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    Flow Turbulence Combust (2008) 80:119132DOI 10.1007/s10494-007-9080-8

    Large-eddy Simulation of Film Cooling Flows

    with Variable Density Jets

    P. Renze W. Schrder M. Meinke

    Received: 28 August 2006 / Accepted: 10 May 2007 /

    Published online: 23 August 2007 Springer Science + Business Media B.V. 2007

    Abstract The present paper investigates the impact of the velocity and densityratio on the turbulent mixing process in gas turbine blade film cooling. A coolingfluid is injected from an inclined pipe at =30 into a turbulent boundary layerprofile at a freestream Reynolds number of Re = 400,000. This jet-in-a-crossflow(JICF) problem is investigated using large-eddy simulations (LES). The governingequations comprise the NavierStokes equations plus additional transport equations

    for several species to simulate a non-reacting gas mixture. A variation of the densityratio is simulated by the heat-mass transfer analogy, i.e., gases of different densityare effused into an air crossflow at a constant temperature. An efficient large-eddy simulation method for low subsonic flows based on an implicit dual time-stepping scheme combined with low Mach number preconditioning is applied. Thenumerical results and experimental velocity data measured using two-componentparticle-image velocimetry (PIV) are in excellent agreement. The results show thedynamics of the flow field in the vicinity of the jet hole, i.e., the recirculation regionand the inclination of the shear layers, to be mainly determined by the velocity ratio.However, evaluating the cooling efficiency downstream of the jet hole the mass flux

    ratio proves to be the dominant similarity parameter, i.e., the density ratio betweenthe fluids and the velocity ratio have to be considered.

    Keywords LES Jet-in-a-crossflow Film cooling Density ratio Velocity ratio Cooling efficiency

    1 Introduction

    In modern gas turbines film cooling mechanisms protect the turbine componentsfrom the thermal stresses resulting from the exposure to the hot gas stream. Since

    P. Renze (B) W. Schrder M. MeinkeAerodynamisches Institut, RWTH-Aachen, 52062 Aachen, Germanye-mail: [email protected]

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    120 Flow Turbulence Combust (2008) 80:119132

    the technical design process of film cooling systems depends on the exact knowledgeof the generated flow field, a detailed understanding of the flow physics is a must toimprove existing cooling techniques.

    In the present case, the cooling film is generated by an injection of a cooling fluid

    through a row of staggered holes. The flow field resulting from the interaction of theinclined cooling jet and the turbulent boundary layer is governed by complex vortexdynamics. The outer field is dominated by a counter-rotating vortex pair (CVP),which is the leading mechanism in the mixing process between the hot gas and thecoolant. Due to the high impact of film cooling on the thermal efficiency of turbinesa wide range of experimental investigations on this matter can be found in the liter-ature. Andreopoulus and Rodi[2] measured the flow field at different velocity ratiosusing hot-wire probes. In a recent study Plesniak and Cusano [24] provided a detailedanalysis of the evolution of the large-scale vortical structures that dominate the jet-crossflow interaction using laser-Doppler velocimetry (LDV). An extensive study ofthe effect of the density ratio has been presented by Goldstein and Eckert [7]. Ina following investigation Pedersen et al. [21] studied the impact of this parameterapplying the heat-mass transfer analogy. They reported a strong influence of thedensity ratio on the local film cooling effectiveness by measuring the concentration ofa high density cooling gas along a plate. Measurements of cryogenically cooled jetswith thermocouple arrangements have been performed by Pietrzyk et al. [23] andSinha et al. [26]. The authors of the former paper measured the turbulent intensitiesat different density ratios and in the latter article the cooling effectiveness was foundto be improved with increasing density ratio.

