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ESTIMATION OF HULL FORM EFFECTS ON WAKE WITH CFD-TOOLS

M. Hoekstra

Maritime Research Institute Netherlands,

Raagsteeg 2, P.O. Box 28, 6700 AA Wageningen, The Netherlands

ABSTRACT

Numerical predictions are presented of the viscous flOw around a ship, neglecting wave formation The results for two tanker hulls with different. aftbody shapes are compared. After a potential flow analysis, the viscous flow behaviour at the stern is examined. Limiting streamline patterns and velocity distributions are com-pared.. One of the hulls shows flow reversal ahead of the propel-1er, which the propéller action does not remove completely, as additional computations indicate This is sufficient reason to disqualify the design. Neither is the other hull form fülly satis-factory. Suggestions are given for the design of a third variant.

1. INTRODUCTION

Ship designing has a Strong bias towards traditionalism, i.e. it relies heavily on sùccessful hull designs of the past. But even if this often means that only small deviations from earlier hull forms are acceptable, a designer will Once in a while be facing the question: how does this conceived modification affec.t the wake of my ship? Of course, it is not so much the flow field itself that he is

worried about,. but rather the

cnse-quences for propulsive performance, rpm, risk of cavitation, vibration level, etc. However, wake field information is the basic requirement for an estimation of. these consequences.

The usual way of verifying the influence of design variations is by model

test-ing, but not until an advanced phase of the design process has been reached. Ai awkward situation may arise when the

tests show the deslÉn to be unsatisfac-tory: the later the .need for additional modifications comes up, the more costly

is their implementation.

Numerical flow simulations can help to reduce the risk of the designer's choices in an earlier design stage.

-1-Along with the impressive hardware

de-velopments of the last years, the dis-cipline of Computational Fluid Dynamics (CFD) has expanded and continues to pro-duce new or improved tools which can play a useful role, complementary to that of experimental investigation, in a design process. Prediction methods for ship stern flows form one class of tools which has matured considerably. If not yet quantitatively, in full agreement with experimental data, the results Of present-day wake prediction sóftvare can at least indicate the main trends añd the sensitivity of the flow to the hull form change.. The cost at which they are obtained is still appreciable, but there is a safe prospect of réduction In the future. Numerical stern flow prediction. will then be highly suited for

explora-tory work within the margins set by de-sign constraints and within the limited budgets availáble.

This paper gives an example of wake pre-diction by CFD. The flow around two tankers, differing only in aftbody shape,. is predicted and the results are discussed. Our aim is twofold: to show

the present capabilities of CFD in wake

prediction and to indicate how it can fruitfully be sed in designing via com-parative qualification.

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2. OUTLINE OF COMPUTATIONAL APPROACH Since not all readers will be familiar vith the current methodology in numeri-cal wake prediction., a concise introduc-.

t.ion to our approach of the problem may be appropriate.

The numerical simulation of the viscous flow around a ship, even under the sim-plest operating conditions of steady mo tion through still water, is undoubtedly an intricate matter. Although there is a. sound màthematical model (the Navier-Stokes equations for incompressible

flow), the solution for a given set of boundary conditions cannot be obtained without, restrictions. For instance, present-day computers do not allow dis-cretizations fine enough to resolve the small scale motions inherent in

turbu-lence, a phenomenon that always occurs in some parts of the flow field. Conse-quently, the high-frequency motions have to be removed and an estimate of their time-mean effect on the flow as a whole is to be made via a 'turbulence model'. Also the presence of the free surface is a complication, the characteristic dif-ficulty being the imposition of boundary conditions on a surface of which shape and location are to be obtained as a

part of the solution. Under the assump-tion that free surface disturbances have

'a negligible influence on the wake

dis-ttibution, we omit this problem by

treating the undisturbed free surface as

a symmetry plane (no waves; see ref. [1]

for examples how to deal with f

ree-surface problems under. inviscid flow assumptions).

Simplifications of the above kind imply more or less serious shortcomings in the physical representation of the flow.

They are distinct from 'another aspect: accuracy versus cost. It will be clear that any numerical discretization of the mathematical model implies a bound on the quantitative accuracy. With

increas-ing refinement of the discretization, the calculations become more accurate as wll as more. expensive. The cost of the. computations in relation to the quality

of the result is a critical factor for

acceptance.. Any means to reduce the

costs without deteriorating the result is therefore welcome. For the flow

around a ship, characterized by a high Reynolds number, a considerable

reduc-tion of, the computational effort is ob-tained by dividing the flow domainl into regions with different degree of flow complexity and by solving simpler qua-tions in the regions of 'simple' 'flow.

