1. Identificação | |
Tipo de Referência | Artigo em Revista Científica (Journal Article) |
Site | plutao.sid.inpe.br |
Código do Detentor | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identificador | 8JMKD3MGP3W/3HEJGFB |
Repositório | sid.inpe.br/plutao/2014/11.21.17.48 (acesso restrito) |
Última Atualização | 2015:02.11.11.25.01 (UTC) administrator |
Repositório de Metadados | sid.inpe.br/plutao/2014/11.21.17.48.31 |
Última Atualização dos Metadados | 2018:06.04.23.39.33 (UTC) administrator |
DOI | 10.1186/s40623-014-0151-5 |
ISSN | 1343-8832 |
Rótulo | self-archiving-INPE-MCTI-GOV-BR |
Chave de Citação | KozaiMKKBERLSTDHSJSK:2014:SpDeGr |
Título | The spatial density gradient of galactic cosmic rays and its solar cycle variation observed with the Global Muon Detector Network |
Ano | 2014 |
Data de Acesso | 11 maio 2024 |
Tipo de Trabalho | journal article |
Tipo Secundário | PRE PI |
Número de Arquivos | 1 |
Tamanho | 693 KiB |
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2. Contextualização | |
Autor | 1 Kozai, Masayoshi 2 Munakata, Kazuoki 3 Kato, Chihiro 4 Kuwabara, Takao 5 Bieber, John W 6 Evenson, Paul 7 Rockenbach, Marlos 8 Lago, Alisson Dal 9 Schuch, Nelson Jorge 10 Tokumaru, Munetoshi 11 Duldig, Marcus L 12 Humble, John E 13 Sabbah, Ismail 14 Jassar, Hala K Al 15 Sharma, Madan M 16 Kóta, Jozsef |
Identificador de Curriculo | 1 2 3 4 5 6 7 8 8JMKD3MGP5W/3C9JGH3 9 8JMKD3MGP5W/3C9JHUD |
Grupo | 1 2 3 4 5 6 7 8 DGE-CEA-INPE-MCTI-GOV-BR 9 CRS-CCR-INPE-MCTI-GOV-BR |
Afiliação | 1 2 3 4 5 6 7 8 Instituto Nacional de Pesquisas Espaciais (INPE) 9 Instituto Nacional de Pesquisas Espaciais (INPE) |
Endereço de e-Mail do Autor | 1 2 3 4 5 6 7 8 alisson.dallago@inpe.br 9 njschuch@lacesm.ufsm.br |
Endereço de e-Mail | marcelo.pazos@inpe.br |
Revista | Earth, Planets and Space |
Volume | 66 |
Número | 151 |
Páginas | 1-8 |
Nota Secundária | B1_GEOCIÊNCIAS B1_ENGENHARIAS_I B1_ANTROPOLOGIA_/_ARQUEOLOGIA B4_ASTRONOMIA_/_FÍSICA B4_SOCIOLOGIA |
Histórico (UTC) | 2014-11-21 17:48:31 :: marlosrs -> administrator :: 2018-06-04 23:39:33 :: administrator -> marcelo.pazos@inpe.br :: 2014 |
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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 | Diurnal anisotropy North-south anisotropy Heliospheric modulation of galactic cosmic rays Solar cycle variation of the cosmic ray density gradient |
Resumo | We derive the long-term variation of the three-dimensional (3D) anisotropy of approximately 60 GV galactic cosmic rays (GCRs) from the data observed with the Global Muon Detector Network (GMDN) on an hourly basis and compare it with the variation deduced from a conventional analysis of the data recorded by a single muon detector at Nagoya in Japan. The conventional analysis uses a north-south (NS) component responsive to slightly higher rigidity (approximately 80 GV) GCRs and an ecliptic component responsive to the same rigidity as the GMDN. In contrast, the GMDN provides all components at the same rigidity simultaneously. It is confirmed that the temporal variations of the 3D anisotropy vectors including the NS component derived from two analyses are fairly consistent with each other as far as the yearly mean value is concerned. We particularly compare the NS anisotropies deduced from two analyses statistically by analyzing the distributions of the NS anisotropy on hourly and daily bases. It is found that the hourly mean NS anisotropy observed by Nagoya shows a larger spread than the daily mean due to the local time-dependent contribution from the ecliptic anisotropy. The NS anisotropy derived from the GMDN, on the other hand, shows similar distribution on both the daily and hourly bases, indicating that the NS anisotropy is successfully observed by the GMDN, free from the contribution of the ecliptic anisotropy. By analyzing the NS anisotropy deduced from neutron monitor (NM) data responding to lower rigidity (approximately 17 GV) GCRs, we qualitatively confirm the rigidity dependence of the NS anisotropy in which the GMDN has an intermediate rigidity response between NMs and Nagoya. From the 3D anisotropy vector (corrected for the solar wind convection and the Compton-Getting effect arising from the Earths orbital motion around the Sun), we deduce the variation of each modulation parameter, i.e., the radial and latitudinal density gradients and the parallel mean free path for the pitch angle scattering of GCRs in the turbulent interplanetary magnetic field. We show the derived density gradient and mean free path varying with the solar activity and magnetic cycles. |
Área | CEA |
Arranjo 1 | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > The spatial density... |
Arranjo 2 | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > CRCRS > The spatial density... |
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 | Kozai_Spatial.pdf |
Grupo de Usuários | marcelo.pazos@inpe.br marlosrs |
Grupo de Leitores | administrator marcelo.pazos@inpe.br |
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 | |
Vinculação | Trabalho não Vinculado à Tese/Dissertação |
Repositório Espelho | iconet.com.br/banon/2006/11.26.21.31 |
Unidades Imediatamente Superiores | 8JMKD3MGPCW/3EU29DP 8JMKD3MGPCW/3EUFCFP |
Lista de Itens Citando | sid.inpe.br/bibdigital/2013/10.01.22.11 1 |
Divulgação | WEBSCI; PORTALCAPES; SCOPUS. |
Acervo Hospedeiro | dpi.inpe.br/plutao@80/2008/08.19.15.01 |
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6. Notas | |
Campos Vazios | alternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel format isbn lineage mark month nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject tertiarytype url |
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7. Controle da descrição | |
e-Mail (login) | marcelo.pazos@inpe.br |
atualizar | |
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