Multicomponent extensive air shower observations at EAS-TOP.

Details Multicomponent extensive air shower observations at EAS-TOP. Multicomponent extensive air shower observations at EAS-TOP.

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997nuphs..54..263.&link_type=abstract

Nuclear Physics B, Proc. Suppl., Vol. 54B, p. 263 - 270

Physics

Nuclear Physics

Cosmic Rays: Air Showers, Cosmic Rays: Detectors

Scientific paper

The study of cosmic rays at primary energies E0 > 1014eV requires the detection of the different components of extensive air showers through ground based stations. EAS-TOP is such an array (located at Campo Imperatore, National Gran Sasso Laboratories), including detectors of the electromagnetic, muon, hadron and atmospheric Cherenkov light components. The combined operation of the detectors is discussed from the point of view of the capability of measuring the cosmic ray primary spectrum and composition. The main lines for checking the significant features of the high energy hadron interaction model used for the interpretation of the data are outlined.

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