Fechar

1. Identificação
Tipo de ReferênciaArtigo em Evento (Conference Proceedings)
Siteplutao.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
IdentificadorJ8LNKAN8RW/3ARNSJ4
Repositóriodpi.inpe.br/plutao/2011/11.23.20.54.38
Última Atualização2012:01.20.18.11.34 (UTC) secretaria.cpa@dir.inpe.br
Repositório de Metadadosdpi.inpe.br/plutao/2011/11.23.20.54.39
Última Atualização dos Metadados2018:06.05.00.01.40 (UTC) administrator
Rótulolattes: 0549130828972280 10 KozaiMKYKBERLSTDHSAS:2011:AvSpDe
Chave de CitaçãoKozaiMKYKBERLSTDHSASK:2011:AvSpDe
TítuloThe average spatial density gradient of galactic cosmic rays and its temporal variation observed with the Global Muon Detector Network (GMDN)
FormatoDVD
Ano2011
Data de Acesso12 maio 2024
Tipo SecundárioPRE CI
Número de Arquivos1
Tamanho300 KiB
2. Contextualização
Autor 1 Kozai, M.
 2 Munakata, Kazuoki
 3 Kato, Chihiro
 4 Yasue, Shin-ichi
 5 Kuwabara, Takao
 6 Bieber, John W.
 7 Evenson, P.
 8 Rockenbach, Marlos
 9 Lago, Alisson Dal
10 Schuch, Nelson Jorge
11 Tokumaru, Munetoshi
12 Duldig, M. D.
13 Humble, J. E.
14 Sabbah, Ismail
15 Al Jassar, H. K.
16 Sharma, M. M.
17 Kota, J.
Grupo 1
 2
 3
 4
 5
 6
 7
 8
 9 DGE-CEA-INPE-MCT-BR
10 CRS-CCR-INPE-MCT-BR
Afiliação 1 Physics Department, Shinshu University, Matsumoto, Nagano 390-8621, Japan.
 2 Physics Department, Shinshu University, Matsumoto, Nagano 390-8621, Japan.
 3 Physics Department, Shinshu University, Matsumoto, Nagano 390-8621, Japan.
 4 Physics Department, Shinshu University, Matsumoto, Nagano 390-8621, Japan.
 5 Bartol Research Institute and Department of Physics and Astronomy, University of Delaware Newark, DE 19716, USA
 6 Bartol Research Institute and Department of Physics and Astronomy, University of Delaware Newark, DE 19716, USA
 7 Bartol Research Institute and Department of Physics and Astronomy, University of Delaware Newark, DE 19716, USA
 8 Universidade do Vale do Paraíba(UNIVAP), 12244-000, São José dos Campos, SP, Brazil
 9 Instituto Nacional de Pesquisas Espaciais (INPE)
10 Instituto Nacional de Pesquisas Espaciais (INPE)
11 Solar Terrestrial Environment Laboratory, Nagoya University, Nagoya, Aichi 464-8601, Japan
12 School of Mathematics and Physics, University of Tasmania, Hobart, Tasmania 7001, Australia
13 School of Mathematics and Physics, University of Tasmania, Hobart, Tasmania 7001, Australia
14 Department of Natural Sciences, College of Health Sciences, Public Authority of Applied Education and Training, Kuwait.
15 Physics Department, Kuwait University, Kuwait 13060
16 Physics Department, Kuwait University, Kuwait 13060
17 Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721, USA.
Endereço de e-Mail do Autor 1
 2
 3
 4
 5
 6
 7
 8
 9
10 njschuch@lacesm.ufsm.br
Endereço de e-Mailnjschuch@lacesm.ufsm.br
Nome do EventoInternational Cosmic Ray Conference, 32.
Localização do EventoBeijing, China
Data11-18 Aug
Título do LivroAnais
Tipo TerciárioArtigo
Histórico (UTC)2011-11-24 11:03:17 :: lattes -> secretaria.cpa@dir.inpe.br :: 2011
2012-02-24 02:24:39 :: secretaria.cpa@dir.inpe.br -> administrator :: 2011
2018-06-05 00:01:40 :: administrator -> ana.silveira :: 2011
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
Solar cycle variation of the cosmic-ray density gradient
Heliospheric modulation of galactic cosmic rays
ResumoWe deduce the spatial gradient of galactic cosmic rays in three dimensions from the fist order anisotropy observed with the Global Muon Detector Network. The anisotropy vector is first corrected for the solar wind convection and the Compton-Getting effect arising from the solar wind and the Earths orbital motion around the Sun. We then convert the component anisotropy perpendicular to the interplanetary magnetic field to the spatial density gradient by assuming that the perpendicular anisotropy is mainly due to the diamagnetic streaming. In this paper, we analyze the solar cycle variation of the gradient observed with the GMDN during ten years between 2001 and 2010 and show that the derived density gradient is clearly decreasing with increasing solar activity toward the solar activity minimum in 20082009. We also find a clear seasonal variation in each of the radial and longitudinal component of the gradient vector in a close correlation with the heliographic latitude of the Earth. The amplitude of this seasonal variation also decreases with the increasing solar activity. We discuss the origin of this seasonal variation in terms of the global distribution of cosmic-ray density in the heliosphere.
ÁreaCEA
Arranjo 1urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > The average spatial...
Arranjo 2urlib.net > BDMCI > Fonds > Produção anterior à 2021 > CRCRS > The average spatial...
Conteúdo da Pasta docacessar
Conteúdo da Pasta sourcenão têm arquivos
Conteúdo da Pasta agreementnão têm arquivos
4. Condições de acesso e uso
URL dos dadoshttp://urlib.net/ibi/J8LNKAN8RW/3ARNSJ4
URL dos dados zipadoshttp://urlib.net/zip/J8LNKAN8RW/3ARNSJ4
Idiomapt
Arquivo AlvoKozai-icrc0376[1].pdf
Grupo de Usuárioslattes
secretaria.cpa@dir.inpe.br
Visibilidadeshown
Permissão de Leituraallow from all
Permissão de Atualizaçãonão transferida
5. Fontes relacionadas
Unidades Imediatamente Superiores8JMKD3MGPCW/3EU29DP
8JMKD3MGPCW/3EUFCFP
Lista de Itens Citandosid.inpe.br/bibdigital/2013/10.01.22.11 1
URL (dados não confiáveis)http://icrc2011.ihep.ac.cn/
Acervo Hospedeirodpi.inpe.br/plutao@80/2008/08.19.15.01
6. Notas
Campos Vaziosarchivingpolicy archivist callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi edition editor isbn issn lineage mark mirrorrepository nextedition notes numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress readergroup resumeid rightsholder schedulinginformation secondarydate secondarykey secondarymark serieseditor session shorttitle sponsor subject tertiarymark type volume
7. Controle da descrição
e-Mail (login)ana.silveira
atualizar 


Fechar