Arid
DOI10.1016/j.nuclphysbps.2009.03.064
The present status of the Telescope Array experiment
Nonaka, T.1; Abu-Zayyad, T.2; Allen, M.2; Azuma, R.3; Belz, J. W.2; Bergman, D. R.4; Blake, S. A.2; Brusova, O.2; Cady, R.2; Cao, Z.2; Chiba, J.5; Chikawa, M.6; Cho, I. S.7; Fujii, H.8; Fujii, T.9; Fukuda, T.3; Fukushima, M.1; Hayashi, K.3; Hayashida, N.1; Hibino, K.10; Honda, K.11; Huentemeyer, P.2; Hughes, G.4; Ikeda, D.1; Inoue, N.12; Ivanov, D.4; Iwamoto, S.11; Jui, C. H.2; Kadota, K.13; Kakimoto, F.3; Kang, H.14; Kasahara, K.15; Kawai, H.16; Kawana, S.12; Kido, E.1; Kitshugi, A.1; Kobayashi, K.5; Kondo, Y.1; Kwon, Y. J.7; Martens, K.2; Matsuda, T.8; Matthews, J. N.2; Nakamura, T.17; Nam, S.18; Ogio, S.9; Ohoka, H.1; Okuda, T.9; Ohnishi, M.1; Oshima, A.9; Ozawa, S.15; Park, I. H.18; Rodriguez, D.2; Ryu, D.19; Sagawa, H.1; Sakurai, N.1; Scott, L.4; Shah, P.2; Shibata, T.1; Shimodaira, H.1; Smith, J. D.2; Sokolsky, P.2; Springer, R. W.2; Stratton, S.4; Takeda, M.1; Taketa, A.1; Takita, M.1; Tameda, Y.3; Tanaka, K.20; Tanaka, M.8; Teshima, M.21; Thomas, S. B.2; Thomson, G. B.4; Tokuno, H.1; Tomida, T.11; Torii, R.1; Tsunesada, Y.3; Tsuyuguchi, Y.11; Uchihori, Y.22; Udo, S.10; Wiencke, L. R.2; Yamakawa, T.1; Yamakawa, Y.1; Yamamoto, K.1; Yang, J.18; Yoshida, S.16; Yoshii, N.23
通讯作者Nonaka, T.
会议名称Cosmic Ray International Seminar
会议日期SEP 15-19, 2008
会议地点Malfa, ITALY
英文摘要

The Telescope Array(TA) experiment located at western desert in Utah USA (N39.3,W112.9) is designed for observation of air shower from extreme high energy cosmic rays. The TA detector consists of 2 types of detector to enable a cross check on systematic difference from the two main methods of observation for the energy region. One is a Fluorescence detector (FD) for detecting fluorescence light from air shower and another is surface detector (SD) array for detecting air shower particles at ground level. Each SD consists of 2 layers of plastic scintillator with 3m(2) of surface and more sensitive to electromagnetic component in air shower. The full operation using 3FD stations and full SD array has started. Here we present the updated status of Telescope Array experiment.


来源出版物NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS
ISSN0920-5632
出版年2009
卷号190
页码26-31
出版者ELSEVIER SCIENCE BV
类型Proceedings Paper
语种英语
国家Japan;USA;South Korea;Germany
收录类别CPCI-S
WOS记录号WOS:000267254300005
WOS关键词SPECTRUM ; END
WOS类目Physics, Particles & Fields
WOS研究方向Physics
资源类型会议论文
条目标识符http://119.78.100.177/qdio/handle/2XILL650/297861
作者单位1.Univ Tokyo, Inst Cosm Ray Res, Chiba, Japan;
2.Univ Utah, High Energy Astrophys Inst, Salt Lake City, UT 84112 USA;
3.Tokyo Inst Technol, Meguro Ku, Tokyo 1528550, Japan;
4.Rutgers State Univ, Piscataway, NJ 08854 USA;
5.Tokyo Univ Sci, Noda, Chiba 2788510, Japan;
6.Kinki Univ, Higashiosaka, Osaka 5778582, Japan;
7.Yonsei Univ, Seoul 120749, South Korea;
8.High Energy Accelerator Res Org, Inst Particle & Nucl Studies, Tsukuba, Ibaraki 3050801, Japan;
9.Osaka City Univ, Sumiyoshi Ku, Osaka 5588585, Japan;
10.Kanagawa Univ, Kanagawa Ku, Yokohama, Kanagawa 2218686, Japan;
11.Univ Yamanashi, Kofu, Yamanashi 4008511, Japan;
12.Saitama Univ, Sakura Ku, Saitama 3388570, Japan;
13.Musashi Inst Technol, Setagaya Ku, Tokyo 1588557, Japan;
14.Pusan Natl Univ, Pusan 609735, South Korea;
15.Waseda Univ, Shinjuku Ku, Tokyo 1698555, Japan;
16.Chiba Univ, Inage Ku, Chiba 2638522, Japan;
17.Kochi Univ, Kochi 7808520, Japan;
18.Ewha Womans Univ, Seoul 120750, South Korea;
19.Chungnam Natl Univ, Taejon 305764, South Korea;
20.Hiroshima City Univ, Asaminami Ku, Hiroshima 7313194, Japan;
21.Max Planck Inst Phys & Astrophys, D-80805 Munich, Germany;
22.Natl Inst Radiol Sci, Inage Ku, Chiba 2638555, Japan;
23.Ehime Univ, Matsuyama, Ehime 7908597, Japan
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Nonaka, T.,Abu-Zayyad, T.,Allen, M.,et al. The present status of the Telescope Array experiment[C]:ELSEVIER SCIENCE BV,2009:26-31.
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