Pergamon
Printed in Great B r i t a i n 0029-8018/94 $7.00 + .00THE CROSS-FLOW DRAG ON A MANOEUVRING SHIP
J . P . H O O F T
M A R I N , Wageningen, The Netherlands
Abstract—In this paper, an analysis is given of the experimentally derived local lateral force on a manoeuvring ship as a reaction to the ship's lateral velocity. The tests were performed with models consisting of several segments. Special attention is paid to the longitudinal distribution of the non-linear component of the lateral force, the so-called cross-flow drag. This aspect is of utmost importance when the non-hnear contribution becomes dominant as will occur in a tight turn during which the ship's drift velocity becomes relatively large compared to the ahead speed.
N O M E N C L A T U R E
AP aft perpendicular C, lift coefficient
drag coefficient
C^j corrected drag coefficient
Fn Froude number = U/(g*Lpp)°-^ FP forward perpendicular
G ship's center of gravity g acceleration due to gravity
L lift on the ship = force perpendicular to the resultant speed U of the ship Lpp ship's length
/„ length of the nth segment
niy added mass in lateral direction per unit length r ship's rate of turning
T ship's draught
t„ draught of the nth segment
ll ship's speed component in the longitudinal direction U resultant speed of ship = ^M^ + v^)°-^
V ship's speed component in the lateral direction
X longitudinal direction in the ship fixed system of coordinates
x^ longitudinal direction in the Earth fixed system of coordinates lateral direction in the Earth fixed system of coordinates Y lateral force to the ship
yawing moment around G
N„ yawing moment around the midship section (3 drift angle = atn(v/M)
p mass density of the water.
1. I N T R O D U C T I O N
FOR T H E prediction of the ship's manoeuvrabiUty, use l:an be made of computer simulations. For this approach mathematical models must be available by which the relevant hydrodynamic forces o n the manoeuvring ship are described.
O f t e n these mathematical descriptions of the hydrodynamic phenomena have been derived f r o m a regression analysis of the results of captive m o d e l tests f o r the ship considered [see H o o f t (1986)]. H o w e v e r , such mathematical descriptions are not always
330 J . P. HOOFT
satisfactory because of tlie lack of a pliysical meaning of the descriptions. This imperfec-tion may lead to the f o l l o w i n g problems:
• The impossibility of comparing the hydrodynamic coefficients of two different ships. This problem may be serious when designing the ship f o r o p t i m u m manoeuvrability. • A l i m i t e d accuracy of the .manoeuvring predictions because of the fact that the
simulation results w i l l depend on the accuracy by which the coefficients have been derived by the regression analysis.
For the prediction o f the ship's manoeuvrability i n the initial design stage, no model test results are usually available f o r the determination o f the hydrodynamic coefficients. One can then use computer simulations only i f the hydrodynamic coefficients can be established otherwise.
Nowadays i t is not yet possible to determine the hydrodynamic manoeuvring coef-ficients by means of theoretical methods. Therefore, empirical methods have been developed by means o f which, i n the initial design stage, the hydrodynamic coefficients can be estimated as a f u n c t i o n of the ship's main dimensions; see, f o r example, Inoue
et al. (1981) and K i j i m a et al. (1990).
I n empirical methods the hnear hydrodynamic coefficients are described rather accu-rately as a f u n c t i o n o f only a f e w aspects of the ship's dimensions. T w o reasons can be given f o r the achieved accuracy:
1. The linear hydrodynamic coefficients are most likely rather independent of local parameters o f the ship's hull f o r m (at the bow and/or the stern).
2. For a wide range of ships the linear hydrodynamic coefficients have been determined experimentally. This means that an acceptable level o f confidence has been achieved in the description o f the coefficients as a f u n c t i o n of the ship's main parameters. I t appears that the non-hnear contribution of the hydrodynamic characteristics can be estimated only roughly by empirical methods. This is very inconvenient when tight turns have t o be predicted by means o f computer simulations. I n such manoeuvres the non-linear contributions play a significant role. Three reasons are mostly given f o r this unfavourable aspect:
1. The non-Hnear hydrodynamic coefficients are rather sensitive to the local f o r m parameters of the ship. This means that much more i n f o r m a t i o n (data) is required as a f u n c t i o n of the larger number o f parameters.
2. O n l y f o r a limited number of ships have non-hnear hydrodynamic coefficients been determined experimentally. This means that only a l i m i t e d level of confidence has been achieved i n the description of the coefficients as a f u n c t i o n of the ship's main parameters.
