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Control Method for Fault-Tolerant Active Power Filters

  • Zhang, Chenyu (School of Electrical Engineering, Southeast University) ;
  • Zheng, Jianyong (School of Electrical Engineering, Southeast University) ;
  • Mei, Jun (School of Electrical Engineering, Southeast University) ;
  • Deng, Kai (School of Electrical Engineering, Southeast University) ;
  • Zhou, Fuju (School of Electrical Engineering, Southeast University)
  • 투고 : 2014.04.28
  • 심사 : 2015.01.24
  • 발행 : 2015.05.20

초록

New direct and indirect current control methods for a fault-tolerant active power filter topology are presented in this paper. Since a three-phase four-switch topology has a phase bridge current which cannot be directly controlled, a hysteresis control method in the α-β plane which controls the three-phase current in the two-phase stationary coordinate system is proposed. The improved SVPWM algorithm is able to eliminate the operation of the trigonometric functions in the traditional algorithm by rotating the α-β coordinates and alternating the sequence of the output vectors, which in turn simplifies the algorithm and reduces the switching frequency. The selection of the DC-side reference voltage and DC-side capacitor equalization strategy are also discussed. Simulation and experiments demonstrate that the proposed control method is correct and feasible.

키워드

I. INTRODUCTION

As a result of the intensive growth of the power quality problems in power systems, the active power filter (APF) has been widely studied and applied as a dynamic shunt compensation device due to its real time harmonic and reactive power compensation [1]-[4]. However, since an APF usually operates in harsh industrial environments with high temperatures in which the power switching device IGBT runs at a high frequency, reliable operation of the power switching device is required to guarantee the stability of the APF [5]. Once the IGBT breaks down due to overvoltage or overcurrent, the general approach is to remove the APF from the grid and wait for repair. With the appearance of the three-phase four-switch APF (TFSSAPF), an APF can continue to operate effectively and reliably by changing its topology when a single-phase power device is dysfunctional. This gives the APF a certain amount of self-healing capability, extends the APF work period and buys more time for fault handling.

The conventional three-phase six-switch APF has been studied a lot since the 1980s [6]-[9], and its control algorithms have been completely developed. Therefore, it does not need to be repeated in this paper. However, the three-phase four-switch APF control strategy within a fault-tolerant topology has not been thoroughly studied. Since the shunt grid voltage source inverter (VSI) control methods are mainly divided into direct current control and indirect current control, new direct and indirect control schemes for the TFSSAPF topology are proposed in this paper.

For the direct control method, a hysteresis current control in the α-β coordinate system for the TFSSAPF is proposed. Since the TFSSAPF has a direct connection between the phase bridge and the midpoint of the DC side, the phase current is no longer independently controlled. In the proposed method, two hysteresis comparators separately control the two-phase stationary coordinates on the α-β axes. Then the overall control of the abc three-phase current is achieved.

For the indirect control method, some studies [10]-[14] analyze the three-phase four-switch inverter fault-tolerant control strategy. The study in [15] introduces this kind of control strategy to the control of an APF and the study in [16] discusses the operation of a TFSSAPF when the three-phase grid voltage is unbalanced and the grid is under a short-time fault. However, in these papers the sector of the vector is classified by the phase angle of the reference vector, which requires a massive trigonometric function calculation. In order to avoid the use of a look-up table by the digital processor to obtain the trigonometric calculation results and to get the sector number through the positive and negative values of the line voltage in the same way as the three-phase six-switch APF, the study in [17] greatly reduces the complexity of the algorithm by means of vector rotation. Based on that, the study in [18] proposes a five-segment-type SVPWM modulation algorithm. Based on former studies, an improved SVPWM modulation algorithm for the TFSSAPF is proposed in this paper. First, the α-β coordinates are rotated 120° clockwise to obtain the g-h coordinates to coincide the basic vectors with the new axes. In this way, the sector of the reference vector can be directly determined through the basic operations of the line voltage, which saves a lot of trigonometric calculations in the traditional α-β coordinate system. Then the five-segment-type SVPWM modulation algorithm described in [18] is further improved so that only one phase switching state changes within each sector to simplify the algorithm and to reduce the switching frequency.

