Atmospheric Circulation (College Board AP® Environmental Science): Study Guide

Alistair Marjot

Written by: Alistair Marjot

Reviewed by: Jacque Cartwright

Updated on

Atmospheric circulation & global wind patterns

  • Global atmospheric circulation can be described as the worldwide system of winds that move solar heat energy from the equator to the poles to reach a balance in temperature

Wind formation

  • Air always moves from areas of higher pressure to lower pressure and this movement of air generates wind

    • Winds are large scale movements of air due to differences in air pressure

    • This pressure difference is because the Sun heats the Earth's surface unevenly

    • Insolation that reaches the Earth's surface is greater at the equator than at the poles

      • This is due to the Earth's curvature and the angle of the Earth's tilt

Diagram showing how angle of insolation spreads solar radiation over a wider area at the poles than at the equator
The angle of insolation spreads solar radiation over a wider area at the poles than at the equator
  • This irregular heating of the Earth’s surface creates pressure cells

    • In these pressure cells, hot air rises and cooler air sinks through the process of convection

Diagram of a wind pressure cell showing six steps of air movement due to heating, rising, cooling, sinking, and pressure differences creating winds.
A typical wind pressure cell system showing the distribution of pressure at Earth's surface and upper atmosphere
  • Air movement within the cell is roughly circular and moves surplus heat from equatorial regions to other parts of the Earth

  • In both hemispheres (the Northern hemisphere and the Southern hemisphere), heat energy transfer occurs where different atmospheric circulation cells meet

    • There are three types of cell

    • Each cell generates different weather patterns

  • These are the Hadley, Ferrel and Polar cells

    • Together, these three cells make up the tricellular model of atmospheric circulation:

Diagram showing the tricellular model of atmospheric circulation
Heat energy flow and surface winds can be explained using the tricellular model of atmospheric circulation

The tricellular atmospheric wind model

  • Each hemisphere has three cells (the Hadley cell, Ferrel cell and Polar cell) that circulate air from the surface, through the atmosphere, and back to the Earth's surface again

  • The Hadley cell is the largest cell and extends from the equator to between 30° and 40° north and south

    • Trade winds blow from the tropical regions to the equator and travel in an easterly direction

    • Near the equator, the trade winds meet, and the hot air rises and forms thunderstorms (tropical rainstorms)

    • From the top of these storms, air flows towards higher latitudes, where it becomes cooler and sinks over subtropical regions

    • This brings dry, cloudless air, which is warmed by the Sun as it descends: the climate is warm and dry (hot deserts are usually found here)

  • The Ferrel cell is the middle cell and generally occurs from the edge of the Hadley cell to between 60° and 70° north and south of the equator

    • This is the most complex cell because it moves in the opposite direction from the Hadley and Polar cells, similar to a cog in a machine

    • Air in this cell joins the sinking air of the Hadley cell and moves at low altitudes to mid-latitudes, where it rises along the border with the cold air of the Polar cell

    • This occurs around the mid-latitudes, contributing to frequent unsettled weather

  • The Polar cell is the smallest and weakest of the atmospheric cells, extending from the edge of the Ferrel cell to the poles at 90° north and south

    • Air in these cells is cold and sinks, creating high pressure over the highest latitudes

    • The cold air flows out towards the lower latitudes at the surface, where it is slightly warmed and rises to return at altitude to the poles

Diagram of global atmospheric circulation showing Polar, Ferrel, and Hadley cells, with associated air movements, clouds, and wind directions.
Global atmospheric circulation showing Polar, Ferrel, and Hadley cells

Coriolis effect

  • Each cell has prevailing winds associated with it 

  • These winds are influenced by the Coriolis effect

  • The Coriolis effect is the appearance that global winds and ocean currents curve as they move

  • The curve is due to the Earth's rotation on its axis, and this forces the winds to actually blow diagonally

  • The Coriolis effect influences wind direction around the world in this way:

    • In the northern hemisphere, it curves the winds to the right

    • In the southern hemisphere, it curves them left

  • The exception is when there is a low-pressure system:

    • In these systems, the winds flow in reverse (counterclockwise in the northern hemisphere and clockwise in the southern hemisphere)

Global wind belts: surface winds

  • The combination of pressure cells, the Coriolis effect, and the 3 cells produces wind belts in each hemisphere:

    • The trade winds blow from the subtropical high-pressure belts (30° north and south) towards the Equator's low-pressure zones and are deflected by the Coriolis force

    • The westerlies blow from the sub-tropical high-pressure belts to the mid-latitude low areas but again are deflected by the Coriolis force

    • The easterlies, polar easterlies, meet the westerlies at 60° south

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Alistair Marjot

Author: Alistair Marjot

Expertise: Biology & Environmental Systems and Societies

Alistair graduated from Oxford University with a degree in Biological Sciences. He has taught GCSE/IGCSE Biology, as well as Biology and Environmental Systems & Societies for the International Baccalaureate Diploma Programme. While teaching in Oxford, Alistair completed his MA Education as Head of Department for Environmental Systems & Societies. Alistair has continued to pursue his interests in ecology and environmental science, recently gaining an MSc in Wildlife Biology & Conservation with Edinburgh Napier University.

Jacque Cartwright

Author: Jacque Cartwright

Expertise: Geography Content Creator

Jacque graduated from the Open University with a BSc in Environmental Science and Geography before doing her PGCE with the University of St David’s, Swansea. Teaching is her passion and has taught across a wide range of specifications – GCSE/IGCSE and IB but particularly loves teaching the A-level Geography. For the past 5 years Jacque has been teaching online for international schools, and she knows what is needed to get the top scores on those pesky geography exams.