2.1. Jet nozzle facility and operating condition

As shown in figure 2(a), we consider the configuration of dual nozzles to introduce the air-jet flow into a transparent chamber ($300 \times 300 \times 780\ {\rm mm}^{3}$) made of $12$ mm thick acrylic plates. The nozzle assembly, fixed to the ceiling of the chamber, consists of a circular centre nozzle through which the liquid (tap water) column flow is injected vertically, and two annular-slit (widths $w_{1} = 0.9$ mm and $w_{2} = 0.5$ mm, respectively) gas nozzles (figure 2b). The liquid nozzle has inner diameter $D_L=5$ mm and length $40$ mm. In order to maintain the lowest perturbation in the initial liquid column, a $5$ mm long sponge filter is installed just before the exit of the liquid nozzle. Thus no agitation (or external forcing) on the surface of the falling water, other than that by the gas jet, was observed. We consider a flow rate $0.5\unicode{x2013}2.5\ {\rm l}\ \min ^{-1}$ of water, which corresponds to Reynolds number ($Re_L$) 2400–11 900 based on bulk water velocity and $D_L$. The exit of the upper gas nozzle is located $13$ mm above the liquid column exit, by which the upper gas nozzle can be kept away from the atomized liquid being flowed back and attached, following the conventional design of a dual-nozzle atomizer (Aliseda et al. Reference Aliseda, Hopfinger, Lasheras, Kremer, Berchielli and Connolly2008; Ridolfi & Folgarait Reference Ridolfi and Folgarait2020). The exit of the lower jet is positioned $20$ mm below the liquid jet exit for the purpose of controlling post-atomization. The circumferential diameters of the upper and lower slits are $D_{1} = 18.4$ mm and $D_{2} = 40$ mm, respectively (figure 2b), and the gas nozzles are aligned to have inclination angles $\theta _1$ and $\theta _2$ against the vertical axis. In this study, we vary $\theta _2$ as $20^{\circ }$, $40^{\circ }$ and $60^{\circ }$ to find out its effect on the flow field and the atomization process, while $\theta _1$ is fixed at $17^{\circ }$. The slight inclination of the upper nozzle helps the upper jet to interact with the liquid column right below the liquid exit, despite the presence of the wall splitting the liquid and gas flows (Zhao et al. Reference Zhao, Cao, Ning and Sun2009). As mentioned above, the vertical and horizontal distances between the exits of gas and liquid flow are necessary to avoid the nozzle clogging or to insulate the liquid nozzle with temperature-sensitive liquid, if necessary, for atomizing molten metal and polymeric material, etc. Regarding the relatively large gap between the liquid and gas flows, Tian et al. (Reference Tian, Zhao, Liu, Li and Xu2014) reported that the undulation frequency of the liquid interface is scaled consistently with $(u_{i}/\delta _{\circ })(\rho _{g}/\rho _{l})^{0.5}$, where $u_i$, $\delta _{\circ }$, $\rho _g$ and $\rho _l$ denote the interfacial velocity, the vorticity layer thickness at the nozzle exit, the gas density and the liquid density, respectively (Lasheras, Villermaux & Hopfinger Reference Lasheras, Villermaux and Hopfinger1998; Marmottant & Villermaux Reference Marmottant and Villermaux2004). Thus it can be inferred that the key mechanisms (or features) – e.g. formation and breakup of the liquid ligaments, behaviour of the liquid core, secondary breakup, and so on – involved in the flow-assisted atomization will not deviate from the canonical coaxial flows. The absolute magnitude in the frequency and wavelength (near the upper gas nozzle) of the present conditions might be different from the literature; however, it would not be critical in this study since the momentum of the upper jet is found to be the primary parameter to classify the regimes and breakup types below the lower nozzle ($y > 0$), as will be discussed in § 4.

Two air compressors with capacities $10$ HP (COMPWORLD, CWK-903N) and $4.5$ HP (Airbank, AB350) supply air to the upper and lower nozzles, respectively, and filters are installed in the middle of each gas supply pipe to remove oil (airborne) droplets, humidity and dust (figure 2b). Each nozzle receives air from four passages drilled through the nozzle edges, for the purpose of minimizing the asymmetry of the jets, and the pressure regulators are used to control the speed of the jet. The pressures applied to the nozzles are 0–0.1 MPa and 0–0.4 MPa for the upper and lower nozzles, respectively, and the jet exit velocities at maximum pressure are $144\ {\rm m}\ {\rm s}^{-1}$ and $389\ {\rm m}\ {\rm s}^{-1}$, respectively. In table 1, we have summarized the ranges of conditions tested in the present study.

Table 1.

Nozzle geometry and gas–liquid flow conditions tested in the present study, where S indicates shadowgraphy, and P indicates particle image velocimetry.

During the experiments, it is possible for the jet flow to bounce back from the chamber walls and affect the measurements. Even if we consider the worst case (all of the jet bounces back and flows upward), its velocity is scaled as $u_{rev} \sim (w_{j}/w_{chamber})^{2} u_{j} {< 0.046 u_{j}}$, where $u_j$ and $w_j$ are the jet velocity and width, respectively, and $w_{chamber}$ is the width of the chamber. Thus the confinement effect is estimated to be less than $5\,\%$ of the jet flow. However, to avoid clearly the unwanted recirculating flow inside the chamber, the guide-vane is placed at the bottom of the chamber, guiding the jet flow to the four exit ducts located at the bottom of the side-walls (figure 2a). At the end of the exit duct, a mini-pleat-type HEPA filter (with pressure loss $140$ Pa, negligible compared with the nozzle pressure ${\sim }10^{5}$ Pa) is installed to eliminate the smoke particles, used for the particle image velocimetry, while the liquid flows down through the slit placed near the edge of the vane and is drained via the outlet at the bottom wall. As a result, the disruption of flow is imperceptible; it is noted that the time-averaged vertical velocity is almost zero at $x/D_{2}>0.5$ in figures 5 and 6.

2.2. Particle image velocimetry to measure the gas flow

We use particle image velocimetry (PIV) to measure the gas-phase flow from the dual nozzle (figure 2a). The smoke generator (FOG 2010, Dantec Dynamics) connects the smoke seeder (Fog Fluid Blitz, SAFEX) to the smoke chamber placed above the atomization chamber (figure 2a). During the operation of the jet, the smoke is entrained through the smoke outlet to descend gently and spread uniformly inside the chamber. The rate at which the smoke is added (${\sim }0.5\ {\rm m}\ {\rm s}^{-1}$) is negligibly small compared to the jet (${\sim }0.25\,\%$ of the jet speed ${\sim }200\ {\rm m}\ {\rm s}^{-1}$), thus it does not disturb the flow. To illuminate the seed particles, a double-pulsed Nd:YAG laser (EverGreen, Quantel) with optics (cylindrical lens) is used to generate the laser sheet of $532$ nm wavelength with pulse energy $200$ mJ and repetition rate $15$ Hz. A PCO camera (PCO.1600, PCO AG) captures the particle image with resolution $1600 \times 1200$ pixels. We use a signal synchronizer (Timing Hub, IDT) to provide signals for laser triggering and the opening and closing of the camera shutter, by which two particle images are obtained with a $6\ \mathrm {\mu }{\rm s}$ time interval. For the evaluation of velocity vectors, we used the adaptive PIV algorithm (Dantec Dynamic Studio 5.1), in which the size and shape of the interrogation window are determined by the multi-pass calculation considering the brightness inside the interrogation window and the velocity gradient, yielding final vector fields with grid size $16 \times 16$ pixels. It is known that the adaptive schemes can provide a reliable spatial resolution of velocity fields in a highly stretching flow like a shear layer (Scarano Reference Scarano2002). As can be imagined, it is not easy to measure the flow field where the gas and liquid phases coexist (i.e. two-phase flow), owing to the high density and large size of the atomized droplets covering and blocking the field of view (FoV) and laser sheet, respectively. Thus we decided to measure the gas-phase flow without introducing the liquid jet, which we think is sufficient for understanding its influence on the atomization process, especially when the ratio of liquid-to-gas mass flux is as low as $O(10^{-4}\unicode{x2013}10^{-1})$, such that the liquid phase modifies weakly the gas phase (Kourmatzis & Masri Reference Kourmatzis and Masri2015; Rajamanickam & Basu Reference Rajamanickam and Basu2017). In the present study, the mass flux ratio $m_{L2}$ ranges from $0.0056$ to $0.14$ (table 1). On the other hand, we measured the gas velocity fields for the cases with the liquid column being atomized, at the positions where the direct interference from the liquid interface is not significant (see the supplementary material available at https://doi.org/10.1017/jfm.2022.435). Compared with the single-phase gas velocity, it is confirmed that the statistics (mean and fluctuating velocities) of the gas-phase outside of the liquid column would not change significantly (see figure S1 in the supplementary material), despite the widespread spray along the horizontal direction.

We measure the velocity fields at the centre ($z = 0$) plane, and the field of view is $-0.8 \leqslant x/D_{2} \leqslant 0.8$ and $0.15 \leqslant y/D_{2} \leqslant 1.4$ (the origin is located at the centre of the lower nozzle) (figure 2b). Thus, in the present set-up, the spatial resolution of the velocity measurement is $0.84$ mm ($= 0.021D_{2}$). For each condition in table 1, more than $500$ instantaneous flow fields were measured and analysed, which was found to be sufficient for obtaining the converged flow statistics.

In general, the uncertainty of the PIV measurement comes from various sources. Simply, the velocity ($u_{piv}$) evaluated from the particle image can be expressed as $u_{piv} \sim M\,\Delta s/\Delta t$ (where $M$ is the pixel magnification factor, $\Delta t$ is the time difference between two particle images, and $\Delta s$ is the particle displacement through $\Delta t$). Based on the error propagation analysis (Clifford Reference Clifford1973), the uncertainty in $u_{piv}$ can be estimated as $\delta (u_{piv})=\sqrt {\delta (M)^{2}+\delta (\Delta s)^{2}+\delta (\Delta t)^{2}}$ (Lawson et al. Reference Lawson, Rudman, Guerra and Liow1999; Choi & Park Reference Choi and Park2018; Choi, Lee & Park Reference Choi, Lee and Park2019; Maeng & Park Reference Maeng and Park2021). Here, $\delta (x)$ denotes the percentage error in measuring $x$. In the present set-up, the uncertainty in the magnification factor is calculated as $0.42\,\%$ with $M = 53.0\ \mathrm {\mu }{\rm m}\ {\rm pixel}^{-1}$. The inter-frame time interval was $1.0\ \mathrm {\mu }{\rm s}$, thus the error involved in operating time separation is estimated as $0.05\,\%$, where the time interval between the pair of images is $2.0$ ms. Finally, the uncertainty of $\Delta s$ is calculated as $3.8\,\%$, with average particle displacement $3.0$ pixels, which is found to be the dominant error source (Scarano Reference Scarano2002). Combining all contributions, the overall uncertainty for the velocity measurement is approximately $3.8\,\%$.

In the present experiment, it was not possible using PIV to measure directly the flow in the region $0.3 \lesssim |x/D_{2}| \lesssim 0.5$, $0.2 \lesssim y/D_{2} \lesssim 0.5$ close to the exit of the lower nozzle. Owing to the very high speed ($O(10^{2})\ {\rm m}\ {\rm s}^{-1}$) of the jet there, it is not allowed to capture the displacement of the seeders with the given interrogation window. It is noted that the atomization occurs mostly at $|x/D_{2}|\lesssim 0.2$ and $0.2\lesssim y/D_{2} \lesssim 1.0$, quite far from the lower nozzle exit, thus we have masked the region where the evaluated velocity vectors are not reliable. While we think that the flow field at the jet exit would not be critical for understanding the interaction between the liquid column and jet flow, we tried to estimate the jet exit velocity using particle tracking velocimetry and the conservation of momentum (for the details, see the supplementary material), which is used to characterize the jet flow.

2.3. Shadowgraph for the atomization visualization and droplet size measurement

We use the high-speed shadowgraph to visualize the pattern of atomization and measure the size of atomized droplets (see figure S4 in the supplementary material). The high-speed camera (NX5, IDT) is used to capture the high-resolution ($2337 \times 1728$ pixels) images at frame rate 730–1710 Hz for the visualization (and $200$ Hz for the measurement of droplet diameter) depending on the gas jet velocity, and a short exposure time is set to freeze the flow illuminated by a $750$ W tungsten light source (ARRILITE 750, ARRI). To aid the visualization of atomization, a diffuser plate is located between the chamber and the light source to distribute the light intensity uniformly. The camera is equipped with a $50$ mm lens (Samyang Optics), and its magnification factor is $63.6 \mathrm {\mu }{\rm m}\ {\rm pixel}^{-1}$. The FoV is, in general, $-0.5 \leqslant x/D_{2} \leqslant 0.5$ and $0 \leqslant y/D_{2} \leqslant 1.3$ (the origin is located at the centre of the lower gas nozzle). On the other hand, a longer FoV ($-0.5 \leqslant x/D_{2} \leqslant 0.5$ and $0 \leqslant y/D_{2} \leqslant 2.7$) is set when $\theta _{2} = 20^{\circ }$, as the atomization proceeds further downstream ($y/D_{2} > 1.0$) than other cases.

