Introduction - University of Pittsburgh · events from PDF ensemble, via REA method, on Senegal...

18
FURTHER NUMERICAL TESTS OF ENSEMBLE EDDY VISCOSITY METHODS NAN JIANG AND WILLIAM LAYTON Abstract. This supplementary material complements the report with similar title. 1. Introduction The problem of computing ensembles, u j ,p j , of solutions of the Navier-Stokes equations (NSE): u j,t + u j ·∇u j - ν 4u j + p j = f j (x, t), in Ω, j =1, ..., J (1.1) ∇· u j = 0, and u j (x, 0) = u 0 j (x), in Ω and u j = 0, on Ω. was studied in a paper with similar title. This supplement presents further tests. The method uses two new ensemble eddy viscosity (EEV) type turbulence models with turbulent viscosity parametrizations EEV1: ν T = μ 1 4x|u 0 |, and EEV2: ν T = μ 2 |u 0 | 2 4t. These are based on direct parameterization of the energy in the turbulent fluctu- ations, 1 2 |u 0 | 2 and a redefinition of the LES lengthscale from (the usual) l = 4x to l = distance a fluctuating eddy travels in one time step = |u 0 |4t . 1.1. Methods. The euclidean length of a vector and Frobenius norm of an array is |·|. The symmetric part of the velocity gradient tensor is denoted s . The ensemble mean <u>, fluctuation u 0 j , its magnitude |u 0 | and the induced kinetic energy density k 0 are mean: <u>:= 1 J J X j=1 u j , fluctuation: u 0 j := u j - <u> , |u 0 | 2 := J X j=1 |u 0 j | 2 and energy density: k 0 = 1 2 |u 0 | 2 (x, t). Date : June 2013. 2000 Mathematics Subject Classification. Primary 65M12; Secondary 65J08 . Key words and phrases. NSE, ensemble calculation, UQ. The research herein was partially supported by NSF grant DMS 1216465 and Air Force grant FA 9550-12-1-0191. 1

Transcript of Introduction - University of Pittsburgh · events from PDF ensemble, via REA method, on Senegal...

  • FURTHER NUMERICAL TESTS OF ENSEMBLE EDDY

    VISCOSITY METHODS

    NAN JIANG AND WILLIAM LAYTON

    Abstract. This supplementary material complements the report with similar

    title.

    1. Introduction

    The problem of computing ensembles, uj , pj , of solutions of the Navier-Stokesequations (NSE):

    uj,t + uj · ∇uj − ν4uj +∇pj = fj(x, t), in Ω, j = 1, ..., J(1.1)∇ · uj = 0, and uj(x, 0) = u0j (x), in Ω and uj = 0, on ∂Ω.

    was studied in a paper with similar title. This supplement presents further tests.The method uses two new ensemble eddy viscosity (EEV) type turbulence modelswith turbulent viscosity parametrizations

    EEV1: νT = µ14x|u′|, andEEV2: νT = µ2|u′|24t.

    These are based on direct parameterization of the energy in the turbulent fluctu-ations, 12 |u

    ′|2 and a redefinition of the LES lengthscale from (the usual) l = 4xto

    l = distance a fluctuating eddy travels in one time step = |u ′|4t .

    1.1. Methods. The euclidean length of a vector and Frobenius norm of an arrayis | · |. The symmetric part of the velocity gradient tensor is denoted ∇s. Theensemble mean < u >, fluctuation u′j , its magnitude |u′| and the induced kineticenergy density k′ are

    mean: < u >:=1

    J

    J∑j=1

    uj , fluctuation: u′j := uj− < u > ,

    |u′|2 :=J∑

    j=1

    |u′j |2 and energy density: k′ =1

    2|u′|2(x, t).

    Date: June 2013.

    2000 Mathematics Subject Classification. Primary 65M12; Secondary 65J08 .

    Key words and phrases. NSE, ensemble calculation, UQ.The research herein was partially supported by NSF grant DMS 1216465 and Air Force grant

    FA 9550-12-1-0191.

