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

The EAS-TOP·MACRO Collaborations
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Abstract

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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The EAS-TOP, MACRO Collaborations. 2001-12-20. Study of CR primaries and their cascades at E0 = 10-100 TeV through EAS-TOP and MACRO. https://arxiv.org/abs/astro-ph/0112475

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