MET 005
Atmospheric circulation
Wind
What wind is, and five ways it matters to the traffic.
Air in motionCaused by differences in pressure (MET 002).
Why it matters
- Over the groundWind affects an aircraft’s motion over the ground.
- Landing and take-offMade into the wind. Hazardous windshear, turbulence and crosswind.
- VectoringThe differences between track and heading, and between airspeed and groundspeed.
- Friction layersThe wind changes through the friction layers.
- Route and levelRoute and level changes due to head- and tailwind, such as the jet stream.
Meteorological scales
Four scales, from the largest to the smallest.
GlobalTrade winds and global weather patterns.
SynopticCyclones, low- and high-pressure systems, fronts.
MesoscaleLand and sea breeze, föhn wind (MET 004), squall lines, individual thunderstorms.
MicroscaleLocal turbulence.
Global atmospheric circulation
The large-scale movement of air.
How heat is shared outThe means, together with the smaller oceanic circulation, by which thermal energy is distributed on the surface of the Earth.
What drives itDifferent amounts of solar radiation are absorbed at different latitudes (MET 003).
Surface heated from the sun
- Air expands and starts risingBecause of heating at the surface.
- Lower pressure at the surfaceAn area with relatively lower pressure is created at the surface.
- It moves horizontally, then descendsAs the air stops rising, it moves horizontally, loses its heat and eventually descends again.
- Higher pressure at the surfaceAn area with relatively high pressure develops where it meets the surface.
Different surface heating
Why the sun heats some latitudes more than others, and the circulation that follows.
Tilted 23.5°Earth’s axis is tilted 23.5° from the perpendicular to its orbit (the ecliptic).
SeasonsThis causes seasonal variations, depending on latitude.
Angle and daylightIt affects the angle of incidence and the duration of the day.
Global circulation of air reduces the heat difference between the equator and the poles.
The Coriolis effect
The apparent deflection, seen from the turning Earth, of anything moving freely over its surface.
One rate of turningThe whole Earth turns at one rate. The ground moves faster at the equator than near the poles.
Air overtakes the groundAir moving away from the equator moves over ground that is moving more slowly, and so it overtakes the ground.
In the northern hemisphere, moving air is deflected to the right.
The three-cell model
The northern hemisphere in cross-section, from the North Pole to the equator.
Polar cellBetween the pole and 60°N. Along the ground the air flows from the pole to 60°N.
Ferrel cellBetween 60°N and 30°N. Along the ground the air flows from 30°N to 60°N.
Hadley cellBetween 30°N and the equator. Along the ground the air flows from 30°N to the equator.
The tropopauseRises from the pole towards the equator (MET 002). It breaks at about 60°N, where the polar jet is, and again at about 30°N, where the subtropical jet is.
Reading material
Meteorology
MET 005 Atmospheric Circulation PowerPoint / PDF
EPN Group Training Document Meteorology, chapter 5 Reading list, course material
Lankford, Terry T., Aviation Weather Handbook, 1st edition, 2000 Reference, paid
EUMeTrain, SatManu: Manual of Synoptic Satellite Meteorology (Conceptual Models) (viewed 20 September 2019) Reference, free