Primary mass composition investigations at energies 104 - 107GeV and selection of EAS at mountain altitudes.

Details Primary mass composition investigations at energies 104 - 107GeV and selection of EAS at mountain altitudes. Primary mass composition investigations at energies 104 - 107GeV and selection of EAS at mountain altitudes.

Feb 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995nuphs..39..242p&link_type=abstract

Nuclear Physics B - Proceedings Supplements, vol. 39, issue 1, pp. 242-250

Physics

Nuclear Physics

1

Cosmic Rays: Energy Spectra, Cosmic Rays: Masses

Scientific paper

A new EAS selection method is developed for observation levels 500 ≤ χ0 ≤ 700 g cm-2 and energies 104 - 107GeV. This gives the possibility to obtain a practically unbiased energy spectrum and mass composition estimation in this energy interval. Specific EAS experiments placed at observation levels 500 - 600 g cm-2 are necessary in order to calibrate the indirect methods for obtaining the energy spectrum and mass composition of the primary cosmic flux at energies higher than 106 GeV.

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