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Velocity intermittency in turbulence : how to objectively characterize it ?

Antoine Naert, Laurent Puech, Benoît Chabaud, Joachim Peinke, Bernard Castaing, Bernard Hebral

To cite this version:

Antoine Naert, Laurent Puech, Benoît Chabaud, Joachim Peinke, Bernard Castaing, et al.. Veloc-

ity intermittency in turbulence : how to objectively characterize it ?. Journal de Physique II, EDP

Sciences, 1994, 4 (2), pp.215-224. �10.1051/jp2:1994124�. �jpa-00247956�

(2)

J. Phys II France 4 j1994) 215-224 FEBRUARY 1994, PAGE 215

Classification Physics Abstracts

47.25

Velocity intermittency in turbulence

:

how to objectively

characterize it ?

Antoine Naert, Laurent Puech, Benoit Chabaud, Joachim Peinke, Bemard

Castaing

and

Bernard Hebral

Centre de Recherches sur (es Trds Basses Tempdratures (*), CNRS, B-P- 166, 3804? Grenoble Cedex 9, France

(Received 22 Marc-h J993, re>,ised 2J september J993, accepted 25 October J993j

R4sum4. L'dvolution d'un certain paramdtre A~ ddfini dans l'article a dtd utilisde pour tenter de trancher entre diffdrents moddles de l'intermittence en turbulence. Le but de cet article est de valider une mdthode

e~pdrimentale

de ddterrnination de ce paramdtre,

inddpendamment

de tout

meddle, h partir des densitds de

probabilitd

de diffdrences de vitesse (pdo. Les conditions

expdrimentales

qui

perrnettraient

de pousser plus loin la caractdrisation de ces pdf sent dgalement discutdes.

Abstract. The evolution of A~, a parameter whose definition is recalled in the paper, has been used in order to test various interrnittency models in turbulence. This paper aims to validate an experimental, model independent, method for

extracting

this parameter from the

velocity

difference

probability density

functions

(pdo.

We also discuss the charactenstics of an experiment which could push further the analysis of these pdf.

1. Introduction.

Statistics of

velocity

difference between two

points

is the main tool for

characterizing developed

turbulent flows

[1, 21. Recently

the

interejt

shifted from the moments of the

distribution of these

velocity

differences to the

study

of the whole

probability density

function

(pdf~ [3-51.

Models were

proposed [4-91,

based on various

physical grounds,

each one

giving

a

good

agreement with the observed

pdfs.

Thus the

problem

is less in this agreement than in the

insight

the

corresponding analysis gives

into the

underlying physics.

Most of the

proposed

models can be

presented

in a unified way

connecting

the

pdf

at a scale

r to the

large

scale one

[10, 1].

If &u is the considered component of the

velocity

difference

&u

=

u,(x

+

r) u~(x)

(*) Laboratoire associd h l'Universitd Joseph Fourier.

(3)

and

P~

~~ its

probability density

function

(m)

=

(&u~) ),

these models assume that

"r "r

)Pr~~) "iGr~~)PL()j$ (I)

r r r

where L is the

large integral

scale and G a distribution which

depends

on the model.

In this paper we show the interest of

using

a

log

normal ansatz for G~:

~

ln~ «/«~

G~ cc exp

~

(2)

"r 2 A

(in general

«~, which

gives

the maximum of

G,

is different from

«~).

This interest does not

only

lie in that this should be the

limiting

form for G~ at a small r

lO].

The

major

interest is that the parameter A~ obtained in

fitting

the

experimental P~

with

equations (1, 2),

measures the

mean

squared

deviation

((&

In

«)~),

even if G~

significantly

differs from a

log

normal distribution. This is

important

for the

following

reasons. The

existing

theories on

intermittency

in

developed

turbulence

predict

both different

shapes

for G and different behaviours for

((&

In

«)~)

ve;sus r,

Physically (

(& In

«)~)

measures the

progression

of

intermittency along

the scales

(number

of steps in the cascade

models).

