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x - ESA Conference Bureau
8th European Symposium on Aerothermodynamics for Space Vehicles NUMERICAL STUDIES OF 3D INSTABILITIES PROPAGATING IN SUPERSONIC COMPRESSION-CORNER FLOW Andrey Novikov, Alexander Fedorov, Ivan Egorov Central Aerohydrodynamic Institute named after prof. N.E. Zhukovsky (TsAGI), Russia Moscow Institute of Physics and Technology (State University) (MIPT), Russia 8th European Symposium on Aerothermodynamics for Space Vehicles Introduction Laminar-turbulent transition (LTT) leads to substantial increase of the surface heating and aerodynamic drag of high-speed vehicles, and affects the efficiency of propulsion system and control surfaces. LTT problem needs clarifying physical mechanisms. Holistic computation of all LTT stages is possible only using DNS, which gives full information about 3D disturbance field and enables to identify and study in detail different LTT mechanisms. Most DNS for hypersonic boundary layers were conducted for simple configurations like a flat plate and a cone at 0 AoA. LTT in locally separated boundary layers is of practical interest. Herein DNS of artificially excited 3D instabilities propagating through the 5.5° compression-corner flow with separation at M∞=5.373 is performed using inhouse solver “HSFlow”. “Young” turbulent wedge is observed in the case of low-frequency forcing. 8th European Symposium on Aerothermodynamics for Space Vehicles Problem formulation 3D Navier-Stokes equations for viscous compressible perfect gas 2 steps calculation: Grid: Laminar steady flow • 87.5×106 nodes Artificial disturbances via (2801x221x141) suction-blowing actuator • 120 lines in BL & separation zone symmetry no-slip, isothermal M∞ = 5.373 Re∞1 = 14.3×106 m-1 L* = 0.316103 m Re∞L = 5.667×106 T∞ = 74.194 K Tw = 300.0 K = 4.043 γ = 1.4; Pr = 0.71 Freestream conditions from 2D calcs suctionblowing • P.Balakumar, H.Zhao, H.Atkins (2005). Stability of Hypersonic Boundary Layers over a Compression Corner. AIAA J. 43(4) • I.Egorov, A.Novikov, A.Fedorov (2006) Numerical Modelling of the Disturbances of the Separated Flow in a Rounded Compression Corner. Fluid Dynamics. 41(4) 8th European Symposium on Aerothermodynamics for Space Vehicles Disturbances generator Periodic suction-blowing through 2 rectangular holes on the wall Boundary condition on mass flow perturbation: V ρv x1 < x < x2 ; z1 < z < z2 ; 0 < t < ∞ x1 x2 h = 0.004075 (h*=1.3 mm) x1=0.0358 (x1*=11.3 mm); x2 = x1+2h; z1 = -h; z2 = h Frequencies: • ω = 450 (f* = 210.02 kHz) – typical for 2nd mode • ω = 125 (f* = 58.37 kHz) – typical for 1st mode Forcing amplitude: ε = 0.001 (linear disturbances evolution) 8th European Symposium on Aerothermodynamics for Space Vehicles Numerical method HSFlow (High-Speed Flow) in-house solver (с) TsAGI Navier-Stokes or Reynolds equations in dimensionless conservative form in curvilinear coordinates Fully implicit finite-volume shock-capturing method, 2ndorder approximation in space and time Godunov-type scheme with Roe approximate Riemann solver, WENO-3 reconstruction to cell edges Newton method for system of discretized grid equations, GMRes algorithm for linear system on each Newton step Structured multi-block grids Block-based parallelisation, MPI & PETSc library of linear algebra subroutines – computations on HPC clusters 8th European Symposium on Aerothermodynamics for Space Vehicles Numerical method validation Flat plate 2nd-mode wave packet evolution generated by short impulse f*=313.48 kHz M∞ = 5.35; Re∞ = 14.3×106 m-1; T∞ = 64.32 K; Tw = 300.0 K; γ = 1.4; Pr = 0.71 Sivasubramanian, J. & Fasel, H.F. (2011) Transition Initiated by a Localized Disturbance in a Hypersonic Flat-Plate Boundary Layer. AIAA paper. 