Understanding the physics of energetic ions, in particular their nonlinear resonance interactions with Alfvén waves, is central to more » improving the heating performance of magnetically confined plasmas for future energy generation. The ability of computational models to properly account for physical effects that underlie such interactions, namely ion kinetic, ion cyclotron, Hall, collisional and ionization processes is important for the success and planning of experimental research in plasma physics. Global interactions of energetic ions with magnetoplasmas and neutral gases lie at the core of many space and laboratory plasma phenomena ranging from solar wind entry into and transport within planetary magnetospheres and exospheres to fast-ion driven instabilities in fusion devices to astrophysics-in-lab experiments. = in excess of 4 could be achieved in this manner.
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