1. What is Stefan boltzmann Law? According to Stefan boltzmann law, the amount of radiation emitted per unit time from an area A of a black body at absolute temperature T is directly proportional to the fourth power of the temperature
Stefan
2. Stefan boltzmann Constant is denoted by Greek letter σ
Stefan
3. The Stefan boltzmann Constant, σ, is equal to 5.67 x 10-8 W/(m2 • K4)
Stefan
4. Stefan boltzmann constant – Uses and application
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5. Stefan boltzmann Law is also known as Stefan's Law
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6. The Stefan boltzmann Law is a means of determining total energy radiated by any object, based entirely on its temperature
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7. Set this parameter equal to the Stefan boltzmann constant
Set, Strong, Stefan
8. For example, Stefan boltzmann = 5.669 × 10 −8 joule per sec m 2 kelvin 4 in SI units
Strong, Stefan, Sec, Si