High-speed camera observation
A high-speed camera (Os7, IDT Vision, USA) equipped with two F-mount lenses (ATX 16–28 mm and 100 mm, Tokina, Japan) was used for the direct observation of the flow visualization process. A 100 W LED lamp (LED-100-T, Visico, China) was used to continuously illuminate the observed area, which enabled the acquisition of clear images with a short exposure time of the high-speed camera. The high-speed images were captured at different frame rates, including 2700, 4000, and 8000 fps. The analysis of the videos obtained was carried out using the Motion Studio software. All the high-speed videos were played at a frame rate of 30 fps using the images obtained at different frame rates.
Computational fluid dynamics (CFD) simulations
In this study, we examined the transition from a uniform laminar airflow to turbulence induced by a grid structure, a phenomenon pivotal in the breakup of droplets. To accurately replicate this transition, a series of comprehensive three-dimensional direct numerical simulations (DNSs) were conducted. These simulations employed an in-house CFD code, which integrates the finite difference method (FDM) and the immersed boundary method (IBM), as detailed in previous works51,52. The computational model and domain are illustrated in Supplementary Fig. 4, where D is the separation between wire centerlines, s denotes the distance from the inlet to the central plane of the grid structure, L is the streamwise domain length, and W and H specify the width and the height of the computational domain, respectively.
In the present study, the velocity range of interest for the airflow is considerably below the speed of sound. Consequently, the airflow dynamics are governed by incompressible and isothermal Naiver-Stokes equations as follows,
$$\:\begin{array}{c}\frac{\partial\:\varvec{u}}{\partial\:\text{t}}+\left(\varvec{u}\cdot\:\nabla\:\right)u=-\frac{1}{{\rho\:}_{f}}\nabla\:p+\nu\:{\nabla\:}^{2}u+f \left(1\right)\end{array}$$
$$\:\begin{array}{c}\nabla\:\cdot\:u=0\:. \left(2\right)\end{array}$$
Here, \(\:\varvec{u}\) is the velocity of airflow, \(\:{\rho\:}_{f}\) represents the density of air, p is the pressure, \(\:\nu\:\) is the kinematic viscosity of air, and \(\:\varvec{f}\) encapsulates the additional forces exerted on the fluid by the grid structure.
To model the effect of the grid structure within the airflow, IBM was utilized to model the boundary of the grid structure. The surface of the grid structure was discretized into a uniform grid, with the discretization points denoted as X, located on the fixed boundary of the grid structure. Concurrently, a set of immersed boundaries (IB) points \(\:{\varvec{X}}_{ib}\) were employed to passively trace the flow, originating from the locations at X. To constraint IB points \(\:{\varvec{X}}_{ib}\) to the fixed points X, a weak coupling scheme was imposed by exerting IB forces \(\:{\varvec{F}}_{L}\)on the surface of the grid structure, as expressed in the following equation,
$$\:\begin{array}{c}{\varvec{F}}_{L}=-\gamma\:\left[{\int\:}_{0}^{t}\left({\varvec{U}}_{ib}-\varvec{U}\right)dt+{\Delta\:}t\left({\varvec{U}}_{ib}-\varvec{U}\right)\right], \left(3\right)\end{array}$$
