Science

Why the wind blows, and why it does not blow straight

Air moves from high pressure to low pressure. It then gets deflected by the rotation of the planet, which is why weather maps look the way they do.

A bank of low cloud approaching across open country ahead of a front.
Approaching cloud ahead of a front. Photograph by Famartin, CC BY-SA 4.0, via Wikimedia Commons.

Key takeaways

  • The Sun heats the Earth unevenly, which produces differences in air pressure.
  • Air accelerates from high pressure towards low pressure; that is the wind.
  • The Earth's rotation deflects moving air, to the right in the northern hemisphere.
  • Away from the surface those two effects balance and wind runs parallel to the isobars.
  • Friction near the ground weakens the deflection, so surface wind spirals into a low.

Wind is air moving from where there is more of it to where there is less. That is nearly the whole answer, and it would be the whole answer if the planet were not spinning.

Uneven heating makes uneven pressure

The Sun does not warm the Earth evenly. The tropics receive sunlight close to head-on and the poles receive it at a glancing angle spread over more surface. Land heats faster than sea. A clear field heats differently from a forest.

Warm air expands, becomes less dense, and rises, which lowers the pressure at the surface beneath it. Cool air sinks, which raises it. Within hours you have regions of higher and lower pressure sitting next to each other.

Air, being a fluid, does not tolerate that. It accelerates from the high towards the low. The force driving it is called the pressure gradient force, and its strength depends on how sharply pressure changes over distance, which is exactly what the spacing of isobars on a weather map shows you.

The sea breeze, which is the whole thing in miniature

Stand on a beach on a sunny afternoon and you can watch this happen at a scale you can hold in your head.

Water has a large heat capacity and mixes heat down through its depth, so the sea warms slowly. Land has neither property, so its surface warms quickly. By early afternoon the air over the land is distinctly warmer, it rises, pressure at the surface falls, and air flows in from the sea to replace it. That is the onshore breeze, and it strengthens as the temperature difference grows.

At night it can run backwards. Land loses heat faster than water, so the sea is now the warmer surface and the breeze blows offshore.

Then the planet turns underneath it

If that were the end of it, wind would blow straight from high pressure to low, and weather maps would be simple. They are not, because the Earth is rotating and the air is not attached to it.

A parcel of air moving across the surface travels in a fairly straight line through space while the ground beneath it turns. To anyone standing on that ground, the air appears to curve. This apparent deflection is the Coriolis effect: to the right in the northern hemisphere, to the left in the southern.

It is not a force in the ordinary sense. It is what a straight line looks like when you are watching from a rotating platform. It is also zero at the equator and strongest near the poles, and it grows with the speed of the air, so it matters most for fast-moving air over long distances.

Which is why wind follows the isobars

Now put the two together. Air starts moving directly from high towards low. As it picks up speed the deflection grows, curving it sideways. It keeps turning until the deflection is pulling exactly opposite to the pressure gradient force.

At that point the two are in balance and the air stops turning. It is now travelling at right angles to the pressure gradient, which means it is running parallel to the isobars rather than across them. Meteorologists call this the geostrophic wind, and it is a good description of the wind well above the surface.

This is the counterintuitive part. Air is not flowing from high pressure to low pressure. It is circulating around the low, held in orbit by the balance between the two effects. It is why weather systems on a map are rotating spirals rather than arrows pointing inward.

Why wind ends up running along the isobars instead of across themThree stages. Air first accelerates directly from high pressure towards low pressure under the pressure gradient force. As it gains speed, the Coriolis effect deflects it to the right in the northern hemisphere. It keeps turning until the deflection exactly opposes the pressure gradient, at which point it travels parallel to the isobars and stops turning. Near the ground, friction slows the air and weakens the deflection, so the balance tips back and the wind crosses the isobars at an angle, spiralling inward towards the low, where it must rise, cool and form cloud.Two forces, and where they settleHIGHLOWisobars1. straight for the lowpressure gradient force2. deflected rightCoriolis, growing with speed3. balancednow parallel to theisobars, and it stopsturningAir is not flowing into the low. It is circulating around it, which is why maps show spirals not arrows.Near the ground, friction spoils the balanceDrag slows the air, the deflection weakens, and the wind crosses the isobars at an angle, spiralling into the low.That inward air has one way to go: up. Rising air cools, vapour condenses, so a low means cloud and rain.
Tightly packed isobars mean a steep pressure gradient and therefore strong wind, and the wind runs along them rather than across them. Both facts fall out of the same balance. Diagram by HRITU; northern hemisphere, where the deflection is to the right.

Near the ground, friction spoils the balance

Close to the surface, air is dragged on by ground, trees and buildings. That slows it, and because the Coriolis deflection depends on speed, slowing the air weakens the deflection.

The balance tips back towards the pressure gradient, and the wind crosses the isobars at an angle instead of running along them, angled inward towards the low. So surface air spirals into a low-pressure system rather than circling it.

That inward spiral has to go somewhere, and the only direction available is up. Rising air cools, water vapour condenses, and cloud forms. This is why low pressure is associated with unsettled weather, and why high pressure, where air is sinking and spreading outward, brings clear skies.

It is also the basis of an old sailor’s rule: stand with your back to the wind in the northern hemisphere, and low pressure is on your left.

Reading a forecast map

Three things follow directly. Tightly packed isobars mean strong wind. Wind runs roughly along the isobars, not across them. And a low on the map means air converging and rising, which means cloud and rain.

More atmosphere

For what the same atmosphere does to sunlight, why the sky is blue and not violet. For a large-scale rhythm driven by something outside the Earth entirely, why the tide comes in twice a day.

Sources

  1. Wind
  2. Coriolis force
  3. Geostrophic wind

Frequently asked questions

It is a sea breeze, and it is the mechanism in miniature. Land heats faster than water under the same sunshine because water has a much greater heat capacity and mixes heat downward. The air over the land warms, rises, and cooler air flows in off the sea to replace it. The effect builds through the day as the temperature difference grows, and it often reverses overnight when the land cools faster than the sea.

Those lines, isobars, join points of equal pressure. Where they are close together, pressure changes rapidly over a short distance, which is a steep pressure gradient and therefore a large force on the air. Widely spaced isobars mean a gentle gradient and light winds. The map is effectively a contour map, and the wind is steepness.

No, and this is a persistent myth. The effect is far too weak to matter at the scale of a sink; the direction there is set by the shape of the basin and how the water was already moving. It becomes significant only over large distances and long times, which is why it shapes weather systems and ocean currents but not plumbing.

HRITU Editorial Desk is the byline for pieces produced in-house by the HRITU editorial team. We write about cooking, travel, science and everyday knowledge, and we explain the reasoning behind what we publish rather than just stating conclusions. Every article is checked against primary or reference sources before it goes out, dated on publication, and updated in the open when we learn something is wrong. Corrections and questions are welcome at info@hritu.com.

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