# Numerical Simulation on the Effect of Turbulence Models on Impingement Cooling of Double Chamber Model

Authors: Zhenglei Yu; Tao Xu; Junlou Li; Hang Xiu; Yun Li
Journal: Mathematical Problems in Engineering
 (2013)

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## Abstract

Investigation of the effects of impingement cooling for the different turbulence models and study of the aerodynamic behavior of a simplified transition piece model (TP) are the two themes of this paper. A model (double chamber model) of a one-fourth cylinder is designed which could simulate the transition piece structure and performance. The relative strengths and drawbacks of renormalization group theoryk-ε (RNG), the realizable k-ε (RKE), the v2-f, the shear stress transport k-ω (SST), and large-eddy simulation (LES) models are used to solve the closure problem. The prediction of the inner wall temperature, cooling effectiveness, and velocity magnitude contours in various conditions are compared in five different turbulence models. Surprisingly, the v2-f and SST models can produce even better predictions of fluid properties in impinging jet flows. It is recommended as the best compromise between solution speed and accuracy.


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## Body

## 1. Introduction

Given the large number of sustained operational hours required for industrial turbines, two important demands placed on such engines are component life and overall engine performance. These demands are somewhat conflicting because high temperatures are required at turbine combustor in order to achieve high performance; however, increasing combustor outlet temperature in turn reduced component life, high repair costs, and downtime costs. Impingement cooling is an enhanced heat transfer method capable of cooling a transition piece (TP) without injecting cool air directly into the gas chamber. Cooling the transition piece from the gas inlet enables engineers to dissipate the heat load and maintains more uniform temperatures in the turbine region needed for efficient turbine [1].In the example of turbine cooling applications [2], impinging jet flows may be used to cool several different sections of the engine such as the combustor case (combustor can walls), turbine case/liner, and the critical high temperature turbine blades. General applications and performance of impinging jets had been discussed in a number of reviews [3–6]. The jet impingement angle has an effect on heat transfer and was studied frequently [3, 4]. Göppert et al. [5] investigated the effects of an unstable precessing jet over a fixed target plate. Hwang et al. [6] altered the flow pattern in the initial shearing layer by using coaxial jets.Numerical modeling of impinging jet flows and heat transfer is employed widely for prediction, sensitivity analysis, and device design. Finite element, finite difference, and finite volume computational fluid dynamics (CFD) models of impinging jets have succeeded in making rough predictions of heat transfer coefficients and velocity fields. Turbulent impinging jet CFD employs practically all available numerical methods that will be critically reviewed in the following sections.An earlier critical review of this topic was conducted by Polat et al. [7] in 1989. Since that date, the variety of numerical models have been established and computational research in predicting the physical behavior of impinging jets. Tzeng et al. [8] compared seven low Re modifications of the k-ε model using a confined turbulent slot jet array problem with three adjacent jets at H/B=1. Heck et al. [9] showed the RNG model that provided a close match of Nu in the wall-jet region but an error up to 10% in the stagnation region. Modeling by Cziesla et al. [10] demonstrated the ability of LES to predict local Nu under a slot jet within 10% of experimental measurements. Silieti et al. [11] investigated the numerical prediction of cooling effectiveness in 2D and 3D gas turbine end walls/shrouds for the cases of conjugate and adiabatic heat transfer models. They considered different cooling hole geometries, that is, cooling slots, cylindrical, and fan-shaped cooling holes at different blowing ratios. They incorporated the effects of different turbulence models in predicting the surface temperature and hence the cooling effectiveness.There is a great interest in the application of impingement cooling to protect the transition piece from high temperature gas streams. The model created in the paper looks like a quarter torus with the curved double chambers simulating the structure of the transition piece. The relative strengths and drawbacks of renormalization group theoryk-ε model (RNG), the realizable k-ε model (RKE), the v2-f model, the shear stress transport k-ω model (SST), and large-eddy simulation model (LES) for impinging jet flow and heat transfer are compared. As well, the velocity and temperature fields, in addition to centerline and two-dimensional impingement cooling effectiveness, will be presented.


