Haiping Li^{1} , Jianmin Zhao^{2} , Wenyuan Song^{3} , Hongzhi Teng^{4}
^{1, 2, 3, 4}Mechanical Engineering College, Shijiazhuang, 050003, China
^{4}Lanzhou Maintenance Centre, Lanzhou, 730060, China
^{1}Corresponding author
Journal of Vibroengineering, Vol. 17, Issue 2, 2015, p. 705719.
Received 24 December 2014; received in revised form 30 January 2015; accepted 11 February 2015; published 31 March 2015
Copyright © 2015 JVE International Ltd.
Planetary gearbox is increasingly used in many kinds of rotary machinery in recent years. Due to the specialty of its structure, fault diagnosis for planetary gearbox is very difficult compared with the fixed shaft gearbox. This paper proposed an offline fault diagnosis method for planetary gearbox based on empirical mode decomposition and adaptive multiscale morphological gradient filter. Firstly, the framework of the method proposed in this paper was introduced. Then, experimental data and industrial data were utilized to validate the effectiveness of the method. And the combination of empirical mode decomposition and adaptive multiscale morphological dilationerosion gradient filter was found very suitable to be used in the planetary gearbox fault diagnosis compared with other five filters. The proposed method was demonstrated to be of good performance on both extracting faults characteristic frequency and denoising.
Keywords: planetary gearbox, fault diagnosis, empirical mode decomposition, mathematical morphology, morphological gradient filter.
Planetary gearbox plays an important role in large and complicated mechanical equipments, such as wind turbine, helicopter and crane, etc. And the working environment of these equipments is often very terrible. The main components of single stage planetary gearbox usually consist of one sun gear, one ring gear, one planet carrier and three or four planet gears. The structure of planetary gearbox is compact relatively, so it can achieve larger transmission ratio compared with fixed shaft gearbox. However, the terrible environment and the special structure also make it very difficult to assess the health condition of the planetary gearbox [1]. Therefore, efficient and accurate fault diagnosis methods for planetary gearbox are particularly needed to prevent the equipments from failure.
The fault diagnosis methods for planetary gearbox can be divided into two types, online and offline. The online method is implementing condition monitoring on machinery through some instruments. It is often an automatic method due to the instruments can give out the indicator whether the machine can run continually or not. The offline method is analyzing the data acquire from the equipments to assess the health condition of the planetary gearbox. It is usually an artificial method. In the general, the two kinds of methods can be utilized together to improve the performance of fault diagnosis.
The procedure of the online and a part of intelligent offline fault diagnosis methods is made up by data acquisition, data processing, features extraction and fault diagnosis. In this aspect, major efforts have been made by many researchers and organizations. Feng and Zuo et al [24] developed a series of experiments using a twostage planetary gearbox testrig with considering different fault modes, fault levels and working conditions. They acquired a great deal of vibration data. Some documents [57] introduced the common fault features in detail, such as maximum, minimum, kurtosis and energy, etc. In addition, the data processing techniques that utilized to extract the features were also explained by them. A variety of intelligent fault diagnosis methods have been proposed, such as Support Vector Machine (SVM) [8, 9], Wavelet Packet Transformation (WPT) [10, 11] and Hidden Markov Model (HMM) [1214]. Empirical Mode Decomposition (EMD) [1518], as the kernel of HilbertHuang Transform (HHT), was popular in recent years due to its good performance on signal processing and mechanical fault diagnosis.
Anyway, the intelligent methods are often limited in a settled condition and would not work to all cases. Therefore, artificial methods are needed to cooperate with the intelligent ones. Frequency spectrum analysis [19] is one of the most useful means and it is based on the amplitude changing of fault characteristic frequency. In recent years, some researchers introduced mathematical morphology (MM) [2023] to fault diagnosis field. Fault frequencies of gears can be extracted more explicit using mathematical morphological filters than traditional frequency analysis method. However, the structure of planetary gearbox is very complicate and many different feature frequencies can be depicted in its frequency spectrum. The amplitudes of ring gear and planet gears fault frequencies are very low. In addition, noise interference is very serious because of the awful working condition. So, it is still a challenge to assess the health condition of planetary gearbox.
In this study, an offline fault diagnosis method for planetary gearbox based on EMD and adaptive multiscale morphological gradient filter (AMMGF) is presented. Due to the minor changes of fault frequencies will be very obvious after processed by EMD and researches have demonstrated better result can be obtained when utilized EMD. In addition, AMMGF is the most effective filter than other morphological filters.
The remaining sections of this paper are organized as follows. Section 2 introduces the proposed planetary gearbox fault diagnosis method in details. Section 3 and Section 4 validates the effectiveness of the proposed method using experimental data and industrial data, respectively. Finally, the conclusions were drawn in Section 5.
EMD is a popular method and its fundamental theory can be found in documents [1517]. Thus, the theory of EMD will be not introduced in details and only the specific application will be illustrated in this paper.
Mathematical morphology (MM) was originally put forward by Matheron and Serra as an image processing method in 1964. In recent years, it was applied in fault diagnosis field as a vibration signal processing technique and even embedded in some software. For example, there are readymade program of MM in MATLAB. The application of it in fault diagnosis field is to modify the shape of a signal by predefined structuring element so that to achieve the aim of extracting faults characteristic frequency and denoising. Generally, two kinds of basic algorithms are defined by MM: dilation and erosion, as follows.
Assume that $A$ is an image and $B$ is the structuring element, then $B$ dilates or erodes $A$ can be defined as $A\oplus B$ and $A\odot B$, respectively:
where ${A}_{b}$ and ${A}_{b}$ are defined as:
