Stabilization of Power Hardware-in-the-Loop simulations of electric energy systems

Stabilization of Power Hardware-in-the-Loop simulations of electric energy systems

Simulation Modelling Practice and Theory 19 (2011) 1699–1708 Contents lists available at ScienceDirect Simulation Modelling Practice and Theory jour...

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Simulation Modelling Practice and Theory 19 (2011) 1699–1708

Contents lists available at ScienceDirect

Simulation Modelling Practice and Theory journal homepage: www.elsevier.com/locate/simpat

Stabilization of Power Hardware-in-the-Loop simulations of electric energy systems Alexander Viehweider a,⇑, Georg Lauss b, Lehfuss Felix b a b

Department of Advanced Energy, The University of Tokyo, Japan Business Unit Electric Energy Systems, Energy Department, Austrian Institute of Technology, Austria

a r t i c l e

i n f o

Article history: Received 3 October 2010 Received in revised form 10 March 2011 Accepted 4 April 2011

Keywords: Hardware-in-the-Loop Stability Filtering Multi-rate

a b s t r a c t Power Hardware-in-the-Loop – as a particular simulation technology that includes real hardware with high power rating in the simulation loop – is used more and more in the scientific field. Power Hardware-in-the-Loop simulations may suffer – depending on the attached power hardware and the simulated subsystem – from the drawback of becoming unstable without appropriate countermeasures. This contribution introduces and compares three methods to guarantee stability under unfavorable stability conditions. The three methods behave differently as far as accuracy is concerned. Multi-Rate Partitioning is introduced as a good compromise between effort and performance. Ó 2011 Elsevier B.V. All rights reserved.

1. Introduction The Hardware-in-the-Loop (HIL) simulation is a recognized simulation method in different engineering areas (e.g. automotive applications). Power Hardware-in-the-Loop (PHIL) simulations as an extension of classical HIL applications is gaining ground especially in the field of electric energy systems [2,6,7,10,13,14,16,18,19]. The Power Hardware-in-the-Loop simulation allows for system and component test scenarios that would otherwise be impossible to implement. The test of a hardware component (load, generator, inverter . . .) with an extended electrical network (simulated) becomes feasible. One of the main issues is if the whole PHIL simulation runs stably. This can be considered as a necessary condition within this context. Additionally stability should come with an acceptable accuracy of the results extracted from the PHIL simulation. Accuracy is a sufficient condition for a successful PHIL simulation. Stability and accuracy are highly dependent on the way software simulation and hardware under test (HuT) are interfaced, the so called interfacing algorithm (IA) [11,15]. A good overview of interfacing algorithms is given in the PhD thesis by Ren [3]. The author concluded that only two algorithms out of five have good accuracy and acceptable stability properties. Early publications in the field dealt with quite simple hardware under test. For example, Ayasun et al. in [4,5] and Wu et al. in [21,22] looked at a simple network consisting of a voltage source, two resistors and an inductance. They attached a series connection of a resistor and an inductance as real hardware to the PHIL simulation. The trend now moves to more sophisticated applications of this simulation technology (e.g. [2,10,13,18,20]), but stability still remains an issue.

⇑ Corresponding author. Address: Department of Advanced Energy, The University of Tokyo, Trans-disciplinary Sciences Bldg., 5-1-5, Kashiwanoha, Kashiwa, Chiba 277-8561, Japan. Fax: +81 4 7136 3873. E-mail address: [email protected] (A. Viehweider). 1569-190X/$ - see front matter Ó 2011 Elsevier B.V. All rights reserved. doi:10.1016/j.simpat.2011.04.001

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This article introduces three methods to stabilize Power Hardware-in-the-Loop simulations that use the Ideal Transformer Method (ITM) as IA. The method easiest to implement is the Hardware Inductance Addition (HIA) method, but accuracy is generally poor. Feedback Current Filtering (FCF) may outperform HIA, but accuracy may still not be sufficient. The third one, Multi-Rate Partitioning (MRP), is demanding as far as the implementation is concerned since it demands a multi-rate real time computing system, but leads to interesting stability and accuracy results. The merit of this paper is to systematically compare and verify the three methods by applying them to an application with photovoltaic generation. To compare the three methods of stabilization a small low voltage grid attached to a photovoltaic inverter (modeled as a current source with output filter) is introduced and the analytic results compared.

