FORCE AND MOMENT ON A SLENDER BODY OF REVOLUTION MOVING IN WATER OF FINITE DEPTH by William R. McCreight B.S., Webb Institute of Naval Architecture (1967) SUBMITTED INPARTIAL FULFILLMENT OF THE REQUIREMENTS FOR THE DEGREE OF MASTER OF SCIENCE at the MASSACHUSETTS INSTITUTE OF TECHNOLOGY June 1970 Signature of Author .................................................... Department of Naval Architecture and Marine Engineering, June 1970 Certified by ............ . ... .. u.. .. .......... ... .. ....... Thesis Supervisor Accepted by ......... , hairman, Departmental Committee on Graduate Students Archives JAN 2N 1i71 ,trap'a T Nau XTziý 1 - ii - FORCE AND MOMENT ON A SLENDER BODY OF REVOLUTION MOVING IN WATER OF FINITE DEPTH by William R. McCreight Submitted to the Department of Naval Architecture and Marine Engineering on June 3, 1970 in partial fulfillment of the requirement for the degree of Master of Science. ABSTRACT A consistent first-order theory is derived for the heave force and pitching moment on an arbitrary slender body of revolution moving horizontally with constant velocity in water of finite depth. A computer program is given for evaluating the resulting expression. Numerical results obtained using this program are presented and compared with previous theory and with published experimental results for the case of a Rankine ovoid. Thesis Supervisor: Title: John Nicholas Newman Associate Professor of Naval Architecture - iii - ACKNOWLEDGMENTS The author is indebted to his advisor, Professor J. Nicholas Newman, for his advice and encouragement throughout the course of this thesis. Thanks are due to Miss J. A. Davis for her excellent typing. All computations were performed at the Computation Center of the Massachusetts Institute of Technology. - iv - TABLE OF CONTENTS Page 1. INTRODUCTION 1 2. FORMULATION OF THE PROBLEM FOR THE POTENTIAL 3 3. SOLUTION FOR THE POTENTIAL 8 4. APPROXIMATE FAR-FIELD SOLUTION USING GREEN'S THEOREM 16 5. FORCE AND MOMENT 24 6. NUMERICAL RESULTS 30 7. CONCLUSION 4o 8. REFERENCES 41 APPENDIX: PROGRAM LISTING - V - LIST OF FIGURES AND TABLES Figures Page 1 The Coordinate System and Flow Geometry 2 The Surface 3 Shape of Rankine Ovoid Used in Calculations 32 4 Heave Force on Rankine Ovoid at 0.144L Submergence 33 5 Pitching Moment on Rankine Ovoid at 0.144L Submergence 34 6 Heave Force on Rankine Ovoid at 0.266L Submergence 35 7 Pitching Moment on Rankine Ovoid at 0.266L Submergence 36 8 Heave Force on Rankine Ovoid as a Function of Submergence and Depth of Water 37 Pitching Moment on Rankine Ovoid as a Function of Submergence and Depth of Water 38 9 S for Applying Green's Theorem Tables 1 EFFECT OF SUBMERGENCE AND DEPTH OF WATER ON FORCE AND D MDMENT ON A RANKINE 4 17 1. INTRODUCTION When a submerged body moves horizontally near a free surface, the body experiences a vertical force and a pitching moment due to the presence of the free surface. If the water is shallow, there will also be a force and moment due to the presence of the bottom. In addition, in this case the free surface waves, and hence the force and moment due to the presence of the free surface, will be altered. The magnitude and sign of the force and moment will depend in a complicated manner on the geometry, location and Froude number of the body, and on the depth of water. In order to obtain a tractable problem, some simplifying assumptions must be made. The flow is considered to be inviscid, incompressible, homogeneous, and irrotational. The analysis is carried out for a slender body of revolution, which can be represented by a line distribution of sources along the body axis, as is usual for a slender body, and a similar distribution of vertical dipoles to correct for the crossflow induced by the presence of the free surface and bottom. Although the source distribution is of lower order than the dipole distribution, both result in contributions to the moment of equal order. The expression for the potential is also obtained directly for the far field by applying Green's theorem, which justifies the assumed form of the potential. Numerical results are presented for the case of