Computer Science
Scientific paper
Aug 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc....5..344l&link_type=abstract
IN: International Cosmic Ray Conference, 18th, Bangalore, India, August 22-September 3, 1983, Conference Papers. Volume 5 (A85-2
Computer Science
Cosmic Rays, Hadrons, Monte Carlo Method, Particle Intensity, Sea Level, Computerized Simulation, Energy Spectra, Environment Simulation, High Energy Interactions, Lower Atmosphere, Nucleon-Nucleon Interactions, Pions
Scientific paper
Predictions for the intensities of accompanied particles in ground level detectors have been calculated by using a Monte Carlo method for the simulation of hadron cascades in the atmosphere. Estimates for the intensities of all hadrons and of groups of more than one hadron per square meter are given. Also the pion-to-nucleon ratio has been determined as a function of primary energy. The results are compared with experimental measurements made with a hadron spectrometer.
Lumme M.
Nieminen M.
Peltonen Juhani
Torsti Jarmo
Vainikka E.
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