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Stefan–Boltzmann Radiation

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Net radiative heat transfer between two grey surfaces: Q = ε·σ·A·(T₁⁴ − T₂⁴).

Formula

$$ Q = \varepsilon \cdot \sigma \cdot A \cdot (T_1^4 - T_2^4), \; \sigma = 5.67 \times 10^{-8} $$

Symbol legend

SymbolMeaningUnitSource
$ε$Emissivity-material property
$σ$Stefan-Boltzmann constantW/(m²·K⁴)5.67e-8
$A$Surface areageometry
$T_1, T_2$Hot and cold surface temperaturesKconverted from °C
$Q$Radiative heat flowkWresult

Sources

  • Incropera - Fundamentals of Heat and Mass Transfer.