ARCh
STEVENS INSTITUTE OF TECHNOLOGYDavidson Laboratory i
Hoboken, New Jersey
Lab. y. Scheepowue
Technische Hoescoo
DeHt
VIRTUAL MASS AND SLENDER-BODY THEORY FOR BODIES IN WAVES
by
Dr. Paul Kaplan
and
Dr. Purig Nien Hu
Submitted to the Midwestern Conference
on Fluid and Solid Mechanics, University
àf Texas September 1959.
June 1959 Note 543
Errata for "Virtual Mass and Slender-Body Theory fôr Bodies in Waves"
Second terni in Eq. [41] should be -Im(n)
Eq. [46) should Iave term in
f
}as
-lb-R1
(b-R)3 R1'2
14 R R2 (b-R)2(b+R) (.. + sin 4 b(_.+1+-.)+
8b3 R 1/2 14 R R2)(b-R)2(R)4
(T 1 b-R i òcL
(3
E
+ + 8b3 . + sin Eq. [47] should ber___
(b-R)3 R 1/2 14 R R2 (b-R)2(b+R)4 (libR1
+s1n1
A42=L
(-3..
+ 1. +_..) 8b3 Eq. [48) should be dL= -
D iL'
Sentence following Eq. [48) should have the word "negative"
before "rate of change".
Abstract
The hydrodynamic forces and moments actiron slender submerged bodies and body-appendage combinations which move oblique to the crests of regular waves are found by application of slender-body theory, utilizing two-dimensional cross-flow techniques. A simple
interpretation of the results leads to identificätionof two components,
one due to change of fluid momentum and the other a convergence effect due to a pressure gradient in spatially nonuniform flow (an extension
of a result due to G.I. Taylor). Corrections are made to dome. previous erroneous results for this problem. Particular examples illustrate the
interference between a body and its appendages in regard to the wave
forces.
N-543
-1-Nomenclature
A(x) cross-sectional area of submerged body
A virtual moment Qf inertia
42 ¡
a wave amplitude
b fin semi-span
c wave propagation speed D
total time derivative
g gravitational acceleration
h depth of centerline of submerged body below calm free
surface . imaginary unit 2ír g k=--
--
wave number L rolling moment M pitching momentm mass of displaced fluid
virtual mass
N yawing moment
p pressure
R radius of circular cross-section r radial polar coordinate
t time V
V forward speed
v,w lateral and vertical orbital velocities, respectively
y ,w values of v,w taken at center of cross-section o o
X surging force
x,y,z rectangular coordinates V Y lateral force
Z vertical fórce
angle between x-axis and normal to wave crests
= y+iz complex coordinate
angular polar coordinate X wave length
p water density
N-543
-3-total velocity potential
(2) total velocity potential in reference (2) velocity potential of waves
øw value of Ø taken at center of cross-section
.øvo velocity ooential due to forward motion Of body
Introduction
In a previous
paper(l)1, one of the authors applied the
slender-body theory to evaluate the forces and moment acting on slender
sub-merged bodies aid surface ships moving normal to the crests of regular
waves.
The same method was used in (2) for slender bodies and
body-appendage combinations, in oblique waves.
The well-known slender-body
theory, which was originally dealing with either steady or unsteady
potential flows representing a body pláced in a spatially uniform
stream, has thus been extended to this particular flow problem which
is both time-dependent and spatially nonuniform.
Since the technique
is two-dimensional, a great simplification is therefore accomplished
as compared with the three-dimensional treatments by Havelock
(3) and Cummins (4).
Also, the influence of appendages can be easily
determined by this method.
However, due to an erroneous boundary
condi-tion and an incomplete expression for the pressure2 (which, fortunately,
does not effect the results for a body of revolution), a simple physical
interpretation could not be given to the results obtained in (2) for the
forces acting on finned bodies.
In the present paper, the corrected
boundary condït'ion will be used to investiate the same problem, and the
nonlinear terms in the pressure equation will be taken into account.
In addition, the forces and rolling moment acting ori
.n asymmetrically
finned body will also be evaluated.
It will be shown that the use of the
correct boundary condition and the nonlinear terms in the pressure equation
leads to a simple physical interpretation of the results.
