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Validating modeling assumptions of alpha particles in electrostatic turbulence

机译:验证静电湍流中α粒子的建模假设

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To rigorously model fast ions in fusion plasmas, a non-Maxwellian equilibrium distribution must be used. In this work, the response of high-energy alpha particles to electrostatic turbulence has been analyzed for several different tokamak parameters. Our results are consistent with known scalings and experimental evidence that alpha particles are generally well confined: on the order of several seconds. It is also confirmed that the effect of alphas on the turbulence is negligible at realistically low concentrations, consistent with linear theory. It is demonstrated that the usual practice of using a high-temperature Maxwellian, while previously shown to give an adequate order-of-magnitude estimate of the diffusion coefficient, gives incorrect estimates for the radial alpha particle flux, and a method of correcting it in general is provided. Furthermore, we see that the timescales associated with collisions and transport compete at moderate energies, calling into question the assumption that alpha particles remain confined to a flux surface that is used in the derivation of the slowing-down distribution.
机译:要严格模拟聚变等离子体中的快速离子,必须使用非麦克斯韦平衡分布。在这项工作中,已经针对几种不同的托卡马克参数分析了高能α粒子对静电湍流的响应。我们的结果与已知的标度和实验证据一致,即α粒子通常被很好地限制在:几秒钟的数量级。还证实了,与线性理论一致,在实际较低的浓度下,α对湍流的影响可以忽略不计。结果表明,使用高温麦克斯韦原理的惯常做法虽然先前已显示出对扩散系数的适当数量级估计,但对径向α粒子通量却给出了不正确的估计,以及一种校正方法。提供一般。此外,我们看到与碰撞和传输相关的时标在中等能量下竞争,这使人们对以下假设提出了质疑:α粒子仍被限制在用于减慢分布的通量表面中。

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