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THr AEnoNAUTTcAL ]ounxnr

Apru12001

ABSTRACT

A m e t h o d i s p r o p o s e d by which a direct numerical simulation of the c o m p r e s s i b l e N a v i e r - S t o k e s equations may be embeddecl within a more general aeronautical cFD code. The methocl rray be applied to a n y c o d e w h i c h s o l v c s the Euler eqLrations or the Favre-averagecl N a v i e r - S t o k e s e q u a t i c l n s . A f b r m a l d e c o m p o s i t i o n of the flowfielil is L r s e d t o d e r i v e m o d i f i e d equations tor use with direct numerical sim-L r l a t i o n s o l v e r s . S o m e p r e l i m i n a r y applications fbr model flows with t r a n s i t i o n a l s e p a r a t i o n bubbles are given.

1 . 0 IN T R O D U C T I O N

Applied careful ly. aeronauticul cornpr-rtational f-luicl dynamics (cFD)

codes can deliver usefirl predictions of flow aroun<J aircrafi. The

r.nethods generally work well when the f-low is fLrlly tLrrbulent ancl

rcmains attached to the surface. The standard rnethods work much

less well when transition to turbulcnce must be taken into accollnr or

when the turbulenr flow is subjected to rapicl changes in the imposed

strain field. The rnodels are particularly challengecl in regions where

I'low scperration or reattachment takes place. By contrasl direct

nr_r-merical simLrlations (DNS). whereby the governing equations are

solved in full, are too expensive fbr complete calcujations of flows

with aeronar-rtical application, but can deliver accurate solutions of

simpler problems withoLrt modelling errors. The range of problems

that can be tackled by DNS is increasing as the po*.r of computers

increases and DNS and the relatecr approach o1'large-edcly

simula-tion (LES) are bein-e applied to more ancr more complex -eeomerries

and f-low fieldstr-r). The ob,jective of the current research is to link

the two apprcaches by providing a framework whereby an

aeronauti-cal cFD code can provide the context fbr a iletailed DNS. which in

turn can automatically f'eedback improved physical modellin-r of

Iocal phenomena to improve the quality of the overall prediction.

As a model problern we consider thc case of a separation bLrbble.

irritially laminar. but undergoing transition to turbulence ancl

reattaching as a turbulent boundary layer. In high lift confi-surations

sLrch bubbles rnay form on the slat and a failure of the flow to

reattach ultirnately causes stall of the configuration. prediction of the

conect flow with conventional cFD is irnpossible as typically a

tran-sition point must be flxed close to the location where separation

takes place, in order to get a convergecl resr-rlt. However this fix

r93

Embedded

direct numerical

simulation

for

aeronautical

CFD

N . D . S a n d h a m , M . A l a m a n d S. Morin S c h o o l o f E n g i n e e r i n g S c i e n c e s U niversity of Southampton S o u t h a m p t o n , U K

precludes calculation of the maximum lifi coefficient. a quantity

fbr-which accurate predictions at'e essential i1'clesign is to be optirnised.