If the regions are properly chosen, this

d'oes no real harm to the quality of the physical flOw representation. In the

method to be used here, three zones are distinguished (Fig. 1):

zone I, the external flow region, .where the flow is assumed to be

invis-cid and irrotational;

- zone II, the boundary-layer region, covering the forward part of the hull, where boundary-layer theory

issup-posed to give añ adequate description of the flow;

- zone III., the stern-flow-and-wake region, where the Reynolds-averaged Navier-Stokes equations are. solved..

loe

Figure 1:

Division of flow field into three zOnes.

The solutions in the three zones cän be linked, by schemes of varying degree of interaction; here, the link has been assumed non-interactive., which is not completely correct but good enough for practical purposes. Solution Of the

ensuing reduced problem is feasible at present.

Thus, in order to predict the nominal wake of a ship, we calculate the f low

around a double model of its submerged part by a combination of three computa-tional elements: a potential flow code, a boundary-layer method and a stern-flow solver. The potential flow code is based on a boundary-integral method, employing

,a Rankine source distribution on the

hull surface. it supplies boundary con-ditions for the boundary-layer method and the stern-flow solver. The latter

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are both finite-difference methods, and require the generation of a grid in the space chosen for the calculation (zónés II and III respectively). To each grid node discrete values of the variables (velocity components ánd pressure) are assigned which are the unknovn tó be solved iteratively. The viscous flow methods are described in some detail in [2,3,4].

3. HULL GEOMETRIES

Results vilI be presented för two tank-ers which differ only in. the aftbödy shape. The main dimensions of both hulls are the same and are listed below:

Length between perpendiculars L = 253.0 m Breadth B

38.33m

Dra ugh t T = 14.20 ni Displacement volume V = 117000 rn Wetted surface S = 14755 in Block coefficient Cb = 0.85 Even the lengthwise position of the cen-tre of buoyancy has

been fixed at 32

pér cent of the ship's length ahead of midship for both hUlls. Most statistical drag prediction methods., based on módel

-3-test resúlts of the. past and describing

the hull gèóinetry in terms of global fotm parameters such as L/B, Cb, etc., would therefore not be able to indicate a preference.

The differences betveèn the two hull

forms are apparent in the frame shapes. The body plans and stern contours are compared in Fig. 2. Tanker 2 has pro-nounced U-type frame lines in the region directlyf ahead of the propeller. Those tanker 1 tend to b moré V-shaped. Moreover, the frame lines show a com-pletely different character in the upper stern region. The curves of sectional areas are only marginally different,

though.

Insiders will recognize the two hull

forms as the test cases for a workshop

on stern flow prediction, held recently in Sweden.

For later reference, a coordinate x is introduced here - pôinting from bow to

stern, and with the origin at the bow -by which a lengthwise pOsition along the hull can be indicated. Thus, x/L = O corresponds with the position of the fOrward perpendicular, x/L = i with the áf t perpendicular.

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4. POTENTIAL FLOW

In this section the results of the Po-tential flow calculations will be consi-dered separately. It may seem

paradoxi-cal to do so because the main Interest is in the wake, the structure of which is primarily determined by viscous ef-fects. However, it is to emphasize that the potential flow results - which are obtained at relatively low cost - give us a meaningful global impression of the flow around the hull. Moreover, they usually allow some qualitative

specula-tion on the behaviour of the viscous f low.

As mentioned earlier, the potential flow calculations have been carried out with a Rankine source panel method. Approxi-mately 2000 panels were distributed over the submerged part of the hull, with a

concentration of panels on the aftbody.

Fig. 3 shows the calculated streamlines on the hull surface, while the pressure distributions are given in Fig.

4.

These results indicate some small but

important differences.

In the lower stern area, the streamlines are more bent for tanker 2; in the upper stern area an opposite effect can be observed. The pressure distributions confirm that tanker 2 has a more pro-nounced aft shoulder: at the end of the parallel midbody, the pressure is lower near the waterline. For both hulls, a depression is found in the bilge region just ahead of the stern, but it is stronger for.tanker 2. This is relevant

(a) Tanker i

for the wake distribution because these depressions are related to the formation of longitudinal vortices.

