Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are...

233
Edinburgh Wave Power Project Bending Moments in Long Spines

Transcript of Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are...

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Edinburgh Wave Power Project

Bending Moments in Long Spines

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B E N D I N G M O M E N T S I N L O N G S P I N E S

A r e p o r t t o t he Wave Energy S t e e r i n g Committee

covering work supported by the United Kingdom Department of Energy

EDINBURGH UNIVERSITY WAVE POWER PROJECT

Univers i ty of Edinburgh

Mayf i e l d Road

Edinburgh 9

031 667 1081 e x t 3276

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C O N T E N T S

INTRODUCTION

MAIN CONCLUSIONS

D E S C R I P T I O N O F THE MODEL

WAVES

POX PLOTS

POX P L O T S WITH GHOST WAVEFRONTS

3 D WAVE P L O T S

BENDING MOMENTS

SCATTER DIAGRAM EXPLORING

E F F E C T O F VARYING J O I N T S T I F F N E S S

E F F E C T O F VARYING S E A O F F S E T ANGLE AND ENERGY P E R I O D

E F F E C T O F VARYING S E A O F F S E T ANGLE AND SPREAD

BENDING MOMENTS I N THE SOUTH U I S T SPECTRA

E F F E C T O F S T I F F N E S S VARIATIONS I N SOUTH U I S T S E A S

SHAPE O F BENDING MOMENT D I S T R I B U T I O N I N SOUTH U I S T S E A S

BENDING MOMENTS I N ANGLED MONOCHROMATIC WAVES

E F F E C T O F LENGTH I N SOUTH U I S T S E A S

E F F E C T O F LENGTH I N ANGLED MONOCHROMATIC S E A S

E F F E C T O F MOORING M O D I F I C A T I O N S

E F F E C T O F BROKEN J O I N T S

ANGLES

CUMULATIVE J O I N T ANGLES

MAXIMUM J O I N T ANGLE I N FREAK WAVE

APPENDICES

WAVELENGTHS

POWER R A T I O

C R E S T LENGTHS

TANK L I M I T S

INHERENT J O I N T S T I F F N E S S

TIME S E R I E S AND HISTOGRAMS

THE SOUTH U I S T 46 SPECTRA

CONVERTING BENDING MOMENTS TO ANGLES

C A L I B R A T I O N S AND ACCURACIES

USEFUL EQUATIONS

REFERENCES

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1. A INTRODUCTION

While it is unusual to test tank-models with controlled, variable

elasticity there are several reasons why we believe that it is important

to exert the large effort required.

1. The convenient model-building materials are much too stiff to

represent the proper behaviour of concrete and steel at full scale.

2. We believe that, although the close-packed, crest-spanning terminator

configuration is the best possible arrangement for a wave-energy

device, it is not economic to resist bending moments greater than

those which would occur at the power limit. This means that non-

destructive yielding to bigger waves must be achieved. This will

not only save money on the spine structure but will also produce

dramatic reductions in mooring forces.

3. Work in the narrow tank had shown that the correct control of

a duck mounting could produce large improvements in duck performance,

doubling the efficiency in waves twenty-five duck diameters in

length. We had also discovered that the best values of mounting

stiffness were low, less than those that would be provided by

post-tensioned concrete at full scale, and that the mounting movement

could itself be a useful power-generating mechanism. Furthermore

the hardware needed to provide non-destructive yielding needed

very little modification to provide intelligent control and the

extra generating capability. We realised that the sof tware

requirements would be formidable - well beyond our present knowledge. But we were confident that the existence of a controlled model

would, as so often before, stimulate theoretical work. Furthermore

we were quite certain that the progress of computer technology

between now and the date of the return of energy shortage would

be so enormous that any level of control sophistication could

be safely assumed to be available at virtually zero cost. On

many occasions it has seemed that this view was not shared by

the civil and marine engineers who assess our progress.

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The work reported in this volume covers the measurements of bending

moments and joint angles as a function of sea conditions, model lengths

and stiffness, for circular spine sections without ducks. Other volumes

will contain the observations of shear, axial, torsion and mooring

forces, for spines with various appendages.

We found that it was necessary to put a very great deal of effort

into the presentation of the data if the essential truth was to be

revealed. The graphs in this report are about one twentieth of those

plotted during the analysis of the results. They are largely the

work of Mr. J.R.M. Taylor.

In parallel with the experimental programme sponsored by the

Department of Energy was a computer simulation study which formed

the doctoral thesis of Ian Bryden, supported by the SERC. Copies

of this thesis have been sent to the Energy Technology Support Unit

at Harwell and the UK Department of Energy. I would like to draw

the attention of WESC to the close correspondence of theoretical

simulation and experimental tests even for the most bizarre model

behaviour.

The Wave Energy Steering Committee will not be surprised to read

that the problem of plant availability has been given a great deal

of attention. Several papers on the subject have been submitted to

WESC through Harwell. I would like to emphasise the importance which

we attach to the questions raised in these papers.

S. H. Salter

August 1984

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l . B M A I N CONCLUSIONS

1. There seems t o be no obvious r e l a t i o n s h i p between l eng th and bending

moment f o r long compliant sp ines . Length squared and l eng th cubed

r u l e s do not apply.

2. Bending moments a r e nea r ly independent of energy per iod over t h e

c e n t r a l p a r t of t h e use fu l energy-generating spectrum and f a l l

f o r t h e very s h o r t e s t per iods .

3. Heave bending moments a r e propor t iona l t o t h e f i r s t power of wave

amplitude.

4. Surge bending moments r i s e with wave amplitude t o t h e power 0.8.

5. Surge bending moments a r e nea r ly always about twice heave moments.

For engineering purposes it is s a f e t o assume t h a t t h e r e is a

90° phase s h i f t between heave and surge moments. We can reduce

t h e quan t i t y of s t e e l used f o r r e s i s t i n g heave loading.

6. Bending moments r i s e r a t h e r gen t ly with s t i f f n e s s . A logari thm

r e l a t i o n s h i p f i t s our t e s t range. Reducing s t i f f n e s s makes t h e

e f f e c t s of per iod change even smal le r .

7. Changing t h e s t i f f n e s s i n one d i r e c t i o n produces l i t t l e e f f e c t

on t h e bending moments i n t h e o the r . We cannot run away from

surge moments by y i e l d i n g i n heave.

8. Seas wi th a mean approach d i r e c t i o n of 90' t o t h e l eng th of t h e

sp ine produce a bending moment p a t t e r n which o s c i l l a t e s about

a mean l e v e l i n t h e c e n t r a l reg ions ai-~d which is r a i s e d a t po in t s

approximately a wave-length i n from each end.

9. Seas which approach t h e sp ine from an obl ique d i r e c t i o n produce

smal le r moments a t t h e up-wave end and much l a r g e r ones a t t h e

down-wave end.

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10. The down-wave enhancement factor in monochromatic waves can be

as high as twenty five so that obliquity is by far the most powerful

variable. As it is a relatively narrow effect (changing over

one or two degrees) we must do some careful experiments to decide

whether or not the use of 75-tooth comb spectra is sound.

11. We believe that enhancement happens when the velocity of a flexural

wave along the length of the spine is close to the velocity of

an intersecting wave crest. As flexural propagation velocity

is a function of spine rigidity the effects can be controlled

by the use of intelligent joints and perhaps even turned to

advantage for power generation.

12. Changes to the mooring pattern, including the removal of a large

fraction of the moorings, do not significantly change bending

moment. We can afford to lose a lot of moorings and need not

repair them immediately.

13. The maximum joint angle in the steepest, largest, credible wave

is only just over 4 O so that the 12' design allowance is generous.

The result is unaffected by any attempt to stiffen or loosen

the joint.

14. Broken joints reduce their own bending moment and raise the moments

at adjacent joints.

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2. D E S C R I P T I O N O F THE MODEL

F ig 2.1 shows t h e genera l arrangement of t h e model, i t s moorings

and t h e w i r e l e s s mast which c a r r i e s t h e mul t ip le c o n t r o l boards.

A t t h e back of t h e drawing can be seen some of t h e e igh ty wavemakers.

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Fig 2.2 shows more detail of the spine sections and gives leading

dimensions, weights and calibrations.

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~ ..

. .. .SPINE UNIT PITCH --

WEIGHT SRNE ~ t i ~ +Sol&? RI& 58303 = 9.57 Ql.4 CALI bRA7iON 5 V O u d E , ' " ~ . o ~ T R E ~ O U ~ ~ / M T O R Q E / ~ N G MWEHT K)NH/V FREEBOARD 12.5~ 10% OF P W E ~ TORWE COMHAfiD IO*/V BuoYANcT WRPLUS 2.0 N a 5 N/N VELcurY 0.1 R A D ] ~ ~

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OW STATUS IZ ' I7 =Z8 sdB 6- 7np)t(DICt) few STATYJ I 2 8 3 = 1 8 d ~ P ~ I E E D = E R ~ ~

HO WING SEA GOING CONF IGURAllON WIm ELECTRICAL & AIR CONNECTIONS k -$- 'u0jNTS OPENED UP)

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Fig 2.3 shows the mooring arrangements used for these experiments.

The system is symmetrical fore and aft. It is an adaptation of the

system developed for full scale ducks and based on force measurements

in the narrow tank (ref e).

It is designed to provide a restoring force by changing the direction

of a rode rather than the magnitude of its tension. In many ways

it performs too well with rms tension variations less than 0.5% of

the mean value. Other configurations have also been tested.

The cost of the full-scale sinker weights is high but they can

very conveniently make use of the scrap obtained when round gyros

discs are made from rectangular steel sheet.

Model anchors are placed 2 metres up- and down-wave of the mean

spine centre-line. We have two types of anchor block. The passive

ones are plastic lunch boxes filled with scrap steel and cement.

Force-sensing ones use a steel base-plate with a square-bar cantilever

fitted with vertical and horizontal strain gauges.

The experiments in section 4.M show the effects of making a major

change to the mooring system.

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MOORING SYSTEM. General arrangemen t showing 40 spine joints with mooring attached a t every 8th jo int .

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Photograph 2.4 shows a spine section with its outer skin removed.

The spines are connected to one another by finger clamps which

can be tightened by radial screws. These can be seen protruding from

the inner ring at the near end of the spine. Between the fingers

is a flat beryllium-copper strip which acts as a low-rate torsion

spring to centralise the AC-coupled stiffness control.

Inside the bulkhead we can see the triangular plate torque-arm

with two of the four strain-gauges which sense fluid loading. Note

the T-shaped slots which concentrate strain under the gauges.

The far end of the triangular plate can be moved through an angle

of 2 4 . 2 O by a pair of steel-reinforced polyurethane toothed belts.

These run on pulleys with tension-adjusting eccentrics.

The low-inertia motor and its 18:l gear box can just be seen

behind the torque arm. The length of the torque arm contributes the

final stage of the step-down gearing which has an overall ratio of

565:l from motor shaft to joint angle.

The low-inertia motors are fitted with tacho-generators. We

use integrated velocity to indicate position.

Although rotation is constrained by carbon steel ball-bearings

exposed to the water, the addition of a corrosion inhibitor known

as 'Cimplus' has prevented problems and the original joint bearings

are still in use.

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Photograph 2.5 shows a spine section with electronic control

board. Signals from the strain-gauge bridge are conditioned and sent

to a control computer which decides the correct command signal to

be sent to the servo-motor. This moves the joint via belts and torque

arm. The tank operator can control both stiffness and damping at

each joint. We can also send a series of command signals to induce

eel-like swimming motions in the model.

We had to fit a 16 channel bi-directional multiplexer to measure

and control the spine joint and the duck which will be mounted on

it. Each spine section contains two servo amplifiers. Their power

transistors can be seen to the left of the board and are in excellent

thermal contact with the water. One amplifier will be used for duck

control.

In front of the spine is a collection of its machined parts.

The entire assembly is enclosed in a centrifugally cast G.R.P. tube

with light alloy end rings. We found that G.R.P. shows some long

term porosity and that after a few years the bond between epoxy resin

and freshly anodised light alloy is degraded. We are replacing the

outer tubes with light alloy. Cimplus does not get through G.R.P.

and there was quite serious corrosion on the pulley bearings inside

the spine. These were all replaced and arrangements were made to

pass a slow current of dry air through the model.

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Figure 2.6 shows a circuit diagram of the spine electronics.

This diagram divides roughly into three sections:

Section 1: (ICS 1 to 3) shows the conditioning and pre-

amplification for the strain gauge bridge and the tacho-

generator. At the right-hand end can be seen the resistive

divider that drives the "BLOTIt leak detector. It normally

sits at -10V, but water in the module will change it to

about -3V.

Section 2: (IC 10 down to IC 9) shows the multiplex section. There

are 3 lines multiplexed out, labelled ZERO, BB (backbone

or spine) and DUCK. (The line marked (DUCK) is connected

to the local duck.) The Harris HI-507 chip handles most

of the switching and an HI-201 the rest. Clocking is

managed by a "token passingtt system. Clock pulses are

fed to either "CK1" or ItCK2" (it doesn't matter which)

and the spine counts eight of them, sending out spine

and duck data appropriately. At this point IC 9 closes

a switch between "CKltt and I1CK2", allowing the clock pulses

to go on to the next spine in line. This system allows

all spines to be electronically identical.

IC8 is a 4-bit counter that sets the "STATUS" of the spine.

It programmes the gain of IC15 and thus the overall spine

force-feedback loop gain.

Section 3: ICll down. This circuitry comprises a sample and hold

(ICs 11 and 14) which handles the local duck multiplex,

and op-amps 16, 17 and 15, which optimise the frequency

responses of the duck and spine feedback loops. The bottom

row, ICs 18 and 19, shows the two power amplifiers needed

to drive the duck and spine motors. These amplifiers

are based on the LM391 IC which is designed for hi-fi

work but, when combined with a pair of Darlington transistors,

makes a very compact servo unit.

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Photograph 2.7 shows David J e f f r e y and a p i l e o f sp ine s e c t i o n s

p r i o r t o launching.

Each is connected t o i ts neighbours with a waterproofed multiway

p lug c a r r y i n g power and s i g n a l s . Two u n i t s i n f r o n t of t h e p i l e have

t h e i r ducks f i t t e d .

A t t h e t op r i g h t of t h e photograph we can s e e a few o f t h e c i r c u i t

boards which s e l e c t d a t a channels f o r c o n t r o l and measurement. The

boards a r e mounted on a t r i angu la r - sec t ion w i r e l e s s mast which spans

t h e e n t i r e width of t h e tank and is used t o launch and recover models.

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Photograph 2.8 shows Chris Retzler checking the clamping of a

joining ring.

The model is hanging up by nylon ropes from its wireless mast.

When this is pulled back over the work platforms which cover our beaches

we can get convenient access to both mechanical and electronic bits.

Launching the model and connecting all the moorings takes one

person less than 3 minutes.

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Photograph 2.9 shows t h e sp ine model i n t h e tank. J o i n t d e f l e c t i o n

can be c l e a r l y seen. Grid l i n e s on t h e tank f l o o r a r e a t 5 metre

i n t e r v a l s . The j o i n t p i t c h is 0.4 metres.

The w i r e l e s s mast has been moved beachward t o al low a c l e a r e r

view. For t e s t i n g it would be placed s o a s t o minimise t h e drag of

l i f t i n g ropes and umbi l ica l cab les . I n i t i a l t e s t s of candida te cab le s

i n t h e narrow tank showed t h a t t h i s drag was about 5% of t h e mooring

fo rce .

A l i n e of mooring f l o a t s can be seen t o t h e r i g h t of t h e model.

We found t h a t t hese could be rep laced by o t h e r s one t h i r d of t h e

displacement.

The t h r e e heavy b a r s on t h e f r o n t of t h e w i r e l e s s mast d i s t r i b u t e

power t o t h e model. Each group of fou r sp ines is p ro t ec t ed by sepa ra t e

fu ses and over-voltage crow ba r s . One sp ine caught f i r e bu t t h e damage

w a s contained.

A l l t h e mult iplex con t ro l boards a r e mounted on t h e beachward

s i d e of t h e wi re l e s s mast. Their Terry-cl ip attachments can be seen.

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Fig 2.10 shows a block diagram of the data collection and model

control system.

We found that the combination of distributed multiplex boards,

differential signal-pairs and insulation-displacing ribbon-cable

connectors has produced excellent reliability. The settling time

of the 30 metre length of the wireless mast data-collection system

is about 12 microsecond with a noise level of 1.5 millivolts. We

ran into a problem with a residual dielectric 'remnance' which required

the signal wires to be 'cleaned-out' by the subtraction of a small

charge which depended on the previous measurement.

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3.A POX-PLOTS

Introduction

We find visual representations of the sea states very useful

both as a check that we are getting the sea that we want and as an

aid to understanding test results. We found that the most useful

representation is the 'pox-plot'. An example is shown below. Each

individual pox-plot identifies, with a dot or cross, the period and

angle of the component wavefronts making up a sea state. The number

of wavefronts is limited to 75 by the current wavemake~controlling

computer. Angle is shown as the horizontal variable, usually scaled

between -70 and +70 degrees, with period increasing from 0 to 2.0

seconds vertically. A separate diagram on each page of pox-plots

shows the scaling in use.

Information about wave height is not displayed graphically, but

as a single value of Hrms (in centimetres) below and to the left of

each plot. This is the mean of several measurements made at different

times during the course of the experiments. We use a row of sixteen

conductivity-corrected wave gauges placed 2 metres in front of the

wavemakers.

-70 Fig 3.1 The pox-plot for a 1.2 second Pierson Moskowitz sea +70

with a Mitsuyasu spread.

I I 1 1 I 1 +

+

+ *

+ + + .- +

PERIOD + + + .& (seconds) + +

+ + + + + + + +

+ + + + + -

+ + + + +

+

+

+

4

+ r + +

--+ + + +

+ + + +

+ + + + +

+ + + +

+ + + +

+ + + + +

+ +

+

+ --

ANGLE (degrees) - -- - -- - - . - --

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In this section we include diagrams of every sea used in the

experiments. The pox-plots are produced by reading back tank data

files normally sent to the wave-making computer, and then performing

a 'reverse tank transfer function' to convert back to amplitudes,

periods and angles. On more than one occasion this process has uncovered

faults in our tank software.

We lay out pox-plots in 2-dimensional arrays to match test results

given in other sections. Where appropriate, rows and columns of the

array are assigned particular values of a sea constant such as energy

period or Hrms, which varies vertically or horizontally. The names

of these variables are then printed with a large set of cross-arrows

at the top left of the page. In the case of the South Uist spectra

the Institute of Oceanographic Science reference number is placed

at the bottom right of each plot.

The lack of height information about individual wavefronts is

not a drawback with single-component monochromatic seas, or with our

standard Pierson-Moskowitz spectra, which comprise equal amplitude

' teeth' , each representing a wavefront of identical energy.' The

South Uist seas, however, are made up by combining up to 3 separate

'sub-seas' (see section 6.G), each of which has its own fixed tooth

size, so dots may represent wavefronts of slightly differing heights.

1 In fact at low frequencies the heights of wavefronts are adjusted

slightly to maintain constant energy in finite tank-depth (see

section 6.B).

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t nergy PERIOD (seconds)

Hrms MULTIPLIER

10 (seconds)

tfcms

39 s e a s w i t h P i e r s o n - M o s k o w i t z s p e c t r a l s h a p e ,

M i t s u y a s u s p e a d i n g and mean a n g l e o f 0 d e g r e e s . 9 v a l u e s o f E n e r g y P e r i o d , 5 m u l t i p l e s o f Hrms.

The 4 0 t h s e a w o u l d h a v e b e e n t o o b i g f o r t h e wavemakers .

X PLOTS SEA SET: PM'm 1.4

t ter diagram explorer'

. . - . .

0.51 1.03 2.04 2 .86 3 .38

.. ... sea

too b ig

0.56 1 .14 2.23 3.02

GRAPH 3 . 2

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However our measured H r m s va lues a r e up t o 10% lower than t h e s e

co r r ec t ed t h e o r e t i c a l values. The most l i k e l y cause is t h e reduct ion

t h a t we make i n wavemaker d r i v e command s i g n a l s as wavefront angle

i nc reases . This is p a r t of t h e wide tank ' t r a n s f e r f u n c t i o n ' . We

mul t ip ly by t h e square r o o t of t h e cos ine of t h e wavefront angle .

A quick t e s t confirms t h a t t h i s is too severe a co r rec t ion f o r angles

g r e a t e r than about 40° , s o t h a t wavefronts near t h e s i d e s of t h e p l o t s

a r e being over-at tenuated.

A l l t e s t r e s u l t s i n t h i s r e p o r t use a c t u a l measured va lues s o

t h a t dev ia t ions from our i n i t i a l tank t r a n s f e r func t ion do not a f f e c t

conclusions. We hope t o produce an improved multi-parameter t r a n s f e r

func t ion f o r f u r t h e r r e p o r t s .

Graph 3.3 shows t h e H r m s and Te t e s t p o i n t s superimposed on a

South U i s t s c a t t e r diagram. Lines of cons t an t power dens i ty have

been added.

These seas were used f o r t h e s c a t t e r diagram explor ing experiments

i n s e c t i o n 4.A. The 1 .0 second s e a with nominal H r m s o f 1.36 cm was

used f o r t h e s t i f f n e s s v a r i a t i o n experiments i n s e c t i o n 4 . B .

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GRAPH 3 . 3

-.

scale: 1/107.7 k j280,+&

..

. .

. . . 2 . . .

. . . 4 9 5 1 9 - 5

I I I I I I I I I I I I I 4 5 6 7 8 9 10 1 1 12 13 14 15 16

T, (seconds)

Whole Year South U i s t s c a t t e r diagram, with ' Sca t t e r Diagram Explorer' sea-set superimposed. sca le : 1/107.7

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Sea S e t PM ' a ' Graph 3.4

These a r e s tandard Pierson-Moscowitz s e a s with Mitsuyasu spreading.

We wanted t o i n v e s t i g a t e t h e e f f e c t of angled s e a s , and t o check

tank angular symmetry. The wavefront angles a r e b iased p o s i t i v e l y

and nega t ive ly .

Energy per iod v a r i e s v e r t i c a l l y with a h igher maximum value than

i n t h e previous s e t .

The expected H r m s l o s s e s due t o frequency c l i p p i n g range from

0.4% a t an energy period of 1.0 seconds, t o 9.3% a t 1 .6 seconds.

The expected l o s s e s due t o angular c l i p p i n g average about 1.3% f o r

t h e O 0 o f f s e t s e a s , and about 7% f o r t h e 40° seas . The combined e f f e c t s

range from a t o t a l expected H r m s l o s s of 2% a t 1 second and 0 ° , t o

15% a t 1 .6 seconds and 40°.

Measured H r m s va lues a r e lower than these expec ta t ions by an

average of 7%, the e r r o r s being worst a t 1 .4 and 1.6 seconds, and

a t 40° o f f s e t .

These s e a s were used f o r t h e experiments of s e c t i o n 4.C.

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Sea S e t CO ' a ' G r a ~ h 3 .5

These a r e Pierson-Moskowitz s p e c t r a aga in , bu t spreading is S

according t o t h e cos model. We va r i ed s from 2 t o 10,000. (This

is deemed t o be wi th in a few percent of i n f i n i t y ! ) Of f se t angle is

a l s o va r i ed aga in bu t t h i s time only i n a p o s i t i v e sense , away from

t h e g l a s s .

Nominal H r m s f o r a 1 second Pierson-Moskowitz s e a is 1.36 cm.

The expected l o s s due t o frequency c l ipp ing is cons tan t throughout

t h i s s e t , a t 0.4%. Angular c l i pp ing is most severe f o r t h e widely

spread s e a s and f o r those with l a r g e angular o f f s e t s . Even a t 0'

o f f s e t , H r m s w i l l be reduced by 8% f o r a spread exponent of 2 and

a t 50° o f f s e t t h i s i nc reases t o 16%.

