Abstract

Presented article shows rigorous method how derive non-stationary turbulent boundary layer equations by perturbation analysis. The same method is used for analysing behaviour of “k-omega” and “k-epsilon” turbulent models. The analysis is divided into two parts: near wall behaviour – boundary conditions, and behaviour in “log-layer” – wall functions. Both parts have important place in CFD. Boundary conditions are important part of CFD. “k-omega” and “k-epsilon” are related by one simple formula, but they yield to different solutions. Exact values for k, omega and epsilon on a wall are evaluated and all theoretical results are compared with numerical solutions. Special treatment is dedicated to “k-epsilon” model and Dirichlet boundary condition for “epsilon, instead of standard Neumann boundary condition. “Log-Layer” is well known from experiments and it is used for setting constants in turbulent models. Standard equations are derived by perturbation analysis. In presented article are these equations derived with 3 more terms, than in standard case. This yields to sharper approximation. These new equations are solved and solution is a bit different, than in standard case. Due to 3 extra terms is possible to get better approximation for k and new view into problematic..

Highlights

  • Two equations turbulent models are widely used in CFD - they give ”good” results in ”good” time

  • The analysis is divided into two parts: near wall behaviour - boundary conditions, and behaviour in ”log-layer” - wall functions

  • Boundary conditions are important part of CFD. ”k-omega” and ”k-epsilon” are related by one simple formula, but they yield to different solutions

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Summary

Introduction

Two equations turbulent models are widely used in CFD - they give ”good” results in ”good” time. The most common are ”k − ω” and ”k − ε”. This article is about turbulent boundary layer equations and perturbation analysis of turbulent models - on a wall and in ”log-layer”. On a wall - boundary conditions, and in “log-layer” - wall functions. We need to close the Navier-Stokes equations by a turbulent model. K is called kinetic turbulent energy, is called dissipation of turbulent energy.

Turbulent boundary layer equations
Behaviour on a wall and boundary conditions
Wall functions
Impossibility theorem
Comparison and figures
Conclusion
Full Text
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