| 1. Identificação | |
| Tipo de Referência | Artigo em Evento (Conference Proceedings) |
| Site | mtc-m16d.sid.inpe.br |
| Código do Detentor | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
| Identificador | 8JMKD3MGP7W/39CMNCN |
| Repositório | sid.inpe.br/mtc-m19/2011/03.22.13.41.35 |
| Última Atualização | 2020:11.17.13.46.17 (UTC) marciana |
| Repositório de Metadados | sid.inpe.br/mtc-m19/2011/03.22.13.41.36 |
| Última Atualização dos Metadados | 2020:11.17.13.46.18 (UTC) marciana |
| Rótulo | self-archiving-INPE-MCTIC-GOV-BR |
| Chave de Citação | SchuchMDDEGSRPKBVSARKKFFBEKDHCSJ:2010:GMSpSi |
| Título | The Global Muon Detector Network - GMDN and the space situational awareness  |
| Ano | 2010 |
| Data de Acesso | 19 maio 2024 |
| Tipo Secundário | PRE CI |
| Número de Arquivos | 1 |
| Tamanho | 80 KiB |
| 2. Contextualização | |
| Autor | 1 Schuch, Nelson Jorge 2 Munakata, Kazuoki 3 Dal Lago, Alisson 4 Denardini, Clezio Marcos 5 Echer, Ezequiel 6 Gonzalez Alarcon, Walter Demetrio 7 Silva, Marlos Rockenbach da 8 Rigozo, Nivaor R. 9 Petry, Adriano 10 Kirsch Pinheiro, Damaris 11 Braga, Carlos Roberto 12 Vinicius Dias Silveira, Marcos 13 Stekel, Tardelli Ronan Coelho 14 Antunes, Cassio Espindola 15 Ramos Vieira, Lucas 16 Kemmerich, Níkolas 17 Kato, Chihiro 18 Fushishita, Akira 19 Fujii, Zenjirou 20 Bieber, John W. 21 Evenson, Paul 22 Kuwabara, Takao 23 Duldig, Marcus L. 24 Humble, John E. 25 Chilingarian, Ashot 26 Sabbah, Ismail 27 Jansen, Frank |
| Grupo | 1 CRS-CCR-INPE-MCT-BR 2 3 DGE-CEA-INPE-MCT-BR 4 DAE-CEA-INPE-MCT-BR 5 DGE-CEA-INPE-MCT-BR 6 DGE-CEA-INPE-MCT-BR 7 8 CRS-CCR-INPE-MCT-BR 9 CRS-CCR-INPE-MCT-BR 10 11 DGE-CEA-INPE-MCT-BR 12 13 CRS-CCR-INPE-MCT-BR 14 15 16 CRS-CCR-INPE-MCT-BR |
| Afiliação | 1 Instituto Nacional de Pesquisas Espaciais (INPE) 2 Shinshu University 3 Instituto Nacional de Pesquisas Espaciais (INPE) 4 Instituto Nacional de Pesquisas Espaciais (INPE) 5 Instituto Nacional de Pesquisas Espaciais (INPE) 6 Instituto Nacional de Pesquisas Espaciais (INPE) 7 Instituto Nacional de Pesquisas Espaciais (INPE) 8 Instituto Nacional de Pesquisas Espaciais (INPE) 9 Instituto Nacional de Pesquisas Espaciais (INPE) 10 Santa Maria Space Science Laboratory -LACESM/CT-UFSM 11 Instituto Nacional de Pesquisas Espaciais (INPE) 12 Instituto Nacional de Pesquisas Espaciais (INPE) 13 Instituto Nacional de Pesquisas Espaciais (INPE) 14 Instituto Nacional de Pesquisas Espaciais (INPE) 15 Instituto Nacional de Pesquisas Espaciais (INPE) 16 Instituto Nacional de Pesquisas Espaciais (INPE) 17 Shinshu University 18 Shinshu University 19 Solar-Terrestrial Environment Laboratory, Nagoya University 20 Bartol Research Institute, Univ Delaware 21 University of Delaware 22 University of Delaware 23 Australian Antarctic Division 24 University of Tasmania 25 Yerevan Physics Institute 26 Kuwait University, BA DLR, Institute of Space Systems |
| Endereço de e-Mail | lise@dpi.inpe.br |
| Nome do Evento | 38th COSPAR Scientific Assembly |
| Data | n/a 1, 2010 |
| Volume | 38 |
| Páginas | 4252 |
| Histórico (UTC) | 2011-03-22 13:41:36 :: administrator -> lise@dpi.inpe.br :: 2011-09-13 12:42:37 :: lise@dpi.inpe.br -> administrator :: 2010 2018-06-05 04:35:37 :: administrator -> marciana :: 2010 |
| 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 | Space weather forecasting is a very important tool for the space situational awareness to the space objects, the space environment and related threats and risks for manned and non-manned spacecrafts. The global network of ground based multi-directional detectors (GMDN) can be considered as one example of an important emerging Space Situational Awareness program around the world, since its requirements needs global technical, scientific and logistic collab-oration between several countries in different continents. ICMEs accompanied by a strong shock often forms a high-energy galactic cosmic rays (GCRs) depleted region behind the shock known as a Forbush decrease. The ICME arrival also causes a systematic variation in