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KB7 io

RSITAT HAMBUR

TEHIU8HE UNIVERSITEIT

Lsboradwn voor

MsIu,Iwss2,2cD o&

015- IIIVS 015. 781836

CAVITATION AND ITS INFLUENCE ON INDUCED

HULL PRESSURE AMPLITUDES

-RECENT RESEARCH AT

THE

INSTITUT FÜR

(2)

CAVITATION AND ITS INFLUENCE ON

INDUCED HULL PRESSURE AMPLITUDES

-Recent Research at che

Institut für Schiffbau

der

Universität Hamburg

by

E.-A, WEITENDORF

Hamburg University / Hamburg Model Tank

Bib;ofheek van de

Sche?pvartkun

le h

H

E? D

Left

t;

- i o

DATUM:

(3)

Abstract

Introduction

Measurements and Calculations of Propeller-excited

Pressure-Amplitudes

Measurements and Calculations of the Pressure

?iels on Propeller Slaes

4

Influence of Undissolved

Air Content

on Cavitation

Phenomena at the Propeller Blades

and ori Induced

iull Pressure Amplitudes

Theoretical Research

on Cavitation Inception

with Application of Bubble Dynamics

Conclusion

References

Figures

Contents

ha

Archief

Nek&weg 2, 2628 cl)

Deift

(4)

i

Ab st ra c t

A critical review of the

following subjects is given:

Measurement _adcacujatipQ of

Propeller

excited

Pressure-Ampli-tudes.

It was found that in the case of heavily cavitating frigate

pro-pellers a decrease of the pressure amplitudes occurs in front

of

and directly above the

propeller compared with

noncavitating

condit-ions. Behind the propeller

plane the cavitating tip

vortx with

nooes having a mean diameter of

about 3 to 5 per cent of

the screw

diameter amplifies the

pressure impulses. By means of

theoretical

and experimental investigations it could be proved

that the wave

length (i.e. distance

between two nodes) of the

cavitating tip

vortex causes amplitudes of

discrete frequencies. The

wave length

itsSelf depends on the meandiameterof

the cavitating vortex

and the

cavitation number. If the wave lenght x attains

a value

corres-ponding to the number of

propeller blades e.g.

= 1200 for a three

bladed propeller, the

amplitudes of the blade frequency will be

amplified. Analog effects will

happen at twice the blade

frequency

with a wave length of

=

60°.

Measurement and Çcylton_of

the Pressure _Fields

on Propeller

Blades.

The measurement of the

instationary pressures at 235 points

on the

blades of a 1.40

m model propeller were

executed in a ship-like

wake

in a wind tunnel at Göttingen. The results of these

measurements at

Göttingen are compared

with the results of

an instationary lifting

surface theory. For

one case they agree

very well, but from

(5)

real

pressure distribution of the propeller investigated.

3. Influence of Undissolved Air Content

on Cavitation Phenomena at

the Pro_pelTer Blades and on nuced_HilJ Pressure

Amplitudes.

This investigation consisted of the

application of the Scatterad Light Technique for measuring the undissolved

air conteìt of a

cavi-tation tunnel and

simultaneous measurements of propeller-excited pressure amplitudes on a flat plate above

the propeller.

The main results of the measurements

are:

Increasing relative free gas volume for cavitation

tests and

higher revolutions of the model

propeller in a wake causes earlier inception and

increase in the size of the cavity and

tnerefore increasing nondimensional

pressure amplitudes. Cavitation tests for estimating the propeller-excited

pressure amplitudes should include the simultaneous

determination of the relative free gas content and later on its possible

con-trol

4. Theoretical Research

on

of Bubble Dynamics.

The theoretical research on this

subject uses as input the nuclei

distribution measured in the above

mentioned point 3. Not only the pressure field for a two phase flow around

a hydrofoil is

cal-culated but also the growth of single

bubbles in this pressure

field. The result

(6)

greater number of smaller bubbles with a diameter less than

lO,Mm have an important influence on the cavitation phenomena, if

the

(7)

1. Introduction

The paper presented here gives a review of propeller and cavi-tation research con ducted at the Institut für Schiffbau of the Hamburg University within the Special Research Pool "Schiffs-technik und Schiffbau" (SFB 98) during the last four years.

Since there were several activities in this field, it is impossible to describe them all in detail. That is feasible only for those topics which are directly implied by the title. Others an only be mentioned by way of suggestion in this introduction.

For instance Laudan ti] has complemented the Wageningen

"four-quadrant" measurements of propellers f2) in open water. He per-formed the "four quadrant" propeller measurements in a quasi-steady manner using four typical ship models in front of the propellers.

In this way global statements about the wake fraction and thrust deduction fraction were found: the wake fraction remains constant from the condition of operation to the reversing point, afterwards decreasing to zero. On the other hand the thrust deduction fraction diminishes in a linear way from the point of operation to a

nega-tive value.

In an additional investigation Laudan (3] measured the influence of the cavitation on the propeller-forces occuring during crash stops on straight courses. The measurements were performed in a

cavitation tunnel in a quasi steady way. For the propellers used here it was shewn that the influence of the cavitation was not excessive. But at least the result was that the stopping time was prolonged by 20 per cent and the stopping distance was increased by 15 per cent.

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Furthermore this project "Safety against collision" of the SFB 98

investigated the influence of oblique flow on the propeller having different advance angles

{43

and made threedimensional

wake measure-ments during oblique towing of the ship model

[57.

But now results are to be presented,whose origin

concerns the author directly.

2. Measurement and Calculation of Propeller-excited Pressure

iplitudes

2.1. Measurements of Pressure Arn2uitudes for heavil,

cavitatinS

fr19

292!1

In order to study the influence of cavitation on the blade fre-quency pressures for heavily cavitating

frigate propellers of different design, measurements with seven

pressure pick-ups on a,

flate plate (Fig. 1) were carried Out in the medium sized cavitation

F. I

tunnel of the Hamburg Model Basin (HSVA). These investigations

E6]

contain numereous results with a wide variation of the main

para-meters of these three, four - and five bladed propellers

(9)

valid for homogeneous but also for inhomogeneous flow, can be

found in Fig. 2.

