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AMERICAN UNIVERSITY OF BEIRUT MAXIMUM POWER POINT TRACKING SYSTEM: AN ADAPTIVE ALGORITHM FOR SOLAR PANELS by MOHAMMED ALI SERHAN A thesis submitted in partial fulfillment of the requirements for the degree of Master of Engineering to the Department of Electrical and Computer Engineering of the Faculty of Engineering and Architecture at the American University of Beirut Beirut, Lebanon January 2005

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PV modules used to be expensive, but in recent years, their price has beenslowly dropping, and as they become increasingly economical, they will be used inmore applications. In the U.S. the cost of installing solar had fallen from $55 per peakwatt in 1976 to about $4 per peak watt in 2001 [1]. PV modules output efficiency hasalso increased in recent years. PV cells, having power conversion efficiencies as high as31%, have been developed in a laboratory environment over the last decade [2]. Withthese growths in photovoltaic technology, there is no doubt that PV will have a goodstand in the near future. However in this thesis, the emphasis is on the study of PVsystem control part.1.2.

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AMERICAN UNIVERSITY OF BEIRUT

MAXIMUM POWER POINT TRACKING SYSTEM: AN ADAPTIVE ALGORITHM FOR SOLAR PANELS

by MOHAMMED ALI SERHAN

A thesis submitted in partial fulfillment of the requirements

for the degree of Master of Engineering to the Department of Electrical and Computer Engineering

of the Faculty of Engineering and Architecture at the American University of Beirut

Beirut, Lebanon January 2005

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AMERICAN UNIVERSITY OF BEIRUT

MAXIMUM POWER POINT TRACKING SYSTEM: AN ADAPITIVE ALGORITHM FOR SOLAR PANELS

by MOHAMMED ALI SERHAN

Approved by: ______________________________________________________________________ Dr. Sami Karaki, Professor Advisor Electrical and Computer Engineering ______________________________________________________________________ Dr. Fouad Morad, Professor Member of Committee Electrical and Computer Engineering ______________________________________________________________________ Dr. Riad Chedid, Professor Member of Committee Electrical and Computer Engineering Date of thesis defense: January 7, 2005

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AMERICAN UNIVERISTY OF BEIRUT

THESIS RELEASE FORM

I, Mohammed Ali Serhan authorize the American University of Beirut to supply copies of my thesis to

libraries or individuals upon request. do not authorize the American University of Beirut to supply copies of my thesis to

libraries or individuals for a period of two years starting with the date of the thesis defense.

____________________ Signature

____________________ Date

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v

ACKNOWLEDGMENTS

I would like to thank my advisor Dr. Sami Karaki for the enlightening advice and guidance he provided during the elaboration of this work. Many thanks go to Dr. Fouad Mrad and Dr. Riad Chedid, who were in my committee, for providing a lot of insightful comments during the presentation of this thesis. I'm also very grateful to the dearest Dr. Lana Al Chaar, who proposed the topic in the first place, for her support. All respect and admiration go to Mr. Antoine Al Asal, a true brother, partner and friend. Warm love and support from my parents is the main factor of success throughout all years of study. Lastly, praise goes to Almighty Allah whose help and guidance has given me the strength needed to complete this work.

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AN ABSTRACT OF THE THESIS OF

Mohammed Ali Serhan for Master of Engineering Major: Electrical Engineering

Title: Maximum Power Point Tracking System: An Adaptive Control Algorithm for Solar Panels.

Energy is fundamental to the wellbeing of our society—it powers our homes, businesses, and industries. However, energy, obtained from fossil fuels is presenting challenges to many nations; not only these energy resources are depletable but are also major contributors to atmospheric pollution and global warming. ‘Renewable Energy’ is a new trend in clean energy production. This includes power generated from water, wind, solar radiation, biomass and other resources. This development of renewable power sources will save fossil fuel resources, and help improve the quality of our environment. One of the renewable energy sources, Photovoltaic systems have a great potential because it makes use of the most abundant energy on earth that is sunlight.

As the maximum power operating point (MPP) of the PV module changes with atmospheric conditions, e.g. solar radiation and temperature, an important consideration in the design of efficient PV system is to track the MPP correctly. The objective of this thesis is to design and build a Maximum Power Point Tracker (MPPT) to charge a lead acid battery.

The design consists of a PV panel, a 12V battery, H-bridge converter and a control module that uses the PIC16F874 microcontroller. The controller obtains the current and voltage values from the PV array and performs pulse width modulation (PWM) on the converter to charge the battery with maximum available power. Battery’s state of charge is also controlled by the microcontroller to protect the battery from being overcharged. The Perturb and Observe (PAO) method is used as an algorithm to track the maximum power point of the PV array. The performance of the PAO algorithm in tracking maximum power point has been improved by implementing an adaptive perturbation scheme to track correctly the MPP in case of rapidly varying weather conditions and to get high conversion efficiency.

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CONTENTS

Page

ACKNOWLEDGEMENTS ...………………………………..………… v ABSTRACT…...……………………………………….……………….….… vi LIST OF ILLUSTRATIONS……………….…………………...……… x LIST OF TABLES......................................................................................... xv Chapter 1. INTRODUCTION…….….…………………………………………... 1 1.1. An Overview ……………………..…………..…….………..... 1 1.2. Brief Background ………….…………………...……………..... 1 1.3. Problem definition and motivation …...……………………..….. 2 1.4. Scope ……………………………………………………………… 3 2. LITERATURE REVIEW …………………………………………. 4 2.1 Maximum Power Point Tracker …..…………....................... 4 2.2. Switched-Mode Converters….……………......................... 5 2.3. Controller ………….………………………………………….... 5 2.3.1 Voltage feedback control …………………………….. 5 2.3.2 Power feedback control ………………………………. 6 2.4. MPPT control Algorithms …………………………………....... 6 2.4.1 Perturb and Observe technique ……………………….. 6 2.4.2 Incremental Conductance technique ………………….. 8 2.4.3 Constant Reference Voltage ………………………….. 10 2.4.4 Other techniques: CMPPT, VMPPT…………………… 11 2.5. Comparative Study………………………………………………. 12 vii

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2.6. Contribution of this Thesis………………………………………… 13 3. SYSTEM COMPONENTS MODELING ............…………... 14 3.1. Photovoltaic ………..……………………………………....…….. 14 3.1.1 Solar Cells ………………………………………………. 14 3.1.2 Photovoltaic effect …………… ………………………… 15 3.1.3 Electric Model of the PV cell …………………………… 15 3.3.4 Irradiation and cell Temperature effect ………………. 17 3.3.5 PV models and PV arrays ………………………………. 18 3.2. Battery ……………………………………………………………. 18 3.2.1 Lead Acid battery ………………………………………. 19 3.2.2 Battery Chemistry ……………………………………. 19 3.2.3 Amp-Hour Capacity and Charge Rate ……………….. 20 3.2.4 State of Charge 20 3.2.5 Deep cycles vs. starter batteries ……………………… 21 3.2.6 Lifespan of batteries ……………………………………. 22 3.2.7 Battery hazards …………………………………………. 22 3.3. DC-DC Converters …………………………….………………… 23 3.3.1 Switching converter Topologies ……………………….. 23 3.3.2 Non-Isolated Switching converters …………………….. 24 3.3.2.1 Buck Converter 24 3.3.2.2 Boost Converter 32 3.3.2.3 Buck-Boost Converter 34 3.3.3 Isolated DC-DC Converters ……………………………. 35 3.3.3.1 Flyback Conveter 36 3.3.3.2 Forward Converter 37 3.3.3.3 H-bridge Converter 38 3.4. Zero Voltage Switching ……………………..…………………… 39

4. MPPT SIMULINK MODEL ………………………………… 42 4.1. Introduction……………………………....…….………………….. 42 4.2. Simulink Blocks …………….……………………………………. 42 4.3. What is an S-Function …………………………………………… 43 4.4. Implementation of PV cell using S-Function ………………….… 44

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4.5 Converter and Controller Blocks ………………………………… 45 4.6 Battery Block ……………………………………………………. 49 5. MPPT SYSTEM IMPLEMENTATION …………………… 52

5.1. Introduction ……………………………………………………….. 52

5.2. MPPT System ……………………………………………………….. 52 5.2.1 Microcontroller …………………………………………. 53 5.2.2 PV-PIC Interface Circuit ………………………………. 54 5.2.3 Buck-Boost Converter …………………………………. 54 5.2.4 PIC-Converter Interface Circuit …………………….. 54

5.3. Hardware Design ……………..………………………………….. 55

5.3.1 Controller and Converter Design ……………………. 55 5.3.2 Phase Splitter circuit …………………………………. 59 5.3.3 Switch Driver ‘A’ and ‘B’ …………………………… 60 5.3.4 H-Bridge …………………………………………………. 62 5.3.5 Transformer, Rectifier and Filter ………………………. 63

5.4. Software Design …………………………………...……………... 66 5.4.1. Main Program …………………………………………. 66 5.4.2. Charging-Tracking mode ……………………………… 67

6. SYSTEM RESULTS AND DISCUSSION……………….... 74 6.1. Introduction ……………………………..…..….………………... 74 6.2. PV model Validation ……………………..…………………….... 74 6.3. Simulink Simulation Results …………………………….……..… 78 6.4. Hardware Results ………………………………………………… 81 6.5. Comparison of Tracking algorithm ………….………………….. 85 6.5.1 Minor change in the weather conditions ………………. 85 6.5.2 Major change in the weather conditions ………………. 87 6.6. Power Budget ................................................................................. 88 6.6.1. Inductor conduction loss 88 6.6.2. Diode conduction loss 89 6.6.3. MOSFET conduction loss 89 6.6.4. Transformer power loss 90

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6.6.5. Other power factor factors 92 7. CONCLUSIONS AND FUTURE WORK …......................... 94 7.1. Summary ………………………………………………………... 94 7.2. Testing Environment ……………………………………………… 94 7.3. Better Tracking Algorithm ……………………………………….. 95 7.4. Simulink Model ………………………………………………….. 96 7.5. Future Work ……………………………………………………… 96 APPENDIX A……..………………………………………………………….. 98 1. Matlab program code ……………………………………………... 98 APPENDIX B…………………………………………………………………. 102 1. PCB circuit design ……………………………………………..... 102 APPENDIX C…………………………………………………………………. 105 1. Assembly program code ………………..………………………..... 105 APPENDIX D……………………………………………………………….. 130 1. Datasheet ………………………………………………………... 130

REFERENCES……..……………………………………………………… 132

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ILLUSTRATIONS Figure Page 1.1. (a) The I-V characteristic curve, (b) The PV panel Maximum Power

Point.......................................................................................................... 2

2.1. (a) PV panel Insolation characteristics (b) PV panel Temperature characteristics …………………………………………………………. 4

2.2. PAO technique ……………………………............................................ 7

2.3. Deviation of the PAO technique from the MPP ...................................... 8

2.4. The slope ‘conductance’ of the P-V curve …………………………… 8

2.5 Flow chart of ICT algorithm…………………………………………… 9

2.6. MPPT control system with constant voltage reference ........................... 11

2.7. The conventional MPPT controller using open circuit voltage (Voc) ... 12

3.1. The PV cell ……...................................................................................... 14

3.2. Model for a PV cell ................................................................................. 15

3.3. (a) Effect of Varied Irradiation, (b) Effect of Varied Temperature on

the PV cell …………….……………………………………………. 17

3.4. (a) PV Module, (b) PV Array ………………….................................... 18

3.5. Buck Converter …….............................................................................. 24

3.6. Voltage and current changes ………………………………………….. 25

3.7. Inductor current for (a): continuous mode (b): discontinuous mode … 27

3.8. Buck Converter at Boundary ……........................................................... 27

3.9. Buck Converter - Discontinuous Conduction ......................................... 28

3.10. Output Voltage vs Current …….............................................................. 30

3.11. Output voltage ripple in a step-down converter ...................................... 31

3.12. Boost Converter Circuit ……………....................................................... 32

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3.13. Voltage and current waveforms (Boost Converter) ……………………. 33 3.14. Schematic for buck-boost converter ........................................................ 34

3.15. Waveforms for buck-boost converter …………………………………. 35

3.16. Flyback converter ………………………….………………................... 36

3.17. Forward Converter ………….................................................................. 37

3.18. H-bridge Converter .................................................................................. 39

3.19 Waveforms …………………………………………………………….. 39

3.20. Power loss associated with high switching frequencies ......................... 40

3.21. ZVS resonant-switch dc-dc converter ………….................................... 41

4.1. PV array 'MPPT' system ……………………..………........................... 43

4.2. S-Function block with three inputs and two outputs …........................... 43

4.3. Model for a PV cell ................................................................................. 44

4.4. PV Cell S-Function block ……............................................................... 45

4.5. Buck converter and Controller blocks ..................................................... 46

4.6. Controller Block Implementation ……………........................................ 46

4.7. MPP tracking algorithm Flow Chart …………....................................... 47

4.8. Different current levels with respect to variable duty cycle ................... 48

4.9. MPPT tracking scheme using a variable step size ……………………. 49

4.10. Battery Model Block ………………………......................................... 50 4.11. PV array 'MPPT' system ………………………………………………. 50 5.1. The PV maximum power point tracking system …………………........ 53 5.2. Converter and Controller ……………………………………………… 55 5.3. (a) 50% duty cycle switching (b) variable duty cycle switching……… 56 5.4. Bridge output due to small and large phase difference ………………. 56

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5.5. Case of zero phase difference between V1 and V2 ……………………. 57 5.6. Case of V1 and V2 being out of phase ……………………………….. 57 5.7. PWM output controls the Bridge output ……………………………… 58 5.8. PWM, Bridge, Rectified and Filtered voltage waveforms …………… 58 5.9. Phase splitter output waveforms …………………………………….. 59 5.10. Phase splitter schematic diagram ……………………………………. 60 5.11. Driver A output waveforms ………………………………………….. 60 5.12. Driver ‘A’ schematic diagram ……………………………………….. 61 5.13. Charging and discharging stages …………………………………….. 62 5.14. Bridge Converter schematic diagram ………………………………… 63 5.15. Transformer, Rectifier and Filter waveforms ……………………….. 64 5.16. Main Program Flow Chart ……………………………………………. 67 5.17. The conventional PAO algorithm Flow Chart ………….………….… 68 5.18 Scanning with small step in case of varying weather conditions …….. 69 5.19 The Adaptive PAO algorithm Flow Chart ……………………………. 70 5.20. Hunting with large step size ∆ ………………………………………. 70 5.21. Hunting with smaller step size ∆/2 ………………………………….. 71 5.22. MPP scanning direction ……………………………………………… 72 5.23. Locking on the MPP with duty-cycle ratio 1/255 …………………… 72 5.24. Scanning in case of varying weather conditions …………………….. 73 6.1. I-V characteristic curves for different Insolation levels ……………… 75 6.2. P-V characteristic curves for different Insolation levels …………….. 75 6.3. I-V characteristic curves for different temperatures …………………. 76 6.4. P-V characteristic curves for different temperatures ………………… 76 6.5. Load circuit schematic diagram ……………………………………… 77

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6.6. PV characteristic curves under different Insolation levels …………. 77 6.7. Characteristic curves of the 'BP 380' PV module using the load circuit 78 6.8. Characteristic curves of the 'BP 380' module using the Simulink model 78 6.9. MPPT Simulink Model ………………………………………………... 79 6.10. P-V characteristic curve of the PV array at 800W/m2, 27oC …………. 79 6.11. Switching Power, Voltage, and Current supplied to the converter …… 80 6.12. Power, Voltage, and Current delivered to the battery ………………… 80 6.13. Characteristic curves: (a) I-V curve, (b) P-V curve ………………….. 81 6.14. VB performance monitor ……………………………………………. 82 6.15 Tracking the MPP in case of varying Insolation level ………………. 84 6.16 Tracking scheme for minor change in the weather conditions ………. 86 6.17 Tracking scheme for major change in the weather conditions ………. 88 6.18 Primary winding current waveform…………………………………… 90 6.19 Waveforms across the terminals of the transformer ………………… 90 6.20. Diodes’ current waveform during different intervals ………………… 91 6.21. Transformer windings contribution to power loss …………………… 92

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TABLES Table Page 6.1. MPP readings on a sunny day in October……........................................ 81

6.2. Snapshots of MPP Recorded Data............................................................ 83

6.3. MPP Daily Average Recorded Data 2004…............................................ 83

6.4. Tracking with adaptive incremental step ∆a ………………………..…….. 87

6.5. Scanning with adaptive incremental step ∆a ………………………..…….. 88

6.6. Power Budget……………………........................................................... 93

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To My Family …..

