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SENSITIVITY BASED VOLT/VAR CONTROL AND LOSS OPTIMIZATION
By
ANURAG R. KATTI
A THESIS PRESENTED TO THE GRADUATE SCHOOLOF THE UNIVERSITY OF FLORIDA IN PARTIAL FULFILLMENT
OF THE REQUIREMENTS FOR THE DEGREE OFMASTER OF SCIENCE
UNIVERSITY OF FLORIDA
2012
c⃝ 2012 ANURAG R. KATTI
2
To my parents
3
ACKNOWLEDGMENTS
I thank all the people who have supported me over the duration of this thesis and
beyond. In particular I would like to thank my parents and my advisor Dr. Pramod
Khargonekar at the Dept. of Electrical and Computer Engineering. I would also like to
thank Dr. Wonsuk ”Daniel” Lee at the Dept. of Agriculture and Biological Engineering,
University of Florida for giving me the opportunity to work on interesting projects, my
friends and colleagues in the Precision Agriculture Laboratory. And last but not the
least, I would like to thank my friends and past roommates Diwakar Raghunathan, Kiran
Tumkur, Niki Nachappa and Ugandhar Reddy and all my friends over the years.
4
TABLE OF CONTENTS
page
ACKNOWLEDGMENTS . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 4
LIST OF TABLES . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 6
LIST OF FIGURES . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 7
ABSTRACT . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 8
CHAPTER
1 INTRODUCTION . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 9
2 OVERVIEW . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 12
2.1 Motivation . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 122.2 Distributed Generation . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 132.3 Distribution Networks . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 162.4 Voltage and Reactive Power Control . . . . . . . . . . . . . . . . . . . . . 18
3 PROBLEM DESCRIPTION . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 22
4 LITERATURE REVIEW . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 25
5 VOLTAGE-VAR CONTROL AND LOSS MINIMIZATION . . . . . . . . . . . . . 32
5.1 Voltage Sensitivity . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 325.2 Centralized Voltage Control and Loss Optimization . . . . . . . . . . . . . 34
5.2.1 Objective Function . . . . . . . . . . . . . . . . . . . . . . . . . . . 365.2.2 Constraints and Optimization Problem . . . . . . . . . . . . . . . . 39
5.3 Decentralized Voltage Control and Loss Optimization . . . . . . . . . . . . 395.4 Optimization Algorithm . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 42
5.4.1 Quadratic Programming . . . . . . . . . . . . . . . . . . . . . . . . 425.4.2 Particle Swarm Optimization . . . . . . . . . . . . . . . . . . . . . . 43
5.5 Results and Observations . . . . . . . . . . . . . . . . . . . . . . . . . . . 44
6 GENERATOR SITING AND SIZING . . . . . . . . . . . . . . . . . . . . . . . . 49
6.1 Generator Siting . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 496.2 Generator Sizing . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 536.3 Impact of DG Penetration on Loss . . . . . . . . . . . . . . . . . . . . . . 55
7 CONCLUSION . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 57
APPENDIX: FEEDER CONFIGURATIONS . . . . . . . . . . . . . . . . . . . . . . . 59
REFERENCES . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 61
5
BIOGRAPHICAL SKETCH . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 65
6
LIST OF TABLES
Table page
2-1 Comparison of voltage, current and loss with and without DG . . . . . . . . . . 19
5-1 Comparison of optimization performance for case 1 . . . . . . . . . . . . . . . 45
5-2 Comparison of optimization performance for case 2 . . . . . . . . . . . . . . . 46
5-3 Comparison of optimization performance for case 3 . . . . . . . . . . . . . . . 47
7
LIST OF FIGURES
Figure page
2-1 Schematic of a Power grid . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 16
2-2 N+1 load feeder with a distributed generator connected at the last node . . . . 19
2-3 Current drawn at different voltages for different load types . . . . . . . . . . . . 20
5-1 Sensitivity of 34 node feeder for four different DG positions . . . . . . . . . . . 33
5-2 Variation of sensitivity . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 35
5-3 No result condition of the 13 node feeder . . . . . . . . . . . . . . . . . . . . . 47
6-1 Sensitivity of 34 node feeder for six different DG positions . . . . . . . . . . . . 50
6-2 Sensitivity for a decreasing voltage profile . . . . . . . . . . . . . . . . . . . . . 50
6-3 Sensitivity for an increasing voltage profile . . . . . . . . . . . . . . . . . . . . . 51
6-4 Sensitivity of current to DG location . . . . . . . . . . . . . . . . . . . . . . . . 52
6-5 Sensitivity of power loss to DG location . . . . . . . . . . . . . . . . . . . . . . 53
6-6 Variation of losses for different penetration levels and number of DGs . . . . . 55
A-1 Schematic of IEEE 13 node test feeder . . . . . . . . . . . . . . . . . . . . . . 59
A-2 Schematic of IEEE 34 node test feeder . . . . . . . . . . . . . . . . . . . . . . 60
8
Abstract of Thesis Presented to the Graduate Schoolof the University of Florida in Partial Fulfillment of the
Requirements for the Degree of Master of Science
SENSITIVITY BASED VOLT/VAR CONTROL AND LOSS OPTIMIZATION
By
ANURAG R. KATTI
May 2012
Chair: Pramod KhargonekarMajor: Electrical and Computer Engineering
The objective of this study is to control voltage at different points in a distribution
grid to within a specified range and minimize power loss. Sensitivity coefficients are
used to determine the reactive power dispatch of distributed generators connected in the
grid. Power loss is also represented in terms of sensitivity coefficients to simultaneously
optimize the voltage profile and power loss. Two variants of the optimization algorithm
are discussed - a centralized control algorithm based on the complete state of the
system and a decentralized algorithm using only the local information.
To study the influence of the location of generators in the grid, the properties of
sensitivity and its variation for different generator locations are studied. Two different
sensitivity coefficients - current and power loss sensitivity with respect to location of
generator are developed from the voltage sensitivity values. The use of these sensitivity
coefficients in siting and sizing of generators are discussed. And finally the influence
of the number of generators and penetration of distributed generation on voltage and
distribution loss are discussed through simulations.
9
CHAPTER 1INTRODUCTION
Distribution systems are the last stage in the delivery of power to the customer.
Power produced by generators is transported through the transmission network at high
voltages to distribution networks and delivered to the customer at the utility voltage
typically around 120V/240V for residential customers and possibly for other types of
customers with larger power requirements. The transfer of power from the substation -
the beginning of the traditional distribution system to the customer causes current to flow
downstream in the distribution grid. Currents in a circuit cause a voltage drop between
nodes and power loss in the conductor joining them. To deliver the maximum power
to the end user, the power lost during the transfer of energy must be minimized. Utility
companies must also ensure the quality of power at the output terminals. One aspect
of power quality deals with the voltage magnitude voltage at the outlets must not vary
more than 5% of the nominal voltage (120V) according to ANSI standards [1].
To ensure quality of power and provide the most efficient transfer of power, the
distribution company has to perform voltage control and loss minimization respectively.
In the traditional distribution grid, control was achieved by adjusting the taps on the
on load tap change transformer and voltage regulators or adjusting the reactive power
compensation of any capacitor banks or other compensation devices. To ensure the
most economical compensation, optimization was necessary. Because of the use of
reactive power (VAR) sources for compensation, the operation is called Volt/VAR control.
The optimization function could be the cost of compensation, the number of tap changes
since the lifetime of tap change transformers is limited, loss, etc.
In recent times however, there’s been a call to upgrade the distribution grid and
make it more smarter and allow it to handle power flow in the opposite directions as
well, among a list of other improvements i.e. allow for generators to be connected at
the distribution level (called distributed generators or DGs) and not just at the high
10
voltage (HV) level. This initiative has come to be known as smart grid and a few such
installations are already in development [2]. Customers who use generators for stand-by
power or cheap, alternative power are embracing the idea of DGs. This has encouraged
planners to envision a grid that can accommodate generators on the consumer
side from which the utilities can purchase excess energy during shortages. Such
improvements would make it unnecessary to buy more power or invest in expensive
generators to satisfy the growing demands.
While distributed generation has many advantages to offer, its effect on the grid is
still being studied, especially at high penetrations. In the current state of low penetration
of DGs in the grid, their effect is negligible. However, it is expected that the penetration
of DGs will increase in the future. Ambitious targets of 30% renewable penetration
in the US grid by 2030 have been made. Although not all of it is in the form of DGs,
they are expected to form a significantly large portion of renewable sources. European
countries already have a significant percentage of their generation produced by DGs
and renewable energy [3] and it is estimated to grow further in the future.
With the growing presence of DGs, studying its effects at high penetrations
becomes necessary because generators will affect the direction of power flow; their
effects need to be considered more carefully when multiple generators are connected at
multiple locations. Integration of new sources leads to problems with control, protection,
islanding and maintenance, to list a few. Multiple new sources embedded into the grid
would only complicate the matter. This study explores one aspect of integration of DGs
called Voltage/VAR Control which aims to control the voltage and power flow in the
distribution grid through VAR compensation using DGs. Another aim of this study is to
minimize loss during power flow in the distribution grid - called distribution losses.
Loss profile can also benefit from the proper placement of DGs on the grid; for
example, a thumb rule is line currents can be reduced by placing power sources close
to load centers. Since loss is directly proportional to the square of magnitude of line
11
current, reducing the line current reduces losses. Similarly, observations can be made
on sizing of DGs in a grid and the effect of higher penetration of DGs on the loss profile.