where \(\:\gamma\:\) is a large constant, \(\:\varDelta\:t\) is the time interval of the simulation, \(\:{\varvec{U}}_{ib}\) and \(\:\varvec{U}\) represent velocities of IB points \(\:{\varvec{X}}_{ib}\) and fixed points \(\:\varvec{X}\) on boundary, respectively. Note that \(\:\varvec{U}\) is set to zero during computation adhering to the no-slip velocity condition at the boundary, while \(\:{\varvec{U}}_{ib}\) is computed by interpolating the local fluid velocity from adjacent Eulerian grid points \(\:\varvec{x}\), as follows,
$$\:\begin{array}{c}{\varvec{U}}_{ib}=\sum\:u{\delta\:}_{h}\left(\varvec{X}-\varvec{x}\right)\varDelta\:V. \left(4\right)\end{array}$$
Here, u represents the fluid velocity at the Eulerian grid points x. The term \(\:\varDelta\:V={h}^{3}\) represents the volume of each grid cell, where h is the cell size. Note that the Cartesian grids encompassing the surface of grid structure are uniformly sized with h in all three spatial directions. Furthermore, the delta function \(\:{\delta\:}_{h}\) is formulated as
$$\:\begin{array}{c}{{\delta\:}}_{\text{h}}\left(x\right)=\frac{1}{{h}^{3}}\varphi\:\left(\frac{x}{h}\right)\varphi\:\left(\frac{y}{h}\right)\varphi\:\left(\frac{z}{h}\right), \left(5\right)\end{array}$$
where
$$\:\begin{array}{c}\varphi\:\left(r\right)=\left\{\begin{array}{c}\frac{1}{8}\left(3-2\left|r\right|+\sqrt{1+4\left|r\right|-4{r}^{2}}\right),\:\:\:\:\:\:\:0\le\:\left|r\right|<1,\\\:\frac{1}{8}\left(5-2\left|r\right|-\sqrt{-7+12\left|r\right|-4{r}^{2}}\right),\:1\le\:\left|r\right|<2,\\\:0,\:\:\:\:\:\:\:\:\:\:\:\:\:\:\:\:\:\:\:\:\:\:\:\:\:\:\:\:\:\:\:\:\:\:\:\:\:\:\:\:\:\:\:\:\:\:\:\:\:\:\:\:\:\:\:\:2\le\:\left|r\right|\end{array}\right. \left(6\right)\end{array}$$
denotes a four-point smoothed delta function53.
Similarly, \(\:\varvec{f}\) at the Eulerian grids is derived by interpolating the forces \(\:{\varvec{F}}_{L}\) exerted on the surface of the grid structure, i.e.,
$$\:\begin{array}{c}f=\sum\:{\varvec{F}}_{L}{{\delta\:}}_{\text{h}}\left(\varvec{x}-\varvec{X}\right)\varDelta\:V \:\left(7\right)\end{array}$$
For the flow solver, we adopted an implicit velocity decoupling procedure on staggered Cartesian grid system to solve the incompressible Navier-Stokes equations, as delineated by Kim et al54. The computational domain of the entire fluid field is set as \(\:15D\times\:9D\times\:9D\) for \(\:L,W\) and \(\:H\), respectively. The characteristic length scale is defined by the distance between the centerlines of nearby wires, with D being 25.4mm divided by the mesh count. The distance between the inlet and the center plane of the grid structure s is equal to D. This study employs a grid resolution of 32 uniform grids per length D, resulting in a total grid number of approximately 40 million. Periodic boundary conditions for velocity and pressure are imposed in both the \(\:y\) and z directions. The inlet velocity is uniform, expressed as \(\:\varvec{u}={U}_{g}{\varvec{e}}_{x}\), where \(\:{U}_{g}\) is the airflow velocity and \(\:{\varvec{e}}_{x}\) is the unit vector in the streamwise direction. At the outlet, a convective boundary condition is implemented. The kinematic viscosity of airflow is 1.48\(\:\times\:{10}^{-5}{m}^{2}/s\), and the inlet airflow velocity is around 18 m/s. Three different grid structures with mesh counts of 30, 60, and 150 were simulated, yielding Reynolds numbers based on D of \(\:Re={U}_{g}D/{\nu\:}_{g}=1100\), 550 and 220, respectively.
