<strong>Liquid</strong> <strong><strong>in</strong>terfaces</strong> <strong>in</strong> <strong>viscous</strong> stra<strong>in</strong><strong>in</strong>g <strong>flows</strong> 185(a)0.100.08h0.060.04(h c – h)/h c10 010 –110 –210 –5 10 –4(b)0.0210 –310 –6010 –610 210 –4 10 –2 10 0(Q c – Q)/Q c10 –3 10 –2 10 –1 10 010 110 010 0κ10 –1(k c – k)/k c10 010 –210 –210 –6 10 –4 10 –210 –1 (Q c – Q)/Q c10 –310 –6 10 –4 10 –2 10 0(Q c – Q)/Q cFigure 4. Evolution of the calculated steady-state hump shape with withdrawal flux Q.The model parameters are S =0.2 and p 0 =0.01. We f<strong>in</strong>d the transition flow rate to beQ c =0.0731094. Us<strong>in</strong>g fits to the numerical data at this flow rate, we f<strong>in</strong>d that the hump heighth c =0.09680 and the hump curvature κ c =76.453. (a) Humpheighth vs. Q c − Q/Q c . The <strong>in</strong>setshows (h c − h)/h c approaches saturation as √ (Q c − Q)/Q c .(b) Mean curvature κ at hump tipversus Q. The <strong>in</strong>set shows (κ c − κ)/κ c approaches saturation as √ (Q c − Q)/Q c . The dashedl<strong>in</strong>e depicts a square-root power law.This suggests there exists an <strong>in</strong>termediate critical shape perturbation that neitherdecays nor grows upwards, but simply rema<strong>in</strong>s steady over time (figure 5a). Thiscritical shape perturbation would correspond to an unstable hump solution.Figure 5(b) illustrates the evolution of the hump curvature as a function of theflow rate for stable and unstable hump solutions. At low withdrawal flux values,
186 M. Kle<strong>in</strong>e Berkenbusch, I. <strong>Cohen</strong> and W. W. Zhang(a)(b)κUnstable humpUnstable steady state solutionκ cStable humpNo hump solutionStable steady state solutionQ cQFigure 5. (a) Stable and unstable hump solutions <strong>in</strong> steady-state selective withdrawal. (b)Saddle-node bifurcation diagram illustrat<strong>in</strong>g the evolution of the hump curvature <strong>in</strong> thenselective withdrawal regime.only a very large shape perturbation can cause the <strong>in</strong>terface to be drawn <strong>in</strong>to thes<strong>in</strong>k, we therefore expect the stable and the unstable hump shapes to be widelyseparated. This means the unstable hump must lie close to the s<strong>in</strong>k and, as a result,has a very curved tip. At moderate withdrawal flux values, the perturbation sizerequired to destabilize the hump solution becomes smaller, imply<strong>in</strong>g that the unstableand stable solutions now lie closer to each other. Concurrently, the curvature of thestable solution <strong>in</strong>creases, and the curvature of the unstable solution decreases. Neartransition, even a small perturbation causes the <strong>in</strong>terface to become unstable andgrow towards the s<strong>in</strong>k. This suggests the two solutions lie very close each other andare nearly identical. Therefore it is reasonable to expect the two solutions to becomeidentical, or co<strong>in</strong>cide, at Q c , thereby br<strong>in</strong>g<strong>in</strong>g about a saddle-node bifurcation of thehump solution. The square-root scal<strong>in</strong>g corresponds to a smooth merg<strong>in</strong>g of the twosolutions, so that the κ(Q) curve at Q c has the shape of a parabola ly<strong>in</strong>g on its side.The scal<strong>in</strong>g dynamics associated with how the hump solution saturates as Qapproaches Q c is consistent with a saddle-node bifurcation at Q c .Thisisagenericmechanism for transition to one type of solution from another <strong>in</strong> a dynamicalsystem with only a few degrees of freedom and suggests that the dynamics of theentire <strong>in</strong>terface is coupled. However, the quantitative analysis <strong>in</strong> figure 4 shows anatypical feature: the hump height and curvature saturate towards the f<strong>in</strong>al scal<strong>in</strong>gbehaviour at very different δq values. Specifically, the square-root scal<strong>in</strong>g <strong>in</strong> h c − his evident throughout its evolution, even at large δq. In contrast, the square-rootscal<strong>in</strong>g for κ c − κ becomes evident only when δq has decreased below 10 −3 .Thisbehaviour suggests the hump shape does not approach the transition uniformly. Totest this idea, we plot the hump radius at z = h/2 as a function of Q (figure 6). Wef<strong>in</strong>d that the radius at the half-height saturates to the f<strong>in</strong>al scal<strong>in</strong>g behaviour laterthan h, but earlier than κ as δq approaches 0. This behaviour <strong>in</strong>dicates that, as Qapproaches Q c , the overall shape of the hump, e.g. the hump height or its lateral extent,saturates first, followed by features on smaller length scales. The shape of the hump atits tip, which corresponds to a feature on the smallest length scale, saturates last. Thiscascade of events is more typical of an approach towards a s<strong>in</strong>gular shape, <strong>in</strong> whichfeatures evolv<strong>in</strong>g on different length scales are nearly decoupled, so that features onsmaller length scales saturate later than features on large length scales.To obta<strong>in</strong> some <strong>in</strong>sight <strong>in</strong>to this unusual hybrid character of the <strong>in</strong>terface evolutionnear transition, we plot κ as a function of h (figure 7). At Q = 0, the <strong>in</strong>terface shape