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UNIVERSITY OF MINNESOTA
,~' 5"/31/6 "2-
Permanent File Copy St. Anthony Falls Hydraulic Laboratory
ST. ANTHONY FALLS HYDRAULIC LABORATORY LORENZ G. STRAUB, Director
Technical Paper No. 34, Series B
Unsteady, Symmetrical, Supercavitating Flows Past a Thin Wedge in a Jet
by
C. S. SONG
Prepared for OFFICE OF NAVAL RESEARCH
DEilpartrnent of the Navy Wq:shington, D. C.
Contract Nonr 710(24), Task NR 062-052.
IgIltl,(::~ly H!62 Minneapolis, MinnEilsQtq
UNIVERSITY OF MINNESOTA
ST. ANTHONY FALLS HYDRAULIC LABORATORY LORENZ G. STRAUB, Director
Technical Paper No. 34, Series B
Unsteady, Symmetrical, Supercavitating Flows Past a Thin Wedge in a Jet
by
C. S. SONG
Prepared for OFFICE OF NAVAL RESEARCH
Department of the Navy Washington, D. C.
Contract Nonr 710(24), Task NR 062-052
January 1962 Minneapolis, Minnesota
Reproduction in whole or in part is permitted
for any purpose of the United states Government
A B ST R ACT
Problems of symmetrica~ two-dimensional supercavitating flow about
a thin wedge in a finite fluid with two free surfaces are solved Qy means of
a linearized method utilizing the complex acceleration potential. Taking ad
vantage of the symmetry, the otherwise doubly conl'1ected region is divided in
to two identical simply connected regions. Conformal mapping technique is
then applied to the upper half of the flow region. An oscillatory-type motion
as well as general types of unsteady motions are considered.
The soluti.on contains no singularity and, as a result, pressure is
ever,rwhere finite. The mathematical condition required for the existence of
a singularity-free solution leads to an equation which gives the relationship
between the cavity length and the cavitation number. The theoretical results
are in good agreement with experImental data for the steady-flow case, but
data for the unsteady case are not yet available.
iii
-----_._----
Abstract • • • • • • • List of Illustrations. Lis~of Symbols. • • •
• • • • • • • • • • • • • • • • • • •
• • • • • • • • • • • • • • • • · . . . . . . . . . . . . . . . . • • • • • • • • • • • • • • • • •
Page
iii v
vi
I.
II.
III.
IV.
V.
INTRODUCTION • • • • • • • • • • • • • • • • • • • • • • • •
THE ACCELERATION POTENTIAL AND BOUNDARY CONDITIONS • • • • • • •
THE CONFORMAL TRANSFO~~TIONS. • • • • • • • • • • • • • • • • •
METHOD OF SOLUTION . • • • • • • • • • • • • • • • • • • • • • • Ao Infinite-Cavity Case. • · • • · • • • • • • • • • • • • B. Infinite-Fluid Case · • • • • • • • • • • • • • • • • • C. General Case. • • • • • • • • • • • • • • • • • • • • •
CONCLUSIONS. • • • • • • • • • • • • • • • • • • • • • • • • • •
1
2
7
8 11 15 20
23
List of References • • • • • • • • • • • • • • • • • • • • • • • • •• 25 Figures 1 through 12 • • • • • • • • • • • • • • • • • • • • • • • •• 29 Appendix A - Evaluation of the Function ~(t). • • • • • • • • • • •• 39
A. Oscillatory Motion. • • • • • • • • • • • • • • • • •• 39 B. General Motion with Infinite Cavity • • • • • • • • •• L~o
Appendix B - Evaluation of Integrals • • • • • • • • • • • • • • • •• 45 A. Evaluation of 10 • • • • • • • • • • • • • • • • • •• L5 B. Evaluation of LO and Ll " • " " •• " • • • •• 46
iv
;
L T
L
L
Figure
1
2
3
5
6
7
8
9
LIS T 0 F ILL U S T RAT ION S
Flow Configuration and Linearized Boundary Conditions. . . • •
The Conformal Transformations ••••• • • • • • • • • • • • •
Reduced Cavity Length as a Function of Actual Cavity Length
Page
29
30
and Jet Width. • • • • • • • • • • • • • • • • • • • • • • •• 31
The Effect of Jet Width on the Drag Coefficient for the Infinite-Cavity Case •••••••••••••••••• • • •
The Effect of Acceleration on the Cavity Length (0-= 0.1) • •
The Wash-Off Condition •• • • • • • • • • • • • • • • • • • •
The Effect of Cavity Length on the Drag Coefficient for Infinite-Fluid Case. • • • • • • • • • • • • • • • • •• • • •
The Effect of Jet Width and Cavity Length on the Steady Part of the Drag Coefficient ••••••••••••••••••••
The Effect of Jet Width and Cavity Length on the Added Mass' Part of the Drag Coefficient • • • • • • • • • • • • • • • • •
31
32
32
33
34
34
10 The Effect of Jet \l,Tidth and Cavity Length on the Pressure
11
12
Function, L2• • • • • • • • • • • • • • • • • • • • • • • •• 35
Steady Cavity Length as a Function of Cavitation Number. • • •
Steady Drag Coefficient as a Function of Cavitation Number • •
v
------- -~-~~-----
35
36
LIST OF SYMBOLS
A - Displacement of a body.
A -.. A
A - Amplitude of oscillation. o -t a Acceleration.
b - Jet width.
CD - Total drag coefficient.
Coo - Drag coefficient due to velocity.
CDl - Drag coefficient due to acceleration.
CD2 Drag coefficient due to finite cavity.
CDS Steaqy part of drag coefficient.
E(~, k) - Incomplete elliptic integral of second kind.
F(~, k) Incomplete elliptic integral of first kind.
F(z) , Fer) Complex acceleration potential. -t
F . Force.
f l , f2' Fl , F2, G - Functions.
f - Reduced frequency.
Hcr) Homogeneous solution.
h - Vertical coordinate of wedge surface or cavity wall.
I O' I l , LO' L l , etc. Integrals.
i, j Unit of imaginary numbers.
K(kl ) Complete elliptic integral of first kind.
k, kl - Modulus.
t - Cavity length •
.e - Reduced cavity length.
vi
M .. Mass.
o Order of magnitude.
P - Ambient pressure.
p Pressure.
Pc Cavity pressure. -q - Velocity
qc Speed on cavity wall.
Re Real part of.
S Cavity area.
t Time.
U - Ambient speed.
tl - Horizontal component of perturbation velocity or incomplete elliptic integral of first kind.
v - Vertical component of perturbation velocity.
W - Complex velocity.
x, y - Space variables.
x o Reduced jet width 2n 1
[(exp - - 1)- ].
>- r' z, ~, Complex variables. b
~ Half vertex angle of a wedge.
