliação | 1 Instituto Nacional de Pesquisas Espaciais (INPE) 2 3 4 5 6 Instituto Nacional de Pesquisas Espaciais (INPE) 7 Instituto Nacional de Pesquisas Espaciais (INPE) 8 Instituto Nacional de Pesquisas Espaciais (INPE) |
| Endereço de e-Mail do Autor | 1 2 3 4 5 6 7 adriano.petry@crs.inpe.br |
| Endereço de e-Mail | adriano.petry@crs.inpe.br |
| Nome do Evento | 12th International Congress of the Brazilian Geophysical Society |
| Localização do Evento | Rio de Janeiro |
| Data | 2011 |
| Título do Livro | Proceedings |
| Histórico (UTC) | 2011-09-23 14:11:21 :: lattes -> secretaria.cpa@dir.inpe.br :: 2011 2012-02-24 02:24:38 :: secretaria.cpa@dir.inpe.br -> ana.silveira :: 2011 2012-06-14 12:54:01 :: ana.silveira -> administrator :: 2011 2018-06-05 00:01:30 :: administrator -> ana.silveira :: 2011 |
| 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 |
| Resumo | The main objective of this work is to present an overview of the space weather and its relation with the global network of ground-based multi-directional muon detectors (GMDN). The GMDN is an international collaboration consisting of 10 institutions from 6 countries in 5 continents. A multi-directional muon detector for measuring high-energy galactic cosmic rays (GCRs) was installed in 2001 and expanded in its detection area in 2005, through an international cooperation between Brazil, Japan and USA, and has been in operation since then at the Southern Space Observatory - SSO/CRS/INPE -MCT, (29,4º S, 53,8º W, 480 m a.s.l), São Martinho da Serra, RS, in southern Brazil, as an important component of the GMDN. The observations conducted by this detector are used for forecasting the arrival of the interplanetary coronal mass ejections (ICMEs) and the geomagnetic storms at the Earth. The detector measures high-energy GCRs by detecting secondary muons produced from the hadronic interactions of primary GCRs (mostly protons) with atmospheric nuclei. While muons have a relatively short life-time (about 2.2 microseconds at rest), they can reach the detector at ground level because of the relativistic effect of the time dilation with heir high speed (~0.96c), preserving the incident direction of primary particles. The multi-directional detector can measure the GCR intensity in various directions at a single location, such as SSO in Brazil. ICMEs accompanied by a strong shock often forms a GCR depleted region behind the shock. The Forbush decrease is observed when the Earth enters in this depleted region. Some particles from this depleted region leak into the downstream, traveling with almost the speed of light, much faster than the approaching shock, and creating the precursory loss-cone anisotropy around the sunward IMF direction at the Earth. Loss-cones are typically visible 4-8 hours prior to the shock arrival and the onset of major geomagnetic storm at the Earth. This cosmic-ray precursor can be detected sometimes as early as ten hours prior to the shock arrival at the Earth. With the real time data from the upgraded GMDN, its methodology and data reduction techniques permits accurate Space Weather forecasting. |
| Área | CEA |
| Arranjo 1 | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Space Weather and... |
| Arranjo 2 | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > CRCRS > Space Weather and... |
| 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 | |
| URL dos dados | http://plutao.sid.inpe.br/ibi/J8LNKAN8RW/3AFLGR5 |
| URL dos dados zipados | http://plutao.sid.inpe.br/zip/J8LNKAN8RW/3AFLGR5 |
| Idioma | en |
| Arquivo Alvo | Resumo Expandido -Space Weather and-CiSBGF -.pdf |
| Grupo de Usuários | ana.silveira lattes secretaria.cpa@dir.inpe.br |
| Visibilidade | shown |
| Permissão de Leitura | allow from all |
| Permissão de Atualização | não transferida |
| 5. Fontes relacionadas | |
| Unidades Imediatamente Superiores | 8JMKD3MGPCW/3EU29DP 8JMKD3MGPCW/3EUFCFP |
| Acervo Hospedeiro | dpi.inpe.br/plutao@80/2008/08.19.15.01 |
| 6. Notas | |
| Campos Vazios | archivingpolicy archivist callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi edition editor format isbn issn keywords lineage mark mirrorrepository nextedition notes numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress readergroup resumeid rightsholder schedulinginformation secondarydate secondarykey secondarymark serieseditor session shorttitle sponsor subject tertiarymark tertiarytype type url volume |
| 7. Controle da descrição | |
| e-Mail (login) | ana.silveira |
| atualizar | |