49th AIAA Aerospace Sciences Meeting including the New Horizons Forum and Aerospace Exposition 4 - 7 January 2011, Orlando, Florida AIAA 2011-597 Dependence of the Bluff Body Wake Structure on Flame Temperature Ratio Benjamin Emerson1, Julia Lundrigan2, Jacqueline O’Connor1, David Noble3, Tim Lieuwen4 Georgia Institute of Technology, Atlanta, GA, 30318 This paper describes an experimental investigation of the wake and flame characteristics of a bluff body stabilized flame. Prior investigations have clearly shown that the wake structure is markedly different at “high” and “low” flame density ratios. This paper describes a systematic analysis of the dependence of the flow field characteristics and flame sheet dynamics upon flame density ratio, ρu/ρb, over the range 1.7< ρu/ρb <3.4. This paper shows that two fundamentally different flame/flow behaviors are observed – characterized here as Kelvin-Helmholtz and Von-Karman vortex street dominated - at high and low ρu/ρb values, respectively. These are interpreted here as a transition from a convectively to absolutely unstable flow. This transition manifests itself in several ways with decreasing ρu/ρb values, including (1) the spectrum of the flame motion and flow field transitions from a distributed to a narrowband peak at St~0.24, and (2) the correlation between the two flame front branches monotonically increases. Finally, the intermittent nature of the flow field is emphasized, with the relative fraction of the two different flow/flame behaviors monotonically varying with ρu/ρb. Nomenclature A D ṁ Re StD T U c f k t v = = = = = = = = = = = = flow cross-sectional area bluff body diameter mass flowrate Reynold’s number, UlipD/ν Strouhal number, fD/Ulip temperature time-averaged axial velocity modal wave propagation speed frequency, Hz wavenumber time instantaneous transverse velocity Greek Characters β ζL ζU ν ρ ρf ρU,L ρt τ = = = = = = = = = backflow ratio, -U(y=0)/U(y=∞) lower flame edge position upper flame edge position kinematic viscosity gas density correlation coefficient between sine fit and original time signal correlation coefficient between upper and lower flame edge positions correlation coefficient threshold temporal duration of a sinusoidal chunk of signal 1 Graduate Research Assistant, School of Aerospace Engineering, 270 Ferst Dr, AIAA Student Member. Undergraduate Research Assistant, School of Aerospace Engineering, 270 Ferst Dr, AIAA Student Member. 3 Research Engineer, School of Aerospace Engineering, 270 Ferst Dr, AIAA Member. 4 Professor, School of Aerospace Engineering, 270 Ferst Dr, AIAA Associate Fellow. 1 American Institute of Aeronautics and Astronautics 2 Copyright © 2011 by Benjamin Emerson, Julia Lundrigan, Jacqueline O'Connor, David Noble, and Tim Lieuwen. Published by the American Institute of Aeronautics and Astronautics, Inc., with φ ω = equivalence ratio = frequency, rad/s 0 b i lip max ref u = = = = = = = ’ = unsteady component Subscripts zero group velocity burned imaginary component bluff body trailing edge lip maximum reference velocity unburned Superscripts I. Background Bluff bodies are a common mode of flame stabilization in a variety of practical combustion devices 1. The unsteady flow fields in bluff body flows, both with and without the presence of combustion, are often dominated by large scale coherent structures, embedded upon a background of acoustic waves and broadband fine scale turbulence. These large scale structures play important roles in such processes as combustion instabilities, mixing and entrainment, flashback, and blowoff. The objective of this study is to experimentally characterize the role of flame density ratio upon the appearance and characteristics of these structures in a reacting bluff body wake. These large scale structures arise because of underlying hydrodynamic instabilities of the flow field 2. The concepts of convective and absolute stability of the base flow3-5 upon which these flow disturbances are initiated, and subsequently amplified or damped, will play an important role in the subsequent discussions, so it is helpful to review a few key concepts. In an unstable flow, disturbances are amplified. These amplified disturbances in a convectively unstable flow are swept downstream so that the response at any fixed spatial point eventually tends toward zero. In contrast, perturbations in absolutely unstable flows increase in amplitude at a fixed spatial location, even as the actual flow particles are convected downstream6. The implications of this absolute/convective instability distinction are important. A “convectively unstable” flow acts an amplifier, in that a disturbance created at some point grows in amplitude as it is convected out of the system. However, the oscillations are not self-excited but require