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Near-singular equilibrium currents near magnetic islands with broken symmetry

机译:对称破坏的磁岛附近的近奇异平衡电流

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摘要

The conventional cylindrical analytical model of a magnetic island is symmetric with respect to combined reflection in the poloidal and toroidal angles, a symmetry property sometimes called 'stellarator symmetry'. There are cancellations in the pressure driven currents when an island is stellarator symmetric that are not there when the symmetry is broken. When the symmetry is broken, new aspects of the island physics emerge. The diamagnetic current driven by the scalar pressure is no longer ambipolar. The pressure-driven current generally has a logarithmic (integrable) singularity at the island separatrix. These effects manifest themselves when taking into account incomplete flattening of the pressure along magnetic field lines. A small magnetic island has only a small effect on the ambient pressure gradient, so that the pressure is not constant on the flux surfaces near the island. For larger islands, this behavior persists near the X-lines. The equilibrium solutions with a small island are to be compared with three-dimensional magnetohydrodynamic equilibrium solutions that are constrained to have simply nested flux surfaces, where the pressure-driven current goes like 1/x near rational surfaces, where x is the distance from the rational surface. This paper presents an investigation of the pressure driven current near a small magnetic island in a cylindrical magnetic field with perturbed circular flux surfaces. The conventional analytical cylindrical model of a field with a magnetic island is augmented with a resonant component that breaks the stellarator symmetry without breaking the flux surfaces. The effects of stellarator symmetry on magnetic islands in tokamaks are of particular interest in the context of the stabilization of edge localized modes by resonant magnetic perturbations. In stellarators, the design studies for the major contemporary devices have discarded half the design parameters available for optimization at the outset by assuming stellarator symmetry.
机译:磁岛的常规圆柱分析模型相对于多角和环形角度的组合反射是对称的,这种对称特性有时称为“恒星对称”。当岛为恒星对称时,压力驱动电流会抵消,而对称性破坏时则不会。当对称性破裂时,岛屿物理学的新方面应运而生。由标量压力驱动的反磁性电流不再是双极性的。压力驱动的电流通常在岛分离线处具有对数(可积分)奇点。当考虑到沿磁力线的压力不完全平坦时,这些效果就会显现出来。较小的磁岛对环境压力梯度的影响很小,因此在岛附近的磁通表面上压力不是恒定的。对于较大的岛屿,此行为在X线附近持续存在。带有小岛的平衡解应与三维磁流体动力学平衡解进行比较,后者必须具有简单的嵌套磁通面,其中在有理面附近,压力驱动电流近似为1 / x,其中x是与磁通面的距离。合理的表面。本文介绍了在圆柱磁场中具有扰动的圆形通量表面的小磁岛附近的压力驱动电流的研究。具有磁岛的磁场的常规分析圆柱模型增加了一个共振分量,该共振分量破坏了恒星的对称性而不破坏通量表面。在通过共振磁扰动稳定边缘局域模的情况下,恒星的对称性对托卡马克中磁岛的影响尤为重要。在恒星器中,主要的现代设备的设计研究已经通过假设恒星器的对称性一开始就丢弃了可用于优化的一半设计参数。

著录项

  • 来源
    《Nuclear fusion》 |2019年第5期|056016.1-056016.11|共11页
  • 作者

    Reiman A. H.; Radhakrishnan D.;

  • 作者单位

    Princeton Univ, Princeton Plasma Phys Lab, Princeton, NJ 08544 USA;

    NYU, New York, NY 10003 USA;

  • 收录信息 美国《科学引文索引》(SCI);美国《工程索引》(EI);美国《生物学医学文摘》(MEDLINE);
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

    magnetic islands; RMP ELM suppression; stellarator optimization;

    机译:磁岛;RMP ELM抑制;恒星优化;
  • 入库时间 2022-08-18 04:20:08

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