a Rankine ovoid to demonstrate the effect of depth of submergence, depth of water, and Froude number. These results are compared with published experimental results for the case of infinite depth of water. - 2 This problem has been studied previously by Havelock [1] for the special case of a prolate spheroid in deep water. He justifies the second (dipole) term in the expression for the moment on order of magnitude grounds and suggests its applicability to other bodies. Pond [2] , who has studied the case of a Rankine ovoid moving in deep water, derives the dipole term by a heuristic argument and justifies its use by comparison with experimental results. The other limiting case has been studied by Newman [3], who calculated the force and moment on a slender body of revolution moving laterally near a wall, but with no free surface. -32. FORMULATION OF THE PROBLEM FOR THE POTENTIAL We assume a slender body of revolution to be moving horizontally with a constant velocity U parallel to its axis at a depth free surface of a body of water of uniform depth h . b Let beneath the Oxyz be a Cartesian coordinate system with the z-axis upward moving with velocity in the direction Ox parallel to the body axis. U The origin is located on the free surface directly above the midpoint of the body axis. This is shown in Figure 1. We nondimensionalize all quantities with respect to body length L , the velocity U , and the fluid density p . With the further assumption of irrotational flow in an inviscid, incompressible, and homogeneous fluid, there exists a potential (u,v,w) that the velocity components such are given by From the continuity equation and the assumption of incompressibility, we obtain Laplace's equation + .. = O (2) On the free surface, which is at an unknown location which is to be found as a part of the solution of the problem, the dynamic boundary condition that the pressure be constant must be satisfied. equation, 2. 2IN7ý1 -P + Thus from Bernoulli's - 4ý z K: Figure 1 The Coordinate System and Flow Geometry -5where C(t) p is the pressure, g is the gravitational acceleration, and is a function of time only, which we may take as identically zero. On the free surface we must also satisfy the kinematic boundary condition, which requires that a particle of fluid on the surface remains on the surface; that is, has the same velocity normal to the surface as the surface itself has. Thus if the free surface is given by we must have D O= (5) Dt on the surface, where D Z D/Dt is the substantial derivative +b a (6) On any solid boundary we require that the velocity be tangent to the surface, or - = O(7) on the surface, where )/An is the derivative normal to the surface. In the case of a horizontal bottom, this is just O 0- on z = -h (8) The fluid velocities must be bounded everywhere in the fluid. Finally, to insure uniqueness of the solution, we must impose a radiation condition at infinity. If the problem were formulated as the limit for large time of an initial value problem, this difficulty would not arise -6(Stoker, [4]). However, it is simpler to avoid the time dependence by solving a steady-state problem with the appropriate additional condition. Thus we require that ahead of the body the motion must vanish, except for the uniform stream, (-LU ,oo ) ± (9) Since we want the potential for a body in a uniform stream, it is natural to write = where $ is the disturbance potential due to the presence of the body. , Twe obtain the problem Then in terms of S• on (10) z = S( - from equations (3) and (5) D•v, on the body surface, Sn (12) for the time-independent case, (13) -7- on z = -h, and the radiation condition (15) )= $ de also require that be bounded at infinity. The bottom condition for h - c is 7k= O (16) The free surface condition (12) is nonlinear and must be evaluated at an unknown location. By expanding the potential in a Taylor series about z = 0 and taking the lowest order terms in 5, we obtain the linearized free surface condition D + WID :0 to be satisfied on the undisturbed free surface and Laitone, [5J). z = 0 (cf. Weyhause The wave height is, to lowest order, and thus we