a constant disturbance source to persist. In any real situation, there are a variety of background disturbances, such as broadband turbulence and harmonic acoustic disturbances, that provide this consistent source of excitation. The flow then selectively filters these background disturbances. For example, in convectively unstable shear flows, the spectrum shows a distributed peak around a frequency associated with the most rapidly amplified mode7. When such systems are forced by external disturbances, such as acoustic waves, these disturbances are easily discerned in the system response. An absolutely unstable system is an oscillator – it exhibits intrinsic, self-excited oscillations and does not require external disturbances to persist. In such a self-excited system, the amplitude grows before saturating into a limit cycle oscillation. Moreover, the spectrum of oscillations shows a narrowband peak associated with this natural frequency. When externally forced, the limit cycle behavior remains essentially independent of the external forcing, unless the amplitude is high enough that the phenomenon of “lock-in” occurs8-9. In other words, in a convectively unstable flow, there is a monotonic relationship between forcing amplitude and system response, while in an absolutely unstable system, the limit cycle oscillations persist despite this forcing, except at high forcing levels. These distinctions are important in combustion instability problems, where vortical structures excited by acoustic waves play important roles in the feedback mechanism. In one case, low amplitude acoustic excitation will induce a proportional response while in the other it may not. In turn, this has important implications on which type of flow instabilities can be involved in linear combustion instability mechanisms. As shown in Figure 1, there are two key flow features downstream of the bluff body, the separating free shear layer10 and the wake, both of which strongly influence the flame. These two flow features are discussed further next. 2 American Institute of Aeronautics and Astronautics Figure 1. Schematic of non-reacting flow past a bluff body at Re = 10,000. Reproduced from Prasad and Williamson11 The separated shear layer evolves in a similar manner to a mixing layer given a sufficiently long recirculation zone length. It is convectively unstable due to the Kelvin-Helmholtz mechanism for ReD> ~1200, leading to shear layer rollup into tightly concentrated vorticity. In most practical configurations, the flame lies nearly parallel to the flow and, thus, almost directly in the bluff body shear layer for practical high velocity flows. The separating vorticity sheet on both sides of the bluff body rolls up, which induces a flow field that wraps the flame around these regions of intense vorticity. In non-reacting flows, the bluff body wake is absolutely unstable, and characterized by large scale, asymmetric vortex shedding12 known as the Von Karman vortex street. This instability has a characteristic frequency of11 f BVK StD U D (1) where StD is the Strouhal number. For circular cylinders, StD is independent of Reynolds number (StD = 0.21) in the turbulent shear layer, laminar boundary layer regime, ~1000<ReD<~200,00013. Above ReD = ~200,000, the boundary layer starts to transition to turbulence and there are some indications that this Strouhal number value changes14-15. This Strouhal number value is a function of bluff body shape9. In particular, StD is lower for “bluffer” bodies, i.e., those with higher drag and wider wakes16. For example, StD ~ 0.18 for a 90 degree “v-gutter” and drops to 0.13 for a sharp edge, vertical flat plate17. Roshko suggests that StD fundamentally scales with the wake width16, 18 and, therefore, care must be applied in inferring Strouhal numbers from one bluff body shape to another. For example, flow separation is retarded for circular bluff bodies when the boundary layer transitions to turbulence, implying a reduction in wake width and turbulent vortex roll-up19. In contrast, the flow separation point would not move in bluff bodies with sharp separation points. There is a large literature on the effects of wake heating18-21, splitter plates10, and wake bleeding on the absolute stability characteristics of the wake. Of most interest to this study are analyses showing that a sufficiently hot wake relative to the free stream eliminates the absolute instability of the wake, so that its dynamics are then controlled by the convectively unstable shear layers. For example, Yu20 and Monkewitz6, 20 reported the results of a parallel stability analysis in an unconfined domain. They show that the absolute stability boundary depends upon density ratio between the outer flow and wake, and the ratio of reverse flow velocity in the wake to outer flow velocity, β, defined below: u( y u( y 0) ) (2) The resulting convective/absolute stability boundary is plotted in Figure 2. For the purpose of this study, only the sinuous (asymmetric) mode stability boundary is plotted, as it is more easily destabilized in wakes than the varicose (symmetric) mode. This plot shows that absolute instability is promoted with lower density ratios, ρu/ρb, and higher wake reverse flow velocities. In other words, as the reverse flow velocity in the wake increases, the flow becomes more absolutely unstable. For this study, the density ratios plotted in the figure equal the temperature ratio, Tb/Tu , to within a fraction of a percent. 