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ANALYSIS OF A TENSEGRITY SYSTEM FOR OCEAN WAVE ENERGY HARVESTING By RAFAEL ESTEBAN V ´ ASQUEZ MONCAYO A DISSERTATION PRESENTED TO THE GRADUATE SCHOOL OF THE UNIVERSITY OF FLORIDA IN PARTIAL FULFILLMENT OF THE REQUIREMENTS FOR THE DEGREE OF DOCTOR OF PHILOSOPHY UNIVERSITY OF FLORIDA 2011

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ANALYSIS OF A TENSEGRITY SYSTEM FOROCEAN WAVE ENERGY HARVESTING

By

RAFAEL ESTEBAN VASQUEZ MONCAYO

A DISSERTATION PRESENTED TO THE GRADUATE SCHOOLOF THE UNIVERSITY OF FLORIDA IN PARTIAL FULFILLMENT

OF THE REQUIREMENTS FOR THE DEGREE OFDOCTOR OF PHILOSOPHY

UNIVERSITY OF FLORIDA

2011

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c© 2011 Rafael Esteban Vasquez Moncayo

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I dedicate this work to my love (G), my family and my friends

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ACKNOWLEDGMENTS

I express my gratitude to my supervisory committee: Dr. Carl Crane, Dr. Jacob

Hammer, Dr. John Schueller, Dr. Warren Dixon and Dr. Julio Correa for their time,

effort, and invaluable contributions to my academic growth during my time at the

University of Florida.

This research was done with financial support from the U.S. Department of State,

through the Fulbright Program; the University of Florida, through the Center for Latin

American Studies and the Department of Mechanical and Aerospace Engineering;

the Colombian Administrative Department of Science, Technology and Innovation:

Colciencias; and the Universidad Pontificia Bolivariana, Medellin.

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TABLE OF CONTENTS

page

ACKNOWLEDGMENTS . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 4

LIST OF TABLES . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 7

LIST OF FIGURES . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 8

ABSTRACT . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 10

CHAPTER

1 INTRODUCTION . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 11

1.1 Ocean Energy . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 121.1.1 Wave Energy . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 131.1.2 Wave Energy Resource . . . . . . . . . . . . . . . . . . . . . . . . . 141.1.3 Wave Energy Technology . . . . . . . . . . . . . . . . . . . . . . . . 15

1.2 Tensegrity Systems . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 161.2.1 Advantages of Tensegrity Systems . . . . . . . . . . . . . . . . . . . 161.2.2 Motion Applications of Tensegrity Systems . . . . . . . . . . . . . . 181.2.3 Ocean Applications of Tensegrity Systems . . . . . . . . . . . . . . . 19

2 OCEAN WAVE MECHANICS . . . . . . . . . . . . . . . . . . . . . . . . . . . 21

2.1 Airy’s Linear Wave Theory . . . . . . . . . . . . . . . . . . . . . . . . . . . 212.2 Traveling Waves . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 242.3 Water Particle Motions . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 272.4 Wave Energy and Power . . . . . . . . . . . . . . . . . . . . . . . . . . . . 282.5 Wave Mechanics Numerical Example . . . . . . . . . . . . . . . . . . . . . 30

2.5.1 Kinematic Properties . . . . . . . . . . . . . . . . . . . . . . . . . . 302.5.2 Water Particles Motion . . . . . . . . . . . . . . . . . . . . . . . . . 312.5.3 Wave Energy . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 31

2.6 Wave-Structure Interaction . . . . . . . . . . . . . . . . . . . . . . . . . . . 322.6.1 Heaving and Pitching Body Motions . . . . . . . . . . . . . . . . . . 322.6.2 Heaving Equation of Motion . . . . . . . . . . . . . . . . . . . . . . 34

2.6.2.1 Mass and Added Mass . . . . . . . . . . . . . . . . . . . . 352.6.2.2 Radiation and Viscous Damping . . . . . . . . . . . . . . . 36

2.6.3 Wave-Induced Forces . . . . . . . . . . . . . . . . . . . . . . . . . . 372.6.4 Steady State Solution of the Heaving Equation . . . . . . . . . . . . 38

3 TENSEGRITY MECHANISM . . . . . . . . . . . . . . . . . . . . . . . . . . . 39

3.1 Morphology Definition . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 393.2 Position Analysis . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 40

3.2.1 Forward Position Analysis . . . . . . . . . . . . . . . . . . . . . . . 403.2.2 Reverse Position Analysis . . . . . . . . . . . . . . . . . . . . . . . . 42

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3.2.3 Numerical Example . . . . . . . . . . . . . . . . . . . . . . . . . . . 433.3 Velocity Analysis . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 44

3.3.1 Forward Velocity Analysis . . . . . . . . . . . . . . . . . . . . . . . 453.3.2 Reverse Velocity Analysis . . . . . . . . . . . . . . . . . . . . . . . . 463.3.3 Numerical Example . . . . . . . . . . . . . . . . . . . . . . . . . . . 47

3.4 Equation of Motion . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 493.4.1 Assumptions . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 493.4.2 Kinetic Energy . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 503.4.3 Potential Energy . . . . . . . . . . . . . . . . . . . . . . . . . . . . 513.4.4 Friction Vector . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 533.4.5 Generalized Forces . . . . . . . . . . . . . . . . . . . . . . . . . . . 53

4 OCEAN WAVE ENERGY HARVESTING . . . . . . . . . . . . . . . . . . . . . 54

4.1 Electrical Generators for Wave Energy Harvesting . . . . . . . . . . . . . . 544.2 Sea State Selection . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 55

4.2.1 Wave Power and Wave Kinematic Properties . . . . . . . . . . . . . 564.3 Direct Drive Heaving System . . . . . . . . . . . . . . . . . . . . . . . . . 574.4 Tensegrity System . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 594.5 Discussion of Results . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 62

5 CONCLUSIONS AND FUTURE WORK . . . . . . . . . . . . . . . . . . . . . . 64

5.1 Conclusions . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 645.2 Future Work . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 65

REFERENCES . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 66

BIOGRAPHICAL SKETCH . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 76

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LIST OF TABLES

Table page

1-1 Ocean energy global resource . . . . . . . . . . . . . . . . . . . . . . . . . . . . 12

3-1 Mechanism parameters for kinematic chain . . . . . . . . . . . . . . . . . . . . . 40

3-2 Position analysis numerical example results . . . . . . . . . . . . . . . . . . . . . 43

4-1 Direct drive heaving float coefficients . . . . . . . . . . . . . . . . . . . . . . . . 57

4-2 Tensegrity harvesting system coefficients . . . . . . . . . . . . . . . . . . . . . . 60

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LIST OF FIGURES

Figure page

1-1 Ocean energy conversion development . . . . . . . . . . . . . . . . . . . . . . . . 13

1-2 Global coastal wave power estimates . . . . . . . . . . . . . . . . . . . . . . . . 14

1-3 Tensegrity morphologies . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 16

2-1 Notation for the linear wave analysis . . . . . . . . . . . . . . . . . . . . . . . . 22

2-2 Particle paths predicted by Airy’s linear wave theory . . . . . . . . . . . . . . . 28

2-3 Notation for the wave energy analysis . . . . . . . . . . . . . . . . . . . . . . . . 28

2-4 Example water particles motion . . . . . . . . . . . . . . . . . . . . . . . . . . . 31

2-5 Rigid body with six degrees of freedom . . . . . . . . . . . . . . . . . . . . . . . 32

2-6 Floating bodies undergoing heaving or pitching motion . . . . . . . . . . . . . . 33

2-7 Floating bodies: pure heaving and pitching conditions . . . . . . . . . . . . . . . 33

2-8 Added mass and added-mass moment of inertia coefficients for a rectangular body 35

2-9 Non-dimensional radiation damping coefficient for a heaving rectangular section 36

3-1 Concept of a wave energy harvester based on tensegrity systems . . . . . . . . . 39

3-2 Kinematic diagram of the mechanism . . . . . . . . . . . . . . . . . . . . . . . . 40

3-3 Vector diagram of the mechanism . . . . . . . . . . . . . . . . . . . . . . . . . . 41

3-4 Position analysis numerical example . . . . . . . . . . . . . . . . . . . . . . . . . 43

3-5 Velocity analysis numerical example . . . . . . . . . . . . . . . . . . . . . . . . . 48

3-6 Velocity analysis numerical example results . . . . . . . . . . . . . . . . . . . . . 48

4-1 Location and bathymetry of Isla Fuerte, Colombia . . . . . . . . . . . . . . . . . 56

4-2 Wave power variation for the sea state at 9.408◦ N, 76.180◦ W . . . . . . . . . . 57

4-3 Heaving body simulation: wave-induced force . . . . . . . . . . . . . . . . . . . 58

4-4 Heaving body simulation response . . . . . . . . . . . . . . . . . . . . . . . . . . 58

4-5 Tensegrity simulation: wave-induced forces . . . . . . . . . . . . . . . . . . . . . 60

4-6 Tensegrity simulation: surging, heaving and pitching motions . . . . . . . . . . . 61

4-7 Tensegrity simulation: instant dissipated power . . . . . . . . . . . . . . . . . . 62

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4-8 Tensegrity simulation: motion in generators and springs . . . . . . . . . . . . . 62

4-9 Variation of power dissipation with mechanism parameters . . . . . . . . . . . . 63

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Abstract of Dissertation Presented to the Graduate Schoolof the University of Florida in Partial Fulfillment of theRequirements for the Degree of Doctor of Philosophy

ANALYSIS OF A TENSEGRITY SYSTEM FOROCEAN WAVE ENERGY HARVESTING

By

Rafael Esteban Vasquez Moncayo

December 2011

Chair: Carl D. Crane IIIMajor: Mechanical Engineering

Tensegrity systems have been used in several disciplines such as architecture,

biology, aerospace, mechanics and robotics during the last fifty years. However, just

a few references in literature have stated the possibility of using tensegrity systems in

ocean or energy-related applications. This research addresses the analysis of a tensegrity

mechanism for ocean wave energy harvesting.

The mechanics of ocean waves is described using the linear theory developed by

George B. Airy. The kinematic properties of the waves, the motion of particles and wave

power calculation are addressed. Then, the fluid structure interaction is reviewed making

emphasis on the concepts of radiation damping and viscous damping.

A planar tensegrity mechanism is proposed based on a planar morphology known

as “X-frame” that was developed by Kenneth Snelson in 1960s. A geometric approach

is used to solve the forward and reverse displacement problems. The theory of screws is

used to perform the forward and reverse velocity analyses of the device. The Lagrangian

approach is used to deduce the equations of motion considering the interaction between

the mechanism and ocean waves.

The tensegrity configuration is compared to a purely heaving body that is commonly

used in ocean wave energy harvesting. The result shows that tensegrity systems could

play an important roll in the expansion of clean energy technologies that help the world’s

sustainable development.