For instance the

Kolmogorov

Obukhov

theory [2],

which can be seen as one

particular

multifractal model,

predicts

a

logarithmic dependence

1(&

in

«)~)

=

(

in ~

On the other

hand,

the variational model [71

gives

a power law

dependence

(

(b In «

)~)

cc r~ P

Our message is that

discriminating

between these models

by looking

at the behaviour of

((&

In «

)~)

versus r is much easier than

by determining

the

shape

of

G,

to which the

pdf

of

3u is

poorly

sensitive,

We demonstrate this

point

in sections 2 and 3

by constructing

an artificial

pdf

for

&u

using equation (I)

where G is

deliberately

different from a

log

normal distribution, In section 3 we use a binomial distribution

recently proposed

as

corresponding

to the random beta model, a multifractal type one, In each case we show that the behaviour of A~ well reflects that of

(

In « )~

)

In section 4 we address the

question

of the

shape

of G. We discuss the characteristic of an

experiment

which could

adequately

discriminate between different

proposed shapes.

We show that a

large

number of

significant

measurements are necessary, of the order of 10?

points.

2. A first

example.

As discussed in the introduction we now construct an artificial

pdf using equation ii)

P~~(x)

=

~~

~~~

i~~

exp

~~~

(l + b

In~

«

~

exp

~~

~

(3)

(2

ar « 2 A 2

«

where x stands for ~~ and « for

I

and

A~ is the normalisation factor. We denote it

«~ «~

(4)

N° 2 MEASURING INTERMITTENCY IN TURBULENCE 217

P~~

because we shall treat it as an

experimental

distribution and search for the parameter A which makes the « theoretical » distribution

~~~~~

(2

A

$

~~~

)~A~

~~P

~

~~~

having

a

shape

the closest

possible

to the

P~~

one. We then compare A ~ with :

n ~r

~~~

~~l

Ae (in

« )2 ~~~

in2

fi

« ~~ ~ ~ ~~~ "

~

d in « ~~~

We have thus first to

adequately

determine the difference in

shape

between

P~~

and

~ih

We

begin by normalizing

them to the same mean

squared

value,

namely1, Pe(X')

" "e

Pex("eX~) (6)

p,(x<)

= «~

p~(«~x<) (7)

with

+JJ

+JJ

x'~ P~(x')d~<'=

j

(a~x')~P~~(a~x') d(a~,<')

=

£Ye

~-«

and

+~J

+~

X~~

~t(X~)

i~~

~ j

(£Yt~')~ ~th(£YtX~) d(£YtX~)

~ l

-oJ £Yt -~

In a real

experiment,

the

pdf

is constructed

by accumulating

the events in

histograms

where x' has a

given

value

xl

within A. Let

n~ be the number of events such as

X,' ~,t~

~ X,' + d.

If N is the total number of measurements, P

(x,')

= 2

A

The difference between two models for the

pdf

has to be

compared

to the difference we

expect between two realisations of the same

experiment,

which is

given by

(n~

h,)~

= h~

and thus

(P (x,') > (x;'))~

~

~

In a first

approach,

a measure of the difference between

P~~

and P~~ could thus be the

integral

~+"

(Pe(x') P,(x'))~

~,

-m

Pt(x')

P~(P

~) is the normalised version of

P~,(P~~).

See

equations

(6,

7).

However such an

expression

could not converge if

P~

and

P~

has very different

asymptotic

behaviour when x'

~ ± oo

(see

(5)

Sect.

4).

We thus

prefer

to define

~

+°~

~

(Pe(x'l-Pt(x'l)~

~, ~

~

_~

P~(.<')+P~(x')

Let us now compare

P~~ given by equation (3)

with

A~

=

0.49 to P

~~

(Eq. (4)).

The

integrals giving P~(x')

and

P,(x')

have been calculated

by

the

trapezoidal

rule with an absolute

precision

of 10-~°

((3

In

«)~)

has been evaluated within 10-5 of relative

precision

and

X~(A

~) was calculated within 10-2 of relative

precision [12].

The minimum of

X~(A

~) was estimated

by

the method of Brent

[121.

Three A~ values are chosen in the

neighbourhood

of the

expected optimum

: A

),

A

j,

and a

parabola

is fitted with

the three

corresponding X~' X~(A)),

The minimum of this

parabola gives Al,

The process is

then iterated with

Al

and the two closest of the

preceding Al,

It is

stopped

when two successive minima differ

by

less than 10-3 in absolute

precision,

6 0" ~

x2

4

0'~

2 0" ~

b

0 0.2 0.4 0.6 0.8

Fig.