V Gradient operator.
Ao(O, kl ) Heuman's lambda function.
~ - Real part of complex acceleration.
v Negative of the imaginary part of complex acceleration.
~, 11 Real and imaginary part of r. 2
n( a. , k) - Complete elliptic integral of third kind.
2 n(~, a. , k) Incomplete elliptic integral of third kind.
p Mass denSity.
(T - Cavitation number.
vii
T - A variable of integration.
p - Acceleration potential. ,
'lI( t), 'lI (t) - Function of time.
~ - Conjugate harmonic function of acceleration potential.
~l ~ on wedge surface.
w - Angular speed.
viii
U N S TEA D Y, S Y M MET RIC A L -------- -----------~Q~!~2!!!~!~!~Q !~2~~ ~!~~
A THIN WEDGE IN A JET
J. INTRODUCTJ ON
Recentdevelopments in high-speed sea crafthave stimulated research
workon unsteady super cavitating flows. Unfortunately, unsteady supercavitat
ing problems are considerably more difficult than their steady counterparts,
and the development of an exact theory on general unsteady flows seems very
remote. The only exact theory known to the writer is that due to Von Karman
on a specialtype of unsteady supercavitating flow [lJ* where the time varia
ble in the velocity potential may be separated from the space variables and
the rear stagnation point occurs on the free surface. More recently, this
special theory was refined and generalized by Yih [2]. Additional difficul
ties arise when a finite fluid instead of infinite fluid is considered. For
this reason, attention has been directed mainly to solving problems in infin
ite fluid by means of linearized m~thods. So much progress has been made by
many investigators in tLis field that it is felt timely to take up a problem
of unsteady super cavitating flow in a finite fluid.
Solutions of st.eady supercavitatingflows with zero cavitation num
ber under the influence of one or two free surfaces can be fOlmd elsewhere.
For example, the problem of an inclined flat plate in a jet of finite width
was solved by Silberman (J] and the problem of an inclined hydrofoil of finite
aspect ratio undera free surface was treated by Johnson [4]. These problems
were solved by the usual conformal mapping technique. When the cavitation
number is not equal to zero, it is more convenient to use the method of dis
tributing sources and vortices. An excellent example was shown by Cohen and
Tu [5J, who considered a steady supercavitating flow past a thin wedge in a
jet.
Since the known quantity on a free surface is the pressure and not ,
the velocity, unsteady supercavitating problems can be solved more advanta-
geously by considering the acceleration potential rather than the velocity
potential. It has been shown that if the problem can be linearized by using
* Numbers in brackets refer to the List of References on p. 25.
II, ill
2
perturbation velocities, the acceleration potential satisfies the Laplace equa
tionand, hence, conformal mapping technique can be applied. This is the meth
od most frequently used and is also the method to be used in this paper. A
supercavitating thin wedge at zero cavitation number symmetrically placed in
a jet and performing symmetrical motions is considered first. Then, the sim
ilar problem wi tb finite cavity but in infini te fluid is treated. Finally,
the general case of fin:i.te cavity in finite fluid is considered.
This research has been supportedby the Office of Naval Research of
the U. S. Departmentof the Navy under Contract Nonr 710 (24), Task NR 062-052.
The author is indebted to Professor Edward Silberman, who has critically re
v'iewed the present work. Mr •. Frank Tsai is credited with carrying out some
61'the integrations and Mr. Paul Edstrom has carried out most of the numeri
cal computations. The manuscript was preparedfor printing by Marveen Minish
and Marjorie Olson under the general supervision of Mr. Loyal Johnson.
II. THE ACCELERATION POTENTIAL AND BOUNDARY CONDITIONS
Newton's equation of motion upon which fluid mechanics stands is
--t --t
F = M a (1)
...... --t
where F, M, and a are force, mass, and acceleration, respectively. In
particular, when the mass distribution is uniform and the system is conserva
tive, the force per unit mass is derivable from a scalar potential function,
and
CIa)
Itis thus clear that an acceleration potential function exists when
flow is incompressible and frictionless. For a gravitation-free field, the
Euler equation of.motion is
...... aq 1 f! = -- + rq . V )q = - - Vp (lb)
at p
where q is the flow velocity, p is the pressure, p is the density of
the liquid, and t is the time.
3
For a steady, irrotational motion, Eq. (lb) may be integrated to
yield the Bernoulli equation
1 2 p +-p q
2
1 ::: p + _p U2
2
where P and U are the pressure and the speed at infinity, respectively_
Furthermore, for flow containing a cavity, it is known that the pressure in
side a natural cavity is constant, for example p, except within a small c
region nearthe end of the cavity. The speedon the cavitybOlmdary, qc' is
q =U~ c (2 )
where (f is the cavitation number defined as
1 (f = (p - p )/(-p if)
c 2
For steady flow problems, it is customary to use rather than U as the
reference speed since the flow near the body is of interest. For general un
steady flows, however, the speed on the cavity boundary is not a constant,
but is a function of time and space. Nevertheless, it is still possible to
use the steady flow value, qc' of Eqs. (2) and (3) as the reference speed.
With this understanding, the velocity of flow q(x, y, t) may be written as
q(x, y, t) = (1 + u, v)
and the Euler equation of motion may be written as
-aq
at
where
P - P
2 P qc
(4)
(5)
(6)
" ,I , ji,l ,'I, I
I,
',1
I" \
II I
I , ,
:i,1 "I , I II, ,', 1:[ 1,1
Iii
ii'
'The addition of P in (6) was possible because P is a constant. This is done merely for convenience.
It is further assumed that the body plus cavity is thin and the motion is such that both u and v are much smaller than unit yin most of the flow region. Then Eq. (5) may be linearized to
¢ -1 = u + u x qc t x' " -1 jU =q vt+v y c x (7)
Hence, it follows from the continuity equation V'. q = 0 that
(8)
Itis thus shown that the linearized acceleration potentialis a harmonic function. This implies the existence of a conjugate harmonic function if; (x, y, t) such that
wi th aj'q 2 = (J.L, v). Therefore, the complex' acceleration potential and the c complex conjugate acceleration defined as
F(z, t) = ¢(x, y, t) + i if;(x, y, t)
aF(z, t) q -2 a(z, t) = c J.L(x, y, t) - iv(x, y, t) = ----
az
are analytic functions of z = x + i y.
Also, ~. (7) may be written as
aF 1 a a = (-- -- + --) W(z, t)
az qc at az
with If denoting the complex conjugate velocity
W(z, t) = u(x, y, t) - iv(x, y, t)
(10)
(11)
It is readily seen that for the steady flow case, F(z) is identical with W(z) up to a constant of integra.tion which may be set equal to zero.
