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Metadados

1. Identificação
Tipo de ReferênciaArtigo em Evento (Conference Proceedings)
Siteplutao.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador8JMKD3MGP3W/3KBB3R8
Repositóriosid.inpe.br/plutao/2015/09.29.17.43   (acesso restrito)
Última Atualização2015:09.29.17.56.03 (UTC) administrator
Repositório de Metadadossid.inpe.br/plutao/2015/09.29.17.43.28
Última Atualização dos Metadados2018:06.04.23.39.46 (UTC) administrator
Rótuloself-archiving-INPE-MCTI-GOV-BR
Chave de CitaçãoKozaiMKSKBERLSTDHSASK:2013:SpDeGr
TítuloThe spatial density gradient of galactic cosmic rays and its solar cycle variation observed with the Global Muon Detector Network
Ano2013
Data de Acesso10 maio 2024
Tipo SecundárioPRE CI
Número de Arquivos1
Tamanho176 KiB
2. Contextualização
Autor 1 Kozai, Masayoshi
 2 Munakata, Kazuoki
 3 Kato, Chihiro
 4 S. , Yasue
 5 Kuwabara, Takao
 6 Bieber, John W.
 7 Evenson, Paul
 8 Rockenbach, Marlos
 9 Lago, Alisson Dal
10 Schuch, Nelson Jorge
11 Tokumaru, Munetoshi
12 Duldig, Marcus L.
13 Humble, John E.
14 Sabbah, Ismail
15 Al Jassar, Hala K.
16 Sharma, Madan M.
17 Kóta, Jozsef
Identificador de Curriculo 1
 2
 3
 4
 5
 6
 7
 8
 9 8JMKD3MGP5W/3C9JGH3
10 8JMKD3MGP5W/3C9JHUD
Grupo 1
 2
 3
 4
 5
 6
 7
 8
 9 DGE-CEA-INPE-MCTI-GOV-BR
10 CRS-CCR-INPE-MCTI-GOV-BR
Afiliação 1
 2
 3
 4
 5
 6
 7
 8
 9 Instituto Nacional de Pesquisas Espaciais (INPE)
10 Instituto Nacional de Pesquisas Espaciais (INPE)
Endereço de e-Mail do Autor 1
 2
 3
 4
 5
 6
 7
 8
 9 alisson.dallago@inpe.br
10 njschuch@lacesm.ufsm.br
Endereço de e-Mailmarcelo.pazos@inpe.br
Nome do EventoInternational Cosmic Ray Conference, 33. The Astroparticle Physics Conference.
Localização do EventoRio De Janeiro
Páginas4pp
Nota SecundáriaB1_GEOCIÊNCIAS B1_ENGENHARIAS_I B1_ANTROPOLOGIA_/_ARQUEOLOGIA B4_ASTRONOMIA_/_FÍSICA B4_SOCIOLOGIA
Histórico (UTC)2015-09-29 17:43:28 :: marcelo.pazos@sid.inpe.br -> administrator ::
2015-09-29 17:56:03 :: administrator :: 2014 -> 2013
2018-06-04 23:39:46 :: administrator -> marcelo.pazos@inpe.br :: 2013
3. Conteúdo e estrutura
É a matriz ou uma cópia?é a matriz
Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
Tipo de Versãopublisher
Palavras-Chavediurnal anisotropy
north-south anisotropy
heliospheric modulation of galactic cosmic rays
solar cycle variation of the cosmic ray density gradient
ResumoWe 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.
ÁreaCEA
Tipojournal article
Arranjo 1urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > The spatial density...
Arranjo 2urlib.net > BDMCI > Fonds > Produção anterior à 2021 > CRCRS > The spatial density...
Conteúdo da Pasta docacessar
Conteúdo da Pasta sourcenão têm arquivos
Conteúdo da Pasta agreement
agreement.html 29/09/2015 14:43 1.0 KiB 
4. Condições de acesso e uso
Idiomaen
Arquivo AlvoThe spatial density gradient of galactic.pdf
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Permissão de Leituradeny from all and allow from 150.163
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5. Fontes relacionadas
VinculaçãoTrabalho não Vinculado à Tese/Dissertação
Repositório Espelhoiconet.com.br/banon/2006/11.26.21.31
Unidades Imediatamente Superiores8JMKD3MGPCW/3EU29DP
8JMKD3MGPCW/3EUFCFP
Acervo Hospedeirodpi.inpe.br/plutao@80/2008/08.19.15.01
6. Notas
Campos Vaziosarchivist booktitle callnumber copyholder copyright creatorhistory date descriptionlevel dissemination doi edition editor format isbn issn lineage mark nextedition notes numberofvolumes orcid organization parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress rightsholder schedulinginformation secondarydate secondarykey serieseditor session shorttitle sponsor subject tertiarytype url volume
7. Controle da descrição
e-Mail (login)marcelo.pazos@inpe.br
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