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Cosmic-ray mass composition with the TA SD 12-year data
2021
Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021)
unpublished
Telescope Array (TA) is the largest ultra-high-energy cosmic-ray (UHECR) observatory in the Northern Hemisphere. It is dedicated to detect extensive air showers (EAS) in hybrid mode, both by measuring the shower's longitudinal profile with fluorescence telescopes and their particle footprint on the ground from the surface detector (SD) array. While fluorescence telescopes can measure the most composition-sensitive characteristic of EAS, the depth of the shower maximum (X max ), they also have
doi:10.22323/1.395.0300
fatcat:asqmty7qzbgzbnxra5hlrmnoba