scholarly journals Steep capillary-gravity waves in oscillatory shear-driven flows

2009 ◽  
Vol 640 ◽  
pp. 131-150 ◽  
Author(s):  
SHREYAS V. JALIKOP ◽  
ANNE JUEL

We study steep capillary-gravity waves that form at the interface between two stably stratified layers of immiscible liquids in a horizontally oscillating vessel. The oscillatory nature of the external forcing prevents the waves from overturning, and thus enables the development of steep waves at large forcing. They arise through a supercritical pitchfork bifurcation, characterized by the square root dependence of the height of the wave on the excess vibrational Froude number (W, square root of the ratio of vibrational to gravitational forces). At a critical valueWc, a transition to a linear variation inWis observed. It is accompanied by sharp qualitative changes in the harmonic content of the wave shape, so that trochoidal waves characterize the weakly nonlinear regime, but ‘finger’-like waves form forW≥Wc. In this strongly nonlinear regime, the wavelength is a function of the product of amplitude and frequency of forcing, whereas forW<Wc, the wavelength exhibits an explicit dependence on the frequency of forcing that is due to the effect of viscosity. Most significantly, the radius of curvature of the wave crests decreases monotonically withWto reach the capillary length forW=Wc, i.e. the lengthscale for which surface tension forces balance gravitational forces. ForW<Wc, gravitational restoring forces dominate, but forW≥Wc, the wave development is increasingly defined by localized surface tension effects.

Progressive, irrotational gravity waves of constant form, with all crests in a wave train identical, exist as a two-parameter family. The first parameter, the ratio of mean depth to wavelength, varies from zero (the solitary wave) to infinity (the deep-water wave). The second parameter, the wave height or amplitude, varies from zero (the infinitesimal wave) to a limiting value dependent on the first parameter. Solutions of limiting waves, with angled crests, have been presented in a previous paper; this paper considers near-limiting waves having rounded crests with a very small radius of curvature, in some cases as little as 0.0001 of the water depth. The com puting method is a modification of the integral equation technique used for limiting waves. Two leading terms are again used to give a close approxim ation to the flow near the crest and hence minimize the num ber of subsequent terms needed; the form of these leading terms is suggested by earlier work of G. G. Stokes ( Mathematical and physical papers , vol. 1, pp. 225-228. Cambridge University Press (1880)), M. A. G rant ( J.F luid Mech. 59, 257-262 (1973)) and L. W. Schwartz Fluid Mech. 62, 553-578 (1974)). To achieve satisfactory accuracy, however, it is now necessary to add a set of dipoles above the crest in the complex potential plane, as previously used by M. S. Longuet-Higgins & M .J . H. Fox ( J. Fluid Mech. 80, 721-741 (1977)). The results include the first fully detailed calculations of non-breaking waves having local surface slopes exceeding 30°. The local profile at the crest, despite its very small scale, is shown to tend with increasing wave height to the asymptotic self-similar form previously com puted by Longuet-Higgins & Fox. Their predictions of an ultim ate m aximum slope of 30.37° and a vertical crest acceleration of 0.388g are supported. The results agree well with earlier calculations for steep waves at the two extremes of solitary and deep-w ater waves. In particular, it is confirmed that in the approach to limiting height the phase velocity and certain integral quantities possess not only the well-known m aximum but also a subsequent minimum, the first in the infinite series of extrema predicted theoretically by M. S. Longuet-Higgins & M .J . H. Fox ( J. Fluid Mech . 85, 769-786 (1978)). Briefly considered also are the level of action of near-limiting deep-w ater waves, the decay of surface drift velocity from the limiting value and the method established for com puting waves of all lesser heights.


1979 ◽  
Vol 90 (1) ◽  
pp. 161-178 ◽  
Author(s):  
R. H. J. Grimshaw

A Helmholtz velocity profile with velocity discontinuity 2U is embedded in an infinite continuously stratified Boussinesq fluid with constant Brunt—Väisälä frequency N. Linear theory shows that this system can support resonant over-reflexion, i.e. the existence of neutral modes consisting of outgoing internal gravity waves, whenever the horizontal wavenumber is less than N/2½U. This paper examines the weakly nonlinear theory of these modes. An equation governing the evolution of the amplitude of the interface displacement is derived. The time scale for this evolution is α−2, where α is a measure of the magnitude of the interface displacement, which is excited by an incident wave of magnitude O(α3). It is shown that the mode which is symmetrical with respect to the interface (and has a horizontal phase speed equal to the mean of the basic velocity discontinuity) remains neutral, with a finite amplitude wave on the interface. However, the other modes, which are not symmetrical with respect to the interface, become unstable owing to the self-interaction of the primary mode with its second harmonic. The interface displacement develops a singularity in a finite time.


Wave Motion ◽  
2020 ◽  
pp. 102702
Author(s):  
M.A. Manna ◽  
S. Noubissie ◽  
J. Touboul ◽  
B. Simon ◽  
R.A. Kraenkel

2000 ◽  
Author(s):  
Hsien-Hung Wei ◽  
David S. Rumschitzki

Abstract Both linear and weakly nonlinear stability of a core annular flow in a corrugated tube in the limit of thin film and small corrugation are examined. Asymptotic techniques are used to derive the corrugated base flow and corresponding linear and weakly nonlinear stability equations. Interesting features show that the corrugation interaction can excite linear instability, but the nonlinearity still can suppress such instability in the weakly nonlinear regime.


2006 ◽  
Vol 18 (3) ◽  
pp. 171-176 ◽  
Author(s):  
Xiao-Bo CHEN ◽  
Wen-Yang DUAN ◽  
Dong-Qiang LU

1994 ◽  
Vol 258 ◽  
pp. 115-129 ◽  
Author(s):  
Michael S. Longuet-Higgins ◽  
R. P. Cleaver

It is shown theoretically that the crest of a steep, irrotational gravity wave, considered in isolation, is unstable. There exists just one basic mode of instability, whose exponential rate of growth β equals 0.123(g / R)½, where g denotes gravity and R is the radius of curvature at the undisturbed crest. A volume of water near the crest is shifted towards the forward face of the wave; the ‘toe’ of the instability is at a horizontal distance 0.45R ahead of the crest. The instability may represent the initial stage of a spilling breaker. On small scales, the ‘toe’ may be a source of parasitic capillary waves.


2008 ◽  
Vol 315 (1-3) ◽  
pp. 136-146 ◽  
Author(s):  
Y. Leong Yeow ◽  
Christopher J. Pepperell ◽  
Firdaus M. Sabturani ◽  
Yee-Kwong Leong

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