For t h e f i r s t t ime, many of t h e s e a s i n t h i s s e t have measured

H r m s va lues g r e a t e r than expected, and i n many cases g r e a t e r than

t h e nominal value. For i n s t a n c e , H r m s f o r t h e bottom l e f t s e a is

10% higher and t h e e f f e c t is c l e a r l y r e l a t e d t o angular spread and

mean angle.

I n t h e ' i n f i n i t y ' row some of t h e upper wavefronts a r e seen breaking

away from t h e l i n e . This is t h e r e s u l t of an i n s u f f i c i e n t l y s u b t l e

shallow-water co r r ec t ion . The symptoms a r e hard t o s e e i n t h e a c t u a l

tank s e a , even t o a well-briefed observer .

Occasional wavefronts seen wandering well away from t h e herd ,

near t h e bottom r i g h t of t h e p l o t s , a r e symptoms of t h e ' t ank l i m i t s '

problem discussed i n s e c t i o n 6.D, and a r e i l l u s t r a t e d more c l e a r l y

i n t h e a d d i t i o n a l s e t of pox-plots i n s e c t i o n 3.B.

These s e a s were used f o r t h e experiments descr ibed i n s e c t i o n

4.D.

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t nergy PERIOD (seconds)

Offset I ANGLE -> (degrees)

POX P SEA SET:

45 s e a s w i t h P i e r s o n - M o s k o w i t z s p e c t r a l shape , n o m i n a l Hrms a n d M i t s u y a s u

s p r e a d i n g . 5 v a l u e s o f E n e r g y P e r i o d , 9 d i f f e r e n t o f f s e t a n g l e s .

''c)oo,ZJ PMmn 4. mk " GRAPH 3 . 4

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Offset ANGLE -> POX PLOTS

'?(degrees) - I SEA S E T : C O ~ '

36 P i e r s o n - M o s c o w i t z s p e c t r a w i t h 1.0 s e c o n d E n e r g y P e r i o d , a n d n o m i n a l Hrms. 6 d i f f e r e n t o f f s e t a n g l e s a n d 6 v a l u e s o f 1 s ' f o r a l c o s S s p r e a d i n g f u n c t i o n .

2 a n o m a l i e s a r e p a r t i c u l a r l y c l e a r w i t h t h e ' i n f i n i t y ' row. The a n g l e s o f l o n g p e r i o d c o m p o n e n t s w e r e i n c o r r e c t l y c a l c u l a t e d , and t h e p r e s e n c e o f ' g h o s t ' w a v e f r o n t s a t b i g a n g l e s i s i n d i c a t e d

a t s h o r t p e r i o d s .

GRAPH 3.5

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(3.A c o n t )

Sea S e t s : South U i s t ' s u ' ' a ' , ' b ' , ' c ' & ' d l Graphs 3.6 - 3.9

The South U i s t s e a s make much more i n t e r e s t i n g pox-plots. Our

tank implementation of t h e I n s t i t u t e of Oceanographic Science ( 1 0 s )

da t a is descr ibed i n s e c t i o n 6.H.

An a d d i t i o n a l image on each page d e p i c t s our t ank and model i n

t h e i r working r e l a t i o n s h i p s t o t h e compass.

Components i n t h e r i g h t h a l f of each p l o t r e p r e s e n t wavefronts

approaching from t h e sou th of t h e mean d i r e c t i o n , and those t o t h e

l e f t approach from n o r t h o f t h e mean d i r e c t i o n .

The s e p a r a t e wind, swe l l and o l d wind components a r e o f t e n c l e a r l y

v i s i b l e . Swell is u s u a l l y i n t h e upper p a r t o f t h e p l o t and t i g h t l y

bunched i n spread . The width o f spread i n d i c a t e s t h e s i z e and d i s t a n c e

of t h e o r i g i n a t i n g weather. Wind s e a is u s u a l l y a t lower f requenc ies

near t h e bottom o f t h e p l o t s , and wel l spread. The e f f e c t o f t h e

s p e c t r a l width parameter i n compressing t h e frequency range of wavefronts

is a l s o o f t e n c l e a r .

Sea number 223A (graph 3.6) has only a s i n g l e component from

a well-defined and small swel l source . Sea 371A (graph 3 .6) has a

wide swe l l source t o t h e no r th and i t s 'wind' and ' o l d wind' components

a r e n o t superimposed on t h e pox-plot.

Measured H r m s va lues f o r a s c a l e o f 107.7 a r e g iven i n cen t imet res

a t t h e bottom l e f t of each p l o t . They gene ra l l y i n c r e a s e with s e a

number.

Although 13 of t h e 46 s p e c t r a a r e n o t very accu ra t e ly represen ted

by t h e ' a ' ve r s ion (graph 3.6) we used them f o r most of our experiments.

There a r e enough v a r i a t i o n s i n t h i s one group t o t e s t ou t any bending

moment t h e o r i e s and model deployment is very much e a s i e r when p a r a l l e l

t o t h e wavemakers.

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IOSdata adjusted for 100m water depth and rescaled at 1/108 POX PLOTS

SEA SET: SU 'a' 46 The ' 4 6 s p e c t r a 1 , b a s e d o n b u o y d a t a o f f t h e c o a s t o f s o u t h U i s t , w i t

bSPECTRA - 10 lsecords) !-='I f r o m w i n d r e c o r d s . The 46 a r e s e l e c t e d t o be r e p r e s e n t a t i v e o f a l l s e a s o n s , b u t t h e i r w e i g h t i n g s

a r e n o t e q u a l . F o r t h e l a t s e t , t h e n o r m a l t o t h e wavemaker a x i s r e p r e s e n t s a compass b e a r i n g o f 260 d e g r e e s w i t h t h e mode l p a r a l l e l t o t h e wavemakers . 13 o f t h e 46 s p e c t r a a r e p o o r l y

b

'a' set Bnfh r e p r e s e n t e d by t h e l a 1 v e r s i o n , a n d t h e I b I o r l c l v e r s i o n i s a c l o s e r match .

Nominal Westerly seas

ANGLE -70 W -40 -20 0 +20 +?+qo

r20

GRAPH 3 . 6

Page 39: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

The ' b ' s e t (graph 3.7) provide improved ve r s ions of t hose s e a s

which have s t r o n g sou the r ly components. The model is r o t a t e d clockwise

40 degrees and t h e tank mean heading s h i f t s t o 220°. It is i n t e r e s t i n g

t o compare t h e ' a t and ' b ' vers ion of t h e same sea . The swel l components

c l e a r l y s h i f t l e f t and t h e number of wavefronts a l l o c a t e d t o them

a r e reduced, a s t h e new o r i e n t a t i o n al lows wind s e a components t o

be r e a l i s e d wi th in t h e wavemaker angular range.

The ' c t s e t (graph 3.8) provide improved ve r s ions of those s e a s

which have s t r o n g n o r t h e r l y components. The mean wave d i r e c t i o n

r ep re sen t s a compass bear ing of 310 degrees. Swell now moves t o t h e

r i g h t compared with t h e ' a t s e t .

It is n o t very convenient t o yaw t h e model clockwise f o r t h e

' b ' s e t and then anti-clockwise f o r t h e ' c t s e t . I n p r a c t i c e we use

the ' d l s e t t o implement a mirror image of t h e ' c t s e t . The model

need only be yawed another lo0 clockwise from t h e p o s i t i o n f o r t h e

' b t s e t . The Hebrides look s t r a n g e t h a t way round, bu t it makes l i t t l e

d i f f e r ence t o our bending moment t e s t s .

The South U i s t s e a s were used f o r t h e experiments descr ibed i n

s e c t i o n s 4.E t o 4.H, and 4.L t o 4 . M .

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I the

[SPECTRA 1

Southerly seas .I

IOSdata adjusted for 100m water depth and rescaled at 1/108

ANGLE Ibegrees) -n41-40-2C 9 +?l+F+a

r 2 0

POX PLOTS SEA SET: SU'b'

10 (seconds) f-1 9 o f t h e 46 s p e c t r a w h i c h a r e p o r l y r e p r e s e n t e d b y t h e l a 1 s e t . F o r t h e s e , t h e n o r m a l t o t h e

w a v e m a k e r a x i s r e p r e s e n t s a c o m p a s s b e a r i n g o f 220 d e g r e e s when t h e m o d e l i s s e t a t an a n g l e o f 4 0 d e g r e e s t o t h e w a v e m a k e r .

% ttcms w

""",-J-",,'r.\ Y... - GRAPH 3 . 7

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Sea S e t s : MO ' a ' . ' b ' & ' c ' G r a ~ h s 3.10 - 3.12

Regular s e a s do n o t make very i n t e r e s t i n g pox-plots.

We increased t h e angular l i m i t of t h e tank t o 80° f o r t h e s e waves.

The nominal H r m s is 1.414~111 f o r t h e ' a ' s e t , and l.Ocm f o r t h e ' b '

and ' c ' s e t s .

I n a l l 3 s e t s , t h e v e r t i c a l v a r i a b l e is energy per iod with a

range of 0 .8 t o 1 .6 seconds i n 5 s t e p s .

' a ' s e t : (g raph 3.10)

The nominal c r e s t angle v a r i e s from -lo0 t o -80°. A t long per iods

and extreme angles (bottom r i g h t co rne r ) t h e a c t u a l angles produced

i n t h e tank a r e v i s i b l y lower than t h e i r nominal va lues . This was

t h e first i n d i c a t i o n of a f a u l t y shallow water c o r r e c t i o n i n our sea-

gene ra t i ng sof tware . The e f f e c t is a l s o c l e a r l y v i s i b l e i n Graph

3.5.

These s e a s were used f o r t h e experiments i n s e c t i o n 4.1.

' b ' s e t : (graph 3.11)

The c r e s t l eng th is va r i ed from 2 t o 12 metres i n 2 metre s t e p s .

These s e a s were used f o r t h e experiments i n s e c t i o n 4.5.

' c ' s e t : (g raph 3.12)

I n a d d i t i o n t o angle and c r e s t l e n g t h we discovered t h a t it was

u se fu l t o desc r ibe wavefronts i n terms of t h e v e l o c i t y of movement

of t h e c r e s t a long t h e sp ine . The c r e s t v e l o c i t y is va r i ed from 2

t o 8 metres pe r second.

These s e a s were used f o r t h e experiments i n s e c t i o n 4.K and 4.L.

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40 m o n o c h r o m a t i c s e a s g i v i n g known c r e s t a n g l e s a t v a r i o u s p e r i o d s , w i t h n o m i n a l Hrms o f 1.414cm. The a n g u l a r l i m i t s o f t h e wavemakers were i n c r e a s e d t o 80 d e g r e e s f r o m t h e n o r m a l v a l u e o f 70 d e g r e e s . The f a l l o f f i n m e a s u r e d Hrms v a l u e s a t l a r g e a n g l e s shows i n c o r r e c t a m p l i t u d e

c o m ~ e n s a t i o n i n t h e t a n k t r a n s f e r f u n c t i o n .

POX PLOTS SEA - SET: - Mob'

- - Crest

(degrees) 1 ANGLE-

ANGLE ki.e.greesl -804-40-20 0 +20+40+60+80

r 2 0

1.0 (seconds) P-I

(monochromatic)

S R A P H 3.1 0

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37 m o n o c h r o m a t i c s e a s g i v i n g known c r e s t l e n g t h s a t v a r i o u s p e r i o d s , w i t h n o m i n a l The wavemak ing a n g u l a r l i m i t s w e r e i n c r e a s e d t o 80 d e g r e e s , b u t 3 s e a s were s t i l l a t 2 m e t r e s . Hrms f o r t h e 4 m e t r e s e a a t 1.2 s e c o n d s was i n a d v e r t e n t l y d o u b l e d . i n measured Hrms v a l u e s a t l a r g e a n g l e s shows i n c o r r e c t a m p l i t u d e c o m p e n s a t i o n i n t r a n s f e r f u n c t i o n .

Crest

I (metres)

Hrms o f 1.0cm. p OX u n r e a l i s a b l e The f a l l o f f t h e t a n k

(monochromatic)

GRAPH 3.11

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33 monochromat ic seas g i v i n g known c r e s t v e l o c i t i e s a t v a r i o u s p e r i o d s , w i t h n o m i n a l Hrms o f 1 cm. The wavemaking a n g u l a r l i m i t s were i n c r e a s e d t o 80 degrees, b u t 2 seas were s t i l l u n r e a l i s a b l e a t 2 metres /sec . The f a l l o f f i n measured Hrms v a l u e s a t l a r g e a n g l e s shows i n c o r r e c t a m p l i t u d e compensat ion i n t h e t a n k t r a n s f e r f u n c t i o n .

POX PLOTS SEA SET: MOkJ

GRAPH 3.1 2

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3.B POX-PLOTS WITH GHOST WAVEFRONTS Graphs 3.13 - 3.19

The restrictions on frequencies and angles due to the finite

width of wavemakers are discussed in section 6.D.

An absolute upper tank limit exists at 2.26 hz, the frequency

at which the wavelength is equal to wavemaker pitch. Between 1.6

hz and 2.26 hz the maximum permissible wavefront angle drops steadily

from ?9O0 to OO. Wavefronts transgressing this envelope acquire one

or more 'ghost siblingst at the same frequency but at a different

angle. Below 1.6 hz the theoretical angular limit is over 90°. Below

0.5 hz the wavemakers have too little displacement to work effectively.

We have not yet made any measurements of the unwanted wavefronts but

their amplitudes are visibly of the same order as the principal wavefront.

These modified pox-plots show the effect on our sea sets of using

a simple rectangular limit (?70°, 0.5 - 3.0 hz) when calculating wavefront frequencies and angles. The limit has been over-drawn on each plot

as a roughly horizontal line. Any intended wavefront below these

lines acquires a ghost. Both wavefront and ghost are drawn as a dot.

The number of ghosts is totalled at the top left of each plot. Naturally

the effect is most obvious at high frequencies, so that in the scatter

diagram set (graph 3.13), the seas at Te = 0.7 seconds have the most

ghosts. The effect of angular offsets is to increase marginally the

number of ghosts (graphs 3.14 & 3.15). On average the basic westerly

set of South Uist spectra have 8 ghosting wavefronts, but this rises

to 21 for the southerly set, and 14 for the northerly set (graphs

3.16 - 3.19).

Generally the effect of having too many fronts outside the tank

limits is to widen the angular distribution of energy at short periods.

Test work in monochromatic seas, (section 4.H, and more recent work

still to be reported) suggests that the spine model is comparatively

insensitive to short-period, off-axis wavefronts. Our wavemaking

software will in future represent only those parts of spectra which

fall within the tank limits. An override facility will allow deliberate

transgressions.

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Offset I ANGLE 2 I

Enerav (degrees)

(seconds) I

wavefronts BELOW Line have ghost sibling

Ref&

POX PLOTS SEA SET: PM*aO

rshowina HIGH FREQUENCY limit 1

''C)co,2~S3 PM mn 4. TNk " GRAPH 3 . 1 4

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+70

wavefronts BELOW Line have ghost

Offset ANGLE r->

I i d e q r ees)

sibling

POX PLOTS SEA SET:CO'CI'

showing HIGH FREQUENCY limit

GRAPH 3.1 5

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>

showing HIGH FREQUENCY limit

c-

the IOSdata adjusted for 100m water depth and rescaled at 1/108 POX PLOTS

SEA SET: SU'aJ

26

GRAPH 3 . 1 6

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IOSdata adjusted for 100m water depth and rescaled at 1/108

'D- set

Southerly seas J

+70

wavefronts BELOW line have ghost

~~

POX PLOTS SEA SET: SU 'b'

sibling (showina HIGH FREQUENCY limit 1

GRAPH 3.1 7

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showing HIGH FREQUENCY limit

b

the IOS data adjusted for lOOm water depth and rescaled at 1/108

+70

POX PLOTS 46 SPECTRA

SEA SET: SU'cJ wavefronts BELOW l ~ n e have ghost s~b l~ng

'c' set

Northerly seas

N . .

: ;:..:..: : .. - . . *

..:a-.-,.,. .. : .

W,3pJ*wn~~rrk '

GRAPH 3 .18

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mlrrored Nort herlv seas J

showing HIGH FREQUENCY l imit i

GRAPH 3.1 9

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3.C 3D WAVE PLOTS

In t roduc t ion

3D p l o t s add another dimension t o pox-plots. They g ive a b e t t e r

impression of t h e o v e r a l l s i z e of s e a s , bu t they have lower r e s o l u t i o n

on t h e per iod /angle p lane .

We inc lude two s e p a r a t e groups of 3D p l o t s :

I n t h e 1st group - graphs 3.20 t o 3.26 - t h e he igh t of p l o t

is p ropor t i ona l t o wavefront amplitudes:

I n t h e 2nd group - graphs 3.27 t o 3.32 - t h e volume under

t h e p l o t is p ropor t i ona l t o t o t a l power i n s ea .

The l ayou t of each page of 3D p l o t s matches t h e corresponding

page of pox-plots and bending moment t e s t r e s u l t s . The range of per iods

and angles a r e t h e same. The v e r t i c a l s c a l e s a r e unique t o each page,

s o he igh t comparisons between pages should n o t be made.

The nodes of each 3D p l o t form t h e b i n s o f a 2-dimensional histogram.

Each wavefront a l l o c a t e s s co re s t o t h e b i n s i n i ts v i c i n i t y according

t o a smoothing func t ion .

The number of per iod and angle increments depends on t h e t h i cknes s

of our p l o t t e r pens. We inc rease t h e r e s o l u t i o n f o r t h e v a r i a b l e

spread s e t i n graph 3.22 by p l o t t i n g a t a l a r g e r s c a l e and then reducing

t h e whole page on a cop ie r .

The Pierson-Moskowitz/Mitsuyasu s p e c t r a i n graphs 3.20 & 3.21

a r e d e l i g h t f u l l y smooth. The cut-off enforced by t h e l i m i t e d angular

range of t h e tank i s apparen t on t h e r i g h t edge of many s p e c t r a .

We increased t h e per iod and angle r e s o l u t i o n t o t r y t o show t h e

dramatic change i n angular d i s t r i b u t i o n i n graph 3.22. Ghost

wavefronts show up a s detached outcrops i n t h e p l o t s a t t h e lower

l e f t .

Swell components show up c l e a r l y i n t h e South U i s t s e t s

(graphs 3.23 - 3.26) bu t it is q u i t e d i f f i c u l t t o s e p a r a t e wind s e a

and old-wind s e a components.

Page 56: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

a Hrms

t nergy HEIGHTS

PERIOD pFoportiona1 to AMPLITUDES

(seconds

3D PLOTS SEA \ SET: PM8m 1.4

'scatter diagram explorer'

Page 57: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

Offset + ANGLE -> I

Energy PERIOD (seconds)

(degrees) /

HEIGHTS proportional

to AMPLITUDES

PLOT SEA SE

V

I ANGLE (degrees)

I " c ] c o , ~ J P ~ n w h .7Nk" I

GRAPH 3.21

Page 58: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

Offset

rr I (degrees) SEA S E T : C O ~ ' ANGLE--> 3D

EXPONENT I 0 10 20 30 40 50 r 1

HEIGHTS 51 2

'infinity' ~.

GRAPH 3 . 2 2

Page 59: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

I SPECTRA I 'a' set

Nominal Wes terlv seas J

HEIGHTS proportional

to AMPLITUDES

3D PLOTS SEA SET: SU 'a'

IOSdata adjusted for 100m water depth and rescaled at 1/108

GRAPH 3 . 2 3

Page 60: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

Southerly I

#

the 46 *SPECTRA

seas I

HEIGHTS proportional

to AMPLITUDES

3D PLOTS SEA SET: SU 'bJ

ANGLE (degrees) IOSdata adjusted for 100m water depth

GRAPH 3 . 2 4

'b'set and rescaled a t 1/108

I I

Page 61: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

IOS data adjusted for 100m water depth and rescaled at 1/108

Nort herlv seas J

3D PLOTS SEA SET: SU 'c'

GRAPH 3 . 2 5

Page 62: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

3D PLOTS SEA SET: SU ' dJ

Page 63: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

Hrms 0.25 0.5 -MULTIPLIER* - 1.0 - 1.5 - 2.0 C 1 t nergy VOLUME under surface 0.7

0.8

1.2

1.3

3D PLOTS SEA SET: PM'm a 1.4

'scatter diagram explorer' b-

GRAPH 3 . 2 7

Page 64: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

Off set ANGLE -> 3D PLOTS

t-- (degrees) VOLUME under surface SEA SET: PM'a* Energy proport ~onal

to POWER

PERIOD (seconds)

-30 -20 -- -- - -10 0 - - +I0 2 0 + 30 + 40 1

Page 65: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

'a' set

Nominal Westerly seas

VOLUME under surface 3D PLOTS SEA SET: SU 'a'

IOSdata adjusted for 100m water depth and rescaled a t 1/108

- LJw,5aJWnnnP,.~NR-

GRAPH 3 . 2 9

Page 66: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

VOLUMEunder surface proportional

to POWER

Sout herlv seas J

3D PLOTS SEA SET: SU 'b'

IOS data adjusted for 100m water depth and rescaled a t 1/108

"--ow,-- q %., -. - GRAPH 3 . 3 0

Page 67: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

the

I SPECTRA I 'c' set

Nort herb seas

VOLUME under surface proportional

to POWER

3D PLOTS' SEA SET: SU 'cJ

IOS data adjusted for 100m water depth and rescaled at 1/108

GRAPH 3.31

Page 68: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

3D PLOTS SEA SET: SU ' dJ

Page 69: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

4.A SCATTER DIAGRAM EXPLORING

Bending Moment Resul t s

I n graph 4.1 we draw s e t s of sub-graphs of t h e r o o t mean square

bending moment a t each j o i n t along t h e sp ine . The po in t s a r e connected

by s t r a i g h t l i n e s bu t a s t h e r e a r e u sua l ly s o many j o i n t s we g e t t h e

impression of a reasonably f a i r p a t t e r n .

A s i n most of t h e t e s t s i n t h i s r e p o r t we recorded 1024 measurements

from each j o i n t a t a sampling r a t e of 20 Hertz. With 44 j o i n t s t o

t h e model each sub-graph is t h e r e f o r e based on 45,056 measurements

and t h e a r r a y of 39 t e s t s shown on t h i s page needed 1,757,184

observa t ions .

Bending moment s c a l e s a r e given on t h e r i g h t of t h e diagram.

The u n i t s a r e Newton metres a t model s c a l e . They can be convenient ly

read with t h e a i d of a p a i r of d i v i d e r s . The most h ighly s t r e s s e d

j o i n t on t h i s page had an r m s bending moment j u s t under 10 Newton

metres.

Tick marks along t h e top and bottom of t h e diagram allow us t o

i d e n t i f y j o i n t numbers. A t a s c a l e of 107.7 t h e 44 j o i n t model would

cover nea r ly 1.9 ki lometres of s e a , equiva len t t o twelve wavelengths

of a 10 second period wave.

Each sub-graph is l a i d out a s a member of an a r r a y corresponding

t o t h e p o s i t i o n of t h e s e a s t a t e given i n i ts corresponding pox-plot.

I n t h i s case it would be t h e pox-plot on graph 3.2. The reader w i l l

f i n d it he lp fu l t o r e f e r backwards and forwards. The columns show

t h e f a c t o r by which we mul t ip ly t h e Pierson Moskowitz norm f o r each

of t h e va lues of Te shown i n rows. Amplitude and per iod a r e of course

i n t e r r e l a t e d i n t h e P ierson Moskowitz formula. A x2 m u l t i p l i e r f o r

a 1 . 4 second s e a is very l a r g e , with power equiva len t t o 3.75 MWatts/metre

a t f u l l s c a l e .

The mean d i r e c t i o n of t h i s s e a is a t 90° t o t h e l eng th of t h e

sp ine . The c e n t r a l reg ions show o s c i l l a t i o n s about a mean l e v e l with

an inc rease a t each end. Surge moments a r e always bigger than heave

ones. The r a t i o is about two f o r small s eas but f a l l s f o r bigger

ones.

