<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">OJMS</journal-id><journal-title-group><journal-title>Open Journal of Marine Science</journal-title></journal-title-group><issn pub-type="epub">2161-7384</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/ojms.2016.61009</article-id><article-id pub-id-type="publisher-id">OJMS-63231</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Earth&amp;Environmental Sciences</subject></subj-group></article-categories><title-group><article-title>
 
 
  Numerical Simulation of Water Waves’ Modulational Instability under the Effects of Wind’s Stress and Gravity Force Relaxation
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>héodule</surname><given-names>Nkoa Nkomom</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>César</surname><given-names>Mbane Biouele</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Jeannot</surname><given-names>Mane Mane</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref></contrib></contrib-group><aff id="aff1"><addr-line>Laboratory of Earth’s Atmosphere Physics, Department of Physics, University of Yaoundé I, Yaoundé, Cameroun</addr-line></aff><aff id="aff2"><addr-line>Ecole Nationale Supérieure Polytechnique (National Advanced School of Engineering), Department of Mathematics and Physical Sciences, University of Yaoundé I, Yaoundé, Cameroon</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>cesar.mbane@yahoo.fr(CMB)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>22</day><month>12</month><year>2015</year></pub-date><volume>06</volume><issue>01</issue><fpage>93</fpage><lpage>102</lpage><history><date date-type="received"><day>28</day>	<month>December</month>	<year>2015</year></date><date date-type="rev-recd"><day>accepted</day>	<month>26</month>	<year>January</year>	</date><date date-type="accepted"><day>29</day>	<month>January</month>	<year>2016</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p>
 
 
  The waves driven by the wind do not move on the water as ordinarily done by sailboats. Indeed, the movement of the waves driven by the wind is more complex than the sailboats’ translation movement that we know. The movement of the wave in our particular case results from the chain-job done by wind’s stress and gravity forces: material is collected upstream (erosion phenomenon) and then deposited on the wave’s summit by the wind. This material deposited on the summit of the wave by the wind is then removed and dispatched on the downstream side of the wave by gravity forces. As always happens in any chain-job: if the wind works faster than gravity forces, great accumulation of material will occur at the summit of the wave that will lead to an increase in its (the wave in this case) height. If conversely the wind works more slowly, a deficit in material delivery will occur and gravity force goes directly to remove material on the wave’s summit and lead to a decrease in its height.
   
  In terms of Mechanics,
   
  we know that the main obstacle that can seriously disturb the work of the wind is the unavailability of water or so its viscosity. Given the complexity of the process to be studied, it seemed necessary for us to make a use of modulational instability theories such as the standard NLSE in order to better understand the contribution of wind and water viscosity to modulations of driven waves’ amplitudes (or phases): modulations which sometimes can accidentally trigger unpredictable rogue waves.
 
</p></abstract><kwd-group><kwd>Waves Driven by the Wind</kwd><kwd> Standard Nonlinear Schr&#246;dinger Equation</kwd><kwd> Modulations of Driven Waves’ Amplitudes or Phases</kwd><kwd> Unpredictable Rogue Waves</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Descriptions of unusually high waves appearing on the sea surface for a short time (freak, rogue or killer waves) have been considered as a part of marine folklore for a long time. A number of instrumental registrations have appeared recently making the community to pay more attention to this problem and to reconsider known observations of freak waves whose existences are now universally recognized [<xref ref-type="bibr" rid="scirp.63231-ref1">1</xref>] -[<xref ref-type="bibr" rid="scirp.63231-ref21">21</xref>] . Furthermore, images on the extent of damage caused by these monsters of the ocean are available. However, the physics of processes responsible for the formation (or origin) and propagation of these phenomena as well as their prediction is not completely understood. Contrary to developed country researchers’ opinion, physics of spectacular phenomenon like rogue waves is not easily obtainable by the only use of advance data provided by high technology equipment like: Powerful Computers; sophisticated WIS (Weather Information Systems); Wind’s Profilers; Radar Drones; Lidar Drones; Satellites; etc. Indeed, rogue waves are a combination of multi-spectral processes that occur under the thermodynamic and dynamic accuracy conditions. Mathematical models [<xref ref-type="bibr" rid="scirp.63231-ref22">22</xref>] -[<xref ref-type="bibr" rid="scirp.63231-ref25">25</xref>] offer more tremendous opportunities for understanding of the systems whose physics is, at the present level of our knowledge, difficult