AND

To All Palestinians Who Struggle For Freedom!

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CHAPTER 1

INTRODUCTION

1.1. An Overview

As green house effects and environmental issues become more of a concern,

renewable energy is one of the options in reducing pollution. Furthermore, fossil fuel

resources used in the production of power are dwindling and becoming more expensive;

‘Renewable Energy’ is the new trend in energy production to reduce emission in the

long run. This includes power generated from water, wind, solar radiation, biomass and

other resources. These resources are considered to be clean and continuously found in

nature.

PV modules used to be expensive, but in recent years, their price has been

slowly dropping, and as they become increasingly economical, they will be used in

more applications. In the U.S. the cost of installing solar had fallen from $55 per peak

watt in 1976 to about $4 per peak watt in 2001 [1]. PV modules output efficiency has

also increased in recent years. PV cells, having power conversion efficiencies as high as

31%, have been developed in a laboratory environment over the last decade [2]. With

these growths in photovoltaic technology, there is no doubt that PV will have a good

stand in the near future. However in this thesis, the emphasis is on the study of PV

system control part.

1.2. Brief Background

The world trend nowadays is to find a non-depletable and clean source of

energy. The most effective and harmless energy source is probably solar energy, which

1

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for many applications is so technically straightforward to use. Use of solar energy

instead of fuel combustion, particularly for simple application like low and medium

temperature water heating and for stand alone PV systems in rural areas, can reduce the

load on the environment.

Solar energy for electricity generation can be harvested by the use of

photovoltaic (PV) array, which has an optimum operating point called the maximum

power point (MPP) as shown in Fig. 1.1. This MPP varies depending on cell

temperature and the present insolation level [3]. To get the maximum power from the

PV, a maximum power point tracker (MPPT) must be used.

Fig. 1.1 (a) The I-V characteristic curve, (b) The PV panel Maximum Power Point

1.3. Problem Definition and Motivation

Several maximum power point tracker (MPPT) algorithms are implemented to

track this MPP, yet many research works to implement a low-cost highly efficient

MPPT algorithm are being conducted. This algorithm should respond in a short time to

the change in the atmospheric conditions to avoid energy loss. Moreover it should not

2

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be stuck in local power peaks if any; this happens in case of partial shadowing or dust

on the PV panel.

Furthermore, the converter has to be very efficient, in order to transfer more

energy to the load. This is achieved by using a simple soft-switched topology. Much

higher conversion efficiency at lower cost will then result, making the MPPT an

affordable solution for small PV energy systems.

1.4. Scope

The objective of this thesis is to design and build an experimental model,

develop a Simulink model of a stand-alone photovoltaic system with an MPPT

controller, and to analyze its operation.

Chapter 2 reviews the various literature of maximum power point tracking

algorithms. Perturb and Observe, Incremental conductance, Constant reference voltage

and other algorithms are presented in this chapter.

Chapter 3 will highlight the equations that are needed to implement the MPPT

system. PV cells electrical representation and current-voltage relation, Lead acid battery

chemistry and hazards, and dc-dc converters are presented in this chapter.

Chapter 4 and Chapter 5 show the Simulink block and the experimental model

that were implemented. Chapter 6 will discuss the simulated and experimental results.

In this chapter the hardware model data for changing weather conditions are evaluated.

Chapter 7 will conclude the thesis and will look on the future development of

the thesis. References and appendices are attached at the end of this thesis report.

3

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CHAPTER 2

LITERATURE REVIEW

2.1. Maximum Power Point Tracker

Solar energy can be harvested by the use of a photovoltaic (PV) array, which

has an optimum operating point called the maximum power point (MPP) as shown in

Fig. 1.1(b). The I-V curve will change as the temperature and insolation levels change

as shown in Fig. 2.1, thus the MPP will vary accordingly [4]. So we need to control

either the operating voltage or the current to get maximum power from the PV panel at

the prevailing temperature and insolation conditions using a maximum power point

tracker (MPPT) which should meet the following conditions [5]:

• Operate the PV system as close as possible to the MPP irrespective of the

atmospheric changes.

• Have low cost and high conversion efficiency.

• Provide an output interface compatible with the battery-charging

requirement.

Fig. 2.1 (a) PV panel Insolation characteristics (b) PV panel Temp characteristics [4]

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The MPPT consists of two basic components: a switched-mode dc-dc converter

and a controller.

2.2. Switched-mode dc-dc converter

The origins of switched-mode converters are linked with the developments in

inverter circuitry. An inverter is a processor for generating AC from DC and is,

therefore, a constituent of some forms of switched-mode power supplies. The DC-DC

converter will change the energy at one potential, stored as magnetic energy in an

inductor, to another potential. Different topologies can be used to construct DC-DC

converters: step down converter (buck converter), step up converter (boost converter),

or a combination of both step up- step down converter (buck-boost converter). The

converter in MPPT will adjust the PV array output voltage to the battery voltage while

driving the PV panel at its MPP.

2.3. Controller

The controller should keep testing if the PV system is operating at the PV

maximum power point; it should force the system to track this MPP. This could be done

by continuously measuring the voltage and current from the PV array, and then

performing either voltage or power feedback control [6].

2.3.1 Voltage feedback control

The control variable here is the PV array terminal voltage. The controller

forces the PV array to operate at its MPP by changing the array terminal voltage.

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However it has a major drawback where it neglects the variation in the temperature and

insolation level [6, 7].

2.3.2 Power feedback control

The control variable here is the power delivered to the load. To achieve

maximum power the quantity dvdp is forced to zero. This control scheme is not

affected by the characteristics of the PV array, yet it maximizes power to the load and

not power from the PV array [6, 7].

2.4. MPPT controller Algorithms

Several algorithms were proposed to accomplish MPPT controller. Published

MPPT methods include: (1) Perturb and Observe (PAO) [3], (2) Incremental

Conductance Technique (ICT) [3], and (3) Constant Reference Voltage/Current [3, 5].

2.4.1. Perturb and Observe (PAO)

The Perturb and Observe method has a simple feedback structure and few

measured parameters. It operates by periodically perturbing (i.e. incrementing or

decrementing) the duty cycle controlling the array current as shown in Fig. 2.2 and

comparing the PV output power with that of the previous perturbation cycle. If the

perturbation leads to an increase (or decrease) in array power, the subsequent

perturbation is made in the same (or opposite) direction. In this manner, the peak power

tracker continuously seeks the peak power condition. The flow chart for this algorithm

will be discussed in chapters 4 and 5.

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Fig. 2.2 PAO technique [5]

The PAO technique is easily implemented, costs the least among the other

available techniques, and is considered to be a very efficient scheme in terms of power

being extracted from the PV array [8]. However the PAO technique will be tricked in

catching the MPP under rapid varying solar radiation [3]. If the Insolation level

increases (I2 > I1) then the controller will assume that the incremental step should keep

moving in the same direction toward point when the new MPP is really in the other

direction at point as shown in Fig. 2.3 [3]. So for the PAO algorithm, the power

has increased because the new MPP is toward the right whereas it has already been

passed at point . In the following perturbation the PAO algorithm will increment

the array operating voltage further right, point . In this way the PAO algorithm will

continue to deviate from the actual MPP, with a corresponding power loss, until the

solar radiation change slows or settles down. [3]

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Fig. 2.3 Deviation of the PAO technique from the MPP [3]

2.4.2. Incremental Conductance Technique (ICT)

The basic idea is that the derivative of the power with respect to the voltage

( dvdp ) vanishes at the MPP since it is the maximum point on the curve as shown in

Fig. 2.4. It is also noticeable from Fig. 2.4 that to the right of the MPP the derivative is

decreasing while to the left of the MPP it is increasing.

Fig. 2.4 The slope ‘conductance’ of the P-V curve [9]

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Furthermore the derivative dvdp can be written as:

dVdP = dVVId ).( = I + V VddI ; where ∆G = VddI is the incremental

conductance.

Hence: (V1 ) dVdP =

VI + VddI ; where G =

VI is the source conductance.

So at the MPP ( dvdp =0), we get VddI = V

I− i.e. G = - ∆G.

The ICT algorithm checks for MPP by comparing VddI againstV

I− till it

reaches the voltage operating point at which the incremental conductance is equal to the

source conductance [3, 10]. The flow chart for the ICT algorithm is shown in Fig. 2.5.

Fig. 2.5 Flow chart of the ICT algorithm [3]

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The algorithm starts by obtaining the present values of I and V, then using the

corresponding values stored at the end of the preceding cycle, Ib and Vb, the incremental

changes are approximated as: dI = I – Ib, and dV =V - Vb and according to the result of

this check, the control reference signal Vref will be adjusted in order to move the array

voltage towards the MPP voltage. At the MPP, VddI = V

I− , no control action is

needed, therefore the adjustment stage will be bypassed and the algorithm will update

the stored parameters at the end of the cycle as usual. Another check is included in the

algorithm to detect whether a control action is required when the array was operating at

the previous cycle MPP (dV = 0); in this case the change in weather condition will be

detected using (dI ≠ 0) [3].

This technique offers good performance under varying atmospheric conditions

contrary to the PAO technique. However it requires complete mathematical model for

the topology used and its complex circuitry adds to the cost of the MPPT controller [9].

2.4.3. Constant Reference Voltage

One very common MPPT technique is to compare the PV array voltage (or

current) with a constant reference voltage (or current), which corresponds to the PV

voltage (or current) at the maximum power point, under specific atmospheric conditions

Fig. 2.6. The resulting difference signal (error signal) is used to drive a power

conditioner, which interfaces the PV array to the load. Although the implementation of

this method is simple, the method itself is not very accurate, since it does not take into

account the effects of temperature and irradiation variations [5].

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Fig. 2.6 MPPT control system with constant voltage reference [5]

2.4.4. Other techniques

Other techniques exist such as current-based maximum power point tracker

‘CMPPT’ and voltage-based maximum power point tracker ‘VMPPT’ [9]. Employed

numerical methods show a linear dependence between the “cell currents corresponding

to maximum power” and the “cell-short circuit currents”. The current IMPP operating at

the MPP is calculated using the following equation:

IMPP = MC ISC (2.1)

where MC is called the ‘current factor’ and differs from one panel to another. This factor

MC differs from one panel to another and is affected by the panel surface conditions,

especially if partial shading covers the panel [11].

Similarly the MPP operating voltage is calculated directly from VOC:

VMPP = MV VOC (2.2)

where MV is the ‘voltage factor’.

The open circuit voltage VOC is sampled by analogue sampler, and then VMPP is

calculated by equation (2.2). This operating VMPP voltage is the reference voltage for the

voltage control loop as shown in Fig. 2.6. This method always, “results in a

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considerable power error because the output voltage of the PV module only follows the

unchanged reference voltage during one sampling period” [12].

Fig. 2.7 The conventional MPPT controller using open circuit voltage Voc [12]

Others argue that these two techniques are considered to be “fast, practical,

and powerful methods for MPP estimation of PV generators under all insolation and

temperature conditions” [13].

2.5. Comparative Study

A comprehensive experimental comparison between different MPPT

algorithms was prepared at South Dakota State University [14]. After presenting the

advantages and disadvantages of each algorithm, an experiment for the same PV array

setup was run. Results showed that the ICT method has the highest efficiency (98%) in

terms of power extracted from the PV array, next is the PAO technique efficiency

(96.5%), and finally the Constant Voltage method efficiency (88%).

Although the ICT method offers good performance under rapidly changing weather

conditions and seems to provide the highest tracking efficiency, four sensors are

required to perform the measurements for computations and decision making [3]. If the

system requires more conversion time in tracking the MPP, a large amount of power

loss will occur [6]. On the contrary, if the sampling and execution speed of the

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perturbation and observation method is increased, then the system loss will be reduced.

Moreover, this method only needs two sensors, which results in the reduction of

hardware requirement and cost. Thus, the complexity of the ICT algorithm and the

increased cost of its circuitry, “encourage all to implement the PAO technique” [14].

2.6 Contribution of this Thesis

In this thesis, a hardware MPPT system and a Simulink MPPT model are

designed and tested for different PAO algorithms. The conventional PAO algorithm is

enhanced in a way to overcome the loss in the solar power tracking efficiency

associated with being misled by the scanning direction under rapidly varying weather

conditions. So an adaptive PAO algorithm, which forces the system to respond faster to

any changes in the insolation level irrespective of where the previous operating point

MPP was and without deteriorating the tracking efficiency, is implemented. Chapter 5

discusses the implementation of this algorithm.

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CHAPTER 3

SYSTEM COMPONENT MODELING

3.1. Photovoltaic

The word photovoltaic is a combination of the Greek word for light and the

name of the Italian physicist Alessandro Volta. It refers to the direct conversion of

sunlight into energy by means of solar cells. The conversion process is based on the

photoelectric effect discovered by Alexander Becquerel in 1839.

3.1.1. Solar Cells

A solar cell is a device that uses the photoelectric effect to generate electricity

from light. Over 95% of all the solar cells produced worldwide are composed of the

semiconductor material Silicon (Si) with efficiency up to about 17% [15]. However

solar cells, having power conversion efficiencies as high as 31%, have been developed

over the last decade in laboratory environment [2]. It consists of a moderately p-doped

base substrate and a thin heavily n-doped top layer. Thin metal contacts on the surface

and a plain metal layer on the back connect this photovoltaic element to the load as

shown in Fig. 3.1.

Fig. 3.1 The PV cell [16]

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3.1.2. Photovoltaic Effect

The photovoltaic effect is a basic physical process through which a PV cell

converts sunlight into electricity. Sunlight is composed of photon-packets of solar

energy, which contain different amounts of energy that correspond to different

wavelengths of the solar spectrum. When photons strike a PV cell, they may be

reflected or absorbed, or they may pass right through. Absorbed photons, with energy

greater than the band-gap energy of the semiconductor, generate electron-hole pairs.

