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Modeling helioseismic modes in the magnetic atmosphere of the Sun
B. Pintér
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Corresponding author for this work
Department of Physics
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Physics
Acoustic Wave
50%
Atmospheric Effects
50%
Atmospherics
50%
Frequencies
100%
Linewidth
50%
Lower Atmosphere
50%
Magnetic Fields
50%
Magnetohydrodynamics
50%
Model
50%
Oscillation
50%
Solar Interior
50%
Solar Surface
50%
Utilization
50%
Wave Propagation
50%