3 American Institute of Aeronautics and Astronautics Figure 2. Dependence of convective/absolute stability limit upon backflow and density ratio, as predicted by 2D parallel flow stability analysis Figure 3. Illustration of the bluff body flowfield, showing region of reverse flow in the wake centerline (ballistic bluff body at 50 m/s, ρu/ρb = 1.7) Computations demonstrating this same effect in combusting flows have also been presented by Erickson et al.21. Their results show that the BVK instability magnitude gradually grows in prominence as density ratio across the flame is decreased below values of approximately 2-3. This observation is quite significant as it shows that the dominant fluid mechanics in a lab scale burner with non preheated reactants, which have a “high” density ratio, can be very different from that of a facility with highly preheated reactants. Similarly, other experiments have clearly shown that the BVK instability becomes prominent either at low flame density ratios 22-23 or for flames close to blowoff22, 24. The objective of this study is to characterize the unsteady flow evolution as the flame density ratio is monotonically varied across this bifurcation in flow structure. While other experimental studies have clearly demonstrated the structural flow change at high and low density ratios, there does not yet appear to be a study where density ratio is systematically varied, particularly while keeping other key flow parameters, such as flow velocity, constant. Additionally, the experiments performed in this study have been designed in order to facilitate a comparison to parallel stability theory. That comparison is presented in a companion work25. 4 American Institute of Aeronautics and Astronautics Figure 4. Computationally predicted vorticity field and instantaneous flame edge for various flame temperature ratios, produced by Erickson21 II. Experimental Facility, Diagnostics, and Testing Procedures The experimental rig, shown in Figure 5 and Figure 6, consists of two premixed, methane-air combustors in series. The first combustor is swirl stabilized and used to vitiate the flow. The bluff body stabilized combustor section consists of a rectangular section with a bluff body spanning the width of the combustor, creating a nominally 2D flow. The aspect ratio of bluff body height to chamber width is 0.15. This combustor has quartz windows for optical access from all four sides. Two different bluff bodies were used in the test section: a 2D ballistic shape (shown in Figure 7a), and a V-gutter (shown in Figure 7b). From here on, the 2D ballistic shape will be referred to as the ballistic bluff body. Vitiator Test Section Secondary Air Inlet Secondary Fuel Inlet Flow Direction Figure 5. Schematic and photograph of the atmospheric pressure, vitiated, bluff body rig Figure 6. Schematic of test section with ballistic bluff body installed 5 American Institute of Aeronautics and Astronautics a) b) Figure 7. Schematics of bluff bodies, a) ballistic, b) V gutter Primary air and fuel were premixed upstream of the vitiator. Secondary air and fuel were plumbed into the rig and premixed in a 1.4 m long settling section aft of the vitiator, and upstream of the test section. The primary and secondary air and fuel each have their flowrates adjusted individually. This design allows the flame density ratio and bluff body lip velocity to be varied independently in the test section, by adjusting the air flowrate and stoichiometry in the vitiator and test section separately. The test matrix was developed such that primary and secondary air flowrates and primary and secondary equivalence ratio could be adjusted to achieve a variety of density ratios at a fixed velocity. Mass flowrates for the primary and secondary air and fuel were measured across calibrated knife-edge orifice plates using the static upstream pressure and the differential pressure across the plate, measured with Omega PX209 solid state pressure transducers and Omega PX771A differential pressure transmitters, respectively. The temperature just upstream of the vitiator (after addition of secondary air