A 3D mean-field dynamo model tracks helicity flux from emerging active regions and finds that their self-induced twist dominates early, while differential rotation controls the late-stage hemispheric helicity rule.
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Helicity Fluxes and Hemispheric Helicity Rule of Active Regions Emerging from the Convection Zone Dynamo
A 3D mean-field dynamo model tracks helicity flux from emerging active regions and finds that their self-induced twist dominates early, while differential rotation controls the late-stage hemispheric helicity rule.