Introduction

Flow in the axial compressor is quite complex because it contains kinds of unsteady flow structures such as the tip leak flow (Booth et al., 1982), the rotor-stator interacting (Liu et al., 2019a, 2023), the corner separation flow (Zhong et al., 2024) and boundary layer transition (Liu et al., 2024c). Among them, tip leakage flow (TLF) is a typical compressor secondary flow caused by the pressure difference between the blade's pressure side and the suction side. The leakage jet interacts with the passage flow and forms the tip leakage vortex (TLV). TLF has a significant effect on the efficiency (Inoue et al., 1986), flow stability (Adamczyk et al., 1993; Tan et al., 2010), and noise generation of the compressor (Hsiao and Chahine, 2005). With the development of the compressor design toward more compact and higher loading, the effect of the TLF is increasingly significant.

Computational fluid dynamics (CFD) has become an important tool for studying compressor flow. In the current design process, the Reynolds-averaged Navier-Stokes (RANS) method is widely used because it is cheap in consumption, and many endeavors have been made to modify turbulence models (Li and Liu, 2022; Liu et al., 2011, 2020, 2023, Liu et al., 2024c). Alternatively, high-fidelity CFD methods, including direct numerical simulations (DNS) and large eddy simulation (LES), can supply detailed information on flow structures, which is critical for flow physics studies and flow control (Xie et al., 2023). Recently, hybrid methods, which combine the advantages of the Reynolds-averaged Navier-Stokes (RANS) and LES, have drawn increased attention. Hybrid methods use the RANS model to solve the flow within the boundary and use the LES at the main flow. Therefore, it can reach a high accuracy using a much lower computational consumption. Commonly used hybrid methods include DES (Spalart et al., 1997), DDES (Spalart et al., 2006), and GAS (Wang and Liu, 2022). DDES has already been used to study the unsteady flow characteristics of the tip leakage flow in a compressor rotor, and the results are compared with URANS results (Liu et al., 2019b). Then, a physical flow model aimed at simulating the TLF is proposed to reproduce the flow shear mechanism between jet flow and the main flow of tip leakage vortex roll-up (Gao and Liu, 2019). Flow visualization technology, including the pathline and streakline, has also been used to analyze the vortex transportation of the tip leakage vortex under different working conditions based on the results from DDES (Hou et al., 2022). The vortex structures and vortex instability are found to be crucial to describing the TLF, and the advanced vortex identification methods are important tools for studies of TLV, such as the local trace criterion (LTcri) (Liu and Tang, 2019; Liu et al., 2021) and the VR helicity (Tang and Liu, 2022). With the help of the vortex identification method, the different swirling patterns of complex vortices could be distinguished through regional indication. The computational consumption of the high-fidelity method is very large. The RANS method is still widely used in the compressor design stage. Therefore, turbulence modeling for the TLF in RANS simulation is also an important research area (Liu et al., 2008). Traditional turbulence models are found hard to accurately modeling the turbulence characteristic in the TLV (Gao et al., 2016) in a low-speed large-scale axial compressor rotor. Then, a modification of the zonal function is proposed to correct the excessive dissipation of the modeled turbulence kinetic energy (TKE) (Gao and Liu, 2020) in the tip leakage vortex region.

The TLF has been found to be highly unsteady in many previous studies (Zhang et al., 2006; Tong et al., 2007), and its unsteady characteristics affect the noise, blade vibration, and loss generation (Wisler, 1985). Many types of unsteadiness have been reported for TLF. The dynamic interaction of the incoming main flow and the tip leakage flow could induce self-induced unsteadiness in the TLF (Du et al., 2010), and the oscillation of the TLV could also be attributed to an induced vortex and the shock-vortex interaction (Hah et al., 2006). Vortex breakdown is another unsteady flow feature. The breakdown of the TLV could enlarge the blockage region in the tip region (Wang et al., 2021). The stability of the compressor rotor is also related to the unsteadiness of the TLV (Furukawa et al., 1999). Rotating instability vortex are found to be the leading cause of unsteadiness during the development of rotating instability in a low-speed axial flow compressor (März et al., 2002). Therefore, detailed studies on the unsteadiness of TLF are needed to develop new modeling and flow control techniques.

