Gallery of COOLFluiD Results
Chapter 7
Gallery of COOLFluiD results
Although the emphasis of the thesis has been on aerothermodynamics appli- cations, the developments reported in Part I and in Part II Chapter 5 have been used in many other applications, which was also part of this thesis and the main goals of the COOLFluiD project. In this chapter, we present a gallery of CFD simulations that have been performed with COOLFluiD, while reusing some of the functionalities. The aim is to demonstrate the wide range of applicability of the platform and to show how the framework and the many modules implemented during this thesis have been the basis for the developments and research study of many other team members.
7.1 Aeronautics
The FV and RD solvers implemented in this thesis have been applied to solve inviscid flows on complex configurations. Fig. 7.1 shows the solution in terms of Mach number on a Dassault Falcon aircraft at M ∞ = 0.85 and α = 1 o given by the second order FV and RD methods on the same fully tetrahedral mesh.
The result of a more challenging simulation on a F15 geometry (621,636 nodes, 3,558,667 tetrahedral cells) using the first order N scheme with M ∞ = 0.95 and α = 0 o is presented in terms of pressure coefficient C p in Fig. 7.2.
The Mach number field on the windward and leeward sides is shown in Figs.
7.3a and 7.3b.
7.2 Magneto Hydro Dynamics
After having developed the RD solver for Euler equations, we ported some
of the functionalities developed in [8] in order to handle ideal Magnetohy-
drodynamics (MHD) applications. The first and second order solutions of a
MHD flow inside a channel with a sinus bump, computed with the Nc and
(a) Mach field given by LDA/N scheme (b) Mach field given by Roe scheme with LS reconstruction and Barth limiter
Figure 7.1: Mach number isolines/contours in the Euler flow on the Das- sault Falcon at M ∞ = 0.85, α = 1 o .
Bc schemes respectively, are presented in Figs. 7.4a and 7.4b, in terms of density and magnetic field lines (which, in this case, are supposed aligned with the flow).
In [170, 172], the basic explicit/implicit FV solver has been extended to handle ideal MHD applications with an Artificial Compressibility Approach.
In this case, the augmented set of PDE’s equations to solve is given by:
∂
∂t
ρ ρu
B ρE
Φ
+ ∇ ·
ρu
ρuu + (p + B · B/2) ˆ I − BB uB − Bu + IΦ
(ρE + p + B · B/2)u − B(u · B) β 2 B
= 0 (7.1)
where, unlike in the traditional approach based on the non conservative Powell source term to guarantee solenoidality of the magnetic field B, an additional advection equation for the scalar potential function Φ is consid- ered. Herein, β is a reference speed and the total energy can be expressed as
E = p
ρ(γ − 1) + 1 2
�
V 2 + B 2 ρ
�
(7.2)
Figure 7.2: C p distribution in the inviscid flow on a F15 (N scheme) at M ∞ = 0.95, α = 0 o .
(a) View on the windward side (b) View on the leeward side
Figure 7.3: Mach number field on the F15 windward and leeward sides at M ∞ = 0.95, α = 0 o .
The result of the 3D simulation of the interaction between the Solar wind
and the Earth magnetosphere, modeled as a dipole, obtained in [172] by
means of a Lax-Friedrichs scheme with interactively tunable dissipation is
shown in Fig. 7.5a in terms of isolines of magnetic field B. The visual com-
(a) Nc solution (b) Bc solution
Figure 7.4: Density contours and overposed magnetic field lines in the MHD flow inside a channel with a sinusoidal bump.
parison between the numerical solution and the expected flowfield depicted in Fig. 7.5b indicates that the main physical phenomena have been captured correctly.
(a) Isolines of magnetic field in Earth mag- netosphere on the symmetry plane
(b) Schematic of the interaction between Solar wind and Earth magnetosphere
Figure 7.5: Simulation of the interaction between Solar wind and Earth magnetosphere in [172].
7.3 Complex laminar viscous flows
In the context of transition from laminar to turbulent regime, some prelim-
inary work has been conducted on the numerical investigation of roughness
induced vortical structures on a 3D flat plate by [125]. The conditions for
this testcase are: T ∞ = 300 [K], M ∞ = 0.6, Re L = 1289, L = 2 [mm], where
the latter is the size of the roughness. The simulation was run with the im-
plicit Navier-Stokes FV solver on a hexaedral mesh generated with ANSYS Gambit, using AUSM+-up scheme and LS reconstruction. Fig. 7.6a shows the skin friction line pattern around a cubic roughness element on top of a flat plate. The computed laminar solution compares qualitatively reason- ably well with the experimental measurements in Fig. 7.6b, where the flow past the cube is in fact turbulent. More detailed views of the flow near the cubic roughness, on the symmetry plane and on the plate surface, are shown in Figs. 7.7a and 7.7b.
