Cosmic ray composition between 10 to the 15th power - 10 to the 17th power eV obtained by air shower experiments

Details Cosmic ray composition between 10 to the 15th power - 10 to the 17th power eV obtained by air shower experiments Cosmic ray composition between 10 to the 15th power - 10 to the 17th power eV obtained by air shower experiments

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....2..178m&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 2 p 178-181 (SEE N85-34006 22-93)

Computer Science

Chemical Composition, Cosmic Ray Showers, Energy Spectra, Particle Interactions, Primary Cosmic Rays, Collision Parameters, Collision Rates, Iron Isotopes, Monte Carlo Method, Protons, Scattering

Scientific paper

Based on the air shower data, the chemical composition of the primary
cosmic rays in the energy range 10 to the 15th power - 10 to the 17th
power eV was obtained. The method is based on a well known
Ne-N sub mu and Ne-N sub gamma. The simulation is
calibrated by the CERN SPS pp collider results.

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