2. PHIL simulation system model with Ideal Transformer Method Interface 2.1. General overview In Fig. 1 a general overview of a PHIL simulation system for electric energy system simulation is given. A real time simulation of an electrical network runs on a real time computing system. The real time computing system drives a power amplifier that is connected to real hardware, the so called Hardware under Test (HuT). The power amplifier exchanges power (usually in the range of some hundred watts to 1 MW [17] in the field of electric energy system simulation). Depending on the application the power amplifier must be able to provide power (if an electric load is attached) or absorb power (if a generator is attached). From the HuT a signal (usually the current through the HuT) is fed back into the real time system in order to capture the interaction between the HuT and the simulated network. The power amplifier and the way signals are exchanged between the software and hardware side (the interface algorithm IA) constitute the so called Power Interface (PI). It goes without saying that a sophisticated real time computing system is needed for this type of simulation. The minimal achievable step size TS (computing time) of the real time system heavily influences stability and accuracy of the whole PHIL simulation.

2.2. Modeling Modeling of the configuration in Fig. 1 (which as a combination of a continuous and discrete time system is a hybrid system) is approached in different ways. Ren [3,15] and Hong et al. [8] use a quasi-continuous approach (analysis in the continuous time domain) for the whole system description in the Laplace domain approximating the discrete time behavior of the real time computing system, whereas Ayasun et al. in [4,5] use discrete time models in the z domain. Within this article the quasi-continuous approach is used where the effect of the discrete time behavior of the real time computing system is modeled as additional time delay in the continuous time domain. A lot of problems in the field of PHIL simulation can be reduced to the configuration in Fig. 2 (left), where the voltage source U0 and the impedance ZA(s) are simulated (computed) in software and the impedance ZB(s) characterizes the HuT that is attached via the PI to the real time computing system. For the time being it is assumed that the HuT is a passive load. From the stability point of view it does not change anything if we add a current source or voltage source on the hardware side – in

Fig. 1. Overview of PHIL setup for electric energy system simulation.

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Fig. 2. Introducing the Power Interface with the interface algorithm into the model of the real system.

Fig. 3. The Ideal Transformer Method interface algorithm.

order to model power generation – since it is assumed that the whole system is linear. Configuration Fig. 1 (left) is especially suited to introduce basic issues in PHIL simulation. The introduction of the PI with its interface algorithm transforms the system into the system in Fig. 2 (right) from a modeling point of view, where A(s) is an appropriate matrix description of the PI with the interface algorithm in the Laplace domain (e.g. chain matrix, impedance matrix, . . .). In the ideal case (the power amplifier and the sensors are ideal and the real time computing system is infinitely fast) the system model on the right side of Fig. 2 would be completely identical to the left system model, since the chain matrix A(s) would reduce to the identity matrix. In the case of a real PHIL experiment non-idealities affect the simulation; the chain matrix A(s = jw) differs from the unity matrix especially for higher frequencies. This is due to the fact that the power amplifier and the sensors have a limited bandwidth and the real time computing system works in a discrete time manner, introducing additional delay within this quasicontinuous approach. Besides that, quantization noise and amplifier noise are introduced; these effects are not considered within this contribution.

2.3. The Ideal Transformer Method interface algorithm The Ideal Transformer Method (ITM) voltage type as shown in Fig. 3 is one of the most straightforward interface models and often used in practice [3,9,15]. It is characterized by a fictional current controlled current source on the software side and a voltage controlled voltage source on the hardware side. The software current source is driven by the current i2 measured through the HUT. The computed voltage u1 over the software current source is the driving signal for the controlled ‘‘real hardware’’ voltage source (= voltage amplifier). The signal flow diagram can easily be derived for the ITM IA. It is assumed that the dynamic behavior of the voltage amplifier and the current sensor can be described by the transfer function TVA(s), TC(s) in the Laplace domain. Additionally TD1 and TD2 are the delays in the forward and feedback path due to the computational time of the model and the A/D, D/A converters. Therefore, it follows that

u01 ðsÞ ¼ esT D1 T VA ðsÞu1 ðsÞ

ð1Þ

0

i2 ðsÞ ¼ esT D2 T C ðsÞi2 ðsÞ; and as a consequence

 AðsÞ ¼

esT D1 T VA ðsÞ

0

0

esT D2 T C ðsÞ

 :

The signal flow diagram shown in Fig. 4 results; it clearly shows the closed loop character of the PHIL simulation.

