nasatmx- · tst - tw u w - w u (2) : r w e where, tst is the local stagnation temperature, t r is...

32
•- NASA TECHNICAL ::: MEMORANDUM NASATMX-54843 ; (NAS&oTB-.-64843) A PHOCEDBRE YOE N7q-25804 k- C&LCULATION OF BOOND&R! LA¥.ER TRIP ,_ . _ROTU_ERANCES IN OVEREXPANDED _OCKET NOZZLES(NASAl 35 p HC $3.25 CSCL 20D Bnclas .: g3/12 q0157 J, g : £ _. A PROCEDURE FORCALCULATION OF _;; BOUNDARYLAYERTRIPPROTUBERANCESIN _'- OVEREXPANDED ROCKET NOZZLES __ By Robert H. Scl,mucker !_i- Astronautics Laboratory ;c g" April 2, 1973 NASA i George C.Marshall Space Flight Center Marshall SpaceFlight Center, Alabama MSFC - Form a190 {Rev ,fume 1971', https://ntrs.nasa.gov/search.jsp?R=19740017691 2020-04-01T06:01:15+00:00Z

Upload: others

Post on 24-Mar-2020

0 views

Category:

Documents


0 download

TRANSCRIPT

Page 1: NASATMX- · Tst - Tw u W - W u (2) : r w e where, Tst is the local stagnation temperature, T r is the stagnation tempera- ,! ture at the boundary layer edge, and r is the wall temperature

•- NASA TECHNICAL

::: MEMORANDUM

NASA TMX-54843

; (NAS&oTB-.-64843) A PHOCEDBRE YOE N7q-25804k- C&LCULATION OF BOOND&R! LA¥.ER TRIP,_ . _ROTU_ERANCES IN OVEREXPANDED _OCKET

NOZZLES (NASAl 35 p HC $3.25 CSCL 20D Bnclas.: g3/12 q0157

J,

g:

£

_. A PROCEDUREFORCALCULATIONOF_;; BOUNDARYLAYERTRIPPROTUBERANCESIN_'- OVEREXPANDEDROCKETNOZZLES

__ By Robert H. Scl,mucker

!_i- Astronautics Laboratory;c

g" April 2, 1973

NASA

i GeorgeC. Marshall Space Flight Center

Marshall SpaceFlight Center, Alabama

MSFC - Form a190 {Rev ,fume 1971',

1974017691

https://ntrs.nasa.gov/search.jsp?R=19740017691 2020-04-01T06:01:15+00:00Z

Page 2: NASATMX- · Tst - Tw u W - W u (2) : r w e where, Tst is the local stagnation temperature, T r is the stagnation tempera- ,! ture at the boundary layer edge, and r is the wall temperature

TECHNICAL REPORT $TANDARG TITLE PAGE

1. REPORT NO. JZ. GOVERNMENT ACCE'SSiOk NO. 3. RIECIP|ENT'S CATALOG NO.TM X- 64843..... ,,, . • , , ,

4. TITLE AI_O SUilTITLE S. REPORT DATE

A Procedure for Calculation of Boundary Layer Trip April 2, 1973Protuberances ia Overexpanded Rocket Nozzleb 6. p_mro_u,_; OR_A,,TAT'D,¢_E

7. AUT.O_ ..... e.P_RPORMI_OR_AmZAT,O;;REPORrRobert H. Schmucker*

9. PERFORMING ORGANITATION gAME ,_UiO'ADOfZE_S "" 10. WORK UN.T._,;O.

: George C. Marshall Flight CenterMarshall Space Flight Center, Alabama 35812 il. Cm_rRACTONGnat NO.

15. TYPE OF REPOR"¢' & PERIOD COVl_ED

_z. sP0,soRI,G _'zscv ,AM_ANDAOO_SS .... Technical Memorandum

National Aeronaut':cs and Space Administrationi"

Washington, D.C. 20.546 14. SPONSORING AGENCY CODE '"

,S. SUPPLEMENTARY N()TES

Prepared by Astronautics Laboratory, Science and Engineering

• National Research Council, National Academy of Sciences, Washington, D.C. 20546, . J .,,,

II. ABSTRACT

A procedure is described for sizing, scaling, positioning and performance loss calculationof a boundary layer trip protuberance. The theoretical results are compared with some

' experimental data.

t

I?. KET WORDS 1 18. DISTRIBUTION STATEMENT

' Flow separation Unclassified-unlimited

Bom_dary layer i

+_+ ;.i_Id rocket engines : _ //_C_'_ ++ _ "_i S _ forces ' " 7

19. SECtq_ITY CLASSIF. (et 1Iris iml_lt1 20, SECUiqlTY CLASSIF. (o/tMll Nit) Zl, NO. OF PAGES 22. PRICE

+ 1 Uncls ssffied Unclassified 32 NTIS' i 1111 . + II i I I i Jl. J Ill I II _ II i

+ MIIIt¢ • ]P'ommI lIDII (Itw n4mmll_n, 1II I ) ° Foe Ilk by NllliOltil 'rlClllltCld IstO4mlltton _tv4_e, SIM'lnllkld, Vhrlb_ :1_1'1_ I '+! .

