Study of the c.r. composition and interaction at E0=10-100TeV from the observation of H.E. muons and atmospheric Cherenkov light in EAS

Details Study of the c.r. composition and interaction at E0=10-100TeV from the observation of H.E. muons and atmospheric Cherenkov light in EAS Study of the c.r. composition and interaction at E0=10-100TeV from the observation of H.E. muons and atmospheric Cherenkov light in EAS

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999nuphs..75..259a&link_type=abstract

Nuclear Physics B Proceedings Supplements, Volume 75, Issue 1-2, p. 259-261.

Physics

Nuclear Physics

1

Scientific paper

In the energy region 10-100TeV both the c.r. composition from direct measurements and the cross section for high energy secondary production in the very forward region for p-air interactions are rather uncertain. Contemporaneous measurements of the total energy and of the threshold energy/nucleon of the primary particle can be provided by the atmospheric Cherenkov light and high energy muons. These measurements are performed by the combined operation of the Cherenkov array of the EAS-TOP experiment on the surface (810gcm2 atmospheric depth) and of the LVD experiment in the underground Gran Sasso Laboratories (3300mw.e.; Eμth=1.3TeV) leading to the measurement of (Eμ>1.3TeV,E0) in the given energy range. The combined operation of the experiments and preliminary results are reported.

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