application of modern tools for the thermo-acoustic study of annular combustion chambers franck...
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Application of modern tools for the thermo-acoustic study of
annular combustion chambers
Franck NicoudUniversity Montpellier II – I3M CNRS UMR 5149
and
CERFACS
November, 2010 VKI Lecture 2
Introduction
A swirler (one per sector)
November, 2010 VKI Lecture 3
Introduction
One swirler per sector
10-24 sectors
November, 2010 VKI Lecture 4
Y. Sommerer & M. BoileauCERFACS
Introduction
November, 2010 VKI Lecture 5
Introduction
November, 2010 VKI Lecture 6
SOME KEY INGREDIENTS
• Flow physics– turbulence, partial mixing, chemistry, two-phase flow , combustion
modeling, heat loss, wall treatment, radiative transfer, …
• Acoustics– complex impedance, mean flow effects, acoustics/flame coupling,
non-linearity, limit cycle, non-normality, mode interactions, …
• Numerics– Low dispersive – low dissipative schemes, non linear stability,
scalability, non-linear eigen value problems, …
November, 2010 VKI Lecture 7
PARALLEL COMPUTING
• www.top500.org – june 2010# Site Computer
1 Oak Ridge National LaboratoryUSA
Cray XT5-HE Opteron Six Core 2.6 GHz
2 National Supercomputing Centre in Shenzhen (NSCS)China
Dawning TC3600 Blade, Intel X5650, NVidia Tesla C2050 GPU
3 DOE/NNSA/LANLUSA
BladeCenter QS22/LS21 Cluster, PowerXCell 8i 3.2 Ghz / Opteron DC 1.8 GHz, Voltaire Infiniband
4 National Institute for Computational SciencesUSA
Cray XT5-HE Opteron Six Core 2.6 GHz
5 Forschungszentrum Juelich (FZJ)Germany
Blue Gene/P Solution
6 NASA/Ames Research Center/NASUSA
SGI Altix ICE 8200EX/8400EX, Xeon HT QC 3.0/Xeon Westmere 2.93 Ghz, Infiniband
7 National SuperComputer Center in Tianjin/NUDTChina
NUDT TH-1 Cluster, Xeon E5540/E5450, ATI Radeon HD 4870 2, Infiniband
8 DOE/NNSA/LLNLUSA
eServer Blue Gene Solution
9 Argonne National LaboratoryUSA
Blue Gene/P Solution
10 Sandia National LaboratoriesUSA
Cray XT5-HE Opteron Six Core 2.6 GHz
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00 p
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November, 2010 VKI Lecture 8
PARALLEL COMPUTING
• www.top500.org – june 2007 (3 years ago …) # Site Computer
1DOE/NNSA/LLNLUnited States
BlueGene/L - eServer Blue Gene SolutionIBM
2Oak Ridge National LaboratoryUnited States
Jaguar - Cray XT4/XT3Cray Inc.
3NNSA/Sandia National LaboratoriesUnited States
Red Storm - Sandia/ Cray Red Storm,Cray Inc.
4IBM Thomas J. Watson Research CenterUnited States
BGW - eServer Blue Gene SolutionIBM
5Stony Brook/BNL, New York Center for Computional United States
New York Blue - eServer Blue Gene SolutionIBM
6DOE/NNSA/LLNLUnited States
ASC Purple - eServer pSeries p5 575 1.9 GHzIBM
7Rensselaer Polytechnic Institute, Computional Center United States
eServer Blue Gene SolutionIBM
8NCSAUnited States
Abe - PowerEdge 1955, 2.33 GHz, InfinibandDell
9Barcelona Supercomputing CenterSpain
MareNostrum - BladeCenter JS21 Cluster,IBM
10Leibniz RechenzentrumGermany
HLRB-II - Altix 4700 1.6 GHzSGI
10 0
00 p
roce
ssor
s or
mor
e
(
fact
or
7)56
Tflo
ps o
r m
ore
(
fact
or
8)
November, 2010 VKI Lecture 9
PARALLEL COMPUTING
• Large scale unsteady computations require huge computing resources, an efficient codes …
processors
Spe
ed u
p
November, 2010 VKI Lecture 10
PARALLEL COMPUTING
November, 2010 VKI Lecture 11
Thermo-acoustic instabilities
The Berkeley backward facing step experiment.The Berkeley backward facing step experiment.
