The Stefan-Boltzmann law describes the relationship between the temperature of a blackbody and its total energy radiated per unit surface area. The formula for outgoing longwave radiation (L) is given by:
sigma = Stefan-Boltzmann constant (5.67 Γ 10β»βΈ W mβ»Β² Kβ»β΄)
T = Absolute temperature in Kelvin
What is longwave radiation?
How does temperature affect outgoing longwave radiation?
What is the Stefan-Boltzmann constant?
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What is the formula for outgoing longwave radiation?
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