Underground Prototype Water Cherenkov Muon Detector with the Tibet Air Shower Array

Journal Article · Tue Dec 23 23:00:00 EST 2008 · AIP Conference Proceedings

DOI:https://doi.org/10.1063/1.3076780· OSTI ID:21255176

Amenomori, M; Nanjo, H ^[1]; Bi, X J; Ding, L K; Feng, Zhaoyang; He, H H; Hu, H B; Lu, H; Lu, S L; Ren, J R; Tan, Y H; Wang, B; Wang, H; Wang, Y; Wu, H R; Zhang, H M; Zhang, J L; Zhang, Y ^[2]; Chen, D; Kawata, K ^[3]

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1. Department of Physics, Hirosaki University, Hirosaki 036-8561 (Japan)
2. Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049 (China)
3. Institute for Cosmic Ray Research, University of Tokyo, Kashiwa 277-8582 (Japan)

We are planning to build a 10,000 m{sup 2} water-Cherenkov-type muon detector (MD) array under the Tibet air shower (AS) array. The Tibet AS+MD array will have the sensitivity to detect gamma rays in the 100 TeV region by an order of the magnitude better than any other previous existing detectors in the world. In the late fall of 2007, a prototype water Cherenkov muon detector of approximately 100 m{sup 2} was constructed under the existing Tibet AS array. The preliminary data analysis is in good agreement with our MC simulation. We are now ready for further expanding the underground water Cherenkov muon detector.

• OSTI ID: 21255176
• Journal Information: AIP Conference Proceedings, Journal Name: AIP Conference Proceedings Journal Issue: 1 Vol. 1085; ISSN 0094-243X; ISSN APCPCS
• Country of Publication: United States
• Language: English

Related Subjects

79 ASTRONOMY AND ASTROPHYSICS
99 GENERAL AND MISCELLANEOUS
DATA ANALYSIS
EXTENSIVE AIR SHOWERS
GAMMA ASTRONOMY
GAMMA DETECTION
GAMMA RADIATION
MUON DETECTION
MUONS
SIMULATION
TEV RANGE
UNDERGROUND FACILITIES