Solar UV-B irradiance and total ozone in Italy: Fluctuations and trends

Solar UV irradiance spectra (290–325 nm) together with daily total ozone column observations have been collected since 1992 by means of Brewer spectrophotometers at two Italian stations (Rome and Ispra). The available Brewer irradiance data, recorded around noon and at fixed solar zenith angles, tog...

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Veröffentlicht in:Journal of Geophysical Research 2000-02, Vol.105 (D4), p.4895-4901
Hauptverfasser: Casale, G. R., Meloni, D., Miano, S., Palmieri, S., Siani, A. M., Cappellani, F.
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container_end_page 4901
container_issue D4
container_start_page 4895
container_title Journal of Geophysical Research
container_volume 105
creator Casale, G. R.
Meloni, D.
Miano, S.
Palmieri, S.
Siani, A. M.
Cappellani, F.
description Solar UV irradiance spectra (290–325 nm) together with daily total ozone column observations have been collected since 1992 by means of Brewer spectrophotometers at two Italian stations (Rome and Ispra). The available Brewer irradiance data, recorded around noon and at fixed solar zenith angles, together with the output of a radiative transfer model (the STAR model) are presented and analyzed. The Brewer irradiance measurements and total ozone fluctuations and anomalies are investigated, pointing out the correlation between the high‐frequency O3 components and irradiance at 305 nm. In addition, the total ozone long time series of Arosa (170 km apart from Ispra) and Vigna di Valle (very close to Rome) are analyzed to illustrate evidence of temporal variations and a possible trend.
doi_str_mv 10.1029/1999JD900303
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source Wiley Journals; Wiley-Blackwell AGU Digital Library; Wiley Online Library (Open Access Collection); Alma/SFX Local Collection
subjects Earth, ocean, space
Exact sciences and technology
External geophysics
Meteorology
Radiative transfer. Solar radiation
title Solar UV-B irradiance and total ozone in Italy: Fluctuations and trends
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