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Observation of primary cosmic rays with the new Tibet hybrid experiment (YAC-II + Tibet-III + MD)

Abstract:

We have started a new hybrid air shower experiment in Yangbajing (4300 m a.s.l.) in Tibet since February 2014. This new hybrid experiment consists of the YAC-II comprised of 124 core detectors placed in the form of a square grid of 1.9 m spacing covering about 500 m2, the Tibet-III AS array with the total area of about 50,000 m2 and the undergroundMDarray consists of 80 cells, with the total area of ∼4,500 m2. This hybrid-array system is used to observe air showers of high energy celestial gamma-ray origin and those of nuclear-component origin. Prototype experiment YAC-I was successfully carried out in 2009-2010 together with Tibet-III air-shower array. In this paper, performance of YAC-II and the preliminary results of YAC-I are presented.

Año de publicación:

2015

Keywords:

    Fuente:

    scopusscopus

    Tipo de documento:

    Conference Object

    Estado:

    Acceso restringido

    Áreas de conocimiento:

    • Rayo cósmico
    • Ciencia planetaria

    Áreas temáticas:

    • Física moderna
    • Astronomía y ciencias afines
    • Cuerpos y fenómenos celestes específicos

    Contribuidores:

    Shibata M.Shibata M.
    Labaciren Labaciren
    Hotta N.Hotta N.
    Jia H.Y.Jia H.Y.
    Chen T.L.Chen T.L.
    Kasahara K.Kasahara K.
    Sakata M.Sakata M.
    Lu H.Lu H.
    Nakamura Y.Nakamura Y.
    Bi X.J.Bi X.J.
    Amenomori M.Amenomori M.
    Danzengluobu Danzengluobu
    Zhaxisangzhu Zhaxisangzhu
    Yuan A.F.Yuan A.F.
    Zhou X.X.Zhou X.X.
    Gou Q.B.Gou Q.B.
    Tsuchiya H.Tsuchiya H.
    Liu C.Liu C.
    Ding L.K.Ding L.K.
    Huang J.Huang J.
    Qu X.B.Qu X.B.
    Li H.J.Li H.J.
    Cui S.W.Cui S.W.
    Zhang H.M.Zhang H.M.
    Hibino K.Hibino K.
    Udo S.Udo S.
    Li W.J.Li W.J.
    Xue L.Xue L.
    Nanjo H.Nanjo H.
    Li A.F.Li A.F.
    Mizutani K.Mizutani K.
    Wu H.R.Wu H.R.
    Tan Y.H.Tan Y.H.
    Niwa T.Niwa T.
    Chen D.Chen D.
    Guo Y.Q.Guo Y.Q.
    Hu H.B.Hu H.B.
    T. K. SakoT. K. Sako
    Kajino F.Kajino F.
    Takita M.Takita M.
    Hu H.B.Hu H.B.
    Miyazaki T.Miyazaki T.
    Torii S.Torii S.
    Zhai L.M.Zhai L.M.
    Shirai T.Shirai T.
    Ohnishi M.Ohnishi M.
    Wang H.Wang H.
    Yamamoto Y.Yamamoto Y.
    Feng Z.Y.Feng Z.Y.
    Kozai M.Kozai M.
    Feng Z.Y.Feng Z.Y.
    Nishizawa M.Nishizawa M.
    Yasue S.Yasue S.
    Feng C.F.Feng C.F.
    Kato C.Kato C.
    Zhang J.L.Zhang J.L.
    Zhang X.Y.Zhang X.Y.
    Liu M.Y.Liu M.Y.
    Chen W.Y.Chen W.Y.
    Yang Z.Yang Z.
    Zhang Y.Zhang Y.
    Meng X.R.Meng X.R.
    Zhang Y.Zhang Y.
    Qian X.L.Qian X.L.
    Yuda T.Yuda T.
    He H.H.He H.H.
    Shiomi A.Shiomi A.
    Zhang Y.Zhang Y.
    Le G.M.Le G.M.
    Tateyama N.Tateyama N.
    Saito T.Y.Saito T.Y.
    Ozawa S.Ozawa S.
    Nakajima T.Nakajima T.
    Katayose Y.Katayose Y.
    He Z.T.He Z.T.
    Saito T.Saito T.
    Jiang L.Jiang L.
    Munakata K.Munakata K.
    Sugimoto H.Sugimoto H.
    Ohta I.Ohta I.
    Shao J.Shao J.
    Yamauchi K.Yamauchi K.
    Kawata K.Kawata K.
    Liu J.S.Liu J.S.