Multi-symplectic structure of fully-nonlinear weakly-dispersive internal gravity waves

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1 Multi-symplectic structure of fully-nonlinear weakly-dispersive internal gravity waves Didier Clamond, Denys Dutykh To cite this version: Didier Clamond, Denys Dutykh. Multi-symplectic structure of fully-nonlinear weakly-dispersive internal gravity waves. Journal of Physics A: Mathematical and Theoretical, IOP Publishing, 2016, 49, pp.31lt01. < < / /49/31/31LT01>. <hal v2> HAL Id: hal Submitted on 17 Jun 2016 HAL is a multi-disciplinary open access archive for the deposit and dissemination of scientific research documents, whether they are published or not. The documents may come from teaching and research institutions in France or abroad, or from public or private research centers. L archive ouverte pluridisciplinaire HAL, est destinée au dépôt et à la diffusion de documents scientifiques de niveau recherche, publiés ou non, émanant des établissements d enseignement et de recherche français ou étrangers, des laboratoires publics ou privés. Distributed under a Creative Commons ttribution - NonCommercial - NoDerivativesttribution - NonCommercial - NoDerivatives 4.0 International License

2 Didier Clamond Université de Nice Sophia Antipolis, France Denys Dutykh CNRS LAMA, Université Savoie Mont Blanc, France Multi-symplectic structure of fully-nonlinear weakly-dispersive internal gravity waves arxiv.org / hal

3 Last modified: June 17, 2016

4 Multi-symplectic structure of fully-nonlinear weakly-dispersive internal gravity waves Didier Clamond and Denys Dutykh Abstract. In this short communication, we present the multi-symplectic structure for the two-layer Serre Green Naghdi equations describing the evolution of large amplitude internal gravity water waves when both layers are shallow. We consider only a two-layer stratification with rigid bottom and lid for simplicity, generalisations to several layers being conceivable. This multi-symplectic formulation allows the application of various multi-symplectic integrators (such as Euler or Preissman box schemes) that preserve exactly the multi-symplecticity at the discrete level. Key words and phrases: internal waves, two-layer flow, multi-symplectic structure, shallow water, Serre Green Naghdi equations MSC: 2010] 76B55 (primary), 76B15, 76M30 (secondary) PACS: 2010] Bb (primary), N- (secondary) Key words and phrases. internal waves, two-layer flow, multi-symplectic structure, shallow water, Serre Green Naghdi equations. Corresponding author.

5 Contents 1 Introduction Model derivation Ansatz Equations of motion Multi-symplectic structure Conservation laws Momentum flux Energy flux Conclusions and perspectives A Complementary equations Acknowledgments References

6 D. Clamond & D. Dutykh 4 / Introduction The density stratification in oceans exists due, mainly, to the dependence of the water density on temperature and salinity 14]. The density stratification supports the so-called internal waves. These are ubiquitous in the ocean and, comparing to surface waves, internal waves may have a huge amplitude of the order of hundreds of meters 13]. These waves play an important role in ocean dynamics and they attract permanent attention of several scientific communities. Compared to surface gravity waves, the physics of internal waves is richer and their modelling leads to more complicated equations, in general (see the reviews 1, 20] for more information). Lagrangian and Hamiltonian formalisms are tools of choice in theoretical physics, in particular for studying nonlinear waves. Quite recently, the multi-symplectic formalism have been proposed as an attractive alternative. This formulation generalises the classical Hamiltonian structure to partial differential equations by treating space and time on the equal footing 5]. Multi-symplectic formulations are gaining popularity, both for mathematical investigations and numerical modelling 7, 19]. Multi-symplectic formulations of various equations modelling surface waves can be found in the literature. However, to our knowledge, no such formulations have been proposed for internal waves. In this note, we show that the multi-symplectic structure of a homogeneous fluid should be easily extended to fluids stratified in several homogeneous layers. For the sake of simplicity, we focus on two-dimensional irrotational motions of internal waves propagating at the interface between two perfect fluids, bounded below by an impermeable horizontal bottom and bounded above by an impermeable rigid lid. The present article should be considered as a further step in understanding the underlying mathematical structure of an important model of long internal waves the socalled two-layer Serre equations 21] where the thicknesses of the fluid layers are small compared to the characteristic wavelength (shallow layers). Serre s equations are approximations for large amplitude long waves. This model is sometimes referred to as weakly-dispersive fully-nonlinear and was first derived by Serre for surface waves 21]. Its generalisation for two layers internal waves was apparently first in the late nineteen eighties 4, 16, 18], both with a rigid lid and with a free surface, and later re-derived using different approaches 2, 3, 9]. The Hamiltonian formulation for the classical Serre equations describing surface waves can be found in 15], for example. However, this structure is non-canonical and quite nontrivial. The two-layer Serre equations also have a non-canonical Hamiltonian structure 2, 11]. In the present study, we propose a multi-symplectic formulation of the two-layer Serre equations with a rigid lid. This work is a direct continuation of 8] where the multi-symplectic structure was proposed for the original Serre equations. The results obtained in this study can be used to propose new structure-preserving numerical schemes to simulate the dynamics of internal waves. Indeed, now it is straightforward to apply the Euler-box or the Preissman-box schemes 19] to two-layers Serre

