EGU2020-12559, updated on 12 Jun 2020
https://doi.org/10.5194/egusphere-egu2020-12559
EGU General Assembly 2020
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.

Satellite-derived Indian methane emission sources with TROPOMI retrievals and a high-resolution modelling framework: Initial comparison with WRF-GHG model results

Dhanyalekshmi Pillai1, Monish Deshpande1, Julia Marshall2, Christoph Gerbig2, Oliver Schneising3, and Michael Buchwitz3
Dhanyalekshmi Pillai et al.
  • 1Indian Institute of Science Education and Research Bhopal (dhanya@iiserb.ac.in), India
  • 2Max Planck Institute for Biogeochemistry, Jena, Germany
  • 3Institute of Environmental Physics (IUP), University of Bremen FB1, Bremen, Germany

In accordance with the Global stocktake under Article 14 of Paris Agreement, each county estimates its own greenhouse gas (GHG) emissions based on standardised bottom-up management methods. However, the accuracy of these methods along with the standards differs from country to country, resulting in large uncertainties that make it difficult to implement effective climate change mitigation strategies. India plays an important role in global methane emission scenario, necessitating the accurate quantification of its sources at the regional and the local levels. However, the country lacks sufficient long term, continuous and accurate observations of the atmospheric methane which are required to quantify its source, to understand changes in the carbon cycle and the climate system. Recent technological advancements in the use of satellite remote-sensing dedicated to the greenhouse gases enforce international standards for the observation methods; hence enabling those high-resolution-high-density observations to be utilised for this quantification purpose. This study focuses on exploring the use of such dedicated observations of the column-averaged dry-air mixing ratio of methane (XCH4) retrieved from TROPOMI onboard Sentinel-5 Precursor to quantify the major CH4 anthropogenic and natural emission fluxes over India.

Our inverse modelling approach at the mesoscale includes a high-resolution atmospheric modelling framework consisting of the Weather Research and Forecasting model with greenhouse gas module (WRF-GHG) and a set of prior emission inventory model data. We use TROPOMI retrievals derived using the Weighting Function Modified Differential Optical Absorption Spectroscopy (WFM-DOAS) retrieval algorithm. WRF-GHG simulations are performed in hourly time intervals at a horizontal resolution of 10 km ×10 km for a month. In order to compare our CH4 simulations with the satellite column data, we have also taken into account the different vertical sensitivities of the instrument by applying the averaging kernel to the model simulations. To demonstrate the model performance, our simulations are also compared with the CAMS reanalysis product based on ECMWF (European Centre for Medium-Range Weather Forecasts) numerical weather prediction reanalysis data available at a horizontal resolution of 0.25o × 0.25o. Our comparison of these modelling results against unique satellite dataset indicates high potential of using TROPOMI retrievals in distinguishing the major CH4 anthropogenic and natural sources over India via inverse modelling. The results will help to objectively investigate the claims of emission reductions and the efficiency of reduction countermeasures, as well as the establishment of standards and advancement of technology. The details about our approach and preliminary results based on our analysis using above satellite measurements and WRF-GHG simulations over India will be presented.  

 

How to cite: Pillai, D., Deshpande, M., Marshall, J., Gerbig, C., Schneising, O., and Buchwitz, M.: Satellite-derived Indian methane emission sources with TROPOMI retrievals and a high-resolution modelling framework: Initial comparison with WRF-GHG model results, EGU General Assembly 2020, Online, 4–8 May 2020, EGU2020-12559, https://doi.org/10.5194/egusphere-egu2020-12559, 2020

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