Thermal Boundary Conditions

When you are simulating non-isothermal flow, you are required to specify how the energy flow across wall boundaries is determined. Simcenter STAR-CCM+ provides various options such as defining an adiabatic wall, prescribing a fixed wall temperature, or assuming convective flow at the external side of the boundary.

The following diagram illustrates the heat transfer at a wall boundary with one of its neighboring cells:

Boundary Inputs

For non-isothermal wall boundaries, depending on the thermal specification, you prescribe the following variables:
Inputs Adiabatic Convection Heat Flux Heat Source Temperature
Static temperature T spec
Heat flux q ˙ s p e c
Heat source S Q
Ambient temperature T
Heat transfer coefficient h ext
Thermal resistance R th

Computed Values

At non-isothermal wall boundaries, depending on the thermal specification at the boundary, Simcenter STAR-CCM+computes the following values at the boundary faces:
  • Static fluid temperature at the wall T w
  • Heat flux q ˙
Adiabatic
An adiabatic wall does not permit heat transfer across the boundary. Therefore:
q ˙ = 0
(1670)
The fluid temperature at the wall is calculated as:
Figure 1. EQUATION_DISPLAY
T w = T s ext
(1671)

where T s ext is the static fluid temperature extrapolated from the near-wall cell center at the interior of the domain.

Temperature

The fluid temperature at the wall is set to the user-specified temperature:

Figure 2. EQUATION_DISPLAY
T w = T spec
(1672)
When the temperature is specified at the boundary, Simcenter STAR-CCM+ calculates the heat flux (without radiation) from the wall into the domain as:
q ˙ = k T w
(1673)

where T w is the temperature gradient at the wall and k is the conductivity.

This is discretized as described by Eqn. (898):

D f = Γ f ϕ f a = Γ f [ ( ϕ 1 - ϕ 0 ) α a + ϕ ¯ a - ( ϕ ¯ ds ) α a ]

where:

  • Γ f = k
  • ϕ f = T w
  • ϕ 0 = T c (the temperature gradient in the near-wall cell)
  • ϕ f = T w
  • ϕ 0 = T c

Prior to taking the dot product with area a, this expression is:

k T = k [ ( T w - T c ) α + T c - ( T c ds ) α ]

Which can be rearranged to:

k T = k [ T c - ( T c ds ) α ] - k α T c + k α T w + 0 T w 4

The wall heat flux q . is linearized as:

Figure 4. EQUATION_DISPLAY
q . = A + B T c + C T w + D ( T w ) 4
(1675)

where T c and T w are the cell and wall temperatures, respectively. A, B, C, and D are the net wall heat flux coefficients.

The internal heat flux coefficients are then obtained as:

  • A internal = k [ T c - ( T c ds ) α ]
  • B internal = - k α
  • C internal = k α
  • D internal = 0
Heat Flux
For this thermal specification, you specify the heat flux density q ˙ at a wall. From this heat flux density, Simcenter STAR-CCM+ computes the fluid temperature at the wall according to:
Figure 5. EQUATION_DISPLAY
T w = q ˙ s p e c k
(1676)

The same linearization applies as described for the temperature specification.

Convection
The convection wall boundary takes into account a convective heat flux from the environment to the external side of the boundary:
q ˙ = h e x t ( T w T )
(1677)

where T is the user-specified ambient temperature and h ext is the user-specified heat transfer coefficient outside the fluid domain.

The conductive heat flux is given by Eqn. (1673). The heat flux q ˙ and the fluid temperature at the wall T w are then determined iteratively.

Through a user-specified thermal resistance R th , you can model a fictitious thickness of the wall boundary:
Δ = 1 R th
(1678)
This fictitious wall thickness allows you to consider heat conduction through the wall as if it were a solid. However, the thermal resistance does not take into account the thermal capacity nor heat conduction in the lateral direction of the wall.
Heat Source
You specify the total heat Q ˙ over the entire wall boundary. Simcenter STAR-CCM+ imposes:
q ˙ = Q ˙ A
(1680)

where A is the area of the wall boundary.