1. Introduction
It is widely recognized that the DC side of single-phase inverter systems can generate double frequency (2ω) current ripple as a result of pulsating power [
1]. The 2ω ripple power can exert harmonic stresses on the DC side of the inverter, causing overheating and inefficiencies, as well as significantly impacting system functionality [
2]. In photovoltaic power generation applications, low-frequency pulsating currents can affect the Maximum Power Point Tracking (MPPT) of the circuit and the energy utilization of the photovoltaic panel, ultimately resulting in a reduction in the power generation efficiency of photovoltaic power generation systems [
3,
4,
5,
6,
7]. In addition, for the chargers of electric vehicles, in the Vehicle-to-Grid (V2G) operation mode, the secondary ripple component on the DC side is more severe, further reducing the life and performance of the battery pack [
8,
9]. For three-phase systems, in the event of an asymmetrical fault, the AC side will also produce 2ω ripple, and the 2ω ripple can seriously affect the DC bus voltage and even the generation side. Therefore, research efforts focused on suppressing low-frequency pulsating power in new energy supply systems as an important research direction. The methods of suppressing 2ω ripple in traditional inverters are usually divided into passive filtering and active filtering [
10,
11].
Passive techniques involve the use of inductors and capacitors as LC passive filters on the DC side to absorb low-frequency ripple. The passive power decoupling technology employed in traditional voltage-source and current-source inverters does not require additional active switches, making it simple to implement with straightforward control. Voltage-source inverters usually employ large-capacity electrolytic capacitors to suppress high-frequency switching ripple voltage and low-frequency ripple voltage [
12]. However, the equivalent series resistance of the electrolytic capacitor leads to power loss during operation, which can cause its temperature to rise and significantly shorten the lifespan of the electrolytic capacitor. Two-stage inverters are widely utilized in applications where the input voltage on the DC side undergoes significant changes, or when there is a substantial difference between the input voltage on the DC side and the output voltage on the AC side. Such inverters comprise a DC-DC converter in the front stage and an inverter in the rear stage. However, ripple power may generate a secondary ripple current in the input current of the rear-stage inverter. This secondary ripple current flows back to the front-stage DC-DC converter and the DC input source, increasing the current stress of the power switches and resulting in power loss. Typically, a DC-side electrolytic capacitor is utilized to absorb the secondary ripple current in parallel, which places significant demands on the capacitor. To mitigate this issue, the authors of [
13] proposed a current compensation control scheme with repetitive control. Additionally, [
14] and [
15] propose different control methods to suppress the secondary ripple current of the Two-Stage Power Factor Correction (PFC) converter and AC/DC/AC converter, respectively. The impedance-source converters are widely used in various fields, such as fuel cells, photovoltaic arrays, and electric vehicles [
16,
17,
18]. However, there is secondary ripple power on the DC side of single-phase impedance-source inverters, and impedance-source converters generally require a large impedance-source network to filter out low-frequency ripple [
16,
19,
20]. To decrease the demand for electrolytic capacitors, impedance-source inverters typically optimize the impedance-source network parameters in terms of passive power decoupling topology. The authors of [
21] proposed an effective method for suppressing secondary ripple that reduces the capacitor requirements for single-phase Z-source/quasi-Z-source inverters, storing secondary ripple energy in
C1 and
C2. Compared to traditional quasi-Z-source inverter photovoltaic power generation systems, although the capacitance value is reduced, the voltage stress of the switch increases slightly, leading to a decrease in efficiency.
