1. Introduction
Outdoor air conditioning units commonly employ semi-open axial flow fans [
1] without external shrouds or guide vanes. The absence of confining flow passage boundaries leads to the formation of pronounced leakage vortices [
2] in the tip clearance region. The flow field of a semi-open axial flow fan is subject to the combined effects of protective grilles, wall obstructions, and varying outdoor wind speeds. Consequently, it exhibits significant three-dimensionality and strong unsteady fluctuations, which hinder the analysis of complex flow behaviors and the optimization of fan performance. Conventional contact-based, single-point measurement techniques, such as Pitot tubes [
3] and hot-wire anemometers [
4], not only introduce flow field distortion due to probe interference but also fail to resolve the high-frequency spatiotemporal evolution of vortex structures in the tip clearance region and the near wake. Particle image velocimetry (PIV) is a non-intrusive, high-spatial-resolution diagnostic technique for global flow fields [
5]. It enables the acquisition of high-accuracy instantaneous two-dimensional or three-dimensional velocity vector distributions while preserving the original flow field. Furthermore, high-fidelity flow field snapshots acquired by PIV enable the application of data-driven modal analyses, such as proper orthogonal decomposition (POD) [
6,
7,
8] and dynamic mode decomposition (DMD) [
9,
10,
11]. These techniques can extract the dominant coherent structures from highly turbulent and complex flows. The modal energy contributions and frequency characteristics derived from these decomposition methods quantitatively characterize the internal turbulent structures of the axial flow fan [
12]. These results provide indispensable empirical support for elucidating the low-dimensional evolution features [
13] of turbulence, assessing flow instability, and optimizing blade geometries. Therefore, conducting PIV flow field measurements and coherent structure analysis for semi-open axial flow fans is of significant importance for flow physics diagnosis and the implementation of advanced flow control strategies.
PIV experimental techniques have been widely adopted to investigate the complex internal flow in axial fans, resulting in substantial insights into core issues such as instability evolution, jet development, and tip leakage. In the context of instability dynamics, Hribernik et al. [
14] employed phase-resolved PIV [
15] to measure the angle-resolved flow field within the rotor passage under rotating stall conditions. The integration of low-frequency PIV systems with advanced data post-processing methods enables accurate measurement of high-frequency, unsteady flow phenomena such as rotating stall. This approach offers an economical and efficient means of advancing the understanding of rotating stall flow mechanisms [
16]. When an axial fan operates away from its design condition, a complex structure comprising alternating high-momentum jet regions and low-momentum wake regions develops within the blade passage. Hofer et al. [
17] conducted three-dimensional reconstruction of the free jet field in a small-scale axial flow fan using high-resolution 2.5D PIV [
18] volumetric scanning. Their results demonstrated that the jet from the small-scale fan exhibits pronounced rotating-jet characteristics, with diffusion and rotation rates that decay nonlinearly along the streamwise direction. The velocity profiles in the jet core region deviate markedly from classical free-jet theory. Tip clearance flow constitutes a major source of flow losses and is a primary cause of hazardous conditions such as stall and surge in axial fans. Dellacasagrande et al. [
19] applied two-dimensional PIV measurements in the meridional plane upstream of the annular fan rotor tip clearance. Under moderate load conditions, the leakage flow displays periodic radial oscillations [
20] that are independent of the blade passing frequency. Furthermore, the migration of these non-periodic, large-scale coherent structures across different radial positions [
21] significantly enhances turbulent momentum transport.
In the downstream region, the turbulent flow characteristics have also been extensively investigated. Čantrak et al. [
22] conducted experimental measurements of turbulent swirling flow in the duct downstream of an axial fan using high-speed stereoscopic PIV and performed a comprehensive analysis of the anisotropic turbulent state based on invariant mapping theory. The study found that, under swirling effects, the near-wall region of the duct exhibits significant turbulent anisotropy. A strong dynamic correlation exists between the periodic oscillation of the vortex core and the axial migration of the minimum total-velocity location [
23]. On the issue of tip leakage vortex behavior, Yu et al. [
24] performed phase-averaged measurements of the internal and surrounding flow fields of an axial fan using a high-resolution stereoscopic PIV system, obtaining three-dimensional flow structures inside and outside the rotor passage. The results revealed a strong tip leakage vortex in the tip clearance region, which undergoes intense mixing with the main flow during downstream transport and exhibits significant circumferential non-uniformity [
25] in both trajectory and intensity. Nevertheless, the flow field in the tip region of semi-open axial impellers possesses even more complex vortical structures, and few studies have conducted detailed experimental investigations of the tip vortex, tip leakage vortex, leading edge separation vortex, and related structures.
