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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
Surface Waves
100%
Fast Mode
100%
Magnetohydrodynamics
100%
Energy Transport
100%
Kelvin-Helmholtz Instability
100%
Velocity Shear
75%
Shear Layer
75%
Wave Energy
62%
Plane Wave
25%
Mach number
25%
Mach Cone
25%
Magnetosphere
12%
Group Velocity
12%
Magnetic Field Lines
12%
Ambient Plasma
12%
Magnetohydrodynamic Simulation
12%
Energy Flux
12%
Two-fluid Magnetohydrodynamics
12%
Surface Perturbation
12%
Transport Velocity
12%
Engineering
Theoretical Study
100%
Energy Transport
100%
Shear Layer
100%
Kelvin Helmholtz Instability
100%
Magnetohydrodynamics
100%
Wave Energy
83%
Simulation Result
50%
Mach Number
33%
Plane Wave
33%
Mach Cone
33%
Energy Engineering
16%
Two Dimensional
16%
Group Velocity
16%
Magnetic Field Line
16%
Energy Flux
16%
Transport Velocity
16%
Emitted Wave
16%
Earth and Planetary Sciences
Theoretical Study
100%
Magnetohydrodynamics
100%
Kelvin-Helmholtz Instability
100%
Surface Wave
100%
Shear Layer
75%
Wave Energy
62%
Mach Number
25%
Plane Wave
25%
Mach Cone
25%
Magnetosphere
12%
Group Velocity
12%
Energy Flux
12%
Magnetohydrodynamic Simulation
12%
Physics
Magnetohydrodynamics
100%
Kelvin-Helmholtz Instability
100%
Surface Wave
100%
Shear Layer
75%
Plane Wave
25%
Mach Number
25%
Mach Cone
25%
Blood Plasma
25%
Magnetic Field
12%
Magnetosphere
12%
Group Velocity
12%
Magnetohydrodynamic Simulation
12%