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Fig. 3 | Earth, Planets and Space

Fig. 3

From: Utility of Slepian basis functions for modeling near-surface and satellite magnetic anomalies of the Australian lithosphere

Fig. 3

a S360 model predictions of the near-surface total magnetic intensity anomalies for mainland Australia and Tasmania and b their differences; c commensurate near-surface total intensity anomaly differences between the S360 model and the degree 360 estimates of the NGDC720 model, and d the anomaly differences between the input near-surface low-pass-filtered total magnetic intensity anomaly grid and the degree 360 estimates of NGDC720. The statistics for these comparisons are listed in Tables 1 and 2

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