However, extracting key flow features from unsteady flow fields is also challenging because the dataset is massive for high-fidelity simulation results or experimental results. With the progress of computer technology, data-driven approaches have become increasingly prevalent in fluid mechanics, including deep learning, reinforcement learning, modal analysis, etc. These techniques are crucial in feature identification, flow field prediction, and flow control (Liu et al., 2024a,b). Recently, dynamic mode decomposition (DMD) (Schmid, 2010) has been proposed as a data-driven approach to analyze unsteady flow. DMD belongs to the mode analysis method derived from Koopman's theory (Rowley et al., 2009). DMD can extract coherent spatiotemporal structures from time series data. Then, a low-dimensional linear model describing the evolution of these dominant coherent structures can be built. Compared with proper orthogonal decomposition (POD), DMD can provide spatial information in each mode and temporal information embedded in each eigenvalue. This advantage leads to the extensive usage of DMD in analyzing flow phenomena and modeling flow dynamics (Taira et al., 2017; Kunihiko et al., 2020). Application of the DMD or other mode analysis methods has already been conducted in turbomachinery flow, such as the analysis of the pressure pulsation in centrifugal compressor dynamic structures (Zhang et al., 2022) and the analysis of the experimental data to describe the transition process of separation flow (Lengani et al., 2016). Additionally, DMD is also helpful in the development of the reduced order model (ROM) and has been used in isolated airfoils and turbomachinery cascades (Florea and Hall, 1998; Dowell et al., 1999). Since the TLF has abundant unsteady motions, DMD is also valuable for analyzing its flow feature.

This work investigates the unsteady characteristics of the TLF in a rotor based on the unsteady flow field dataset simulated via the DDES. The LTcri method and VR helicity are used to identify the vortex structure, and then DMD for single variables matrix is conducted to extract the spatial-temporal unsteady flow structures. Finally, DMD is conducted for the velocity vector matrix, and the contribution of different DMD modes to the vortex structure of TLV and loss generation are analyzed based on the flow field rebuilt using different modes of the velocity vector.

Case description and numerical method

Test case description

The axial rotor studied in this work is a low-speed compressor that has been tested using the stereoscopic particle image velocimetry (SPIV) method in a low-speed large-scale axial compressor test facility at Beihang University (Liu et al., 2006). The schematic of this experimental rig and the SPIV measurement locations are shown in Figure 1, and the details of the design parameters are summarized in Table 1. The flow in this test compressor, such as the mechanism of the formation and development of the TLV, has also been discussed in our previous papers (Hou and Liu, 2023; Hou et al., 2022). The design point of this rotor is defined as the mass flow coefficient of 0.58, and the near-stall point is defined as the mass flow coefficient of 0.39. The numerical result is validated in our previous work, and the DDES results show a good accordance with the experimental data (Liu et al., 2006).

Figure 1.

Schematic Layout of the SPIV Measurement Cross Sections of the Axial Rotor (Liu et al., 2008).

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Table 1.

Parameters of the rotor.

Outer diameter (m)1.0
Aspect ratio (−)0.6
Design speed (rpm)1,200
Flow coefficient in design condition (−)0.58
Loading coefficient in design condition (−)0.45
Design mass flow rate (kg/s)22.4
Reynold number based on the rotor tip chord (−)7.5 × 105
Inlet guide vane rotor axial gap (mm)41.9

Numerical method

The software Numeca Autogrid 5 is used to generate a high-quality structure grid. The grid of the rotor blade uses the O4H-type topology. To better capture the structure of TLF in the tip region, the grid within 20% of the span height to the shroud is refined with a maximum expansion ratio of 1.05. and the grid spacings are kept as Δx + <120, Δy + <110, and Δz + <1, respectively. The total number of grid points is 6.17 × 106, and details of the final grid are shown in Figure 2.

Figure 2.

Grid of the Rotor.

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The numerical simulations use the pressure-based implicit solver from the commercial solver Ansys Fluent and the iterative time advancement solution method is used. The SIMPLE algorithm is used for the simulation. A central differencing scheme is employed for spatial integration, and the implicit second-order time integration is adopted for temporal discretization. The time step for the outer time marching is set to 3 × 10−6 s, which is approximately 1/1,000 times the blade passing the time (TBP), and 30 iterations are set at each inner iteration. The first sample time of the DDES is considered to be tNS/TBP=0 at the near-stall condition. A statistical steady state is reached for all calculations. The instantaneous flow fields are sampled with a time interval (t) of 3 × 10−5 s. More details of the computational setting can be found in our previous work (Liu et al., 2019b).

