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The Application of 20 inch PMT in LHASSO-WCDA
2021
Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021)
unpublished
On behalf of LHAASO collaboration In the Large High Altitude Air Shower Observatory (LHAASO), the main physics objective of the Water Cherenkov Detector Array (WCDA) is to survey the gamma-ray sky continuously in the energy range from 100 GeV to PeV. The Water Cherenkov detector array, covering an area of about 78,000 2 area, is constituted by 3120 detector units divided into 3 separate arrays. In the second and third array are installed 2220 20" PMTs instead of the 8 PMT used in the first 150
doi:10.22323/1.395.0696
fatcat:vvgt3cwj2zbc7ezeqxglvhfvo4