Data used in the figures of the article "A cool runaway greenhouse without surface magma ocean"

<p>These data have been generated with the codes Exo k and PCM.</p> <p>Exo k is an open-source software. A complete documentation on how to install and use it can be found at http://perso.astrophy.u-bordeaux.fr/&sim;jleconte/ exo k-doc/index.html.<br> The generic Global Climate Model PCM (formerly known as LMDZ.generic) used in this work is the version 2528 that can be downloaded with documentation from the SVN repository at https://svn.lmd.jussieu.fr/Planeto/trunk/ LMDZ.GENERIC/. More information and documentation are available at http://www-planets.lmd.jussieu.fr.</p> <p>The archive is organized as follows:<br> ├─ Fig1 (comparison of atmospheric profiles with a same Outgoing Thermal Radiation)<br> │&nbsp; ├─ OTR274.txt (profiles with a 274 W/m2 bolometric emission)<br> │&nbsp; ├─ OTR10000txt (profiles with a 1000 W/m2 bolometric emission)<br> │<br> ├─ Fig2 (Outgoing Thermal Radiation as a function of surface temperature)<br> │&nbsp; ├─ Geoflux=0 (internal heat flux = 0 W/m2)<br> │&nbsp; │&nbsp; ├─ T1_0_ISR_Tsurf_OTR_ALB.dat<br> │&nbsp; │&nbsp; ├─ Proxima_0_ISR_Tsurf_OTR_ALB.dat<br> │&nbsp; │&nbsp; ├─ M3_0_ISR_Tsurf_OTR_ALB.dat<br> │&nbsp; │&nbsp; ├─ Sun_0_ISR_Tsurf_OTR_ALB.dat<br> │&nbsp; │&nbsp; ├─ F1_0_ISR_Tsurf_OTR_ALB.dat<br> │&nbsp; ├─ Geoflux=0.09Wm-2 (internal heat flux = 0.09 W/m2)<br> │&nbsp;&nbsp;&nbsp;&nbsp; ├─ T1_0.09_ISR_Tsurf_OTR_ALB.dat<br> │&nbsp;&nbsp;&nbsp;&nbsp; ├─ Sun_0.09_ISR_Tsurf_OTR_ALB.dat<br> │<br> ├─ Fig3 (Trappist-1b profiles and spectra)<br> │&nbsp; ├─ Profiles<br> │&nbsp; │&nbsp; ├─ Adiabatic<br> │&nbsp; │&nbsp; │&nbsp;&nbsp; ├─ Trappist1b_adiabatic_profile_1EO.txt (1x Earth Ocean)<br> │&nbsp; │&nbsp; │&nbsp;&nbsp; ├─ Trappist1b_adiabatic_profile_3EO.txt (3x Earth Ocean)<br> │&nbsp; │&nbsp; │<br> │&nbsp; │&nbsp; ├─ Converged<br> │&nbsp; │&nbsp; │&nbsp;&nbsp; ├─ Trappist1b_profile_1EO_geoflux=0W.txt (1x Earth Ocean, internal heat flux = 0 W/m2)<br> │&nbsp; │&nbsp; │&nbsp;&nbsp; ├─ Trappist1b_profile_1EO_geoflux=5W.txt (1x Earth Ocean, internal heat flux = 5 W/m2)<br> │&nbsp; │&nbsp; │&nbsp;&nbsp; ├─ Trappist1b_profile_3EO_geoflux=0W.txt (3x Earth Ocean, internal heat flux = 0 W/m2)<br> │&nbsp; │&nbsp; │&nbsp;&nbsp; ├─ Trappist1b_profile_3EO_geoflux=5W.txt (3x Earth Ocean, internal heat flux = 5 W/m2)<br> │&nbsp; │&nbsp; │<br> │&nbsp; ├─ Spectra<br> │&nbsp; │&nbsp; ├─ Adiabatic<br> │&nbsp; │&nbsp; │&nbsp;&nbsp; ├─ Trappist1b_adiabatic_spectra_1EO.txt (1x Earth Ocean)<br> │&nbsp; │&nbsp; │&nbsp;&nbsp; ├─ Trappist1b_adiabatic_spectra_3EO.txt (3x Earth Ocean)<br> │&nbsp; │&nbsp; │<br> │&nbsp; │&nbsp; ├─ Converged<br> │&nbsp; │&nbsp; │&nbsp;&nbsp; ├─ Trappist1b_spectra_1EO_geoflux=0W.txt (1x Earth Ocean, internal heat flux = 0 W/m2)<br> │&nbsp; │&nbsp; │&nbsp;&nbsp; ├─ Trappist1b_spectra_1EO_geoflux=5W.txt (1x Earth Ocean, internal heat flux = 5 W/m2)<br> │&nbsp; │&nbsp; │&nbsp;&nbsp; ├─ Trappist1b_spectra_3EO_geoflux=0W.txt (3x Earth Ocean, internal heat flux = 0 W/m2)<br> │&nbsp; │&nbsp; │&nbsp;&nbsp; ├─ Trappist1b_spectra_3EO_geoflux=5W.txt (3x Earth Ocean, internal heat flux = 5 W/m2)<br> │<br> ├─ Fig4_(net stellar and emission fluxes for a converged and adiabatic profiles)<br> │&nbsp; ├─profiles_Sun_adia_converged_netfluxes.txt<br> │<br> ├─ Fig5 (Profiles for different instellations, for each star)<br> │&nbsp; ├─ T1_profiles.txt<br> │&nbsp; ├─ Proxima_profiles.txt<br> │&nbsp; ├─ M3_profiles.txt<br> │&nbsp; ├─ K5_profiles.txt<br> │&nbsp; ├─ Sun_profiles.txt<br> │&nbsp; ├─ F1_profiles.txt<br> │<br> ├─ Fig6 (Comparison 1D vs 3D)<br> │&nbsp; ├─ 1D<br> │&nbsp; │&nbsp; ├─ exok_1D_PTH_trappist1.txt<br> │&nbsp; │&nbsp; ├─ exok_1D_PTH_Proxima.txt<br> │&nbsp; │&nbsp; ├─ exok_1D_PTH_M3.txt<br> │&nbsp; ├─ 3D<br> │&nbsp;&nbsp;&nbsp;&nbsp; ├─ PT_trappist1_3D.dat<br> │&nbsp;&nbsp;&nbsp;&nbsp; ├─ PT_Proxima_3D.dat<br> │&nbsp;&nbsp;&nbsp;&nbsp; ├─ PT_M3_3D.dat<br> │&nbsp;&nbsp;&nbsp;&nbsp; ├─ HeatingRates_3D_trappist1.dat<br> │&nbsp;&nbsp;&nbsp;&nbsp; ├─ HeatingRates_3D_trappist1.dat<br> │&nbsp;&nbsp;&nbsp;&nbsp; ├─ HeatingRates_3D_trappist1.dat<br> │<br> ├─ Fig7 (Profiles for 2 values of instellation and 3 values of cp)<br> │&nbsp; ├─ profiles_cp_Sun.txt &nbsp;<br> │<br> ├─ Fig8 (Profiles for 3 values of instellation and continuums from 2 version of MT_sCKD)<br> │&nbsp; ├─ profiles_2continuums_Sun.txt &nbsp;<br> │<br> ├─ Fig9 (Profiles as a function of surface pressure and internal heat fluxes)<br> │&nbsp; ├─ EarlyVenus<br> │&nbsp; │&nbsp; ├─ profiles_fig9_EarlyVenus_0.1bar.txt<br> │&nbsp; │&nbsp; ├─ profiles_fig9_EarlyVenus_1bar.txt<br> │&nbsp; │&nbsp; ├─ profiles_fig9_EarlyVenus_10bar.txt<br> │&nbsp; │&nbsp; ├─ profiles_fig9_EarlyVenus_100bar.txt<br> │&nbsp; │&nbsp; ├─ profiles_fig9_EarlyVenus_270bar.txt<br> │&nbsp; ├─ Trappist1<br> │&nbsp;&nbsp;&nbsp;&nbsp; ├─ profiles_fig9_Trappist1_0.1bar.txt<br> │&nbsp;&nbsp;&nbsp;&nbsp; ├─ profiles_fig9_Trappist1_1bar.txt<br> │&nbsp;&nbsp;&nbsp;&nbsp; ├─ profiles_fig9_Trappist1_10bar.txt<br> │&nbsp;&nbsp;&nbsp;&nbsp; ├─ profiles_fig9_Trappist1_100bar.txt<br> │&nbsp;&nbsp;&nbsp;&nbsp; ├─ profiles_fig9_Trappist1_270bar.txt<br> │<br> ├─ readme.txt</p> <p>&nbsp;</p> <p>&nbsp;</p>