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TCcfi BVET

abbraum voor

Stheopshydrmechanlca

Aichief

Mekelweg 2,2828 CD Delit

TWO DEGREE-OF-FREEDOM NUMERICAL SIMULATION OF FARADAY WAVES

by

Cbñstopher Wayne Carter

A Thesis submitted in partial fulfillment of the requirements for the degree of

Master of Science

(Naval Architecture and Marine Engineering) at the University of Michigan

1998

Thesis Advisor

(2)

Iwould like to dedicate this thesis toy mother, for without her I would have never accomplished this much,

and to my soon-to-be-Wife, Karlie, who always supported me while I was at graduate school,

even through the toughest of times, andencouraged

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ACKNOWLEDGMENTS

I would like to thank my thesis advisor, Associate Professor Dale 0.IaiT His guidance and patience in completing this thesis was invaluable I can say, with out a doubt, that without his support, this thesis would have never been completed In addition, I would like to thank Professor Marc Perhn for his assistance with this thesis He was my main source of information on the Faraday wave expenments Without his help, much of the insight about the prior research would have gone unnoficed.

I would like to thank the faculty and staff of the Department of Na'al Architecture and Marine Engineering who all had some impact on my time at the University of Michigan I would also like to give a special thanks to Ms Colleen Vogler Without hersuperior administrative

skills, I would have never gotten anything done while in graduateschool.

Finally, I want to thank my family and friends whO supported me during my graduate

(4)

TABLE OF CONTENTS DEDICATION 2

ACNOtIEDGME1S

.1

3 LIST OF FIGURES 5 ABSTRACT 8

CHAR

L INTRODUCTION 9

U. SYSTEM MODEL AND DERIVATION OF EQUATIONS 10

rn. NUMERICAL ANALYSIS OF EQUATIONS OF MOTION 22

3.1 State space representation 22

32 Fortran program 25

IV CALCULATIONS OF PARAMETERS 29

4.1 Mass and rod length - 30

4.2 DerivatiOn of equations of motion Using linear theory ... 31 4.3 Linearization of non-linear equations of motion ... 34

4.4 Calculations of cOnstants 38

V. NONLINEAR SIMULATION RESULTS 49

V CONcLUSION - 57

APPENDDCA 58

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LIST OF FIGURES

Figure

1 Sketch of Faraday wave with proposed model

2 Sketch of three degree-of-freedom model of system

3 Sketch of simplified two degreeof-freedom model of system 4 Sketch of forces acting on the model used to find the moment about

the pin connection R

Sketch of forces acting on the model used to find the moment about the first point mass M3

6 Sketch of the di.tnensions of tank

7 Sketch of model showing coordinate transfOrmation 8 Graph of the linear response of system of first mode shape

0= l.5717963268rad,$=1.5707963268rad, O =4)

=0

9 Graph of the linear response of system of second. mode shape

0= 1.5707963268 r $= 1.5717963268 O = 4

=0

10 Graph of the linear response of system with both M1 and M2 displaced

0=1.5687963268rad,4)=1.57l7963268rad, O =

=0

11 Graph of damped sine wave With envelope curve (D=lOandI3=O.3/sec

12 Graph of the Wave-peak decay with least-square approximation

0.3Isec

13 Graph of linear response of M1 with envelope curve 0= l.5717963268rad,$= 1.5707963268rad,

=4

=0

44 45 46 46 47 pg. # 10 11 12 12 12 30 31

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14 Graph of the wave-peak decay with least-square approximation

= 0.05/sec 47

15 Graph of System response wIth period one standing wave 0= 1.9394222 tad, 4, = 0.75032909 tad, O = 7.6655593 tad/sec.

4) = 7.3153634rad/sec, amp = 0.006 meters, CO = 10.2324844 rad/sec 50

16 Graph of phase plane of system period one

o = 1.9394222 tad, 4, = 0.75032909 rad, 0 = 7.6655593 rad/sec,

4) = 73153634 ra /sec, amp =0.006 meters, w= 10.2324844 tad/sec 50

17 Graph of system response, from rest, of period one standing waves o 1.5707963268 rad, 4,= 1.5707963268rad, O =4)

=0,

amp = 0.00265 meters, w = 10.053 rad/sec 51 18 Graph of system rsponse, from.rest, of period one standing wave

from 190 sec to 200 sec: 0= 1.5707963268 rad, $ = 1.5707963268 rad,

O=4)=0,amp=0.Oo265meters,co=1O.O53radIseC 51

19 Graph ofphase plane of system, from rest, from 190 sec to 200 sec:penod one 0= 1.5701963268 rad, 4, = 1.5707963268 rad, O = 4) = 0,

amp = 0.00265 meters, co = 10.053 rad/sec 51 20 Sketch of dimpled standing wave with idealized model 52 21 Graph of system response of period one dimple

o = 1.5707963268 rad, 4, = 1.5707963268 tad, 0 = 4) = 0,

amp 0.003705 meters, o 10.053 tad/sec

::

52

22 Graph of system response with period three standing wave o = 1.9817702 rad, 4, = 0.66793155 rad, é = 7.6345674 rad/sec,

4) = 7.2529606 rail/sec. amp 0.006 meters, w = 10.18336536 rail/sec 53 23 Graph of phase plane of system: period three

o = 1.9811702 rad, $ = 0.66793155 ra, 0 = 7.6345674 rail/see,

4) = 7.2529606 rad/sec, amp 0.006 meters,0 = 10.18336536 rail/sec

53,

24 Graph of system response, from rest, of penod three standing wave,

0= 1.5707963268rad,4,= 1.5707963268rad, 0 = 4)

=0,

(7)

25 Graph of system response, from rest, of period three standing wave from 240 sec to 250 ec: 0= 1.5707963268 rad, = 13707963268 rad,

O==0,arnp=O.O038meters,co1O.O53rad/sec

26 Graph of phase, plane of system, from rest, from 240 sec to 250 sec: period

three 0= 1.5701963268 rad, $ = 1.5707963268 rad, 6 =

=0,

amp = 0.0038 meters, o = 10.053 tad/sec =

27 Graph of system demonstrating breaking Waves for height of M1 8= 1.5707963268 tad, = 1.5707963268 rad, O = 4, =

amp=0.0045 metes, (0= I0.OS3rad/sec

28 Gtaph of system demonstrating breaking Waves for angle of O 0= 1.570796328 rad,4 = 1.5707963268 rad, = 4, =0, amp = 0.004 neters, o = 10.053 rad/sec

29 Graph of phase plane of system demonstrating braking waves (0 vs. 0)

0= 1.5707963268rad,4=1.5707963268rad, 0 =4,

=0,

amp = 0.0045 neters, (0= 10.053 rad/sec

54 54 55 55 55 3

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ABSTRACT

Previous research at the University of Michigan included experiments with Faraday waves. Researchers were able to excite the system and find both period one and period three breaking standing waves. Further excitation led to increased breaking waves. During that research, questions arose as to the behavior that the Faraday wave was exhibiting. One method to help explain that behavior is to create a numerical model of the Faraday wave. The purpose of this thesis is to create a discrete model of the system and test it to ensure that the model has the same characteristics as the Faraday wave in the experiment. A simplified two degree-of-freedom

model is designed and its differential equations of motion derivecL The equations Of motion are

programmed in Fortran '71 and solved with the aid of the "isoda" software package. Values for constant parameters are calculated using a linear model of the system and linear response data from the experiment. The model is successfully excited to both a period one and period three

standing wave.