The perturbation problem of general, lIDsteady, supercavitating flow
is now reduced to the problem of finding the analytic flIDction F(z, t) reg
ular everywhere in the flow field satisfying given boundary conditions. Of
eourse,.it is assumed that there exists a basic steady flow of characteristic
. speed q and that the perturbation speeds defined by Eq. (4) are small com-e
pared to unity in most of the' flow region. Here, the lIDsteady motion is as-
sumed to be due to a perturbation velocity, dA/dt, of the body along the
direction of its basic motion. The boundary conditions are listed below.
(Also see Fig. 1.)
(1) On the free surface, p = P, hence from Eq. (6)
(2 )
~ = 0
On the cavity boundary, p = p c'
(3), and (6)
hen ce from Eqs. (2) ,
(f
~=----2 (1 + (f )
(3) ·When a wedge performs a general motion along the x"':dire c
tion, the equation of the solid boundary wri.tten for a
coordinate system fixed in the basic steady motion is
hex, t) = ± -r [A(t) + x]
where h is the vertical distance, -r is the half-wedge
angle, and ACt) is the distance between the nose and the
origin of the coordinates at any instant.
The y-componentof the nondimensional velocityat the sol
id boundary is, up to the first order approximation,
v = q -1 ht + h = ± -r[l + A/q ] c x c
. Note that the velocity A = dA(t)/dt should be small com-
pared with the reference speed, qc' in order that the
linearization be valid, whereas the acceleration A need
not be small. Now, by Eqs. (7), (9), and (15), it fol
lows that
(12)
(14)
(15)
II11
11\
I 1
i 1
II III II !
11'11 .dl illl il II I Ii II II :1 ~ : II . I
I
I
I II I!
o
on the wedge. By integration,
I where ~ (t) is an arbitrary function of time to be de-termined later. Equation (16) is the boundary condition on the wedge surface.
(4) Since the flow at x = :I: (X) should not be disturbed by the unsteady motion of the wedge, the complex acceleration potential must be a constant at x = ± 00. On line oc (y=O, x<-A) andline ef (y=O, x>.e-A), \
V :: 0, by symmetry. Hence,
'" ;::: 0
Here, the constantis chosen to be equal to zero to agree with the steady flow condition. The only exceptional case J_S the case when (1;::: O. In this case, .e -+- + (X) and '" at + 00 is equal to 'V at + (X) which is not equal to zero.
(16)
(17)
The aforementioned boundary conditions are just enough to determine . , the complex acceleration potential uniquely, provided that the function ~ (t) is known.
1 The arbitrary function ~ (t) should be chosen so that the kine-matic conditionon the wedge surface is also satisfied by the velocity field. The integral of the se cond equation of (7), satisfying the conditions tha t v = 0 at x;::: - (X) is, Ref. [1),
x
(18)
Equation (18) is the additional condition requiredto solve the problem (kinematic and dynamic) uniquely.
7
It should be noted that the so-called closure condition [6, 7, 8]
or the second additional condition [9] is not necessary_ For an unsteady
flow, the cavity boundary is not a material line and the closure condition
would be written
f ah
--dx=O ax
(19)
where the integration is meant to be carried over the closed boundary of the
boQy plus cavity. Upon substitution, Eq. (19) leads to
f ah . J dS -- dx = q vdx = --at c dt
(19a)
where S is the cross-sectional area of the cavity. No additional inforn~
tion can be derived from Eq. (19a). Wu [10] assumed constant-cavity volume
(dS/dt = 0) but this was unnecessary.
III. THE CONFOR}ffiL T&hl~SFORY~TIONS
The linearized physical plane is shown in Fig. lb. In this case,
the flow is symmetrical with respectto the x-axis and only the region y ~ 0
need be considered.
The Schwarz-Christoffel transfornmtion
1 Z = -- log r - A
b (20)
2n
transforms the upper half strip of the linearized z-planeinto the upper half t
of the r -plane as shown in It'ig. 2a. It is more convenient to work on the t
r-plane which is relatedto the r -plane by the following linear transforma-
tion.
t 2n r = U - 1) / (exp - - 1)
b (21)
The ·resulting transformation does not alter the body size but transforms the
points at - (Xl to (-x, 0) , the nose of the wedge to (0, 0) , and the o
8
I I tail of the cavity to lowing formula s.
(.e, 0). Here, x and.e are given by the folo
2n -1 x =: (exp - - 1)
o b' (22)
I .e .. x (exp -- - 1) o
2il.e (23)
b
I where .e may be called the reduced cavity length and lndlcates the extent of free surface effect on cavity length, .e. Equation (23) is plotted in Fig. 3.
I It is interesting to riote that when b-+ 00, then x -+ ro and .e -+.e, o the net result of the transformation is only to shift the origin to the nose of the wedge. Thismeans,for b-+oo, the transformation Eqs. (20) and (21) transform the flow into itself. Hence, it is obvious that the transformation indicates the effect of a finite stream. It should be further noted that the transformation does not specify the boundary condition and, hence, it may be applied both for the flow in a jet and for the flow in a solid channel. However, the boundary conditions are written on the figure for the jet.
IV. METHOD OF SOLUTION
It is required that an analytiC function F( n be found which is regular everywhere on the upper half of the {-plane and satisfying the following condition on the real axis.
(1)· ~ < - x, ~ = 0 o
(2) -x<~<O ..p=0 o '
(3)
(4) I CT
l<~<.e, ~=----2(1 + 0")
(5) I
.e < ~, ..p = 0
(6) ~ .. :!: 00, ¢ = ..p = 0 except when .e = 00
(24)
On the r -pla.ne, the fl.lnction "'I is
where
f ..
b A
"'I = -'Y 2 2nq c
A log (1 + ~/xo) + 2 ---- + 1
qc
.. '1'( t) = J< t) - A t
qc
•
9
(16a)
(25)
The unknown f1.lnction wet) is shown to be equal to -A/q in Appendix A for c the special cases when the motion dA/dt is of an oscillatory type along the
x-axis or when the cavity is infinitely long.
To solve the mixed boundary value problem of the type of Eq. (24),
the generalized method of solution due to Cheng and Rott [11] may be applied.
