2D Relativistic MHD simulations of the Kruskal-Schwarzschild instability in a relativistic striped wind

Keyphrases

• Acceleration Mechanism 33%
• Active Galactic nuclei 33%
• Bulk Flow 33%
• Bulk Velocity 33%
• Current Layer 66%
• Dissipation Rate 33%
• Drip 33%
• Dripping 33%
• Effective Gravity 33%
• Energy Dissipation Rate 33%
• Evacuation 33%
• Gamma-ray Bursts 33%
• Hot Plasma 100%
• Instability Growth Rate 33%
• Kelvin-Helmholtz Instability 33%
• Kruskal 100%
• Linear Regime 33%
• Linear Stability Analysis 33%
• Magnetic Energy 33%
• Magnetic Field 33%
• Magnetic Field Lines 33%
• Magnetic Reconnection 33%
• Magnetohydrodynamic Simulation 66%
• MHD Simulation 100%
• Microquasars 33%
• Nonlinear Development 33%
• Nonlinear Regime 33%
• Parallel Magnetic Field 33%
• Plasma Layer 33%
• Rayleigh-Taylor Instability 33%
• Reconnecting 33%
• Reconnection 100%
• Relativistic Magnetohydrodynamics 66%
• Relativistic MHD 100%
• Schwarzschild 100%
• Self-sustaining 33%
• Small Aspect Ratio 33%
• Steady State 33%
• Sweet 33%
• Turbulence 33%
• Turbulent Velocity 33%
• Two Dimensional 100%

Physics

• Active Galactic Nuclei 33%
• Aspect Ratio 33%
• Blood Plasma 33%
• Gamma Ray Burst 33%
• High Temperature Plasmas 100%
• Kelvin-Helmholtz Instability 33%
• Magnetic Field 100%
• Magnetohydrodynamic Generator 100%
• Magnetohydrodynamic Simulation 66%
• Plasma Layer 33%
• Quasar 33%
• Steady State 33%
• Taylor Instability 33%
• Volume 66%