ð2Þ

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Fig. 4. Signal flow diagram of the PHIL configuration.

Fig. 5. Relative error for the PHIL configuration according to Fig. 3 (ZA = 1, ZB = 2, TS = 25 ls, TVA(s) according to Appendix A).

In Fig. 4 the delay of the forward and backward path TD1, TD2 has been combined into the whole time delay TD and the dynamic behavior of the sensor is assumed to be ideal (TC(s) = 1). Usually the time delay TD can be set to twice the computing time (step size) of the real time computing system TS. For more information on this topic, confer [12]. In order to show how accuracy of a PHIL simulation with an ITM IA is computed a very simple example is given. It is assumed that the voltage ratio between the voltage over the HuT ZB (according to Fig. 2) and the internal voltage source U0 is of interest. According to Kirchhoff’s law this voltage ratio is given in the Laplace domain for the original system by

T IDEAL ðsÞ ¼

Z B ðsÞ Z A ðsÞ þ Z B ðsÞ

ð3Þ

Since the interface is not ideal, the voltage ratio obtained with PHIL using ITM IA is given by

T PHIL ðsÞ ¼

Z B ðsÞ T VA ðsÞesTD Z A ðsÞT VA ðsÞesT D þ Z B ðsÞ

ð4Þ

This means that there is a difference between the ideal voltage ratio and the voltage ratio obtained by PHIL simulation and one can compute a relative error a(w) in dB given by

T REAL ðs ¼ jwÞ  T IDEAL ðs ¼ jwÞ aðwÞ ¼ 20 log T IDEAL ðs ¼ jwÞ

ð5Þ

This error a(w) takes into account the relative difference between the ideal ratio and the ratio obtained by PHIL simulation. It depends heavily on the frequency. It is typically small for low frequencies and large for high frequencies because of the delay and the limited bandwidth of the PHIL system. In Fig. 5 the accuracy is shown under the assumption that the impedances ZA and ZB are real valued (defined as ZA = RA = 1 O and ZB = RB = 2 O), the voltage amplifier described in the Appendix A is used and that the sampling (computing) time TS (=step size) of the real time computing is 25 ls.

3. Stabilization methods for PHIL Different methods to improve the stability properties of the ITM interface are introduced. They differ as far as their ease of implementation and their efficiency is concerned. An efficient stabilization would guarantee both: good stability properties and high fidelity of the PHIL simulation.

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Fig. 6. ITM IA with Hardware Inductance Addition.

3.1. Hardware Inductance Addition (HIA) method The simplest way of improving stability is to add in series with the HuT an inductor of a certain inductance LADD as shown in Fig. 6: The open loop transfer function of the PHIL constellation amounts now to:

F O ðsÞ ¼

Z A ðsÞ T VA ðsÞesT D sLADD þ Z B ðsÞ

ð6Þ

It is assumed that ZA(s) and ZB(s) are realizable, strictly passive impedances; both of them have the following structure:

ZðsÞ ¼

NðsÞ ; DðsÞ

ð7Þ

where the numerator N(s) is a polynomial of degree dN and the denominator D(s) a polynomial of degree dD. From network theory it follows that the degree of the numerator and the denominator are related in the following way:

dN ¼ dD or dN ¼ dD  1;

ð8Þ LADD,



Therefore, it follows that there exists a limit value so that impedance values LADD > LADD stabilize the system. This is due to the fact that the amount of the open loop transfer function |FO(jw)| can be made as small as necessary at frequencies wC where <(FO(jwC)) = 180°. From the accuracy point of view the additional inductance should be as small as possible. 3.2. Feedback current filtering (FCF) method HIA may lead to poor accuracy results. Often in order to guarantee stability the value of the additional inductance has to be chosen very high, so that results are very inaccurate especially for higher frequencies. Since the value of the inductor is the only parameter to choose for this method the degree of freedom is equal to 1 and therefore really limited. The feedback current filtering method has more degrees of freedom has. As the name suggests the measured current through the HuT is filtered appropriately. The filter order depends on the HuT. The open loop transfer function in this case is

F O ðsÞ ¼

Z A ðsÞ T F ðsÞT VA ðsÞesT D ; Z B ðsÞ

ð9Þ

where TF(s) is the transfer function of the feedback current filter. The filter can be optimized in order to meet the stability and accuracy requirements.

Fig. 7. System partitioned for MRP.

