An analysis of primary cosmic-ray composition at energies around 10 to the 14th eV using single-shower events observed by mountain emulsion chamber

Details An analysis of primary cosmic-ray composition at energies around 10 to the 14th eV using single-shower events observed by mountain emulsion chamber An analysis of primary cosmic-ray composition at energies around 10 to the 14th eV using single-shower events observed by mountain emulsion chamber

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987hepnp..10..641h&link_type=abstract

(High Energy Physics and Nuclear Physics, vol. 10, Dec. 1986, p. 641-646) Chinese Physics (ISSN 0273-429X), vol. 7, July-Sept. 1

Physics

Nuclear Physics

2

Chemical Composition, Cosmic Ray Showers, Nuclear Emulsions, Particle Energy, Primary Cosmic Rays, Attenuation, Computerized Simulation, Energy Spectra, Hadrons, Monte Carlo Method, Spectral Energy Distribution

Scientific paper

Emulsion chamber X-ray films with 8.3 sq m x yr exposure from the Mt. Kanbala experiments were measured and the energy spectra, attenuation lengths, and vertical fluxes of single gamma rays and hadron showers with visible energies of 3-20 TeV were obtained. A hadronic interaction model was constructed empirically by analyzing the collider data, and was used to simulate the atmospheric propagation of cosmic ray particles in the primary energy region 5 x 10 to the 12th to 10 to the 15th eV. Comparison of the simulation results with the experimental data provided a preliminary determination of the primary composition of cosmic rays at energies around 10 to the 14th eV.

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