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Quantifying methane emissions from the largest oil-producing basin in the United States from space

  • Yuzhong Zhang*
  • , Ritesh Gautam
  • , Sudhanshu Pandey
  • , Mark Omara
  • , Joannes D. Maasakkers
  • , Pankaj Sadavarte
  • , David Lyon
  • , Hannah Nesser
  • , Melissa P. Sulprizio
  • , Daniel J. Varon
  • , Ruixiong Zhang
  • , Sander Houweling
  • , Daniel Zavala-Araiza
  • , Ramon A. Alvarez
  • , Alba Lorente
  • , Steven P. Hamburg
  • , Ilse Aben
  • , Daniel J. Jacob
  • *Corresponding author for this work

Research output: Contribution to JournalArticleAcademicpeer-review

Abstract

Using new satellite observations and atmospheric inverse modeling, we report methane emissions from the Permian Basin, which is among the world's most prolific oil-producing regions and accounts for >30% of total U.S. oil production. Based on satellite measurements from May 2018 to March 2019, Permian methane emissions from oil and natural gas production are estimated to be 2.7 ± 0.5 Tg a−1, representing the largest methane flux ever reported from a U.S. oil/gas-producing region and are more than two times higher than bottom-up inventory-based estimates. This magnitude of emissions is 3.7% of the gross gas extracted in the Permian, i.e., ~60% higher than the national average leakage rate. The high methane leakage rate is likely contributed by extensive venting and flaring, resulting from insufficient infrastructure to process and transport natural gas. This work demonstrates a high-resolution satellite data-based atmospheric inversion framework, providing a robust top-down analytical tool for quantifying and evaluating subregional methane emissions.

Original languageEnglish
Article numberaaz5120
Pages (from-to)1-10
Number of pages10
JournalScience Advances
Volume6
Issue number17
DOIs
Publication statusPublished - 22 Apr 2020

Funding

We thank the team that realized the TROPOMI instrument and its data products, consisting of the partnership between Airbus Defense and Space Netherlands, KNMI, SRON, and TNO, commissioned by NSO and ESA. Sentinel-5 Precursor is part of the EU Copernicus program, and Copernicus Sentinel data 2018-2019 have been used. We acknowledge the provision of publicly available VIIRS night-fire data. We also acknowledge NOAA Earth System Research Laboratory's Global Greenhouse Gas Reference Network for providing methane measurements at MLO, WKT, and TGC. This work was supported by the Kravis Scientific Research Fund, the Robertson Foundation, GALES project (#15597) by the Dutch Technology Foundation STW, and the TROPOMI national program through NSO. Y.Z. was funded by the Kravis Fellowship through EDF and by Harvard University. P.S. and S.P. are funded through the GALES project (#15597) by the Dutch Technology Foundation STW, which is part of the Netherlands Organization for Scientific Research (NWO). A.L. acknowledges funding from the TROPOMI national program through NSO. R.G., M.O., D.L., D.Z.-A., R.A.A., and S.P.H. were funded by the Robertson Foundation. D.J.J. was funded by the NASA Carbon Monitoring System.

FundersFunder number
Kravis Scientific Research Fund
NOAA Earth System Research Laboratory
Netherlands Organization for Scientific Research
SRON
TGC
National Aeronautics and Space Administration
Harvard University
Robertson Foundation15597
Elizabeth Dole Foundation
European Commission
Nederlandse Organisatie voor Wetenschappelijk Onderzoek
Stichting voor de Technische Wetenschappen
Koninklijk Nederlands Meteorologisch Instituut
Airbus Defense and Space

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