    1

  • 2 NAN JIANG AND WILLIAM LAYTON

    Suppress the secondary spacial discretization and let superscripts denote the timestepnumber. Thus, for example, < u >n, u′nj denote respectively approximations to

    1

    J

    J∑j=1

    uj(·, tn) and uj(·, tn)− < u >n, tn := n4t.

    We have the method: for j = 1, ..., J, ∇ · un+1j = 0, and

    un+1j − unj∆t

    + < u >n ·∇un+1j + (unj− < u >n) · ∇unj(1.2)

    +∇pn+1j − ν∆un+1j −∇ · (νT (l

    n, k′n)∇sun+1j ) = fn+1j .

    The ensemble eddy viscosity parameterization is the coefficient νT (·). Briefly, theKolmogorov-Prandtl relation gives

    νT (·)=Const.l√k′

    l = mixing length of fluctuations,

    k′ = kinetic energy in fluctuations.

    Often extensive (and optimistic) modelling steps are needed to generate repre-sentations of these two quantities, e.g., [34], [29]. Algorithm (1.2) allows directcalculation of both:

    k′ =1

    2|u′|2 and l =

    {either 4x,or |u′|4t .

    This gives

    EEV1: νT = µ14x|u′|, andEEV2: νT = µ2|u′|24t.

    2. Supplementary Material: Further Numerical Tests of EnsembleEddy Viscosity Methods

    In our report, the following tests are presented.Test 1 was for flow between offset cylinders driven by a rotating body force

    (Re = 800).Test 2 compared EEV1 and EEV2 for the same geometry atRe = 800, 1200, 2400

    and constant timestep 4t = 0.025.Test 3 (results given in the supplementary materials) repeated these two tests

    but reinitialized the perturbations at t = 1, 2, 3, · · · . The conclusions regardingstability were not altered by reinitialization.

    Test 4 was an accuracy test with a smooth, known exact solution. In Test 4both EEV1 and EEV2 produced 2 significant digits of accuracy with 4x = 0.1, anacceptable result.

    Test 5 is a flow in a channel with 2 outlets and a constriction from [4, 18, 23].Both EEV1 and EEV2 gave the correct general outlines of the flow (compared toothers published results) and differences in the smaller details of the flow.

  • FURTHER NUMERICAL TESTS OF ENSEMBLE EDDY VISCOSITY METHODS 3

    We performed further tests of EEV1 and EEV2 and variants that, while inter-esting, confirmed or were consistent with the preliminary results presented in ourreport. We present some of these explorations in this supplementary section.

    Test 1: Stability of no EEV vs. EEV2 for flow between offset circles.Recall that the domain is

    Ω = {(x, y) : x2 + y2 ≤ r21 and (x− c1)2 + (y − c2)2 ≥ r22}

    a disk with a smaller, off-center obstacle inside with no-slip boundary conditionson both circles. Let r1 = 1, r2 = 0.1, c = (c1, c2) = (

    12 , 0). The flow is driven by:

    f(x, y, t) = (−4y ∗ (1− x2 − y2), 4x ∗ (1− x2 − y2))T .

    The mesh has n = 40 mesh points around the outer circle and m = 10 mesh pointsaround the immersed circle, and extended to Ω as a Delaunay mesh. We begin withRe = 800 and then increase Re.

    Generation of the initial conditions. Perturbations of u0j , j = 1, 2, and u00

    (with � ≡ 0, ‘no perturbation’), are generated by solving the steady Stokes problemon the same geometry with � = 10−3 and

    f1(x, y, t) = f(x, y, t) + � ∗ (sin(3πx)sin(3πy), cos(3πx)cos(3πy))T ,f2(x, y, t) = f(x, y, t)− � ∗ (sin(3πx)sin(3πy), cos(3πx)cos(3πy))T ,

    The Navier-Stokes equations are then solved with these initial conditions, givingu1, u2, uave = (u1 + u2)/2 and u0 (initial condition u

    00 -‘no perturbation’).

