| MadSci Network: Earth Sciences |
It all starts with the sun. Incoming solar radiation heats the land and water surfaces, which in turn re-radiate energy heating the atmosphere overlying them. Differential heating (heating at different rates due to differences in the surface doing the re-radiating) creates areas of relatively lower and higher pressure. The relationship between temperature and pressure is given by: P = (Density) x (Constant) x (Temperature) The resulting pressure gradient force causes the wind to move from areas of high pressure toward areas of low pressure. This movement of air is the wind. Some factors affecting global circulation include: 1) The Coriolis Effect, which arises from the fact that the earth is rotating beneath the atmosphere. 2) The positions of continental land masses and oceans which affects ocean circulation patterns, ocean temperatures and in turn the heating of the overlying atmosphere. 3) Large scale terrain features like the Rocky Mountains and the Himalyas which deflect the wind flow at various levels in the atmosphere forcing winds upward or downward. In the case of Mount Everest, this deflection reaches well above 25,000 ft. into the region of the jet stream. Local effects can arise from smaller scale terrain features which may cause local lifting or downward motion, bodies of water which may produce sea or lake breezes due to differential heating, and even frictional effects with the land surface which may turn or slow the wind from its original speed and direction. Very localized effects can be produced by tall buildings which may create wind flows not represented by the general flow away from the city. Learn more about wind from these links: USATODAY
The University of Illinois' On-Line Meteorology Guide
Texas A&M University's Laboratory for the Exploration of Atmospheric Processes
Try the links in the MadSci Library for more information on Earth Sciences.