Accurate and scalable receiver-level flux prediction: A fully data-driven solution
Concentrated Solar Technologies (CST) systems, particularly central tower configurations with heliostat fields, play a critical role in the renewable energy landscape. By focusing sunlight from thousands of heliostats onto a central receiver, these systems generate high-temperature heat, which serves as a key resource for dispatchable power generation and industrial processes. Accurate receiver-level flux prediction, which depends on precise heliostat characterization, is essential for optimizing efficiency and operational control. However, existing characterization methods face trade-offs between accuracy and scalability, limiting their practicality for large-scale deployment. To overcome these limitations, this study introduces a fully data-driven framework that unifies heliostat characterization and flux prediction, leveraging operational data from standard calibration procedures. Expanding upon previous work that employed StyleGAN for beam-characterization-based predictions, this approach advances the methodology to achieve accurate receiver-level flux predictions. While the prior method demonstrated a proof of concept for a unified data-driven approach, it remained constrained to flux predictions on the calibration target itself. This study introduces key innovations, including aim point generalization strategies and a novel receiver projection technique, effectively bridging the gap between beam-characterization-based heliostat characterization and accurate receiver-level flux predictions. The proposed Transformer-based architecture achieves receiver-level focal spot prediction errors below 12%, exceeding the accuracy of state-of-the-art deflectometry-enhanced ray tracing. By relying exclusively on standard calibration images, the method remains both cost-efficient and scalable, offering a practical solution for large-scale CST applications. • Data-driven Flux Prediction approach relies on calibration target images. • Projection and aim point generalization enable receiver-level flux prediction. • Novel projection method applies to any receiver type, including cavity receivers. • Outperforms deflectometry-enhanced ray tracing with receiver-level errors below 12%. • Requires only five calibration images per heliostat for large-scale deployment.
Authors
- Mathias Kuhl (ORCID: https://orcid.org/0000-0003-0097-7260)
- Robert Pitz‐Paal (ORCID: https://orcid.org/0000-0002-3542-3391)
- Daniel Maldonado Quinto (ORCID: https://orcid.org/0000-0003-2929-8667)
- Max Pargmann (ORCID: https://orcid.org/0000-0002-4705-6285)
Institutions
- LVR-Klinik Köln (DE)
- RWTH Aachen University (DE)
Publication Details
- Journal
- Solar Energy
- Published
- 2025-06-18
- DOI
- https://doi.org/10.1016/j.solener.2025.113631
- Primary Topic
- Nuclear reactor physics and engineering
- Type
- article
- Field-Weighted Citation Impact
- 0.00
Funders
- Helmholtz-Gemeinschaft
- Deutsches Zentrum für Luft- und Raumfahrt
- Helmholtz Association
- Helmholtz Artificial Intelligence Cooperation Unit