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arXiv 2012.12213physics.plasm-ph
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准对称仿星器中无碰撞纬向流阻尼的局部与全局回旋动理学计算比较

Comparison of local and global gyrokinetic calculations of collisionless zonal flow damping in quasi-symmetric stellarators

J. Smoniewski, E. Sánchez, I. Calvo, M. J. Pueschel, J. N. Talmadge

AI总结:

本文在准对称仿星器中比较了磁通管、磁通面和全体积三种几何下的纬向流无碰撞阻尼计算,揭示了局部计算在中等径向波数下可准确再现全体积残余,但小径向波数时振荡与阻尼时间尺度偏长。

摘要:

针对准对称仿星器平衡,分别在磁通管、磁通面和全体积几何中计算了纬向流的线性无碰撞阻尼。所研究的平衡包括螺旋对称实验装置(HSX)的准螺旋对称位形、HSX 的破缺对称位形,以及国家紧凑仿星器实验装置(NCSX)的准轴对称几何。纬向流振荡和长时间阻尼会影响纬向流演化,且当径向波数较小时,纬向流残余趋于零。振荡频率和阻尼率与反弹平均径向粒子漂移的关系符合理论预期。尽管磁通面上的每个磁通管都是独特的,但在 HSX 或 NCSX 中,只要具有足够的平行延伸长度,若干个不同的磁通管就能再现磁通面计算得到的纬向流阻尼。对于中等大小的 $k_x$,磁通面或磁通管计算能够准确再现全体积长时间残余,但在局部表示中振荡和阻尼时间尺度更长,尤其是当 $k_x$ 较小并接近系统尺寸时。

英文摘要:

The linear collisionless damping of zonal flows is calculated for quasi-symmetric stellarator equilibria in flux-tube, flux-surface, and full-volume geometry. Equilibria are studied from the quasi-helical symmetry configuration of the Helically Symmetric eXperiment (HSX), a broken symmetry configuration of HSX, and the quasi-axial symmetry geometry of the National Compact Stellarator eXperiment (NCSX). Zonal flow oscillations and long-time damping affect the zonal flow evolution, and the zonal flow residual goes to zero for small radial wavenumber. The oscillation frequency and damping rate depend on the bounce-averaged radial particle drift in accordance with theory. While each flux tube on a flux surface is unique, several different flux tubes in HSX or NCSX can reproduce the zonal flow damping from a flux-surface calculation given an adequate parallel extent. The flux-surface or flux-tube calculations can accurately reproduce the full-volume long-time residual for moderate $k_x$, but the oscillation and damping time scales are longer in local representations, particularly for small $k_x$ approaching the system size.

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