Physics
Scientific paper
Aug 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....2..154l&link_type=abstract
In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol.2 p 154-157 (SEE N85-34006 22-93)
Physics
Cosmic Ray Showers, Energy Spectra, Nucleons, Electron Energy, Electrons, Muons, Neutrinos, Spectrum Analysis
Scientific paper
Both the maximum size Nm and the sea level muon size Nmu have been used separately to find the all-particle energy spectrum in the air shower domain. However the conversion required, whether from Nm to E or from Nmu to E, has customarily been carried out by means of calculations based on an assumed cascase model. It is shown here that by combining present data on Nm and Nmu spectra with data on: (1); the energy spectrum of air shower muons and (2) the average width of the electron profile, one can obtain empirical values of the Nm to E and Nmu to E conversion factors, and an empirical calorimetric all-particle spectrum, in the energy range 2 x 10 to the 6th power E 2 x 10 to the 9th power GeV.
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