Abstract
Abstract. The short- and long-term variability of the surface spectral solar ultraviolet (UV) irradiance is investigated across Italy using high-quality ground-based measurements from three locations: Aosta (45.7∘ N, 7.4∘ E, 570 m a.s.l.), Rome (41.9∘ N, 12.5∘ E, 15 75 m a.s.l.), and Lampedusa (35.5∘ N, 12.6∘ E, 50 m a.s.l.). The three sites are characterized by different environmental conditions and represent almost the full latitudinal extent of the Italian territory. Data of two periods were analysed: 2006–2020 (all sites) and 1996–2020 (Rome only). The main objective of this study is to quantify the effect of the geopotential height (GPH) at 250 hPa on total ozone, and spectral irradiance at 307.5 and 324 nm. We first show that monthly anomalies in GPH, total ozone, and spectral irradiances are correlated amongst the three sites, suggesting that Italy is often affected by the same synoptical weather systems. We further find statistically significant anticorrelations between GPH and monthly anomalies in total ozone for all stations and months. Conversely, we identify positive correlations between GPH and monthly anomalies in spectral irradiance at 307.5 nm for most months. The influence of GPH on short-term variability also hold for long-term trends. For example, long-term changes in total ozone over the period 2006–2020 were associated with changes in GPH for all stations. This suggests that observed negative trends in total ozone were mainly driven by changes in lower-stratospheric ozone as upper-stratospheric ozone was increasing over this period. For several months of the year, positive trends in UV irradiance were observed, and we found that these trends were predominantly caused by changes in clouds and/or aerosols instead of total ozone. For the longer period of 1996–2020, a statistically significant annualized decrease in total ozone of ∼ 0.1 % per year was identified for Rome and could subsequently be attributed to decreasing lower-stratospheric ozone. While positive trends in spectral irradiance at 307.5 nm were observed for several months of this extended period, the negative trend in total ozone did not lead to a positive trend in the spectral irradiance at 307.5 nm in the deseasonalized data. Our study provides evidence that dynamical processes taking place in the troposphere lead to significant variability in total ozone and surface solar UV irradiance.
Highlights
The amount of solar ultraviolet radiation (UVR) reaching the Earth’s surface is an important environmental, ecological, and atmospheric parameter to be measured and studied
Deriving trends of the total ozone from MERRA-2 is more uncertain than deriving trends from good-quality ground-based measurements (Zhao et al, 2021), the graphs in Fig. 9 still show clearly that for the 2 months considered (April and September), negative trends in total ozone coincided with positive trends in the geopotential height (GPH) over wide areas
The variability of solar UV irradiance at 307.5 and 324 nm and the 307.5/324 nm ratio was analysed with respect to the variability of total ozone and GPH
Summary
The amount of solar ultraviolet radiation (UVR) reaching the Earth’s surface is an important environmental, ecological, and atmospheric parameter to be measured and studied. Dynamical phenomena occasionally (once every few years) favour extensive destruction of Arctic stratospheric ozone in early spring (Dameris et al, 2021; Manney et al, 2011; Pommereau et al, 2018; Varotsos et al, 2012; Wohltmann et al, 2020), leading to reduced ozone over Northern Hemisphere high latitudes and midlatitudes (due to the transport of poor-ozone air masses from the poles towards midlatitudes) and subsequently to very high levels of solar UVB radiation at the Earth’s surface (Bernhard and Stierle, 2020; Petkov et al, 2014).
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