The thickness of the shower disc as observed in showers produced by primaries above 10 (19)eV

Details The thickness of the shower disc as observed in showers produced by primaries above 10 (19)eV The thickness of the shower disc as observed in showers produced by primaries above 10 (19)eV

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....7..332l&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 7 p 332-335 (SEE N85-35968 24-93)

Physics

Angular Distribution, Cerenkov Radiation, Cores, Cosmic Ray Showers, Particle Density (Concentration), Radiation Counters, Zenith, Charged Particles, Galactic Cosmic Rays, Particle Interactions

Scientific paper

The thickness of the shower disk has been measured in showers initiated by primaries of energy to 10 the 19th power eV using the large area water Cerenkov detectors of the Haverah Park array. Results are presented which (1) provide supporting evidence for the accuracy of analysis procedures in giant showers, (2) offer an evaluation of the mini-array technique for the detection of giant showers and (3) extend earlier work on developmental fluctuations above 10 to the 19th power eV.

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