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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

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