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Moeck, Jonas P. and Durox, Daniel and Schuller, Thierry and Candel, Sébastien Nonlinear
thermoacoustic mode synchronization in annular combustors. (2018) Proceedings of the
Combustion Institute, 37 (4). 5343-5350. ISSN 1540-7489
OATAO
Nonlinear
thermoacoustic
mode
synchronization
in
annular
combustors
Jonas
P.
Moeck
a,b,∗,
Daniel
Durox
c,
Thierry
Schuller
c, d,
Sébastien
Candel
caDepartmentofEnergyandProcessEngineering,Norwegian UniversityofScienceandTechnology,Trondheim7491, Norway
bInstitutfürStrömungsmechanikundTechnischeAkustik,TechnischeUniversitätBerlin,Berlin10623,Germany cLaboratoireEM2C,CNRS,CentraleSupélec,Université Paris-Saclay,Gif-sur-Yvettecedex92292,France dInstitutMécaniquedesFluidesdeToulouse,Université deToulouse,CNRS,INPT,UPS,Toulouse31400,France
Abstract
Nonlinearcouplingbetweenazimuthalandaxisymmetricmodesinannularcombustorsisstudied
analyti-cally.Basedonthethermoacousticwaveequation,amodelfeaturingthreenonlinearlycoupledoscillatorsis
derived.Twooscillatorsrepresentthedynamicsofanazimuthalmode,andthethirdaccountsforthe
axisym-metricmode.Aslow-timesystemfortheevolutionofthemodeamplitudesandphasesisobtainedthrough
theapplicationofthemethodofaveragin g.Theaveragedsystemisshowntoaccuratelyreproducethe
solu-tionsofthefulloscillatormodel.Analysisofthisfive-dimensionaldynamicalsystemshowsthatastanding
azimuthalmodemaysynchronizewithanaxisymmetricmode,providedthattheirindividualresonance
fre-quenciesandgrowthratesaresimilar.Thisphase-coupledtwo-modeoscillationcorrespondstotheso-called
slantedmode,observedinrecentexperimentsinvolvinganannularmodelcombustionchamber.Quantitative
conditionsfortheoccurrenceofmodesynchronizationarederivedintermsofthegrowthrateratioanda
frequencydetuningparameter.Theanalysisresultsarefoundtobeconsistentwithexperimentalobservations
oftheslantedmode.
Keywords: Combustioninstability;Azimuthalmode;Nonlinearsynchronization;Annularchamber;Slantedmode
∗Correspondingauthorat:DepartmentofEnergyand ProcessEngineering,NorwegianUniversityof Science andTechnology,Trondheim7491,Norway.
E-mail addresses: jonas.moeck@ntnu.no,
jonas.moeck@tu-berlin.de(J.P.Moeck).
1. Introduction
Thermoacoustic instabilities occur in many
technicalapplicationswhereheatisaddedthrough
combustion,prominentexamplesbeingstationary
gasturbinesforpowergenerationandaero-engines
[1,2].Insimplified laboratoryconfigurationsthat
in the axial direction and the associated modes
arereadilyobtainedfromelementarycalculations.
Combustion chambers in the applications
men-tionedabove,however,featureanannular
geome-try,inwhichmultipleflames,typicallymorethan
10,aredistributedcircumferentially.Theseannular
combustionchambershost,inaddition,azimuthal
modes,forwhichthedominantpressurevariation
occursalongtheangularcoordinate.Infull-scale
engines,combustioninstabilitiesarethusoften
ob-served to couplewith the lower-order azimuthal
modes[3,4].
Overthelastdecade,azimuthalinstabilitiesin
annularchambershavebeenintenselystudiedby
experimental andnumerical means [5–8] andby
using analytical methods [9]. Many elementary
propertiesofazimuthalinstabilitymodesarewell
understoodby now,particularly those pertaining
to the linear dynamics, such as the degeneracy
of azimuthalmodes in systemswith discrete
ro-tational symmetry. The most prominent action
of the nonlinearflame response is to destabilize
thestanding-wave pattern sothata spinning
az-imuthal mode is established at finite oscillation
levels [10,11]. Comprehensive nonlinear analysis
[12] shows more complex phenomena, such as
thesimultaneousexistenceof stablestandingand
spinningwaves,recentlyobservedin theformof
mode hysteresis [13]. Another phenomenon
spe-cifictoannularchambersanddiscoveredrecently
istheoccurrenceof anonlinearcouplingbetween
axisymmetricandazimuthalmodes,givingriseto
aslantedpatternof theperturbedflamesaround
the combustion chamber circumference [8]. The
present article is concerned with explaining the
manifestation of the slanted mode based on a
nonlinearthermoacousticmodel.
