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dc.contributor.authorFauchez, TJ
dc.contributor.authorTurbet, M
dc.contributor.authorWolf, ET
dc.contributor.authorBoutle, I
dc.contributor.authorWay, MJ
dc.contributor.authorDel Genio, AD
dc.contributor.authorMayne, NJ
dc.contributor.authorTsigaridis, K
dc.contributor.authorKopparapu, RK
dc.contributor.authorYang, J
dc.contributor.authorForget, F
dc.contributor.authorMandell, A
dc.contributor.authorGoldman, SDD
dc.date.accessioned2020-04-09T10:40:06Z
dc.date.issued2020-02-21
dc.description.abstractUpcoming telescopes such as the James Webb Space Telescope (JWST), the European Extremely Large Telescope (E-ELT), the Thirty Meter Telescope (TMT) or the Giant Magellan Telescope (GMT) may soon be able to characterize, through transmission, emission or reflection spectroscopy, the atmospheres of rocky exoplanets orbiting nearby M dwarfs. One of the most promising candidates is the late M-dwarf system TRAPPIST-1, which has seven known transiting planets for which transit timing variation (TTV) measurements suggest that they are terrestrial in nature, with a possible enrichment in volatiles. Among these seven planets, TRAPPIST-1e seems to be the most promising candidate to have habitable surface conditions, receiving ~ 66 % of the Earth's incident radiation and thus needing only modest greenhouse gas inventories to raise surface temperatures to allow surface liquid water to exist. TRAPPIST-1e is, therefore, one of the prime targets for the JWST atmospheric characterization. In this context, the modeling of its potential atmosphere is an essential step prior to observation. Global climate models (GCMs) offer the most detailed way to simulate planetary atmospheres. However, intrinsic differences exist between GCMs which can lead to different climate prediction and thus observability of gas and/or cloud features in transmission and thermal emission spectra. Such differences should preferably be known prior to observations. In this paper we present a protocol to intercompare planetary GCMs. Four testing cases are considered for TRAPPIST-1e, but the methodology is applicable to other rocky exoplanets in the habitable zone. The four test cases included two land planets composed of modern-Earth and pure-CO2 atmospheres and two aqua planets with the same atmospheric compositions. Currently, there are four participating models (LMDG, ROCKE-3D, ExoCAM, UM); however, this protocol is intended to let other teams participate as well.en_GB
dc.description.sponsorshipNASA Planetary Science Division's Internal Scientist Funding Modelen_GB
dc.description.sponsorshipEuropean Union’s Horizon 2020en_GB
dc.description.sponsorshipNASA Astrobiology Programen_GB
dc.identifier.citationVol. 13 (2), pp. 707-716en_GB
dc.identifier.doi10.5194/gmd-13-707-2020
dc.identifier.grantnumber832738/ESCAPEen_GB
dc.identifier.urihttp://hdl.handle.net/10871/120631
dc.language.isoenen_GB
dc.publisherEuropean Geosciences Union (EGU)/Copernicus Publicationsen_GB
dc.rights© Author(s) 2020. This work is distributed under the Creative Commons Attribution 4.0 License.en_GB
dc.titleTRAPPIST-1 Habitable Atmosphere Intercomparison (THAI): Motivations and protocol version 1.0en_GB
dc.typeArticleen_GB
dc.date.available2020-04-09T10:40:06Z
dc.identifier.issn1991-959X
dc.descriptionThis is the final version. Available from European Geosciences Union via the DOI in this record. en_GB
dc.descriptionExoCAM (Wolf and Toon, 2015) is available on GitHub: https://github.com/storyofthewolf/ExoCAM (last access: 8 February 2020). The Met Office Unified Model is available for use under license; see http://www.metoffice.gov.uk/research/modelling-systems/unified-model (Met Office, 2020, last access: 8 February 2020). ROCKE-3D is public domain software and available for download for free from https://simplex.giss.nasa.gov/gcm/ROCKE-3D/ (last access: 8 February 2020, NASA Goddard Institute for Space Studies, 2020a). Annual tutorials for new users take place annually, whose recordings are freely available online at https://www.youtube.com/user/NASAGISStv/playlists?view=50&sort=dd&shelf_id=15 (last access: 8 February 2020b, NASA Goddard Institute for Space Studies, 2020b). LMDG is obtainable upon request from Martin Turbet (martin.turbet@lmd.jussieu.fr) and François Forget (francois.forget@lmd.jussieu.fr).en_GB
dc.identifier.journalGeoscientific Model Developmenten_GB
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/en_GB
dcterms.dateAccepted2019-12-05
exeter.funder::Leverhulme Trusten_GB
exeter.funder::Science and Technology Facilities Councilen_GB
rioxxterms.versionVoRen_GB
rioxxterms.licenseref.startdate2019-12-05
rioxxterms.typeJournal Article/Reviewen_GB
refterms.dateFCD2020-04-09T10:32:32Z
refterms.versionFCDVoR
refterms.dateFOA2020-04-09T10:40:16Z
refterms.panelBen_GB
refterms.depositExceptionpublishedGoldOA


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© Author(s) 2020. This work is distributed under the Creative Commons Attribution 4.0 License.
Except where otherwise noted, this item's licence is described as © Author(s) 2020. This work is distributed under the Creative Commons Attribution 4.0 License.