Etudes et évaluation de processus océaniques par des hiérarchies ...
Etudes et évaluation de processus océaniques par des hiérarchies ... Etudes et évaluation de processus océaniques par des hiérarchies ...
158 CHAPITRE 4. ETUDES DE PROCESSUS OCÉANOGRAPHIQUES 14 6 Discussion I have demonstrated, that friction parameters and laws in gravity currents can be estimated using data assimilation. The results clearly show that friction follows a linear Rayleigh law for small Reynolds numbers and the estimated friction coefficient agrees well with the analytical value obtained for non-accelerating Ekman layers. A significant and sudden departure towards a quadratic drag law at Reynolds number of around 800 is shown, roughly in agreement with laboratory experiments (Nikuradse 1933, Schlichting & Gertsen 2000). Although the quadratic drag law is dominated by the linear friction at the Reynolds numbers considered in this study, the assimilation procedure clearly manages to detect its appearance and consistently estimate its value. The drag coefficient obtained ≈ 1.5 · 10 −4 (see table 2) is on the lower end of classical values over smooth surfaces (see Stull 1988, Schlichting & Gertsen 2000). This comes at no surprise as only part of the turbulent small scale motion, responsible for the turbulent viscosity, is explicitly resolved in the non-hydrostatic model, due to the strong anisotropy in the numerical grid (see subsection 2.3). The experiments were performed for moderate surface Rossby numbers as: (i) the numerical resolution in the Navier-Stokes model does not allow for an explicit representation of the fully turbulent Ekman layer (see subsection 2.3) and (ii) with increasing Rossby number non-hydrostatic effects become important, neither explicitly resolved nor implicitly included (parametrised) in the shallow water model used for the assimilation. tel-00545911, version 1 - 13 Dec 2010 Comparison of free runs of the shallow-water model with the estimated parameter values clearly show that the shallow-water model performs well in the vein, whereas it deteriorates in the friction layer with increasing temperature anomaly. In these areas the local Froud number is larger than unity and the oscillations of the interface and its breaking starts to develop. These non-hydrostatic processes are neither explicitly included in the (hydrostatic) shallow-water model nor are they parametrised. The parametrisation of the dynamics at the interface, including the mixing, entrainment and detrainment, is subject to current research, using higher resolution three dimensional non-hydrostatic simulations of only a small part of the gravity current. Furthermore, to represent the bottom friction in the shallow water model I supposed that unaccelerated linear Ekman layer theory applies to leading order. This assumption is questionable when non-linear effects, leading to a drag law, become dominant. I demonstrated that the linear dynamics and the nonlinear departure from it are well captured in the present work. I also showed that data assimilation is a powerful tool in systematically connection models in a model hierarchy. The parameters of the two most observed and employed friction laws, Rayleigh friction and the drag law, are estimated here. The methodology is not restricted to this two laws, this linear and quadratic laws can also be seen, pragmatically, as the beginning of a Taylor series. Friction forces are difficult to observe directly or to determine in laboratory experiments, as forces exerted on the boundary are small, inhomogeneous in space and intermittent in time. I have also performed laboratory experiments on rotating gravity currents on the Coriolis platform in Grenoble (France) and measured its thickness. The quantity of data measured was not sufficient to determine the friction parameters and laws. Further laboratory experiments with a substantially increased number of observations are planed.
4.8. ESTIMATION OF FRICTION LAWS AND PARAMETERS IN GRAVITY CURRENTS BY DATA 15 A Appendix: Calculation of the Coriolis-Boussinesq parameter for linear Ekman layers The Solution for the Ekman spiral of a fluid moving with a constant geostrophic speed of V G in the y-direction is given by: ũ = V G exp(−z/δ) sin(z/δ) (19) ṽ = V G (1 − exp(−z/δ) cos(z/δ)) , (20) where I have denoted ũ the variable that has a dependence in the z-direction as opposed to vertically averaged value u = 〈ũ〉 = 1 R h h 0 ũdz. The vertical average of the velocity component in the x-direction and its square, using eq. (19), are: u = 〈ũ〉 = 1 h u 2 ≠ 〈ũ 2 〉 R h 0 ũdz = V G h R h 0 exp(−z/δ) sin(z/δ)dz = V Gδ 2h = V 2 G h R h 0 exp(−2z/δ) sin2 (z/δ)dz = V 2 G δ 8h = V G 4β = V 2 G 16β (21) (22) β = 〈ũ2 〉 〈ũ〉 2 = h 2δ (23) tel-00545911, version 1 - 13 Dec 2010 Please note that equation (21) shows that the mean velocity in the x-component is only one quarter of geostrophic velocity divided by β. Linear Ekman layer theory shows, that the frictional force is equal in both directions, so that in the friction term the u value has to be multiplied by 4β. The non-linear term in the v-equation is u∂ xv is vanishing to leading order of β −1 as the u-velocity is concentrated in the Ekman layer, whereas the bulk of the v-momentum is above it. I used: Z exp(−z/δ) sin(z/δ)dz = −δ (sin(z/δ) + cos(z/δ)) and (24) 2 Z exp(−2z/δ) sin 2 (z/δ)dz = − exp(−2z/δ) (2sin 2 (z/δ) + sin(z/δ) cos(z/δ) + 1). (25) 8 I emphasise that these calculations are only valid for the unaccelerated laminar Ekman layer. References 1. K. Brusdal, J.M. Brankart, G. Halberstadt, G. Evensen, P. Brasseur, P.J. van Leeuwen, E. Dombrowsky, & J. Verron (2003) A demonstration of ensemble-based assimilation methods with a layered OGCM from the perspective of operational ocean forecasting systems J. Marine Systems. 40-41, 253–289. 2. G. Burgers, P. van Leeuwen & G. Evensen (1998) Analysis scheme in the ensemble Kalman filter Mon. Weather Rev. 126, 1719–1724. 3. G. Evensen (1994), Sequential data assimilation with a nonlinear quasi-geostrophic model using Monte Carlo methods to forecast error statistics. J. Geophys. Res. 99, 10,143–10,162. 4. G. Evensen (2003), The ensemble Kalman filter: theoretical formulation and practical implementation. Ocean Dyn . 53, 343–367. 5. Frisch U., S. Kurien, R. Pandit, W. Pauls, S. Sankar Ray, A. Wirth, and J.-Z. Zhu, “Hyperviscosity, Galerkin Truncation, and Bottlenecks in Turbulence” Phys. Rev. Lett., 101, 144501, 2008. 6. N. Grianik, I. M. Held, K. S. Smith & G. K. Vallis (2004) The effects of quadratic drag on the inverse cascade of two-dimensional turbulence, Phys. Fluids 16, 73; doi:10.1063/1.1630054. 7. J. Jiménez (2004), Turbulent flows over rough walls, Ann. Rev. Fluid Mech 36, 173–196.
