Astronomy and Astrophysics – Astrophysics
Scientific paper
May 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ap%26ss..69..461b&link_type=abstract
Astrophysics and Space Science, vol. 69, no. 2, May 1980, p. 461-470. Research supported by the University Grants Commission.
Astronomy and Astrophysics
Astrophysics
5
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.
Bhatia V. S.
Singh Gurpadam
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