Suppose a steady solenoidal velocity satisfies , and spatial averaging permits integration by parts without boundary terms. For a uniform test magnetic field , the small-magnetic Reynolds number expansion gives and . Using the self-adjointness of the Laplacian inside the average,
The second equality concerns the averaged mean-field electromotive force; it does not assert that the quadratic forcing itself is monochromatic.
// Target: fluid-mechanics.bigb
For , the cross product identity and integration by parts give . Its alpha tensor is
Interchanging reverses the cross product, showing that the coefficient is an antisymmetric matrix. Such a coefficient represents a turbulent magnetic pumping contribution rather than the symmetric part of the alpha effect.
// Target: fluid-mechanics.bigb
The first coefficient of the alpha tensor is . Its contraction with the Levi-Civita symbol is
by incompressibility and vanishing averages of total derivatives. Every antisymmetric second-rank tensor in three dimensions is detected by this contraction, so the coefficient is a symmetric matrix. The proof needs no Fourier analysis.
// Target: fluid-mechanics.bigb
Turbulent magnetic pumping is an effective transport of the mean magnetic field produced by correlations in inhomogeneous or anisotropic turbulence. Its contribution to the mean-field electromotive force is . In the mean induction equation this enters as , the same algebraic form as advection by a velocity . Thus it supplements the mean material velocity without requiring an equal mean mass flow. Downward pumping can help retain or couple fields in a solar dynamo.
For the ideal magnetic response to a cylindrical cyclonic event, the plane-integrated -component of at duration is
This follows from and azimuthal integration. If boundary terms vanish, integration by parts gives the equivalent form . For on , zero outside, the response is
The value at zero is its continuous limit zero. It is initially , but changes sign repeatedly at the nonzero roots of , with oscillatory envelope of order . The flow's kinetic helicity density is , showing that the sign of a finite-duration ideal response is not fixed by the instantaneous helicity sign.
A space-time average over periodic modes integrates over the spatial periodic cell and one temporal period. For real spatial Fourier modes sharing a wavevector, . A matching sine or cosine temporal factor supplies another . Opposite wavevectors can have nonzero spatial cross averages, so their temporal coefficients must be checked rather than discarded merely because the wavevectors are distinct.

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