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The Status of the Telescope Array experiment

Title
The Status of the Telescope Array experiment
Authors
Tokuno H.Abu-Zayyad T.Aida R.Allen M.Azuma R.Barcikowski E.Belz J.W.Benno T.Bergman D.R.Blake S.A.Brusova O.Cady R.Cheon B.G.Chiba J.Chikawa M.Cho E.J.Cho L.S.Cho W.R.Cohen F.Doura K.Ebeling C.Fujii H.Fujii T.Fukuda T.Fukushima M.Gorbunov D.Hanlon W.Hayashi K.Hayashi Y.Hayashida N.Hibino K.Hiyama K.Honda K.Hughes G.Iguchi T.Ikeda D.Ikuta K.Innemee S.J.J.Inoue N.Ishii T.Ishimori R.Ivanov D.Iwamoto S.Jui C.C.H.Kadota K.Kakimoto F.Kalashev O.Kanbe T.Kang H.Kasahara K.Kawai H.Kawakami S.Kawana S.Kido E.Kim B.G.Kim H.B.Kim J.H.Kitsugi A.Kobayashi K.Koers H.Kondo Y.Kuzmin V.Kwon Y.J.Lim J.H.Lim S.I.MacHida S.Martens K.Martineau J.Matsuda T.Matsuyama T.Matthews J.N.Minamino M.Miyata K.Miyauchi H.Murano Y.Nakamura T.Nam S.W.Nonaka T.Ogio S.Ohnishi M.Ohoka H.Okuda T.Oshima A.Ozawa S.Park I.H.Rodriguez D.Roh S.Y.Rubtsov G.Ryu D.Sagawa H.Sakurai N.Scott L.M.Shah P.D.Shibata T.Shimodaira H.Shin B.K.Smith J.D.Sokolsky P.Sonley T.J.Springer R.W.Stokes B.T.Stratton S.R.Suzuki S.Takahashi Y.Takeda M.Taketa A.Takita M.Tameda Y.Tanaka H.Tanaka K.Tanaka M.Thomas J.R.Thomas S.B.Thomson G.B.Tinyakov P.Tkachev I.Tomida T.Torii R.Troitsky S.Tsunesada Y.Tsuyuguchi Y.Uchihori Y.Udo S.Ukai H.Vanklaveren B.Wada Y.Wood M.Yamakawa T.Yamakawa Y.Yamaoka H.Yang J.Yoshida S.Yoshii H.Zundel Z.
Ewha Authors
양종만
SCOPUS Author ID
양종만scopus
Issue Date
2011
Journal Title
Journal of Physics: Conference Series
ISSN
1742-6588JCR Link
Citation
vol. 293, no. 1
Indexed
SCOPUS scopus
Abstract
The purpose of The Telescope Array experiment is to identify origin of the ultra high energy cosmic rays. The Telescope Array is a hybrid detector consists of a surface detector array and air fluorescence detectors. This hybrid detector is observing extensive air showers to measure the energy spectrum, anisotropy and composition of Ultra High Energy Cosmic Rays. The detector construction has been completed in March 2008, and the hybrid observation with the full configuration has been running since that time. In this talk, the status of observation and our prospects are described.
DOI
10.1088/1742-6596/293/1/012035
Appears in Collections:
자연과학대학 > 물리학전공 > Journal papers
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