Questions? Call 888-624-8373

Rights & Permissions

topleft topright

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

Page
423
bottomleft bottomright
Page
423
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)

Below are the first 10 and last 10 pages of uncorrected machine-read text (when available) of this chapter, followed by the top 30 algorithmically extracted key phrases from the chapter as a whole.
Intended to provide our own search engines and external engines with highly rich, chapter-representative searchable text on the opening pages of each chapter. Because it is UNCORRECTED material, please consider the following text as a useful but insufficient proxy for the authoritative book pages.

Do not use for reproduction, copying, pasting, or reading; exclusively for search engines.

OCR for page 423
Validation of High Reynolds Number, Unsteady Multi-Phase CFD Modeling for Naval Applications J. Lindau R. Kunz D. Boger D. Strnebring H. Gibeling (Penn State Applied Research Laboratory, University Park, Pennsylvania 16802) Abstract Un teddy, high Rey old number validation cases for c multi-phase CFD analysis tool have been pu sued Tbe tool, designated UNCLE-M has c wide r mge of applicability including flows of naval relevance Tbis in ludes supercc itating Ed cavitating flows, bubbly flows, Ed water entry flows Tbu far the tool has been applied to c variety of co figurations A isymmehic sheet cavity flow-fields have been modeled in putic jar, m crempt to validate file unsteady r liability of UNCLE M wibb consideration of the effect of cavitati m number, Rey olds number Ed tubulen model has been mad Analy is of the modeled Em teddy fl w field is also mad Ed con lusions regarding the c uses of su cess Ed sho tcom logs m the computational re mlts are d awn Introduction Tbe ctility to properly model unsteady multiphase flows is of g eat impo tance, particularly in naval applications Cavitation may occu in submerged high peed vehicles es well es rotating mcchin y. nozzles, Ed mmmerou of her vend s Traditionally, ca anon on has bad n dative implications associated with damage Ed or noise However, for high speed submerged vehicles, file red ~ tion in d cg associated with c natural or ventilated cavity has g eat pote ticl ben ft. Yet, cavitation mod leg remain c difficult task, Ed only recently have full Rey olds-avemged, tb ee-dimensional, multi-phase, Navier-Stokes tools reached the level of utility Nat fLey might be applied for engine enog p moses UNCLE-M (Klutz, 19990,11)) is c fully implicit, pa -conditi med. multi-phase, 3-D, fully gen mlized multiblock, parallel, Rey olds~eraged Navier-Stokes solver Tbe code was initially evolved from c version of the single-phase UNCLE code developed et Mississippi State University (Taylor, 1995), Ed hr. undergone sig fficmt flubber development UNCLE-M in omorctes mixture volume Ed constituent volume faction trmsport/gen ration for liquid, condensable vapor Ed non-condensable gas fields Mixture momentum Ed tubulen e scalar equations are also solved Flu limiting has been applied to file in iscid flu temms based m file local slope of file solution volume Faction As c r suit, high- 1 order accurate solutions containi g crisp, physically reasonable mte faces et tb cavity boundary may be obtain d wibb minimal nonphysical oscillations Non equilibrium mass transfer mod leg is employed to ccptme liquid Ed vapor physic excb mge Tbe code c m b male buoyancy effects Ed the presen e/ interaction of condensable Ed non-condemctle field. Tbis level of modeling complexity represents file tate- of-the art in CFD crurlysis of ca vitation Tbe resh ictions in r mge of applicability associated with in iscid flow, slender body theo y Ed of her simplffyi g assumptions are not pa sent In particohr, the code m plushly add ens the physics associated wibb high-speed manes rs, body-cc ity interactions Ed viscous effects such as flow separation Tbe principal interest here is in modeling high Rey olds number, umstecdY flow cutout bodies wibb rummg cavities These cc ities me presumed to be sheet cavities amenable to c h mogen ous approach other words, it is presumed flat file non quibbrmm dynamic for es of bubbles are of n gligible mug it de In the present work, file effect of surface tension is not in crporcted, sin e inte face cu vatmes are very mall for the co figurations considered Tbis cssumpti m is supported by model results of sheet cavitati m with c full two-fluid approach (Grogger Ed Akjbegovic, 1 993) In pa vious work Mum, 1 99hT!), file fidelity of UNCLE-M has been demonstrated for steady state fluid flows However, du to the reenh mt jet, cavity pinching, Ed of her effects of turbulent separated flow, m iti-phase flows of naval importance me generally unsteady ~ the work pa sented her, UNCLE-M will be applied to several co figurations of naval relevance Each of these co Migrations pa sents m experimentally documented, unsteady fluid dy amic test case Model remits will be presented for several ballistic, cavitatcr geometries Bobb file steady (averag d) Ed unsteady (time domain Ed pectn 1) behavior of the flow will be presented Ed compared wibb data h addition, intere img urn he tdy mmmerical results will be presented in a field form for comparison with photon sphic dhtn By comparison of file m merical Ed me tsured results, the nlhbility of file umsteldy capabilities of file code m to he understood

OCR for page 424
Symbols: Cl,C2 Cdest. Cprod Cp cd D dm f gi k L . i Prn ~Pr p ReD Sh tu bule pe model const mts mass hemsfer model comstemts pressure coefficient d cg coefficient body diemeter bubble diemeter cyclingfiequ py Hz) g~avity vector tmbuient kmetic energy bubble le 3th mass t msfer rctes tmbulent kmetic energy produption tu bulent P mdtl numbers for k emd e press lre Rey olds number beped on body diemeter Shonh~lfrequ py (fD)/U= e P ienf h clong co figmation (clso secomds) t, t=, At physiccl time, meem flow time sccle, time step velocity mcg itude Cc tesi m velocity components Cc tesi m coordinctes U Uj Y+ D p U p Subscripts, Superscripts: D t dimensionless wall di te pe (p yU~)/~ volume f ction, emgle of ctt~ck preconditionmg pe emeter pseudo-time tu bulence dissipation rcte molecohr viscosity density cc itstionmmber( = P= Pv 1/2p,U body diemeter liquid ml tme noncond nsable gas tmbulff~t condemctle vapor free t~eem valu Physical Model he phy iccl model equ~tions solved he~e have been decribed previpmsly ~u d 1999 0,11)) he basis of the model is the i pomp~ ble multiphase Rey olds Avereged Ne ier Stokes Equstipms in c homog neous form Each phcse is treeted es c new species emd requi es the mclusion of c sepe cte contimmity equstion Ihree species, ~epresenti g c liquid, c condensable vapor, emd c no pond nsable gas, e e i pluded Miss hem fer betw en fhe liquid emd vapor phcses is cchieved f ough c dffferenticl model ther resee chers have cpplied simile models with c smgle species cpprocch How ver, the multiple species model of multiphase flow is p~esented es c mme flexible physiccl cpprocch A high Rey olds m mber fomm of twocqu~tion models with stemde d wall fu ptions provides tu buie pe closu e he govermog dffferenticl equ~tions, cept m Cc tesiem tensor form e e given es Equ~tion (1): ( 2~a~+a~j (P~Uj)+d p~Uj)+a] (p~UjUJ a~i ~ ~i jap+a~i+ a i ~p 2)a~ a~ a~p at +( p2~ +a~ e+d (~eU) = 0 ( )( ) , Pi PV = dPx +a~j(~mytW)+p~g (~ U ~ = (m +m ) (1) Where ml tue densit emdtubulentvicosity have been deftned m Equ~hon (2) pm = p,~ + Pv4 + P~d~d p~C~k F~' e (2) In fhe present work, fhe density of ecch constituent is teken es comtemt Equ~tion (1) rep~esents the conservation of mixtme volume, ml tme momentum, liquid phcse plume f ction emd nom condensable gas volume f ction, respectively Physiccl time derivatives e e i pluded for umstecdy computations he formuletion mcorpomtes p~e- conditioned pseudo-time-derivatives (a/8s terms), defmed by pe emeter p, which provide fe orable converge pe che cteri tics for stecdy state emd umstecdy compu ctions, es discussed fu ther below he formation emd colhpse of c cc ity is modeled es c phase t msfommation Debiled modeling of fhis process requi es k owledge of fhe themmodynamic behavior of the fluid nee c phepe t msition pomt emd the fommation of interf ces Simplffied models ere presented here, ~esulting m fhe use of empi iccl f ctors Given es Equ~tion (3), two sepe cte models e e used to descobe fhe t msfommation of liquid to vapor emd fhe t msfommation of vapor back to liquid For hemsformation of liquid to vapor, i is modeled es being proportiom~l to fhe produpt of fhe hqmd volume fi ctmn emd fhe d'fferffce between fhe 2

