Astrophysical gyrokinetics: Kinetic and fluid turbulent cascades in magnetized weakly collisional plasmas

Keyphrases

• Alfvn Waves 100%
• Turbulence 100%
• Collision-free 100%
• Collisional Plasma 100%
• Magnetohydrodynamic Equations 100%
• Reduced Magnetohydrodynamics 100%
• Gyrokinetics 100%
• Inertial Range 100%
• Turbulent Cascade 100%
• Field Lines 50%
• Interstellar Medium 50%
• Magnetic Field Strength 50%
• Accretion Discs 50%
• Mean Free Path 50%
• Phase Space 50%
• Astrophysical Plasmas 50%
• Density Field 50%
• Scaling Relations 50%
• Electromagnetic Fluctuation 50%
• Density Fluctuations 50%
• Kolmogorov 50%
• Ion Heating 50%
• System of Equations 50%
• Kinetic Problems 50%
• Turbulent Motion 50%
• Cyclotron Frequency 50%
• Slow Mode 50%
• Wave Energy 50%
• Plasma Physics 50%
• Plasma Fluctuations 50%
• Ion Cyclotron 50%
• Fully Kinetic 50%
• Particle Heating 50%
• Electron Diffusion 50%
• Plasma Turbulence 50%
• Astrophysical Applications 50%
• Mean Magnetic Field 50%
• Turbulent Fluctuation 50%
• Astrophysical Observations 50%
• Phase Lead 50%
• Entropy Fluctuations 50%
• Diffusion Scale 50%
• Fluid-like 50%
• Linear Kinetic Equations 50%
• Outer Scale 50%
• Entropy Mode 50%
• Special Scales 50%
• Media Cluster 50%
• Mean-field 50%
• Solar Wind 50%
• Galaxy Clusters 50%

Physics

• Magnetohydrodynamics 100%
• Magnetic Field 100%
• Collisional Plasmas 100%
• Entropy 100%
• Physics 50%
• Magnetohydrodynamic Generator 50%
• Interstellar Matter 50%
• Field Strength 50%
• Mean Free Path 50%
• Astrophysical Plasma 50%
• Galaxy Clusters 50%
• Theoretical Model 50%
• Cyclotron Frequency 50%
• Solar Wind 50%
• Circumstellar Disks 50%
• Plasma Turbulence 50%
• Kinetic Equation 50%
• Electromagnetism 50%
• Density Fluctuation 50%