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    Voltage control in low voltage networks by

    Photovoltaic Inverters PVNET.dk

    Case-study Bornholm

    Adrian Constantin, Radu Dan Lazar and Dr. Sren Bkhj Kjr

    Danfoss Solar Inverters A/S, December 2012

    This report can also be downloaded athttp://www.danfoss.com/solarand atwww.PVNET.dk

    Research supported partly by Energinet.dk, under grant number ForskEL 10698

    Danfoss can accept no responsibility for possible errors in catalogues, brochures and other printedmaterial. Danfoss reserves the right to alter its products without notice. This also applies to productsalready on order provided that such alterations can be made without subsequential changes beingnecessary in specifications already agreed. All trademarks in this material are property of the respectivecompanies. Danfoss and the Danfoss logotype are trademarks of Danfoss A/S. This work is licensedunder aCreative Commons Attribution-NoDerivs 3.0 Unported License

    http://www.danfoss.com/BusinessAreas/Solar+Energy/All+products/Literature+knowledge+database.htm?showliterature=true&literaturetype=literaturehttp://www.danfoss.com/BusinessAreas/Solar+Energy/All+products/Literature+knowledge+database.htm?showliterature=true&literaturetype=literaturehttp://www.danfoss.com/BusinessAreas/Solar+Energy/All+products/Literature+knowledge+database.htm?showliterature=true&literaturetype=literaturehttp://www.pvnet.dk/http://www.pvnet.dk/http://www.pvnet.dk/http://creativecommons.org/licenses/by-nd/3.0/http://creativecommons.org/licenses/by-nd/3.0/deed.dahttp://creativecommons.org/licenses/by-nd/3.0/http://www.pvnet.dk/http://www.danfoss.com/BusinessAreas/Solar+Energy/All+products/Literature+knowledge+database.htm?showliterature=true&literaturetype=literature
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    Summary

    This report provides an analysis on the main voltage regulation techniques that can be

    applied in the low voltage (LV) network with standard photovoltaic (PV) inverter technology. The

    main purpose of the research is to verify if reactive power can be used in LV networks to increasethe hosting capacity, by controlling the voltage and hereby increase the hosting capacity of the LV

    networks.

    The hosting capacity of a LV network is defined by the amount of PV power which can be

    installed in the network before certain limits are reached. The evaluated limits in this report are:

    overloading of LV cables, overloading of MV/LV transformers and overvoltage at the outermost

    distribution box. Two types of Volt-VAR control schemes are presented: the power factor

    depending on active power output of the PV inverters - PF(P) and reactive power depending on

    the terminal voltage of the PV inverter - Q(U). A generic LV grid model with 71 users and a 100 kVA

    feeding transformer is used in the simulations, being considered as representative for the

    Bornholm network. All users are equipped with PV systems, each of equal power size and PV panelorientation. Furthermore, a simple MV network is implemented in order to observe the voltage

    variations in the 10 kV network as well. The energy consumption for each of the 71 users is based

    on time-series of generic consumption. The PV generation is based on synthesized hourly

    irradiance by the PVsyst software, taking both clear sky and covered sky into consideration.

    The results indicate that without voltage control the overvoltage phenomena starts for a PV

    capacity of 1.5 kW per residence (total 107 kW). By applying a standard PF(P) control scheme, the

    overvoltage condition is avoided up to a PV penetration level of 1.8 kW per residence (total 124

    kW) and still keeps the amount of exchanged reactive power low, PF > 0.95. By applying Q(U)

    control, the overvoltage condition is mitigated up to 2.0 kW (total 144 kW) penetration and still

    keeping the power factor above 0.90. The overvoltage issue is not solved by upgrading the feedingtransformer, on the contrary increasing the size of the transformer has a slight negative effect. The

    total hosting capacity for the LV networks on Bornholm is estimated to 50 60 MW, which can

    cover 1520% of the yearly energy consumption.

    Overall, it has been found that applying standard voltage control techniques in the LV

    networks helps to increase the PV penetration by approximately 30% from 1.5 kW to 2.0 kW per

    residence. For higher PV penetration levels, additional solutions must be applied: more complex

    voltage control schemes, increased self-consumption, storage solutions or active power

    curtailment. Both PF(P) and Q(U) control types are improving the maximum voltage profile at the

    outermost distribution box. Based on these results, if overvoltage is observed at the end-customer

    site the following order of actions are suggested:

    Apply voltage control for the inverters, e.g. PF(P), Q(U) or more complex schemes

    Lower the tap position in the LV/MV transformer and apply Q(U) round the clock

    Increase self-consumption at peak production hours

    Lower active output power of inverters (only in emergency cases for short periods)

    Upgrade cables, upgrading the transformer does not help

    Install storage, i.e. battery systems

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    Table of Contents

    1 INTRODUCTION 7

    1.1 Problem statement 7

    2 METHODS 10

    2.1 Definition of hosting capacity for the electrical network 10

    2.2 Definition of PV penetration for the electrical network 13

    2.3 Reactive power by grid voltage - Q(U) 14

    2.4 Power Factor by Active Power PF(P) according to VDE AR N 4105 17

    2.5 Generic LV network 18

    2.6 Statistical Data Used for Consumption and Generation 202.6.1 Electrical energy consumption 202.6.2 PV generation 20

    2.7 Simulation model 222.7.1 Dynamic inverter model description 222.7.2 Dynamic AC load modeling 23

    2.8 Simulation study cases 23

    3 RESULTS 26

    3.1 Results of the base study case 26

    3.2 Overview of comparisons between the simulated results 34

    3.3 Varying the dead-band of the Q(U) controller 36

    3.4 Varying the voltage sensitivity of the Q(U) controller 38

    3.5 Comparison for varying the transformer power rating with and without Q(U) voltage control 42

    3.6 Comparison for varying the transformer power rating with PF(P) voltage control 44

    3.7 Comparison of Q(U) and PF(P) 46

    3.8 Comparison of hosting capacity for the cases 48

    4 CONCLUSION 50

    4.1 Obtained results 50

    4.2 Recommendations for voltage control in LV feeders 52

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    4.3 Future Work 52

    5 WORKS CITED 54

    6 APPENDIX A 56

    7 APPENDIX B 58

    7.1 Study case 2 58

    7.2 Study case 3 62

    7.3 Study case 4 67

    7.4 Study case 5 71

    7.5 Study case 6 76

    7.6 Study case 7 80

    7.7 Study case 8 84

    7.8 Study case 9 89

    7.9 Study case 10 93

    7.10 Study case 11 97

    7.11 Study case 12 102

    7.12 Study case 13 106

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    Nomenclature

    DNO Distribution Network Operator

    EPIA European Photovoltaic Industry Association

    HV High Voltage

    LV Low Voltage

    MV Medium Voltage

    OLTC On load tap changer

    PF Power factor (acc. To IEEE convention)

    PV Photovoltaic

    TSO Transmission System Operator

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    1IntroductionThis study is part of the project Application of smart grid in photovoltaic power systems

    PVNET.dk, ForskEL Programme 2011 partly sponsored by Energinet.dk. This work package

    provides one possible and economically viable solution of overcoming technical difficulties which

    may appear due to the ever increasing amount of PV generation at the LV distribution network

    level. Namely, it analyses the performance of reactive power control of the PV inverters connected

    to the LV network. This solution is intended to be tested in the laboratory and afterwards

    deployed on PV inverters on the island of Bornholm. Two types of Volt-VAr control are under

    study: reactive power by voltage - Q(U) and power factor depending on the output power - PF(P)

    of the PV inverters, both which are commonly used in Germany. The advantages and

    disadvantages of using reactive power control in a LV feeder are exemplified based on a generic LV

    network model for the Bornholm network. This network describes a typical residential topology on

    the island.

    1.1 Problem statement

    In Denmark only, PV installations are expected to increase at a very high pace with an

    estimated amount of installed power exceeding 1000 MW in 2020 [1]. As of February 2012, there

    are a total of 11 MW installed PV capacity in Denmark providing approximately 0.03% of the total

    energy consumption. This figure is comparable to approximately 3% in Germany [2]. Most of these

    PV installations in Denmark are being built in the 0.4 kV feeders of the distribution network.

    Reference [3] estimates a total of 140 MW by the end of September 2012 comprising more than

    25 000 installations.

