The dynamo threshold, cycle period, and surface toroidal field depend on the coronal-to-convective turbulent diffusivity jump, with a large jump restoring vacuum-like boundary conditions.
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Effects of harmonic magnetic field boundary conditions in mean-field solar dynamo
The dynamo threshold, cycle period, and surface toroidal field depend on the coronal-to-convective turbulent diffusivity jump, with a large jump restoring vacuum-like boundary conditions.