This s e t of measurements was made a t a s t i f f n e s s of 1 ,000 Nm/radians

with a whole sp ine l eng th of 18 metres.

Page 70: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

& A i l & 4 L JOINTS 6 MOORINGS

Hrms IMULTIPLIER 0.25 0.5 1 .O 1.5 2 .O +

Energy PERIOD 0.7 (seconds)

rms maximum BENDING J/ 1 value surge I 0 NOMENT 0.8 / have ( ~ m )

T-l-TTl 1 - 0

1 5 10 1520 JOINT n u m b e r

SURGE & HEAVE JOINTS l o Stiffness: 1000 Nm/rad

exploring the 1.2 SCATTER DIAGRAM 1

L PM spectra,Mi tsuyasu spreading 44joints

1.3 ] P = = = ~ F Z ~ B B sea set: PM 'm'

GRAPH 4.1

UULLULLLLLLLulU IIII/IIIIIIlIIIIIIdu lllllllllLllllllllllI IIIIIIIIIIILLILuLL LLLLLUA

1% 1 :: A - A --- -- -- -- E3

7

1 C" ! E I E Z G X ~ ~ -

t 1

0.9:- ,___ 1

f -- -- -=-I -r ] - B 1

i t

i h e s a & a - --- le23mm; 4 t 1- -_

I -- -- lE??3 ,-m

Page 71: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

In graph 4.2 we have increased the stiffness to 3,500 ~ / m radian.

The very big seas at this stiffness might have damaged our control

motors so we leave blanks.

Page 72: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

C]

6 MOORINGS

Hrms IMULTIPLIER LIULUILLLLILUulU 0.25 l.dldd 0.5 1 .O 1.5 2 .O Energy p uLLU LLUILI~LLLL~UIL IIIIllllllllllllllll~ u.llu LLLUII ILLLLLIl

PERIOD i I- :: 0.7 j t (seconds) -- m B L 0

-- - v===4,l!sss3m ' TmT-FT

1 k

1 5 10 1520 JOINT number

0.9 ] -- ~ Z Z Z ~ H B I 1

SURGE & HEAVE JOINTS loo W- M -- - H ~k St iff ness: 3500 Nm/rad _i' f

1.1 j - WHH t

i 1.2 : t

h L 3 d e G a H 1 f L

1.3 1 7

I 1 ::

1.4 1 t LZ01%J~ ,~*~wn*d l t 0

Iln[n"TTT"F'pl WmlTTT T T n T T I T nnllllllllllPTn W n F T 1 5 10 15 20 1 5 10 1520

GRAPH 4.2

exploring the SCATTER DIAGRAM PM spectra,Mitsuyasu spreading 44joints sea set: PMml

SEAS TOO B I G

Page 73: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

In graph 4.3 we re-plot only the surge results but superimpose

projections to the right column and bottom row. This useful technique

highlights the changes between each test condition. It looks as though

surge bending moments are rising rather less rapidly than wave amplitude.

Page 74: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

(seconds)

P R O J E C T I O N S Hrms -2 0.25 0.5 1.0 1.5 2.0 - -MULTIPLIER ulvulvuLwLuvLwLvrLurluuvlvllvrlvlrlvvvLvlluuluvLu--

& & A h & 6 MOORINGS

Energy PERIOD 0.71

V

l -7 -T-F 1 5 10 1520

JOINT number

- ---p-pF- I k0 a

SURGE JOINTS

rms BENDING MOMENT

Stiffness: 1000Nm/rad - 1.2

the SCATTER DIAGRAM PM spectra,Mitsuyasu spreading 44joints sea set: PM 'm'

GRAPH 4.3

Page 75: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

I n graph 4.4 we re -p lo t t h e surge d a t a bu t d iv ide each va lue

by t h e measured value of H r m s f o r each t e s t . We found t h a t us ing

a d i v i s o r of H r m s t o t h e power 0.8 produces very c l o s e matching i n

t h e r i g h t hand column, sugges t ing t h a t t h i s is t h e r i g h t r e l a t i o n s h i p

between wave amplitude and bending moment f o r surge i n a l l p a r t s of

t h e sp ine .

Page 76: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

P R O J E C T I D N S Hrrns -1 0.25 0.5 1.0 1.5 2.0 ---+ 1-MULTIPLIER &II~~III~I~II -- 111111 --

Energy PERIOD o~~IE~P""?'"Y (seconds)

MOMENT

T-rTmT 0.0

1 5 10 1520 JOINT number

I

SCATTER DIAGRAM PMspectra'Mi tsuyasu spreading 44joints sea set: PMm'

BENDING MOMENTS divided by(Hrms -- GRAPH 4.4

SURGE JOINTS Stiffness: 1000 - Nm/rad

1.2

exploring the

l-~lEEEr-'@,~~ 1 ' E E E P P W I I-~~EEP!~E m[

Page 77: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

I n graph 4.5 we inc rease s t i f f n e s s t o 3500 Nm/rad and then f o r

graph 4.6 we normalise by H r m s t o t h e power 0.8, The same amplitude

t o bending moment r u l e a p p l i e s .

I n graphs 4.7 t o 4.10 e x a c t l y t h e same procedure is c a r r i e d o u t

f o r heave b u t we found t h a t t h e b e s t normal i se r was H r m s t o t h e first

power.

Page 78: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

P R O J E C T I O N S Hrms - 0.25 0.5 1.0 1.5 2.0 - , '7 MULTIPLIER tjlll-1111111---

Energy PERIOD

[11 6 6 4 L JOINTS (seconds)

5 F~ ING 10 MOMENT

m u

1 5 10 1520 JOINT number

SURGE JOINTS St iff ness: 3500 Nm/rad

the SCATTER DIAGRAM PM spectra,Mitsuyasu spreading 44joints sea set: PM 'm'

GRAPH 4.5

Page 79: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

& & & A & L JOINTS 6 MOORINGS

==FT-FF 1 5 10 1520

JOINT number

SURGE JOINTS St iff ness: 3500 Nm/rad

SCATTER DIAGRAM PMspectra,Mitsuyasu spreading

GRAPH 4.6

Page 80: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

& 6 & & & 6 MOORINGS

P R O J E C T I O N S Hrms - 0.25 0.5 1.0 1.5 2.0 - , ?MULTIPLIER 1111111111111111111111---

Energy PERIOD 0.7

HEAVE JOINTS

I * - 7.5

1- --. -- -----, - - Ekl kzzL&&ak:::

pa;igrn Tnds) rms 0.8 ' BENDING 5 @MOMENT

(Nm)

=TTT-T k - 0.0

0.9

' St iff ness: 1000 Nm/rad ~ - 4 ~ ~ r n ~ D exploring the

1 5 101520

i JOINT number

-I

- d c = = = 5 ~ ~ ~ ~

-r--------,- 1 izzxlmm

SCATTER DIAGRAM

1

i

PM spectra'Mi tsuyasu spreading 44joints sea set: PM 'm'

GRAPH 4 . 7

Page 81: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

P R O J L C T I O N S Hrms -> 0.25 0.5 1.0 1.5 2.0 ------+ IMULTIPLIER Ulllltlljlllllllll 111 - IIL_l u u l l I u h ~ ~~ Energy F 3 . 0

0.7 ~ ~ ~ ~ m , ~ -_. t2.0

PERIOD C t . 0 L0.0

(seconds) LL JOINTS 6 MOORINGS

1 5- 1.0 1'5 20 JOINT number

HEAVE JOINTS St iff ness: 1000 - Nm/rad

exploring the SCATTER DIAGRAM PMspectra,Mitsuyasu spreading

1 . 4 1 l r " \ ~ ~ ~ 2 L r m , ~ l @ l P ~ w ~ ~

i l l ~ 3 . 0 44joints sea set: PM 'm' F j I

1 ::: 0 '-r '-T"w '"T-lnrrlmrln nrll""l""T""1" IllrlllllT"'?T Ttl- -l'-T'rrlmT"

C 0 . 0

BENDING MOMENTS divided by Hrms 1 5 10 1520

GRAPH 4.8

Page 82: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

& i t l r ! l 44 JOINTS 6 MOORINGS

P R O J E C r I O N S Hrms - 0.25 0.5 1.0 1.5 2.0 - ,

c---=zzrzh m =TT"=FT 1 5 101520

JOINT number

HEAVE JOINTS Stiffness:3500 Nm/rad

SCATTER DIAGRAM PM spectra,Mitsuyasu spreading 44joints sea set: PM'm'

VIIT TT~*T~'T" TT*TT~ TT+*P~T m ? f - ~ ~ ~ ~ ~ r ~ ~ mafrlTTmrlfmr N 1 5 10 1520 3 1 5 10 1520

m

GRAPH 4.9

Page 83: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

6 44 JOINTS

HEAVE JOINTS St iff ness: 3500 Nm/rad

exploring . . the SCATTER DIAGRAM PM spectra'Mi tsuyasu spreading . I . . . 44jolnt-s sea set: PM m'

BENDING MOMENTS divided by Hrms GRAPH 4.10

Page 84: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

Having shown t h e d i s t r i b u t i o n of bending moment along t h e sp ine

we now want t o e x t r a c t t h e r u l e s f o r o t h e r v a r i a b l e s . Graph 4.11

p l o t s t h e r o o t mean square bending moment f o r a l l j o i n t s i n t h e model

f o r heave and surge a g a i n s t H r m s a t each energy period.

Heave f a m i l i e s a r e very s t r a i g h t , confirming t h e H r m s t o t h e

f i r s t power r u l e . Surge values show t h e H r m s t o t h e power 0.8 e f f e c t .

Heave per iod curves a r e a l l c l o s e , showing t h a t per iod is having

very l i t t l e e f f e c t . Surge per iods a r e a l s o f a i r l y c l o s e except f o r

t h e s h o r t e s t per iod of 0.7 seconds.

Graph 4.12 shows t h a t i nc reas ing t h e s t i f f n e s s t o 3500 Nm/radians

r a i s e s t h e s lope but no t by a s much a s 3.5. I t a l s o seems t o s epa ra t e

t h e surge per iod curves.

I n graph 4.13 we a r e p l o t t i n g s i m i l a r d a t a but draw l i n e s f o r

each j o i n t . The s t i f f n e s s is 1000 Nm/radian. We can s e e t h e bunched

r e s u l t s f o r t h e c e n t r a l r eg ion , two o r t h r e e j o i n t s with h igher values

near t h e end and low ones a t t he very end. We must remember t h a t

heave and surge j o i n t s a l t e r n a t e .

Heave l i n e a r i t y is evident even with such s c a t t e r e d po in t s .

Surge non- l inear i ty is a l s o c l e a r .

I n 4.14 we r e p e a t t h e procedures f o r an increased s t i f f n e s s of

3500 Nm/radian. Everything is exac t ly a s expected.

Page 85: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

exploring the SCATTER DIAGRAM -

BENDING MOMENTS PM Spectra, Mitsuyasu, 44joints :

I (varying Hrms Multiplier &Energy Period)

SURGE

r M S Bend i ng Mornen t (Nm)

r m s Wave Height Ccrn)

HEAVE

STIFFNESS 1000 Nm/rad RMS v a l u e s a v e r a g e d o v e r w h o l e s p i n e

and grouped in fami lie-according t o Te

GRAPH 4.1 1

Page 86: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

exploring the SCATTER DIAGRAM - - BENDING MOMENTS

PM Spectra, Mitsuyasu, 44joints (varying Hrms Multiplier &Energy Period)

SURGE

Bend i ng Moment

r MS

Bend i ng M o m e n t (Nml

HEAVE

STIFFNESS 3500 Nm/rad RMS values averaged over whole spine

and grouped in families according to Te

GRAPH 4.12

Page 87: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

exploring the SCATTER DIAGRAM BENDING MOMENTS

PM Spectra, Mitsuyasu, 44joints (varying k Multiplier 8 Energy Period)

r MS

Bend i ng SURGE

Moment 14.00 CNm>

10.00

0.00 0.00 1 .OO 2.00 3.00

Bend i ng Moment 14.00

HEAVE

- -

.OO 1 .OO 2.00 3.00 r m s Wave Height (cm)

STIFFNESS - - 1000 Nm/rad RMS values a t EVERY JOINT

with c u r v e s fitted

GRAPH 4.13

Page 88: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

exploring - the SCATTER DIAGRAM

r m s Bend i ng Moment 14. (Nml

BENDING MOMENTS PM Spectra. Mitsuyasu. 44joints (varying H m Mukiplier &Energy Period)

SURGE 00

00

00 0.00 1 .OO 2.00 3.00

rms Wave Height ( c m l

r m s Bend i ng HEAVE Moment 14.00 CNm>

r m s Wave Height (cml

STIFFNESS 3500 ~m/ rad - RMS va lues at EVERY JOINT

with curves fitted

GRAPH 4.1 4

Page 89: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

exploring the SCATTER DIAGRAM BENDING MOMENTS

PM Spectra, Mitsuyasu, 44joints (varying Hrms Multiplier &Energy Period)

Bend i ng Moment 14. CNm)

10.

r m s

WHOLE SPINE AVERAGES a

SURGE C3500Nm/radI

SURGE <1000Nm/rad> HEAVE ( 3500Nm/r a d >

HEAVE ( 1000Nm/radl

rms Wave Height Ccml

ENERGY PERIOD : l.Osec Comparisons of SURGE and HEAVE values

for 2 stiffnesses, at fixed Te

0 0

00 -

80 3

GRAPH 4.1 5

I I I

nm,sz6>~,n~,r6l,w mmlvldai

MAXIMUM VALUES SURGE I3500Nm/radl

/'" SURGE (1000Nm/rad> . HEAVE (3500Nm/r ad)

/ I 1 I

0.00 1 .OO 2 .08 3.00 rms Wave Height (cml

Page 90: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

I n graph 4.15 we e x t r a c t t h e maximum value and t h e whole sp ine

averages f o r heave and surge f o r t h e two s t i f f n e s s e s . We were su rp r i s ed

t o s e e t h e heave l i n e s f o r two s t i f f n e s s values i n t e r s e c t i n g a t very

low wave amplitudes. We p r e f e r t o use da t a from l a r g e r samples bu t

a s i m i l a r e f f e c t is ind ica t ed f o r t h e whole s p i n e averages and we

a r e i n c l i n e d t o t r u s t t h e r e s u l t .

The maximum r o o t mean square surge va lue i s more than twenty

times t h e y i e l d l i m i t o f our 1981 reference design. The peak

ins tan taneous value would have been about t h r e e t imes t h e r m s va lue

and so t h e peak-to-yield r a t i o would be about s i x t y . Our preference

f o r c o n t r o l l e d y i e l d p o i n t s seems t o be sound.

Graph 4.16 shows t h e r e l a t i o n s h i p of bending moment t o wave period

f o r cons t an t H r m s . The maximum values occur i n t h e cen t r e of t h e

use fu l energy-generating band but t h e reduct ion t o e i t h e r s i d e i s

bare ly d e t e c t a b l e except f o r t h e very s t i f f e s t condi t ions . Energy

period is t h e l e a s t important va r i ab l e .

GRAPH 4.16rms bending moments (average for all joints) against energy period, for Hrms = l.Ocm

Page 91: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

Graph 4.17 shows superimposed simultaneous plots of surge moment

against heave moment for every joint of a 36 joint model in a 1.0

sec PM cos2 sea. The joint stiffness was 1,000 Nm/rad. The heave

data were obtained by taking the average values of the heave moment

at either of the surge joints.

This method of deriving a synthetic heave measurement for a notional

heave sensor at the position of a surge joint is open to some question

because the correlation coefficient between the two heave joints is

only 0.8. However we found that the rms value of the synthetic time

series is on average only 1% lower than the value of the true time

series.

The plot allows us to judge the accuracy of our estimate that

there is about 90° phase shift between the two channels. It is

interesting to compare this with page 28 of our slamming test report

(ref L).

Each dot represents a probability density of 1 in 18,432.

It is premature to claim that the cost of post-tensioning steel

and joint power plant can be reduced by as much as 25% because these

measurements were taken without the torque limit which would have

occurred at 1.5 Nm. Furthermore we should recall that the narrow

tank variable coefficient work shows that, in many sea states, the

required heave stiffness is a little greater than that for surge.

Nevertheless there are some grounds to hope for savings in capital

cost.

Page 92: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

Instantaneous Bending Moments a i n s t HEAVE

36 j o i n t s x 512 samples 1 sec, PM, C o s 2

s t i f f n e s s : 1000 ~m/rad

GRAPH 4.17

Page 93: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

EFFECTS OF VARYING J O I N T STIFFNESS

We wanted t o know:

a ) How do sp ine bending moments vary with j o i n t s t i f f n e s s ?

b ) Are surge bending moments independent of heave s t i f f n e s s ?

c ) Are heave bending moments independent of surge s t i f f n e s s ?

We used t h e same Pierson-Moskowitz s e a throughout wi th an energy

period of 1 second, a measured H r m s of 1.26cm and Mitsuyasu spreading.

The sp ine was 18 metres long with 44 a c t i v e j o i n t s and 6 moorings.

We va r i ed surge and heave s t i f f n e s s independently i n 6 s t e p s between

250 and 8000 Nm/rad, doubling t h e value a t each change.

Graph 4.20 shows t h e bas i c r e s u l t s with bending moment a r r a y s f o r

surge and heave p l o t t e d toge the r . Except where otherwise marked, t h e

top curve i n each p l o t is surge . The heave a r r a y s tend t o be about h a l f

t he s i z e of t h e surge a r r a y s f o r equal surge and heave s t i f f n e s s e s .

Surge bending moments tend t o be about 50% higher near t h e ends than

they a r e i n t h e middle, bu t i n heave t h e r e s u l t s a r e more even.

Page 94: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

6 MOORINGS

effect of JOINT STIFFNESS on Bending Moments independently varying Surge and Heave stiffness

SAME sea throughout : l.OseclPM,Mitsuyasul (pml04m) Hrms: 1.26cm 44 joints

250 500 1000 111I1I1IIIIItlltlllllllltlilf---

HEAVE St iff ness Nm/rad 500

3 1000 1 lczrZ.5- rms

10 ENDING 2000 I / MOMENT (Nm) L ? z z z r l m B

0 1 1 1 1 1 1 1

t 5 Ib 15 20

JOINT number

Page 95: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

Graphs 4.21 and 4.22 show t h e d a t a s e p a r a t e l y i n surge and heave

with t h e a r r a y s a l s o c o l l e c t e d toge ther i n t o ' p r o j e c t i o n s ' a t t h e ends

of rows and t h e bottoms of columns. We f i n d t h i s a u s e f u l way o f

summarising t h e e f f e c t s of t h e 2 v a r i a b l e s . Note t h a t t h e surge v e r t i c a l

s c a l e is twice t h e heave one.

On t h e surge page (graph 4 .21) , t h e r i g h t hand column of p r o j e c t i o n s

summarises t h e e f f e c t of varying surge s t i f f n e s s . Each doubling of

s t i f f n e s s produces an approximately equal increment i n t h e bending

moment. The row of p r o j e c t i o n s a t t h e bottom shows t h a t surge s t i f f n e s s

v a r i a t i o n s have very l i t t l e e f f e c t on heave bending moments.

Page 96: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

Moments independently varying Surge and Heave stiffness

SAME sea throughout: l.Osec,PM,Mitsuyasu, (pmlO4m) e. Hrms: 1.26cm 44 joints

P R O J E C T I O N S

v 1 5 I0 1520

JOINT number

I--.E~B pml04m

GRAPH 4.21

Page 97: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

On t h e heave page, (graph 4.22) t h e row of p r o j e c t i o n s a t t h e bottom

again shows t h a t heave bending moment increments a r e about cons t an t f o r

doublings of s t i f f n e s s . But t h e column of p r o j e c t i o n s a t t h e r i g h t shows

a l i t t l e more ' c r o s s t a l k ' than is v i s i b l e on t h e surge page. A t low

heave s t i f f n e s s e s heave bending moments i n t h e middle of t h e sp ine tend

t o i nc rease with surge s t i f f n e s s , while a t high heave s t i f f n e s s e s

bending moments a t t h e ends tend t o g e t smal le r . However t h e e f f e c t s

a r e small and it is s a f e t o say t h a t , f o r engineering purposes, t h e two

d i r e c t i o n s a r e independent. We cannot r e l i e v e t h e surge bending moments

by running away i n heave. We had hoped t h a t t h i s would be poss ib l e when

we discovered t h e death v a l l e y e f f e c t ( s e e page 4.1 of our 4 t h year

repor t , r e f b ) .

Page 98: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

1 i

L JOINTS

ef f e d of JOINT STIFFNESS on Bending Moments --

independently varying Surge and Heave st iff ness SAME sea throughout: l.Osec,PM,Mitsuyasu, (pml04ml

Hrms: 1.26cm 44 joints

HEAVE joints 250 500 1000 2000 4000 8000 ....E..I..$

-vivuLwlv.rlv--IUrllllllllllllllllII--lllllllnllllllllllllI--

HEAVE 250 St iff ness

lzEIIEl-mmmm

Nm/rad

El5 MOMENT

v 0 . 0

1 5 10 1520

JOINT number

AA5.U I d e g s m l -70 4 4 0 - 2 0 0 +20+4O+M ,n rIrn 10 lsecordsl

a5 C

pmlOr*m T 0

N 1 S

2 o o o j l " - - ? ~ ~ ~ ~ ~ 40001mmmmmL"? 80oo~mmm~"y my""?

~ l l l ~ l l l l ( ~ ~ ~ ~

I 5 I0 1520 I 5 I0 15 20

GRAPH 4.22

Page 99: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

Summary of E f f e c t s of Varying J o i n t S t i f f n e s s : graphs 4.23 and 4.24

Graph 4.23 shows t h e d a t a re -p lo t ted t o i l l u s t r a t e t h e r e l a t i o n s h i p

between s t i f f n e s s and bending moment.

Separa te curves a r e drawn i n surge and heave f o r :

1. t h e r m s bending f o r t h e most h ighly s t r e s s e d j o i n t ;

2. t h e average of t h e r m s bending moment f o r t h e middle s i x j o i n t s ;

3. t h e average of t h e r m s bending moments of a l l t h e j o i n t s .

The top graph has a l i n e a r ho r i zon ta l s t i f f n e s s s c a l e , and t h e

bottom one has a l o g s c a l e .

The cu rva tu re s a t t h e l e f t on t h e upper p l o t do n o t suggest ze ro

bending moments f o r zero appl ied s t i f f n e s s e s , and some r e s i d u a l r eac t ion

fo rces a t t h e j o i n t a r e c l e a r l y i nd ica t ed . The j o i n t c o n t r o l system

( s e e s e c t i o n 2 ) had a r a t h e r low c losed loop-gain of about 2.7 i n t h e

conf igura t ion used f o r t h e lowest s t i f f n e s s experiments, implying t h a t

t h e background s t i c t i o n and damping of t h e j o i n t s would only be reduced

t o about 40% of t h e inhe ren t va lues . Since t h e s e experiments we have

a l t e r e d feed back cu r ren t va lues t o allow more loop-gain a t very low

s t i f f n e s s .

The l o g p l o t s a r e remarkably s t r a i g h t from 500 Nm/rad upwards.

However t h e h igher s t i f f n e s s values w i l l i n f a c t be modified by t h e

inherent compliance of t h e sp ine u n i t s ( s e e s e c t i o n 6.E), s o t h a t t h e

bending moment graphs should r e a l l y be compressed ho r i zon ta l ly a t t h e

r i g h t . This is done on t h e next page.

Page 100: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

effect of JOINT STIFFNESS on Bending Moments independently varying Surge and Heave s t i f f ness

44 joints l.OsecfPMfMitsuyasuf Hrms: 1.26cm

+0 - I I t I 1 1 , , I

LOG scale I , . I - r m s

SURGE tmVE Bend i ng x c maximum values +

Momen t A V average of middle 6 joints n O average of all joints

/hrms

(NM/cm> 5-

.

10 * b * l * * * l l * * l * * l l l l . l 1 1 1 1 . 1 1 1 . 1 . 1 . .