Sensitivity is a concept associated with the power flow Jacobian and is calculated
by inverting the Jacobian matrix. Sensitivity of a node denotes the change in voltage at
that node for a unit change in power at some node on the grid. If the power change can
be affected by a DG, sensitivity can indicate the amount of power output necessary to
effect a required change.
Based on the concept of sensitivity VVC, loss minimization, siting and sizing of
DGs and the effect of DG penetration on losses are studied. The study has been
organized as follows: chapter 2 discusses the motivation for the study and gives an
overview of distribution networks, distributed generation, the Voltage-VAR control
problem and distribution losses. Chapter 3 formulates the voltage/VAR control problem
mathematically. Chapter 4 lists past studies in Voltage-VAR control, use of distributed
generators for voltage control, distribution loss and optimization and a compensation
technique based on sensitivity. Chapter 5 discusses a modified algorithm based on
sensitivity to incorporate loss optimization in the Volt-VAR control problem. Chapter
6 discusses siting and sizing of DGs and the effect of increasing DG penetration in
distribution networks. Chapter 7 concludes the study with a note on the applications of
DGs, VVC and loss minimization using DGs and future work.
12
CHAPTER 2OVERVIEW
The power industry is experimenting with changes in the manner of power delivery
and new avenues of power generation and improvement in delivery are being sought.
The changes bring with them a new set of challenges and problems. This study aims
to tackle a small set of those challenges pertaining to the inclusion of distributed
generation and comment on the effect of increased penetration of these generators in
the grid and their effect on the distribution system losses.
2.1 Motivation
This study aims to accomplish a fourfold objective:
1. Voltage control with reactive power compensation using DGs2. Distribution loss minimization3. Siting and sizing of DGs4. Study the effect of increasing penetration of DGs in the distribution grid
Voltage control is a necessary operation required to be performed by a distribution
company to maintain power quality. Traditionally DGs haven’t been included in the
control operations but with the increasing number of DGs [4], [5], it may soon become
feasible to use them for control operations. DGs, especially the inverter interfaced DGs
have quick response rates and can respond quickly to changing conditions.
Losses are a big concern in electricity transmission and distribution. The U.S.
is among the biggest consumers of electric power but it loses over 260 billion kWh
every year - the highest in the world, despite having an efficient system that loses only
6% [6], [7]. The lost energy translates to a cost of about $20 billion [5], [7]. China,
with comparable power consumption to the U.S. loses less power in transmission and
distribution. European countries have a similarly efficient system. Smaller land area
also limits the losses in these nations. But larger countries like India and Brazil with
much lower consumptions than the U.S. lose nearly a quarter and a sixth of its energy
respectively in transmission and distribution. India is in fact second only to the U.S. in
13
the absolute amount of power lost (nearly 220 billion kWh). There is thus a need to
improve efficiency in both transmission and distribution for economic reasons.
Increasing distribution efficiency would also reduce the energy loss in the
transmission system due to the reduction in power transmitted over long lines. DGs
with their local siting offer the possibility of reducing energy transmission over long
ranges. Technological improvements in the field of renewable energy generation also
offers the possibility that further expansion in generation distributed or otherwise and
power consumption can be from clean energy with a smaller carbon footprint.
However a framework for their use and control needs to be developed. This study
is a step in that direction with control and compensation achieved using sensitivity
coefficients. Chapter develops the mathematical formulation of the voltage control
problem but a brief overview of the popular DG technologies, distribution systems and
voltage and loss control in sections 2.2 -2.4.
2.2 Distributed Generation
Distributed generation is a blanket term used to describe small scale power
generators that are connected at the distribution level or on the customer side of
power meter [8]. While there’s no consensus on the power output of DGs, most studies
consider outputs ranging from kilowatts (KW) to a few megawatts (MW) as distributed
generation. DGs have been classified in some studies [4] into micro: up to 5KW; small:
5KW-5MW; medium: 5MW-50MW; and large: 50MW-300MW.
Despite the growing interest and the reducing costs of renewable electricity such
as wind and solar, fossil fuel based generators are still the most economical and
reliable forms of generation and micro turbines are among the cleanest of combustion
based generators and when used as a cogeneration unit it can have efficiencies of
80% and above. Micro turbines burn fuel at high temperature and pressure and the
resulting fumes cause rotation of turbines blades at high speeds. When coupled with an
alternator, this produces electricity. Micro turbines can be designed for a wide variety of
14
fuels such as fuel oil, natural gas, etc. Micro turbines are small in size, clean and can
operate for long periods of time with low maintenance [8].
Fuel cells [8] generate electricity through electrons generated by an electrochemical
reaction. The electrons travel through the electrical circuit connected to the cell
producing direct current. Fuel cells require a constant supply of fuel - for example,
hydrogen to operate. Fuel cells can have an efficiency of over 50% even without CHP
and over 80% with cogeneration.
Unlike fuel based generators, renewables harness the natural sources of energy
which also makes them intermittent sources; for example: solar cells cannot work
efficiently on a cloudy day, a wind turbine cannot generate electricity when there is no
wind and droughts will halt production in a hydroelectric power station.
The most popular forms of renewable energy are solar-thermal power, solar
photo-voltaic cells but the most popular is probably wind energy. Wind energy has
been used to do work for a long time and they’re being used to generate electricity
as well. Wind turbines are designed to intercept the path of the wind which causes
rotation of the turbine blades. They are typically connected to an induction generator to
produce electricity but synchronous generators are in use as well [9]. To produce usable
electricity, steady winds are necessary. Wide open spaces are therefore ideal to set up
wind turbines and wind farms; for example, Midwest USA is well suited for large wind
farms. But some of the strongest winds are observed over the sea and it is estimated
that wind energy is more abundant off-shore than on-shore [10]. Despite having one
of the largest installed wind capacities in the world, USA does not have many off-shore
farms. Off-shore farms are abundant in many European countries where wind power is
already a significant portion of the generated power; example: 20% in Denmark or 10%
in Ireland and Spain [11].
Solar power is utilized in two ways - directly converting to electricity with a
photovoltaic cell or indirectly with a concentrated solar power where the sunlight is
15
focused to a small region using lenses and mirrors to generate steam to rotate turbines.
Photovoltaic cells convert solar energy to electricity using the photovoltaic effect where
a voltage difference is induced across P-N junction by shining radiation (solar radiation)
on one of the surfaces [12]. Photovoltaic cells generate DC voltage and additional
electronics (called inverters) are needed to convert it to AC for interconnection with the
grid. While the cost of solar generator modules is reducing, it is still more expensive to
produce a unit of energy using solar that the more traditional generators.
With the emphasis on revamping the grid into a smart grid which seeks to support
plug and play usage capability for DGs, it can be assumed that DGs are going to
become an integral part of the electric grid because DGs can be used to expand the
power capacity of a distribution system without purchasing additional power or build
expensive, new generator stations. Another advantage of distributed generation is
that the generators are much smaller than the centralized generation resources and
therefore cheaper. Therefore new technological improvements can easily be deployed in
the form of distributed generators.
Distributed generators do not currently have an active role in providing ancillary
services to the grid; they are instead expected to produce power at a constant rate at
a constant power factor. During low voltage situations they are required to ride through
or disconnect from the grid in severe cases. Two reasons [13], [14] for their passive
connection are 1> DGs do not have sufficient generation capability to have a significant
effect and 2> a control algorithm operating in parallel with the utility control operations
might aggravate the situation. However with modern, fast acting, electronic control
systems and communication networks, DGs can be included in a coordinated control
plan to provide voltage and power support. This study is an attempt to devise such a
coordinated control technique.
16
2.3 Distribution Networks
Due to economies of scale, generation of power was traditionally done at remote
locations close to the fuel source and away from the consumers. Distribution networks
are delivery systems to bring power from the generators though the transmission grid to
the consumer. The transmission system which begins at the generator and ends at the
distribution substation is a meshed network for increased reliability and power sharing.
But the distribution system (beginning at the distribution substation and ending at the
customer’s premises) is mainly radial i.e. lines starting from the substation rarely form
loops.
Figure 2-1. Schematic of a Power grid. Source: US Department of Energy [15]
Most nodes of a distribution system are rarely connected to more than two other
nodes. The series of branches forming a chain are known as feeder lines and the
feeder(s) connected to the substation bus are known as the main feeder. The others
are known as laterals or sub-feeders. Nodes are any points of interest in the network,
generally points with a connected load, a lateral, a transformer, DG, regulator, etc.
Another difference between distribution and transmission systems is that series
resistance of distribution lines as a fraction of the series reactance (typically referenced
by R/X ratio) is much higher for distribution lines whereas in transmission lines the
reactance is dominant. A consequence of this property is real power can also be
dispatched for voltage regulation whereas in transmission systems, reactive power
produces a bigger voltage change for the same amount of dispatch. Although this
17
study is limited to the conventional reactive power (VAR) support, from a voltage
regulation stand-point, real power dispatch can produce a similar result assuming the
line reactance and resistance are comparable.
A distribution system may also be unbalanced i.e. all three phases of the power
system may not be equally loaded; one or more phases may not even be used. This is
one of the reasons that traditional power flow algorithms used for transmission systems
cannot be used for distribution systems. Due to the unbalanced nature, the high R/X
ratios and the radial nature of the grid, Newton-Raphson type methods may fail to
converge. Therefore other methods better suited for radial distribution system conditions
have been developed. The forward-backward method sweep based on ladder theory
[16] is used in this study for all power flow operations.
The power flow algorithm treats the substation bus as the slack node and the
remaining nodes as PQ nodes. Including PV nodes in the feeder complicates power
flow because keeping a constant voltage at a particular node requires a VVC operation.
