EAS accompanied by gamma-families at Mt. Norikura and comparison with Monte Carlo simulation

Details EAS accompanied by gamma-families at Mt. Norikura and comparison with Monte Carlo simulation EAS accompanied by gamma-families at Mt. Norikura and comparison with Monte Carlo simulation

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....6..301s&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 6 p 301-304 (SEE N85-35848 24-93)

Computer Science

Cosmic Ray Showers, Gamma Rays, Ionization Cross Sections, Monte Carlo Method, Atmospheric Scattering, Energy Distribution, Particle Size Distribution, Primary Cosmic Rays, Protons

Scientific paper

The experimental data of extensive air showers (EAS) accompanied by gamma-families, with total energy greater than 10 TeV, were compared with a Monte Carlo simulation with a rising cross section proportional to E0.04 for the p-air inelastic cross section. It is found that the absolute intensity of size spectrum of such EAS is strongly affected by the primary protons intensity at 10 to the 15th power approx. 10 to the 16th power eV region and the experimental size spectrum agrees with the simulated spectra for the p-poor primary composition better than the p-rich one.

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