LINEAR scale

0 ) , I I [ 3 c o t 3 ~ b b f i @ ~ p ~ ~ ~ d a t I I 250 500

I

1000 I

2000 4000 8000 Joint Stiffness <NM/radl

rrns SURGE HEAM Bend i ng- x +- maximum values

sw/ __ --

S V R G E ~ A Y ALL. /- - --

---------- 5 M & ~ ! ! ' 4 = A

----:------------- -- N U ~ ~ MA% +

_*-C-SC---C---- ------ NUIA~~* - I m y & ~ ~ - - A L L

0 LW,326] S,H@&?NOMM-~&

1 ' . ' 1 ' . . ~ ' . ' ~ ' . . ~ ' l . l l ' . , . , , l , .

GRAPH 4.23

- - - - - - - - -

0 1000 2000 3000 4000 5000 6000 7000 8000 Joint Stiffness CNM/rodl

Page 101: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

Graph 4.24 shows r m s bending moments p l o t t e d a g a i n s t s t i f f n e s s

with t h e nominal s t i f f n e s s va lues ' c o r r e c t e d ' u s ing t h e va lues suggested

i n t a b l e 6.7 ( s e c t i o n 6.E) . Upward tendenc ies a r e v i s i b l e i n t h e l o g

p l o t s f o r t h e maximum va lues , though t h e average va lues f o r t h e whole

sp ine a r e f a i r l y l i n e a r over t h e range of s t i f f n e s s e s from 1000 t o 5000

Nm/rad .

The r e s u l t s of v a r i a b l e c o e f f i c i e n t c o n t r o l i n t h e narrow tank l ead

us t o b e l i e v e t h a t t h e d e s i r a b l e j o i n t s t i f f n e s s w i l l be much lower than

we had expected when t h e model w a s designed and we do n o t propose t o

improve high s t i f f n e s s performance.

Page 102: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

effect of JOINT STIFFNESS onBendingMoments

with estimated s t if fness CORRECTIONS

LINEAR scale Bend i ng Moment / h r ms

Bend i ng Moment

1 " ' 1 " ' 1 " ' 1 " ' 1 " ' 1 " ' 1 ' " 1 ' .

0 1000 2000 3000 4000 5000 6000 7000 8000 Joint Stiffness CNM/radl

LOG scale SURGE HEAVE

x -+ maximum values A v average of midd le 6 j o i n t s R 0 average o f a1 l joints

- . . . . . . . . 2150 5'00 10'00 20'60 40'00 8000 J o i n t Stiffness CNM/radl LOG SCALE

GRAPH 4 . 2 4

Page 103: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

4.C EFFECT OF VARYING SEA OFFSET ANGLE AND ENERGY PERIOD

A l l p rev ious t e s t s used s e a s wi th a mean approach angle o f 90° ,

i . e . w e s t e r l i e s h i t t i n g a s p i n e l y i n g nor th-south .

I n t h i s s e c t i o n we vary both t h e approach d i r e c t i o n and t h e energy

per iod . The amplitude w a s he ld t o t h e P ie rson Moskowitz norm f o r each

energy per iod . S t i f f n e s s was 1000 Nm/rad throughout and t h e Mitsuyasu

spread was used throughout. The pox-plot f o r t h e s e t e s t s is t h a t of

graph 3.4. The r e s u l t s a r e given i n graph 4.30.

Cen t r a l approach d i r e c t i o n s have equal a m p l i f i c a t i o n s of bending

moments a t each end as expected from previous work.

O f f s e t approach angles r a i s e t h e moments a t t h e down-wave end and

depress those a t t h e windward end. The r a t i o approaches 3 : l f o r

40 degree o f f s e t .

When surge bending moments a r e normalised by d i v i s i o n by H r m s t o

t h e power 0.8 we can s e e on graph 4.31 a f l a t c e n t r a l reg ion f o r low

va lues o f Te bu t a t t h e l onges t ones t h e r e is a r i s e with d i s t a n c e a long

t h e sp ine .

The accumulations p r o j e c t e d t o t h e right-hand column show a very

n i c e symmetry,at l e a s t a s far a s a Te of 1 .4 seconds. They a l s o show

t h a t t h e r e is more bending moment skew a t longer Te.

Graph 4.32 shows t h e same e f f e c t s a r e p re sen t bu t l e s s pronounced

f o r normalised heave.

Page 104: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

Offset SEA OFFSET ANGLE and ENERGY PERIOD F ANGLE &-> (degrees) maximum Energy 44 joints

PERIOD 10 B ~ D I N G

MOMENT Nrn/rad (Nm) pectra, ~ i t s u ~ a s u spreading; sea set: PM'a'

Q ? ? Q ? 1 1 I I i T I I I

I 1 L

0 (seconds) 6 6 d k i - r p - m p m i 6 MOORINGS 1 5 1 8 ,s 20

SURGE & HEAVE I JOINT number

GRAPH 4.30

Page 105: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

effect on Bending Moment of varyhg -

t nergy

(seconds)

Offset ANGLE

(degrees)

6 r ! l i l & 6 MOORINGS

SEA OFFSET ANGLE and ENERGY PERIOD St i f f ness: 1000 Nm/rad 44 joints

PMspectra, Mitsuyasu spreading; sea set: PM'a'

SURGE NORMALISATION: data divided by (~rrnsf' +30 +40 P R o J L c T x o H s

rl"l""l'"'l'"'l"--"T'III11TIII1(IIlrlnrlnplrilrlrrll-nrln---- 1 5 I0 1520 1 5 I0 I5 20

GRAPH 4.31

Page 106: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

effect on Bending Moment of varyhg -

t nergy PERIOD

Offset I ANGLE -> (degrees)

6 MOORINGS

SEA OFFSET ANGLEand ENERGY .- PERIOD - -. - - --

St if fness: 1000Nm/rad 44 joints PM spectra, Mitsuyasu spreading; sea set: PM 'a'

I HEAVE . NORMALISATION: data divided by Hrms

GRAPH 4.32

Page 107: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

4.D EFFECT OF VARYING SEA OFFSET ANGLE AND SPREAD

I n t h i s s e r i e s we va r i ed angular spread ( t h e va lue o f S i n t h e toss spreading f u n c t i o n ) and angular o f f s e t , keeping energy per iod cons t an t

a t 1 second and s t i f f n e s s cons t an t a t 100 Nm/rad. The pox-plot is g iven

i n graph 3.5.

It i s n o t s u r p r i s i n g t o s e e i n graph 4.40 t h a t narrow spreads

gene ra t e wide v a r i a t i o n s of bending moments f o r small o f f s e t angles

whereas wide s e a s wi th s = 2 show no change with angle . A spread of

s = 2 is a l i t t l e wider than Mitsuyasu. The Mitsuyasu func t ion is more

t i g h t l y bunched a t i ts c e n t r a l per iods and angles ( s e e pox-plots 3.4

and 3 .5 ) .

It is very unusual t o s e e t h a t , f o r 1 0 degrees o f f s e t and t h e

narrowest sp read , t h e heave moments a t one j o i n t exceed t h e surge value.

The normalised r e s u l t s on graphs 4.41 and 4.42 show t h a t heave

maxima occur a t about 10 degrees of o f f s e t whereas surge maxima

a r e a t 20°.

Page 108: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

effect on Bending Moments of varying SEA OFFSET ANGLE and SPREAD 44joints

Stiffness:1000Nm/rad

rn 1 5 10 1520

JOINT number L & h k z s ~ M LE9Bw-w

- Irlrl""l["'1'"[[['m--lrlrr

1 5 10 15 20 1 5 10 1520

GRAPH 4 .40

Page 109: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

effect on Bending Moments of varying - SEA OFFSET ANGLE and SPREAD Stiffness: 1000Nm/rad 44joints

PM spectra,Te:l .Osec,Coss spreading sea set: CO'a'

NORMALISATION: data divided by (~rrnsf' Spread 0 10 20 30 40 50 p R O J L c T I o N s - EXPONENT -"""".-- -"""". - - - -

GRAPH 4.41

this page: SURGE Bending Moments 128

~ ~ I F E E P E E 1- I/--n [d

i i

Page 110: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

GRAPH 4 . 4 2

effect on Bending Moments of varyhg SEA OFFSET ANGLE and SPREAD Offset Stiffness: 1000Nm/rad 44joints

ANGLE -> PM spec tra,Te:l .Osec,CosS spreading sea set: CO 'a'

(degrees) NORMALISATION: data divided by Hrms Spread 0 10 20 30 40 50 p R o J L c T I O _ N S

7

EXPONENT

4 this page: HEAVE Bending Moments 128 11

I 1 512 [I1 d b b f i i

4 4 JOINTS 6 MOORINGS

'infinity1 P

ij 1 I 0 N S

' wIljll-----

2lrni,,mai"" .̂mmJ:::

* I D B B H ~ ~ 321m~1"lic"\~r--?

1- F\ m, b 2

rzl l c h c z 3 ~ ~ ~ L ~4r13mu-!,,

i i i i

J- i

k+--=q M m3wmA& l ; mm-m-m-

1 5 10 15 20 1 5 10 15 20 -

Page 111: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

4.E BENDING MOMENTS I N THE SOUTH UIST SPECTRA

In t h i s s e r i e s of t e s t s we use t h e IOS s e t o f 46 s p e c t r a measured

a t South U i s t . (The s e l e c t i o n procedure is descr ibed i n s e c t i o n 6.G).

The surge and heave bending moments of t h e 46 ' a ' s e t a r e shown

on graph 4.50. Model length was increased t o 48 j o i n t s and t h e s t i f f n e s s

was held a t 1000 Nm/radian. It is i n t e r e s t i n g t o look a t t h e normalised

surge r e s u l t s i n graph 4.51 i n which bending moments a r e divided by

measured ~ r m s ~ * ~ - Compare r e s u l t s f o r s e a s 220 and 223 and then look

a t t h e i r pox-plots on graph 3.6.

We s e e l i t t l e end-enhancement f o r low spread s e a s , f o r example 201,

210, 212, and some asymmetrical enhancements p red ic t ab le from our e a r l i e r

o f f s e t t e s t s .

I n normalised heave (graph 4 .52 , in which s c a l e is doubled) we s e e

much l e s s d i f f e r e n c e between seas . Look aga in a t 220 and 223.

Test 378 shows r e l a t i v e l y more enhancement than f o r t h e

corresponding surge r e s u l t .

Page 112: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

827 Q++Q

w. v 1 5 10 1520 JOINT number

'a' set

Bending Moments in the South Uist 46 SPECTRA St iff ness: 1000 - Nm/rad

sea set: SU 'a '

; & & & A h & L8 JOINTS 7 MOORINGS SURGE & HEAVE joints

--

GRAPH 4.50

Page 113: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

L *3g 1 I

""l-Tm'r-r- 1 5 10 1520 JOINT number

'a' set

rms BENDING MOMENT ( Nm)

Bending Moments in the South Uist 46 SPECTRA NORMALISATION : data divided by ( ~rrns)O~

&joints St iff ness: 1000 Nm/rad sea set: SU 'a '

r ; & 2.l A r; 7 MOORINGS SURGE joints

-

I(lljll(lllllllllltllltl-----w 18

~ 2 3 8

1 1 7 r m r l r l m 1 I l 1 l r I ) l l l 1 l I I o l l T n 1 1 ~ m T m T 1 - " T m r T m t ~ ~ n n l r m l n n - y l r l l l l l n ~ p m l r r n p m 1 5 10 1520 1 5 10 1520

GRAPH 4.51

Page 114: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

- 1 5 101520 JOINT number

'a' set

Bending Moments in the South Uist 46 SPECTRA NORMALISATION : data divided by Hrms

Bjoints St iff ness: 1000 Nm/rad sea set: SU'a'

1 1 I I 6 6 6 6 d 48 JOINTS 7 MOORINGS HEAVE joints

GRAPH 4.52

Page 115: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

For t h e next s e r i e s of t e s t s we va r i ed t h e t o t a l model l e n g t h ,

keeping t h e 46 ' a ' s e t and 1000 Nm/rad j o i n t s t i f f n e s s .

The r e s u l t s on graph 4.53 a r e f o r 36 j o i n t s and on graph 4.54 a r e

f o r 22 j o i n t s . For graph 4.55 we use a 22 j o i n t model swung round t o

t h e South ' b t s e r i e s of s e a s . The r e s u l t s a r e c l o s e t o t h e ' a t s e r i e s

with t h e except ion of s e a number 3.78. Relevant pox-plots a r e graphs

3.6 and 3.7.

Graph 4.56 shows t h e r e s u l t s of t e s t i n g 22 j o i n t s i n t h e ' d t s e r i e s

s e a s . The mir ror image r e v e r s a l f o r s e a 359 is b e a u t i f u l l y shown. There

is a wide d i f f e r e n c e f o r s e a 223 between graph 4.56 and 4.54. Again

t h e pox-plots on 3.9 and 3.6 show why.

The s e r i e s of graphs 4.57 t o 4.61 is an exac t r e p e a t of t h e previous

group with t h e s t i f f n e s s increased t o 3500 Nm/rad. The shapes of t h e

a r r ays a r e s i m i l a r , and t h e only obvious e f f e c t of changing s t i f f n e s s

is t o i nc rease bending moments i n a l l j o i n t s and i n a l l s ea s .

Page 116: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

nr7rnlllmTrrlllllll 1 5 101520 JOINT number

rms BENDING MOMENT I Nm)

Bending Moments in the South Uist 46 SPECTRA

6 6 5 MOORINGS

S t iff ness: 1000 Nm/rad sea set: SU 'a '

SURGE & HEAVE joints

4

' 9 0 p j -2 -4 -8 -9 -2

1 W - W 9 ks$* ks& r1° C w, h1 LP~%]s~~~,M~SU~MF+.~ .z G "" C

nrryllrlmlmfTrm "'TT-Jt"Tm mrlcrr V'""PnTtnll"'flfT "' '"7'mT'"T'T" mrlrmTT- nnl"nrllllllT 1 5 10 1520 1 5 10 1520

Ir

GRAPH 4 .53

I 1 PECTRA

'a' set

IIII1IIb ,,LJuhdUllllt)lllt ,Ld,du'l,& ,.u&dd&

1 p_--- b 089 4\08 -2 i ~ z 2 a , b b m 1 22 1 54 1 68 171 177

* i : r r , , - -8 G-c? ,, 1 3@ 228 !zzz2!2 238 ,-- 24 1 - 242 b 244 - 249 IbL-, 267 V\rzzl. 268

4

1 i F

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-

GRAPH 4.54

10 Bending Moments in the South Uist 46 SPECTRA

L O & [ $ 22joints - St iff ness: 1000 Nm/rad

359 - sea set: SU 'a ' - S/OS 1 5 10 1520 JOINT number %f SURGE & HEAVE joints

FI PECTR A 'a' set 1

- (Illltlllllllljtll-(ItlllllllfflILtlllll(lIIIII1IIIJ11hLh--

,. 10

D e 089 L

1 08 La&

1.1.2 b

1 22 1 54 kz% 1 68 l.k& , 171 Id&&

1 77 i.., 1, 180 ESh 200 -. 20 1 w=e%!zs 21 0 - 21 2 f2S9

21 8 LEA 220 - 223 i i@!4 228 k 2 238 - 24 1 ~ 1 9 b Le!?=s

242 244 249 l&Lh 267 E2s3

I,rn E%?l 291 - 292 E% 294 - 318 - 31 9 b 322 141 324 268 i 3- 336 - 346 l @ ! A A b H M h [ 347 352 355 359 360 366

b ? l @ J ! ? d 4 B k 37 1 377 378 38 1 388 39 1 ~!3343263~1, Wl9nrnA .ol&

-I"." v v v -r"'F"Tmllm T T T m r p m 1 5 10 1520 1 5 10 1520

i :

Page 118: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

1 5' 1s 1'5 20 JOINT number

p I PECTRA

rms BENDING MOMENT (Nm)

Bending Moments in the South Uist 46 SPECTRA

'b'set

2 - joints S t iff ness: 1000 Nm/rad sea set: SU 'b'

SURGE & HEAVE joints

GRAPH 4.55

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T'W 1 5 101520 JOINT number

PECTRA 'd'set

rms BENDING MOMENT ( Nm)

0

Bending Moments in the South Uist 46 SPECTRA

22 JOINTS13 MOORING

St iff ness: 1000 Nm/rad sea set: SU 'd

SURGE & HEAVE joints lllllltltlltllllll&uul-l"."Illll.tltltlllLtllltlllIlllllt)l(llltltltlllltt&L--

i;: 1 k4 223 E 1 E 1 i 1 i 1 [ ~ @ @ $ @ , @ Y J O M ~ * ~

m v m l r l l l r T l r r p V W W T W 1 5 10 1520 1 5 10 1520

GRAPH 4 .56

Page 120: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

Bending Moments in the South Uist 46 SPECTRA &joints St iff nessz3500 Nm/rad

sea set: SU 'a '

JOINT number CI

18 JOINTS 7 MOOR/NGS SURGE & HEAVE joints ,,.uhLI1Llll(lllll.ljllll111111111 IIIIIII11II1II1 IJlljllttlllttll1111.1111- 11111- I11I.I,,.i,."J-l- &'.duAd-L,,,,

'a' set --- - 089 108 112 J & z = Z Z % ~ ~ ~ ~ 1 22 1 54 1 68 171 177

- ~ = = = = z ? ? - = +

- - 228 24 1 242 244 249

""r"T'=r"''P" TFflrrrlTm v rlllrmlnlllrllllm v ' " - ' r " r p f T ' ~ rlT- rmPmTmtlrnrpm 1 5 10 1520 1 5 101520

GRAPH 4.57

Page 121: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

TnmTm 1 5 101520 JOINT number

PECTRA 'a' set

0 @:DING MOMENT

0 ( Nm)

Bending Moments in the South Uist 46 SPECTRA

5 MOORINGS

S t iff ness: 3500Nmhad sea set: SU 'a '

SURGE & HEAVE joints

GRAPH 4.58

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rntP'~l7nrrlrm 1 5 10 1520 JOINT number

10 FSNDING MOMENT

0 ( Nml

Bending Moments in the South Uist 46 SPECTRA 22 joints - St iff ness: 3500 Nm/rad

sea set: SU 'a '

SURGE & HEAVE joints , . u ~ L L ~ l l l l t l IlllltUlfllllllllll ,,,,l-JJLItILLLLLILI &ILJII& w- &LItllllflltIt &&

'a' set ICkL 089 h 1 08 Cs=c2\ L&& 1 54 V\, 1 68 171 l.&i 1 77

112 L a

1 22

GRAPH 4.59

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"'T"Tm'l-l- 1 5 10 1520 JOINT number

1 0 ~~~ESNDING MOMENT 1 Nrnl

Bending Moments in the South Uist 46 SPECTRA 22 joints - St iff ness: 3500Nm/rad =

sea set:SU1b'

SURGE 8 HEAVE joints

GRAPH 4.60

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JOINT number

PECTRA 'd' set

l 0 FSNDING MOMENT INml

Bending Moments in the South Uist 46 SPECTRA St iff ness: 3500 Nm/rad

sea set: SU 'd'

SURGE & HEAVE joints

GRAPH 4.61

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4.F EFFECT OF STIFFNESS VARIATIONS IN SOUTH UIST SEAS

In this series of experiments the 46 'a1 set seas are used on a

48 joint model with three different stiffness values; 1000, 3500 and

5000 Nm/rad.

Graphs 4.70 and 4.71 show the raw data for the three stiffnesses.

Graphs 4.72 and 4.73 show them normalised by division by Hrms.

The very small heave bending moments for sea 122 look suspiciously

jagged when normalised and we suspect a communication fault for the left

hand half of the spine.

In general, the relationship of bending moments to stiffness follows

the approximately logarithmic pattern shown in graph 4.23 of section

4B, with little change between stiffnesses of 3500 Nm/rad and

5000 Nm/rad. However, the difference between the down-wave peaks in

strongly offset seas is greater than expected when the stiffness

increases from 1000 Nm/rad to 3500 Nm/rad. Sea number 220 is again the

obvious example. It is reasonable to hope that lower model stiffness

will reduce the severity of down-wave enhancement.

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1 5 101520 'OS JOINT number

sed PPF

Bending Moments in the South Uist 46 SPECTRA 3 St i ff nesses : 1000,3500,5000 Nm/rad

&joints St iff ness: 1000 Nm/rad

! ! I ; / / a o o o o l 8 JOINTS 7 MOORINGS

sea set: SU 'a '

' SURGE joints -

-(IIII1-*----

PECTRA 'a' set l i e E % s 3 - d - h h & [ & 089 1 08 112 1 22 1 54 1 68 171 177

GRAPH 4.70

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,,vl,l,, ' 0 . 1 5 10 1520 JOINT number

S ~ d PQf

'a' set

Bending Moments in the South Uist 46 SPECTRA 3 Stiffnesses: 1000,3500,5000 Nm/rad

& , ! I 0 1 8 JOINTS 7 MOORINGS

St iff ness: 1000 - Nm/rad sea set: SU'a'

HEAVE joints

III?(II1/11101lljnnnnlll l l l l lr l l l l l l lm-m

GRAPH 4.71

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-6 l l l l T ~ ~ T l l ~ l T 1 ~

1 5 10 1520 JOINT number

Bending Moments in the South Uist 46 SPECTRA data 'normalised' 3 St i f f nesses : 1000,350015000 Nm/rad

by d i v i d i n g b y ~ ~ r m s P 8 - &joints St iff ness: 1000 Nm/rad

l i i ! . . 1 1 0 0 0 C J C J O ~ 18 JOINTS 7 MOORINGS

sea set: SU'a'

PECTRA 'a' set

I - @ % z F v t

GRAPH 4.72

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1000 Nm/rad Bending Moments in the South Uist 46 SPECTRA

(Nml

I B~DING data 'normalised' 3 St i f f nesses : 1000,3500,5000 Nm/rad MOMENT

by dividing by Hrms - &joints S t iff ness: 1000 Nm/rad ~ n ~ " 1 q I T l r r "

1 5 10 1520 'O.Y sea set: SU 'a' 'Qd pQf

JOINT number O c l C l r 3

18 JOlNrS 7 MOORINGS HEAVE jo

PECTRA 'a' set

GRAPH 4 . 7 3

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4.G SHAPE OF BENDING MOMENT DISTRIBUTION I N SOUTH UIST SEAS

I n t h i s s e c t i o n we a r e t r y i n g t o show t h e shape o f t h e d i s t r i b u t i o n

o f bending moment a long t h e sp ine . Data from t h e previous t e s t s a r e

s ca l ed t o make t h e maximum va lue t h e same f o r each t e s t . For example

i n graph 4.80 t h e double hump i n s e a 223 was u s u a l l y t o o small t o show

up wel l even i n normalised p l o t s .

We p l o t su rge and heave s e p a r a t e l y f o r l eng ths o f 48, 36 and 22

j o i n t s wi th s t i f f n e s s he ld cons t an t a t 1000 Nm/rad.

Heave r e s u l t s a r e g e n e r a l l y f l a t t e r t han su rge bu t s e a s 228, 224

and 378 a r e except ions ( s e e graph 4 .83) .

We a r e susp i c ious of t h e first t h r e e r e s u l t s on graph 4.83. The

reduced moment f o r one j o i n t i n s e a 089, which is ad j acen t t o r a i s e d

moments on e i t h e r s i d e , i s c h a r a c t e r i s t i c o f a loose model j o i n t ( s e e

s e c t i o n 4.M).

Shortening t h e model by a f a c t o r of two has removed t h e asymmetry

of 223, bu t i n gene ra l shape is no t much changed by sho r t en ing ( s e e

f o r example s e a 366) .

The s h o r t e s t model was swung round t o be t e s t e d i n t h e ' b ' and ' d l

South U i s t s e a s . The b igges t changes a r e f o r s e a 346 i n graph 4.86 and

223 i n graphs 4.88 and 4.89. A l l t h e o t h e r s look very much l i k e t h e i r

' a ' s e r i e s ve r s ions .

