Ground solar absorption observations of total column CO, CO₂, CH₄, and aerosol optical depth from California's Sequoia Lightning Complex Fire: emission factors and modified combustion efficiency at regional scales
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Abstract
With global wildfires becoming more widespread and severe, tracking their emissions of greenhouse gases and air pollutants is becoming increasingly important. Wildfire emissions have primarily been characterized by in situ laboratory and field observations at fine scales. While this approach captures the mechanisms relating emissions to combustion phase and fuel properties, their evaluation on regional-scale plumes has been limited. In this study, we report remote observations of total column trace gases and aerosols during the 2020 wildfire season from smoke plumes in the Sierra Nevada of California with an EM27/SUN solar Fourier transform infrared (FTIR) spectrometer. We derive total column aerosol optical depth (AOD), emission factors (EFs) and modified combustion efficiency (MCE) for these fires and evaluate relationships between them, based on combustion phase at regional scales. We demonstrate that the EM27/SUN effectively detects changes in CO, CO₂, and CH₄ in the atmospheric column at ∼10 km horizontal scales that are attributed to wildfire emissions. These observations are used to derive total column EF_(CO) of 120.5 ± 12.2 and EF_(CH₄) of 4.3 ± 0.8 for a regional smoke plume event in mixed combustion phases. These values are consistent with in situ relationships measured in similar temperate coniferous forest wildfires. FTIR-derived AOD was compared to a nearby AERONET (AErosol RObotic NETwork) station and observed ratios of X_(CO) to AOD were consistent with those previously observed from satellites. We also show that co-located X_(CO) observations from the TROPOspheric Monitoring Instrument (TROPOMI) satellite-based instrument are 9.7 ± 1.3 % higher than our EM27/SUN observations during the wildfire period. Finally, we put wildfire CH4 emissions in context of the California state CH₄ budget and estimate that 213.7 ± 49.8 Gg CH₄ were emitted by large wildfires in California during 2020, about 13.7 % of the total state CH₄ emissions in 2020. Our work demonstrates a novel application of the ground-based EM27/SUN solar spectrometers in wildfire monitoring by integrating regional-scale measurements of trace gases and aerosols from smoke plumes.
Additional Information
© Author(s) 2023. This work is distributed under the Creative Commons Attribution 4.0 License. This article is part of the special issue "The role of fire in the Earth system: understanding interactions with the land, atmosphere, and society (ESD/ACP/BG/GMD/NHESS inter-journal SI)". It is a result of the EGU General Assembly 2020, 4–8 May 2020. Isis Frausto-Vicencio acknowledges the support from the National Science Foundation Graduate Research Fellowship Program. We thank the principal investigator Michael Garay and site manager Scott Scheller for their effort in establishing and maintaining the AERONET Fresno_2 site. We thank Nicole Jacobs for providing the code to apply the averaging kernel correction to the EM27/SUN X_(CO) observations. We thank Jacob Hedelius for providing code through EGI to read micro-windows from EM27/SUN retrievals. Finally, the authors thank William Porter for the assistance and access to University of California, Riverside (UCR), Aldo cluster. This research has been supported by the Office of the President, University of California (grant no. LFR-18-548581). Author contributions. IFV and SH contributed to the paper via conceptualization and data curation. IFV and HAP contributed to the data collection. IFV, SH, and AGM contributed via formal analysis. The publication was written by IFV, and all authors reviewed the paper and contributed to the discussion of the paper. FMH and MD contributed to funding acquisition. Data availability. The EM27/SUN retrievals used in this study are available at https://osf.io/ntzk8/ (last access: 31 March 2023). TROPOMI carbon monoxide and aerosol layer height products can be downloaded from https://s5phub.copernicus.eu (last access: 15 July 2022; ESA, 2022). We acknowledge the use of imagery from the NASA Worldview application (https://worldview.earthdata.nasa.gov/, last access: 15 July 2022; NASA, 2022a), which is part of the NASA Earth Observing System Data and Information System (EOSDIS). Version 3 AOD data are available from the AERONET website (https://aeronet.gsfc.nasa.gov, last access: 15 June 2022, NASA, 2022b). Fire radiative power data can be downloaded from https://firms.modaps.eosdis.nasa.gov/ (last access: 15 June 2022; NASA, 2022c). NOAA Physical Science Laboratory (PSL) wind data can be downloaded from ftp://ftp1.psl.noaa.gov/psd2/data/realtime/Radar915/ (last access: 15 June 2022; NOAA, 2022). The supplement related to this article is available online at: https://doi.org/10.5194/acp-23-4521-2023-supplement. At least one of the (co-)authors is a member of the editorial board of Atmospheric Chemistry and Physics. The peer-review process was guided by an independent editor, and the authors also have no other competing interests to declare.Attached Files
Published - acp-23-4521-2023.pdf
Supplemental Material - acp-23-4521-2023-supplement.pdf
Files
acp-23-4521-2023-supplement.pdf
Additional details
Identifiers
- Eprint ID
- 121345
- Resolver ID
- CaltechAUTHORS:20230509-823969500.10
Funding
- NSF Graduate Research Fellowship
- University of California, Office of the President
- LFR-18-548581
Dates
- Created
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2023-05-15Created from EPrint's datestamp field
- Updated
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2023-05-15Created from EPrint's last_modified field