2018
DOI: 10.5194/amt-11-5105-2018
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Examination on total ozone column retrievals by Brewer spectrophotometry using different processing software

Abstract: Abstract. The availability of long-term records of the total ozone content (TOC) represents a valuable source of information for studies on the assessment of short- and long-term atmospheric changes and their impact on the terrestrial ecosystem. In particular, ground-based observations represent a valuable tool for validating satellite-derived products. To our knowledge, details about software packages for processing Brewer spectrophotometer measurements and for retrieving the TOC are seldom specified in studi… Show more

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Cited by 24 publications
(30 citation statements)
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“…The standard uncertainty (for wavelengths above 305 nm and solar zenith angles (SZA) below 75 • ) of the UV spectra is estimated as 5% for Rome and 3% for Aosta [96,106]. The accuracy of the total ozone measurements from Brewer spectrophotometers is estimated to be 1% [118,119]. Spectra from the two stations have been processed using the SHICrivm algorithm [120] in order to correct them for the effect of wavelength shift, and extend the spectra up to 400 nm for Brewer #067 (in order to calculate erythemal irradiance).…”
Section: Uv In Rome and Aostamentioning
confidence: 99%
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“…The standard uncertainty (for wavelengths above 305 nm and solar zenith angles (SZA) below 75 • ) of the UV spectra is estimated as 5% for Rome and 3% for Aosta [96,106]. The accuracy of the total ozone measurements from Brewer spectrophotometers is estimated to be 1% [118,119]. Spectra from the two stations have been processed using the SHICrivm algorithm [120] in order to correct them for the effect of wavelength shift, and extend the spectra up to 400 nm for Brewer #067 (in order to calculate erythemal irradiance).…”
Section: Uv In Rome and Aostamentioning
confidence: 99%
“…Total ozone data from the Brewer#067 and the Brewer with serial number 66 (Brewer#066) were analyzed for Rome and Aosta respectively. UV and total ozone datasets from the two stations have all been subjected to quality control/quality assurance (QC/QA), and are traceable to international reference standards [97,106,118]. The standard uncertainty (for wavelengths above 305 nm and solar zenith angles (SZA) below 75 • ) of the UV spectra is estimated as 5% for Rome and 3% for Aosta [96,106].…”
Section: Uv In Rome and Aostamentioning
confidence: 99%
“…CC BY 4.0 License. (Siani et al, 2018). Yet, individual total ozone values were discarded when standard deviation is above 2.5 DU and ozone air mass (defined as the ratio of the actual ozone path length taken by the direct solar beam to the analogous vertical ozone path when the Sun is overhead from the surface to the top of the atmosphere) is above 3.5.…”
Section: Methodsmentioning
confidence: 99%
“…The standard uncertainty (for wavelengths above 305 nm and SZAs below 75°) of the UV spectra is estimated as 5% for Rome and 3% for Aosta [94,104]. The accuracy of the total ozone measurements from Brewer spectrophotometers is estimated to be ~1% [116,117]. Spectra from the two stations have been processed using the SHICrivm algorithm [118] in order to correct them for the effect of wavelength shift, and extend the spectra up to 400 nm for Brewer #067 (in order to calculate erythemal irradiance).…”
Section: Uv In Rome and Aostamentioning
confidence: 98%
“…Total ozone data from the Brewer#067 and the Brewer with serial number 66 (Brewer#066) have been analyzed for Rome and Aosta respectively. UV and total ozone datasets from the two stations have all been subjected to quality control/quality assurance (QC/QA), and are traceable to international reference standards [95,104,116]. The standard uncertainty (for wavelengths above 305 nm and SZAs below 75°) of the UV spectra is estimated as 5% for Rome and 3% for Aosta [94,104].…”
Section: Uv In Rome and Aostamentioning
confidence: 99%