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Physics design of a high-beta quasi-axisymmetric stellarator

机译:高β准轴对称恒星的物理设计

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Key physics issues in the design of a high-beta quasi-axisymmetric stellarator configuration are discussed. The goal of the design study is a compact stellarator configuration with aspect ratio comparable to that of tokamaks and good transport and stability properties. Quasi-axisymmetry has been used to provide good drift trajectories. Ballooning stabilization has been accomplished by strong axisymmetric shaping, yielding a stellarator configuration whose core is in the second stability regime for ballooning modes. A combination of externally generated shear and non-axisymmetric corrugation of the plasma boundary provides stability to external kink modes even in the absence of a conducting wall. The resulting configuration is also found to be robustly stable to vertical modes, increasing the freedom to perform axisymmetric shaping. Stability to neoclassical tearing modes is conferred by a monotonically increasing i profile. A gyrokinetic delta f code has been used to confirm the adequacy of the neoclassical confinement. Neutral beam losses have been evaluated with Monte Carlo codes. [References: 26]
机译:讨论了高β准轴对称恒星器配置设计中的关键物理问题。设计研究的目标是紧凑的恒星构造,其纵横比与托卡马克相当,并具有良好的运输和稳定性能。准轴对称已用于提供良好的漂移轨迹。通过强大的轴对称成形已经实现了气球膨胀的稳定,从而产生了一种星状配置,其核心处于气球膨胀模式的第二个稳定状态。即使在没有导电壁的情况下,外部产生的剪切力和等离子体边界的非轴对称波纹的组合也为外部扭结模式提供了稳定性。还发现所得的构造对于垂直模式具有鲁棒的稳定性,从而增加了执行轴对称成形的自由度。单调增加的i轮廓赋予了新古典撕裂模式的稳定性。陀螺动力学代码已被用于确认新古典禁闭的适当性。中性光束损失已通过蒙特卡洛代码进行了评估。 [参考:26]

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