Articles | Volume 11, issue 10
https://doi.org/10.5194/amt-11-5673-2018
© Author(s) 2018. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
https://doi.org/10.5194/amt-11-5673-2018
© Author(s) 2018. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
Quantifying methane point sources from fine-scale satellite observations of atmospheric methane plumes
Daniel J. Varon
CORRESPONDING AUTHOR
School of Engineering and Applied Sciences, Harvard University, Cambridge, MA 02138, USA
GHGSat, Inc., Montréal, QC H2W 1Y5, Canada
Daniel J. Jacob
School of Engineering and Applied Sciences, Harvard University, Cambridge, MA 02138, USA
Jason McKeever
GHGSat, Inc., Montréal, QC H2W 1Y5, Canada
Dylan Jervis
GHGSat, Inc., Montréal, QC H2W 1Y5, Canada
Berke O. A. Durak
GHGSat, Inc., Montréal, QC H2W 1Y5, Canada
Department of Atmospheric and Oceanic Sciences, McGill University, Montréal, QC H3A 0B9, Canada
Department of Atmospheric and Oceanic Sciences, McGill University, Montréal, QC H3A 0B9, Canada
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Saved (final revised paper)
Latest update: 23 Nov 2024
Short summary
Methane is a powerful greenhouse gas emitted from numerous human activities. Space-based observation of point sources would be a cost-effective monitoring solution, but the resolution of most current and planned methane-observing satellites is too coarse to resolve individual emitters. We simulate fine-resolution (50 m) satellite observations of methane plumes as would be measured by GHGSat (to be launched in 2019) and show that such data can usefully quantify large methane point sources.
Methane is a powerful greenhouse gas emitted from numerous human activities. Space-based...