Consider the complex field before taking its real part. Put and . Both components are perpendicular to , so the solenoidal magnetic-field constraint holds. The time-dependent phase obeysbecause and . Moreover , and magnetic stretching is . Thus the changing basis exactly supplies the shear-stretching term. Finally,and acts as . Equating coefficients verifies
Take and first . Remove magnetic diffusion by writing , , whereThen , , and . Equivalently, rescaling time by and replacing by gives the pair used in the question. Its growing WKB approximation isThe complex relative phase follows directly from ; the printed is sufficient for magnitudes but omits that phase.
The phase-averaged magnetic energy is , hence for a nonzero growing-mode componentAt , , so its leading exponential isThe positive quadratic term permits strong amplification before the negative cubic diffusion term dominates. The leading maximum occurs near . Put and . A well-separated late-time growing interval requiresThe first ensures ; the second ensures the WKB condition at the peak, since . For fixed nonzero both follow by taking sufficiently small positive . The peak's leading exponent is , whereas the eventual exponent tends to minus infinity. This is mean-field shearing-wave transient amplification, not sustained dynamo action.
Growth from the initial instant is possible explicitly: choose with . The initial logarithmic energy derivative is when . Growth is not asserted for every initial polarization, for example an identically zero field. If , the amplitudes simply diffuse and the energy is proportional to ; shear can still give algebraic transient amplification of an in-plane field for small diffusivity, but a purely vertical field only decays. Positive diffusivity is essential to the final decay.
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