Data acquisition system of surface detector array of the telescope array experiment

Shunsuke Ozawa; M. Fukushima; S. Kawakami; E. Kido; T. Nonaka; H. Ohoka; T. Okuda; H. Sagawa; M. Takeda; A. Taketa; J. Thomas; S. Yoshida

Data acquisition system of surface detector array of the telescope array experiment

Shunsuke Ozawa, M. Fukushima, S. Kawakami, E. Kido, T. Nonaka, H. Ohoka, T. Okuda, H. Sagawa, M. Takeda, A. Taketa, J. Thomas, S. Yoshida

研究成果: Conference contribution

1 被引用数 (Scopus)

抄録

The Telescope Array(TA) experiment will investigate the origin of the extremely high energy cosmic rays (EHECRs). This experiment is a hybrid observation of an air shower array and fluorescence telescopes installed in Utah, USA. We finised deploying 485 Surface Detectors(SDs) for AS array to our site in winter of 2006-2007, and start operation from April 2007. Effective area of this array is 760km2, each detector set up at intervals of 1.2km and has 2 layers of 3m2, 1.2cm thick scintilator. Its energy threshold for air shower event is 1019eV or more. The detector has the power supply to operate electronics and them for the data collection respectively. The data from detectors are transmited to a trigger center by wireless LAN modem. We develop a data acquisition system for SDs on this wireless communication. In this presentation, we will report about the data acquisition system of SD array.

本文言語	English
ホスト出版物のタイトル	Proceedings of the 30th International Cosmic Ray Conference, ICRC 2007
出版社	Universidad Nacional Autonoma de Mexico
ページ	1109-1112
ページ数	4
巻	5
版	HE PART 2
出版ステータス	Published - 2007
外部発表	はい
イベント	30th International Cosmic Ray Conference, ICRC 2007 - Merida, Yucatan, Mexico 継続期間: 2007 7月 3 → 2007 7月 11

Other

Other	30th International Cosmic Ray Conference, ICRC 2007
国/地域	Mexico
City	Merida, Yucatan
Period	07/7/3 → 07/7/11

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

Ozawa, S., Fukushima, M., Kawakami, S., Kido, E., Nonaka, T., Ohoka, H., Okuda, T., Sagawa, H., Takeda, M., Taketa, A., Thomas, J., & Yoshida, S. (2007). Data acquisition system of surface detector array of the telescope array experiment. In Proceedings of the 30th International Cosmic Ray Conference, ICRC 2007 (HE PART 2 ed., Vol. 5, pp. 1109-1112). Universidad Nacional Autonoma de Mexico.

Ozawa, S, Fukushima, M, Kawakami, S, Kido, E, Nonaka, T, Ohoka, H, Okuda, T, Sagawa, H, Takeda, M, Taketa, A, Thomas, J & Yoshida, S 2007, Data acquisition system of surface detector array of the telescope array experiment. in Proceedings of the 30th International Cosmic Ray Conference, ICRC 2007. HE PART 2 edn, vol. 5, Universidad Nacional Autonoma de Mexico, pp. 1109-1112, 30th International Cosmic Ray Conference, ICRC 2007, Merida, Yucatan, Mexico, 07/7/3.

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title = "Data acquisition system of surface detector array of the telescope array experiment",

abstract = "The Telescope Array(TA) experiment will investigate the origin of the extremely high energy cosmic rays (EHECRs). This experiment is a hybrid observation of an air shower array and fluorescence telescopes installed in Utah, USA. We finised deploying 485 Surface Detectors(SDs) for AS array to our site in winter of 2006-2007, and start operation from April 2007. Effective area of this array is 760km2, each detector set up at intervals of 1.2km and has 2 layers of 3m2, 1.2cm thick scintilator. Its energy threshold for air shower event is 1019eV or more. The detector has the power supply to operate electronics and them for the data collection respectively. The data from detectors are transmited to a trigger center by wireless LAN modem. We develop a data acquisition system for SDs on this wireless communication. In this presentation, we will report about the data acquisition system of SD array.",

author = "Shunsuke Ozawa and M. Fukushima and S. Kawakami and E. Kido and T. Nonaka and H. Ohoka and T. Okuda and H. Sagawa and M. Takeda and A. Taketa and J. Thomas and S. Yoshida",

year = "2007",

language = "English",

volume = "5",

pages = "1109--1112",

booktitle = "Proceedings of the 30th International Cosmic Ray Conference, ICRC 2007",

publisher = "Universidad Nacional Autonoma de Mexico",

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note = "30th International Cosmic Ray Conference, ICRC 2007 ; Conference date: 03-07-2007 Through 11-07-2007",

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TY - GEN

T1 - Data acquisition system of surface detector array of the telescope array experiment

AU - Ozawa, Shunsuke

AU - Fukushima, M.

AU - Kawakami, S.

AU - Kido, E.

AU - Nonaka, T.

AU - Ohoka, H.

AU - Okuda, T.

AU - Sagawa, H.

AU - Takeda, M.

AU - Taketa, A.

AU - Thomas, J.

AU - Yoshida, S.

PY - 2007

Y1 - 2007

N2 - The Telescope Array(TA) experiment will investigate the origin of the extremely high energy cosmic rays (EHECRs). This experiment is a hybrid observation of an air shower array and fluorescence telescopes installed in Utah, USA. We finised deploying 485 Surface Detectors(SDs) for AS array to our site in winter of 2006-2007, and start operation from April 2007. Effective area of this array is 760km2, each detector set up at intervals of 1.2km and has 2 layers of 3m2, 1.2cm thick scintilator. Its energy threshold for air shower event is 1019eV or more. The detector has the power supply to operate electronics and them for the data collection respectively. The data from detectors are transmited to a trigger center by wireless LAN modem. We develop a data acquisition system for SDs on this wireless communication. In this presentation, we will report about the data acquisition system of SD array.

AB - The Telescope Array(TA) experiment will investigate the origin of the extremely high energy cosmic rays (EHECRs). This experiment is a hybrid observation of an air shower array and fluorescence telescopes installed in Utah, USA. We finised deploying 485 Surface Detectors(SDs) for AS array to our site in winter of 2006-2007, and start operation from April 2007. Effective area of this array is 760km2, each detector set up at intervals of 1.2km and has 2 layers of 3m2, 1.2cm thick scintilator. Its energy threshold for air shower event is 1019eV or more. The detector has the power supply to operate electronics and them for the data collection respectively. The data from detectors are transmited to a trigger center by wireless LAN modem. We develop a data acquisition system for SDs on this wireless communication. In this presentation, we will report about the data acquisition system of SD array.

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UR - http://www.scopus.com/inward/citedby.url?scp=84899537935&partnerID=8YFLogxK

M3 - Conference contribution

AN - SCOPUS:84899537935

VL - 5

SP - 1109

EP - 1112

BT - Proceedings of the 30th International Cosmic Ray Conference, ICRC 2007

PB - Universidad Nacional Autonoma de Mexico

T2 - 30th International Cosmic Ray Conference, ICRC 2007

Y2 - 3 July 2007 through 11 July 2007

ER -

Data acquisition system of surface detector array of the telescope array experiment

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Other

ASJC Scopus subject areas

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