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close this bookNatural Energy and Vernacular Architecture: Principles and Examples with Reference to Hot Arid Climates (UNU, 1986, 172 pages)
close this folderPart 1. Man, natural environment, and architecture
close this folder2. Architectural thermodynamics and human comfort in hot climates
View the document(introductory text...)
View the documentTemperature
View the documentThermal conduction and resistance
View the documentRadiation
View the documentThermal convection
View the documentAtmospheric pressure
View the documentWater vapor
View the documentCooling by evaporation
View the documentThermal gain
View the documentThermal loss
View the documentDynamic thermal equilibrium
View the documentHeat-regulating mechanisms of the human body
View the documentMeasurement of conditions of human comfort

Atmospheric pressure

Air exerts a pressure on any surface in the atmosphere which corresponds to the weight of the column of air that it supports. Every surface in the neighborhood of sea level carries a load of about 1 kg per cm², or 1 ton per ft². As the altitude increases above sea level, the atmosphere below no longer contributes to the pressure, which is correspondingly reduced.

Using this concept, atmospheric pressure can be expressed as the height of a column of mercury in a barometer, in millimeters or inches, with the pressure at sea level being 760 mm or 29.9 inches of mercury at a standard temperature of 0 °C (32 °F). The barometer reading must be corrected for the temperature of the mercury as well as for the latitude.

The bar is the unit of pressure in an absolute system of measurement adopted for scientific use to replace the arbitrarily chosen column of mercury. Atmospheric-pressure measurements in meteorological work are normally expressed in units of one millibar. One bar corresponds very nearly to 750 mm or 29.5 inches of mercury at 0 °C (32 °F), or 1019 cm or 401 inches of water, which is the atmospheric pressure a little above sea level.