1 / 21

Understanding Reynolds-Averaged Navier-Stokes Equations: Modeling and Numerical Methods

Explore the fundamentals of Reynolds Averaged Navier-Stokes equations (RANS) with a focus on turbulence modeling and numerical solutions. Learn about modeling Reynolds stresses, eddy viscosity models, turbulent viscosity, and General Transport Equation.

palmerr
Download Presentation

Understanding Reynolds-Averaged Navier-Stokes Equations: Modeling and Numerical Methods

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. Objective • Review Reynolds Navier Stokes Equations (RANS) • Learn about General Transport equation • Start with Numerics

  2. From the previous classReynolds Averaged Navier Stokes equations Reynolds stresses total 9 - 6 are unknown (incompressible flow) same Total 4 equations and 4 + 6 = 10 unknowns We need to model the Reynolds stresses !

  3. From the previous classModeling of Reynolds stressesEddy viscosity models Average velocity Boussinesq eddy-viscosity approximation Is proportional to deformation Coefficient of proportionality k = kinetic energy of turbulence Substitute into Reynolds Averaged equations

  4. From the previous classReynolds Averaged Navier Stokes equations Continuity: 1) Momentum: 2) 3) 4) Similar is for STy and STx 4 equations 5 unknowns → We need to model

  5. Modeling of Turbulent Viscosity Fluid property – often called laminar viscosity Flow property – turbulent viscosity MVM: Mean velocity models TKEM: Turbulent kinetic energy equation models Additional models: LES: Large Eddy simulation models RSM: Reynolds stress models

  6. Kinetic energy and dissipation of energy Kolmogorov scale Eddy breakup and decay to smaller length scales where dissipation appear

  7. One equation models: Prandtl Mixing-Length Model (1926) Vx y x l Characteristic length (in practical applications: distance to the closest surface) -Two dimensional model -Mathematically simple -Computationally stable -Do not work for many flow types There are many modifications of Mixing-Length Model: - Indoor zero equation model: t = 0.03874  V l Distance to the closest surface Air velocity

  8. Two equation turbulent model model Energy dissipation Kinetic energy From dimensional analysis constant We need to model Two additional equations: kinetic energy dissipation

  9. Reynolds Averaged Navier Stokes equations Continuity: 1) Momentum: 2) 3) 4) General format:

  10. General CFD Equation Values of , ,eff and S

  11. Numerics

  12. - Conservation of ffor the finite volume Divide the whole computation domain into sub-domains Finite Volume Method One dimension: n h P E W dx dx w e s Dx w e l - Finite volume is a fixed space in the flow domain with imaginary boundaries that allow the fluid to flow in and out. - Integral conservation of the quantities such as mass, momentum and energy. f

  13. General Transport Equation -3D problem steady-state H N W E P S L Equation for node P in the algebraic format:

  14. 1-D example of discretization of general transport equation dxw dxe P Steady state 1dimension (x): E W Dx e w Point W and E represent the cell center of the west and east neighbors of cell P and w, e the neighboring surfaces. Integrating with Gaussian theorem on this control volume gives: To obtain the equations for the value at point P, assumptions are used to convert the surface values to the center values.

  15. Convection term dxw dxe P E W Dx e w – Central difference scheme: - Upwind-scheme: If Vx>0 and and If Vx<0

  16. Diffusion term dxw dxe P E W Dx e w

  17. Summary: Steady–state 1D I) X direction If Vx > 0, If Vx < 0, Convection term - Upwind-scheme: P E W dxe dxw and a) and Dx e w Diffusion term: b) When mesh is uniform: DX = dxe = dxw Assumption: Source is constant over the control volume Source term: c)

  18. 1D example - uniform mesh After substitution a), b) and c) into I): We started with partial differential equation: same and developed algebraic equation: We can write this equation in general format: Unknowns Equation coefficients

  19. 1D example multiple (N) volumes N unknowns i N 1 2 N-1 3 Equation for volume 1 N equations Equation for volume 2 …………………………… Equation matrix: For 1D problem 3-diagonal matrix

  20. 3D problem Equation in the general format: H N W E P S L Wright this equation for each discretization volume of your discretization domain A F 60,000 elements 60,000 cells (nodes) N=60,000 = x 60,000 elements 7-diagonal matrix This is the system for only one variable ( ) When we need to solve p, u, v, w, T, k, e, C system of equation is larger

  21. Convection term dxw dxe P E W Dx e w – Central difference scheme: - Upwind-scheme: and and

More Related