    There are several technical issues which may appear when increasing the penetration levelof renewable energy in a LV distribution network:

    Transformer overloading

    Cable overloading

    Overvoltage phenomena

    Voltage unbalance

    Reverse power feed-in

    Protection System failure

    The first three issues are the most urgent and the DNOs are trying to address them first. This

    document will focus on these. Voltage unbalance has been studied within this project in paralleland documented in reference [4]. Reverse power flow and protection system failure are not

    covered by this report due to the limited influence that PV inverters can have in mitigating these

    effects without corresponding communication channels or storage devices (which increase self

    consumption).

    The first three forementioned issues are present with different occurrence probabilities

    depending on the type and layout of each LV distribution network and the PV penetration level.

    Thus, from the point of view of categorizing the distribution networks upon the type of end

    customers, the technical literature uses the following grid naming [5]: Urban, Sub-urban, Rural and

    Farms. The current study has the objective of focusing on a sub-urban grid type due to the high

    relevance in connection to the electrical network of Bornholm.

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    A comprehensive analysis has been done by Dansk Energi in a recently published report [6].

    As in most theoretical analyses simplifying assumptions have been used (3 phased PV systems,

    hourly load/generation data, grid data only from one DNO, even distribution of PV throughout the

    network). In this report a total of 1110 0.4 kV feeders are evaluated for susceptibility of violating

    the +/- 10% voltage design criterium when introducing PV generation from 0 to 50% penetration.One of the results in their report is that while a PV penetration level of 13.5% in 2030 is expected,

    only 0.7-0.8% of the total number of feeders (containing more than 5 consumers) will experience

    overvoltage at that moment. For higher penetration levels the probability of having these types of

    problems will eventually increase, therefore, the associated costs of reinforcing the network will

    increase accordingly.

    Several solutions have been suggested until now in order to cope with the overvoltage

    phenomena at high PV penetration levels of distributed generation in LV:

    1.Voltage control using reactive power generation from PV inverters

    2.

    Voltage control at the LV side of the LV/MV transformer by on-load tap changers3.Active power derating of the PV production in case of overvoltage conditions

    4.Battery storage/Energy buffer at PV generator and MV distribution level

    5.Network upgrade

    6.(Seasonal) changes of the tap position of the LV/MV distribution transformer

    Each solution is currently investigated by different stakeholders and their feasibility is

    assessed.

    Method 1, voltage control through reactive power generation from PV inverter, is one of the

    easiest to implement because of the versatility of the inverter unit in providing a plethora of

    voltage control techniques. A good overview of the available Volt-VAr methods is presented in [5].

    These are constant power factor (PF), constant reactive power, local Q(U) and local PF(P). The

    same reference provides two proposals for optimized local Volt-VAr control: local Q(U,P) and local

    PF(U,P). The last two methods are claimed to increase the PV penetration levels while keeping the

    reactive power flow to a minimum (thereby minimizing the reactive power exchange) and also

    avoiding overvoltage situations. Regarding the local Q(U) regulation algorithm a recent study has

    assessed its stability when applying it to PV inverters installed in LV networks [7]. In their report

    the integration of Q(U) in the standard requirements for LV connected PV inverters in Germany is

    recommended. Another author analyses and verifies the efficacy of several other different types

    of voltage control methods based also on the local Q(U) principle [8]. Several claimed

    disadvantages of the existent methods are: need for overrating the PV inverter, increasing the

    losses in the grid due to reactive current circulation, compensation in the MV network of the

    generated inductive reactive currents. All the previously mentioned control methods are intended

    to function autonomously. Still, in the future, by leveraging the Smart Grid functionality,

    communication means will be available to the inverters as well. Therefore, the voltage control

    through reactive power generation can be optimized by coordinated/scheduled control.

    Method 2, is proposed by several transformer manufacturers and DNOs [9] [10]. Pilot

    projects are already under development in order to assess the efficacy of the on load tap

    changer type transformers[6] [10] [11]. Still, the solution is not mature enough to be accepted as

    being feasible. Moreover, the high investment costs and the additional service required make this

    option less attractive.

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    Method 3, active power derating, has been investigated by researchers [12] [13] and DNOs

    [14]. Usually, the PV plant owner cannot estimate the impact of this control scheme upon the

    economical aspects of the investment. Furthermore, the PV owners which will be at the end of the

    LV feeders will be the first to be affected. An interesting conclusion is that: At first glance it seems

    that local or central regulation of reactive power comes first among the possible strategies. Activecurtailment would then be activated when reactive compensation is no longer sufficient to avoid

    upper voltage constraints[14].

    Method 4, battery storage/energy buffer at PV generator level, is promoted by several PV

    inverter manufacturers with the scope of shifting the PV grid injection peaks, thus avoiding

    overloading the network [15]. EPIAs report Connecting The Sun [16] describes as a valid solution

    the combination between active power derating and storage which will result in peak shaving at

    noon hours and feeding energy during the evening hours.The energy buffer system can be a

    battery (bidirectional power flow) or a controllable AC load (unidirectional power flow e.g. heat

    pumps). The main disadvantage of the storage solution is the high cost of an integrated battery +

    inverter system even for small capacity batteries. The life-time of the battery is also difficult to

    estimate considering the unpredictability of the full load hours to be applied. Regarding the use of

    batteries at the MV distribution level, several pilot projects are being implemented by DNOs in

    order to get more experience with the use and advantages of such a control method. Although

    providing a very good technical solution, the storage technologies are not yet price competitive

    enough for the lifetime and capacity required. Further investigations are necessary.

    Method 5, comprises the standard approach of increasing the grid capacity by upgrading the

    LV/MV transformer to a higher power rating or by reinforcing the LV feeders by addition of parallel

    lines or replacement of old lines with higher ampacity ones.

    Method 1 is the main focus in this work, the authors wishing to take advantage of theversatility of the PV inverters in providing voltage control schemes. Thus, the subject of employing

    reactive power control techniques in the LV distribution networks is discussed in this analysis. The

    main outcome of this work is intended to be a generic design guideline for mitigating effects of

    increased PV penetration, thus increasing the network integration of solar energy in the power

    system.

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    2MethodsThis Chapter represents the main part of the study and contains an analysis method

    description in order to draw guiding conclusions over the feasibility of the use of reactive power in

    LV grids for increasing PV penetration.

    2.1

    Definition of hosting capacity for the electrical network

    The reactive power supply from PV inverters is currently used in all types of networks in

    Germany (e.g. in LV and MV [17] [18]), while many other european countries are in the process of

    enforcing such requirements. On the other hand, in islanded systems it is common practice to use

    droop control to maintain the grid operation. It is therefore interesting to find out to what extent

    the reactive power control can be used in low voltage networks in terms of voltage control. This

    analysis provides study case answers to questions such as:

    What is the benefit of using the PV inverters in reactive power mode in LV networks?How much can we increase the level of PV penetration in the distribution network if

    reactive power support methods are used in the PV inverters?

    What are the limiting factors when increasing the level of PV penetration (transformer

    overloading, cable overloading or overvoltage situations) ?

    What is the influence of different grid specific parameters to the overall results (MV grid

    impedance, transformer size, cable length)?

    Reference [6] discusses in great detail the overvoltage limitations that can be encountered

    when increasing the PV generation in the LV network. Due to the high number of studied feeders

    it provides a high confidence level of the results. The voltage allocation ranges are clearly specifiedfor each component in the 10 and 0.4 kV network in such a manner that the +/- 10% voltage range

    criterium holds according to the EN50160 standard [19]. The analysis from [6] is based on

    measuring the relative difference between the secondary side of the transformer and the

    outermost distribution box in LV network. As a guiding rule, the relative voltage is allowed to vary

    to maximum -5% in case of a load and maximum +2.5% in case of PV generation [6]. In the future

    with more distributed generation in the network this might change to -2.5% to +5% voltage

    variation.

    A relatively different analysis approach is taken in this report in comparison with reference

    [6]. An absolute voltage range allocation is performed based on Figure 1. While this case is

    considered to be representative for the current analysis, other different designs may also be foundin real situations. The figure contains a one line diagram of a distribution system and the

    corresponding voltage allocation ranges. It contains a 60/10 kV transformer with on load tap

    changer controlling the voltage on the secondary side. A MV cable distribution system is shown

    connecting the 60/10 kV transformer to a 10/0.4 kV transformer. The latter contains an off load

    tap changer adjusting the voltage on the secondary side. A LV distribution network follows

    towards the farthest located distribution box. A load and a PV system are depicted as being

    connected to the network. It can be seen that at each location in this network certain minimum

    and maximum voltage limits apply. The narrowest allocated range is at the secondary side of the

    60/10 kV transformer where the voltage is allowed to vary within a 2% interval. The widest band is

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    allocated to the outermost distribution box for which the +/-10% voltage limits are applied. This

    figure represents one of the main requirements for the voltage ranges in this report.