The processed results of dilation and erosion can be illustrated visually by Fig. 1. As the figure shows, when the structuring element moves by the outside of an image, the area encircled by the center of the structuring element is the dilated result. Similarly, when the structuring element moves by the inside of an image, the area encircled by the center of the structuring element is the eroded result. The two results can be illustrated more visually by Fig. 2.
Fig. 1. The processed results of dilation and erosion
Fig. 2. Dilation and erosion of image: a) original image; b) dilation of a); c) erosion of a)
a)
b)
c)
In general, as the fundamental algorithms of MM, the processed results of dilation and erosion cannot be recovered. Namely, the original image cannot be obtained through dilation and then erosion or the contrary order. However, the two orders are another two important algorithms of MM, opening and closing, and they can be denoted as $A\circ B$ and $A\u2022B$:
Fig. 3. The processed results of opening and closing
Fig. 4. Opening and closing of image: a) original image; b) opening of a); c) closing of a)
a)
b)
c)
Similarly, the processed results of opening and closing can be illustrated by Fig. 3. It can be seen from the figure that opening and closing have the function of smooth edge and fill leak, respectively. The two results can be illustrated more visually by Fig. 4.
Section 2.1 introduced the fundamental theory of MM and its application on image processing. In recent years, mathematical morphological filters (MMFs) which mainly constituted by dilation, erosion, opening and closing were applied in fault diagnosis field.
Assume that $f\left(n\right)$, $F=\{0,1,2,\dots ,N1\}$ and $g\left(m\right)$, $G=\{0,1,2,\dots ,M1\}$$(N\gg M)$ are input signal and structuring element, respectively. Then four basic MMFs can be defined as:
where $\oplus $, $\odot $, $\circ $ and $\u2022$ mean dilation, erosion, opening and closing filter, respectively.
The functions of the four basic MMFs are different though all of them can extract the faults characteristic frequency from vibration signal. Fig. 5 shows the differences of them. The analyzed signal is a standard sine signal $x=\mathrm{s}\mathrm{i}\mathrm{n}2\pi t$ and the sampling frequency is 100 Hz. As the figure shows, dilation filter can control the plus pulse and sharp the minus pulse but erosion filter is just the reverse. Opening filter can eliminate the plus pulse and keep the minus pulse but closing filter is the reverse.
Fig. 5. Results of the four basic MMFs (   Original signal, — Results of the four basic MMFs)
a) Result of dilation filter
b) Result of erosion filter
c) Result of opening filter
d) Result of closing filter
As described above, each of the four MMFs could only extract one of the plus or minus pulse information from vibration signal. However, the general condition in practical is that plus and minus pulse are needed at the same time. Therefore, the combination of the two of them were proposed and named morphological gradient filters (MGFs). Two MGFs, morphological dilationerosion gradient filter (MGF_{DE}) and morphological closingopening gradient filter (MGF_{CO}), can be defined as follows:
MGFs can take into account both plus and minus pulse. In addition, they can also extract the wanted faults characteristic frequency and weaken the interference of other signal.
In general, different results will be obtained when selecting different structuring elements. Smallscale structuring element can keep the specific characteristic of pulse signal while bigscale structuring element can weaken the interference of noise signal. Therefore, selecting a suitable structuring element is very important. This paper proposed the adaptive multiscale morphological gradient filter (AMMGF).
Assume that $X$ is dispersed signal, $T$ is morphological transform, and then the AMMGF can be summarized as the set of $\left\{{T}_{\lambda}\left\lambda >0,\lambda \in Z\right.\right\}$. Where ${T}_{\lambda}$ was defined as:
Similarily, assume that $f\left(n\right)\text{,}$$F=\{0,1,2,\dots ,N1\}$ and $g\left(m\right)\text{,}$$G=\{0,1,2,\dots ,M1\}$$(N\gg M)$ are input signal and structuring element, respectively. Then the multiscale morphological dilation and erosion filters can be defined as:
where $\lambda g$ is the structuring element which its scale is $\lambda $. It can be obtained through dilate $g$ by $n1$ times, as follows:
At the same time, the algorithems also can be applied to the followed equations:
The multiscale morphological opening, closing and two gradient filters can be obtained according to the above equations, as follows:
Many multiscale morphological transformed results would be getted through the method described above. Then how to merge them together is another problem. This paper utilized weighting and average method.
Assume that the set of all scales of structuring elements is $\lambda =\left\{{\lambda}_{1},{\lambda}_{2},\dots ,{\lambda}_{J}\right\}$, the obatined $J$ filtered results are $f{g}_{j}\left(n\right)$, $j=1,2,\dots ,\text{}J$, $n=0,1,2,\dots ,N1$. Then the results can be merged using weighting and averaging method, as follows:
where ${w}_{j}={\lambda}_{j}/\sum _{j=1}^{J}{\lambda}_{J}$, $j=1,2,\dots ,J$.
Theoretically, the above AMMGF can both keep the specific characteristic of pulse signal and weaken the interference of noise signal. However, due to the specialty of planetary gearbox, the practical application result was unsatisfactory. Therefore, this paper proposed the fault diagnosis method for planetary gearbox based on EMD and AMMGF. The framework of the method proposed in this paper can be seen in Fig. 6. And the specific procedures can be described as follows.
1. Decomposing the original signal using EMD and getting $I$ IMFs.
2. Processing every IMF using AMMGF and obtaining a lot of processed results with different scales of structuring elements.
3. Merging the processed result of each IMF using weighting and averaging method, getting AMMGF results of $I$ IMFs.
4. Calculating the mean value of the $I$ results as the final signal.
5. Analyzing the frequency spectrum of the final signal and assessing the health condition of planetary gearbox.
Fig. 6. Framework of the method proposed in this paper
The data this example used to validate the effectiveness of the method proposed in this paper was acquired from a seeded failure experiment of planetary gearbox. The experimental system consists of a tested planetary gearbox, a drive motor, a speed and torque sensor and a magnetic powder brake. And between the two of them is connected by coupling, as shown in Fig. 7.
Four accelerometers were mounted on the tested planetary gearbox, wherein the first one and the second one are mounted on the input side of the gearbox, the third one is on the top of the casing and the fourth is fixed on the output side. The specific location of every accelerometer is as depicted in Fig. 8(a). Fig. 8(b) is the structure of the planetary gearbox. And the configuration parameters of the planetary gearbox can be seen in Table 1.
Table 1. Planetary gearbox configuration parameters
Gear

