4.1.1. Wake and Potential Disturbances
It is well known that the upstream IGV induces wake and potential field, which propagate axially and excite the downstream rotor blade at the same frequency. To clear the dominant excitation source of the rotor blade, it is necessary to evaluate the effect of the wake and potential field on the rotor blade, which also helps to reveal the formation process of IGV–R1 interactions. Hence, the axial propagation characteristic and the strength of the wake and potential field were analyzed in this section.
To accurately simulate the IGV disturbances and characterize their interactions with the rotor blade, the computational results for the IGV/R1 coupled configuration (Case B) were analyzed. The instantaneous entropy and static pressure contours, which can well characterize the wake and potential disturbances in the flow field, showing the wake–rotor and potential field–rotor interactions at 30% span, are plotted in
Figure 6a,b respectively. The results show that the IGV wake propagates downstream and its strength weakens significantly due to blade chops when reaching the LE of the rotor blade. In terms of the IGV potential field,
Figure 6b shows that it propagates upstream and downstream and its strength decays rapidly in the axial direction. Meanwhile, the dense and non-uniform distribution of contour lines near the R1 LE indicates strong IGV–R1 interactions (
Figure 6b).
For the axial propagation characteristics of the wake and potential disturbances, the above results only give qualitative evaluations, and further quantitative analyses were needed to evaluate and compare their effects on the rotor blade. Therefore, discrete Fourier transform (DFT) of the circumferential symmetric total pressure and static pressure was carried out, and the amplitude of the first-harmonic content of the IGV wake and potential disturbances with an aerodynamic wave number of 19 (19AWN) were analyzed [
31].
Figure 7 shows the axial distribution of the 19AWN amplitude, from the trailing edge (TE) of IGV to a plane mid-distance between IGV TE and IGV exit at 30% span. The reason for analyzing the midplane is that its axial location, marked as a blue dotted line in
Figure 1, is less affected by IGV–R1 interactions than the IGV exit (shown in
Figure 6b). The results show that the strength of the wake (total pressure line) decreases slowly at a certain distance away from the IGV TE and the amplitude decreases by 0.5% per 0.001m, while the potential disturbance (static pressure line) decays exponentially and the attenuation coefficient is 88% per 0.001 m. By comparing the amplitude of the total pressure and static pressure at the midplane, it indicates that the strength of the wake is three times larger than that of the potential field. It is worth noting that there is still a 0.029 m axial distance between the midplane and R1 LE, and it can be inferred that the strength of the potential field will decrease to 4.3% of the midplane, while the wake will only decrease by about 15%. Therefore, it can be concluded that IGV disturbances are dominated by the upstream wake and may significantly contribute to the vibration amplitude of the rotor blade, which will be studied below.
4.1.2. IGV–R1 Interactions
For the IGV–R1 configuration, the rotor blade may be excited not only by the upstream IGV wake but also by the spinning modes resulting from IGV–R1 interactions.
Figure 8 shows the spectrum of IGV–R1 interaction modes, which was calculated by the DFT of the circumferential instantaneous static pressure at 30% span at the IGV exit. The result shows that the compressor pressure field can be very complex due to the presence of multiple significant frequency peaks associated with the IGV–R1 interactions in the mode spectrum. Thanks to Tyler and Sofrin [
12], the source of IGV–R1 interactions can be identified based on the spinning mode theory [
13].
In general, when the rotor blades pass through the IGV wakes, the circumferential non-uniform flow causes unsteady loads on the blades and generates the primary discrete pressure wave, which has the same AWN and frequency as the IGV wakes [
33]. According to the spinning mode theory, the scattering occurs at the rotor row and the discrete pressure wave is scattered to an infinite number of continuous pressure waves. These scattered waves have the same frequency as the IGV wakes in the relative frame (
), while their AWNs become the combination of IGV and R1 blade numbers (
), where subscript 1 and subscript 2 denote the quantities for the stator row (stationary frame) and the rotor row (relative frame), respectively;
represents the blade number,
refers to the integer scattering indices, and
is the rotational speed. The negative sign represents a backward traveling pressure wave in the opposite direction of the rotor, whereas the positive sign presents a forward traveling pressure wave.
The scattered pressure waves travel upstream and downstream and some of them reach the IGV row. Their frequencies are shifted in the stationary frame due to the Doppler effect (), whereas the aerodynamic wave numbers do not change (). The pressure waves subsequently impinge the IGV and are being scattered and shifted again, possibly reflecting back and interacting with the rotor blades. The frequency and AWN of reflected pressure waves are the same as the IGV wakes.
According to the formation process of IGV–R1 interactions described above, the spinning modes at the IGV exit are mainly upstream propagating pressure waves generated from the R1 row. Therefore, the source of spinning modes can be identified with different scattering indices (
), and their frequencies in the relative frame and stationary frame are
and
respectively. The properties of spinning modes in
Figure 8 are listed in
Table 5.
