Extended Data Table 2 Typical P- and S-waves velocity and density values used to estimate the S-wave reflection coefficient for models with a BML

From: Geophysical evidence for an enriched molten silicate layer above Mars’s core

  1. Typical values of Vp, Vs and density above and below the BML used to calculate the amplitude ratio between the reflected and the incident Sv-waves at the base of the partially molten BML.
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