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Office of Naval Research Department of the Navy Contract No,

N62558-2269

Unsteady motion of a flat plate in a cavity flow

by

JA. Geurst

Reproduction in whole or in part is permitted for any purpose of the United States Government

June 1 959.

Instjtuut voor Toegepaste Wiskuride Technische Hogeschool te

Delft Nederland.

(2)

C 0NTEI'TS.

Introduction

Part I. Reentrant-jet flow with unsteady perturbations0 Summary

The steady flow

Li..

The unsteady motion as a perturbation of the steady flow Additional conditions

First order approximation for small breadth

Part II. Linearized theory of the unsteady cavity flow Summary

Linearized theory of the steady flow

The unsteady flow; method of the complex velocity Linearized unsteady cavity flow as a first order approximation

11 The unsteady flow; method of the complex acceleration potential

The drag

(3)

2.

1. Introduction.

The publ±catjons about the unsteady motion of a body in a fluid with free streamlines can be divided roughly into three categories.

The first category deals with exact solutions. In that case it is necessary to restrict the field to instationary motions of a

special ty-pe. Voii Krmàn [i.] was the first, who

took

that direction,

Later on publications appeared by Gilbarg [2] and Woods [3]. Under the second category we will class those articles, in which the unsteady motion is considered as a perturbation of the

steady flow. Woods [Li.] investigated in that way the instationary

motion of a flat plate according to the Helrnholtz,-Kjrchhoff

model. Wu gave in [5] a formulation of a boundary-value prOblem for the Roshko model (also named transition model). Closely

connected with this is the research on the stability of free streamline flows. Ablo.w and Hayes [6] published a report on the subject,Thejr

results were extended by Fox and Morgan in [7].

The third category contains papers, in which the whole flow is linearized. Tulin [8] was the first, who applied the

linearization on a steady flow, arkin [9] solved the unsteady problem of an in±inite cavity behind a flat plate under incidence and gave a formulation of the finite cavity case. Wu developed in [-lOjand [5]. a theory f or theuneteady finite cavity case, Tiirnan [1-1] and

the

author [12] treated the case of a partially cavitated flat

plate

under incidence. The unsteady motion is considered small with respect to the steady flow (second linearization). In order to

get a closed cavity they assumed a discontinuity in the unsteady vertical pertur-bation velocity in the wake of the body. Another possibility is to

abandon the closure of the cavity for the unsteady case and to re-quire that the normal.component of the unsteady perturbation velocity

(4)

3.

should be Continuous in the wake. As a result of a discussion with Dr. Eisenberg and Dr. Tulin this last possibility

will be investi-gated in this report by comparing the linearized cavity flow with the corresponding reentrant-jet flow. For a steady cavity flow it has been proved, that linearized theorrjs

a first order approxi-mation to reentrant -jet flow theory [13] . From the following it will appear that also in the unsteady case linearized theory can be formulated in such a way that it becomes a first-order approximation to reentrant-jet theory. We will prove this connection, just as in

[13]

, for the siiiplest

case of a flat plate, moving perpethicular to its plane. The research splits up into two

parts.

In the first part we consider'the reentrant-jet

flow with un-steady disturbances9 As a result of the linearization

we can assume this motion to be harmonic in time without

loss of generality.

In the second part we treat the linearized problem. The solution is obtained by two different methods. The first method uses the

complex velocity and is directly connected with

the first part of our research. The second method starts with the

complex accelera±jon potential an

offers the best perspectives for more complicated problems9

Finally it should be

remarked that we have omitted in this introduction papers, that deal with the

beginning of the unsteady motion. Several Russian authors have worked in that direction e.g.

Gurevich [iLi.]. Their investigations are directed towards the

deter-mination of the cavity induced mass (see

Birkhoff and Zarantdnello [15]). In this report however, we are interested in the

instationary motion as a whole.

(5)

I. Reentrant-jet flow with unsteady perturbations. 2. Summar

A flat plate is placed in a flow of an incompressible non-viscous fluid with uniform velocity perpendicular to the plate. Behind the plate a cavity with reentrant

jet has formed. The jet is supposed to disappear on a second sheet of the physical plane considered as a Riernann surface. This artifice is used to represent within the framework of potential theory the dissipation of energy, that is observed at the rear end and in the interior of the

cavity, (see Bjrkhoff and Zarantonello {15]). We prefer here th

reentrant-jet model above the Riabouchinsky.model, since the former shows

more resemblance to experimental observations (see Eisenberg [i6]).When the plate performs an unsteady motion, th shape and size of the cavity will change. If we assume that the deviation from the

steady position. is small in a certain sense, this unsteady motion can be considered as a perturbat.jon of the original steady flow (lineari-zation of the unsteady effects),

We treat first the stationary flow Next we investigate the effect of the unsteady motion.

3e The steady flow.

The steady symmetric flow about a perpendicular flat reentrant jet is shown in fig. I

Bv

fig. I.

plate with

(6)

5.

The Cartesian coordinate-system has been chosen in such a way that the middle of the plate lies in the origin and that the velocity of the fluid at infinity has the direction of the positive x-axis. We denote half the breadth of the plate by b. We assume the fluid to be incompressible and non-viscous and the motion to be steady and

irrotational. The relation between the pressure and velocity is then given by the Bernoullian law:

p+pU2

=

p±pq2

+

(3.1)

where q magnitude of velocity

p pressure

U velocity at infinity p pressure at infinity

velocity on the cavity

PC constant pressure on the cavity

p constant density of the fluid

We choose the units of length and time in such a way, that the

constant fluid velocity q0 on the cavity is equal to I The suscep-tibility of the fluid for the occurrence of cavitation is characterized. by the cavitation number cr, that is defined by

p -p

o 00

(3.2)

1

Prom (3.1) and (3.2) follows that

equations

= 0

ox

oy

+ - 0

ox

0y continuity equation irrotationality

(3.Li)

These equations express, that w = u-iv is a holomorphic function of z=x-i-iy in the interIor of the fluid. On account of (3.Lj.) we can define a velocity potential c and a stream function ? by

u = (i+oj (3.3)

Let the velocity vector = (u,v), where u and v are the x- and y-cornponents of the fluid velocity. u and. V have to satisfy the

(7)

(a) 0

(c,a)

(do)

fig.

2.

We now determine, in a) and b) (see below)

respectively and w as a function of t. The conformal mapping i.e.

z as a function of t is then given by 6.