," • t I

. .. .++ . . . ++

] 9740] 769]-002

Page 3: NASATMX- · Tst - Tw u W - W u (2) : r w e where, Tst is the local stagnation temperature, T r is the stagnation tempera- ,! ture at the boundary layer edge, and r is the wall temperature

ACKNOWLEDGMENTS

This research was performed under the NRC Resident Research Asso-

ciateship Program of the National Academy of Sciences at the AstronauticsLaboratory, Propulsion and Thermodynamics Division, NASA Marshall Space

Flight Center (MSF_), Huntsville, Alabama. The encouragement given byC. R. Bailey, Scientific Advisor, K. W. Gross, H. G. Paul, Division Chief,

and D. Pryor during the tenure is highly appreciated.-o

_r

¢.

1974017691-003

Page 4: NASATMX- · Tst - Tw u W - W u (2) : r w e where, Tst is the local stagnation temperature, T r is the stagnation tempera- ,! ture at the boundary layer edge, and r is the wall temperature

TABLEOFCONTENTS

Page

SUMMARY .......................................... 1

INTRODUCTION ...................................... 1

TRIP WIRE SIZING .................................... 2

Boundary Layer Model ............................. 3

Performance Loss ................................ 6

Wire Size and Flow Separation ........................ 9

SCALING OF TRIP PROTUBERANCE ........................ 14

TRIP PROTUBEI:L_NCE POSITION .......................... 16

CONC LUSION ........................................ 18

APPENDrX .......................................... 19

REFERENCES ........................................ 24

I.

iii

1974017691-004

Page 5: NASATMX- · Tst - Tw u W - W u (2) : r w e where, Tst is the local stagnation temperature, T r is the stagnation tempera- ,! ture at the boundary layer edge, and r is the wall temperature

LISTOFILLUSTRATIONS

Figure Title Page

1. Nozzle flow separation, with and without boundary

layer trips ................................ 3

2. Boundary layer model ......................... 4

3, Trip protuberance and boundary layer .............. 7

4. Experimental flow separation data and Crocco-Probstein

flow separation criterion ....................... 10

_o Control volume for trip size calculation ............. 11

6. Calculated and measured separation pressure ratio ..... _3

4

7. Geometry of a conical nozzle .................... 16

8. Position oI trip protuberance .................... 17

A1. Flow field and pressure distribution at boundarylayer trip ................................. 20

A2. Simplified pressure distribution at trip ............. 21

:" t

, iV :

1974017691-005

Page 6: NASATMX- · Tst - Tw u W - W u (2) : r w e where, Tst is the local stagnation temperature, T r is the stagnation tempera- ,! ture at the boundary layer edge, and r is the wall temperature

LISTOFSYMBOLS

Symbols Definition

c specific heat at constant pressureP

C constant

CD drag coefficient

CF thrust coefficient

d diameter

D1 drag per unit length

:. F thrust

i trip number

I momentum

M Mach number

p pressure

R gas constant

S stagnation pressure ratio

T temperature

'_ u velocity

x distant from throat

y coordinate normal to wall

_, _ 7 isentropic exponent

t, 8 boundary layer thickness°_

"_,'"4 i • -, I. I

1974017691-006

Page 7: NASATMX- · Tst - Tw u W - W u (2) : r w e where, Tst is the local stagnation temperature, T r is the stagnation tempera- ,! ture at the boundary layer edge, and r is the wall temperature

LISTOFSYMBOLS(Concluded)

Symbol Definition

AF thrustloss

_p pressure change

E expansionratio

v viscosity

p density

: 0 wall angle

Subscripts

a ambient

c combustionchamber

e boundary layer edge

i minimum pressure point (startpoint of the separationregion _ trip location)

n nozzle

ot without trip

r recovery

', st stagnation

:" t throat

tw trip

w wall

i wt with trip

vi

k

" '\_ _ ' ..... _, k

1974017691-007

Page 8: NASATMX- · Tst - Tw u W - W u (2) : r w e where, Tst is the local stagnation temperature, T r is the stagnation tempera- ,! ture at the boundary layer edge, and r is the wall temperature

TECHNICAL MEMORAN_DUM X-(;4843

A PROCEDUREFORCALCULATIONOFBOUNDARYLAYERTRIP PROTUBERANCESIN OVEREXPANDEDROCKETNOZZLES

SUMMARY

Side forces occur during rocket engine start and shutdown in ambientpressures greater than zero. These forces are caused by non-axisymmetricalflow separation. One method of avoiding this undesirable effect is by using :.a boundary layer trip to force a clean, axisymmetrical separation line.

Since boundary layer disturbaqces generate shock waves and reduce rnozzle performance, boundary layer tl!p sizing m,Jst represent a compromise _between performance reduction and trlpeffectlveness.. Procedures forcalculating trip• sizes, required positions, scaling effects and performancereduction plus a comparison between theory and available experimental data iare presented.

t

INTRODUCTION

During rocket engine start and shutdown In ambient pressures greaterthan zero, nonaxial thrust components act as side loads on rocket nozzlewalls. These unsteady, random[y oriented side forces are caused by un-symmetrical flow separgtion, and can impose a requirement for additionalstructural support thereby increasing the weight of the engine and mountings.

