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Upper Limit of Iodine Oxide in the Lower Stratosphere

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Abstract

It has been suggested that iodine oxides, IOx, could play a significant role in the ozone destruction in the lower stratosphere. To investigate this suggestion, spectra from nine SAOZ uv-visible spectrometer balloon flights were examined for the IO absorption signature between 405 and 450 nm. IO was not detected, either at mid- or high latitude, in the morning or the evening, in summer or winter. An upper limit of 0.2 parts per trillion by volume (pptv) at 20 km and 0.1 pptv at 15 km at the 95% confidence level (2σ), was derived from the best measurements at 90° SZA at sunset and sunrise. Since a photochemical model shows that 70% of inorganic iodine should be in the form IO at that time, it is concluded that unless iodine chemistry is different from that assumed at the moment, the role of iodine in stratospheric ozone depletion is small.

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Pundt, I., Pommereau, JP., Phillips, C. et al. Upper Limit of Iodine Oxide in the Lower Stratosphere. Journal of Atmospheric Chemistry 30, 173–185 (1998). https://doi.org/10.1023/A:1006071612477

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  • DOI: https://doi.org/10.1023/A:1006071612477

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