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    Propagation of cosmic rays in the galaxy (1974)
    In:  CASI
    Details
    Publication Date: 2019-06-27
    Description: The characteristics of a model for analyzing the propagation of cosmic rays are discussed. The requirements for analyzing the relevant observational data on cosmic rays are defines as: (1) the chemical and isotopic composition of cosmic rays as a function of energy, (2) the flux and energy spectrum of the individual nucleonic components, (3) the flux and energy spectrum of the electronic component, (4) the cosmic ray prehistory, and (5) the degree of isotropy in their arrival directions as a function of energy. It is stated that the model which has been able to bring to pass the greatest measure of success is the galactic confinement model.
    Keywords: SPACE RADIATION
    Type: NASA-CR-141190 , TR-75-028
    Format: application/pdf
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