Turbulence-reduced high-performance scenarios in Wendelstein 7-X

O. Ford, M. Beurskens, S. Bozhenkov, S. Lazerson, Lilla Vano, Arturo Alonso, J. Baldzuhn, C. Beidler, Christoph Biedermann, R. Burhenn, Golo Fuchert, D. Hartmann, Matthias Hirsch, A. Langenberg, Heinrich Laqua, P. McNeely, N. Pablant, E. Pasch, Felix Reimold, T. Romba, N. Rust, Ralf Schroeder, Evan Scott, Torsten Stange, Hakan M Smith, D. Gradic, R. C. Wolf, Daihong Zhang
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引用次数: 2

Abstract

In the Wendelstein 7-X (W7-X) stellarator, turbulence is the dominant transport mechanism in most discharges. This leads to a 'clamping' of ion temperature over a wide range of heating power, predominantly flat density profiles where hollow profiles driven by neoclassical thermo-diffusion would be expected and by rapid impurity transport in injection experiments. Significantly reduced turbulent transport is observed in the presence of strong core density gradients found transiently after core pellet injection and irregularly after boronisation or boron pellet injection. Density peaking is also achieved in a controlled manner in purely neutral beam heated discharges where particle transport analysis reveals an abrupt reduction in the main-ion particle flux leading to significant density profile peaking not explained by the NBI particle source alone. The plasmas exhibit a heat diffusivity of around chi=0.25±0.1 m^2 s^-1 at mid radius, a factor of around 4 lower than ECRH dominated discharges. Despite the improved confinement, the achieved ion temperature is limited by broader heat deposition and the lower power-per-particle given the higher density. This is overcome with limited reintroduction of ECRH power, where the low heat diffusivity diffusivity is maintained, the density rise supressed and ion temperatures above the clamping limit are achieved. The applicability of these plasmas for a high performance scenario on transport relevant time scales is assessed, including initial predictions for planned heating upgrades of W7-X, based on a range of assumptions about particle transport.
文德尔施泰因 7-X 中减少湍流的高性能方案
在温德斯坦 7-X (W7-X) 恒星器中,湍流是大多数放电的主要传输机制。这导致离子温度在很宽的加热功率范围内受到 "钳制",在新古典热扩散和注入实验中的快速杂质传输所驱动的空心剖面中,主要是平坦的密度剖面。在堆芯颗粒注入后瞬时出现的强堆芯密度梯度以及硼化或硼颗粒注入后的不规则密度梯度中,观察到湍流输运显著减少。在纯中性束加热的放电中,密度峰值也是以受控方式实现的,粒子输运分析表明,主离子粒子通量的突然减少导致了显著的密度剖面峰值,而这不能仅用 NBI 粒子源来解释。等离子体在中半径处的热扩散率约为 chi=0.25±0.1 m^2 s^-1,比 ECRH 主导的放电低约 4 倍。尽管封闭性有所改善,但由于热沉积较广,而且密度较高,单粒子功率较低,因此达到的离子温度受到了限制。有限度地重新引入 ECRH 功率可以克服这一问题,从而保持低热扩散系数、抑制密度上升并达到高于箝位极限的离子温度。根据对粒子传输的一系列假设,评估了这些等离子体在传输相关时间尺度上对高性能方案的适用性,包括对 W7-X 计划加热升级的初步预测。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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