Include MORE simulation results for Earth model

intercomparison/inputs/more/evolution-model1-earth-config.in

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+Mp_E = 1
+CMF = 0.35
+Rp = 6378100.0 # in m; if 0 then calculated after Noack and Lasbleis 2020
+Rc = 3507955.0000000005 # same as for Rp 
+Mass_mantle = Mp_E*5.97219e24 * (1-CMF)
+CO2_ini = 1e+21
+H2O_ini = 4.2e+21
+N2_ini = 0
+CO2_ini_ppm = CO2_ini/Mass_mantle * 1e6
+H2O_ini_ppm = H2O_ini/Mass_mantle * 1e6
+N2_ini_ppm  = N2_ini/Mass_mantle * 1e6
+redox_buffer_vec [= 4,4] # Delta IW buffer variation evolving linearly during freezing, constant if same value for ini and end redox value 
+Tsurf = 2000 # in K
+MO_depth_km = (1-0.55)*6378.1 # note that calculated Rp and Rc in Int Struct model might slightly differ 
+star = Sun
+p_prim = 0 # primordial atmosphere in bar derived from stellar composition
+dF_end = 0.05
+dF_nr=1000
+ingassing = 1
+speciation = 1
+equilibrium = 1
+escapeH2 = 0 # 0-no excape, 1-full escape of all free H2, values inbetween scale erosion efficiency
+escapeHe = 0 # same for He
+trap_percent = 1
+D_H2O = 0.01 # partition coefficient of water
+D_CO2 = 0.001 # partition coefficient of CO2
+D_N = 0.001 # partition coefficient of N based on Keppler et al., 2022
+CO2_max_solid = 0.01 # 10 000 wt-ppm carbon max in solid mantle

intercomparison/inputs/more/evolution-model1-earth-grid-Hhigh-Chigh-config.in

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+Mp_E = 1
+CMF = 0.35
+Rp = 6378100.0 # in m; if 0 then calculated after Noack and Lasbleis 2020
+Rc = 3507955.0000000005 # same as for Rp 
+Mass_mantle = Mp_E*5.97219e24 * (1-CMF)
+CO2_ini = 2e+21
+H2O_ini = 1.4e+22
+N2_ini = 0
+CO2_ini_ppm = CO2_ini/Mass_mantle * 1e6
+H2O_ini_ppm = H2O_ini/Mass_mantle * 1e6
+N2_ini_ppm  = N2_ini/Mass_mantle * 1e6
+redox_buffer_vec [= 4,4] # Delta IW buffer variation evolving linearly during freezing, constant if same value for ini and end redox value 
+Tsurf = 2000 # in K
+MO_depth_km = (1-0.55)*6378.1 # note that calculated Rp and Rc in Int Struct model might slightly differ 
+star = Sun
+p_prim = 0 # primordial atmosphere in bar derived from stellar composition
+dF_end = 0.05
+dF_nr=1000
+ingassing = 1
+speciation = 1
+equilibrium = 1
+escapeH2 = 0 # 0-no excape, 1-full escape of all free H2, values inbetween scale erosion efficiency
+escapeHe = 0 # same for He
+trap_percent = 1
+D_H2O = 0.01 # partition coefficient of water
+D_CO2 = 0.001 # partition coefficient of CO2
+D_N = 0.001 # partition coefficient of N based on Keppler et al., 2022
+CO2_max_solid = 0.01 # 10 000 wt-ppm carbon max in solid mantle

intercomparison/inputs/more/evolution-model1-earth-grid-Hhigh-Clow-config.in

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+Mp_E = 1
+CMF = 0.35
+Rp = 6378100.0 # in m; if 0 then calculated after Noack and Lasbleis 2020
+Rc = 3507955.0000000005 # same as for Rp 
+Mass_mantle = Mp_E*5.97219e24 * (1-CMF)
+CO2_ini = 5e+20
+H2O_ini = 1.4e+22
+N2_ini = 0
+CO2_ini_ppm = CO2_ini/Mass_mantle * 1e6
+H2O_ini_ppm = H2O_ini/Mass_mantle * 1e6
+N2_ini_ppm  = N2_ini/Mass_mantle * 1e6
+redox_buffer_vec [= 4,4] # Delta IW buffer variation evolving linearly during freezing, constant if same value for ini and end redox value 
+Tsurf = 2000 # in K
+MO_depth_km = (1-0.55)*6378.1 # note that calculated Rp and Rc in Int Struct model might slightly differ 
+star = Sun
+p_prim = 0 # primordial atmosphere in bar derived from stellar composition
+dF_end = 0.05
+dF_nr=1000
+ingassing = 1
+speciation = 1
+equilibrium = 1
+escapeH2 = 0 # 0-no excape, 1-full escape of all free H2, values inbetween scale erosion efficiency
+escapeHe = 0 # same for He
+trap_percent = 1
+D_H2O = 0.01 # partition coefficient of water
+D_CO2 = 0.001 # partition coefficient of CO2
+D_N = 0.001 # partition coefficient of N based on Keppler et al., 2022
+CO2_max_solid = 0.01 # 10 000 wt-ppm carbon max in solid mantle