The created charge carriers in the depletion region are separated by the existing electric

field. This leads to a forward bias of the p-n junction and builds up a voltage potential.

When a load is connected to the cell, this voltage will cause a current to flow through

the load.

3.1.3. Electric Model of the PV cell

A solar cell equivalent electrical circuit can be represented by a current source

in parallel with a diode as shown in Fig. 3.2. This is a simplified PV model where the

shunt resistance Rsh is neglected [17].

Fig. 3.2: Model for a PV cell [17]

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The model contains a photocurrent source Iph, one diode and a series resistance RS,

which represents the series resistance inside each cell.

Thus the Load current IL is the difference between the photocurrent Iph and the

normal diode current ID.

IL = Iph - ID = Iph – I0 (expmkT

RIVq SL )( +- 1) (3.1)

Iph = Iph(T1) (1 + K0 (T – T1)) (3.2)

Iph(T1) = G * Isc(T1,nom) / G(nom) (3.3)

K0 = (Isc(T2) - Isc(T1)) / (T2 -T1) (3.4)

I0 = I0(T1) * (T/T1)3/n * e-qVg / nk * (1/T – 1/T1) (3.5)

I0(T1) = Isc(T1) / (e-qVoc(T1) / nkT1 – 1) (3.6)

Where m is the ideality factor (ranges between 1 and 2), k is the Boltzmann’s

constant, T is the absolute temperature of the cell, q is the electronic charge and V is the

voltage across the cell. I0 is the dark saturation current and it depends on the

temperature, G is the Insolation level, K0 is the temperature coefficient at Isc, Vg is the

band gap voltage and T1 is a reference temperature supplied by the manufacturer [18].

The most important parameters for PV cells are the short circuit current 'ISC',

the open-circuit voltage 'VOC', and the maximum power point 'MPP'. The short circuit

current (Isc ≈ Iph) is the greatest current value generated by the cell under short circuit

conditions (V=0). The open circuit voltage (VOC), is the voltage across the p-n

junction/diode when IL=0 and when ID = Iph. It represents the voltage of the cell when it

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is in the dark. The maximum power point (MPP) is the point on the (I-V) characteristic

curve of a PV cell, where power is maximum, as shown earlier in Fig. 1.1.

3.1.4. Irradiation and Cell Temperature Effect on the I-V characteristic curve

Using equation (3.1), we can draw the (I-V) characteristic curves for different

irradiation levels and for different temperature values as shown in Fig. 3.3. It can be

easily interpreted that the open circuit voltage increases logarithmically while the short

circuit current increase linearly as the insolation level increases [18]. Also increasing

the cell’s temperature, decrease the open circuit voltage, thus the cell is less efficient in

terms of power level. The short circuit current increases slightly with cell temperature.

Fig. 3.3 (a) Effect of Varied Irradiation, (b) Effect of Varied Temperature on the PV cell

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3.1.5. PV Modules and PV Arrays

Single PV cells are combined into PV modules that are usually supplied with

NP parallel branches each with NS solar cells in series as shown in Fig. 3.4 (a). Yet in

photovoltaic energy systems PV modules are connected in arrays. Fig. 3.4 (b) shows an

array of the modules with MP parallel branches each with MS modules in series.

Fig. 3.4 (a) PV Module, (b) PV Array [18]

3.2. Battery

The purpose of a battery is to store chemical energy and to convert this

chemical energy into electrical energy when the need arises. Batteries are divided in two

ways, by application (what they are used for) and construction (how they are built). The

major applications are automotive, marine, and deep-cycle. The major construction

types are flooded (wet), gelled, and AGM (Absorbed Glass Mat). In solar systems it is

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important to note that nearly all of the batteries commonly used are deep cycle Lead-

Acid batteries [19].

3.2.1. Lead Acid Batteries

A lead-acid battery is an electrical storage device that uses a reversible

chemical reaction to store energy. It uses a combination of lead plates or grids and an

electrolyte consisting of a diluted sulfuric acid to convert electrical energy into potential

chemical energy and back again. A battery consists of a series of cells where each cell

provides about two volts. Connected in series, these cells will provide the desired

battery output voltage.

3.2.2. Battery Chemistry

A voltaic cell develops a potential difference when electrodes of two different

metals are immersed in an electrolyte. One electrode accumulates a positive charge

while the other accumulates negative charge. The potential difference is due to the

difference in charge between the two electrodes [20].

The chemical equation for a lead-acid battery during discharge is:

PbO2 + Pb + 2H2SO4 discharge → 2PbSO4 + 2H2O

The chemical equation for a lead-acid battery during charge is:

PbO2 + Pb + 2H2SO4 charge ← 2PbSO4 + 2H2O

The lead-acid battery uses dilute sulfuric acid for the electrolyte, lead for the

anode, and lead oxide, PbO2, for the cathode. The sulfuric acid dissociates into

hydrogen and sulfate ions. The sulfate ion reacts with the lead anode to form lead

sulfate and releases two electrons through the external circuit. This is the oxidation

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reaction. At the cathode, the two electrons cause a reaction to create lead sulfate and

water. This is the reduction reaction. The half-cell reactions are:

Pb + SO42-=PbSO4

2- (sol) + 2 e-

PbO2 + 4 H+ + 2 e- + SO42-=PbSO4

2- (sol)

At full discharge, both anode and cathode are covered with lead sulfate, and the

electrolyte is mostly water. Reversing the current flow reverses the reactions, recharging

the battery.

3.2.3. Ampere-Hour Capacity and Charge Rate

The Ampere-hour (Ah) Capacity of a battery tries to quantify the amount of

usable energy it can store at a nominal voltage. All deep cycle batteries are rated in

ampere-hours. An ampere-hour is one ampere for one hour, or 10 A for 1/10 of an hour

and so forth [21]. A good charge rate is approximately 10% of the total capacity (of the

battery) per hour (i.e. 200 amp hour battery charged at 20 amps.) This will reduce

electrolyte loss and damage to the plates. [20]

3.2.4. State of Charge

The State of Charge describes how full a battery is. This can be determined by

one of three ways:

• Voltage measurement, for a battery at 'rest' this method can show the state

of charge by comparing the voltage to a chart showing the percentage of charge relative

to voltage.

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• Electrolyte density measurement, a sample of the electrolyte is drawn into a

hydrometer, which shows the density of the liquid. The heavier the electrolyte (higher

gravity), the more acid in solution, the higher the state of charge.

• Ampere-hour metering, this method uses an ampere-hour meter, which is set

using the specifications of a new battery at full charge. It measures and records power

going into and coming out of the battery and keeps an electronic balance sheet.

3.2.5. Deep Cycle versus Starter Batteries

Batteries are typically built for specific purposes and they differ in construction

accordingly. Broadly speaking, there are two applications that manufacturers build their

batteries for: Starting and Deep Cycle discharge.

As the name implies, Starter Batteries are meant to get combustion engines

going. They have many thin lead plates, which allow them to discharge a lot of energy

very quickly for a short amount of time. However, they do not tolerate being discharged

deeply, as the thin lead plates needed for starter currents degrade quickly under deep

discharge and re-charging cycles. Most starter batteries will only tolerate being

completely discharged a few times before being irreversibly damaged.

Deep Cycle batteries have thicker lead plates that make them tolerate deep

discharges better (in many cases down to 20% of capacity). They cannot dispense

charge as quickly as a starter battery but can also be used to start combustion engines..

The thicker the lead plates, the longer the life span, all other things being equal. Battery

weight is a simple indicator for the thickness of the lead plates used in a battery. The

heavier a battery for a given group size, the thicker the plates, and the better the battery

will tolerate deep discharges. [20]

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3.2.6. Lifespan of Batteries

The lifespan of a battery will vary considerably with how it is used, how it is

maintained and charged, temperature, and other factors. Battery manufacturers define

the end-of-life of a battery when it can no longer hold a proper charge (for example, a

cell has shorted) or when the available battery capacity is 80% or less than what the

battery was rated for. The life of Lead Acid batteries is usually limited by several

factors:

Cycle Life is a measure of how many charge and discharge cycles a battery can

take before its lead-plate grids/plates are expected to collapse and short out. Moreover

the greater the average depth-of-discharge, the shorter the cycle life [20].

Age also affects batteries as the chemistry inside them attacks the lead plates.

The healthier the "living conditions" of the batteries, the longer they will serve you.

Lead-Acid batteries like to be kept at a full charge in a cool place.

Sulfation is a constant threat to batteries that are not fully re-charged. A layer

of lead sulfate can form in these cells and inhibit the electro-chemical reaction that

allows you to charge/discharge batteries.

3.2.7. Battery Hazards

Both electrodes dissolve into the electrolyte during the discharge reaction.

When charged the reverse reactions occur. Overcharge will lead to the electrolysis of

water and consequent production of (hazardous) H2 (gas) at the cathode. Precautions

must be routinely practiced to prevent explosions from ignition of the flammable gas

mixture of hydrogen and oxygen formed during overcharge of lead-acid cells.

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3.3. DC-DC Converters

A DC-to-DC converter is a device that accepts a DC input voltage and

produces a DC output voltage, which is at a different voltage level than the input. DC-

DC converters are widely used in regulated switch-mode dc power supplies and in dc-

motor drive applications. These converters are usually used with an electrical isolation

transformer in the switch mode dc power supply, and without an isolation transformer

in case of dc-motor drive [22].

3.3.1. Switching Converter Topologies

Topology refers to the various configurations of power-switching and energy-

storage elements that can be used to transfer, control and regulate power (voltage) from

an input voltage source. The many different switching-regulator topologies can be

grouped into two basic categories: non-isolated, in which the input source and the

output load share a common current path during operation, and isolated, in which the

energy transfer is achieved by a mutually-coupled magnetic element (a transformer),

and the coupling from the source to the load is achieved by means of a magnetic flux

rather than a common current. One topology is selected over another based upon the

cost goals, performance objectives and input-line/output-load characteristics of the

system in which it is to operate. Any one topology is not “better” than another in all

respects. Each has desirable characteristics and shortcomings, and selection is a matter

of properly applying the correct power converter to the system requirement.

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3.3.2. Non-Isolated Switching Converters

There are four, non-isolated, switching-regulator topologies applicable to

modular DC/DC converters. They are the buck, or step-down converter, the boost, or

step-up converter, the buck-boost converter, and the Cuk converter.

3.3.2.1. Buck Converter (step-down converter)

As the name implies, a step-down converter produces a lower average output

voltage than the dc input voltage. Its operation is straightforward. When the switch Tr,

in Fig. 3.5, is turned on, the input voltage is applied to inductor L and power is

delivered to the output. This voltage will tend to cause the inductor current to rise.

When the switch Tr is OFF, the current will continue flowing through the inductor L but

now flowing through the diode.

Fig. 3.5 Buck Converter

To analyze the voltages of this circuit let us consider the changes in the

inductor current over one cycle as shown in Fig. 3.6.

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25

Fig. 3.6 Voltage and current changes [22]

The voltage across the inductor shown in Fig. 3.5 is given by

dtdiLVV ox =− (3.8)

the change of current satisfies

( )⎟⎟⎟

⎜⎜⎜

∫ −= dtI

IVoVx

Ldi

2

1

1 (3.9)

For steady state operation the current at the start and end of a period T will not

change. To get a simple relation between voltages we assume no voltage drop across

transistor Tr or diode while ON and a perfect switch change. Thus during the ON time

Vx=Vin and in the OFF period Vx=0. Thus

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26

dtoVdtoVinVdiofftont

ont

ont∫ −+−∫==

+

)()(00

(3.10)

which simplifies into

Tont

inVoV

= where T = ton + toff (3.11)

Defining "duty cycle" as

Tont

D = (3.12)

the input-output voltage relationship becomes

Vo=D Vin (3.13)

Since the circuit is lossless and the input and output powers must match on the

average (Vo* Io = Vin* Iin). Thus the average input and output current must satisfy

Iin =D Io (3.14)

These relations are based on the assumption that the inductor current does not

reach zero.

• Discontinuous-Conduction Mode

Thus, the buck is a step-down type, where the output voltage is always lower

than the input (Since D never reaches one). Varying the duty cycle of the switch

provides output voltage regulation. The LC arrangement provides very effective

filtering of the inductor current. Hence, the buck and its derivatives all have very low

output ripple characteristics. The buck is normally always operated in continuous mode

(inductor current never falls to zero) where peak currents are lower as shown in Fig. 3.7,

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27

and the smoothing capacitor requirements are smaller. There are no major control

problems with the continuous mode buck.

Fig. 3.7 Inductor current for (a): continuous mode (b): discontinuous mode [22]

• Boundary Between Continuous and Discontinuous Conduction

When the current in the inductor L remains always positive then either the

transistor Tr or the diode D must be conducting. For continuous conduction the voltage

Vx is either Vin or 0. If the inductor current ever goes to zero then the output voltage will

not be forced to either of these conditions. At this transition point the current just

reaches zero as seen in Fig. 3.8.

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Fig. 3.8 Buck Converter at Boundary

During the ON time Vin-Vo is across the inductor thus

Lt

VVI onOinL peak ).()( −= (3.15)

The average current, which must match the output current, satisfies

)(2

)(2

)()( transition

peakaverage outoin

LL I

LdTVVII =−== (3.16)

If the input voltage is constant the output current at the transition point satisfies

TL

ddVI inout transition2

)1()( −= (3.17)

• Voltage Ratio of Buck Converter (Discontinuous Mode)

As for the continuous conduction analysis, the fact that the integral of voltage

across the inductor is zero over a cycle of switching T is used. The transistor OFF time

is now divided into segments of diode conduction δdT and zero conduction δoT as shown

in Fig. 3.9. [22]

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29

Fig. 3.9 Buck Converter - Discontinuous Conduction

The inductor average voltage thus gives:

0)()( =−+− TVDTVV dooin δ (3.18)

Then

din

o

dd

VV

δ+= where 1<+ dd δ (3.19)

To resolve the value of dδ consider the output current which is half the peak

when averaged over the conduction times dd δ+ .

dL

out dI

Ipeak

δ+=2

)( (3.20)

Considering the change of current during the diode conduction time

LTV

I doL peak

)()(

δ= (3.21)

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Thus from equations (3.20) and (3.21) we can get

LdTV

I ddoout 2

)( δδ += (3.22)

using the relationship in (3.19)

LTdV

I dinout 2

δ= (3.23)

and solving for the diode conduction

dTVLI

in

outd

2=δ (3.24)

The output voltage is thus given as

)2

(2

2

TVLI

d

dVV

in

outin

out

+= (3.25)

defining k = 2L/(Vin T), we can see the effect of discontinuous current on the voltage

ratio of the converter.

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Fig. 3.10 Output Voltage versus Current [22]

As seen in Fig. 3.10 once the output current is high enough, the voltage ratio

depends only on the duty ratio "d". At low currents the discontinuous operation tends to

increase the output voltage of the converter towards Vin.

