Climate scientists use the StefanBoltzmann Law R = T 4 to estimate the change in the
Chapter 3, Problem 94(choose chapter or problem)
Climate scientists use the StefanBoltzmann Law R = T 4 to estimate the change in the earths average temperature T (in kelvins) caused by a change in the radiation R (in joules per square meter per second) that the earth receives from the sun. Here, = 5.67 108 Js1m2K4. Calculate dR/dt, assuming that T = 283 and dT dt = 0.05 K/year. What are the units of the derivative?
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