## 2. Turbulence Models

### 2.1. The Renormalization Group Theoryk-ε Model (RNG)

The RNGk-ε turbulence model is derived from the instantaneous Navier-Stokes equations, using a mathematical technique called renormalization group (RNG) methods, borrowed from quantum mechanics. The analytical derivation results in a model with constants different from those in the standard k-ε model, and it results in additional terms and functions in the transport equations for the turbulent kinetic energy (k) and for dissipation rate (ε). A more comprehensive description of RNG theory and its application to turbulence can be found in [12, 13]. The governing equations for this model are as follows:k equation
(1)ρDkDt=∂∂xj[(μ+μtσk)∂k∂xj]+μtS2-ρε-giμtρPrk∂ρ∂xi-2ρεkγRT,ε equation
(2)ρDεDt=∂∂xj[(ατμeff)∂ε∂xj]+εk(C1τμτS2-ρεC2τ*),
where D/Dt is the convective (or substantial time) derivative,
(3)DDt=∂∂t+V→·∇,
and S is related to the mean strain tensor, Sij=(1/2)(∂ui/xj+∂uj/xi), as S=2SijSji, C1τ=1.42, C2τ=1.68,   Cμ=0.0845,  η=S(k/ε), μt=ρCμ(k2/ε), and C2τ*=C2τ+((Cμρη3(1-(η1/η0)))/(1+βη3)).


### 2.2. The Realizablek-ε Model (RKE)

The term realizable means that the model satisfies certain mathematical constraints on the normal stresses consistent with the physics of turbulent flows. In this model, thek equation is the same as in RNG model; however Cμ is not a constant and varies as a function of mean velocity field and turbulence (0.09 in log-layer S(k/ε)=3.3, 0.05 in shear layer of S(k/ε)=6). The equation is based on a transport equation for the mean-square vorticity fluctuation [14] as
(4)ρDεDt=∂∂xj[(μ+μtσ)∂ε∂xj]+C1Sρε-C2ρε2k+ve,
where C1=max[0.43,η/(η+1)] and C2=1.0. This model is designed to avoid unphysical solutions in the flow field.


### 2.3. Thev2-f Model

Durbin'sv2-f model, also known as the “normal velocity relaxation model,” has shown some of the best predictions to date, with calculated Nu values falling within the spread of experimental data [15]. The v2-f model uses an eddy viscosity to increase stability with two additional differential equations beyond those of the k-ε model, forming a four-equation model. The additional equations are defined as
(5)DkDt=∂∂xj[(v+v′)∂k∂xj]+2v′SijSij-ε,v′=Cμv2¯Tscale,DεDt=cε1′2v′SijSij-cε2εTscale+∂∂xj[(v+v′σε)∂ε∂xj],Dv2¯Dt=kfwall-v2¯εk+∂∂xj[(v+v′)∂v2¯∂xj],fwall-Lscale2∂∂xj∂f∂xj=(C1-1)((2/3)-(v2¯/k))Tscale+C22v′SijSijk,Lscale=CLmax(min(k3/2ε,13k3/2v2¯Cμ2SijSij),Cμ(v3ε)1/4min(k3/2ε,13k3/2v2¯Cμ2SijSij)),Tscale=min(max(kε,6vε),α3kv2¯Cμ2SijSij),cε1′=1.44(1+0.045kv2¯),
where Cμ=0.19, cε2=1.9, σε=1.3, C1=1.4, C2=0.3, Cη=70.0, CL=0.3, and α=0.6. Similar equations exist for predicting the transport of a scalar (e.g., thermal energy) with a Pr′ as a funtion of v and v′.