7 Multi-symplectic structure of long internal waves 5 / 14 Figure 1. Sketch of the two-fluid domain. equations. The advantage of this approach is that such schemes preserve exactly the multisymplectic form at the discrete level 5, 7]. To our knowledge, this direction is essentially open. We are not aware of the existing structure-preserving numerical codes to simulate internal waves. This situation may be explained by higher complexity of these models compared to, e.g. surface waves. The present manuscript is organised as follows. In Section 2, we present a simple variational derivation of the governing equations. Their multi-symplectic structure is provided in Section 3 and the implied conservation laws are given in Section 4. The main conclusions and perspectives of this study are outlined in Section Model derivation We consider a two-dimensional irrotational flow of an incompressible fluid stratified in two homogeneous layers of densities ρ j, subscripts j = 1 and j = 2 denoting the lower and upper layers, respectively. The fluid is bounded below by a horizontal impermeable bottom at y = d 1 and above by a rigid lid at y = d 2, y being the upward vertical coordinate such that y = 0 and y = η(x,t) are, respectively, the equations of the still interface and of the wavy interface (see Figure 1). Here, x denotes the horizontal coordinate, t is the time, g is the downward (constant) acceleration due to gravity and surface tension is neglected. The lower and upper thicknesses are, respectively, h 1 = d 1 +η and h 2 = d 2 η, def such that h 1 + h 2 = d 1 + d 2 := D is a constant. Finally, we denote u j = (u j,v j ) the velocity fields in the j-th layer (u j the horizontal velocities, v j the vertical ones). We derive here the fully-nonlinear weakly-dispersive long wave approximation Serre-like equations 4, 9] following a variational approach initiated in 22] for the (one-layer) classical Serre equations. Further relations are given in the Appendix A.

8 D. Clamond & D. Dutykh 6 / Ansatz In order to model long waves in shallow water with rigid horizontal bottom and lid, the velocity fields in each layer is approximated as u j (x,y,t) ū j (x,t), v j (x,y,t) ( ( 1) j d j y ) ū jx, (2.1) η d 1 u 1 dy, def where ū j is the horizontal velocity averaged over the j-th layer, i.e., ū 1 := h1 1 def ū 2 := h2 1 d2 u η 2 dy. The horizontal velocities u j are thus (approximately) uniform along the layer column and the vertical velocities v j are chosen so that the fluid incompressibility is fulfilled together with the bottom and the lid impermeabilities. With the ansätze (2.1), the vertical accelerations are def { D t v j := v jt + u j v jx + v j v jy γ j h 1 dj ( 1) j y, where D t is the temporal derivative following the motion and γ j are the vertical accelerations at the interface, i.e. γ j def := D t v j y=η ( 1) j h j {ūjxt + ū j ū jxx ū 2 jx. (2.2) The kinetic and potential energies of the liquid column are, respectively, j K def := V def := ˆ η u1 2 ρ +v2 1 1 dy + d 1 2 ˆ η d 1 ρ 1 g(y +d 1 ) dy + ˆ d2 η ˆ d2 η ρ 2 u 2 2 +v2 2 2 dy 2 j=1 ρ j ( 1 h ) 2 jūj h3 j ū2 jx, ρ 2 g(y +d 1 ) dy = 1 2 (ρ 1 ρ 2 )gh ρ 2gD 2. Note that the potential energy is defined relatively to the bottom without loss of generality. The incompressibility of the fluids and the impermeabilities of the lower and upper boundaries being fulfilled, a Lagrangian density L is then obtained from the Hamilton principle: the Lagrangian is the kinetic minus potential energies plus constraints for the mass conservation of each layer, i.e. L def := K V + ρ 1 {h 1t + h 1 ū 1 ] x φ 1 + ρ 2 {h 2t + h 2 ū 2 ] x φ 2, (2.3) where φ j are Lagrange multipliers and with the constraint h 2 = D h 1 being assumed. The latter could be relaxed adding λ(h 1 + h 2 D) (λ another Lagrange multiplier) into the right-hand side of (2.3) 6]. However, we do not do it here in order to handle fewer equations.

