Gravity-wave polarization theory is extended to non-axisymmetric stellar magnetic fields, revealing avoided crossings and a new mixing threshold distinct from the magnetic-suppression threshold.
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Synthetic spectra show that observational biases cause dipole mode visibilities to be overestimated by up to 20 percent on the red-giant branch, while partial energy preservation under magnetic damping can produce both present and absent mixed-mode signatures.
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Extending asteroseismic magnetometry across the diverse landscape of magnetic structures
Gravity-wave polarization theory is extended to non-axisymmetric stellar magnetic fields, revealing avoided crossings and a new mixing threshold distinct from the magnetic-suppression threshold.
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Oscillations of red giant stars with magnetic damping in the core. II. Mixed mode visibilities on the red-giant branch
Synthetic spectra show that observational biases cause dipole mode visibilities to be overestimated by up to 20 percent on the red-giant branch, while partial energy preservation under magnetic damping can produce both present and absent mixed-mode signatures.