    Quantities plotted. The report gave plots of volume averaged statistics. Herewe supplement these with streamlines and contour plots of vorticity over 0 ≤ t ≤ 10. The timestep is adapted as in the report. First we plot total energy dissipationrates of EEV2 and noEV and power input rates of both.

    Next plotted is EEV2 and noEV velocity vectors at ν = 1/800. Note that at thisReynolds number the flow already begins to have interesting features and that thenoEV velocities begin to exhibit radial oscillations.

    This pattern is confirmed by the contour plots of vorticity. The noEV vorticitycontours reveal small scale oscillations clearly.

    Next the Reynolds number was increased to Re = 1200 and 2400. We observedthat EEV2 remained stable with 4t = 0.05 at both Re = 1200 and 2400. WithNoEV, adapting the timestep ensured stability but forced a very small timestepand execution time so long that the method failed to reach the final time. TheEEV2 solutions are given below.

    Test 2: Stability of EEV1 vs. EEV2. Test 1 was repeated comparingEEV1 and EEV2 for Re = 800 and constant timestep. We take ∆t = 0.025, Re =800, µ2 = 1, µ1∆x = 0.2. The streamlines very clearly show that by t = 10.0,the EEV1 approximation returns to the Stokes flow initial condition while EEV2continues its evolution.

    The over diffusion in EEV1 vs. EEV2 is also clear from the kinetic energy plot.Test #3: Re-initialization: We repeat Test 2 but reinitialize the perturbation

    at t = 1, 2, 3, · · ·, restarting with initial data being the average produced up to thatpoint and the same perturbations as at t = 0, as in Test #1. We use the sameconstant timestep ∆t = 0.025, Re = 800, µ2 = 1, µ1∆x = 0.2 . The plots show thatEEV1 results improved somewhat but still EEV1 over-diffuses while EEV2 doesnot.

  • 4 NAN JIANG AND WILLIAM LAYTON

    Dissipation

    0 1 2 3 4 5 6 7 8 9 100

    1

    2

    3

    4

    5

    6

    7

    8

    9

    epsilon1= 0.001, epsilon2= −0.001, Re=800

    time

    Dis

    sip

    atio

    n

    EV2−u

    1

    EV2−u2

    NoEV−u1

    NoEV−u2

    Power Input

    0 1 2 3 4 5 6 7 8 9 100

    1

    2

    3

    4

    5

    6

    7

    8

    9

    epsilon1= 0.001, epsilon2= −0.001, Re=800

    time

    Po

    we

    r In

    pu

    t

    EV2−u

    1

    EV2−u2

    NoEV−u1

    NoEV−u2

    Figure 1. EV2 vs. NoEV: Dissipation & Power Input, ν = 1/800

    References

    [1] O. Axelsson, A survey of preconditioned iterative methods for linear systems of algebraic

    equations, BIT, 25 (1985), 166-187.[2] L.C. Berselli, On the large eddy simulation of the Taylor-Green vortex, J. Math. Fluid

    Mech., 7 (2005), S164-S191.

    [3] L.C. Berselli, T. Iliescu and W. Layton, Mathematics of Large Eddy Simulation ofTurbulent Flows, Springer, Berlin, 2006.

    [4] A.L. Bowers and L.G. Rebholz, Numerical study of a regularization model for incom-

    pressible flow with deconvolution-based adaptive nonlinear filtering, CMAME, 258 (2013),1-12.

    [5] S. Brenner and R. Scott, The Mathematical Theory of Finite Element Methods, Springer,

    3rd edition, 2008.[6] M. Carney, P. Cunningham, J. Dowling and C. Lee, Predicting Probability Distributions

    for Surf Height Using an Ensemble of Mixture Density Networks, International Conference

    on Machine Learning, (2005).[7] M. Case, V. Ervin, A. Linke and L. Rebholz, A connection between Scott-Vogelius ele-

    ments and grad-div stabilization, SINUM 49(2011), 1461-1481.[8] Y.T. Feng, D.R.J. Owen and D. Peric, A block conjugate gradient method applied to linear

    systems with multiple right hand sides, CMAME 127 (1995), 203-215.