Several direct simulations of complete separation bubbles hlve

been carried out recently. These simulations include the larninar

sep-aration, transition process. turbulent reattachment. and relaxation o1,

the turbulent boundary layer downstrearn of reattachment. Spalart

and Streletstat specified a fiee stream normal velocity profile and

simr-rlated a bubble with a length of approxirnately 300 tirnes the

momentum thickness at separation. Alam and Sandhllnr5r 11secl o

sirnilar Inethod fbr prescribing the fl'ee stream velocity distribLrtion

but focLrsed on shorter br-rbbles with lengths of the order of 40 times

the momentum thickness at separation. The bubble phenomena

reproduced in these simulations closely match earlier experintental

work. Besides providin_u data firr understanding flow instability

mechanisms (Alam and Sandham). comparisons with aergnaLrticiil

codes (Spalart and Strelets) and turbLrlence rnodelling (Hatlzic alti

Hanjalictot, Howard et ultl)) the simr-rlations also demonstratc the

f-ea-sibility of simr-rlating flow phenomena at realistic Reynolds numbers

on modern computers. It is therefbre f-easible computationally to

consider a direct simulation of a slat separation bubble (which may

only occupy lc/c of chord) and a simultaneous CFD simulation of the

rest of the f'low. The problern which we attempt to adclress in the

present work concerns the details involved in coirplin-u the twcr

approaches. In Section 2.0 we present the governing equation ancl their

Favre-averaged counterparts. such as mery be usecl in cFD cocles. In

Section 3.0 we introduce a f-low decomposition techniqtre using thc

Euler equations and the Favre-averaged equatior-rs as examples. This

technique is then applied in Section 5.0, usin-e clirect simulation

numerical methods given in Section 4.0. Finally in Section 6.0 we

present results fiom a calculation using a Favre-averagecl base f1ow.

All the equations and exanrple are presentecl fbr compressible 1low.

2.0 GOVERNING

EQUATIONS

2.1 Instantaneous

equations

The governing equations fbr mass, momentllnt and energy conserva_

tion ntay be written in Cartesian tensor notation as:

February 2000, accepted l8 Januarv 2001.

(2)

194

THE AenoNAUTrcAL lounNar- A p r u 1 2 0 0 1

( l o t

t l l r

( l2 )

( r 3 )

( 1 4 )

l p t ( p r r , ) n 6t i.r,

r 1 ( p r r , ) ,

? ( P u 1 t , )

_ C p

;

-8t d.t, 6,t,

t ) = ( y - l ) p e

with y the ratio of specfic i s N e w t o n i a r n a n d f o l l o w s

( l )

Arii

d t ,

heats. Aclditionally we asslrme that,n. tj,1Li

Fourier's law for heat conduction:

d r , 2 A D , ' *

)

- r - - - - | ) i i

I

0 r , 3 0 r ^ " )

( 2 )

_ | C u ,

T , , : L l l

r l . l l

\ c'{i

a n d w e h a v e a s s u m e d th a t

I E , c [ ( 6 , + p ) t r , ] ? q , , ? ( ' c , , t t , )

T

-Ar Ar d-r, 6-r,

where Er = p @ + t/zLt1t), e bein-e the irlternill energy. The fluid is

assumed to fbllorv the perf'ect gas law with constant snecific heats

( 3 )

. . . ( b )

where pt is the viscosity, -uiven by apower law tirnctictn of

tempera-ture, ancl r is the thermal condr-rctivity. The Euler eqr-rations arise

when the terms involving viscclsity and thermal condr"rctivity are

dropped fiom the right hand sides of Equations (2) and (3).

2.2 F avre-averaged equations

In Navier-Stokes calculations with a turbulence rnoclel a flow

decomposition into an average and a f-luctuuting conrptlnent is used.

For the compressible equations considered here. a convenient tbrrn

which preserves the original structure of the ecluations is thc Favre

method of mass-wei-qhted variables defined according to

u = i , + t t ' , ' p = p + p '

T - - 7

+ 7 "

t : - f - + F - ' " r " I

p = p + p '

w h e r e i , = p u , / p a n d w e c a n a l s o w r i t e E , = p E w i t h E = E + E " .

lt shoLrld be noted that fbr anv function l:

F o r l o w M a c h n u m b e r f l o w s t h e F a v r e d e c o m p o s i t i o n r e d u c e s to t h e L r s u a l R e y n o l d s - a v e r a g e c l f o r m o f t h e e q u a t i o n s .

T h e F a v r e - a v e r a s e d m a s s c o n s e r v a t i o n e u u r " r t i o n i s

I

T h e m o m e n t L l l n e q u a t i o n s a r e :

T I r c l e r r n s , i . pu,, ,'t.p,qr1, ,,td pi,- .,,,, hc rnodelletl

by vr. ui. \,-r (e u,le.r,). \,r tiA/i.r, ) and v r (ieli.r,;

respectively (see Vy'i lcoxtst).