Sun gear

Planet gear (number)

Ring gear

Number of teeth

13

64 (3)

146

Fig. 7. Planetary gearbox experimental system
Fig. 8. a) Mounted location of each accelerometer; b) structure of the tested planetary gearbox
a)
b)
The wear failure is seeded on one tooth of sun gear, planet gear and ring gear, respectively. The specific failures are as Fig. 9 shows. The sampling frequency of this experimental system is 20 kHz, and 240000 points of data are recorded for every signal. The input shaft, shaft 1, was driven by the motor at three kinds of rotary speed, 400, 800 and 1200 rpm. To each speed, four different kinds of loads are implemented. They are 0, 0.4, 0.8 and 1.2 Nm, respectively.
Fig. 9. Seeded wear failure of every gear: a) sun gear; b) planet gear; c) ring gear
a)
b)
c)
According to the configuration parameters of the planetary gearbox, the relevant fault characteristic frequencies can be obtained. The specific values of the frequencies can be seen in Table 2.
Firstly, the sun gear fault signal which acquired from the working condition of 1200 rpm and 1.2 Nm was analyzed to validate the effectiveness of the method proposed in this paper. The fault characteristic frequency of the sun gear in this condition is 55.093 Hz. The vibration signal acquired by Accelerometer 3 was utilized in this example.
Table 2. Fault characteristic frequencies of every gear
Rotary speed (rpm)

Meshing frequency (Hz)

Fault frequency of sun gear (Hz)

Fault frequency of planet gear (Hz)

Fault frequency of ring gear (Hz)