9 Multi-symplectic structure of long internal waves 7 / Equations of motion The Euler Lagrange equations for the functional L dxdt yield (together with h 2 = D h 1 and for j = 1,2) δφ j : 0 = h jt + h j ū j ] x, (2.4) δū j : 0 = φ j h jx h j φ j ] x 1 3 h3 j ūjx] x + h j ū j, (2.5) ( δh 1 : 0 = 1 ρ1 ū ρ ) ( 2ū2 2 (ρ1 ρ 2 )gh ρ1 h ū2 1x ρ 2h2 2x) 2 ū2 ρ 1 φ 1t + ρ 2 φ 2t ρ 1 ū 1 φ 1x + ρ 2 ū 2 φ 2x. (2.6) Adding the two equations (2.4) and integrating the result, one obtains h 1 ū 1 + h 2 ū 2 = Q(t), Q being an integration constant (U m def := Q/D is often called mix velocity in the theory of multiphase flows). The relation (2.5) can be rewritten thence φ jx = ū j 1 3 h 1 j h 3 j ūjx] x = ū j 1 3 h2 j ūjxx h j h jx ū jx (j = 1,2), (2.7) h 1 φ 1x + h 2 φ 2x = Q 1 3 h3 1 ū1x + h 3 2 ū2x] x, (2.8) ρ 1 φ 1x ρ 2 φ 2x = ρ 1 ū 1 ρ 2 ū 2 ρ 1 u 1 φ 1x ρ 2 u 2 φ 2x = ρ 1 ū 2 1 ρ 2 ū 2 2 The equation (2.6) then gives ( ρ 1 φ 1t ρ 2 φ 2t = 1 ρ1 h ū1x 2 ρ 2 h2 2 ū2x ρ 1h 1 1 h 3 1 ū1x] x ρ 2h 1 2 h 3 2 ū2x] x, (2.9) 1 3 ρ 1u 1 h 1 1 h 3 1 ū 1x ] x ρ 2u 2 h 1 2 h 3 2 ū 2x ] x. (2.10) ) ( ) 1 ρ1 ū ρ 2 ū2 2 (ρ1 ρ 2 )gh ρ 1ū 1 h 1 1 h 3 1 ū1x] x 1 3 ρ 2ū 2 h 1 2 h 3 2 ū2x] x, (2.11) and eliminating φ j between (2.9) and (2.11), one obtains t { ρ1 ū 1 ρ 2 ū ρ 1h 1 1 h 3 1 ū1x] x ρ 2h 1 2 h 3 2 ū2x] x + x { 1 2 ρ 1ū ρ 2ū (ρ 1 ρ 2 )gh ρ 1h 2 1 ū2 1x ρ 2h 2 2 ū2 2x 1 3 ρ 1ū 1 h 1 1 h 3 1 ū 1x ] x ρ 2ū 2 h 1 2 h 3 2 ū 2x ] x = 0, (2.12) that, physically, is an equation for the conservation of the difference between the tangential momenta at the interface. One can also easily derive a non-conservative equation for the horizontal momentum ρ 1 (ū 1t + ū 1 ū 1x ) ρ 2 (ū 2t + ū 2 ū 2x ) + (ρ 1 ρ 2 )gh 1x ρ 1h 1 1 h 2 1 γ 1 ] x ρ 2h 1 2 h 2 2 γ 2 ] x = 0. (2.13) On the other hand, equations for the momentum and energy fluxes are not easily derived from these equations. This is where a multi-symplectic formulation comes to help.

