A new simple model for equatorialy mirroring protons, based on classic
al radial diffusion, is used here to understand the global long term d
ynamics of the ring current ion population. The convection access for
low energy particles coming from the plasmasheet is used as a source p
opulation. Then magnetospheric acceleration processes are reproduced b
y using a Kp dependent radial diffusion coefficient. Comparing the res
ults with CRRES satellite energetic ion measurements from the fifteen
months of the total mission yields very good quantitative agreement fo
r similar to 80 keV ring-current protons and good qualitative agreemen
t with similar to 300 keV ions.