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CHAPTER 1INTRODUCTION

Due to sustainability concerns, a world race started several years ago to incentivize

the research, development and utilization of renewable energy sources [1–3]. The ocean

represents an enormous potential energy source [4, 5]; however, its exploitation is still

incipient compared to other well-established power harvesting technologies such as wind

and solar energies [6].

Ocean energy can be obtained from waves, tides, currents, thermal gradients and

salinity gradients. During the last 30 years the R&D works in all these resources have

increased considerably [7–17]. Several assessment studies to evaluate the amount of ocean

energy which is available at a particular region, and to determine the technology that is

convenient for the local conditions have been conducted in different countries [17–26].

Wave energy constitutes the most noticeable form of ocean energy, maybe because

of its (often impressive) destructive capabilities [27]. The U.S. Department of Energy

(DoE) developed the Marine and Hydrokinetic Technology Database [28], as a shared

resource for the marine/hydrokinetic industry and government. There are more than 160

different devices for ocean energy harvesting registered in the data base, with about 40%

corresponding to wave energy.

The word tensegrity is a combination of the words tension and integrity [29].

Tensegrity systems were introduced in the 20th century by Fuller [29], Emmerich [30]

and Snelson [31]. These systems are formed by a combination of rigid elements (struts)

under compression, and elastic elements (ties) under tension [32, 33].

Tensegrity systems have been used in several disciplines such as architecture, biology,

aerospace, mechanics and robotics during the last fifty years [34]. Applications in sciences

and engineering include, among others, development of structural domes and bridges

[35–40], deployable systems for space applications [41–46], description and modelling of

living organisms and biological systems [47–51], and applications in robotics [52–60].

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Just a few references in literature have stated the possibility of using tensegrity

systems in ocean applications. Scruggs and Skelton [61] made a preliminary investigation

in the potential use of controlled tensegrity structures to harvest energy, and suggested

their suitability to harvest energy from ocean waves. They showed how a tensegrity

structure, with one active bar, can be used to effectively harvest energy when it is excited

at a single frequency. Jensen et al. [62] proposed tensegrity structures in the design of

wave compliant structures for offshore aquaculture; they studied different combinations of

pre-stress and determined how it influences the stiffness of the whole structure. Wroldsen

[63] developed analysis tools based on differential-algebraic equations (DAEs) of motion,

and extended the formulation to include the dynamics of relatively long and heavy cables

with increased computational efficiency. Tensegrity systems could play an important roll

in the expansion of clean energy technologies that would contribute to world’s sustainable

development. Therefore, this can be a promising field of development that is still on a

conceptual level and needs to be explored.

1.1 Ocean Energy

The oceans contain a large amount of renewable energy. Reports of the estimated

global resource, presented by AEA Energy & Environment [6] and the U.S. Department of

Energy [64], are summarized in Table 1-1.

Table 1-1. Ocean energy global resource.

Energy type Estimated global resourceWave energy 80000 TWh/yTidal energy 300+ TWh/yMarine current 800+ TWh/yThermal energy 10000 TWh/ySalinity gradient 2000 TWh/y

The International Energy Agency (IEA) [14] reported the global status of technology

development for ocean energy systems, Figure 1-1A, highlighting the United Kingdom,

the United States, Canada and Norway, as leaders in development. Figure 1-1B shows the

emphasis placed on the development of wave energy technologies.

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Concept designPart-scale (Tank)Part-scale (Sea)Full-scalePre and commercial production

B Technology status.

Figure 1-1. Ocean energy conversion development [14].

Although environmental legislation for the deployment of ocean energy projects is

not clear yet in plenty of countries, several studies are being carried out around the world

to demonstrate sustainability and commercialization potentials of ocean energy, and to

fulfill legislative requirements that aim to protect the environment near exploitation areas

[65–67]. In this direction, the Department of the Interior of the United States [68] stated

policies about the use of renewable energy and alternate uses of existing facilities on

the outer continental shelf. Additionally, Det Norske Veritas (DNV) [69] developed the

Offshore Service Specification DNV-OSS-312, which presents the principles and procedures

with respect to certification of tidal and wave energy converters.

1.1.1 Wave Energy

Wave energy is an indirect form of solar energy. Temperature differences produced

by the solar radiation around the world create winds that blow over the ocean surface,

generating waves. Such waves can travel thousands of kilometers through deep waters with

minimal loss of energy, representing a source with higher power density than wind or solar

power [70].

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1.1.2 Wave Energy Resource

Waves transport both kinetic and potential energy. The total energy of a wave

depends mainly on its height (H) and its period (T ), and is usually measured in Watt

per meter (W/m) of wave front. The global wave power potential is of the same order of

magnitude as the world’s electricity consumption, around 1-10 TW [4]. Cruz [71] states

that it is possible to extract 10-25 % of this energy, suggesting that wave power could

make a significant contribution to the renewable energy industry. The best wave climates,

whose annual average power levels are between 20 and 70 kW/m or higher, are found in

zones from 30 to 60 degrees latitude, Figure 1-2. Nonetheless, attractive wave climates are

found also within ±30 degrees latitude, where the lower power level is compensated by

smaller power variability [4].

Figure 1-2. Global coastal wave power estimates from the Topex altimeter [72].

As deep-water waves approach shallow waters, they slow down, their wavelength

decrease and their height grows, which leads to breaking. The major losses of energy are

due to breaking and to friction with the seabed; therefore, only a fraction of the resource

reaches the shore [71]. Not all sites are suitable for deployment of harvesting devices for

several reasons, including unsuitable geomorphologic conditions at the shoreline, excessive

tidal range and environmental impact [4]. Nonetheless, shoreline devices could provide a

substantial contribution to the electric energy demands in small islands or isolated coastal

regions where the energy consumption is small.

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1.1.3 Wave Energy Technology

There are several technologies that result from different ways in which the energy can

be harnessed from waves, depending on the water depth and the location (i.e. shoreline,

near-shore, offshore) [27]. Several ways to classify wave energy devices have been proposed.

Falcao [27] recently proposed a classification based on the type, the deployment style, and

the deployment place as follows:

• Oscillating water columns (OWC) are devices that have a partially submergedstructure, open below the water surface which holds air inside. The incident wavesthat go through the OWC, create oscillating motion of the air inside the chamber,forcing the air to flow through a turbine which drives an electrical generator.Self-rectifying turbines which provide a unidirectional rotation for an alternating airflow, such as the Wells turbine [73, 74], are often used in such devices.

• Oscillating body systems are generally located offshore (water depth > 40 m), andcan be either floating or fully submerged [27, 75]. The main element of these systemsis an oscillating body that either floats or is submerged near the surface [4]. Severalconfigurations such as single-body heaving buoys, two-body heaving systems, fullysubmerged heaving systems, pitching devices and bottom-hinged systems, havebeen used to build this type of energy converters [27]. Several techniques havebeen proposed to harness the energy with oscillating bodies, using either linear(translational) or rotational electrical generators.

• Overtopping converters constitute another type of wave energy converters. Thewater in the wave crest is introduced by overtopping through a sloping wall or rampinto a reservoir located at a level higher than the surrounding water surface. Thepotential energy of the water is then converted into useful energy through an arrayof low-head hydraulic turbines (e.g. Kaplan turbines) [27, 76].

Dunnett and Wallace [77] proposed an alternative classification for wave energy

converters. This classification method is based on how the devices get the mechanical

energy from the waves:

• Point absorbers are devices whose surface area is very small in comparison to thewavelength of ocean waves.

• Attenuators are relatively long devices that are placed parallel to the generaldirection of wave travel.

• Terminators are placed perpendicularly to the waves and are intended to absorb alarge proportion of the energy of the wave.

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1.2 Tensegrity Systems

Skelton and de Oliveira [34] recently defined a tensegrity configuration as follows:

“In the absence of external forces, let a set of rigid bodies in a specific configuration have

torqueless connections. Then this configuration forms a tensegrity configuration if the

given configuration can be stabilized by some set of internal tensile members, i.e. connected

between the rigid bodies.”.

Figure. 1-3 shows three different tensegrity morphologies that have been extensively

addressed in literature for different applications.

A X-frame [31]. B Octahedron. C 6-bar prism.

Figure 1-3. Tensegrity morphologies.

1.2.1 Advantages of Tensegrity Systems

Tensegrity systems offer a number of advantages as described by Skelton et al. [78]

and Wroldsen [63]. Such characteristics are summarized in the following paragraphs.

Stabilizing tension. A tensegrity structure gets a stable static equilibrium configuration

when all ties are in tension and all struts are in compression (in the absence of external

forces or torques) [63]. Compressive members lose stiffness as they are loaded, whereas

tensile members, possessing less weight, gain stiffness as they are loaded [78].

Geometry and structural efficiency. Traditionally, structures tend to be made with

orthogonally arranged elements [78]. However, this type of architecture does not usually

yield minimal mass designs for given sets of stiffness properties [79]. Tensegrity systems,

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on the other hand, use longitudinal members arranged in unusual patterns, to achieve

strength conditions with less mass [78].

Deployability and small storage volume. Since the members in compression are either

disjoint or connected by simple joints, large displacement, deployability, and stowage in a

compact volume appear as advantages of tensegrity systems [46, 78].

Tunable stiffness. One remarkable property of tensegrity systems is the possibility

to change shape without changing stiffness and vice versa [80]. These structures usually

have low structural damping, leading to challenges/opportunities with respect to vibration

in some applications [63]. Skelton et al. [78] addressed that structures designed to allow

tuning would play an important role in the development of next generation mechanical

systems.

Reliability in modelling. Since most members in a tensegrity system are axially

loaded, the equations needed to represent the static and dynamic behavior requires, in

general, less simplifications, resulting into more reliable models [63, 78].

Active control. A single member of a tensegrity system can serve multiple functions:

as a load-carrying member, a sensor, an actuator, etc. This flexibility provides an

encouraging opportunity for integrating structural and control design processes [78, 81].

Motivation from Biology. Ingber [47, 49] and Huang et al. [50] stated that tensegrity

is a fundamental building architecture of life. Hence, if tensegrity is part of nature’s

building architecture, the capabilities of tensegrity could make the efficiency present in

natural systems transferable to man-made systems [78].

Modularity through cells. Tensegrity systems are often made using a large number

of identical building blocks, or cells. The modularity facilitates large-scale production of

identical units that can be later assembled [63].

Robustness through redundancy. Using more ties than strictly needed (redundancy)

increases the system robustness and helps to avoid infinitesimal mechanisms [63].

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1.2.2 Motion Applications of Tensegrity Systems

The involvement of tensegrity systems in motion applications is relatively new,

and several works have been increasingly appearing during the last twenty years. At

the beginning of the 1990’s, Pellegrino [82] presented a theory for the matrix analysis

of kinematically indeterminate prestressed assemblies made from pin-jointed bars based

on a linear approach. Calladine and Pellegrino [83] discussed the analytical conditions

under which a pin-jointed assembly, which has independent states of self-stress and m

independent mechanisms, tightens up when its mechanisms are excited. Djouadi et al.