### 2.4. The Shear Stress Transportk-ω Model (SST)

There are two major ways in which the SST model differs from the standardk-ω model. The first is the gradual change from the standard k-ω model in the inner region of the boundary layer to a high Reynolds-number version of the k-ε model in the outer part of the boundary layer. The second is the modified turbulent viscosity formulation to account for the transport effects of the principal turbulent shear stress. The SST (shear stress transport) model consists of the zonal (blended) k-ω/k-ε equations and clips of turbulent viscosity so that turbulent stress stays within what is dictated by structural similarity constant. The k equation is the same as the standard k-ω model whereas the resulting blended equation for ω is [16]
(6)ρDωDt=γvtτij∂Ui∂xj-ρβω2+∂∂xj[(μ+μτσω)∂ω∂xj]+2ρ(1-F1)σω21ω∂k∂xj∂ω∂xj,
where F1=1 in the inner layer and F1→0 in the outer layer, and σω2=1.168.


### 2.5. Large-Eddy Simulation (LES)

Large-eddy simulation (LES) is a technique intermediate between the direct simulation of turbulent flows and the solution of the Reynolds-averaged equations. In LES the contribution of the large, energy-carrying structures to momentum and energy transfer is computed exactly; well only the effect of the smallest scales of turbulence is modeled. Since the small scales tend to be more homogeneous and universal and less affected by the boundary conditions than the large ones, there is hope that their models can be simpler and require fewer adjustments when applied to different flows than similar models for the RANS equations [17, 18].


## 2.1. The Renormalization Group Theoryk-ε Model (RNG)

The RNGk-ε turbulence model is derived from the instantaneous Navier-Stokes equations, using a mathematical technique called renormalization group (RNG) methods, borrowed from quantum mechanics. The analytical derivation results in a model with constants different from those in the standard k-ε model, and it results in additional terms and functions in the transport equations for the turbulent kinetic energy (k) and for dissipation rate (ε). A more comprehensive description of RNG theory and its application to turbulence can be found in [12, 13]. The governing equations for this model are as follows:k equation
(1)ρDkDt=∂∂xj[(μ+μtσk)∂k∂xj]+μtS2-ρε-giμtρPrk∂ρ∂xi-2ρεkγRT,ε equation
(2)ρDεDt=∂∂xj[(ατμeff)∂ε∂xj]+εk(C1τμτS2-ρεC2τ*),
where D/Dt is the convective (or substantial time) derivative,
(3)DDt=∂∂t+V→·∇,
and S is related to the mean strain tensor, Sij=(1/2)(∂ui/xj+∂uj/xi), as S=2SijSji, C1τ=1.42, C2τ=1.68,   Cμ=0.0845,  η=S(k/ε), μt=ρCμ(k2/ε), and C2τ*=C2τ+((Cμρη3(1-(η1/η0)))/(1+βη3)).


## 2.2. The Realizablek-ε Model (RKE)

The term realizable means that the model satisfies certain mathematical constraints on the normal stresses consistent with the physics of turbulent flows. In this model, thek equation is the same as in RNG model; however Cμ is not a constant and varies as a function of mean velocity field and turbulence (0.09 in log-layer S(k/ε)=3.3, 0.05 in shear layer of S(k/ε)=6). The equation is based on a transport equation for the mean-square vorticity fluctuation [14] as
(4)ρDεDt=∂∂xj[(μ+μtσ)∂ε∂xj]+C1Sρε-C2ρε2k+ve,
where C1=max[0.43,η/(η+1)] and C2=1.0. This model is designed to avoid unphysical solutions in the flow field.


## 2.3. Thev2-f Model

Durbin'sv2-f model, also known as the “normal velocity relaxation model,” has shown some of the best predictions to date, with calculated Nu values falling within the spread of experimental data [15]. The v2-f model uses an eddy viscosity to increase stability with two additional differential equations beyond those of the k-ε model, forming a four-equation model. The additional equations are defined as
(5)DkDt=∂∂xj[(v+v′)∂k∂xj]+2v′SijSij-ε,v′=Cμv2¯Tscale,DεDt=cε1′2v′SijSij-cε2εTscale+∂∂xj[(v+v′σε)∂ε∂xj],Dv2¯Dt=kfwall-v2¯εk+∂∂xj[(v+v′)∂v2¯∂xj],fwall-Lscale2∂∂xj∂f∂xj=(C1-1)((2/3)-(v2¯/k))Tscale+C22v′SijSijk,Lscale=CLmax(min(k3/2ε,13k3/2v2¯Cμ2SijSij),Cμ(v3ε)1/4min(k3/2ε,13k3/2v2¯Cμ2SijSij)),Tscale=min(max(kε,6vε),α3kv2¯Cμ2SijSij),cε1′=1.44(1+0.045kv2¯),
where Cμ=0.19, cε2=1.9, σε=1.3, C1=1.4, C2=0.3, Cη=70.0, CL=0.3, and α=0.6. Similar equations exist for predicting the transport of a scalar (e.g., thermal energy) with a Pr′ as a funtion of v and v′.


