Interplanetary shocks generated by expanding magnetic loops

Keyphrases

• Magnetic Loops 100%
• Interplanetary Shocks 100%
• Outer Heliosphere 40%
• Numerical Model 20%
• Shock Waves 20%
• Heat Conduction 20%
• Turbulence 20%
• Magnetic Field Strength 20%
• Coronal Mass Ejections 20%
• Magnetic Clouds 20%
• Energy Exchange 20%
• Heliosphere 20%
• Shock 20%
• Navier-Stokes Equations 20%
• Viscous Heating 20%
• Two-fluid 20%
• Initial Perturbation 20%
• Ion Energy 20%
• Plasma Motion 20%
• Strong Shock 20%
• Magnetohydrostatics 20%
• Relaxation Zone 20%
• Modified Coefficient 20%
• Typical Features 20%
• Weak Shock 20%
• Shock Wave Formation 20%
• Ion Viscosity 20%
• Upper Boundary 20%
• Shock Parameters 20%
• Transient Shock 20%

Physics

• Shock Wave 100%
• Heliosphere 100%
• Interplanetary Shock Wave 100%
• Magnetic Field 33%
• Numerical Model 33%
• Field Strength 33%
• Transients 33%
• Magnetic Clouds 33%
• Energy Transfer 33%
• Navier-Stokes Equation 33%
• Conductive Heat Transfer 33%
• Magnetohydrostatics 33%