Premixed gas
November, 2010 VKI Lecture 12
Thermo-acoustic instabilities
• Self-sustained oscillations arising from the coupling between a source of heat and the acoustic waves of the system
• Known since a very long time (Rijke, 1859; Rayleigh, 1878)
• Not fully understood yet …
• but surely not desirable …
November, 2010 VKI Lecture 13
Better avoid them …
LPP SNECMA
AIR
FUEL
LPP injector(SNECMA)
November, 2010 VKI Lecture 14
Flame/acoustics coupling
COMBUSTION
ACOUSTICS
Modeling problem Wave equation
Rayleigh criterion:Flame/acoustics coupling promotes instability if pressure and heat release fluctuations are in phase
November, 2010 VKI Lecture 15
A tractable 1D problem
BURNT GASIMPOSEDVELOCITY
IMPOSEDPRESSURE
FLAME
n , t
FRESH GAS
0),0(' tu 0),(' tLp
0 LL/2
1T 12 4TT
Kaufmann, Nicoud & Poinsot, Comb. Flame, 2002
lag time:
indexn interactio :n releaseheat unsteady for the model
2),2/('
1),(' 0
n
LxtLun
ptxq
November, 2010 VKI Lecture 16
Equations
0),0(' tu 0),(' tLp
0 L
1T 12 4TT
0''
:2
0
2
2212
2
x
pc
t
p
Lx
0''
:2
2
2222
2
x
pc
t
p
LxL
CLASSICAL ACOUSTICS2 wave amplitudes
CLASSICAL ACOUSTICS2 wave amplitudes
RELATIONS JUMP TWO
,2/''and0' 2/2/
2/2/
tLunup LL
LL
November, 2010 VKI Lecture 17
Dispersion relation
• Solve the 4x4 homogeneous linear system to find out the 4 wave amplitudes
• Consider Fourier modes
• Condition for non-trivial (zero) solutions to exist
tjexptxp )(ˆ),('
03
1
4
1
4
3
4cos
4cos
1
2
1
j
j
ne
ne
c
L
c
L
Coupled modes
mode amplified :0
mode damped :0
Uncoupled modes
November, 2010 VKI Lecture 18
Stability of the coupled modes• Eigen frequencies
• Steady flame n=0:
• Asymptotic development for n<<1:
03
1
4
1
4
3
4cos
1
2
j
j
ne
ne
c
L
,...2,1,0,23
2arccos
4 10,
mm
L
cm
)(sincos2/sin9
4
shifpulsationComplex
0,0,10,
10, noj
cLL
cn
t
mmm
mm
Kaufmann, Nicoud & Poinsot, Comb. Flame, 2002
November, 2010 VKI Lecture 19
Time lag effect
• The imaginary part of the frequency is
• Steady flame modes such that
• The unsteady HR destabilizes the flame if
02/sin 10, cLm
0,0,
0,0, 20]2[00sin m
mmm T
T
0 2/0,mT 2/3 0,mT 2/5 0,mT0,mT 0,2 mT 0,3 mT
unstableunstable unstable unstable
10,
0,1
2/sin9
sin4
cLL
cn
m
m
November, 2010 VKI Lecture 20
Time lag effect
• The imaginary part of the frequency is
• Steady flame modes such that
• The unsteady HR destabilizes the flame if
10,
0,1
2/sin9
sin4
cLL
cn
m
m
02/sin 10, cLm
0 2/0,mT 2/3 0,mT 2/5 0,mT0,mT 0,2 mT 0,3 mT
unstable unstable unstable
0,0,0,
0,0, 2]2[20sin mm
mmm TT
T
November, 2010 VKI Lecture 21
Numerical example
Steady flame
STA
BL
EU
NS
TAB
LE
Real frequency (Hz)
Imag
inar
y fr
eque
ncy
(Hz)
Unteady flamen=0.01t=0.1 ms
STA
BL
EU
NS
TAB
LE
Real frequency (Hz)
Imag
inar
y fr
eque
ncy
(Hz)m 5.0
K 3001
L
TUncoupled modes
November, 2010 VKI Lecture 22
OUTLINE
1. Computing the whole flow
2. Computing the fluctuations
3. Boundary conditions
4. Analysis of an annular combustor
November, 2010 VKI Lecture 23
OUTLINE
1. Computing the whole flow
2. Computing the fluctuations
3. Boundary conditions
4. Analysis of an annular combustor
November, 2010 VKI Lecture 24
BASIC EQUATIONS reacting, multi-species gaseous mixture
November, 2010 VKI Lecture 25
BASIC EQUATIONS energy / enthalpy forms
Sensible enthalpy of species k
Specific enthalpy of species k
Sensible enthalpy of the mixture
Specific enthalpy of the mixture
Total enthalpy of the mixture
Total non chemical enthalpy of the mixture
E = H – p/r Total non chemical energy of the mixture
November, 2010 VKI Lecture 26
BASIC EQUATIONS Diffusion velocity / mass flux
Practical model
Satisfies mass conservation
Exact form
November, 2010 VKI Lecture 27
BASIC EQUATIONS Stress and heat flux
PrpC
November, 2010 VKI Lecture 28
Turbulence 1. Turbulence is contained in the NS
equations
2. The flow regime (laminar vs turbulent) depends on the Reynolds number :
Re Ud
Velocity Length scale
viscosity
Re
laminar turbulent
November, 2010 VKI Lecture 29
RANS – LES - DNS
time
Str
eam
wis
e ve
loci
ty
RANS
DNS LES
November, 2010 VKI Lecture 30
About the RANS approach
• Averages are not always enough (instabilities, growth rate, vortex shedding)
• Averages are even not always meaningful
T1 T2>T1
T
time
Oscillating flameT2
T1
Prob(T=Tmean)=0 !!