    According to [6] the voltage ranges fromTable 1 are reserved from the full +/-10% interval.

    Based on the above relative values of Table 1, the absolute voltage ranges from Figure 1 have

    been deduced.

    Voltage range allocated for: Size [%] Size applied

    inFigure 1

    [%]

    Tap changer at 60/10 kV transformer 2 2

    Voltage fall in the 10 kV network 5 5

    Non-optimal tap position of the 10/0.4

    transformer

    2.5 -

    Voltage drop of the 10/0.4 kV transformer 1.5 1.5

    Unsymmetrical loading 1 1

    Voltage increase in the LV installation (after the

    outermost distribution box)

    0.5 -

    Voltage increase in the LV lines - 2.5

    Voltage increase in the MV lines - 2.5

    Voltage increase in the 10/0.4 transformer - 0.5

    Tap position 10/0.4 transformer (maximum load) - 2.5

    Tap position 10/0.4 transformer (maximum PV) - 2.5

    Total 12.5 20

    Table 1: Voltage reserves allocated in the 10 and 0.4 kV network [6]

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    Figure 1: Allowed voltage ranges for different points in the 10 and 0.4 kV distribution network

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    2.2

    Definition of PV penetration for the electrical network

    The PV penetration levels are defined in this study in accordance to the definition used in

    [6]. Therefore, under the present legislative framework it is expected that an economical

    investment in a residential solar plant will result in an installed capacity of 5 kVA. Having all theconsumers in a residential feeder installing a 5 kVA/kWp solar system would therefore be

    equivalent with 100% PV penetration in the respective network feeder [6]. This method to

    estimate the amount of PV in the network has the advantage of creating a uniform distribution

    across the entire feeder of PV power. Practical cases may differ from this situation. The PV

    penetration level is expressed in percent and in combination with the number of consumers

    and the maximum rated power of one PV inverter Sr (5 kVA) it determines the total

    installed PV power in the respective feeder as in Equation 1.

    Equation 1

    InTable 2 are shown the chosen values for which calculations have been done in Section3.

    PV penetration level

    [%]

    Power Rating of

    inverter [kVA]

    Total PV power for a LV

    network with 71 customers

    [kVA]

    0 0.0 0

    10 0.5 36

    20 1.0 71

    30 1.5 107

    40 2.0 142

    50 2.5 178

    60 3.0 213

    Table 2: Selected PV penetration levels in the simulation

    Regarding the orientation of the PV panels in the PV plant it is assumed that all systems are

    oriented south with a 45 degrees vertical inclination, seeFigure 2.This case is considered to be the

    worst case scenario since in the summer months the peak production will be higher for this

    orientation than in any other situation (any orientation and any season).Figure 2 also shows that

    by scattering the PV systems in orientation and inclination the PV penetration can be further

    increased with more than 10% without negative impacts from overloading.

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    Figure 2: Typical output power from a 1 kWp PV system in clear sky conditions. The green curve shows the

    power from aggregated systems pointing all south. The red curve shows the corresponding power for 10 systems

    which are scattered from East to West with 30 and 45 inclination.

    2.3 Reactive power by grid voltage - Q(U)

    The main purpose when applying a Q(U) control algorithm is to use the reactive power of the

    inverter in such a way that in case of overvoltage conditions the control will decrease to a certain

    degree the mains voltage and in case of undervoltage situations the control will tend to increase

    the voltage towards a prescribed value. This control needs to take also into account the standard

    tap changer position of the MV/LV transformer.

    The Q(U) control is normally implemented as in Figure 3. The voltage at the inverter bus

    terminals can be used as an input value to the controller. This voltage is computed as the averaged

    RMS value of the three phases and expressed in per unit system like suggested in IEC 61850-90-7[20]. A reactive power versus voltage dependency is defined using a piecewise linear curve as

    drawn with red and green in Figure 3. The red curve contains additionally a dead band

    characteristic, commonly used in medium voltage applications. A low pass filter is added to the

    controller in order to increase stability by making the controller slower (e.g. the inverter will not

    interact with faster automatic voltage regulators).

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    Figure 3: PV inverter Q(U) control algorithm

    The slope m of the Q(U) characteristic represents the sensitivity of the reactive power

    controller versus voltage changes. In this report the term voltage sensitivity is used

    interchangeably with the term slope m of the Q(U). It is defined as inEquation 2.In the case of a

    multi segment curve as it is the case of the red curve inFigure 3,one voltage sensitivity value is

    defined for each interval. Dead-band may also be programmed in the reference curve. Thus,

    different voltage sensitivity values can be defined for under/over excited operation modes,therefore the voltage sensitivity will be calculated using a different references inEquation 2.

    maxmin

    minmax

    UU

    QQ

    U

    Qm

    Equation 2

    If analyzing a Q(U) curve there are several defining parameters (denoted by their name) and

    intervals (marked by a capital letter) as shown inFigure 4.

    Q*[pu]

    Uinv[pu]

    Umin Umax

    Qmax

    Qmin

    A B C

    Udmin UdmaxUref

    Figure 4: Generic Q(U) curve and defining parameters. The curve could also have another shape, with more points.

    IEEE power factor convention, see Section2.4.

    The operation intervals defined inFigure 4 are:

    Interval A: overexcited (capacitive) operation of the PV inverter; the main objective is

    to increase the mains voltage.

    Interval B: Dead-band in which the controller is not injecting reactive power for a

    predefined voltage range.

    Interval C: underexcited (inductive) operation of the PV inverter; the objective is to

    decrease the mains voltage.

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    The relevant parameters shown in the figure above are:

    : Minimum voltage value for which the controller should apply maximum

    capacitive reactive power at the inverters terminals .

    : Minimum voltage of dead-band interval. For lower voltages overexcited(capacitive) inverter operation is chosen while for higher values the PV inverter does

    not inject any reactive power.

    : Maximum voltage of dead-band interval. For lower values the PV inverter

    does not inject reactive power while for higher values the underexcited (inductive)

    inverter operation mode is chosen.

    : Reference voltage for dead-band selection. This parameter is chosen according

    to the selected output voltage of the LV/MV transformer at the secondary side (LV

    side) and in accordance with the voltage tap-setting. This parameter has no other

    purpose but to correctly determine suitable values for and .

    : Maximum voltage value for which the controller should apply minimum(inductive) reactive power at the inverters output terminals .

    : Minimum reactive power generated by inverter. This parameter refers to the

    underexcited reactive power operation of the inverter. The value can reach up to the

    maximum underexcited reactive power capability of the inverter.

    : Maximum reactive power generated by inverter. This parameter refers to the

    overexcited reactive power operation of the inverter. The value can reach up to the

    maximum overexcited reactive power capability of the inverter.

    Additionally to the fore-mentioned parameters, the controllers low pass filter is defined by

    a time constant. The German authority BDEW recommends in the MV networks the use of a

    settling time between 10 and 40 seconds for Q(U) [17].

    The parameter is usually chosen depending on the applicable under-voltage limits of

    the inverters. For EN50160 [19] standard the -10% limit is used in case of long-term voltage

    variations with averaging periods for 10 minutes. Therefore, if the fore-mentioned standards

    apply:

    The same design criterion is employed for defining the parameter: a value of maximum

    +10% in voltage will correspond to:

    Parameters and are defining the width of the voltage dead band in which the

    Q(U) control should not generate any reactive power. This region should restrict the inverters

    injecting unnecessary reactive power while small variations in voltage are present around the

    nominal prescribed value at the LV side of the distribution transformer. A too broad dead band

    will also have negative effects since inverters closer to transformer station will not participate at

    all in regulating the voltage while inverters at the remote ends will provide maximum reactive

    power.

    Parameter may be chosen based on the rated PCC voltage and the position of the tap-

    changer on the LV/MV transformer.