'Nurnibers
in parentheses refer to the Bibliography at the end of the paper.
2Theauthors are indebted to Dr. John R.
preiter for his discussion about
these points.
N-543
4-A cartesian coordinate system is chosen with the axes fixed in the body, which is constrained to translate horizontally to the right. The x-axis is positive in the cirection of motion, the y-axis is positive to port, and the z-axis is positive upward. The origin is placed on the
axis of the body, located at a depth h below the free surface..
The free surface i disturbed by waves which propagaté with speed
c in a drection oblique to the forward motior of the submerged body. The angle betweèn the x-axis and the normal to the crests is denoted by
, which lies in the range
-T1/2rT/2
as shown in Fig. 1./
N'
Velocity Potential of Waves Near the Body
Fig. i Relation of body to waves
The wave propagation speed c is > O for following seas and c<.O for head seas.
The velocity potent ial of the waves with wavelength X , amplitud , with wave propagation speed c is given by
N-543
-kh k[z+i[xcos + sinn
+(v
cos -c)t)}=ace
ewhere k = = , = is the imaginary unit and only the real part of the velocity potential is to be taken.
In the plane of the cross-section of the body, i.e., the planes parallel to the y-z plane, the vertical and lateral components cf the orbital velocity of waves are
w=-
Wk
ace_ek
{+tx
cos + sin+(v
cos-
c)tJ} [2]or
fil
where the spatial nonuniformity of the flow ìs evidenced by the dependence
of the velocities on the coordinates y and z.
Assuming that the linear dimensions of the. cross-section are small
relative to the wavelength, the velocity potential of the waves may then be expanded near the body intö a power series around the center, y=z=O,
of the crosssection. Neglecting the higher order terms beyond the linear,, this yields
ac e [l+k(z+j y sin)
ek cos+(vcos-c)tJ
-
V Y-W Z
o o
where
0
,
y and w are the values ofw o o
o
taken at the center of the cross-section.
y, and w, respectively, [5]
quatïon [5J shows that the velocity potential of waves near the body may be recognized to be contributed by three components: a uniform
stream y in the y-direction, another uniform stream w0 in the z-direction,
and a spatially independent (in the plane of the cross secion) velocity
N-543
-6-a rid
potential term. Consequently, the potential due to the presence of the body in waves, known as the wave-body interaction potential, may be
determined by the usual, two-dimensional treatment for unifOrm potential flows.
Forces and Moments on a Submerged Body of Revolution
FOr a body of revolution, the cross-section is a circle with its
center located at the point y=z=O . The wave-body interaction potential,
denoted by 0wb' is therefore found to be
2
--(vcos9+wsin9)
r o o
where r and = tan - are the polar coordinates, arid
R=R (x) is the local radius of the body.
Due to the effect of thé forward motion of the body, tiEnormal velocity on the boundary of the cross-section is no longer zero as in the case of pure two-dimensional streaming flow past the section. For a body of revolution, this normal velocity yields a boundary condition for the
total velocity potential , which is
() =V
rr=R dx
Since, the velocity potential terms previously considered (2) satisfy the boundary candit ion
-s [8]
r=R
the additional term due to forward speèd, , also satisfies Eq. [7] and
it is fòund to be
dR
= VR .- log r
Which represents a to-dimensional point source located at the center o
the circle.
The total cross flow potential ' near the body is then
[7]
[g]
N-543
=
=0w0wb'V
in consideration of the order of magnitude of the .nqnlinear terms, where
Therefore, the pressure on the body contour, r=R , is given by
p = -ipage_<'[l + 2(kR - i -)(sin9 +. isin cose))
'.
eb05c0stpy2dj21ogR
-2pa gk e (cos Q. - i sin sin2Q - sin sin Q).
i2k[x.co+(Vco -c)tJ
i .2 (dR2
-p
Integrating the pressure along the body contour, the elemental
lateral and vertical forces are given by
[14)
N-543
-8-2 2
0-v0(r+) cos9
- (r + _.)siri9 + VR log r [10)A substitution of the values of Ø'
, V
and w givesW O O
o.
= ace
h[11(
)(siriO + sinos9)3
eiXC5 + (V cos-c)ti,.