and fuel) was measured by a type K thermocouple and an Omega TX13 Smart Temperature Transmitter. Values were recorded once every second for ten seconds, and then averaged. During all tests, the measured primary air and fuel flowrates as well as the measured temperature just before the test section were recorded. On average, the measured absolute temperature entering the test section was 26% and 31% lower than the calculated adiabatic temperature for 50 m/s tests and 20 m/s tests, respectively. Bluff body lip velocity was calculated as Ulip=ṁlip/(ρlipAlip). For this lip velocity calculation, the total measured mass flowrate and the flow cross sectional area at the bluff body trailing edge were used. The density for the lip velocity calculation was determined from the temperature measured just before the test section and the gas composition of the secondary air and fuel adiabatically mixed with the equilibrium vitiated gas. An equilibrium gas solver was then used to calculate the adiabatic density ratio across the test section flame. For PIV tests a reference velocity (Uref) was determined directly from the PIV velocity field as the time-averaged axial velocity just aft of the bluff body, located transversely in the center of the bulk flow. Samples of the design parameters used and the density ratios and lip velocities obtained are presented below. For the 50 m/s cases, uncertainty was about 2% for the measured gas flowrates and the resulting temperature and density ratios. For the 20 m/s cases, uncertainty was about 4% for the measured gas flowrates, about 9% for the resulting density ratios, and about 10% for the density ratios. Uncertainties are bounded by worst case combinations of maximum and minimum flowrates and thermocouple readings for a given test. Differences between Ulip (based on flowrate measurements) and Uref (based on PIV measurements) are 0.6 m/s and 6 m/s for the 20 and 50 m/s cases, respectively. Figure 8 shows the experimental air flowrates and equivalence ratios from the ballistic bluff body at 50 m/s. Uncertainty in thermocouple reading was less than 1%. The charts in Figure 8, shown for the ballistic 50 m/s cases, demonstrate how air flowrates and equivalence ratios in the two burners may be adjusted so that the density ratio can be swept while lip velocity is held nearly constant. 6 American Institute of Aeronautics and Astronautics a) b) Figure 8. Experimental design parameters for ballistic bluff body at 50 m/s, showing a) primary and secondary air flowrates and b) equivalence ratios in both combustors Test matrix design was motivated by Figure 2. Actual conditions tested are provided in Figure 9, where the maximum backflow ratio max was determined from the maximum reverse flow velocity, and overlaid on the absolute stability map from Figure 2. Note that the ballistic bluff body provides a lower maximum backflow ratio than the V-gutter. Contours of constant ω0,iD/Ulip (corresponding to the temporal growth rate of the absolute instability) are provided as well. Note that these are theoretical values that are deduced from assumptions of tophat density and velocity profiles and inviscid flow; more complex hyperbolic tangent profiles have been investigated by Monkewitz26. Figure 9. Tested conditions overlaid onto map obtained from 2D parallel flow stability analysis Experimental diagnostics consisted of high speed, line of sight imaging of flame chemiluminescence and particle image velocimetry (PIV). High speed video was captured for the ballistic bluff body only. High speed imaging was performed with a Photron Fastcam SA3 camera to capture chemiluminescence at a 3000 Hz frame rate at a resolution of 512 x 256 pixels. This CMOS camera operates nearly continuously at 3000 Hz. The flame was imaged through a BG-28 filter for CH* chemiluminescence imaging. This filter transmission exceeds 10% for wavelengths between 340 and 630 nm, and peaks at 82% transmission at 450 nm. The flame was imaged from the bluff body trailing edge to approximately nine bluff body diameters downstream. A total of 8029 images were stored in each run. PIV was conducted for both the ballistic bluff body and the V-gutter at conditions identical to those for high speed video. The PIV system is a LaVision Flowmaster Planar Time Resolved system that allows for twodimensional, high-speed velocity measurements. The laser is a Litron Lasers Ltd. LDY303He Nd:YLF laser with a wavelength of 527 nm and a 5 mJ/pulse pulse energy at a 10 kHz repetition rate. The laser is capable of repetition 7 American Institute of Aeronautics and Astronautics rates up to 10 kHz in each of the two laser heads. The Photron HighSpeed Star 6 camera has a 640x448 pixel resolution with 20x20 micron pixels on the sensor at a frame rate of 10 kHz. In the current study, 2000 