EGU26-4840, updated on 13 Mar 2026
https://doi.org/10.5194/egusphere-egu26-4840
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Diurnal Ammonia Mapping based on Deep Learning from Geostationary Hyperspectral Infrared Sounder Observations
Xinran Xia1, Min Min1, Jun Li2, and Ling Gao2
Xinran Xia et al.
  • 1School of Atmospheric Sciences and Guangdong Province Key Laboratory for Climate Change and Natural Disaster Studies, Sun Yat-sen University and Southern Laboratory of Ocean Science and Engineering (xiaxr@mail2.sysu.edu.cn)
  • 2Innovation Centre for Fengyun Meteorological Satellite (FYSIC), National Satellite Meteorological Centre, China Meteorological Administration

Atmospheric ammonia (NH₃) is a key air pollutant with high spatiotemporal variability, challenging the observation of its diurnal cycle. The Fengyun-4B Geostationary Interferometric Infrared Sounder (FY-4B/GIIRS) offers high-frequency measurements that capture this variability. We introduce a novel Multi-modal Fusion Transformer (MF-Transformer) to retrieve NH₃ total columns directly from hyperspectral radiances, meteorology, and ancillary data, circumventing costly radiative transfer simulations. Our retrievals are consistent with the IASI (Infrared Atmospheric Sounding Interferometer) NH₃ product (correlation coefficient, R=0.79) and Optimal Estimation (OE) retrievals (R=0.75), outperform benchmark machine learning models by ~20% in accuracy, and eliminate unphysical negative values. The method is orders of magnitude faster than OE approach, enabling global full-disk processing in tens of seconds. This advance allows the resolution of rapid NH₃ variations, demonstrating a transformative capability for operational monitoring.

How to cite: Xia, X., Min, M., Li, J., and Gao, L.: Diurnal Ammonia Mapping based on Deep Learning from Geostationary Hyperspectral Infrared Sounder Observations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4840, https://doi.org/10.5194/egusphere-egu26-4840, 2026.