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Atmospheric Convection Plays a Key Role in the Climate of Tidally Locked Terrestrial Exoplanets: Insights from High-resolution Simulations

  • Authors: Denis E. Sergeev, F. Hugo Lambert, Nathan J. Mayne, Ian Boutle, James Manners, and Krisztian Kohary

2020 The Astrophysical Journal 894 84.

  • Provider: AAS Journals

Caption: Figure 8.

Latitudinal cross section of the zonal transport of sensible (cpT, black contours, solid—positive, dotted—negative) and latent (Lq, color shading) heat (﹩{10}^{6}\,{\rm{W}}\,{{\rm{m}}}^{-2}﹩) through the eastern terminator (90°E) in (left column) the Trappist-1e case and (right column) the Proxima b case in (a) and (b) MassFlux, (c) and (d) Adjust, and (e) and (f) NoCnvPm simulations.

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