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FOR FL UlD DYNAMlCS

TECHNICAL NOTE 129

ONE VIMENSIONAL VESIGN OF CENTRIFUGAL COMPRESSORS TAKING INTO ACCOUNT FLOW SEPARATION IN THE IMPELLER

TECHNISCHE UNIVERSITEIT DELFT LUCHTVAART· Er~ RUIMTEVAARTTECHNIEK

BIBUOTHEEK

K!uyverweg 1 - 2629 HS DELFT

'

7 JAN.

1988

P. FRIGNE & R. VAN DEN BRAEMBUSSCHE

JUNE 1979

~A~

-~O~-

RHODE SAINT GENESE BELGIUM

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CHAUSSEE DE WATERLOO~ 72

B - 1640 RHODE SAINT GENESE~ BELGIUM

TECHNICAL NOTE 129

ONE VIMENSIONAL VESIGN OF CENTRIFUGAL COMPRESSORS TAKING INTO ACCOUNT FLOW SEPARATION IN THE IMPELLER

P. FRIGNE* & R. VAN DEN BRAEMBUSSCHE

JUNE 1978

* NAVORSINGSSTAGIAIR VAN HET I.W.O.N.L.

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TABLE OF CONTENTS Summary

.

.

. .

List of Symbols

Lis t of Figures

. .

.

Introduction

CHAPTER 1 - BRIEF DESCRIPTION OF THE FLOW THROUGH A CENTRIFUGAL MACHINE .

CHAPTER 2 - INLET GUlDE VANES (IGV) 2.1 Purpose of IGV . . . . 2.2 Isentropic calculation of IGV .

2.2.1 Constant prerotation IGV 2.2.2 Free vortex IGV . . 2.2.3 Forced vortex IGV . 2.3 Calculation of IGV losses CHAPTER 3 - THE ROTOR .

3.1 General geometry 3.2 The inlet blockage

3.3 Determination of the inducer hub and tip radii 3.3.1 Determination of the inducer hub radius. 3.3.2 Determination of the inducer tip radius 3.4 The inducer flow . . . .

3.4.1 Physical model and diffusion ratio 3.4.2 Geometrical model . . . .

3.4.3 Flow equations . . . .

3.4.4 Calculation of the separation point 3.5 The impeller flow . . . .

3.5.1 Real floweffects . . . . . 3.5.2 Flow equations for the jet 3.5.3 Flow equations for the wake

3.5.4 The energetical value of jet and wake flow 3.5.5 Influence of the parameter v on

impeller performance . . . . 3.5.6 Influence of the impeller outlet width b

i i i v 1 2 4 4 6 7 8 9 9 11 11 12 14 14 14 18 18 20 22 26 27 27 28 32 34 36 38

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3.6.2 Equations for the impeller outlet flow 3.6.3 The impeller work equation

3.7 Disc friction . . . SHAPTER 4 - THE MIXING PROCESS 4.1 Introduction . . . .

4.2 Theoretical computation of the mixing wake flow, taking into account the of the fluid . . . . 4.2.1 Assumptions . . . .

zone of a jet-compressibility

4.2.2 Forces acting upon the jet and the wake 4.2.3 Equations for the mixing process

4.2.4 Solution of the equations for the mixing process 4.3 Results of the theoretical computations

CHAPTER 5 -VANELESS DIFFUSERS 5.1 Application field.

5.2 5.1.1 Advantages 5.1.2 Dtsadvantages 5.2 Computation method

CHAPTER 6 - VANED ISLAND DIFFUSERS 6.1 General geometry . . . .

6.2 Computation method . . . 6.2.1 The vaneless space 6.2.2 Semi-vaneless space 6.2.3 The divergent channel 6.3 Dump diffusion

REFERENCES

APPENDIX - SOLUTION OF THE EQUATIONS FOR THE MIXING PROCESS

TABLES FIGURES 40 42 43 45 45 45 45 46 47 50 50 52 52 52 52 53 54 54 ~4 55 55 56 58 61 65 67 69

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A one dimensional computation method for the design of a centrifugal compressor is developed, which takes into account various real floweffects, such as flow separation in the impeller, jet-wake mixing in the vaneless space, transonic vaned diffuser performance and diffuser outlet dump diffusion. Several numerical examples are worked out in detail, to show the influence of different important geometrical and aerodynamical parameters on the compressor performances.

This approach is also the one used for a VKI computer program COMRAD.

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A AR a a* b cf cM Cm Cp Cp °ax OR Dh d E ,

.

m

N

s PR p q q Q R

Rc

RG RPM LIST OF SYMBOLS geometric area area ratio sonic speed critical speed axial width

wall friction coefficient

jet-wake shear friction coefficient disc friction coefficient

specific heat

static pressure recovery impeller axial length diffusion ratio

hydraulic diameter

impeller blade thickness energy

friction force

::;:lf:::::1P~=

ó:l

static enthalpy

absolute wall roughness blockage factor

curvature Laval number

r~ach number

relative Mach number mass flow

specific speed (Baljé) pressure ratio

sta tic pre ss u re

inducer blade blockage :

pressure fluctuation in vaneless space inlet volume flow

radius

radius of curvature gas constant

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RV s S S T U V W z 8 0* e: 80

28

n nss ntt nst K À À )..l \! \! p T T w

inducer hub to tip radius ratio axia1 gap behind impe11er disc entropy surfaee statie temperature eireumferentia1 speed absolute ve10eity re1ative ve10eity

number of impe11er b1ades absolute flow ang1e

re1ative flow ang1e displacement thickness impe11er b1ade clearance wake width

momentum thickness vanes diffuser ang1e adiabatic efficiency

static to static efficiency tota1 to tota1 efficiency static to tota1 efficiency isentropic exponent

re1ative wake mass flow head 10ss coefficient slip factor

kinematic viscosity

wake to jet re1ative velocity ratio density

time

shear stress

angu1ar po1ar coordinate in meridiona1 p1ane 10ss tota1 pressure 10ss coefficient

angu1ar speed Subscripts

o in1et plenum

1 inducer in1et

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2 impeller discharge

3 diffuser leading edge

4 diffuser throat section

5 diffuser channel outlet

6 dump diffusion a absolute h hub j jet m meridional n normal t tip u tangential w wake w wa 11 bl blade cl clearance df disc friction diff diffuser fr friction hom homogeneoLis imp impeller i nd inducer mn mean pr pressure side sh shear layer

suc suction side

Superscripts

0 total

i s isentropic

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LIST OF FIGURES

number title page

1 Schematic of compressor stage flow regions . 69 2 Baljé-diagram for optimum specific speed. 70 3 Influence of PR on MWlt for different 70 values of NS . . . . .. . . . . 70

4 Inlet velocity triangles . 71

5 Influence of prerotation on MWlt and M2' for

different values of PR 71 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29

Inlet guide vane losses

Geometry of centrifugal compressor rotor

Influence of blade blockage on inlet velocity triangle . . . . Influence of RV on MWlt Influence of RPM on MWlt Influence of al on MWlt Influence of Rlh on MWlt Adjustment of RV . . . . Adjustment of RPM

Influence of wall curvature on boundary layer development . . . . Influence of OR on compressor efficiency

Comparison of diffusion performances of rotating inducers and stationary diffusers . . . Influence of DR and MWlt on compressor

effi ci ency nc . . . . . Eckardt's impeller - elliptical profile

approxi-mation of a real impeller

Elliptical profile approximation of a real impeller . . . .

