EGU26-22088, updated on 14 Mar 2026
https://doi.org/10.5194/egusphere-egu26-22088
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Oral | Tuesday, 05 May, 14:24–14:27 (CEST)
 
vPoster spot 4
Poster | Tuesday, 05 May, 16:15–18:00 (CEST), Display time Tuesday, 05 May, 14:00–18:00
 
vPoster Discussion, vP.86
Hierarchical Bayesian Modeling of Solar Irradiance under Extreme Weather in the Tucson Electric Power Region
Jyotsna Singh
Jyotsna Singh
  • College of Information Science, University of Arizona, United States of America (jyotsnasingh@arizona.edu)

Accurate forecasting of surface solar irradiance is needed, as it helps in PV power system planning, particularly under extreme weather conditions. Deterministic and persistence-based forecasting methods generally fail under extreme weather conditions. The present study develops a hierarchical Bayesian spatio-temporal model to forecast solar radiation in the Tucson Electric Power (TEP) region, Arizona, United States. Satellite-derived (CERES SYN1deg) and reanalysis (MERRA-2) solar radiation data have been used in the present study to identify variability across the four TEP stations. The hierarchical Bayesian spatio-temporal model outperformed the persistent model. The findings also highlight that, instead of focusing on point forecasts, we should focus on uncertainty-aware forecasts.

 
 

How to cite: Singh, J.: Hierarchical Bayesian Modeling of Solar Irradiance under Extreme Weather in the Tucson Electric Power Region, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22088, https://doi.org/10.5194/egusphere-egu26-22088, 2026.