3.0 A DECOMPOSITION

APPROACH

The basic idea of the present contribLrtion is to perfirrm a direct

numericitl simulation fclr phenonrena such as transition and

turbu-lence r-rsing as base flows solutions nhich mar arise fiom standard

aeronautical CFD calculations of cornpressiblc flow. A conceptr-rally

sirnple way of arran-uin-e this is to consider tlie total flow to be a

superposition of a known base flow and an unknou n tinte-dependent

perturbation fiomthis to be deterntined bv direct nunterical

simula-tion. In the fbllowing subsections we derir e the relevant eqLrations

for a base flow which satisfies either the ELrler equations or the

Favre-averaged eclr-rations firr turbulent flori. Sintilal br-rt sirnpler

ecluations can be derived fbr incompressible f-lou.

3.1 Euler base flow decomposition

As a first example of the techniqr-re we consider a clecorlpositit'rn

into an Er-rler component p,'.tii', Ei: which is iisslrrned to have been

computed from a separate Euler solver, and a der iation li'ont this

which we label pt,.t/1. Ef). Insertin-e this clecornprosition into the

-rov-ernin-9 equations and subtracting the ELrlcr solution of the equations

l e a d s t o t h e fo l l o w i n g e c l u a t i o n s . F o r c o n t i n u i t y u c h a r e :

T h e e n e r g y e q u a t i o n b e c o m e s

- F - ^ . , 7

i E , , i l ( E , + F ) n l * a E

-?t

e,r,

cl:.r

a ( , - , , | , , , , , \ ( ^ ( p t " t t " ) * ; _

[ 4 , , , , , * u i p u i u -

) P u , u I t - ' l

^

- - , r \ / . l ( . \

T h e m o m e n t u r n e q u a t i o n b e c o m e s :

i ) .

t (

_ - r - L P r r i | | r cI cxi

t E r D l T l '

. t ' , , o . t t t t i t ' l ) " ' t i i ( ' r ( D t l ' , - D ' / i , ) ' = i F

-| '

,^,,, t-:r, ,tt, i:v,

i l t r l t

r

-i.r

(-5 )

/ ^ \

l ? u c l t , 2 ? . u ^ I

T - r r l ' - !

r , , - l r | | v I

" I l r i . v , I i . r , " )

\ / r ^ /

( ' l 4 i = - l ( ^

cti

I li,'

( 7 )

( u )

t = o l

7 = o l

a p l ( p D l ) n

(3)

SaNnsav ET AL

and the energy equation is:

A r D A

? * .

[ 1 6 r ' + p o 1 u ,

ot oxi

6 r l , t '

, 0 1 r l u , )

r

-Ar,

tr,

where

+ ( E f + p E ) u l 1 =

Evngnoen DIRECT NUMERICAL sIMULATIoN FoR AERoNAUTTcAI cFD

195

,

( e,,,o attl 2 cri - )

T u = f . l l 1 + . - ^ ^ : 0 , , 1

\ c.r, c_ri J a.rr )

p o = ( p r ' - p o r u ) ( y - l )

. . r i \

, r [ r t t , t t , t t o t , ? " . I

, u = ; l n ' - p o ( e u

* T ' , - r t r t t i l i + , , i , , !

l l

3.2 Favre base flow decomposition

A similar procedure leads to equations fbr the f'low-fielcl p,t.,,,,'. Elt

computed as a perturbation fiom a Favre-averaged base flow pi',r|. E.f. . For the continuity equation we have:

4 . 0 N U M E R I C A L

M E T H O D

F O R D N S

The new formulations of the governing equations for mass,

momen-tum and energy given in Section 3.0 are solved numerically using

techniques that are suitable fbr efficient calculation of f'lows with a

wide range of length and time scales. Time discretisation is achieved

with an explicit low-storage third-order Runge-Kutta scheme. The

time step is fixed to be well within the stability limit to ensure

tem-poral stability. Spatial discretisation is by means of compact

pacld-type high order schemes with ave-point stencil on the right hand side

and a three point stencil on the lefi hand side. These rnethocls require

only a tridiagonal matrix solver. They achieve sixth order accuracy in the inner part of the domain, reducing to third order at boundaries

and have good wave resolution properties (Leleror;.