The above, results have been obtained under the assumption of the fluid being inviscid. What can be said in

anticipa-tion about the behaviour of the real

(viscous) flow, merely on the basis of these potential flow data?

Let us first recall some basic facts about boundary-layer development, by considering four classes of flpv in

order of increasing complexity:

a. The thickness of a two-dimensional boundary layer on a flat surfacé will slowly grow in the streamwise

direc-tion. That is because momentum is needed to overcome the

fricjonal

forces.

b If the flat surface is replaced by a

two-dimensional displacement body, an additional effect occurs: there is a pressure variation over the body. A favourable pressure gradient (from high to lw pressure) tends sup-press the rate of thickening of the boundary-layer, an adverse pressure gradient to enhance it.

c. Another feature enters when

aisym-metric bodies are considered, viz.

convergence or divergence.of

stream-lines. Diverging streamlines - as over the front part of the body - act to reduce the growth rate., convrging streamlines to increase it.

(b) Tanker 2 Figure 3: Streamlines along the hull in potentiàl flow.

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(a) Tanker i

(b) Tanker 2

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d. We finally make the step to a three-dimensional body like a ship. All above effects are present, but in ad-dïtion there are lateral pressure gradients. They imply streamline cur-vature in planes locally tangent to

the hull, but also cross-flow in the

boundary layer. This can be made un-derstandable as follows. To first approximation the pressure is uniform in the boundary layer along a normal to the hull, and hence the lateral pressure gradient too. At the outer edge of the boundary layer the veloc-ity is high and only a slight stream-line curvature is sufficient to bal-ance the pressure gradient by a cen-trifugal force. Inside the boundary layer the speed is lower and more streamline curvature is required for

- a balance (near the surface, shear

forces assist the centrifugal förce to balance the pressure force, pre-venting the streamline curvature from becoming infinite). It follows that the direction of the flow near the hull surface can differ significantly from .the direction of the outer-flow streamlines (Fig. 5).

STREAMWISE VOCrTY. pço

W4LL CROSS . ANOLE

Figute 5:

Cross-flow in a boundary layer.

When these simple rules are applied to

the present potential flow data, some features of the viscous flow can readily be predicted. The pressure rises towards

\ VLcITY PROFILE

CROSS - WISE

the stern, particularly ovér the last ten per cent of the length, so that a rapidly growing boundary layer can be expected there. But the streamlinés are seen to diverge strongly from thè keel, whence the boundary layer growth along the keel line will be suppressed. Qn the other hand, they converge along a line along the hull just above the conavity in the frame lines. Accordingly, the

boundary layer is expected to be

rela-tively thick there..

Appreciable streamline curvature (in

planes tangential to the hull surface) has been observed also, notably over the foot of the stern frames, and at the

stern close to the waterline where the streamlines bend upwards. The flOw in-side the boundary layer can be predicted to bend in the same direction but more than the potential flow streamlines do. As cross-flow develops, the near-surface

flow streamlines will converge at quite another place as the outer-bounary-layer flow does.

Thus, by potential flow calculations alone, a qualitative picture of the global boundary-layer behaviour can be established. I.n order to go beyondthis qualitative guess., we have to enter the domain of the viscous flow calculations.

5. VISCOUS FLOW

Where an ideal fluid can slide over the hull surface, a real fluid adheres to it, causing the formation of a boun4ary layer. The development of this boundary

layer over the forward portion of the hull has been simulated, assuming fiFst_ order boundary-layer theory to apply.

Aft of station 7 (at 65 per cent of' the ship's length), we adopted a slightly reduced form of the Reynolds-averaged Navier-Stokes equations as the mathema-tical model. The calculations have been carried out at a. Reynolds number Rn = 5*10 , which is typical for the

experi-mental situatiOn in a towing tañk.

Let us concentrate immediately on the

results in the stern region.. Consider

first Fig. 6(a)., displaying the

disttri-bution of the longitudinal (axial) ve-locity component for tanker 1 at xII. =

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varïa-tion of the boundary layer thickness along the girth. In accordance with the speculations in the previous section, .a bulge appears just above mid-girth, while the boundary layer is very thin at the keel. It is also thin at the water-line, which is a transverse curvatúre effect: the angle betveen..vaterline and frame line increases tovads the stern, implying that more space

becomesgrad-uaily available for the fluid near the waterline, which has a thinning effect on the boundary layer.

