The system of DAQ for TA surface array

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

Research output: Chapter in Book/Report/Conference proceedingConference contribution

2 Citations (Scopus)

Abstract

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.

Original languageEnglish
Title of host publication29th International Cosmic Ray Conference, ICRC 2005
PublisherTata Institute of Fundamental Research
Pages177-180
Number of pages4
Volume8
Publication statusPublished - 2005
Externally publishedYes
Event29th International Cosmic Ray Conference, ICRC 2005 - Pune, India
Duration: 2005 Aug 32005 Aug 10

Other

Other29th International Cosmic Ray Conference, ICRC 2005
CountryIndia
CityPune
Period05/8/305/8/10

ASJC Scopus subject areas

  • Nuclear and High Energy Physics

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