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CHAPTER I

INTRODUCI1ON

Previous research at the University of Michigan included laboratory expenments on

Fara-day waves. In a study by Jiang, Ting, Perlin and Schultz [1.], a low aspect ratiotanic, flllçd with water, was oscillated vertically. At a certain frequency and amplitude, the water began to form a standing wave of the first subharmonic. The first subhaflnomc wave length wasthe length of the tank This wave was found to be a.period one Standing wave (11. In a second paper by Jiang, Per-li and Schultz [2], the researchers found that by increasing the ampPer-litude and changingthe fre-quency slightly, they were able to find a period three standing wave. After increasing the amplitude further, the wave began to break and exhibit chaotic behavior (2]. This is not consid-ered a northal route to chaos. The normal route to chaos is through period doubling [3]. So the question arises, is the route through period three evidence that this System may becomechaotic. In the se ond paper, the authors stated that they wanted to çxplore numerical methods to qualita-tively describe period tripling [2].

The purpose of this thesis is to create a non-linear discrete spring-mass-dashpot model that

will simulate the behavior of the Faraday wave. The idea is to cteate a reduced finite degree-of-freedom tractable model that will make this complex system easier to analyze. Thismodel would

then help explain some of the physics of the Faraday wave and maybe explain how period tripling

could be. a possible route to chaos. Though the final goal of all the research is to describe the physics of the system, this thesis deals with creating the model and fliIcing it match the behavior of the Faraday waves. This includes the period one and period three response of the system. Fur-ther research is necessary to better understand the Faraday vrave.

(10)

0.5

-0

0.5

1

-CHAPTER II

SYSTEM MODEL AND DERiVATION OF EQUATIONS

For the purposes of thi thesis, the simplest discrete model was sought which could cap-ture the salient feacap-tures of the actual system. It is known that the type of wave of interest is a

standing wave at, the fi±st sub.harmothc frequency. For a standing wave, there are two nodes that

will result from the resonant frequency. Becatise of this, the system will be modeled by using only the section of the standing wave between the two nodes. Figure 1 is a diagram of an ideal standing wave used as a visual example. Also in Figure 1 is a rough sketch of the systembeing considered for simulation to capture important results from the original Farathy experiments of references [1] and [2]. Superimposed on the standing wave is a three degree of freedom

oscillat-ing system.

0 1 2 3 4

Figure 1

Sketch of Faraday wa'e with proposed model

(11)

The Faraday wave can be modeled approximately using this three degree of freedom spring-dashpot system. The system consists Of three point masses in conjunction with a spring

and damper for each mass. The outside edges of the model are connected using pin connections, which are the nodes as indicated. This will ensure that the pin connections donot move relative to the base. The system is forced using abase excitation. The forced motion of the base,flz),is

rep-resented using a sinusoidal wave with a constant amplitude and frequency. Figure 2 is a more detailed sketch of the model being considered.

-

_____

- _/t

- - _____

ftt)J

Figure 2

Three degree-of-freedom model of system

The three point masses are connected by massless rods Each point mass is of equal weight and has a respective spring coefficient,A; and damping coefficient, c. The length of the total system is equal to half the length of the tank Advantage is taken of the symthetry of the sys-tem to create a two degree-of-freedom simplified syssys-tem. Figure 3 is a sketch of thenew and final system that will be smulated.

The length of the system when horizontal is 1, which is equivalent to a quarter of the length

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x2

Figure4

Sketch of forces ting on the model Used to

flid the moment about the pin connection R

Figure 3

Simplified two degree-of-freedom model of system

same as they were with the full system. The valtiesof m2, k2 c2ar considered to be half of the original values m order to rnalntain the use of symrnetly. In oilier worth, when the model was cut in half, thó Values for the middle components werealso cut in half. TO compensate for the

effects of the right part of the system, k3 and C3 are added.

Figure 5

Sketch of forces acting on tl model used to find the mnt about the first point mass M1

(13)

Two equations of motion are needed to properly model a two degree of freedomsystem. The moment about the pin connection R and the moment about the first pointmass, m1, are used to find the equations of motion. A simplified model of the system is shown in Figure 4 which will

help in finding the moment about R; Figure 4 shows the forces acting on the model that are

rele-vant to determining the moment about the pinned connection, R.

Figure 5 shows a sub-section model used in determining the moment about m1. Figure 5

is a sketch of the system that shows the forces acting on the model that are relevant to determining

the moment about the flit pointmass, m1.

Before the equations of motion are determined, the following kinematic relationsare

defined. Referring to Figure 3 again, x1 is the displacement ofm1 in the x direction relative to the

pinned connection. The lisplacement is related to the angle e by

=

The velocity and acceleration are calculated by finding the first and second derivative ofx1 with respect to time (as indicated by x and 1 respectively):

1. = OcosO

=

[ésin(0)+cos(0)]

Also, y is defined as the displacement of the first pointmass, m1, with respect to the base of the system in the y direction. The displacementy , the velocity and the acceleratiOn $7 are defined respectively as follows:

Yi = cosO

(14)

yI 1[O2cos(0)+Osin(0)]

Finally, z1 is defined as the vertical displacement of in1 relative to afixed datum. The position of

the base is given by the displacement forcing function,itt). Hence, z1 and its derivatives are

defined as follows:

z1 =

f(t)+y1

=

The relative acceleration for mass One in the y direction1 j' , wasdefined above. Substituting this

into the acceleration gives

f(t)_(è2cosO+OsmO]

Next the displacement variables for mass two, in2, will be defined. x2 is the displacement

of the point mass,rn2,in the x direction relative to the pin contion. x2 is equal to the displace-ment of the fit mass, x1, plus the horizontal distance betweenthe two masses.

1.

1

+sm$= (sm8+sin)

The velocity and acceleration are found by calculating the first and second derivative of the

dis-placement.x2.

(15)

Also,Y2 is the vertical displacement of m2 with respectto the base of the system. Y2 is equal to the

displacement of the flit mass, Yi plus the vertical distance between m1 and m2. The relative dis. placement velocity and accelerationare given as foI1Ows

Y2

y1+cosO=(cos6+cos)

92 =

[Osin9-4sin]

=

The last definition needed isz2 which is the veitical displacement between m2 and the fixed

datum. z2 is equal the displacement of the secOndmass with respect to the base,Y2 plus the

dis-tance from the datum to the base. z2 and its derivatives are thus as follows.

z2 =f(t)+y2

Z2 = f(r)+92

= /(t)+y2

Substitution of the relathre acceleration ofmass two, y2, into the acceleration gives the equation:

12

f(t)=[2cosO+OsinO+$2cos$+sm]

With all the necessaiy variables defined, the two differential equationsof motion can be

determined. The first equation is found using Figure 4 as a guide. The first equation is

deter-mined by Summing the moments about the pinned connection, R.

= 0 = x1[m1z1 +m1g +k1(y1 y)+c191]y1m1X1 +x2[rn212+m2g '

(1)

+ k2(y2

-

+ c,j2] y2[m212 + k3(x2 x) + c3x]

(16)

moments about the point mass m1.

Mm = 0 =

c4(_O)+k4(4'_O°)+(y2yi)[m2I2+k3(Xz4)+C32]

(2)

(x2x1)(m212 +

m2g

+ k2(y2 y) +

c22]

These are the two differential equations of motion that will be used to model the system. The next step is to substitute the values of the displacements, velocities and accelerations that

Were determined from above into the equations of motion so as to representthe model in terms of

9 and 4'and their derivatives1 Substituting these values into equation (1), gives the following:

sin8[mi(j(t)_(O2cos9

+ sin9))+ mg +

ki(cos9 p;)

+

ci_ôsiñO)]

-

(3)

cose(m1)[O sinO +

OcosO]

+ (sm9 + sin$)

[m2(f(:) - (O2cosO + sin9 + 42cos$ + sin,)) +m2g +

k2((cosO

+ cos4') y;)

+ c2(Osm9

-

4sin4')]_ (cosO + cos$)[m:z(_O2sin9 + cosO

+cos4')

+

k3((sinO

+ sin$)

+ c3(cosO +

4'cos$)] o

After algebraic mmipu1atiOn, the first equation of motion can be rewritten:

01(mi +m2)+

m2(sin4sinO +

cos$cosO)+2m2(sinOcos4'_

cosOsin4')J(t)

