EGU23-15415, updated on 26 Feb 2023
https://doi.org/10.5194/egusphere-egu23-15415
EGU General Assembly 2023
© Author(s) 2023. This work is distributed under
the Creative Commons Attribution 4.0 License.

Validation of DSCOVR-based albedo estimate using a weather model

Maksym Vasiuta1, Lauri Tuppi2, Antti Penttilä3, Karri Muinonen3, and Heikki Järvinen2
Maksym Vasiuta et al.
  • 1University of Helsinki, Institute for Atmospheric and Earth System Research, Dynamic meteorology, Helsinki, Finland (maksym.vasiuta@helsinki.fi)
  • 2University of Helsinki, Institute for Atmospheric and Earth System Research, Dynamic meteorology, Helsinki, Finland
  • 3University of Helsinki, Faculty of Science, Department of Physics, Helsinki, Finland

The Deep Space Climate Observatory (DSCOVR) is located near the Lagrangian L1 point of the Earth. Their EPIC images indicate exceptionally large values of the Earth's planetary albedo in December 2020, having daily average surged above 0.320 for consecutive three weeks. Independent evaluation of the Earth’s albedo using a numerical weather prediction model (OpenIFS of ECMWF) suggests that this is an over-estimate. Given the difference between satellite-based and model-based albedo estimates, the reconstructed from images top-of-atmosphere short-wave radiosity is over-estimated. We suggest the discrepancy is explained by a weakness of short-wave angular distribution models (ADMs) based on Clouds and the Earth's Radiant Energy System’s The Tropical Rainfall Measuring Mission (CERES/TRMM) in full back-scattering geometry. This conclusion is supported by disk-integrated short-wave anisotropy factors in December 2020, estimated using CERES ADMs, being lower than measured by NIST Advanced Radiometer (NISTAR).

How to cite: Vasiuta, M., Tuppi, L., Penttilä, A., Muinonen, K., and Järvinen, H.: Validation of DSCOVR-based albedo estimate using a weather model, EGU General Assembly 2023, Vienna, Austria, 24–28 Apr 2023, EGU23-15415, https://doi.org/10.5194/egusphere-egu23-15415, 2023.