The Hadley cell, named after George Hadley, is a global scale tropical atmospheric circulation that features air rising near the equator, flowing poleward at 10-15 kilometers above the surface, descending in the subtropics, and then returning equatorward near the surface. This circulation creates the trade winds, tropical rain-belts and hurricanes, subtropical deserts and the jet streams.
In each hemisphere, there is one primary circulation cell known as a Hadley cell and two secondary circulation cells at higher latitudes, between 30° and 60° latitude known as the Ferrel cell, and beyond 60° as the Polar cell. Each Hadley cell operates between zero and 30 to 40 degrees north and south and is mainly responsible for the weather in the equatorial regions of the world.
The major driving force of atmospheric circulation is the uneven distribution of solar heating across the Earth, which is greatest near the equator and lesser at the poles. The atmospheric circulation transports energy polewards, thus reducing the resulting equator-to-pole temperature gradient. The mechanisms by which this is accomplished differ in tropical and extratropical latitudes.
Hadley cells exist on either side of the equator. Each cell encircles the globe latitudinally and acts to transport energy from the equator to about the 30th latitude. The circulation exhibits the following phenomena:
The Hadley circulation exhibits seasonal variation. During the solstitial seasons (DJF and JJA), the upward branch of the Hadley cell occurs not directly over the equator but rather in the summer hemisphere. In the annual mean, the upward branch is slightly offset into the northern hemisphere, making way for a stronger Hadley cell in the southern hemisphere. This evidences a small net energy transport from the northern to the southern hemisphere.
The Hadley system provides an example of a thermally direct circulation. The thermodynamic efficiency of the Hadley system, considered as a heat engine, has been relatively constant over the 1979~2010 period, averaging 2.6%. Over the same interval, the power generated by the Hadley regime has risen at an average rate of about 0.54 TW per yr; this reflects an increase in energy input to the system consistent with the observed increasing of tropical sea surface temperatures.
Overall, mean meridional circulation cells such as the Hadley circulation are not particularly efficient at reducing the equator-to-pole temperature gradient due to cancellation between transports of different types of energy. In the Hadley cell, both sensible and latent heat are transported equatorward near the surface, while potential energy is transported above in the opposite direction, poleward. The resulting net poleward transport is only about 10% of this potential energy transport. This is partly a result of the strong constraints imposed on atmospheric motions by the conservation of angular momentum.
In the early 18th century, George Hadley, an English lawyer and amateur meteorologist, was dissatisfied with the theory that the astronomer Edmond Halley had proposed for explaining the trade winds. What was no doubt correct in Halley's theory was that solar heating creates upward motion of equatorial air, and air mass from neighboring latitudes must flow in to replace the risen air mass. But for the westward component of the trade winds Halley had proposed that in moving across the sky the Sun heats the air mass differently over the course of the day. Hadley was not satisfied with that part of Halley's theory and rightly so. Hadley was the first to recognize that Earth's rotation plays a role in the direction taken by an air mass as it moves relative to the Earth. Hadley's theory, published in 1735, remained unknown, but it was rediscovered independently several times. Among the re-discoverers was John Dalton, who later learned of Hadley's priority. Over time the mechanism proposed by Hadley became accepted, and over time his name was increasingly attached to it. By the end of the 19th century it was shown that Hadley's theory was deficient in several respects. One of the first who accounted for the dynamics correctly was William Ferrel. It took many decades for the correct theory to become accepted, and even today Hadley's theory can still be encountered occasionally, particularly in popular books and websites. Hadley's theory was the generally accepted theory long enough to make his name become universally attached to the circulation pattern in the tropical atmosphere. In 1980 Isaac Held and Arthur Hou developed the Held-Hou Model to describe the Hadley circulation.
The region in which the equatorward moving air masses converge and rise, is known as the intertropical convergence zone, or ITCZ. Within that zone develops a band of thunderstorms that produce high-precipitation.
Having lost most of its water vapor to condensation and precipitation in the upward branch of the Hadley cell circulation, the descending air is dry. As the air descends, low relative humidities are produced as the air is warmed adiabatically by compression from the overlying air, producing a region of higher pressure. The subtropics are relatively free of the convection, or thunderstorms, that are common in the equatorial belt. Many of the world's deserts are located in these subtropical latitudes. Although the deserts do not extend to the eastern side of the various continents because of ocean currents caused by the Trade Winds.
There is some evidence that the expansion of the Hadley cells is related to climate change. The majority of Earth's arid regions are located in the areas beneath the descending part of the Hadley circulation at around 30 degrees latitude. Those models show that the Hadley cell will expand with increased global mean temperature (perhaps by 2 degrees latitude over the 21st century ). This might lead to large changes in precipitation in the latitudes at the edge of the cells. Scientists fear that global warming might bring changes to the ecosystems in the deep tropics and that the deserts will become drier and expand. As the areas around 30 degrees latitude become drier, those inhabiting that region will see less rainfall than traditionally expected, which could cause difficulty with food supplies and livability. There is strong evidence of paleoclimate climate change in central Africa's rain forest in c. 850 B.C. Palynological (fossil pollen) evidence shows a drastic change in rain forest biome to that of open savannah as a consequence of wide-scale drying not connected necessarily to intermittent drought but perhaps to gradual warming. The hypothesis, that a decline in solar activity reduces the latitudinal extent of the Hadley Circulation and decreases mid-latitudinal monsoon intensity, is matched by data, showing increased dryness in central west Africa and increase in precipitation in temperate zones north. Meanwhile, mid-latitudinal storm tracks in the temperate zones increased and moved equatorward.