More l eng th v a r i a t i o n s a r e given i n s e c t i o n 4.K.

Note t h e s t r i k i n g s i m i l a r i t y of s e a s 201, 210, 212, 291, 292, 322

and 336. We s e e t h a t t h e r e a r e c e n t r a l moments very c l o s e i n va lue t o

end peaks.

We can a l s o n o t i c e t h e s i m i l a r i t y o f t h e pox-plots i n graph 3.6.

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MOMENT 1- '0.0 VK '0s

1 5 101520 S ~ ~ e f JOINT number

Bending Moments in the South Uist 46 SPECTRA self-scaled to show SHAPES of arrays

!&joints St iff ness: 1000 Nm/rad sea set: SU 'a '

SURGE joints

GRAPH 4.80

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mm(lsed BENDING MOMENT

id L 0 . 0 -v '0s

1 5 10 1 5 2 0 S@dr@f JOINT number

Bending Moments in the South Uist 46 SPECTRA self-scaled to show SHAPES of arrays

48joints - Stiffness: 1000Nm/rad --

sea set: SU'a'

6 6 A A & L8 JOINTS HEAVE joints

GRAPH 4.81

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D Q ~ M BENDING MOMENT

I-* ' -0.0 -y /os

1 5 10 1 5 2 0 JOINT number

sQf@f

Bending Moments in the South Uist 46 SPECTRA - self-scaled to show SHAPES of arrays

L6 joints Stiffness: 1000Nm/rad --

sea set: SU 'a '

& l ! I i l l ! I & 36 JOINTS 5 MCh3RINGS SURGE joints

t 5 101520

GRAPH 4.82

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DP&& BENDING MOMENT

JOINT number

p ' i PECTRA

'a' set

Bending Moments in the South Uist 46 SPECTRA self-scaled to show SHAPES of arrays

34 joints S t iff ness: 1000 Nm/rad sea set: SU 'a '

HEAVE joints

GRAPH 4.83

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Bending Moments in the South Uist 46 SPECTRA 110mk4d

P3 , il:l BENDING self-scaled to show SHAPES of arrays

MOMENT 22 joints St iff ness: 1000 Nm/rad - -

-y '0s sea set: SU 'a ' 1 5 10 1 5 2 0 S~+Qf JOINT number SURGE joints

1 5 101520

GRAPH 4.84

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Bending Moments in the South Uist 46 SPECTRA -- - -- --

self-scaled to show SHAPES of arrays - 22 joints St iff ness: 1000 Nm/rad

il sea set: SU 'a'

JOINT number

GRAPH 4.85

Page 137: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

m d c d BENDING MOMENT

LJ 378 L 0 . 0 -y 'OS

1 5 10 1 5 2 0 sed ref JOINT number

Bending Moments in the South Uist 46 SPECTRA - - - - - --

self-scaled to show SHAPES of arrays 2 joints S t iff ness: 1000 -- Nm/rad

sea set: SU 'b' I SURGE joints I

'b' set

GRAPH 4.86

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normaksd BENDING MOMENT - 346 L O . O

-7 '0s 1 5 10 1 5 2 0 S ~ d ref JOINT number

' b' set

Bending Moments in the South Uist 46 SPECTRA - self-scaled to show SHAPES of arrays

22joints Stiffness: 1000 Nm/rad sea set: SU 'b'

HEAVE joints

GRAPH 4.87

Page 139: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

pi, IIQT~B~~sE! BENDING MOMENT

1 ' -0.0 -\ los

1 5 10 1 5 2 0 Sed ref JOINT number

FI PECTRA

'd' set

Bending Moments in the South Uist 46 SPECTRA self-scaled to show SHAPES of arrays

a jo in t s Stiffness: 1000Nm/rad sea set: SU 'd'

SURGE joints

GRAPH 4.88

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11mm BENDING MOMENT

1 5 10 1 5 2 0 JOINT number

p 1 PECTRA

Id' set

Bending Moments in the South Uist 46 SPECTRA self-scaled to show SHAPES of arrays

u j o i n t s Stiffness: 1000 Nm/rad sea set: SU 'd'

joints

1 t 1 1

1.0

[?@,%I rnl~OnQ-IW

11111(111]11111111111111rlllrlll111111(---7- 1 5 10 1520 1 5 101520

GRAPH 4.89

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4.H BENDING MOMENTS I N ANGLED MONOCHROMATIC WAVES

By t h i s s t a g e i n t h e t e s t s it was c l e a r t o u s t h a t by f a r t h e most

i n t e r e s t i n g phenomenon w a s t h e enhancement of bending moment a t t h e down

wave end of t h e sp ine . We formed a theory t o exp la in t h e e f f e c t and

c a r r i e d ou t t h e next s e r i e s of t e s t s i n monochromatic waves t o t e s t it.

We were i n t e r e s t e d i n c r e s t l e n g t h , c r e s t angle and c r e s t v e l o c i t y

and we va r i ed them toge the r with energy per iod f o r two sp ine s t i f f n e s s e s .

The r e s u l t s a r e dramatic. Look a t graph 4.90 f o r 40° c r e s t angle and

1 .6 seconds per iod . The surge t r a c e shows growing c y c l i c a l v a r i a t i o n s

of bending moment as we move along t h e sp ine . The behaviour is repea ted

f o r s h o r t e r pe r iods and smal le r o f f s e t angles so t h a t a group of s i m i l a r

p l o t s l i e on a diagonal of t h e page. The v io lence of t h e v a r i a t i o n s

seems t o be growing a s we move t o longer per iod and b igger o f f s e t s .

Despi te t h e f a c t t h a t t h e s e a s were nominally t h e same amplitude

(1.414 cm) we g e t bending moment v a r i a t i o n of a t l e a s t 20 : l f o r t h e same

o f f s e t angle and even more i f we change o f f s e t and per iod .

In graphs 4.91 we have normalised t h e r e s u l t s by d iv id ing by t h e

measured value of wave amplitude t o c o r r e c t f o r any minor v a r i a t i o n s

and superimposed rows and columns a t bottom and r i g h t .

The heave r e s u l t s i n graph 4.92 show s l i g h t l y l e s s dramatic changes

bu t neve r the l e s s t h e e f f e c t is c l e a r l y v i s i b l e f o r 0.8 second per iod

and -10 degrees of o f f s e t . The number of humps decreases from 4 t o 2

a s t h e per iod inc reases .

A l l t h e t e s t s s o f a r descr ibed i n t h i s s e c t i o n were c a r r i e d ou t

with a s t i f f n e s s of 3500 Nm/rad. When i n graph 4.93 we c u t s t i f f n e s s

t o 1000 Nm/rad we can s e e t h a t t h e enhancement r i d g e is moved t o b igger

o f f s e t angles . Normalisation and superpos i t ion of rows and columns i s

as before.

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monochromatic seas effect on Bending Moments of varyhg CREST ANGLE and Energy Period

Crest ANGLE->

(degrees)

monochromatic 20 rms

BENDING 1 0 MOMENT n (Nml

seas, Hrms: 1.414cm sea se t :MO1a'

SURGE & HEAVE joints

P'ERIOD JOINT number

-1 0 -20 -30 -40 -50 - 60 -70 -80 (seconds) -I,,,,- ----I,,,,

DcoJQ W ~ M J h A &T

- ~ = ~ . ~ c r o a d ~ t E C - - - --

1.4 r & z E e G 3

1.6 1 - lizes 1 5 10 15 20 1 5 10 15 28

GRAPH 4.90

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monochromatic seas effect on Bending Moments of varykg CREST ANGLE and Energy Period

Crest - b. ANGLE^-> monochromatic seas, Hrms: 1.414cm sea se t :MO'af

(degrees) NORMALISATION: data divided by ( ~ r m s f SURGE joints P~RIOD . -10 -20 -30 -40 -50 -60 -70 -80 P R O J E C T I O N S - (seconds)

>

1 5 18 1-5 20 -U.lllllllllllllttllJIIllllllllljlltlllllllII----

1.0 - . - - - - - . " - . - - -

GRAPH 4.91

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monochromatic seas

effect on Bending Moments of varying CREST ANGLE and Energ.y Period

Crest 44 joints St if fness3500Nm/rad

monochromatic seas, Hrms: 1.414cm sea set :MO1a' ANGLE->

' F i d e g r e e s ) NORMALISATION: data divided by Hrms HEAVE joints

GRAPH 4.92

P'ERIOD . I 5 -10 16 IS 20 -20 -30 -40 -50 -60 -70 -80 1 5 10 15 20

P R O J E C T I O N S ____B

(seconds)

4 1.0

1.2

-LAAA -LLLL -J-LAA - ...11....1....1..11111- - - - 0*8m~__-- - - - G '4. r -- [I

is--.; k2cclE3=e?3-----

j k G c l G i 3 b V l _ _ , u - - - 4

1 I F

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monochromatic seas

effect on Bending Moment y Period 44 joints St iff ness:1000 Nm/rad

-> monochromatic seas, Hrms: 1.414cm sea set :MOta'

NORMALISATION: data divided by joints P'ERIOD . 1 5 10 IS 15 20 -20 -30 -40 -50 -60 -70 -80 I 5 10 15 20

P R O J E C T I O N S ___B

(seconds) ..................... ...................... ...................... ...................... ...................... .................... - - - J/ 0.8 1 l Z l d ! ~ ~ - ~ - - -

1.0 1 E;: -

GRAPH 4.93

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Next, i n graphs 4.94 t o 4.96, we c a r r i e d out a f r e s h s e r i e s of t e s t s

i n which t h e v a r i a b l e is c r e s t l ength . For a s i n g l e wavefront s e a we

def ine c r e s t l e n g t h a s t h e d i s t ance a long t h e sp ine between p o i n t s of

t h e same phase. Some sub-graphs a r e missing because they would l i e

ou t s ide t h e tank envelope. Once aga in we s e e t h e same p a t t e r n of

p rog res s ive ly inc reas ing bending moments a s we move down-wave along t h e

sp ine . The obl ique r idge has moved nea r ly t o t h e v e r t i c a l . The maximum

surge va lues a r e between 5 and 6 metres c r e s t l eng th , independent of

per iod.

Surge moments g e t worse with longer per iods bu t i n graph 4.96 t h e

oppos i te is t r u e f o r heave. Note t h e sp lendid e f f e c t f o r 6 metres a t

1 .0 second.

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monochromatic seas

effect on Bending Moments of varying - CREST LENGTH - and Energy Period 44jo ints St i f fness:WOONm/rad

monochromatic seas, Hrms:l.Ocm sea s e t :MO 'b'

&[~:%& (Nm)

SURGE & HEAVE joints T T " T T r T T T F

1 5 10 15 20

~ERIOD JOINT number

(seconds) 2 4 5 6 7 8 I0 12 lllllllillIf&111-I1I1IIIII11UlllllljlI1111III1III1IIII1IIII1-*&

[~co,U6pm ~ ~ B c h t 1 5

w&m-- -- t l 0 0

GRAPH 4.94

Page 148: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

monochromatic seas effect on Bending Moments of v a r y g - CRESTLENGTH a n d Energy Period

44 joints St iff ness:1000 Nm/rad monochromatic seas, Hrms:l.Ocm sea set :MO 'b'

P R O J E C T I O N b

ekZ22!---.--

- LcIz ! ! eEa - - -

GRAPH 4.95

Page 149: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

monochromatic seas effect on Bending Moments of varying - CREST LENGTH and Energy Period

Crest monochromatic seas, Hrms:l.Ocm sea se t :MO 'b'

t- LENGTH-> NORMALISATION: data divided by Hrms HEAVE Joints (metres)

(seconds)

1.6 P R

1 1 1 I 0 n s nq~n~[:n~p-q"mrlnlq~ir l imp rmlrrn lrnrpmpi r n r p ~ r p rn l r q n mpmp-qtnqt~ nqrnrprlrrrrpl mqmrpnpntp rn~lt-m rr1npnq-n ~ T T - n lnl ~lni~yit

1 5 10 15 20 1 5 18 I5 20

GRAPH 4.96

2 4 5 6 7 8 10 12 P R O J E C T I O N S - ~I~ILIJIILLLU LLLLLUJ~IJLI[IULLLI U I L ~ L U L L I U L L U U U L L U J I U L U L L U I A L L I U U I L I & ~ d ~ l & ULLLULLJLILUILLU U+LLJLJLIULI~U LLLLL~uuIuLJIJ

1- l!?'?Xl -- - - - -. Mkf!!!!ma-- -

- .- - - - - iru4EYkW MMm-m - --

t i t

Page 150: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

Our next v a r i a b l e is t h e v e l o c i t y of t h e c r e s t a s it moves along

t h e sp ine . Graph 4.97 shows heave and surge superimposed f o r a s t i f f n e s s

of 3500 Nm/rad. Peak surge va lues a r e always b igger than peak heave

except i n t h e top r i g h t t e s t . The maximum enhancement f o r heave occurs

a t 8m/sec (it might st i l l have been g e t t i n g b igge r ) and 0.8 seconds

whereas t h e surge e f f e c t is b igges t a t 4 rn/sec and 1.6 seconds.

In graphs 4.98 and 4.99 we s e p a r a t e heave and surge and superimpose

rows and columns t o emphasise t h e wide range of v a r i a t i o n . While o n e ' s

eyes a r e n a t u r a l l y drawn t o t h e most dramatic r e s u l t s we should not

overlook t h e 8 m/sec 1 .6 s e c en t ry on graph 4.98, which has a peak-free

f l a t response. This is what a naive expec ta t ion might have been bu t

it is extremely r a r e f o r long sp ines . The only o t h e r examples i n t h i s

r e p o r t a r e f o r r a t h e r s h o r t l eng ths .

Next we reduced t h e s t i f f n e s s t o 1000 Nm/rad f o r graphs 4.100 t o

4.102. Note t h a t t h e v e r t i c a l s c a l e is a l s o changed. I n both surge

and heave t h e maximum enhancement has moved t o t h e l e f t , i . e . toward

slower c r e s t v e l o c i t i e s , and t h e number of humps has increased from 4

t o 5.

Page 151: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

monochromatic - - - . -- seas e f fec t on Bending Moments - of varying - CREST VELOCITY and Energy Period

j 1 1 ! 1 / 6 tj 6 0 6 b

44 JOINTS . 6 MOORINGS

1 5 1'0 1'5 20 J O I N T number

monochromatic seas, Hrms:l.Ocm sea set :MO 'c'

PERIOD 2 3 4 5 6 7 8

GRAPH 4.97

Crest SURGE & HEAVE joints (m/sec) TVE L ° C ' T y ~

( second s)

0.8

u~ru ~LL&& U L L A ~ ~ ~ ~ U L A U ~ I I U L I L L L I U U M I U ~ ~ U L L ~ YULU ULJI LJI& ~ L U L U -

? j _, ?a&-- -- - --

I L--sc-wd

'I r

Page 152: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

monorhromat ic seas effect on Bending Moments of varyhg - [REST VE LOCITY - - and Energy Period

GRAPH 4.98

Page 153: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

monochromatic seas e f fec t on Bending Moments of varying - CREST VELOCITY and Energy Period

44 joints S t iff ness:3SOONm/rad - - monochromatic seas, Hrms:l.Ocm sea se t :MO 'c'

SATION: data divided by Hrms P R O J E C T I O N S

7-[/YCCh?wm

1*2jL ----,-v--JY G S w s \ w m r c c 2 / f l *

--

W s -"l'-' " T T " T m mrirrrr lnm m nnlnrrlrllrTrmln Trrrln~Tmrln 771'nfrrrrln ""TrnT

1 5 10 15 20 1 5 10 15 20

GRAPH 4.99

Page 154: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

jnonochromat ic seas ef fect on Bending Moments of varying - CREST VELOCITY and Energy Period

[I] il r!l

4G JOINTS 6 MOORINGS

&joints - St if fness:lOOQNm/rad monochromatic seas, Hrms:l.Ocm sea set :MO 'c'

Crest SURGE & HEAVE joints (m/sec) IVE L°C'TY-+

r - m ~ r r ~ rprrr1 m i q n

1 5 10 15 20 JOINT number

PERIOD 2 3 4 5 6 7 8

GRAPH 4.100

(seconds) 4 Oo8 vv~vllull~urlu uu~urlwllrvr~u u l r ~ u r l ~ ~ h UILU WLULMLIA ~~ - -

f I

Page 155: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

monochromatic seas ef fect on Bending Moments of varying - CREST VELOCITY and Energy Period

44 joints St iff ness:1000 Nm/rad - monochromatic seas. Hrms:l.Ocm sea set :MO 'c'

P R O J E C T I O N S

L c L c Q L l r ~ y i l E 1 / ~ - i ? m

- l a . z 5 L e j / l h ? S E - w

- w@@m--

GRAPH 4.101

Page 156: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

rnonochromat ic seas e f fec t on Bending Moments of varying - CREST YELOCITY -- -- and Energy Period

W o i n t s Stiffness:1000Nm/rad - monochromatic seas, Hrms:l.Ocm sea s e t :MO 'c'

ON: data divided by Hrms HEAVE joints P R O J E C T I O W S

~ ~ V ? " w v \

LcekCkl P-wmM--

N s 1 - r n r-1 I-lmT-FT rrrrTrmllllllrrrr;n rn 7 - -

1 5 10 15 20 1 5 10 15 20 Y

GRAPH 4.102

Page 157: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

Our next v a r i a b l e was t o t e s t c r e s t v e l o c i t y a g a i n s t per iod f o r

s h o r t e r l eng ths and two s t i f f n e s s e s . Graph 4.103 f o r 28 j o i n t s shows

t h a t t h e maximum value of t h e peaks is about t h e same and occurs i n

nea r ly t h e same t e s t condi t ions . There is only room f o r 2 o r 3 peaks

but otherwise t h e r e s u l t s a r e very c l o s e t o those f o r longer l eng ths .

Clear ly t h e l eng th is not t h e cause of t h e enhancement. The unusual

zero r i p p l e surge r e s u l t f o r 8m/sec and 1.6 seconds on graph 4.98 does

no t occur on 4.104 although t h e r e a r e two such r e s u l t s f o r heave on

4.105.

Cut t ing t h e s t i f f n e s s f o r t h e 28 j o i n t sp ine (graphs 4.106 t o

4.108) shows t h e same le f tward movement of maximum enhancement and r a t h e r

l e s s r i p p l e i n surge f o r t h e h igher v e l o c i t i e s . V e r t i c a l s c a l e s a r e

changed.

Cut t ing t h e l eng th even more t o 16 j o i n t s i n graphs 4.109 t o 4.111

f o r 3500 Nm/rad g ives us l o t s of s i n g l e hump r e s u l t s . There is a

suspic ion of double humps beginning i n t h e top l e f t diagonal of t h e

diagram. The maximum value has dropped but nowhere near a s much a s a

l eng th squared r u l e would p r e d i c t . Cut t ing t h e l eng th by t h r e e has

reduced peak bending moment t o about two t h i r d s . However, i f we average

t h e va lues of t h e h ighes t peak of a long sp ine with i t s adjacent t rough

( (24 + 4.0) + 2 = 14 Nm on graph 4.98) t h e r e s u l t is l e s s than t h e

16 Nm peak i n t h e c e n t r e of a s h o r t sp ine on graph 4.110. We expect

t h a t bending moment enhancement w i l l be u s e f u l l y suppressed by t h e

presence of j o i n t genera t ion and t h a t power-generating j o i n t s i n long

sp ines w i l l be s u b j e c t t o lower f l u i d loading than t h e concre te of s h o r t

sp ines . The presence of ducks w i l l a l s o reduce t h e e f f e c t s .

Graphs 4.112 t o 4.114 show t h e 16 j o i n t sp ine with s t i f f n e s s reduced

t o 1,000 Nm/rad. V e r t i c a l s c a l e s a r e changed. I n surge t h e a r r ays a r e

more o f t e n doubly humped t h a t a t 3,500 Nm/rad. I n heave t h e peak bending

moments occur a t a longer per iod and a s h o r t e r wave v e l o c i t y .

Page 158: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

monochromatic seas e f fect on Bending Moments of varying - - CREST VELOCITY and Energy Period

3 - joints St if fness:3500Nm/rad monochromatic seas, Hrms:l.Ocm sea s e t :MO 'c'

Crest SURGE & HEAVE joints

(m/sec) IVE PERIOD (seconds)

MOMEN

T r r r 1 1 n rr 1 1 1 l?n 0

1 5 10 15 20 JOINT number

1.4

GRAPH 4.103

Page 159: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

monochromatic seas

GRAPH 4.104

effect on Bending Moments of varying - CREST VELOCITY and Energy Period Crest - 28 joints St i f fness:350ONm/rad

monochromatic seas, Hrms:l.Ocm sea s e t :MO 'c' (m/sec) RMALlSATlON : data divided by(Hrrns) O8 SURGE joints

3 4 5 6 7 8 P R O J E C T I O N S

PERIOD & r l u ~ ~ U -AWL& &dud& YlilLULLY'LlLLLY U L J U U d - . L Y I d -L".J.U~U d.-.L-"..J-L

t2@ i ':

I

(seconds) 4

- w LC!!

1.0 j - k d l l.23

- Lcb4 E

W$&#~MO~M~& N m v 7 T T " '-"lmT"m n rrlrrrrlrrrllrlrlTrr"TT"rrln '-rrrirmlnrrTmrTn ITnI-rl" mrlmnnm

1 5 10 15 20 1 5 10 15 20

1.41

1.6 P

!izh LC!!

] w m C S \ U r , , r \ ikd'l

Page 160: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

monochromatic seas e f fec t on Bending Moments of varying - CREST VE LOCITY --- .- - and Energy Period

Crest 28 joints St if fness:35OONm/rad - VE LOCITY

/m/sec) monochromatic seas, Hrms:l.Ocm sea s e t :MO 'c'

ISATION: data divided by Hrms' HEAVE joints

G R A P H " 4.105

P'ERIOD ,,ul.uLJLLLLUILI 2 3 ,J.duLIULLUJLU 4 u'luluuu 5 , , . d U L ~ ~ L J ~ L 6 w 7 L4ALLdmu9-- 8 7

P I O J E C T I O N S ____e_

(seconds)

J, 1.0

0-81- kz=KL. w w j LCdYh B

p kg i 0.0

t

Page 161: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

monochromatic seas ef fect on Bending Moments - of varying - CREST VELOCITY and Energy Period -

a j o i n t s Stif fness:lOOO Nm/rad monochromatic seas, Hrms: l.Ocm sea set :MO 'c'

SURGE & HEAVE joints Crest

PERIOD 2 3 4 5 6 7 8 (seconds) uduLuLurlu u u L u I W urrluuluuluh ududwLullu u d r w L u r U vvlvuLurluuLu

OW8 j- !ksseG

4-

M rn - w t

1 - =T-rT-P

L4222 1 5 10 15 20

JOINT number

L d ? F h rrnFT-r"lT mrlrmFTmrFrrnTm7""pmF rmpmPT-"'r"

1 5 18 15 20 I- T T ~ r ? ' m l " rrrrlrmrnl-m?n

-- 1 5 10 15 20 J

GRAPH 4.106

Page 162: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

Sea Set: PM 'm' 'Scatter Diagram Explorer' Graph 3.2

This is a basic set of Pierson-Moskowitz spectra with energy

period and Hrms varying independently. We use a modification of the

standard PM spectrum as described in our 4th year report, (see ref

b, page 6.9).

The directional spread is based on the Mitsuyasu formula discussed

in ref b, page 6.10.

We limited the spectral frequencies to the range 0.5 to 3.0 Hz,

corresponding to periods of 0.33 to 2.0 seconds. The noticeable

similarity between the patterns of dots shows that the same random

number seed was used throughout to initiate the choice of angles.

