Plasma waves in the inner magnetosphere play an important role in the dynamics of the radiation belts and ring current (e.g., Thorne, 2010). Gyro-resonant wave-particle interactions in the inner magnetosphere (and space plasmas in general) are typically described in terms of quasilinear (QL) theory (Kennel & Engelmann, 1966). According to this theory, the dynamics of particles are described by a Fokker-Planck-type diffusion equation (Schulz & Lanzerotti, 1974). The diffusion coefficients in this equation encapsulate the physics of wave-particle interactions in the QL limit. As diffusion simulations are the only practical way to model the long-term behavior of the radiation belts and ring current at present, calculation of the diffusion coefficients appropriate for the inner magnetosphere has been the focus of numerous studies (e.g.,