10 D. Clamond & D. Dutykh 8 / Multi-symplectic structure A system of partial differential equations has a multi-symplectic structure if it can written as a system of first-order equations 5, 17] M z t + K z x = z S(z), (3.1) where a dot denotes the contracted (inner) product, z R n is a rank-one tensor (vector) of state variables, M R n n and K R n n are skew-symmetric rank-two tensors (matrices) and S is a smooth rank-zero tensor (scalar) function depending on z. S is sometimes called the Hamiltonian, though it is generally not a classical Hamiltonian. The multi-symplectic structure for the one-layer Serre equations is already known 8]. This structure can be easily extended to two (and more) layers. The multi-symplectic formulation for one layer involves 8-by-8 matrices. For two layers, we then expect a priori a multi-symplectic formulation with 16-by-16 matrices. However, since we consider a rigid lid, one variable can be eliminated, thus reducing the formulation to 15-by-15. Thus, introducing h 1 = h and h 2 = D h for brevity, we seek for a multi-symplectic structure with z = he 1 + ϕ 1 e 2 + ū 1 e 3 + ṽ 1 e 4 + p 1 e 5 + q 1 e 6 + r 1 e 7 + s 1 e 8 + ϕ 2 e 9 + ū 2 e 10 + ṽ 2 e 11 + p 2 e 12 + q 2 e 13 + r 2 e 14 + s 2 e 15, (3.2) (e i standard unitary basis vectors) and M = ρ 1 (e 1 e 2 e 2 e 1 ) ρ 1(e 1 e 5 e 5 e 1 ) ρ 2 (e 1 e 9 e 9 e 1 ) 1 3 ρ 2(e 1 e 12 e 12 e 1 ), (3.3) K = 1 3 ρ 1(e 1 e 7 e 7 e 1 ) ρ 1 (e 2 e 6 e 6 e 2 ) 1 3 ρ 2(e 1 e 14 e 14 e 1 ) + ρ 2 (e 9 e 13 e 13 e 9 ), (3.4) S = ρ 1 ( 1 6ṽ ū s 1ū 1 ṽ 1 ) h + ρ2 ( 1 6ṽ ū s 2ū 2 ṽ 2 ) (D h) 1 2 (ρ 1 ρ 2 )gh ρ 1p 1 (ū 1 s 1 ṽ 1 ) 1 3 ρ 2p 2 (ū 2 s 2 ṽ 2 ) + ρ 1 q 1 (ū s 1ṽ 1 ) ρ 2 q 2 (ū s 2ṽ 2 ) 1 3 ρ 1r 1 s ρ 2r 2 s 2. (3.5) These two-layer expressions for z, M, K and S are simple duplication of the corresponding expression for one layer 8]. We show below that they indeed lead to the two-layer Serrelike equations derived in the previous Section. Physically, ϕ j are the velocity potentials written at the interface, while φ j are related to the velocity potentials integrated over the fluid layers. Using the velocity potentials at the interface, we obtained rather easily the multi-symplectic structure of the Serrelike equations. Conversely, with the equivalent formulation involving φ j it is difficult, and likely impossible, to obtain a multi-symplectic structure of the Serre-like equations. It is reminiscent of the classical Hamiltonian formulation for finite-depth two-layer flow with a rigid lid, where the weighted difference between the velocity potentials at the interface turns out to be the correct canonical variable 10].

