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Nuclear challenges and progress in designing stellarator fusion power plants

Over the past 5–6 decades, stellarator power plants have been studied in the US, Europe, and Japan as an alternate to the mainline magnetic fusion tokamaks, offering steady-state operation and eliminating the risk of plasma disruptions. The earlier 1980s studies suggested large-scale stellarator pow...

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Bibliographic Details
Published in:Energy conversion and management 2008-07, Vol.49 (7), p.1859-1867
Main Authors: El-Guebaly, L.A., Wilson, P., Henderson, D., Sawan, M., Sviatoslavsky, G., Tautges, T., Slaybaugh, R., Kiedrowski, B., Ibrahim, A.
Format: Article
Language:English
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Summary:Over the past 5–6 decades, stellarator power plants have been studied in the US, Europe, and Japan as an alternate to the mainline magnetic fusion tokamaks, offering steady-state operation and eliminating the risk of plasma disruptions. The earlier 1980s studies suggested large-scale stellarator power plants with an average major radius exceeding 20 m. The most recent development of the compact stellarator concept delivered ARIES-CS – a compact stellarator with 7.75 m average major radius, approaching that of tokamaks. For stellarators, the most important engineering parameter that determines the machine size and cost is the minimum distance between the plasma boundary and mid-coil. Accommodating the breeding blanket and necessary shield within this distance to protect the ARIES-CS superconducting magnet represents a challenging task. Selecting the ARIES-CS nuclear and engineering parameters to produce an economic optimum, modeling the complex geometry for 3D nuclear analysis to confirm the key parameters, and minimizing the radwaste stream received considerable attention during the design process. These engineering design elements combined with advanced physics helped enable the compact stellarator to be a viable concept. This paper provides a brief historical overview of the progress in designing stellarator power plants and a perspective on the successful integration of the nuclear activity into the final ARIES-CS configuration.
ISSN:0196-8904
1879-2227
DOI:10.1016/j.enconman.2007.09.032