How Does Wind Form?

Start with sunlight warming the ground and see how temperature differences create pressure differences that set air in motion, giving rise to wind.

Start exploring
How Does Wind Form?

How Does Wind Form? Knowledge file

Wind is the horizontal flow of air: the Sun heats the surface, uneven heating creates pressure differences, air flows from high pressure to low, Earth's rotation bends it, and land-sea contrasts breed breezes and monsoons.

At a glance

Nature of wind
Horizontal air flow
Energy source
Solar radiation
Deflection rule
Right north, left south
Monsoon scale
Seasonal

Core concepts

Cause

Uneven heating is the source of wind

Land warms and cools faster than water, and the equator and poles are heated unevenly. Temperature differences create pressure differences, and air flowing from high to low pressure is wind.

Deflection

Coriolis bends the wind

Earth's rotation deflects winds to the right in the Northern Hemisphere and to the left in the Southern Hemisphere. The stronger the wind and the higher the latitude, the greater the bend—large-scale winds never blow straight.

Circulation

Sea breezes and monsoons share a cause

By day the sea breeze blows from ocean to land; at night the land breeze reverses. Scale the same land-sea contrast up to a season and you get the monsoon, which shapes life for billions.

Ways to understand

  1. Phase 1Heating and rising

    Sunlight warms the land quickly; the warm air expands and rises, leaving low pressure at the surface.

  2. Phase 2Driven by pressure differences

    High and low pressure face off, air flows from high to low, and that horizontal current is wind.

  3. Phase 3Deflection and circulation

    The Coriolis effect bends the wind, and alternating land-sea heating drives sea breezes and monsoons.

What to observe

  1. ObserveWatch the airflow arrows

    Air always flows from the cool high-pressure zone over the sea toward the warm low-pressure zone over land, reversing between day and night.

  2. ObserveNotice the paths curve

    In stage 6 the airflow arrows gradually bend to one side—the cumulative effect of Coriolis deflection over long distances.

  3. ConsiderWhy the air is never perfectly still

    As long as the surface heats unevenly, pressure differences exist and air must move. Wind is how Earth redistributes heat.