EGU26-16526, updated on 14 Mar 2026
https://doi.org/10.5194/egusphere-egu26-16526
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Oral | Friday, 08 May, 14:10–14:20 (CEST)
 
Room E2
Constraining ammonia emissions and deposition through joint NH3-NO2 satellite data assimilation in LOTOS-EUROS
Tyler Wizenberg1, Enrico Dammers1,2, Arjo Segers1, Beatriz Herrera Gutierrez1, Martijn Schaap1, Mark Shephard4, Pierre Coheur5, Martin Van Damme5,6, Henk Eskes7, Roy Wichink Kruit8, and Shelley van der Graaf8
Tyler Wizenberg et al.
  • 1The Netherlands Organization for Applied Scientific Research (TNO), Utrecht, Netherlands (tyler.wizenberg@tno.nl)
  • 2Institute of Environmental Sciences, Universiteit Leiden, Leiden, the Netherlands
  • 4Environment & Climate ge Canada (ECCC), Toronto, Canada
  • 5Université libre de Bruxelles (ULB), BLU-ULB research Center, Spectroscopy, Quantum Chemistry and Atmospheric Remote Sensing (SQUARES), Brussels, Belgium
  • 6Royal Belgian Institute for Space Aeronomy (BIRA-IASB), Brussels, Belgium
  • 7Royal Netherlands Meteorological Institute (KNMI), De Bilt, The Netherlands
  • 8National Institute for Public Health and the Environment (RIVM), Bilthoven, The Netherlands

Ammonia (NH3) and nitrogen dioxide (NO2) are key components of reactive nitrogen, with strong impacts on air quality, ecosystems, and nitrogen deposition. Long-term constraints on ammonia emissions and deposition remain uncertain due to sparse in situ measurements and limitations of individual satellite products. Here, we jointly assimilate five years (2018-2022) of NH3 and NO2 satellite observations over the Netherlands to improve constraints on reactive nitrogen concentrations, emissions, and deposition.

NH3 retrievals from the Infrared Atmospheric Sounding Interferometer (IASI) and Cross-track Infrared Sounder (CrIS) are assimilated along with NO2 observations from the TROPOspheric Monitoring Instrument (TROPOMI) within the Long Term Ozone Simulation-EURopean Operational Smog (LOTOS-EUROS) chemical transport model using a Local Ensemble Transform Kalman Filter (LETKF). The co-assimilation produces consistent year-to-year adjustments in modeled NH3 concentrations, emissions, and deposition, reflecting the chemically linked nature of reduced and oxidized nitrogen. Our model results are evaluated against independent surface observations from the Dutch National Air Quality Monitoring Network (LML), showing reduced surface biases, improved correlations, and a clearer representation of diurnal variability. Sensitivity experiments demonstrate that including TROPOMI NO2 alongside NH3 observations leads to the lowest NH3 surface biases, highlighting the added value of jointly assimilating chemically coupled species. Comparisons with the Dutch Measurements of Ammonia in Nature (MAN) network data show improved temporal correlations but persistent spatial biases related to representativeness differences, while MAN sensors co-located with LML stations exhibit consistent improvements.

In addition, synthetic NH3 observations from the geostationary Meteosat Third Generation Infrared Sounder (MTG-IRS) are assimilated in a separate experiment to assess the potential of future high-temporal-resolution measurements. These experiments indicate that MTG-IRS will provide substantial added value for constraining ammonia emissions and deposition at diurnal scales. Our results demonstrate that co-assimilation of NH3 and NO2 satellite observations provides a robust pathway toward improved monitoring of reactive nitrogen and supports the design and exploitation of next-generation atmospheric composition missions.

How to cite: Wizenberg, T., Dammers, E., Segers, A., Herrera Gutierrez, B., Schaap, M., Shephard, M., Coheur, P., Van Damme, M., Eskes, H., Wichink Kruit, R., and van der Graaf, S.: Constraining ammonia emissions and deposition through joint NH3-NO2 satellite data assimilation in LOTOS-EUROS, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16526, https://doi.org/10.5194/egusphere-egu26-16526, 2026.