Use The Model In Fig 3 10 But Distribute The Solar Heating Such That 0 3sigmate

use the model in fig 3.10, but distribute the solar heating such that 0.3sigmaTe^4 is absorbed in each of the two atmospheric layers and the remaining 0.4sigmaTe^4 is absorbed at the surface. Calculate the new radiative equilibrium temperature profile. How does it differ from the case where all of the solar heating is applied at the surface?

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