11 Multi-symplectic structure of long internal waves 9 / 14 The substitution of (3.2) (3.5) into (3.1) yields the fifteen equations ρ 1 { ϕ1t p 1t r 1x ρ2 { ϕ2t p 2t r 2x = (ρ1 ρ 2 )gh + ρ 1 { 1 6 ṽ ū ū1ṽ 1 s 1 ρ2 { 1 6 ṽ ū ū2ṽ 2 s 2, (3.6) ρ 1 {h t + q 1x = 0, (3.7) { 0 = ρ 1 q1 h ( ū ṽ1s ) s 1, (3.8) 0 = 1 ρ 3 1{p 1 h(ṽ 1 ū 1 s 1 ) q 1 s 1, (3.9) 1 3 ρ 1h t = 1 3 ρ 1{ṽ 1 s 1 ū 1, (3.10) ρ 1 ϕ 1x = ρ 1 {ū s 1ṽ 1, (3.11) 1 3 ρ 1h x = 1 3 ρ 1s 1, (3.12) 0 = 1 3 ρ 1{r 1 + hū 1 ṽ 1 p 1 ū 1 q 1 ṽ 1, (3.13) ρ 2 {h t + q 2x = 0, (3.14) { 0 = ρ 2 q2 + (D h) ( ū ṽ2s ) s 2, (3.15) 0 = 1 ρ 3 2{p 2 + (D h)(ṽ 2 ū 2 s 2 ) q 2 s 2, (3.16) 1 3 ρ 2h t = 1 3 ρ 2{ṽ 2 s 2 ū 2, (3.17) ρ 2 ϕ 2x = ρ 2 {ū s 2ṽ 2, (3.18) 1 3 2h x = 1 ρ 3 2s 2, (3.19) 0 = 1 ρ 3 2{r 2 (D h)ū 2 ṽ 2 p 2 ū 2 q 2 ṽ 2. (3.20) Twelve of these equations are trivial and can be simplified as (with j = 1,2) q j = ( 1) j 1 h j ū j, p j = ( 1) j 1 h j ṽ j, s j = ( 1) j 1 h jx, r j = ū j p j, ṽ j = ( 1) j 1 (h jt + ū j h jx ), ϕ jx = ū j s jṽ j, the remaining three giving the mass conservation equations (together with h 1 +h 2 = D) h 1t + h 1 ū 1 ] x = 0, h 2t + h 2 ū 2 ] x = 0, (3.21) and, exploiting the relations (3.21), the equation for the tangential momenta at the interface ( ) ( ) ρ 1 ϕ 1t ρ 2 ϕ 2t = 1 ρ1 h ū1x 2 ρ 2 h2 2 ū2x 2 1 ρ1 ū ρ 2 ū ρ 3 1ū 1 h1 1 h1 3 ū1x] x 1 ρ 3 2ū 2 h2 1 h2 3 ū2x] x ρ 1h 2 1 ū 1x ] t 1 3 ρ 2h 2 2 ū 2x ] t (ρ 1 ρ 2 )gh 1. (3.22) One can verify that these equations are equivalent to the ones obtained above. The multi-symplectic structure described above involves the potentials ϕ j that are different from the potentials φ j used to derive Serre-like equations of the section 2. After elimination of φ j and ϕ j, the two systems of equations are identical. Indeed, the differences between these two velocity potentials are from (2.7), (3.17) and (3.21) given by ϕ jx φ jx = 1 h 3 jx(h jt + u j h jx ) h2 j ūjxx + h j h jx ū jx = 1 3 h2 j ū jxx + 2 h ] 3 j h jx ū jx = 1 3 h 2 j ū jx, (3.23) x

