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Modeling the phase curve of hot rocky planets with 3D climate models
FORGET, F.
Université Pierre et Marie Curie - Paris 6 [UPMC]
Laboratoire de Météorologie Dynamique (UMR 8539) [LMD]
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Université Pierre et Marie Curie - Paris 6 [UPMC]
Laboratoire de Météorologie Dynamique (UMR 8539) [LMD]
FORGET, F.
Université Pierre et Marie Curie - Paris 6 [UPMC]
Laboratoire de Météorologie Dynamique (UMR 8539) [LMD]
< Reduce
Université Pierre et Marie Curie - Paris 6 [UPMC]
Laboratoire de Météorologie Dynamique (UMR 8539) [LMD]
Language
en
Communication dans un congrès
This item was published in
2011epsc.conf.1344S, 2011epsc.conf.1344S, EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. p.1344, 2011, 2011, Nantes. 2011-10p. 1344
English Abstract
Using a 3D climate model, we study how the apparent emission of a hot terrestrial exoplanet varies with wavelength and orbital phase, for different atmospheric pressures, and inclinations, in the case of a tidally-locked ...Read more >
Using a 3D climate model, we study how the apparent emission of a hot terrestrial exoplanet varies with wavelength and orbital phase, for different atmospheric pressures, and inclinations, in the case of a tidally-locked planet. Based on these synthetic thermal phase curves, we investigate how the planet and its atmosphere could be characterized by spatiallyunresolved spectro-photometry of the system with JWST and EChO.Read less <
Origin
Hal imported