U=-

y

ôy

= -

(3.5) 'Then

= c+ip

is a holomorphic function of z=x+iy, and

w=a

(3,6)

At the moment we consider only the upper half of the physical

plane i.e. the upper half of the region taken by the fluid0 As

a result of the presence of the reentrant jet this region is

two-sheeted. Since the region is

simp1y-connec,

we can map it conforrnally onto the upper-half of a t-plane (t= cT+iT).,

Remark: this o is as a matter of

course different from the a- defined

b

(3.2)...

This will cause no confusion in the following. The images of 3 points on the boundary

can be fixed arbitrarily. We choose the image of Z=oo as t = oo

the image of A as t = -a and the image of B as t = 0. a is a given positive

number (see fig. 2).

clz=w'1 d =w'

dt dt

or z

=fw

(8)

K dt t-c where K is a real constant

and = K [ t-(d-c) log (t-c) ] + constant

7.

(3.8)

(3.9)

b) Determination of w as a function of t. We introducefl log w = log q-ii9' , where

is the angle between the velocity vector and the positive x-axis. fL is a holomorphic function of t in the upper half-plane. has to satisfy the following mixed boundary conditions:

o°<o<a

=Q

or

ImS=0

-a

<o-< 0

or

Irn!l=-0 < o < c q = I or ReS1 = 0 (3.10) c

<cr<d

=-7

or

Im2=jr

d

<o<oo

9=Q

or

irnLO

For the solution of this boundary value problem we continue IL analy-tically into the lower half-plane by means of the reflection

principle of Schwarz £2.(t) (3.11) a) Determination of as a function of t. We consider .

is a holomorphic function of t in the upper half-plane. Since the real axis is the image of streamlines (where

= constant), is real along the real axis, By means of the

re-flectjon principle of Schwarz we can continue

analytically into the lower half-plane,

can have singularities on the real axis. These can be no essential singularities (for

a proof see Birkhoff and Zarantonello [15] ). Singularities can only occur at t= and. t=c. From a consideration of the local behaviour fllows, that remains finite at t=oo and behaves like

at .t=ó. As a result of the

branching of the streamlines at the point D,

will have a siniple

(9)

8.

The boundary value problem is now equivalent with thefollowing

Riemam-i-Hi]jjer problem (see Muskhelishvili [i 7]).

Determine .cL(t), holomorphjc in the upper and lower half-plane, with

the following linear rel.tions.on the real axis.

oo<cT<

a - a

< T

< 0 - 7rj +

O<O<c

1+=O

(3.12) c < 0 < d. - = 2 gj +

d<o-<00

ü

and STL denote the boundary values .l assumes in approaching the

real axis resp. from the upper and lower side.

Moreover Si has to be continuous at the pOints t = 0 and t = c. At infinity Si must remain finite.

We consider first the homogeneous Riemarin-Hilbert problem i.e. the above mentioned problem with the right hand sides in (3.12) replaced

by 0. A solution of this homogeneous problem is.

= ft(t-c)

(3.13)

The cut in order to make the scjuare root single-valued is taken along the real axis from t = 0 to t = c. The branch is chosen in such a way that

trt(tc) t

as too

The Riemann-Eilbert problem (3.12) can now be formulated as follows Determine Si(t) in such a way that' on the real axis th'e following

relations are fulfilled

oo<cr<--a

{-].-i-] =0

- a < o < 0

+7j

(10)

< 0- < d

After some calculations we arrive at

fl=- log

w=

-a t

.11k

27i

[]

- [ci

=

__

+ log C ['fd( t-c) ft(d-c)] and Iid(t-c)-Tt(4-c)1 [Tt(c+a)fa(t-)] ' [Td(t-c)ft(d-c)]

The expression for z as a function of t can now be written as

z =K

f4G

d$.

td-c

dt

J [It(c+a)_fa(t_c)]2 [tfd(t_c)4t(dc)] t-c

9.

(3018 )

Remark: (3.16) and

(3.17)

represent and w also in the lower half of the physical plane when we map it. coaformally onto the lower half of the t-plane by means of (3.18).

In the solution,which is the combination of

(3.17)

and

(3.18)

,three unknown constants viz. K, c and d. still occur. These unknowns are

determined by the following conditions

i ) at t oo we must have w = U = (i -for

z has to be a single-valued function of t

the distance between A and B = b = half the breadth of the flat plate.

We first formulate conditions 2) and 3) mathematically..

The condition that z should be a single-valued. function of t, reads e dt = 0

(3.19)

d < cr<oo

=0

(3.1 L)

By theans of the formulas of Plemelj (see Mukhe1ishvilj [i71)we find

0 d. fL=a/t(t_c) _t.[

f

+

f

2i d

(3.15)

27V1j

o-o)(o-t)

J {'ft(c+a) -fa( t- )]

(11)

Condition

3)

can be written as

fedt=i

-a

We now apply the .3 conditiOns to the solution we have found. Condition i gives us

(i +o) rc+a-'f]

[J3.

Condition 2) furnishes the equation

Cf

+c=0

Prom condition

3)

we obtain

0 .1 K

I [L±.ac-c

2 dT-c-Th- d-c = bj (3.2L.)

I

[!o(ca).4a(T_c)]2 {d(-c)--T(d-c)]

OC

Elimination of between

(3.22)

and

(3.23)

gies the following relation between c and

o.

(3.25)

1+0- =

[j1

+11+

Moreover it can be derived that

ry

[i-

/

-1

(3.26)

and

d-c =

(3.27)

The integral in (3.2)-i.) can be expressed in elementary

functions,Sjnce we don't need ouch an.expre5sion in connection with the purpose of our research and since the expression would become rather unwieldy,

we

omit the expression here.

10.

where C is a closed contour surrOunding the plate and cavity i.e. surrounding that part of the real axis that lies between -a and d. Application of the theorem of residues on the exterior of C giveS

res. e

dt

too

= 0

(3.20)

(3.21)

(3.22)

(12)

It.

(3.25)

gives the relation between c and o-.. Prom

(3.27)

follows the connection between d en o. Finally (3.2L1.)determines K as a. fuii.ction

of b and a-. Thus the solution for the steady case. is completely

determined.

The unstead motion as a êrturbation of the steady flow. jwT.

Let the flat plate perform an oscillation.of the form he normal to the ma±ri flaw. ByT we denote the time variable, h is the ampli-tude of the oscillation. The dev±ation is taken positive in the

direction of the negative x-axis, Thus the normal velocity in the

jw7

direction of the negative x-axis is equal to jwh e

Remark: it is asEumed tacitly that of all expressions, in which occur exponential terms complex with respect to j, we must take the real part in order to get the true time behaviour0 Since we linearize the unsteady part of the motion, this procedure will cause no troubles. Finally as a matter of sourse the imaginary units i and j are

dis-connected; we have i2 -I and = -I , but ij is not reducible..

