High-energy cosmic-ray physics with an EAS array on the top of the Gran Sasso Laboratory

Details High-energy cosmic-ray physics with an EAS array on the top of the Gran Sasso Laboratory High-energy cosmic-ray physics with an EAS array on the top of the Gran Sasso Laboratory

Apr 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ncimc...9..262a&link_type=abstract

(Symposium on Underground Physics, 1st, Saint Vincent, Italy, Apr. 25-28, 1985) Nuovo Cimento C, Serie 1 (ISSN 0390-5551), vol.

Astronomy and Astrophysics

Astronomy

29

Cosmic Ray Showers, Gamma Ray Astronomy, High Energy Interactions, Muons, Primary Cosmic Rays, Scintillation Counters, Energy Spectra, Hadrons

Scientific paper

An EAS array comprising 28 10-sq-m scintillator modules (separated by 25 m in a central region and by 100 m in an outer region) and one 12-layer 200-sq-m iron-concrete/streamer-tube hadron-muon detector is proposed for installation above the large-volume detector planned for Gran Sasso Laboratory. The scientific goals of the array include measurement of the total primary energy of multimon events, ultrahigh-energy gamma-ray astronomy, and studies of the primary composition and anisotropies of cosmic rays. Drawings, graphs, and tables of predicted performance data are provided.

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