Comparing numerical methods for isothermal magnetized supersonic turbulence

Keyphrases

• Supersonic Turbulence 100%
• Numerical Methods 100%
• Numerical Dissipation 100%
• Star Formation 66%
• Numerical Algorithms 66%
• Spatial Reconstruction 66%
• Turbulence Decay 66%
• Molecular Clouds 33%
• Popular 33%
• Numerical Resolution 33%
• Turbulent Flow 33%
• Magnetic Field 33%
• Finite Volume 33%
• Power Spectrum 33%
• Lorentz Force 33%
• Numerics 33%
• Integration Techniques 33%
• Scale Density 33%
• Shock Waves 33%
• Conservation Laws 33%
• Numerical Scheme 33%
• Statistical Measures 33%
• Time Integration 33%
• Solenoid 33%
• Finite Difference 33%
• Riemann Solver 33%
• Spectral Width 33%
• Divergence-free 33%
• Velocity Components 33%
• High-order Accuracy 33%
• Pluto 33%
• Scientific Applications 33%
• MHD Code 33%
• Astrophysical Applications 33%
• RAMSES 33%
• Constrained Transport Method 33%
• Robust Representation 33%
• Artificial Viscosity 33%
• Free Evolution 33%
• Force Computation 33%
• Effective Reynolds number 33%
• Solution Accuracy 33%
• Transverse Gradient 33%
• Informed Choice 33%
• Code Comparison 33%
• Divergence Preserving 33%
• Divergence Cleaning 33%
• Benchmark Test Problems 33%
• Gradient Interpolation 33%
• MHD-methods 33%
• Decay Test 33%
• Ppml 33%

Physics

• Magnetohydrodynamic Generator 100%
• Supersonics 100%
• Mathematical Method 100%
• Star Formation 40%
• Molecular Clouds 20%
• Turbulent Flow 20%
• Magnetic Field 20%
• Power Spectra 20%
• Lorentz Force 20%
• Reynolds Number 20%
• Conservation Law 20%
• Shock Wave 20%
• Finite Difference Method 20%
• Transportation 20%
• Reynolds' Number 20%