For the measurement of the droplet size, the droplet images are captured using a 180 mm lens with an extension tube (Canon, magnification factor $5\ \mathrm {\mu }{\rm m}\ {\rm pixel}^{-1}$). For Weber numbers 80–800, the droplet size was reported to be $150\unicode{x2013}500\ \mathrm {\mu }{\rm m}$ (Marmottant & Villermaux Reference Marmottant and Villermaux2004). Considering that the maximum effective Weber number is around $253$ in the present conditions (see § 2.4), and the population of the atomized droplets is not dense to prevent optical visualization, the shadowgraph with the macro lens set-up (resolution of the shadowgraph approximately 3 pixels ($\simeq 15.0\ \mathrm {\mu }{\rm m}$)) is sufficiently affordable to capture the droplets. While measuring droplet size, the diffuser plate is removed, since the macro lens requires a strong intensity of backlight owing to its narrow angle of view. The size of the droplets is quantified by applying the image processing algorithm (Kim & Park Reference Kim and Park2019; Piao & Park Reference Piao and Park2019; Lee & Park Reference Lee and Park2020) to the raw images (see figure S5 in the supplementary material). The raw droplet image is converted into a black-and-white colour scheme with respect to the prescribed threshold value adjusted adaptively according to the average intensity around each pixel location (Bradley & Roth Reference Bradley and Roth2007). After binarization, the hole inside the binarized area of the droplet (i.e. minima) is eliminated and the out-focused droplet is excluded if the magnitude of intensity gradient $(\partial I/\partial x)^{2}+(\partial I/\partial y)^{2}$ (where $I(x,y)$ denotes the local light intensity) on the droplet edge is less than the assigned threshold. Finally, the equivalent diameter of the droplet is calculated assuming that it is oblate shaped. The field of view for droplet size measurement is located at $-0.15 \leqslant x/D_{2} \leqslant 0.15$ and $14.4 \leqslant y/D_{2} \leqslant 14.6$, determined to capture the close-to-final droplet size, based on previous results (Aliseda et al. Reference Aliseda, Hopfinger, Lasheras, Kremer, Berchielli and Connolly2008; Hinterbichler et al. Reference Hinterbichler, Steiner and Brenn2020). Aliseda et al. (Reference Aliseda, Hopfinger, Lasheras, Kremer, Berchielli and Connolly2008) observed that using phase Doppler particle analysis, the size of the atomized water droplets from the dual nozzle converges after $y/D_{1} \geqslant 30$, where $D_1$ is the diameter of the upper nozzle (it is $y/D_{1} = 30.4$ for the present study), and Hinterbichler et al. (Reference Hinterbichler, Steiner and Brenn2020) showed that distant from the nozzle, the size distribution becomes saturated along the radial direction. Thus the measured diameter is expected to converge, and we think it is enough to analyse comparatively the relation between the atomization process and the resulting characteristics of sprays. To obtain the statistically meaningful probability density function (p.d.f.) for the droplet size distribution (see the supplementary material for the p.d.f. of measured droplet size), more than 100 instantaneous images (including approximately 60 000 droplets) are used for each case, which was found to be enough to have a converged result. Furthermore, we calculated that the time duration of measuring the droplets is sufficiently longer than the expected breakup time scale of the liquid jet estimated from the maximum growth rate so that the present droplet size converges statistically.

Regarding the droplet size estimation, we performed the uncertainty analysis using error propagation theory. The uncertainty of the droplet diameter measurement (Asgarian et al. Reference Asgarian, Yang, Tang, Bussmann and Chattopadhyay2020) is obtained as $\delta d_{32}=\sqrt {(\delta d_{res}^{2}+\delta d_{thresh}^{2})/m}$, where $\delta d_{res}$ and $\delta d_{thresh}$ denote the errors caused by the resolution of the image and threshold of binarization, respectively, and $m$ is the total number of detected droplets. For the resolution error, the pixelated droplet can be larger than up to $1$ pixel in diameter than the exact value, thus $\delta d_{res} < 1\ {\rm pixel} = 5.0 \ \mathrm {\mu }{\rm m}$. During thresholding, the raw image is converted to the binarized (pixelated) image. In this process, the false pixel that does not contain the bubble area might be converted as the bubble (on the other hand, the bubble-containing pixel can be precluded). Asgarian et al. (Reference Asgarian, Yang, Tang, Bussmann and Chattopadhyay2020) estimated the thresholding error as $\delta A_{thresh}/A = 8\unicode{x2013}12\,\%$ (where $A$ denotes the exact area occupied by the droplet) for resolution $2.4\unicode{x2013}19.8\ \mathrm {\mu }{\rm m}\ {\rm pixel}^{-1}$ ($5.0\ \mathrm {\mu }{\rm m}\ {\rm pixel}^{-1}$ in this study). Taking the droplet diameter as $d_{32}=\sqrt {4A/{\rm \pi} }$, we obtain $\delta d_{32}/d_{32}=0.5\delta A/A$. Thus the upper limit of $\delta d_{thresh}$ is $6\,\%$ of $d_{32}$. Given that $95\,\%$ of the droplet population is below $2000\ \mathrm {\mu }{\rm m}$, the upper bound $\delta d_{thresh}$ is ${\sim }30\ \mathrm {\mu }{\rm m}$. Combining these, the total uncertainty is calculated as $\delta d_{32}= 0.12\ \mathrm {\mu }{\rm m}$, which is less than $1\,\%$ of $d_{32}$, indicating that the measurement error is not significant.

2.4. Parameter ranges investigated

In addition to varying the angle of the lower jet ($\theta _2$), we consider a range of flow conditions by controlling the pressure of the upper ($P_{1}=0\unicode{x2013}0.1$ MPa) and lower ($P_{2}=0\unicode{x2013}0.4$ MPa) jets independently, by which we achieve the exit velocity of the upper and lower jets up to $u_{1} = 144\ {\rm m}\ {\rm s}^{-1}$ and $u_{2} = 389\ {\rm m}\ {\rm s}^{-1}$, respectively (table 1). The Reynolds number for the annular jet is defined as $Re_{i}=u_{i}\sqrt {4D_{i} w_{i}}/\nu _{g}$, where $D_i$ is the annular diameter and $w_i$ is the slit width (subscripts $i = 1$ and $2$ denote the upper and lower nozzles, respectively), based on the assumption that it has the same momentum with the circular nozzle emitting the gas at the same exit velocity ($u_i$) (Rehab et al. Reference Rehab, Villermaux and Hopfinger1997; Villermaux & Rehab Reference Villermaux and Rehab2000). The Reynolds numbers ranges for the upper and lower jets for the shadowgraph are $Re_{1} = 3.9\unicode{x2013}6.2 \times 10^{4}$ and $Re_{2} = 5.3\unicode{x2013}8.5 \times 10^{4}$, respectively, and set to be slightly lower than that ($Re_{1} = 6.8\unicode{x2013}10.9 \times 10^{4}$ and $Re_{2} = 1.9\unicode{x2013}2.4 \times 10^{5}$) for the PIV measurement (see table 1). This is because the atomization process occurring under a high-Reynolds-number jet tends to be unresolved because of the limited spatial and temporal resolution of present measurement set-up. The choice of different $Re$ ranges for velocity measurement and visualization was also inevitable but justified in previous studies with two parallel coaxial gas jets (Au & Ko Reference Au and Ko1987; Dahm et al. Reference Dahm, Frieler and Tryggvason1992; Rehab et al. Reference Rehab, Villermaux and Hopfinger1997). Au & Ko (Reference Au and Ko1987) performed a visualization and velocity measurement of the coaxial jet at Reynolds numbers $1.4 \times 10^{5}$ and $4 \times 10^{4}$, respectively, to elucidate the vortical structure, and Rehab et al. (Reference Rehab, Villermaux and Hopfinger1997) showed that the global vortical structure in the coaxial gas jets is dominated by the velocity ratio of jets, rather than the Reynolds number (tested at $5 \times 10^{2}\unicode{x2013}1.4 \times 10^{5}$). If the Reynolds number is high enough to have a shear-layer instability, then the resulting large-scale vortical structure is affected weakly by the Reynolds number (Dahm & Dimotakis Reference Dahm and Dimotakis1987; Dowling & Dimotakis Reference Dowling and Dimotakis1990; Dahm et al. Reference Dahm, Frieler and Tryggvason1992). For the problem of jet–crossflow interaction, it is well known that the resulting vortex dynamics is independent of the Reynolds number (Broadwell & Breidenthal Reference Broadwell and Breidenthal1984; Smith & Mungal Reference Smith and Mungal1998; Shan & Dimotakis Reference Shan and Dimotakis2006; Park & Park Reference Park and Park2021). In the considered range of Reynolds numbers, therefore, the momentum flux ratio between two gas jets is more relevant to the jet interaction than the Reynolds number. The momentum flux ratio, defined as $m_{12}=m_{1}/m_{2}=u_{1}^{2} A_{1}/(u_{2}^{2} A_{2})$ (where $A_i$ is the nozzle exit area), varies from $0.043$ to $1.25$.

In addition, the momentum flux ratios between the liquid flow and each gas jet, defined as $m_{L1}=m_{L}/m_{1}=\rho _{L} u_{L}^{2} A_{L}/(\rho _{G} u_{1}^{2} A_{1})=0.084\unicode{x2013}0.39$ and $m_{L2}=m_{L}/m_{2}=\rho _{L} u_{L}^{2} A_{L}/(\rho _{G} u_{2}^{2} A_{2})=0.0056 \unicode{x2013}0.14$, respectively, are found to be important in determining the atomization regime and liquid core length. As a measure of atomization performance, the Weber numbers ($We_{i}=\rho _{G} u_{i}^{2} D_{L}/\sigma$) of the upper ($We_1$) and lower ($We_2$) jets were calculated to be $O(10^{2}\unicode{x2013}10^{4})$ (table 1). Compared to previous studies on liquid atomization, this $We$ range is quite high, which is caused by the relation between characteristic velocity scale and the atomization process. That is, in previous studies, the liquid and gas flows interact immediately at the nozzle exit, thus it is reasonable to choose the nozzle-exit velocity as the characteristic velocity. In the present study, on the other hand, the interaction occurs far away from the nozzle (approximately $13h_1$ and $40h_2$ from the upper and lower nozzle exits, respectively), at which point the gas momentum that incurs the liquid atomization has decreased significantly compared to the nozzle exit. Based on this, we newly defined the effective Weber number, $We_{eff}$, based on the gas velocity at which the atomization actually takes place. For the upper jet, the mean vertical velocity at $y/D_{2}=-0.2$ is selected as a characteristic velocity, measured as $\bar {u}_{y}/u_{1} = 0.35$. At the lower atomization site ($y/D_{2} > 0$), the lower jet is responsible for the atomization of the liquid column, and the corresponding gas velocity was measured as $\bar {u}_{y}/u_{2} = 0.1$ ($y/D_{2} = 0.8$ and $\theta _{2} = 20^{\circ }$), $0.2$ ($0.5$ and $40^{\circ }$) and $0.3$ ($0.4$ and $60^{\circ }$). As a result, the effective Weber numbers for the upper and lower jets are obtained as $We_{eff1} = 2.2\unicode{x2013}13.8$ and $We_{eff2} = 11\unicode{x2013}468$, respectively, similar to previous studies. Below, we show that the atomization regime and the size of atomization droplets are correlated well with $We_{eff}$. Finally, the Ohnesorge number ($Oh=\mu _{L}/(\rho _{G} D_{L} \sigma )^{0.5}$) is calculated as $0.043$, indicating that the viscous time scale is much shorter than the capillary time scale in the process of the water droplet deformation or breakage. Considering all the variations of nozzle geometry and flow conditions, in total, the experiments were carried out for $24$ and $68$ different cases for the atomization visualization (including droplet size measurement) with the high-speed shadowgraph and gas-phase velocity measurement with the PIV, respectively.

3.1. Analysis of the gas-phase jet flow

Figures 5 and 6 show the gas-phase flow structures depending on the momentum flux ratio ($m_{12}$) with the angle of the lower nozzle at $\theta _{2} = 20^{\circ }$ and $40^{\circ }$, respectively (the lower jet is fixed at $Re_{2} = 1.09 \times 10^{5}$). When the upper jet is idling, the dual-peaked flow, a typical feature of an annular jet, is generated from the lower nozzle (figure 5a), in which a strong vertical velocity fluctuation ($u'_{y,rms}$) takes place following the shear layers (figure 5c) and the horizontal velocity ($u'_{x,rms}$) as well, with a smaller intensity (figure 5b). As the flow evolves downstream, the two peaks approach the centreline as the inner shear layers collide at $y/D_{2} \simeq 0.7$, as shown in figures 5(a–c), and develop into a single-core jet at $y/D_{2} > 1.3$ (not shown here, since it is outside of the present FoV). At the vicinity of the lower nozzle ($y/D_{2} \simeq 0.5$), horizontal velocity fluctuations of a stronger intensity are induced, compared with the vertical component. This indicates that the flow agitation comes mostly from the merging process of annular jets into the single-core jet, not from the roll-up process of the jet shear layer. Without the upper jet, there is a backflow near the lower-nozzle exit at $-0.2 < x/D_{2} < 0.2$ and $y/D_{2} < 0.6$ (figure 5a), which prevented the liquid column from descending (figure 4a). One of the advantages of the dual-nozzle configuration is shown well in figure 5(d), such that backflow is removed completely by operating the upper jet as well as the lower one, even at a relatively weak pressure ($m_{12}$ is as small as $0.11$). Since backflow is an important phenomenon causing the degradation of atomization performance (inconsistent droplet size distribution and the spray angle, but it is better to produce finer droplets, as we will show below), we will discuss the condition for its occurrence in detail later. With a dual-nozzle operation, the upper jet prevents the collision of inner shear layers of the lower jet (figure 5d), thus $u'_{x,rms}$ is suppressed substantially at the centreline (figure 5e), and $u'_{y,rms}$ is predominant on the edges of the upper and lower jets (figure 5f). This jet interaction increases the horizontal distance between the position (at $y/D_{2} \simeq 0.9$) of maximum velocity fluctuation (figures 5e, f), at which the major atomization occurs. Note that the interaction between the upper jet and the inner shear layer of the lower jet at $-0.2< x/D_{2}<0.2$ and $0.3< y/D_{2}<0.8$ causes a reduction of $u'_{y,rms}$ (figure 5f), and $u'_{x,rms}$ becomes slightly stronger than that of the outer shear layer (figure 5e), which is different from the case without the upper jet (figures 5b,c). In the present configuration, the water column is atomized mainly at $x/D_{2} = 0$ and $y/D_{2} \simeq 0.2\unicode{x2013}1.0$ (figures 3, 4b and 4c). Therefore, the liquid column begins to be disturbed (and atomized) when it meets the inner shear layer of the lower jet, indicating that the strength of the shear layer is an important parameter to determine the atomization performance.