Geometrical model for separation Impeller blade shape . . . . Flow angle variation . . . . Meridional velocity profile Separation section geometry Jet-wake model . . . .

Tangential equilibrium at impeller outlet T,S diagram of impeller flow. . . . . .

Inf~u~~ce ,of ,v = W2W/W2j on the wake width E2 and ón thê wake mass flow À

72 _ 73 73 74 74 75 75 76 76 77 77 78 78 79 80 81 82 82 83 83 84 85 86

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31 32 33 34 35 36 37 38 39 40 41 42 43 44

Influence of the impeller width b2 on

the losses. . . . . .

Jet-wake velocity triangles . .

Disc friction coefficient cM versus axial gap S T,S diagram of the impeller outlet state

Pressure fluctuations in the vaneless space. Mixing process . . . . Vaneless diffuser boundary layer development Vaned island diffuser geometry . . .

Diffuser channel geometry . . .

Calculation of diffuser leading edge state Diffuser throat blockage versus actual static

pressure recovery from leading edge to throat Channel pressure recovery versus AR and L/W . Maximum pressure recovery versus aspect ratio AS

and throat blockage B Dump d.iffusion process

88 89 90 91 92 93 95 95 96 96 97 97 98 98

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INTRODUCTrON

The real flow through a radial compressor is essen-tially three dimensional, viscous and instationary. Up to now, there is no mathematical model which allows to predict the flow in such a machine without neglect;ng some important aspects of the problem. In fact, it would be extremely complicated both due to the complexity of the flow and the complexity of the boundaries of the machine.

Nevertheless, there is an urgent need for the designer to dispose of a calculation method which allows to predict the main characteristics of a centrifugal compressor and to inves-tigate the influence of various parameters on the compressor behaviour. Therefore, the calculation method has to be fast enough to allow iterative operation, but at the same time suf-ficiently elaborated to take into account some important flow phenomena, such as separation, Mach number influence, boundary layer blockage, losses, etc.

The approach described in this report is the one used in a VKI computer program (COMRAD) to calculate the performances and dimensions of a radial compressor, starting from mass flow, required pressure ratio, RPM and some geometrical relations~

The method is based on the actual knowledge of real flow in a centrifugal compressor, as described briefly in chapter 1. In the following chapters, the flow in the different parts (IGV, rotor, diffusor, etc.) will be described in more detail and at the same time the equations used in the program are derived.

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CHAPTER 1 - BRIEF DESCRIPTION OF THE FLOW THROUGH A CENTRIFUGAL MACHINE

A compressor can be divided into different parts, as shown in figure 1 (Ref. 1). Af ter being deflected by the inlet guide vanes (IGV) the flow enters the inducer where it is decelerated and turned into the radial direction. The pre-sence of a radial velocity component is responsible for

coriolis forces, which together with the blade curvature ef-fect, tends to stabil ize the boundary 1 ayer at the suction side of theinducer (Refs. 2,3). Due to this stabilization, the boundary layer becomes less turbulent, ánd will easily separate under influence of an adverse pressure gradient.

Once the flow is separated, we distinguish a high energetic jet, with a high relative Mach number and a low energetic wake,feeded by secondary flows. The jet can be con-sidered as an isentrQpic core with a constant Mach number in the flow direction (Ref. 1).

Af ter leaving the impeller, a strong mixing takes place between jet and wake, due to the difference in angular momentum. This results in an intensive energy exchange and a fast uniformization of the flow.

In case of a vaned diffuser, the flow enters the semi-vaneless space - this is the region between the leading edge and the throat section of the diffuser - and a rapid adjustment rearranges the isobare pattern from parallel to perpendicular to the flow direction. If the Mach number is higher than 1, a shock wave system will decelerate the flow in such a way that the throat ~ection becomes subsonic (design condition) .

In the divergent channel, a further decrease of the velocity is realized with a subsequent increase of static

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weak that separation occurs, which limits the st~ix pressure rise. In case of vaneless diffusers, af ter the jet-wake mixing process, the flow is further decelerated by an increase of flow section corresponding to the radius increase and influenced by friction on the lateral walls. Each part of the compressor can be characterized by one or more typical parameters, p.e., the diffusion ratio OR for the inducer, the mass flow ratio ~

for the separated impeller flow, the pressure recovery Cp for the diffuser, etc. Their values are based on experimental data and empirical correlations.

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CHAPTER 2 - lNLET GUlDE VANES (IGV)

2.1 Purpose of lGV

Figure 2 shows the Baljé-diagram (Ref. 4), which gives the variation of adiabatic compressor efficiency 6na d versus

the specific speed N : s

N s

=

RPM·v 3 Q

6H~

with Q

~H

inlet volume flow manometer height

(ft3jsec)

(ft)

( 2 . 1 )

For th~seunits, the optimum specific speed is approximately 120. For an increasing pressure ratio, PR, at constant value of the specific speed and inlet volume flow, the inducer relative tip Mach number MWlt will increase too. This variation has been

calculated by Dean (Ref. 1) for different values of Ns (Fig. 3). From this figure, it can be seen that for the

speed Ns

=

100, the critical value MWlt

=

1 will already be reached for PR =4, while for a 8:1 compressor this relative tip Mach number will be as high as 1.4.

The supersonic Mach number will not only give rise to strong shock losses, but will also induce early flow separa-tion, which results in very high losses. A possible solution for this problem consists in reducing the specific speed Ns by lowering the RPM (Fig. 3). This has of course its influence on the rotor design. The impeller channels will be longer and more narrow, which involves additional shroud leakage, friction

losses and secondary flows, with a subsequent efficiency drop. Another possibility ;s to make use of preswirl vanes. This can be explained by means of velocity triangles (Fig. 4).

A turning of the flow in the direction of rotation results in a noticeable decrease of the relative velocity component and relative flow angle. When lookin~ to the Euler

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equation :

( 2 .2)

we remark a decrease of rotor-work, due to the fact that the inlet tangential velocity is no longer zero. Consequently, an increase of the rotor diameter will be necessary to hold the same pressure ratio. However, the impeller outlet Mach number will increase too. This mechanism is shown in figure 5.

We see that for a PR equal to 6, and the inlet flow prerotation varying from 0° to 40°, the inducer tip Mach number will de-crease from .9 to .7, while the impeller outlet Mach number increases from 1.1 to 1.2. Roughly, as long as

( 2 .3)

IGV are efficient.

