Core structure of EAS in 10(15) to 10(17) eV

Details Core structure of EAS in 10(15) to 10(17) eV Core structure of EAS in 10(15) to 10(17) eV

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....7...77h&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 7 p 77-80 (SEE N85-35968 24-93)

Computer Science

Attenuation, Cosmic Ray Showers, Particle Density (Concentration), Calorimeters, Chemical Composition, Energy Spectra, Heavy Nuclei, Scintillation Counters

Scientific paper

With the use of Akeno calorimeter, the attenuation of particles in concrete is analyzed as the function of the shower size of 10 to the 5th power to 10 to the 7th power. The attenuation length does not depend much on the shower size but depends a little on the shower age. The average value is approx. 150 g/sq cm for s = 0.5 to 0.85 and approx. 40 g/sq cm for s = 0.85 to 1.15. These values and their fluctuations are consistent with the equi-intensity curves of extensive air showers (EAS).

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