[84] described a numerical scheme of active nonlinear control of tensegrity systems for

space applications. Stern [41] developed generic design equations to find the lengths of

the struts and elastic ties needed to create a desired geometry. Sultan [85] worked on

modelling, design, and control of tensegrity structures for several applications. Duffy et al.

[42] presented a review of a family of tensegrity structures that self deploy from a stowed

or packed configuration. Knight [43] addressed the problem of stability of tensegrity

structures for the design of a deployable antenna. Pellegrino et al. [44] studied deployable

structures for small satellite missions. Sultan et al. [52] proposed the development of a

flight simulator based on a tensegrity structure.

Starting the decade of 2000s, Oppenheim and Williams [86] examined the dynamic

behavior of a simple elastic tensegrity structure. Skelton et al. [87] developed an explicit

analytical model of the nonlinear dynamics of a large class of tensegrity structures. Sultan

et al. [88] formulated the general prestressability conditions for tensegrity structures,

expressed as a set of nonlinear equations and inequalities on the tendon tensions.

Kanchanasaratool and Williamson [54] developed a passive nonlinear constrained particle

dynamic model for a class of tensegrity platform structures. Sultan et al. [89] derived

the linearized equations of motion for tensegrity structures around arbitrary equilibrium

configurations. Tibert [45] worked on the development of deployable tensegrity structures

for space applications. Tran et al. [53] performed the reverse displacement and compliance

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analysis of a tensegrity based parallel mechanism. Sultan and Skelton [46] presented a

strategy for tensegrity structures deployment using sets of equilibria. Bossens et al. [90]

analyzed the dynamic behavior of a tensegrity structure by comparing a finite element

model with an experimental model. Chan et al. [91] used simple control strategies for

the active vibration control of a three-stage tensegrity structure. Marshall and Crane [56]

proposed a six-degree-of-freedom tensegrity-based parallel platform which combines rigid

and elastic elements. Sultan and Skelton [55] used the intrinsic properties of tensegrity

structures to construct a smart force/torque sensor.

More recently, Crane et al. [92] obtained the equilibrium position for a general

skew-prismatic structure with a variety of external loads and moments acting on the

structure, using the virtual work principle. Arsenault and Gosselin [57–59] addressed the

possibility of the tensegrity systems to be used in the development of new lightweight

mechanisms for motion applications where only rigid-link robots have been considered.

Bayat and Crane [93] presented a closed-form analysis of a series of planar tensegrity

structures to determine all possible equilibrium configurations for each device when

no external forces or moments are applied. Arsenault and Gosselin [94] used general

static balancing conditions adapted for the case of tensegrity mechanisms. Vasquez

and Correa [60] presented the kinematic and the dynamic analyses, and a nonlinear

control strategy for a planar three-degree-of-freedom tensegrity robot manipulator.

Crane et al. [95] performed the equilibrium analysis of a planar tensegrity mechanism

showing the complexity that results from non-zero free lengths in the compliant elements.

Arsenault and Gosselin [96] presented the direct and inverse static analyses for a new

spatial tensegrity mechanism minimizing its potential energy. Wroldsen et al. [97] used a

non-linear feedback control law for non-minimal realizations of tensegrity systems.

1.2.3 Ocean Applications of Tensegrity Systems

Scruggs and Skelton [61] made a preliminary investigation in the potential use of

controlled tensegrity structures to harvest energy. They presented an approach to use

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linear regenerative actuators as active bars into the structure. They illustrated the

approach in a simulation example for a small scale one-actuator system, and suggested the

suitability of tensegrity systems to harvest energy from ocean waves.

Jensen et al. [62] and Wroldsen [63] proposed tensegrity structures in the design

of wave compliant structures for offshore aquaculture. They addressed the promising

properties with respect to control of geometry, stiffness and vibration, that could make

tensegrity an enabling technology for future developments in open ocean aquaculture

construction systems for high energy environments.

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CHAPTER 2OCEAN WAVE MECHANICS

Ocean waves can be generated by several phenomena, such as motions of celestial

bodies (sun and moon), seismic disturbances (earthquakes), moving bodies (ships) and

winds. The wind produces waves of different types, from the short capillary wave to the

long swell, that can be classified as follows [98]:

• Linear waves (sinusoidal profiles).

• Nonlinear waves (non-symmetrical profiles).

• Random seas (predictable in the frequency domain under certain assumptions).

For this research, a linear model of wind-generated waves, developed by George B.

Airy in 1841 [99], is used.

2.1 Airy’s Linear Wave Theory

George B. Airy developed the first meaningful analysis of ocean waves [100]. It

involves the solution of the linear equation of continuity (conservation of mass) for an

irrotational flow subject to linearized boundary conditions. The wave properties derived

with this theory are good approximations for small values of the wave steepness (defined

as the ratio between the wave height H and the wave length λ, Figure 2-1) [98, 101], i.e.

waves with relatively small amplitudes.

The following parameters are defined for the linear wave analysis, Figure 2-1:

SWL: still water level.

h: water depth, measured from the floor to SWL.

H: wave height, measured from the trough to the crest.

λ: wave length, measured from crest to crest.

η: vertical free-surface displacement, measured from the SWL. This parameter is a

function of x and t.

c: wave celerity (phase velocity).

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Figure 2-1. Notation for the linear wave analysis [98].

The conservation of mass theorem is expressed by the equation of continuity, whose

differential form is given by

− ∂ρ

∂t= ∇ · (ρV) , (2–1)

where the del operator is given in Cartesian coordinates by

∇ =∂

∂xi +

∂yj +

∂zk, (2–2)

and the fluid velocity vector is given by

V = ui + vj + wk. (2–3)

The flow beneath the free surface is assumed to be irrotational, i.e. ∇× V = 0. Then,

the velocity of water particles is a conservative vector field that can be represented by a

potential function, in this case, the velocity potential φ, as follows

V = ∇φ. (2–4)

Substituting (2–4) into (2–1), and assuming a steady and incompressible flow, gives

∇2φ = 0. (2–5)

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Equation (2–5) is an elliptic partial differential equation (Laplace’s equation),

that can be solved, subject to a set of boundary conditions, to determine the velocity

potential φ. The boundary conditions are given by:

Kinematic free-surface condition: the velocity of a particle on the free surface must

equal the velocity of the free surface itself.

V|z=η ≈ ∂η

∂tk ≈ ∂φ

∂z

z=0

k. (2–6)

Sea-floor condition: adjacent particles to the sea floor can not cross the solid

boundary.

V · N|z=−h =∂φ

∂z

z=−h

= 0. (2–7)

Dynamic free-surface condition: the pressure on the free surface is zero.

η = −1

g

∂φ

∂t

z=η

. (2–8)

Combining (2–6) and (2–8), and eliminating η yields the linearized free-surface

boundary condition, which is given by

{

1

g

∂2φ

∂t2+∂φ

∂z

}∣

z=η≈0

= 0. (2–9)

The solution of (2–5) can be found by separation of variables for a traveling wave in

the form

φ = X(x± ct)Z(z) = X(ξ)Z(z). (2–10)

Substituting (2–10) into (2–5) yields

1

X

d2X(ξ)

dξ2= − 1

Z

d2Z(z)

dz2= −k2, (2–11)

where k is a constant.

The general solution of the two ordinary differential equations is given by

X(ξ) = Cξ sin(kξ + α), (2–12)

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Z(z) = Cz cosh(kz + β), (2–13)

where Cξ, Cz, α and β are arbitrary constants.

Since the origin of the x (and ξ) coordinate is arbitrary, α can be assigned a zero

value without loss of generality. Therefore, (2–12) becomes

X(ξ) = Cξ sin(kξ). (2–14)

Applying the sea-floor boundary condition (2–7) to (2–13), we get β = kh, which gives

Z(z) = Cz cosh[k(z + h)]. (2–15)

Substituing (2–14) and (2–15) back into (2–10) yields

φ = Cφ cosh[k(z + h)] sin(kξ), (2–16)

where Cφ = CξCz.

Now, using the linearized free-surface boundary condition (2–9), Cφ can be removed

from (2–16). Hence, the velocity potential for a traveling wave is given by

φ± = ±H2

g

kc

cosh[k(z + h)]

cosh(kh)sin[k(x∓ ct)], (2–17)

where the upper (+) sign in φ represents right-traveling waves, and the lower (-) sign

represents left-traveling waves.

2.2 Traveling Waves

Two-dimensional problems in wave mechanics generaly consider right-traveling

waves [70, 98, 101]. From the combitation of the linearized free-surface condition (2–9)

and the general solution for the velocity potential (2–16) (eliminating φ, and using the

definition of the horizontal coordinate ξ), it is possible to demonstrate that the free-surface

displacement caused by the wave is given by

η =H

2cos[k(x− ct)]. (2–18)

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Since the free-surface displacement from the SWL is sinusoidal in both space and

time, the maximum value for η (the crest), occurs when

k(x− ct) = 0,±2π,±4π, . . . (2–19)

For t = 0, the distance between two successive crests is the wavelength λ. Then, from

(2–19) we can compute the wave number k, as follows

k =2π

λ. (2–20)

Now, for x = 0, the time lapse between two succesive crests is the wave period T .

From (2–19)

kc =2π

T= 2πf ≡ ω, (2–21)

where f is the wave frequency in Hz and ω is the circular wave frequency in rad/s.

From (2–20) and (2–21), we can compute the celerity or phase velocity as

c =λ

T. (2–22)

The velocity potential can be written in terms of the circular wave frequency as

φ =H

2

g

ω

cosh[k(z + h)]

cosh(kh)sin(kx− ωt). (2–23)

Eliminating the velocity potential from (2–9) and (2–23), the circular wave frequency

can be computed as

ω =√

gk tanh(kh). (2–24)

Combining (2–20) and (2–24), results in an expression for the wave length given by

λ =2π

k=

2πg

ω2tanh(kh) =

gT 2

2πtanh

(

2πh

λ

)

= cT. (2–25)

Equation (2–25) is transcendental because λ can not be isolated and solved

analytically. Therefore, a numerical technique is required for its solution.

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Because of the behavior of the hyperbolic tangent (tanh(kh) → 1 as kh → ∞) in

(2–25), it is a common practice in ocean engineering to divide the infinite space of h/λ

into three regions which define the relative sea depth as follows [98]:

1. Shallow water: h/λ ≤ 1/20

2. Intermediate water: 1/20 ≤ h/λ ≤ 1/2

3. Deep water: h/λ ≥ 1/2

As a result, approximations are used in the computation of the wave length for

shallow and deep water conditions, because the difference between the values of kh and

tanh(kh) is about 3% or less for h/λ ≤ 1/20, whereas for h/λ ≥ 1/2 the difference between

tanh(kh) and unity is less than 0.4% [98].