OCR for page 425
computatlord~l cell pr ssme md the vapor pressu e This model is simibr to fhe or used by Merkle et cl (1998) for bodh evaporction md condensatior For trmsformation of vapor to liquid, c simplffied form of the Girdbuglmd~u potff~tial is used for fhe mas trmsfer rcte ~ ~ = cdestpv~iMIY[O P [v] ( Pi =)= + CpVodPv~i (} ~i) Cde~t mdCrOdare mpiricclconstmts Forcll work preented here, Cd~st = CprOd = 105 Both mass trmsfer rctes are nom-dimenriord~lized with r spect to c me m flow time sccle In fhis work, c high Rey olds mmber two- equation tmbulerpe model wifh st mdard wall f mctions hcs been implemfftted to provide tubulerpe closue Eifher the k-e or RNG k-e (Orszag et cl 1993) model cc represented m Equation (4): i(P~t)+~(P~tU,) = a~,(Pvtta—X,)+P ps i ~ a~j ~ J a~j( t~a~,) I ~ t) (4) As with velocity, th tmbulffce pclars are interpr ted dP being mixtme qu mtities Numerical Method The baselme mmmericcl method hcs been evolved from the work of Tcylor md his coworkers et Mississippi State University (Tcylor et cl (1995), for e dmple) Prim~tive varictle mterpolmt t pe Roe flu d'ffer rce spl~rmg ~s ued for spat~cl d' pret~zatmn A implicit procedme is cdopted wifh ir i pid md vi cour flu Jccobi ms cpproximated m mericclly A block symmehic G mss-Seidel itemtion is employed to solve the cppr oxim ate Newt on ystem et eah t ime step Th multi-phase extemion of the code retams the e umderlymg mmmencs but mpo porctes two cdditiorul volume fraption constit ent trmsport equations Du ing flu formulation, c Jdmeron-style (Jdmeron 1981) flux limiter bced on liq id volume frdption is cpplied to th primitive mte pol mts A nom diagord~l pseudo -tim e- deflvat ive prec onditi onmg matrix ~s clso employed Wh~le fhe t~me denvat~ve term mishes from the mixtue contmnity equation es fhe limit of mcompr ss~ble con titu nt phcses is cpprpahed, the effect of pr conditionmg is to redupe the daocidted stiffLess This preconditior r gives rise to c system with w 11-conditioned eigern~lu s which cc mdependent of densdy mtm md loccl volume frd ption This sy tem is w 11 suited to high density rctio, phcse-separcted two-phcse flpws, such es the cavitatmg sy tems of mter st her A t mporally secomd-ord r cocu cte dpal-time scheme was impleme ted for physiccl time integ ction At eah time step, the tmbulerpe trmsport equations are solved mbsequ nt to solution of fhe me m flow equations The multiblock code is inshumented wifh MPI for pmallel execution based on domcm decomposition Du ing umstecdy time mteg ction, to obtarn remits presented her message pcsstog WdP ') cpplied dfter eah symmetric G mss-Seidel sw ep Each imer iterdte ir plved twenty symmehic Gmss-Seidel sw eps, md eah time tep mvolved ffteen imer iterctions This procedu e was s fficient to relialy red p the umstecdy residual by et lecst two orders of mcgmitude However, c pcse by pcse e cmird~tion lik Iy could have redu d fhe expended computatlord~l effort yieldi g remits similar in solutiom fidelity Fu th r detcils on fhe m mericcl method md code are available inKu det cl (199900 Results A isymmehic sheet pavity flow-felds have been mod led in putic dar, m crempt to validate fhe umstecdy relictility of c m dtiphcse, computatlord~l fluid dyrdmms tool w~fh com~demtmn of th dffectr R y olds number md tu bulerpe model hdP beff~ mcde Stecdy, averag, mecsurements of rlevmt cavitation pardmeters tor the shapes chosen have been documentedbyRouse mdMcNow (1949) Stinebring et cl (1983) documented the um tecdy cycling behavip of evercl axi mmetric cavitators Their report irpluded r suits for bodh ventilated md natu cl cavitation The umstecdy pe form mpe of c 45° (22 5° in profle from centerlire to outer edge) conical, hemisphericcl, ad Occhber ogival pavitatms et c rage of cavitatipm m mbers w re documented Aifhough UNCLE-M hcs the ccpability to model ventilated cavitation Ku d 1999([)), only rd~tmcl cavitation re mlts have been irpluded here it should be noted that the results of Rouse md M Now (1948) indicated that for the pavitatm t pes md flows et or ctove the r mge of experimental R y olds m mbers r ported md ir stigated here, the flow should be tu bulent over c sig if icmt portion of the forebody Therefore, fp smgle phcseflow. particohrlyfor geometricclly smooth shapes, this should ser to avoid the w 11 k ow chcotic, criticcl kmmar separction md tr msition regime The m merical r suits employ c fully tu bulent model R suits pre ented her are given in fhe model computatiord~l system (S~ umits For cll computations, the free str dm velocity was set to I (m/s), the liqmid density WdP 1 OOO kg m3), md the vapor density was I kgm3) For most computations, fhe liquid vicosity was then set equal to 10 3 P~s), md that of the gas phcses was set to 10 5 Pc-s) Then the body diameter was chosen to ahieve fhe desi ed model R y olds m mber In fhe case of the hemisphericcl forebody rm et c body didmeter based R y olds m mber of 1 36xl 07, the liquid kir matic viscosity was then set equal to 10 5 3

OCR for page 426
(Pa-s), and that of the gas phases was set to 10-7 (Pa-s). The model body diameter for this case was thus, 0.136 (m). Prior to initiating unsteady computations, for purposes of computational expediency, a steady state, At = no, integration was carried out. At the completion of this integration, it was possible to determine if the model solution was physically unsteady. In general, physically unsteady conditions were indicated by marginally convergent, flat-lined steady-state residual histories, themselves containing large amounts of unsteadiness. .. ~ —i s —1 · _ ~ - 1 ~ _ Figure 1: Zero caliber ogive in water tunnel at Re(D)=2.9xlO5, 0=0.35 (approximate) (Stinebring, 1976). A photograph of a O-caliber axisymmetric cavitator operating at conditions similar to those modeled here is given in Figure 1 (Stinebring 1976) Figure 2 contains a series of snapshots of the volume fraction field from an unsteady model computation of flow over a blunt cavitator. Here the Reynolds number (based on diameter) was 1.46x105 and the cavitation number was 0.3. The time history for this case is given in model seconds, and at t=O, unsteady integration was initiated after obtaining a steady-state, At = no, initial condition. Thus it is expected that there was some start- up transient associated with initialization from an artificially maintained set of conditions. For the volume fraction contours, dark blue indicates vapor, a liquid volume fraction of less than 0.005, and bright red indicates liquid, a volume fraction of one. Some significant numerical integration time parameters for this case are the body diameter to free stream velocity ratio, D/Uo<' = 0.146 seconds, and the physical integration step size, At = 0.001 seconds. This result is presented over an approximate model cycle. The figure also includes the corresponding time history of drag coefficient. Note that the spikes in drag near t=37.725 and t=38.925 seconds correspond to reductions in the relative amount of vapor near the sharp leading edge. This marks the progress of a bulk volume of liquid from the closure region to the forward end of the cavity as part of the reentrant jet process. Although far from regular, these spikes also delineate the approximate model cycle. This picture serves to illustrate the basic phenomenon of natural sheet cavitation as it is best captured by UNCLE-M. This result is notable for the spatial and temporally irregular nature of the computed flow field. Even after significant integration effort, a clearly periodic result 1.~: v ~ . 1.4 1.1 t (s) Figure 2: Modeled flow over a O-caliber ogive. Liquid volume fraction contours and corresponding drag history. UNCLE-M result. o=0.3. ReD=1.46xlO5. 4

