Malinowski Karol, Chernyshova Maryna, Jabłoński Sławomir, Czarski Tomasz, Wojeński Andrzej, Kasprowicz Grzegorz
Institute of Plasma Physics and Laser Microfusion, Hery 23, 01-497 Warsaw, Poland.
Institute of Electronic Systems, Warsaw University of Technology, Nowowiejska 15/19, 00-665 Warsaw, Poland.
Sensors (Basel). 2024 Aug 7;24(16):5113. doi: 10.3390/s24165113.
The objective of the proposed research is to develop plasma soft X-ray (SXR) radiation imaging that includes spectral information in addition to standard SXR tomography for the purpose of studying, for example, tungsten transport and its interplay with magnetohydrodynamics (MHD) in tokamak plasmas in an ITER-relevant approach. The SXR radiation provides valuable information about both aspects, particularly when measured with high spatial and temporal resolution and when tomographic reconstructions are performed. The spectral data will facilitate the tracking of both light and high-Z impurities. This approach is pertinent to both the advancement of a detailed understanding of physics and the real-time control of plasma, thereby preventing radiative collapses. The significance of this development lies in its ability to provide three-dimensional plasma tomography, a capability that extends beyond the scope of conventional tomography. The utilization of two-dimensional imaging capabilities inherent to Gas Electron Multiplier (GEM) detectors in a toroidal view, in conjunction with the conventional poloidal tomography, allows for the acquisition of three-dimensional information, which should facilitate the study of, for instance, the interplay between impurities and MHD activities. Furthermore, this provides a valuable opportunity to investigate the azimuthal asymmetry of tokamak plasmas, a topic that has rarely been researched. The insights gained from this research could prove invaluable in understanding other toroidal magnetically confined plasmas, such as stellarators, where comprehensive three-dimensional measurements are essential. To illustrate, by attempting to gain access to anisotropic radiation triggered by magnetic reconnection or massive gas injections, such diagnostics will provide the community with enhanced experimental tools to understand runaway electrons (energy distribution and spatial localization) and magnetic reconnection (spatial localization, speed…). This work forms part of the optimization studies of a detecting unit proposed for use in such a diagnostic system, based on GEM technology. The detector is currently under development with the objective of achieving the best spatial resolution feasible with this technology (down to approximately 100 µm). The diagnostic design focuses on the monitoring of photons within the 2-15 keV range. The findings of the optimization studies conducted on the amplification stage of the detector, particularly with regard to the geometrical configuration of the GEM foils, are presented herein. The impact of hole shape and spacing in the amplifying foils on the detector parameters, including the spatial size of the avalanches and the electron gain/multiplication, has been subjected to comprehensive numerical analysis through the utilization of Degrad (v. 3.13) and Garfield++ (v. bd8abc76) software. The results obtained led to the identification of two configurations as the most optimal geometrical configurations of the amplifying foil for the three-foil GEM system for the designed detector. The first configuration comprises cylindrical holes with a diameter of 70 μm, while the second configuration comprises biconical holes with diameters of 70/50/70 μm. Both configurations had a hole spacing of 120 μm.
拟开展的研究目标是开发等离子体软X射线(SXR)辐射成像技术,除了标准的SXR层析成像外,该技术还包括光谱信息,旨在以与国际热核聚变实验堆(ITER)相关的方法研究托卡马克等离子体中的钨输运及其与磁流体动力学(MHD)的相互作用。SXR辐射能提供有关这两个方面的宝贵信息,特别是在以高空间和时间分辨率进行测量以及进行层析重建时。光谱数据将有助于追踪轻杂质和高Z杂质。这种方法对于深入理解物理过程和等离子体的实时控制都具有重要意义,从而防止辐射坍缩。这一进展的意义在于其能够提供三维等离子体层析成像,这一能力超越了传统层析成像的范畴。利用环形视角下气体电子倍增器(GEM)探测器固有的二维成像能力,结合传统的极向层析成像,能够获取三维信息,这将有助于研究例如杂质与MHD活动之间的相互作用。此外,这为研究托卡马克等离子体的方位不对称性提供了宝贵机会,而该主题此前鲜有研究。从这项研究中获得的见解对于理解其他环形磁约束等离子体,如仿星器,可能具有极高价值,因为在仿星器中全面的三维测量至关重要。例如,通过尝试获取由磁重联或大量气体注入引发的各向异性辐射,此类诊断将为科学界提供更强大的实验工具,以理解逃逸电子(能量分布和空间定位)以及磁重联(空间定位、速度……)。这项工作是基于GEM技术为这种诊断系统设计的检测单元优化研究的一部分。目前正在开发该探测器,目标是实现该技术可行的最佳空间分辨率(低至约100μm)。诊断设计聚焦于监测2 - 15keV范围内的光子。本文展示了在探测器放大阶段进行的优化研究结果,特别是关于GEM箔片的几何构型。通过使用Degrad(v. 3.13)和Garfield++(v. bd8abc76)软件,对放大箔片中孔的形状和间距对探测器参数(包括雪崩的空间尺寸和电子增益/倍增)的影响进行了全面的数值分析。所得结果确定了两种构型为所设计探测器的三箔GEM系统放大箔片的最优几何构型。第一种构型包括直径为70μm的圆柱形孔,而第二种构型包括直径为70/50/70μm的双锥形孔。两种构型的孔间距均为120μm。