Dynamic model decomposition

DMD was developed based on the theory of the Koopman operator (Rowley et al., 2009; Schmid, 2010). It is a popular method to extract the temporal-spatial coherent structure in unsteady flow and develop reduced-order modeling (Dowell et al., 1999). Compared with the traditional POD method, DMD could supply more information in the temporal domain. The algorithm of the DMD is introduced as follows. First, snapshots of data must be collected, and these data are arranged as columns of matrices X and Y as follows:

(1)
X=[x(t1)x(t2)x(tm)]Rn×mY=[x(t2)x(t3)x(tm+1)]Rn×m

Then, the relationship between the snapshots can be considered linearly, as follows

(2)
X=AY

The eigenvalues and modes of DMD are defined as the eigenvectors of A. The reduced SVD of X is performed, letting X be denoted as:

(3)
X=UΣVT

Then let

(4)
A~=UTAU=UTYVΣ1Rr×r

Solve the eigenvalues λi and eigenvectors υ~i of with A~υ~j=μjυ~j. The λi is the eigenvalue of DMD

Then, the DMD mode υi is given by the following:

(5)
υi=λi1YV1υ~i

If we need to rebuild the flow, the initial variant b needs to be calculated through the following equation:

(6)
b=x(t1)υ1

where x(t1) is the unsteady flow field at the first snapshot. The DMD mode and time eigenvalues are used to rebuild the unsteady flow field as follows:

(7)
Ux,k=i=1mbiλikυi

where λi is the eigenvalue of matrix A, and the matrix λik can be written in Vandermonde matrix form as follows:

(8)
λik=[1λ11λ1k11λ21λ2k11λm1λmk1]

Vortex identification method

To study the vortex structures of the TLF, the VR Helicity (Tang and Liu, 2022) and LTcri (Liu and Tang, 2019) methods are utilized. The VR helicity can extract the vortex with a nonzero vorticity component in its rotational axis. The rotational axis of the local vortex is considered to be aligned with the VR direction. The VR helicity density is a strong candidate and Galilean invariance can be guaranteed.

(9)
u=VΛV1u=[vr,vcr,vci][λr000λcrλci0λciλcr][vr,vcr,vci]1
(10)
HvR={ωvrλr00λr=0

The local trace criterion (LTcri) with the LTcri-based elliptical region (LTER) is another method to identify the vortex. The magnitude of LTcri is defined as the value of the first invariant of the tensor. The LTcri is expressed as follows:

(11)
LTcri=12λr2λcr2+λci2

Furthermore, a projection plane with a divided elliptical region is constructed with LTcri. The projection plane of LTcri (the LT-plane) is also designated as a positive-delta space. The abscissa axis of the LT-plane are defined as ξ=λr/|λci|, and the ordinate axis is defined as η=λcr/|λci|. Figure 3 shows the elliptical region that is defined by LTcri>0 in the LT plane. The elliptical region is divided into six parts, each region represent a different combination of compressibility and swirling pattern. Parts 1, 2, and 3 represent the expansion pattern, and Parts 4, 5, and 6 represent the compression pattern.

Figure 3.

Elliptical Region Characterized by LTcri in LT-plane (Liu and Tang, 2019).

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Flow structure of tip leakage flow

3D vortical flow structures identified by the LTcri and the VR helicity are displayed in Figure 4a and b. The primary tip leakage vortex structures are effectively identified via the two methods. In the graphic of LTcri shown in Figure 4a, the threshold is set with an absolute value of 5 × 10−6 s−2. The primary tip leakage vortex is first generated due to the jet from the tip leakage, and then the secondary tip leakage vortex forms in the developing stage of the primary tip leakage vortex. After, the vortex breaks down into small-scale vortices and mixes with the main flow.

Figure 4.

Vortex Structure Under an Instantaneous Flow Field at the Near-Stall Condition. (a) Isosurface of LTcri = 5 × 106 (s−2) and (b) Isosurface of VR helicity = ±5,000 (s−1).

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In the graphic of the VR helicity method shown in Figure 4b, the threshold has an absolute value of 5,000 s−1. The isosurface colored in blue represents the negative values, and the isosurface colored in red represents the positive values for the helicity methods. The primary tip leakage vortex corresponds to negative values, and the second vortex corresponds to positive values due to the relative movement of the casing. Strong shear in the blade tip region induces a different rotation direction between the primary and second vortex. Furthermore, the normalized helicity methods can extract both strong and weak vortices.

