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• W2069927928 startingPage "2063" @default.
• W2069927928 abstract "In solar cycles 22–23, all solar indices showed maxima near 1990 and 2000 and minima in 1996. The maximum to minimum variation was only ∼1–2% in the UV range 240–350nm. Dobson ozone intensities did not show any clear relationship with solar cycle and ozone variations were less than 10%. The UV-B (295–325nm) observed at ground by Brewer spectrophotometers at some locations had variations of ∼50–100% for 295–300nm, and ∼20–50% for 305–325nm. The maxima were in different years at different locations (even with separations of only ∼300km), did not match with the solar cycle, and were far too large to be explained on the basis of ozone changes (1% decrease of ozone is expected to cause ∼2% increase of UV-B). Thus, if the data are not bad, the UV-B changes do not match with solar activity or ozone changes and must be mostly due to other local effects (clouds, etc.?). When data are averaged over wide geographical regions, UV-B variation ranges are smaller (∼10–20%, probably because localised, highly varying cloud effects get filtered out), and are roughly as expected from ozone variations." @default.
• W2069927928 created "2016-06-24" @default.
• W2069927928 creator A5087949757 @default.
• W2069927928 date "2002-12-01" @default.
• W2069927928 modified "2023-10-16" @default.
• W2069927928 title "Mismatch between variations of solar indices, stratospheric ozone and UV-B observed at ground" @default.
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• W2069927928 doi "https://doi.org/10.1016/s1364-6826(02)00219-5" @default.
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