Composition of Primary Cosmic Rays Beyond the ``Knee''from Emulsion Chamber Observations

Details Composition of Primary Cosmic Rays Beyond the ``Knee''from Emulsion Chamber Observations Composition of Primary Cosmic Rays Beyond the ``Knee''from Emulsion Chamber Observations

1996-02-21

arxiv.org/abs/astro-ph/9602108v1

Phys.Rev. D54 (1996) 5558-5562

Astronomy and Astrophysics

Astrophysics

Revtex, 11 pages, 5 postscript figures ("\special" command used to embed figures at end of tex file). Compressed postscript ve

Scientific paper

10.1103/PhysRevD.54.5558

We show that the simplest assumptions for the dynamics of particle production
allow us to understand the fluxes of hadrons and photons at mountain altitudes
as well as the structure of individual events. The analysis requires a heavy
nuclear component of primary cosmic rays above the ``knee" in the spectrum with
average mass number $ = 7.3 \pm 0.9$.

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