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If the voltage amplifier has sufficient behavior and the computational time of the real time computing system is very short, then in order to guarantee accuracy the TF(s) should be close to 1 in a broad frequency range, guaranteeing at the same time that the system with the open loop transfer functions according to (9) is stable. The needed filter order depends on the HuT attached. For example if ZB(s) is a series connection of a resistor and a capacitor ZB(s) = R + 1/(sC) and ZA(s) is a pure resistance the filter must be at least of n order n = 2 in order that the PHIL simulation runs stably. 3.3. Multi-Rate Partitioning (MRP) MRP is a method inspired by the architecture of modern real time computing systems. Modern real time computing systems allow for subsystems with higher sampling rates (smaller step sizes). Unfortunately the size of the fast sampled subsystems is limited – usually the very fast subsystems are computed on a FPGA board. MRP partitions the system to simulate different subsystems with different sampling rates. Ideally the ratio of the sampling rates of the single subsystem should be very high in order to obtain good dynamic decoupling. Fig. 7 shows the main procedure: the system to be simulated is split into a large subsystem with a large step size and a small subsystem with a very small step size. If the ratio between the step size of the large subsystem and the small subsystem is very high, then stability could checked in a two step procedure: First, the stability of the PHIL simulation with only the fast subsystem as the simulated part together with the hardware is determined; it is a necessary condition. Secondly, the stability of the whole system is determined. The partitioning depends strongly on the topology and the elements of the networks. If carried out appropriately, it can guarantee certain accuracy together with a reasonable stability margin. Usually, the method is combined with FCF, but the cut-off frequency of the current feedback filter can be chosen with a high value. For stability reasons the fast subsystem should be large and comprise a high portion of the original system; this may not be feasible due to computing limitations of the real time computing hardware. Therefore, as much as possible of the system should be computing with the fast sampling rate (small step size). For each configuration stability has to be checked separately. 4. Accuracy comparisons of the stabilization methods – an example The introduced methods from chapter 3 (HIA, FCF, MRP) are applied to a real world problem: a photovoltaic inverter is connected to a low voltage grid via a long transmission line. The low voltage grid should be simulated and the photovoltaic inverter attached as a real hardware device via the Power Interface to the real time computing system as shown in Fig. 8. The three approaches for stabilization are applied to this problem and the analytic results shown. This contribution focuses on theoretical and analytical results, therefore the PHIL experiment is not carried out with real hardware, but a simulated PHIL simulation is used for the analytical discussion. 4.1. Simulated Power Hardware-in-the-Loop Simulation A Simulated Power Hardware-in-the-Loop Simulation (SPHIL) is a pure software simulation (model) where the properties of the Power Interface of the PHIL configuration are included in the simulation and a simulation model for the HuT is available and used. It means simulating the system as shown in Fig. 2 (right side) with an appropriate matrix A(s) in order to capture the effects of the non-ideal coupling between hardware and software parts of the PHIL simulation. It is a highly efficient tool for prediction of the behavior of the PHIL simulation but accurate models of the power amplifier and the sensors and the hardware under test are necessary. 4.2. Modeling and computation The low voltage grid consists of an infinite bus (a voltage source) and a long cable that is modeled with some p-sections (R0 , L0 , C0 ). The photovoltaic inverter is modeled very simply; an AC current source is attached to an output filter. It is true that

Fig. 8. Overview of the considered PHIL simulation.

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Fig. 9. Model of the PHIL simulation.

Fig. 10. Relative error of the simulated PHIL configuration depending on the stabilization method.

this model cannot reflect the intrinsic complexity of a modern photovoltaic inverter, but as shown in [8] the output filter influences heavily the stability properties of the PHIL simulation. The output filter consists mainly of capacitors; capacitors on the hardware side of the voltage type ITM filter drastically reduce the stability margin if sufficient countermeasures are not taken. 4.3. Experiment and results The PHIL simulation of the system shown in Fig. 9 with the parameter values as given in Appendix B would not run stably without any countermeasure. The three introduced methods are therefore applied and the accuracy properties of the single methods compared. Additionally very fast sampling of the real time computing system is also considered for reference. As criteria for the accuracy of the system the amount of the relative error in dB between the voltages over the hardware under test U2 and the voltage of the infinite bus U0 is used and the phase for U2 for the real system (without PI) and the PHIL simulation (with PI) compared. In order to guarantee stability for the HIA method an inductor of 4 mH had to be added, for the FCF method a Butterworth filter of order 3 with cut-off frequency 4 kHz and for the MRP method a Butterworth filter of order 3 with cut-off frequency

Fig. 11. Phase of U2 for the ideal system and the PHIL configuration for different stabilization methods.