have neglected terms of order condition. (17) 0( 2) in the boundary -83. SOLUTION FOR THE POTENTIAL We now seek an approximate solution to the linearized free surface problem formulated in the preceding section. The solution will be obtained ye first consider a line distribution using a slender-body approximation. of sources of arbitrary strength cO(x) on the body axis over the interval i J/ ((19) 2 wrhere 2 p = O 2(½) = y 2 + (z+b) 2 . Integrating by parts and assuming c(-) = [8], , we obtain, as in Newman (20) Then, with the body shape defined by here the parameter slenderness 4here the slenderness parameter is defined as the ratio of the maximum(21) is defined as the ratio of the maximum -9p = O(C) radius to the body length, the limit of (20) for is (22) -2c (/) 47 P - o (Cer) On the body surface we must satisfy the boundary condition (13), which can be written S---where ao( denotes the derivative normal to the curve the plane x = constant (23) plrX. r = R(x) in The normal derivative of (22) is IL :B- z 2(z - ) (24) 2o Since 0:) o = O(e) , the second term is 0(d/E ) , while the first is Thus the source strength is found from (23) and (24) to be C:-64)where .Oi(E (25) 24Q(5L L4 Tra/?( S(x) =yR 2 (x) is the nondimensional sectional area of the body, and the body boundary condition is satisfied to O(c-) . We see from (25) that there are certain restrictions on the geometry of the body near - 10 - the ends if the assumption of d(--) that the derivative of S(x) =c(½) = 0 is to be correct; namely, must disappear at the ends. If F is the distance from the end of the body and for small , then and thus we must have below that we must have c,> for S = 0 S' = 0 at the end. at the ends of the body. It will be shown Tuck [7] presents a detailed discussion of this point. The boundary conditions (14) and (17) on the bottom and the free surface are not satisfied. By using the source-like Green's function which satisfies these conditions instead of the free-space Green's function, these conditions will be met, but only at the expense of introducing an additional error in the body boundary condition. The required Green's functions satisfy ,0OK) "G-____ % = (> (26) - 11 as appropriate, and the radiation condition + -a CO 17.",,OZ, I/.z (27) The required Green's functions are given by Wehausen and Laitone, [5]. For finite depth GYF I S0 -TTT zC cw cOjt( 2 4A ) [CAeAJ3f~) (I ~f Lc~e~ V(:O< U(IX7 T) 10 O -ITI'2 -aR e IH+ Co42O 0zý, where and PV k o [,o(-x) LLB~t Vj -P)l 2/) ~P~R.-~a~c~R-hec co · 91.1401 CU4 v) - ý(4 FI(I ) (28) (L eI Ac~t ^ z2R COIC-oc EAo (40•) 4re] de denotes the principle value, is the real positive root of a ee( ts- a e :=O/ (29) - 12 - 2.j= CA/U2ý1 a.Y~cr..o3Siz7IF O6, where oC = O 1P -r1 > In the case of water of infinite depth, the Green's function is +±LH r ro P F,~7KY TT _~~-r/2 C"O Eý (I -i) (/X C4S) , A11j +': 4.prO1 4( c~IL/-lA:~ 4~ j (30) where t-2 - ý(7_ý (-,-1 + The functions H 4~-s2· ~+) -- MZd r~~l=~ (t- S are the part of the Green's function which are analytic in the fluid domain and which must be added to the free-space Green's function 1/r to satisfy the boundary conditions on the free surface and the bottom. Using the Green's function above, the potential can be written ( Y-) J = I,, +I, ~~ J 3/ 0,)-b) J - 13 - ) H('6, + c7- (31) The error in meeting the boundary condition on the body is now OQ(6) O(621,Q)= + (32) This error is of lower order than the error in the free surface condition, which is 0(02 ) = 0(6 ) . It will be shown in section 5 that this error leads to an error in the pitching moment which is of the same order as the leading term in the moment obtained using the potential (19). The error in the heave force is of higher order. To obtain the next term in the potential, we consider a line distribution of vertical dipoles of arbitrary strength axis over the interval -1 x < .j(x) on the body . 