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AGU: Geophysical Research Letters

 

Index Terms

  • Magnetospheric Physics: Radiation belts
  • Magnetospheric Physics: Energetic particles: precipitating
  • Magnetospheric Physics: Energetic particles: trapped
  • Magnetospheric Physics: Magnetosphere: inner
  • Space Plasma Physics: Wave/particle interactions

Abstract

Multidimensional quasi-linear diffusion of radiation belt electrons

J. M. Albert

Space Vehicles Directorate, Air Force Research Laboratory, Hanscom Air Force Base, Massachusetts, USA

S. L. Young

Space Vehicles Directorate, Air Force Research Laboratory, Hanscom Air Force Base, Massachusetts, USA

We consider diffusion of outer zone radiation belt electrons by chorus waves. Quasi-linear diffusion coefficients valid outside the plasmasphere have only been calculated recently, and indicate that the energy and cross diffusion rates can be comparable to that for pitch angle diffusion. Proper solution of the diffusion equation for phase space density must therefore be based on the full diffusion tensor, but this has been plagued by numerical problems associated with the large and rapidly varying cross terms. To circumvent this, techniques are developed for transforming to variables in which the cross diffusion term vanishes. A model calculation shows significant diffusion of phase space density at L = 4.5 from 0.2 MeV up to a few MeV in less than a day.

Received 8 April 2005; accepted 28 June 2005; published 28 July 2005.

Citation: Albert, J. M., and S. L. Young (2005), Multidimensional quasi-linear diffusion of radiation belt electrons, Geophys. Res. Lett., 32, L14110, doi:10.1029/2005GL023191.

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