Introduction
• This lesson explores atmospheric heating and horizontal air movement, resulting in wind.
• The sun's energy drives air movement, but not directly.
Heating of the Atmosphere
• The atmosphere is transparent to solar radiation and acquires virtually no heat energy directly from the sun.
• Solar radiation heats the earth's surface, and non-uniform heating has meteorological consequences.
• Factors causing uneven heating:
◦ Spherical shape of the earth.
◦ The oblique angle of the atmosphere at different latitudes.
• Tropical areas receive a higher concentration of insolation (solar radiation) than polar regions.
• The earth's surface absorbs energy, which is then transferred to the troposphere through:
◦ Conduction (near the surface).
◦ Terrestrial radiation (especially at lower levels).
◦ Convection (vertical movement of air currents).
• The atmosphere is heated from below.
• The Earth's tilt causes hemispheres to receive varying solar energy concentrations based on Earth's position in its orbit, creating seasons.
• Surface temperatures are warmer at the equator due to concentrated solar energy.
Factors Affecting Atmospheric Heating
• Uneven surface heating leads to a circulation of air.
◦ Air at the tropics is warmed, becomes less dense, rises, and spreads out.
◦ Cold ground at the poles cools the air, increasing its density.
• This results in:
◦ High pressure at the poles.
◦ Low pressure in the tropics.
◦ Air moving from high to low pressure (surface wind) from the poles to the tropics.
• Modifying factors:
◦ Different surfaces have different heating properties.
▪ Land heats and cools quickly (hourly changes).
▪ Water changes temperature slowly (monthly changes).
▪ Oceans retain heat after summer and cool slowly through winter.
• Uneven heating of the earth's surface creates areas of high and low pressure.
• Air flows from high to low pressure, creating wind.
Measurement of Pressure
• Knowledge of pressure distribution is important for weather assessment and forecasting.
• Meteorological stations measure surface atmospheric pressure.
• Complicating factor: observing points are at different elevations (altitudes above sea level).
◦ Example: Blackpool Airport is 37 ft AMSL, Biggin Hill is about 600 ft AMSL.
◦ Elevation differences cause pressure differentials (approximately 27 ft = 1 mb).
• Direct plotting of surface pressure measurements is pointless due to different elevations.
• To create a uniform datum, observed pressure is increased using a standard formula to calculate the pressure at sea level.
• A chart of observed pressures is drawn with all figures based on a common sea-level datum.
• This sea level pressure datum is called QFF.
Isobars
• Pressure measurements are plotted on a chart.
• Lines are drawn joining points of equal sea-level pressure; these lines are called isobars.
• Isobars are similar to contour lines on a map, indicating:
◦ High pressure areas.
◦ Low pressure areas.
◦ Pressure gradients.
• 'Isobar' is derived from Greek words: 'isos' (equal) and 'baros' (weight) - lines of equal weight of atmosphere.
Horizontal Pressure Gradient
• Air flows down a pressure gradient from high to low pressure, like water flowing downhill.
• Steeper ground slope corresponds to closer contour lines.
• Steeper pressure gradient (close isobars) means a large pressure change over a short distance, indicating stronger winds.
• Slack pressure gradient (widely spaced isobars) indicates light winds.
• Relationship between isobar spacing and wind strength allows estimation of wind strength from weather charts.
Convergence and Divergence
• Surface low-pressure systems cause air to rush in from all directions.
• The air collides and rises, leading to convection and cloud formation.
• Rising air diverges in a higher-pressure system near the troposphere (an 'upper high').
• Surface high-pressure systems lead to divergence.
• Divergence leads to subsidence and an upper low near the troposphere.
• In active pressure systems, pressure patterns at the surface and the tropopause are generally opposite.
Coriolis Force
• Air doesn't flow directly from high to low pressure due to the Coriolis force.
• Coriolis force is a consequence of the earth's rotation.
• Imagine drawing a straight line from the center of a rotating disc; the rotation curves the line.
• Coriolis force acts similarly on moving particles.
• In the northern hemisphere, the force acts at 90° to the right of the moving particle.
• In the southern hemisphere, the force acts at 90° to the left.
• Coriolis force is strongest at the poles and zero at the equator.
• The Coriolis 'force' is not a Newtonian force but the result of linear and rotational movement.
• Often referred to as the Coriolis 'effect', named after Gustave-Gaspard Coriolis.
Geostrophic and Gradient Winds
• Air movement due to a pressure gradient is deflected by the Coriolis 'force' (to the right in the northern hemisphere).
• Deflection 'curves' the path of air particles.
• If the deflection is sufficient, air flows parallel to straight isobars.
• This occurs when the pressure gradient force equals the Coriolis 'force', resulting in the geostrophic wind.
• Geostrophic wind applies to straight isobars; curved isobars (around high or low pressures) result in the gradient wind.
• A practical feature of gradient wind is that for equally spaced isobars, wind speed around a low-pressure system is often less than around a high-pressure system.
Measurement of Wind
• Wind is measured and forecast as a velocity (direction and speed).
• Wind direction is the direction from which the wind is blowing.
• Weather forecasts/reports use degrees 'true', while ATSUs use degrees 'magnetic'.
• Wind speed is measured by an anemometer and reported in knots (KT, nautical miles per hour), sometimes metres per second (MPS) or kilometres per hour (KMH).
• The knot is standard in aviation, but metres per second are used in eastern Europe.
• Met surface pressure charts use isobars to estimate wind direction and spacing to estimate wind strength.
• Surface friction changes both speed and direction.
• A rule-of-thumb conversion: double the metres per second figure to obtain the speed in knots (10 MPS ≈ 20 KT).
• Wind velocity is reported as direction and speed (e.g.,