• Output Voltage Ripple

For continuous mode of operation the output ripple voltage can be calculated

by considering the waveform in Fig. 3.11. Assuming that the entire ripple component in

iL flows through the capacitor and its average component flows through the load

resistor, the shaded area in Fig. 3.11 represents an additional charge ∆Q. Therefore, the

peak-to-peak voltage ripple ∆Vo can be written as:

∆Vo = 222

11 TICC

Q L ⋅∆

=⋅=∆ (3.26)

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32

Fig. 3.11 Output voltage ripple in a step-down converter [22]

From Fig. (7) during toff

TDL

VI L )1(0 −=∆ (3.27)

Then substituting ∆IL from Eq. 20 into previous equation, we get:

TDL

VCTV )1(

80

0 −=∆ (3.28)

222

0

0 )1(2

)1(81

⎟⎟⎠

⎞⎜⎜⎝

⎛−=

−=

∆∴

ff

DLC

DTVV cπ (3.29)

where, f = 1/T is the switching frequency and LC

fc π21

= .

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3.3.2.2. Boost Converter (step-up converter)

The schematic in Fig. 3.12 shows the basic boost converter. This circuit is used

when the output voltage is required to be higher than the input..

Fig. 3.12 Boost Converter Circuit

While the switch Tr is ON then Vx =Vin, and in the OFF state the inductor

current flows through the diode giving Vx =Vo. For this analysis it is assumed that the

inductor current always remains flowing (continuous conduction). The voltage across

the inductor is shown in Fig. 3.13 and the average must be zero for the average current

to remain in steady state.

Fig. 3.13 Voltage and current waveforms (Boost Converter).

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34

Thus

0)( =−+ offtoVinVontinV (3.30)

This can be rearranged as

)1(1

DofftT

inVoV

−== (3.31)

and for a lossless circuit the power balance ensures

)1( DinIoI

−= (3.32)

Since the duty ratio "D" is between 0 and 1 the output voltage must always be

higher than the input voltage in magnitude. The negative sign indicates a reversal of

sense of the output voltage.

3.3.2.3. Buck-Boost Converter

A buck-boost converter can be obtained by cascading the step-down converter

and the step-up converter. The cascade connection can be combined into the topology of

the buck-boost converter using a single switch as shown in Fig. 3.14.

Fig. 3.14 schematic for buck-boost converter

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35

With continuous conduction for the Buck-Boost converter Vx =Vin when the

transistor is ON and Vx =Vo when the switch (Tr) is OFF. For zero net current change

over a period the average voltage across the inductor is zero as shown in Fig. 3.15.

Thus:

0=+ offtoVontinV (3.33)

Fig. 3.15 Waveforms for buck-boost converter

Which gives the voltage ratio

DD

VV

in

o

−−=

1 (3.34)

and the corresponding current

DD

II

in

o −−=

1 (3.35)

Since the duty ratio "D" is between 0 and 1 the output voltage can vary

between lower or higher than the input voltage in magnitude. The negative sign

indicates a reversal of sense of the output voltage.

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36

3.3.3. Isolated DC-DC Converters

In many DC-DC applications, multiple outputs are required and output

isolation may need to be implemented depending on the application. In addition, input

to output isolation may be required to meet safety standards and / or provide impedance

matching. There are several isolated switching converter topologies; however, three will

be discussed, which are the flyback, forward and H-bridge power converters. For these

circuits, all energy transfer from the input power source to the load is achieved via a

transformer or other flux-coupled magnetic element.

3.3.3.1. Flyback Converter

The flyback switching regulator converts an input voltage into a regulated,

lower or higher-valued output voltage depending on its transformer’s turns ratio. The

flyback converter can be developed as an extension of the Buck-Boost converter Fig.

3.14. A simplified circuit diagram is shown in Fig. 3.16.

Fig. 3.16 Flyback converter

Concerning the input-to-output transfer function, the on-time energy is given by:

Eon = (Vin / N) ton (3.36)

and the off-time energy is given by:

Eoff = (Vo) toff (3.37)

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37

Where toff = T – ton and N is the transformer’s turns ratio.

Substituting yields:

(Vin /N) ton = Vo (T – ton) (3.38)

(VIN) ton = N Vo (T – ton) (3.39)

but

Vo = (Vin) ton /(N T – N ton) (3.40)

where

ton /T = D (3.41)

Vo /Vin = D / (N – N D) (3.42)

Vo / Vin = (1 / N) (D / (1 – D)) (3.43)

3.3.3.2. Forward Converter

The forward switching regulator converts an input voltage into a regulated,

lower or higher-valued output voltage depending on its transformer’s turns ratio. A

simplified circuit diagram is shown in Fig. 3.17.

Fig. 3.17 Forward Converter

In determining the input-to-output transfer function, the on-time energy is given by:

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38

Eon = (Vin / N – Vo) ton, (3.44)

and the off-time energy is given by:

Eoff = (Vo) toff, (3.45)

where

toff = T – ton and N is the transformer’s turns ratio.

Substituting yields:

(Vin / N – Vo) ton = Vo (T – ton) (3.46)

Vo = (Vin / N)(ton / T) (3.47)

Vo / Vin = (1 / N) D (3.48)

3.3.3.3. H-bridge Converter

The H-bridge inverter changes a dc input voltage into a symmetrical ac output

voltage of desirable magnitude and frequency. The output voltage could be fixed or

variable at a fixed or variable frequency. A variable output voltage can be obtained by

varying the gain of the inverter, which is normally done by pulse-width-modulation

(PWM) control within the inverter. Then the rectifier, and filter circuit is used to extract

the average value (dc) of the voltage and current. A simplified circuit diagram is shown

in Fig. 3.18. When switches S1 and S4 are turned on simultaneously, the input voltage Vs

appears across the terminals (A & B) of the transformer T. If switches S2 and S3 are

turned on at the same time, the voltage VAB is reversed and is - Vs. The waveform for the

output voltage is shown in Fig. 3.19.

The rms output voltage can be found from:

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39

Vo = s

T

s VdtVT

=⎟⎟

⎜⎜

⎛∫

2/1

0

2

0

02 (3.49)

Fig. 3.18 H-bridge Converter

Fig. 3.19 Waveforms

This type of converters was shown for the hardware design because it employs

electronic switches that are driven by square wave signals (50% duty cycle). This

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40

permits good operation at high frequencies, avoiding problems that may arise when

using simple buck converter topology with variable duty cycle switching. This is

illustrated in Chapter 5, section 5.3.1.

3.4. Zero Voltage Switching

Switching frequencies in the megahertz range are being contemplated to reduce

the size and the weight of transformers and filter components and hence to reduce the

cost as well as the size and the weight of power electronics converters. Realistically, the

switching frequencies can be increased to such high values if the problems of switch

stresses, switching losses, and EMI associated with the switch-mode converters can be

overcome.

Therefore, to realize high switching frequencies in converters, the

aforementioned shortcomings are minimized if each switch in a converter changes its

status (from on to off and vice versa) when the voltage across it ‘Vs’ and/or the current

through it ‘is’ is zero at the switching instant. Otherwise power loss PS in the switch,

being proportional to the switching frequency limits how high the switching frequency

can be pushed, without significantly degrading the system efficiency. The power loss PS

in the switch during turn-off and turn-on is shown in Fig. 3.19.

Fig. 3.20 Power loss associated with high switching frequencies.

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41

In these converters, the resonant capacitor Cr produces a zero voltage across

the switch at which instant the switch can be turned on or off. Such a step-down

converter circuit is shown in Fig. 3.20, where a diode Dr is connected in antiparallel

with the switch [22].

Fig. 3.21 ZVS resonant-switch dc-dc converter [22]

After implementing this type of ZVS buck converters in the hardware model,

the power electronics efficiency decreased severely. After all, the implemented system

switching frequency (40khz) is much less than megahertz and the resonant inductor Lr

added more power loss in the form of heat dissipation. So the resonant elements were

removed and an H-bridge converter was built. The H-bridge converter is discussed in

chapter 5.

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CHAPTER 4

MPPT SYSTEM SIMULINK MODEL

4.1. Introduction

In this chapter, the mathematical models of the MPPT system implemented in

Simulink will be highlighted.

Simulink is a platform for multi-domain simulation and model-based design of

dynamic systems. It provides an interactive graphical environment and a customizable

set of block libraries that let you accurately design, simulate, implement, and test

control, signal processing, communications, power electronics and other time-varying

systems.

Simulink has an advantage when building hierarchical model system because

of the possibility to test the system at different levels. It also provides the possibility to

build modular models, which means that models can be easily connected to simulate

certain system.

4.2. Simulink Blocks

Simulink possesses a variety of block libraries to represent time varying

systems. However present Simulink libraries don’t include one for PV systems; there is

no solar cell equivalent block. However at one university, a PV toolbox with a PV

module, battery, and battery charge controller had been designed and is being tested

[20]. Fig. 4.1 shows the PV array MPPT system block that includes: PV cell block,

converter block, controller block and the battery load block.

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In the next few sections, these blocks will be discussed individually. The

sections will investigate how the models are implemented.

Fig. 4.1 PV array 'MPPT' system

4.3. What is An S-Function

An S-Function is a mechanism that allows the user to implement Matlab source

code as a Simulink compatible block. The S-function block is always drawn with one

input port and one output port, regardless of the number of inputs and outputs of the

contained subsystem. To have access to more than one input and output through an s-

function block, a multiplexer and a de-multiplexer are respectively used as shown in

Fig. 4.2.

Fig. 4.2 S-Function block with three inputs and two outputs

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4.4. Implementation of PV cell using S-Function

One can use the circuit model shown in Fig. 4.3 to represent the solar cell using

the 'SimPower System’ library, or can develop a solar cell block using S-function

Block.

Testing the circuit model during initialization, it was difficult to set Iph and ID

values with respect to varying Insolation and temperature values respectively. Moreover

during simulation, it was also difficult to control these two values while varying the

converter duty cycle using the circuit model.

Fig. 4.3 Model for a PV cell

So using the S-Function approach, a model for the PV cell was developed as

shown in Fig. 4.4. The inputs are the Insolation level (W/m2), the Temperature (oC), and

the current Iin (A) absorbed by the load. The code, implemented in the PV cell block,

defines the set of equation that describes the voltage and current relations as given in

Chapter 3. This code is given in Appendix A.

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Fig. 4.4 PV Cell S-Function block

4.5. Converter and Controller Blocks

It was decided to use a buck converter as the integrated MPPT's converter. The

buck converter features "low ripple and switching device currents compared to other

converter topologies" [24]. The buck converter model is built using the 'SimPower

System' Simulink library as shown in Fig. 4.5. The power MOSFET is chosen as a

switching device since it has higher switching speed capabilities as compared to BJTs.

It has four pins, where the g pin represents the gate terminal, d the drain, and s the

source. The m pin is used for measurements so it is connected to a terminator box. The

diode model is selected from the Simulink power electronics library. A snubber

resistance (500 ohm), connected in parallel with the diode, is used to reduce the

switching current overshoots. The inductor that maintains current continuity is placed in

parallel with a 10-kΩ resistance to agree with the Simulink environment. The values of

the inductor 200µH and capacitor 220µF are calculated using equations 3.26 and 3.27.

The procedure, used to calculate these values, is present in Chapter 5

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Fig. 4.5 Buck converter and Controller blocks

To complete the system, a model for the controller, to drive the switching

mechanism of the power MOSFET, was also developed as shown in Fig. 4.6. The PAO

control algorithm varies the duty cycle of the input current, supplied by the PV cell, to

allow the maximum power point (MPP) to be reached. Fig. 4.6 illustrates how the

controller system was built.

Fig. 4.6 Controller Block Implementation

The saw-tooth signal is compared to a controlled constant level with threshold

value k. This level value k will vary according to the algorithm implemented in the S-

function block named threshold level.

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The PAO algorithm depends on the present value of the current I, and voltage

V, and on the previous value of the threshold value k, and the power Pr supplied by the

PV cell. The voltage V and current I are directly supplied to the 'threshold level' block

while the constant k and the power Pr values are passed first through a delay box,

present in the Simulink library and labeled withz

1, to supply their previous values to

the 'threshold level' block as shown in Fig. 4.6. If this delay box is not inserted, the

present value of the power (I.V) will be compared with itself instead of being compared

to the previous power Pr value.

The flow chart, describing the PAO tracking algorithm implemented in the S-

function block named threshold level, is shown in Fig. 4.7. If the present value of the

power P(n) is greater than the previous value P(n-1), then the threshold value k is

incremented by an incremental step delta; this means that the duty cycle of the

rectangular signal is increased. Otherwise the threshold value k is decremented by delta;

this means that the duty cycle d of the rectangular signal is decreased.

Fig. 4.7 MPP tracking algorithm Flow Chart

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Moreover as the duty cycle d increases, then the average current Iavg increases and vice

versa. This is illustrated in Fig. 4.8 where the level value k2 is larger than k1, thus the

duty cycle d2 is larger than d3. Therefore the average current Iavg2 is greater than Iavg1.

The algorithm will keep changing the duty cycle until the MPP is reached. The matlab

code for this algorithm is given in Appendix A.

Fig. 4.8 Different current levels with respect to variable duty cycle

To illustrate more on the PAO algorithm, consider the tracking scheme

presented in Fig. 4.9. The algorithm starts hunting for the maximum power point by

changing the duty cycle d in a series of relatively large steps ∆. After each new step, it

measures the voltage Vs and current Is, multiplies their values, and compares the newly

obtained power level Pn with the former value Pn-1. Two cases may arise as a result of

this comparison:

• If the newly obtained power Pn is larger, the algorithm continues changing

the duty cycle d monotonically in the same direction, using the same step size delta (∆).

• If the newly obtained power Pn is lower, the algorithm reverses the direction

of changing the duty cycle d, and divides the step size delta by two )(2∆ .

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Eventually, the algorithm will reach a stage in its search for the maximum power point,

where it jumps around the maximum power point in very fine steps. The algorithm

should keep scanning, since the MPP is expected to vary due to changes of illumination

and temperature depending on daytime, weather conditions, and shadow effects.

Fig. 4.9. MPPT tracking scheme using a variable step size

4.6. Battery Block

The load, in our case a battery, is approximated by a dc voltage source Vb in

series with a small resistance r. The dc voltage source Vb is set to 12V and the resistance

r is set to 0.01Ω as shown in Fig. 4.10. The battery output voltage Vout will increase as

more current passes through the resistance r.

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Fig. 4.10 Battery Model Block

Thus the over all, maximum power point tracking (MPPT), system is shown in

Fig. 4.11. The Insolation value (1000 W/m2) and the temperature (22 oC) are introduced

as de-multiplexed inputs to the PV cell block using s-function constant value blocks.

Fig. 4.11 PV array 'MPPT' system

The current Iin is also fed as an input to the PV cell; the load nature will force a

current to flow through, after applying a voltage across the load. The current Iin is

passed first through a delay block to guarantee that the controller algorithm will

compare the present value of the power with that of the previous (delayed) power; else

the system simulation will not converge.

