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Twenty-Third Symposium on Naval Hydrodynamics (2001)
Naval Studies Board (NSB)

Page
780
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Page
780
Front Matter (R1-R19)
Modern Seakeeping Computations for Ships (1-45)
Forces, Moment and Wave Pattern for Naval Combatant in Regular Head Waves (46-65)
New Green-Function Method to Predict Wave-Induced Ship Motions and Loads (66-81)
Validation of Time-Domain Prediction of Motion, Sea Load, and Hull Pressure of a Frigate in Regular Waves (82-97)
Ship Motions and Loads in Large Waves (98-111)
Prediction of Vertical-Plane Wave Loading and Ship Responses in High Seas (112-125)
Basic Studies of Water on Deck (126-142)
Second Order Waves Generated by Ship Motions (143-156)
Prediction of Nonlinear Motions of High-Speed Vessels in Oblique Waves (157-170)
Optimizing Turbulence Generation for Controlling Pressure Recovery in Submarine Launchways (171-180)
Hull Design by CAD/CFD Simulation (181-190)
Steady-State Hydrodynamics of High-Speed Vessels with a Transom Stern (191-205)
Practical CFD Applications to Design of a Wave Cancellation Multihull Ship (206-222)
Simulation of Ship Maneuvers Using Recursive Neural Networks (223-242)
Flow- and Wave-Field Optimization of Surface Combatants Using CFD-Based Optimization Methods (243-261)
Marine Propulsor Noise Investigations in the Hydroacoustic Water Tunnel 'G.T.H.' (262-283)
Propulsor Design Using Clebsch Formulation (284-300)
Unsteady Flow Quantities on Two-Dimensional Foils: Experimental and Numerical Results (301-313)
Hydrofoil Turbulent Boundary Layer Separation at High Reynolds Numbers (314-329)
Pressure Fluctuation on Finite Flat Plate Above Wing in Sinusoidal Gust (330-341)
Control of the Turbulent Wake of an Appended Streamlined Body (342-354)
Investigation of Global and Local Flow Details by a Fully Three-Dimensional Seakeeping Method (355-367)
Prediction of Wave Pressure and Loads on Actual Ships by the Enhanced Unified Theory (368-384)
Frequency Domain Numerical and Experimental Investigation of Forward Speed Radiation by Ships (385-401)
International Collaboration on Benchmark CFD Validation Data for Surface Combatant DTMB Model 5415 (402-422)
Validation of High Reynolds Number, Unsteady Multi-Phase CFD Modeling for Naval Applications (423-440)
Free Surface Viscous Flow Computation Around A Transom Stern Ship by Chimera Overlapping Scheme (441-456)
Anti-Roll Tank Simulations With A Volume of Fluid (VOF) Based Navier-Stokes Solver (457-473)
Validation of Tab Assisted Control Surface Computation (474-484)
Experimental and Numerical Investigation of the Flow Around the Appendices of a Whitbread 60 Sailing Yacht (485-492)
Propeller Wake Analysis by Means of PIV (493-510)
Experimental and Numerical Investigation of the Unsteady Flow Around a Propeller (511-526)
Simulation of Incompressible Viscous Flow Around a Ducted Propeller Using a RANS Equation Solver (527-539)
On Submerged Stagnation Points and Bow Vortices Generation (540-552)
Numerical Prediction of Scale Effects in Ship Stern Flows with Eddy-Viscosity Turbulence Models (553-568)
The Experimental and Numerical Study of Flow Structure and Water Noise Caused by Roughness of a Body (569-578)
Large-Eddy Simulations of Turbulent Wake Flows (579-598)
Instability of Partial Cavitation: A Numerical/Experimental Approach (599-615)
An Unsteady Three-Dimensional Euler Solver Coupled with a Cavitating Propeller Analysis Method (616-638)
On the Flow Structure, Tip Leakage Cavitation Inception and Associated Noise (639-653)
An Experimental Investigation of Cavitation Inception and Development of Partial Sheet Cavaties on Two-Dimensional Hydrofoils (654-669)
Modeling 3D Unsteady Sheet Cavities Using a Coupled UnRANS-BEM code (670-686)
Ship Wake Detectability in the Ocean Turbulent Environment (687-703)
An Experimental and Computational Study of the Effects of Propulsion on the Free-Surface Flow Astern of Model 5415 (704-712)
Breaking Waves in the Ocean and Around Ships (713-745)
Numerical and Experimental Study of the Wave Breaking Generated by a Submerged Hydrofoil (746-761)
The Numerical Simulation of Ship Waves Using Cartesian Grid Methods (762-779)
Radiation Loads on a Cylinder Oscillating in Pycnocline (780-791)
Wave Resistance Computations - A Comparison of Different Approaches (792-804)
Computations of Nonlinear Turbulent Free Surface Flows Using the Parallel Uncle Code (805-819)
Submarine Maneuverability Assessment Using Computational Fluid Dynamic Tools (820-832)
Simulation of UUV Recovery Hydrodynamics (833-847)
Reynolds-Averaged Modeling of High-Froude-Number Free Surface Jets (848-862)
On Roll Hydrodynamics of Cylinders Fitted with Bilge Keels (863-880)
Combining Accuracy and Effciency with Robustness in Ship Stern Flow Computation (882-896)
An Unstructured Multielement Solution Algorithm for Complex Geometry Hydrodynamic Simulations (897-909)
Ship Stern Flow Calculations on Overlapping Composite Grids (910-926)
Study on the Prediction of Flow Characteristics Around a Ship Hull (927-940)
Analysis of Turbulence Free-Surface Flow Around Hulls in Shallow Water Channel by a Level-Set Method (941-956)
A Design Tool for High Speed Ferries Washes (957-967)
Flow Around Ships Sailing in Shallow Water - Experimental and Numerical Results (968-982)
Ship Stability Study in the Coastal Region: New Coastal Wave Model Coupled with a Dynamic Stability Model (983-992)
Waves and Forces Caused by Oscillation of a Floating Body Determined Through a Unified Nonlinear Shallow-Water Theory (993-1005)