When $\theta _2$ increases to $40^{\circ }$ (figure 6), it is observed that backflow still exists when operating the lower nozzle only, appearing further upstream ($y/D_{2} < 0.3$; figure 6a). The inner shear layers interact also earlier at $y/D_{2} < 0.5$ (figure 6b), beyond which the dual-peaked jet merges into the single-core jet with an accelerated velocity but a smaller lateral jet width, compared with the case $\theta _{2} = 20^{\circ }$ (figure 5a). As the lateral distance between jet shear layers is reduced faster, the interaction of the inner shear layers is more concentrated at the centre region, enhancing $u'_{x,rms}$ (figure 6b), while $u'_{y,rms}$ is relatively weaker (figure 6c), which is opposite to the case $\theta _{2} = 20^{\circ }$. Likewise, backflow disappears when the mass flux ratio increases to $m_{12} = 0.11$ (figure 6d), and the upper jet tends to reduce both $u'_{x,rms}$ and $u'_{y,rms}$ in the core region by inhibiting the interaction of the inner shear layers (figures 6e, f). As the single-core jet evolves ($y/D_{2} > 0.5$), $u'_{x,rms}$ is enhanced more than $u'_{y,rms}$ along the centreline.

For further analysis, the vertical profiles of time-averaged vertical velocity and root-mean-square (r.m.s.) velocity fluctuations are plotted along the centreline ($x = 0$), depending on $m_{12}$ and $\theta _2$, in figure 7. When the upper nozzle is idling ($m_{12} = 0$), the negative $\bar {u}_{y}$ (i.e. backflow) exists for all $\theta _2$, and its coverage is reduced from $y/D_{2} < 0.7$ to $0.2$ with increasing $\theta _2$ (figures 7a–c). Increasing $m_{12}$, this reversed flow is mitigated and suppressed completely above a certain value of $m_{12}$, which increases as $m_{12} = 0.067$ (for $\theta _{2} = 20^{\circ }$), $0.11$ ($40^{\circ }$) and $0.17$ ($60^{\circ }$). It is noted that figure 7(c) does not indicate that the strength of backflow ($m_{12} = 0$) is reduced substantially by larger $\theta _2$, but most of the backflow region ($y/D_{2} < 0.2$) is not optically accessible, owing to the set-up. For all cases, as the flow evolves downstream, the vertical velocity ($\bar {u}_{y}$) increases gradually to the maximum, which is also shifted upstream with increasing $\theta _2$, since the jets merge earlier, as shown in figures 5 and 6. As $m_{12}$ increases, on the other hand, $\bar {u}_{y}$ is accelerated before the inner shear layers of the lower jet collide (figures 7a–c). While the velocity fluctuation is more intensified, for $m_{12}=0$, along the vertical and horizontal direction for $\theta _{2} = 20^{\circ }$ and $40^{\circ }$, respectively, before the single-core jet is formed (figures 7d,e,g,h), both fluctuations tend to decrease with increasing $m_{12}$. As we have shown above, this is because the upper jet reduces the strength of the lower-jet shear layer and also delays further the collision of the inner shear layers in the lower jet. For the largest $\theta _{2} = 60^{\circ }$ among those tested, exceptionally, the strengths of $u'_{x,rms}$ and $u'_{y,rms}$ are comparable (figures 7f –i). This is because the lower jet is directed almost horizontally towards the centreline, thereby generating a highly deflected flow along both directions.

Figure 7.

(a–c) Time-averaged vertical velocity profiles ($\bar {u}_{y}/u_{2}$), (d–f) horizontal r.m.s. velocity fluctuation profiles ($u'_{x,rms}/u_{2}$), and (g–i) vertical r.m.s. velocity fluctuation profiles ($u'_{y,rms}/u_{2}$) along the centreline ($x = 0$), where: (a,d,g) $\theta _{2} =20^{\circ }$; (b,e,h) $40^{\circ }$; (c,f ,i) $60^{\circ }$. Symbols: $\circ$ indicates $m_{12} = 0$; $\times$ indicates $m_{12} = 0.067$; $\vartriangle$ indicates $m_{12} = 0.11$; $+$ indicates $m_{12} = 0.14$; $\lozenge$ indicates $m_{12} = 0.17$. For all cases, $We_{eff2} = 83\unicode{x2013}747$ and $Re_{2} = 1.9 \times 10^{5}$. The arrows denote the direction of increasing $m_{12}$.

As the flow develops into a single-core jet after the maximum $\bar {u}_{y}$, the resulting flow velocity decays gradually downstream (figures 7a–c), which is faster for the stronger upper jet ($m_{12}$) when $\theta _{2} = 20^{\circ }$ and $40^{\circ }$. This is because the upper jet delays the lower-jet merging and subsequently expands the jet width, resulting in the decrease in the jet velocity following the momentum conservation. For the largest $\theta _{2} = 60^{\circ }$, on the other hand, the vertical velocity is almost independent of $m_{12}\ (>0)$ (figure 7c), as the lower jet from larger $\theta _{2}$ will block the upper jet. After the jet merging, the dependency of velocity fluctuations on $m_{12}$ is not clear, because the difference in fluctuations is more prominent at the shear layer rather than the centreline (see $x/D_{2} = 0$ and $y/D_{2} > 1.0$ in figures 5 and 6). In relation to the flow structures analysed, we will discuss the process of water atomization below.

3.2. Water column atomization

To help in catching the general picture of the atomization process and the underlying physics, in figure 8, we show the sequential process of water column atomization, depending on the angle ($\theta _2$) of the lower nozzle. Other parameters are fixed as $m_{12} = 0.11$, $We_{eff2} = 28\unicode{x2013}252$, $Re_{2} = 1.1 \times 10^{5}$ and $m_{L2} = 0.051$. As the liquid column descends, it is perturbed locally by the upper jet (larger-scale waviness indicated by an arrow in figures 8ai–ci). As it encounters the inner shear layer of the lower jet, it is further pushed downwards and the water droplets are spread out (dispersed in a wider angle as $\theta _2$ increases). Owing to the interaction with the lower jet, the water column becomes thinner, forming incipient membranes (indicated by an arrow in figures 8aii–cii). When this membrane reaches a critical thickness below which it cannot be any thinner, it is developed into the membrane with a multiple-cell shape having a certain wavelength while remaining at a constant thickness (highlighted by an arrow in figures 8aiii–ciii). This kind of disturbance in the liquid–air interface is typical in the Rayleigh–Taylor instability, which occurs when two fluids with different densities are accelerated across the interface (Taylor Reference Taylor1950), and has been discussed as one of the major mechanisms of liquid atomization by prior studies (Joseph et al. Reference Joseph, Belanger and Beavers1999; Varga et al. Reference Varga, Lasheras and Hopfinger2003; Marmottant & Villermaux Reference Marmottant and Villermaux2004; Kourmatzis & Masri Reference Kourmatzis and Masri2015). Finally, the cell-like membrane structures are broken into the droplets (noted by an arrow in figures 8aiv–civ). As the visualization indicates its importance, we will discuss the quantitative aspect of Rayleigh–Taylor instability in more detail later.

Figure 8.

Sequential atomization process of the falling water column with (a) $\theta _{2} = 20^{\circ }$; (b) $\theta _{2} = 40^{\circ }$; (c) $\theta _{2} = 60^{\circ }$. The time difference between two instants is $1.4$ ms in (a,b), and $0.45$ ms in (c). For all cases, $m_{12} = 0.11$, $We_{eff2} = 28\unicode{x2013}252$, $Re_{2} = 1.1 \times 10^{5}$, and $m_{L2} = 0.051$.

Meanwhile, the location where the atomization starts approaches closer to the lower nozzle with increasing $\theta _2$: $y/D_{2} \simeq 1.0$ (for $\theta _{2} = 20^{\circ }$), $0.4$ ($40^{\circ }$) and $0.3$ ($60^{\circ }$), which corresponds to the maximum $\bar {u}_{y}$ shown in figures 7(a–c). Except for the case $m_{12} = 0$, the slope $\partial (\bar {u}_{y}/u_{2})/\partial (y/D_{2})$ becomes steeper with increasing $\theta _{2}$; the maximum slope increases, measured upwards from $0.12$ at $y/D_{2} \simeq 0.8$ ($\theta _{2} = 20^{\circ }$) to $0.86$ at $0.3$ ($60^{\circ }$). Thus it can be said that the vertical acceleration in the flow by the dual nozzle is the main driving source of the liquid atomization. In addition, it should be noted that the effective atomizing gas is the resultant flow of the axisymmetric introduction of the jet, which is parallel statistically to the liquid. As shown in figures 8(ai)–8(ci), the atomization occurs near the centreline of the nozzle ($-0.1 < x/D_{2} < 0.1$) where the horizontal velocity of the gas jet flow weakens significantly or cancels out on average (see $-0.1 < x/D_{2} < 0.1$ in figures 5a, 5d, 6a, 6d). As the width of this region ($5.44D_{L}$) encompasses the diameter of the liquid column ($D_L$), the gas flow can be regarded to be statistically and locally parallel to the liquid jet at the atomization site. The visualization also shows that the liquid breakup occurs near the centreline ($-0.1 < x/D_{2} < 0.1$). In figure 8, the liquid bulk is disintegrated by the lower gas jet along the centreline as indicated by the arrows, despite the gas jet being introduced initially with a non-zero angle.

The atomization process also varies significantly depending on the mass flux of the liquid column (i.e. $m_{L2}$). Shown in figure 9 (see also supplementary movie 2) is the atomization pattern for different liquid flux ratios ($m_{L2}$) when the upper nozzle is idling ($m_{1} = 0$). When the liquid flux is relatively smaller than the gas, the water column tends to stagnate near the nozzle exit (highlighted with a solid arrow in figure 9a), rather than descending. The momentum of the backflow induced by the lower jet is strong enough to prevent the water column from falling. The condition on which this event occurs will be discussed analytically in § 4.1. On the other hand, the intermittent pouring of a sustained water lump occurs when backflow no longer bears the weight of the stagnated water and the downward momentum of the falling liquid column (shown with a solid arrow in figure 9b). Therefore, two ways of atomization are found in the case $m_{L2}=0.0056$, $We_{eff2}=112$, $Re_{2}=1.1 \times 10^{5}$ and $\theta _{2}=40^{\circ }$. First, the atomization is driven by the shearing of the lower jet occurring at the bottom of the stagnated liquid (noted with a dashed arrow in figure 9a), and the next process occurs along with the intermittent pouring of stagnated liquid (figure 9b). As the liquid flux increases, this liquid puddle disappears (figures 9c,d), but a strong backflow still occurs (not strong enough to lift up the liquid column as seen in figures 9a,b) and draws back a large number of droplets upwards (figure 9c). For the largest volume flux (momentum) of the liquid column, which is large enough to overcome backflow, the liquid is not fully atomized by the lower jet and forms a large lump in a spray (solid arrow in figure 9d).

Figure 9.

Representative instantaneous flows showing the atomization process of the falling water column depending on (a,b) $m_{L2} = 0.0056$, (c) $m_{L2} = 0.051$, (d) $m_{L2} = 0.14$. For all cases, $We_{eff2} = 112$, $Re_{2} = 1.1 \times 10^{5}$ and $\theta _2 = 40^{\circ }$. See also supplementary movie 2.