## 2.4. The Shear Stress Transportk-ω Model (SST)

There are two major ways in which the SST model differs from the standardk-ω model. The first is the gradual change from the standard k-ω model in the inner region of the boundary layer to a high Reynolds-number version of the k-ε model in the outer part of the boundary layer. The second is the modified turbulent viscosity formulation to account for the transport effects of the principal turbulent shear stress. The SST (shear stress transport) model consists of the zonal (blended) k-ω/k-ε equations and clips of turbulent viscosity so that turbulent stress stays within what is dictated by structural similarity constant. The k equation is the same as the standard k-ω model whereas the resulting blended equation for ω is [16]
(6)ρDωDt=γvtτij∂Ui∂xj-ρβω2+∂∂xj[(μ+μτσω)∂ω∂xj]+2ρ(1-F1)σω21ω∂k∂xj∂ω∂xj,
where F1=1 in the inner layer and F1→0 in the outer layer, and σω2=1.168.


## 2.5. Large-Eddy Simulation (LES)

Large-eddy simulation (LES) is a technique intermediate between the direct simulation of turbulent flows and the solution of the Reynolds-averaged equations. In LES the contribution of the large, energy-carrying structures to momentum and energy transfer is computed exactly; well only the effect of the smallest scales of turbulence is modeled. Since the small scales tend to be more homogeneous and universal and less affected by the boundary conditions than the large ones, there is hope that their models can be simpler and require fewer adjustments when applied to different flows than similar models for the RANS equations [17, 18].


## 3. Computational Model, Boundary Conditions, and Grid

### 3.1. Model Description

Transition piece develops heat transformation on both internal and external walls to eliminate resonant frequency concerns. As well the transition piece conducts gas flow directly from the corresponding combustion liners toward the first stage of the gas turbine (stator). The discrete coolant jets, forming a protective film chamber on the side of transition piece, are drawn from the upstream compressor in an operational gas turbine engine. From the supply plenum, the coolant is ejected through the several rows of discrete holes over the external boundary layer against the local high thermal conduction on the other side of the transition pieces [19]. The model, as a one-fourth cylinder, could simulate the transition piece’s structure and performance, to elaborate the turbulence effect on the impingement-cooling performance over a concave surface (see Figure 1) [4].Figure 1
Impingement-cooling concave model.A schematic diagram of the flow domain along with boundary conditions and dimensions is given in Figure2(a). As shown in the figure, the one-fourth cylinder model has two layers of chambers with a length of 1050 mm and an outer radius and an inner radius of 200 mm and 162 mm, respectively. In the diagram, one side of the outer chamber called the coolant chamber is closed; contrarily, both sides of the mainstream chamber as the inner chamber are unfolding in which gas could flow through from one side to the other. There are 18 holes distributed uniformly in three rows on the surface of the outer wall. The distance between the two rows is 68 mm and the diameter of all the holes is about 10.26 mm. In this scenario, the velocity of the coolant flow is set at 6 m/s; the temperatures of the coolant flow and the mainstream flow are set as 300 K and 1300 K, respectively.Computational domain showing boundary conditions.
(a)
(b)


