Abstract
Coupling a high-performance core to a low heat flux to the divertor is a crucial step for ITER and any future reactor. DIII-D recently expanded the steady-state hybrid scenario to high density and divertor impurity injection, to study the impact of increased density at high power and the feasibility of a radiating mantle solution. This work presents the physics basis for the trade-offs between density, current drive and stability to tearing modes at high beta. EC power is crucial to tailor the plasma profiles into a passively stable state, and to eject impurities from the core. Off-axis EC depositions decrease the heating efficiency, but calculated electron heat transport coefficients show that this effect is partially mitigated by improved confinement inside the EC deposition. The reduction in pressure is recovered by increasing the density. This favorable scaling of confinement with density was observed in high power plasmas for years, and this work provides a comprehensive explanation. ELITE predictions indicate that a path in peeling-ballooning stability opens up for certain conditions of density, power, q95 and shaping, allowing the edge pressure to continue increasing without encountering a limit. In the core, calculated anomalous fast-ion diffusion coefficients are consistent with density fluctuation measurements in the TAE range, showing that smaller fast-ion losses contribute to the enhanced confinement at high density. The edge integration study shows that divertor heat loads can be reduced with Ne and Ar injection, but this eventually triggers a cascade of n$=$1,2,3 core tearing modes. We can now show that impurity radiation in the core is small and it is not the cause for the drop in confinement at high Ar and Ne injection. The overlap between the core tearing modes is consistent with the loss of pressure as estimated by the Belt model for the coupled rational surfaces. Optimization of these trade-offs has achieved plasmas with sustained H98y2$=$1.7, fGW$=$0.7 and $\sim $85{\%} mantle radiation.
* Work supported in part by the U.S. Department of Energy under DE-FG02-04ER54761, DE- AC02-09CH11466, DE-FC02-04ER54698 and DE-SC0014005. DIII-D data shown in this paper can be obtained in digital format by following the links at $https://fusion.gat.com/global/D3D_DMP.$ Disclaimer: This report was prepared as an account of work sponsored by an agency of the United States Government. Neither the United States Government nor any agency thereof, nor any of their employees, makes any warranty, express or implied, or assumes any legal liability or responsibility for the accuracy, completeness, or usefulness of any information, apparatus, product, or process disclosed, or represents that its use would not infringe privately owned rights.