We now suppose that Wh is small with respect to unity. In that case the unsteady motion can be considered as a perturbation of the steady flow. We will neglect, as usual, second and higher powers in the dis-turbance against first order terms.

As a result of the unsteady motion c and d will become functions of the time T, Also the boundary conditions will change

a) On the flat plate, i.e. on the interval -a < a-< 0 of the real axis of the t-plane, we will now have in a first order approximation

=

e'

(Li..i)

(see fig. 3), where q0 is the magnitude of velocity in the unperturbed steady flow.

(13)

1L

SWy

fig. 3.

Remark: quantities referring to the steady floW will be denoted by the suffix 0, and these referring to the first order terms of the unsteady perturbation by the suffix 1.

b) On the boundary of the cavity, i.e. at 0

< 0

< C,

the instationary Bernoullian law will now be true:

+

q2 + = c(T) (L.2)

We put

=

o + and p = p0 + p1.

In a first order approximation (L1.,2) can be written as

+ q + q02( -)+ + C(T)

or as ±

q02

- + - = D(T).

q1

If we put

= r , the Bernoullian law becomes

0 1

a OT

p

± q r1 ±

= DT)

(L1.5)

Remark: At the partial differentiation against T the space variables are kept constant; this amounts to the fact, that rp0 and are kept constant.

On the boundary of the cavity we have p1 = 0, thus

+ qr1 = D(T)

oh the cavity Li..6)

12.

We apply this equation on the boundary of the unperturbed cavity. The corresponding points are found by orthogonal projection. In that case

(L.6) is in a first order approximation replaced by

+ r1 = D(T) on the unperturbed cavity

(14)

13.

since .there %=1. Moreover on the boundary of the unperturbed cavity it is true that

= constant

On differentiation of (L1..7) against we get 0.

We will show first that

lj

oo

-r and

I

2) r1 - i&1 is a holomorphic function

of t, with = Putting = + have d. dz W (

o)

-

-

dz - - I .1

In a first order approximatio

w = e = e a I

= e°(1cL1) =

w0(I+1)

or

L.1

=-w0

Always in the seine order of approximation

= log w = log q - i& =

log q0(i

- i& -= log + r1

-- i1

+ r

-Thus = r1

- is a holornorphic function of t.

Prom (L.IO), (L.i2) and (1.iL) it follows finally that

= =

r

q.e.d. (.15)

On the unperturbed cavity the boundary condition now reads

as

(Lj..iG)

or r1 =

(Lj..i 7)

i.e. r1 is a function of T-cp

In our case of harmonic lime dependence we have

j w (T-cø)

r1 = g e

where g is a still

unknown

constant, real with respect to 1, but possibly complex with respect to j.

a

vnw'

F

-(L1.,9)

(15)

ILl..

We anticipate here this harmOnic time dependence. The justification follows only by (5.1.5), since it expresses g linearly in h.

For S1 = Sl + the following mixed boundary value problem can now

be formulated.

Determine fl.(t), holomorphic in the upper half pland, in such a way

that it assumes on the real axis the following boundary values

<o-<-

a

orlmfl=o

- a<

o-<

0

oo<cr<a

-

a < cr< 0

0 < 0

<

c

C < O- < d

d<0<oo

+

e'

or Im =

-

jwh eT

2 q0 2 ci.

jw(T-)

j(T-p ).

0

< o

< c log q0+r1 =g e or Re l = g e 0 (Li..i 9)

c<cr<d

=-7r

orImS=+7r

d<0<oo

=0

orlmfl=O

Putting

fL(t)

= T3T

according to the Schwarzian reflection

principle we can transform the mixed boundary value problem into a

Riemann-Hubert problem with the following linear relations along the real axIs

-a<o-<O

_fL...ti_2j.2eJ0

-

.

w(T..p)

0<

cr<

c Sl +fl

= 2ge

+

c<o-<d

fi -Si

=27ri.

d<0<oo

Remark: g can be taken equal to zero at c < 0- <

c if c0 < c. Letting c=c0+c1 and d=d0+d1, this Riemann-Hilbert

problem (Ll..20) can

be split up into the following

Riemann-Hjlbert problems for 11p and

çL where fl =flp

PLp-

cLp = 0 -ALp

7r1

+ Sip

+fLp =0

clp - SaD = 22ti - flp = 0 and (Ll..20) (Lj..21 )

(16)

00<0<-a

ci+SL_O

S S

-a<o-<Q

s S q

o <

o- <, c0 fL+ + =

2ge'

C

<0<oo

fl+fLO

0 S S

According to (3.16), the solution of

(Lj.2i)

is

= ..

L(c±aHcJJ.

+ log L[d(t-à)ftLd-c)i

(Li..23)

{Tt(c+a)fa(t-c)] [fd(t-c)t(d-c)] We now determine the solution of (Lt..22). By means of the

solution of the homogeneous problem = t(t-c0) the R.H.-problem (L1.22)

can be written as follows - <

0- < -

a

-a<< 0

0<o<

0

-a

ci

-=0

cih+

[fd(c-.r)

+'I-o-(d-c)]

Jo(c0-o) (o-t)

(L1.22) (L..2L1.)

(L..25)

(L.26)

Using the formulas of Plemelj (see [16]) we get finally ci=

et(t-c )

J [a(c-0-)-[-0-(c+a)]

[Id0(C-o)-J-d-(d-c)]

c ,jWK[cr-(d

-C )

log (c .o-)]

____ -

e AJt(t_c e 0

I-cr(c0-cr)(o-t)

C0 < 0- <

00 It

atO<o-<cwehave

= .K [-.(c10-c0) log (c0-)] and by virtue of (3.17) at - a < < 0

[Ja(c0)(ca)]

'I = -2i jaa 2ge

(17)

1.6. From (Li..23) and (L...27) we

find

=

t

a

d1

ft(t-c0)

/

d

+ .i_wh

et(t-c)

Ed(:_)-(d-c)]

J

[IdC-)J(d-c)]

'dcr

-

£ ei°7'rit(tcjf -(d0-c0) log

(c0-c)]

(Li..28)

5

Additional conditjohs.

In the expression (L..28) for three unknowns still occur viz. g,

C1 and d1 ; g is a constant, possibly complex with respect to j, since

we have already anticipated the time behaviour of GT-cD); the two other unknowns, C1 and d1 are functions of T, complex with respect to j, which will appear to be of the exponential type too. All

three

quantities are real with respect to 1. For their determination we have the following three additional conditions:

i) The perturbation velocity must vanish at infinity i.e.