(4)

sinO(m1 + rn2) - gsin9(m1 + m)k1

sinO(cosOY) k4sinO(cosO

+ cos4') + Ic2

.v sinO +

k3çcoso(sine

+ sin4') k3 x cosO +

cifO(sinO)2

+

c2(O(sinO)2

4'sinesin4')+ c3f(O(cose)2

+$cosOcos$)

=

_[m4sinOsin

+ cosOcos$) + 2m2(cosOsin4'

- cos$sinO) + m-

J(t)m2

Sin4' - gm2sin$ - k2çsin,(coso

+ cost) + k2

v sin$ +

k3fcos$(sinO + sin$)

(17)

Similarly from equation (2) we find:

C4(4 O) +k9(4 =

8

0)+

((cos8

+

cos$).

cos9) (5)

[m2(o2sino

+OcosO

-

2sin+ cos)k3((sinO

+

sm$)

x;)

+ c(OcosO

+

4cos)]

-

((smO

+

sink) -

sinO)

[m2(f(t)

(O2cos8+ sm8+ cos +

si$])

+ m2g

+

k2((cos9

+

cos) y

)+

c4(=OsinO

sin)]

= o

Again, common algebraic expressions are collected to yield:

c4( - O)k9(Ø

°)

=O(m cos$cos8 (6)

+O2(=m22cossin8+

nzsincosO)+ (m2(cos$)2

+

m2(sm$)2)

+

2(_m2cosqsin

+rn2çsinscos.)+

f(t)(_msin$)

+

g(_m2sin)

k2(_sin(cosO

+

cos.))

+ k2

y sine

+

k3cos(sinO

+

sin)

1c3 xcos

+

c4OsinOsinl)

+

4(Sin)2)

+c3(OcosOcos4 +

(cos)2)

Notice that the nght hand side of equation (4) s equal to the right hand side of equation (6). Equation (6) an therefore be substituted into equation(4) Also the trigonometric identities

of [sin( -0)

= cosOsin$ cos4säiOJ and [cos( -0) =cos4,cos0+sin$sinO] can be Used to further

simplify the equations. Making these substitutions into equations (4) and (6) gives the following

(18)

+ m2) + m2cos( 0)

02r.

-0)-f(t)sm9(,n1

+

m2)-gsm0

(7)

(m1 +m2)-/c1

sine(cose_YT)k2...Sifle(_...(COSe+cosØ)+

+k3cose(L(sifle+

sin$)_ r;)+k4(,_e +

O)

cO(sjne)2c2.L

(O(sinQ)2

+ )sin0sjn$) + c3(OcosOcos

(cos$)2)

+ C4( -

= 0

(cos(,

-0)

m2+O2m2!sjn,

-0)

- f(t)rn2sjn4)

-g?nsin$

+k2i (8) sinO(_

(cos0 + cos)

+

2)+

k3cos$(_(sm0

+ sin$) -

x)

-0-

0)

+ c2sin*(0Sm9 + $sin)

+ c3cos$(9cos0 + $cos$) + c4($ -0)

= 0

Next, the equations of mot on are simplified further for ease of

use. A new variable M is

defined as the totalmass of the system and the

two point massesare flOimSI ze with respect to

the total mass tocreate M1 and M2.

M = nz1+m2

m1 andin2can therefore be defined as follows:

m1 =

M1 M

?n2 =

hi2 M.

Substituting the definitions of m1 and in2 intoequation (7) and(8)yields: -.

(19)

and

efM

+ fMM2cos(

9)

MM2sin(

- 0)f(MsinOgMsin8

(9) - k1

siiio(cose_y;)+

k2sin0(-(cos0

+

cos)+

+

k3cos8((sin9

+sin4,) -

)+

k4(

- 9+ °) +

c1çO(sili0)2+ c2

(O(sin0)2

+ sinOsin) +

c3f(é(cose)2 + cOs9cos$)

+ c(+O)

=0

for the first equationof motion and,

12 .

12.2

12 ..

i

i

OMM2cos(d)

- 9)+ MM2

+0

MM2rifl( - 0)

f(t)MM2sin*gMM2-2sin

(10)

+ k2.sin4(_ (cos0

+.cos) +

2)

+ k3cOs$((sm0

+ sink)

-

x;)

+ k4($

°)'

+ c2sin$(0 sinG

+ sin) + c cos(0cos9

cos) + c ( 0)

= 0

4.

.34

4 for the secondequation of motion.

Next multiplyingequations (9) and(10)by

j2 we get

+ M2cos($

- 0) 42M2sin($ - 0)f(t)sin9gsin0

-

sin8(cos0_.)

sin0(._

(cosO + cos4i) +

+

cos9(si9

+ sink

22.]+

8

O)

+1è(sjfl0)2

+

sin0(sinO + 4sin)

+ f-cos0(Ocos0

+ 4cos) +

0) =0

M

. M

(20)

-

Cl

c1=Ii

-

C2

c2=

f =

Asin(o)t)

-6M2cos( 0)

+ +O2M2sm(4

- e) - JO)M2sin$ gM2sin +

(12) sin

(cosO + cos) +

2L)

cos4{sin0+ sin_22.)+!2(,_e_o)

+

sin$(ésine +4sin$)+

cosq(écos0 + $cos$)+

t(Q_ O) 0

M M

Mi2 To further simplify theequations of motion, the

constant variables in the equation can be

norniliwj First, the spring

coefficients can be divided by thetotal mass:

-

4k4.

K4---iF'

Mi2

The damping rates can be normalized with tespecuo the total mass by dividing the damping val-ues by M:

-

4C4

c4=___

'.4 Mi2

The forcing frequency is a sinusoidal wave in Wbih the amplitudeand frequency can be

speci-fied, f

Asin(wt). The forcing frequencyand the gravity term

are nOrn11i7ed with respect to

the length of the massless bar that connects the twomasses together. Dividing the forcing fre-quency and gravity by this lengthgives:

__2g

g The last normalizetjvalues to be defihed

are those for the initial positions of the masses.

hpartic-ular

y, ,;

, and These values are normalized with

respect to the length of the massless bars.

(21)

=

2.

2

Substituting these definitjons intoequations (11) and (12) yields the final

differential equationsof motion that are used to model the system:

o+ ØM2co(

-

-2M2sm(

- O)f(t)sjn9sm

1sinO(cose_y1)2sjflo(.., cosO Cos+2)

+K3cosO(sifle+sifl$)($0e_.2

C2SinO(sjn9 +4sin4)

C3cos9(9cosO

+$cosØ)+ C4( 0)

=

0

iJ2cos(4,-. O)M2

+ O2M2sin(?p_

O)-1(t)M2sin_M2sin,+R2

Sifl(_COSO_COS+y2)+COS$(SjflO+S.._)A;

=

0

(13)

(22)

CHAFrER ifi

NUMERICAL ANALYSIS OF EQUATIONSOF MOTION

It would beveiy diffictilt, if not impossible, to find a closed form solution for the equations

of motion of the system being modeled. Becauseof this, a numerical simulation program to com-pute the response of the system is used. A powerful software package named "isoda"[4] is used

to simulate the system response. "Lsoth" is a computer simulation that solves diffçrential equa-tions numerically. A subroutine must be Written to properly call up the Isoda package. The pro-gram and subroutine are given at the end of this sçction. To use "isoda", the deferential equations of motion must be in state space form because Isçda can n1y solve first order differential equa-tions and the model has second order differential equaequa-tions. Therefore, the equaequa-tions of motion derived chapter 2 must be rewritten in state space form.

