haruspex said:
That a parcel of air expands, and therefore cools, as it rises cannot stand alone as an explanation for why it is cooler with increasing altitude. If the atmosphere were the same temperature (and same composition) all the way up, there would be no convection. So we have to start with why that is not the situation.
There would be no conduction, but not necessarily no convection. To have no convection the atmosphere would have to be isothermal and be in hydrostatic equilibrium.
The answer to your question, "why is that not the situation", is simple: The planet surface is at a different temperature from that of the atmosphere. Planetary rotation (at a rate other than the orbital rate) alone will make this happen. You don't need greenhouse gases to get advection. Those greenhouse gases however do play a very important role.
The U Texas site linked above gets part of the way there, explaining that the lower atmosphere is heated from below. To complete the picture, you have to have the upper layers of the troposphere losing heat upwards. If the atmosphere were composed entirely of O2 and N2, there would be no mechanism for this, and it would all be at the same temperature as the Earth's surface. The presence of GHGs - H2O mostly - is the key.
I agree that the presence of greenhouse gases is the key to how our real atmosphere behaves. I disagree as the lack of greenhouse gases would not create an isothermal atmosphere, at least not near the surface.
An atmosphere that is transparent to both incoming solar radiation and outgoing thermal radiation would be very different from our actual atmosphere. With a transparent atmosphere there would be huge day/night temperature extremes on the planet's surface, similar to those on the Moon. These huge swings would drive the behavior of the atmosphere near the surface. Daytime temperatures in the atmosphere near the surface would drop at the adiabatic rate (the dry adiabatic rate; a transparent atmosphere rules out H
2O) as surface air heated by the planet rises. The rapid daytime heating of the surface precludes an isothermal atmosphere, at least near the surface during daytime. There would be an isothermal atmosphere above a rather low altitude that varies with time of day, nearly touching the Earth at the dawn boundary.
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To get back to the OP's (chingel's) confusion, one needs to look at what causes temperature to vary within the atmosphere. There are four primary mechanisms:
- Conduction at the surface of the Earth,
- Adiabatic cooling/heating as parcels of air rise/fall,
- Atmospheric mixing as those moving parcels mix with the air around them,
- Radiative transfer, which is only possible due to the presence of greenhouse gases, and
- Diffusion, or molecular level heat transfer.
Diffusion would slowly drive the atmosphere to an isothermal state were it not for those first four mechanisms. Diffusion is very slow compared to those first four, making diffusion pretty much a non-factor given that those first four mechanisms do exist.
It's important to understand that second process, adiabatic cooling and heating. This is where I think chingel still has problems. A rising or sinking parcel of air isn't subject to conduction; that happens at the Earth's surface. The parcel is mixing only at its periphery, and only slightly, so that is a non-factor. Radiative transfer is typically slow, so that too is a non-factor. There is effectively no heat transfer with the environment, so adiabatic conditions apply. Couple this adiabatic behavior with the decrease in pressure with increasing altitude and the parcel must decrease in temperature as it rises. It's a simple matter of thermodynamics.
The parcel will stop rising eventually. If nothing else, it will hit the tropopause. There is very little mixing between the troposphere and stratosphere because a temperature inversion exists at the boundary between the two layers. Typically a rising parcel will stop rising long before the tropopause. One reason is that the environmental lapse rate is typically less than the adiabatic lapse rate. Rising air under such conditions quickly cools to a point where the temperature is equal to that of the surrounding environment. This stops the rise in its tracks. This is a stable atmosphere; not much is happening here.
The environmental lapse rate can at times be higher than the adiabatic lapse rate. The rising air continues to rise, eventually reaching a point where the relative humidity is 100%. The release of energy from condensation counteracts the cooling to some extent (the moist adiabatic rate is only 6°/km, about 4°/km less than the dry rate). These rising parcels of air in an unstable atmosphere are what give us our weather. The net result is to cool the surface of the Earth and heat the atmosphere.
Radiative transfer has the opposite effect. It acts to raise the temperature of the surface of the Earth and reduce the temperature of the atmosphere. Radiative transfer and advection battle one another. Note that there is no radiative transfer without greenhouse gases. Our weather depends on those greenhouse gases.