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Langley Research CenterTurbulence Modeling Resource |
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2D Zero Pressure Gradient High Mach Number Flat Plate Validation Case
EASMko2003-S Model Results
Link to EASMko2003-S equations
Note that thorough
grid studies were not performed for validation cases such as this one.
Some effort was made to ensure reasonable grid resolutions, but there may still be
small noticeable discretization errors. Therefore, these validation results shown should be considered
representative, but not "truth."
Above results are from CFL3D on the 545x385 grid.
Note, however, that for these high-speed cases the computed variable
Note that this model is currently assigned
MRR Level 1 for the purposes of this website.
This is because at this time the TMBWG has results for this model
from only one code. The results on this page are therefore not necessarily
reliable until additional independent code(s) can be used to verify the model implementation.
Jump to: SA Results,
SST-Vm Results,
Wilcox2006-klim-m Results,
K-e-Rt Results Return to: High Mach Number Flat Plate Validation Intro Page Return to: Turbulence Modeling Resource Home Page
Responsible NASA Official:
Ethan Vogel
is limited to 0.025 (rather than 0.0005).
CFL3D used freestream turbulence intensity=0.004% (M=2) and 0.002% (M=5) and freestream turbulent viscosity (relative to laminar)=0.009
(additional details can be found in the CFL3D User's Manual, Appendix H).
Please read note 5 on Notes on running CFD page.
The right-hand plot is extracted from the location where Retheta=10000.
Note that these are
compressible code results using no compressibility corrections.
Furthermore, as for other two-equation model cases posted on the TMR website, the
term in the production was ignored (often the default for codes whose predominant applications are low-speed
or transonic cases).
Generally speaking, for high-speed cases, this term could be significant.
However, testing for the 2DZPH case with the SST-Vm model
has shown that including
or ignoring this term only makes relatively minor differences
(on the order of the differences seen between the codes).
Page Curator:
Clark Pederson
Last Updated: 03/23/2021