3.3. Size of atomized droplets

We have shown that the atomization process differs substantially depending on $m_{12}$, $\theta _{2}$ and $m_{L2}$. To understand the effect of each variable on the resulting outcome, we measured the size of the droplets according to these variables. As we have explained in § 2.3, the droplet size was measured at a downstream location where $-0.15 \leqslant x/D_{2} \leqslant 0.15$ and $14.4 \leqslant y/D_{2} \leqslant 14.6$ to capture the representative droplet information, which is adequate to analyse comparatively the relation between the atomization process and the resulting characteristics of sprays. In figure 10(a), we have plotted the variation of the Sauter mean diameter ($d_{32}$) – defined as $d_{32}= \sum _{i=1}^{m}d_{i}^{3}/\sum _{i=1}^{m}d_{i}^{2}$, where $d_i$ is the droplet diameter, and $m$ denotes the total number of droplets – while varying $m_{12}$ (with $u_2$ fixed). For $\theta _{2} = 20^{\circ }$ and $m_{L2} = 0.051$, the droplets are larger than for other cases because a portion of liquid lump falls without being fully atomized. Similar results were reported when the liquid jet width (i.e. liquid flux) is large (Lasheras & Hopfinger Reference Lasheras and Hopfinger2000; Marmottant & Villermaux Reference Marmottant and Villermaux2004). For other cases, the liquid column is atomized substantially into smaller droplets and, interestingly, the droplet size does not change much as the strength of the upper jet increases, although the gas-phase flow structure (and corresponding atomization regime, see § 3.4) changes significantly; for example, with $\theta _2 = 40^{\circ }$ and $m_{L2} = 0.027$, the atomization regime transitions as a floating liquid column regime, a backflow regime, a bulk atomization regime, and a droplet atomization regime, with $m_{12} = 0$, 0.11, 0.17 and $0.27$, respectively (see § 3.4 for the regime classification). This is because the upper and lower jets play opposite roles in determining the atomization outcomes. The disintegration of the liquid column occurs earlier above the lower nozzle ($y < 0$) as the upper jet becomes stronger; however, the relative velocity at the interface of the droplets against the lower jet weakens because it has been accelerated already by the upper jet. Thus the additional atomization of the droplets by the lower jet is mitigated. When the upper jet is weak, on the other hand, most of the atomization occurs when the weakly perturbed liquid column interacts with the lower jet. More theoretical background to this argument will be given in § 4.5. Looking closely, the droplet size decreases slightly with $m_{12}$, corresponding to the backflow and floating liquid column regimes (except for the case $\theta _{2}=20^{\circ }$ and $m_{L2}=0.051$). This is because the strong velocity gradient (at $x/D_{2} \simeq 0$) forces the disintegration of the liquid column into smaller ligaments, resulting in finer droplets. In addition, comparing the open and closed symbols in figure 10, the droplet size increases with the liquid flux ratio ($m_{L2}$), indicating the decrease of relative strength of the atomizing gas. As shown in figures 4(c) and 4(d), which correspond to $m_{L2} = 0.051$ and $0.027$, respectively, the finer droplets are formed for $m_{L2} = 0.027$.

Figure 10.

Sauter mean diameter ($d_{32}$) of the atomized droplets depending on (a) momentum flux ratio between the two gas jets ($m_{12}$), (b) angle of the lower nozzle ($\theta _2$), and (c) momentum flux ratio of the liquid to the lower gas jet ($m_{L2}$). For (a,b): closed symbols use $m_{L2} = 0.051$, $We_{eff2} = 28\unicode{x2013}252$, $Re_{2} = 1.1 \times 10^{5}$; open symbols use $m_{L2} = 0.027$, $We_{eff2} = 52\unicode{x2013}468$, $Re_{2} = 1.5 \times 10^{5}$. For (c), $\theta _{2} = 40^{\circ }$, $m_{12} = 0$, $We_{eff2} = 112$ and $Re_{2} = 1.1 \times 10^{5}$.

Figure 10(b) shows the variation of $d_{32}$ with $\theta _2$, for the same data as in figure 10(a). As $\theta _2$ increases, the droplet size decreases in all cases. This is because the inertial acceleration experienced by the liquid column increases as $\theta _2$ increases, as discussed for figures 7(a–c). Therefore, in order to analyse the droplet size depending on $\theta _2$, it is important to understand the acceleration of the flow in the region of the liquid atomization (the discussion is given in § 4.1). On the other hand, at each $\theta _2$ and $m_{L2}$, the small difference according to $m_{12}$ shows again the weak dependency of $m_{12}$ on the droplet size. Finally, in figure 10(c), the dependency of $d_{32}$ on the flux of the liquid column ($m_{L2}$) is shown. As expected, the droplet size increases gradually as the mass flux of the liquid column increases, and it is partly because the liquid column does not have enough time to interact with the dual-jet flow as $m_{L2}$ increases.

Even considering the effective Weber number that we have defined in order to characterize the atomization process more closely, the present droplet size is larger than those reported in the literature (Lasheras et al. Reference Lasheras, Villermaux and Hopfinger1998; Varga et al. Reference Varga, Lasheras and Hopfinger2003; Marmottant & Villermaux Reference Marmottant and Villermaux2004; Baillot et al. Reference Baillot, Blaisot, Boisdron and Dumouchel2009; Kourmatzis & Masri Reference Kourmatzis and Masri2015). In addition, we noted that the initial diameter of the liquid column (i.e. size of the liquid outlet) affects the final droplet size (Dumouchel Reference Dumouchel2008; Baillot et al. Reference Baillot, Blaisot, Boisdron and Dumouchel2009). The present liquid outlet is wider ($D_{L} = 5$ mm) than others ($D_{L} = 0.11\unicode{x2013}2.9$ mm for Lasheras et al. Reference Lasheras, Villermaux and Hopfinger1998; Varga et al. Reference Varga, Lasheras and Hopfinger2003; Kourmatzis & Masri Reference Kourmatzis and Masri2015). Concerning these, we have plotted the dimensionless droplet diameter ($d_{32}/D_L$) based on the effective Weber number (figure 11). It is noted that the present data were chosen for operating the upper or lower nozzle only, to compare with the previous results obtained with the single-nozzle configuration. As shown, it is interesting to see that all the data from different conditions (present and previous studies) collapse well into a single curve of $d_{32}/D_{L} \sim We_{eff}^{-0.7}$. This strong dependency of droplet size on the liquid outlet size and effective Weber number will be investigated in future work.

Figure 11.

Variations of the droplet diameter ($d_{32}$) normalized by the liquid exit size depending on the effective Weber number. The dashed line corresponds to the curve $d_{32}/D_{L} \sim We_{eff}^{-0.7}$.

Figure 12 shows the distribution of droplet size depending on the gas velocity of the lower nozzle and the operation of dual nozzles. For the sole operation of the lower nozzle, the distribution becomes concentrated in the small droplet size (${\sim }30 \mathrm {\mu }{\rm m}$) as the gas velocity (i.e. $We_{eff}$) increases. It is measured that for $We_{eff2} = 210$, the addition of the upper jet ($We_{eff1} = 210$) lowers the peak value and results in larger droplets, which resembles the distribution of the single-nozzle atomization with the lower $We_{eff1}$. This is attributed to the reduced strength of the spatial velocity gradient owing to the upper gas jet. It was reported that the size of the atomized droplets can be dictated by a single distribution, such as the log-normal (Ling et al. Reference Ling, Fuster, Zaleski and Tryggvason2017), gamma (Huck et al. Reference Huck, Osuna-Orozco, Machicoane and Aliseda2022) or multimodal (Balachandar et al. Reference Balachandar, Zaleski, Soldati, Ahmadi and Bourouiba2020; Jiang & Ling Reference Jiang and Ling2021) distribution, when more than one formation process is involved. The log-normal and gamma distributions are expressed as $p(d)=(1/(d\hat {\sigma }\sqrt {2{\rm \pi} }))\cdot \exp (-(\ln {d}-\hat {\mu })^{2}/(2\hat {\sigma }^{2}))$ and $p(d)=(\beta ^{\alpha }/\varGamma (\alpha ))d^{\alpha -1}\exp (-\beta d)$, respectively. Here, $\hat {\mu }$ and $\hat {\sigma }$ denote the expected average and standard deviation of $\ln {d}$, $\varGamma$ corresponds to the gamma function, and $\alpha$ and $\beta$ are defined as $\alpha = (\tilde {\mu }/\tilde {\sigma })^{2}$ and $\beta = \alpha /\tilde {\mu }$, respectively, where $\tilde {\mu }$ and $\tilde {\sigma }$ are the mean and standard deviation of $d$, respectively. The inset of figure 12 shows the droplet size distributions for the single and dual nozzle in a log-log scale with the fitted log-normal and gamma distributions, where $(\hat {\mu }, \hat {\sigma }, \tilde {\mu }, \tilde {\sigma }) = (1.8, 0.30, 68, 45)$ for the single nozzle, and $(\hat {\mu }, \hat {\sigma }) = (1.9, 0.33)$ for the dual nozzle. (Here, the gamma distribution is fitted only for the single nozzle for the sake of clarity.) It is seen that the log-normal distribution follows the data accurately where the gamma distribution deviates from the measurement for the small ($d < 30 \mathrm {\mu }{\rm m}$) and large droplet sizes ($d > 180\ \mathrm {\mu }{\rm m}$). It is interesting to see that the atomized droplet sizes from both single and dual nozzles follow the log-normal distribution, indicating that the same mechanism holds irrespective of their different flow conditions. The universality of the log-normal distribution is consistent with the argument of the present study; that is, the Rayleigh–Taylor instability dictates the differentiation of the droplets in the present configuration (see figure 18 below).

Figure 12.

The probability distribution function of the droplet size depending on $We_{eff2} = 45$ ($\circ$), $72$ ($\times$), $114$ ($\vartriangle$), and $210$ ($+$), when $m_{12} = 0$. The symbol $\lozenge$ corresponds to the dual-nozzle case ($We_{eff1} = 210$, $We_{eff2} = 210$ and $m_{12} = 0.27$). For all cases, $\theta _{2} = 40^{\circ }$. Inset shows the p.d.f. for single ($+$) and dual ($\lozenge$) nozzle in log-log scale, and the solid and dashed lines denote the fitted log-normal curve for single and dual nozzles, respectively, while the dotted line denotes the gamma distribution.

3.4. Classification of the atomization process

Based on the jet flow structure, atomization pattern and resulting droplet size, it was possible to establish the atomization regime map with major parameters identified together (figure 13). As shown, we classified four regimes – backflow, floating liquid column, bulk atomization and droplet atomization (the representative snapshots visualizing the corresponding atomization process are shown as insets) – in terms of the momentum flux ratio between two gas jets ($m_{12}$), the angle of the lower nozzle ($\sin {\theta _2}$), and the relative mass flux of the liquid to the lower jet ($m_{L2}$). By projecting the data onto the $x$–$z$, $s$–$z$, and $x$–$y$ planes, three two-dimensional regime maps can be extracted in figure 14, which will be used to elucidate the mechanism driving each regime. Here, the $s$-coordinate denotes the direction of $m_{12} = m_{L2}$. As said, the controlling parameters used for the classification correspond to each major operating condition of the dual-nozzle configuration. The governing parameters should be able to characterize the balance of three jets, which can be determined by two ratios of mass flux; we used the relative liquid flux ($m_{L2}$) and the mass flux ratio between gas jets ($m_{12}$), since they represent the liquid flux and the balance of the upper and lower gas jets, respectively. Also, the nozzle geometry variation is represented as $\sin \theta _2$. In § 4, these parameters are also deduced from the analytic solution by the control volume analysis.

Figure 13.

Atomization regime map according to the momentum flux ratio between two gas jets ($m_{12}$), the angle of the lower nozzle ($\theta _2$), and the mass flux ratio of the liquid jet ($m_{L2}$). Representative snapshots visualizing the instantaneous atomization process are shown together, being matched with each symbol in the regime map. Here, the coordinate $s$ is set to the line $m_{12} = m_{L2}$.

Figure 14.

Two-dimensional regime maps projected on (a) the $m_{12}$–$\sin \theta _2$ plane, (b) the $(m_{12} + m_{L2})$–$\sin \theta _2$ plane, and (c) the $m_{12}$–$m_{L2}$ plane, from the data in the three-dimensional map (figure 13). The dashed lines in (a,b,c) correspond to equations (4.7), (4.9) and (4.12), respectively.

We first define the backflow regime as the multiphase flow containing the reversal gas flow near the nozzle (e.g. at $y/D_{2} \lesssim 0.6$ in figures 5a and 6a), resulting in the upward-moving droplets differentiated partially from the falling liquid column (see the snapshots for inverted triangle in figure 13). With a further increase of the lower jet, backflow can fully lift and radially expand the falling liquid, which is specified as the floating liquid column regime (see the snapshots for triangle in figure 13). The occurrence of backflow is identified in the $m_{12}\unicode{x2013}\sin {\theta _2}$ plane (figure 14a). Since backflow occurs when the momentum of the upper jet is weaker than that of the lower jet (i.e. lower $m_{12}$), its critical value ($m_{12,crit}$) increases with $\theta _2$. As shown in figure 14(a), the backflow regime is separable by two parameters ($m_{12}, \sin {\theta _2}$), which is justified from the control volume analysis (see § 4.1). The droplet size in the backflow regime is slightly smaller than other regimes without a backflow (figure 10), which is attributed to the enhancement of the interfacial excitation deforming the water lump (figures 5a and 6a). While this backflow regime may be beneficial to obtain fine droplets, it involves issues such as nozzle bearding and clogging, as mentioned earlier.

When $m_{12}$ decreases (or $\sin {\theta _2}$ increases) further in the backflow regime, the floating liquid column regime appears (figure 14a), in which backflow becomes strong enough to support (or lift up) the falling liquid and make it stagnate near the nozzle (figure 9a). In order to support the liquid lump, not only do we need to have the strong contribution of the lower jet (i.e. small $m_{12}$ and large $\theta _2$), but the liquid jet ($m_{L2}$) needs to be weak comparatively. For example, in figure 14(a), six different cases of $m_{L2}$ are overlapped at the single point $(m_{12}, \sin {\theta _{2}}) = (0, 0.64)$. To clarify the condition of regime transition, we projected the data in figure 13 onto the $s$–$z$ plane to examine the dependency on the combined contribution of $m_{12}$ and $m_{L2}$ as $m_{12} + m_{L2}$ (figure 14b). As shown, it is possible to predict the boundary condition of the floating liquid column regime, for which the analytical argument will be given in § 4.2. In this regime, atomization is driven by two ways of shearing at the bottom of the stagnated liquid and the intermittent pouring of over-filled liquid.