  • FURTHER NUMERICAL TESTS OF ENSEMBLE EDDY VISCOSITY METHODS 5

    t=0 t=0.5

    t=5.0 t=10.0

    Figure 2. EV2: Velocity, ν = 1/800

    [9] P.F. Fischer, Projection techniques for iterative solution of Ax=b with successive right-hand

    sides, CMAME, 163, 1998, 193-204.[10] R.W. Freund and M. Malhotra, A block QMR algorithm for non-Hermitian linear systems

    with multiple right-hand sides, Linear Algebra and its Applications, 254, 1997, 119-157.

    [11] E. Gallopulos and V. Simoncini, Convergence of BLOCK GMRES and matrix polynomi-als, Lin. Alg. Appl., 247 (1996), 97-119.

    [12] J.D. Giraldo and S.G. Garćıa Galiano, Building hazard maps of extreme daily rainy

    events from PDF ensemble, via REA method, on Senegal River Basin, Hydrology and EarthSystem Sciences, 15 (2011), 3605-3615.

    [13] M.D. Gunzburger, Finite Element Methods for Viscous Incompressible Flows - A Guide toTheory, Practices, and Algorithms, Academic Press, (1989).

    [14] A.E. Green and G.I. Taylor, Mechanism of the production of small eddies from largerones, Proc. Royal Soc. A., 158 (1937), 499-521.

    [15] J.L. Guermond and L. Quartapelle, On stability and convergence of projection methodsbased on pressure Poisson equation, IJNMF, 26 (1998), 1039-1053.

    [16] T.M. Hamill, J.S. Whitaker, M. Fiorino, S.E. Koch and S.J. Lord, Increasing NOAA’scomputational capacity to improve global forecast modeling, NOAA White Paper, 19 July

    2010.[17] F. Hecht and O. Pironneau, FreeFEM++, http://www.freefem.org.[18] J. Heywood, R. Rannacher and S. Turek, Artificial boundaries and flux and pressure

    conditions for the incompressible Navier-Stokes equations, IJNMF, 22 (1996), 325-352.

    [19] T.J.R. Hughes, A.A. Oberai and L. Mazzei, Large eddy simulation of turbulent channelflows by the variational multiscale method, Phys. Fluids., 13 (2001), 1784-1799.

    [20] T. Iliescu and W. Layton, Approximating the Larger Eddies in Fluid Motion III: theBoussinesq Model for Turbulent Fluctuations, An. St. Univ. ”Al. I. Cuza”, vol. 44, (1998),245-261.

  • 6 NAN JIANG AND WILLIAM LAYTON

    t=0 t=0.540771

    t=5.09414 t=10.0

    Figure 3. NoEV: Velocity, ν = 1/800

    [21] N. Jiang and W. Layton, An algorithm for fast calculation of flow ensembles, submit-ted, April 2013, available at: http://www.mathematics.pitt.edu/sites/default/files/research-

    pdfs/ensemble2April2013.pdf.

    [22] V. John, Large Eddy Simulation of Turbulent Incompressible Flows. Analytical and Nu-merical Results for a Class of LES Models, Lecture Notes in Computational Science and

    Engineering 34, Springer-Verlag, Berlin, 2004

    [23] P. Kuberry, A. Larios, L. Rebholz and N. Wilson, Numerical approximation of the Voigtregularization for incompressible Navier-Stokes and magnetohydrodynamic flows, Comput.

    Math. Appl., 64 (8) (2012), 2647-2662.

    [24] W. Layton and R. Lewandowski, Analysis of an eddy viscosity model for large eddy sim-ulation of turbulent flows, J. Math. Fluid Mechanics, 2 (2002), 374-399.

