Properties of 10 (18)-10 (19)eV EAS at far core distance

Details Properties of 10 (18)-10 (19)eV EAS at far core distance Properties of 10 (18)-10 (19)eV EAS at far core distance

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....7..320t&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 7 p 320-323 (SEE N85-35968 24-93)

Physics

Charge Distribution, Cores, Cosmic Ray Showers, Density Measurement, Directivity, Electron Distribution, Lateral Stability, Particle Density (Concentration), Shock Fronts, Thermal Neutrons, Charged Particles, Galactic Cosmic Rays, Rates (Per Time)

Scientific paper

The properties of 10 to the 18th power - 10 to the 19th power eV EAS showers such as the electron lateral distribution, the muon lateral distribution ( 1Gev), the ratio of muon density to a electron density, the shower front structure and the transition effects in scintillator of 5cm thickness are investigated with the Akeno 4 sq km/20sq km array at far core distances between 500m and 3000m. The fluctuation of densities and arrival time increase rapidly at core distances greater than 2km.

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