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Radiation Loads on a Cylinder Oscillating in Pycnocline E Ermanyuk, N Gavrilov, I Sturova (Lavrent,vev Institute of Hydrodynamics, Russia) ABSTRACT The results of experimental and theoretical studies of the mdintion loads (added mass and damping) on n horizontal circular cylinder oscillating in n trot Ned fluid are presented Two cases of the density distribution over depth are considered: a) linearly stratified fluid of limited depth, b) two layers of mis cible fluids with the region of high density gradient (pJcnocline) in between The experimental technique for evaluation of the frequency dependent added mass and damping is based on the Fourier analysis of damped horizontal oscillations of the cylinder in strntifled and homage neons fluids The linear 2 D wave radiation probl ered theoretically both for horizontal of three Infers (the upper and lower Infers are homogeneous and the middle layer is linearly strntifled), what provides an approximate model of the experimental conditions The Boussinesq npprcximation is used By introducing n Green function, the boundary integml equation for the disturbance pressure is formulated Comparison of the theoretical and experimental data is presented INTRODUCTION The internal waves generated by n body oscillat ing in n stmtifled fluid h we been studied in some details both theoretically and experimentally A comprehensive bibliography on this problem is given -- T rner (1973), StepanJnnts et cl (1987), Voisin (1991) Recent progress in the technique of inter nal wave vi ualizati:n is described by Sutherland et cl (1999) How ver, it should be emphasized that only few authors have been concerned with evaluate tion of hydrodynamic loads acting on n body in n strntifled fluid despite the fn t that this problem has an engineering counterpart relevant to the predic tion of the I w speed and I w frequency motions of marine structures and deep submersibles in real sea environment which is characterized by the presence of vertical density gradient A bibliographic survey on this problem has been presented -- E rmanyuk & Sturova (1996) Let us note that continuous density distribu tion over depth which is normally observed in nature causes some specific properties of internal w wes The fundamental characteristic of n strntifled fluid with density distribution p(y) is the buoyancy (Brunt Vnisaln) frequency defined as N(y) = ~ where p is the gravity acceleration and y axis is di rected vertically upwards The maximum Brunt Vnisaln frequency for n given density distribution over depth defines the upper cut fl frequency for in ternal w e effects Thus, in contrast with infinite frequency spectrum of surface waves, the frequency spectrum of internal w wes is finite Moreover, when the oscillation frequency of n body is I wer, equal or higher than the buoyancy frequency, the equations of fluid motion are of hyperbolic, parabolic or elliptic type, respectively, what, once gain, is in contrast with free surface problems which are described by the Lnplace equation The major part of the stud ies on the body oscillations in continuously strut idled fluid is pe formed within the model of ideal, uniform :, strntifled (the Brunt Vnisaln frequency is assumed to be constant), Boussinesq fluid of ink nite extent in particular, the tim~domnin analy sis of damped oscillations of n sphere and circular cylinder is given in Larsen (1969b) and the solo tions in frequency domain Ewe been given -- Lay & Lee (1981) for vertical oscillations of n spheroid and by HurieJ (1997) for nrbitrarJ dire ted oscillate tions of an elliptic cylinder Mention should be made of the study performed -- Gorodt ov & Teodorovich (1986) To evaluate the p wer radiated with inter nal w wes by an oscillating body, they h we used the Green fun tion approach while the body geometry has been m: dsllsd -- the distribution of singularities borrowed from the solution of the pe tinent problem in homogeneous fluid Their results are found to be in dis greement with the results by HurieJ (1997) and Lay & Lee (1981) H wever, the disagreement is entirely caused -- the form of the surface source distribution For a correct form of the source, the for mulas presented in Gorodtsov & Tsodorovich (1986) will give a correct a timats The result presented in Hurled (1997) h we been sxpsrimentally confirmed

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-- ErmanJuk (2000) for the horizontal oscillations of n circular cylinder Let us note that, strictiJ speaking, oscillations of n 5: d:, in n stratified fluid can excite su face w wes H wever, the maximum buoyancy frequency is nor mnllJ much lower than the typical frequency of sig nificnnt surface wave effect For this reason, once we are concerned with the don mic e' ts due to in ternal w wes, the effects at free surface can be safely neglected so that the free surface itself can be con sidered as n rigid lid The present paper deals with experimental and theoretical investigation of the force coefi cients (added mass and damping) for n circular cylinder oscillating in n linearly stratified fluid of finite depth and in n pycnocline of finite thickness IMPULSE RESPONSE TECHNIQUE The technique used in the present study is simi Ian to the one described in Ermanyuk (2000) (see, also Cummins (1962) for theoretical background and Kerwin & Nnritn (1965) for pioneering experiment ) Foil wing this approach, we make use of experi mental records of damped oscillations of n cylinder (impulse response functions) in fluid and Fourier transform the problem from time to frequency domain in order to evaluate the frequency dependent added mass and damping coefi cient Let us assume that n 5: d:, pe forming small oscil lotions in n continuously stratified fluid can be ide Sized as n linear sy tem it is well kn wn that, once the response of any stable linear system to n unit impulse r(t) is known, the response of the system to an nrbitrarJ force f (t) may be written as the convo lotion integral ad)= I r(r)f(t r)dr (1) For the particular case of harmonic excitation, the equation of body motion in reduces to the second order ii tion with frequency depends ~ ?