THE NATURAL ENVIRONMENT

Geography 101 Online
     

 

ToC

WIND

Forces

Motion

Global

Local

 

Global Winds

 
  1. If Earth did not rotate, what would the global atmospheric circulation be like?
  2. What is the Hadley Cell?
  3. Low pressure systems are the ITCZ, polar fronts, and subpolar Lows. At what latitude are they located and what are their characteristics?
  4. High pressure systems are the subtropical Highs (horse latitudes), and polar Highs. At what latitude are they located and what are their characteristics?
  5. Based on your knowledge of sky conditions for High and Low pressure, at what latitude do you think the subtropical deserts are located? The tropical rainforests?
 
BOX 1

At the most fundamental level, the global winds are set in motion by differential heating of Earth's surface by sunlight, i.e. the tropics are warm and polar areas cold. This differential heating gives rise to pressure differences and, therefore, the pressure gradient force that compels air to move. Ultimately, as we saw earlier, the moving air redistributes heat from areas of surplus to areas of deficit.

global air circulation of VenusRemember the vertical motion of air at High and Low pressure centers described in the previous section, Motion? At the equator, the warm surface causes low pressure and rising air. At the poles, cold air produces high pressure and sinking air. If Earth did not rotate, this would describe the global circulation. Air would rise at the equator, flow at high altitude to the Poles, where it would sink and return to the equator along the surface, forming two gigantic circulation cells. On Venus, which does not rotate on its axis enough to produce appreciable Coriolis, this is, in fact, what happens.

Global Pressure

On Earth, however, Coriolis makes the situation a bit more complicated. Air rises near the Equator, but rather than flowing all the way to the poles, Coriolis force causes air to sink at about 30° north and south latitudes as shown on the right side of the diagram below. This vertical motion in the tropics is so well defined that it has a name: the Hadley Cell. Rising air in the Hadley cell along the equator produces deep clouds, thunderstorms, and rain in a band of low pressure called the Intertropical Convergence Zone (ITCZ). Sinking air near 30° latitude causes high pressure areas called the subtropical highs. The highs produce clear skies and calm winds in a latitude band sometimes called the Horse Latitudes (which lie just north of the Hawaiian Islands and dominate Hawaiian weather).

Coriolis makes the air flow at higher latitudes even more complicated, but in general air flows out of the subtropical highs poleward along the surface then rises again at the Polar Front (which wobbles around between 50° and 70° latitude). At the polar front, air rises, producing cloudy skies in a band of bad weather sometimes called the Subpolar Low.

global wind and pressure systemsAt the highest latitudes, the circulation is similar to the Hadley cell, except much smaller. Air sinks over the poles (Polar High pressure, clear skies, cold air), then flows equatorward and rises again at the Polar Front.

Global pressure bands are related to the vertical circulation of the air as discussed above and are shown in the diagram as HIGH (30° latitude and the poles) and LOW (equator and 40-70° latitude). These surface pressure bands not only determine the climate at their location, but also drive the horizontal surface winds. Studying the diagram will help you, not only in this class, but in understanding the weather wherever you travel in the world.

 

Global Winds

The diagram above shows two idealized views of air motion, the vertical cross-section shown on the right and the horizontal winds shown over the image of Earth. Look at the very center near the word "Equator." Notice high pressure is to the north and low pressure is at the equator itself. Remember the rules regarding air motion in relation to pressure differences from the Motion section? Imagine standing on the high pressure area in the northern hemisphere looking equatorward and holding out your right arm. Air flows from you toward the equatorial low and is deflected to the right, in the direction your arm points. That motion forms the northeast trade winds as shown in the diagram. Now do the same for the southern hemisphere. Imagine standing on the high in the South Pacific, and looking north toward the equator, holding out your left arm this time. Air is deflected by Coriolis to the left, in the direction your arm is pointing, forming the southeast trade winds. The trade winds, so-named because of their dependability for sailing ships, are usually very reliable and cover nearly one half of Earth's surface. Trade wind weather is generally dry and sunny because of the subtropical High pressure influence. In equatorial areas, dominated by the ITCZ, winds are generally light or calm, a condition that mariners term the doldrums.

global wind and pressure system names

Summary of Global Wind and Pressure Belts

(This is a good point to note how winds are named: winds are named for the direction they come from. So, northeast trade winds come from the northeast, westerly winds come from the west, sea breezes come from the sea, valley breezes come from the valley, and so on.)

 
  1. Where do the global trade winds occur and why there?
  2. Where do the global westerly winds occur and why there?
  3. What direction are Polar winds generally and why?
  4. How are winds named?
  5. Which pressure belt is closest to the Hawaiian Islands (20° N latitude) and what wind system dominates?
  6. If the Equator was a High pressure belt and Low pressure occurred at 30° latitude, what direction would tropical winds blow?
  7. What is the relationship between wind and surface ocean currents?
  8. What are oceanic gyres and what causes them?
  9. Explain how and where ocean currents transport heat to higher latitudes.
 
BOX 2

Now apply the same reasoning to the winds between the subtropical highs and the polar front, or subpolar lows. Air flows from high to low pressure and Coriolis deflection produces westerly winds in both the northern and southern hemispheres between about 30° and 60° latitude. Westerly winds tend to shift direction much more than the trades and also tend to be more blustery. In the southern hemisphere, they blow with such ferocity that mariners named these latitudes the Roaring Forties, Furious Fifties, and Screaming Sixties. The highest average wind speed, in fact, occurs off the coast of Antarctica near 60° S latitude at over 60 kilometers (37 miles) per hour. That's average wind speed.

Cold Polar Easterlies cover the highest latitudes for the same reason easterly trade winds prevail in the tropics.

Finally, one should note that the diagram shows a very idealized version of the global winds. Heating and cooling of land surfaces causes much variation, such as seasonal monsoons in tropical Asia. Nonetheless, it generally holds true, especially over the oceans. For testing purposes, memorizing the yellow global wind and pressure belt diagram will be quite helpful.

Ocean Surface Currents

Friction from surface winds drives the global ocean surface currents. These huge flows of water have an enormous impact on regional climates as they transport heat poleward, and return cool water back to the tropics. The largest ocean circulations are huge gyres in the major ocean basins centered on sub-tropical High pressure centers as shown below.

Remember earlier, when discussing the global temperature map (Chapter 3 -> Temperature), we noted differences between the Australian and South American sides of the South Pacific Ocean? The surface current map shows this same phenomenon in more detail. An enormous gyre in the South Pacific sends warm water poleward near Australia and cool water equatorward along South America. As a general rule, remember that ocean current direction matches surface wind direction, and that gyres transport heat poleward on the western sides of ocean basis and return cool water equatorward on the eastern sides of ocean basins.

global ocean surface currents

     
   

ToC | WIND | Forces| Motion | Global | Local

Dennis Nullet
Kapiolani Community College Geography