OCR for page 427
had not emerged. Thus, to deduce the dominant frequency with some confidence, it was necessary to apply ensemble averaging. An examination of the flow pattern captured suggests qualitative validity. Note, in Figure 2. that over a significant portion of the sequence, the leading, or formative, edge of the cavity sits slightly downstream from and not attached to the sharp corner. In their experiments, Rouse and McNown (1948) observed this phenomenon. They suggested that this delay in cavity formation was due to the tight separation eddy which forms immediately downstream of the corner and, hence, locally increases the pressure. The corresponding evolution of cavitation further downstream, at the separation interface, was proposed to be due to tiny vortices. These vortices, after some time, subsequently initiate the cavity. Figure 3 shows a single frame at t=37.8 seconds from the same model calculation (as shown in Figure 24. Here, to clarify what is captured, the volume fraction contours have been enhanced with illustrative streamlines. Note that these are streamlines drawn from a frozen time slice. Nonetheless, if all of the details envisioned by Rouse and McNown were present, the streamlines should , indicate smaller/tighter vertical flows. The current level V of modeling was unable to capture small vertical structures in the flow. However, the overall computation was apparently able to capture the gross affects of these phenomena and reproduce a delayed cavity. In fact from examination of the cavity cycle evolution shown in Figure 2, and the streamlines shown in the snapshot, it appears that gross unsteadiness is driven by a combination of a reentrant jet and some type of cavity pinching (Brennan 19924. The pinching process is particularly well demonstrated in Figure 2 from t=38.125 to 38.325 seconds. However, rather than complete division and convection into the free stream, it should be noted that, in later frames of Figure 2, the pinched portion of the cavity appears to rejoin the main cavity region. Figure 3: Snapshot of modeled flow over a O-caliber ogive. Liquid volume fraction contours and selected streamlines. UNCLE-M result. o=0.3. ReD=1.46xlO5. The low frequency mode apparent in most of the experimental O-caliber results appears to have been captured at the lowest cavitation number (~=0.3), as shown in Figure 2, and is evidenced in the test photograph (Figure 14. In Figure 4, the drag coefficient history for a 40 model second interval from the same computation as in Figure 2 is shown. Here, a clear picture of the persistence, over a long integration time, of the irregular flow behavior is documented. At higher cavitation numbers, the current set of O-caliber cavitator results indicate a more regular periodic motion. This is contrary to the experimental data. However, as Figure 3 indicates, the ability to capture this motion at any cavitation number may not necessarily require the explicit capture of the finer flow details of the vertical flow structure. This is encouraging and suggests that with increased computational effort, without altering the current physical model, the representation of this phenomenon could be improved over a greater range of cavitation numbers. 1 f 1.' t (s) 40 Figure 4: Model time record of drag coefficient for flow over a O-caliber ogive at ReD=1.46xlO5 and o=0.3. In model units, D/U~ = 0.146 (s), physical time step, At = 0.001 (s). Figure 5 presents the spectral content of the result given in Figure 4. This power spectral density plot is based on four averaged Hanning windowed data blocks of the time domain result. To eliminate the start- up transient effect, the record was truncated, starting at t=10 seconds and, to tighten the resulting confidence intervals, more time domain results, after t=40 seconds were included. As is typical of highly nonlinear sequences, the experience of this unsteady time integration demonstrated that, additional time records merely enrich the power spectral density function. However, the additional records do serve to improve the confidence intervals, and, therefore, add reliability to the numerical convergence process. The model result used, was, as indicated by the confidence intervals, sufficient for a comparison to experimental, unsteady results. Figure 6 contains a time record of drag coefficient during modeled flow over a O-caliber ogive at a Reynolds number of 1.46x105 and cavitation number of 0.35. The Strouhal frequency based on this result is 0.0909. Here it is apparent that the computational modeling was incapable of reproducing 5

OCR for page 428
a' 3 CAL, 2.5 ¢ 2 V 4 35 . . 1.5 ~ o O ~ ~ 4 f (Hz) 6 8 10 Figure 5: UNCLE-M result. O-caliber ogive at ReD=1.46xlO5 and o=0.3. Power spectral density function with 50% confidence intervals shown. what should have been a lower frequency result with flow around the forebody dominated by a more irregular cavity. It is supposed that the correct result, in comparison with the experimental data in the Strouhal frequency plot (Figure 22) would have been similar in nature to the results presented for a cavitation number of 0.30 in Figure 4. In addition to lacking the rich frequency content of the result for lower cavitation numbers, it appears that the amplitude of the unsteadiness present is an order of magnitude lower. 1.171r 1.1705 1.1695 ~ ~9 1.1685 Figure 6: UNCLE-M result. Time record of drag coefficient for flow over a O-caliber ogive at ReD=1.46xlO5 and o=0.35. In model units, D/Uo<' = 0.146 (s), physical time step, At = 0.001 (s). Figure 7 contains a series of snapshots from the unsteady model computation of a hemispherical cavitator at a Reynolds number (based on diameter) of 1.36x105 and a cavitation number of 0.2. This result is presented over a period slightly longer than the approximate model cycle. In this case the model Strouhal frequency is 0.0326. There are ten frames presented, and the first (or last) nine of those ten constitute an approximate model cycle. The drag history trace in Figure 8 demonstrates how, relative to the modeled flow over the blunt forebody, the pattern of flow over the hemispherical forebody is regular and periodic. This is consistent with experimental observations made (for example) by Rouse and Figure 7: Liquid volume fraction contours. Modeled flow over a hemispherical forebody and cylinder. UNCLE-M result. o=0.2, Re(D)=1.36xlO5. Mcnown (19484. Note the evolution of flow shown in Figure 7 as it compares to the drag history shown in Figure 8. As would be expected, the large spike in drag corresponds to the minimum in vapor shown near the modeled t=1.6 seconds. The next three figures demonstrate the expected and captured dependence of Strouhal frequency on cavitation number. Here the trend of increasing cycling frequency with cavitation number during flow over a hemispherical forebody is reproduced. The result has been demonstrated at a Reynolds number of 1.36x105. This Reynolds number was intended to scale the problem properly with the data available. Here, the magnitude of the drag and the amplitude of the unsteadiness may be examined. Figure 9 contains a time record of drag coefficient during modeled flow over a hemispherical forebody and 6

