Extended Data Table 2 Summary of time-variable gravity analyses for the C20 and C30 coefficients

From: Glacial isostatic adjustment reveals Mars’s interior viscosity structure

  1. Values for m and b are for the mx + b linear fit to the residuals. The p-value tests the null hypothesis that the residuals have no correlation with time based on Wald’s test, and the r-value provides the Pearson correlation coefficient of the residuals with time.
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