Therefore, for simplicity even DGs are considered as PQ nodes with a negative load
value to indicate that they feed power into the network instead of consuming it.
As evidenced by the radial topology, the distribution grid was not originally designed
for a bidirectional flow of power. Although the cables can handle the reverse flow of
current, protection devices such as distance relays assume a unidirectional flow of
current. A bidirectional flow will cause a reduction in line currents which can adversely
affect the detection capacities of the relay. It is also a concern for service personnel
operating on a faulty line - in a radial structure it is easy to de-energize a line by cutting
off the main supply to the line. But with DGs connected, the line may be islanded -
which implies that the line is carrying current from the DGs but not the main supply.
Line voltage regulators operation is also affected since they estimate voltage at a
downstream node based on the current through its line compensation circuit and
a secondary source located downstream disrupts this relation. Therefore a control
18
procedure that does not depend heavily on line currents to estimate voltage must be
made available for use with DGs.
2.4 Voltage and Reactive Power Control
The ANSI standard [1] requires the voltages during steady state operation to be as
follows: on a nominal voltage of 120V, the service voltage is allowed a leeway of
Voltage-VAR control or VVC refers to regulating the voltage by feeding or consuming
reactive power as necessary. While real and reactive powers and node voltage and
phase are all intricately linked, there’s a stronger relation between reactive power and
voltage magnitude; between real power and voltage angle. This phenomenon exists
because of the decoupling of real and reactive power that occurs if the line resistance
is much smaller than the reactance and voltage magnitude at all nodes is maintained at
around 1pu. Line impedance is a fixed parameter and has to be chosen during system
design but the second condition is valid when the grid is adequately controlled and
maintained. For the case of transmission lines, line reactive impedance is indeed more
than resistance, but for distribution lines it is not necessarily true. Depending on the
ratio of reactance and resistance of a line both active and reactive power may have
equal effect on the voltage of the grid but by convention, reactive power is chosen for
compensation. In case of reactive power (VAR) compensation, the rule of thumb is:
injecting VAR into the grid increases the voltage while absorbing it reduces the voltage.
Traditionally voltage control has been done using switching circuits, transformers,
line drop compensators, step voltage regulators, load shedding, reactive power
compensation using capacitor banks, etc. With the growing popularity of distributed
generation or disperse generation other avenues of compensation have opened up. This
study is concerned with VVC but one that is based on sensitivity of voltage to reactive
power injections from DGs. The study also explores the possibility of using voltage
sensitivity and VVC to reduce distribution power loss.
19
Reducing losses involves reducing line currents all along the feeder. This can also
be restated as reducing the voltage difference between adjacent nodes. It is easy to
prove that distributing power sources across the feeder reduces the line current and
thereby losses. For example in Figure 2-2, a single DG is connected at the last node of
an N + 1 node feeder. Assuming all the nodes have an equal sized load connected to
it and they draw the same amount of current irrespective of the voltage at the node, the
current at the source bus is N ∗ Iload without the DG. If the DG assumes an equal load,
the current drawn from each source would be N ∗ Iload/2. Table 1 compares the lowest
voltage, maximum current and losses for the case with and without DG. Without any
form of voltage control or compensation, voltage magnitude decreases steadily along
the length of the feeder beginning at the substation (node 0).
Figure 2-2. N+1 load feeder with a distributed generator connected at the last node
With the DG however, the decrease in voltage is lower because the net current from
a single source is smaller than the current drawn from the substation without any DG.
Therefore, the voltage reduces moving from either end of the feeder towards the center.
For simplicity N is taken to be even.
Table 2-1. Comparison of voltage, current and loss with and without DGWithout DG With DG
Lowest voltage V0 − ZlineNIload V0 − ZlineNIload/2
Maximum current NIload1
2NIload
Total power loss 1
6N(N + 1)(2N + 1)I 2loadRline
1
12N(N + 1)(N + 2)I 2loadRline
20
It can be inferred that increasing the number of power sources reduces the
maximum line current. Since loss is proportionate to the square of the line current,
reducing the maximum current magnitude has a huge impact on the total distribution
loss in a feeder. In the example, reduction is by almost a factor of 4. In the example
of Figure 2-2 the type of load used is constant current load - where the current drawn
is independent of the voltage. Power consumed by a load is given by VI*, therefore
if a constant current load is connected at a higher voltage it consumes more power.
The other commonly used types of load are constant power and constant impedance.
Constant power loads draw the same amount of power irrespective of the voltage
but current drawn reduces with increasing voltage. Constant impedance loads have
constant impedance regardless of the voltage but power increases as the square of
voltage and current increases linearly with voltage.
Figure 2-3. Current drawn at different voltages for different load types
If all loads on a grid were of the same type, loss minimization would be a simple
problem. For a constant power load a higher voltage load is preferred therefore letting
the node with the highest voltage to be at 1.05 pu. (maximum allowed voltage according
to ANSI standards) would be sufficient. For constant impedance letting the lowest
voltage be 0.95 pu. would solve the control problem. For constant current loads as
long as the nodal voltages are within allowable limits, no control is necessary. For a
21
homogeneous load type control is simple irrespective of the load sizes but actual loads
are not homogeneous and optimization is required to determine the best configuration
and dispatch. Chapter 3 lists some of the techniques used in previous studies.
22
CHAPTER 3PROBLEM DESCRIPTION
An electrical system is governed by power flow equations which are a result of
Kirchhoff’s current law and Ohm’s law. These equations define the relationship between
the voltage at each node in the grid and the loads or generators connected to them.
Knowing the voltage at each node, it is possible to know the current in all the lines; the
exact power consumed or injected at each node and other metrics such as stability
of the grid etc. The voltages at all nodes (defined by a voltage phasor magnitude and
angle) are known as the state of the system. The set power flow equations can be
represented as
F (x , u) = 0
where x is the state vector and u is the vector of all control variables such as tap position
or voltage regulator, on load tap changing transformer, generator power output, etc. and
the loads at different nodes. F is the relation between x and u defined by Kirchhoff’s
current law and Ohm’s law. For ease of calculation all variables are represented in the
per unit system.
Voltage control according to ANSI standards requires that the utility voltage not vary
more than 5% from the nominal voltage of 1 pu. If x can be separated as
x =
|V |
θ
where |V | is the vector of node voltage magnitudes and θ is the bus angle, then voltage
control implies 0.95 ≤ |Vi | ≤ 1.05 for all nodes i = 1, 2, ...N
if Vi goes out of bounds, ucontrol can be adjusted so that Vi is within limits again.
In
u =
ucontrol
uload
23
ucontrol is a vector of all control variables and uload is the vector of load values. The vector
of control signals, ucontrol , can be chosen in different ways to achieve the required result.
Hence an objective function is necessary to choose best vector based on some criteria.
If tap changing transformers are used, the number of tap changes is often a criterion. If
compensation methods are being used and it costs the utility different rates for different
types of compensation then the most economical dispatch is sought. Line losses are
also often considered for optimization since losses can be controlled by varying the
voltage at the different nodes.
The power lost as heat on a single line between nodes i , j , is given as
Pilossj = Ii
2
j Ri j = (Vi − Vj)2/Ri j
where V = |V | ∗ e j θ and Ri j is the resistance of the line between nodes i and j .
Power systems however, are not single lines but have three phases, which in case of
a distribution network may be unbalanced. Therefore the total loss is calculated as a
product of vectors and matrices as:
Pilossj = Real {VI ∗} = Real
{(Vi − Vj)Zi
∗j−1(Vi − Vj)
∗}If the system is three phase, Vi is a 3× 1 complex vector of voltages of the three phases
of each node and Zi j is a 3× 3 complex matrix.
The total system loss is obtained by adding the loss over all the lines
P losstotal =
∑i ,j
Real{(Vi − Vj)Zi
∗j−1(Vi − Vj)
∗} (3–1)
For two nodes i , j not connected to each other, Z ∗i−1
j is a zero matrix and doesn’t
contribute to the loss. Therefore the general VVC with loss optimization problem can be
written as
24
Minimize P losstotal =
∑i ,j
Real{(Vi − Vj)Z
∗i−1
j Vi − Vj∗} (3–2)
Such that F (x , u) = 0
0.95pu ≤ |Vi | ≤ 1.05pu and
umini ≤ ui ≤ umax
i ∀i = 1, 2, ...M
where ui are the control variables.
In this study the control variables used are the reactive power produced by DGs
connected at different nodes in the distribution grid. Adjusting the power production
may not always be sufficient control mechanism and voltage regulators may need to
be adjusted as well. The tap changing operation is not included in the optimization but
performed if optimization fails to produce a feasible result. The optimization and results
are discussed in depth in chapter 5.
Chapter 4 discusses the past studies done in the field of voltage VAR control, siting
and sizing of reactive power sources and use of voltage sensitivity for control. In addition
to VAR optimization, placement of DGs on the feeder can also be used to adjust losses -
some positions are better suited for loss reduction than others. Similarly the capacity of
the DGs can also be optimized for a better performance. The optimal siting and sizing of
DGs is discussed in chapter 6. Also discussed in the chapter is the effect of increasing
penetration of DGs on distribution losses.
25
CHAPTER 4LITERATURE REVIEW
Voltage and reactive power control (Volt/VAR control or VVC) is an important
task that has been studied many times for both the transmission grid and distribution
grid. While new innovative techniques are being sought for voltage control, the most
commonly used methods are still the time tested ones such as feeder reconfiguration
[17], [18] to minimize line currents. The radial structure of the distribution system also
supports regulation through step voltage regulator with line drop compensator [16].