to obtain. To allow a better understanding of the behavior of rogue waves triggered by winds in terms of their origin and spatiotemporal evolution, that is, their motion and also in terms of mechanical transformations that these systems may suffer in their dealings with other systems, the standard nonlinear Schr&#246;dinger equation of off balance systems is implemented in the specific case of waves driven by wind and gravity forces. A mathematical model based on Navier-Stokes and Euler Lagrange equations coupled with assumptions derived from the literature on the nature of the training locations (or birth places) of rogue waves is developed to enhance the wind and gravity force effects on the behavior of surface waves. Given the complexity of the process to be studied, it seemed necessary for us to make a use of modulational instability theories such as the standard NLSE in order to better understand the contribution of wind and water viscosity to modulations of driven waves’ amplitudes (or phases): modulations which sometimes can accidentally trigger unpredictable rogue waves.</p></sec><sec id="s2"><title>2. Navier-Stokes and Euler Lagrange Equations</title><p>The general fluid continuity equation is given by:</p><disp-formula id="scirp.63231-formula533"><label>(1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/9-1470250x7.png"  xlink:type="simple"/></disp-formula><p>This leads to the continuity equation for an incompressible fluid</p><disp-formula id="scirp.63231-formula534"><label>(2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/9-1470250x8.png"  xlink:type="simple"/></disp-formula><p>The kinematic boundary conditions</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-1470250x9.png" xlink:type="simple"/></inline-formula>, at <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-1470250x10.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-1470250x11.png" xlink:type="simple"/></inline-formula> (3)</p><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-1470250x12.png" xlink:type="simple"/></inline-formula> is the unit vector normal to the boundary surfaces and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-1470250x13.png" xlink:type="simple"/></inline-formula> is the sea surface elevation. Hence:</p><p><img src="http://html.scirp.org/file/9-1470250x14.png" />,<img src="http://html.scirp.org/file/9-1470250x15.png" /> (4)</p><p>Equation of motion in natural coordinates</p><disp-formula id="scirp.63231-formula535"><label>(5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/9-1470250x16.png"  xlink:type="simple"/></disp-formula><p>According to (5): solutions of the equation of motion depends mainly on pressure P (closely related to the prevailing winder over the ocean); gravity g and water viscosity (n). Only mathematical models (theories) that incorporate best these different parameters will next be considered.</p></sec><sec id="s3"><title>3. Weakly Nonlinear Approach: The Nonlinear Schr&#246;dinger Equation</title><p>Under the effects of wind and gravity, the wave moves through successive deformations of its surface (<xref ref-type="fig" rid="fig1">Figure 1</xref>). This situation is perfectly described by the Nonlinear Schr&#246;dinger Equation (NLSE) which can be obtained from the fully nonlinear potential theory by using the multi-scale method [<xref ref-type="bibr" rid="scirp.63231-ref1">1</xref>] - [<xref ref-type="bibr" rid="scirp.63231-ref7">7</xref>] . The Taylor developing-series allows the NLSE to be expanded around a small wave steepness ε. Thereafter, the equation obtained is a third order in ε approximation of the system formed by equations 1 to 4. To investigate both damping and amplification effects on the Benjamin-Feir instability, we have use the forced and damped nonlinear Schr&#246;dinger equation (fdNLSE),</p><disp-formula id="scirp.63231-formula536"><label>(6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/9-1470250x17.png"  xlink:type="simple"/></disp-formula><p>Herein, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-1470250x18.png" xlink:type="simple"/></inline-formula>represents the wind effect, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-1470250x19.png" xlink:type="simple"/></inline-formula>is the group velocity of the carrier wave and ν, ρ, ρ<sub>air</sub>, g, u<sub>∗</sub>, and k are well-known parameters [<xref ref-type="bibr" rid="scirp.63231-ref1">1</xref>] - [<xref ref-type="bibr" rid="scirp.63231-ref12">12</xref>] . Equation (6) describes the spatial and temporal evolution of the envelope of the surface elevation<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-1470250x20.png" xlink:type="simple"/></inline-formula>, for weakly nonlinear and dispersive gravity waves on deep water when dissipation (due to viscosity), and amplification (due to wind), are considered. If considering the right hand side of this equation, it can be rewritten as</p><disp-formula id="scirp.63231-formula537"><label>(7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/9-1470250x21.png"  xlink:type="simple"/></disp-formula><p>The stability of the envelope depends on the sign of K. For values of K ˂ 0, solutions are found to be stable, while for values of K ≥ 0, solutions are