Stefan-Boltzmann Law:
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The Stefan-Boltzmann Law describes the power radiated from a black body in terms of its temperature. Specifically, it states that the total energy radiated per unit surface area of a black body across all wavelengths per unit time is directly proportional to the fourth power of the black body's thermodynamic temperature.
The calculator uses the Stefan-Boltzmann Law:
Where:
Explanation: The law quantifies the relationship between temperature and radiant energy emission, with real-world objects having emissivity values less than 1 (perfect black body).
Details: Calculating emitted power is crucial for thermal management, climate studies, energy efficiency assessments, and various engineering applications in South Africa's diverse climate conditions.
Tips: Enter emissivity (between 0 and 1) and temperature in Kelvin. Ensure values are within valid ranges for accurate results.
Q1: What is emissivity?
A: Emissivity is the measure of an object's ability to emit thermal radiation compared to a perfect black body (which has emissivity = 1).
Q2: Why is temperature in Kelvin?
A: The Stefan-Boltzmann law requires absolute temperature, and Kelvin is the SI unit for thermodynamic temperature.
Q3: What are typical emissivity values?
A: Black body: 1.0, Human skin: ~0.98, Aluminum foil: ~0.03, Concrete: ~0.85-0.95.
Q4: How does this apply to South Africa specifically?
A: South Africa's varied climate and solar radiation levels make thermal calculations important for building design, agriculture, and energy systems.
Q5: Can this calculate cooling requirements?
A: Yes, the emitted power calculation helps determine radiative heat loss, which is important for thermal management and cooling system design.