02.08.2013 Views

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

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

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

SHOW MORE
SHOW LESS

You also want an ePaper? Increase the reach of your titles

YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.

ment, but also micro- and macro-instabilities – that is, turbulent transport and global stability.<br />

The different approaches might also vary in optimal aspect ratio, how they simplify the coil structures,<br />

or how they approach a 3-d divertor design.<br />

The promise of stellarators is well recognized within the fusion community. stellarator research<br />

is a mature field with many experiments worldwide including large per<strong>for</strong>mance extension facilities.<br />

Recommendation 4 in the Fesac “Priorities, Gaps, and opportunities” report (PGo) urges<br />

consideration of a major initiative (i-5) <strong>for</strong> an “advanced experiment in disruption-free concepts,”<br />

of which the stellarator would be the most likely facility. The Fesac taP report states: “There is<br />

little doubt that a stellarator configuration can confine plasma at the parameters necessary <strong>for</strong><br />

fusion burn” and that stellarator research “is likely to contribute significantly to the optimization<br />

of tokamaks and perhaps to other confinement concepts.” This motivated the stellarator iteR-era<br />

goal reported by the taP:<br />

Develop and validate the scientific understanding necessary to assess the feasibility of a burning plasma<br />

experiment based on the quasi-symmetric (QS) stellarator.<br />

a critical gap exists in the worldwide stellarator program in that there are no moderate scale experiments<br />

investigating quasi-symmetry. There is an immediate need to explore quasi-symmetry<br />

with sufficient breadth and scale to achieve the iteR-era goal.<br />

Scientific issues and <strong>Research</strong> Requirements<br />

intEgRatED HigH PERFORManCE OF QuaSi-SyMMEtRiC OPtiMizED<br />

StELLaRatORS<br />

There is a need to study a plasma in a quasi-symmetric stellarator that has both high plasma pressure<br />

and low ion collisionality. such a test of quasi-axisymmetry was to be per<strong>for</strong>med on the national<br />

compact stellarator experiment (ncsX), which was under construction until 2008. its cancellation<br />

has left a gap in the worldwide program of exploring the science of quasi-symmetry and the<br />

potential of the concept. as described earlier, quasi-symmetric stellarators may differ in how they<br />

approach neoclassical and turbulent transport as well as macrostability. There<strong>for</strong>e, there is a need<br />

<strong>for</strong> multiple quasi-symmetric configurations to assess high-beta, low collisionality, t i ~ t e plasmas<br />

with good confinement. because of the centrality of the issue of disruption control, one approach is<br />

to differentiate the experiments based on the amount of bootstrap current present <strong>for</strong> a given set of<br />

plasma parameters. The configurations will differ in other attributes such as divertors or impurity<br />

control. based on the results of the multiple experiments, theory and modeling, in<strong>for</strong>mation gained<br />

from the international stellarator program, a per<strong>for</strong>mance extension (Pe) level quasi-symmetric<br />

stellarator that extrapolates to burning plasma per<strong>for</strong>mance would be designed and constructed.<br />

research requirements<br />

The multiple quasi-symmetric stellarators would have a common set of research requirements.<br />

These requirements serve as definitions of “integrated high per<strong>for</strong>mance.” implicit within these<br />

requirements is sufficient operational flexibility of the magnetic geometry and plasma parameters<br />

to test theory and modeling predictions.<br />

178

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!