(~)]~ + N(~)~ + cow = mins 1962) Here, M is inertia of n body, q(h~) is one degree of freedom near difierentinl equal at coefi cients (Cum fo exp(f t) (a) the added mass, N(h~) is damping coefi cient, c is restoring force coef ficient, an overdot indicates difierentintion with re spect to time t Combining (2) and (3) and using linearity of the system one can write the formulas for frequency dependent coefi cients /(hl)=Cl1 ~iCOS[9(hl)]}/hl2 M (4) N(h~)=cR~sin[9(h~)]/h3, He= R(0) / R(h3) (5) Here 11(0) denotes the amplitude of the frequency response function at zero frequency As the ah ye considerations are applicable for the unit impulse em citation, the use of experimental records obtained for an nrbitrarJ value of impulse necessitates the nor mnlisation of JI(h~) by 11(0) The above described approach can be applied to prove the identity of Lnrsen's (1969b) and Hurled s (1997) solutions to the problem on the vertical oscil lotions of n circular cylinder in unbounded stratified fluid with N = coast Consider n cylinder of dinm eter D and the mass per unit length m floating at the horizon of -e :-:.1 equilibrium so that m = p,S, where pa, is the fluid density at the depth correspond ing to the cylinder center, S = xrD2/4 is the cams sectional area Assume that the cylinder undergoes small harmonical vertical oscillations The restoring force coefi cient can be evaluated from hJdrostntics as c = gSdp/dz Then, for non dimensional added mass and damping coefi cients, defined as air) = / v~r)J:t rear I) Jo Con = q/p,S, Cz = N/p,SN (6) In the particular case of harmonic force F(fh3) = the equations (4), (5) yield To exp(fhtt) one obtains x(t) = foexp(fhtt)Tt(fhl) (2) ~ Q2 [ ~2] ' ~ ~2' N ( ) where the complex frequency response function Tt(f(AJ) is defined as Fourier transform of the impulse response fun tion [~(f(A3)=T(.((A3) fTt6((A3)=; r(r)exp( f~r)dr F rthermore, we can introduce the amplitude To = [ .] + . .] ) and the phase 9 = nrctan(1l6/1l,) of the frequency response function As it is found -- Larsen (1969b), the time hi tory :(t) of damped oscillations of n cylinder, which was initially held at the vertical distance Jo from the horizon of -e :-:.1 buoyancy and then released with zero initial velocity, is described -- the function h(t) = :(t)/:o = Jo(Nt) e: Jo is the Bssssl func tion As follow from (1), the unit impulse response function r(t) is related to the unit top response function h (a) by time difisrsntiation r(t) = h(t) Thus, the impulse response function of a cylinder

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in uniform :, stratified fluid is r(t) = NJi(Nt) The Fourier tm form of the function NJi(Nt) (see, e g Ditkin & Prudnikov 1961) is [~6 = ~/~ ~ 1 516=0, 51,= (172 1) I/2(17+V~) (~>1) By substituting these expressions in (7) one can obt in CHICO, C>=~/~ (~<1) (8) C=, C>=0 (~>1) (9) what exactly coincides with Hurled s (1997) results for z circular cylinder in similar manner, it can be sh wn that Lzrsen's (1969b) solution for z sphere coincidm with the one given in Lay & Lee (1981) It is important to note that zdded mass q(h~) and damping coed cient N(h~) are interrelated by the Kramers Kronig relations The derivation of these relations is presented in detail in Landau & Lit hits (1958) The relevance of the Kramers Kronig relay tions to the theory of ship motions was first recog nized -- Kotik & Mangulis (1962) Foll wing Lain dau & Lit hits (1958) we can write, in our notations, ?(~) ?(CO) = 7r`.l; N(~) 2 2 (10) i(h)= 2h32`,/; 1~(o) ( )1 do i(0) (11) Here Woo) is the limit of zdded mass at hi ~ co The above expressions are different from those ones given in WeEzusen (1971) -- the presence of the last term in (11) As discussed in Landau & Lit hits (1958) this term is to be zdded when the function q(h~) + fi(h~)/h~ has z simple pole at hi ~ O For many problems of 5: d:, oscillations in surface waves there is no singularity at zero frequency (see, Kotik & Mzngulis 1962, WeEzusen 1971) However, the pole at zero frequency does occur for Hurled s (1997) so lotion There are reasons to believe that the similar situation may tzLe place in other 2 D problems of body oscillations in continuously stratified fluid The validity of formulas (10), (11) for Hurled s (1997) solution can be verified by the residue cal culus TzLing into account the finite spectrum of internal w es (12 < 1), eq (10) can be rewritten in non dimensional form as toll ws Cr(l:) Cr(ca = rr J o Of ,,2 Keeping in mind that ~ (hi) and ~ (hi) /h~ are even ~ uL cv, rmpectivelJ, the integml in (12) can be represented as the integml along the unit circle C by substituting a= cm c and the trigonometric functions in complex for ~l; ~82 C22= 1 / (zag 2z2 + 1) do f JO 'l + 2 (1 2172) Z2 + 1] Z It can be easily verified that for O is one simple pole at z = 0 inside L When 12 = 0, two dditional poles of der appear at the contour C in the The residue at z = 0 is I while t z = if ore zero Correspondingly, f:r the zdded mass coed cient is Cal = 0 (for circular cylinder Cr(ca) = 1) When 12 > 1, in addition to the pole at z = 0, there ore four poles corre sponging to the roots of the biquadratic equation 29 + 2 (I 2122) 22 + I = 0 The calculation of the residues at these poles gives Hurled s (1997) expres sion for the zdded mass coed cient (9) The validity of the eq (11) which in the present problem tzLes the form expressing Cz (17) = 2172 ~l; [C r(r) 1] 82 C22 + I can be proven in z similar manner it should be also noted that the presence of the singularity at zero frequency in the function q(h~) + f i(h3)/h) necessi tatm the correction of .- ~ popular formula for the zdded mass coed cient which is of use in the the ore of su face wa:vm According to WeEzusen (1971), this formula looks as rod / [? (hi) ~ (CO)] do, = 0 Jo (13) Using the prope to that ~ (hi) is even function, the integral in (13) can be evaluated viz residue calculus as the integral for the function ~ (hi) + f i(h3)/h) in the upper half plane along the closed contour which consists of the real axis (the path of integmtion goes around the pole at hi = 0 -- z semicircle of infiniteiJ small mdius) and the infiniteiJ la go semicircle in non dimensional form, for Hurled s (1997) solution the integration Jioids `,/; [Cal (hi) Cal (co)] dO = x/2 Similar result (i g the nonhero value of the integml (12) (13)) may 59 expected for other 2 D problem in

