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Type-Ⅰ ELM precursor modes in JET

机译:JET中的I型ELM前体模式

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Clear low frequency (typically 5-25 kHz) coherent type-Ⅰ ELM precursor modes have been identified in JET. They are detected through various diagnostics, especially in the ECE and Mirnov signals, but also on the SXR cameras and the multichannel O-mode edge reflectometer. The modes propagate in the direction of the ion-diatnagnetic drift and are usually accompanied by a slight rise in the divertor D_α-emission. The precursors show no radial phase inversions and are localized to a few centimetres inside the separatrix, in the pedestal region. The time by which the precursor onset precedes the ELM event varies greatly, and ranges from 0.2 ms up to several tens of milliseconds, though the timescale has no effect on the characteristics of the precursors. During their lifetime, the precursor amplitude is often seen to fluctuate, and the frequency and dominant n -number of the precursors can change rapidly, typically within 1 ms. The range of toroidal precursor mode numbers n which have been observed is 1-13. Parametric studies show that n seems to be mainly prescribed by a combination of the electron pedestal pressure and the (normalized) electron pedestal collisionality ν_e~*, with increasing ν_e~* leading to higher n-numbers. Above a certain edge collisionality (roughly ν_e~* > 1-3) the precursors seem to be absent, indicating that a sufficiently high edge current is important to destabilize the precursors. The low-n precursors are known to be external kinks (also known on JET as Outer Modes), while experimental findings and their comparison with stability calculations suggest that the precursor modes with higher n are not pure external kinks but coupled ballooning-kink modes. Several hundred discharges have been analysed, and, in discharges with low to moderate edge collisionality, the precursors could be detected prior to most type-Ⅰ ELMs, while prior to type-Ⅲ ELMs the modes were not encountered. In spite of their regular occurrence, there is no evidence of the precursor mode growth rate rapidly accelerating before the ELM, indicating that type-Ⅰ ELMs on JET are not triggered by these modes.
机译:在JET中已经确定了清晰的低频(通常为5-25 kHz)相干的Ⅰ型ELM前体模式。通过各种诊断可以检测到它们,尤其是在ECE和Mirnov信号中,在SXR摄像机和多通道O模式边缘反射仪上也可以检测到。这些模式沿离子-菱形漂移的方向传播,通常伴随着发散角D_α发射的轻微上升。前体未显示出径向相变,并且位于基座区域中的分离线内部几厘米处。前驱物发生在ELM事件之前的时间变化很大,范围从0.2毫秒到数十毫秒,尽管时间尺度对前驱物的特性没有影响。在它们的寿命期间,通常可以看到前体振幅波动,并且前体的频率和主要n值可以快速变化,通常在1 ms内。观察到的环形前体模数n的范围是1-13。参数研究表明,n似乎主要由电子基座压力和(规范化的)电子基座碰撞性ν_e〜*的组合规定,随着ν_e〜*的增加,n值越高。在一定的边缘碰撞性之上(大约ν_e〜*> 1-3),似乎没有前体,这表明足够高的边缘电流对于稳定前体很重要。低n前体已知是外部纽结(在JET上也称为外部模式),而实验结果及其与稳定性计算的比较表明,具有较高n的前体模式不是纯外部纽结,而是耦合的膨胀-纽结模式。已经分析了数百次放电,并且在低至中等边缘碰撞性的放电中,可以在大多数Ⅰ型ELM之前检测到前体,而在Ⅲ型ELM之前则没有遇到这种模式。尽管它们定期发生,但没有证据表明前体模式增长率在ELM之前迅速加速,这表明JET上的Ⅰ型ELM不受这些模式触发。

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