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Comprehensive results are presented in graphic form for nucleons with energies equal to or greater than 500 MeV., based on calculations using a new cross section for nucleon-nucleon collisions and in the light of recent experimental evidence. The results obtained are in good agreement with existing experimental observations and it is felt that the high-energy nucleon component of the cosmic radiation can now be satisfactorily accounted for by our theory. The basic assumptions underlying the theory are discussed
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H. Messel (1951) studied this question.
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