unstable. Physically, they interpreted this result in terms of frequency of the carrier wave ω<sub>0</sub> and friction velocity u<sub>∗</sub> of the wind over the waves. We plotted (<xref ref-type="fig" rid="fig2">Figure 2</xref> &amp; <xref ref-type="fig" rid="fig3">Figure 3</xref>) the critical curve separating stable envelopes from unstable envelopes. Namely, they showed that for a given friction velocity u<sub>∗</sub>, only carrier wave of frequency ω<sub>0</sub> which satisfies the following condition are unstable to modulational perturbations</p><disp-formula id="scirp.63231-formula538"><label>(8)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/9-1470250x22.png"  xlink:type="simple"/></disp-formula><fig id="fig1"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref></label><caption><title> Driven wave’s velocity profile [<xref ref-type="bibr" rid="scirp.63231-ref1">1</xref>] </title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/9-1470250x23.png"/></fig><fig id="fig2"  position="float"><label><xref ref-type="fig" rid="fig2">Figure 2</xref></label><caption><title> Growth rate versus of the wave number of the perturbation k for positive values of K (A<sub>0</sub> = 0.2 and θ = 35)</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/9-1470250x24.png"/></fig><fig id="fig3"  position="float"><label><xref ref-type="fig" rid="fig3">Figure 3</xref></label><caption><title> Growth rate versus of the wave number of the perturbation k for negative values of K (A<sub>0</sub> = 0.2 and θ = 35)</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/9-1470250x25.png"/></fig><p>We can transform this Equation (8) to have a standard nonlinear Schr&#246;dinger equation in 3D.</p><disp-formula id="scirp.63231-formula539"><label>(9)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/9-1470250x26.png"  xlink:type="simple"/></disp-formula><p>And then introduce an oblique coordinates (S) associated with the direction of the spatial modulation</p><disp-formula id="scirp.63231-formula540"><label>(10)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/9-1470250x27.png"  xlink:type="simple"/></disp-formula><p>Substuting Equation (10) and (9) in (8) we obtain:</p><disp-formula id="scirp.63231-formula541"><label>(11)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/9-1470250x28.png"  xlink:type="simple"/></disp-formula><p>K values are very small and this make possible to do Taylor expansion in first order of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-1470250x29.png" xlink:type="simple"/></inline-formula> and obtain (12)</p><disp-formula id="scirp.63231-formula542"><label>(12)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/9-1470250x30.png"  xlink:type="simple"/></disp-formula><p>Taking <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-1470250x31.png" xlink:type="simple"/></inline-formula></p><p>Moving from the NLS equation to the standard NLS become possible if <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-1470250x32.png" xlink:type="simple"/></inline-formula> is a linear</p><p>function in T. We can therefore consider the following new variable:</p><disp-formula id="scirp.63231-formula543"><label>(13)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/9-1470250x33.png"  xlink:type="simple"/></disp-formula><p>And obtain</p><disp-formula id="scirp.63231-formula544"><label>(14)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/9-1470250x34.png"  xlink:type="simple"/></disp-formula><p>Therefore</p><disp-formula id="scirp.63231-formula545"><label>(15)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/9-1470250x35.png"  xlink:type="simple"/></disp-formula><p>where</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-1470250x36.png" xlink:type="simple"/></inline-formula>and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-1470250x36.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-1470250x37.png" xlink:type="simple"/></inline-formula> (16)</p><p>As said before, wave trains are unstable to small perturbation of other wave travelling in the same direction [<xref ref-type="bibr" rid="scirp.63231-ref2">2</xref>] . The standard stability analysis consist in linearizing around the monochromatic wave solution of the nonlinear Schr&#246;dinger equation</p><disp-formula id="scirp.63231-formula546"><label>(17)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/9-1470250x38.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.63231-formula547"><label>(18)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/9-1470250x39.