The basic idea of LES
k
)(kE
ck
Modeled scalesResolved scales
November, 2010 VKI Lecture 31
November, 2010 VKI Lecture 32
LES equations
• Assumes small commutation errors
• Filtered version of the flow equations :
November, 2010 VKI Lecture 33
Laminar contributions
• Assumes negligible cross correlation between gradient and diffusion coefficients:
November, 2010 VKI Lecture 34
Sub-grid scale contributions
• Sub-grid scale stress tensor to be modeled
• Sub-grid scale mass flux to be modeled
• Sub-grid scale heat flux to be modeled
jijisgsij uuuu ~~
jkjksgs
jk uYuYJ ~~,
jjsgsj uEuEq ~~
November, 2010 VKI Lecture 35
The Smagorinsky model
• From dimensional consideration, simply assume:
• The Smagorinsky constant is fixed so that the proper dissipation rate is produced, Cs = 0.18
ijijssgs SSC~~
22
i
j
j
iijijkkijsgsij
sgskk
sgsij x
u
x
uSSS
~~
2
1~ with ,
~
3
1~2
3
1
November, 2010 VKI Lecture 36
The Smagorinsky model• The sgs dissipation is always
positive
• Very simple to implement, no extra CPU time
• Any mean gradient induces sub-grid scale activity and dissipation, even in 2D !!
• Strong limitation due to its lack of universality. Eg.: in a channel flow, Cs=0.1 should be used
ijijsgsijsgsijsgs SSS
~~2
~
Solid wall
0 and )( because
0but 0
12
SyUU
WV sgs
No laminar-to-turbulent transition possible
November, 2010 VKI Lecture 37
The Dynamic procedure (constant r)• By performing , the following sgs contribution appears
• Let’s apply another filter to these equations
• By performing , one obtains the following equations
• From A and B one obtains
jijisgs
ij uuuuT
jijisgsij uuuu
NS
NS
jijisgsij uuuu
j
sgsijij
ij
jii
xx
P
x
uu
t
u
j
sgsijij
ij
jii
xx
P
x
uu
t
u
j
sgsijij
ij
jii
x
T
x
P
x
uu
t
u
A
B
jijisgsij
sgsij uuuuT
November, 2010 VKI Lecture 38
The dynamic Smagorinsky model• Assume the Smagorinsky model is applied twice
• Assume the same constant can be used and write the Germano identity
ijijijsijsgskk
sgsij SSSC 22
3
1 2
ijijijsijsgs
kksgs
ij SSSCTT 223
1 2
jijisgsij
sgsij uuuuT
jijiijsgskkijijijsij
sgskkijijijs uuuuSSSCTSSSC
3
122
3
122
22
ijijs LMC 2 Cs dynamically obtained from the solution itself
November, 2010 VKI Lecture 39
The dynamic procedure
The dynamic procedure can be applied locally :
• the constant depends on both space and time
• good for complex geometries,
• but requires clipping (no warranty that the constant is positive)
scales resolved thefrom computed becan
model SGS on the depends
2
ij
ij
ijij
ijij
L
M
MM
MLC
How often should we accept to clip ?
November, 2010 40 VKI Lecture
1. Example of a simple turbulent channel flow
2. Not very satisfactory, and may degrade the resultsY+
% c
lipp
ing
Y+
U+
Local Dynamic
Smagorinsky
Plane-wise Dynamic
Smagorinsky
DNS
The global dynamic procedure
The dynamic procedure can also be applied globally:
• The constant depends only on time
• no clipping required,
• just as good as the static model it is based on
• Requires an improved time scale estimate
November, 2010 41 VKI Lecture
scales resolved thefrom computed becan
model SGS on the depends
2
ij
ij
ijij
ijij
L
M
MM
MLC
Sub-grid scale model
1. Practically, eddy-viscosity models are often preferred
2. The gold standard today is the Dynamic Smagorinsky model
3. Looking for an improved model for the time scale
November, 2010 42 VKI Lecture
122 scale time Csgs
ijijSS2:ratestrain Dynamically Computed
From the grid or filter
width
Null for isotropicNull for axi-symmetic flows
Null for 2D or 2C flows Null only if gij = 0
Description of the s - model
• Eddy-viscosity based: • Start to compute the singular values of the velocity gradient tensor
(neither difficult nor expensive)•
21
322131scale time
ANDnear-wall behavioris O(y3) !!
