<?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.2015.51005</article-id><article-id pub-id-type="publisher-id">OJMS-53014</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>
 
 
  Relationship between Sea Surface Single Carrier Waves and Decreasing Pressures of Atmosphere Lower Boundary
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>aika</surname><given-names>Augustin</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>Mbane</surname><given-names>Biouele César</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</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><author-notes><corresp id="cor1">* E-mail:<email>cesar.mbane@yahoo.fr(MBC)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>22</day><month>12</month><year>2014</year></pub-date><volume>05</volume><issue>01</issue><fpage>45</fpage><lpage>54</lpage><history><date date-type="received"><day>13</day>	<month>October</month>	<year>2014</year></date><date date-type="rev-recd"><day>28</day>	<month>October</month>	<year>2014</year>	</date><date date-type="accepted"><day>8</day>	<month>November</month>	<year>2014</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>
 
 
  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. To allow a better understanding of the behavior of rogue waves associated with tornadoes in terms of their origin, the nonlinear theory of off-balance systems is developed in the specific case of strong agitations constantly seen on the surface of extensive and deep rivers, when they are crossed by an atmosphere’s low pressure system (tornadoes, cyclones, hurricanes, etc.). A mathematical model based on the Navier-Stokes and Euler Lagrange equations coupled with assumptions derived from instrumental registrations on the training locations (or birth places) of freak waves is developed to enhance the physics of processes responsible for the formation (or origin) of the waves associated with atmosphere’s low pressure systems. Freak waves births’ constraints are mainly the need for both consistent water (
  i.e.
  ,
   
  extensive-deep rivers) and potential velocity flow availabilities. Numerical simulations, based on the use of the NLSE (Nonlinear Schrodinger Equation) are performed
   
  to validate our mathematical model on the births of single carrier waves associated with atmosphere’s low pressure systems.
 
</p></abstract><kwd-group><kwd>Nonlinear Theory of Off-Balance Systems</kwd><kwd> Births of Single Carrier Waves Associated with  Atmosphere’s Low Pressure Systems</kwd><kwd> NLSE (Nonlinear Schrodinger Equation)</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>The existence of rogue waves is now universally recognized [<xref ref-type="bibr" rid="scirp.53014-ref1">1</xref>] - [<xref ref-type="bibr" rid="scirp.53014-ref21">21</xref>] and many 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.53014-ref22">22</xref>] -[<xref ref-type="bibr" rid="scirp.53014-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 tornadoes in terms of their origin and spatio- temporal evolution, that is, their motion and also in terms of mechanical transformations that these systems may suffer in their dealings with other systems, the nonlinear physics of off-balance systems is developed in the specific case of strong agitations constantly seen on the surface of extensive and deep rivers, when they are crossed by an atmosphere’s low pressure system (tornadoes, cyclones, hurricanes, etc.). 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 physics of processes responsible for the formation (or origin) of the waves associated with atmosphere’s low pressure systems. Indeed, Navier-Stokes and Euler Lagrange equations provide evidence that waves may form on the surface of water as a reaction to impact of the decreasing pressures of the atmosphere lower boundary. It is precisely in this case, the materialization of action triggers reaction Physics’ Principle and then of a manifestation among many others of the evidence of Atmosphere-Oceans coupling. The rogue waves births’ constraints are mainly the need for both consistent water (i.e., extensive-deep rivers) and potential velocity flow domain. Numerical simulations, based on the use of the NLSE (nonlinear Schr&#246;dinger equation) on amplitude and phase modulations are performed to validate our mathematical model on the births of rogue waves associated with atmosphere’s low pres- sure systems.