Stefan-Boltzmann and Wien's laws
Stefan-Boltzmann and Wien's laws are fundamental principles in physics that describe the relationship between temperature and the radiation emitted by objects, including those in remote sensing.
The Stefan-Boltzmann Law states that the total energy radiated by a blackbody is directly proportional to the fourth power of its temperature. Mathematically, it is expressed as:
\[ E = \sigma T^4 \]
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