@InProceedings{MendonçaRaBrDaEcMu:2018:AnSoCy,
               author = "Mendon{\c{c}}a, Rafael Rodrigues Souza de and Raulin, Jean-Pierre 
                         and Braga, Carlos Roberto and Dal Lago, Alisson and Echer, 
                         Ezequiel and Munakata, Kazuoki",
          affiliation = "{Center for Radio Astronomy and Astrophysics at Mackenzie} and 
                         {Center for Radio Astronomy and Astrophysics at Mackenzie} and 
                         {Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto 
                         Nacional de Pesquisas Espaciais (INPE)} and {Instituto Nacional de 
                         Pesquisas Espaciais (INPE)} and {Shinshu University}",
                title = "Analysis of the solar cycle modulation in the cosmic ray intensity 
                         observed at South America in the last decade",
                 year = "2018",
         organization = "Latin American Conference on Space Geophysics, 11. (COLAGE)",
             abstract = "Cosmic rays are energetic particles (mostly protons that can have 
                         energy from MeV to ZeV) which presented a practically isotropic 
                         flow in the space region close to the Earth. Solar and 
                         interplanetary phenomena affect the cosmic ray intensity observed 
                         at ground producing different transient and periodic variations. 
                         In this work, we analyze the 11 and 22-year cosmic ray intensity 
                         variation observed by three cosmic rays detectors. We compare the 
                         sunspot number and mean solar magnetic field obtained by the WSO 
                         (Wilcox Solar Observatory) with the cosmic ray intensity observed 
                         by the Sao Martinho da Serra (Brazil) and CARPET (Argentina) 
                         detectors between 2006 and 2017. In addition, we compare the 
                         results with that obtained comparing these solar activity 
                         parameters with the cosmic ray intensity observed by the Nagoya 
                         (Japan) detector between the last 4 decades (from 1971 until 
                         2017).",
  conference-location = "Buenos Aires, Argentina",
      conference-year = "16-20 abr.",
             language = "en",
           targetfile = "Abstract_COLAGE_RRSM.pdf",
        urlaccessdate = "28 abr. 2024"
}