Speaker
Description
In helioseismology, traditional analytical models often neglect the effects of rotation and magnetic fields, limiting their applicability. However, observations frequently reveal instances where these elements are critical. Previous studies have investigated the influence of externally imposed magnetic fields on seismic modes using idealized 2D MHD simulations. Here, we extend this work by performing 3D MHD simulations using the Pencil Code to examine the impact of self-sustained, dynamo-generated magnetic fields on seismic modes, particularly the
Contribution Type | Poster |
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Theme | Solar Magnetism over Long-Time Scales |