Figure 5 from Atmospheric Convection Plays a Key Role in the Climate of Tidally Locked Terrestrial Exoplanets: Insights from High-resolution Simulations

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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 5.

Atmospheric circulation regimes of (crosses) Trappist-1e and (circles) Proxima b simulations with (blue) MassFlux, (orange) Adjust, and (green) NoCnvPm setup, defined by the estimates of the nondimensional Rossby deformation radius (L_d/R_p, x-axis) and the nondimensional Rhines length (L_R/R_p, y-axis).

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