Physics
Scientific paper
Aug 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975phlc...20...59h&link_type=abstract
Physics Letters, Section C - Physics Reports, vol. 20C, Aug. 1975, p. 59-136.
Physics
Energy Spectra, Particle Flux Density, Primary Cosmic Rays, Radiation Measurement, Bibliographies, Cosmic Ray Showers, Electron Flux Density, Galactic Radiation, Gamma Rays, High Energy Interactions, Solar System, Synchrotron Radiation
Scientific paper
This report summarizes recent developments relating to the primary cosmic-ray flux, the origin of these particles, and their propagation. Topics include the flux of nuclei below 1000 GeV, the primary flux between 10 to the 11th power and 10 to the 20th power eV, problems of high-energy interactions, the electron flux, primary gamma rays, arrival directions of cosmic rays, penetration of cosmic rays into the solar system, propagation of cosmic-ray particles in the galaxy, cosmic rays of extragalactic origin, and possible sources of cosmic rays. It is concluded that most cosmic rays with energies of at least 100 MeV most probably originate in our Galaxy.
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