2011-374. [AIAA 2011-374] this work Wall pressure disturbances t = 0.017 ms t = 0.041 ms t = 0.291 ms 8th European Symposium on Aerothermodynamics for Space Vehicles Steady laminar flow field Computations on HPC cluster of Flowmodellium Lab at MIPT using 768 CPU cores shocklet from reattachment region shocklet from separation region bow shock Separation & reattachment xsep = 0.857 xatt = 1.136 0.0010 skin friction coefficient cf 0.0005 0.0000 x 0.2 0.4 0.6 0.8 1.0 1.2 1.4 8th European Symposium on Aerothermodynamics for Space Vehicles (movie) corner flat plate f*=210 kHz ,Wall pressure disturbances Leading wave-packet consists of 1st and 2nd unstable Mack’s mode Finally 2D harmonic disturbance sets in associated with 2nd mode Inside the separation bubble 2nd mode have lower amplitudes as in 2D computations [P.Balakumar, H.Zhao, H.Atkins (2005) AIAA J. 43(4)], [I.Egorov, A.Novikov, A.Fedorov (2006) Fluid Dynamics. 41(4)] 8th European Symposium on Aerothermodynamics for Space Vehicles corner t* = 0.051 ms flat plate f* = 210 kHz ,Wall pressure disturbances Leading wave-packet consists of 1st and 2nd unstable Mack’s mode Finally 2D harmonic disturbance sets in associated with 2nd mode Inside the separation bubble 2nd mode have lower amplitudes as in 2D computations [P.Balakumar, H.Zhao, H.Atkins (2005) AIAA J. 43(4)], [I.Egorov, A.Novikov, A.Fedorov (2006) Fluid Dynamics. 41(4)] 8th European Symposium on Aerothermodynamics for Space Vehicles (movie) corner flat plate f*=58.4 kHz ,Wall pressure disturbances Leading wave-packet and whole disturbance consists mainly of 1st unstable Mack’s mode Disturbances grow rapidly inside the separation bubble and downstream the reattachment line, so that laminar-turbulent transition begins. 8th European Symposium on Aerothermodynamics for Space Vehicles corner flat plate f*=58.4 kHz ,Wall pressure disturbances Leading wave-packet and whole disturbance consists mainly of 1st unstable Mack’s mode Disturbances grow rapidly inside the separation bubble and downstream the reattachment line, so that laminar-turbulent transition begins. 8th European Symposium on Aerothermodynamics for Space Vehicles f*=58.4 kHz, Skin friction distribution cf cf flat plate 0.0030 0.0592 Rex-1/5 laminar disturbed turbulent (correlation) 0.0025 0.0020 laminar disturbed 0.0030 0.0025 0.0020 0.0015 0.0015 transition not finished 0.0010 0.0010 0.0005 0.0005 0.0000 0.0000 x -0.0005 0.2 • corner 0.0035 0.0035 0.4 0.6 0.8 1.0 1.2 cf for disturbed flow – average through instantaneous flow fields 1.4 rapid growth x -0.0005 0.2 0.4 0.6 0.8 1.0 1.2 separation zone length is reduced 8th European Symposium on Aerothermodynamics for Space Vehicles f*=58.4 kHz, Spatial vorticity structures Iso–surfaces of Q–criterion Q=100 colored with x-velocity magnitude flat plate spreading half-angle ≈3° agrees with the experimental data [Fisher, M.C. (1972). Spreading of a Turbulent Disturbance. AIAA J. 10(7)] corner “young” turbulent wedge 8th European Symposium on Aerothermodynamics for Space Vehicles Conclusions Propagation of 3D disturbances through the 5.5° compression-corner flow and flat plate boundary layer at M∞ = 5.373 is numerically simulated. The disturbances are generated by periodic suction-blowing through the hole on the wall. 3D Navier–Stokes equations for viscous compressible perfect gas are solved using the in-house parallel HSFlow solver on a fine grid (87.5×106 nodes). Unstable disturbances are excited relevant to the first and/or second mode of instability. The instabilities evolving through the separation region exhibit nontrivial behaviour, not captured by 2D simulations. “Young” turbulent wedge is observed. Our DNS method resolves fine structures of disturbances on the nonlinear stage of transition. The detailed numerical solutions will be used in future for analysis of space and time spectra as well as average characteristics of the disturbance fields to clarify physical mechanisms of the transition process. • This work was supported by Russian Scientific Foundation grant No.14-19-00821 in Moscow institute of Physics and Technology (State University) (MIPT). 8th European Symposium on Aerothermodynamics for Space Vehicles Ongoing activity DNS on longer computational domain, grid ~250 ×106 nodes Spectral analysis of numerical solutions Comparison with wind-tunnel data flat plate Iso–surfaces of Q– criterion Q=100 colored with xvelocity magnitude