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continuously stratified fluid. Let us note that in 3-D problem the Eqs. (10), (11) and (13) can be used in their standard form (Wehausen 1971) since the singularity at zero frequency does not occur. EXPERIMENTAL ARRANGEMENT The experiments were carried out in a test tank (0.15m wide, 0.32m deep and 2m long). The scheme of the experimental installation is shown in Fig. 1. The damped oscillation tests were performed with the help of a cross-shaped pendulum. A circular cylinder of diameter D = 3.7cm was attached to the lower end of the pendulum. The gaps between the ends of the cylinder and the side walls of the tank were equal to 0.5mm. The volume of the immersed streamlined part of the pendulum was less than 1/ of the cylinder volume. nut n screw ball o sensors 1 at, ,, 11 1 ·- l Yn = ~ I I I I I I L ~ L test tack H 1 1 11 pendulums | cylinder v _ L b P(Y) Figure 1. The upper part of the pendulum had a micrometric screw with a nut of mass me = 188g. The variation of the vertical coordinate of the nut In allowed to change the restoring moment of the pendulum. The distance between the point of rotation of the pendu- lum and the center of the cylinder was b = 60cm. As the angular deflection of the pendulum in exper- iments did not exceed 0.5°, the horizontal oscilla- tions of the cylinder center could be with high accu- racy considered as rectilinear. The maximum mag- nitude of the horizontal displacement of the cylinder in experimental runs did not exceed 0.14D. The mo- ment of inertia of the pendulum Io (without nut) was measured with the accuracy of 0.5/, the measured value being I = 1.12 x 106g cm2. The total moment of inertia is I = Io + mrly2. Correspondingly, the value of inertial term in the equation of the rectilin- ear motion (3) and formulas (4), (5) is M = I/b2. The oscillations of the pendulum were induced by dropping a steel ball on a pre-tensioned rubber mem- brane attached to the end of the horizontal bar of the pendulum. The history of damped oscillations was measured by an electrolytic sensor whose output was sampled at 20Hz with a 12-bit analog-to-digital con- vertor. Let us note that the sensor produced very low liquid friction proportional to the first power of ve- locity. The final results were corrected for this value. The tests of damped oscillations in air demonstrated that all other kinds of frictional losses in the sys- tem including the friction at supports were negligi- bly small. To evaluate the restoring force coefficient c, a static calibration ire site was performed by load- ing a light bowl at the end of the horizontal bar of the pendulum with standard calibrated weights. De- pending on the vertical coordinate of the nut, typical full load used for calibration varied from 0.5g down to O.Olg. The accuracy of this procedure was about 0.57. Because of the high sensitivity of the experi- mental system, special care was taken to protect it from mechanical vibrations and air currents. To pre- vent the reflection of waves at the ends of the test tank, we used two types of wave-absorbing devices. In the case of linear stratification the wave energy of incident internal waves was effectively dissipated by perforated flat plates installed parallel to the end of the test tank. In experiments with a pycnocline the wave-energy absorber represented a 'sandwich' set of two perforated flat plates combined with an opaque plate inclined at small angle to horizon. The perfor- mance of the wave absorbers proved to be sufficiently effective. A weak solution of glycerine (linear stratification) or sugar (pycnocline) in water was used to produce a prescribed density distribution in the present exper- iments. Linear stratification was created by slowly filling the test tank with several layers of fluid having a prescribed density difference between the layers. For different values of fluid depth H. the thickness of one layer was about 1.5 . 2cm. The layered struc- ture eventually disappeared due to diffusion so that two days after filling the tank the density distribu- tion was perfectly linear. The linearity of the den- sity distribution was checked by the measurements of conductivity by a probe calibrated over the samples of solutions of known density. These data were used to evaluate the Brunt-Vaisala frequency. A smooth density profile with a pycnocline was created by filling the test tank with two layers of mis- cible fluids. Owing to diffusion, initial sharp interface between the layers evolved into a smooth density pro- file. In the coordinate system with the origin taken at free surface and y-axis directed vertically upwards the measured density distribution over depth fitted the following approximation p~y)=pO~1 - -2tanh:2˘~/~> i')~\