12 scale time Csgs
November, 2010 43 VKI Lecture
November, 2010 VKI Lecture 44
Sub-grid scale contributions• Sub-grid scale stress tensor
• Sub-grid scale mass flux of species k and heat flux
• In practice, constant SGS Schmidt and Prandtl numbers
model based ~~sgsjiji
sgsij uuuu
jkjksgs
jk uYuYJ ~~,
jjsgsj uEuEq ~~
5.0Pr;Pr
7.0; sgssgs
psgssgs
sgsksgs
k
sgssgsk
CSc
ScD
November, 2010 VKI Lecture 45
Sub-grid scale heat release• The chemical source terms are highly non-linear (Arrhenius type of
terms)
• The flame thickness is usually very small (0.1 - 1 mm), smaller than the typical grid size
Poinsot & Veynante, 2001
November, 2010 VKI Lecture 46
The G-equation approach• The flame is identified as a given surface of a G field
• The G-field is smooth and computed from
• “Universal “ turbulent flame speed model not available …
Poinsot & Veynante, 2001
November, 2010 VKI Lecture 47
The thickened flame approach• From laminar premixed flames theory:
• Multiplying a and dividing A by the same thickening factor F
Poinsot & Veynante, 2001
November, 2010 VKI Lecture 48
The thickened flame approach• The thickened flame propagates at the proper laminar speed but it is
less wrinkled than the original flame:
Total reaction rate R1 Total reaction rate R2
• This leads to a decrease of the total consumption: 1
121 R
E
RRR
November, 2010 VKI Lecture 49
The thickened flame approach• An efficiency function is used to represent the sub-grid scale
wrinkling of the thickened flame
• This leads to a thickened flame (resolvable) with increased velocity (SGS wrinkling) with the proper total rate of consumption
• The efficiency function is a function of characteristic velocity and length scales ratios
g wrincklinSGS thickening
//:constant tialPreexponen
:yDiffusivit
FEAFAA
EFaFaa
00LL
sgs
FS
u
November, 2010 VKI Lecture 50
The thickened flame approach• Advantages
1. finite rate chemistry (ignition / extinction)2. fully resolved flame front avoiding numerical problems3. easily implemented and validated4. degenerates towards DNS: does laminar flames
• But the mixing process is not computed accurately outside the reaction zone
1. Extension required for diffusion or partially premixed flames
2. Introduction of a sensor to detect the flame zone and switch the F and E terms off in the non-reacting zones
November, 2010 VKI Lecture 51
• In the near wall region, the total shear stress is constant. Thus the proper velocity and length scales are based on the wall shear stress tw:
• In the case of attached boundary layers, there is an inertial zone where the following universal velocity law is followed
About solid walls
ulu w
25 ,constant" Universal" :
0.4 constant,Karman Von :
,,ln1
.CC
yuy
u
uuCyu
y
u
November, 2010 VKI Lecture 52
• A specific wall treatment is required to avoid huge mesh refinement or large errors,
• Use a coarse grid and the log law to impose the proper fluxes at the wall
Wall modeling
u
vt12
modelt32model
yu
Exact velocity gradient at wall
Velocity gradient at wall assessed from a coarse grid
November, 2010 VKI Lecture 53
• Close to solid walls, the largest scales are small …
About solid walls
Boundary layer along the x-direction: Vorticity wx
- steep velocity profile, Lt ~ ky
- Resolution requirement:Dy+ = O(1), Dz+ and Dx+ = O(10) !!
