Winds and global circulation
Winds and global circulation
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A snapshot of METEOSAT shows regions of the Earth with substantial cloud cover and other regions with clear skies (Photo: ESA)
Learning Objectives
- Explain what causes wind
- Describe the forces that initiate and modify winds
- Explain what causes certain regions of our planet to be dry and cloudless while others are wet and cloudy
 
 
Why does the wind blow?
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Why does the wind blow?
Three main factors affect the horizontal motion of the air:
- Pressure gradient force: drives flow
- Coriolis effect: “deflects” flow
- Friction: slows flow
The velocity (speed and direction) of the wind at any time is the result of these three vector forces.
Atmospheric Pressure \(P_a\)
- Recall: \(P_a\) decreases exponentially with height
- \(P_a \approx\) Weight of the air
 
- Following the ideal gas law, \(P_a\) is a function of temperature and density
\[
PV=nRT
\qquad(1)\]
 
 
Atmospheric Pressure (iClicker)
What happens if we warm up a column of air? Assume there is no horizontal flow.
- A The air contracts, the column shrinks
- B The air expands, the column stretches
- C The column does not change
 
 
Atmospheric Pressure (iClicker)
In this scenario the column expands:
- \(rho\) decreases
- \(P_a\) (at the surface) remains the same
- Mass of air above surface does not change
 
 
 
Atmospheric Pressure \(P_a\)
\(P_a\) is not uniform across the Earth’s surface.
- High (H): areas with relatively high \(P_a\) at sea level
- Low (L): areas with relatively low \(P_a\) at sea level
- Lines of equal pressure on a map are called isobars.
 
 
Atmospheric Pressure \(P_a\)
\(P_a\) is not uniform across the Earth’s surface.
- High (H): areas with relatively high \(P_a\) at sea level
- Low (L): areas with relatively low \(P_a\) at sea level
- Lines of equal pressure on a map are called isobars.
 
 
Pressure Gradient Force
Air flows from higher to lower pressure. This is the main driving force for winds.
- Speed set by spacing of the isobars
- i.e. the pressure gradient
- Acts at right angles to the isobars.
 
 
 
Creating a Pressure Gradient
What happens if we warm up the middle column of air?
 
 
Creating a Pressure Gradient
What happens if we warm up the middle column of air?
- The warmed column expands creating a pressure gradient aloft
 
 
Creating a Pressure Gradient
Winds redistribute mass to equalize the gradient
- Divergence of mass aloft will reduce \(P_a\) at surface
 
 
Creating a Pressure Gradient (iClicker)
Which air column experiences the lower pressure at sea level?
 
 
Thermal Lows
- Heating causes expansion
- Divergence aloft reduces surface pressure
- This is a thermal low
- Creates a pressure gradient at the surface
 
 
Thermal Lows
- Common in equatorial regions and over large continents during summer
- Responsible for trade winds and monsoons
 
 
 
Creating a Pressure Gradient
What happens if we cool down the middle column of air?
 
 
Creating a Pressure Gradient
What happens if we cool down the middle column of air?
- The cooled column compresses creating a pressure gradient aloft
 
 
Creating a Pressure Gradient (iClicker)
Which air column experiences the higher pressure at sea level?
 
 
Thermal Highs
- Cooling causes compression
- Convergence aloft increases surface pressure
- This is a thermal high
- Creates a pressure gradient at the surface
 
 
Thermal Highs
- Common in polar regions and over large continents during winter
- Typically located over Siberia and Canada in winter
- Responsible for persistent windy conditions in the prairies
 
 
 
Semi-Permanent Highs and Lows
Semi-permanent High and Low pressure systems occur in preferred locations (e.g. Hawaiian, Bermuda, Siberian Highs; Aleutian, Icelandic Lows)
- Patterns are clearer in the Southern Hemisphere because the distribution of land-sea is simple
- Pay-to-day these systems tend to move continuously (in the mid-latitudes typically from west to east)
Coriolis Effect
An apparent force due to the rotation of Earth.
- Rotation of the Earth’s around its axis “deflects” winds
- Primary reason flow is not parallel to isobars
 
 
 
Coriolis Effect
An apparent force due to the rotation and curvature of Earth.
Coriolis Effect
A function of wind speed (\(V\)), Earth’s rotational velocity (\(\Omega\)), and latitude (\(\phi\)):
\[
F_c = 2V\Omega sin \phi
\qquad(2)\]
- Deflects flow to the right (left) in the N (S) Hemisphere
- Strongest at the poles, zero at the equator
 
 
Coriolis Effect (iClicker)
All else equal, at which Latitude would the Coriolis effect be the strongest?
- A 10 \(^\circ\) N
- B 20 \(^\circ\) S
- C 50 \(^\circ\) N
- D 65 \(^\circ\) S
Heating on a global scale
Lower latitudes show a radiative surplus, the higher latitudes show a radiative deficit. Global wind system is driven by unequal heating of the Earth by the Sun.
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The Three-Cell Model
Poleward transport of energy aims to “correct” the imbalance. Winds are deflected by Coriolis force, resulting in trade winds, westerlies, and polar easterlies.
The Three-Cell Model
The three cells form bands of uplift (cloudy, stormy, wet) around Equator (ITCZ = Inter Tropical Convergence Zone) and Polar front and subsidence (cloud-free, dry) in Sub-tropical desert belt and Poles.
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The Three-Cell Model
The three-cell model describes “average” global circulation patterns, but in reality there are seasonal and longitudinal variations due to the change in the Sun’s position and the ocean-land distribution.
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Coriolis Effect
As winds move across a pressure gradient, they are deflected by the Coriolis effect, causing them to flow parallel to the pressure gradient.
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Frictional force
- Friction (aka drag) of air over the Earth’s surface slows the wind.
- Effect is greatest near the surface
 
- Since the Coriolis is a function of wind speed:
- Coriolis force is weaker near the surface
- Deflection due to Coriolis force is greater aloft
 
Effects of Friction on Wind
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An idealized example showing the effects of pressure gradient (Fp), Coriolis (Fc) and friction (Ff) forces in the “free atmosphere” and near the surface.
Winds in Pressure Systems
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Shown here for the the Northern hemisphere. In the Southern hemisphere, rotation is opposite.
Cyclones
- A cyclone is a large area which experiences rotating winds, which circle around the lowest pressure
- Winds circle in anti-clockwise direction on the northern hemisphere, and in clockwise direction on the Southern hemisphere
 
 
Anticyclones
- An anticyclone is a large area which experiences rotating winds, circling around the region with high pressure.
- Winds circle in clockwise direction on the northern hemisphere, and in anti-clockwise direction on the southern hemisphere.
 
 
Explore for Yourself
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Figure 1: Windy.com is a fun tool you can use to explore for yourself.
Take home points
- Winds are caused by the pressure gradient force which is equalizing horizontal pressure differences.
- Once in motion, the Coriolis force and friction act, causing deflection and slowing of the wind.
- On a global scale the energy transport is deflected, creating three distinct cells (Hadley, Ferrel and Polar cell) in each hemisphere.
- On a smaller scale it creates thermal lows and highs (cyclones and anticyclones).