I. The difference X~ versus the deformation parameter b.

In

figure

I we have

plotted

the smallest

X~ (Eq, (8))

versus b which measures the difference between the

«

experimental

» G distribution and a

log

normal distribution,

The

X~

values are

rising

rather

rapidly

with b, Then

they

saturate at a

relatively

small b value. This can be understood. When b is

large

the width of the distribution G becomes very small. G is then similar to a Dirac

distribution,

whatever its

shape

and the

corresponding pdf

goes to a Gaussian

shape (see Eqs,

(Ii and

(4)),

Thus

X~

should go to zero when

b goes to

infinity,

For b

= loo,

X~

is

equal

to 1,7 x

10~~.

The small values of

X~

are coherent with the small difference observed between

A~ and

(

(3 In «

)~) (Eq. (5)),

This is shown in

figure

2, The decrease in A~

corresponds

to the

above mentioned

sharpening

of G when b grows,

Looking

at different

A~

values

(A~

=

0.49,

0.7 and

I)

we have been able to summarize the

X~

behaviour

by

an

approximate scaling (Fig. 3).

Within a few percent,

X~/A~

behaves as a universal function of bA. This

scaling

is

probably

fortuitous and not even true in the

neighbourhood

of b

=

0. However the values we have

spanned

are the

experimentally interesting

ones

[7, 1II

and this

approximate scaling

could

help

in

estimating

an effective b value from the measured

X~

and A 2 values.

The conclusion of this section is thus clear : the parameter ~ obtained from the

experimental

method we discuss

always gives

a

good

estimate of

((31n«)~)

even if the real

G function is

significantly

different from a

log-normal

distribution. As this result has been

(6)

N° 2 MEASURING INTERMITTENCY IN TURBULENCE 219

o.5

,-

0.45

0. 4

0.35

0 3

<ln20~

0.25

~2 0.2

0 0.2 0.4 0,6 O-S I

b Fig. ?. Comparison between and

((6

In rr

)~).

0 0 0 6 , ~ -. .i T --1 .-~-r i~

xz/~4

0.004

0.002

b~

0

0 0.1 0.2 0.3 0.4 0.5

Fig. 3. The appro~imate sc311ng ~ummanzing the X~ behaviour 1,e13us and b.

obtained

through

a very

peculiar

and ad hoc class of G function. we shall

strengthen

the argument

by using

a more credible class of function,

recently propo~ed.

This will in

particular

introduce the effect of the asymmetry of G iersiis In r,, Another conclusion is that the value of

X~

if

;tati,tically ~ignificant,

could

help

in

revealing

a difference between the real G and a

log-normal

distribution. This last

point

will be

developed

in the fourth section, 3. The binomial distribution.

Recently

Benzi et al.

[81

derived a formula for the

pdf

of

velocity

differences within the framework of the random beta model

[131.

Their result for the

pdf

at the scale r is

P~(&v

cc

~ ~j

~ a "

~(

l a

)~

B~~~~

ii

"~

exp[- CB~

~'~

ii ~'~(3v

)~

(9)

~~

K~

where

f,,

=

'

=

2~" C

=

(2 Vi j~' Vo being

the characteristic

velocity

difference at

large

L

~cale. a

=

7/8 and B

=

1/2 are chosen such i to

reproduce

the

(~

values obtained

by fitting

the

experimental p-order

moment

((3uy)

with a power law in I

((&CY)

CC i~~

I<fi ~'ii Iii i'ili'i'jt it -T ' lL3W'Rh1>»~ '

(7)

With the notation of our

equation (1)

we have

" "

V0 ~i~ B~~~

" "n

B~~~ (lo)

The distribution G is

given by

G(I

cc

( [~j a~~~(I

-a)~B~3(In ~i +~lnB), (11)

~n K=0

~ ~n 3

Thus

~3

In "

~)

=

~~~

j~ ((3K)~)

~n 3

=

n(

~~~

)~ "~~

"~~

(12)

3 (~x +

B(1

a

))~

Following

the same process as in section 2 we

identify

the

pdf given by equation (9)

with

P~~(3u).

We then normalize it

through equation (6),

and we compare this normalized

pdf P~(x')

with the normalized

«

log

normal» one

P~, searching

for the minimum of

X~. This minimum value and the

corresponding

A~ value are

given

in

figures

4 and 5, for a

large

range of values of n,

~ , ~. 4 X2

4

10"~

2

0'~

n

0 20 40 60 80 100

Fig, 4, The difference X~ versus n for the binomial distribution,

0 3

~~ ~,

,

;

;

~" <ln2~

0 .2 '

o. i

n

0

0 20 40 60 80 100

Fig.