OCR for page 429
lo is t (s) 1 1 30 3s Figme 8 Unsteadyd agcoefficient Flow over6 hemispheric6 I forebody 6md cylmder UNCLE-M res flt 3=0 2, R ~)=1 36xl 05 in model mits, D/U== 0136(s),physic61timestep,At = 0001(s) cylmder 6t 6 Rey olds mmber of 1 36xl05 6md c6 itation n mber of 0 25 The Stro~l frequency based on this resflt is 0 0484 Figme 10 contams 6 simil6 time record of d 6g coefficient durmg modeled flow over 6 hemispheric61 forebody 6md cylmd r 6t 6 " ~' R y olds n mber of 1 36xl 05 6md cavibtion n mber of 0 30 The Stro~l fiequency based on 6his resflt is 00622 Figure 11 contains 6 time record of dag 0465 coefficient durmg modeled flow over 6 hemispheric61 forebody 6md cylinder rt 6 Rey olds m mber of 1 36xl05 6md c6 itation mmber of 0 35 The Sho~l f~equency b6 sed on 6his re mlt is 0 0933 in 6 ddition, 6he higher 3, higher fiequency ~esflts co tain sm611er c6 ities in 6hese sit rti ms, c6 ities d ive the over611 msteadiness of the flow, 6md 6he problem of s fficient g id pomts to defme 6m msteady c6 ity becomes 6pp6 ent Th3s, by p3shing the limits of ~easom~ble discretization, 6he limits of effective modeling also 6re te ted Figme 12 contams 6 time lecord of dag coefficient durmg modeled flow over 6 hemispheric61 forebody 6md cylinder rt 6 Rey olds m mber of 1 36x105 6md c6 itation n mber of 0 3 Th Stro~l f~equency based on 6his resflt is 00614 Figme 13 contains 6 time record of d rg coefhcient during modeled flow over 6 hemispheric61 forebody 6md cylmder 6t 6 Rey olds mmber of 1 36xl07 6md c6 itation n mber of 0 3 The Sh o~l f~equency based on this remit is 0 133 Here, 6he stamd6 d t~end of inmeased turbflent cycle fiequency with increased R y olds m mber mpe6 s to have been p~esented Figme 14 contams 6 time lecord of dag coefficient durmg modeled flow over 6 conic61 forebody 6md cylinder rt 6 Rey olds m mber of 1 36xl05 6md c6 itation n mber of 02 Th Stro~l f~equency b6 sed on 6his res flt is 0 0383 As 6mticipa ted, due to the expected stability of c6 ities 6bo 3t this 7 04 _ 044 ll 04 1e 043 043 Figme 9: UNCLE-M res flt Time record of d 6g coefficient for flow over 6 hemispherical forebody 6md cylmderatR D=1 36xlO56md 3=025 ~model mits, D/U~ = 0 136 (s), physic61 time step, At = 0 0025 (s) 0 475 _ 20 Figme 10: UNCLE-M res flt Time lecord of d 6g coefficient for flow over 6 hemispherical forebody 6md cylmder 6tReD=1 36xl05 6md 3=0 3 Inmodel mits, D/U~ = 0 136 (s), physic61 time step, At = 0 0025 (s) shape, 6his model flow e hibited very regmbr cycling with little 6 dditiom~l sh ong compone ts from second6 Y modes Figme 15 contams 6 time record of dag coefficient durmg modeled flow over 6 hemispheric61 forebody 6md cylinder rt 6 Rey olds m mber of 1 36xl 05 6md c6 ibtion m mber of 0 25 This is 6moth r UNCLE-Mresflt;how ver,ratherthmthe tamd6 dk 3 mod 1, 6he RNG k-3 tmbflence model has been 6pplied For the h ml pheric61 forebody wi6h cylmd ic61 6fterbody, when 3smg the stmd6 d k 3 model, to obtain, during 6 complete d al time cycle, 6 reduction m the mstecdy residual of two orders of magmit3de, it was mfficient to 6pply 6 time step, At=0 0025 seconds However, wi6h the RNG k 3 m odel, to obt6 in the same ~eduction in 6he mste6 dy ~esid al, it

OCR for page 430
0 496 _ O AOA ~ 492 Figme 11: NCLE-M ~esult Time ~ecord of d cg coefficient for flow c er c hemispherical forebody md cylmder ctReD=1 36xl05 md 5=0 35 Inmodel mits, D/U~ = 0 136 (s), physiccl time step, At = 0 0025 (s) Figmel2: NCLE-Mremlt Time~ecordofdag coefficient for flow c er c hemispherical forebody md cylmderstRD=136xlO6 md 5=03 Inmodl mits, D/U~ = 1 36 (s), physiccl time step, At = 0 025 (s) was nes ssary to m c physiccl time step of 0 001 seconds Note that in this time hi to y hcse, there is c g est decl of m tecdmess The result mpears far less cohe~ent th m the st mdard k-7 re mlt given m Figme 9 The Sh o~l fieque sy based on 6his ~esult is 0 1855 Bcsed on 6he mecsured dsh (Stinebring 1983), this f~eque sy is far too high When cpplied for c higher cavitation n mber, 5=0 30, the RNG k'based model cgam requi cd c smeller time tep (O 001 mits) md predicted c Sh o~l f~eque sy of 0 068 Here 6he value is nearly th ssme es 6~t predicted by 6he model using the k~ turbule se mod I Clearly, the t~end based on these results is i sorrect it cppears that 6he current implementation of the RNG model hcs yielded ~esults consistent wi6h the k-7 model st one savitation m mber, 5=0 30, but et c 1ower value, the cycle f~eque sy is far g ester 6 m the t mdard k-7 modeled ~esult or 6he measured data it seems probable that wi6h finer time s &ilO 15 ~o t (s) Figme 13: NCLE-M result Time ~ecord of d cg coefficient for flow c r c hemispherical forebody md cylmder ctReD=1 36xl07 md 5=0 3 Inmodel mits, D/U~ = 0 136 (s), physiccl time step, At = 0 0025 (s) Figme 14: NCLE-M result Time ~ecord of d cg coefficient for flow over c comccl forebody md cylind r st R D=1 36xl05 md 5=0 3 Inmodel mits, D/U~ = 0 136 (s), physiccl time step, At = 0 0025 (s) md spcse di sretization. the cmrent RNG k-7 model implementstion wo 5d cchieve remits comparable wi6h the k~ mod I et cll cavitation n mbers As expected, the RNG model i sreased 6he owxcll m tecdmess of the ~esults How ver, the computatiorurl cost of 6he cunent res 5ts is checdy sig ffic mt, md based on 6he NCLE-M sohtiom obtamed thns far, md comparison to experimentcl data, little benefit mpears to be had from 6he cun ent cpp licati on of the RN G k-7 m o de l Whe~e mplic~ole, for 6he unstecdy ~esults presented he~e, the ari6 meticclly avemged re mlts h~ve been compmed to the ~esults of Rouse md McNswn (1948) Figme 16 contams c comparison for flow over the O-caliber savitstor. Figm~e 17 contains c similar comparison for flow owx c hem isphericcl cc itator, md Figme 18 contams c similar comparison for flsw over c 8