The flow structure of a semi-open axial flow fan, unconstrained by a closed casing, exhibits pronounced three-dimensionality and strong unsteady fluctuations [
26]. The core flow phenomena include complex vortical structures in the tip region [
27], periodic wake evolution [
28], and flow instability under off-design conditions [
29]. Liang et al. [
30] employed large eddy simulation [
8] to reveal that the flow field in the tip region of an open axial fan rotor consists of the tip vortex, leading edge separation vortex, and tip leakage vortex. The interaction among these three vortices gives rise to complex tip-flow phenomena, with the tip leakage vortex being dominant. Xie et al. [
31] elucidated the evolutionary process of the tip vortex from its generation at the blade leading edge to its development and dissipation downstream. They showed that, over time, the tip vortex extends to the rotor outlet region along an oblique line opposite to the direction of rotation. Jung et al. [
32] numerically obtained the total pressure loss distribution at the impeller outlet of an open axial flow fan, where the wake region accounts for 11.8% of the loss, the tip region 69.7%, and the hub region 18.5%. As it moves along the suction surface, the tip vortex continuously absorbs energy and intensifies, eventually detaching from the surface and entering the shroud region. During interaction with the shroud, the tip vortex is further stretched and squeezed, ultimately impacting and breaking up against the pressure surface of the downstream blade [
33]. In the trailing-edge tip region covered by the shroud, a tip leakage vortex analogous to that in closed axial flow fans is formed [
34], with its vortex scale and intensity comparable to those of the tip vortex [
35,
36]. Consequently, the tip leakage vortex not only weakens the work capacity of the tip region, causing significant aerodynamic losses, but also has a substantial impact on the aeroacoustic characteristics during fan operation [
37]. Nevertheless, the mechanisms underlying the unsteady evolution and the low-dimensional coherent structures of the tip leakage vortex in semi-open axial flow fans remain to be further investigated.
This study addresses two specific questions regarding the internal flow of a semi-open axial flow fan: (i) what are the dominant evolution modes and characteristic frequencies of the tip leakage vortex in the absence of a confining shroud, and (ii) how does the TLV interact with the CSV within the blade passage, and what are their combined effects on the downstream turbulent wake? High-resolution PIV measurements are conducted across multiple regions and viewing angles to capture transient flow structures (
Figure 1). DMD is subsequently applied to extract low-dimensional spatial modes and frequency characteristics from the acquired snapshots. This combined experimental and modal analysis approach quantitatively characterizes the periodic shedding behavior of the TLV, the coupling mechanisms between the TLV and CSV, and the spectral composition of the wake turbulence. The findings provide a physically grounded basis for flow diagnosis and blade design optimization of semi-open axial flow fans used in outdoor air conditioning units. The remainder of this paper is organized as follows:
Section 2 describes the PIV measurement methodology for the semi-open axial flow fan,
Section 3 presents the transient flow field analysis based on PIV, and
Section 4 discusses the coherent structure analysis. Finally, the main conclusions of this study are summarized in
Section 5.
2. PIV Measurement Method for a Semi-Open Axial Flow Fan
The PIV experimental platform established in this study integrates a comprehensive measurement system incorporating high-precision optical, mechanical, electrical, and computational technologies. The system consists of four core subsystems: a light-source subsystem, an imaging subsystem, a synchronization-control subsystem, and a data-acquisition-and-processing subsystem.
Figure 2a illustrates the working principle of the PIV system. The light source system employs a high-energy dual-pulse laser. An optical lens group shapes the laser beam into a light sheet with adjustable thickness to illuminate the target measurement plane within the flow field. The imaging system is equipped with a high-resolution, high-frame-rate scientific-grade CMOS camera. It precisely captures images of tracer particles illuminated by the light sheet. The synchronization control system coordinates the timing of laser pulses and camera exposure with nanosecond-level precision. This ensures accurate displacement calculation. The data acquisition and processing system integrates specialized control software. It is responsible for system control, image acquisition, and real-time processing of large-volume data. Advanced cross-correlation algorithms and GPU acceleration techniques are employed to rapidly compute the velocity field and derived physical quantities from raw particle images.
Figure 2b shows the PIV test platform built in this study and the on-site test arrangement.
2.1. PIV System Configuration and Experimental Protocol
- (1)
High-precision image acquisition
The imaging system is equipped with two high-resolution scientific-grade CMOS high-speed cameras (model: SM-CCDB29M4). The resolution reaches at least 6600 × 4400 pixels, and the pixel size is as small as 5 μm. These specifications ensure high-signal-to-noise ratio particle images across both large fields of view and microscopic scales. The high-speed cameras offer a fast acquisition rate, resulting in good temporal continuity of the captured flow field. This capability allows effective imaging of the high-velocity regions associated with local tip leakage vortices. In PIV mode, the minimum exposure time interval is ≤600 ns. The full-resolution acquisition rate is 4.7 frames per second. In framing mode, the maximum acquisition rate reaches 16 frames per second. The system is equipped with an NIKON 50 mm/F1.4 professional optical lens and a 100 mm/F2.8 macro lens. These lenses enable the acquisition of local flow fields in small regions.