Active filtering is the method of using active filters usually composed of power switches and energy storage elements to buffer low-frequency ripple [
22,
23,
24]. To reduce the demand for DC side inductors and capacitors, a separate active power buffer can be designed. Low-frequency ripple power can be handled using additional power electronic devices and energy storage elements. Since the voltage or current of the storage element in the separate active power buffer can be controlled independently, the volume of the power buffer can be reduced through increasing the AC variation in the voltage or current of the storage element. The authors of [
25] integrated the single-phase switched boost inverter (SBI) with a separate boost-type active power buffer to reduce passive components on the switch impedance network. The authors of [
26] proposed an Active Low-Frequency Ripple Control Device (ALFRCD) and control method for Building-Integrated Photovoltaic (BIPV) systems, which reduces the use of electrolytic capacitors and improves the lifespan and reliability of the photovoltaic system through introducing a boost-type active low-ripple control device. The authors of [
22] proposed three control methods for the voltage and ripple of the energy storage capacitor of the active power buffer, including voltage set-point control, ripple ratio control, and minimum voltage set-point control. Buck-boost-type active power buffers have wide voltage adjustment characteristics, and there is no upper limit on the voltage set-point of the energy storage capacitor; however, when it is much lower than the DC bus voltage, it may affect the effectiveness of the secondary ripple suppression. In addition, to suppress the influence of dc-link voltage ripple on the back-stage DAB, the authors of [
27] proposed a feedback linearization control strategy; however, this technique is designed for two-stage converters and cannot achieve good ripple suppression for single-stage inverters.
However, conventional inverters contain only one degree of control freedom, and when the desired AC side voltage amplitude is higher than the given DC voltage value, a DC-DC converter must be integrated to form a two-stage structure to meet the demand [
28].
Compared to conventional inverters, the quasi-Z-source inverter (QZSI) [
29] offers several advantages that make it an attractive alternative. Firstly, the QZSI has two independent degrees of control freedom—the shoot-through duty cycle and the modulation—providing greater flexibility in controlling the output. Secondly, its unique impedance network structure allows for both boost and buck functions of a DC-DC converter, resulting in a single-stage system that is more cost effective. Thirdly, the QZSI permits bridge leg shoot-through and exhibits stronger anti-electromagnetic interference (EMI) capability. These features make the QZSI a more appealing option for power electronics applications. Similar to traditional inverters, QZSI can also absorb 2ω ripple using passive filtering techniques. [
30,
31] analyzed the relationship between the 2ω current and capacitor voltage of the impedance network and the impedance network parameters based on the small signal model. The authors of [
30] provided a principle for designing LC parameters using the allowable ripple percentage of inductor current and capacitor voltage under symmetric parameter conditions. The authors of [
31] stated that a higher percentage of ripple is needed to meet the demand under asymmetric parameters. However, the method proposed in [
30,
31] requires large-capacity capacitor and inductor impedance networks, which will not only lead to large volume, heavy weight, and high cost of inverters, but will also reduce the efficiency and reliability of the system.
The authors of [
32,
33] proposed methods to reduce the 2ω ripple through adjusting the shoot-through duty cycle. The authors of [
32] proposed a current damping control method, which can completely eliminate the low-frequency ripple in the inductor current of the impedance network. However, this method requires a complex and sophisticated control system. On the other hand, [
33] presented a hybrid pulse width modulation technique that can significantly reduce the required inductance and capacitance values. Nevertheless, the system must be paralleled with a large-capacity DC power supply terminal capacitor.
To minimize the 2ω ripple on the DC input side without increasing the parameters of the impedance network, this paper proposes a novel single-phase three-leg QZSI topology. This topology is based on the active filtering techniques of traditional inverters and injects harmonic voltage into an additional third bridge leg to buffer low-frequency pulsating power, effectively suppressing input current ripple. Compared with the passive filtering suppression method, the additional power switching device used in this approach is smaller in size and weight. Furthermore, the impedance network only needs to avoid the switching frequency ripple setting, which significantly improves the power density of the inverter. The paper is organized as follows:
Section 2 introduces the circuit topology and ripple suppression principle of single-phase three-leg QZSI,
Section 3 discusses the control strategy of the system,
Section 4 designs the system parameters,
Section 5 shows simulation results, and
Section 6 concludes this work.
2. Circuit Topology and Operating Principle of the Proposed Inverter
2.1. Traditional Quasi-Z-Source Inverter and the Analysis of Its Secondary Ripple
The traditional single-phase QZSI contains two bridge legs, and there are two operating modes: the shoot-through state and the non-shoot-through state. The circuit topology is shown in
Figure 1.