Fromamoregeneralpointofview,theslanted
mode is the manifestation of nonlinear mode
coupling that involves synchronization of two
modeswithsimilarindividualresonance
frequen-cies.Otheraspectsofsynchronizationhaverecently
beenstudiedinthefieldofthermoacoustics[14,15],
viz. forced synchronization and synchronization
of differentfields. However,thepresentcase
pre-ciselycorrespondstothescenariolabeledas
‘mu-tualsynchronizationofself-sustainedoscillators’in
thestandardreference[16,Chap.4].
Fromexperimental and theoreticalstudies of
thermoacousticinstabilitiesinlongitudinal
config-urations,itappearsthatwhenevertwomodeswith
differentresonancefrequenciesareunstableatthe
sametime,theprevailingtendencyisthatonlyone
modesurvivesandtheotherissuppressed [17],or
aquasi-periodic solutionemerges, inwhichboth
modes oscillate with different, generally
incom-mensuratefrequencies [18,19].Sincesingle-burner
configurations host only longitudinal modes in
thelow-frequencyregime,twomodescannothave
close resonance frequencies, unless the system
features decoupled plenum and chamber modes
[20];therefore, synchronizationbetween different
modesislesslikelytooccurinthesesystems.An
annular chamber, however, has a significantly
highermodaldensitysothatitmayindeedhappen
thattwomodeshavesimilarresonancefrequencies,
givingrisetosynchronization.
Ouranalysis isbasedon theoscillator model
introducedbyNoirayetal. [11]forthe
investiga-tionof theeffectof asymmetryonthestanding–
spinningmodestructure.Thesamemodelwasused
byGhirardoetal. [21]toexplainstandingmodes
insymmetricsystemsthroughanonlinear
mech-anism involving transverse velocity fluctuations.
Thismodel isextendedhere toexaminethe
cou-plingbetween anazimuthalandanaxisymmetric
mode,correspondingtotheslantedoscillation
pat-tern observed in previous experiments [8]. Since
theazimuthaleigenspaceisspannedbytwomode
shapes(sineandcosineorclockwiseand
counter-clockwiserotating),theadditionofan
axisymmet-ricmodeyieldsasetofthreeoscillatorequations
describingtheevolutionofthemodesintime.
Be-causethemodeshapesareorthogonal,thereisno
linearcouplingbetweentheoscillators.Their
inter-actionemergesonlythroughthecubictermandis
thereforefullynonlinear.Theoscillatorequations
andanassociatedslow-timesystemforthe
ampli-tudesandphasesarederivedin Section 2.
Com-prehensiveanalysisofthissystemiscarriedoutin
Section3.Section4discussestheanalyticalresults
inviewofexperimentalobservations.
2. Modelequations
Theoscillatormodelwe considerissimilarto
theoneproposedbyNoirayetal. [11].However,
weincludeanadditionalaxisymmetricmodeand
focusoncaseswheretheresonance frequencyof
thisaxisymmetricmodeisclosetothatof the
az-imuthalmode.Asinpreviouswork,westartfrom
thewaveequationfortheacousticpressurewitha
sourcetermassociatedwiththeunsteadyheat
re-leaserateintheflames:
∂ 2p ˜ ∂t ˜2 +α˜ ∂ p ˜ ∂t ˜ − c R 2∂ 2˜p ∂θ2 + ω 2 0p ˜=(γ − 1) ∂ q ˜ ∂t ˜. (1)
Here, p ˜is theacousticpressure,α a˜ damping
coefficient,c thespeedofsound,R themeanradius
oftheannulus,θ theangularcoordinate,γ the
ra-tioofspecificheats,andq ˜theheatreleaserate.The
resonancefrequency of thefirst azimuthalmode
is ω a= c/R .Theterm ω 20p ˜representsthe
axisym-metricmode,withresonancefrequencyω 0.An
ax-isymmetricmodehasthesamephaseatthe
circum-ferentiallocationsoftheflames;assuch,itcanbe
alongitudinaloraHelmholtzmode.Theω 2
0p ˜term
canbe motivated bythefactthat applicationof
theLaplaciantoanaxisymmetricmoderesultsina
termproportionaltoω 2
0p ˜, withanadditionalfactor
Non-dimensionalvariablesareintroduced: t =
˜
t ω a, p = p ˜/ (ρc 2), q =q ˜ρc 2ω a/ (γ − 1) , α = α/ω ˜ a, =ω0/ωa;ρ denotesthemeanfluiddensity.The
unsteadyheatreleaserate q istakentodependon
the local pressure according to q (p)=β p− κ p3
[11];β andκ arepositiveconstants.Thisflame
re-sponsemodelissimplebuthasbeenusedinmany
recenttheoreticalstudies (e.g.,Refs. [11,21])asit
encapsulatesthemostimportantnonlineareffect,
viz.saturation.
