Performance of the Tibet-III Air Shower Array

Details Performance of the Tibet-III Air Shower Array Performance of the Tibet-III Air Shower Array

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....5.3019a&link_type=abstract

Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I

Physics

2

Scientific paper

: The Tibet-I I I air shower array (36900 m2 ) has been successfully operating at Yangba jing (4300 m a.s.l.), China. The threshold energy of observed air shower is estimated to be 1.5 TeV and 1.0 TeV for protons and gamma rays, respectively. The angular resolution is estimated to be 0.95° ± 0.01° around 3 TeV using a Monte Carlo simulation. This angular resolution is well confirmed by the cosmic-ray shadow by the moon observed during 83.0-day live time.

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