= .0 as Iti

+o

(5.1)

This gives us as a result of the symmetry of the problem only one condition real with respect to i.

2) The perturbation cannot have a source or sink at infinity. This condition is equivalent to the requirement, that the pressure should remain finite at infinity Moreover it is the generalization of

the

closure condition to the unsteady case...Mathematically it is formu-lated by

res. S?1 = 0

as

It!

(5.2)

The same remark as under i) applies..

.3) Finally we have to ensure that the presaure on th

cavity is not only constant in space, but also constant in time. This

last condition is not expressed by the boundary condition, since the boundary

(18)

17.

condition (Li..i.6) has been obtained by partial differentiation against

We shall now formulate condition 3) mathematically.

The instationary Bernoullian law reads according to (Li..5) as 2

+ q.0 r1

-+ -'= D(T)

we have D(T) 0.

Prom -- = r follows that on tl2e real axis

LçD I d. = r1 d =

f

r dcr = 00

-t-d.

=Ir K- °dLr=Re

I

K°dt

I cr-c0 J I t-c1 (.5.3) We define =0 as o-

forT

0; cr and

are the coordinates in the t-plane. We are allowed to do tha,t, ince is determined except for a constant and since is finitea-L infinity as a result of the absence of a source there. Since st infinity r1 = 0 and p1=0,

(5.Li.)

where the path of integration in the last integial can be deformed according to Cauchy's theorem,

On the cavity the following identities are valid.

jw(T-ç)

r1 =ge

-, p1 =0.

Thus (5..3) can be written on the cavity as

jw(T-ç)

or using (5.L1) as

t-d jw(T- )

ReKf...00dt=_ge

00

This is the mathematical form of the third additional condition.

It

is easy to prove that this condition is independent of the choice of t in the above mentioned interval.

We have seen now that the 3 additional conditions are linear in the unknowns, Since the known members of the equations have harmonic time dependence, we can put

c1 =c1 e

,d1 =d e

(19)

If we

Re

Kf

For

GT-cp0)

we have anticipated this time beha;iour, remarked. c and are real with respect to

complex with respect to j.

gives us

c

with Q(o-) =

Applying (5.2) and using (5.8) we arrive at

ti

--- +

c0+a

['!a(c).f(c+a)]

hfQ)

a

'fo-(c0o-) d

Al

d

___ -

d1f

ç;:;

From (5.8) and (5.9) it can be derived that

fd

d A +

_-Q ](2

-1) 2

c+a

d-ó

c 0 0 0 0 =

P 1(°-)

(d0-oi

d l-cr(c0-r)

d0dJ d.

0 d -c 0 0 0 [rfd0 ( c0-cr) [Td0(c-a-) -jwK{cr -(d0-c0 (.2 -i) = 0 0 0 -a

10-jWK{0(d-c) log (c0-)]

(-)

(c0-)

+tfd-c)]

1 8. as already i, but in general (.7) (5,9) log (c0o)] crdo 1cr(c0-cr) -jwK[0-(d -c )log(c0-o)j (d0-o)dø-0 0 (5.11) =0 o t <

We shall now use the 3 additional conditions for the

determination of the 3 unknovm constants, c', d and. g. Application of (5.1)

let L1. = e ,

(5.6)

goes over into

t-d t-c dt = w.

ge

-K[ t-(d0--c0) log (c0-t)] 7r e

=0

(5.8)

(20)

Using (5.10) and (51iYwe find =

t(tco)f

Q -jWK[0-(d-c) log (c-o-)] o-(c-o-)(o-t) (t-c) (t-d) - t(t_co)f°

The first integral in (5.12) can be expressed in. elementary functions. We will not do that, since in view of the purpose of our research we

don't need such an expression. We can now apply condition 3) as expressed by 'ormu1a (5.7), We take first t=o in (5.7) and se formula (5.12) to substitute for Sl, The left hand member of

.7)

now replaced by a repeated integral. Since the integrand of this integral is except for the endpoint t = 0 a holomorphic function of t, the integration with respect to t can be performed along a path, which meets the interval [-a, c0] of the real axis only in the point

t = 0. We now move the endpoint of the path of integration from t=0 to a neighbouring point t

= C,

with Im e 0. Since both integrals in the repeated integral are now absolutely convergent, we

can change the order of integration. Evaluating the inner integral and letting afterwards

C -

0, which is legitimate on account of the uniform convergence

K[-2f

-[-+

-jwK[cr-(cl-c)

of the outer integral, we get

d -c

do--jwK[cr-(d0-c0)log I, Jt(t-c)dt Re urn I e-+OJ (t-c)2(o--t) 0

I.Q(

d

-C0 -a (c-o-)] (ci0-o-) log log (c -o-)] 0 rt 27 L -arcs1n (-0

Use has been made of the following identities

C 2 [[c_o-_iT ] [w

c-7+Af;J

do- + 19. (5.1 2) =

e0

log C0 (5.13)

[[c -o--'T&]

_o-log 0 0

[Wc4

at

7

< 0

(21)

and

2 . 2o- / 0- 1

= - + i. -arcsin (s- - )] ' at 0 < o- < .c

0 0 0 0

The last integral in (5.13) can be reduced as follows

fC0

-K[cr-(d -c ) log (c0-o-)] .

e ° °

[-arsn (- -1)

do- =

0

=

f[

-arcsin ( -1)] d

e_T_

Q00) log (c0-r)]

0. = -jwK(d0-c0)log C0 c -iwK[o--(d0-c0)log(c0-o-)]

WKe

+f-. J 'io'(c0-o-) 6, First order a finally as

roximation for small breadth.

S.

20.

(5.13a)

(.5.1 L)

0

The integral occurring in the last member of (5.ILi.) and the integral of the same type in (5.13) can be expressed in confluent

hyper-geometric functions0

Using (5.ILi.) we can write (5.13)

9 d -o- 9 d -o- [i c

-jwh [ 2 Q(o-) - -- do- + f Q(o-) - log

0

do-]

J tJ-O(c j 00

0-[Wc0-r-"f]

0

Formula (5.15) gives us g; c and d1 are then found from (5.10) and (5.11). The solution is now completely determined.

c0

wK[(d)1(]

---_

.[2(d0)-

] = 0.

