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Long-Term Variations of Global Solar Radiation and Its Potential Effects at Dome C (Antarctica)

An empirical model to predict hourly global solar irradiance under all-sky conditions as a function of absorbing and scattering factors has been applied at the Dome C station in the Antarctic, using measured solar radiation and meteorological variables. The calculated hourly global solar irradiance...

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Autores principales: Bai, Jianhui, Zong, Xuemei, Lanconelli, Christian, Lupi, Angelo, Driemel, Amelie, Vitale, Vito, Li, Kaili, Song, Tao
Formato: Online Artículo Texto
Lenguaje:English
Publicado: MDPI 2022
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8910517/
https://www.ncbi.nlm.nih.gov/pubmed/35270776
http://dx.doi.org/10.3390/ijerph19053084
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author Bai, Jianhui
Zong, Xuemei
Lanconelli, Christian
Lupi, Angelo
Driemel, Amelie
Vitale, Vito
Li, Kaili
Song, Tao
author_facet Bai, Jianhui
Zong, Xuemei
Lanconelli, Christian
Lupi, Angelo
Driemel, Amelie
Vitale, Vito
Li, Kaili
Song, Tao
author_sort Bai, Jianhui
collection PubMed
description An empirical model to predict hourly global solar irradiance under all-sky conditions as a function of absorbing and scattering factors has been applied at the Dome C station in the Antarctic, using measured solar radiation and meteorological variables. The calculated hourly global solar irradiance agrees well with measurements at the ground in 2008–2011 (the model development period) and at the top of the atmosphere (TOA). This model is applied to compute global solar irradiance at the ground and its extinction in the atmosphere caused by absorbing and scattering substances during the 2006–2016 period. A sensitivity study shows that the responses of global solar irradiance to changes in water vapor and scattering factors (expressed by water vapor pressure and S/G, respectively; S and G are diffuse and global solar irradiance, respectively) are nonlinear and negative, and that global solar irradiance is more sensitive to changes in scattering than to changes in water vapor. Applying this empirical model, the albedos at the TOA and the surface in 2006–2016 are estimated and found to agree with the satellite-based retrievals. During 2006–2016, the annual mean observed and estimated global solar exposures decreased by 0.05% and 0.09%, respectively, and the diffuse exposure increased by 0.68% per year, associated with the yearly increase of the S/G ratio by 0.57% and the water vapor pressure by 1.46%. The annual mean air temperature increased by about 1.80 °C over the ten years, and agrees with the warming trends for all of Antarctica. The annual averages were 316.49 Wm(−2) for the calculated global solar radiation, 0.332 for S/G, −46.23 °C for the air temperature and 0.10 hPa for the water vapor pressure. The annual mean losses of solar exposure due to absorbing and scattering substances and the total loss were 4.02, 0.19 and 4.21 MJ m(−2), respectively. The annual mean absorbing loss was much larger than the scattering loss; their contributions to the total loss were 95.49% and 4.51%, respectively, indicating that absorbing substances are dominant and play essential roles. The annual absorbing, scattering and total losses increased by 0.01%, 0.39% and 0.28% per year, respectively. The estimated and satellite-retrieved annual albedos increased at the surface. The mechanisms of air-temperature change at two pole sites, as well as a mid-latitude site, are discussed.
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spelling pubmed-89105172022-03-11 Long-Term Variations of Global Solar Radiation and Its Potential Effects at Dome C (Antarctica) Bai, Jianhui Zong, Xuemei Lanconelli, Christian Lupi, Angelo Driemel, Amelie Vitale, Vito Li, Kaili Song, Tao Int J Environ Res Public Health Article An empirical model to predict hourly global solar irradiance under all-sky conditions as a function of absorbing and scattering factors has been applied at the Dome C station in the Antarctic, using measured solar radiation and meteorological variables. The calculated hourly global solar irradiance agrees well with measurements at the ground in 2008–2011 (the model development period) and at the top of the atmosphere (TOA). This model is applied to compute global solar irradiance at the ground and its extinction in the atmosphere caused by absorbing and scattering substances during the 2006–2016 period. A sensitivity study shows that the responses of global solar irradiance to changes in water vapor and scattering factors (expressed by water vapor pressure and S/G, respectively; S and G are diffuse and global solar irradiance, respectively) are nonlinear and negative, and that global solar irradiance is more sensitive to changes in scattering than to changes in water vapor. Applying this empirical model, the albedos at the TOA and the surface in 2006–2016 are estimated and found to agree with the satellite-based retrievals. During 2006–2016, the annual mean observed and estimated global solar exposures decreased by 0.05% and 0.09%, respectively, and the diffuse exposure increased by 0.68% per year, associated with the yearly increase of the S/G ratio by 0.57% and the water vapor pressure by 1.46%. The annual mean air temperature increased by about 1.80 °C over the ten years, and agrees with the warming trends for all of Antarctica. The annual averages were 316.49 Wm(−2) for the calculated global solar radiation, 0.332 for S/G, −46.23 °C for the air temperature and 0.10 hPa for the water vapor pressure. The annual mean losses of solar exposure due to absorbing and scattering substances and the total loss were 4.02, 0.19 and 4.21 MJ m(−2), respectively. The annual mean absorbing loss was much larger than the scattering loss; their contributions to the total loss were 95.49% and 4.51%, respectively, indicating that absorbing substances are dominant and play essential roles. The annual absorbing, scattering and total losses increased by 0.01%, 0.39% and 0.28% per year, respectively. The estimated and satellite-retrieved annual albedos increased at the surface. The mechanisms of air-temperature change at two pole sites, as well as a mid-latitude site, are discussed. MDPI 2022-03-06 /pmc/articles/PMC8910517/ /pubmed/35270776 http://dx.doi.org/10.3390/ijerph19053084 Text en © 2022 by the authors. https://creativecommons.org/licenses/by/4.0/Licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license (https://creativecommons.org/licenses/by/4.0/).
spellingShingle Article
Bai, Jianhui
Zong, Xuemei
Lanconelli, Christian
Lupi, Angelo
Driemel, Amelie
Vitale, Vito
Li, Kaili
Song, Tao
Long-Term Variations of Global Solar Radiation and Its Potential Effects at Dome C (Antarctica)
title Long-Term Variations of Global Solar Radiation and Its Potential Effects at Dome C (Antarctica)
title_full Long-Term Variations of Global Solar Radiation and Its Potential Effects at Dome C (Antarctica)
title_fullStr Long-Term Variations of Global Solar Radiation and Its Potential Effects at Dome C (Antarctica)
title_full_unstemmed Long-Term Variations of Global Solar Radiation and Its Potential Effects at Dome C (Antarctica)
title_short Long-Term Variations of Global Solar Radiation and Its Potential Effects at Dome C (Antarctica)
title_sort long-term variations of global solar radiation and its potential effects at dome c (antarctica)
topic Article
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8910517/
https://www.ncbi.nlm.nih.gov/pubmed/35270776
http://dx.doi.org/10.3390/ijerph19053084
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