Modeling the phase curve of hot rocky planets with 3D climate models
Idioma
en
Communication dans un congrès
Este ítem está publicado en
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
Resumen en inglés
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 ...Leer más >