RF stabilization of plasma instabilities: a note on physical mechanism

被引:0
作者
Sen, S. [1 ,2 ]
Martinell, J. [3 ]
Imadera, K. [4 ]
Kishimoto, Y. [4 ]
Vahala, G. [2 ]
机构
[1] Natl Inst Aerosp, Hampton, VA 23666 USA
[2] William & Mary, Williamsburg, VA 23185 USA
[3] Univ Nacl Autonoma Mexico, Mexico City, DF, Mexico
[4] Kyoto Univ, Uji, Kyoto, Japan
来源
RADIATION EFFECTS AND DEFECTS IN SOLIDS | 2018年 / 173卷 / 1-2期
关键词
Plasma; diffusion; technology; RADIO-FREQUENCY WAVES; GRADIENT-DRIVEN MODES; GYROKINETIC SIMULATION;
D O I
10.1080/10420150.2018.1449211
中图分类号
TL [原子能技术]; O571 [原子核物理学];
学科分类号
0827 ; 082701 ;
摘要
In a series of recent works, we have developed models including realistic spatial profiles of both flow and radio-frequency-induced ponderomotive force. With these inclusions, the picture of stability of various plasma and fluid instabilities is expected to be changed drastically with ground-breaking consequences. The inhomogeneous parallel flow and the radio-frequency waves can actually stabilize turbulence. This is different from the prevalent notion that both parallel flow shear and radio-frequency waves are responsible for the excitation (destabilization) of plasma turbulence. This model thus aims to open-up new channels and provide a major breakthrough in our knowledge of plasma and fluid turbulence and its consequent roles in energy, space and processing technology. In this short note, we elucidate the physical mechanism behind this novel observation.
引用
收藏
页码:165 / 168
页数:4
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    [J]. RADIATION EFFECTS AND DEFECTS IN SOLIDS, 2017, 172 (1-2): : 32 - 38
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    [J]. RADIATION EFFECTS AND DEFECTS IN SOLIDS, 2016, 171 (1-2): : 52 - 59
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