Since such weight increases are undesirable, several methods of reducing themagnitude of the side forces have been l_roposed. [ 1]

One method of reducing side loads Is to force clean, axisymmetric

separation lines. This can potentially be accomplished through the usboundary layer trips such as secondary Injection, wall angle dlscontinuL;,es.circumferential grooves, and circumferential trip protuberances. The useof a protuberance can be accomplished by installing a trip wire which has an

i; advantage that It can usually be [nmtalled aRe___.rthe development of an engineand nozzle without any change of the basic configuration.

i

f

.,

1974017691-008

Page 9: NASATMX- · Tst - Tw u W - W u (2) : r w e where, Tst is the local stagnation temperature, T r is the stagnation tempera- ,! ture at the boundary layer edge, and r is the wall temperature

Any protuberance of a nozzle wall generates drag losses and shock waveswhich reduce engine performance. Since the size of the protuberahce or trip

wire affects the flow separation behavior, performance reduction and flowseparation characteristics are related. A trip wire sizing and positioningprocedure is required, therefore, to provide the combination of preciseseparation and minimum performance reduction. ,.

This report describes one method for sizing, scaling, and positioningof trip protuberances. Some experimental results are presented, allowbg a

comparison between theory and experiment. The main purpose howe,.L-, isto outline the rationale of the proposed calculation method.

i

TRIPWIRESIZING

'I?

The objective in using trip wires is to achieve a forced separation of theflow. This separation should always occur at a higher walt pressure than

without a trip wire. One or more trip wires in a nozzle are used as shown :_in Figure 1. During transient start and shutdown, the chamber pressure islower than during main stage operation and the flow separates from the wall.At a given chamber pressure, the gases expand into the nozzle and flow overthe trip wires, 1 to I - 1. At trip wire l, the flow disturbance is sufficient

that the flow separates. Without a wire installed, the flow would have sep- :istated further downstream in the nozzle. When the chamber pressure isincreased, the gases finally overflow this trip wire. Then the next wire, l+l,

has been positioned such that at i+l forced separation is achieved. A further i:increase of the chamber pressure lets the flow jump to wire i+2 and at last timnozzle flows full.

Although this approach of having many or an almost "continuous" seriesof trip wires along the nozzle wall see_s to be promising, some of the disad-vantages accrued appear to favor the use of only one or a few trip wires. The

performance loss increases with the number of trip wires, and the change ofthe flow field over the trip is so severe that a certain distance between the

trip wires is required so that the disturbances can decay.

The flow separation process is a boundary layer effect. Therefore, ashort description of the boundary layer model, which is used for calculations,

is neceuary.

2

1974017691-009

Page 10: NASATMX- · Tst - Tw u W - W u (2) : r w e where, Tst is the local stagnation temperature, T r is the stagnation tempera- ,! ture at the boundary layer edge, and r is the wall temperature

') WI.II"HOUT TRIP

J U_NSYMMETRICAL ((NATURAL SEPARATION)

I I | J | I WITH TRIP

1121 | i i+11 i+2 ! SEPARATED JET

FORCED SEPARAT_

BOUNDARY LAYER TRIPS

Figure 1. Nozzle flow separation, with and without boundary layer trips.

BoundaryLayerModel •

The boundary layerwhich approachesthetripwire ispresentedinFigure 2, together with the associated nomenclature. Since performanceefficiencyrequiresa small tripsize,a tripheightofabout1/10 ofthe boundary '_layer thickness should not be greatly exceeded, Therefore the distribution of

flow properties at the boundary layer edge is of little interest.

The usualassumptionforthevelocityprofilewithintheboundary layer

isa 1/7power law, Denotingthevelocityas u, thevelocityattheboundary -_

layer edge as Ue, the boundary layer thickness as 5, and the coordinate normal

to the. wall as y, this distribution is e.xpressed by:

4:

3

Ii

1974017691-010

Page 11: NASATMX- · Tst - Tw u W - W u (2) : r w e where, Tst is the local stagnation temperature, T r is the stagnation tempera- ,! ture at the boundary layer edge, and r is the wall temperature

Y

ue Te' (e) BOUNDARY _... _.F...;-{

T_ _f- "w _ (w) NOZZLEWALL

i.g

Figure 2. Boundary layermodel. "--

(_;)'4 .- = - (1)Ue

The existence of a laminar sublayer will be neglected within the o__ccuracythis calculation.

The temperature distribution can be related to the velocity distribution ':.by the Crocco equation:

%

Tst - T uw

W - W u (2) :r w e

where, Tst is the local stagnation temperature, T is the stagnation tempera- ,!r

ture at the boundary layer edge, and r is the wall temperature. Since T is; W r

only slightly different from the combustion _.hamber temperature To, with the, energy equation

¢

4

1974017691-011

Page 12: NASATMX- · Tst - Tw u W - W u (2) : r w e where, Tst is the local stagnation temperature, T r is the stagnation tempera- ,! ture at the boundary layer edge, and r is the wall temperature

u2

T = Tst - _ ' (3)2cP

the local static temperature T can be obtained from:

T = u (T - Tw)+ T u2u c w - 2c (4/e p

Rearranging with the static temperature at the boundary layer edge

TC

T - , (b)e 1 + 7-1_ M 2

2 e

yields

1T u u _M 2

T = W + _ - _ 2 e (6)

In these equations, M desc_lbes the Mach number at the boundarye

layer edge and 7 the isentropic exponent of the gases, which are assumed to beideal.