With these three inputs (In, T, Is), the PV cell block will supply the output

voltage Vs. The controller will force the buck converter to draw more current Iin from

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the PV cell until the MPP is reached. This way the buck converter will charge the

battery with maximum, PV cell, available power.

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CHAPTER 5

MPPT SYSTEM IMPLEMENTATION

5.1. Introduction

In this chapter, the hardware and software design of the MPPT system is

presented and discussed.

The system consists of a PV module, an H-bridge converter, a 12-volts lead

acid battery, and a control circuit that uses the PIC16F874 microcontroller. The

controller obtains the information (current and voltage) from the PV array through the

microcontroller’s analog and digital (A/D) ports. The microcontroller performs the

pulse width modulation (PWM) to the dc-dc converter through its PWM built-in special

register. It then finds the duty cycle at which the converter loads the PV module at the

maximum power point (MPP) when charging the battery. The battery’s state of charge

is also controlled by the microcontroller to protect the battery from being overcharged.

5.2. MPPT System

The complete solar MPPT system is shown in Fig. 5.1. However the most

critical section of the MPPT system is that of the controller and converter. The

controller should keep track and force the system to operate at the maximum power

point of the PV array as the weather conditions change. The dc-dc converter will charge

the battery with maximum power available so any resistance or loss in the converter

will contribute to power loss of the system.

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5.2.1. Microcontroller

PIC16F874 microcontroller is used in the control section. This microcontroller

is responsible for different tasks. The MPP tracking algorithm is implemented in the

microcontroller. So it computes where the MPP of the PV array is and accordingly

control the PWM scheme of the converter. It controls the A/D converter ports to

represent the analog voltage Vs and current Is of the PV array in digital format. It also

monitors the state of charge of the battery to prevent overcharge damage. The

PIC16F874 is a perfect combination of features, performance, and low power

consumption for this application. It has 4K x 14 bits of flash memory, 192 x 8 bytes of

data memory (RAM), two D/A and five A/D channels.

Fig. 5.1 The PV maximum power point tracking system

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5.2.2. PV Array to PIC Interface Circuit

The PV-PIC interface circuit shown in Fig. 5.1 provides the microcontroller

with appropriate voltages that it can endure. The PV output voltage Vs is fed to the

microcontroller using a voltage divider circuit. The current Is is fed to the

microcontroller after passing through a 0.01 ohm resistance rs to get a voltage

representation of the current. These analog voltages are fed to the microcontroller via

two built in A/D channels to represent digitally the voltage Vs and current Is of the PV

array.

5.2.3. H-bridge Converter

The converter transfers energy from the PV array to the battery by regulating its output

voltage to essentially match that of the battery. Since energy will flow in the converter,

resistance heat loss, and switching losses should be minimized. To reduce these loses an

H-bridge converter is used. The H-bridge reduces to and operates as a buck converter

during each half switching cycle [22]. The H-bridge is discussed in the Hardware

Design section.

5.2.4. PIC-Converter Interface Circuit

The PIC-Converter interface circuit is used to control the PWM scheme

needed to drive the dc-dc converter. This board will include a phase splitter and a driver

circuit that will provide the right signals to control the switching scheme of the bridge.

These signals should have the appropriate voltages to turn on or off the bridge switches.

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5.3. Hardware Design

The schematics design and operation of the MPPT hardware system are

discussed in the following sections. The PCB layouts are given in Appendix B.

5.3.1. Controller and Converter Design

The H-bridge converter that was discussed in Chapter 3 (pp. XX) was

implemented as shown in Fig. 5.2. It employs electronic switches that are driven by

square wave signals (50% duty cycle). This permits good operation at high frequencies,

avoiding problems that may arise when using simple buck converter topology with

variable duty cycle switching; after all the switch may fail to turn off when the off time

Toff is small incase of a variable duty cycle switching as shown in Fig. 5.3 (b). Due to

the ideality of the components, a simple buck converter was used in the Simulink model

because the case where the switch fails to turn off does not exist.

Fig. 5.2 Converter and Controller

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Fig. 5.3 (a) 50% duty cycle switching (b) variable duty cycle switching

The square wave signals that drive the bridge switches are phase-shifted by an

amount equal to the turn-on time of the PWM microcontroller’s output. The control of

the output voltage (V1 – V2) of this converter depends on controlling the phase

difference between the voltages V1 and V2. This difference (V1 – V2) is the output of the

switch bridge.

Fig. 5.4 shows the impact of phase difference between V1 and V2, on the

output of the bridge for a small and large phase difference. Fig. 5.5 and Fig. 5.6 show

the bridge output when the phase difference is zero and 180o respectively. However in

the software design, the duty cycle has an upper and lower limit as discussed later in the

Software Design section.

Fig. 5.4 Bridge output due to small and large phase difference

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Fig. 5.5 Case of zero phase difference between V1 and V2

Fig. 5.6 Case of V1 and V2 being out of phase

A phase splitter circuit is designed to generate the phase difference between V1

and V2. This circuit is controlled by the width of the pulses generated by the PWM

output of the microcontroller. V1 changes (inverts) its value with each rising edge of the

PWM output (from 0 volts, to VDD). V2 changes its value to follow that of V1 with each

falling edge of the PWM output (from VDD to 0 volts). This causes the output of the

bridge to become nonzero with the rising edge of the micro-controller’s PWM output,

and zero with the falling edge. Fig. 5.7 below shows the relationship between the PWM

waveform, and the waveforms of V1 and V2.

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Fig. 5.7 PWM output controls the Bridge output

The output of the bridge is then rectified and filtered to give as a final result, a

DC voltage that is directly proportional to the phase difference between V1 and V2

(subsequently proportional to the pulse width of the micro-controller’s PWM output).

Fig. 5.8 shows the relationships between these signals.

Fig. 5.8 PWM, Bridge, Rectified and Filtered voltage waveforms

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5.3.2. Phase Splitter Circuit

The phase splitter circuit provides two outputs. The first output (Square wave

output A) changes with each rising edge of the micro-controller’s PWM output. The

second output (Square wave output B) changes with the falling edge of the PWM output

as shown in Fig. 5.9.

Fig. 5.9 Phase splitter output waveforms

To construct this circuit, two type–D edge–triggered flip–flops are used (7474).

One (FF1) is used to toggle with each rising edge of the PWM output, as shown below

in Fig. 5.10. The second (FF2) is forced to follow the change of the first with each

falling edge (rising edge of the inverted PWM wave). Changing the pulse width of the

PWM output changes the phase difference between the output A and the output B.

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Fig. 5.10 Phase splitter schematic diagram

5.3.3. Switch Drivers ‘A’ and ‘B’

The bridge consists of four switches T1, T2, T3, and T4. These switches are, in

fact, MOSFETs having high current handling capability (IRFZ46). To provide these

MOSFETs with the right signals to turn on or off, a driver circuit is designed.

T1 and T2 form a switch pair that controls the voltage V1 and are driven by the

driver circuit ‘A’. T3 and T4 switch pair similarly controls the voltage V2, and are driven

by the driver circuit ‘B’. The operation of the driver circuit A is next explained. The

operation of the driver circuit B will be similar to that of driver circuit A.

Fig. 5.11 Driver A output waveforms

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Switches T1 and T2 are operated by anti–phase driving signals (when T1 is

closed, T2 is open and vice versa) as shown in Fig. 5.11. Furthermore, the anti – phase

signals should provide a dead – time interval during the transitions to permit the

complete turn OFF of the switch (that was ON), before turning ON the other switch;

this is necessary to avoid the flow of excessive currents in the transition interval, due to

both switches being ON at the same time as shown in Fig. 5.12.

Fig. 5.12 Driver ‘A’ schematic diagram

The driver circuit shown in Fig. 5.12 provides driving pulses to the gates of

transistors T1 and T2, with an amplitude of 12 volts to ensure the complete turn ON of

the switch that should be in the active mode (to have a low ON state resistance), and a

fast turn OFF of the switch that should be deactivated.

The comparators are used to convert the 5 volts logic levels (microcontroller

output) to the 12 volts logic levels used to drive the gates of the MOSFETs. The

MOSFETs are driven with two anti-phase signals. The 1 kΩ and the 1 nF capacitors are

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used to delay the turn ON of each transistor, for an interval sufficient to make sure that

the other transistor reaches the OFF state, when turned OFF. The clearance interval

(dead time) is labeled by Td in Fig. 5.12. Quick turn OFF is achieved by rapidly

discharging the gate capacitance, and the 1nf capacitor, using a diode (D1 and D2) that

provides low resistance path for discharging current. Fig. 5.13 shows the details of

operation for the gate circuit.

The MOSFET will not turn ON, till the voltage between the gate and source

reaches the threshold value (about 3 volts).

Fig. 5.13 Charging and discharging stages

5.3.4. H-bridge

The standard H-bridge transformer coupled converter is shown in Fig. 5.14.

Switches T1 and T2 are driven by anti – phase signals generated by the driver circuit A.

Similarly switches T3 and T4 are driven by anti – phase signals generated by the driver

circuit B. These switches are n-channel enhanced mode power MOSFETs IRFZ46 that

are characterized with its high speed-switching capabilities [23]. The device is rated at

50V and 50A, which means that the rating is well above maximum operating voltage

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and current which are 20 V and 6 A of the converter. It has a maximum leakage current

of only 100 nA and very low on state resistance of 0.024Ω and hence small conduction

loss that makes it a highly efficient switching device.

Fig. 5.14 Bridge Converter schematic diagram

Although not shown in figure, each transistor is equipped with a built – in fast

– recovery power diode that provides a path for free – wheeling currents that flow

during certain phases of operation.

5.3.5. Transformer, Rectifier, and Filter Circuit

Fig. 5.15 shows the schematics for the transformer, rectifier and filter with the

voltage waveforms present at each stage. The transformer used here has a voltage

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transformation ratio of 1:1.5. Fast recovery diodes are used to rectify the bridge output

by providing a unidirectional voltage. This voltage is then filtered to produce DC output

that is equal to the average value of the pulse train.

Fig. 5.15 Transformer, Rectifier and Filter waveforms

The elements of the rectifier and filter are chosen on the following basis.

• Inductor

Inductor design is almost the hardest among the other elements since there is

no variety of inductor values in the market. The inductor has a certain number of turns

winded around a coil to establish the inductance needed for the converter. However any

additional turn (additional wire length) will add to the coil resistance value. This

additional value will contribute to resistance loss.

The value of inductance is calculated by considering the extreme case; when

the PV array operates at its maximum capacity (70 Watts). Therefore the output current

can be calculated by using the equation Pout = Vo × Io

Hence, Io = Po / Vo = 70 / 12 = 5.8 Amps

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As discussed in section 3.3.2.1, the amplitude of the inductor current ripple is

selected to be 10% of its dc value. (i.e. LI∆ = Io × 0.1 = 5.8 × 0.1 = 0.58A).

If the converter is assumed to operate at frequency 40 kHz (i.e. Ts = 25 µs),

and the inductor current is assumed to be equal to the output current having 10% current

ripple.

Equation (3.27) gives: sL

TDI

VL )1(0 −

∆=

where D is the duty cycle and is calculated using equation (3.13)

D = Vo/Vd = 12/18 = 0.65

Thus the inductance value is

L = (12 × 0.35 × 25 × 10-6) / (0.58) = 181µH

This is the least inductance value that can endure a current of 5.8 A, so an

inductor of 200µH is chosen for the converter.

• Capacitor

To obtain a desired output voltage ripple, the capacitor value is determined.

Once again, the extreme case is considered. The output current is 4.1A, D = 0.65, Ts =

25µs. Assume that the output voltage ripple is 0.1% of its dc value (i.e. ∆Vo = 0.012V).

Equation (3.26) gives:

C = 222

11 TIVo

L ⋅∆⋅⋅

∆=

Then C = (0.58 × 25 × 10-6) / (8 × 0.012) = 150µF

The minimum capacitance value needed for the converter is 150µF. Hence, a

220µF is chosen for the design smooth more the ripple voltage.

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• Diode

Diode choice is a trade off between forward bias voltage, and speed. Higher

forward bias voltage will result in more power dissipation and loss. Moreover, a fast

diode that can switch at high frequencies is needed. If the diode is slow to react, the

efficiency of the converter will drop. The best diode combining these features, that

could be found, was the STPS3045CPI from SGS-THOMSON. It has 0.57v of forward

drop at the expected currents of 15A.

5.4. Software Design

The next step in the design is to implement the MPP tracking algorithm on the

microcontroller chip. The PIC16F874 microcontroller is used to carry out the algorithm

function. It operates at speed of 10MHz so each instruction code will be executed at

0.4µs. The program is written in assembly language and is given in Appendix C.

A new strategy in programming the PIC 16F874 chip to track the MPP is adopted. This

new strategy is based on the Perturb and Observe (PAO) technique using an adaptive

incremental step scheme. The maximum power point is quickly hunted using a variable

step size. This adaptive technique reduces the number of iterations needed to catch this

MPP, thus resulting in much faster tracking compared to conventional methods [24].

5.4.1. Main Program

The main program flow chart is shown in Fig. 5.16. The program starts by

initializing the A/D module and the PWM module. Then the battery state of charge is

checked to prevent overcharge damage. The PWM module is turned off at this stage

and the program runs A/D conversion to measure the battery voltage. The measured

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voltage is then compared to a predefined value (13.8V) to determine the state of charge

of the battery. If the battery voltage is greater than 13.8V (almost fully charged) the

program goes to sleep for 1 second and then goes back to measure the battery voltage

again. If the battery voltage is less than 13.8V the program goes to the Charging-

Tracking mode.

Fig. 5.16 Main Program Flow Chart

5.4.2. Charging-Tracking mode

The microcontroller has a PWM output, having a duty cycle that is controllable

by the microcontroller’s software. The micro-controller provides a duty – cycle ratio

limited to the range [1/255 254/255]. The microcontroller starts hunting for the

maximum power point by changing the duty cycle in a series of relatively large steps.

After each new step, it measures the solar voltage Vs and current Is using the PIC built in

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A/D channels, multiplies their digital representation, and compares the newly obtained

power level with the former value.

The flow chart for the conventional PAO algorithm is shown in Fig. 5.17. If the

newly obtained power Pn is larger than the previous power value Pn-1, the

microcontroller continues changing the duty cycle d monotonically in the same

direction, using the same step size delta (∆). Otherwise the microcontroller reverses the

direction of changing the duty cycle, and divides the step size delta by two (2∆ ). The

microcontroller will finally lock on the MPP with fine step size as shown before in Fig.

4.9.

Fig. 5.17 The conventional PAO algorithm Flow Chart

This algorithm showed good performance for stable weather conditions where

the tracking efficiency ξTr reached 95%. However, this algorithm fails to track the MPP

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correctly in case of rapidly varying weather conditions where ξTr deteriorated to less

than 85%. This is due to the small incremental step that was reached while tracking the

old MPP. This small incremental step would continue to be used when searching for the

new MPP as shown in Fig. 5.18, which will increase the number of iterations needed to

lock on the new MPP. When frequent weather changes occur, the system will not be

able to track and lock onto the new MPP.

