Heat flux calculation in radiative heat transfer
The thermal solver computes the incident, reflected, absorbed, and transmitted energy fluxes for radiative heat transfer analysis.
Total incident heat flux
Radiated heat flux tracked through the system for ray-traced heat flux view factors.
Radiated heat flux tracked through the system for non-ray-traced heat flux view factors.
Heat flux absorbed by the element ifor non-ray-traced heat flux view factors.
The total incident diffuse flux on element i of the heat flux view factor Vi.
Heat flux reflected specularly for ray-traced heat flux view factors.
Heat flux reflected specularly for non-ray-traced heat flux view factors.
Heat flux transmitted through a material for ray-traced heat flux view factors.
Heat flux transmitted through a material for non-ray-traced heat flux view factors.
In these equations:
- Vi is the heat flux view factor, albedo factor, Earth view factor, or heat flux view factor to the element.
- Ai is the area of the element. If VFMERGE option is used, this is the merged area of the element.
- τi is the transparency of element i.
- ρsi is the average specular reflectivity, calculated by averaging the data in the array.
- PS is the emitted power per unit area of the source element. PS is the collimated solar spectrum radiative source's (sun's) power output per unit area arriving at the element for solar or albedo calculations, and the heat load per unit area leaving the surface of the Earth for IR spectrum calculations. PS=1 for heat flux view factor calculations because Vi already includes the source element’s emitted power per unit area.