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Investigation of flute instability in application to laboratory astrophysics and Z-pinch experiments

机译:长笛不稳定性在实验室天体物理学和Z捏实验中的应用研究

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Interaction of plasma flows with magnetic fields can lead to excitation of flute-like oscillations. These oscillations can also be excited in Z-pinch plasmas. We have developed understanding of nonlinear dynamics of compressible flute mode turbulence with spatial scales comparable to the ion Larmor radius in a high beta plasma, when these modes become electromagnetic and in the presence of a non-uniform magnetic field. It is shown that the flute waves are responsible for generation of large scale structures of streamer and zonal flow types as well as Kolmogorov type spectra in the short scale region. The relevance of the obtained results to laboratory astrophysics and Z-pinch experiments is discussed. Keywords Flute instability - High beta plasma - Nonlinear wave dynamics - Laboratory astrophysics experiments - Z-pinches
机译:等离子体流与磁场的相互作用会导致产生类似长笛的振荡。这些振荡也可以在Z捏等离子体中激发。我们已经了解了可压缩的长笛模式湍流的非线性动力学,其空间尺度可与高贝塔等离子体中的离子拉莫尔半径相媲美,当这些模式变为电磁且存在非均匀磁场时。结果表明,在短尺度范围内,长笛波是流形和纬向流型以及Kolmogorov型谱的大尺度结构生成的原因。讨论了获得的结果与实验室天体物理学和Z捏实验的相关性。长笛不稳定性-高β等离子体-非线性波动力学-实验室天体物理学实验-Z夹点

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