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Stellar mixing - I.?Formalism

机译:恒星混合-I.形式主义

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In this paper we use the Reynolds stress models (RSM) to derive algebraic expressions for the following variables: a) heat fluxes; b)?μ fluxes; and c) momentum fluxes. These relations, which are fully 3D, include: 1) stable and unstable stratification, represented by the Brunt-V?is?la frequency, ; 2) double diffusion, salt-fingers, and semi-convection, represented by the density ratio Rμ?=??μ(?????ad)-1; 3) shear (differential rotation), represented by the mean squared shear Σ2 or by the Richardson number, Ri?=????N2Σ-2; 4) radiative losses represented by a Peclet number, Pe; 5) a complete analytical solution of the 1D version of the model. In general, the model requires the solution of two differential equations for the eddy kinetic energy K and its rate of dissipation, ε. In the local and stationary cases, when production equals dissipation, the model equations are all algebraic.
机译:在本文中,我们使用雷诺应力模型(RSM)导出以下变量的代数表达式:a)热通量; b)?μ通量; c)动量通量。这些完全为3D的关系包括:1)以Brunt-V?isla频率表示的稳定和不稳定分层; 2)以浓度比Rμπ=Δεμ(ΔεΔεad)-1表示的双扩散,盐指和半对流; 3)剪切力(微分旋转),由均方剪切力Σ2或理查森数(Ri?= ????N2Σ-2)表示; 4)用佩克利数Pe表示的辐射损耗; 5)一维模型的完整分析解决方案。通常,该模型需要两个微分方程的解来求解涡动能K及其耗散率ε。在局部和固定情况下,当生产等于耗散时,模型方程都是代数的。

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