论文标题
恒星湍流中的陀螺仪模拟中血浆动力学的统计分析方法
A statistical analysis approach of plasma dynamics in gyrokinetic simulations of stellarator turbulence
论文作者
论文摘要
几何方法用于分析血浆湍流中的随机过程。热力学状态之间的距离可以根据热力学长度方法来计算,该方法允许在相空间上使用riemannian度量。几何方法是适当的,以了解参与例如订单disorder跃迁,预计距离会突然增加。考虑到恒星W7-X的核心区域中的离子 - 温度梯度(ITG)模式驱动的湍流,具有逼真的准静脉拓扑结构。在陀螺仪等离子体湍流模拟中,雪崩,例如经常发现热量和颗粒,在这项工作中,研究了一种新的检测方法。这种新方法结合了奇异频谱分析算法和层次聚类,从而将陀螺仪仿真时间序列分解为有用的物理信息和噪声的一部分。时间序列的信息组成部分用于计算赫斯特指数,信息长度和动态时间。基于这些度量,揭示了时间序列的物理特性。
A geometrical method is used for the analysis of stochastic processes in plasma turbulence. Distances between thermodynamic states can be computed according the thermodynamic length methodology which allows the use of a Riemannian metric on the phase space. A geometric methodology is suitable in order to understand stochastic processes involved in e.g. order-disorder transition, where a sudden increase in distance is expected. Gyrokinetic simulations of Ion-Temperature-Gradient (ITG) mode driven turbulence in the core-region of the stellarator W7-X, with realistic quasi-isodynamic topologies are considered. In gyrokinetic plasma turbulence simulations avalanches, e.g. of heat and particles, are often found and in this work a novel method for detection is investigated. This new method combines the Singular Spectrum Analysis algorithm and Hierarchical Clustering such that the gyrokinetic simulation time series is decomposed into a part of useful physical information and noise. The informative component of the time series is used for the calculation of the Hurst exponent, the Information Length and the Dynamic Time. Based on these measures the physical properties of the time series is revealed.