Intensities of high-energy cosmic rays at Mount Kanbala

Details Intensities of high-energy cosmic rays at Mount Kanbala Intensities of high-energy cosmic rays at Mount Kanbala

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....6..439r&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 6 p 439-442 (SEE N85-35848 24-93)

Computer Science

Bubble Chambers, Cosmic Ray Showers, Energy Spectra, Gamma Ray Bursts, Hadrons, Monte Carlo Method, Primary Cosmic Rays, Proton Beams, Scaling Laws, Scattering Cross Sections, Simulation, Galactic Cosmic Rays, Quantum Chromodynamics

Scientific paper

General features of family events with Summary Egamma 200 TeV, observed by the emulsion chambers at Mt. Kanbala, are presented in comparison with the Monte Carlo simulation. The lateral and cluster structure, and the energy spectra of constituent gamma-rays and hadrons are shown to be consistent with the Monte Carlo results calculated under the assumption of heavy-enriched primary, scaling, QCD jets and increasing cross-section.

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