Surface variability of short-wavelength radiation and temperature on exoplanets around M dwarfs
It is a common practice to use 3D General Circulation Models (GCM) with spatial resolution of a few hundred kilometers to simulate the climate of Earth-like exoplanets. The enhanced albedo effect of clouds is especially important for exoplanets in the habitable zones around M dwarfs that likely have fixed substellar regions and substantial cloud coverage. Here, we carry out mesoscale model simulations with 3 km spatial resolution driven by the initial and boundary conditions in a 3D GCM and find that it could significantly underestimate the spatial variability of both the incident short-wavelength radiation and the temperature at planet surface. Our findings suggest that mesoscale models with cloud-resolving capability be considered for future studies of exoplanet climate.
document
http://n2t.net/ark:/85065/d7gm893s
eng
geoscientificInformation
Text
publication
2016-01-01T00:00:00Z
publication
2017-03-10T00:00:00Z
Copyright 2017 the American Astronomical Society.
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