In addition, for the DC-side capacitor voltage control, this paper discusses the selection of the initial value of the DC-side voltage for the TFSSAPF and the solution of the capacitors voltage equalization. Finally, simulations and experiments which verify both the correctness and feasibility of this algorithm are presented.

This paper is organized as follows. Fault tolerance mechanisms for APFs are reviewed in Section II. A current control scheme for the TFSSAPF is presented in Section III. A DC voltage control scheme is illustrated in Section IV. Simulation and experimental results are given in Section V.

 

II. FAULT TOLERANCE MECHANISMS

Since they are operated in special industrial field environments, IGBT are vulnerable devices in extreme working conditions in which the fault detection and tolerance mechanism of the APF is an essential element. A three-phase four-switch APF tolerant topology circuit is introduced in this paper. It is a fault-tolerant solution when one phase power device of the APF opens circuit under normal operating conditions (when IGBT short circuits due to the breakdown of each series of fast fuse switches immediately disconnect the phase, so that in this article it will be considered as a phase IGBT short circuit breaker) is given. Fig. 1(a) shows the APF tolerant topology, where KM1, KM3, and KM5 are open contactors; KM2, KM4, and KM6 are close contactors; and S1 ~ S6 are six-leg three-phase power switches. When S5 or S6 fails in phase c, the c-phase bridge connects to the middle of the DC-side capacitors so that the APF topology is changed from Fig. 1(b) to Fig. 1(c).

Fig. 1.Fault-tolerant topology of APF.

In Fig. 1, the TFSSAPF reduces one phase bridge arm which in turn decreases the number of switching states from six to four. This inevitably leads to a lower modulation accuracy, but also reduces the cost of the power switches and drivers. As a fault-tolerant solution, it extends the lifetime of the APF which gives it research and application potential.

 

III. CURRENT CONTROL SCHEMES

When an APF encounters a single phase open circuit fault, it automatically cuts the damaged phase current through a self-fault diagnosis in which the topology switches to a three-phase four-switching state. Due to this change, the current control scheme is no longer the same as the traditional three-phase six-switch topology.

A. Hysteresis Control

When a c-phase circuit experiences an open-circuit fault, the topology circuit is switched to the three-phase four-switching state. When the DC-side capacitor voltage control is at the steady state and the capacitor voltage is equalized such that uc1 = uc2 = udc/2, only the output line voltages uao and ubo can be directly controlled since the c-phase bridge is connected to the middle of the DC-side capacitors. Each of the switching state diagrams is shown in Fig. 2(a)-(d).

Fig. 2.Switching status of TFSSAPF.

When the switch of Sa and Sb is open, it is equal to 1 and vice versa. Then, the switching states of the TFSSAPF can be described as:

The stationary three-phase coordinates can be transformed to α-β coordinate as:

Equation (2) can be written in a matrix as:

Where:

Since output voltage uoc is always 0, combining equation (1) with equation (3) yields:

Equation (5) gives the relationship between the switching signals and voltage space vectors in the α-β coordinate system as shown in Table I.

TABLE IRELATIONSHIP BETWEEN SWITCHING SIGNALS AND VOLTAGE SPACE VECTORS IN α-β COORDINATE

The new APF topology cannot control the c-phase output current independently. Therefore, three independent hysteresis comparator cannot be used to control the three-phase current. A hysteresis current control method in α-β coordinate system for the TFSSAPF is proposed in this paper, where the hysteresis controls the α-β axis in the two-phase stationary coordinate system in order to achieve complete control of the abc three-phase current. A diagram of the hysteresis control in α-β coordinate system is shown in Fig. 3.

Fig. 3.Diagram of hysteresis control in α-β coordinate.

Table I and Fig. 3 are combined and the α-axis is taken as an example. When the actual output current is greater (less) than the reference value, dα = -1 (1), the output of the α-axis need a negative (positive) voltage to reduce (increase) the actual output current. This is similar to the β-axis control principle. Therefore, the hysteresis output state dα, dβ in the α-β coordinate system determines the switching state Uk which is shown in Table II.

