A new global instability of toroidal magnetic fields in stars is reported that grows on the Alfvén time, is less dissipation-sensitive than the Tayler instability, and may affect angular momentum transport.
C., Mathis, S., & Astoul, A
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Chiral magnetic effect generates magnetar-strength dipoles independently of initial net helicity via localized structures on decade timescales.
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.
citing papers explorer
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Beyond the Tayler instability: A new global instability of toroidal magnetic fields in stars
A new global instability of toroidal magnetic fields in stars is reported that grows on the Alfvén time, is less dissipation-sensitive than the Tayler instability, and may affect angular momentum transport.
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Magnetar field dynamics driven by chiral anomalies without magnetic helicity
Chiral magnetic effect generates magnetar-strength dipoles independently of initial net helicity via localized structures on decade timescales.
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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.