5.

Comparison

between A~ and

((6

In

«)~)

for the binomial distribution.

(8)

N° 2 MEASURING INTERMITTENCY IN TURBULENCE 221

The difference between A~ and

( (3

In «

)~),

and the minimum values of

X~

are

larger

here than in the

previous

case. This is

probably

due to the

large dissymmetry

in In « of the

« binomial » distribution,

This

dissymmetry

appears when

comparing

a

typical

« binomial »

pdf

(n = 15 with the

«

log

normal » one

giving

the lowest

X~

(see

Fig. 6).

Our choice of

X~ (Eq. (8)) clearly

emphasizes

the center of the

distribution,

where the

experimental precision

is the best one, The

discrepancy

appears in the

wings.

lo(~P

3

5 P

/ P

(n=15)

',

,' b~

7

-lo .5 0 5 lo

x

Fig,

6.

Comparison

between the « binomial

» pdf (n = 15) (full line) and the best fitted « log normal »

one (dashed line), The experimental points are given to

figure

a

typical uncertainty.

Here the number of

independent

measurements is 2 x 10~. A significant

comparison

needs to take account of the skewness

through

the asymmetry of Pi (Eq. (I)). See reference [71.

We note however that the difference between

A~

and

((3

In

«)~)

remains within 15 fl.

More

important,

A~ appears as

nearly

linear in n in the present range, which is a

significant

characteristic of

( (3

In «

)~)

in this type of models. The behaviour of A~ thus well reflects the behaviour of

((3

In

«)~),

even in this extreme case.

In

particular

the recent evidence

[7, 121

for a power law behaviour versus r for

A~ shows that

((3

In

«)~)

presents a similar behaviour. In the cascade models like the

random-beta one discussed in this

section,

the number of steps n should not be taken as linear in In r but

proportional

to

r~P

4. The statistical error.

The minimum

x~

values obtained in the two

previous

sections were

relatively

small. So the

question

raises of the

experimental

accuracy needed to

distinguish

between a

log

normal distribution of « and a deformed one for instance, In this section we estimate the minimum

x~

to be

expected

if one compares an

experimental pdf (with

N measurement

points)

with its

exact

shape, asymptotically

obtained with an infinite number of measurements.

Let us call J the size of a class, like in section 2. We have to estimate

X~=2 ( ~~~~~'~ ~'~~'~~~A= ( E, (13)

,=-«

Pe(x,)+Pt(.«)

,=_«

(9)

where

P~

i~ now the

experimental pdf

and

Pj

its

asymptotic

limit when N

~ oo. The number of

points

in the class is n, N

~P~(,i,

) for our

particular experiment

and it~ average

expectation

value is

h,

= N

APj(.i,).

Two

limiting

ca~es have to be considered.

2

k,

~~ ~~'~ ~' ~~~~

~~~~'~

~

~~~"'~

NJ

(F~(v, P~(

i,

I

=

~ (ii~ fi,

I

=

~'

(14)

N- J- N-

J~

as~uming

a Poisson distribution for ii,. We get

2 (P

~(.t',

Pi (,ii

)~

~ l

~~ ~ P

~

(.t,

+ P (-I,) N

iii

h,

« I. If fi~ i~ zero we have

E,

k~

=

2 ~P i-r, 2

If ii, is or

larger,

we can

neglect P~(,i,)

and

E,

n,

=

2

AP~(,1,

=

2

Calling ar(fi,)

the N

probability

to get n, we have

E, =2r(0)j+2zar(fi,)(=2(1+ 7r(01)(=/=4AP~(_r,).

(16) Note that if

x~

were defined with

only P~

(and not

P~

+

Pj)

in the denominator, the sum of

equation

(13) would

diverge.

We shall

interpolate

between these two

limiting

case~

taking E,

= 4

k,/N

for fi, w and

E,

=

for

k,

m Let us call 2 i~ the

length

of the interval on

which k~ m For a

large

N the

major

contribution to X~ comes fmm this interval and

4

~

2,ij,

X~=- (17)

We can go a step further

assuming

a

particular shape

for

P,.