3. O f t e n only the hydrodynamic coefficients have been pubhshed w i t h o u t the actual model test results. Some of the authors use quadratic non-linear coefficients, while others apply tertiary non-linear coefficients. I n this way the validity o f a presented non-linear coefficient is hmited and cannot be compared w i t h the corresponding coefficient f o r another hull f o r m .
I t was thought that a better description of the non-linear component of the lateral force could be achieved i f one could establish the local non-linear force component
instead o f tlie total force on the ship. This local component was defined by the local cross-flow drag coefficient; see, f o r example. H o o f t (1987).
Burcher (1972), Clarke (1972), Matsumoto (1983) and Beukelman (1988) have presented the results of their experiments w i t h segmented models. F r o m these tests the lateral forces o n each of the segments can be derived. I n the present paper a description is given of the analysis of test results w i t h segmented models. Based o n this analysis an empirical method can be derived to estimate the distribution o f the non-linear lateral force component over the ship's length. The intention of this method is:
1. T o achieve a more accurate prediction of the non-linear component o f the lateral force.
2. T o realize a more accurate mathematical description of the hydrodynamic forces f r o m measurements on the t o t a l model.
3. T o estabhsh eventually a simulation program that is capable of predicting the ship's manoeuvrability w i t h sufficient accuracy. Such a manoeuvring prediction method would provide a means to investigate the effect o f the variations o f the ship's h u l l f o r m o n its manoeuvrability.
2. T H E V A R I A T I O N O F T H E L A T E R A L V E L O C I T Y O V E R T H E L E N G T H O F
While considering the ship's manoeuvring performance, three velocity components can be discerned at each instant (see Fig. 1):
• u, the ahead velocity of the centre of gravity G
• V, the lateral velocity o f the centre of gravity
• r, the rate o f turning around the vertical axis.
The combination of d r i f t velocity v and yaw rate r leads to a local lateral velocity v(x) that varies over the length of the ship:
When considering a t u r n by a port (positive) rudder angle then i t is seen that the ship w i n t u r n to port (negative r) at a positive d r i f t velocity v. I n this t u r n the local
T H E S H I P
v(x) = V + x*r . (1)
xe
yet
332 J . P. HOOFT
d r i f t velocity becomes zero (the turning p o i n t ) somewhere near the bow of the ship
(x>0), while at the stern the lateral velocity wiU become quite large relative to the
ship's ahead speed. A s a consequence of this resuh i t is f o u n d that, i n general, the lateral hydrodynamic reaction force:at the bow w i l l be small, while at the stern quite a large force w i h be experienced.
3. T H E L A T E R A L F O R C E AS A R E A C T I O N T O T H E D R I F T V E L O C I T Y W h e n considering first the lateral hydrodynamic force on the ship as a reaction to the ship's d r i f t velocity v only (at zero rate of t u r n i n g ) , the foUowing description is o f t e n applied:
Y(v) = Y^^*u*v + Y^^*v*/v/ (2)
or, i n a non-dimensional f o r m :
Y O ) ' = y ^ * c o s ( p ) * s i n O ) + y^p*sin((3)*/sin((3)/ (3) i n which the lateral force has been made non-dimensional by dividing by 0.5p Lpp^U'^
or 0.5p LppTU^ w i t h the total velocity U defined by:
The d r i f t angle |3 is defined by:
(3 = a r c t a n ( v / w ) . (5) The total lateral force Y{v) is the resuhant of all lateral forces y „ ( v ) o n each of the
segments i n which the ship model has been subdivided:
Y{v) = E Yniv) (6) while the total yawing moment around the center of gravity amounts to:
N{v)^J,{x^*Y^{v)). (7)
For f u r t h e r analysis the local lateral force on each segment is w r i t t e n i n a non-dimensional f o r m according to:
F „ ( P ) ' = y „ ( v ) / ( 0 . 5 p / A f / " ) (8) w i t h /„ the length of the segment and t„ hs average draught; see, f o r example, Fig. 2.
According to Equation ( 3 ) one now describes the non-dimensional local lateral force Yni^y by means of a hnear coefficient Cy„ and a non-linear coefficient Cdn.
y „ ( p ) ' = C y „ * s i n O ) * c o s ( p ) - C r f „ * s i n ( p ) * / s i n ( ( 3 ) / (9) i n which the hnear coefficient Cy^ corresponds to the derivative Y'„^ and the drag
coefficient Crf„ corresponds to - Y n p p .