    Most numerical investigations of the JICF problem have been based on Reynolds-averaged NavierStokes equations, e.g., Hoda and Acharya [13] or the systematicstudy of film cooling physics by Walters and Leylek [29]. However, since the JICFproblem is influenced by effects of wall-bounded and free turbulence, most standardturbulence models like zero-, one- or two-equation models fail to correctly predictthe resulting flow field. For this reason, it is necessary to apply a more generalnumerical ansatz such as large-eddy simulation (LES) to investigate JICF problems.Such an analysis was performed, for instance, by Tyagi and Acharya [28]. In this workrandom perturbations have been introduced at the inlet of the turbulent boundarylayer. An LES study that includes an accurate treatment of the incoming turbulent

    boundary layer and a plenum area was performed by Guo et al. [11], who investigatedamong other issues the effects of inclination angle and blowing ratio on the flowfield. In[14] a similar study has been reported based on likewise ideas as far as thegeometry and the numerical set-up is concerned as in the analysis discussed in theprior publications by Guo et al. [912].

    In the present paper the impact of the density ratio between coolant andcrossflow is analyzed by LES and compared with experimental data. Accordingto Pietrzyk et al. [23] there are three different ways to vary the density ratioparameter: a heated freestream flow, cryogenically cooled injectant flow, and foreign

    gas injection. Since the first two options require very complex and expensive windtunnel measurements and such experiments are performed in [16] for comparisonreasons, the density ratio parameter is studied by the heat-mass transfer analogy, i.e.,a foreign gas (CO2) jet is injected into an air crossflow.

    The paper is organized as follows. After a succinct description of the governingequations and the numerical method the flow configuration and the boundary

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    Flow Turbulence Combust (2008) 80:119132 121

    conditions are presented. In the results section the flow structures of a round jetin a crossflow are analyzed and the impact of velocity ratio and the density ratio willbe studied in detail. The findings of the numerical simulations will be compared withtwo-component particle-image velocimetry (PIV) measurements of Jessen et al. [16].

    Finally, the cooling efficiency will be evaluated.

    2 Governing Equations

    The simulation of a turbulent and non-reacting multicomponent flow is considered.The governing equations are the NavierStokes equations including conservationequations for the partial densitiesn ofN 1 species, where Nis the total numberof different species. In tensor notation and in terms of dimensionless conservativevariables the equations read in a Cartesian coordinate system

    Q

    t +(FC F

    D ), = 0 , Q = [n, , u , E]

    T , (1)

    where Q is the vector of the conservative variables and FC denotes the vector of the

    convective and FD of the diffusive fluxes

    FK FD =

    nuu

    u u + p

    u (E+ p)

    +

    1

    Re

    jn0

    u + q

    . (2)

    The stress tensoris written as a function of the strain rate tensor S

    = 2

    S

    1

    3S

    with S =

    1

    2(u, + u, ) . (3)

    The mass diffusion jn is described by Ficks law

    jn = Dn

    Sc0Yn, , (4)

    where Ynis the mass fraction of the species n,Dnis the diffusion coefficient computedwith mixing rules from the binary diffusion coefficients, Sc0 =0/D0 is the Schmidtnumber, and the subscript 0 indicates the reference state of the mixture. Fourierslaw of heat conduction is used to compute the heat fluxq

    q = k

    Pr0(0 1)T, , (5)

    wherePris the Prandtl number. The system is closed with the equation of state for amixture of ideal gases:

    p=

    n

    pn with pn = T

    0n Rn , (6)

    whereis the ratio of the specific heats, Tthe temperature, pthe pressure, and Rthe gas constant.

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    All transport coefficients are assumed to be a polynomial function of 4th order ofthe temperature, e. g., for the coefficient of heat conductivity k

    ln kn = i

    ain (ln T)i1 . (7)

    The superscript denotes dimensional values. The values of the transport coeffi-cients for the mixture of the species are determined according to the mixing rules ofWilke[30] and Bird[3], for the diffusion coefficient and the viscosity, respectively,and according to Mathur [18] for the heat conductivity. In the mixing rule for thediffusion coefficient Dnthe pressure dependence is taken into account.

