Modeling helioseismic modes in the magnetic atmosphere of the Sun

Physics

• Frequencies 100%
• Wave Propagation 50%
• Acoustic Wave 50%
• Magnetohydrodynamics 50%
• Lower Atmosphere 50%
• Solar Interior 50%
• Model 50%
• Atmospherics 50%
• Linewidth 50%
• Solar Surface 50%
• Magnetic Fields 50%
• Utilization 50%
• Oscillation 50%
• Atmospheric Effects 50%