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		<doi>10.1007/s11214-014-0048-4</doi>
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		<citationkey>RockenbachDSMKOEBMKKTBEDHJSS:2014:GlMuDe</citationkey>
		<title>Global Muon Detector Network used for space weather applications</title>
		<year>2014</year>
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		<secondarytype>PRE PI</secondarytype>
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		<author>Rockenbach, Marlos,</author>
		<author>Dal Lago, Alisson,</author>
		<author>Schuch, Nelson Jorge,</author>
		<author>Munakata, K.,</author>
		<author>Kuwabara, T.,</author>
		<author>Oliveira, A. G.,</author>
		<author>Echer, Ezequiel,</author>
		<author>Braga, Carlos Roberto,</author>
		<author>Mendonça, Rafael Rodrigues Souza de,</author>
		<author>Kato, C.,</author>
		<author>Kozai, M.,</author>
		<author>Tokumaru, M.,</author>
		<author>Bieber, J. W.,</author>
		<author>Evenson, P.,</author>
		<author>Duldig, M. L.,</author>
		<author>Humble, J. E.,</author>
		<author>Jassar, H. K. Al,</author>
		<author>Sharma, M. M.,</author>
		<author>Sabbah, I.,</author>
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		<affiliation>Instituto Nacional de Pesquisas Espaciais (INPE)</affiliation>
		<affiliation>Instituto Nacional de Pesquisas Espaciais (INPE)</affiliation>
		<affiliation>Instituto Nacional de Pesquisas Espaciais (INPE)</affiliation>
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		<affiliation></affiliation>
		<affiliation>Instituto Nacional de Pesquisas Espaciais (INPE)</affiliation>
		<affiliation>Instituto Nacional de Pesquisas Espaciais (INPE)</affiliation>
		<affiliation>Instituto Nacional de Pesquisas Espaciais (INPE)</affiliation>
		<electronicmailaddress></electronicmailaddress>
		<electronicmailaddress>alisson.dallago@inpe.br</electronicmailaddress>
		<electronicmailaddress>njschuch@lacesm.ufsm.br</electronicmailaddress>
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		<e-mailaddress>marcelo.pazos@inpe.br</e-mailaddress>
		<journal>Space Science Reviews</journal>
		<volume>180/1-4</volume>
		<secondarymark>A1_ENGENHARIAS_III A1_GEOCIÊNCIAS A2_ASTRONOMIA_/_FÍSICA A2_ENGENHARIAS_IV</secondarymark>
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		<keywords>space weather, cosmic ray precursors, cosmic ray anisotropy, Global Muon Detector Network.</keywords>
		<abstract>In this work, we summarize the development and current status of the Global Muon Detector Network (GMDN). The GMDN started in 1992 with only two muon detectors. It has consisted of four detectors since the Kuwait-city muon hodoscope detector was installed in March 2006. The present network has a total of 60 directional channels with an improved coverage of the sunward Interplanetary Magnetic Field (IMF) orientation, making it possible to continuously monitor cosmic ray precursors of geomagnetic storms. The data analysis methods developed also permit precise calculation of the three dimensional cosmic ray anisotropy on an hourly basis free from the atmospheric temperature effect and analysis of the cosmic ray precursors free from the diurnal anisotropy of the cosmic ray intensity.</abstract>
		<area>CEA</area>
		<language>en</language>
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