EGU26-21929, updated on 14 Mar 2026
https://doi.org/10.5194/egusphere-egu26-21929
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Poster | Wednesday, 06 May, 08:30–10:15 (CEST), Display time Wednesday, 06 May, 08:30–12:30
 
Hall X4, X4.20
Estimation and spatial prediction methods for high-frequency space-time solar irradiance
William Kleiber and Nicolas Coloma
William Kleiber and Nicolas Coloma
  • University of Colorado, Department of Applied Mathematics, Boulder, United States of America (william.kleiber@colorado.edu)

As the power grid moves to a more renewable future, energy sources from weather-driven phenomena such as solar power will form an increasingly large portion of electricity generation.  The predicatibility, non-Gaussianity and intermittency of solar resources challenge current grid operation paradigms, and realistic data scenarios are required for grid planning and operational studies.  However, such data are not available at the space-time resolution needed for realistic grid models.  Given sparse spatial samples that are high-resolution in time, we introduce a framework for spatiotemporal prediction and downscaling in a functional data analysis framework when data exhibit nonstationary phase misalignment.  The approach is illustrated on a challenging irradiance dataset and compares favorably against existing methods.

How to cite: Kleiber, W. and Coloma, N.: Estimation and spatial prediction methods for high-frequency space-time solar irradiance, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21929, https://doi.org/10.5194/egusphere-egu26-21929, 2026.