intercomparison/inputs/more/evolution-model1-earth-grid-Hhigh-Cmid-config.in

@@ -0,0 +1,28 @@
+Mp_E = 1
+CMF = 0.35
+Rp = 6378100.0 # in m; if 0 then calculated after Noack and Lasbleis 2020
+Rc = 3507955.0000000005 # same as for Rp 
+Mass_mantle = Mp_E*5.97219e24 * (1-CMF)
+CO2_ini = 1e+21
+H2O_ini = 1.4e+22
+N2_ini = 0
+CO2_ini_ppm = CO2_ini/Mass_mantle * 1e6
+H2O_ini_ppm = H2O_ini/Mass_mantle * 1e6
+N2_ini_ppm  = N2_ini/Mass_mantle * 1e6
+redox_buffer_vec [= 4,4] # Delta IW buffer variation evolving linearly during freezing, constant if same value for ini and end redox value 
+Tsurf = 2000 # in K
+MO_depth_km = (1-0.55)*6378.1 # note that calculated Rp and Rc in Int Struct model might slightly differ 
+star = Sun
+p_prim = 0 # primordial atmosphere in bar derived from stellar composition
+dF_end = 0.05
+dF_nr=1000
+ingassing = 1
+speciation = 1
+equilibrium = 1
+escapeH2 = 0 # 0-no excape, 1-full escape of all free H2, values inbetween scale erosion efficiency
+escapeHe = 0 # same for He
+trap_percent = 1
+D_H2O = 0.01 # partition coefficient of water
+D_CO2 = 0.001 # partition coefficient of CO2
+D_N = 0.001 # partition coefficient of N based on Keppler et al., 2022
+CO2_max_solid = 0.01 # 10 000 wt-ppm carbon max in solid mantle

intercomparison/inputs/more/evolution-model1-earth-grid-Hlow-Chigh-config.in

@@ -0,0 +1,28 @@
+Mp_E = 1
+CMF = 0.35
+Rp = 6378100.0 # in m; if 0 then calculated after Noack and Lasbleis 2020
+Rc = 3507955.0000000005 # same as for Rp 
+Mass_mantle = Mp_E*5.97219e24 * (1-CMF)
+CO2_ini = 2e+21
+H2O_ini = 1.4e+21
+N2_ini = 0
+CO2_ini_ppm = CO2_ini/Mass_mantle * 1e6
+H2O_ini_ppm = H2O_ini/Mass_mantle * 1e6
+N2_ini_ppm  = N2_ini/Mass_mantle * 1e6
+redox_buffer_vec [= 4,4] # Delta IW buffer variation evolving linearly during freezing, constant if same value for ini and end redox value 
+Tsurf = 2000 # in K
+MO_depth_km = (1-0.55)*6378.1 # note that calculated Rp and Rc in Int Struct model might slightly differ 
+star = Sun
+p_prim = 0 # primordial atmosphere in bar derived from stellar composition
+dF_end = 0.05
+dF_nr=1000
+ingassing = 1
+speciation = 1
+equilibrium = 1
+escapeH2 = 0 # 0-no excape, 1-full escape of all free H2, values inbetween scale erosion efficiency
+escapeHe = 0 # same for He
+trap_percent = 1
+D_H2O = 0.01 # partition coefficient of water
+D_CO2 = 0.001 # partition coefficient of CO2
+D_N = 0.001 # partition coefficient of N based on Keppler et al., 2022
+CO2_max_solid = 0.01 # 10 000 wt-ppm carbon max in solid mantle