The spinning modes listed above have 0 frequency and the first three harmonics of IGV blade passing frequency (BPF, namely 19EO) in the relative frame. However, for R1 blade vibrations, excited by the first harmonic of the upstream IGV, only the 19EO frequency contributes to the excitation of blade vibration. Hence, modes ,, and are the pressure waves of interest, and they can be characterized by of −1. Among them, modes and correspond to the first and second R1-scattered pressure waves, respectively, and the mode is the primary pressure wave due to the IGV wake. To clear the dominant excitation source of the rotor blade, the acoustic property (cut-on/cut-off) and the strength of these modes were analyzed.
A wave equation in cylindrical coordinated was solved to obtain the axial wavenumber
, which determines the cut-on/cut-off of an acoustic mode, written as [
34]:
where
and
are mean axial and circumferential Mach numbers, respectively;
is the freestream wave number calculated by the freestream speed of sound
and the angular frequency in the stationary frame;
represents the radial-circumferential wave number calculated by the Bessel function. According to the
, the acoustic cut-on frequency
is defined by:
The last column of
Table 5 shows the acoustic property of the spinning modes of interest. Modes
and
are cut-on upstream, which demonstrates that they propagate in the axial direction without any attenuation, can impinge on the IGV, and may reflect back, and interact with the rotor blades. In terms of the mode
, it is cut off upstream and decays exponentially, and thus has little effect on the rotor blades. To compare the strength of modes
and
, the fluctuation amplitude normalized by the strength of the R1 wake at 99% span is shown in the second column of
Table 5. The results show that the amplitude of the mode
is approximately nine times larger than that of the mode
. Hence, it can be concluded that the IGV–R1 interactions are dominated by the mode
, which is generated by the interaction between the first harmonic of IGV and the first harmonic of R1, and its dominance is related to the close blade number of IGV and R1.
4.1.3. Contribution of Upstream Disturbances to Blade Vibration Amplitude
The above analyses have clarified the dominant IGV disturbances and the IGV–R1 interactions. However, since the rotor blade was excited by them at the same frequency, their contributions to the blade vibration cannot be distinguished. Hence, in this section, the calculation results of the decoupled (Case A-1 and Case A-2) and coupled (Case B and Case C) configurations were compared to reveal the dominant excitation source of the blade vibration.
Before comparing the results for different cases, it is critical to ensure that the working conditions of the rotor blade are the same. The deviation of mass flow rate, total pressure ratio, and adiabatic efficiency among the four cases were less than 0.2%. Meanwhile, the time-averaged pressure of the rotor blade at 30% span was compared, and the results show that the blade loading of the decoupled and coupled cases is the same, as presented in
Figure 9. Therefore, it is reasonable to compare the blade vibration amplitude among different cases; the results are shown in
Table 6.
For the rotor blades subjected to 19EO excitation arising from the IGV wake and IGV–R1 interactions (mode
), no matter which is dominant, the response will occur in BM6/4ND. This is because the aerodynamic wave number of the former is 19, which is higher than the half number of rotor blades (23), thus the 4ND response is excited through the spatial aliasing, while the mode
will excite the 4ND response directly. Hence, the amplitude of the BM6/4ND modal force was computed, and the maximum vibration amplitude in
Table 6 was calculated using Equation (8).
The response of all cases was normalized by the vibration amplitude of Case C, the response of Case B was only 1% less than Case C, indicating that the downstream S1 has little influence on the BM6/4ND response of the rotor blade, and the two-row coupled configuration (IGV/R1) can accurately predict the blade vibration amplitude. In terms of Case A-1 and Case A-2, the vibration amplitude predicted by the former was 21% less than Case B, whereas the latter was only 4%. To explain the difference between the results of the two decoupled configurations, the radial distribution of the fluctuating amplitude of entropy (19AWN) at the IGV exit was computed to compare the wake strength of different cases, as plotted in
Figure 10. Consistent with the results reported in the literature, the wake strength of Case A-1 is lower than that of Case B or Case C in all spans because of the use of the mixing plane. Hence, the 21% difference in blade response is not only the contribution of IGV–R1 interactions but also due to the underestimation of the wake forcing function. With respect to Case A-2, the wake strength is more similar to that of Case B, being higher only at low spans, and this difference does not have a large impact on the blade vibration amplitude because the BM6 mode shape near this region is small (shown in
Figure 2). Therefore, the 4% difference is considered to be mainly contributed by the IGV–R1 interactions. According to the above analyses, the dominant excitation source of the R1 blade vibration induced by upstream aerodynamic disturbances is the IGV wake, and the decoupled method is still applicable in this case.