+ g

f

e

a) We determine first the first order approximation for the steady flow. For that purpoe we put K = I and consider first a as unknown instead of K. Formula (3.2Li.) gives then by means of (3.25) and (3.26) or (3.27) the relation between a on the one hand and b and 0- on the other hand. We shall now consider a and.c as given and determine b and o- as functions of a and c. We suppose a to be small, It will appear that then for fixed c P alsob is small, i.e. as a tends to zero, also b tends tQ zero. The cavitation humber o- as a function of a and c is given by (3.25).We expand this expression into powers of

(22)

La

-

1

-

+

ad-c

]2

Lj.ac(c+a)(i-y2)

(6'3)

I C d c+a 1+y

Ec(iy)2

ay2

where

Ja(c,)-

(ca

is the new variable of integration.

sfà(c-o-)+ 'i-cr(c+a)

According to (3.26) and (3.27) we have in a first order approximation

and

d-

C

=0

Hence in a second order approximation the expression in (6.3) becomes

I

equal to La

f

y2

ly

dy

=

(7rL)

(6.5)

.(1+y)

In the

same

order of approximation we find for b

b =

L)

(6.6)

Expanding expression (3.17) for

w into ascending powers of,we get

w=i

±...

(6.7) and using (6.2) a [tJa(c...iy)....

w=1

-0- c+a c+a)] 0- r t-c

T

o'-d

[Jd(c-)-

tf.o(d_c)] 0--c

+[:L.]

t-c

In a first order approximation it is also true

thatdz=dt

Hence in that approximation w is given by

w=1

+

...

(6.8)

21

1 +o=

+Li:F+...

(6i)

Hence we have in a first order approximation

(62)

We now expand the integral in

(3.2Li.) into

powers of , using (3.26) of (3.27). For that purpose we introduce first a new

variable of integration and

take

the real part of the integral.

(23)

A I (5.10) yields c' F

jh

(i-+2)

F

Co

-functions C 0 0

f

e&r

J0 'o-(c-.c- -C

= jw

e -r

_/°

t t-c0 tc t I -b-c0

t-c0

j

Co U 0 CO - jw 2 J(w -=) I

C -0

0 o--t ±a

-_j

0 C0

t(t-c)(t-c)

jW0-,) .pii dO

Relation (5.15) between h and g gives in the same approximation

2(c

0)

--2jWh(7+2)

'T

c.. + g

f

-2-__W

y dy (i )2 e 1) C 0 YCC

-;p)----'

C e 2 [JJct.)+jj

(w.f)J

2 L) 2 22.

The relation between b,, c and 0 reads

= 2b

(6.11)

Expansion (6.iO) is uniformly valid in the interIor of the physical

plane.

j3) First order approximation for the unsteady motion.

We first expand into ascending powers of

- . Introducing

again y as a new variable of integration by means of (6.3a), we find. from (5.12) in a first ordei approximation

(6.-i 2)

= 0

(6.-13)

(6.iL.)

The integrals in (6.ii) and (6.-12) caiibe expressed in cylindrical

(24)

23.

Hence (6.13) can be written as

-2jwh C0 + ge 2 [J0(w )(c0 -

+ j c0

1 (w )]=o

(6.17)

and

(6.lLi.) as

= 2h

c - gc e

[J(w

)+j

(W)(618)

Combination of

(6.17)

and (6.i8) gives

'C

= g e 2 J0(w

(6.19)

where use has been made of (6,6) in order to eliminate a.

For d1 we find the same expression as for

In the foregoing we have supposed that < 1, but also that Wh

-

; In other words

-

cannot be taken to small, since

Co

otherwise we should have taken into account higher order approximations for the consideration of the unsteady effects i.e. we should have

calculated the coefficients of higher powers of 'T in the expansions,

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II..Linearjzed theory of the unsteady cavity flow.

u1ary

In the linearisd theory the flat plate is replaced by a

singularity for the complex velocity. It will appoar, that for the steady flow the expression for the comolex veloc:.ty is identical with the first order term in (6.iO). It i pcssile then by means of the calculations in

6a.)

to express the strength of-e

singularity in half the breadth b of the flat Dlate This will be done in 8).

Assuming that the unsteady effects can he considered as small perturbations of the linearized steady flow (second Unearizatioii),

a

we can proceed in a maniier analogous to that fcr the steady óase It

wl± again

appear that the unsteady part of the flow can be idenifi;:. with the first order term of fL1, s derived in 6 ). In this cose too the unsteady part of the strength or the ringurity can be brought into connection with the amplitude h and the circular frequency w of the harmonic oscillation of the flat plate. The calculations can be found in 9) and iO).

Finally we show that the application of the acceleration poten-tial methodmon the unsteady cavity flow gives the same results

as the foregoing treatment by means of the complex 7eloctv.

8. Linearized theor Of the steady f1ow

We suppose that the flow pattern as a result of the presence of the flat plate can be considered as a small erthrbtion of the original uniform flow field0 This will generlly be the case if the breadth 2b of the plate is small with respect to the cavity length0 The plate can then be replaced by a singularity. The rear end of the cavity will show a similar singularity. Within the framework of linearized

(26)

theory the occurrence of these singularities can be inferred from the presence of a stagnation point in the neighbourhood. We shall not go into further details but refer to [18].

We choose the Cartesian coordinate system in such a way that the cavity extends between the points (o,o) and (.,o). The velocity at infinity has the direction of the positive x-axis The units of length and time are chosen such, that the constant velocity

along the cavity is equal to I We put = (i +u,v). Since 1-U < I , we have u < I and v < I We will neglect second and higher powers of

u and v. (linearization)0 w = u-iv is a holomorphic function of

z=x+iy.

The linearized Bernoullian law reads

PPc=PU

(8.1)

Hence we derive u = - (8.2"

00 2

On the cavity we have u = 0, (8.3)

Since the maximum width of the cvit.y is o± the same order of magni-tude as the perturbation velocities, we can apply condition

(83)

on the x-axis between (0,0) and. (e,o) instead of on the cavity. The holomorphic function w has now to satisfy the following mixed boundary value problem (see fig. Li.).

= 0

25.

( oJ

(t0

fig. L.

Determine v(z), .olomorphic in the upper half of the z-plane, such that it assumes the following boundary values on the real axis:

-00<

x< 0

v=O

orlmw=0

O<x<e

u=O

orRew=0

(8Lj)

(27)

26,

By means of the Schwarzian reflection principle this boundary value problem for w(z) can be transformed into a Riemam-i--Hilbert problem with the following linear relations along the real axis.

