EGU23-9174, updated on 08 Feb 2024
https://doi.org/10.5194/egusphere-egu23-9174
EGU General Assembly 2023
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

Detection of local atmospheric methane enhancements by analyzing Sentinel-5 Precursor satellite data

Steffen Vanselow, Oliver Schneising-Weigel, Michael Buchwitz, Heinrich Bovensmann, and John P. Burrows
Steffen Vanselow et al.
  • University of Bremen, Institute of Environmental Physics (IUP), Physics, Bremen, Germany (vanselow@iup.physik.uni-bremen.de)

Methane CH4 is an important anthropogenic greenhouse gas and its rising concentration in the atmosphere contributes significantly to global warming. Satellite measurements of the column-averaged dry-air mole fraction of atmospheric methane, denoted as XCH4, can be used to provide information about the location of methane sources and on their emissions, which can help to improve emission inventories and review policies to mitigate climate change.   

The Sentinel-5 Precursor (S5P) satellite with the TROPOspheric Monitoring Instrument (TROPOMI) onboard was launched in October 2017 into a sun-synchronous orbit with an equator crossing time of 13:30. TROPOMI measures reflected solar radiation in different wavelength bands to generate various data products and combines daily global coverage with high spatial resolution. TROPOMI's observations in the shortwave infrared (SWIR) spectral range yield methane with a horizontal resolution of typically 5.5 x 7 km2

We used a monthly XCH4 data set (2018-2021) generated with the WFM-DOAS retrieval algorithm, developed at the University of Bremen, to detect regions with temporally persistent, locally enhanced XCH4. At first, we applied a spatial high-pass filter to the XCH4 data set to filter out the large-scale methane fluctuations. The resulting anomaly ΔXCH4 maps show the difference of the local XCH4 values compared to its surroundings. We then analyzed the monthly anomaly maps to identify potential source regions with persistent XCH4 enhancements by utilizing different filter criteria, such as the number of months in which the local methane anomalies ΔXCH4 must exceed certain threshold values. As a next step, we used a simple mass balance method to estimate the monthly emissions and the corresponding uncertainties of the detected potential source regions from the monthly averaged XCH4 maps. In the last step, we interpreted the emissions of the potential source regions in terms of the source type, by comparing the detected potential source regions with emission databases based on a spatial analysis. 

In this presentation, the algorithm and initial results concerning the detection of regions with temporally persistent, local XCH4 enhancements, originating from localized potential methane sources (e.g., wetlands, coal mining areas, oil and gas fields) are presented.     

How to cite: Vanselow, S., Schneising-Weigel, O., Buchwitz, M., Bovensmann, H., and Burrows, J. P.: Detection of local atmospheric methane enhancements by analyzing Sentinel-5 Precursor satellite data, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-9174, https://doi.org/10.5194/egusphere-egu23-9174, 2023.