400

79.579

18.364

1.243

1.635

800

159.158

36.729

2.487

3.270

1200

238.738

55.093

3.730

4.906

Fig. 10 shows the waveform in time domain and frequency spectrum of the sun gear fault signal. The 1 and 2 times of sun gear fault characteristic frequency can be seen in the figure, but the amplitudes of them are much lower compared to the disturbed signal’s. Therefore, the health condition of the sun gear cannot be assessed.
Fig. 10. Sun gear fault signal: a) waveform in time domain; b) frequency spectrum
Fig. 11 shows the envelope analysis results of the sun gear fault signal. It can be seen from the figure that the 1, 2 and 3 times of sun gear fault characteristic frequency are very obvious. However, the noise interference is also very serious. The results are obtained based on the seeded wear failure experiment which the damage is a little severe. If the failure is slight or initial in the industrial machine, the result will be not so obvious. Therefore, it is needed to study a more effect method.
Fig. 11. Envelope analysis of sun gear fault signal: a) waveform in time domain; b) frequency spectrum
Figs. 1217 show the results of the six kinds of filters. Figs. 1215 are the results of the four basic filters. They are dilation, erosion, opening and closing. Figs. 1617 are the results of MGF_{DE} and MGF_{CO}. In the six figures, the bold and thin lines in (a) are the results of filters and the waveform in time domain of original signal, respectively.
It can be seen from Figs. 1215 that the results of the four basic filters are similar. All of the four basic filters can extract 1, 2 and 3 times of the sun gear fault characteristic frequency. However, the amplitudes of these frequencies have not increased compared to the envelope analysis result. Even the amplitudes of some results have reduced, such as the results of opening and closing. In addition, the interference come from the low frequency noise is still very serious.
Fig. 12. Sun gear fault signal: a) result of dilation; b) frequency spectrum
Fig. 13. Sun gear fault signal: a) result of erosion; b) frequency spectrum
Fig. 14. Sun gear fault signal: a) result of opening; b) frequency spectrum
Fig. 15. Sun gear fault signal: a) result of closing; b) frequency spectrum
Fig. 16. Sun gear fault signal: a) result of MGF_{DE}; b) frequency spectrum
Fig. 16 and Fig. 17 are the results of MGF_{DE} and MGF_{CO}. Comparing to the results of the four basic filters, the amplitudes of the extracted sun gear fault characteristic frequency have increased obviously. This effect is significant to the frequency spectrum analysis of the signal acquired from the equipment with slight failure.
Fig. 17. Sun gear fault signal: a) result of MGF_{CO}; b) frequency spectrum
It also can be seen from the comparison of Fig. 16 and Fig. 17 that the effect of MGF_{DE} is better than the effect of MGF_{CO} due to the fault characteristic frequency amplitude extracted by MGF_{DE} is higher than by MGF_{CO}. In addition, another conclusion can be drawn from Eqs. (6)(11) that MGF_{DE} needs about half steps compared with MGF_{CO}. Therefore, the after study is mainly implemented based on MGF_{DE}.
Fig. 18 shows the result of AMMGF_{DE}. The 1, 2 and 3 times of the sun gear fault characteristic frequency are extracted obviously. And the amplitudes of them is much higher than the above six results. In addition, the effect of denoising is also satisfactory.
Fig. 18. Sun gear fault signal: a) result of AMMGF_{DE}; b) frequency spectrum
Fig. 19 shows the result of EMD and AMMGF_{DE} which is the method proposed in this paper. It can be seen from the figure that the denoising effect is also satisfactory. More important is that the amplitudes of the extracted sun gear fault characteristic frequencies are much higher than before. In addition, the fault characteristic frequencies of planet and ring gears are very low. So, the proposed method is more suited to planetary gearbox fault diagnosis.
Fig. 19. Sun gear fault signal: a) result of EMD and AMMGF_{DE}; b) frequency spectrum
Fig. 20 and Fig. 21 are the results of EMD and AMMGF_{DE} that applied to planet and ring gears, respectively. In order to achieve the goal of considering all working conditions, the data acquired from 400 rpm and 0.4 Nm condition is utilized when analyzing planet gear signal. And when analyzing ring gear signal, the data acquired from 800 rpm and 0.8 Nm condition is used. The fault characteristic frequencies of the planet gear and ring gear in the two conditions are 1.243 and 3.270 Hz, respectively.
It can be seen from Fig. 20 and Fig. 21 that the proposed method can extract the fault characteristic frequencies of the planet and ring gear obviously even though the frequencies are very low. In addition, the effect of denoising of the proposed method is also satisfactory.
Above discussion demonstrates the offline fault diagnosis method for planetary gearbox proposed in this paper can extract fault characteristic frequencies more prominent compared to the four basic filters (dilation, erosion, opening and closing) and two MGFs (MGF_{DE} and MGF_{CO}). And the denoising effect of the proposed method is also satisfactory. In addition, the performance of EMD and AMMGF_{DE} is the best among all of the filters.
Fig. 20. Planet gear fault signal: a) result of EMD and AMMGF_{DE}; b) frequency spectrum
Fig. 21. Ring gear fault signal: a) result of EMD and AMMGF_{DE}; b) frequency spectrum
In order to further validate the effectiveness of the offline fault diagnosis method for planetary gearbox proposed in this paper, industrial data acquired from a helicopter was analyzed.
Planetary gearbox is a main part of helicopter engine and this is the reason why select the data acquired from helicopter to analyze. Due to the reason of secrecy, the photo of the helicopter and the inside structure of planetary gearbox cannot be showed here. But the configuration parameters of the planetary gearbox can be seen in Table 3.
Table 3. The configuration parameters of the planetary gearbox of a helicopter
Gear