VR log r
This form of the potential obviously satisfies the same boundary condition
[7) , and will be used to determine the pressure
on the boundary of the cylinder.
Lighthill (5) and Spreiter (6) pointed out that the pressure equation for the slender body should be written as
2 2]
[U
.
and Xb and N xs = 2îr sine Rd9 o
= i2page_lth(A(x) -
..L)e1k[XCOS
+ (Vcos -c)t]2cdx
where A(x) = hR2 is the cross-section area.
Integrating the elemental forces over the length of the body,
where x and Xb denote the stern and bow x-c.00rdinates respectively, the total lateral force Y , for the body o revolution, is given by
Y = -2pagk sin
eh(l_
cos)
A(x)e.X. cosp+(vcosc)tJdX[17]
dY
X dx
Where the fact that
A(x)
= A(xb) = O has»bè.en used.Similarly, the total vertica1fòrceis equal to
Z =
pagkeh(1_
cos)
A(x)eWOS0_t]
[16]
['9]
[20]
N-543
-9-The moments about the y- and z-axes, denoted as M and N respectively, are given by
M = - ( x j dx Jx s.
- = -
dYJ p cos@
Rd dx o -kh( VdA e[0
+ (Vcos -c)t],Substituting [15] and [16] leads to M =
2pageh
-ik(1-cos)x1
A(x)ei XC0SC0S-)tJ
dx Xb xcos+(vcos_c)t)dXf 22 J
The longitudinal surging force due to Waves may also be determined
from the present analysis. Following theprocedure used in (2) with the present pressure expression, the final value for the surging force is found
tobe
.kh
X -pagk coso e ,
A(x)etXCO5C9_t3dx
X
s
where only linear terms in kR have been retained (it is assumed throughout. dR
the analysis that the quantities kR and are of the same order of magnitude).
The results given by [17], [18], [21], [221 and [23] are exactly the same as those of Cummins (4), who evaluated the forces and moments on a
lender body of revolution due to waves by application of his extension of Lagallyts theorem to unsteady flows (7), Le. by use of a three-dimensional theory. They are also the same as the resultS of (2) for the case of a body of revolution, therefore demonstrating that the additional source potential
has no influence on the values of the forces and moments for this class
:f bodies.
[23] N-543 lo
-[i
L
+k(i-f
co5)x]
A(x)eN = -2pg sinn e_kh
f
X
s
[21]
Fig. 2 Transverse cross-section of a symmetrical'finned body
The finned circle contour of Fig. 2 is transformed into the upper and lower side of the flat plate strip c'Ç , where
= b + R2
f24)
by means of the transformation
N-543
Symmetrically Finned Bodies
One of the major advantages of the present technique is the fact that conformal mapping methods may be utilized because of the
two-dimensional nature of the slender-body treatment. Slender bodies which are not bodies of revolution, and hence do not have circular cross-sections, may be treated by proper mpping of representative transverse contours
into either ¿ cIrcle or any other simple shape that may be easily solved by
ùse of the methods described above. Some particular configurations will )5e
treaedherein to illustrate the application of these methods.
A particular body that cannot be treated easily or properly by any
of the previous techniques applied to the study of forces in wavés is a slender body of revolution with tail fins terminating at the stern end
of the body. Thi restriction is imposed in order to avoid any complications
due to the trailing vortex sheets behind the fins.
Consider a body with a pair of horizontal tail fins. A transverse cross-section through the tail region is shown in Fig. 2.
AZ
[27] N-543 12 -R2 rl = + -z-. [25]
The velocity potential. for the finned circle of Fig. 2 in.the .-plane
when it is placed in a horizontal stream. y
'O,.
and, a vertical stream W, o
will be the safne as that of the flat plate'.in the r'plane placed in the same streams. This potential may be written as
- vRe(rl) w Re(c2... rl2)i/2
[26]
where the upper sign hold for the 'upper"side of the body (and a similar statement for the lower sign), and Re epresents the réai part of the complex quantities. The. wave-bödy interactió'ñ pQtential will be the potential .given by [26] after subtractin thepotential due to the uniform horizontal and vertical streams y and w . Together with
- O ' O
the potential of the waves and the potentiaÏ duetO the forward motion
of the body, the total potential near the-contour is
=Ø
- vRe()
w0Re(2_)1/2+
VR log r -,Substituting thevalues and expressing the coordinates in polar form in the
-plane results in
ace<e
[xcos+(Vcos13_c)tsiñ(r+ )cösQ
r 4 -., 4
11/2
+k Re [b2+ - - (r2+ .)cos2Q - i(r2- ..)sin2Qj
-
b r rdR
+ VR log r
, [28]where this form of the potential satisfies the boundary condition
=V
at r=R.