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.63231-formula548"><label>(19)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/9-1470250x40.png"  xlink:type="simple"/></disp-formula><p>Here K and Ω referring respectively to the perturbation wave number and frequency of the perturbation amplitude. Substituting this equation in Equation (8) we obtain the growth rate of instability:</p><disp-formula id="scirp.63231-formula549"><label>(20)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/9-1470250x41.png"  xlink:type="simple"/></disp-formula><p>It is well known that one of the main effects of Modulational instability, which refers to the growth of certain modulation sideband of nonlinear plane waves propagating in a dispersive medium as deep water is a result of the interplay between nonlinearity, gravity and dispersion effects. In this case of forced/damped regime in deep water, instability is significantly influenced by K (Figures 4-9). It is seen that the growth rate increases (or decreases)</p><fig id="fig4"  position="float"><label><xref ref-type="fig" rid="fig4">Figure 4</xref></label><caption><title> η = η(S) at: −100 ≤ t ≤ 100</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/9-1470250x42.png"/></fig><fig id="fig5"  position="float"><label><xref ref-type="fig" rid="fig5">Figure 5</xref></label><caption><title> η = η(x, y) at: t = 0; η<sub>max</sub> = 1.8</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/9-1470250x43.png"/></fig><fig id="fig6"  position="float"><label><xref ref-type="fig" rid="fig6">Figure 6</xref></label><caption><title> η = η(x, y) at: t = 10; η<sub>max</sub> = 2.0</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/9-1470250x44.png"/></fig><fig id="fig7"  position="float"><label><xref ref-type="fig" rid="fig7">Figure 7</xref></label><caption><title> η = η(x, y) at: t = 25; η<sub>max</sub> = 4.0</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/9-1470250x45.png"/></fig><fig id="fig8"  position="float"><label><xref ref-type="fig" rid="fig8">Figure 8</xref></label><caption><title> η = η(x, y) at: t = 35;<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-1470250x47.png" xlink:type="simple"/></inline-formula></title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/9-1470250x46.png"/></fig><fig id="fig9"  position="float"><label><xref ref-type="fig" rid="fig9">Figure 9</xref></label><caption><title> η = η(x, y) at: t = 50;<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-1470250x49.png" xlink:type="simple"/></inline-formula></title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/9-1470250x48.png"/></fig><p>with the increasing (decreasing) values of forcing/damping coefficient K. It is evident to say that wind effect destabilize the wave train in deep water in two dimensional directions however the dissipation stabilize the wave train.</p></sec><sec id="s4"><title>4. Conclusion</title><p>The upsurges of abnormally large waves on the sea surface are due to complex physical mechanisms. In this paper, we discuss the modulational instability scenario of a single freak wave formation in 3D (i.e., time-space scales). One of the important properties of an unstable wave packet is the growth rate. Small amplitude modulation theory for the NLS equation predicts a number of interesting features about the nonlinear propagation of initially small amplitude sine wave modulations. One of the most important is shown in Figures 5-7 where carrier-wave’s amplitude increases with respect to t (e.g., when comparing: <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-1470250x50.png" xlink:type="simple"/></inline-formula>to <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-1470250x50.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-1470250x51.png" xlink:type="simple"/></inline-formula> or<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-1470250x50.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-1470250x51.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/9-1470250x52.png" xlink:type="simple"/></inline-formula>. A later time after, the carrier wave’s amplitude modulation escapes from our prediction (we observe the upsurge of amplitude’s modulational instability. e.g., amplitude of the carrier wave at t = 35 (<xref ref-type="fig" rid="fig8">Figure 8</xref>) becomes lesser than amplitude of the same carrier wave at t = 50 (<xref ref-type="fig" rid="fig9">Figure 9</xref>) where 03 complete summits are observed). According to pertinent results obtained in this paper, wind alone cannot easily generate rogue waves; effect of winds combined with other physical mechanisms (e.g., viscosity and gravity force) may provide a fuller explanation of upsurge of freak wave phenomena. As wind blows over the ocean, its momentum is transferred to water molecules located at the surface of the sea. When strong winds (e.g., winds triggered by cyclones) blow in the opposing direction of the ocean current, its intensity might be strong enough to randomly generate rogue waves. Viscosity and gravity force contributions to the behavior of wind’s carrier waves are well described by our adopted weakly nonlinear approach and the related NLSE (Nonlinear Schr&#246;dinger Equation).</p></sec><sec id="s5"><title>Cite this paper</title><p>Th&#233;odule NkoaNkomom,C&#233;sar MbaneBiouele,Jeannot ManeMane, (2016) Numerical Simulation of Water Waves’ Modulational Instability under the Effects of Wind’s Stress and Gravity Force Relaxation. Open Journal of Marine Science,06,93-102. doi: 10.4236/ojms.2016.61009</p></sec><sec id="s6"><title>NOTES</title></sec></body><back><ref-list><title>References</title><ref id="scirp.63231-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Touboul, J., Kharif, C., Pelinovsky, E. and Giovanangeli, J.P. (2008) On the Interaction of Wind and Steep Gravity Wave Groups Using Miles’ and Jeffreys’ Mechanisms. Nonlinear Processes in Geophysics, 15, 1023-1031.  
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