- (2)
High-energy laser system
The PIV system employs two high-energy, high-frequency dual-pulse lasers as light sources (model: SM-LASER-BM500-10). The high-energy laser has a wavelength of 532 nm and a pulse energy of ≥2 × 1000 mJ. This provides sufficient illumination for large-scale flow field measurements. The high-frequency laser has a repetition rate of 0.2–10 kHz. It delivers high-repetition-rate pulsed light to capture high-frequency unsteady vortex dynamics. The laser beam is guided through a high-precision integrated beam transmission system and an adjustable light-sheet optics module. This forms a light sheet with a thickness of ≤1 mm and a maximum divergence angle of ≥75°. The light sheet can precisely illuminate the target measurement plane from the tip region to the main flow area. The laser sheet optics allow independent adjustment of the light-sheet length, thickness, and divergence angle. Depending on the test scenario of the internal flow field, a long light sheet with a small divergence angle can be selected. This configuration focuses illumination on the tip leakage flow region.
Before laser operation, the laser chiller must be turned on first. The chiller temperature should stabilize at 21 °C ± 0.2 °C. The laser temperatures should stabilize at 45 °C ± 0.1 °C, 45 °C ± 0.1 °C, and 28 °C ± 0.1 °C, respectively, before the laser power supply is switched on. The maximum laser current is 31 A, and the minimum current for laser emission is 8 A. During testing, the energy outputs of the two laser paths are not perfectly identical. Therefore, the brightness of the captured images should be monitored, and the current of one path may need to be increased by approximately 0.5 A, as appropriate.
- (3)
Precise synchronization and tracer particle seeding
The synchronous controller serves as the timing core of the system. Its time accuracy reaches ≤0.25 ns. This ensures nanosecond-level strict synchronization between laser pulses and camera exposure, enabling high-precision instantaneous velocity measurements. The particle generator provides water-based and DEHS oil-based tracer particles with high flow rates and stable concentrations. These particles cover a wide velocity range from low-speed flows up to 500 m/s. The system allows flexible switching according to experimental requirements. This ensures good particle-tracking fidelity and consistent scattering intensity across different flow regimes, including low-speed leakage flows and high-speed main flows.
- (4)
Intelligent calibration, control, and advanced data processing
The robotic assistance system consists of two high-precision collaborative robots (with a repeated positioning accuracy of ±0.05 mm). One robot carries the camera, and the other carries the laser light-sheet module. Through custom software, fully automatic joint calibration and scanning measurements of the optical path and imaging perspective are achieved. This greatly improves experimental efficiency and positioning accuracy in complex spatial configurations. The integrated software platform for system control and post-processing manages all experimental hardware. It also incorporates powerful post-processing algorithms for complex flows. In addition to standard cross-correlation analysis, the platform supports GPU acceleration, which significantly enhances computational efficiency. The platform also includes a continuous light-sheet system for flow visualization, a helium bubble generator for seeding in large-scale spaces, complete calibration targets, optical adjustment mechanisms, and a workstation.
The PIV experimental platform established in this study focuses on the processing and analysis of tip leakage vortices. It provides a functionally comprehensive and technically advanced fluid mechanics experimental platform capable of accurately capturing leakage flows. The specific procedure for the PIV experiments on the semi-open axial flow fan used in air conditioning units is shown in
Figure 3. To accurately capture and quantify the multi-scale vortex structures within the fan, the positions of the laser and camera were adjusted and tested before image acquisition.
For the overall flow field structure of the fan, non-intrusive water mist or helium bubbles were used as tracers. Single-shot coverage achieves a maximum area of 2500 mm × 1000 mm (2D2C), enabling observation of the entire fan or large-scale vortex structures. To precisely capture the transient generation, evolution, and breakdown of the leakage vortex within the tip clearance (typically <5 mm), the system is equipped with a high-frequency acquisition module. The maximum acquisition rate reaches 160,000 frames per second. Combined with a minimum light-sheet thickness of 1 mm, this configuration resolves high-frequency flow details within a microscopic field of view of 20 mm × 20 mm. This provides a wealth of refined flow field data to elucidate the complex, unsteady internal flow mechanisms.
Depending on the test scenario of the internal flow field, a long light sheet with a small divergence angle can be selected. This configuration focuses illumination on the tip leakage flow region. Before laser operation, the laser chiller must be turned on first. The chiller temperature should stabilize at 21 °C ± 0.2 °C. The laser temperatures should stabilize at 45 °C ± 0.1 °C, 45 °C ± 0.1 °C, and 28 °C ± 0.1 °C, respectively, before the laser power supply is switched on. The maximum laser current is 31 A, and the minimum current for laser emission is 8 A. During testing, the energy outputs of the two laser paths are not perfectly identical. Therefore, the brightness of the captured images should be monitored, and the current of one path may need to be increased by approximately 0.5 A, as appropriate.
