October,
1969.
EDDY MACH WAVE NorSE FROM A
SIMPLIFIED MODEL
OF
A SUPERSONIC
MIXING
LAYER
by
H.
S. Ribner
EDDY MACH WAVE NOISE FROM A
SIMPLIFIED MODEL OF A SUPERSONIC
MIXING LAYER
by
H
.
S. Ribner
Manuscript received Ju1y 1
9
6
9
ACKNOWLEDGEMENT
This research
was sponsored
by
the Air Force Office of Scientific
Research, Office of Aerospace Research, United States Air Force, under
AFOSR Grant No.
67-o672A.
SUMMARY
A simplified flow model is presented for simulating features of
noise generation by supersonic jets and rockets.
'Eddy Mach waves' appear
as a consequence of balancing internal and external pressures, and noise
power may be estimated.
Specifically, the turbulent IDlxlng layer of a supersonic jet is
modeled as a layer of two-dimensional square 'eddies'; this separates the
main flow U. from fluid at rest and moves at an intermediate speed.
(In
an improvedJmodel the square eddies are replaced by a turbulent flow layer
constrained by Plans. interfaces).
The initially plane interfaces, because
of unopposed internal pressures, will ripple slightly such that Mach waves
a
rise and effect a pressure balance
.
The Mach wave noise pattern is
readily calculated as well as the acoustic energy flux.
In an example simulating a round rocket jet the effective mixing
layer area is taken to be
6
~ (diameters)2, the r.m.s. eddy velocity is
0.1 Uj' and Uj
= 6
times external sound speed.
The efficiency (noise power
/
flow power) comes out to be about 1/3%, which is of the order of measured
values for rocket noise.
TABLE OF CONTENTS
NOTATION
INTRODUCTION
THE MODEL
RIPPLE AMPLITUDE
ACOUSTIC ENERGY FLOW
NOISE FROM ROuND JET
EXAMPLE AND DISCUSSION
IMPROVED FLOW MODEL
COMPARISON WITH OTHER MODELS
REFER ENC ES
FIGURES
'.1
1
2
3
3
4
4
6
7
c
D
f
I
kL
M
n
p
U
u
,
v
x,
y
w
13
8
'I/J
p 1]Subscripts
abs
j
m
0 "NOTATION
sound speed
jet diameter
frequency of eddy Mach waves
acoustic ene
r
gy
flux
per unit area normal to
mixing layer
wave nurnber
(2H/wave length)
edge length of square cells ('eddies')
Mach
number
based on external sound speed (U/c )
o
effective length of mixing region (diameters)
Perturbation pressure
(p
abs
-p)
0local mean flow speed
components of local
perturbation
velocity
co-ordinate
frame (x aligned with flow)
r.m.s
.
(spatial
average) velocity
in square 'eddies'
.J
M
2
-1
m
angle with
horizontal of
normal
to Mach
waves
stream
function
density
efficiency (noise power/flow power)
absolute
main jet flow
mixing layer
ambient (outside
jet)
INTRODUCT ION
The present paper studies a s
i
mplified flow model simulating features
of 'eddy Mach wave' generatio
n
i
n
t
h
e
n
oise from supersonic jets and rockets
.
Shadowgraphs show these Mach waves emanat
i
ng from the turbulent mixing layer
s
eparating the core of the
j
et from the
fu~bientfluid. This mixing layer
is not of constant width, b
u
t
c
on
t
i
nu
a
ll
y sp
r
eads in the downstream direction.
It can be described loosely i
n
te
r
ms i
rr
egular unsteady 'eddies' which defy
a precise description.
In this model the ir
r
eg
u
larity and the spreading are suppressed in
a deliberate o
v
e
r
simplification
.
The mi
x
ing layer is postulated as an array
of square flow cells (models of eddies) convected at the supersonic mean
flow speed of the layer
.
It is thought tha
t
some broad features of the
phy-sical processes responsible for noise ge
n
e
r
ation are retained and displayed
ve
r
y simply
.
THE MODEL
The
s
quare eddy model o
f
the mi
xin
g laye
r
i
s
sho
w
n in Fig.l
.
The
eddy flow i
s
given by
w
c
o
s
kx cos ky
u
J2
( 1)
w
si
n kx
sin
ky
v
='J2'"
with
s
tre
a
m fun
c
tion
?jJ
w
c
o
s kx
s
in
k
y
kJ2
( 2)
He
r
e w i
s
the r
.
m
.
s
.
velo
city in t
he
c
e
ll
a
n
d the wave number k is related
to the laye
r
thickne
ss
L b
y kL
=
rr
.
