Computer Science – Numerical Analysis
Scientific paper
Aug 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....8..180l&link_type=abstract
In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 8 p 180-183 (SEE N85-36066 24-93)
Computer Science
Numerical Analysis
Cosmic Rays, Flux Density, Muons, Neutrinos, Particle Diffusion, Charge Distribution, Computerized Simulation, Energy Spectra, Numerical Analysis, Ratios
Scientific paper
The diffusion equation for neutrino-induced cosmic ray muons underground was solved. The neutrino-induced muon flux and charge ratio underground have been calculated. The calculated horizontal neutrino-induced muon flux in the energy range 0.1 - 10000 GeV is in agreement with the measured horizontal flux. The calculated vertical flux above 2 GeV is in agreement with the measured vertical flux. The average charge ratio of neutrino-induced muons underground was found to be mu+/mu- = 0.40.
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