Mars Planetary Climate Model (MPCM) simulations during higher spin-axis obliquity periods

MPCM output used for the Figures in the paper "Increased Hydrogen escape from Mars atmosphere during periods of high obliquity" accepted on Nature Astronomy. FIgure 1 uses netcdf files called "concat_PhiH*nc" containing the H-escape rate (s-1) simulated for the corresponding Mars Years: concat_PhiH_MY28.nc, concat_PhiH_MY32.nc, concat_PhiH_MY33.nc 2. Figure 2 uses netcdf files called "concat3my*nc" containing the simulations for the reference simulation, for obliquity 30º and obliquity 35º, and corresponding start files: H-escape rate (s-1): concat3my_ref_PhiH.nc, concat3my_obl30_PhiH.nc, concat3my_obl35_PhiH.nc 3. Figure 3 uses netcdf files called "concat3my*nc" containing the simulations for the reference simulation, for obliquity 30º and obliquity 35º Temperature (K) and water vapour density (cm-3): concat3my_ref_temp_h2o.nc, concat3my_obl30_temp_h2o.nc, concat3my_obl35_temp_h2o.nc EXTENDED DATA: Figure 1 uses the netcdf files called "concat_PhiH*nc" containing the H-escape rate for: the simulation without microphisics and without extended ion reactions (concat_PhiH_nomicro_noh2oplus.nc), the simulation including the H2O microphysical model but not the H2O-ion photochemistry (concat_PhiH_noh2oplus.nc), a simulation including the both the H2O microphysical model and the extended H2O ionospheric reactions (concat_PhiH_ref.nc) Figure 2 uses the netcdf files called: Figure 3 uses the netcdf files called: concat_PhiH_MY25.nc, concat_PhiH_MY28.nc and concat_PhiH_MY34.nc (without Global Dust Storm), and concat_PhiH_MY25_dustclim.nc, concat_PhiH_MY28_dustclim.nc and concat_PhiH_MY34_dustclim.nc (with GDS)