Upstream of the trip outside of its influential range a constant static

. pressure across the boundary layer is assumed. With the gas equation thedensity p is expressed by

pp = _ , (7)RT

_ where p represents _he static pressure and R the gas constant.

¢

5

1974017691-012

Page 13: NASATMX- · Tst - Tw u W - W u (2) : r w e where, Tst is the local stagnation temperature, T r is the stagnation tempera- ,! ture at the boundary layer edge, and r is the wall temperature

PerformanceLoss

The estimation of the performance loss by the trip protuberancesrequires some assumptions. The tr_p wire is small c .-mpared with the bound-

art layer and therefore the shock, which is generated in front of the disturb-ance, becomes weaker towards the boundary layer edge and should disappear.Then the wall pressure further downstream of the trip de-liates only slightlyfrom the undisturbed wall pressure and the performance loss due to wall

Pressure reduction can be neglected. With this assumption, the performance iloss is generateff only by the drag _i the trip wire.

The drag is normally calculated by the dynamic pressure and a suitably

defined drag coefficient CD. Since the v(_locity and density upstream of the

trip varies normal to the wall, an integration is necessary. Then the drag per

length D 1 is (Fig. 3)

dtw

P_dy (8)D1 = f cD(y)_0

• In CD aU effects such as low pressure at the back side of the trip protuberance

are included. With the equations (6) and (_), the drag can be expressed by

D1 = / CD (9)

2R T c + .... 2 eu M_e 1+

In order to simplify Re calculations_ a constant, properly defined CD

is useful. An approximate value can be obtained from the various drag meas-urements of different body shapes. Rearranging with the boundary layer ed,;c

_ velocity of sound and equations (1) and ' ," resplts ha

; 8

1974017691-013

Page 14: NASATMX- · Tst - Tw u W - W u (2) : r w e where, Tst is the local stagnation temperature, T r is the stagnation tempera- ,! ture at the boundary layer edge, and r is the wall temperature

%'°= 7 14 -_-_ _e_f _±

D1 CD Me2 P_ -1 T (1 T-_w_ Me2-_'(_)"-, #-_""4 -o % %[-W _ M_ "e

(lo)

Th6¢exact integration of equation (10) requires the use of a decompe,,_ition topartial fractions. An approximate solution can be obtained by the fact thatabove a distance o[ O.O1 5, the integrand of (]0) increases rather linearly.

- NOZZLE AXiS

({11

Y

, ,./_//,//_

/

Figure 3. Trip protuberance arid boundary layer.

1974017691-014

Page 15: NASATMX- · Tst - Tw u W - W u (2) : r w e where, Tst is the local stagnation temperature, T r is the stagnation tempera- ,! ture at the boundary layer edge, and r is the wall temperature

Therefore, equation (10) can be written with little error

The racer k represents the rather linear increase of pu with y/5 in the regiondiscussed and has a value of O. 5.

For a quick estimation of the second term on the right side of equation ?

(11), some typical numbers for the different symbols are:

M =3 -.e

dtw/5 = 0.1 "-

T /T = 0.5W C

T = 1.25

and equation (11) yields

0.35 PTdtw

: D 1 = C D M 2 . (12) ;

e 1 + M e

The thrust loss is obtained by multiplyingthe drag per unit length with

the nozzle perimeter, using only the axivl component. With the nozzle diam-

eter dn and the wall angt O n, the thrust loss AFtw can be expressed by

L_

_Ftw = D l_d ncos_n " (13)

: LIi

! L:

[

1974017691-015

Page 16: NASATMX- · Tst - Tw u W - W u (2) : r w e where, Tst is the local stagnation temperature, T r is the stagnation tempera- ,! ture at the boundary layer edge, and r is the wall temperature

The previous listed typical values can be used for a simple, approximateequadorL of the thrust loss. Assumiag a dra..g coefficient of 0.8, which is sim-

ilar to those for spheres or cylinders, equations (12) and (13) result in

_Ftw = 0.5 M 2e p dtw .dn (14)

Equation (14) indicates that only very small trip sizes lead to negligible per-formance loss.

Wire SizeandFlewSeparation

A turbulent boundary layer in a rocket nozzle can only withstand acertain overexpanded condition. This condition is expressed by the separation

criterion, which describes the ratio of the minimum full flowing wall pressure

Pi to the ambient pressure Pa" The use of a trip _hanges this behavior, always

achieving separation at a higher wall pressure than would be achieved withouta trip.

Although the natural separation phenomenon in an overexpanded rocket

nozzle is far from being solved completely, cer+_in methods are available

which describe the experimentally observed res s reasonably well. I Thetheory, whici_ was derived by Crocco and Probste.n [2], achieves the bestagreement with test data. The numerical results of this theory and the avai-lable separation data of hot firing nozzles are plotted in Figure 4.

The calculation of the relation between trip protuberance size and

separation behavior can be done by a momentum approach. 2 The control

volume, which is used mr the analysis, agrees with that of Crocco-Probstein

1. Schmucker, R. H. : Status of Flow Separation Prediction in Liquid

Propellant Rocket Nozzles. NASA TM X (to be published), MarshallSpace Flight Center, Alabama 35812.