(a) Skin friction line pattern in the com- puted solution
(b) Experimental visualization in oil of the skin friction line pattern
Figure 7.6: Simulation of vortical structures induced by a cubic roughness element on a flat plate at M ∞ = 0.6 and Re L = 1289 in [125].
7.4 Turbulence RANS flows
In [126, 169, 174] some turbulence models were integrated in the COOLFluiD framework and the FV solver was adapted to handle them. This has also of- fered a good occasion to validate our implementation of the Newton method for weakly coupled systems explained in Sec. 5.1.1. The overall linear sys- tem associated to the discretization of the Reynolds Averaged Navier-Stokes equations, in the example of a 2-equation model like k − ω, can be cast as
∂ R ˜
1∂ P
1(P) 0 0
0 ∂ ∂ R P ˜
22
(P) 0
0 0 ∂ ∂ R P ˜
33
(P)
∆P 1
∆P 2
∆P 3
= −
R ˜ 1 (P) R ˜ 2 (P) R ˜ 3 (P)
(7.3)
where the update variables are given by:
(a) Pressure isolines on the symmetry plane (b) Skin friction line pattern on the plate surface and pressure isolines on the symme- try plane
Figure 7.7: Different views of the flow induced by a cubic roughness ele- ment on a flat plate at M ∞ = 0.6 in [125].
P =
P 1
P 2
P 3
, P 1 = (p, u, T ) T , P 2 = k, P 3 = ω (7.4) Herein the weak coupling translates into the fact that the off-diagonal blocks
∂ R ˜
i∂ P
jwith i �= j in the global system matrix can be assumed to be equal to 0, allowing us to solve three independent systems and save memory storage.
The 2D Delery channel testcase has been chosen in [169] to validate the FV solver for turbulent flows. The geometry of the problem is sketched in Fig. 7.8.
The distributions of pressure on the upper and lower wall of the Delery channel given by BSL and SST turbulent models with COOLFluiD are pre- sented in Figs. 7.9a and 7.9b and compared with the corresponding THOR solutions [154] and experimental measurements. The AUSM+-up scheme and LS reconstruction have been used for this simulation.
In particular, for both COOLFluiD and THOR, the SST model shows the
better agreement with the reference experimental data. This is testified by
the good shock capturing exhibited in Fig. 7.10, where the Mach isolines
corresponding to the COOLFluiD solution with SST are plotted.
Figure 7.8: Geometry of the Delery channel.
(a) Distribution on the upper wall (b) Distribution on the lower wall
Figure 7.9: Static pressure distribution on the upper and lower walls of the Delery channel in [169]. Comparison against THOR results and experiments.
7.5 Inductively Coupled Plasma flows
In order to design thermal protection systems for space vehicles prior to
flight, high-temperature wind tunnels have been developed, offering an al-
Figure 7.10: Mach number isolines computed on the Delery channel [169]
at M in = 0.6 with the SST model.
ternative way to the prohibitively expensive option of inflight testing. In ICP torches, the test samples are subjected to a hot plasma jet, which is created by exposing the test gas to an intense electro-magnetic field, gen- erated by a radio-frequency electric current running through an inductor surrounding the plasma torch, as shown in Fig. 7.11.
Figure 7.11: An argon plasma inside the VKI facility.
The induced electric current heats up the gas through Ohmic dissipation to a partially ionized plasma, reaching peak temperatures of approximately 10000K. ICP torches are typically used to perform experimental measure- ments in subsonic chemically reacting boundary layers and stagnation re- gions downstream bow shocks.
In order to validate inhouse experiments, a structured FORTRAN90 code (ICP) for the simulation of axisymmetric plasma flows in thermo-chemical equilibrium or nonequilibrium in ICP torches was developed at the VKI by [7, 94, 140].
Under the author’s supervision, some effort has been devoted to transfer
these simulation capabilities from the ICP code to COOLFluiD [62, 129].
At the time of writing the migration is yet to be completed, but a 2D axisym- metric parallel unstructured LTE-FEF solver for incompressible ICP flows is already available.
In this truly multi-physical case, two subsystems of equations, one corre- sponding to the incompressible Navier-Stokes equations in LTE-FEF (1) and the other one being the magnetic induction (2) equations, are solved in a weakly coupled manner with the implicit Newton procedure explained in Sec. 5.1.1. The global linear system to be solved is
� ∂ R ˜
1∂ P
1(P) 0 0 ∂ ∂ R P ˜
22