Volume of Fluid (VOF) method
The Volume of Fluid (VOF) method55 is one of the most commonly used interface capturing methods for simulating multiphase flows due to its mass conserving property, and ease in handling large interfacial deformations. In VOF framework, the different fluid phases interfaces are identified by an indicator fraction, α, which is chosen to be the fluid volume fraction on the Eulerian mesh. The fluid volume fraction α is given by
$$\:\begin{array}{c}\alpha\:=\left\{\begin{array}{c}0,\:\:for\:fluid\:A\\\:0<\alpha\:<1,\:\:mixing\:region\:between\:fluid\:A\:and\:B\:\\\:1,\:\:for\:fluid\:B\end{array}\right. \left(8\right)\end{array}$$
In VOF method, the fluid interface is reconstructed by the above fluid volume fraction, which is advected with the flow. The evolution of fluid volume fraction is modeled by
$$\:\begin{array}{c}\frac{\partial\:\alpha\:}{\partial\:t}+\nabla\:\cdot\:\left(\varvec{u}\alpha\:\right)+\nabla\:\cdot\:\left[\alpha\:\left(1-\alpha\:\right){\varvec{U}}_{r}\right]=0 \left(9\right)\end{array}$$
in which, Ur is the artificial compression velocity on the fluid interface to guarantee the sharpness of the fluid interface56.
The effect of the surface tension of the two-phase flow is determined by the Continuum Surface Model (CSF)57 in the momentum equation and continuity equation.
$$\:\begin{array}{c}\frac{\partial\:\rho\:\varvec{u}}{\partial\:t}+\nabla\:\cdot\:\left(\rho\:\varvec{u}\varvec{u}\right)=-\nabla\:{p}_{\text{r}\text{g}\text{h}}-\left(\mathbf{g}\cdot\:\mathbf{x}\right)\nabla\:\rho\:+\nabla\:\cdot\:\left[\mu\:\left(\nabla\:\varvec{u}+{\left(\nabla\:\varvec{u}\right)}^{T}\right)\right]+\sigma\:\kappa\:\nabla\:\alpha\: \left(10\right)\end{array}$$
$$\:\begin{array}{c}\nabla\:\cdot\:u=0\:. \left(11\right)\end{array}$$
where ρ and µ are the average density and viscosity weighted by the fluid volume fraction α, respectively. prgh is the pressure excluding hydrostatic pressure, g is the gravity acceleration, σ is the surface tension coefficient, and κ is the mean curvature of the fluid interface.
The mathematical models are also utilized to simulate the grid-turbulence atomization proposed in the present study. Moreover, the above multiphase flow model is solved with an open-source CFD platform, i.e., OpenFOAM. The grid structures, mesh resolution, and inlet airflow velocity are the same as those used in single-phase airflow simulation.
Q Criterion
The Q criterion is used to distinguish the vorticity-dominant region (Q > 0) and strain-dominant region (Q < 0). It is defined by the formula,
$$\:\begin{array}{c}Q=\frac{1}{2}\left(Tr\left({\varvec{\varOmega\:}}^{2}\right)-Tr\left({\varvec{S}}^{2}\right)\right), \left(12\right)\end{array}$$
where \(\:\varvec{\varOmega\:}\) is the fluid rotation tensor, and expressed as,
$$\:\begin{array}{c}\varOmega\:=\frac{1}{2}\left(\nabla\:\varvec{u}-\nabla\:{\varvec{u}}^{\text{T}}\right), \left(13\right)\end{array}$$
and \(\:\varvec{S}\) is the fluid strain-rate tensor as follows,
$$\:\begin{array}{c}S=\frac{1}{2}\left(\nabla\:\varvec{u}+\nabla\:{\varvec{u}}^{\text{T}}\right). \left(14\right)\end{array}$$
Note that \(\:\nabla\:\varvec{u}\) is the fluid velocity gradient tensor, \(\:Tr(\cdot\:)\) represents an operator of the trace.
Turbulence Intensity and Anisotropy
Turbulence intensity at a given position x is calculated using the following formula,
$$\:\begin{array}{c}I\left(x\right)=\frac{{{u}^{{\prime\:}}\left(x\right)}_{rms}}{⟨U\left(x\right)⟩}. \left(15\right)\end{array}$$
Here, \(\:{u}^{{\prime\:}}{\left(x\right)}_{rms}\) represents the root-mean-square of the velocity fluctuations in y-z plane at position x, and \(\:⟨U\left(x\right)⟩\) is the ensemble-averaged velocity in y-z plane at the same position x. Note that \(\:⟨\cdot\:⟩\) represents the ensemble-averaging in y-z plane.
