Supporting Information for "Insights into Venus' crustal plateaus from dyke trajectories below craters" (Simulation results)

This repository contains the results presented in the article submitted to Journal of Geophysical Research: Planets entitle "Insights into Venus' crustal plateaus from dyke trajectories below craters" by Le Contellec A., Michaut C., Maccaferri F., Pinel V., Chambat F., Smrekar S.. 

It provides the simulations parameters and results of dyke propagation in a crater stress field in the conditions of Venus, using the dyke propagation code developped by F. Maccaferri (Maccaferri et al, 2020) and a stress field computation code (Le Contellec, 2024) to compute the crater stress field. 

The classification of the results corresponds to the categories defined in Section 4 of the article and are as follows: (1) corresponds to no dykes reaching the surface (green triangles), (2) to dykes reaching the surface within and outside the crater (blue dots), (3) to dykes reaching the surface exclusively within the crater (pink stars), and (4) to dykes reaching the surface exclusively outside the crater (orange diamonds).Parameters used are: crater radius R in km, initial depth (i.e. crustal thickness) Di in km, magma density ⍴mag in kg.m3, crust density ⍴c in kg.m3, density ratio ⍴mag/⍴c, initial length of the dyke L in km, initial fluid overpressure calculated from Weertman's formula ΔPi (Equation 14 of the article) in MPa, maximum value of the stress component σrr,max in MPa, maximum shear stress component on the coordinate planes σrz,max in MPa, dimensionless number ẟ (Equation 18 of the article), dimensionless number Γ (Equation 16 of the article) and the classification of the simulation result (1 to 4 depending on the observed behaviour).