General Circulation

Meteorology · Chapter 20 · DGCA CPL and ATPL

The planet-sized wind machine: why the tropics are rainy, the deserts sit at 30°, the trade winds blow so steadily and mid-latitude weather drifts from west to east.

Remember

Why does the air move round the globe at all?

A planet-sized engine

Four cards with real satellite images. Swipe or tap Next.

  1. Hot belly, cold head Near the equator each square metre gets far more sunshine than near the poles. Averaged over a year the whole Earth balances what comes in and what goes out, but by latitude it does not: a surplus in the tropics, a deficit at the poles. This AIRS map of temperature shows the warm tropics (red) and the cold poles (blue and purple).
  2. Winds and currents spread it out To stop the tropics getting ever hotter and the poles ever colder, the atmosphere and oceans move heat (and momentum) poleward. Averaged over a long time, the winds that do this form the general circulation of the atmosphere. Day-to-day systems (highs, lows, cyclonic circulations) move within it; studying them is synoptic meteorology.
  3. Why deserts sit near 30° Air that rose at the equator sinks again around 30° N and S, under the subtropical highs. Sinking air warms and dries and stops cloud forming. That is why the great deserts, the Sahara, Arabia, the Thar, Australia and the Kalahari, lie near 30°.
  4. Which way will it move? A low forms over the Bay of Bengal in the tropical easterlies, and another forms over Europe in the westerlies.

Takeaway: Unequal heating drives the circulation: the tropics gain more energy than they lose, the poles lose more than they gain, and the winds carry the difference.

Why must the atmosphere move heat around?

Surplus and deficit

Energy coming in and going out over a year, by latitude. Tap Next.

  1. Incoming sunlight The sun heats the equator far more, for each square metre, than the poles. Near the equator the sun is high and its rays hit the ground almost straight on. Near the poles the sun is low, so the same beam is spread over a much larger area and also passes through more air. That is why the yellow curve peaks at the equator.
  2. Outgoing heat The Earth loses heat to space as long-wave radiation, from every latitude and much more evenly. Over the whole globe and the whole year, what comes in and what goes out nearly balance: the energy balance.
  3. Surplus and deficit But it does not balance at each latitude. The tropics get more than they lose: a surplus. The polar regions lose more than they get: a deficit. The tropics have a radiation surplus.
  4. So the air moves Winds and ocean currents carry the extra heat towards the poles and even it out. These are the transport processes. The long-term average of all those winds is the general circulation. The study of the moving highs, lows and other systems within it, and their weather, is synoptic meteorology. Studying the moving weather systems is synoptic meteorology.

Memory hook: Surplus in the tropics, deficit at the poles, so winds and currents carry heat poleward.

Takeaway: Over the whole Earth and a whole year, the sunlight coming in (short-wave) and the heat going out (long-wave) balance. But the tropics take in more than they lose (a surplus) and the polar regions lose more than they take in (a deficit). Winds and ocean currents carry the extra heat towards the poles. That long-term pattern of moving air is the general circulation.

How big is each weather system?

Weather by size

Sort each system into its scale.

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What does the three-cell model look like from the side?

Three cells, sliced

A slice from the equator (left) to the pole (right). Tap Next.

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How do the three cells fit together?

Three-cell globe

Tap a belt to light it up on the globe and in the cross-section. Switch season to move the belts.

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How do the cells and winds wrap round the Earth?

The cells in 3D

NASA's Blue Marble with the cells drawn along 75°E and the surface winds round the globe. Heights stretched. Drag to turn it.

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What are the planet's surface pressure belts and winds?

Belts and winds

The idealised pattern of Figures 20.2 and 20.4. Tap Next.

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Can you see the circulation from space?

The cells from space

A real NASA satellite day, 15 January 2020, from Arabia to Sumatra. Tap the pins.

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Which cell does each feature belong to?

Which cell?

Tap a feature, then its cell.

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Why do some lows move east and others west?

Upper winds steer the weather

A real map with the winds high up and the weather systems they carry. Tap Next.

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Why don't the westerlies just blow in a circle?

Standing and Rossby waves

Looking down on the North Pole. Tap Next.

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What happens higher up?

Upper winds and waves

Each pair looks alike. The rule underneath tells them apart.

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Numbers to know

The figures the exam keeps asking for.

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Test yourself

Quick test

10 questions to check this chapter. Each answer explains why.

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