Let and suppose a growing normal mode has , taking without loss of generality. Since never vanishes on the real channel, choose a continuous square-root branch and write . Direct differentiation givesSubstitution into the Taylor–Goldstein equation and division by givesThus the required transformation isThe impermeable walls give , hence . Multiply by , integrate across the channel, and use integration by parts. With the boundary term zero, the resulting power-transformed Taylor–Goldstein energy identity isBoth and are real. Since and , its imaginary part, divided by , isIf everywhere, the integrand is nonnegative and the first two terms have positive integral for any nonzero mode. This contradicts the identity. Therefore instability requiresThis is the necessary instability condition of the Miles–Howard theorem. Where , it says that the gradient Richardson number must be below somewhere. It is not a sufficient condition for instability, and the conclusion concerns exponential normal-mode growth, not exclusion of the algebraic lift-up effect in part (a). The algebra uses the given nondimensional ; in dimensional notation its counterpart is the squared buoyancy frequency.
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