The experimental procedure for PIV measurements on the semi-open axial flow fan is depicted in the flowchart in
Figure 3 and is summarized as follows. Before data acquisition, the laser sheet position and camera viewing angle were precisely aligned according to the measurement planes defined in
Section 2.3. The laser chiller was activated and allowed to reach thermal equilibrium at 21 °C ± 0.2 °C before the laser power supply was engaged. Tracer particles, either water-based or DEHS oil-based, were introduced into the flow field at a controlled concentration to achieve uniform particle distribution and sufficient scattering intensity. The synchronization controller was programmed to trigger the dual-pulse lasers and camera exposure with a timing accuracy of ≤0.25 ns, and a series of image pairs was recorded at each measurement plane. For each operating condition, at least 500 instantaneous image pairs were collected to ensure statistical convergence of the mean velocity field and turbulence statistics. Following acquisition, the raw particle images were processed using a multi-pass cross-correlation algorithm with progressively decreasing interrogation window sizes (from 64 × 64 to 16 × 16 pixels, with 50% overlap), resulting in final velocity vectors with a spatial resolution of approximately 0.5 mm. Vector validation and outlier removal were conducted using a local median filter.
2.2. Optical Modification and Specimen Preparation
This study provides a clear, unobstructed optical path for the laser light sheet to ensure accurate measurement of the internal flow field using particle image velocimetry. Given the compact structure and complex components of the outdoor air conditioning unit, the test fan was specifically modified to provide optical access (
Figure 4). First, the housing was treated to improve light transmission. The original fan housing was made of metal, which could not transmit laser light. Therefore, a transparent housing was custom-manufactured from high-transmittance acrylic panels. The transmittance of this housing at 532 nm exceeds 99%. This minimizes the attenuation of laser energy during incidence and ensures adequate illumination of tracer particles within the measurement region.
Second, surface reflection was suppressed. The motor support and the blades are the main internal components along the laser incidence path. Their metallic surfaces tend to generate strong reflected light, which creates background noise and interferes with particle image acquisition. To address this, a black matte paint was uniformly sprayed onto the surfaces of these components. This effectively reduces the surface reflectivity to below 5% and significantly suppresses stray light interference with camera imaging.
Finally, after the above optical modifications and component treatments, the experimental model meets the optical requirements for PIV measurements while maintaining the original aerodynamic integrity. Commissioning results demonstrate that this optical path design yields clear particle images. This provides a reliable experimental basis for subsequent flow field measurements and vortex-structure analysis.
2.3. Measurement Area Calibration
This study aimed to accurately capture the complex three-dimensional unsteady flow structures within a semi-open axial fan system. Accordingly, the measurement regions and viewing angles for particle image velocimetry (PIV) were systematically designed based on the fan geometry and flow characteristics, as shown in
Figure 5. The measurement scheme followed the principles of zonal measurement and multi-view complementarity. The internal flow field was divided into three regions: the inlet, guide vane, and outlet regions. Flow field acquisitions were conducted from four key orientations, enabling refined observation of the core vortex structures, including the tip vortex, leading edge separation vortex, and tip leakage vortex.
The inlet region measurements focused on the upstream flow patterns of the impeller. The flow field in this region was influenced by the inlet grille of the outdoor unit and the heat exchanger wake, exhibiting significant non-uniform inflow characteristics. The measurement plane was set as a meridional plane parallel to the impeller rotation axis. It mainly captured the inflow angle, the degree of inflow distortion, and their influence on the impeller inflow conditions. The guide vane region measurements constituted the core observation area, with particular attention paid to the leakage flow near the tip clearance. The measurement plane was arranged perpendicular to the impeller axis, covering the entire tip region from the blade leading edge to the trailing edge. By shifting the laser sheet radially, instantaneous velocity fields at different blade span sections were obtained. These were used to resolve the generation location, development trajectory, and interaction mechanisms of the tip vortex with the leakage flow. The outlet region measurements were intended to reveal the wake flow and vortex dissipation characteristics. The measurement plane also adopted a cross-sectional layout perpendicular to the axis. It mainly observed the wake width, velocity deficit, and turbulence intensity distribution downstream of the blade trailing edge, and assessed the evolution and decay of the vortex structures in the outlet section.
Based on the above imaging plan and the zonal flow characteristics within the fan, three measurement orientations were designed to acquire refined measurements of key flow features in the inlet, guide vane, and outlet regions, as shown in
Figure 5. Orientation 1 was the inlet-region measurement. The laser sheet was aligned with the fan meridional plane, making it coplanar with the impeller rotation axis. The camera was placed at the side of the inlet, with its optical axis perpendicular to the laser sheet plane, and imaging was conducted through the high-transparency acrylic casing. This orientation mainly captured the velocity distribution and distortion characteristics of the non-uniform inflow in the inlet section. Orientation 2 was the guide vane region—tip passage measurement. To resolve the complex vortex structures in the tip region, an oblique-view imaging scheme was adopted. Both the laser sheet and the camera optical axis was adjusted to form a 45° angle with the meridional plane and to be perpendicular to each other. This arrangement effectively captured the generation and evolution of the tip vortex and tip leakage vortex inside the blade passage. Orientation 3 was the guide vane region—outlet cross-section measurement. The laser sheet was arranged parallel to the impeller outlet plane, and the camera was positioned for orthogonal front-view imaging. This orientation was used to acquire instantaneous velocity fields at the outlet cross-section of the guide vane region, with a focus on analyzing wake flow, vorticity distribution, and turbulence characteristics.