The deep-water approximation of (2–25) is given by

λ ≡ λ0 ≈gT 2

2π≈ c0T, (2–26)

where the subscript 0 is used to identify the deep-water properties.

The shallow-water approximation of (2–25) is given by

λ ≈ gT 2

2πkh =

gT 2

2πh

λ=gT 2h

λ≈ cT, (2–27)

then

λ =√

ghT ≈ cT. (2–28)

The result in (2–26) shows that the deep-water wavelength and celerity are functions

of the wave period only. On the other hand, the result in (2–28) shows that the shallow-water

wavelength is a function of both depth and period, and that the celerity is a function of

depth and independent of period. Consequently, we see that waves shorten and slow down

as they approach the shoreline.

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2.3 Water Particle Motions

The Cartesian velocity components in a two-dimensional irrotational flow are given, in

terms of the velocity potential, by the Cauchy-Riemann equations

u =∂φ

∂x=∂ψ

∂z, (2–29)

w =∂φ

∂z= −∂ψ

∂x, (2–30)

where the scalar function ψ is called the stream function.

Then, the velocity components in traveling waves can be computed substituting

(2–23) into (2–29) and (2–30), which yields

u =Hω cosh[k(z + h)]

2 sinh(kh)cos(kx− ωt), (2–31)

w =Hω cosh[k(z + h)]

2 sinh(kh)sin(kx− ωt). (2–32)

The horizontal and vertical displacements (ξ, ζ) of a particle about a fixed mean point

(xo, zo), are found substituting (x, y) by (xo + ξ, zo + ζ), expanding the results in Maclaurin

series in ξ and ζ, and finally, integrating the Cartesian velocity components (2–31) and

(2–32) over time.

The result expressions are, to the first order, given by

ξ =

udt|xo,zo= −H cosh[k(zo + h)]

2 sinh(kh)sin(kxo − ωt), (2–33)

ζ =

wdt|xo,zo=H sinh[k(zo + h)]

2 sinh(kh)cos(kxo − ωt). (2–34)

Then, the position of a particle measured from the mean position (xo, zo) is given by

the position vector

r = ξi + ζk. (2–35)

Substituting (2–33) and (2–34) into (2–35) yields

r =H/2

sinh(kh){− cosh[k(zo + h)] sin(kxo − ωt)i + sinh[k(zo + h)] cos(kxo − ωt)k} . (2–36)

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Figure 2-2 shows the particle paths predicted by by Airy’s linear wave theory, using

appropriate approximations for the hyperbolic functions in (2–36).

A Deep water. B Intermediate water. C Shallow water.

Figure 2-2. Particle paths predicted by Airy’s linear wave theory [98].

2.4 Wave Energy and Power

The mass of an element displaced above the SWL, Figure 2-3, is given by

δm = ρη(δx)b, (2–37)

where b is the width of the wave crest.

Figure 2-3. Notation for the wave energy analysis [98].

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The center of mass is located at a distance η/2 above the SWL. So, the potential

energy of the element is given by

δEp = g(δm)η

2=

1

2ρgη2(δx)b. (2–38)

The total potential energy of the elements above the SWL is given by

Ep =ρgH2

8b

∫ λ

0

cos2(kx− ωt)dx =ρgH2λb

16. (2–39)

The kinetic energy of a submerged element is given by

δEk =1

2ρ(u2 + w2)bδxδz, (2–40)

where (u,w) are the particle Cartesian velocity components given by (2–31) and (2–32).

The total kinetic energy of the submerged elements is given by

Ek =1

2ρb

∫ 0

−h

∫ λ

0

(u2 + w2)dxdz =ρgH2λb

16. (2–41)

Finally, the total energy of a linear wave, which is equally divided between potential

and kinetic energy, is given by

E = Ep + Ek =ρgH2λb

8. (2–42)

Substituting (2–26) and (2–28) into (2–42) results into approximations for deep- and

shallow-water, which are respectively given by

E0 =ρg2H2T 2b

16π, (2–43)

E =ρg3/2H2h1/2Tb

8. (2–44)

The time-rate of change of energy transmission per unit area normal to the

flow direction, i.e. the energy flux, can be computed by using the equation of energy

conservation for an irrotational flow, i.e. a simplified form of Bernoulli’s equation. The

following assumptions were made to use the simplified expression: the pressure at the

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free surface is zero, and the kinetic energy term (ρV 2/2) is negligible for waves with small

steepness (H/λ << 1). The simplified Bernoulli’s equation is given by

ρ∂φ

∂t+ ρgz + p = 0. (2–45)

The only time-dependent part in (2–45) is the first term, that represents both the

unsteady kinetic energy and the dynamic pressure. Therefore, the energy flux is given by

the product of the dynamic pressure and the fluid veloctiy, as follows

ρ∂φ

∂tV = ρ

∂φ

∂t∇φ. (2–46)

The total energy flux can be computed substituting (2–23) into (2–46) and integrating

over both the normal area (bh) and the wave period (T ). The resulting expression is

considered the wave power [98], and is given by

P = ρb1

T

∫ T

0

∫ 0

−h

∂φ

∂t∇φdzdt =

ρgH2cb

16

[

2kh

sinh(2kh)+ 1

]

i. (2–47)

Deep- and shallow-water approximations are respectively given by

P0 =ρg2H2Tb

32πi, (2–48)

P =ρg3/2H2h1/2b

8i. (2–49)

2.5 Wave Mechanics Numerical Example

Let us suppose that a wave is traveling in water that is 10 m deep (h = 10 m).

Measurements indicate that the wave has a period of 3 seconds (T = 3 s) and an

amplitude of 2 meters (H = 2 m).

2.5.1 Kinematic Properties

Iteratively solving Equation (2–25) yields

λ = 14.0367 m.

Then, equations (2–20), (2–22) and (2–21), can be used to compute the other

kinematics properties of the wave, which gives

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k = 0.4476 rad/m,

c = 4.6789 m/s,

ω = 2.0944 rad/s.

The ratio h/λ = 0.7124, indicates that we have deep water conditions.

2.5.2 Water Particles Motion

The wave can be represented graphically using Equation (2–36). Figure 2-4 shows

a discrete plot of water particles for the given wave at a particular instant of time.

The small closed path is described by the motion of one surface particle. As predicted

by Airy’s wave theory, for deep water conditions such path is circular (compare to

Figure 2-2A).

0 5 10 15 20 25 30

−10

−5

0

Distance, x (m)

Dep

th,z

(m)

Figure 2-4. Example water particles motion.

2.5.3 Wave Energy

For the given wave, the total energy and power per unit of wave front, i.e. b = 1 m,

can be computed using equations (2–43) and (2–48). Substituting the corresponding values

in such equations yields

E = 70.8471 kJ,

P = 11.8078i kW.

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2.6 Wave-Structure Interaction

2.6.1 Heaving and Pitching Body Motions

The motion of a rigid body in the three-dimensional space is characterized by six

components corresponding to six degrees of freedom (6-dof). In ocean engineering it is

common to define such motions as depicted in Figure 2-5 and named as follows:

1. Surge: displacement along x axis.

2. Sway: displacement along y axis.

3. Heave: displacement along z axis.

4. Roll: rotation about x axis.

5. Pitch: rotation about y axis.

6. Yaw: rotation about z axis.

For an axisymmetric (or another not-elongated) body, e.g. an sphere, the numbers 1

and 2 (and 4 and 5) are ambiguous (i.e. they can be arbitrarily interchanged). However,

this ambiguity is removed by defining the x direction as the wave propagation direction.

Figure 2-5. Rigid body with six degrees of freedom.

Since this work considers a two-dimensional linear model for ocean waves, only three

degrees of freedom (3-dof) are of interest. The motion is analyzed in the x − z plane,

hence, only surge, heave and pitch motions are considered. Figure 2-6 shows two of such

configurations in which a floating body can be excited by ocean waves.

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A Purely heaving float. B Purely pitching float.

Figure 2-6. Floating bodies undergoing heaving or pitching motion [70].

Assuming a sinusoidal wave profile, we can see that when λ = L, no heaving motion

will occur since a crest and a trough of a wave act simultaneously over the body as in

Figure 2-7B. Therefore, there is not vertical force acting on the float and no heaving

motions when

L = Nλ, N = 1, 2, 3, · · · (2–50)

Conversely, when an extra crest (or trough) act over the body, there is a net vertical

force that creates heaving motions. Heaving can be expected when

L =Nλ

2, N = 1, 3, 5, · · · (2–51)

The body depicted in Figure 2-6B is allowed to rotate (pitch) about its center of

gravity. A minimum pitching moment is experienced by the body under the condition

described by (2–51) when N = 3. On the other hand, a maximum pitching moment occurs

when 2–50 is satisfied.

A Pure heaving condition. B Pure pitching condition.

Figure 2-7. Floating bodies: pure heaving and pitching conditions [70].

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2.6.2 Heaving Equation of Motion

The law of conservation of linear momentum states that the rate of change of the

linear momentum of the system in an inertial reference frame, is equal to the total

external force acting on the system. For a purely heaving floating body the equation of

motion is given by [98]

md2z

dt2= − awz

d2z

dt2− brz

dz

dt− bvz

(

dz

dt

) ∣

(

dz

dt

)∣

N

− bpzdz

dt− ρgAwpz −Nksz + Fzo cos(ωt+ αz).

(2–52)

McCormick [98] defines each term in the right hand side of (2–52) as follows:

1. Inertial reaction force of the water, where awz is the added mass.

2. Radiation damping force, where brz is the damping coefficient.

3. Viscous damping force, where bvz is the viscous damping coefficient.

4. Damping due to power take off, where bpz is the power take-off coefficient.

5. Hydrostatic restoring force, where Awp is the waterplane area when the body is atrest.

6. Mooring restoring force, where ks is the effective mooring spring constant of eachline, and N is the number of lines.

7. Wave induced vertical force, where Fzo is the force amplitude, ω = 2π/T is thecircular wave frequency (T is the wave period), and αz is the phase angle betweenthe wave and the wave-induced force.

The power N on the viscous damping term depends on the flow regime, N = 0 for

laminar flow and N = 1 for turbulent flow. When N = 1 the equation of motion is

nonlinear. In this work, we assume that the flow is laminar and N = 0. Therefore, bvz is

replaced by a linear damping coefficient bvz. Reorganizing terms in (2–52), the linearized

equation of motion is given by

(m+ awz)d2z

dt2+ (brz + bvz + bpz)

dz

dt+ (ρgAwp +Nks)z = Fzo cos(ωt+ αz). (2–53)

ρ is the density of seawater (1030 kg/m3), g is the acceleration due to gravity (9.8 m/s2).

