大型等离子体装置中镜面几何形状的湍流和传输

Phil Travis, Troy Carter
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摘要

由于等离子体科学和使能技术的进步,人们正在重新考虑将镜像设备用于核聚变发电厂,并将其作为可能的核聚变体积中子源。利用大型等离子体装置(LAPD)的灵活磁性几何结构,研究了镜像配置中的湍流和传输问题。研究了从 $ M = 1 $ 到 $ M = 2.68 $ 的多个镜像比和从 $L = 3.51 $m 到 $L = 10.86 $m 的三个镜像单元长度。使用朗缪尔探针和磁探针测量了密度、温度、电势和磁场曲线。波动驱动的 $ \tilde{ E } \times B $ 粒子通量\times B $粒子通量是根据这些数据计算出来的。两种探针相关技术被用来推断波数和二维结构。跨场粒子通量和密度波动功率随着镜像比的增加而减小。核心密度和温度与镜像比保持相似,但径向线积分密度有所增加。通过在源区使用更高的磁场,镜室中的等离子体发生了物理膨胀,这可能导致密度波动功率因梯度尺度长度的增加而降低。尺度长度的增加降低了旋转交换和漂移类不稳定性的增长速度和饱和水平。尽管引入了磁曲率,但没有观察到镜像驱动的不稳定性--交换、速度空间或其他。对于曲率引起的互换,存在许多可能的稳定机制,抑制了不稳定性的可见性。
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Turbulence and transport in mirror geometries in the Large Plasma Device
Thanks to advances in plasma science and enabling technology, mirror machines are being reconsidered for fusion power plants and as possible fusion volumetric neutron sources. However cross-field transport and turbulence in mirrors remains relatively understudied compared to toroidal devices. Turbulence and transport in mirror configurations were studied utilizing the flexible magnetic geometry of the Large Plasma Device (LAPD). Multiple mirror ratios from $ M = 1 $ to $ M = 2.68 $ and three mirror-cell lengths from $L = 3.51 $m to $ L = 10.86 $m were examined. Langmuir and magnetic probes were used to measure profiles of density, temperature, potential, and magnetic field. The fluctuation-driven $ \tilde{ E } \times B $ particle flux was calculated from these quantities. Two probe correlation techniques were used to infer wavenumbers and two-dimensional structure. Cross-field particle flux and density fluctuation power decreased with increased mirror ratio. Core density and temperatures remain similar with mirror ratio, but radial line-integrated density increased. The physical expansion of the plasma in the mirror cell by using a higher field in the source region may have led to reduced density fluctuation power through the increased gradient scale length. This increased scale length reduced the growth rate and saturation level of rotational interchange and drift-like instabilities. Despite the introduction of magnetic curvature, no evidence of mirror driven instabilities -- interchange, velocity space, or otherwise -- were observed. For curvature-induced interchange, many possible stabilization mechanisms were present, suppressing the visibility of the instability.
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