- Number of grid points: O(Rt2) for wall resolved LES
z
y
x
u
• Not even the most energetic scales are resolved when the first
off-wall point is in the log layer
• No reliable model available yet
k
)(kEModeled scalesResolved scales
ck
November, 2010 VKI Lecture 54
Wall modeling in LES
November, 2010 VKI Lecture 55
OUTLINE
1. Computing the whole flow
2. Computing the fluctuations
3. Boundary conditions
4. Analysis of an annular combustor
November, 2010 VKI Lecture 56
Considering only perturbations
November, 2010 VKI Lecture 57
Linearized Euler Equations
assume homogeneous mixture neglect viscosity
decompose each variable into its mean and fluctuation
assume small amplitude fluctuations
0
00
0
1
0
1
;1
ln,,,;1
pc
c
pCsTpf
f
fv
u
),()(),( 10 tfftf xxx
November, 2010 VKI Lecture 58
Linearized Euler Equations
• the unknown are the small amplitude fluctuations,
• the mean flow quantities must be provided
• requires a model for the heat release fluctuation q1
• contain all what is needed, and more …: acoustics + vorticity + entropy
November, 2010 VKI Lecture 59
Zero Mach number assumption
• No mean flow or “Zero-Mach number” assumption
• Probably well justified below 0.01
pCsTpf
f
ftfftf v ln,,,;1);,()(),(
0
110 xxx
0
00
0
110 ;1);,()(),(
p
cc
tt u
xuxuxu
s thicknesflame:th wavelengacoustic: fa LL
November, 2010 VKI Lecture 60
Linear equations
0:Mass 01101
uudivt
110011
0:Energy qpTt
TCv
uu
11
0:Momentum pt
u
0
1
0
1
0
1:StateT
T
p
p
- The unknowns are the fluctuating quantities
- The mean density, temperature, … fields must be provided
- A model for the unsteady HR q1 is required to close the system
1111 ,,, pTu
November, 2010 VKI Lecture 61
Flame Transfer Functions
• Relate the global HR to upstream velocity fluctuations
• General form in the frequency space
• n-t model (Crocco, 1956), low-pass filter/saturation (Dowling, 1997), laminar conic or V-flames (Schuller et al, 2003), entropy waves (Dowling, 1995; Polifke, 2001), …
• Justified for acoustically compact flames
),(ˆ)()(ˆ refuFQ x
dtqtQ ),()( 11 x
November, 2010 VKI Lecture 62
Local FTF model
• Flame not necessarily compact• Local FTF model
• The scalar fields must be defined in order to match the actual flame response
• LES is the most appropriate tool assessing these fields
:,
),(ˆ),(
),(ˆ
bulk
refref),(
mean
ll
jl
n
Uen
q
ql
nxux
x x
Two scalar fields
VKI Lecture63
November, 2010
ACOUSTIC VELOCITY
AT THE REFERENCEPOSITION
FLUCTUATING HEAT RELEASE
+ACOUSTIC WAVE
refref
),(
),(ˆ),(ˆ
),(nxu
xx x
Tj
llen
Giauque et al., AIAA paper 2008-2943
Local FTF model
November, 2010 VKI Lecture 64
Back to the linear equations
• Let us suppose that we have a “reasonable” model for the flame response
• The set of linear equations still needs to be solved
0:Mass 01101
uudivt
110011
0:Energy qpTt
TCv
uu
11
0:Momentum pt
u0
1
0
1
0
1:StateT
T
p
p
November, 2010 VKI Lecture 65
Time domain integration
• Use a finite element mesh of the geometry
• Prescribe boundary conditions
• Initialize with random fields
• Compute its evolution over time …
• This is the usual approach in LES/CFD !
November, 2010 VKI Lecture 66
A simple annular combustor (TUM)
Pankiewitz and Sattelmayer, J. Eng. Gas Turbines and Power, 2003
Unsteady flame modelwith characteristic time delay t
November, 2010 VKI Lecture 67
Example of time domain integration
Pankiewitz and Sattelmayer, J. Eng. Gas Turbines and Power, 2003
TIME DELAY LEADS TOSTABLE CONDITIONS
TIME DELAY LEADS TOUNSTABLE
CONDITIONS
ORGANIZEDACOUSTIC
FIELD
November, 2010 VKI Lecture 68
The Helmholtz equation
• Since ‘periodic’ fluctuations are expected, let’s work in the frequency space
• From the set of linear equations for r1, u1, p1, T1 , the following wave equation can be derived
qjppp ˆ1ˆˆ1 2
00
tj
tjtj
eqtq
eteptp
xx
xuxuxx
ˆ,
ˆ, ˆ,
1
11
November, 2010 VKI Lecture 69
3D acoustic codes• Let us first consider the simple ‘steady flame’ case
• With simple boundary conditions
• Use the Finite Element framework to handle complex geometries
