等离子体平衡的测试粒子计算

Jonathan Sullivan-Wood, D. Holland
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引用次数: 0

摘要

我们提出了一种自洽计算等离子体平衡的数值技术,在边界上有规定的源和汇,即散射系统。将该方法应用于地球磁尾。该方法在规定的磁场中跟踪单个粒子,同时计算粒子对均匀间隔网格的密度、电流和压力。对单个粒子进行加权以模拟给定的源分布,并评估包括产生的磁场在内的总平衡特性。然后将计算的磁场与规定的磁场进行比较。如果字段差异很大,则将两个字段混合并重复该过程。收敛到自一致域通常需要100到150次迭代。
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Test Particle Calculation of Plasma Equilibria
We present a numerical technique for self-consistently calculating plasma equilibria with prescribed sources and sinks on the boundaries, i.e. a scattering system. The method is applied to the earth’s magnetotail. The method follows individual particles through a prescribed magnetic field, while calculating the density, current and pressure that the particle contributes on a uniformly spaced grid. The individual particles are weighted to model a given source distribution and the total equilibrium properties, including the resulting magnetic field, are evaluated. The calculated and prescribed magnetic fields are then compared. If the fields differ significantly, the two fields are mixed and the process repeated. Convergence to the self-consistent field typically takes between 100 and 150 iterations.
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