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Pa = 2 ~ e = P where h is the depth of the upper Inter, f is the char act ritic thickness of the pJcnocline, PI and /2 are the fluid densities in the upper and lower Inters, re affectively Let us note that according to theoretical solution for the problem of did ion of n weak admix tore (see, for example, Landau & Lit hits 1987) the density profile is described by error function H w ever, in Taylor serim for error function and for ho perbolic tangent the first two terms coincide while the third terms differ by only 25~o As result, both functions provide good approximations to the exper imental data H wever, from practical point of vi w, the use of n simple anal tical function, such as ho perbolic tangent, is more convenient in accordance with theoretical predictions the characteristic thick nerd of the PJ cnocline increases with time as f ~ tt/2 Owing m - -- low rat of glycerine and sugar diffusion in water, the characteristic time scale of this gr wth is measured -- days There was no detectable in crease of f within few hours needed to perform n series of experiments The experiments were per formed at e = 0 009 For each set of experimental conditions we recorded about n dozen of impulse response func tions at different valum of the re toring force coed cient c Theoretically, n single realization of impulse response function allow to evaluate q(h~) and N(h~) for any frequency O < hi < co in practice, n reliable estimate of the frequency dependent coed cients may be obtained in n certain frequency range in the vicinity of the frequency his correspond ing to the resonant peak of P(h~) To study the whole frequency range of interest, it is necessary to perform n series of experiments for n set of his and match the results at n common plot so that the data obt .=- d at different his overlap The variation of his can be easy attained -- variation of the restoring force coed cient c THEORETICAL ANALYSIS It is assumed that the :=-_ :d incompressible fluid occupies the region x < co, No < y = y+EI~ < Elf and there are three Inters: homogeneous upper and low r ones and n linearly stratified middle one Thus, density stratification in an undisturbed tat p(y) takes the form P(Y) = 1 ~ [1 sb/H2] /2 where 11~, ET2, ET3 = ET ET2 are the depths of the upper, middle and lower Inters, :-_ tiveiJ The circular cy linger is situated entirely within the middle layer and undergoes mall oscillations in the two possible degrees of freedom (surge and he we) with n frequency Lo The radiation and difiraction problems for n circular cylinder located beneath n pJcnociine in n constant density layer h we been con ridered -- Sturova (1999) The reciprocity relations are derived for the solutions of these problems Assuming the perturbed oscillatory motion of fluid P(')(x bit) = plRe[exp(ih3t)~ fpf (A A)] )=t where the superscript s = 1, 2, 3 denotes the values in the upper, middle and I wer Inters, respectiveiJ In the homogeneous fluid layers the functions pa t) p(3) satisfy the Lnplace equation Z\pft)=o (o2) (X> y) satisfies the equation zip) where N = v - nre imposed or fluid Opt t)/5y = o =, 2 ~2 ( H2 < y < 0) (16) ^ /~7~ The impermeability conditions .. the upper and I wer boundaries of (y = Hi) Ups 3)/ Y = o (y = al) while the fluid motions at the interfaces betw en the Inters should meet the matching conditions t) p2) 62Spt)l~y= p(2)/ y (y=o) 2) p 3) 62:p>3)l y = ~p(2)l~y (y = i/2) (19) where 62 = N2/h,2 1 in the far field the radiation condition is to be satisfied At the contour S: X2 + (y + h)2 = s2 located in the middle Inter we should pose the impermeability condition (Orb < He), ( H2 OCR for page 785
the distance between the center of the cylinder and the upper boundary of the middle layer Omitting the hydrostatic term, the hydrodynamic forces F = (Fl, Fz) acting on the oscillating cylinder can be determined by integrating the pressure over the contour S 2 Fu = I, f rut (k = 1, 2) )=t rug = h~2qu: forum = Pl, J P>2)~Uds (21) YE Nu: are the added mass and damping coed crents, respectively To solve the formulated problem, let us use the method of singularities in terms of unkn wn source distribution o>(x) over contour S. the fluid pressure in the middle layer can be represented in the form 2)(x) = J o,(x~)G(2)(x, x~)ds x= (x,b), X, = ( I,YI) Here G(2)(x,x~) is the Green function in the mid die layer for the problem under consideration This function can be determined from the solution of the foil wing system of equations AG(~) = 0 (0 < y < Al) (22) 52G(2) 625 G() =47r62f(x Xl) ( 11z N (62 < 0), for nil real valum of hi the men tioned equations are elliptic; the generation of inter nal waves does not occur in what foil ws we con .o Gl2) = 4,7rp6~( z=t k,)K(k,,b)K(k,,YI)X :e (I) = k(l tlt DY(k) K(k, :) = cos(k 6~) + to sin(k 6~) to = tank kale, t3 = tank kll3 D(k) = (p62tlt3 I)tan(k6112) 6(t~ n the middle layer (26) ~ respect to k The values Kit (Kit < kz < ) given by real valued positive roots of the equation D(k) = 0 represent the wave numbers of internal waves in the general case at Z ~ co k, ~ Z7r/(6ETz) In the form analogous to (26) the Green function has been obtained -- Robinson (1969) in the tudJ on the scattering of internal w wes at vertical barrier in n channel filled with linearly stratified fluid The source distribution o>(x) should be formu Inted in terms of continuous functions since the use of point singularities lends to the parndcx of infinite losses of energy (Gorodtsov & Teodorovich 1986) in traducing the polar coordinate system a, P with the origin taken in the center of the contour S. let us for mulate the foil wing representation for the functions of: he foil wing representation for the fun of (a, d) = ~ am sin ma for horizontal oscillations and (27) .o 02 (I, a) = ~ am con ma (28) m=t for vertical oscillations Substituting these relay tions in Eq (25), sequentinllJ multiplying it by sin~P(cos~P) and integrating over S (note that for n circular cylinder ~~ = sing, ~2 = COST), we

