Fig. 4

Impact of CO2 ice clouds on the surface temperature in atmospheres of planets around different main-sequence stars. Surface temperatures are shown as a function of optical depth (at a wavelength of λ = 0.1 μm) and effective particle size of the CO2 ice clouds. The black contour lines are given in steps of 5 K. The white contour line indicates the clear-sky case.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.