1. Identificação | |
Tipo de Referência | Artigo em Revista Científica (Journal Article) |
Site | mtc-m21c.sid.inpe.br |
Código do Detentor | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identificador | 8JMKD3MGP3W34R/44JA9AB |
Repositório | sid.inpe.br/mtc-m21c/2021/04.26.12.24 (acesso restrito) |
Última Atualização | 2021:04.26.12.24.43 (UTC) administrator |
Repositório de Metadados | sid.inpe.br/mtc-m21c/2021/04.26.12.24.44 |
Última Atualização dos Metadados | 2022:04.03.22.39.37 (UTC) administrator |
DOI | 10.1029/2020SW002531 |
ISSN | 1539-4956 |
Chave de Citação | KiharaMKKKMKKTMEDSSBBASDHESK:2021:PeICEv |
Título | A Peculiar ICME Event in August 2018 Observed With the Global Muon Detector Network |
Ano | 2021 |
Mês | Mar. |
Data de Acesso | 02 jan. 2025 |
Tipo de Trabalho | journal article |
Tipo Secundário | PRE PI |
Número de Arquivos | 1 |
Tamanho | 1241 KiB |
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2. Contextualização | |
Autor | 1 Kihara, W. 2 Munakata, K. 3 Kato, C. 4 Kataoka, R. 5 Kadokura, A. 6 Miyake, S. 7 Kozai, M. 8 Kuwabara, T. 9 Tokumaru, M. 10 Mendonça, R. R. S. 11 Echer, Ezequiel 12 Dal Lago, Alisson 13 Silva, Marlos Rockenbach da 14 Schuch, Nelson Jorge 15 Bageston, José Valentin 16 Braga, C. R. 17 Al Jassar, H. K. 18 Sharma, M. M. 19 Duldig, M. L. 20 Humble, J. E. 21 Evenson, P. 22 Sabbah, I. 23 Kóta, J. |
Identificador de Curriculo | 1 2 3 4 5 6 7 8 9 10 11 8JMKD3MGP5W/3C9JH3D 12 8JMKD3MGP5W/3C9JGH3 13 14 8JMKD3MGP5W/3C9JHUD |
ORCID | 1 0000-0003-1367-0727 2 0000-0002-2131-4100 3 0000-0002-4913-8225 4 0000-0001-9400-1765 5 0000-0002-6105-9562 6 0000-0002-3067-655X 7 0000-0002-3948-3666 8 0000-0001-6584-9054 9 0000-0002-2982-1887 10 0000-0002-0417-6877 11 0000-0002-8351-6779 12 0000-0002-4361-6492 13 0000-0002-9737-9429 14 0000-0002-7720-6491 15 0000-0003-2931-8488 16 0000-0003-1485-9564 17 0000-0002-4486-237X 18 19 0000-0001-7463-8267 20 0000-0002-4698-1671 21 0000-0001-7929-810X 22 0000-0002-7037-322X 23 0000-0002-3715-0358 |
Grupo | 1 2 3 4 5 6 7 8 9 10 GES-CEA-DIPGR-INPE-MCTI-GOV-BR 11 DIHPA-CGCE-INPE-MCTI-GOV-BR 12 DIHPA-CGCE-INPE-MCTI-GOV-BR 13 DIHPA-CGCE-INPE-MCTI-GOV-BR 14 COESU-CGGO-INPE-MCTI-GOV-BR 15 COESU-CGGO-INPE-MCTI-GOV-BR |
Afiliação | 1 Shinshu University 2 Shinshu University 3 Shinshu University 4 National Institute of Polar Research 5 National Institute of Polar Research 6 National Institute of Technology 7 Japan Aerospace Exploration Agency 8 Chiba University 9 Nagoya University 10 Instituto Nacional de Pesquisas Espaciais (INPE) 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 George Mason University 17 Kuwait University 18 Kuwait University 19 University of Tasmania 20 University of Tasmania 21 University of Delaware 22 College of Technological Studies 23 University of Arizona |
Endereço de e-Mail do Autor | 1 19ss204g@shinshu-u.ac.jp 2 3 4 5 6 7 8 9 10 11 ezequiel.echer@gmail.com 12 alisson.dallago@inpe.br 13 marlosrs@gmail.com 14 njschuch@gmail.com 15 jose.bageston@inpe.br |
Revista | Space Weather |
Volume | 19 |
Número | 3 |
Páginas | e2020W002531 |
Histórico (UTC) | 2021-04-26 12:24:44 :: simone -> administrator :: 2021-04-26 12:24:45 :: administrator -> simone :: 2021 2021-04-26 12:27:33 :: simone -> administrator :: 2021 2022-04-03 22:39:37 :: 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 |
Tipo de Versão | publisher |
Palavras-Chave | coronal mass ejection corotating interaction region cosmic‐
ray geomagnetic storm magnetic flux rope solar minimum |