Injecting reactive power using compensation devices such as static VAR compensators
(SVCs), static synchronous compensators (STATCOMs) and other flexible alternating
current transmission system (FACTS) devices can be used to boost voltage as well
as control the phase angle [19]. The simplest and most commonly used form of
compensation though is capacitor banks which may be located at the substation or
along the feeder line. Traditional control techniques have dealt with optimizing the
positions of the taps in the transformers or controlling the output of the compensation
devices [20] or both while optimizing for economic or other system constraints. Due to
the non-linearity of the control problem, evolutionary algorithms such as particle swarm
optimization [21], [22] or genetic algorithm [23], [24] have been extensively used for
optimization.
Recent technological improvements have made DGs popular as a parallel source of
power for important or sensitive loads. Their capacity to inject excess power into the grid
has made them a viable option for compensation. Although DGs are being connected
to the grid, their involvement in providing ancillary services is negligible. There is still
concern regarding integration and control of new generators in the distribution grid
although extensive literature is available on various aspects of DG integration and
utilization from the various technologies it entails [4], [5], [8], [25], their impact - both
economic [26] and on the voltage profile [27], [28]; and incentives to promote their use
26
[29]; to the concerns and challenges of using DGs [25], [30]. A lot of research work has
also been done on control involving DGs [13], [27], [31], [32] and more importantly sizing
and siting the DGs on the grid [28], [33], [34].
With the current focus on upgrading the electric grid to a smart grid with support for
decentralized control, different methods of decentralized control are being researched.
Multi agent systems (MAS) [35], [36] are among the ideas being explored. The algorithm
developed by Baran and Markabi [37] to determine the optimum reactive power dispatch
of DGs using linear programming, is an example. A similar algorithm that dispatches
both real and reactive is discussed in [38].
Sensitivity of different types have also been used to determine the location of DGs
on the grid [39], [40] as well. But Gozel and Hocaoglu [41] with an intention to avoid
Jacobian and admittance matrix, developed an analytical method to locate and size
DGs on a radial system using a loss sensitivity factor based on the current injection
matrix. The goal was to determine the amount of injection required to reduce the losses
to a minimum. But with a loss function that can be derived from measured voltage
sensitivities, it may be easier to calculate the loss sensitivity coefficients.
Voltage and Reactive Power control using Sensitivity. The algorithm developed
by Markabi and Baran [37] implemented a simple multi-agent distributed VVC algorithm
based on sensitivity coefficients. They used sensitivity coefficients derived from the
power flow Jacobian to determine dispatch using linear programming. However, to
make the algorithm decentralized and independent of the grid architecture, sensitivity
coefficients of nodes without a DG were eliminated through Kron reduction. But the
new coefficients are not measurable quantities since they have been adjusted by Kron
reduction and made system dependent. Nevertheless, the concept of using sensitivity
to determine dispatch is a useful result. Dispatch is can still be calculated using the
measured sensitivity values which are the true instantaneous sensitivity values.
27
A single feeder line with multiple DGs connected along the length of it with the DGs
carrying most of the load was considered in the study. Each DG is assumed to be an
agent with intelligence. The remaining nodes are passive with no intelligence. All the
agents can communicate among themselves to share any necessary information. Each
agent performs three important tasks monitoring, moderating and dispatch.
Monitoring refers to checking the node voltage and verifying that it is always within
the specified range (within 5% of the nominal). When the voltage is no longer within
limits, the agent corresponding to the (most) affected node acts as the moderator.
They note that the voltages of the downstream nodes are usually the most severely
affected and it might be necessary to have a dummy DG with no output connected
at these nodes to monitor the voltage at the these points. It essentially translates to
having a measuring device like a PMU connected at the end node and extending the
communication networks till the end of the feeder. If that may not be possible then some
method of estimating the voltage at the end is necessary for example by assuming a
constant voltage difference between the end of the feeder and its nearest DG unit.
When a nodal voltage violates the operating limits, the closest DG senses it and
communicates with the other DGs and requests for reactive support and receives
their bids. The bids are the maximum support each DG can lend and the sensitivity
coefficient for the particular node. The moderator then decides the optimal dispatch
scheme for DGs. The DGs on receiving the dispatch change the output power to suit
requirements. This is the dispatch mode.
In general, feeding reactive power into the grid increases the voltage while
consuming it reduces the voltage magnitude. This behavior is captured by the sensitivity
coefficients and simple linear programming can calculate the dispatch scheme. The
problem is formulated as
Minimize∑i
�Qi (4–1)
28
Such that �Vk = Vmin − V 0
k and
Qmini ≤ Q0
i + �Qi ≤ Qmaxi
where �Qi is the change in reactive power output of i th DG, V 0k is the current voltage at
node k and Q0i is the current reactive power output of i th DG.
The DG causing the highest sensitivity to the affected node is chosen and it
supports the node to whatever extent it can. If the reactive power support of that DG
does not suffice, the DG with the next highest sensitivity helps and so on until the
voltage excess or deficiency has been compensated and all the voltages are within the
specified limits. If there are n nodes in the distribution system and V1,V2 ...Vn are the
node voltage magnitudes (assuming a balanced feeder, but the theory can easily be
expanded to unbalanced systems) and there are m (m ≤ n) DGs with reactive power
Q1,Q2 ...Qm, the voltage sensitivity is defined as
βi j =∂Vi
∂Qj
∀i = 1, 2, ... n and ∀j = 1, 2 ...m (4–2)
The partial derivatives form the Jacobian matrix used in Newton-Raphson power flow
and it defines the relation between VAR support of the DGs and voltage at the nodes.
The effect of the m DGs on its node voltage can be more accurately expressed by
considering that the net reactive power injection at most nodes is zero. Hence n voltage
equations can be reduced to only m equations by Kron reduction. The coefficients of the
variables obtained thus are the required sensitivities. It is easy to determine the VAR
support from equations (4–3) and (4–4).
If H is the Jacobian matrix, P is the vector of real power injections are each node, Q
is the reactive power injected, x is the vector of voltage magnitudes and θ is the vector of
node voltage angles, then
f =
P
Q
and x =
θ
V
29
�f = H × �x
H =
HPθ HPV
HQθ HQV
(4–3)
HQV is the partial of reactive power with respect to voltage magnitude. Reactive support
can be obtained using real and reactive power decoupling, which is based on the fact
that the voltage magnitude at a node affects the reactive power injected at that node
rather than the real power which is affected by the voltage angle. Hence
�Q/V = HQV�V (4–4)
�Q is divided by the node voltage, V , to linearize the power flow equations. Since �Q is
zero for the load nodes, the rows and columns of HQV can be rearranged to
HQV =
B11 B12
B21 B22
where
B11 = partial derivative of reactive power injection at the load nodes with respect to
voltages at the DG nodes
B12= partial derivative of reactive power injection at the load nodes with respect to
voltages at the DG nodes
B21= partial derivative of reactive power injection at the DG nodes with respect to
voltages at the load nodes
B22= partial derivative of reactive power injection at the DG nodes with respect to
voltages at these nodes. 0
�Q/V
=
B11 B12
B21 B22
�VL
�VDG
(4–5)
�VL is the vector of voltages at the load nodes.
30
Therefore,
�VDG = (B22 − B21B1−1
1 B12)−1�QDG/V or (4–6)
�VDG = β�QDG (4–7)
β is the sensitivity matrix. The elements of β determine the reactive support that each
DG provides. Therefore equation (4–1) changes to
Minimize∑i
�Qi (4–8)
Such that �Vk =
m∑i=1
βk i�Qi = Vmin − V 0
k
0 ≤ Q0
i + �Qi ≤ Qmaxi
Equation (4–8) indicates that the best solution to this problem is to have maximum
dispatch for the DG with the highest sensitivity until generator capacity is reached. If that
is not sufficient, DG with the next largest sensitivity adjusts its output and so forth until
the voltage drop has been compensated. A drawback of this algorithm is that it adjusts
the voltage to bring it within acceptable operating range but only barely. So if voltage
exceeds 1.05pu it is lowered to 1.05pu, if it falls below 0.95pu it is raised to 0.95pu. This
may not be the best voltage profile for a distribution feeder since the load is always
changing; even small variations in load or DG output can cause the voltages to go out
of range again. To maintain it at a voltage slightly higher than acceptable level might
seem like a good option but that only invites the question, ’how high?’. The answer lies
not in raising or lowering the voltage to a fixed level, but to optimize the voltage for other
parameters. Loss is the objective chosen in this study because it not only reduces the
wastage of energy lines but also frees up the line capacity for more useful power flow.
A new set of constraints and optimization function can therefore be devised to
account for these. A few modifications to the algorithm are suggested which employ a
quadratic optimization function rather than a linear one. This is discussed in chapter
31
5. Chapter 5 also discusses voltage sensitivity and its behavior to changes in load and
power generation.
32
CHAPTER 5VOLTAGE-VAR CONTROL AND LOSS MINIMIZATION
The objective of voltage-VAR control can be expanded from just maintaining the
voltage at the end of each feeder node within the specified voltage range to also protect
the voltage against variations in the system conditions such as loading, faults, loss
of power, etc. With access to power generation sources at different locations in the
grid it becomes possible to not only maintain voltages within operable regions but
manipulate the power flow so that other objectives can be achieved. The most important
advantage of using voltage sensitivity for this purpose is it allows for the estimation
of the new state - and subsequently other parameters that are a function of nodal
voltage - without performing load flow analysis. A complex set of nonlinear equations
can be approximated to a linear combination of sensitivity coefficients, saving precious
computation resource and time.
