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dc.contributor.authorMarshall, John C
dc.date.accessioned2022-09-16T19:45:56Z
dc.date.available2021-10-27T19:56:49Z
dc.date.available2022-09-16T19:45:56Z
dc.date.issued2021
dc.identifier.urihttps://hdl.handle.net/1721.1/133817.2
dc.description.abstract©2020. The Authors. Simulations of the CMIP6 historical period 1850–2014, characterized by the emergence of anthropogenic climate drivers like greenhouse gases, are presented for different configurations of the NASA Goddard Institute for Space Studies (GISS) Earth System ModelE2.1. The GISS-E2.1 ensembles are more sensitive to greenhouse gas forcing than their CMIP5 predecessors (GISS-E2) but warm less during recent decades due to a forcing reduction that is attributed to greater longwave opacity in the GISS-E2.1 pre-industrial simulations. This results in an atmosphere less sensitive to increases in opacity from rising greenhouse gas concentrations, demonstrating the importance of the base climatology to forcing and forced climate trends. Most model versions match observed temperature trends since 1979 from the ocean to the stratosphere. The choice of ocean model is important to the transient climate response, as found previously in CMIP5 GISS-E2: the model that more efficiently exports heat to the deep ocean shows a smaller rise in tropospheric temperature. Model sea level rise over the historical period is traced to excessive drawdown of aquifers to meet irrigation demand with a smaller contribution from thermal expansion. This shows how fully coupled models can provide indirect observational constraints upon forcing, in this case, constraining irrigation rates with observed sea level changes. The overall agreement of GISS-E2.1 with observed trends is familiar from evaluation of its predecessors, as is the conclusion that these trends are almost entirely anthropogenic in origin.en_US
dc.language.isoen
dc.publisherAmerican Geophysical Union (AGU)en_US
dc.relation.isversionof10.1029/2019MS002034en_US
dc.rightsCreative Commons Attribution 4.0 International licenseen_US
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/en_US
dc.sourceAmerican Geophysical Union (AGU)en_US
dc.titleCMIP6 Historical Simulations (1850–2014) With GISS‐E2.1en_US
dc.typeArticleen_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciencesen_US
dc.relation.journalJournal of Advances in Modelling Earth Systemsen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dc.date.updated2021-09-17T13:42:28Z
dspace.orderedauthorsMiller, RL; Schmidt, GA; Nazarenko, LS; Bauer, SE; Kelley, M; Ruedy, R; Russell, GL; Ackerman, AS; Aleinov, I; Bauer, M; Bleck, R; Canuto, V; Cesana, G; Cheng, Y; Clune, TL; Cook, BI; Cruz, CA; Del Genio, AD; Elsaesser, GS; Faluvegi, G; Kiang, NY; Kim, D; Lacis, AA; Leboissetier, A; LeGrande, AN; Lo, KK; Marshall, J; Matthews, EE; McDermid, S; Mezuman, K; Murray, LT; Oinas, V; Orbe, C; Pérez García-Pando, C; Perlwitz, JP; Puma, MJ; Rind, D; Romanou, A; Shindell, DT; Sun, S; Tausnev, N; Tsigaridis, K; Tselioudis, G; Weng, E; Wu, J; Yao, M-Sen_US
dspace.date.submission2021-09-17T13:42:34Z
mit.journal.volume13en_US
mit.journal.issue1en_US
mit.licensePUBLISHER_CC
mit.metadata.statusPublication Information Neededen_US


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