As backflow is suppressed, we have two regimes of bulk atomization and droplet atomization, where we can eliminate the reversing droplets, achieving effectively the improved atomization assisted by the dual-jet operation. Morphologically, the bulk atomization regime is characterized by the undisturbed liquid column near the nozzle (the upward-moving droplets disappear) since backflow vanishes completely (see snapshots for square in figure 13). Finally, for the droplet atomization regime, the liquid column transforms completely to the falling cloud of droplets, therefore only the falling droplet is observed but not the column in the shadowgraph (see snapshots for circle in figure 13). In common, both regimes refer to the cases where the liquid passes through the lower-jet core, which can be in the state of lump or droplets. The state of falling liquid before interacting with the lower jet is dependent on the level of perturbation given by the upper jet, rather than by the lower jet. It is evidenced by the fact that the cases of the droplet and bulk atomization are overlapped at $m_{12} = 0.27$ and $\sin {\theta _{2}} = 0.34\unicode{x2013}0.64$ (figure 14a). As we need other parameters relevant to classifying the bulk and droplet atomization, in figure 14(c), we show that the linear curve with slope $m_{L1}=m_{L2}/m_{12}$, and the momentum flux ratio between the liquid and the upper jet, clearly distinguish them in the $m_{12}$–$m_{L2}$ plane. We will discuss this in § 4.4. While the atomization mechanism between the droplet and bulk atomization regimes differs, interestingly, there is a marginal difference in the resulting droplet sizes (figure 10). This can be explained by the argument on the relative velocity between the lower jet and liquid flow (see § 4.5).

The present classification is based on the existence of two essential flow features (i.e. the backflow and liquid core at the lower-jet exit) involved in the liquid atomization. Thus it can be said that all possible flow regimes with the dual nozzle were identified and categorized, as shown in figures 13 and 14. However, there is a condition for both droplet (4.12) and backflow atomization (4.7) regimes to hold simultaneously. In this case, the liquid core length is shorter than the nozzle distance ($h_2$), thus only droplets may pass through the centre of the lower nozzle. In addition, backflow dominates under the lower jet, thereby forcing some of the droplets to be entrained in the upward direction. Similarly, there is also an overlap between the floating liquid column (4.9) and droplet atomization (4.12) regimes. In this condition, the visualization shows clearly the dense cloud of particles passing through the lower nozzle, and some of the particles are moving upwards owing to the strong backflow (see figures 13 and 14). Meanwhile, the breakup pattern in the bulk and droplet atomization can be also specified using Hopfinger's diagram (Lasheras & Hopfinger Reference Lasheras and Hopfinger2000). For the $We_{eff}$ range in this study ($We_{eff1} = 2.2\unicode{x2013}13.8$ and $We_{eff2} = 11\unicode{x2013}468$, where subscripts $1$ and $2$ correspond to the upper and lower nozzles, respectively), the type of liquid disintegration falls mostly into the Rayleigh, shear and membrane breakup in the diagram. For the upper jet, the Weber number ($We_{eff1}$) spans the Rayleigh–Plateau instability and shear breakup with the liquid flow $Re_{l} = 7132$. In the present study, we observed the generation of a series of blobs caused by the redistribution of the interfacial energy (Rayleigh–Plateau instability) for the case $We_{eff1} = 4.82$ and $We_{eff2} = 0$ (see figure 20a). On the other hand, figures 20(b–e) show the active atomization by the gas momentum corresponding to the membrane breakup. For the lower jet, $We_{eff2}$ belongs to the membrane breakup. As shown in figures 8 and 17, the membrane breakup occurs actively during the sole operation of the lower jet, which agrees reasonably with the diagram.

It would be meaningful, on the other hand, to specify the limiting case for each controlling parameter. If $m_{12} = \infty$, then only the upper jet prevails, thus making a coaxial-like nozzle. On the other hand, when $m_{12} = 0$, only the lower jet operates, and the nozzle becomes a free-fall atomizer or the open-type atomizer (Fritsching & Uhlenwinkel Reference Fritsching and Uhlenwinkel2012). When it comes to $m_{L2}$, if the liquid jet is sufficiently strong ($m_{L2} = \infty$), then the gas flow no longer assists the atomization, and the pressurized atomization would prevail (Dumouchel Reference Dumouchel2008). In contrast, the case $m_{L2} = 0$ corresponds to the gas-phase jet that has no liquid atomization. For $\sin \theta _{2} = 0$, the flow becomes a coaxial jet that has a shear layer at a compassing annular gas jet. This kind of jet is also used for the sake of noise reduction and heat transfer (Sevilla, Gordillo & Martínez-Bazán Reference Sevilla, Gordillo and Martínez-Bazán2002), while the case $\sin \theta _{2} = 1.0$ corresponds to just one of the configurations of the dual nozzle. In sum, we think our experimental condition covers sufficiently the flow regimes achievable with the dual-nozzle atomization.

The unsteady (time-dependent) aspect of the liquid column dynamics is also dependent on the atomization regimes. We have quantified the (lateral) flapping frequency of the liquid column (for the detailed procedures, see the supplementary material) by applying the fast Fourier transform to the binarized instantaneous liquid column images. It is found that the flow regimes involving backflow are characterized by the lower frequency (${<}50$ Hz) since the wake-like behaviour of gas-phase flow decelerates the liquid oscillation. In contrast, if the upper jet overcomes backflow and the flow regime transitions to the bulk or droplet atomization regime, then the unsteadiness becomes stronger, with a higher flapping frequency (${\sim }100$ Hz) of the liquid column, driven by the coaxial-like behaviour of the gas phase. The trend of frequency also provides quantitative evidence for flow regime classification between the backflow and non-backflow regimes.

Here, we can summarize the role of the lower jet, for which the effect on the liquid atomization would vary depending on the operating and geometric conditions such as the nozzle angle ($\theta _2$), the gas exit velocity ($u_2$), and the momentum flux ratio to the liquid jet ($m_{L2}$). For lower $m_{12}$, the lower nozzle plays the main atomizer while the upper jet serves as the auxiliary one. In this case, the strength of the gas jet, responsible for the atomization performance, increases with the angle of the lower nozzle and the gas exit velocity (figure 16), affecting the global flow structure and triggering the appearance of the backflow (or floating liquid column) regime. The spread angle of the atomized droplets is also widened, as described in § 3.2. Also, the lower jet can be used as an auxiliary atomizing gas when the upper jet mainly disintegrates the liquid column (corresponding to the droplet atomization regime). Actually, this case corresponds to the conventional coaxial nozzle, and the lower jet modifies only the spray angle while the droplet size is retained (Aliseda et al. Reference Aliseda, Hopfinger, Lasheras, Kremer, Berchielli and Connolly2008; Ketterhagen et al. Reference Ketterhagen, Aliseda, Am Ende, Berchielli, Doshi, Freireich and Prpich2017). This corresponds to the case $m_{12}=\infty$ in the regime map (figures 13 and 14). However, it should be noted that the sole use of the upper jet puts a limitation on the upper bound of the gas jet velocity owing to the emergence of backflow and increase in the base pressure near the outlet of the liquid nozzle, incurring clogging (Fritsching & Uhlenwinkel Reference Fritsching and Uhlenwinkel2012; Shah et al. Reference Shah, Sandhu, Choi, Chokshi and Malick2014). This can be overcome in the dual-nozzle configuration by designating the lower (upper) nozzle as a main (auxiliary) atomizer. In this way, the lower nozzle, with the interplay with the upper one, can play the major or auxiliary atomizing gas jet, resulting in the different flow (atomization pattern) regime. This will provide the flexibility in the choice of operating condition of the gas atomizer to optimize the properties of atomized liquid droplets, not to mention the capability of avoiding backflow (or clogging) near the liquid outlet.

Considering the nature of the phenomena, we are tempted to suggest the practical aspects of our findings. In the backflow and floating liquid column regimes, reversing droplets are present, which can be harmful when atomizing the adherable (or temperature-sensitive) material. On the other hand, in the backflow regime, one may obtain smaller droplets as an output. Whether backflow is present or suppressed, the selection of the specific flow regime can be controlled by adjusting the flow and nozzle conditions. Depending on the flow regime, the spray characteristics such as the jet angle differ largely, as shown in figures 4 and 9. In addition, it is possible to obtain the desired size of droplets (depending on the application), which is a function of the acceleration experienced by the liquid column, by manipulating the operating conditions.

4.1. Backflow regime

As backflow occurs, in general, it is characterized by the following parameters: $\theta _2 = 20^{\circ }$, $m_{12} = 0$; $\theta _2 = 40^{\circ }$, $m_{12} \leqslant 0.067$; $\theta _2 = 60^{\circ }$, $m_{12} \leqslant 0.14$ (figures 7a–c). To understand further the meaning of this, we performed a control volume analysis (figure 15), based on the axisymmetric volume defined as $C_1$ in the figure. The top surface of $C_1$ includes the exit plane of the upper jet ($S_1$) and the liquid ($S_L$) nozzle, through which the fluid enters into $C_1$ with velocities (pressures) $u_1$ and $u_L$ ($p_1$ and $p_L$), respectively. The lower and side surfaces of $C_1$ match with the exit of the lower nozzle. When we apply momentum conservation along the vertical ($y$) direction for the time-averaged flow in the volume $C_1$, we have

(4.1)\begin{align} &\int_{S_1}p_{1}\,{\rm d}A+\int_{S_L}p_{L}\,{\rm d}A+\int_{S_3}p_{3G}\,{\rm d}A \nonumber\\ &\quad = \rho_{G}u_{1}^{2}A_{1}+\rho_{L}u_{L}^{2}A_{L}+\rho_{G}\int_{S_3}v_{3G}(v_{3G} \cdot\bar{n})\,{\rm d}A+\rho_{L}\int_{S_3}v_{3L}(v_{3L}\cdot\bar{n})\,{\rm d}A. \end{align}

Here, $A_1$ and $A_L$ denote the cross-sectional areas of the upper gas and liquid nozzles, respectively. It is assumed that the flow velocity ($v_{3i}$) and pressure ($p_{3i}$) – where subscript $i$ can be $L$ or $G$ for the liquid or gas phase, respectively – apply on the bottom surface ($S_3$) of $C_1$, and the vertical momentum flux through the side control surface, via the jet entrainment, is negligibly small compared with those through the top and bottom surfaces. In (4.1), the first two terms on the left-hand side can be ignored also, since the exit pressure of the slit jet is comparable with the ambient pressure (i.e. $p_{1}\sim p_{L} \sim p_{\infty }$) and decreases rapidly downstream owing to the production and redistribution of turbulence (Quinn Reference Quinn2005). In addition, the areas for pressures $p_1$ and $p_L$ also occupy a quite small fraction of the top control surface. Then the equation can be rearranged as

(4.2)\begin{equation} \rho_{G}\hat{v}_{3G}\,|\hat{v}_{3G}|\,\hat{A}_{3G} + \rho_{L}\hat{v}_{3L}\,|\hat{v}_{3L}|\,\hat{A}_{3L} = \int_{S_3}p_{3G}\,{\rm d}A - \rho_{G}u_{1}^{2}A_{1}-\rho_{L}u_{L}^{2}A_{L}. \end{equation}

Here, $\hat {A}_{3i}$ and $\hat {v}_{3i}$ denotes the effective area and flow velocity, respectively, satisfying $\int _{S_3}v_{3i}(v_{3i}\cdot \bar {n} )\,{\rm d}A= \hat {v}_{3i}\,|\hat {v}_{3i}|\,\hat {A}_{3i}$. Considering that the backflow is relevant to the negative $v_{3G}$, the condition $\hat {v}_{3G}=0$ should be satisfied when the backflow is about to appear, e.g. $\bar {u}_{y} \simeq 0$ near the nozzle ($y/D_{2} < 0.4$) for the case $m_{12} = 0.11$ and $\theta _2 =20^{\circ }$ (figure 7b). Together, the momentum of the falling liquid is balanced by the backflow, represented by the momentum flux through the bottom control surface: $\rho _{L}\hat {v}_{3L}\,|\hat {v}_{3L}|\,\hat {A}_{3L} \sim -\rho _{L}u_{L}^{2}A_{L}$. The effect of the gravity was neglected, since the flow-induced acceleration is far dominant, and (4.2) is reduced to

(4.3)\begin{equation} \rho_{G}\hat{v}_{3G}\,|\hat{v}_{3G}|\,\hat{A}_{3G} = \int_{S_3}p_{3G}\,{\rm d}A - \rho_{G}u_{1}^{2}A_{1}. \end{equation}

Equation (4.3) states reasonably that the backflow (i.e. sign of $\hat {v}_{3G}$) is determined by the pressure at the plane of the lower nozzle exit and the momentum of the upper jet. The pressure at the surface $S_3$ is contributed by (i) the pressure drop by the entrainment of surrounding air, and (ii) the pressure rise owing to the lower jet. For the entrainment effect, the pressure drop is formulated as $p_{ent} = -\alpha ^{2}[1-(u_{2}/u_{1})]^{2}\rho _{G}u_{2}^{2}/2$ (Browand & Latigo Reference Browand and Latigo1979; Rehab et al. Reference Rehab, Villermaux and Hopfinger1997; Villermaux Reference Villermaux1998). The constant $\alpha$ was determined empirically as $0.17$ for the mixing layer between fluids with different velocities (Brown & Roshko Reference Brown and Roshko1974; Hussain & Zedan Reference Hussain and Zedan1978). On the other hand, the pressure rise ($p_{dyn}$) is the inviscid phenomenon and thus proportional to the dynamic pressure of the horizontal momentum of the lower jet:

(4.4)\begin{equation} \int_{S_3}p_{dyn}\,{\rm d}A \simeq B\rho_{G}u_{2}^{2}\sin{\theta_2}\,A_{2}. \end{equation}

Here, $B$ is a proportional constant that is to be determined empirically. Assuming linear superposition of $p_{ent}$ and $p_{dyn}$, (4.3) can be expressed further as

(4.5)\begin{equation} \rho_{G}\hat{v}_{3G}\,|\hat{v}_{3G}|\,\hat{A}_{3G} = \left[ B\rho_{G}u_{2}^{2}\sin{\theta_2}\,A_{2} - \alpha^{2}[1-(u_{2}/u_{1})]^{2}\rho_{G}u_{2}^{2}A_{3}/2 \right] - \rho_{G}u_{1}^{2}A_{1}. \end{equation}

In the present conditions, we found that the pressure drop due to the jet entrainment is approximately $10$ times smaller than the pressure rise. Therefore, the critical condition for the occurrence of backflow ($\hat {v}_{3G}=0$) is obtained as

(4.6)\begin{equation} \rho_{G}\hat{v}_{3G}\,|\hat{v}_{3G}|\,\hat{A}_{3G} = B\rho_{G}u_{2}^{2}\sin{\theta_2}\,A_{2} - \rho_{G}u_{1}^{2}A_{1} = 0. \end{equation}

Dividing both sides of (4.6) by $\rho _{G}u_{2}^{2}\sin {\theta _2}\,A_{2}$, it can be rewritten in dimensionless form as

(4.7)\begin{equation} \frac{u_{1}^{2}A_{1}}{\rho_{G}u_{2}^{2}\sin{\theta_2}\,A_{2}} = \frac{m_{12}}{\sin{\theta_2}} = B. \end{equation}

Figure 15.

