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dc.contributor.authorEager-Nash, JK
dc.contributor.authorMayne, NJ
dc.contributor.authorNicholson, AE
dc.contributor.authorPrins, JE
dc.contributor.authorYoung, OCF
dc.contributor.authorDaines, SJ
dc.contributor.authorSergeev, DE
dc.contributor.authorLambert, FH
dc.contributor.authorManners, J
dc.contributor.authorBoutle, IA
dc.contributor.authorWolf, WT
dc.contributor.authorKamp, IEE
dc.contributor.authorKohary, K
dc.contributor.authorLenton, TM
dc.date.accessioned2023-02-22T09:59:22Z
dc.date.issued2023-03-01
dc.date.updated2023-02-22T08:42:11Z
dc.description.abstractMethane is thought to have been an important greenhouse gas during the Archean, although its potential warming has been found to be limited at high concentrations due to its high shortwave absorption. We use the Met Office Unified Model, a general circulation model, to further explore the climatic effect of different Archean methane concentrations. Surface warming peaks at a pressure ratio pCH4:pCO2 of approximately 0.1, reaching a maximum of up to 7 K before significant cooling above this ratio. Equator-to-pole temperature differences also tend to increase up to pCH4 ≤ 300 Pa, which is driven by a difference in radiative forcing at the equator and poles by methane and a reduction in the latitudinal extend of the Hadley circulation. 3D models are important to fully capture the cooling effect of methane, due to these impacts of the circulation.en_GB
dc.description.sponsorshipUK Research and Innovationen_GB
dc.description.sponsorshipLeverhulme Trusten_GB
dc.description.sponsorshipScience and Technology Facilities Council (STFC)en_GB
dc.identifier.citationVol. 128 (6), article e2022JD037544en_GB
dc.identifier.doi10.1029/2022JD037544
dc.identifier.grantnumberMR/T040866/1en_GB
dc.identifier.grantnumberST/R000395/1en_GB
dc.identifier.urihttp://hdl.handle.net/10871/132519
dc.identifierORCID: 0000-0001-6707-4563 (Mayne, Nathan)
dc.language.isoenen_GB
dc.publisherAmerican Geophysical Unionen_GB
dc.relation.urlhttps://doi.org/10.24378/exe.4347en_GB
dc.rights© 2023. The Authors. This is an open access article under the terms of the Creative Commons Attribution License, which permits use, distribution and reproduction in any medium, provided the original work is properly cited.
dc.title3D climate simulations of the Archean find that Methane has a strong cooling effect at high concentrations (article)en_GB
dc.typeArticleen_GB
dc.date.available2023-02-22T09:59:22Z
dc.identifier.issn2169-897X
dc.descriptionThis is the final version. Available on open access from via the American Geophysical Union the DOI in this recorden_GB
dc.descriptionOpen Research: The research data supporting this publication are openly available from the University of Exeter’s institutional repository at: https://doi.org/10.24378/exe.4347 with CC BY 4.0 (Eager-Nash et al., 2022)en_GB
dc.identifier.journalJournal of Geophysical Research: Atmospheresen_GB
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/en_GB
dcterms.dateAccepted2023-02-19
dcterms.dateSubmitted2022-07-22
rioxxterms.versionVoRen_GB
rioxxterms.licenseref.startdate2023-02-19
rioxxterms.typeJournal Article/Reviewen_GB
refterms.dateFCD2023-02-22T08:42:14Z
refterms.versionFCDAM
refterms.dateFOA2023-03-24T15:34:52Z
refterms.panelBen_GB


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© 2023. The Authors.
This is an open access article under
the terms of the Creative Commons
Attribution License, which permits use,
distribution and reproduction in any
medium, provided the original work is
properly cited.
Except where otherwise noted, this item's licence is described as © 2023. The Authors. This is an open access article under the terms of the Creative Commons Attribution License, which permits use, distribution and reproduction in any medium, provided the original work is properly cited.