Observation of the spatial growth of self-excited dust-density waves

被引:62
作者
Flanagan, T. M. [1 ]
Goree, J. [1 ]
机构
[1] Univ Iowa, Dept Phys & Astron, Iowa City, IA 52242 USA
基金
美国国家科学基金会;
关键词
CURRENT GLOW-DISCHARGE; ACOUSTIC-WAVES; TRANSVERSE-WAVES; PLASMAS; INSTABILITY; CONFINEMENT; PRESSURE; CRYSTALS; MODES;
D O I
10.1063/1.3524691
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 growth of a naturally occurring dust-density wave (DDW) is experimentally observed using high-speed imaging. This low frequency wave (similar to 25 Hz) grows in amplitude as it propagates downward through a dusty plasma. The wave's linear growth rate -k(i) is measured using a phase-sensitive analysis method. For the conditions studied here, the growth rate increases as gas pressure decreases. At a critical gas pressure, which is observed, a balance between an ion-flow instability and dissipation by neutral gas drag determines a threshold for wave propagation. A linear dispersion relation is derived, taking into account the effects of strong-coupling, to compare to the experiment. (C) 2010 American Institute of Physics. [doi: 10.1063/1.3524691]
引用
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页数:9
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