2. Another method for the determk_ation of size effect on separation behavior

: ispresentedintheAppendix. This approach isbased on the suggestionthatthe shock waves in the boundary layer change within a small region of thewallpressure, so thatseparationcan occur.

9

I

- , I _ J . r

1974017691-016

Page 17: NASATMX- · Tst - Tw u W - W u (2) : r w e where, Tst is the local stagnation temperature, T r is the stagnation tempera- ,! ture at the boundary layer edge, and r is the wall temperature

0._ mi II

0.4 _ ,

__ T ',1.41.3

1.2 _'

0.21 2 3 4 §

Mi (MACH NUMBER AT POINT OFMINIMUM WALL PRESSURE)

Figure 4. Experimental flow separation data and Crocco-Probstein flow sepa-

ration criterion (Data points represent averaged hot firing data).

[2], and is presented in Figure 5. The momentum balance between the point L,which Is upstream o5 the trip, and a point downstream of the trip (which is

described by the subscript a for convenience), yields:

I i _ Ia . D1 = 8i(Pa - Piwt ) , (15)

where I is the momentum and the subscript wt describes the condition "with

trip". Without a trip, equation (15) is written

I l - I = 81 Pa - Pl0ta

• 10 •

1974017691-017

Page 18: NASATMX- · Tst - Tw u W - W u (2) : r w e where, Tst is the local stagnation temperature, T r is the stagnation tempera- ,! ture at the boundary layer edge, and r is the wall temperature

EPARATION/ SHOCK

WAVE

EDGE - ; - _ CONTROL SURFACE '

,/////// ///////// /i SEPARATION a "

: Figure 5. Control volume for trip size calculation.

with subscript ot as "without trip". The latter condition corresponds to

normal separation in a nozzle. Combining equations (15) and (16) results in

Piwt Piot D1

Pa Pa 5iPa (17) "

The pressure in equation (11) Ior the protuberance drag is the un-

disturbed pressure upstream of the trip. Relating the wire drag in equation

(17) to this pressure results in

L

Pi_..___= i (is)Pio

":" Pa \"_'__1 D1 " i

I"

L

11 :"

• ! f

1974017691-018

Page 19: NASATMX- · Tst - Tw u W - W u (2) : r w e where, Tst is the local stagnation temperature, T r is the stagnation tempera- ,! ture at the boundary layer edge, and r is the wall temperature

The separationconditionswith a tripprotuberanceare calculatedby using _equation(18),theboundary layerdata,and theseparationdatawithouttrip.The lattercan be obtainedfrom Figure 4.

iEquation(18)indicatesa ratherlinearrelationbetween theseparation

pressure change Piwt-Plotand thewire size,normalizedwiththeboundary.

layerthickness.With increasedwallcooling,theeffectivenessofthetrip

increasessincethedensityofcombustiongases near to thewall isincreased.

The combinationofequation(18)and (t2),togetherwithnumericalvaluesallowsthederivationofa simple,approximate equationfor a roughestimationofthetripeffect

Plwi_ /. _I

i dtw 'Pa _a) - 0.16 Mi2

M. is the Mach number at the boundary layer edge at the trip location (at point1 _,

i).

The inversion of equation (18) allows the calculation of the trip size fora desired separation pressure change. Since the trip drag of equation (11) "'

depends on the 1/7 and 2/7 power of a trip size, only an iterative solution is

possible. A simple approximation is obtained by equation (19), using Aptw forthe pressure increase,

1 + PW

'5

Equation(20)shows a strongInfluenceofthe Mach number, indicatinga, decrease of the normalized wire size along the nozzle wall. But since the

boundary layerthicknessincreaseswith tl_elength,thePbsolutevalueofthetripsize increasesalso.

12

"t.

1974017691-019

Page 20: NASATMX- · Tst - Tw u W - W u (2) : r w e where, Tst is the local stagnation temperature, T r is the stagnation tempera- ,! ture at the boundary layer edge, and r is the wall temperature

In Figure 6, some experimental data together with thcoretieal cfilc_llation

are prescnted. The test data are obtained from a 4k H2/LOX engine at NASA's

Marshall Spacc Flight Center. They represent thc minimum wall pressure

Pi during the test. Since this nozzle was uncooled and therefore changed itswt :

temperature during the tests, the calculations were performed for two wall

temperature ratios.

Tw_= 0,145 0.30T c _

0.5 ,- .

NO SepARATION

0.4

t .

=:-0.3 L ,_

,... :NO TRIPS

" SEPARATION-,

0.2 0 0,01 0.10 0.15 0.20

dtw/51 :.

Figure 6. Calculated and measured separation pressure ratio (lV[1=3.6 ,7=1. 26)

(Test data obtained with NASA-MSFC 4-k Hz/O 2 engine}. ,:

The agreement between theory and experiment is rather good. The

theoretical calculated values represent an upper limit, which is not exceeded

by the test data. The measured separation pressures are normally lower than

the theoretical limit, since the trip location does not agree with the upper trip

position, (See later discussion of Trip Protuberance Position.) The testdata ,_

,

13

]9740]769]-020

Page 21: NASATMX- · Tst - Tw u W - W u (2) : r w e where, Tst is the local stagnation temperature, T r is the stagnation tempera- ,! ture at the boundary layer edge, and r is the wall temperature

|nm_,,_-_,e'_,v,_,.,:_,l_,,. ..... _.,., ,,.,.,,., .,, ,_..,: ,,-' _ . -:,,,.."...,.,mm_,,.'..,,,....... ,,.:,.,_,. .... ,' ., .;,..-.... ---,.,_,,,._,,,'..,,,_..;-,_ ,,. ' _-,.-,,....