PIV image pairs were taken at a frame rate of 10 kHz with 12 s between image pairs. The DaVis 7.2 software from LaVision was used to process the PIV data, performing background subtraction and then calculating the velocity fields. A sample time-averaged velocity field from PIV is provided above in Figure 3. III. Results - Flame and Flow Dynamics A. Spectral and Correlation Analysis This section will discuss several characteristics of the flame and flow dynamics for the ballistic bluff body at a lip velocity of 50 m/s, which will be used as a representative case; data taken at other conditions show similar trends. Flame dynamics, measured by high speed video, were quantified via the transverse position of the top and bottom flame branch edges, ζU(x,t) and ζL(x,t), as a function of axial position and time (see Figure 10). This resulted in time series for edge positions along both flame branches, at each axial position. These time series are Fourier transformed to determine their temporal spectra, given by ζU(x,f) and ζL(x,f). Figure 10. Coordinate system and instantaneous flame edge position definition from edge tracking, 50 m/s, ρu/ρb = 1.7. PIV data were used for corresponding analysis of flowfield dynamics. PIV data shown in this section were taken from the transverse centerline velocity v’(x,y=0,t), whose Fourier transform is given by v’(x,y=0,f). The rest of this section summarizes the key results obtained from analysis of the time series and spectra of both flame and flow dynamics as a function of flame density ratio. Figure 11a shows spectra from the upper flame branch at x/D=3.5 at three different density ratios as a function of Strouhal number, St=fD/Ulip. At the highest density ratio shown, ρu/ρb=2.4, the spectrum is fairly evenly distributed across all frequencies, with a small bump at St ~0.24. As the density ratio is decreased to 2.0, a clear feature appears centered near St = 0.24. As the density ratio is further decreased to 1.7, the response at St = 0.24 becomes narrowband and quite prominent. Figure 11b shows spectra of the unsteady transverse velocity for the same flow conditions, and demonstrates that the flow similarly exhibits a growing narrowband spectral feature at St=0.24. 8 American Institute of Aeronautics and Astronautics a) b) Figure 11. Spectra for ballistic bluff body at 50 m/s and x/D = 3.5 for a) upper flame edge and b) centerline transverse unsteady velocity magnitude In order to focus on the characteristics near the frequency of peak response, the integrated power under the spectral peak between Strouhal numbers of 0.20 and 0.28 as a function of density ratio is computed for the flame response spectra in Figure 11a, and for the unsteady transverse velocity spectra in Figure 11b. This power is converted to a root mean square (RMS) of the signal at the response frequency by use of Parseval’s theorem, using the relation below that relates RMS of the time series s(t) of duration T and spectrum φ(f), srms 1 f 2 ( f ) df (3) f These RMS values are presented in Figure 12 for both the flame and the flow. The flame data in Figure 12 show that the normalized fluctuation in flame position has a value of roughly 4% over the 2.4<ρu/ρb<3.4 range. Below a value of ρu/ρb=2.4, the response gradually increases to 18% at ρu/ρb=1.7. Comparing the flame to the flow data again demonstrates similarities. This plot also indicates that the transition in flow and flame characteristics is not an abrupt bifurcation with change in density ratio, but a more gradual increase in narrowband response as the density ratio decreases. Figure 12. Spectral energy vs density ratio for ballistic bluff body at 50 m/s and x/D = 3.5, expressed as RMS flame edge fluctuation averaged over both flame branches, and RMS centerline transverse unsteady velocity. The correlation coefficient between the two flame branches, U,L (defined below), provides important information on the scale and/or correlation between the underlying flow structures perturbing them. 9 American Institute of Aeronautics and Astronautics U ,L U ( x) ( ( x, t ) L ( x, t ) (4) 2 ( L ( x, t )) 2 U ( x, t )) Note that negative and positive correlation coefficients mean an asymmetric and symmetric flame, respectively. Furthermore, a near zero correlation coefficient implies that the flame is disturbed by uncorrelated structures much smaller than their transverse separation distance, roughly the bluff body diameter. The dependence of correlation coefficient upon ρu/ρb is plotted in Figure 13, showing that the correlation coefficients are near zero, but possibly slightly positive, for ρu/ρb> ~2.5. The correlation coefficient monotonically decreases towards values of ρU,L ~ -0.6, indicative of growing correlation and antisymmetric motion with decreasing flame density ratio. Figure 