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Langley Research CenterTurbulence Modeling Resource |
Exp: NASA Juncture Flow (JF) - Turbulent Symmetric Wing
Return to: Exp: NASA Juncture Flow - Intro Page
Return to: Data from Experiments - Intro Page Return to: Turbulence Modeling Resource Home PageThis is a sub-page of the
NASA Juncture Flow (JF) website.
These data are from the Phase 3 TURBULENT testing on a symmetric wing shape.
The wing itself is a blend of NACA 0015 at the root,
NACA 0012 mid-span, and NACA 0010 near the tip. The wing also includes a horn
(a fillet or extension between the wing and body at the wing leading edge, whose
purpose is to eliminate or lessen the strength/influence of the horseshoe vortex).
This symmetric wing produces a much smaller separation than on
the F6-based wing, helping explore the ability of CFD to capture incipient separation.
Some relevant information is given here.
1Because the crank chord was
different between the F6-based wing and the symmetric wing, the Reynolds number
per mm was different (
4307.4515
for the F6-based wing and
4132.8291
for the symmetric wing ).
TURBULENT SYMMETRIC WING GEOMETRY
TURBULENT SYMMETRIC WING BOUNDARY CONDITIONS
TURBULENT SYMMETRIC WING EXPERIMENTAL DATA
LINK TO EXISTING TURBULENT
SYMMETRIC WING CFD GRIDS AND SOLUTIONS
Return to: Exp: NASA Juncture Flow - Intro Page
Responsible NASA Official:
Ethan Vogel
2For the purpose of maintaining some consistency between input parameters for nondimensional CFD codes,
the nominal M and T were chosen to be the same between the F6 and symmetric wing
(because they were both well within the ranges experienced during each test).
However, note that the velocity and Q end up to be somewhat different for the two wings because of the
different unit Reynolds numbers.
Page Curator:
Clark Pederson
Last Updated: 03/13/2023