Jianying Zhang , Shaogang Lei , Yu Tian , Yibo Zhao , Meng Li , Shengya Sun
{"title":"Intelligent monitoring of photovoltaic panel cleaning status: Fine-Scale dust accumulation estimation using hyperspectral data and mixed-pixel model","authors":"Jianying Zhang , Shaogang Lei , Yu Tian , Yibo Zhao , Meng Li , Shengya Sun","doi":"10.1016/j.renene.2026.125206","DOIUrl":null,"url":null,"abstract":"<div><div>Dust accumulation on the surface of photovoltaic panels is one of the key factors affecting the operational performance of PV systems. Hyperspectral remote sensing, with its high-dimensional and fine spectral resolution, shows great potential in PV pollution monitoring. However, our observations indicate that, for dust-covered PV panels, each spectral pixel often contains a composite signal generated by both the PV surface and the deposited dust. This microscopic mixed-pixel phenomenon is often overlooked, limiting existing monitoring approaches—based on single-spectrum analysis or traditional image processing—to macroscopic identification, and making it difficult to reveal the intrinsic relationship between dust density and spectral response. To address this issue, this study proposes a dust monitoring method for PV panels that integrates mixed-pixel spectral unmixing, enabling high-precision monitoring of different dust accumulation states. A spectral-index-optimized non-negative least squares method was first applied to estimate the abundances of the PV panel and dust components. The resulting abundance information was then incorporated into a dust density inversion model, and multiple machine learning algorithms were used to systematically compare the effects of different preprocessing strategies and sensitive-band extraction methods on model performance. The results showed that incorporating mixed-pixel abundance features significantly improved model accuracy and stability (R<sup>2</sup> = 0.9615, RMSE = 10.0092 g/m<sup>2</sup>). When the dust density reached 46.21 g/m<sup>2</sup>, the reflectance in the 440–675 nm range exhibited an inflection point, changing from a decreasing to an increasing trend. The corresponding dust proportion (64 %) slightly exceeded 50 %, making dust the dominant contributor to the spectral signal and indicating a transition in the dust layer from single to multiple scattering. This study provides theoretical support and technical foundations for intelligent PV soiling monitoring and optimized cleaning scheduling.</div></div>","PeriodicalId":419,"journal":{"name":"Renewable Energy","volume":"261 ","pages":"Article 125206"},"PeriodicalIF":9.1000,"publicationDate":"2026-04-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Renewable Energy","FirstCategoryId":"5","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0960148126000315","RegionNum":1,"RegionCategory":"工程技术","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"2026/1/9 0:00:00","PubModel":"Epub","JCR":"Q1","JCRName":"ENERGY & FUELS","Score":null,"Total":0}
引用次数: 0
Abstract
Dust accumulation on the surface of photovoltaic panels is one of the key factors affecting the operational performance of PV systems. Hyperspectral remote sensing, with its high-dimensional and fine spectral resolution, shows great potential in PV pollution monitoring. However, our observations indicate that, for dust-covered PV panels, each spectral pixel often contains a composite signal generated by both the PV surface and the deposited dust. This microscopic mixed-pixel phenomenon is often overlooked, limiting existing monitoring approaches—based on single-spectrum analysis or traditional image processing—to macroscopic identification, and making it difficult to reveal the intrinsic relationship between dust density and spectral response. To address this issue, this study proposes a dust monitoring method for PV panels that integrates mixed-pixel spectral unmixing, enabling high-precision monitoring of different dust accumulation states. A spectral-index-optimized non-negative least squares method was first applied to estimate the abundances of the PV panel and dust components. The resulting abundance information was then incorporated into a dust density inversion model, and multiple machine learning algorithms were used to systematically compare the effects of different preprocessing strategies and sensitive-band extraction methods on model performance. The results showed that incorporating mixed-pixel abundance features significantly improved model accuracy and stability (R2 = 0.9615, RMSE = 10.0092 g/m2). When the dust density reached 46.21 g/m2, the reflectance in the 440–675 nm range exhibited an inflection point, changing from a decreasing to an increasing trend. The corresponding dust proportion (64 %) slightly exceeded 50 %, making dust the dominant contributor to the spectral signal and indicating a transition in the dust layer from single to multiple scattering. This study provides theoretical support and technical foundations for intelligent PV soiling monitoring and optimized cleaning scheduling.
期刊介绍:
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