TJ-II 恒星器中的扫频阿尔芬模式建模

Adriana Gabrielle Ghiozzi, Mervi Mantsinen, Pol Pastells, D. Spong, A. Melnikov, Leonid E Eliseev, S. Sharapov
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摘要

在 TJ-II 恒星器中观测到了阿尔弗涅活动,它类似于托卡马克中阿尔弗涅级联模式所显示的频率扫描。使用简化的磁流体动力(MHD)模型进行了数值验证研究,结果表明只有在旋转变换曲线非单调的放电中才能观测到这种模式。在实验过程中,线圈电流的变化会导致旋转变换曲线最小值的移动。为了模拟这种效应,我们研究了简化 MHD 模型预测的阿尔费尼科活动,该模型适用于一组具有不同最小值的输入旋转变换剖面。我们发现了一种模式,其环形和极环形模式数与实验中预测的相吻合,随着旋转变换剖面最小值的增大/减小,该模式的频率会向下/向上扫描。这些结果证明了磁流体动力学光谱学的有效性和实用性。
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Modeling of frequency-sweeping Alfvén modes in the TJ-II stellarator
Alfvénic activity has been observed in the TJ-II stellarator which resembles the frequency sweeping demonstrated by Alfvén cascade modes in tokamaks. A numerical validation study was conducted using a reduced magnetohydrodynamic (MHD) model to show that such modes could only have been observed in discharges where the rotational transform profile was non-monotonic. During experiments, coil current was varied which resulted in shifting of the minimum value of the rotational transform profile. To mimic this effect, we study the Alfvénic activity predicted by the reduced MHD model for a set of input rotational transform profiles with varying minima. A mode is found whose toroidal and poloidal mode numbers match those predicted in experiments which sweeps downward/upward in frequency as the minimum value of the rotational transform profile is increased/decreased. The results serve as a demonstration of the validity and utility of magnetohydrodynamic spectroscopy.
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