(
Th
e laye
r
may be general
i
zed to n cells
thicknes
s i
f des
i
red u
si
ng
kL
=
nrr~t
he ph
ysic
al arguments will be unaltered).
It is a
ss
umed that w i
s suffi
c
i
e
nt
l
y s
ma
l
l so that the eddy flow (not the
main flow) may be
c
onside
r
ed
inc
o
m
p
r
e
ss
ible
f
o
r
simplicity
.
The pressure
field in t
h
is laye
r
would be
, if c
o
n
st
r
a
in
ed between rigid plane boundaries
ky
=
0, - rr
s
o t
h
at (1) ho
l
d
s accur
a
t
el
y
,
2
p
w
m.
(co
s 2
k
y
-
c
o
s 2
kx
)
+
constant
2
by integ
r
ation of Euler's equa
ti
o
n
s
.
T
he a
v
e
r
age value of this along the
boundarie
s
ky
=
0, - rr is taken to
m
a
t
ch the ambient pressure p . ,The
o
perturbation pressure p b
a s o
- P
is th
e
n
2
p
p
w
_
m
""'
2
- -
cos
2 kx
(4)
The boundaries, however, are not rigid and are not capable of
sup-porting the pressure difference p of equation
(4).
On removing the artificial
constraint of rigidity the boundaries
will
deform into ripples which, because
of their downstream motion, will generate Mach waves (Fig.2). An equilibrium
can be specified in which the Mach
wave
pressure field will balance the 'eddy'
pressure field
(4).
It will be justified a posteriori that the distortion will be so
small that the errors introduced into equations (1) to
(4)
will be negligible.
Then the pressure enforced in the wave field is merely (4) at the interface
y
=
0,
and for y
~0
it is
p
-2
P
w
m2
cos 2k (x
+
f3y)
which corresponds to Mach waves inclined as dictated by the Mach
,
number M
=
UJc (Ref
.1).
m
Equations
(1)
to (5) apply in a frame of reference moving in the
positive x-direction with the ripple speed Um.
In a stàtionary frame (5)
becomes
p
2
P
w
m- 2 -
cos
2
kx
(x - U t
m+
f3y)
(6)
which exhibits the Mach waves as moving sound waves.
The waves move past a
fixed point with speed Um' giving rise to frequency f
=
k
uJ~
=
UJL.
The sound pressure
(5)
or
(6)
in this Mach wave field by our
physi-cal argument matches the 'eddy' pressure field at the boundary of the mixing
layer; we may call the latter the 'near fi
'
eld' of the simulated turbule nt
jet. The Mach waves thus extend the near field pressures to the radiation
field.
RIPPLE AMPLITUDE
We now explore whether the
ripple
amplitude is small compared with
the 'eddy' edge length L as has been assumed.
The boundary conditions are:
a) The pressure must be equal
011opposite sides of the rippled
inter-face.
This is met by
(5)
and
(6).
b) The streamline slopes must be equal on opposite sides, in the
ripple-attached
reference
frame.
Condition (b) will be
automatically
enforced when we choose the
ripple
u
amplitude compatible with the Mach wave pattern
(5);
it is given by
(Ref.l)
.
[
p
f3
U 2Po m
o
2
2
1Pm
(
~m)
t3
COS2kx
2"Po
2
1
Pm
(~
)
t3
sin 2kx
y
=4k
-Po
m
(8 )
Since
kL
TTthe
ripple
ampli
tu
de
is
2
t3
Pm (w )
L
Ymax
Tm
Po
Urn
in terms of the r.m.s. turbulence level
w/U.
As a severe test case
take~w/U
m
= 1/3 (an upper limit),
M
m
3
(or
t3
=m
2
~), prnfp
o
= 1. Then
Ymax
= 0.025
L
(10 )
This confirms that the
ripple~am
plitude is very much less than the
eddy length
L.
The distortio
n
of
the initial square shape
may thereby be
neglected insofar
as
its effect on
the internal
pressure and velocity fields
is concerned. This neglect is
not wholly
defensible at the higher turbulence
velocities
where
the assumption of
incompressible internal
flow becomes poor.
ACOUSTIC ENERGY FLOW
The
flux
of acoustic e
n
ergy
through
unit area is p2/p c
in a
direction normal to the
Mach waves.
