Anomalous radial diffusion by pitch-angle scattering on split drift shells: Calculations

Physics – Plasma Physics

Scientific paper

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[2730] Magnetospheric Physics / Magnetosphere: Inner, [2774] Magnetospheric Physics / Radiation Belts, [7807] Space Plasma Physics / Charged Particle Motion And Acceleration, [7867] Space Plasma Physics / Wave/Particle Interactions

Scientific paper

For geomagnetically trapped particles, when pitch-angle scattering occurs in the presence of drift-shell splitting, radial diffusion occurs as a consequence. Preliminary calculations indicate that during magnetic storms, radiation belt electrons in the vicinity of and beyond geosynchronous orbit may experience such radial diffusion. We present diffusion coefficients for such anomalous radial diffusion, computed for quiet and storm-time magnetic field configurations and plasma wave populations. We compare these calculations to published radial diffusion coefficients for ULF pulsations to determine when and where in phase space this anomalous radial diffusion is significant.

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