论文标题
DIII-D与C-MOD模拟与XGC1之间的边缘湍流特性的比较
Comparison of edge turbulence characteristics between DIII-D and C-Mod simulations with XGC1
论文作者
论文摘要
在边缘区域进行的物理过程对于托卡马克人的运行至关重要,因为它们控制着热等离子体与容器壁的相互作用。具有最新代码的边缘的数值建模试图阐明控制SOL区域物理设置的新古典漂移,湍流,多构和平行流之间的相互作用。在这里,我们介绍了来自陀螺仪代码XGC1的模拟的后处理分析,将DIII-D模拟的边缘湍流特性与C-MOD之一进行了比较。我们发现,分离质的平衡$ e \ times b $通量在两种放电中都具有相似的螺状模式,可以通过磁漂移和捕获的离子偏移来解释。但是,碰撞性发挥了主要作用,因为它可以防止本地指控积累在C模型中产生全球影响。在这两种情况下,湍流的电子热通量都高于离子。这似乎是Tokamak Edge的普遍特征。我们在两个模拟中确定了主要模式的湍流频率和增长率。在C模型中,这些数字指向漂移波的存在。在DIII-D中,具有基因的线性模拟揭示了被困的电子模式。此外,我们介绍了两个模拟的斑点的幅度和大小分布。振幅分布与实验观察符合定性一致,而大小分布与大多数斑点没有连接到分流板的事实是一致的,并建议它们是通过湍流模式的剪切而产生的。
The physical processes taking place at the edge region are crucial for the operation of tokamaks as they govern the interaction of hot plasma with the vessel walls. Numerical modeling of the edge with state-of-the-art codes attempts to elucidate interactions between neoclassical drifts, turbulence, poloidal and parallel flows that control the physical set-up of the SOL region. Here, we present post-processing analysis of simulations from the gyrokinetic code XGC1, comparing edge turbulence characteristics from a simulation of DIII-D against one of C-Mod. We find that the equilibrium $E \times B$ flux across the separatrix has a similar poloidal pattern in both discharges which can be explained by magnetic drifts and trapped ion excursions. However, collisionality is noted to play a major role in that it prevents local charge accumulations from having global effects in C-Mod. In both cases, turbulent electron heat flux is higher than the ion one. This seems to be a universal characteristic of the tokamak edge. We identify turbulent frequencies and growth rates of the dominant mode in both simulations. In C-Mod, these numbers point to the presence of a drift wave. In DIII-D, linear simulations with Gene reveal a trapped electron mode. Furthermore, we present the amplitude and size distributions of the blobs from both simulations. Amplitude distributions are in qualitative agreement with experimental observations while size distributions are consistent with the fact that most blobs are not connecting to the divertor plates and suggest that they are generated by the shearing of the turbulent modes.