3.1 StatE space representalion

The state space representation is the mathematical representation of the system such that the state of the system is described by the Set offirst-order differential equations written in tenDs of a common state variables [5]. The equationsof motion derived in the previous sections is one mathematical representation of the dynamical system. However, "isoda" needs the equations of motion in state space representation. First recall the original equations of motion equations (13) and (14):

(23)

O + M2cos($

-' 0)

$2M2sin(4,

- 0)f t)sinejsinO

(15)

X sin0(cos0

)+ siñ0( cosO. cOs +)

A3cós9(sin9 + sn;) +k(o

+°)+ C1(sin0)2

+ C2s1fl0(OsinO + sin) + 3cosO(Ocos4 +4cosØ)

+ C4( 0)

=0

for the first equation and the secondequation is:

M2cos( 0) + $M2 + 2M2sin( 0) 7(t)M2sm

M2sin + K2

(16

sin$(cOsOcos$+2) +K3cOs$(sin0+

sin$-;)-.4($-e-°)

= 0 The newstate Space variables are defined as the following:

Yi 0.

Y2 =

y3 =$

y4 Taking the derivative of each gives:

91 = = Y2

Y2

y3 = =

y4 =

The two equations, (15) and (16),can, be used to solve for 0 and . Using (15) and (16) pluS the

(24)

y1 = Y2

=

[1

2][M2sin(y3_yi)(ycos(y3_y1)+y)

I M2(cos(y3y1))

+f(t)(M2cos(y3 y1)sin(y3)+ sin(y1))

+(M2COS(Y3_Yl)sin(y3)+.sm(y))_isin(y)(cos(y).)

K2(cos(y1)

cOS(y3)+92)(_Sin(y3)cos(y3_y1)+ sin(y1)) A3(sin(y1)+ sin(Y3);)(CO$(Y3)CO(3_1) cos(y1)) K4(y1y3+)(cos(y3_y1)+ I)-1(y2)(sin(y1))2

C2((y2)sin(y1) + (y4)sin(y3))(sin(y3)cos(y3 y1)

+ sn(y1)) C3((Y2)cOs(y1)+ (Y4)cos(y3))(cos(y3)cos(y3 y1) +

cos(y))

C4(y4+y2)(COs(y3_y1)+1)] y3 = y4 2 M2-M2(cos(y3 y1))

J(t)M2(cos(y3 y1)sm(y1)- sin(y3))

s (y3))) + R1M2 sin(y1)(=cos(y1)

cos(y3 y1) +K2(COS(y1)

-

cos(y3)

+92)(M2sin(y1)cos(y3 y1) -

sn(y3))

+K3(sm(YI)+S1n(y3);)(M(Y)COS(YY))

+C2((y2)i(y1)+

(Y4)sin(y3))(M2sin(y1)cos(y3y1) - sin(y3)) + C3((y2)cos(y1) +

(Y4)Cos(y3))(M2cos(y1)cos(y3._y1)_ cos(y3))

(25)

C C

C

These are the final equations, which are in state space form,

that are Used in the "Isoda" package.

3.2

For an.

program

To use the isoclasoftware, an intetface fortran progr

m must be Written to call Isoda. This prograni is given below.

The state space equations are entered into the Isoda software package using a subroutine.

c2345678901234567890123456789012345

PROGRAM MAIN

C

c This program calls up the isoda

c equatjo

of motion for the two

c model. The program uses a subr

c of motion in

state, space form.

C C

C to COmpile:

c f77 -cg89

-o faraday.exe faraday.f -L/usr/fth,lib

-lcmix -lslatec -lb].as

C

C

real*8 kone, ktwo, kthree,kfour, cone

CtWo,ctee cfour

real*8 mone, mtwo length, gray,

amp, w, xinot

implicit real*8 (a-h, o-z)

dimension y(4), ato].(4), rwor]c(182)

iwork(30) v(4)

C

coxon /great/ mone,mtwo, length,

gray, anp,w,xot common /damp/ kone,ktwo

kthree, kfou.r,cone Ctwo, cthree

four

external fcñ

C

neq = 4

software package to solve the

degree of freedom Faraday wave

outjne that has the equations

OPENI1, PILE= 'fa.raday.dat') OPEN(2, FILE='Statespace out )

OPEN(3,FILE=thetaajg.)

OPDi(4,ILEphi.glea)

OPEN(5SFILE= 'theta Phase'

°P6IPILE'phi.phasel)

OPEN(7,pi='massl.heightu)

OPEN(8.FILE1ss2'.height.)

OPEN(9DFILE=Imesstàtal.height)

OPEN(lO, PILE 'massi .phase')

ON(1l,FILE=Imess2phasel)

(26)

C C C C C C C C C C C

arid the initial conditions for the (v) vector

are given in v(i), 1=1,2,3,4 Here Cv) is

determined from the equations of motion:

(vdot) = [H]Cv} + (g) {f)

Use English units consistent with the input of

ubroutine indat read (1, *) read(1, *) read(1, *) read(1, *) t = 0.OdO tout = 0..OdO itol = 2 rtol = 1.Od-12 atol(l) = 1.Qd-12 ato].(2) 1.Od-12 atol(3) = 1.Od-12 ató].(4) = l.Od-j2 itask = 1 istate = 1 iopt = 0 lrw = 182 liw = 30 jt = 2 do 40 iout = l,ntjines do -ideq = 1,neg y(ideq) v(ideg) end do C C

1 iopt,rwork, lrw, iwork, liW,

jdurn, jt)

call lsoda(fcri,neq,y t, tout, itol,rtol,atol,jtaskjstate

20 for2nat(5ej8.j)

write (2,20)t,y(1) ,y(2),y(3) ,y(4)

write (3, 20) t,y(1) write(4,20)t,y(3) write(5,20)y(1) ,y(2) Write(6,20)y(3) ,y(4) ethl=.075*cos(y(1)) eth3=.o75*COS((3)) eth2=ethl+eth3 write(7,20) t, ethl write(8,20) t, eth2 write(9,20)t, eth3 write(1O,20)ethjy(2) write(lj., 20)eth3,y(4) ntiines, delt (V(i), i1,4)

morxé,mtwo, length, gray, amp,w,xino

(27)

40 tout = tout+delt

stop

end

C *

subroutine fcn(neq, t,y, f)

C

c this subroutine

defines the state space

representation c for the

equations of

motion of the modeled system

C implicit rea].*8 (a-h, o-z) C real*8 mone,mtwo,length,grav,amp,w,xinot

reàl*8 kone,ktwó, kthree,

kfour, cone,

ctwo,cthree, cfour

real*8

m2,x2bar,ylbar,y2bar,gbar, fbar

real*8

k1,k2,k3,k4,ci,c2,c3c4 dimension

y(4),f(4),g(4)

common /great/

mone, mtwo, length,

gray, amp, w, xinot common /danp/

kone, ktwo, kthree, kfour,

cone, ctwo, cthree,cfour

C m2 = mtwo/ (mone+flitwo) c2bar=2.0 ylbar= (2*mone*grav) / (kone*length)

y2bar= (2*mtwo*grav)I(ktwot

length) gbar= 2*grav/length fbar= 2*amp/length k1 konef(mone+mtwo) k2= ktwo/ (mone+rntwo) k3= kthree/ (mone+mtwo) k4 4*kfou.r/ (length* (mone+mtwo)) cl= cone/(mone+mtwo,) c2= ctwo/ (mone+mtwo) c3= cthree/(ne+mtwo) c4= 4*cfôur/(].ength* (mone+mtwo)) C C C sy3yl=dsin(y(3)-y(l)) cy3yl=dcos(y(3)-y(].)) syl=dsirt(y(1)) sy3=dsin(y(3)) cyl=dcos(y(1)) cy3=dcos(y(3)) force=_fbar*w*w*sin(w*t) denoml=1-in2 *cy3y1*cy3yl denoni2=m2 -m2* tcy3yl *cy3yl

*sy3yl*(y(2)*y(2)*cy3yl+y(4)*y(4))

h2= force*syl_force*m2 *cy3y1 tsy3

h3=gbar* syl _gbar *m2 *Cy3yj *y3

h4=kl*syl*

(-cy1+ylbar)

hS=k2 * (-cy].