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    2.4

    Power Factor by Active Power PF(P) according to VDE AR N 4105

    In this report only one typical PF(P) curve has been analyzed, identical with the one defined

    in VDE AR N 4105 and shown in Figure 5. The IEEE power factor convention has been chosen

    throughout this report, as shown in Figure 6. Throughout the report lagging power factor andinductive reactive power are describing the same phenomena. It can be observed inFigure 5 that

    the PV inverters are required to inject reactive power (inductive) starting at 50% power generation

    and at 100% the power factor reaches 0.9 (lagging) for units with rated power above 13.8 kVA and

    0.95 (lagging) for units below this level. For the Danish standard TF 3.2.1 the same requirement is

    stated but with a rated power limit of 11 kVA for the 0.95/0.9 power factor. One property of this

    type of control is that the inverters will inject reactive power independently of the location in the

    feeder in comparison with Q(U) algorithm in which the farthest inverter would inject always more

    reactive power than the ones closer to the transformer. Thus, overall better control of the voltage

    is assumed, since all inverters in the network are taking part. The disadvantage is that the

    inverters might inject reactive power into the network even though it may not be required (noovervoltage situation).

    Figure 5: Power factor by active power control as defined in VDE AR N 4105

    Figure 6: IEEE power factor convention

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    2.5

    Generic LV network

    One representative LV network has been selected for the Bornholm distribution network for

    the project PVNet.DK [21] and it is depicted inFigure 7.It contains two LV feeders supplied by one

    MV/LV 100 kVA Transformer with parameters shown in Appendix A,a number of 71 consumersand the corresponding cable interconnections (also detailed in Appendix A). The two feeders

    contain 52 and 19 consumers respectively. This LV network supplies energy to a residential (sub-

    urban) area on the island of Bornholm. The generic LV network described in this Section is

    assumed as representative for a residential Danish LV distribution network in the island of

    Bornholm and corresponding to a suburban network (shown inFigure 7).

    Figure 7: Generic LV network analyzed in this study

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    For an average consumption case and no PV generation, the voltage profile in this network

    would look as inFigure 8.

    Figure 8: Voltage profile in the generic LV network for average consumption levels and no PV generation

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    2.6

    Statistical Data Used for Consumption and Generation

    In order to obtain realistic results, several sets of historical data have been used. Statistical

    and historical energy consumption and generation data are presented in this section.

    2.6.1

    Electrical energy consumption

    The electrical energy consumption in the residential sector in Denmark has been obtained

    at an hourly rate for one typical year as can be seen inFigure 9.A total of 8760 sample points are

    stored. The plotted values are normalized to the maximum hourly recorded consumption value

    through the entire year. This data will be later normalized to the average yearly consumption level

    of one Danish residence which in 2009 was 3.44 MWh [22].

    Figure 9: Electrical energy consumption over one year for a typical Danish residence.

    2.6.2

    PV generation

    For PV generation yearly profile data, synthesized values (using PVsyst) for one location in

    Denmark have been used as shown inFigure 10 andFigure 11 at an hourly time sample. In order

    to make use of these data a simple linear scaling to any other inverter with different power ratinghas been done. Therefore, if considering a 2 kW PV system, all the production values have been

    multiplied by 2 thus obtaining the equivalent production data for a 2 kW reference system size.

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    Figure 10: Yearly synthesized PV production data for Brdstrup, Denmark, of a 1 kWp PV plant

    Figure 11: Power generation each hour of day for a 1 kWp PV unit for Brdstrup, Denmark, during one year

    The data shown inFigure 10 andFigure 11 corresponds to a PV system oriented to south and

    with an inclination of 45%. To have a better understanding of the difference between yearly

    production levels and peak production for different types of PV systems,Table 3 is shown below.

    In this report, in order to address the worst case scenario for PV panel orientation, all PV systems

    installed are pointing south with an inclination of 45 degrees, marked with green inTable 3.

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    PV Orientation [] PV inclination [] Peak hourly

    produced energy

    [Wh]

    Total produced energy

    [kWh]

    -90 (west) 30 870 895

    -45 (west) 30 892 1021

    0 30 850 1066

    45 (east) 30 864 1013

    90 (east) 30 809 884

    -90 (west) 45 888 847

    -45 (west) 45 918 1004

    0 45 940 1059

    45 (east) 45 876 995

    90 (east) 45 798 833

    0 20 825 1043

    Table 3: Peak and yearly PV production for different orientations of a 1 kWp PV system in Brdstrup,

    Denmark, (synthesized data from PVsyst)

    2.7

    Simulation model

    2.7.1

    Dynamic inverter model description

    The dynamic model of the inverter is a three-phase RMS model. It supports several

    operating modes:

    o

    Normal mode: Q = 0o Local Q(U) mode

    o Local PF(P) mode

    o Constant PF mode

    o Constant Q mode

    A functional diagram of the implemented model is shown inFigure 12.The AC active power

    output data is used by the PF(P), constant power factor and by the apparent power rating

    limitation block P,Q limit. The control mode switch is operated by a separate reference signal.

    The measured RMS voltage of the connection point is used to compute the reactive power

    contribution in case of Q(U) operation mode. The AC grid block is entirely describing the

    components in the AC grid and modeled within Power Factory DIgSILENT grid diagrams. The

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    inverter model injects balanced, three phase currents. In steady state the inverter will act as a

    constant power source.

    PV power

    P

    Q

    P,Q

    limit

    Pout

    Qout

    AC

    Grid

    Urms

    Q

    U

    Control

    Mode

    Cos )

    P

    Const Q

    Const

    PF

    Q=0

    Figure 12: PV inverter RMS model

    2.7.2

    Dynamic AC load modeling

    A simple AC load model has been developed in Power Factory to model the consumption of

    a typical consumer connected to the LV network. A reference power factor has also been used.

    Throughout the simulations, for simplicity, a constant power factor 0.95 inductive has been

    selected.

    P consumptionP

    P,Q

    calculation

    Pout

    Qout

    AC

    Grid

    Cos()

    Figure 13: AC load RMS model

    2.8

    Simulation study cases

    To the base network of Figure 7, PV inverters have been added to each consumer and

    different PV penetration levels have been chosen as inTable 2.Additionally, a very simple 10 kV

    MV network has been included to model the voltage variations in the 10 kV network. The lengths

    of the MV cables have been intentionally increased in order to simulate a high impedance MV

    network. Also, to represent a cluster of 10/0.4 distribution networks a simple aggregated model of

    the reference network of Figure 7 has been added. Details regarding the components are

    documented inAppendix A.The resulting electrical network is shown inFigure 14.

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    Aggregated

    distribution

    networks

    P,Q

    4

    Figure 14: Generic network with PV generation at each consumer. The indicated number of inverters in the

    boxes means a lumped inverter model.

    Themain assumptionsfor all study cases are:

    Hourly samples for both PV generation and AC loads consumption are used. This translates

    as described in Section2.7.1. PV irradiation profile is the same for each connected inverter in the network. This

    assumption can be considered valid if the simulation is done on hourly measurement samples.

    Local loads follow a similar consumption curve, each load varying from the reference

    measurement with a maximum of +/- 10%; All loads are three phase balanced.

    The same control characteristic is set for each PV inverter in the network.

    All PV inverters are balanced, three phased units. All PV inverters have the same power

    rating as described in Section2.2.

    The relevant parameters used to select different study cases are documented in Section2.3.

    Additionally, two more sizes of the LV/MV transformer have been selected (160 and 200 kVA) in

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    order to observe the influence of the transformer rating to the overall Q(U) and PF(P) efficacy.

    Considering a 60% PV penetration in the generic LV network, this will correspond to 213 kW PV

    capacity. Hence, the biggest chosen value for the connecting transformer is 200 kVA. Since in the

    cases of PV penetration higher than 30% the rating of the cables may also be exceeded an analysis

    of the cables loading is also of interest. The simulated study cases are shown inTable 4 for Q(U)andTable 5 for PF(P).

    For Qminand Qmaxequal to 0.6 p.u. values inTable 4,this corresponds to a maximum active

    power of 0.8 p.u. for the apparent power S= 1. Study cases 5 and 6 are using different maximum

    intervals: for case 5 a Qminand Qmax equal to 0.48 p.u., while for case 6 a Qminand Qmax equal to

    0.4 p.u. Thus, the minimum power factor is equal to 0.8 (lagging & leading) in the Q(U) cases

    2,3,4,8 and 10. To make a better comparison of Q(U) against PF(P) control as defined in VDE AR-N

    4105 [23] study cases 5 and 6 are performed. For these cases the equivalent minimum power

    factor (when voltage is at overvoltage limit) is 0.89 and 0.92 respectively.

    Studycase

    no.