### 3.2. Boundary Conditions

Boundary conditions are applied to specific faces within the domain to specify the flow and thermal variables that dictate conditions within the model. Figure2(a) discloses the boundary conditions used in the model in which the cooling air and gas are moving along, respectively, in the two layers of chambers in opposite directions. In the cooling chamber, the simulation is performed by using air as the cooling flow, while velocity and temperature are set on the jet holes, with pressure on the exit. In another chamber, it is assumed that the mainstream is a mixture of O2, H2O, CO2, N2, and some rare gases. The model created is considered as boundary condition (Table 1) [4]. Assumption of the solid wall of the quarter torus is formed with a hypothesis of negligible thermal resistance by conduction; the thermal properties of the material were considered by Nimonic 263.Table 1
Boundary conditions.
Component
Boundary conditions
Magnitude
Mainstream inlet
Mass flux rate
31.46 (kg/s)
Gas temperature
1300 (K)
Turbulent intensity
5 (%)
Hydraulic diameter
0.324 (m)
Mainstream outlet
Pressure
1.512 (MPa)
Turbulent intensity
5 (%)
Hydraulic diameter
0.324 (m)
Convection coefficient
10 (W/m2K)
Coolant chamber
Air temperature
300 (K)
Pressure
1.4552 (MPa)
Pressure recovery coefficient
0.95
Turbulent intensity
5 (%)
Hydraulic diameter
0.01026 (m)


### 3.3. Meshing and Simulation Procedures

The computational domain incorporates the model, the HEXA mesh in the software, ICEM/CFD, used to generate the structured multiblock and the body-fitted grid system. In this study, the grid system associated with the parts of the mainstream and the coolant supply plenum is H-type. Figure3 shows the grids of the computational domain, and the total number of the cells for the 3D domain is 776,828. Local grid refinement is used near the hole regions.Figure 3
Meshes.The wallY-plus (7) is a nondimensional number similar to local Reynolds number, determining whether the influences in the wall-adjacent cells are laminar or turbulent, hence indicating the part of the turbulent boundary layer that they resolve:
(7)y+=uτairyvair.The subdivisions of the near-wall region in a turbulent boundary layer can be summarized as follows [20]:(a)
y+<5: in the viscous sublayer region (velocity profiles are assumed to be laminar and viscous stress dominates the wall shear),(b)
5<y+<30: buffer region (both viscous and turbulent shear dominate),(c)
30<y+<300: fully turbulent portion or log-law region (corresponds to the region where turbulent shear predominates).As it can be seen in Figure4, for all cases, all nodes on the inner wall surface have the Y-plus value smaller than 300.Figure 4
Y-plus distribution on the inner wall surface.This study is using a commercial CFD code based on the control-volume method, ANSYS-FLUENT 12.0.16, which in order to predict temperature, impingement-cooling effectiveness, and velocity fields. All runs were made on a PC cluster with sixteen Pentium-4 3.0 GHz personal computers. The convergence criteria of the steady-state solution are judged by the reduction in the mass residual by a factor of 6, typically, in 2000 iterations.


## 3.1. Model Description

Transition piece develops heat transformation on both internal and external walls to eliminate resonant frequency concerns. As well the transition piece conducts gas flow directly from the corresponding combustion liners toward the first stage of the gas turbine (stator). The discrete coolant jets, forming a protective film chamber on the side of transition piece, are drawn from the upstream compressor in an operational gas turbine engine. From the supply plenum, the coolant is ejected through the several rows of discrete holes over the external boundary layer against the local high thermal conduction on the other side of the transition pieces [19]. The model, as a one-fourth cylinder, could simulate the transition piece’s structure and performance, to elaborate the turbulence effect on the impingement-cooling performance over a concave surface (see Figure 1) [4].Figure 1
Impingement-cooling concave model.A schematic diagram of the flow domain along with boundary conditions and dimensions is given in Figure2(a). As shown in the figure, the one-fourth cylinder model has two layers of chambers with a length of 1050 mm and an outer radius and an inner radius of 200 mm and 162 mm, respectively. In the diagram, one side of the outer chamber called the coolant chamber is closed; contrarily, both sides of the mainstream chamber as the inner chamber are unfolding in which gas could flow through from one side to the other. There are 18 holes distributed uniformly in three rows on the surface of the outer wall. The distance between the two rows is 68 mm and the diameter of all the holes is about 10.26 mm. In this scenario, the velocity of the coolant flow is set at 6 m/s; the temperatures of the coolant flow and the mainstream flow are set as 300 K and 1300 K, respectively.Computational domain showing boundary conditions.
(a)
(b)


