Introduc)on to modeling turbulence in oceanic flows
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1 Introducon to modeling turbulence in oceanic flows Mehmet Ilıcak Uni Research, Bjerknes Centre for Climate Research, Bergen Norway. School on Ocean Climate Modelling, 05, Ankara, Turkey 09/8/05
2 The biggest challenge in geophysical flows Large scale motion, L ~ O0-000 km. High Reynolds number, Re UL/ν ~ O 0. Sampling/observation is a challenge: Lab. experiments are limited. Difficult to get χx,y,z,t in the real ocean/atmosphere. Rotation of Earth. Stratification: effect of density differences Vertical displacement are restricted. Mixing between different density layers. Presence of internal waves. 09/8/05
3 Geophysical flows Gulf Stream Great Red Spot gulfstream0image.gif 09/8/05
4 Turbulent coherent structures Lab experiment: Re400 Oil discharge from a ship: Re~0 7 from p. 00 of Van Dyke 98 09/8/05 4
5 Navier- Stokes equaons!u!t u!u!x v!u!y w!u!z "!p!x! #!x "!u $!x!v!t u!v!x v!v!y w!v!z "!p!y! #!x "!v $!x!w!t u!w!x v!w!y w!w!z "!p!z " g! '! #!x "!w $!x!u i!t u j!u i "!p! ' " g i!!x j!x i! # '!y "!u! # $!y '!z "!u $!z '! # '!y "!v! # $!y '!z "!v $!z '! # '!y "!w! # $!y '!z "!w $!z ' # "!u i!x j $!x j ' i, j,, 09/8/05 5
6 Modeling turbulent spectrum!u i!t u j!u i "!p! ' " g i!!x j!x i # "!u i!x j $!x j ' Re UL! Re [m / s]!00!0 [m] 0 " [m / s] 0 logek Energy containing range P ~k -5/ Inertial range fre Dissipation range ε logk 09/8/05
7 Possible modeling approaches Direct Numerical Simulations Resolved all scales of motion i.e. molecular viscosity, but how? DNS!u i!t u j RANS!u i "!p! ' " g i!!x j!x i LES # "!u i!x j $!x j ' Ilıcak et al /8/05 7
8 Possible modeling approaches DNS Resolved all scales N ~ Re 9/4 RANS Re! U!x RANS Resolved! mean state!u LES i!t u!u i j "!p! ' " g i! # "!u i!x Resolved large eddies j!x i!x j $!x j DNS LES ' Ilıcak et al /8/05 8
9 Kelvin-Helmholtz instability from p. 89 of Van Dyke 98 Upper fluid column is moving to the right faster then the lower one. 09/8/05 9
10 Direct numerical simulation DNS z D Non-hydrostatic model grid points in x,y and z directions Run in 8 processors x 09/8/05 0
11 Reynolds Averaging Navier- Stokes RANS u i U i uʹ i!u i!t!u U i j! u" j u i "!x j!x j #!p! # g i! $ "!U i!x i!x j!x j ' uʹ uʹ i t j U k uʹ uʹ i x k j uʹ uʹ uʹ k x i k j P ij ij ε ij x k uʹ ʹ iu j ν xk # unknowns > # equaons System is NOT closed The famous Turbulence Closure Problem 09/8/05
12 Turbulence closure models!u i!t!u U i j! u" j u i "!x j!x j #!p! # g i! $ "!U i!x i!x j!x j ' Eddy viscosity approach U uʹ wʹ K M z We need to find a way to compute eddy viscosity/diffusivity. Ex: KPP, k- epsilon, k- omega, MY, standard Smagorinsky. 09/8/05
13 Large Eddy Simulaons LES Large Eddy Simulation LES: Mixing by the large, energy-containing, eddies is handled through computation, while the effect of small, dissipative, turbulent eddies is modeled analytically.! < u > i!t u i < u > i u i!! < u > < u > i j!! ij "!p! " g i!!x j!x j!x i # "! < u > i!x j $!x j '! ij K M! < u > i!x j! < u > j!x i 09/8/05
