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Differential Equations and Nonlinear Mechanics
Volume 2008 (2008), Article ID 135982, 11 pages
Research Article

Numerical Simulation of the Field Velocities and Local Disturbances of a Long Gravity Wave Passing above an Immersed Vertical Barrier

Department of Mathematics, University of Annaba, P.O. Box 12, 23000 Annaba, Algeria
Department of Physics, University of Annaba, P.O. Box 12, 23000 Annaba, Algeria

Received 20 October 2007; Revised 21 July 2008; Accepted 26 August 2008

Academic Editor: Roger Grimshaw

Copyright © 2008 Laouar Abdelhamid and Guerziz Allaoua. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.


This work is interested in the study of the passage of a long gravity wave above an immersed vertical barrier. The latter is placed at a right angle in the middle of the occupied fluid domain which is limited vertically by both a free surface and an impermeable horizontal bottom. We want to determine the field velocity and the local disturbances in the vicinity of the barrier. For this, we use the generalized theory of shallow water and complex variables method. For illustration, we consider a solitary wave as an emitted long wave.

1. Introduction

The problem of the passage of gravity waves above an immersed obstacle was studied by several authors (cf. [15]). Thus we mention some results already obtained in this field. Dean's work [2] is classified in the theory of the short waves; it concerns particularly the determination of the coefficients of reflection and transmission of the waves passing a completely immersed obstacle (e.g., a barrier). Gulli [4] has studied a same type of obstacle but in the case of the long waves and he has concluded, at the first order of approximation, that there is not a reflected wave by the obstacle. The studies of Seabra-Santos et al. [5] concern the deformation and the dephasing of the free surface in shallow water due to the solitary mutual interactions or with an isolated obstacle. The theoretical and experimental contributions of Barthélemy et al. [1] concern the phenomena resulting from the internal long waves. In [6], the study of a passage of a long wave over vertical barrier, Germain's shallow water theory associated with the complex variable method has been used to determine the flow.

Our objective in the present paper is to apply the shallow water theory and complex variable method in order to determine the local disturbances at the vicinity of the obstacle and simulate the velocity field. So, we would like to know particularly with accuracy the kinematic of the flow at the vicinity of the obstacle while the passage of the long gravity wave above the thin immersed vertical barrier. For illustration, we consider a solitary wave generated at the upstream by a piston wave maker.

The plan of this paper is as follows. Section 2 contains two parts: the first part describes the phenomenon, the second part gives general equations and mathematical model. Section 3 gives a determination of the system of equations and the technique of resolution. The last section presents an application and a numerical simulation.

2. Position of the Problem

2.1. Description of the Phenomenon

We consider a fixed 𝑂𝑥𝑦 reference system, where the axis 𝑂𝑦 is vertically ascendant and the axis 𝑂𝑥 coincides with the initial free surface. The position of the fluid particle at the moment 𝑡, 𝑡>0, is denoted by (𝑥,𝑦) and their coordinates at the initial position by (𝑎,𝑏), where 𝑎, 𝑏, and 𝑡 are the variables of Lagrange. Now we introduce new components 𝑋 and 𝑌 as follows: 𝑋(𝑎,𝑏,𝑡)=𝑥(𝑎,𝑏,𝑡)𝑎,𝑌(𝑎,𝑏,𝑡)=𝑦(𝑎,𝑏,𝑡)𝑏.(2.1) The assumption of the shallow water theory (see [3]) introduces distortion space and temporal variables, translating the difference in scale between the horizontal and vertical sizes. This distortion will be characterized by the small parameter which is dependent on the relative long wave amplitude. Thus 𝛼=𝜀𝑎,𝛽=𝑏,𝜏=𝜀𝑔𝑡,(2.2) where 𝑔 represents the critical celerity of the propagated long waves ( and 𝑔 are depth of fluid at rest and gravity, resp.).

The description of the phenomenon is as follows: we consider the domain 𝐷 occupied by fluid of an infinite horizontal band which is limited vertically by a free surface 𝛽=0 and an impermeable horizontal bottom 𝛽=. A vertical, thin, and impermeable barrier is placed in the middle of the occupied fluid at right angle to the bottom. The top of the barrier is defined by (𝛼=0; 𝛽=𝑙). A data long wave 𝑋𝑒(𝛼𝜏) emitted upstream passes above the obstacle by creating local disturbances in its vicinity (see Figure 1).