## 3.2. Boundary Conditions

Boundary conditions are applied to specific faces within the domain to specify the flow and thermal variables that dictate conditions within the model. Figure2(a) discloses the boundary conditions used in the model in which the cooling air and gas are moving along, respectively, in the two layers of chambers in opposite directions. In the cooling chamber, the simulation is performed by using air as the cooling flow, while velocity and temperature are set on the jet holes, with pressure on the exit. In another chamber, it is assumed that the mainstream is a mixture of O2, H2O, CO2, N2, and some rare gases. The model created is considered as boundary condition (Table 1) [4]. Assumption of the solid wall of the quarter torus is formed with a hypothesis of negligible thermal resistance by conduction; the thermal properties of the material were considered by Nimonic 263.Table 1
Boundary conditions.
Component
Boundary conditions
Magnitude
Mainstream inlet
Mass flux rate
31.46 (kg/s)
Gas temperature
1300 (K)
Turbulent intensity
5 (%)
Hydraulic diameter
0.324 (m)
Mainstream outlet
Pressure
1.512 (MPa)
Turbulent intensity
5 (%)
Hydraulic diameter
0.324 (m)
Convection coefficient
10 (W/m2K)
Coolant chamber
Air temperature
300 (K)
Pressure
1.4552 (MPa)
Pressure recovery coefficient
0.95
Turbulent intensity
5 (%)
Hydraulic diameter
0.01026 (m)


## 3.3. Meshing and Simulation Procedures

The computational domain incorporates the model, the HEXA mesh in the software, ICEM/CFD, used to generate the structured multiblock and the body-fitted grid system. In this study, the grid system associated with the parts of the mainstream and the coolant supply plenum is H-type. Figure3 shows the grids of the computational domain, and the total number of the cells for the 3D domain is 776,828. Local grid refinement is used near the hole regions.Figure 3
Meshes.The wallY-plus (7) is a nondimensional number similar to local Reynolds number, determining whether the influences in the wall-adjacent cells are laminar or turbulent, hence indicating the part of the turbulent boundary layer that they resolve:
(7)y+=uτairyvair.The subdivisions of the near-wall region in a turbulent boundary layer can be summarized as follows [20]:(a)
y+<5: in the viscous sublayer region (velocity profiles are assumed to be laminar and viscous stress dominates the wall shear),(b)
5<y+<30: buffer region (both viscous and turbulent shear dominate),(c)
30<y+<300: fully turbulent portion or log-law region (corresponds to the region where turbulent shear predominates).As it can be seen in Figure4, for all cases, all nodes on the inner wall surface have the Y-plus value smaller than 300.Figure 4
Y-plus distribution on the inner wall surface.This study is using a commercial CFD code based on the control-volume method, ANSYS-FLUENT 12.0.16, which in order to predict temperature, impingement-cooling effectiveness, and velocity fields. All runs were made on a PC cluster with sixteen Pentium-4 3.0 GHz personal computers. The convergence criteria of the steady-state solution are judged by the reduction in the mass residual by a factor of 6, typically, in 2000 iterations.


## 4. Results and Discussion

### 4.1. Inner Wall Temperature

Figure5 shows the temperature contours predicted by five turbulence models. The figure illustrates that the temperature at the starting point of the wall is high and then starts to go down. The starting point is cooled by the coolant holes at the curve Z=430 mm on the outer wall while the same temperature is maintained throughout the coolant holes. After the coolant strikes the inner wall, there are vortexes formed. The jet impingement and the vortex formed out of the coolant flow cool the surface of the inner wall. The delicate color region (orange, yellow, and green region) is approximately the region where the coolant strikes the inner wall after being reflected by the coolant holes, in which the inner wall is cooled purely by impingement cooling. These figures confirm that the v2-f model has well simulation of heat transfer in the double chamber model. The calculated temperature at the center line of the inner wall is presented in Figure 5(b); there is a difference among the predictions of SST, LES, and RKE models. Both the temperature contours and the color lines have the same trend in the five turbulence models whereas the calculated temperatures between Z=400 and 600 mm are diverse for all turbulence models. All turbulence models continue to predict similar wall temperatures, while the RNG model underpredicts the temperature by up to 5%–8% in the same location.Comparative analysis of inner wall temperature using different turbulence models: (a) temperature distribution of inner wall; (b) temperature along the center line.
(a)
(b)