    PVpenetration

    [%]

    [pu]

    [pu]

    [pu]

    [pu]

    Voltagesensitivity

    m

    [pu]

    [pu]

    Trafo

    [kVA]

    1 0:10:60 1 1 0 0 0 1 1 100

    2 0:10:60 0.9 1.1 -0.6 0.6 6 1 1 100

    3 0:10:60 0.9 1.1 -0.6 0.6 7.5 0.98 1.02 100

    4 0:10:60 0.9 1.1 -0.6 0.6 10 0.96 1.04 100

    5 0:10:60 0.9 1.1 -0.48 0.48 4,8 1 1 100

    6 0:10:60 0.9 1.1 -0.4 0.4 4 1 1 100

    7 0:10:60 1 1 0 0 0 1 1 160

    8 0:10:60 0.9 1.1 -0.6 -0.6 6 1 1 160

    9 0:10:60 1 1 0 0 0 1 1 200

    10 0:10:60 0.9 1.1 -0.6 -0.6 6 1 1 200

    Table 4: Simulated study cases and chosen parameters for Q(U) control strategy

    Study

    case

    no.

    PV

    penetration

    [%]

    Trafo

    [kVA]

    Maximum

    PF (lagging)

    11 0:10:60 100 0.95

    12 0:10:60 160 0.95

    13 0:10:60 200 0.95

    Table 5: Simulated study cases and chosen parameters for PF(P) control strategy

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    3 ResultsEach study case provides numerous results to be analysed. Due to the high number of

    parameters that can be observed for each case, only the base case (no. 1) will be shown in Section

    3.1, while the complete set of results can be viewed in Appendix B. Moreover, a comparison

    between the study cases is of greater interest and will be discussed in Sections3.2 and onwards.

    3.1

    Results of the base study case

    Study case 1 represents the situation in which the PV inverters have no voltage control

    algorithm implemented. It is also assumed that the low voltage side of the 60/10 kV transformer is

    dispatched to a constant 0.995 per unit voltage level, as depicted in Figure 1. The 10/0.4 kV

    transformer is using a constant tap position resulting in a +2.5% voltage increase at the secondary

    side.Figure 15 andFigure 16 display the minimum and maximum year round voltage levels at each

    busbar of feeder 1 and 2 respectively for variable PV penetration levels from 0 to 60% in steps of10% as inTable 2.

    The voltage level is represented by vertical bars of different width for each PV penetration

    level. On the horizontal axis, the voltage of each busbar is ordered from left to right according to

    the electricaldistanceto the transformer. The first set of vertical bars (left most) corresponds to

    the voltage at the primary side of the 10/0.4 kV transformer, while the second set of bars

    corresponds to the secondary side.

    It is obvious that at the outermost busbar (vertical bars on the right) the highest voltage

    variations will be observed (bus 360 inFigure 14). The minimum voltage value for a specific busbar

    is the same for all PV penetration levels since at maximum load hours (during evening) no changes

    are performed by the PV inverters. Increasing the PV penetration to 60% will result in a high

    maximum voltage increase of approximately 1.17 per unit in feeder 1. A smaller variation is

    observed in feeder 2 (app. 1.13 p.u. voltage for 60% PV penetration at the outermost distribution

    box bus 9925 in Figure 14) since the cable distances are smaller, as well as the number of

    customers being serviced.

    InFigure 15 andFigure 16 there are also shown the +/-10% voltage limits. It can be seen that

    for PV penetration levels higher than 30% (excluded) the allowed voltage variation is exceeded in

    feeder 1. These 2 feeders will therefore be declared as being challenged for a PV penetration level

    higher than 30%, corresponding to 107 kW. Thus, their hosting capacity is said to be 30%.

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    Figure 15: Study case 1 - Maximum/Minimum yearly voltage for each bus of feeder 1 for variable PV

    penetration

    Figure 16: Study case 1 - Maximum/Minimum yearly voltage for each bus of feeder 2 for variable PV

    penetration

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    Figure 17 displays an overview of the simulated voltage levels at different relevant points in

    the network and for different penetration levels. This locus plot is shown in connection with the

    allowed voltage limits in each point. If analysing the locus of the voltage for the outermost

    distribution box it can be seen that the maximum PV penetration level would be just below the

    30% marker, which also is the case for most of the other locations in the network.

    Figure 17: Study case 1voltage locus at different points in the network and different PV penetration levels

    Figure 18 shows the evolution of the transformer loading (in per cent) when an increasing

    amount of PV penetration is installed in the LV network (as inTable 2). The graphic represents a

    histogram plot viewed from above. Therefore, it can be observed that irrespectively of the PV

    penetration, most of the hours in a year are spent by the transformer under a loading from 10 to

    40%. Also, by increasing the PV penetration it is seen that the peak at 40% loading is shifting

    towards the 20% loading. This could potentially increase the life-time of the transformer. The

    uncoloured regions represent zero hours of operation at that specific loading level. For PV

    penetration levels lower than 30% (and including) the peak transformer loading occurs during

    hour 18:00 the 25th

    of December.

    Furthermore, due to increasing PV power capacity for PV penetrations higher than 30%,there appear a few hours per year with a very high transformer loading (at noon, mostly during

    spring). For a 60% PV penetration the transformer is maximally loaded at approximately 150%.

    This overloading coincides with high reverse power generation of the transformer and has a

    duration of not more than 2 hours per occurrence (3 times per year) as shown inTable 6.It can be

    seen that in this specific case of the Bornholm generic network, the limiting parameter for

    increased PV generation is also the transformer rating. The hosting capacity of the transformer is

    therefore around 40%, corresponding to 142 kW PV power, when all PV systems are pointing

    south. When the PV systems are scattered, the hosting capacity could increase up to

    approximately 160 kW, corresponding to a 45% penetration.

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    Figure 18: Study case 1Histogram of the yearly transformer loading for variable PV penetration (legend

    hours per year)

    PV

    penetration

    [%]

    Number of hours for a loading level at:

    100% 110% 120% 130% 140% 150%

    0 1 0 0 0 0 0

    10 1 0 0 0 0 0

    20 1 0 0 0 0 0

    30 1 0 0 0 0 0

    40 14 0 0 0 0 0

    50 142 76 27 3 0 0

    60 147 131 127 48 17 6

    Table 6: Study case 1 - Number of overloading hours of the 10/0.4 transformer

    Figure 19 displays the loading performance of the LV cable system in the network. A similar

    histogram as inFigure 18 has been plotted for the loading of the cables. For each hour in the year

    the maximum loading of any of the cables has been selected as the reference for the calculation.

    Based on these 8760 result points, the histogram ofFigure 19 is obtained while the PV penetration

    level is varied as in Table 2. The uncoloured regions represent zero hours of operation at that

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    specific loading level. A PV penetration of maximum 50% is possible without overloading the LV

    cables, corresponding to approximately 180 kW PV systems.

    Figure 19: Study case 1Histogram of the yearly cable loading (all maximum) for variable PV penetration

    (legendhours per year)

    As it is expected, the reactive power of the outermost located inverter is always zero for this

    study case, as shown inFigure 20.

    Figure 20: Study case 1No volt-VAr controlQ(U) locus plotsfarthest inverter

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    Figure 21: P(U) locus for Study case 1farthest inverter

    The active power losses of the distribution transformer, the LV cable system and the total

    losses for this simulation case are plotted inFigure 22.Each point represents the sum of the yearly

    losses of all LV cables in the distribution network for that specific PV penetration level. As in the

    case of the transformer losses, a minimum is reached for the 20% PV penetration level.

    Figure 22: Active power losses for Study case 1

    The transformer losses are varying slower than the cable losses when installing more PV in

    the network. The minimum power loss is achieved for a PV penetration level of 20%. This

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    minimum level is due to the fact that at 20% PV the power transfer in the network is minimized

    both in the generation and the load hours. As it will be seen in the cases for applying Q(U) control

    in the undervoltage region (practically this means the high load hours), the reactive power transfer

    will increase the power losses both in the generation and consumption periods. To understand the

    magnitude of potential energy savings in study case 1 for 20% PV installations one intuitivecalculation is given. Subtracting the total power losses at 20% PV from the value at 0% PV more

    than 800 kWh can be saved per year. With 957 10/0.4 kV stations on Bornholm [24] with the same

    rated power as here, a 20% PV penetration would save 766 MWh energy per year, which

    corresponds to the average consumption of 220 households.

    The active power transfer at the MV side of the distribution transformer is displayed in

    Figure 23.Minimum, maximum and average values are shown. It can be observed that there are

    high differences between the average and the minimum/maximum recorded values, especially in

    cases of high PV penetration.