I t can be shown that i n E q u a t i o n (2) the linear term is linearly dependent on the longhudinal velocity component u and not o n the total velocity U. This means that f o r zero f o r w a r d speed {u = 0) no linear contribution i n the lateral force exists. This
Todd 7 0 m o d e l ; Lpp/T = 17 .5; z e r o t r i m . 5 t h segment f r o m t h e bow; Fn = 0 . 15. 0 0 2 - + • } • 0 0 1 -0 1 - -t-0 • ] 1 \ 5 1 0 2 0 0 0 1 • 0 . 0 2 - +
FIG. 2. Example of the measured lateral force on a segment as a function of the drift angle (3; obtained from Beukelman (1988).
holds not only f o r the lateral force on the total ship but also f o r the local lateral force on each of the segments o f a ship model.
I f one considers the l i f t L to be a lateral force that is perpendicular to the total undisturbed incoming flow U, then the coefficient Cy„ is related to the local l i f t coefficient Cl^(n) as foUows:
C y „ = - a p ( n ) * c o s O ) . (10) Inserting this result into E q u a t i o n (9) leads to:
y „ ( p ) ' = - a p ( n ) * s i n ( p ) * c o s ( p ) 2 - C4H=sin(p)*/sin((3)/. (11) I n the application of E q u a t i o n (11), use is made of the assumption that the l i f t
coefficient C/p(n) is independent of the d r i f t angle p. This means that i t is accepted that the local cross-flow drag coefficient is a f u n c t i o n of the d r i f t angle p . Various physical arguments can be given to prove this assumption to be correct. I t should be borne i n m i n d that both the l i f t coefficient and the cross-flow drag coefficient vary over the length of the ship.
F r o m the test results o n each segment as presented i n Fig. 2 one determines the local l i f t coefficient Cl^(n) at the range of small d r i f t angles p . W i t h this value of C/p(«) one determines f o r each segment the cross-flow drag coefficient f r o m the measurements at higher d r i f t angles:
r , rn, - - Y n i ^ y - a p ( » ) * c o s ( p ) ^ . s i i > ( p )
"^"""^^^ s i n ( p ) * / s i n ( p ) / ~ • ^^^^ F r o m this equation one finds, i n Table 1, the values of the drag coefficients Cd^ f o r
334 J. P . HOOFT
TABLE 1. EXAMPLE OF THE DERIVATION OF THE CROSS-FLOW DRAG COEFFICIENTS Cd„ FROM THE MEASUREMENTS
Drift angle p (in degrees)
Measured dimensionless latitudinal force Y'^
Drag coefficient Cd^ with C/p (5) = -0.287 4 +0.01478 1.057 8 -H0.01906 1.038 12 -1-0.00806 1.134 16 -0.00398 1.015 20 -0.02001 0.912
Todd 70 model (7 segments); LppIT = 17.5; zero trim; 5th segment from the bow; Fn = 0.15. 4 . T H E L O C A L L I F T C O E F F I C I E N T Cl^{x)
According to Jones (1946), one finds tliat the local l i f t per unit length is determined by the instantaneous apparent acceleration o f the local lateral added mass of water alongside the ship:
Lg = v*w*m^g (13) w i t h THy being the lateral added mass of water per unit length of the ship and ^ being
the distance o f the cross-section f r o m the f o r w a r d perpendicular. I n Equation (13) the derivatives Lg and m^g are defined by:
Lg = éLlAi • ruy^ = dmy/d^ . (14) F r o m integration o f Lg i n Equation (13) one finds that the l i f t force L over a distance
between 4/ and ^„ ( w i t h ^/ being the closest t o the FP) amounts to: p a
L = v * M * my^di = v*u*(my{^,)-my(^f)) (15)
kf
f r o m which i t is seen that i n theory the total l i f t o n the ship w i l l be zero (paradox o f d ' A l e m b e r t ) because of the fact that in an ideal fluid the added mass per unit length
niy is zero at the bow (^/ = 0) as weh as at the stern (^„ = Lpp).
