.Buildings.ThermalZones.Detailed.BaseClasses.InfraredRadiationExchange

Information

This model computes the infrared radiative heat transfer between the interior surfaces of a room. Each opaque surface emits radiation according to

Ei = σ   Ai   εi   (Ti)4,

where σ is the Stefan-Boltzmann constant, Ai is the surface area, εi is the absorptivity in the infrared spectrum, and Ti is the surface temperature. If the parameter linearizeRadidation is set to true, then the term (Ti)4 is replaced with T03 Ti, where T0 = 20°C is a parameter.

The incoming radiation at surface i is

Gi = -∑j   Fj,i   Jj

where Fj,i is the view factor from surface j to surface i, Jj is the radiosity leaving surface j and the sum is over all surfaces. For opaque surfaces, it follows from the first law that the radiosity Ji is

Ji = -Ei - (1-εi)   Gi.

For windows, the outgoing radiosity is an input into this model because the window model computes this quantity directly.

For each surface i, the heat balance is

0 = Qi + Ji + Gi.

For opaque surfaces, the heat flow rate Qi is set to be equal to the heat flow rate at the heat port. For the glass of the windows, the radiosity outflow at the connector is set to the radiosity Gi that is leaving the surface.

The view factor from surface i to j is approximated as

Fi,j = Aj ⁄ ∑k Ak.

Revisions


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