/"

with the smaller trip size agree with the theoretical line. This indicates that

the test results should be very sensitive to boundary layer changes. Duringthese tests the separation point jumped from one trip to the next, and was

probably caused by the wall temperature increase.

SCALINGOFTRIP PROTUBERANCE

The performance loss and effectiveness depends on the drag of the tripprotuberance. The exact numbers and relations of drag coefficient, velocity,and temperature distribution are not known. The measarement of separation

behavior avoids tfiis _!ifficulty, since integral quantities in equations (14) and

(20) are obtained. _!

For a measured separation pressure ratio and a fixed Mach number andtrip shape, equation (20) can be simplified and the trip size is _

dtw = C1 6.1 " (21) f

The trip protuberance height is a certain fraction of the boundarylayer thickness. If the boundary layer thickness is known, the required size

is obtained from equation (21) using test results for C I.

If no boundary layer data are available, a rough estimation is possibleusing the boundary layer thickness of a flat plate. For convenience a conical

nozzle is assumed (Fig. 7). Then, with the len_h x which _tarts at the throat,the boundary layer thickness can be written [3]

¢

0.2

5. = 0.37 /--v_ x 0"8 ; (22) :

where u t is the velocity at the boundary layer edge, 6. is the boundary layer1

thickness at the trip location i, and v is the viscosity. The length x can be

' approximated by

(

14

• t-.................. i

1974017691-021

Page 22: NASATMX- · Tst - Tw u W - W u (2) : r w e where, Tst is the local stagnation temperature, T r is the stagnation tempera- ,! ture at the boundary layer edge, and r is the wall temperature

/ !'

mm

d

n (23)x = 2sinen

Introducing the thrust equation

7[

F -- Pc dt2_ CF ' (24) i

where dt describes the throat diameter and C F the thrust coefficient, thus

yielding:

= (F_ °'5 E°'s (25)

x \_-c/ CF°'Ssin O _0.sn

Combining (22)and (25)resultsin

°''dtw = \Pc/ C2 ' (26)

where allconstantsare comprised inC2. The tripwire sizeincreaseswiththe 0.4th power of thrust and decreases in the same way with chamber

. pressure.

The previous described scaling procedure is ,.nly valid for scaling to aL

: different engine with the same boundary layer conditions. A scaling to otherconditions,such as expansionratioe, Mach number, etc.,requiresa changeoftheconstantC 2. These effectscan be estimatedby theproportionality

t

: _0. 1+ M

' C2 (_ " ' 27)4

: _ CF°" ui°'2M_

i

. 15 '_/

b

% .... '_ .... . =, ,. ,_, ||1

, o . ....

1974017691-022

Page 23: NASATMX- · Tst - Tw u W - W u (2) : r w e where, Tst is the local stagnation temperature, T r is the stagnation tempera- ,! ture at the boundary layer edge, and r is the wall temperature

!• "]_ -----1- - -- NOZZLE AXISdt

/ /

.- X _

TRIP LOCATION (i)

Figure 7. Geometry Of a cotiical nozzle.

but the accuracy of such an approach is very questionable. Equation (27)

should therefore only be used for the estimation of trends.

: TRIPPROTUBERANCEPOSITION

\

The calculation of the trip protuberance size requires, besides thewall temperature and the Mach number, the desired wall pressure at which the

flow separates. It is obvious that this condition can only be fulfilled at a cer-: tain chamber p_'essure. During transient conditions, the chamber pressure

changes and the trip device is only effective during a certain chamber pressurerange. Therefore, the trips have to be positioned such that natural separationcannot occur anywhere.

For calculation of the possible location range for the trip protuberance,: Figure 8 can be used. At a certain chamber pressure, an undisturbed wall

pressure profile is obtained like that of Figure 8. According to the wall pres-

; sure distribution, a Mach number can be calculated at every station and, with= the data of Figure 4, the natural separation pressure can be plotted. The inter-

, section of the wall pressure profile and the separation pressure profile de-scribes the natural separation point. Since a deviation from these ideal values

"i always occurs, a small scatter must be introduced to get reliable numbers.Assuming a certaintripsizeallows,togetherwith thelocalboundary layer

, thicknessand walltemperature,thecalculationofthetripdrag. With the

separationpressure and equation(18),thisleadstothe separationpressure

L

: I

16

i

"19740"1769"1-023

Page 24: NASATMX- · Tst - Tw u W - W u (2) : r w e where, Tst is the local stagnation temperature, T r is the stagnation tempera- ,! ture at the boundary layer edge, and r is the wall temperature

with trip. The intersection of this distribution with the undisturbed wall

pressure results in the upper limit for the trip position. Placing the trip up-stream of this point would result in a reattachment of the flow after the trip.The use of a trip protuberance downstream of the lower limit does not effectthe natural flow separation at all. Therefore, a trip wire of a fixed sizeshould only be placed in this described range.

i ||11ml,i

1° ° I

i • _ SEPARATIONI" I__._ _ / PREUURE WITH I

I NATURALSEPARATION

wRESSURE

SCATTER

UPPER LIMIT LOWER LIMIT OF TRIPOF TRIPLOCATION _ _ LOCATION (dtw - CONST) ,

: _w" CONST)

!: ' RANGE OF TRIPi POSITION

AXIAL DI|TANCE PROM THROAT

)

, ) Figure 8. Position of trip protuberance (dtw = eonst).