I n Tables 2 and 3 the local l i f t coefficient Cl^(n) on each of the seven segments o f TABLE 2. COMPARISON BETWEEN MEASURED AND CALCULATED LINEAR LATERAL FORCE COMPONENT ( I N A NON-DIMENSIONAL FORM) ON EACH OF THE SEVEN SEGMENTS OF A MODEL OF THE TODD 70 SERIES, NO TRIM, Fn = 0.15;
SEE BEUKELMAN (1988)
Lpp/T = 22.81 Lpp/T = 17.50 Lpp/T = 14.20
Segment No.
Cip Ctp C^ip C^ip C'i.p C'z.p
Segment No. (measured) (calculated) (measured) (calculated) (measured) (calculated)
1 + 1.233 + 1.134 + 1.387 + 1.440 + 1.577 + 1.655 2 +0.301 +0.312 +0.401 +0.370 +0.487 +0.487 3 +0.172 +0.115 +0.186 +0.142 +0.215 +0.176 4 0 -0.009 -0.040 -0.003 0 -0.001 5 -0.199 -0.259 -0.215 -0.299 -0.242 -0.329 6 -0.172 -0.437 -0.287 -0.606 -0.356 -0.722 7 +0.284 -0.944 +0.143 -0.934 +0.072 -1.109
TABLE 3. COMPARISON BETWEEN MEASURED AND CALCULATED LINEAR LATERAL FORCE COMPONENT ( I N A NON-DIMENSIONAL FORM) ON EACH OF THE SEVEN SEGMENTS OF A MODEL OF THE TODD 70 SERIES, LppIT = 17.5,
Fn = 0.15; SEE BEUKELMAN (1988)
Trim = -3.46° Zero trim Trim = + 3.4°
Segment No.
Ci,p Cz,p Cz.p C'ip
Segment No. (measured) (calculated) (measured) (calculated) (measured) (calculated)
1 + 1.577 + 1.730 + 1.387 + 1.440 + 1.090 +1.034 2 +0.158 +0.125 +0.401 +0.370 +0.659 +0.756 3 -0.229 -0.352 +0.186 +0.142 +0.602 +0.680 4 -0.373 -0.559 -0.040 -0.003 +0.502 +0.548 5 -0.573 -0.826 -0.215 -0.299 +0.201 +0.179 6 -0.502 -0.762 -0.287 -0.606 0 -0.324 7 -0.401 -0.742 +0.143 -0.934 +0.244 -1.197
the ship model is given as derived f r o m the experim.ents described by Beukelman (1988). I n these tables the local l i f t coefficients are also presented, derived f r o m E q u a t i o n (15).
F r o m the comparison between the experimental and theoretical values i n Tables 2 and 3 h is seen that the theoretical values f o r the h u l l f o r m considered agree weh w i t h the measurements f o r the five most f o r w a r d segments.
The theory by Jones (1946) f o r determining the local l i f t force can also be checked in another way while applying Equation (15). For this purpose one reduces f r o m the measurements the distribution of m^(^) by a summation of the l i f t derivative L^^{n) over the segments after E q u a t i o n (15) has been rewritten by:
niyiUn)) = my{Un-l)) + L „ , ( n ) (16) w i t h rriy being zero at the f o r w a r d perpendicular.
I n Figs 3 and 4 the experimental values of my are presented as derived by means of Equation (16) using f r o m the model test results presented by Beukelman (1988). I n Figs 3 and 4 the theoretical values of niy are also plotted. F r o m the comparison of the theoretical and experimental values i n these figures it is seen that the theory should be corrected f o r three-dimensional effects on the value o f niy leading to my^.
myXk) = C^{i)*my{i) (17) i n which C^ii) is the correction t e r m as a f u n c t i o n of the longhudinal location. H a v i n g
determined the corrected lateral "added mass" distribution niyj^^) it w i h be possible to determine the corrected derivative
niy^c-niy^M) = niy^Xk) = dmyXi)IAi,. (18) A p p l y i n g the value m^^^ i n E q u a t i o n (15) one now finds .that the t o t a l l i f t o n the ship
amounts to:
L^v*u* my^^d^ = v*u*my^(i = ^^pp). (19) J^FPP
336 J. P . HOOFT calculated measured LPP/T = 22.81 \ LPP/T = 17.50 X LPP/T = 14.20 —, / y
/
/ /
/ /
w
-~ r—7/ /
' /
/
/
/
\ N \ \ \\ v \\
\
/ / / ^ ^ \ 60 20 APP 0.8 0.6 0.4 0.2 FPPFIG. 3. Comparison of the calculated lateral mass niy per unit length with the values derived from the experiments with segmented models for a Todd 70 hull form without trim at ¥n = 0.15; see Beukelman
(1988).
