Lab Instructions: Climatological Structure of the Atmosphere
Part I: Latitudinal temperature structure and baroclinic instability
In this experiment, we will try to set up a system that allows us to see rotational dynamics at work. We take a cylindrical fish tank, filled with clear water. In the center of the tank we place a thin cylinder, sealed at the bottom, filled with red-colored fluid that is denser than the surrounding fluid. If we then remove the seal at the bottom of the cylinder, thus allowing the two fluids to come into contact, what happens? Observe how the water moves from the cylinder to the rest of the tank and how long it takes to reach a final equilibrium. Sketch what the pressure gradient force would be at the moment the bottom seal is removed and the fluid of different densities come into contact. No, you will not "see" the pressure gradient force, but knowing the densities of the two fluids, you should be able to sketch it.
Compared with real atmospheric circulation, the scale of motions in the tank is so small that the Coriolis force does not matter much. The previous experiment therefore gives you an idea of how atmospheric or ocean circulation might behave on a non-rotating planet. But what will happen on one that is rotating? Let's repeat the previous experiment on a rotating table. The rotation of the table introduces the "Coriolis effect." What will happen this time? Observe the differences and sketch the final equilibrium state as well as the pressure gradient force. If you have any background in mechanics or physics, think about the force balance.
Data