Data for "Climate Patterns of Spin-Orbit Resonant Exoplanets Around Low-Mass Stars"

Dataset analysed in order to obtain the results published in "Climate Patterns of Spin-Orbit Resonant Exoplanets Around Low-Mass Stars":

IGCM_data: atmospheric data obtained by using the flux programme on the outcome of the FORTE2.0 climate simulations for both the dynamic ocean (named "resonance") and the thermodynamic ocean (named "nodynamics")

MOMA_data: oceaninc data of the FORTE2.0 climate simulations for both the dynamic ocean (named "resonance") and the thermodynamic ocean (named "nodynamics")

Details of the data used to produce each figure:

Figure 2: MOMA_data.zip/fkph*_resonance_equator_*days_3to2_halfday.nc

Figure 3: MOMA_data.zip/fkph*_resonance_equator_*days_3to2_halfday.nc and MOMA_data.zip/fkph*_nodynamics_equator_*days_3to2_halfday.nc -

Figure 4: MOMA_data.zip/fkph*_resonance_equator_*days_3to2_halfday.nc

Figure 5: IGCM_data.zip/HALFDAY_raintemp_equator_fkph*_resonance_*days.cdf 

Figure 6: IGCM_data.zip/HALFDAY_raintemp_equator_fkph*_resonance_*days.cdf

Figure 7: IGCM_data.zip/HALFDAY_winds_equator_fkph*_resonance_*days.cdf and IGCM_data.zip/HALFDAY_winds_120_fkph*_resonance_*days.cdf 

Figure 8: IGCM_data.zip/HALFDAY_fluxes_equator_fkph*_resonance_*days.cdf

Figure 9: IGCM_data.zip/HALFDAY_fluxes_equator_fkph*_resonance_*days.cdf and IGCM_data.zip/HALFDAY_fluxes_equator_fkph*_nodynamics_*days.cdf

The FORTE2.0 code, compilation instructions and example run scripts, together with all necessary ancillary files, are accessible at doi.org/10.5281/zenodo.4108373 (Blaker et al., 2020).