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Profiles for key stratospheric fluorine species are presented along with HF:HCl ratio. Discrepancies between theory and observation are examined and their implications are discussed. Our results indicate that the HF:HCl ratio depends critically on OH concentration between 20‐30 km and it might provide an indirect check on the present stratospheric OH chemistry or H2O abundances which are of central importance to stratospheric chemical processes.
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Nien Dak Sze (1978) studied this question.
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