Magnetized plasma pressure filaments: Analysis of chaotic and intermittent transport events driven by drift-Alfven modes

被引:3
|
作者
Karbashewski, S. [1 ]
Sydora, R. D. [2 ]
Van Compernolle, B. [3 ,4 ]
Simala-Grant, T. [2 ]
Poulos, M. J. [3 ,5 ]
机构
[1] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
[2] Univ Alberta, Dept Phys, Edmonton, AB T6G 2E1, Canada
[3] Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA 90095 USA
[4] Gen Atom, San Diego, CA 92121 USA
[5] Princeton Plasma Phys Lab, Princeton, NJ 08536 USA
基金
美国国家科学基金会; 加拿大自然科学与工程研究理事会;
关键词
CLASSICAL HEAT-TRANSPORT; FLUCTUATIONS; TURBULENCE;
D O I
10.1063/5.0104283
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
The origin of intermittent fluctuations in an experiment involving several interacting electron plasma pressure filaments in close proximity, embedded in a large linear magnetized plasma device, is investigated. The probability density functions of the fluctuations on the inner and outer gradient of the filament bundle are non-Gaussian and the time series contain uncorrelated Lorentzian pulses that give the frequency power spectral densities an exponential shape. A cross-conditionally averaged spatial reconstruction of a temporal event reveals that the intermittent character is caused by radially and azimuthally propagating turbulent structures with transverse spatial scales on the order of the electron skin depth. These eruption events originate from interacting pressure gradient-driven drift-Alfven instabilities on the outer gradient and edge of the filament bundle. The temporal Lorentzian shape of the intermittent structures and exponential spectra are suggestive of deterministic chaos in the underlying dynamics; this conclusion is supported by the complexity-entropy analysis (CH-plane) that shows the experimental time series are located in the chaotic regime. Published under an exclusive license by AIP Publishing.
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页数:15
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