Figure 1: Local disturbances at vicinity of the barrier.
2.2. General Equations and Mathematical Model

General equations and mathematical model are listed below: (i)the kinematic condition expresses the incompressibility of fluid𝜕𝑌𝜕𝛽+𝜀𝜕𝑋+𝜕𝛼𝜕𝑋𝜕𝛼𝜕𝑌𝜕𝛽𝜕𝑋𝜕𝛽𝜕𝑌𝜕𝛼=0;(2.3)(ii)the dynamic condition for an irrotational movement𝜕2𝑋𝜕𝛽𝜕𝜏+𝜀𝜕𝑋𝜕𝜕𝛼2𝑋𝜕𝛽𝜕𝜏𝜕𝑋𝜕𝜕𝛽2𝑋+𝜕𝛼𝜕𝜏𝜕𝑌𝜕𝜕𝛼2𝑌𝜕𝛽𝜕𝜏1+𝜕𝑌𝜕𝜕𝛽2𝑌𝜕𝛼𝜕𝜏=0;(2.4)(iii)the impermeability boundary conditions𝜕𝑌𝜕𝜕𝛼+𝜀2𝑋𝜕𝜏2+𝜀2𝜕𝑋𝜕𝜕𝛼2𝑋𝜕𝜏2+𝜕𝑌𝜕𝜕𝛼2𝑌𝜕𝜏2=0atthefreesurface(𝛽=0),𝑌(𝛼,𝛽,𝜏)=0,atthebottom(𝛽=),𝑋(𝛼,𝛽,𝜏)=0,ontheobstacle;(2.5)(iv)the initial conditions𝑋(𝛼,𝛽,)=0,𝑌(𝛼,𝛽,)=0(atrest).(2.6) The resolution of (2.3)–(2.6) requires that the solutions take into account the interaction fluid-obstacle. According to the shallow water theory (see Germain [3]), the solution will be calculated under the entire series in 𝜀: 𝑋(𝛼,𝛽,𝜏)=𝑛=1𝜀𝑛𝑋𝑛,0(𝛼,𝛽,𝜏)+𝑚=1𝑋𝑛,𝑚(𝛼,𝛽,𝜏)exp𝑚𝜆𝛼𝜀,𝑌(𝛼,𝛽,𝜏)=𝑛=1𝜀𝑛𝑌𝑛,0(𝛼,𝛽,𝜏)+𝑚=1𝑌𝑛,𝑚(𝛼,𝛽,𝜏)exp𝑚𝜆𝛼𝜀,(2.7)where 𝜆 is a determining constant.

The double sum (𝑚0) in the formula (2.7) characterizes the local disturbances whose amplitude decreases exponentially with the distance. The technique of resolution consists to inject these series in the general equations and to write that they are satisfied with the order (𝑛,𝑚) desired. For example, at the first order of approximation (i.e., 𝑛=1), the components 𝑋𝑛,𝑚 and 𝑌𝑛,𝑚 for 𝑚=0 are given as 𝑋1,0(𝛼,𝛽,𝜏)=𝑋1,0𝑌(𝛼,𝜏),1,0(𝛼,𝛽,𝜏)=0,(2.8) and for any 𝑚0,𝑋1,𝑚(𝛼,𝛽,𝜏)=𝐴1,𝑚𝑌(𝜏)cos𝑚𝜆𝛽,1,𝑚(𝛼,𝛽,𝜏)=𝐴1,𝑚(𝜏)sin𝑚𝜆𝛽.(2.9)

3. Local Disturbances (Case the Obstacle is a Barrier)

3.1. System of Equations

At the first order of approximation (𝑛=1), we will calculate the coefficient of the local disturbances. for this, we process as follows. We divide the domain 𝐷 into two parts 𝐷={𝛽0;𝛼<0} and 𝐷+={𝛽0;𝛼>0} (see Figure 2). On each domain 𝐷 or 𝐷+, according to the point of view of Lagrange, the horizontal and vertical components of the displacement of particle (𝑋1, 𝑌1) and (𝑋+1, 𝑌+1), respectively, can be written as follows:𝐷𝑋1(𝛼,𝛽,𝜏)=𝑋𝑒(𝛼𝜏)+𝑚=1𝐴1,𝑚(𝜏)cos𝑚𝜆𝛽exp𝑚𝜆𝛼𝜀,𝑌1(𝛼,𝛽,𝜏)=𝑚=1𝐴1,𝑚(𝜏)sin𝑚𝜆𝛽exp𝑚𝜆𝛼𝜀,𝐷(3.1)+𝑋+1(𝛼,𝛽,𝜏)=𝑋𝑒(𝛼𝜏)+𝑚=1𝐴+1,𝑚(𝜏)cos𝑚𝜆+𝛽exp𝑚𝜆+𝛼𝜀,𝑌+1(𝛼,𝛽,𝜏)=𝑚=1𝐴+1,𝑚(𝜏)sin𝑚𝜆+𝛽exp𝑚𝜆+𝛼𝜀.(3.2)𝐴1,𝑚𝐴+1,𝑚 and 𝜏 are unknown functions depending on the variable 𝐷, characterizing the amplitude of local disturbances in the domains 𝐷+ and 𝜆, respectively, and 𝜆+ and 𝜆+=𝜆=𝜆=𝜋/ are given coefficients (we take here (1,𝑚)). We note that the approximation equations of the phenomenon have been written at the first order of approximation 𝐷+.

