tue casa day 22 november 2006 wiener-hopf solutions of aircraft engine noise models
DESCRIPTION
TUE CASA Day 22 November 2006 Wiener-Hopf Solutions of Aircraft Engine Noise Models. Ahmet Demir Generalisation and Implementation of Munt’s Model. Munt’s Model. - PowerPoint PPT PresentationTRANSCRIPT
TUE CASA Day 22 November 2006
Wiener-Hopf Solutions of Aircraft
Engine Noise Models
Ahmet Demir
Generalisation and Implementation of Munt’s Model
Munt’s Model
For over 25 years (1977-2003) there was “asleep” the very advanced but technically complicated solution by Munt for sound radiation from a straight hard-walled hollow duct with piecewise uniform mean flow.
It was proposed for TURNEX to take this as a starting point for similar, but extended and more advanced models.
New Models based on Munt Model
0000 ,c , U,M
jjjj ,c , U,M
1R
0R
0000 ,c , U,M
jjjj ,c , U,M
1R
0R
0000 ,c , U,M
jjjj ,c , U,M
1R
0R
0000 ,c , U,M
jjjj ,c , U,M 0R
Case 1 : Hollow duct
Case 1b : Lined Centerbody Case 1c : Lined Afterbody
Case 1a : Annular duct
lininglining
Coplanar Exhaust and Burried Nozzle
More advanced generalisations:
R0
R1
0000 ,c , U,M
jjjj ,c , U,M
2222 ,c , U,M
R0
R1
0000 ,c , U,M
jjjj ,c , U,M
2222 ,c , U,M
Analytical Solution
Solution is in the form of a complex Fourier integral
(where P is also defined by a complex integral) constructed by subtle complex-functional methods, variations of the Wiener-Hopf method.
Important issues, which can now be studied more exactly : - Vortex shedding from trailing edge - Kutta condition at trailing edge - Instability of the jet (vortex sheet unstable for all frequencies; finite
shear layer not)
dueurPetrzp uziimti ,,,,
Formulation of Lined afterbody
0M)(1
1
2
012
2
21
21
zi
r
m
rrr
rr
0MC)(1
2
2
12122
2
22
22
zi
r
m
rrr
rr
convected wave equations
0000 ,c , U,M
jjjj ,c , U,M
1R
0R
1exp,exp,
1exp,,,,
2
1
rhtiimzrtiimzr
rtiimzrtzr
i
1rhpC , , MD
1rp , , M
212211
110
v
v
zip
zip
scattered field:
mnmnmnmnmmnmnm mmYhJJhY 1
'''' 0 ,
mn
mn
tiimzrtzr ii exp,,,,
rYhJrJhYr mnmmnmmnmmnmmn ''
zirzr mnmni exp,
is axial wave number, is the root of equation
where:
Incident wave (hard-walled mode):
0j1j010j100001 /D , c/cC , c/UM , c/UM , R/R h
Dimensionless parameters:
0M
00,1
01 zz
zi
zz
r
0M
00,1
12 zz
zi
zz
r
0z , ,1M,1,1MD 10211
zz
izzz
i i
boundaryconditionsat hub andr = 1
continuity of pressure at vortex sheet
continuity of displacement
soft wall
00,2
zzhr
,
0,,,, 2
2
12
zzhzhz
MiZi
Dzhzh
r ii , 1
0000 ,c , U,M
jjjj ,c , U,M
1R
0R
hard wall
Kutta condition and instability: trailing edge behaviour, vortex shedding, excitation of instability
singular, stable
smooth, unstable
singular, unstable
Fourier Integral Representation of Velocity Potentials
duerHuAzr uzim
0
)2(1 )(
2,
duerYuCrJuBzr uzimm
112 )()(2
,
0Im , M1)( 022
00 uuu 0Im , M1C)( 122
1211 uuu
0
)'2(0
0M1)(
mH
uFuiuA
1
'1
'1 ,,
1,)(
mmYuZJuZ
uFuMuZiuB
mm
m
JYY 1
uBuZ
uZuC
m
m
,
,)(
YJ
Simultaneous Wiener-Hopf Equations (results from B.C. r=1)
1'
1'
1
31
2
1111 ,,
)1(21)()(
mmYuZJuZhZ
uFuMD
uZ
MhDuuNu
mmmn
mnmn JY
1
)(
)()(
uK
uKuK
mn
mnmn
mn
mnmn
mm
u
MDuG
uZ
MhDu
YuZJuZ
uMDiuKuF
mm
)1(1)(
1)(
,,
)1(22
111
1'
1'
1
1
11
1
JY
)(
)()(
uN
uNuN
note : B.C. at hub yields relation between B(u) and C(u).
