The system of DAQ for TA surface array

Shunsuke Ozawa, H. Ohoka, M. Takeda, N. Sakurai, S. Yoshida, S. Kawakami, H. Tanaka

研究成果: Conference contribution

2 引用 (Scopus)

抜粋

The installation of The Telescope Array experiment started in earnest. Since observation by combine two different type air shower detector, we aim to search super GZK cosmic ray and determine accurately the energy of these CRs. In past, extensive air shower observations using scintillation detector array give many good results Utilize these experience, we combine scintillator array and fluorescence detectors for determination for EAS energy scale, core position and incoming direction. In this paper, we introduce the electronics and data acquisition system for our scintillator array; call Surface Detector (SD). The engineering array that constituted 18 scintillation detectors was installed on December 2004. We have tested our electronics and DAQ on this small array. Complete SD will have 576 detectors, around 900 km2. This will be about 9 times larger than AGASA.

元の言語English
ホスト出版物のタイトル29th International Cosmic Ray Conference, ICRC 2005
出版者Tata Institute of Fundamental Research
ページ177-180
ページ数4
8
出版物ステータスPublished - 2005
外部発表Yes
イベント29th International Cosmic Ray Conference, ICRC 2005 - Pune, India
継続期間: 2005 8 32005 8 10

Other

Other29th International Cosmic Ray Conference, ICRC 2005
India
Pune
期間05/8/305/8/10

    フィンガープリント

ASJC Scopus subject areas

  • Nuclear and High Energy Physics

これを引用

Ozawa, S., Ohoka, H., Takeda, M., Sakurai, N., Yoshida, S., Kawakami, S., & Tanaka, H. (2005). The system of DAQ for TA surface array. : 29th International Cosmic Ray Conference, ICRC 2005 (巻 8, pp. 177-180). Tata Institute of Fundamental Research.