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Analyse expérimentale et modélisation du transfert de matière et du ...

Analyse expérimentale et modélisation du transfert de matière et du ...

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Annexe Chapitre 2Reynolds stress tensor is d<strong>et</strong>ermined. Th<strong>et</strong>ransport equation of the Reynolds stresstensor written as:D ' 'u u = P + Πi j ijDtwherestresses,ij− εij(7)P is the pro<strong>du</strong>ction term of the ReynoldsijΠ represents the redistribution by theijpressure fluctuations and ε ijis the dissipationterm of the Reynolds stresses transport equations.The pro<strong>du</strong>ction term doesn’t need mo<strong>de</strong>lling, butclosures are required for the redistribution and thedissipation terms. For this purpose, the standardsecond or<strong>de</strong>r turbulence mo<strong>de</strong>l, in homogeneousturbulence, proposed by Laun<strong>de</strong>r <strong>et</strong> al. [10] isused. Thus, the terms of right hand si<strong>de</strong> oftransport equation (7) are written as follows:⎛⎞⎜∂U' ' j ' ' ∂UiP = − u u + u u ⎟(8)iji kj k⎜⎟⎝∂x∂xkk ⎠⎛ ⎞ ε ⎛⎞Πij= −γ⎜ P −2 ' 2ijPδij ⎟ − C ⎜uiu'j− kδij ⎟ (9)1⎝ 3 ⎠ k ⎝ 3 ⎠2ε ij= εδ ij(10)3where P = trace( P ii); C1= 1. 8 and γ = 0. 6 .According to equation (10), thedissipation rate of the turbulent energy εis assumed to be isotropic in accordancewith the local isotropy hypothesis. Th<strong>et</strong>ransport equation of the dissipation rateε is mo<strong>de</strong>lled using a classical transportequation. In homogeneous uniformlysheared turbulence, this transportequation writes:2Dεε ' ' ∂Uε= −Cu v − C(11)1ε2εDt k ∂ykWhere C1 ε= 1. 44 and C2 ε= 1. 9 . And th<strong>et</strong>ransport equations of the principal componentsthe Reynolds stress tensor are finally mo<strong>de</strong>led as:DuDt'2DvDt'2Du vDt' ' ∂U= −2u v −∂y− Cε ⎛⎜uk ⎝2ε32 ⎞ ⎛− k ⎟ − ⎜ P −113 ⎠ ⎝'2γ123⎞P⎟⎠(12)⎛ ⎞= −2 ε ' 2ε − C ⎜v2− k1 ⎟3 k ⎝ 3 ⎠⎛ 2 ⎞− γ ⎜ P − P⎟(13)22⎝ 3 ⎠∂U∂yεk' ''2' '= −v− C u v − γP(14)112A two-dimensional numerical co<strong>de</strong> hasbeen <strong>de</strong>veloped for parabolic flowresolution. The numerical m<strong>et</strong>hod isbased on a finite-difference scheme andthe equations are solved with an explicitm<strong>et</strong>hod.Because the turbulent passive scalar fluxdoes not affect the velocity field, we firststarted by validating the second or<strong>de</strong>rturbulence mo<strong>de</strong>l. The full equations ofthe second or<strong>de</strong>r mo<strong>de</strong>l wereapproximated by finite difference schemeand solved. For this purpose, the inl<strong>et</strong>conditions were suitably adjusted in or<strong>de</strong>rto repro<strong>du</strong>ce the evolution of theReynolds stress tensor. The numericalresults are confronted to the DirectNumerical Simulation (DNS) data ofRogers <strong>et</strong> al. [1] obtained inhomogeneous turbulent pure shear flowwith a constant mean shear and aconstant mean temperature gradient inthe x 2 direction. Figure 1 show goodagreement b<strong>et</strong>ween the numerical resultsand the DNS data of Rogers <strong>et</strong> al. [1].168

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