Non-ref'lecting characteristic boundary conditions are useiJ at the

in f-low and outf-low boundaries. The methods used at the outf'low

were originally proposed by Thompson (19137) and invorve

criagonal-ising the Euler equations and zeroing out the rows containing

char-acteristic velocities that are pointing inwards into the computational

domain. At the in flow boundary we use a modification to this

approach fiom Sandhu and Sandham(tot whereby the basic inflow is

fixed but with the outgoing characteristic added by integrating it

along with the rest of the Navier-Stokes equations. This provides a

rnethod of fixing an inflow condition while allowing souncl waves to

pass smoothly through the inflow boundary. For Navier-Stokes

cal-culations a boundary-layer profile is needed at the infrow. This is

found fiom a similarity solution of the compressibre raminar

bound-ary-layer equations.

No slip conditions are used fbr the lower boundary to simulate a

smooth surf'ace. A mixed set of boundary conditions are used at the

upper boundary to maintain the flow fleld. A non-reflecting

charac-teristic boundary condition is used for density and a zero vorticity

boundary condition is implemented by settin-q

; l ) ^ I )

c't I - c\J"

o.y' d,r

and we set

u D = 0

. (24)

r ? 5 r

It should be noted that the boundary conditions specil'ied here need

not be the same as those used fbr the base flow calculation which is

one of the strengths of the decomposition method. In the examples in

this paper we use Dirichlet conditions fbr the base f-row and mixed Neumann-Dirichlet conditions fbr the full simulation. Alternative ways of specitying the upper boundary are currently under review to

fully utilise the flexibility off-ered by the decomposition approach.

For all the simulations presented in the fbllowing two sections the

computational box lengths are l0b* in the wall-normal direction and

120b" in the streamwise direction where 6" represents the

displace-ment thickness of the incoming boundary layer. The grid is stretched

in the wall-normal direction to cluster more points in the boundary layer. The number of grid points used were 140 in the wail-normal

direction and 100 in the streamwise direction. For viscous

calcula-tions the Reynolds number was fixed to be -500. the prandtl number

to 0.72, and viscosity varied i1s 1,1 - f t)67.

5 . 0 E U L E R - D N S

S I M U L A T I O N

O F A

SEPARATION

BUBBLE

The first step in producing a simulation is to compute an Euler

solu-tion. In the anticipated applications this would conre from a standard

aeronautical Euler solver. Here we consider simpler rnodel problerns

to demonstrate the techniqr-res. An external velocity profile which

can be used to produce a separation bubble is

. ( t 6 )

. . . ( 1 8 )

. (20)

a ,r)

c'P c' , rr

- - + . ( p r r i + p ' u !

7 = g

CI C-T,

The momentum equation is:

a / l ) ,

. ' ( p r l , ) C I _ ^

#

CI

+ - " - lptr,D

C.T,

l t r l + , , i i l +

a F . ^ n t D n l - - - - i - i i t " ' ( 1 9 )

@tt?

+ po,,o,

' '

) !!.- = - ry- *!- *

o\Ptt'tr'

)

A-r., 6-t, 0-,, 6, ,

and the energy equation becomes:

+.3

6 t d r , "

t,r.' + pD

t

)tt,

+ (Ef + pF

)u?1=

t D ^

o0, c

- ; : 1 - "

f t l u

, + 'i u l )

c.r, o.ri

^ t - - r - - t F

n

n , l- t , , t t " , + u , p t t ' , u " , I - p u ' . i r " , u " , + y p e " i ' ,f

where

n ? u ! C u l 2 ? u ! T ; = F ( . + ^ - ; ^ - - d , , )(--r,

c.I; J r:r{

p ' = ( p u ' - p , u o ' X y - l )

')l

n o

= ! l u " - o'( ,

p L

\

' ' ' ( 2 1 1

r ) ) r

. (23)

, , / D I )

f - I t , I t i ) t l u ; u , n + l - n ' I

(4)

196

U(.r) = A - B TanhlC(.r - D)l (26\

w h e r e A . B , C a n d D a r e c o n s t a n t s . w h i c h c a n b e f i x e d t o d e t c r n l i n e t h e r a t c a n c l s i z e o f t h e d r o p i n l r e e s t r e a n t v e l o c i t y . F o r t h e s i m t t l a -t i o n s i n -t h i s s e c -t i o n w e L -t s c A = 0 ' 9 1 . B = 0 0 9 . C = 0 ' 0 u a n d D = 4 0 . w h i c h l e a c l s t o a f l ' e e s t r e a m d r o p o f 1 8 % c o n f i n e d w i t h i n t h e d o m a i n .