A pre-test flow visualization using a continuous-wave laser was performed before formal PIV acquisition to align the laser sheet with the targeted vortex structures. By tracing the streak lines of seeded particles, we identified the core trajectory of the tip leakage vortex and the accumulation region of the corner separation vortex. The light-sheet positions for the three orientations were then adjusted to ensure the measurement planes intersected the characteristic regions and to avoid optical obstructions from the motor support and the downstream components. This approach ensures that the captured velocity fields represent the dominant coherent structures rather than arbitrary flow cross-sections.
The primary source of measurement uncertainty in the current PIV system is the sub-pixel interpolation algorithm used in cross-correlation analysis. A standard Gaussian peak-fitting routine provides a displacement resolution of approximately 0.1 pixels. In high-velocity mainstream regions, where particle image displacements are typically 8–12 pixels, the relative velocity error is estimated at ±1–2%. In low-velocity vortex-core and near-wall regions, with displacements of about 3–5 pixels, the relative error increases to ±2–3%. To reduce random errors, all instantaneous velocity fields and DMD analyses used over 500 snapshots, ensuring statistical convergence of the dominant frequencies and spatial modes. The timing controller’s synchronization accuracy (≤0.25 ns) and the robotic positioning system’s repeatability (±0.05 mm) further support the reliability of the data.
Through combined multi-zone and multi-view measurements, a comprehensive capture of the three-dimensional unsteady flow field inside the semi-open axial fan was achieved. This not only ensured the completeness of the flow field information but also enabled spatial resolution and dynamic tracking of key vortex structures, such as the tip vortex and leakage vortex. The experimental design provided high-confidence data to reveal the mechanisms of flow loss and locate aeroacoustic noise sources.
4. Coherent Structure Analysis
The PIV transient flow field data allow direct observation of the periodic evolution of the tip leakage vortex, the formation and squeezing of the counter-rotating vortex pair within the blade passage, and the asymmetric distribution of the wake deficit region at the outlet cross-section. However, these instantaneous snapshots essentially represent superimposed projections of turbulent full-scale fluctuations and background noise in physical space. The highly nonlinear, multiscale coupling of the flow field causes the dominant large-scale coherent structures to be closely mixed with random small-scale fluctuations in the original variable space. This makes it difficult to reliably identify the dynamic modes governing the flow evolution from a single or a few instantaneous images. Therefore, dynamic mode decomposition is employed to extract coherent structures from the PIV transient flow field, providing a quantitative basis for further elucidating the unsteady flow-loss mechanisms arising from multi-vortex coupling within the impeller.
DMD can be viewed as a finite-dimensional approximation of the Koopman operator [
44,
45,
46]. Consider a discrete-time dynamical system for which a sequence of snapshot data [x
0, x
1, …, x
n] is observed. Assume that the snapshots evolve approximately under an unknown linear operator
A:
Two data matrices offset by one time step,
X = [x
0, x
1, …, x
n−1] and
X′ = [x
1, x
2, …, x
n], approximate the relationship between them via a linear operator
A (i.e., X′ ≈ AX). Singular value decomposition [
47] is applied to matrix
X with a low-rank truncation at rank
r (i.e.,
X ≈
UrΣrVr*). Projecting A onto the subspace spanned by Ur yields a low-dimensional approximate matrix
:
The approximate matrix
captures the action of matrix
A on the dominant proper orthogonal decomposition (POD) modes, thereby avoiding the need to handle large n × n matrices. The eigendecomposition of
is computed as
W =
WΛ, where
Λ = diag(λ
1, …, λ
r) and
W is the eigenvector matrix [w
1, w
2, …, w
r]. The DMD modes are defined as:
Each column
Φj corresponds to an eigenvalue
λj and satisfies the approximate eigenrelation
AΦj ≈ λ
jΦj.
λj is the eigenvalue of the DMD mode, describing the dynamic behavior of the corresponding mode. Combining the modes and eigenvalues, the snapshot at any time instant can be expanded as:
where
b = (
b1, …,
br)
T is the modal amplitude at the initial time.
To ensure the reliability of the dynamic mode decomposition (DMD) results and to substantiate the conclusions derived from the modal analysis, three validation checks were conducted: spectral resolution, statistical convergence, and spatial resolution. The total sampling duration (T = N × Δt = 500 × 0.213 s ≈ 106.5 s) provides a frequency resolution of approximately 1/T ≈ 0.009 Hz. This resolution is sufficient to distinguish the dominant frequencies of interest, such as 98.5 Hz and 16.44 Hz (
Section 4.1), as well as their higher harmonics. For spatial resolution, the local microscopic field of view (FOV) of 20 mm × 20 mm, combined with the camera resolution and a final interrogation window size of 32 × 32 pixels with 50% overlap, results in a vector spacing of approximately 0.096 mm. This spacing is significantly smaller than the estimated vortex core diameter (2–3 mm), ensuring adequate resolution of the velocity gradients within the tip leakage vortex. In terms of noise suppression, the overall velocity error remains within ±1–3%. The high-quality particle image velocimetry (PIV) data provide a sufficient signal-to-noise ratio for subsequent DMD analysis.
