紧凑型仿星器反应堆中热粒子和α粒子的分流热负荷

T. Mau, T. Kaiser, J. Lyon, R. Maingi, A. Raffray, X. Wang, L. Ku, M. Zarnstorff
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摘要

在基于ncsx的紧凑型仿星器反应堆中,对热粒子和α粒子引起的转向器热负荷分布进行了评估。设想了一个分流板系统,每个场周期有4个板,覆盖等离子体表面积的7%。采用场线跟踪技术;对于热通量,采用传统的方法,而对于阿尔法,它们从等离子体和随后的陀螺轨道的特征出口模式是近似的。对于ARIES-CS参考设计点(R=7.75 m, A=4.5, B=5.7 T, beta=6.4%, Pnet=1000 MW),在假设核心和边缘的辐射分数为75%,α损失分数为5%的情况下,获得了板上5 -18 MW/m2范围内的综合峰值热负荷。热通量可能是一个主要的决定因素。进一步的优化研究是有必要的,以降低所有的峰值热负荷,以满足小于10兆瓦/平方米的可接受极限。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Divertor Heat Loads from Thermal and Alpha Particles in a Compact Stellarator Reactor
Divertor heat load distributions due to thermal and alpha particles have been assessed in an NCSX-based compact stellarator reactor. A divertor plate system is envisaged, with 4 plates per field period and covering 7% of the plasma surface area. The field-line tracing technique is employed; for thermal flux, the conventional approach is used, while for alphas, their characteristic exit pattern from the plasma and subsequent gyro- orbits are approximated. For the ARIES-CS reference design point (R=7.75 m, A=4.5, B=5.7 T, beta=6.4% and Pnet=1000 MW), combined peak heat loads in the 5 -18 MW/m2 range on the plates have been obtained, assuming a 75% radiation fraction both in the core and at the edge, and a 5% alpha loss fraction. The alpha heat flux could be a dominant determining factor. Further optimization study is warranted to lower all peak heat loads to satisfy the accepted limit of les10 MW/m2.
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