Schematic for the control volume analysis to analyse the backflow ($C_1$, dotted red line) and the velocity gradient ($C_2$, solid blue line). Note that the control volume is assumed to be axisymmetric against the vertical centreline.

Clearly, (4.7) supports our understanding given so far, based on the velocity measurement and atomization visualization, that the backflow is determined by the angle ($\theta _2$) of the lower nozzle and the momentum flux ratio ($m_{12}$) between the gas jets. To check the validity of the obtained relation, the cases of the backflow regime, satisfying $\bar {u}_{y} < 0$ at $x/D_{2} = 0$ and $y/D_{2} = 0.15\unicode{x2013}0.2$ (i.e. based on the gas-phase information only), are arranged in terms of $u_{1}^{2}A_{1}$ and $u_{2}^{2}\sin {\theta _2}\,A_{2}$ in figure 16(a). As shown, (4.7) (where the proportionality constant is determined to be $B = 0.1$) sets the boundary between the cases with and without backflow successfully. The same relation also holds for the classification based on the multiphase flow (i.e. judged by the atomization visualization); see the dashed line in figure 14(a), but with constant $B = 0.3$. The slight deviation of constant $B$ seems to originate from the difference in the measured variables; for multiphase flow, the backflow regime was identified by the reversal movement of droplets only, thus it is possible to miss the case of a backflow that is evident but not strong enough to push the droplets upwards (e.g. the case $m_{12}=0$, $\sin {\theta _{2}}=0.34$ and $m_{L2}=0.027$ in figures 13 and 14a). This is supported by the steeper slope of the boundary in multiphase cases compared to single-phase cases. Nonetheless, it is clear that the present analytical form in terms of $m_{12}$ and $\sin {\theta _2}$ determines the occurrence of the backflow regime.

Figure 16.

(a) Condition for the backflow regime in terms of momentum flux of the upper jet ($u_{1}^{2}A_{1}$) and the horizontal momentum flux of the lower jet ($u_{2}^{2}\sin {\theta _2}\,A_{2}$). The dashed line corresponds to (4.7) with $B = 0.1$. (b) Comparison of velocity gradient (${\rm d}\bar {u}_{y}^{*}/{{\rm d} y}^{*}$) with the analytical estimation ($\Delta \hat {v}^{*}$).

Extending the control volume analysis, we estimate the maximum velocity gradient (${\rm d}\bar {u}_{y}/{{\rm d} y}$) along the centreline (in the absence of the liquid column), which we raised as an important variable for atomization performance. Now, we consider the control volume $C_2$, illustrated in figure 15, which shares the top control surface with $C_1$ but is extended downwards by the distance $h=D_{2}/2$, representing the vertical position where the maximum ${\rm d}\bar {u}_{y}/{{\rm d} y}$ takes place (see figures 7a–c). Then the velocity gradient can be approximated as ${\rm d}\bar {u}_{y}/{{\rm d} y} \simeq (\hat {v}_{4G}-\hat {v}_{3G})/h$, where $\hat {v}_{4G}$ is the effective jet velocity passing through the bottom control surface ($S_4$) of $C_2$. Therefore, the velocity gradient can be expressed as

(4.8)\begin{equation} \frac{{\rm d}\bar{u}_{y}}{{\rm d} y} \sim \frac{\hat{v}_{4G}-\hat{v}_{3G}}{D_{2}/2}. \end{equation}

This relation can be modified in a dimensionless form as ${\rm d}\bar {u}_{y}^{*}/{{\rm d} y}^{*} = {\rm d}(\bar {u}_{y}/u_{2})/{\rm d}(y/D_{2}) = 2(\hat {v}_{4G}-\hat {v}_{3G})/u_{2} \equiv \Delta \hat {v}^{*}$. Considering the gas phase only ($\hat {v}_{3L}=0$ and $u_{L}=0$) in (4.2), the downward velocity ($\hat {v}_{4G}$) can be estimated as $\hat {v}_{4G}^{2} A_{4} = u_{2}^{2}\cos {\theta _2} + u_{1}^{2} A_{1}$ ($\hat {v}_{4G}$ is always positive). Here, the effective area ($\hat {A}_{4G}$) of the downward gas jet at the bottom surface of $C_2$ can be calculated as $\hat {A}_{4G} = {\rm \pi}\hat {D}_{4G}^{2}/4$, where $\hat {D}_{4G}$ denotes the effective jet width. From the experimental observation in figures 5 and 6, $\hat {D}_{4G}$ can be obtained as $\hat {D}_{4G}=k_{1}D_{2}/\sin {\theta _2}$, meaning that $\hat {D}_{4G}$ decreases with the increase of $\theta _2$ (here, $k_1$ is the empirical coefficient). Meanwhile, the effective jet width ($\hat {D}_{3G}$) through the control surface $S_3$ is independent on $\theta _2$ and should be smaller than $D_2$. Thus we introduce an empirical relation $\hat {D}_{3G}=k_{2} D_{2}$ with a constant $k_2$. Now, we can estimate $\hat {v}_{3G}$ from (4.6) with the coefficients $k_{1}\ (=0.2)$ and $k_{2}\ (=0.25)$, and the maximum velocity gradient can be calculated from (4.8) using the experimental data given in figure 4.7. In figure 16(b), we plotted the estimated dimensionless velocity gradient (${\rm d}\bar {u}_{y}^{*}/{{\rm d} y}^{*} = \Delta \hat {v}^{*}$) with the measured data, which shows good agreement between them in spite of the wide range of the jet angle ($\theta _{2}=20^{\circ }\unicode{x2013}60^{\circ }$). While the present control volume analysis is quite meaningful and reliable to predict the governing parameter related to the liquid atomization, it is slightly overestimated by (4.8). This is attributed to the deflection of the lower jet depending on the momentum ratio ($m_{12}$), shown in figures 5(b,e), changing the effective jet angle with which the jet collides. This will affect the calculation of dynamic pressure. In the present study, no further assumption is to be made because we think that the results from our analysis are still clear and useful practically. The estimation of $\hat {v}_{3G}$ and $\hat {v}_{4G}$ will be used further to predict the length scale of liquid atomization (see § 4.3). In the above control volume analysis, we did not consider the effect of the presence of the liquids (interfacial dynamics or instability) on the gas flow velocity; however, the consequent prediction of the flow regime matched the experimental measurements. To quantify such influences from the liquids, on the other hand, we have estimated the interfacial friction at the interface of the liquid column (see the supplementary material), and found that the gas velocity ($\hat {v}_{3G}$) at the bottom surface of control volume $C_1$ would vary within $2\,\%$ owing to the liquid column, supporting that our approach is reasonable.

4.2. Floating liquid column regime

When the liquid flow rate is quite low, the liquid column tends to stagnate owing to the lower-jet-induced backflow. The stagnant liquid column loses downward momentum and spreads along the horizontal direction (figure 9a); this can be understood simply as the vertical momentum of liquid and upper gas jet completely cancels out at the bottom of the control volume $C_1$ in figure 15, i.e. $\hat {v}_{3G} = \hat {v}_{3L}=0$ in (4.2). From (4.2) and (4.4), we have $B'\rho _{G}u_{2}^{2}A_{2}\sin {\theta _{2}} = \rho _{L}u_{L}^{2}A_{L} + \rho _{G}u_{1}^{2}A_{1}$; that is, the left-hand side of the equation denotes the contribution from the dynamic pressure of the horizontal momentum of the lower jet, and the two terms on the right-hand side are the vertical momentum fluxes of the liquid and the upper gas jet. By dividing both sides by the momentum flux of the lower jet ($\rho _{G}u_{2}^{2}A_{2}$), this becomes $B'\sin {\theta _2} = (\rho _{L}u_{L}^{2}A_{L} + \rho _{G}u_{1}^{2}A_{1})/(\rho _{G}u_{2}^{2}A_{2})$. Therefore, using the definition of mass flux ratio, it is possible to define the critical condition for the floating liquid column regime as

(4.9)\begin{equation} \frac{m_{L2}+m_{12}}{\sin{\theta_2}} = B'. \end{equation}

The model shows that the greater the relative strength ($u_2$) and angle ($\theta _2$) of the lower jet, the greater the possibility of the occurrence of the floating liquid column regime. And, as expected, the floating liquid column regime disappears when the flux of the liquid column ($u_L$) increases (see figure 9d). As we have shown already in figure 14(b), (4.9) distinguishes the floating liquid column regime with others well, and it has slope $\sin {\theta _{2}}/(m_{L2}+m_{12}) = 1.14$ (or $B' = 0.88$).

4.3. Bulk atomization regime

In the bulk atomization regime, the liquid column is accelerated rapidly and atomized by the lower jet, as shown in figure 8. The accelerated water column develops into the multiple-cell-shaped membrane, which is reminiscent of the Rayleigh–Taylor instability. During the acceleration ($a$) of the interface, the perturbation wave is generated on the interface between two fluids of different densities ($\rho _L$ and $\rho _G$) with wavenumber $k$ and angular frequency $\omega$. It is known that in only a specific range of $k$, $\omega$ is amplified (while in other ranges it is dissipated), according to the dispersion relation (Rayleigh Reference Rayleigh1883) for the case $k > 0$ (Charru Reference Charru2011):

(4.10)\begin{equation} (\rho_{L}+\rho_{G})\omega^{2}- k[(\rho_{L}-\rho_{G})a-k^{2}\sigma]=0. \end{equation}

