
BAS Radiation Belt Model (BAS-RBM)
Simulates changes in the high-energy electron population of the radiation belts taking into account effects such as the changing solar activity and wave-particle interactions.
Simulates changes in the high-energy electron population of the radiation belts taking into account effects such as the changing solar activity and wave-particle interactions.
PADIE [Glauert & Horne, JGR, 2005] calculates relativistic quasi-linear pitch-angle and energy diffusion coefficients for resonant wave-particle interactions in a magnetised plasma.
tracing electromagnetic waves in hot magnetised plasma