Cosmic Ray Energetics And Mass : Expected Performance

Details Cosmic Ray Energetics And Mass : Expected Performance Cosmic Ray Energetics And Mass : Expected Performance

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....6.2159a&link_type=abstract

Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int

Physics

1

Scientific paper

The Cosmic Ray Energetics And Mass (CREAM) experiment is being constructed to study high energy cosmic rays over the approximate energy range from 1 TeV to > 5 × 1014 eV. CREAM is enabled by the Ultra Long Duration Balloon (ULDB) capability being developed by NASA, which will provide 60 to 100 days of flight duration. The instrument includes a sampling tungsten calorimeter, a transition radiation detector, and a timing-based charge detector. We will present details of the instrument configuration and simulated results of its performance, including trigger and data rates, energy resolution, energy response, etc.

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