12 D. Clamond & D. Dutykh 10 / 14 thence with ϕ j = φ j h2 jūjx substituted into (3.22), the equation (2.11) is recovered. 4. Conservation laws From the multi-symplectic structure, one obtains local conservation laws for the energy and the momentum E t + F x = 0, I t + G x = 0, (4.1) where E(z) = S(z) z x K z, F(z) = 1 2 z t K z, G(z) = S(z) z t M z and I(z) = 1 2 z x M z. For the Serre-like equations, exploiting the results of the previous section and after some algebra, one obtains E = ρ ϕ 1h 1 ū h3 1 ū1ū 1x ]x 1 2 ρ 1h 1 ū ρ 1h 3 1 ū2 1x + ρ ϕ 2h 2 ū h3 2 ū2ū 2x ]x 1 2 ρ 2h 2 ū ρ 2h 3 2 ū2 2x 1 6 ρ 2D h 2 2 ū2ū 2x ]x 1 2 (ρ 1 ρ 2 )gh 2 1, (4.2) F = ρ ϕ 1h 1 ū h3 1 ū 1 ū 1x ] t ρ 1 h 1 ū 1 ( 1 2 ū h2 1 ū 2 1x h 1γ 1 ) ρ ϕ 2h 2 ū h3 2 ū2ū 2x ] t ρ 2 h 2 ū 2 ( 1 2 ū h2 2 ū2 2x 1 3 h 2γ 2 ) ρ 2D h 2 2 ū2ū 2x ]t (ρ 1 ρ 2 )gh 2 1 ū1 + ρ 2 Qφ 2t ρ 2Qū 2 2 ρ 2 Q 1 2 h2 2 ū2ū 2x ]x + 1 ρ 6 2Qh2 2 ū2ū 2xx, (4.3) G = ρ 1 h 1 ū (ρ 2 1 ρ 2 )gh ρ 3 1h1 2 γ 1 + ρ 1 1 ϕ 2 1h h3 1 ū 1x ]t 1 ρ 2 2(h 1 h 2 )ū2 2 1 ρ 3 2h2 2 γ 2 + ρ 1 2 ϕ ] 2 2h h3 2 ū2x t 1 ρ 2 2Dφ 2t + 1 ρ 2 2D h2 2 ū2ū 2x ]x 1 ρ 6 2Dh2 2 ū2ū 2xx, (4.4) I = ρ 1 h 1 ū 1 ρ 1 1 ϕ ] 2 1h h3 1 ū1x 1 ρ x 2 2Dφ 2x + ρ 2 h 2 ū 2 ρ 1 2 ϕ ] 2 2h h3 2 ū2x. (4.5) x Note that these relations involve both ϕ j and φ j in order to handle more compact expressions Momentum flux From the relations (4.4) and (4.5), after simplifications and some elementary algebra, one obtains the equation for the conservation of the momentum 2 j=1 tρ j h j ū j ] + x ρj h j {ū2 j ( 1) j 1 2 gh j ( 1) j 1 3 h jγ j ] = Dρ 2 x φ2t ū2 2 h 2 h 2x ū 2 ū 2x 1 2 h2 2 ū 2 2x 1 3 h2 2 ū 2 ū 2xx gh 2 ], (4.6) and comparison with the equation (A.2) gives an expression for the pressure at the interface P /ρ 2 = K 2 (t) φ 2t 1 2 ū2 2 + h 2h 2x ū 2 ū 2x h2 2 ū2 2x h2 2 ū2ū 2xx + gh 2, (4.7)

13 Multi-symplectic structure of long internal waves 11 / 14 where K 2 (t) is an arbitrary function (integration constant ). The horizontal derivative of this relation, with (2.4) and (2.7), yields after some algebra ] P x /ρ 2 = gh 2x ū 2t ū 2 ū 2x h 1 2 h 2 2 γ 2, (4.8) x that is the upper-layer averaged horizontal momentum equation (A.3), as it should be. We have obtained the Cauchy Lagrange equation (4.7) because we used h = h 1 as main variable for the interface in the multi-symplectic formalism and because we eliminated φ 1 from the equations. Had we instead used h 2 and eliminated φ 2, we would have obtained a Cauchy Lagrange equation for the lower layer. The latter can be easily derived in the form P /ρ 1 = K 1 (t) φ 1t 1 2 ū2 1 + h 1h 1x ū 1 ū 1x h2 1 ū2 1x h2 1 ū1ū 1xx gh 1. The arbitrary functions K j are Bernoulli constants. Their determination requires gauge conditions on φ j and P j (in order to have unequivocal definitions of these quantities) and a precise definition of the mean interface level and of the frame of reference Energy flux From the relations (4.2) and (4.3), after simplifications and some elementary algebra, one obtains the equation for the conservation of the energy flux 2 1 ρ {ū2 2 jh j j h2 j ū2 jx ] ( 1)j gh j + j=1 t x ρ j h j ū j { 1 2 ū2 j h2 j ū2 jx ( 1)j 1 3 h j γ j ( 1) j gh j ] = Qρ 2 x φ2t ū2 2 h 2 h 2x ū 2 ū 2x 1 2 h2 2 ū 2 2x 1 3 h2 2 ū 2 ū 2xx gh 2 ]. (4.9) The right-hand sides of equations (4.6) and (4.9) both involve φ 2. The latter can be eliminated computing D (4.9) Q (4.6), yielding after one integration by parts 2 1 Dρ {ū2 2 jh j j h2 j ū2 jx ] ( 1)j gh j Qρj h j ū j j=1 t + x Dρ j h j ū j { 1 2 ū2 j h2 j ū 2 jx ( 1) j 1 3 h jγ j ( 1) j gh j Qρ j h j {ū2 j ( 1) j 1 2 gh j ( 1) j 1 3 h jγ j ] = dq dt {ρ 1h 1 ū 1 + ρ 2 h 2 ū 2 = ρ 2 Q dq dt 5. Conclusions and perspectives dq dt (ρ 1 ρ 2 )h 1 ū 1. (4.10) We have derived the shallow two-layer Serre-type equations from a variational framework. The main contribution of this study is that we presented their multi-symplectic structure. The rather complicated nonlinear dispersion of the Serre-like equations makes