Wenowassumeasolutionoftheform
p(θ, t) =ηc(t)cosθ + ηs(t)sinθ + η0(t). (2)
This corresponds to the expression used in
Refs. [11,12,21], except the additional term η0,
which represents the axisymmetric mode. The
cosθ and sinθ terms span the two-dimensional
eigenspace of the degenerate azimuthal mode.
For a spinning mode, theamplitudes of ηc and
ηs areequal,andtheirphasedifferenceis ± π/2.
A standing wave has arbitrary amplitudes but a
phasedifferencebetweenηcandηsof0or π.
Theansatz (2)isnowintroducedintothewave
equation(1),andafterprojectionontothespatial
basis{cosθ, sinθ, 1},coupledoscillatorequations
forηc,ηs,and η0areobtained:
¨ ηc/s+ηc/s= (β−α) η˙c/s− 3 4κ 3η2 c/s+η 2 s/c+4η 2 0 ˙ ηc/s +2ηc/sηs/cη˙s/c+8ηc/sη0η˙0 , (3a,b) ¨ η0+2η0= (β − α0)η˙0− 3κ (ηcη˙c+ηsη˙s)η0 +η2 c/ 2+ η 2 s/ 2+η 2 0 ˙ η0 . (3c)
Here, (·)˙ denotes a derivative with respect
to time, andthe damping coefficient for the
ax-isymmetricmode, α0,has beenendowedwithan
additional subscript to indicate thatthis
param-eter should be allowed to be generally different
fromthosecorrespondingtotheazimuthalmode.
The damping rate depends on the spatial
struc-tureof themodeandtherefore maybe different
for each oscillator. Conversely, β is a property
of the flame response and thusidentical forall
modes/oscillators.
Dampingandlinearflameresponse gainonly
appearasdifferencesin Eq.(3),correspondingto
thelineargrowthratesofthemodes.Inthe
follow-ing,thesegrowthratesaredenotedby σa= β − α
fortheazimuthalmodeandσ0= β − α0forthe
ax-isymmetricmode.Sincewewishtostudythe
inter-actionof azimuthalandaxisymmetricmodes, σa
andσ0areassumedpositive.
Thetermsinthesquarebracketsmultiplyingη˙c/s
in Eq.(3a,b)andη˙0 in (3c)correspondto
nonlin-eardamping,whichwilllimittheamplitudegrowth
of therespectivemodeatfiniteoscillationlevels.
The term4η2
0 willthusreducethegrowthof the
azimuthalmode whilethe terms (η2
c+ηs2)/ 2 will
damptheaxisymmetricmode.Thisscenario
pro-motes mode competition. Also note that in the
absence of theaxisymmetric mode, with η0=0,
Eq.(3a,b)areidenticaltothesystemconsideredby
Noirayetal. [11]inthestudyofapureazimuthal
mode.
Foragivensetof parametersandinitial
con-ditions,theoscillator equations(3)canbesolved
numerically, but this approach does not provide
muchinsight.Wewillinsteadapplythemethodof
averaging [22]tothesystemofcoupledoscillators,
which allows drawing more general conclusions
about the system dynamics. The solutions are
assumedtobeoftheform
ηi= A i(t)cos[t +φi(t)], i ={c,s,0},
wheretheamplitudesA iandphasesφiareassumed
tobeslowlyvaryingfunctionsof time.Notethat
theoscillationfrequencyisnotapriorifixedto1
(ωa in dimensionalvariables). A small deviation
from the resonance frequency of the uncoupled
modecanbeaccommodatedintheslowlyvarying
phasetermφ( t ).
Followingstandardprocedures [22],the
evolu-tionequationsfortheslowlyvaryingamplitudeand
phasevariablesareobtainedbyaveragingthe
con-tributionsoftheoscillatingquantitiesoverone
pe-riod: ˙ A i=−f isin(t+φi), φ˙i=− 1 A i f icos(t+φi), (4)
wherethe f iaretherighthandsidesof Eq.(3),and
theangledbracketsdenoteanaverageoverone
pe-riodoftheuncoupledazimuthalmode.Notethata
delayintheflameresponsemodelonlyaffectsthe
lineargainbutnotthestructureoftheaveraged
sys-tem [11].
There are four parameters in the oscillator
system: the growth rates of the azimuthal and
theaxisymmetric modes σa and σ0,theratio of
the oscillationfrequencies , and thesaturation
coefficient κ from the nonlinear flame model.