Sun gear

Planet gear (number)

Ring gear

Number of teeth

94

36 (10)

167

Eight accelerometers are installed on the engine of the helicopter and the first, sixth and seventh were installed on the casing of the planetary gearbox. The diagram of the specific locations can be seen in Fig. 22.
The rotary speed of the sun gear shaft was 574.74 rpm and it is constant due to the speciality of helicopter. Three kinds of torque are implemeted and they are 30 %, 40 % and 50 % of the rated torque of the helicopter. The data is acquired during the flight time 600 h to 800 h. It is found through opengearbox examination that the planetary gearbox is healthy after testing. Continue experiment has not been implemented with considering the economy and safety.
Fig. 22. The diagram of accelerometers installed on the casing of the planetary gearbox
Similarily, according to the configuration parameters of the helicopter planetary gearbox, the relevant fault characteristic frequencies can be obtained. The specific values of the frequencies can be seen in Table 4.
Table 4. Fault characteristic frequencies of every gear of helicopter planetary gearbox
Rotary speed (rpm)

Meshing frequency (Hz)

Fault frequency of sun gear (Hz)

Fault frequency of planet gear (Hz)

Fault frequency of ring gear (Hz)

574.74

576.15

61.29

16.00

34.50

Firstly, the frequency spectrum of the acquired signal is analyzed. This paper utilizes the vibration signal acquired by Accelerometer 1. Fig. 23 shows the frequency spectrum analysis of the vibration signal. Only the 1, 2 and 3 times of the planetary gearbox gear meshing frequency appeared. This is a normal phenomenon and it also can demonstrate the planetary gearbox is healthy. In addition, it can be seen in Fig. 23, the frequency amplitudes of some other structures are very high. If the planetary gearbox is damaged, these frequencies will disturb the fault diagnosis of it. Therefore, an effective fault diagnosis method for helicopter planetary gearbox is very important.
Fig. 23. Frequency spectrum analysis of the signal acquired from the helicopter planetary gearbox
Generally, due to the planetary gearbox is healthy, but the effectiveness of the proposed method also can be validated if the proposed method has good performance when analyzing the data acquired from different working conditions. Therefore, the signal acquired from the three kinds of torques is analyzed in this section and the results can be seen in Fig. 24, 25 and 26.
Fig. 24. The signal of 30 % rated torque: a) results of EMD and AMMGF_{DE}; b) frequency spectrum
Fig. 25. The signal of 40 % rated torque: a) results of EMD and AMMGF_{DE}; b) frequency spectrum
Fig. 26. The signal of 50 % rated torque: a) results of EMD and AMMGF_{DE}; b) frequency spectrum
It can be seen from the three results that there is not fault characteristic frequency of any structure of the helicopter engine in each frequency spectrum. Only 1 and 2 times of the planetary gearbox meshing frequency appear in the frequency spectrum of 50 % rated torque. So, it can be assessed that the planetary gearbox is healthy. In addition, disturbed frequencies can not be seen in each frequency spectrum compared with the original analysis in Fig. 23. Therefore, the effectiveness of the method proposed in this paper can be further validated.
An offline fault diagnosis method for planetary gearbox based on EMD and AMMGF was proposed in this paper. Firstly, the basic theory of MM was introduced thoroughly and the framework of the proposed method was given out. Then, experimental data and industrial data were utilized to validate the effectiveness of the method. And the combination of EMD and AMMGF_{DE} was found very suitable to be used in the planetary gearbox fault diagnosis compared with other six filters (dilation, erosion, opening, closing, MGF_{DE} and MGF_{CO}). The results from the two kinds of data show that the proposed method has good performance on both extracting fault characteristic frequency and denoising. Therefore, the method is very suitable for offline planetary gearbox fault diagnosis.