Telescope array; progress of surface array

H. Kawai; T. Nunomura; N. Sakurai; S. Yoshida; H. Yoshii; K. Tanaka; F. Cohen; M. Fukushima; N. Hayashida; M. Ohnishi; H. Ohoka; Shunsuke Ozawa; H. Sagawa; T. Shibata; H. Shimodaira; M. Takeda; A. Taketa; M. Takita; H. Tokuno; R. Torii; S. Udo; H. Fujii; T. Matsuda; M. Tanaka; H. Yamaoka; K. Hibino; T. Benno; M. Chikawa; T. Nakamura; M. Teshima; K. Kadota; Y. Uchihori; Y. Hayashi; K. Matsumoto; Y. Matsumoto; T. Matsuyama; S. Ogio; A. Ohshima; T. Okuda; D. R. Bergmann; G. B. Thomson; N. Inoue; Y. Wada; K. Kasahara; J. W. Belz; M. Fukuda; T. Iguchi; F. Kakimoto; R. Minagawa; Y. Tameda; Y. Tsunesada; J. A J Matthews; T. Abu-Zayyad; R. Cady; Z. Cao; P. Huentemeyer; C. C H Jui; K. Martens; J. N. Matthews; J. D. Smith; P. Sokolsky; R. W. Springer; S. B. Thomas; L. R. Wiencke; T. Doyle; M. J. Taylor; V. B. Wickwar; T. D. Wilkerson; K. Hashimoto; K. Honda; T. Ishii; T. Kanbe

Telescope array; progress of surface array

H. Kawai, T. Nunomura, N. Sakurai, S. Yoshida, H. Yoshii, K. Tanaka, F. Cohen, M. Fukushima, N. Hayashida, M. Ohnishi, H. Ohoka, Shunsuke Ozawa, H. Sagawa, T. Shibata, H. Shimodaira, M. Takeda, A. Taketa, M. Takita, H. Tokuno, R. ToriiS. Udo, H. Fujii, T. Matsuda, M. Tanaka, H. Yamaoka, K. Hibino, T. Benno, M. Chikawa, T. Nakamura, M. Teshima, K. Kadota, Y. Uchihori, Y. Hayashi, K. Matsumoto, Y. Matsumoto, T. Matsuyama, S. Ogio, A. Ohshima, T. Okuda, D. R. Bergmann, G. B. Thomson, N. Inoue, Y. Wada, K. Kasahara, J. W. Belz, M. Fukuda, T. Iguchi, F. Kakimoto, R. Minagawa, Y. Tameda, Y. Tsunesada, J. A J Matthews, T. Abu-Zayyad, R. Cady, Z. Cao, P. Huentemeyer, C. C H Jui, K. Martens, J. N. Matthews, J. D. Smith, P. Sokolsky, R. W. Springer, S. B. Thomas, L. R. Wiencke, T. Doyle, M. J. Taylor, V. B. Wickwar, T. D. Wilkerson, K. Hashimoto, K. Honda, T. Ishii, T. Kanbe

研究成果: Conference contribution

3 被引用数 (Scopus)

抄録

The telescope Array (TA) experiment, currently under construction in Utah, USA, is an array of surface detectors with air fluorescence telescopes to study the highest energy cosmic rays of energy beyond 10²⁰eV. The TA surface detector array will consist of 576 plastic scintillation counters, on a square grid with 1.2 km spacing, covering the ground area of 760 km². Each surface detector is outfitted with two layers of scintillators of 3m ² area, readout electronics, and wireless LAN communication system, which are powered by solar system. The test of an Engineering Array with 18 surface detectors is currently operating after being deployed in December 2004. Here we present the design and the progress of the surface detectors of TA, focusing on the status of the Engineering Array.

本文言語	English
ホスト出版物のタイトル	29th International Cosmic Ray Conference, ICRC 2005
出版社	Tata Institute of Fundamental Research
ページ	181-184
ページ数	4
巻	8
出版ステータス	Published - 2005
外部発表	はい
イベント	29th International Cosmic Ray Conference, ICRC 2005 - Pune, India 継続期間: 2005 8月 3 → 2005 8月 10

Other

Other	29th International Cosmic Ray Conference, ICRC 2005
国/地域	India
City	Pune
Period	05/8/3 → 05/8/10

ASJC Scopus subject areas

核物理学および高エネルギー物理学

他のファイルとリンク

引用スタイル

Kawai, H., Nunomura, T., Sakurai, N., Yoshida, S., Yoshii, H., Tanaka, K., Cohen, F., Fukushima, M., Hayashida, N., Ohnishi, M., Ohoka, H., Ozawa, S., Sagawa, H., Shibata, T., Shimodaira, H., Takeda, M., Taketa, A., Takita, M., Tokuno, H., ... Kanbe, T. (2005). Telescope array; progress of surface array. In 29th International Cosmic Ray Conference, ICRC 2005 (Vol. 8, pp. 181-184). Tata Institute of Fundamental Research.

