Tayler-Spruit magnetic fields can convert low-frequency internal gravity waves to magneto-gravity waves in low-mass star cores, with effects strongest on the red giant branch in central regions.
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Six seismic solar analogs have masses 0.91-1.04 solar masses, radii 0.95-1.08 solar radii, and ages 1.8-9.1 Gyr, with one star matching the Sun closely enough to be called a solar twin.
citing papers explorer
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Co-existence of Internal Gravity Waves and Tayler-Spruit Magnetic Fields in the Radiative Core of Low-mass Stars
Tayler-Spruit magnetic fields can convert low-frequency internal gravity waves to magneto-gravity waves in low-mass star cores, with effects strongest on the red giant branch in central regions.
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Characterizing six seismic solar analogs observed by Kepler, K2, and HERMES
Six seismic solar analogs have masses 0.91-1.04 solar masses, radii 0.95-1.08 solar radii, and ages 1.8-9.1 Gyr, with one star matching the Sun closely enough to be called a solar twin.