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2.6.2.1 Mass and Added Mass

The mass of a float must be equal to the mass of displaced water. Hence, the mass for

a rectangular floating body can be computed as

m = ρdAwp, (2–54)

where the waterplane area is given by

Awp = LB. (2–55)

The added mass is the inertia added to a system due to the presence of a structure in

a moving fluid or due to the motion of a structure in a stationary fluid. The magnitude of

such mass is proportional to the inertial reaction force on the body [98]. For rectangular

solids such the ones shown in Figure 2-6, the added-mass and the added-mass moment of

inertia are given respectively by [70]

awz =KmπρLB

2

4, (2–56)

Aw =KIπρL

4B

16. (2–57)

The values for the coefficients Km and KI can be found graphically from Figure 2-8.

0 5 10 15 200.5

0.75

1

Km

B/d

A Added mass coefficient.

2 4 6 8 100.05

0.075

0.1

0.15

KI

L/d

B Added-mass moment of inertia coefficient.

Figure 2-8. Added mass and added-mass moment of inertia coefficients for a rectangularbody [70].

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2.6.2.2 Radiation and Viscous Damping

Due to body motions near to the fluid free surface, waves are also created. Such

waves take energy away from the body. This energy loss is called radiation damping. For

rectangular solids such the ones shown in Figure 2-6, the radiation damping coefficient is

given by [98]

brz = b′

rL =ρg2

ω3R2

ZL, (2–58)

where b′

r is the radiation damping coefficient per unit length, and RZ is the ratio of the

radiated-wave amplitude and the body motion amplitude, and is given by

RZ = 2e−ω2

gd sin

(

w2

g

B

2

)

. (2–59)

Both the added mass and the radiation damping coefficients vary with frequency.

However, McCormick [98] states that a frequency-invariant value for the added mass given

by (2–56) and the expression for the radiation damping coefficient given in (2–58) match

measurements done by Vugts [102] for a body with a rectangular section. Figure 2-9 shows

the variation of radiation damping coefficient for a heaving rectangular section when the

draft is the half of the length, i.e. d = L/2.

0 0.5 1 1.50

1

brz

(ρd√

2Lg)

ω

L

2g

Figure 2-9. Non-dimensional radiation damping coefficient for a heaving rectangularsection.

The nonlinear viscous damping coefficient in (2–52) is given by

bvz ≈1

2ρCdAd, (2–60)

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where Ad is the projected area, i.e. Awp for a rectangular body, and Cd is the drag

coefficient. For a rectangular body in heaving motion in laminar flow, the drag coefficient

is Cd = 1.2 [103].

McCormick [98] states that the nonlinear and the linear viscous damping coefficients

in (2–52) and (2–53) are related by the following expression

bvz =8

3

ω

πZobvz, (2–61)

where Zo is the heaving amplitude which is computed as in Section 2.6.4. Since Zo

depends on bvz, a nonlinear equation must be solved for Zo to compute the linear viscous

damping coefficient.

2.6.3 Wave-Induced Forces

The wave-induced heaving force on a rectangular float in a linear wave is given by [70]

Fz(t) = Fzo cos(ωt), (2–62)

where

Fzo =ρgHBλ

(

e−2πdλ + 1

)

sin

(

πL

λ

)

. (2–63)

The wave-induced moment on a rectangular float (assuming the draft d to be

constant) in a linear wave is given by [70]

Mθ(t) = Mθo sin(ωt), (2–64)

where

Mθo =ρgHBλ

(

e−2πdλ + 1

)

[

λ

πsin

(

πL

λ

)

− L cos

(

πL

λ

)]

. (2–65)

The phase angle between the wave and the wave-induced force/moment, αz, is equal

to zero (αz = 0) for a body that is symmetric about the x− z and y − z planes [70].

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2.6.4 Steady State Solution of the Heaving Equation

Equation (2–53) is a second-order ordinary differential equation whose steady-state

solution can be found easily and is given by

zss(t) = Zo cos(ωt+ αz − εz), (2–66)

where

Zo =

Fzo

(ρgAwp +Nks)√

(

1 − ω2

ω2n

)2

+

[

ωn

(brz + bvz + bpz)

bcz

]2cos (ωt+ αz − εz) . (2–67)

In (2–66) the natural heaving frequency is given by

wnz =2π

Tnz

=

ρgAwp +Nks

m+ awz

, (2–68)

where Tnz is the natural heaving period; the critical damping coefficient is given by

bcz = 2√

(m+ awz)(ρgAwp +Nks); (2–69)

and the phase angle between the force and motion is given by

εz = arctan

[

ωn

(brz + bvz + bpz)

bcz

]

(

1 − ω2

ω2n

)

. (2–70)

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CHAPTER 3TENSEGRITY MECHANISM

Salter et al. [104] stated that most wave energy harvesters must have, among others,

the following subsystems:

• Slow primary displacing element, such as a float or buoy.

• Connecting linkage to transmit the wave-generated forces (analyzed in this work).

• Electrical generators, electrical network, transformers and switchgear.

3.1 Morphology Definition

The proposed tensegrity mechanism is based on the two-dimensional “X-frame”

morphology proposed by Kenneth Snelson in [31], Figure 1-3A. The mechanism comprises

four members in tension and two members in compression. The members in compression

can be replaced by two bars connected by prismatic joints which represent the electrical

generators. Two of the ties have a very high modulus of elasticity (the mechanism base

and the element excited by ocean waves) with respect to the other two ties. Therefore,

the deformations of the base and the buoyant element are negligible and the lateral ties

are the two deformable members under tension that are necessary to keep the tensegrity

configuration. Figure 3-1 depicts the concept of a tensegrity-based wave energy harvester.

Figure 3-1. Concept of a wave energy harvester based on tensegrity systems.

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The kinematic diagram of the proposed tensegrity mechanism is shown in Figures

3-2 and 3-3. The mechanism parameters for the selected kinematic chain are listed in

Table 3-1.

0 1

1 2

2 3

3 4

4 5

5 6

Figure 3-2. Kinematic diagram of the mechanism.

Table 3-1. Mechanism parameters for kinematic chain.

Link length, m Twist angle, deg Joint offset, m Joint angle, dega1 = 0 α1 = 90 0S1 = 0 0θ1 = variablea2 = 0 α2 = 90 1S2 = variable 1θ2 = 180a3 = L α3 = 0 2S3 = 0 2θ3 = variablea4 = 0 α4 = 90 3S4 = 0 3θ4 = variablea5 = 0 α5 = 90 4S5 = variable 4θ5 = 180a6 = L0 α6 = 0 5S6 = 0 5θ6 = variable

3.2 Position Analysis

3.2.1 Forward Position Analysis

The forward position analysis allows one to determine the position and orientation of

one of the links for a specified set of joint variables. The problem is stated as follows:

• Given: the constant mechanism parameters a3, a6 and Lpxz (position of point p onthe top platform); and the set of joint variables, 1S2, 4S5 and 0θ1.

• Find: the position and the orientation of the top platform, xm, zm and φ.

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��

��

��

��

��

��

��

��

�����

��

������

��

Figure 3-3. Vector diagram of the mechanism.

Let us define the following vectors

S2 = 1S2 cos (0θ1)i + 1S2 sin (0θ1)k, (3–1)

a6 = a6i. (3–2)

From Figure 3-3, the following vector loop equation can be written

LB = S2 − a6. (3–3)

Equation (3–3) permits to evaluate LB and θB. The angle δ3 can be computed using

the cosine law

δ3 = arccos

(

L2B + 4S

25 − a2

3

2LB4S5

)

. (3–4)

Hence,

5θ6 = θB + δ3 + π. (3–5)

Then, the vector S5 is given by

S5 = 4S5 cos (5θ6)i + 4S5 sin (5θ6)k. (3–6)

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From Figure 3-3, other two vector loop equations can be written as

LA = a6 − S5, (3–7)

a3 = LA − S2. (3–8)

Equation (3–8) permits to evaluate the orientation φ. There are two solutions for δ3,

however, only the one in the first quadrant is taken for this mechanism’s configuration.

Finally, the position of the point p = [ xm 0 zm ]T can be computed as

p = S2 +Lpxz

La3. (3–9)

The length of the springs denoted by vectors LA and LB can be computed in terms of

the position and orientation (φ = θ + π) of the top platform, when Lpxz = L/2, as follows

LA =[

(xm − L/2 cos θ)2 + (zm − L/2 sin θ)2]

1

2 , (3–10)

LB =[

(xm + L/2 cos θ − L0)2 + (zm + L/2 sin θ)2

]

1

2 . (3–11)

3.2.2 Reverse Position Analysis

The reverse position analysis allows one to determine the position and orientation of

one of the links for a specified set of joint variables. The problem is stated as follows:

• Given: the constant mechanism parameters a3, a6 and Lpxz; and the position and theorientation of the top platform, xm, zm and φ.

• Find: the set of joint variables, 1S2, 4S5 and 0θ1.

Let us define the following vector

a3 = a3 cos (φ)i + a3 sin (φ)k. (3–12)

From Figure 3-3, the following vector loop equations can be written

S2 = p − Lpxza3, (3–13)

LA = S2 + a3, (3–14)

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S5 = a6 − LA. (3–15)

Equation (3–13) permits to evaluate 1S2 and 0θ1, and (3–15) permits to evaluate 4S5.

3.2.3 Numerical Example

Let the constant mechanism parameters be L = 3 m, L0 = 4.5 m and Lpxz = 1.5

m. To verify the position analysis, a desired path can be defined in the Cartesian space.

Then, the values of the joint variables that satisfy the path can be found using the reverse

kinematics. Finally, the forward kinematics can be used to compute the points in the

Cartesian space that are generated with each set of joint variables. Figure 3-4 shows the

mechanism in the final position and the path. Table 3-2 shows the numerical results which

indicate that the reverse and forward kinematics functions work as expected.

−1 0 1 2 3 4 5 6

0

1

2

3

4

5

6

Position in x (m)

Position

inz

(m)

Figure 3-4. Position analysis numerical example.

Table 3-2. Position analysis numerical example results.

Original path Reverse kinematics Forward kinematicsxmd (m) zmd (m) φd (deg) 1S2 (m) 4S5 (m) 0θ1 (deg) xm (m) zm (m) φ (deg)

1.50 2.00 170 3.4482 5.0155 30.2969 1.5000 2.0000 170.00001.75 2.25 175 3.8751 4.8664 33.1537 1.7500 2.2500 175.00002.00 2.50 180 4.3012 4.7170 35.5377 2.0000 2.5000 180.00002.25 2.75 185 4.7242 4.5695 37.5735 2.2500 2.7500 185.00002.50 3.00 190 5.1428 4.4267 39.3445 2.5000 3.0000 190.0000

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3.3 Velocity Analysis

The velocity state is defined as a set of parameters from which the velocity of any

body/point of the linkage can be determined relative to a reference body [105]. Then,

using this concept, the velocity analysis allows one to obtain the relationships between the

velocity of any body/point of the mechanism and the velocities of the joint variables. Rico

et al. [106] and Crane et al. [105] presented the concept of velocity state using the theory

of screws, developed by Sir Robert Stawell Ball [107].

