Intermittent turbulence and turbulent structures in a linear magnetized plasma

Intermittent turbulence and turbulent structures in a linear magnetized plasma
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DOI:
10.1063/1.2158929
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发表时间:
2005-04
期刊:
影响因子:
2.2
通讯作者:
T. Carter
T. Carter
中科院分区:
物理与天体物理3区
文献类型:
--
作者:
T. Carter

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在美国加州大学洛杉矶分校的大型等离子体装置中,在限制器的阴影中观察到了强间歇性湍流[W。Gekelman等人,Rev. Sci.仪器。62,2875(1991)]。湍流的振幅概率分布函数是强烈偏斜的,其中密度耗尽事件(或“空穴”)在高密度区域中占主导,而密度增强事件(或“斑点”)在低密度区域中占主导。二维交叉条件平均表明,斑点是分离的,向外传播的对流结构具有明确的偶极电位,而孔似乎是一个更广泛的湍流结构的一部分。对这些斑点的统计研究显示,它们的典型尺寸是离子声音回旋半径的十倍,典型速度是声速的十分之一。
Strongly intermittent turbulence is observed in the shadow of a limiter in the large plasma device at UCLA [W. Gekelman et al., Rev. Sci. Instrum. 62, 2875 (1991)]. The amplitude probability distribution function of the turbulence is strongly skewed, with density depletion events (or “holes”) dominant in the high-density region and density-enhancement events (or “blobs”) dominant in the low-density region. Two-dimensional cross-conditional averaging shows that the blobs are detached, outward-propagating filamentary structures with a clear dipolar potential, while the holes appear to be part of a more extended turbulent structure. A statistical study of the blobs reveals a typical size of ten times the ion sound gyroradius and a typical velocity of one-tenth the sound speed.