OCR for page 431
0 44s n~ 0 425 4, 8 t (s) FigmelS: NCLE-M tNGk-8turbulencemodel result Time record of d cg coefficient for flow over c hemisphericcl forebody md cylmder et ReD =1 36xl 05 md 5=025 ~model mits,D/U~ = 0136 (s),physiccl time step, At = 0 001 (s) i i\ i _ _ _ oomput diOn, GO 3 ~ ~ dd~G03 o ~ 1 i oomp d diOn, GO 4 o ~ T i ~ dd~G04 O Ll i i i v~o ~ I i i,~.~ i i O I i W O ? ~ ~ O~ i i 0 1 4 ~d 6 8 10 Figme 16: Flow owx c Occliber cavitator (s/d~rc ienf h over dismeter) Averaged m tecdy pressure computations mdmecsuredGtc Rouse mdMcNown 1 948) coniccl cavitatcr in ecch of 6hese figmes, 6he overcll pe formance of 6he cod setms to g nerclly cg ee with the Gh Clearly es the cavitation m mber is ~educed, the NCLE-M result tends fur6her fiom 6he mta For both the m mericcl md experimental ~esults, 6he a~emge initiction md temmim~tion pomt of 6he cavity may be deduced fiom 6his figme Accordingly, 6he ctility of the code to properly model the average cavity is well ~epresented in 6hese fgmes The a~emged pe formance over the Occliber G itator cppears better th m that of eithb of the others The pe fommance over the coniccl shape is the wor t it is clear th~t 6he fommation pomt of the average cc ity should be well defmed m the axisymmehic shapes wi6h dicontmoous os oc ,~o. ~ r ~ oomput diOn, G0 1 \ ~ dd~G02 . | oomput diOn, c=0 3 dd~G03 1 ' ~ t i i i o ~ 1 ~ s, i o ~ . --=~-t-~ o~ 04 . i i i 0 1 ~ 3 4 5 6 ~d Figme 17: Flow over c h m isphericcl ca vitator (s/d~rc ienf h over d smeter) Averaged mstecdy pressure computations mdmeaeuredGtc Rouse mdMcNown 1 948) o. v o. Ob oomput diOn, GO 3 06 ~ dd~G03 0 4 oomput diOn, GO 4 ~ ~ dd~G04 O? :~. . i i _ O ~ ''~'~ O ~ ':,~' ~ ~ - ~ .~iL . 0 ~d ; Figm~e 18: F!ow owx cconiccl G itator (sM~rc ienf h overd~smeter) Avemged mstecdypressure computations mdmeaeuredGtc Rouse mdMcNown 1 948) Severcl parsmeters of ~elevance m 6he charcterization of cavitation bubbles inchde body dismeter, D, bubble ienf h, L, bubble dismetb, dm, md fomm d cg coefficie t cssocicted wi6h th cavitator, Cd Some smbig ity is mherent m both the expb imentcl md computatmrurl dehmhon of the ktter th ee of these parsmeters Bubble closme location is difficult to defne due to mstecdmess md ~ts dependence on diter- body d6smeter (which c m r mge from O [isohted camtator] to the camtator d~smeter) Acccrdmgly, bubble length is often, md he~e, tskb es twice 6he 9

OCR for page 432
distance from cavity leading edge to the location of maximum bubble diameter (see Figure 194. The form drag coefficient is taken as the pressure drag on an isolated cavitator shape. For cavitators with afterbodies, such as here, the pressure contribution to Cd associated with the back of the cavitator is assumed equal to the cavity pressure (- Pv) For the model computations, dm is determined by examining the al = 0.5 contour and determining its maximum radial location. In Figure 20, the quantity L/(DC4/2) is plotted against cavitation number for experimental data sets assembled by May (19754. Arithmetically averaged UNCLE-M results are included for ten unsteady computations made with three cavitator shapes. The correlation between L/(DC4/2) and ~ has been long established (see Reichardt (1946), Garabedian (1958), for example). Despite the significant uncertainties associated with experimental and computational evaluation of L and CD, the data and simulations do correlate well, close to independently of cavitator shape. ~.................... Figure 19: Definition used to determine bubble length, L, and diameter, dm. loot , , ,,,,,, I i 1 0 . . . . . . ... . . . . . . . . . . . . . . . ::::::::::::: .................... .. . ~ :::::::: ...................... . ....... ....................... : : : : : ::: 1 0° lo-2 lo-l 10° UNCLE-M hemisphere UNCLE-M O-caliber UNCLE-M cone data sphere data stagnation cup data cone Figure 20: Dimensionless drag to bubble length parameter and cavitation number. Flow over axisymmetric cavitators. Arithmetically averaged, unsteady UNCLE-M results and data (May 19754. Another parameter that has been established to be well correlated with cavitation number is the fineness ratio, L/dm. May (1975) noted that this parameter is particularly independent of ambient pressure, vapor pressure, free stream velocity, and whether the cavity was filled with vapor or a mixture of vapor and air. Once again, May assembled a large quantity of experimental results for this parameter. Figure 21 contains a comparison of the fineness ratio, L/dm, for averaged unsteady UNCLE-M computations and data. As a blanket observation, the spread of data between the experiments and computations in Figure 22 appears to be rather large. However, there are several encouraging items to be reviewed. It is clear that (for a given cavitation number) the computational results are bounded by the experimental data, and the proper trends (rate of change of Strouhal frequency with cavitation number) are well captured. More insight into the physical relevance of the data requires examination of specific results. 2 lol 10° 10 -- O UNCLE-M hemisphere UNCLE-M O-caliber ~ D UNCLE-M cone --I + data cone -I -- X data stagnation cup ~ ~ data sphere ~ + data disk ~ 10-2 ~ 10 10° Figure 21: Cavity fineness ratio and cavitation index. Flow over axisymmetric cavitators. Arithmetically averaged, unsteady, UNCLE-M results and data (May 19754. When run at similar cavitation numbers, the extremely low frequencies observed in the 0-caliber ogive testing was not captured by the model. However, considering only model results at a cavitation number of 0.3 (see Figure 4), it appears that the observed of behavior was captured. Figure 22 contains a large survey of unsteady computational and experimentally obtained data (Stinebring 19834. The numerical results in this figure summarize this validation effort. Here, Strouhal frequency is shown over a range of cavitation numbers. Computational results are given for hemispherical, 1/4- caliber, conical, and 0-caliber forebodies. Unsteady experimental data is included for the hemispherical, conical and 0-caliber shapes. Computational results for the hemisphere, 1/4-caliber and conical forebodies, were obtained at a Reynolds number based on diameter 10

