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

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stand the relative roles of long-to-intermediate wavelength versus short wavelength turbulence<br />

in causing electron transport. Given the very high plasma energy confinement potentially needed<br />

<strong>for</strong> the st-ctF application, very low recycling regimes should be tested on present and near-term<br />

experiments to assess predictions of improved confinement at the reduced toroidal magnetic field<br />

and high-b of the st.<br />

increased nbi current drive efficiency and control is needed to test fully noninductive operation<br />

of an st as needed <strong>for</strong> an st-ctF. Reduced collisionality, increased nbi heating power, and injection<br />

geometries more favorable <strong>for</strong> nbi current drive and current profile control are needed<br />

to assess the predicted nbi current drive capabilities. These additional capabilities are especially<br />

important <strong>for</strong> testing ramp-up of the plasma current that is assumed to be achieved using nbi<br />

heating and current drive in an st-ctF. st operating scenarios could have a substantial population<br />

of super-alfvénic ions and associated energetic particle instabilities. since these instabilities<br />

can result in fast ion transport — which is not presently well understood — improved diagnosis<br />

and theory and computation of fast ion redistribution by alfvénic activity is needed <strong>for</strong> reliably<br />

projecting the per<strong>for</strong>mance of future sts. sufficient plasma duration (~10 1 to 10 2 s) is required to<br />

achieve full plasma current profile relaxation following plasma ramp-up and during the sustainment<br />

phase, and to demonstrate profile controllability.<br />

exhaust solutions <strong>for</strong> high-particle flux and ctF-relevant high-heat flux must also be developed<br />

and assessed <strong>for</strong> compatibility with a sustained, fully noninductive, integrated high-per<strong>for</strong>mance<br />

core plasma. such solutions might include liquid metal plasma facing components and/or high<br />

flux expansion and increased scrape-off layer magnetic field line-length as embodied in the X and<br />

super-X divertor configurations. The above core and edge plasma integration must ultimately be<br />

achieved using the first-wall materials and operating conditions expected in an st-ctF and/or<br />

reactor to ensure that acceptably low tritium retention can be achieved and that the first wall can<br />

tolerate infrequent off-normal events such as elms and disruptions.<br />

Finally, new computational and theoretical capabilities supporting comprehensive time-dependent<br />

integrated modeling of the plasma evolution, using reduced models <strong>for</strong> core and edge transport<br />

and stability, are needed to develop and understand st integrated scenarios, and to reliably<br />

project to the per<strong>for</strong>mance needed <strong>for</strong> an st-ctF and beyond.<br />

St available Means <strong>for</strong> <strong>Research</strong> and actions to address <strong>Research</strong> needs<br />

Present Us and large international st research facilities include (in order of decreasing plasma<br />

current capability) the nstX (1 ma), PeGasUs, and ltX in the Us, mast (1 ma) in the U.k., and<br />

QUest in Japan. many smaller devices are operating internationally (see Fesac taP report <strong>for</strong><br />

greater detail). Proposed upgrades <strong>for</strong> these devices that have gone through initial review include<br />

nstX-U and mast-U (both 2 ma). These upgrades are critical to pursuing the iteR-era st goal,<br />

but they and further upgrades may not be sufficient to fulfill this goal. defining additional steps<br />

to resolve the st physics issues described above and advance to an st-ctF is evolving through<br />

the ReneW process and beyond. The fusion nuclear science and technology actions <strong>for</strong> a ctF are<br />

addressed in Thrust 13.<br />

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