EAS development curve at energy of 10(16) - 10(18) eV measured by optical Cerenkov light

Details EAS development curve at energy of 10(16) - 10(18) eV measured by optical Cerenkov light EAS development curve at energy of 10(16) - 10(18) eV measured by optical Cerenkov light

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....7..171h&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 7 p 171-174 (SEE N85-35968 24-93)

Mathematics

Atmospheric Attenuation, Cerenkov Radiation, Cosmic Ray Showers, Energy Spectra, Cerenkov Counters, Computerized Simulation, Mathematical Models, Spectral Energy Distribution

Scientific paper

The data of optical Cerenkov light from extensive air shower observed at the core distance more than 1 Km at Akeno are reexamined. Applying the new simulated results, the shower development curves for the individual events were constructed. For the showers of 10 to 17th power eV the average depth at the shower maximum is determined to be 660 + or - 40 gcm/2. The shower curve of average development is found to be well described by a Gaisser-Hillas shower development function with above shower maximum depth.

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