Since the position analysis is complete, the directions of the unit vectors isi+1 along

each axis as well the coordinates of one point ri on each joint axis are known. Then,

Plucker coordinates of the lines along the revolute joint axes are given by

{isi+1; isi+1OL} = {isi+1; ri × isi+1}. (3–16)

The coordinates of the line at infinity associated with the prismatic joints are given

by

{isi+1; isi+1OL} = {0; ri × isi+1}. (3–17)

Then, using (3–16) and (3–17), the Plucker coordinates of the lines along the joint

axes are given by

0$1 = {0s1; 0s1OL} = {s1;0 × s1}, (3–18)

1$2 = {0; 1s2OL} = {0; s2}, (3–19)

2$3 = {2s3; 2s3OL} = {s3; S2 × s3}, (3–20)

3$4 = {3s4; 3s4OL} = {s4; LA × s4}, (3–21)

4$5 = {0; 4s5OL} = {0; s5}, (3–22)

5$6 = {5s6; 5s6OL} = {s6; a6 × s6}. (3–23)

All the unit vectors in (3–18) to (3–23) are known from the position analysis and are

given by:

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s1 = s3 = s4 = s6 = [ 0 −1 0 ]T ,

s2 =S2

|S2|,

s5 =S5

|S5|.

Since the mechanism is a closed-loop kinematic chain, bodies 0 and 6 are the same

(i.e. the ground of the mechanism).

3.3.1 Forward Velocity Analysis

The forward velocity analysis allows one to determine the velocity state of one of the

links for a given set of joint rates. The problem is stated as follows:

• Given: the constant mechanism parameters a3, a6 and Lpxz; the set of joint variables,

1S2, 4S5 and 0θ1; and the set of velocities of the joint variables 1v2, 4v5 and 0ω1.

• Find: the velocity state of the top platform[

0ω3 0v3O

]Tand xm, zm and φ.

The velocity for the closed kinematic chain can be written in screw form as follows,

[105, 106]:

0ω10$1 +1 v2

1$2 +2 ω32$3 +3 ω4

3$4 +4 v54$5 +5 ω6

5$6 = 0. (3–24)

Substituting (3–18) to (3–23) into (3–24) yields

0ω1

0

−1

0

0

0

0

+ 1v2

0

0

0

s2x

0

s2z

+ 2ω3

0

−1

0

s2z

0

−s2x

+ 3ω4

0

−1

0

LAz

0

−LAx

+ 4v5

0

0

0

s5x

0

s5z

+ 5ω6

0

−1

0

0

0

−a6x

= 0

(3–25)

Equation (3–25) can be written as a 3x3 system in matrix form as follows

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−1 −1 −1

s2zLAz

0

−s2x−LAx

−a6x

2ω3

3ω4

5ω6

= −0ω1

−1

0

0

− 1v2

0

s2x

s2z

− 4v5

0

s5x

s5z

(3–26)

The solution of (3–26) gives the magnitudes of the angular velocities between

consecutive bodies. Then, the velocity state of the top platform can be computed as

0ω3

0v3O

=0 ω1

0$1 +1 v21$2 +2 ω3

2$3. (3–27)

Now the velocity of any point p on the top platform, whose position is represented by

rO→P , is given in terms of the velocity state by

0v3p = 0v3

O + 0ω3 × rO→P . (3–28)

Equations (3–26), (3–27) and (3–28) complete the forward velocity analysis and allows

one to compute the velocity of any point in the top platform of the mechanism for a given

set of velocities of the joint variables.

3.3.2 Reverse Velocity Analysis

The reverse velocity analysis allows one to determine the set of joint rates for a given

velocity state of one of the links. The problem is stated as follows:

• Given: the constant mechanism parameters a3, a6 and Lpxz; the set of joint variables,

1S2, 4S5 and 0θ1; and the velocity state of the top platform[

0ω3 0v3O

]Tin terms

of xm, zm and φ.

• Find: the set of velocities of the joint variables 1v2, 4v5 and 0ω1.

Since the the velocity of the point p (0v3p = xmi + zmk), and the angular velocity of

the top platform (0ω3 = φj) are known, the element associated with linear velocities in the

velocity state can be computed using (3–28) as

0v3O = 0v3

p − 0ω3 × rO→P . (3–29)

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Equation (3–27) defines the velocity state of the top platform. Substituting (3–27)

into (3–24) yields

0ω3

0v3O

= −3ω4

3$4 −4 v54$5 −5 ω0

5$0. (3–30)

Since the velocity state of the top platform is known, the joint velocities of the

mechanism can be computed from (3–27) and (3–30) as follows

−1 0 −1

0 s2xs2z

0 −s2z−s2x

0ω1

1v2

2ω3

=

0ω3

0v3x

0v3z

, (3–31)

−1 0 −1

LAzs5x

0

−LAxs5z

0

3ω4

4v5

5ω6

= −

0ω3

0v3x

0v3z

. (3–32)

Equations (3–31) and (3–32) complete the reverse velocity analysis and allows one

to compute the velocities of the joint variables (and all the joint velocities) for a given

velocity state of the top platform.

3.3.3 Numerical Example

Let the constant mechanism parameters be L = 3 m, L0 = 4.5 m and Lpxz = 1.5 m.

Then, we define a circular path in the Cartesian space, centered in the point (xm, zm) =

2.5i + 3k with a radius of 0.5 meters, Fig 3-5A. We want the mechanism to follow such

path in 5 seconds with constant celerity and fixed orientation (φ = 190 deg). Fig 3-5B

shows the corresponding desired position and velocity of the point p (centered in the top

platform of the mechanism), which are computed using the following parametric equations

(parameter t0) of the circle

(xm, zm) = [x0 + r cos(t0)]i + [z0 + r sin(t0)]k. (3–33)

The velocity of p can be computed using the derivative with respect to the time of (3–33).

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Finally, the reverse position and the reverse velocity analysis equations can be used

to compute the corresponding values of the joint variables that would make the point p

follow the described Cartesian path.

Figure 3-6 shows the results with the joint variables values and their corresponding

velocities.

−1 0 1 2 3 4 5 6

0

1

2

3

4

5

6

Position in x (m)

Pos

itio

nin

z(m

)

A Mechanism and Cartesian path.

0 1 2 3 4 50

2

4

Time (s)

Position

(m)

xz

0 1 2 3 4 5−1

0

1

Time (s)

Vel

oci

ty(m

/s)

xz

B Position and velocity of point p.

Figure 3-5. Velocity analysis numerical example.

0 1 2 3 4 53.5

4

4.5

5

5.5

Time (s)

Posi

tion

(m)

1S 2

4S 5

0 1 2 3 4 5−2

−1

0

1

Time (s)

Vel

oci

ty(m

/s)

1v2

4v5

A Position and velocity for 1S2, 4S5.

0 1 2 3 4 535

40

45

50

Time (s)

0θ1

(deg

)

0 1 2 3 4 5−0.2

0

0.2

Time (s)

1(r

ad/s)

B Position and velocity for 0θ1.

Figure 3-6. Velocity analysis numerical example results.

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3.4 Equation of Motion

The differential equation of motion can be obtained using the Lagrangian approach.

This equation represents the dynamic behavior of the mechanism, and is given, in terms of

the generalized coordinates and its derivatives (q, q, q), by

M(q)q + N (q, q) + G(q) = Q, (3–34)

where:

M(q) is defined as the inertia matrix,

N (q, q) = V (q, q) + F (q) accounts for Coriolis/centripetal effects and friction,

G(q) is called the gravity vector, and

Q is the generalized force vector.

The Lagrange’s equation of motion is given, in terms of the generalized terms, by

[108, 109]

d

dt

∂EK

∂q− ∂EK

∂q+∂EP

∂q= Q, (3–35)

where:

EK is the kinetic energy,

EP is the potential energy,

Q is the generalized force vector,

q is the vector of generalized coordinates,

q is the vector of generalized coordinates derivatives (velocities).

3.4.1 Assumptions

The following assumptions are made for the tensegrity mechanism

• The links of the mechanism, except for the top platform, are massless. It is assumedthat they can be designed to have neutral buoyancy.

• The elastic ties are massless.

• The stiffness of each tie is constant, i.e. they behave as linear springs.

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• The vector of generalized coordinates is defined as

q =

q1q2q3

=

xm

zm

θ

. (3–36)

3.4.2 Kinetic Energy

Since the links of the mechanism are considered massless, the kinetic energy of the

mechanism is all concentrated at the top platform. The kinetic energy of the top platform

due to surge, heave and pitch motions is given, in terms of the generalized coordinates, by

EK =1

2(m+ awx) q1

2 +1

2(m+ awz) q2

2 +1

2(Iy + Aw) q3

2, (3–37)

where m is the mass, Iy = m(L2 + Z2)/12 is the mass moment of inertia, awx = 1/4ρπd2B

and awz are the added masses due to surging and heaving, and Aw is the added-mass

moment of inertia due to pitching.

The first and term of (3–35) is obtained by taking the derivative of (3–37) with

respect to the generalized coordinates as

∂EK

∂q=

(m+ awx) q1

(m+ awz) q2

(Iy + Aw) q3

, (3–38)

and then, taking the derivative of (3–38) with respect to the time gives

d

dt

∂EK

∂q=

(m+ awx) q1

(m+ awz) q2

(Iy + Aw) q3

. (3–39)

Equation (3–39) can be written in matrix form as

d

dt

∂EK

∂q= Mq =

(m+ awx) 0 0

0 (m+ awz) 0

0 0 (Iy + Aw)

q. (3–40)

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From (3–37) we see that the kinetic energy of the top platform does not depend on

the position. Hence, the second term of (3–35) is given by

∂EK

∂q= 0. (3–41)

3.4.3 Potential Energy

The potential energy due to heaving and pitching motions of the top platform are

described by McCormick [70] as

EPz =1

2ρgAwpq

22, (3–42)

EPθ =1

2Cq2

3, (3–43)

where Awp is the waterplane area and C is the restoring moment constant which is

defined, for a bottom-flat body in terms of the draft, as

C =gIyd. (3–44)

The potential energy of the elastic ties is given by

EPk =1

2kA (LA − LA0

)2 +1

2kB (LB − LB0

)2 , (3–45)

where LA0, LB0

; and kA, kB; are the free lengths and the stiffnesses of the ties respectively.

Substituting (3–10) and (3–11) into (3–45) gives

EPk =1

2kA

(

[

(q1 − L/2 cos q3)2 + (q2 − L/2 sin q3)

2]

1

2 − LA0

)2

+1

2kB

(

[

(q1 + L/2 cos q3 − L0)2 + (q2 + L/2 sin q3)

2]

1

2 − LB0

)2

.

(3–46)

The total potential energy of the mechanism, EP = EPz + EPθ + EPk, is given by

EP =1

2ρgAwpq

22 +

1

2Cq2

3

+1

2kA

(

[

(q1 − L/2 cos q3)2 + (q2 − L/2 sin q3)

2]

1

2 − LA0

)2

+1

2kB

(

[

(q1 + L/2 cos q3 − L0)2 + (q2 + L/2 sin q3)

2]

1

2 − LB0

)2

.

