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

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Annexe Chapitre 2equation of the scalar flux, can beconcisely written as:D ' 'u iθ = Pθi+ Πθi− εθi(3)Dtwhere P θ iis the pro<strong>du</strong>ction term, Πθiis thepressure-scalar gradient correlation and εθiis thedissipation of the scalar flux.Laun<strong>de</strong>r <strong>et</strong> al. [10] assumed that thedissipation term is negligible at highReynolds number but the two terms Π<strong>et</strong> ε are usually mo<strong>de</strong>lled tog<strong>et</strong>her andθisimilar m<strong>et</strong>hods than those used in theclosure of the Reynolds Stress transportequation are used [5, 6]. Wikström <strong>et</strong> al.[6] proposed a closure of the differenceb<strong>et</strong>ween the pressure-scalar gradientcorrelation and the dissipation term in thefollowing general form:⎛ k ⎞' '⎜∂ΘC C u ⎟ε ' 'Π − ε = −ui i+ θmiq xθθ θθ1θ 5⎝ ε ∂ km ⎠∂U∂U' ' i' ' j+ Cθ2ujθ+ Cθ3ujθ∂x∂xji' ' ∂Θ+ C u uθ 4 i j(4)∂xjwhere Cθ1, Cθ 2, Cθ 3, Cθ 4and Cθ 5are constants,'2' 'θuq = is the scalar variance,iuk = iis the22turbulent kin<strong>et</strong>ic energy and ε its dissipation rate.In homogeneous turbulence, the transport equationof q writes:Dq = Pθ − ε θDtwhereθi(5)= u'jθ 'θis a pro<strong>du</strong>ction term of the∂xjP∂Θ' '∂θ∂θscalar variance q , ε θ= σ is its∂x∂x j jdissipation rate. The transport equation of ε θismo<strong>de</strong>lled according to Abe <strong>et</strong> al. [4] and Farshchi<strong>et</strong> al. [11].2D ε P Pθ θ * ε εθθ * εεθε = C + C − C − C (6)θ γ 1γ 1γ 2γ 2Dt 2qk 2qk**where C ,γ 1C , C and C are constants and Pγ 2 γ 1γ 2is the pro<strong>du</strong>ction term of the Reynolds stress.The mo<strong>de</strong>l of the pressure-scalar gradientcorrelation proposed by Wikström <strong>et</strong> al.[6] which comprises five constants,generalizes a certain number of existingmo<strong>de</strong>ls. When only the first constant isr<strong>et</strong>ained with the value Cθ1= 3. 2 , themo<strong>de</strong>l (4) re<strong>du</strong>ces to the linear mo<strong>de</strong>l oflaun<strong>de</strong>r [9]. When the constant C θ 2isad<strong>de</strong>d, we obtain the non linear mo<strong>de</strong>l ofLaun<strong>de</strong>r [9] with Cθ 2= 0. 5 or the nonlinear mo<strong>de</strong>l Daly and Harlow [12] withCθ 2= 1. Wikström <strong>et</strong> al. [6] tried differentmo<strong>de</strong>ls using different combinations andformulations of the constants in themo<strong>de</strong>l (4) as illustrated in table 1.Table 1: Different formulations of the pressure-scalargradient mo<strong>de</strong>l (equation 4) Wikström <strong>et</strong> al. [6]Mo<strong>de</strong>l Cθ1Cθ 2Cθ 3Cθ 4Cθ 5(a) 3.2 0.5 0.5 0 0(b) 2.5 0 0 0.35 0(c)r + 11.6r0 0 0 0.5In the mo<strong>de</strong>l (c), Wikström <strong>et</strong> al. [6]qετθ1intro<strong>du</strong>ced the time ratio r = = =kεθτ Rin the formulation of the param<strong>et</strong>er Cθ1.kWhere τ = is the dynamic time scale ofεqturbulence, τ = is characteristic scalartime scale.ε θThe transport equation of the turbulentscalar flux tog<strong>et</strong>her with the transportequations of the scalar variance q and itsdissipation rate ε θallow computing th<strong>et</strong>urbulent scalar flux provi<strong>de</strong>d that the167

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