To further study the unsteady motion of the TLF. A streakline and four pathlines, which are selected to represent typical flow particles in the TLF, are drawn in Figure 5a and b, respectively. The streakline and pathline are extracted by recording the path of fluid particles being released at a series of instantaneous times for a specific period (David and Robert, 1995; Hou et al., 2022). Based on the streakline, the primary TLV behaves as an oscillation in a limited range as it is just generated. Downstream, a helical roll-up occurs, and then the TLV suddenly breaks down. At the same time, flow particles disperse in a much larger region than the primary vortex. Figure 5b displays four pathlines passing through the tip leakage vortex, and the axial velocity colors the pathline. Pathline-1 and pathline-2 represent the particles that pass through the primitive TLV and are kept in the original passage. Pathline-3 and pathline-4 represent the particles passing through the primitive TLV and then enter the adjacent passage. Here, pathline-2 is selected for further analysis in Section 4 because it represents the motion of most particles within the TLF at the tip region.

Figure 5.

Streakline and Pathlines of the TLF Under the Near Stall Condition. (a) Streaklines (released at the TLV core) and (b) Four typical pathlines of TLV.

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Based on the analysis of the vortex structure and the streamlines, the evolution of the TLV can be divided into three phases (Hou et al., 2022) as shown in Figure 5b. The first phase is the formation or generation phase of the primary TLV, and the second phase is the development of TLV. The breakdown of the primary vortex occurs at the end of the development phase. The third phase is the dissipation process, where the TLF is mixed with the primary passage flow. From the above analysis, the vortex identification method and the streakline can provide much information on a predetermined instantaneous period. However, they cannot extract the spatial-temporal coherent structure for an extended period. As a comparison, the DMD algorithm can deal with the gathered flow field both in space and time, which is crucial to describe the detailed unsteady motion of the TLF.

DMD analysis

This section analyses the 3-dimensional unsteady flow field of this rotor based on the DMD for two single variables at the near stall condition. The time-space matrix for the variable of static pressure P, and the time-space matrix of the radial velocity Wr are conducted DMD separately, and then the mode characteristic and mode shapes are listed and compared.

Overview of DMD characteristics of the TLF

A partial computational domain that contains the tip region is used to reduce the memory requirements, and the location is shown in Figure 6. The total grid number of the computational domain is 3.81 million. In the calculation of DMD, 1,500 snapshots are used, the time interval between two snapshots is 3×105s, and the whole time is approximately 15.3TBP(TBP=2.94×104s).

Figure 6.

Computational Domain of the DMD.

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DMD modes in this work are sorted in positive order based on their frequency. This means that the mode with the lowest frequency is marked as mode 1 (the stationary mode), and mode 1 corresponds to the time-averaged flow field in this case. The mode appears in conjugate mode pairs, which share the same altitude and the opposite real value. Mode energy is also calculated to measure the amplitude of the fluctuation corresponding to this mode, which is defined as the time average of the square of each component, as follows:

(12)
Me¯=i=1nj=1mu2(xi,tj)/m

where n is the total number of discrete grid points m is the total time snapshot of the dataset, in this work, n is 3.81 million and m is 1,500. Details of the dataset parameters of DMD are shown in Table 2.

Table 2.

Dataset parameters of the DMD analysis.

CaseVariableGrid numberTotal snapshotsTime interval (TINT)TS/TBP
1P(pa)3.81×1061,5003×105s15.3
2wr(m/s)3.81×1061,5003×105s15.3

Figure 7a shows the diagram of the mode frequency and mode energy of static pressure, the abscissa represents the mode frequency (normalized by the blade passaging frequency, BPF), and the ordinate represents mode energy. Table 3 lists the details of the mode parameters. The mode with 0.57 BPF has the largest mode energy for static pressure, which accounts for 18.1% in total, and the following are modes with frequencies equal to 0.91 BPF and 3.54 BPF. For the radial velocity Wr, the mode with the highest energy corresponds to a frequency of 2.26 BPF, followed by modes with 1.35 BPF and 0.35 BPF.

Figure 7.

Mode Characteristics of the Static Pressure and Radial Velocity. (a) Frequency-energy diagram of static pressure P and (b) Frequency-energy diagram of the radial velocity Wr.

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Table 3.

Mode parameters.