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Table 1 Evaluation summary of the stabilization methods. Method

HIA

FCF

MRP

Very fast sampling

Implementation effort

Low (hardware inductance needed)

Low (software filter needed)

Very high (very fast real time computing system needed)

Analytic complexity (effort to analyze analytically the whole PHIL setup) Stabilization

Low

Medium

High (multi-rate capable real time system needed) Very high

Always possible if cutoff frequency is low enough Medium Always

In combination with FCF always possible

Accuracy Feasibility

Always possible if inductance value is high enough Poor Always

There may necessary unrealistic sampling rates for stabilization Very high Only for small systems

Overall score

+

+

High Often, depends on topology ++

Low

+

Fig. 12. Step function response of the used voltage amplifier.

7 kHz. The order and cut-off frequency of the Butterworth filter has been chosen by evaluating the Nyquist criteria for the whole setup (for FCF by using Eq. (9) and for MRP by using a quasi continuous model) The filter order is a compromise between achieved stability margin and accuracy of the PHIL setup. Therefore filter order and cut-off frequency have been determined in an iterative way. For the MRP method the transmission has been split into two pieces: two thirds of the long cable is simulated with large step size and one third with small step size. The reason behind is the dynamic decoupling that is achieved by doing so. The effective impedance ratio between software part and hardware part changes, allowing for more stability margin of the setup. Also for fast sampling FCF a Butterworth filter of order 3 and cut-off frequency 9 kHz was necessary. In Fig. 10 the outcomes for the different stabilization methods are shown. The frequency bandwidth of accuracy of the PHIL configuration is defined as the bandwidth, where the relative error is lower than 20 dB (=10% relative error). As expected, HIA has the smallest accuracy bandwidth up to 380 Hz. FCF with an optimized feedback filter is much better with a bandwidth up to 620 Hz. It comes as no surprise that faster sampling of the real time computing system (1 ls) leads to the best results, but it is astonishing how close MRP comes to faster sampling. On the other hand, a multi-rate real time computing system (25 ls, 1 ls) is needed for MRP and part of the system to simulate is computed with the high rate (1 ls). A similar outcome is obtained by comparing the phases of the voltage U2 for the ideal case and the PHIL configuration (Fig. 11). For HIA already at low frequency heavy phase inaccuracies occur. FCF is more accurate and MRP leads to the best results comparable to a very fast real time computing system that computes the whole simulation model at a fast rate. This may not be possible for large systems, but it may be possible to simulate part of the system at a fast rate and the rest with a slow rate. In Table 1 a short evaluation summary of the single stabilization methods is given.

5. Conclusions This contribution compared three ways of establishing stability for a PHIL simulation with the ITM IA in the case of an unstable PHIL configuration. They differed as far as their complexity for implementation is concerned: HIA is the simplest

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method bu demands an additional hardware inductance; FCF uses a filter that can be implemented on the software side of the PHIL simulation and MRP requires a multi-rate capable real time computing system and is therefore the most demanding as far as the equipment is concerned but the method with best accuracy results. The stabilization results should be further evaluated for uncertain parameters and nonlinear settings. Nonlinearity in the general context asks for other methods for stabilization like the Popov criteria [1]. In the case of weak nonlinearities, the methods discussed in this contribution may suffice to guarantee stability and accuracy depending on the needed fidelity of the simulation. Appendix A. Dynamic model of the power (voltage) amplifier The transfer function TVA(s) of the voltage amplifier, whose model is used in chapter 4 has been identified by using the step function response shown in Fig. 12. The used voltage amplifier is a linear amplifier (as opposed to switched-mode amplifiers) and has a maximal power rating of 10 kW. The transfer function obtained by curve fitting is:

T VA ðsÞ ¼ esð4 lsÞ

1 1 þ sð8 lsÞ þ s2 ð2:91e  13 s2 Þ

This transfer function proved to be a good model of the dynamic behavior in the whole power range. Appendix B. Parameter values for the experiment

Cable

Filter

Generation

Length l R0 L0 C0 C1 C2 L R I0

0.5 km 0.06 O/km 2 mH/km 12 nF/km 1 lF 2.2 lF 12 mH 2.9 4O 4 A, 50 Hz

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