Abstract
The importance of bromine chemistry was recognized shortly after Molina and Rowland1 had drawn attention to chlorine atom-catalysed destruction of ozone. Bromine atoms are even more efficient catalysts than chlorine2,3, and both may act synergistically to deplete ozone in the lower stratosphere4. Some measurements of bromine-containing source gases, such as CH3Br, CHBr3, CH2BrCH2Br, CH2Br2, CBrF3 and CBrClF2 have been reported for the troposphere5–8, their vertical distribution in the stratosphere is unknown except for CBrF3 (CFC-13B1) and CH3Br (ref. 6). These, together with the fully halogenated CBrClF2 (CFC-12B1), are probably the most important source gases for stratospheric bromine radicals. We report here the first stratospheric profiles of CBrClF2 up to 25 km, measured at 44° N during three consecutive years. From these data it follows that the atmospheric abundance of this halocarbon is growing rapidly, at a rate of 20% per year in the Northern Hemisphere, corresponding to a worldwide emission of ∼3.6×103 tons per year.
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References
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Lal, S., Borchers, R., Fabian, P. et al. Increasing abundance of CBrClF2 in the atmosphere. Nature 316, 135–136 (1985). https://doi.org/10.1038/316135a0
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DOI: https://doi.org/10.1038/316135a0
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