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Geoscientific Model Development An interactive open-access journal of the European Geosciences Union
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GMD | Articles | Volume 13, issue 2
Geosci. Model Dev., 13, 707–716, 2020
https://doi.org/10.5194/gmd-13-707-2020
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.
Geosci. Model Dev., 13, 707–716, 2020
https://doi.org/10.5194/gmd-13-707-2020
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.

Model experiment description paper 21 Feb 2020

Model experiment description paper | 21 Feb 2020

TRAPPIST-1 Habitable Atmosphere Intercomparison (THAI): motivations and protocol version 1.0

Thomas J. Fauchez et al.

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Status: closed
Status: closed
AC: Author comment | RC: Referee comment | SC: Short comment | EC: Editor comment
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Peer review completion

AR: Author's response | RR: Referee report | ED: Editor decision
AR by Thomas Fauchez on behalf of the Authors (03 Nov 2019)  Author's response    Manuscript
ED: Publish subject to minor revisions (review by editor) (19 Nov 2019) by Julia Hargreaves
AR by Lorena Grabowski on behalf of the Authors (02 Dec 2019)  Author's response
ED: Publish as is (05 Dec 2019) by Julia Hargreaves
Publications Copernicus
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Short summary
Atmospheric characterization of rocky exoplanets orbiting within the habitable zone of nearby M dwarf stars is around the corner with the James Webb Space Telescope (JWST), expected to be launch in 2021. Global climate models (GCMs) are powerful tools to model exoplanet atmospheres and to predict their habitability. However, intrinsic differences between the models can lead to various predictions. This paper presents an experiment protocol to evaluate these differences.
Atmospheric characterization of rocky exoplanets orbiting within the habitable zone of nearby M...
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