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Mean-field electrodynamics, including both {α} and {β} effects while accounting for the effects of small-scale magnetic fields, is derived for incompressible magnetohydrodynamics. The principal result is {α}=(α₀+β₀R{·}{∇}×{}R)/(1+R²), {β}=β₀; where α₀,β₀ are conventional kinematic dynamo parameters, the reduction factor is proportional to the mean magnetic field R=Rₘ1/2B/({ρ}V²{)}1/2$, ${R}ₘ$ is the magnetic Reynolds number, and V is the characteristic turbulent velocity. This result follows from a generalization of the Zeldovich theorem to three dimensions, exploiting magnetic helicity balance.
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Gruzinov et al. (1994) studied this question.
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