0< x<

< x< 0

< x <

The general solution with intëgrable singularities at z=0 and z=e

is

(8.6)

The cut for both square roots is made from 0 to £; the.branches

are

chosen such that

asz-c

(8.7)

We assume that the strength of the singularity at z=0, determined by the flat plate, is given. We have there

wA1I

(8.8)

Hence the strength of the singularity = AJ7

This gives us one relation between A and For the determination of the tmknowns A, B and e we stll need two relations, These

are

furnished by the following additional conditions.

-i ) w = - at z= according to (8.2)

(8.9)

2)

res. w= 0 at z =c

(8io)

This condition is equivalent to the closure of the cavity (see [18]). From (8.9) we deduce

and from

(8.10)

A - B= 0

(8.12)

These equations result n

+ w - w = 0 +

w +w =0

+

w -w =0

(8.5)

(28)

Thus w have for w the formula

This expression agrees with the first order term in

(6.i 0

identify c and From (6.9) follows that

27.

(8.iL.)

if we

Afe 2b (8.1 5)

This is the connection between the strength of the singularity at

z = d

and the breadth 2b of the plate. We have shown now that

linearized theory can be understood as a first order approximation of reentrant-jet theory. The same statement holds as to the

Riabouchinsky-flow. (see [13]).

,9..The unstead flow method of the corn lex velocit

The coordinate system and the units of length and time are chosen as under 8). As a result of the harmonic oscillation of the flat plate (amplitude h, circular frequency w), the strength of the singulaiity at z = 0 will vary harmonicly with time. We assume that the amplitude of the time dependent part is small with respect to the time independent part, but large with respect to second and higher powers of the last one. This assumption enables us to treat the

unsteady effects as linear perturbations of the linearized steady flow (second linearization). Hence all quantities can be split up addi-tively in their steady and unsteady parts. We put accordingly

A u = u0 + u1 with u1 = U1 e3 A jwt

v=v+v1

v1=v1 e

A = A0 + A1 A1 = A7 jWt (9.1)

B = B0

+

B1 = B

jwt e = + = e

et

A jwt e

Remark: the time variable is denoted as usually by t instead of by T, as we did above As a result of the unsteady motion the boundary

(29)

28.

condition on the cavity will changes For its derivation we start with the linearized Euler equations of motion f or an ideal fluid:

+_u

ôt ôx

..x

-at

ôx

_1E

p ox

On the cavity we have p PC

According to (9.2) we get there Ou Ou + = Substituting (9.1 ) we arrive at ,' 0u1

j

w 1 + = 0

The general solution of this differ-ntial equation is ul

thus =

0.

the following mixed boundary value problem. in the upper half of the z-plane and

00 <

< 0

O<x<e

<x<0o

The solution is w

= -

e jwt

fz

(z )

I

1'dx

(9,2)

real with respect to 1, but possibly

+

w -w =0

+

-

A. w + w = 2geU w - w = 0

x(ex)(xz)

(9.7)

+B

[.

(9

8)

assuming the following boundary values on the real axis

00<

x<O

v=O

orlmw0

0 < x. < e

u=gei°:t)

or Re w =

(9.6)

e

v= 0

or Imw=O

By means of the reflection principle of Schwarz this

boundary. value

problem can be transfol'med into a Riemami-IIjThert problem with the following linear relations along the real axis:

A

where g is an arbitrary constant, complex with respect to je

For w = w0 + w1 we now have Determine w(z), holomorphic

(30)

29.

We now divide this expression for w into its steady part w0 and its unsteady part w1. We find

w0=A0J-2+B/

z-e 0

(9.9)

w=_eWtiz(z_e )r

-A

+B _1

I

ooJ

ix(ex)(xz)

o 2 0 2

z-e0 z-e0

I

z-+A'

2

I z

For the relation between A0 and the breadth 2b of the flat plate, the determination of B0 and the connection between and the cavitation number 0 we refer to 8).

Assuming that in (9i0) the strength of the singularity at z=0 is given, we still need 3 other conditions for the determination of

/\ A

the Li. unknowns, g, e

-and B1 These conditions read as follows

i) as under 8) we must have

0

w=-

&t=oo

or WI = 0

This condition means that the Derturbatjon velocities vanish at infinity,

res. w = 0

at z

or according to 8)

res. w1 0 at

z =

00 (9.12)

This condition means that there is no source or sink at infinity. We know already that there is no vortex at infinity as a result of the

smnyietry of the problem. As a result of this condition the pressure remains finite at infinity in the unstesdy case toO..

Boundary condition (.9.5) on the cavity has been obtained by

partial differentiation against x Heice it is possible that a time dependent additive function with a constant as a special case has been differentiated away. In any case it is necessary to connect the

-'-au Z oo

pJ (9.10)

(31)

30.

pressure on the cavity with the pressure at infinity. This is the third condition0 We formulate it now mathematically.

According to (9.2) we have

= -

p

op1 ouI

= -

p

(j w

UI

The unsteady motion is not allowed to disturb the connection between the pressure at infinity and. the pressure on the cavity, i.e. we have to require that

P1,

-P1,=

0 (9.11-i.) or by virtue of (9.13), that +L) 0

f(

w. + )dx = 0 (9.15) 00 Integrating we obtain +0

j

wf

u1dx

= -

i'

(+0,0) -

(9.16)

or

/

i dx = (9.17) 00

Application of (9.11) and (9.12) gives respectively

A D and

+Aj

+

=0

dx +

©e

x dx] :

Wx(e-x)

A I' A A

Since A0 = B0 - , it follows that

e0=O

(9.1 8)

(9.1 9)

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By means of (9,10) and (9.20) we find

A

A

J(e

I

-x(e0-x) / . 8

We can now apply (9.17)

f(e0-)def

-

mf

(-x)(-x)

(9.22)

The inversion of the order of integration can be justified in the same way as in 5). We now use the following ideitities

0 0

I

[arcsin0+))f

dx 2

J

'-x(e0-x)(-x)

i(e0)

2

(-x)(e0-x)

£0

(9.23)

Integrating partially we get from (9.22)

e

.,\ o-W

_/e3Xd

0J

J.x(e-x)

31.. (9.21)

By means of (6.i 5) the integral in this formula can be expressed in a Besse function,

This yields

3W A JW

Lj.

=ge

Remark: it is possible to write the solution (9.8) of the boundary value problem (9.6) at once in the following form

w=et

i_J

z(z-e)

. x-z

By putting A=A0 and B=B0, the conditions (9.11) and (9.12) are automatically satisfied. Finally it. is possible to get from (9.22)

to (9.2L1.) withdut evaluating the first integral in (9.23). Intht case one uses the fact, that the integral can be considered as the

solution of a certain boundary value problem.