It can be seen fr om figure 5 that this condition will be ful-filled for al

<

30° (N s

=

70).

For higher values of PR, the increase of M2 will be more im-portant than the decrease of M~lt when prerotation becomes

greater than 30°. The range of IGV is thus limited by an optimi-zation of the Mach number dependent lo~ses in wheel and diffuser.

In conclusion it can be said that IGV provide an addi-tional degree of freedom in determining the relative Mach number at the inducer tip.

For an investigation of the influence of compressor inlet adjustable guide vanes for the control of single shaft gas turbines, we refer to reference 5. This study shows that the use of a variable prewhirl control to produce rated power under a wide range of ambient conditions is very promising, helping the designer to meet specifications otherwise impos-sible to meet.

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2.2 Isentropic calculation of IGV

We consider a compressor with a straight inlet channel wherein the flow is uniform. The IGV modifie this velocity

distribution by creating a tangential velocity component Vu. The radial equilibrium at the outlet of the IGV can be expres-sed as

2

l

~

=

Vu

P dR R

( 2 .4)

The equation of Barré de Saint-Venant gives arelation between p, V, Po and Po V2 + 2 K

11K

Po K-1 Po p K-1 K

K

Po ( 2 . 5 ) = -K-1 Po

Wh en this equation is differentiated and substituted in (2.4), together with relations deduced from the velocity triangles, we obtain dV! 2 .

11K

1 Vasln et det + 1

[P;

1

~ = 0 ( 2 .6) - - + 2cos2et dR COS 3et dR Po dR

As the flow between the inlet plenum and the IGV is isentropic, we have

( 2 .7)

Introducing ( 2 . 7 ) in (2.6) gives

2

1 dVa

+ 2tget det + 2 sin2et = 0

-V2 dR dR R

a

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Equation (2.8) allows to calculate the Va(R)-distribution that corresponds to a given a(R)-distribution. In what follows, this

is done for three"different typical prewhirl models, which are avai lable as options for program COMRAD.

This type of IGV has already been used and experimental results are available (Refs. 6, 7).

Substitution of da

=

0 in eq. (2.8) gives :

2 1 dVa - - - + V 2 dR a 2 Sln . 2 a R dR

=

0

Equation (2.9) can be integrated

( 2 .9)

( 2 . 10)

The coefficient al can be deduced from the volume flow equation RIt

J

-sin2"

Q

=

a I R 21TR dR Rlh

( 2 .11 )

With Rlh hub radius of IGV RIt tip radius of IGV

Elimination of al from (2.10) and (2.11) gives the distribution of the axial velocity component Va in function of the radius R and the choosen pr~rotation angle a :

Q(1+cos 2a)

( 2 . 12) 1+cos 2a 1+cos 2a

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With the assumptions of isentropic and uniform flow, the values pI,T1 and PI can be calculated as :

(2.13) K K=T PI

=

Po

l:: 1

(2.14) _I_ K-I PI

=

Po

l:: 1

(2.15)

A similar method of calculation has been proposed by Vavra (Ref. 8).

K

V =

-u R

A free vortex flow is defined by

The absolute flow angle a follows from

tana

=

V

u K

=

By substitution of (2.17) in (2.8), it can be shown that

=

0 (2.18)

(2.16)

(2.17)

The axial flow component is thus constant over the blade height and can be determined by the continuity equation :

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The values of PI' Tl' PI can be calculated with equations (2.13),

(2.14), (2.15).

2.2.3 Forced vortex IGV

---A forced vortex flow is defined by

v

= K R

u

The absolute flow angle a follows from

Substitution of (2.21) in (2.8) gives 2 R _2_ da + 2sin2a

=

0 tana dR R Integration of (2.22) yields R

=

Cl ~ina !1+sin2a for a

>

0

The integration factor Cl can be determined by continuity

(2.20 )

(2.21)

(2.22 )

(2.23)

(2.24)

The values of PI' Tl' PI can be calculated with equations (2.13),

(2.14), (2.15).

2.3 Calculation of IGV losses

The losses in the IGV are very small compared with the losses in other parts of the compressor, and can normally be

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neg1ected except in high def1ection cases.

Figure 6 (Ref. 6) gives a qua1itative sketch of the main parameters determining the IGV losses. It can be seen that: - The 10ss coefficient depends strong1y upon the span.

High 10sses at the tip of IGV (100% span). Neg1igib1e 10sses at the hub (0% span).

- Negative preswir1 (opposite to the direction of rotation) gives rise to astrong increase of the 10ss coefficient. For a theoretica1 and quantitative 10ss computation, we refer to Stewart (Ref. 9).

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CHAPTER 3 - THE ROTOR

3.1 General geometry

Figure 7 gives the general geometry of a centrifugal compressor rotor. In our model, three important flow sections are taken into account:

- The inlet section (1)

- The separation section (SEP)

- The outlet section (2).

At the inlet section, the flow is axisymmetric. However, all flow quantities vary with the radius R : Pl(R), T1(R), V1(R), 0l(R), The relative flow is then decelerated between the rotor blades until separation occurs. Due to coriolis and curvature effects, the separation point will be located at the shroud-suction side intersection. The separation section is defined as the cross section through the separation point.

In this way the rotor has been devided into two parts which are treated separately :

- the inducer flow (1 + SEP),

- the impeller flow (SEP + 2)

The impeller flow can also be divided into two subflows - the jet flow (SEP + 2J)

- the wake flow (SPE + 2W).

This division of the rotor flow into subflows is an important feature in our approach, because in this way some real flow pheno-mena can be included in the computations.

One of the most important parameters determining the rotor losses will be the wake width E2' which is function of

the separation point location. If the inducer is well designed, and much deceleration can be achieved before separation occurs, this point will be located near to the impeller outlet, and the wake will not develop as much. The wake width E2 will be

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At the contrary, if we have a bad inducer, and early separation occurs, th en the wake will grow to a large part of the impeller flow and the mixing process behind the wheel will involve very high losses with a subsequent drop of the efficiency.

3.2 The inlet blockage

When the flow enters the wheel, the free frontal area is reduced by the presence of the blades. This involves a flow con-tra c t ion wh i eh · eh a n ges t h e vel 0 c i t Y tri a n 9 1 e s b y a c c e 19" a tin 9 t h e

axial velocity component from Va to V~ (Fig.

8).

The relative flow angle BI will be turned over an angle ikB

l to the new value B~. If the influence of the blade curvature is neglected, then

I

the optimum BI has to be equal to the geometrie blade angle Blbl. From Stanitz (Ref~ 10) we get the value of ikB :

1

ta n i kB

1

k

Bl represents the procentual free stream section

=

1

-with d

z R

dz

the blade thickness (normal to camber) number of rotor blades

radius.

