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1. Identificação
Tipo de ReferênciaArtigo em Revista Científica (Journal Article)
Siteplutao.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
IdentificadorJ8LNKAN8RW/3E7UE8S
Repositóriodpi.inpe.br/plutao/2013/05.31.17.14.30   (acesso restrito)
Última Atualização2013:07.15.12.31.05 (UTC) administrator
Repositório de Metadadosdpi.inpe.br/plutao/2013/05.31.17.14.31
Última Atualização dos Metadados2022:03.18.22.15.27 (UTC) administrator
DOI10.1088/1742-6596/409/1/012137
ISSN1742-6588
Rótulolattes: 4050318480364899 1 BragaCampSchuLago:2013:PrCoRe
Chave de CitaçãoBragaCampSchuLago:2013:PrCoRe
TítuloA proposal of a counting and recording system for cosmic ray muon detectors
Ano2013
Data de Acesso28 abr. 2024
Tipo SecundárioPRE PI
Número de Arquivos1
Tamanho452 KiB
2. Contextualização
Autor1 Braga, Carlos Roberto
2 Campos, A
3 Schuch, N J
4 Lago, Alisson Dal
Identificador de Curriculo1
2
3
4 8JMKD3MGP5W/3C9JGH3
Grupo1 GESATM-CEA-SPG-INPE-MCTI-GOV-BR
2
3 CRS-CCR-INPE-MCTI-GOV-BR
4 CRS-CCR-INPE-MCTI-GOV-BR
Afiliação1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Technology Center, Federal University of Santa Maria, Santa Maria, RS, Brazil
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 Instituto Nacional de Pesquisas Espaciais (INPE)
Endereço de e-Mail do Autor1 crbraga@dge.inpe.br
2
3 njschuch@lacesm.ufsm.br
4 dallago@dge.inpe.br
Endereço de e-Mailcrbraga@dge.inpe.br
RevistaJournal of Physics: Conference Series
Volume409
Número1
PáginasArticle number 012137
Nota SecundáriaB2 B2 B3 B5 B5 C C C C
Histórico (UTC)2013-05-31 17:14:31 :: lattes -> administrator ::
2022-03-18 22:15:27 :: 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-Chaveenergy cosmic ray
muon
Global Muon Detector Network (GMDN)
Space Weather
ResumoA multidirecional high energy cosmic ray (muon) telescope is operational at the Southern Space Observatory, in Sao Martinho da Serra, RS, Brazil. This telescope is part of the Global Muon Detector Network (GMDN) and aims to study and forecast Space Weather. This paper proposes a new counting, correlation and recording solution based on an embedded system able to interface observational data by internet for remote monitoring. It is built around a Rabbit 3000 microcontroller with TCP/IP Ethernet 10Base-T connectivity. It is able to detect and count 200 ns pulses generated by the sensor system (scintillator plastics coupled with photomultipliers) during a specified period of time (generally one second). A preliminary version of a monitoring web page was developed and it is able to show the cosmic ray (muon) data of one detector in real time. The current system is an attempt to improve the reliability of the telescope when comparing to the recording system based on a personal computer, currently under operation. One advantage is the easy maintenance, since all the counting and correlation boards currently under operation can be replaced by an embedded system. Besides, as the hardware is off-the-shelf, it is only necessary to develop software routines, which is based on royalty-free libraries. 1. Introduction The multidirectional muon telescope of Sao Martinho da Serra (Brazil) is installed in Southern Space Observatory (geographic coordinates: 29.4º S, 53.8º W, 488 m). It has detection area of 28 m 2 and is multidirectional, allowing simultaneous record of the intensities in various directions of viewing. This detector has an identical design to other detectors installed in Nagoya (geographic coordinates 35.1ºN, 137.0º E, 77 m) and Hobart (43.0ºS, 147.3º E, 65 m), except for the detection area which is 36 m 2 for Nagoya and 16 m 2 for Hobart [2]. These detectors, combined with a muon hodoscope installed in Kuwait City, are part of a network called Global Muon Detector Network [1]. It has been shown that combining data of all stations allows the determination of the spatial gradient of the galactic cosmic ray density in three-dimensions and, therefore, to study precursors of geomagnetic storms [3,4], magnetic cloud geometry [5] and corotating interaction regions [1]. Each detector consists of two horizontal layers of plastic scintillators, vertically separated by 1.73 m, with an intermediate 5 cm layer of lead to absorb the soft component radiation in the air. Each layer comprises an array of 1 m 2 unit detectors, each with a 0.1 m thick plastic scintillator viewed by a photomultiplier tube of 12.7 cm diameter. An electronic amplifier circuit which converts the current.
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Conteúdo da Pasta agreementnão têm arquivos
4. Condições de acesso e uso
Idiomapt
Arquivo Alvo1742-6596_409_1_012137.pdf
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5. Fontes relacionadas
Repositório Espelhoiconet.com.br/banon/2006/11.26.21.31
Unidades Imediatamente Superiores8JMKD3MGPCW/3EUFCFP
8JMKD3MGPCW/3F2PBEE
DivulgaçãoWEBSCI; PORTALCAPES; SCOPUS.
Acervo Hospedeirodpi.inpe.br/plutao@80/2008/08.19.15.01
6. Notas
Notas23rd European Cosmic Ray Symposium, ECRS 2012 and 32nd Russian Cosmic Ray Conference; Moscow; Russian Federation; 3 July 2012 through 7 July 2012
Campos Vaziosalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel format isbn lineage mark month nextedition orcid parameterlist parentrepositories previousedition previouslowerunit progress project rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url
7. Controle da descrição
e-Mail (login)marcelo.pazos@inpe.br
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