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dc.date.accessioned2021-04-21T20:00:19Z
dc.date.available2021-04-21T20:00:19Z
dc.date.created2021-02-22T12:12:00Z
dc.date.issued2021
dc.identifier.citationMazzini, Adriano Sciarra, Alessandra Etiope, Giuseppe Sadavarte, P. Houweling, S. Pandey, S. Husein, A. . Relevant methane emission to the atmosphere from a geological gas manifestation. Scientific Reports. 2021, 11(1), 984-997
dc.identifier.urihttp://hdl.handle.net/10852/85437
dc.description.abstractAbstract Quantifying natural geological sources of methane (CH 4 ) allows to improve the assessment of anthropogenic emissions to the atmosphere from fossil fuel industries. The global CH 4 flux of geological gas is, however, an object of debate. Recent fossil ( 14 C-free) CH 4 measurements in preindustrial-era ice cores suggest very low global geological emissions (~ 1.6 Tg year −1 ), implying a larger fossil fuel industry source. This is however in contrast with previously published bottom-up and top-down geo-emission estimates (~ 45 Tg year −1 ) and even regional-scale emissions of ~ 1–2 Tg year −1 . Here we report on significant geological CH 4 emissions from the Lusi hydrothermal system (Indonesia), measured by ground-based and satellite (TROPOMI) techniques. Both techniques indicate a total CH 4 output of ~ 0.1 Tg year −1 , equivalent to the minimum value of global geo-emission derived by ice core 14 CH 4 estimates. Our results are consistent with the order of magnitude of the emission factors of large seeps used in global bottom-up estimates, and endorse a substantial contribution from natural Earth’s CH 4 degassing. The preindustrial ice core assessments of geological CH 4 release may be underestimated and require further study. Satellite measurements can help to test geological CH 4 emission factors and explain the gap between the contrasting estimates.
dc.languageEN
dc.rightsAttribution 4.0 International
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/
dc.titleRelevant methane emission to the atmosphere from a geological gas manifestation
dc.typeJournal article
dc.creator.authorMazzini, Adriano
dc.creator.authorSciarra, Alessandra
dc.creator.authorEtiope, Giuseppe
dc.creator.authorSadavarte, P.
dc.creator.authorHouweling, S.
dc.creator.authorPandey, S.
dc.creator.authorHusein, A.
cristin.unitcode185,15,22,40
cristin.unitnameSenter for Jordens utvikling og dynamikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode1
dc.identifier.cristin1892275
dc.identifier.bibliographiccitationinfo:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Scientific Reports&rft.volume=11&rft.spage=984&rft.date=2021
dc.identifier.jtitleScientific Reports
dc.identifier.volume11
dc.identifier.issue1
dc.identifier.doihttps://doi.org/10.1038/s41598-021-83369-9
dc.identifier.urnURN:NBN:no-88104
dc.type.documentTidsskriftartikkel
dc.type.peerreviewedPeer reviewed
dc.source.issn2045-2322
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/85437/1/Mazzini_2021_SCIREP_Lusi_flux.pdf
dc.type.versionPublishedVersion
cristin.articleid4138
dc.relation.projectNFR/288299
dc.relation.projectNFR/223272
dc.relation.projectEC/FP7/308126


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