Here the nondimensional pressure amplitude

K z

p3

Ap

n D

is plotted against the coordinate in flow direction x/R. The figure concerns homogeneous flow. The upper diagram stands for a

propeller (HSVA-Propeller 1240), whose maximal circulation or

loa-ding is drawn to inner radii, the lower stands for an optimal pro-peller (HSVA-Propro-peller 1283). Both propro-pellers possess three blades. Parameter of the curves is the cavitation number

VA I

4A

p - VA2

In this definition VA means the speed of advances of the propeller. The solid curves are valid for the cavitation free condition of the propeller, i.e. there was an open connection between the test section of the tunnel and the atmosphere. The procedure of the tests was that the pressure in the tunnel was reduced step by step. So

the cavitation numbers,given in the legend of the figure, were reached. For the optimal propeller the following result for the cavitating condition was found:

In front of and directly above the propeller plane a decrease of the pressure amplitude occurs when compared with the cavitation-free condition. The decrease of the pressure amplitude by cavitation

i

(10)

can be explained in the following manner:

The propeller excited pressure amplitude is caused by two influ-ences, i.e. the thickness and the loading of the blade. Since in case of heavy cavitation the thrust breaks down, the loading

in-fluence can be reduced more than the thickness inin-fluence will

in-crease from cavitation. The smaller dein-crease of the amplitudes for the "noiseless" propeller in the upper diagram is due to the greater cavitation-free area of this propeller.

Behind the plane of propeller 1283 the increase of the amplitudes, compared with the cavitation free condition (ATM),

is caused by the cavitating tip vortex. Already

by observing the stroboscopic photographs of both propellers in

Fig.3 the influence of the

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cavitating tip vortex on the pressure amplitudes can be detected: The optimal propeller 1283 possesses a thick tip vortex and

accord-ingl,y in Fig. 2 an increase of the amplitudes. On the contrary

the noise-less propeller 1240 shows very little of a cavitating tip vortex in Fig. 3 and correspondingly

no amplification of the amplitudes behind the propeller plane in Fig. 2. In order to avoid misunderstanding at the end of this chapter, it must be stressed that this practice of unloading the propeller

ip can only be applied for propellers in wake fields of fast ships, mainly navy

(12)

-

6-2.2. InvestiSations of the Cavitatin Tip Vortex with nodes

Looking more precisely in Fig. 4 at some cavitating tip vortices in homogeneous flow, the following can be discovered:

At constant advance coefficient, bu4iecreasing cavitation number

VA the cavitating tip vortex becomes more and more thick.

Finally this vortex shows nodes at regular intervals which are marked by arrows in the photographs of Fig. 4. These notes are

stationary with respect to the running propeller. The poitions of the nodes are determined by the mean radius of the tip vortex and by the cavitation number

dVA. This was, already shown 1930 by

Ackeret [7J . Turning with the propeller, this cavitating tip vortex contracted at different positions causes pressure amplitudes of discrete frequencies, depending on the wave length of the vortex,

i.e. the distance between two nodes.

In the theoretical investigations {8J of this physical phenomenon the pressure impulses,created by the cavitating tip vortex, were regarded as an effect of displacement. This was simulated by suitable source-sink-distributions, arranged on the spiral line described by the propeller tip in operation. Now it is imaginable that the pressure amplitude, created by the displacement of a body, is proportional to the variation of the cross-section of this body,

namely

K

dx)

if z. is the circumferential coordinate.

In the calculations the

(13)
(14)

Fcx

(R

9sin2(xr))

'1

R

R0 Xø

/

(-x

J

is built up of two parts: the round bracket

stands for the

wave-like and cavitati.ng hollow vortex (sketch No. 1), and

the square

yort

bracket for the ellipsoidal hollowYThe

designations in the round

bracket for the wave-like hollow vortex are:

= tne nican radius of the

cavitating tip vortex,

nD

Ram

= amplitude of the cross-section of the tip

vortex,

to be taken from photographs,

=

wave length of the hollow vortex in the theory by Ackeret [7],

R.,

Çkefc

i/o'i

R K

ç

N

RiRa

K1 z = a = 1 4 (2.2) VA

the propeller blade,

coefficient,

number of blades,

inner and outer radius of

= thrust

Qfl

D4 V.A = advance coefficient,

R0,

ir

(2.1)

m

(15)

- circumferential coordinate

The designations in the square bracket for the ellipsoidal hollow

vQ'rtL)( (scetci No2

are:

kefcb W04

A initial value of the hollow vortex,

s

final value of the hollow vortex,

m parameter of inclination.

The cross-sections applied in the theoretical investigations correspond to formula (2.1). Some examples

of cavitating tip vortices used in the calculations are shown in Fig. 5.

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9

In the calculations the value - O

lies at

the position

of

the lifting line vortex of

the propeller blade,

i.e. trie 1/4 - point of the propeller profile. The different

in-fluences of the shape parameters in formula (2.1), namely

Rk the mean radius of the cavitating tip vortex,

Ram

a the amplitude

of

the cross-section of the tip

vortex,

a the wave length, the mitai value, the phase angle,

m = the parameter of inclination,

were investigated in a computer program. In order to enable

com-parisons with the present measurements [6] ,

the computer program contains all contributions of the propeller excited pressure am-plitudes, namely the influence of the loading

of

the blades,

in-cluding the steady cavitation, the influence of the thickness

of

the blades and the influence of the wave-like cavitating tip vortex with its effect of displacement. In the detailed report

8) all

re-sults of these calculations are given. But here the results of the variation of the wave length only can be shown in

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This figure contains two diagrams, the upper results are valid for the third harmonic order of the pressure fluctuations (blade frequency) and the lower for twice the blade frequency. The non-dimensional pressure amplitudes K3 and K6 are plotted against the flow direction x/R4. Behind the propeller plane in the region

> 1.0 the normal contribution of the propeller, i.e. thick-ness and loading effects of the blades have vanished. This is the reason for showing the results up to x/R = 2.0. Parameter of the different curves in Fig. 6 is the wave length x0.If the

wave length x attains the value = = 1200 for N = 3, then the

third harmonic of the pressure will be the strongest amplitude. If the wave length

x

is equal 60°, twice the blade

frequency will

be thgreatest. This can clearly be found in Fig. 6. The oscillat-ions of different curves in Fig. 6 are due to the wave length. Since these contracted tip vortices leaving the different blades are stationary with the positionsof their nodes with respect to the propeller, all respective nodes of different blades must be in one plane. This plan is located parallel to the propeller plane. The distances between two such planes, corresponding to the oscillation ir Fig. 6, are equal to the value x/R = X =

X0.

As the theory by Ackeret

[73

shows, the wave length

x depends on

the mean radius 0f the cavitating hollow vortex. In the present

investigation

[83

this statement was also confirmed for the spiral

curved tip vortex of a propeller. Ackeret's result namely was valid for a straight hollow vortex. The mean radius of the cavitating tip vortex depends on the cavitation number, the propeller loading and is inversely proportional to the blade

(18)

u

-in formula (2.2). In this way all dependencies not only for the

t

wave length x0 but also forean diameter of the cavitating tip

vortex are formulated. But the merely theoretical calculation of the pressure amplitudes of a cavitating tip vortex with nodes is not feasible, for the position of the first node, the initial and final value of the vortex and its shape amplitude

Rkam can only be

ob-tained from measurements. From photograph of corresponding tests these value are gathered. The valuesare used for the calculations whose results are shown in Fig. 7.