The vertical
component in
0 0Fig. 2 is
2"
I
-
p
----
si
n
8
Poco
The mean square pressure
is P
2w
4
/8
fr
o
m
(6),
and sin8
=
~
2_1/M
t3
/
M,
m m m
m
giving
I
2
4
Pm
w
8
Po
(n)
as the flux of acoustic ene
r
gy
through unit
area normal to the mixing layer.
NOISE FROM ROUND JET
We
will
curve
the
plane
mlXlnglayer, equations (1) to
(3),
into
a cylinder to simulate the mixing layer of a round jet (Fig.3).
Since our
model is
at
best a crude one we
shall
assume that the energy flux per unit
area, equation (11), is still app
r
oxi
m
ately valid.
The effective
length
of the
supersonic
mlXlng layer will be taken
as n diameters, giving a
total surface area
nD.
no.
The
acoust
ic
power
radiated from this
area will
then be
noise
power
= TTn
D I
2
(1
2)
And
by
comparison the mechanical power expended in the kinetic energy of
the jet flow will be
flow
power
8
P.U.
J J
3
(13 )
The ratio (noise power/flow power) is the
acous
tical
efficiency
2
4
2n
_:_m_
p
_._
(U
~
)
o J
J
(1
4
)
where
the mean speed Urn of the mixing layer has been taken to
be (1
/2
)
U.'
J
EXAMPLE
AND
DISCUSSION
In an example
intended
to simulate
crudely
a
rocket jet
-it
will
be convenient to
a
pproximate
p
as a
geometric mean density.
The
m
example
specif
ic
ations are:
n
=
6,
U.
= 6
c
.
w
J O '
2
0.1 U. ;
p
/p
p.
=1
J
m
0J
Insertion into
(14)
yields the acoustical efficiency as
~
=0.0034
or
0.34%
(15)
It is rather striking that this is of the order of magnitude of measured
efficiences of rocket jet noise generation.
Other proposed mechanisms for the noise generation - for example
the Lighthill quadrupole model with supersonic convection factor
-
do
pre-dict comparable efficiences (Refs.
2
-
4).
Thus the present model
cannot
be
affirmed as
necessarily
simulating
a dominant mechanism of noise
genera-tion by supersonic jets. The physical arguments
with
support of the
example
results
sugges
t
it may be
an
important mechanism.
A word about accuracy: the equations employed herein, as applied
to the specified flow model, are as
accurate
as the
Lighthill
equations
for
flow noise
in
their general form, and are more
accura
te than the usual
solution
with the
const
ant
density approximation.
The approximation
is
in
the flow model, not in the mathematics
.
IMPROVED
FLOW MODEL
It is possible to improve the model to better simulate features
of
a turbulent mixing layer
while
still retaining the
basic
simplici ty.
In the
improved model
we
replace the square eddies by random turbulence, retaining
the plane interfaces. To show that this is possible consider tÈat
a
infinite uniform flow with superposed turbulence and its mirror image will
be separated by aplane stream surface.
In
the model we remove the image
'
flow and
replace
it by fluid at
rest.
As in the square-eddy model, unopposeà
pressures on
the
plane interface
will cause
it to
ripple
and develop Mach
waves
to effect a pressure balance.
The
pressure field, either in the simulated layer, or in the Mach
wave field is no longer sinusoidal, but is random.
If
we
make
a
Fourier
analysis,
the square
eddy solution behaves
like
a single sinusoidal Fourier
component
of this more general patte
rn
.
The Mach wave
pressure field will
n
ow
have
a broad band spectrum
in
place of
the former
single line or pure
tone.
However, the results for
mean
square pressure and noise-generating
efficiency will be
unaltered, assuming
postulated turbulence is
a
'frozen'
co
nv
ected pattern
.
The improved model still differs
cfrom a real turbulent mixing
layer in retaining
quasi-planar
interfaces. Nevertheless,
it
wou~d s~emthat
a mechanism
rather
like
the
one proposed
here
is operative in the
~ealflow
to
generate
'eddy
Mach
waves'.
Their role
is
to match
the
near field
pres
sur
es and extend them to
the radiation
field. The virtue of the model
is the conceptual
simplicity of
the
generation p
r
ocess
and
the ease with
which
predictive
formulas can
be ext
r
acted
.
COMPARISON
WITH
OT
HER M
ODELS
The Lighthill
model as extended by
Ff
owcs Williams (Ref
.2
) or by
Ri
b
n
e
r
(Ref.3)
deals
with
a
supersonic
mixi
n
g layer in
terms
o~
the
source-motion Doppler
e
f
fect
.
