Direct Numerical Simulation of Pressure Fluctuations Induced by Supersonic Turbulent Boundary Layers

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Direct Numerical Simulation of Pressure Fluctuations Induced by Supersonic Turbulent Boundary Layers PI: Lian Duan --- NSF PRAC 1640865- --- Missouri U. of S&T Project Members: Chao Zhang, Junji Huang, Ryan Krattiger Blue Waters Symposium 2017 Sunriver, OR, USA, May 16-19, 2017 1

Background Boundary-Layer-Induced Pressure Fluctuations Knowledge of pressure distribution in a flow field is a primary concern in many engineering applications Engineering applications - lift and form drag of an aerodynamic body - flow-induced vibration & noise (Blake 1986) - cavitation (Arndt 2002) Theoretical significance - Vorticity dynamics (high vorticity ó low pressure) - turbulence modeling (pressure-strain terms in the transport equacons for the Reynolds stresses) (Pope 2000) Pressure fluctuations from supersonic boundary layers p w : vibrational loading of flight vehicles p : freestream noise of supersonic wind tunnels 2

Background Application: Freestream noise in High-Speed Wind-Tunnel Facilities Acous*c Radia*on Test Rhombus Upstream Disturbance Blanchard et al. 1997 Flow Laminar Tunnel-Wall Boundary Layer Turbulent Tunnel-Wall TransiCon Boundary Layer Shadowgraph of the radiated noise from a Mach 3.5 tunnel-wall turbulent boundary layer (courtesy of NASA Langley) In a conventional tunnel (M > 2.5), tunnel noise is dominated by acoustic radiation from turbulent boundary layers on tunnel side-walls (Laufer, 1964) 3

Motivation Boundary-Layer-Induced Pressure Fluctuations Limited understanding of global pressure field induced by high-speed turbulent boundary layers theory unable to predict detailed pressure spectrum experiment unable to measure instantaneous spatial pressure distribution susceptible to measurement errors (Beresh 2011) numerics largely limited to incompressible boundary layers freestream pressure fluctuations not studied Direct Numerical Simulation (DNS) is used to investigate boundarylayer-induced pressure field statistical and spectral scaling of pressure large-scale pressure structures correlation between regions of extreme pressure and extreme vorticity acoustic radiation in the free stream 4

Focus of Current Project Boundary-Layer-Induced Pressure Fluctuations Develop a DNS database of high-speed turbulent boundary layers (Duan et al., JFM 2014, 2016) across a broad range of freestream Mach number, wall-to-recovery temperature ratio, and Reynolds number Acoustic radiation - M = 2.5-14 - T w /T r = 0.18-1.0 - Re τ 400 2000 turbulent boundary layer with grids designed to adequately capture both the boundary layer and the near field of acoustic fluctuations radiated by the boundary layer Conduct statistical and structural analysis of the global pressure field induced by the boundary layers (Zhang et al., JFM 2017) 5

Why Blue Waters? Boundary-Layer-Induced Pressure Fluctuations World-class computing capabilities of Blue Waters required for DNS of turbulent boundary layers at high Reynolds numbers Extremely fine meshes required to fully resolve all turbulence scales Large domain sizes needed to locate very-large-scale coherent structures large number of time steps required for the study of low-frequency behavior of the pressure spectrum N x N y N z L x /δ i L y /δ i L z /δ i Δx + Δy + Δz + min Δz + max 6700 800 1500 60.0 6.0 30.0 6.5 5.0 0.51 5.33 Estimated computation size for DNS of a supersonic turbulent BL at Re τ = 2000 Total number of meshes: ~ 8.0 billion Single flow field data size: ~ 320 GB Production runs require up to ~10% of the total XE nodes of Blue Waters require up to 2,000 compute nodes belong to the capability class of petascale computing 6

DNS methodology DNS code porting Outline Domain Decomposition Strategy Profiling & Parallel Performance Parallel Input/Output (IO) Results of Domain Science Boundary-layer-induced pressure statistics & structures Boundary-layer freestream radiation Summary and future work 7

Background DNS for Compressible Turbulent Boundary Layers Conflicting requirements for numerical schemes Shock capturing requires numerical dissipation Turbulence needs to reduce numerical dissipation Starting a simulation from a laminar/random initial condition very costly hard to control final flow conditions Require continuous inflow conditions Boundary layer is inhomogeneous in the streamwise direction 8