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For the purpose of comparison the results of the measurements are given additionally, obtained with the five pressure pick-ups located along the direction of flow (see Fig. 1). In Fig. 7 results of calculations and measurements for J 0.72 up to the 9th

har-monic order are given for the cavitation numbers

p-pv

-2.0, 1.75, 1.50, 1.25 and 1.14.

VA

-

-Comparing the results of calculations and measurements, a quite satisfactory agreement can be found, especially for = 1.75. For this case an exellent agreement occurs, above all

at the

position p 4 and P5, where the

cavitating tip vortex is of do-ininating influence. For this case not only photographs but also

coloured slides were available. These were used for determining the shape parameters of the vortex needed for the calculations. Here one can see, how important the accurate determination of the shape parameters is. Only if the input values of the computer program conform to reality, an agreement between measurement and calculation can be obtained.

In order to avoid the drawback of every time having to take

photographs for the input data of the computer program, empirical formulas for the shape parameters of the tip vortex were

develop-ed . By means of these emperical

formulas, it seems possible to compute approximately the pressure fluctuations caused by cavitating tip vortices without having to take photographs. At the er1d of this chapter the following

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13

-the influence of -the cavitating tip vortex with nodes shall be

given:

Not only by measurements but also by calculation

it was proved

that the cavitating tip vortex with nodes, having a mean diameter of about 4 per cent of the propeller diameter,

causes greater am-plitudes of higher blade frequencies. These can be observed in full

scale and model

measurements. The phenomenon of these nodes occurs

in a ship wake too.

An additional aim should be the calculation of the cavitating

tip

vortex with nodes in a ship wake. Preliminary

calculation of this problem are already carried out for single

screw container ships using the above mentioned

computer program in a quasi steady manner for different loadings

of the propeller in the wake. The result was that the pressure amplitude excited by the cavitating vortex was of minor magnetude

compared with the other con-tributions of the propeller. A concluding

statement about the influence of the cavitating tip vortex with

nodes in a wake can

only be drawn after having performed extensive theoretical

in-stationary calculations. It is imaginable

that the instationary variation of the shape of the cavitating

tip vortex in the wake

may generate pressure amplitudes of the same magnitude as the other exitations of the propeller.

3. Measurement and Calculation of the Pressure

Fields on Pro2elier

Blades

Concerning a realistic

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the propeller, the

inflow condition at the stern as well as the pressure distribution on the pressure and

suction side of the blades is needed.

Regarding the pressures on the propeller, auxiliary means consist of calculations of the unsteady

lifting

surface theory and measurements. In cooperation

between the In-stitut für Schiffbau Hamburg (Special

Research Pool 98) and the Aerodynamische Versuchsanstalt (AVA) in Gottingen measurements of the pressure

distributions on both side of a model

prpeller

were carried out in a wind tunnel with

a cross-section of g m2 (10, 113. The tests were

performed in a ship like wake flow. On the 4 blades of the 1,4 meter wide model 235 orifices

were

distributed, mostly concentrated at the leading edges and

the

outer radii. The measurements

were performed by means of the so called "indirect

method", i.e. the 235 orifices were connected to one pressure

pick-up using five scanning valves. In

this way

'n

a calibration of plitude and phase

was necessary for each orifice. In the figures 8 to 10 for instance,

results of the measured

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(23)

pressure distributions for the radii r/Ra - 0.50, 0.90 and 0,975 are shown. Here the nondimensional pressure coefficient

p po

cpb)

QW2

2

R

is plotted against the relative position along the chordlength

xii (x . distance from leading edge, i chord length).

X/

With the exception of the blade tip (see Fig. 10),the influence

of the inhomogeneous inflow (ship wake) is concentrated on the fore part of the chord, i.e. x/i 0.5. The influence becomes dominant at the leading edge. The lowest pressure, giving a

pressure coefficient c = -0,362 at the blade position y = 30° ra

at chord station xii = 0.007, was found on the radius r/Ra = 0.80. The influence of the tip vortex can be seen in Fig. 10 for the suction side. The great pressure &ifferences between pressure and suction side at the trailing edge indicate the threedimens-ionai flow around the blade tip, being typical for the tip vortex

roiling up.

The choice of air as fluid medium has the advantage that no cavitation can occur. The eperimental parameters were such that the flow remained incompressible so that the incompressible lifting surface theory could be applied for the calculations. Hence suitab1e possibility for the comparison between the re-sults from theory and measurements is available. Furthermore,

by using such a big model of 1.4 meter diajneter, the orifices

for the measurements could be placed very near to the leading edge. On the other hand, a drawback of using air as the fluid

(24)

17

-medium was the lower density of air compared with water. This leads to smaller pressure difference between suction and pressure side, approximately 0.025 bar. Above all, using the "indirect method" of pressure testing, these small pressure differences could only be obtained with a lowered accuracy. To some extent, the determination of the zero level for the pressure coefficient gave rise to certain difficulties, which only could be overcome by most precise measurements of the atmospheric pressure during the repeat tests. All in all, the AVA in Göttingen estimates the error of the whole measurement at 5 per cent with respect to the experi ence with other measuring techniques. This value

of ± 5 per cent seerr6 to be pretty good. Here it cannot be

de-cided whether the pressure differences at the leading edge could be measured with the necessary accuracy considering the ine-vitable inaccuracies of manufacturing in the profiles of the model propeller. This is the occcasion to give the hint that the AVA in Göttingen at this moment is pursuing the fundamental problem of measuring pressure differences on foils of rotating systems. The result of this investigation may give an additional insight into the accuracy of the propeller measuremnt reported here. Nevertheless this propeller measurement leads to the

possibility of comparing the results of lifting surface theories. For this reason these wind tunnel tests were ordered by the

Special Research Pool (SF8 98), in order to compare the results of a computer program [12] based on the lifting surface theory [13) developed at the Institut für Schiffbau of the Hamburg

University.