The equivalent circuits for the non-shoot-through state and the shoot-through state are shown in
Figure 2 and
Figure 3, respectively.
As the impedance network is a symmetrical network,
C1 =
C2 and
L1 =
L2, which can be obtained as follows:
where
VC1 and
VC2 represent the voltages across the capacitors
C1 and
C2, while
VL1 and
VL2 denote the voltages across inductors
L1 and
L2, respectively.
In the non-shoot-through state, the inductors
L1 and
L2 store energy, while capacitors
C1 and
C2 release energy. Equations (2) and (3) can be obtained using Kirchhoff’s Voltage Law (KVL) and Kirchhoff’s Current Law (KCL):
where
Vi represents the DC input current, and
VPN represents the DC bus voltage.
where
iC1 and
iC2 represent the currents flowing through capacitors
C1 and
C2, respectively.
iVD represents the current flowing through diode VD.
iL1 and
iL2 represent the currents flowing through inductors
L1 and
L2, respectively.
iPN represents the DC bus current.
In the shoot-through state, H-Bridge is short-circuited and the diode VD is in the off state. The inductors
L1 and
L2 release energy, while the capacitors
C1 and
C2 store energy. Equations (4) and (5) can be obtained from KVL and KCL:
At steady-state, the voltages across the inductors
L1 and
L2 are both zero within one cycle. Using Equations (2) and (4) and the volt-second balance, Equation (6) can be obtained:
where
and
are the average values of the voltage across the inductors over one cycle,
T0 is the time in the shoot-through state,
T1 is the time in the non-shoot-through state, and the period
T =
T0 +
T1.
At steady state, the capacitor current is zero over one period. Using Equations (3) and (5) and the charge balance, Equation (7) can be obtained:
where
and
are the average values of the capacitor currents over one period.
Equation (8) can be obtained from Equations (6) and (7),
where
D represents the duty cycle of the shoot-through state, while
.
and
are the average values of the inductor currents about
L1 and
L2.
From Equations (2) and (8), Equation (9) can be obtained:
where
B is the boost factor,
.
The output voltage and current on the AC side can be written as follows:
where ω is the fundamental angular frequency, φ
L is the power factor angle, and
Vo and
Io are the rms output voltage and current, respectively.
The expression of the output instantaneous power on the AC side is
The relationship between the output voltage and the DC bus voltage
VPN can be expressed as
From Equations (10) and (12), the peak output voltage of the single-phase inverter is given by
where
M is the modulation index, and
G is the boost coefficient of the quasi-Z-source inverter.
When the circuit is in the shoot-through state, the DC bus voltage is zero; when the circuit is in the non-shoot-through state, the power is transferred from the DC side to the AC side. If the intermediate losses are neglected, Equation (14) can be written as
The DC bus current expression can be obtained using Equations (12) and (14)
where
IPN is the DC component, and
is the 2ω component of the DC bus current. The inductor currents
iL1 and
iL2 and capacitor voltages
vC1 and
vC2 in the impedance network are directly influenced via
iPN, so that
where
are the 2ω components of the corresponding currents and voltages, respectively.
When the DC input voltage is constant, the power supply and capacitors charge the inductors in the shoot-through state, and there exists a 2ω component relationship.
In the non-shoot-through state, the power supply and the inductors charge the capacitors with the following 2ω component relationship.
The impedance network is a symmetrical structure, (i.e.,
L1 =
L2 =
L,
C1 =
C2 =
C). From Equations (17) and (18), one can write
are in the same phase with
, while
are at a phase lag of 90 degrees with
; thus, it follows that
where
and
are the peak values of 2ω ripple in the current of inductor
L1 and the voltage of capacitor
C1, respectively.
