In the most basic terms, the Hadley circulation can be thought of as a large-scale overturning of the atmosphere driven by latitudinal heating gradients, extending roughly between the Tropics of Cancer and Capricorn covering roughly half the surface area of the planet. Rising air occurs near the equator with subsidence in the subtropics. The circulation has a strong seasonal variability. It is manifested during the equinoxes as a pair of rei atively weak cells with a common rising zone near the equator termed the Intertropical Convergence Zone (ITCZ). A much stronger cross-equatorial cell marks the solstitial seasons with rising motion in the summer hemisphere and widespread descending air in the winter hemisphere. The meridional circulations are instrumental in determining where tropical rainfall occurs and where the great deserts are located. Variability of the location and intensity of the Hadley circulation (or its regional manifestation such as the monsoons), through the ages has helped shape the history of mankind, either spawning regions of civilization by providing an abundance of rainfall for agriculture or destroying them by periods of drought. The variability of the Hadley circulation is also manifested on interannual times scales as an important component of the waxing and waning of El Nino in the Pacific Ocean, perturbing seasonal climates worldwide.The Hadley circulation was the first phenomenon to be described by using the physical insight of the natural system emerging out of the Renaissance. Both Halley (1686) and Hadley (1735) provided basic accounts of the physical processes that drive the meridional cells. However, a detailed examination of the phenomenon, using data sets that are now available, shows that many questions cannot be answered in the confines of the Halley-Hadley model. An attempt is made to answer these questions from a fundamental physical 9 H.F. Diaz and R.S. Bradley (eds.), The Hadley Circulation: Present, Past and Future,