MHD stability of JT-60SA operation scenarios driven by passing energetic particles for a hot Maxwellian model
J. Varela, K. Y. Watanabe, K. Shinohara, M. Honda, Y. Suzuki, J., Shiraishi, D. A. Spong, L. Garcia

TL;DR
This paper investigates how passing energetic particles influence MHD stability in JT-60SA, predicting potential instabilities and their effects on plasma confinement using advanced modeling techniques.
Contribution
It introduces a comprehensive analysis of energetic particle effects on MHD modes in JT-60SA using the FAR3d code with a Maxwellian EP distribution, including acoustic mode effects.
Findings
Destabilization of specific Alfvén eigenmodes at certain frequencies.
Increased EP beta leads to overlapping AEs and potential transport enhancement.
EPs can stabilize resistive ballooning modes, especially with low-energy populations.
Abstract
We analyze the effects of the passing energetic particles on the resistive ballooning modes (RBM) and the energetic particle driven modes in JT-60SA plasma, which leads to the prediction of the stability in N-NBI heated plasma. The analysis is performed using the code FAR3d that solves the reduced MHD equations describing the linear evolution of the poloidal flux and the toroidal component of the vorticity in a full 3D system, coupled with equations of density and parallel velocity moments for the energetic particle (EP) species assuming an averaged Maxwellian EP distribution fitted to the slowing down distribution, including the effect of the acoustic modes. The simulations show the possible destabilization of a 3/2-4/2 TAE with a frequency (f) of 115 kHz, a 6/4-7/4 TAE with f=98 kHz and a 6/4 or 7/4 BAE with f=57 kHz in the ITER-like inductive scenario. If the energetic particle beta…
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