Abstract
In this brief review we are able only to consider the general characteristics of the trapped ≽ 100 keV proton population, the principal time variations observed, and the status of major source and transport mechanisms with primary emphasis on diffusion by violation of the third adiabatic invariant.
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Williams, D.J. (1970). Trapped Protons ≽100 ke V and Possible Sources. In: McCormac, B.M. (eds) Particles and Fields in the Magnetosphere. Astrophysics and Space Science Library, vol 17. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-3284-1_37
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DOI: https://doi.org/10.1007/978-94-010-3284-1_37
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