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Research Needs for Magnetic Fusion Energy Sciences - US Burning ...

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influence on plasma per<strong>for</strong>mance, and an improved understanding of this area will be necessary<br />

to optimize the configuration. The current profile and the transport of particles and energy are<br />

strongly coupled, particularly when the current and heating source are dominantly from the plasma<br />

itself. The longest time scale <strong>for</strong> core plasma physics is the current profile redistribution time<br />

(t J ). The transport of the energetic alpha-particles and impurities (intentional and unintentional)<br />

must be understood to control the distribution of power onto the various material surfaces in the<br />

tokamak. all of these issues contribute to the critical need <strong>for</strong> experimental demonstrations of a<br />

high-per<strong>for</strong>mance plasma core with the many simultaneous processes associated with a burning<br />

plasma as it approaches the self-organized regime.<br />

Magnetohydrodynamic stability<br />

The magnetohydrodynamic (MHD) stability properties of a high-per<strong>for</strong>mance core plasma will determine<br />

the maximum fusion power density achievable. The understanding of stabilizing a plasma above the nowall<br />

beta limit, as a function of the plasma rotation, background error fields, and feedback control, is<br />

critical to accessing the highest possible per<strong>for</strong>mance. In the burning plasma state with low rotation,<br />

fast alpha particles, and strong pedestals, what maximum stability properties will<br />

the plasma access?<br />

experimental results indicate that in the presence of a conducting wall, even slow plasma rotation<br />

– less than 0.5% of the alfvén wave velocity – is sufficient to maintain plasma stability up to b n<br />

(normalized plasma pressure) values close to the maximum with-wall limit. although this is encouraging<br />

<strong>for</strong> future large devices where the plasma rotation is expected to be small, a reliable extrapolation<br />

to demo requires a deeper understanding of the stabilization physics. it is expected<br />

that the remaining error fields in the plasma are affecting the stability threshold. although projections<br />

to high fusion power plasmas consider feedback control as the sole stabilization method, it<br />

should be recognized that sustained, direct feedback-stabilization without the stabilizing effect of<br />

rotation or fast particles has not been demonstrated yet in a high-beta tokamak. The range of plasma<br />

betas, in the demo regime, is between the value requiring no conducting wall (b n no wall ) and<br />

that requiring a conducting wall (b n with wall ). on a time scale longer than a resistive time, feedback<br />

is complicated by the nonideal response of the plasma. The benefits of operating above the no-wall<br />

beta limit are clear, and reliable stabilization methods to access this regime are necessary.<br />

The self-heating of the plasma comes from the 3.5 mev alpha particles slowing down and heating<br />

the ions and electrons. Fast ions can drive instabilities, causing enhanced transport of the energetic<br />

particles necessary <strong>for</strong> heating, and possibly damaging the first wall through losses from the<br />

plasma. These fast particles can play an important role in the global stability of the plasma, contributing<br />

to the access to high beta.<br />

The region near the plasma edge, featuring a transport barrier referred to as the pedestal, strongly<br />

determines the core plasma properties. high pressure at the top of the pedestal can support<br />

high overall per<strong>for</strong>mance in a fusion plasma. The magnitude of this pressure is a key parameter<br />

requiring more accurate prediction <strong>for</strong> demo. a key additional issue <strong>for</strong> the pedestal is that its<br />

density and temperature must be consistent with the high-per<strong>for</strong>mance core plasma, fueling, and<br />

the divertor where particles and power are received.<br />

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