4.1. Coherent Structure Analysis of the Tip Leakage Vortex
Based on the transient flow fields in the tip clearance region acquired from PIV Orientation 1 (
Figure 5), DMD was performed on a flow field snapshot matrix with a size of 2666 × 500.
Figure 10a shows that the modes appear in conjugate pairs, with each pair sharing the same energy but opposite frequencies. The first ten modes with the highest energy were analyzed in detail, and the spatial distributions of the real and imaginary parts of the dominant modes are shown in
Figure 10b.
DMD Mode
Φ1 accounting for the largest share of the total energy, accounting for about 88.5%. The characteristic frequency of Mode
Φ1 is f = 98.5 Hz, and its spatial structure consists of two pairs of symmetrically distributed vortex clusters [
48]. Vortex A near the pressure surface represents the concentrated vorticity of the blade passage main flow, which is driven by the pressure difference across the tip clearance and migrates toward the suction surface side in region B. Vorticity shedding and separation occur in the direction of region C. This spatial evolution path is highly consistent with the generation and shedding trajectory of the tip leakage vortex observed in the PIV time-averaged field and instantaneous snapshots. The vortex shedding frequency [
49] (f
TLV = 98.5 Hz) is approximately 2.19 times the blade passing frequency (f
BPF = 45 Hz), indicating that about two complete leakage vortex generation–shedding cycles occur within one blade passing period (120°). From the initial formation of the leakage vortex in
Figure 6a to the splitting tendency shown in
Figure 6e, and then to the re-expansion of sub-vortex A1 in
Figure 6g, which evolves into the large-scale low-speed region of the next cycle, the temporal sequence clearly exhibits a characteristic frequency that is a multiple of the blade passing frequency. The spatially symmetric vortex pair structure of DMD Mode 1 is precisely the low-dimensional representation of this dominant-frequency periodic shedding in spectral space.
The second-highest-energy mode (3.1% of the total energy), Mode
Φ3, corresponds to the second harmonic of the tip leakage vortex (approximately 197 Hz). Its spatial distribution exhibits an antisymmetric structure along the blade passage outflow direction, and the radial distribution of the main flow also displays antisymmetric features. This harmonic mode reflects the asymmetric evolution of the leakage vortex over one fundamental period (as shown in
Figure 6e–g). The leakage vortex splits into asymmetric sub-vortices A1 and A2; the differences in their spatial scales, vorticity intensities, and migration directions constitute the physical origin of the second harmonic. The appearance of the antisymmetric structure indicates that the periodic development of the leakage vortex is not a simple linear oscillation but rather contains a significant dipole component. This is closely associated with the asymmetric distortion induced by the shearing effect of the main flow in the blade passage and the squeezing between the upper low-speed and lower high-speed fluids.
Mode
Φ5 (energy contribution: 3.09%) captures the macroscopic coherent structures of the blade-passage turbulence, with a frequency lower than that of the main leakage vortex mode. Its spatial mode exhibits an antisymmetric distribution along the flow direction, corresponding to shear-layer oscillations between the main flow and the secondary flow induced by the leakage vortex within the blade passage. In conjunction with the three-layer zonal structure of the blade passage flow and the blockage effect of the large-scale separation on the pressure surface side shown in
Figure 8, the antisymmetric structure of Mode Φ5 can be interpreted as alternating high- and low-speed streaks spanning the blade passage in the radial direction. Mode
Φ7 (energy contribution: 1.21%) represents the high-frequency turbulent structures within the blade passage. Its frequency scale corresponds to the turbulent fluctuations accumulated over a complete rotation cycle (360°) of the three blades. This mode integrates the composite turbulent effects resulting from the shedding of the leakage vortex, the migration of the corner separation vortex, and the mixing of multi-scale vortex clusters within the blade passage. In physical space, this mode may correspond to the small-scale vortex groups that undergo squeezing deformation and dissipate along the flow direction, as shown in
Figure 8d,e. Its high-frequency characteristics reflect the energy contributions from the roll-up of intense shear layers and near-wall turbulent bursts within the blade passage.
Mode
Φ10 (energy contribution 0.89%) reveals the shedding direction structure of the third harmonic (approximately 295.5 Hz) of the tip leakage vortex. Its spatial distribution extends along the direction indicated by the yellow dashed line in the figure, forming a certain angle with the main shedding direction of Mode Φ1. This higher-order harmonic reveals the nonlinear three-wave interaction occurring during the periodic shedding of the leakage vortex. The fundamental vortex shedding and the second-harmonic distortion generate higher-order frequency components through phase coupling. Although the third-harmonic mode has a relatively low energy contribution, it provides an important dynamic contribution to the fine modulation of the periodic morphology of the leakage vortex and to the excitation of high-frequency wake fluctuations. This corresponds one-to-one to the higher-frequency secondary vortex shedding process during the transition from vortex splitting to reconstruction, as shown in
Figure 6f–h.
4.2. Coherent Structures in Non-Uniform Blade Passage Flow
Based on the time series of the blade passage flow field acquired from PIV Orientation 2 (
Figure 5), DMD was performed on the flow field snapshot matrix with a size of 3969 × 500 (
Figure 11).