-cy3+y2bar) * (y3*cy3y1+sy1)

h6=k3 *

(syl+sy3-x2 bar) *(y3 cy3yl+cyl)

h7k4*

(y(1)-y(3)4xinot) *

(cy3yl+1)

h8=cl*y(2)*syl*syl

(28)

C

hlO=c3(y(2) *cyl+y(4) *cy3) *(j3*y3y1+,j)

h11c4*(_y(4)+y(2) )(cy3yi+i)

pl=m2*sy3yl,* (y(4) *y(4) *1fl2*cy3y1+y(2) *y(2))

p2force*xn2* (syltcy3yl_sy3)

p3g**

(syl*cy3y1_y3)

p4=kl*m2*syl* (-cyl+ylbar) *cy3yl

p5=k2* (-cy1-cy3+y2) * (*Cy3y1*Sy1....Sy3) p6=k3* (syl+sy3-x21,ar) * p8=cl*y(2) *syl*sy**y3 p9=c2*(y(2) PlOC3*(y(2)*cy1+y(4)*cy3)*(m2*cy3y1*l_Cy3) P1lc4*(y(2)_y(4))*(m2*cy3yl+1) ht=hl+h2+h3 -h4-hh6_h7_h8...h9_h1O...h11 Pt=-pi-p2-p3 +P4+PS+p6+p7+pB+p9+plO+pll g(2)=ht/deno g (4) Pt/denom2 g(1) = O.dO g(3) O.dO = y(2) = g(2) = y(4) = g(4) return end

(29)

CHAPTIR lv

CALCULATIONS OF PARAMFTERS

Now that the equations ofmotion have been derived and the computer simulation code has been written, numerical valuesfor the constant Variables of the system need to be determined

so as to match the characteristics of the Faraday wave. These constants are themasses, dashpots, springs and length of the rods. Data from the Faraday eperiment [1] is used tocompute the cOn-stants. information about the tank size and water volume is usedto determine the values for the mpsses and the length of the rods. Linear Faraday wave dataaxe used to determine the values for the spring and damping coefficients.

The determination of these valuescan be very difficult in a non-linear problem such as this one. Simpliflcations must be used to create a physical model whoseconstants can be easily deter-mined. In the Faraday experiment [I], to measure damping, thetank was forced at a resonate fre-quency to generate a standing wave. The excitation was stopped, and thestanding wave was

allowed top out completely.

Wave amplitude data

were collected to compute the damping

effects of the Faradaywave. Reference [1] has a graph of the

amplitudes of the wave on page 286,

figure 4. The peak amplitudes show a decay with a calculated decay rate of 0.050 1/s. Thisvalue is used to determine the dampingand spring constants.

It is noted that the decay rate was determined when the amplitude was small Thiscan be

considered as part of the linearregion of the system. Therefore, to simplify the calculations of the constants, it is beneficial to linearize the current model and then use theexperimental data to determine the values of the constants. The equations 6f motion forthe linear model must now be derived. The linear model will be derived in two ways. First, a linear model will be usedand the equations of motion will be determined from this model. Second,to serve as a check the n-lin-ear equations of motion will be linn-lin-earized to find the inn-lin-ear equations ofmotion.

(30)

4.1 Mass and rod length

Before derivingthe linear and

linearized equationsof motion, the

values for each point mass and the values of the niasslessrods that

connects each point mass are determined. Figure 6 shows a sketch of the tank, itsdimensions, and the

model.

Figure 6

Sketch of thedifliensions of tank Geometry is usedto help find the values of thC point

masses and the lengthsof the rods. The length of the tank is 600 mm. Thethree degree of

freedom system goes from node to node, hence it is equal to half the length of the tank fora linear

wave. The length of the two degree of freedom model is equal to half the length ofthe three degree

of freedom model. Therefore,the System being modeled is 150 mm long and eachmassless rod is 75

mm long.

For the masses, let each onerepresents a certain section

of the tank. Ifthe volume ofeach

section is the same, then the weight foreach mass is the

same. When the model Was simplifiedto

a tWOd

-of.frjom system,

the systemmass was bayed. This

means that the mass, M2,is

also half its original mass. Forsimplicity, the total

(31)

unity. This is acceptable because the system was normalized with respect to the total mass. This meansthatM1 will be 2/3 of the total mass and M2 will be 1/3 of the totalmass Actual values for

the masses can be found byusing the density of water, but this is unnecessary because the

system

is normalized with respect to the total mass Only proper ratiosare necessary.

4.2 Derivation of equations of motion using linear theory

The first derivation of the linearequations of mOtion is from a lineat model of the system. There are a few assumptions that are used in liflear theory that will be discussed1ater To start, it is assumed that the model is lying horizontally Two new angles are used to represent thetwo

degrees of freedom.

Figure 7

Sketch of model showing coordinate transfonnation

Figure 7 shows a simplified model of the system with the two new angles. For the linear derivation, the equations of motion are derived from these angles. Using linear theory, thesmall

angle approximation is used. This approxixnadon assumes that the angles O and 02.aresmall. This allows the following simplifications to the trigonometric values of the angles

(32)

Again, two equations of motion

are needed to describe the two degree offreedom system. Twomoments are used

as before to find the equations of motion:the moment about

the pin con-nection, R, and the mOmer about M1. Inthe linear model, c3 and k3 do not have

an effect on the

system fOr smallangles

ofpeturbatio therefore, they

can be ignoredj It will be seen, later in

this paper, that k4 and c4 are not needetj in thismodel and are not used in the linear

model. c4 and are retained to allow for theiruse in future research

projects. First, the moment about the pin

Connection, R, is found to get the following:

MR = 0 = kI6I+k2(oe)cll2

Rearranging this equation gives:

12i..

2,

1121r?

{mi+rn2_]O1

+{rn2Je2+[c_.cjo

+{c2jO2+[kl_+k...jo

+ Next the moment about the firstmass, M1, is found

to get the f011owing.

M1=-

rn1

(rn1 +rn2) k1

+rn2)

m(61

+e2)

= 0 (17)

1Mm

+ 62) +

c(e

+ O2) + m2(O1 Again, rearranging this equationproduces:

[rn2çjo1

+[rn2çJ2+{c2çje1

+IIc2c]92+fk2cjel+{k2]e2

= 0 (18)

Equations (17) and(18) are the equations of motion for the

linear system. To simplify the system and to match the equations of motionto what were derived

from before, thefollowing termsare defined;

(33)

k2

+ m2)

C2_(_+)

-Substitute these definitionsinto equations (17)

and (18), and multiply each by to get:

12(m1 +m2)

[M1 + 2M2Je1 + [2M2]O2 + +

+ [22]O2 +[R +2A2jo1 + [2k2]02 = 0

(19)

.+ [M2J2 + [C2J01

+ [2]

+ [R2]81 + [A2]02 = 0

(20) Next, rewriteequation (19) to get the following form.

[M1 + M]O1 + [M2]e2 + [C1 + c2191 + [c2je2+ [K1 +K2J0, + [K2]O

= [[M2101 +[M2]02 + [c2]e1 + [C2 102 + [K2]01 +

[K2J02]

Observe that the righthand side ofequation

(21) is equal to the lefthand side of equation (20) which is equal tozero. This means that the

right hand side of equation (21) is equalto zero. Also

note that M1 is twice themass of M2. Recall the

mass ratios discussed from before where M1 is

equal to 2/3 and M2 is equal to 1/3. Therefore,

the total mass is equal to one or M1 +M2 =

Equations (20) and (21) can be written as:

+ [M]02 + E:c1 + c2je1 +[c2102 + (K1 + K2J01

+ [2]02 = 0

(22)

[M2j1 + [M2]02 + [2JO1 + [2]O2 + [K2]O,

+ [Rj02 = 0

(23)

Equations (22) and (23) are the final equations ofmotion for the linear modeL

(34)

4.3 Linearization of

flon-Jine equatio of motion

Now the non-linear equations

of motion, thatwere derived in chapter 2,

will be linearjed

to derive the lineareqUations of motion.

This will verifythat the linear equations that were derived usinga linear model are correct.

