1978
DOI: 10.1029/gl005i001p00037
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Stratospheric nitric oxide and ozone measurements using photoionization mass spectrometry and UV absorption

Abstract: Nitric oxide has been measured in situ between 38.4 and 29.8 km by a new technique, photoionization mass spectrometry. Data indicate a peak mixing ratio of 5.7 ± 0.35 ppbv at 37.5 km and only 0.2 ± 0.2 ppbv at 32.8 km with a sharp gradient in concentration between 33 and 34 km. Simultaneous in‐situ measurements of the ozone concentration show no significant feature at that altitude. The rapid decrease in mixing ratio is not predicted by current theory.

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Cited by 20 publications
(5 citation statements)
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“…The indirect nature of this inference implies substantial uncertainty in the inferred values, but these numbers are in broad agreement with balloon and rocket observations of NO for the middle stratosphere, as discussed, for example, by World Meteorological Organization [1981]. At 35 km, the derived mixing ratio at 32øN in January is about 11 ppbv, in slightly better agreement with the observations of Ridley and Schiff [1981] than the single measurement reported by Maier et al [1978], but we again emphasize that the inference is quite indirect.…”
Section: Results and Analysissupporting
confidence: 84%
“…The indirect nature of this inference implies substantial uncertainty in the inferred values, but these numbers are in broad agreement with balloon and rocket observations of NO for the middle stratosphere, as discussed, for example, by World Meteorological Organization [1981]. At 35 km, the derived mixing ratio at 32øN in January is about 11 ppbv, in slightly better agreement with the observations of Ridley and Schiff [1981] than the single measurement reported by Maier et al [1978], but we again emphasize that the inference is quite indirect.…”
Section: Results and Analysissupporting
confidence: 84%
“…At lower altitudes, data from this flight are comparatively low, especially around the measured minimum at 50 mbar. A similar strong gradient in the NO mixing ratio was also found by Maier et al [1978], though at higher altitudes. Drummond et al [1977] found a strong gradient at lower altitudes.…”
Section: No2 + No3 + M--> N205supporting
confidence: 78%
“…We will report below on a program to measure simultaneously stratospheric total column abundances above 12 km of Ja The variability in the amounts of N20, NO, NO2, and HNO3 with respect to changing latitude, season, and solar input will be examined in turn. Figure 1 shows measured profiles of N20, NO, NO2, and HNO3 as reported by various investigators [Schutz et al, 1970;Goldman et al, 1973Goldman et al, , 1978Marries, 1973;Marries et al, 1974;Ehhalt et al, 1974;Lazrus and Ganø drud, 1974;Ridley et al, 1974Ridley et al, , 1975Ridley et al, , 1976Ackerman et al, 1975;Bloxam et al, 1975;Chaloner et al, 1975;Evans et al, 1975Evans et al, , 1976Fontanella et al, 1975;Schmeltekooef et al, 1975Schmeltekooef et al, , 1977Meidt et al, 1976;Kerr and McElroy, 1976;Drummond et al, 1977;Krey et al, 1977;Loewenstein et al, 1978a, b;Maier et al, 1978;Fedder et al, 1978]. While these profiles show var-iabilities that are due to both natural and instrumental sources, they do demonstrate the typical stratospheric vertical distribution characteristics of each species.…”
Section: Introductionmentioning
confidence: 77%