W e c o m p u t e t h e b a s e E , u l e r f ' l o w f o r t h i s s i r n p l e c a s e b y s o l v i n g t h e f u l l c o m p r e s s i b l e p o t e n t i a l e q u a t i o n

, t , - , , . ' . ' , r r - ' - l d - Q , ' - Q _ I l f c Q ), ' - Q I t a I r ' Q I

^ . - r ^ - - " l { - ^ l ^ ' - l - l ^ - 1

( y - ( ' y - r t - [ \ r l r l ( i r - \ r ' y l , ' y - _ ]

. . . ( ) l l

2 eb

a0 a-0

f t ^ ^

-ct- ox cy cxcy

r , v h c r e t h e s o r , r n d s p e e d a i s f i x e d r e l a t i v e t o s t l t g n r t i t t l t c o n d i t i o n s a . b y

2 C 4 C b

Streamwise velocity contours of a 2D self-excited bubble at

different times.

[image:4.612.332.575.87.371.2] [image:4.612.52.299.560.732.2]

T i m e

Figure 3. Time history oJ a wall normal velocity at various heights

s h o w i n g u n s t e a d y s h e d d i n g .

There havc been susl-ricions in the past that shedtlirtg tttav be

trig--Uerc-d nunterically so it is rtsel'ltl to havc pt'eclictiotls ol' tltc slttllc

phcnotlena witlr c()ntpLlter progrilnrs that use clil'lcrcrtt rttcthttcls.

Fig-ture rl shows the tinre avcraged bLrbble. Scpanttetl I'lori is fttttttcl fitr

- 5 0 < . r < 7 0 .

6.0 EXAMPLE

OF FAVRE-DNS

SIMULATION

F o r t h e s i n r u l l t i o r - r s in t l - r i s s c c t i o n \ \ c u \ L - . 1 = ( ) ' t ) - 1 . l l = 0 ' 0 ( t . C = 0 . 0 U a n d l ) = : 1 0 . w h i c h l e a d s t o a f t ' c - c \ t r c r t r l l d r o p o l ' l l % c o n -f i n c d w i t h i n t h e d o m a i n . T h i s r e s u l t s in a n u r g i n r L l l r - s c p u r u t e c l f l o u ' a n d w c a p p l y t i r r c i u - u a t t h e i n l - l o $ ' t o t r i g g c l ' t h c \ o t ' t e r s l l e d d i n g i n a c l e t e r m i n i s t i c w a y . T h e f o r c i n - s is g i v e n b r

s ' = 4 , . 1 ( . r ' ) S i n ( t ' r r ) . . . ( 1 9 )

w l r e r c /(r') is it norrlalisccl f'r-rnciton o f .r uitlt rt Ittrlritt'tttt.tt r a l t t c o f u n i t y a r , d a p e a k i l t - \ ' = I w i t h t h e c t ' r l l s t a t l t \ \ e l . l \ , , = ( ) ' 0 1 - 5 a t l c l t ' r =

0 . 1 2 .

T o g e n c r a t e a F a v r e b a s c l ' l o w u ' e f i r : t o 1 ' r i l l n r n r L n E L t l e t ' c l e c o t t . t -p o s i t i o n c a l c u l a t i o n t i r r t l t e -p r e s c r i b c c l [ l ( ) t c n t r i . r ] I ' l r r r t . [l c : t t l t s l k r r t t t h i s c a l c r r l l t t i t l n a r e s h o w n o l l F i g ' 5 ' A g a i r l u c ' ] l ' t t ' \ ( ) l . l c \ s h e t l d i n g ' b u t t h i s t i n t e i t i s r c g u l a r a n c l p r e c l i c t a b l c . l - h c r . c . t L l l . t r ( ) n t tl t i s s i t t t t t -l a t i t -l t -l a r e t h e t -l a v c r a g e c -l o v e r o l l e c v c l c t l l ' t l l e 1 r ; 1 ' i . , r ' 1 1 ' s h c t l c l i t l g t t l c l c t e n t r i n e tl r e I - - a v r c - l r v e r a g e c l n t e a n l n c l l ' l L t e t t L . t l t , ) n t a l ' l l \ . r \ t t h i s -p o i n t w ' c h a v c t h e s t a t i s t i c l l l e r l u i v r t l e n t o l ' i t . r L l . L t l . r l i l t t i r l t l l c F a r " r c

