Energy flux to subgrid scales as obtained from particle tracking

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1 Energy flux to subgrid scales as obtained from particle tracking Beat Lüthi & Søren Ott Jacob Berg Jakob Mann Risø National Laboratory Denmark/DTU

2 Motivation à ij properties LES context What can 3D-PTV contribute? so far: HPIV, 2D PIV, DNS

3 Content of this presentation 3D particle tracking filtered derivatives energy flux how to decompose/represent it energy flux from PTV & nonlinear model correction for nonlinear model conclusions

4 Main idea of 3D-PTV to follow a 3D (!) particle position as opposed to 2D PIV! started 1983

5 List of technical aspects flow tracers illumination cameras observation volume camera callibration particle detection from 2D to 3D positions particle tracking

6 Flow tracers high tech, accurate, expensive: low tech, accurate, cheap: Idea: Søren Ott & Jakob Mann, Risø, Denmark fly ashøsievingø 50-60µm

7 Illumination LED array, TU/e Lorenzo del Castello, Herman Clercx trend towards smarter solutions

8 Fast digital cameras pixel: 500x500 frame rate: 50Hz pixel: 1000x1000 frame rate: 5000Hz or pixel: 250x250 frame rate: Hz data storage is main bottelneck

9 Camera callibration teach the cameras with know grid points problem: how to have space filling target? solution in part: callibration on flow tracers

10 From 2D to 3D position callibration and 2D position accuracy, seeding density, etc. r(x,y,z,t) Camera 3 Camera 4 Camera 1 z y Camera 2 x

11 Tracking through consequtive images tracking criteria: particle must not travel further than their typical spacing codes available at

12 Many dependencies, many choices flow speed trackability camera recording rate illumination flow scales one would like to resolve field of view depth of view number of tracer particles optical working distance particle diameter camera pixel resolution

13 Final output is the start for analysis if all goes well, one can finally start learning about the flow

14 Velocity derivatives differentiate convoluted velocity field to get velocity derivatives challenge to get HIGH SEEDING DENSITY B. Lüthi ETH, Søren Ott Risø, Jacob Berg, Jakob Mann

15 Particle seeding, scales? How dense can we track?? How fast can we record?? Δ=? current seeding range η L current Re λ : 170, L/ η ~200

16 Velocity gradients

17 Velocity gradients

18 Self amplification

19 Structure

20 RQ invariant maps

21 LES context Jörg Ziefle, Kleiser LES group ETH

22 Definition of SGS TKE production rate 1 or energy flux also referred to as: energy flux SGS dissipation

23 Role of PTV for LES? holographic PIV, Tao et al. 2002, van der Bos et al sonic anemometer array, Higgins et al D-PTV check SGS modeling assumptions check is possible in real flows

24 Energy flux from 3D-PTV mean flux ~ 0.7 ε Tao et al. 2002: mean flux > 2 ε how to trust flux? analysis and sources of error?

25 Eigenvalues of τ ij Chumakov 2006 JFM also introduces q*

26 Alignment of τ ij to s ij (Tao et al. 2002) causes backscatter backscatter backscatter downscale downscale Smagorinsky case

27 Contributions to flux most important τ 1 least important τ 2

28 Alignment of τ ij to s ij τ 1, τ 3 most relevant τ 1 aligned with λ 3 τ 2,τ 3 perpendicular to λ 3

29 Alignment of τ ij to s ij λ 1 λ 2

30 Flux in terms of RQ van der Bos et al. 2002, Physics of Fluids 14(7) holographic PIV

31 Flux in terms of RQ

32 Flux in terms of RQ PTV DNS public data from Biferale, Boffetta, Toschi etc.

33 Smagorinsky, nonlinear, mixed, scalar eddy viscosity: related to strain no backscatter possible stable tensor eddy viscosity: related to strain and vorticity production allows for backscatter is unstable

34 Validation : Eigenvalues of τ ij nonlinear model: overestimates large τ 1 underestimates τ 2 and τ 3

35 Validation : Alignment of τij to sij

36 Validation: Alignment of τ ij to s ij λ 3 λ 3 λ 1 λ 2 λ 1 λ 2 nonlinear model: too deterministic too little τ 1 λ 3 alignment too much τ 2 λ 1 alignment

37 Flux error in terms of RQ

38 Flux error in terms of RQ

39 Possible correction for nonlin. model 2 rotations to get τ 1 right 1 rotation around τ 1 λ 2 λ 2 λ 3 λ 1 blue on red more backscatter blue on blue more energy flux to small scales λ 3 λ 1 green on red more backscatter green on green more Smagorinsky more energy flux to small scales

40 Possible correction

41 Conclusion particle tracking can access (LES) energy flux can be used to study SGS models e.g. the nonlinear model we find systematic misalignment corrected model has less flux error need&possibility for more specific experiments

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