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Liner-on-plasma system near stagnation: Stabilizing effect of a magnetic cushion

机译:接近停滞的等离子体衬里系统:磁垫的稳定作用

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This brief communication is concerned with the adiabatic compression of a high-beta plasma by a heavy liner. Elongated cylindrical and quasi-cylindrical geometries are considered. The magnetic field in a plasma is parallel to the axis, whereas the drive field has azimuthal direction. During the liner acceleration, the most dangerous modes are axisymmetric (m = 0) modes. Near stagnation, these modes are further amplified at the inner surface, as the liner is decelerated by the isotropic pressure of a high-beta plasma. This picture, however, is not complete: due to a heat loss from the plasma core to the relatively cold liner, a zone of a strong axial magnetic field may appear between a hot, high-beta plasma and a cold liner. This magnetic cushion is backed from inside by a very high-beta plasma. The stability of such a system with respect to m = 0 modes is studied and the conclusion is drawn that the stabilizing effect of the magnetic cushion remains strong even for relatively thin cushions and moderate magnetic fields in them.
机译:这种简短的交流与沉重衬里对高β等离子体的绝热压缩有关。考虑了细长的圆柱和准圆柱几何形状。等离子体中的磁场平行于轴,而驱动场具有方位角方向。在线性加速期间,最危险的模式是轴对称(m = 0)模式。由于高β等离子体的各向同性压力使衬管减速,在近乎停滞时,这些模式在内表面上进一步放大。但是,此图片并不完整:由于从等离子体核心到相对较冷的衬套的热损失,在高β的热等离子体和冷衬套之间可能会出现强轴向磁场区域。该磁性垫从内部通过非常高的beta等离子体提供支持。研究了这种系统相对于m = 0模式的稳定性,得出的结论是,即使对于较薄的缓冲垫和适度的磁场,磁性缓冲垫的稳定效果仍然很强。

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