The OH number density in the stratosphere has been measured over the altitude interval of 37 to 23 km at midday via a balloon‐borne gondola launched from Palestine, Texas on July 6, 1988. OH radicals are detected with a laser induced fluorescence instrument employing a 17 kHz repetition rate copper vapor laser pumped dye laser optically coupled to an enclosed flow, in‐situ sampling chamber. OH abundances ranged from 88±31 pptv (1.1 ± 0.4 × 107 molec cm−3) in the 36 to 35 km interval to 0.9 ± 0.8 pptv (8.7 ± 7.7 × 105 molec cm−3) in the 24 to 23 km interval. The stated uncertainty (±1σ) includes that from both measurement precision and accuracy. Simultaneous detection of ozone and water vapor densities was carried out with separate on‐board instruments.
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Stimpfle et al. (1989) studied this question.
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