Published 2024 | Version v1

FEA simulation output for Dome Craters on Ganymede and Callisto May Form by Topographic Relaxation of Pit Craters Aided by Remnant Impact Heat

Authors/Creators

  • 1. ROR icon University of Illinois Chicago

Description

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

Files

Marc_Output_Table1_Caussi.zip

Files (138.0 kB)

Name Size Download all
md5:bb015f53f435c1c92e094fbd1dc27d73
138.0 kB Preview Download