(9.26)

A

o-eJW

Lj. (9.2L1.)

(33)

?r(e

(i 0.2) We have already identified, in 8) the following quantities viz. t and

z;

c0

and

e0.

If we now can identify also g and g

, the two

expres-sions (10.1) and (10.2) become the same. Since however,

we have

assumed that the strength of the singularity for WI at z = 0 is given and is equal to the strength of the cinularity for at t=0, we infer from both formulas that indeed, g and g must be

identified. This gives the proof of the statement, that for the unsteady case too linearized cavity theory is a first order approximation of reentrant-jet theory.

From (6.19) and (925) We see that also C1 and must be identified,

Finally we derive an expression for the strength of the

singula-rity at z = 0 in terms of h and W. This expression can most easily be

derived from (6.12). According to that formula has the following behaviour near t = 0

- jwh (-t (10.3)

0'

U

32.

-1 0. Linearized unstead cavjt flow as a first order_approximation.

1'

We shall derive expressions for and w1 , which can be compared in

order to show that WI is a first order approximation to S.

For that purpose we express SL1 in terms of g, and WI in terms of g.

From (6.12) and (6.13) we find for

9'o_.

/'(c-r)do - I I e

_______ +

I t(t-c )

00

I

C -joxJ-+

Q)fl'

. F

t(tc

)P

"Icr(c,,cr)

Combination of (9.10), (9.20) and (9.2L1) gives us

A e A

_j

g

I P e ' + I r e LI D I

-rz(z_e

') 2) 7r 1 / (i 0.1 )

(34)

function by means of p-pc

-

-Hence (11 .1 ) can be written as

+ =.

a-b ôL. ox

(11

.3)

at ax Oy

is called the acceleration potential. As a result of the incom-pressfbility and irrotationality cp is a harmonic function. We can

now introduce its conjugate harmonic function according to ax - ay

8y Ox

Now F(z) = + is a holomorphic function of z=x+iy,

for which we have ]? ow aw az - at + (11 .2) (11 .5)

F(z) is the complx acceleration potential. We may formulate the

linearized cavity problem of 9) now as the following mixed boundary value problem for F(z).

3.

where (-t is positive for real t < 0. Application of (6.6) gives

us

'.-.

_)h2J

-t)

(i o.Li.)

11 The iinstead. flow method of the com.lex. acceleration otential.

The coordinate system and. the units of length and time are chosen as under 9). We start from the linearized Euler equations

ôt ôx ,ô;x

(11 .1)

ôt ôx

pay

In these equations we have linearized with respect to =i , the velocity on the cavity in the steady case. We introduce the

(35)

where a and b are quantities,

only dependent on t and real with

respect to 1. Remark: this

a is different from the a used in

part I.

According to the second

linearization we can write

F = F

+ F1

with F1

= F1

et

A

jwt

a=a+a1

a1 =a1 e

(11.8)

b = b0 + b1

b1

= b'

e0)t

We identify F0 and

w0. This is in accordance with the

foregoing

equations. Thus

= -

H'

.

+PJ.j]

(11.9)

For F1 we now get the expression

2. F

= -a

- -=.---

+ b

+ 1 °

2tIz(ze)

02

Jz(z-e0)

z-+ a1

+ b

where

=e

-

(11.16)

In this expression for F1

3 unknowns viz, 7, a1

and

still occur,

For their determination

we have the following 3 conditions

i)

F1

= 0

at z =

(11 .11)

i.e. the perturbation pressure vanishes at infinity.

2) the velocity must be a single-valued functions

As a matter of

course this requiremeritis fulfilled

for the

horizontal component of the

perturbation velocity u1 by virtue of

the symmetry of the problem:

there is no vortex sheet in

the wake.

F(z) = a 'J

z

+ b

z-e

(11

.7)

Zi

Determine F(z), holomorphic in the

upper half of the zpine

and assuming on the real axis the

fpllowing boundary values

oo <x<0

orlmp=0

0

< x< e

cp =0

orReP=0

(ii .6)

e

< x<oo

=0

orlmF=O

(36)

C

71

-'.5.

So condition 2) expresses the fact, that there is no line of discontinuity for the vertical.component of the perturbation

velocity v1

3)

the relation connecting the unsteady part of the singularity

for P(z) at z = 0 and the given unsteady part of the singularity for w(z) there.

As to

3)

we will prose that the unsteady parts of the

singularities for F(z) and w(z) at z = 0 are the same.

According to (11 .5) ve have

A +

o

-

'I

from which follows that Z

-

e I - J oc 00 = (z)

-f

e

F(C)dC

(11.13)

Use has been made of (ii .11 )

-Since the integral in the last member of (11.13) is finite at z=0, A

WI and F1 have the same behaviour at z=0. q.e0d.

Equating the strngths of the two singularities we obtain

A a2. A

a1 + = A1J + A0

(11 .iL)

This is the mathematical expression of condition

3).

Application of condition i) gives us

(-ii

.is)

We shall now formulate condition 2) mathematically.

Using

(11.13)

we can assert that the single-valuedness of w

is

equivalent with

e F1(c)dC - Q

(ii.i6)

where C is a contour surrounding the cut from 0 to e in the z-plane. For (z) is already a single-valued fction.

(37)

Since a = A0 = - , we can write

F(Z) =a

-+i_

A A o2. a -

J

...j..

-.8

Z

where use has been made of (11 .1 5).

Coiidjtjon (11 .1 6) now reads as

A j jwz oX jw a1 e

0 j

dz +

- fe

(-)

'+ Cf

z-eo

+ j JI

kfz(zC)

z Lj. dz z-.e

e0x

x dz = 0 A or jWCp

A______

a1 0

r

dx ± J eJWX X

e-x

-

Wx(-x)

Replacing in the integrals x by e0-x as variable Co

"

f

dx

°i

jW

a1e0 +

J

- tfx(C0x)

or using (6.15) and (6.i6)

A o-7

jw

(w2)

+-_j

[

From (9.20) and (9.2L) we can derive

A e e A1

J(w

2) +

[J(w

Q)

+ j

j1 (w

2)]

dx dx = 0 C 0 2

=0

0

Combination

of (11.iL), (11.21)

and (11.22)

yields

A A A

a1 =A1 andA1

=e1

This means that both methods, viz, the method of the acceleration potential and the method of the complex

lead to. the same results. ThIs is

important, because (11 .19) of intwgratjon we get (11.20) (11 022) (11.23) complex velocity, the method of the complex acceleration potential is preferable in

more complicated problems.

iTrg0

We calculate the drag by applring the

mornentui theorem on the interior

of the contour indicated in fig, 5.