Resumo | We demonstrate that global observations of high-energy cosmic rays contribute to understanding unique characteristics of a large-scale magnetic flux rope causing a magnetic storm in August 2018. Following a weak interplanetary shock on August 25, 2018, a magnetic flux rope caused an unexpectedly large geomagnetic storm. It is likely that this event became geoeffective because the flux rope was accompanied by a corotating interaction region and compressed by high-speed solar wind following the flux rope. In fact, a Forbush decrease was observed in cosmic-ray data inside the flux rope as expected, and a significant cosmic-ray density increase exceeding the unmodulated level before the shock was also observed near the trailing edge of the flux rope. The cosmic-ray density increase can be interpreted in terms of the adiabatic heating of cosmic rays near the trailing edge of the flux rope, as the corotating interaction region prevents free expansion of the flux rope and results in the compression near the trailing edge. A northeast-directed spatial gradient in the cosmic-ray density was also derived during the cosmic-ray density increase, suggesting that the center of the heating near the trailing edge is located northeast of Earth. This is one of the best examples demonstrating that the observation of high-energy cosmic rays provides us with information that can only be derived from the cosmic ray measurements to observationally constrain the three-dimensional macroscopic picture of the interaction between coronal mass ejections and the ambient solar wind, which is essential for prediction of large magnetic storms. |
Área | CEA |
Arranjo 1 | urlib.net > BDMCI > Fonds > Produção pgr ATUAIS > GES > A Peculiar ICME... |
Arranjo 2 | urlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > A Peculiar ICME... |
Arranjo 3 | urlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGGO > A Peculiar ICME... |
Conteúdo da Pasta doc | acessar |
Conteúdo da Pasta source | não têm arquivos |
Conteúdo da Pasta agreement | |
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4. Condições de acesso e uso | |
Idioma | en |
Arquivo Alvo | kihara_peculiar.pdf |
Grupo de Usuários | simone |
Grupo de Leitores | administrator simone |
Visibilidade | shown |
Política de Arquivamento | denypublisher denyfinaldraft |
Permissão de Leitura | deny from all and allow from 150.163 |
Permissão de Atualização | não transferida |
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5. Fontes relacionadas | |
Unidades Imediatamente Superiores | 8JMKD3MGPCW/3F2PBEE 8JMKD3MGPCW/46KTFK8 8JMKD3MGPCW/46KUBT5 |
Lista de Itens Citando | sid.inpe.br/mtc-m21/2012/07.13.14.39.46 9 sid.inpe.br/bibdigital/2022/04.03.22.35 9 sid.inpe.br/bibdigital/2013/10.12.21.02 6 |
Divulgação | WEBSCI |
Acervo Hospedeiro | urlib.net/www/2017/11.22.19.04 |
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6. Notas | |
Campos Vazios | alternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn label lineage mark mirrorrepository nextedition notes parameterlist parentrepositories previousedition previouslowerunit progress project rightsholder schedulinginformation secondarydate secondarykey secondarymark session shorttitle sponsor subject tertiarymark tertiarytype url |
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7. Controle da descrição | |
e-Mail (login) | simone |
atualizar | |
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