    Figure 23: Active power transfer through 10/0.4 kV transformerStudy case 1

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    The reactive power transfer at the MV side of the distribution transformer is displayed in

    Figure 24.Since the load profile is not changing there are no visible modifications to the reactive

    power consumption during a full day.

    Figure 24: Reactive power transfer through 10/0.4 kV transformerStudy case 1

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    3.2

    Overview of comparisons between the simulated results

    Starting from this base case, several comparisons have been performed on the obtained

    results of all of the simulated study cases. A synthesis of the contents of this Section is shown in

    Table 7.

    Study

    case

    Deadband

    evaluation

    Voltagesensitivity

    w&w/oQ(U)

    100/160/200kVA

    NoQ(U)

    100/160/200kVA

    Q(U)

    100/160/200kVA

    PF(P)

    Q(U)vs.PF(P)

    1 X X X x

    2 X X X x

    3 X

    4 X

    5 X

    6 X

    7 X

    8 X

    9 X

    10 X

    11 X x

    12 X

    13 X

    Table 7: Comparisons performed between different study cases

    Figure 25 displays a comparison of all study cases regarding the active power losses of the

    distribution transformer. It can be observed that no significant changes are present. For the NO

    PV case the power losses are around 2.77 MWh for a 100 kVA unit, 3.8 MWh for a 160 kVA unit

    and 4.5 MWh for a 200 kVA unit. It can be seen that by increasing the PV power penetration, a

    minimum of the transformer losses is achieved at the 20% PV level, irrespective of the simulated

    study case. Even for a 30% PV generation level, the transformer losses are kept below the NO PV

    case, while at 40% a slight increase is observed.

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    3.3

    Varying the dead-band of the Q(U) controller

    By varying the dead band of the Q(U) controller, one may get a good impression of the

    influence this dead band has upon the voltage regulation capability of the inverters. Figure 27

    shows the Q(U) scatter plots for the two applied dead bands (+/-2% and +/-4%) and the case withno dead band selected for the inverter at the outermost distribution box. It can be easily observed

    that the bigger the dead-band the steeper the Q(U) curve will be in the active region. Additionally,

    the plot shows also that by applying a dead band, the maximum voltage (during one year) will

    increase at that specific inverter terminals. Still, even for an 8% dead band the maximum voltage

    will still be lower than the maximum in the case of no Volt-VAr control.

    Figure 27: Q(U) locus plots for variable Q(U) dead bandfarthest inverter

    A good overview of the influence of different dead band selection is seen inFigure 28.It can

    be observed that in the case of using a Q(U) control scheme with no dead band, the highest

    voltage regulation capability is obtained at the outermost distribution box (case (b) shown in

    figure). Therefore, if comparing the case of having no Volt-VAr control (a) with the case (b) the PV

    penetration level can be increased from below 30% to more than 40%. If applying a dead band (as

    in cases (c) and (d)) the efficacy of the reactive power control method decreases slightly but still

    providing a higher PV penetration level than in the base case (a). Note that the minimum voltage

    level in case of Q(U) is increased in Figure 28, since the inverters also exchange reactive power

    with the network during the night (corresponding to the locus in the left half side ofFigure 27).

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    Figure 28: Comparison of different deadband settings - voltage locus for specific points in the network (with

    variable PV generation)

    Figure 29 displays a comparison between the transformer yearly power losses when varying

    the dead-band of the Q(U) controller. As it is expected, a larger dead-band would result in lower

    losses in the transformer. For the case with no dead-band and a 40% PV penetration level there is

    an increase in the transformer loss of only 7 % compared to Study case 1 No Volt VAr Control.

    Figure 29: LV transformer power losses for variable Q(U) dead band study cases

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    The total cable losses are shown in Figure 30.As expected, by adding a dead-band to the

    controller the total power losses are being decreased compared to Study case 2 Q(U) no dead-

    band. At 40% PV penetration level an increase of around 35% is observed compared to Study

    case 1No Volt VAr Control

    Figure 30: LV Cable system total power losses for variable Q(U) dead bands

    3.4

    Varying the voltage sensitivity of the Q(U) controller

    By varying the voltage sensitivity of the Q(U) controller a less steeper reference curve is

    programmed in the inverter, resulting in a lower reactive power injection for the same variation of

    input voltage. The voltage sensitivity m (as defined inEquation 2)of the compared study cases is

    shown inTable 8.

    Study case number Voltage sensitivity m

    1 0.0

    2 6.0

    5 4.8

    6 4.0

    Table 8: Chosen voltage sensitivities for compared cases

    This can be easily observed inFigure 31.The consequence is that the PV inverter will be able

    to control less the terminal voltage, reaching a maximum of 2% voltage decrease when comparing

    study case 1 and 6.

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    Figure 31: Q(U) locus plots for variable voltage sensitivityfarthest inverter

    An overview of the influence of variable voltage sensitivity settings towards the maximum

    and minimum simulated voltage levels is shown inFigure 32.It is observed that by lowering the

    Q(U) slope of the Q(U) characteristic the maximum observed voltage at the outermost distribution

    box increases.

    Figure 32: Comparison of different voltage sensitivity settings - voltage locus for specific points in the

    network (with variable PV generation)

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    Figure 33 describes the transformer losses for variable Q(U) voltage sensitivity. The results

    are similar between each other, a decrease in total power losses being observed for decreasing

    sensitivity levels and high PV generation levels. For smaller PV penetration levels there are no

    significant differences, since the reactive power flow is also at minimum.

    Figure 33: LV transformer power losses for variable voltage sensitivity study cases

    The LV cable system power losses are shown in Figure 34. While for low PV penetrationlevels the total losses are decreased by using Q(U) control, from the 30% generation level there

    are increased losses in comparison to the No Volt VAr Control case. For a 60% PV penetration

    the cable losses are doubling between Study case 1 and 2. By decreasing the voltage sensitivity

    (Study cases 3 and 4) the power losses in the cables are also decreased.

    Figure 34: LV cable system losses for variable voltage sensitivity

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    Several diagrams of the reactive power transfer for variable voltage sensitivity and different

    PV penetration levels are displayed in Figure 35,Figure 36 and Figure 37.By analysing all these

    figures, it is observed that a minimum of reactive power transfer (on average) is achieved for PV

    penetration levels from 10 to 30%. If observing the curve for Study case 2 with PV generation

    levels of 10% inFigure 35, it can be seen that it provides the minimum reactive power transferround the clock at the transformer site. If the PV generation increases, there will be an even

    larger amount of inductive reactive power transfer at the MV side of the transformer during the

    noon hours, and a capacitive reactive power transfer during the high load hours in the evening.

    Figure 35: Reactive power at MV side of transformer for varying voltage sensitivity of Q(U) (0,10,20%PV)

    Figure 36: Reactive power at MV side of transformer for varying voltage sensitivity of Q(U) (0,30,40%PV)

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    Figure 37: Reactive power at MV side of transformer for varying voltage sensitivity of Q(U) (0,50,60%PV)

    3.5 Comparison for varying the transformer power rating with and without Q(U)

    voltage control

    The influence of upgrading the 10/0.4 kV transformer upon the maximum/minimum voltage

    limits is shown in Figure 38. Comparing base case (a) 100 kVA unit with a higher ratingtransformer it can be observed that the maximum simulated voltage at the outermost distribution

    box is slightly increasing while the minimum value is slightly decreasing. The overall effect is that

    although solving the overloading problem, the voltage at the feeder ends may slightly increase.

    Figure 38: Comparison of normal operation (No Q control) with different LV/MV transformers - voltage locus

    for specific points in the network (with variable PV generation)

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    An overview of the influence of upgrading the 10/0.4 kV transformer towards the maximum

    and minimum simulated voltage levels is shown inFigure 39.

    Figure 39: Comparison of Q(U) with different LV/MV transformers - voltage locus for specific points in the

    network (with variable PV generation)

    Figure 40 displays a comparison between the transformer yearly power losses when using

    Q(U) and upgrading the transformer power rating.

    Figure 40: LV transformer power losses for variable Q(U) dead band study cases

    200 kVA

    160 kVA

    100 kVA

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    3.6

    Comparison for varying the transformer power rating with PF(P) voltage

    control

    Using a power factor depending on the injected PV power level, PF(P), has the primary

    objective to decrease the voltage level only at the moment the PV inverter is producing power.This has the advantage that the inverter will not produce reactive power outside the production

    times and also it will be independent of the location of the inverter in respect to the distribution

    transformer. One disadvantage may be that it will inject reactive power even at times when it is

    not necessary e.g. voltage is well within limits. Study cases 11, 12 and 13 use inverter models with

    the PF(P) reactive power control.

