Global Methane Emissions Through an Isotopic Lens
<p>Changes in atmospheric methane (CH<sub>4</sub>) are mainly driven by natural, anthropogenic and pyrogenic emissions and oxidation by OH.</p><p>There is no consensus about the underlying explanations about hemispheric-scale changes in atmospheric methane (CH<sub>4</sub>). This is partly due to sparse data that do not exclusively identify individual changes in surface emissions and surface and atmospheric losses of CH<sub>4</sub>. This challenge represents a major scientific weakness in our understanding of this potent greenhouse gas, with implications for meeting global climate policy obligations. &#160;A confounding challenge is that the regional importance of individual emission sources change with time due to, for example, innovations in agricultural practices, climate-sensitive wetlands, and political decisions associated with climate friendlier transitional fuels. &#160;</p><p><br>Here we use bulk isotope ratios &#948;<sup>13</sup>C and &#948;D of CH<sub>4</sub> that have been previously shown to provide effective constraints on source apportionment: different CH<sub>4</sub> sources have characteristic isotope ratios. One of the key challenges associated with using these data is that region-specific isotope ratios change with time due to varying source prevalance, in addition to source signatures having inherent uncertainties. We use the GEOS-Chem global 3-D chemical transport model to describe the spatial and temporal isotopic behaviour of atmospheric CH<sub>4</sub>. We develop a Maximum A-Posteriori inverse method to simultaneously infer time dependent CH<sub>4</sub> emissions and isotope ratios from in situ data.&#160;</p><p>We will report the magnitude, distribution and source attribution of CH<sub>4</sub> emissions from 2004 to 2017, inferred from in situ measurements of total atmospheric CH<sub>4</sub> mole fraction and the corresponding measurements of &#948;<sup>13</sup>C and &#948;D. We will compare our results with previous studies.</p>