2 (33) aS L13~'/-~at PV~l/X- 4 Zpi-) ~e 2 P2pljd '2 - - 14 4(-) by the procedure used above, for tan -l z+b!y . In terms of I12 and = 4() I2 = 0 , where , the condition (13) becomes -"- + (34) since (23) is satisfied using series in y and Ill as . Expanding 112 in a Taylor z about the body axis and taking account of transverse symmetry, we obtain (35) Now (36) p2 Thus (37) It is seen that we have assumed result. to order S(-) = S(-½) = 0 in deriving this Since from (35) the boundary condition on the body is satisfied 0(/6 E ) = O( E) , there is no inconsistency in including a term O(6 ) in the potential. also O( C ) , we may use just the free-space dipole Green's function. Since the error in the free surface is - 15 - The error in force and moment resulting from neglecting the free surface condition for the dipole distribution will be shown to be of higher order. In the usual slender-body approach (Tuck, [7]), it is necessary to find an inner expansion for the potential and match the outer limit of this solution with the inner limit of the outer solution, which is the line singularity distribution. We have been able to avoid this because of the particularly simple form of the boundary condition to be met on a body of revolution, and hence have been able to use the inner limit of the outer solution to satisfy the boundary condition directly. - 16 4. APPROXIMATE FAR-FIELD SOLUTION USING GREEN'S THEOREM The results obtained in the preceding section can be obtained, in the far-field, by applying Green's theorem. This more direct approach, in which it is not necessary to assume a form of the solution a priori, is of considerable interest. It is necessary only to apply the slender-body assumption in the approximate evaluation of the surface integral in Green's theorem, which is an exact result. Green's theorem has been used to find the near-field potential in various slender-body problems involving a free surface by Vossers [81, Newman [61, [9J, If S and Joosen [10]. is a surface enclosing a volume V in which the disturbance potential satisfies Laplace's equation (11), then the potential inside V is given in terms of the values of the potential and its normal derivative on the surface S by 5 where ;/~n (38) denotes the inward normal derivative, and function given in the preceding section. body surface SS , the free surface vertical cylindrical surface SR , the bottom SFS of radius The surface is is the Green's We take as the surface surrounding the body, and a tube connecting down to a vanishing line. G R SS S the , and a SB centered at the origin and SFS which we shrink shown in Figure 2. - 17 - U Figure 2 The Surface S for Applying Green's Theorem - 18The integral over (14). S3 is zero due to the bottom boundary condition On the free surface (39) where the integral is taken around the intersection of In the limit as R - c , this integral is zero since both satisfy the radiation condition. the surface SR SFS and • and SR G For the same reason the integral over also vanishes in *the limit R- with the integral over the surface of the body. , and we are left Thus we want to solve the integral equation (4o) c •3) [, -Vd, -d We will find an approximate solution valid in the far-field for small values of the slenderness parameter E . We split the integral into two parts where A ds (42) - 19 - and I J,= 21T I:Lpm '3ZVI%~ - 4Tw Ln (43) jej From the body boundary condition (23), we have -6Y1 D& In the integral and I" about 31 J1 f = 0 " r/ we expand and /Y-V, ,-z a" -It 0(3) G(x,y,z;g,j,C) (44) in a Taylor series in C = -b and obtain -[_ , 6) ,; j (45) CE O?;I ,;D C-E~t ; RMli Since R is constant on a body of revolution for 66: 0 4)qb T constant, the second and third terms integrate out, and we have the result (1(46) This potential, a distribution of sources on the axis proportional to the derivatives of the sectional area curve, is the usual result of slenderbody theory (Tuck, [7]). Since in the above, we have expanded the 1/r - 20 - term in a Taylor series, these results are valid only for small It S(E) is sometimes more convenient to have the integral in terms of . Thus, integrating by parts, we obtain I J-1(/,-) = S~r) (/X7 C), ) dl iY 2 This represents an axial distribution of doublets (cf. Batchelor, [11]). We now consider the integral , equation (43). J2 Using Jl for in this integral, we see that O(e J'> O (3) =C2 and thus we need use