Figure 2: Domains 𝐷 and 𝑋1(0,𝛽,𝜏)=𝑋+1𝑌(0,𝛽,𝜏),𝛼=0,𝛽0,(3.3a)1(0,𝛽,𝜏)=𝑌+1𝑋(0,𝛽,𝜏),𝛼=0,𝑙𝛽0,(3.3b)+1(0,𝛽,𝜏)=0,𝛼=0,𝛽𝑙.(3.3c).

Both the continuity conditions of the flow at the border of the two domains and the impermeability condition of the barrier imply that 𝐴1,𝑚(𝜏)=𝐴+1,𝑚(𝜏)=𝐴1,𝑚(𝜏).(3.4)[𝛼=0;𝑙𝛽0]𝑚=1𝐴1,𝑚(𝜏)sin𝑚𝜋𝛽𝑋=0,𝛼=0,𝑙𝛽0,(3.5)𝑒(𝜏)+𝑚=1𝐴1,𝑚(𝜏)cos𝑚𝜋𝛽=0,𝛼=0,𝑙𝛽0.(3.6) The condition (3.3a) applied to (3.1) and (3.2) gives the equality 𝑋𝑒(𝜏)0 The latter expresses the symmetry of the local disturbances at the vicinity of the barrier.

The continuity conditions (3.3a) and (3.3b) of the flow on the segment 1+𝑚=1𝑎1,𝑚cos𝑚𝜋𝛽=0,(3.7)where𝑎1,𝑚=𝐴1,𝑚(𝜏)𝑋𝑒(𝜏)isaconstant.(3.8) give the following equations:1+𝑚=1𝑎1,𝑚cos𝑚𝜋𝛽=0,𝛼=0,𝛽𝑙,𝑚=1𝑎1,𝑚sin𝑚𝜋𝛽=0,𝛼=0,𝑙𝛽0.(3.9)𝑎1,𝑚 By considering the linearity of (3.6), if 𝐷+, we have𝑋+1The problem leads us to solve the following system:𝑌+1Thus the coefficients 𝑧=(𝛼/𝜀𝑖𝛽) are obtained starting from these two time-independent equations.

3.2. Technique of Resolution

In the domain 𝑓+𝛼𝜀𝑖𝛽=1+𝑚=1𝑎1,𝑚𝜋exp𝑚𝛼𝜀𝑖𝛽.(3.10), we consider two relations (3.2) of the components 𝐷+ and 𝛽=0 and (3.8). We can then construct an analytic complex variable function 𝛽= such that𝑌+(𝛼,𝛽)=Im𝑓+𝛼𝜀𝑖𝛽=0,ontheboundaries𝛽=0,𝛽=,(3.11)This function bounded in the domain 𝑋+(𝛼,𝛽)=Re𝑓+𝛼𝜀𝑖𝛽=0,onthesegment(𝛼=0;𝛽𝑙).(3.12) except at the singular points satisfies the impermeability condition at the free surface 𝐷 and the bottom 𝑧=𝛼/𝜀𝑖𝛽. Therefore, 𝑓𝛼𝜀𝑖𝛽=1+𝑚=1𝑎1,𝑚𝑚𝜋exp𝛼𝜀𝑖𝛽.(3.13) and the impermeability condition of the barrier leads to 𝑓+𝛼𝜀𝑖𝛽=𝑓𝛼𝜀𝛼𝑖𝛽=𝑓𝜀𝑖𝛽.(3.14) In the same way, we build in 𝑎1,𝑚 a second analytical complex variable function 𝑓 as follows:{<𝛼<+;𝛽0}The continuity conditions at the border of the two domains and by the analytical extension allow the following equality:{𝛼=0;𝛽𝑙}The determination of local disturbances 𝛼Im𝑓𝜀𝛼𝑖𝛽=0,ontheboundaries𝛽=0,𝛽=,Re𝑓𝜀𝑓𝛼𝑖𝛽=0,on[𝛼=0;𝛽𝑙],𝜀𝑖𝛽equaltounityatinnity.(3.15) leads to find a function 𝛿=(cos(𝜋𝑙/2))1, analytical in the domain (𝑧) without the segment (𝜁). This function is bounded in this domain except at the singularity point. Furthermore, it verifies the following restrictions:=20cm According to [6], we can obtain a conform transformation of this domain on the superior half-plane (see Figure 3) and seek an analytic function satisfying the conditions on the boundaries in the later. We find, in particular, the value of 𝑙=10cm (see [6]).