Twooftheseparameterscanberemovedthrough
suitablerescaling.Tothiseffect,weintroduce
ˆ A i=Ai κ σ0 1/2, σ = ˆ σa σ0 , = ˆ 2− 1 2σ0 , τ = tσ0.
Furthermore,the amplitudeandphaseevolution
equations do not depend on the phasevariables
independently but only on their differences. We
therefore introduce phase-difference variables,
definedasψ i j= φi− φj.
Usingtheaveraging ansatz (4),theamplitude
andphase-shift evolutionequationsarethen
ˆ A c/s= ˆ A c/s 32 16σ − 3ˆ 3A ˆ2c/s+ 2A ˆ 2 s/c+ 8A ˆ 2 0 (5a,b) +A ˆ2 s/ccos2ψcs+4A ˆ20cos2ψc/s0 , ˆ A 0= ˆ A 0 32 16− 34(A ˆ2c+ ˆA 2 s+ ˆA 2 0) +2A ˆ2 ccos2ψ c0+2A ˆ2scos2ψ s0 , (5c) ψ cs = 3 32 ˆ A 2 s + ˆA 2 c sin2ψ cs +4A ˆ2 0(sin2ψ c0− sin2ψ s0) , (5d) ψ c0 =− ˆ + 3 32 ˆ A 2 ssin2ψ cs+4A ˆ20sin2ψ c0 +2A ˆ2 csin2ψ c0+2A ˆ2ssin2ψ s0 . (5e)
Here,ψs0=ψc0− ψcs,and(·)denotesa
deriva-tive with respecttothescaled time τ. Alsonote
thatto leading order, thefirst term onthe right
handsideof Eq.(5e)correspondstothefrequency
differencebetweentheazimuthalandthe
axisym-metricmode.Forsmallamplitudes,thephasesof
the axisymmetric and the azimuthal modes will
thusdivergeatarateequaltothefrequency
differ-encewhentheiruncoupledresonancefrequencies
arenotidentical.However,thenonlineartermsin
(5e)may compensate the frequency difference to
es-tablishafixedphasedifferencebetweenazimuthal
andaxisymmetricmodes incaseof
synchroniza-tion.Furthermore, it isevident from the system
(5)thatcouplingbetween themodes occursina
purelynonlinearfashion.
In the following, we consider the system of
nonlinearlycoupleddifferential equations(5)that
evolvethesystemstateinafive-dimensionalspace.
Theadvantageofstudyingtheaveragedsystemis
thatperiodicandquasi-periodicsolutionscanbe
determinedmucheasiercomparedtotheoscillator
Eqs.(3).Periodicsolutionsofanykindare
charac-terizedbyfixedpointsoftheaveragedsystem,i.e.
[A ˆc,A ˆs,A ˆ0,ψcs,ψc0 ]=0, withatleast oneof the
amplitudesbeingnon-zero.Aquasi-periodic
solu-tionwouldbecharacterizedbyatleastoneofthe
azimuthalmodeamplitudesandtheaxisymmetric
modeamplitudebeingnon-zeroandallofthe
pre-viously mentioned state variables being constant
exceptfor ψ c0,whichwouldvarylinearlyintime,
driven by the frequency difference between the
azimuthalandtheaxisymmetricmode.Stabilityof
theindividualperiodicorquasi-periodicsolutions
thatmayexistforcertainvaluesoftheparameters
isalsomoreeasilydeterminedfromtheaveraged
system.Oneonlyneedstoinspecttheeigenvalues
of the Jacobian evaluated at the corresponding
equilibriumstate.
Fig. 1.Comparison of numerical solutionsof the os-cillator equations(3)andtheaveragedsystem (5).Top: modecoefficients ηi andmode amplitudesAi;the lat-terareshownasgraylines.Bottom: phaseshiftsfrom thenumericalsolutionoftheaveragedsystem. =1.03, σa=0.1,σ0=0.09,κ =0.2,correspondingtoσ ≈ 1ˆ .11 and ≈ 0ˆ .338.