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obt fn the infinite svstem of linear enuation for un .fi cients am(tm) .o 2 ~ amAm~ = 2 m=t 27r h,2 27r 2~ 2~ Am~= / sinmr / sin~Px Jo Jo / SG(2) cosr5G(2)\ sinr— 2 — IdPdr :~ 6 Yt J r2~ r2~ Bm~= / cosmr / cos~Px Jo Jo ( i SG(2) C°S75G(2))d~d S~ 6 yt r = zrctan[x~/(y~ + h)], f~ is the Kroneker deltz (29) Since the exprmsions for Am~, Bm~ zre rather cumbersome, let us describe the basic principles of their evaluation The integrals in the exprmsions for the imaginarJ pz ts of Am~, Bm~ can be evaluated znalJticallJ bJ using the foll wing tzbulated formu las (Abram witz & Stegun 1964) r2~ / cos mz cos(X6 cos z) cos(xsin z)dz = JO ~rlm cos mf Jm(q) r2~ / cos mzsin(X 6 cos z) cos(xsin z)dz = JO ~rlm sin mf Jm (q) J sin mz cos(x 6 cos z) sin(X sin z)dz = o ~rlm cos mf Jm(q) .,/; sin mz sin(X 6 cos z) sin(X sin z)dz = ~rlm sin mf Jm(q) where f = zrctan 6, q = X/12, X = ak, Im = I ( I)m, Jm zre the Bersel fun tions of the first I (31) (32) (33) (34) cind evaluating the Am~, Bm~ For evaluation we use well kn wn ex pansions (Abmm witz & Stegun 1964) cos[qsin(r + f)] = Jo(q) + 2 ~ Jzv(q) cos[2~(r+ f)] (35) .o sin[qsin(r + f)] = 2 ~ Jzv+r(q) sin[(2~ + I)(r + f)] v=o The summation i (36) .... , , ;o the number of term which zll wed to ensure the rela~ tive inaccumcJ of order 10 Z in the calculations of integrals for each wwe mode in Am~ Bm~ The solution of the sJstems (29), (30) mzJ be trun eating the infinite series zt z finite number of term, which depends on the desired zccuracJ Once the coefi cient am tm zre obtained, we can determine zll the cEzmcteristic of the fiuid motion In the far field, the fiuid motion represents z super position of infinite number of w e modes Thus, for ex mple, the pressure in the middle IzJer zt x ~ co has the form n (351. (36) was executed UD ~ co i2) = ~ ~ Er (k,)K(k,, y) exp(+f k,x) .=t ~o P i2) = ~ Ez (k,)K(k,, y) exp(+f k,x) Et(k) = 4~r2~6~(k) ~ amJm(q)(lmcm + I+Sm) m=t co E2(k) = 4f7r2~6~(k) ~ tmJm(q)(l+Cm + ImCm) m=t Cm = (h, 6t~h6) cos mf, Sm = (h6+ 6t~h,)sinmf h, = cos k 6h, h6 = sin k 6h The pressure in the upper znd I wer IzJers can be determined using the form of the eigenfunctions of the given problem (see, for example, Sturova 1999) According to (21), the hJdrodJnamic load is ~2~ ;~,:~ = m=t 2~ 2~ tm / stn mr / sm PG dPdr (37) JO JO h~2~22 fh3~22 = .o :2~ 2~ p~a ~tmJ cosmr cosPG(2)dPdr (38) of the hJdrodJnamic zero The kn wn zpproach to zpprcximate solution of the present problem uses the expressions for am, tm which zre borr wed from the solution for zn infinite homogeneous fiuid: ar = tr = h32/(27r), am =

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bm = 0 (m > 2) Under this assumption, the damp ing coed cient can be determined from the imag inarJ part of the Green fun tion (26) in nddi tion, taking into account (31) (34), the integration in (37), (38) can be performed anal tically For n layer of n linearly stratified fluid bounded -- rigid horizontal lids the npprcximate solution is given by Gorodt ov & Teodorovich, 1986 How ver success fund the above mentioned npprcximation has been used in the study of the surface w wes, it cannot pro (2) X~ smam(D + ;? ) vide n consistent result for the hydrodynamic lo ding P' _, m m on n body oscillating in n linearly stratified fluid This fn t can be convenientiJ illustrated for uni form y stratified fluid of infinite e tent The total hydrodynamic lo d acting on n circular cylinder in this case has been determined by Hurled, (1997) (see (8), (9)) ?~t = ?22 = 0, Ntt = N22 = 7rp~s ?~t = Y22 (hi < N) = 7rpl~ ~/h3, Nt (hi > N) An interesting property of this solution is the fact that the horizontal and vertical loads coincide The npprcximate solution for diagonal damping coed cients takes the form (Gorodt ov & Teodorovich 1986) Ntt = 41rpt~2hd2~iN2 N22 = 47rp~2(N2 :~,2~372yN2 (IS < N (39) =22=0 (40) (41) tween (39), (40) and (41), (42) When Lo > N. one can use the integral equation (25) with the Green function e cylinder We seek the solution of the problem (14) (20) in the form In this case, the fluid tion of x, while for vertical .o Pit) = ~ smamFm (0 < y < B ) (43) m=t ( Bz < y < 0) (44) Pi3) = ~ mTm ( B < y < B2) m=t 1 rho Fm(~ A)= ~ / km Icoshk(y B ) (45) sin kxA(k)dk Dm(~>y) = ( I)'x JO km le ~u(f +~) sin kid k (y + h > 0) l)m+l ~ km t3~u(f +~) sin kid k (y + h < 0) ;7m(~>Y) = ( 1)'`,/; km t[B(k)3]U(f+~)+ C(k)3 ~U(f+~)] sin kink Tm(~ A)= ( I)! J km tcosEk(y+B)x sin kxW(k)dk The fun tions A(k), B(k), C(k), W(k) determined from the matching conditions at the boundaries of fluid layers (18), (19) are equal to G(2) = 2~[1nP `.l; T(k) t)~(k)dk] ( ) cost B Z2(k)' B(k)= 2Z (k) Zi(k)e here C(k)= ( i3)Z3(k)3~U(6 82) ~2 = (A ~1)2 + :2(y yl)2 :2 = 6Z 2Z (k) (ok) = cosh[k:(y + Or + Bz)](l ~ tots)+ ~sinh[k:(y + Or + H2)](t3 to)+ +exp( k H2)cosh[k (y Vl)](l 7tr)(l to) T(k) = (1+~2t~t3) sinh(k H2)+~(tr+t3) cosh(k:Bz) H wever, for circular cylinder the method of mul tipole expansions is more effective The standard application of this method is ferment d, for exam pie, in Sturova, 1999 Since the solution is rather cumbersome, we shall consider bel w the horizontal W (k) = cosh kB Zz (k) Zi(k) = (1+ t3)e~(82 6) ( I)m(l tt3)3~u(~ 82) Zz (k) = ~r(tr+t3 ) cosh (~kH2 )+ (1+~2tlt3 ) sinh(:kB z) Z3(k) = (1 :~)3 ~u~ ( 1)m(l +.~t ) ~u~ The unkn wn con tant Sm are to be determined from the boundarJ condition (20) nt the contour S This condition cnn be written as n sJstem of linenr equntions bJ consecutive multiplication bJ sin ~P nnd integrntion over P from O to 2~r The integrnls which

