Decaying columnar magnetic fields spontaneously isotropize and reproduce the expected helical and nonhelical MHD decay scalings, with the Hosking integral conserved for initially pointwise nonhelical fields.
Mean-field dynamo action from delayed transport
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abstract
We analyze the nature of dynamo action that produces horizontally averaged magnetic fields in two particular flows that were studied by Roberts (1972, Phil. Trans. R. Soc. A 271, 411), namely his flows II and III. They have zero kinetic helicity either pointwise (flow II), or on average (flow III). Using direct numerical simulations, we determine the onset conditions for dynamo action at moderate values of the magnetic Reynolds number. Using the test-field method, we show that the turbulent magnetic diffusivity is then positive for both flows. However, we demonstrate that for both flows large-scale dynamo action occurs through delayed transport. Mathematically speaking, the magnetic field at earlier times contributes to the electromotive force through the off-diagonal components of the alpha tensor such that a zero mean magnetic field becomes unstable to dynamo action. This represents a qualitatively new mean-field dynamo mechanism not previously described.
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Inverse cascade from helical and nonhelical decaying columnar magnetic fields
Decaying columnar magnetic fields spontaneously isotropize and reproduce the expected helical and nonhelical MHD decay scalings, with the Hosking integral conserved for initially pointwise nonhelical fields.