dx
The pressure near the body is iven by [12 j. Substituting [ 28 j and setting r = R , the pressure on the circle is (neglecting the second
p
pgi e11XC0
0tj
2ksin Rcos9C
- d
(b2 - 2R2cos2e)1/2_i_i i sink os9
cdx
b2 C dx
ik(b+ - 2R2cos2e)1Í21 - çV2 q::: log R
- d2R2 log r - R2 fdR\2
2 'dx1 r
The lateral force on the body is not influenced by the presence of the fins and hence the same value is obtained äs in[15]. The vertical elemental forces on the circular body and the fins are calcu1ted separately in
'accordance with the dif.ferent pressure expressions, and for the circle
the vertical force is given by '
4pagehe1k[05C0_t]
L
+ (b2+R2) sin 2Rb b2+R2 2h 4Rb2 + ikR I b2-R2 (b2+R2)2sin1
2Rb L 2b 4Rb2 b2+R2 1 2 dR 2 v ( [29]Siniilarly, setting 9 = O , the pressure on the fin becomes (neglecting
[30]
N-543
-13-the second harmonic terms with larger depth
-kh ik[xcos(Vcos-c)t] Pf Page e
-Vd
2 R4 R4)1/2 - - (b +-cdx
2 2 r attenuation) R2sin(r
+ { V R dR (r-R4 2 R42
R4 -1/2--
)(b + ---r b r --1
r -. 2. R4 2 R4 1/2 V 3R R3 dR s in (_. + ik (b +.-b.
r - _-) r i rn
[31]When
b=
R , this value reduces to that obtained for a circle alone, which serves as a check' on the answer.For the fins, the vertical force per unit length is
b
1dZ\
'dx'f
JR
(P»
dr
,
[32]where (Pf) arid (P» are the pressures on
the
lower and upper sides of£ u
the fin respectively0 Substituting [30 1 leads to
= a e
ik[xcos+(vcosp-c)tjívf d (bR\
dx g ecI2
dx '; b '+ sin
b2-R2
d(b+R)
IT dR(b2-R2)2
2 dR22 dx
b 2 dx R 2 dx - b dR(b2+R2)2
-1
b2R2i
.[
b2-R
irb-R2
2 d -sin. 2 2 ' > Rbb+RJ
b2+R2 2 -1b2-R2
'Combining the forces on the cylinder and the fins, the
total elemental forceon the cross sect-ion may 'be expressed as
dZ
-kh[
2 R4 .V d
'2
R4=
ìîrpage
Lk(b
)-i -.
(b +
etxc05_c0s
)t][34]
Since the virtual mass in the vertical direction of the configuration in
Fig. 2 is
- 4
& =
rrp(b2+ ì-
-
R2)b.
(see Kuerti, McFadden and
Shanks (8)), Eq.
[343 may then be expressed as Dw dZ = Di,
otm W)+ m
)] [333 N-543 14 -2 2b +R
N-543
where th = pirR is the mass of displaced fluid.
The above result demonstrates that the, force on the body cross-section is cdntributed by two components. The first term n the right hand side may be identified. as the time rate of change of fluid momentum associated
with the particular section, and the second term s the force arising dUe
to the spatial nonuniformity of the flow (the action of a pressure gradient
across the. body). This latter term is expressed as the product of the mass
of the displaced fluid with the orbital wave acceleration at the center of
the section. When the body is purely two-dimensional, then %- and
the result given in Eq. [36] reduces to that obtained by Taylor () for a two-dimensional body placed in a spatially nonuniform flow. Theréfore, [36].. may be considered as an extension of Taylor's result to the case of slender bodies of varying' cross-section.