TABLE IISWITCHING STATE TABLE

Hysteresis control in the α-β coordinate system for the TFSSAPF effectively solves the problem of a phase current connection with a midpoint of the output capacitor that cannot be directly controlled. The control method has excellent dynamic response. However, the compensation precision and switching frequency are affected by the width of the hysteresis ring.

B. SVPWM Control

According to Table I, the TFSSAPF basic output voltage space vector in the α-β coordinate system is not on the basic axes. This leads to the need for a α-β component projection of the reference voltage vector to the direction of the basic space vector. This process requires a lot of phase transformation and trigonometric function operations. In order to simplify the SVPWM control method, the α-β coordinates are rotated 120° clockwise to obtain the g-h coordinates so that the basic vector U0 coincides with the positive g-axis, while the reference voltage vector is projected to the g-h coordinates for operation, which is shown in Fig. 4.

Fig. 4.Distribution diagram of the basic voltage space vectors.

According to Fig. 4(b), the three phase stationary coordinate is projected to g-h coordinate system so that:

Equation (6) can be written in matrix form as:

Where:

In addition, it is assumed that c-phase current is under a fault and that uco is always 0. Combining equation (1) with (7) yields:

Equation (9) gives the relationship between the switching signals and the voltage space vectors in g-h coordinate system as Table III.

TABLE IIIRELATIONSHIP BETWEEN SWITCHING SIGNALS AND VOLTAGE SPACE VECTORS IN g-h COORDINATE

In the α-β coordinate system, the angle of the reference vector should be calculated first to determine the sector. However, in the g-h coordinate system the sector can be directly obtained by looking at the signs of ug and uh as shown in Fig. 4(b). This improvement greatly reduces the amount of arithmetic operations.

Due to the absence of a zero sequence current component in the three-phase three-wire system and the three-phase asymmetry, the output voltage can be decomposed into positive sequence component and negative sequence component, as shown in Fig. 5. When the TFSSAPF equivalent output requires the three-phase positive sequence components, the vector diagram is shown in Fig. 5(c).

Fig. 5.Vector diagrams of output voltage.

According to Fig. 5(c), the following is obtained:

In addition:

Combining equation (10) with (11) yields:

According to equations (12) and (13), the sector of the current vector is obtained by determining the sign of uac + ubc and uac - ubc without calculating ug and uh.

According to Table IV, the total reaction time of the effective basic short vectors (U0, U3) in each cycle is:

where Ts is the unit time period. The total reaction time of the effective basic long vectors (U1, U2) in each cycle is:

TABLE IVJUDGMENT OF SECTOR

When tg + th > Ts, tg’ = tgTs /(tg + th) and th’ = thTs/(tg + th) after modification. The action time of the zero vector t0 = Ts - tg - th. Since the fundament vectors of the TFSSAPF do not have a zero vector and each of the individual long vectors do not change the equalization voltage of the capacitors, the corresponding long vectors (U1, U2) are added up to get the equivalent zero vector. With the zero vector, the study in [18] proposed a five-segment-type SVPWM algorithm. Based on this study, an improved SVPWM modulation algorithm is proposed for the TFSSAPF to reduce the switching frequency.

In addition, according to Fig. 3, only the long vectors do not change the equalization voltage of the capacitors. Therefore, the long vectors are used to get the zero vector. However, the zero vector does not utilize the centralized policy. Therefore, the long vectors are inserted in the middle of the synthesis zero vector. In this method, the phase switching state only changes once per unit time period Ts and there is no interchange between each of the short vectors. Thus, the switching frequency is effectively reduced.

In Table V, the total reaction time of the effective basic long vectors is th, the total reaction time of the effective basic short vectors is (Ts - tg + th)/2 and the reaction time of the equivalent zero vector is (Ts - tg + th)/2. According to Table V and the reaction time of the basic vectors, a timing sequence diagram of the switching signals is shown in Fig. 6.

TABLE VIMPROVED ALGORITHM OF SVPWM

Fig. 6.Timing sequence diagram of the switching signals.

