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Cosmic X-Rays, γ-Rays, and Electrons

  • R. R. Daniel

Abstract

When cosmic rays were discovered during the beginning of this century, they were thought to be all due to electrons.‡ However, subsequent work clearly demonstrated that this was incorrect and that, cosmic rays consist almost exclusively of protons and heavier nuclei. The search for a small flux of electrons, however, continued without much success for a long time. It was only during the last five years or so that the existence of a small but finite flux of electrons of cosmic origin has been conclusively established. As for X-rays it was only in 1962 that the first observations were made on X-rays of extrasolar origin. The discovery of these two weak components of the cosmic radiation is a natural consequence of recent advances achieved in detector systems and in the technology of high flying stratospheric balloons and space vehicles.

Keywords

Compton Scattering Weak Magnetic Field Cosmic Radiation Production Spectrum Discrete Source 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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References

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    B. Agrinier, Y. Koechlin, B. Parlier, J. Vasseur, C. J. Bland, G. Boella, G. Degli Antoni, C. Dilworth, B. Scarsi, and G. Sironi, Proc. of the International Conference on Cosmic Rays, The Institute of Physics and the Physical Society, London, 1965.Google Scholar
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    R. R. Daniel and S. A. Stephens, Rhys. Rev. Letters. 15: 768 (1965).ADSGoogle Scholar
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    Brunstein and Cline, preprint, 1965.Google Scholar

Copyright information

© Springer Science+Business Media New York 1968

Authors and Affiliations

  • R. R. Daniel
    • 1
  1. 1.Tata Institute of Fundamental ResearchBombayIndia

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