The first step is to find the homogeneous solution H(r) satisfy
ing the following homogeneous boundary conditions:
(1) ~ < - x 0' ¢ = 0
(2) - x < ~ < 1, '" = 0 0
, (24a) (3) 1 < ~ < e , ¢ = 0
(4) ,
e < ~,
Since the pressure must be finite everywhere, the only possible homogeneous
solution is
(26)
Suppose the complete solution of the given problem with boundary conditions
of Eq.'(24) is F(n - ¢(~) + i¥t(~). Then the imaginary part of the function
Gcn defined by
F(n G(t) ,. a p(~, 1]) + i q(s, 7])
H(O (27)
10
is completely specified on the real axis. That is,
-i on the part where ~(s) is known q(s) =
on the part where ~(s) is known
Thus, the problem is reduced to a regular boundary value problem for the function G(r). The solution is
+00
G(r) = -=- f q( T)
dT n T _ r (28)
-00
or by Eq. (27)
+00
F(n = -=- H(n f q( T) dT
n T ... r (29)
-00
provided that F({) satisfies the boundar,r condition at infinity [11]. For the present problem,
(24b)
2(1 + 0")
J ______ 1;.:.-. ___ ,,--__ , 1 < T < t t
~ ( T + X ) (T - 1) (t - T) o
q( T) .. 0 for all other values of T
By substitution, Eq. (29) reads
11
1 ~ . I f 1/11 (T) dT [
1
;or - (r + xo) ( r - 1) (r - f, ) . _
n . 0 ~ (T + xo) ( T - 1) (T - f, ') (T - r)
I
(f $. ] i . . dr ..
1 ~ ( T + xoH T - 1)($ I - T)( T - n (29a) +----
Equation (29a) is an elliptic integral. The resulting drag coef
ficient will be discussed in the latter part of the paper. For the special
cases of infinite cavity or infinite fluid, the equation is reduced to elemen
tary integrals and their values can readily be computed.
A. Infinite-Cavity Case ,
Since .e -+ 00 and (f = 0, the complex acceleration potential is
.. ~ ( r + x ) ( r - 1) o
Here, .. q is equivalent to U • c and the function i' is determined to be
-A/qc (see Appendix A).
Since p = P, the drag coefficient may be written as c
1 - A
drag J CD = 1/2PU2 = -4Y ~(x. 0) dx
- A
or in the r-plane
12
21'b
n
where Re means ureal part of."
1
1 Re F(!;)
o
d!;
!;+x o
By substitution it follows that
where
81'2 A
°DO = (1 +-) bI U
0 n
81'2 .. A 2
°D1 = --"2 b 11 n U
with 10 and 11 meaning
1 10g(1 + T Ix )d r 0 =
(31)
(32)
(33)
(4)
di; (36)
1 t 1
1) ] ~ Re ~(!; + x o)(!; - 1) J 11
8n2 (T - t[,)~ (T + xo) ( T - t[,+x o 0 0
The double integral Eq. (35) can be integrated and yields (see Appendix B for
the detail of computa tion)
1 1 I = -- (arc sin )2 o 2n ~1 + Xo
(37)
It should be noted that when flow is steady A = A = 'II = 0 and the
drag coefficient given by Eqs. (33) and (37) is identical to the steady-flow
solution given in Ref. [5]. It is also interesting to note that for infinite
fluid case
lim
b ~oo
bI = 1 o
13
(38)
and Coo is reduced to the steady-flow solution given by 11. P. Tulin [6].
B.1 changing the order of integration, Eq. (36) is reduced to
1 arc sin ----
1
J log(l
o
~l + x o
1 ( dr J log(l + r/x )
o ~ (r + xo)(l - r) o
dr (J6a)
Integrating the second integral by parts, Eq. (36a) is changed to a more con
venient form for numerical computation
I :: 1
where
When Xo > 1, 12
The results are
1
( 2 arc sin
1 ~l + x 0
8n2
~o (36b)
1 f log(l + ~/x )d~
12 = J ~ (1 + ~/x ) (~ _ ~) o 0
(39)
1 2
~ log (1 + six )d~ I = 1/2 . 0
3 ~ (1 + ~/x ) (1 - ~) o 0
(40)
-1 may be expanded into infinite series in x • Q
14
4 4 23 176 1,126 ,12 (1/3 - + +
3,46.5x 4 . ) =-
2 945x 3 • • x l.5x 10.5x
0 0 0 0 0
(39a)
2 2 43 76 12,139 13 = (1/3 - + +
3l,18.5x 04
. . . ) 2 lO.5x 0
2 Id9x 3 x 5x 0 0 0
(40a)
For the infinite-fluid case, calculation shows that
lim
b ~oo
-The drag coefficient for the infinite cavity in infinite fluid is, therefore,
• •• A A.
GDoo = -- (1 + - + ---y-) n U U
(42)
For other values of x , x ~ 1, Eqs. (39) and (40) were integra-o 0 ted numerically. The effect of jet width on the drag coefficient is shown in Fig. 4 where both bIo and b2Il are plotted as functions of b. It should be noted that at the other limit where b = 0 both bIO and b2Il are equal to zero.
This section can be concluded by remarking that the added mass of a supercavitating wedge at zero cavitation number is
2 -- p b II
which takes the maximum value of plies that the added mass effect is tion
n
4'Y2 n p in infinite fluid. It also im-
important when the dimensionless accelera-
.. AG
7 (43)
is not too small compared to unity. Here C is the wedge chord. As an example, if a one-foot-chord wedge is moving at 60 ft per sec, the acceleration
15
term of the drag force can be equal to the steady force when the acceleration
is equal to 111 g.
B. Infinite-Fluid Case
It is readily seen that the transformation given by Eqs. (20) and
(21) degenerate to a parallel translation when b approaches infinity. Hence,
the problem could be solved either on the r-plane or on the z-plane. Since I
$ = .$, the acceleration potential on the r-plane is
F(n • - -=-~(r - 1)( r_ $) 1t ~( r- 1)( r- $)( r - n
(44)
•• 1 A f rdr
J ~(r-l)(r-$){r-n o
(f J -r======-==-d_r --1 ( r - 1)($ - r)( .,. - n
1
When the perturbation velocity A is an OSCillatory motion, '11 is found to . be -A/q (see Appendix A). Only this type of motion is considered herec after. In order that the acceleration potential given by Eq. (44) satisfy
the conditions at infinity, it is further required that
1 .. 1
A 1 d1' A
S rdr
'Y(l + -) +'Y 2 q ~( T - 1)( r - $) qc ~( r - 1)( r - $) c 0 0
.e (f J
dr = 0 (45)
2(1 + (f) .oJ( r - 1)( 7'" - t) 1
Performing the integrations, this leads to the following forrnulc: which re
lates the cavitation number and the cavity length.
16
A -{t + 1 A [-{i 21'(1 +-) log +1' 2
qc ..Jt-l qc
~+l ]- nO' + (t + 1) log ::: 0 (4Sa)
..J-e-l 2(1 + 0')
For harmonic oSCillations, by writing A = A sin wt, the equation is changed o to
0' 41' f cos wt)
..Jt + 1 ::: (1 + log
1 + 0' n ..J {- 1
21'12 [-V + (t + 1) .ft+ 1 ] sin wt log
nA ..J e - 1 0
where A = dimensionless amplitude normalized with the chord, and o
A w o --= reduced frequency.
