Radiative Equilibrium Temperature for the Earth
Use Stefan-Boltzman Law
We know that earth emits 240 Watts m-2
Using E = s Te4
then Te = (E/s)1/4
So, for the simplified case of no atmosphere, then Te = ANSWER
Radiative Equilibrium Temperature for the Earth Use Stefan-Boltzman Law We know that earth emits 240 Watts m-2 Using E = s Te4 then Te = (E/s)1/4 So, for the simplified case of no atmosphere, then Te = ANSWER |
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