(3–47)

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The last term of (3–35) is computed taking the derivative of (3–47) with respect to

each generalized coordinate as follows:

∂EP

∂q1= kA

(

[

(q1 − L/2 cos q3)2 + (q2 − L/2 sin q3)

2]

1

2 − LA0

)

· (q1 − L/2 cos q3)[

(q1 − L/2 cos q3)2 + (q2 − L/2 sin q3)

2]

1

2

+ kB

(

[

(q1 + L/2 cos q3 − L0)2 + (q2 + L/2 sin q3)

2]

1

2 − LB0

)

· (q1 + L/2 cos q3 − L0)[

(q1 + L/2 cos q3 − L0)2 + (q2 + L/2 sin q3)

2]

1

2

,

(3–48)

∂EP

∂q2= ρgAwpq2

+ kA

(

[

(q1 − L/2 cos q3)2 + (q2 − L/2 sin q3)

2]

1

2 − LA0

)

· (q2 − L/2 sin q3)[

(q1 − L/2 cos q3)2 + (q2 − L/2 sin q3)

2]

1

2

+ kB

(

[

(q1 + L/2 cos q3 − L0)2 + (q2 + L/2 sin q3)

2]

1

2 − LB0

)

· (q2 + L/2 sin q3)[

(q1 + L/2 cos q3 − L0)2 + (q2 + L/2 sin q3)

2]

1

2

,

(3–49)

∂EP

∂q3= Cq3

+ kA

(

[

(q1 − L/2 cos q3)2 + (q2 − L/2 sin q3)

2]

1

2 − LA0

)

· [(q1 − L/2 cos q3)L/2 sin q3 − (q2 − L/2 sin q3)L/2 cos q3][

(q1 − L/2 cos q3)2 + (q2 − L/2 sin q3)

2]

1

2

+ kB

(

[

(q1 + L/2 cos q3 − L0)2 + (q2 + L/2 sin q3)

2]

1

2 − LB0

)

· [− (q1 + L/2 cos q3 − L0)L/2 sin q3 + (q2 + L/2 sin q3)L/2 cos q3][

(q1 + L/2 cos q3 − L0)2 + (q2 + L/2 sin q3)

2]

1

2

.

(3–50)

Equations (3–48), (3–49) and (3–50) can be written in matrix form as

∂EP

∂q= G(q) =

[

∂EP

∂q1

∂EP

∂q2

∂EP

∂q3

]T

. (3–51)

Equations (3–40), (3–41) and (3–51) represent the first and third terms of (3–34).

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3.4.4 Friction Vector

As described in Section (2.6.2.2), the most important characteristic in the fluid-structure

interaction phenomenon is the presence of damping due to viscous effects and radiation of

waves. Viscous damping is considered in both surging and heaving motions, and radiation

damping is considered for heaving and pitching motions. The friction vector is then given

by

F (q) =

bvxq1

(brz + bvz)q2

brθq3

, (3–52)

where the damping coefficients in the heave/surge directions are given by (2–58) and

(2–61), and the radiation damping coefficient due to pitching motion is given by

brθ = b′

r

L3

12, (3–53)

where b′

r is the radiation damping coefficient per unit length given in (2–58).

3.4.5 Generalized Forces

The generalized force vector is formed by the wave-induced forces that act over the

generalized coordinates. Since the generalized coordinates were chosen to describe directly

the motion of the float, the generalized force vector is given by

Q(t) =

0

Fzo cos(ωt)

Mθo sin(ωt)

. (3–54)

The complete equation of motion is then given by

m+ awx 0 0

0 m+ awz 0

0 0 Iy + Aw

q +

bvxq1

(brz + bvz)q2

brθq3

+

∂EP

∂q1∂EP

∂q2∂EP

∂q3

=

0

Fzo cos(ωt)

Mθo sin(ωt)

.

(3–55)

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CHAPTER 4OCEAN WAVE ENERGY HARVESTING

4.1 Electrical Generators for Wave Energy Harvesting

Several works have been done with electrical generators for wave energy harvesting.

Baker and Muller [110] and Muller [111] investigated the concept of direct drive wave

energy converters. Salter et al. [104] described a range of different control strategies

for wave energy power conversion mechanisms. Danielsson [112] designed a three-phase

permanent magnet linear generator for direct coupling to a floating buoy. Baker et al.

[113] outlined the performance and modeling of a prototype linear tubular permanent

magnet machine with an air cored stator. Polinder et al. [114] described the main

characteristics of the Archimedes Wave Swing. Thorburn et al. [115] presented different

topologies for the electrical system transmitting power to the grid. Mueller and Baker

[116] investigated the issues associated with converting the energy produced by marine

renewable energy converters using direct drive electrical power take-off. Leijon et al.

[117] presented a novel approach for electric power conversion discussing also the

economical and some environmental considerations. Rhinefrank et al. [118] described

the research, design, construction and prototype testing process of a novel ocean energy

direct drive permanent magnet linear generator buoy. Danielsson [119] studied the

electromagnetic properties, built a laboratory prototype and analyzed the performance of

linear synchronous permanent magnet generators. Muller et al. [120] described different

power take off mechanisms and described how some disadvantages shown by conventional

rotary generators can be overcome with direct drive systems. Szabo et al. [121] proposed a

novel modular permanent magnet tubular linear generator, analyzed by means of numeric

field computations. Trapanese [122] performed the optimization of a permanent magnet

linear generator directly coupled to sea waves. Elwood et al. [123] developed a hybrid

numerical/physical modeling approach for the design of a 10kW energy conversion system.

Liu et al. [124] presented an analytical model for predicting the electromagnetic and

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electromechanical characteristics of a slotless tubular linear generator. Ruellan et al. [125]

presented a design methodology for the all-electric solution adapted to SEAREV. Cheng et

al. [126] presented a study of a multi-pole magnetic generator for energy harvesting at low

frequencies.

Since this research involves the first analysis of a tensegrity system for energy

harvesting under the influence of sea waves, the work is concentrated into the behavior

of the connecting linkage which transmits the wave-generated forces to the electrical

generators. Therefore, the electrical model is not included and is considered as damping

due to power take off, as suggested in [123] and described in (2–52), where bpz is the

power take-off damping coefficient. The efficiency of permanent magnet linear generators

used in ocean wave energy conversion is about 75-85%. [70, 112, 112].

4.2 Sea State Selection

Although the best wave climates are found in zones from 30 to 60 degrees latitude

as stated in Section 1.1.2, attractive wave climates are found also within ±30 degrees

latitude, where the lower power level is compensated by smaller power variability.

Additionally, there are several isolated places that can not be connected to continental

power grids in a lot of countries around the world, making ocean energy a feasible

renewable energy source. Therefore, wave energy can be especially useful for small

communities living near shore or in islands, avoiding the transportation and utilization of

fossil fuels.

Osorio et al. [127] developed a road map for harnessing marine renewable energy

for Colombia, pointing out that a profound knowledge of the available resource and

oceanographic conditions is required. In that sense, Ortega et al. [128] designed a

methodology for estimating wave power potential in places lacking instrumentation by

using reanalysis winds and wave generation models.

Ortega [129] performed a study on the exploitation of wave energy for Isla Fuerte, a

small Colombian island, located in the Caribbean Sea that does not have access to electric

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power from the national grid and generates its power using fossil fuels. The wave available

resource and its time behavior was identified using third generation wave generation

models, with bathymetries and reanalysis winds as inputs. Ortega selected a place with

coordinates 9.408◦ N and 76.180◦ W, whose depth is around thirty meters, i.e. h = 30 m.

Such place was chosen taking in account environmental issues in order to protect the coral

reef, which is found even near places with higher wave power availability, Figure 4-1.

A Isla Fuerte. Taken from Google EarthTM.

LAT

LON

25

30

35

40

45

50

45

40

35

30

25

10

5

10 15

20

10

20

15

5

-76.22 -76.21 -76.2 -76.19 -76.18 -76.17 -76.16 -76.15

9.34

9.35

9.36

9.37

9.38

9.39

9.4

9.41

9.42

9.43

B Bathymetry of Isla Fuerte [129].

Figure 4-1. Location and bathymetry of Isla Fuerte.

4.2.1 Wave Power and Wave Kinematic Properties

At the selected location the wave height and period vary from 0.2 to 1.2 meters

and from 3 to 10 seconds respectively; and the joint probability for H and T shows that

H ∈ [0.4 0.6] m and T ∈ [4 6] s [129]. Using (2–48) with h = 30 m, the available power

per meter of wave front can be computed over the range of T and H. From Figure 4-2, the

maximum available power, P = 2.125 kW/m, is found at H = 0.6 m, T = 6 s.

The wave properties for h = 30 m, H = 0.6 m, T = 6 s can be found by solving

(2–25), and substituting the result into (2–20), (2–22) and (2–21), yields

λ = 56.1081 m, k = 0.1120 rad/m, c = 9.3514 m/s, ω = 1.0472 rad/s.

The ratio h/λ = 0.5347 ≥ 1/2, indicates that we have deep water conditions.

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4

5

6

0.4

0.5

0.6

1

1.5

2

T (s)H (m)

P(k

W/m

)

Figure 4-2. Wave power variation for the sea state at 9.408◦ N, 76.180◦ W.

4.3 Direct Drive Heaving System

Several direct drive wave energy converters behave as a purely heaving body,

connected to electrical generators, see [110, 111, 117, 118, 121, 122] for reference. The

dimensions of the heaving float, as the one shown in Figure 2-6A, are L = 2 m, Z = 0.5 m,

B = 1 m, and d = 0.25 m.

The coefficients of (2–52) can be calculated using equations described in Section 2.6.2

and are listed in Table 4-1.

Table 4-1. Direct drive heaving float coefficients.

Coefficient Value Units Equationm = 515 kg (2–54)awz = 1.09×103 kg (2–56)brz = 2.04×103 N-s/m (2–58)bvz = 695.09 N-s/m (2–61)bpz = 0 N-s/m AssumedAwp = 2 m2 (2–55)N = 0 −− Assumedks = 0 N/m AssumedFzo = 1.19×104 N (2–63)αz = 0 rad Symmetric body in long waveswnz = 3.55 rad/s (2–68)

bcz = 1.14×104√

N (2–69)εz = 0.2090 rad (2–70)Zo = 0.6327 m (2–67) & (2–61)

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Figure 4-3 shows the force that the wave induces over the body, and Figure 4-4 shows

the position, velocity and instant power dissipated by the float.

0 2 4 6 8 10 12−1.5

−1

−0.5

0

0.5

1

1.5x 10

4

t (s)

Fz(t

)(N

)

Figure 4-3. Heaving body simulation: wave-induced force.

0 2 4 6 8 10 12−1.5

−1

−0.5

0

0.5

1

1.5

t (s)

z(t)

(m),

z(t

)(m

/s)

z(t)z(t)

A Position and velocity.