"- } 17

1974017691-024

Page 25: NASATMX- · Tst - Tw u W - W u (2) : r w e where, Tst is the local stagnation temperature, T r is the stagnation tempera- ,! ture at the boundary layer edge, and r is the wall temperature

A changing chamber pressure varies only the undisturbed wall press,_reprofile. If the trip is positioned in the previous mentioned region of thenozzle, an increasing chamber pressure moves the condition to the upper

limit. Finally" the chamber pressure is high enough that the gases overflow" the trip. In this case, at the lower limit of the trip location, a new trip de-: vice has to be located so that natural separation can be avoided. This holds :

/

true for every trip protuberance. The nozzle exit can also be considered as atrip.

The separation pressure increase with trip depends on the trip size.Smaller trips are less effective and require a larger number of devices.

Bigger trip_ allow larger spacing and are not so sensitive to boundary layerchanges. This favors the suggestion that for flow separation with trips, onlya few or even one trip wire should be used. _

\

:' CONCLUSION ,

Boundary layer trip protuberances _re a promising approach for side _ "load reduction in overexpanded rocket nozzles by forcing a clean, axisym- '

metrical separation line. Effectiveness can easily be _erified by installing acircumferential trip wire.

A sizing, scaling, and positioning procedure for the trip protuberances ,:is described, and is based on the momentum equation. This derivationindicates that performance loss and trip effectiveness are related. The

performance loss is very sensitive to trip size, but only very small trips are

necessary for the significant change of the separation•behavior. Some ex- i: perimental data are pre_ented, which show good agreement with the theoretical

: results, This suggests that the theory presented describes the real phenomena

• rather well. i

The scaling of trips requires some information about the boundary _-layer. A simplified scaling procedure relates thrust, chamber pressure, and -:

trip size for a fixed boundary layer condition. Positioning and spacing of trips

'_ is based on the natural separation behavior and the change caused by the ti'ips. _;' i Larger spacing, which is desired for less boundary layer disturbance, can be

,. achieved by a few bigger trips. The last trip has to be in such a position that

! _ the nozzle exit is being considered as a final trip. ;_i

,) ' ,

i '": 18

\ , '_ i ,

1974017691-025

Page 26: NASATMX- · Tst - Tw u W - W u (2) : r w e where, Tst is the local stagnation temperature, T r is the stagnation tempera- ,! ture at the boundary layer edge, and r is the wall temperature

h

PENDIX

CALC!3i OFTHETRIP SIZE BYWALt. ' •;,IRECHANGEDUETOSHOCKS

I

The t l_,w fie_ : _ :'¢_ur,d the trip protuberance and the wall pressuredistribution is pres_':_ted inFigure A1. Upstream of the wire the flow is

compressed and sc:_::_cates from the wall. A curve shock emerges in thisregion, decreasing in strength with Increasing distance from the wall. Theseparated stream line reattaches at a certain point from the protuberance. In

the separated region the wall pressure increases. Downstream of the first re-attachment point the flow expands and the wall pressure drops. The trip size

is so small that the area ratio of the nozzle can be considered as unchanged.Due to the shock wave the local stagnation pressure in the boundary layer _,

drops. At a certain point from the trip protuberance, the flow separates again "and the wall pressure drops. If the chamber pressure is high enough, the ,.gases flow over this protuberance and reattach downstream of the trip. There- :fore, a reattachment shock is generated, which leads to a further stagnationpressure loss. Since the disturbance of the flow field occurs only in a small

region near to the wall, the mixing process damps the differences of thestagnation pressures and the deviation from the theoretical wail pressure ,.

profile decays very fast. The final pressure distribution should be slightly _.below the disturbed pressure profile, but the deviations are almost too smallto be measured. (Wall pressure measurements in a small nozzle with rectan.-

gular trip wires do not show any deviation from the wall pressure without

trips.) If the chamber pressure is low enough, the expansion downstream ofthe trip prevents a reattachment and a forced separation is achieved,

Downstream of each reattachment point the static wall pressure is _"

lower than upstream of the wire since shock waves decrease the local stag-nation pressure. This favors the suggestion that w_th a fixed trip configuration,a certain chamber pressure range exists which will always lead to forcedseparation. The lower limit of this range corresponds to separation at the

• edge of the trip. _ The higher limit corresponds to the condition just before re-attachment after the trip.

3. The' flow always sep_zrates at the trip or upstream of the trip if thechamber pressure is lower than this lower limit. Therefore this chamber "

- pressure must be considered as a theoretical lower limit.

19

] 9740] 769]-026

Page 27: NASATMX- · Tst - Tw u W - W u (2) : r w e where, Tst is the local stagnation temperature, T r is the stagnation tempera- ,! ture at the boundary layer edge, and r is the wall temperature

¢ •

, %

COREFLOW

W

:= UNDISTURBEDWALL-J PRESSUREPROFILE

-J EXPANSION.i

< _ / _'_ MIXING OFBOUNDARY LAYER '-

AXIAL DISTANCE

FigureA I. Flowfieldandpressuredistribution_atboundarylayertrip.

: For calculationo[thetripsizebythewallpressurechangeduetotheshockssome assumptionshavetobe made. InFigureA2, thesimplifiedflowfieldispresented.The detailsolpressuredistributionneartothetripdevice

:. can be neglected, The presence o! a trip protuberance decreases the static ,

wallpressureatorshortlydownstreamofthetrip.The pressuredropAPtw

: is_heresuRofa stagnationpressuredecreaseo[thatstreamline,whichisthesame distance from the wall as the upper effective limit of the trip. The

t,

_ 20

; /}

Page 28: NASATMX- · Tst - Tw u W - W u (2) : r w e where, Tst is the local stagnation temperature, T r is the stagnation tempera- ,! ture at the boundary layer edge, and r is the wall temperature

-!

prcszure change i3 described by a normal shock. This can be considered as

a mean between the previous mentioned upper and lower limit of the separationcondition.

i

I

_........._ UNDISTURBED :PRESSUREPROFILE

L _Ptw

I

/

AXIAL DISTANCE

Figure A2, Simplified pressure distribution at trip.

, Denoting Stw aF the stagnation pressure ratio of the trip edge stream

i line across the shock waves, the expression for the wall pressure is

T

21

/t

1974017691-028

Page 29: NASATMX- · Tst - Tw u W - W u (2) : r w e where, Tst is the local stagnation temperature, T r is the stagnation tempera- ,! ture at the boundary layer edge, and r is the wall temperature

Pa \ Pal

The stagnation pressure ratio is obtained by the usual shock relations !4],

T

..... 1 T (A2)

In the interesting Maeh _umber range this expression can be simplified by a -linear relation,

i

stw = 1.45..M.o.36 (A3)1

The Mach number is calculated by equation (1), (6), and (7) :

U

Ue

M = M

,, 1+_" Me' +_e'e - TJ - _e" , +_-_-M_

)

.: , _4)

and the pressure ratio with trip results in,

i

!

22 -

1974017691-029

Page 30: NASATMX- · Tst - Tw u W - W u (2) : r w e where, Tst is the local stagnation temperature, T r is the stagnation tempera- ,! ture at the boundary layer edge, and r is the wall temperature

(AS)

M. represents the boundary layer edge Math number at the trip position.l

A comparison of the results ot equation (AS) with the test data ofFigure 6 indicates that the assumption of a normal shock leads to discrepancieswith the measuremerLts. Although equation (A5) predicts rather small tripqize.q and the correct trend of the wall temperature effect, the deviation fromthe reai phenomenon Is excesswe. Therefore trip w_e sizing based on shock

• _,eneration is not an acceptable approach.

, ?

%

4

i

_ 23

,k" -_, % -o ", _, ._. t,_lm,.im,m :"

1974017691-030

Page 31: NASATMX- · Tst - Tw u W - W u (2) : r w e where, Tst is the local stagnation temperature, T r is the stagnation tempera- ,! ture at the boundary layer edge, and r is the wall temperature

REFERENCES

I. Schmucker, R. H. : Side Loads in Liquid Rocket Engines. Paper pre- ." sented at the first annual Research and Technology Review, NASA:

MSFC, 1973.

2. Crocco, L. ; and Probstein, R. F. : The Peak Pressure Rise Across

an Oblique Shock Emerging From a Turbulent Boundary I,ayer Over aPlane Surface. Princeton Universits, Report 254, March, 1954.

3. Eckert, E. G. R. ; and Drake, R. : Mass and Heat Transfer. MacGrawHill, New York, 1959.

4. Shapiro, A. : The Dynamics and Thermodynamics of Compressible

Fluid Flow. The Ronald Press Company, New York, 1954. /

F

/

• -f

i

_ °

• 24 '"

t

1974017691-031

Page 32: NASATMX- · Tst - Tw u W - W u (2) : r w e where, Tst is the local stagnation temperature, T r is the stagnation tempera- ,! ture at the boundary layer edge, and r is the wall temperature

APPROVAL

. A PROCEDUREFORCALCULATIONOFBOUNDARYLAYI=RTRIP PROTUBERANCESIN OVEREXPANDEDROCKETNOZZLES

By Robert .q. Sch_nucker

• The information in this report has been reviewed for security classifi-

; cation. Review of any information concerning Department of Defense or

Atomic Energy Commission programs has been uade by the MSFC Security

Classification Officer. This report, in its entirety, has been determined to beunclassified.

This document has also been reviewed and approved for technical

accuracy.

A. A. McCool

Acting Director, Astronautics Laboratory

C. C. WOOD

'Acting Chief, Propulsion and' Thermodynamics Division

qj_. L_X_DOChief, Liquid Proputs£onand Pc_cer Branch

_= Chief, Propuls ion" _ Thermosciences Sect ion

t

• !

1_ U.S. GOVERNMENT PRINTING OFFICE 1974 - 748 298 / 170 REGION NO. 4 ,-u

\

1974017691-032