(4Sb)
In particular, when the flow is steady, then A::: A 0 and the condition
(LSa) is simplified to
0' 41' ~ + 1 --- ::: -- log r:==:.-
n ~t-l (4Sc)
1 +, 0'
It can be noted that Eq. (LfSC) is almost identical to an equation developed
by Fabula for his open-cavity model (12J.
To show the effect of acceleration on cavity length, Eq. (L.5b) is
plot/ted in Fig • .5 for the case of u ::: 0.1 and 1'::: IS degrees. The upper
graph shows that the amplitude of cavity-length oscillation increases if A . a decreases when f is kept constant. Two limiting cases when f> > i jA ,
~ ~ 0 small added mass effect, and f < < f jA , large added mass effect, respective-a ly are shown in graph b. The 90-degree phase shift between the two curves
should be observed. The following explanation is offered to facilitate better
understanding of the effect of acceleration on cavity lengtho
...,
-It is known that the acceleration of a solid surface into
a fluid creates a positive hydrodynamic pressure on the
surface due to the added mass effect of the fluid. This
pressure impulse is propagated in all directions with the
speed of sound (which is infinite when the fluid is in
compressible). Negative pressure is created when the ac
celeration is. away from the fluid. When the body under
takes an oscillatory motion, as in the case considered
here, a continuously varying pre ssure field exists. Since
the pressure on a free surface remains constant, the var
iable pressure field has a similar effect as a variable
cavitation number. Therefore, it is expected that the
cavity is longer when the acceleration is toward the cav
ity than when the acceleration is toward the liquid. This
is clearly shown by the first curve of Fig. 5b.
17
Moreover, Fig. 5a suggests that the cavity may disappear at a cer
tain instant if the acceleration te);'m is of such magnitude that the minimum
.e is less than or equal to 1. This is the condition for which the cavity
is t~washed off lt the body. Thus, the wash-off condition, by setting .e = 1
in Eq. (4~b), is
[1 + f cos
This equation leads to
re t-
A o
",2 f
sin wt]. = 0 nun
A = -----
o -Vl-f'2 (46)
Note that the wash-off condition (46) is independent of q and 'Y. Equation
(46) is plotted in Fig. 6. Since the linear theory is not accurate for small
.e, Eq. (46) must be applied with caution. The drag coefficient is
c = D
1 - A
S (p
-A
1 - A
pc)dx = 2'Yq - 4'Y(1 + q) f ~(x)dx -A
18
or on the r -plane
1
CD = 2'Yq - 4'Y(1 + q) J Re F( l;) dl;
o
Substituting Eq. (44) into Eq. (45a) , it follows that
",here
• A
Coo = -- (1 + --) (1 + q) LO
and
1 [1 La - 1/2 Re 11~ (~ -1) (~- $) ! d1"
~(T - l)(T - t)(T - l;)
1 ~1 L1 = 1/2 Re \ ~ ~ (~ - 1) (~- $) ~ Td.,-
~( T - 1)( T - $)( T - l;)
1
(~ - $) [1 L2 = 1 - ~ J ~ (l; - 1) d1"
~( 1'" - 1) (t - T) ( T - l;) 0
(47a)
(48)
(49)
(50)
(51)
1 d~1 (52)
1 d~ (53)
1 ds (54)
The details of the evaluation of the fil:'st two integrals are shown in the Appendix. The results are
{i + 1 1 L =~log .. +-
1 ~t-l' 4 r -($ - 1)
~ direct integration,
L = 0 2
19
(52a)
log -;===- 2 ~ +1 ]'
vt - l (53a)
(54a)
It is readily seen that when (I = 0 and t-+ 00, Eq. (48) is re
duced to Eq. (42).
Wu has worked out a problem of an accelerat'ing wedge in infinite
fluid [13]. He considered a case wherein a wedge was given a sudden acceler
ation of magnitude a at t = 0 and maintained the same acceleration there
after. He assumed that for small t the velocity potential may be expanded
into a power series of t and, hence, the drag coefficient would be
He then concluded that
+
8,2 Coo = - (1 + (I) (---)
n t - 1
2 ..J t - l ] {t+l - '($ - 1) log _r: . iog_f:
~ t - 1 ~t - 1
Q (-{t --)
'Ya
..Jt-l + 1) log w
-fi - 1
(55)
(56)
(57)
where Q is the rate of cavity-volume increase assumed to be a consta:tlt. He
did not compute CD2 and higher-order terms. It is readily seen that the
present solution agrees with Wu I s solution, (56) and (57), up to the order of
,e-l/2 (order of (I) if Q is set equal to zero.
20
To give an idea of the relative importance of the cavity-length effect, the functions LO and ~ are plotted in Fig. 7. It is seen from Fig. 7 that the cavity-length effect is very small for a long cavity and this is the reason why most of the linear theories give reasonably good prediction of the drag coefficient even though the cavity length is not accurately predicted.
C. General Case
Here, the general case of a finite cavity in a finite jet will be considered. The complex acceleration potential in the r -plane is given by Eq. (29a). Moreover, to satisfy the boundary condition at infinity, F(±oo):: 0,
__ the following equation must hold.
1 dr f \]11 ,"'"
o ..J(e'_T) (1 - T) (T + X ) 0
I t
0- f ~ ($'
dT + = 0
2(1 + 0-) _ T) ( T - 1) (T + X ) 0
Equation (58) may be simplified to
. 21'(1 + A/q ) F(fP, k) c
------- = ----------~----------1 + 0-
'YbA + ---2""'---
nqc K(kl )
K(kl )
1 f log(l + T/X )dr
J -;:=:::::=========o======..J ~ t I _ r) (1 _ T) (T + X ) o 0
where F(fP, k).= incomplete elliptic integral of first kind, K(kl ) = complete elliptic integral of first kind,
If' = arc sin
I X +.e o
I I .e (x + 1 ) o
argument,
(58)
(58a)
k = 1 +- x
o --="', --- = modulus, and f, + x
o
~ t - 1 kl = I = modulus •
.e + x o
For steaqy supercavitating flows, Eq. (58a) is reduced to
u ---.=-----
21
(59)
The drag coefficient can still be written as the sum of three terms,
as indicated by Eqs. (48) through (.?l). How"ever, the meanings of 10 , 11'
and 12 are different from those given by Eqs. (52), (53) , and (54). The new
quantities are given by the following double integrals.
1
H(~) ~ 1
b J dt-
10 =-Re dl; (60) 4n l; + x (r - l;) H( r)
0 o 0
~ " ~!~ J H(s) ~ log (1 + r/x ) d 1 ds \
0 (61) 8n 0 l; + Xo 0 ( r - s) H(r)
1 b J H(l;) dr
1 == 1 -2 [fJ (t' 1 ds (62) 2n2 l; + x
0 0 _ r) ( r - 1) (T + X ) ( r - l;)
0
where the function H is defined by Eq. (26).
