American Journal of Fluid Dynamics
p-ISSN: 2168-4707 e-ISSN: 2168-4715
2015; 5(A): 1-11
doi:10.5923/s.ajfd.201501.01
Mrinal Kaushik 1, Rakesh Kumar 2, Humrutha G. 1
1Department of Aerospace Engineering, Indian Institute of Technology, Kharagpur, India
2Department of Aerospace Engineering, Indian Institute of Technology, Kanpur, India
Correspondence to: Mrinal Kaushik , Department of Aerospace Engineering, Indian Institute of Technology, Kharagpur, India.
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The present work reviews the CFD studies carried out in the last more than fifty years to understand the uncontrolled and controlled jet characteristics. The chronological evolution of investigations on jets are reviewed, however they are presented according to their relevance in the discussion. The study also highlights the complexities involved in adaptive turbulence models in a realistic simulation of free jets. These complexities are largely due to entrainment of jets, large perturbations present at low Reynolds numbers in subsonic jets and strong wave interactions in jets exiting at supersonic Mach numbers from convergent-divergent nozzles. The accurate capturing of these perturbations, shock-cell structures in jets poses a real challenge in the CFD analysis. The complexities of capturing shock and expansion waves accurately in supersonic jets, is the critical step in the simulation.
Keywords: Free jets, Numerical simulation, Turbulence models, Shock-Cell structure, Entrainment, Jet centerline velocity
Cite this paper: Mrinal Kaushik , Rakesh Kumar , Humrutha G. , Review of Computational Fluid Dynamics Studies on Jets, American Journal of Fluid Dynamics, Vol. 5 No. A, 2015, pp. 1-11. doi: 10.5923/s.ajfd.201501.01.
![]() | Figure 1. Schematic diagram of different zones in the development of a subsonic jet |
![]() | Figure 2. Schematic diagrams of (a) overexpanded jet, (b) under expanded jet |
Furthermore, they also observed that the rate at which streamwise vorticity develops is strongly affected by the ratio of the streamwise and azimuthal perturbation amplitudes. However, the assumption of inviscid flow in the vortex filament technique is obviously unable to capture the viscous effects in the actual flow field. Miller et al (1995) [7] studied the entrainment of the subsonic jet flows originating from elliptic, rectangular and triangular nozzles with aspect ratios of 1:1 and 2:1 using the compressible Navier-Stokes equations, and a passive scalar conservation equation with the Fourier heat conduction and the Fickian diffusion assumptions. These equations were solved numerically without resorting to any turbulence or imposed subgrid models. The results were compared with those of a circular jet of the same equivalent diameter to determine the relative efficiency of non-circular nozzles in mixing enhancement. Though the flow structure was predicted, but the effectiveness of the compressible or the time-independent Navier-Stokes equation in the simulation of subsonic jet or in predicting the three-dimensional vortical structures, remained unexplained. There remains a necessity to obtain the accurate aerodynamic and aeroacoustic prediction tools for analyzing exhaust nozzle systems and the turbulent jet flowfields. To this end, initial successful attempts were made using the Reynolds-Averaged Navier-Stokes (RANS) method. A brief summary of some of the remarkable attempts in this direction is given below.
and u' i.e., intoits time-averaged and fluctuating quantities respectively. The RANS equations are primarily used in analyzing turbulent flows, with approximations based on knowledge of the flow properties to give approximate time-averaged solutions to the Navier–Stokes equations. This method attempts to model all turbulent fluid dynamic effects with a turbulence model. Currently, RANS methods are used for a vast majority of calculations. Two-equation models, such as k-ϵ, Menter’s SST formulations and k-ω modelare widely used to solve for the turbulent kinetic energy in the jet environment.Thies and Tam (1996) [9] used the k-ϵmodel with a correction factor as developed by Pope (1978) [10], and Sarkarand Lakshmanan (1991) [11]. They attempted to predict the flow characteristics of the jets having high convective Mach number. The axisymmetric and non-axisymmetric jet mean flow results over the Mach number range of 0.4-2.0 were compared with the available experimental data. Interestingly, although this model was observed to reproduce the core length and shock-cell length to some extent, the quantitative data such as turbulent intensities were found to be in error. It has now been known that the standard k-ϵ model always over predicts the turbulent kinetic energy growth rate in compressible mixing layer types of flows such as a free high-speed jet. Although, the characteristics and dynamics of fine-scale turbulence may be the same for all turbulent flows, the large turbulence structures, having dimensions comparable to the local length scale of the flow, are significantly influenced by local boundary conditions and geometry. Thus, Thiesand Tam (1996) [9] proposed that there is no universally applicable turbulence model and model has to be chosen depending upon the flow configuration. This creates the necessity to introduce limiting and correction terms. Durbin (1996) [12] proposed to limit the eigenvalues of the Reynolds stress. He mentioned that the limits of the Reynolds stress eigen values must be between zero and twice of the turbulent kinetic energy. The ‘Durbin realizable model’ is proposed to