-Tu l, AEnoNAUTICAI Tounxal Aprul 2001

F i g u r e 2 .

( ao

)'l

T l ^ I 1

\ d v l ]

0 - - - t l ^ ( 2 8 )

A t t h e s u b s o n i c M a c h n u m b e r s u s e d h e r e t h e r i g h t h a n c l s i d e o f E q u a t i o n ( 2 7 ) i s s u f f i c i e n t l y s r - n a l l t h a t i t e r a t i r , ' c n u t l e r i c u l m e t h o c l s s L r i t a b l e f o r L a p l a c e ' s e c l u u t i o n s t i l l c t t n v e r ' - u c . W e t t s e a s t r a i Q h t f b r -w a r d G a u s s - S e i d e l p r o c c d u r e b a s e d o n s e c t t n c l - o r d e r f i n i t e d i t t c r -c n -c e s . T h e s o l u t i o n i s t h e n i n t e r p o l a t e -c l o n t o t h e a -c t l l a l m e s h t t l b e L r s e d i n t h e d i r e c t n u m c r i c a l s i m u l a t i o n s .

T h e s i m u l a t i o n u s i n g t h e E u l e r b a s e 1 ' l o w d e c o t n p o s i t i o n l l ' o t l l S e c t i o n 2 . 1 w a s r l l n u p t < t t i t n e / = , 5 0 0 . I n s t a n t a n e t ) L l s s n a P \ h ( ) t s () f t h e t c r t a l v e l o c i t l , f i e l d ( i . e . u = u t ) + r r l l ) ti r r t t a n c l t' a r e s h t l w n o n F i g . I ( a ) a n d ( d ) t o - s e t h e r w i t h t h e s t r e u m w i s e v a r i a t i o n o f s k i n l l ' i c t i o n ( b ) and the pressure field (c). It can be seen that there is an Llnsteady s e p a r a t i o n b L r b b l e w i t h w e a k n a t t t t ' a l v o r t e x s h e d d i n - e fr o r n b e h i n d t h e b u b b l e . A t i r n e s e r i e s o f t h e s l i e d d i n g . a s i t a p p e a r s in t h e s t r e i l n l -w i s e v e l o c i t y f i e l d i s s h o -w n o n F i - s . 2 . T h e r e s l t l t t h a t t h e r e i s v o t ' t e x s l r e d d i n g f i r r t h i s o w c o n c l i t i o n i s c o n s i s t c n t w i t h t l i e e a r l i e r s i t n u l i i -t i o n o l ' R i s -t e r r 1 1 ( l l ) . A d d i t i o n a l l y t i n r e s e r i e s n r e i - r s L r r c n r c n t s f r o t - t - t w i t h i n t l i e s h e d d i n g r e - e i o n (F i - s . 3 ) s h o w i t s h e c l d i n g in t l . r e f i r r r t l o f w a v e p a c k e t s w h i c h i s a l s o c o n s i s t e n t w i t h t h e p r e v i o t - t s fi n c l i n g s .

( o l

( b )

( . )

( d )

F i g u r e ' 1 . A 2 D s h e d d i n g b u b b l e . F i g u r e s t o p to b o t t o m s h o w i n g : ( a )

contours of streamwise velocity, (b) skin-friction, (c) contours of

pressure and (d) wall-normal velocity.