Fig. 5.18 Scanning with small step in case of varying weather conditions

To improve the performance of the conventional PAO algorithm, an adaptive

PAO algorithm is implemented. The flow chart for the adaptive PAO algorithm is

shown in Fig. 5.19. The micro-controller provides a duty–cycle ratio limited to the

range [1/255 254/255]. The microcontroller starts with a duty–cycle ratio of 1/255. It

increments the duty cycle in steps of 32/255 as long as it detects that the power

extracted from the PV module increases with each step (∆). When power drop is

detected, the software starts decrementing the duty cycle. However the new step size

(2∆ ) is half the step size used in the previous stage. The process of reversing the

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scanning direction, while decrementing the duty cycle, continues until the step size

reaches the value 1/255.

Fig. 5.19 The adaptive PAO algorithm flow chart

Three different cases may arise:

• Starting up from zero power conditions

The microcontroller starts with a duty–cycle ratio of 1/255. It increments the

duty cycle in steps of 32/255 as long as it detects that the power extracted from the PV

module increases with each step (∆) as shown in Fig. 5.20.

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Fig. 5.20 Hunting with large step size ∆

However, when a power drop is detected, the software starts decrementing the

duty cycle with a new step size (2∆ ) that is half the step size used in the previous stage.

As long as the power increases, the microcontroller continues to decrement the duty-

cycle ratio as shown in Fig. 5.21.

Fig. 5.21 Hunting with smaller step size

2∆

When another power drop is detected, the software increments its duty-cycle

ratio with a new step size equal to half the previous step size. The process of reversing

the scanning direction, while decrementing the duty cycle, continues until the step size

reaches the value 1/255 as shown in Fig. 5.22. In summary, the algorithm starts by

increasing the duty cycle by a given step size ∆. For each increment, power is calculated

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so that when a power drop is detected the scanning direction is reversed and the duty

cycle is decreased by a new step size ∆/2 equal to half the previous step.

Fig. 5.22 MPP scanning direction

• Hunting around the peak power point

As long as the illumination condition does not change, the microcontroller’s

software keeps hunting around the MPP with increments/decrements of 1/255, as shown

in Fig. 5.23.

Fig. 5.23 Locking on the MPP with duty-cycle ratio 1/255

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• Changes in the illumination condition

Illumination will vary due to changing weather conditions (presence or absence

of clouds). Hunting for the MPP, the microcontroller detects the power change while

changing the pulse width. If the power increases, as shown in Fig. 5.24(a), the

microcontroller continues to change the pulse width in the same direction causing this

power increase. After four consecutive steps in the same direction, the microcontroller

doubles the step size to speed up the process of tracking the new MPP.

Similarly, if power decreases the microcontroller starts scanning by a small step. After

four consecutive steps in the same direction, it doubles the step size to speed up the

process of tracking the new MPP as shown in Fig. 5.24(b).

Fig. 5.24 Scanning in case of varying weather conditions

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CHAPTER 6

SYSTEM RESULTS AND DISCUSSION

6.1. Introduction

The objective of this thesis is to evaluate the model that represents a stand-

alone PV system charging a lead acid battery through Simulink simulation and present

results of the experimental setup. The Simulink and experimental part consists of the

BP380 solar module (Appendix D), an H-bridge converter, a controller, and a 70Ah

battery that were discussed in Chapters 4 and 5. Results will be presented to assess how

efficient is the algorithm, implemented in the controller, in tracking the MPP; i.e. how

much power is extracted from the PV array. The model will also examine the power

electronics efficiency; i.e. how much power is delivered to the battery.

6.2. PV Model Validation

The PV Simulink model is tested under different atmospheric conditions to

prove its validity. It is first simulated for different insolation levels while keeping the

temperature constant (23oC) as shown in Fig. 6.1 and Fig. 6.2. Then it is tested for

different temperatures while keeping the Insolation constant (1000 W/m2) as shown in

Fig. 6.3 and Fig. 6.4 [9]. To draw the real life characteristic curves, the 'BP 380' PV

module was subjected to a variable load circuit shown in Fig. 6.5. The computer issues

a series of increasing digits that are converted to analog voltages using a D/A converter

(R-2R ladder). These increasing digits will load the PV module with increasing current

value IT (where IT = 4 IC ≈ 4 IE = V* / R ≈ Vin / R). Recording the values of the PV

currents IT and their respective PV voltages VT, the module characteristic curves were

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drawn as shown in Fig. 6.6, where this model also proved its validity under the

influence of varied insolation levels and different cell temperatures.

Fig. 6.1 I-V characteristic curves for different Insolation levels

Fig. 6.2 P-V characteristic curves for different Insolation levels

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Fig. 6.3 I-V characteristic curves for different temperatures

Fig. 6.4 P-V characteristic curves for different temperatures

It was observed that the short circuit current Isc of the PV module depends

linearly on the irradiation, while the open-circuit voltage Voc increases logarithmically

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with irradiation, as shown in Fig. 6.1 [25]. Increasing the cell temperature would

decrease the open circuit voltage Voc. The results relates to the theory that can be found

in chapter 3 [2].

Fig. 6.5 Load circuit schematic diagram

Fig. 6.6 PV characteristic curves under different Insolation levels

To test if the Simulink model and the hardware model match, the characteristic

curves of BP380 solar panel were first drawn using the load circuit as shown in Fig. 6.7,

where the reported radiation flux and temperature were 523.44W/m2 and 16.81oC

respectively on the eleventh of January, 2005 at 2:33 pm. Then these curves were

drawn, for the same data, using the Simulink model as shown in Fig. 6.8. The MPP

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reading of the hardware model was 40.42W, and that of the Simulink model was

40.76W, which shows that they agree fairly well.

Fig. 6.7 Characteristic curves of the 'BP 380' PV module using the load circuit

Fig. 6.8 Characteristic curves of the 'BP 380' PV module using the Simulink model

6.3. Simulink Simulation Results

The MPPT Simulink model shown in Fig. 6.9 was simulated for different

temperature and insolation level values. After each run the power, extracted by the

MPPT system, was recorded and then compared to the PV module maximum affordable

power.

Fig. 10 shows the P-V characteristic curve of the PV module for an Insolation

level 800W/m2 and temperature 27oC. The graph readings of the MPP, are: Impp =

3.59A, Vmpp= 18V and Pmpp= 64.7W.

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Fig. 6.9 MPPT Simulink Model

With the adaptive PAO algorithm implemented in the controller, the MPPT

system was simulated for the same input data (T= 27oC and In = 800W/m2). The average

values of the switching current, voltage and power were recoded as follows: Pavg =

62.5W, Iavg = 3.8A and Vavg = 16.4V as shown in Fig. 6.11. These recorded values prove

that the PAO algorithm tracking efficiency is about 96% (ξT = 62.5/ 64.7 = 0.96).

Fig. 6.10 P-V characteristic curve of the PV array at 800W/m2, 27oC

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The power electronics efficiency in the Simulink model is also assessed. The

power delivered to the battery, for the same case, came to be 48W, which means that the

power electronics efficiency is only 80% (ξPE = 50/62.5 = 0.8) as shown in Fig. 6.12.

Fig. 6.11 Switching Power, Voltage, and Current supplied to the converter

Fig. 6.12 Power, Voltage, and Current delivered to the battery

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6.4. Hardware Results

The MPPT hardware system was also examined for different weather

conditions. First the variable load circuit was used to record the MPP data of the PV

module on a clear sunny day at noontime in October as shown in Table 6.1. The MPP

readings came to be: Impp = 4.13A, Vmpp= 13.6V and Pmpp= 56.16W. The characteristic

curves were also plotted as shown in Fig. 6.13.

Fig. 6.13 characteristic curves: (a) I-V curve, (b) P-V curve

Table 6.1 MPP readings on a sunny day in October

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Immediately after recording the MPP data, the MPPT hardware system was set

into action. The visual basic VB program, developed to draw the voltage, current, and

power versus time during tracking action, recorded the following data: Psavg = 53.4W,

Isavg = 4.1A and Vsavg = 13V as shown in Fig. 6.14, where Psavg is the power extracted

form the solar panel. Then the tracking efficiency was calculated as: ξT = Psavg / Pmpp =

53.4 / 56.168 = 0.95. The power electronics efficiency was also measured: ξPE = Pb /

Psavg =43.3/ 53.4 = 0.81, where Pb is the average voltage delivered to the battery.

Fig. 6.14 VB performance monitor

Table 6.2 shows a few selected results taken on various dates and different

daytimes for few minutes of MPPT system operation. It is worth mentioning that as the

solar current Is increases, the power electronics efficiency decreases. This is due to the

fact that the power losses in the hardware design are calculated as the square of the solar

current Is multiplied by the equivalent resistance (Ploss = I2 R), while the input power is

directly proportional to the current and voltage (Pinput=I V). Table 6.3 presents the daily

average reading obtained between 10:00 am and 5:00 pm for the various mentioned

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dates. The average value for the tracking efficiency was recognized at 95% while the

power electronics efficiency at 80% only.

Table 6.2 Snapshots of MPP Recorded Data

Date-Hour Weather condition

Pmmp (W)

Is (A)

Vs (V)

Ps (W)

Pb

(W)

ξT %

ξPE %

29/4/2004 12:50 pm

Sunny day Few clouds

53.4 3.28 15.37 50.42 39.8 94.4 78.9

29/4/2004 3:40 pm

Sunny day Few clouds

50 3.0 15.77 47.32 38 94.6 80.3

30/4/2004 3:30 pm

Sunny day Few clouds

51 3.18 15.12 48.09 38.48 94.3 80

30/4/2004 5:13 pm

Sunny day Few clouds

46.4 2.85 15.51 44.21 36 95.2 81.4

20/10/2004 11:35 am

Hot Sunny day

56 3.4 15.51 52.75 41.8 94.2 79.2

20/10/2004 11:55 am

Hot Sunny day

58 3.3 16.82 55.68 45.34 96 81.4

23/11/2004 10:30 am

Cold Sunny day

49.79 3.06 15.68 48 38.7 96.4 80.6

23/11/2004 10:40 am

Cold Sunny day

50.5

3.06 15.68 48

38.7

95

80.6

Table 6.3 MPP Daily average Recorded Data 2004

Date Weather condition

Pmmp(W) Ps(W) Pb (W) ξT % ξPE %

29/4/2004

Sunny day Few clouds

49.9 47.47 37.97 95 80

30/4/2004

Sunny day Few clouds

49.8 47.2 38.2 94.7 81

20/10/2004

Hot Sunny day

54.7 52.32 42 95.6 80.3

23/10/2004

Hot Sunny day

54.4 51.8 41 95.2 79

23/11/2004

Cold Sunny day

62.7 59.7 48.9 95.2 82

24/11/2004

Cold Sunny day

60.4 57.5 46.2 95.2 80

Average value 95 80

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On a cold sunny day, the average power extracted from the PV module is

greater than that of a hot sunny day. This is due to the fact that Voc increases as

temperature decreases. Consequently the MPP value is raised as shown in Fig. 6.4.

Fig. 6.15 shows how fast is the PAO algorithm, implemented inside the

controller, in tracking the MPP in case of changing weather conditions (varying

insolation level due to the presence of clouds).

Fig. 6.15 Tracking the MPP in case of varying Insolation level

The peaks, present inside the circled region, occur when the MPPT system

starts up and quickly searches for the duty cycle, which loads the PV module at the

MPP. These peaks are issued due to the VB software failure in interpreting the first

input byte by the micrcontroller at startup. These peaks are present for just few

microseconds. Curve (a) represents the PV module varying MPP values due to changing

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weather conditions while curve (b) represents the power extracted from the PV module.

Still the tracking efficiency ξTr was 95% on average.

6.5. Comparison of Tracking Algorithms

The adaptive PAO algorithm showed better performance than the

conventional PAO described in the literature [14] under varying weather conditions

because it can lock on the new MPP with less time than the conventional PAO can. To

compare between the two algorithms, two cases are considered. The first case compares

between the speeds of the algorithms for a minor change in the weather conditions

while the second compares between the speeds for a major change in the weather

conditions.

6.5.1. Minor change in the weather conditions

The conventional PAO algorithm locks on the MPP with a small incremental

step size ∆c of value 1/255. So if a quick change in the weather conditions occurs, the

conventional PAO algorithms starts searching for the new MPP with this small

incremental step as shown in Fig. 6.16. In the shown case the old MPP readings were

recognized at 50.76W and 2.75A for a 600W/m2 radiation flux and 27oC temperature,

while the new MPP readings at 77.86W and 4.14A for a 900W/m2 radiation flux and

27oC temperature. The current values for the old and new MPP on the 255 scale are 117

and 176. For the conventional PAO method, 60 iterations are needed to lock on the new

MPP (176-117= 59, 59+1=60). In the adaptive PAO method, the incremental step ∆a is

doubled after four consecutive increasing power steps. This way the number of

iterations is reduced to 21 based on the tracking scheme shown in Table 6.4. This table

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shows how the incremental step is changing as the power is increasing or decreasing.

The initial incremental step ∆a is taken to be 1 assuming that system was locking on a

MPP. So after four consecutive steps the current is 121 (=117 + 1× 4). Since the power

is still increasing the incremental step is doubled (2×1) and after four consecutive steps

the current is 129 (=121+4×2). The scanning method will continue until a power drop is

sensed, where the scanning direction will be reversed, the incremental step is halved and

the increments will be changed into decrements and vice versa. When the value of the

current reaches 177, a power drop is sensed so the direction of scanning is reversed, the

incremental step is halved (4), and the current is decremented. After one iteration the

value of the current reaches 173 (=177 – 1 × 4)) where another power drop is detected,

so again the direction of scanning is reversed, the incremental step is halved (2), but

now the current is incremented. This tracking scheme will continue until the

incremental step ∆a reached the smallest value i.e. one at the MPP. This means that the

adaptive PAO scheme is 2.875 (60/21) times faster than the conventional one. Thus the

tracking efficiency was increased by 10% using this adaptive technique where it was

85% on the best estimate for the conventional algorithm.

Fig. 6.16 Tracking scheme for minor change in the weather conditions

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Table 6.4 Tracking with adaptive incremental step ∆a

∆a value Previous current value

Number of iterations

Number of increments

New current value

Power condition

1 117 4 4 121 increase

2 121 4 8 129 increase

4 129 4 16 145 increase

8 145 4 32 177 drop

4 177 1 - 4 173 drop

2 173 2 4 177 drop

1 177 2 - 2 175 drop

Total number of iterations 21

6.5.1. Major change in the weather conditions

In this case the old MPP readings were recognized at 22.4W and 1.36A for a

300W/m2 radiation flux and 30oC temperature, while the new MPP readings at 82.4W

and 4.56A for a 1000W/m2 radiation flux and 30oC temperature as shown in Fig. 6.17.

The current values for the old and new MPP on the 255 scale are 58 and 194. For the

conventional PAO method, 137 iterations are needed to lock on the new MPP (194-58=

136, 136+1=137). In the adaptive PAO method, the number of iterations is reduced to

33 based on the tracking scheme shown in Table 6.5 where exactly the same procedure

is followed as in the previous case. So the adaptive PAO scheme is 4.1 (=137/ 33) times

faster than the conventional one in this case. Therefore the adaptive PAO algorithm

reacts faster than the conventional one, especially under quickly varying weather

conditions where the conventional technique fails to track the MPP correctly.

