FEA simulation output for Dome Craters on Ganymede and Callisto May Form by Topographic Relaxation of Pit Craters Aided by Remnant Impact Heat
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Text files containing the FEA outputs for each simulation in Table 1 X : Radial distance from center of crater (meters) Y : Displacement in the vertical direction (meters) Time in seconds
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Zenodo创建时间：
2024-03-28