In Fig. 11 and 12a comparison is

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(26)

19

-results from AVA [111 and the -results of the Hamburg calculation E123 for the position 00 (12 o'clock position) and - 3300

(starboard) at the radius r/R = 0.90. For this case the agreement between computation and test seems pretty good. But using the same computer program for the HSVA-propeller 1917 leads to a substantially different picture in Fig. 13. For both the blade

positions

°0

-

00 and

) 330° (starboard) the cavity lengths

at the radius r/R - 0.90 for the cavitation number

p - p

C

= z 0.211

n

,2 (nD)2

are shown. In the calculation the vapour pressure, corresponding

to = 0.211, is only obtained for ten per cent of the chord length, whereas the real cavity lenght of a corresponding

cavitation test is extended over 55 per cent of the chord length

(see Fig. 18, upper row). This suggests that the mere application

of the cavitation number of the prototype is insufficient. It could be important to take into consideration the dynamics of the cavitating gas bubbles additionally.

Corresponding to the blade position = 330° in Fig.13, the vapour pressure corresponding 0.211, which is approximately necessary for the cavitation inception, is not attained in the calculations. This statement gives rise to the assumption that the pressure distribution of the computer program [123 does not fit the real values of the propeller pressures of a cavitation

test.

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(28)

21

-to compute the circulation distribution of the HSVA propeller 1917 in an axial model wake. This circulation can be used for the cal-culation of the blade frequency pressure without cavitation on a

flate plate

[83.

The result is shown in Fig. 14. Again

the

the-oretical values do not match the measurements. Once more the suspicion rises that the computer program f123 gives too small pressure differences between pressure and suction side compared with the reality. On the other hand, it must be admitted that the calculated blade frequency pressures on a flate plate do not indicate whether the calculated pressure differences on the

blades are right or wrong. For instance, computations of the

pressure differences on the blades of the HSVA-propeller 1917

Hamburg

ordered by the Institut fUr SchiffbaJ'?rom

another institute gave unsatisfactory results, inspite of better agreement of the

simutaneously calculated calculated blade frequency pressures on a flat plate with the measurements in Fig. 14.

Concerning the calculations of the pressure differences on the propeller blades in a ship wake by means of the lifting surface theory, it would be of utmost interest to see what the comparison of different lifting surface theories proposed by the ITTC would look like. Beside the AVA-model propeller the HSVA-propeller

1917

(Zeise-design) would offer a suitable object for purposes of

(29)

at the ProEeller Blades and on Induced Hull Pressure Am2litudes In a paper on propeller-excited hull forces given in 1972 by

van Oossanen and van der Kooy 14J, it was evident that for equal nondimensional flow conditions but different absolute revolutions (i.e. n = 20 and n = 30 Hz),the nondimensional

propeller-excited pressure amplitudes were different. That means an uncertainty with respect to the evaluation of the vibratory behavior of a ship.

Two possible influences concerning these differences were taken

into account:

the influence of the neglected Froude law of similarity and the free air content of the tunnel water.

Using the Froude law of similarity, the correct pressure distribution on the propeller blades in radial direction is guaranteed. But normally the revolution based on the Froude number can not be realized, because it is out of the range of a normal cavitation tunnel.

With respect to the free air content, this content of the tunne' water, i.e. the free gas bubbles of test water, governs the cavitation inception.

Taking the above mentioned influences into account as much as possible, new tests were performed in the medium sized cavitation tunnel of the Hamburg Model Basin in November and December of 1974. The axial component of the flow field in the propeller plane

(30)

23

-was simulated by grids of varying density.

Three kinds of measurements were executed simultaneously:

Measurement of the undissoived air content by the laser light

scattering method.

Measurement of the propeller-excited pressure amplitudes on a fiat plate above the propeller.

Stereometric photography of the extension of the cavitation on the propeller blades.

In this lecture a short review of the above mentioned measure-ments under number 1) and 2) shall be given. A more detailed description of these measurements was given in the IfS-Report

312 A [15).

The scattered light technique was applied in close cooperation with A. Keller of the Technical University Munich. He developed this method up to practical application of cavitation

tests [16].

(F

.1),

In our case of applRà Tàthe optical control volume defined

by the cross-sectional dimensions of the light beam and the optics of the system detecting the scattered light had a cross-section of 1.2 m2. The control volume was located in front of the propeller plane. Directly behind the control volume, the flow velocity

was

measured by a Prandtl tube. The flow velocity is required for the estimation of nuclei concentration of the fluid. The

ca-libration of the photomultiplier used as the scattered light detector was performed with latex spheres of known diameter. These were injected into the control volume. The electrical

output pulses of the photomul tipi ier which are proportional to

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the "nucleus size were evaluated by an HP-computer in an on-line mode. Thereby, it was possible to print a nucleus size histogram immediately after each test.

For the example of degassed water, a histogram is shown in Fig. 16. The abscissa is the size o the bubbles measured in the range

between 20 and 350 microns.

The recommendation of the ITTC Cavitation Committee, taken

into consideration in this case, is the following that the nuclei size should be measured from 10 to 250 microns in diameter.The dashed line in Fig. 16 is the size histogram. Additionally, the diagram contains the fraction of the relative free gas

volume

d

per bubble range (full line). The relative free gas volumec& is the ratio of all measured gas bubbles per volume

unit to the volume unit of the fluid. As mentoned, the full line represents the fraction of all measured relative free gas volumes per bubble range, i.e. between 20 and 69,6 microns. Summing up all the fractions of the relative free gas volumes per range,

we obtain the total measured relative free gas volume, i.e.

c= 0.118 x 10 in the figure.

By gassing and degassing, it was possible to vary the free air content of the test water in a rather wide range. For the case of gassed water, the respective figure like Fig. 16 contains

a greater number of bubbles and greater relative free gas volume. After and before each test series the total air content c0 was determined by a van-Slyke-apparatus.

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25

-As mentioned before the propeller-excited pressure amplitudes were measured on a flat plate above the propeller. The sketch of

the test setup and positions of pressure pickups were shown in Fig. 1. The first tests of the heavely cavitating frigate propeller (HSVA-propeller 1283) with open water conditions were performed without artificially changing the free gas

con-tent of the tunnel water. The purpose of this procedure was to find the connection to experimental results gained in 1972

[6]. The free gas volume changed in a way which is probably normal during a testing duration of eight to ten hours. The

results of these tests are the following that in case of existing cavitation the nondimensional pressure amplitudes of the blade

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frequency are not affected by the free air content or by the chosen propeller revolutions. This result is confirmed by the extension of the cavitation photographed.

