By taking advantage of the trace approximation, one can gain an enormous computational advantage when solving for the global turbulent transport of impurities. In particular, this makes feasible the study of non-Maxwellian transport coupled in radius and energy, allowing collisions and transport to be accounted for on similar time scales, as occurs for fast ions. In this work, we study the fully-nonlinear ITG-driven trace turbulent transport of locally heated and injected fast ions. Previous results indicated the existence of MeV-range minorities heated by cyclotron resonance, and an associated density pinch effect. Here, we build upon this result using the t3core code to solve for the distribution of these minorities, consistently including the effects of collisions, gyrokinetic turbulence, and heating. Using the same tool to study the transport of injected fast ions, we contrast the qualitative features of their transport with that of the heated minorities. Our results indicate that heated minorities are more strongly affected by microturbulence than injected fast ions. The physical interpretation of this difference provides a possible explanation for the observed synergy when NBI heating is combined with ICRH. Furthermore, we move beyond the trace approximation to develop a model which allows one to easily account for the reduction of anomalous transport due to the presence of fast ions in electrostatic turbulence.Fast ions are an important component of a fusion device, being responsible for a portion of heating required to bring tokamaks and stellarators up to fusion-relevant temperatures. Various phenomena can cause radial transport and hence a redistribution of this energy, including: neoclassical transport, transport from nonaxisymmetric magnetic "ripples", stochastic magnetic field regions, Alfvén waves driven unstable by the fast ions themselves, and microturbulence. This latter effect is what we focus on in this work, taking advantage of recently developed tools to study the coupled radiusenergy phase space transport of trace non-Maxwellian species.With the ion cyclotron resonance heating (ICRH) technique, electromagnetic waves are launched into the plasma at a frequency resonant with that of ion cyclotron motion at some locations. Under certain circumstances, a very small population of minority ions can very efficiently absorb the power and be heated up to MeV-range energies [1].