Following a method similar to that used to evaluate Eq. (52) and
shown in AppendixB, 10 of Eq. (60) is found to be
10 = ~ F(CP, k) [2E(CP' 2n
, f, - 1
k) - __ ,=----- F( cP , k) - 2 .e + x o
-f,"-:'-( f,_x~o_+-x-o-) } 600)
22
where E(~, k) = incomplete elliptic integral of second kind.
It is readily checked that when b--+ (X) Eq. (60a) is reduced to Eq. , (52a) and when t --+ 00, it is reduced to bIO of Eq. (33).
The exact value of Ll is rather difficult to compute. Howeve~, since t'·~ t > 1, the integral may be expanded into power series of lit • The result is
where 0 means order of magnitude.
,-2 + oCt )
1 ) a rc sin --;:::=:::::;::
-Vxo + 1
~61a)
The function L2 ting once with respect to integrals (14].
reduces to the following expression after integraT and by using an identity formula of elliptic
(62a)
(3
where Ao «(), kl ) = Heuman's lambda function,
fJ • arc Sin~ 1 :OXo ' and
() = variable of integration.
The function 10 , which indicates the effect of jet width and cavity length on'the steady part of the drag coefficient, is plotted in Fig. 80 It is noteworthy that, for any given jet width and relatively large t, the effect of cavity length on drag coefficient is very small. The added mass function 11 is computed up to the second term and the result is plotted in Fig. 9. Since the second term is positive and is a monot0nically increasing function of t-l , the added mass is greater when the cavity is shorter. The origin of the function L2 may be traced back to the fact that the pressure
- --------~~~ -- ~~--------
2.3
in the cavity is different from the ambient pressure. It varies from one to
zero as the jet width changes from zero to infinity. This statement has the
following physical significance: for a very narrow jet, the pressure on the
wedge surfaces is almost equal to the ambient pressure and the drag is almost
equal to the pressure differen,ce between the ambient and the cavity. The func
tion L2 will be called the "pressure function. tI The pressure function ~
is plotted in Fig. 10. It can be observed from Fig. 10 that L2 is a weak
function of cavity length.
There is no theoretical result or experimental data available to
check the unsteady part of the pre,sent theory. Only the steady part of the
solution could be verified by experimental data. The steady cavity length
given by Eq. (59) is plotted in Fig. lla for four different jet widths. Also
Shown in the same figure are Cohen and Tu's [5] curve for b = 10 case and
Wu's curve based on infinite-fluid theory. Some new data were taken in the
free-jet turmel of the St. Anthony Falls Hydraulic Laboratory for two wedges
of different chord and wedge angle. These data are quite similar to those
obtained previously in the same tunnel with a less sophisticated dynamometer
[.3] and are compared with the theor,y in Fig. lIb. Considering the fact that
the cavity length has always been difficult to measure and predict, the agree
ment is fairly good. The steady part of the drag coefficient given by the
present theory is plotted in Fig. l2a for a IS-degree wedge. Cohen-Tu and
WU IS results are very close to the present result and they are not shown in
Fig. l2a. Figure l2b shows the comparison of the data with the theory. Here, ~k
the agreement is very good.
v. CONCLUSIONS
A linearized acceleration-potential method has been applied and a
singularity-free solution has been obtained for a problem of unsteady super
cavitating flow about a wedge in a finite jet when the flow is symmetrical
with respect to the x-axis. The most important conclusion that can be drawn
from the present study is the fact that a singularity-free solution (finite
* For a steady infinite cavity an exact theory due to Siao and Hubbard is available [.3]. For ~ = 15 degrees and b = 10, CD = 0.140 by this theory andthis result maybe compared with the present theoryinFig.12b. (CD = 0.140 is somewhat larger than the result quoted in Ref. [3], a numerical error having been found in the computation for that reference.)
i
I
I
24
pressure everywhere) exists even with linearization. The existence of a sin
gularity-free solution requires a new condition (mathematical but not physical)
which gives the relation between the cavity length and the cavitation number.
By this method, not only the need for the additional physical condition or
the closure condition is eliminated, but also the process is considerably sim
plified. Since a steady-flow problem is a special case of an unsteady-flow
problem, and in view of the good agreement between the theory and steady-flow
data, the present method can also be applied to solving other steady, super
cavitating-flow problems with advantage.
[1]
[2]
[3]
[4]
[5]
[6]
[7J
LIST OF REFERENCES
Von Karman, Theodore. "Accelerated Flow of an Incompressible Fluid with Wake Formation, II Annali di Maternatica Pura ed Applicata, Series IV, Vol. 29, pp. 247-249. 1949. Collected Works, Vol~ IV, pp. 396-398.
Yih, C. S. UFinite Two-Dimensional 9avities," Proceedings of the R~~al Society of London, (A), 25tl, 1292, pp. 90-100. October 19 o.
Silberman, Edward. "Experimental Studies of Supercavitating Flow about Simple Two-Dimensional Bodies in a Jet," Journal of Fluid Mechanics, Vol. 5, Part 3, Appendix B. 1959.
Cohen,
pages.
Hirsh and Tu, Yih-O. A Comparison of Wall Effects on SupercavHating Flows Past Symmetric Bodies in Solid Wall Channels and Jets. Rensseler Polytechnic Institute, RPI Math Report No. 5. October 1956. 13 pages.
Min, M. P. Steady Two-Dimensional CavitrloWS About Slender Bodies. David Taylor Model Basin Report 34. May 1953. 29 pages.
Parkin, B. R. Full -Cavitatin H drofoils in Nonstea fornia Institute of Technology, Report No. 74 pages.
Motion. Cali-5-2. July 1957.
[8] Timman, R. itA General Linearized Theory for Cavitating Hydrofoils in Nonsteady Flow ,It Second Symposium on Naval Hydrodynamics, edited by R. D. Cooper, Office of Naval Research. August 1958.
[9] Geurst, J. A. A Linearized Theory for the Unsteady Motion of a Supercavitating HydrQfoil. Institut voor Toegepaste Wiskunde, Technische Hogeschool,Delft, Nederland, Report No. 22. April 1960. 83 pages.
[10] Wu, T. Yao-tsu. A Linearized Theory for Nonsteady Cavity Flows. California Institute of Technology, Report No. 85-6. September 1957 • 28 page s.
[11] Cheng, H. K. and Rott, N. IlGeneralizations of the Inversion Formula of Thin Airfoil Theory, II Journal of Rational Mechanics and Analysis, Vol. 3,No. 3. 1954. Indiana University, Bloomington, Indiana.
[12] Fabula, A. G. A lication of Thin-Airfoil Theo to drofoils with Cut-Off Ventilated Trailin~ Edge. NAVWEPS Report 7 71, NOTS TP 2547, September 1960. 0 pages.