For a standard Pierson-Moskowitz spectrum the theoretical value

of Hrms is related to energy period by:

Hrms (cm) = 1.361 ~e'

Wavemaking geometry sets limits on the range of wavefront frequencies

and angles (section 6.D), so the realisable Hrms is reduced. The amount

of this reduction clearly depends on the energy period and the directional

spread of each spectrum. The seas here all have Mitsuyasu spread

with mean direction of zero degrees, so the reduction in Hrms due

to angular limits is low and virtually constant at 1.5%. The tank

frequency limits have varying effects. Hrms is reduced by only 0.5%

at an energy period of 1 second, but this increases to a maximum of

3% at 1.4 seconds. The combined effect is to reduce the realisable

Hrms values from 2% to 4.5%.

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monochromatic seas effect on Bending Moments of varying -- CREST VELOCITY - and Energy Period

28 joints Stiffness:1000Nm/rad - monochromatic seas. Hrms:l.Ocm sea se t :MO 'c'

P R O J E C T I O N S

GRAPH 4.107

Page 164: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

GRAPH 4.108

monochromatic seas effect on Bending Moments of varying - CREST V E L O o r g n e r g y - Period

Crest a joints Stiffness:1000Nm/rad monochromatic seas, Hrms:l.Ocm sea s e t :MO 'c'

(m/sec) ON: data divided by Hrms HEAVE joints 3 4 5 6 7 8 P R O J E C T I O N S

____e_ PERIOD u l ~ l , , l ~ u l , ~ l , l l ~ ...................... ...................... ..................... ...................... ...................... - - 7

k?!E!l

(seconds)

k 3 3 W M M W U M M

1.2

1.4

- j

Page 165: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

monochromatic seas effect on Bending Moments of varying - CREST VELOCITY and Energy Period

monochromatic seas, Hrms:l.Ocm sea set :MO 'c' Crest SURGE & HEAVE joints

(seconds)

I 5 10 1'5 20 JOINT number

GRAPH 4.109

Page 166: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

monochromatic seas ef fect on Bending Moments of varyhg - CREST VELOCITY and Energy Period

16 joints St if fness:35OONm/rad monochromatic seas. Hrms:l.Ocm sea set :MO 'c'

O8 SURGE joints : data divided by (Hrms)

~ ~ ~ w m mrTTm- T r p v l T rrrrTmrT.7nTn'T-l m r " . T r m T n V ~ T r r t T m r T n ri"lr"-'PnlmrTn

GRAPH 4.1 1 0

Page 167: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

monochromatic seas effect on Bending Moments of varying - CREST VELOCITY and Energy Period

16 joints S t iff ness:35OONm/rad monochromatic seas, Hrms:l.Ocm sea se t :MO 'c'

ON: data divided by Hrms P R O J E C T I O N S

GRAPH 4.11 1

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monochromatic seas ,effect on Bending Moments of varying - CREST VELOCITY and Energy Period

6 JOINT= MOORING

16 joints Stiffness:1OOONm/rad monochromatic seas, Hrms:l.Ocm sea s e t :MO 'c'

SURGE & HEAVE joints Crest

(m/sec) IVE L°C'TY-+ PERIOD 2 3 4 5 6 7 8

i r r l r l n r r l 11 ITn

1 5 10 15 20 JOINT number .I

f

GRAPH 4.11 2

Page 169: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

monorhromat IC seas ef fect on Bending Moments of varyhg - CREST VE -- LOUTY - - and Energy - Period

16 joints St if fness:1000 Nm/rad monochromatic seas. Hrms:l.Ocm sea set :MO 'c'

O8 SURGE joints ON: data divided by(Hrms1 P I O J E C T I O N S

GRAPH 4. I 1 3

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monochromatic seas effect on Bending Moments of varyiog - CREST VELOTI -- TY and Energy Period

- -

crest 16 jo ints S t if fness:1000 Nm/rad monochromatic seas. ~ r m s : l . ~ c m sea set :MO 'c'

: data divided by Hrms HEAVE joints 3 4 6 7 8 P R O J E C T I O N S

____e_

7.5

I4 u t 1:: D t

GRAPH 4 . 1 1 4

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4.5 EFFECT OF LENGTH I N SOUTH UIST SEAS

In t h i s s e c t i o n we a r e t r y i n g t o i d e n t i f y t h e var ious e f f e c t s of

l eng th changes. Three d i f f e r e n t l eng ths , 48, 36 and 22 j o i n t s a r e t e s t e d

i n t h e South U i s t s p e c t r a a t two d i f f e r e n t s t i f f n e s s va lues . The s c a l e

f o r each sepa ra t e s e a is adjus ted t o make t h e maximum moment i n t h e

s h o r t e s t sp ine equal t o u n i t y .

The r e s u l t s of l eng th changes a r e l e s s obvious than f o r a l l t h e

previous v a r i a b l e s of s t i f f n e s s , c res t -angle , c r e s t - l eng th ,

c r e s t -ve loc i ty , energy per iod and wave amplitude.

In some c a s e s i nc reas ing t h e l eng th makes bending moments b igge r ,

i n some cases t h e oppos i te . I n some cases t h e in te rmedia te l eng th has

t h e l a r g e s t moments. But even i n s e a 220 t h e changes a r e no t v i o l e n t .

Seas 280 and 318 (graph 4.123) show a lef t -hand peak f o r a s h o r t sp ine

and a right-hand peak f o r a long one.

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ef fec t of LENGTH on Bendinq Moments

ISPECTRAJ 'a' set

S C A L I N G For each sea the relative values of Bending Moments for the 3 different lengths are correct. They are scaled so that the maximum Bending Moment in the

3 different Lengths: 22,36,48 joints

S m joints St iff ness: 3500Nmhad

shortest spine i s unity. sea set: SU 'a' - ---- - -l-l-L, ---- e

3. ,& - u u L L u l a - a d A uuLuuLU;LA~,l,,,,, 1

GRAPH 4.120

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ef fec t of LENGTH on Bendinq Moments

SPECTRA 'a' set

S C A L I N G For each sea the relative values of Bending Moments for the 3 different lengths are correct. They are scal ;d so that the maximum Bending Moment in the shortest spine is unity.

3 different lengths: 22,36,48joints

HEAVE joints Stiffness: 3500 Nm/rad

sea set: SU 'a'

GRAPH 4.121

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SPECTRA 'a' set

S C A L I N G For each sea the relative values of Bending Moments f o r the 3

ef fec t of L E NGTH on Bendinq Moments

different lengths are correct. They are scaled so that the maximum Bending Moment in the

3 different lengths: 22,36,48joints

SURGE joints Stiffness: j000 Nm/rad

- shortest spine is un i t y . sea set: SU 'a'

GRAPH 4.122

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ef fect of LENGTH on Bendinq Moments S C A L I N G For each sea the relative values o f Bending Moments for the 3 different lengths are correct They are scaled so that the maximum Bending Moment in the shortest spine i s unity.

3 different lengths: 22,36,48 joints

HEAVE joints Stiffness: 1000 Nm/rad

sea set: SU 'a'

GRAPH 4.123

Page 176: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

The d i f f i c u l t y of i n t e r p r e t i n g t h e graphs 4.120 t o 4.123 l e d us

t o t r y r e p l o t t i n g the same d a t a i n graphs 4.124 and 4.125. Here we use

t h e s h o r t e s t s p i n e a s a r e f e rence and p l o t South U i s t r e s u l t s f o r o t h e r

lengths i n terms of t h e i r r a t i o t o t h e s h o r t e s t .

Data a r e s epa ra t ed i n t o t h e maximum s i n g l e h ighes t va lue , t h e mean

of t h e e n t i r e sp ine and t h e mean of t h e c e n t r a l t h r e e . Each s e a is shown

a s a s h o r t dash, t h e r o o t mean square of a l l t h e r e s u l t s as a longer

one, and t h e mean of a l l a s t h e longes t dash. A s some of s eas g ive

i d e n t i c a l r e s u l t s wi th in t h e p l o t t i n g r e s o l u t i o n , they a r e repea ted a s

sideways histogram blocks.

No c l e a r p a t t e r n emerges. We might have thought t h a t i nc reas ing

length was inc reas ing bending moment bu t sometimes t h e 36 j o i n t model

has higher va lues than t h e 44 j o i n t one. While we s e e low heave r e s u l t s

f o r both longer lengths i n graph 4.124 we f i n d t h e oppos i te when

s t i f f n e s s is reduced i n graph 4.125. The only c e r t a i n conclusion is

t h a t t h e length squared and l eng th cubed t h e o r i e s a r e i n c o r r e c t f o r t hese

lengths and s t i f f n e s s va lues .

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1 . 6 Bending Moment , $

ratio

1.2

,effect of LENGTH 0n-q- 3 different lengths: 22,36,48 joints

South Uist 46 spectra : SU1cl

SURGE HEAVE B E E D I N G M O M E N T R A T I O

A G A I N S T S F I N E L E N G T H + " " " '

- - rms - mean

-

E E N D I N G M O M E N T R A T I C A G A I N S T S P I N E L E r J G T H

I . ! .

- mean L

MAXIMUM -single - highest value - I

! 4 -

! 2 -

I

0 8 -

. I " " " ' . " ' + 1 .6 - - rms i

Bending - - Ploment 1.4 - ratio

I i 1 . 2 -

0 . 8 -

0 . 6 , - , , 0 10 20 30 4 0 50 60

+ " " I '

1 6 - - rms - - mean 1 I I

1 . 4 - P 4 -

1 .2 -

1 0

0 .8-

0 6 0 20 30 40 50 60

0 10 20 30 4E 58 GC

L Id :' i'i 1

reference iq length -=&? = * - J .O------------------X---------- --- -- -2- --- -

: 14 I-

0 6 ; . , . . . 1

RMS - of ALL joints

-

t " " " " " ' 1.6- - rms -

Bending - - mean Yoment ! , 4 - - rat l o

1.2-

3 . 8 -

0 6 , . . . . 0 10 28 30 40 50 60

Number of J o ~ n t s I . . . I ' " ' ~ " - " ' " " " ' '

0 5 113 15 20 Length (metres)

Number of J o ~ n t s \ . . . , . . . . , . . . ' I . ' ' r ' ' . -

0 5 1 e I S 26 Length (metres)

-

1 .6 -

1 .4-

RMS - of MIDDLE 3joints @,%I S,H L $ , ~ + ~ S U ~ A . + . . 1

' ~FECTRAI STIFFNESS 3500 -- Nm/rad

C " " " " " "

GRAPH 4 . 1 2 4

- rms - mean i I

Page 178: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

effect of LENGTH on Bending Moments 3 different lengths: 22,36,48joints

South Uist 46 spectra : SU1c'

SURGE HEAVE

I MAXIMUM -single highest value --

t " " " " ' L

1 . 6 - - rms m e a n

t Bending - ?- Eoment , 4 - rotic

1 .2 -

E.8-

0 . 6 , . . . 9 . . . 8 0 1 e 20 30 40 59 60

r

t ~ ' ~ ' " ' ' ~ " . C

1 6 - - r m s - mean

1 . 4 - i

1.2- ;-i -

) 4

8 . 8 -

0 . 6 . 0 10 20 30 4C 50 6@

RMS - of ALL joints

i ' " " " " ' ~

1.6- - rms - - m e a n Bending -

Momen! : , r; - rot lo

1.2-

1

b . 8 -

8 . 6 , 0 10 20 30 40 58 6e

Number o t Joints > . . . I

0 5 10 i 5 20 Length (metres)

RMS - of MIDDLE 3 joints ~lo0~326\s.~i (61,03,d? SMA.+

STIFFNESS 1000 Nm/rad GRAPH 4.125

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4.K EFFECT OF LENGTH I N ANGLED MONOCHROMATIC SEAS

I n t h i s s e c t i o n we cont inue t h e s ea rch f o r a theory f o r length-

e f f e c t s . We use monochromatic wavefronts , varying both c r e s t v e l o c i t y

and per iod f o r two s t i f f n e s s va lues and f o r t h r e e s p i n e l eng ths . The

s h o r t e s t sp ine l eng th is p l o t t e d more heav i ly t o a s s i s t i d e n t i f i c a t i o n .

'Telegraph-poles ' a r e added t o mark t h e maximum va lues .

Resu l t s a r e a l i t t l e c l e a r e r than f o r t h e South U i s t s ea s . For

surge a t 3500 Nm/rad i n 4.130 it looks a s though t h e longer l eng th sp ine

r e s u l t s a r e p ivo ted about t h e maximum o f t h e s h o r t one. Only f o r 8 m/sec

and 0.8 seconds i s t h e r e a dramatic enhancement f o r a l l t h e l eng th o f

t h e longer s p i n e s . This is accompanied by a g r e a t r educ t ion a t t h e

bottom o f t h e 8 m/sec column. The o v e r a l l enhancement e f f e c t s vanish

f o r t h e lower s t i f f n e s s i n graph 4.132, which shows p ivo t ing n e a r l y

everywhere. I n heave on graphs 4.131 and 4.133 t h e p a t t e r n is s i m i l a r .

Corresponding histograms a r e given on graphs 4.134 and 4.135.

Rat ios up t o 3 .5 a r e ev iden t bu t t h e r e a r e a l s o some depress ions . I n

graph 4.134 t h e c e n t r a l j o i n t s a r e a s low a s 0.35 o f t h e s h o r t e s t sp ine .

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PERIOD (seconds)

The line for the shortest spine is thickened to help separate it from the other 2 1 ' I nes .

e f fect of LENGTH on Bending Moments 3different lengths: 16,28,44 joints

S C A L I N G For each sea the relative values of Bending Moments for the 3 SmF; joints

Crest different lengths are correct. ~h~~ are scaled SO that the Stiffness: 3500Nm/rad maximum Bending Moment in the E LOCIT~-> shortest spine is uni ty. Monochromatic sea set: MO'C'

(m/sec) 2 3 4 5 6 7 8 1 &Ah------ I

GRAPH 4.130

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effect of LENGTH on Bendinq Moments 3different lengths: 1628~44 joints

PERIOD (seconds)

The line for the shortest spine is thickened to help separate i t from the other 2 lines.

S C A L I N G For each sea the relative values of Bending Moments for the 3

HEAVE joints Crest different lengths are correct.

They are scaled so that the Stiffness: - 3500 Nm/rad

maximum Bending Moment in the ELOCITY~-> .,ortestspine isunit,. Monochromatic sea set: MO1c' (m/sec) 2 3 4 5 6 7 8

, l l t l l t d ! 1 L u l d d u b - - - - &&--A& 0.0 1.0

GRAPH 4.131

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PERIOD (seconds)

Crest

ef fect of LENGTH on Bendinq Moments 3different lengths: '& 28,44 joints

S C A L I N G For each sea the relative values of Bending Moments for the 3 different lengths are correct. Thev are scaled so that the

S m joints Stiffness: Nm/rad

maximum Bending Moment in the shortest spine is unity. Monochromatic sea set: MO'C'

4 5 6 7 8

The line for the shortest spine is thickened to help separate it from the other

1.2 2 I ' I nes .

GRAPH 4.132

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ef fec t of LENGTH on Bending Moments

The line for the shortest sp i ne is thickened to help separate i t from the other

I nes . 2 1 '

PERIOD (seconds)

I

3different Lengths: 16 28,44 joints S C A L I N G For each sea the relative values of Bending Moments for the 3

HEAVE joints Crest different lengths are correct.

he^ are sca I ed SO that the Stiffness: Id000 Nm/rad maximum Bending Moment in the E LOCITY'-> .,,test spine is uni L,. Monochromatic sea set: MO1c'

(m/sec) 2 3 4 5 6 7 8 I 1

~ 1 1 1 1 1 1 1 1 I 1 1 1 1 I 1 1 , I I I I I I ~ I I I I - - - - - 0.8 1

1.6 1 ~ M ~ M , W M ~ 1m-w-m-

1 5 10 15 20 1 5 10 15 20

GRAPH 4.133

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3 different lengths: 16,28: 44 joints Monochromatic sea set: MO1c'

SURGE HEAVE

MAXIMUM -single - highest value (near end)

B E N D I N G M O M E N T R A T I O B E N D I N G M O M E N T R A T I O A G A I N S T S P I N E L E N G T H I A G A I N S T S P I N E L E N G T H

I - rms 3.0 - mean 2 .5

2.0

1.5

1.0 ------------++---- 0.5

0.0 , 0 10 20 30 40 50 60

Bend i ng Moment 3.0 ratio

2.5

2.0

I .5

1.0

0 .5

0 . 0 .

RMS - of ALL ioints

3 . 5 ' . 1 . 1 . 1 . t . . q - rms - mean !I

>

------------x------

I . I . I . I . 1 . I

2

1 .o:-------------x------- 0.5

0 . 0 . . , . , . , . , . , . . 0 10 20 30 40 50 60

Number of J o b L 0 $ 10 15 20

0 10 20 30 40 50 60 0 10 20 30 40 50 60

Length (metres)

RMS - of MIDDLE 3 joints O~~,UJS,H OZ,O~,OBMO~C.M

STIFFNESS 350OA Nm/rad GRAPH 4 . 1 3 4

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effect of LENGTH on Bending Moments 3 different lengths: 16,28,44 joints

Monochromatic sea set : MO1cl

SURGE HEAVE B E N D I N G M O M E N T R A T I O

A G A I N S T S P I N E L E N G T H B E N D I N G M O M E N T R A T I O / A G A I N S T S P I N E L E N G T H

MAXIMUM -single highest value (near end)

RMS - of ALL ioints

0 10 20 30 ' . . . . . "

1 Q Length (metres)

RMS - of MIDDLE 3joints m~%,s,l ~ , ~ , ~ l u l o r W I c . w

STIFFNESS 1000 Nm/rad GRAPH 4 . 1 3 5

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4.L EFFECT OF MOORING MODIFICATIONS

If t h e s a f e t y o f an i n s t a l l a t i o n depends on t h e i n t e g r i t y o f i ts

moorings t h e r e must be s t r i n g e n t r u l e s about i n spec t ion . We wanted t o

f i n d ou t whether bending moments would be changed by t h e l o s s of

moorings.

We measured bending moments i n t h e 46 South U i s t s e a s f o r t h e normal

5 mooring l a y o u t , and then moved t h e number 2 mooring t o a p o s i t i o n

between numbers 4 and 5 , as shown i n graph 4.140, f o r a r e p e a t t e s t .

The r e s u l t s f o r heave and surge before and a f t e r t h e changes a r e super-

imposed. I n many cases they a r e wi th in t h e l i n e t h i cknes s o f t h e p l o t t e r

pen. The b igges t d i f f e r e n c e occurs when l o s t moorings a r e a t t h e down-

wave end of t h e sp ine . Compare, f o r example, s e a numbers 378 and 220.

We su f f e r ed a mul t ip lex f a i l u r e f o r s e a numbers 112 and 377.

The d a t a a r e r e p l o t t e d i n graphs 4.141 and 4.142 s e p a r a t e l y f o r

heave and surge wi th s c a l e changes t o make maximum va lues a l l t h e same.

This a l lows shape comparisons t o be made more e a s i l y . Surge behaviour

looks more r e p e a t a b l e a f t e r a mooring change than does heave.

A s t h e first cond i t i on i t s e l f represen ted only 25% o f t h e planned

mooring d e n s i t y , we can be conf ident t h a t t o l e r a n c e t o t h e l o s s o f

moorings i s very high. While we must r e p e a t t h e t e s t s when ducks a r e

mounted on t h e s p i n e it would seem t h a t l e av ing moorings t o f a i l and

r ep l ac ing them t h e fo l lowing summer could wel l be t h e b e s t maintenance

po l i cy d e s p i t e i t s h e r e t i c a l imp l i ca t i ons .

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Bending Moment change with major MOORING MODIFICATION Lom~ar~son w ~ t h reaular arranaemenf

BEFORE CHANGE AFTER-CHANGE %joints S t i ff ness: 1000 Nm/rad sea set: SU 'a '

! ! ! & O O b SURGE & HEAVE joints 1 1 , , 1 1 , 1 ! 1 1 1 1 1 , , 1 1 1 , , , ~ ~ l i , t l ~ 1 ~ ~ ~ ~ i ! ~ , i-I , A & u L d - 111111111111111111 lllli171;-jllllllll Lld-Adu

4

PECTRA #a1 set 089 108 1 1 2 ~ - - - 2 b b ~ m 122 154 168 171 177 t 1

GRAPH 4.140

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Bending Moment change with major MOORING MODIFICATION -- - -

Comparison. with regular arrangement BEFORE CHANGE CHANGE %joints St i f f ness: 1000 Nm/rad

sea set: SU 'a ' ! ! !

6 A h 6 each test self-scaled SURGE joints 6 0 0 0

I PECTRA

'a' set

GRAPH 4 .141

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Bending Moment change with major MOORING MODIFICATION Comparison. w i t h regular arrangement

BEFORE CHANGE AFTER CHANGE &joints S t i f f ness: 1000 Nm/rad

KJ ~1 sea set: SU 'a I ! ! !

6 6 A & & 0 tl o o o ~ J ~ N T S 5 r p - a r r a n g e d ~ ~ ~ ~ l ~ ~ each t e s t self-scaled HEAVE joints

GRAPH 4 . 1 4 2

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4.M EFFECT OF BROKEN JOINTS

I n graph 4.150 we show t h e e f f e c t of an acc iden ta ly cracked f i n g e r

clamp. (These were designed t o s a c r i f i c e themselves before damage t o

t h e i n s i d e of t h e s p i n e . ) The j o i n t w a s s t i l l a b l e t o pas s shea r f o r c e s .

Both heave and surge moments a r e reduced a t t h e break and e l eva t ed t o

e i t h e r s i d e . The model i s behaving l i k e a p a i r of s h o r t e r s t r i n g s .

r m s bending moment

I

I r m s bending moment

1

I 0 . i

'\

0 0j 5 0 10 0 15 0 20.0

S U R a j o i n t number

HEAVE j o i n t number

GRAPH 4.150 E f f e c t o f a broken s u r g e j o i n t on measured bending moments

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5.A CUMULATIVE JOINT ANGLES

We define cumulative joint angle as the total travel of a joint

during a given period. It is a useful number to know if you are

designing full-scale spine joints for long maintenance-free periods at

sea. Values are calculated from the spine tacho-generator velocity

signals, by integrating their moduli. They are surprisingly low.

Each test lasted 51.2 seconds. For a scale of 107.7 the degrees-

per-test result should be multiplied by the numbers shown below to give

values for total angular excursion over longer periods. (Angles remain

the same at all scales.)

t i m e

1 hour

1 day

1 year

25 years

The data are plotted separately in surge and heave. The spine has

40 joints, and the cumulative angle at each joint is shown as a short

bar. The range of values along the spine is clearly shown. In graph

5.1 joint stiffness was varied in four steps from 500 to 5000 Nm/rad.

Energy Period and wave amplitude were kept constant. We see that angles

rise with the inverse root of stiffness. Heave angles are about half

the size of surge angles.

In seas equivalent to our 1 second Pierson-Moskowitz with

Hrms = 1.46111 and Te = 10.4 seconds, a central surge joint with stiffness

equivalent to 1000 Nm/rad would be moving through 50 degrees per test.

Although this is a very rough sea (power = 173 kW/m, about three times

our power limit) the full scale joint would only be moving at 0.94

revolutions per hour. It is likely that attempts to make more use of

the power-generating capacity of joints will produce much larger values

of cumulative angle. But we can go a long way in this direction before

wear becomes a problem.

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Cumulative Anales J

l.Osec PM, Mitsuyasu, 40 joints

GRAPH 5.1

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I n graph 5.2 t h e s e a amplitude m u l t i p l i e r was r a i s e d i n 5 s t e p s

from 0.25 t o 2.0. Energy pe r iod was kept cons t an t a t 1 .0 s ec . S t i f f n e s s

was kept cons t an t a t 1000 Nm/rad.

We s e e t h a t surge angles a r e r i s i n g l i n e a r l y with H r m s except f o r

t h e b igges t ones. The t r ends f o r t h e s e remind us of t h e 0.8 power r u l e

( s e c t i o n 4 . A ) . Heave angles r i s e very s l i g h t l y f a s t e r than t h e first

power of amplitude.