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158 CHAPITRE 4. ETUDES DE PROCESSUS OCÉANOGRAPHIQUES<br />
14<br />
6 Discussion<br />
I have <strong>de</strong>monstrated, that friction <strong>par</strong>am<strong>et</strong>ers and laws in gravity currents can be<br />
estimated using data assimilation. The results clearly show that friction follows a linear<br />
Rayleigh law for small Reynolds numbers and the estimated friction coefficient<br />
agrees well with the analytical value obtained for non-accelerating Ekman layers. A<br />
significant and sud<strong>de</strong>n <strong>de</strong><strong>par</strong>ture towards a quadratic drag law at Reynolds number of<br />
around 800 is shown, roughly in agreement with laboratory experiments (Nikuradse<br />
1933, Schlichting & Gertsen 2000). Although the quadratic drag law is dominated<br />
by the linear friction at the Reynolds numbers consi<strong>de</strong>red in this study, the assimilation<br />
procedure clearly manages to d<strong>et</strong>ect its appearance and consistently estimate<br />
its value. The drag coefficient obtained ≈ 1.5 · 10 −4 (see table 2) is on the lower end<br />
of classical values over smooth surfaces (see Stull 1988, Schlichting & Gertsen 2000).<br />
This comes at no surprise as only <strong>par</strong>t of the turbulent small scale motion, responsible<br />
for the turbulent viscosity, is explicitly resolved in the non-hydrostatic mo<strong>de</strong>l, due<br />
to the strong anisotropy in the numerical grid (see subsection 2.3). The experiments<br />
were performed for mo<strong>de</strong>rate surface Rossby numbers as: (i) the numerical resolution<br />
in the Navier-Stokes mo<strong>de</strong>l does not allow for an explicit representation of the fully<br />
turbulent Ekman layer (see subsection 2.3) and (ii) with increasing Rossby number<br />
non-hydrostatic effects become important, neither explicitly resolved nor implicitly inclu<strong>de</strong>d<br />
(<strong>par</strong>am<strong>et</strong>rised) in the shallow water mo<strong>de</strong>l used for the assimilation.<br />
tel-00545911, version 1 - 13 Dec 2010<br />
Com<strong>par</strong>ison of free runs of the shallow-water mo<strong>de</strong>l with the estimated <strong>par</strong>am<strong>et</strong>er<br />
values clearly show that the shallow-water mo<strong>de</strong>l performs well in the vein, whereas<br />
it d<strong>et</strong>eriorates in the friction layer with increasing temperature anomaly. In these areas<br />
the local Froud number is larger than unity and the oscillations of the interface<br />
and its breaking starts to <strong>de</strong>velop. These non-hydrostatic processes are neither explicitly<br />
inclu<strong>de</strong>d in the (hydrostatic) shallow-water mo<strong>de</strong>l nor are they <strong>par</strong>am<strong>et</strong>rised.<br />
The <strong>par</strong>am<strong>et</strong>risation of the dynamics at the interface, including the mixing, entrainment<br />
and d<strong>et</strong>rainment, is subject to current research, using higher resolution three<br />
dimensional non-hydrostatic simulations of only a small <strong>par</strong>t of the gravity current.<br />
Furthermore, to represent the bottom friction in the shallow water mo<strong>de</strong>l I supposed<br />
that unaccelerated linear Ekman layer theory applies to leading or<strong>de</strong>r. This assumption<br />
is questionable when non-linear effects, leading to a drag law, become dominant.<br />
I <strong>de</strong>monstrated that the linear dynamics and the nonlinear <strong>de</strong><strong>par</strong>ture from it are well<br />
captured in the present work. I also showed that data assimilation is a powerful tool<br />
in systematically connection mo<strong>de</strong>ls in a mo<strong>de</strong>l hierarchy.<br />
The <strong>par</strong>am<strong>et</strong>ers of the two most observed and employed friction laws, Rayleigh<br />
friction and the drag law, are estimated here. The m<strong>et</strong>hodology is not restricted to<br />
this two laws, this linear and quadratic laws can also be seen, pragmatically, as the<br />
beginning of a Taylor series.<br />
Friction forces are difficult to observe directly or to d<strong>et</strong>ermine in laboratory experiments,<br />
as forces exerted on the boundary are small, inhomogeneous in space and<br />
intermittent in time. I have also performed laboratory experiments on rotating gravity<br />
currents on the Coriolis platform in Grenoble (France) and measured its thickness.<br />
The quantity of data measured was not sufficient to d<strong>et</strong>ermine the friction <strong>par</strong>am<strong>et</strong>ers<br />
and laws. Further laboratory experiments with a substantially increased number of<br />
observations are planed.