Study of CR primaries and their cascades at E0 = 10-100 TeV through EAS-TOP and MACRO

Details Study of CR primaries and their cascades at E0 = 10-100 TeV through EAS-TOP and MACRO Study of CR primaries and their cascades at E0 = 10-100 TeV through EAS-TOP and MACRO

2001-12-20

arxiv.org/abs/astro-ph/0112475v1

Astronomy and Astrophysics

Astrophysics

Contribution to TAUP2001, Sep. 8-12, 2001, Assergi (Italy)

Scientific paper

A measurement of the lateral distribution of Cherenkov light in Extensive Air Showers (EAS) at E0 = 10-100 TeV and a study of the compatibility of the photon number spectra with the expectations from the direct measurements of p and He spectra and the Corsika-QGSJET propagation code in the atmosphere have been performed at the National Gran Sasso Laboratories by the EAS-TOP and MACRO arrays. The telescope array of EAS-TOP has been used as the Cherenkov light detector. The muon tracking system of MACRO in the deep underground Gran Sasso Laboratories (Emuon> 1.3 TeV) served as the EAS detector, including core localization and arrival direction.

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