5.1 Voltage Sensitivity
Sensitivity has been defined in chapter 4 (equation (4–5)) as the inverse of the
power flow Jacobian. Voltage sensitivity with respect to change in reactive power
injection at a node (hereby referred to as voltage sensitivity or just sensitivity; this study
deals exclusively with reactive power and voltage change unless otherwise specified) is
an n × n block in the 2n × 2n Jacobian matrix. Sensitivity is an easy way of estimating
the new state of the grid when the DG outputs are changed since it is the observed,
steady state voltage change for a unit change in power production. Figure 5-1 shows
the sensitivity of phase A for all nodes of a 34 node feeder for 1KVAR change in output
power of a DG when connected at four different locations. The missing sensitivity values
are a consequence of an unbalanced feeder - not all nodes utilize all three phases.
Using sensitivity, for some change in power production, the voltage change in the
feeder nodes can be estimated by scaling the sensitivity at these nodes the appropriate
amount. The relation is described by equation (4–7). However, the expression for β,
33
the sensitivity is modified from equation (4–6); instead of using sensitivity of only small
subset of nodes from a reduced set of power flow equations, the sensitivity of all nodes
represented by the columns of HQ−1
V are used. Equation (4–6) exploits the fact that
power injection at non-DG nodes is zero. Hence the sensitivity calculated from only
DG connected nodes does not represent the the measurable change in voltage at the
particular nodes; it is a calculated quantity, although it may still be numerically similar
to the measurable sensitivity. Since the magnitude of voltage change is quite small (of
the order of 10−4p.u./KVAR change in power injection), the mismatch between the
calculated and the observed value may go unnoticed. Patterns and trends [42] similar
to those of the calculated sensitivity of equation (4–6) are also observable for the actual
measured sensitivity coefficients.
Figure 5-1. Sensitivity of 34 node feeder for four different DG positions
For a perfectly decoupled system, the sensitivity parameters are a constant with
HQV given by the admittance matrix. But even for a lossless line it is not possible
to have a perfectly decoupled system and the sensitivity varies with voltage. Over
large voltage ranges sensitivity is non-linear but over smaller ranges - such as in LV
or MV compensation schemes it can be approximated to a linear trend (figure 5-2).
Mathematically this observation can be made by not approximating the nodal voltage to
34
1pu. This is also the expression used in this study. But the most accurate value can be
obtained by inverting the Jacobian
H =
HPθ HPV
HQθ HQV
with no assumptions or approximations. The columns represent the sensitivity
coefficients for all the nodes - except the substation bus - for all possible DG locations.
The sensitivity of the substation bus is 0 due to the control action of the substation
control system. In the Jacobian of dimension 2n × 2n (when number of nodes in the
feeder is n + 1; sensitivity of the substation bus is zero) and the voltage sensitivity to
reactive power is a n × n block in the bigger matrix.
Figure 5-2 is the plot of sensitivity of a particular node with DG fixed at a different
node and the reactive power output of the DG is varied from from -100 KVAR to
+100KVAR in steps of 1 KVAR. Plot A is the result of repeating the process for different
values of real power output. While plot A is for all three phases, plot B displays the
sensitivity for a single phase (phase A) with respect to the node voltage instead of the
reactive power output.
Figure 5-2 is typical of most nodes. It is observed that while sensitivity is not a
constant, it can be approximated as a linear function for most cases. The centralized
voltage control optimization function is derived assuming a constant sensitivity and the
consequences of assuming linearly varying sensitivity are explained.
5.2 Centralized Voltage Control and Loss Optimization
If the sensitivity is fairly constant, a single coefficient can be selected for each
node and phase for control. But due to the varying voltage and loading and injection
conditions, sensitivity also varies. Hence there are fewer approximations. The
centralized control approach uses all the voltage and approximate sensitivity values for
voltage and loss estimation. The decentralized algorithm which is given to a coordinated
35
A Variation with change in reactive dispatch
B Variation with node voltage
Figure 5-2. Variation of sensitivity
control structure based on local information is discussed in section 5.3 but both of them
optimize the same quantity - loss. The decentralized version is an extension of the
centralized version.
36
5.2.1 Objective Function
The expression for distribution loss on a single branch was derived in equation
(3–1) as
Minimize P losstotal =
∑i ,j
Real{(Vi − Vj)Z
∗i−1
j (Vi − Vj)∗}
Such that F (x , u) = 0
0.95pu ≤ |Vi | ≤ 1.05pu and
umini ≤ ui ≤ umax
i ∀i = 1, 2, ...M
where Zi j is the impedance between two nodes i and j . Considering the total loss and
not only the real power loss,
lossi j = (V2 − V1)Z∗−1
12 (V2 − V1)∗
If the voltages after optimization are V ′1 and V ′
2 then
lossi j = (V ′2 − V ′
1)Z∗−1
12 (V ′2 − V ′
1)∗
but V ′ = V + �V and �V can be estimated using voltage sensitivity as
lossi′j = (V2 + �V2 − V1 − �V1)Z
∗−1
12 (V2 + �V2 − V1 − �V1)∗
Simplifying,
lossi′j =(V2 − V1)Z
∗−1
12 (V2 − V1)∗ + (�V2 − �V1)Z
∗−1
12 (�V2 − �V1)∗
+ (V2 − V1)Z∗−1
12 (�V2 − �V1)∗ + (�V2 − �V1)Z
∗−1
12 (V2 − V1)∗
The first term on the right of the equation is lossi j hence
lossi′j − lossi j = (�V2 − �V1)Z
∗−1
12 (�V2 − �V1)∗
+ (V2 − V1)Z∗−1
12 (�V2 − �V1)∗ + (�V2 − �V1)Z
∗−1
12 (V2 − V1)∗ (5–1)
37
Since lossi j denotes the initial (or current) state of loss in the line, it is a constant with
respect to optimization and can be neglected. This corresponds to optimizing for change
in total loss rather than the total loss itself.
Thus the new value of f is f ′
f ′ =∑i ,j
(Vi − Vj)Zi∗−1
j (�Vi − �Vj)∗ + (�Vi − �Vj)Zi
∗−1
j (Vi − Vj)∗
+∑i ,j
(�Vi − �Vj)Zi∗−1
j (�Vi − �Vj)∗ (5–2)
The change in voltage at k th node �Vk , can be represented as
�Vk =∑i
β ik ∗ �Q i
DG
Or, in vector form:
�Vk = �QTDGβ (5–3)
Substituting in equation (5–1) and simplifying,
f ′ =∑i ,j
(Vi − Vj)Zi∗−1
j (βi∗j �QDG) + (�QT
DGβi j)Zi∗−1
j (Vi − Vj)∗
+∑i ,j
(�QTDGβi j)Zi
∗−1
j (βi∗j �QDG)
where βi j = βi − βj is a 3×m matrix containing the sensitivity coefficients of each of the
three phases of a particular node with respect to all the connected DGs. Therefore,
f ′ =∑i ,j
((Vi − Vj)Z∗−1βi
∗j )�QDG + �QDG(βi jZ
∗−1(Vi − Vj)∗)
+∑i ,j
�QDG(βi jZ∗−1βi
∗j )�QDG
This can be further simplified to a quadratic equation in vector form as
f ′ = A�QDG + �QTDGB + �QT
DGC�QDG
38
Considering only the real power loss, the final objective function is
f ′ = P�QDG +�QTDGQ�QDG (5–4)
where P = Real{A+ B} and Q = Real{C}
A second voltage regulator control level exists above this DG dispatch control to
utilize the control options already incorporated in the feeder. Due to the existence of
DGs, tap positions cannot be accurately selected by the line compensator circuit and
downstream voltage has to be communicated to the regulator controller or the tap can
be shifted by one position at a time. For each change in tap settings, the optimization
algorithm for the DGs is executed. The combination of both these operations determines
the ideal settings.
Unlike the compensation algorithm of Markabi and Baran, this method of loss
control is not given to dispersive control; this is a centralized power flow and loss control
algorithm because to develop the objective function all the node voltages are necessary.
An agent based decentralized variant of this algorithm can also be devised; discussed
in section 5.3. However with the increasing incorporation of communication channels
between the agents of a power grid, it becomes possible to locate the control center
at any location, including a node on the feeder line. It is through the communication
network that a dispersed control of the grid can be achieved.
Another important note regarding the centralized algorithm is that �V used in
the derivation is a complex quantity whereas voltage sensitivity in the Jacobian is the
change in voltage magnitude with respect to DG output, which is a real number. Using
angular sensitivity and voltage sensitivity to reactive power and the voltage profile, the
complex �V can be calculated. In the simulations however, the complex voltage change
is measured. By choosing a small enough change in reactive power injection and using
that for sensitivity the magnitude of the complex value and the actual change in voltage
39
magnitude can be made comparable. For the IEEE 13 node and 34 node feeders,
1KVAR was found to serve the purpose.
5.2.2 Constraints and Optimization Problem
The general constraints of the system are the voltage constraints given in equation
(3–1) are:
0.95pu ≤ |Vi |+ |�Vi | ≤ 1.05pu
and capacity constraints of the DGs
Qmini ≤ Qi + �Qi ≤ Qmax
i ∀i . (5–5)
Using the relation (5–2) in equations (5–4) and (5–5)
0.95− |Vi | ≤ |�Vi | = �QTDGβi ≤ 1.05− |Vi | (5–6)
And
Qmini −Qi ≤ �Qi ≤ Qmax
i −Qi (5–7)
The complete optimization problem can, therefore, be defined as
Minimize f ′ = P�QDG + �QTDGQ�QDG (5–8)
Such that: Vmini ≤ �QDG
Tβi ≤ Vmi ax and
Qmini −Qi ≤ �Qi ≤ Qmax
i −Qi
An evolutionary technique called particle swarm optimization (PSO) is used to solve the
optimization problem.