The corresponding results of tanker 2 in Fig. 6(b) indicate similar tendencies, but there are already small differences in the flow structure (e.g. the boundary layer at the keel is thicker, and lower near-hull velocities are found near the concavity in the frame line).

To get an overall impression of the be-haviour of the flow close to the hull sürface, visualization of the hull shear stress direction (limiting streamlines) is helpful. The experimental equivalent is the 'paint test'. The computational results are presented for the two hulls

in Figs. 7 and 8. tn Fig. 7 'tufts' are

used to indicate the direction (not the magnitude!) of the local skin frictIon

1.0

vector in a side view; Fig. 8 shows the limiting streamlines as derived from such a tuft plot, but now in a rear

vi ev.

A comparison with the potential flow streamliñes - which are representative for the flow direction in the outer part of the böundary layer - reveals appreci-able differences, indicating the strong three-dimensionality of the flow. Both hulls show a confluence of limiting streamlines in the lower stern region which marks the origin of a longitudinal vortex, On tanker 2 there is in addition a congestion of limiting streamlines in the upper stern region, along an almost horizontal line. But the flow behaviour in its neighbourhood is quite different since it is a line of flow attachment (limiting streamlines are pointing away from it, not towards it).

The most significant difference is of course the flow reversal at the stern of tanker 1, which has been avoided on tanker 2 by moving the stern post aft. Notice, however, that there is a region

on tanker 2 as far upstream as x/L =

0.9, where the flow is close to

rever-sal. Recovery from this near-calamity occurs further downstreäm by lateral momentum supply.

Figure 6: Axial velocity distribution at stationx/L = 0.908.

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(a) Tanker i

(a) Tanker ]r

x/L = 1.0

.966 .937 .908 - .878

(b) Tanker 2

Figure 7: Direction of shear stress vector on the hull surface.

:-_--- -

--

,

i i

--

,

/

i___.

.-

--.

-

-

/ /

-

-

/

, ; ,__

-

--S-.-..

,,_.

-- ---

S--

-

--

-

-

-.

.-- .-- ____.--.--.--__ S.--

-.

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The occurrence of flow separation on tanker 1 has been confirmed experimen-tally by an oil-flow test in a wind tunnel (5J.

The wake fields in the propeller

planes - visualized as usual by a contour plot of the lines of equal axial velocity and a vector plot of the transverse velocity components = are shown in Figs 9 and 10. Notice that the location of thq pro-peller plane of the two ships is differ-ent; for tanker 1 it is at x/L = 0.976, and for tanker 2 at x/L = 0.991.

In both wakes a longitudinal vortex is present but it is more developed and stronger for tanker 2. This correlates with the more pronounced depression in,

the bilge region that we saw in the

po-tential flow results, although

the ef-fects are enhanced by the more rearward propeller plane position. We would try to avoid these vortices but for their favourable equalizing effect on the

axial velocity distribution. The

inten-tional creation of vortices is therefore justified in a lot of cases.

Disappointingly, the calculated axial velocity distribütions are rather

unre-(a) Tanker i (x/L 0.976)

Figure 9: Axial velocity distribution in propeller plane.

alistic in the propeller disk area, an observation that is confirmed by the comparison with experimental data [6J in Fig. 9(a). Somehow the computations fail to produce the retardation of the axial velocity near the corè of the vortex. The narrowness of the predicted wake is

the more surprisingin view of the flow reversal further ahead fr tanker 1. The reasons for this anomaly have not yet been resolved completely, but it is of course a serious shortcoming that has to

be carefully studied and as soon as pos-sible removed. In other respects the

axial flow is fairly well predicted.

Moreover, the results give clear evi-dence of the wake peak in the longitudi-nal centreplane being more pronounced

for tanker 1, although the distance

be-tween propeller plane and stern is al-most equal for both hulls. The effect of

the difference in stern contour

is

no-ticeable in the lower part of the wakes. So far, we have only pointed out certain differences in the flow around the two

hulls. The necessary next step is to talk about their possible

implications,

in order to allow a decision On a

pref-erence. of the one hull over the Other, or a suggestion for design adaptations.

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(a) Tanker i (xi!.. = 0.976)

N

N

N

\\\\\\

N

N

N

N

\\\

\

\

N

fffl\\\\\

\\

'11''' \'

\ \

\

\

\

\ \

\

-N

N

N

N

N

\

(b) Tanker 2 (x/L = 0.991)

Figure 10: Transverse components in propeller plane.