26
[13] Wu, T.
[14] Byrd, P. F .. and Friedman, M. D. Handbook of Elliptic Integrals for Engineers and Physicists. Lange, Maxwell, and Springer Ltd., New York. 1954.
FIGURES -------(1 through 12)
29
y
p=p 0'
b a
b '2
u c 0 h (x,t) '>
p= Pc e f x
b ~I~ i: '2 ht) =1 II
! ~ p=p
(a) True z - Plane
y
0' 4>=0 b a
cr
1J1=0 1J1=1/I, d 4> = 2(1+cr) 1J1=0 o I e f c x
S Atl) ~ ----1 ~(t) -I
4> :0
(b) Linearized z - Plane
Fig. 1 - Flow Configuration and Linearized Boundary Conditions
30
a
a
'1]'
cp=O 0/=0 -I" 0/='" , o· b, e 0
r-- I I~ 211"
ell 21Tl
ell
(a) ~' - Plane
cp = 0 --r+- 1/1=0
x = o
b,c
I-- Xo --·t4<---- I --121ft
2 Xo ----.!.r4--111 - i' = e2: -I eli -I
2w eb-I
(b) ~ - Plane
+ d
~I
Fig. 2 - The Conformal Transformations
cp = 2(~CT) + 0/ =0
e f ,(
~
f
"0< ..
.£: -0' C
~ ~ > 8 "C Q) (,) ::I
"C Q) a::
1-1
N.o
0 1-1 .J:l
40
20
10
6
4
2
1.0
0.9
0;8
0.7
2 4 6 8 10 20 40 100
Cavity Length, l
Fig, 3 - Reduced Cavity Length as a Function of Actual Cavity Length and Jet Width
~ F-IJ ";:7
~
1 ~ ,...;
b2 I I/
/ ViIa I ~ 0.6
0.5
V /
0.4 If II
0.3 I 2 4 10 20 40 100 1000
Jet Width b
Fig. 4 - The Effect of Jet Width on the Drag Coefficient for the Infinite-Cavity Case
31
32
26
24
22
20
.18 ~ -CI
Ii 16 ..J
:t:.:;; 14 c (.)
12
10
8
6
~
~~-\
.........
~ ~ --- ---~ ~ ...........
i\ -............ -\
"'-r--V
r-. I / \.3 Ao=0.02
/ \ / 1\
/ 2'A"O.!~ :! /l~ --- __ I --- V ~~~ ---
// ~ V Steady Cavity
1 V (a) f =0.1 Case
18'---~--~--~--~--~--~--~--~---T--~--~--~ -.c 16 j----t---''''''-:-;!.-. -CI c: j 14~~r===~~~==;=~~~~===r===f~~==~~~~~ >.
~ 12t---t---tl==f===~~~~jt~~~~---+---+---1--~ (.)
100 30 60 90 120 150 180 210 240 270 300 330 360 Phase, wt
Fig. 5 - The Effect of Acceleration on the Cavity Length (0- = 0.1)
5
2 V-
.,,/ -2 IxlO 0-4 2 I x I .
, ,
/'" I--'
Wash-off Region ,,/V
~- 2- I"
Note: Three Points ,,/
Correspond to Finite Cavity Region Three Conditions
IIII1 I in Fig. 5 (a) - - -5 Ixl0 3 2 5 Ixl022 5 IxlOI 2
Dimesionless Amplitude, Ao
Fig. 6 - The Wash-Off Condition
2.2
2.0
...J
-g c o
1.8
1.6
...J 1.4
1.2
1.0
0.90 0.1 0.2 0.3 0.4 0.5 0.6 0.7 I
T Reciprocal Cavity Length,
Fig. 7 - The Effect of Cavity Length on the Drag Coefficient for Infinite-Fluid Case
0.8 0.9 1,0
'vJ VJ
2.0 I 1.6
b= en
1.8 1.4
1.6 1.2 , , I
I
1.4 1.0
0 C\l,o
...J 1.2 I 0.8 J
1.0 0.6
L
/ II
b=i
/ 0.8 0.4
0.6 0.2 //
/' ~ ~ I~ ------OA 08 o 0.2 0.4 0.6 . 1.0
o o 0.2 0.4 0.6 0.8 r.o Reciprocal Cavity Length,-t
Fig. 8 - The Effect of Jet Width and Cavity Length on the Steady Part of the Drag Coeffi c ient
Reciprocal Cavity Length,t
Fig. 9 - The Effect of Jet Width and Cavity Length on the Added Mass Part of the Drag Coefficient
1.6
1.4
1.2
1.0
C\l ...J 0.8
0.6
0.4
0.2
a
b=O
I
1
b .. 2 --- r- b=5 I
~
I---I
---- i ------- b=IO -- r----. b=20 :---~ -
b= en - -o 0.2 0.4 0.6 0.8 1.0
Reciprocal Cavity Length, t Fig. 10 - The Effect of Jet Width and Cavity length on the Pressure Function, l2
\JJ .r=-
-.-.~".~i!li
0.5
014
b
.: 0.3 CD
.Q
E ::s ;Z
c: 0
+= 0.2 0 .-'> 0 0
0.1
0.5
014
b .: .8 0.3 E ::s
Z
c: o
~ 0.2 o o
0.1
35
co .. ~ L _ E 59 2,b=10 A q. 3,b=5
~ V 4,b=2 A / --- Wu, b=<» '
~ / --- Cohen-Tu,b=IO ~ /
/ /' d ~ V L
if' I ~ V V l / /
/ I ~ ~ / V
I A 1/ I
~ V V I I ./
i / ~ V V V
/ , I
~ V V /,~ ./
~ V (0) Comparison of Theories for r=15°
0.1 0.2 0.3 0.4 0.5 0.6 0.7
Reciprocal Cavity Length, t v
0 r = 15°, b=IO V t--- 0 r =7.5°, b=5
V - Eq.59 /'
V /
/ V
(")
/V 0
l.....--::: f-'
0
00 /
V V ~ n ........-0 y V V-0 1M --v: 0 V ~ d J::j0 3--
It y y (b) Comparison of Theory and Data
·1 I 0.1 0.2 0.3 0.4 0.5
Reciprocal Cavity Length, t 0.6 07
Fig. 11 - Steady Cavity Length as a Function of Cavitation Number
0.8
OJ ~I ----~----+_----+_----~--~----_4
0.6 rl -T-+-+--L- I o I J b=o:> u I b=IO t.5 ~g:~ I
'(3
;::-0.4 1 ~ ~ /1
U
gO.3 1 I#ZI ~ M9 A
o
0.2 I :/9'lf A
0.1
0.2 0.4 0.6 0.8 Cavitation Number, (j
1.0
(a) Drag Coefficient for y=15°
o U .. -c: Q)
'(3
O~ ~I-----.----~-----.-----..-----r---~
0.3 I j"{
y=15°, b=IO :E 0.2 Q) o
U
CI o 10. o
" " 0.1 I 1 ....... ,.eJ t
y=7.5°, b=5
00 0.1 0.2 0.3 0.4 Cavitation Number, (j
0.5
(b) Comparison of Theory and Dota
0.6
Fig. 12 - Steady Drag Coefficient as a Function of Cavitation Number
__ ~" •• ,~ ________ ?_~ ___ ~ ___ c_~~·
w a-
f F I [
APPENDIX A --------EVALUATION OF '!HE FUNCTION iT(t)
39
APPENDIX A
EVALUATION OF THE FUNCTION wet)
The evaluation of wet) for the most general case is rather in
volved and will not be attempted here. When the unsteady motion is of oscil
latory type or when the cavity is infinitely long, then time and space vari
ables may be separated and the problem is particularly simple.
