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dc.contributor.authorBrewer, J.F.
dc.contributor.authorMillet, D.B.
dc.contributor.authorWells, K.C.
dc.contributor.authorPayne, V.H.
dc.contributor.authorKulawik, S.
dc.contributor.authorVigouroux, C.
dc.contributor.authorCady-Pereira, K.E.
dc.contributor.authorPernak, R.
dc.contributor.authorZhou, M.
dc.date2024
dc.date.accessioned2024-09-11T15:52:21Z
dc.date.available2024-09-11T15:52:21Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/13436
dc.descriptionEthane is the most abundant non-methane hydrocarbon in the troposphere, where it impacts ozone and reactive nitrogen and is a key tracer used for partitioning emitted methane between anthropogenic and natural sources. However, quantification has been challenged by sparse observations. Here, we present a satellite-based measurement of tropospheric ethane and demonstrate its utility for fossil-fuel source quantification. An ethane spectral signal is detectable from space in Cross-track Infrared Sounder (CrIS) radiances, revealing ethane signatures associated with fires and fossil fuel production. We use machine-learning to convert these signals to ethane abundances and validate the results against surface observations (R2 = 0.66, mean CrIS/surface ratio: 0.65). The CrIS data show that the Permian Basin in Texas and New Mexico exhibits the largest persistent ethane enhancements on the planet, with regional emissions underestimated by seven-fold. Correcting this underestimate reveals Permian ethane emissions that represent at least 4-7% of the global fossil-fuel ethane source.
dc.languageeng
dc.titleSpace-based observations of tropospheric ethane map emissions from fossil fuel extraction
dc.typeArticle
dc.subject.frascatiEarth and related Environmental sciences
dc.audienceScientific
dc.source.titleNature Communications
dc.source.volume15
dc.source.issue1
dc.source.pageA7829
Orfeo.peerreviewedYes
dc.identifier.doi10.1038/s41467-024-52247-z
dc.identifier.url


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