Published July 5, 2022 | Version Published + Supplemental Material
Journal Article Open

Hydrocarbon Tracers Suggest Methane Emissions from Fossil Sources Occur Predominately Before Gas Processing and That Petroleum Plays Are a Significant Source

  • 1. ROR icon California Institute of Technology
  • 2. ROR icon National Oceanic and Atmospheric Administration
  • 3. ROR icon University of Miami
  • 4. ROR icon Cooperative Institute for Research in Environmental Sciences
  • 5. ROR icon University of California, Irvine

Abstract

We use global airborne observations of propane (C₃H₈) and ethane (C₂H₆) from the Atmospheric Tomography (ATom) and HIAPER Pole-to-Pole Observations (HIPPO), as well as U.S.-based aircraft and tower observations by NOAA and from the NCAR FRAPPE campaign as tracers for emissions from oil and gas operations. To simulate global mole fraction fields for these gases, we update the default emissions' configuration of C₃H₈ used by the global chemical transport model, GEOS-Chem v13.0.0, using a scaled C₂H₆ spatial proxy. With the updated emissions, simulations of both C₃H₈ and C₂H₆ using GEOS-Chem are in reasonable agreement with ATom and HIPPO observations, though the updated emission fields underestimate C₃H₈ accumulation in the arctic wintertime, pointing to additional sources of this gas in the high latitudes (e.g., Europe). Using a Bayesian hierarchical model, we estimate global emissions of C₂H₆ and C₃H₈ from fossil fuel production in 2016–2018 to be 13.3 ± 0.7 (95% CI) and 14.7 ± 0.8 (95% CI) Tg/year, respectively. We calculate bottom-up hydrocarbon emission ratios using basin composition measurements weighted by gas production and find their magnitude is higher than expected and is similar to ratios informed by our revised alkane emissions. This suggests that emissions are dominated by pre-processing activities in oil-producing basins.

Additional Information

© 2022 The Authors. Published by American Chemical Society. Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0). Received 11 February 2022. Accepted 18 May 2022. Revised 18 May 2022. Published online 14 June 2022. Published in issue 5 July 2022. This work was supported by the Resnick Sustainability Institute, including computations conducted in the Resnick High Performance Computing Center. A.L.T. received funding from NSF Award No. DGE-1745301. NOAA support was provided for HIPPO by NSF Award No. AGS-0628452; California Institute of Technology support for ATom was provided by NASA Grant Award No. NNX15AG61A. NOAA support for ATom was provided by NASA EVS2 Award No. NNH17AE26I; additional support was provided by NASA Upper Atmosphere Research Program award No. NNH13AV69I. NOAA laboratory and salary support is from NOAA Climate Change Program. S.A.M. acknowledges funding in part from NOAA Climate Program Office's AC4 Program. NOAA flask sampling and technical support was provided by Dr. Fred Moore of NOAA/CIRES. Additional technical support was provided by C. Siso, B. Miller, M. Crotwell, C. Sweeney, A. Andrews, J. Higgs, D. Neff, J. Kofler, K. McKain, M. Madronich, P. Handley, and S. Wolter. We thank IHS Markit for providing PointLogic economic data. The authors declare no competing financial interest.

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Published - acs.est.2c00927.pdf

Supplemental Material - es2c00927_si_001.pdf

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Additional details

Identifiers

PMCID
PMC9260955
Eprint ID
115474
Resolver ID
CaltechAUTHORS:20220711-653341000

Funding

Resnick Sustainability Institute
NSF Graduate Research Fellowship
DGE-1745301
NSF
AGS-0628452
NASA
NNX15AG61A
NASA
NNH17AE261
NASA
NNH13AV69I
National Oceanic and Atmospheric Administration (NOAA)

Dates

Created
2022-07-12
Created from EPrint's datestamp field
Updated
2022-07-12
Created from EPrint's last_modified field