Fig. 3.

(a): prior and posterior distributions for the waveguide density in the inversion of Eq. (9) with vph = 1030 ± 410 km s−1, under model M1. (b): comparison between the marginal posteriors for magnetic field strength in the same inversion for the cases of uniform and Gaussian prior on the waveguide density. (c) and (d): comparison between the joint two-dimensional posterior distributions for the internal density of the waveguide and the magnetic field strength obtained for the inference with vph = 1030 ± 410 km s−1, under model M1, for the cases of uniform priors (c) and a Gaussian prior for the internal density with μρi = 1.9 × 10−12 kg m−3 and σρi = 0.5μρi (d). The inference with the more informative prior on density leads to G and
kg m−3. Bottom panels: the outer boundaries of the light grey and dark grey shaded regions indicate the 95% and 68% credible regions.
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