Stefan Boltzmann Constant

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Stefan Boltzmann Constant

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(symbol σ). A universal constant of proportionality between the radiant emittance of a black body and the fourth power of the body's absolute temperature; 5.6697 X 10E-5 erg centimeter squared second degrees KE4. [[/a>|/a> ]]

References

This article is based on NASA's Dictionary of Technical Terms for Aerospace Use