the GCR streaming (i.e. the directional anisotropy of intensity). The magnitude of the streaming is small (about 1 % or less), but its variation is relevant. Some particles from this suppressed density region traveling with about the speed of light leak into the upstream region, much faster than the approaching shock, creating the possibility of being observed at the earth, by a global net-work of ground based multi-directional detectors (GMDN), as precursory loss-cone anisotropy. Loss-cones are typically visible 4-8 hours ahead of shock arrival for shocks associated with ma-jor geomagnetic storms. A multi-directional muon detector for detection of GCR was installed in 2001, 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, (29.4° S, 53.8° W, 480m a.s.l), Sao Martinho da Serra, RS, in southern Brazil. The detector's capability and sensitivity were upgraded in 2005. The observations conducted by this detector are used for forecasting the arrival of the geomagnetic storm and their interplanetary coronal mass ejec-tion (ICME) drivers in the near-earth geospace. The detector measures high-energy GCRs by detecting secondary muons produced from the hadronic interactions of primary GCRs (mostly protons) with atmospheric nuclei. Since muons have a relatively long life-time (about 2.2 mi-croseconds at rest) and can reach the detector at ground level preserving the incident direction of primary particles, the detector can measure the GCRs intensity in various directions with a multidirectional detector at a single location, such as in Brazil. The Brazilian muon detector (MD), at SSO, is a part of the GMDN, an international collaboration consisting of 10 insti-tutions from 6 countries, with real time data generated by the GMDN, which was developed at Shinshu University, Japan. With the expectation of the approval by European Commission of the NESTEC (NExt generation Space TEChnology) Project, the GMDN may be upgrade in 2010 including new muon detectors in Bremen, Germany and in Hermanus, South Africa. Therefore the ICMEs traveling in the interplanetary space and reaching the Earth -cause re-duction in cosmic ray counts at the Earth by one to ten percent, and can be detected sometimes as much as ten hours before their arrival at Earth -with the GMDN, thus permitting accurate and reliable Space Weather forecasting and for the space situational awareness. |
| Área | CEA |
| Arranjo 1 | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAE > The Global Muon... |
| Arranjo 2 | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > The Global Muon... |
| Arranjo 3 | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > CRCRS > The Global Muon... |
| 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://urlib.net/ibi/8JMKD3MGP7W/39CMNCN |
| URL dos dados zipados | http://urlib.net/zip/8JMKD3MGP7W/39CMNCN |
| Idioma | en |
| Arquivo Alvo | schuch_global.pdf |
| Grupo de Usuários | administrator lise@dpi.inpe.br |
| Visibilidade | shown |
| Permissão de Leitura | allow from all |
| Permissão de Atualização | não transferida |
| 5. Fontes relacionadas | |
| Unidades Imediatamente Superiores | 8JMKD3MGPCW/3ETL868 8JMKD3MGPCW/3EU29DP 8JMKD3MGPCW/3EUFCFP |
| Lista de Itens Citando | sid.inpe.br/bibdigital/2013/09.29.20.43 5 |
| URL (dados não confiáveis) | http://adsabs.harvard.edu/abs/2010cosp...38.4252S |
| Acervo Hospedeiro | sid.inpe.br/mtc-m19@80/2009/08.21.17.02 |
| 6. Notas | |
| Campos Vazios | archivingpolicy archivist booktitle callnumber conferencelocation copyholder copyright creatorhistory descriptionlevel dissemination doi edition editor electronicmailaddress format isbn issn keywords lineage mark mirrorrepository nextedition notes numberofvolumes orcid organization parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress readergroup resumeid rightsholder schedulinginformation secondarydate secondarykey secondarymark serieseditor shorttitle sponsor subject tertiarymark tertiarytype type |
| 7. Controle da descrição | |
| e-Mail (login) | marciana |
| atualizar | |