Sorry, Wogoga, you're simply wrong; you are probably used to thinking about buoyancy only for incompressible objects and incompressible fluids.
Ben, I've changed my mind several times. Just after having convinced myself once again that I'm rather wrong than right, I noticed in the
table posted by Ziggurat in post #19 a column with the name
Autoconvective Lapse Rate. Its value is 47 K/Km for Venus, which comes quite close to my above rough calculation (showing that vertical convection on Venus near ground only starts if actual lapse rate is higher than around 50°K/Km).
Then I found this quote from
Basic Convection (for students of meteorology):
In many situations, surface heating is so intense that even convection is not enough to transfer the heat. This condition can happen near the surface in quite shallow layers, at locations where the vertical motions generated by convection are limited by the shallowness of the layer. Then it is possible for extremely high lapse rates to develop. The lapse rate can become sufficiently high so that density increases with height. It can be shown that a hydrostatic atmosphere in which density doesn’t change with height has a lapse rate of g/R. This rate turns out to be about 34 C km-1 [on Earth] and is known as the autoconvective lapse rate. If the environmental lapse rate exceeds this value, not even a butterfly’s flapping is necessary to initiate overturning; overturning is spontaneous in the same way that a brick held and then released in the air falls spontaneously!
Perhaps the answer is more obvious if you treat it as a Hamiltonian system---does the system's total gravitational potential energy increase, or decrease, as the *net* effect (including adiabatic heating, hydrostatic pressure increase, etc.) of swapping Air Parcel #1 with Air Parcel #2?
Sounds reasonable.
If the answer is "decrease", then there's a buoyancy force working to carry out that swap.
It is rather the contrary: If actual lapse rate is between adiabatic (10.5°C/Km on Venus) and autoconvective (47°C/Km) lapse rate, then only a forced vertical convection
opposing buoyancy can start a movement. Buoyancy itself has a stabilizing effect.
Only after a movement in the right direction has started, it is more and more reinforced by buoyancy, because adiabatic temperature changes (in function of changing height) are weaker than corresponding volume changes. In the case of sinking air parcels, this means that, as long as they sink, they become heavier and heavier in comparison with their environment.
Thus, an actual lapse rate between the adiabatic and the autoconvective one leads rather to what can be called a
meta-stable atmosphere. I do not exclude that actual lapse rate on Venus may have been in the lower meta-stable range over hundreds of millions of years.
A further quote from
Basic Convection:
Unless the lapse rate exceeds the autoconvective, the parcels will not rise spontaneously.
Anyway, as actual lapse rate on Venus is even lower than the adiabatic one, your claim of post #75 that heating the atmosphere from the crust would predict "
that the lower atmosphere is circulating like crazy due to convection" is simply untenable.
Cheers, Wolfgang