EGU26-13181, updated on 14 Mar 2026
https://doi.org/10.5194/egusphere-egu26-13181
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Poster | Friday, 08 May, 16:15–18:00 (CEST), Display time Friday, 08 May, 14:00–18:00
 
Hall X5, X5.141
Spatial solar irradiance emulation of Monte Carlo ray tracing with multi-view all-sky imagery
Max Aragon Cerecedes1, Yves-Marie Saint-Drenan1, Yehia Eissa1, Philippe Blanc1, Menno Veerman2, Chiel van Heerwaarden2, and Thomas Schmidt3
Max Aragon Cerecedes et al.
  • 1O.I.E. Centre Observation, Impacts, Energy, Mines Paris PSL, Valbonne, France (max.aragon_cerecedes@minesparis.psl.eu)
  • 2Meteorology and Air Quality Group, Wageningen University & Research, Wageningen, the Netherlands (chiel.vanheerwaarden@wur.nl)
  • 3German Aerospace Center (DLR) – Institute of Networked Energy Systems, Oldenburg, Germany (th.schmidt@dlr.de)

Explicit 3D radiative transfer captures the complex spatial variability of global horizontal irradiance (GHI) under shallow cumulus clouds, but is computationally prohibitive for real-time operational use. We address this by introducing a simulation-to-reality framework that emulates 3D radiative transfer via a neural network trained on synthetic data to translate multi-view all-sky imagery into 2D GHI maps. To produce the training data, we ran large eddy simulations at 50 m horizontal resolution for 10 selected cloud dynamic days (April to July 2022) over a 14 km x 14 km domain. The resulting cloud fields were coupled with Monte Carlo ray tracing to render synthetic all-sky images from virtual camera locations matching the Eye2Sky camera network and to compute the corresponding GHI maps. Two datasets are generated, (1) raw synthetic renderings and (2) enhanced renderings with camera-specific characteristics from the real-world. Identical image-to-image neural networks are trained on these datasets and applied to real Eye2Sky imagery, with predicted GHI maps validated against co-located pyranometers. By incorporating sensor-specific characteristics, we quantify the benefit of reducing the simulation-to-reality gap and assess whether synthetic pre-training using neural network emulations can support operational solar irradiance mapping as an alternative to computationally expensive physical simulations.

How to cite: Aragon Cerecedes, M., Saint-Drenan, Y.-M., Eissa, Y., Blanc, P., Veerman, M., van Heerwaarden, C., and Schmidt, T.: Spatial solar irradiance emulation of Monte Carlo ray tracing with multi-view all-sky imagery, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13181, https://doi.org/10.5194/egusphere-egu26-13181, 2026.