3. Results,discussion,andfurtheranalysis
To assess the ability of the slow-time model
(5) to represent the dynamics of the original
coupledoscillatorsystem (3),numericalsolutions
based on both sets of equations are compared
(Fig.1,topframe). Theamplitudesfromthe
av-eragedsystemappearasenvelopesof the
oscilla-torsolutions,anditisapparentthattheaveraged
systemisaverygoodapproximationthatcaptures
eventhenon-monotonicamplitudeevolution
ac-curately. The parameter values for this case are
= 1 . 03, σa= 0. 1, σ0= 0. 09, κ = 0 . 2, withlinear
growthratesandsaturationcoefficient chosenas
inRef. [11].Intermsof therescaledparameters,
thiscorresponds toa growthrate ratioσ ≈ 1 ˆ . 11
andfrequencydetuning parameter ≈ 0 ˆ . 338.In
theinitiallinearstage,allamplitudesgrow
expo-nentiallybecauseofthepositivegrowthrates.After
atransientstagewithnon-trivialamplitude
evolu-tion,theaxisymmetricmodeeventuallydecaysto
zeroandcosineandsineamplitudesattain
identi-caloscillationlevels.Thephasebetweencosineand
sinemodes,ψcs,settlesat−π/2(Fig.1,bottom),
whichshowsthatapurelyspinningmodeis
estab-lished.Alsonotehowthephaseshiftbetween
az-imuthalandaxisymmetricmodes,hererepresented
through ψ c0,increaseslinearlyatsmalloscillation
amplitudes,isnearlyconstantintheintermediate
regimewhenallmodesfeatureappreciable
ampli-tudes,andfinallydriftsoffwhentheaxisymmetric
modehasvanished.Thisindicatesthatthesystem
isalreadyclosetosynchronization.
Now the frequency ratio is decreased to
= 1. 01, correspondingtoafrequencydetuning
parameter = ˆ 0. 112 (Fig. 2). The solution of
~ ;§. 0.5
1
0î
-0.5 -1 ~ - - - - ~ - ~ - - ~ - - - - ~tJ
0~
50 100 150 200 250:
300l
non-dimensional time tFig.2. As Fig.1butwith =1.01,correspondingto ˆ
≈ 0.112.
theaveraged systemagaincorresponds wellwith
that of the oscillator model. In contrast to the
previouscasewithalargerfrequencydetuning,all
modessurviveinthelong-timelimitandsettleon
constant amplitudes (visible attimes larger than
showninFig.2).Wenotethattheazimuthalmode
isstanding,indicatedby ψ cs=0(Fig.2,bottom).
Theamplituderatioofthecosineandsine
compo-nentsdeterminestheorientationofthenodalline
of the standing azimuthal mode. In the present
axisymmetric setting, all orientationsareequally
permissible,anditdependsontheinitialconditions
whichisestablished.Furthermore,thephase
differ-encebetweentheazimuthalandtheaxisymmetric
mode,ψ c0,settlesonafixedvalue,slightlylessthan
π/2. Afixedphasedifference ψ c0 impliesthatthe
twomodes,whichhavedifferentlinearresonance
frequencies,havebecomesynchronizedthroughthe
nonlinearcoupling.Thisscenarioprecisely
corre-spondstotheslantedmodedocumentedinRef.[8].
A phaseshift closeto π/2 between azimuthal
andaxisymmetricmodesisalsoobservedinthe
av-eragedmodelandinexperimentaldata,tobe
dis-cussedinthefollowing,andthereforeappearsto
bearobustfeatureof thephenomenon.
Further-more,thisphaseshiftisonlyinsignificantlyaffected
by atime delay inthe flame response model, as
wasverifiednumericallyonthebasisofthe
oscilla-torsystem (3).Whileadelayintheflameresponse
wouldgenerallyaffectthephaseshiftbetween
pres-sureandheatreleaserate,thenonlinearcoupling
ofthetwomodesoccursonlythroughthepressure
atthelocationof theflames.Inthephase-locked
state,bothmodesoscillateatthesamefrequency
and,hence,acquirethesamephaseshiftfromthe
flameresponse;thephaseshiftbetweenthemodes
is therefore unaffected by the delay. Similarly, a
morerealisticburnerimpedanceisnotexpectedto
affectthisphaseshift.
In the following, we analyze the averaged
system (5)to establishconditions inthereduced
parametersσ (growth ˆ rateratio)and (frequencyˆ
detuning),forwhichtheslantedmode,i.e.,the
syn-chronizedoscillationbetweenanaxisymmetricand
anazimuthalmode,existsandisstable.Sincethere
isrotationalsymmetry,wecanassumewithoutloss
ofgeneralitythat A s=0forastandingazimuthal
mode.Theamplitude Eqs.(5)thentaketheform
ˆ A c= ˆ A c 32 16σ − 3ˆ 3A ˆ2c+ 4A ˆ 2 0(2+cos2ψc0) , (6a) ˆ A 0= ˆ A 0 32 16− 34A ˆ20+ 2A ˆ 2 c(2+cos2ψc0) , (6b)
withphase-differenceequation
ψ c0=− ˆ + 3 16 ˆ A 2 c+ 2A ˆ 2 0 sin2ψ c0. (6c)
Since A s=0, thephasedifference ψ cs is
irrele-vant.Foraslantedmode,therighthandsidesof
Eqs.(6)mustvanishfornon-zeroA ˆc andA ˆ0.We
firstdetermine conditionson andˆ σ forˆ which
suchsolutionsexistandthenaddressthestability
ofthesynchronizedstate.
