EGU24-22506, updated on 11 Mar 2024
https://doi.org/10.5194/egusphere-egu24-22506
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

Quantification of CH4 Emissions from the EMIT and AVIRIS-3 Imaging Spectrometers

Red Willow Coleman1, Philip Brodrick1, K. Dana Chadwick1, Adam Chlus1, Michael Eastwood1, Clayton Elder1, Jay Fahlen1, Sergio Gomezbeltran2, Francesca Hopkins2, David Thompson1, Andrew Thorpe1, and Robert Green1
Red Willow Coleman et al.
  • 1NASA Jet Propulsion Lab, Pasadena, CA, USA
  • 2University of California Riverside, Riverside, CA, USA

Spaceborne and airborne imaging spectrometers can identify methane (CH4) plumes and enable emission quantification and direct sectoral attribution necessary to better constrain methane emissions and inform mitigation strategies. We will show CH4 emission quantification results and accompanying uncertainty products for CH4 plume observations from NASA’s Earth surface Mineral dust source InvesTigation (EMIT) imaging spectrometer onboard the International Space Station, as well as the recently developed Airborne Visible/Infrared Imaging Spectrometer 3 (AVIRIS-3). The differing spatial resolution and instrument sensitivity of the EMIT and AVIRIS-3 sensors are highly complementary for tiered CH4 plume detection and quantification. The large spatial coverage from EMIT allows us to identify and quantify previously unknown emissions from CH4 point sources across large regions of the Earth’s surface, while AVIRIS-3 has higher sensitivity and increased spatial resolution for characterizing CH4 emissions below EMIT’s detection limit.

Building on a legacy of greenhouse gas retrievals first developed for airborne imaging spectrometers (e.g., AVIRIS, AVIRIS-NG), we use a matched filter approach to retrieve CH4 enhancements and the per-plume integrated mass enhancement (IME) method with windspeed data to estimate hourly CH4 emission rates. We take a two-pronged approach to validating our CH4 emission detection and quantification method: (1) an AVIRIS-3 CH4 controlled release experiment with multiple flow rates, and (2) evaluation of a simultaneous collection of AVIRIS-3 and EMIT in West Texas’ Permian Basin oil-and-gas producing region. This validation work will help provide confidence in EMIT’s plume quantification approach, which is important as imaging spectrometers are necessary for more comprehensive understanding of global CH4 point source emissions and greenhouse gas budgets, particularly in areas with limited reporting requirements. Lastly, the EMIT greenhouse gas portal (https://earth.jpl.nasa.gov/emit/data/data-portal/Greenhouse-Gases/) is actively distributing methane data products in support of NASA’s Open Source Science Initiative and AVIRIS-3 data will soon be publicly available for interested decision-makers and users (e.g., U.S. Greenhouse Gas Center).

How to cite: Coleman, R. W., Brodrick, P., Chadwick, K. D., Chlus, A., Eastwood, M., Elder, C., Fahlen, J., Gomezbeltran, S., Hopkins, F., Thompson, D., Thorpe, A., and Green, R.: Quantification of CH4 Emissions from the EMIT and AVIRIS-3 Imaging Spectrometers, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-22506, https://doi.org/10.5194/egusphere-egu24-22506, 2024.

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