The old subgiant 31 Aql exhibits a strong non-cycling magnetic field and revived wind braking torque consistent with a shift to anti-solar differential rotation.
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2026 2representative citing papers
3D RT in a MURaM-ChE enhanced network simulation produces Mg II h&k lines closer to IRIS data than 1.5D, showing larger 1.5D-3D discrepancies than Bifrost due to horizontal velocities and more scatter in correlations.
citing papers explorer
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Anti-Solar Differential Rotation May Have Revived Magnetic Braking in the Subgiant 31 Aquilae
The old subgiant 31 Aql exhibits a strong non-cycling magnetic field and revived wind braking torque consistent with a shift to anti-solar differential rotation.
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Mg II h&k spectral line properties computed using 3D radiative transfer in an enhanced network region simulated with the MURaM-ChE code
3D RT in a MURaM-ChE enhanced network simulation produces Mg II h&k lines closer to IRIS data than 1.5D, showing larger 1.5D-3D discrepancies than Bifrost due to horizontal velocities and more scatter in correlations.