    [25] O.P. Le Maitre and O.M. Kino, Spectral methods for uncertainty quantification, Springer,Berlin, 2010.

    [26] O.P. Le Maitre, O.M. Kino, H. Najm and R. Ghanem, A stochastic projection method forfluid flow, I. Basic Formulation, JCP, 173 (2001), 481-511.

    [27] W. Layton and L. Tobiska, A Two-Level Method with Backtracking for the Navier–StokesEquations, SINUM, 35 (1998), pp. 2035-2054.

    [28] M. Leutbecher and T.N. Palmer, Ensemble forecasting, JCP, 227 (2008), 3515-3539.[29] R. Lewandowski, The mathematical analysis of the coupling of a turbulent kinetic energy

    equation to the Navier-Stokes equation with an eddy viscosity, Nonlinear Analysis, 28 (1997),393-417.

    [30] J.M. Lewis, Roots of ensemble forecasting, Monthly Weather Rev., 133 (2005), 1865-1885.[31] W.J. Martin and M. Xue, Initial condition sensitivity analysis of a mesoscale forecast using

    very-large ensembles, Mon. Wea. Rev., 134 (2006), 192-207.[32] D.P. O’Leary, The block conjugate gradient algorithm and related methods, Linear Algebra

    and its Applications, 29 (1980), 293–322,[33] M. Olshanskii and A. Reusken, Grad-Div stabilization for the Stokes equations, Math. of

    Comp. 73 (2004) 1699-1718.

  • FURTHER NUMERICAL TESTS OF ENSEMBLE EDDY VISCOSITY METHODS 7

    t=0 t=0.5IsoValue122.656233.046343.437453.827564.217674.608784.998895.3891005.781116.171226.56

    IsoValue25.010947.520770.030592.5403115.05137.56160.07182.579205.089227.599250.109

    t=5.0 t=10.0IsoValue24.412546.383768.354990.3261112.297134.269156.24178.211200.182222.153244.125

    IsoValue27.233451.743576.2535100.764125.274149.784174.294198.804223.314247.824272.334

    Figure 4. EV2: Contours of Vorticity, ν = 1/800

    [34] P. Sagaut, Large eddy simulation for Incompressible flows, Springer, Berlin, 2001.

    [35] D.J. Stensrud, Parameterization schemes: Keys to numerical weather prediction models,

    Cambridge U. Press, 2009.[36] G.I. Taylor, On decay of vortices in a viscous fluid, Phil. Mag., 46 (1923), 671-674.

    [37] Z. Toth and E. Kalney, Ensemble forecasting at NMC: The generation of perturbations,

    Bull. Amer. Meteor. Soc., 74 (1993), 2317-2330.

    (All authors) Dept. of Mathematics, Univ. of Pittsburgh, Pittsburgh, PA 15260, USAE-mail address: [email protected], [email protected]

    URL: www.math.pitt.edu/~wjl

  • 8 NAN JIANG AND WILLIAM LAYTON

    t=0 t=0.540771IsoValue-1226.56-1103.9-981.248-858.592-735.936-613.28-490.624-367.968-245.312-245.312-122.6560122.656245.312367.968490.624613.28735.936858.592981.248

    IsoValue-189.511-170.56-151.609-132.658-113.707-94.7556-75.8045-56.8534-37.9022-37.9022-18.9511018.951137.902256.853475.804594.7556113.707132.658151.609

    t=5.09414 t=10.0IsoValue-218.375-196.537-174.7-152.862-131.025-109.187-87.3498-65.5124-43.6749-43.6749-21.8375021.837543.674965.512487.3498109.187131.025152.862174.7

    IsoValue-144.006-129.605-115.204-100.804-86.4034-72.0028-57.6022-43.2017-28.8011-28.8011-14.4006014.400628.801143.201757.602272.002886.4034100.804115.204