intercomparison/inputs/more/evolution-model1-earth-grid-Hlow-Clow-config.in

@@ -0,0 +1,28 @@
+Mp_E = 1
+CMF = 0.35
+Rp = 6378100.0 # in m; if 0 then calculated after Noack and Lasbleis 2020
+Rc = 3507955.0000000005 # same as for Rp 
+Mass_mantle = Mp_E*5.97219e24 * (1-CMF)
+CO2_ini = 5e+20
+H2O_ini = 1.4e+21
+N2_ini = 0
+CO2_ini_ppm = CO2_ini/Mass_mantle * 1e6
+H2O_ini_ppm = H2O_ini/Mass_mantle * 1e6
+N2_ini_ppm  = N2_ini/Mass_mantle * 1e6
+redox_buffer_vec [= 4,4] # Delta IW buffer variation evolving linearly during freezing, constant if same value for ini and end redox value 
+Tsurf = 2000 # in K
+MO_depth_km = (1-0.55)*6378.1 # note that calculated Rp and Rc in Int Struct model might slightly differ 
+star = Sun
+p_prim = 0 # primordial atmosphere in bar derived from stellar composition
+dF_end = 0.05
+dF_nr=1000
+ingassing = 1
+speciation = 1
+equilibrium = 1
+escapeH2 = 0 # 0-no excape, 1-full escape of all free H2, values inbetween scale erosion efficiency
+escapeHe = 0 # same for He
+trap_percent = 1
+D_H2O = 0.01 # partition coefficient of water
+D_CO2 = 0.001 # partition coefficient of CO2
+D_N = 0.001 # partition coefficient of N based on Keppler et al., 2022
+CO2_max_solid = 0.01 # 10 000 wt-ppm carbon max in solid mantle

intercomparison/inputs/more/evolution-model1-earth-grid-Hlow-Cmid-config.in

@@ -0,0 +1,28 @@
+Mp_E = 1
+CMF = 0.35
+Rp = 6378100.0 # in m; if 0 then calculated after Noack and Lasbleis 2020
+Rc = 3507955.0000000005 # same as for Rp 
+Mass_mantle = Mp_E*5.97219e24 * (1-CMF)
+CO2_ini = 1e+21
+H2O_ini = 1.4e+21
+N2_ini = 0
+CO2_ini_ppm = CO2_ini/Mass_mantle * 1e6
+H2O_ini_ppm = H2O_ini/Mass_mantle * 1e6
+N2_ini_ppm  = N2_ini/Mass_mantle * 1e6
+redox_buffer_vec [= 4,4] # Delta IW buffer variation evolving linearly during freezing, constant if same value for ini and end redox value 
+Tsurf = 2000 # in K
+MO_depth_km = (1-0.55)*6378.1 # note that calculated Rp and Rc in Int Struct model might slightly differ 
+star = Sun
+p_prim = 0 # primordial atmosphere in bar derived from stellar composition
+dF_end = 0.05
+dF_nr=1000
+ingassing = 1
+speciation = 1
+equilibrium = 1
+escapeH2 = 0 # 0-no excape, 1-full escape of all free H2, values inbetween scale erosion efficiency
+escapeHe = 0 # same for He
+trap_percent = 1
+D_H2O = 0.01 # partition coefficient of water
+D_CO2 = 0.001 # partition coefficient of CO2
+D_N = 0.001 # partition coefficient of N based on Keppler et al., 2022
+CO2_max_solid = 0.01 # 10 000 wt-ppm carbon max in solid mantle

