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High Energy Radiation Near the Earth

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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.

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References

  1. S. C. Freden and R. S. White, Particle Fluxes in the Inner Radiation Belt. J. Geophys. Res. 65, 1377–83 (1960).

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  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 - 96

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© 1964 Springer-Verlag

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Singer, S.F. (1964). High Energy Radiation Near the Earth. In: Ehmert, A. (eds) The Space Environment / Le Milieu Spatial. Springer, Vienna. https://doi.org/10.1007/978-3-7091-5479-3_7

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  • DOI: https://doi.org/10.1007/978-3-7091-5479-3_7

  • Publisher Name: Springer, Vienna

  • Print ISBN: 978-3-7091-5481-6

  • Online ISBN: 978-3-7091-5479-3

  • eBook Packages: Springer Book Archive

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