    Figure 5. NoEV: Contours of Vorticity, ν = 1/800

    t=0 t=0.45

    t=5.2 t=10.0

    Figure 6. EEV2: Velocity, ν = 1/1200

  • FURTHER NUMERICAL TESTS OF ENSEMBLE EDDY VISCOSITY METHODS 9

    t=0 t=0.45IsoValue183.984349.57515.155680.741846.3261011.911177.51343.081508.671674.251839.84

    IsoValue10.886120.683630.481140.278650.076159.873669.671179.468689.266199.0636108.861

    t=5.2 t=10.0IsoValue20.454138.862957.271675.680394.0891112.498130.907149.315167.724186.133204.541

    IsoValue22.448942.65362.85783.0611103.265123.469143.673163.877184.081204.285224.489

    Figure 7. EEV2: Contours of Vorticity, ν = 1/1200

    t=0 t=0.523633

    t=5.01582 t=10.0

    Figure 8. EEV2: Velocity, ν = 1/2400

  • 10 NAN JIANG AND WILLIAM LAYTON

    t=0 t=0.523633IsoValue367.968699.1391030.311361.481692.652023.822354.992686.173017.343348.513679.68

    IsoValue13.969326.541739.114151.686464.258876.831289.4036101.976114.548127.121139.693

    t=5.01582 t=10.0IsoValue11.258621.391431.524141.656851.789661.922372.055182.187892.3206102.453112.586

    IsoValue17.067132.427647.78863.148478.508893.8692109.23124.59139.95155.311170.671

    Figure 9. EEV2: Contours of Vorticity, ν = 1/2400

    t=0 t=0.5

    t=5.0 t=10.0

    Figure 10. EV1 gives Stokes flow: Velocity, ν = 1/800

  • FURTHER NUMERICAL TESTS OF ENSEMBLE EDDY VISCOSITY METHODS 11

    t=0 t=0.5

    t=5.0 t=10.0

    Figure 11. EV2: Velocity, ν = 1/800

    t=0 t=0.5IsoValue122.656233.046343.437453.827564.217674.608784.998895.3891005.781116.171226.56

    IsoValue8.7285916.584324.4432.295840.151548.007255.86363.718771.574479.430287.2859

    t=5.0 t=10.0IsoValue0.7643431.452252.140162.828073.515984.203894.891795.57976.267616.955527.64343

    IsoValue0.7643431.452252.140162.828073.515984.203894.891795.57976.267616.955527.64343

    Figure 12. EV1 gives Stokes flow: Contours of Vorticity, ν = 1/800

  • 12 NAN JIANG AND WILLIAM LAYTON

    t=0 t=0.5IsoValue122.656233.046343.437453.827564.217674.608784.998895.3891005.781116.171226.56

    IsoValue15.49529.440543.38657.331671.277185.222699.1681113.114127.059141.005154.95

    t=5.0 t=10.0IsoValue25.540748.527371.513994.5005117.487140.474163.46186.447209.434232.42255.407

    IsoValue24.159345.902667.64689.3893111.133132.876154.619176.363198.106219.849241.593

