Relative abundances of nuclei of Z not less than 10 and not greater than 26 in medium energy cosmic rays

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Abundance, Cosmic Rays, Interstellar Matter, Nuclear Particles, Particle Energy, Approximation, Energetic Particles, Ionization Potentials, Normal Density Functions, Nuclear Fusion, Solid State Devices

Scientific paper

Abundances of primary cosmic-ray nuclei from neon to iron, in the energy interval 200 to 650 MeV/n, have been determined using a balloon-exposed cellulose nitrate plastic detector. These abundances have been extrapolated back to the source regions using various models of cosmic ray interstellar propagation. Some aspects of cosmic-ray propagation and origin have been discussed in the light of results of the present experiment.

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