5.3 Decentralized Voltage Control and Loss Optimization
Decentralized voltage control is implemented using data available locally to the
controller. Unlike the case of centralized control where data from all the sensors in
the network are to be collected at an aggregator site before decisions are taken,
decentralized controller reacts to local phenomena. This is particularly useful when
40
communication systems are experiencing problems due to weather or other reasons.
Implementing a system with multiple decision making bodies also makes the system
robust to other contingencies and intentional attacks. In this study however, the myriad
controllers do not act individually, rather each one monitors the local conditions and
coordinates with other such controllers called agents to achieve the required goal. This
is known as a multi agent system.
The control structure is similar to the one described in section 4 with changes in the
information being exchanged, and the optimization algorithm used to decide dispatch.
The agents control DG installations and voltage regulators and perform monitoring (of
voltage it its point of contact), moderation (negotiate with other agents) and dispatch
(execute optimization algorithm and communicate dispatch scheme to other agents)
operations.
Due to the absence of all node voltages, equation (5–8) cannot be used. A
small modification to the objective function of equation (5–8) can be used for local
optimization. The central control scheme generates a new objective function before
optimization to reflect the voltage profile of the feeder which is an operation the control
agent cannot perform. If a reference voltage profile of the feeder could be used instead,
voltage data collection would be unnecessary to determine the objective function. For
example, equation (5–1) determines the change in the loss with respect to the initial
condition - the voltage condition on the entire feeder before optimization. Similarly if
the initial condition can be measured against a fixed reference, a new function does not
have to be calculated before each execution. A base case voltage profile - for example,
when none of the DGs were connected - can be used as a reference,. If the voltages for
this case are represented as V refk , change in loss can be calculated as
lossi′j = (V ref
i +δV refi +�Vi−V ref
j −δV refj −�Vj)Zi
∗−1
j (V refi +�Vi+δV ref
i −V refj −�Vj−δV ref
j )∗
41
where V refi + δV ref
i + �Vi = V ′i , the new voltage to be estimated and V ref
i + δV refi = Vi is
the voltage before control.
lossi′j =
((V ref
i + δV refi − V ref
j − δV refj ) + (�Vi − �Vj)
)× Zi
∗−1
j
((V ref
i + δV refi − V ref
j − δV refj ) + (�Vi − �Vj)
)∗lossi
′j = (V ref
i + δV refi − V ref
j − δV refj )Z ∗−1(V ref
i + δV refi − V ref
j − δV refj )∗
+ (�Vi − �Vj)Z∗−1(V ref
i + δV refi − V ref
j − δV refj )∗
+ (V refi + δV ref
i − V refj − δV ref
j )Z ∗−1(�Vi − �Vj)∗
+ (�Vi − �Vj)Z∗−1(�Vi − �Vj)
∗
The first term of lossi ′j is lossi j , line loss for the current voltage profile. Therefore,
lossi′j − lossi j = (�Vi − �Vj)Z
∗−1(V refi − V ref
j + δVirefj )∗
+ (V refi − V ref
j + δVirefj )Z ∗−1(�Vi − �Vj)
∗
+ (�Vi − �Vj)Z∗−1(�Vi − �Vj)
∗ (5–9)
The first term of lossi ′j can be ignored as it is a constant with respect to the optimization
problem. The remaining three terms form the optimization function. V refk is known since
it is the reference profile; an approximate value for δV refk will be calculated using local
voltage information. The precise value is not necessary since the value required for
estimating the loss is (δV refi − δV ref
j ) the change in voltage difference between two
adjacent nodes. Similar to equations (5–1) to (5–3), by substituting (5–2) in (5–9) and
simplifying,
f =∑i ,j
lossi′j − lossi j = A�QDG + B�QDG + �QT
DGC�QDG (5–10)
Such that: Vmink ≤ �QT
DGβi ≤ Vmaxk and
Qmini −Qi ≤ �Qi ≤ Qmax
i −Qi∀i = 1, 2, ...m
42
Where
A =∑i ,j
((V refi − V ref
j )Zi∗−1
j βi j + (V refi − V ref
j )′Zi∗−1
jTβi j) and
B =∑i ,j
(δVirefj Z ∗−1βi j + δVi
refj
TZ ∗−1Tβi j) and
C =∑i ,j
(βiTj Zi
∗−1
jTβi j)
δVirefj = (δV ref
i − δV refj ) is estimated using the local voltage value. Since a local event
such as a voltage violation triggers the optimization, it is assumed that the voltage at
the specific node is known. The reference voltage at that node is also known. Using
the difference between the two known voltages, some compensation dispatch that will
bridge the difference is calculated i.e. (�QDG) such that (�QDG) ∗ βk = δV refk at errant
node k is calculated. The dispatch scheme does not necessarily have to be feasible
since it is a theoretical value used to estimate δVirefj . It is possible to allocate the entire
dispatch to one generator but it is preferred to use as many generators as possible. With
(�QDG) known, δV refi = (�QDG) ∗ βi can be calculated for all nodes; subsequently, B
can also be calculated.
5.4 Optimization Algorithm
5.4.1 Quadratic Programming
The basic quadratic optimization problem is defined by the objective function G
where x is the vector to be optimized, H is a symmetric matrix and f is a vector:
Minimize G =1
2xTHx + f Tx (5–11)
Such that
Ax ≤ b
Aeqx = beq
lb ≤ x ≤ ub
43
In the loss minimization problem however, the H matrix is not symmetric due to the
complex nature of voltage, sensitivity and line series impedance; also due to the use of
complex conjugates to calculate the H matrix. Therefore H is made symmetric with the
relation
H = (H + HT )/2
However, despite converting the Hessian to a symmetric matrix, the Matlab function
quadprog for quadratic programming failed to produce feasible results.
5.4.2 Particle Swarm Optimization
Due to the failure of constrained quadratic optimization, a swarm based technique
called Particle Swarm Optimization (PSO) [21], deriving inspiration from the flocking
behavior of birds was chosen.
PSO employs a large swarm of agents each of which can save information about
itself and the swarm and also change its course of motion according to this information.
The agents are initiated at random locations in the search space which denotes the
range of values each variable in the optimization problem can take. The variables to
be determined form the ”location” vector of the agent. Each location in the search
space has an associated fitness value which is the value of the objective function for
the particular sequence of variable values. During an iteration of the algorithm, each
agent updates its location value by adjusting it velocity according to equations (5–12)
and (5–13). During this ”exploration” each stores its personal (pbest) and the swarm’s
global (gbest) best values. These indicate the best location where the particular agent
experienced the best objective value function and the best value for the whole swarm
respectively. Each agent has its own personal best but the swarm shares a common
global best location and value. By updating its own location based on pbest and gbest ,
every agent converges to the optimal location.
vi = w ∗ vi + c1 ∗ rand ∗ (pbesti − xi) + c2 ∗ rand ∗ (gbest − xi) (5–12)
44
xi = xi + vi (5–13)
where xi is the position vector of agent i , pbesti is the best location it has been to, gbest
is the best position for the entire swarm. c1 and c2 are constants and w is the inertial
constant.
5.5 Results and Observations
The performance of three algorithms:
1. Dispatch linearly proportional to the sensitivity of the affected node (Linear)2. Centralized compensation using PSO (PSO)3. Decentralized compensation using PSO (Dispersed)
are tested for 3 different cases: case 1> optimizing when reactive output of all DGs is
zero; case 2> all the loads are scaled down to 80% and; case 3> all the loads are scaled
up to 130%.
In the first case, all the DGs are connected to the grid but the DGs are working
at power factor=1. By adjusting the reactive power output of each DG, total system
loss is optimized. While the test feeders assume a static load, real loads are changing
constantly. Assuming that the the loads do not generally change steeply, 20% reduction
in all loads or 30% increase in all values from the base load is considered the worst
case scenario and the performance is measured for both these conditions. An
implication of low sensitivity values is that large dispatches are necessary to be able
to effect a significant change on the voltage. A very optimistic case where the DGs bear
most of the load is considered. But a consequence of this is that power production (both
real and reactive) needs to be stepped down when the loads are scaled down or the
substation will behave like a load and absorb power instead of feeding it to the grid.
Therefore, the DGs are scaled down by a factor of 30%. The DGs are not scaled up
when the load increases though.
The three algorithms for the three cases are tested on the IEEE 13 and 34 node
feeders (Appendix). For both the feeders, the capacitor banks are ignored and all
45
reactive support is assumed by the DGs. While the capacitor can also be modeled as a
DG with discrete output values and zero real power, it is simpler to ignore the capacitors.
Additionally, for the case of the 34 node feeder, the load on node 27 is not scaled since it
is a very large load and it is connected after a step down transformer. Hence voltage is
very sensitive to even minor changes in the size of this load (figure 5-1). It is assumed to
be a constant load.