Turbulence anisotropy \(\:\eta\:\) is a measure used to estimate the anisotropy of Reynolds stress in turbulent flows. The Reynolds stress in y-z plane at position x is denoted as \(\:⟨{u}_{i}^{{\prime\:}}{u}_{j}{\prime\:}⟩\), where \(\:{u}_{i}{\prime\:}\) is the component of fluid velocity fluctuation. The anisotropy factor \(\:\eta\:\) is defined as the second invariant of a normalized tensor\(\:{b}_{ij}\), which is calculated as,
$$\:\begin{array}{c}{b}_{ij}=\frac{⟨{u}_{i}^{{\prime\:}}{u}_{j}{\prime\:}⟩}{⟨{u}_{k}^{{\prime\:}}{u}_{k}{\prime\:}⟩}-\frac{1}{3}{\delta\:}_{ij}, \left(16\right)\end{array}$$
namely \(\:\eta\:={b}_{ij}{b}_{ji}\). When \(\:\eta\:\) approaches \(\:0\), the Reynolds stress becomes more isotropic, indicating the same statistics of fluid in any direction. Conversely, a higher \(\:\eta\:\) indicates a more anisotropic state of Reynolds stress.
Flow Visualization
Flow visualization was realized using a smoke-wire system in a wind tunnel (Supplementary Fig. 6), which is composed of a smoke-wire controller (SW02, Dalian Hanghua Science & Technology Co., Ltd, China), a resistance wire with a diameter of 0.1 mm, a flashlamp, and a digital camera (Canon 850D). In the experiment, paraffin oil was coated on the resistance wire to produce a smoke line under the control of the controller. The smoke line was blown forward in the wind tunnel and captured by the camera. The flashlamp was used to illuminate the flow field. Photographs of the smoke line's trajectory characterized the flow characteristics and vortex dynamics.
Spray Particle Size Measurement
The spray particle sizes, specifically the volume distribution of the droplets, were measured using a spray laser particle size analyzer (PW180-B, Shandong NKT Analytical Instrument Co., Ltd, China). The measuring axial distance was approximately 100 mm. The instrument was able to measure sprays of diverse substances by leveraging a built-in database containing material parameters. Data analysis was conducted using accompanying software provided by the manufacturer.
To determine the average diameter of the droplets, the Sauter Mean Diameter (SMD) was used, calculated using the formula:
$$\:\begin{array}{c}SMD=\frac{\sum\:\left({d}_{i}^{3}{n}_{i}\right)}{\sum\:\left({d}_{i}^{2}{n}_{i}\right)}, \left(17\right)\end{array}$$
where \(\:{d}_{i}\) represents the diameter of individual droplets, and \(\:{n}_{i}\) is the number of droplets with that diameter.
Evaluation of Humidification Efficiency of the Atomization System
To gauge the efficiency of the atomization system, a humidification experiment was conducted in an enclosed room of dimensions 2m × 3m × 4m (Supplementary Fig. 18a). The ambient humidity was initially reduced to 20% using a dehumidifier. Once this was achieved, the dehumidifier was turned off and the atomization system was activated. A digital hygrometer was employed to monitor and record the rise in humidity in real-time.
Morphology and structure Characterizations
The morphological properties and elementary composition of particles were measured by a field-emission scanning electron microscope (FE-SEM, LEO-1530, Zeiss, Germany) equipped with energy-dispersive X-ray spectroscopy (EDS). The diameter distribution of the particles was measured with a laser particle sizer (Mastersizer 3000, Malvern, UK). Crystal structure of SiO2, Al2O3, ZrO2, Li7La3Zr2O12, and LiNi0.8Co0.1Mn0.1O2 powder were determined by XRD (D/Max 2,500, Rigaku, Japan), where the X-ray was Cu-Kα radiation, scanning speed was 5°/min, and the scanning range was 10° − 80°.