Articles | Volume 13, issue 2
https://doi.org/10.5194/gmd-13-707-2020
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
https://doi.org/10.5194/gmd-13-707-2020
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
Model experiment description paper
| Highlight paper
| 
21 Feb 2020
Model experiment description paper | Highlight paper |
| 21 Feb 2020
| 21 Feb 2020
TRAPPIST-1 Habitable Atmosphere Intercomparison (THAI): motivations and protocol version 1.0
Thomas J. Fauchez
CORRESPONDING AUTHOR
Goddard Earth Sciences Technology and Research (GESTAR), Universities Space Research Association (USRA), Columbia, MD, USA
NASA Goddard Space Flight Center, Greenbelt, MD, USA
GSFC Sellers Exoplanet Environments Collaboration, Greenbelt, MD, USA
Martin Turbet
Laboratoire de Méteorologie Dynamique, IPSL, Sorbonne Universités, UPMC Univ. Paris 06, CNRS, 4 Place Jussieu, 75005 Paris, France
Observatoire Astronomique de l'Université de Genève, Université de Genève, Chemin des Maillettes 51, 1290 Versoix, Switzerland
Eric T. Wolf
Laboratory for Atmospheric and Space Physics, Department of Atmospheric and Oceanic Sciences, University of Colorado Boulder, Boulder, CO, USA
Virtual Planetary Laboratory, NASA Astrobiology Institute, Seattle, WA, USA
Ian Boutle
Met Office, Exeter, UK
Michael J. Way
NASA Goddard Institute for Space Studies, New York, NY 10025, USA
GSFC Sellers Exoplanet Environments Collaboration, Greenbelt, MD, USA
Anthony D. Del Genio
NASA Goddard Institute for Space Studies, New York, NY 10025, USA
Nathan J. Mayne
University of Exeter, Exeter, UK
Konstantinos Tsigaridis
NASA Goddard Institute for Space Studies, New York, NY 10025, USA
Center for Climate Systems Research, Columbia University, New York, NY, USA
Ravi K. Kopparapu
NASA Goddard Space Flight Center, Greenbelt, MD, USA
GSFC Sellers Exoplanet Environments Collaboration, Greenbelt, MD, USA
Department of Atmospheric and Oceanic Sciences, School of Physics, Peking University, Beijing 100871, China
Francois Forget
Laboratoire de Méteorologie Dynamique, IPSL, Sorbonne Universités, UPMC Univ. Paris 06, CNRS, 4 Place Jussieu, 75005 Paris, France
Avi Mandell
NASA Goddard Space Flight Center, Greenbelt, MD, USA
GSFC Sellers Exoplanet Environments Collaboration, Greenbelt, MD, USA
Shawn D. Domagal Goldman
NASA Goddard Space Flight Center, Greenbelt, MD, USA
GSFC Sellers Exoplanet Environments Collaboration, Greenbelt, MD, USA
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- Idealized 2D Cloud-resolving Simulations for Tidally Locked Habitable Planets Q. Song et al. 10.3847/1538-4357/ac7879
- Simulations of idealised 3D atmospheric flows on terrestrial planets using LFRic-Atmosphere D. Sergeev et al. 10.5194/gmd-16-5601-2023
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- Longitudinally Asymmetric Stratospheric Oscillation on a Tidally Locked Exoplanet M. Cohen et al. 10.3847/1538-4357/ac625d
- Assessment of a physics-based retrieval of exoplanet atmospheric temperatures from infrared emission spectra F. Schreier et al. 10.1093/mnras/stad1526
- Asymmetry and Variability in the Transmission Spectra of Tidally Locked Habitable Planets X. Song & J. Yang 10.3389/fspas.2021.708023
- The TRAPPIST-1 Habitable Atmosphere Intercomparison (THAI). III. Simulated Observables—the Return of the Spectrum T. Fauchez et al. 10.3847/PSJ/ac6cf1
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- The Impact of the Explicit Representation of Convection on the Climate of a Tidally Locked Planet in Global Stretched-mesh Simulations D. Sergeev et al. 10.3847/1538-4357/ad4ecd
- Simulating biosignatures from pre-oxygen photosynthesizing life on TRAPPIST-1e J. Eager-Nash et al. 10.1093/mnras/stae1142
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- Detecting the proposed CH4–CO2 biosignature pair with the James Webb Space Telescope: TRAPPIST-1e and the effect of cloud/haze T. Mikal-Evans 10.1093/mnras/stab3383
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- Detectability of Molecular Signatures on TRAPPIST-1e through Transmission Spectroscopy Simulated for Future Space-based Observatories D. Pidhorodetska et al. 10.3847/2041-8213/aba4a1
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- Numerical dissipation strongly affects the equatorial jet speed in simulations of hot Jupiter atmospheres M. Hammond & D. Abbot 10.1093/mnras/stac228
- A detailed analysis of the Gl 486 planetary system J. Caballero et al. 10.1051/0004-6361/202243548
- How Does Background Air Pressure Influence the Inner Edge of the Habitable Zone for Tidally Locked Planets in a 3D View? Y. Zhang & J. Yang 10.3847/2041-8213/abb87f
- EOS-ESTM: a flexible climate model for habitable exoplanets L. Biasiotti et al. 10.1093/mnras/stac1642
- General Circulation Model Errors Are Variable across Exoclimate Parameter Spaces P. Kopparla et al. 10.3847/1538-4357/ac2d27
- Phase Modeling of the TRAPPIST-1 Planetary Atmospheres S. Kane et al. 10.3847/1538-3881/abcfbe
Discussed (final revised paper)
Latest update: 22 Nov 2024
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...