From Equations (19) and (20), the inductance and capacitance 2ω ripple expression in the impedance network can be presented by
The expression for the inductor current and capacitor voltage 2ω ripple of a conventional QZSI impedance network can be found in Equation (21). If the 2ω pulsating power in Equation (21) is made to be zero, and can be realized, which constitutes the active decoupling method for the integrated third bridge leg.
2.2. Circuit Topology of the Proposed Inverter
The circuit topology of the single-phase three-leg QZSI is shown in
Figure 4.
The circuit is designed to be integrated with an additional third bridge leg, which is based on a conventional single-phase QZSI. Through injecting harmonic voltage into the third leg of the bridge, the output 2ω ripple power is reduced to zero (i.e., ), thus reducing the 2ω ripple in the impedance network of inductors and capacitors to a very small value. Notably, the impedance network is still designed with symmetrical parameters, where L1 = L2 and C1 = C2.
2.3. Operating Principle of the Proposed Inverter
The single-phase three-leg QZSI has two operating states: the shoot-through state and the non-shoot-through state. In the non-shoot-through state, the upper and lower switches in the same bridge leg of the inverter conduct in a complementary manner.
Using
ST indicates the shoot-through state, while
S (
SA,
SB,
SE) indicates the non-shoot-through state, where
SA,
SB, and
SE can take the value of 0 or 1, the value of 0 indicates that the switch below the corresponding bridge leg is turned on, and the value of 1 indicates that the switch above the corresponding bridge leg is turned on. The topology operating states and points
A,
B, and
E voltage are shown in
Table 1.
Based on
Table 1, it can be observed that the voltages at points
A,
B, and
E, which are denoted as
vA,
vB, and
vE, respectively, only have two possible values:
VPN and 0. Using the Fourier transform,
vA,
vB, and
vE can be expressed as follows
where
VdcA represents the DC component of the voltage at point
A, while
An represents the amplitude of the nth harmonic component of the voltage at point
A.
VdcB represents the DC component of the voltage at point
B, and
Bn represents the amplitude of the nth harmonic component of the voltage at point
B.
Vdc2 represents the DC component of the voltage at point
E, and
Vn represents the amplitude of the nth harmonic component of the voltage at point
E.
The expression of the fundamental frequency component of the output voltage is shown in Equation (10), and if the filter inductor voltage drop values are neglected, the following can be obtained
The following Equation (24) is given by Equations (10), (22), and (23).
It can be seen that the addition of the third bridge leg does not affect the inverter output. To simplify the analysis, the following relationship is taken.
Vdc1 represents the DC component of the voltage at point
A and point
B.
The output filter capacitor voltage and inductor current can be written as follows
where
vo1 and
vo2 represent the voltages across the output filter capacitors
Cf1 and
Cf2, respectively, while
io1 and
io2 represent the currents through the output filter inductors
Lf1 and
Lf2, respectively.
Cf denotes the output filter capacitor,
Cf1 =
Cf2 =
Cf,
Vdc =
Vdc2 −
Vdc1, and
The instantaneous power of the output filter capacitor is given by
Substituting
A1 +
B2 = 0 into Equations (24) and (27), the following results can be obtained
Using
buffer
, such that
. To eliminate
, only the second harmonic is retained in Q
E; therefore, Q
E can be expressed as follows
Equation (31) can be obtained from the above analysis
Using the 2ω pulsating power to offset
, the amplitude and phase of the injected second harmonic voltage can be obtained
Although the 2ω pulsating power is buffered when injecting the second harmonic voltage in the third bridge leg, a new 4ω pulsating power is generated. If the third bridge leg simultaneously injects a fourth harmonic voltage, the following results can be obtained
Through setting
in Equation (33), Equation (34) can be obtained as follows
Based on Equation (34), the amplitude and phase of the injected fourth harmonic voltage can be obtained as follows
It can be observed that injecting low-frequency harmonic voltages into the third bridge leg can eliminate the ripple power at the pre-determined frequency; however, at the same time, new frequency-dependent ripple power is generated. If a third harmonic voltage is injected simultaneously, the following results can be obtained
It can be deduced from Equation (36) that, in this case, the ripple power at 6th harmonic frequency can be eliminated; however, at the same time, new ripple powers at the first, second, third, fifth, seventh, and eighth harmonic are generated.