Kawai, H, Nunomura, T, Sakurai, N, Yoshida, S, Yoshii, H, Tanaka, K, Cohen, F, Fukushima, M, Hayashida, N, Ohnishi, M, Ohoka, H, Ozawa, S, Sagawa, H, Shibata, T, Shimodaira, H, Takeda, M, Taketa, A, Takita, M, Tokuno, H, Torii, R, Udo, S, Fujii, H, Matsuda, T, Tanaka, M, Yamaoka, H, Hibino, K, Benno, T, Chikawa, M, Nakamura, T, Teshima, M, Kadota, K, Uchihori, Y, Hayashi, Y, Matsumoto, K, Matsumoto, Y, Matsuyama, T, Ogio, S, Ohshima, A, Okuda, T, Bergmann, DR, Thomson, GB, Inoue, N, Wada, Y, Kasahara, K, Belz, JW, Fukuda, M, Iguchi, T, Kakimoto, F, Minagawa, R, Tameda, Y, Tsunesada, Y, Matthews, JAJ, Abu-Zayyad, T, Cady, R, Cao, Z, Huentemeyer, P, Jui, CCH, Martens, K, Matthews, JN, Smith, JD, Sokolsky, P, Springer, RW, Thomas, SB, Wiencke, LR, Doyle, T, Taylor, MJ, Wickwar, VB, Wilkerson, TD, Hashimoto, K, Honda, K, Ishii, T & Kanbe, T 2005, Telescope array; progress of surface array. in 29th International Cosmic Ray Conference, ICRC 2005. vol. 8, Tata Institute of Fundamental Research, pp. 181-184, 29th International Cosmic Ray Conference, ICRC 2005, Pune, India, 05/8/3.

@inproceedings{d471744890ac4080804d3c85e1dc17ee,

title = "Telescope array; progress of surface array",

abstract = "The telescope Array (TA) experiment, currently under construction in Utah, USA, is an array of surface detectors with air fluorescence telescopes to study the highest energy cosmic rays of energy beyond 1020eV. The TA surface detector array will consist of 576 plastic scintillation counters, on a square grid with 1.2 km spacing, covering the ground area of 760 km2. Each surface detector is outfitted with two layers of scintillators of 3m 2 area, readout electronics, and wireless LAN communication system, which are powered by solar system. The test of an Engineering Array with 18 surface detectors is currently operating after being deployed in December 2004. Here we present the design and the progress of the surface detectors of TA, focusing on the status of the Engineering Array.",

author = "H. Kawai and T. Nunomura and N. Sakurai and S. Yoshida and H. Yoshii and K. Tanaka and F. Cohen and M. Fukushima and N. Hayashida and M. Ohnishi and H. Ohoka and Shunsuke Ozawa and H. Sagawa and T. Shibata and H. Shimodaira and M. Takeda and A. Taketa and M. Takita and H. Tokuno and R. Torii and S. Udo and H. Fujii and T. Matsuda and M. Tanaka and H. Yamaoka and K. Hibino and T. Benno and M. Chikawa and T. Nakamura and M. Teshima and K. Kadota and Y. Uchihori and Y. Hayashi and K. Matsumoto and Y. Matsumoto and T. Matsuyama and S. Ogio and A. Ohshima and T. Okuda and Bergmann, {D. R.} and Thomson, {G. B.} and N. Inoue and Y. Wada and K. Kasahara and Belz, {J. W.} and M. Fukuda and T. Iguchi and F. Kakimoto and R. Minagawa and Y. Tameda and Y. Tsunesada and Matthews, {J. A J} and T. Abu-Zayyad and R. Cady and Z. Cao and P. Huentemeyer and Jui, {C. C H} and K. Martens and Matthews, {J. N.} and Smith, {J. D.} and P. Sokolsky and Springer, {R. W.} and Thomas, {S. B.} and Wiencke, {L. R.} and T. Doyle and Taylor, {M. J.} and Wickwar, {V. B.} and Wilkerson, {T. D.} and K. Hashimoto and K. Honda and T. Ishii and T. Kanbe",

year = "2005",

language = "English",

volume = "8",

pages = "181--184",

booktitle = "29th International Cosmic Ray Conference, ICRC 2005",

publisher = "Tata Institute of Fundamental Research",

note = "29th International Cosmic Ray Conference, ICRC 2005 ; Conference date: 03-08-2005 Through 10-08-2005",

}

TY - GEN

T1 - Telescope array; progress of surface array

AU - Kawai, H.