</p></sec><sec id="s2"><title>2. Kinematics’ Constraints Associated with Births of Tornadoes’ (or Cyclones’) Rogue Waves</title><p>The general fluid continuity equation is given by:</p><disp-formula id="scirp.53014-formula1558"><label>(1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-1470167x6.png"  xlink:type="simple"/></disp-formula><p>This leads to the continuity equation for an incompressible fluid</p><disp-formula id="scirp.53014-formula1559"><label>(2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-1470167x7.png"  xlink:type="simple"/></disp-formula><p>The kinematic boundary conditions</p><disp-formula id="scirp.53014-formula1560"><label>(3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-1470167x8.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-1470167x9.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/5-1470167x10.png" xlink:type="simple"/></inline-formula> is the sea surface elevation. Hence:</p><disp-formula id="scirp.53014-formula1561"><label>(4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-1470167x11.png"  xlink:type="simple"/></disp-formula><p>Equation of motion in natural coordinates</p><disp-formula id="scirp.53014-formula1562"><label>(5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-1470167x12.png"  xlink:type="simple"/></disp-formula><p>For an inviscid fluid, Equation (5) is simplify to</p><disp-formula id="scirp.53014-formula1563"><label>(6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-1470167x13.png"  xlink:type="simple"/></disp-formula><p>When the flow is irrotational, one can write</p><disp-formula id="scirp.53014-formula1564"><label>(7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-1470167x14.png"  xlink:type="simple"/></disp-formula><p>The related velocity potential is so given by</p><disp-formula id="scirp.53014-formula1565"><label>(8)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-1470167x15.png"  xlink:type="simple"/></disp-formula><p>The continuity equation in regard to irrotational flow</p><disp-formula id="scirp.53014-formula1566"><label>(9)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-1470167x16.png"  xlink:type="simple"/></disp-formula><p>The kinematic boundary condition at the bottom of irrotational flow</p><disp-formula id="scirp.53014-formula1567"><label>(10)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-1470167x17.png"  xlink:type="simple"/></disp-formula><p>The kinematic boundary condition at the surface of the same flow</p><disp-formula id="scirp.53014-formula1568"><label>(11)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-1470167x18.png"  xlink:type="simple"/></disp-formula><p>Integrating Equation (6) with respect to<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-1470167x19.png" xlink:type="simple"/></inline-formula>, leads to Bernoulli equation. Arbitrary functions of integration<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-1470167x20.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-1470167x21.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-1470167x21.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-1470167x22.png" xlink:type="simple"/></inline-formula>must be the same function<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-1470167x21.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-1470167x22.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-1470167x23.png" xlink:type="simple"/></inline-formula>, which can be absorbed by the velocity</p><p>potential, yielding exactly the same flow</p><disp-formula id="scirp.53014-formula1569"><label>(12)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-1470167x24.png"  xlink:type="simple"/></disp-formula><p>where, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-1470167x25.png" xlink:type="simple"/></inline-formula>is the density of liquid water; <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-1470167x25.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-1470167x26.png" xlink:type="simple"/></inline-formula>the sea-level dynamic pressure and P<sub>0</sub> the sea-level static pressure.</p><p>Due to the smallest-vertical extend of oceans with regard to earth’s radius, we can consider <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-1470167x27.png" xlink:type="simple"/></inline-formula> constant throughout it <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-1470167x27.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-1470167x28.png" xlink:type="simple"/></inline-formula> making the gravitational force conservative and able to derive from a potential energy through- out the ocean. We can also neglect the surface tension.</p><p>When atmosphere’s low pressure systems (LOW on <xref ref-type="fig" rid="fig1">Figure 1</xref>) cross the ocean: The atmosphere low boundary decreasing pressures field above the ocean replaces <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-1470167x29.png" xlink:type="simple"/></inline-formula> in Equation (12).