Dust impact on surface solar irradiance assessed with model simulations, satellite observations and ground-based measurements

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Kosmopoulos, Panagiotis G., Kazadzis, Stelios, Taylor, Michael ORCID: https://orcid.org/0000-0002-3473-3478, Athanasopoulou, Eleni, Raptis, Panagiotis I., Speyer, Orestis, Marinou, Eleni, Proestakis, Emmanouil, Solomos, Stavros, Gerasopoulos, Evangelos, Amiridis, Vassilis, Bais, Alkiviadis and Kontoes, Charalabos (2017) Dust impact on surface solar irradiance assessed with model simulations, satellite observations and ground-based measurements. Atmospheric Measurement Techniques, 10. pp. 2435-2453. ISSN 1867-1381

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Official URL: https://amt.copernicus.org/articles/10/2435/2017/

Abstract

This study assesses the impact of dust on surface solar radiation focussing on an extreme dust event. For this purpose, we exploited the synergy of AERONET measurements and passive and active satellite remote sensing (MODIS and CALIPSO) observations, in conjunction with radiative transfer model (RTM) and chemical transport model (CTM) simulations and the 1-day forecasts from the Copernicus Atmosphere Monitoring Service (CAMS). The area of interest is the eastern Mediterranean where anomalously high aerosol loads were recorded between 30 January and 3 February 2015. The intensity of the event was extremely high, with aerosol optical depth (AOD) reaching 3.5, and optical/microphysical properties suggesting aged dust. RTM and CTM simulations were able to quantify the extent of dust impact on surface irradiances and reveal substantial reduction in solar energy exploitation capacity of PV and CSP installations under this high aerosol load. We found that such an extreme dust event can result in Global Horizontal Irradiance (GHI) attenuation by as much as 40–50 % and a much stronger Direct Normal Irradiance (DNI) decrease (80–90 %), while spectrally this attenuation is distributed to 37 % in the UV region, 33 % in the visible and around 30 % in the infrared. CAMS forecasts provided a reliable available energy assessment (accuracy within 10 % of that obtained from MODIS). Spatially, the dust plume resulted in a zonally averaged reduction of GHI and DNI of the order of 150 W m−2 in southern Greece, and a mean increase of 20 W m−2 in the northern Greece as a result of lower AOD values combined with local atmospheric processes. This analysis of a real-world scenario contributes to the understanding and quantification of the impact range of high aerosol loads on solar energy and the potential for forecasting power generation failures at sunshine-privileged locations where solar power plants exist, are under construction or are being planned.

Item Type:	Article
Faculty \ School:	Faculty of Science > School of Environmental Sciences University of East Anglia Research Groups/Centres > Theme - ClimateUEA
UEA Research Groups:	Faculty of Science > Research Groups > Climatic Research Unit
Depositing User:	LivePure Connector
Date Deposited:	06 Aug 2020 23:53
Last Modified:	25 Sep 2024 15:41
URI:	https://ueaeprints.uea.ac.uk/id/eprint/76360
DOI:	10.5194/amt-10-2435-2017

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