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High Energy Radiation Near the Earth

  • S. F. Singer
Conference paper

Abstract

It is well to have a term which specifically denotes the solar high-energy particles, in contradistinction to the galactic cosmic rays and the low-energy particles which come from the sun and which are responsible for the aurora, magnetic storms and so forth. A term for solar high-energy particles, which is currently being used by such people as Neher, Gold, Kellogg and Winckler, is the SHEP. As SHEPs consist mainly of protons, this terminology might also stand for “solar high-energy proton.” To be specific, however, we usually speak of SHEP-protons, SHEP-alphas, etc.

Keywords

Solar Flare Radiation Belt Trap Particle High Energy Radiation GEIGER Counter 
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

  1. 1.
    S. C. Freden and R. S. White, Particle Fluxes in the Inner Radiation Belt. J. Geophys. Res. 65, 1377–83 (1960).ADSCrossRefGoogle Scholar
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    A. M. Lenchek and S. F. Singer, Geomagnetically Trapped Protons from Cosmic- Ray Albedo Neutrons. J. Geophys. Res. 67, 1263–87 (1962).ADSCrossRefGoogle Scholar
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    A. M. Lenchek et al., Geomagnetically Trapped Electrons from Cosmic-Ray Neutrons. J. Geophys. Res. 66, 4027–46 (1961).ADSCrossRefGoogle Scholar
  4. 4.
    S. F. Singer and A. M. Lenchek, Geomagnetically Trapped Radiation. Progress in Elementary Particle and Cosmic-Ray Physics, edited by J. G. WILSON and S. A. Wouthuysen, Vol. 6, p. 247–385. Amsterdam: North Holland Publ. Co., 1962.Google Scholar
  5. 5.
    D. K. Bailey, Time Variations of the Energy Spectrum of Solar Cosmic Rays in Relation to the Radiation Hazard in Space. J. Geophys. Res. 67, 391 - 96Google Scholar

Copyright information

© Springer-Verlag 1964

Authors and Affiliations

  • S. F. Singer
    • 1
  1. 1.National Weather Satellite CenterU.S. Weather BureauWashington, D.C.USA

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