Figure 7 from Atmospheric Convection Plays a Key Role in the Climate of Tidally Locked Terrestrial Exoplanets: Insights from High-resolution Simulations

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

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 7.

Meridional average of vertically integrated divergence of (solid lines) MSE flux and its (dashed lines) dry and (dotted lines) latent parts (﹩{\rm{\nabla }}\cdot \left({\boldsymbol{u}}h\right)﹩, ﹩{\rm{W}}\,{{\rm{m}}}^{-2}﹩) in (a) the Trappist-1e case, and (b) the Proxima b case, in the (blue) MassFlux, (orange) Adjust, and (green) NoCnvPm simulations.

Other Images in This Article

Copyright and Terms & Conditions