OCR for page 433
of 1.36x105. For the O-caliber ogive, computations were made at a Reynolds number of 1.46x105. In addition, for the hemisphere, results are included for Reynolds numbers of 1.36x106 and 1.36x107. The experimental results included in the figure were obtained at Reynolds numbers ranging from 3.5x105 to 1.55x106. 0.5 0.4 hemisphere ReD=(0.35-1.55)xlO O-cal ReD=(0.96-1.46)xlO5 cone ReD=3.9xlO5 model 1/4 calReD=1.36xlO5 model O caliber ReD= 1 .46x105 model hemisphere ReD=1.36xlO5 model hemisphere ReD=1.36xlO model hemisphere ReD=1.36xlO7 model cone ReD= 1.36x105 0.3 0.2 0.1 _ 0 0. `1' - - · ~,~ & ~ 0.2 0.3 0.4 0.5 Figure 22: Axisymmetric running cavitators with cylindrical afterbodies. Strouhal frequency and cavitation number. UNCLE-M results (open symbols) and data reported in Stinebring (19834. For the hemispherical forebody results, as may be seen in Figure 22, there is a significant but almost constant offset between the measured unsteady data and the modeled results both of which appear to follow a linear trend over the range presented. An interesting result occurs in the model data for the hemispherical forebody with a Reynolds number of 1.36x107 (pentagrams in Figure 224. Here the numerical results appear to agree quite well with the experimental data for hemispherical forebodies. The experiments were taken at an order of magnitude lower Reynolds number, but the agreement is apparent in both cases where model results have been obtained. For design purposes, this may suggest an avenue towards model calibration. Another result found in the Str versus ~ plot (Figure 22) is the tendency of the modeled flows to become steady at higher cavitation numbers. For the 0- caliber or the conical cavitators, this is the reason model results are not included for cavitation numbers greater than 0.4. For the modeled hemisphere, the upper limit of cavitation number to yield unsteady model results was found to be Reynolds number dependent. At a ReD=1.36xlO5, the maximum cavitation number yielding an unsteady result was on 0.35, at ReD=1.36xlO6, that number was ~ ~ 0.45, and at ReD=1.36xlO7, the maximum cavitation number for unsteady computations was not determined. This result may indicate a limit of the computational grid applied to the problems rather than a limit of the level of physical modeling. In addition, physically in the mode of unsteadiness present, a transition does occur from cavity driven to separated, turbulent, but single phase driven flow. For the conical forebody, the datum shown in Figure 22 suggests that the cycling frequency should be higher, 0.123. It is worth considering that the Reynolds number of the experimental flow was 3.9x105 and that the general trend with increasing Reynolds numbers is to increased frequency. However, based on the standard level of dependence of Strouhal frequency (see Schlicting 1979 for example) on Reynolds number for bluff body flows, it would seem unlikely that the rate of change in frequency with Reynolds number (at ReD~ 105) would be as high as three to two. In addition, compared to shapes with geometrically smooth surfaces, the nature of unsteady flow over a conical shape is not expected to be nearly so dependent on Reynolds number. In the case of a cone, at low values of cavitation number (i.e. o=0.3), the separation location, and, hence, the likely forward location of the cavity, is rarely in question. A trend that is captured in the model results but not represented in the experimental data included here, is the tendency for the Strouhal frequency of a given cavitator shape to exhibit two distinct flow regimes. The first regime exists at moderate cavitation numbers and is indicated by a low Strouhal frequency where the value of Str will have an apparent linear dependence on is. The second regime tends toward much higher cycling frequencies. Here the dependent Strouhal frequency appears to asymptotically approach a vertical line with higher cavitation number, just prior to the complete elimination of the cavity. This is documented in Stinebring (1983) and demonstrated in Figure 22 for the modeled hemisphere at ReD=1.36xlO6. Based on the model results, it appears that this is characteristic of a change from a flow mode dominated by a large unsteady cavity to one dominated by other, single-phase, turbulent, sources of unsteadiness. During this investigation, some effort towards the establishment of temporal and spatial discretization independence was made. As a requirement of the model, to accommodate the use of wall functions, for regions of attached liquid flow, fine-grid near-wall points were established at locations yielding lO OCR for page 434
(sh wn) flequ n ies, 6here was very similar modal behavior Unfortmutely only 6he fin -g id models t nd d to pro ide umstecdy remits Thus time md spaticl fidelity w re indged mdependently A demonstmtion of the tecdy-state spaticl convergen Of the modeled coniccl forebody md cylind iccl dfterbody is given m Figme 24 m~ V I O Figme 23: Spectrcl comparison of effect of phy iccl integ ction time step si:D: on Cd history UNCLE-M ~esult Flow over c hem i phericcl forebody wi6h cylind iccl sfterbody R D=1 36xl05 5=0 3 o ~ = Medium Gnd l \ 1 \ ~ ~ 1~ . \ 1! I // I . . I . . I . . I . . I 0 1 ~ 3 4 5 s/d Figme 24: Comparison of p~edicted su f cc p~essme dish~butiom fornatucllycavitsti gaxi mmetric flow over c conical cavitator with cylind iccl sfterbody. 5 = 03 Coarse(65xl7),medium(129x33) mdfin 257x65) mesh solu i ms are plotted It should be noted 6~t du mg this investigation, stesdy tate res its (time mtegations based on ~t = = ) usmg UNCLE-M have been foumd to be quite comistent with arithmeticclly averaged time- dependent results This ~esult is expected to be u eful m expeditmg the fuu e mtemretation of complex 6 ee- dimensional flows in cddition, reel si gle phcse flows, et the R y olds numbers considered, over these axi mmetric bodies cc in fct umstecdy Howewx, with the g ids md level of modeling cpplied he~e, 6he UNCLE-M solutmns tended to be stecdy it seems poss~ble that in recsed resolution md in omorction of low R y olds number tmbulen e modelmg w mid resolve 6his issu Conclusions The effect of Rey olds m mber on the ~esults for 6he h misphericcl cavitator was not mticipated it was cssumed that with the cppropricte mplication of the high Rey olds number tmbul nce model et th wall, the inviscid extenurl flow would dominate the flow- field, determinmg cavity shape md si:D: (ie suLce pressue) How ver, it cppears that shong flow-field interacti ms du to the highly tmbulent separcted closure ~egion are impo t mt to determming 6he umstecdy mode To some extent, based on the avemge re mlts, these phenomena are being ecu stely ccptmed How ver, there are shortcommgs m 6he cunently employed level of single-phcse tu bulen e modelmg The validstion cases e smmed have demon trsted the ccpabilities of UNCLE-M over c rmge of importmt flow conditions The most promin nt ~esult for validation is that th umstecdy flequ n ies obtain d in mmmericcl remits cppear to be boumded by 6he experimentcl data of Stmebrmg (1983) for cll the mod led cases ther quclitative observations mcd regarding 6he modeled case of the Occliber cavitator et c cavitati m m mber of 0 3 mggest that UNCLE-M hcs 6he ctility to ccrrectly represent 6he overcll natme of umstecdy. complex, multiphcse flows without n cessarily ccptu ing some of the fmer flow detsils This m itseif is c validsti m of the cpproach tak n h re Validsted mod Img based on parsmeters reiated to profile d cg, cavity ienf h, cavity shape, md t~ends of Stro~l flequ n y with cavitation m mber hcs been cc mplished it seems clear 6~t wi6h hig)~er fidelity tubulen e md mass t msfer modeling md subsequ nt improved modeling of the closme ~egion, c ben flt to 6he modelmg of umstesdy cavitating flows wo id be obtcin d How ver, 6he cunent cpprocch has cllowed rendering of unstecdy multiphcse flows et R y olds m mbers relev mt to engin ering cpplications in c m odeling method smenable to compl :x geomeh ies md des~g cpplcatmns The cuthors contmu to develop 6he ccp~oilities of UNCLE-M This in ludes the pu suit relev mt validation cases for compl :x th ee-d6m nsional flows in cdditi m, n w levels of physiccl modelmg, such es compressible phcses vie isodhermcl md full en rgy modeling, will be in crporcted These n w ccp~oilities, in cddition to 6he cl~ecdy in crporcted ctilities to model buoyancy md ventilation, cc criticcl 12

OCR for page 435
to c cunent research goal, fhe ful co figmation modeling of c high speed supercc itating vehicle umdergomg mcneu rs Acknowledgments This work is mpported by fhe Office of Naval R search, contmct kN00014-98-0143, wifh Dr Kam Ng es contmct monitor References Brennan, CE., Ccvit~tion md Bubble Dvrumics, O ford University Press, New York, 1995 Garabedfian, P.R., Colculation of Asiolly S mm tric CoviLes and Jet, Pao J. of Mcfh 6, 1958 Grogger, H.A. & Alajbegovie, A., Colculahon of the Covit tingFlowinVmturiGeom tnesUsingTw Fhid Model, ASME Pcper FEDSM 98-5295 1998 Jameson, A., Schmidt, W., & E. Turkel, Numencol SoluLons of theEuler Eg uoti ms byFinit VohmeMe6h od Using Runge Kutto Tme St pping Sch mes, A AA Pcper 81-1259, 1981 Kunz, Robert F. et al., Multi Phose CFD Anolysu of Noturol and Vmtilot d Covitohon obout Subm ged Bodies, ASMEPcperF DSM99-7364,1999~ Kunz, Robert F. et al., A Pnecondihoned Novier Stokes Methodfor Tw Phose Flow wi 6h Applicoh on to Covit tion Pr d icohon, A AA Pcper 99-3329, 1999 ([1) to be pub lished in Comruters md Fluids May, A., Wote r Ent y and the Covih Running Behov iour of Missles, Na val See Systems Comm md Hyd oballi tics Advisory Committee Techmiccl R port 75-2, 1975 Merkde, C.L., Feng, J., & Buelow, P. E.O., Computm tionol Modelingof th Dyn mics of SheetCavitotim, 3rd h temational Symposium on Cc itati m, G en ble, France, 1998 Orvag, S.A. et al., Rmo~lizohon GnoupModeling and Turbulence Simulohons, Near Well Tu bulent Flows, Elsevier Scien e Publishers B V, Amsterdam, TheNetherkmds, 1993 Reichardt, H., The ws of Covit tion Bubbles ot Asi ol ySymmet icol Bodies in oFlow, Mini try of Al cmft Produ tion Vo kem ode, MAP-VG R ports md Tr msk - tions 766, Of fice of Na~l R search, 1946 Rouse, H. & MeNown, J. S., Covitotion and Pnessu~e Dut ibuLon, Heod Forms ot 7em Angle of Y w, Studies in E gmeermg Bulletin 32, State University of lowc, 1 948 Sehdichting, H., Boumdarv-Lawv Theorv, M Gmw- Hill, N w York, 1979 Stindh ring, D.R., Bdlet, M.L., & Holl, J.W., An Inrer tigotion of Covi y Cycl ing for Vmtilot d ond Noturol CoviLes, TM 83-13, The Pemmsyl mic State University Applied Research Laboratory, 1983 Sthdhrhg, DR., Sccling of Ccvitation Dcmcg, M S Thesis, The Pemmsylv mic Sbte Uniwvsity, University Park, Pemm yl mi~, Augu t 1976 Taylor, L. K., Arahshahd, A., & WhdtfiAd, D. L., Unsteody Th ee Dimensionol IncompnessibleNoviem Stokes Computohonsfor o Pnolote Sphenoid Unde going Tm Dep md mtMoneurerr, A AA Pcper 95-0313, 1995 13