Refer backto Figure 7. It

can be Seen that if the model is to be horizontal,the angles 0

and must have the value

of

. Therefore, the angles 0 and canbe converted

to the angles

0 and

e2 by using the

foUowingdefinjtj5

Next, thesedefinitions are used

to make a

transfomajo of the

tiigonoznetrjc functions from the original non-linear equalion of motionto angles in the

linearized equations Of motion in thenew

coordinate system. The definition for the sine

and cosine of 0 and$ are converted to angles

of 0

and 02, and are linearized using

a small angle approxij0

The linearized definitions of the

sin(0) and the cos(0) are as follows:

sin(_O1)

cos(01)

= 1

cos(_o1)

= sin(01) = 8,

On a side note, the followingtrigonometric identities

ate necessazy to complete theconversions.

sin(xy)

= sinxc,sy... cosxsiny

Cos(xy)

cosxcosy+ sinxsiny

The final

conversion definitions for sin(0) and cos(0)are found using the above

trigonometric identities:

.II,

,$i IC.

m_01)

=

= cos91

cos(_91)

= coscos01

+

si4sine,

(35)

Therefore:

sin01

cOs001

The same logic is used tofind the final conversion definitions

for the sin($) and the cos(0).

sm4)l

cos$=02

Looking at the non-linear equations of motion, note thatthere are terms of sm(-0) and cos(40) in the equations. To convert these to the linearized form in the flew coordinate system, the above trigonometric identities are used. Then, using the srtiallangle .approxim2tjon the sine and cosine

terms are converted.

s'n(-0)

=

sin$cOsOcos$sjn0

= 01+02

cos($ 0)

=

coscosO + sinsin0

= °I°2

+ 1 =

1aOTo

The cos($.0)conversion creates a term that has

the product of two angles. This value is a higher order term (H.O.T) and is considered srnall

enough to ignore. Next the conversions for the deny-athres of the angle 0need to be determined and

expressed in terms of the fltt and secOnd deriva-tive of 01.

Notice that the firstand second derivative of 0 is

equal to the negative ofthe derivatives of 0.

The. same derivative

conversions are Computed for theangle$.

$ =

Now that all of theconversion de nitions have been derived, all of these

conversions.

be used to linearizethe non-linear equations

of motion into the new oordinate system. Referring to equation (13) again from the original non4inear equations:

(36)

o + 4M2cos(q. 8)-2M2sin($_

O)f(t)sjnO_sm9

_K!sine(cose_yI)+;2sme(cosO

= COS 'Y2)

+K3coso(sjo+

* c2slno(esine

+ $sin) + 3coS9(co

+ cos) + C4(= 8)

= 0

Substitute the

Conversion lefinitions derived above intothi equation:

(24)

Recall, in chapter 2, some ofthe defiñitio that were made

during the original derivation of the quaxions of motion.

Simp1iflcation.o the linearized equation ofmotion can be made using these definitions. Note thefollowing:

x2

Notice that; is in the 1inearjj

equation above as part of the A'

term. With x2 equalto2, the K3 term is then equal to zero.

= 0

Note also that (O2)2, (O1)2

(OiO) and

(2O2) are áIlhigherorder When looking

atjust

the linear case, these higherorder terms do

not contribute Significantlyto the equations and can

therefore be ignorelas was stated above.

Remember that 5 was defined as follows:

For this system,

y

(37)

Now for the and A2 terms, recall:

Usingthesedefinitions,

and .v2 can be multiplied by and

A.

2m1g

1

l(rn1+m2) K2y2=

l(m1 +m2)

Adding these two prOducts together gives:

-

2(m1+rn2)g K1y1+K2y2=

l(m1+m2) 1

Also recall = Using all the above definitions

and substituting them into equatiOn (24)

gives:

01

+M202+(clc2)9Jc?82(KK)e+K$

= 0

(25)

Equation (25) is flual linearized equation of

motion for the first non-linear equation. Now reca1i

equation (14) whichwas the second original non-linear equation of motion.

yI Likewise

-

2m2g Y2 - IL

"2

2m1g 1k1

(38)

OM2cOs(s_e)+sM2+e2Msn(.e)y(t)M,

sin(_ cosO

cos4

Y2)+ K3cosO(srne +

+C2s1n$(6sine+qsin4)+cos4,(Oe._

o

First substitute the conversion

for the angle factors.

81M2--02M2+(_eI)2M2(91

+O2)M2+2(...O.

02Y2)+K392(1 + I

X)

= o

Note that 2gM2

-2m2g

jM2 =

= l(m1+m2)

= K2y2

Using this definition and thedefinitions from above,

the final linearizedequation of motion

can be calculated for the second non-iinear equation:

M2OI+M2e2+C28I+.9+KOKe

= o

(26)

Now it can be seen that the linearized

equations of motion and the linearequations of motionare exactly the same. With these

equations, values for the spring and dampingcoefficients can be derived to matchthe ch ctensties of the Faraday

waves. 4.4 Calculations of constants

Now thata linear model of the

system has been derived,

values for the constaflt variables

can be found thatmatch the characterjstic

of the Faraday wave. A modalatialysis of the linear equations of motionwill allow for the

determination of themode shapes that will give

a linear response. This linear response will allow fora comparison of the

response of the computer

sixnu-lation to the response of the experiment data at small

angles. Thiscompanson will verify if the

modeled system has the same characteristi

as the actual Faraday wave. Recall the linear equa-lions of motion for the thodeledsystem equations (25) and (26).

(39)

01 +M20 +(C1+

C2)O1 + C202+(K1 +K2)91 + K202 = 0

M201+M202+c201+c282+K291+K202

0

These equations can be rewri ten to take thefollowing form:

M22 + C202 + K282 -(11201 + C20i + 28i1, (27) and

M202 + C202 + K262 = [Gi + (C1 + C2)0i +(K1 + K2)01] (28) Notice that the right hand side of equations (21) and (28) are equal toeach Other Setting the left

hand side Of eachequation equal to each othergives:

O1+(C1+C2)0i+(Kl+t2)O1 =

M201+C201+K201

After some algebraicmanipulations the following tWOequations of motion are ascertained:

.u_M2)ei+clel+KIel

0 . (29)

and

M20I+M202+C20l+C202tK2O12O2 =

0

(30)

In matrix form, these arewritten;

[1 M

011011 +

1i

o

[o1 + fR

011011 = rol L M2 M2J 1.oI L2 C2J Le2] [2 K2] L02i L0J

(40)

Next, rewriting eqIatiOn (29) to get

-1

= (1_M2)61(1_M2) I

Equation (31) is then substituted into equation (30):

1-I

2L(l_M2)01_(l_M)01]+M202+C201+C202+K201+K202 = 0

(32)

Rearranging equation (32) gives:

M2O2+

(2

(1 M))01 + C202+

(2

-

(iM2))°' + K202 = 0

(33) Eqüations(29) and (33) are used to find the equations of motion in matrix form.

11M2 o111

0 1e11

0

Fe11 lol

[

0

Mj

Lo2i

c2(-(

C Le2i

+ K2(l)

K2 Loj = Loi

From the previous sections, it is known that the masses, spring coefficients, and

danipingcoeffi-cientsmaintaincertainratiostoeachother. Thisprovidesthat M1

,M2 =

andthat

2R2 =

C1 = 22. Substituting these values into the above matrix gives:

o11oI1+12X2 01181 rol

o

LJ

0 c2j 1e21

[ 0 K2j

L02]

iq

Multiplying the first row by and multiplying the second row by3 gives:

(41)

F101111+32 0

Fei LO 1J[o2j

0 32 [e2

i32 ol[ei

L 0 3R2j [02 -.101 LqI -4' This produces two decoupled, single degree-offreedoni equations of motion that have the form:

01+3C201+3K201 = 0 - (34)

02+3C202+3K292 0 (35)

This shows that the masses are uncoupled. In other words, in the linear case, the position and velocity of one mass does not, have an effect on the position of the second mass. One of the m2in reasons is that in the linear case, K3 and C3 have no effe t on the system. Without these, the total

system is juM tWo uncoupled systems.

