3D solar dynamo simulations require active region disconnection from the convection zone base to match calibrated 2D surface flux transport models, but increasing diffusivity to achieve this prevents the dynamo from sustaining itself over a full cycle.
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The need for active region disconnection in 3D kinematic dynamo simulations
3D solar dynamo simulations require active region disconnection from the convection zone base to match calibrated 2D surface flux transport models, but increasing diffusivity to achieve this prevents the dynamo from sustaining itself over a full cycle.