Preprints
https://doi.org/10.5194/acp-2022-671
https://doi.org/10.5194/acp-2022-671
14 Oct 2022
 | 14 Oct 2022
Status: a revised version of this preprint was accepted for the journal ACP and is expected to appear here in due course.

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 large scales

Isis Frausto-Vicencio, Sajjan Heerah, Aaron G. Meyer, Harrison A. Parker, Manvendra Dubey, and Francesca M. Hopkins

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 large scale plumes has been limited. In this study, we report remote observations of total column trace gases and aerosols in the 2020 wildfire season of smoke plumes from 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 (EF) and modified combustion efficiency (MCE) for these fires, and evaluate relationships between them based on combustion phase at large scales. We demonstrate that the EM27/SUN effectively detects changes of CO, CO2 and CH4 in the atmospheric column at ~10 km scales that are attributed to wildfire emissions. These observations are used to derive total column EFCO of 120.5 ± 12.2 and EFCH4 of 4.3 ± 0.8 for a large 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 station and observed ratios of AOD to XCO were consistent with those previously observed from satellites. We also show that co-located XCO observations from the TROPOMI satellite-based instrument are 9.7 % 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 13.6 % of the total state CH4 emissions in 2019. Our novel application of an EM27/SUN solar spectrometer to quantify wildfire emission ratios at large scales follows predictive relationships that are consistent with in situ studies, offering promise for extensive monitoring from ground networks and satellite remote sensing.

Isis Frausto-Vicencio et al.

Status: closed

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse
  • RC1: 'Comment on acp-2022-671', Anonymous Referee #1, 09 Nov 2022
    • AC1: 'Reply on RC1', Isis Frausto-Vicencio, 01 Feb 2023
  • RC2: 'Comment on acp-2022-671', Anonymous Referee #2, 10 Nov 2022
    • AC2: 'Reply on RC2', Isis Frausto-Vicencio, 01 Feb 2023

Status: closed

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse
  • RC1: 'Comment on acp-2022-671', Anonymous Referee #1, 09 Nov 2022
    • AC1: 'Reply on RC1', Isis Frausto-Vicencio, 01 Feb 2023
  • RC2: 'Comment on acp-2022-671', Anonymous Referee #2, 10 Nov 2022
    • AC2: 'Reply on RC2', Isis Frausto-Vicencio, 01 Feb 2023

Isis Frausto-Vicencio et al.

Isis Frausto-Vicencio et al.

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Short summary
Wildfires are increasing in the Western US making it critical to understand the impacts of greenhouse gases and air pollutants to the atmosphere. We used a ground-based remote sensing technique to measure the amount of greenhouse gases and aerosol present in the atmosphere. We isolate a large smoke plume being transported and calculate variables to understand the fuel properties and combustion phases. We find that a significant amount of methane is emitted from wildfires.
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