Energy from the Sun heats the entire Earth, but this heat is unevenly distributed across the Earth's surface. Equatorial and tropical regions receive far more solar energy than the midlatitudes and the polar regions.
The tropics receive more heat radiation than they emit, while the polar regions emit more heat radiation than they receive. If no heat was transferred from the tropics to the polar regions, the tropics would get hotter and hotter while the poles would get colder and colder. This latitudinal heat imbalance drives the circulation of the atmosphere and oceans. Around 60% of the heat energy is redistributed around the planet by the atmospheric circulation and around 40% is redistributed by the ocean currents.
1. Planet Earth from Space.
One way to transfer heat from the equator to the poles would be to have a single circulation cell where air moved from the tropics to the poles and back. This single-cell circulation model was first proposed by Hadley in the 1700’s.
2. Air circulation around the globe would be simple (and the weather boring) if the Earth did not rotate and the rotation was not tilted relative to the Sun.
3. Hypothetical circulation for a non-rotating Earth. Source: National Weather Service, Southern Regional Headquarters - USA.
Since the Earth rotates, its axis is tilted and there is more land in the Northern Hemisphere than in the Southern Hemisphere, the actual global air circulation pattern is much more complicated. Instead of a single-cell circulation, the global model consists of three circulation cells in each hemisphere. These three cells are known as the tropical cell (also called the Hadley cell), the midlatitude cell and the polar cell.
4. Rotating Earth
5. Idealised global circulation. Source: National Weather Service, Southern Regional Headquarters - USA.
1. Tropical cell (Hadley cell) - Low latitude air moves towards the Equator and heats up. As it heats it rises vertically and moves polewards in the upper atmosphere.
Due to the Coriolis effect, the direction of th is upper level air flow becomes more and mo re westerly with growing distance from the Equator . Finally the carried air loses its poleward momentum and descends around the 30 ° latitude forming a convection cell that dominates tropical and sub-tropical climates.
2. Midlatitude cell (Ferrel cell) - A mid-latitude mean atmospheric circulation cell for weather named by Ferrel in the 19th century. In this cell
w est erly winds are dominated both near the ground surface and in the upper levels of the atmosphere. However, the m eridional air exchange is supported by the frequent cyclo nes and anticyclones of the zon e .
3. Polar cell - Here the cold air sinks forming the polar highs. At the surface, the air spreads out from the polar highs. Surface winds in the polar cell are easterly (polar easterlies).
In the upper level s the prevailing flow is westerly and poleward
Although still oversimplified, this three cell model can describe the main features of atmospheric circulation.
Surface Features of the Global Atmospheric Circulation System
Main wind belts:
Because the Coriolis force acts to the right of the flow (in the Northern Hemisphere), the flow around the 3-cells is deflected. This gives rise to the three main wind belts in each hemisphere at the surface:
· The easterly trade winds in the tropics
· The prevailing westerlies
· The polar easterlies
The doldrums are the region near the equator where the trade winds from each hemisphere meet. This is also where you find the intertropical convergence zone (ITCZ). It is characterized by hot, humid weather with light winds. Major tropical rain forests are found in this zone. The ITCZ migrates north in July and south in January.
The horse latitudes are the region between the trade winds and the prevailing westerlies. In this region the winds are often light or calm, and were so-named because ships would often have to throw their horses overboard due to lack of feed and water.
The polar front lies between the polar easterlies and the prevailing westerlies.
6. Global Circulation. Source: http://www.geocities.com
The three-cell circulation model has the following pressure belts associated with it:
· Equatorial low – A region of low pressure associated with the rising air in the ITCZ. Warm air heated at the equator rises up into the atmosphere leaving a low pressure area underneath. As the air rises, clouds and rain form.
· Subtropical high – A region of high pressure associated with sinking air in the horse latitudes. Air descends in the subtropics creating areas of high pressure with associated clear skies and low rainfall. The descending air is warm and dry and deserts form in these regions.
· Subpolar low – A region of low pressure associated with the polar front.
· Polar high – A high pressure region associated with the cold, dense air of the polar regions.
In reality, the winds are not steady and the pressure belts are not continuous.
7. a) "Ideal" Zonal Pressure Belts
An imaginary uniform Earth with idealised zonal (continuous) pressure belts.
b) Actual Zonal Pressure Belts
Large landmasses disrupt the zonal pattern breaking up the pressure zones into semipermanent high and low pressure belts.
There are three main reasons for this:
· The surface of the Earth is not uniform or smooth. There is uneven heating due to land/water contrasts.
· The wind flow itself can become unstable and generate “eddies.”
· The sun doesn’t remain over the equator, but moves from 23.5 oN to 23.5 oS and back over the course of a year.
Instead, there are semi-permanent high- and low-pressure systems. They are semi-permanent because they vary in strength or position throughout the year.
· Polar highs develop over Siberia and Canada
· The Pacific High, Azores High (parts of the subtropical high pressure system) Aleutian Low and Icelandic Low form
· The Azores high migrates westward and intensifies to become the Bermuda High
· The Pacific high also moves westward and intensifies
· Polar highs are replaced by low pressure
· A low pressure region forms over southern Asia
About this page:
Author: Vera Schlanger – Hungarian Meteorological Service
reviewing: Dr. Ildikó Dobi Wantuch / Dr. Elena Kalmár - Hungarian Meteorological Service, Budapest
Last updated: 2004-02-12