Enhanced On-Site Characterization of Heliostat Surface via Direct Calculation of Reflected Beam’s Normal Vectors

SolarPACES 2024 Conference

Authors

DOI:

https://doi.org/10.52825/solarpaces.v3i.2402

Keywords:

Helioscharplus, Temporal Constraints, Spatial Constraints, Normal Vectors

Abstract

In this study, the results obtained through the algorithm presented for calculating the surface error will be analyzed. This aims to achieve a more precise characterization of the heliostat surface, independent of external conditions such as environment or solar field configuration. This can be accomplished by acquiring data obtained through HelioscharPlus characterization system, which has been presented in previous works and is distinguished by being based on data measured in real conditions, providing insights into the actual operation of the heliostat. This measurement mode offers the possibility to apply refinement process to the results, crucial for enhancing the accuracy of the characterization and aligning it more closely with real-world conditions. 

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References

[1] A. Peña et al., “Novel scanner-based methodology for a fast and complete high quality characterization of all solar field heliostats, their facets, and corresponding reflected beams,” p. 3, 2023, doi: 10.1117/12.2677246

[2] A.Peña-Lapuente et al., “Initial validation of an advanced heliostat characterizationsystembased on cameras and light detectors,” AIP Conf. Proc., vol. 2445, 2022, doi: 10.1063/5.0085728

[3] J. Yan, Z. R. Cheng, and Y. D. Peng, “Effect of tracking error of double-axis tracking de-vice on the optical performance of solar dish concentrator,” Int. J. Photoenergy, vol. 2018, 2018, doi: 10.1155/2018/9046127

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Published

2025-11-25

How to Cite

Aginaga Etxamendi, K. I., Angel M. Andueza, Peña-Lapuente, A., Escorza, S., & Marcelino Sanchez. (2025). Enhanced On-Site Characterization of Heliostat Surface via Direct Calculation of Reflected Beam’s Normal Vectors : SolarPACES 2024 Conference. SolarPACES Conference Proceedings, 3. https://doi.org/10.52825/solarpaces.v3i.2402
Received 2024-09-09
Accepted 2025-04-28
Published 2025-11-25