I n Graph 5.3 we va r i ed energy per iod by s i x s t e p s from 0.7 t o 1 . 5

seconds while wave amplitude and s t i f f n e s s were kept cons t an t . Both

heave and surge angles r i s e r a p i d l y between 0.7 and 0.9 seconds with

another r i s e from 1 . 3 t o 1 .5 seconds. Heave angles a r e about h a l f t h e

s i z e of corresponding surge ones except a t 1 . 5 seconds where they r i s e

t o about two-thirds .

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Cumulative Angles

Varying Hrms MULTIPLIER G R A P H 5.2

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Cumulative Anales a

PM, Mitsuyasu, 1000Nm/rad, 40 joints

I Energy Period (sec)

A & A r l l LO XWNTS 6 MOORINGS

Energy Period (sec)

Varying ENERGY PERIOD GRAPH 5 .3

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5.B MAXIMUM J O I N T ANGLE I N FREAK WAVE

Graph 5.4 shows a t ime s e r i e s from a s p i n e su rge j o i n t dur ing t h e

passage of an extreme wave. This was t h e l a r g e s t angular excursion of

a l l j o i n t s .

The s e a was a s tandard Pierson-Moskowitz spectrum wi th 1 .0 second

energy per iod and Mitsuyasu spread. We arranged t h e s t a r t i n g phases

such t h a t c r e s t s i n each of t h e 75 component wavefronts would occur a t

t h e same p l ace and time. We chose t h e p l ace t o be a t t h e j o i n t which

s u f f e r e d t h e b i g g e s t bending moment i n normal 1 second Pierson-Moskowitz

s e a s .

We inc reased t h e wavemaker d r i v e vo l t age t o g i v e a well-defined

plunging breaker . This command s i g n a l had an r m s va lue f o u r t imes t h e

Pierson-Moskowitz norm.

The r e s u l t i n g wave (used t o s i n k model t r a w l e r s dur ing tank

demonstrat ions) is o u t s i d e t h e range of our wave gauges. We t h e r e f o r e

took a video f i l m of t h e wave h i t t i n g a metre-s t ick and by use of a

s i n g l e frame playback judged its trough-to-crest he igh t t o be 32 cm.

A t f u l l s c a l e t h i s would be equ iva l en t t o 34.5 metres - about t h e 50

year extreme f o r S t a t i o n I n d i a and wel l above anything expected a t South

U i s t .

J o i n t angle r eco rds were i d e n t i c a l r e g a r d l e s s of whether we were

t r y i n g t o make t h e sp ine a s compliant o r a s stiff a s pos s ib l e .

The t ime-ser ies was produced by t ak ing t h e i n t e g r a l of t h e j o i n t

angular v e l o c i t y . The maximum value of 4.01° is j u s t a f r a c t i o n l e s s

than t h e maximum design angle o f t h e j o i n t , 4.2O, bu t t h e r e is no

evidence of c l i p p i n g i n t h e ang le waveform.

We conclude t h a t t h e 212O j o i n t angle es t imated f o r t h e p re sen t

r e f e r ence des ign provides a generous allowance.

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Maximum JOINT ANGLE in 'FREAK WAVE' PM Spectrum, Mi t suyasu Spread, Te =I .Osec

G R A P H 5 . 4

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6.A WAVELENGTHS

Tables 6.1 and 6.2 compare deep water wavelengths with the

wavelengths in the narrow and wide tanks, for a number of frequencies

and periods.

Graph 6.1 shows the ratio of shallow-water wavelength to deep-water

wavelength for both tanks.

The expression for wavelength L of small amplitude waves as a

function of period is:

9T2 2 n d = - tanh (T) 2n

and as a function of frequency:

9 m - - 2 tanh ( L ) - 2xf

where : g = gravitational acceleration = 9.81 m/s2

d = water depth (metres)

T = period (sec)

f = frequency (hertz)

L appears on both sides of the equations, and it is usually found

by an iterative process starting by inserting the deep water value

on the right.

In both tanks the effect of the tanh correction drops to less

than one part in a thousand at 1.3 hertz and above.

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W I D E B NflRROW TANK

W R V E L E b I G T H R A T I O

WAVELENGTH RATIO 1 1 -

1 - 0 --------- --------

deep wide narrow period. water tank tank

( set ) (1.2m) (0.6m)

0.4 0.5 rE471--, 0.6 0.562 0.562 0.562 0.7 0.766 0.766 0.765 0.8 1.000 1.000 0.999 0.9 1.265 1.265 1.259 1 .O 1.562 1.562 1.539

1 .I 1.890 1.889 1.830 1.2 2.250 2.244 2.124 1.3 2.640 2.623 2.417 1.4 3.062 3.021 2.706 1.5 3.515 3.430 2.992

1.6 3.999 3.844 3.273 1.7 4.515 4.260 3.550 1.8 5.062 4.675 3.824 1.9 5.640 5.086 4.095 2.0 6.249 5.494 4.363-

1

I I

1 I

1 1

Table 6.1: WAVELENGTHS against FREQUENCY Table 6.2: WAVELENGTHS against PERIOD

t deep wlde narrow frequency water tank tank

(hz ) t

0.5

0.6 0.7 0.8 0.9 1.0

1 .I 1.2 1 .3 1.4 1 .5

1.6 1.7 1.8 1.9 2.0

2.1 2.2 2.3 2.4 2.5

(1.2m) (0.6m)

6.249 5.494 4.363

4.340 4.122 3.458 3.188 3.137 2.788 2.441 2.431 2.271 1.929 1.927 1.863 1.562 1.562 1.539

1.291 1.291 1.284 1.085 1.085 1.083 0.924 0.924 0.924

I-, 0.797 -1 0.694

0.610 0.541 0.482 0.433 0.391

0.354 0.323 0.295 0.271 0.250

i

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6 . B POWER RATIO

T h i s is t h e r a t i o o f t h e power of a r e g u l a r wave i n water of

f i n i t e d e p t h , t o t h e power i n a wave o f t h e same h e i g h t and p e r i o d

t r a v e l l i n g i n water o f i n f i n i t e dep th .

The energy E , i n a r e g u l a r wave o f u n i t w i d t h , b u t one wavelength

l o n g , can be w r i t t e n a s ( r e f g , p 2 1 ) :

where: is wate r d e n s i t y

g i s g r a v i t a t i o n a l a c c e i e r a t i o n

H r m s is r o o t mean s q u a r e wave h e i g h t

L i s wavelength

The power d e n s i t y P can be c a l c u l a t e d by d i v i d i n g t h e energy

by t h e t ime t a k e n f o r it t o c r o s s a l i n e p e r p e n d i c u l a r t o i ts d i r e c t i o n

of t r a v e l . I f t h e energy t r a v e l l e d a t t h e phase v e l o c i t y ( t h e v i s u a l l y

a p p a r e n t speed o f t h e t r o u g h s and c r e s t s ) t h i s t ime i n t e r v a l would

be t h e wave p e r i o d T , b u t i n f a c t i t t r a v e l s more s lowly a t t h e group

v e l o c i t y . Denot ing t h e r a t i o o f group t o phase v e l o c i t i e s a s n, power

d e n s i t y can be w r i t t e n a s :

Combining (1) and ( 2 ) : P = n L e 3 14'R.s

T

Both t h e v e l o c i t y r a t i o n , and t h e wavelength L a r e f u n c t i o n s o f wa te r

d e p t h :

d i s wate r d e p t h

z L = 3T - pwk 2TTd ( s e e s e c t i o n 6.A) -

2 lT L

The v a l u e o f n i n c r e a s e s from 0 . 5 i n deep w a t e r t o 1 i n v e r y

s h a l l o w w a t e r , whi le L g e t s s h o r t e r a s d e p t h d e c r e a s e s . The combined

e f f e c t s o f t h e s e v a r i a t i o n s causes t h e power r a t i o t o v a r y w i t h wave

f requency a s shown i n Graph 6.2 f o r t h e narrow and wide t a n k s , and

Tab les 6 . 3 and 6 .4 l i s t v a l u e s f o r some s e l e c t e d f r e q u e n c i e s and p e r i o d s .

The t a n k t r a n s f e r f u n c t i o n t a k e s bo th e f f e c t s i n t o accoun t b u t can

be r e p l a c e d by an ' a m p l i t u d e p r i o r i t y ' one f o r over- topping exper iments .

Page 201: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

W 1 D E 8 N f l R R O W T f l N K P O W E R R F I T I O

GRAPH 6.2: Power Ratio agzinst Frequency

WAVE FREQUENCY Chz)

. wide narrow

frequency tank tank (hz (1.2m) (0.6m)

t

0.5

0.6 0.7 0.8 0.9 1 .O

1 .I 1.2 1 .3 1.4 1 .5

Table 6.3 : POLTER RATIO/FREQUENCY Table 6.4: POWER RATIO/PERIOD

v

wide narrow period tank tank ( sec (1.2m) (0.6m)

I

1.191 1.141

1.129 1.195 1.061 1.193 1.021 1.154 1.005 1.102 1.001 1.057

1 .OOO 1.027 1.000 1.011 1.000 1.004 1 .OOO 1.001 1.000 1.000

0.5

0.6 0.7 0.8 0.9 1 .O

1 .I 1.2 1.3 1.4 1.5

1.6 1.7 1.8 1.9 2.0

1.000 1.000

1 .OOO 1 .OOO 1 .OOO 1.001 1 .OOO 1.007 1.000 1.025 1.001 1.057

1.005 1.098 1.014 1.137 1.030 1.168 1.053 1.189 1.081 1.198

1.110 1.199 1.138 1.192 1.161 1.179 1.178 1.161 1.191 1.141

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6.C CREST-LENGTHS

For a regular wave, crest-length is the distance between crests

along a line parallel to the wavemakers.

rz ~n A where L is the wavelength = ?- bm ' (, )

2-K a is the angle that the wavefront makes

with the wavemakers.

Tables 6.5 and 6.6 list crest-lengths against frequency and period,

for a number of wave angles. The values in the 90 degree columns

are of course the same as the wavelengths. These tables avoid the

need for the unpleasant iterative solution of the TANH equation.

They allow for the tank depth of 1.2 metres but do not take larger

amplitude effects into account. These become significant for breaking

waves. We have not yet thought of a way to incoporate amplitude effects

into the tank transfer function.

Page 203: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

for wide tank (depth: 1.2m)

Table 6.5 WST-LENGTHS (metres) against FREQUENCY

frequency (hz

0.5

0.6 0.7 0.8 0.9 1 .O

1 .I 1.2 1.3 1.4 1.5

1.6 1.7 1.8 1.9 2.0

2.1 2.2 2.3 2.4 2.5

a n g l e ( d e g r e e s ) 5 10 1 5 20 25 30 35 40 45 50 55 60 65 70 75 80 85

63.05 31.65 21.23 16.07 13.00 10.99 9.58 8.55 7.77 7.17 6.71 6.35 6.06 5.85 5.69 5.58 5.52

47 .3023 .7415 .9312 .05 9.75 8.24 7.19 6.41 5.83 5.38 5.03 4.76 4.55 4.39 4.27 4.19 4.14 36 .0018.0712.12 9.17 7.42 6.27 5.47 4.88 4.44 4.10 3.83 3.62 3.46 3.34 3.25 3.19 3.15 27.9014.00 9.40 7.11 5.75 4.86 4.24 3.78 3.44 3.17 2.97 2.81 2.68 2.59 2.52 2.47 2.44 22.1211.10 7.45 5.64 4.56 3.86 3.36 3.00 2.73 2.52 2.35 2.23 2.13 2.05 2.00 1.96 1.93

90

5.49

4.12 3.14 2.43 1.93

17.93 9.00 6.04 4.57 3.70 3.12 2.72 2.43 2.21 2.04 1.91 1.80 1.72 1.66 1.62 1.59 1.57 i1 .56

14.82 7.44 4.99 3.78 3.06 2.58 2.25 2.01 1.83 1.69 1.58 1.49 1.42 1.37 1.34 1.31 1.30 12.45 6.25 4.19 3.17 2.57 2.17 1.89 1.69 1.53 1.42 1.32 1.25 1.20 1.15 1.12 1.10 1.09 10.61 5.32 3.57 2.70 2.19 1.85 1.61 1.44 1.31 1.21 1.13 1.07 1.02 0.98 0.96 0.94 0.93

9.15 4.59 3.08 2.33 1.89 1.59 1.39 1.24 1.13 1.04 0.97 0.92 0.88 0.85 0.83 0.81 0.80

1.29 1.08 0.92 0.80

7.97 4.00 2.68 2.03 1.64 1.39 1.21 1.08 0.98 0.91 0.85 0.80 0.77 0.74 0.72 0.71 0.70 10.69

7.00 3.52 2.36 1.78 1.44 1.22 1.06 0.95 0.86 0.80 0.75 0.70 0.67 0.65 0.63 0.62 0.61 1 0.61 6.20 3.11 2.09 1.58 1.28 1.08 0.94 0.84 0.76 0.71 0.66 0.62 0.60 0.58 0.56 0.55 0.54 5.53 2.78 1.86 1.41 1.14 0.96 0.84 0.75 0.68 0.63 0.59 0.56 0.53 0.51 0.50 0.49 0.48 4.97 2.49 1.67 1.27 1.02 0.87 0.75 0.67 0.61 0.57 0.53 0.50 0.48 0.46 0.45 0.44 0.43 4.48 2.25 1.51 1.14 0.92 0.78 0.68 0.61 0.55 0.51 0.48 0.45 0.43 0.42 0.40 0.40 0.39

4.07 2.04 1.37 1.04 0.84 0.71 0.62 0.55 0.50 0.46 0.43 0.41 0.39 0.38 0.37 0.36 0.36 3.70 1.86 1.25 0.94 0.76 0.65 0.56 0.50 0.46 0.42 0.39 0.37 0.36 0.34 0.33 0.33 0.32 3.39 1.70 1.14 0.86 0.70 0.59 0.51 0.46 0.42 0.39 0.36 0.34 0.33 0.31 0.31 0.30 0.30 3.11 1.56 1.05 0.79 0.64 0.54 0.47 0.42 0.38 0.35 0.33 0.31 0.30 0.29 0.28 0.28 0.27 2.87 1.44 0.97 0.73 0.59 0.50 0.44 0.39 0.35 0.33 0.31 0.29 0.28 0.27 0.26 0.25 0.25

0.54 0.48 0.43 0.39

0.35 0.32 0.30 0.27 0.25

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period ( set

- -- - - - -

a n g l e ( d e g r e e s ) 5 10 15 20 25 30 35 40 45 50 55 60 65 70 75 80 85

44.12 22.14 14.86 11.24 9.10 7.69 6.70 5.98 5.44 5.02 4.69 4.44 4.24 4.09 3.98 3.90 3.86 48.89 24.54 16.46 12.46 10.08 8.52 7.43 6.63 6.03 5.56 5.20 4.92 4.70 4.53 4.41 4.33 4.28 53.6526.9318.0713.6711.06 9.35 8.15 7.27 6.61 6.10 5.71 5.40 5.16 4.98 4.84 4.75 4.69 58.37 29.30 19.66 14.87 12.04 10.17 8.87 7.91 7.19 6.64 6.21 5.87 5.61 5.41 5.27 5.17 5.11 63.05 31.65 21.23 16.07 13.00 10.99 9.58 8.55 7.77 7.17 6.71 6.35 6.06 5.85 5.69 5.58 5.52

f o r wide tank (depth:

Table 6.6 CREST-LENGTHS (metres) against PERIOD

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6.D TANK LIMITS

Sea s t a t e s i n t h e wide tank a r e composed of up t o 75 s e p a r a t e

wave f r o n t s . Each is defined by an amplitude, a f requency, an ang le ,

and a s t a r t i n g phase.

The range of u se fu l angles is l i m i t e d by t h e p i t c h of i nd iv idua l

wave makers.

Angles a r e produced by ar ranging a cons tan t phase d i f f e r e n c e ,

9 between t h e command s i g n a l s t o each wavemaker.

where P is t h e p i t c h of t h e wavemaker

L is t h e wavelength co r r ec t ed f o r shal low water e f f e c t s

a is t h e r equ i r ed wavefront angle

Inve r se ly , phase d i f f e r e n c e d produces angle a:

Phase d i f f e r e n c e f ~ $ between wavemaker n and wavemaker n + 1, I

impl ies phase d i f f e r e n c e d = (2r- d ) between wavemaker n and wavemaker

n - 1. This may r e s u l t i n a second wave a t angle a' i f t h e expression I

i n bracke ts above is l e s s than o r equal t o 1 when / is rep laced by $.

This is shown i n graph 6.3. Lines of cons t an t wave angle a r e

p l o t t e d a g a i n s t wave making frequency and phase d i f f e r ence . Normal

tank ope ra t ion corresponds t o t h e 2 t runca ted t r i a n g u l a r a r e a s a t

top and bottom, where only one wavefront is poss ib l e . The a r e a where

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I W I D E T A N K A N G U L A R E N V E L O P E I

1.5 2.0 2.5 3.0 WAVEMAKING FREQUENCY ( h z >

GRAPH 6 .3 . The w i d e tank angular envelope.

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secondary wave f r o n t s w i l l occur i s t o t h e r i g h t where a n g l e l i n e s

i n t e r s e c t . A t f r e q u e n c i e s above 2.26 h e r t z , w h e r e t h e wavemaker p i t c h

is e q u a l t o o r g r e a t e r t h a n wave l e n g t h , secondary f r o n t s a r e i n e v i t a b l e ,

whatever t h e ang le . Phase d i f f e r e n c e s and f r e q u e n c i e s i n t h e whi te

a r e a produce l o t s o f movement a t t h e wavemakers b u t l i t t l e i n t h e

t a n k . The waves a r e t r y i n g t o go backwards ' i n t o t h e c a r - p a r k ' .

Phase d i f f e r e n c e s # and 6 ' a r e o f course t h e same a s

F i g 6 . 4 shows t h e a r e a s where t h e s e ' g h o s t s ' w i l l appear i n t h e t a n k .

Graph 6 . 5 shows how we could make t h e t a n k b e t t e r o r worse by

changing t h e p i t c h o f t h e wavemakers from t h e p r e s e n t 12". Very narrow

wavemakers p r e s e n t a s e v e r e h inge d e s i g n problem.

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W I D E T A N K A N G U L A R E N V E L O P E

WAVEMAKING FREQUENCY Chz)

GRAPH 6.4: Wide Tank angular envelope - extended

Page 209: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

W I D E T A N K A N G U L A R E N V E L O P E

Pitch: 6"

Pitch: 3"

GRAPH 6.5 Angular envelope for 4 different wavemaker pitches

0 5 I 0 1 5 2 0 2 5 3 0 3 5 4 0 4 5 5 0 WAVEMAKING FREQUENCY (hz)

Page 210: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

6.E INHERENT J O I N T STIFFNESS

The s p i n e model is designed s o t h a t bending f o r c e s a r e opposed

by a motor dr iven arm. There a r e a l s o small t o r s i o n sp r ings with

s t i f f n e s s of 15NM/rad a t each j o i n t t o provide mean r e fe rence p o s i t i o n s

f o r t h e j o i n t s .

In a d d i t i o n t o t h e s e known compliances, t h e mechanical components

of t h e sp ine u n i t s d e f l e c t under t he a c t i o n of t h e t r ansmi t t ed f o r c e s ,

such t h a t t h e angular d e f l e c t i o n s of t h e j o i n t s may be a l i t t l e g r e a t e r

than ind ica t ed by t h e i n t e g r a t e d angular v e l o c i t y s i g n a l s from t h e

tacho-generators. We measured t h e combined s t i f f n e s s c h a r a c t e r i s t i c s

of 5 j o i n t s and t h e r e s u l t s a r e shown i n graph 6.6.

We used a metal-working l a t h e t o provide a r i g i d r e f e rence frame.

The a c t i v e j o i n t was gr ipped by t h e chuck, and a con ica l cen t r e a t tached

t o t h e t a i l s t ock provided a shear r e a c t i o n a t t h e pas s ive end without

e x e r t i n g any a d d i t i o n a l torque.

With s i n u s o i d a l command s i g n a l s app l i ed , t h e f o r c e feedback c i r c u i t

drove t h e j o i n t motor back and f o r t h through whatever angle was requi red

t o match and cancel t h e command torque. A s t h e ends were he ld r i g i d l y

by t h e l a t h e , t h i s angular movement was e n t i r e l y a func t ion of t h e

inhe ren t compliance of t h e sp ine components.

We recorded bending moments a t t h e s t r a i n gauges and divided

them by angular d e f l e c t i o n s ca l cu la t ed from t h e i n t e g r a l o f t h e tacho

v e l o c i t y s i g n a l s . The graph shows these der ived s t i f f n e s s e s p l o t t e d

aga ins t t h e bending moments.

The curves f o r a l l sp ines a r e s i m i l a r . The inhe ren t s t i f f n e s s

i nc reases wi th appl ied torque and then f l a t t e n s ou t . The most obvious

source of t h e non-linear p a r t of t h e c h a r a c t e r i s t i c is t h e toothed

d r ive b e l t s . They a r e made with s t e e l r e i n f o r c i n g bands encased i n

polyurethane.

Page 211: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

Inherent Stiffness of Spine Joints as a function of Bending Moment

5 different joints

Applied Joint Torque Nrn

20 a . . . . 1 . . . . 1 . . . .

Status:lO :

GRAPH 6.6: Joint inherent stiffness against applied torque

Measured Joint 15- S t i ffness: Nn/rad *18 :

10-

TABLE 6.7 Approximate asymptotic net s t i f fness of joints and estimated bending momnt multipliers, against nominal s t i f fnesses .

- - --.

Nominal Stiffness Net Stiffness

Moment Multiplier

-

-

5 -

250 500 1000 2000 3500 4000 5000 8000 (Nm/rad) 245 485 930 1750 2800 3100 3700 5100 (Nm/rad)

1 .OO 1.00 1.01 1.08 1.12 1 .I4 1 .I7 1 .I7

-

0 1 - - . - 1 - - - - 1 . - . .

0 5 10 15 20

Page 212: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

The inherent stiffness is in series with the 'electronic' joint

stiffness and so the net stiffness is calculated using the reciprocal

of the sum of the reciprocals of the separate values.

In practice it is not easy to adjust single rms bending moment

values for the effect of inherent stiffness, because it varies throughout

the original time series, depending on the instantaneous forces.

The actual joint stiffness will always be lower than desired, but

the effect will be worse for higher nominal stiffnesses. We were

relieved when narrow tank results showed that required stiffness values

were going to be at the bottom end of the range.

Table 6.7 shows the effect of adding the average asymptotic value

of 14,000 Nm/rad suggested by graph 6.6 to various nominal stiffnesses

and lists estimated correction multipliers for bending moments.

Page 213: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

6.F TIME SERIES AND HISTOGRAMS

a ) Mixed Seas

Most o f t h e d a t a i n t h i s r e p o r t a r e presented a s a r r a y s of r o o t

mean square ( r m s ) va lues , each of t hese numbers i t s e l f being a func t ion

of a complete t ime s e r i e s .

Using r m s va lues reduces t h e amount of d a t a t h a t we have t o d i sp l ay

and s t o r e , t y p i c a l l y by a f a c t o r of 1024. This was necessary before

we i n s t a l l e d t ape handl ing equipment f o r bulk d a t a s to rage . The use

of r m s va lues impl ies t h e assumption of a shape of t h e d i s t r i b u t i o n

of t h e measurements. Graphs 6.7 and 6.8 show compressed Bending Moment

time s e r i e s i n Surge and Heave f o r each j o i n t i n a sp ine o f 35 j o i n t s .

Histograms der ived from t h e time s e r i e s a r e drawn a t t h e bottom o f

t h e pages a s s e t s of v e r t i c a l l i n e s . A normal d i s t r i b u t i o n curve

with a s tandard dev ia t ion equal t o t h e r m s va lue of t h e time s e r i e s

is p l o t t e d over each histogram. A t h e o r e t i c a l normal d i s t r i b u t i o n

curve is p l o t t e d over each histogram, with s tandard dev ia t ion equal

t o t h e r m s of t h e time s e r i e s .