From requiring that the right hand sides of
Eqs. (6) vanish, an equation only involving the
phase-shiftvariableψ c0canbeobtained:
2(2+cos2ψ c0)2− 3 ˆ = 1/ 2+σ + ˆ (1+σ ) ˆ cos2ψ c0 sin2ψ c0. (7)
This equation is quartic in cos2ψ c0 and thus
may have four real solutions in any half-closed
interval of length π. It appears that these
so-lutions cannot be expressed in simple form for
arbitrary andˆ σ .ˆ We therefore consider first
the special casewhere theresonance frequencies
of theazimuthalandtheaxisymmetricmodeare
identical, i.e., =ˆ 0. Equation (7) then has the
four solutions ψc0={0,π/2,a,−a}, where a is
given by a =arccos[−(σ +ˆ 1/2)/(σ +ˆ 1)], which
areallmodulo π. Whenthesesolutionsareused
inrequiringthattherighthandsidesof (6a)and
(6b) vanish, explicit expressions for the squared
amplitudes of thetwo modes are obtained. The
solutions ψ c0=±a lead to negative amplitude
squaresfortheaxisymmetricmodeandtherefore
canbediscarded.Withtheothertwosolutionsof
thephase-shift equation(7),weobtain
ψ c0=0: A ˆ2c= 16 45(3− ˆσ ) , A ˆ 2 0= 4 15(2σ − 1) ˆ , (8) ψc0= π 2 : A ˆ 2 c= 16 3 (σ − 1)ˆ , A ˆ 2 0= 4 3(3− 2σ )ˆ . (9)
These solutions correspond to phase coupled
oscillationsof anazimuthalandanaxisymmetric
~
i.
0.5 ] 0 'à ~ -0.5 -1 ...__ ... _ _ ..__ ... _ _ ..._ _ __. _ _ _.I~
0~
50-
100~
150 200~
: :
250 300l
non-dimensional time tu~~-~-~-~-~~-~-~~ 1.6 <b 1.5 .g 1.4
e
~ 1.3 .c 1.2!
1.: 0.9 0.8 '---'---'----'----'---''----'----'----' -0.3 -0.2 -0.1 0 0.1 0.2 0.3frequency detuning 6
Fig. 3. Existence and stability domain (gray shaded) of the phase-coupled two-mode solution - the slanted mode - in parameter space. Stars indicate parame-ter combinations for which phase planes are shown in
Fig. 4. Diamond and square correspond to parameters of
Figs. 1 and 2, respectively.
mode, and it can be verified numerically that these are indeed equilibrium states of the full system given by Eqs. (5). Since the amplitude squares need
to be positive, the conditions for the existence of a phase-coupled two-mode solution with phase
shift O and 7r/2 are 1/2 < 8 < 3 and 1 < 8 < 3/2, respectively. As we will show Jater in this section, the in-phase solution with
V/d)
=
0 is unstable so that the occurrence of a slanted mode is limited to the stricter requirement on the growth rate ratio.When the frequencies of the two modes are not identical, i.e.,
!!>
=I= 0, the phase-shift Eq. (7) can-not be solved in simple terrns. However, the rangeof growth rate ratios 8 that permits a stable
phase-coupled solution can be determined numerically as a fonction of the frequency detuning
6.,
as shownin Fig. 3. The effect of the frequency detuning is
to reduce the range of growth rate ratios for which a slanted mode occurs. For
1
6.
I
~ 0.273, nosta-ble phase-coupled two-mode solution exists for any growth rate ratio. For a non-dimensional growth
rate a0
=
0.2, this corresponds to a frequency dif-ference of about 5%. The stability domain of the slanted mode is symmetric with respect to!!>
be-cause the system (6) has the symmetry (!!>, 1/f,,,) ~(-!!>,
-
VJ,,,).
When!!>
«
1 is assumed, which is rea-sonable in view of Fig. 3, the effect of the fre-quency detuning on the phase shift can be deter-mined to Jeading order from Eq. (7) as 1/f"'=
7r /2-6.
(modulo7r). Hence, the azimuthal and theax-isymmetric modes will always be approximately in
quadrature when they are phase coupled.
