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An improved current potential method for fast computation of stellarator coil shapes

机译:一种快速计算恒星线圈形状的改进的电流势方法

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Several fast methods for computing stellarator coil shapes are compared, including the classical NESCOIL procedure (Merkel 1987 Nucl. Fusion 27 867), its generalization using truncated singular value decomposition, and a Tikhonov regularization approach we call REGCOIL in which the squared current density is included in the objective function. Considering W7-X and NCSX geometries, and for any desired level of regularization, we find the REGCOIL approach simultaneously achieves lower surface-averaged and maximum values of both current density (on the coil winding surface) and normal magnetic field (on the desired plasma surface). This approach therefore can simultaneously improve the free-boundary reconstruction of the target plasma shape while substantially increasing the minimum distances between coils, preventing collisions between coils while improving access for ports and maintenance. The REGCOIL method also allows finer control over the level of regularization, it preserves convexity to ensure the local optimum found is the global optimum, and it eliminates two pathologies of NESCOIL: the resulting coil shapes become independent of the arbitrary choice of angles used to parameterize the coil surface, and the resulting coil shapes converge rather than diverge as Fourier resolution is increased. We therefore contend that REGCOIL should be used instead of NESCOIL for applications in which a fast and robust method for coil calculation is needed, such as when targeting coil complexity in fixed-boundary plasma optimization, or for scoping new stellarator geometries.
机译:比较了几种计算恒星线圈形状的快速方法,包括经典的NESCOIL程序(Merkel 1987 Nucl。Fusion 27 867),使用截断的奇异值分解进行广义化以及Tikhonov正则化方法(我们称为REGCOIL),其中包括平方电流密度在目标函数中。考虑到W7-X和NCSX的几何形状,以及对于任何所需的正则化水平,我们发现REGCOIL方法可同时实现较低的表面平均和电流密度(在线圈绕组表面)和法向磁场(在所需的等离子体上)的最大值表面)。因此,该方法可以同时改善目标等离子体形状的自由边界重构,同时实质上增加线圈之间的最小距离,防止线圈之间发生碰撞,同时改善端口和维护的通道。 REGCOIL方法还允许对正则化水平进行更精细的控制,它保留凸度以确保找到的局部最优值是全局最优值,并且消除了NESCOIL的两种病态:产生的线圈形状变得独立于用于参数化的角度的任意选择线圈表面,并且随着傅立叶分辨率的提高,最终的线圈形状收敛而不是发散。因此,我们认为,对于需要快速而稳健的线圈计算方法的应用,例如在固定边界等离子体优化中针对线圈复杂性或确定新的恒星几何时,应使用REGCOIL而不是NESCOIL。

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