0ˆˆ1 2
00
ppp
0ˆˆor0ˆ 0 nnu pp
November, 2010 VKI Lecture 70
Discrete problem• If m is the number of nodes in the mesh, the unknown is now
• Applying the FE method, one obtains
02 PAP
Tmppp ˆ,...,ˆ,ˆ 21P
00
1:of versiondiscrete
p
LinearEigenvalue
Problemof size N
matrix square:A
November, 2010 VKI Lecture 71
Solving the eigenvalue problem
• The QR algorithm is the method of choice for small/medium scale problems Shur decomposition: AQ=QT, Q unitary, T upper triangular
• Krylov-based algorithms are more appropriate when only a few modes needs to be computed
Partial Shur decomposition: AQn=QnHn+En with n << m
• A possible choice: the Arnoldi method implemented in the P-ARPACK library (Lehoucq et al., 1996)
November, 2010 VKI Lecture 72
Solving the eigenvalue problem
November, 2010 VKI Lecture 73
Computing the TUM annular combustor
• FE mesh of the plenum + 12 injectors + swirlers + combustor + 12 nozzles
• Mean temperature field prescribed from experimental observations
• Experimentally, the first 2 modes are :– 150 Hz (1L)– 300 Hz (1C plenum)
PLENUM
COMBUSTOR
SWIRLED INJECTORS
November, 2010 VKI Lecture 74
TUM combustor: first seven modes
f (Hz) type
143 1L
286 1C plenum
503 2C plenum
594 2L
713 3C plenum
754 1C combustor
769 3L
November, 2010 VKI Lecture 75
An industrial gas turbine burner
• Industrial burner (Siemens) mounted on a square cross section combustion chamber
• Studied experimentally (Schildmacher et al., 2000), by LES (Selle et al., 2004), and acoustically (Selle et al., 2005)
November, 2010 VKI Lecture 76
Instability in the LES
• From the LES, an instability develops at 1198 Hz
November, 2010 VKI Lecture 77
Acoustic modes
f (Hz) type
159 1L
750 2L
1192 1L1T
1192 1L1T’
1350 3L
1448 2L1T
1448 2L1T’
November, 2010 VKI Lecture 78
Turning mode
• The turning mode observed in LES can be recovered by adding the two 1192 Hz modes with a 90° phase shift
LES SOLVER: 1198 Hz ACOUSTIC SOLVER: 1192 Hz
PRESSUREFLUCTUATIONSFOR 8 PHASES
Selle et al., 2005
November, 2010 VKI Lecture 79
Realistic boundary conditions• Complex, reduced boundary impedance
• Reflection coefficient
• Using the momentum equation, the most general BC is
nu
ˆ
ˆ
c
pZ
1
1
Z
Z
A
AR
out
in
ninAoutA
0ˆˆ pcZ
jp
n
0ˆ
0ˆ0 :..
nuZ
pZge
November, 2010 VKI Lecture 80
Discrete problem with realistic BCs
• In general, the reduced impedance depends on w and the discrete EV problem becomes non-linear:
0TermsBoundary 2
ˆ)(
ˆ
PAP
n
p
cZ
jp
02 CPBPAP matrices square:,, CBA
QuadraticEigenvalue
Problemof size N
parameters,,;1
)(
1210
21
0
CCZC
CZZ
• Assuming
November, 2010 VKI Lecture 81
From quadratic to linear EVP• Given a quadratic EVP of size N:
• Add the variable:
• Rewrite:
• Obtain an equivalent Linear EVP of size 2N and use your favorite method !!
PR
00
0
R
P
C0
0I
R
P
BA
I0
CRBRAP
IPIR
02 CPBPAP
November, 2010 VKI Lecture 82
Academic validation
1T 12 4TT
0Z
m 5.0
ACOUSTIC SOLVER
EXACT
Z
UN
STA
BLE
STA
BLE
jZ 2/1
UN
STA
BLE
STA
BLE
UN
STA
BLE
STA
BLE
jZ 2/1
November, 2010 VKI Lecture 83
Multiperforated liners
Multiperforated plate(????)
Solid plate(Neumann)
Dilution hole(resolved)
Example of a TURBOMECA burner
November, 2010 VKI Lecture 84
Multiperforated liners• Designed for cooling purpose …
• … but has also an acoustic effect.
Cold gas(casing)
Burnt gas(combustion chamber)
November, 2010 85
Multiperforated liners400 Hz 250 Hz
Abs
orpt
ion
coef
ficie
nt
November, 2010 86VKI Lecture
• The Rayleigh conductivity (Howe 1979)
• Under the M=0 assumption:
U
aSt
(impedance-like condition)
Multiperforated liners
November, 2010 VKI Lecture 87
Academic validation
Hz 97534 if Hz 18382 if
November, 2010 VKI Lecture 88
Question• There are many modes in the low-frequency regime
• They can be predicted in complex geometries
• Boundary conditions and multiperforated liners have first order effect and they can be accounted for properly
• All these modes are potentially dangerous
Which of these modes are made unstable by the flame ?
