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Wednesday 3 August 2011

Heat Transportation in the Atmosphere


  • Without the Sun’s presence, weather would not exist as it is the main source of energy.
  • Global variations in solar radiation receipt lead to a constant imbalance of energy.

Factors affecting radiation receipt:
  • Latitudinal variations. This energy is redistributed from areas of high solar radiation receipt at the equatorial and tropics, to areas of low solar radiation receipt near the poles – as it strives to reach a global equilibrium.


  • Diurnal (daily) variations exist i.e maximum receipt at midday when the Sun is at its greatest angle.
  • Temporal (time dependent) variations exist due to the altering tilt of the Earth’s axis.
How does wind form?
    1. Inequalities in solar radiation over the Earth’s surface causes differences in air pressure, hence movement of energy as hot air rises and displaces cold air.  
    2. The Earth’s rotation influences its direction by the Coriolis force – the deflection of motion to the right in the northern hemisphere and to the left in the southern hemisphere.
    3. Friction the Earth’s surface roughness including the presence of mountain belts, sand dunes, tower blocks etc, perturbs air flow causing it to converge into a low which rises above the obstruction or to diverge away into a high.
Properties of the atmosphere


Recommended website:
http://www.geol.umd.edu/~jmerck/geol100/lectures/33.html  (Excellent diagrams and RS images displaying atmospheric stratification and global convection cells).

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