Primary Composition and Energy Spectrum Measurement near 1015 eV with the DICE Detector

Details Primary Composition and Energy Spectrum Measurement near 1015 eV with the DICE Detector Primary Composition and Energy Spectrum Measurement near 1015 eV with the DICE Detector

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998tx19.confe.632k&link_type=abstract

Abstracts of the 19th Texas Symposium on Relativistic Astrophysics and Cosmology, held in Paris, France, Dec. 14-18, 1998. Eds.:

Astronomy and Astrophysics

Astrophysics

Scientific paper

We present the results of a primary composition and primary energy spectrum measurement around 1015 eV made with the DICE-CASA-MIA experiment. We present new data on the muon and electron densities associated with the previously measured Cerenkov light images. An interpretation of the shower parameters and the dept of shower maximum in therms of a primary composition model will be presented.

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