Origin of long-wavelength variations in crustal thickness on telluric planet -- Data & Software
Abstract
This is the data and software used for the paper : Origin of long-wavelength variations in crustal thickness on telluric planet submitted to Geophysical Research Letters.
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0 20 40 60 80 100 Crust thickness, km Hot hemisphere, E = 0 Hot hemisphere, E = 26 Cold hemisphere, E = 0 Cold hemisphere, E = 26 0.00 0.05 0.10 0.15 0.20 Melt fraction 0.0 0.5 1.0 1.5 Time, Gyr 0 5 10 15 20 25 30 35 Thermal lithopshere and crustal dichotomy, km 0.0 0.5 1.0 1.5 Time, Gyr Dc , E = 0 Dc , E = 26 0.0 0.5 1.0 1.5 Time, Gyr DL , E = 0 DL , E = 26 Moon-like Mercury-like Mars-like a) b) c) d) e) f) g) h) i)