Preprints
https://doi.org/10.5194/egusphere-2026-2775
https://doi.org/10.5194/egusphere-2026-2775
27 May 2026
 | 27 May 2026
Status: this preprint is open for discussion and under review for Atmospheric Measurement Techniques (AMT).

Dust Radiative Effects and Impact on Energy Production over the Mediterranean Basin

Dimitra Kouklaki, Georgia Charalampous, Anna Moustaka, Alkistis Papetta, Celia Herrero del Barrio, Rizos-Theodoros Chadoulis, S. Yeşer Aslanoğlu, Sara Herrero-Anta, Michail Mytilinaios, Nikolaos Papadimitriou, Katerina Anyfanti, Christos Spyrou, Daniela Meloni, Konstantinos Fragkos, Yevgeny Derimian, Tatiana Di Iorio, Rodanthi-Elisavet Mamouri, Vassilis Amiridis, Stavros Solomos, Stelios Kazadzis, and Ilias Fountoulakis

Abstract. Atmospheric aerosols are among the key factors affecting the Earth’s radiation budget, playing a fundamental role in understanding climate forcing, feedback mechanisms, and their impact on future climate projections and on solar energy systems. More specifically, dust aerosol particles, which are characterized by high complexity of their optical and microphysical properties, remain one of the most uncertain components. In this study, we focus on four severe dust events across multiple sites in the broader Mediterranean Basin between 2021 and 2022. We employ a combination of ground-based 
remote sensing observations along with Radiative Transfer (RT) modelling, with the libRadtran package and METAL-WRF scheme, as well as photovoltaic (PV) power generation simulations using the Global Solar Energy Estimator (GSEE) to investigate the impact of the different optical and geometrical aspects of these events on solar radiation and solar energy. The results revealed that the strongest dust-induced attenuation was systematically observed in the direct component of solar radiation (DNI), with maximum losses frequently exceeding 60–80%, while Global Horizontal Irradiance (GHI) typically ranged between 5% and 25%. These findings were reflected directly into substantial PV power output losses, for both fixed tilt and two-axis tracking systems, reaching ~45% and 80%, respectively, with the impact on the latter being significantly higher due to their strong dependence on DNI. A sensitivity analysis based on how aerosol optical properties and solar geometry jointly influence PV energy production revealed that Solar Zenith Angle (SZA) plays the most dominant role, followed by Aerosol Optical Depth (AOD), which leads to strong attenuation independently of SZA under altered aerosol load conditions. Finally, the comparison of the modelled PV output estimated from the modelled irradiances based on the two different RT models with the PV output considering ground-based GHI measurements revealed a similar agreement under clear sky conditions, while under cloudy conditions, the analysis revealed the critical role of the diffuse horizontal irradiance (DHI) component in the simulations.

Competing interests: At least one of the (co-)authors is a member of the editorial board of Atmospheric Measurement Techniques.

Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims made in the text, published maps, institutional affiliations, or any other geographical representation in this paper. While Copernicus Publications makes every effort to include appropriate place names, the final responsibility lies with the authors. Views expressed in the text are those of the authors and do not necessarily reflect the views of the publisher.
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Dimitra Kouklaki, Georgia Charalampous, Anna Moustaka, Alkistis Papetta, Celia Herrero del Barrio, Rizos-Theodoros Chadoulis, S. Yeşer Aslanoğlu, Sara Herrero-Anta, Michail Mytilinaios, Nikolaos Papadimitriou, Katerina Anyfanti, Christos Spyrou, Daniela Meloni, Konstantinos Fragkos, Yevgeny Derimian, Tatiana Di Iorio, Rodanthi-Elisavet Mamouri, Vassilis Amiridis, Stavros Solomos, Stelios Kazadzis, and Ilias Fountoulakis

Status: open (until 02 Jul 2026)

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Dimitra Kouklaki, Georgia Charalampous, Anna Moustaka, Alkistis Papetta, Celia Herrero del Barrio, Rizos-Theodoros Chadoulis, S. Yeşer Aslanoğlu, Sara Herrero-Anta, Michail Mytilinaios, Nikolaos Papadimitriou, Katerina Anyfanti, Christos Spyrou, Daniela Meloni, Konstantinos Fragkos, Yevgeny Derimian, Tatiana Di Iorio, Rodanthi-Elisavet Mamouri, Vassilis Amiridis, Stavros Solomos, Stelios Kazadzis, and Ilias Fountoulakis
Dimitra Kouklaki, Georgia Charalampous, Anna Moustaka, Alkistis Papetta, Celia Herrero del Barrio, Rizos-Theodoros Chadoulis, S. Yeşer Aslanoğlu, Sara Herrero-Anta, Michail Mytilinaios, Nikolaos Papadimitriou, Katerina Anyfanti, Christos Spyrou, Daniela Meloni, Konstantinos Fragkos, Yevgeny Derimian, Tatiana Di Iorio, Rodanthi-Elisavet Mamouri, Vassilis Amiridis, Stavros Solomos, Stelios Kazadzis, and Ilias Fountoulakis
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Short summary
In the present study we investigated how aerosols, and specifically dust, affect solar radiation and energy production by investigating several dust events across multiple sites in the Mediterranean Basin between 2021 and 2022 through ground-based observations and model simulations. The results revealed that dust can significantly attenuate solar radiation and, therefore, lead to considerable losses in solar power generation, specifically in the case of solar tracking systems.
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