Thermal wall function for natural convection
For natural convection in turbulent flows, the flow solver uses a new h correlation derived from a general temperature wall function for natural convection.
For natural convection in turbulent flows, the flow solver uses a new h correlation derived from a general temperature wall function for natural convection. The flow solver computes the temperature wall function [23], which is valid for turbulent natural convection for any Prandtl number, and for any surface inclination. A complete treatment of turbulent natural convection boundary layers includes the implementation of a natural convection velocity wall function. Implementing such a wall function however, has implications in the treatment of the production and the dissipation of the turbulence kinetic energy in the k-epsilon turbulence model.
The flow solver uses the thermal wall function, which takes into account the effect of Prandtl number as well as the influence of the surface angle with respect the gravity vector, in general form:
The coefficients in the thermal wall function are:
Ct is dependent on the Pr number as well as on the angle of surface with respect to the gravity vector. Raithby et al [23] proposed the following general formulation:
with the following definitions for the angle ϕ:
For Tw > 0
- ϕ = 0° if the surface is horizontal, facing upward
- ϕ = 180° if the surface is horizontal, facing downward
for Tw < T0
- ϕ = 0° if the surface is horizontal, facing downward
- ϕ = 180° if the surface is horizontal, facing upward
The correlations of Raithby [23] for Cu is adopted with a small modification to make it compatible with the value of Cu = 0.15 for air. The Cu correlation is:
A new correlation for Cv as a function of Pr is derived so that the Nusselt relationship Nu = CvRa1/3 matches as close as possible: