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• W2000646112 abstract "Solar ultraviolet flux changes associated with the 27-day solar rotational period cause corresponding variations in mesospheric ozone near the maximum of the 11-year sunspot cycle. This statement is based on a correlation and spectral analysis of ozone mixing ratios, deduced from Solar Mesospheric Explorer satellite-based measurements of 1.27-µm O2 airglow emission and solar flux observations made from the same spacecraft in 1982. With the Lyman α flux taken as an indicator of solar ultraviolet variability, spectral analysis shows a primary period of 27.1 days with a secondary period of 13.5 days. The 27.1- day period is observed in the ozone mixing ratio data together with other periods, including 13.5 days. Both a classical statistical analysis and a time series treatment show that for 244 days there is a correlation between ozone and solar flux near 50 km and between 65 and 70 km. Calculations predict a positive correlation over the entire mesosphere if there is no change in temperature accompanying the solar flux. Lack of correlation is temperature induced." @default.
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• W2000646112 date "1986-05-01" @default.
• W2000646112 modified "2023-10-16" @default.
• W2000646112 title "Mesospheric ozone changes associated with 27 day solar ultraviolet flux variations" @default.
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• W2000646112 doi "https://doi.org/10.1029/gl013i005p00427" @default.
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