DMD ModeFrequency (BPF)Energy proportion
p13/140.254.0%
17/180.5718.1%
27/280.916.3%
103/1043.546.2%
Wr10/110.3510.3%
26/270.857.7%
42/431.3518.6%
70/712.2647%

Figure 8a–c show the isosurface of three typical modes shape of the static pressure P (the value rebuilt by the selected mode at an instantaneous). Mode 2 is located at the suction of the mid-span near the surface at the tip region. Mode 13 is located around the trajectory of the primary tip leakage vortex and the pressure surface of the adjacent rotor. Mode 27 is located around the blockage cell near the pressure surface. The frequencies of mode 2, mode 13, and mode 27 are 0.1 BPF, 0.57 BPF, and 0.91 BPF, respectively. Based on the mode shape and location, it indicates that mode 2 corresponds to the pressure fluctuation around the suction surface. Mode 13 corresponds to the fluctuation caused by the oscillation of the primary TLV. Mode 27 corresponds to the fluctuation of the TLV and the interaction between TLF and the pressure surface. Figure 9a–c show the isosurfaces of mode 10, mode 26, and mode 43 of the radial velocity Wr. Based on the locations and mode shape, it indicates that mode 12 reflects the motion of the primary TLV, while mode 26 and mode 70 reflect the fluctuation structures at the dissipation phase of the TLF.

Figure 8.

Mode Shape of the Static Pressure P (Pa). (a) Mode 2 (0.1 BPF) isosurface of P2=±20, (b) Mode 13 (0.57 BPF) isosurface of P13=±300, and (c) Mode 27 (0.91 BPF) isosurface of P27=±100.

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Figure 9.

Mode Shape of the Radial Velocity Wr (m/s). (a) Mode 12 (0.35 BPF) isosurface of Wr12=±20, (b) Mode 26 (0.85 BPF) isosurface of Wr26=±10, and (c) Mode 70 (2.26 BPF) isosurface of Wr70=±30.

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Figure 10a–c show the distribution of mode 13 of the static pressure P at 95% span and a meridian surface. At a 95% span, the area with high amplitude is located approximately around the trajectory of the primary TLV. This indicates that the unsteady motion at the generation phase of the TLV oscillates in the tangential direction. Figure 10b and d show the distribution of mode 26 Wr (radial speed in the relative frame of the rotor) at 90% span and a meridian surface. This mode is primarily located near the block cell induced by the TLF, and a negative and positive value appears alternately in the axial direction near the pressure suction surface of the blade. The volume of this mode increases downstream, indicating that the unsteady blockage cell extends its size when transported downstream.

Figure 10.

Two-Dimensional Distribution of the DMD Modes. (a) Mode 13 of P(pa) at 95% span, (b) Mode 26 of Wr (m/s) at 90% span, (c) Mode 13 of P (pa) at a meridional surface, and (d) Mode 26 of Wr (m/s) at a meridional surface.

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Mode analysis along the pathline

The mode shapes shown above indicate that the TLF is composed of unsteady flow structures with different temporal-spatial scales. The time-space diagram Wr along pathline-2 (shown in Figure 5) is drawn in different phases of the TLF. Figure 11a shows the location of the sampled pathline. Figure 11b and c show the time-space diagram of the original signal and rebuilt signal using the first 100 modes. The abscissa of this diagram is the time, and the coordinate is the non-dimensional axial location. The comparison shows that the signal can be effectively rebuilt using only the first 100 modes at the start of the trajectory. However, as the TLF transports downstream, some high-frequency signals occur. Figure 11d and e display two primary mode signals with frequencies of 0.35 BPF and 0.85 BPF, accounting for most of the total signal. The space-time diagram shown in Figure 11 shows that the oscillating frequency is approximately 0.35 BPF at the start along the vortex core, and then this signal decreases, while the signal with 0.85 BPF suddenly increases.

Figure 11.

Time-space Diagram of Wr (m/s) along the Vortex Core at the Generation Phase. (a) Sampling line, (b) Original Wr, (c) Wr rebuilt from 1 to 100 modes, (d) Wr rebuilt by Mode 10 (0.35 BPF) and (e) Wr rebuilt by mode 33 (1.04 BPF).

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Then, the time-space diagram of the original and rebuilt signal at the development phase of the line is displayed in Figure 12b and c, and the location of the development phase in the streamline is shown in Figure 12a. At this phase, the primary TLV interacts with other flow structures, such as the vortex rope (Hou et al, 2022), and it finally breaks down into vortices with smaller scales. Figure 12c and d show two primary modes rebuilt by modes 13 and 27. This indicates that the frequency of the primary mode is much higher than that of the generation stage, which is approximately 1.35 BPF and 2.26 BPF, respectively.