( y - 1 ) [ f u o ) '

-

, Lt&,

\ l

I

/

(5)

Saxnunur ET AL

( a ) c o n t o u r s o f s t r e a m w i s e v e l o c i t y and (b) s k i n - f r i c t i o n .

i l

l =

197

less empiricism than is possible at present. It should be noted that the

techniques apply equally well to large-eddy simularion (LES) as to

the direct simr-rlation approach nsed as an example here. Provided the

sub-grid models and LES techniqr-res are validated for the cornplex

ow phenomena. this represent a cost-effective way of uetting

sintula-tion techniques into ereronautical applications.

Another techr-rique which links simulation with conventional

mod-ellin-e approaches is the detached eddy simLrlarion (DES) approach

proposed by Spalarttll). The idea of this approach is to have a

sintu-lation techniqLre (LES) which reduces to a turbulence model as the

wall is approached. As an example if we have fully separatecl flow

the LES would be used for cornputing all the vortex events awi.ry

fion-r the surl-ace, while the conventional one- or two-eqLlation

turbu-lence models would pnrvicle reascxrablc wall bounclary conditions fbr

the LES. In many ways this techniclue is the oppositc of that

pro-posed here. where we propose to Llse DNS/LES near tlre wall in

dif-f'icult regiclns. and use conventional methods clsewhere. Ranges of

validity of the two approached rentain tcl be identified in tutr-rre

work.

In principle the tcchniques -{iven here cor"rld be applicd to other

re-gions of flow. An example might bc to trailin-e-edge f-lows. where

the f-easibility of simulations has already been demonstrated(r). An

additional problem here relates to the need to specify turbulent

inflow conditions. A sirnr-rlation approach is ofien used when

accu-rate in flow data is required.but there is a need fbr cheap methods of

prescribin-e tirre-dependent turbLrlent boundary laryer data over a

range of Reynolds numbcrs and upstrearn strain histories.

ACKNOWLEDGEMENTS

The authors are grateful for financial support fbr this pro.ject frorn

the Engineering and Physical Sciences Research CoLrncil. under

grant GR/M 21516. They woLrld also like to acknowledge hclpful

cornr.nents fiorn Mr Alan Gould of BAE Systents. Sowerbv

Research Centre.

R E F E R E N C E S

l . M o l N . P . a n d M , \ H E S H . D i r e c t n u t ' u e r i c a l s i n r u l a t i o n : a t o o l i n t u r b u l e n c e research. Atut Rev F'luitl Mecltrurr..i, 1998. 30.pp 539--5713.

2 . A t l , t N { s . N . A . D i r e c t n u t ' t ' t c t ' i c a l s i t n u l a t i o r . r o f t u l b n l e n l c o m p r e s s r o n rarnp flow. Tlteoretitul utttl Cotrtlttrlttliotrul f-lrtid Dyrttttirrr'.r. 1998. l2 ( 3 ) . p p I O L ) - 1 2 9 .

3 . Y . A . o . Y . , S l N n H , r l r . N . D . . T u c l H t , r s . T . G . a n d W r r _ r _ r , q n r s . J . J . R . S t u d y o l ' t u r b r - r l e n t t r a i l i n - l - e c l g e f l o w u s i n - u d i l e c t n n r n c r i c a l s i m u l a t i o n . P r o c In t

Evsgonno DrREC'r NUMERTcAI. sTMULATToN FOR AERoNAUTICAI. cFD

( o )

t c /

( d )

6 0 8 C l C C

X O

O

3

L)

(rj\\

a 2 c

F i g u r e 4 . M e a n b u b b l e :

( o )

( b )

-t c ,

( d )

a v e r a g e d e q l l a t i o n s u s i n g a p e r f ' e c t t u r b u l e n c e model. This is then s t o r c d a n d u s e d a s t h c b a s e f l o w f b r a sintr_rlation with the F a v r c / D N S d e c o r l p o s i t i o n e q u a t i o n \ , ( I f i 2 - r t .

R e s u l t s f r o m t h e F a v r e / D N S s i m u l a t i o n are shown on Fig. 6. As e x p e c t e d t h e f l o w p h e n o m e n o n o f s h e d d i n - e i n r e s p o n s e to L r p s t r e a n t f b r c i n g i s r e p r o d u c e d b y t h i s r n e t h o d .