Here, $\sigma$ is the surface tension. From this relation, the wavelength $\lambda _{max}$ with the maximum temporal growth rate $\omega _{i,max}$ (the imaginary part of $\omega$) satisfying the solution of (4.10) can be calculated as $\lambda _{max}=2{\rm \pi} (3\sigma /\rho _{L}a)^{0.5}$, which is most likely to appear in the real flow (Varga et al. Reference Varga, Lasheras and Hopfinger2003; Kourmatzis & Masri Reference Kourmatzis and Masri2015). To calculate this length scale, the acceleration on the interface should be measured first, which is determined by the flow structure formed by the upper and lower jets. Thus we estimate the acceleration normal to the liquid interface using the concept of hydrodynamic force (Kourmatzis & Masri Reference Kourmatzis and Masri2015; Sharma et al. Reference Sharma, Singh, Rao, Kumar and Basu2021). When the liquid droplet (or ligament) is located in the gas stream, the acceleration of the liquid interface can be estimated as $a = F_{d}/m_{d}$, where $F_d$ and $m_d$ denote the drag force and mass of liquid, respectively. The drag force is expressed as $F_{d} = C_{d} \rho _{g} (\Delta u)^{2} A_{d}/2$, where $A_d$ and $\Delta u$ are the cross-sectional area of the most-flattened droplet (or liquid column) and the relative velocity between phases, respectively, and $C_d$ is the drag coefficient ($C_d=1.2$ in Zhao et al. Reference Zhao, Wu, Li, Xu and Liu2018). The liquid mass is expressed as $m_{d} = \rho _{l} V_{d}$, where $V_d$ is the liquid volume, detached from the bulk. Combining these, the acceleration is obtained as $a = C_{d} \rho _{g} (\Delta u)^{2} A_{d}/(2\rho _{l} V_{d})$. The relative velocity ($\Delta u$) is defined as $\Delta u = u_{g,a}-u_{i,a}$, where $u_{g,a}$ and $u_{i,a}$ are the gas velocity and the convection velocity of the liquid surface wave at the atomization site, respectively (figure 8) (Varga et al. Reference Varga, Lasheras and Hopfinger2003; Kourmatzis & Masri Reference Kourmatzis and Masri2015; Sharma et al. Reference Sharma, Singh, Rao, Kumar and Basu2021). The $u_i$ can be estimated by the Dimotakis velocity; since the atomization occurs at the centreline of the nozzle, the liquid mass is accelerated mostly by the vertical gas stream. At this site ($-0.1 < x/D_{2} < 0.1$), the liquid and gas flow are parallel locally and the stress balance results in the Dimotakis velocity, which is defined as $u_{i} = (\sqrt {\rho _{g}}\,u_{g,a} + \sqrt {\rho _{l}}\,u_{l,a})/(\sqrt {\rho _{g}} + \sqrt {\rho _{l}})$ (Dimotakis Reference Dimotakis1986). Here, $u_{g,a}$ can be assumed to be comparable to the resultant jet ($\hat {v}_{4G}$) velocity at $y = D_{2}/2$, i.e. $u_{g,a} \simeq \hat {v}_{4G}$ by (4.8). The Dimotakis velocity $u_{i,a}$ may be determined by the upper gas jet and the liquid jet, expressed as $u_{i,a} = (\sqrt {\rho _{g}}\,u_{g,1} + \sqrt {\rho _{l}}\,u_{l,1})/(\sqrt {\rho _{g}} + \sqrt {\rho _{l}})$. Here, the characteristic velocities for the gas ($u_{g,1}$) and liquid ($u_{l,1}$) phases are selected as the resultant gas velocity ($\hat {v}_{3G}$) at the centre of the lower nozzle ($y/D_{2} = 0$) and the liquid exit velocity ($u_L$). The area ($A_d$) and volume ($V_d$) of the liquid segment are assumed to be identical to the equivalent sphere with diameter $D_L$. For the conventional coaxial liquid–gas flow, $V_d$ is determined by the length scale of the Kelvin–Helmholtz instability. However, the Kelvin–Helmholtz instability pattern is suppressed for our range of $We_{eff}$, which will be discussed later. Thus the Rayleigh–Taylor instability pattern may grow from the liquid bulk with size $D_L$, and the acceleration of the liquid interface is scaled as $a \sim 3C_{d} \rho _{g} (\Delta u)^{2}/(4\rho _{l} D_{L})$, where $\Delta u = \hat {v}_{4G}-(\sqrt {\rho _{g}}\, \hat {v}_{3G} + \sqrt {\rho _{l}}\,u_{L})/(\sqrt {\rho _{g}} + \sqrt {\rho _{l}})$. Insertion of this relation into the solution of (4.10) results in the wavelength ($\lambda _{max}$) with the maximum growth rate:

(4.11)\begin{equation} \lambda_{max}(=\lambda_{RT,est}) \sim 4{\rm \pi} \sqrt{\frac{\sigma D_{L}}{C_{d} \rho_{g} (\Delta u)^{2}}}. \end{equation}

In the present condition, the falling speed of the liquid column ($u_L$) is measured to be $2.91\ {\rm m}\ {\rm s}^{-1}$ at the centre of the upper gas nozzle, $\bar {u}_y$ is assumed to be equal to $\hat {v}_{3G}$, and the spatial gradient ($\partial \bar {u}_y/\partial y$) is obtained from (4.8). Equation (4.11) shows that the length scale of the instability decreases in inverse proportion to the velocity and angle of the lower jet. To confirm this, the characteristic length of the low-$We_2$ cases ($We_{eff2} = 11\unicode{x2013}252$) was quantified, in which the cell-like liquid membrane structure was visible with the current spatial and temporal resolution of the high-speed camera. The irregular shape of the Rayleigh–Taylor cell is approximated as circles having an equivalent area using the in-house software (figure 17) (Joseph et al. Reference Joseph, Belanger and Beavers1999; Varga et al. Reference Varga, Lasheras and Hopfinger2003). For each case, 14 cells were quantified; their size range was 2.04–5.54 mm, with standard deviation less than $19.5\,\%$ for all cases.

Figure 17.

(a–c) Instantaneous atomization images showing the disintegration process of the liquid column by the gas jet. Rectangular boxes indicate the measurement area in which the Rayleigh–Taylor instability occurs. (d–f) Results of pattern identification (thick circles) corresponding to the Rayleigh–Taylor length scale: (a,d) $\theta _{2} = 20^{\circ }$; (b,e) $\theta _{2} = 40^{\circ }$; (c, f) $\theta _{2} = 60^{\circ }$. Here, $m_{L2} = 0.051$, $We_{eff2} = 28\unicode{x2013}252$ and $Re_{2} = 1.1 \times 10^{5}$.

In figure 18(a), we have plotted the results of measurements by comparing with the estimation of (4.11). The horizontal bars on each symbol denote the range of uncertainty (maximum $2.75\,\%$) in estimating $\hat {v}_{3G}$ caused by the existence of the liquid column (see the supplementary material). It is found that the first-order proportionality (indicated by the dashed line in figure 18a) is salient between (4.11) and the Rayleigh–Taylor cells observed experimentally (indicated by arrows in figure 18b), considering the relatively wide range $\theta _{2}=20^{\circ }\unicode{x2013}60^{\circ }$ and various jet conditions ($m_{12} = 0\unicode{x2013}0.27$, $Re_{2} = 0.69\unicode{x2013}1.1 \times 10^{5}$ and $m_{L2} = 0.051\unicode{x2013}0.13$). Therefore, it can be said that the breakage mechanism of the liquid column is governed by the Rayleigh–Taylor instability, similar to previous studies (Marmottant & Villermaux Reference Marmottant and Villermaux2004; Aliseda et al. Reference Aliseda, Hopfinger, Lasheras, Kremer, Berchielli and Connolly2008; Kourmatzis & Masri Reference Kourmatzis and Masri2015). The difference in the absolute magnitude is attributed to the uncertainty in estimating the acceleration ($a$) and the size of liquid segment ($V_d$). From figure 18, it can be compensated with the correlation equation $\lambda _{RT,est} = Q_{1}4{\rm \pi} \sqrt {\sigma D_{L}/(C_{d} \rho _{g} (\Delta u)^{2})}+Q_{2}$, where $Q_{1}=1.32$ and $Q_{2}=0.57$. Now, using this relation with (4.8) and (4.11), the Rayleigh–Taylor length scale can be calculated for all cases of visualization displayed in figures 17 and 18(b). These estimations might be helpful to reveal the mechanism of the atomization for each regime. During the breakup process, the observation of the wavelength due to the Rayleigh–Taylor instability is a challenging task because multiple instabilities (including Kelvin–Helmholtz and Rayleigh–Plateau instabilities) may occur simultaneously. Researchers have analysed the unclear-looking (but consistent) pattern as reminiscent of Rayleigh–Taylor instability during the gas-assisted breakup of a single droplet, the coaxial jet, and the annular jet (Joseph et al. Reference Joseph, Belanger and Beavers1999; Varga et al. Reference Varga, Lasheras and Hopfinger2003; Dhivyaraja, Jegan & Vadivukkarasan Reference Dhivyaraja, Jegan and Vadivukkarasan2021). These images (or evidence), used to extract the relevant wavelength, have in common a small number (less than 10) of geometric features for the instability. Thus it is hard to be quantified statistically, and it is anticipated that inevitably, a certain level of uncertainty is involved. On the other hand, Varga et al. (Reference Varga, Lasheras and Hopfinger2003) have shown that the maximal growth rate of the Rayleigh–Taylor instability ($\omega _{max,RT}$) is four times greater than that of the Kelvin–Helmholtz instability ($\omega _{max,KH}$, which is also the prepotent candidate of the breakup mechanism) at the slip velocity $u_{g} - u_{l} > 20\ {\rm m}\ {\rm s}^{-1}$. For the present cases, the slip velocity is roughly faster than $10\ {\rm m}\ {\rm s}^{-1}$, and the instability theory predicts that $\omega _{max,RT}>3.71\omega _{max,KH}$ (please refer to figure 30 in Varga et al. Reference Varga, Lasheras and Hopfinger2003). We think that this also supports that the interfacial acceleration plays an important role in the liquid breakup (i.e. Rayleigh–Taylor instability).

Figure 18.

(a) Comparison between theoretical estimation on the length scale of the Rayleigh–Taylor instability ($\lambda _{RT,est}$) and the length scale measured experimentally ($\lambda _{RT,exp}$). Here, $m_{12} = 0\unicode{x2013}0.27$, $Re_{2} = 0.69\unicode{x2013}1.1 \times 10^{5}$ and $m_{L2} = 0.051\unicode{x2013}0.13$. (b) Representative atomization visualizations showing the Rayleigh–Taylor cells (indicated by arrows) corresponding to each case (symbols from (a) are noted at bottom right in each image).

In addition to the Rayleigh–Taylor instability, the Kelvin–Helmholtz instability has also been raised as a driving mechanism of liquid atomization (Gordillo et al. Reference Gordillo, Pérez-Saborid and Gañán-Calvo2001). To compare their roles in the present problem, we have calculated the dependency of the size of atomized droplets on the characteristic length scales across the flow regimes (figure 19). It is noted that the case $\theta _{2} = 20^{\circ }$ and $m_{L2} = 0.027$ (closed circles in figure 10) was not included in the calculation, since the liquid column was not fully atomized into droplets with its interfacial instability. The Kelvin–Helmholtz instability in the present study might be affected by various factors, such as the boundary layer thickness, momentum deficit near the interface, and absolute instability (see § 1); however, its strong dependence on the gas boundary layer thickness at the liquid–gas interface should be more influential. Hence the length scale related to the Kelvin–Helmholtz instability ($\lambda _{KH}$) is proportional to $(\rho _{L}/\rho _{G})^{0.5} \delta _G$, where $\delta _G$ is the thickness of the vorticity layer, scaled with the Reynolds number of each gas jet as $\delta _{G,(i)} \sim Re_{i}^{-0.5}$ (Lasheras & Hopfinger Reference Lasheras and Hopfinger2000; Varga et al. Reference Varga, Lasheras and Hopfinger2003; Marmottant & Villermaux Reference Marmottant and Villermaux2004). Here, $i = 1$ (upper jet) or $i = 2$ (lower jet). Thus $\lambda _{KH}$ can be estimated as $\lambda _{KH(i),est} \simeq (\rho _{L}/\rho _{G})^{0.5}Re_{i}^{-0.5}$. Figure 19(a) shows that the ratios related to $\lambda _{KH(1),est}$ and $\lambda _{KH(2),est}$ vary according to the flow regime (furthermore, the scattered range of the data is quite large even in the same regime), indicating that the size of an atomized droplet is not determined by the strength of each jet (i.e. $Re_i$) only (other geometrical and flow parameters should be considered together, as we have shown so far), or Kelvin–Helmholtz instability may not be the universal atomization mechanism in the present problem. Interestingly, the ratio becomes larger as the flow regime transitions from floating liquid column to droplet atomization, and the reduction of velocity gradient (${\rm d}\bar {u}_y/{{\rm d} y}$) across this transition (figures 6a,d) is not addressed adequately by the Kelvin–Helmholtz instability. It is noted that the droplet size was insensitive to the jet strength ratio (figure 10a). On the other hand, the ratio against the lower nozzle ($d_{32}/\lambda _{KH(2),est}$) is relatively larger, because the lower jet is stronger than the upper one in the present set-up (table 1). Thus a characteristic length scale other than $\lambda _{KH}$ is needed to correlate the droplet size and underlying mechanism of the atomization process.

Figure 19.

Ratio of the Sauter mean diameter ($d_{32}$) to (a) $\lambda _{KH,est}$ and (b) $\lambda _{RT,est}$, depending on the flow regime.

Figure 20.

Instantaneous atomization images showing the pre-atomized water column depending on the flux of upper jet ($u_{2} = 0$): (a) $M_{L1} = 0.2$; (b) $0.12$; (c) $0.095$; (d) $0.078$; (e) $0.067$. Here, $We_{eff1} = 4.6\unicode{x2013}13.6$ and $Re_{1} = 4.9\unicode{x2013}8.5 \times 10^{4}$.