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Fig. 6.17 Tracking scheme for major change in the weather conditions

Table 6.5 Scanning with adaptive incremental step ∆a

∆a value Previous current value

Number of iterations

Number of increments

New current value

Power condition

1 58 4 4 62 increase

2 62 4 8 70 increase

4 70 4 16 86 increase

8 86 4 32 118 increase

16 118 4 64 182 increase

32 182 1 32 214 drop

16 214 2 -32 182 drop

8 182 2 16 198 drop

4 198 2 -8 190 drop

2 190 3 6 196 drop

1 196 3 -3 193 drop

Total number of iterations 33

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6.6. Power Budget

The power losses in the whole design system is calculated and summarized in

Table 6.6. The MPPT system was assumed to operate at MPP (70W) and the switching

frequency f of 40 kHz (T = 1/f = 25µs) with the duty cycle D set to 65%. The load

current IL was 5.8A and a battery voltage of 12V.

6.6.1. Inductor conduction loss

The conduction loss in the inductor can be found by considering the load

current and the winding copper resistance. The measured inductor current is equal to

5.8A and the measured inductor resistance is 0.03Ω. Therefore, the power loss due to

the conduction loss in the inductor is: Pind = I2ind . Rind = 1.009W

6.6.2. Diode conduction loss

The diode conduction loss can be calculated using the following equation:

Pd = IL . Vf = 3.306W

where, from data sheet the forward bias of the diode, Vf = 0.57V.

6.6.3. MOSFET conduction loss

Fig. 6.18 shows the waveform for the current Ip that flows in the primary

winding of the transformer T5 shown before in Fig. 5.14. Since the transformer turns

ratio is 1:1.5, then: Ipon = 1.5 IL = 8.7A.

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Fig. 6.18 Primary winding current waveform

The power loss due to the MOSFETs conduction loss is calculated by

considering the switching current waveforms for each pair of switches as shown in Fig.

6.19.

PTr = (Ipon)2. Ron. ton /(2T) = 0.59W

Where, D = ton / T and from data sheet the on resistance of the MOSFET, Ron =

0.024Ω.

Then the power loss PTR for the four MOSFETs is:

PTR = 4.PTr = 2.36W

Fig. 6.19 Waveforms across the terminals of the transformer

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6.5.4. Transformer power loss

The measured resistance for the primary winding Rpri is 0.0053Ω while that of

the secondary winding Rsec is 0.012Ω.

The waveforms for the current that flows in the secondary winding of the

transformer and the rectifying diodes (D1 and D2) are shown in Fig. 6.20.

Fig. 6.20 Diodes’ current waveform during different intervals

Thus the average power loss in the transformer windings over one cycle can be

divided into two intervals t1 and t2.

During interval t1, only diode D1 of Fig. 5.14 is conducting so the primary

winding and half of the secondary winding contribute to power loss as shown in Fig.

6.21(a). During interval t2, both diodes are conducting so only the secondary winding

contribute to the power losses as shown in Fig. 6.21(b). These two intervals will repeat

but for the next MOSFETs switching period where diode D2 will be conducting as

shown in Fig. 6.21(c).

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Fig. 6.21 Transformer windings contribution to power loss

Thus the energy loss in the transformer during interval t1 can be calculated as:

Et1 = [(Ipon)2 . Rpri + (IL)2 . Rsec ]. ton

During interval t2 the energy loss is calculated as:

Et2 = 2 . [(IL/2)2 . Rsec] . (T-ton)

The average power loss in the transformer Ptrans over one period T is given by:

Ptrans = (Et1 + Et2)/ T = 0.594W

6.5.5. Other power loss factors

Other factors contribute to power loss, among which are the voltage and

current sensing circuit, the microcontroller circuit, the printed copper track resistances

and copper wiring resistance.

A rough estimate calculation was made for the power loss due to these factors

and was found to be 6W.

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Table 6.5 Power Budget

Power Budget Component Input Power Power Loss

BP380 Solar Panel 70W

Inductor 1.009W

Diode 3.306W

MOSFETs 2.36W

Transformer 0.594W

Other Factors 6W

Balance 70W- 13.27W= 56.73W

Power electronics efficiency

ξPE = 56.73/ 70 = 81%

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CHAPTER 7

CONCLUSION AND FUTURE WORK

7.1. Summary

Photovoltaic power production is gaining more significance as a renewable

energy source due to its many advantages. These advantages include pollution free

energy production scheme, ease of maintenance, no noise and direct sunbeam to

electricity conversion [29]. However the high cost of PV installations still forms an

obstacle for this technology. Moreover the PV array output power fluctuates as the

weather conditions, such as the Insolation level, and cell temperature. In order to make

use of the high initial cost it is very important to extract maximum power from the solar

panels for all weather conditions [30]. Stand-alone PV systems cannot supply enough

energy all day long or when no or little solar irradiation exits. Battery storage

capabilities are required in these systems.

So when the PV array is used as a source of power supply to charge a 12V lead

acid battery, it is necessary to use the MPPT to get maximum power from the PV array.

In this work, the MPPT is implemented by using an H-bridge converter, which is

designed to operate under continuous conduction mode and a microcontroller to control

the PWM signals to the converter and also to monitor the state of charge of the battery.

The Perturb and Observe Algorithm is used as the control algorithm for the MPPT.

7.2. Testing Environment

The solar system consists of an 80W PV module, a converter, a controller and a

70Ah battery. The system was designed, built and tested for a period of ten months and

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for different weather conditions. As the main system component, an H-bridge converter

was constructed for the design. By changing the transformer windings ratio, this bridge

can be easily made to work as either a buck or a boost converter. A turn ratio greater

than one means that the output signal will be amplified resulting in a boosted signal,

whereby a turn ratio smaller than one will result in reducing the output signal amplitude

which is the case of buck converter. Moreover unlike the buck converter, the H-bridge

converter operates with 50% duty cycle driving signals, which reduces the switching

failure associated with the buck converter during the turning on or off transitions for

small or large duty cycle driving signals. However the H-bridge converter has four

switching devices while the buck converter has only one. Having an excellent

combination of features, performance, and low power consumption, the PIC16F874

microcontroller is used in the control section. It has 4K x 14 bits of flash memory, 192 x

8 bytes of data memory (RAM), two D/A and five A/D channels. The tracking

algorithm is implemented in the microcontroller where it senses the present values of

the solar current and voltage and compares resultant power with the previous power and

accordingly controls the PWM scheme of the converter.

7.3. Better Tracking Algorithm

The Perturb and Observe, Incremental Conductance, and other maximum

power point tracking algorithms were reviewed and discussed. Although the ICT

technique offers higher tracking efficiency, the PAO algorithm was chosen to track the

MPP since it has lower cost, easier circuitry and less complicated algorithm. However

the conventional PAO was developed to respond faster for quickly varying weather

conditions. An adaptive incremental step was introduced where the performance of the

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algorithm was 2.5 to 4 times faster than the conventional one depending on the location

of the new MPP with respect to the old one. Moreover experimental results have shown

that the MPPT using an adaptive PAO has a tracking efficiency of 95% with a converter

efficiency examined and measured to be 80%.

7.4. Simulink Model

The solar system was also designed and simulated using the matlab Simulink

environment. A model that represents the solar module was created using the Simulink

S-function capability. The controller was also implemented with the help of the S-

function block. The converter and battery were modeled using the Simulink power

electronics library. To match the hardware system and the Simulink software

simulation model, both were tested for a specific flux density and temperature. The

MPP reading of both systems showed that they match up as high as 99%.

7.5. Future Work

The MPPT system that was designed and tested can achieve 76% of total

conversion efficiency so it is still possible to improve its efficiency. The component

choice is very important in the design of the MPPT system. Higher power conversion

efficiency can be achieved by using rectifying diodes with less forward bias voltages,

inductors of lower resistive material, transformer with high magnetic flux density, and

MOSFETs with lower on-state resistance. Moreover the size of the MPPT could be

more compact if surface mount devices SMDs are used and if the system is to operate at

higher switching frequencies where the size of the inductor and transformer will be

reduced. This is part of what should be done in the future for a simple stand-alone PV

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system. However to build a complete system utilizing solar energy for power

generation, a highly efficient dc-ac converter should be implemented. Now instead of

controlling four, six switches should be driven by the control section where it should

keep supplying the correct phase (120o) between the lines. Moreover the transformer-

winding ratio should be carefully chosen to provide 220V on the secondary windings.

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APPENDIX A

MATLAB PROGRAM CODE

function k = pulse01(t,x,u) k(1) = u(1); I = u(2); V = u(3); Pr = u(4); delta = u(5); Pn = I * V; if(delta > 0.000000001) if (Pn >= Pr) k(1) = k(1) + delta; if (k(1) < 3) k(1) = 3; end if (k(1) > 24) k(1) = 23; end elseif (Pn < Pr) delta = delta/2; k(1) = k(1) - delta; if (k(1) < 3) k(1) =3; end if (k(1) > 24) k(1) = 23; end end end k(3) = (delta); Pr = Pn;

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k(2) = Pr; function [sys,x0,str,ts]= pulse01_s(t,x,u,flag) switch flag, case 0 % Initialization s = simsizes; s.NumContStates = 0; s.NumDiscStates = 0; s.NumOutputs = 3; % dynamically sized s.NumInputs = 5; % dynamically sized s.DirFeedthrough = 1; % has direct feedthrough s.NumSampleTimes = 1; sys = simsizes(s); x0 = []; str = []; ts = [-1 0]; % inherited sample time case 3 sys= pulse01(t,x,u); case 1, 2, 4, 9 sys=[]; otherwise error(['Unhandled flag = ',num2str(flag)]); end

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% this mfile represents the PV module voltage and current relations. % it has three inputs which are the insolation G, the temperature T and the current I function V = PV_Cell(t,x,u) G= u(1); %here is the 1st input G T= u(2); %here is the 2nd input T I= u(3); %here is the 3rd input I Rs=0.1; Rsh=10000; Gnom=1000; k=1.38e-23; q=1.6e-19; A=1.5; Vg=1.12; Ns=36; Voc_T1=22.1/Ns; T1=273+25; T3=273+75; Isc_T1=4.8; Isc_T3=5.04; T0=273+T ; %T k0=(Isc_T3-Isc_T1)/(T3-T1); I0_T1=Isc_T1/(exp((q*Voc_T1)/(A*k*T1))-1); b=(Vg*q)/(A*k); b1=q/(A*k*T0); Iph_T1=Isc_T1*G/Gnom; %G Iph=Iph_T1*(1+k0*(T0-T1)); I0=I0_T1*[(T0/T1)^ (3/A)]*[exp(-b*[(1/T0)-(1/T1)])]; Isc=(k0*(T0-T1)+Isc_T1); % Output Voltage: if (I >= Iph) V=0; else V=(1/b1)*[log(((Iph-I)/I0)+1)]*36; end

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function [sys,x0,str,ts]= PV_Cell_s(t,x,u,flag) switch flag, case 0 % Initialization ; s = simsizes; s.NumContStates = 0; s.NumDiscStates = 0; s.NumOutputs = 1; % dynamically sized s.NumInputs = 3; % dynamically sized s.DirFeedthrough = 1; % has direct feedthrough s.NumSampleTimes = 1; sys = simsizes(s); x0 = []; str = []; ts = [-1 0]; % inherited sample time case 3 sys= PV_Cell(t,x,u); case 1, 2, 4, 9 sys=[]; otherwise error(['Unhandled flag = ',num2str(flag)]); end

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APPENDIX B

PCB CIRCUIT DESIGN

Current and voltage sensing circuitry

102

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H-Bridge circuit

103

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Transformer, Rectifier, Filter circuit

Load circuit

104

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APPENDIX C

ASSEMBLY PROGRAM CODE

#INCLUDE<P16F874A.INC> ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;; ;registers LOOP EQU H'20' COUNTER EQU H'21' VACCUH EQU H'22' VACCUL EQU H'23' IACCUH EQU H'24' IACCUL EQU H'25' REFH EQU H'26' REFL EQU H'27' TESTH EQU H'28' TESTL EQU H'29' DIRECTION EQU H'2A' STEP EQU H'2B' SAME EQU H'2C' RESULT EQU H'2D' OUTPUTVALEQU H'2E' SCRATCHH EQU H'2F' SCRATCHL EQU H'30' TEMPO EQU H'31' SHFTCOUNT EQU H'32' ACCUH EQU H'33' ACCUL EQU H'34' SHIFTH EQU H'35' SHIFTL EQU H'36' ROTATERI EQU H'37' FLAG EQU H'38' VAVERAGE EQU H'39' IAVERAGE EQU H'3A' PERIOD EQU H'3B'

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DEFAULTTIME EQU H'3C' SCRATPER EQU H'3D' SCRAT1PER EQU H'3E' RIPPLEREG EQU H'3F' DELDUMMY EQU H'40' VOREG EQU H'41' PARAMETERTURN EQU H'42' ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;; ;constants VPOINTER EQU H'81' IPOINTER EQU H'89' VOPOINTER EQU H'91' RIPPLEINP EQU H'99' IOINP EQU H'A1' MINIDUTYCYC EQU H'01' MAXDUTYCYC EQU H'FE' ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;; ;startup vector ORG H'0000' GOTO MAIN ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;; ;interrupt vector ORG H'0004' GOTO ISR ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;; main ;precautions MOVLW H'00' MOVWF PORTD MOVWF PORTB

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;preparing variables ;loop register CLRF LOOP ;defaulttime register MOVLW H'04' MOVWF DEFAULTTIME ;same register (no. of passes before incrementing step) MOVLW H'07' MOVWF SAME ;initialization of step register by 32 decimal (H'20') MOVLW H'20' MOVWF STEP ;initialization of direction register CLRF DIRECTION ;initialization of reference register CLRF REFH CLRF REFL ;initialization of result register MOVLW H'30' MOVWF RESULT ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;; ;port configuration BSF STATUS,RP0 ;A - analog input MOVLW H'FF' MOVWF TRISA

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;B - digital output - duty cycle variable MOVLW H'00' MOVWF TRISB ;C - pin no.1: capture input ;C - pin no.2: pwm output ;C - pin no.6: serial communication with pc (TX)(PROJECTED) ;C - pin no.7: serial communication with pc (RX)(PROJECTED) MOVLW H'B3' MOVWF TRISC ;E - analog input MOVLW H'07' MOVWF TRISE ;D - digital output MOVLW H'00' MOVWF TRISD BCF STATUS,RP0 ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;; ;pwm preparation ;setting timer2 period BSF STATUS,RP0 MOVLW H'40' MOVWF PR2 BCF STATUS,RP0 ;setting a dummy pulse width for startup MOVLW H'20' MOVWF CCPR1L ;activate timer 2 with zero prescaling on input and output MOVLW H'04'