only the order term of surface S J2 . Jl term of (48) to evaluate the lowest Since Green's theorem for a point (x,y,z) on the is (49) -C C)T we must take 2J; ~, (50) in the evaluation of equation (43). and J12 function. , corresponding to the Then we write J2 2 We divide 1/r and as the sum of H J into two parts, Jll terms of the Green's J21 21. and J22 22 corresponding - 21 - to Ill and 112 respectively. Thus ( 51 Then aL J.aL c DcTG&J 4 D33 4 (52) - Expanding these derivatives in Taylor series about = O, 01 = -b , w obtain (53) Glrx~rr;i~t;S Jll is a function of x 4 and -b)] p sn? de Br +O0(64 only. Hence it is a constant on each section on a body of revolution, and the first two terms in integrate to zero leaving J21 J11 = O(E4) Finally, we consider e -2 2n (54) - 22 - Expanding 112 and AG/ýn in a Taylor series about the body axis, we have (25 (55) 1-3 44 C(oczr;l~,q-b m;ej Then integrating and noting 12 = 0 -- + (6i R(nYd~d due to transverse symmetry of the H-term of the Green's function, we obtain the result 2 21 Since J12 = 0(C2) discarding terms also. (56) O( , we have J = 0( ) . Because we have been 4) all along, to be consistent we should drop However, it will be shown in the next section that J22 J22 leads to a contribution to the moment of leading order, while the discarded terms will lead to higher order force and moment terms. The part of J22 due to the H-term of the Green's function in equation (42) also leads to a higher order force and moment and hence need not be included. In addition, in the previous section it was shown that in the near-field the - 23 dipole term is needed to satisfy the boundary condition on the body to the same order as the free surface condition. - 24 5. FORCE AND MOMENT The force and moment on the body may be calculated by several methods. We shall simply integrate the pressure over the body. The vertical force and pitching moment are given by (57) where n is the outward unit normal on the body. For a slender body of revolution whose shape is defined by (21), e . 0 (C) rl, = 4-3 0) 40,+OC where e S2Tr _ F,•, is defined as above. f) MA; - Thus the integral can be written 0ki ,) •( +- + 0 (6 ,.) • (58) 2 · i) + kc 001 0 &ý C) r = O(C) since on the body. - 25 From Bernoulli's equation the pressure is <)Pg )7~ The pgz - P 2 (59) term yields the hydrostatic force and moment 8 F6 V,-/0o where * buoyancy. ,-(n -P I- is the body volume, and (60) x o is the x-coordinate of the center of We will neglect this hydrostatic force and moment in the follow- ing. In terms of the disturbance potential -p·-P ý , the pressure is 2 22 I -/y+., 2U CUZ Oý4 (61) ýA The U2 term isa constant and hence isintegrated out. The terms /y, and y 2 z are higher order and will be neglected. 2, Thus the dynamic pressure to order is SPUT~l 4 ~ (62) The disturbance potential near the body has been found to be -VI Z. -) 2- :5- 47 I'~cr)Wr··,L·,b;i46)~I L (63) 4 -2,( I-~O (E - 26 where now 2 r respectively. = y 2 2. and 0J and are given by (25) and (37) Then (/9(c,A:;1,2 t + (z+b) 2 -2 3 a~L~x) a~c ',,:e(f c'(t D2 H(/?ý d~cC(~19-b; (64) r (1) 4;, o,-~lq-) r On a body of revolution, the first and second terms of (64) are functions of x only and hence integrate out. _~( -P•~ ( I, The third term yields VGc) A ekt dLWJ, (65) -6 '44-_ J2 S jý-a3 H(/x, 2.3 2. J,,-bd~x The contribution to the moment from this term is 5 D o0 2 (66) _ -_ 4p 51~~3 ·r 5-i~~3 I -l5V)~o) -r~ ~~-) - 27 - From the last term of , we have the force contribution x 22·n (67) according to the assumptions made in the derivation in section 3. The corresponding contribution to the moment is 222 These expressions are all . O( C) lead to force and moment terms O( The 5) 2 and , and higher. terms resulting from the dipole distribution are z terms in (61) The free surface 0(4 ) and clearly will result in higher order contributions to the force and moment and hence can be neglected. Combining (66) and (68), we have the result I C r-r I _ (69) It is of some interest to obtain these results by applying Lagally's theorem (Cummins, [12j). The force on a source is equal to -4 Treco" , - 28 where c et is is the flow velocity