Fig. 6 shows the timing sequence diagrams of the switching signals from the study in [18] and the proposed method in this paper. In the proposed method, the phase switching state changes only once per unit time period, and the switching state changes when the sector switches between sector II and sector III or between sector IV and sector I. As a result, there are 5 switches in the 4 switching periods of Ts and the switching frequency f1 = 5/(4Ts). From the study in [18], the switching state in two sectors changes twice per unit time period. Adding up the changes when the sector switches results in a total of 7 switches in the 4 switching period of Ts and the switching frequency f2 = 7/(4Ts). In conclusion, with the equivalent control effect, the switching frequency of the proposed SVPWM method is reduced to 2/7 of the previous method.

 

IV. DC VOLTAGE CONTROL SCHEME

Since the APF itself is a device which cannot produce (consume) power, the three-phase output current is in equilibrium and the DC-side capacitor voltage does not change when the APF is at the steady state. The problem with the APF DC-side capacitor voltage regulator is equivalent to the problem with the active power balance between the DC-side and the power grid, which has been studied a great deal. The TFSSAPF DC-side voltage stability control method is the same as the three-phase six-switch APF DC-side capacitor voltage stability control method, which will not be repeated in this paper.

However, it is worth pointing out that, according to Fig. 4 and Table III, when the reference vector is a quadrilateral inscribed circle composed of basic vectors, the TFSSAPF maximum modulation ratio is With the three-phase six-switch APF the maximum modulation ratio is and the utilization rate of the DC-side voltage is only half that under the normal topology condition. Therefore, in order to achieve the required inverter voltage, the TFSSAPF DC-side voltage should be set to twice the normal value. Taking the increased power loss in the higher DC-side voltage into account, the DC-side voltage general is little less than double.

Since the c-phase bridge is directly connected to the middle of C1 and C2, the midpoint voltage is not spontaneously equalized but is affected by the c-phase bridge current. Stabilizing the voltage of the DC-side capacitors is an important issue to guarantee the steady-state compensation accuracy.

According to Fig. 2 and the analysis above, when the power grid contains all three-phase positive sequence components, only the active component in phase c affects the midpoint voltage. Therefore, the active component current can be controlled in phase c to solve the two capacitors equalization problem. The revised three-phase reference currents are:

According to equation (16), when uc2 > uc1, the active component of icref increases, which makes uc2 decrease. Since udc = uc1 + uc2, uc1 increases when udc is stable. Then, uc1 = uc2 eventually. When uc2 < uc1, the situation is similar.

 

V. SIMULATION AND EXPERIMENTAL RESULTS

A. Simulation

To verify the feasibility and correctness of the proposed method in this paper, a TFSSAPF system model based on Matlab/Simulink is established. Assuming that the c-phase circuit is open, the c-phase bridge is directly connected to the middle of the DC side capacitors after fault diagnosis. The simulation parameters are: C1 = C2 =6800μF, US = 220V, Udc = 1400V, L1 = 1mH, and RL = 23Ω.

Waveforms of the grid current after compensation with the hysteresis control method in the α-β coordinate system proposed in this paper, the SVPWM modulation algorithm proposed in the study in [18], and the improved SVPWM modulation algorithm proposed in this paper are shown in Fig. 7.

Fig. 7.Grid current after Compensation.

According to Fig. 7, both of the methods proposed in this paper can control the TFSSAPF effectively. They both have a good compensation effect and the THD of the grid current after compensation is kept within 5%.

Compared with the study in [18], the improved SVPWM modulation algorithm only changes the sequence of the basic vector output. Thus, one phase switching state changes per unit time period. Fig. 8(a) and Fig. 8(b) show the drive waveforms of the five-segment-type SVPWM modulation algorithm proposed in [18] and the improved SVPWM modulation algorithm proposed in this paper, respectively. Fig. 8(c) and Fig. 8(d) shows the switching frequencies of these two methods, respectively.

Fig. 8.Waveform of drive signal. (a) Drive signal with the method in the literature [18]. (b) Drive signal with the method in this paper. (c) Switching frequency statistics with the method in the literature [18]. (d) Switching frequency statistics with the method in this paper.