Data that was derived, in the original Faraday experiment [1], is used to calculate the

-spring and damping values. The forcing frequency of oscillation for the period one Wave was 3.23

H2 [1] The frequency of the period one wave was -at half this 'alue. Therefore, the frequency was 10.147 rad/sec. This is the natural damped frequency of the model, Wd. It is also known that

the. ihmping tate of the faraday wave was 0.O5 [1]. This informati- on is used to compute a value

for the spring and damping coefficients

Under standard vibration theory s the damping tate of a one degree of freedom system usually defined as [7]:

and the damping ratio is:

r

2Ma) Therefore

(42)

, C 3 2

Because the damping rate beta is equalto 0.05 the damping values

0 the system is calculated to betobe, C2

= 0.o. Because

istwicethevalueof2

= 0.0g.

The dampedfrequency for a single degree of freedom

spring-dashpot system is [6]:

=

Jj2

Using the definitions

of and o, the

equation for the dampedfrequency can be modified

to be:

£

Knowing that 0d= 10.147 and = 0.05, simple

calculation provide that A;2

= 34.323. This

means that A;1 = 68.64& Tis information

can be used to simulatethe free vibration of the sys.

tern.

When simulatingthe free vibration,it is important

to note the value of the dampingrate. To see if the system matches the llneai

response produced by thefaraday wave, the computer

sini-ulation has to be tested using small angles as initialconditions.

One otherproblem that arises is that

the system has two degrees of freedom

and not one.

This means that the system has two mode shapes thatneed to be found

to simulate the linear damping. The mode shapes are found by findingthe eIgenvecto

of the linear system.

The mode shapesof the system vill be

calculated by finding the mode Shapesof the linear form of the model.

Recall equations (25) and (26) which are the linear equationsof motion. Ignoring the damping coefficients, these equationsin matrix form are:

11 MJ Foil

[M2

M2JLJ

For simplification,use the following

nOtation [61:

112211°1l

= fol

I

2 A;2][02] [.0I

(43)

Me+X0

= 0

This can be rewritten to be [6]:

Mke

The linear equations are. now in state space form. From heredefine the A matrix to be [6]:

=

To find the mode shapes ofthe linear system, flhd theeigenvectors of the A matrix [6].

The mode shapes for this systemare:

['liol

The first mode shape will be sun lated as a checL The initial angular velOcities for each

angleiszero. Thismeansthem

esstartfromrest Letthein

angu1arpositionofo...

+ 0.001 1.5717963268. Because the initial

angular position of the secondmass is uncoupled, it

does not matter where the mass is placed. For this test, let have an initial angular position

of

= = 1.5707963268. This is a value that has the

second mass flat with respect to the horizontal.

Figure 8 shows the results of this simulation. Notice thateven though mass one is oscillating,

mass to remains horizontal. Thisshows that the

movement of mass One does not affect the

movement of mass two. Next, thesame Simulation will be tried but in

reverse order. Begin, again, with zero initial angular velocity.This time 0will have a hOrizontal initial condition, or 0=

3

= 1.57079632, and

will have an initial position of =

+ 0.001 = 15717963268.

Figure 9 shows the result of this simulation. Again, the Same results as in the first simula don are shown in thesecond simulation. For

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3

II

--height of meBa I'andmaee

2(metere) ---'. .4... -S ...p S...IP St... I-. Lii -.1 II

jTf'':

1:1

0

o

height of mesa land

rnass2. (meters)

21

I

(45)

which both masses are going to oscillate. Again stall frothrest by having bothangular velocities zero. Consider initial angular positions

of 0=

- 0.002= 1.5687963268, and $ = + 0.001 =

1.5717963268. Figure 10 shows this results of' this simulation.

0.00015 0.0001 os -0.00015 0

Ii

2 4 $ (sec) A 9 10 Figure 10

Linear response of system with bothM1 and 142 displaced 0 = 1.5687963268 rad, = 1.5717963268 rad, 0 =$= 0

With this simulation, it is again verified that the two degrees of freedom are indeed uncoupled. The position of mass one was initially started at twice theheight of mass two. Throughout the oscillation, mass one was always double the height of mass two. The masses alsomaintained the same damped frequency. The movement of one mass did not affect themovement of the other mass.

It needs to be determined whether the response of the system matches the time histoty

of

the Faraday wave. A fortran programwas written that is able to determine the time and heights of the peak elevation for each oscillation, With this, thedamped frequency and the damping rate

can be calculated. To find the damping frequency, the period of eachrnaxnnum needs to be deter-mined and then converted to rad/sec. To filid the dampingrate, the natural log oEeach maximum is calculated and plotted, then the leastsquare line that best approxirn2u's the

points is found. The

lIlItIf H III! 1111i1ii

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slope of the line wiljb

the am,ing rate

To assist in the visualization Of this, the followingexample was created. The following formula is used to demonstrate a damped oscillating Wave: y(t) = esin(cot). Figure

11 shows the

time history of thedamped sine wave using

a natural frequency of o = 10 rad/sec and a damping

rate of 0.3/sec.

-i

Figure 11 Figure 12

Plot of damped sine wave with envelope curve Plot of the wave-peak decay

with least-square

w lOandP=O.3/sec

approximation 5=O3Isec The wave is dampedby the e terni and forms the envelope

curve. is the dampingrate that

was discussed previously in this section. From this, the peakvalues that form the envelope curve are found. Two of these peak values can be used to find thedamp

frequency. The damped fre-quency is found by:

COd(.)(

Remember that the dampedfrequency is not the Same

as the natural frequency. From before, the damped frequency isequal to

0d=

With a dampingrate of 03 arni a natural frequency of

10 rad/sec, the dampedfrequency should be about9.995 rad/sec. Using the data from the computer simulation,

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calculated to be 9973 rad/sec. This is very close to the atual value.

To calculate the dampingrate of the Simulation, begin by looking at the part of the

equa-tion that has. the dampingrate by iseif. The equation isas follows:

y(t) =: Ae

Taking the naturaj logarithm of each side and doingsome algebraic manipulation, gives the fol-lowing:

ln(y) = ln(A)z

Notice that this fonxaila has.the same format asa for ula for a line in Which

is the slope.

Divide each peak value bythe value of the very first peak.and then take the iaturai logarithm of it.

A.=

(H

Figure 12 show a plot of all these points. Using a least squares approxinition, the slope Of the line can. be found and thiswill give the value of the damping

rate. For the example problem, the damping rate is 0.300844, which is very close to the original damping rate of 03.

figure 13

Linear response of M1 with envelope curve

0=1.5717963268 md, =1.5707963268 rad, 0=41 = 0

figure 14

Plot of the wave-peak decay with least-square

approximation = 0.05/sec

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Now look at thedamping rate for the system that

was originally modeled. The flstmode

shape is used and onlythe response of the first

mass isplottecL Figures 13 and 14 showthe response of the system and the leastsquares approximation. For this Simulation,

the damped fre-quency was calculated to be 10.150 rad/sec which is very close to the Faraday waves 10. 147 rad/ sec. The damping ratewas found to be O.OS00008/sec which

is the same as the Faradaywaves

O.OSIsec. This shows thatthe computer modelhas the same linear characteristics as the linear rsponse of the Faraday wave.

Next, the system will be forced at the proper frequency

and amplitude to get a period one

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CHAPTERS V

NONLINEAR SIMULATION RESULTS

Now that a computer simulation of the model that matches the characteriStics of the Fara-day wave exists for the linear case, tests need to be performed to ensure that the model matches the character tics for forced amplification. Simulations need to be completed to find period one and period three waves. The period one and penod three waves are found through trial and error by running numerous Simulations and changing initial, conditions., Te initial conditions that are

changed are the angular pOsition and angular Velocity of the two degrees of freedom 0 and . The forcing frequency and forcing amplitUde is also changed. After this, 'it is important to see if the

period one and period three wave can be attained by starting the system from rest in the horizontal

position and then using oüly the forcing frequency to excite the system to a period one and period

three wave.

