THESE de DOCTORAT - cerfacs
THESE de DOCTORAT - cerfacs
THESE de DOCTORAT - cerfacs
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32 Chapter 2: Computation of noise generated by combustion<br />
ings [106]. As stated in the introductory part of this section, the acoustic operator of Lighthill’s<br />
analogy does not account for acoustic-flow interactions. All these possible interactions are implicitly<br />
inclu<strong>de</strong>d in the source terms and therefore <strong>de</strong>nsity fluctuations on the sources cannot<br />
be neglected. However, in or<strong>de</strong>r to compute this compressible sources it would be necessary to<br />
resolve the pressure field in which these sources are embed<strong>de</strong>d or, in other words, to solve the<br />
problem itself. Some simplifications then must be consi<strong>de</strong>red.<br />
Simplifying Lighthill’s Analogy<br />
Equation (2.41) is an exact result <strong>de</strong>rived from the conservation equations for mass, momentum,<br />
energy and species and therefore until now no assumptions or simplifications have been<br />
introduced. Nevertheless, this equation in this way does not present a significant utility. Assumptions<br />
must be consi<strong>de</strong>red so that Lighthill’s equation becomes tractable and therefore<br />
solvable. The i<strong>de</strong>a is then only to consi<strong>de</strong>r the predominant mechanisms generators of noise.<br />
In doing so, diffusive fluxes of species J k and the dissipation function τ ∂u i<br />
∂x j<br />
˙Q vanishes if no external energy sources are applied to the system and ∂q i<br />
∂x i<br />
are first neglected.<br />
is zero if heat fluxes<br />
are consi<strong>de</strong>red small. Moreover, at high Reynolds number the viscous tensor τ ij is negligible if<br />
compared to the Reynolds stresses ρu i u j and the propagation medium is consi<strong>de</strong>red homogenous<br />
(p, ρ, c → p ∞ , ρ ∞ , c ∞ ) so that all the third line disappears. Further on, combustion can be<br />
consi<strong>de</strong>red isomolar if air is used as oxidizer so that D Dt<br />
(ln r) vanishes and for low Mach numbers<br />
M the acceleration of <strong>de</strong>nsity inhomogeneities<br />
∂2<br />
∂x j ∂t (ρ eu j ) can be neglected . The simplified<br />
Lighthill Equation then reads<br />
1<br />
c 2 ∞<br />
∂ 2 p<br />
∂t 2 − ∂2 p<br />
∂xi<br />
2 = ∂2 ( ) (γ − 1) ∂ ˙ω<br />
ρ∞ u i u j + T<br />
∂x i ∂x j c 2 ∞ ∂t<br />
(2.42)<br />
Hassan <strong>de</strong>monstrates in his work [32] that noise produced by combustion is much more important<br />
than the one generated by turbulence. Note that the combustion source of noise is a<br />
monopole ( ∂ ∂2<br />
∂t<br />
) whereas the aerodynamic source of noise is a quadrupole ( ). A quadrupolar<br />
∂xi<br />
2<br />
source of noise is known to be a bad radiator of sound if compared to a monopolar source and<br />
therefore the aerodynamic source can be neglected. Finally, heat release ˙ω T and pressure p are<br />
<strong>de</strong>composed by its mean and fluctuating parts (p = ¯p + p ′ , ˙ω T = ¯˙ω T + ˙ω<br />
T ′ ). Combustion<br />
noise in a quiescent medium is given then by<br />
1<br />
c 2 ∞<br />
∂ 2 p ′<br />
∂t 2 − ∂2 p ′<br />
∂x 2 i<br />
=<br />
(γ − 1)<br />
c 2 ∞<br />
∂ ˙ω ′ T<br />
∂t<br />
(2.43)<br />
where ∂ ¯p<br />
∂x i<br />
≈ 0 due to the M = 0 assumption. It is useful also to solve this wave equation in<br />
the frequency domain. Consi<strong>de</strong>ring harmonic perturbations of pressure p ′ and the heat release