AU - Nunomura, T.

AU - Sakurai, N.

AU - Yoshida, S.

AU - Yoshii, H.

AU - Tanaka, K.

AU - Cohen, F.

AU - Fukushima, M.

AU - Hayashida, N.

AU - Ohnishi, M.

AU - Ohoka, H.

AU - Ozawa, Shunsuke

AU - Sagawa, H.

AU - Shibata, T.

AU - Shimodaira, H.

AU - Takeda, M.

AU - Taketa, A.

AU - Takita, M.

AU - Tokuno, H.

AU - Torii, R.

AU - Udo, S.

AU - Fujii, H.

AU - Matsuda, T.

AU - Tanaka, M.

AU - Yamaoka, H.

AU - Hibino, K.

AU - Benno, T.

AU - Chikawa, M.

AU - Nakamura, T.

AU - Teshima, M.

AU - Kadota, K.

AU - Uchihori, Y.

AU - Hayashi, Y.

AU - Matsumoto, K.

AU - Matsumoto, Y.

AU - Matsuyama, T.

AU - Ogio, S.

AU - Ohshima, A.

AU - Okuda, T.

AU - Bergmann, D. R.

AU - Thomson, G. B.

AU - Inoue, N.

AU - Wada, Y.

AU - Kasahara, K.

AU - Belz, J. W.

AU - Fukuda, M.

AU - Iguchi, T.

AU - Kakimoto, F.

AU - Minagawa, R.

AU - Tameda, Y.

AU - Tsunesada, Y.

AU - Matthews, J. A J

AU - Abu-Zayyad, T.

AU - Cady, R.

AU - Cao, Z.

AU - Huentemeyer, P.

AU - Jui, C. C H

AU - Martens, K.

AU - Matthews, J. N.

AU - Smith, J. D.

AU - Sokolsky, P.

AU - Springer, R. W.

AU - Thomas, S. B.

AU - Wiencke, L. R.

AU - Doyle, T.

AU - Taylor, M. J.

AU - Wickwar, V. B.

AU - Wilkerson, T. D.

AU - Hashimoto, K.

AU - Honda, K.

AU - Ishii, T.

AU - Kanbe, T.

PY - 2005

Y1 - 2005

N2 - The telescope Array (TA) experiment, currently under construction in Utah, USA, is an array of surface detectors with air fluorescence telescopes to study the highest energy cosmic rays of energy beyond 1020eV. The TA surface detector array will consist of 576 plastic scintillation counters, on a square grid with 1.2 km spacing, covering the ground area of 760 km2. Each surface detector is outfitted with two layers of scintillators of 3m 2 area, readout electronics, and wireless LAN communication system, which are powered by solar system. The test of an Engineering Array with 18 surface detectors is currently operating after being deployed in December 2004. Here we present the design and the progress of the surface detectors of TA, focusing on the status of the Engineering Array.

AB - The telescope Array (TA) experiment, currently under construction in Utah, USA, is an array of surface detectors with air fluorescence telescopes to study the highest energy cosmic rays of energy beyond 1020eV. The TA surface detector array will consist of 576 plastic scintillation counters, on a square grid with 1.2 km spacing, covering the ground area of 760 km2. Each surface detector is outfitted with two layers of scintillators of 3m 2 area, readout electronics, and wireless LAN communication system, which are powered by solar system. The test of an Engineering Array with 18 surface detectors is currently operating after being deployed in December 2004. Here we present the design and the progress of the surface detectors of TA, focusing on the status of the Engineering Array.

UR - http://www.scopus.com/inward/record.url?scp=84860724349&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84860724349&partnerID=8YFLogxK

M3 - Conference contribution

AN - SCOPUS:84860724349

VL - 8

SP - 181

EP - 184

BT - 29th International Cosmic Ray Conference, ICRC 2005

PB - Tata Institute of Fundamental Research

T2 - 29th International Cosmic Ray Conference, ICRC 2005

Y2 - 3 August 2005 through 10 August 2005

ER -

Telescope array; progress of surface array

抄録

Other

ASJC Scopus subject areas

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