On the halo events observed by Mount Fuji and Mount Kanbala Emulsion Chamber Experiments

Details On the halo events observed by Mount Fuji and Mount Kanbala Emulsion Chamber Experiments On the halo events observed by Mount Fuji and Mount Kanbala Emulsion Chamber Experiments

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....6..336r&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 6 p 336-339 (SEE N85-35848 24-93)

Computer Science

Cosmic Rays, Gamma Rays, Halos, Models, Nuclear Interactions, Protons, Abundance, Cosmic Ray Showers, Detection, Energy Spectra, Monte Carlo Method, Nuclear Emulsions, Protons, Scaling Laws, Simulation

Scientific paper

The intensity of big gamma-ray families associated by halo is obtained from Mt. Fuji experiment (650 g/sq.cm. atmospheric depth) and Mt. Kanbala experiment (515 g/sq.cm.). The results are compared with Monte Carlo calculation based on several assumptions on interaction mechanisms and the primary cosmic ray composition. The results suggest more than 3 times lower proton abundance among primaries than that of 10 to the 12th to 10 to the 13th eV region within the framework of quasi-scaling model of multiple production.

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