It is now instructive to consider the structure of the state space defined by the system (6) to under-stand the qualitative changes in the stability of the
synchronized two-mode solution. To this purpose, we plot the vector field defined by (6a) and (6b) cor-responding to different points in the parameter space (Fig. 4a). The system is three-dimensional, and the 1/f"' coordinate can be thought of as
pointing out of the paper plane; however, we have already shown that only the immediate vicinity of the planes
V/d)
=
0 andV/d)
=
7r /2 are of interest.Figure 4 illustrates the state space dynamics at
1/f"'
=
7r /2 for zero frequency detuning and a growth rate ratio of 8=
1.25, which is most favor-able for the existence of the slanted mode accordingto the stability map (a in Fig. 3). By construction,
the origin is a repeller; the single-mode limit cy-cles found on the axes, where one mode has zero amplitude, both correspond to saddles: they are
at-tracting in the direction of the non-zero mode, but repelling perpendicular to it. The in-quadrature
synchronized two-mode solution is a stable node,
globally attracting in the 1/f,,,
=
7r /2 slice of the state space. ln the slice corresponding to in-phasetwo-mode oscillations, 1/f"'
=
0 (Fig. 4b), the roles of the single-mode and the two-mode oscillations are reversed; the latter cannot occur as it isunsta-ble. Also note that the single-mode oscillations are attracting only in this plane, as the phase
equilib-rium at 1/f,,,
=
0 is unstable according to Eq. (6c).As the growth rate ratio 8 is decreased from 1.25, the stable node, corresponding to the
synchro-nized two-mode solution, successively approaches the saddle corresponding to the single-mode
ax-isymmetric oscillation. When 8 is decreased below
1 (see Fig. 3), the node collides with the saddle,
rendering the single-mode axisymmetric limit cycle stable (Fig. 4c). When 8 is increased beyond 3/2, the stable two-mode oscillation collides with the
single-mode azimuthal limit cycle, which is then the only stable solution (Fig. 4d). These latter effects are not
entirely surprising when one recalls that 8 is the
ra-tio of the growth rates of the azimuthal and the
ax-isymmetric mode.
Only the case with zero frequency detuning is
depicted in Fig. 4. However, the (Â~. Â
0)
vect or-field varies smoothly with 1/f ,,,, and the equilibriumphase shift changes only slightly with
!!>.
Qualita-tively, the dynamics therefore remains similar to that shown in Fig. 4 even when!!>
is non-zero, aslong as a stable synchronized two-mode solution exists
(
l
!!i
l
;§
0.273, Fig. 3). Whenl
!!i
l
increases be-yond this value, the synchronized two-modesolu-tion only exists as an unstable saddle, as in Fig. 4b,
and the only stable solutions are single-mode limit cycles.
4. Modeling results and experimental observations
The analysis in the previous section showed that
the slanted mode [8] arises from a synchronization
process between unstable azimuthal and
axisym-metric modes. Furtherrnore, this synchronization
is only possible when the individual resonance
fre-quencies of the modes are close and when their growth rates are similar. This is consistent with
oc-Fig. 4. Phase planes for the amplitude dynamics of the reduced standing-azimuthal-axisymmetric system, Eqs. (6a}-(6b). a)â = 1.25,
t,.
= 0, iftc0 = :ir/2; b)â = 1.25,t,.
= 0, iftc0 = 0;c)â = 0.9,t,.
= 0, iftc0 = ,r/2;d)â = 1.6,t,.
= 0, iftc0 = ,r/2. The amplitude range is Âc = 0 ... 1.6 for a)-c) and Âc = 0 ... 1. 7 for d). Âo ranges from O to 1.6 in ail frames. Filled circles represent stable equilibrium solutions, open circles unstable ones. Background color corresponds to the norm of the amplitude rate of change, ((Â~)2+
(Â0
)2)112; colorscaJe saturates at value 1.
curs only in a very narrow region in the operating space (see Fig. 4 in Ref. [13D.
lt would be interesting to test the predicted dependence of the slanted mode solution on the frequency detuning and the growth rate ratio, as illustrated in Fig. 3. This is unfortunately not possible because (i) the frequency detuning and the growth rates cannot be varied independently in the experiment, and (ii) these parameters can-not be accurately measured. However, the phase shift between the azimuthal and the axisy=etric mode, 1/fc0, which is predicted to be close to 1e/2
from the analysis, can be retrieved from available experimental data. To this purpose, we analyze high-speed images of the flames' light emission acquired during conditions corresponding to the slanted mode (same data set as was used in Ref. [8]). The images were acquired with a Photron Fastcam APXii at a framerate of 12,000 images per second. A subset of 1000 images was analyzed by means of proper orthogonal decomposition (POO). Increas-ing the number of images did not noticeably affect the results presented in the following.
