Method
For a surface that effectively views uniform surroundings, Q̇ = ε × F × σ × A × (Ts4 − Tsur4). Temperatures must be absolute temperatures, so the calculator converts °C and °F to kelvin before applying the fourth-power relation.
Worked example
A 1 m² surface at 80 °C with ε = 0.9 and F = 1 facing 20 °C surroundings emits roughly 417 W of net thermal radiation under this simplified model. At the same conditions for one hour, that is about 0.417 kWh.
Important limits
This calculator is a first-pass enclosure model. It does not account for multiple surfaces, reflected radiation, participating gases, convection or conductive heat paths. Use a radiation-network method for an enclosure with several effective surfaces or a detailed view-factor analysis.
Frequently asked questions
What radiation equation does this calculator use?
It uses Q̇ = ε × F × σ × A × (Ts⁴ − Tsur⁴), where ε is emissivity, F is the effective view factor and σ is the Stefan-Boltzmann constant. Temperatures are converted to kelvin before the equation is applied.
When should the effective view factor be 1?
Use 1 when the whole emitting surface effectively sees the stated large uniform enclosure. For smaller targets or several facing surfaces, use a radiation-network method rather than treating the view factor as a complete geometry model.
Why can the result be negative?
A negative result means the surface is cooler than the stated surroundings, so it absorbs more thermal radiation than it emits. It does not mean the calculation has failed.
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