The blade angle can thus -be calculated as

I

Blbl

=

BI = BI - ikB

l

I

The new relative velocity Wl can be calculated as

The new axial velocity component is

( 3 . 1 )

(3.2)

( 3 .3)

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The absolute flow ang1e al follows from

a~

=

arctg [tga l t9S ;] tgs 1

I

The ve10eity VI is

The absolute flow ang1e al can a1so be ea1eu1ated as

( 3 . 5 )

(3 .6)

( 3 .7)

( 3 .8)

The new statie temperature T~ ean be derived from the energy equation, when accepting that no work has been done on the f1uid during the eontraction.

(3 .9)

Supposing an isentropie proeess, the statie pressure PI beeomes

K

K-l

P;

=

P,

[~:]

(3.10)

The new density PI fo11ows from the idea1 gas equation

I

PI PI

=

I

RGTI

(3.11)

It is important to notice in previous ea1eu1ations that, sinee UI varies with the radius R, all quantities VI' WI' al' BI' PI' Tl' and PI are funetion of R.

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-3.3 Determination of the inducer hub and tip radii

The minimum hub radius Rl h. isfjxed by mechanical mln

considerations; Two criteria hold in this case:

- The minimum hub radius can be determined by strength considera-tions, which require a minimum sectional area for the axis to transmit the engine torque and to avoid critical velocities. - The minimum hub radius Rlh. can be limited by the maximum

mln blade blockage qmax at the hub :

dz (3.12)

=

Rlh. is of ten limited by the minimum shaft diameter and is mln

therefore used as an input parameter in our program. The cor-responding blockage qmax is calculated.

The determination of RIt is more complicated, because we want to limit the relative inducer tip Mach number MWlt. The

relation between these two parameters can be demonstrated with a simple example. Suppose a centrifugal compressor for freoo .

with following characteristics :

mass flow

m

=

2.5 kg/s gas constant isentropic exponent inlet density - maximum inlet blockage - inlet temperature RG = 75.3 J/kgOK K

=

1.136 PI

=

4. kg/m3 l-k BI

=

.02 Tl = 283 ° K

The rotational speed RPM, the prerotation angle al and the inducer hub radius Rlh are taken as input parameters. The sonic velocity a I i s :

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For a uniform inlet flow with constant prerotation, following equations are valid

UIt

=

2lrRPM Rl t 60

.

VI a

=

2 m 2 k BI lr(Rlt-Rlh)PI

In our model, the inducer hub and tip radii are taken together

in one parameter RV

=

Rlh/Rl t ·

The inducer tip relative Mach number MWlt can also be expressed

as a function of the following parameters or

l · r

t"RPM

Rl h _ tga 1

1

2 1 m m M = WIt al 2 1 -1) 60 RV 2 (_1_ kB lrPIRlh ( - - kBllrPIRl h -1) 1 Rv2 RV2 ( 3 .13 ) In figure 9 this equation i s plotted versus RV for

RPM

=

16 000

This graph presents a minimum value of MWlt

=

.85 for an inducer

hub-tip radius ratio RV

=

.6. At the left of this point, for

smaller values of RV, the Mach number M ~J will increase, due to

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the higher values of the circumferential velocity Ult. At the right of point M, for higher values of RV, the Mach number MWlt will increase as well, because the inlet flow section is reduced, with a subsequent increase of the axial velocity Vla'

An important conclusion is that, for a given value of RPM, al and Rlh' it will not always be possible to find a solution for RV (say RIt)' if the relative tip Mach number is limited.

The only way to overcome this difficulty is to adapt one of the parameters RPM, al or Rlh' Figures la, 11 and 12 show the in-fluence of each of these parameters respectively.

Figures la and 11 show that reduction of RPM or use of positive preswirl resul~ in a decrease of the relative inducer tip Mach number. This conclusion has already been drawn when discussing the IGV (cfr Chapter 2).

Figure 12 shows only a slight decrease of the minimum relative Mach number when the hub radius is reduced. Keeping al and RPM unchanged, it will not always be possible to keep Mlt below a given value by variation of Rlh and RV only.

In the program COMRAD, following procedure has been adopted

- The prerotation angle al and MWlt,max are fixed input data.

- RPM and RV are also input data, but one of them can be adjusted, in order to reduce the inducer tip Mach number below a given maximum value. The adjustment is done automatically and the new value of the parameter is printed out. (see Figs. 13, 14).

- The inducér hub radius Rlh is initially equal to its minimum value Rlh ,mln . ~which is an input value. For given values of , Rlh/R 1t , and RPM, the program will increase Rlh with steps of 5% until MWlt becomes less th~n MW1t,max' If this is not pos-sible, one of the parmeters RV or RPM will be adjusted, ac-cording to the key value 1 and the procedure starts again from R1h

=

Rlh,min'

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3.3.2.1 ~dÏu~tme~t_of ~V

This method is explained in figure 13. Suppose that a large value is choosen for RV (.75). R1h is then increased from Rlh,min (point a) with steps of 5%. As long as MWlt is decreasing, we continue the iterations. At the right of the minimum b of the curve, MWlt will increase again, without having reached the value of MWlt ,max .

The program will then automatically decrease the value of the hub-tip radius ratio and start again from R1h = Rlh,min

(point c). The new minimum value is less and a new iteration cycle can start (c ~ d). Adjustment of RV will occur as long as the minimum of the curves is higher than MW1t,max. The computa-tion stops at point h.

It is important to notice that the reduction of the minimum of the curves for decreasing RV is rather weak, and

limited by that value of RV that gives a minimum for MWlt at R1h

=

R1h,min·

3.3.2.2 ~dÏu~t~e~t_of ~P~

This method is very similar to the previous one (cfr Fig. 14). The shift of the minimum of the curves when RPM is

decreasing is more important and not limited, because the minimum is shifting to the right of the plane (away from Rlh,min).

Nevertheless, the RPM of a machine is very of ten determined by mechanical considerations, and has a direct influence on specific speed and thus also on maximum efficiency.

REMARK : No iteration will ne carried out when MWlt is less than MW1t,max at the beginning of the computation. R1h is then set equal to R1h,min.

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3.4 The inducer flow

As shown in § 3.1, the inducer is defined as that part of the rotor where the boundary layers are attached. The purpose of the inducer is threefold

- deflection of the flow in axial direction; - deflection of the flow in radial direction;

- diffusion of the relative flow to increase static pressure. This results in a heavy loa~ for the boundary layer, especially at the shroud-suction side intersection. Next considerations explain briefly why.

A. Adverse pressure gradient : diffusion means a deceleration

or conversion of dynamic energy into static pressure. Consequently, there will exist an adverse pressure gradient.

Separation of the boundary layer will occur when the kinetic energy available in the boundary layer and the one added by en-trainment is dissipated.

