Three-dimensional MHD modeling of the solar wind structures associated with 13 December 2006 coronal mass ejection

Keyphrases

• Ambient Solar Wind 25%
• Coronal Mass Ejections 100%
• Dynamic Parameters 25%
• Geometric Dynamics 25%
• Geometric Parameters 25%
• In Situ 25%
• In Situ Observation 25%
• Interplanetary Magnetic Field 50%
• Interplanetary Propagation 25%
• Interplanetary Shocks 25%
• Magnetic Clouds 25%
• Magnetic Field 25%
• Magnetic Parameters 25%
• Magneto-hydrodynamic Modeling 100%
• Magnetohydrodynamic Simulation 25%
• Solar Wind 25%
• Solar Wind Structure 100%
• Spheromak 50%
• Three-dimensional (3D) 100%
• Wind Model 25%

Earth and Planetary Sciences

• Coronal Mass Ejection 100%
• Interplanetary Magnetic Field 50%
• Interplanetary Shock Wave 25%
• Magnetic Clouds 25%
• Magnetohydrodynamic Simulation 25%
• Magnetohydrodynamics 100%
• Solar Wind 100%
• Spacecraft 25%
• Spheromaks 50%

Physics

• Interplanetary Magnetic Field 66%
• Interplanetary Shock Wave 33%
• Magnetic Clouds 33%
• Magnetic Field 33%
• Magnetohydrodynamic Simulation 33%
• Magnetohydrodynamics 100%
• Solar Wind 100%
• Spacecraft 33%
• Spheromaks 66%