Crustal thickness and effective elastic thickness models of Venus

For details see Jiménez-Díaz et al. (2015). - Spherical harmonic coefficients of the shape of the crust-mantle interface: Venus_Moho.sh - Crustal thickness model with a spatial resolution of 0.5 degrees, in grid (*.grd) and data table (*.xyz) formats: Venus_Crustal_Thickness.grdFormat:Gridline node registration used [Geographic grid]x_min: 0 x_max: 360 x_inc: 0.5 (30 min) name: longitude n_columns: 721y_min: -90 y_max: 90 y_inc: 0.5 (30 min) name: latitude n_rows: 361z_min: 12.2915114449 z_max: 100.372141356 name: data Venus_Crustal_Thickness.xyzFormat:# longitude latitude thickness (km)N = 260281 <0/360> <-90/90> <12.292/100.372> Effective elastic thickness model (v2015) Effective elastic thickness (Te) and internal load fraction (F) models with a spatial resolution of 1 degree, in grid (*.grd) and data table (*.xyz) formats.

The effective elastic thickness model ranges from 14 (the minimum resolvable Te value in our analysis) to 94 km. For details see Jiménez-Díaz et al. (2015). - Effective Elastic Thickness, Te (km): Venus_Elastic_Thickness_2015.grdFormat:Gridline node registration used [Geographic grid]x_min: 0 x_max: 360 x_inc: 1 name: longitude n_columns: 361y_min: -90 y_max: 90 y_inc: 1 name: latitude n_rows: 181z_min: 14 z_max: 93.9320602417 name: z Venus_Elastic_Thickness_2015.xyzFormat:# longitude latitude thickness (km)N = 65341 <0/360> <-90/90> <14.000/93.932> - Internal Load Fraction, F: Venus_Internal_Load_Fraction_2015.grdFormat:Gridline node registration used [Geographic grid]x_min: 0 x_max: 360 x_inc: 1 name: longitude n_columns: 361y_min: -90 y_max: 90 y_inc: 1 name: latitude n_rows: 181z_min: 0.121833771467 z_max: 0.804488778114 name: z Venus_Internal_Load_Fraction_2015.xyzFormat:# longitude latitude FN = 65341 <0/360> <-90/90> <0.122/0.804>