For a body with a pair of vertical tail fins of semi-span b, a simi.-lar'résult will be obtained, atìd the valué 6f the'hòrizontal eiethentalforce on:the cross-section is
-ïpag sin
ek(b2+
4)_i
(+
-
R)
ik[xcos+ (Vcos-c)tJ
f37]
which may again be expressed in the same manner, since the virtual mass
in this case is also given by [34].
In each of the above cases, there is no rolling moment because of the symmetry of the configuration.
Asymmetrical Finned Body
Consider now the case of a body of revolution with a single vertical
tail fin terminating at the stern end. A transverse cross-section through
the tail region is shown in Fig. 3..
liz
"y
Fig0 3 Transverse cross-section of an asymmetrically finned body
The finned circle contour of Fig. 3 is transformed into the right arid léÍt
The total velocity potential due to the waves, the wave-body interaction
and the f or.ward motion of the body is then bound to be
= 0W wRe(,u vRe(/42+c2)1/2+ \ÏR L log r
[413
where the upper sign holds for the right side holds for the right side of
the. body (and a similar meaning for the lower sign). A substitution of
the proper values leads to
N-543 16
-side of the flat plate strip
-j/k
i, where
by means of two successive transformations
1 = - j;-and /.4=T)-[38] [39] [40)
dY -kh = - ilpag sinn e k
i-L4
b+R)4_2R2]
the above result agrees. exactly with that in [36].
The elemental rolling
moment about -the x-axis is only contributed by
the force on the fin, and may be expressed as
-
JL]
r dr. [45]where (Pf) and (Pe)
are the pressure on the left and right side of r
the f-in respectively..
Substituting the pressure yields
N-543 17
-= ace hik[ xcos+(Vcos-c)t
j. + k(r+ )sirie
p
+ 1k -sin Re
[(2+
-)cos28 - 2R2+ (b2+R2)+ (r+
R2)(bR)2.9
+i(2-
)sin29 -i(r-R2)(bR2)Q]h/2}
- R)4_3R2]} 1k[xcos+(Vcos-)tJ
. [43]
Since the virtual mass in this case (8) is
=
p [(b+R)4_12R2b2] ,
[44J + VR log r
[42 J
The pressure on the body may be calculated from { 12
J, but the result is
too complicated to be written down here. However, integrating the pressure over the contour, the vertical elemental force on the contour is the same as obtained for a body of revolution, and the horizontal elemental force. is
= k Í2
()l/2 (3b+2Rb43R)
4b2 b+R)3 (b-R)2 (- b-R)] - . V df
2(b-R)3 Rl'23b2+2Rb+3R21cdxl
b b l2b ) + _.(b+R)3(b-R)2(- + sineXCO5CO5_tj
[46]Since the virtual moment of inertia about the x-axis of the finned circle due to a horizontal motion can be shôwn to be
- 12(b-R)3 i/ 3b2+2Rb+3R2)
b l2b
.+
;.
(b+R)3(b-R)2(-+sin )] [47]where A42 is the appropriate tensor element in the general expression of the virtual inertia tensor (see Landweber nd YÌh (lo)), Eq. [47] may be
written as
-dL D r
;z=t-
LA42v0. [48]which shows that the moment on the bòdy is'equal to the rate of change of the ¿ngular momentum of the fluid. In this particular case., the spatial nonuniformity does not hsve any effect on the' moment because of the fact that 'the moment is contribütéd by the fòrce on the fih alone, where the convergence effect along the y-direction is zero.
N-543 18
-Conclusions
The results obtained above have demontrated the successful application of slender-body theory to the evaluation of the forces
and
moments acting on a submerged body moving under waves. The extension of slender-body theory to take account of the spatial non-uniformity of the wave orbital
velocities leads to results' for a body' of revolution
that òheck with those of
other investigations, which were obtained by
different and more.jnvolved methods Complicated cross-sections of
interest,
such as body-appendage combinations, can also be treated
by the same technique and three cases are evaluated. All of the results
can be inter-preted in terms of virtual masses and inertias, and reduce
to Taylor's results in pure two-dimensional flows.
Although it has not yet been
demonstrated that this simple
interpretation is also true' in the general
case of an arbitrary body, the téchnique offers a great simplification over the existing methods because of
the two-dimensional nature of the slender-body theory,
N-543 19