one then finds f o r the t o t a l yawing moment due to the l i f t force distribution over the ship's length:
around the midship section) = v * « * (0. SLpp - Q * my^^dè, Hfpp
calculated measured
LPP/T = 17.50 Tir
1
APP
FIG. 4. Comparison of the calculated lateral mass per unit length with the values derived from the experiments with segmented models for a Todd 70 huU form with Lpp/T = 17.5 at Fn = 0.15; see Beukelman
(1988).
or
f^APP
No = v*u* [-my,(^APp)*Lpp/2 + rriyXO dQ. (20) kppp
338 J. P. HOOFT
5. T H E L O C A L C R O S S - F L O W D R A G C O E F F I C I E N T Cd(^)
A f t e r having determined the l i f t coefficient Cl^{n) on each segment, one then establishes the cross-flow drag coefficient Cd^i3 j o n each segment by means of Equation (12). Some o f the results derived in^this way are presented i n Fig. 5. I n this figure the distribution o f C J „ over the ship length has been plotted f o r various d r i f t angles (3.
The f o l l o w i n g comments on the results i n Fig. 5 can be given:
The cross-flow drag coefficient on the first segment f r o m the bow has most probably been caused by the bow wave. Therefore i t is assumed that this value depends o n the f o r w a r d speed of the ship; see also the findings by Matsumoto (1983).
Aside o f the cross-flow drag coefficient o n the most f o r w a r d segment(s) i t is seen f r o m the resuhs in Fig. 5 that f o r small d r i f t angles (3 the value of Cd w i h increase at larger distances f r o m the bow u n t h some m a x i m u m value is attained after which Cd w i l l decrease a little. A t increasing d r i f t angles p this curve of Cd over the ship's length wih move f o r w a r d .
For large d r i f t angles of approximately 90° the ship sails nearly abeam. I n this condhion the distribution of the cross-flow drag coefficient over the ship's length mainly depends o n the f o r m of the ship's h u h and to a lesser degree on the local Reynolds number. I n Fig. 6 this distribution of Cd is presented f o r a containership and a tanker; the results in this figure f o l l o w f r o m Matsumoto (1983).
The value o f Cd{^) at a given cross-section w i h vary at increasing d r i f t angles f r o m the values shown i n Fig. 5 to the values shown i n Fig. 6.
One now considers the relation between C(i„(p 90°) at an arbitrary d r i f t angle and C(i„(P = 90°) at a d r i f t angle of 90° f o r the various ship types and ship conditions.
For this purpose use is made of the corrected drag coefficient C c J „ f p) which is defined
by:
C 4 P ^ 9 0 )
^^^^^^ ~ C ^ P = 90) ^^^^ leading to the fact that at 90° d r i f t angle the coefficient Ccd equals unity over the
whole length of the ship.
Combining the results i n Figs 5 and 6 according to E q u a t i o n (21) w i h yield the results presented i n Fig. 7. I n Fig. 8 the course o f Ccd over the ship length is sche-matically indicated f o r increasing d r i f t angles.
F r o m the results o f the corrected drag coefficient Ccrf„(p) i n Fig. 7 i t is concluded that this coefficient is stiU dependent o n the longitudinal location and the d r i f t angle, but is no longer dependent on the ship's h u h f o r m .
6 . C O N C L U S I O N S
Experiments have been carried out w i t h segmented models during which the lateral forces on each of the segments were measured. These tests were performed as a f u n c t i o n of the ship's lateral velocity ( i n a towing t a n k ) and as a f u n c t i o n o f the ship's rate of t u r n i n g (under a rotating arm f a c i l i t y ) .
I n this paper the results are presented of the analysis o f the experiments w i t h segmented models as a f u n c t i o n of the ship's lateral velocity. The same k i n d of results were f o u n d by analysing the rotating arm tests as a f u n c t i o n of the ship's rate of turning.
o L P P / T = 22.81 L P P / T = 17.50 L P P / T -= 14.20 1.4' 1.0 Ü 0.6- 0.2- -0.2-APP O . ° « " c <T) > 1 Q O A • A • 0.5 FPP 1.4-1.0 = 12 0,6- 0,2- -0.2-APP ê B D 0 < A ) 0 t a Ï k é UJ a a 0 0 5 FPP 1.4-1.0 0.6- 0.2- -0.2-APP /S = 16° A A m 0 O A D ° * • r A O ) i a • • • fi 0.6 FPP 1.4 |9 = 20 1.0 Ü 0.6- 0.2- -0.2-APP O O a o A O • 0.5 O A FPP
FIG. 5. Distribution of the cross-flow drag coefficient over the ship's length, derived from the experiments with a segmented model for a Todd 7 0 hull form without trim at Fn = 0.15; see Beukelman ( 1 9 8 8 ) .