be effective up to Mach 3. Further examination of the effect of compressibility on turbulent flows led to the conclusion that the compressibility effects can be categorized into two basic groups namely, the dilatational and structural compressibility effects. The dilatational compressibility effects are related to variations of the mean mass desnity or variations in the instantaneous mass density whereas, the structural compressibility has significant influence on the structure of turbulent flows. Zeman (1990) [13] and Sarkaret al (1991) [14] modeled the dilatation dissipation based on the results of direct numerical simulation of isotropic compressible turbulence subjected to strong compression. Heinz (2003) [15] proposed a model to account for the structural compressibility effects by re-modeling the turbulence production term. These compressibility corrections terms are employed in the standard k-ϵ turbulencemodel. Several modified linear two-equation turbulence models developed specifically to improve jet flow predictions were compared to the standard RANS turbulence models. Tandraet. al (2006) [16] developed a modified model of k-epsilon with three additional terms to predict the flow properties of high subsonic and supersonic jets up to Mach 2.8. Combining the correction terms proposed by Durbin (1996) [12], Sarkar et al (1991) [14], and Heinz (2003) [15], the modified k-ϵ model was formulated. The performance of the developed numerical model in predicting the free jet flows, a jet propagating between smooth flat plates and a jet impact on an object was tested. The jet centerline velocity, centerline pressure, radial velocity and pressure profiles of the free jet of Mach 0.67, 2.22, 2.3 and 2.8 were compared with the available experimental data. A good agreement with the data was obtained, demonstrating the efficacy of the modeified k-ϵ model. Berget al (2006) [17] compared the two equation turbulence models of k-ω and standard k-ϵ incalculating the properties of a turbulent flow from a aspect ratio 2.0 rectangular Mach 0.17 free jet. Two types of inlet velocity profile boundary conditions such as uniform profile and profile from experimental results were analyzed by two turbulence models of k–ε and k–ω. The results concluded that, the simulation by k–ε model with parameters adapted from experimental results best predicted the centerline velocity decay of the jet. It was found that the conventional density based algorithms become inefficient and often unstable at low Mach numbers. Birky and Page (2001) [18] suggested the adaption of modified pressure based methodology with compressibility correction in simulating the sonic jet in under expanded condition. They proposed that the pressure-based approach with a correctly formulated compressible treatment can accurately compute flows containing both high and low Mach number zones. This numerical scheme uses a basic first-order upwind scheme discretized in an implicit manner. They adapted a higher-order discretization scheme using a total variation diminishing (TVD) method as an explicit correction to the basic upwind scheme. The flow of interest contains a high-speed jet core exhausting into ambient where the flow is at rest. For nozzle pressure ratio (NPR) 3.5, the results from the standard k-ϵ with and without compressibility correction are compared with their experimental counterpart. By varying the NPR from 3.5 to 30, the location of the Mach disk was found to be in agreement with the experimental data. It was observed that the k-ϵ model with compressibility correction produces a faster decay as compared to the experimental results even though the shock cell lengths were in good agreement. The compressibility correction to the turbulence model was found to have almost no effect on the shock cell structure. Chauvetet al, (2007) [19] used the Spalart-Allmaras turbulence model in predicting the jet flow characteristics. From the series of RANS computation and experiments conducted, they showed that the under expanded sonic jets experienced higher mixing enhancement under the influence of radially injected secondary jets. The Spalart-Allmaras model was used to correlate the strong distortion of the jet interface under the action of the longitudinal vortices. Various nozzle configuations having 2, 4 and 8 numbers of radial injections and various secondary orifice jet aspect ratios of 0.5, 1.0, 2.5 and 10 were studied and numerical results were compared with the obtained experimental data. They proposed that, the ideal configuration for an efficient mixing should have four or less number of injectors with a low aspect ratio orifice to prevent premature vortex interaction and excessive diffusion. They stated that the modification of the inside supersonic waves do not contribute to the mixing enhancement. The comparison of plots depicting the numerical and experimental results exibited some discrepencies, which neccesitated the adoption of improved numerical schemes, as discussed in the following sections.
(2001) [34] with the Smagorinsky (1963) [35], and Yoshizawa (1993) [36], linear SGS models. The effectiveness of all these five numerical methods, in predicting the jet flow characteristics were also compared with the Direct Numerical Simulation (DNS) and experimentaldata. They observed that except for
model, where the small scale vortex stretching is supressed, the difference in results obtained with the other models were insignificant. Therefore, the researchers established that corrections in the basic LES models do not show a clear improvement.