Figure 3: Transformation of the plane 𝜀=0.6. on the half plane =20cm.
Figure 4: The field velocity 𝑙=10cm, 𝜀=0.6., and 𝑧=𝜋ln(𝜁21tan(𝜋𝑙/2)𝜁21+tan(𝜋𝑙/2)),(3.16)
Figure 5: The local disturbances 𝜁=1+tan2𝜋𝑙2coth2𝜋𝑧2.(3.17), 𝐻(𝜁)=𝑓(𝑧), and A3

By using the formula of Schwarz-Christofel [6], the conform transformation is written asIm[𝐻(𝜁)]=0,onthesegment[A6,A1];[A1,A2],Re[𝐻(𝜁)]=0,onthesegment[A2,A3];[A3,A4],Im[𝐻(𝜁)]=0,onthesegment[A4,A5];[A5,A6].(3.18)and its inverse transformation is1𝐻(𝜁)=(sin(𝜋𝑙/2)𝜁21𝜁),(3.19)The function 𝑧 is holomorphic in the superior half-plane and also bounded except at the point 𝑓𝛼𝜀𝑖𝛽={sin𝜋𝑙21+tanh(𝜋/2)(𝛼/𝜀𝑖𝛽)tan(𝜋𝑙/2)2}1.(3.20). On the real axis, this function verifies the following conditions:𝑎1,𝑚By applying the formula of Signorini [6], we find the function𝛼=0and returning to the 𝑓(𝑖𝛽)=2cos(𝜋𝛽/2)cos(𝜋𝛽/)cos(𝜋𝑙/).(3.21)-plane using (3.17), we finally find𝑓(𝑖𝛽)=1+𝑚=1𝑎1,𝑚cos𝑚𝜋𝛽+𝑖sin𝑚𝜋𝛽,(3.22)This function describes the full flow in particular the field of the disturbances in the vicinity of the barrier. The coefficients 𝑎1,𝑚 can be calculated easily. In fact on the vertical [,0]., the function (3.20) is𝑎1,𝑚=20𝑓(𝑖𝛽)cos𝑚𝜋𝛽𝑑𝛽.(3.23) Furthermore the relations (3.10) to (3.14) permit the function𝑎1,𝑚=𝑃𝑚cos𝜋𝑙+𝑃𝑚1cos𝜋𝑙,(3.24)where the coefficients 𝑃𝑚 are obtained by using the Fourier series expansion on the interval 𝑃𝑚1

It follows that𝑚Thus𝑚1 where 𝑃𝑚 and 𝑃𝑚cos𝜋𝑙=21.3.5(2𝑚1)2.4.62𝑚cos𝑚𝜋𝑙+1𝑚1(2𝑚1)cos(𝑚2)𝜋𝑙+1.3𝑚(𝑚1)1.2(2𝑚1)(2𝑚3)cos(𝑚4)𝜋𝑙.+(3.25) are the Legendre polynomials of degree 𝐷 and 𝑋1(𝛼,𝛽,𝜏)=𝑋𝑒(𝛼𝜏)+𝑋𝑒(𝜏)𝑚=1𝑎1,𝑚cos𝑚𝜋𝛽||𝛼||exp𝑚𝜋,𝑌𝜀1(𝛼,𝛽,𝜏)=𝑋𝑒(𝜏)𝑚=1𝑎1,𝑚sin𝑚𝜋𝛽||𝛼||exp𝑚𝜋,𝜀(3.26), respectively, in the third integral representation.

The 𝑋1 formula is given below:𝑌1 Using (3.1), (3.2), (3.4), (3.8), and (3.14), the horizontal and vertical components of the displacement of the flow, in all domain 𝑋1(𝛼,𝛽,𝜏), can be written as follows:𝑌1(𝛼,𝛽,𝜏)where 𝑋𝑒(𝛼𝜏) and 𝜏=0 are, respectively, the horizontal and vertical components of the displacement of the particle.