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MOVWF T2CON ;setting pwm mode for module 1 MOVLW H'0F' MOVWF CCP1CON ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;; ;capture preparation ;setting the mode of timer1 MOVLW H'05' MOVWF T1CON ;preparing module 2 to operate as a capture module on rising edge MOVLW H'05' MOVWF CCP2CON ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;; ;timer0 preparation ;initializing the period register (used by TMR0) MOVLW H'C3' MOVWF SCRATPER COMF SCRATPER,F INCF SCRATPER,F ;scratper by now, contains the exact number needed by TMR0 at 50 Hz. MOVF SCRATPER,W MOVWF PERIOD ;initializing TIMER0 BSF STATUS,RP0 MOVLW H'C2' MOVWF OPTION_REG

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BCF STATUS,RP0 ;presetting timer0 with the default value MOVF PERIOD,W MOVWF TMR0 ;initializing the same register CLRF SAME ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;; ;preparing the a/d conversion module ;configuring analog pins, and output data format in ADRESH, and ADRESL BSF STATUS,RP0 MOVLW H'00' MOVWF ADCON1 BCF STATUS,RP0 ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;; ;arranging for interrupts globally ;enabling TIMER0 interrupts BSF INTCON,T0IE ;enabling capture interrupts BSF STATUS,RP0 BSF PIE2,CCP2IE BCF STATUS,RP0 ;enabling peripheral interrupts

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BSF INTCON,PEIE ;enabling interrupts globally BSF INTCON,GIE ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;; ;serial communications preparation BSF STATUS,RP0 MOVLW H'40' MOVWF SPBRG MOVLW H'26' MOVWF TXSTA BCF STATUS,RP0 ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;; TRAPLOOP CLRWDT GOTO TRAPLOOP ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;; ;interrupt subroutine root ISR BTFSC INTCON,T0IF ;check whether TMR0 interrupt occured GOTO TMR0SR BTFSC PIR2,CCP2IF ;check whether a capture interrupt occured GOTO CAPTINT RETFIE ;false interrupt indication (normally unreachable) ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;

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;capture interrupt branch CAPTINT CLRF TMR1L CLRF TMR1H BCF PIR2,CCP2IF MOVF CCPR2H,W MOVWF SCRAT1PER COMF SCRAT1PER,F INCF SCRAT1PER,F MOVF SCRAT1PER,W MOVWF PERIOD MOVLW H'04' MOVWF DEFAULTTIME RETFIE ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;; ;timer 0 interrupt branch ;recharge timer with period value TMR0SR MOVF PERIOD,W MOVWF TMR0 ;clear timer0 overflow flag BCF INTCON,T0IF INCF LOOP,F ;check turn of sumup,communication,or normal MOVF LOOP,W SUBLW H'80' BTFSC STATUS,Z GOTO SUMUP BTFSC STATUS,C GOTO NORMAL

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;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;; ;collecting data for i and v averages NORMAL MOVLW VPOINTER MOVWF ADCON0 CALL WAITACQ BSF ADCON0,2 WAIVOL BTFSC ADCON0,2 GOTO WAIVOL ;add the resulting voltage sample to the voltage accumulator (data available in adresh) CALL ADDVACCU MOVLW IPOINTER MOVWF ADCON0 CALL WAITACQ BSF ADCON0,2 WAICURR BTFSC ADCON0,2 GOTO WAICURR CALL ADDCURRACCU GOTO FUNNEL1 ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;; SUMUP DECFSZ DEFAULTTIME,F GOTO BULK MOVF SCRATPER,W MOVWF PERIOD ;obtaining averages BULK MOVLW H'07'

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MOVWF COUNTER SHIFTV BCF STATUS,C RRF VACCUH,F RRF VACCUL,F DECFSZ COUNTER,F GOTO SHIFTV MOVF VACCUL,W MOVWF VAVERAGE CLRF VACCUL MOVLW H'07' MOVWF COUNTER SHIFTI BCF STATUS,C RRF IACCUH,F RRF IACCUL,F DECFSZ COUNTER,F GOTO SHIFTI MOVF IACCUL,W MOVWF IAVERAGE CLRF IACCUL ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;; ;performing multiplication CALL IVMULTIPL MOVF ACCUH,W MOVWF TESTH MOVF ACCUL,W MOVWF TESTL ;compare the new test value with the refference VALUE MOVF REFH,W SUBWF TESTH,W ;TESTH = REFH?

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BTFSC STATUS,Z GOTO HEQUAL ;TESTH = REFH, continue comparing TESTL and REFL ;testh not equal to REFH. find which is greater. BTFSC STATUS,C GOTO TESTGTREF ;test is greater than refference GOTO REFGTTEST ;refference is greater than test ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;; HEQUAL MOVF REFL,W SUBWF TESTL,W ;TESTL = REFL? BTFSC STATUS,Z GOTO TESTGTREF ;behave as if test is greater than refference BTFSC STATUS,C GOTO TESTGTREF ;test is greater than refference GOTO REFGTTEST ;refference is greater than test ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;; REFGTTEST INCF DIRECTION,F ;reorient the direction of search ;divide step by 2 BCF STATUS,C RRF STEP,F ;reset the same register CLRF SAME ;goto next stage GOTO FUNNEL2 ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;

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TESTGTREF INCF SAME,F ;check whether the step remained in the same direction for more than 4 times MOVLW H'07' SUBWF SAME,W BTFSS STATUS,C ;not yet GOTO FUNNEL2 ;same greater than or equal to H'07' CLRF SAME ;multiply step by 2 BCF STATUS,C RLF STEP,F ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;; ;check whether step is within boundaries (1<=step<=32) FUNNEL2 MOVLW H'01' SUBWF STEP,W BTFSS STATUS,C ;less than 1 GOTO EQUALIZE1 MOVF STEP,W SUBLW H'20' BTFSS STATUS,C ;greater than h'20'

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GOTO EQUALIZE32 ;within boundaries GOTO CONTINUE ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;; ;load step with h'01' EQUALIZE1 MOVLW H'01' MOVWF STEP GOTO CONTINUE ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;; ;load step with h'20' EQUALIZE32 MOVLW H'20' MOVWF STEP ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;; ;decide whether to increment or decrement CONTINUE BTFSS DIRECTION,0 GOTO ADDSTEP GOTO SUBSTEP ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;; ADDSTEP MOVF STEP,W ADDWF RESULT,F BTFSS STATUS,C GOTO FUNNEL3 ;result exceeds H'FF' MOVLW H'FF'

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MOVWF RESULT ;change the direction of scanning INCF DIRECTION,F GOTO FUNNEL3 ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;; SUBSTEP MOVF STEP,W SUBWF RESULT,F BTFSC STATUS,C GOTO FUNNEL3 ;result is less than H'00' CLRF RESULT ;change the direction of scanning INCF DIRECTION,F ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;; ;set recent test values as future refference values FUNNEL3 MOVF TESTH,W MOVWF REFH MOVF TESTL,W MOVWF REFL ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;; ;result correction if output voltage exceeds maximum value FUNNEL1 MOVLW VOPOINTER MOVWF ADCON0

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CALL WAITACQ BSF ADCON0,2 ;wait for A/D process completion WAIVO BTFSC ADCON0,2 GOTO WAIVO MOVF ADRESH,W ;;;;;;;;;;;;;;;; MOVWF VOREG ;;;;;;;;;;;;;;;; SUBLW H'80' BTFSS STATUS,C GOTO VOGTLIMIT GOTO VOLTLIMIT ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;; ;decrement duty cycle VOGTLIMIT MOVLW H'08' SUBWF RESULT,F BTFSC STATUS,C GOTO EXOUT MOVLW H'01' ;set the minimum. subject to change MOVWF RESULT ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;; EXOUT MOVF RESULT,W MOVWF OUTPUTVAL GOTO FUNNEL4 ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;

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VOLTLIMIT MOVLW RIPPLEINP MOVWF ADCON0 CALL WAITACQ BSF ADCON0,2 MORETIME BTFSC ADCON0,2 GOTO MORETIME MOVF ADRESH,W MOVWF RIPPLEREG SUBLW H'80' BTFSC STATUS,Z GOTO EQUAL BTFSC STATUS,C GOTO RECLTREQ GOTO REQLTREC ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;; EQUAL MOVF RESULT,W MOVWF OUTPUTVAL GOTO FUNNEL4 ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;; RECLTREQ MOVF RIPPLEREG,W SUBLW H'80' MOVWF OUTPUTVAL MOVF RESULT,W

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ADDWF OUTPUTVAL,F BTFSS STATUS,C GOTO FUNNEL4 MOVLW H'FF' MOVWF OUTPUTVAL GOTO FUNNEL4 ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;; REQLTREC MOVLW H'80' SUBWF RIPPLEREG,W SUBWF RESULT,W BTFSS STATUS,C GOTO ADJUSTOUT MOVWF OUTPUTVAL GOTO FUNNEL4 ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;; ADJUSTOUT MOVLW H'00' MOVWF OUTPUTVAL GOTO FUNNEL4 ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;; ;checkpoint for final values to be outputted FUNNEL4 MOVLW MINIDUTYCYC SUBWF OUTPUTVAL,W BTFSC STATUS,C

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GOTO SECONDTEST MOVLW MINIDUTYCYC MOVWF OUTPUTVAL GOTO EXPORT ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;; SECONDTEST MOVF OUTPUTVAL,W SUBLW MAXDUTYCYC BTFSC STATUS,C GOTO EXPORT MOVLW MAXDUTYCYC MOVWF OUTPUTVAL GOTO EXPORT ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;; EXPORT MOVF OUTPUTVAL,W ;export the value through the portb MOVWF PORTB ;prepare the number to be exported through the duty cycle register MOVWF SCRATCHH CLRF SCRATCHL ;shift two times BCF STATUS,C RRF SCRATCHH,F RRF SCRATCHL,F BCF STATUS,C RRF SCRATCHH,F

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RRF SCRATCHL,F BCF STATUS,C ;prepare the two least significant bits RRF SCRATCHL,F BCF STATUS,C RRF SCRATCHL,F BCF STATUS,C MOVLW H'30' ANDWF SCRATCHL,F MOVF CCP1CON,W ANDLW H'CF' IORWF SCRATCHL,W MOVWF CCP1CON MOVF SCRATCHH,W ANDLW H'3F' MOVWF CCPR1L MOVF STEP,W MOVWF TEMPO MOVLW H'3F' ANDWF TEMPO,F BTFSS DIRECTION,0 GOTO DISPRES GOTO DISPSET DISPRES BCF TEMPO,6 GOTO STATION2 DISPSET BSF TEMPO,6 STATION2 BSF TEMPO,7 MOVF TEMPO,W

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MOVWF PORTD RETFIE ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;; ;subroutines ;IV multiplication subroutine IVMULTIPL MOVLW H'08' MOVWF SHFTCOUNT CLRF ACCUL CLRF ACCUH CLRF SHIFTH MOVF VAVERAGE,W MOVWF SHIFTL MOVF IAVERAGE,W MOVWF ROTATERI ;;;;;;;;;;;;;;;; BACKAA BCF STATUS,C RRF ROTATERI,F BTFSC STATUS,C CALL ADD_SR CALL SHIFTSR DECF SHFTCOUNT,F BTFSS STATUS,Z GOTO BACKAA RETURN ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;; ADD_SR CLRF FLAG MOVF SHIFTL,W ADDWF ACCUL,F BTFSC STATUS,C INCF FLAG,F

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MOVF SHIFTH,W ADDWF ACCUH,F BTFSC FLAG,0 INCF ACCUH,F RETURN ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;; SHIFTSR BCF STATUS,C RLF SHIFTL,F RLF SHIFTH,F RETURN ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;; WAITACQ MOVLW H'0E' MOVWF DELDUMMY DELBACK DECFSZ DELDUMMY,F GOTO DELBACK RETURN ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;; ADDVACCU MOVF ADRESH,W ADDWF VACCUL,F BTFSC STATUS,C INCF VACCUH,F RETURN ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;; ADDCURRACCU MOVF ADRESH,W ADDWF IACCUL,F BTFSC STATUS,C INCF IACCUH,F RETURN ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;

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;communications subroutine COMMUNICAT MOVF LOOP,W ANDLW H'07' SUBLW H'04' BTFSS STATUS,Z GOTO FUNNELEX MOVF LOOP,W MOVWF PARAMETERTURN MOVLW H'78' ANDWF PARAMETERTURN,F BCF STATUS,C RRF PARAMETERTURN,F BCF STATUS,C RRF PARAMETERTURN,F BCF STATUS,C RRF PARAMETERTURN,F BCF STATUS,C MOVLW H'0F' ANDWF PARAMETERTURN,F MOVF PARAMETERTURN,W SUBLW H'00' BTFSC STATUS,Z ;export average input voltage GOTO EXPOVAVERAGE MOVF PARAMETERTURN,W SUBLW H'01' BTFSC STATUS,Z ;export average input current GOTO EXPOIAVERAGE MOVF PARAMETERTURN,W

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SUBLW H'02' BTFSC STATUS,Z ;export lower byte of power output GOTO EXPOPL MOVF PARAMETERTURN,W SUBLW H'03' BTFSC STATUS,Z ;export upper byte of power output GOTO EXPOPH MOVF PARAMETERTURN,W SUBLW H'04' BTFSC STATUS,Z ;export output voltage value GOTO EXPOVO MOVF PARAMETERTURN,W SUBLW H'05' BTFSC STATUS,Z ;export duty cycle GOTO EXPODUTY MOVF PARAMETERTURN,W SUBLW H'06' BTFSC STATUS,Z ;export step GOTO EXPOSTEP MOVF PARAMETERTURN,W SUBLW H'07'

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BTFSC STATUS,Z ;export direction register GOTO EXPODIR MOVF PARAMETERTURN,W SUBLW H'08' BTFSC STATUS,Z ;export output current GOTO EXPOIO MOVF PARAMETERTURN,W SUBLW H'0F' BTFSC STATUS,Z ;export zero flag GOTO EXPOZERO ;export flag (H'FF') GOTO EXPOFLAG ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;; EXPOVAVERAGE MOVF VAVERAGE,W MOVWF TXREG GOTO FUNNELEX EXPOIAVERAGE MOVF IAVERAGE,W MOVWF TXREG GOTO FUNNELEX EXPOPL MOVF TESTL,W MOVWF TXREG GOTO FUNNELEX EXPOPH MOVF TESTH,W MOVWF TXREG GOTO FUNNELEX

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EXPOVO MOVF VOREG,W MOVWF TXREG GOTO FUNNELEX ;************************************ EXPOIO MOVLW IOINP MOVWF ADCON0 CALL WAITACQ BSF ADCON0,2 WAK BTFSC ADCON0,2 GOTO WAK MOVF ADRESH,W MOVWF TXREG GOTO FUNNELEX ;************************************ EXPOFLAG MOVLW H'FF' MOVWF TXREG GOTO FUNNELEX EXPOZERO MOVLW H'00' MOVWF TXREG GOTO FUNNELEX EXPODUTY MOVF RESULT,W MOVWF TXREG GOTO FUNNELEX EXPOSTEP MOVF STEP,W MOVWF TXREG GOTO FUNNELEX EXPODIR MOVF DIRECTION,W MOVWF TXREG GOTO FUNNELEX FUNNELEX RETURN ;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;;; END

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APPENDIX D

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