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Coarse grained velocity derivatives

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Coarse grained velocity derivatives. Beat L thi. Jacob Berg. S ren Ott. Jakob Mann ... If we take more than 12 particles then it is ok. Motivation 1. Technical ... – PowerPoint PPT presentation

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Title: Coarse grained velocity derivatives


1
Coarse grained velocity derivatives
  • Beat Lüthi
  • Jacob Berg
  • Søren Ott
  • Jakob Mann
  • Risø National Laboratory Denmark

2
Motivation
  • 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
3
How to get Ãij from points?
Motivation 1 Technical 1/4 Properties 6 Multi
particles 4 Energy flux 5 Flux
modelling 5 Conclusion 1
4
Particle 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
5
How many points?
Motivation 1 Technical 3/4 Properties 5 Multi
particles 4 Energy flux 5 Flux
modelling 5 Conclusion 1
6
Convergence
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
7
Orientation of Ãij as f(D)
Motivation 1 Technical 4 Properties 1/6 Multi
particles 4 Energy flux 5 Flux
modelling 5 Conclusion 1
8
Time 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
9
Eigenvalues of strain
Motivation 1 Technical 4 Properties 3/6 Multi
particles 4 Energy flux 5 Flux
modelling 5 Conclusion 1
10
Vorticity 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
11
RQ
Motivation 1 Technical 4 Properties 5/6 Multi
particles 4 Energy flux 5 Flux
modelling 5 Conclusion 1
12
RQ in mean strain
Motivation 1 Technical 4 Properties 6/6 Multi
particles 4 Energy flux 5 Flux
modelling 5 Conclusion 1
13
Multi 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
14
Description of shape evolution
Motivation 1 Technical 4 Properties 6 Multi
particles 2/4 Energy flux 5 Flux
modelling 5 Conclusion 1
15
Alignment to strain
Motivation 1 Technical 4 Properties 6 Multi
particles 3/4 Energy flux 5 Flux
modelling 5 Conclusion 1
16
Significant 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!
17
Definition 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

18
Energy flux from DNS
Motivation 1 Technical 4 Properties 6 Multi
particles 4 Energy flux 2/5 Flux
modelling 5 Conclusion 1
19
Energy flux from Experiment
None homogeneous forcing
Motivation 1 Technical 4 Properties 6 Multi
particles 4 Energy flux 3/5 Flux
modelling 5 Conclusion 1
20
Alignment 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
21
Alignm. 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
22
Smagorinsky, 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
23
Testing 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
24
RQ mapping of energy flux
Motivation 1 Technical 4 Properties 6 Multi
particles 4 Energy flux 5 Flux
modelling 3/5 Conclusion 1
25
RQ 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
26
Alternative mapping Q-sss and s2-sss
Motivation 1 Technical 4 Properties 6 Multi
particles 4 Energy flux 5 Flux
modelling 5/5 Conclusion 1
27
Conclusion
  • 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
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