Study of Cosmic Ray Primaries between 1012 and 1016 eV from EAS-TOP

Details Study of Cosmic Ray Primaries between 1012 and 1016 eV from EAS-TOP Study of Cosmic Ray Primaries between 1012 and 1016 eV from EAS-TOP

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....1..147n&link_type=abstract

Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I

Physics

5

Scientific paper

The EAS-TOP experiment has been in operation since January 1989 to May 2000 in the study of cosmic ray physics in the energy range between the direct measurements and the "giant" air shower arrays (E0 = 1012 ÷ 1016 eV, including the knee of the primary spectrum). The array was located at Camp o imperatore, 2000 m a.s.l., 300 with respect to the vertical of the underground Gran Sasso Laboratories, which allowed operation in stand alone mode, and in coincidence with the underground TeV muon detectors (MACRO, LVD). Different detectors and techniques: hadrons, EAS Cherenkov light and TeV muons, e.m., GeV, and TeV muon EAS components, and their correlated analysis, have been exploited, providing measurements in different energy ranges. The resulting scenario of the high energy galactic cosmic radiation concerning the primary spectrum, composition and anisotropies is presented.

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