stefan_boltzmann_law | R Documentation |

Calculates the radiant emittance of a body as a function of its absolute temperature.

stefan_boltzmann_law(temp, epsilon = 1)

`temp` |
absolute temperature (K) |

`epsilon` |
body's emissivity (adimensional between 0 and 1). A value of 1 calculates black body radiant emittance. |

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