Comparison of hadron chamber data from the PAMIR experiment with model calculations for different chemical compositions of primary cosmic rays

Details Comparison of hadron chamber data from the PAMIR experiment with model calculations for different chemical compositions of primary cosmic rays Comparison of hadron chamber data from the PAMIR experiment with model calculations for different chemical compositions of primary cosmic rays

Apr 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993roizf..57...53b&link_type=abstract

Rossijskaya Akademiya Nauk, Izvestiya, Seriya Fizicheskaya (ISSN 0367-6765), vol. 57, no. 4, p. 53-55.

Computer Science

Cosmochemistry, Energetic Particles, Hadrons, Primary Cosmic Rays, Gamma Rays, Monte Carlo Method

Scientific paper

Data obtained from nine hadron chambers used in the Pamir experiments are compared with the results of a Monte Carlo simulation of hadron and gamma families for various assumptions concerning the composition of primary cosmic rays. It is found that the characteristics of the families eliminate the possibility of iron dominance in the primary cosmic rays.

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