B o u n d a r y c o n d i t i o n s a r e t h e m a i n area that requires further work. I d e a l l y b o r " r n d a r i e s w i l l a l l o w s p e c i f i c a t i o n o f s t e a d y i n f k r w p r o f i l e s . w h i l s t s i m u l t a n e o u s l v a l l o w i n - s w a v e s g e n e r a t e d within the simula-t i o n simula-t o l e a v e s m o o simula-t h l y . T h e p r e s e n simula-t c h a r a c simula-t e r i s simula-t i c - b a s e d nsimula-tesimula-thocls l e a d t o a s l i g h t d r i f t i n t h e m e a n f l o w e u r d w e ilre expcrinrenting with n e w b o u n d a r y c o n d i t i c l n s to o v e r c o m c t h i s p r o b l e r n .

7 . 0 D I S C U S S I O N

A N D C O N C L U S I O N S

We have prescnted a new decomposition approach to solvin-g

acro-nautical CFD problents. The philosophy of the merhod is ro apply

the ri-cht rnethods to the right parts of the f1ow. using conventional

Er-rler and Favre-averaged-Reynolds-averaged methods firr relatively

simple parts of the flow. bLrt inserting a time-dependent simulation

when the l1ow phenomena are complex. In the exantple shown here

we consider the case o1' leading-edge separation br_rbbles where the

idea is firr thc simulation techniqLre to treat the immediate vicinity of

the bubble, f'eeding back infbrr.niltion to the Favre-averaged tlow

cal-culation o1'the rest of the confi-uuration. It is hopecl in the firture to

[image:5.612.318.559.79.249.2]
(6)

1 9 8 Tue AEnoNAUTTcAL

lounNar-C o n f o n T u r b u l e n c e a n d S h e a r F l o w P h e n o m e n a . S a n t a B a r b a r a , 1 9 9 9 . St',,\r-,ARr. P.R. and SrREr-n'rs. M.K. Direct and Reynolds-averaged nu-merical simulation of a transitional separation bubble. J Fluitl Mer:h, 2000. 403. pp 329-349.

Alav. M. and SnNoH,A.Na. N.D. Direct numerical simulation of 'short' laminar separation bubbles with turbLrlent reattachment. J Fluid Mec.h, 2 0 0 0 , 4 1 0 . p p 1 - 2 8 .

HRozrc, and HnN:alrc. K. Separation-induced transition to turbulence; second-moment closure modelling. J Flotr, Turbulenc'e tnd C o r n b u s r i o n . 2 0 0 0 . 6 3 , p p 1 5 3 - 1 7 3 .

H o w e n o , R . J . A . , A l e . l r , M . a n d S a N o s a n r , N . D . Trvo-equation turbulence rnodelling of a transitional separation bubble, J Floyt, Turbulenc:e and Combustion, 2000.63, pp I 7-5- l9l .

W t t . c o x . D . C . T u r b u l e n c e m o d e l l i n g f b r C F D . 1 9 9 4 . D C W I n d u s t r i e s . LEI-E. S.K. Compact finite diff'erence schemes with spectral-like resolu-tion, -/ Computtttionol Physic's, 1992,28. pp 16-42.

S R N o H u , H . S . a n d S n N o H e u , N . D . S i m u l a t i o n s o f l e a d i n g - e d g e r e c e p -tivity to fiee-stream disturbances, 1996. lnternal Report EP-lll0 Faculty of E,ngineering, Queen Mary and Westfield College. University of Lclndon.

RIsr', U. Nonlinear ettects of 2D and 3D disturbances on laminar sepa-ration bubbles, Proc IUTAM Symposium on nonlinear instability of non-parallel flows. New York, 1993.

Spnla.nr. P.R. Strategies tbr turbulence modelling and simulations, 4th I n t S y m p E n g T u r b M o d e l l i n g a n d M e a s u r e m e n t s , C o r s i c a , M a y 1 9 9 9 .

Aprur

2001

4 .

7 .

Figure

Figure 3. Time history oJ a wall normal velocity at various heightsshowing unsteady shedding.
Figure 4. Mean bubble:(a) contours of streamwise velocity and (b)

References

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