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mericallJ The constants Sm be culate the pressure at Ration (21) When hi has real value and is c mass ~Pt ?~t :~2 where sing detern contour S > N. the hydrodynamic load letermined only -- the added ' (m 1)l (Xm + Ym)~ ?2t = 0 Xm = 2r(m)1m `.l; (72 Coz2 P + sin2 p)m/2 sin (m arctan ) do ~ [ (I 7) (I + 7) ] ,.o / x ~7m(q)[B(x) + C(x)]dx Jo P(m) is gamma~function Since the Boussinmq approximation is used, in the limit case of high frequency oscillations of a cylinder the problem reduces to the description of the cylinder motion in the layer of constant density and the full depth B ~ + B At G~ ~ co () ~ 1), the used approach reduces to the standard method of multipole expansions NUMERICAL RESULTS When LO < N. the investigation of the accuracy of numerical results depending on the number of terms Nl in expansions (27), (28) and the number of in ternal wave modes N2 in the Green function (26) is of considerable inter t The non dimensional added mass MI I and damping Let coed cient for horizontal oscillations of the cylinder at BI = B3 = 0, Bz/a = 5, F/~ = 2 are presented in Table for three values of the non dimensional frequency 12 = 0 3; 0 6; 0 9 The toll wing notations are introduced M)) = PZZ L>> = N. (j = 1,2) Let us note that the non dimensional coed cients M)) and L>> are identical with the coed cients Cal and Cv introduced in (6), being different only -- the definition of the reference density For a weakly stratified fluid, this difference can be safely neglected Also presented are the complex values of the first three coed cients am = 27ram/hd2 it of ~~ show that they are essentially different from those used in the approximate solution Both real and imaginary parts of ~~ depend on frequency At certain frequencies, the absolute values of real and imaginary part are close to each other The modules of the two successive coed cients cry and ~3 h we the same order of magnitude as the modulus of ~~ The necessity to take into account a large num her of internal w e modes in investigation of their propagation in the layer of linearly stratified fluid has been emphasized -- Larsen (1969a) This e' t can be explained -- the absence of any viscous effects in the model considered The inclusion of viscous ef fects into analysis of the wave motion should lead to better convergence of the solution with the increase of N2 The hydrodynamic loads for horizontal and verti cal oscillations of the cylinder are sh wn in Fig 2 in numerical calculations at LO < N we use Nl = 20 and N2 = 200 At LO > N. 15 term in the expan sion (43) (45) are taken into account The solution (39), (40) is sh wn in Fig 2 -- solid line it is appar ent that the hydrodynamic loads essentially depend on the type of oscillations what is especially notable at I w frequencies The increase of the added mass at I w frequency horizontal oscillations can be ex plained by blocking With the increase of the strut Ned layer thickness, the numerical solutions gradu ally approach to the dependencies (39), (40) what is most pronounced for the case of vertical oscillate tions The hydrodynamic lo ds are also fected by the presence of sup cientiJ deep homogeneous layers Let us note that in the presence of homogeneous layers the added massm for horizontal and vertical oscillations of the cylinder practically coincide at hi > N in all the cases presented The limit values M)) at G~ ~ co are essentially different from I only for B = B3 = 0, Bz/a = 5, h/n = 2 These values MII = 1 3326 and M22 = 1 165 are sh wn by the dash lines in Fig 2 (: ompari.on with experimental rezultz The results of the theoretical and experimental evaluation of the added mass and damping coed cients of the cylinder in the linearly stratified fluid of limited depth are shown in Figs 2, 4 for a layer of linearly stratified fluid and in Figs 5, 6 for pJcno cline in numerical calculations the thickness of the middle layer H2 was taken equal to 5

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N1 N2 Q 0.3 0.6 0.9 Q m 0.3 2 3 1 0.6 2 3 0.9 2 3 10 100 1 100 Ml1 0.626 -0.036 -0.079 Realm 0.981 0.005 0.037 0.581 0.004 0.065 0.547 0.014 0.015 Ll1 0.465 0.452 0.141 Imorm -0.929 -0.002 -0.118 -0.456 0.002 0.018 -0.042 0.075 -0.156 Ml1 0.630 -0.034 -0.079 Realm 0.983 0.005 0.041 0.585 0.004 0.068 0.551 0.017 0.015 Ll1 0.463 0.453 0.142 Imorm -0.920 -0.002 -0.106 -0.455 0.002 -0.014 -0.043 0.077 -0.154 Ml1 0.626 -0.034 -0.079 Realm 0.978 0.005 0.031 0.581 0.004 0.063 0.550 0.014 0.014 Table 20 200 Ll1 0.467 0.453 0.143 Imorm -0.927 -0.001 -0.122 -0.453 0.002 -0.021 -0.040 0.079 -0.157 Ml1 0.624 -0.034 -0.079 Realm 0.977 0.005 0.028 0.580 0.004 0.061 0.549 0.013 0.014 1. 1 to ~r 1 =~ 0.5 The solid lines in Figs.3-6 correspond to analyt- ical solution (8), (9) for the unbounded exponen- tially stratified fluid. In non-viscous stratified fluid the generation of internal waves is the sole physical mechanism of the energy dissipation. The numeri- cal simulation gives zero damping coefficient when Q > 1. As the depth of stratified layer decreases, the calculated values of the damping coefficient at Q < 1 also decrease. The physical reason for this be- havior is the effect of the wave-guide. In particular, when Q ~ 1, the internal waves with nearly vertical vector of the group velocity undergo multiple reflec- tions when travelling between the cylinder and the bottom. As result, a certain portion of wave energy is 'trapped' instead of being effectively radiated. Ll1 0.468 0.453 0.143 Imorm 0.928 -0.001 -0.126 -0.452 0.003 -0.023 -0.039 0.079 -0.158 j=1 j=2 hick H1/a Hz/a H3/a | · 2 0 5 0 1 V ~ 2 100 5 100 1 O · 25 0 50 0 Hurley (1997) Figure 2. Ml1 0.624 -0.034 -0.079 Realm 0.976 0.005 0.027 0.581 0.004 0.062 0.549 0.013 0.013 .5 Q 2 Ll1 0,467 0.454 0.143 Imorm 0.926 -0.001 -0.122 -0.452 0.003 -0.023 -0.039 0.079 -0.158 Ejj~ 0.51 n : 0.5 Q In experiments, dissipation of energy is due to combination of wave and viscous effects. The con- tribution of the wave damping to the total value of Cx can be roughly represented as the difference be- tween the values of Cx measured in the stratified and homogeneous fluids at the same H/D. The exper- iments conducted in homogeneous fluid show that Cx increases when H/D decreases. Having this in mind, one can note reasonably good agreement be- tween the numerical and experimental data for suf- ficiently large Q. Numerical results for the added mass coefficient Cll shown in Figs.3, 5 seem to cap- ture well the main experimentally observed effects at Q > 1. However, at low Q the behavior of numerical and experimental data is quite different. It seems

