Very high energy cosmic ray events

Details Very high energy cosmic ray events Very high energy cosmic ray events

Apr 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984nupha.418..139j&link_type=abstract

Nuclear Physics A, Volume 418, p. 139-160.

Physics

Nuclear Physics

5

Scientific paper

High energy cosmic rays are reviewed in terms of our present understanding of prominent features in the primary energy spectrum. The spectral change observed around 1015 eV can be explained either by a change in the primary chemical composition or by a change in the nuclear interaction characteristics. Anomalous interactions are prevalent at about the same energy where galactic propagation effects are expected to lead to the dominance of iron nuclei.
Research supported by the U.S. National Science Foundation.

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