论文标题

不可压缩的圆柱等离子体中负能量表面磁流体动力波的激发

Excitation of negative energy surface magnetohydrodynamic waves in an incompressible cylindrical plasma

论文作者

Yu, D. J., Nakariakov, V. M.

论文摘要

负能波现象可能在存在波衰减机制和外部能量供应的情况下出现在剪切流中。我们研究在不可压缩极限下在等离子体圆柱体中的负能表面波的出现。气缸被轴向磁场和不同密度的等离子体包围。考虑到内部的流动和磁管外部的粘度,我们得出了分散关系,并获得了波浪的相位速度和生长速率(增量)的分析溶液。发现与负能量波(新闻)和开尔文 - 赫尔姆霍尔茨不稳定性(KHI)相关的耗散不稳定性的临界速度剪切依赖轴向波长。对于最长的轴向波长来说,新出现的香肠出现的临界剪切最低,而对于扭结波,对于与圆柱体直径相当的轴向波长,达到了临界剪切的最小值。耗散不稳定性的临界速度和KHI阈值之间的范围取决于气缸内外的AlfVén速度的差。对于所有轴向波数,剪切流速低于KHI阈值的新出现。在不足的圆柱体中兴奋的是比浓度更容易。可以有效地针对具有较大的轴向波数的方位角数$ m = 0 $生成负能量表面波,并且具有较小的轴向波数的较高模式($ m> 0 $)。

Negative energy wave phenomena may appear in shear flows in the presence of a wave decay mechanism and external energy supply. We study the appearance of negative energy surface waves in a plasma cylinder in the incompressible limit. The cylinder is surrounded by an axial magnetic field and by a plasma of different density. Considering flow inside and viscosity outside the flux tube, we derive dispersion relations, and obtain analytical solutions for the phase speed and growth rate (increment) of the waves. It is found that the critical speed shear for the occurrence of the dissipative instability associated with negative energy waves (NEWs) and the threshold of Kelvin--Helmholtz instability (KHI) depend on the axial wavelength. The critical shear for the appearance of sausage NEW is lowest for the longest axial wavelengths, while for kink waves the minimum value of the critical shear is reached for the axial wavelength comparable to the diameter of the cylinder. The range between the critical speed of the dissipative instability and the KHI threshold is shown to depend on the difference of the Alfvén speeds inside and outside of the cylinder. For all axial wavenumbers, NEW appears for the shear flow speeds lower than the KHI threshold. It is easier to excite NEW in an underdense cylinder than in an overdense one. The negative energy surface waves can be effectively generated for azimuthal number $m=0$ with a large axial wave number and for higher modes ($m>0$) with a small axial wave number.

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