Originally posted by Phobos Although I have to wonder about the different cloud bands being as, or more important, than the Coriolis effect. Would a differential in the velocity of the upper and lower cloud bands keep the GRS going? Anyone have info on this?
O.K. I found out the answer. You were on the verge of it here, Phobos.
Here is how the coriolis effect figures into the GRS:
As Phobos uncovered, the GRS is a high pressure island. This would imply, by Earth weather standards that it is a subsiding, sinking area of cooler temperature gas that is thereby denser. This is what differentiates it from the surrounding lower pressure atmosphere to begin with.
It should dissipate into the lower pressure and disappear but it doesn't. Some dynamic is keeping it contained, or perhaps feeding it roughly in proportion to whatever high pressure it may lose.
(That's a different topic. My question is about how the coriolis effect figures in.)
As the presumedly more dense atmosphere rotates beneath it, the edge of the spot closer to the equator is subjected to greater surface speeds, running along beneath, than the edge farther away from the equator. If we say, for instance, that one edge is just touching the equator and the other is touching a tropic, the edge at the equator will have a greater circumference running beneath it than the edge at the tropic. This imbalance of force between the two edges is, obviously, what torques the GRS.
I was having a hard time figuring out where the torque was coming from. I see now that it is the result of two different surface speeds arising from the spherical shape of the planet.
(I discovered, too, that winds will take a different route around a high pressure area than they do around a low pressure area, and that these directions are flopped, mirror-like; Those in the northern hemisphere are enantiomorphs, so to speak, of those in the southern.)
-Zooby