Published September 1, 2025 | Version Supplemental material
Journal Article Open

Observing carbon monoxide and volatile organic compounds from Canadian wildfires in 2023 from FengYun-3E/HIRAS-II in a dawn-dusk sun-synchronous orbit

  • 1. ROR icon Peking University
  • 2. ROR icon China Meteorological Administration
  • 3. ROR icon Beijing Institute of Technology
  • 4. ROR icon Environment and Climate Change Canada
  • 5. ROR icon University of Toronto
  • 6. ROR icon Université Libre de Bruxelles
  • 7. LATMOS/IPSL, Sorbonne Université, UVSQ, CNRS, Paris, France
  • 8. ROR icon California Institute of Technology

Abstract

This study presents the first attempt to observe wildfire enhancements of carbon monoxide (CO) and volatile organic compounds (VOCs) around sunrise and sunset from a hyperspectral infrared sounder in a dawn-dusk sun-synchronous orbit. The 2nd generation of High Spectral Infrared Atmospheric Sounder (HIRAS-II) on board FengYun-3E (FY-3E), the world's first civilian dawn-dusk orbit meteorological satellite, provides global observations in the thermal infrared spectral range with equatorial overpass times of 5:30 am/pm local solar time (LST). The spectral observations are used to retrieve CO, formic acid (HCOOH) and peroxyacetyl nitrate (PAN) emitted from three major Canadian wildfire events from June to August 2023. Extreme enhancements of CO, HCOOH and PAN were detected in the 2023 Canadian wildfires which are unprecedented in time and spatial scales and intensity. The HIRAS-II successfully captured the strong signals of CO, HCOOH, and PAN. The averaging kernel (AK) matrix, indicative of detection vertical sensitivity, peaks mostly in the free troposphere where extensive transport typically takes place. Comparison with the Infrared Atmospheric Sounding Interferometer (IASI) and the Cross-track Infrared Sounder (CrIS) reveals that the spatial distribution patterns of the total columns extracted from HIRAS-II are in good agreement. Validation with the CAMS model and ground-based observations from TCCON and NDACC confirms that HIRAS-II retrievals are consistent. The HCOOH-to-CO and the PAN-to-CO column enhancement ratios derived from HIRAS-II are close to those derived from IASI. This paper exhibits the capability of FY-3E/HIRAS-II in observing wildfire emissions during dawn and dusk hours, which will potentially enhance the climate-monitoring capability of low-orbit meteorological satellites.

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Acknowledgement

Z.-C. Zeng acknowledges funding from the National Natural Science Foundation of China (grant no. 42275142 and no. 12292980), the National Key Research and Development Program of China (grant no. 2022YFA1003801). This work was also supported by High-performance Computing Platform of Peking University. Research at the National Satellite Meteorological Center (NSMC) was funded by NSMC of China Meteorological Administration (CMA) under the program of Calibration Technology Development and Level-1 Data Production for the Hyperspectral Imaging and Sounding Instruments onboard FY-3E and FY-4B Satellites (FY-APP-2021.0507). L. C. is Senior Research Associate with the Fonds de la Recherche Scientifique – FNRS. Activities at ULB have been supported by the HIRS Prodex arrangement (ESA – BELSPO).

Data Availability

FY-3E/HIRAS-II Level 1 data are publicly available from the FengYun Satellite Data Center at http://satellite.nsmc.org.cn/portalsite/default.aspx. The retrieval datasets are publicly available at https://doi.org/10.5281/zenodo.15490285. The surface emissivity datasets are from the Global Infrared Land Surface Emissivity: UW-Madison Baseline Fit Emissivity Database at https://cimss.ssec.wisc.edu/iremis/. The ECMWF ERA5 reanalysis datasets are available from the Copernicus Climate Data Store at https://cds.climate.copernicus.eu/. The ECMWF atmospheric composition datasets and the CAMS global atmospheric composition forecasts are available from the Copernicus Atmosphere Data Store at https://ads.atmosphere.copernicus.eu/. The TCCON data are obtained from the TCCON Data Archive hosted by CaltechDATA at https://tccondata.org. The TAO data are available through the NDACC website www.ndacc.org. IASI is a joint mission of EUMETSAT and the Centre National d'Études Spatiales (CNES, France). It is flown aboard the Metop satellites as part of the EUMETSAT Polar System. The authors thank AERIS and AC-SAF Eumetsat for distributing and generating the L2 CO data (https://iasi.aeris-data.fr/co/). The ANNI HCOOH v4 product from IASI is publicly accessible on AERIS (https://iasi.aeris-data.fr/hcooh/). The PAN v4 products from IASI are available from ULB's authors upon request. The TROPESS CrIS-JPSS1 L2 CO and PAN products are publicly available at https://disc.gsfc.nasa.gov/datasets/TRPSDL2COCRS1FS_1/summary and https://disc.gsfc.nasa.gov/datasets/TRPSDL2PANCRS1FS_1/summary.

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Additional details

Related works

Funding

National Natural Science Foundation of China
42275142
National Natural Science Foundation of China
12292980
Ministry of Science and Technology of the People's Republic of China
2022YFA1003801
Peking University
China Meteorological Administration
FY-APP-2021.0507
Fund for Scientific Research
Belgian Federal Science Policy Office
National Meteorological Satellite Center

Dates

Accepted
2025-05-19
Available
2025-05-27
Available online
Available
2025-05-27
Version of record

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Division of Geological and Planetary Sciences (GPS)
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Published