This
is
embodied
in a
'convection factor' that
multiplies the
int
ensity
that would
occur
for unconvected
eddy sound sources.
The
emission has
the
characte
r
of
Mach waves, with
peak
intensity
normal
to
the Mach cones
of
the
moving eddie
s.
The ed
dy
sound
sources
are identified
as perturbations of tne
Reyn
olds
stresses
or
r
ate of
momentum flow.
These
generate a near field
(
'p
se\ld.
osoun
d
'
)
a
nd.
a far field
.
The convection factor
dictates the 'eddy
Mach wave' character
of the
far field,
but
it does
not
apply
to the near
fiel
d
,
since the
moving ed
di
es emi
t
into
locally co-movi
n
g fluid.
Thus the
extended
Li
ght
hi
l
l
theory
predicts both the near field
and
the
far
field
in
terms o
f
pe
rturbati
ons of
rat
e of momentum flow in
the
~ddiestogether with
eddy
c
onvection effe
ct
s
.
An integral formalism is
us
ed
,
and it
is
as
ac
cur
ate as the
turbulence description
fed into it.
A
n
other important model
is that
of Phil
li
ps (Refs. 3,5). His eddy
sound
sources - equivalent
to Lighthill's in their
tot al emission - are
identified as products of pairs of
velocity
gradients
.
(These can be
~elatedt
o
t
he deformation of fluid elements).
The
method of solution applied to a
supersonic shear
layer leads
directly
to
~ddyMach waves as the far field;
.
'
the
near
field
is not
obtained although
in
p
r
inciple it could beo
.
' .In the
dilatation theo
ry
(Refs.
3,6) the
eddy sound sour
.
ces are
identified
as
the
volume fluctuations of
fluid
elements in response to the
near field
pressure
.
This
leads
to
an
int
egral
re
lat
i:ç.g
. t
.
he far field
pressure to
(essentially) the near field pressure .
In tl1is reppeet it
<
.
resembles the
present
model (although sharing the
ri
gor of
the
Lighthill
formalism) , but in the present model the connection is much more
direct:
a matching,
in facto
The present
model,
lik
e
the
othe
rs~
predicts
both near field
and
far field sound
f
r
om
the 'turbulence
'
flow
fie
ld
properties.
But the
turbulence
is
highly idealized, and
th
e
continu
ous shear in the mixing
layer is idealized into two
plana
r
slip
s
urfac
es
.
The greater simplici ty
appears in both the physics and mathematics of
th
e
Mach wave generàtiQn
p
rocess .
.
.,.
1. Liepmann, H. W.
Roshko, A.
2. Lighthill,
M •• J.
3. Ribner, H. S.
4. Ffowes Williams,
J.
E.
5. Phillips, O. M.
6. Ribner, H. S.
REFERENCES
Element
s
of Gasdynamies, John Wiley
&
Sons,
New York 1957, (Lib. Congress 56-9823), p. 426.
"Wright Brothers Leeture. Jet Noise" AlM
Journal
.
Vol.l, no.?, pp.1507-1517, July,
196
3
.
"The Generation of Sound by Turbulent Jets" ,
Vol.8. Advanees in Applied Meehanies,
pp.1
03
-182, Academie Press, New York (1964).
"Some Open Q.uestions on the Jet Noise Problem"
Unpublished paper (1967). Dept. of Mathematies,
lmperial University.
"On the Generation of Sound by Supersonie
Turbulent Shear L
a
yers ,
J.
Fluid Meeh. 9,
1-
2
8 (1
9
6
0
).
-"Aerodyn
a
mie Sound from Fluid Dilatations.
A Theory of the
S
ound fr
o
m Jets and Other
Flo
ws
" .
Uni v
.
of Toronto, lnst. Aerosp
i:
lCe
Studies, UTIAS Report. 86, (1
9
62).
·
Ky
0
FLUID AT REST
0h\
l'S
I~
KX
~
MIXING
~
U
m
LAYER
~
I
l}---/
I '---../
'---../
-1T
To
MAIN FLOW
~
U·
J
FIG. I MODEL SIMULATING FEATURES OF ROCKET NOISE GENERATION .
I. TURBULENT MIXING LAYER IS SIMULATED BY AN ARRAY OF SQUARE
"EDDIES" . NOTICE UNBALANCED PRESSURES ACROSS PLANE INTERFACES.
