Study of high energy cosmic ray interactions and primary composition at energies 1015 1017 eV using mountain based detectors

Details Study of high energy cosmic ray interactions and primary composition at energies 1015 1017 eV using mountain based detectors Study of high energy cosmic ray interactions and primary composition at energies 1015 1017 eV using mountain based detectors

Apr 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002phrvd..65g2004k&link_type=abstract

Physical Review D, vol. 65, Issue 7, id. 072004

Physics

7

Cosmic-Ray Interactions

Scientific paper

A new analysis of mountain-top x-ray emulsion chamber data is presented. We utilize a refined experimental apparatus and a standardized analysis approach, including the simulated data. The results indicate that most of the phenomena reported previously can be explained as fluctuations within standard hadronic interaction physics. In the wide energy region we see no indication of a large change in the primary composition.

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