    3 Numerical Method

    The discretization of the governing equations is based on a mixed central-upwindAUSM (advective upstream splitting method) scheme using a centered 5-point lowdissipation stencil to compute the pressure derivative in the convective fluxes. Thelarge-eddy simulations are carried out using the MILES technique as reported byFureby and Grinstein [6,8] to represent the effect of the non-resolved subgrid scales.As a consequence, the intrinsic dissipation of the numerical scheme is assumed totransfer energy from the large to the small scales. Thus, it serves as a minimal implicitSGS model. An extensive study of the AUSM algorithm with different SGS models

    and its dependence on the grid solution has been reported by Meinke et al. [19].A more detailed discussion of the application of the MILES technique is given inRtten et al.[25].

    The temporal approximation is based on an implicit dual time-stepping scheme. Aconvergence acceleration of the low Mach number problem is achieved using multi-grid methods and preconditioning. This dual time stepping algorithm is describedin Alkishriwi et al. [1]. Therefore, a derivative with respect to the pseudo-time isintroduced in (1)

    1

    Q

    +

    Q

    t +

    R= 0

    . (8)

    The matrix of the preconditioned scheme has been introduced by Turkel et al.[27]and is modified to account for the additional mass-fraction equations. R representsthe convective and viscous fluxes. A 5-step Runge-Kutta method is applied topropagate the vector of solution Q in(1) from pseudo-time levelnto n +1.

    4 Boundary Conditions

    In large-eddy simulations of spatially developing boundary layers the treatmentof the inflow boundary of the computational domain is one of the most difficultproblems. In general and in particular in the JICF problem, the flow depends highlyon the solution prescribed at the inlet.

    The most physical ansatz to meet this challenge is to start to compute the flow rightat the leading edge where the boundary layer emanates. However, the computational

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    costs would be too extensive for the present problem. Tyagi and Acharya [28]prescribed a turbulent profile and superimposed random fluctuations, which on theone hand, is based on minimum effort, on the other hand, however, generates aslightly discontinuous solution, e.g., of the wall shear stress. The following detailed

    analysis of the vortical structures in the vicinity of the jet hole does suffer from suchunphysical inlet conditions of the boundary layer.

    Therefore, in the present work an independent spatially developing boundarylayer simulation is performed and based on a slicing technique the inflow distributionis prescribed using the velocity profile possessing the boundary layer parametersnecessary at the inflow boundary of the jet-in-a-crossflow problem. This method isindicated in Fig.1.

    The auxiliary flat plate flow simulation generates its own turbulent inflow datausing the compressible rescaling method proposed by El-Askary et al. [4, 5]. Therescaling method is a means of approximating the properties at the inlet via asimilarity approach applied to the downstream solution. A detailed validation ofthis inflow generation method and its application to the JICF problem is given byGuo et al. [11].

    A sketch of the whole computational domain, which consists of the auxiliarydomain, the JICF domain, a plenum, and a pipe, from which the cooling jet is injectedinto the crossflow, is shown in Fig. 1. In the spanwise direction full periodic boundaryconditions are applied. Thus, an infinite row of staggered holes at a distance ofS= 3D between the centerlines is simulated. At the inlet of the plenum area thestagnation pressure is prescribed. The cooling fluid is driven through the pipe by

    the pressure difference between crossflow and plenum. The stagnation pressure iscontrolled by the calculation of the mass flux through the pipe to enforce a correctmass flux ratio. At the outer circumferential surface of the plenum the mass flux isassumed to vanish asymptotically.