EDDY MACH WAVFS
,I"I~I~
---""'.~
Urn
MOVING RIPPLES IN STATIONARY FRAME
P2
/pë
FIG.2
MODEL SIMULATING FEATURES OF ROCKET NOISE GENERATION .
11. TRAVELLING RIPPLES DEVELOP IN INTERFACFS AND .GENERATE 'EDDY
MACH WAVES· (NOISE) ; WAVE AMPLITUDE IS SUCH AS TO ACHlEVE A
PRESSURE BALANCE ACROSS INTERFACES.
~~~I~~
R~:D
I .
nD
SUPERSONIC ZONE
FIG.3 MODEL SIMULATING FEATURES OF ROCKET NOISE
GENERATION . 111. GEOMETRY FOR ESTIMATING RATIO (NOISE
POWER
IJ
ET FLOW POWER) FOR SIMPLIFIED "ROCKET JET".
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3.
REPORT TlTLE
EDDY MACH WAVE NOISE FROM A SIMPLIFIED MODEL OF A S UPERSONIC MIXING LAYER
4·
DESCRIPTIVE NOTES
(Type ol report anct In"lualve dat ... )Scientific
Interim
5·
AUTHOR(S)
(Laat name. lirat name. In/llat)H. S. Ribner
6·
REPORT DATE
7a·TOTAL NO. OF PAGES
1
7b.NO.
6
0F REFS
October, 1969.
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Sa.
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urIAS Technical Note No.146
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13.
ABSTRACT
A simplified flow model is presented for simulating features of noise generation
by supersonic jets and rockets.
'Eddy Mach
waves' appear
as a consequence of
balancing internal and external pressures, and noise power may be estimated.
Specifically, the turbulent mixing layer of a supersonic jet is modeled as a
layer of two-dimensional square 'eddies'; this
separates
the main flow Uj from
fluid at rest and moves at an intermediate
speed.
(In an improved model the
square eddies are replaced by a turbulent flow layer constrained by plane
interfaces) • The initially plane interfaces, because of unopposed internal
pressures,
will
ripple
slightly
such that Mach
waves
arise and effect a pressure
halance. The Mach
wave
noise pattern is readily calculated as weIl as the
acoustic energy flux.
In an example simulating a round rocket jet the effective
mixing layer area is taken to be 6 H(diameters)2, the r.m.s. eddy velocity is
0.1 Uj , and Uj
=6 times external sound speed. The
efficiency
(noise power/
flow power) comes out to be about 1/3%,
which
is of the order of measured values
for rocket noise •
•
"
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14·KEY WORDS LIIiIK A
LINK. LINK C "OLIt WT "OLIt WT
1) Jet Noise
2) Rocket Noise
3)
Acoustics
4)
Aeroacoustics
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l1rIAS Technical Note No. 146
Institute for Aerospace Studies, University of T oronto
~
Eddy Mach Wave N01se from a S1mpl1f1ed Model of a Supersonic !41x1ng Layer
Ribner, H. S. 6 pages 3 figures
1. Jet Noise 2. Rocket Noise 3. Acoustics 4. Aeroacoustic.
I. .Ribner, H. S. Il. l1rIAS Technical Not. No. 146
A simplified flow model is presented" tor simulating features of noise generation by supersonic jets a..'"ld rackets. 'Eddy Mach waves I appear as a consequence of b~anc1ng 1nternal a.nd external
pressures) and noise power may be estimated. Specifically, the turbulent mixing layer of' a
supersonic jet is modeled as a layer of two-dimensional square 'eddies'; this separates the
r.:ai" flow Uj from fluid at rest and moves at an intermediate speed. (In an improved model the
squa:e eddies are replaeed by a turbulent flow 'layer constrained by plain interfaces). The
ini tially plane interfaces, becallse of unopposed interna.l pressures, will ripple slightly such
t!:at Y~ch waves arise and effect a pressure balanee . The Mach wave noise pattern is readily
ealeulated as weil as the acoustic energy flux. In an example simulating e. round 'rocket jet
the effeetive mixing layer area i. taken to be 6 7T(diameters)2, the r.m .•• eddy·velocity i.
0.1 U.i' and Uj = 6 times external sOWld speed. The efficiency (noioe power/now power) come. out to 'oe &bout 1/310, which ls of the order of mea.sured values tor rocket Doise.
