Relation between gamma-ray family and EAS core: Monte-Carlo simulation of EAS core

Details Relation between gamma-ray family and EAS core: Monte-Carlo simulation of EAS core Relation between gamma-ray family and EAS core: Monte-Carlo simulation of EAS core

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....6..407y&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 6 p 407-410 (SEE N85-35848 24-93)

Computer Science

Collision Parameters, Cosmic Ray Showers, Electron Density Profiles, Gamma Ray Bursts, Hadrons, Models, Monte Carlo Method, Particle Interactions, Simulation, Spark Chambers, Transverse Acceleration, Balloon-Borne Instruments, Charged Particles, Galactic Cosmic Rays, Heavy Nuclei, Helium, Mountains

Scientific paper

Preliminary results of Monte-Carlo simulation on Extensive Air Showers
(EAS) (Ne=100,000) core is reported. For the first collision at the top
of the atmosphere, high multiplicity (high rapidity, density) and a
large Pt (1.5GeV average) model is assumed. Most of the simulated cores
show a complicated structure.

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