13. Correlation coefficient between top and bottom flame edge position for ballistic bluff body at 50 m/s. To summarize these data, Figure 12 shows that there is a gradual increase in spectral energy at the asymmetric vortex shedding frequency, and Figure 13 shows a gradual increase in asymmetry and large scale structures in the wake. The very narrowband spectral nature of the flow in Figure 11 suggests that the flow evolves to a limitcycling, absolutely unstable flow at low density ratios. These data also suggest that the limit cycle amplitude of the absolutely unstable flow oscillator grows monotonically in amplitude with decreases in density ratio for ρu/ρb<2.4. B. Intermittency The above measures of the flame structures are averaged temporal attributes and do not illustrate that the flame dynamics are actually highly intermittent in time. As will be shown next, it appears that rather than characterizing the limit cycle amplitude as monotonically growing in amplitude with ρu/ρb, a better description is that the flow has two possible states and intermittently flips between them. The relative fraction of time the flow spends in each state monotonically varies with density ratio. This intermittent character is evident from Figure 14, which shows two images of the flame at the same operating conditions, but different instances of time. 10 American Institute of Aeronautics and Astronautics a) b) Figure 14. Intermittent wake structure evident in two flame images from the same high speed video for ballistic bluff body at 50 m/s, ρu/ρb = 1.7 In order to quantify this intermittency, the time series were locally fit to a sinusoidal fluctuation with a fixed frequency of fo=0.24Uo/D=~630Hz over a two period window. Within each window, a correlation coefficient, f (defined below), was calculated between the sine fit and the actual data, providing a measure of the goodness of fit. f U ( x) ( ( x, t ) sin(2 f 0t ) (5) 2 (sin(2 f 0t )) 2 U ( x, t )) A sample plot of the temporal dependence of ρf at ρu/ρb =1.7 is plotted in Figure 15, illustrating that it spends a significant fraction of time between 0.9-1.0 for flame edge position (slightly less for velocity), but also has certain periods of time where it drops to values well below 0.5. a) b) Figure 15. Correlation coefficient between sine fit and time signal for ballistic bluff body at 50 m/s, x/D = 3.5, for upper flame edge position and centerline transverse unsteady velocity at a) ρu/ρb = 1.7, b) ρu/ρb = 2.4 The fraction of time that this correlation coefficient exceeds a specified threshold value, ρt, was then computed at each spatial location and density ratio. Figure 16 plots a typical result at two threshold values. Notice the similarities between the spectral energy plot, Figure 12, and the intermittency plot, Figure 16. 11 American Institute of Aeronautics and Astronautics a) b) Figure 16. Percent of time that sine fit correlation coefficient is greater than the threshold value for ballistic bluff body at 50 m/s, x/D = 3.5 for a) upper flame edge and b) centerline transverse unsteady velocity. Results for two threshold values are presented with symbol x for ρt = 0.5 and symbol o for ρt = 0.8. Although not shown for reasons of space, results at other spatial locations indicate qualitatively similar results. The fraction of time that the flow spends in the “periodic state” monotonically grows with downstream distance. These data clearly support the notion that the rise in narrowband energy is associated with an increased fraction of time that the flow spends in a limit-cycling state, manifested by asymmetric structures with length scales of the order of the bluff body diameter. These results raise the question of how much the growth in amplitude with decreasing density ratio shown in Figure 11 is due to intermittency effects, and how much to a rise in limit cycle amplitude. The answer appears to be both, as shown next. From the sine fits in the previous section, we determined the conditional amplitude of the fit averaged over the time intervals where ρf>ρt, denoted by ζ’rms(ρf>ρt) in Figure 17. This may be compared to the density ratio dependency of the intermittency as shown previously in Figure 16. From this figure, it is clear that the apparent monotonic increase in the flame’s limit cycle amplitude is not due only to the intermittency, but that the limit cycle amplitude of the sinusoidal configuration also grows as density ratio decreases. Figure 17. Effect of density ratio and intermittency on limit cycle amplitude for ballistic bluff body at 50 m/s, x/D = 3.5, shown by comparing a) amplitude of flame edge fluctuation only during sinusoidal times, and b) percent of time that flame edge fluctuation is in a sinusoidal configuration, based on ρt = 0.8 The statistics of the conditioned