0 2 4 6 8 10 12−5

0

5

10

15

t (s)

P(t

)(k

W)

B Instant dissipated power.

Figure 4-4. Heaving body simulation response.

The power of the heaving body is given by

Pz(t) = Fz(t)dz(t)

dt. (4–1)

The average power over one period of time is given by

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Pave =1

T

T

Pz(t)dt. (4–2)

Applying (4–2) over one wave period (in steady-state) of the function shown in

Figure 4-4B, gives an average power Pave = 0.82 kW. Since the float’s breadth is 1 m, then

we can compare this result with the power contained in one meter of wave front.

The available power for take-off, Ppz, is given by the difference between the wave

power and the power dissipated due to radiation (Prz) and viscous effects (Pvz)

Ppz = Pwz − Prz − Pvz =1

2ω2bpzZ

2o , (4–3)

where Pwz is the available wave power.

From Figure 4-2 the average power per meter of wave front is P = 2.125 kW.

Therefore, 38.6% of the wave energy is dissipated as radiation and viscous damping; hence

1.3 kW are available to be harvested with electrical generators (61.4% of the wave power).

From (4–3), the maximum damping coefficient due to power take-off is given by

bpz =2Ppz

ω2Z2o

. (4–4)

Equation (4–4) gives a rough estimate of the maximum additional damping that can

be added to the system using an electrical generator to harvest energy. This equation

becomes useful in design stages where the physical parameters of the system have to be

determined in order to develop a wave energy harvesting device.

4.4 Tensegrity System

Let the dimensions of the top platform be the same of the float in Section 4.3, i.e.

L = 2 m, Z = 0.5 m, B = 1 m, and d = 0.25 m. The additional constant mechanism

parameters are L0 = 6 m and Lpxz = 1/2L m. The base of the mechanism is located at

a depth hm = 6 m. The coefficients in all the terms of (3–55) can be calculated using

equations described in Chapters 2 and 3. Table 4-2 contains the values of the coefficients.

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Table 4-2. Tensegrity harvesting system coefficients.

Coefficient Value Units Equationm = 515 kg (2–54)awx = 50.56 kg (3–37)awz = 1.09×103 kg (2–56)Aw = 240.45 kg (2–57)Iy = 182.4 kg-m2 (3–37)C = 7.15×103 N-m/rad (3–44)

LA0= 4.32 m Reverse kinematics

LB0= 4.32 m Reverse kinematics

kA = 200 N/m AssumedkB = 200 N/m Assumedbrz = 2.04×103 N-s/m (2–58)brθ = 679.24 N-m-s/rad (3–53)bvx = 6.95 N-s/m (2–61)bvz = 6.95 N-s/m (2–61)bpz = 0 N-s/m AssumedAwp = 2 m2 (2–55)Fzo = 1.19×104 N (2–63)Mθo = 445 N-m (2–65)αz = 0 rad Symmetric body in long waves

Figure 4-5 shows the forces that the wave induces over the body. Figure 4-6 shows the

position and velocity response of the top platform the three directions of motion: surge,

heave and pitch.

0 2 4 6 8 10 12−2

−1

0

1

2x 10

4

t (s)

Fz(t

)(N

)

0 2 4 6 8 10 12−500

0

500

t (s)

Mθ(t

)(N

-m)

Figure 4-5. Tensegrity simulation: wave-induced forces.

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0 5 10

−1.2

−1

−0.8

−0.6

−0.4

−0.2

0

0.2

t (s)

x(t

)(m

),x(t

)(m

/s)

x(t)x(t)

A Surging motion.

0 5 10−1.5

−1

−0.5

0

0.5

1

1.5

t (s)

z(t)

(m),

z(t

)(m

/s)

z(t)z(t)

B Heaving motion.

0 2 4 6 8 10 12−6

−4

−2

0

2

4

6

8

10

t (s)

θ(t)

(deg

),θ(t

)(d

eg/s)

θ(t)

θ(t)

C Pitching motion.

Figure 4-6. Tensegrity simulation: surging, heaving and pitching motions.

Figure 4-7 shows the instantaneous power of the body. This power is a measure of

the energy that is being dissipated due to radiation and viscous effects. Applying (4–2)

over one wave period (in steady-state) gives an average power Pave = 0.6231 kW. Since

the float’s breadth is 1 m, then we can compare this result with the power contained

in one meter of wave front. The available wave power for take-off was computed as

P = 2.125 kW. Therefore, 29.31% of the available energy is being dissipated due to

radiation and viscous effects; hence, 1.5 kW are available to be harvested by electrical

generators (70.69% of the wave energy).

The solution of the differential equation of motion of the tensegrity mechanism was

performed for a set of generalized coordinates defined in the Cartesian space. Hence, the

reverse kinematic analysis developed in Chapter 3 allows one to compute the values of any

variable in the joint space.

Figure 4-8A shows the behavior of the hypothetical electrical generators; the required

displacement of such generators is less than 2 m, a value that can be achieved for modern

linear permanent magnet generators. The position and velocity data can be used as inputs

in the analysis of the electrical devices in future work.

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0 2 4 6 8 10 12−10

−5

0

5

10

15

20

t (s)

P(t

)(k

W)

Figure 4-7. Tensegrity simulation: instant dissipated power.

Figure 4-8B shows the lengths of the springs, which are always greater than the free

length, a requirement to maintain the tensegrity configuration of the mechanism.

0 2 4 6 8 10 126

7

8

9

10

11

t (s)

Posi

tion

(m)

1S 2

4S 5

0 2 4 6 8 10 12−2

0

2

4

t (s)

Vel

oci

ty(m

/s)

1v2

4v5

A Motion of generators.

0 2 4 6 8 10 122

4

6

8

t (s)

Len

gth

(m)

LA

LA0

0 2 4 6 8 10 122

4

6

8

t (s)

Len

gth

(m)

LB

LB0

B Length of elastic ties.

Figure 4-8. Tensegrity simulation: motion in generators and springs.

4.5 Discussion of Results

From sections 4.3 and 4.4, we see that the tensegrity configuration dissipates less

energy than the same float in pure heaving motion. The direct drive heaving system allows

to harvest 1.3 kW (61.4% of the wave power) while the tensegrity mechanism allows to

harvest 1.5 kW (70.69% of the wave energy). This value is about 10% more than the

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value given by the configuration that is used in most direct drive systems such the ones in

[110, 111, 117, 118, 121, 122].

Additionally, no parameters, other than the dimensions of the float, can be modified

in the purely heaving device. On the other hand, several parameters can be changed in

the tensegrity configuration to modify the energy dissipation due to radiation and viscous

effects. For instance, Figure 4-9 shows the variation of the percentage of the available

power that is dissipated due to radiation and viscous damping, as a function of the base

length (Figure 4-9A) and the stiffness of the elastic ties (Figure 4-9B).

2 4 6 8 1028

28.5

29

29.5

30

30.5

31

31.5

32

L0 (m)

Pave

(%)

A Variation of Pave with L0.

500 1000 1500 200029

30

31

32

33

34

35

36

kA, kB (N/m)

Pave

(%)

B Variation of Pave with kA, kB .

Figure 4-9. Variation of power dissipation with mechanism parameters.

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CHAPTER 5CONCLUSIONS AND FUTURE WORK

5.1 Conclusions

The idea of getting energy from ocean waves is not new, and only a few references

in literature have stated the possibility of harvesting energy from external disturbances

in a tensegrity structure. This research presented the first approximation to the energy

harvesting potential of a tensegrity system interacting with ocean waves.

This work addressed the analysis of a tensegrity mechanism for ocean wave energy

harvesting. A planar tensegrity morphology was selected for the system, and the dynamic

analysis was performed considering a two-dimensional linear model of the ocean surface

waves, considering the added mass, radiation damping and viscous damping phenomena.

The forward and reverse position analyses were performed using a geometric

approach. The forward and reverse velocity analyses were performed using theory of

screws. Numerical examples are provided in both cases. The Lagrangian approach

was used to deduce the equations of motion of the mechanism subject to the action of

wave-induced forces and moments.

The tensegrity potential for wave energy harvesting was demonstrated by comparison

with a purely heaving configuration that is commonly used in harvesting devices. It

was shown that the tensegrity configuration allows to harvest about 70% of the energy

contained in a linear wave, against 60% that was allowed by the conventional system using

the same floating body as input into the system. It was shown how the change in some

reconfigurable parameters of the tensegrity system affect the power dissipation due to

radiation and viscous damping.

The interaction between ocean waves, a multi-degree-of-freedom linkage and electrical

generators poses challenging problems in terms of mathematical modeling and simulation.

Nonetheless, the ideas presented in this document will be useful for the analysis and

testing of more advanced and complex energy harvesting devices.

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This research constitutes an interesting approach to show how the extensive

knowledge acquired in the analysis and design of mechanism can be used in new

applications that contribute to the world’s sustainable development.

5.2 Future Work

One important stage in the development of wave energy converters is the experimental

phase. Since this research included only simulation results, it would be interesting to

develop a physical scale model to be tested in a tank. Appropriate power scaling methods

are well referenced in literature and must be taken in account.

In this research we used a linear model for the sea waves, and the analysis was

performed for a planar mechanism. However, more realistic nonlinear and random models

for the behavior of ocean waves can be used. Such models would allow one to use not only

a planar linkage, but spatial tensegrity mechanisms and several different morphologies.

Optimization tools can be used to improve the performance of the analyzed

mechanism, and to to find a more suitable, or maybe optimal, tensegrity morphology

for ocean wave energy harvesting.

Because there are several options for electrical generators, further studies must

be carried out in order to determine which configuration offer better conditions to be

used with different tensegrity configurations. Additionally, the control methods and the

connection to a power grid or energy storage options shall be addressed in order to develop

a commercial device.

Future projects can include the development of mobile ocean energy harvesting

stations. Such stations can serve as complementary energy sources to relatively small

ocean devices such as underwater remotely operated vehicles.

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BIOGRAPHICAL SKETCH

Rafael E. Vasquez received his B.S. in mechanical engineering in 2002 and his

M.Sc. in engineering with emphasis in automation in 2007, both from the Universidad

Pontificia Bolivariana UPB, Medellin, Colombia. He joined the faculty of the UPB

in 2003 where he is associate professor in the area of dynamics, systems and control.

He is currently completing a doctoral degree in mechanical engineering, under a

Fulbright-Colciencias-DNP scholarship, at the Center for Intelligent Machines and

Robotics (CIMAR) at the University of Florida, Gainesville, Florida. His research

interests are theory of mechanisms; design, analysis and control of dynamic systems

and new technologies for energy harvesting. He is member of the American Society of

Mechanical Engineers (ASME) since 2005. After completing his PhD, Rafael will go back

to Colombia to conduct research and teach in the Department of Mechanical Engineering

at the Universidad Pontificia Bolivariana UPB, Medellin, Colombia.

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