### 4.2. Cooling Effectiveness

To define cooling effectiveness, the surface temperature downstream of the cooling hole has to be measured. The adiabatic cooling effectiveness (η) is used to examine the performance of cooling. The definition of η is
(8)η=Tm-TawTm-Tc,
where Tm is the mainstream hot gas inlet temperature, which is a fixed value for calculation of the adiabatic cooling effectiveness of any location, and Tc is the temperature of the coolant, which is assigned as a constant of 300 K in this issue. Taw is the adiabatic wall temperature [21].Figures6(a) and 6(b) exhibit the comparison of cooling effectiveness on distribution and averaged cooling effectiveness along the z-axis, respectively. It could be concluded that the effectiveness is high at the beginning of the film while decreasing gradually in downstream. The distribution of the cooling effectiveness of the v2-f and SST model cases is significantly different. The centerline effectiveness by using the five turbulence model cases is shown in Figure 6(b). Overall, particularly the v2-f model gave better results compared to other models. Values of cooling effectiveness compare with the RNG model case, there is an approximately 30% difference in v2-f model case.Comparative analysis of cooling effectiveness in five turbulence models: (a) cooling effectiveness distribution of inner wall; (b) averaged cooling effectiveness.
(a)
(b)


### 4.3. Characteristics of the Flow Field

Since the thermal field of a jet-in-crossflow interaction is dictated by the hydrodynamics, the flow field results were predicted by five turbulence models. Figure7(a) shows the velocity contours at the section plane of coolant chamber. As it can be seen, all models predicted the low momentum region along the downstream edge and the corresponding high momentum or jetting region along the upstream edge within the cooling holes. The predicted reattachment region by SST and v2-f model cases is approximately at the inlet of the cooling chamber, whereas LES, RKE, and RNG predict a larger separation bubble and the flow separates behind the cooling holes. The computed near inner wall velocity contours (m/s) along the centerline plane are shown in Figure 7(b), where the turbulence closure was simulated using the five different turbulence models. All predictions are extremely close to each other with a skewed upstream velocity profile.Coolant velocity contours predicted by various turbulence models: (a)X-Y cross-section velocity distribution; (b) averaged coolant velocity.
(a)
(b)The actual computational cost will of course vary with model complexity and computing power. With the parallel computing resources of a desktop computer available at the time of writing, six Pentium-4 typically 3 GHz processors, for a high-resolution two-dimensional problem, the steady time-averaged eddy viscosity models (RNG, RKE) will have computation times of a few hours (0.5–1.5). In comparison, the more complex SST andv2-f could take 2–4 hours depending on how smoothly the model converges. Based on recent work, unsteady LES models have computation times at least two orders of magnitude higher; a well-resolved three-dimensional LES impinging jet model could take a day to provide a solution.


## 4.1. Inner Wall Temperature

Figure5 shows the temperature contours predicted by five turbulence models. The figure illustrates that the temperature at the starting point of the wall is high and then starts to go down. The starting point is cooled by the coolant holes at the curve Z=430 mm on the outer wall while the same temperature is maintained throughout the coolant holes. After the coolant strikes the inner wall, there are vortexes formed. The jet impingement and the vortex formed out of the coolant flow cool the surface of the inner wall. The delicate color region (orange, yellow, and green region) is approximately the region where the coolant strikes the inner wall after being reflected by the coolant holes, in which the inner wall is cooled purely by impingement cooling. These figures confirm that the v2-f model has well simulation of heat transfer in the double chamber model. The calculated temperature at the center line of the inner wall is presented in Figure 5(b); there is a difference among the predictions of SST, LES, and RKE models. Both the temperature contours and the color lines have the same trend in the five turbulence models whereas the calculated temperatures between Z=400 and 600 mm are diverse for all turbulence models. All turbulence models continue to predict similar wall temperatures, while the RNG model underpredicts the temperature by up to 5%–8% in the same location.Comparative analysis of inner wall temperature using different turbulence models: (a) temperature distribution of inner wall; (b) temperature along the center line.
(a)
(b)


