EGU24-7848, updated on 08 Mar 2024
https://doi.org/10.5194/egusphere-egu24-7848
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

Analysis of radiocarbon in atmospheric methane: technological advances and interpretation of measurements

Giulia Zazzeri1, Lukas Wacker2, Negar Haghipour3, and Heather Graven4
Giulia Zazzeri et al.
  • 1RSE, Sviluppo Sostenibile e Fonti Energetiche, (giulia.zazzeri@rse-web.it)
  • 2ETH, Laboratory of Ion Beam Physics
  • 3ETH, Geological Institute
  • 4Imperial College London, Department of Physics

Radiocarbon (14C) is an optimal tracer of methane emissions, as 14C measurements enable distinguishing fossil from biogenic methane. However, we are not yet applying these measurements in monitoring programs for quantification of sources contribution, because of the technical challenges associated with the 14C analysis and the bias introduced by 14C emissions from nuclear power plants.

Studies in London and in Switzerland demonstrate how the nuclear influence should be accurately modelled for a quantitative interpretation of 14C measurements and that a robust uncertainty estimate of the fossil and biogenic proportion of CH4 emissions is highly needed.

Here we present the technological advances in the 14CH4 analysis, including the achievement of high precision 14CH4 measurements (5 ‰) using a new portable sampler developed at the laboratory of Ion Beam Physics, and the potential of expanding these measurements for an improved understanding of sources. We will present the first quantification of fossil methane emissions in London using 14C, demonstrating that, by increasing the measurement capability, we can use 14C to constrain the methane budget at regional scale.

How to cite: Zazzeri, G., Wacker, L., Haghipour, N., and Graven, H.: Analysis of radiocarbon in atmospheric methane: technological advances and interpretation of measurements, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-7848, https://doi.org/10.5194/egusphere-egu24-7848, 2024.