Figure 12.

Time-space Diagram of Wr (m/s) along the Vortex Vore at the Development Phase. (a) Sampling line, (b) Original Wr, (c) Rebuilt Wr from 1 to 100 modes, (d) Rebuilt Wr by Mode 42 (1.35 BPF), and (e) Wr rebuilt by mode 70 (2.26 BPF).

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Figure 13b and c show the original and rebuilt spatial-temporal signal Wr from the 70% chord at pathline-2, and the location of the dissipation phase is shown in Figure 13a. The periodicity of the signal at this phase is also significant. Figure 13c and d show two of the primary DMD modes with a frequency of 0.45 BPF and 1.49 BPF. It indicates that the signal with the lower frequency component increases amplitude as the particle moves downstream.

Figure 13.

Time-Space Diagram of Wr Along the Vortex Core at the Dissipation Phase. (a) Sampling line, (b) Original Wr, (c) Rebuilt Wr from 1 to 100 modes, (d), Rebuilt Wr by mode 12(0.35 BPF), and (e) Rebuilt Wr by mode 26(0.85 BPF).

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The above analysis indicates that the TLV has three typical unsteady characteristics at its generation, development, and dissipation phases. In the generation phase, the primary TLV has an oscillation motion with a frequency of about 0.35 BPF. Then at the development phase, some small-scale flow structures are generated due to the breakdown of the primary TLV, and the periodicity of the fluctuation is weakened. Finally, the periodicity of the fluctuation is rebuilt in the dissipation phase, with a frequency of approximately 0.85 BPF.

Effect of the DMD mode on the vortex structure and loss generation

This section studies the effect of the DMD mode on the formation of vortex structures and loss generation. The flow field is rebuilt using different numbers of the DMD mode, and then the LTcri method is used to identify the vortex structure. In addition, the unsteady loss is also analyzed based on the entropy production rate.

To recover the entire velocity vector flow field, DMD is conducted on the variable matrix X, which is defined as follows:

(13)
X=[Wxt1Wyt1Wzt1Wxt2Wyt2Wzt2WxtmWytmWztm]

where Wxti, Wxt1, and Wxt1 are the velocity components in three directions of the entire flow field at an instant. Five hundred snapshots are used to build the spatial-temporal matrix X, and the space domain is kept the same as shown in Figure 6. The DMD mode is also ranked ascending by frequency in this section. It should be noted that the mode characteristics are different from those in Section 4 since their input dataset matrix is different.

Effect of modes on the vortex structure

Based on the results shown in Section 4, the motion of vortices with TLF is unsteady, especially at the development and dissipation phases. On the other hand, the unsteady flow field can be rebuilt by different modes corresponding to different spatial-temporal flow structures. Figure 14 shows the isosurface of LTcri with the threshold equal to 8×106s2, and the isosurface is colored by the number of quadrants in LTER. Figure 14a–d shows the vortex structures rebuilt using mode 1, modes from 1 to 3, 1 to 6, and 1 to 100, respectively. The isosurface of LTcri in the original unsteady flow field is also shown in Figure 14e. It should be noticed that the mode 1 is the stationary mode corresponding to the time average flow field with a zero-decay rate. The comparison indicates that the primary TLV at the generation phase is effectively recovered by the stationary mode, while the small-scale unsteady vortex structure, including part of the second tip leakage vortex (S-TLV), is filtered. If mode 3 and mode 5 are used, the S-TLV can be recovered. A comparison between the vortex structure rebuilt using different modes also shows that the interaction between the primary TLV and vortex rope is an unsteady process, it cannot be recovered by the stationary component. In addition, more small-scale vortices appear at the development and dissipation phases. Figure 14e shows that the entire vortex structure can be recovered if all modes were used to rebuild the flow field.

Figure 14.

Vortex Structures at an Instantaneous Flow Field. (a) Rebuilt by mode 1, (b) Rebuilt from mode 1 to mode 3, (c) Rebuilt from mode 1 to mode 6, (d) Rebuilt from mode 1 to mode 100, and (e) Original unsteady flow field.

