Speakers
Dr
Bo Gao
(Institute of High Energy Physics, CAS)Prof.
Chunxu Yu
(School of Physics, Nankai University)Dr
Hanrong Wu
(Institute of High Energy Physics, CAS)Mr
Huicai Li
(School of Physics, Nankai University)Dr
Mingjun Chen
(Institute of High Energy Physics, CAS)Ms
Xiaojie Wang
(Institute of High Energy Physics, CAS)Prof.
Zhiguo Yao
(Institute of High Energy Physics, CAS)
Description
The Large High Altitude Air Shower Observatory (LHAASO) project is to be built at Daocheng, Sichuan Province, 4400 m a.s.l., in a few years. As one of the major components of the LHAASO project, LHAASO-WCDA, a water Cherenkov detector array with an area of 90000 m2, contains around 400,000 tons of purified water. To gain full knowledge of the water Cherenkov technique and to investigate the engineering issues, a 9-cell detector array has been built at the Yang-Ba-Jing site. With the array, a method of water quality monitoring and measurement with cosmic muon signals is studied, whose results show that a precision at some ten percentages can be achieved, satisfying the requirement of the experiment. The results are compared with those from a full Monte Carlo simulation. This method is proposed to be applied in the LHAASO-WCDA project.
Registration number following "ICRC2015-I/" | 811 |
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Collaboration | LHAASO |
Primary author
Mr
Huicai Li
(School of Physics, Nankai University)
Co-authors
Dr
Bo Gao
(Institute of High Energy Physics, CAS)
Prof.
Chunxu Yu
(School of Physics, Nankai University)
Dr
Hanrong Wu
(Institute of High Energy Physics, CAS)
Dr
Mingjun Chen
(Institute of High Energy Physics, CAS)
Ms
Xiaojie Wang
(Institute of High Energy Physics, CAS)
Prof.
Zhiguo Yao
(Institute of High Energy Physics, CAS)