Ava'jlal:ile copies of this report are limited. Return this card to UTIAS, if you reqUire a copy.
l1rIAS TEX:HNICAL NOTE NO. 146
Institutefor Aerospace Studies, University of T oronto
Eddy Mach Wave Noise from a Simplif1ed Model of a Super sonic )lixing Layer
~
Ribner.) H. S. 6 pages 3 figures
1. Jet Noise 2. Rocket Noise 3. Acoustics 4. Aeroacoustics
I. .Ribner, H. S. II. l1rIAS Technical Note No. 146
A simplified flow model is presenteà.· for simulating features of noise generation by supersonic
jets a.'"ld rackets. I Eddy Mach waves I appear as a consequence of b~ancing internal and external
pre~sures, and noise power may be estimated. Specifically, the turbulent mixing le.yer of a
supersonic jet is modeled as a layer of two-diIDensional square leddies'; thls separates the
I:lain flow Uj from fluid at rest and moves at an intermediate speed. (In an improved model ~pe
sq".l.a!"e eddies are replaced by a turbulent flow layer constrained by plain interfaces). The
ini tially plane interfaces, beca~e of unopposed internal pressures, will ripple slightly such
that 1-1ach waves arlse ani effect a pressure balance. The Mach wave noise pattern is readily
calculated as weU as the acoustic energy flux. In an example simulating a. round 'rocket Jet
the effective mixing layer area is taken to be 6 7T(diameters)2, the r.m ••• eddy·velocity i.
0.1 Uv and Uj = 6 times external sOWld speed. The efficiency (noise power/flOW power) comes
out tI:> be about 1/3'{., which is of the order of measured value. for rocket noise.
l1rIAS Technical Note No. 146
Institute for Aerospace Studies, University of T oronto
~
Eddy Mach Wave Noise from a Simpl1fied Model of a Supersonic Mixing Layer
Ribner, H. S. 6 pages 3 figures
1. Jet Noise 2. Rocket Noise 3. Acoustics 4. Aeroacoustics
I. Ribner, H. S. II. l1rIAS Technical Note No. 146
A simplified flow lOOdel is presenteà' for simulating features of noise generatian by supersanic
jets and rackets. 'Eddy Mach waves' appear as a consequence of b~lancing internal and. external
pressures, and noise power may be estimated. Specifically, the turbulent mixing layer of a supersonic jet is modeled as a layer of two-dimensional square 'eddies'; this separates the
main flow Uj from fluid at rest and moves at an intermediate speed. (In an impraved model the
square eddies are replaeed by e. turbulent flow layer constrained by plain interface.). The
ini tially plane interfaces, beca~e of unopposed intern~l pressures, will ripple slight1y such
that Mach waves arise and effect a pressure balance. The Mach wave noise pattern is readily calculated as weU as the acoustic energy flux. In an example simulat1ng a. round ':racket Jet
the effective mixing layer area is taken to be 6 7T(diameters)2, the r.m ••• eddy·velocity i.
~.l Ui' and Uj = 6 times external sOWld speed. The efficiency (noise power/flOW power) come.
out tb be about 1/3'{., which is of the order of measured value. for rocket noi.e.
Available copies of
th
is
report: are limited. Return this card to UTIAS, if you require a copy.JrIAS TEX:HNICAL NOTE NO. 146
Institute for Aerospace Studies, University of T oronto
~
Eddy Mach Wave Noise from a Simplified Model of a Supersoillc !41xing Layer
Ribner, H. S. 6 pages 3 figures
1. Jet Noise 2. Rocket Noise 3. Acoustics 4. Aeroacoustics
I. .Ribner, H. S. II. l1rIAS Technical Note No. 146
A simp1ified flow model is presented' for simulating :features of noise generation by supersarrlc
jets a."ld rockets . I Eddy Mac~ }rIaves' appear as a consequence of b~ancing internal and external
pressures, and noise power may be estimated. Specific8.lly, the turbulent mixing layer of a supersonic jet is modeled as a layer af two-dimensional square 'eddies I; this separates the min flow Uj from fluid at rest and moves at an intermediate speed. (In 8.n lmproved model the square eddies are replaced by 8. turbulent flow layer constrained by plain interfaces). The
ini tially plane interfaces, beca'.;1Se of unopposed inter~l pressures, nU ripple slightly such
that Mach waves arise ani effect a pressure balanee . The Mach wave noise pattern is readily calculated as weU as the acoustic energy flux. In an example simulating a raund 'racket ~et the effective mixing layer area is taken to be 6 7T(diameters)2, the r.m .•• eddy·velocity i .
0.1 U.i , and Uj = 6 times external sOWld .peed. The efficiency (noise power/now power) comes