.36.

(38)

C

fig.

5.

.c represents the linearized version of the flat plate. The whole contour is denoted by C. We use the method of the complex velocity.

It is clear by virtue of the symmetry with respect to the x-axis that the component of the force perpendicular to the main stream

vanishes. Sinee the horizontal sections of C give no contribution to the x-component of the force and the contribution of the vertical end sections can be made arbitrarily small by making the contour thinner, the momentum theorem can be written as

(p-p)d.y = (1+u)v dx

(i 2.1 )

C

where p is the pressure exerted by the fluid on the flat plate and the direction of C and C is chosen positive i.e. such that the interior of C lies on the left.

Since the drag D = P (p-p)dy, we have

at z=O

(i 2.2)

w_i[ljwhaejwt]z_

atz=

(i 2.3)

C

370

D=p

(1+u)vc=-Imp

wdz-Imp

ImP /Tfrdz=_rpRe

res. w21

z=O

By virtue of (8.15)

wo - I (I and by virtue of (IO.)-i)

WI

-±jWh---i

v+L 2 A 7C-F2 2b at z=O Hence we have

(39)

Substituting in (12.2) we find

D = p 2b Yr [1+2jwh

eJt

]

and

CD = [i+2jwh

e]

(125)

--pU 2b

In (12.5) we have neglected the factOr (i-f) in accordance with the order of approximation we have tied throughout. In [13] we have proved that for the steady case the insertion of the factor (1

)

- already known as the (i ) rule - gives the correct next order of

approximation. 13. Conclusions.

In the foregoing sections we have shown that linearized cavity theory can be formulated in suh a way that it becomes a first order approximation to reent±ant-jet theory. For the proof we have chosen the simple exomplC of a flat plate normal to the main stream direction since in that case the calculations are as simple as possible. This choice does .ot restrict the validity of our results. For it may be safely assumed that the behaviour at the end of the cavity, which is the important point in the steady as well as in the unsteady case, will not be influenced by the shape of the body in front. After

linearization the flat platebocmeasingalarjty, as one would expect. We have assthned that the unsteady motion is small with respect o the steady part of the .distubance field caued by the body and the cavity. For the non-linear theory i.e. the reentrant-jet theory, this assumption was necessary to attack the problem in a reasonable way, for the linearized theory it enabled us to produce explicit results.. Moreover we may expect that the condition of small unsteady

(40)

I

We have shown that for the linearized

cavity flow the method

of the complex acceleration potential leads to the same result as

the method of the complex velocity,

provided appropriate additional

conditions are applied. In the

case of the second method these

conditions can be derived easily

as a result of the linearization

by comparing the linearized flow

with the reentrant-jet flow. A

condition, which seems to be

new, is the one relating the pressure

at infinity and the pressure on the cavity. From our analysis it is

clear that in the case of the former

method, i.e. the method of the

complex acceleration potential,

it must berequ±red explicitly that

the normal component of the

perturbation velocity should be continuous

in the wake. Since this condition

has been overlooked hitherto,

we

lay stress upon it here,

In addition the above linearization of

the flat plate into a

singularity, which may be considered

as a slight generalization of

linearized theory as used up till

now, enables us to treat more

com-plicated problems in a relatively simple

way, E.g. the effects of

gravity on a cavity has been dealt with recently in that way.

In following reports

we will treat the unsteady cavity flo* past

a lifting profile, f or the partially

as well as for the fully

cavitated case, by the methods outlined

in this report.

Acknowledgement.

The author is indebted to Prof. dr. R.

Timnmnan for interesting

discussions and for reading and criticizing

the manuscript.

(41)

L.Os

References.

[i] Th. von Kármàn, Accelerated flbw of an incompressible fluid with

wake formation, Annali d.i Mat0

pura ed appi. IV, 2.(19L..9),

2Li7 - 2L.9,

D. Gilbarg, Unsteady flows with fre boundaries,

ZOA.M,P,,

(i952),

3L1 Li.2,

L.C, Woods, Unsteady cavitating flow

past curved obstacles;

A.R.C. Techn0 Report C.P. No. 1L1.9

(i95Li)0

[Lj.]

L.C. Woods, Unsteady plane flow

past curved obstacles with

infinite wakes, Proc0 Roy. Soc. London,

A

(i 955), 1 52 - 1 80.

T.Y. Wu, Unsteady super cavitating

flows, Second Symposium on

Naval Hydrodynamics, Washington D.C.,

1958.

C,M. Ablow and W.D. Hayes, Perturbation

of free surface flows,

Techn. Report, Graduate Division f

or Appl.Math.,Brown

University, i 951

[.7] J.L. Fox and G.W. Morgan, On the stability of some flows of an

ideal fluid with free surfaces,

Quart. of Appl. Math. 11

(195L.), Li.39-L,56.

M.P. Tulin, Steady two-dimensional

cavity flows about slender

bodies, David W..Taylor Model Basin Report 83L, Washington D.C.,

1953.

B,R, Parkin, Fully cavitating

hydrofoils in nonsteady motion,

California Institute of Techn. Report

no. 85-2,Pasadena, 1 957.

T.Y. Wu, A linearized theory for

nonsteady cavity flows,

California Inst. of Techn. Report

no. 85-6, Pasadena, 1957.

[11 3

R. Tiniman, A general linearized

theory for cavitating hydrofthjls

in nonsteady flow, Second Symposium

on Naval Hydrodyn.,

Washington D.C.)i 958..

J.A, Geurat, A linearized theory

for the unsteady motion of

a

partially cavitated profile (in Dutch),

inst. voor Toegep. Wisk., Techn.

Hogeschool te Deift,

Rapport TW I

,

1958.

.

J.A. Geurst, Der Zusamenhang zwischen den linearen und

nicht-linearen Theorien derStrömungen mit

Kavitation, GAIVIM-Tagung

Hannover, 1 959.

[iLi-] LI. Gurevich, The impact on a lemma with discontinuous

(42)

a

U

41% [15] G. Birkhoff and E.H. Zarantonello, Jets, wakes and cavities,

New York 1 957.

P. Eisenberg, On the mechanism and prevention of

cavitation, David W. Taylor Model Basin Report 71 2,

1 950.

N.10 Muskhelishvjii, Singular integral

equations, Groningen, 1 95.3.

1.A. Geurst, Linearized theory for partially cavitated hydrofoils, International Shipbuilding Progress., to be published.

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