The seasonal variations of ozone and temperature in the middle and the upper stratosphere
The seasonal variations in ozone and temperature inferred from the Nimbus-4 BUV (Backscatter Ultraviolet Spectrometer) and the SCR (Selective Chopper Radiometer) experiments are compared with predictions based on a simplified radiative photochemical model. It is shown that the observations, in agreement with the model calculations, show a systematic phase shift from a summer maximum at 10 mb to a winter maximum at 1 mb with equinoctial maxima at intermediate heights. In contrast, the temperature between these pressure levels shows no appreciable phase shift and the summer maximum prevails at all heights. The observed phase differences in ozone and temperature are shown to be a manifestation of the radiative feedback on the photochemistry of the upper stratosphere.