14 Possible modeling approaches DNS N ~ Re 9/ 4 Resolved all scales RANS Resolved mean state LES Resolved large eddies DNS RANS LES Ilıcak et al /8/05 4
15 Possible modeling closures SGS turbulence closures; RANS Constant eddy viscosity/diffusivity Prandtl s 95 eq. model KPP Large et al. 994 eq. turbulence closures k-epsilon, k-omega, k- kl, MY LES Constant eddy viscosity/diffusivity Standard Smagorinsky Dynamical Smagorinsky #U u! w! "K M #z K M K M C! # $ kl "U i "x j "U j "x i ' 09/8/05 5
16 Ocean model equaons!u!t u!u!x v!u!y w!u!z "!p!x! #!x A M $!u!x! # '!y A M $!u!y! # '!z K M $!u!z '!v!t u!v!x v!v!y w!v!z "!p!y! #!x A M $!v!x! # '!y A M $!v!y! # '!z K M $!v!z '!T!t u!t!x v!t!y w!t!z! " $!x A H # Smagorinsky Biharmonic viscosity Leith Numerical i.e. ROMS!T!x '! " $!y A H #!T!y '! " $!z K H # Constant eddy viscosity Ad- hoc i.e. Price- Turner, KPP One/two eq. turbulence schemes.!t!z ' 09/8/05
17 One-equation turbulence closure K M kl! k / l where l is prescribed. 09/8/05 7
18 Two-equation turbulence closures K K M H c c kls kls M H 09/8/05 8
19 Dynamical Smagorinsky c < M L > ij ij < M M > ds kl M ij!!!! s!u! s!u ij "!! s u! s uij! "! s!u! s!u "!s ij u! s u! M ij! M ij /! kl c ds! < M Lij ij >!! < M kl M kl > 09/8/05 9
20 Eddy viscosity diffusivity #U u! w! "K M #z #T T 'w' "K H #z K K M H c c kls kls M H Pr t K K M H S S M H K M Eddy viscosity K H Eddy diffusivity kturbulent kinec energy lturbulent length scale Pr t Turbulent Prandtl Number S M and S H Very complex stability funcons 09/8/05 0
21 Pr t Ri g Pr K Pr t M 0 Pr π 0 0.; Ri exp Pr0 Ri k ; ε Ri f K H g f 0. K Pr M t Ri Ri g f Ilicak et al /8/05
22 Red Sea overflow T0 T 09/8/05
23 Experiments KPP K-Profile Parameterization PB07 Peters and Baumert 007 CA Canuto-A, CB Canuto-B G88 Galperin et al. 988, KC Kantha-Clayson 09/8/05
24 Propagaon of overflow 09/8/05 4
25 Eddy diffusivity Northern Channel 09/8/05 5
26 Summary There are different approaches to tackle turbulence in ocean models; DNS, RANS, LES Eddy viscosity/diffusivity approach is a modelling strategy. Different complexity of parameterizaons out there. Be aware of shortcomings and advantages of these models. 09/8/05
27 Upwelling test case C P P C 09/8/05 7
28 Upwelling test case 09/8/05 8
29 Upwelling test case 09/8/05 9
30 Stability funcons / ; / m m h h m h m h M m h H G f b G G f b G f b G f b G f b b cff cff G f s G f s s S cff G f s G f s s S Galperin et al. 988 h h H M h H A A G G S A A A A B S B A A G B A A S / ; / Canuto A and B / 4 / ; 4 4 / ; 7 ; 4 / / / ; ; /8 / / ; / µ c f b b b b b b s s s s s s 09/8/05 0
31 Hydrostatic vs. Non-hydrostatic Hydrostac model Non- hydrostac model Cannot resolve shear instabilities such as KH rolls. Depend on full closures such as nd order turbulence models Algebraic models P z Can resolve shear instabilities. Depend on resolution and subgrid scale parameterization LES VLES dw P ρg κ w dt z ρ ρg ρ 09/8/05 0 0
32 Vercal coordinate in OGCMs ρ z * σ 09/8/05
33 The turbulent Prandtl number Venayagamoorthy and Stretch 00 09/8/05
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