POO decomposes snapshots of a space and time
dependent observable into orthogonal modes and
ranks them according to their fluctuation energy [23]. The fluctuation energy of the first 100 modes relative to the total fluctuation energy is shown in
Fig. 5. l'wo modes are clearly dominant, ail others contributing with Jess than 1% to the total fluctu-ation energy. The first two POO modes are shown in Fig. 5 as insets. The POO mode with the largest fluctuation energy can be identified as axisymmet-ric thermoacoustic mode, all flames featuring the same sign of the heat release rate perturbation. ln contrast, the POO mode with the second highest fluctuation energy is a first-order azimuthal mode, with positive and negative heat release rate fluc-tuations varying sinusoidally around the circum-ference. This corresponds to a standing azimuthal mode; a rotating azimuthal mode would be repre-sented by two POO modes rotated with respect to each other by an angle of 1e/2.
~
:.
0 -...
-
.
-~max~
:in
0 ~.
.
_ ... ... . ..
.
.
.
.
.
.
.
0 0.
1!
.. •
•• ·-
•
.
:•
·
-
::,i
---1 10• modenumber..
Fig. 5. Relative fluctuation energy of the first 100 POO modes obtained from high-speed imaging of the flames'
light emission in the MICCA combustor when the slanted mode is observed. A Jong-exposure photo is shown in the inset to the Jower Jeft. The first two POO modes are shown as insets to the upper right. The light that can be seen ad-jacent to the actual, disk-shaped flames stems from light reflections on the quartz combustor walls.
0.1 ~ - ~ - ~ - ~ - ~ - ~ - ~ - - ~
- axisymmetric - azimuthal
] 0.05
l
o .g ~ -0.05 -0.1 ' - - - ~ - ~ - ~ - ~ - ~ - ~ - - . . . _ , 0 2 4 6 8 10 12 14 time (ms)Fig. 6. Amplitudes corresponding to the axisymmetric and the azimuthaJ modes, obtained from POO of the high-speed images.
The phase relation of the two dominant POO modes can be deduced from their associated time coefficients. These indeed exhibit a phase shift very close to 1e/2, showing that the two modes are in quadrature (Fig. 6). The precise value of the mean
phase shift is obtained from the cross spectrum
of the two time coefficients; this evaluates to
1.595 rad at the dominant frequency (450 Hz),
whichdeviatesfromexactquadraturebylessthan
2%. This result corroborates the analysis in the
preceding section,which predicted a quadrature
relation whenever an azimuthal and an
axisym-metricmodebecomesynchronizedinatwo-mode
oscillation. Theinstantaneous phaseshiftcan be
determinedfromtheassociatedanalyticsignalsvia
the Hilbert transform. This quantity shows very
littledeviationfromthemeanvalue,witha
stan-darddeviationof lessthan0.03rad,highlighting
propersynchronizationbetweenthetwomodes.
5. Conclusion
Nonlinear couplingof thermoacoustic modes
inannularcombustorswasinvestigated.A
synchro-nized two-mode limit cycle involving a standing
azimuthal and an axisymmetric oscillation, as
recentlyobservedinanannularmodelcombustor
[8], was analyzed. This phase-coupled two-mode
oscillation occurs provided that the individual
resonance frequencies of the two modes and
theirgrowthratesaresimilar.Thesefindingswere
obtained bystudyingareduced systemthatonly
allowsforastandingazimuthalmodeinaddition
to the axisymmetric mode. However, it can be
shown that a synchronized oscillation involving
aspinningazimuthalmodeandanaxisymmetric
modedoesnotexist.
Through suitable rescaling, the dependence
of the system dynamics on the cubic coefficient
κ, which controls the saturation of the flame
response,isremoved(providedκ remains positive).
Theexistenceoftheslantedmodesolutionisthus
supportedby alargeclassof flame modelswith
saturation nonlinearity. The specific value of κ
affectsthesolutiononaquantitativelevel(the
os-cillationamplitude),buttheanalysisshowedthat
thequalitativedynamics,i.e.,single-mode
oscilla-tions or phase-locked two-mode oscillations,are
unaffected.Thequalitativedynamicsdependonly
onthetwonon-dimensionalparametersσ and ˆ ,ˆ
correspondingtogrowthrateratioandfrequency
detuning,respectively.Wecanthenexpectthatthis
nonlinearlysynchronizedtwo-modeoscillationisa
rathergenericfeatureofthermoacousticinstability
inannularcombustorsthatmayappearwhenthe
resonancefrequenciesandthegrowthratesof an
azimuthalandanaxisymmetricmodeareclose.
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