    Figure 13. EV2: Contours of Vorticity, ν = 1/800

    0 1 2 3 4 5 6 7 8 9 100

    5

    10

    15epsilon1= 0.001, epsilon2= −0.001, dt=0.025, Re=800

    time

    Ener

    gy

    EV1

    EV2

    Figure 14. Energy: EV1 Vs EV2, ∆t = 0.025, ν = 1/800

  • FURTHER NUMERICAL TESTS OF ENSEMBLE EDDY VISCOSITY METHODS 13

    EV1

    0 1 2 3 4 5 6 7 8 9 100

    0.5

    1

    1.5

    2

    2.5

    3

    3.5

    4epsilon1= 0.001, epsilon2= −0.001, dt= 0.025, Re= 800

    time

    An

    gula

    r M

    om

    entu

    m

    u1

    u2

    Average

    no perturbation

    EV2

    0 1 2 3 4 5 6 7 8 9 100

    1

    2

    3

    4

    5

    6

    7epsilon1= 0.001, epsilon2= −0.001, dt= 0.025, Re= 800

    time

    Angula

    r M

    om

    entu

    m

    u1

    u2

    Average

    no perturbation

    Figure 15. Reinitialize: Angular Momentum, ν = 1/800

  • 14 NAN JIANG AND WILLIAM LAYTON

    EV1

    0 1 2 3 4 5 6 7 8 9 100

    1

    2

    3

    4

    5

    6epsilon1= 0.001, epsilon2= −0.001, dt= 0.025, Re= 800

    time

    En

    erg

    y

    u1

    u2

    Average

    no perturbation

    EV2

    0 1 2 3 4 5 6 7 8 9 100

    1

    2

    3

    4

    5

    6

    7

    8epsilon1= 0.001, epsilon2= −0.001, dt= 0.025, Re= 800

    time

    En

    erg

    y

    u1

    u2

    Average

    no perturbation

    Figure 16. Reinitialize: Energy, ν = 1/800

  • FURTHER NUMERICAL TESTS OF ENSEMBLE EDDY VISCOSITY METHODS 15

    EV1

    0 1 2 3 4 5 6 7 8 9 100

    200

    400

    600

    800

    1000

    1200

    1400

    1600

    1800epsilon1= 0.001, epsilon2= −0.001, dt= 0.025, Re= 800

    time

    En

    str

    op

    hy

    u1

    u2

    Average

    no perturbation

    EV2

    0 1 2 3 4 5 6 7 8 9 100

    200

    400

    600

    800

    1000

    1200

    1400

    1600

    1800

    2000epsilon1= 0.001, epsilon2= −0.001, dt= 0.025, Re= 800

    time

    En

    str

    op

    hy

    u1

    u2

    Average

    no perturbation

    Figure 17. Reinitialize: Enstrophy, ν = 1/800

  • 16 NAN JIANG AND WILLIAM LAYTON

    t=0 t=1

    t=5.0 t=10.0

    Figure 18. Reinitialize EV1: Stokes flow velocity, ν = 1/800

    t=0 t=1

    t=5.0 t=10.0

    Figure 19. Reinitialize: EV2: Velocity, ν = 1/800

  • FURTHER NUMERICAL TESTS OF ENSEMBLE EDDY VISCOSITY METHODS 17

    t=0 t=1IsoValue122.656233.046343.437453.827564.217674.608784.998895.3891005.781116.171226.56

    IsoValue1.541392.928644.31595.703157.09048.477659.8649111.252212.639414.026715.4139

    t=5.0 t=10.0IsoValue0.7643431.452252.140162.828073.515984.203894.891795.57976.267616.955527.64343

    IsoValue0.7643431.452252.140162.828073.515984.203894.891795.57976.267616.955527.64343

    Figure 20. Reinitialize: EV1: Contours of Vorticity, ν = 1/800

    t=0 t=1IsoValue122.656233.046343.437453.827564.217674.608784.998895.3891005.781116.171226.56

    IsoValue15.931630.2744.608458.946973.285387.6237101.962116.301130.639144.977159.316

    t=5.0 t=10.0IsoValue19.593237.22754.860972.494790.1286107.762125.396143.03160.664178.298195.932

    IsoValue26.322950.013473.70497.3946121.085144.776168.466192.157215.847239.538263.229

    Figure 21. Reinitialize: EV2: Contours of Vorticity, ν = 1/800

  • 18 NAN JIANG AND WILLIAM LAYTON

    0 1 2 3 4 5 6 7 8 9 100

    1

    2

    3

    4

    5

    6

    7

    8epsilon1= 0.001, epsilon2= −0.001, dt=0.025, Re=800

    time

    Energ

    y

    EV1

    EV2

    Figure 22. Reinitialize: Energy: EV1 Vs EV2, ∆t = 0.025, ν = 1/800