Table 2 presents the correlation between the input current harmonic content and the frequency of the injected harmonic voltage in the additional bridge leg, with parameters set to
f = 50 Hz, P = 300 W,
Vi = 144 V,
Vdc = 150 V,
Cf = 52 μf,
Vo = 110 V, and φ
L = 0. Analysis of
Table 2 indicates that the harmonic content of the input current is relatively insignificant in comparison to the DC component when the additional bridge leg injects second and fourth harmonic voltages simultaneously. However, injecting second, third, and fourth harmonic voltages actually increases the ripple content of the input current. These observations reveal that injecting specific combinations of harmonic voltages can impact the harmonic content of the input current, highlighting the importance of carefully selecting the appropriate harmonic injection strategy to minimize undesirable effects on the system.
The expressions for the voltages at points
A,
B, and
E when the additional bridge leg injects second-frequency and fourth-frequency harmonic voltages are as follows
The following relationships need to be satisfied for the shoot-through modulation signals
Vcom1 and
Vcom2.
Based on the above equation, when vA, vB, and vE satisfy Equations (37) and (38), the inverter can simultaneously achieve boosting, inversion, and low-frequency ripple suppression of input current.
3. The Control Strategy of the Proposed Inverter
Figure 5 illustrates the control strategy employed for the single-phase three-bridge-leg of QSZI. The shoot-through state modulation is achieved using open-loop simple boost control, while constant output voltage control is employed for the two bridge-leg of H-Bridge. For the additional third bridge-leg, a control method is employed that injects specific frequency harmonic voltage and suppresses newly generated low-frequency components of the input current. The controllers utilize a quasi-PR (QPR) control strategy. The transfer function of the QPR control incorporates the transfer function of the sinusoidal signal, which is represented as ω/s
2 + ω
2. This process enables accurate tracking of the sinusoidal signal without any static errors.
Figure 6 illustrates a comparison of the Bode diagrams for the PI, PR, and QPR controllers. It is evident that the QPR controller exhibits superior bandwidth and enhanced stability, even in the presence of output target frequency perturbations, as compared to the PI and PR controller.
The amplitude–frequency characteristics of the QPR controller clearly indicate that the gain approaches zero at frequencies other than the resonant frequency point. This characteristic empowers the QPR controller with the ability to effectively suppress harmonics at specific frequencies.
Figure 7 presents the structural diagram of QPR2, which is designed based on this principle.
The modulation waveforms of the system are shown in
Figure 8, where the
A and
B bridge legs, as well as the
E bridge leg, adopt independent simple Sinusoidal Pulse Width Modulation (SPWM) strategies. The modulation waveforms of the three bridge legs are represented by
urA,
urB, and
urE, with a triangular waveform
uc as the carrier signal. When
ur ≥
uc, the switches of the upper leg of the corresponding bridge leg are turned on, while the switches of the lower leg are turned off. When
ur ≤
uc, the switches of the upper leg of the corresponding bridge leg are turned off, and the switches of the lower leg are turned on. When
uc ≥
Vcom1 or
uc ≤
Vcom2, the bridge leg is in a shoot-through state.
4. Parameter Design of the System
4.1. Parameter Design of Inductance and Capacitance in Impedance Network
The implementation of the active filtering technique effectively minimizes ripple power in the output power, resulting in the complete suppression of 2ω ripple on the DC side. Therefore, the inductors and capacitors in the impedance network do not need to buffer the 2ω ripple according to Equation (21), but only need to suppress the switching frequency ripple. When the inductances
L1 and
L2, as well as the capacitance
C1 and
C2 in the impedance network, satisfy the following relationship, they can suppress the switching frequency current ripple and voltage ripple, respectively.
where
W1 denotes the percentage of current ripple at the frequency of the inductive switch,
W2 represents the percentage of voltage ripple at the frequency of the capacitive switch,
W1 is usually selected as 20%, and W
2 is selected as 1%.
