Abstract
This study experimentally validates and numerically models the flux-spreading effect in a light-trapping planar-cavity solar receiver) for particle-based concentrating solar power systems. The receiver's shallow cavity with vertical planar walls redistributes concentrated solar flux, reducing peak intensity and achieving uniform heat flux. On-sun tests at National Renewable Energy Laboratory's High-Flux Solar Furnace under flux up to 1500 kW/m2 measured cavity wall temperatures, which were compared with Monte Carlo ray-tracing (SolTrace) and computational numerical simulations. Three angular absorptance models were evaluated: constant absorptance, a Pyromark-based directional model, and a Fresnel-based Cr2O3 model. The Fresnel-derived model showed the best agreement with experiments, achieving high correlation (PC > 0.85), structural similarity (SSIM > 0.98), and signal-to-noise ratios (PSNR > 40 dB), with temperature prediction errors of 1-11%. Results confirm that flux spreading mitigates local overheating and validate the integrated modeling approach, supporting the solar receiver scalability for high-efficiency, high-temperature concentrating solar power applications.
| Original language | American English |
|---|---|
| Number of pages | 15 |
| Journal | Applied Thermal Engineering |
| Volume | 296 |
| DOIs | |
| State | Published - 2026 |
NLR Publication Number
- NLR/JA-5700-94863
Keywords
- concentrating solar thermal power
- directional solar absorptance
- flux spreading
- Monte-Carlo ray-tracing
- numerical modeling
- particles
- planar cavity solar receivers
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