due to external singularities, and the source strength. the moment is given by To lowest order, the force on a dipole is zero, and -4vrpcp , where now c is the external flow velocity component normal to the dipole.axis, in this case the stream velocity U , to lowest order, and p is the dipole strength. The "Lagally" force and moment on the source distribution are easily found to be, to lowest order, I 0 (70) MSL2w~ma~ Z-a ldd Similarly, the force and moment due to the dipole distribution are FDL- O The expressions for the force are the same as obtained by integrating the linearized pressure, (65) and (67), but the moments due to the source and dipole distributions are not those obtained previously. ML = MS + MDL However, the sum - 29 - is that given by (69) and thus the final results are identical. This discrepancy in the intermediate results for the moment is a direct consequence of the fact that the source distribution (19) alone does not satisfy the body boundary condition. In the first calculation we found the force and moment on the surface which was to be represented by the source distribution, while the application of Lagally's theorem has given the force and moment acting on the surface which is actually represented by the source distribution, which clearly is significantly different from what is wanted. Similarly, the integral of the pressure over the intended body surface gives the contribution to the moment due to the dipoles, while the Lagally moment on the dipoles does not correspond to the moment on any given body, since a line distribution of vertical dipoles in a uniform horizontal stream by itself does not by itself represent a body, but rather represents the effect of a correction to the shape of the body represented by the source distribution. - 30 6. NUMERICAL RESULTS A program has been written to evaluate the expressions for the force and moment on a body of revolution moving horizontally in water of finite depth, equations (65) and (69). The program is listed in the appendix. Figures 4, 5, 6, and 7 show the force and moment on a Rankine ovoid of length-diameter ratio 10.5 for two different submergences in infinitely deep water, along with the experimental results obtained by KorvinKroukovsky, et al., [13] for comparison. The shape of the body is shown in Figure 3. The agreement between calculated and measured results for the moment is very good. The agreement for the force is not as good. Figures 5 and 7 also show the results of computations by Pond [2ý who used the exact uniform flow potential (a source and a sink) instead of the source distribution obtained by using the slender-body approximation. The dipole terms were calculated in the same manner as was used above, based on a heuristic argument. Both the moment on the source-sink combination alone, calculated by Lagally's theorem (labeled "Pond's First Result"), and the moment on the source, sink, and dipoles are given. It is clear from these curves that the source potential alone is insufficient from a practical point of view. The calculations using equation (69) agree very closely with Pond's results in spite of the difference in the source potential and the bluntness of the body. Figures 8 and 9 and Table 1 present the results of calculations for Froude number 0.55, depth of submergence varying from 0.144L to 2.5L, and depth of water varying from 0.5L to infinite depth. It is clear that for a body near the surface the effect of the bottom is not felt if the water - 31 is deeper than about two body lengths. Furthermore, from Table 1 it is clear that if the body submergence is more than about one or two body lengths the force and moment due to the free surface are very small, unless the body is close to the bottom, in which case the force and moment are due to the wall effect of the bottom. - 32 - Surface of water corresponding to submergence b = 0.266L Surface of water corresponding to submergence b = 0.144L Ir max -I- T r- Only one quarter of body is shown length/diameter = 10.5 Figure 3 Shape of Rankine Ovoid used in Calculations - 33 - 1.0 0.0 0 (C -2.0 00 S-3.0 0 -4.0 -5.0 0.2 0.3 0.4 Froude Number F Figure 4 0.6 0.5 0.7 V/1 Heave Force on Rankine Ovoid at 0.144L Submergence - 34 - / / /l 3.0 2.0 0 V 1.0 N // 4•- K I I 0.0 C-H 0l II 0, -1.0 Program (equation 69) - Model test results (Korvin-Kroukovsky, et. al. 131) Pond's first result -2.0 (Pond [21) "" Pond's second result 0.3 I· I· 0.4 0.5 (Pond [2J) I· 0.6 1 0.7 Froude Number Fn = Vi1L Figure 5 Pitching Moment on Rankine Ovoid at 0.144L Submergence - 35 - 2. 