In contrast to this instance of existing cavitation the relative free gas vo1ume. has an extreme influence on the pressure

amplitudes K = of a propeller in a wake. In Fig. 17 some results of pressure amplitudes of the model propeller

of S.S. "Sydney Express" (HSVA-propeller 1917 - Zeise-design) are shown. Here the nondimensional pressure amplitudes K5

of the middle pickup (position 3) are shown for the advance coefficient

KT 0.61 and the cavitation number

C. =

PPv

=0.211 n

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27

-The abscissa is the measured relative free gas volumec. The

pa-rameter of the diagram is the chosen number of revolutions, i.e.

n = 15, 20 and 30 Hz, that means different pressure conditions in the test section according to the law of similarity of equal cavitation numbers. Mainly for the revolutions of n = 15 and n - 20 Hz, there are great influences on the pressure amplitudes by the relative free gas vo1umec,. Stereometric photographs of the blade in several positions

show that for a lower relafive free gas volume the cavity starts later than in case of the higher free gas volume. The

photographs underline the fact that the inception of the cavitation in the wake field and

conse-quently its disappearance,

influenced by the free gas volume, control the pressure amplitudes.

In Fig. 18 two sets of photographs for the observed propeller blaae in several positions are shown. The upper row is valid for the speed of revolution

n = 30 Hz, the lower for n = 15 Hz. The reason for the great difference in inception and extent

of the

ca-vitation is the fact that for the higher revolution the absolute pressure is lower (sometimes below zero) than for n 15 Hz; and

the absolute pressure is responsible for the expansion of the free gas bubbles. A more detailed explanation of this physical

behaviour shall be given in the last chapter of this paper.

Another interesting result of these investigations on the influence of the free gas content shall be mentioned

briefly, though the corresponding photographs cannot be shown here

because of

(35)
(36)

-29-more and -29-more stable, when the gas content was increased from lower to higher values, i.e. the intermittend

cavitation observed

here is a sheer model effect.

Before finishing this chapter, it has to be mentioned that the model speed of revolution o S.S. "Sydney Express"

regarding the Froude law of similarity was n = 9.7 Hz. According to Fig. 17 this influence of the free gas volume at this revolution

would be extra-ordinary. This speed could not be used because of the too low

tunnel pressure which is necessary for equal cavitation numbers of model and full scaie

It is obvious that the influence of the free gas volume is compensated to a certain extent by the greater revolutions, often used for cavitation tests.

The main results of the described measurements are as follows Increasing relative free gas volume for cavitation tests in a wake field ¿auses earlier inception and stronger extension of the cavity and therefore

increasing nondimensional pressure

ampi i tudes.

Cavitation tests for estimating the

propeller-excited pressure amplitudes should include the simultaneous determination of the relative free gas content and later on its possible control. The last statement

involves the question of the correct relative free gas volume in cavitation tests. The answer of this question is of highest importance for all cavitation

facilities, especially those with a free surface.

Moreover the main results confirm that the free gas volume scaling the cavity is of the same

importance as the correction of the wake field in the cavitation test.

(37)

In connection with the free gas volume it is to be mentioned here that a research project of the Special Research Pool at Hamburg in cooperation with the HSVA, The Technical University of Munich and D n V is going on. Besides cavitation observation

L-and pressure fluctuation measurements the free air content of the seawater shall be measured as the maintask in this project.

5. Theoretical Research on Cavitation Ince2tion with

A22lication of Bubble 0namics.

In Fig. 17 it could be observed that for the higher revolutions n = 30 Hz and additionally in all cases of the HSVA-propeller 1283

in homogeneous flow no dependence of the pressure amplitudes K

on the relative free gas volume ci. could be stated. On the other

hand for the lower revolutions (n = 15 Hz and n = 20 Hz) not only the pressure amplitudes on the plate but also the observed cavi-tation were dependent on the relative free gas volumec& to a high extent. Trying to find an explanation for this dependence one has to remind that, applying the value c, the behaviour of the single bubbles in a flow field with pressure gradient is neglected. Thus it was attempted to explain the differences in cavitation extent and pressure amplitudes for equal propeller loading and equal cavitation number, but different revolutions (e.g. Fig. 17) by means of a theoretical analysis of the dynamic expansion of single bubbles in a flow with pressure gradients. Such theoretical in-vestigations were carried out by Lederer (173 for steady hydrofoil flow in compressible water. The procedure was the following:

(38)

Iterative computations for the pressure distribution in compressible water with gas - content around hydrofoils were carried out accor-ding to the following formula

P

I

u

2rrp

A

-

31

-(x-x)

dr1

-

ì4

(._ r1) . xs. A

yd

1rO -A r)O

The notation used can be found in sketch No. 3:

Skec'ì Wo3

The formula (5.1) is derived in a paper by Isay and Roestel 1183. in this connection gas means the content of free air in the water as well as the vapour in the interior of the cavitation bubbles.

The si ip velocity of these bubbles shall be, neglected and a further

assumption is that the bubbles are moving along streamlines. Using these assumptions the dynamic behaviour of a single bubble

+

(5.1)

(39)

in a temporally changing pressure field is described by a diffe-rential equation of the second order. This is thewell known Rayleigh-Plesset equation .. 4 1

*

2c5

(5.2)

-

-4.RR

R

In this case R stands for the radius and R for the wall velocity of the bubble. The indes i is the designation for water r vapour, the index 2 for dissolved or undissolved air. The star belongs to the gas phase and Ö is the surface tension.

The growth of different initial radii

R0 was calculated by Lederer

(173 applying equation (5.2), which was solved with a Runge-Kutta method. The streamlines, along which the bubbles are moving, were

substituted by straight lines y

= n parallel to the x-axis.

For

further understanding of the procedure of Lederer [l7Jthe

following ought to be mentioned:

During an air content measurement [153 Z = 1000 bubbles were measured, flowing through a cross-section F0 with a velocity u

in a time ç. Dividing

the measured radii (e.g. Fig 16) into

ranges

j

1,2 J, if the number of bubbles in a range is equal to Z0,

then the gas volume of the flow is

(40)

'f

-

33

-For the radii range R0 the number of bubbles is denoted by

o3

Ri

I

\I

.4.

\Vw

co

'J 3 (Rfl)3

L

j4

So the number n3 of bubbles per unit volume of the flow is

z05=>

oj

O O O

(5.5).

(5.6).

Comparing an initial state ck at a point x = xo with a state at a

point x lying downstream and applying the conservation-equation, wnich means that the number of bubbles remains constant, one can

find

J

=

(M)

j'4

If the bubbles of the different bubble ranges contribute uni-formly to the compressibility, equation (5.7) leads to

(5.4),

(5.7)

(5.8).

which is referred to unit volume. Using the gas volume ratio

vg0

of the flow, then one 't.

(41)

For a point x (dównstream from the point x0) one can determine

3 3

--

3

The expansion of the radius of the single bubble from the

initial radius in the pressure field p(x) is calculated by means of the Rayleigh-Plesset equation (5.2). ¡f

s

(5.9)

R

=

B(R0,x)

(5.10)

B

is the solution of equation (5.2), the local gas volume ratio in the hydrofoil flow can be derived from the equations (5.7) and (5.8) and it follows

3

3

(x,y)

3:4

(5.11).

