On the characteristics of emulsion chamber family events produced in low heights

Details On the characteristics of emulsion chamber family events produced in low heights On the characteristics of emulsion chamber family events produced in low heights

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....6..212j&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 6 p 212-215 (SEE N85-35848 24-93)

Computer Science

Cosmic Rays, Inelastic Scattering, Nuclear Emulsions, Nuclear Interactions, Coulomb Potential, Height, Monte Carlo Method, Particle Production

Scientific paper

The uncertainty of the primary cosmic ray composition at 10 to the 14th power -10 to the 16th power eV is well known to make the study of the nuclear interaction mechanism more difficult. Experimentally considering, if one can identify effectively the family events which are produced in low heights, then an event sample induced by primary protons might be able to be separated. It is undoubtedly very meaningful. In this paper an attempt is made to simulate the family events under the condition of mountain emulsion chamber experiments with a reasonable model. The aim is to search for the dependence of some experimentally observable quantities to the interaction height.

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