31) 1. IN> 0. 4cA . O C-2. 0II -3. 0.3 o.4 0.5 o.6 0.7 Froude Number F n = V/ n Figure 6 Heave Force on Rankine Ovoid at 0.266L Submergence - 36 - Program (equation 69) Model test results (Korvin-Kroukovsky, et. al. [131) O M 1.0 c4 0.0 II E* el2 -2.0 O -p -3.0 0.2 0.3 0.4 0.5 0.6 Froude Number Fn = V/! Figure 7 Pitching Moment on Rankine Ovoid at 0.266L Submergence - 37 - -tO -3.0 r. .rCU b = 0.144 a, o 0 .r -2.0 L. II 4, r4 0 b = 0.266 1.0 k- b = 0.500 0.0 0.0 1.0 2.0 3.0 4.o Depth of water/body length Froude Number = 0.55 Figure 8 Heave Force on Rankine Ovoid as a Function of Submergence and Depth of Fluid - 38 - b = 0. 144 3.0 O 2.0 b = 0.266 0a, o 4- 1.0 E b = 0.500 0 0.0 0.0 I 1.0 2.0 Depth of water 3.0 4.o / Body length Froude Number = 0.55 Figure 9 Pitching Moment on Rankine Ovoid as a function of Submergence and Depth of Water - 39 - TABLE 1. EFFECT OF SUBMERGENCE AND DEPTH OF WATER ON FORCE AND MOMENT ON RANKINE OVOID Froude Number = 0.55 Submergence 1.OL Depth of Water Force Coefficient Moment Coefficient 2.OL - 1.22 x 106 5.11 x 108 3.OL - 2.59 x 10-6 3.86 x 10-7 - 2.86 x 10- 6 4.10 x 10-7 Deep Water 1.5L 9.48 x 10o 3.0 - 1.29 x 10- 7 Deep dater 2.OL 2.5L -6b 2.0 3.0 -7 - 4.67 x 10 -7 9.54 x 10-7 Deep dater 3.0 - 1.26 x 10 - 7 9.65 x 10 - 6 Deep dater - 4.72 x 10 - 8 - 3.97 x 106 - 6.24 x lO-8 1.20 x 10 -- 8 - 3.47 x 10 - 7 3.76 x 10-10 - 3.98 x 10 1.22 x 10- 11 - 40 7. CONCLUSION The theory of Havelock and Pond for the force and moment on a body of revolution moving under a free surface has been shown to be a consistent first-order theory, while theories derived ignoring the effect of the body generated waves on the flow near the body are not. The theory has been extended to the case of an arbitrary slender body of revolution and to include the effect of finite depth of water. This more general theory compares very well with the theory of Pond and with experimental results for the special case of a Rankine ovoid in infinite depth water. - 41 8. 1 REFERENCES HAVELOCK, T. H., Quart. Journ. Mech. and Applied Math., Vol. V, pt. 2 (1952). 2 POND, H. L., Journal of Ship Research, Vol. 2, No. 4 (1959). 3 NEWMAN, J. N., David Taylor Model Basin Report 2127 (1965). 4 STOKER, J. J., Comm. Pure and Appl. Math. IX, pp. 577-595 (1965). 5 WEHAUSEN, J. V., and E. V. LAITONE, "Surface Waves", Vol. IX, Part III of Handbook of Physics, S. Flugge, Ed., Berlin, Springer-Verlag (1960). 6 NEWMAN, J. N., J. Fluid Mech., Vol. 18, pt. 4, pp. 602-618 (1964). 7 TUCK, E. 0., "The Steady Motion of a Slender Ship", Ph.D. Thesis, Cambridge (1963). 8 VOSSERS, G., "Some Applications of the Slender Body Theory in Ship Hydrodynamics", Thesis, Delft (1962). 9 NEWMAN, J. N., "Lectures on the Theory of Slender Ships", Berkeley, California (1963). 10 JOOSEN, W., "Oscillating Slender Ships at Forward Speed", Publication 268, Netherlands Ship Model Basin, Wageningen, Holland. 11 BATCHELOR, G. K., An Introduction to Fluid Dynamics, Cambridge (1967). 12 CUMMINS, W., Journal of Ship Research, Vol. 1, No. 1, pp. 7-18 (1957). 13 KORVIN-KROUKOVSKY, B. V., F. R. CHABROW, P. M. BELOUS, and W. H. SUTHERLAND, "Theoretical and Experimental Investigation of the Interaction of a Free Fluid Surface and a Body of Revolution Moving under It', Experimental Towing Tank, Stevens Institute of Technology, Report 390 (1950). - 42 - APPENDIX PROGRAM LISTING - 43 - A-4P- P-4 ZZZ V-4 P-4 P--0-4 . NNNN o N NN ZZZZZZZZZZZZZ ZZ - 0Ev -0 ON N * II < tJ -j a1 CI -0 '4CIL u O - E- -E EX - - 44 - a, o P-4 m %r un ZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZZ N %0 *__ -W CV_- N4 M * ýC f- W C %, 0 SW 4 v- N M - -t 1- f- M r--4 - C' Z U. o t S4 % w v0. 0. 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