As already mentioned, the precise determination of the streamline is neglected. Instead of this, the straight lines y = y parallel to the chord (x-axis) are regarded.

Knowing the pressure distribution p(x, y) along the lines y

=

according to equation (5.1) and using a nuclei distribution from a laser scattered light measurement (e.g. Fig. 16), the local gas volume ratio oc(x, y) of the flow can be calculated with the aid of equation (5.11).

The computations by Lederer L173 were carried out for two foil sections, a curved and an uncurved section. For the latter section

(42)

35

-results are shown in Fig. 19 to 21. The chordlengths for both were assumed to be ?A = lo cm.

The nuclei distributions of the computation were adapted to the results of the laser scattered light measurement[15J. Since more-over the growth of a single bubble depends on the absolute value of the initial radius R0, the measure bubble histograms were divided

into four ranges:

s

R01

5,m;

R02 = 35,m; R03 = 65,um; R04 . 95,,um.

These ranges were applied in two different nuclei distributions for the calculations:

Nuclei distribution No. 1:

= 50;

o2 = 20; o3 = 5; o4 = i with

-= number of bubbles of the range j) Nuclei distribution No.2;

oi

= 200;02 = 20;

o3 i with c. = 1,3 . 10

o

The increase of the number.çof the small bubbles by a factor four means practically no change in the free gas volume ratio of the

flow.

The occurrence of diffusion is neglected for this theoretical investigations, since this phenomenon develops too slowly, com-pared with the pressure changes on the foil section. Futherinore, the interaction between the different bubbles was ignored.

VG0

z 1,3 10

(43)

In order to show clearly the influence of the nuclei present in the flow, the expansion of a single bubble in the pressure field is displayed in Fig. 19. There the results of calculations for the r smallest bubble R01 and the greatest one R04 are shown. Fig. 19

J

is valid for the cavitation number

p

- p

=

EO.3

V

The pressure Po = 1 kp/cm2 and Po = 0.2 kp/cm2 in the flow

corres-pond nearly to the revolutions n = 30 Hz and n = 15 Hz in the ex-periments from 1974 [15J . The results of the computation, given

in Fig. 19 and plottet against the chordlength 2A, show clearly that the smallest bubble R01 is expanded after a short distance from the leading edge, if the inflow pressure is Po = 1 kp/cm2. The same bubble R01 is not expanded, if the inflow pressure is

Po 0.2 kp/Cm2. The reason for the latter fact is that the

pressure on the foil section does not reach stronger negative values because of the lower inflow velocity for the constant cavitation number 0.3. This can be found in Fig. 20, if the

pressure distributions for the two inflow pressures p0 = 1 kp/cm2

'\

and po = 0.2 kp/cm are compared in the region 0.01 0.06.

Trie strongly negative pressurés therefore lead to the expansion of small bubbles. On the other hand a difficult problem of substant-ial importance appears, if the question should be answeredto what values the pressure in real water with free gas content may drop.

(44)

37

-Nevertheless Keller (see p. 96 in [163) found that during cavitation inception the absolut pressure on a body in the flow decreased

to negative values, whose magnitude depended on the nuclei distri-bution, i.e. the pretreatment of the water.

From Figs. 19 and 20 it becomes understandable, why the cavity

extent in Fig. 18 for n = 30 Hz is greater than for n = 15 Hz: The first reason is that the absolute pressure at the foil section for

n = 30 Hz reaches stronger negative values than for n = 15 Hz, and the second reason is that the number of small bubbles (see Fig. 16) is always greater than that of the great bubbles.

Additionally the great bubbles are further displaced from the foil section (screening effect).

The number of bubbles has in influence of the local free gas

volume c«x, (see eq. 5.11). In this connection the results calculated by Lederer r173 for the local free gas volume K(x,

on the suction side at a distance y/A = 0.005 are given in Fig. 21.,/' Here the nuclei distribution No. 2 for Po = 1 kp/cm2 attains the

greatest value c..(x, since the number of small bubbles R01

is four times as great as in the distribution No. 1. By the way, in this theorie with spherical symmetry for the bubble, the value c.= i means pure cavitation. This theory of the behaviour of single bubbles becomes meaningless, when the single bubbles grown and touch each other. In this relation of exspanding single bubbles

a question concerning Fig. 17 emerges. There the nondimensional pressure amplitude K5 on the flat plate is plotted against the relative free gas volume .But the que'stion is, whether the value c& is the right parameter for plotting the results, because,using

(45)

is ignored. But a better presentation of the results like Fig. 17 needs the measurement of smaller bubbles as measured in Fig. .16.

In this respect the recommendation given by the

ITTC-Cavitation-tö

Committee measure the bubble radii between 10,tm and 250,m should be supplemented: Nuclei should additionally be measured between 5 and 10pm radius.

At the end of this chapter on cavitation inception and bubble dynamics questions on future work should be discussed.

Normally the cavitation number and the thrust - or torque coefficient of model and prototype are kept equal for cavitation tests. This does not always lead to geometrically similar extent of cavitation (see Fig. 18), since the number and size of nuclei are important parameters in the reaction to the pressure field of the foil . Thus

geosim tests with hydrofoils or propellers should be performed with simultaneous measurement and possibly control of the free air content.

of the

Supplementary investigations'b'theory of bubble dynamics described

above should accompany the geosim tests. Furthermore for additional similarity conditions of cavitation tests it is necessary to know

the nuclei distribution in seawater around a ship. Other important factors are the basic behaviour of the cavitation facilities and the effect of installed flow regulators upon the free air content. These amount to a stronger consideration

of the quality of the flow medium for cavitation tests.

Efforts regarding these three tasks in cavitation research, namely geosim test for cavitating hydrofoils or propellers,

(46)

39

-tunnels and

determination of free air content in seawater

are being pursued in Hamburg at the Hamburg model tank (HSVA) and the Institute for shipbuilding (IfS) within the special research pooi for shipbuilding (SF8 98).

6. Conclusions.

The following conclusions can be drawn from the results presented

The hull surface forces excited on fast naval vessels by a cavitating tip vortex can be decreased by shifting the maximum circulation

to inner radii of the propeller. This method is probably useless for tankers and container ships, because of their wake distribution. In the theoretical field the estimation of the variation of the cavitating tip vortex in a ships's wake would be an interesting task. Afterwards it would be possible to account for the cavitating tip vortex in the total vibration excitation by the propeller.

