Set and , so and . Away from , the logarithmic derivative givesFor , and . The Taylor–Goldstein equation residual divided by consequently simplifies toThus the neutral mode of the equal-width Hazel model requiresThe qualifier “solution” needs care at the critical level of an internal gravity wave . For , and : it is a solution separately on either side, not a classical smooth eigenfunction across the critical level of an internal gravity wave. A branch for negative is also needed. For example, a limit from assigns on .
The critical-layer regularity of a neutral Hazel mode further gives local finite horizontal kinetic energy only for , since incompressible flow gives and then converges. At , and is smooth after the removable quotient is continued. At , and the formal profile does not decay at infinity, so it fails the remote endpoint condition. These qualifications prevent interpreting the whole closed parameter interval as a family of classical decaying modes.
For the equal-width Hazel model with stable density stratification ,The Miles–Howard theorem therefore excludes exponentially growing regular normal modes for . The candidate neutral modes of the equal-width Hazel model instead lie onThe parabola touches the sufficient-stability threshold at its maximum. There is no contradiction: neutrality has , whereas the proof in part (a) assumes . Moreover, the profile has a singular critical-layer derivative and logarithmically divergent horizontal kinetic energy; it is not a regular growing mode satisfying the proof's hypotheses.
For , the local gradient Richardson number condition permits instability but does not establish it. Substitution of a neutral ansatz alone also does not determine on which side of the curve unstable eigenvalues lie. It identifies the formal neutral curve; concluding a full stability boundary requires additional continuation analysis of the eigenvalues. The nondecaying endpoint and the smooth endpoint have the distinct qualifications described above.
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