总100页4 等离体不稳定性分类(1) 宏观(流体)的不稳定性(3维坐标空间)--磁(单)流体不稳定性---理想的磁流体(Ideal MHD)不稳定性理想的磁流体(Ideal MHD)不稳定性---电阻(耗散)的磁流体不稳定性总100页5--电磁(双)流体不稳定性 微观(动理学)的不稳定...
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本文利用理想磁流体力学(MHD)模型对含有轴向流动的Z箍缩等离子体不稳定性进行了分析。
A linear analysis of the ideal magnetohydrodynamic (MHD) stability of the Z-pinch is presented in which plasma flows are included in the equilibrium.
采用理想磁流体力学方程组(MHD)作为太阳大气动力学过程的控制方程组，定性数值模拟日冕物质抛射(CME)现象。
The ideal Magnetohydrodynamic equations (MHD), the governing equations of the solar atmosphere dynamical process, are taken to numerically simulate Coronal Mass Ejection (CME) phenomena.
现有鱼骨模理论是建立在理想磁流体近似基础上的，它预言有两支不稳定分支。
Theoretical analyses of fishbone modes based on the ideal MHD framework have predicted that two branches of modes exists.
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