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When air moving pole-ward gets to about 30°, the speed of particles gets to be too fast, and the strip of air becomes unstable, leading to a wavering strip of air as shown in Figure 1. Wind beyond this point to about 60° is very chaotic and unpredictable. The overturning circulation from the equator to around 30° is Hadley circulation, and the chaotic motion is eddy circulation. From this point on, the focus is on Hadley circulation.

Atmospheric Data of Hadley Circulation

In order to show Hadley circulation in the atmosphere, it is important to show several different atmospheric variables: vertical pressure velocity, potential temperature, and zonal and meridional wind. Following (Figures 3-10) are zonally averaged profiles of these variables averaged from 1948 to 2012 (ESRL). Examples will be given from both January and July. Firstly, Figure 3 and 4 are of vertical pressure velocity, measured in Pascals/second. The uprising occurs where heat is greatest, which results in greater uprising of particles on the side of the equator that is experiencing summer (January – Southern Hemisphere, July – Northern Hemisphere). The air then sets at around 30° on the winter hemisphere, and around 45° on the summer side. As will be seen in all the following atmospheric figures, Hadley circulation is stronger in the hemisphere experiencing winter.

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