There are numerous initial conditions that can be used to produce a period one wave. Some of the waves initiate as period one and then become unstable overtime. Further research would be to find all the stable and unstable period one waves and determine areas of stability.

To demonstrate the period one wave, the following initial conditions are chosen. For this example, the initial condition ofOis 0 = 1.9394222 rad.. This is equivalent to starting at 0.027025 meters below the horizontal. The initial condition of is Q 0.75032909 rad which is 0.05486 meters above the horizontal. The initial angular velocities are 7.665593 rad/sec for 0 and 7.3153634 rad/sec for 4,. The forcing function has an amplitude of 0.006 meters and a frequency of 10.2324844 tad/sec. Figure 15 exhibits the time history of the response Of the System. The first plot is the response of just mass one. This is the height of the point mass M1 relative to the horizontaL The second line represents the height of the.second point mass M2 relative toM1. The

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third response is a time history of the total height of the system relativeto the horizontal. When

a

standing wave is being simulated,as in this case, the total height is the maximum amplitude of the system.

-Figure 15

System response with period one standingwave

Figure 16

Phase plane of system: periodone

Figure 16 is the phase plane plot of the firstpoint mass M1. This shows that the

system is a stable period one standing wave.

Obviously, trying to start a system like this in a laboratory environment using these initial conditions is very unrealistic. In the original Faradayexperiments, the tank was started from

rest. Over time, the water in the tank evolved to a standing wave of period one. For the computer model, it is desired to match the results of the experiment In the experiment, an amplitude of 0.00265 meters and a frequency of 20.106 rad/sec [2]. This gave a damped frequency of 10.053 rad/sec (the Faraday wave isa first subharmonic, which means that the forcing frequency

is twice the frequency of the Faraday wave). The model in this thesis is not garnered in the same manner as the Faraday wave. The forcing frequency for all of the computer simulations will be the same as the damped frequency from the experiments. For this example the frequency used is 10.053 rad/sec. The initial angular velocity forboth B and is set to zero and the system isstarted in the horizontal position, which is for both angles. Figure 17 shows the time history of the simula-tion for these condisimula-tions.

53 t 1.1

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E 0.08 0.06 0.04 0.02 0 -0.02 -0.04 -0.06 -0.08 0 20 40 60 80 100 me (see) Figure 17

System response, from rest, of periodone standing waves amp =0.00265metezs, w = 10.053 rad/sec

Note that after about 150 seconds the system is in period one motion. To better analyze the sys-tem, figure 18 shows the response of the M1 component of the system from 190 seconds to 200

seconds.

Figure 18

System response, from rest, of periodone

standing wave from 190 sec to 200 sec amp = 0.00265 meters, w = 10.053 red/sec

Figure 19

Phase plane of system, from rest from l9Osect000secpeiiodcee amp = 0.00265 meters, 0=10.053 md/sec

I'S IN * , 120 140 160 180

-I

(52)

From figure 18, itappears that the system is exhibiting periodic motion and specifically penod

one motion. To check this, the phase of thesystem is plotted using only data points from 190 sec-onds to 200 secsec-onds. Figure 19 showsthe phase plane and it is seen that thesystem is period one. These simulations demonstrate that the computermodel can be started from rest and resonated to a period one standing wave using the same amplitude and frequency as in the physical Faraday

wave experiments.

One of the periodone responses of the Faraday wave in the original experiment had a dim-ple in the free surface [1] If this dimpled crest can be simulated, it will provide cv dence that the

model matches some features of the Fataday wave. The dimple effect.is Illustrated using Figure 20. The figure shows that as the wave is at its max mum elevation, a dimpled crest forms at the peak of the wave [1]. In the experiment,the dimpled wave was found usinga forcing amplitude of 0.00385 meters. Figure 21 shows the response of the system using a forcing amplitude of

0.003705 meters and the same forcing frequency, 10.053 rad/sec.

Figure 20

Sketch of dimpled standingwave with idealized model

a

jut:

V I I I V

ti

t q

___=

a I Figure 21

System response of periOd one dimple amp = 0.003705 meters,

0

= 10.053 rad/sec

Figure 21 is the corresponding system response andit shOws that the system exhibits the dimpled response. The model shows that the dimple occurs at both the maximupi and minimum elevations

unlike the Faraday Wave experiment.

To further test the model, it is desirable to match the period three response of the experi-mental system. Again, trial and error was used to find initial conditions that have a period three

$ I

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response. The initial position of 0 was 0 = 1.9817702 rad and fore was$ =0.66793155 rad. These are equivalent to placing M1 at 0.02996267meters below the horizontal and placing M2 at 0.0588828 meters above the horizontal. The initial angular velocities are 0 = 7.6345674 rad/sec

and 4) = 7.2529606 rad/sec. The forcing function has an amplitude of 0.006meters at a frequency of 10.18336536 rad/sec. Figure 22 shows theresponse of the system using these initial condi-tions. Figure 23 is the phase plane of the system forM1.

2 $ Figure 22

-at -to S Figure 23

System response with peiiod three standing wave Phase plane of system: penod three

From the phase plane, it can be seen that the system is a period three standing wave. Again, these initial conditions are not easily implemented in a laboratory setting. The system should be tested from rest, using a forcing frequency and amplitude,and excited to a period three wave. This

proved to be a difficult task.

As with the period one standing wave, the initialangular velocity is zero for both 0 and . The initial angular positions for e and are , or horizontal. In the original Faraday wave exper-iments, the period three standing wave was obtained using a forcing frequency of 10.053 Hzand an amplitude of 0.0046 meters [21.

Using these values in the simulation didnot generate a period three standingwave. The model showed this wave to be breaking. Theexplanation of the simulated breaking wave will be explained shortly. To find the period three standingwave, the value of the amplitude of the

fore

(54)

ing was varied,while the forcing frequency was held constant. The amplitude was changed until period three was found. At an amplitude of 0.0038meters, a period three standing wave was

found using the computer simulation. Figure 24 shows the time histoiy of the response.

E

Figure 24

System response, from rest, of period three standing wave, amp= 0.0038 meters,0= 10.053 rad/sec

.0 S

-Figure 25 FIgure 26

System response, from rest, of period three Phase plane of system, from rest,

standing wave from 240 sec to 250 sec from 240 sec to 250 sec: period three amp = 0.0038 meters, o = 10.053 rad/sec amp =0.0038 meters, 0=10.053 radFsec

I

I

3 3 3 S

(55)

To facilitate viewing the period three motion, Figure 25 is a graph of the system from 240 seconds

to 250 seconds. Figure 26 shows the phase plane of the system with these sair data. It is clear that the system is exhibiting period three behavior. Note that this is a very stable period three

standing wave.

Figure 27 Figure 28

Plot of system demonstrating breaking waves Plc of system demonstrating breaking waves for height of M1: amp = 0.0045 meters, for angle of 0: amp = 0.0045 meters,

W= 10.OS3rad/sec (U= 10.053 rad/sec

IO 0 10 20 30 40 70

Figure 29

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Increasing the forcing amplitude to 0.0045meters was done next to demonstrate chaotic behavior. Figure 27 shows the results of the smulation. Itis difficult to see whether the system is

exhibiting breaking wave behavior in Figure 27. To facilitatethis, Figure 28 is a plot of the angu-lar position Of 0 for the same simulation. It is clear that the mo el is rotating about the pin con-nect.ion. For this model, this behavior is considered wave breaking. A plot of the phase is shown in Figure 29. This shows that the system does not become periodic. The system shows contiñu-ous breaking wave behavior. It is easily seen that increasing the amplitude of the forcing gener-ates more breaking waves and chaotic-like behavior of the system. This then shows considerable similarity with the results of the Faraday experiment in that thesystem goes from period one, to periOd three, to bteaking.

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