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Overview

Our world is a complex system. Different types of conservation apply in different regions: conservation of energy and conservation of momentum—as already studied in the previous projects.

If we consider the earth as a one big system, we may find that there is not only one large circulation that transport all the heat from the equator to the poles. In fact, there are couple smaller circulations, due to the effects of rotation, that are responsible to for the heat transportation and effects of the angles between the surfaces and the sun.   In this study, there are two circulation regimes of interest:

1)         The Hadley Cell Circulation: the regime near the equator where the solar radiation strikes the Earth relatively directly and the effects of rotation (Coriolis forces) are small.

2)         The Eddy Cell Circulation: the regime in the mid latitudes where the solar radiation strikes the Earth with relatively indirect and the effects of rotation are slightly biggerADD SOME STUFF ABOUT GENERAL CIRCULATION...

In order to understand the different regimes in the atmosphere, we performed two experiments on rotating tanks of water. Both experiments used the same sized tank, with a metal bucket filled with ice at the center. This setup acted as an analog to the atmosphere on our rotating earth, with the cold polar region reproduced by the ice bucket. Varying the rotation rate of the tank was akin to altering the latitudinal location on the earth. In both experiments, temperature sensors were placed radially along the bottom the the tank to track the movement of heat over the course of the experiment, as well as two 10 cm above - one taped to the ice bucket and one to the edge of the larger tank. Particles were also dropped onto the water to track surface motion, and drops of dye used to visualize flows.

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Hadley

At low latitudes near the equator, atmospheric circulation is mostly axisymmetric. Warm air rises at the equator, moves to about 30ºN or south, where it then descends and returns to the equator. This circulation is called the Hadley Cell, which we will explore in more detail in this section.

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Tank Experiment

In order to imitate the circulation in the low latitudes, the first experiment was performed with a very slowly rotating tank - moving at just 1 revolution per minute. Observed from the counter-clockwise rotating reference frame, particles on the surface circled the tank, moving faster than the speed of the tank's rotation. Those towards the center of the tank were much faster than those on the outside. Dye dropped into the tank created trails that also circled the ice bucket. The dye that sank further moved more slowly and moved slightly radially outwards, while the dye that remained near the surface circled more quickly, and also moved radially inwards. These motions created a lengthening tendril of dye, which, seen from above, appeared to spiral towards the ice bucket.

P1010848.JPG

After many rotations, the spiral eventually morphed into a cone of dye around the ice bucket, just like the cone we saw in the second lab experiment. Potassium permanganate (bright purple streaks below) dropped onto the bottom of the tank also revealed the flows at depth. The dye created streaks that spread radially outwards and clockwise (counter the direction of rotation).

lowO.PNGPhoto Apr 25, 2 05 48 PM.jpg

This behavior can be explained by radial overturning and thermal wind balance.

The cold water near the tank is more dense than the warmer water at the extremities, and hence sinks and spreads along the bottom due to hydrostatic balance:

hydrostatic balance.PNG

This states that the vertical pressure gradient is equal to the negative of the density times the gravitational acceleration. The result of this is that the dye at the surface moved inwards, and that at the bottom moved outwards.

However, the radial temperature gradient also imposes vertical wind shear, according to the equation for thermal wind:

thermal wind (T).PNG

where the left hand side is the change in azimuthal velocity with height, α is the coefficient of thermal expansion, f is the coriolis parameter, and T is the temperature gradient. In the tank, the temperature gradient then causes "winds" to develop that increase in speed with height. This is why the dye spread into long trails around the ice bucket.

The positions of the particles at the surface could be monitored using a particle tracking software. Data showed that they followed circular paths around the center of the tank. Azimuthal velocities of the particles were calculated to be around 2 cm/s.

ptracks1-1.png

 

The temperature data from the thermometers revealed that an overall trend of decreasing temperature in the tank, as a result of the melting of the ice. The sensors at the bottom of the tank maintained a near-constant radial temperature over time, of about 4ºC. The temperatures higher up in the tank evolved differently however. The sensor on the edge of the tank measured a high temperature of about 21.2 ºC throughout the experiment, and the one on the ice bucket, gave a reading higher than all but the furthest sensor from the ice bucket at the bottom. These high temperatures are a result of the overturning circulation seen in the non-rotating case as well. Cold water near the ice bucket sinks and spreads along the bottom, leaving the surface water much warmer than that below.

tank T all.png

 Discretizing the equation for thermal wind and solving for u gives

u_geostrophic.PNG

where the coriolis parameter, f, has been replaced by 2Ω, L is the radial distance between the ice bucket and the edge of the tank, and H is the height of the water.

We can use the temperature data to calculate the right hand side of the equation, and compare it to the observed surface velocities of the paper dots.

hadley tank calc.PNG

The result is close to the particle velocities found of about 2 cm/s, showing that the theory explains the observed phenomena well within margin of measurement and calculation error.

 

 

 

 

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Atmospheric Data

 

 

 

 

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