When Ts = 2e-4s, the switching frequency of the traditional five-segment-type SVPWM algorithm in [18] is about 8.75kHz, while the switching frequency of the improved algorithm is about 6.25kHz. This is a reduction of 2/7 as expected. The results without affecting the compensation accuracy are shown in Fig. 7, which also effectively reduces the switching frequency and the switching losses.

In order to verify the DC-side capacitor voltage equalization scheme, through a simulation study, the DC-side capacitor voltage waveform is shown in Fig. 9.

Fig. 9.Waveform of DC voltage. (a) DC-side voltage waveform without equalization scheme. (b) DC-side voltage waveform with equalization scheme.

Fig. 9(a) is the waveform without the DC capacitor voltage equalization scheme. The phase c current is not corrected so that uc1 and uc2 are about 700V. However, this cannot achieve full equalization. Fig. 9(a) is the waveform of that current after revision. The waveforms of uc1 and uc2 nearly overlap with the setting value of 700V, and the DC-side capacitor voltage gets effectively equalized.

B. Experiment

To further verify the correctness and feasibility of the proposed methods, a 5KW prototype has been implemented in the laboratory. The prototype control unit utilizes a TMS320F28335 DSP chip combined with a FPGA chip EP2C20F256, dual-core for better computing and logic functions. The IGBT modules use Simon Kang SKM400GB176Ds and the IGBT drivers use Simon Kang SKHI23/17(R)s. The prototype experimental parameters are shown in Table VI. The other parameters of the experiment are consistent with the simulation. A TEK oscilloscope DPO2024 and a FLUKE 43B power quality analyzer record the data and waveforms.

TABLE VIPARAMETERS OF EXPERIMENT

Fig. 10 shows the current waveform after a normal three-phase six-switch APF compensation with the hysteresis control method.

Fig. 10.Current waveform after compensation.

According to Fig. 10, the grid current waveform after compensation with the traditional APF topology has no offset, the total harmonic distortion (THD) of the system current drops by 27% to 2.8%, and the low-order harmonics of the non-linear load are effectively eliminated.

When the APF has a phase switch fault, the topology turns to the TFSSAPF. Fig. 11 shows the current waveform after compensation with the hysteresis control method in the α-β coordinate system proposed in this paper.

Fig. 11.TFSSAPF waveform after compensation with hysteresis control.

According to Fig.11, the THD of the system current after compensation is 5.8%. This shows that the TFSSAPF cannot use three independent hysteresis comparators to control the three-phase current. However, the hysteresis current control method can control two-phase stationary coordinates on the α-β axis to achieve complete control of the abc three-phase current. From Fig. 10 and Fig. 11, due to the lack of two switching states, the modulation accuracy of the TFSSAPF is less than the traditional three-phase six-switching APF. However, the results still meet the compensation standards of industrial applications.

Fig. 12 shows the TFSSAPF experimental waveforms after compensation with the SVPWM modulation algorithm. Fig. 12(a) and Fig. 12(b) are the results with the algorithm in [18], and Fig. 12(c) and Fig. 12(d) are results with the improved algorithm and capacitor voltage equalization method in this paper.

Fig. 12.TFSSAPF waveform after compensation with SVPWM control.

From a comparison of Fig. 12(a) and Fig. 12(c), it can be seen that the compensation effects of the two modulation methods are similar, and that the compensated grid current THDs are 6.8% and 6.6%. However, from a comparison of Fig. 12(a) and Fig. 12(c), it can be seen that the improved method effectively reduces the switching frequency to about 5/7 of that in [18]. Fig. 12(b) shows the method without the DC-side capacitor voltage equalization scheme in which there exists a voltage difference between the two capacitors. From Fig. 12(d), it can be seen that the method with the DC-side capacitor voltage equalization scheme makes the DC-side capacitor voltage equalized and stable. The simulation and experimental results are consistent, which further verifies the correctness of the proposed control methods in this paper.

 

VI. CONCLUSION

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피인용 문헌

  1. Performance Analysis and Comparison of Post-Fault PWM Rectifiers Using Various Space Vector Modulation Methods vol.16, pp.6, 2016, https://doi.org/10.6113/JPE.2016.16.6.2258