A Diffusion Model of Radial Distributions of Energetic Protons in Saturn's Magnetosphere

Details A Diffusion Model of Radial Distributions of Energetic Protons in Saturn's Magnetosphere A Diffusion Model of Radial Distributions of Energetic Protons in Saturn's Magnetosphere

Jul 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004cosre..42..370g&link_type=abstract

Cosmic Research, v. 42, Issue 4, p. 370-373 (2004).

Physics

Scientific paper

A simple diffusion model of Saturn's radiation belts with a constant internal source and particle losses at the boundaries is considered. The radial diffusion coefficient is supposed to be DLL ~ L4. The analytical solution to the stationary diffusion equation describes well the observed radial profiles of the distribution function of energetic protons in Saturn's magnetosphere.

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