B. Coriolis effects : because of the radial velocity component, important coriolis accelerations can exist in radial impellers. It is shown by Rothe

&

Johnston (Ref. 2), that due to the corio-lis forces, the boundary layer on the pressure side is desta-bilized and becomes more turbulent. On the suction side, the. boundary layer is stabilized and has less turbulent mixing. Turbulent mixing increases the entrainment and thus also post-pones the separation point. We thus can conclude that in a radial impeller separation occurs, or is likely to take place at the suction side of the blades and is very unlikely on the pressure side of the blades. However, the loading distribution along the

~

blade and the existence of a relative flow vortex -2w can

dece-l~rate the flow on the pressure side to negative values, so that return flow and a potential separation bubble can occur on the pressure side. The last possibility is not considered in our method because this should be avoided by a good blade to blade design.

(31)

C. Wall curvature effects : wall curvature is also creating a transverse pressure gradient. This one is related to

centri-petal accelerations (Fig. 15). Turbulence is influenced by

centripetal accelerations in a very similar way as by coriolis

accelerations. The boundary layer is stabilt~ed on the convex

surface and destabilized on the concave surface. In a radial compressor rotor the shroud is an annular convex surface and the relative flow will be less resistant against separation. In combination with the coriolis forces on the suction side, we can expect that flow separation starts at the suction side-shroud intersection line. Similar as for axial compressors, the relative velocity at separation can be related to inlet velocity by a diffusion ratio

OR =

=

Relative flow velocity at inducer tip

WSEP Relative flow velocity at separation point

The higher the diffusion ratio, the further downstream will be the separation point and the smaller will be the separated region. Consequently, the efficiency will increase.

According to Oean (Ref. 1), the compressor efficiency

relates to OR and CPd (diffusor pressure recovery) as ~own in

figure 16. For constant Cpd , the efficiency increases with DR.

For values of OR higher than 1.4, the efficiency curves become very flat, and it seems to be more interesting to pay attention for the diffuser rather than for the impeller diffusion process.

In our one dimensional design program, the expected OR has to be defined and the method is valid only if the predicted OR can also be achieved. The OR is mainly a function of rotor geometry which means that this one dimensional design method must be completed by a detailed three dimensional design.

Reasonable values of OR are shown in figure 17 (Ref. 1) as a

function of inducer tip relative Mach number MW1t. On the same

figure the maximum diffusion ratio for radial diffusers (OR

(32)

by coriolis forces and curvature.

An increase of MWIt at constant DR will result in a higher separation velocity Wand W2 · (relative velocity of

sep J

jet flow at outlet of impeller) will increase proportionally. This results in higher "mixing losses" at the impeller outlet

(Fig. 18) and shock losses when the flow becomes transonic.

3.4.2.1 Hub- and shroud contour

For the computation of toe inducer flow, the shroud and hub contour have been represented in the meriodional plane by elliptical profiles. Comparison with data from literature (Ref. 11) shows that good agreement is obtained (Fig. 19). This method has the important advantage that both hub- and shroud contours can be determined completely with only 5 parameters: RIh , RIt' R2 , b2 , DAX. The impeller considered

at figure 20 is a small radial compressor with an inducer, similar to those commercially available for turbochargers (Ref. 11bis). In this case, the substitution of hub- and shroud contours by elliptical profiles is not so good due to the linear hub shape at the impeller outlet.

The inducer is further divided into 5 equidistant annular stream surfaces (1 to 5 on Fig.. 21) and a hub (6) and shroud (7) stream surface. They will be used to calculate approximated values of local parameters, and also facilitate the calculation of mass averaged values at different sections.

3.4.2.2 ~l!d! ~n~l~ ~a~i~tlo~

The blade angle variation used in our model is an approximated one and is based on an investigation of blade profiles of jmpellerswith elliptical inducer blade shape. E. Schnell (Ref. 12) shows that an optimal blade loading is obtained using this kind of inducer shape. However, our

(33)

defi-nition makes an extension for the impellers with backward bended blades (Fig. 22) : Definition: O<~~.!. 3 3.4.2.3 Il~w_a~gle_v~ria!io~ (3.14)

At the outlet of the wheel, the flow angle 82 differs from the blade angle S2bl due to the effect of the slip factor

1.I (cfr 3.6). When ]l is known (from experimental correlation), the flow angle 82 can be calculated. In our model, we agree that the slip effect starts at ~

=

60°. From the inducer inlet to

~

=

60°, the flow is supposed to be tangent to the blades. From

~ = 60° to the outlet, a gradual increase of the slip is taken into account Definition 8

=

Sb 1 (~- .!.) S = 8 b 1 -;-f (S2-'82bl) 3 .!.< 'IT ( 3 .15 ) ~ ~ -'IT 3 2 -6

(34)

3.4.3.1 ~elo~i!y_p~o!ile_i~ !h! ~e~i~i~n~l_pla~e According to Vavra (Ref. 13), following relation exists for an axisymmetric stream surface :

(3.16)

with the relative meridional velocity

km the curvature

n the normal direction.

For an annular stream tube (Fig. 24), this expression can be in teg ra ted : W m = 'W m. e 1

r

k m· ( n -

.!!!.)

2b + k mJ.

.!!!.]

2b l 1 with km

>

0 b small compared to R., R .. 1 J

The relation between Wmi and Wmj is

= ~I e

J

(3.17)

(35)

With this equation, the ~lative meridional velocity W

m can be determined along each intersection line with the elliptical stream surfaces (Fig. 21).

shroud W

msep

The calculation starts at the shroud, where shroud

(3.19)

cos (13 )

sep

When the meridional velocity profile is determined, the relative velocity follows from :

; COs(Ssep)

i refers to a stream

surface (3.20)

Remark : The curvature km in a point (xo,Yo) on the ellipse x2 y2

+ --

=

1 can be calculated with A2 B~

(3.21)

3.4.3.2 fo~s!a~t_r~t~alpl

This equation is derived from the energy law and is also valid for non-isentropic flow

2 2

=

Wli-Wsep,i

2 2 (3.22)

It shows that the increase of enthalpy Cp(T e sp, , .-T l ,.) between inlet and separation is composed of :

(36)

2 2

-+ WIi-Wsep,i kinetic energy drop according to the variation of

velocity. This term is strongly dependent on the i nducer des 19n.

2

2

i ncrease of 11 centri fuga 1" energy.

This term cannot be improved, because it is not dependent on the flow.

3.4.3.3 ~t~tlc_p~e~s~r~

For an isentropic flow, the variation of static pres-sure is given by

IS

P .

sep,' (3.23)

A loss coeffic;ent w. d allows to correct for real flow friction , n

losses

IS

Psep,i

=

Psep,i (3.24)

where PI and WI are mass averaged values of Pli and WIi ·

Psep,i

=

ckage ê *

Psep,i (3.25)

3.4.3.5 ~o~n~a~y_l~y~r_ê~l~ula!i~n

The loss coefficient w. , n d and the boundary layer blo-are calculated by an approximated boundary layer cal-culation as explained by A. Sarmento in refe ence 14.