Figure 11a shows that the energy proportions of the first ten modes are 52.8%, 15.6%, 7.8%, 3.7%, and 2.1%, respectively.
Figure 11b presents the DMD mode with the largest energy proportion (characteristic frequency f = 97.99 Hz), which is highly consistent with the dominant frequency of the tip leakage vortex (98.5 Hz) extracted from Orientation 1. This further confirms the absolute dominance of the tip leakage vortex in the blade passage flow field. The high-amplitude region is concentrated near the tip clearance, forming a vortex shedding region with its core on the suction surface. Its spatial morphology is consistent with the characteristics of the high-Q-value vortex core at the blade tip and its evolution into a counter-rotating vortex pair structure identified by the Q-criterion in
Figure 7b–d. The leakage vortex rolls up due to the pressure difference across the tip clearance, and its vorticity is highly concentrated at the suction surface and the blade tip. The amplitude gradient of the real part clearly delineates the spatial boundary and the direction of intensity decay of the leakage vortex core. The spatial distribution of the imaginary part reveals the coupled origin of the leakage vortex generation. The vorticity originates not only from the jet shear at the tip clearance but also from the secondary flow induced by the hub corner separation vortex. The generation of the tip leakage vortex is not an isolated leakage flow behavior; rather, it is a product of the mutual entrainment and phase coupling among three flows: the blade passage main flow, the tip leakage flow, and the hub corner secondary flow.
Figure 11c corresponds to the large-scale vortex shedding mode associated with one full impeller revolution (360°). Its real part exhibits streak structures of large-scale vortices along the tangential direction, encompassing the traces of periodic transport and shedding of the main flow vortex, the tip leakage vortex, and the corner separation vortex. The imaginary part focuses on the antisymmetric spatial structure of the corner separation vortex at the hub, which precisely corresponds to the physical process captured by the Q-criterion in
Figure 7c,d, showing the evolution from a small-scale counter-rotating vortex pair to a large-scale one. After the corner separation vortex rolls up at the suction surface and hub corner, the induced secondary flow and the main flow form a counter-rotating vortex pair. The antisymmetric distribution of the DMD imaginary part is exactly the complex amplitude representation of this vortex pair structure in the modal space.
Figure 11d shows the second-harmonic mode of the tip leakage vortex (f = 196.59 Hz). The spatial distribution of its real part clearly delineates the shear layer boundaries between the tip leakage vortex and the corner separation vortex, as well as between these two and the main flow. This boundary divides the blade passage into three flow zones along the blade rotation direction. The hub corner flow is deflected toward the hub due to entrainment by the corner separation vortex. The tangential main flow in the mid-passage and the flow in the tip leakage-vortex influence zone near the blade tip accelerate in the direction of the blade passage outflow. This three-zone structure corresponds one-to-one to the three-layer zonal flow on the pressure surface side observed in
Figure 8a,f. The second-harmonic leakage vortex undergoes asymmetric evolution within one fundamental period, as shown in
Figure 7e,f, where the high-Q-value vortex core is squeezed and stretched by low-Q-value fluid, splitting into sub-vortices A1 and A2 of unequal size. This asymmetry excites the second harmonic, which is captured in Mode 3 as an antisymmetric oscillation along the shear layer boundary.
Figure 11e captures the dominant frequency mode of the hub corner separation vortex, with a frequency of f = 16.44 Hz. This frequency is close to but slightly higher than the frequency corresponding to one impeller revolution (15 Hz). The corner separation vortex completes one coherent shedding slightly earlier than the blade passing frequency within one full blade rotation cycle. As the main flow in the blade passage is expelled at high speed, the corner separation vortex, under the combined effects of a strong adverse pressure gradient and endwall friction, is the first to detach from the suction surface and hub corner region, resulting in a shedding phenomenon with a frequency slightly higher than the rotational frequency. In the spatial mode, regions A and B mark the secondary flow entrainment path from the main flow into the hub corner region. This entrainment provides a continuous supply of low-momentum fluid to the corner separation vortex, enabling it to maintain a coherent structure along the rotation axis. This entrainment-and-shedding cycle corroborates the physical process observed in
Figure 7g,h, where sub-vortex A1 gradually accumulates in region B and develops into a vortex cluster of considerable size. The periodic shedding of the corner separation vortex provides the low-speed recirculation zone and initial vorticity for the inception of the tip leakage vortex in the next cycle.
Figure 11f shows a mode whose frequency is composed of a combination of the corner separation vortex frequency and the blade rotation frequency. This frequency occurs before the impeller rotates through 120° (corresponding to 45 Hz), revealing the asymmetric accelerated evolution of the corner separation vortex within a fundamental period. Within one blade passing period, the corner separation vortex undergoes a complete cycle of formation, development, and ultimate disruption of the main flow. During its development stage, it entrains and blocks the region from the suction surface to the hub corner, thereby reducing the effective flow area. During its disruption stage, it vigorously mixes with the main flow and breaks into turbulent structures of various scales. These fragmented turbulent clusters constitute an important source of high-frequency turbulent energy in the blade passage.
