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URANS Simulations of RotorStator Cavity Flow

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Centrifugal forces induce radial outflow near rotor and inflow near stator ... Using laminar viscosity only (deactivating turbulence model) ... – PowerPoint PPT presentation

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Title: URANS Simulations of RotorStator Cavity Flow


1
URANS Simulations of Rotor-Stator Cavity Flow
  • T. J. Craft, S. E. Gant, H. Iacovides, B. E.
    Launder

2
Contents
  • Introduction
  • Experiments
  • Numerical Methods
  • 2-D Steady RANS Results
  • 3-D URANS Results
  • Conclusions

3
Rotor-Stator Cavity
  • Two discs rotor and stator
  • Bottom disc rotates
  • Top disc and walls stationary
  • No through-flow
  • Centrifugal forces induce radial outflow near
    rotor and inflow near stator
  • Relevant to cooling systems in gas turbines

4
Rotor-Stator Cavity Experiments
  • Czarny, Iacovides Launder, 2002
  • Ink injected using hypodermic needle into
    water-filled cavity
  • Coherent structures at certain rotational
    Reynolds numbers/cavity heights

ReWRH/n166,000 H/R0.195
ReWRH/n112,000 H/R0.126
Aim to reproduce coherent structures observed
experimentally using URANS.
5
Numerical Methods 2D Steady Flow
  • TEAM code
  • Finite-volume
  • Staggered velocity/pressure nodes
  • Launder-Sharma k-e turbulence model
  • Numerical wall function which solves
    thin-boundary-layer equations across embedded
    grid.

6
Rotor-Stator 2D Steady Simulations
  • Itoh et al. test case ReWR2/n106, H/R0.08
  • Numerical wall function results agree well with
    full low-Re model
  • No problem with internal corner cells.

7
Rotor-Stator 3D Simulations
  • STREAM code parallelized using domain
    decomposition and MPI
  • 2-block axisymmetric grids running on local linux
    cluster
  • 8-block version running on SGI Origin/Altix at
    CSAR
  • Number of main-grid nodes in (R,q,Z) (60,50,37)
    plus 30 subgrid nodes on each wall.
  • Reynolds Number ReWRH/n112,000
  • Disc spacing H/R0.126

8
Rotor-Stator Quasi-LES
Using laminar viscosity only (deactivating
turbulence model)
Radial velocity isocontours (yellowpositive
bluenegative)
Axial velocity contours near stator surface (at
z/H 0.79)
9
Rotor-Stator Quasi-LES
Using laminar viscosity only (deactivating
turbulence model)
Radial velocity
Tangential velocity
(Profiles taken at r/R0.79, towards the outer
rim of the cavity)
10
Rotor-Stator URANS
Realizable k-e model
Eddy-viscosity contours (red, yellow, green) ?
(40?, 30?, 20?)
Axial velocity contours near stator surface
(scale WRmax 1.0)
11
Rotor-Stator URANS
Realizable k-e model
Radial velocity
Tangential velocity
(Profiles taken at r/R0.79, towards the outer
rim of the cavity)
12
Rotor-Stator URANS
  • Models Tested
  • Linear k-e with/without Yap
  • Realizable k-e
  • Cubic non-linear k-e
  • Linear Production (LP) (Laurence Guimet)
  • Organized Eddy Simulation (OES) (Braza) with Cm
    0.02
  • Filter-based URANS (Johansen et al.)
  • Different Initial Conditions
  • Lower initial turbulence levels
  • Zero initial turbulence levels in core of domain
  • Periodic Disturbances
  • Rotor velocity sinusoidal function or spiked
    profile for W
  • Eccentric axis of rotation (in progress).

13
Rotor-Stator OES
(The only model to show continued presence of
turbulent structures)
Axial velocity near stator surface (at z/H 0.79)
Radial velocity at r/R 0.79
14
Concluding Remarks
  • Standard RANS models are too dissipative to
    simulate 3-D turbulent structures in rotor-stator
    cavity (grid resolution? numerical viscosity?).
  • Eddy structures can be resolved by decreasing the
    eddy-viscosity by a factor of 4.5 (OES) or
    removing it entirely (mt 0) (rigorous model
    definition?).

Future Work
  • Investigate further filter-based LES/URANS model
    of Johansen et al.
  • Grid refinement (although this is costly!)
  • Investigate other LES approaches (LNS, DES etc.)

15
Filter-Based URANS
  • Standard k-e model with clip on mt based on the
    grid dimension, D

where the filter width, D, is given by
L is a characteristic dimension and cD 0.15
  • In the rotor-stator the above formulas lead to
    steady, axisymmetric flow.
  • Testing with cD 0.06 and different formulations
    for smaller D

16
Filter-Based URANS
Using cD 0.15
Radial velocity isocontours (yellowpositive
bluenegative)
Radial velocity at r/R 0.79
17
Subgrid Transport Equations
Simplified low-Re transport equations for U, k,
and T in plane Cartesian coordinates (convection
terms in non-conservative form).
18
Wall Function Generalization to 3-D Flows
  • Generic form of subgrid transport equations (f ?
    U, V, k, e)

where (U, V, W) are grid-aligned contravariant
subgrid velocity components in the (x, h, z)
directions, J is the Jacobian (equivalent to cell
volume), gii and gjj are metric tensors and the
source term C includes pressure gradient,
turbulence-equation sources and geometric terms.
  • Multi-block implementation using subgrid halo
    cells
  • Efficient interpolation scheme to minimize cost
    of calculating geometric terms

z
z
y
h
x
x
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