14 D. Clamond & D. Dutykh 12 / 14 non-trivial the derivation of the multi-symplectic structure, a priori. However, we have shown here that this structure for fluids stratified in several homogeneous layers can be rather easily obtained from the one layer case. For the sake of simplicity, we focused here on two layers in two-dimension with horizontal bottom and lid. Generalisations for three-dimensional several-layer stratifications should be straightforward from the multisymplectic structure of the one-layer three-dimensional Serre equations with a varying bottom. This will be the subject of future investigations. The size of the multi-symplectic structure increases rapidly with the number of layers and the number of spatial dimensions. However, the matrices involved are sparse and most of the equations are algebraically elementary. Thus, the calculus can be achieved easily and straightforwardly with any Computer Algebra System capable of performing symbolic computations. Finding a multi-symplectic structure opens up new directions in the analysis and numerics of equations. In this paper, we illustrate another advantage of the multi-symplectic formalism: it also provides an efficient tool of calculus. Thanks to the multi-symplectic formalism, the conservation laws are obtained automatically, and thus the conserved quantities and their fluxes are obtained as well. The automatic derivation of these conservation laws is an advantage of the multi-symplectic structure. As the main perspective, we would like to mention the structure-preserving numerical simulations of nonlinear internal waves. The proposed multi-symplectic structure can be transposed to the discrete level if one employs a multi-symplectic integrator 7, 19]. These schemes were already rested in complex KdV simulations 12], but this direction seems to be essentially open for internal wave models. A. Complementary equations Multiplying by (y + d 1 ) and (d 2 y) the vertical momentum (full Euler) equation for the lower and upper layers, respectively, and integrating over the layer thicknesses, we have Dv1 ρ 1 (y +d 1 ) d 1 Dt Dv2 ρ 2 (d 2 y) Dt ˆ η ˆ d2 η ] ˆ η + g dy = ] + g dy = (y +d 1 ) P 1 d 1 y dy = h 1 ˆ d2 η (d 2 y) P 2 y dy = h 2 ( P1 P), ( P P2 ), where P is the (unknown) pressure at the interface and P j is the layer-averaged pressure. With the ansätze (2.1) one obtains P j = P + ( 1) j ρ j gh j + ( 1) j ρ j h j γ j, (j = 1, 2).

