POWER LAWS and VORTICAL STRUCTURES P. Orlandi G.F. Carnevale, S. Pirozzoli Universita' di Roma “La Sapienza” Italy.

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Presentation transcript:

POWER LAWS and VORTICAL STRUCTURES P. Orlandi G.F. Carnevale, S. Pirozzoli Universita' di Roma “La Sapienza” Italy

POWER LAWS Non-linear terms create wide E(k)‏ Triadic interaction in K space Vortical structures in physical space At high Re and at low K K n Turbulence ≠ 0 high K exp(-  K)‏ Kolmogorov n=-5/3 Analysed structures with strong  Worms or tubular structures

INVISCID FLOWS Lack of dissipation Possibility of a FTS E(k) varies in time Before singularity n=-3 Initial conditions important Interacting Lamb dipoles n=-6 Taylor-Green t=0 E(1)‏

COMPARISON Comparison viscous inviscid Difference in n related to structures Filtering the fields Possibility to isolate structures Selfsimilarity in the range K n Shape of structures related to n

NUMERICAL TOOLS 2° order accuracy more than sufficient Stable Physical principle reproduced in discrete Mass conservation Energy conservation inviscid Finite difference simple Reproduce all the requirements IMPORTANT to resolve the flow NOT the accuracy

time reversibility Duponcheel et al Taylor-Green Forward up to t=10 V(t,X)=-V(t,X)‏ From t=10 to t=20 equivalent To backward At t=20 V(20,X)=V(0,x)‏ Comparison R-K-low storage FD2 with FD4 and Pseudospectral

RESULTS time reversibility

RESULTS Grafke et al Interacting dipoles

FORC ISOTROPIC DISS.

FORC Inertial Gotoh

FORC Inertial Jimenez

INVISCID SOLUTION Question? Has Euler a Finite Time Singularity Does it depend on the Init. Condit. Several simulations in the past Pumir, Peltz, Kerr, Brachet Interest on the Euler equations Mostly by Pseudospectral Init. condition Ortogonal Dipoles Taylor-Green Kida-Peltz

SOLID PROOF Infinite space-time resolution near singularity From well resolved simulations indications E.G. derive one model equation having FTS dx/dt= x 2

LAMB dipoles I.C. Self preserving vortex Traslating with U Solution 2D Euler

LAMB DIPOLES

LAMB spectra LD1

Compensated SPECTRA LD1

Lamb Evolution t=1

Vorticity amplification

INITIAL CONDITIONS

SPECTRA near FTS

VORTICITY near FTS

Component along S_2 Strain in the principal axes Simulation shows that S 2 prop ω 2

Vorticity amplification

Enstrophy prod. amplification

Taylor-Green Spectra CB

Taylor-Green Spectra Or Spectra during evolution do not have a power law

Taylor-Green  max

T-G Compensated Spectra

T-G Spectra

T-G Enstrophy Prod.

Spectra of the fields

Vortical structures Lamb

Vortical structures T-G

Filtering To investigate the strutures in a range of K From physical to wave number Set u(K)=0 for Kl < K < Ku Back from wave to physical

Filtering Lamb  (max)=50

Filtering Lamb  (max)=410

Filtering Lamb  (max)=240

Filtering Lamb  (max)=225

Lamb self-similarity

Filtering T-G  (max)=4.2

Filtering T-G  (max)=13.8

Filtering T-G  (max)=20.7

Filtering T-G  (max)=17.6

Filtering T-G  (max)=12.5

T-G selfsimilarity

Pdf 

Lamb Pdf 

T-G Pdf 

FORCED ISOTROPIC –Kolmogorov with n=-5/3 –Why?

DNS with SMOOTH I.C Comprehension non linear terms - Inviscid leads to FTS (personal view)‏ - I would like to know which is a convincing proof Well resolved leads to n=-3 - Viscous lead to n=-5/3 No FTS for N-S (personal view) Different equations Small ν leads to exp range in E(k)‏ R‏esolution important

ONE LAMB viscous and inviscid

ENSTROPHY

Spectra before FTS

Spectra after FTS

LAMB COUPLES Re=3000

Three LAMB viscous and inviscid

SPECTRA Enstr. amplification

SPECTRA Enstr. max

SPECTRA Enstr. decay

ENSTROPHY Eq.

ENSTROPHY balance

ENSTROPHY production

Enstrophy prod. Princ. axes

Rate enstrophy prod.

Jpdf Enstr. Prod. ; Rs amplification

Jpdf Enstr. Prod. ; Rs maximum

Jpdf Enstr. Prod. ; Rs decay

STRUCTURES Eduction of tubes Swirling strength criterium Eduction of sheets Largest eigenvalues of Red sheets, yellow tubes

Lamb weak interaction

Lamb strong interaction

Lamb max enstrophy

Kolmogorov range formation Before t* vortex sheets and tubes Amplification stage sheets formations At t* intense curved sheets After t* tubes form from sheet roll-up Tubes interact with sheets Sheets more compact K- 5/3 Bottleneck forms At large times K -3/2 –

Lamb vs Isotropic Energy and enstrophy

Lamb vs Isotropic Spectra

Lamb vs Isotropic Velocity derivatives skewness

Lamb vs Isotropic Velocity derivatives flatness

Conclusions EULER have a FTS Navier-Stokes do not have FTS View of engineers from DNS Of different smooth I.C. Lamb dipole a good I.C. Shape preserving Spectra evolve maintaining power law Interaction with matematician necessary To find the relevant proofs Necessity of large CPU (common effort)‏

Vortical structures Forc Turb

Filtering Isot. Turb.  (max) =64

Filtering Isot. Turb.  (max) =106

Filtering Isot. Turb.  (max) =114

Filtering Isot. Turb.  (max) =144

Iso. Turb. Pdf 