    The outflow boundary conditions are based on the conservation equations writtenin characteristic variables. To damp numerical reflections at the outflow boundariessponge zones are introduced into the computational domain, as indicated in Fig. 1. Inthese regions source terms are superposed onto the right-hand side of the governing

    Fig. 1 Schematic of the computational domains and the boundary conditions of the JICF simulation

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    1.5D

    Y

    X

    X12DD

    3D

    7D

    35.6D

    3D

    7.6D

    3D

    plenum

    flat plate

    pipe

    Z

    Fig. 2 Schematic of the flow configuration in thex-y-plane (left) and thex-z-plane (right)

    equations to drive the instantaneous solution of Q to a desired target solution Qt,e.g., the logarithmic boundary layer profile. The source terms are formulated as

    S= (Q(t,x) Qt(x)) , (9)

    where the parameter is a polynomial function of the distance to the outflowboundary and decreases frommaxto 0 within the boundary layer.

    On the wall the no-slip conditions are prescribed, the pressure gradient is assumedto be negligible, and adiabatic conditions are imposed.

    5 Flow Configuration

    The domain of integration of the JICF simulation is shown in Fig. 2. The dashed linesmark the outer boundaries of the computational domain. The cooling fluid is drivenby a pressure gradient from a plenum into the boundary layer flow through a 30o

    streamwise inclined pipe. The origin of the frame of reference is located at the jethole center. The coordinates x,y, zrepresent the streamwise, normal, and spanwise

    direction.To mimic the flow parameters in a gas turbine a cooling fluid is injected from acomplete row of jets into a turbulent flat plate boundary layer at a Mach numberMa=0.2 and a local Reynolds number of Re= 400,000 based on the length fromthe leading edge of the flat plate to the hole. The ratio of the local boundary layerthickness to the hole diameter is 0/D=2. The relevant flow parameters and the

    Table 1 Flow and geometry parameters

    Case Re Ma D[mm] 0/D V R DR MR

    1 400,000 0.2 30 10 2 0.1 1 0.1

    2 400,000 0.2 30 10 2 0.28 1 0.28

    3 400,000 0.2 30 10 2 0.48 1 0.48

    4 400,000 0.2 30 10 2 0.1 1.53 0.153

    5 400,000 0.2 30 10 2 0.28 1.53 0.43

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    Flow Turbulence Combust (2008) 80:119132 125

    geometrical parameters are summarized in Table1.The velocity, density, and massflux ratio are defined as

    V R= uj

    u, DR=

    j

    , and MR=

    juj

    u, (10)

    where the subscripts jand denote the jet and the crossflow fluid. The mass fluxis varied as three different velocity ratios are investigated V R= 0.1, 0.28and 0.48.Two different values of the density ratioDR, an air-to-air injection withDR= 1 anda CO2-to-air injection withD R= 1.53, are considered. All cases are listed in Table 1.

    6 Results and Discussion

    The result section possesses the following structure. First, some computationaldetails are explained. Then, the impact of the velocity and the density ratio on theflow field is discussed. Subsequently, the findings are compared with experimentaldata to show the quality of the computational method. Next, the instantaneousmixing process is analyzed and the characteristic properties of the jet-crossflowinteraction are explained. Finally, the cooling efficiency is studied by means of themixture fraction distribution of the denser gas.

    6.1 Computational details

    All simulations have been performed on a block-structured mesh shown in Fig.3. Itconsists of 5.65 million cells distributed over 24 blocks. The purpose of the blocksupstream of the jet hole is to deliver an independent boundary layer simulation asmentioned above. The grid points are clustered near the solid walls of the flat plateand the pipe. The wall-normal distance of the control volume at the flat plate has adimension ofy= 0.004D, which corresponds to y+ = 1.0.

    Fig. 3 Block-structured mesh used for the JICF simulation; left: 3d view of the pipe-to-plate junction;right: cross section at y/D= 0; every second node shown

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    The physical time step is t= 0.02D/U. To obtain the time-averaged statisticsthe flow field has been sampled over 8 time periods. Here, one period is the time thecrossflow fluid needs to pass over the length of the plate.