Hybrid WENO/Central Difference Method High-order non-dissipative central schemes for capturing broadband turbulence (Pirozzoli, JCP, 2010) DNS Methodology Numerical Methods Weighted Essentially Non-Ocillatory (WENO) adaptation for capturing shock waves (Jiang & Shu JCP 1996, Martin et al. JCP, 2006) Rely on a shock sensor to distinguish shock waves from smooth turbulent regions - physical shock sensor based on vorticity and dilatation (Ducro, JCP, 2000) - numerical shock sensor based on WENO smoothness measurement and limiter (Taylor et al, JCP 2007) 9

DNS Methodology Inflow turbulence generation Recycling-rescaling (RR) based method (Xu & Martin Phys Fluids, 2004) based on recycling and rescaling turbulence structures within the DNS/LES domain an equilibrium region required to invoke scaling arguments Digital-filtering (DF) based method (Touber & Sandham, Theor. Compt. Fluid Dyn. 200 inflow mean flow and Reynolds-stress profiles required from RANS inflow profiles seeded RR DF (Huang & Duan, AIAA 2016-3639) 10

DNS Methodology Software Structure Flow chart of the code Programming language and model Fortran 2003 Parallel MPI-only I/O in parallel HDF5

DNS Methodology Domain Decomposition 2D domain decomposition z pencil used z is the wall-normal direction y z x computaconal domain copied part of computaconal domain ghost cells Static data decomposition and ghost cell update between four processors

DNS Methodology Software Profiling Total compute *me breakdown (6400x320x500) Total compute *me breakdown (6400x1280x500) 100% 80% 60% 40% 20% 0% 100% 80% 60% 40% 20% 0% XE Nodes: 250 nodes, 8000 cores Pencil size: 16x16x500 Computing time: 90% IO time: 3% XE Nodes: 1000 nodes, 32000 cores Pencil size: 16x16x500 Computing time: 76% IO time: 13% 13

Strong Scaling (Total Time) DNS Methodology Parallel Performance Weak Scaling (Total Time) Software scales well up to 500 XE nodes (16,000 cores) Scalability deteriorate at 1,000 XE nodes (32,000 cores) 14

Strong Scaling (Computation Time only) DNS Methodology Computation Performance Weak Scaling (Computation Time only) Computation scales well to 1000 XE nodes (32,000 cores) 15

Weak Scaling (I/O Time only) DNS Methodology IO Performance Parallel IO: parallel HDF5 Pencil size: 16x16x500 Data Size/core: 7.6 MB on each core Stripe count = 4 IO Scalability deteriorate at 1,000 XE nodes (32,000 cores) 16

Results of Domain Science Multivariate statistics and structure of global pressure field induced by high-speed turbulent BLs 17

(a) Wall (b) z ref /δ = 0.15 Spatial Pressure Structure M = 5.86, T w /T r = 0.25 Re τ = 450 (Zhang et al. JFM 2017) C pp ( Δx, Δy, z, z p'( x, y, z ref ) =, t) p'( x + Δx, y + Δy, z, t) ref 2 2 2 ( p' ( x, y, z, t) ) ( ) 1/ p' ( x x, y y, z, t) 1/ 2 ref + Δ + Δ (c) z ref /δ = 0.73 (d) Free stream

Freestream Acoustic Radiation M = 5.86, T w /T r = 0.25, Re τ = 450 (Zhang et al. JFM 2017) Gray contours: density gradient Color contours: magnitude of vorticity

Spatial-Temporal Correlation of Pressure Structures pressure structure at t = 0, x = 0 C pp (Δx, 0, 0) with zero time delay pressure structure at t = Δt, x = U c Δt (i) frozen propagation (Taylor s hypothesis) (ii) non-frozen propagation (Propagation + Evolution) (correlation decays) C pp (Δx, 0, 0) with time delay Δt U c Δt Space-time correlation C pp (Δx, 0, 0, Δt) 20

Propagation of Pressure Structures M = 5.86, T w /T r = 0.25, Re τ = 450 (Zhang et al. JFM 2017) Propagation speed defined by finding a value of U c that minimizes the difference between the real time evolution of p(x, t) and a frozen wave p(x U c t) (Del Alamo & Jimenez, JFM 2009) U c ( p / t)( p / x) ( p / x) 2 Within most of the boundary layer, U c <u> (similar to incompressible flow results by Kim & Hussain 1993) In the free stream, U c departs from Taylor s hypothesis and is significantly lower than the local mean velocity <u> 21

