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en:praktikum:sunspot-temp [2014/12/11 20:33] – msteinke | en:praktikum:sunspot-temp [2016/06/28 00:15] (current) – [Theory] rhainich | ||
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===== Theory ===== | ===== Theory ===== | ||
- | The Stefan-Boltzmann law gives a correlation between emitted radiative power P of a black body, the emitting area A and its absolute temperature T: | + | The Stefan-Boltzmann law gives a correlation between emitted radiative power P of a black body, the emitting area A, and its absolute temperature T: |
- | < | + | \begin{equation*} |
P = \sigma \cdot A \cdot T^4 | P = \sigma \cdot A \cdot T^4 | ||
- | </ | + | \end{equation*} |
For details, see the relevant literature or [[https:// | For details, see the relevant literature or [[https:// |