15 Multi-symplectic structure of long internal waves 13 / 14 Integrating over the layer thicknesses the horizontal momenta, one obtains ˆ η ˆ Du η 1 P )] 1 ρ 1 dy = d 1 Dt d 1 x dy = h 1 ( P P1 h 1 Px, x ˆ d2 ˆ Du d2 2 P )] 2 ρ 2 dy = Dt x dy = h 2 ( P P2 h 2 Px, x η η thence with the ansätze (2.1) (with j = 1,2) h j ū j ] t + ] h j ūj 2 ( 1) j 1 2 gh2 j ( 1) j 1 3 h2 j γ j = x ρ 1 j h j Px. From these relations, we obtain at once (with Q = dq/dt) Q + h 1 ū1 2 + h 2ū2 2 + gdh h2 1 γ h2 2 γ ] 2 = ( ) h x 1 ρ1 1 + h 2 ρ2 1 Px, (A.1) 2 { ρ j h j ū j ] j=1 t + ] h j ūj 2 ( 1) j 1 2 gh2 j ( 1) j 1 3 h2 j γ j = D P x x, (A.2) ū jt + ū j ū jx ( 1) j gh jx ( 1) j 1 3 h 1 j h 2 j γ j ]x = ρ 1 j P x. (A.3) The elimination of P x between the two equations (A.3) yields (2.13). Acknowledgments The authors would like to acknowledge the support from CNRS under the PEPS 2015 Inphyniti programme and exploratory project FARA. The authors are grateful to the anonymous referees whose remarks enhanced our manuscript. References 1] J. R. Apel, L. A. Ostrovsky, Y. A. Stepanyants, and J. F. Lynch. Internal solitons in the ocean and their effect on underwater sound. J. Acoust. Soc. Am., 121(2):695, ] R. Barros and S. Gavrilyuk. Dispersive Nonlinear Waves in Two-Layer Flows with Free Surface Part II. Large Amplitude Solitary Waves Embedded into the Continuous Spectrum. Stud. Appl. Math., 119(3): , oct ] R. Barros, S. L. Gavrilyuk, and V. M. Teshukov. Dispersive Nonlinear Waves in Two-Layer Flows with Free Surface. I. Model Derivation and General Properties. Stud. Appl. Math., 119(3): , oct ] E. Barthélémy. Etude des ondes longues internes et de leur dynamique dans les zones côtières. Phd thesis, University Joseph Fourier, , 5 5] T. J. Bridges. Multi-symplectic structures and wave propagation. Math. Proc. Camb. Phil. Soc., 121(1): , jan , 5, 8 6] T. J. Bridges and N. M. Donaldson. Reappraisal of criticality for two-layer flows and its role in the generation of internal solitary waves. Phys. Fluids, 19(7):072111, ] T. J. Bridges and S. Reich. Multi-symplectic integrators: numerical schemes for Hamiltonian PDEs that conserve symplecticity. Phys. Lett. A, 284(4-5): , , 5, 12

16 D. Clamond & D. Dutykh 14 / 14 8] M. Chhay, D. Dutykh, and D. Clamond. On the multi-symplectic structure of the Serre- Green-Naghdi equations. J. Phys. A: Math. Gen, 49(3):03LT01, jan , 8 9] W. Choi and R. Camassa. Fully nonlinear internal waves in a two-fluid system. J. Fluid Mech., 396:1 36, oct , 5 10] P. Christodoulides and F. Dias. Stability of capillary-gravity interfacial waves between two bounded fluids. Phys. Fluids, 7(12):3013, ] V. Duchêne, S. Israwi, and R. Talhouk. A new class of two-layer Green-Naghdi systems with improved frequency dispersion. Stud. Appl. Math., In press, ] D. Dutykh, M. Chhay, and F. Fedele. Geometric numerical schemes for the KdV equation. Comp. Math. Math. Phys., 53(2): , ] C. Garrett and W. Munk. Space-time scales of internal waves: A progress report. J. Geophys. Res., 80(3): , jan ] C. Garrett and W. Munk. Internal Waves in the Ocean. Ann. Rev. Fluid Mech., 11(1): , jan ] R. S. Johnson. Camassa-Holm, Korteweg-de Vries and related models for water waves. J. Fluid Mech., 455:63 82, ] Z. L. Maltseva. Unsteady long waves in a two-layer fluid. Dinamika Sploshn. Sredy, 93-94:96 110, ] J. E. Marsden, G. W. Patrick, and S. Shkoller. Multisymplectic geometry, variational integrators, and nonlinear PDEs. Comm. Math. Phys., 199(2):52, ] M. Miyata. Long internal waves of large amplitude. In Nonlinear Water Waves: IUTAM Symposium, pages , Tokyo, Japan, Springer. 4 19] B. Moore and S. Reich. Multi-symplectic integration methods for Hamiltonian PDEs. Future Generation Computer Systems, 19(3): , , 12 20] L. Ostrovsky, E. Pelinovsky, V. Shrira, and Y. Stepanyants. Beyond the KdV: Post-explosion development. Chaos, 25(9):097620, sep ] F. Serre. Contribution à l étude des écoulements permanents et variables dans les canaux. La Houille blanche, 8: , ] R. Staub. Contribution à l étude des ondes de gravité en eau peu profonde. Phd thesis, University of Grenoble, Laboratoire J. A. Dieudonné, Université de Nice Sophia Antipolis, Parc Valrose, Nice cedex 2, France address: diderc@unice.fr URL: LAMA, UMR 5127 CNRS, Université Savoie Mont Blanc, Campus Scientifique, Le Bourget-du-Lac Cedex, France address: Denys.Dutykh@univ-savoie.fr URL:

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