EGU25-12043, updated on 15 Mar 2025
https://doi.org/10.5194/egusphere-egu25-12043
EGU General Assembly 2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
Oral | Thursday, 01 May, 11:35–11:45 (CEST)
 
Room 2.95
Assessing drivers of uncertainty in simulating δ¹³C-CH4 at global scale
Emeline Tapin1, Antoine Berchet1, Adrien Martinez1, Malika Menoud1,2, Xin Lan3,4, Sylvia Michel5, and Marielle Saunois1
Emeline Tapin et al.
  • 1Laboratoire des Sciences du Climat et de l’Environnement, LSCE/IPSL, CEA-CNRS-UVSQ, Université Paris-Saclay, F-91191 Gif-sur-Yvette, France
  • 2now at : International Methane Emissions Observatory (IMEO), United Nations Environment Programme (UNEP), Paris, France
  • 3CIRES, University of Colorado Boulder, CO, 80309, United States
  • 4NOAA Global Monitoring Laboratory, Boulder, CO, 80305, United States
  • 5Institute of Arctic and Alpine Research (INSTAAR), University of Colorado Boulder, CO, 80303, United States

Methane (CH4), the second-largest contributor to global warming, necessitates a detailed examination of its sources and sinks to understand the recent rise in atmospheric CH4 mole fractions. Atmospheric isotopic signals, especially δ¹³C-CH4, offer critical insights for disentangling sectoral contributions and addressing these uncertainties.

This study focuses on enhancing our understanding of CH4 sources and sinks by incorporating updated δ¹³C-CH4 source signature datasets into atmospheric modeling. First, we updated these datasets to reflect the latest knowledge of methane emission processes. Next, we assessed the sensitivity of key modeling parameters such as atmospheric chemistry, the aggregation of δ¹³C-CH4 source signatures, and prior flux estimates on simulated CH4 signals and mole fractions. This analysis aims to validate the updated datasets and identify primary drivers of uncertainty in the simulations. We conducted forward modeling using the Global Circulation Model LMDZ coupled with the Community Inversion Framework (CIF), based on surface observations of methane and its isotopic signal from 1998 to 2022. These efforts lay the groundwork for improving the robustness of future isotopic inversions.

Building on these findings, our future work will focus on transitioning from forward simulations to atmospheric inversions to analyze global methane concentration trends. Initially, we will perform inversions using in-situ data from 1998 to 2022, leveraging the updated δ¹³C-CH4 source signature datasets and setups. Subsequently, we will analyze trends from 2018 to 2022 by integrating satellite observations of total methane columns with surface isotopic measurements. This approach utilizes the high-resolution, global coverage of TROPOMI (TROPOspheric Monitoring Instrument) onboard the Sentinel-5P platform, which measures column-averaged methane dry-air mole fractions X(CH4). By combining satellite and surface observations, we aim to enhance our ability to monitor methane dynamics and deepen our understanding of CH4 source and sink interactions. These advancements will provide critical insights for designing more effective climate mitigation strategies.

How to cite: Tapin, E., Berchet, A., Martinez, A., Menoud, M., Lan, X., Michel, S., and Saunois, M.: Assessing drivers of uncertainty in simulating δ¹³C-CH4 at global scale, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12043, https://doi.org/10.5194/egusphere-egu25-12043, 2025.