Splitting first Equation: weak factorization in lined duct wave number
1
2
11
2
111
1
2
11
1'
1'
1
311
11)(
1
1
,,
)1(2)(
p mp
mp
mnmn
mnmn
mn
mnmn
p mp
mp
mnmn
mnmn
mm
u
a
NuZ
MhD
uZ
MhDu
uN
u
a
NuZ
MhD
uNYuZJuZhZ
uFuMD
uN
u
mm
JY1
'1
'1
'1
3
1
,,
)1(2
mpmm ummmpmp
mpmpmp
YuZJuZN
FM
hZ
Da
JY
1
note : no left running contribution in z>0
mp
Splitting second Equation: essentially with the same way:weak factorization in lined duct wave number
mp
1
2
111
1'
1'
1
1
1
)1(1)(
1)(
,,
)1(2
p mp
mp
mn
mnmn
mn
mnmn
mm
p mp
mp
u
buK
u
MDuGuK
uZ
MhDu
YuZJuZ
uKuMDi
u
buKuF
mm
11
1
JY
mnmp
mnmnmp
ummmp
mpmpmp Z
MhD
YuZJuZ
KMDib
mpmm
2
111'
1'
1'
1
1 1)(
,,
)1(2
JY
1
note : no right running soft wall modes from z<0.
Solution to second Equation: for far field we need only F+
mpp mp
mp
u
uu
u
buKuF 0
1 0
mnmnmr
mnmn
p mpmr
mp
ummmrmrmr
mrmr
NZ
MhD
a
YuZJuZNKMD
bimrmm
2
11
1
'
1'
1'
1
1
1
,,)1(2
1
JY1
mpmr
mr
p mp
mp
ummmr
mrmrmrmr
u
u
b
YuZJuZMD
NKhZa
mrmm
0
1 0
'
1'
1'
31
1 ,,)1(2
1
JY1
Coefficients amp and bmp are determined by the following infinite linear system
Complex Contour Integral
Careful management & bookkeeping of poles and other singularities is necessary for correct answer
Total field (double integral: takes more time)
iZ 2
w = 15, Mode(4,1)
w = 25, Mode(4,1)
975.0943.053.03.0667.0 1110 C DMMh
Lined Centerbody
Far Field
Far field pressure for ωr → ∞.
imtimiM
MMRi
R
Dzrp p
21
1
sin1cosexp
)(,
20
2/12200
'sin
')'1(
0)'2(
2
uH
uFMuD
m
p
0directivity
2
0
0
2/1220
M1
MsinM1cos'
u
Numerical Examples
Case 1
Approach Mode(0,1)
without mean flow with mean flow
0000 ,c , U,M
jjjj ,c , U,M 0R
Approach Mode(17,1)without mean flow with mean flow
Cutback Mode(23,1)without mean flow with mean flow
Case 1a : Effect of hub (Kutta on)
Approach Mode(17,1)Approach Mode(0,1)
0000 ,c , U,M
jjjj ,c , U,M
1R
0R
Cutback Mode(23,1)Cutback Mode(0,1)
Case 1b,1c : Effect of lining and semi-lining (Kutta on)
Approach Mode(9,1)Approach Mode(0,1)
0000 ,c , U,M
jjjj ,c , U,M
1R
0R
0000 ,c , U,M
jjjj ,c , U,M
1R
0R
Approach and Cutback mean : different flows inside and outside the duct (specific parameters for the project)
Cutback Mode(23,1)Cutback Mode(0,1)
Comparison with numerical models
Case 1: Flesturn (METU)
and Actran (FFT) results
Approach parameters
Modes (0,1),(10,1),(19,1)0000 ,c , U,M
jjjj ,c , U,M 0R
Zero flow Mode(0,1) Zero flow Mode(19,1)
Case 1a : METU, NLR and FFT results
Approach Mode(17,1)
0000 ,c , U,M
jjjj ,c , U,M
1R
0R
SPL (dB)
0
30
60
90
120
0 20 40 60 80 100
analytic (TUE)coarse gridmedium gridfine grid
SPL (dB)
0
30
60
90
120
0 20 40 60 80 100
analytic (TUE)coarse gridmedium gridfine grid
Cutback Mode(23,1)Cutback Mode(0,1)
Case 1c : METU and FFT results (liner impedance Z = 2 - i)
0000 ,c , U,M
jjjj ,c , U,M
1R
0R
FFT-Actran vs TUE results
Coplanar Exhaust : TUE and METU results R0
R1
0000 ,c , U,M
jjjj ,c , U,M
2222 ,c , U,M
Zero flow Mode(2,1) Zero flow Mode(10,1)
Approach Mode(10,1)
R0
R1
0000 ,c , U,M
jjjj ,c , U,M
2222 ,c , U,M
Conclusions A series of non-trivial extensions of the classical Munt problem have
been successfully solved and implemented.
Comparison with fully numerical solutions have been very favourable and encourages their trustful use in industrial applications.
Case 1b+1c (lined centerbody+lined afterbody) has been published: Sound Radiation from an Annular Duct with Jet Flow and a Lined Center Body, A. Demir and S.W. Rienstra, AIAA 2006-2718, 12th AIAA/CEAS Aeroacoustics Conference, 8-10 May 2006, Cambridge, MA, USA
First results show that lining of centerbody reduces sound field only in crosswise direction.
Effect of instability is for these high frequencies acoustically small in all cases considered