The t ime s e r i e s a r e p l o t t e d t o a common v e r t i c a l s c a l e on each

page, bu t t h e histograms a r e ad jus ted s o t h a t t h e h ighes t t o o t h i n

each case i s t h e same h e i g h t , and t h e a r e a s under t h e normal curves

a r e made equal t o those under t h e histogram.

The s e a used is one of t h e sma l l e s t o f t h e South U i s t s p e c t r a ,

so we would expect t o s e e any imperfect ions i n t h e j o i n t hinge

mechanism, p a r t i c u l a r l y i n end sp ines where t h e bending moments u sua l ly

f a l l t o t h e i r lowest va lues , and i n heave where t h e va lues tend t o

be about h a l f o f those i n surge.

I n f a c t t h e q u a l i t y of f i t of t h e measured histograms t o t h e

normal curves is g r a t i f y i n g . Occasional high t e e t h near t h e middle

of t h e histograms suggest s lackness i n t h e d r i v e b e l t , with an apprec iab le

delay before t h e motor can r eve r se i ts r e a c t i o n a s t h e wave-induced

f o r c e s change p o l a r i t y . Low t e e t h i n t h e middle of histograms sugges t

s t i c t i o n i n t h e d r ive s o t h a t waves have t o work e x t r a hard t o g e t

t h e j o i n t s moving.

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spine - joint TORQUE SIG NALS Time Series & Histograms Stiffness: 1000Nm/rad, Status:lO

Sampling: 1024 points at 20Hz = 5I.Zsec Time Series

4 Histograms I I 7

I

South Uis t sea: 089 (small)

SURGE joints GRAPH 6.7

Page 215: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

spine joint TORQUE SIGNALS -

Time Series & Histograms Stiffness: 1000Nm/rad, Status:10

Sampling: 1024 points at 20Hz = 51.2sec Time Series

H istoqrams

South Uis t sea: 089 (small) -- Hrms=0,38cm

Page 216: Wave Power Project - University of Edinburgh Energy/Old reports... · 3. Heave bending moments are proportional to the first power of wave amplitude. 4. Surge bending moments rise

b) Regular Waves

Graphs 6.9 and 6.10 show time series and histograms for the joints

in a regular wave.

The time series on each page are plotted to the same vertical

scale, but the histograms are individually scaled according to the

highest tooth. The horizontal time-scale is one quarter of that used

in the preceding South Uist plots, although, for the monochromatic

wave tests shown elsewhere in this report, the test times were the

same.

The time series in surge are strikingly symmetrical. With only

256 data samples per plot shown here, the sampling time steps are

clearly visible. Most of the peaks are ragged, and the histograms

are fairly noisy versions of the U shapes expected with approximately

sinusoidal signals. The effect of stiction is particularly visible

in the histogram for joint number 039 which had unusually low loading

for this sea.

In heave, the striking asymmetry of the time series is reminiscent

of our work with cylinders in the narrow tank (see page 15.2 of our

1976 report). Frequency doubling is evident in many of the joints

and the 2 least distorted waveforms, 040 and 042, show interesting

modulation in their envelopes, suggestive of beating. We know that

wave amplitude stability is much better than that.

Before plotting each time series we subtracted the mean value

of the time series from each data point to remove the effects of any

electrical offsets in the system. At this stage, we are not able

to distinguish genuine non-zero bending moment means from such offsets,

so the apparent asymmetry of positive and negative peak values should

be treated with caution. This caveat applies particularly to the

modulus results in section 4.A. However it is difficult to imagine

a hydrodynamic mechanism which could induce permanent bending moment

offsets in a free floating structure of constant section and weight

distribution.

We have now installed economic mass data storage in the wide

tank. Magnetic tape is used to record the millions of numbers produced

during each experiment and so we can, in future, maintain access to

the original time series indefinitely.

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spine joint TORQUE SIG - NALS Time Series & Histograms Stiffness: 1000Nm/rad, Status:10

Sampling: 256 points a t 20t - i~ = 12.8sec Time Series r

H istoqrams I I

Monochromatic sea: ~ = l . l s e c , ~ n ~ l e = 3 ~ Hrms=1.414cm

SURGE joints --

GRAPH 6.9

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spine joint TORQUE SIGNALS -

Time Series & Histograms Stiffness: 1000Nm/rad, Status:10

Sampling: 256 points at 20Hz = 12.8sec Time Series r 1

Histoqrams -

Monochromatic sea: ~ = l . l s e c , ~ n ~ l e = 3 $ Hrms=1.414cm

HEAVE joints GRAPH 6.10

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6 . G THE SOUTH UIST 46 SPECTRA

In t roduc t ion

Crabb has given an e x c e l l e n t d e s c r i p t i o n o f t h e c o l l e c t i o n and

a n a l y s i s o f wave d a t a from s e a s o f f South U i s t c a r r i e d out by t h e

I n s t i t u t e of Oceanographic Sciences ( r e f a ) . Wave measurement had

s t a r t e d i n March 1976 with a waverider buoy ope ra t ing 8 n a u t i c a l miles

o f f sho re i n 1 5 metres depth , and a t 2 o t h e r s i t e s i n 23 metres depth

and 100 metres depth (Mollison r e f f ) .

They produced a group of 399 evenly weighted s p e c t r a , c o l l e c t i v e l y

r e p r e s e n t a t i v e of a ' s t anda rd ' Hebridean yea r , with wave d i r e c t i o n s

synthes ised from h indcas t s us ing l o c a l and d i s t a n t wind da ta .

The ind iv idua l s p e c t r a were expressed a s combinations of up t o

3 components :

a ) Wind s e a : t h e higher frequency p a r t of t h e spectrum caused by l o c a l winds concurrent with t h e wave record .

b ) Swell s e a : t h e low frequency p a r t of t h e spectrum a t t r i b u t a b l e t o e a r l i e r and d i s t a n t wind condi t ions .

c ) Old Wind Sea: a c e n t r a l p a r t of t h e spectrum caused by l o c a l winds which had changed j u s t p r i o r t o t h e wave sampling per iod .

Graph 6.11, reproduced from r e f a , shows a t y p i c a l measured South

U i s t spectrum with c l e a r l y v i s i b l e 'wind' and ' s w e l l ' components.

S. Uist spectrum 86 76 173 14 58 10 1

SIGNIFICANT WAVE HEGHT 1 l7me4res

ZERO CROSSlffi P E I O D 3 68 %&s WIND SPEED I 4 k n o l l

WIND OlRECTlON 150 d e g r ~ s

Freauancy Hz

GRAPH 6.11

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Se lec t ion of a Sub-Set

Subsequently, IOS were asked by t h e Department of Energy's

c o n s u l t a n t s , Rendal, Palmer and T r i t t o n , t o s e l e c t a small subse t

of about 40 s p e c t r a which would c o l l e c t i v e l y r e f l e c t t h e p r i n c i p a l

c h a r a c t e r i s t i c s of t h e 399, bu t which could convenient ly be used i n

s c a l e model t e s t s ( r e f s k & j ) .

IOS f i r s t s o r t e d t h e 399 s p e c t r a i n t o c l a s s e s according t o 3

parameters ( r e f i ) :

a ) 'Frequency-Width' : t h e frequency i n t e r v a l wi th in which 80% of t h e power is conta ined , ( 4 c l a s s e s )

b ) 'Direct ion-Width ' : t h e angular i n t e r v a l wi th in which 80% of t h e power i n t h e frequency width is contained. ( 4 c l a s s e s )

c ) Energy Period Te: ( 5 c l a s s e s )

Within each c l a s s t h e 399 s p e c t r a were f u r t h e r so r t ed i n t o groups

according t o power dens i ty .

Even wi th t h i s grouping process it was found t h a t t h e number

of s e a types was too g r e a t t o be adequately represented by a small

sub-set and s o 2 sepa ra t e sub-sets were proposed:

S e t 1 - A group of s p e c t r a covering a s wide a range a s poss ib l e of frequency width, d i r e c t i o n width and energy per iod b u t r e s t r i c t e d i n t h e range of power and t h e d i r e c t i o n s of peak power. 38 s p e c t r a were eventua l ly s e l e c t e d f o r t h i s group and it was suggested t h a t they be used t o p r e d i c t f u l l - s c a l e system behaviour from 2-dimensional model t e s t da t a .

S e t 2 - A group of s p e c t r a covering a s wide a range a s poss ib l e of frequency width, d i r e c t i o n width, energy period and power, a s soc i a t ed with those s p e c t r a which con ta in t h e bulk of t h e power a r r i v i n g a t South U i s t . 46 s p e c t r a were eventua l ly s e l e c t e d f o r t h i s group, which was intended f o r use i n a s se s s ing f u l l - s c a l e output p roduc t iv i ty of wave energy devices . S e t 2 is t h e group of South U i s t s p e c t r a implemented i n t h e wide tank and r e f e r r e d t o below and throughout t h i s r e p o r t .

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Selection of the 46 S~ectra

The classification of the 399 spectra, by frequency-width,

direction-width, energy period and power density produced a 4-dimensional

histogram, with 107 occupied cells, each of which should ideally have

a representative assigned to Set 2. By excluding from representation

sea states which did not greatly contribute to the annual energy available

a further reduction of numbers was made.

The rules chosen for exclusions were:

a) power density too low ( 10 kW/m) b) power density too high ( 300 kW/m) c) energy period too low ( 7.0 sec ) d) energy period too high ( 12.9 sec ) e) 'unusual' combinations of Energy Period, Power, Spectral

Width, Directional Spread and Principal Direction

This reduced the number of spectra to be represented to 267,

occupying 46 different cells of the histogram. 76.5% of the total

energy in the 399 spectra is accounted for by these cells. (see below

for details of 46 spectra weightings.)

The Set 2 spectra were made up by selecting, from each of the

46 occupied cells, a spectrum whose power density was near the average

for that cell and whose direcion of peak power was close to either

240 degrees or 270 degrees.

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Wide Tank I m ~ l e m e n t a t i o n o f t h e 46 S ~ e c t r a

Our c u r r e n t f u l l - s c a l e des igns a r e based on 1 4 metre ducks.

The wide t ank model u se s 130mm ducks on 125mm diameter s p i n e s , implying

a tank s c a l e of 1 4 metres/l30mm1 o r 107.7.

The IOS s p e c t r a a r e based on wave d a t a c o l l e c t e d a t 42 metres

depth , bu t we favour ope ra t i on around t h e 100 metre contour . The

small amount of d a t a c o l l e c t e d by IOS a t t h e i r 100 metre s i t e allowed

us t o make frequency dependent c o r r e c t i o n s t o t h e 46 s o a s t o e s t ima te

t h e i r s p e c t r a l con ten t a t 100 metres. The d i r e c t i o n a l d i s t r i b u t i o n s

a l r eady ass igned t o t h e 42 metre s e t by IOS, a r e i n f a c t more app rop r i a t e

t o our deep water s i t e . (Moll ison, r e f f ) .

The t h r e e p o s s i b l e sub-spectra i n t h e s e a s t a t e s were each descr ibed

by IOS us ing a Pierson-Moskowitz model ( r e f b , pp6.8-6.9) with assigned

va lues of H r m s and Te, and a modified ' s p e c t r a l width parameter ' which

allowed t h e range o f wavefront f requenc ies t o be compressed o r expanded.

The s p e c t r a l width parameter is analogous t o our 'compression f a c t o r ' .

D i r e c t i o n a l i t y is i n d i c a t e d by a ' p r i n c i p a l d i r e c t i o n ' parameter ,

and an angular d i s t r i b u t i o n model with exponent i f app rop r i a t e .

The t a b l e below summarises t h e parameters used:

Component 1 Parameters s p e c i f i e d I angular I d i s t r i b u t i o n name I f o r a l l components I d i s t r i b u t i o n model I exponent

I

Our c u r r e n t wavemaking computer can produce 75 s e p a r a t e wavefronts

f o r each s e a s t a t e . We make b e s t use o f t h i s l i m i t e d number by a r ranging

t h a t t h e t o t a l energy i n t h e s e a i s , where p o s s i b l e , evenly d iv ided

between them bu t we must a l s o ensure t h a t t h e range o f f requenc ies

is reasonably covered. We used a s imple r u l e and d iv ided t h e 75

wavefronts between t h e 3 s e a components i n p ropor t i on t o t h e product

of H r m s and t h e s p e c t r a l width parameter f o r t h a t component.

Wind s e a

w e s e a

Old Wind s e a

We ignored s e v e r a l wind s e a components wi th e a s t e r l y mean d i r e c t i o n s ,

a s i n every such ca se t h e energy con t r ibu t ed was 3% o r l e s s .

frequency- dependent

s v a r i e s

s = 6

I

H r m s , Energy pe r iod

S p e c t r a l Width

P r i n c i p a l D i r ec t i on

M i t suyasu

~ - 8 e - q C O S ~ ~ ( Q -ed

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Angle Considerations

The 46 spectra contain energy arriving from all compass bearings,

but a line of wavemakers has a limited angular range. At frequencies

below 1.6 Hz the theoretical angle limit is k90°, and it rapidly falls

off to 0 degrees at 2.26 Hz (see Section 6.D). We can make 90° waves

at the wavemakers but they do not find their way into the centre of

the tank. The width of tank usefully served by the wavemakers is reduced

by the product of the tangent of the wavefront angle and the distance

of the model from the wavemakers. We lose this width at both ends

of the tank if there are positively and negatively angled wavefronts,

so that very long models in mixed seas must be deployed as close to

the wavemakers as possible.

We used an angular range of -70° to +70°, and a frequency range

of 0.5 to 3.0 Hz in implementing the 46 spectra. With hindsight these

limits are clearly too wide. The second set of pox-plots (section

3.B) show the presence of numerous additional 'ghost' wavefronts wherever

the specified wavefronts fall outside the tank angular envelope (see

section 3.B, and section 6.D). Current tank work, to be reported

later, suggests that the 'ghost' wavefronts are at frequencies and

angles generally benign to spines, but we propose creating further

sets of 46 tank spectra with better limits.

The closest that we can get spine models to the wavemakers is

about 2 metres. The ?70° limit suggests that the maximum width of

model exposed to all wavefronts would be equal to the width of wavemakers

minus 11.0 metres, which works out at 14.0 metres for 82 wavemakers.

This is equivalent to 35 of our spine units. In practice, deployment

of the models so close to the wavemakers is difficult because of mooring

access problems, and we usually work further out into the tank. The

monochromatic spine tests in section 4.H suggest that bending moments

rise towards the down-wave end so this problem is unlikely to affect

the maximum values recorded.

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Alternative Realisations

Most of the 46 spectra can be reasonably realised with the model

lying parallel to the wavemakers, so that their normal represents

a compass bearing of 260°, which is thought to be the angle of optimum

energy capture for a line of wave energy absorbers. However, 13 of

the spectra have important amounts of energy approaching from southerly

or northerly directions which fall outside the ?70° limit discussed

above. We cannot increase the tank angular window above 140° but

we can improve the representation of these spectra by moving the model.

We produced a second set of 9 spectra for southerly seas with the

model yawed through +40° (clockwise from above), so that the normal

to the wavemakers represents a bearing of 220°. A third set of 4

spectra cater for northerly seas with the model yawed through -50°

to make the wavemaker normal represent a bearing of 310°. In practice,

in this latter case, a mirror image set is used to invert the angles

and allow the direction of yaw to be the same as in the second set.

These alternative realisations limit the model length to about 22

units .

The 4 sets of South Uist spectra are depicted in the pox-plots

and 3-D plots of Section 2.

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Weinhtinns of the 46 S~ectra

The selection of a sub-set of spectra from the original 399 equally

weighted South Uist seas results in an unequally weighted set of 46.

Table 6.8 below shows the number of original spectra represented

by each of the 46 and, by implication, their relative weightings.

(A method suggested by Rendel, Palmer and Tritton for weighting test

results to represent performance over the whole year is described

in ref j.)

Weights total: 267 -

TABLE 6.8 Weightings for the 46 South Uist Spectra (source: ref i)

IOS relative IOS relative IOS relative ref WEIGHT ref WEIGHT ref WEIGHT no no no

1 089 4 2 108 4 3 112 3 4 122 4 5 154 8

6 168 7 7 171 1 9 8 177 6 9 180 6

10 200 9

11 201 2 1 1 2 210 20 1 3 212 3 1 4 218 9 1 5 220 4

16 223 5 1 7 228 3 1 8 238 6 1 9 241 4 20 242 4

21 244 1 5 22 249 3 23 267 4 24 268 2 25 280 7

26 291 5 27 292 7 28 294 3 29 318 6 30 319 8

31 322 4 32 324 3 33 336 3 34 346 4 35 347 2

36 352 2 37 355 2 38 359 11 39 360 3 40 366 3

41 371 5 42 377 5 43 378 2 44 381 2 45 388 3 46 391 4

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6.H CONVERTING BENDING MOMENTS TO ANGLES

Most of t h e graphs i n t h i s r e p o r t show bending moments. I f we

assume t h a t t h e j o i n t s a r e behaving a s undamped, l i n e a r sp r ings with

known s t i f f n e s s t h e conversion is obvious. One d iv ides a bending

moment r e s u l t by t h e s t i f f n e s s a t which it was measured t o ob ta in

a va lue of j o i n t movement i n rad ians .

Af te r t h e angular measurements i n extreme waves showed t h a t j o in t -

angle would be t h e very l e a s t of our problems we decided t o de fe r

t he p re sen ta t ion of angle da t a t o a l a t e r r e p o r t which w i l l dea l with

t h e e f f e c t s of torque l i m i t s and j o i n t damping.

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6.J CALIBRATIONS AND ACCURACIES

Wave Height Measurement

Our knowledge of t h e wave he igh t i n t h e tank depends on two th ings :

1. Wave gauge c a l i b r a t i o n .

An a r r a y of 16 three-wire conductivity-compensating gauges is

arranged about 2 metres i n f r o n t of t h e wavemakers. These a r e c a l i b r a t e d

before every experiment. A monthly check was made of t h e i r d r i f t ,

and over t h e per iod January t o J u l y 1983 t h e RMS monthly e r r o r was

1.43% (Note t h a t an average monthly e r r o r would have been l e s s due

t o c a n c e l l a t i o n ) . Most gauges managed t o s t a y wi th in 'I%, bu t t h e

RMS is pu l l ed up by the occasional rogue.

2. Tank r e p e a t a b i l i t y .

Experiments on long sp ines a r e done by measuring t h e s e a i n t h e

absence of t h e model, and r e l y i n g on r e p e a t a b i l i t y t o ensure t h e model

s ee ing t h e same waves. ( I n t h e narrow tank with r e g u l a r waves we

can s e p a r a t e i nc iden t and r e f l e c t e d waves. This is no t poss ib l e i n

t he wide tank and wave measurements done with t h e model i n t h e water

a r e always high because of r e f l e c t i o n . ) Over a t e s t , t he wavemaking

system g ives u s an RMS r e p e a t a b i l i t y of b e t t e r than 2%, while

ins tan taneous wave he ight can have up t o 5% e r r o r .

Spine Torque Measurement

Spine torque is measured with a br idge of 4 s t r a i n gauges on

t h e torque p l a t e . These a r e pos i t ioned s o t h a t a l l torque is appl ied

through them with t h e fol lowing except ions:

1. Spine angle-centr ing torque s p r i n g

2. Spine bearing f r i c t i o n

The s t i f f n e s s of t h e c e n t r i n g s p r i n g i s known, a t 1 5 Nm/rad ( t h i s

is approximately 0.1% of t h e maximum s t i f f n e s s o b t a i n a b l e ) , while

t he bear ing f r i c t i o n of a new sp ine is l e s s than 1% of t h e f u l l - s c a l e

torque l i m i t .

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The strain gauge circuit is calibrated using a special calibration

rig. We trim every spine to better than 0.5% but the combination

of drift and non-linearity increases this error. We believe that

most spines have a worst error of less than 2%.

The torque calibration is 10 Nm/volt.

Spine Velocity Measurement

This is done using a tacho-generator on the back of the spine

motor. We calibrate it by mounting the spine on a special rig and

allowing it to move through a precise angle between end stops: the

output of the tacho-generator is accurately integrated, and the output

of the integrator compared with the angle it has gone through. We

aim at calibrating this to better than 0.25%. However, the 'inherent

stiffness' (see graph 6.6) means that if the joint is experiencing

a high torque it will underread its velocity. The 'movement multiplier',

mentioned in Table 6.7, can be used to generate a correction if necessary.

The velocity calibration is 0.1 rad/sec/volt.

This is obtained by doing a digital integration of the sampled

velocity signal in the Plessey Miproc computer. Its accuracy therefore

is no worse than the velocity from which it is derived.

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6.K USEFUL EQUATIONS

A Note on Scale

If dynamic similarity exists between model and prototype, we

can get full-scale figures from model figures with the right scaling

factor. This is best described by some index of scale. These are

listed below for various parameters. The second column gives actual

multiplication factors for our current wide tank scale of 107.7

PARAMETER FOR FULL SCALE

INDEX OF SCALE MULTIPLY BY

Bending moments 4 135 x lo6

Wave height and length Period Frequency

Distances Linear Velocities Linear accerations

Angles Angular velocity Angular acceleration

Buoyancy Inertial forces Velocity forces Drift forces

Torque Power

Power per unit length Force per unit length Torque per unit length

Mass 3 Inertia per unit length 4 Buoyancy spring per unit length 3 Damping per unit length 3.5

Stiffness density Compliance density

Beam stiffness EI 5 14.5 x 10 9

The ratio of wavelength to diameter L/D is the most useful

indicator of dynamic similarity. The ratio of wave height to diameter

should also be considered. Scale effects should be less of a worry

for inertia-dominated wave behaviour than in other fields.

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Vibrations In the following, k is spring stiffness, c a viscous damping constant, a,, an undanlped natural frequency and 1 7 1 . M masses.

Free vibration with viscous damping

For a inass nz the undamped natural frequency is

w, = d ( k l m )

the critical damping constant is

cc = 2d(km)

the damping ratio is ( = c/cc and the logarithmic dec reme~l t is

Steady-state vibration with viscous damping

The ratlo of peak amplitude X t o the steady d~splacement X o = P/k IS

and the phase angle 4 is glven by

tan 6 = 2cw/w,

1 - ( w / ~ , ) ~

t P s ~ n ~t These relations yield the curves given below.

Frequency rat lo 3"

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R E F E R E N C E S

Crabb, J. A., Synthesis of a Directional Wave Climate, in 'Power from Sea Waves', Count, B. ed., pp 41 - 74, Academic Press, London, 1980.

4th Year Report, Vol 1, Edinburgh Wave Power Project.

4th Year Report, Vol 3, Edinburgh Wave Power Project.

Salter, S.H., Absorbing Wave-Makers and Wide Tanks, in Proceedings of the Conference on Directional Wave Spectra Applications, Wiegel, R.L. ed., pp 185 - 202, American Society of Civil Engineers, New York, 1981.

Edinburgh SCOPA Laing report, 1979.

Mollison, D., Wave Energy Losses in Intermediate Depths, Applied Ocean Research, Vol. 5, No. 4, pp 234 - 237, 1983.

Wiegel, R. L., Oceanographic Engineering, Prentice-Hall, New Jersey, 1964.

Gilbert, G., Generation of Oblique Waves, H.R.S. Notes No.18, pp 3-4, May 1976.

Crabb, J.A., personal communication.

Anon, Consultant's Methodology for Establishing Annual Device Productivity Using the 46 Selected Spectra, Rendal, Palmer and Tritton consultants' working paper no 42, 1981, London.

Anon, Transformation of the 46 Selected Multidirectional Spectra for Tests of the Devices in the Tank. Rendal, Palmer and Tritton consultants' working paper no. 39, 1981, London.

4th year report, Vol 2, Edinburgh Wave Power Project.

Bryden, I. G., Long Floating Cylinders in Three-Dimensional Random Seas, PhD Thesis, University of Edinburgh, 1983.

2nd year report, Edinburgh Wave Power Project.