Dust potency in the context of solar photovoltaic (PV) soiling loss

We report on the impact of natural soiling on PV module performance loss in terms of dust potency (i.e., soiling loss per unit area dust mass) affected by dust composition and environmental conditions. Samples of accumulated dust mass (ADM) on PV panels from Doha, Qatar, were collected at different periods over two years. Our analysis demonstrated that dust accumulation rate and dust potency exhibited seasonal patterns influenced by environmental conditions. The measured dust potency varied significantly from month to month, ranging from 2 to 3.7% g-1 m2 that situates in the range of 2 - 8% g-1 m2 found in the literature. The lower dust potency was observed during the summer months, characterized by strong winds and low humidity. Soiling loss may be seen as a function of ADM and the dust potency, with the latter being a function of dust physico-chemical properties. ADM also has a significant seasonal fluctuation both in terms of particle size distribution and chemical composition. The dust potency is found to be impacted by the particle size, elemental carbon (EC), organic carbon (OC), and ions contents of the dust. ADM with lower dust potency has shown larger size particles and low EC/OC contents, while the effect of soluble ions on dust potency is found to be complex, due most probably to the interactions with humidity. Finally, based on the experimental and literature data, we developed a practical and straightforward model to estimate PV soiling loss as a function of dust mass and dust potency.

Automated summary

This study investigated the impact of dust on PV module performance loss, showing variations in dust potency under different seasonal patterns and environmental conditions. Factors such as particle size, elemental carbon, organic carbon, and ions contents were found to influence the dust potency, with complex interactions potentially involving humidity.