November, 2010 VKI Lecture 89
Accounting for the unsteady flame• Need to solve the thermo-acoustic problem
• In discrete form
qjppp ˆ1ˆˆ1 2
00
model" local" ˆ,
1ˆ1 :e.g.
refref
,
bulk0
meanFTFpen
Uρ
qγ- qγjω lτj
lref,x
nxx
x
PDCPBPAP )(2 matrices square :,,, DCBA
Non-LinearEigenvalue
Problemof size N
November, 2010 VKI Lecture 90
Iterative method1. Solve the Quadratic EVP
2. At iteration k, solve the Quadratic EVP
3. Iterate until convergence
is solution of the thermo-acoustic problem
0)( 21 CPBPPDA kkk
0200 CPBPAP
tol1 kk
P,k
November, 2010 VKI Lecture 91
Comparison with analytic resultsIN
LE
T
OU
TL
ET
n=5 , t=0.1 ms
exact modes
Iteration 0
Iteration 1
Iteration 2
Iteration 3
November, 2010 VKI Lecture 92
About the iterative method
• No general prove of convergence can be given except for academic cases
• If it converges, the procedure gives the exact solution of the discrete thermo-acoustic problem
• The number of iterations must be kept small for efficiency (one Quadratic EVP at each step and for each mode)
• Following our experience, the method does converge in a few iterations … in most cases !!
November, 2010 VKI Lecture 93
OUTLINE
1. Computing the whole flow
2. Computing the fluctuations
3. Boundary conditions
4. Analysis of an annular combustor
November, 2010 VKI Lecture 94
BC essential for thermo-acoustics
u’=0p’=0
Acoustic analysis of a Turbomeca combustor includingthe swirler, the casing and the combustion chamber
C. Sensiau (CERFACS/UM2) – AVSP code
LESor
Helmholtz solver
Boundary Conditions
November, 2010 95VKI Lecture
Acoustic boundary conditions
•Assumption of quasi-steady flow (low frequency)
•Theories (e.g.: Marble & Candle, 1977; Cumpsty & Marble, 1977; Stow et al., 2002; …)
•Conservation of Total temperature, Mass flow, Entropy fluctuations
M
2
M
1
Nozzle Inlet Nozzle Outlet
Analytical approach
November, 2010 96VKI Lecture
Mass
Momentum
Energy
1 2
Analytical approach
November, 2010 97VKI Lecture
Analytical approach
Compact systemsEntropy wave
Acoustic wave
Acoustic wave
November, 2010 98VKI Lecture
Example: Compact nozzle
1. Compact choked nozzle:
2. Compact unchoked nozzle:
2/11
2/11
1
1
M
M
2/112/111
2/112/111221
2121
221
2121
MMMMM
MMMMM
1M 2M
November, 2010 99VKI Lecture
Non compact elements
The proper equations in the acoustic element are the quasi 1D LEE:
1M 2M
Due to compressor or turbine
November, 2010 100VKI Lecture
Principle of the method
1. The boundary condition is well known at xout (e.g.: p’=0)
2. Impose a non zero incoming wave at xin
3. Solve the LEE in the frequency space
4. Compute the outgoing wave at xin
5. Deduce the effective reflection coefficient at xin
November, 2010 101VKI Lecture
Example of a ideal compressor
Imposed boundary condition
p’ = 0
?
November, 2010 102VKI Lecture
Example of a ideal compressor
Compressor
?Imposed boundary condition
p’ = 0
November, 2010 103VKI Lecture
Example of a ideal compressor
41
2 t
tc p
p
Compact theory
November, 2010 104VKI Lecture
Realistic air intake
November, 2010 105VKI Lecture
Acoustic modes of thecombustion chamber
?
Need to be computed
Outlet Choked B.C. ( taken as an acoustic wall )
Intlet B.C
Realistic air intake
November, 2010 106VKI Lecture
BP Compressor HP CompressorIntake
Air-Intake duct
Outlet Choked B.C. ( taken as an acoustic wall )
Intlet B.C ?
Realistic air intake
November, 2010 107VKI Lecture
BP Compressor HP CompressorIntake
R ?
Realistic air intake
November, 2010 108VKI Lecture
BP Compressor HP CompressorIntake
R ?
November, 2010 VKI Lecture 109
OUTLINE
1. Computing the whole flow
2. Computing the fluctuations
3. Boundary conditions
4. Analysis of an annular combustor
VKI Lecture110
November, 2010
• Helicopter engine
• 15 burners
• From experiment: 1A mode may run unstable
Overview of the configuration
VKI Lecture111
November, 2010
700 Hz 500 Hz 575 Hz 609 Hz
• When dealing with actual geometries, defining the computational domain may be an issue
• Turbomachinery are present upstream/downstream
• The combustor involves many “details”: combustion chamber, swirler, casing, primary holes, multi-perforated liner – Dassé et al., AIAA 2008-3007, …
Combustion Chamber CasingCC + casing
+ swirlerCC + casing + swirler
+ primary holes
About the computational domain
Frequency of the first azimuthal mode – 1A
VKI Lecture112
November, 2010
• The acoustic mode found at 609 Hz has a strong azimuthal component, like the experimentally observed instability
• Its stability can be assessed by solving the thermo-acoustic problem which includes the flame response
• In this annular combustor, there are 15 turbulent flames …
• Do they share the same response ?
