Simulation of two PMTs layout differences for the imaging atmospheric Cherenkov Telescope

Haoshen Fan

doi:10.1117/12.2690163

17 August 2023 Simulation of two PMTs layout differences for the imaging atmospheric Cherenkov Telescope

Haoshen Fan

Proceedings Volume 12757, 3rd International Conference on Laser, Optics, and Optoelectronic Technology (LOPET 2023); 1275730 (2023) https://doi.org/10.1117/12.2690163
Event: 3rd International Conference on Laser, Optics and Optoelectronic Technology (LOPET 2023), 2023, Kunming, China

Abstract

One of the crucial tools for measuring the extensive atmospheric showers brought on by cosmic rays is the imaging atmospheric Cherenkov telescope. There are hundreds to tens of thousands of distinct photomultiplier tube arrays or pixels inside each imaging atmospheric Cherenkov telescope. The size of the array spans the area corresponding to each telescope’s field of view. This paper discusses the differences between the square and stagger arrangement of the photomultiplier array along with compares the photon collection capabilities of the two arrangements. The results reveal that the experiment works better using a square arrangement of the photomultiplier array.

Citation Download Citation

Haoshen Fan "Simulation of two PMTs layout differences for the imaging atmospheric Cherenkov Telescope", Proc. SPIE 12757, 3rd International Conference on Laser, Optics, and Optoelectronic Technology (LOPET 2023), 1275730 (17 August 2023); https://doi.org/10.1117/12.2690163

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