Structure of air shower disc near the core

Details Structure of air shower disc near the core Structure of air shower disc near the core

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....7..316i&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 7 p 316-319 (SEE N85-35968 24-93)

Physics

Cosmic Ray Showers, Coulomb Collisions, Photomultiplier Tubes, Relativistic Particles, Spectral Energy Distribution, Time Dependence, Transverse Acceleration, Cascade Flow, Charged Particles, Electromagnetic Radiation, High Energy Interactions

Scientific paper

The longitudinal structure of the air shower disk is studied by measuring the arrival time distributions of air shower particles for showers with electron size in the range 3.2 x 10 to the 5.5. power to 3.2 x 10 to the 7.5 power in the Akeno air-shower array (930 gcm squared atmospheric depth). The average FWHM as a parameter of thickness of air shower disk increases with core distances at less than 50m. AT the present stage, dependence on electron size, zenith angle and air shower age is not apparent. The average thickness of the air shower disk within a core distance of 50m could be determined by an electromagnetic cascade starting from the lower altitude.

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