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A simulation and theoretical study of energy transport in the event of MHD Kelvin-Helmholtz instability
S. H. Lai
, Ling-Hsiao Lyu
太空科學與科技研究中心
太空科學與工程學系
研究成果
:
雜誌貢獻
›
期刊論文
›
同行評審
10
引文 斯高帕斯(Scopus)
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Keyphrases
Ambient Plasma
12%
Energy Flux
12%
Energy Transport
100%
Fast Mode
100%
Group Velocity
12%
Kelvin-Helmholtz Instability
100%
Mach Cone
25%
Mach number
25%
Magnetic Field Lines
12%
Magnetohydrodynamic Simulation
12%
Magnetohydrodynamics
100%
Magnetosphere
12%
Plane Wave
25%
Shear Layer
75%
Surface Perturbation
12%
Surface Waves
100%
Transport Velocity
12%
Two-fluid Magnetohydrodynamics
12%
Velocity Shear
75%
Wave Energy
62%
Engineering
Emitted Wave
16%
Energy Engineering
16%
Energy Flux
16%
Energy Transport
100%
Group Velocity
16%
Kelvin Helmholtz Instability
100%
Mach Cone
33%
Mach Number
33%
Magnetic Field Line
16%
Magnetohydrodynamics
100%
Plane Wave
33%
Shear Layer
100%
Simulation Result
50%
Theoretical Study
100%
Transport Velocity
16%
Two Dimensional
16%
Wave Energy
83%
Earth and Planetary Sciences
Energy Flux
12%
Group Velocity
12%
Kelvin-Helmholtz Instability
100%
Mach Cone
25%
Mach Number
25%
Magnetohydrodynamic Simulation
12%
Magnetohydrodynamics
100%
Magnetosphere
12%
Plane Wave
25%
Shear Layer
75%
Surface Wave
100%
Theoretical Study
100%
Wave Energy
62%
Physics
Blood Plasma
25%
Group Velocity
12%
Kelvin-Helmholtz Instability
100%
Mach Cone
25%
Mach Number
25%
Magnetic Field
12%
Magnetohydrodynamic Simulation
12%
Magnetohydrodynamics
100%
Magnetosphere
12%
Plane Wave
25%
Shear Layer
75%
Surface Wave
100%