    6.2 Time-averaged quantities

    The interaction of the turbulent boundary layer with a high density cooling jet isshown in Fig.4.The velocity ratio is V R= 0.28and the density ratio is DR= 1.53,which resembles the CO2-air mass flux ratio. The upper left view displays the JICFpart of the computational domain. The velocity field is emphasized by streamlinesto show the deflection of the crossflow by the jet and the swirling motion of thejet fluid being entrained by the crossflow. In several cross sections at different x/Dlocations contours of the mean mixture fraction fof the jet fluid are shown. The

    cross sections are enlarged and vectors to evidence the secondary velocity field areadded. Atx/D= 0 the high density fluid starts to penetrate into the crossflow and theshear layers start to roll up at the jet hole edges. At x/D= 1.5the counter-rotatingvortex pair (CVP) resulting from the shear of the crossflow fluid by the jet [22] isalready fully developed. The mixing between both fluids follows the development ofthe vortex pair. The maximum values of the mixture fraction fmark the center ofthe unmixed jet fluid. This is lifted off the wall as low density fluid from the crossflowis entrained between the wall and the jet by the CVP. The cross section at x/D= 3shows the streamwise development of the CVP that continuously grows. The vorticity

    Fig. 4 V R= 0.28 and DR = 1.53, streamlines and contours of the mixture fraction f at differentcross sections (upper left), contours of fand velocity vectors in the cross section at x/D= 0(upperright), cross section atx/D= 1.5(lower left), and cross section at x/D= 3 (lower right)

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    Fig. 5 Mach number contoursin the JICF symmetry planeand streamlines atV R= 0.28and DR = 1(left), atV R= 0.48and DR = 1(center), atV R= 0.28andDR = 1.53(right)

    magnitude is decreased, the centers of the CVP approach each other and drift awayfrom the surface.

    To figure out the impact of the velocity ratio and the density ratio on the coolingefficiency the parameters V R and DR are varied in the large-eddy simulations. InFig.5Mach number contours and streamlines are extracted in the JICF symmetryplane for three different cases. It is obvious from the left and center illustrations that

    a variation of the velocity ratio has a large impact on separation and reattachmentbehavior as well as the strength of the penetration into the crossflow.

    However, a variation of the density ratio at a constant velocity ratio, which is givenin the left and right illustrations, has only a minor effect on the dynamics of theflow field in the vicinity of the jet hole. The size of the recirculation region, the wallnormal velocity gradients, and the penetration depth show only small differences ifthe velocity ratio is kept constant. Just the lateral spreading of the jet fluid is slightlyincreased at a higher jet density. This result agrees with the conclusion reportedin [23].

    The same behavior becomes evident when turbulent quantities are considered. In

    Fig.6the contours of the time-averaged streamwise velocity fluctuation (u2)1/2/U

    Fig. 6 Contours of the streamwise velocity fluctuation (u2)1/2/U in the symmetry plane atDR = 1,V R= 0.28(left) and profiles of the streamwise velocity fluctuation for D R= 1 and D R=1.53at differentx/Dlocations (right)

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    are shown in the symmetry plane at DR= 1and V R= 0.28. The highest turbulencelevels are clearly located at the windward side of the jet exit, i.e., just upstream ofthe jet hole, and in the shear layer between the recirculation region and the jet. Inthe latter zone the major part of the mixing between both fluids takes place. The high

    shear between the jet and the wake region also possesses a high density gradient sincecrossflow fluid is entrained between the wall and the jet.

    Profiles of the streamwise velocity fluctuation at different x/Dlocations also areshown in Fig. 6 at two different density ratios DR= 1 and DR= 1.53. The wallnormal distribution and the peak levels almost match at both density ratios. This isexpected as the velocity gradients in the mean flow field are almost identical.