Not only the technique for measuring the instationary pressure

distribution on propeller blades in a ship 's wake but also the three-dimensional lifting surface theory for the same purpose must be

improved. For the measuring technique the so-called direct method should be applied, i.e. pressure pick-ups mounted in the surface of the propeller blades.

(47)

The influence of the free air or gas content on cavitation

in-ception makes it necessary to determine the nuclei distribution during cavitation tests, where simultaneously

propeller-excited pressure amplitudes are to be measured. The

possible control of the free air content

would balueable

tool for these tests.

e

From the theoretical

investigations on bubble dynamics it can be

concluded that the theoretical model of the bubble and its behaviour in pressure fields' should be

checked by means of geósim tests. Another problem would be scale effects

on cavitation, which should be pursued with

(48)

7.

References

Lauaan, J.: Propellerkr.fte und

-vomente beim

geradlinigen Stoppmanöver.

(Propeller forces and moments during a

straight-lined crash stop). HSVA-Bericht

F )4/744 fUr den

3FB 98.

f2

van Larnmeren, W.P.A., vari Manen, J.D.,

Osterveld, M.W.C.: The Wageningen B-Screw Series.

Transactions

SNAME Vol.

77

(1969)

f3]

Laudan, J.: Einfluß der Kavitation auf die

Propel-lerkcräfte und -momente beim

geradlinigen

Stopp-manöver.

(The

influence

of the cavitation on the propeller

forces and torque during a straight-lined crash

stop). HSVA-Bericht Nr. F

8/76.

Laudan, J.: Einfluß der

Schrganströmung auf die

Propelierkräfte und -momente bei

verschiedenen

Fahrtsteigungswinkeln.

(Tne influence of the oblique flow on propeller

forces and torque for different advance angles.)

HSVA-Bericht Nr. F 9/76.

(49)

(Wake measurements with a series 60

model.)

Institut f1r Schiffbau,

Bericht Nr.

340

(1976).

[63

Weitendorf, E.-A.: Experimentelle

Untersuchungen

der durch kavitierende

Propeller erzeugteì

Druck-schwankungen.

(Experimental investigations on the pressure

fluctuations caused by cavitating

propellers.)

Schiff und Hafen,

Heft 11 (1973),

25. Bd.,

5. 1040-1060.

nj

Ackeret, J.: Ober stationäre Hohiwirbel.

(On stationary

hollow vortices.)

Ing.-Archiv (1930),

S.

399-402.

f

87

Weitendorf, E.-A.:

KavitationseinflUsse

auf die

vom Propeller induzierten

Druckschwankungen.

(Cavitation influences

ori the propeller

induced

fluctuations.)

Institut fUr Schiffbau der Universität

Hamburg,

bericht Nr. 338

(Sept. 1976).

(50)

Chijupiri, A.I.; Weitendorf,

E.-A.: Berechnungen

von

Druckamplituden mittels einer verbesserten

Quellen-Senken-Verteilung

fur

einen

kavitierenden

Spitzen-wirbel mit Knoten und Vergleich mit Messungen.

(Calculations of pressure amplitudes

by means of

an improved source-sink distribution for a

cavita-ting tip vortex with nodes,

and comparison with

measurements.)

Institut fUr Schiffbau der Universität Hamburg,

Bericht Nr. 339 (August

1976.)

10;

Xienappel, K.; Triebstein, H.

und Wagener, J.:

Messung der instationären Druckverteilung und der

Kräfte ari einem Propeller im

Schiffsnachstrorn.

(Measurements of the instationary pressure

distri-bution and forces on a propeller in a ship'8 wake.)

Internal

DFVLR-AVA Report No. IB 253-76 C 04

(March 1976).

11

Kienappel, K.: Wiederholungsrnessung

der

instatio-nären

Druckverteilung eines Propellers im

Schiffs-nachstrom.

(Repeated measurement of the instationary pressure

distribution on a propeller in a ship's wake.)

DFVLR-AVA Report No. IB 253-76

J 09 (Sept.

(51)

Xrfte an Propellern

im Schiffsnachstrom.

(On the calculation

of the pressure distribution

and the forces on propellers in a ßhip'8 wake.)

Rep. No 309 Institut

für Schiffbau der

Universität

Hamburg (Oktober 1974).

r13

Isay, W.-H.: Moderne

Probleme der Propellertheorie.

(Modern problems

on propeller theory.)

Berlin - Heidelberg

- New York, Springer-Verlag

(1970).

van Oossanen, P., and

van der Kooy, J.: Vibratory

null forces induced by

cavitating propellers.

Trie Royal Institution of Naval Architects,

Spring

Meeting (1972).

)15

Keller, A.?., and Weitendorf,

E.-A.: Der Einfluß

'- J

dea ungelösten

Gasgehaltes auf die

Kavitations-erscheinungen an einem

Propeller und auf die

von

ihm erregten

Druckschwarikurigen.

(Influence of undissolved

air content on cavitation

phenomena at the propeller

blades and on induced

hull pressure amplitudes.)

Rep. No 321 A Institut für Schiffbau der

(52)

L161

Keller, A.?.: Experimentelle und theoretische

Untersuchungen zum Problem der modellmßigeri

Behandlung von

Strömungskavitation.

(Experimental and theoretical investigations on

the problem of cavitation in a flow with models.)

Versuchsanstalt für Wasserbau der T.U. München,

Bericht 26 (1973).

Lederer, L. :

Profilströmungen unter

Berücksichti-gung der Dynamik von Kavitationsblasen.

(Hydrofoil flow with regard to bubble dynamics.)

F(ep. No 31 Institut für Schiffbau der Universitat

Hamburg (Oktober 1976).

Isay, W.-H., and Roestel, Th.: Berechnungen der

Druckverteilung an Flügeiprofilen in gashaltiger

Wasserst römung.

(Calculations of pressure distributions

on

hydro-foils in water flow with

gas content.)

Zeitschrift für angewandte Mathematik und Mechanik

(53)

Fi g.

Caption

No

i

Test setup for pressure amplitudes

and

coordi-nates for measurements

2

Nondimensional blade frequency pressure

amplitu-des K3 in x-direction for

two propellers in

homogeneous flow

3

Cavitating propellers in homogeneous flow

Optimal propeller 1283 in homogeneous flow

under different cavitation

conditions

5

Different shapes of the

cross-section of

cavi-tating tip-vortices used

for calculations

6

Calculated pressure amplitudes

and

with

variations of the wavelength

X0

7

Calculated and measured pressure-amplitudes

(including those owing to a cavitating tip vortex)

on a flat plate

8

Measured instationary pressureon the

propeller-blades in a ship's wake

9

Measured instationary pressures on the

propeller-blades in a ship's wake

(54)

Fig.