D denotes the duty cycle of the shoot-through, and
fs represents the switching frequency.
4.2. Parameter Design for Modulation of the Third Bridge Leg
The selection of parameters Vdc and Cf in Equation (32) is directly correlated with crucial circuit parameters, such as the input voltage level and the voltage stress on switches, which impact the overall performance of the circuit. Therefore, a more comprehensive and in-depth analysis is required to thoroughly understand the interdependence of these parameters.
Based on Equation (33), the relationship between the values of the DC bias voltages
Vdc and
V2 can be obtained when
S = 300 VA,
Cf = 52 μf, and φ
L= 0, as shown in
Figure 9. From
Figure 9, it can be inferred that the value of
V2 decreases as the value of
Vdc increases. Hence, it is crucial to avoid selecting an excessively small value for
Vdc to prevent
V2 from becoming excessively large. Furthermore, the values of
Vdc and
V2 are closely related to the magnitude of
VPN; the DC bus voltage, which is dependent on the input voltage; and the shoot-through duty cycle. As a result, the value of
Vdc should also not be excessively large.
Based on the analysis, it is concluded that selecting
Vdc within the range of 100 V to 200 V is more reasonable. The minimum value of
VPN is related to other parameters, as shown in
Table 3. It is worth noting that
VPNmin remains constant for both schemes. According to Equation (31), when the second harmonic power in the output power is cancelled out due to the second harmonic power in the
p2cf, Equation (40) can be obtained.
Through analysis, when Vdc1 is greater than Vdc2, the following situations occur:
When φV2 is located in the second quadrant. When φV2 is located in the third quadrant.
When Vdc1 is less than Vdc2, φV2 is always located in the first or fourth quadrant. Therefore, it can be seen that selecting the second scheme where Vdc1 ≤ Vdc2 is more in line with the actual situation and easier to implement. Therefore, Vdc1 is chosen to be less than or equal to Vdc2, and the value of Vdc is set to 150 V.
In comparison to the conventional two-leg inverter, the three-leg inverter topology necessitates a higher DC bias value, resulting in a corresponding requirement for a higher DC bus voltage. As shown in Equations (37) and (38), the DC bus voltage needs to satisfy the following expression
Since
Vdc1 ≤
Vdc2,
Vdc = 150 V is chosen, and one can simply write
The correlation between the minimum DC bus voltage,
VPNmin, and capacitance, C
f, is presented in
Figure 10 for the specific case of S = 300 VA,
Vdc = 150 V, and φ
L = 0. Furthermore,
Figure 10 depicts the relationship between
VPNmin and the power factor angle, φ
L, in the case of S = 300 VA,
Cf = 52 uF, and
Vdc = 150 V.
The selection of the injected secondary harmonic voltage V2 should be 20 to 30% of Vdc when Vdc is chosen as 150 V. Otherwise, it will affect the boosting capability of the quasi-Z-source inverter, thus affecting the value of the DC bus voltage. From Equation (42), the relationship between the injected secondary voltage amplitude V2 and the filter capacitor Cf can be obtained. Based on the range of values for the injected secondary voltage amplitude, the range of Cf can be determined to be 36 to 56 μF.
The results of this investigation highlight that the selection of capacitance Cf is intimately tied to both the voltage stress experienced by the switches and the overall capacity of the system. Hence, a comprehensive evaluation of these factors is crucial in determining the optimal value for capacitance Cf. If the capacitance is too large, it will significantly increase the size of the inverter and the current flowing through the capacitor, which reduces the power density of the inverter and increases the current stress on the power switching devices. Similarly, if the capacitance is too small, the demand for the minimum DC bus voltage is too high, and the voltage stress on the power switching devices increases, which limits the selection of the switching devices.
Taking into account the above analysis, a relatively appropriate range of values can be obtained, and selecting values within this range is acceptable. Finally, a capacitance value of 52 μF was selected.