Andre
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haruspex said:no?
No, you really need to have a good look at convection. Let's try another example, let's take the moon. Daytime temperature at the equator reaching up to 390K and nighttime only 100K. Now imagine hypothetically, that we give the moon an atmosphere of N2 and O2 only, which are almost transparant for both visible light and infrared.
So looking at a certain part on the equator, as the sun rises it starts heating the moon surface only from 100K slowly to 390K at zenith, the surface infrared radiation increases - counteracting the radiation inbalance, but that does nothing with our hypothetically transparent atmosphere. The radiation disappears into space.
But the heated surface also agitate the N2 and O2 molecules directly in contact with the surface, conduction of heat. This hot boundary layer gets less dense and the buoyancy causes it to rise. A hot air balloon without a balloon. As it rises into less dense pressure heights, it expands, which cools it adiabatically, but the surrounding atmosphere is also cooling with altitude, so as long as the rising air remains warmer than the environment, it continues to rise. On the Earths equator deep convection in the Hadley cell may continue to the tropopause.
Obviously, in this process, the molecules at the surface boundary layer are replaced with others which heat up at their turn and because of that start to rise too, etc etc. creating a vertical heat circulation system in the hypothetical atmosphere.
When the sun sets, the moon surface cools rapidly, due to out radiation of infra red. This still doesn't change anything in the inert transparent atmosphere. But as the surface cools so does the boundary layer of the atmosphere at the surface due to conduction, the molecules slow down hence it gets more dense, hence less buoyant and therefore it stays put*. There is no negative convection. Consequently, lacking radiative properties, the higher parts of the hypothetical atmosphere have no other means to cool down by conduction by contact with the lower boundary layer and obviously that is very ineffective.
So as the daily cycle repeats, the one way heat transport into the atmosphere continues until equilibrium, when the rising cooling air is equal in temperature with the environment, so that even at the highest surface temperature, there is no more convection.
Note also that this doesn't change the heating-cooling sequence of the moon surface a lot, the exchange of heat energy merely slows down the heating and cooling rate a little bit. Bottom line is that if the atmosphere can't radiate heat out, it continues to accumulate heat by means of convection until equilibrium with the highest temperature is reached, not the 'grey' body temperature.
* (we see that on Earth too, it's called ground inversion).
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