</p><fig id="fig1"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref></label><caption><title> LOW (low pressure systems) and HIGH (higher pressure system) on a mean sea-level pressure (millibars) map</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/5-1470167x30.png"/></fig><p>And then, taking <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-1470167x31.png" xlink:type="simple"/></inline-formula> constant and equal to 0 at<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-1470167x31.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-1470167x32.png" xlink:type="simple"/></inline-formula>, gives Formula (13) which describes the geometry of ocean’s surface single carrier waves:</p><disp-formula id="scirp.53014-formula1570"><label>(13)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-1470167x33.png"  xlink:type="simple"/></disp-formula><p>Formula (13) is our mathematical model on the occurrence of oceans’ surface single carrier waves associated with atmosphere’s low pressure systems (i.e., the mainly origin of tornadoes; cyclones or hurricanes related waves).</p><p>- <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-1470167x34.png" xlink:type="simple"/></inline-formula>is the sea surface temperature;</p><p>- <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-1470167x35.png" xlink:type="simple"/></inline-formula>is the sea-level decreasing pressure below atmosphere’s low pressure systems (Figures 2(a)-(d));</p><p>- <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-1470167x36.png" xlink:type="simple"/></inline-formula>is the sea-level static pressure<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-1470167x36.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-1470167x37.png" xlink:type="simple"/></inline-formula>.</p><p>According to Formula (13), the height of single carrier waves depends mainly on low pressure deepest. i.e.,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-1470167x38.png" xlink:type="simple"/></inline-formula>.</p></sec><sec id="s3"><title>3. Implementation of NLSE</title><p>According to the nonlinear Schr&#246;dinger equation (NLSE), the combination of unstable waves can trigger a sin- gle wave which can reach up to three or five times the amplitude of the single carrier waves (that is, the wave energy is basically concentrated in a single wave number). Let’s consider a surface wave whose main compo-</p><p>nent <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-1470167x39.png" xlink:type="simple"/></inline-formula> is of the form<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-1470167x39.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-1470167x40.png" xlink:type="simple"/></inline-formula>, then Benjamin-Feir integral equation developed in [<xref ref-type="bibr" rid="scirp.53014-ref3">3</xref>] for this type of wave has the form:</p><disp-formula id="scirp.53014-formula1571"><label>(14)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-1470167x41.png"  xlink:type="simple"/></disp-formula><p>We consider the case of energy concentrated mainly around two-wave numbers</p><disp-formula id="scirp.53014-formula1572"><label>(15)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-1470167x42.png"  xlink:type="simple"/></disp-formula><p>where A and B satisfy the Coupled Nonlinear Schr&#246;dinger Equations [<xref ref-type="bibr" rid="scirp.53014-ref22">22</xref>] :</p><disp-formula id="scirp.53014-formula1573"><label>(16)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-1470167x43.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.53014-formula1574"><label>(17)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-1470167x44.png"  xlink:type="simple"/></disp-formula><p>Here, we took into account that the energy distribution is almost monochromatic and the Taylor expansion of the pulse around the two wave numbers.</p><p>If the energy concentrated mainly around a wave number, the evolution of a waveform produced by a group unstable wave only on the nonlinear Schrodinger equation is:</p><disp-formula id="scirp.53014-formula1575"><label>(18)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-1470167x45.png"  xlink:type="simple"/></disp-formula><p>Putting the previous relation (18) under the dimensionless form, we obtain the nonlinear Schr&#246;dinger equation rewrites in the form [<xref ref-type="bibr" rid="scirp.53014-ref23">23</xref>] [<xref ref-type="bibr" rid="scirp.53014-ref24">24</xref>] :</p><disp-formula id="scirp.53014-formula1576"><label>(19)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-1470167x46.png"  xlink:type="simple"/></disp-formula><p>This is an integrable equation. We can find solution which form is:</p><disp-formula id="scirp.53014-formula1577"><label>(20)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-1470167x47.