Previous studies have also shown that the Rayleigh–Taylor instability is related to the final droplet size. Varga et al. (Reference Varga, Lasheras and Hopfinger2003) reported that $d_{32}/\lambda _{RT} \simeq 0.2$ with a wide range of slip velocity ($u_{g}-u_{l} = 69\unicode{x2013}165\ {\rm m}\ {\rm s}^{-1}$, where $u_g$ and $u_l$ denote the gas and liquid velocities, respectively). On the other hand, $d_{32}/\lambda _{KH}$ had a dependency on the gas jet velocity as it is scaled with $u_{g}^{-3/4}$. Kourmatzis & Masri (Reference Kourmatzis and Masri2015) mentioned that both ratios are affected similarly by the slip velocity as $d_{32}/\lambda _{KH} \simeq 0.29$ and $d_{32}/\lambda _{RT} \simeq 0.20$, if the turbulence intensity is less than $0.25$. Unlike the present study, Singh et al. (Reference Singh, Kourmatzis, Gutteridge and Masri2020) showed a strong dependency on $\lambda _{KH}$ ($d_{32}/\lambda _{KH} \simeq 0.2\unicode{x2013}0.4$), while $d_{32}/\lambda _{RT}$ varies significantly with the gas jet velocity. In their set-up, the gas jet immediately strikes the liquid flow coming out from the nozzle, forming a shear layer at the interface where the liquid jet is broken, thus it is related to the length scale ${\sim }(\rho _{L}/\rho _{G})^{0.5}Re^{-0.5}$, following the Kelvin–Helmholtz instability. However, in the present configuration, the liquid column is atomized far away from the gas nozzles. Thus the droplet size is dictated by the resultant flow acceleration (as shown in figure 8) set through the balance of two gas jets at the site of atomization ($x/D_{2} \simeq 0$ and $y/D_{2} = 0.2\unicode{x2013}1.0$), rather than by the shearing mechanism near the two gas nozzles. Therefore, the length scale relevant to the Rayleigh–Taylor instability is more adequate for the present problem, as derived in (4.11). In figure 19(b), the ratio of measured Sauter mean diameter ($d_{32}$) to the estimated Rayleigh–Taylor length scale (4.11) is plotted with the four regimes. The ratio is almost constant at approximately $0.12$ for all atomization regimes. In addition, compared to the ratios against $\lambda _{KH}$, the range of scattered data is quite narrow, indicating that the Rayleigh–Taylor instability owing to the rapid acceleration of the liquid column is more plausible in explaining the sizes of droplets generated in all regimes and operating conditions. According to previous studies of a single-nozzle configuration (Varga et al. Reference Varga, Lasheras and Hopfinger2003; Kourmatzis & Masri Reference Kourmatzis and Masri2015), $d_{32}/\lambda _{RT}$ is also found to be constant, around 0.2–0.3, which is slightly higher than the present value. The discrepancy might be related to the different measurement location (e.g. $x/D_{1} = 30$ in our study, $x/D_{1} = 5\unicode{x2013}60$ in Varga et al. Reference Varga, Lasheras and Hopfinger2003) of the droplet, and the selection of measurement method (e.g. PDPA and shadowgraph), including its intrinsic characteristics of bias (Singh et al. Reference Singh, Kourmatzis, Gutteridge and Masri2020). Nevertheless, the present result is consistent with previous studies within its order of magnitude ($O(10^{-1})$), and it shows clearly the dominance of the characteristic length scale ($\lambda _{RT}$) in all atomization regimes. Meanwhile, although the atomization process in the floating liquid column regime is quite different from that in other regimes ( figures 9a,b), interestingly, the droplet size is dependent on $\lambda _{RT}$ as in other regimes. It is suspected that the second atomization (by pouring) in figure 9(b) would be responsible for this, as suggested by Kourmatzis & Masri (Reference Kourmatzis and Masri2015); however, it is not feasible currently to measure it due to its highly irregular behaviour. It is noted that the ratio $d_{32}/\lambda _{RT,est}$ in the droplet regime is slightly greater than in others. It is speculated that another length scale (together with $\lambda _{RT}$), or mechanism, may intervene in the droplet atomization regime. Since the liquid column is fully disintegrated into multiple droplets before being affected by the lower jet, the size of this pre-atomized droplet will influence greatly the atomization by the lower jet.

On the other hand, the transition from Rayleigh–Taylor to Kelvin–Helmholtz instability has been reported in the literature (Theofanous Reference Theofanous2011; Theofanous et al. Reference Theofanous, Mitkin, Ng, Chang, Deng and Sushchikh2012; Sharma et al. Reference Sharma, Singh, Rao, Kumar and Basu2021); in general, it occurs in the Weber number range $10^{2} < We_{d} < 10^{3}$, where $d$ is the droplet diameter (at $Oh < 0.1$). At this transition regime, the ratio between the droplet size and the instability length scale, i.e. $d/\lambda _{KH}$, is known to determine the transition, and its critical value is around $10$ (Sharma et al. Reference Sharma, Singh, Rao, Kumar and Basu2021). For the droplet atomization regime in the present study, $We_{d} < 119$ and $4.4 < d/\lambda _{KH} < 7.7$, implying that such a transition would be inhibited and the Rayleigh–Taylor instability dominates (a detailed explanation is given in the supplementary material).

4.4. Droplet atomization regime

Let us discuss the conditions of the droplet atomization regime. We define the vertical range where the liquid column is fully atomized from the exit of the liquid nozzle as the liquid core length $l_c$, which has been considered to be an indicator of atomization performance (Lasheras & Hopfinger Reference Lasheras and Hopfinger2000; Dumouchel Reference Dumouchel2008). If we consider a volume of liquid cone that is splitting droplets continuously at velocity $u_s$ in its surface, then the application of mass conservation for the process is expressed as $u_{L}({\rm \pi} D_{L}^{2}/4)= u_{s}({\rm \pi} D_{L}l_{c}/2)$, where $D_L$ is the exit diameter of the liquid jet. Thus the liquid core length is expressed as $l_{c} = (0.5u_{L}D_{L})/u_{s}$. For the velocity $u_s$, we follow the model introduced by Lasheras & Hopfinger (Reference Lasheras and Hopfinger2000). A fraction of the dynamic pressure of the gas jet is balanced by the dynamic pressure of the perturbed liquid and the interfacial force, which is expressed as $\rho _{L} u_{s}^{2}+b\sigma /\delta = c\rho _{G}u'_{G}$. Here, $\delta$ is the thickness of the gas jet shear layer, and $u'_G$ is the r.m.s. gas velocity fluctuation at the centre of the shear layer, expressed as $u'_{G} = c_{r}(u_{G}-u_{L})$. Here, $c_r$ needs to be determined empirically, and we use the value $0.07$ adopted from Rehab et al. (Reference Rehab, Villermaux and Hopfinger1997), in which the velocity fluctuation along the centreline of the nozzle was measured. For the gas velocity, we use the exit velocity ($u_1$) of the upper jet, which is a reasonable choice for the droplet atomization regime. The thickness of the jet shear layer around the liquid column can be assumed to be the annular radius of the upper nozzle, $\delta = D_{1}/2$. The contribution factors of $b$ and $c$ are determined empirically as $10^{-3}$ and $0.25$, respectively (Rehab et al. Reference Rehab, Villermaux and Hopfinger1997). Finally, the initial diameter of the liquid column ($D_L$) is assumed to be the same as $D_1$, since the liquid cone shedding droplets spans quickly along the upper jet owing to the dominant momentum of the gas jet ($m_{L1} \ll 1.0$). Substituting these relations, we now have the equation for the liquid core length as

(4.12)\begin{equation} \frac{l_c}{D_1} \simeq \frac{14.3}{[1-2b(\rho_{G}/\rho_{L})We_{D_{1}/2}^{{-}1}]^{0.5}}\, M_{L1}^{0.5} \simeq 14.3M_{L1}^{0.5}. \end{equation}

Here, $M_{L1}$ denotes the dynamic pressure ratio between the liquid column and the upper gas jet ($M_{L1}= \rho _{L}u_{L}^{2}/(\rho _{G} u_{G}^{2}$)), and the Weber number is defined as $We_{D_{1}/2} = \sigma u_{1}^{2}(D_{1}/2)/\rho _G$, ranging from $178$ to $842$. Since the travelling directions of gas and liquid are almost parallel in this case, it is understood that the dynamic pressure ratio ($M_{L1}$) determines dominantly the liquid core length. With the modelling of $l_c$, we can set the condition of the droplet atomization regime such that it appears when $l_c$ is shorter than the distance between the liquid nozzle and the lower gas nozzle ($h_{2} = 4D_{L}$) as $l_{c} < 4D_{L}$. Since the effect of the surface tension can be neglected compared to the dynamic pressure of the gas jet, the critical condition in which the droplet atomization regime appears can be obtained as $M_{L1} < (4/14.3)^{2} = 0.078$. Thus increasing the velocity of the upper jet results in the transition from the bulk atomization to the droplet atomization regime. Figure 20 (see also supplementary movie 3) shows the liquid column perturbed by the upper jet depending on the dynamic pressure ratio $M_{L1}$, while the lower jet rests. As shown, the upper jet weakly perturbs the liquid column, and the liquid core is maintained below the lower nozzle for $M_{L1} > 0.078$ (figures 20a–c). On the contrary, the liquid core is already fully atomized and falls in the form of a spray below the lower nozzle when $M_{L1} < 0.078$ (figure 20e). Thus the criterion of the droplet atomization regime is determined by the dynamic pressure ratio $M_{L1}$. Recalling the regime map with respect to $m_{12}$ and $m_{L2}$ (figure 14c), the slope of $m_{L1}$ can be calculated from $M_{L1} = \rho _{L}u_{L}^{2}/(\rho _{G}u_{1}^{2})$ as $m_{L1,crit} = M_{L1,crit} \cdot A_{L}/A_{1} = 0.118$, where $A_L$ and $A_1$ denote the exit areas of the liquid and the upper gas nozzle, respectively. It can be seen that the linear curve with the predicted slope $m_{L1}$ distinguishes precisely the droplet atomization regime from others. In this case, the lower jet was idle to reveal the sole effect of the upper jet on the liquid jet. Thus the liquid core length might differ when the lower jet operates by creating a modified pressure gradient downstream. This may affect (4.12); however, we noted that it is not dependent on the lower gas jet in the present study. The droplet atomization regime remains when $m_{12}$ decreases from $0.27$ to $0.17$ (figure 14c), despite the strong introduction of the lower gas jet and the occurrence of backflow (see the corresponding image in figure 13). This is attributed to (i) the low $m_{L1}$ (or $M_{L1}$) that implies the strength of the upper gas jet is sufficient for fully destabilizing the liquid jet, and (ii) the ambivalence of the lower gas jet that hinders the fragmentation process near the liquid outlet ($y < 0$) and destabilizes above the liquid column. To elucidate this, the measurement of the interaction between the gas jets inside the nozzle ring is required. However, due to the optical limit of the velocity field between the upper and the lower nozzle, the effect of the lower jet on the upper jet ($y > 0$) is hard to measure. To count this modification roughly, the error on the averaged jet velocity at the lower jet exit ($\hat {v}_{3G}$, see figure 15) in (4.12) is estimated. When the lower jet operates, the change of the averaged jet velocity at the lower nozzle exit can be calculated using (4.6). For the droplet atomization regime in figure 13, $\hat {v}_{3G}$ is calculated and compared with the case $u_{2} = 0$. It is found that $\hat {v}_{3G}$ is decelerated approximately $15\,\%$ maximum. Thus the effective value of $M_{L1}$ can increase by as much as $38.4\,\%$ of the predicted values in this section.

4.5. Further discussion on the atomized droplet size

In this section, we briefly address our arguments on droplet size in the droplet atomization regime. As we have explained above, in this regime, the liquid column is atomized substantially by the upper jet, and the secondary atomization occurs by the lower jet. For the atomization by the upper jet, the initial liquid column flows nearly parallel to the upper jet and is atomized by the shearing force. For this situation, Lasheras & Hopfinger (Reference Lasheras and Hopfinger2000) proposed a model such that the droplet size ($d_p$) is proportional to $u_{GL}^{-4/5}$ (where $u_{GL}$ denotes the relative velocity of the droplet with respect to the surrounding gas flow, and $u_{GL} = u_{1}-u_{L} \simeq u_{1}$ since the gas jet velocity is much faster than the liquid) when the Weber number is $We = \rho d_{p} u_{GL}^{2}/\sigma \sim 10^{2}$, based on the balance between the strain rate and viscous diffusion. On the other hand, Villermaux (Reference Villermaux1998) scaled the droplet size in the form $d_{p} \sim u_{GL}^{-1}$ for a laminar exit condition and $d_{p} \sim u_{GL}^{-6/5}$ for a turbulent condition, using linear instability theory, assuming inviscid velocity profile (reasonably applicable to higher Weber number). Thus, in general, the final droplet size is scaled as $d_{p} \sim u_{GL}^{-1} \simeq u_{1}^{-1}$. When the fragmented droplets or ligaments by the upper jet reach the downstream area where the lower jet dominates, they are atomized further into multiple smaller droplets. Here, we can apply the droplet size model for the secondary atomization, which has been proposed as $d_{s}/d_{p} \sim Oh^{0.5}We_{d}^{-0.25}$ (Hsiang & Faeth Reference Hsiang and Faeth1992), where $d_s$ and $d_p$ are the diameters from the secondary and primary atomization droplets, respectively. The Ohnesorge and Weber numbers were defined as $Oh = \mu _{L}/(\rho _{g} d_{p} \sigma )^{0.5}$ and $We_{d} = \rho _{G} u_{r}^{2} d_{p}/\sigma$, respectively. Here, the relative velocity ($u_{r} \sim u_{2}-u_{1}$) between the droplet and the surrounding gas has been used. Now, the scaling relation with respect to the jet velocity on the final size of the droplets can be obtained by multiplying the two models as $d_{s} = (d_{s}/d_{p}) \cdot d_{p} \sim (u_{r}^{-0.5} d_{p}^{-0.25}) \cdot d_{p} \sim (u_{r}^{-0.5} u_{1}^{0.25}) \cdot u_{1}^{-1} \sim (u_{2}-u_{1})^{-0.5} \cdot u_{1}^{-0.75}$. Thus it is understood that the increase of the upper jet velocity $u_1$ results in two opposite contributions of $(u_{2}-u_{1})^{-0.5} \cdot u_{1}^{0.25}$ and $u_{1}^{-1}$ on the droplet diameter. As the upper jet increases, the droplet size from the primary atomization decreases as $u_{1}^{-1}$, but the droplet is accelerated rapidly by the lower jet, and its relative velocity is reduced substantially, thereby increasing the droplet size from the secondary atomization as $(u_{2}-u_{1})^{-0.5} \cdot u_{1}^{0.25}$. On the other hand, if the velocity of the upper jet decreases, then the droplet size due to the primary atomization becomes larger, but by the lower jet, the droplets are accelerated strongly, resulting in smaller droplets. This explains the experimental results shown in figure 10(a), which shows that the particle size is almost constant irrespective of the strength of the upper jet.