skip to content

NASA Logo

Langley Research Center

Turbulence Modeling Resource


 

Return to: Turbulence Modeling Resource Home Page


 

3DSSD: 3D Supersonic Square Duct Validation Case

The purpose here is to provide a validation case for turbulence models. Unlike verification, which seeks to establish that a model has been implemented correctly, validation compares CFD results against data in an effort to establish a model's ability to reproduce physics. A Fortran program to create nested grids of the same family is provided here if desired. Data are also provided for comparison. For this particular supersonic square duct case (from Davis and Gessner), the data are from experiments.

The experiment utilizes a constant area square duct of height and width D=25.4 mm, with length x/D=50.

The primary focus of this case is to assess turbulence models for internal duct flow with corners. In such cases, turbulent anisotropies can be important because normal stress differences induce flowfield behavior that cannot be captured with models that make use of the Boussinesq assumption.

The reference Mach number is 3.9, and the flow develops over a length of 50 D. As we are interested in comparing data at 50 D, the CFD grid is made slightly longer: 52 D. The walls of the duct are modeled as adiabatic solid walls, although due to symmetry only one quarter of the duct is computed, and symmetry boundary conditions are applied on two boundaries. The following plots shows the layout of this case, along with the boundary conditions. (Note that particular variations of the BCs at the inflow and outflow boundaries may also work and yield similar results for this problem.)

Note: at high Mach numbers (e.g., M > 2), CFD transition to fully turbulent wall-bounded flow can be delayed compared with flow at lower M. Also, the delayed transition location can vary significantly with the freestream levels set. See, for example, Journal of Spacecraft and Rockets, Vol. 47, No. 1, 2010, pp. 11-20 and AIAA Journal, Vol. 47, No. 4, 2009, pp. 982-993 (which is based on AIAA Paper 2008-4403). For this test case, results are only plotted for regions of the flow that were fully turbulent.

3D supersonic square duct grid layout & BCs, part 1

3D supersonic square duct grid layout & BCs, part 2

GRIDS

Some of the experimental data for this case will be shown below. The profiles highlighted here are near the downstream end of the duct at x/D=40 and 50, with a particular focus at x/D=50.

The experimental data reference is: Davis, D. O. and Gessner, F. B., "Further Experiments on Supersonic Turbulent Flow Development in a Square Duct," AIAA Journal, Vol. 27, No. 8, August 1989, pp. 1023-1030, https://doi.org/10.2514/3.10216.

Note that skin friction coefficient values are given here based on Uref and rhoref, for convenience when comparing against CFD results. However, the original reference gives Cf based on local edge velocity and edge density. The translation was accomplished using approximate values taken from figs. 8 and 11(b) of the reference. Also note that all of the experimental data provided here were digitized from figures in the reference, so they should be used with caution.

Exp velocity profiles at x/D=20 Exp velocity profiles at x/D=40

Exp Cf at x/D=40 and 50

A main focus of this case is the ability (or lack thereof) of the turbulence models to capture the secondary flow features. Within a given x=constant plane, the in-plane flow should exhibit flow from the channel center region toward the corners, with two counter-rotating vortical features within each quadrant. The following figure is a very crude representation of the in-plane velocity vectors from fig 5(b) of the experimental reference, showing one quadrant of the duct at x/D=50. This is only an approximation achieved by tracing over parts of the original figure; see the original reference for more details.

Approximation of exp velocity vectors at x/D=50

The experimental data for most of the plots above can be found in the following files: uprofiles_exp.dat, cfinf_exp.dat.
 
 

What to Expect:
RESULTS
LINK TO EQUATIONS
MRR Level
SA
SA eqns
4
SA-QCR2000
SA-QCR2000 eqns
3
SSTm
SSTm eqns
3
SSG/LRR-RSM-w2012
SSG/LRR-RSM-w2012 eqns
3
EASMko2003-S
EASMko2003-S eqns
1
GLVY-RSM-2012
GLVY-RSM-2012 eqns
1

(Other turbulence model results may be added in the future.)

Note that the OVERFLOW code has documented its results for this validation case (for the SA-noft2, SA-noft2-QCR2000, SST, and SST-QCR2000 turbulence models) in NAS Technical Paper 2016-01 (pdf file) (18.3 MB) by Jespersen, Pulliam, and Childs.
 
 

Return to: Turbulence Modeling Resource Home Page


 
 


Recent significant updates:
03/21/2023 - mentioned possible delay in transition to fully turbulent flow at higher M

Privacy Act Statement

Accessibility Statement

Responsible NASA Official: Ethan Vogel
Page Curator: Clark Pederson
Last Updated: 03/21/2023