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-1470167x48.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-1470167x48.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-1470167x49.png" xlink:type="simple"/></inline-formula> are both arbitrary functions. We assume that <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-1470167x48.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-1470167x49.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-1470167x50.png" xlink:type="simple"/></inline-formula> is real function.</p><fig-group id="fig2"><label><xref ref-type="fig" rid="fig2">Figure 2</xref></label><caption><title> (a) Barograph Trace showing the passage of an immature hurricane at low latitude. The sea-level pressure drops from reference index_<sub>30</sub> to index_<sub>28.50</sub>; (b) Barograph Trace accompanying the passage of a small, intense hurricane. The sea- level pressure drops from reference index_<sub>30</sub> to index_<sub>28.00</sub>; (c) Barograph Trace indicating the passage of a mature hurricane. The ground surface pressure drops from reference index_<sub>30</sub> to index_<sub>27.30</sub>; (d) One of the deepest barometer readings for the entire world. The ground surface pressure drops from reference index_<sub>30</sub> to index_<sub>27.00</sub>, Hurricane “Janet”_Ghetumal (Mexico) Barograph Trace.</title></caption><fig id ="fig2_1"><label>(b)</label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/5-1470167x51.png"/></fig><fig id ="fig2_2"><label>(c)</label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/5-1470167x52.png"/></fig><fig id ="fig2_3"><label>(d)</label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/5-1470167x53.png"/></fig><fig id ="fig2_4"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/5-1470167x54.png"/></fig></fig-group><p>Substitution of (20) in (19), gives (21):</p><disp-formula id="scirp.53014-formula1578"><label>(21)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-1470167x55.png"  xlink:type="simple"/></disp-formula><p>We are interested in a homoclinic orbit to the fixed point and we obtain finally the solution (22):</p><disp-formula id="scirp.53014-formula1579"><label>(22)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-1470167x56.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.53014-formula1580"><label>(23)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-1470167x57.png"  xlink:type="simple"/></disp-formula><p>Below is an exact analytical solution of Equation (19):</p><disp-formula id="scirp.53014-formula1581"><label>(24)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-1470167x58.png"  xlink:type="simple"/></disp-formula><p>with <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-1470167x59.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-1470167x59.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-1470167x60.png" xlink:type="simple"/></inline-formula>.</p><p>Relation (24) can reach to a family of spatiotemporal solutions of breather type with the advantage that they describe the plane wave. The rational solitons’ family can be transform to Peregrine breather type of solution:</p><disp-formula id="scirp.53014-formula1582"><label>(25)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-1470167x61.png"  xlink:type="simple"/></disp-formula></sec><sec id="s4"><title>4. Results and Discussion</title><p>According to scientists’ common opinion, questions raised by observations lead to physics’ laws while observations can in no way serve as physics’ laws. Indeed, advance equipment like powerful computer; sophisticated WIS (Weather Information Systems); Wind’s Profilers; Radar Drones; Lidar Drones; Satellites, etc., cannot completely solve problems regarding the adverse effects of climate change without the contributions of performing mathematical models on physics of processes responsible of that climate change. Earth’s ecosystem is considerably modified by adverse effects of climate change and this irreversible process reveals human beans vulnerability vis-&#224;-vis of phenomenon like rogue waves; landslides; coastal cities floods, etc. Geometries of sea surface carrier waves associated with atmosphere low pressure systems are drawn on Figures 3(a)-(c) and <xref ref-type="fig" rid="fig4">Figure 4</xref>. Taking into account the Barograph Traces, one can see that the atmosphere low pressure systems can take more than two days to cross a Weather Station. Barograph traces also show that the deepest of impacts on sea- level pressure depends on many weather’s parameters. Figures 3(a)-(c) represent carrier-waves for different wave numbers. Single carrier waves Interferences (or combinations) are shown on <xref ref-type="fig" rid="fig4">Figure 4</xref>. The resulting wave (<xref ref-type="fig" rid="fig4">Figure 4</xref>) reveals that Interferences are mainly constructive in the case of sea-surface carrier waves. On <xref ref-type="fig" rid="fig5">Figure 5</xref>(a) and <xref ref-type="fig" rid="fig5">Figure 5</xref>(b), one can see lands’ and oceans’ tornadoes respectively. Overland Tornadoes are daily phe- nomena (<xref ref-type="fig" rid="fig5">Figure 5</xref>(a)) which occur only during sunny days due to additional greenhouse effects [<xref ref-type="bibr" rid="scirp.53014-ref26">26</xref>] [<xref ref-type="bibr" rid="scirp.53014-ref27">27</xref>] . The same thermodynamics’ process occurs over oceans even by night (<xref ref-type="fig" rid="fig5">Figure 5</xref>(b)) and in this case, it escapes to vi- gilance of weather alert instruments and represents a higher risk for airline pilots as well as seamen’s. This is, according to Mbane’s previous publications [<xref ref-type="bibr" rid="scirp.53014-ref26">26</xref>] -[<xref ref-type="bibr" rid="scirp.53014-ref28">28</xref>] , the main reason why many planes have disappeared when crossing oceans by night. There is convincing evidence that Air France and Malaysian Airlines planes are recent victims of nightly oceans’ tornadoes epiphenomenon.</p></sec><sec id="s5"><title>5. Conclusion</title><p>Many avenues of scientific research (including ours) are now open to better understand the physics, structure, composition and functioning of atmosphere lower pressure systems and their impacts on oceans, mainly in the case of rogue waves’ implementation. Indeed, Earth’s atmosphere is in contact with the oceans, oceans affect it, but in return it acts upon them: We speak of oceans-atmosphere coupling. To study the physics of rogue waves associated by tornadoes (cyclones or hurricanes) in terms of their origin, the nonlinear physics of off-balance systems has been developed in the specific case of strong agitations constantly seen on the surface of extensive and deep rivers, when these rivers are crossed by an atmosphere’s low pressure system. Euler-Lagrange and</p><fig-group id="fig3"><label><xref ref-type="fig" rid="fig4">Figure 4</xref></label><caption><title> Simulations of geometry of oceans’ surface multispectral carrier wave associated with atmosphere low pressure systems shown on <xref ref-type="fig" rid="fig5">Figure 5</xref>(b).</title></caption><fig id ="fig3_1"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/5-1470167x62.png"/></fig><fig id ="fig3_2"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/5-1470167x63.png"/></fig><fig id ="fig3_3"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/5-1470167x64.png"/></fig><fig id ="fig3_4"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/5-1470167x65.png"/></fig></fig-group><fig-group id="fig4"><label><xref ref-type="fig" rid="fig5">Figure 5</xref></label><caption><title> (a)-(b) Tornadoes 3D-profiles ((a), above the land; (b), above the ocean). One may note that: Tornadoes can occur even by night on the Oceans (b) and represent in this case a higher risk for aircrafts. This thermodynamics’ process is impossible by night on the Land (due to land’s thermal inertia).</title></caption><fig id ="fig4_1"><label> (b)</label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/5-1470167x66.png"/></fig><fig id ="fig4_2"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/5-1470167x67.png"/></fig></fig-group><p>Navier-Stokes equations have provide evidence that waves may form on the surface of water as a reaction to impacts of sea-level decreasing pressures of the atmosphere lower boundary. That is precisely the materializa- tion of action triggers reaction Physics’ Principle and then of a manifestation among many others of the convinc- ing evidence of Atmosphere-Oceans coupling. A mathematical model based on the Navier-Stokes equations coupled with assumptions derived from advance data bases on rogue waves has been developed to allow a better understanding of processes responsible for the formation (or origin) of sea surface waves. The rogue waves births’ constraints are mainly the need for availability of both consistent water (i.e., extensive-deep rivers) and potential velocity flow. Numerical simulations, based on NLSE (nonlinear Schr&#246;dinger equation) on amplitude and phase modulations has been successfully performed to validate our relationship between sea-surface strong agitations and decreasing pressure of atmosphere lower boundary.</p></sec><sec id="s6"><title>NOTES</title></sec></body><back><ref-list><title>References</title><ref id="scirp.53014-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Touboul, J., Kharif, C., Pelinovsky, E. and Giovanangeli, J.P. 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