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Krishna
2024-11-17 17:37:11 -06:00
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content/physics/thermodynamics.md
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@@ -99,7 +99,7 @@ $$
$$
Albedo is given by:
$$
\alpha=\frac{P_\text{reflected}{P_{\text{incoming}}}}
\alpha=\frac{P_\text{reflected}}{P_{\text{incoming}}}
$$
This is where the Boltzmann law comes in to play. In order to calculate the emissivity of an object, you first need bot: the power of emissions from the target object, and the Power that would be emitted by a black body of the same temperature. This value can be procured using the Stefan Boltzmann Law of Radiation.