The characteristics of simulated superfamilies of the energy above 400 TeV detected in gamma block of an emulsion chamber

Details The characteristics of simulated superfamilies of the energy above 400 TeV detected in gamma block of an emulsion chamber The characteristics of simulated superfamilies of the energy above 400 TeV detected in gamma block of an emulsion chamber

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aipc..276..414k&link_type=abstract

The seventh international symposium on very high energy cosmic-ray interactions. AIP Conference Proceedings, Volume 276, pp. 41

Computer Science

Cosmic Rays

Scientific paper

The results of simulations of superfamilies (ΣEγ>~500 TeV) are presented by using two-component model. The special processing with γ-quanta far from a family centre is proposed. These γ-quanta carry some information on the development of high energy core of EAS and although this information is poor, the experimental data are rather reliable.

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