2020
DOI: 10.3390/atmos11080873
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Investigation of the Vertical Influence of the 11-Year Solar Cycle on Ozone Using SBUV and Antarctic Ground-Based Measurements and CMIP6 Forcing Data

Abstract: The 11-year solar activity cycle in the vertical ozone distribution over the Antarctic station Faraday/Vernadsky in the Antarctic Peninsula region (65.25° S, 64.27° W) was analyzed using the Solar Backscatter Ultra Violet (SBUV) radiometer data Version 8.6 Merged Ozone Data Sets (MOD) over the 40-year period 1979–2018. The SBUV MOD ozone profiles are presented as partial column ozone in layers with approximately 3-km altitude increments from the surface to the lower mesosphere (1000–0.1 hPa, or 0–64 km). Perio… Show more

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Cited by 5 publications
(5 citation statements)
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References 65 publications
(115 reference statements)
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“…The results indicated in Figs. 2 and 3 agree with a study of ozone thickness relation with the solar cycle, in which an 11-year cycle is found only at the low latitude due to Brewer-Dobson circulation (Grytsai et al 2020 ). And the unclear relation between ozone thickness and solar activity in middle and high latitudes is also found by the ground UV-B exposure study using a proxy of pollen grains (Jardine et al 2020 ).…”
Section: Resultssupporting
confidence: 89%
“…The results indicated in Figs. 2 and 3 agree with a study of ozone thickness relation with the solar cycle, in which an 11-year cycle is found only at the low latitude due to Brewer-Dobson circulation (Grytsai et al 2020 ). And the unclear relation between ozone thickness and solar activity in middle and high latitudes is also found by the ground UV-B exposure study using a proxy of pollen grains (Jardine et al 2020 ).…”
Section: Resultssupporting
confidence: 89%
“…It should also be mentioned that relative variations of the ozone concentration in the upper stratosphere and lower mesosphere related to solar activity are more significant than those of the corresponding integral ozone content. For example, it is reported that in the 23rd cycle, relative ozone changes between the solar minimum and maximum in the region of the Antarctic ozone hole amounted to 6.8-9.6% at altitudes of 22-31 km [31]. So, this effect could be considered as one of reasons for the decrease in variances in the 2007-2017 decade.…”
Section: Discussionmentioning
confidence: 99%
“…The raw response uncertainty for each SABER channel was estimated using Equation (30). This uncertainty represents the short-term temporal measurement errors for each individual measurement.…”
Section: Response Noise and Uncertaintymentioning
confidence: 99%
“…This uncertainty represents the short-term temporal measurement errors for each individual measurement. (30) where:…”
Section: Response Noise and Uncertaintymentioning
confidence: 99%