    6.3 Comparisons with PIV measurements

    The LES technique of the present study is validated by comparing the time-averaged flow field with the particle-image velocimetry (PIV) measurements ofJessen et al. [16]. In Fig.7 profiles of the streamwise velocity are compared for twodifferent density ratios (DR= 1, DR= 1.53) and at two different velocity ratiosV R= 0.1and V R= 0.28. The profiles are located in the spanwise symmetry plane(z/D= 0) at different streamwise locations (x/D= 1, 0, 1, 1.5, and 2). The loca-tionx/D= 1corresponds to the upstream edge of the jet hole. The boundary layerflow is nearly undisturbed at this location and the velocity profile matches the fullydeveloped turbulent profile at the corresponding Reynolds number. Atx/D= 0andx/D= 1 the boundary layer is lifted by the jet. In the case of the higher velocity

    U/Uoo

    y/D

    0

    0.5

    1

    1.5

    2VR=0.1DR=1

    U/Uoo

    y/D

    0

    0.5

    1

    1.5

    2VR=0.1DR=1.53

    U/Uoo

    y/D

    0

    0.5

    1

    1.5

    2VR=0.28DR=1

    U/Uoo

    y/D

    0

    0.5

    1

    1.5

    2VR=0.28DR=1.53

    Fig. 7 Profiles of streamwise velocity in the symmetry plane at different streamwise locations,top left: V R= 0.1, DR = 1, bottom left: V R= 0.28, DR = 1, top right: V R= 0.1, DR = 1.53,bottom right:V R= 0.28, D R= 1.53, experimental dataempty box: x/D= 1,triangle: x/D= 0,inverted triangle: x/D= 1,diamond: x/D= 1.5,circle: x/D= 2,solid lines: LES data

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    Fig. 8 Instantaneous mixture fraction contours and velocity vectors at X/D= 1 (left) and X/D=2.0(right),V R= 0.28, DR = 1.53

    ratio the jet is separated at x/D= 1.5 and reattached at x/D= 2. In all four casesthe predicted flow field is in excellent agreement with the PIV measurements. Minor

    deviations occur atV R= 0.28and DR= 1.53at a streamwise location ofx/D= 1,that coincides with the trailing edge of the jet hole. The deviations are due to laserlight reflections at this sharp edge. As mentioned before, the velocity field in thevicinity of the jet injection is very similar for both density ratios.

    6.4 Characteristics of the jet-crossflow interaction

    The coupling of the flow dynamics to the turbulent mixing process of the differentspecies is closely connected to the formation of the counter-rotating vortex pair(CVP) downstream of the jet hole. There are different explanations for the genera-tion of the CVP, e.g., those from Kelso and Smitts[17] or Morton and Ibbetson [20].The present study agrees with the hypothesis discussed in detail by Peterson andPlesniak[22]. They state the reason for the initial formation of the CVP to be theshear of the boundary layer fluid by the jet.

    Due to the high resolution as well as the time accuracy of the present numericalscheme and the possibility to track the passive mixture fraction scalar a detailedanalysis of the formation of the CVP and the initial mixing process can be performed.In Fig.8 two cross sections at x/D= 1, i.e., directly at the trailing edge of the hole,and further downstream at x/D= 2.0 display contours of the mixture fraction f

    and vectors of the secondary velocity field at the same instantaneous time level. Thevelocity ratio is V R= 0.28and the density ratio is DR= 1.53. The vorticity, which

    Fig. 9 Left: Instantaneous contours of the mixture fraction f in the symmetry plane at a velocityratio ofV R= 0.28, DR = 1.53,right: coherent structures indicated by the2criterion with mappedon mixture fraction f

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    originates from the spanwise edges of the jet hole, causes the initial roll-up in theshear zone. The resulting eddies are already lifted off the plate at x/D= 1. Themixture fraction on the plate wall is reduced as crossflow fluid is entrained underthe jet by the large-scale vortices. Further downstream, in the zone that is governed

    by oscillating separation and reattachment the vortical structures possess a smallerscale, are more intense and intricate, and as such the mixing process is accelerated.

