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Equivalent source mapping of the lunar crustal magnetic field using ABIC

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Figure

Table 1. Two LP magnetometer datasets used for testing the scheme at the Reiner Gamma anomaly
Fig. 3.ABIC values plotted versus the hyper-parameter α for the mid-dle altitude data group
Fig. 4. Magnetic field maps computed from (a) model L and (b) model M at an altitude of 20 km
Fig. 6.Magnetic field maps computed from model H at an altitude of20 km. The contour interval is 5 nT
+3

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