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Based on the LTER indication, vortices with different vortical flow patterns can be distinguished. Figure 14a shows the time-averaged TLV is in the expansion state as it just generates, and then the TLV turns into the compression state at approximately 10% chord downstream. As the mode number used to rebuild the flow field increases to three, vortices in the compression state occur at the end of the primary TLV. Those small-scale unsteady vortices recovered by mode 3 to mode 6, primarily located in the vortex interaction and breakdown regions, are in the expansion state.

Effect of modes on the entropy production

Vortex flow can produce irreversible viscosity loss and, therefore, has a large effect on the efficiency of the rotor. The loss induced by viscosity can be quantitated by the viscosity entropy production rate (Moore and Moore, 1983), which is defined as follows:

(14)
S˙visc=2μs¯ijs¯ijT¯+2μsijsijT¯

where μ represents the molecular viscosity ecoefficiency, s¯ij represents the time average strain ratio, sij represents the instantaneous fluctuation of the strain ratio, and T¯ is the time-averaged temperature (288.15 K used in this case). Equation (13) shows that the viscosity loss is composed of time-averaged and instantaneous components. Therefore, the entropy production is highly correlated to the unsteady vortex structure through the instantaneous item. Figure 15a and b show the S˙visc at an instantaneous and time-averaged flow field. The time-averaged S˙visc is consistent with the total S˙visc at the generation phase of the TLV, indicating that the entropy production is mainly composed of its steady component before the primary TLV breakdown. In addition, the area with a high entropy production rate is located at the edge of the primary TLV. Figure 15c and d display the S˙visc obtained by DMD mode 2 and mode 4. The area with high S˙visc in mode 2 is located at the center region of the TLF at the dissipation phase. As a comparison, mode 4 is near the hub of the dissipation phase. The loss produced by mode 4 is also smaller than that produced by mode 2 in amplitude.

Figure 15.

Energy Production at an Instantaneous Flow Field. (a) S˙visc at an instantaneous flow field, (b) Time-averaged S˙visc, (c) S˙visc in the flow field rebuilt by mode 2/3 (d), and S˙visc in the flow field rebuilt by mode 3/4.

https://journal.gpps.global/f/fulltexts/191168/JGPPS-00204-2023-01.15_min.jpg

Conclusion

This work investigates the unsteady tip leakage flow of a rotor under the near-stall condition. First, DMD is used for the 3D flow field calculated via DDES to extract the spatial-temporal structures. Next, the unsteady characteristics are analyzed based on the different modes. Finally, the effect of flow unsteadiness on the vortex structure and loss generation is analyzed. The conclusions of this work can be drawn as follows.

  1. In the generation phase of the TLV, the unsteadiness behaves as the oscillation of the primary TLV. In the development phase of TLV, the unsteadiness of TLV behaves as the interaction between the primary TLV and other vortex structures. In the dispassion phase, TLV finally breaks down into small-scale unsteady vortices.

  2. Unsteady motions of the tip leakage vortex can be reflected by the different DMD modes. The unsteady fluctuation of the vortex rope has a relatively lower frequency, and it is reflected by the first 2 modes. The unsteady motion of the main TLV has the highest fluctuation amplitude and corresponds to pressure mode 13. DMD can also provide information about the frequency and amplitude of different unsteady motions.

  3. Vortex structures and loss generations can be divided into steady and different unsteady components through DMD. In the generation phase, entropy production is primarily composed of its steady component. Conversely, vortex structure and loss generation are mainly composed of unsteady components after the primary TLV breakdown.

The mode information provided by DMD facilitates a novel view to describe the motion of the TLF. The dynamic characteristics are also valuable for the development of data-driven modeling or flow control methods for the TLF.

Nomenclature

BPF

blade passing frequency

TBP

blade passing time

TLF

tip leakage flow

TLV

tip leakage vortex

W

relative velocity

S˙

entropy production

f

frequency

vi, vj, vk

velocity components for the spatial point

u

velocity fluctuation

μ

molecular viscosity [kg/(m·s)]

ω

vorticity vector

sij

strain rate tensor

vci

eigenvector of u according to λci

vcr

eigenvector of u according to λcr

vr

eigenvector of u according to λr

r

radial direction

z

axial direction

t

tangential direction

Greek symbols

λci

the imaginary part of the complex eigenvalue of u

λcr

the real part of the complex eigenvalue of u

λr

the real eigenvalue of u when >0

Ω

vorticity tensor

Δ

discriminant of the velocity gradient tensor