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 |
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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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R. ; Meloni, D. ; Miano, S. ; Palmieri, S. ; Siani, A. M. ; Cappellani, F.</creator><creatorcontrib>Casale, G. R. ; Meloni, D. ; Miano, S. ; Palmieri, S. ; Siani, A. M. ; Cappellani, F.</creatorcontrib><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.</description><identifier>ISSN: 0148-0227</identifier><identifier>EISSN: 2156-2202</identifier><identifier>DOI: 10.1029/1999JD900303</identifier><language>eng</language><publisher>Washington, DC: Blackwell Publishing Ltd</publisher><subject>Earth, ocean, space ; Exact sciences and technology ; External geophysics ; Meteorology ; Radiative transfer. 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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.</description><subject>Earth, ocean, space</subject><subject>Exact sciences and technology</subject><subject>External geophysics</subject><subject>Meteorology</subject><subject>Radiative transfer. 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Solar radiation</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Casale, G. R.</creatorcontrib><creatorcontrib>Meloni, D.</creatorcontrib><creatorcontrib>Miano, S.</creatorcontrib><creatorcontrib>Palmieri, S.</creatorcontrib><creatorcontrib>Siani, A. M.</creatorcontrib><creatorcontrib>Cappellani, F.</creatorcontrib><collection>Istex</collection><collection>Pascal-Francis</collection><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Journal of Geophysical Research</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Casale, G. R.</au><au>Meloni, D.</au><au>Miano, S.</au><au>Palmieri, S.</au><au>Siani, A. M.</au><au>Cappellani, F.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Solar UV-B irradiance and total ozone in Italy: Fluctuations and trends</atitle><jtitle>Journal of Geophysical Research</jtitle><addtitle>J. Geophys. Res</addtitle><date>2000-02-27</date><risdate>2000</risdate><volume>105</volume><issue>D4</issue><spage>4895</spage><epage>4901</epage><pages>4895-4901</pages><issn>0148-0227</issn><eissn>2156-2202</eissn><abstract>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.</abstract><cop>Washington, DC</cop><pub>Blackwell Publishing Ltd</pub><doi>10.1029/1999JD900303</doi><tpages>7</tpages></addata></record> |
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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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