Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc....7...54m&link_type=abstract
IN: International Cosmic Ray Conference, 18th, Bangalore, India, August 22-September 3, 1983, Conference Papers. Volume 7 (A85-2
Astronomy and Astrophysics
Astronomy
Cosmic Rays, Monte Carlo Method, Muons, Cosmic Ray Showers, Gamma Ray Astronomy, High Energy Interactions
Scientific paper
Monte Carlo simulations are made in order to determine the cosmic ray composition between 10 to the 14th eV and 10 to the 15th eV, using recent results of CERN pp-collider experiments. Positive evidence for the increasing heavy nuclei in the cosmic rays between 10 to the 14th eV and 10 to the 15th eV could not be found. It is shown that an underground muon detector with total area of 10,000 sq m will be able to measure the cosmic ray composition between 10 to the 16th eV and 10 to the 17th eV. High energy astronomical gamma-rays will be possibly detected by this system, selecting mu-less air showers.
Bianco Pasquale
Muraki Yasushi
Okada Akihiko
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