Non-linear dynamo waves in magnetized shear flows: a candidate mechanism for the solar cycle

arXiv:2609.30367 · astro-ph.SR, astro-ph.EP, astro-ph.HE, physics.plasm-ph · Submitted 2026-09-24 · Read on arXiv

astro-ph.SR, astro-ph.EP, astro-ph.HE, physics.plasm-ph

Submitted: 2026-09-24

Updated: 2026-09-24

Terminology

• Alignment — 3× in this paper · explained in 1 episode
• Actor — 2× in this paper · explained in 3 episodes
• Active Regions — 1× in this paper · explained in 1 episode
• Conservation Laws — 1× in this paper · explained in 3 episodes
• Fine-Tuning — 1× in this paper · explained in 5 episodes
• Trace — 1× in this paper · explained in 2 episodes
• Verification — 1× in this paper · explained in 2 episodes

Sources

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• Synthetic solar cycle for active regions violating the Hale's polarity law
• Observing and modeling the poloidal and toroidal fields of the solar dynamo
• On the magnetic field required for driving the observed angular-velocity variations in the solar convection zone
• Hemispheric Magnetic Asymmetry and Cross-Equatorial Circulation Cells within the Sun's Near-Surface Shear Layer
• Characteristics of solar meridional flows during solar cycle 23
• Inferring the Solar Meridional Circulation Flow Profile by Applying Bayesian Methods to Time-distance Helioseismology
• Revisiting the solar tachocline: Average properties and temporal variations
• Latitude-Dependent Time Variations of the Solar Tachocline
• Resolving the Tachocline using Inversion of Rotational Splitting Derived from Fitting Very Long and Long Time Series
• Probing the large-scale magnetic field inside the Sun from three decades of observed surface magnetograms
• The Sun's acoustic asphericity and magnetic fields in the solar convection zone
• Helioseismic Evidence That the Solar Dynamo Originates near the Tachocline
• Hale cycle in solar hemispheric radio flux and sunspots: Evidence for a northward shifted relic field

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