Is this mode stable ?
VKI Lecture113
November, 2010
Large Eddy Simulation of the full annular combustion chamber Staffelbach et al., 2008
• The first azimuthal mode is found unstable from LES, at 740 Hz
• Same mode found unstable experimentally
Using the brute force …
VKI Lecture114
November, 2010
• In annular geometries, two modes may share the same frequency
• These two modes may be of two types
• Consider the pressure as a function of the angular position
Mode structure
θ
A+ A-
From simple acoustics:
VKI Lecture115
November, 2010
Turning mode. A+ = 1 & A- = 0
Companion mode turns counter clockwise
VKI Lecture116
November, 2010
Standing mode. A+ = A- = 1
Companion mode has its nodes/antinodes at opposite locations
VKI Lecture117
November, 2010
LES mode. A+ = 1 A- = 0.3
• A simple analytical model can explain the global mode shape obtained from LES
• Can we predict the stability by using the Helmholtz solver ?
VKI Lecture118
November, 2010
• Because of the self-sustained instability, the pressure in front of each burner oscillates
• This causes flow rate oscillations
• Because the unstable mode is turning, the flow rate through the different burners are not in phase
Responses of the burners
VKI Lecture119
November, 2010
Global Response of the flames
• From the full LES, the global flame transfer of the 15 burners can be computed from the global HR and the flow rate signals
• For all the 15 sectors, the amplitude of the response is close to 0.8 and the time lag is close to 0.6 ms
• This result support the ISSAC assumption …
VKI Lecture120
November, 2010
• As far as the flame response is concerned
• Independent Sector Assumption for Annular Combustor
• Allows performing a single sector LES with better resolution to obtain more accurate FTF
• Of course the1A mode cannot appear is such computation
• FTF deduced from single sector LES pulsated at 600 Hz
15
ISAAC Assumption
VKI Lecture121
November, 2010
Typical field of interaction index
Local flame transfer function
VKI Lecture122
November, 2010
• Define one point of reference upstream of each of the 15 burners
• Use the ISAAC Assumption
• the interaction index , and the time delay are the same in all sectors
15sector in if),(ˆ),(
14sector in if),(ˆ),(
2sector in if),(ˆ),(
1sector in if),(ˆ),(
),(ˆ
15ref
15ref
),(
14ref
14ref
),(
2ref
2ref
),(
1ref
1ref
),(
xnxux
xnxux
xnxux
xnxux
x
x
x
x
x
l
l
l
l
jl
jl
jl
jl
T
en
en
en
en
),( xl),( xln
Extended the local n-t model
VKI Lecture123
November, 2010
• Assume ISAAC and duplicate the flame transfer function over the
whole domain
• In the same way, duplicate the field of speed of sound
Extended the local n-t model
VKI Lecture124
November, 2010
• The 1A mode from the Helmholtz solver looks like the 1A from the full LES
• BUT …
1. Its frequency remains close to 600 Hz instead of 740 Hz
2. It is found stable !
Stability of the 1A mode
Helmholtz LES
VKI Lecture125
November, 2010
• The 1A modes from the Helmholtz and LES solvers resemble …
• But a closer look reveals important differences
• What is observed in the Helmholtz solver
1. Pressure amplitude (slightly) larger upstream of the burners
2. No phase shift between upstream and downstream
Shape of the 1A mode
Helmholtz solver
angle (rad) angle (rad)
LES solver
VKI Lecture126
November, 2010
• The Helmholtz solver is not as CPU demanding and allows parametric studies
• The 1A mode is found stable for time delays smaller than T/2
• At 600 Hz, this corresponds to t < 0.83 ms
• The time delay of the FTF (0.65ms) is below this critical value
What’s wrong ?
VKI Lecture127
November, 2010
• Remember the full LES oscillates at 740 Hz
• This corresponds to a critical value for the time delay of T/2 = 0.67 ms, very close to the prescribed time delay
• From the LES, the flow rate and HR are indeed in phase opposition
What’s wrong ?
VKI Lecture128
November, 2010
• Instead of imposing the time delay in the FTF, let’s impose the phase shift between flow rate and HR
• The 1A mode is now found unstable by the Helmholtz solver, consistently with LES and experiment
• The mode shape is also in better agreement
Back to the stability of the 1A mode
Helmholtz solver LES solver
November, 2010 VKI Lecture 129
THANK YOU
More details, slides, papers, …
http://www.math.univ-montp2.fr/~nicoud/