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1. Identity statement
Reference TypeConference Paper (Conference Proceedings)
Sitemtc-m16d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP7W/36KUDB8
Repositorysid.inpe.br/mtc-m19@80/2009/12.23.22.04   (restricted access)
Last Update2010:01.20.22.51.18 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m19@80/2009/12.23.22.04.56
Metadata Last Update2018:06.05.04.36.08 (UTC) administrator
Citation KeyGramsBrKaEcMu:2009:PrStSt
TitlePreliminary statistical study of the directional intensity of cosmic ray muons observed at the brazilian southern space observatory
Year2009
Access Date2024, May 02
Secondary TypePRE CI
Number of Files2
Size30 KiB
2. Context
Author1 Grams, Guilherme
2 Nelson Jorge Schuch
3 Braga, Carlos Roberto
4 Kane, Rajaram Purushottam
5 Echer, Ezequiel
6 Munakata, Kazuoki
Resume Identifier1
2
3
4 8JMKD3MGP5W/3C9JJ4U
5 8JMKD3MGP5W/3C9JH3D
Group1 CRS-CCR-INPE-MCT-BR
2 CRS-CCR-INPE-MCT-BR
3
4 DGE-CEA-INPE-MCT-BR
5 DGE-CEA-INPE-MCT-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3
4 Instituto Nacional de Pesquisas Espaciais (INPE)
5 Instituto Nacional de Pesquisas Espaciais (INPE)
Conference Name60th International Astronautical Congress - IAU
Conference LocationRio de Janeiro, RS
DateAugust, 13-14
History (UTC)2010-01-21 04:03:31 :: seeger5 -> administrator ::
2018-06-05 04:36:08 :: administrator -> seeger5 :: 2009
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
AbstractCosmic rays are high-energy particles with source in the interstellar space. When these impinge the top of the atmosphere, interact with atmospheric constituents, producing secondary particles. Among them are the muons that have a huge penetration capacity and maintain the incident direction of the primary cosmic rays. A multi-directional telescope (MDT) for detection of high-energy galactic cosmic rays (GCRs) - muons was installed in 2001 and upgraded in 2005, through an international cooperation between Brazil, Japan and USA, and operated since then at the Southern Space Observatory - SSO/CRS/INPE - MCT, (29,4ºS, 53,8ºW, 480m), Sao Martinho da Serra, RS, in the South of Brazil. This telescope is a component detector of the Global Muon Detector Network (GMDN), which has been developed in an international collaboration lead by Shinshu University, Japan. The main objective of this work is to study the directional intensity of muons, which are produced by primary cosmic rays with energy between 50 GeV and 170 GeV and observed at the Earths surface. We analyze the data collected by the muon detector telescope MDT at the SSO in 2006 and 2007. The Telescope consists of two layers of 4x7 detectors with a total observation area of 28 square meters. The counting of muons in each directional channel is made by a coincidence of pair of pulses, one from a detector in the upper layer and the other from a detector in the lower layer. The SSOs MDT equipped with 119 directional channels for muon count rate measurement is capable of detecting muons incident with the zenith angle between 0º and 75,53º. A statistical analysis was made with the MDT muon count rate for all the directional channels. The average and the standard deviation of the muon count rate in each directional component are calculated to deduce the zenith angle dependence of the rate. Preliminary results have shown lower (higher) count rate with larger (smaller) zenith angle, as expected from the production and propagation of muons in the atmosphere.
AreaCEA
Arrangement 1urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Preliminary statistical study...
Arrangement 2urlib.net > BDMCI > Fonds > Produção anterior à 2021 > CRCRS > Preliminary statistical study...
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source Directory Contentthere are no files
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4. Conditions of access and use
Languageen
Target FileAbstract IAU-2009_Guilherme_Grams.pdf
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5. Allied materials
Mirror Repositorysid.inpe.br/mtc-m19@80/2009/08.21.17.02.53
Next Higher Units8JMKD3MGPCW/3EU29DP
8JMKD3MGPCW/3EUFCFP
Host Collectionsid.inpe.br/mtc-m19@80/2009/08.21.17.02
6. Notes
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