Title: Coarse grained velocity derivatives
1Coarse grained velocity derivatives
- Beat Lüthi
-
- Jacob Berg
- Søren Ott
- Jakob Mann
- Risø National Laboratory Denmark
2Motivation
- Ãij properties
-
-
-
-
-
- LES context
-
-
-
- What can 3D-PTV contribute?
-
- so far HPIV, 2D PIV, DNS
Motivation 1 Technical 4 Properties 6 Multi
particles 4 Energy flux 5 Flux
modelling 5 Conclusion 1
3How to get Ãij from points?
Motivation 1 Technical 1/4 Properties 6 Multi
particles 4 Energy flux 5 Flux
modelling 5 Conclusion 1
4Particle seeding, scales?
How dense can we track??
How fast can we record??
D?
Motivation 1 Technical 2/4 Properties 6 Multi
particles 4 Energy flux 5 Flux
modelling 5 Conclusion 1
current seeding range ½-1½ L
h
L
current Rel 170, L/ h 200
5How many points?
Motivation 1 Technical 3/4 Properties 5 Multi
particles 4 Energy flux 5 Flux
modelling 5 Conclusion 1
6Convergence
Motivation 1 Technical 4/4 Properties 6 Multi
particles 4 Energy flux 5 Flux
modelling 5 Conclusion 1
If we take more than 12 particles then it is ok
7Orientation of Ãij as f(D)
Motivation 1 Technical 4 Properties 1/6 Multi
particles 4 Energy flux 5 Flux
modelling 5 Conclusion 1
8Time scale t
Motivation 1 Technical 4 Properties 2/6 Multi
particles 4 Energy flux 5 Flux
modelling 5 Conclusion 1
rh t t h rgt h tr2/3
9Eigenvalues of strain
Motivation 1 Technical 4 Properties 3/6 Multi
particles 4 Energy flux 5 Flux
modelling 5 Conclusion 1
10Vorticity alignment with strain, f(D)?
w switches from l2 to l1!
Ref to porter paper
Motivation 1 Technical 4 Properties 4/6 Multi
particles 4 Energy flux 5 Flux
modelling 5 Conclusion 1
similar observation
11RQ
Motivation 1 Technical 4 Properties 5/6 Multi
particles 4 Energy flux 5 Flux
modelling 5 Conclusion 1
12RQ in mean strain
Motivation 1 Technical 4 Properties 6/6 Multi
particles 4 Energy flux 5 Flux
modelling 5 Conclusion 1
13Multi particle constellations
w2A/R2
Motivation 1 Technical 4 Properties 6 Multi
particles 1/4 Energy flux 5 Flux
modelling 5 Conclusion 1
gieigenvalues of moment of inertia tensor gab
14Description of shape evolution
Motivation 1 Technical 4 Properties 6 Multi
particles 2/4 Energy flux 5 Flux
modelling 5 Conclusion 1
15Alignment to strain
Motivation 1 Technical 4 Properties 6 Multi
particles 3/4 Energy flux 5 Flux
modelling 5 Conclusion 1
16Significant small scale contribution
total
total
large scales
large scales
Motivation 1 Technical 4 Properties 6 Multi
particles 4/4 Energy flux 5 Flux
modelling 5 Conclusion 1
Significant contribution from small scales!
17Definition of SGS TKE production rate1, or
energy flux
Motivation 1 Technical 4 Properties 6 Multi
particles 4 Energy flux 1/5 Flux
modelling 5 Conclusion 1
- Also referred to as
- energy flux
- SGS dissipation
18Energy flux from DNS
Motivation 1 Technical 4 Properties 6 Multi
particles 4 Energy flux 2/5 Flux
modelling 5 Conclusion 1
19Energy flux from Experiment
None homogeneous forcing
Motivation 1 Technical 4 Properties 6 Multi
particles 4 Energy flux 3/5 Flux
modelling 5 Conclusion 1
20Alignment of tij with sij
compressing producing SGS
stretching backscattering
Motivation 1 Technical 4 Properties 6 Multi
particles 4 Energy flux 4/5 Flux
modelling 5 Conclusion 1
21Alignm. of tij with sij for backscatter
stretching backscattering
compressing producing SGS
Motivation 1 Technical 4 Properties 6 Multi
particles 4 Energy flux 5/5 Flux
modelling 5 Conclusion 1
22Smagorinsky, non-linear, mixed,
- scalar eddy viscosity
- related to strain
- no backscatter possible
- stable
- tensor eddy viscosity
- related to strain and vorticity production
- allows for backscatter
- is instable
Motivation 1 Technical 4 Properties 6 Multi
particles 4 Energy flux 5 Flux
modelling 1/5 Conclusion 1
23Testing the non-linear model for flux
DNS
Experiment
Motivation 1 Technical 4 Properties 6 Multi
particles 4 Energy flux 5 Flux
modelling 2/5 Conclusion 1
24RQ mapping of energy flux
Motivation 1 Technical 4 Properties 6 Multi
particles 4 Energy flux 5 Flux
modelling 3/5 Conclusion 1
25RQ mapping for error
too little backscatter
too much backscatter
Motivation 1 Technical 4 Properties 6 Multi
particles 4 Energy flux 5 Flux
modelling 4/5 Conclusion 1
26Alternative mapping Q-sss and s2-sss
Motivation 1 Technical 4 Properties 6 Multi
particles 4 Energy flux 5 Flux
modelling 5/5 Conclusion 1
27Conclusion
- perform more experiments
- measure Ãij and tij
- influence of complex mean strain?
- because with 3D-PTV we can
Motivation 1 Technical 4 Properties 6 Multi
particles 4 Energy flux 5 Flux
modelling 5 Conclusion 1