    The PF(P) scatter plot is shown in Figure 41. With small exceptions there is no significant

    difference when using each of the three types of transformers.

    Figure 41: PF(P) locus plot of farthest located inverter

    The transformer power losses can be observed inFigure 42.It is obvious that by upgrading

    the MV/LV transformer the overall power losses will increase due to higher no-load losses. By

    upgrading to a 200 kVA from 100 kVA transformer, the transformer losses will increase by 50%.

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    Figure 42: Losses in the 10/0.4 transformer - Comparison for different power ratings of transformer and use of PF(P)

    control

    As it was expected, the power losses on the cables have no significant changes irrespective

    of the PV generation level, as shown inFigure 43.

    Figure 43: Losses in the LV cables - Comparison for different power ratings of transformer and use of PF(P) control

    200 kVA

    160 kVA

    100 kVA

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    3.7

    Comparison of Q(U) and PF(P)

    A small comparison between the efficacy of Q(U) and PF(P) control algorithms is shown in

    Figure 44.In all displayed cases the transformer used was fixed to a 100 kVA rating. Plot set (a)

    corresponds to Study Case 1 and represents the voltage levels in different points of the networkwithout using any reactive power control strategies. Plot set (b) corresponds to Study Case 2 and

    uses a higher maximum reactive power generation level than the PF(P) plot set (d). Finally plot set

    (c) corresponds to Study Case 6 which has a similar maximum reactive power generation level

    compared to PF(P). Both Q(U) control cases are contributing to lift the minimum voltage at the

    outermost distribution box while PF(P) has no influence.

    Figure 44: Comparison of Q(U) and PF(P) - voltage locus for specific points in the network (with variable PV

    generation)

    Figure 45 displays the transformer power losses in the power transformer. If comparing both

    Q(U) methods (Study case 2 and 6) with the PF(P) case it is observed that minimum power loss is

    achieved by using PF(P). This fact is normal since both Q(U) cases are injecting reactive power also

    during night (round the clock operation). Also note that by using Q(U) at night time, the

    minimum voltage at the outermost distribution box is increased. Thus Q(U) could be used at nightin combination with lowering the tap-position of the MV/LV transformer. Q(U) at night could also

    be used to compensate for nightly heavy duty loads, e.g. heat pumps and electrical vehicles. For a

    60% PV penetration level, the PF(P) algorithm increases losses by 3%, the Q(U) study case 6 by

    13% and Q(U) study case 2 by 20%.

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    Figure 45: Losses in the 10/0.4 transformer - Comparison between the use of PF(P) and Q(U) control

    The losses in the LV cables when using PF(P) and Q(U) control types is shown in Figure 46.

    The same dependency as in the case of transformer power losses fromFigure 45 is observed. In

    the case of 60% PV generation, for PF(P) control the losses increase by 8%, for Q(U) study case 6

    by 60% and for Q(U) study case 2 by 95%.

    Figure 46: Losses in the LV cables - Comparison between the use of PF(P) and Q(U) control

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    3.8

    Comparison of hosting capacity for the cases

    The results from 13 study-cases are compiled inTable 9.The cases are rearranged in order of

    hosting capacity. The first column shows the hosting capacity for the particular case seen from an

    overvoltage and a transformer loading perspective; the second is the case-number and the third isa short description of the case. The fourth column is the maximum amount of exchanged reactive

    power for the inverters at the outermost distribution box and the fifth column is the

    corresponding PF. The sixth column shows the yearly energy losses in the transformer and cables

    and finally the seventh column shows the maximum exchanged reactive power through the

    transformer into the MV network.

    Hosting capacity

    [%]

    O.V. / Trafo

    Study

    Case

    Note Maximum Q

    outermost

    PV inverter

    [p.u.]

    Minimum PF

    outermost PV

    inverter

    (lagging)

    Yearly

    energy

    loss

    [MWh]

    Maximum hourly

    reactive power

    exchange through

    transformer [kVArh]

    30% 40-50% 1 Base case 0.0 1.00 5.5 -30 (ind)

    30% n.a. 7 160 kVA trafo 0.0 1.00 6.6 -30 (ind)

    30% n.a. 9 200 kVA trafo 0.0 1.00 7.3 -30 (ind)

    35% ~40% 11 PF(P) -0.25 0.97 6.0 -53 (ind)

    35% n.a. 12 160 kVA trafo

    PF(P)

    -0.25 0.97 7.1 -52 (ind)

    35% n.a. 13 200 kVA trafo

    PF(P)

    -0.25 0.97 8.6 -53 (ind)

    40% 30-40% 6 Q(U)

    low sens.

    -0.4 0.92 7.0 -66 (ind)

    40% ~40% 4 Q(U)

    8% dead band

    -0.6 0.8 6.8 -72 (ind)

    40% 30-40% 5 Q(U)

    mid sens.

    -0.5 0.87 7.2 -74 (ind)

    40% n.a. 10 200 kVA

    Q(U)

    -0.6 0.8 9.5 -91 (ind)

    45% 30-40% 3 Q(U)

    4% dead band

    -0.6 0.8 8.2 -93 (ind)

    45% n.a. 8 160 kVA

    Q(U)

    -0.6 0.8 10 -104 (ind)

    47% 30-40% 2 Q(U) -0.6 0.8 10 -98 (ind)

    Table 9: Comparisons of hosting capacity for the 13 cases, in increasing order. For the loading of the

    transformer: a range is given when the sum of overloading hours is higher than 86 hours per year and an

    approximate value is given when the sum is below 86 hours per year.

    Case number 1 is the first entry with a hosting capacity of 30% (1.5 kWp per residence)

    without taking any reactive power control measures into consideration. Increasing the capacity of

    the transformer (cases 7 and 9) does not increase the hosting capacity when overvoltage is the

    issue. Thus, case 1 is marked green as the optimum solution for the 30% penetration.

    The usage of the standard PF(P) in case 11 increases the hosting capacity to 35% (1.8 kWp

    per residence). The maximum hourly exchange of reactive power is increased from 30 to 53 kVArh

    and the yearly losses in the transformer and cables are increased with 500 kWh. Again, using the

    PF(P) with large transformers does not increase the hosting capacity. Therefore, case 11 is marked

    green as the optimum solution for the 35% penetration.

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    The hosting capacity is increased further to 40% (2.0 kWp per residence) in case 6 by

    applying Q(U) control with a low sensibility. This could also be achieved with the Q(U) scheme with

    high sensibility and 8% dead-band, but this would increase the exchange of reactive power

    through the transformer. The yearly energy loss is increased with 1.5 MWh compared with the

    base case and using a large transformer does not have any impact on the hosting capacity.Consequently, case 6 is marked green as the optimum solution for the 40% penetration.

    A hosting capacity of 45% (2.3 kWp per residence) requires Q(U) control with high sensitivity

    and 4% dead-band as in case 3 and can be further increased a few per cent by removing the dead-

    bands as in case 2. However, the transformer is being overloaded to some extent.

    The hosting capacity for the 100 kVA transformer is in section3.1 found to minimum 40%

    and maximum 50%, corresponding to a minimum of 140 kW PV systems, when the PV systems are

    pointing south. If the PV systems are scattered, the hosting capacity is increased to 45%, which

    corresponds to a total of 160 kW PV systems. In both cases, no voltage control is applied. The

    PF(P) control scheme decreases the hosting capacity of the transformer to around 40% and usingthe Q(U) with low sensitivity reduces it even further to minimum 30% and maximum 40%. The

    scale 30% - 50% corresponds to 120 kWp200 kWp when the systems are scattered.

    A PV penetration of maximum 50% is possible without overloading the LV cables,

    corresponding to 180 kW PV systems, when no voltage control is applied. Applying voltage control

    will decrease the hosting capacity of the LV cables due to the additional reactive current.

    According to [24], there are 957 MV/LV transformers on Bornholm with a total of 28 000

    private and commercial customers. The peak demand is 55 MW and the yearly energy

    consumption is 268 GWh. When each of the 28 000 customers have a PV system and by using the

    results obtained in this research, the hosting capacity of the LV feeders on Bornholm is in the

    range 4256 MW, when all systems are pointing south. If the PV systems would be scattered, the

    range is 4864 MW. Assuming that each of the 957 transformers can host 140 160 kW PV, the

    hosting capacity of the transformers is within the range 130 MW 150 MW. Summing up, the

    hosting capacity of the LV networks and MV/LV transformers on the island of Bornholm is in the

    range 50 60 MW, which could cover the peak demand (during noon hours) and 15-20% of the

    yearly energy consumption.