The tables below tabulate the results for the three cases for the two feeder
configurations. Both Linear and Dispersed varieties optimize the reactive powers only if
a node is violating the voltage limits. PSO variety on the other hand, attempts to reduce
loss in any situation. If node voltage is outside limits, even that is adjusted. Therefore in
Tables 5-1 and 5-2 the gain in loss savings is zero for Linear and Dispersed for 13 node
feeder. In case of the 34 node feeder, because the voltage regulator taps cannot be
calculated accurately, not all the voltages are within acceptable limits, therefore the DG
outputs are varied. A huge gain in loss savings is observed for the 34 node feeder with
the maximum being achieved by the Dispersed method. But the method also required
the changing of taps. Since taps are changed only when DG optimization fails, it can be
inferred that PSO performs better in terms of optimization even if the results are not as
good. For the 13 node feeder, a modest 5% savings was observed.
Table 5-1. Comparison of optimization performance for case 1
Feeder Optimization Optimized Saving Estimation Tap Power Reductiontype Algorithm Loss (KW) (%) Error (KW) changes (KVA)
Linear 0 0 0 0 013 PSO 61.04 5.73 0.03 0 67.45
Dispersed 0 0 0 0 0
Linear 62.06 34.30 1.26 0 82.1534 PSO 55.10 41.67 0.39 0 53.46
Dispersed 47.26 49.98 0.50 3 82.53
The 34 node feeder seems to be more amenable to optimization. Significant
savings can be observed through optimization. Dispersed and PSO appear to be
46
working equally well although PSO gave slightly better results overall for case 2 (table
5-2). Because Linear limits itself to adjusting the voltage to the ANSI standard, its loss
optimization performance is not on par with the others.
Table 5-2. Comparison of optimization performance for case 2
Feeder Optimization Optimized Saving Estimation Tap Power Reductiontype Algorithm Loss (KW) (%) Error (KW) changes (KVA)
Linear 0 0 0 0 013 PSO 40.26 5.80 0.03 0 80.31
Dispersed 0 0 0 0 0
Linear 64.00 22.47 1.22 0 119.734 PSO 48.31 41.47 1.29 0 84.83
Dispersed 49.71 39.79 1.28 0 72.71
In table 5-3, ’NA’ implies that a steady state condition with no voltage violations
was not achieved through optimization. Fig 5-3 depicts the cause for this. It can be
seen in graph of phase C that after optimization, the minimum voltage is just above
0.95pu whereas the maximum voltage is far above 1.05pu. The reactive power dispatch
necessary to reduce the peak voltage will also push the lower voltage below the 0.95
range. In the next iteration, the minimum value is raised but the maximum value also
breaks the upper limit. The cycle repeats and a solution cannot be found. It needs
a concerted effort of the regulators and DGs to solve it. Hence PSO and Dispersed
converged to a solution but Linear did not.
In case of the 34 node feeder, node 5 just before the first regulator experiences a
low voltage which is further aggravated by the increase in load. The DG at the node
does not have sufficient capacity to raise the voltage. The voltage may in fact have been
made worse by the presence of the DG because the current flow from the DG may have
increased the voltage drop in the region. Therefore none of the methods have a positive
influence on the voltage and loss problem.
It can be seen that all the methods had a positive loss saving despite the magnitude
in some cases. Optimization also led to an overall reduction in power consumption in
47
Table 5-3. Comparison of optimization performance for case 3
Feeder Optimization Optimized Saving Estimation Tap Power Reductionnodes Algorithm Loss (KW) (%) Error (KW) changes (KVA)
Linear NA NA NA NA NA13 PSO 108.02 17.49 4.56 5 187.13
Dispersed 108.33 17.26 5.32 5 97.61
Linear NA NA NA NA NA34 PSO NA NA NA NA NA
Dispersed NA NA NA NA NA
A Phase A B Phase B
C Phase C
Figure 5-3. No result condition of the 13 node feeder
48
all cases. Therefore optimization is economical for not only reducing the line losses
but also the total power consumption. Thus if power has an associated generation and
distribution cost, expenses can be reduced with the use of DGs.
It is observed that the loss estimation error is also quite small. With increasing
scaling of the loads though, the error increases due to the approximations involved in the
sensitivity parameter, such as approximating the sensitivity curve to a linear relationship,
the minor influence of increasing reactive dispatch on sensitivity of DGs connected at
other locations, etc. Therefore, it might be useful to continuously monitor voltage and
dispatch reactive power rather than perform optimization when a voltage violation occurs
so that voltage difference and sensitivity variation can be contained.
It was observed in figure 5-2 that sensitivity is not a constant but can be approximated
to a linearly varying quantity. Then the sensitivity can be written as
β = α�Q + β0
where α is the slope of the line. Therefore
V = β�Q = α(�Q)2 + β0�Q
If voltage is a quadratic function, loss would be a quartic function. But the observed
improvement in estimation due to a quartic loss function was not significant enough to
account for a higher order loss function.
49
CHAPTER 6GENERATOR SITING AND SIZING
Chapter 5 discussed optimization of DG output for optimal loss performance where
the DGs were already connected at certain locations on the grid. However, looking at
the voltage sensitivity values, it is apparent that connecting DGs at some positions yield
better sensitivity than other nodes i.e. the same amount of power produces a higher
voltage difference for some DG locations than others. In this chapter sensitivity as
applied to determining the position of the DG and its size are discussed. The effect of
having too many or too few DGs are also considered.
6.1 Generator Siting
The location of the DG on the feeder is an important factor in determining the effect
it has on voltages at other nodes, power flow in the grid and consequently power loss.
For example, DGs connected lower down the feeder causes a greater change in voltage
for the same power than a DG connected upstream to it. Generally, farther away from
the substation a DG is located, higher are the sensitivity coefficients corresponding
to it. Figure 6-1 plots sensitivities for phase A of the 34 node feeder for 6 different DG
locations. Sensitivity is higher for almost all nodes when the DG is located at the last
node of the main feeder. The sixth scenario has the DG located on a lateral branch
rather than the main feeder unlike the first 5 cases.
Even when a node has a DG connected to it, it had a lower sensitivity when
compared to a DG located lower downstream. It should be noted that this relation
is valid for a general decreasing trend in the voltages. For other types of profiles,
the sensitivity patterns are different. Example, figure 6-2 shows the sensitivity for a
uniformly decreasing voltage profile on a 21 node feeder for different DG locations;
figure 6-3 shows sensitivity for an increasing trend. Similarly based on the true voltage
conditions, the sensitivity pattern for any feeder configuration may be calculated. In
50
Figure 6-1. Sensitivity of 34 node feeder for six different DG positions
general the voltage profile on most feeders is of the decreasing type, therefore sensitivity
of becomes more negative moving down the feeder.
Figure 6-2. Sensitivity for a decreasing voltage profile for different DG locations
For voltage control operations, achieving a large voltage change with a small
amount of dispatch is desirable for economic reasons. Based on the sensitivity values
we can infer that to conserve power, it is ideal to locate the DG on the node with the
highest impact on voltage - typically the nodes at the end of feeder lines and laterals.
But for loss optimization, it is not only necessary to use the least amount of power for
51
Figure 6-3. Sensitivity for an increasing voltage profile for different DG locations
compensation, it is also essential that lines carry the least amount of current. Current
and power sensitivity coefficients are useful in comparing these performances. Both
these indices however, can be derived from voltage sensitivity. Power sensitivity is
the total change in power that a unit amount of reactive power generation causes i.e.
equation (5–3) for a single DG and �QDG = 1unit. Comparing the power sensitivity at
different nodes and choosing the node with the smallest numerical value can decide the
best location.
Current sensitivity by definition, is the rate of change of line currents with change
in DG injection power. But current in a line can be represented using the voltage at the
nodes at the end of the line as:
Ii j = (Vi − Vj)/Zi j or
Ii j + �Ii j = (Vi + �Vi − Vj − �Vj)/Zi j
But �Vk = βk × 1, therefore
�Ii j = βi j/Zi j (6–1)
52
By comparing the �Ii j values for all pairs i , j and all DG locations, DG sites can
be identified. Figure 6-4 plots the current sensitivity values for all the nodes for all
possible DG locations on an example 20 node feeder (Appendix). Since the aim is to
reduce loss by reducing current, the DG site should be chosen so that the reduction in
current is maximum. For the first few candidate sites, current sensitivity is nearly flat
downstream of the DG node and drops for nodes upstream to it. For the last few nodes,
current sensitivity drops from around node 10 but increases downstream to it. This is not
preferable. Hence the best candidate is node 10 and the nodes immediately adjacent to
it.
Figure 6-4. Sensitivity of current to DG location
The selection procedure can be made even simpler considering loss sensitivity.
Loss sensitivity has already been defined in equations (5–1) and (5–2). By setting
�Vk = βk ∗ 1unit, loss sensitivity for a DG location can be obtained. Figure 6-5 plots
the variation of loss with different DG locations. Locating it at node 10 reduces loss the
maximum, hence it is the ideal candidate.
If multiple DGs are to be installed then it is better to choose one position at a time.
When another DG location is being cited, all the previously selected DGs are connected
to their respective nodes, then the loss sensitivities are calculated for all the candidate
nodes to decide the new DG location.
53
Figure 6-5. Sensitivity of power loss to DG location
Using power loss sensitivity also accounts for load distribution in the grid and
positioning the DG close to the load center so that current flow is reduced. The example
feeder had most of the load concentrated between node 4 and node 10 of the feeder.
The optimal node, as selected by power loss sensitivity and current sensitivity is the
node at the end of the load concentration, which also implies that of the 7 nodes with
the highest loads, node 10 has the highest voltage sensitivity. Therefore power loss
sensitivity combines the advantage of both voltage and current sensitivities into a single
quantity.
