Cosmic ray spectra measurements at the Yakutsk EAS array

Details Cosmic ray spectra measurements at the Yakutsk EAS array Cosmic ray spectra measurements at the Yakutsk EAS array

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....2..198g&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 2 p 198-200 (SEE N85-34006 22-93)

Physics

Cerenkov Radiation, Cosmic Ray Showers, Energy Spectra, Cerenkov Counters, Cosmic Rays, Energy Distribution

Scientific paper

The extensive air showers (EAS) spectra on rho 600 obtained at the Yakutak array for 38000 operation hours in 1974 to 1982 are presented. The refined value of the conversion factor from rho 600 to Eis given and based on it the primary energy spectrum is obtained. The Yakutsk EAS array classifies the showers on parameters which are well measured in real showers: in the central part - on Rho300 and on the whole array - on Rho600. The shower spectra are constructed first on these parameters, than - a single spectrum on Rho600. The RHO300 and Rho600 values are determined on the particle lateral distribution function (LDF) obtained in Yakutsk and on approximation Rho approx. R sup/n using the experimental points closest to R* (300 and 600 m).

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