(37)

8 X+~X (3.26)

can be integrated along the surfaces, assuming a linear variation of pand W between inlet and separation point, and by

intro-ducing following empirical correlations from reference 15 : _.265 -1.56II:f Cf

=

.246 Re e (3.27) H

=

1. 63

-

.0775 10gI0(Re) (3.28) • 8 v • 2 80

=

.2 RIt

( - )

WIt (3.29)

Once we know 8 and H (function of the change in relative velocity) we can calculate the boundary mayer blockage 0*, that will be

used in the continuity equation.

The total friction force Fr in the inducer can be calculated as 'w dS =

J

S. d 1n 1 p cf ~J2 dS 2

with Sind : the total wall surface of the inducer. The loss coefficient wind is then :

~o Pind Fr wind = 1

PIW~

1 A A 2 PIWISsep 2 2 0

wi til llPind the total

I pressure loss in the inducer

Ss ep the area of the separation section.

(3.30)

(38)

3.4.3.6 fo~tln~i!y

The mass flow through an annular flow section 21) of the separation section is equal to (Fig. 25) :

(F i 9 .

m

.

= p .W . (21fR .b .coSB .-z·b .(d+ó*))

sep,l sep,l sep,l sep,l sep,l sep,l sep,l

with d blade thickness

Ó* boundary layer blockage

z number of blades.

The total mass flow is then

.

~ m .

i sep,l

(3.32)

( 3.33)

To perform calculations following basic assumption has been made: "when the deceleration of the relative flow at

W1t

the shroud streamline reaches the value - - , separation occurs. OR

This point on the shroud contour is cal led separation point, defined by the radius Rsep. The flow section through this point, normal to each of the elliptical stream surfaces (Fig. 21), is defined as the separation section. The calculation starts with an arbitrary first guess of R . The meridional velocity

pro-sep

file, function only of the impeller geometry, can then be cal-culated assuming also that Wsep

=

W1t/OR. The other flow condi-tions are then given by the equacondi-tions 3:16 - 3.31.

The value of the mass flow

m

sep is then calculated with eq. (3.32) and will generally by different from the input data

m,

due to the misestimation of R sep . By checking continuity we will change the value of R in an iterative procedure.

sep

The value of R in two consecutive iterations is given by

(39)

n+l Rsep

=

n n-1 R -R sep sep .n n-l msep-lfIsep n (ril -ril) sep

with n : the iteration number.

(3.34)

The iteration stops when the computed value of msep is equal to m within a precision of 1~.

3.5 The impeller flow 3.5.1 Real floweffects

---Figure 26 shows schematically the jet-wake model as used in the program. To find arelation between flow conditions at the separation point and the impeller exit, it is necessary to make the following important approximation, as suggested by Dean (Ref. 1). He asserted that the jet flow is little subjected to shear stresses in the rotor and can be considered as an isen-tropic core. All flow outside this core can be considered as belonging to the wake. This is evenmore true when there is a tangential pressure gradient over the jet, due to the rotor work creating secondary flow that moves all low energy fluid to the suction side. For a compressible, flow, Dean shows that the mean relative Mach number remains constant along the jet from separation to rotor outlet :

MWj

=

cst or

(3.35)

(3.36)

The mass flow in the wake is not zero and has been characterized as a percentage of the total mass flow

.

mw À

=

-

.

m

.

,

mw is developed by secondary flows and by "tip leakage".

(40)

The wake can be look~d at as a pool, wherein all low energetic fluid is flowing together. All friction- and leakage losses are accummulated in the wake and the corresponding losses will be added to the main flow during the mixing process downstream of the impeller.

In our model, the parameter determining the jet-wake velocvty profile in the wake-jet relative velocity ratio v :

v

=

(3.38)

By fixing v, instead of À, the mass flow in the wake will depend

also on the extent of the wake. Obviously, the choice of v is not free. It should be correlated to the influencing parameters, secondary flow, clearance, wake width €2' etc. However, at the actual state of research, this correlation is unknown. The

designer can handle it as a supplementary degree of freedom. Our experience has learnt us to choose the parameter v not too large. Based on the results of Eckardt (Ref . 16) and Fowler (Ref. 17), this value can be fixed at

v

=

.2.

Another important feature of our model is that the same relative outlet angle 82 is used for the jet and the wake

(3.39)

Energy equation

=

Wsep-W2j + U2-U sep (3 : 40)

2 2

Tsep' Wsep' Usep are the mass mean values of Tsep,i' Wsep,i' Usep,i'

(41)

Model equation Constant relative Mach number along the jet flow Gas equation P 2'

=

J P2 . J (3.41) (3.42)

Continuity equation From the definition of the wake to total mass flow ratio À, we can deduce that :

(3.43 )

wh ere E2 is the procentual passage at the outlet, occupied by the wake. À is not an input data, but will be calculated in

function of v. Statie pressure P2j K-1

.

[T

2'l

K

P2j

=

Psep

~

Tsep IS

The statie pressure isentropic value P2j IS

IS 1

p

For an isentropic jet flow we have

(3.44)

j i s calculated by correction of i ts by means of a loss coefficient Wjet

.

.

·2

P2'

=

P2 .

-

Wjet Psep

W

sep (3.45)

J J 2

In Dean's theory, the jet flow is assumed isentropic, and all losses are connected with the wake flow. Consequently, Wjet is zero. However, this excludes the possibility to analyze wall friction losses and clearance losses as a function of rotor geometry.

(42)

Therefore, in our model, the jet loss coefficient is a function of the wall friction losses and clearance losses:

(3.46)

The wake flow takes only into account the separation losses. (a) The friction 10ss coefficient wfr

wfr is estimated by means of hydraulic diameters of and length between the separation section and the rotor outlet

D

=

4 hsep D

=

4 h2 . J L hsep ,2j Area Conto u r Area Contour ~ 4 sep 21TR 2b2 ~ 4 z z 2 2 1T(R sep ,7- Rsep,6) Z cos<j> cos<j> (1-E:2) 2j 2· 21TR 2 (l-E:2)+2b 2 Z R2- Rsep

,3]

cos<j> (~ - <j» 2 8 +8 1 cos( sep,3 2,b) 2 (3.47) (3.48) (3.49) (3.50 )

The Reynolds number in the impeller Reimp is calculated at the separation section :

(43)

(3.51)

The wall friction coefficient cf is a function of the Reynol.ds number and of the relative wall roughness

0

k :

hsep

(3.52)

This relationship is calculated using implicit formula of Colebrook and White for the head loss coefficient À :

~

= -

210 9 [ k + 2.51

1

3 . 7 0 h R e\/ À

(3.53)

The wall friction coefficient is then

À

cf

=

4 (3.54)

Expression (3.53) can also be written in an explicit form .0625

-21

0g ( k

)]llj2

Re 3.7D h

U

(3.55)

(b) The clearance 10s5 coefficient wcl

According to Jansen (Ref. 18), the clearance 105s coefficient can be expressed as 2 2 °Cl RIt U2 w cl

=

2.43 ( 1

-

- ) (3.56) b2 R2 W2 sep

(44)

Energy equation

A2 2 2 A2

=

Wsep-W2w + U2-U sep

(3.57)

2 2

Model equation : The re1ative wake velocity is determined by the parameter v, called the wake)jet re1ative velocity ratio:

(3.58)

Gas equation

P2w

=

(3.59)

Continuity equation : The wake mass flow is determined by the parameter À, which has to be ca1cu1ated in function of v :

Tangentia1 equilibrium : T~e wake ~tatic pressure P2w cannot be determined by the isentropic equation plus 10ss coefficient, because this flow is essentia11y irreversib1e. It accumu1ates near1y all the rotor losses. Therefore we deduce the tangentia1 pressure gradient at the rotor outlet from equilibrium equations and derive the mean static wake pressure P2w from the static pressure in the jet, P2j'

Figure 27 represents the equilibrium of inertia1 forces for the jet. RC2 is the radius of curvature of the stream1ines at the rotor outlet, and is supposed to be constant over the who1e section. Starting from

P2,pr

.