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cat '' 1/65 CO !"- :: 1 ++-+- I've ~ 00 O,0 O,5 1,0 1 5 Q 2,O O 1 0 O 1 5 1 1 0 Q 1 1 5 Figure 6. Figure 3. 2- Cp 1~ o HID + 1.65 ~ · x 2.19 +\° ~ 3.24 \\ ~ a~ AA a A A ~ - ~~X AX _ ~ _ a' O1 0 O1 5 115 l Ci, 1 1° 0,0 - Exp.(^ · o) Num.(+ x a) l 1 1° Figure 4. E~p.~.o. ~ a) Num.(+ x i) . . . me. O1 5 ~: l l l 1 15 Q TO dID 0~43 0 0~78 + · 1~24 x ~ 1~62 3' ' 2~62 0 8 god ~N<~.~,~9~4 . . O. 0 O1 5 1 1 0 Q 1 1 5 Figure 5. likely, that some additional theoretical analysis is to be done in future to establish the exact asymptotic at Q ~ 0. In experiments, for low values of the pycnocline thickness (5 < D), the dissipation of energy due to internal wave radiation is low. Correspondingly, the damping coefficient is small and Cat is close to 1 (i.e. the value it takes in homogeneous fluid). As the thickness of the pycnocline increases, the depen- dencies of the added mass and damping approach asymptotically those ones corresponding to the case of infinitely deep exponentially stratified fluid. CONCLUSION To our knowledge, this report presents the first experimental and numerical investigation of the hy- drodynamic loads acting on a 2-D body oscillating in a continuously stratified fluid of limited depth. The density stratification is shown to have a strong ef- fect on the frequency-dependent hydrodynamic coef- ficients (added mass and damping). As the thickness of linearly stratified layer decreases, the portion of energy radiated with internal waves also decreases. The results obtained for stratification with a smooth pycnocline allow to estimate the ranges of applicability of the most popular theoretical ideal- izations, namely, the model of two-layer fluid with an interface and the model of exponentially strat- ified unbounded fluid, for the description of a real stratification observed in natural conditions. The future research in the field will be aimed to the investigation of a 3-D problem. Acknowledgments: This research has been supported by Council "Leading Scientific Schools", grant N 00-15-96162,

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Pussian Foundation of Basic P search, grant N 0001 00812, SD PAS integrate Project N 1 2000 and grant N 6 for young scientists REFERENCES M.Abram witz & I.A.Stegun, 'Handbook of Mathematical Functions', NBS, 1964 W.E.Cumminz, 'The impulse response function and ship motions' Schifl technik, Vol 9, Up 101 109, 1962 V.A.Ditkin & A.P.Prudnikov, 'Integral T ans form and Operational Calculus' Gos Izd Fin Mat Lit Mosc w, 1961, (in Pursian) E.V.Ermanyuk, 'The use of impulse response functions for evaluation of added mass and damping coed cient of a circular cylinder oscillating in linearly stratified fluid', Exp Fluids, Vol 28, Up 152 159, 2000 E.V.Ermanyuk & I V Sturoza, 'Hydrodynamic loads on a body in a stratified fluid', Proc I t Int Conf Marine lad try, Varna, 1996 V.A.Gorodtzov & E.V.Teodorovich, 'Study of internal w wes in the case of rapid horizontal motion of cylinders and spheres', Fluid Don, Vol 17, Up 893 898, 1982 V.A.Gorodtzov & E.V.Teodorovich, 'Energy characteristics of harmonic internal wwe genera tore', J Appl Mech Tech PhJs, Vol 27, Up 523 529, 1986 D.G.Hurley, 'The generation of internal w ves -- vibrating elliptic cylinders Part I I viscid sol tron', J Fluid Mech, Vol 351, Up 105 118, J.E.Ke win & H.Narita, 'Determination of ship motion parameters by a step response technique', J Ship Research, Vol 9, Up 183 189, 1965 J.Kotik & V.Manguliz,'On the Framers Kronig relations for ship motions', Int Shipbuilding Frog, Vol 9, Up 351 368, 1962 R.Y.S.Lai & C.-M.Lee, 'Added mass of a spheroid oscillating in a linearly Ratified fluid', Int J Engng Sci Vol 19, Up 1411 1420, 1981 L.D.Landau & E.M.Lif hits, 'Statistical Physics' Addison Wesley Pub, 1958 L.D.Landau & E.M.Lif hits, 'Fluid Mechanim' Butt Worth Heineman, 1987 Landau, L D & Lit hits, E M 1987 L.H.Larzen, 'Internal Owes incident upon a knife edge barrier', Deep Sea Fe Vol 16, Up 411 419, 1969a L.H.Larzen, 'Oscillations of a neutrally buoyant sphere in a Ratified fluid', Deep Sea P search, Vol 16, Up 587 603, 1969b R.M.Robinzon,'The Alec t of a vertical barrier on internal Owes'. DeeD Sea P a. Vol 16. DO 421429. 1969 Yu.A.Stepanyantz, I.V.Sturova, E.V.Teodor vich, 'The 5Dear theory of the generation of the surface and iDt mal w wes, it hi Nauki i TeLhniki MeLhaDik Zhidkosti i Gaza, Vol 21, Up 92 179, 1987, (in Pussian) I.V.Sturova, 'Diffraction and radiation problems for the circular cyiiDder in stratified fluid', Fluid DJD, Vol 34, Up 81 94, 1999 B.R.Sutherland, S.B.Dalziel, G.O.Hughez, P.F.Linden, 'Visualization and measurement of iDterDai w wes -- synthetic schtieren Part I Vertically oscillating cylinder' J Fluid Mech, Vol 390, Up 93 126, 1999 J.S.Turner, 'BUOJaDCJ Eflects in Fluids' Cam bridge; Cambridge UDiv Press, 1973 B.Voizin, Internal w ve generation in uniformly stratified fluids Part I Green s function and point sources', J Fluid Mech, Vol 231, Up 439 480, 1981 J.V.Wehauzen, 'The motion of floating bodies', ADD P v Fluid Mech, Vol 3, Up 237 268, 1971 J.-H.Wu, X.-H.Wu, S.-M Li, 'A theory of wwe diffraction and radiation by a large body in stratified ocean (111) Boundary element method', J HydrodyD, -e- A, Vol 5, Up 74 80, 1990

Representative terms from entire chapter:

added mass