No Capt i on

10

Measured inatationary pressures on the

propeller-blades in a ship's wake

11

Comparison between measured and calculated

pressures on propeller blades

12

Comparison between measured

and calculated

pressures distribution on propeller

blades

13

Comparison between calculated pressure and

cavity extent at radius

riRa

0.90

14

Nondimensional blade frequency pressure

amplitudes K5 in axial wake without

cavitation

15

Test setup for laser light scattering

method

16

Nucleus size histogram and fraction of relative

free gas volume

17

Noridimensiona]. blade frequency

pressure

amplitu-des Xp5 in an axial wake dependent on measured

relative free gas volume

18 1-LSVA propeller 1917 in

a wake for two propeller

revolutions with low free gas volume

19

Calculated (in 117] ) growth of

a single bubble

(55)

20

Calculated (in

fi7J )

pressure distribution

on a hydrofoil in stationary flow

21

Calculated (in

j17j )

local relative free gas

volume

on a hydrofoil in stationary flow

Sketch No.

1:

Wave-like hollow vortex

Sketch No. 2:

Ellipsoidal hollow vortex

Sketch No.

3:

Notation for hydrofoil in

water with gas-content

(56)

B5

BL.

Direction of

flow

e= 30mm

ig.1: Test setup for pressure am plitudes

and coordinates for measurements

(57)

0.06

0.04 0.02 O

fK3

..

in front of Prop.

-.05

Pos.

Propeller 120; N'3

Advance

- Ratio J = 0.8 03

Max. Circulation drawn to inner radii

0.12

0.08

0.04

¡n front of prop.

Prop.-plane

-0.25

2 3 O 'r Prop. pLane

0.25

I.

44

4J

0.5

a.x/R

5

aIR' 0.109

a/Rs 0.109

g.2: Non dimensional

blade frequency

pressure amplitudes Kp3

Ifl

x-direction for two propellers in

homogeneous flow

-0.5

-0.25

25

0.5 Pos. i 4 5

xIR

ATM

=

3.00

2.00

1.75

1.50

1.25

1.1b

PropelLer 1283 ;

Ns 3

Advance - Ratio

J a 0.803

(58)

Fig.3: Cavitating

propelters in

homogeneous flow

P l283, Nz3

P 12h0

Nz3

Optimal distribution

Maximal circulation

of circulation

drown to inner radii

(59)

4 Optimut

propeLler

1283 in homogeneous

flow under

different cavitation

condition

(60)

Wavelength X0 = 600

ig. 5: Different shapes of the

cross

section of cavitating tip vortices

(61)

0 16

0.08

0.02

o

0.40

0.32

0.24

0.08

0.16

-0.02

o

- 0.5

o

Fig. 6: Calculated

pressure amplitudes

Kp3 und Kp6 with variation of

the wavelength Xo

60°

45°

150°

0.5 1.0 1.5

2.0 xIR0

I

.1

I

150°

i.

TAj,A;A

p

HSVA-Prop. 1283; homog .flow

Cavitating tip-vortex

Advance Ratio J = 0.803

m 24; RK0m /R0 :0.0252

Tip-clearance aIR0

0.109

XA: 20°; X.t.p

00

Cav.-num berGVA 1.14 .RK/RQ0.0143

0 24

90°

60°

(62)

<phri 0.2 0.1 O 0.2 0. 1 O 0.2 0.1 o 0.2 0.1 O 0.2 0.1 O

n

e

e

6VA *

2.0

1.75

1.50

1.25

1.16

Fig. 7:

Calculated and measured

pressure amphtudes (in

-cluding those owing to

a

ccivitating tip vortex) on a flat plate

3. 5. 9. 3. 6. 9.

in front of prop.

Pos.

Pl

P2

HSVA-Prop.1283;N3

Homogeneous flow

Advance Ratio

J 0.72 3. 6. 9. 3 .

Prop. plana

P3

P4

Calculations with

VA 9.

)(

3.

6.harm Order

behind prop.

P5

RKam/Ra

Tip cearence a/R=O.1O9

2

660

100

410

0.010

1.75

700

15°

31°

0.014

1.50

750

15°

43°

0.017

Measurement U

1.25 1.14

1020

110°

20°

20°

41°

46°

0.018

0.018

(63)

o Q. Q.

3

0.16

-0.12

-0.16

nondirnens Rad. r/Ra 2 0.50

pressure side

suction side

0° 30° 90°

1800 2700 3300

o

o

A

9

Fig.8: Measured instationary

pressures

on the propeller-blades in

a ship's

wake

ç

0 0.1 0.2 0.3 0.4 0.5

0.6

0.7 0.8 0.9

(64)

-i

cp

0.12 O

-0.0/.

- O. C 8

-0.12

-0.16

-0.20

-0.2/.

-0.28

-0.32

-0.36

o

pressure side

suction side

AVA Propeller

non-dimens. Rad. nR0 a 0.90

0° 30° 90°

180°

2700 330°

D O

A

90° 0.1 0.2 0.3 0./.

0.5

0.6 0.7 0.8 0.9

chordtength

Fig. 9: Measured instationary pressures

on the propeller blades in a ship's

(65)

Q? Q. Q. u

3

o-0.08 0.04 C

-0.04

-0.08

-0.12

-0.16

-0.20

-0.24

nondimens. Rad. r/R

'0.975

pressu re side

.

suction side

..

_

lu

I,

j

'A P0

0° 30

90°

180°

2700 3300

D O A 0. 0.2 0.3 Od. 0.5 0.6

0.7

0.8

0.9

chord length

Fig. 10:

Measured instationary

pressures on

the propeller

(66)

pressure

coefficient

$ 0.08 0.0 ¿ o

-0.04

-0.08

-0.12

-0.1 6

-0.20

-0.24

-0.28

Fig.11: Comparison between

measured

and calculated

pressure

distri-bution on propeller blades

nondimens. Rad. r/R' 0.90

\

u

o

/7

u

I

I

--e-- measured

po*0o

catcuLated

r

I

-i

i

u

AVA-PropeUer

p-p-

0.12

Cpa

ÇW2R

0 6

0.8

-.. chordtength

0./. 0.1 0.2

(67)

coefficient

2

C

Ppw2R 2

0.08

0.04

o

-0.04

-0.08

-0.12

-0.16

-0.20

-0.24

-0.28

0

0.2

0.4

0.6

0.8

1.0

chord length

Fig.12: Comparision between measured

and calculated

pressures on

propeller blades

£

L

Blade pos. p0:330°

JTw

--L--I

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