OCR for page 436
DISCUSSION '' Shyy University of Florida, USA Inthis pap u She mthorshave summari edavast amount of information resulting from Heir :- search in developing Ed refming c CFD tool for single- Ed multi-phcse flows The r suits have been impressive in particular, it seems that mm- less She fl O..- Is massively separated Ed or cavi- tated, the present CFD tool c m perform quite w 11, esp ciclly in temms of pressure coefficients Ed main time-dependent features The mfhors should be con hammed for their accomplish- ments to date With regard to the unresolved issues, Here are se- oral that or c m Rome First, the mule phs e. time dependent (for the ensemble averaged qu mtities) turbulent flowsis obviously e major challenge On the or h Ed, there me interactions between different physical mechsni ms which produce, dissipate, cormect, Ed diffuse the tur- bulent kmetic en rgy Ed the Rey olds shess compor nts, on the other h Ed, there is subst m- tial mass, momentum, Ed en rgy exch mge be- tw en liquid Ed vapor phases The resulting physical framework is extr mely complicated beyond what w have been Cole to pa diet with adequate co flder e There is no quick, prscti al solution to handle this challenge How ver, to the least, models capable of hurdling (i) sub- st mticl depart r from quilibrium betw en pa - duction Ed dissipation of the turbulent kinetic en rgy, (ii) misohopy between mom Rey olds sin ss compor nts, Ed (iii) turbuler e-erJkmced mass tr m fer across the phase interface, should be emphasized The second issue is related to the r ed for ~ - solvmg the liquid-vapor boundary with due accu- racy This issue is difhcult to h mdle bee mse the interface's location, shape, Ed velocity must be computed es part of the solution, resulting in c syst m that doesn't have either c pa determir d co figuration geometrically, or c fixed mass, momentum Ed en rgy budget withm its domain A accurate Ed robust interface tracking sch me c m help improve She performance of the present CFD tool The third issue is related to the mmmericcl eb- ments, in luding feet res such es dynamic cdap- tation of the grid to help mcmtam den tble resolution, satisfactory conhol of mmmericcl dis- persion Ed dissipation in view of the highly cormective multi-phcse flows, Ed way to e. p e- dite Ed tabili e the computttior~tl procedures Suffice it to say that She hors have Greedy developed c highly impressive Ed effective CFD capabilities in each of She issues discussed clove, efforts are being made to help f rther improve its performance in various difhcult Ed import mt application areas To help develop these advanced cmctilities, or mu t appreciate the r ed for acquiring experimental i fommation withadequcteresolution md compreh nor en ss For example, t rbulent qu mtities, precise mter- face deli nmn Ed con- ffnon-d~flunon ratios are some key i fommation Nat to date, we have not been Cole to document based on it tt-htnd experimental i formation Author's Reply: Professor Shyy has made several valuable com- ments regarding She difficulties of resolving complex, multi-phcse flows With r gard to his suggestions for improved turbuler e mod in ~ the mfhors suspect that She in orporction of such models lies in the futur of fi is Ed other Rey- nolds-Averaged Na vier-Stokes based efforts The mthors pram to continue to incorporate improved turbuler e mod leg in addition, the mthors hope to in orporcte some better form of turbu- ler e erJkmced mi ing Particularly of mterest to the mthors, in the context of She cure nt model- ing method, is the proper physics to apply m the preser e of multiple gaseous spemes Ed c smgle liquid species The mfhors consider the second Ed third issues raised by Professor Shyy to be r cessarily i Icted it is believed Nat, for complex en m ering co figurations, with current computstior~tl lim- its, c r ssor~tble way to ccpt re sheet cavities is by application of c method similar to what has been applied her; i e the interfaces to be ccp- tured will be c solution to the home en ous mint re flow equations, possibly with multiple species, mass h msfer, Ed equations of state Thus, the inte face will be finite Ed sharps ss will be grid dependent This is srLtlogous to the mo t popular methods of shock capt ring for en mee~mg purposes during modeling of com- pressible flows As Professor Shyy has noted, when such a method is combir d with grid td- sptition, signiflcmt improvement in solution quality may be achieved

OCR for page 437
DISCUSSION J. R. dwa do North Ca olina State University, USA This paper details the validation of c sophisti- cated CFD approach for modeling mcompressi- ble, unsteady cavitating flows Attention is cor- rectly focused on resolving the time-dependent aspects of cavity fommation Ed growth, es such processes are i herently unsteady Ed should be modeled es such The approach is shown to pa - diet time-averaged su face pressure distributions togoodaccord Discrpcnciesevider edmaybe c consequer e of the modeling but it mu t be kept in mind chat the Rouse Ed McNown date- base is over 50 years old, Ed measurement tech- niques have improved substmticlly over the years The model also predicts bubble shapes that correlate well with moo r cent experimental date, giving co fider e in its civility to resolve the buk features of axisymmetric sheet cavity Ho.. IN ids The unsteady validation of the model is pr- sented es plots of d cg coefhcient versus time, with dominant frequer ies exhacted fiom the signal by c spectral analysis While the corn et to nd of m in r use in He Strouhal mmmber with in r using cavitation mmmber is evider ed, the actual values are not in accord with experimental date The mfhors conjecture that These deviations may result from se- eral factors, in luding insuf- ficie t grid resolution particularly for higher cavitation mmmbers) Ed He quality of She turbu- ler~e model Factors that also could i Sued e these comparisons in lude again the quality of the experimental date Ed th ee-dimensior~l effects There is certainly no guar mtee that the cavity motion will rmcin axisymmehic over time 2 Some questions that might be posed to the mthors during She discussion section are as fol- Iows: I Are there my prams to rep at my of the ccl- culations es th ee-dimensior~l runs? It would be inter sting to see if the unsteady results ch mge 2 The ~ hors employ m empirical rate equation to model the con- erimn of liquid to vapor Ed vice verse es the pressure d ops below the vapor pressure How sensitive are She results obtain d to the rate coefficients, particularly es regards the fir e-a-em ed predictions? 3 The ~ hors note Nat " tecdy-state" r suits (using ve y large time steps) for surface pressure di tributions are "quite consistent with arithmeti- cclly averaged time-depffndent results" p 12) Does this comment apply to the wake predictions es w 11? It would appear that ccpt rmg the large- sccle motion of the re-entr mt jet would be e;- senticl in predicting he conect delayed r covery of the pressure I would fhmk Nat the "steady" calculations would predict c more cbmpt recov- ery In eon lusion, I find She mthors' work to be truly representative of the i~a~e-ol:~h -art in cavitation mod leg Only She extension to thee dimen- sions Ed the validation thereof is required b:- fore c high-fidelity tool for unsteady cavitation prediction will emerge Author's Reply: Professor Edwards makes insightful commentary regarding the th ee-dimensiorslity Ed tr msient nature of sheet cavitation it is clear that he has spent c greet deal of effort studying Ed model- ing such flows Responses to his th ee questions me listedbelow: l Subsequent to the comments of Professor Edwards, She mthors have begun to under- take some f ee-dimensior~l modeling of the ogive cases that w re originally mecs- ured experimentally by Rouse Ed McNow Farticlly completed results me included here in Figure A These results seem to indicate the preser e of thee-dimensiorsl modes How ver, c complete study, in luding sen sitivity to smell mgles of attack, was not reedy es of the time of the deadly for this reply The rate equation used for mass h msfer is c w ok Imk m our model However, it hr. been applied m c consistent maimer The rate coefhcient was original y chosen em- piricclly es or which produces cppro i- mately correct stecdy-state cavity si e for c given ogive et c specific cavitation mmmber After this initial calibration, She rate coeffi- cient hr. been left unch urged for all com- putations This consistent application of the rate coefhcient should allow results to be fauly sssest d No sensitivity study has been prefommed on d is value