A. Oscillatory Motion
If the unsteady motion is of oscillatory type and is given by
A(t) = AO exp(jwt)
the imaginary part of the complex acceleration potential may be written as
~ = ~O(x, y) exp(jwt)
where j stands for ~ (but ij f -1) and Eq. (18) is reduced to
x wx ( wr
V :: - exp(-j-) J exp(j-) qc qc
-00
Integrating by parts, Eq. (A-I) is reduced to
w WX V ::: - ~(x, y) + j -- exp(-j --)
qc qc
01/1 -dr
{).,.
x , WT ) ~exp(j --)d r
qc -00
(A-I)
(A-la)
Therefore, since ~ = 0 on (y = 0, x < -A), the condition (18) applied at
the nose of the wedge is
A 2A 'Y (1 + -) = +-- + w) (A-lb)
qc
Hence
['
40
•
\}I(t) = - - (A-2)
B. General Motion with Infinite Cavity
It is more convenient to rewrite the complex acceleration potential
given by Eq. (30) as
where
2A ,::::t~ fl (t)·-;; '1'(1 + - + \}I)
U
'YbA f 2(t) :; -~
2nU2
1 F 2 (n := - ~ ({' + x 0) ({' - 1)
n
1
1 ( log(l + r/x ) dr
J ~(r ± X ) (T - ~) (r - () o o
With these notations, Eq. (18) is reduced to
-00
X T
- - +_\ i
X T dF2 - - + -) Im(-)dr
q q dz c c
(A-3)
(A-5)
Again integrating Eq. (A-5) by parts and setting x:= -A and y = 0, the
additional condition is reduced to
• A
1'(1 + -) = u
-A
J afl <3f2 fl(t) - Im (- F + F2)dr aT 1 ar (A-6)
41
Since the imaginary parts of Fl and F 2 are both equal to zero on (y = 0,
- 00 <x <-A), the integral of Eq. (A-6) is zero if fl and f2 are differ
entiable. Under this circumstance, Eq. (A-6) is identical to Eq. (A-lb) and,
hence, the function tJ;( t) is given by Eq. (A-2) 0
!.!:!:!!iQI! B
EVALUATION OF INTEGRALS
45
APPENDIX B ~------- -
EVALUATION OF INTEGRALS
A. Evaluation of 10
Here, the integral in Eq. (35) is to be evaluated. It is more con
venient to rewrite the equation as
(B-1)
By changing the order of integration, it may also be written as
(B-2)
Since
1
Equation (B-2) may be separated into two integrals. That is,
4n 10 = Re l!~_l T--+ x
o 0
1 1
J d -Re
.,J ( T + X )(.T - 1) o 0
S dJ;
~ (J; + x )(~ - 1) o 0
Interchange T and J; and it yields
46
He!l rp+-X10 [~o· ---;=dT=. =1) 1 d'; ~ ';;Xo J. (1" - .;) ~(T + Xo) (T -
(B-3)
Finally, Eqs. (B-1) and (B-3) lead to
1 ( ) 2 arc sin -;:===-
~l + Xo
(B-4)
B. Evaluation of LO and Ll
Straight-forward double integrations of LO and Ll are quite in
volved. Here, similar techniques used for the evaluation of IO can also be
used and reduced the labor of calculations considerably.
By changing the order of integration in Eq. (52), Lom;ay be writ-
ten as
1
1 S 1 LO = --;- He 0 ~ (1 _ T)( t _,.)
1 J ..J (1 - ~)(t - ~)d, d1'
l' - ~ (B-5)
o
Now, by introducing partial fractions, the inte grand of t he first integral
may be separated into two terms in two different ways. They are
~ (1 - ~) (t - ~) =8€ 1 -1" (B-6)
7 - .; 1 - .; 1 - ~ l' - .;
and
..J (1 - ';)($ - ~)
B~ t -i
- $ - ~ + t - ~ (B-7) -r: - ~ " - ~
Using Eq. (B-6) , Eq. (B-5) becomes
1
1 =~S o 2 o
-r====d=T===-f -~ d1; ...j(l-T)(t-T) o~
1 +- dT
2
Using Eq. (B-7) , Eq. (B-5) becomes
1 1 =-o 2
1 +- Re
2
1 1 dT
J 1Ed" ~ (1 - T) (t - T) .e - '{:: ... 0 0
~.re:-r J~~ o
---dT Jf1=T ~~ dl;
o
47
(B-8)
(B-9)
By interchanging the variables l' and l; and changing order of integration,
it can be shown that the second term of Eq. (B-3) is equal to the negative of
the second term of Eq. (B-9). Therefore, by eliminating the second terms be
tween Eq. (B-8) and (B-9), 10 is found to be
1
~ dT
o ...j (1 - t) (.e - 1')
~+l =-{elog --
{i - 1 (B-IO)
Since 10 is knovm, Ll can be most conveniently evaluated by
first writing it as
'{ ...... , <,
"'--
48
1:t = La + 2- Re J~ (1 - ~) (t - ~) J.~ d" d~ 2 0 o~ 1'- ~
(B-ll)
By changing the order of integration and by partial fractions, the second term
of Eq. (B-ll) is reduced to
1
J~ 1Jg ~ Re J~ (1 - ~)(t d,..
- ~) d~ = ---. d~
2 0 T - ~ 2 t - 'J: 0 o ."
!~ 1 J~: : 1
~ ) 'Ii (1 -r)(t - r) . . dr + - Re dtd~ (B-12)
t -,.. 2 ~ ,.. - ~
0 0 0
Again, the second term of the right-hand side of Eq. (B-12) is equal to the
negative of the left-hand side and, thus,
+ ~(i f1-7 d'V2
4 ~~ o
V+l 1 _r: {"i+12 =-{i log {i + - [V.e - (t - l)log -{i ]
t - 1 4 t - 1 (B-13)
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