.

the static pressure at the pressure side of the b1ade P2,SUC: the static pressure at the suction side of the b1ade P2,sh the sta tic pressure at the shear 1ayer between jet and

(45)

we define

P2 . J

=

P2

,e

r +P2 ,Sh

2 ( 3 . 61)

P2w

=

P2,sh+ P2,SUC

2 (3.62)

The inertial forces in the jet, which are acting upon a flow particle with mass dm, are

a) the coriolis forces t

Fcor,j

=

2dm 0 W2j (3.63)

b) the centrifugal forces t

Fcentr,j = dm 02 R2 (3.64)

c) the normal component of the relative flow inertial force t

F re , n , 1 J . (3.65)

d) the tangential component of the relative flow inertial force t

Frel,t,j

=

=

time) (3.66)

All these forces are balanced by a force F, corresponding to a tangential pressure gradient apj/au. By expressing the tan-gential equilibrium of forces

t t t t

F + F cor,J,u . + F 1 re ,n,j,u + F t · + F 1 t · cen r,J,u r e " J , u = 0 (3.67)

(46)

[

~]

=

p~

~

COS82· (2nW 2

·-a u 2j -J J J

(3.68)

R

C2 is positive when opposite to the direction of rotation. For the wake, we have similarly

If

P2w P2 .

J is known, we can deduce P2w

1 21TR 2 (1-E2)

[:~l.

-

1

=

P2· -J 2 z 2 J 1 21TR2(1- E2)

=

P2j + 2 z

[~l

[~l.

J w (3.69) and P2 pr ' P2 s h' P2 SUC 21TR2E2

[:

~l

(3.70 ) z w (3.71)

[

:~l

w (3.72) (3.73)

The problem with this method is the radius of curvature Rc2 , which is a functi·on of slip factor and blade geometry at the rotor outlet. As this is beyond the scope of this program, we introduce the value of R

C2 as an input data.

The jet flow is not subject to any noticeable diffu-sion. The increase of static pressure is almost completely due to the effect of centrifugal forces. This is also true for the

(47)

static temperature increase. Equation (3.40) can be written as

" "

=

Tsep + Tsep + (3.74)

In the wake, on the contrary, the static temperaure increase is considerable, because it is not only dependent on the effect of

U2_U2 '.<12 - W2

centri fuga 1 forces, 2 se p , but al so on the term . sep 'Ji.I

2c p 2c p

(cfr eq. 3.57). Sy making the approximation

equation 3.57 can be written as

(3.76)

It shows that there will always be a positive temperature dif-ference between jet and wake.

On the other hand, the static pressure in the wake will be lower than in the jet. Sy recombining eqs. 3.43, 3.60, 3.61, 3.69, 3.70, one obtains, for a sufficiently high radius of curvature RC2

.

st m e::

with n : the angular velocity (rad/s).

(3.77)

Using the parameter À, we can define the mean static values at

the impeller outlet (subscript 2mn)

(48)

P 2 .

J (3.79 )

(3.80)

Assuming an isentropic jet flow, we can use eqs. 3.76, 3.77, 3. 78, 3.80 to draw a T,S diagram of the impeller flow (Fig. 28).

From this figure we can see that the wake flow suffers an important entropy increase, which results in heavy losses for the mean flow.

3.5.5 lDflYê~Çê_Qf_~bê_Q~r~ID~~~r_~

Q~_i~e~11~r_E~rfQr~2~~~

From equation (3.76) it is evident that the impeller separation losses are strongly dependent on the parameter v, which determines the relative velocoty profile at the impeller outlet. However, v is also influencing the wake width S2 and the wake mass flow ratio À. In order to inv~stigate the influence of v

on impeller performances, we first look how S2 and À are

varying with v. From the continuity equations (3.43) and (3.60)

we can derive that

(3.81)

I-v

with

.

c

=

---~--- ~ m (3.82)

W2hom corresponds to a homogeneous impeller outlet velocity; C is a constant which is inversely proportional to the amount of separated flow :

o

<

C

<

1 C + 1

for separated flow for unseparated flow.

(49)

From a physical point of view, we know that the wake width E2 must be lower than 1, so that eq. 3.81 limits the choice for v

to be lower than the limiting value C : v ~ C

From eq. 3.43 we find an expression for À

v l-C

À~----I-v C

(3.83)

(3.84)

Equations (3.81) and (3.84) are represented in figure 29. We now derive expressions for the static to statie efficiency of the jet, the wake and the mean flow (Fig. 28). a) Jet flow:

(neglecting friction and clearance losses) b) Wake fl ow IS S,S T2 - Tsep = w nwake T2 -w Tsep

=

T

sep

[~::J

K-I

-r

- 1 s,s => nwake - A

B+(I-v

2 ) c) Mean flow IS S,s T -T nmean = 2mn sep T 2mn -T sep A,B = Tsep T 2mn -T sep i ndependent on v (3.85 ) K=.l K

r

p2mn] lPsep

-I

(50)

=> n

mean ~ ---BI

+À(1-\l2 )

A I, BI independent of \I

By introducing (3.84) into (3.86) we obtain s,s nnean ~ A" B"+v(1+v) A" ,B 11 independent of v (3.86) (3.87)

Figure 30 represents equations (3.85), (3.86), (3.87) for a particular case with C

=

.7. It is worth mentioning that these efficiencies are valid for the rotor only and do not include the mixing losses.

From figure 30 we see that when v is increasing the

wake flow efficiency is increasing. This is due to the fact that the temperature difference between jet and wake becomes smaller (cfr eq. 3.76). In spite of this, the mean flow efficiency n~!an is decreasing. The reason for this is that the mass flow through the wake (À

=

mw/m) is strongly increasing with v (cfr Fig. 29) which means that the wake flow becomes more important compared with the jet flow. We see that in eq. (3.86) À appears in a

posi-tive term of the denominator. This explains the shape of the

n~!an curve. The mean flow efficiency is thus decreasing because

the wake mass flow is increasing faster with v than the wake

efficiency. It is clear from figure 30 that the parameter v has

an important influence on the compressor charactersitics. The choice is judicious, but we suggest to start calculations with small values for v (f.i., \I = .2), according to the measurements

of Eckardt (Ref. 16).