OCR for page 438
3 The original eon lusions of the ~ hors :- gardmg the unsteady calculations r fleet c com- parison of the nme-c- em ed unsteady computed pressur field to the steady state computed pres- sure field on the surface of the ogi es Thus it appears to the mthors that the computed m steady motion of the reenh mt wake is captured in c maimer that approximates he computed steady- tate average Ed the average yielded by the datccollectedbyMcy DISCUSSION El. Fa fell ARL, The Per sylva la State Urlver- slty, USA First, I would I he to con r~mh~e my colleagues for m out t mding modeling effo t in the area of time-dependent multi-phase flows, which are of particular mterest in the hyd odyrumics of m- derwater high speed vehicles I cppl md Heir persister e to push Heir analysis to the realm of en m ering usefulr .., where He true utility of the computttior~tl tool c mbe realized The success of th simplified mass h m fer mo d- els is notable Whet is the r~tur of the higher fidelity mass tr msfer models that you are con- sidermg Ed their intended t en fit? Please di - cuss He relative merits of advanced turbuler e modeling versus mass tr msfer mod in g in im- proving the prediction of the unsteady cavity dynamics Author's Reply: The mfhors me pleased to receive such fa vorable commentary fiom Dr Farrell it was due to his expertise in the field of cavitation in eption Ed cavitation modeling that it was suggested that he be m in ited discusser Regrettably, the mthors have not been Cole to advance She physical quality of mass h msfer modeling beyond the simple rate coefficient based model presented in the text it is hoped that m in eption model may be developed with physics based on the Jaundice of cavitation mmclei in She flow This might be similar to work] thathcsbeendor byDr Farrell[1] The effect of turbuler e mod in g on the civility to capture c cavity flows is suspected to be strong Some of the short omings of the wall- fur tion based, two~quction approach when applied to single-phcse flows have been com- mented on here by Professor Shyy Ed elsewhere by Wilcox [2], Ed others A greet deal of :- search ht. been devoted to turbulent flows Ed turbulent modeling Thus, it is unlkely Butt. in the r ar future, c signifc mt improvement in applicable t rbuler e models will be developed In comparison, She mass h msfer model em- ployed is suppo ted by far less research Thus, it is su pected that, in the r ar term, improvements in applicable mass tr msfer mod leg will be found Ed in orporcted into She mmmericcl model it may then become clear whether im- provement in quality of r suits is cttcir~ble by improvement in mass tr m fer mod in g DISCUSSION R. Ar dt Urlverslty of Mlr esota, USA 1) How do you explain the discrepancy between frequer y of pulsing cavities d- temmmed mmmericclly Ed experimentally? 2) Have you carried out my crurlysis of partial cavitation on hyd of oils? Author's Reply: The mthors suspect Nat turbuler e mod in ~ mass transfer modeling, Ed th e-dimensiortl effects all contributed to the k k of absolute agreement with experimental unsteady r suits Of these possible avenues of improvement, the mthors have included some f e-dimensiortl results m Figure A A preliminary examination of these results do indicate the preser e of cddi- tior~l modes However, et the decdlme for sub- mission of f is reply, results are not yet com- plete The mfhors do also intend to apply the current Ed fur re version of the computstior~tl model on ocher en treeing co figurations including partially cavitatmg hyd of oils However nor of this modeling is yet complete DISCUSSION ]. Cc lk West Vlrglrla Urlverslty, USA Strouhal mmmber, i e the frequer y of the pn- mary vortex shedding, c m be easily pa dieted by RANS codes if they are 2 order in time A

OCR for page 439
more appropriate validation is to compare the centerline velocity variation in the value of a bluff body. The code treats volume fraction of gas as a pas- sive scalar and solves mixture momentum equa- tions with variable density. In this regard it is not truly a multi-phase flow code. The slip between the two phases were not accounted for, and this can have significant consequences. Author's Reply: The authors thank Professor Celik for his n- sightful comments. Unfortunately the centerline velocity data for the experimental results used for comparison was not available. The authors readily acknowledge that the absence of a slip model renders the method less capable of cap- turing certain cavitation phenomena. This would probably manifest itself in flows dominated by bubbles. However, flows that the authors have concentrated on here are essentially phase sepa- rated, actually sheet cavities. For this type of flow, it is hypothesized that the inability to prop- erly represent certain bubble physics is insignifi- cant. A wide range of cavitating flows may be properly represented by homogeneous, equilib- rium two-phase models. Successful researchers have modeled unsteady sheet and even cloud cavitation with homogeneous models: See, for example, Arndt, Song, et al. t34. In the current work, the volume fraction is not thought to be a passive scalar. Here liquid vol- ume fraction, id, is solved for in the liquid vol- ume continuity equation as a dependent variable. It appears in the momentum equations via the formulation of Am and m Mass transfer from liquid to vapor and from vapor to liquid takes place due to source terms in the continuity rela- tions. Thus ~ is fully coupled to and interde- pendent with solution of the flow field. If, for example, a different ~ field is created due to alteration of some flow condition such as Rey- nolds Number or cavitation number, the rest of the solution flow field will be significantly i- tered as well. DISCUSSION H. Kato, Tokyo University, Japan Estimation of vaporization/condensation rate is important when we analyze cavitating flow b=- cause it decides the amount of vapor in the flow. I'd like to know how the authors decided the mass transfer rate at the interface between vapor and water, and how the authors verified it. Author's Reply: The reply to Professor Kato's question has been given in the earlier reply to Part 2 of the ques- tions by Professor Edwards. Figure A: Three-dimensional, wall-function based, turbulent, unsteady, two-phase result. 1,245,184 cell grid. Modeled flow (from right to left) over blunt ogive (shown in gray) with an isosurface of volume fraction, ~=0.9, colored by velocity magnitude on a field colored by velocity magnitude. s=0.30. ReD= 1 .46x 105. Integration time step size Unit /D = 0.00685 a)Ut/D=6.85 b) U. t/D=10.27 Figure appears to show the capture of an ~n- steady and three-dimensional sheet-cavity flow.

OCR for page 440
References for Discussion: I Farr 11, K J. An Euleriar~/Lcgnmgi m ComPutationai Analvsis for fhe Prediction of Ccvitation in eption, Ph. D Thesis, D - putment of Mech miccl md Nuclear E gi- n ermg, Pemmsyl mic State University, August 2000 2 Wilcox, D C, Turbulen e Modeling for CPD, DCW Indushies, Lc Canadc, Califor- nr, USA, I 99S 3 A ndt, Song, et cl, Inst bilih of Portiol Covit tion: A Nurnericol/Experirnentol Ap prooch, ONR 23 Symposium on Naval Hyd odynamics, val de Reuil, Pmnce, 17-22 Septermber, 2000

Representative terms from entire chapter:

rey olds