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    Another interesting result is the advantage of using Q(U) feature of the PV inverters even for

    low PV penetration levels. For example, at 20% PV generation, the PV inverters can supply reactive

    power to AC loads (even at evening hours) and thus minimizing the reactive power flow in the

    network. As a consequence, the power losses in the transformer and cable system are lowered

    slightly.

    The results indicate that without any Volt-VAr control the overvoltage phenomena starts for

    PV generation levels at 30%, corresponding to 1.5 kW PV per residence.

    By applying a PF(P) control scheme as in study case 11, the overvoltage condition is avoided

    and the PV penetration can be increased to 35% and still keep the amount of exchanged reactive

    power low. By applying a Q(U) control scheme with a low sensitivity as in study case 6, the

    overvoltage condition is avoided up to 40% PV penetration and still keeping the power factor

    above 0.92. Finally, by using Q(U) with high sensitivity and dead-band, study case 3, the

    penetration can be increased further to 45% and perhaps also to 50% if the dead-band is removed

    as in study case 2. However, the yearly losses in the transformer and cable system are almostdoubled compared with the base case with only 30% penetration.

    One more conclusion that can be drawn is that the overvoltage phenomena is not overcome

    by upgrading the transformer, on the contrary increasing the size of the transformer has a slight

    negative effect. Transformer upgrading should be taken into consideration only with the purpose

    of mitigating the transformer overloading issues.

    If reactive power control is provided round the clock then the PV inverters can help

    controlling the voltage during high load hours, e.g. during charging of electrical vehicles or when

    the heat pumps are turned on in order to utilize free energy from the wind -turbines. For the

    case of 40% PV penetration the minimum yearly simulated voltage has improved from 0.91 p.u. to

    0.93 p.u. (an increase of 2%-point). This feature may allow the PV penetration level to be

    increased even further by lowering the tap position in the 10/0.4 distribution transformer

    provided that sufficient PV capacity is installed in order to provide reactive power during the load

    peaks.

    For PV generation levels lower than and including 30% the 100 kVA transformer will not be

    subjected to overloading. The peak-load of the transformer is reduced for PV penetrations up to

    20%. This could potentially increase the life-time of the transformer. For 40% PV penetration

    levels, a limited amount of overloading hours are observed, thus having a limited impact over the

    lifetime of the transformer. The hosting capacity of the transformer is therefore around 40%,

    corresponding to 142 kW PV power, when all PV systems are pointing south. When the PV systemsare scattered, the hosting capacity could increase up to approximately 160 kW, corresponding to a

    45% PV penetration. For higher PV penetration levels, additional solutions must be applied:

    increased self-consumption, storage solutions, transformer upgrading or active power curtailment.

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    4.2

    Recommendations for voltage control in LV feeders

    As a guiding rule, if overvoltage is observed at the end-customer site the following order of

    actions should be followed:

    1.

    Apply PF(P) for all inverters on the feeder2. Apply Q(U) for all inverters on the feeder

    3. Lower the tap position in the LV/MV transformer and apply Q(U) round the clock

    4. Increase self-consumption at peak production hours

    5. Lower active output power of inverters (only in emergency cases for short periods)

    6. Upgrade cables, upgrading the transformer does not help

    7. Install storage

    Overall, it has been found that applying reactive power control strategies in the LV networks

    have a beneficial influence in respect to a limited increase of the PV penetration. Both PF(P) and

    Q(U) control types are improving the maximum voltage profile at the outermost distribution box.

    Only by using Q(U) round the clock, thus by providing capacitive reactive power during high AC

    load hours, it is possible to provide an improvement of the minimum voltage profile.

    4.3

    Future Work

    The work presented in this report provides a starting point for other more in depth analyses.

    One example is redoing the simulations of Chapter2.8 on a large number of grid types. Such

    an exhaustive approach would offer a much better indication of the actual efficacy of the reactive

    power control techniques for many types of LV networks. Moreover, one reactive power control

    technique may be recommended for one network type while it would have negative impact on a

    different type. Another possibility may come from the need of applying different control strategiesdepending on seasonal, daily and hourly schedules.

    Finding an optimum generic Q(U) curve could also be investigated. For this reason, one

    suggestion is shown in Figure 47. The main objective of the curve is to provide higher voltage

    sensitivities to the inverter connected closer to the transformer terminals.

    U

    Q

    96,0

    102.5,0

    105,33

    110,44

    Figure 47: Proposed Q(U) curve for further analysis

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    Several more study cases could be performed on Q(U) and PF(P) where not only one PF(P)

    reference is given but several. Each PF(P) curve could then be compared with its similar

    counterpart in terms of maximum reactive power contribution. Additionally, several Q(U) curves

    with dead band and fixed voltage sensitivity (varying end point) could be selected and analysed.

    One more study case could be performed with a different set value for the fixed tap position ofthe 10/0.4 kV transformer, e.g. neutral position, together with Q(U). Also Q(U) and PF(P) curves

    which generates the same amount of reactive energy should be compared, as well as curves which

    have the same limits for exchange of reactive power.

    One additional future study direction is the analysis of more advanced reactive power

    control algorithms such as Q(U,P) or PF(U,P) documented in [5]. An optimized control would

    ensure minimum reactive power injection from the PV inverters to avoid overvoltage phenomena

    and thus would minimize the power losses in the AC cables.

    As another possible future analysis, the same subject can be studied with the inclusion of

    new and modern types of consumers. Heat pumps and electrical vehicles (EV) are showing strongmomentum in mass deployment. The influence of these consumer types towards the PV inverter

    performance can be thus analysed. A more detailed modelling of the EV units can be developed

    and thus smart storage control algorithms may be included.

    This report provides a starting point for additional economic analyses on the total cost of

    using reactive power control methods in LV networks in order to increase the PV penetration level.

    These cost analyses may include the cost of energy losses in the power network, the transformer

    lifetime expense when temporarily overloading it, as well as the amount of power factor

    correction capacity in the 60 kV station to cover peak generation hours. A comparison with the

    cost of upgrading the network in order to accommodate more PV can also be performed. This also

    includes the changes in transformer life-time as function of the PV penetration.

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    5Works Cited

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    [2] S. F. Jensen, Solceller Nu og i fremtiden, 30 01 2012. [Online]. Available:

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    [6] Dansk Energi, Solceller og spaendingsvariationer i 0.4 kV net, Copenhagen, 2012.

    [7] P. Esslinger, Studie Q(U), Technischen Universitt Mnchen, Mnchen, 2012.

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    6e4efe/$file/2ucd301118_a%20pcs100%20avr%20case%20study%20-%20english%20vers.pdf.

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    [13] L. Chia-Hung, . H. Wei-Lin, C. Chao-Shun and H. Cheng-Ting , Optimization of Photovoltaic

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    /Spannungskennlinie Q(U) fur Erzeugungsanlagen am Mittelspannungnetz, 2011.

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    6Appendix ALow voltage cable parameters:

    Cable name Busbar1 Busbar2 Type Length in km

    125LV_528 125LV 528 4X150 AL-M PEX 0,084

    125LV_533 125LV 533 4X95 AL-M PVIKS 0,03

    528_529 528 529 4X50 AL-M PEX 0,105

    528_1046 528 1046 4X50 AL-M PEX 0,033

    533_535 533 535 4X95 AL-M PVIKS 0,047

    533_534 533 534 4X50 AL-M PVIKS 0,103

    529_530 529 530 4X50 AL-M PEX 0,053

    529_531 529 531 4X95 AL PVIKS 0,076

    529_10150 529 10150 4X150 AL-M PEX 0,055

    529_10157 529 10157 4X150 AL-M PEX 0,003

    10146_10147 10146 10147 4X50 AL-M PEX 0,068

    535_536 535 536 4X95 AL-M PVIKS 0,068

    531_532 531 532 4X50 AL-M PEX 0,076

    531_540 531 540 4X50 AL-M PEX 0,056

    10150_10151 10150 10151 4X150 AL-M PEX 0,07

    10147_10148 10147 10148 4X50 AL-M PEX 0,072

    540_10149 540 10149 4X150 AL-M PEX 0,032

    10151_10152 10151 10152 4X150 AL-M PEX 0,026

    10151_10156 10151 10156 4X50