When the impeller outlet width b is decreased for constant value of v, the wake width will become smaller and smaller until the outlet section is completely occupied bj the jet flow, and consequently there are no wake flow losses.

(51)

On the other hand, the throughflow section of the jet becomes more and more rectangular, and so the hydraulic diameter Dh

2 will decrease. We see from eq 3.50 that wfr will increase

considerably due to wall friction.

Equation (3.56) shows that also the clearance losses will decrease when the impeller width is increased.

Friction losses, separation losses and clearance losses are shown on figure 31 in a qualitative way. Figure 31 makes clear that there exists an optimum value for b2/R2 where the total losses

are minimum.

Remark : to take into account normal boundary layer blockage when the flow is unseparated, a min-mum wake width €2

min can be imposed. When €2 becomes less than €2

min' the model equation for the wake (3.58) cannot be sustained anymore and must be rep 1 aced by :

3.6 The impeller outlet tip

3.6.1 Ib~_~liQ_f~ç~Qr_g_fQr_~_j~~

~~Q_~~~~_çQ~fig~r~~iQ~

(3.88)

Due to the limited number of blades, the relative flow at rotor outlet will not ba tangent to the blade profile. This has no direct influence on efficiency, but on the rotor work output: ~H

=

U2V U2

-

U1Vu 1 (3.89) The rati 0 VU2 ~

=

00 Vu 2 (3.90) is ca 11 ed s 1 i p factor.

(52)

V

U2

=

real tangential velocity at rotor exit

VOO

=

tangential velocity at rotor exit for infinite blade number

U2

A broad review on the values of the slip factor ~ has been per-formed by Wiesner (Ref. 19).

For one dimensional calculations we propose the formula of Eck :

~

=

1 (3.91)

1 + ~ n COSB2bl

2 R2 +R2

z(l-

lh lt)

2R2 2

The formula of Buseman is better suited for a first guess, when the rotor outlet radius is not yet known :

(3.92 )

Z"7

To determine the slip factor of the jet ~j and of the wake ~w

separately, we consider the slip f~ctor ~ for a uniform flow as being the mass mean value of the jet wake flow:

(3.93)

The calculation of velocity triángles at the impeller outlet is based on the assumption th at the jet and wake flow have the same flow direction in the relative motion as stated in

eq. (3.39) :

Based on the velocity triangles (Fig. 32), the absolute veloci-ties in jet and wake are given by :

(53)

jw~.

2

V 2 .

=

+ U2 + 2U 2W2j sin(32j

J J (3.94)

.Jw~

2

V2 W

=

w + U2 + 2U2W2Wsin(32W (3.95)

The relation between the relative flow angle (3 and the blade angle

Sbl is deduced from figure 32, and is given as a function of the slip factor ~ by the following equations, for jet and wake respectively (1 -

-.!..)]

~ . J (3.96) (3.97)

Arelation between the slip factor ~j and ~w can be found in

function of the absolute flow angles, by combining (3.96), (3.97) and (3.39) (_1 _ 1) (3.98) ~w or lJw = tana2j ~ + (tana2w-tana2j) (3.99) j

The absolute flow angles of jet and wake are related to the relative flow angles by (Fig. 32)

U2+W 2Wsin(32

(54)

=

U2+W2jsinS2 W2jCOSS2

or af ter combination of (3.100) and (3.101)

Replacing U2 by 2nR 2RPM/60 in eq. (3.101), we obtain

2n RPM 60

(3.101)

(3.102)

(3.103)

All equations (3.93) - (3.102) can be used directlyor by itera-tion to determine the flow characteristics at the impeller out-let : ~, ~j' ~w' V2j ' V2W ' S2' a2j' a2w·

Equation (3.103) is used to evaluate the impeller radius R2 .

In order to calculate the total enthalpy rise, the Euler equation has to be applied to jet and wake

óHo

=

Cpl>To = (l->.)U2 " .Voo HU2 " VOO - l(1\(R)U 1 (R)Vu (R)dR

J U2j W U2w ~~ 1

lh

The integral rerm, however, drops out in case of an axial flow at the rotor inlet.

Af ter some transformations, this equation can be written as :

RIt K-1

J

,i, (

R ) UI (R) VI ( R) sinadR) dR (3.104)

.

m ao ao Rl h

(55)

which is the general expression of the impeller work equation. 3.7 Disk friction

At the back side of the rotor disc there is a statio-nary wall very close to it. The fluid between these two walls is rotating with the rotor disc at one slde, but stationary at the fixed wall side. This fluid rotation produces intensive whirl and energy dissipation. The extra torque due to this friction is given by :

LW

=

wall shear stress (3.105)

We define the disc friction coefficient as

(3.106)

The rate of dissipated energy is

(3.107)

The value of cm is dependent on the type of flow between the two walls. Four flow regimes can be discerned

I laminar with separated boundary layers Illaminar with interfering boundary layers 111 turbulent with separated boundary layers

IV turbulent with interfering boundary layers The extent of those regimes is varying with: - the axial gap s between rotor and wall

- the Reynolds number based on the disc radius and the circumferential velocity

(56)

four flow regimes.

The energy dissipation is going to heat the flow in the impeller, changing the outlet flow temperature and then affecting the rotor performances.

The flow temperature at the rotor discharge will be :

E (3.109)

The optimal value of S/R2 can be chosen from figure 33.

We see that S/R2 = .05 is a good value, because it results in a

5

(57)

CHAPTER 4 - THE MIXING PROCESS

4.1 Introduction

In section 3 we explained how the flow between the blades of a radial impeller gives rise to a jet wake configuration. At the discharge of the impeller, an intensive energy exchange takes place between the two subflows with different angular momentum (Fig. 32), resulting in a transfer of the impeller separation losses from the wake to the nearly isentropic jet. The mixing process we describe here applies only to separated flows in

rotating systems. The behaviour of stationary separated boundary layers, as generated in stationary cascades, is completely dif-ferent. It is also worth to notice that the denomination "mixing process" does not refer to a "mass exchange" between jet and wake, which is nearly negligible, but rather to the "energy ex-change" together with the uniformization of the flow.

4.2 Theoretical computation of the mixing zone of a jet-wake flow, taking into account the compressibility of the fluid

This theory is an extension of the theory of Dean and Senoo for incompressible fluids (Ref. 22) and of the study by Bex (Ref. 23).

a. Identical relative flow angle 8 for jet and wake;

b. The relative velocity distribution at the impeller outlet is rectangular as shown in figure 26;

c. The development of boundary layer blockage along the walls is neglected;

d. The blade blockage at the impeller discharge is not taken into consideration;

e. The statie quantities are identical for jet and wake.

Their initial value is equal to the mass mean value at the impeller outlet (Fig. 34). Consequently, the mixing process

Cytaty

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