time intervals of the “sinusoidal” and “random” bursts in the flame edge time series was also determined, suggesting that these behaviors are stochastic in nature. Although not shown, probability density functions of these time intervals are log-normal in behavior; averages of the “sinusoidal” time intervals, τ, 12 American Institute of Aeronautics and Astronautics are plotted against density ratio in Figure 18. This result shows that the time length of the “sinusoidal bursts” monotonically increases with decreasing density ratio. Figure 18. Density ratio dependence of average duration of the times when ρf > ρt, based on ρt = 0.8, at x/D = 3.5 IV. Concluding Remarks These results clearly show that the bluff body wake structure is a strong function of density ratio, but that no sharp bifurcation occurs with variations in ρu/ρb. Rather, at intermediate density ratios the wake exhibits two structures intermittently. Further understanding of the flow intermittency at realistic density ratios and conditions is a critical step in predicting bluff body flame response characteristics. A companion paper will describe comparisons of these data with parallel stability analyses25, as well as the frequency and amplitude characteristics of the externally forced flame and flow field as a function of ρu/ρb. References 1 Shanbhogue, S. J., Husain, S., and Lieuwen, T. "Lean blowoff of bluff body stabilized flames: Scaling and dynamics," Progress in Energy and Combustion Science Vol. 35, No. 1, 2009, pp. 98-120. 2 Criminale, W. O., Jackson, T. L., and Joslin, R. D. Theory and Computation in Hydrodynamic Stability. Cambridge: The Press Syndicate of the University of Cambridge, 2003. 3 Godreche, C., and Manneville, P. Hydrodynamics and Nonlinear Instabilities. Cambridge: University Press, Cambridge, 1998. 4 Schmid, P. J., and Henningson, D. S. Stability and Transition in Shear Flows. New York: Springer, 2001. 5 Anderson, K. R., Hertzberg, J., and Mahalingam, S. 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E., Chong, M. S., and Lim, T. T. "The vortex shedding process behind two-dimensional bluff bodies," Journal of Fluid Mechanics Vol. 116, 1982, pp. 77-90. 13 Cantwell, B., and Coles, D. "An experimental study of entrainment and transport in the turbulent near wake of a circular cylinder," Journal of Fluid Mechanics Vol. 136, 1983, pp. 321-374. 14 Bearman, P. "On vortex shedding from a circular cylinder in the critical Reynolds number regime," J. Fluid Mech Vol. 37, 1969, p. 577. 15 Roshko, A. "Experiments on the flow past a cylinder at very high Reynolds numbers," Journal of Fluid Mechanics Vol. 10, 1961, pp. 345-356. 13 American Institute of Aeronautics and Astronautics 16 Roshko, A. "On the Wake and Drag of Bluff Bodies," Journal of the Aeronautical Sciences Vol. 22, No. 2, 1955, pp. 124- 132. 17 Huang, R. F., and Chang, K. T. "Oscillation Frequency in Wake of a Vee Gutter," Journal of Propulsion and Power Vol. 20, No. 5, 2004, pp. 871-878. 18 Roshko, A. "On the drag and shedding frequency of two-dimensional bluff bodies." National Advisory Committee on Aeronautics, 1954. 19 Zdravkovich, M. M. Flow Around Circular Cylinders: A Comprehensive Guide Through Flow Phenomena, Experiments, Applications, Mathematical Models, and Computer Simulations: Oxford University Press, 1997. 20 Yu, M.-H., and Monkewitz, P. A. "The effect of nonuniform density on the absolute instability of two-dimensional inertial jets and wakes," Phys. Fluids Vol. 2, No. 7, 1990. 21 Erickson, R. R., Soteriou, M. C., and Mehta, P. G. "The Influence of Temperature Ratio on the Dynamics of Bluff Body Stabilized Flames," 44th AIAA Aerospace Sciences Meeting & Exhibit. Reno, Nevada, 2006. 22 Kiel, B., Garwick, K., Lynch, A., Gord, J. R., and Meyer, T. "Non-Reacting and Combusting Flow Investigation of Bluff Bodies in Cross Flow," 42nd AIAA/ASME/SAE/ASEE Joint Propulsion Conference & Exhibit. Sacramento, California, 2006. 23 Cross, C., Fricker, A., Shcherbik, D., Lubarsky, E., Zinn, B. T., and Lovett, J. A. "Dynamics of Non-Premixed Bluff BodyStabilized Flames in Heated Air Flow," ASME Turbo Expo. Glasgow, UK, 2010. 24 Kiel, B., Garwick, K., Lynch, A., and Gord, A. "A Detailed Investigation of Bluff Body Stabilized Flames," 45th AIAA Aerospace Sciences Meeting & Exhibit. Reno, Nevada, 2007. 25 Emerson, B., Lundrigan, J., O'Connor, J., Noble, D., and Lieuwen, T. "Convective and Absolute Instabilities in Reacting Bluff Body Wakes," ASME Turbo Expo. Vancouver, BC, 2011. 26 Monkewitz, P. A. "The absolute and convective nature of instability in two-dimensional wakes at low Reynolds numbers." Department of Mechanical, Aerospace, and Nuclear Engineering, Los Angeles, CA, 1988. 14 American Institute of Aeronautics and Astronautics
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