Remark 3.1.According to (3.1), (3.2), and (3.26), one notices that displacements 𝜏=𝜏0 and 𝑋𝑒3(𝛼𝜏)=𝜀1tanh4𝛼𝜏𝜏0.(4.1) are the independent contributions of the parts “wave” and “local disturbances” of the flow. On the first order of approximation, the part “wave” of the flow imposes a uniform distribution of displacements and speeds on a vertical. The part “disturbances local” permits to take into account the presence of the obstacle.

4. Application

For illustration, we consider as an example a solitary wave (see [5]) 𝛽 which is emitted at the upstream at time 𝑡 and arrives exactly above the barrier at time 𝑢1: 𝑣1 Now, we calculate the velocity field and the local disturbances of the flow. We observe that the horizontal displacement is independent of the variable 𝑢1=34𝜀2𝑔1tanh234𝛼𝜏𝜏0+34𝜀2𝑔×1tanh234𝜏𝜏0𝑚=1𝑎1,𝑚cos𝑚𝜋𝛽||𝛼||exp𝑚𝜋,𝑣𝜀1=34𝜀2𝑔1tanh234𝜏𝜏0𝑚=1𝑎1,𝑚sin𝑚𝜋𝛽||𝛼||exp𝑚𝜋.𝜀(4.2) in accordance with the theory of long gravity waves.

The derivative of the expression (3.26) with respect to 𝑢1(𝛼,𝛽)=𝑢1(𝛼,𝛽) gives the horizontal and vertical components, respectively, 𝑣1(𝛼,𝛽)=𝑣1(𝛼,𝛽) and 𝑢1 of the velocity field𝑣1 We observe that the horizontal (vertical) components of the velocity is symmetric, that is, 𝑢1=34𝜀2𝑔1tanh234𝜏𝜏0𝑚=1𝑎1,𝑚cos𝑚𝜋𝛽||𝛼||exp𝑚𝜋,𝑣𝜀1=34𝜀2𝑔1tanh234𝜏𝜏0𝑚=1𝑎1,𝑚sin𝑚𝜋𝛽||𝛼||exp𝑚𝜋.𝜀(4.3) (resp., antisymmetric, i.e., 𝑢1).

From (4.2), we deduce the horizontal and vertical components, respectively, 𝑣1 and 𝑢1=𝑐(𝜏)𝑢1𝑣(𝛼,𝛽),1=𝑐(𝜏)𝑣1(𝛼,𝛽),(4.4) of the field local disturbances3𝑐(𝜏)=4𝜀2𝑔1tanh234𝜏𝜏0,𝑢1(𝛼,𝛽)=𝑚=1𝑎1,𝑚cos𝑚𝜋𝛽||𝛼||exp𝑚𝜋,𝑣𝜀1(𝛼,𝛽)=𝑚=1𝑎1,𝑚sin𝑚𝜋𝛽||𝛼||exp𝑚𝜋.𝜀(4.5)The components 𝑐(𝜏) and 𝑡=𝑡0 can be written as=20cmwhere𝑙=10cmEquations (4.4) show that the coefficient 𝜀=0.6 intervenes only as a parameter of scale of the local disturbances (i.e., the kinematic of the flow remains unchanged qualitatively whatever the position of the wave relatively to the barrier). Naturally the intensity of the local disturbances is maximum at the moment 38cm/s.

4.1. Numerical Simulation

The numerical simulation is realized on the Apollo station by using the subprogram of the Legendre polynomials. The data used are 103, 104, and . The maximum velocity of incident flow is approximately . We note that the series (3.26) converge slowly, for this, we have used 5 terms. The criterion of convergence is the impermeability condition of the barrier (i.e., the norm of the horizontal component remains within a specified tolerance ).

The graphical representation of the field of velocity and the local disturbances are given, respectively.

The shallow water theory at the first order of approximation permits to determine in a simple way the velocity field and the local disturbances when the interaction of a solitary wave occurs with an isolated obstacle. The numerical simulation illustrates the flow at the vicinity of the barrier and shows, in particular, the zone of the influence of the local disturbances.

In a future work, we intend to study the problem by using the shallow water theory at the second order of approximation in order to consider, further, the effects of the reflected wave on the kinematic flow barrier.


The work simulation is realized in the Computer Center of the Laboratoire des Ecoulements Géophysiques et Industriels (L.E.G.I), Joseph Fourier University of Grenoble (France).


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