Composition of Primary Cosmic Rays at Energies ˜ 10**15 - 10**16 Ev: Analysis of High Energy Muons in Air Showers

Details Composition of Primary Cosmic Rays at Energies ˜ 10**15 - 10**16 Ev: Analysis of High Energy Muons in Air Showers Composition of Primary Cosmic Rays at Energies ˜ 10**15 - 10**16 Ev: Analysis of High Energy Muons in Air Showers

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc....9..187y&link_type=abstract

Proceedings from the 18th International Cosmic Ray Conference, held in Bangalore, India, 22 August - 3 September, 1983. Volume

Computer Science

Scientific paper

The authors compare experimental data on high energy muons with
expectations from their simulations.

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