An

exponential shape

has often been used to fit such

pdf.

It

gives

P,(.1)

=

~-exp(-

i-11

,'2)

, 2

(the

variance of

P~(,i)

is I). ~i~ is

given by

~~

exp(-.ij,

,. 2)

=

, 2 4

or .i~, =

~-

ln (2

, 2 NJ1

,, 2 The contribution of j-v ~_<~ is

m

,/j

2 4

P,(~<)

d~< = 4 exp (- iii , 2)

=

~

'i,

(10)

N° 2 MEASURING INTERMITTENCY IN TURBULENCE 223

Then

X~"~(l

+ In

(2,2NA)), (18)

The result

depends

on the size of the class as too small a class

gives large

statistical errors in the

counting,

On the other hand too

large

classes introduce errors in

estimating

the

integrals,

We shall take J

= 1/30 as a

compromise,

that it classes 30 times smaller than the root mean

square of 3u,

From the

preceding

section we know that an order of

magnitude

for

X~

which allows some distinction between the

possible shapes

is lo ~ This ask for N m

lo?

uncorrelated measure-

ments. This is close to the

large~t samples

used yet

[71.

For

distinguishing

between two

proposed shapes

the strategy is thus clear. First the number

of measurements must be sufficient for the

« statistical

»

X~ being

smaller than that

giving

the difference between the two

shapes.

Second the

X~

must be estimated

using alternatively

the two

proposed shapes

as the

« theoretical » one, The smaller X~ is the be~t and must be of order of the

« statistical

» value to be the

good

one.

5. Conclusion.

The conclusion of this

study

is that the

shape

of the

pdf

i~ more sensitive to the width of the distribution G of In « than to its exact

shape.

The parameter ~ obtained

by using

a

log

normal

ansatz for G is

always

a reasonable measure of

((3

In jr

)2),

Physically

this parameter is an

objective

measure of the evolution of the difference of

velocity pdfs,

In all models

referring

to an energy cascade, as for instance the random beta model discussed here in ~ection 3,

(

In «

j~)

is

proportional

to the number of cascade steps.

Our

study

thus

fully

validate~ an

experimental

way of

measuring

this

important

parameter,

This method ha~

already

shown that

((&

In

(,)~)

does not behave as In r, as is

generally

assumed, but more as a power law in ;.

The second

question

addressed in this paper concerned the

shape

of the distribution of

i, ; G. We have shown that a

significant

check of this

shape

asks for very

large

statistical

~ample,,

however not out of the present

experimental possibilitie~.

In

particular, distinguishing

between a binomial di~tribution as

proposed

in reference

(8]

and a

log

normal one as

proposed

in

[41

i~

certainly

feasible.

Acknowledgments.

Thi~ work has been

partly ,upported by

a DRET contract (N° 9?/105) and the

Rdgion

Rhbne-

Alpe,,

References

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[21 Monin A. S.~ Yaglom A, M., Statistical Fluid Mechanic~ (the MIT Press, 1975).

[3] Gagne Y., Thesis (19871 (Institut National Polytechnique de Grenoble, unpublished) Advances in Turbulence 3

(Springer Verlag

1991).

[4j Castaing B., C-R At-ad. SC (Pa;is) 309 ~erie II (19891503.

(5] Kraichnan R., Pfi,vs Rei Lett. 65 j1990j 575 She Z. S., F/ilid Din. Research 8 j1991j 143.

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[61 Andrews L. C.,

Phillips

R. L,,

Shivamoggi

B. K,, Beck J. K., Joshi M. L., Phys. Fluids Al (1989j 999.

[7]

Castaing

B., Gagne Y.,

Hopfinger

E,,

Physica

D 46

(1990j

177.

[81 Benzi R,, Biferale L., Paladin G., Vulpiani A.,

Vergassola

M., Phys. Re». Lett. 67 (1991) 2299.

[91 Eggers J., Grossmann S., Phys. Rev. A 45 (1992) 2360,

[10]

Castaing

B,, Gagne Y., Turbulence in

Spatially

Extended

Systems,

R. Benzi Ed, jLes Houches 19931.

[tl]

Castaing

B,, Gagne Y., Marchand M., to appear in Physica D.

[12] Press W. H.,

Flannery

B. P,,

Teukolsky

S. A.,

Vetterling

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