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首页> 外文期刊>Plasma physics and controlled fusion >Edge turbulence effect on ultra-fast swept reflectometry core measurements in tokamak plasmas
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Edge turbulence effect on ultra-fast swept reflectometry core measurements in tokamak plasmas

机译:对托卡马克等离子体超快速扫描反射芯测量的边缘湍流效应

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Ultra-fast frequency-swept reflectometry (UFSR) enables one to provide information about the turbulence radial wave-number spectrum and perturbation amplitude with good spatial and temporal resolutions. However, a data interpretation of USFR is quiet tricky. An iterative algorithm to solve this inverse problem was used in past works, Gerbaud (2006 Rev. Sci. Instrum. 77 10E928). For a direct solution, a fast 1D Helmholtz solver was used. Two-dimensional effects are strong and should be taken into account during data interpretation. As 2D full-wave codes are still too time consuming for systematic application, fast 2D approaches based on the Born approximation are of prime interest. Such methods gives good results in the case of small turbulence levels. However in tokamak plasmas, edge turbulence is usually very strong and can distort and broaden the probing beam Sysoeva et al (2015 Nucl. Fusion 55 033016). It was shown that this can change reflectometer phase response from the plasma core. Comparison between 2D full wave computation and the simplified Born approximation was done. The approximated method can provide a right spectral shape, but it is unable to describe a change of the spectral amplitude with an edge turbulence level. Computation for the O-mode wave with the linear density profile in the slab geometry and for realistic Tore-Supra density profile, based on the experimental data turbulence amplitude and spectrum, were performed to investigate the role of strong edge turbulence. It is shown that the spectral peak in the signal amplitude variation spectrum which rises with edge turbulence can be a signature of strong edge turbulence. Moreover, computations for misaligned receiving and emitting antennas were performed. It was found that the signal amplitude variation peak changes its position with a receiving antenna poloidal displacement.
机译:超快速频率扫描反射仪(UFSR)使得能够提供有关湍流径向波数频谱和具有良好空间和时间分辨率的扰动幅度的信息。然而,USFR的数据解释是安静的棘手。解决这个逆问题的迭代算法在过去的作品中使用了Gerbaud(2006年版SCI。仪器。77 10E928)。对于直接解决方案,使用快速1D Helmholtz求解器。二维效应强劲,在数据解释过程中应考虑到。由于2D全波代码仍然太耗了系统应用,基于出生的近似的快速2D方法是主要的兴趣。这种方法在小湍流水平的情况下提供良好的结果。然而,在托卡马克等离离子体中,边缘湍流通常非常强烈,并且可以扭曲和拓宽探头梁Sysoeva等(2015 Nucl。融合55 033016)。结果表明,这可以改变来自等离子体芯的反射计相位响应。 2D完全波计算与简化出生近似之间的比较。近似方法可以提供右谱形状,但是它不能描述具有边缘湍流电平的光谱幅度的变化。基于实验数据湍流幅度和光谱,进行平板几何形状和逼真的TORE-SUPRA密度分布的具有线浓度曲线的O模式波的计算,以研究强边湍流的作用。结果表明,信号幅度变化光谱中的光谱峰值,其上升的边缘湍流可以是强边湍流的特征。此外,执行用于未对准接收和发射天线的计算。发现信号幅度变化峰值改变其与接收天线面块位移的位置。

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