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Comparing Numerical Methods for Isothermal Magnetized Supersonic Turbulence
A.G. Kritsuk...[et al.],
Åke Nordlund
, D. Collins, P. Padoan
Astrofysik og Planetforskning
Niels Bohr Institutet - Afd.
85
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Keyphrases
Numerical Dissipation
100%
Supersonic Turbulence
100%
Turbulence Decay
66%
Numerical Algorithms
66%
Numerical Resolution
33%
Time Integration
33%
Force Computation
33%
Benchmark Test Problems
33%
Divergence-free
33%
Integration Techniques
33%
Conservation Laws
33%
Pluto
33%
Riemann Solver
33%
Shock Waves
33%
Solution Accuracy
33%
Robust Representation
33%
Solenoid
33%
Constrained Transport Method
33%
MHD-methods
33%
Decay Test
33%
Gradient Interpolation
33%
Statistical Measures
33%
MHD Code
33%
Artificial Viscosity
33%
Code Comparison
33%
Effective Reynolds number
33%
High-order Accuracy
33%
Divergence Preserving
33%
RAMSES
33%
Transverse Gradient
33%
Divergence Cleaning
33%
Astrophysical Applications
33%
Finite Volume
33%
Spectral Bandwidth
33%
Velocity Components
33%
Earth and Planetary Sciences
Mathematical Method
100%
Star Formation
100%
Molecular Clouds
50%
Interpolation
50%
Conservation Law
50%
Lorentz Force
50%
Reynolds Number
50%
Power Spectra
50%
Shock Wave
50%
Magnetism
50%
Turbulent Flow
50%
Mathematics
Numerical Algorithm
100%
Test Problem
100%
Time Integration
50%
Finite Difference Method
50%
Transverse Gradient
50%
Numerical Approach
50%
Artificial Viscosity
50%
Conservation Law
50%
Velocity Component
50%
Physics
Supersonics
100%
Conservation Law
20%
Lorentz Force
20%