Monte Carlo simulation of EAS generated by 10(14) - 10(16) eV protons

Details Monte Carlo simulation of EAS generated by 10(14) - 10(16) eV protons Monte Carlo simulation of EAS generated by 10(14) - 10(16) eV protons

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....7..143f&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 7 p 143-146 (SEE N85-35968 24-93)

Other

Cosmic Ray Showers, Electron Distribution, Energy Spectra, Monte Carlo Method, Simulation, Altitude, Chemical Composition, Electron Photon Cascades, Gamma Ray Telescopes, Sea Level

Scientific paper

Detailed Monte Carlo simulations of extensive air showers to be detected by the Homestake Surface Underground Telescope and other similar detectors located at sea level and mountain altitudes have been performed for 10 to the 14th power to 10 to the 16th power eV primary energies. The results of these Monte Carlo calculations will provide an opportunity to compare the experimental data with different models for the composition and spectra of primaries and for the development of air showers. The results obtained for extensive air showers generated by 10 to the 14th power to 10 to the 16th power eV primary protons are reported.

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