C pp (Δx, 0, 0, Δt) Evolution of Pressure Structures M = 5.86, T w /T r = 0.25, Re τ = 450 (Zhang et al. JFM 2017) Δt=0 Curve of maximum correlation (C pp ) max Δx (C pp ) max measures the rate of evolution and defines the Lagrangian decorrelation length of coherent pressure structures or wavepackets 22

Sources of Freestream Acoustic Radiation M = 5.86, T w /T r = 0.25, Re τ = 450 (Zhang et al. JFM 2017) Acoustic analogy (Phillips 1960) D 2 Dt 2 Wave Operator @ a 2 @ p log @x i @x i Linear source @u i @u j = 2 @U @x j @x i @z p 0 Acoustic source term = @u i @u j, @x j @x i Nonlinear source @w 0 @x + @u0 @u 0 i j @x j @x i Nonlinear source (NLS) dominates over linear source (LS) Total acoustic source term peaks in the buffer layer (z + pk 20) 23

Summary Cutting-edge computational power of the Blue Waters is used to generate a DNS database of high-speed turbulent boundary layers M = 2.5 14 T w /T r = 0.18-1.0 Re τ 400 2000 DNS database is used to study the boundary-layer-induced global pressure field pressure statistics and structures freestream acoustic radiation DNS code is being modernized on the Blue Waters to enable petascale simulations at higher Reynolds numbers Software profiling Parallel I/O Hybrid MPI-OpenMP 24

Future Work Conduct DNS of supersonic turbulent boundary layers at Re τ 2000 investigate statistical and spectral scaling of the global pressure field dependence of the induced pressure field on Reynolds number DNS code modernization hybrid MPI-OpenMP parallel structure An additional dimension of domain decomposition 25

MPI-OpenMP Hybridization Thread level pencils, here called windows Computational Domain MPI rank Pencil MPI ranks decomposeinto pencils (2D decomposition) Thread Current work

Acknowledgment Dr. Meelan Choudhari at NASA Langley Research Center for collaboration Funding Support AFOSR (Award No. FA9550-14-1-0170) NASA (Cooperative Agreement No. NNL09AA00A) Computing resources NCSA through NSF PRAC (Award No. ACI-1640865) DoD High Performance Computing Modernization Program NASA Advanced Supercomputing Division 27

Publications J. Huang and L. Duan, Turbulent Inflow Generation for Direct Simulations of Hypersonic Turbulent Boundary Layers and Their Freestream Acoustic Radiation, AIAA Paper 2016-3639, 46th AIAA Fluid Dynamics Conference, Washington, DC, June, 2016. http://arc.aiaa.org/doi/abs/10.2514/6.2016-3639 C. Zhang and L. Duan, Multivariate Statistics Analysis of the Pressure Field Induced by High-Speed Turbulent Boundary Layers, AIAA Paper 2016-3090, 46th AIAA Fluid Dynamics Conference, Washington, DC, June, 2016. http://arc.aiaa.org/doi/abs/10.2514/6.2016-3190 L. Duan, M. M. Choudhari and C. Zhang, Pressure fluctuations induced by a hypersonic turbulent boundary layer. Journal of Fluid Mechanics, 2016, 804, 578-607. C. Zhang, L. Duan and M. M. Choudhari, Effect of wall cooling on boundary-layer-induced pressure fluctuations at Mach 6, Journal of Fluid Mechanics, in press, 2017.

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Taylor, E. M., Wu, M., & Martín, M. P. (2007). Optimization of nonlinear error for weighted essentially non-oscillatory methods in direct numerical simulations of compressible turbulence. Journal of Computational Physics, 223(1), 384-397. Ducros, F., Laporte, F., Souleres, T., Guinot, V., Moinat, P., & Caruelle, B. (2000). High-order fluxes for conservative skew-symmetric-like schemes in structured meshes: application to compressible flows. Journal of Computational Physics, 161(1), 114-139. Xu, S., & Martin, M. P. (2004). Assessment of inflow boundary conditions for compressible turbulent boundary layers. Physics of Fluids, 16(7), 2623-2639. Del Álamo, J. C., & Jiménez, J. (2009). Estimation of turbulent convection velocities and corrections to Taylor's approximation. Journal of Fluid Mechanics, 640, 5-26. Kim, J., & Hussain, F. (1993). Propagation velocity of perturbations in turbulent channel flow. Physics of Fluids A: Fluid Dynamics, 5(3), 695-706. Phillips, O. M. (1960). On the generation of sound by supersonic turbulent shear layers. Journal of Fluid Mechanics, 9(01), 1-28. 30

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