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..204r&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 6 p 204-207 (SEE N85-35848 24-93)

Physics

1

Cosmic Rays, Energy Spectra, Hadrons, Heavy Nuclei, Nuclear Emulsions, Flux (Rate), Optical Density, Particle Production

Scientific paper

The energy spectra of atmospheric cosmic rays at Mt. Kanbala (520 g/cm2) are measured with emulsion chambers. The power indices of the spectra are values of about 2.0 for both gamma-rays and hadrons. Those fluxes are consistent with the ones expected from the model of primary cosmic rays with heavy nuclei of high content in the energy around 1015eV.

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