Fluctuations of development maximum depth and nuclear composition of primary cosmic radiation

Details Fluctuations of development maximum depth and nuclear composition of primary cosmic radiation Fluctuations of development maximum depth and nuclear composition of primary cosmic radiation

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....2..182d&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 2 p 182-185 (SEE N85-34006 22-93)

Computer Science

Cerenkov Radiation, Depth Measurement, Electron Photon Cascades, Energy Spectra, Primary Cosmic Rays, Proton Density (Concentration), Atomic Structure, Chemical Composition, Cosmic Ray Showers, Nuclear Chemistry

Scientific paper

The extensive air showers (EAS) cascade curves from the Cerenkov light lateral distribution measurements are recovered and the maximum depth fluctuations of the shower development theta xm both on the Cerenkov and charged EAS components are defined. At E0 approximates 10 to the 18th power eV the mean content of protons is greater than 85%, and p-air cross section theta0 p-air 750mb.

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