N

N

N

N

\

N

N

\

n

\ \

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x/L = 1.0 .966 .937.

Tanker i has flow reversal in the. lover stern region which causes the hull re-sistance to be greater. The calculations have identified thé increase as extra pressure resistance; the tvo hulls have practically equal frictional drag. In addition, the wake peak above the shaft

in the respective Propeller planes is more pronounced for tanker 1. This tends to increase the. variation of the propel-1er blade loading during a revolution and hence the risk of vibrations.

Superficially, therefore, it is tempting to choose tanker 2 as the best of the two. But it should be borne in mind that

the interaction with the propeller may change a lot. Could it be, for instance, that the flow reversal at the stern of

tanker i disappears. when the propeller is operating? Because this can be veri-fied computationally, we have repeated

the calculations for tanker i with

addi-tion of a propeller, represented by an actuator disk. For convenience, we have applied thrust forces only; forces in

radial and circumferential direction have been omitted (N.B. inclusion of the latter would imply the loss of port-starboard symmetry of the flow and thus considerably more computational work). The propeller loading - with a radially varying but circumferentially uniform distribution - was chosen approximately in accordancé with the self-propulsion condition. Further, we omitted the hub in order to avoid an

adaptation of the computational grid.

As a result, the hull shear stress di-rection as modified by the propeller action is presented in Fig. li. Indeed,

the flow reversal has disappeared

below the propeller shaft, but not

above it. Ve expect that it wOuld not, disappear even if we more realistically

-had concentrated a greater part of the pro-peller loading in the top sector of the disk. Therefore it seems that the design of tanker i requires some modification. Since we do not liké either 'the almost-flow-reversal on tanker 2 near x/L = 0.9 - which is unlikely to be affected by the propeller -, and ve prefer the milder aft shoulder of tanker 1, a third variant is considered as the best op-tion. We would copy the design of tanker

i somewhere up to x/L = 0.9, move the propeller slightly aft, which allows the waterlines to be stretched, sufficient to avoid flow reversal in the propelled mode. The design of the lover stern area (frame foot) would depend on the in-stalled power and the risk for

vibra-tions. We would try to create a strong

vortex (as on tanker 2) in case of a

serious risk, .but a weaker vortex (as on

tanker 1) in the opposite circumstances.

6. CONCLUDING REMARKS

The results of the numerical simulation of the flow around two slightly

differ-ent hull forms have been presented. We

hope to have shown that such results yield useful information for a ship de-signer. Admittedly, the prediction of

the axial velocity distribution

in the propeller plane. has turned out to be defective for the subject hulls.

Never-theless, the amount of detail and real-ism of the overall result is sufficient to allow preferential choices to be made

.908

, __

--_

__

---.----.

Figure 11:

Direction of shear stress direction on the hull with operating propeller (Tanker 1).

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or certain design improvements to be suggested. Anyway, the information is better than what the best-informed

guess, derived from

experience or sta-tistical/empirical methods, could pro-vide This will be reason enough for a more frequent application of

numerical vàke prediction to design

problems. Further improvements and extensions

of the code, and the

expected reduction Of

the expenditure, involved

in is use,

will have a favourable

and stimulating influence on this development.

REFERENCES

Eli

Van den Berg, W. et al., "Free-sur-face potential flàw calculations for merchant vessels", paper

presented at this Symposium.

[2] Hoekstra, M., "Applicatij

of a high_order fini te-différence method

to the solution of the

boundary_ layer equations", MARIN Report

No.

44519-2-SR, Nov. 1981.

[31

Hoekstra, M., "Computation f Steady

visCOuS

flow near a ship's stern" Notes on Numerical Flüid Mechanics Vol. 17, ed. P. Wesseling,!

Vieweg Verlag, 1987.

[4]. Hoekstra, M., "Recent

deveopments

in a ship stern flow prediction

code", 5th Conf. on

Numerical Ship Hydrodynamics, Hiroshima, 1989. [5] Kux,

j, "Berechnungsverfh

der Schiffshydrodynamjk - Vergleich der Ergebnisse mit Messungen",

Jahrbuch STG, 83 Band, 1989.

[61 Wieghardt, K. and Kux, J.,

"Nomi-neller Nachstrom auf Grund von Wind-kanalvrsuchen", Jahrbuch STG 74, pp. 303-318, 1980.:

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