6.2 Generator Sizing
Generator sizing and generator siting are two interdependent operations with the
location of the DG site influencing the amount generation necessary at a particular
position and the size of already installed DGs influencing how many more generators
are necessary and where. Generator sizing can be done in many ways: generation
capacity can be added in multiples of some base quantity as needed through optimization
but usually sizing and siting is performed as a combined operation. Some DG
configurations are considered for installation in the system and optimization is carried
out to determine the best candidates from the available choices and the optimal site for
their installation.
54
In [41] sizing operation was done using loss sensitivity parameters to optimize
the loss characteristics of the grid. An analytical expression for loss was derived from
the current equations and bus incidence matrix. By differentiating this expression and
equating it to zero, the size of the DG was calculated so that net loss in the circuit is
minimum. With the loss expression of equation (5–1) and (5–2), the problem can be
solved as a simple quadratic equation. If the new configuration does not lead to out of
range voltages, the DG is retained. For example, for the 34 node feeder a -80 KVAR DG
was indicated as necessary to minimize loss.
But in line with the aim of compensation during faults and expansion of generation
capability using DGs, the intent is to calculate the minimum size of DG. In the IEEE 34
node feeder, node 27 often suffers from low voltage, reaching down to less than 0.9pu
in some cases. A DG which can provide for such a situation is required. If sensitivity is
assumed to be a constant, the amount of reactive power necessary can be calculated
as QDG = �V /β. The value of QDG might turn out to be too high. A work around for
this is to share the necessary power over multiple DGs. Or some portion of the reactive
power can be relegated to real power. Depending on the grid conditions, the real and
reactive power sensitivity values may be comparable. In such a case it maybe useful to
provide the minimum voltage support using real power injection and protection against
changes using reactive power dispatch. For example: if the lowest voltage is 0.88pu,
sensitivity is 6 × 10−4pu/KVAR and support capability up to 1pu is necessary, then
Q = 0.12/6 × 10−4 = 200KVAR. If the real power sensitivity is equal to the reactive
power sensitivity, for a DG operating at 0.85 power factor, the ratio of reactive and real
power is roughly 0.6. Therefore, P = 125KW and Q = 75KVAR.
If there’s more than one node to account for, a linear programming with inequality
constraints may be set up to simultaneously solve for multiple DG sizes as:
n∑j=1
βiqj Qj + βi
rjRj ≥ Vi ∀i = 1, ...m, j = 1, ... n (6–2)
55
where m is the number of nodes and n are the number of DGs and
Qj/Rj ≤ tan(cos−1 (θj)
)(6–3)
θj is the power factor of the DG.
6.3 Impact of DG Penetration on Loss
To study DG impact, the 34 node feeder was chosen. Up to 10 DGs were free to be
placed. DGs were added one at a time and each one was placed at a node so that the
total loss was a minimum. The size of the DGs was varied depending on the number of
generators. The DG size was fix calculated as Loadtotal/3 ∗ P/100/N where Loadtotal is
the total load on all the 3 phases of the system, P is the penetration in percent and N is
the number of DGs. Penetration was varied in steps of 5% from 0 to 80% and number of
DGs was varied from 1 to 10 in steps of 1. Losses were plotted a function of the number
of DGs and penetration (figure 6-6).
Figure 6-6. Variation of losses for different penetration levels and number of DGs
The observed data suggests that loss reduces with increasing DG penetration but
the reduction with increasing number of DGs is not very apparent. At larger penetration
levels, having more DGs does seem to be helpful but in the case of the 34 node feeder,
10 were not necessary. Similar loss levels were observed even with 5 or 6 DGs. It
was also observed that while multiple DGs were located at the same node at lower
56
penetrations, they were scattered across a few nodes at higher penetration and
DG count; clustering of DGs at the a node indicates that a bigger sized generator is
necessary at that location and the total number of DGs necessary is not really 10 but
the number of unique DG locations. This also suggests that loss may increase if N
unique locations are desired and different size DGs are not preferred. Siting and sizing
therefore plays an important role in loss minimization.
57
CHAPTER 7CONCLUSION
Integration of distributed generation into the grid is a hot research topic and it
promises many benefits. But it also brings with it many problems related to control,
protection, islanding, etc. In this thesis one aspect of that problem, namely distribution
line loss, was tackled using sensitivity coefficients. An algorithm was devised to mitigate
the losses and improve power flow.
It was found that including distributed generation in the distribution grid can help
reduce the line losses by reducing the maximum current flowing in a line. Since loss is
proportional to the square of the current, even small reduction in current can improve the
voltage and loss profile significantly. Inclusion of DGs and proper dispatch of reactive
power also led to a reduction in the total power consumed in the feeder. Therefore DGs
can play an important role in peak shaving operations. It is economically advantageous
to integrate DGs into the grid. DGs also contribute to the capacity expansion of the utility
grid and prevent the purchase of expensive power from the energy market.
However, DGs in large numbers can play havoc with existing control operations
such as voltage regulation. A line voltage regulator estimates the voltage condition at
a downstream node and adjusts its taps to control the voltage at the target node. The
estimation is based on the current flowing through its line drop compensator circuit.
By changing the current flow pattern, DGs cause the regulators to underestimate the
severity of voltage problems and cause inadequate control. Therefore, when DGs are
included in the grid in sufficient quantity it is essential for voltages to be measured rather
than estimated. And it may also become necessary for DGs themselves to participate in
the control operation.
Optimizing loss in the grid requires complete knowledge of the system conditions for
efficient operation. It is better performed as a centralized control technique. However, it
is still possible to obtain satisfactory results through localized control with coordination
58
of the other DGs. Such a technique was implemented using a multi agent control
operation.
Loss optimization can greatly benefit from the proper location of DGs in the
distribution system. From simulations on an example system it was observed that
placing DGs close to the load concentration is beneficial even though voltage sensitivity
would indicate placement near the end of the feeder line because the same amount
of power dispatch can effect a larger change in voltage. Loss sensitivity is a better
parameter to decide the siting of DGs. It has also been found possible to decide the size
of the DG using voltage sensitivity. Simulations on the penetration of DGs in the grid and
to an extent, increasing the number of DGs were found to favor minimization of loss. All
results regarding loss seem to favor the inclusion of distributed generators into the grid.
However some observations during the study do call for further research such as:
the small value of sensitivity. It implies large dispatch for a significant change in voltage,
which further implies large DGs. That may cause the substation to absorb power instead
of supplying it. Therefore, care must be taken during DG sizing to ensure that current
flow is not reversed at the substation bus. A fixed DG size would interfere with this when
the load is varying. Therefore real power output of the DGs must also be varied along
with the reactive power, especially in small systems.
Simulations in this study were implemented on small sized systems with very few
nodes. Simulations on bigger and more complicated networks need to be performed and
studied, particularly the behavior of sensitivity and the effect of penetration and number
of DG on the system. Future studies including the model of the distributed generator
and its response to the the dynamic behavior of the grid are necessary. The response to
increasing penetration of the distributed generators,the varying load conditions and the
ability of the generators to track load changes and control operations without interfering
with each other even at high penetrations need to be studied.
59
APPENDIX: FEEDER CONFIGURATIONS
Standard IEEE test feeders were chosen for all voltage control and power
optimization simulations [43]. The feeders chosen were of 13 nodes and 34 nodes
respectively. The one line diagrams of the two feeders are shown in Figure 7 and 7.
An example 20 node feeder was used to test DG location using the various sensitivity
coefficients.
IEEE 13 Node Feeder. The 13 node feeder is a small, highly loaded, wye-connected,
unbalanced test feeder [44] with capacitor compensation as well as a voltage regulator.
The nodes have been renumbered according to Figure 7 for convenience. For voltage
control simulations, two DGs at nodes 2 and 8 are considered. Both the DGs are of the
same capacity - 500KW and a maximum of 300KVAR. The DGs are considered to have
a constant real power output but the reactive power is varied according to necessity.
Figure A-1. Schematic of IEEE 13 node test feeder. Source: IEEE 13 Node Feeder [43]
60
IEEE 34 Node Feeder. The 34 node feeder is a long, lightly loaded, wye-connected,
unbalanced test feeder [44] based an an actual feeder in Arizona. It has two capacitor
banks and two lne voltage regulators for voltage control. The nodes have been
renumbered according to Figure 7 for convenience. For voltage control simulations,
five DGs are located at nodes 5, 9, 15, 19 and 27. Attempting to size all the DGs
equally resulted in voltge violations so they are sized at either 100 KW or 120 KW and a
maximum of 60KVAR.
Figure A-2. Schematic of IEEE 34 node test feeder. Source: IEEE 34 Node Feeder [43]
Example 20 node Feeder. The 20 node feeder is an overloaded feeder with a
major load concentration at the beginning of the feeder with about 75% of the total
load connected equally to the nodes 4 through 10. It was designed primarily to check
if the load center can be detected by the different sensitivity coefficients. The feeder
is a balanced system with nodes located at uniform distances and the lines having
R = 1,X = 1 and no impedance between the phases. Like the 34 node standard feeder
it operates at 24.9 KV.
61
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BIOGRAPHICAL SKETCH
Anurag R. Katti completed his Bachelor of Engineering in electronics and communication
engineering from Visvesvaraya Technological University, Belgaum in 2008. He worked at
the Indian Institute of Science, Bangalore after graduation on swarm based optimization,
pattern recognition, robotics and control. In 2009 he decided to pursue graduate studies
and he was admitted to the University of Florida for the Master of Science program in
electrical engineering with a focus on control systems. He soon realized his interest in
green energy and power systems. His current research interests include power systems
and control, smart grids, distribution systems, green energy and optimization. This
thesis is the culmination of his work in the field and completes the Master of Science
thesis requirements.
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