@Article{SavianSLEVMGSAS:2007:FoDeNo,
               author = "Savian, Jairo Francisco and Silva, Marlos Rockenbach da and Lago, 
                         Alisson Dal and Echer, Ezequiel and Vieira, Luis Eduardo Antunes 
                         and Munakata, Kazuoki and Gonzalez, Walter Demetrio and Schuch, 
                         Nelson Jorge and Alarcon, Walter Dem{\'e}trio Gonzalez and 
                         Schuch, Nelson Jorge",
          affiliation = "Southern Regional Space Research Center INPE/MCT, Santa Maria and 
                         Southern Regional Space Research Center INPE/MCT, Santa Maria and 
                         National Institute for Space Research, S{\~a}o Jos{\'e} dos 
                         Campos and National Institute for Space Research, S{\~a}o 
                         Jos{\'e} dos Campos and National Institute for Space Research, 
                         S{\~a}o Jos{\'e} dos Campos and Physics Department, Faculty of 
                         Science, Shinshu University, Matsumoto and {} and Southern 
                         Regional Space Research Center INPE/MCT, Santa Maria and National 
                         Institute for Space Research, S{\~a}o Jos{\'e} dos Campos and 
                         Southern Regional Space Research Center INPE/MCT, Santa Maria",
                title = "Forbush decreases in November 6-20, 2004 by the Muon Detector 
                         Network",
              journal = "Revista Brasileira de Geof{\'{\i}}sica",
                 year = "2007",
               volume = "Vol. 25",
               number = "Suplemento 2",
                pages = "169--173",
             keywords = "interplanetary medium, cosmic rays, Muon Telescope, Forbush 
                         decreases, space weather, magnetic storms.",
             abstract = "In this paper we study the relationship between Interplanetary 
                         Coronal Mass Ejections (ICMEs) and the muon count rate decreases 
                         detected of the Muon Detector Network on November 6-12, 2004. The 
                         Muon Detector Network is composed by the detectors installed at 
                         Nagoya (Japan), Hobart (Australia) and the prototype detector 
                         installed at the {"}Observat´orio Espacial do Sul - 
                         OES/CRSPE/INPE-MCT{"}, located in S{\~a}o Martinho da Serra, RS, 
                         Brazil. With the muon count rate observed by the Muon Detector 
                         Network, we will be able to observe, in the future, the direction 
                         in which a given ICME moves, and with that, we will be able to 
                         calculate their angle of incidence on the Earth. Also, with this 
                         muon network, we will be able to send alerts of up to 12 hours 
                         before the arrival of a shock or an ICME. The Space Weather 
                         forecast method using cosmic rays will be a very important tool 
                         because it provides a forecast with good antecedence.",
                 issn = "0102-261X",
             language = "en",
           targetfile = "savian_forbush.pdf",
        urlaccessdate = "12 maio 2024"
}