Relative abundances of 10≤Z≤26 nuclei in medium energy cosmic rays |
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Authors: | V S Bhatia Gurmukh Singh |
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Institution: | (1) Physics Department, Panjab University, Chandigarh, India |
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Abstract: | Abundances of primary cosmic-ray nuclei from neon to iron, in the energy interval 200 to 650 MeV n–1, 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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