4.3. Coherent Structures in Wake Flow
Figure 12 presents the DMD results based on the time series of the wake flow field at the outlet cross-section acquired from PIV Orientation 3 (
Figure 5).
Figure 12a shows that the energy proportions of the first ten modes are 4.1%, 3.9%, 3.3%, 2.8%, and 2.5%, respectively. Compared with the tip leakage and blade passage flows, the energy distribution among the DMD modes here is more uniform. The DMD mode with the highest energy (
Figure 12b) has a frequency of f = 248.45 Hz. This frequency can be interpreted as the nonlinear superposition of the second harmonic of the tip leakage vortex dominant frequency (f
TLV = 98.5 Hz, i.e., 197 Hz), the corner separation vortex frequency (f
CSV = 16.44 Hz), and the blade passing frequency (f
BPF = 45 Hz). The dominant coherent structure in the outlet wake is not a linear continuation of a single vortex system but rather a composite mode formed by the full coupling of the two dominant upstream vortex systems with the blade passing effect in the wake. Near the grille outlet (regions A and B), local small-scale vortices exhibit asymmetric coherent structures, reflecting the intensity asymmetry and phase difference between the high-frequency component of the tip leakage vortex and the low-frequency component of the corner separation vortex in the near-field wake. Along the wake development and flow direction, the small-scale vortices gradually merge, roll up, and evolve into large-scale vortices, forming a large-scale antisymmetric vortex shedding coherent structure in regions C and D. This spatial evolution from near-field small scales to far-field large scales represents a classical Kármán vortex street mechanism driven by wake shear layer instability and vortex pairing and merging, operating under the composite frequency modulation.
The mode with the second-highest energy (
Figure 12c) has a frequency of f = 186.34 Hz. Its frequency composition can be decomposed as the sum of the tip leakage vortex dominant frequency (f
TLV = 98.5 Hz) and twice the blade passing frequency (2 × f
BPF = 90 Hz). This mode characterizes the coupling effect between the coherent shedding of the tip leakage vortex and the periodic blade sweep. The spatial structure shows that small-scale vortices still accumulate near the grille outlet and develop in the flow direction. The wake development is governed by the joint frequency action of the tip leakage vortex frequency and the blade rotation frequency. The harmonic component of the blade rotation frequency provides a modulation envelope for the periodic shedding of the leakage vortex. The proximity of the two frequencies (98.5 Hz and 90 Hz differ by only about 9%) leads to a beat frequency effect, which manifests as periodic expansion and contraction of the spanwise vortex intensity in the wake.
Figure 12d presents the characteristics of the coherent structure with a frequency of f = 124.22 Hz. This frequency can be decomposed as the sum of the tip leakage vortex frequency (f
TLV = 98.5 Hz) and the blade passing frequency (f
BPF = 45 Hz), minus the corner separation vortex frequency (f
CSV = 16.44 Hz). The blade rotation promotes the generation and development of the tip leakage vortex (providing a positive frequency contribution), whereas the corner separation vortex acts as a reverse frequency coupling component. In the spatial distribution of the imaginary part, staggered phase jumps of the coherent structure along the radial direction can be observed. The negative modulation by the corner separation vortex causes the vortex shedding events associated with the leakage vortex in the wake to be delayed or attenuated in time, reflecting an antagonistic relationship between the two vortex systems during wake evolution.
The coherent structure shown in
Figure 12e has a frequency of f = 62.11 Hz, which can be decomposed as the sum of the blade passing frequency and the corner separation vortex frequency. This mode directly characterizes the nonlinear interference between the corner separation vortex and the blade rotation effect. In conjunction with the spatial evolution characteristics of the corner separation vortex within the blade passage when the blade rotates approximately 120°, as shown in
Figure 8d, this frequency exactly corresponds to the coherent variation in the corner separation vortex over the time scale of approximately 120° blade rotation. Within this interval, the corner separation vortex undergoes formation, development, and nonlinear interference with the main flow, ultimately disrupting the main flow and generating turbulent structures of various scales.
Figure 12f presents the spatial distribution pattern of a high-frequency coherent structure (f = 559.0 Hz). Its frequency can be decomposed as the superposition of the second harmonic of the tip leakage vortex (2f
TLV = 197 Hz) and the modal frequency shown in
Figure 12d (f = 62.11 Hz). The actual frequency is even higher, possibly incorporating additional higher-order harmonic components. The time scale corresponding to this high-frequency mode is an extremely short period of approximately 9.7° of blade rotation. The higher harmonics of the tip leakage vortex, the low-frequency oscillation of the corner separation vortex, and the blade rotation effect are mutually entangled and strongly nonlinearly coupled, forming highly complex turbulence patterns. The spatial distribution exhibits fragmented and irregular small-scale vortex clusters without distinct large-scale organizational features. This frequency has entered the inertial subrange, where turbulent energy is transferred from low-frequency coherent structures to high-frequency dissipation scales through the vortex energy cascade.