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Soft sensors for dust estimation with high accuracy: AI-driven approach for CSP solar mirror soiling classification
Ayoub Oufadel, Masaab El Ydrissi, Ibrahim Taabane, Alae Azouzoute, Alami Hassani Aicha, Hicham Ghennioui

Soft sensors for dust estimation with high accuracy: AI-driven approach for CSP solar mirror soiling classification

Science & Mathematics Published 2025 Verification Pending

Overview & Synopsis

Concentrating solar power plants convert solar energy into electricity by using mirrors to concentrate sunlight, but dust, particularly in arid and semi-arid regions, reduces their efficiency. This study proposes an innovative AI-based approach for monitoring and predicting soiling. For real-time analysis of CSP mirror images, a ResNet-50 convolutional neural network (CNN) is used, while a recurrent neural network (RNN) with a long, short term memory (LSTM) architecture predicts future soiling rates using the temporary variation in this parameter. By integrating mirror imagery and meteorological data, our hybrid AI model effectively combines CNN for image analysis and RNN temporal predictions, with high accuracy ranging from 89.5% to 95.2%, depending on the application. The application of advanced AI techniques can significantly improve the management of concentrated solar power plants and lead to significant breakthroughs in the solar energy industry.

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Document Information

Document Title Soft sensors for dust estimation with high accuracy: AI-driven approach for CSP solar mirror soiling classification
Author / Organization Ayoub Oufadel, Masaab El Ydrissi, Ibrahim Taabane, Alae Azouzoute, Alami Hassani Aicha, Hicham Ghennioui
Subject & Discipline Multidisciplinary Academic Open Research
Categories Science & Mathematics
Publication Year 2025
License / Rights Open Access / Creative Commons
Resource Verification Listed PDF (Verification Pending)
Original Host Website HAL Open Science (hal.science)
File Format application/pdf (Portable Document Format)
Language EN
Catalog ID DOC-72918
Original Source Link Visit Source Page on hal.science »