The Dobson unit (DU) is a unit of measurement of the amount of a trace gas in a vertical column through the Earth's atmosphere. It originated, and continues to be primarily used in respect to, atmospheric ozone, whose total column amount, usually termed "total ozone", and sometimes "column abundance", is dominated by the high concentrations of ozone in the stratospheric ozone layer.
The Dobson Unit is defined as the thickness (in units of 10 µm) of that layer of pure gas which would be formed by the total column amount at standard conditions for temperature and pressure (STP). This is sometimes referred to as a 'milli-atmo-centimeter.' A typical column amount of 300 DU of atmospheric ozone therefore would form a 3 mm layer of pure gas at the surface of the Earth if its temperature and pressure conformed to STP.
The Dobson unit is named after Gordon Dobson, a researcher at the University of Oxford who in the 1920s built the first instrument to measure total ozone from the ground, making use of a double prism monochromator to measure the differential absorption of different bands of solar ultraviolet radiation by the ozone layer. This instrument, called the Dobson ozone spectrophotometer, has formed the backbone of the global network for monitoring atmospheric ozone and was the source of the discovery in 1984 of the Antarctic ozone hole.
Relation to SI units
The Dobson Unit is not part of the SI International System of Units. To address this shortcoming, a brief study in 1982 examined a number of alternative SI-based units suitable for column amounts of not only ozone but any gas in any planetary atmosphere and proposed the use of the unit of mole per square metre for all cases. Examples range from Earth’s trace gases at levels of micro moles per square meter to Venus’ carbon dioxide at mega moles per square meter:
- One mmol m−2 is approximately equivalent to 2,241 DU.
- One DU is equivalent to 0.4462 mmol m−2.
- One DU is also equivalent to 2.687×1020 molecules per square metre.
Typical values of total ozone in the Earth’s atmosphere are conveniently represented in millimoles per square metre (mmol m−2).
A later examination in 1995 of units for use in atmospheric chemistry by the Commission on Atmospheric Chemistry, a part of the International Union of Pure and Applied Chemistry (IUPAC), discouraged the use of special names and symbols for units that are not part of the SI and are not products of powers of SI base units. Although it overlooked the 1982 article it concurred with the view that the Dobson unit should eventually be replaced by an appropriate SI unit and that the unit mmol m-2 was the most convenient and least cumbersome option. It expressed the hope that this unit would eventually supplant the Dobson Unit. However, as of March 2017, there is little evidence that this has occurred; for example the Dobson unit is still used by NASA and by the World Ozone and Ultraviolet Radiation Data Center in their reporting of total ozone amount.
NASA uses a baseline value of 220 DU for ozone. This was chosen as the starting point for observations of the Antarctic ozone hole, since values of less than 220 Dobson units were not found before 1979. Also, from direct measurements over Antarctica, a column ozone level of less than 220 Dobson units is a result of the ozone loss from chlorine and bromine compounds.
In addition, Dobson units are often used to describe total column densities of sulfur dioxide, which occurs in the atmosphere in small amounts due to the combustion of fossil fuels, from biological processes releasing dimethyl sulfide, or by natural combustion such as forest fires. Large amounts of sulfur dioxide may be released into the atmosphere as well by volcanic eruptions. The Dobson unit is used to describe total column amounts of sulfur dioxide because it appeared in the early days of ozone remote sensing on ultraviolet satellite instruments (such as TOMS).
The Dobson Unit arises from the ideal gas law. From the real gas law:
where P and V are pressure and volume, respectively, and n, R and T are the number of moles of gas, the gas constant (8.314 J/mol K), and T is temperature in Kelvin (K).
The number density of air is the number of molecules or atoms per unit volume:
and when plugged into the real gas law, the number density of air is found by using pressure, temperature and the real gas constant.
The number density (molecules/volume) of air at standard temperature and pressure (T = 273K and P = 101325 Pa) is, by using this equation:
With some unit conversions of Joules to Pascals, the equation for molecules/volume is
A Dobson Unit is the total amount of a trace gas per unit area. In atmospheric sciences, this is referred to as a column density. How, though, do we go from units of molecules per cubic meter, a volume, to molecules per square centimeter, an area? This must be done by integration. To get a column density, we must integrate the total column over a height. Per the definition of Dobson Units, we see that 1 DU = 0.01 mm of trace gas when compressed down to sea level at standard temperature and pressure. So if we integrate our number density of air from 0 to 0.01 mm, we find the number density which is equal to 1 DU:
And thus we come up with the value of 1 DU, which is 2.69×1020 molecules per meter squared.
- "Ozone Hole Watch: Facts About Dobson Units".
- IUPAC, Compendium of Chemical Terminology, 2nd ed. (the "Gold Book") (1997). Online corrected version: (2006–) "Dobson unit in atmospheric chemistry".
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