Size distributions of air showers accompanied with high energy gamma ray bundles observed at Mt. Chacaltaya

Details Size distributions of air showers accompanied with high energy gamma ray bundles observed at Mt. Chacaltaya Size distributions of air showers accompanied with high energy gamma ray bundles observed at Mt. Chacaltaya

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....6..300m&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 6 p 300 (SEE N85-35848 24-93)

Computer Science

Cosmic Ray Showers, Energy Distribution, Gamma Rays, High Energy Interactions, Nuclear Interactions, Particle Size Distribution, Primary Cosmic Rays, Atmospheric Attenuation, Clumps, Precipitation Particle Measurement, Protons, Size Determination

Scientific paper

Size distributions of air showers accompanied with bundle of high energy gamma rays and/or large size bursts under emulsion chambers, to study the composition of primary cosmic rays and also characteristics of high energy nuclear interaction. Air showers initiated by particles with a large cross section of interaction may develop from narrow region of the atmosphere near the top. Starting levels of air showers by particles with smaller cross section fluctuate in wider region of the atmosphere. Air showers of extremely small size accompanied with bundle of gamma rays may be ones initiated by protons at lower level after penetrating deep atmosphere without interaction. It is determined that the relative size distribution according to the total energy of bundle of gamma rays and the total burst size observed under 15 cm lead absorber.

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