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- W2149166120 abstract "The predictions of a radiative-photochemical model are compared with observations of the diurnal variation of mesospheric ozone obtained from rocket-borne experiments. Temperature observations from the SAMS instrument on the Nimbus-7 satellite are used to define the basic atmospheric state. Good agreement is found, provided that low water vapour abundances are accepted, together with slow rate coefficients for the recombination of odd hydrogen species. Sensitivity tests performed with the model show that uncertainties in the ozone calculations arise chiefly from uncertainties in water vapour concentrations, solar irradiance, O2 absorption cross-sections and certain rate coefficients, and that the sensitivity of ozone to these parameters may be markedly different at different times of day, especially above 60 km. The model's representation of the ozone variation around dawn is also used to estimate the error caused by the assumption of spherical uniformity when deriving ozone concentrations from solar occultation experiments." @default.
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- W2149166120 date "1984-01-01" @default.
- W2149166120 modified "2023-09-30" @default.
- W2149166120 title "Mesospheric ozone — theory and observation" @default.
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- W2149166120 doi "https://doi.org/10.1002/qj.49711046316" @default.
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