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dc.contributor.authorChristie, DA
dc.contributor.authorLee, EKH
dc.contributor.authorInnes, S
dc.contributor.authorNoti, PA
dc.contributor.authorCharnay, B
dc.contributor.authorFauchez, TJ
dc.contributor.authorMayne, NJ
dc.contributor.authorDeitrick, R
dc.contributor.authorDing, F
dc.contributor.authorGreco, JJ
dc.contributor.authorHammond, M
dc.contributor.authorMalsky, I
dc.contributor.authorMandell, A
dc.contributor.authorRauscher, E
dc.contributor.authorRoman, MT
dc.contributor.authorSergeev, DE
dc.contributor.authorSohl, L
dc.contributor.authorSteinrueck, ME
dc.contributor.authorTurbet, M
dc.contributor.authorWolf, ET
dc.contributor.authorZamyatina, M
dc.contributor.authorCarone, L
dc.date.accessioned2022-10-19T11:59:52Z
dc.date.issued2022-11-28
dc.date.updated2022-10-19T10:39:57Z
dc.description.abstractWith an increased focus on the observing and modelling of mini-Neptunes, there comes a need to better understand the tools we use to model their atmospheres. In this paper, we present the protocol for the CAMEMBERT (Comparing Atmospheric Models of Extrasolar Mini-neptunes Building and Envisioning Retrievals and Transits) project, an intercomparison of general circulation models (GCMs) used by the exoplanetary science community to simulate the atmospheres of mini-Neptunes. We focus on two targets well studied both observationally and theoretically with planned JWST Cycle 1 observations: the warm GJ 1214b and the cooler K2-18b. For each target, we consider a temperature-forced case, a clear sky dual-grey radiative transfer case, and a clear sky multi band radiative transfer case, covering a range of complexities and configurations where we know differences exist between GCMs in the literature. This paper presents all the details necessary to participate in the intercomparison, with the intention of presenting the results in future papers. Currently, there are eight GCMs participating (ExoCAM, Exo-FMS, FMS PCM, Generic PCM, MITgcm, RM-GCM, THOR, and the UM), and membership in the project remains open. Those interested in participating are invited to contact the authors.en_GB
dc.description.sponsorshipScience and Technology Facilities Council (STF)en_GB
dc.description.sponsorshipUKRIen_GB
dc.description.sponsorshipLeverhulme Trusten_GB
dc.description.sponsorshipInstitute of Physicsen_GB
dc.description.sponsorshipSNSFen_GB
dc.description.sponsorshipGSFC Sellers Exoplanet Environments Collaboration (SEEC)en_GB
dc.description.sponsorshipEuropean Research Council (ERC)en_GB
dc.identifier.citationVol. 3 (11), article 261en_GB
dc.identifier.doi10.3847/PSJ/ac9dfe
dc.identifier.grantnumberST/R000395/1en_GB
dc.identifier.grantnumberMR/T040866/1en_GB
dc.identifier.grantnumberRPG-2020-82en_GB
dc.identifier.grantnumber193448en_GB
dc.identifier.grantnumber740963en_GB
dc.identifier.urihttp://hdl.handle.net/10871/131328
dc.identifierORCID: 0000-0001-6707-4563 (Mayne, Nathan)
dc.language.isoenen_GB
dc.publisherIOP Publishingen_GB
dc.relation.urlhttps://ckan.emac.gsfc.nasa.gov/organization/cuisines-camemberten_GB
dc.relation.urlhttps://github.com/projectcuisines/camemberten_GB
dc.rights© 2022. The Author(s). Published by the American Astronomical Society. Open access. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.
dc.subjectMini Neptunesen_GB
dc.subjectExoplanet Atmospheresen_GB
dc.titleCAMEMBERT: A Mini-Neptunes General Circulation Model Intercomparison, Protocol Version 1.0.A CUISINES Model Intercomparison Projecten_GB
dc.typeArticleen_GB
dc.date.available2022-10-19T11:59:52Z
dc.identifier.issn2632-3338
dc.descriptionThis is the final version. Available on open access from IOP Publishing via the DOI in this recorden_GB
dc.descriptionThe data resulting from the simulations and analysis will be uploaded to the CAMEMBERT permanent repository at https://ckan.emac.gsfc.nasa.gov/organization/cuisines-camembert by participating scientists. These data will be made available for public access upon the publication of the results. Pre-publication access can be requested by contacting the authors. Inputs described in this protocol and scripts related to the analysis of data and production of plots for the publications will be made available on the CAMEMBERT GitHub repository at https://github.com/projectcuisines/camembert. Inputs will be available immediately while scripts to reproduce results will be made publicly available upon the publication of the results.en_GB
dc.identifier.journalThe Planetary Science Journalen_GB
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/en_GB
dcterms.dateAccepted2022-10-14
dcterms.dateSubmitted2022-07-29
rioxxterms.versionVoRen_GB
rioxxterms.licenseref.startdate2022-10-14
rioxxterms.typeJournal Article/Reviewen_GB
refterms.dateFCD2022-10-19T10:40:00Z
refterms.versionFCDAM
refterms.dateFOA2022-12-19T17:05:59Z
refterms.panelBen_GB


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© 2022. The Author(s). Published by the American Astronomical Society. Open access. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.
Except where otherwise noted, this item's licence is described as © 2022. The Author(s). Published by the American Astronomical Society. Open access. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.