In this video we solve three examples using the Stefan Boltzmann Law. The Stefan Boltzmann Law describes the emissive power of a blackbody in a vacuum, and can be adjusted to be used on real bodies through the addition of the emissivity term.
This timeline is meant to help you better understand how to solve problems using the Stefan Boltzmann Law:
0:00 Introduction.
0:06 Review of the Stefan Boltzmann Law.
0:30 Stefan Boltzmann Law Example 1.
1:45 Stefan Boltzmann Law Example 2.
3:21 Stefan Boltzmann Law Example 3.
4:45 Outro
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This video is part of our Heat Transfer course. Heat Transfer is an interesting field of study and focuses primarily around the three modes of heat transfer, that is conduction, convection and radiation. This is taught in just about all engineering courses and I hope that this playlist will make what is typically considered a tough course much easier for you.
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The constant is 5.67×10^-8 w m^-2 k^-4
It would be beter if you use W for power and not KW, because people can confuse it with K(Kelvin).
super
THANK YOU SO MUCH FOR THE EXCELLET EXPLANATION, YOU REALLY DID HARDWORK WHICH I APPRICIATE THANKS ALOT
What does Eb stand for?
Great video
شكرا الك مبدع ولله