    The separation-reattachment zone can be identified in Fig. 9. The mixture fractionf is shown at an instantaneous time level in the streamwise symmetry plane. Onthe right, coherent structures indicated by the 2 criterion [15] with mapped onmixture fraction distribution fare depicted. The selected views in Fig. 9 visualize theinteraction of the inherent hairpin vortices of the turbulent boundary layer with theeffusing jet fluid. The hairpin-like structures in the upper part of the boundary layerare lifted and entrain jet flow fluid only after they passed the trailing edge. The lowerpart of the boundary layer is deflected by the blockage effect of the jet. The smallscale structures lead to the initial mixing in the shear zones. Further downstream themixing process is significantly accelerated in the separation region.

    6.5 Cooling efficiency

    Following the heat-mass transfer analogy the penetration of the CO2 jet into an aircrossflow mimics the density ratio between the cooling fluid and the hot boundarylayer flow in a gas turbine. Hence, the distribution of the mean mixture fraction falong the flat plate downstream of the jet hole resembles the film-cooling efficiency.

    The data has been averaged over time and in space with respect to the jet symmetryplane. The contours of the mixture fraction falong the plate at two different velocityratios V R= 0.1 and V R= 0.28, respectively, and a density ratio of DR= 1.53areshown in Fig.10.The coverage of the plate is significantly improved at a higher massflux ratio. The lower figure on the left shows a stronger lateral spreading of the densefluid and higher peak values that exist further downstream.

    The graph on the right shows the mean mixture fraction along the plate centerlineas a function of the streamwise coordinate for the higher velocity ratio case V R=0.28that corresponds to a mass flux ratio ofMR= 0.43. The data is compared with

    x/D

    meanmixturefractionf

    0 5 10 150

    0.2

    0.4

    0.6

    0.8

    1

    LES - mixture fraction

    Sinha (1991)

    Fig. 10 Left: contours of the mean mixture fraction falong the flat plate at MR= 0.153(top) andat MR= 0.43(bottom);right: mean mixture fraction along the centerline at MR= 0.43comparedwith the film cooling efficiency measured at M R= 0.5by Sinha et al.[26]

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    the findings of Sinha et al. [26]. The symbols represent the measured film coolingefficiency , which is a temperature based variable. The mass fraction of the dense gasis related to the cooling efficiency for the analogous heat transfer situation. It is = fas stated in [21]. In the experiments the density ratio is DR= 2 and V R= 0.25,

    which leads to a slightly higher mass flux ratio ofMR= 0.5. Nevertheless, it can beconcluded that the good agreement between both curves shows the mixture fractiondistribution along the plate to correctly predict the film cooling efficiency of suchflow configurations.

    7 Conclusion

    Large-eddy simulations of the jet-in-a-crossflow problem have been performed toinvestigate in detail the impact of the density ratio parameter on the physics of filmcooling flows. The high resolution of the computational domain, the time accuracy,and the possibility to track the passive mixture fraction scalar fof the cooling fluidallows a detailed analysis of the mean and the instantaneous flow field. The numericalsimulations are conducted using the same flow parameters as the simultaneouslyperformed PIV measurements. The LES predictions for the velocity distributionsare in excellent agreement with the experimental data.

    Variations of the velocity ratio parameter significantly impacts the flow field withrespect to the dynamic separation and reattachment process, the turbulence statistics,and the cooling efficiency, whereas a variation of the density ratio has only a minor

    influence, if the velocity ratio is kept constant.The flow physics is discussed by identifying the dominant vortical structures. The

    formation of the CVP is generated by the initial shearing of the boundary layer by thejet. Finally, the cooling efficiency along the flat plate is identified by the mean mixturefraction distribution. Comparisons with findings from the literature convincinglyshow the validity of the heat-mass transfer analogy to investigate such flows. Theevaluation of the cooling efficiency is strongly dependent on density effects and thus,the mass flux ratio has to be considered.

    Acknowledgements The support of this research by the Deutsche Forschungsgemeinschaft (DFG)in the frame of SFB 561 is gratefully acknowledged.

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