intercomparison/inputs/more/evolution-model1-earth-grid-Hmid-Chigh-config.in

@@ -0,0 +1,28 @@
+Mp_E = 1
+CMF = 0.35
+Rp = 6378100.0 # in m; if 0 then calculated after Noack and Lasbleis 2020
+Rc = 3507955.0000000005 # same as for Rp 
+Mass_mantle = Mp_E*5.97219e24 * (1-CMF)
+CO2_ini = 2e+21
+H2O_ini = 7.5e+21
+N2_ini = 0
+CO2_ini_ppm = CO2_ini/Mass_mantle * 1e6
+H2O_ini_ppm = H2O_ini/Mass_mantle * 1e6
+N2_ini_ppm  = N2_ini/Mass_mantle * 1e6
+redox_buffer_vec [= 4,4] # Delta IW buffer variation evolving linearly during freezing, constant if same value for ini and end redox value 
+Tsurf = 2000 # in K
+MO_depth_km = (1-0.55)*6378.1 # note that calculated Rp and Rc in Int Struct model might slightly differ 
+star = Sun
+p_prim = 0 # primordial atmosphere in bar derived from stellar composition
+dF_end = 0.05
+dF_nr=1000
+ingassing = 1
+speciation = 1
+equilibrium = 1
+escapeH2 = 0 # 0-no excape, 1-full escape of all free H2, values inbetween scale erosion efficiency
+escapeHe = 0 # same for He
+trap_percent = 1
+D_H2O = 0.01 # partition coefficient of water
+D_CO2 = 0.001 # partition coefficient of CO2
+D_N = 0.001 # partition coefficient of N based on Keppler et al., 2022
+CO2_max_solid = 0.01 # 10 000 wt-ppm carbon max in solid mantle

intercomparison/inputs/more/evolution-model1-earth-grid-Hmid-Clow-config.in

@@ -0,0 +1,28 @@
+Mp_E = 1
+CMF = 0.35
+Rp = 6378100.0 # in m; if 0 then calculated after Noack and Lasbleis 2020
+Rc = 3507955.0000000005 # same as for Rp 
+Mass_mantle = Mp_E*5.97219e24 * (1-CMF)
+CO2_ini = 5e+20
+H2O_ini = 7.5e+21
+N2_ini = 0
+CO2_ini_ppm = CO2_ini/Mass_mantle * 1e6
+H2O_ini_ppm = H2O_ini/Mass_mantle * 1e6
+N2_ini_ppm  = N2_ini/Mass_mantle * 1e6
+redox_buffer_vec [= 4,4] # Delta IW buffer variation evolving linearly during freezing, constant if same value for ini and end redox value 
+Tsurf = 2000 # in K
+MO_depth_km = (1-0.55)*6378.1 # note that calculated Rp and Rc in Int Struct model might slightly differ 
+star = Sun
+p_prim = 0 # primordial atmosphere in bar derived from stellar composition
+dF_end = 0.05
+dF_nr=1000
+ingassing = 1
+speciation = 1
+equilibrium = 1
+escapeH2 = 0 # 0-no excape, 1-full escape of all free H2, values inbetween scale erosion efficiency
+escapeHe = 0 # same for He
+trap_percent = 1
+D_H2O = 0.01 # partition coefficient of water
+D_CO2 = 0.001 # partition coefficient of CO2
+D_N = 0.001 # partition coefficient of N based on Keppler et al., 2022
+CO2_max_solid = 0.01 # 10 000 wt-ppm carbon max in solid mantle

intercomparison/inputs/more/evolution-model1-earth-grid-Hmid-Cmid-config.in

@@ -0,0 +1,28 @@
+Mp_E = 1
+CMF = 0.35
+Rp = 6378100.0 # in m; if 0 then calculated after Noack and Lasbleis 2020
+Rc = 3507955.0000000005 # same as for Rp 
+Mass_mantle = Mp_E*5.97219e24 * (1-CMF)
+CO2_ini = 1e+21
+H2O_ini = 7.5e+21
+N2_ini = 0
+CO2_ini_ppm = CO2_ini/Mass_mantle * 1e6
+H2O_ini_ppm = H2O_ini/Mass_mantle * 1e6
+N2_ini_ppm  = N2_ini/Mass_mantle * 1e6
+redox_buffer_vec [= 4,4] # Delta IW buffer variation evolving linearly during freezing, constant if same value for ini and end redox value 
+Tsurf = 2000 # in K
+MO_depth_km = (1-0.55)*6378.1 # note that calculated Rp and Rc in Int Struct model might slightly differ 
+star = Sun
+p_prim = 0 # primordial atmosphere in bar derived from stellar composition
+dF_end = 0.05
+dF_nr=1000
+ingassing = 1
+speciation = 1
+equilibrium = 1
+escapeH2 = 0 # 0-no excape, 1-full escape of all free H2, values inbetween scale erosion efficiency
+escapeHe = 0 # same for He
+trap_percent = 1
+D_H2O = 0.01 # partition coefficient of water
+D_CO2 = 0.001 # partition coefficient of CO2
+D_N = 0.001 # partition coefficient of N based on Keppler et al., 2022
+CO2_max_solid = 0.01 # 10 000 wt-ppm carbon max in solid mantle