340 J. P . HOOFT • CONTAWER O TANKER 8 0.8 • O 0 O O 0 0 • 0 D 0 ID n • Q = = = 1 1 APP 0.8 0.6 0.4 0.2 FPP
FIG. 6. Distribution of the cross-flow drag coefficient over the ship's length, derived from the captive drift tests with two segmented model at (3 = 90°; see Matsumoto (1983).
The conclusions obtained i n the present study can be summarized as follows: • Based o n Jones' theory (1946), the distribution of the linear lateral force over the
ship length can be predicted as a f u n c t i o n of the ship's f o r m by means o f empirical formulations.
© A L P P / T = 22.81 L P P / T = 17.50 L P P / T = 14.20 = 8 1.4 1.0 Ü 0.6- 0.2- -0.2-APP • S O J A 0 n o a A • 0.5 = 12° 1.4 1.0 X) 0.2- -0.2-• O s C ) ) 0 • • ê FPP APP 0.6 FPP 1.4 1.0 = 16° O 0.6. 0.2- -0.2-m • . 1 s n A E D APP •O.S FPP 1.4 jg = 20° 1.0 •a O 0.6. 0,2 -0.2-1 APP A O 0.5 •
FIG. 7. Distribution of the corrected cross-flow drag coefficient Ccd over the ship's length, derived from the experiments with a segmented model for a Todd 70 hull form without trim at F« = 0 15- see Beukelman
342 J . P. HOOFT
A P P 0 . 5 F P P
g
FIG. 8. Schematic indication of the forward shift of the distribution of Ccd{£,) at increasing p.
• The distribution of the cross-flow drag coefficient can be predicted f o r a lateral d r i f t i n g ship ( p = 90°) as a f u n c t i o n o f the ship's f o r m parameters by means o f empirical formulations.
• W i t h the knowledge of the drag coefficient f o r 90° d r i f t i n g it is possible to predict the cross-flow drag coefficient f o r any d r i f t angle p as a f u n c t i o n o f the ship's f o r m parameters by means of empirical formulations.
• The results presented i n this paper show that i t is possible to develop a manoeuvring prediction program that is based o n a physical theory rather than on regression. Such a program leads to more accurate predictions o f the ship's manoeuvrabihty because the effects o f local h u l l f o r m parameters are taken i n t o account.
R E F E R E N C E S , BEUKELMAN, W . 1988. Longitudinal distribution of drift forces for a ship model. Technical University of
Delft, Department of Hydronautica, Report No. 810.
BURCHER, R . K . 1972. Developments in ship manoeuvrability. J. R. Inst. nav. Archit. 114, 1-32.
CLARKE, D . 1972. A two-dimensional strip method for surface ship hull derivatives: comparison of theory with experiments on a segmented tanker model. J. mech. Engng Sci. 14, 5 3 - 6 1 .
HOOFT, J. P. 1986. Computer simulations of the behavior of maritime structures. Mar. Technol. 23, 1 3 9 - 1 5 7 . HOOFT, J. P. 1987. Further considerations on mathematical manoeuvring models. RINA International
Confer-ence 'On Ship Manoeuvrability—Prediction and Achievement', London, U.K.
INOUE, S., HIRANO, M . , KUIMA, K . and TAKASHINA, J. 1981. A practical calculation method of ship
manoeuvr-ing motion. Int. Shipbuildmanoeuvr-ing Prog. 28, 2 0 7 - 2 2 2 .
JONES, R . T . 1946. Properties of low-aspect ratio pointed wings at speeds below and above the speed sound. N A C A Report No. 835.
KIJIMA, K . , NAKIRI, Y . , TANAKA, S. and FURUKAWA, Y . 1990. On a numerical simulation for predicting ship
manoeuvring performance. 19th ITTC, Madrid, Spain.
MATSUMOTO, N . and SUEMITSU, K . 1983. Hydrodynamic force acting on a hull in manoeuvring motion. J. Kansai Soc. nav. Archit. 190, 3 5 - 4 4 .