Assessment of spectral UV radiation at Marambio Base, Antarctic Peninsula

This study aims to assess the dependence of spectral UV radiation on different atmospheric and terrestrial factors, including solar zenith angle, ozone, and cloud cover, in the southern polar environment. For this purpose, 23 260 spectra (300–363 nm), obtained by the B199 Mk-III Brewer spectrophotom...

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Published in:Atmospheric Chemistry and Physics
Main Authors: Čížková, Klára, Láska, Kamil, Metelka, Ladislav, Staněk, Martin
Format: Text
Language:English
Published: 2023
Subjects:
Online Access:https://doi.org/10.5194/acp-23-4617-2023
https://acp.copernicus.org/articles/23/4617/2023/
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spelling ftcopernicus:oai:publications.copernicus.org:acp105343 2023-06-11T04:06:54+02:00 Assessment of spectral UV radiation at Marambio Base, Antarctic Peninsula Čížková, Klára Láska, Kamil Metelka, Ladislav Staněk, Martin 2023-04-18 application/pdf https://doi.org/10.5194/acp-23-4617-2023 https://acp.copernicus.org/articles/23/4617/2023/ eng eng doi:10.5194/acp-23-4617-2023 https://acp.copernicus.org/articles/23/4617/2023/ eISSN: 1680-7324 Text 2023 ftcopernicus https://doi.org/10.5194/acp-23-4617-2023 2023-04-24T16:23:13Z This study aims to assess the dependence of spectral UV radiation on different atmospheric and terrestrial factors, including solar zenith angle, ozone, and cloud cover, in the southern polar environment. For this purpose, 23 260 spectra (300–363 nm), obtained by the B199 Mk-III Brewer spectrophotometer at Marambio Base, Antarctic Peninsula region, over the period 2010–2020, were studied. A neural network model was developed to investigate the effects of the explanatory variables at 127 wavelengths in the interval 300–363 nm, with a 0.5 nm sampling interval. Solar zenith angle (SZA) proved to be the most important parameter, followed by cloud cover, total ozone column (TOC), and surface albedo. The relative SZA effect is greatest at the shortest wavelengths, where a 1 ∘ decrease in SZA results in a 6 %–18 % increase in UV irradiance (305 nm). TOC particularly affects the short wavelengths below approximately 320–325 nm, when for example at 305 nm a 10 DU decrease in TOC causes a 7 %–13 % increase in UV irradiance. The large-scale ozone holes (e.g., in 2011–2012, 2014–2015, 2018–2019) caused the spectral UV irradiance at very short wavelengths to peak in spring, whereas in other seasons (e.g., 2010–2011, 2012–2013), the maxima at all wavelengths were recorded in summer (November to January). Absorption of UV radiance by the ozone also affected the temporal distribution of very high spectral UV irradiances (i.e., highest 10 % of the distribution), when at 305 nm they were observed both in spring and summer months, and at 340 nm they occurred mostly in summer. The effect of cloud cover was strongest near the fully cloudy sky and in the summer months, when the Antarctic clouds tend to be thickest. Text Antarc* Antarctic Antarctic Peninsula Copernicus Publications: E-Journals Antarctic Antarctic Peninsula Marambio ENVELOPE(-56.750,-56.750,-64.283,-64.283) The Antarctic Atmospheric Chemistry and Physics 23 8 4617 4636
institution Open Polar
collection Copernicus Publications: E-Journals
op_collection_id ftcopernicus
language English
description This study aims to assess the dependence of spectral UV radiation on different atmospheric and terrestrial factors, including solar zenith angle, ozone, and cloud cover, in the southern polar environment. For this purpose, 23 260 spectra (300–363 nm), obtained by the B199 Mk-III Brewer spectrophotometer at Marambio Base, Antarctic Peninsula region, over the period 2010–2020, were studied. A neural network model was developed to investigate the effects of the explanatory variables at 127 wavelengths in the interval 300–363 nm, with a 0.5 nm sampling interval. Solar zenith angle (SZA) proved to be the most important parameter, followed by cloud cover, total ozone column (TOC), and surface albedo. The relative SZA effect is greatest at the shortest wavelengths, where a 1 ∘ decrease in SZA results in a 6 %–18 % increase in UV irradiance (305 nm). TOC particularly affects the short wavelengths below approximately 320–325 nm, when for example at 305 nm a 10 DU decrease in TOC causes a 7 %–13 % increase in UV irradiance. The large-scale ozone holes (e.g., in 2011–2012, 2014–2015, 2018–2019) caused the spectral UV irradiance at very short wavelengths to peak in spring, whereas in other seasons (e.g., 2010–2011, 2012–2013), the maxima at all wavelengths were recorded in summer (November to January). Absorption of UV radiance by the ozone also affected the temporal distribution of very high spectral UV irradiances (i.e., highest 10 % of the distribution), when at 305 nm they were observed both in spring and summer months, and at 340 nm they occurred mostly in summer. The effect of cloud cover was strongest near the fully cloudy sky and in the summer months, when the Antarctic clouds tend to be thickest.
format Text
author Čížková, Klára
Láska, Kamil
Metelka, Ladislav
Staněk, Martin
spellingShingle Čížková, Klára
Láska, Kamil
Metelka, Ladislav
Staněk, Martin
Assessment of spectral UV radiation at Marambio Base, Antarctic Peninsula
author_facet Čížková, Klára
Láska, Kamil
Metelka, Ladislav
Staněk, Martin
author_sort Čížková, Klára
title Assessment of spectral UV radiation at Marambio Base, Antarctic Peninsula
title_short Assessment of spectral UV radiation at Marambio Base, Antarctic Peninsula
title_full Assessment of spectral UV radiation at Marambio Base, Antarctic Peninsula
title_fullStr Assessment of spectral UV radiation at Marambio Base, Antarctic Peninsula
title_full_unstemmed Assessment of spectral UV radiation at Marambio Base, Antarctic Peninsula
title_sort assessment of spectral uv radiation at marambio base, antarctic peninsula
publishDate 2023
url https://doi.org/10.5194/acp-23-4617-2023
https://acp.copernicus.org/articles/23/4617/2023/
long_lat ENVELOPE(-56.750,-56.750,-64.283,-64.283)
geographic Antarctic
Antarctic Peninsula
Marambio
The Antarctic
geographic_facet Antarctic
Antarctic Peninsula
Marambio
The Antarctic
genre Antarc*
Antarctic
Antarctic Peninsula
genre_facet Antarc*
Antarctic
Antarctic Peninsula
op_source eISSN: 1680-7324
op_relation doi:10.5194/acp-23-4617-2023
https://acp.copernicus.org/articles/23/4617/2023/
op_doi https://doi.org/10.5194/acp-23-4617-2023
container_title Atmospheric Chemistry and Physics
container_volume 23
container_issue 8
container_start_page 4617
op_container_end_page 4636
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