Preprints
https://doi.org/10.5194/egusphere-2026-3365
https://doi.org/10.5194/egusphere-2026-3365
03 Jul 2026
 | 03 Jul 2026
Status: this preprint is open for discussion and under review for Atmospheric Measurement Techniques (AMT).

Operational XCH4 Retrievals from MethaneSAT: Demonstrating Sensor Performance for Constraining Regional Methane Emissions

Christopher Chan Miller, Sébastien Roche, Jonas Wilzweski, Xiong Liu, Kelly V. Chance, Bingkun Luo, Kang Sun, Jonathan E. Franklin, Joshua S. Benmergui, Maya Nasr, David J. Miller, Sean Crowell, Nathan Leisso, Eleanor Walker, Ritesh Gautam, Nicholas LoFaso, Sasha Ayvazov, David Wells, Carlos Cervantes, Christopher Hairfield, and Steven Wofsy

Abstract. MethaneSAT, launched in March 2024, was designed to quantify regional methane (CH4) emissions, with a primary focus on the oil and gas (O&G) sector. The satellite mission bridges the gap between coarse-resolution global flux mappers and high‑resolution plume imagers by combining fine spatial resolution (~110 x 400 m2 pixels at nadir), high spectral resolution (~0.23 nm FWHM), and a ~220 km swath at nadir. In this study, we present the first operational retrievals of CH4 column-averaged dry-air mole fractions (XCH4) using the CO2‑proxy method. We assess the instrument and retrieval algorithm performance relative to the mission's precision and accuracy requirements needed to constrain CH4 emissions at the scale of individual O&G basins.

We focus on evaluating the retrieval against four major potential sources of systematic error: albedo dependent CH4/CO2 column retrieval sensitivity differences, cross-track stripe biases, aerosol-induced light path errors, and subscene CO2 variability. Tuning the a priori covariance matrix suppresses albedo-dependent errors caused by the influence of priors to sub ppb levels. Through a careful selection of homogeneous validation targets, we show that XCH4 cross-track biases strongly correlate with changes in the apparent instrument spectral response function (ISRF). We develop a stripe-correction algorithm using retrieved ISRF variations in a regression model combined with wavelet-Fourier filtering to reduce stripe noise from approximately 15 ppb standard deviation to near the random noise limit.

Analysis of the homogeneous validation scenes shows that single-pixel precision is approximately 30 ppb for conditions from a typical bare-ground O&G scene (0.4 albedo, 30° SZA), corresponding to ~3 ppb at 2 x 2 km2, and thus well within the mission requirement of 3 ppb at 5 x 5 km2. This requirement is also met for all targeted viewing geometry/albedo combinations. Comparisons with XCH4 from TROPOMI show excellent agreement, with a mean bias of 0.1 ppb and a regression slope of 0.99 when using XCO2 from the CAMS greenhouse gas forecast as the prior in place of the GINPUT prior used operationally. The spatial pattern of Permian basin XCH4 enhancements between the two instruments is highly consistent.

Observations of a Pseudo-Invariant Calibration site in Libya confirm that the CO2-proxy approach effectively mitigates biases induced by cloud and aerosol scattering, with subscene XCO2 variability emerging as the most challenging remaining error source; gradients of a few ppm can lead to XCH4 errors comparable to typical basin enhancements, though such conditions appear infrequent in both MethaneSAT observations and CAMS GHG forecast simulations. Overall, MethaneSAT retrieves XCH4 with the precision and accuracy required for basin-scale emissions inversion. These results suggest that the CO2-proxy approach remains the most viable retrieval approach for regional CH4 emission mapping, with improved treatment of subscene XCO2 variability representing the key priority for future work.

Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims made in the text, published maps, institutional affiliations, or any other geographical representation in this paper. While Copernicus Publications makes every effort to include appropriate place names, the final responsibility lies with the authors. Views expressed in the text are those of the authors and do not necessarily reflect the views of the publisher.
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Christopher Chan Miller, Sébastien Roche, Jonas Wilzweski, Xiong Liu, Kelly V. Chance, Bingkun Luo, Kang Sun, Jonathan E. Franklin, Joshua S. Benmergui, Maya Nasr, David J. Miller, Sean Crowell, Nathan Leisso, Eleanor Walker, Ritesh Gautam, Nicholas LoFaso, Sasha Ayvazov, David Wells, Carlos Cervantes, Christopher Hairfield, and Steven Wofsy

Status: open (until 08 Aug 2026)

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Christopher Chan Miller, Sébastien Roche, Jonas Wilzweski, Xiong Liu, Kelly V. Chance, Bingkun Luo, Kang Sun, Jonathan E. Franklin, Joshua S. Benmergui, Maya Nasr, David J. Miller, Sean Crowell, Nathan Leisso, Eleanor Walker, Ritesh Gautam, Nicholas LoFaso, Sasha Ayvazov, David Wells, Carlos Cervantes, Christopher Hairfield, and Steven Wofsy
Christopher Chan Miller, Sébastien Roche, Jonas Wilzweski, Xiong Liu, Kelly V. Chance, Bingkun Luo, Kang Sun, Jonathan E. Franklin, Joshua S. Benmergui, Maya Nasr, David J. Miller, Sean Crowell, Nathan Leisso, Eleanor Walker, Ritesh Gautam, Nicholas LoFaso, Sasha Ayvazov, David Wells, Carlos Cervantes, Christopher Hairfield, and Steven Wofsy
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Short summary
Reducing oil and gas methane emissions is among the fastest ways to slow near-term climate change, and satellites offer a transparent means of verifying progress. MethaneSAT fills a gap between existing instruments, which either measure methane accurately but at coarse scales, or detect large leaks at fine resolution without the accuracy to account for all sources. We present the first measurements and show they meet the accuracy requirements for regional emissions mapping at the 2–4 km2 scale.
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