Comments on the measurements of multiple muon phenomena

Details Comments on the measurements of multiple muon phenomena Comments on the measurements of multiple muon phenomena

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....8...73s&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 8 p 73-76 (SEE N85-36066 24-93)

Astronomy and Astrophysics

Astrophysics

Atmospheric Energy Sources, Cosmic Ray Showers, Gamma Rays, Muons, Particle Trajectories, Astrophysics, Computerized Simulation, Monte Carlo Method, Muon Spin Rotation, Primary Cosmic Rays

Scientific paper

The extensive air showers in the energy around 10 to the 15th power eV include those initiated by astrophysical primary gamma-rays. The observations need a precise measurement on the directions of primary particles. It is one of the methods to measure the directions of high-energy muons in air showers. The accuracy in measuring the direction, by calculating the cosmic-ray phenomena in the atmosphere at very high energy was investgated. The results calculated by Monte Carlo method suggest that one may determine the direction of primary cosmic-rays within errors of 10/3 rad in observing muons of above 100 GeV at sea level.

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