1. Identificação | |
Tipo de Referência | Artigo em Evento (Conference Proceedings) |
Site | mtc-m21c.sid.inpe.br |
Código do Detentor | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identificador | 8JMKD3MGP3W34R/44CTAPS |
Repositório | sid.inpe.br/mtc-m21c/2021/03.24.11.55 |
Repositório de Metadados | sid.inpe.br/mtc-m21c/2021/03.24.11.55.01 |
Última Atualização dos Metadados | 2022:04.03.19.25.07 (UTC) administrator |
Chave Secundária | INPE--PRE/ |
Chave de Citação | VieiraDSGSCASJ:2021:INCoIn |
Título | INGV contribution to international Space Weather initiatives |
Ano | 2021 |
Data de Acesso | 04 maio 2024 |
Tipo Secundário | PRE CN |
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2. Contextualização | |
Autor | 1 Vieira, Luis Eduardo Antunes 2 Dal Lago, Alisson 3 Silva, Marlos Rockenbach da 4 Guarnieri, Fernando Luís 5 Silva, Ligia Alves da 6 Carlesso, Franciele 7 Alves, Livia Ribeiro 8 Souza, Vitor Moura Cardoso e Silva 9 Jauer, Paulo Ricardo |
Identificador de Curriculo | 1 2 8JMKD3MGP5W/3C9JGH3 |
Grupo | 1 DIHPA-CGCE-INPE-MCTI-GOV-BR 2 DIHPA-CGCE-INPE-MCTI-GOV-BR 3 DIHPA-CGCE-INPE-MCTI-GOV-BR 4 5 DIHPA-CGCE-INPE-MCTI-GOV-BR 6 DIHPA-CGCE-INPE-MCTI-GOV-BR 7 DIHPA-CGCE-INPE-MCTI-GOV-BR 8 DIHPA-CGCE-INPE-MCTI-GOV-BR |
Afiliação | 1 Instituto Nacional de Pesquisas Espaciais (INPE) 2 Instituto Nacional de Pesquisas Espaciais (INPE) 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) |
Endereço de e-Mail do Autor | 1 luis.vieira71@googlemail.com 2 alisson.dallago@inpe.br 3 marlosrs@gmail.com 4 fernando.guarnieri@gmail.com 5 ligia.alves01@gmail.com 6 fccarlesso@gmail.com 7 livia.alves@inpe.br 8 vitormoura21@gmail.com |
Nome do Evento | Simpósio Brasileiro de Geofísica Espacial e Aeronomia, 8 (SBGEA) |
Localização do Evento | Online |
Data | 22-26 mar. |
Histórico (UTC) | 2021-03-24 11:55:01 :: simone -> administrator :: 2021-06-22 19:11:15 :: administrator -> simone :: 2021 2021-06-22 21:00:58 :: simone -> administrator :: 2021 2022-04-03 19:25:07 :: administrator -> simone :: 2021 |
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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 |
Resumo | The Galileo Solar Space Telescope (GSST) is a cornerstone mission to provide accurate measurements of the magnetic field in the photosphere and outer layers of the solar atmosphere to be proposed to the Brazilian Space Agency (AEB) within the international effort to understand of the evolution of the Heliosphere. The solar electromagnetic and corpuscular emissions are strongly modulated by the evolution of the magnetic structure of the solar atmosphere. The solar magnetism is driven by the energy transport from the inner layers of the Sun to its atmosphere. Although systematic observations since the invention of the telescope have revealed several features related to the evolution of solar activity, there is not a complete explanation of the physical processes that lead to solar activity cyclic variability and its long-term changes. Here we describe the status of missions Phase 0/A. The underlying basic questions to be addressed by the GSST mission are: What are the fundamental physical/plasma processes at work in the Sun? How does the solar dynamo work? What is the relative contribution of different physical processes that lead to the heating of the outer layers (Chromosphere to Corona)? What are the effects of the magnetic structure of the outer layers of the Sun on the evolution of the Earths highly coupled atmosphere-ocean system? What is the response of the magnetic field and energetic particles in the vicinity of our planet, i.e. the Earths inner magnetosphere region, due to different solar wind structures? Taking into account these open scientific questions, the Galileo Solar Space Telescope proposed mission is to perform solar observations in high spatial and temporal resolution to characterize the evolution of the magnetic structure of the photosphere, chromosphere, transition region, and corona and its impact on the Geospace. Specifically, the mission has three main objectives: (1) Contribute to the understanding of the evolution of the magnetic structure of the Sun; (2) Contribute to the understanding of the Suns influence on Earths Climate; and, (3) Contribute to the understanding of the Suns impact on the Geospace. This contribution is an update of the previous version presented at the AGU Fall Meeting 2019. |
Área | CEA |
Arranjo | urlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > INGV contribution to... |
Conteúdo da Pasta doc | não têm arquivos |
Conteúdo da Pasta source | não têm arquivos |
Conteúdo da Pasta agreement | |
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4. Condições de acesso e uso | |
Idioma | en |
Grupo de Usuários | simone |
Grupo de Leitores | administrator simone |
Visibilidade | shown |
Permissão de Atualização | não transferida |
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5. Fontes relacionadas | |
Unidades Imediatamente Superiores | 8JMKD3MGPCW/46KTFK8 |
Acervo Hospedeiro | urlib.net/www/2017/11.22.19.04 |
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6. Notas | |
Campos Vazios | archivingpolicy archivist booktitle callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi e-mailaddress edition editor format isbn issn keywords label lineage mark mirrorrepository nextedition notes numberoffiles numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress readpermission rightsholder schedulinginformation secondarydate secondarymark serieseditor session shorttitle size sponsor subject targetfile tertiarymark tertiarytype type url versiontype volume |
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7. Controle da descrição | |
e-Mail (login) | simone |
atualizar | |
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