Status and performance of the AS array of the Tibet AS sub. gamma. experiment
Conference
·
· AIP Conference Proceedings (American Institute of Physics); (United States)
OSTI ID:5667260
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- Hirosaki University, Hirosaki, Japan (JP)
- Utsunomiya University, Utunomiya, Japan (JP) Saitama University, Urawa, Japan (JP) ICRR, University of Tokyo, Tanashi, Japan (JP) Kanagawa University, Yokohama, Japan (JP) Yokohama National University, Yokohama, Japan (JP) Shonan Institute of Technology, Fujisawa, Japan (JP) Konan University, Kobe, Japan (JP) IHEP, Academia Sinica, Bei
The Tibet AS{gamma} experiment, which has started since January, 1990, is located at an altitude of 4,300m at Yangbaging in Tibet, China (90.5{degree} E, 301{degree} N). The air-shower array is composed of 49 scintillation counters for fast timing (FT), each counter having an area of 0.5 m{sup 2}, in a grid pattern with a spacing of 15 m and 16 density detectors. The density detectors surrounding the FT detectors are planned to select the showers of which core are inside the FT array. For the constant and continuous opeation, the system for laser calibration, the ADC,TDC module calibration and the power check system were installed. A Rb clock is used for the phase analysis of {gamma}-rays.
- OSTI ID:
- 5667260
- Report Number(s):
- CONF-9010289-; CODEN: APCPC; TRN: 91-020029
- Journal Information:
- AIP Conference Proceedings (American Institute of Physics); (United States), Vol. 220:1; Conference: International conference on high energy gamma ray astronomy, Ann Arbor, MI (United States), 2-5 Oct 1990; ISSN 0094-243X
- Country of Publication:
- United States
- Language:
- English
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Related Subjects
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COSMIC GAMMA SOURCES
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COSMIC RAY DETECTION
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GENERAL PHYSICS
46 INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY
COSMIC GAMMA SOURCES
ENERGY SPECTRA
GAMMA DETECTION
COSMIC RAY DETECTION
SCINTILLATION COUNTERS
PERFORMANCE
ENERGY RESOLUTION
EXPERIMENTAL DATA
MONTE CARLO METHOD
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TEV RANGE
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NUMERICAL DATA
RADIATION DETECTION
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