## 4.2. Cooling Effectiveness

To define cooling effectiveness, the surface temperature downstream of the cooling hole has to be measured. The adiabatic cooling effectiveness (η) is used to examine the performance of cooling. The definition of η is
(8)η=Tm-TawTm-Tc,
where Tm is the mainstream hot gas inlet temperature, which is a fixed value for calculation of the adiabatic cooling effectiveness of any location, and Tc is the temperature of the coolant, which is assigned as a constant of 300 K in this issue. Taw is the adiabatic wall temperature [21].Figures6(a) and 6(b) exhibit the comparison of cooling effectiveness on distribution and averaged cooling effectiveness along the z-axis, respectively. It could be concluded that the effectiveness is high at the beginning of the film while decreasing gradually in downstream. The distribution of the cooling effectiveness of the v2-f and SST model cases is significantly different. The centerline effectiveness by using the five turbulence model cases is shown in Figure 6(b). Overall, particularly the v2-f model gave better results compared to other models. Values of cooling effectiveness compare with the RNG model case, there is an approximately 30% difference in v2-f model case.Comparative analysis of cooling effectiveness in five turbulence models: (a) cooling effectiveness distribution of inner wall; (b) averaged cooling effectiveness.
(a)
(b)


## 4.3. Characteristics of the Flow Field

Since the thermal field of a jet-in-crossflow interaction is dictated by the hydrodynamics, the flow field results were predicted by five turbulence models. Figure7(a) shows the velocity contours at the section plane of coolant chamber. As it can be seen, all models predicted the low momentum region along the downstream edge and the corresponding high momentum or jetting region along the upstream edge within the cooling holes. The predicted reattachment region by SST and v2-f model cases is approximately at the inlet of the cooling chamber, whereas LES, RKE, and RNG predict a larger separation bubble and the flow separates behind the cooling holes. The computed near inner wall velocity contours (m/s) along the centerline plane are shown in Figure 7(b), where the turbulence closure was simulated using the five different turbulence models. All predictions are extremely close to each other with a skewed upstream velocity profile.Coolant velocity contours predicted by various turbulence models: (a)X-Y cross-section velocity distribution; (b) averaged coolant velocity.
(a)
(b)The actual computational cost will of course vary with model complexity and computing power. With the parallel computing resources of a desktop computer available at the time of writing, six Pentium-4 typically 3 GHz processors, for a high-resolution two-dimensional problem, the steady time-averaged eddy viscosity models (RNG, RKE) will have computation times of a few hours (0.5–1.5). In comparison, the more complex SST andv2-f could take 2–4 hours depending on how smoothly the model converges. Based on recent work, unsteady LES models have computation times at least two orders of magnitude higher; a well-resolved three-dimensional LES impinging jet model could take a day to provide a solution.


## 5. Conclusion

A numerical simulation has been performed to study the flow and heat transfer of impinging cooling on the double chamber model, and a comparative study, indicating the ability of five turbulence models, is presented. The research of turbulence model tasks is important to improve the design and resulting performance of impinging jets.During this investigation, numerical simulation is impacted with five turbulence models, which has some practical value for real processing and guiding significance for theory. To date, the SST andv2-f models offer the best results for the least amount of computation time. It is very important to consider the effect of heat conduction within the metal on the predictions of an accurate surface temperature and hence impingement-cooling effectiveness. The validation of the present study has confirmed angle cases and will be employed in future studies of impingement-cooling parameters optimization.



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*Source: 170317-2013-12-08.xml*