They also studied the influence of the inflow boundary conditions on the jet characteristics and found that the effect on the flow is very strong and long living throughout the computational domain of the jet. From the above studies, it is seen that the turbulent jets of various configurations were tested using DNS approach in recent past. Balaracet al (2005) [47], performed DNS and LES studies of the coaxial jets and studied the influence of Reynolds number on coherent vortices and jet mixing. Reynolds number was varied; for lower Reynolds number ( ≈ 3000), DNS approach was adopted, whereas large eddy simulation was carried at higher Reynolds number (6000, 10000 and 30000) for annular to core flow velocity ratios of 5 and 17. At lower Reynolds numbers, the vortical structures appear downstream, whereas an increase in Reynolds number leads to appearance of these structures right in front of the nozzle lip. At annular to core flow velocity ratio of 17, they observed the formation of recirculation bubble, which at higher Reynolds numbers, was recorded to exhibit decreased size and non-stationary characteristics. The researchers from the results of DNS concluded that the recirculation bubble ensures early turbulent activity and also enhances mixing characteristics even at the beginning of the jet itself. Muppidi and Mahesh (2008) [48] used DNS to study passive scalar transport and mixing in a low Reynolds number rounded turbulent jet placed in a laminar cross-flow. The ratio of jet centerline velocity to cross-flow velocity of 5.7 with a Schmidt number of 1.49 in the scalar field was used to compute entrainment of the cross flow fluid by the jet. Also, interestingly, the transverse jet was found to entrain more fluid than a regular jet even when the jet was not yet bent into the cross flow. Here, the transverse jet’s enhanced entrainment was explained in terms of the pressure field around the jet. The acceleration imposed by the cross-flow deformed the jet cross-section on the downstream side, inducing a pressure gradient that drives downstream cross-flow fluid toward the jet. The simulation results were used to comment on the applicability of the gradient diffusion hypothesis to compute passive scalar mixing in this flow field. Computed values of the instantaneous contours of passive scalar, scalar flux, entrainment plot and eddy diffusivity showed significant scatter and pronounced anisotropy. The near field also exhibited counter gradient diffusion.The passive control of jets using DNS approach was found to give results with exceptional accuracy for various control devices. Caiet al (2010) [49] performed numerical simulation using DNS method and conducted experiments to compare the mixing characteristics of circular nozzle, V-shaped notched nozzle and an A-shaped notched nozzle of same circular cross-sectional area. The dye visualization technique revealed that in addition to azimuthal vortex rings created because of the shear-layer, the stream-wise vortex pairs (both inside and outside the vortex rings that spread outward as the vortex rings move downstream) greatly enhanced the entrainment and mixing of the ambient fluid with the jet core. It was seen that the production of stream-wise vortex pairs for the notched circular nozzles owned peak and trough locations unlike their circular counterpart. They concluded from the results of instantaneous vorticity visualisations that the mixing characteristics of the three types of nozzles is such that the jet spreads faster in the peak-to-peak and trough-to-trough cross-planes than in other directions. Thus, the notches in the nozzle exit significantly enhanced jet mixing as shown by the centerline velocity decay plot. In contrast to the RANS and LES approaches, direct numerical simulation (DNS) methods successfully provided the entire turbulent energy spectrum by resolving all turbulent scales ranging from integral length scale down to the Kolmogorov scale. Although this avoids the limitations associated with turbulence modeling, DNS methods may remain computationally impractical in the foreseeable future for all but the simplest configurations.Rembold et al (2002) [50] performed the DNS simulation of a Mach 0.5 jet exiting from an aspect ratio 5 rectangular nozzle at Re = 2000. For spatial discretization, they used the 5th order compact upwind biased scheme for the convective terms and a 6th order compact central scheme for the diffusive terms. They triggered the transition process by the most unstable symmetric linear Eigen mode of a parallel laminar jet profile at the nozzle exit. They observed the transition process, in which the initial 2-dimensional disturbances in the inflow region of the laminar jet rapidly resulted in 3-dimensional turbulence. The shear layer roll-up for the laminar jet and a subsequent rapid transition to small-scale turbulence was observed from the instantaneous and statistically averaged results. Because of vortex shedding from the jet periphery, the symmetrical rectangular jet cross-section got distorted to an elliptic cross-section. Furthermore, it is understood from the vortex theory that size of a vortex is propotional to the radius of curvature of the surface from which it is shed. Since the relatively larger eddies are shed along the major axis and smaller ones along the minor axis, the jet spread rate was found to be rapid along the major axis direction due to higher mass engulfment. This diffrenetial rate in spreading leads to rotation of axes known as ‘axis-switch’ as shown in Figure 3.![]() | Figure 3. A typical schematic diagram of ‘axis-switch’ phenomena |
![]() | Figure 4. Schematic diagram of a jet impinging on a flat plate |