The tri-cellular model of atmospheric circulation
Each hemisphere has three cells — Hadley, Ferrel and Polar — that turn heat into a pattern of winds and pressure belts.
The uneven heating of the Earth is the engine of the whole atmosphere. The Equator receives concentrated solar energy (a surplus) while the poles receive very little (a deficit), and the atmosphere responds by circulating to move the surplus heat polewards. This circulation is organised into three cells in each hemisphere — the tri-cellular model.
- Hadley cell (0–30°) — the largest and most powerful, and a direct (thermally driven) cell. Intense heating at the Equator makes air rise at the ITCZ (low pressure, heavy rain); the air moves polewards aloft, then sinks at ~30° (high pressure, deserts) and returns to the Equator as the trade winds.
- Ferrel cell (30–60°) — a weaker, indirect mid-latitude cell. Air sinks at 30° and rises at 60°; its surface flow gives the westerlies. Its real weather is largely controlled by the jet stream and depressions rather than simple thermal circulation.
- Polar cell (60–90°) — cold, dense air sinks at the pole (polar high) and flows towards 60° as the polar easterlies, rising again at the polar front.
The rising and sinking limbs of these cells create the alternating pressure belts: low at the Equator and ~60°, high at ~30° and the poles. This is why the world's climate falls into great latitudinal bands — wet Equator, dry subtropics, wet mid-latitudes, dry poles.
- Hadley (0–30°): rises at the Equator (rain), sinks at 30° (deserts) — a direct, thermal cell.
- Ferrel (30–60°): weak, indirect cell; surface flow = the westerlies; controlled by the jet stream.
- Polar (60–90°): cold air sinks at the pole, flows out as polar easterlies, rises at 60°.
- Rising air → low pressure → rain; sinking air → high pressure → dry.
See the full worked example for global atmospheric circulation →