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For a temporally unstable base flow, the relevant saddle growth rate along a ray distinguishes two cases in the chosen observation frame:A convective hydrodynamic instability amplifies a travelling wave packet but lets a localized disturbance decay at any fixed point. An absolute hydrodynamic instability grows at a fixed point. The separating case $\sigma (0)=0$ is marginal in exponential rate and can have an algebraic prefactor. In a frame moving with $V$, replace $\sigma (0)$ by $\sigma (V)=\mathrm{Im}({\omega }_{\star }-V{k}_{\star })$: this distinction depends on the observation frame.

The dispersion relation gives the zero-group velocity saddleThus the absolute growth rate is $\sigma (0)=\mu -U^2/[4(1+c_d^2)]$. More generally the saddle growth rate along a ray isso a frame travelling at $V=U$ sees the maximal rate $\mu$.

For $U>0$, the three open regions areThe line $\mu =0$ is the temporal marginal boundary; the parabola $\mu =U^2/[4(1+c_d^2)]$ is the convective-to-absolute boundary. The Green function of the linear complex Ginzburg-Landau equation has the prefactor $t^{-1/2}$, so zero exponential rate on the latter boundary still allows algebraic decay of the impulse response. This is the stability diagram of the linear complex Ginzburg-Landau equation.