@InProceedings{MunakataKKKBESDSDHSAS:2015:NoAnGa,
               author = "Munakata, K and Kozai, Masayoshi and Kato, Chihiro and Kuwabara, 
                         T. and Bieber, John W. and Evenson, Paul and Silva, Marlos 
                         Rockenbach da and Dal Lago, Alisson and Schuch, Nelson Jorge and 
                         Duldig, M. L. and Humble, J. E. and Sabbah, I. and Al Jassar, H. 
                         K. and Sharma, M. M.",
          affiliation = "{Shinshu University} and {Shinshu University} and {Shinshu 
                         University} and {Chiba University} and {University of Delawar} and 
                         {University of Delawar} and {Instituto Nacional de Pesquisas 
                         Espaciais (INPE)} and {Instituto Nacional de Pesquisas Espaciais 
                         (INPE)} and {Instituto Nacional de Pesquisas Espaciais (INPE)} and 
                         {University of Tasmani} and {University of Tasmani} and {Public 
                         Authority of Applied Education and Training} and {Kuwait 
                         University} and {Kuwait University)}",
                title = "North-south anisotropy of galactic cosmic rays observed with the 
                         Global Muon Detector Network (GMDN)",
            booktitle = "Proceedings...",
                 year = "2015",
                pages = "466--467",
         organization = "International Cosmic Ray Conference, 34. (ICRC)",
             abstract = "We analyze the north-south anisotropy (NSA) of galactic cosmic 
                         rays (GCRs) observed with the GMDN on hourly basis in the toward 
                         (T) and away (A) IMF sectors separately. From the monthly mean and 
                         its standard error of NSA in each of T and A sectors, we deduce 
                         the T/A separation and its temporal variation during a period 
                         between 2006 and 2014. We also examine the success rate which is a 
                         ratio of the number of hours when the sign of the observed NSA is 
                         positive (negative) in T (A) IMF sector to the total number of 
                         hours and is introduced as a parameter indicating to what extent 
                         we can infer the IMF sector polarity from the sign of the observed 
                         NSA. The temporal variations of T/A separation and success rate 
                         will be discussed in relation to the solar modulation of GCRs in 
                         the Solar Cycle 24.",
  conference-location = "Hague",
      conference-year = "30 July - 06 Ago.",
                label = "lattes: 0549130828972280 7 MunakataKKKSDSASDHBS:2015:NoAnGa",
             language = "en",
           targetfile = "munakata_north.pdf",
        urlaccessdate = "28 abr. 2024"
}